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Performance of the BACCUS Transition Radiation Detector

The Boron And Carbon Cosmic rays in the Upper Stratosphere (BACCUS) balloon-borne exper-iment flew for 30 days over Antarctica in December 2016. It is the successor of the CREAMballoon program in Antarctica which recorded a total cumulative exposure of 161 days. BAC-CUS is primarily aimed to measure...

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Autores principales: Picot-Clémente, Nicolas, Amare, Y, Anderson, T, Angelaszek, D, Anthony, N, Cheryian, K, Choi, G H, Copley, M, Coutu, S, Derome, Laurent, Eraud, Ludo, Hagenau, L, Han, J H, Huh, H G, Im, S, Jeon, J A, Jeong, S, Kim, K C, Kim, M H, Lee, H Y, Lee, J, Lee, M H, Liang, J, Link, J T, Lu, L, Lutz, L, Menchaca-Rocha, A, Mernik, T, Mitchell, J W, Mognet, S I, Morton, S, Nester, M, Nutter, S, Ofoha, O, Park, I H, Quinn, R, Seo, E S, Smith, J R, Walpole, P, Weinmann, R P, Wu, J, Yoon, Y S
Lenguaje:eng
Publicado: SISSA 2017
Materias:
Acceso en línea:https://dx.doi.org/10.22323/1.301.0246
http://cds.cern.ch/record/2676810
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author Picot-Clémente, Nicolas
Amare, Y
Anderson, T
Angelaszek, D
Anthony, N
Cheryian, K
Choi, G H
Copley, M
Coutu, S
Derome, Laurent
Eraud, Ludo
Hagenau, L
Han, J H
Huh, H G
Im, S
Jeon, J A
Jeong, S
Kim, K C
Kim, M H
Lee, H Y
Lee, J
Lee, M H
Liang, J
Link, J T
Lu, L
Lutz, L
Menchaca-Rocha, A
Mernik, T
Mitchell, J W
Mognet, S I
Morton, S
Nester, M
Nutter, S
Ofoha, O
Park, I H
Quinn, R
Seo, E S
Smith, J R
Walpole, P
Weinmann, R P
Wu, J
Yoon, Y S
author_facet Picot-Clémente, Nicolas
Amare, Y
Anderson, T
Angelaszek, D
Anthony, N
Cheryian, K
Choi, G H
Copley, M
Coutu, S
Derome, Laurent
Eraud, Ludo
Hagenau, L
Han, J H
Huh, H G
Im, S
Jeon, J A
Jeong, S
Kim, K C
Kim, M H
Lee, H Y
Lee, J
Lee, M H
Liang, J
Link, J T
Lu, L
Lutz, L
Menchaca-Rocha, A
Mernik, T
Mitchell, J W
Mognet, S I
Morton, S
Nester, M
Nutter, S
Ofoha, O
Park, I H
Quinn, R
Seo, E S
Smith, J R
Walpole, P
Weinmann, R P
Wu, J
Yoon, Y S
author_sort Picot-Clémente, Nicolas
collection CERN
description The Boron And Carbon Cosmic rays in the Upper Stratosphere (BACCUS) balloon-borne exper-iment flew for 30 days over Antarctica in December 2016. It is the successor of the CREAMballoon program in Antarctica which recorded a total cumulative exposure of 161 days. BAC-CUS is primarily aimed to measure cosmic-ray boron and carbon fluxes at the highest energiesreachable with a balloon or satellite experiment, in order to provide essential information for abetter understanding of cosmic-ray propagation in the Galaxy. The payload is made of multipleparticle physics detectors which measure the charge up to Z=26 and energy of incident particlesfrom a few hundred GeV to a few PeV. The newly designed Transition Radiation Detector (TRD)measures signals that are a function of the charge and Lorentz factor. In April 2016, BACCUSwas taken to CERN in its flight configuration to characterize its detectors’ response to beams ofelectrons and pions. The performance of the TRD using beam test data are reported in this paper.
id oai-inspirehep.net-1686195
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2017
publisher SISSA
record_format invenio
spelling oai-inspirehep.net-16861952019-10-15T15:20:31Zdoi:10.22323/1.301.0246http://cds.cern.ch/record/2676810engPicot-Clémente, NicolasAmare, YAnderson, TAngelaszek, DAnthony, NCheryian, KChoi, G HCopley, MCoutu, SDerome, LaurentEraud, LudoHagenau, LHan, J HHuh, H GIm, SJeon, J AJeong, SKim, K CKim, M HLee, H YLee, JLee, M HLiang, JLink, J TLu, LLutz, LMenchaca-Rocha, AMernik, TMitchell, J WMognet, S IMorton, SNester, MNutter, SOfoha, OPark, I HQuinn, RSeo, E SSmith, J RWalpole, PWeinmann, R PWu, JYoon, Y SPerformance of the BACCUS Transition Radiation DetectorDetectors and Experimental TechniquesThe Boron And Carbon Cosmic rays in the Upper Stratosphere (BACCUS) balloon-borne exper-iment flew for 30 days over Antarctica in December 2016. It is the successor of the CREAMballoon program in Antarctica which recorded a total cumulative exposure of 161 days. BAC-CUS is primarily aimed to measure cosmic-ray boron and carbon fluxes at the highest energiesreachable with a balloon or satellite experiment, in order to provide essential information for abetter understanding of cosmic-ray propagation in the Galaxy. The payload is made of multipleparticle physics detectors which measure the charge up to Z=26 and energy of incident particlesfrom a few hundred GeV to a few PeV. The newly designed Transition Radiation Detector (TRD)measures signals that are a function of the charge and Lorentz factor. In April 2016, BACCUSwas taken to CERN in its flight configuration to characterize its detectors’ response to beams ofelectrons and pions. The performance of the TRD using beam test data are reported in this paper.SISSAoai:inspirehep.net:16861952017
spellingShingle Detectors and Experimental Techniques
Picot-Clémente, Nicolas
Amare, Y
Anderson, T
Angelaszek, D
Anthony, N
Cheryian, K
Choi, G H
Copley, M
Coutu, S
Derome, Laurent
Eraud, Ludo
Hagenau, L
Han, J H
Huh, H G
Im, S
Jeon, J A
Jeong, S
Kim, K C
Kim, M H
Lee, H Y
Lee, J
Lee, M H
Liang, J
Link, J T
Lu, L
Lutz, L
Menchaca-Rocha, A
Mernik, T
Mitchell, J W
Mognet, S I
Morton, S
Nester, M
Nutter, S
Ofoha, O
Park, I H
Quinn, R
Seo, E S
Smith, J R
Walpole, P
Weinmann, R P
Wu, J
Yoon, Y S
Performance of the BACCUS Transition Radiation Detector
title Performance of the BACCUS Transition Radiation Detector
title_full Performance of the BACCUS Transition Radiation Detector
title_fullStr Performance of the BACCUS Transition Radiation Detector
title_full_unstemmed Performance of the BACCUS Transition Radiation Detector
title_short Performance of the BACCUS Transition Radiation Detector
title_sort performance of the baccus transition radiation detector
topic Detectors and Experimental Techniques
url https://dx.doi.org/10.22323/1.301.0246
http://cds.cern.ch/record/2676810
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