<?xml version="1.0" encoding="utf-8"?><!DOCTYPE article PUBLIC "-//ES//DTD journal article DTD version 5.4.0//EN//XML" "art540.dtd" [<!ENTITY gr001 SYSTEM "gr001" NDATA IMAGE><!ENTITY gr002 SYSTEM "gr002" NDATA IMAGE><!ENTITY gr003 SYSTEM "gr003" NDATA IMAGE><!ENTITY gr004 SYSTEM "gr004" NDATA IMAGE><!ENTITY gr005 SYSTEM "gr005" NDATA IMAGE>]><article xmlns="http://www.elsevier.com/xml/ja/dtd" xmlns:ce="http://www.elsevier.com/xml/common/dtd" xmlns:sa="http://www.elsevier.com/xml/common/struct-aff/dtd" xmlns:sb="http://www.elsevier.com/xml/common/struct-bib/dtd" xmlns:xlink="http://www.w3.org/1999/xlink" docsubtype="sco" xml:lang="en"><item-info><jid>PLB</jid><aid>31619</aid><ce:pii>S0370-2693(15)01015-1</ce:pii><ce:doi>10.1016/j.physletb.2015.12.067</ce:doi><ce:copyright type="other" year="2015">CERN for the benefit of the ALICE Collaboration</ce:copyright><ce:doctopics><ce:doctopic id="doc0010"><ce:text>Experiments</ce:text></ce:doctopic></ce:doctopics></item-info><ce:floats><ce:figure id="fg0010"><ce:label>Fig. 1</ce:label><ce:caption id="cp0010"><ce:simple-para id="sp0010">(a): Measured d<ce:italic>E</ce:italic>/d<ce:italic>x</ce:italic> in the TPC as function of momentum <ce:italic>p</ce:italic> expressed as a deviation from the expected energy loss of electrons, normalised by the energy-loss resolution (<ce:italic>σ</ce:italic><ce:inf>TPC</ce:inf>) after eID with TOF. The solid lines indicate the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si39.gif"><mml:msubsup><mml:mrow><mml:mi>n</mml:mi></mml:mrow><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">TPC</mml:mi></mml:mrow></mml:msubsup></mml:math> selection criteria for the TPC and TOF eID strategy. (b): <ce:italic>E</ce:italic>/<ce:italic>p</ce:italic> distribution of electrons (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si40.gif"><mml:mo>−</mml:mo><mml:mn>1</mml:mn><mml:mo>&lt;</mml:mo><mml:msubsup><mml:mrow><mml:mi>n</mml:mi></mml:mrow><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">TPC</mml:mi></mml:mrow></mml:msubsup><mml:mo>&lt;</mml:mo><mml:mn>3</mml:mn></mml:math>) and hadrons (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si41.gif"><mml:msubsup><mml:mrow><mml:mi>n</mml:mi></mml:mrow><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">TPC</mml:mi></mml:mrow></mml:msubsup><mml:mo>&lt;</mml:mo><mml:mo>−</mml:mo><mml:mn>3.5</mml:mn></mml:math>) in the transverse momentum interval 6<ce:hsp sp="0.2"/>&lt;<ce:hsp sp="0.2"/><ce:italic>p</ce:italic><ce:inf>T</ce:inf><ce:hsp sp="0.2"/>&lt;<ce:hsp sp="0.2"/>8 GeV/<ce:italic>c</ce:italic>. The <ce:italic>E</ce:italic>/<ce:italic>p</ce:italic> distribution of hadrons was normalised to that of electrons in the lower <ce:italic>E</ce:italic>/<ce:italic>p</ce:italic> range (0.4–0.6), where hadrons dominate. The solid lines indicate the applied electron selection criteria. (For interpretation of the references to color in this figure legend, the reader is referred to the web version of this article.)</ce:simple-para></ce:caption><ce:link locator="gr001" xlink:type="simple" xlink:href="pii:S0370269315010151/gr001"/></ce:figure><ce:figure id="fg0020"><ce:label>Fig. 2</ce:label><ce:caption id="cp0020"><ce:simple-para id="sp0020">Invariant mass distributions of unlike-sign and like-sign electron pairs for the inclusive electron <ce:italic>p</ce:italic><ce:inf>T</ce:inf> interval 0.5<ce:hsp sp="0.2"/>&lt;<ce:hsp sp="0.2"/><ce:italic>p</ce:italic><ce:inf>T</ce:inf><ce:hsp sp="0.2"/>&lt;<ce:hsp sp="0.2"/>0.6 GeV/<ce:italic>c</ce:italic>. The difference between the distributions yields the photonic contribution.</ce:simple-para></ce:caption><ce:link locator="gr002" xlink:type="simple" xlink:href="pii:S0370269315010151/gr002"/></ce:figure><ce:figure id="fg0030"><ce:label>Fig. 3</ce:label><ce:caption id="cp0030"><ce:simple-para id="sp0030">The <ce:italic>p</ce:italic><ce:inf>T</ce:inf>-differential invariant cross section of electrons from heavy-flavour hadron decays in minimum-bias p–Pb collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif"><mml:msqrt><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">NN</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>5.02</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math>, comparing the results of the eID strategies in the two transition regions at 2.5 and 6 GeV/<ce:italic>c</ce:italic>. The centre values are slightly shifted along the <ce:italic>p</ce:italic><ce:inf>T</ce:inf>-axis in the transition regions for better visibility. The results agree within 1%. Details on the eID strategies can be found in the text.</ce:simple-para></ce:caption><ce:link locator="gr003" xlink:type="simple" xlink:href="pii:S0370269315010151/gr003"/></ce:figure><ce:figure id="fg0040"><ce:label>Fig. 4</ce:label><ce:caption id="cp0040"><ce:simple-para id="sp0040">The <ce:italic>p</ce:italic><ce:inf>T</ce:inf>-differential invariant cross section of electrons from heavy-flavour hadron decays in minimum-bias p–Pb collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif"><mml:msqrt><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">NN</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>5.02</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math>. The pp reference obtained via the interpolation method is shown, not scaled by <ce:italic>A</ce:italic>, for comparison. The statistical uncertainties are indicated for both spectra by error bars, the systematic uncertainties are shown as boxes.</ce:simple-para></ce:caption><ce:link locator="gr004" xlink:type="simple" xlink:href="pii:S0370269315010151/gr004"/></ce:figure><ce:figure id="fg0050"><ce:label>Fig. 5</ce:label><ce:caption id="cp0050"><ce:simple-para id="sp0050">Nuclear modification factor <ce:italic>R</ce:italic><ce:inf>pPb</ce:inf> of electrons from heavy-flavour hadron decays as a function of transverse momentum for minimum-bias p–Pb collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif"><mml:msqrt><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">NN</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>5.02</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math>, compared with theoretical models <ce:cross-refs refid="br0250 br0270 br0450 br0480 br0750" id="crs0010">[25,27,45,48,75]</ce:cross-refs>, as described in the text. The vertical bars represent the statistical uncertainties, and the boxes indicate the systematic uncertainties. The systematic uncertainty from the normalisation, common to all points, is shown as a filled box at high <ce:italic>p</ce:italic><ce:inf>T</ce:inf>.</ce:simple-para></ce:caption><ce:link locator="gr005" xlink:type="simple" xlink:href="pii:S0370269315010151/gr005"/></ce:figure><ce:table xmlns:tb="http://www.elsevier.com/xml/common/table/dtd" id="tl0010" frame="topbot" rowsep="0" colsep="0"><ce:label>Table 1</ce:label><ce:caption id="cp0060"><ce:simple-para id="sp0060">Systematic uncertainties for the different momentum intervals.</ce:simple-para></ce:caption><tgroup cols="4"><colspec colnum="1" colname="col1" align="left"/><colspec colnum="2" colname="col2" align="left"/><colspec colnum="3" colname="col3" align="left"/><colspec colnum="4" colname="col4" align="left"/><thead valign="top"><row rowsep="1"><entry role="rowhead">Variable</entry><entry>0.5<ce:hsp sp="0.2"/>&lt;<ce:hsp sp="0.2"/><ce:italic>p</ce:italic><ce:inf>T</ce:inf><ce:hsp sp="0.2"/>&lt;<ce:hsp sp="0.2"/>2.5 GeV/<ce:italic>c</ce:italic></entry><entry>2.5<ce:hsp sp="0.2"/>&lt;<ce:hsp sp="0.2"/><ce:italic>p</ce:italic><ce:inf>T</ce:inf><ce:hsp sp="0.2"/>&lt;<ce:hsp sp="0.2"/>6 GeV/<ce:italic>c</ce:italic></entry><entry>6<ce:hsp sp="0.2"/>&lt;<ce:hsp sp="0.2"/><ce:italic>p</ce:italic><ce:inf>T</ce:inf><ce:hsp sp="0.2"/>&lt;<ce:hsp sp="0.2"/>12 GeV/<ce:italic>c</ce:italic></entry></row></thead><tbody valign="top"><row><entry role="rowhead">Tracking</entry><entry>4.3%</entry><entry>2.2%</entry><entry>3%</entry></row><row><entry role="rowhead">Matching</entry><entry>4.2%</entry><entry>3%</entry><entry>3.2%</entry></row><row><entry role="rowhead">eID</entry><entry>3.6%</entry><entry>3.6%</entry><entry>3.2% (6–8 GeV/<ce:italic>c</ce:italic>)</entry></row><row><entry role="rowhead"/><entry/><entry/><entry>5.1% (8–10 GeV/<ce:italic>c</ce:italic>)</entry></row><row><entry role="rowhead"/><entry/><entry/><entry>15.1% (10–12 GeV/<ce:italic>c</ce:italic>)</entry></row><row><entry role="rowhead" morerows="1">Photonic method</entry><entry>6.9% (0.5–1 GeV/<ce:italic>c</ce:italic>)</entry><entry>2.4%</entry><entry>4.5%</entry></row><row><entry colname="col2">3.7% (1–2.5 GeV/<ce:italic>c</ce:italic>)</entry><entry colname="col3"/><entry colname="col4"/></row><row><entry role="rowhead">Unfolding</entry><entry>1%</entry><entry>1%</entry><entry>&lt;1%</entry></row><row><entry role="rowhead" namest="col1" nameend="col4" align="left"><ce:vsp sp="0.5"/></entry></row><row><entry role="rowhead">Total</entry><entry>9.9% (0.5–1 GeV/<ce:italic>c</ce:italic>)</entry><entry>5.8%</entry><entry>7.1% (6–8 GeV/<ce:italic>c</ce:italic>)</entry></row><row><entry role="rowhead"/><entry>8.0% (1–2.5 GeV/<ce:italic>c</ce:italic>)</entry><entry/><entry>8.1% (8–10 GeV/<ce:italic>c</ce:italic>)</entry></row><row><entry role="rowhead"/><entry/><entry/><entry>16.4% (10–12 GeV/<ce:italic>c</ce:italic>)</entry></row></tbody></tgroup></ce:table></ce:floats><head><ce:title id="ti0010">Measurement of electrons from heavy-flavour hadron decays in p–Pb collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif"><mml:msqrt><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">NN</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>5.02</mml:mn><mml:mspace width="0.25em"/><mml:mtext>TeV</mml:mtext></mml:math></ce:title><ce:author-group id="ag0010"><ce:collaboration id="co0010"><ce:text>ALICE Collaboration</ce:text><ce:cross-ref refid="fn0040" id="crf0010"><ce:sup>⋆</ce:sup></ce:cross-ref><ce:author-group id="ag0020"><ce:author id="au0010" author-id="S0370269315010151-8b18b433990f9b8105d02f6a5c0371eb"><ce:given-name>J.</ce:given-name><ce:surname>Adam</ce:surname><ce:cross-ref refid="aff0400" id="crf0020"><ce:sup>40</ce:sup></ce:cross-ref></ce:author><ce:author id="au0020" author-id="S0370269315010151-0eab85892b6d74b18661e74a7987c599"><ce:given-name>D.</ce:given-name><ce:surname>Adamová</ce:surname><ce:cross-ref refid="aff0830" id="crf0030"><ce:sup>83</ce:sup></ce:cross-ref></ce:author><ce:author id="au0030" author-id="S0370269315010151-73b4c3024ff04dff21b938181b2a84c8"><ce:given-name>M.M.</ce:given-name><ce:surname>Aggarwal</ce:surname><ce:cross-ref refid="aff0870" id="crf0040"><ce:sup>87</ce:sup></ce:cross-ref></ce:author><ce:author id="au0040" author-id="S0370269315010151-ed2d58d89990c41bb43c091d01e5029a"><ce:given-name>G.</ce:given-name><ce:surname>Aglieri Rinella</ce:surname><ce:cross-ref refid="aff0360" id="crf0050"><ce:sup>36</ce:sup></ce:cross-ref></ce:author><ce:author id="au0050" author-id="S0370269315010151-0c7a7863b7384aa5fdf06a0f187949c8"><ce:given-name>M.</ce:given-name><ce:surname>Agnello</ce:surname><ce:cross-ref refid="aff1100" id="crf0060"><ce:sup>110</ce:sup></ce:cross-ref></ce:author><ce:author id="au0060" 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id="crf0310"><ce:sup>107</ce:sup></ce:cross-ref></ce:author><ce:author id="au0300" author-id="S0370269315010151-51fafbdf488707238bb68ddcfdcc1d43"><ce:given-name>P.</ce:given-name><ce:surname>Antonioli</ce:surname><ce:cross-ref refid="aff1040" id="crf0320"><ce:sup>104</ce:sup></ce:cross-ref></ce:author><ce:author id="au0310" author-id="S0370269315010151-6e095add140944d2ab055d51972eed48"><ce:given-name>L.</ce:given-name><ce:surname>Aphecetche</ce:surname><ce:cross-ref refid="aff1130" id="crf0330"><ce:sup>113</ce:sup></ce:cross-ref></ce:author><ce:author id="au0320" author-id="S0370269315010151-0e6d19528507f8cc3f37539a3381820b"><ce:given-name>H.</ce:given-name><ce:surname>Appelshäuser</ce:surname><ce:cross-ref refid="aff0530" id="crf0340"><ce:sup>53</ce:sup></ce:cross-ref></ce:author><ce:author id="au0330" author-id="S0370269315010151-680f2a41c459bec210e2ebd5a58612be"><ce:given-name>S.</ce:given-name><ce:surname>Arcelli</ce:surname><ce:cross-ref refid="aff0280" id="crf0350"><ce:sup>28</ce:sup></ce:cross-ref></ce:author><ce:author id="au0340" author-id="S0370269315010151-ab22692334a2fe57e1742058759c61dd"><ce:given-name>R.</ce:given-name><ce:surname>Arnaldi</ce:surname><ce:cross-ref refid="aff1100" id="crf0360"><ce:sup>110</ce:sup></ce:cross-ref></ce:author><ce:author id="au0350" author-id="S0370269315010151-1114b75c14379f8d1f0f908b0dd0f59e"><ce:given-name>O.W.</ce:given-name><ce:surname>Arnold</ce:surname><ce:cross-ref refid="aff0370" id="crf0370"><ce:sup>37</ce:sup></ce:cross-ref><ce:cross-ref refid="aff0920" id="crf0380"><ce:sup>92</ce:sup></ce:cross-ref></ce:author><ce:author id="au0360" author-id="S0370269315010151-697698547c36f9d3e7187cd6f06d1183"><ce:given-name>I.C.</ce:given-name><ce:surname>Arsene</ce:surname><ce:cross-ref refid="aff0220" id="crf0390"><ce:sup>22</ce:sup></ce:cross-ref></ce:author><ce:author id="au0370" author-id="S0370269315010151-ff7baf83a4c274c1a18de37c9dc67976"><ce:given-name>M.</ce:given-name><ce:surname>Arslandok</ce:surname><ce:cross-ref refid="aff0530" id="crf0400"><ce:sup>53</ce:sup></ce:cross-ref></ce:author><ce:author id="au0380" author-id="S0370269315010151-9c0c134b5e5fefcb5faa12330a978012"><ce:given-name>B.</ce:given-name><ce:surname>Audurier</ce:surname><ce:cross-ref refid="aff1130" id="crf0410"><ce:sup>113</ce:sup></ce:cross-ref></ce:author><ce:author id="au0390" author-id="S0370269315010151-755bc219fdc7b4d25c2e083c10e7e386"><ce:given-name>A.</ce:given-name><ce:surname>Augustinus</ce:surname><ce:cross-ref refid="aff0360" id="crf0420"><ce:sup>36</ce:sup></ce:cross-ref></ce:author><ce:author id="au0400" author-id="S0370269315010151-e39ad2348626d77041016a5dd27ef327"><ce:given-name>R.</ce:given-name><ce:surname>Averbeck</ce:surname><ce:cross-ref refid="aff0960" id="crf0430"><ce:sup>96</ce:sup></ce:cross-ref></ce:author><ce:author id="au0410" author-id="S0370269315010151-9477d32af0ceb836b9acd7ac436a380f"><ce:given-name>M.D.</ce:given-name><ce:surname>Azmi</ce:surname><ce:cross-ref refid="aff0190" id="crf0440"><ce:sup>19</ce:sup></ce:cross-ref></ce:author><ce:author id="au0420" author-id="S0370269315010151-7c7197c0ac2a51bf94b01b500c38aedc"><ce:given-name>A.</ce:given-name><ce:surname>Badalà</ce:surname><ce:cross-ref refid="aff1060" id="crf0450"><ce:sup>106</ce:sup></ce:cross-ref></ce:author><ce:author id="au0430" author-id="S0370269315010151-e2f139312a0e407b3c4d2412844bc5b9"><ce:given-name>Y.W.</ce:given-name><ce:surname>Baek</ce:surname><ce:cross-ref refid="aff0670" id="crf0460"><ce:sup>67</ce:sup></ce:cross-ref></ce:author><ce:author id="au0440" author-id="S0370269315010151-192b19c1e857022f3f545fa2c80afaf8"><ce:given-name>S.</ce:given-name><ce:surname>Bagnasco</ce:surname><ce:cross-ref refid="aff1100" id="crf0470"><ce:sup>110</ce:sup></ce:cross-ref></ce:author><ce:author id="au0450" author-id="S0370269315010151-04bb83e7910b72460bb5a8aa2184d9e6"><ce:given-name>R.</ce:given-name><ce:surname>Bailhache</ce:surname><ce:cross-ref refid="aff0530" id="crf0480"><ce:sup>53</ce:sup></ce:cross-ref></ce:author><ce:author id="au0460" author-id="S0370269315010151-9fb0ec712dc4e6ddbda7e348eaa5aa42"><ce:given-name>R.</ce:given-name><ce:surname>Bala</ce:surname><ce:cross-ref refid="aff0900" id="crf0490"><ce:sup>90</ce:sup></ce:cross-ref></ce:author><ce:author id="au0470" author-id="S0370269315010151-139e513e7bdef112603b9937bdd15344"><ce:given-name>A.</ce:given-name><ce:surname>Baldisseri</ce:surname><ce:cross-ref refid="aff0150" id="crf0500"><ce:sup>15</ce:sup></ce:cross-ref></ce:author><ce:author id="au0480" author-id="S0370269315010151-00599ef3fa5a766b5d9a28a9bae34839"><ce:given-name>R.C.</ce:given-name><ce:surname>Baral</ce:surname><ce:cross-ref refid="aff0610" id="crf0510"><ce:sup>61</ce:sup></ce:cross-ref></ce:author><ce:author id="au0490" author-id="S0370269315010151-c4d3d0c805435554468b7135659c23d7"><ce:given-name>A.M.</ce:given-name><ce:surname>Barbano</ce:surname><ce:cross-ref refid="aff0270" id="crf0520"><ce:sup>27</ce:sup></ce:cross-ref></ce:author><ce:author id="au0500" author-id="S0370269315010151-34de4a3f87192e0e6f4308aac96e6dc4"><ce:given-name>R.</ce:given-name><ce:surname>Barbera</ce:surname><ce:cross-ref refid="aff0290" id="crf0530"><ce:sup>29</ce:sup></ce:cross-ref></ce:author><ce:author id="au0510" author-id="S0370269315010151-b79598b96041bc2c53efd57884b3ad8a"><ce:given-name>F.</ce:given-name><ce:surname>Barile</ce:surname><ce:cross-ref refid="aff0330" id="crf0540"><ce:sup>33</ce:sup></ce:cross-ref></ce:author><ce:author id="au0520" author-id="S0370269315010151-6cc8c551caade64d21a326a2042741be"><ce:given-name>G.G.</ce:given-name><ce:surname>Barnaföldi</ce:surname><ce:cross-ref refid="aff1350" id="crf0550"><ce:sup>135</ce:sup></ce:cross-ref></ce:author><ce:author id="au0530" author-id="S0370269315010151-e5502945a2b5f28905e341734bcb3b15"><ce:given-name>L.S.</ce:given-name><ce:surname>Barnby</ce:surname><ce:cross-ref refid="aff1010" id="crf0560"><ce:sup>101</ce:sup></ce:cross-ref></ce:author><ce:author id="au0540" author-id="S0370269315010151-73acb1b6c325d96b54abe7b64278d6ea"><ce:given-name>V.</ce:given-name><ce:surname>Barret</ce:surname><ce:cross-ref refid="aff0700" id="crf0570"><ce:sup>70</ce:sup></ce:cross-ref></ce:author><ce:author id="au0550" author-id="S0370269315010151-4f275ed0a1a673c459491cce998dfa09"><ce:given-name>P.</ce:given-name><ce:surname>Bartalini</ce:surname><ce:cross-ref refid="aff0070" id="crf0580"><ce:sup>7</ce:sup></ce:cross-ref></ce:author><ce:author id="au0560" author-id="S0370269315010151-99991a11640d18ba216157ce9bd24b50"><ce:given-name>K.</ce:given-name><ce:surname>Barth</ce:surname><ce:cross-ref refid="aff0360" id="crf0590"><ce:sup>36</ce:sup></ce:cross-ref></ce:author><ce:author id="au0570" author-id="S0370269315010151-64e7615858875feebe67be9ca74611a3"><ce:given-name>J.</ce:given-name><ce:surname>Bartke</ce:surname><ce:cross-ref refid="aff1170" id="crf0600"><ce:sup>117</ce:sup></ce:cross-ref></ce:author><ce:author id="au0580" author-id="S0370269315010151-7b25cdf12989c93bb0b35e9a7b6c993e"><ce:given-name>E.</ce:given-name><ce:surname>Bartsch</ce:surname><ce:cross-ref refid="aff0530" id="crf0610"><ce:sup>53</ce:sup></ce:cross-ref></ce:author><ce:author id="au0590" author-id="S0370269315010151-66deed9a1673ac50b22cfa6abcc4b6a1"><ce:given-name>M.</ce:given-name><ce:surname>Basile</ce:surname><ce:cross-ref refid="aff0280" id="crf0620"><ce:sup>28</ce:sup></ce:cross-ref></ce:author><ce:author id="au0600" author-id="S0370269315010151-ffe3cbf955e2397362cc39ed0f8eb51b"><ce:given-name>N.</ce:given-name><ce:surname>Bastid</ce:surname><ce:cross-ref refid="aff0700" id="crf0630"><ce:sup>70</ce:sup></ce:cross-ref></ce:author><ce:author id="au0610" author-id="S0370269315010151-1b8917b5d28e8d66a2eaf20a4369cc82"><ce:given-name>S.</ce:given-name><ce:surname>Basu</ce:surname><ce:cross-ref refid="aff1320" id="crf0640"><ce:sup>132</ce:sup></ce:cross-ref></ce:author><ce:author id="au0620" author-id="S0370269315010151-2259cb02dbf9b3d7951214bcf902e272"><ce:given-name>B.</ce:given-name><ce:surname>Bathen</ce:surname><ce:cross-ref refid="aff0540" id="crf0650"><ce:sup>54</ce:sup></ce:cross-ref></ce:author><ce:author id="au0630" author-id="S0370269315010151-2fee908da21994198610c94092286ad8"><ce:given-name>G.</ce:given-name><ce:surname>Batigne</ce:surname><ce:cross-ref refid="aff1130" id="crf0660"><ce:sup>113</ce:sup></ce:cross-ref></ce:author><ce:author id="au0640" author-id="S0370269315010151-4b403ca82962f55a0269a2d0b95611fd"><ce:given-name>A.</ce:given-name><ce:surname>Batista Camejo</ce:surname><ce:cross-ref refid="aff0700" id="crf0670"><ce:sup>70</ce:sup></ce:cross-ref></ce:author><ce:author id="au0650" author-id="S0370269315010151-f1278714281193a9113b12f11f4b9fc7"><ce:given-name>B.</ce:given-name><ce:surname>Batyunya</ce:surname><ce:cross-ref refid="aff0660" id="crf0680"><ce:sup>66</ce:sup></ce:cross-ref></ce:author><ce:author id="au0660" author-id="S0370269315010151-0ae119c8ef0ed2a2c68580e1463298d5"><ce:given-name>P.C.</ce:given-name><ce:surname>Batzing</ce:surname><ce:cross-ref refid="aff0220" id="crf0690"><ce:sup>22</ce:sup></ce:cross-ref></ce:author><ce:author id="au0670" author-id="S0370269315010151-6ce098f5eecbf05e4aaa4608b11de130"><ce:given-name>I.G.</ce:given-name><ce:surname>Bearden</ce:surname><ce:cross-ref refid="aff0800" id="crf0700"><ce:sup>80</ce:sup></ce:cross-ref></ce:author><ce:author id="au0680" author-id="S0370269315010151-4e2d9629abca6bf56844117c95c47ac6"><ce:given-name>H.</ce:given-name><ce:surname>Beck</ce:surname><ce:cross-ref refid="aff0530" id="crf0710"><ce:sup>53</ce:sup></ce:cross-ref></ce:author><ce:author id="au0690" 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author-id="S0370269315010151-0e194c0ad078438bf71482e49c2edfdd"><ce:given-name>Y.</ce:given-name><ce:surname>Miake</ce:surname><ce:cross-ref refid="aff1280" id="crf5880"><ce:sup>128</ce:sup></ce:cross-ref></ce:author><ce:author id="au5490" author-id="S0370269315010151-a59a89b866e46799327bc72c8360c456"><ce:given-name>M.M.</ce:given-name><ce:surname>Mieskolainen</ce:surname><ce:cross-ref refid="aff0460" id="crf5890"><ce:sup>46</ce:sup></ce:cross-ref></ce:author><ce:author id="au5500" author-id="S0370269315010151-38f09e4de019d55f2f02af6568866c3a"><ce:given-name>K.</ce:given-name><ce:surname>Mikhaylov</ce:surname><ce:cross-ref refid="aff0660" id="crf5900"><ce:sup>66</ce:sup></ce:cross-ref><ce:cross-ref refid="aff0580" id="crf5910"><ce:sup>58</ce:sup></ce:cross-ref></ce:author><ce:author id="au5510" author-id="S0370269315010151-715ea5c7af16e72028125c38c9a42976"><ce:given-name>L.</ce:given-name><ce:surname>Milano</ce:surname><ce:cross-ref refid="aff0360" id="crf5920"><ce:sup>36</ce:sup></ce:cross-ref></ce:author><ce:author id="au5520" author-id="S0370269315010151-253853274ee39041c15cb5865ff95c89"><ce:given-name>J.</ce:given-name><ce:surname>Milosevic</ce:surname><ce:cross-ref refid="aff0220" id="crf5930"><ce:sup>22</ce:sup></ce:cross-ref></ce:author><ce:author id="au5530" author-id="S0370269315010151-f9388f6dfcf13ce7143be1302cc4bf3e"><ce:given-name>L.M.</ce:given-name><ce:surname>Minervini</ce:surname><ce:cross-ref refid="aff1030" id="crf5940"><ce:sup>103</ce:sup></ce:cross-ref><ce:cross-ref refid="aff0230" id="crf5950"><ce:sup>23</ce:sup></ce:cross-ref></ce:author><ce:author id="au5540" author-id="S0370269315010151-cc38341b24441c4cbe0892b494abbf1a"><ce:given-name>A.</ce:given-name><ce:surname>Mischke</ce:surname><ce:cross-ref refid="aff0570" id="crf5960"><ce:sup>57</ce:sup></ce:cross-ref></ce:author><ce:author id="au5550" author-id="S0370269315010151-559e4d90ae5661c2eeeb2c90664b0cf7"><ce:given-name>A.N.</ce:given-name><ce:surname>Mishra</ce:surname><ce:cross-ref refid="aff0490" id="crf5970"><ce:sup>49</ce:sup></ce:cross-ref></ce:author><ce:author id="au5560" author-id="S0370269315010151-11f22e778a9776fc0fb59c6d4d8f1bd0"><ce:given-name>D.</ce:given-name><ce:surname>Miśkowiec</ce:surname><ce:cross-ref refid="aff0960" id="crf5980"><ce:sup>96</ce:sup></ce:cross-ref></ce:author><ce:author id="au5570" author-id="S0370269315010151-5f8e69801dc0070ed86b7778435eb908"><ce:given-name>J.</ce:given-name><ce:surname>Mitra</ce:surname><ce:cross-ref refid="aff1320" id="crf5990"><ce:sup>132</ce:sup></ce:cross-ref></ce:author><ce:author id="au5580" author-id="S0370269315010151-b82629e711ea1dc7182921cffc8ce706"><ce:given-name>C.M.</ce:given-name><ce:surname>Mitu</ce:surname><ce:cross-ref refid="aff0620" id="crf6000"><ce:sup>62</ce:sup></ce:cross-ref></ce:author><ce:author id="au5590" author-id="S0370269315010151-6beff8693d057402d84bfa70c6787f44"><ce:given-name>N.</ce:given-name><ce:surname>Mohammadi</ce:surname><ce:cross-ref refid="aff0570" id="crf6010"><ce:sup>57</ce:sup></ce:cross-ref></ce:author><ce:author id="au5600" author-id="S0370269315010151-41ecee891e15cd078816eed128811f97"><ce:given-name>B.</ce:given-name><ce:surname>Mohanty</ce:surname><ce:cross-ref refid="aff0790" id="crf6020"><ce:sup>79</ce:sup></ce:cross-ref><ce:cross-ref refid="aff1320" id="crf6030"><ce:sup>132</ce:sup></ce:cross-ref></ce:author><ce:author id="au5610" author-id="S0370269315010151-186643e865a23a60fd55015e80a3f828"><ce:given-name>L.</ce:given-name><ce:surname>Molnar</ce:surname><ce:cross-ref refid="aff0550" id="crf6040"><ce:sup>55</ce:sup></ce:cross-ref><ce:cross-ref refid="aff1130" id="crf6050"><ce:sup>113</ce:sup></ce:cross-ref></ce:author><ce:author id="au5620" author-id="S0370269315010151-67a5a442fc7d90e347c88ddcdb6c89df"><ce:given-name>L.</ce:given-name><ce:surname>Montaño 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author-id="S0370269315010151-d5dd71c1a20dddaa53467a877c13c4ec"><ce:given-name>S.</ce:given-name><ce:surname>Moretto</ce:surname><ce:cross-ref refid="aff0300" id="crf6110"><ce:sup>30</ce:sup></ce:cross-ref></ce:author><ce:author id="au5670" author-id="S0370269315010151-76c47686c17c0b8392691e46e84c6cd3"><ce:given-name>A.</ce:given-name><ce:surname>Morreale</ce:surname><ce:cross-ref refid="aff1130" id="crf6120"><ce:sup>113</ce:sup></ce:cross-ref></ce:author><ce:author id="au5680" author-id="S0370269315010151-3b644752f2833a280590e7d2cb815635"><ce:given-name>A.</ce:given-name><ce:surname>Morsch</ce:surname><ce:cross-ref refid="aff0360" id="crf6130"><ce:sup>36</ce:sup></ce:cross-ref></ce:author><ce:author id="au5690" author-id="S0370269315010151-64a6ab0403f8cd64a5dff0e5eb920af6"><ce:given-name>V.</ce:given-name><ce:surname>Muccifora</ce:surname><ce:cross-ref refid="aff0720" id="crf6140"><ce:sup>72</ce:sup></ce:cross-ref></ce:author><ce:author id="au5700" author-id="S0370269315010151-a0c40dcd3bce329a03e938ee3cced0d4"><ce:given-name>E.</ce:given-name><ce:surname>Mudnic</ce:surname><ce:cross-ref refid="aff1160" id="crf6150"><ce:sup>116</ce:sup></ce:cross-ref></ce:author><ce:author id="au5710" author-id="S0370269315010151-dbf9e7107a1a9afac70727ed6bca2a6f"><ce:given-name>D.</ce:given-name><ce:surname>Mühlheim</ce:surname><ce:cross-ref refid="aff0540" id="crf6160"><ce:sup>54</ce:sup></ce:cross-ref></ce:author><ce:author id="au5720" author-id="S0370269315010151-b2ff5bf3b45a3f5a117d5b53ed508ff9"><ce:given-name>S.</ce:given-name><ce:surname>Muhuri</ce:surname><ce:cross-ref refid="aff1320" id="crf6170"><ce:sup>132</ce:sup></ce:cross-ref></ce:author><ce:author id="au5730" author-id="S0370269315010151-91e6cd358f0fb709b51d5a354b105d75"><ce:given-name>M.</ce:given-name><ce:surname>Mukherjee</ce:surname><ce:cross-ref refid="aff1320" id="crf6180"><ce:sup>132</ce:sup></ce:cross-ref></ce:author><ce:author id="au5740" 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author-id="S0370269315010151-68219ddebcaeab26e2fa5bb9813a53ea"><ce:given-name>S.</ce:given-name><ce:surname>Oh</ce:surname><ce:cross-ref refid="aff1360" id="crf6560"><ce:sup>136</ce:sup></ce:cross-ref></ce:author><ce:author id="au6100" author-id="S0370269315010151-fcc85b491c88808354bad61f6e61e664"><ce:given-name>S.K.</ce:given-name><ce:surname>Oh</ce:surname><ce:cross-ref refid="aff0670" id="crf6570"><ce:sup>67</ce:sup></ce:cross-ref></ce:author><ce:author id="au6110" author-id="S0370269315010151-68c856e3e31ba9ae46e1a3cf0fd7b39f"><ce:given-name>A.</ce:given-name><ce:surname>Ohlson</ce:surname><ce:cross-ref refid="aff0360" id="crf6580"><ce:sup>36</ce:sup></ce:cross-ref></ce:author><ce:author id="au6120" author-id="S0370269315010151-fe23496516c9ed6c194b1a1223c5a5f7"><ce:given-name>A.</ce:given-name><ce:surname>Okatan</ce:surname><ce:cross-ref refid="aff0690" id="crf6590"><ce:sup>69</ce:sup></ce:cross-ref></ce:author><ce:author id="au6130" author-id="S0370269315010151-fd9a823bfe4db3fef209eaf96bcad8aa"><ce:given-name>T.</ce:given-name><ce:surname>Okubo</ce:surname><ce:cross-ref refid="aff0470" id="crf6600"><ce:sup>47</ce:sup></ce:cross-ref></ce:author><ce:author id="au6140" author-id="S0370269315010151-1a8a9b16797c3284a57ed8daa0e8cd57"><ce:given-name>L.</ce:given-name><ce:surname>Olah</ce:surname><ce:cross-ref refid="aff1350" id="crf6610"><ce:sup>135</ce:sup></ce:cross-ref></ce:author><ce:author id="au6150" author-id="S0370269315010151-4b54637a0b3dbb9f03da377fb857f191"><ce:given-name>J.</ce:given-name><ce:surname>Oleniacz</ce:surname><ce:cross-ref refid="aff1330" id="crf6620"><ce:sup>133</ce:sup></ce:cross-ref></ce:author><ce:author id="au6160" author-id="S0370269315010151-e919d0a3ebb4bb927bf3a87e6fc67c88"><ce:given-name>A.C.</ce:given-name><ce:surname>Oliveira Da Silva</ce:surname><ce:cross-ref refid="aff1200" id="crf6630"><ce:sup>120</ce:sup></ce:cross-ref></ce:author><ce:author id="au6170" author-id="S0370269315010151-ee3f97c8e319fe4cdf98e0660785c85a"><ce:given-name>M.H.</ce:given-name><ce:surname>Oliver</ce:surname><ce:cross-ref refid="aff1360" id="crf6640"><ce:sup>136</ce:sup></ce:cross-ref></ce:author><ce:author id="au6180" author-id="S0370269315010151-11a9f3028601db0ab23d6bc6cd1a8906"><ce:given-name>J.</ce:given-name><ce:surname>Onderwaater</ce:surname><ce:cross-ref refid="aff0960" id="crf6650"><ce:sup>96</ce:sup></ce:cross-ref></ce:author><ce:author id="au6190" author-id="S0370269315010151-dda435886a590cbfc7ea1d77af3e51f5"><ce:given-name>C.</ce:given-name><ce:surname>Oppedisano</ce:surname><ce:cross-ref refid="aff1100" id="crf6660"><ce:sup>110</ce:sup></ce:cross-ref></ce:author><ce:author id="au6200" author-id="S0370269315010151-bbf1c200812926ad8b90f09db055572f"><ce:given-name>R.</ce:given-name><ce:surname>Orava</ce:surname><ce:cross-ref refid="aff0460" id="crf6670"><ce:sup>46</ce:sup></ce:cross-ref></ce:author><ce:author id="au6210" author-id="S0370269315010151-c6a2d1996925547f52c523a908287916"><ce:given-name>A.</ce:given-name><ce:surname>Ortiz Velasquez</ce:surname><ce:cross-ref refid="aff0630" id="crf6680"><ce:sup>63</ce:sup></ce:cross-ref></ce:author><ce:author id="au6220" author-id="S0370269315010151-d7f1b48c18151d2adcfd0901daea63ca"><ce:given-name>A.</ce:given-name><ce:surname>Oskarsson</ce:surname><ce:cross-ref refid="aff0340" id="crf6690"><ce:sup>34</ce:sup></ce:cross-ref></ce:author><ce:author id="au6230" author-id="S0370269315010151-453c2920b4d8be43344a508683c61206"><ce:given-name>J.</ce:given-name><ce:surname>Otwinowski</ce:surname><ce:cross-ref refid="aff1170" id="crf6700"><ce:sup>117</ce:sup></ce:cross-ref></ce:author><ce:author id="au6240" author-id="S0370269315010151-ef1f97862dcdec187e1b2f91615f60fb"><ce:given-name>K.</ce:given-name><ce:surname>Oyama</ce:surname><ce:cross-ref refid="aff0930" id="crf6710"><ce:sup>93</ce:sup></ce:cross-ref><ce:cross-ref refid="aff0760" id="crf6720"><ce:sup>76</ce:sup></ce:cross-ref></ce:author><ce:author id="au6250" author-id="S0370269315010151-082d0c7173979bbf3fd55fa1de32e7ce"><ce:given-name>M.</ce:given-name><ce:surname>Ozdemir</ce:surname><ce:cross-ref refid="aff0530" id="crf6730"><ce:sup>53</ce:sup></ce:cross-ref></ce:author><ce:author id="au6260" author-id="S0370269315010151-02951a4df40a044a3fdcb144a019433a"><ce:given-name>Y.</ce:given-name><ce:surname>Pachmayer</ce:surname><ce:cross-ref refid="aff0930" id="crf6740"><ce:sup>93</ce:sup></ce:cross-ref></ce:author><ce:author id="au6270" author-id="S0370269315010151-5b1e150104060015d5e1c47b94b66264"><ce:given-name>P.</ce:given-name><ce:surname>Pagano</ce:surname><ce:cross-ref refid="aff0310" id="crf6750"><ce:sup>31</ce:sup></ce:cross-ref></ce:author><ce:author id="au6280" author-id="S0370269315010151-ce839a94242220bf435631842afb0293"><ce:given-name>G.</ce:given-name><ce:surname>Paić</ce:surname><ce:cross-ref refid="aff0630" id="crf6760"><ce:sup>63</ce:sup></ce:cross-ref></ce:author><ce:author id="au6290" author-id="S0370269315010151-c33ee1a975926fdc234aa14e27db2b81"><ce:given-name>S.K.</ce:given-name><ce:surname>Pal</ce:surname><ce:cross-ref refid="aff1320" id="crf6770"><ce:sup>132</ce:sup></ce:cross-ref></ce:author><ce:author id="au6300" author-id="S0370269315010151-91a644f892941ae95721b27159cabf53"><ce:given-name>J.</ce:given-name><ce:surname>Pan</ce:surname><ce:cross-ref refid="aff1340" id="crf6780"><ce:sup>134</ce:sup></ce:cross-ref></ce:author><ce:author id="au6310" author-id="S0370269315010151-273ae852b4b71271ca9ab96ccaee962c"><ce:given-name>A.K.</ce:given-name><ce:surname>Pandey</ce:surname><ce:cross-ref refid="aff0480" id="crf6790"><ce:sup>48</ce:sup></ce:cross-ref></ce:author><ce:author id="au6320" author-id="S0370269315010151-e133909d3904f97b2c57bcf066a070fe"><ce:given-name>P.</ce:given-name><ce:surname>Papcun</ce:surname><ce:cross-ref refid="aff1150" 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author-id="S0370269315010151-50d34f5c70fe3bc231e08d678bed943a"><ce:given-name>E.</ce:given-name><ce:surname>Perez Lezama</ce:surname><ce:cross-ref refid="aff0530" id="crf6970"><ce:sup>53</ce:sup></ce:cross-ref></ce:author><ce:author id="au6490" author-id="S0370269315010151-9ea99718c0474303d27c260a69e44fc3"><ce:given-name>V.</ce:given-name><ce:surname>Peskov</ce:surname><ce:cross-ref refid="aff0530" id="crf6980"><ce:sup>53</ce:sup></ce:cross-ref></ce:author><ce:author id="au6500" author-id="S0370269315010151-b2a1cbaa55a74f346f1338623a67cd26"><ce:given-name>Y.</ce:given-name><ce:surname>Pestov</ce:surname><ce:cross-ref refid="aff0050" id="crf6990"><ce:sup>5</ce:sup></ce:cross-ref></ce:author><ce:author id="au6510" author-id="S0370269315010151-45f917c01c367be5af8a10d42512d4c3"><ce:given-name>V.</ce:given-name><ce:surname>Petráček</ce:surname><ce:cross-ref refid="aff0400" id="crf7000"><ce:sup>40</ce:sup></ce:cross-ref></ce:author><ce:author id="au6520" author-id="S0370269315010151-dbee9581f6b117e88194a9f22c5368c0"><ce:given-name>V.</ce:given-name><ce:surname>Petrov</ce:surname><ce:cross-ref refid="aff1110" id="crf7010"><ce:sup>111</ce:sup></ce:cross-ref></ce:author><ce:author id="au6530" author-id="S0370269315010151-727e781718043733efb713fa083fe9a6"><ce:given-name>M.</ce:given-name><ce:surname>Petrovici</ce:surname><ce:cross-ref refid="aff0780" id="crf7020"><ce:sup>78</ce:sup></ce:cross-ref></ce:author><ce:author id="au6540" author-id="S0370269315010151-fe630e6881c0d28baa9294582efd234c"><ce:given-name>C.</ce:given-name><ce:surname>Petta</ce:surname><ce:cross-ref refid="aff0290" id="crf7030"><ce:sup>29</ce:sup></ce:cross-ref></ce:author><ce:author id="au6550" author-id="S0370269315010151-78123ee98907dd03c1791d033e172234"><ce:given-name>S.</ce:given-name><ce:surname>Piano</ce:surname><ce:cross-ref refid="aff1090" id="crf7040"><ce:sup>109</ce:sup></ce:cross-ref></ce:author><ce:author id="au6560" author-id="S0370269315010151-946883e1f561d1a058691674b9d6bd2e"><ce:given-name>M.</ce:given-name><ce:surname>Pikna</ce:surname><ce:cross-ref refid="aff0390" id="crf7050"><ce:sup>39</ce:sup></ce:cross-ref></ce:author><ce:author id="au6570" author-id="S0370269315010151-527c1efc9afeb3aa34f6162708c25dbc"><ce:given-name>P.</ce:given-name><ce:surname>Pillot</ce:surname><ce:cross-ref refid="aff1130" id="crf7060"><ce:sup>113</ce:sup></ce:cross-ref></ce:author><ce:author id="au6580" author-id="S0370269315010151-cb4892c3af4fce0f3301066e18feebc7"><ce:given-name>O.</ce:given-name><ce:surname>Pinazza</ce:surname><ce:cross-ref refid="aff1040" id="crf7070"><ce:sup>104</ce:sup></ce:cross-ref><ce:cross-ref refid="aff0360" id="crf7080"><ce:sup>36</ce:sup></ce:cross-ref></ce:author><ce:author id="au6590" author-id="S0370269315010151-f12732ef44b9fddd17576a6bf3d93dd4"><ce:given-name>L.</ce:given-name><ce:surname>Pinsky</ce:surname><ce:cross-ref refid="aff1220" 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author-id="S0370269315010151-ce5d8d52aff3b9a257186938eba69940"><ce:given-name>M.</ce:given-name><ce:surname>Slupecki</ce:surname><ce:cross-ref refid="aff1230" id="crf8720"><ce:sup>123</ce:sup></ce:cross-ref></ce:author><ce:author id="au8100" author-id="S0370269315010151-4dff2a8cce793ddddad546bf49106817"><ce:given-name>N.</ce:given-name><ce:surname>Smirnov</ce:surname><ce:cross-ref refid="aff1360" id="crf8730"><ce:sup>136</ce:sup></ce:cross-ref></ce:author><ce:author id="au8110" author-id="S0370269315010151-e12bdf24e76db6c87b277836cf233019"><ce:given-name>R.J.M.</ce:given-name><ce:surname>Snellings</ce:surname><ce:cross-ref refid="aff0570" id="crf8740"><ce:sup>57</ce:sup></ce:cross-ref></ce:author><ce:author id="au8120" author-id="S0370269315010151-6ad8e1ac9a7b06f1b550a4ddf56de241"><ce:given-name>T.W.</ce:given-name><ce:surname>Snellman</ce:surname><ce:cross-ref refid="aff1230" id="crf8750"><ce:sup>123</ce:sup></ce:cross-ref></ce:author><ce:author id="au8130" 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author-id="S0370269315010151-657fdca353e29412dc258d4f8080fd5e"><ce:given-name>F.</ce:given-name><ce:surname>Soramel</ce:surname><ce:cross-ref refid="aff0300" id="crf8800"><ce:sup>30</ce:sup></ce:cross-ref></ce:author><ce:author id="au8180" author-id="S0370269315010151-08d0e06daec8127f6f7fd46b9d3ad98b"><ce:given-name>S.</ce:given-name><ce:surname>Sorensen</ce:surname><ce:cross-ref refid="aff1250" id="crf8810"><ce:sup>125</ce:sup></ce:cross-ref></ce:author><ce:author id="au8190" author-id="S0370269315010151-060f73dc170e1ee6653f543651bad3ad"><ce:given-name>F.</ce:given-name><ce:surname>Sozzi</ce:surname><ce:cross-ref refid="aff0960" id="crf8820"><ce:sup>96</ce:sup></ce:cross-ref></ce:author><ce:author id="au8200" author-id="S0370269315010151-df8c4c7b753f86c7c18d99f08dc64e7e"><ce:given-name>M.</ce:given-name><ce:surname>Spacek</ce:surname><ce:cross-ref refid="aff0400" id="crf8830"><ce:sup>40</ce:sup></ce:cross-ref></ce:author><ce:author id="au8210" 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author-id="S0370269315010151-9bbc6e85901f5a2aff91bd9e4c4af616"><ce:given-name>G.</ce:given-name><ce:surname>Trombetta</ce:surname><ce:cross-ref refid="aff0330" id="crf9290"><ce:sup>33</ce:sup></ce:cross-ref></ce:author><ce:author id="au8650" author-id="S0370269315010151-506889cabc7808922c96b983210184de"><ce:given-name>V.</ce:given-name><ce:surname>Trubnikov</ce:surname><ce:cross-ref refid="aff0030" id="crf9300"><ce:sup>3</ce:sup></ce:cross-ref></ce:author><ce:author id="au8660" author-id="S0370269315010151-e248aa646c1f5daa31a6d10f338f7b99"><ce:given-name>W.H.</ce:given-name><ce:surname>Trzaska</ce:surname><ce:cross-ref refid="aff1230" id="crf9310"><ce:sup>123</ce:sup></ce:cross-ref></ce:author><ce:author id="au8670" author-id="S0370269315010151-187d6f082ce2dde0d6a2c1d036819263"><ce:given-name>T.</ce:given-name><ce:surname>Tsuji</ce:surname><ce:cross-ref refid="aff1270" id="crf9320"><ce:sup>127</ce:sup></ce:cross-ref></ce:author><ce:author id="au8680" 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author-id="S0370269315010151-16744cdffdd2d05c4a90183baa267f56"><ce:given-name>A.</ce:given-name><ce:surname>Zimmermann</ce:surname><ce:cross-ref refid="aff0930" id="crf10530"><ce:sup>93</ce:sup></ce:cross-ref></ce:author><ce:author id="au9810" author-id="S0370269315010151-83f726d69156d0cdbbe02a363e9af585"><ce:given-name>M.B.</ce:given-name><ce:surname>Zimmermann</ce:surname><ce:cross-ref refid="aff0540" id="crf10540"><ce:sup>54</ce:sup></ce:cross-ref><ce:cross-ref refid="aff0360" id="crf10550"><ce:sup>36</ce:sup></ce:cross-ref></ce:author><ce:author id="au9820" author-id="S0370269315010151-2ad055472e2fac995111c51c08396d0c"><ce:given-name>G.</ce:given-name><ce:surname>Zinovjev</ce:surname><ce:cross-ref refid="aff0030" id="crf10560"><ce:sup>3</ce:sup></ce:cross-ref></ce:author><ce:author id="au9830" author-id="S0370269315010151-e89eb5f8577f69075c9476c1cf97ae8c"><ce:given-name>M.</ce:given-name><ce:surname>Zyzak</ce:surname><ce:cross-ref refid="aff0430" 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Alikhanyan National Science Laboratory (Yerevan Physics Institute) Foundation</sa:organization><sa:city>Yerevan</sa:city><sa:country>Armenia</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0020"><ce:label>2</ce:label><ce:textfn>Benemérita Universidad Autónoma de Puebla, Puebla, Mexico</ce:textfn><sa:affiliation><sa:organization>Benemérita Universidad Autónoma de Puebla</sa:organization><sa:city>Puebla</sa:city><sa:country>Mexico</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0030"><ce:label>3</ce:label><ce:textfn>Bogolyubov Institute for Theoretical Physics, Kiev, Ukraine</ce:textfn><sa:affiliation><sa:organization>Bogolyubov Institute for Theoretical Physics</sa:organization><sa:city>Kiev</sa:city><sa:country>Ukraine</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0040"><ce:label>4</ce:label><ce:textfn>Bose Institute, Department of Physics and Centre for Astroparticle Physics and Space Science (CAPSS), Kolkata, India</ce:textfn><sa:affiliation><sa:organization>Bose Institute</sa:organization><sa:organization>Department of Physics</sa:organization><sa:organization>Centre for Astroparticle Physics and Space Science (CAPSS)</sa:organization><sa:city>Kolkata</sa:city><sa:country>India</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0050"><ce:label>5</ce:label><ce:textfn>Budker Institute for Nuclear Physics, Novosibirsk, Russia</ce:textfn><sa:affiliation><sa:organization>Budker Institute for Nuclear Physics</sa:organization><sa:city>Novosibirsk</sa:city><sa:country>Russia</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0060"><ce:label>6</ce:label><ce:textfn>California Polytechnic State University, San Luis Obispo, CA, United States</ce:textfn><sa:affiliation><sa:organization>California Polytechnic State University</sa:organization><sa:city>San Luis Obispo</sa:city><sa:state>CA</sa:state><sa:country>United States</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0070"><ce:label>7</ce:label><ce:textfn>Central China Normal University, Wuhan, China</ce:textfn><sa:affiliation><sa:organization>Central China Normal University</sa:organization><sa:city>Wuhan</sa:city><sa:country>China</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0080"><ce:label>8</ce:label><ce:textfn>Centre de Calcul de l'IN2P3, Villeurbanne, France</ce:textfn><sa:affiliation><sa:organization>Centre de Calcul de l'IN2P3</sa:organization><sa:city>Villeurbanne</sa:city><sa:country>France</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0090"><ce:label>9</ce:label><ce:textfn>Centro de Aplicaciones Tecnológicas y Desarrollo Nuclear (CEADEN), Havana, Cuba</ce:textfn><sa:affiliation><sa:organization>Centro de Aplicaciones Tecnológicas y Desarrollo Nuclear (CEADEN)</sa:organization><sa:city>Havana</sa:city><sa:country>Cuba</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0100"><ce:label>10</ce:label><ce:textfn>Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Madrid, Spain</ce:textfn><sa:affiliation><sa:organization>Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT)</sa:organization><sa:city>Madrid</sa:city><sa:country>Spain</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0110"><ce:label>11</ce:label><ce:textfn>Centro de Investigación y de Estudios Avanzados (CINVESTAV), Mexico City and Mérida, Mexico</ce:textfn><sa:affiliation><sa:organization>Centro de Investigación y de Estudios Avanzados (CINVESTAV)</sa:organization><sa:city>Mexico City and Mérida</sa:city><sa:country>Mexico</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0120"><ce:label>12</ce:label><ce:textfn>Centro Fermi – Museo Storico della Fisica e Centro Studi e Ricerche “Enrico Fermi”, Rome, Italy</ce:textfn><sa:affiliation><sa:organization>Centro Fermi – Museo Storico della Fisica e Centro Studi e Ricerche “Enrico Fermi”</sa:organization><sa:city>Rome</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0130"><ce:label>13</ce:label><ce:textfn>Chicago State University, Chicago, IL, USA</ce:textfn><sa:affiliation><sa:organization>Chicago State University</sa:organization><sa:city>Chicago</sa:city><sa:state>IL</sa:state><sa:country>USA</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0140"><ce:label>14</ce:label><ce:textfn>China Institute of Atomic Energy, Beijing, China</ce:textfn><sa:affiliation><sa:organization>China Institute of Atomic Energy</sa:organization><sa:city>Beijing</sa:city><sa:country>China</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0150"><ce:label>15</ce:label><ce:textfn>Commissariat à l'Energie Atomique, IRFU, Saclay, France</ce:textfn><sa:affiliation><sa:organization>Commissariat à l'Energie Atomique</sa:organization><sa:organization>IRFU</sa:organization><sa:city>Saclay</sa:city><sa:country>France</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0160"><ce:label>16</ce:label><ce:textfn>COMSATS Institute of Information Technology (CIIT), Islamabad, Pakistan</ce:textfn><sa:affiliation><sa:organization>COMSATS Institute of Information Technology (CIIT)</sa:organization><sa:city>Islamabad</sa:city><sa:country>Pakistan</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0170"><ce:label>17</ce:label><ce:textfn>Departamento de Física de Partículas and IGFAE, Universidad de Santiago de Compostela, Santiago de Compostela, Spain</ce:textfn><sa:affiliation><sa:organization>Departamento de Física de Partículas</sa:organization><sa:organization>IGFAE</sa:organization><sa:organization>Universidad de Santiago de Compostela</sa:organization><sa:city>Santiago de Compostela</sa:city><sa:country>Spain</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0180"><ce:label>18</ce:label><ce:textfn>Department of Physics and Technology, University of Bergen, Bergen, Norway</ce:textfn><sa:affiliation><sa:organization>Department of Physics and Technology</sa:organization><sa:organization>University of Bergen</sa:organization><sa:city>Bergen</sa:city><sa:country>Norway</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0190"><ce:label>19</ce:label><ce:textfn>Department of Physics, Aligarh Muslim University, Aligarh, India</ce:textfn><sa:affiliation><sa:organization>Department of Physics</sa:organization><sa:organization>Aligarh Muslim University</sa:organization><sa:city>Aligarh</sa:city><sa:country>India</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0200"><ce:label>20</ce:label><ce:textfn>Department of Physics, Ohio State University, Columbus, OH, United States</ce:textfn><sa:affiliation><sa:organization>Department of Physics</sa:organization><sa:organization>Ohio State University</sa:organization><sa:city>Columbus</sa:city><sa:state>OH</sa:state><sa:country>United States</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0210"><ce:label>21</ce:label><ce:textfn>Department of Physics, Sejong University, Seoul, South Korea</ce:textfn><sa:affiliation><sa:organization>Department of Physics</sa:organization><sa:organization>Sejong University</sa:organization><sa:city>Seoul</sa:city><sa:country>South Korea</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0220"><ce:label>22</ce:label><ce:textfn>Department of Physics, University of Oslo, Oslo, Norway</ce:textfn><sa:affiliation><sa:organization>Department of Physics</sa:organization><sa:organization>University of Oslo</sa:organization><sa:city>Oslo</sa:city><sa:country>Norway</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0230"><ce:label>23</ce:label><ce:textfn>Dipartimento di Elettrotecnica ed Elettronica del Politecnico, Bari, Italy</ce:textfn><sa:affiliation><sa:organization>Dipartimento di Elettrotecnica ed Elettronica del Politecnico</sa:organization><sa:city>Bari</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0240"><ce:label>24</ce:label><ce:textfn>Dipartimento di Fisica dell'Università ‘La Sapienza’ and Sezione INFN Rome, Italy</ce:textfn><sa:affiliation><sa:organization>Dipartimento di Fisica dell'Università</sa:organization><sa:organization>‘La Sapienza’</sa:organization><sa:organization>Sezione INFN</sa:organization><sa:city>Rome</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0250"><ce:label>25</ce:label><ce:textfn>Dipartimento di Fisica dell'Università and Sezione INFN, Cagliari, Italy</ce:textfn><sa:affiliation><sa:organization>Dipartimento di Fisica dell'Università</sa:organization><sa:organization>Sezione INFN</sa:organization><sa:city>Cagliari</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0260"><ce:label>26</ce:label><ce:textfn>Dipartimento di Fisica dell'Università and Sezione INFN, Trieste, Italy</ce:textfn><sa:affiliation><sa:organization>Dipartimento di Fisica dell'Università</sa:organization><sa:organization>Sezione INFN</sa:organization><sa:city>Trieste</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0270"><ce:label>27</ce:label><ce:textfn>Dipartimento di Fisica dell'Università and Sezione INFN, Turin, Italy</ce:textfn><sa:affiliation><sa:organization>Dipartimento di Fisica dell'Università</sa:organization><sa:organization>Sezione INFN</sa:organization><sa:city>Turin</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0280"><ce:label>28</ce:label><ce:textfn>Dipartimento di Fisica e Astronomia dell'Università and Sezione INFN, Bologna, Italy</ce:textfn><sa:affiliation><sa:organization>Dipartimento di Fisica e Astronomia dell'Università</sa:organization><sa:organization>Sezione INFN</sa:organization><sa:city>Bologna</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0290"><ce:label>29</ce:label><ce:textfn>Dipartimento di Fisica e Astronomia dell'Università and Sezione INFN, Catania, Italy</ce:textfn><sa:affiliation><sa:organization>Dipartimento di Fisica e Astronomia dell'Università</sa:organization><sa:organization>Sezione INFN</sa:organization><sa:city>Catania</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0300"><ce:label>30</ce:label><ce:textfn>Dipartimento di Fisica e Astronomia dell'Università and Sezione INFN, Padova, Italy</ce:textfn><sa:affiliation><sa:organization>Dipartimento di Fisica e Astronomia dell'Università</sa:organization><sa:organization>Sezione INFN</sa:organization><sa:city>Padova</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0310"><ce:label>31</ce:label><ce:textfn>Dipartimento di Fisica ‘E.R. Caianiello’ dell'Università and Gruppo Collegato INFN, Salerno, Italy</ce:textfn><sa:affiliation><sa:organization>Dipartimento di Fisica ‘E.R. Caianiello’ dell'Università</sa:organization><sa:organization>Gruppo Collegato INFN</sa:organization><sa:city>Salerno</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0320"><ce:label>32</ce:label><ce:textfn>Dipartimento di Scienze e Innovazione Tecnologica dell'Università del Piemonte Orientale and Gruppo Collegato INFN, Alessandria, Italy</ce:textfn><sa:affiliation><sa:organization>Dipartimento di Scienze e Innovazione Tecnologica dell'Università del Piemonte Orientale</sa:organization><sa:organization>Gruppo Collegato INFN</sa:organization><sa:city>Alessandria</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0330"><ce:label>33</ce:label><ce:textfn>Dipartimento Interateneo di Fisica ‘M. Merlin’ and Sezione INFN, Bari, Italy</ce:textfn><sa:affiliation><sa:organization>Dipartimento Interateneo di Fisica ‘M. Merlin’</sa:organization><sa:organization>Sezione INFN</sa:organization><sa:city>Bari</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0340"><ce:label>34</ce:label><ce:textfn>Division of Experimental High Energy Physics, University of Lund, Lund, Sweden</ce:textfn><sa:affiliation><sa:organization>Division of Experimental High Energy Physics</sa:organization><sa:organization>University of Lund</sa:organization><sa:city>Lund</sa:city><sa:country>Sweden</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0350"><ce:label>35</ce:label><ce:textfn>Eberhard Karls Universität Tübingen, Tübingen, Germany</ce:textfn><sa:affiliation><sa:organization>Eberhard Karls Universität Tübingen</sa:organization><sa:city>Tübingen</sa:city><sa:country>Germany</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0360"><ce:label>36</ce:label><ce:textfn>European Organization for Nuclear Research (CERN), Geneva, Switzerland</ce:textfn><sa:affiliation><sa:organization>European Organization for Nuclear Research (CERN)</sa:organization><sa:city>Geneva</sa:city><sa:country>Switzerland</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0370"><ce:label>37</ce:label><ce:textfn>Excellence Cluster Universe, Technische Universität München, Munich, Germany</ce:textfn><sa:affiliation><sa:organization>Excellence Cluster Universe</sa:organization><sa:organization>Technische Universität München</sa:organization><sa:city>Munich</sa:city><sa:country>Germany</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0380"><ce:label>38</ce:label><ce:textfn>Faculty of Engineering, Bergen University College, Bergen, Norway</ce:textfn><sa:affiliation><sa:organization>Faculty of Engineering</sa:organization><sa:organization>Bergen University College</sa:organization><sa:city>Bergen</sa:city><sa:country>Norway</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0390"><ce:label>39</ce:label><ce:textfn>Faculty of Mathematics, Physics and Informatics, Comenius University, Bratislava, Slovakia</ce:textfn><sa:affiliation><sa:organization>Faculty of Mathematics, Physics and Informatics</sa:organization><sa:organization>Comenius University</sa:organization><sa:city>Bratislava</sa:city><sa:country>Slovakia</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0400"><ce:label>40</ce:label><ce:textfn>Faculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague, Prague, Czech Republic</ce:textfn><sa:affiliation><sa:organization>Faculty of Nuclear Sciences and Physical Engineering</sa:organization><sa:organization>Czech Technical University in Prague</sa:organization><sa:city>Prague</sa:city><sa:country>Czech Republic</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0410"><ce:label>41</ce:label><ce:textfn>Faculty of Science, P.J. Šafárik University, Košice, Slovakia</ce:textfn><sa:affiliation><sa:organization>Faculty of Science</sa:organization><sa:organization>P.J. Šafárik University</sa:organization><sa:city>Košice</sa:city><sa:country>Slovakia</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0420"><ce:label>42</ce:label><ce:textfn>Faculty of Technology, Buskerud and Vestfold University College, Vestfold, Norway</ce:textfn><sa:affiliation><sa:organization>Faculty of Technology</sa:organization><sa:organization>Buskerud and Vestfold University College</sa:organization><sa:city>Vestfold</sa:city><sa:country>Norway</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0430"><ce:label>43</ce:label><ce:textfn>Frankfurt Institute for Advanced Studies, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany</ce:textfn><sa:affiliation><sa:organization>Frankfurt Institute for Advanced Studies</sa:organization><sa:organization>Johann Wolfgang Goethe-Universität Frankfurt</sa:organization><sa:city>Frankfurt</sa:city><sa:country>Germany</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0440"><ce:label>44</ce:label><ce:textfn>Gangneung-Wonju National University, Gangneung, South Korea</ce:textfn><sa:affiliation><sa:organization>Gangneung-Wonju National University</sa:organization><sa:city>Gangneung</sa:city><sa:country>South Korea</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0450"><ce:label>45</ce:label><ce:textfn>Gauhati University, Department of Physics, Guwahati, India</ce:textfn><sa:affiliation><sa:organization>Gauhati University</sa:organization><sa:organization>Department of Physics</sa:organization><sa:city>Guwahati</sa:city><sa:country>India</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0460"><ce:label>46</ce:label><ce:textfn>Helsinki Institute of Physics (HIP), Helsinki, Finland</ce:textfn><sa:affiliation><sa:organization>Helsinki Institute of Physics (HIP)</sa:organization><sa:city>Helsinki</sa:city><sa:country>Finland</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0470"><ce:label>47</ce:label><ce:textfn>Hiroshima University, Hiroshima, Japan</ce:textfn><sa:affiliation><sa:organization>Hiroshima University</sa:organization><sa:city>Hiroshima</sa:city><sa:country>Japan</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0480"><ce:label>48</ce:label><ce:textfn>Indian Institute of Technology Bombay (IIT), Mumbai, India</ce:textfn><sa:affiliation><sa:organization>Indian Institute of Technology Bombay (IIT)</sa:organization><sa:city>Mumbai</sa:city><sa:country>India</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0490"><ce:label>49</ce:label><ce:textfn>Indian Institute of Technology Indore, Indore (IITI), India</ce:textfn><sa:affiliation><sa:organization>Indian Institute of Technology Indore</sa:organization><sa:city>Indore (IITI)</sa:city><sa:country>India</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0500"><ce:label>50</ce:label><ce:textfn>Inha University, Incheon, South Korea</ce:textfn><sa:affiliation><sa:organization>Inha University</sa:organization><sa:city>Incheon</sa:city><sa:country>South Korea</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0510"><ce:label>51</ce:label><ce:textfn>Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud, CNRS-IN2P3, Orsay, France</ce:textfn><sa:affiliation><sa:organization>Institut de Physique Nucléaire d'Orsay (IPNO)</sa:organization><sa:organization>Université Paris-Sud</sa:organization><sa:organization>CNRS-IN2P3</sa:organization><sa:city>Orsay</sa:city><sa:country>France</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0520"><ce:label>52</ce:label><ce:textfn>Institut für Informatik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany</ce:textfn><sa:affiliation><sa:organization>Institut für Informatik</sa:organization><sa:organization>Johann Wolfgang Goethe-Universität Frankfurt</sa:organization><sa:city>Frankfurt</sa:city><sa:country>Germany</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0530"><ce:label>53</ce:label><ce:textfn>Institut für Kernphysik, Johann Wolfgang Goethe-Universität Frankfurt, Frankfurt, Germany</ce:textfn><sa:affiliation><sa:organization>Institut für Kernphysik</sa:organization><sa:organization>Johann Wolfgang Goethe-Universität Frankfurt</sa:organization><sa:city>Frankfurt</sa:city><sa:country>Germany</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0540"><ce:label>54</ce:label><ce:textfn>Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, Münster, Germany</ce:textfn><sa:affiliation><sa:organization>Institut für Kernphysik</sa:organization><sa:organization>Westfälische Wilhelms-Universität Münster</sa:organization><sa:city>Münster</sa:city><sa:country>Germany</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0550"><ce:label>55</ce:label><ce:textfn>Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg, CNRS-IN2P3, Strasbourg, France</ce:textfn><sa:affiliation><sa:organization>Institut Pluridisciplinaire Hubert Curien (IPHC)</sa:organization><sa:organization>Université de Strasbourg</sa:organization><sa:organization>CNRS-IN2P3</sa:organization><sa:city>Strasbourg</sa:city><sa:country>France</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0560"><ce:label>56</ce:label><ce:textfn>Institute for Nuclear Research, Academy of Sciences, Moscow, Russia</ce:textfn><sa:affiliation><sa:organization>Institute for Nuclear Research</sa:organization><sa:organization>Academy of Sciences</sa:organization><sa:city>Moscow</sa:city><sa:country>Russia</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0570"><ce:label>57</ce:label><ce:textfn>Institute for Subatomic Physics of Utrecht University, Utrecht, Netherlands</ce:textfn><sa:affiliation><sa:organization>Institute for Subatomic Physics of Utrecht University</sa:organization><sa:city>Utrecht</sa:city><sa:country>Netherlands</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0580"><ce:label>58</ce:label><ce:textfn>Institute for Theoretical and Experimental Physics, Moscow, Russia</ce:textfn><sa:affiliation><sa:organization>Institute for Theoretical and Experimental Physics</sa:organization><sa:city>Moscow</sa:city><sa:country>Russia</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0590"><ce:label>59</ce:label><ce:textfn>Institute of Experimental Physics, Slovak Academy of Sciences, Košice, Slovakia</ce:textfn><sa:affiliation><sa:organization>Institute of Experimental Physics</sa:organization><sa:organization>Slovak Academy of Sciences</sa:organization><sa:city>Košice</sa:city><sa:country>Slovakia</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0600"><ce:label>60</ce:label><ce:textfn>Institute of Physics, Academy of Sciences of the Czech Republic, Prague, Czech Republic</ce:textfn><sa:affiliation><sa:organization>Institute of Physics</sa:organization><sa:organization>Academy of Sciences of the Czech Republic</sa:organization><sa:city>Prague</sa:city><sa:country>Czech Republic</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0610"><ce:label>61</ce:label><ce:textfn>Institute of Physics, Bhubaneswar, India</ce:textfn><sa:affiliation><sa:organization>Institute of Physics</sa:organization><sa:city>Bhubaneswar</sa:city><sa:country>India</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0620"><ce:label>62</ce:label><ce:textfn>Institute of Space Science (ISS), Bucharest, Romania</ce:textfn><sa:affiliation><sa:organization>Institute of Space Science (ISS)</sa:organization><sa:city>Bucharest</sa:city><sa:country>Romania</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0630"><ce:label>63</ce:label><ce:textfn>Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Mexico City, Mexico</ce:textfn><sa:affiliation><sa:organization>Instituto de Ciencias Nucleares</sa:organization><sa:organization>Universidad Nacional Autónoma de México</sa:organization><sa:city>Mexico City</sa:city><sa:country>Mexico</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0640"><ce:label>64</ce:label><ce:textfn>Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico</ce:textfn><sa:affiliation><sa:organization>Instituto de Física</sa:organization><sa:organization>Universidad Nacional Autónoma de México</sa:organization><sa:city>Mexico City</sa:city><sa:country>Mexico</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0650"><ce:label>65</ce:label><ce:textfn>iThemba LABS, National Research Foundation, Somerset West, South Africa</ce:textfn><sa:affiliation><sa:organization>iThemba LABS</sa:organization><sa:organization>National Research Foundation</sa:organization><sa:city>Somerset West</sa:city><sa:country>South Africa</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0660"><ce:label>66</ce:label><ce:textfn>Joint Institute for Nuclear Research (JINR), Dubna, Russia</ce:textfn><sa:affiliation><sa:organization>Joint Institute for Nuclear Research (JINR)</sa:organization><sa:city>Dubna</sa:city><sa:country>Russia</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0670"><ce:label>67</ce:label><ce:textfn>Konkuk University, Seoul, South Korea</ce:textfn><sa:affiliation><sa:organization>Konkuk University</sa:organization><sa:city>Seoul</sa:city><sa:country>South Korea</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0680"><ce:label>68</ce:label><ce:textfn>Korea Institute of Science and Technology Information, Daejeon, South Korea</ce:textfn><sa:affiliation><sa:organization>Korea Institute of Science and Technology Information</sa:organization><sa:city>Daejeon</sa:city><sa:country>South Korea</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0690"><ce:label>69</ce:label><ce:textfn>KTO Karatay University, Konya, Turkey</ce:textfn><sa:affiliation><sa:organization>KTO Karatay University</sa:organization><sa:city>Konya</sa:city><sa:country>Turkey</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0700"><ce:label>70</ce:label><ce:textfn>Laboratoire de Physique Corpusculaire (LPC), Clermont Université, Université Blaise Pascal, CNRS-IN2P3, Clermont-Ferrand, France</ce:textfn><sa:affiliation><sa:organization>Laboratoire de Physique Corpusculaire (LPC)</sa:organization><sa:organization>Clermont Université</sa:organization><sa:organization>Université Blaise Pascal</sa:organization><sa:organization>CNRS-IN2P3</sa:organization><sa:city>Clermont-Ferrand</sa:city><sa:country>France</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0710"><ce:label>71</ce:label><ce:textfn>Laboratoire de Physique Subatomique et de Cosmologie, Université Grenoble-Alpes, CNRS-IN2P3, Grenoble, France</ce:textfn><sa:affiliation><sa:organization>Laboratoire de Physique Subatomique et de Cosmologie</sa:organization><sa:organization>Université Grenoble-Alpes</sa:organization><sa:organization>CNRS-IN2P3</sa:organization><sa:city>Grenoble</sa:city><sa:country>France</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0720"><ce:label>72</ce:label><ce:textfn>Laboratori Nazionali di Frascati, INFN, Frascati, Italy</ce:textfn><sa:affiliation><sa:organization>Laboratori Nazionali di Frascati</sa:organization><sa:organization>INFN</sa:organization><sa:city>Frascati</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0730"><ce:label>73</ce:label><ce:textfn>Laboratori Nazionali di Legnaro, INFN, Legnaro, Italy</ce:textfn><sa:affiliation><sa:organization>Laboratori Nazionali di Legnaro</sa:organization><sa:organization>INFN</sa:organization><sa:city>Legnaro</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0740"><ce:label>74</ce:label><ce:textfn>Lawrence Berkeley National Laboratory, Berkeley, CA, United States</ce:textfn><sa:affiliation><sa:organization>Lawrence Berkeley National Laboratory</sa:organization><sa:city>Berkeley</sa:city><sa:state>CA</sa:state><sa:country>United States</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0750"><ce:label>75</ce:label><ce:textfn>Moscow Engineering Physics Institute, Moscow, Russia</ce:textfn><sa:affiliation><sa:organization>Moscow Engineering Physics Institute</sa:organization><sa:city>Moscow</sa:city><sa:country>Russia</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0760"><ce:label>76</ce:label><ce:textfn>Nagasaki Institute of Applied Science, Nagasaki, Japan</ce:textfn><sa:affiliation><sa:organization>Nagasaki Institute of Applied Science</sa:organization><sa:city>Nagasaki</sa:city><sa:country>Japan</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0770"><ce:label>77</ce:label><ce:textfn>National Centre for Nuclear Studies, Warsaw, Poland</ce:textfn><sa:affiliation><sa:organization>National Centre for Nuclear Studies</sa:organization><sa:city>Warsaw</sa:city><sa:country>Poland</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0780"><ce:label>78</ce:label><ce:textfn>National Institute for Physics and Nuclear Engineering, Bucharest, Romania</ce:textfn><sa:affiliation><sa:organization>National Institute for Physics and Nuclear Engineering</sa:organization><sa:city>Bucharest</sa:city><sa:country>Romania</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0790"><ce:label>79</ce:label><ce:textfn>National Institute of Science Education and Research, Bhubaneswar, India</ce:textfn><sa:affiliation><sa:organization>National Institute of Science Education and Research</sa:organization><sa:city>Bhubaneswar</sa:city><sa:country>India</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0800"><ce:label>80</ce:label><ce:textfn>Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark</ce:textfn><sa:affiliation><sa:organization>Niels Bohr Institute</sa:organization><sa:organization>University of Copenhagen</sa:organization><sa:city>Copenhagen</sa:city><sa:country>Denmark</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0810"><ce:label>81</ce:label><ce:textfn>Nikhef, Nationaal Instituut voor Subatomaire Fysica, Amsterdam, Netherlands</ce:textfn><sa:affiliation><sa:organization>Nikhef</sa:organization><sa:organization>Nationaal Instituut voor Subatomaire Fysica</sa:organization><sa:city>Amsterdam</sa:city><sa:country>Netherlands</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0820"><ce:label>82</ce:label><ce:textfn>Nuclear Physics Group, STFC Daresbury Laboratory, Daresbury, United Kingdom</ce:textfn><sa:affiliation><sa:organization>Nuclear Physics Group</sa:organization><sa:organization>STFC Daresbury Laboratory</sa:organization><sa:city>Daresbury</sa:city><sa:country>United Kingdom</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0830"><ce:label>83</ce:label><ce:textfn>Nuclear Physics Institute, Academy of Sciences of the Czech Republic, Řež u Prahy, Czech Republic</ce:textfn><sa:affiliation><sa:organization>Nuclear Physics Institute</sa:organization><sa:organization>Academy of Sciences of the Czech Republic</sa:organization><sa:city>Řež u Prahy</sa:city><sa:country>Czech Republic</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0840"><ce:label>84</ce:label><ce:textfn>Oak Ridge National Laboratory, Oak Ridge, TN, United States</ce:textfn><sa:affiliation><sa:organization>Oak Ridge National Laboratory</sa:organization><sa:city>Oak Ridge</sa:city><sa:state>TN</sa:state><sa:country>United States</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0850"><ce:label>85</ce:label><ce:textfn>Petersburg Nuclear Physics Institute, Gatchina, Russia</ce:textfn><sa:affiliation><sa:organization>Petersburg Nuclear Physics Institute</sa:organization><sa:city>Gatchina</sa:city><sa:country>Russia</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0860"><ce:label>86</ce:label><ce:textfn>Physics Department, Creighton University, Omaha, NE, United States</ce:textfn><sa:affiliation><sa:organization>Physics Department</sa:organization><sa:organization>Creighton University</sa:organization><sa:city>Omaha</sa:city><sa:state>NE</sa:state><sa:country>United States</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0870"><ce:label>87</ce:label><ce:textfn>Physics Department, Panjab University, Chandigarh, India</ce:textfn><sa:affiliation><sa:organization>Physics Department</sa:organization><sa:organization>Panjab University</sa:organization><sa:city>Chandigarh</sa:city><sa:country>India</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0880"><ce:label>88</ce:label><ce:textfn>Physics Department, University of Athens, Athens, Greece</ce:textfn><sa:affiliation><sa:organization>Physics Department</sa:organization><sa:organization>University of Athens</sa:organization><sa:city>Athens</sa:city><sa:country>Greece</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0890"><ce:label>89</ce:label><ce:textfn>Physics Department, University of Cape Town, Cape Town, South Africa</ce:textfn><sa:affiliation><sa:organization>Physics Department</sa:organization><sa:organization>University of Cape Town</sa:organization><sa:city>Cape Town</sa:city><sa:country>South Africa</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0900"><ce:label>90</ce:label><ce:textfn>Physics Department, University of Jammu, Jammu, India</ce:textfn><sa:affiliation><sa:organization>Physics Department</sa:organization><sa:organization>University of Jammu</sa:organization><sa:city>Jammu</sa:city><sa:country>India</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0910"><ce:label>91</ce:label><ce:textfn>Physics Department, University of Rajasthan, Jaipur, India</ce:textfn><sa:affiliation><sa:organization>Physics Department</sa:organization><sa:organization>University of Rajasthan</sa:organization><sa:city>Jaipur</sa:city><sa:country>India</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0920"><ce:label>92</ce:label><ce:textfn>Physik Department, Technische Universität München, Munich, Germany</ce:textfn><sa:affiliation><sa:organization>Physik Department</sa:organization><sa:organization>Technische Universität München</sa:organization><sa:city>Munich</sa:city><sa:country>Germany</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0930"><ce:label>93</ce:label><ce:textfn>Physikalisches Institut, Ruprecht-Karls-Universität Heidelberg, Heidelberg, Germany</ce:textfn><sa:affiliation><sa:organization>Physikalisches Institut</sa:organization><sa:organization>Ruprecht-Karls-Universität Heidelberg</sa:organization><sa:city>Heidelberg</sa:city><sa:country>Germany</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0940"><ce:label>94</ce:label><ce:textfn>Purdue University, West Lafayette, IN, United States</ce:textfn><sa:affiliation><sa:organization>Purdue University</sa:organization><sa:city>West Lafayette</sa:city><sa:state>IN</sa:state><sa:country>United States</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0950"><ce:label>95</ce:label><ce:textfn>Pusan National University, Pusan, South Korea</ce:textfn><sa:affiliation><sa:organization>Pusan National University</sa:organization><sa:city>Pusan</sa:city><sa:country>South Korea</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0960"><ce:label>96</ce:label><ce:textfn>Research Division and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, Germany</ce:textfn><sa:affiliation><sa:organization>Research Division</sa:organization><sa:organization>ExtreMe Matter Institute EMMI</sa:organization><sa:organization>GSI Helmholtzzentrum für Schwerionenforschung</sa:organization><sa:city>Darmstadt</sa:city><sa:country>Germany</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0970"><ce:label>97</ce:label><ce:textfn>Rudjer Bošković Institute, Zagreb, Croatia</ce:textfn><sa:affiliation><sa:organization>Rudjer Bošković Institute</sa:organization><sa:city>Zagreb</sa:city><sa:country>Croatia</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0980"><ce:label>98</ce:label><ce:textfn>Russian Federal Nuclear Center (VNIIEF), Sarov, Russia</ce:textfn><sa:affiliation><sa:organization>Russian Federal Nuclear Center (VNIIEF)</sa:organization><sa:city>Sarov</sa:city><sa:country>Russia</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff0990"><ce:label>99</ce:label><ce:textfn>Russian Research Centre Kurchatov Institute, Moscow, Russia</ce:textfn><sa:affiliation><sa:organization>Russian Research Centre Kurchatov Institute</sa:organization><sa:city>Moscow</sa:city><sa:country>Russia</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1000"><ce:label>100</ce:label><ce:textfn>Saha Institute of Nuclear Physics, Kolkata, India</ce:textfn><sa:affiliation><sa:organization>Saha Institute of Nuclear Physics</sa:organization><sa:city>Kolkata</sa:city><sa:country>India</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1010"><ce:label>101</ce:label><ce:textfn>School of Physics and Astronomy, University of Birmingham, Birmingham, United Kingdom</ce:textfn><sa:affiliation><sa:organization>School of Physics and Astronomy</sa:organization><sa:organization>University of Birmingham</sa:organization><sa:city>Birmingham</sa:city><sa:country>United Kingdom</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1020"><ce:label>102</ce:label><ce:textfn>Sección Física, Departamento de Ciencias, Pontificia Universidad Católica del Perú, Lima, Peru</ce:textfn><sa:affiliation><sa:organization>Sección Física</sa:organization><sa:organization>Departamento de Ciencias</sa:organization><sa:organization>Pontificia Universidad Católica del Perú</sa:organization><sa:city>Lima</sa:city><sa:country>Peru</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1030"><ce:label>103</ce:label><ce:textfn>Sezione INFN, Bari, Italy</ce:textfn><sa:affiliation><sa:organization>Sezione INFN</sa:organization><sa:city>Bari</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1040"><ce:label>104</ce:label><ce:textfn>Sezione INFN, Bologna, Italy</ce:textfn><sa:affiliation><sa:organization>Sezione INFN</sa:organization><sa:city>Bologna</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1050"><ce:label>105</ce:label><ce:textfn>Sezione INFN, Cagliari, Italy</ce:textfn><sa:affiliation><sa:organization>Sezione INFN</sa:organization><sa:city>Cagliari</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1060"><ce:label>106</ce:label><ce:textfn>Sezione INFN, Catania, Italy</ce:textfn><sa:affiliation><sa:organization>Sezione INFN</sa:organization><sa:city>Catania</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1070"><ce:label>107</ce:label><ce:textfn>Sezione INFN, Padova, Italy</ce:textfn><sa:affiliation><sa:organization>Sezione INFN</sa:organization><sa:city>Padova</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1080"><ce:label>108</ce:label><ce:textfn>Sezione INFN, Rome, Italy</ce:textfn><sa:affiliation><sa:organization>Sezione INFN</sa:organization><sa:city>Rome</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1090"><ce:label>109</ce:label><ce:textfn>Sezione INFN, Trieste, Italy</ce:textfn><sa:affiliation><sa:organization>Sezione INFN</sa:organization><sa:city>Trieste</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1100"><ce:label>110</ce:label><ce:textfn>Sezione INFN, Turin, Italy</ce:textfn><sa:affiliation><sa:organization>Sezione INFN</sa:organization><sa:city>Turin</sa:city><sa:country>Italy</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1110"><ce:label>111</ce:label><ce:textfn>SSC IHEP of NRC Kurchatov institute, Protvino, Russia</ce:textfn><sa:affiliation><sa:organization>SSC IHEP of NRC Kurchatov institute</sa:organization><sa:city>Protvino</sa:city><sa:country>Russia</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1120"><ce:label>112</ce:label><ce:textfn>Stefan Meyer Institut für Subatomare Physik (SMI), Vienna, Austria</ce:textfn><sa:affiliation><sa:organization>Stefan Meyer Institut für Subatomare Physik (SMI)</sa:organization><sa:city>Vienna</sa:city><sa:country>Austria</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1130"><ce:label>113</ce:label><ce:textfn>SUBATECH, Ecole des Mines de Nantes, Université de Nantes, CNRS-IN2P3, Nantes, France</ce:textfn><sa:affiliation><sa:organization>SUBATECH</sa:organization><sa:organization>Ecole des Mines de Nantes</sa:organization><sa:organization>Université de Nantes</sa:organization><sa:organization>CNRS-IN2P3</sa:organization><sa:city>Nantes</sa:city><sa:country>France</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1140"><ce:label>114</ce:label><ce:textfn>Suranaree University of Technology, Nakhon Ratchasima, Thailand</ce:textfn><sa:affiliation><sa:organization>Suranaree University of Technology</sa:organization><sa:city>Nakhon Ratchasima</sa:city><sa:country>Thailand</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1150"><ce:label>115</ce:label><ce:textfn>Technical University of Košice, Košice, Slovakia</ce:textfn><sa:affiliation><sa:organization>Technical University of Košice</sa:organization><sa:city>Košice</sa:city><sa:country>Slovakia</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1160"><ce:label>116</ce:label><ce:textfn>Technical University of Split FESB, Split, Croatia</ce:textfn><sa:affiliation><sa:organization>Technical University of Split FESB</sa:organization><sa:city>Split</sa:city><sa:country>Croatia</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1170"><ce:label>117</ce:label><ce:textfn>The Henryk Niewodniczanski Institute of Nuclear Physics, Polish Academy of Sciences, Cracow, Poland</ce:textfn><sa:affiliation><sa:organization>The Henryk Niewodniczanski Institute of Nuclear Physics</sa:organization><sa:organization>Polish Academy of Sciences</sa:organization><sa:city>Cracow</sa:city><sa:country>Poland</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1180"><ce:label>118</ce:label><ce:textfn>The University of Texas at Austin, Physics Department, Austin, TX, USA</ce:textfn><sa:affiliation><sa:organization>The University of Texas at Austin</sa:organization><sa:organization>Physics Department</sa:organization><sa:city>Austin</sa:city><sa:state>TX</sa:state><sa:country>USA</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1190"><ce:label>119</ce:label><ce:textfn>Universidad Autónoma de Sinaloa, Culiacán, Mexico</ce:textfn><sa:affiliation><sa:organization>Universidad Autónoma de Sinaloa</sa:organization><sa:city>Culiacán</sa:city><sa:country>Mexico</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1200"><ce:label>120</ce:label><ce:textfn>Universidade de São Paulo (USP), São Paulo, Brazil</ce:textfn><sa:affiliation><sa:organization>Universidade de São Paulo (USP)</sa:organization><sa:city>São Paulo</sa:city><sa:country>Brazil</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1210"><ce:label>121</ce:label><ce:textfn>Universidade Estadual de Campinas (UNICAMP), Campinas, Brazil</ce:textfn><sa:affiliation><sa:organization>Universidade Estadual de Campinas (UNICAMP)</sa:organization><sa:city>Campinas</sa:city><sa:country>Brazil</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1220"><ce:label>122</ce:label><ce:textfn>University of Houston, Houston, TX, United States</ce:textfn><sa:affiliation><sa:organization>University of Houston</sa:organization><sa:city>Houston</sa:city><sa:state>TX</sa:state><sa:country>United States</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1230"><ce:label>123</ce:label><ce:textfn>University of Jyväskylä, Jyväskylä, Finland</ce:textfn><sa:affiliation><sa:organization>University of Jyväskylä</sa:organization><sa:city>Jyväskylä</sa:city><sa:country>Finland</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1240"><ce:label>124</ce:label><ce:textfn>University of Liverpool, Liverpool, United Kingdom</ce:textfn><sa:affiliation><sa:organization>University of Liverpool</sa:organization><sa:city>Liverpool</sa:city><sa:country>United Kingdom</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1250"><ce:label>125</ce:label><ce:textfn>University of Tennessee, Knoxville, TN, United States</ce:textfn><sa:affiliation><sa:organization>University of Tennessee</sa:organization><sa:city>Knoxville</sa:city><sa:state>TN</sa:state><sa:country>United States</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1260"><ce:label>126</ce:label><ce:textfn>University of the Witwatersrand, Johannesburg, South Africa</ce:textfn><sa:affiliation><sa:organization>University of the Witwatersrand</sa:organization><sa:city>Johannesburg</sa:city><sa:country>South Africa</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1270"><ce:label>127</ce:label><ce:textfn>University of Tokyo, Tokyo, Japan</ce:textfn><sa:affiliation><sa:organization>University of Tokyo</sa:organization><sa:city>Tokyo</sa:city><sa:country>Japan</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1280"><ce:label>128</ce:label><ce:textfn>University of Tsukuba, Tsukuba, Japan</ce:textfn><sa:affiliation><sa:organization>University of Tsukuba</sa:organization><sa:city>Tsukuba</sa:city><sa:country>Japan</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1290"><ce:label>129</ce:label><ce:textfn>University of Zagreb, Zagreb, Croatia</ce:textfn><sa:affiliation><sa:organization>University of Zagreb</sa:organization><sa:city>Zagreb</sa:city><sa:country>Croatia</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1300"><ce:label>130</ce:label><ce:textfn>Université de Lyon, Université Lyon 1, CNRS/IN2P3, IPN-Lyon, Villeurbanne, France</ce:textfn><sa:affiliation><sa:organization>Université de Lyon</sa:organization><sa:organization>Université Lyon 1</sa:organization><sa:organization>CNRS/IN2P3</sa:organization><sa:organization>IPN-Lyon</sa:organization><sa:city>Villeurbanne</sa:city><sa:country>France</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1310"><ce:label>131</ce:label><ce:textfn>V. Fock Institute for Physics, St. Petersburg State University, St. Petersburg, Russia</ce:textfn><sa:affiliation><sa:organization>V. Fock Institute for Physics</sa:organization><sa:organization>St. Petersburg State University</sa:organization><sa:city>St. Petersburg</sa:city><sa:country>Russia</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1320"><ce:label>132</ce:label><ce:textfn>Variable Energy Cyclotron Centre, Kolkata, India</ce:textfn><sa:affiliation><sa:organization>Variable Energy Cyclotron Centre</sa:organization><sa:city>Kolkata</sa:city><sa:country>India</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1330"><ce:label>133</ce:label><ce:textfn>Warsaw University of Technology, Warsaw, Poland</ce:textfn><sa:affiliation><sa:organization>Warsaw University of Technology</sa:organization><sa:city>Warsaw</sa:city><sa:country>Poland</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1340"><ce:label>134</ce:label><ce:textfn>Wayne State University, Detroit, MI, United States</ce:textfn><sa:affiliation><sa:organization>Wayne State University</sa:organization><sa:city>Detroit</sa:city><sa:state>MI</sa:state><sa:country>United States</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1350"><ce:label>135</ce:label><ce:textfn>Wigner Research Centre for Physics, Hungarian Academy of Sciences, Budapest, Hungary</ce:textfn><sa:affiliation><sa:organization>Wigner Research Centre for Physics</sa:organization><sa:organization>Hungarian Academy of Sciences</sa:organization><sa:city>Budapest</sa:city><sa:country>Hungary</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1360"><ce:label>136</ce:label><ce:textfn>Yale University, New Haven, CT, United States</ce:textfn><sa:affiliation><sa:organization>Yale University</sa:organization><sa:city>New Haven</sa:city><sa:state>CT</sa:state><sa:country>United States</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1370"><ce:label>137</ce:label><ce:textfn>Yonsei University, Seoul, South Korea</ce:textfn><sa:affiliation><sa:organization>Yonsei University</sa:organization><sa:city>Seoul</sa:city><sa:country>South Korea</sa:country></sa:affiliation></ce:affiliation><ce:affiliation id="aff1380"><ce:label>138</ce:label><ce:textfn>Zentrum für Technologietransfer und Telekommunikation (ZTT), Fachhochschule Worms, Worms, Germany</ce:textfn><sa:affiliation><sa:organization>Zentrum für Technologietransfer und Telekommunikation (ZTT)</sa:organization><sa:organization>Fachhochschule Worms</sa:organization><sa:city>Worms</sa:city><sa:country>Germany</sa:country></sa:affiliation></ce:affiliation><ce:footnote id="fn0010"><ce:label>i</ce:label><ce:note-para id="np0010">Deceased.</ce:note-para></ce:footnote><ce:footnote id="fn0020"><ce:label>ii</ce:label><ce:note-para id="np0020">Also at: Georgia State University, Atlanta, Georgia, United States.</ce:note-para></ce:footnote><ce:footnote id="fn0030"><ce:label>iii</ce:label><ce:note-para id="np0030">Also at: M.V. Lomonosov Moscow State University, D.V. Skobeltsyn Institute of Nuclear, Physics, Moscow, Russia.</ce:note-para></ce:footnote></ce:author-group></ce:collaboration><ce:footnote id="fn0040"><ce:label>⋆</ce:label><ce:note-para id="np0040"><ce:italic>E-mail address:</ce:italic> <ce:inter-ref xlink:role="http://www.elsevier.com/xml/linking-roles/text/html" xlink:href="mailto:alice-publications@cern.ch" id="inf0010">alice-publications@cern.ch</ce:inter-ref>.</ce:note-para></ce:footnote></ce:author-group><ce:date-received day="12" month="10" year="2015"/><ce:date-revised day="12" month="11" year="2015"/><ce:date-accepted day="21" month="12" year="2015"/><ce:miscellaneous id="ms0010">Editor: L. Rolandi</ce:miscellaneous><ce:abstract id="ab0010"><ce:section-title id="st0010">Abstract</ce:section-title><ce:abstract-sec id="as0010"><ce:simple-para id="sp0070">The production of electrons from heavy-flavour hadron decays was measured as a function of transverse momentum (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>) in minimum-bias p–Pb collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif"><mml:msqrt><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">NN</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>5.02</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> using the ALICE detector at the LHC. The measurement covers the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> interval <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si117.gif"><mml:mn>0.5</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>12</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> and the rapidity range <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si129.gif"><mml:mo>−</mml:mo><mml:mn>1.065</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>y</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">cms</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>0.135</mml:mn></mml:math> in the centre-of-mass reference frame. The contribution of electrons from background sources was subtracted using an invariant mass approach. The nuclear modification factor <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si114.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pPb</mml:mi></mml:mrow></mml:msub></mml:math> was calculated by comparing the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>-differential invariant cross section in p–Pb collisions to a pp reference at the same centre-of-mass energy, which was obtained by interpolating measurements at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si116.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>2.76</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si126.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>7</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math>. The <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si114.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pPb</mml:mi></mml:mrow></mml:msub></mml:math> is consistent with unity within uncertainties of about 25%, which become larger for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> below <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si10.gif"><mml:mn>1</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>. The measurement shows that heavy-flavour production is consistent with binary scaling, so that a suppression in the high-<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> yield in Pb–Pb collisions has to be attributed to effects induced by the hot medium produced in the final state. The data in p–Pb collisions are described by recent model calculations that include cold nuclear matter effects.</ce:simple-para></ce:abstract-sec></ce:abstract></head><body><ce:sections><ce:section id="se0010" role="introduction"><ce:label>1</ce:label><ce:section-title id="st0020">Introduction</ce:section-title><ce:para id="pr0010">The Quark-Gluon Plasma (QGP) <ce:cross-refs refid="br0010 br0020" id="crs0020">[1,2]</ce:cross-refs>, a colour-deconfined state of strongly-interacting matter, is predicted to exist at high temperature according to lattice Quantum Chromodynamics (QCD) calculations <ce:cross-ref refid="br0030" id="crf10580">[3]</ce:cross-ref>. These conditions can be reached in ultra-relativistic heavy-ion collisions <ce:cross-refs refid="br0040 br0050 br0060 br0070 br0080 br0090 br0100" id="crs0030">[4–10]</ce:cross-refs>. Charm and beauty (heavy-flavour) quarks are mostly produced in initial hard scattering processes on a very short time scale, shorter than the formation time of the QGP medium <ce:cross-ref refid="br0110" id="crf10590">[11]</ce:cross-ref>, and thus experience the full temporal and spatial evolution of the collision. While interacting with the QGP medium, heavy quarks lose energy via elastic and radiative processes <ce:cross-refs refid="br0120 br0130 br0140" id="crs0040">[12–14]</ce:cross-refs>. Heavy-flavour hadrons are therefore well-suited probes to study the properties of the QGP. The effect of energy loss on heavy-flavour production can be characterised via the nuclear modification factor (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si11.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">AA</mml:mi></mml:mrow></mml:msub></mml:math>) of heavy-flavour hadrons. The <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si11.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">AA</mml:mi></mml:mrow></mml:msub></mml:math> is defined as the ratio of the heavy-flavour hadron yield in nucleus–nucleus (A–A) collisions to that in proton–proton (pp) collisions scaled by the average number of binary nucleon–nucleon collisions. The <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si11.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">AA</mml:mi></mml:mrow></mml:msub></mml:math> is studied differentially as a function of transverse momentum (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>), rapidity (<ce:italic>y</ce:italic>) and collision centrality. It was measured at the Relativistic Heavy Ion Collider (RHIC) <ce:cross-refs refid="br0150 br0160 br0170 br0180" id="crs0050">[15–18]</ce:cross-refs> and at the Large Hadron Collider (LHC) <ce:cross-refs refid="br0190 br0200 br0210 br0220" id="crs0060">[19–22]</ce:cross-refs>. At RHIC, in central Au–Au collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si12.gif"><mml:msqrt><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">NN</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>200</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext></mml:math> the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si11.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">AA</mml:mi></mml:mrow></mml:msub></mml:math> of charmed mesons and of electrons from heavy-flavour hadron decays shows that their production is strongly suppressed by a factor of about 5 for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si13.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&gt;</mml:mo><mml:mn>3</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> at mid-rapidity. For the most central Pb–Pb collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si14.gif"><mml:msqrt><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">NN</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>2.76</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> at the LHC, a suppression by a factor of 5–6 is observed for charmed mesons for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si15.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&gt;</mml:mo><mml:mn>5</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> at mid-rapidity <ce:cross-ref refid="br0220" id="crf10600">[22]</ce:cross-ref>.</ce:para><ce:para id="pr0020">The interpretation of the measurements in A–A collisions requires the study of heavy-flavour production in p–A collisions, which provides access to cold nuclear matter (CNM) effects. These effects are not related to the formation of a colour-deconfined medium, but are present in case of colliding nuclei (or proton–nucleus). An important CNM effect in the initial state is parton-density shadowing or saturation, which can be described using modified parton distribution functions (PDF) in the nucleus <ce:cross-ref refid="br0230" id="crf10610">[23]</ce:cross-ref> or using the Color Glass Condensate (CGC) effective theory <ce:cross-ref refid="br0240" id="crf10620">[24]</ce:cross-ref>. Further CNM effects include energy loss <ce:cross-ref refid="br0250" id="crf10630">[25]</ce:cross-ref> in the initial and final states and a Cronin-like enhancement <ce:cross-ref refid="br0260" id="crf10640">[26]</ce:cross-ref> as a consequence of multiple scatterings <ce:cross-refs refid="br0250 br0270" id="crs0070">[25,27]</ce:cross-refs>.</ce:para><ce:para id="pr0030">The influence of the CNM effects can be studied by measuring the nuclear modification factor <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si16.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pA</mml:mi></mml:mrow></mml:msub></mml:math>. Like the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si11.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">AA</mml:mi></mml:mrow></mml:msub></mml:math>, the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si16.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pA</mml:mi></mml:mrow></mml:msub></mml:math> is defined such that it is unity if there are no nuclear effects. For minimum-bias p–A collisions, it can be expressed as <ce:cross-ref refid="br0280" id="crf10650">[28]</ce:cross-ref><ce:display><ce:formula id="fm0010"><ce:label>(1)</ce:label><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si17.gif"><mml:mrow><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pA</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mfrac><mml:mn>1</mml:mn><mml:mi>A</mml:mi></mml:mfrac><mml:mfrac><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pA</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">/</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pp</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">/</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac><mml:mtext> </mml:mtext><mml:mo>,</mml:mo></mml:mrow></mml:math></ce:formula></ce:display> where <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si18.gif"><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pA</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">/</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si19.gif"><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pp</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">/</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> are the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>-differential production cross sections of a given particle species in p–A and pp collisions, respectively, and <ce:italic>A</ce:italic> is the number of nucleons in the nucleus.</ce:para><ce:para id="pr0040">Cold nuclear matter effects were recently investigated at the RHIC and the LHC <ce:cross-refs refid="br0290 br0300 br0310 br0320 br0330 br0340 br0350 br0360 br0370 br0380 br0390 br0400 br0410 br0420 br0430 br0440" id="crs0080">[29–44]</ce:cross-refs>. At RHIC, the nuclear modification factor of electrons from heavy-flavour hadron decays in central d–Au collisions (0–20%) at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si12.gif"><mml:msqrt><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">NN</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>200</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext></mml:math> is larger than unity at mid-rapidity in the transverse momentum interval <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si20.gif"><mml:mn>1.5</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>5</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> <ce:cross-ref refid="br0420" id="crf10660">[42]</ce:cross-ref>. The corresponding measurement for muons from heavy-flavour hadron decays in central d–Au collisions shows a suppression at forward rapidity and an enhancement at backward rapidity <ce:cross-ref refid="br0430" id="crf10670">[43]</ce:cross-ref>. Theoretical models that include the modification of the PDF in the nucleus can neither explain the enhancement nor the large difference between forward and backward rapidity. Possible explanations include the Cronin-like enhancement <ce:cross-ref refid="br0260" id="crf10680">[26]</ce:cross-ref> due to radial flow of heavy mesons <ce:cross-ref refid="br0450" id="crf10690">[45]</ce:cross-ref>. At the LHC, the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>-differential nuclear modification factor <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si114.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pPb</mml:mi></mml:mrow></mml:msub></mml:math> of D mesons measured in p–Pb collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif"><mml:msqrt><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">NN</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>5.02</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> <ce:cross-ref refid="br0440" id="crf10700">[44]</ce:cross-ref> is consistent with unity for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si21.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&gt;</mml:mo><mml:mn>1</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> and is described by theoretical calculations that include gluon saturation effects. Both at RHIC and at the LHC, the p/d–A measurements indicate that initial-state effects alone cannot explain the strong suppression seen at high-<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> in nucleus–nucleus collisions.</ce:para><ce:para id="pr0050">In this Letter, the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>-differential invariant cross section and the nuclear modification factor <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si114.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pPb</mml:mi></mml:mrow></mml:msub></mml:math> of electrons from heavy-flavour hadron decays measured in minimum-bias p–Pb collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif"><mml:msqrt><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">NN</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>5.02</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> with ALICE at the LHC are presented. The measurement covers the rapidity range <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si129.gif"><mml:mo>−</mml:mo><mml:mn>1.065</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>y</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">cms</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>0.135</mml:mn></mml:math> in the centre-of-mass system (cms) for electrons with transverse momentum <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si117.gif"><mml:mn>0.5</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>12</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>. This rapidity coverage results from the same rigidity of the p and Pb beams at the LHC, leading to a rapidity shift of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si23.gif"><mml:mo stretchy="false">|</mml:mo><mml:msub><mml:mrow><mml:mi>y</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">NN</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">|</mml:mo><mml:mo>=</mml:mo><mml:mn>0.465</mml:mn></mml:math> between the nucleon–nucleon cms and the laboratory reference frame, in the direction of the p beam. At low <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>, the measurement probes the production of charm-hadron decays <ce:cross-ref refid="br0460" id="crf10710">[46]</ce:cross-ref>, providing sensitivity to the gluon PDF in the regime of Bjorken-<ce:italic>x</ce:italic> of the order of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si24.gif"><mml:msup><mml:mrow><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mo>−</mml:mo><mml:mn>4</mml:mn></mml:mrow></mml:msup></mml:math> <ce:cross-ref refid="br0470" id="crf10720">[47]</ce:cross-ref>, where a substantial shadowing effect is expected <ce:cross-ref refid="br0480" id="crf10730">[48]</ce:cross-ref>.</ce:para><ce:para id="pr0060">To obtain the nuclear modification factor <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si114.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pPb</mml:mi></mml:mrow></mml:msub></mml:math> of electrons from heavy-flavour hadron decays, the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>-differential invariant cross section in p–Pb collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif"><mml:msqrt><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">NN</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>5.02</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> was compared to a pp reference multiplied by 208, the Pb mass number. The pp reference was obtained by interpolating the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>-differential cross section measurements at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si116.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>2.76</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> and 7 TeV.</ce:para><ce:para id="pr0070">The Letter is organised as follows. The experimental apparatus, data sample and event selection are described in Section <ce:cross-ref refid="se0020" id="crf10740">2</ce:cross-ref>. The electron reconstruction strategy and the pp reference spectrum are explained in Sections <ce:cross-ref refid="se0030" id="crf10750">3</ce:cross-ref> and <ce:cross-ref refid="se0040" id="crf10760">4</ce:cross-ref>, respectively. The measured <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>-differential invariant cross section, the nuclear modification factor <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si114.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pPb</mml:mi></mml:mrow></mml:msub></mml:math> of electrons from heavy-flavour hadron decays and comparison of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si114.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pPb</mml:mi></mml:mrow></mml:msub></mml:math> to model calculations are reported in Section <ce:cross-ref refid="se0050" id="crf10770">5</ce:cross-ref>.</ce:para></ce:section><ce:section id="se0020"><ce:label>2</ce:label><ce:section-title id="st0030">Experimental apparatus, data sample and event selection</ce:section-title><ce:para id="pr0080">A detailed description of the ALICE apparatus can be found in <ce:cross-refs refid="br0490 br0500" id="crs0090">[49,50]</ce:cross-refs>. Electrons are reconstructed at mid-rapidity using the central barrel detectors (described below) located inside a solenoid magnet, which generates a magnetic field <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si26.gif"><mml:mi mathvariant="normal">B</mml:mi><mml:mo>=</mml:mo><mml:mn>0.5</mml:mn><mml:mtext> </mml:mtext><mml:mtext>T</mml:mtext></mml:math> along the beam direction.</ce:para><ce:para id="pr0090">The Inner Tracking System (ITS), the closest detector to the interaction point, includes six cylindrical layers of silicon detectors with three different technologies (pixel, drift and strip) at radii between 3.9 cm and 43 cm with a pseudorapidity coverage in the laboratory reference frame in the full azimuth between <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si27.gif"><mml:mo stretchy="false">|</mml:mo><mml:msub><mml:mrow><mml:mi>η</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">lab</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo></mml:math> 2.0 at small radii and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si27.gif"><mml:mo stretchy="false">|</mml:mo><mml:msub><mml:mrow><mml:mi>η</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">lab</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo></mml:math> 0.9 at large radii <ce:cross-refs refid="br0490 br0510" id="crs0100">[49,51]</ce:cross-refs>. The two innermost layers form the Silicon Pixel Detector (SPD), which plays a key role in primary and secondary vertex reconstruction. At an incident angle perpendicular to the detector surfaces, the total material budget of the ITS corresponds on average to 7.7% of a radiation length <ce:cross-ref refid="br0510" id="crf10780">[51]</ce:cross-ref>. The main tracking device in the central barrel is the Time Projection Chamber (TPC) <ce:cross-ref refid="br0520" id="crf10790">[52]</ce:cross-ref>, which surrounds the ITS and covers a pseudorapidity range of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si27.gif"><mml:mo stretchy="false">|</mml:mo><mml:msub><mml:mrow><mml:mi>η</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">lab</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo></mml:math> 0.9 in the full azimuth. The track reconstruction proceeds inward from the outer radius of the TPC to the innermost layer of the ITS <ce:cross-ref refid="br0500" id="crf10800">[50]</ce:cross-ref>. The TPC provides particle identification via the measurement of the specific energy loss <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si29.gif"><mml:mi mathvariant="normal">d</mml:mi><mml:mi>E</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:mi>x</mml:mi></mml:math>. The Time-Of-Flight array (TOF), based on Multi-gap Resistive Plate Chambers, covers the full azimuth and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si27.gif"><mml:mo stretchy="false">|</mml:mo><mml:msub><mml:mrow><mml:mi>η</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">lab</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo></mml:math> 0.9 at a radial distance of 3.7 m from the interaction point <ce:cross-ref refid="br0530" id="crf10810">[53]</ce:cross-ref>. Using the particle time-of-flight measurement, electrons can be distinguished from hadrons for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si30.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>≤</mml:mo><mml:mn>2.5</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>. The collision time, used for the calculation of the time-of-flight to the TOF detector, is measured by an array of Cherenkov counters, the T0 detector, located at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si31.gif"><mml:mo>+</mml:mo><mml:mn>350</mml:mn><mml:mtext> </mml:mtext><mml:mtext>cm</mml:mtext></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si32.gif"><mml:mo>−</mml:mo><mml:mn>70</mml:mn><mml:mtext> </mml:mtext><mml:mtext>cm</mml:mtext></mml:math> from the interaction point along the beam direction <ce:cross-ref refid="br0540" id="crf10820">[54]</ce:cross-ref>. The Electromagnetic Calorimeter (EMCal), situated behind the TOF, is a sampling calorimeter based on Shashlik technology <ce:cross-ref refid="br0550" id="crf10830">[55]</ce:cross-ref>. Its geometrical acceptance is 107° in azimuth and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si27.gif"><mml:mo stretchy="false">|</mml:mo><mml:msub><mml:mrow><mml:mi>η</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">lab</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo></mml:math> 0.7. In this analysis, the azimuthal angle and <ce:italic>η</ce:italic> coverage were limited to 100° and 0.6, respectively, to ensure uniform detector performance.</ce:para><ce:para id="pr0100">The minimum-bias (MB) p–Pb data sample used in this analysis was collected in 2013. The trigger condition required a coincidence of signals between the two V0 scintillator hodoscopes, placed on either side of the interaction point at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si33.gif"><mml:mn>2.8</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>η</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">lab</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>5.1</mml:mn></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si34.gif"><mml:mo>−</mml:mo><mml:mn>3.7</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>η</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">lab</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mo>−</mml:mo><mml:mn>1.7</mml:mn></mml:math>, synchronised with the passage of bunches from both beams <ce:cross-ref refid="br0540" id="crf10840">[54]</ce:cross-ref>. The background due to interactions of one of the two beams and residual particles in the beam vacuum tube was rejected in the offline event selection by correlating the time information of the V0 detectors with that from the two Zero Degree Calorimeters (ZDC) <ce:cross-ref refid="br0500" id="crf10850">[50]</ce:cross-ref>, that are located 112.5 m away from the interaction point along the beam pipe, symmetrically on either side. The primary vertex was reconstructed with tracks in the ITS and the TPC <ce:cross-ref refid="br0500" id="crf10860">[50]</ce:cross-ref>. Events with a primary vertex located farther than <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si35.gif"><mml:mo>±</mml:mo><mml:mn>10</mml:mn><mml:mtext> </mml:mtext><mml:mtext>cm</mml:mtext></mml:math> from the centre of the interaction region along the beam direction were rejected. About 10% of the events do not fulfil this selection criterion. A sample of 100 million events passed the offline event selection, corresponding to an integrated luminosity <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si36.gif"><mml:msub><mml:mrow><mml:mi>L</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">int</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn>47.8</mml:mn><mml:mo>±</mml:mo><mml:mn>1.6</mml:mn><mml:mtext> </mml:mtext><mml:msup><mml:mrow><mml:mtext>μb</mml:mtext></mml:mrow><mml:mrow><mml:mo>−</mml:mo><mml:mn>1</mml:mn></mml:mrow></mml:msup></mml:math>, given the cross section <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si37.gif"><mml:msubsup><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">MB</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">V</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msubsup><mml:mo>=</mml:mo><mml:mn>2.09</mml:mn><mml:mo>±</mml:mo><mml:mn>0.07</mml:mn><mml:mtext> </mml:mtext><mml:mtext>b</mml:mtext></mml:math> for the minimum-bias V0 trigger condition <ce:cross-ref refid="br0560" id="crf10870">[56]</ce:cross-ref>. The efficiency for the trigger condition and offline event selection is larger than <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si38.gif"><mml:mn>99</mml:mn><mml:mtext>%</mml:mtext></mml:math> for non-single-diffractive (NSD) p–Pb collisions <ce:cross-ref refid="br0570" id="crf10880">[57]</ce:cross-ref>.</ce:para></ce:section><ce:section id="se0030"><ce:label>3</ce:label><ce:section-title id="st0040">Analysis</ce:section-title><ce:para id="pr0110">A combination of electron identification (eID) strategies with different detectors offers the largest <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> reach for the measurement of electrons from heavy-flavour hadron decays. In particular, it ensures that the systematic uncertainties and the hadron contamination are small over the whole transverse momentum range. Throughout the paper, the term ‘electron’ is used for electrons and positrons. The capability of the TPC to identify electrons via specific energy loss <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si29.gif"><mml:mi mathvariant="normal">d</mml:mi><mml:mi>E</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:mi>x</mml:mi></mml:math> in the detector was used over the whole momentum range <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si117.gif"><mml:mn>0.5</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>12</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>. However, it is subject to ambiguous identification of hadrons (pions, kaons, protons and deuterons) below <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si42.gif"><mml:mn>2.5</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> and above <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si43.gif"><mml:mn>6</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> in transverse momentum. At low transverse momentum (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si44.gif"><mml:mn>0.5</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>2.5</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>), these ambiguities were resolved by measuring the time-of-flight of the particle from the interaction region to the TOF detector and combining it with the momentum measurement, to determine the particle mass. In the high momentum region (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si45.gif"><mml:mn>6</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>12</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>), the EMCal was used to reduce the hadron contamination. Electrons are separated from hadrons by calculating the ratio of the energy deposited (<ce:italic>E</ce:italic>) in the EMCal to the momentum (<ce:italic>p</ce:italic>). Since electrons deposit all of their energy in the EMCal, the ratio <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si46.gif"><mml:mi>E</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi>p</mml:mi></mml:math> is around unity for electrons, while the ratio for charged hadrons is much smaller on average.</ce:para><ce:para id="pr0120">The selection criteria for charged-particle tracks are similar to those applied in previous analyses measuring the production of electrons from heavy-flavour hadron decays in pp collisions <ce:cross-refs refid="br0580 br0590" id="crs0110">[58,59]</ce:cross-refs>. In order to have optimal eID performance with the TPC, the analysis was restricted to the pseudorapidity range <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si47.gif"><mml:mo stretchy="false">|</mml:mo><mml:msub><mml:mrow><mml:mi>η</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">lab</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo><mml:mn>0.6</mml:mn></mml:math> in the laboratory frame for electrons with transverse momentum <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si117.gif"><mml:mn>0.5</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>12</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>. Up to a <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si43.gif"><mml:mn>6</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>, a signal in the innermost layer of the SPD was required in order to reduce the background from photon conversions. In addition, this selection was further constrained by requiring hits in both SPD layers, to reduce the number of incorrect matches between candidate tracks and hits reconstructed in the first layer of the SPD. At high <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>, where the EMCal was used, tracks with hits in either of the SPD layers were selected in order to minimise the effect of dead areas of the first SPD layer within the acceptance region of the EMCal, as in previous analyses <ce:cross-refs refid="br0580 br0590" id="crs0120">[58,59]</ce:cross-refs>.</ce:para><ce:para id="pr0130">The electron identification with TPC and TOF was based on the number of standard deviations (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si39.gif"><mml:msubsup><mml:mrow><mml:mi>n</mml:mi></mml:mrow><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">TPC</mml:mi></mml:mrow></mml:msubsup></mml:math> or <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si49.gif"><mml:msubsup><mml:mrow><mml:mi>n</mml:mi></mml:mrow><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">TOF</mml:mi></mml:mrow></mml:msubsup></mml:math>) for the specific energy loss and time-of-flight measurements, respectively. The <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si50.gif"><mml:msub><mml:mrow><mml:mi>n</mml:mi></mml:mrow><mml:mrow><mml:mi>σ</mml:mi></mml:mrow></mml:msub></mml:math> variable is computed as a difference between the measured signal and the expected one for electrons divided by the energy loss (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si51.gif"><mml:msub><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">TPC</mml:mi></mml:mrow></mml:msub></mml:math>) or time-of-flight (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si52.gif"><mml:msub><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">TOF</mml:mi></mml:mrow></mml:msub></mml:math>) resolution. The expected signal and resolution originate from parametrisations of the detector signal, which are described in detail in <ce:cross-ref refid="br0500" id="crf10890">[50]</ce:cross-ref>. In the transverse momentum interval <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si44.gif"><mml:mn>0.5</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>2.5</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>, particles were identified as electrons if they satisfied <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si53.gif"><mml:mo>−</mml:mo><mml:mn>0.5</mml:mn><mml:mo>&lt;</mml:mo><mml:msubsup><mml:mrow><mml:mi>n</mml:mi></mml:mrow><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">TPC</mml:mi></mml:mrow></mml:msubsup><mml:mo>&lt;</mml:mo><mml:mn>3</mml:mn></mml:math>, which yields an identification efficiency of 69%. In the transverse momentum interval <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si54.gif"><mml:mn>2.5</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>6</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>, a tighter selection criterion of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si55.gif"><mml:mn>0</mml:mn><mml:mo>&lt;</mml:mo><mml:msubsup><mml:mrow><mml:mi>n</mml:mi></mml:mrow><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">TPC</mml:mi></mml:mrow></mml:msubsup><mml:mo>&lt;</mml:mo><mml:mn>3</mml:mn></mml:math> was applied (with an eID efficiency of 50%) to reduce the hadron contamination at higher transverse momentum. To resolve the aforementioned ambiguities at low transverse momentum (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si30.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>≤</mml:mo><mml:mn>2.5</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>), only tracks with <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si56.gif"><mml:mo stretchy="false">|</mml:mo><mml:msubsup><mml:mrow><mml:mi>n</mml:mi></mml:mrow><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">TOF</mml:mi></mml:mrow></mml:msubsup><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo><mml:mn>3</mml:mn></mml:math> were accepted. <ce:cross-ref refid="fg0010" id="crf10900">Fig. 1</ce:cross-ref><ce:float-anchor refid="fg0010"/>(a) shows the measured <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si29.gif"><mml:mi mathvariant="normal">d</mml:mi><mml:mi>E</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:mi>x</mml:mi></mml:math> in the TPC with respect to the expected <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si29.gif"><mml:mi mathvariant="normal">d</mml:mi><mml:mi>E</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:mi>x</mml:mi></mml:math> for electrons normalised to the expected resolution <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si51.gif"><mml:msub><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">TPC</mml:mi></mml:mrow></mml:msub></mml:math> after the eID with TOF. The solid lines indicate the selection criteria used for the transverse momentum interval <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si44.gif"><mml:mn>0.5</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>2.5</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>, indicating that the hadron contamination within the resulting electron candidate sample is small. In the high momentum region (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si45.gif"><mml:mn>6</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>12</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>), electrons were selected if they satisfied <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si40.gif"><mml:mo>−</mml:mo><mml:mn>1</mml:mn><mml:mo>&lt;</mml:mo><mml:msubsup><mml:mrow><mml:mi>n</mml:mi></mml:mrow><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">TPC</mml:mi></mml:mrow></mml:msubsup><mml:mo>&lt;</mml:mo><mml:mn>3</mml:mn></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si59.gif"><mml:mn>0.8</mml:mn><mml:mo>&lt;</mml:mo><mml:mi>E</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn>1.2</mml:mn></mml:math> (see <ce:cross-ref refid="fg0010" id="crf10910">Fig. 1</ce:cross-ref>(b)).</ce:para><ce:para id="pr0140">The hadron contamination in the electron candidate sample was determined by parametrising the TPC signal in momentum slices for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si105.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>≤</mml:mo><mml:mn>6</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> as done in previous analyses <ce:cross-refs refid="br0580 br0590" id="crs0130">[58,59]</ce:cross-refs>. In the transverse momentum interval <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si45.gif"><mml:mn>6</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>12</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>, the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si46.gif"><mml:mi>E</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi>p</mml:mi></mml:math> distribution for hadrons identified via the specific energy loss measured in the TPC (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si41.gif"><mml:msubsup><mml:mrow><mml:mi>n</mml:mi></mml:mrow><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">TPC</mml:mi></mml:mrow></mml:msubsup><mml:mo>&lt;</mml:mo><mml:mo>−</mml:mo><mml:mn>3.5</mml:mn></mml:math>) was normalised in the lower <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si46.gif"><mml:mi>E</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi>p</mml:mi></mml:math> range (0.4–0.6) to the corresponding <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si46.gif"><mml:mi>E</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi>p</mml:mi></mml:math> distribution for identified electrons (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si40.gif"><mml:mo>−</mml:mo><mml:mn>1</mml:mn><mml:mo>&lt;</mml:mo><mml:msubsup><mml:mrow><mml:mi>n</mml:mi></mml:mrow><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">TPC</mml:mi></mml:mrow></mml:msubsup><mml:mo>&lt;</mml:mo><mml:mn>3</mml:mn></mml:math>) (see <ce:cross-ref refid="fg0010" id="crf10920">Fig. 1</ce:cross-ref>(b)). The number of hadrons with an <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si46.gif"><mml:mi>E</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi>p</mml:mi></mml:math> ratio between 0.8 and 1.2 was thus determined in momentum slices. The hadron contamination ranged from 2% at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si63.gif"><mml:mn>5</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>6</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> to 15% at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si64.gif"><mml:mn>10</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>12</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> and was correspondingly subtracted. For <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si65.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>5</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>, the contamination was found to be negligible.</ce:para><ce:para id="pr0150">The resulting electron candidate sample, also referred to as the ‘inclusive electron sample’ in the following, still contains electrons from sources other than heavy-flavour hadron decays. The majority of the remaining background originates from photon conversions in the detector material (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si66.gif"><mml:mi>γ</mml:mi><mml:mo stretchy="false">→</mml:mo><mml:msup><mml:mrow><mml:mi mathvariant="normal">e</mml:mi></mml:mrow><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:msup><mml:msup><mml:mrow><mml:mi mathvariant="normal">e</mml:mi></mml:mrow><mml:mrow><mml:mo>−</mml:mo></mml:mrow></mml:msup></mml:math>) and Dalitz decays of neutral mesons, e.g. <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si67.gif"><mml:msup><mml:mrow><mml:mi>π</mml:mi></mml:mrow><mml:mrow><mml:mn>0</mml:mn></mml:mrow></mml:msup><mml:mo stretchy="false">→</mml:mo><mml:mi>γ</mml:mi><mml:mspace width="0.25em"/><mml:msup><mml:mrow><mml:mi mathvariant="normal">e</mml:mi></mml:mrow><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:msup><mml:msup><mml:mrow><mml:mi mathvariant="normal">e</mml:mi></mml:mrow><mml:mrow><mml:mo>−</mml:mo></mml:mrow></mml:msup></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si68.gif"><mml:mi>η</mml:mi><mml:mo stretchy="false">→</mml:mo><mml:mi>γ</mml:mi><mml:mspace width="0.25em"/><mml:msup><mml:mrow><mml:mi mathvariant="normal">e</mml:mi></mml:mrow><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:msup><mml:msup><mml:mrow><mml:mi mathvariant="normal">e</mml:mi></mml:mrow><mml:mrow><mml:mo>−</mml:mo></mml:mrow></mml:msup></mml:math>. These electrons are hereafter denoted as ‘photonic electrons’.</ce:para><ce:para id="pr0160">In previous analyses of electrons from heavy-flavour hadron decays in pp collisions by the ALICE Collaboration, the contribution of electrons from background sources was estimated via a data-tuned Monte Carlo cocktail and subtracted from the inclusive electron sample <ce:cross-refs refid="br0580 br0590" id="crs0140">[58,59]</ce:cross-refs>. The pion input to the cocktail was based on pion measurements with ALICE <ce:cross-refs refid="br0600 br0610" id="crs0150">[60,61]</ce:cross-refs>, while heavier mesons were implemented via <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si69.gif"><mml:msub><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> scaling <ce:cross-ref refid="br0620" id="crf10930">[62]</ce:cross-ref>, and photons from hard scattering processes (direct <ce:italic>γ</ce:italic>, <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si70.gif"><mml:msup><mml:mrow><mml:mi>γ</mml:mi></mml:mrow><mml:mrow><mml:mo>⁎</mml:mo></mml:mrow></mml:msup></mml:math>) were obtained from next-to-leading order (NLO) calculations <ce:cross-ref refid="br0630" id="crf10940">[63]</ce:cross-ref>. The resulting systematic uncertainty of the sum of all background sources was large, in particular at low <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>, where the signal-to-background ratio is small <ce:cross-refs refid="br0580 br0590" id="crs0160">[58,59]</ce:cross-refs>. In order to reduce this uncertainty, in this analysis an invariant mass technique <ce:cross-ref refid="br0160" id="crf10950">[16]</ce:cross-ref> was used to estimate the number of electrons coming from background sources.</ce:para><ce:para id="pr0170">Photonic electrons are produced in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si71.gif"><mml:msup><mml:mrow><mml:mi mathvariant="normal">e</mml:mi></mml:mrow><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:msup><mml:msup><mml:mrow><mml:mi mathvariant="normal">e</mml:mi></mml:mrow><mml:mrow><mml:mo>−</mml:mo></mml:mrow></mml:msup></mml:math> pairs and can thus be identified using an invariant mass technique (photonic method). All inclusive electrons were paired with other tracks in the same event passing looser track selection and electron identification criteria (e.g. <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si72.gif"><mml:mo>−</mml:mo><mml:mn>3</mml:mn><mml:mo>&lt;</mml:mo><mml:msubsup><mml:mrow><mml:mi>n</mml:mi></mml:mrow><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">TPC</mml:mi></mml:mrow></mml:msubsup><mml:mo>&lt;</mml:mo><mml:mn>3</mml:mn></mml:math>). Looser selection criteria were applied to increase the efficiency to find the photonic partner. <ce:cross-ref refid="fg0020" id="crf10960">Fig. 2</ce:cross-ref><ce:float-anchor refid="fg0020"/> shows the invariant mass distributions of unlike-sign and like-sign electron pairs for the inclusive electron in the interval <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si73.gif"><mml:mn>0.5</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>0.6</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>. The like-sign distribution estimates the uncorrelated pairs. Subtracting these from the unlike-sign pairs yields the number of electrons with a photonic partner <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si74.gif"><mml:msubsup><mml:mrow><mml:mi>N</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">phot</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">raw</mml:mi></mml:mrow></mml:msubsup></mml:math> (see <ce:cross-ref refid="fg0020" id="crf10970">Fig. 2</ce:cross-ref>). An invariant mass smaller than 0.14 GeV/<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si75.gif"><mml:msup><mml:mrow><mml:mi>c</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup></mml:math> was required. According to simulations, the peak around zero in the photonic electron pair distribution is due to photon conversions; the exponential tail to higher values originates from Dalitz decays of neutral mesons.</ce:para><ce:para id="pr0180">The efficiency <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si76.gif"><mml:msub><mml:mrow><mml:mi>ε</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">phot</mml:mi></mml:mrow></mml:msub></mml:math> to find photonic electron pairs was estimated using Monte Carlo simulations. A sample of p–Pb collisions was generated with HIJING v1.36 <ce:cross-ref refid="br0640" id="crf10980">[64]</ce:cross-ref>. To increase the statistical precision at high <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>, one <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si78.gif"><mml:mi mathvariant="normal">c</mml:mi><mml:mover accent="true"><mml:mrow><mml:mi mathvariant="normal">c</mml:mi></mml:mrow><mml:mo>‾</mml:mo></mml:mover></mml:math> or <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si79.gif"><mml:mi mathvariant="normal">b</mml:mi><mml:mover accent="true"><mml:mrow><mml:mi mathvariant="normal">b</mml:mi></mml:mrow><mml:mo>‾</mml:mo></mml:mover></mml:math> pair decaying semileptonically using the generator PYTHIA v6.4.21 <ce:cross-ref refid="br0650" id="crf10990">[65]</ce:cross-ref> with the Perugia-0 tune <ce:cross-ref refid="br0660" id="crf11000">[66]</ce:cross-ref> was added in each event. The generated particles were propagated through the apparatus using GEANT3 <ce:cross-ref refid="br0670" id="crf11010">[67]</ce:cross-ref> and a realistic detector response was applied to reproduce the performance of the detector system during data taking period. The simulated transverse momentum distributions of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si106.gif"><mml:msup><mml:mrow><mml:mi>π</mml:mi></mml:mrow><mml:mrow><mml:mn>0</mml:mn></mml:mrow></mml:msup></mml:math> and <ce:italic>η</ce:italic> mesons were weighted to match the measured shapes, where the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si106.gif"><mml:msup><mml:mrow><mml:mi>π</mml:mi></mml:mrow><mml:mrow><mml:mn>0</mml:mn></mml:mrow></mml:msup></mml:math> input was based on the measured charged-pion spectra <ce:cross-refs refid="br0680 br0690" id="crs0170">[68,69]</ce:cross-refs> assuming <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si81.gif"><mml:msub><mml:mrow><mml:mi>N</mml:mi></mml:mrow><mml:mrow><mml:msup><mml:mrow><mml:mi>π</mml:mi></mml:mrow><mml:mrow><mml:mn>0</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn>1</mml:mn><mml:mo stretchy="false">/</mml:mo><mml:mn>2</mml:mn><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mrow><mml:mi>N</mml:mi></mml:mrow><mml:mrow><mml:msup><mml:mrow><mml:mi>π</mml:mi></mml:mrow><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mrow><mml:mi>N</mml:mi></mml:mrow><mml:mrow><mml:msup><mml:mrow><mml:mi>π</mml:mi></mml:mrow><mml:mrow><mml:mo>−</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:msub><mml:mo stretchy="false">)</mml:mo></mml:math> and the <ce:italic>η</ce:italic> input was derived via <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si69.gif"><mml:msub><mml:mrow><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> scaling. The efficiency <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si76.gif"><mml:msub><mml:mrow><mml:mi>ε</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">phot</mml:mi></mml:mrow></mml:msub></mml:math> is defined as the fraction of electrons from photonic origin for which the partner could be found within the defined acceptance of the analysis, i.e. the geometrical acceptance of the ALICE apparatus together with the superimposed track selection and electron identification criteria. The efficiency <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si76.gif"><mml:msub><mml:mrow><mml:mi>ε</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">phot</mml:mi></mml:mrow></mml:msub></mml:math> increases sharply with <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> from 35% to 80% between 0.5 and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si83.gif"><mml:mn>3</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> and remains at 80% up to <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si119.gif"><mml:mn>12</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>. The raw photonic electron distribution <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si74.gif"><mml:msubsup><mml:mrow><mml:mi>N</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">phot</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">raw</mml:mi></mml:mrow></mml:msubsup></mml:math> was then corrected by the efficiency <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si76.gif"><mml:msub><mml:mrow><mml:mi>ε</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">phot</mml:mi></mml:mrow></mml:msub></mml:math> as <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si85.gif"><mml:msub><mml:mrow><mml:mi>N</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">phot</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">)</mml:mo><mml:mo>=</mml:mo><mml:msubsup><mml:mrow><mml:mi>N</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">phot</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">raw</mml:mi></mml:mrow></mml:msubsup><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">)</mml:mo><mml:mo stretchy="false">/</mml:mo><mml:msub><mml:mrow><mml:mi>ε</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">phot</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">(</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">)</mml:mo></mml:math> and subtracted from the inclusive electron yield to obtain the yield of electrons from heavy-flavour hadron decays. The signal-to-background ratio (ratio of non-photonic to photonic yield) ranges from 0.2 at 0.5 GeV/<ce:italic>c</ce:italic> to 4 at 10 GeV/<ce:italic>c</ce:italic>.</ce:para><ce:para id="pr0190">The remaining electrons are then those from semileptonic heavy-flavour hadron decays (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si86.gif"><mml:msubsup><mml:mrow><mml:mi>N</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">hfe</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">raw</mml:mi></mml:mrow></mml:msubsup></mml:math>), besides a small residual background contribution originating from semileptonic kaon decays and dielectron decays of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si87.gif"><mml:mi mathvariant="normal">J</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi>ψ</mml:mi></mml:math> mesons. The latter is the only non-negligible contribution from quarkonia. These contributions were subtracted from the corrected invariant cross section, as described later on in this section.</ce:para><ce:para id="pr0200">The <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>-differential invariant cross section <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si88.gif"><mml:msub><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">hfe</mml:mi></mml:mrow></mml:msub></mml:math> of electrons from heavy-flavour hadron decays, <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si89.gif"><mml:mn>1</mml:mn><mml:mo stretchy="false">/</mml:mo><mml:mn>2</mml:mn><mml:mo stretchy="false">(</mml:mo><mml:msup><mml:mrow><mml:mi mathvariant="normal">e</mml:mi></mml:mrow><mml:mrow><mml:mo>+</mml:mo></mml:mrow></mml:msup><mml:mo>+</mml:mo><mml:msup><mml:mrow><mml:mi mathvariant="normal">e</mml:mi></mml:mrow><mml:mrow><mml:mo>−</mml:mo></mml:mrow></mml:msup><mml:mo stretchy="false">)</mml:mo></mml:math>, was calculated as<ce:display><ce:formula id="fm0020"><ce:label>(2)</ce:label><mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si90.gif"><mml:mtable displaystyle="true" columnspacing="0.2em"><mml:mtr><mml:mtd columnalign="left"><mml:mfrac><mml:mn>1</mml:mn><mml:mrow><mml:mn>2</mml:mn><mml:mi>π</mml:mi><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac><mml:mfrac><mml:mrow><mml:msup><mml:mrow><mml:mi mathvariant="normal">d</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup><mml:msub><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">hfe</mml:mi></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mi mathvariant="normal">d</mml:mi><mml:mi>y</mml:mi></mml:mrow></mml:mfrac></mml:mtd></mml:mtr><mml:mtr><mml:mtd columnalign="left"><mml:mspace width="1em"/><mml:mo>=</mml:mo><mml:mfrac><mml:mn>1</mml:mn><mml:mn>2</mml:mn></mml:mfrac><mml:mfrac><mml:mn>1</mml:mn><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>φ</mml:mi><mml:msubsup><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow><mml:mrow><mml:mtext>centre</mml:mtext></mml:mrow></mml:msubsup></mml:mrow></mml:mfrac><mml:mfrac><mml:mn>1</mml:mn><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>y</mml:mi><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac><mml:mfrac><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="normal">c</mml:mi></mml:mrow><mml:mrow><mml:mtext>unfold</mml:mtext></mml:mrow></mml:msub><mml:msubsup><mml:mrow><mml:mi>N</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">hfe</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">raw</mml:mi></mml:mrow></mml:msubsup></mml:mrow><mml:mrow><mml:mo stretchy="false">(</mml:mo><mml:msup><mml:mrow><mml:mi>ϵ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">geo</mml:mi></mml:mrow></mml:msup><mml:mo>×</mml:mo><mml:msup><mml:mrow><mml:mi>ϵ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">reco</mml:mi></mml:mrow></mml:msup><mml:mo>×</mml:mo><mml:msup><mml:mrow><mml:mi>ϵ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">eID</mml:mi></mml:mrow></mml:msup><mml:mo stretchy="false">)</mml:mo></mml:mrow></mml:mfrac><mml:mfrac><mml:msubsup><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">MB</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">V</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msubsup><mml:msub><mml:mrow><mml:mi>N</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">MB</mml:mi></mml:mrow></mml:msub></mml:mfrac><mml:mo>,</mml:mo></mml:mtd></mml:mtr></mml:mtable></mml:math></ce:formula></ce:display> where <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si91.gif"><mml:msubsup><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow><mml:mrow><mml:mtext>centre</mml:mtext></mml:mrow></mml:msubsup></mml:math> are the centres of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> bins with widths <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si92.gif"><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>, and Δ<ce:italic>φ</ce:italic> and Δ<ce:italic>y</ce:italic> denote the geometrical acceptance in azimuth and rapidity to which the analysis was restricted, respectively. <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si93.gif"><mml:msub><mml:mrow><mml:mi>N</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">MB</mml:mi></mml:mrow></mml:msub></mml:math> is the number of events that pass the selection criteria described in Section <ce:cross-ref refid="se0020" id="crf11020">2</ce:cross-ref> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si94.gif"><mml:msubsup><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">MB</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">V</mml:mi><mml:mn>0</mml:mn></mml:mrow></mml:msubsup></mml:math> is the p–Pb cross section for the minimum-bias V0 trigger condition. The raw spectrum of electrons from heavy-flavour hadron decays (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si86.gif"><mml:msubsup><mml:mrow><mml:mi>N</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">hfe</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">raw</mml:mi></mml:mrow></mml:msubsup></mml:math>) was corrected for the acceptance of the detectors in the selected geometrical region of the analysis (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si95.gif"><mml:msup><mml:mrow><mml:mi>ϵ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">geo</mml:mi></mml:mrow></mml:msup></mml:math>), the track reconstruction and selection efficiency (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si96.gif"><mml:msup><mml:mrow><mml:mi>ϵ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">reco</mml:mi></mml:mrow></mml:msup></mml:math>), and the eID efficiency (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si97.gif"><mml:msup><mml:mrow><mml:mi>ϵ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">eID</mml:mi></mml:mrow></mml:msup></mml:math>). These corrections were computed using the aforementioned Monte Carlo simulations. Only the efficiency of the TPC electron identification selection criterion for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si98.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>6</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> was determined using a data-driven approach based on the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si39.gif"><mml:msubsup><mml:mrow><mml:mi>n</mml:mi></mml:mrow><mml:mrow><mml:mi>σ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">TPC</mml:mi></mml:mrow></mml:msubsup></mml:math> distribution <ce:cross-ref refid="br0590" id="crf11030">[59]</ce:cross-ref>. The measurement of the electron <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> is affected by the finite momentum resolution and by electron energy loss due to bremsstrahlung in the detector material <ce:cross-ref refid="br0490" id="crf11040">[49]</ce:cross-ref>, which is not corrected for in the track reconstruction algorithm. These effects distort the shape of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> distribution, which falls steeply with increasing momentum. To determine this correction (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si100.gif"><mml:msub><mml:mrow><mml:mi>c</mml:mi></mml:mrow><mml:mrow><mml:mtext>unfold</mml:mtext></mml:mrow></mml:msub></mml:math>), an iterative unfolding procedure based on Bayes' theorem was applied <ce:cross-refs refid="br0700 br0710" id="crs0180">[70,71]</ce:cross-refs>.</ce:para><ce:para id="pr0210">The aforementioned residual background contributions, electrons from semileptonic kaon decays and dielectron decays of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si87.gif"><mml:mi mathvariant="normal">J</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi>ψ</mml:mi></mml:math> mesons, were estimated as an invariant cross section with Monte Carlo simulations and found to be less than 3% per <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> bin and subtracted from the corrected invariant cross section of non-photonic electrons. More specifically, the contribution from <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si87.gif"><mml:mi mathvariant="normal">J</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi>ψ</mml:mi></mml:math> mesons was implemented by using a parametrisation for pp collisions based on the interpolation of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si87.gif"><mml:mi mathvariant="normal">J</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi>ψ</mml:mi></mml:math> measurements from RHIC at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si101.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>200</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext></mml:math>, Tevatron at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si102.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>1.96</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math>, and the LHC at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si126.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>7</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> according to <ce:cross-ref refid="br0720" id="crf11050">[72]</ce:cross-ref>. Decays of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si87.gif"><mml:mi mathvariant="normal">J</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi>ψ</mml:mi></mml:math> mesons within <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si103.gif"><mml:mo stretchy="false">|</mml:mo><mml:msub><mml:mrow><mml:mi>y</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">lab</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo></mml:math> 1.0 were considered. The parametrisation and its associated systematic uncertainty were scaled from pp to p–Pb collisions assuming binary collision scaling. Potential deviations from binary collision scaling were considered by assigning a 50% systematic uncertainty on the normalisation. The parametrisation with its uncertainties used as input for the Monte Carlo simulations is consistent with the measured <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si87.gif"><mml:mi mathvariant="normal">J</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi>ψ</mml:mi></mml:math> cross section in p–Pb collisions <ce:cross-ref refid="br0380" id="crf11060">[38]</ce:cross-ref>.</ce:para><ce:para id="pr0220">The systematic uncertainties were estimated as a function of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> by repeating the analysis with different selection criteria. The systematic uncertainties were evaluated for the spectrum obtained after the subtraction of the photonic yield <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si104.gif"><mml:msub><mml:mrow><mml:mi>N</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">phot</mml:mi></mml:mrow></mml:msub></mml:math> from the inclusive spectrum and before removing the remaining background contributions originating from semileptonic kaon decays and dielectron decays of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si87.gif"><mml:mi mathvariant="normal">J</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi>ψ</mml:mi></mml:math> mesons. The sources of systematic uncertainty for the inclusive analysis and the determination of the electron background are listed in <ce:cross-ref refid="tl0010" id="crf11070">Table 1</ce:cross-ref><ce:float-anchor refid="tl0010"/>.</ce:para><ce:para id="pr0230">The systematic uncertainties for tracking and eID are <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> dependent due to the usage of the various detectors in the different momentum intervals. The latter also includes the uncertainties due to the determination of the hadron contamination. The 3% systematic uncertainty for the matching between ITS and TPC was taken from <ce:cross-ref refid="br0730" id="crf11080">[73]</ce:cross-ref>, where the matching efficiency of charged particles in data was compared to Monte Carlo simulations. The uncertainty of the TOF-TPC matching efficiency was estimated by comparing the matching efficiency in data and Monte Carlo simulations using electrons from photon conversions, which were identified via topological cuts. The uncertainty amounts to 3%. The TPC-EMCal matching uncertainty was assigned to be 1%, as determined by varying the size of the matching window in <ce:italic>η</ce:italic> and azimuth <ce:italic>φ</ce:italic> for charged-particle tracks that were extrapolated to the calorimeter. The resulting matching uncertainties were combined in quadrature for the various <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> intervals shown in <ce:cross-ref refid="tl0010" id="crf11090">Table 1</ce:cross-ref>.</ce:para><ce:para id="pr0240">The listed uncertainties for the photonic method include the uncertainties on eID and tracking. In addition, the Monte Carlo sample was divided into two halves. The first was treated as real data and the second was used to correct the resulting spectrum. Deviations from the expected <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> spectrum of electrons from heavy-flavour hadron decays resulted in a 2% systematic uncertainty for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si105.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>≤</mml:mo><mml:mn>6</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> and 4% above. The uncertainty on the re-weighting of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si106.gif"><mml:msup><mml:mrow><mml:mi>π</mml:mi></mml:mrow><mml:mrow><mml:mn>0</mml:mn></mml:mrow></mml:msup></mml:math>- and <ce:italic>η</ce:italic>-meson <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> distributions in Monte Carlo simulations was estimated by changing the weights by <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si107.gif"><mml:mo>±</mml:mo><mml:mn>10</mml:mn><mml:mtext>%</mml:mtext></mml:math>. The variation yielded a 2% uncertainty for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si30.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>≤</mml:mo><mml:mn>2.5</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> on the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>-differential invariant cross section of electrons from heavy-flavour hadron decays. This source of uncertainty is negligible at higher <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>. The invariant mass technique gives a systematic uncertainty smaller by a factor of ≥4 and of about 1.4 for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si108.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>≤</mml:mo><mml:mn>1</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si109.gif"><mml:mn>3</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>12</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>, respectively, compared to the one of the cocktail subtraction method <ce:cross-ref refid="br0590" id="crf11100">[59]</ce:cross-ref>. The reduction in uncertainty, in particular at low <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>, proves the advantage of using the invariant mass technique for the estimation of electrons from background sources.</ce:para><ce:para id="pr0250">The uncertainty of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> unfolding procedure was determined by employing an alternative unfolding method (matrix inversion) and, as described in <ce:cross-ref refid="br0590" id="crf11110">[59]</ce:cross-ref>, by correcting the data with two different Monte Carlo samples corresponding to different <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> distributions. In addition to the aforementioned signal-enhanced Monte Carlo sample, a minimum-bias sample was used. The comparison of the resulting <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> spectra revealed an uncertainty of 1% for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si105.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>≤</mml:mo><mml:mn>6</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>, and smaller than 1% above <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si43.gif"><mml:mn>6</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>. The systematic uncertainties of the heavy-flavour electron yield due to the subtraction of the remaining background originating from semileptonic kaon decays and dielectron decays from <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si87.gif"><mml:mi mathvariant="normal">J</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi>ψ</mml:mi></mml:math> mesons are smaller than 0.5%. This was estimated by changing the particle yields by <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si111.gif"><mml:mo>±</mml:mo><mml:mn>50</mml:mn><mml:mtext>%</mml:mtext></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si112.gif"><mml:mo>±</mml:mo><mml:mn>100</mml:mn><mml:mtext>%</mml:mtext></mml:math> for the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si87.gif"><mml:mi mathvariant="normal">J</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi>ψ</mml:mi></mml:math> meson and the semileptonic kaon decays, respectively.</ce:para><ce:para id="pr0260">The individual sources of systematic uncertainties are uncorrelated. Therefore, they were added in quadrature to give a total systematic uncertainty ranging from 5.8% to 16.4% depending on the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> bin. The normalisation uncertainty on the luminosity is of 3.7% <ce:cross-ref refid="br0560" id="crf11120">[56]</ce:cross-ref>.</ce:para><ce:para id="pr0270"><ce:cross-ref refid="fg0030" id="crf11280">Fig. 3</ce:cross-ref><ce:float-anchor refid="fg0030"/> shows the interval <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si113.gif"><mml:mn>2.5</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>8</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>-differential invariant cross section of electrons from heavy-flavour hadron decays in minimum-bias p–Pb collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif"><mml:msqrt><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">NN</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>5.02</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math>, comparing the results of the various eID strategies in the two transition regions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si42.gif"><mml:mn>2.5</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si43.gif"><mml:mn>6</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>. A consistency within 1% is found.</ce:para></ce:section><ce:section id="se0040"><ce:label>4</ce:label><ce:section-title id="st0050">pp reference</ce:section-title><ce:para id="pr0280">In order to calculate the nuclear modification factor <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si114.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pPb</mml:mi></mml:mrow></mml:msub></mml:math>, a reference cross section for pp collisions at the same centre-of-mass energy is needed. Since pp data at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si115.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>5.02</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> are currently not available, the reference was obtained by interpolating the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>-differential cross sections of electrons from heavy-flavour hadron decays measured in pp collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si116.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>2.76</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> and at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si126.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>7</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> <ce:cross-refs refid="br0580 br0590" id="crs0190">[58,59]</ce:cross-refs>. The analysis described in this paper requires a reference in the interval <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si117.gif"><mml:mn>0.5</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>12</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>. While the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si116.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>2.76</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> analysis was carried out in this <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> range, the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si126.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>7</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> measurement is limited to the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> interval <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si118.gif"><mml:mn>0.5</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>8</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>. Thus, to extend the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> interval up to <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si119.gif"><mml:mn>12</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> a measurement by the ATLAS Collaboration in the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> interval <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si120.gif"><mml:mn>7</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>12</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> was used <ce:cross-ref refid="br0740" id="crf11140">[74]</ce:cross-ref>. The published ATLAS measurement, <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si121.gif"><mml:mi mathvariant="normal">d</mml:mi><mml:mi>σ</mml:mi><mml:mo stretchy="false">/</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>, was divided by <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si122.gif"><mml:mn>1</mml:mn><mml:mo stretchy="false">/</mml:mo><mml:mo stretchy="false">(</mml:mo><mml:mn>2</mml:mn><mml:mi>π</mml:mi><mml:msubsup><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow><mml:mrow><mml:mtext>centre</mml:mtext></mml:mrow></mml:msubsup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>y</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>, where <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si91.gif"><mml:msubsup><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow><mml:mrow><mml:mtext>centre</mml:mtext></mml:mrow></mml:msubsup></mml:math> denotes the central values of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> bins, and Δ<ce:italic>y</ce:italic> the rapidity range covered by the measurement. In the overlap interval <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si123.gif"><mml:mn>7</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>8</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> the ALICE and ATLAS measurements, which agree within uncertainties, were combined as a weighted average. The inverse quadratic sum of statistical and systematic uncertainties of the two spectra were used as weights. Perturbative QCD (pQCD) calculations at fixed order with next-to-leading-log (FONLL) resummation <ce:cross-refs refid="br0750 br0760 br0770" id="crs0200">[75–77]</ce:cross-refs> describe all aforementioned pp results <ce:cross-refs refid="br0580 br0590" id="crs0210">[58,59]</ce:cross-refs> within experimental and theoretical uncertainties. The pp references are measured in a symmetric rapidity window (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si124.gif"><mml:mo stretchy="false">|</mml:mo><mml:msub><mml:mrow><mml:mi>y</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">cms</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo><mml:mn>0.8</mml:mn></mml:math> at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si116.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>2.76</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si125.gif"><mml:mo stretchy="false">|</mml:mo><mml:msub><mml:mrow><mml:mi>y</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">cms</mml:mi></mml:mrow></mml:msub><mml:mo stretchy="false">|</mml:mo><mml:mo>&lt;</mml:mo><mml:mn>0.5</mml:mn></mml:math> at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si126.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>7</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math>). The effect due to the different asymmetric rapidity window in this analysis was estimated with FONLL and is much smaller than the systematic uncertainties of the data, therefore is was neglected.</ce:para><ce:para id="pr0290">An assumption about the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si127.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt></mml:math> dependence of the heavy-flavour production cross sections is required for the interpolation. Calculations based on pQCD are consistent with a power-law scaling of the heavy-flavour production cross section with <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si127.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt></mml:math> <ce:cross-ref refid="br0780" id="crf11150">[78]</ce:cross-ref>. Therefore, this scaling was used to calculate the interpolated data points. The statistical uncertainties of the spectra at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si116.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>2.76</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si126.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>7</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> were added in quadrature with weights according to the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si127.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt></mml:math> interpolation. The weighted correlated systematic uncertainties (tracking, matching and eID) of the spectra at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si116.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>2.76</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si126.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>7</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> were added linearly, while the weighted uncorrelated uncertainties (ITS layer conditions, unfolding and cocktail systematics) were added in quadrature. The weights were determined according to the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si127.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt></mml:math> interpolation. The uncorrelated and correlated uncertainties were then added in quadrature.</ce:para><ce:para id="pr0300">The systematic uncertainty of the bin-by-bin interpolation procedure was added in quadrature to the previous ones. It was estimated by using a linear or exponential dependence on <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si127.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt></mml:math> instead of a power law. The ratios of the resulting <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> spectra to the baseline pp reference were used to estimate a systematic uncertainty of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si128.gif"><mml:mmultiscripts><mml:mrow><mml:mtext>%</mml:mtext></mml:mrow><mml:mprescripts/><mml:mrow><mml:mo>−</mml:mo><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mo>+</mml:mo><mml:mphantom><mml:mi>a</mml:mi></mml:mphantom><mml:mn>5</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>.</ce:para><ce:para id="pr0310">The resulting pp reference cross section is well described by FONLL calculations. The systematic uncertainties of the normalisations related to the determination of the minimum-bias nucleon–nucleon cross sections of the input spectra were likewise interpolated, yielding a normalisation uncertainty of 2.3% for the pp reference spectrum, assuming that they are uncorrelated.</ce:para></ce:section><ce:section id="se0050" role="results"><ce:label>5</ce:label><ce:section-title id="st0060">Results</ce:section-title><ce:para id="pr0320">The <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>-differential invariant cross section of electrons from heavy-flavour hadron decays in the rapidity range <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si129.gif"><mml:mo>−</mml:mo><mml:mn>1.065</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>y</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">cms</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>0.135</mml:mn></mml:math> for p–Pb collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif"><mml:msqrt><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">NN</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>5.02</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> is shown in <ce:cross-ref refid="fg0040" id="crf11160">Fig. 4</ce:cross-ref><ce:float-anchor refid="fg0040"/> and compared with the pp reference cross section. The vertical bars represent the statistical uncertainties, while the boxes indicate the systematic uncertainties. The systematic uncertainties of the p–Pb cross section are smaller than those of the pp cross section, in particular at low transverse momentum, mainly as a consequence of the estimation of the electron background via the invariant mass technique. For the pp analysis, the background was subtracted via the cocktail method. At low <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>, the electrons mainly originate from charm-hadron decays, while for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si131.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>≥</mml:mo><mml:mn>4</mml:mn><mml:mtext> GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> beauty-hadron decays are the dominant source in pp collisions <ce:cross-ref refid="br0460" id="crf11170">[46]</ce:cross-ref>.</ce:para><ce:para id="pr0330">The nuclear modification factor <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si114.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pPb</mml:mi></mml:mrow></mml:msub></mml:math> of electrons from heavy-flavour hadron decays as a function of transverse momentum is shown in <ce:cross-ref refid="fg0050" id="crf11180">Fig. 5</ce:cross-ref><ce:float-anchor refid="fg0050"/>. The statistical and systematic uncertainties of the spectra in p–Pb and pp were propagated as independent uncertainties. The normalisation uncertainties of the pp reference and the p–Pb spectrum were added in quadrature and are shown as a filled box at high transverse momentum in <ce:cross-ref refid="fg0050" id="crf11190">Fig. 5</ce:cross-ref>.</ce:para><ce:para id="pr0340">The <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si114.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pPb</mml:mi></mml:mrow></mml:msub></mml:math> is consistent with unity within uncertainties over the whole <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> range of the measurement. The production of electrons from heavy-flavour hadron decays is thus consistent with binary collision scaling of the reference spectrum for pp collisions at the same centre-of-mass energy. The suppression of the yield of heavy-flavour production in Pb–Pb collisions at high-<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> is therefore a final state effect induced by the produced hot medium.</ce:para><ce:para id="pr0350">Given the large systematic uncertainties, our measurement is also compatible with an enhancement in the transverse momentum interval <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si132.gif"><mml:mn>1</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>6</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> as seen at mid-rapidity in d–Au collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si12.gif"><mml:msqrt><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">NN</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>200</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext></mml:math> <ce:cross-ref refid="br0420" id="crf11200">[42]</ce:cross-ref>. Such an enhancement might be caused by radial flow as suggested by studies on the mean <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> as a function of the identified particle multiplicity <ce:cross-ref refid="br0680" id="crf11210">[68]</ce:cross-ref>.</ce:para><ce:para id="pr0360">The data are described within the uncertainties by pQCD calculations including initial-state effects (FONLL <ce:cross-ref refid="br0750" id="crf11220">[75]</ce:cross-ref> + EPS09NLO <ce:cross-ref refid="br0480" id="crf11230">[48]</ce:cross-ref> nuclear shadowing parametrisation). The results suggest that initial-state effects are small at high transverse momentum in Pb–Pb collisions. Calculations by Sharma et al. which include CNM energy loss, nuclear shadowing and coherent multiple scattering at the partonic level also describe the data <ce:cross-ref refid="br0270" id="crf11240">[27]</ce:cross-ref>. Calculations based on incoherent multiple scatterings by Kang et al. predict an enhancement at low <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> <ce:cross-ref refid="br0250" id="crf11250">[25]</ce:cross-ref>. The formation of a hydrodynamically expanding medium and consequently flow of charm and beauty quarks are expected to result in an enhancement in the nuclear modification factor <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si114.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pPb</mml:mi></mml:mrow></mml:msub></mml:math> <ce:cross-ref refid="br0450" id="crf11260">[45]</ce:cross-ref>. To quantify the possible effect on <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si114.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pPb</mml:mi></mml:mrow></mml:msub></mml:math>, a blast wave calculation with parameters extracted from fits to the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> spectra of light-flavour hadrons <ce:cross-ref refid="br0680" id="crf11270">[68]</ce:cross-ref> measured in p–Pb collisions was employed. The model calculation agrees with the data. However, the present uncertainties of the measurement do not allow us to discriminate among the aforementioned theoretical approaches.</ce:para></ce:section><ce:section id="se0060"><ce:label>6</ce:label><ce:section-title id="st0070">Summary and conclusions</ce:section-title><ce:para id="pr0370">The <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>-differential invariant cross section for electrons from heavy-flavour hadron decays in minimum-bias p–Pb collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif"><mml:msqrt><mml:msub><mml:mrow><mml:mi>s</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">NN</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>5.02</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> was measured in the rapidity range <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si129.gif"><mml:mo>−</mml:mo><mml:mn>1.065</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>y</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">cms</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>0.135</mml:mn></mml:math> and the transverse momentum interval <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si117.gif"><mml:mn>0.5</mml:mn><mml:mo>&lt;</mml:mo><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub><mml:mo>&lt;</mml:mo><mml:mn>12</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math> using the combination of three electron identification methods. The application of the invariant mass technique to subtract electrons not originating from open heavy-flavour hadron decays largely reduced the systematic uncertainties with respect to the cocktail subtraction method, in particular at low transverse momentum. The pp reference for the nuclear modification factor <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si114.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pPb</mml:mi></mml:mrow></mml:msub></mml:math> was obtained by interpolating the measured <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math>-differential cross sections of electrons from heavy-flavour hadron decays at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si116.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>2.76</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si126.gif"><mml:msqrt><mml:mi>s</mml:mi></mml:msqrt><mml:mo>=</mml:mo><mml:mn>7</mml:mn><mml:mtext> </mml:mtext><mml:mtext>TeV</mml:mtext></mml:math>. The <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si114.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pPb</mml:mi></mml:mrow></mml:msub></mml:math> is consistent with unity within uncertainties of about 25%, which become larger for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> below <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si10.gif"><mml:mn>1</mml:mn><mml:mtext> </mml:mtext><mml:mtext>GeV</mml:mtext><mml:mo stretchy="false">/</mml:mo><mml:mi>c</mml:mi></mml:math>. The presented calculations describe the data within uncertainties. The results suggest that heavy-flavour production in minimum-bias p–Pb collisions scales with the number of binary collisions, although within uncertainties the data are also consistent with an enhancement above this scaling. The consistency with unity of the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si114.gif"><mml:msub><mml:mrow><mml:mi>R</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">pPb</mml:mi></mml:mrow></mml:msub></mml:math> at high <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.gif"><mml:msub><mml:mrow><mml:mi>p</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">T</mml:mi></mml:mrow></mml:msub></mml:math> indicates that the suppression of heavy-flavour production in Pb–Pb collisions is of different origin than cold nuclear matter effects.</ce:para></ce:section></ce:sections><ce:acknowledgment id="ac0010"><ce:section-title id="st0080">Acknowledgements</ce:section-title><ce:para id="pr0380">The ALICE Collaboration would like to thank all its engineers and technicians for their invaluable contributions to the construction of the experiment and the CERN accelerator teams for the outstanding performance of the LHC complex. The ALICE Collaboration gratefully acknowledges the resources and support provided by all Grid centres and the Worldwide LHC Computing Grid (WLCG) Collaboration. The ALICE Collaboration acknowledges the following funding agencies for their support in building and running the ALICE detector: <ce:grant-sponsor id="gsp0010" sponsor-id="http://dx.doi.org/10.13039/501100007029">State Committee of Science</ce:grant-sponsor>, <ce:grant-sponsor id="gsp0020">World Federation of Scientists</ce:grant-sponsor> (WFS) and <ce:grant-sponsor id="gsp0030">Swiss Fonds Kidagan</ce:grant-sponsor>, Armenia; Conselho Nacional de Desenvolvimento Científico e Tecnológico (<ce:grant-sponsor id="gsp0040" sponsor-id="http://dx.doi.org/10.13039/501100003593">CNPq</ce:grant-sponsor>), Financiadora de Estudos e Projetos (<ce:grant-sponsor id="gsp0050" sponsor-id="http://dx.doi.org/10.13039/501100004809">FINEP</ce:grant-sponsor>), Fundação de Amparo à Pesquisa do Estado de São Paulo (<ce:grant-sponsor id="gsp0060" sponsor-id="http://dx.doi.org/10.13039/501100001807">FAPESP</ce:grant-sponsor>); National Natural Science Foundation of China (<ce:grant-sponsor id="gsp0070" sponsor-id="http://dx.doi.org/10.13039/501100001809">NSFC</ce:grant-sponsor>), the Chinese Ministry of Education (<ce:grant-sponsor id="gsp0080">CMOE</ce:grant-sponsor>) and the Ministry of Science and Technology of China (<ce:grant-sponsor id="gsp0090">MSTC</ce:grant-sponsor>); 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