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Alignment of the ALICE Inner Tracking System with cosmic-ray tracks

The ALICE Inner Tracking System (ITS) consists of six cylindrical layers of silicon detectors with three different technologies; in the outward direction: two pixel, two drift and two strip layers. The number of parameters to be determined in the spatial alignment of the 2198 sensor modules of the I...

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Autor principal: Bombonati, C et al
Lenguaje:eng
Publicado: 2009
Materias:
Acceso en línea:http://cds.cern.ch/record/1225496
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author Bombonati, C et al
author_facet Bombonati, C et al
author_sort Bombonati, C et al
collection CERN
description The ALICE Inner Tracking System (ITS) consists of six cylindrical layers of silicon detectors with three different technologies; in the outward direction: two pixel, two drift and two strip layers. The number of parameters to be determined in the spatial alignment of the 2198 sensor modules of the ITS is about 13,000. The target alignment precision is well below 10 μm in some cases (pixels). The sources of alignment information are the survey measurements and the reconstructed tracks from cosmic rays and from proton–proton collisions. The main track-based alignment method uses the Millepede global approach. An iterative local method was developed and used as well. We present the results obtained for the ITS alignment using about 10 5 charged tracks from cosmic rays that have been collected during summer 2008, with the ALICE solenoidal magnetic field switched off.
id cern-1225496
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2009
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spelling cern-12254962019-09-30T06:29:59Zhttp://cds.cern.ch/record/1225496engBombonati, C et alAlignment of the ALICE Inner Tracking System with cosmic-ray tracksDetectors and Experimental TechniquesThe ALICE Inner Tracking System (ITS) consists of six cylindrical layers of silicon detectors with three different technologies; in the outward direction: two pixel, two drift and two strip layers. The number of parameters to be determined in the spatial alignment of the 2198 sensor modules of the ITS is about 13,000. The target alignment precision is well below 10 μm in some cases (pixels). The sources of alignment information are the survey measurements and the reconstructed tracks from cosmic rays and from proton–proton collisions. The main track-based alignment method uses the Millepede global approach. An iterative local method was developed and used as well. We present the results obtained for the ITS alignment using about 10 5 charged tracks from cosmic rays that have been collected during summer 2008, with the ALICE solenoidal magnetic field switched off.ARDA-Note-2009-001ALICE-Int-2009-035oai:cds.cern.ch:12254962009-11-30
spellingShingle Detectors and Experimental Techniques
Bombonati, C et al
Alignment of the ALICE Inner Tracking System with cosmic-ray tracks
title Alignment of the ALICE Inner Tracking System with cosmic-ray tracks
title_full Alignment of the ALICE Inner Tracking System with cosmic-ray tracks
title_fullStr Alignment of the ALICE Inner Tracking System with cosmic-ray tracks
title_full_unstemmed Alignment of the ALICE Inner Tracking System with cosmic-ray tracks
title_short Alignment of the ALICE Inner Tracking System with cosmic-ray tracks
title_sort alignment of the alice inner tracking system with cosmic-ray tracks
topic Detectors and Experimental Techniques
url http://cds.cern.ch/record/1225496
work_keys_str_mv AT bombonaticetal alignmentofthealiceinnertrackingsystemwithcosmicraytracks