Performance studies of the CMS Strip Tracker before installation

Adam, W.; Giudice, N.; Zito, G.; Chiorboli, M.; Bosi, F.; Sung, K.; Gritsan, A.V.; Richman, J.; Santocchia, A.; Cerati, G.; Maazouzi, C.; Maletta, F.; Speer, T.; Fiori, F.; Stahl, A.; Frühwirth, R.; Moulik, T.; Vander Donckt, M.; Miner, D.; Meschini, M.; Tenchini, R.; Guardone, N.; Van Lancker, L.; Wingham, M.; Tkaczyk, S.; Liu, H.; Demaria, N.; Fahrer, M.; Demina, R.; Spiga, D.; Roberfroid, V.; Zorba, O.; Manna, N.; De Weirdt, S.; Satpathy, A.; Pozzobon, N.; Noy, M.; Gotra, Y.; Jaditz, S.; Parrini, G.; Gay, A.; Heydhausen, D.; Affolder, T.; Klanner, R.; De Callatay, B.; Goorens, R.; Hobson, P.R.; D'Hondt, J.; Amsler, Claude; Wlochal, M.; Fulcher, J.; Daubie, E.; Muller, S.; Reid, I.; Vanlaer, P.; Ambroglini, F.; Cazzola, U.; Friedl, M.; Segneri, G.; Lemaitre, V.; Pooth, O.; Wagner, S.R.; Frosali, S.; Giammanco, A.; De Boer, W.; Bisello, D.; Anagnostou, G.; Hahn, K.A.; Marchioro, A.; Strub, R.; Michal, S.; Sarkar, S.; Loreti, M.; Silvestris, L.; Noto, F.; Alagoz, E.; Shabalina, E.; Ronzhin, A.; Pasztor, G.; Piotrzkowski, K.; Bock, E.; Eppard, M.; Abbaneo, D.; Nikolic, M.; Ostapchuk, A.; D'Alfonso, M.; Kuronen, A.; Siegrist, P.; Miao, T.; Giordano, D.; Landsberg, G.; Perchalla, L.; Trocme, B.; Sala, G.; Regenfus, Christian; Baringer, Philip S.; Bianucci, S.; Feld, L.; Bean, A.; Buchmuller, O.; Tempesta, P.; De Filippis, N.; Mozer, Matthias Ulrich; Pierschel, G.; Florins, B.; Bonnevaux, A.; My, S.; Kalavase, P.; Linari, S.; Covarelli, R.; Jensen, H.; Noeding, C.; Chen, J.; Ageron, M.; Lomtadze, T.; Postema, H.; Marage, P.; Rudolph, M.; Bhat, P.C.; Devroede, O.; Giorgi, M.; Heier, S.; Agram, J.-L.; Allen, A.; Romero, A.; Contardo, D.; Steck, P.; Spagnolo, P.; Chiochia, V.; Honma, A.; Gerber, C.E.; Villella, I.; Focardi, E.; Keutgen, Th.; Foa, L.; Lae, C.K.; Vlimant, J.-R.; Lowette, S.; Moggi, A.; Christofek, L.; de Langhe, E.; Avanzini, C.; Benotto, F.; Ranieri, R.; Uhl, D.; Troska, J.; Ferorelli, R.; Chierici, R.; Shah, Y.; Ulmer, K.A.; Tricomi, A.; Petragnani, G.; Olivetto, C.; Zaccarelli, L.; Albergo, S.; Mariani, F.; Delmeire, E.; Lenzi, P.; Kaminsky, A.; Pantano, D.; Huhtinen, M.; Gennai, S.; Buhmann, P.; Cariola, P.; Schilling, F.-P.; Bacchetta, N.; Michotte, D.; Raffaelli, F.; Wickens, J.; Boccali, T.; Hooper, R.; Martinelli, G.; Gill, K.; Dierlamm, A.; Giusti, S.; Schirra, F.; Goerlach, U.; Rubinstein, N.; Syed, A.; Sigaud, C.; Cripps, N.; Brauer, R.; Stringer, R.; Radicci, V.; Van Mulders, P.; Slav, A.; Petrucciani, G.; Hermanns, T.; Dupasquier, T.; Nahn, S.; Bloch, C.; Macchiolo, A.; Profeti, A.; Tessaro, M.; Dirkes, G.; Sentenac, D.; Teyssier, D.; Ricci, D.; Tran, N.V.; Kyre, S.; Bagliesi, G.; Paillard, C.; Zatserklyaniy, A.; Ljuslin, C.; Palmonari, F.; Khomenkov, V.; Chabanat, E.; Drouhin, F.; Khalatian, S.; Cucoanes, A .S.; Petit, P.; Esser, H.; Harkonen, J.; Dragicevic, M.; Lounis, A.; Staszak, D.; Rouby, X.; Lariccia, P.; Servoli, L.; Mason, D.; Breuker, H.; Incandela, H.; Kortesmaa, J.; Petagna, P.; Blaes, R.; Nigro, M.; Clerbaux, B.; Zhukov, V.; Bruno, G.; Ahmed, I.; Mangano, B.; Potenza, R.; Tuve, C.; Ligabue, F.; Bocci, A.; Tropea, P.; Ciulli, V.; Thomas, M.; Baulieu, G.; D'Alessandro, R.; Robmann, P.; Azzurri, P.; Harris, P.; Rizzi, D.; Tsang, K.V.; Mc Guinness, C.; Kreyer, S.; Kartashov, D.; Liamsuwan, T.; Mattiazzo, S.; Everaerts, P.; Gregoire, G.; Graehling, P.; Nguyen, H.; Candelori, A.; Butt, S.; Schmidt, A.; Sanguinetti, G.; Albert, E.; Pernicka, M.; Swain, S.; Steinbruck, G.; Benedetti, D.; Luzhetskiy, N.; Gillissen, C.; Piccut, C.; Bergauer, T.; Cattai, A.; De Robertis, G.; Olzem, J.; Sanhueza, S.; Hartmann, F.; Preda, M.; Gelin, G.; Abbas, M.; Grabit, R.; Maes, J.; Scarlini, E.; Muffat-Joly, J.; Rolandi, G.; Sutera, C.; Soldani, A.; Quertermont, L.; Steininger, H.; Pernot, J.F.; Paccagnella, A.; Jeng, G.-Y.; Dorigo, T.; Costa, S.; Frey, M.; Azzi, P.; Steiner, S.; Palla, F.; Moccia, S.; Basti, A.; Burke, Samuel P.; Korjenevski, S.; Goitom, I.; De Palma, M.; Bouhali, O.; Yang, Z.; Lungu, G.A.; Taghavi, S.; Giraud, N.; Sprenger, D.; Schleper, P.; Gutsche, O.; Genta, C.; Maenpaa, T.; Garberson, Jeffrey Ford; White, D.; Hauk, J.; Stark, R.; Kcira, D.; Church, I.; Elgammal, S.; Vanzetto, S.; Affolder, K.; Caponeri, B.; Akhtar, I.; Gross, L.; Vasey, M.; Tonelli, G.; Pal, I.; Leonardo, N.; Bilei, G.M.; Guillot, G.; Hinchey, C.; Bagby, L.; Nguyen, D.; Dumitrache, F.; Venturi, A.; Bazterra, V.E.; Kottelat, L.J.; Flucke, G.; Karaevski, S.; Kukulies, C.; Charaf, O.; Creanza, D.; Adler, V.; Balestri, G.; Juillot, P.; Beissel, F.; Messineo, A.; Waltenberger, W.; Sharp, P.; Hamdorf, R.; Bainbridge, R.; Borrello, L.; Ronga, F.; Fano, L.; Paoletti, S.; Ceccanti, M.; Boudoul, G.; Dewulf, J.-P.; Lumb, N.; Hoffmann, K.-H.; Civinini, C.; Hosselet, J.; De Mattia, M.; Cardaci, M.; Orbaker, D.; Militaru, O.; Lampen, T.; Onnela, A.; Teodorescu, L.; Brianzi, M.; Cihangir, S.; de Lentdecker, G.; Schmid, S.; Castello, R.; Wittmer, B.; Karimaki, V.; Giolo-Nicollerat, A.-S.; Hanson, G.; Selvaggi, G.; Mammini, P.; Zoeller, M.H.; Callahan, D.; Ribnik, J.; Della Negra, R.; Tomalin, I.; Biasini, M.; Migliore, E.; Karpinski, W.; Rizzi, A.; Skup, E.; Van Hove, P.; Cecchi, R.; Farano, R.; Anghel, I.; Stoner, J.; Haroutunian, R.; Stoye, M.; Engstrom, P.; Verdini, P.G.; Fiore, L.; Berretta, L.; Robinson, R.; Galanti, M.; Kostesmaa, J.; Kloukinas, K.; Czellar, S.; Raymond, D.M.; Berst, J.-D.; Benucci, L.; Edera, L.M.; Lamb, J.; Johnson, M.; Tavernier, S.; Babucci, E.; Linden, T.; Oberegger, M.; Mantovani, G.; Wilke, L.; Fontaine, J.-C.; Marcantonini, M.; Chabert, E.; Wastiels, C.; Pandoulas, D.; Calzolari, F.; Perries, S.; Kaussen, G.; Van Mechelen, P.; Heyninck, J.; de Wolf, E.A.; Dutta, S .; Simonis, H.-J.; Manolescu, F.; Muller, Th.; Hall, G.; Delattre, M.; Simms, L.; Bernardini, J.; Ledermann, B.; Gateau, M.; Martin, C.; Mirabito, L.; Krammer, M.; Vos, M.; Cole, J.; Saizu, M.A.; Pesaresi, M.; Hale, D.; Tsirou, A.; Weber, M.; Tosi, M.; Tuominen, E.; Landi, G.; Reznikov, S.; Magazzu, G.; Dobur, D .; Pioppi, M.; Vander Velde, C.; Pein, U.; Raupach, F.; Spiegel, L.; Costa, M.; Luukka, P.-R.; Burkett, K.; Incandela, J.; Tolaini, S.; Flugge, G.; Masetti, L.; Schael, S.; Tuominiemi, J.; Delaere, C.; Anttila, E.; Sparti, V.; Rochet, J.; Giassi, A.; Rebassoo, F.; Magini, N.; Massa, M.; Narain, M.; Jahn, D.; Crook, A.; Hammad, G.; Linn, A.; Widl, E.; Coughlan, J.; Bracci, F.; Campagnari, C.; Beaumont, W.; Didierjean, F.; Bonnet, J.-L.; Klein, K.; Hänsel, S.; Mersi, S.; Kaminski, J.; Mills, C.; Hrubec, J.; Postolache, V.; Cerri, C.; Serban, A.T.; Furgeri, A.; Schwering, G.; Sguazzoni, G.; Butz, E.; Poettgens, M.; Mannelli, M.; Borgia, M.A.; Ernenwein, J.-P.; Rommerskirchen, T.; Dell'Orso, R.; Dietch, J.; Barge, D.; Checcucci, B.; Blum, P.; Yumiceva, F.; Betchart, B.; Brom, J.-M.; Zerev, E.; Broccolo, B.; Maggi, G.; Spalding, W.J.; Estre, N.; Kraan, A.; Giubilato, P.; Stuart, D.; Castaldi, R.
doi:10.1088/1748-0221/4/06/P06009
001158708 001__ 1158708
001158708 003__ SzGeCERN
001158708 005__ 20211127042254.0
001158708 0247_ $$2DOI$$a10.1088/1748-0221/4/06/P06009
001158708 0248_ $$aoai:cds.cern.ch:1158708$$pcerncds:CERN$$pcerncds:CERN:FULLTEXT$$pcerncds:cms-notes$$pcerncds:FULLTEXT
001158708 037__ $$9arXiv$$aarXiv:0901.4316$$cphysics.ins-det
001158708 037__ $$aCMS-NOTE-2008-032
001158708 035__ $$9arXiv$$aoai:arXiv.org:0901.4316
001158708 035__ $$9SPIRES$$a8139695
001158708 035__ $$9Inspire$$a811949
001158708 041__ $$aeng
001158708 088__ $$9CERN-CMS-NOTE-2008-032
001158708 100__ $$aAdam, W.$$iINSPIRE-00060887$$uVienna, OAW
001158708 245__ $$aPerformance studies of the CMS Strip Tracker before installation
001158708 246__ $$aSilicon Strip Tracker Detector Performance with Cosmic Ray Data at the Tracker Integration Facility
001158708 269__ $$aGeneva$$bCERN$$c18 Mar 2008
001158708 260__ $$c2009
001158708 300__ $$a40 p
001158708 500__ $$aComments: 40 pages, 39 figures
001158708 500__ $$9arXiv$$a40 pages, 39 figures
001158708 520__ $$9arXiv$$aIn March 2007 the assembly of the Silicon Strip Tracker was completed at the Tracker Integration Facility at CERN. Nearly 15% of the detector was instrumented using cables, fiber optics, power supplies, and electronics intended for the operation at the LHC. A local chiller was used to circulate the coolant for low temperature operation. In order to understand the efficiency and alignment of the strip tracker modules, a cosmic ray trigger was implemented. From March through July 4.5 million triggers were recorded. This period, referred to as the Sector Test, provided practical experience with the operation of the Tracker, especially safety, data acquisition, power, and cooling systems. This paper describes the performance of the strip system during the Sector Test, which consisted of five distinct periods defined by the coolant temperature. Significant emphasis is placed on comparisons between the data and results from Monte Carlo studies.
001158708 540__ $$3Publication$$aCC-BY-3.0
001158708 541__ $$aPatrizia Azzi
001158708 595__ $$aCERN EDS
001158708 595__ $$agiva
001158708 595__ $$aLANL EDS
001158708 595__ $$aFulltext added, see CDS
001158708 595__ $$aOA
001158708 595__ $$aSIS JINST2009
001158708 65017 $$2SzGeCERN$$aDetectors and Experimental Techniques
001158708 65027 $$2arXiv$$aParticle Physics - Experiment
001158708 6531_ $$9CERN$$aTRACKING
001158708 693__ $$aCERN LHC$$eCMS
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001158708 700__ $$aKaussen, G.$$uAachen, Tech. Hochsch.
001158708 700__ $$aLinn, A.$$iINSPIRE-00310205$$uAachen, Tech. Hochsch.
001158708 700__ $$aPerchalla, L.$$iINSPIRE-00311278$$uAachen, Tech. Hochsch.
001158708 700__ $$aPoettgens, M.$$iINSPIRE-00311497$$uAachen, Tech. Hochsch.
001158708 700__ $$aPooth, O.$$iINSPIRE-00314326$$uAachen, Tech. Hochsch.
001158708 700__ $$aStahl, A.$$iINSPIRE-00315629$$uAachen, Tech. Hochsch.
001158708 700__ $$aZoeller, M.H.$$iINSPIRE-00313162$$uAachen, Tech. Hochsch.
001158708 700__ $$aBuhmann, P.$$iINSPIRE-00390551$$uHamburg U.
001158708 700__ $$aButz, E.$$iINSPIRE-00307963$$uHamburg U.
001158708 700__ $$aFlucke, G.$$iINSPIRE-00315660$$uHamburg U.
001158708 700__ $$aHamdorf, R.$$uHamburg U.
001158708 700__ $$aHauk, J.$$iINSPIRE-00309486$$uHamburg U.
001158708 700__ $$aKlanner, R.$$iINSPIRE-00096717$$uHamburg U.
001158708 700__ $$aPein, U.$$iINSPIRE-00315800$$uHamburg U.
001158708 700__ $$aSchleper, P.$$iINSPIRE-00124113$$uHamburg U.
001158708 700__ $$aSteinbruck, G.$$iINSPIRE-00128753$$uHamburg U.
001158708 700__ $$aBlum, P.$$iINSPIRE-00315848$$uKarlsruhe U., EKP
001158708 700__ $$aDe Boer, W.$$iINSPIRE-00067782$$uKarlsruhe U., EKP
001158708 700__ $$aDierlamm, A.$$iINSPIRE-00308534$$uKarlsruhe U., EKP
001158708 700__ $$aDirkes, G.$$iINSPIRE-00308560$$uKarlsruhe U., EKP
001158708 700__ $$aFahrer, M.$$iINSPIRE-00013586$$uKarlsruhe U., EKP
001158708 700__ $$aFrey, M.$$iINSPIRE-00308994$$uKarlsruhe U., EKP
001158708 700__ $$aFurgeri, A.$$iINSPIRE-00309050$$uKarlsruhe U., EKP
001158708 700__ $$aHartmann, F.$$iINSPIRE-00315862$$uKarlsruhe U., EKP$$uCERN
001158708 700__ $$aHeier, S.$$iINSPIRE-00309500$$uKarlsruhe U., EKP
001158708 700__ $$aHoffmann, K.-H.$$iINSPIRE-00309589$$uKarlsruhe U., EKP
001158708 700__ $$aKaminski, J.$$uKarlsruhe U., EKP
001158708 700__ $$aLedermann, B.$$uKarlsruhe U., EKP
001158708 700__ $$aLiamsuwan, T.$$iINSPIRE-00310170$$uKarlsruhe U., EKP
001158708 700__ $$aMuller, S.$$uKarlsruhe U., EKP
001158708 700__ $$aMuller, Th.$$uKarlsruhe U., EKP
001158708 700__ $$aSchilling, F.-P.$$iINSPIRE-00315911$$uKarlsruhe U., EKP
001158708 700__ $$aSimonis, H.-J.$$iINSPIRE-00312118$$uKarlsruhe U., EKP
001158708 700__ $$aSteck, P.$$iINSPIRE-00351849$$uKarlsruhe U., EKP
001158708 700__ $$aZhukov, V.$$iINSPIRE-00170284$$uKarlsruhe U., EKP
001158708 700__ $$aCariola, P.$$uINFN, Bari
001158708 700__ $$aDe Robertis, G.$$iINSPIRE-00308390$$uINFN, Bari
001158708 700__ $$aFerorelli, R.$$uINFN, Bari
001158708 700__ $$aFiore, L.$$iINSPIRE-00081363$$uINFN, Bari
001158708 700__ $$aPreda, M.$$uINFN, Bari
001158708 700__ $$aSala, G.$$iINSPIRE-00392369$$uINFN, Bari
001158708 700__ $$aSilvestris, L.$$iINSPIRE-00126485$$uINFN, Bari
001158708 700__ $$aTempesta, P.$$iINSPIRE-00208528$$uINFN, Bari
001158708 700__ $$aZito, G.$$iINSPIRE-00316344$$uINFN, Bari
001158708 700__ $$aCreanza, D.$$iINSPIRE-00316241$$uINFN, Bari$$uBari U.
001158708 700__ $$aDe Filippis, N.$$iINSPIRE-00316253$$uINFN, Bari$$uBari U.
001158708 700__ $$aDe Palma, M.$$iINSPIRE-00316265$$uINFN, Bari$$uBari U.
001158708 700__ $$aGiordano, D.$$iINSPIRE-00317954$$uINFN, Bari$$uBari U.
001158708 700__ $$aMaggi, G.$$uINFN, Bari$$uBari U.
001158708 700__ $$aManna, N.$$iINSPIRE-00310454$$uINFN, Bari$$uBari U.
001158708 700__ $$aMy, S.$$iINSPIRE-00314209$$uINFN, Bari$$uBari U.
001158708 700__ $$aSelvaggi, G.$$iINSPIRE-00316338$$uINFN, Bari$$uBari U.
001158708 700__ $$aAlbergo, S.$$iINSPIRE-00313816$$uINFN, Catania$$uCatania U.
001158708 700__ $$aChiorboli, M.$$iINSPIRE-00320632$$uINFN, Catania$$uCatania U.
001158708 700__ $$aCosta, S.$$iINSPIRE-00074650$$uINFN, Catania$$uCatania U.
001158708 700__ $$aGalanti, M.$$iINSPIRE-00309073$$uINFN, Catania$$uCatania U.
001158708 700__ $$aGiudice, N.$$iINSPIRE-00351408$$uINFN, Catania$$uCatania U.
001158708 700__ $$aGuardone, N.$$iINSPIRE-00151246$$uINFN, Catania$$uCatania U.
001158708 700__ $$aNoto, F.$$iINSPIRE-00245302$$uINFN, Catania$$uCatania U.
001158708 700__ $$aPotenza, R.$$iINSPIRE-00314332$$uINFN, Catania$$uCatania U.
001158708 700__ $$aSaizu, M.A.$$iINSPIRE-00207800$$uINFN, Catania$$uCatania U.
001158708 700__ $$aSparti, V.$$uINFN, Catania$$uCatania U.
001158708 700__ $$aSutera, C.$$uINFN, Catania$$uCatania U.
001158708 700__ $$aTricomi, A.$$iINSPIRE-00132210$$uINFN, Catania$$uCatania U.
001158708 700__ $$aTuve, C.$$iINSPIRE-00314440$$uINFN, Catania$$uCatania U.
001158708 700__ $$aBrianzi, M.$$iINSPIRE-00351473$$uINFN, Florence
001158708 700__ $$aCivinini, C.$$iINSPIRE-00073624$$uINFN, Florence
001158708 700__ $$aMaletta, F.$$iINSPIRE-00351037$$uINFN, Florence
001158708 700__ $$aManolescu, F.$$iINSPIRE-00206089$$uINFN, Florence
001158708 700__ $$aMeschini, M.$$iINSPIRE-00107084$$uINFN, Florence
001158708 700__ $$aPaoletti, S.$$iINSPIRE-00316496$$uINFN, Florence
001158708 700__ $$aSguazzoni, G.$$iINSPIRE-00125437$$uINFN, Florence
001158708 700__ $$aBroccolo, B.$$uINFN, Florence$$uFlorence U.
001158708 700__ $$aCiulli, V.$$iINSPIRE-00316472$$uINFN, Florence$$uFlorence U.
001158708 700__ $$aD'Alessandro, R.$$iINSPIRE-00075421$$uINFN, Florence$$uFlorence U.
001158708 700__ $$aFocardi, E.$$iINSPIRE-00316484$$uINFN, Florence$$uFlorence U.
001158708 700__ $$aFrosali, S.$$iINSPIRE-00309012$$uINFN, Florence$$uFlorence U.
001158708 700__ $$aGenta, C.$$iINSPIRE-00027840$$uINFN, Florence$$uFlorence U.
001158708 700__ $$aLandi, G.$$iINSPIRE-00099859$$uINFN, Florence$$uFlorence U.
001158708 700__ $$aLenzi, P.$$iINSPIRE-00013336$$uINFN, Florence$$uFlorence U.
001158708 700__ $$aMacchiolo, A.$$uINFN, Florence$$uFlorence U.
001158708 700__ $$aMagini, N.$$iINSPIRE-00310399$$uINFN, Florence$$uFlorence U.
001158708 700__ $$aParrini, G.$$iINSPIRE-00343980$$uINFN, Florence$$uFlorence U.
001158708 700__ $$aScarlini, E.$$iINSPIRE-00350600$$uINFN, Florence$$uFlorence U.
001158708 700__ $$aCerati, G.$$iINSPIRE-00308133$$uINFN, Milan Bicocca$$uMilan Bicocca U.
001158708 700__ $$aAzzi, P.$$iINSPIRE-00063509$$uINFN, Padua
001158708 700__ $$aBacchetta, N.$$iINSPIRE-00316624$$uINFN, Padua$$uCERN
001158708 700__ $$aCandelori, A.$$iINSPIRE-00203050$$uINFN, Padua
001158708 700__ $$aDorigo, T.$$iINSPIRE-00077883$$uINFN, Padua
001158708 700__ $$aKaminsky, A.$$uINFN, Padua
001158708 700__ $$aKaraevski, S.$$uINFN, Padua
001158708 700__ $$aKhomenkov, V.$$uINFN, Padua
001158708 700__ $$aReznikov, S.$$uINFN, Padua
001158708 700__ $$aTessaro, M.$$uINFN, Padua
001158708 700__ $$aBisello, D.$$iINSPIRE-00067193$$uINFN, Padua$$uPadua U.
001158708 700__ $$aDe Mattia, M.$$iINSPIRE-00308388$$uINFN, Padua$$uPadua U.
001158708 700__ $$aGiubilato, P.$$iINSPIRE-00017284$$uINFN, Padua$$uPadua U.
001158708 700__ $$aLoreti, M.$$iINSPIRE-00102673$$uINFN, Padua$$uPadua U.
001158708 700__ $$aMattiazzo, S.$$iINSPIRE-00316680$$uINFN, Padua$$uPadua U.
001158708 700__ $$aNigro, M.$$uINFN, Padua$$uPadua U.
001158708 700__ $$aPaccagnella, A.$$iINSPIRE-00019869$$uINFN, Padua$$uPadua U.
001158708 700__ $$aPantano, D.$$iINSPIRE-00114307$$uINFN, Padua$$uPadua U.
001158708 700__ $$aPozzobon, N.$$iINSPIRE-00008168$$uINFN, Padua$$uPadua U.
001158708 700__ $$aTosi, M.$$iINSPIRE-00028370$$uINFN, Padua$$uPadua U.
001158708 700__ $$aBilei, G.M.$$iINSPIRE-00316745$$uINFN, Perugia$$uCERN
001158708 700__ $$aCheccucci, B.$$iINSPIRE-00313891$$uINFN, Perugia
001158708 700__ $$aFano, L.$$iINSPIRE-00316769$$uINFN, Perugia
001158708 700__ $$aServoli, L.$$iINSPIRE-00125282$$uINFN, Perugia
001158708 700__ $$aAmbroglini, F.$$iINSPIRE-00307350$$uINFN, Perugia$$uPerugia U.
001158708 700__ $$aBabucci, E.$$iINSPIRE-00313849$$uINFN, Perugia$$uPerugia U.
001158708 700__ $$aBenedetti, D.$$uINFN, Perugia$$uPerugia U.
001158708 700__ $$aBiasini, M.$$iINSPIRE-00066890$$uINFN, Perugia$$uPerugia U.
001158708 700__ $$aCaponeri, B.$$iINSPIRE-00015352$$uINFN, Perugia$$uPerugia U.
001158708 700__ $$aCovarelli, R.$$iINSPIRE-00042025$$uINFN, Perugia$$uPerugia U.
001158708 700__ $$aGiorgi, M.$$uINFN, Perugia$$uPerugia U.
001158708 700__ $$aLariccia, P.$$iINSPIRE-00316770$$uINFN, Perugia$$uPerugia U.
001158708 700__ $$aMantovani, G.$$iINSPIRE-00104494$$uINFN, Perugia$$uPerugia U.
001158708 700__ $$aMarcantonini, M.$$uINFN, Perugia$$uPerugia U.
001158708 700__ $$aPostolache, V.$$iINSPIRE-00311539$$uINFN, Perugia$$uPerugia U.
001158708 700__ $$aSantocchia, A.$$iINSPIRE-00316782$$uINFN, Perugia$$uPerugia U.
001158708 700__ $$aSpiga, D.$$iINSPIRE-00030379$$uINFN, Perugia$$uPerugia U.
001158708 700__ $$aBagliesi, G.$$iINSPIRE-00063804$$uINFN, Pisa
001158708 700__ $$aBalestri, G.$$iINSPIRE-00351747$$uINFN, Pisa
001158708 700__ $$aBerretta, L.$$iINSPIRE-00307684$$uINFN, Pisa
001158708 700__ $$aBianucci, S.$$uINFN, Pisa
001158708 700__ $$aBoccali, T.$$iINSPIRE-00058286$$uINFN, Pisa
001158708 700__ $$aBosi, F.$$iINSPIRE-00307835$$uINFN, Pisa
001158708 700__ $$aBracci, F.$$uINFN, Pisa
001158708 700__ $$aCastaldi, R.$$iINSPIRE-00071520$$uINFN, Pisa
001158708 700__ $$aCeccanti, M.$$iINSPIRE-00238612$$uINFN, Pisa
001158708 700__ $$aCecchi, R.$$uINFN, Pisa
001158708 700__ $$aCerri, C.$$iINSPIRE-00203097$$uINFN, Pisa
001158708 700__ $$aCucoanes, A .S.$$iINSPIRE-00367291$$uINFN, Pisa
001158708 700__ $$aDell'Orso, R.$$iINSPIRE-00076544$$uINFN, Pisa
001158708 700__ $$aDobur, D .$$iINSPIRE-00319305$$uINFN, Pisa
001158708 700__ $$aDutta, S .$$iINSPIRE-00319945$$uINFN, Pisa
001158708 700__ $$aGiassi, A.$$iINSPIRE-00316818$$uINFN, Pisa
001158708 700__ $$aGiusti, S.$$iINSPIRE-00352313$$uINFN, Pisa
001158708 700__ $$aKartashov, D.$$iINSPIRE-00205250$$uINFN, Pisa
001158708 700__ $$aKraan, A.$$iINSPIRE-00316820$$uINFN, Pisa
001158708 700__ $$aLomtadze, T.$$iINSPIRE-00310247$$uINFN, Pisa
001158708 700__ $$aLungu, G.A.$$uINFN, Pisa
001158708 700__ $$aMagazzu, G.$$iINSPIRE-00206028$$uINFN, Pisa
001158708 700__ $$aMammini, P.$$iINSPIRE-00351561$$uINFN, Pisa
001158708 700__ $$aMariani, F.$$iINSPIRE-00316844$$uINFN, Pisa
001158708 700__ $$aMartinelli, G.$$iINSPIRE-00206120$$uINFN, Pisa
001158708 700__ $$aMoggi, A.$$iINSPIRE-00310709$$uINFN, Pisa
001158708 700__ $$aPalla, F.$$iINSPIRE-00114061$$uINFN, Pisa
001158708 700__ $$aPalmonari, F.$$iINSPIRE-00170181$$uINFN, Pisa
001158708 700__ $$aPetragnani, G.$$iINSPIRE-00311345$$uINFN, Pisa
001158708 700__ $$aProfeti, A.$$iINSPIRE-00117818$$uINFN, Pisa
001158708 700__ $$aRaffaelli, F.$$iINSPIRE-00314348$$uINFN, Pisa
001158708 700__ $$aRizzi, D.$$iINSPIRE-00351306$$uINFN, Pisa
001158708 700__ $$aSanguinetti, G.$$iINSPIRE-00207850$$uINFN, Pisa
001158708 700__ $$aSarkar, S.$$iINSPIRE-00300217$$uINFN, Pisa
001158708 700__ $$aSentenac, D.$$iINSPIRE-00207954$$uINFN, Pisa
001158708 700__ $$aSerban, A.T.$$iINSPIRE-00312052$$uINFN, Pisa
001158708 700__ $$aSlav, A.$$uINFN, Pisa
001158708 700__ $$aSoldani, A.$$uINFN, Pisa
001158708 700__ $$aSpagnolo, P.$$iINSPIRE-00128022$$uINFN, Pisa
001158708 700__ $$aTenchini, R.$$iINSPIRE-00316868$$uINFN, Pisa
001158708 700__ $$aTolaini, S.$$iINSPIRE-00004787$$uINFN, Pisa
001158708 700__ $$aVenturi, A.$$iINSPIRE-00316881$$uINFN, Pisa
001158708 700__ $$aVerdini, P.G.$$iINSPIRE-00316893$$uINFN, Pisa$$uCERN
001158708 700__ $$aVos, M.$$iINSPIRE-00240580$$uINFN, Pisa
001158708 700__ $$aZaccarelli, L.$$uINFN, Pisa
001158708 700__ $$aAvanzini, C.$$uINFN, Pisa$$uPisa U.
001158708 700__ $$aBasti, A.$$iINSPIRE-00004967$$uINFN, Pisa$$uPisa U.
001158708 700__ $$aBenucci, L.$$iINSPIRE-00314791$$uINFN, Pisa$$uPisa U.
001158708 700__ $$aBocci, A.$$iINSPIRE-00316794$$uINFN, Pisa$$uPisa U.
001158708 700__ $$aCazzola, U.$$iINSPIRE-00350920$$uINFN, Pisa$$uPisa U.
001158708 700__ $$aFiori, F.$$iINSPIRE-00170297$$uINFN, Pisa$$uPisa U.
001158708 700__ $$aLinari, S.$$iINSPIRE-00014095$$uINFN, Pisa$$uPisa U.
001158708 700__ $$aMassa, M.$$iINSPIRE-00310557$$uINFN, Pisa$$uPisa U.
001158708 700__ $$aMessineo, A.$$iINSPIRE-00316856$$uINFN, Pisa$$uPisa U.
001158708 700__ $$aSegneri, G.$$iINSPIRE-00312027$$uINFN, Pisa$$uPisa U.
001158708 700__ $$aTonelli, G.$$iINSPIRE-00316870$$uINFN, Pisa$$uPisa U.
001158708 700__ $$aAzzurri, P.$$iINSPIRE-00063512$$uPisa, Scuola Normale Superiore$$uINFN, Pisa
001158708 700__ $$aBernardini, J.$$iINSPIRE-00307660$$uPisa, Scuola Normale Superiore$$uINFN, Pisa
001158708 700__ $$aBorrello, L.$$iINSPIRE-00313870$$uPisa, Scuola Normale Superiore$$uINFN, Pisa
001158708 700__ $$aCalzolari, F.$$iINSPIRE-00174830$$uPisa, Scuola Normale Superiore$$uINFN, Pisa
001158708 700__ $$aFoa, L.$$iINSPIRE-00144556$$uPisa, Scuola Normale Superiore$$uINFN, Pisa
001158708 700__ $$aGennai, S.$$iINSPIRE-00316806$$uPisa, Scuola Normale Superiore$$uINFN, Pisa
001158708 700__ $$aLigabue, F.$$iINSPIRE-00316831$$uPisa, Scuola Normale Superiore$$uINFN, Pisa
001158708 700__ $$aPetrucciani, G.$$iINSPIRE-00320218$$uPisa, Scuola Normale Superiore$$uINFN, Pisa
001158708 700__ $$aRizzi, A.$$iINSPIRE-00318379$$uPisa, Scuola Normale Superiore$$uINFN, Pisa
001158708 700__ $$aYang, Z.$$uPisa, Scuola Normale Superiore$$uINFN, Pisa$$uPeking U.
001158708 700__ $$aBenotto, F.$$uINFN, Turin
001158708 700__ $$aDemaria, N.$$iINSPIRE-00076589$$uINFN, Turin
001158708 700__ $$aDumitrache, F.$$iINSPIRE-00308649$$uINFN, Turin
001158708 700__ $$aFarano, R.$$uINFN, Turin
001158708 700__ $$aBorgia, M.A.$$iINSPIRE-00307823$$uINFN, Turin$$uTurin U.
001158708 700__ $$aCastello, R.$$iINSPIRE-00308091$$uINFN, Turin$$uTurin U.
001158708 700__ $$aCosta, M.$$uINFN, Turin$$uTurin U.
001158708 700__ $$aMigliore, E.$$iINSPIRE-00107463$$uINFN, Turin$$uTurin U.
001158708 700__ $$aRomero, A.$$iINSPIRE-00121020$$uINFN, Turin$$uTurin U.
001158708 700__ $$aAbbaneo, D.$$iINSPIRE-00317764$$uCERN
001158708 700__ $$aAbbas, M.$$iINSPIRE-00202192$$uCERN
001158708 700__ $$aAhmed, I.$$uCERN
001158708 700__ $$aAkhtar, I.$$uCERN
001158708 700__ $$aAlbert, E.$$uCERN
001158708 700__ $$aBloch, C.$$uCERN
001158708 700__ $$aBreuker, H.$$iINSPIRE-00317899$$uCERN
001158708 700__ $$aButt, S.$$uCERN
001158708 700__ $$aBuchmuller, O.$$iINSPIRE-00069840$$uCERN
001158708 700__ $$aCattai, A.$$iINSPIRE-00320450$$uCERN
001158708 700__ $$aDelaere, C.$$iINSPIRE-00314951$$uCERN
001158708 700__ $$aDelattre, M.$$uCERN
001158708 700__ $$aEdera, L.M.$$iINSPIRE-00308711$$uCERN
001158708 700__ $$aEngstrom, P.$$uCERN
001158708 700__ $$aEppard, M.$$iINSPIRE-00320462$$uCERN
001158708 700__ $$aGateau, M.$$iINSPIRE-00309140$$uCERN
001158708 700__ $$aGill, K.$$iINSPIRE-00314018$$uCERN
001158708 700__ $$aGiolo-Nicollerat, A.-S.$$uCERN
001158708 700__ $$aGrabit, R.$$uCERN
001158708 700__ $$aHonma, A.$$iINSPIRE-00317980$$uCERN
001158708 700__ $$aHuhtinen, M.$$iINSPIRE-00320486$$uCERN
001158708 700__ $$aKloukinas, K.$$iINSPIRE-00205369$$uCERN
001158708 700__ $$aKortesmaa, J.$$iINSPIRE-00352137$$uCERN
001158708 700__ $$aKottelat, L.J.$$iINSPIRE-00391589$$uCERN
001158708 700__ $$aKuronen, A.$$uCERN
001158708 700__ $$aLeonardo, N.$$iINSPIRE-00058895$$uCERN
001158708 700__ $$aLjuslin, C.$$uCERN
001158708 700__ $$aMannelli, M.$$iINSPIRE-00318045$$uCERN
001158708 700__ $$aMasetti, L.$$iINSPIRE-00318057$$uCERN
001158708 700__ $$aMarchioro, A.$$iINSPIRE-00104633$$uCERN
001158708 700__ $$aMersi, S.$$iINSPIRE-00310594$$uCERN
001158708 700__ $$aMichal, S.$$uCERN
001158708 700__ $$aMirabito, L.$$iINSPIRE-00107928$$uCERN
001158708 700__ $$aMuffat-Joly, J.$$uCERN
001158708 700__ $$aOnnela, A.$$iINSPIRE-00314222$$uCERN
001158708 700__ $$aPaillard, C.$$uCERN
001158708 700__ $$aPal, I.$$iINSPIRE-00206864$$uCERN
001158708 700__ $$aPernot, J.F.$$iINSPIRE-00311310$$uCERN
001158708 700__ $$aPetagna, P.$$iINSPIRE-00314270$$uCERN
001158708 700__ $$aPetit, P.$$uCERN
001158708 700__ $$aPiccut, C.$$uCERN
001158708 700__ $$aPioppi, M.$$iINSPIRE-00042013$$uCERN
001158708 700__ $$aPostema, H.$$iINSPIRE-00318148$$uCERN
001158708 700__ $$aRanieri, R.$$iINSPIRE-00047530$$uCERN
001158708 700__ $$aRicci, D.$$iINSPIRE-00493662$$uCERN
001158708 700__ $$aRolandi, G.$$uCERN
001158708 700__ $$aRonga, F.$$iINSPIRE-00055600$$uCERN
001158708 700__ $$aSigaud, C.$$uCERN
001158708 700__ $$aSyed, A.$$uCERN
001158708 700__ $$aSiegrist, P.$$iINSPIRE-00318210$$uCERN
001158708 700__ $$aTropea, P.$$iINSPIRE-00312581$$uCERN
001158708 700__ $$aTroska, J.$$iINSPIRE-00318240$$uCERN
001158708 700__ $$aTsirou, A.$$iINSPIRE-00318252$$uCERN
001158708 700__ $$aVander Donckt, M.$$uCERN
001158708 700__ $$aVasey, M.$$uCERN
001158708 700__ $$aAlagoz, E.$$iINSPIRE-00319780$$uZurich U.
001158708 700__ $$aAmsler, Claude$$iINSPIRE-00318428$$uZurich U.
001158708 700__ $$aChiochia, V.$$iINSPIRE-00072997$$uZurich U.
001158708 700__ $$aRegenfus, Christian$$iINSPIRE-00161899$$uZurich U.
001158708 700__ $$aRobmann, P.$$iINSPIRE-00318434$$uZurich U.
001158708 700__ $$aRochet, J.$$uZurich U.
001158708 700__ $$aRommerskirchen, T.$$iINSPIRE-00311746$$uZurich U.
001158708 700__ $$aSchmidt, A.$$iINSPIRE-00318446$$uZurich U.
001158708 700__ $$aSteiner, S.$$iINSPIRE-00208303$$uZurich U.
001158708 700__ $$aWilke, L.$$iINSPIRE-00046661$$uZurich U.
001158708 700__ $$aChurch, I.$$uRutherford
001158708 700__ $$aCole, J.$$iINSPIRE-00318908$$uRutherford
001158708 700__ $$aCoughlan, J.$$iINSPIRE-00318771$$uRutherford
001158708 700__ $$aGay, A.$$iINSPIRE-00045629$$uRutherford
001158708 700__ $$aTaghavi, S.$$uRutherford
001158708 700__ $$aTomalin, I.$$iINSPIRE-00131746$$uRutherford
001158708 700__ $$aBainbridge, R.$$iINSPIRE-00318783$$uImperial Coll., London
001158708 700__ $$aCripps, N.$$iINSPIRE-00308285$$uImperial Coll., London
001158708 700__ $$aFulcher, J.$$iINSPIRE-00309048$$uImperial Coll., London
001158708 700__ $$aHall, G.$$iINSPIRE-00300982$$uImperial Coll., London
001158708 700__ $$aNoy, M.$$iINSPIRE-00318070$$uImperial Coll., London
001158708 700__ $$aPesaresi, M.$$iINSPIRE-00311333$$uImperial Coll., London
001158708 700__ $$aRadicci, V.$$iINSPIRE-00311590$$uImperial Coll., London
001158708 700__ $$aRaymond, D.M.$$iINSPIRE-00311667$$uImperial Coll., London
001158708 700__ $$aSharp, P.$$iINSPIRE-00314393$$uImperial Coll., London$$uCERN
001158708 700__ $$aStoye, M.$$iINSPIRE-00312258$$uImperial Coll., London
001158708 700__ $$aWingham, M.$$iINSPIRE-00318896$$uImperial Coll., London
001158708 700__ $$aZorba, O.$$iINSPIRE-00209171$$uImperial Coll., London
001158708 700__ $$aGoitom, I.$$iINSPIRE-00309201$$uBrunel U.
001158708 700__ $$aHobson, P.R.$$iINSPIRE-00090509$$uBrunel U.
001158708 700__ $$aReid, I.$$iINSPIRE-00311679$$uBrunel U.
001158708 700__ $$aTeodorescu, L.$$iINSPIRE-00043026$$uBrunel U.
001158708 700__ $$aHanson, G.$$iINSPIRE-00088533$$uUC, Riverside
001158708 700__ $$aJeng, G.-Y.$$iINSPIRE-00019705$$uUC, Riverside
001158708 700__ $$aLiu, H.$$uUC, Riverside
001158708 700__ $$aPasztor, G.$$iINSPIRE-00115001$$uUC, Riverside$$uBudapest, RMKI
001158708 700__ $$aSatpathy, A.$$iINSPIRE-00123446$$uUC, Riverside
001158708 700__ $$aStringer, R.$$iINSPIRE-00011308$$uUC, Riverside
001158708 700__ $$aMangano, B.$$iINSPIRE-00007672$$uUC, San Diego
001158708 700__ $$aAffolder, K.$$uUC, Santa Barbara
001158708 700__ $$aAffolder, T.$$uUC, Santa Barbara
001158708 700__ $$aAllen, A.$$uUC, Santa Barbara
001158708 700__ $$aBarge, D.$$iINSPIRE-00176652$$uUC, Santa Barbara
001158708 700__ $$aBurke, Samuel P.$$uUC, Santa Barbara
001158708 700__ $$aCallahan, D.$$uUC, Santa Barbara
001158708 700__ $$aCampagnari, C.$$iINSPIRE-00070758$$uUC, Santa Barbara
001158708 700__ $$aCrook, A.$$uUC, Santa Barbara
001158708 700__ $$aD'Alfonso, M.$$iINSPIRE-00308310$$uUC, Santa Barbara
001158708 700__ $$aDietch, J.$$uUC, Santa Barbara
001158708 700__ $$aGarberson, Jeffrey Ford$$iINSPIRE-00008636$$uUC, Santa Barbara
001158708 700__ $$aHale, D.$$uUC, Santa Barbara
001158708 700__ $$aIncandela, H.$$uUC, Santa Barbara
001158708 700__ $$aIncandela, J.$$iINSPIRE-00092167$$uUC, Santa Barbara
001158708 700__ $$aJaditz, S.$$iINSPIRE-00319603$$uUC, Santa Barbara
001158708 700__ $$aKalavase, P.$$iINSPIRE-00009336$$uUC, Santa Barbara
001158708 700__ $$aKreyer, S.$$uUC, Santa Barbara
001158708 700__ $$aKyre, S.$$iINSPIRE-00205590$$uUC, Santa Barbara
001158708 700__ $$aLamb, J.$$iINSPIRE-00319030$$uUC, Santa Barbara
001158708 700__ $$aMc Guinness, C.$$uUC, Santa Barbara
001158708 700__ $$aMills, C.$$uUC, Santa Barbara
001158708 700__ $$aNguyen, H.$$uUC, Santa Barbara
001158708 700__ $$aNikolic, M.$$iINSPIRE-00019331$$uUC, Santa Barbara
001158708 700__ $$aLowette, S.$$iINSPIRE-00015180$$uUC, Santa Barbara
001158708 700__ $$aRebassoo, F.$$iINSPIRE-00011252$$uUC, Santa Barbara
001158708 700__ $$aRibnik, J.$$iINSPIRE-00009348$$uUC, Santa Barbara
001158708 700__ $$aRichman, J.$$iINSPIRE-00144326$$uUC, Santa Barbara
001158708 700__ $$aRubinstein, N.$$uUC, Santa Barbara
001158708 700__ $$aSanhueza, S.$$uUC, Santa Barbara
001158708 700__ $$aShah, Y.$$iINSPIRE-00209622$$uUC, Santa Barbara
001158708 700__ $$aSimms, L.$$uUC, Santa Barbara
001158708 700__ $$aStaszak, D.$$uUC, Santa Barbara
001158708 700__ $$aStoner, J.$$uUC, Santa Barbara
001158708 700__ $$aStuart, D.$$iINSPIRE-00129447$$uUC, Santa Barbara
001158708 700__ $$aSwain, S.$$uUC, Santa Barbara
001158708 700__ $$aVlimant, J.-R.$$iINSPIRE-00049075$$uUC, Santa Barbara
001158708 700__ $$aWhite, D.$$iINSPIRE-00209825$$uUC, Santa Barbara
001158708 700__ $$aUlmer, K.A.$$iINSPIRE-00042780$$uColorado U.
001158708 700__ $$aWagner, S.R.$$iINSPIRE-00134528$$uColorado U.
001158708 700__ $$aBagby, L.$$iINSPIRE-00063740$$uFermilab
001158708 700__ $$aBhat, P.C.$$iINSPIRE-00066824$$uFermilab
001158708 700__ $$aBurkett, K.$$iINSPIRE-00070158$$uFermilab
001158708 700__ $$aCihangir, S.$$iINSPIRE-00073533$$uFermilab
001158708 700__ $$aGutsche, O.$$iINSPIRE-00319172$$uFermilab
001158708 700__ $$aJensen, H.$$iINSPIRE-00093329$$uFermilab
001158708 700__ $$aJohnson, M.$$iINSPIRE-00093653$$uFermilab
001158708 700__ $$aLuzhetskiy, N.$$uFermilab
001158708 700__ $$aMason, D.$$iINSPIRE-00105472$$uFermilab
001158708 700__ $$aMiao, T.$$iINSPIRE-00107355$$uFermilab
001158708 700__ $$aMoccia, S.$$iINSPIRE-00310697$$uFermilab
001158708 700__ $$aNoeding, C.$$iINSPIRE-00038804$$uFermilab
001158708 700__ $$aRonzhin, A.$$iINSPIRE-00121104$$uFermilab
001158708 700__ $$aSkup, E.$$iINSPIRE-00319263$$uFermilab
001158708 700__ $$aSpalding, W.J.$$iINSPIRE-00128031$$uFermilab
001158708 700__ $$aSpiegel, L.$$iINSPIRE-00128141$$uFermilab
001158708 700__ $$aTkaczyk, S.$$iINSPIRE-00131631$$uFermilab
001158708 700__ $$aYumiceva, F.$$iINSPIRE-00137869$$uFermilab
001158708 700__ $$aZatserklyaniy, A.$$uFermilab
001158708 700__ $$aZerev, E.$$uFermilab
001158708 700__ $$aAnghel, I.$$iINSPIRE-00008567$$uIllinois U., Chicago
001158708 700__ $$aBazterra, V.E.$$iINSPIRE-00011503$$uIllinois U., Chicago
001158708 700__ $$aGerber, C.E.$$iINSPIRE-00084394$$uIllinois U., Chicago
001158708 700__ $$aKhalatian, S.$$iINSPIRE-00008916$$uIllinois U., Chicago
001158708 700__ $$aShabalina, E.$$uIllinois U., Chicago
001158708 700__ $$aBaringer, Philip S.$$iINSPIRE-00064543$$uKansas U.
001158708 700__ $$aBean, A.$$iINSPIRE-00065301$$uKansas U.
001158708 700__ $$aChen, J.$$uKansas U.
001158708 700__ $$aHinchey, C.$$uKansas U.
001158708 700__ $$aMartin, C.$$iINSPIRE-00374510$$uKansas U.
001158708 700__ $$aMoulik, T.$$iINSPIRE-00109266$$uKansas U.
001158708 700__ $$aRobinson, R.$$uKansas U.
001158708 700__ $$aGritsan, A.V.$$iINSPIRE-00086850$$uJohns Hopkins U.
001158708 700__ $$aLae, C.K.$$iINSPIRE-00042253$$uJohns Hopkins U.
001158708 700__ $$aTran, N.V.$$iINSPIRE-00319500$$uJohns Hopkins U.
001158708 700__ $$aEveraerts, P.$$iINSPIRE-00308780$$uMIT, LNS
001158708 700__ $$aHahn, K.A.$$iINSPIRE-00032436$$uMIT, LNS
001158708 700__ $$aHarris, P.$$iINSPIRE-00319597$$uMIT, LNS
001158708 700__ $$aNahn, S.$$iINSPIRE-00110103$$uMIT, LNS
001158708 700__ $$aRudolph, M.$$iINSPIRE-00176709$$uMIT, LNS
001158708 700__ $$aSung, K.$$iINSPIRE-00312313$$uMIT, LNS
001158708 700__ $$aBetchart, B.$$iINSPIRE-00011868$$uRochester U.
001158708 700__ $$aDemina, R.$$iINSPIRE-00076615$$uRochester U.
001158708 700__ $$aGotra, Y.$$iINSPIRE-00086051$$uRochester U.
001158708 700__ $$aKorjenevski, S.$$iINSPIRE-00004874$$uRochester U.
001158708 700__ $$aMiner, D.$$iINSPIRE-00008862$$uRochester U.
001158708 700__ $$aOrbaker, D.$$iINSPIRE-00011882$$uRochester U.
001158708 700__ $$aChristofek, L.$$uBrown U.
001158708 700__ $$aHooper, R.$$iINSPIRE-00090936$$uBrown U.
001158708 700__ $$aLandsberg, G.$$iINSPIRE-00099870$$uBrown U.
001158708 700__ $$aNguyen, D.$$iINSPIRE-00009056$$uBrown U.
001158708 700__ $$aNarain, M.$$iINSPIRE-00110455$$uBrown U.
001158708 700__ $$aSpeer, T.$$iINSPIRE-00128088$$uBrown U.
001158708 700__ $$aTsang, K.V.$$iINSPIRE-00028609$$uBrown U.
001158708 710__ $$5PH-EP
001158708 710__ $$gCMS Tracker Collaboration
001158708 773__ $$cP06009$$pJINST$$v4$$y2009
001158708 8564_ $$uhttp://lss.fnal.gov/archive/2009/pub/fermilab-pub-09-546-cms.pdf$$yPreprint
001158708 8564_ $$81410770$$s3358069$$uhttps://cds.cern.ch/record/1158708/files/arXiv:0901.4316.pdf
001158708 8564_ $$8526683$$s3556230$$uhttps://cds.cern.ch/record/1158708/files/jinst9_06_p06009.pdf
001158708 8564_ $$81410744$$s33848$$uhttps://cds.cern.ch/record/1158708/files/Figures_ScorDet300.png$$y00061 \sl Signal corrected for the track angle ($S_{ren}$), in full curve without electronic gain calibration and in dots with it.
001158708 8564_ $$81410745$$s12886$$uhttps://cds.cern.ch/record/1158708/files/Figures_TEC-noise-11413-R3.png$$y00039 \sl Noise profiles for T= $-10\,^{\circ}\mathrm{C}$ for different rings of TEC and TID. Gaussian fits are shown. R2 and R3 silicon geometries are the same for TID and TEC. X axis is ADC value
001158708 8564_ $$81410746$$s168362$$uhttps://cds.cern.ch/record/1158708/files/ScorDet000SimuReal.png$$y00023 \sl Signal distribution for clusters on tracks in data (dashed line) and Monte Carlo (solid line). From left to right: TIB, TOB and TEC
001158708 8564_ $$81410747$$s12519$$uhttps://cds.cern.ch/record/1158708/files/Figures_TEC-noise-11413-R1.png$$y00035 \sl Noise profiles for T= $-10\,^{\circ}\mathrm{C}$ for different rings of TEC and TID. Gaussian fits are shown. R2 and R3 silicon geometries are the same for TID and TEC. X axis is ADC value
001158708 8564_ $$81410748$$s13318$$uhttps://cds.cern.ch/record/1158708/files/Figures_TEC-noise-11413-R7.png$$y00043 \sl Noise profiles for T= $-10\,^{\circ}\mathrm{C}$ for different rings of TEC and TID. Gaussian fits are shown. R2 and R3 silicon geometries are the same for TID and TEC. X axis is ADC value
001158708 8564_ $$81410749$$s13011$$uhttps://cds.cern.ch/record/1158708/files/Figures_TEC-noise-11413-R6.png$$y00042 \sl Noise profiles for T= $-10\,^{\circ}\mathrm{C}$ for different rings of TEC and TID. Gaussian fits are shown. R2 and R3 silicon geometries are the same for TID and TEC. X axis is ADC value
001158708 8564_ $$81410750$$s13102$$uhttps://cds.cern.ch/record/1158708/files/Figures_TEC-noise-11413-R5.png$$y00041 \sl Noise profiles for T= $-10\,^{\circ}\mathrm{C}$ for different rings of TEC and TID. Gaussian fits are shown. R2 and R3 silicon geometries are the same for TID and TEC. X axis is ADC value
001158708 8564_ $$81410751$$s12977$$uhttps://cds.cern.ch/record/1158708/files/Figures_TEC-noise-11413-R4.png$$y00040 \sl Noise profiles for T= $-10\,^{\circ}\mathrm{C}$ for different rings of TEC and TID. Gaussian fits are shown. R2 and R3 silicon geometries are the same for TID and TEC. X axis is ADC value
001158708 8564_ $$81410752$$s197253$$uhttps://cds.cern.ch/record/1158708/files/Figures_ScorDet200SimuReal.png$$y00076 \sl Signal distribution for clusters on tracks in data (dashed line) and Monte Carlo (solid line). From left to right: TIB, TOB and TEC
001158708 8564_ $$81410753$$s17175$$uhttps://cds.cern.ch/record/1158708/files/Figures_FitSNcorYZDet001MP-10-C-VR-cal.png$$y00056 \sl $S_{ren}$/N dependence on K for tracks perpendicular to the strip direction (open triangles) , i.e. the XZ local direction, and  for tracks parallel to the strip direction (black circles) , i.e. the YZ local direction, for TIB and TOB.
001158708 8564_ $$81410754$$s83291$$uhttps://cds.cern.ch/record/1158708/files/TrackerHits_R_z_bw.png$$y00022 \em Hit distribution for the cosmic muons in the x-y(left) and y-z(right) plane in Configuration TC
001158708 8564_ $$81410755$$s52701$$uhttps://cds.cern.ch/record/1158708/files/Figures_SNcorDet-12099-10-C-VR-cal.png$$y00053 \sl The signal-to-noise corrected for the track angle for TIB and TOB layers at $T=-10\,^{\circ}\mathrm{C}$.
001158708 8564_ $$81410756$$s19825$$uhttps://cds.cern.ch/record/1158708/files/noise_vs_run_tob_postVPSP.png$$y00007 \sl Noise vs run number for TIB on the left and for TOB on the right.Four periods at different temperatures are visible: $10\,^{\circ}\mathrm{C}$, $0\,^{\circ}\mathrm{C}$, $-10\,^{\circ}\mathrm{C}$ and $-15\,^{\circ}\mathrm{C}$
001158708 8564_ $$81410757$$s19868$$uhttps://cds.cern.ch/record/1158708/files/Figures_Sensor_temp_Warm_TEC.png$$y00014 \sl Sensor temperature distributions at a coolant temperature of $15\,^{\circ}\mathrm{C}$ for TIB, TID, TOB, and TEC.
001158708 8564_ $$81410758$$s25881$$uhttps://cds.cern.ch/record/1158708/files/Figures_Historic_NoisyDead_TEC.png$$y00049 \sl Noisy and dead strips vs run for TIB, TID, TOB, and TEC.
001158708 8564_ $$81410759$$s19825$$uhttps://cds.cern.ch/record/1158708/files/Figures_noise_vs_run_tob_postVPSP.png$$y00044 \sl Noise vs run number for TIB on the left and for TOB on the right. Four periods at different temperatures are visible: $10\,^{\circ}\mathrm{C}$, $0\,^{\circ}\mathrm{C}$, $-10\,^{\circ}\mathrm{C}$ and $-15\,^{\circ}\mathrm{C}$
001158708 8564_ $$81410760$$s19688$$uhttps://cds.cern.ch/record/1158708/files/Figures_Hybrid_temp_Warm_TEC.png$$y00010 \sl Hybrid temperature distributions for TIB, TID, TOB, and TEC at a coolant temperature of $14\,^{\circ}\mathrm{C}$.
001158708 8564_ $$81410761$$s21784$$uhttps://cds.cern.ch/record/1158708/files/Figures_ClusterWidth_Track_Perp_TOB_PosC_p10deg_CTF.png$$y00089 \sl Cluster width for TIB(left) and TOB(right) hits on perpendicular tracks. The black points represent the data, the histogram is obtained from simulation with a 3\% capacitive coupling where the gray band represents the statistical uncertainty.
001158708 8564_ $$81410762$$s13062$$uhttps://cds.cern.ch/record/1158708/files/Figures_TEC-noise-11413-R2.png$$y00037 \sl Noise profiles for T= $-10\,^{\circ}\mathrm{C}$ for different rings of TEC and TID. Gaussian fits are shown. R2 and R3 silicon geometries are the same for TID and TEC. X axis is ADC value
001158708 8564_ $$81410763$$s27328$$uhttps://cds.cern.ch/record/1158708/files/Figures_FitScorDet001MP-10-C-VR-cal.png$$y00062 \sl Distribution of signal ($S_{ren}$) most probable value, module per module for TIB (top left), TEC thin sensors (top right), TOB (bottom left), and TEC thick (bottom right).
001158708 8564_ $$81410764$$s22236$$uhttps://cds.cern.ch/record/1158708/files/Figures_timing_norm_ticks_new.png$$y00025 \sl Tickmark height distribution versus run number. Error bars represent the statistical error of the average value.
001158708 8564_ $$81410765$$s16681$$uhttps://cds.cern.ch/record/1158708/files/Figures_V250_Warm_TEC_good.png$$y00018 \sl 2.5\,V voltage line value measured at the module for TOB, TIB, TEC, and TID.
001158708 8564_ $$81410766$$s192229$$uhttps://cds.cern.ch/record/1158708/files/SNcorDet300SimuReal.png$$y00028 \sl Signal to noise distribution for clusters on tracks in data (dashed line) and Monte Carlo (solid line). From left to right: TIB, TOB and TEC
001158708 8564_ $$81410767$$s18591$$uhttps://cds.cern.ch/record/1158708/files/Figures_ClusterWidthTrack_TOB.png$$y00083 \sl Cluster width for TIB(left) and TOB(right) hits for all tracks and perpendicular tracks
001158708 8564_ $$81410768$$s16042$$uhttps://cds.cern.ch/record/1158708/files/Figures_eta_s_TIB_ZS_3CC.png$$y00086 \sl $\eta$ function for TIB(left) and TOB(right) clusters The data are from Zero Suppressed runs compared with Monte Carlo with 3\% capacitive coupling.
001158708 8564_ $$81410769$$s27545$$uhttps://cds.cern.ch/record/1158708/files/Figures_Historic_NoisyDead_TOB.png$$y00048 \sl Noisy and dead strips vs run for TIB, TID, TOB, and TEC.
001158708 8564_ $$81410771$$s197253$$uhttps://cds.cern.ch/record/1158708/files/ScorDet200SimuReal.png$$y00024 \sl Signal distribution for clusters on tracks in data (dashed line) and Monte Carlo (solid line). From left to right: TIB, TOB and TEC
001158708 8564_ $$81410772$$s168362$$uhttps://cds.cern.ch/record/1158708/files/Figures_ScorDet000SimuReal.png$$y00075 \sl Signal distribution for clusters on tracks in data (dashed line) and Monte Carlo (solid line). From left to right: TIB, TOB and TEC
001158708 8564_ $$81410773$$s32693$$uhttps://cds.cern.ch/record/1158708/files/latencyHistoryPlateauSubdetsCorrFactor.png$$y00012 \sl Offset from the on-peak timing (left) and signal correction factor (right) as function of the run number for thethree sub-detectors TIB/TID, TOB, and TEC.
001158708 8564_ $$81410774$$s176558$$uhttps://cds.cern.ch/record/1158708/files/Figures_SNcorDet000SimuReal.png$$y00077 \sl Signal to noise distribution for clusters on tracks in data (dashed line) and Monte Carlo (solid line). From left to right: TIB, TOB and TEC
001158708 8564_ $$81410775$$s161260$$uhttps://cds.cern.ch/record/1158708/files/Figures_SNcorDet200SimuReal.png$$y00078 \sl Signal to noise distribution for clusters on tracks in data (dashed line) and Monte Carlo (solid line). From left to right: TIB, TOB and TEC
001158708 8564_ $$81410776$$s18925$$uhttps://cds.cern.ch/record/1158708/files/Figures_Angle_XZ_TOB.png$$y00081 \sl Local angle of incidence (XZ) for tracks on sensors in data (points) and MC (histogram) for TIB(left) and TOB(right)
001158708 8564_ $$81410777$$s87252$$uhttps://cds.cern.ch/record/1158708/files/Figures_TrackerHits_x_y_bw.png$$y00072 \em Hit distribution for the cosmic muons in the x-y(left) and y-z(right) plane in Configuration TC
001158708 8564_ $$81410778$$s17190$$uhttps://cds.cern.ch/record/1158708/files/Figures_V250_Warm_TOB_good.png$$y00017 \sl 2.5\,V voltage line value measured at the module for TOB, TIB, TEC, and TID.
001158708 8564_ $$81410779$$s188130$$uhttps://cds.cern.ch/record/1158708/files/triggerlayout_xy_positionA.png$$y00000  Layout of the various trigger scintillator configurations used during the cosmic data taking at the TIF (in chronological order): (a) configuration TA; (b) configuration TB; (c) configuration TC. The $xy$ view is shown on the left side, the $rz$ view is shown on the right. The straight lines connecting the active areas of the top and bottom scintillation counters indicate theacceptance region.
001158708 8564_ $$81410780$$s268353$$uhttps://cds.cern.ch/record/1158708/files/triggerlayout_xy_positionB.png$$y00002  Layout of the various trigger scintillator configurations used during the cosmic data taking at the TIF (in chronological order): (a) configuration TA; (b) configuration TB; (c) configuration TC. The $xy$ view is shown on the left side, the $rz$ view is shown on the right. The straight lines connecting the active areas of the top and bottom scintillation counters indicate theacceptance region.
001158708 8564_ $$81410781$$s191949$$uhttps://cds.cern.ch/record/1158708/files/triggerlayout_xy_positionC.png$$y00004  Layout of the various trigger scintillator configurations used during the cosmic data taking at the TIF (in chronological order): (a) configuration TA; (b) configuration TB; (c) configuration TC. The $xy$ view is shown on the left side, the $rz$ view is shown on the right. The straight lines connecting the active areas of the top and bottom scintillation counters indicate theacceptance region.
001158708 8564_ $$81410782$$s17883$$uhttps://cds.cern.ch/record/1158708/files/Figures_StripOccupancyPerRun_TEC_S2Nabove20_log.png$$y00069 \sl Distribution of strip occupancy for TIB and TEC: upper (lower) plots for S/N below (above) 20.
001158708 8564_ $$81410783$$s15476$$uhttps://cds.cern.ch/record/1158708/files/Figures_V125_Warm_TIB_good.png$$y00019 \sl 1.25\,voltage line value measured at the module for TOB, TIB, TEC, and TID.
001158708 8564_ $$81410784$$s12940$$uhttps://cds.cern.ch/record/1158708/files/StoNTIB_TIF-1.png$$y00013 \sl Signal over noise corrected for the track angle: from the left to the right for TIB and TOB.
001158708 8564_ $$81410785$$s161260$$uhttps://cds.cern.ch/record/1158708/files/SNcorDet200SimuReal.png$$y00027 \sl Signal to noise distribution for clusters on tracks in data (dashed line) and Monte Carlo (solid line). From left to right: TIB, TOB and TEC
001158708 8564_ $$81410786$$s227944$$uhttps://cds.cern.ch/record/1158708/files/Figures_modul_komplett-a-sw_neu.png$$y00053 \sl Angle definitions: $\theta_{3D}$ on the left; $\theta_{XZ}$ on the right.
001158708 8564_ $$81410787$$s12940$$uhttps://cds.cern.ch/record/1158708/files/Figures_StoNTIB_TIF-1.png$$y00055 \sl Signal over noise corrected for the track angle: from the left to the right for TIB and TOB.
001158708 8564_ $$81410788$$s28335$$uhttps://cds.cern.ch/record/1158708/files/Figures_FitScorDet301MP-10-C-VR-cal-thin.png$$y00063 \sl Distribution of signal ($S_{ren}$) most probable value, module per module for TIB (top left), TEC thin sensors (top right), TOB (bottom left), and TEC thick (bottom right).
001158708 8564_ $$81410789$$s33244$$uhttps://cds.cern.ch/record/1158708/files/Figures_ScorDet100.png$$y00059 \sl Signal corrected for the track angle ($S_{ren}$), in full curve without electronic gain calibration and in dots with it.
001158708 8564_ $$81410790$$s14259$$uhttps://cds.cern.ch/record/1158708/files/Figures_V125_Warm_TID_good.png$$y00020 \sl 1.25\,voltage line value measured at the module for TOB, TIB, TEC, and TID.
001158708 8564_ $$81410791$$s53385$$uhttps://cds.cern.ch/record/1158708/files/latencyHistory.png$$y00011 \sl Offset from the on-peak timing (left) and signal correction factor (right) as function of the run number for thethree sub-detectors TIB/TID, TOB, and TEC.
001158708 8564_ $$81410792$$s30197$$uhttps://cds.cern.ch/record/1158708/files/Figures_ScorDet200.png$$y00060 \sl Signal corrected for the track angle ($S_{ren}$), in full curve without electronic gain calibration and in dots with it.
001158708 8564_ $$81410793$$s16598$$uhttps://cds.cern.ch/record/1158708/files/Figures_noise_vs_run_tib_postVPSP.png$$y00046 \sl Noise vs run number for TIB on the left and for TOB on the right. Four periods at different temperatures are visible: $10\,^{\circ}\mathrm{C}$, $0\,^{\circ}\mathrm{C}$, $-10\,^{\circ}\mathrm{C}$ and $-15\,^{\circ}\mathrm{C}$
001158708 8564_ $$81410794$$s48948$$uhttps://cds.cern.ch/record/1158708/files/Figures_subdets_10947_version2.png$$y00055 \sl. Fit of the signal as a function of the latency, for each of the four sub-detectors. Data are from run 10947 and were used to set the latency for the following period.
001158708 8564_ $$81410795$$s32693$$uhttps://cds.cern.ch/record/1158708/files/Figures_latencyHistoryPlateauSubdetsCorrFactor.png$$y00052 \sl Offset from the on-peak timing (left) and signal correction factor (right) as function of the run number for the three sub-detectors TIB/TID, TOB, and TEC.
001158708 8564_ $$81410796$$s14872$$uhttps://cds.cern.ch/record/1158708/files/BarrelEffRoomT.png$$y00015 \sl Summary of layer efficiency at room temperature (left) and at$T=-10\,^{\circ}\mathrm{C}$ (right).
001158708 8564_ $$81410797$$s16782$$uhttps://cds.cern.ch/record/1158708/files/Figures_noise_vs_length_11406.png$$y00045 \sl Noise vs strip length for T= $-10\,^{\circ}\mathrm{C}$.
001158708 8564_ $$81410798$$s268353$$uhttps://cds.cern.ch/record/1158708/files/Figures_triggerlayout_xy_positionB.png$$y00003  Layout of the various trigger scintillator configurations used during the cosmic data taking at the TIF (in chronological order): (a) configuration TA; (b) configuration TB; (c) configuration TC. The $xy$ view is shown on the left side, the $rz$ view is shown on the right. The straight lines connecting the active areas of the top and bottom scintillation counters indicate the acceptance region.
001158708 8564_ $$81410799$$s191949$$uhttps://cds.cern.ch/record/1158708/files/Figures_triggerlayout_xy_positionC.png$$y00005  Layout of the various trigger scintillator configurations used during the cosmic data taking at the TIF (in chronological order): (a) configuration TA; (b) configuration TB; (c) configuration TC. The $xy$ view is shown on the left side, the $rz$ view is shown on the right. The straight lines connecting the active areas of the top and bottom scintillation counters indicate the acceptance region.
001158708 8564_ $$81410800$$s188130$$uhttps://cds.cern.ch/record/1158708/files/Figures_triggerlayout_xy_positionA.png$$y00001  Layout of the various trigger scintillator configurations used during the cosmic data taking at the TIF (in chronological order): (a) configuration TA; (b) configuration TB; (c) configuration TC. The $xy$ view is shown on the left side, the $rz$ view is shown on the right. The straight lines connecting the active areas of the top and bottom scintillation counters indicate the acceptance region.
001158708 8564_ $$81410801$$s83291$$uhttps://cds.cern.ch/record/1158708/files/Figures_TrackerHits_R_z_bw.png$$y00073 \em Hit distribution for the cosmic muons in the x-y(left) and y-z(right) plane in Configuration TC
001158708 8564_ $$81410802$$s22232$$uhttps://cds.cern.ch/record/1158708/files/Figures_ClusterWidth_Track_Perp_TIB_PosC_p10deg_CTF.png$$y00088 \sl Cluster width for TIB(left) and TOB(right) hits on perpendicular tracks. The black points represent the data, the histogram is obtained from simulation with a 3\% capacitive coupling where the gray band represents the statistical uncertainty.
001158708 8564_ $$81410803$$s50681$$uhttps://cds.cern.ch/record/1158708/files/Figures_WidthvsAngle_Pass3_MC_All.png$$y00093 \sl Cluster width versus $\theta_t$ for barrel layers on real data (crosses) compared with Monte Carlo (triangles) using capacitive coupling of 3\%.
001158708 8564_ $$81410804$$s6619$$uhttps://cds.cern.ch/record/1158708/files/MuonEta_confA.png$$y00017 \em Cosmic muon track parameters: $\phi$(left), $\eta$ for scintillator Conf(TA)(middle) and Conf(TC)(right)
001158708 8564_ $$81410805$$s6216$$uhttps://cds.cern.ch/record/1158708/files/MuonEta_confC.png$$y00018 \em Cosmic muon track parameters: $\phi$(left), $\eta$ for scintillator Conf(TA)(middle) and Conf(TC)(right)
001158708 8564_ $$81410806$$s16672$$uhttps://cds.cern.ch/record/1158708/files/Figures_V125_Warm_TOB_good.png$$y00019 \sl 1.25\,voltage line value measured at the module for TOB, TIB, TEC, and TID.
001158708 8564_ $$81410807$$s16042$$uhttps://cds.cern.ch/record/1158708/files/eta_s_TIB_ZS_3CC.png$$y00031 \sl $\eta$ function for TIB(left) and TOB(right) clusters The data are from Zero Suppressed runs compared with Monte Carlo with 3\% capacitivecoupling.
001158708 8564_ $$81410808$$s14853$$uhttps://cds.cern.ch/record/1158708/files/Figures_timing_11176.png$$y00022 \sl APV25 tickmark height distribution after commissioning procedure: run 7096, taken at $T=14\,^{\circ}\mathrm{C}$ (left), and run 11176, taken at $T=-10\,^{\circ}\mathrm{C}$ (right).
001158708 8564_ $$81410809$$s16015$$uhttps://cds.cern.ch/record/1158708/files/Figures_Sensor_temp_Warm_TID.png$$y00010 \sl Sensor temperature distributions at a coolant temperature of $15\,^{\circ}\mathrm{C}$ for TIB, TID, TOB, and TEC.
001158708 8564_ $$81410810$$s18410$$uhttps://cds.cern.ch/record/1158708/files/Figures_FitSNcorYZDet201MP-10-C-VR-cal.png$$y00057 \sl $S_{ren}$/N dependence on K for tracks perpendicular to the strip direction (open triangles) , i.e. the XZ local direction, and  for tracks parallel to the strip direction (black circles) , i.e. the YZ local direction, for TIB and TOB.
001158708 8564_ $$81410811$$s29150$$uhttps://cds.cern.ch/record/1158708/files/Figures_FitScorDet201MP-10-C-VR-cal.png$$y00064 \sl Distribution of signal ($S_{ren}$) most probable value, module per module for TIB (top left), TEC thin sensors (top right), TOB (bottom left), and TEC thick (bottom right).
001158708 8564_ $$81410812$$s16503$$uhttps://cds.cern.ch/record/1158708/files/Figures_Sensor_temp_Warm_TIB.png$$y00009 \sl Sensor temperature distributions at a coolant temperature of $15\,^{\circ}\mathrm{C}$ for TIB, TID, TOB, and TEC.
001158708 8564_ $$81410813$$s14872$$uhttps://cds.cern.ch/record/1158708/files/Figures_BarrelEffRoomT.png$$y00070 \sl Summary of layer efficiency at room temperature (left) and at $T=-10\,^{\circ}\mathrm{C}$ (right).
001158708 8564_ $$81410814$$s6216$$uhttps://cds.cern.ch/record/1158708/files/Figures_MuonEta_confC.png$$y00081 \em Cosmic muon track parameters: $\phi$(left), $\eta$ for scintillator Conf(TA)(middle) and Conf(TC)(right)
001158708 8564_ $$81410815$$s6619$$uhttps://cds.cern.ch/record/1158708/files/Figures_MuonEta_confA.png$$y00080 \em Cosmic muon track parameters: $\phi$(left), $\eta$ for scintillator Conf(TA)(middle) and Conf(TC)(right)
001158708 8564_ $$81410816$$s14891$$uhttps://cds.cern.ch/record/1158708/files/Figures_BarrelEffMinus10Degree.png$$y00071 \sl Summary of layer efficiency at room temperature (left) and at $T=-10\,^{\circ}\mathrm{C}$ (right).
001158708 8564_ $$81410817$$s30815$$uhttps://cds.cern.ch/record/1158708/files/Figures_FitScorDet301MP-10-C-VR-cal-thick.png$$y00065 \sl Distribution of signal ($S_{ren}$) most probable value, module per module for TIB (top left), TEC thin sensors (top right), TOB (bottom left), and TEC thick (bottom right).
001158708 8564_ $$81410818$$s17742$$uhttps://cds.cern.ch/record/1158708/files/Figures_V125_Warm_TEC_good.png$$y00020 \sl 1.25\,voltage line value measured at the module for TOB, TIB, TEC, and TID.
001158708 8564_ $$81410819$$s16095$$uhttps://cds.cern.ch/record/1158708/files/StoNTOB_TIF-1.png$$y00012 \sl Signal over noise corrected for the track angle: from the left to the right for TIB and TOB.
001158708 8564_ $$81410820$$s12547$$uhttps://cds.cern.ch/record/1158708/files/Figures_TID-noise-11413-R2.png$$y00036 \sl Noise profiles for T= $-10\,^{\circ}\mathrm{C}$ for different rings of TEC and TID. Gaussian fits are shown. R2 and R3 silicon geometries are the same for TID and TEC. X axis is ADC value
001158708 8564_ $$81410821$$s12617$$uhttps://cds.cern.ch/record/1158708/files/Figures_TID-noise-11413-R3.png$$y00038 \sl Noise profiles for T= $-10\,^{\circ}\mathrm{C}$ for different rings of TEC and TID. Gaussian fits are shown. R2 and R3 silicon geometries are the same for TID and TEC. X axis is ADC value
001158708 8564_ $$81410822$$s12719$$uhttps://cds.cern.ch/record/1158708/files/Figures_TID-noise-11413-R1.png$$y00034 \sl Noise profiles for T= $-10\,^{\circ}\mathrm{C}$ for different rings of TEC and TID. Gaussian fits are shown. R2 and R3 silicon geometries are the same for TID and TEC. X axis is ADC value
001158708 8564_ $$81410823$$s6930$$uhttps://cds.cern.ch/record/1158708/files/MuonPhi_confC.png$$y00016 \em Cosmic muon track parameters: $\phi$(left), $\eta$ for scintillator Conf(TA)(middle) and Conf(TC)(right)
001158708 8564_ $$81410824$$s50884$$uhttps://cds.cern.ch/record/1158708/files/Figures_TIF_MC_WidthvsAngle.png$$y00090 \sl Cluster width versus $\theta_t$ for barrel layers on Monte Carlo simulated data using capacitive coupling of 7\%(triangles) and 3\% (crosses).
001158708 8564_ $$81410825$$s6930$$uhttps://cds.cern.ch/record/1158708/files/Figures_MuonPhi_confC.png$$y00079 \em Cosmic muon track parameters: $\phi$(left), $\eta$ for scintillator Conf(TA)(middle) and Conf(TC)(right)
001158708 8564_ $$81410826$$s18077$$uhttps://cds.cern.ch/record/1158708/files/Figures_Hybrid_temp_Warm_TIB.png$$y00005 \sl Hybrid temperature distributions for TIB, TID, TOB, and TEC at a coolant temperature of $14\,^{\circ}\mathrm{C}$.
001158708 8564_ $$81410827$$s87252$$uhttps://cds.cern.ch/record/1158708/files/TrackerHits_x_y_bw.png$$y00021 \em Hit distribution for the cosmic muons in the x-y(left) and y-z(right) plane in Configuration TC
001158708 8564_ $$81410828$$s176558$$uhttps://cds.cern.ch/record/1158708/files/SNcorDet000SimuReal.png$$y00026 \sl Signal to noise distribution for clusters on tracks in data (dashed line) and Monte Carlo (solid line). From left to right: TIB, TOB and TEC
001158708 8564_ $$81410829$$s10439$$uhttps://cds.cern.ch/record/1158708/files/EtaSymm_VR_TOB.png$$y00030 \sl $\eta$ function for TIB(left) and TOB(right) clusters. The data are from Virgin Raw runs where the information of the strips below the clustering threshold isavailable.
001158708 8564_ $$81410830$$s14763$$uhttps://cds.cern.ch/record/1158708/files/Figures_V250_Warm_TIB_good.png$$y00013 \sl 2.5\,V voltage line value measured at the module for TOB, TIB, TEC, and TID.
001158708 8564_ $$81410831$$s59196$$uhttps://cds.cern.ch/record/1158708/files/Figures_SNcorDet-13099-10-C-VR-cal.png$$y00054 \sl The signal-to-noise corrected for the track angle for TID and TEC rings at $T=-10\,^{\circ}\mathrm{C}$
001158708 8564_ $$81410832$$s192229$$uhttps://cds.cern.ch/record/1158708/files/Figures_SNcorDet300SimuReal.png$$y00079 \sl Signal to noise distribution for clusters on tracks in data (dashed line) and Monte Carlo (solid line). From left to right: TIB, TOB and TEC
001158708 8564_ $$81410833$$s19043$$uhttps://cds.cern.ch/record/1158708/files/Figures_Angle_XZ_TIB.png$$y00080 \sl Local angle of incidence (XZ) for tracks on sensors in data (points) and MC (histogram) for TIB(left) and TOB(right)
001158708 8564_ $$81410834$$s10334$$uhttps://cds.cern.ch/record/1158708/files/Figures_CAPRICECMSCGEN_corr.png$$y00078 \em The CMSCGEN cosmic muons energy spectrum. Below 2 GeV the events are reweighted according to the CAPRICE spectrum.
001158708 8564_ $$81410835$$s488200$$uhttps://cds.cern.ch/record/1158708/files/modul_komplett-sw_neu.png$$y00009 \sl Angle definitions: $\theta_{3D}$ on the left;$\theta_{XZ}$ on the right.
001158708 8564_ $$81410836$$s47775$$uhttps://cds.cern.ch/record/1158708/files/Figures_WidthvsAngle_Pass3_TIB.png$$y00091 \sl Cluster width versus $\theta_t$ for TIB layers.
001158708 8564_ $$81410837$$s9008$$uhttps://cds.cern.ch/record/1158708/files/Figures_EtaSymm_VR_TIB.png$$y00084 \sl $\eta$ function for TIB(left) and TOB(right) clusters. The data are from Virgin Raw runs where the information of the strips below the clustering threshold is available.
001158708 8564_ $$81410838$$s9008$$uhttps://cds.cern.ch/record/1158708/files/EtaSymm_VR_TIB.png$$y00029 \sl $\eta$ function for TIB(left) and TOB(right) clusters. The data are from Virgin Raw runs where the information of the strips below the clustering threshold isavailable.
001158708 8564_ $$81410839$$s16439$$uhttps://cds.cern.ch/record/1158708/files/Figures_Hybrid_temp_Warm_TID.png$$y00008 \sl Hybrid temperature distributions for TIB, TID, TOB, and TEC at a coolant temperature of $14\,^{\circ}\mathrm{C}$.
001158708 8564_ $$81410840$$s18568$$uhttps://cds.cern.ch/record/1158708/files/Figures_StripOccupancyPerRun_TIB_S2Nless20_log.png$$y00066 \sl Distribution of strip occupancy for TIB and TEC: upper (lower) plots for S/N below (above) 20.
001158708 8564_ $$81410841$$s10334$$uhttps://cds.cern.ch/record/1158708/files/CAPRICECMSCGEN_corr.png$$y00015 \em The CMSCGEN cosmic muons energy spectrum. Below 2 GeV the events arereweighted according to the CAPRICE spectrum.
001158708 8564_ $$81410842$$s14891$$uhttps://cds.cern.ch/record/1158708/files/BarrelEffMinus10Degree.png$$y00016 \sl Summary of layer efficiency at room temperature (left) and at$T=-10\,^{\circ}\mathrm{C}$ (right).
001158708 8564_ $$81410843$$s15343$$uhttps://cds.cern.ch/record/1158708/files/Figures_timing_7222.png$$y00021 \sl APV25 tickmark height distribution after commissioning procedure: run 7096, taken at $T=14\,^{\circ}\mathrm{C}$ (left), and run 11176, taken at $T=-10\,^{\circ}\mathrm{C}$ (right).
001158708 8564_ $$81410844$$s35112$$uhttps://cds.cern.ch/record/1158708/files/Figures_NoisevsStriplength.png$$y00074 \sl Measured noise in the various sub-detectors as a function of strip length compared with the Monte Carlo parameterization. The band corresponds to the spread of the mean noise in the layer.
001158708 8564_ $$81410845$$s21178$$uhttps://cds.cern.ch/record/1158708/files/Figures_Sensor_temp_Warm_TOB.png$$y00011 \sl Sensor temperature distributions at a coolant temperature of $15\,^{\circ}\mathrm{C}$ for TIB, TID, TOB, and TEC.
001158708 8564_ $$81410846$$s227944$$uhttps://cds.cern.ch/record/1158708/files/modul_komplett-a-sw_neu.png$$y00006 \sl Angle definitions: $\theta_{3D}$ on the left;$\theta_{XZ}$ on the right.
001158708 8564_ $$81410847$$s16166$$uhttps://cds.cern.ch/record/1158708/files/eta_s_TOB_ZS_3CC.png$$y00032 \sl $\eta$ function for TIB(left) and TOB(right) clusters The data are from Zero Suppressed runs compared with Monte Carlo with 3\% capacitivecoupling.
001158708 8564_ $$81410848$$s32604$$uhttps://cds.cern.ch/record/1158708/files/Figures_ScorDet000.png$$y00058 \sl Signal corrected for the track angle ($S_{ren}$), in full curve without electronic gain calibration and in dots with it.
001158708 8564_ $$81410849$$s20651$$uhttps://cds.cern.ch/record/1158708/files/Figures_Hybrid_temp_Warm_TOB.png$$y00007 \sl Hybrid temperature distributions for TIB, TID, TOB, and TEC at a coolant temperature of $14\,^{\circ}\mathrm{C}$.
001158708 8564_ $$81410850$$s18039$$uhttps://cds.cern.ch/record/1158708/files/Figures_ClusterWidthTrack_TIB.png$$y00082 \sl Cluster width for TIB(left) and TOB(right) hits for all tracks and perpendicular tracks
001158708 8564_ $$81410851$$s16095$$uhttps://cds.cern.ch/record/1158708/files/Figures_StoNTOB_TIF-1.png$$y00061 \sl Signal over noise corrected for the track angle: from the left to the right for TIB and TOB.
001158708 8564_ $$81410852$$s488200$$uhttps://cds.cern.ch/record/1158708/files/Figures_modul_komplett-sw_neu.png$$y00050 \sl Angle definitions: $\theta_{3D}$ on the left; $\theta_{XZ}$ on the right.
001158708 8564_ $$81410853$$s16166$$uhttps://cds.cern.ch/record/1158708/files/Figures_eta_s_TOB_ZS_3CC.png$$y00087 \sl $\eta$ function for TIB(left) and TOB(right) clusters The data are from Zero Suppressed runs compared with Monte Carlo with 3\% capacitive coupling.
001158708 8564_ $$81410854$$s13851$$uhttps://cds.cern.ch/record/1158708/files/Figures_V250_Warm_TID_good.png$$y00014 \sl 2.5\,V voltage line value measured at the module for TOB, TIB, TEC, and TID.
001158708 8564_ $$81410855$$s201159$$uhttps://cds.cern.ch/record/1158708/files/ScorDet300SimuReal.png$$y00023 \sl Signal distribution for clusters on tracks in data (dashed line) and Monte Carlo (solid line). From left to right: TIB, TOB and TEC
001158708 8564_ $$81410856$$s17643$$uhttps://cds.cern.ch/record/1158708/files/Figures_StripOccupancyPerRun_TIB_S2Nabove20_log.png$$y00068 \sl Distribution of strip occupancy for TIB and TEC: upper (lower) plots for S/N below (above) 20.
001158708 8564_ $$81410857$$s18798$$uhttps://cds.cern.ch/record/1158708/files/Figures_StripOccupancyPerRun_TEC_S2Nless20_log.png$$y00067 \sl Distribution of strip occupancy for TIB and TEC: upper (lower) plots for S/N below (above) 20.
001158708 8564_ $$81410858$$s201159$$uhttps://cds.cern.ch/record/1158708/files/Figures_ScorDet300SimuReal.png$$y00087 \sl Signal distribution for clusters on tracks in data (dashed line) and Monte Carlo (solid line). From left to right: TIB, TOB and TEC
001158708 8564_ $$81410859$$s49975$$uhttps://cds.cern.ch/record/1158708/files/Figures_WidthvsAngle_Pass3_TOB.png$$y00092 \sl Cluster width versus $\theta_t$ for TOB layers.
001158708 8564_ $$81410860$$s53385$$uhttps://cds.cern.ch/record/1158708/files/Figures_latencyHistory.png$$y00051 \sl Offset from the on-peak timing (left) and signal correction factor (right) as function of the run number for the three sub-detectors TIB/TID, TOB, and TEC.
001158708 8564_ $$81410861$$s142403$$uhttps://cds.cern.ch/record/1158708/files/triggerlayout_rz_positionA.png$$y00001 Layout of the various trigger scintillator configurations used during the cosmic data taking at the TIF (in chronological order): (a) configuration TA; (b) configuration TB; (c) configuration TC. The $xy$ view is shown on the left side, the $rz$ view is shown on the right. The straight lines connecting the active areas of the top and bottom scintillation counters indicate theacceptance region.
001158708 8564_ $$81410862$$s164005$$uhttps://cds.cern.ch/record/1158708/files/triggerlayout_rz_positionC.png$$y00003 Layout of the various trigger scintillator configurations used during the cosmic data taking at the TIF (in chronological order): (a) configuration TA; (b) configuration TB; (c) configuration TC. The $xy$ view is shown on the left side, the $rz$ view is shown on the right. The straight lines connecting the active areas of the top and bottom scintillation counters indicate theacceptance region.
001158708 8564_ $$81410863$$s180699$$uhttps://cds.cern.ch/record/1158708/files/triggerlayout_rz_positionB.png$$y00002 Layout of the various trigger scintillator configurations used during the cosmic data taking at the TIF (in chronological order): (a) configuration TA; (b) configuration TB; (c) configuration TC. The $xy$ view is shown on the left side, the $rz$ view is shown on the right. The straight lines connecting the active areas of the top and bottom scintillation counters indicate theacceptance region.
001158708 8564_ $$81410864$$s10439$$uhttps://cds.cern.ch/record/1158708/files/Figures_EtaSymm_VR_TOB.png$$y00085 \sl $\eta$ function for TIB(left) and TOB(right) clusters. The data are from Virgin Raw runs where the information of the strips below the clustering threshold is available.
001158708 8564_ $$81410865$$s164005$$uhttps://cds.cern.ch/record/1158708/files/Figures_triggerlayout_rz_positionC.png$$y00006  Layout of the various trigger scintillator configurations used during the cosmic data taking at the TIF (in chronological order): (a) configuration TA; (b) configuration TB; (c) configuration TC. The $xy$ view is shown on the left side, the $rz$ view is shown on the right. The straight lines connecting the active areas of the top and bottom scintillation counters indicate the acceptance region.
001158708 8564_ $$81410866$$s180699$$uhttps://cds.cern.ch/record/1158708/files/Figures_triggerlayout_rz_positionB.png$$y00004  Layout of the various trigger scintillator configurations used during the cosmic data taking at the TIF (in chronological order): (a) configuration TA; (b) configuration TB; (c) configuration TC. The $xy$ view is shown on the left side, the $rz$ view is shown on the right. The straight lines connecting the active areas of the top and bottom scintillation counters indicate the acceptance region.
001158708 8564_ $$81410867$$s142403$$uhttps://cds.cern.ch/record/1158708/files/Figures_triggerlayout_rz_positionA.png$$y00002  Layout of the various trigger scintillator configurations used during the cosmic data taking at the TIF (in chronological order): (a) configuration TA; (b) configuration TB; (c) configuration TC. The $xy$ view is shown on the left side, the $rz$ view is shown on the right. The straight lines connecting the active areas of the top and bottom scintillation counters indicate the acceptance region.
001158708 8564_ $$81410868$$s16598$$uhttps://cds.cern.ch/record/1158708/files/noise_vs_run_tib_postVPSP.png$$y00004 \sl Noise vs run number for TIB on the left and for TOB on the right.Four periods at different temperatures are visible: $10\,^{\circ}\mathrm{C}$, $0\,^{\circ}\mathrm{C}$, $-10\,^{\circ}\mathrm{C}$ and $-15\,^{\circ}\mathrm{C}$
001158708 8564_ $$81410869$$s29423$$uhttps://cds.cern.ch/record/1158708/files/Figures_Historic_NoisyDead_TIB.png$$y00046 \sl Noisy and dead strips vs run for TIB, TID, TOB, and TEC.
001158708 8564_ $$81410870$$s26562$$uhttps://cds.cern.ch/record/1158708/files/Figures_Historic_NoisyDead_TID.png$$y00047 \sl Noisy and dead strips vs run for TIB, TID, TOB, and TEC.
001158708 8564_ $$81410871$$s48948$$uhttps://cds.cern.ch/record/1158708/files/subdets_10947_version2.png$$y00008 \sl. Fit of the signal as a function of the latency, for each of the four sub-detectors. Data are from run 10947 and were used to set the latency for the following period.
001158708 8564_ $$81410872$$s12610$$uhttps://cds.cern.ch/record/1158708/files/Figures_TIB-noise-11413-L4.png$$y00027 \sl TIB noise profile for T= $-10\,^{\circ}\mathrm{C}$ for layers 1, 2, 3, and 4. Gaussian fit is shown. X axis is ADC value.
001158708 8564_ $$81410873$$s12835$$uhttps://cds.cern.ch/record/1158708/files/Figures_TIB-noise-11413-L2.png$$y00025 \sl TIB noise profile for T= $-10\,^{\circ}\mathrm{C}$ for layers 1, 2, 3, and 4. Gaussian fit is shown. X axis is ADC value.
001158708 8564_ $$81410874$$s12517$$uhttps://cds.cern.ch/record/1158708/files/Figures_TIB-noise-11413-L3.png$$y00026 \sl TIB noise profile for T= $-10\,^{\circ}\mathrm{C}$ for layers 1, 2, 3, and 4. Gaussian fit is shown. X axis is ADC value.
001158708 8564_ $$81410875$$s12772$$uhttps://cds.cern.ch/record/1158708/files/Figures_TIB-noise-11413-L1.png$$y00024 \sl TIB noise profile for T= $-10\,^{\circ}\mathrm{C}$ for layers 1, 2, 3, and 4. Gaussian fit is shown. X axis is ADC value.
001158708 8564_ $$81410876$$s13131$$uhttps://cds.cern.ch/record/1158708/files/Figures_TOB-noise-11413-L1.png$$y00028 \sl TOB noise profile for T= $-10\,^{\circ}\mathrm{C}$ for layers 1, 2, 3, 4, 5 and 6. Gaussian fit is shown. X axis is ADC value
001158708 8564_ $$81410877$$s13127$$uhttps://cds.cern.ch/record/1158708/files/Figures_TOB-noise-11413-L2.png$$y00029 \sl TOB noise profile for T= $-10\,^{\circ}\mathrm{C}$ for layers 1, 2, 3, 4, 5 and 6. Gaussian fit is shown. X axis is ADC value
001158708 8564_ $$81410878$$s13024$$uhttps://cds.cern.ch/record/1158708/files/Figures_TOB-noise-11413-L3.png$$y00030 \sl TOB noise profile for T= $-10\,^{\circ}\mathrm{C}$ for layers 1, 2, 3, 4, 5 and 6. Gaussian fit is shown. X axis is ADC value
001158708 8564_ $$81410879$$s13093$$uhttps://cds.cern.ch/record/1158708/files/Figures_TOB-noise-11413-L4.png$$y00031 \sl TOB noise profile for T= $-10\,^{\circ}\mathrm{C}$ for layers 1, 2, 3, 4, 5 and 6. Gaussian fit is shown. X axis is ADC value
001158708 8564_ $$81410880$$s13144$$uhttps://cds.cern.ch/record/1158708/files/Figures_TOB-noise-11413-L5.png$$y00032 \sl TOB noise profile for T= $-10\,^{\circ}\mathrm{C}$ for layers 1, 2, 3, 4, 5 and 6. Gaussian fit is shown. X axis is ADC value
001158708 8564_ $$81410881$$s13189$$uhttps://cds.cern.ch/record/1158708/files/Figures_TOB-noise-11413-L6.png$$y00033 \sl TOB noise profile for T= $-10\,^{\circ}\mathrm{C}$ for layers 1, 2, 3, 4, 5 and 6. Gaussian fit is shown. X axis is ADC value
001158708 8564_ $$82317498$$s9563$$uhttps://cds.cern.ch/record/1158708/files/fig00000.png$$y00000 noimg: Composition of the Sector Test with the different subdetector layers/disks.:  Dimensions of scintillators used at Sector Test; single and coincidence rates.
001158708 916__ $$sn$$w200847$$ya2009
001158708 960__ $$a13
001158708 961__ $$c20100408$$h1743$$lCER01$$x20090129
001158708 963__ $$aPUBLIC
001158708 981__ $$a002801293CER01
001158708 980__ $$aINTNOTECMSPUBL
001158708 980__ $$aNOTE
001158708 980__ $$aARTICLE
001158708 999C6 $$aInvenio/0.99.90.20100623 refextract/0.99.90.20100623-1298563801-0-1-6-25-0-0-24
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