FMSR (Austria), FNRS (Belgium), FWO (Belgium), CNPq (Brazil), CAPES (Brazil), FAPERJ (Brazil), FAPESP (Brazil), MES (Bulgaria), CERN (China), CAS (China), MoST (China), NSFC (China), COLCIEN-CIAS (Colombia), MSES (Croatia), RPF (Cyprus), Academy of Sciences (Estonia), NICPB (Estonia, Academy of Finland, ME (Finland), HIP (Finland), CEA (France), CNRS/IN2P3 (France), BMBF, Germany, DFG (Germany), HGF (Germany), GSRT (Greece), OTKA (Hungary), NKTH (Hungary), DAE (India), DST (India), IPM (Iran), SFI (Ireland), INFN (Italy), NRF (Korea), LAS (Lithuania), CINVESTAV (Mexico), CONACYT (Mexico), SEP (Mexico), UASLP-FAI (Mexico), PAEC (Pakistan), SCSR (Poland), FCT (Portugal), JINR (Armenia), JINR (Belarus), JINR (Georgia), JINR (Ukraine), JINR (Uzbekistan), MST (Russia), MAE (Russia), MSTDS (Serbia), MICINN (Spain), CPAN (Spain), Swiss Funding Agencies (Switzerland), NSC (Taipei), TUBITAK (Turkey), TAEK (Turkey), STFC (United Kingdom), DOE (USA), NSF (USA), European Union, Leventis Foundation, A.P. Sloan Foundation, Alexander von Humboldt Foundation

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FMSR (Austria), FNRS (Belgium), FWO (Belgium), CNPq (Brazil), CAPES (Brazil), FAPERJ (Brazil), FAPESP (Brazil), MES (Bulgaria), CERN (China), CAS (China), MoST (China), NSFC (China), COLCIEN-CIAS (Colombia), MSES (Croatia), RPF (Cyprus), Academy of Sciences (Estonia), NICPB (Estonia, Academy of Finland, ME (Finland), HIP (Finland), CEA (France), CNRS/IN2P3 (France), BMBF, Germany, DFG (Germany), HGF (Germany), GSRT (Greece), OTKA (Hungary), NKTH (Hungary), DAE (India), DST (India), IPM (Iran), SFI (Ireland), INFN (Italy), NRF (Korea), LAS (Lithuania), CINVESTAV (Mexico), CONACYT (Mexico), SEP (Mexico), UASLP-FAI (Mexico), PAEC (Pakistan), SCSR (Poland), FCT (Portugal), JINR (Armenia), JINR (Belarus), JINR (Georgia), JINR (Ukraine), JINR (Uzbekistan), MST (Russia), MAE (Russia), MSTDS (Serbia), MICINN (Spain), CPAN (Spain), Swiss Funding Agencies (Switzerland), NSC (Taipei), TUBITAK (Turkey), TAEK (Turkey), STFC (United Kingdom), DOE (USA), NSF (USA), European Union, Leventis Foundation, A.P. Sloan Foundation, Alexander von Humboldt Foundation

Authors

Publications

Alignment of the CMS silicon tracker during commissioning with cosmic rays

Chatrchyan, S.; Adžić, Petar; Đorđević, Miloš; Jovanović, Dragana J.; Krpić, D.; Maletić, Dimitrije; Puzović, Jovan M.; Smiljković, Nikola; Milenović, Predrag

(2010) 

TY  - JOUR
AU  - Chatrchyan, S.
AU  - Adžić, Petar
AU  - Đorđević, Miloš
AU  - Jovanović, Dragana J.
AU  - Krpić, D.
AU  - Maletić, Dimitrije
AU  - Puzović, Jovan M.
AU  - Smiljković, Nikola
AU  - Milenović, Predrag
PY  - 2010
UR  - https://vinar.vin.bg.ac.rs/handle/123456789/4069
AB  - 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.
T2  - Journal of Instrumentation
T1  - Alignment of the CMS silicon tracker during commissioning with cosmic rays
VL  - 5
DO  - 10.1088/1748-0221/5/03/T03009
ER  - 
@article{
author = "Chatrchyan, S. and Adžić, Petar and Đorđević, Miloš and Jovanović, Dragana J. and Krpić, D. and Maletić, Dimitrije and Puzović, Jovan M. and Smiljković, Nikola and Milenović, Predrag",
year = "2010",
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.",
journal = "Journal of Instrumentation",
title = "Alignment of the CMS silicon tracker during commissioning with cosmic rays",
volume = "5",
doi = "10.1088/1748-0221/5/03/T03009"
}
Chatrchyan, S., Adžić, P., Đorđević, M., Jovanović, D. J., Krpić, D., Maletić, D., Puzović, J. M., Smiljković, N.,& Milenović, P.. (2010). Alignment of the CMS silicon tracker during commissioning with cosmic rays. in Journal of Instrumentation, 5.
https://doi.org/10.1088/1748-0221/5/03/T03009
Chatrchyan S, Adžić P, Đorđević M, Jovanović DJ, Krpić D, Maletić D, Puzović JM, Smiljković N, Milenović P. Alignment of the CMS silicon tracker during commissioning with cosmic rays. in Journal of Instrumentation. 2010;5.
doi:10.1088/1748-0221/5/03/T03009 .
Chatrchyan, S., Adžić, Petar, Đorđević, Miloš, Jovanović, Dragana J., Krpić, D., Maletić, Dimitrije, Puzović, Jovan M., Smiljković, Nikola, Milenović, Predrag, "Alignment of the CMS silicon tracker during commissioning with cosmic rays" in Journal of Instrumentation, 5 (2010),
https://doi.org/10.1088/1748-0221/5/03/T03009 . .
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