Home > CERN Experiments > LHC Experiments > ALICE > ALICE Preprints > The ALICE Transition Radiation Detector: construction, operation, and performance > HTML MARC |
002281131 001__ 2281131 002281131 005__ 20241127041739.0 002281131 0248_ $$aoai:cds.cern.ch:2281131$$pcerncds:FULLTEXT$$pcerncds:CERN:FULLTEXT$$pcerncds:CERN 002281131 0247_ $$2DOI$$a10.1016/j.nima.2017.09.028 002281131 037__ $$9arXiv$$aarXiv:1709.02743$$cphysics.ins-det 002281131 037__ $$aCERN-EP-2017-222 002281131 035__ $$9arXiv$$aoai:arXiv.org:1709.02743 002281131 035__ $$9Inspire$$aoai:inspirehep.net:1622554$$d2024-11-26T15:21:34Z$$h2024-11-27T03:02:56Z$$mmarcxml$$ttrue$$uhttps://inspirehep.net/api/oai2d 002281131 035__ $$9Inspire$$a1622554 002281131 041__ $$aeng 002281131 088__ $$9CERN-EP-DRAFT-ALICE-2017-020 002281131 100__ $$aAcharya, Shreyasi$$iINSPIRE-00570928$$uCalcutta, VECC 002281131 246__ $$9arXiv$$aThe ALICE Transition Radiation Detector: construction, operation, and performance 002281131 245__ $$9arXiv$$aThe ALICE Transition Radiation Detector: construction, operation, and performance 002281131 269__ $$aGeneva$$bCERN$$c28 Aug 2017 002281131 260__ $$c2018-02-11 002281131 300__ $$a40 p 002281131 506__ $$dcds-edboard-alice@cern.ch 002281131 506__ $$malice-member [CERN] 002281131 506__ $$mcds-ph-ep-publications-referee [CERN] 002281131 500__ $$9arXiv$$a79 pages, 60 captioned figures, 6 tables, authors from page 74, submitted to NIM A, figures at http://aliceinfo.cern.ch/ArtSubmission/node/3740 002281131 520__ $$9Elsevier$$aThe Transition Radiation Detector (TRD) was designed and built to enhance the capabilities of the ALICE detector at the Large Hadron Collider (LHC). While aimed at providing electron identification and triggering, the TRD also contributes significantly to the track reconstruction and calibration in the central barrel of ALICE. In this paper the design, construction, operation, and performance of this detector are discussed. A pion rejection factor of up to 410 is achieved at a momentum of 1 GeV/ c in p–Pb collisions and the resolution at high transverse momentum improves by about 40% when including the TRD information in track reconstruction. The triggering capability is demonstrated both for jet, light nuclei, and electron selection. 002281131 520__ $$9arXiv$$aThe Transition Radiation Detector (TRD) was designed and built to enhance the capabilities of the ALICE detector at the Large Hadron Collider (LHC). While aimed at providing electron identification and triggering, the TRD also contributes significantly to the track reconstruction and calibration in the central barrel of ALICE. In this paper the design, construction, operation, and performance of this detector are discussed. A pion rejection factor of up to 410 is achieved at a momentum of 1 GeV/$c$ in p-Pb collisions and the resolution at high transverse momentum improves by about 40% when including the TRD information in track reconstruction. The triggering capability is demonstrated both for jet, light nuclei, and electron selection. 002281131 540__ $$3Preprint$$aCC-BY-4.0 002281131 540__ $$aCC-BY 002281131 542__ $$3Preprint$$dCERN$$g2017 002281131 562__ $$cPublic comments 002281131 595__ $$aCERN EDS 002281131 6531_ $$9CERN$$adetector 002281131 6531_ $$9CERN$$aparticle identification 002281131 6531_ $$9CERN$$atracker 002281131 6531_ $$9CERN$$atrigger 002281131 65017 $$2SzGeCERN$$aDetectors and Experimental Techniques 002281131 65017 $$2arXiv$$aphysics.ins-det 002281131 693__ $$aCERN LHC$$eALICE 002281131 690C_ $$aCERN 002281131 690C_ $$aARTICLE 002281131 700__ $$aAdam, Jaroslav$$iINSPIRE-00360890$$uCreighton U. 002281131 700__ $$aAdamova, Dagmar$$iINSPIRE-00261412$$uRez, Nucl. Phys. Inst. 002281131 700__ $$aAdler, Clemens$$uHeidelberg U. 002281131 700__ $$aAdolfsson, Jonatan$$iINSPIRE-00571154$$uLund U. 002281131 700__ $$aAggarwal, Madan Mohan$$iINSPIRE-00180711$$uPanjab U. 002281131 700__ $$aAglieri Rinella, Gianluca$$iINSPIRE-00249866$$uCERN 002281131 700__ $$aAgnello, Michelangelo$$iINSPIRE-00360901$$jORCID:0000-0002-0760-5075$$uTurin Polytechnic 002281131 700__ $$aAgrawal, Neelima$$iINSPIRE-00381545$$uIndian Inst. Tech., Mumbai 002281131 700__ $$aAhammed, Zubayer$$iINSPIRE-00180720$$uCalcutta, VECC 002281131 700__ $$aAhmad, Nazeer$$iINSPIRE-00249891$$uAligarh Muslim U. 002281131 700__ $$aAhn, Sang Un$$iINSPIRE-00254695$$uKISTI, Daejeon 002281131 700__ $$aAiola, Salvatore$$iINSPIRE-00381830$$jORCID:0000-0001-6209-7627$$uYale U. 002281131 700__ $$aAkindinov, Alexander$$iINSPIRE-00061314$$uMoscow, ITEP 002281131 700__ $$aAl-turany, Mohammad$$iINSPIRE-00571954$$uDarmstadt, EMMI 002281131 700__ $$aAlam, Sk Noor$$iINSPIRE-00415748$$uCalcutta, VECC 002281131 700__ $$aAntonczyk, Dariusz$$uFrankfurt U., Inst. Kernphys. 002281131 700__ $$aArend, Andreas$$uFrankfurt U., Inst. Kernphys. 002281131 700__ $$aBazo Alba, Jose Luis$$iINSPIRE-00047770$$uLima, Pont. U. 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U., Munich (main) 002281131 700__ $$aHorak, David$$iINSPIRE-00548374$$uPrague, Tech. U. 002281131 700__ $$aHornung, Sebastian$$iINSPIRE-00584070$$uDarmstadt, EMMI 002281131 700__ $$aHosokawa, Ritsuya$$iINSPIRE-00522280$$uTsukuba U.$$uLPSC, Grenoble 002281131 700__ $$aHristov, Peter Zahariev$$iINSPIRE-00091290$$uCERN 002281131 700__ $$aHuber, Sebastian$$uDarmstadt, EMMI 002281131 700__ $$aHughes, Charles$$iINSPIRE-00564077$$uTennessee U. 002281131 700__ $$aHumanic, Thomas$$iINSPIRE-00091603$$uOhio State U. 002281131 700__ $$aHussain, Nur$$iINSPIRE-00416277$$uGauhati U. 002281131 700__ $$aHussain, Tahir$$iINSPIRE-00507708$$jORCID:0000-0002-4951-5756$$uAligarh Muslim U. 002281131 700__ $$aHutter, Dirk$$iINSPIRE-00382970$$jORCID:0000-0002-1488-4009$$uFrankfurt U., FIAS 002281131 700__ $$aHwang, Dae Sung$$iINSPIRE-00091772$$uSejong U. 002281131 700__ $$aIga Buitron, Sergio Arturo$$iINSPIRE-00572756$$uMexico U., ICN 002281131 700__ $$aIlkaev, Radiy$$iINSPIRE-00248935$$uRFNC-VNIIEF, Sarov 002281131 700__ $$aInaba, Motoi$$iINSPIRE-00241821$$uTsukuba U. 002281131 700__ $$aIppolitov, Mikhail$$iINSPIRE-00250300$$uMoscow Phys. Eng. Inst.$$uKurchatov Inst., Moscow 002281131 700__ $$aIrfan, Muhammad$$iINSPIRE-00248911$$uAligarh Muslim U. 002281131 700__ $$aIslam, Md Samsul$$iINSPIRE-00564099$$uSaha Inst. 002281131 700__ $$aIvanov, Marian$$iINSPIRE-00262538$$uDarmstadt, EMMI 002281131 700__ $$aIvanov, Vladimir$$iINSPIRE-00262542$$uSt. Petersburg, INP 002281131 700__ $$aIzucheev, Vladimir$$iINSPIRE-00506818$$uSerpukhov, IHEP 002281131 700__ $$aJacak, Barbara$$iINSPIRE-00155696$$uLBL, Berkeley 002281131 700__ $$aJacazio, Nicolo$$iINSPIRE-00548380$$uBologna U.$$uINFN, Bologna 002281131 700__ $$aJacobs, Peter Martin$$iINSPIRE-00181871$$uLBL, Berkeley 002281131 700__ $$aJadhav, Manoj Bhanudas$$iINSPIRE-00531323$$jORCID:0000-0002-5225-2803$$uIndian Inst. Tech., Mumbai 002281131 700__ $$aJadlovsky, Jan$$iINSPIRE-00537120$$uKosice Tech. U. 002281131 700__ $$aJaelani, Syaefudin$$iINSPIRE-00581977$$uUtrecht U. 002281131 700__ $$aJahnke, Cristiane$$iINSPIRE-00383021$$uMunich, Tech. U., Universe 002281131 700__ $$aJakubowska, Monika Joanna$$iINSPIRE-00537133$$uWarsaw U. of Tech. 002281131 700__ $$aJanik, Malgorzata Anna$$iINSPIRE-00244548$$uWarsaw U. of Tech. 002281131 700__ $$aPahula Hewage, Sandun$$iINSPIRE-00246609$$uHouston U. 002281131 700__ $$aJena, Chitrasen$$iINSPIRE-00181905$$uNISER, Jatni 002281131 700__ $$aJena, Satyajit$$iINSPIRE-00248878$$jORCID:0000-0002-6220-6982$$uHouston U. 002281131 700__ $$aJercic, Marko$$iINSPIRE-00578879$$uZagreb U. 002281131 700__ $$aJimenez Bustamante, Raul Tonatiuh$$iINSPIRE-00355862$$uDarmstadt, EMMI 002281131 700__ $$aJones, Peter Graham$$iINSPIRE-00181937$$uBirmingham U. 002281131 700__ $$aJusko, Anton$$iINSPIRE-00250331$$uBirmingham U. 002281131 700__ $$aKalinak, Peter$$iINSPIRE-00247100$$uKosice, IEF 002281131 700__ $$aKalweit, Alexander Philipp$$iINSPIRE-00248849$$jORCID:0000-0001-6907-0486$$uCERN 002281131 700__ $$aKang, Ju Hwan$$iINSPIRE-00241999$$uYonsei U. 002281131 700__ $$aKaplin, Vladimir$$iINSPIRE-00248837$$uMoscow Phys. Eng. Inst. 002281131 700__ $$aKar, Somnath$$iINSPIRE-00383167$$uCalcutta, VECC 002281131 700__ $$aKarasu Uysal, Ayben$$iINSPIRE-00245978$$uKaratay U. 002281131 700__ $$aKaravichev, Oleg$$iINSPIRE-00262581$$uMoscow, INR 002281131 700__ $$aKaravicheva, Tatiana$$iINSPIRE-00262593$$uMoscow, INR 002281131 700__ $$aKarayan, Lilit$$iINSPIRE-00522297$$uDarmstadt, EMMI$$uHeidelberg U. 002281131 700__ $$aKarczmarczyk, Przemyslaw$$iINSPIRE-00577574$$uCERN 002281131 700__ $$aKarpechev, Evgeny$$iINSPIRE-00248813$$uMoscow, INR 002281131 700__ $$aKebschull, Udo Wolfgang$$iINSPIRE-00248807$$uGoethe U., Frankfurt, Inst. Inform. 002281131 700__ $$aKeidel, Ralf$$iINSPIRE-00248795$$uFachhochsch., Worms 002281131 700__ $$aKeijdener, Darius Laurens$$iINSPIRE-00416339$$uUtrecht U. 002281131 700__ $$aKeil, Markus$$iINSPIRE-00216636$$uCERN 002281131 700__ $$aKetzer, Bernhard Franz$$iINSPIRE-00095813$$uBonn U., HISKP 002281131 700__ $$aKhabanova, Zhanna$$iINSPIRE-00539181$$uNIKHEF, Amsterdam 002281131 700__ $$aKhan, Palash$$iINSPIRE-00289764$$uSaha Inst. 002281131 700__ $$aKhan, Shuaib Ahmad$$iINSPIRE-00243963$$uCalcutta, VECC 002281131 700__ $$aKhanzadeev, Alexei$$iINSPIRE-00242036$$uSt. Petersburg, INP 002281131 700__ $$aKharlov, Yury$$iINSPIRE-00095925$$uSerpukhov, IHEP 002281131 700__ $$aKhatun, Anisa$$iINSPIRE-00564120$$uAligarh Muslim U. 002281131 700__ $$aKhuntia, Arvind$$iINSPIRE-00564138$$jORCID:0000-0003-0996-8547$$uIndian Inst. Tech., Indore 002281131 700__ $$aKielbowicz, Miroslaw Marek$$iINSPIRE-00564106$$uCracow, INP 002281131 700__ $$aKileng, Bjarte$$iINSPIRE-00262606$$uBergen Coll. Higher Educ. 002281131 700__ $$aKim, Byungchul$$iINSPIRE-00645347$$uTsukuba U. 002281131 700__ $$aKim, Daehyeok$$iINSPIRE-00548392$$uYonsei U. 002281131 700__ $$aKim, Dong Jo$$iINSPIRE-00242076$$uJyvaskyla U. 002281131 700__ $$aKim, Hyeonjoong$$iINSPIRE-00410042$$jORCID:0000-0003-3746-5760$$uYonsei U. 002281131 700__ $$aKim, Jinsook$$iINSPIRE-00243973$$uGangneung-Wonju Natl. 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Kernphys. 002281131 700__ $$aKlein, Jochen$$iINSPIRE-00262064$$uCERN 002281131 700__ $$aKlein-boesing, Christian$$iINSPIRE-00003561$$jORCID:0000-0002-7285-3411$$uMunster U. 002281131 700__ $$aKlein-Boesing, Melanie$$uMunster U. 002281131 700__ $$aKliemant, Michael$$uFrankfurt U., Inst. 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Inst. 002281131 700__ $$aKondratyuk, Evgeny$$iINSPIRE-00507275$$uSerpukhov, IHEP 002281131 700__ $$aKonevskikh, Artem$$iINSPIRE-00248772$$uMoscow, INR 002281131 700__ $$aKonno, Masahiro$$uTsukuba U. 002281131 700__ $$aKonyushikhin, Maxim$$iINSPIRE-00381357$$uWayne State U. 002281131 700__ $$aKopcik, Michal$$iINSPIRE-00522467$$uKosice Tech. U. 002281131 700__ $$aKour, Mandeep$$iINSPIRE-00522474$$uJammu U. 002281131 700__ $$aKouzinopoulos, Charalampos$$iINSPIRE-00507396$$uCERN 002281131 700__ $$aKovalenko, Oleksandr$$iINSPIRE-00507510$$uWarsaw, Inst. Nucl. Studies 002281131 700__ $$aKovalenko, Vladimir$$iINSPIRE-00361228$$jORCID:0000-0001-6012-6615$$uSt. Petersburg State U. 002281131 700__ $$aKowalski, Marek$$iINSPIRE-00262137$$uCracow, INP 002281131 700__ $$aKoyithatta Meethaleveedu, Greeshma$$iINSPIRE-00245600$$uIndian Inst. Tech., Mumbai 002281131 700__ $$aKralik, Ivan$$iINSPIRE-00098249$$uKosice, IEF 002281131 700__ $$aKramer, Frederick$$uFrankfurt U., Inst. 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Inform. 002281131 700__ $$aMartinez Hernandez, Mario Ivan$$iINSPIRE-00300172$$uPuebla U., Mexico 002281131 700__ $$aMartinez-garcia, Gines$$iINSPIRE-00105190$$jORCID:0000-0002-8657-6742$$uSUBATECH, Nantes 002281131 700__ $$aMartinez Pedreira, Miguel$$iINSPIRE-00507190$$uCERN 002281131 700__ $$aMasciocchi, Silvia$$iINSPIRE-00272436$$uDarmstadt, EMMI 002281131 700__ $$aMasera, Massimo$$iINSPIRE-00105418$$jORCID:0000-0003-1880-5467$$uTurin U.$$uINFN, Turin 002281131 700__ $$aMasoni, Alberto$$iINSPIRE-00289880$$jORCID:0000-0002-2699-1522$$uINFN, Cagliari 002281131 700__ $$aMasson, Erwann$$iINSPIRE-00575832$$jORCID:0000-0002-5628-8926$$uSUBATECH, Nantes 002281131 700__ $$aMastroserio, Annalisa$$iINSPIRE-00248428$$jORCID:0000-0003-3711-8902$$uINFN, Bari 002281131 700__ $$aMathis, Andreas Michael$$iINSPIRE-00574444$$uMunich, Tech. U., Universe$$uTech. 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Inst. 002281131 700__ $$aMenchaca-rocha, Arturo Alejandro$$iINSPIRE-00244703$$uMexico U. 002281131 700__ $$aMeninno, Elisa$$iINSPIRE-00507326$$jORCID:0000-0003-4389-7711$$uSalerno U.$$uINFN, Salerno 002281131 700__ $$aMercado-perez, Jorge$$iINSPIRE-00289899$$uHeidelberg U. 002281131 700__ $$aMeres, Michal$$iINSPIRE-00245096$$uComenius U. 002281131 700__ $$aMhlanga, Sibaliso$$iINSPIRE-00564240$$uCape Town U. 002281131 700__ $$aMiake, Yasuo$$iINSPIRE-00242486$$uTsukuba U. 002281131 700__ $$aMieskolainen, Matti Mikael$$iINSPIRE-00507452$$uHelsinki Inst. of Phys. 002281131 700__ $$aMihaylov, Dimitar Lubomirov$$iINSPIRE-00580281$$uTech. 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Space Science 002281131 700__ $$aMohammadi, Naghmeh$$iINSPIRE-00416653$$uUtrecht U. 002281131 700__ $$aMohanty, Bedangadas$$iINSPIRE-00146508$$uNISER, Jatni 002281131 700__ $$aKhan, Mohammed Mohisin$$iINSPIRE-00244581$$uAligarh Muslim U. 002281131 700__ $$aMoreira De Godoy, Denise Aparecida$$iINSPIRE-00245954$$uMunster U. 002281131 700__ $$aPerez Moreno, Luis Alberto$$iINSPIRE-00531356$$uPuebla U., Mexico 002281131 700__ $$aMoretto, Sandra$$iINSPIRE-00289922$$jORCID:0000-0002-3136-1736$$uPadua U.$$uINFN, Padua 002281131 700__ $$aMorino, Yuhei$$uTokyo U. 002281131 700__ $$aMorreale, Astrid$$iINSPIRE-00142798$$uSUBATECH, Nantes 002281131 700__ $$aMorsch, Andreas$$iINSPIRE-00289930$$uCERN 002281131 700__ $$aMuccifora, Valeria$$iINSPIRE-00139164$$jORCID:0000-0002-5624-6486$$uFrascati 002281131 700__ $$aMudnic, Eugen$$iINSPIRE-00248333$$uSplit Tech. U. 002281131 700__ $$aMuhlheim, Daniel Michael$$iINSPIRE-00416728$$uMunster U. 002281131 700__ $$aMuhuri, Sanjib$$iINSPIRE-00248321$$uCalcutta, VECC 002281131 700__ $$aMukherjee, Maitreyee$$iINSPIRE-00361435$$uBose Inst., Kolkata$$uCAPSS, Kolkata 002281131 700__ $$aMulligan, James Declan$$iINSPIRE-00507724$$uYale U. 002281131 700__ $$aGameiro Munhoz, Marcelo$$iINSPIRE-00182574$$uSao Paulo U. 002281131 700__ $$aMunning, Konstantin$$iINSPIRE-00564280$$uBonn U., HISKP 002281131 700__ $$aMunzer, Robert Helmut$$iINSPIRE-00531366$$uFrankfurt U., Inst. Kernphys. 002281131 700__ $$aMurakami, Hikari$$iINSPIRE-00548414$$uTokyo U. 002281131 700__ $$aMurray, Sean$$iINSPIRE-00383510$$uiThemba LABS 002281131 700__ $$aMusa, Luciano$$iINSPIRE-00250444$$uCERN 002281131 700__ $$aMusinsky, Jan$$iINSPIRE-00385520$$uKosice, IEF 002281131 700__ $$aMyers, Corey James$$iINSPIRE-00564256$$uHouston U. 002281131 700__ $$aMyrcha, Julian Wojciech$$iINSPIRE-00564291$$uWarsaw U. of Tech. 002281131 700__ $$aMycke, Jan Felix$$uHeidelberg U. 002281131 700__ $$aNag, Dipanjan$$iINSPIRE-00583160$$uBose Inst., Kolkata$$uCAPSS, Kolkata 002281131 700__ $$aNaik, Bharati$$iINSPIRE-00531375$$uIndian Inst. Tech., Mumbai 002281131 700__ $$aNair, Rahul$$iINSPIRE-00531380$$jORCID:0000-0001-8326-9846$$uWarsaw, Inst. Nucl. Studies 002281131 700__ $$aNandi, Basanta Kumar$$iINSPIRE-00182588$$uIndian Inst. Tech., Mumbai 002281131 700__ $$aNania, Rosario$$iINSPIRE-00172055$$uEnrico Fermi Ctr., Rome$$uINFN, Bologna 002281131 700__ $$aNappi, Eugenio$$iINSPIRE-00110416$$jORCID:0000-0003-2080-9010$$uINFN, Bari 002281131 700__ $$aNarayan, Amrendra$$iINSPIRE-00470117$$jORCID:0000-0003-3814-9559$$uIndian Inst. Tech., Mumbai 002281131 700__ $$aNaru, Muhammad Umair$$iINSPIRE-00507883$$uCOMSATS, Islamabad 002281131 700__ $$aFerreira Natal Da Luz, Pedro Hugo$$iINSPIRE-00511516$$uSao Paulo U. 002281131 700__ $$aNattrass, Christine$$iINSPIRE-00301613$$jORCID:0000-0002-8768-6468$$uTennessee U. 002281131 700__ $$aRosado Navarro, Sebastian$$iINSPIRE-00548422$$uPuebla U., Mexico 002281131 700__ $$aNayak, Kishora$$iINSPIRE-00416777$$uNISER, Jatni 002281131 700__ $$aNayak, Ranjit$$iINSPIRE-00548439$$jORCID:0000-0001-6988-0606$$uIndian Inst. Tech., Mumbai 002281131 700__ $$aNayak, Tapan Kumar$$iINSPIRE-00182590$$uCalcutta, VECC 002281131 700__ $$aNazarenko, Sergey$$iINSPIRE-00289965$$uRFNC-VNIIEF, Sarov 002281131 700__ $$aNedosekin, Alexander$$iINSPIRE-00060091$$uMoscow, ITEP 002281131 700__ $$aNegrao De Oliveira, Renato Aparecido$$iINSPIRE-00564311$$uCERN 002281131 700__ $$aNeher, Michael$$uHeidelberg U. 002281131 700__ $$aNellen, Lukas$$iINSPIRE-00110793$$jORCID:0000-0003-1059-8731$$uMexico U., ICN 002281131 700__ $$aNesbo, Simon Voigt$$iINSPIRE-00564307$$uBergen Coll. Higher Educ. 002281131 700__ $$aNg, Fabian$$iINSPIRE-00507999$$uHouston U. 002281131 700__ $$aNicassio, Maria$$iINSPIRE-00246928$$uDarmstadt, EMMI 002281131 700__ $$aNiculescu, Mihai$$iINSPIRE-00361459$$uBucharest, Inst. 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U. 002281131 700__ $$aOrtiz Velasquez, Antonio$$iINSPIRE-00248229$$uMexico U., ICN 002281131 700__ $$aOskarsson, Anders Nils Erik$$iINSPIRE-00242747$$uLund U. 002281131 700__ $$aOtwinowski, Jacek Tomasz$$iINSPIRE-00244142$$uCracow, INP 002281131 700__ $$aOyama, Ken$$iINSPIRE-00113667$$uNagasaki Inst. Appl. Sci. 002281131 700__ $$aPachmayer, Yvonne Chiara$$iINSPIRE-00290030$$uHeidelberg U. 002281131 700__ $$aPacik, Vojtech$$iINSPIRE-00573414$$uBohr Inst. 002281131 700__ $$aPagano, Davide$$iINSPIRE-00313673$$uU. Brescia 002281131 700__ $$aPagano, Paola$$iINSPIRE-00290049$$jORCID:0000-0001-5446-6226$$uSalerno U.$$uINFN, Salerno 002281131 700__ $$aPaic, Guy$$iINSPIRE-00113938$$uMexico U., ICN 002281131 700__ $$aPanebratsev, Yu$$uDubna, JINR 002281131 700__ $$aPalni, Prabhakar$$iINSPIRE-00265540$$uHua-Zhong Normal U. 002281131 700__ $$aPan, Jinjin$$iINSPIRE-00508257$$uWayne State U. 002281131 700__ $$aPandey, Ashutosh Kumar$$iINSPIRE-00522482$$jORCID:0000-0003-4420-7874$$uIndian Inst. 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Kernphys. 002281131 700__ $$aReolon, Anna Rita$$iINSPIRE-00250550$$jORCID:0000-0002-5826-4792$$uFrascati 002281131 700__ $$aReshetin, Andrey$$iINSPIRE-00119738$$uMoscow, INR 002281131 700__ $$aReygers, Klaus Johannes$$iINSPIRE-00242889$$uHeidelberg U. 002281131 700__ $$aRiabov, Viktor$$iINSPIRE-00242892$$uSt. Petersburg, INP 002281131 700__ $$aRicci, Renato Angelo$$iINSPIRE-00119905$$uINFN, Legnaro 002281131 700__ $$aRichert, Tuva Ora Herenui$$iINSPIRE-00361510$$uUtrecht U. 002281131 700__ $$aRichter, Matthias Rudolph$$iINSPIRE-00244201$$uOslo U. 002281131 700__ $$aRiedler, Petra$$iINSPIRE-00120095$$uCERN 002281131 700__ $$aRiegler, Werner$$iINSPIRE-00250574$$uCERN 002281131 700__ $$aRiggi, Francesco$$iINSPIRE-00290213$$jORCID:0000-0002-0030-8377$$uCatania U.$$uINFN, Catania 002281131 700__ $$aRistea, Catalin-lucian$$iINSPIRE-00508900$$uBucharest, Inst. 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Kernphys. 002281131 700__ $$aSahoo, Baidyanath$$iINSPIRE-00564677$$uIndian Inst. Tech., Mumbai 002281131 700__ $$aSahoo, Pragati$$iINSPIRE-00384329$$uIndian Inst. Tech., Indore 002281131 700__ $$aSahoo, Raghunath$$iINSPIRE-00182966$$uIndian Inst. Tech., Indore 002281131 700__ $$aSahoo, Sarita$$iINSPIRE-00508953$$uBhubaneswar, Inst. Phys. 002281131 700__ $$aSahu, Pradip Kumar$$iINSPIRE-00122421$$uBhubaneswar, Inst. Phys. 002281131 700__ $$aSaini, Jogender$$iINSPIRE-00246803$$uCalcutta, VECC 002281131 700__ $$aSakai, Shingo$$iINSPIRE-00182972$$uTsukuba U. 002281131 700__ $$aSakata, Dousatsu$$uTsukuba U. 002281131 700__ $$aSaleh, Mohammad Ahmad$$iINSPIRE-00509062$$uWayne State U. 002281131 700__ $$aSalzwedel, Jai Samuel Nielsen$$iINSPIRE-00361540$$jORCID:0000-0003-4032-9612$$uOhio State U. 002281131 700__ $$aSambyal, Sanjeev Singh$$iINSPIRE-00247865$$uJammu U. 002281131 700__ $$aSamsonov, Vladimir$$iINSPIRE-00242999$$uSt. Petersburg, INP$$uMoscow Phys. Eng. 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Kernphys. 002281131 700__ $$aSchiaua, Claudiu Cornel$$iINSPIRE-00247838$$uBucharest, IFIN-HH 002281131 700__ $$aSchicker, Rainer Martin$$iINSPIRE-00244227$$uHeidelberg U. 002281131 700__ $$aSchmidt, Christian Joachim$$iINSPIRE-00244248$$uDarmstadt, EMMI 002281131 700__ $$aSchmidt, Hans Rudolf$$iINSPIRE-00290373$$uTubingen U. 002281131 700__ $$aSchmidt, Marten Ole$$iINSPIRE-00571169$$uHeidelberg U. 002281131 700__ $$aSchmidt, Martin$$iINSPIRE-00560380$$uTubingen U. 002281131 700__ $$aSchmidt, Nicolas Vincent$$iINSPIRE-00640513$$uOak Ridge$$uFrankfurt U., Inst. 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Eng. Inst.$$uDarmstadt, EMMI 002281131 700__ $$aSenosi, Kgotlaesele$$iINSPIRE-00509280$$uiThemba LABS 002281131 700__ $$aSenyukov, Serhiy$$iINSPIRE-00270653$$jORCID:0000-0003-1907-9786$$uCERN$$uStrasbourg, IPHC$$uBITP, Kiev 002281131 700__ $$aSerradilla Rodriguez, Eulogio$$iINSPIRE-00247783$$uMexico U. 002281131 700__ $$aSett, Priyanka$$iINSPIRE-00411711$$uIndian Inst. Tech., Mumbai 002281131 700__ $$aSevcenco, Adrian$$iINSPIRE-00247771$$uBucharest, Inst. 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U., Munich (main)$$uMunich, Tech. U., Universe 002281131 700__ $$aVoscek, Dominik$$iINSPIRE-00564764$$uKosice Tech. U. 002281131 700__ $$aVranic, Danilo$$iINSPIRE-00290668$$uCERN$$uDarmstadt, EMMI 002281131 700__ $$aVrlakova, Janka$$iINSPIRE-00244985$$uKosice U. 002281131 700__ $$aVulpescu, B$$uHeidelberg U. 002281131 700__ $$aWagner, Boris$$iINSPIRE-00244999$$uBergen U. 002281131 700__ $$aWang, Hongkai$$iINSPIRE-00510390$$uUtrecht U. 002281131 700__ $$aWang, Mengliang$$iINSPIRE-00290694$$uHua-Zhong Normal U. 002281131 700__ $$aWang, Yifei$$uHeidelberg U. 002281131 700__ $$aWatanabe, Daisuke$$iINSPIRE-00255215$$uTsukuba U. 002281131 700__ $$aWatanabe, Kengo$$uTsukuba U. 002281131 700__ $$aWatanabe, Yosuke$$iINSPIRE-00412045$$jORCID:0000-0001-5643-3516$$uTokyo U.$$uTsukuba U. 002281131 700__ $$aWeber, Michael$$iINSPIRE-00349115$$uStefan Meyer Inst. Subatomare Phys. 002281131 700__ $$aWeber, Steffen Georg$$iINSPIRE-00510469$$uDarmstadt, EMMI 002281131 700__ $$aWegerle, Dominik$$uFrankfurt U., Inst. Kernphys. 002281131 700__ $$aWeiser, Dennis Franz$$iINSPIRE-00537176$$uHeidelberg U. 002281131 700__ $$aWenzel, Sandro Christian$$iINSPIRE-00287872$$uCERN 002281131 700__ $$aWessels, Johannes Peter$$iINSPIRE-00178848$$uMunster U. 002281131 700__ $$aWesterhoff, Uwe$$iINSPIRE-00246123$$uMunster U. 002281131 700__ $$aWhitehead, Andile Mothegi$$iINSPIRE-00537181$$uCape Town U. 002281131 700__ $$aWiechula, Jens$$iINSPIRE-00290727$$uFrankfurt U., Inst. Kernphys. 002281131 700__ $$aWikne, Jon$$iINSPIRE-00250749$$uOslo U. 002281131 700__ $$aWilk, Alexander$$uMunster U. 002281131 700__ $$aWilk, Grzegorz Andrzej$$iINSPIRE-00135952$$uWarsaw, Inst. Nucl. Studies 002281131 700__ $$aWilkinson, Jeremy John$$iINSPIRE-00385005$$uHeidelberg U.$$uINFN, Bologna 002281131 700__ $$aWillems, Guido Alexander$$iINSPIRE-00564789$$uMunster U. 002281131 700__ $$aWilliams, Crispin$$iINSPIRE-00254855$$jORCID:0000-0003-3589-0181$$uINFN, Bologna 002281131 700__ $$aWillsher, Emily$$iINSPIRE-00574082$$uBirmingham U. 002281131 700__ $$aWindelband, Bernd Stefan$$iINSPIRE-00246650$$uHeidelberg U. 002281131 700__ $$aWinn, Michael$$uHeidelberg U. 002281131 700__ $$aWitt, William Edward$$iINSPIRE-00564770$$uTennessee U. 002281131 700__ $$aXu, C$$uHeidelberg U. 002281131 700__ $$aYalcin, Serpil$$iINSPIRE-00412449$$uKaratay U. 002281131 700__ $$aYamakawa, Kosei$$iINSPIRE-00639310$$uHiroshima U. 002281131 700__ $$aYang, Ping$$iINSPIRE-00385084$$uHua-Zhong Normal U. 002281131 700__ $$aYano, Satoshi$$iINSPIRE-00385135$$uHiroshima U. 002281131 700__ $$aYin, Zhongbao$$iINSPIRE-00245030$$uHua-Zhong Normal U. 002281131 700__ $$aYokoyama, Hiroki$$iINSPIRE-00245044$$uTsukuba U.$$uLPSC, Grenoble 002281131 700__ $$aYoo, In-kwon$$iINSPIRE-00183678$$uPusan Natl. U. 002281131 700__ $$aYoon, Jin Hee$$iINSPIRE-00537195$$uInha U. 002281131 700__ $$aYurchenko, Volodymyr$$iINSPIRE-00510512$$uBITP, Kiev 002281131 700__ $$aYurevich, Vladimir$$uDubna, JINR 002281131 700__ $$aZaccolo, Valentina$$iINSPIRE-00361691$$uINFN, Turin 002281131 700__ $$aZaman, Ali$$iINSPIRE-00385199$$uCOMSATS, Islamabad 002281131 700__ $$aZampolli, Chiara$$iINSPIRE-00247387$$jORCID:0000-0002-2608-4834$$uCERN 002281131 700__ $$aCorrea Zanoli, Henrique Jose$$iINSPIRE-00510636$$uSao Paulo U. 002281131 700__ $$aZanevski, Yuri$$uDubna, JINR 002281131 700__ $$aZardoshti, Nima$$iINSPIRE-00522360$$uBirmingham U. 002281131 700__ $$aZarochentsev, Andrey$$iINSPIRE-00246638$$uSt. Petersburg State U. 002281131 700__ $$aZavada, Petr$$iINSPIRE-00138107$$uPrague, Inst. Phys. 002281131 700__ $$aZavyalov, Nikolay$$iINSPIRE-00290800$$uRFNC-VNIIEF, Sarov 002281131 700__ $$aZbroszczyk, Hanna Paulina$$iINSPIRE-00183708$$uWarsaw U. of Tech. 002281131 700__ $$aZhalov, Mikhail$$iINSPIRE-00254612$$uSt. Petersburg, INP 002281131 700__ $$aZhang, Haitao$$iINSPIRE-00361703$$uBergen U.$$uHua-Zhong Normal U. 002281131 700__ $$aZhang, Xiaoming$$iINSPIRE-00290818$$uHua-Zhong Normal U. 002281131 700__ $$aZhang, Yonghong$$iINSPIRE-00385253$$uHua-Zhong Normal U. 002281131 700__ $$aChunhui, Zhang$$iINSPIRE-00522436$$uUtrecht U. 002281131 700__ $$aZhang, Zuman$$iINSPIRE-00531444$$uClermont-Ferrand U.$$uHua-Zhong Normal U. 002281131 700__ $$aZhao, Chengxin$$iINSPIRE-00385310$$uOslo U. 002281131 700__ $$aZhigareva, Natalia$$iINSPIRE-00385354$$uMoscow, ITEP 002281131 700__ $$aZhou, Daicui$$iINSPIRE-00290834$$uHua-Zhong Normal U. 002281131 700__ $$aZhou, You$$iINSPIRE-00290856$$jORCID:0000-0002-7868-6706$$uBohr Inst. 002281131 700__ $$aZhou, Zhuo$$iINSPIRE-00417116$$uBergen U. 002281131 700__ $$aZhu, Hongsheng$$iINSPIRE-00361728$$uBergen U. 002281131 700__ $$aZhu, Jianhui$$iINSPIRE-00361715$$uHua-Zhong Normal U. 002281131 700__ $$aZichichi, Antonino$$iINSPIRE-00172134$$uEnrico Fermi Ctr., Rome$$uBologna U.$$uINFN, Bologna 002281131 700__ $$aZimmer, Stefan$$uHeidelberg U. 002281131 700__ $$aZimmermann, Alice$$iINSPIRE-00361741$$uHeidelberg U. 002281131 700__ $$aZimmermann, Markus Bernhard$$iINSPIRE-00385420$$uCERN 002281131 700__ $$aZinovjev, Gennady$$iINSPIRE-00290880$$uBITP, Kiev 002281131 700__ $$aZmeskal, Johann$$iINSPIRE-00564793$$uStefan Meyer Inst. Subatomare Phys. 002281131 700__ $$aZou, Shuguang$$iINSPIRE-00571982$$uHua-Zhong Normal U. 002281131 710__ $$5PH 002281131 710__ $$gALICE Collaboration 002281131 773__ $$c88-127$$pNucl. Instrum. Methods Phys. Res., A$$v881$$y2018 002281131 859__ $$fenrico.scomparin@cern.ch 002281131 8564_ $$81345115$$s7894209$$uhttp://cds.cern.ch/record/2281131/files/CERN-EP-DRAFT-ALICE-2017-020 - draft.pdf$$yDraft (restricted)$$zStamped by WebSubmit: 29/08/2017 002281131 8564_ $$81348013$$s19264$$uhttp://cds.cern.ch/record/2281131/files/TRDPIDPerformancevsNtrl_LHC16q_trdpaper.png$$y00043 Pion efficiency as a function of electron efficiency (left, for 6~detector layers) and as a function of the number of detector layers (right, for 90\% electron efficiency) for the various eID methods. The results are compared for the momentum interval 0.9--1.1\gevc in \ppb collisions at \sqrtsnn~=~5.02~TeV. The results of the truncated mean method are only shown for a minimum of 4~tracklets, where the resolution is better than 18\% (see Fig.~\ref{Figure_truncmeanres}). 002281131 8564_ $$81348014$$s42435$$uhttp://cds.cern.ch/record/2281131/files/LQ1Dwtestbeam_noinsert.png$$y00036 Total integrated charge, normalised to the tracklet length, measured in a single read-out chamber for electrons and pions in \ppb collisions at \mbox{\sqrtsnn~=~5.02~TeV}, in comparison with results from test beam measurements (solid lines)~\cite{Andronic:2004uy,Bailhache:2006hs}. The electrons and pions from test beam measurements were scaled by one common factor to compensate the difference in gain of the two data sets. 002281131 8564_ $$81348015$$s4915$$uhttp://cds.cern.ch/record/2281131/files/gtu_data_flow.png$$y00016 Major design blocks of the TMU and SMU stages of the GTU and data flow. The busy and trigger logic information are combined on the TGU before transmission to the CTP. 002281131 8564_ $$81348016$$s28708$$uhttp://cds.cern.ch/record/2281131/files/trdtrg_leadjetptxi_proj_12h_140424_1046.png$$y00058 Fragmentation functions of leading jets from the TRD-triggered sample for jets in different \pt intervals in pp collisions at \sqrts~=~8~TeV~\cite{Klein:2014rxa}. The leading jets are defined as the jets with the highest \pt in the event. 002281131 8564_ $$81348017$$s8318445$$uhttp://cds.cern.ch/record/2281131/files/arXiv:1709.02743.pdf 002281131 8564_ $$81348018$$s42972$$uhttp://cds.cern.ch/record/2281131/files/TRD_MPV_bgamma.png$$y00037 Most probable charge deposit signal normalised to that of minimum ionising particles as a function of $\beta\gamma$. The data are from measurements performed in test beam runs, \pp collisions at \mbox{\sqrts~=~7~TeV}, and cosmic-ray runs. Uncertainties in momentum and thus $\beta\gamma$ determination are drawn as horizontal and statistical uncertainties as vertical error bars. The shown fits correspond to the Equations~\ref{equ:aleph} and~\ref{equ:logistic} described in the text. 002281131 8564_ $$81348019$$s7609$$uhttp://cds.cern.ch/record/2281131/files/lambda_arkrxe.png$$y00009 Absorption length of X-rays in noble gases in the relevant energy range of TR production. 002281131 8564_ $$81348020$$s33569$$uhttp://cds.cern.ch/record/2281131/files/TPC2TRD.png$$y00024 Dependence of the position resolution on charge over transverse momentum for simulated tracks in the TRD (red) and in the TPC (blue), reconstructed global tracks from simulation (gray) and from \pp collisions at $\sqrt{s} = 13~\mathrm{TeV}$ (black). The label TRD-TPC indicates global tracks reconstructed with the ITS and TPC that were extrapolated to the TRD. The green line represents the theoretical value for the combined resolution of TRD and global tracks. The red line shows a parabolic fit to the corresponding points. 002281131 8564_ $$81348021$$s33107$$uhttp://cds.cern.ch/record/2281131/files/dedxwithsimtestbeam.png$$y00005 Distributions of the ionisation energy loss of pions and electrons with momenta of 2\gevc. The symbols represent the measurements obtained at the CERN PS with prototype read-out chambers that were smaller in overall size (active area ~\SI{25}{\centi\meter}~$\times$~\SI{32}{\centi\meter}) but otherwise similar in construction to that of the final detector. The lines are simulations accounting (continuous line) or not (dashed line) for the long range of $\delta$-electrons as compared to the chamber dimensions. Figure taken from~\cite{Andronic:2003qm}. \TBD{(Replace with GEANT4 once available M.Voelkl)} 002281131 8564_ $$81348022$$s8354$$uhttp://cds.cern.ch/record/2281131/files/pads.png$$y00003 Pad geometry of a TRD read-out chamber in layer~3 (not stack~2). The pad tilt is $\pm$~\ang{2} with respect to the $z$-axis (along the beam direction), with the sign alternating between layers. 002281131 8564_ $$81348023$$s167652$$uhttp://cds.cern.ch/record/2281131/files/cali-kr-pads2.png$$y00031 Relative pad gains for one chamber calibrated with electrons from \Kr decays. 002281131 8564_ $$81348024$$s24959$$uhttp://cds.cern.ch/record/2281131/files/cali-drift.png$$y00033 The derivative of the local tracking $y$ coordinate with respect to the drift time $t$ vs. the tangent of the azimuthal track inclination angle from global tracking. The slope and the offset of the fit (red line) give the drift velocity and the Lorentz angle, respectively. 002281131 8564_ $$81348025$$s3528886$$uhttp://cds.cern.ch/record/2281131/files/General_ALICE_Cross-Section_without_Magnet.png$$y00000 Schematic cross-section of the ALICE detector perpendicular to the LHC beam direction (status of the detector since the start of LHC \run{2}). The central barrel detectors cover the pseudorapidity range $| \eta | \lesssim 0.9 $ and are located inside the solenoid magnet, which provides a magnetic field with strength $B$~=~\SI{0.5}{\tesla} along the beam direction. 002281131 8564_ $$81348026$$s95469$$uhttp://cds.cern.ch/record/2281131/files/TRDPIDdEdxTRD.png$$y00038 Truncated mean signal as a function of momentum for \ppb collisions at \mbox{\sqrtsnn = 5.02 TeV}. The solid lines represent the expected signals for various particle species. 002281131 8564_ $$81348027$$s34901$$uhttp://cds.cern.ch/record/2281131/files/gtu-a-correlation-pp.png$$y00053 Top: Correlation between $1/p_\textrm{T}$ obtained from the online tracking and from a matched offline track for pp collisions at $\sqrt{s} = 8~\mathrm{TeV}$. Bottom: Difference (points) of the online and offline track \pt for data and simulation. The error bars indicate the corresponding width of the difference in $p_\textrm{T}$. 002281131 8564_ $$81348028$$s6463$$uhttp://cds.cern.ch/record/2281131/files/TRsimmeas_sandwich.png$$y00007 Measured and simulated spectra of TR produced by electrons with a momentum of 2\gevc for the ALICE TRD sandwich radiator. Figure adapted from~\cite{Andronic:2005hw}. 002281131 8564_ $$81348029$$s27998$$uhttp://cds.cern.ch/record/2281131/files/cali-pars.png$$y00029 Average pulse height vs.\ drift time plot (derived from Fig.~\ref{fig:ph}) illustrating the main calibration parameters. For better understanding, a sketch of the chamber cross-section with field lines from Fig.~\ref{fig:roccross} is shown at the top. The peak at the left and the edge on the right of the drift time spectrum correspond to the anode wires and the chamber entrance window. The temporal difference between them depends on the drift velocity. The anode-peak position defines the time offset. The mean pulse height and the pedestal width are related to the gain and the pad noise, respectively. 002281131 8564_ $$81348030$$s3858$$uhttp://cds.cern.ch/record/2281131/files/trg_timing.png$$y00050 Timing of the various phases for the online tracking with respect to the interaction. 002281131 8564_ $$81348031$$s41879$$uhttp://cds.cern.ch/record/2281131/files/trdintrackingdata.png$$y00025 Improvement of the $q/$\pt resolution in data when TRD information is included as compared with the performance of tracking without TRD information for various running scenarios. The labels low and high IR indicate interaction rates of 12 and 230~kHz, respectively. 002281131 8564_ $$81348032$$s72629$$uhttp://cds.cern.ch/record/2281131/files/geo_material_budget_new.png$$y00008 The radiation length map in units of $X/X_{0}$ in a zoomed-in part of the active detector area as a function of the pseudorapidity and the azimuthal angle, calculated from the geometry in AliRoot (the colour scale has a suppressed zero). The positions of the MCMs and the cooling pipes are visible as hot spots. The radiation length was calculated for particles originating from the collision vertex. Therefore the cooling pipes of the six layers overlap for small, but not large $\eta$. 002281131 8564_ $$81348033$$s45854$$uhttp://cds.cern.ch/record/2281131/files/TPCnsigmaslice_mb_hse.png$$y00060 Electron selection for triggered data with and without the TRD offline PID (see Section~\ref{Chapterpid}) in Pb--p collisions at \mbox{\sqrtsnn = 5.02 TeV}. Electrons from photon conversions in the detector material were rejected by matching the online track with a track in the TPC. The corresponding distribution for minimum-bias data, scaled to the maximum of the distribution of the triggered data sample, is shown to visualise the TRD trigger capability to enhance electrons. 002281131 8564_ $$81348034$$s9527$$uhttp://cds.cern.ch/record/2281131/files/gtu-eff-pp-simplified.png$$y00052 Acceptance times efficiency of the global online tracking for primary tracks (Data) and tracks in the detector acceptance (Data, TRD acceptance) as function of the transverse momentum of the global offline track (trigger threshold at 2--3\gevc). The results of an ideal simulation, not considering non-operational parts of the real detector, are drawn for comparison. The dotted line shows the theoretical limit of the acceptance with $13$ out of $18$ supermodules installed during the \ppb data taking period in \run{1}. 002281131 8564_ $$81348035$$s33414$$uhttp://cds.cern.ch/record/2281131/files/cali-kr-spectrum2.png$$y00032 Pulse height spectrum before the krypton-based calibration, after one and after two iterations (calibrations performed in consecutive years) for one read-out chamber. 002281131 8564_ $$81348036$$s15583$$uhttp://cds.cern.ch/record/2281131/files/RatioQ_LHC13b.png$$y00041 Ratio of the average signal of electrons to that of pions as a function of the depth in the detector (slice number; the lowest (highest) slice number is farthest away from (closest to) the radiator). 002281131 8564_ $$81348037$$s103538$$uhttp://cds.cern.ch/record/2281131/files/cali-ntrkl.png$$y00035 Two quality-assurance plots (data from \pp collisions recorded in 2015 with all supermodules installed, tracks with at least 70~TPC clusters and $\pt>0.5$\gevc). Left: Efficiency of matching tracklets to TPC tracks. Right: Mean number of layers per track in each stack (cf.\ the discussion of inactive chambers in Section~\ref{Chapterhvinbeam}). 002281131 8564_ $$81348038$$s97151$$uhttp://cds.cern.ch/record/2281131/files/cali-match.png$$y00034 Two quality-assurance plots (data from \pp collisions recorded in 2015 with all supermodules installed, tracks with at least 70~TPC clusters and $\pt>0.5$\gevc). Left: Efficiency of matching tracklets to TPC tracks. Right: Mean number of layers per track in each stack (cf.\ the discussion of inactive chambers in Section~\ref{Chapterhvinbeam}). 002281131 8564_ $$81348039$$s37616$$uhttp://cds.cern.ch/record/2281131/files/tracklet.png$$y00020 Signal produced by a positively charged particle ($\pt = 0.5\gevc$). Left: Total charge per time bin used for particle identification. Right: Ionisation signal vs. pad number and time bin. The cluster positions are shown as reconstructed from the charge distribution (raw clusters) and after correction for the $E \times B$ effect (Lorentz-corr. clusters). 002281131 8564_ $$81348040$$s11266$$uhttp://cds.cern.ch/record/2281131/files/supermodulezdirection.png$$y00002 Cross-section (longitudinal view) of a supermodule. 002281131 8564_ $$81348041$$s12877$$uhttp://cds.cern.ch/record/2281131/files/Vd_Gain_portrait_new.png$$y00010 Left: Drift velocity as a function of the drift field for the nominal gas mixture Xe-CO$_2$ and different admixtures of N$_2$. Right: Gain as a function of the anode voltage for the same gas mixtures. 002281131 8564_ $$81348042$$s12435$$uhttp://cds.cern.ch/record/2281131/files/Schematic_gas_system.png$$y00011 Schematic view of the TRD gas system. The gas circulates in a closed loop pushed by a compressor. The flow for each supermodule is determined by the pressure set at individual pressure reducers in the inlet distribution modules. The overpressure is regulated with individual pneumatic valves at the return modules. The gas is purified at the surface and, when needed, supply gas is mixed and added to the loop. For the filling and the removing of the expensive xenon, semipermeable membranes are used to separate it from the CO$_2$. The recovered xenon can be treated in a cryogenic plant in order to remove accumulated N$_2$, prior to storage. 002281131 8564_ $$81348043$$s21081$$uhttp://cds.cern.ch/record/2281131/files/ph.png$$y00004 Average pulse height as a function of drift time for pions and electrons (with and without radiator). The time axis is shown with an arbitrary offset of \SI{0.3}{\micro\second}. The measurements were performed at the CERN PS with prototype read-out chambers that were smaller in overall size (active area~\SI{25}{\centi\meter}~$\times$~\SI{32}{\centi\meter}) but otherwise similar in construction to that of the final detector. Figure taken from~\cite{Andronic:2004uy}. 002281131 8564_ $$81348044$$s3186$$uhttp://cds.cern.ch/record/2281131/files/pt_upgrade.png$$y00013 In \run{1}, the wake-up signal required for the front-end electronics was generated by a dedicated pretrigger system. In \run{2}, the functionality was implemented in the central trigger processor and the LTU-T serves as an interface to the TRD FEE. 002281131 8564_ $$81348045$$s31269$$uhttp://cds.cern.ch/record/2281131/files/truncmeanres.png$$y00039 Resolution of the truncated mean signal as a function of the number of clusters in \ppb collisions at \mbox{\sqrtsnn~=~5.02~TeV}. 002281131 8564_ $$81348046$$s132973$$uhttp://cds.cern.ch/record/2281131/files/align-befaft.png$$y00028 TRD tracklet to TPC track residuals in $y$ as a function of the $z$~coordinate of the TPC track ($z_{\rm track}$) for supermodules 2~(left) and 6~(right). The colour code is linear in the number of tracks. The upper and lower panels show the situation with the survey alignment and with in addition the external alignment, respectively. The data are from a 2012 run of \pp collisions with B~=~$-$\SI{0.5}{\tesla}. The alignment set used for the lower plots was deduced from the same run. The internal alignment is applied in all four cases. 002281131 8564_ $$81348047$$s16110$$uhttp://cds.cern.ch/record/2281131/files/TRDPIDPerformancevsP_LHC16q_trdpaper.png$$y00044 Pion efficiency (for 90\% electron efficiency) as a function of momentum for the truncated mean, LQ1D, LQ2D, LQ3D, LQ7D and NN methods. The results are from \ppb collisions at \mbox{\sqrtsnn~=~5.02~TeV} and for tracks with signals in six layers. 002281131 8564_ $$81348048$$s10787$$uhttp://cds.cern.ch/record/2281131/files/resboth.png$$y00021 Residuals in $\Delta y$ of tracklets with respect to global tracks as a function of $\pt$ in pp collisions at $\sqrt{s} = 13~\mathrm{TeV}$. For every bin the mean (marker) and r.m.s.\ width (error bar) of the distribution are shown. 002281131 8564_ $$81348049$$s13483$$uhttp://cds.cern.ch/record/2281131/files/TRDPIDPerformance_LHC16q_trdpaper.png$$y00042 Pion efficiency as a function of electron efficiency (left, for 6~detector layers) and as a function of the number of detector layers (right, for 90\% electron efficiency) for the various eID methods. The results are compared for the momentum interval 0.9--1.1\gevc in \ppb collisions at \sqrtsnn~=~5.02~TeV. The results of the truncated mean method are only shown for a minimum of 4~tracklets, where the resolution is better than 18\% (see Fig.~\ref{Figure_truncmeanres}). 002281131 8564_ $$81348050$$s2535$$uhttp://cds.cern.ch/record/2281131/files/plot.png$$y00015 Simulation of the dead time as function of the read-out rate in Pb--Pb collisions for the effective DDL bandwidth in \run{1} (DDL) and \run{2} (DDL2). The simulation assumes a 5\% L1/L0 accept ratio and no L2 rejects. The scenarios central and mix correspond to an event size of 470~kB and 310~kB per supermodule, respectively, mimicking thus different event multiplicities. 002281131 8564_ $$81348051$$s31719$$uhttp://cds.cern.ch/record/2281131/files/align-pp.png$$y00027 Left: Cosmic-ray tracks with at least 100~TPC clusters and 5~TRD layers, recorded without magnetic field, used for the relative $r\varphi$ alignment of the TRD chambers within stacks (internal alignment). Right: Charged-particle tracks with at least 100~TPC clusters and 4~TRD layers from \pp collisions at $\sqrts=8$~TeV, used for the alignment of the TRD with respect to the TPC (external alignment). Both figures show data from 2012 (setup with 13~supermodules). 002281131 8564_ $$81348052$$s32804$$uhttp://cds.cern.ch/record/2281131/files/trdtrg_rej_12h_140426_1812.png$$y00055 Rejection by the level-1 trigger for requiring 1--4 tracks in any stack ($N_{\rm trk}$) above varying \pt thresholds for pp collisions at \sqrts~=~8~TeV~\cite{Klein:2014rxa}. The error bars indicate the statistical uncertainties. The distributions were obtained by counting the number of tracks in a stack above a given threshold and normalised by the number of sampled events. 002281131 8564_ $$81348053$$s5251$$uhttp://cds.cern.ch/record/2281131/files/gtu-tracking-time-tracklets-ppb.png$$y00051 Dependence of the time required for the global online tracking on the tracklet multiplicity in a single stack. 002281131 8564_ $$81348054$$s10180$$uhttp://cds.cern.ch/record/2281131/files/MemSum.png$$y00019 Monitored external DCS memory and occurrences of SEUs as a function of time. The periods of stable beam are indicated as well. 002281131 8564_ $$81348055$$s25733$$uhttp://cds.cern.ch/record/2281131/files/eventsizevsmult.png$$y00018 Event size vs charged-particle multiplicity for various collision systems for one supermodule. To obtain the charged-particle multiplicity, global tracks (see Section~\ref{Chaptertracking}) fulfilling minimum tracking quality criteria were counted on an event-by-event basis. 002281131 8564_ $$81348056$$s33110$$uhttp://cds.cern.ch/record/2281131/files/evview-00101-GEN-event-00101-all-xy-with-pileup.png$$y00049 Event display showing the tracks available for the level-1 trigger from the online reconstruction (green) in comparison with helix fits to the contributing tracklets (blue). The offset $a$ from the primary vertex used as measure for $1/\pt$ is shown as well. The colour coding of the tracklets (small boxes) is according to stacks. 002281131 8564_ $$81348057$$s3697$$uhttp://cds.cern.ch/record/2281131/files/trkl_reco.png$$y00047 Sketch of the tracklet reconstruction. The tracklet reconstruction in the MCMs is performed in a local coordinate system. The tracklet comprises the information on $y$, $d_y$, $z$ and PID. The magnetic and electric field and the effect of the Lorentz angle ($\Psi_{\rm L}$) are indicated as well. 002281131 8564_ $$81348058$$s15462$$uhttp://cds.cern.ch/record/2281131/files/TRD_truncatedmean_separationpower_trdpaper_vsp.png$$y00040 Measured separation power ($\frac{\Delta}{\sigma^{\rm trunc}} = \frac{ S^{\rm trunc}_{ \pi \rm , K } - S^{\rm trunc}_{\rm K, p} }{ \sigma^{\rm trunc} } $) for $\pi$/K and K/p separation as a function of momentum. 002281131 8564_ $$81348059$$s26534$$uhttp://cds.cern.ch/record/2281131/files/trdtrg_leadjetpt_proj_cmp_12h_140806_1847.png$$y00057 Left: \pt spectra of leading jets for the minimum-bias and triggered samples of pp collisions at \sqrts~=~8~TeV~\cite{Klein:2014rxa}. The leading jets are defined as the jets with the highest \pt in the event. Right: For comparison the \pt spectra were scaled to the same yield between 60 and 80\gevc. The spectra were re-binned to calculate the ratios. 002281131 8564_ $$81348060$$s17082$$uhttp://cds.cern.ch/record/2281131/files/tracking-conversion-examples-xy.png$$y00062 Photon converting into an e$^+$~e$^-$ pair at a large radius resembling a high-\pt track for the online tracking (green dashed line) since the offset to the primary vertex is small. 002281131 8564_ $$81348061$$s43479$$uhttp://cds.cern.ch/record/2281131/files/trd_readout.png$$y00012 Detector structures and corresponding read-out stages~\cite{Klein:2014rxa}. The top row of the figure represents the detector and the bottom row the GTU components. The dimensions are not to scale. 002281131 8564_ $$81348062$$s13728$$uhttp://cds.cern.ch/record/2281131/files/match_eff_456.png$$y00023 Fraction of tracks matched between the TPC and the TRD (TPC-TRD) and further the TOF detector (TRD-TOF) as a function of transverse momentum in pp collisions at $\sqrt{s} = 13~\mathrm{TeV}$. 002281131 8564_ $$81348063$$s16574$$uhttp://cds.cern.ch/record/2281131/files/trkl_channels.png$$y00014 Connections in one MCM~\cite{Klein:Diplom08}. 002281131 8564_ $$81348064$$s32933$$uhttp://cds.cern.ch/record/2281131/files/align-cosmics.png$$y00026 Left: Cosmic-ray tracks with at least 100~TPC clusters and 5~TRD layers, recorded without magnetic field, used for the relative $r\varphi$ alignment of the TRD chambers within stacks (internal alignment). Right: Charged-particle tracks with at least 100~TPC clusters and 4~TRD layers from \pp collisions at $\sqrts=8$~TeV, used for the alignment of the TRD with respect to the TPC (external alignment). Both figures show data from 2012 (setup with 13~supermodules). 002281131 8564_ $$81348065$$s9402$$uhttp://cds.cern.ch/record/2281131/files/ntracklets_matched_fullStacks.png$$y00022 Fraction of tracks, originating from the primary vertex, consisting of a given number of layers in pp collisions at $\sqrt{s} = 13~\mathrm{TeV}$. 002281131 8564_ $$81348066$$s109016$$uhttp://cds.cern.ch/record/2281131/files/TPCnsigma_2Dvsp_hse.png$$y00059 $n_{\sigma^\mathrm{TPC}_\mathrm{e}}$ as a function of momentum for Pb--p collisions at \mbox{\sqrtsnn = 5.02 TeV} recorded with the electron trigger (\pt threshold at 3\gevc). Electrons from photon conversions in the detector material were rejected by matching the online track with a track in the TPC. 002281131 8564_ $$81348067$$s78275$$uhttp://cds.cern.ch/record/2281131/files/radiatorcrosssec.png$$y00006 Side (left) and top (right) view of the design of the TRD sandwich radiator~\cite{Cortese:519145}. 002281131 8564_ $$81348068$$s9675$$uhttp://cds.cern.ch/record/2281131/files/gtu-pt-cut-pp-30.png$$y00054 Turn-on curve of the trigger with a \pt threshold of 3\gevc for positively and negatively charged particles in comparison to the same variable computed in simulation with a realistic detector geometry (active channels). Also shown is the corresponding distribution for an ideal detector geometry (ideal simulation, not considering misalignment). The onset is characterised by a fit with a Fermi function. 002281131 8564_ $$81348069$$s83096$$uhttp://cds.cern.ch/record/2281131/files/DCS_scheme.png$$y00017 Overview of the DCS software architecture. The tree structure consists of device units (boxes) and logical control units (ellipses). The abbreviations PT, DR and AN correspond to the pretrigger, the drift and anode channels, respectively. 002281131 8564_ $$81348070$$s25926$$uhttp://cds.cern.ch/record/2281131/files/trklqa_eff_mcpp_test_01.png$$y00048 Reconstruction efficiencies for tracklets as a function of $y$ and $q/\pt$ for Monte Carlo simulations. The $z$-axis entries are zero-suppressed. 002281131 8564_ $$81348071$$s12722$$uhttp://cds.cern.ch/record/2281131/files/trdtrg_leadjetpt_proj_12h_140424_1046.png$$y00056 Left: \pt spectra of leading jets for the minimum-bias and triggered samples of pp collisions at \sqrts~=~8~TeV~\cite{Klein:2014rxa}. The leading jets are defined as the jets with the highest \pt in the event. Right: For comparison the \pt spectra were scaled to the same yield between 60 and 80\gevc. The spectra were re-binned to calculate the ratios. 002281131 8564_ $$81348072$$s12530$$uhttp://cds.cern.ch/record/2281131/files/rawspectra_mb_hse.png$$y00061 \pt spectra of identified electrons for the minimum-bias and TRD-triggered data sample of Pb--p collisions at \mbox{\sqrtsnn = 5.02 TeV}. For the result of the TRD-triggered sample, electrons from photon conversions in the detector material were rejected by matching the online track with a track in the TPC. 002281131 8564_ $$81348073$$s13350$$uhttp://cds.cern.ch/record/2281131/files/cali-kr-spectrum.png$$y00030 Pulse height spectrum accumulated for one pad during the Kr-calibration run~\cite{mh-dipl,js-dipl}. The smooth solid line represents the fit from which the gain is extracted. 002281131 8564_ $$81348074$$s19678$$uhttp://cds.cern.ch/record/2281131/files/mcm-trkl.png$$y00046 Example tracklet in one MCM. The ADC data for 26~time bins (100~ns each) from 21~channels are shown. The found clusters are marked as asterisks and the final tracklet, calculated as a straight line fit through the clusters, with Lorentz correction as a red line. 002281131 8564_ $$81348075$$s41630$$uhttp://cds.cern.ch/record/2281131/files/tpcnsigmaslice_pidsteps.png$$y00045 Difference in units of standard deviations between the measured TPC energy loss of a given track and the expected energy loss of an electron with TOF ($\pm 3 \sigma^\mathrm{TOF}_\mathrm{e}$) and TRD (90\% electron efficiency) electron identification. The distributions are shown for tracks with a momentum of 1.9--2.1\gevc within the TRD acceptance (6~layers in the TRD) in \ppb collisions at \sqrtsnn~=~5.02~TeV. 002281131 8564_ $$81348076$$s13575$$uhttp://cds.cern.ch/record/2281131/files/roccross_new.png$$y00001 Schematic cross-section of a TRD chamber in the $x$-$z$ plane (perpendicular to the wires) with tracks of a pion and an electron to illustrate the ionisation energy deposition and the TR contribution. The large energy deposition due to the TR photon absorption is indicated by the large red circle in the drift region. The drift lines (solid lines) are calculated with Garfield~\cite{garfield} and correspond to the nominal voltage settings for chamber operation. The radiator is not drawn to scale. 002281131 8564_ $$81370136$$s7934640$$uhttp://cds.cern.ch/record/2281131/files/10.1016_j.nima.2017.09.028.pdf$$yFulltext 002281131 9031_ $$aApproval requested for number CERN-EP-2017-222$$bCERN-EP-2017-222$$cEPPHAPP$$d2017-08-29 09:42:59$$e2017-09-05 09:42:59$$fenrico.scomparin@cern.ch$$swaiting 002281131 9031_ $$aDocument approved$$bCERN-EP-2017-222$$cEPPHAPP$$d2017-08-29 10:52:16$$froger.forty@cern.ch$$sapproved 002281131 916__ $$sn$$w201735 002281131 980__ $$aALICE_Papers 002281131 980__ $$aARTICLE