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The DAMPE silicon tungsten tracker

The DArk Matter Particle Explorer (DAMPE) satellite has been successfully launched on the 17th December 2015. It is a powerful space detector designed for the identification of possible Dark Matter signatures thanks to its capability to detect electrons and photons with an unprecedented energy resol...

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Detalles Bibliográficos
Autores principales: Gallo, Valentina, Ambrosi, G, Asfandiyarov, R, Azzarello, P, Bernardini, P, Bertucci, B, Bolognini, A, Cadoux, F, Caprai, M, Domenjoz, M, Dong, Y, Duranti, M, Fan, R, Franco, M, Fusco, P, Gargano, F, Gong, K, Guo, D, Husi, C, Ionica, M, Lacalamita, N, Loparco, F, Marsella, G, Mazziotta, M N, Mongelli, M, Nardinocchi, A, Nicola, L, Pelleriti, G, Peng, W, Pohl, M, Postolache, V, Qiao, R, Surdo, A, Tykhonov, A, Vitillo, S, Wang, H, Weber, M, Wu, D, Wu, X, Zhang, F, De Mitri, I, La Marra, D
Lenguaje:eng
Publicado: SISSA 2017
Materias:
Acceso en línea:https://dx.doi.org/10.22323/1.287.0010
http://cds.cern.ch/record/2287846
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author Gallo, Valentina
Ambrosi, G
Asfandiyarov, R
Azzarello, P
Bernardini, P
Bertucci, B
Bolognini, A
Cadoux, F
Caprai, M
Domenjoz, M
Dong, Y
Duranti, M
Fan, R
Franco, M
Fusco, P
Gargano, F
Gong, K
Guo, D
Husi, C
Ionica, M
Lacalamita, N
Loparco, F
Marsella, G
Mazziotta, M N
Mongelli, M
Nardinocchi, A
Nicola, L
Pelleriti, G
Peng, W
Pohl, M
Postolache, V
Qiao, R
Surdo, A
Tykhonov, A
Vitillo, S
Wang, H
Weber, M
Wu, D
Wu, X
Zhang, F
De Mitri, I
La Marra, D
author_facet Gallo, Valentina
Ambrosi, G
Asfandiyarov, R
Azzarello, P
Bernardini, P
Bertucci, B
Bolognini, A
Cadoux, F
Caprai, M
Domenjoz, M
Dong, Y
Duranti, M
Fan, R
Franco, M
Fusco, P
Gargano, F
Gong, K
Guo, D
Husi, C
Ionica, M
Lacalamita, N
Loparco, F
Marsella, G
Mazziotta, M N
Mongelli, M
Nardinocchi, A
Nicola, L
Pelleriti, G
Peng, W
Pohl, M
Postolache, V
Qiao, R
Surdo, A
Tykhonov, A
Vitillo, S
Wang, H
Weber, M
Wu, D
Wu, X
Zhang, F
De Mitri, I
La Marra, D
author_sort Gallo, Valentina
collection CERN
description The DArk Matter Particle Explorer (DAMPE) satellite has been successfully launched on the 17th December 2015. It is a powerful space detector designed for the identification of possible Dark Matter signatures thanks to its capability to detect electrons and photons with an unprecedented energy resolution in an energy range going from few GeV up to 10 TeV. Moreover, the DAMPE satellite will contribute to a better understanding of the propagation mechanisms of high energy cosmic rays measuring the nuclei flux up to 100 TeV. DAMPE is composed of four sub-detectors: a plastic strip scintillator, a silicon-tungsten tracker-converter (STK), a BGO imaging calorimeter and a neutron detector. The STK is made of twelve layers of single-sided AC-coupled silicon micro-strip detectors for a total silicon area of about 7 $m^2$ . To promote the conversion of incident photons into electron-positron pairs, tungsten foils are inserted into the supporting structure. In this document, a detailed description of the STK construction and its performance on orbit are reported.
id oai-inspirehep.net-1615381
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2017
publisher SISSA
record_format invenio
spelling oai-inspirehep.net-16153812021-05-03T07:54:13Zdoi:10.22323/1.287.0010http://cds.cern.ch/record/2287846engGallo, ValentinaAmbrosi, GAsfandiyarov, RAzzarello, PBernardini, PBertucci, BBolognini, ACadoux, FCaprai, MDomenjoz, MDong, YDuranti, MFan, RFranco, MFusco, PGargano, FGong, KGuo, DHusi, CIonica, MLacalamita, NLoparco, FMarsella, GMazziotta, M NMongelli, MNardinocchi, ANicola, LPelleriti, GPeng, WPohl, MPostolache, VQiao, RSurdo, ATykhonov, AVitillo, SWang, HWeber, MWu, DWu, XZhang, FDe Mitri, ILa Marra, DThe DAMPE silicon tungsten trackerDetectors and Experimental TechniquesThe DArk Matter Particle Explorer (DAMPE) satellite has been successfully launched on the 17th December 2015. It is a powerful space detector designed for the identification of possible Dark Matter signatures thanks to its capability to detect electrons and photons with an unprecedented energy resolution in an energy range going from few GeV up to 10 TeV. Moreover, the DAMPE satellite will contribute to a better understanding of the propagation mechanisms of high energy cosmic rays measuring the nuclei flux up to 100 TeV. DAMPE is composed of four sub-detectors: a plastic strip scintillator, a silicon-tungsten tracker-converter (STK), a BGO imaging calorimeter and a neutron detector. The STK is made of twelve layers of single-sided AC-coupled silicon micro-strip detectors for a total silicon area of about 7 $m^2$ . To promote the conversion of incident photons into electron-positron pairs, tungsten foils are inserted into the supporting structure. In this document, a detailed description of the STK construction and its performance on orbit are reported.SISSAoai:inspirehep.net:16153812017
spellingShingle Detectors and Experimental Techniques
Gallo, Valentina
Ambrosi, G
Asfandiyarov, R
Azzarello, P
Bernardini, P
Bertucci, B
Bolognini, A
Cadoux, F
Caprai, M
Domenjoz, M
Dong, Y
Duranti, M
Fan, R
Franco, M
Fusco, P
Gargano, F
Gong, K
Guo, D
Husi, C
Ionica, M
Lacalamita, N
Loparco, F
Marsella, G
Mazziotta, M N
Mongelli, M
Nardinocchi, A
Nicola, L
Pelleriti, G
Peng, W
Pohl, M
Postolache, V
Qiao, R
Surdo, A
Tykhonov, A
Vitillo, S
Wang, H
Weber, M
Wu, D
Wu, X
Zhang, F
De Mitri, I
La Marra, D
The DAMPE silicon tungsten tracker
title The DAMPE silicon tungsten tracker
title_full The DAMPE silicon tungsten tracker
title_fullStr The DAMPE silicon tungsten tracker
title_full_unstemmed The DAMPE silicon tungsten tracker
title_short The DAMPE silicon tungsten tracker
title_sort dampe silicon tungsten tracker
topic Detectors and Experimental Techniques
url https://dx.doi.org/10.22323/1.287.0010
http://cds.cern.ch/record/2287846
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