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Muons from cosmic-ray interactions in the atmosphere provide a high-statistics source of particles that can be used to study the performance and calibration of the ATLAS detector. Cosmic-ray muons can penetrate to the cavern and deposit energy in all detector subsystems. Such events have played an important role in the commissioning of the detector since the start of the installation phase in 2005 and were particularly important for understanding the detector performance in the time prior to the arrival of the first LHC beams. Global cosmic-ray runs were undertaken in both 2008 and 2009 and these data have been used through to the early phases of collision data-taking as a tool for calibration, alignment and detector monitoring. These large datasets have also been used for detector performance studies, including investigations that rely on the combined performance of different subsystems. This paper presents the results of performance studies related to combined tracking, lepton identification and the reconstruction of jets and missing transverse energy. Results are compared to expectations based on a cosmic-ray event generator and a full simulation of the detector response. RI valente, paolo/A-6640-2010; Rescia, Sergio/D-8604-2011; Castro, Nuno/D-5260-2011; Doyle, Anthony/C-5889-2009; Andreazza, Attilio/E-5642-2011; Jakubek, Jan/E-6530-2011; Marti-Garcia, Salvador/F-3085-2011; Conde Muino, Patricia/F-7696-2011; Stoicea, Gabriel/B-6717-2011; Robson, Aidan/G-1087-2011; Kladiva, Eduard/G-6305-2011; Losada, Marta/B-2261-2010; Bauer, Florian/G-8816-2011; Jones, Roger/H-5578-2011; Gutierrez, Phillip/C-1161-2011; Ferrando, James/A-9192-2012; collins-tooth, christopher/A-9201-2012; Perrino, Roberto/B-4633-2010; De Cecco, Sandro/B-1016-2012; branchini, paolo/A-4857-2011; Wolter, Marcin/A-7412-2012; Rotaru, Marina/A-3097-2011; O'Shea, Val/G-1279-2010; Takai, Helio/C-3301-2012; Britton, David/F-2602-2010; Pina, Joao /C-4391-2012; Li, Xuefei/C-3861-2012; Smirnova, Lidia/D-8089-2012; Smirnov, Sergei/F-1014-2011; Gladilin, Leonid/B-5226-2011; Kramarenko, Victor/E-1781-2012; Prokoshin, Fedor/E-2795-2012; Alexa, Calin/F-6345-2010; Pacheco Pages, Andres/C-5353-2011; Livan, Michele/D-7531-2012; Petrucci, Fabrizio/G-8348-2012; Fabbri, Laura/H-3442-2012; Kurashige, Hisaya/H-4916-2012; Villa, Mauro/C-9883-2009; Delmastro, Marco/I-5599-2012
Muons from cosmic-ray interactions in the atmosphere provide a high-statistics source of particles that can be used to study the performance and calibration of the ATLAS detector. Cosmic-ray muons can penetrate to the cavern and deposit energy in all detector subsystems. Such events have played an important role in the commissioning of the detector since the start of the installation phase in 2005 and were particularly important for understanding the detector performance in the time prior to the arrival of the first LHC beams. Global cosmic-ray runs were undertaken in both 2008 and 2009 and these data have been used through to the early phases of collision data-taking as a tool for calibration, alignment and detector monitoring. These large datasets have also been used for detector performance studies, including investigations that rely on the combined performance of different subsystems. This paper presents the results of performance studies related to combined tracking, lepton identification and the reconstruction of jets and missing transverse energy. Results are compared to expectations based on a cosmic-ray event generator and a full simulation of the detector response.
Muons from cosmic-ray interactions in the atmosphere provide a high-statistics source of particles that can be used to study the performance and calibration of the ATLAS detector. Cosmic-ray muons can penetrate to the cavern and deposit energy in all detector subsystems. Such events have played an important role in the commissioning of the detector since the start of the installation phase in 2005 and were particularly important for understanding the detector performance in the time prior to the arrival of the first LHC beams. Global cosmic-ray runs were undertaken in both 2008 and 2009 and these data have been used through to the early phases of collision data-taking as a tool for calibration, alignment and detector monitoring. These large datasets have also been used for detector performance studies, including investigations that rely on the combined performance of different subsystems. This paper presents the results of performance studies related to combined tracking, lepton identification and the reconstruction of jets and missing transverse energy. Results are compared to expectations based on a cosmic-ray event generator and a full simulation of the detector response.
Studies of the performance of the ATLAS detector using cosmic-ray muons
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A.;Kanzaki J.;Kaplan B.;Kapliy A.;Kaplon J.;Kar D.;Karagounis M.;Karagoz M.;Karnevskiy M.;Kartvelishvili V.;Karyukhin A. N.;Kashif L.;Kasmi A.;Kass R. D.;Kastanas A.;Kataoka M.;Kataoka Y.;Katsoufis E.;Katzy J.;Kaushik V.;Kawagoe K.;Kawamoto T.;Kawamura G.;Kayl M. S.;Kazanin V. A.;Kazarinov M. Y.;Keates J. R.;Keeler R.;Kehoe R.;Keil M.;Kekelidze G. D.;Kelly M.;Kenyon M.;Kepka O.;Kerschen N.;Kersevan B. P.;Kersten S.;Kessoku K.;Khakzad M.;Khalil zada F.;Khandanyan H.;Khanov A.;Kharchenko D.;Khodinov A.;Khomich A.;Khoriauli G.;Khovanskiy N.;Khovanskiy V.;Khramov E.;Khubua J.;Kim H.;Kim M. S.;Kim P. C.;Kim S. H.;Kind O.;King B. T.;King M.;Kirk J.;Kirsch G. P.;Kirsch L. E.;Kiryunin A. E.;Kisielewska D.;Kittelmann T.;Kladiva E.;Klein M.;Klein U.;Kleinknecht K.;Klemetti M.;Klier A.;Klimentov A.;Klingenberg R.;Klinkby E. B.;Klioutchnikova T.;Klok P. F.;Klous S.;Kluge E. E.;Kluge T.;Kluit P.;Kluth S.;Knecht N. S.;Kneringer E.;Ko B. R.;Kobayashi T.;Kobel M.;Koblitz B.;Kocian M.;Kocnar A.;Kodys P.;Koeneke K.;Konig A. C.;Koenig S.;Koepke L.;Koetsveld F.;Koevesarki P.;Koffas T.;Koffeman E.;Kohn F.;Kohout Z.;Kohriki T.;Koi T.;Kolanoski H.;Kolesnikov V.;Koletsou I.;Koll J.;Kollar D.;Kolya S. D.;Komar A. A.;Komaragiri J. R.;Kondo T.;Kono T.;Konoplich R.;Konstantinidis N.;Koperny S.;Korcyl K.;Kordas K.;Korn A.;Korolkov I.;Korolkova E. V.;Korotkov V. A.;Kortner O.;Kortner S.;Kostka P.;Kostyukhin V. V.;Kotov S.;Kotov V. M.;Kourkoumelis C.;Koutsman A.;Kowalewski R.;Kowalski T. Z.;Kozanecki W.;Kozhin A. S.;Kral V.;Kramarenko V. A.;Kramberger G.;Krasny M. W.;Krasznahorkay A.;Kraus J.;Kraus J. K.;Kreisel A.;Krejci F.;Kretzschmar J.;Krieger N.;Krieger P.;Kroeninger K.;Kroha H.;Kroll J.;Kroseberg J.;Krstic J.;Kruchonak U.;Krueger H.;Krumshteyn Z. V.;Kruth A.;Kubota T.;Kuehn S.;Kugel A.;Kuhl T.;Kuhn D.;Kukhtin V.;Kulchitsky Y.;Kuleshov S.;Kummer C.;Kuna M.;Kunkle J.;Kupco A.;Kurashige H.;Kurata M.;Kurochkin Y. A.;Kus V.;Kuze M.;Kwee R.;La Rosa A.;LA ROTONDA, Laura;Labbe J.;Lacasta C.;Lacava F.;Lacker H.;Lacour D.;Lacuesta V. R.;Ladygin E.;Lafaye R.;Laforge B.;Lagouri T.;Lai S.;Lamanna M.;Lampen C. L.;Lampl W.;Lancon E.;Landgraf U.;Landon M. P. J.;Lane J. L.;Lankford A. J.;Lanni F.;Lantzsch K.;Lanza A.;Laplace S.;Lapoire C.;Laporte J. F.;Lari T.;Larner A.;Lassnig M.;Laurelli P.;Lavrijsen W.;Laycock P.;Lazarev A. B.;Lazzaro A.;Le Dortz O.;Le Guirriec E.;Le Menedeu E.;Lebedev A.;Lebel C.;LeCompte T.;Ledroit Guillon F.;Lee H.;Lee J. S. H.;Lee S. C.;Lefebvre M.;Legendre M.;LeGeyt B. C.;Legger F.;Leggett C.;Lehmacher M.;Miotto G. Lehmann;Lei X.;Leitner R.;Lellouch D.;Lellouch J.;Lendermann V.;Leney K. J. C.;Lenz T.;Lenzen G.;Lenzi B.;Leonhardt K.;Leroy C.;Lessard J. R.;Lester C. G.;Cheong A. Leung Fook;Leveque J.;Levin D.;Levinson L. J.;Leyton M.;Li H.;Li X.;Liang Z.;Liang Z.;Liberti B.;Lichard P.;Lichtnecker M.;Lie K.;Liebig W.;Lilley J. N.;Limosani A.;Limper M.;Lin S. C.;Linnemann J. T.;Lipeles E.;Lipinsky L.;Lipniacka A.;Liss T. M.;Lissauer D.;Lister A.;Litke A. M.;Liu C.;Liu D.;Liu H.;Liu B.;Liu M.;Liu Y.;Livan M.;Lleres A.;Lloyd S. L.;Lobodzinska E.;Loch P.;Lockman W. S.;Lockwitz S.;Loddenkoetter T.;Loebinger F. K.;Loginov A.;Loh C. W.;Lohse T.;Lohwasser K.;Lokajicek M.;Long R. E.;Lopes L.;Mateos D. Lopez;Losada M.;Loscutoff P.;Lou X.;Lounis A.;Loureiro K. F.;Lovas L.;Love J.;Love P. A.;Lowe A. J.;Lu F.;Lubatti H. J.;Luci C.;Lucotte A.;Ludwig A.;Ludwig D.;Ludwig I.;Luehring F.;Lumb D.;Luminari L.;Lund E.;Lund Jensen B.;Lundberg B.;Lundberg J.;Lundquist J.;Lynn D.;Lys J.;Lytken E.;Ma H.;Ma L. L.;Goia J. A. Macana;Maccarrone G.;Macchiolo A.;Macek B.;Machado Miguens J.;Mackeprang R.;Madaras R. J.;Mader W. F.;Maenner R.;Maeno T.;Maettig P.;Maettig S.;Martins P. J. Magalhaes;Magradze E.;Mahalalel Y.;Mahboubi K.;Mahmood A.;Maiani C.;Maidantchik C.;Maio A.;Majewski S.;Makida Y.;Makouski M.;Makovec N.;Mal P.;Malecki P.a.;Malecki P.;Maleev V. P.;Malek F.;Mallik U.;Malon D.;Maltezos S.;Malyshev V.;Malyukov S.;Mameghani R.;Mamuzic J.;Mandelli L.;Mandic I.;Mandrysch R.;Maneira J.;Mangeard P. S.;Manjavidze I. D.;Mann A.;Manning P. M.;Manousakis Katsikakis A.;Mansoulie B.;Mapelli A.;Mapelli L.;March L.;Marchand J. F.;Marchese F.;Marchiori G.;Marcisovsky M.;Marino C. P.;Marroquim F.;Marshall Z.;Marti Garcia S.;Martin A. J.;Martin B.;Martin B.;Martin F. F.;Martin J. P.;Martin T. A.;Latour B. Martin Dit;Martinez M.;Outschoorn V. Martinez;Martyniuk A. C.;Marzano F.;Marzin A.;Masetti L.;Mashimo T.;Mashinistov R.;Masik J.;Maslennikov A. L.;Massa I.;Massol N.;MASTROBERARDINO, Anna;Masubuchi T.;Matricon P.;Matsunaga H.;Matsushita T.;Mattravers C.;Maxfield S. J.;Mayne A.;Mazini R.;Mazur M.;Mc Kee S. P.;McCarn A.;McCarthy R. L.;McCubbin N. A.;McFarlane K. W.;McGlone H.;Mchedlidze G.;McMahon S. J.;McPherson R. A.;Meade A.;Mechnich J.;Mechtel M.;Medinnis M.;Meera Lebbai R.;Meguro T.;Mehlhase S.;Mehta A.;Meier K.;Meirose B.;Melachrinos C.;Garcia B. R. Mellado;Mendoza Navas L.;Meng Z.;Menke S.;Meoni E.;Mermod P.;Merola L.;Meronia C.;Merritt F. S.;Messina A. M.;Metcalfe J.;Mete A. S.;Meyer J. P.;Meyer J.;Meyer J.;Meyer T. C.;Meyer W. T.;Miao J.;Michal S.;Micu L.;Middleton R. P.;Migas S.;Mijovic L.;Mikenberg G.;Mikestikova M.;Mikuz M.;Miller D. W.;Mills W. J.;Mills C.;Milov A.;Milstead D. A.;Milstein D.;Minaenko A. A.;Minano M.;Minashvili I. A.;Mincer A. I.;Mindur B.;Mineev M.;Ming Y.;Mir L. M.;Mirabellia G.;Misawa S.;Misiejuk A.;Mitrevski J.;Mitsou V. A.;Mitsui S.;Miyagawa P. S.;Miyazaki K.;Mjornmark J. U.;Moa T.;Moeller V.;Moenig K.;Moeser N.;Mohr W.;Mohrdieck Moeck S.;Moles Valls R.;Molina Perez J.;Monk J.;Monnier E.;Montesano S.;Monticelli F.;Moore R. W.;Herrera C. Mora;Moraes A.;Morais A.;Morel J.;Morello G.;Moreno D.;Moreno Llacer M.;Morettinia P.;Morii M.;Morley A. K.;Mornacchi G.;Morris J. D.;Moser H. G.;Mosidze M.;Moss J.;Mount R.;Mountricha E.;Mouraviev S. V.;Moyse E. J. W.;Mudrinic M.;Mueller F.;Mueller J.;Mueller K.;Mueller T. A.;Muenstermann D.;Muir A.;Munwes Y.;Murray W. J.;Mussche I.;Musto E.;Myagkov A. G.;Myska M.;Nadal J.;Nagai K.;Nagano K.;Nagasaka Y.;Nairz A. M.;Nakamura K.;Nakano I.;Nanava G.;Napier A.;Nash M.;Nation N. R.;Nattermann T.;Naumann T.;Navarro G.;Nderitu S. K.;Neal H. A.;Nebot E.;Nechaeva P.;Negri A.;Negri G.;Nelson A.;Nelson S.;Nelson T. K.;Nemecek S.;Nemethy P.;Nepomuceno A. A.;Nessi M.;Neubauer M. S.;Neusiedl A.;Neves R. M.;Nevski P.;Nickerson R. B.;Nicolaidou R.;Nicolas L.;Nicoletti G.;Nicquevert B.;Niedercorn F.;Nielsen J.;Nikiforov A.;Nikolaev K.;Nikolic Audit I.;Nikolopoulos K.;Nilsen H.;Nilsson P.;Nisati A.;Nishiyama T.;Nisius R.;Nodulman L.;Nomachi M.;Nomidis I.;Nordberg M.;Nordkvist B.;Notz D.;Novakova J.;Nozaki M.;Nozicka M.;Nugent I. M.;Nuncio Quiroz A. E.;Hanninger G. Nunes;Nunnemann T.;Nurse E.;O'Neil D. C.;O'Shea V.;Oakham F. G.;Oberlack H.;Ochi A.;Oda S.;Odaka S.;Odier J.;Ogren H.;Oh A.;Oh S. H.;Ohm C. C.;Ohshima T.;Ohsugi T.;Okada S.;Okawa H.;Okumura Y.;Okuyama T.;Olchevski A. G.;Oliveira M.;Damazio D. Oliveira;Oliver Garcia E.;Olivito D.;Olszewski A.;Olszowska J.;Omachi C.;Onofre A.;Onyisi P. U. E.;Oram C. J.;Oreglia M. J.;Oren Y.;Orestano D.;Orlov I.;Barrera C. Oropeza;Orr R. S.;Ortega E. O.;Osculati B.;Ospanov R.;Osuna C.;Otero y. Garzon G.;Ottersbach J. P.;Ould Saada F.;Ouraou A.;Ouyang Q.;Owen M.;Owen S.;Oyarzun A.;Ozcan V. E.;Ozturk N.;Pacheco Pages A.;Padilla Aranda C.;Paganis E.;Paige F.;Pajchel K.;Palestini S.;Pallin D.;Palma A.;Palmer J. D.;Pan Y. B.;Panagiotopoulou E.;Panes B.;Panikashvili N.;Panitkin S.;Pantea D.;Panuskova M.;Paolone V.;Papadopoulou T.h. D.;Park S. J.;Park W.;Parker M. A.;Parodi F.;Parsons J. A.;Parzefall U.;Pasqualucci E.;Passeri A.;Pastore F.;Pastore F.r.;Pasztor G.;Pataraia S.;Patel N.;Pater J. R.;Patricelli S.;Pauly T.;Pecsy M.;Morales M. I. Pedraza;Peleganchuk S. V.;Peng H.;Penson A.;Penwell J.;Perantonia M.;Perez K.;Perez Codina E.;Perez Garcia Estan M. T.;Reale V. Perez;Perini L.;Pernegger H.;Perrino R.;Persembe S.;Perus P.;Peshekhonov V. D.;Petersen B. A.;Petersen T. C.;Petit E.;Petridou C.;Petrolo E.;Petrucci F.;Petschull D.;Petteni M.;Pezoa R.;Pfeifer B.;Phan A.;Phillips A. W.;Piacquadio G.;Piccaro E.;Piccinini M.;Piegaia R.;Pilcher J. E.;Pilkington A. D.;Pina J.;Pinamonti M.;Pinfold J. L.;Pinto B.;Pizio C.;Placakyte R.;Plamondon M.;Pleier M. A.;Poblaguev A.;Poddar S.;Podlyski F.;Poggioli L.;Pohl M.;Polci F.;Polesello G.;Policicchio A.;Polini A.;Poll J.;Polychronakos V.;Pomeroy D.;Pommes K.;Pontecorvo L.;Pope B. G.;Popeneciu G. A.;Popovic D. S.;Poppleton A.;Bueso X. Portell;Porter R.;Pospelov G. E.;Pospisil S.;Potekhin M.;Potrap I. N.;Potter C. J.;Potter C. T.;Potter K. P.;Poulard G.;Poveda J.;Prabhu R.;Pralavorio P.;Prasad S.;Pravahan R.;Pribyl L.;Price D.;Price L. E.;Prichard P. M.;Prieur D.;Primaveraa M.;Prokofiev K.;Prokoshin F.;Protopopescu S.;Proudfoot J.;Prudent X.;Przysiezniak H.;Psoroulas S.;Ptacek E.;Purdham J.;Purohit M.;Puzo P.;Pylypchenko Y.;Qian J.;Qian W.;Qin Z.;Quadt A.;Quarrie D. R.;Quayle W. B.;Quinonez F.;Raas M.;Radeka V.;Radescu V.;Radics B.;Rador T.;Ragusa F.;Rahal G.;Rahimi A. M.;Rajagopalan S.;Rammensee M.;Rammes M.;Rauscher F.;Rauter E.;Raymond M.;Read A. L.;Rebuzzi D. M.;Redelbach A.;Redlinger G.;Reece R.;Reeves K.;Reinherz Aronis E.;Reinsch A.;Reisinger I.;Reljic D.;Rembser C.;Ren Z. L.;Renkel P.;Rescia S.;Rescigno M.;Resconi S.;Resende B.;Reznicek P.;Rezvani R.;Richards A.;Richter R.;Richter Was E.;Ridel M.;Rijpstra M.;Rijssenbeek M.;Rimoldi A.;Rinaldi L.;Rios R. R.;Riu I.;Rizatdinova F.;Rizvi E.;Roa Romero D. A.;Robertson S. H.;Robichaud Veronneau A.;Robinson D.;Robinson J. E. M.;Robinson M.;Robson A.;de Lima J. G. Rocha;Roda C.;Dos Santos D. Roda;Rodriguez D.;Garcia Y. Rodriguez;Roe S.;Rohne O.;Rojo V.;Rolli S.;Romaniouk A.;Romanov V. M.;Romeo G.;Romero Maltranaa D.;Roos L.;Ros E.;Rosati S.;Rosenbaum G. A.;Rosselet L.;Rossetti V.;Rossi L. P.;Rotaru M.;Rothberg J.;Rousseau D.;Royon C. R.;Rozanov A.;Rozen Y.;Ruan X.;Ruckert B.;Ruckstuhl N.;Rud V. I.;Rudolph G.;Ruehr F.;Ruggieri F.;Ruiz Martinez A.;Rumyantsev L.;Rurikova Z.;Rusakovich N. A.;Rutherfoord J. P.;Ruwiedel C.;Ruzicka P.;Ryabov Y. F.;Ryan P.;Rybkin G.;Rzaeva S.;Saavedra A. F.;Sadrozinski H. F. W.;Sadykov R.;Tehrani F. Safai;Sakamoto H.;Salamanna G.;Salamon A.;Saleem M.;Salihagic D.;Salnikov A.;Salt J.;Ferrando B. M. Salvachua;Salvatore D.;Salvatore F.;Salvucci A.;Salzburger A.;Sampsonidis D.;Samset B. H.;Sandaker H.;Sander H. G.;Sanders M. P.;Sandhoff M.;Sandhu P.;Sandstroem R.;Sandvoss S.;Sankey D. P. C.;Sansoni A.;Rios C. Santamarina;Santoni C.;Santonico R.;Saraiva J. G.;Sarangi T.;Sarkisyan Grinbaum E.;Sarri F.;Sasaki O.;Sasao N.;Satsounkevitch I.;Sauvage G.;Savard P.;Savine A. Y.;Savinov V.;Sawyer L.;Saxon D. H.;Says L. P.;Sbarra C.;Sbrizzi A.;Scannicchio D. A.;Schaarschmidt J.;Schacht P.;Schaefer U.;Schaetzel S.;Schaffer A. C.;Schaile D.;Schamberger R. D.;Schamov A. G.;Scharf V.;Schegelsky V. A.;Scheirich D.;Schernau M.;Scherzer M. I.;Schiavi C.;Schieck J.;Schioppa M.;Schlenker S.;Schmidt E.;Schmieden K.;Schmitt C.;Schmitz M.;Schoening A.;Schott M.;Schouten D.;Schovancova J.;Schram M.;Schreiner A.;Schroeder C.;Schroer N.;Schroers M.;Schultes J.;Schultz Coulon H. C.;Schumacher J. W.;Schumacher M.;Schumm B. A.;Schune P.h.;Schwanenberger C.;Schwartzman A.;Schwemling P.h.;Schwienhorst R.;Schwierz R.;Schwindling J.;Scott W. G.;Searcy J.;Sedykh E.;Segura E.;Seidel S. C.;Seiden A.;Seifert F.;Seixas J. M.;Sekhniaidze G.;Seliverstov D. M.;Sellden B.;Semprini Cesari N.;Serfon C.;Serin L.;Seuster R.;Severini H.;Sevior M. E.;Sfyrla A.;Shabalina E.;Shamim M.;Shan L. Y.;Shank J. T.;Shao Q. T.;Shapiro M.;Shatalov P. B.;Shaw K.;Sherman D.;Sherwood P.;Shibata A.;Shimojima M.;Shin T.;Shmeleva A.;Shochet M. J.;Shupe M. A.;Sicho P.;Sidoti A.;Siegert F.;Siegrist J.;Sijacki D.j.;Silbert O.;Silver Y.;Silverstein D.;Silverstein S. B.;Simak V.;Simic L.j.;Simion S.;Simmons B.;Simonyan M.;Sinervo P.;Sinev N. B.;Sipica V.;Siragusa G.;Sisakyan A. N.;Sivoklokov S. Y.u.;Sjolin J.;Sjursen T. B.;Skovpen K.;Skubic P.;Slater M.;Slavicek T.;Sliwa K.;Sloper J.;Smakhtin V.;Smirnov S. Y.u.;Smirnov Y.;Smirnova L. N.;Smirnova O.;Smith B. C.;Smith D.;Smith K. M.;Smizanska M.;Smolek K.;Snesarev A. A.;Snow S. W.;Snow J.;Snuverink J.;Snyder S.;Soares M.;Sobie R.;Sodomka J.;Soffer A.;Solans C. A.;Solar M.;Solc J.;Camillocci E. Solfaroli;Solodkov A. A.;Solovyanov O. V.;Sondericker J.;Sopko V.;Sopko B.;Sosebee M.;Soukharev A.;Spagnolo S.;Spano F.;Spighi R.;Spigo G.;Spila F.;Spiwoks R.;Spousta M.;Spurlock B.;Denis R. D. S.t.;Stahl T.;Stahlman J.;Stamen R.;Stanecka E.;Stanek R. W.;Stanescu C.;Stapnes S.;Starchenko E. A.;Stark J.;Staroba P.;Starovoitov P.;Stavina P.;Steele G.;Steinbach P.;Steinberg P.;Stekl I.;Stelzer B.;Stelzer H. J.;Stelzer Chilton O.;Stenzel H.;Stevenson K.;Stewart G. A.;Stockton M. C.;Stoerig K.;Stoicea G.;Stonjek S.;Strachota P.;Stradling A. R.;Straessner A.;Strandberg J.;Strandberg S.;Strandlie A.;Strang M.;Strauss M.;Strizenec P.;Stroehmer R.;Strom D. M.;Stroynowski R.;Strube J.;Stugu B.;Sturm P.;Soh D. A.;Su D.;Sugaya Y.;Sugimoto T.;Suhr C.;Suita K.;Suk M.;Sulin V. V.;Sultansoy S.;Sumida T.;Sun X.;Sundermann J. E.;Suruliz K.;Sushkov S.;Susinno G.;Sutton M. R.;Suzuki Y.;Sykora I.;Sykora T.;Szymocha T.;Sanchez J.;Ta D.;Tackmann K.;Taffard A.;Tafirout R.;Taga A.;Takahashi Y.;Takai H.;Takashima R.;Takeda H.;Takeshita T.;Talby M.;Talyshev A.;Tamsett M. C.;Tanaka J.;Tanaka R.;Tanaka S.;Tanaka S.;Tani K.;Tapprogge S.;Tardif D.;Tarem S.;Tarrade F.;Tartarelli G. F.;Tas P.;Tasevsky M.;TASSI, Enrico;Tatarkhanov M.;Taylor C.;Taylor F. E.;Taylor G. N.;Taylorb W.;Castanheira M. Teixeira Dias;Teixeira Dias P.;TenKate H.;Teng P. K.;Tennenbaum Katan Y. D.;Terada S.;Terashi K.;Terron J.;Terwort M.;Testa M.;Teuscher R. J.;Therhaag J.;Thioye M.;Thoma S.;Thomas J. P.;Thompson E. N.;Thompson P. D.;Thompson P. D.;Thompson R. J.;Thompson A. S.;Thomson E.;Thun R. P.;Tic T.;Tikhomirov V. O.;Tikhonov Y. A.;Tipton P.;Viegas F. J. Tique Aires;Tisserant S.;Toczek B.;Todorov T.;Todorova Nova S.;Toggerson B.;Tojo J.;Tokar S.;Tokunaga K.;Tokushuku K.;Tollefson K.;Tomoto M.;Tompkins L.;Toms K.;Tonoyan A.;Topfel C.;Topilin N. D.;Torchiani I.;Torrence E.;Torro Pastor E.;Toth J.;Touchard F.;Tovey D. R.;Trefzger T.;Tremblet L.;Tricoli A.;Trigger I. M.;Trincaz Duvoid S.;Trinh T. N.;Tripiana M. F.;Triplett N.;Trischuk W.;Trivedi A.;Trocme B.;Troncon C.;Trzupek A.;Tsarouchas C.;Tseng J. C. L.;Tsiakiris M.;Tsiareshka P. V.;Tsionou D.;Tsipolitis G.;Tsiskaridze V.;Tskhadadze E. G.;Tsukerman I. I.;Tsulaia V.;Tsung J. W.;Tsuno S.;Tsybychev D.;Tuggle J. M.;Turecek D.;Cakire I. Turk;Turlay E.;Tuts P. M.;Twomey M. S.;Tylmad M.;Tyndel M.;Uchida K.;Ueda I.;Ueno R.;Ugland M.;Uhlenbrock M.;Uhrmacher M.;Ukegawa F.;Unal G.;Undrus A.;Unel G.;Unno Y.;Urbaniec D.;Urkovsky E.;Urquijo P.;Urrejola P.;Usai G.;Uslenghi M.;Vacavant L.;Vacek V.;Vachon B.;Vahsen S.;Valente P.;Valentinetti S.;Valkar S.;Valladolid Gallego E.;Vallecorsa S.;Valls Ferrer J. A.;van der Graaf H.;van der Kraaij E.;van der Poel E.;van der Ster D.;van Eldik N.;van Gemmeren P.;van Kesteren Z.;van Vulpen I.;Vandelli W.;Vaniachine A.;Vankov P.;Vannucci F.;Vari R.;Varnes E. W.;Varouchas D.;Vartapetian A.;Varvell K. E.;Vassilakopoulos V. I.;Vazeille F.;Vellidis C.;Veloso F.;Veneziano S.;Ventura A.;Ventura D.;Venturi M.;Venturi N.;Vercesi V.;Verducci M.;Verkerke W.;Vermeulen J. C.;Vetterli M. C.;Vichou I.;Vickey T.;Viehhauser G. H. A.;Villa M.;Villani E. G.;Villaplana Perez M.;Vilucchi E.;Vincter M. G.;Vinek E.;Vinogradov V. B.;Viret S.;Virzi J.;Vitale A.;Vitells O.;Vivarelli I.;Vives Vaque F.;Vlachos S.;Vlasak M.;Vlasov N.;Vogel A.;Vokac P.;Volpi M.;von der Schmitt H.;von Loeben J.;von Radziewski H.;von Toerne E.;Vorobel V.;Vorwerk V.;Vos M.;Voss R.;Voss T. T.;Vossebeld J. H.;Vranjes N.;Milosavljevic M. Vranjes;Vrba V.;Vreeswijk M.;Anh T. Vu;Vudragovic D.;Vuillermet R.;Vukotic I.;Wagner P.;Walbersloh J.;Walder J.;Walker R.;Walkowiak W.;Wall R.;Wang C.;Wang H.;Wang J.;Wang S. M.;Warburton A.;Ward C. P.;Warsinsky M.;Wastie R.;Watkins P. M.;Watson A. T.;Watson M. F.;Watts G.;Watts S.;Waugh A. T.;Waugh B. M.;Weber M. D.;Weber M.;Weber M. S.;Weber P.;Weidberg A. R.;Weingarten J.;Weiser C.;Wellenstein H.;Wells P. S.;Wenaus T.;Wendler S.;Weng Z.;Wengler T.;Wenig S.;Wermes N.;Werner M.;Werner P.;Werth M.;Werthenbach U.;Wessels M.;Whalen K.;White A.;White M. J.;White S.;Whitehead S. R.;Whiteson D.;Whittington D.;Wicek F.;Wicke D.;Wickens F. J.;Wiedenmann W.;Wielers M.;Wienemann P.;Wiglesworth C.;Wiik L. A. M.;Wildauer A.;Wildt M. A.;Wilkens H. G.;Williams E.;Williams H. H.;Willocq S.;Wilson J. A.;Wilson M. G.;Wilson A.;Wingerter Seez I.;Winklmeier F.;Wittgen M.;Wolter M. W.;Wolters H.;Wosiek B. K.;Wotschack J.;Woudstra M. J.;Wraight K.;Wright C.;Wright D.;Wrona B.;Wu S. L.;Wu X.;Wulf E.;Wynne B. M.;Xaplanteris L.;Xella S.;Xie S.;Xu D.;Yamada M.;Yamamoto A.;Yamamoto K.;Yamamoto S.;Yamamura T.;Yamaoka J.;Yamazaki T.;Yamazaki Y.;Yan Z.;Yang H.;Yang U. K.;Yang Z.;Yao W. M.;Yao Y.;Yasu Y.;Ye J.;Ye S.;Yilmaz M.;Yoosoofmiya R.;Yorita K.;Yoshida R.;Young C.;Youssef S. P.;Yu D.;Yu J.;Yuan L.;Yurkewicz A.;Zaidan R.;Zaitsev A. M.;Zajacova Z.;Zambrano V.;Zanello L.;Zaytsev A.;Zeitnitz C.;Zeller M.;Zemla A.;Zendler C.;Zenin O.;Zenis T.;Zenonos Z.;Zenz S.;Zerwas D.;della Porta G. Zevi;Zhan Z.;Zhang H.;Zhang J.;Zhang Q.;Zhang X.;Zhao L.;Zhao T.;Zhao Z.;Zhemchugov A.;Zhong J.;Zhou B.;Zhou N.;Zhou Y.;Zhu C. G.;Zhu H.;Zhu Y.;Zhuang X.;Zhuravlov V.;Zimmermann R.;Zimmermann S.;Zimmermann S.;Ziolkowski M.;Zivkovic L.;Zobernig G.;Zoccoli A.;Nedden M. Zur;Zutshi V.
2011-01-01
Abstract
Muons from cosmic-ray interactions in the atmosphere provide a high-statistics source of particles that can be used to study the performance and calibration of the ATLAS detector. Cosmic-ray muons can penetrate to the cavern and deposit energy in all detector subsystems. Such events have played an important role in the commissioning of the detector since the start of the installation phase in 2005 and were particularly important for understanding the detector performance in the time prior to the arrival of the first LHC beams. Global cosmic-ray runs were undertaken in both 2008 and 2009 and these data have been used through to the early phases of collision data-taking as a tool for calibration, alignment and detector monitoring. These large datasets have also been used for detector performance studies, including investigations that rely on the combined performance of different subsystems. This paper presents the results of performance studies related to combined tracking, lepton identification and the reconstruction of jets and missing transverse energy. Results are compared to expectations based on a cosmic-ray event generator and a full simulation of the detector response.
Muons from cosmic-ray interactions in the atmosphere provide a high-statistics source of particles that can be used to study the performance and calibration of the ATLAS detector. Cosmic-ray muons can penetrate to the cavern and deposit energy in all detector subsystems. Such events have played an important role in the commissioning of the detector since the start of the installation phase in 2005 and were particularly important for understanding the detector performance in the time prior to the arrival of the first LHC beams. Global cosmic-ray runs were undertaken in both 2008 and 2009 and these data have been used through to the early phases of collision data-taking as a tool for calibration, alignment and detector monitoring. These large datasets have also been used for detector performance studies, including investigations that rely on the combined performance of different subsystems. This paper presents the results of performance studies related to combined tracking, lepton identification and the reconstruction of jets and missing transverse energy. Results are compared to expectations based on a cosmic-ray event generator and a full simulation of the detector response. RI valente, paolo/A-6640-2010; Rescia, Sergio/D-8604-2011; Castro, Nuno/D-5260-2011; Doyle, Anthony/C-5889-2009; Andreazza, Attilio/E-5642-2011; Jakubek, Jan/E-6530-2011; Marti-Garcia, Salvador/F-3085-2011; Conde Muino, Patricia/F-7696-2011; Stoicea, Gabriel/B-6717-2011; Robson, Aidan/G-1087-2011; Kladiva, Eduard/G-6305-2011; Losada, Marta/B-2261-2010; Bauer, Florian/G-8816-2011; Jones, Roger/H-5578-2011; Gutierrez, Phillip/C-1161-2011; Ferrando, James/A-9192-2012; collins-tooth, christopher/A-9201-2012; Perrino, Roberto/B-4633-2010; De Cecco, Sandro/B-1016-2012; branchini, paolo/A-4857-2011; Wolter, Marcin/A-7412-2012; Rotaru, Marina/A-3097-2011; O'Shea, Val/G-1279-2010; Takai, Helio/C-3301-2012; Britton, David/F-2602-2010; Pina, Joao /C-4391-2012; Li, Xuefei/C-3861-2012; Smirnova, Lidia/D-8089-2012; Smirnov, Sergei/F-1014-2011; Gladilin, Leonid/B-5226-2011; Kramarenko, Victor/E-1781-2012; Prokoshin, Fedor/E-2795-2012; Alexa, Calin/F-6345-2010; Pacheco Pages, Andres/C-5353-2011; Livan, Michele/D-7531-2012; Petrucci, Fabrizio/G-8348-2012; Fabbri, Laura/H-3442-2012; Kurashige, Hisaya/H-4916-2012; Villa, Mauro/C-9883-2009; Delmastro, Marco/I-5599-2012
Muons from cosmic-ray interactions in the atmosphere provide a high-statistics source of particles that can be used to study the performance and calibration of the ATLAS detector. Cosmic-ray muons can penetrate to the cavern and deposit energy in all detector subsystems. Such events have played an important role in the commissioning of the detector since the start of the installation phase in 2005 and were particularly important for understanding the detector performance in the time prior to the arrival of the first LHC beams. Global cosmic-ray runs were undertaken in both 2008 and 2009 and these data have been used through to the early phases of collision data-taking as a tool for calibration, alignment and detector monitoring. These large datasets have also been used for detector performance studies, including investigations that rely on the combined performance of different subsystems. This paper presents the results of performance studies related to combined tracking, lepton identification and the reconstruction of jets and missing transverse energy. Results are compared to expectations based on a cosmic-ray event generator and a full simulation of the detector response.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11770/126354
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