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The CMS silicon tracker, consisting of 1440 silicon pixel and 15 148 silicon strip detector modules, has been aligned using more than three million cosmic ray charged particles, with additional information from optical surveys. The positions of the modules were determined with respect to cosmic ray trajectories to an average precision of 3-4 microns RMS in the barrel and 3-14 microns RMS in the endcap in the most sensitive coordinate. The results have been validated by several studies, including laser beam cross-checks, track fit self-consistency, track residuals in overlapping module regions, and track parameter resolution, and are compared with predictions obtained from simulation. Correlated systematic effects have been investigated. The track parameter resolutions obtained with this alignment are close to the design performance.
(2010). Alignment of the CMS silicon tracker during commissioning with cosmic rays [journal article - articolo]. In JOURNAL OF INSTRUMENTATION. Retrieved from http://hdl.handle.net/10446/187118
Alignment of the CMS silicon tracker during commissioning with cosmic rays
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Kotov;A. Kropivnitskaya;T. Kypreos;A. Madorsky;K. Matchev;G. Mitselmakher;Y. Pakhotin;J. P. Gomez;C. Prescott;V. Rapsevicius;R. Remington;M. Schmitt;B. Scurlock;D. Wang;J. Yelton;C. Ceron;V. Gaultney;L. Kramer;L. M. Lebolo;S. Linn;P. Markowitz;G. Martinez;J. L. Rodriguez;T. Adams;A. Askew;H. Baer;M. Bertoldi;J. Chen;W. G. D.;S. V. Gleyzer;J. Haas;S. Hagopian;V. Hagopian;M. Jenkins;K. F. Johnson;E. Prettner;H. Prosper;S. Sekmen;M. M. Baarmand;S. Guragain;M. Hohlmann;H. Kalakhety;H. Mermerkaya;R. Ralich;I. Vodopiyanov;B. Abelev;M. R. Adams;I. M. Anghel;L. Apanasevich;V. E. Bazterra;R. R. Betts;J. Callner;M. A. Castro;R. Cavanaugh;C. Dragoiu;E. J. Garcia-Solis;C. E. Gerber;D. J. Hofman;S. Khalatian;C. Mironov;E. Shabalina;A. Smoron;N. Varelas;U. Akgun;E. A. Albayrak;A. S. Ayan;B. Bilki;R. Briggs;K. Cankocak;K. Chung;W. Clarida;P. Debbins;F. Duru;F. D. Ingram;C. K. Lae;E. McCliment;J. P. Merlo;A. Mestvirishvili;M. J. Miller;A. Moeller;J. Nachtman;C. R. Newsom;E. Norbeck;J. Olson;Y. Onel;F. Ozok;J. Parsons;I. Schmidt;S. Sen;J. Wetzel;T. Yetkin;K. Yi;B. A. Barnett;B. Blumenfeld;A. Bonato;C. Y. Chien;D. Fehling;G. Giurgiu;A. V. Gritsan;Z. J. Guo;P. Maksimovic;S. Rappoccio;M. Swartz;N. V. Tran;Y. Zhang;P. Baringer;A. Bean;O. Grachov;M. Murray;V. Radicci;S. Sanders;J. S. Wood;V. Zhukova;D. Bandurin;T. Bolton;K. Kaadze;A. Liu;Y. Maravin;D. Onoprienko;I. Svintradze;Z. Wan;J. Gronberg;J. Hollar;D. Lange;D. Wright;D. Baden;R. Bard;M. Boutemeur;S. C. Eno;D. Ferencek;N. J. Hadley;R. G. Kellogg;M. Kirn;S. Kunori;K. Rossato;P. Rumerio;F. Santanastasio;A. Skuja;J. Temple;M. B. Tonjes;S. C. Tonwar;T. Toole;E. Twedt;B. Alver;G. Bauer;J. Bendavid;W. Busza;E. Butz;I. A. Cali;M. Chan;D. D'Enterria;P. Everaerts;G. G. Ceballos;K. A. Hahn;P. Harris;S. Jaditz;Y. Kim;M. Klute;Y. J. Lee;W. Li;C. Loizides;T. Ma;M. Miller;S. Nahn;C. Paus;C. Roland;G. Roland;M. Rudolph;G. Stephans;K. Sumorok;K. Sung;S. Vaurynovich;E. A. Wenger;B. Wyslouch;S. Xie;Y. Yilmaz;A. S. Yoon;D. Bailleux;S. I. Cooper;P. Cushman;B. Dahmes;A. D. Benedetti;A. Dolgopolov;P. R. Dudero;R. Egeland;G. Franzoni;J. Haupt;A. Inyakin;K. Klapoetke;Y. Kubota;J. Mans;N. Mirman;D. Petyt;V. Rekovic;R. Rusack;M. Schroeder;A. Singovsky;J. Zhang;L. M. Cremaldi;R. Godang;R. Kroeger;L. Perera;R. Rahmat;D. A. Sanders;P. Sonnek;D. Summers;K. Bloom;B. Bockelman;S. Bose;J. Butt;D. R. Claes;A. Dominguez;M. Eads;J. Keller;T. Kelly;I. Kravchenko;J. Lazo-Flores;C. Lundstedt;H. Malbouisson;S. Malik;G. R. Snow;U. Baur;I. Iashvili;A. Kharchilava;A. Kumar;K. Smith;M. Strang;G. Alverson;E. Barberis;O. Boeriu;G. Eulisse;G. Govi;T. McCauley;Y. Musienko;S. Muzaffar;I. Osborne;T. Paul;S. Reucroft;J. Swain;L. Taylor;L. Tuura;A. Anastassov;B. Gobbi;A. Kubik;R. A. Ofierzynski;A. Pozdnyakov;M. Schmitt;S. Stoynev;M. Velasco;S. Won;L. Antonelli;D. Berry;M. Hildreth;C. Jessop;D. J. Karmgard;T. Kolberg;K. Lannon;S. Lynch;N. Marinelli;D. M. Morse;R. Ruchti;J. Slaunwhite;J. Warchol;M. Wayne;B. Bylsma;L. S. Durkin;J. Gilmore;J. Gu;P. 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Savin;W. H. Smith;A. Sourkov;J. Swanson;M. Weinberg;D. Wenman;M. Wensveen;A. White
2010-01-01
Abstract
The CMS silicon tracker, consisting of 1440 silicon pixel and 15 148 silicon strip detector modules, has been aligned using more than three million cosmic ray charged particles, with additional information from optical surveys. The positions of the modules were determined with respect to cosmic ray trajectories to an average precision of 3-4 microns RMS in the barrel and 3-14 microns RMS in the endcap in the most sensitive coordinate. The results have been validated by several studies, including laser beam cross-checks, track fit self-consistency, track residuals in overlapping module regions, and track parameter resolution, and are compared with predictions obtained from simulation. Correlated systematic effects have been investigated. The track parameter resolutions obtained with this alignment are close to the design performance.
Chatrchyan, S.; Khachatryan, V.; Sirunyan, A. M.; Adam, W.; Arnold, B.; Bergauer, H.; Bergauer, T.; Dragicevic, M.; Eichberger, M.; Ero, J.; Friedl, M...espandi
(2010). Alignment of the CMS silicon tracker during commissioning with cosmic rays [journal article - articolo]. In JOURNAL OF INSTRUMENTATION. Retrieved from http://hdl.handle.net/10446/187118
Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10446/187118
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simulazione ASN
Il report seguente simula gli indicatori relativi alla propria produzione scientifica in relazione alle soglie ASN 2023-2025 del proprio SC/SSD. Si ricorda che il superamento dei valori soglia (almeno 2 su 3) è requisito necessario ma non sufficiente al conseguimento dell'abilitazione. La simulazione si basa sui dati IRIS e sugli indicatori bibliometrici alla data indicata e non tiene conto di eventuali periodi di congedo obbligatorio, che in sede di domanda ASN danno diritto a incrementi percentuali dei valori. La simulazione può differire dall'esito di un’eventuale domanda ASN sia per errori di catalogazione e/o dati mancanti in IRIS, sia per la variabilità dei dati bibliometrici nel tempo. Si consideri che Anvur calcola i valori degli indicatori all'ultima data utile per la presentazione delle domande.
La presente simulazione è stata realizzata sulla base delle specifiche raccolte sul tavolo ER del Focus Group IRIS coordinato dall’Università di Modena e Reggio Emilia e delle regole riportate nel DM 589/2018 e allegata Tabella A. Cineca, l’Università di Modena e Reggio Emilia e il Focus Group IRIS non si assumono alcuna responsabilità in merito all’uso che il diretto interessato o terzi faranno della simulazione. Si specifica inoltre che la simulazione contiene calcoli effettuati con dati e algoritmi di pubblico dominio e deve quindi essere considerata come un mero ausilio al calcolo svolgibile manualmente o con strumenti equivalenti.