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Alignment of the NOMAD-STAR detector
This note describes the alignment of the NOMAD-STAR detector. This is the B/sub 4/C-silicon target installed in the NOMAD spectrometer in 1997. NOMAD-STAR is composed of modules of 12 silicon detectors each giving a total length of 72 cm. Ten of these modules (called ladders) are assembled to form a...
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Lenguaje: | eng |
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2000
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Acceso en línea: | https://dx.doi.org/10.1016/S0168-9002(00)00177-7 http://cds.cern.ch/record/449540 |
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author | Cervera-Villanueva, A |
author_facet | Cervera-Villanueva, A |
author_sort | Cervera-Villanueva, A |
collection | CERN |
description | This note describes the alignment of the NOMAD-STAR detector. This is the B/sub 4/C-silicon target installed in the NOMAD spectrometer in 1997. NOMAD-STAR is composed of modules of 12 silicon detectors each giving a total length of 72 cm. Ten of these modules (called ladders) are assembled to form a layer. There are five layers interleaved with passive boron carbide plates. The total surface of silicon is 1.14 m /sup 2/. Energetic muons from the flat-top of the CERN SPS cycle provide the necessary information to perform a very precise software alignment. This alignment is needed to ensure that the impact parameter measurement needed for the identification of taus in a detector like NOMAD-STAR will not be limited by the error in the alignment. (15 refs). |
id | cern-449540 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2000 |
record_format | invenio |
spelling | cern-4495402019-09-30T06:29:59Zdoi:10.1016/S0168-9002(00)00177-7http://cds.cern.ch/record/449540engCervera-Villanueva, AAlignment of the NOMAD-STAR detectorDetectors and Experimental TechniquesThis note describes the alignment of the NOMAD-STAR detector. This is the B/sub 4/C-silicon target installed in the NOMAD spectrometer in 1997. NOMAD-STAR is composed of modules of 12 silicon detectors each giving a total length of 72 cm. Ten of these modules (called ladders) are assembled to form a layer. There are five layers interleaved with passive boron carbide plates. The total surface of silicon is 1.14 m /sup 2/. Energetic muons from the flat-top of the CERN SPS cycle provide the necessary information to perform a very precise software alignment. This alignment is needed to ensure that the impact parameter measurement needed for the identification of taus in a detector like NOMAD-STAR will not be limited by the error in the alignment. (15 refs).oai:cds.cern.ch:4495402000 |
spellingShingle | Detectors and Experimental Techniques Cervera-Villanueva, A Alignment of the NOMAD-STAR detector |
title | Alignment of the NOMAD-STAR detector |
title_full | Alignment of the NOMAD-STAR detector |
title_fullStr | Alignment of the NOMAD-STAR detector |
title_full_unstemmed | Alignment of the NOMAD-STAR detector |
title_short | Alignment of the NOMAD-STAR detector |
title_sort | alignment of the nomad-star detector |
topic | Detectors and Experimental Techniques |
url | https://dx.doi.org/10.1016/S0168-9002(00)00177-7 http://cds.cern.ch/record/449540 |
work_keys_str_mv | AT cerveravillanuevaa alignmentofthenomadstardetector |