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Performance of the ISS-CREAM Calorimeter
The Cosmic Ray Energetics And Mass experiment for the International Space Station (ISS-CREAM) is scheduled for launch in 2017. It is designed to directly measure and identify theelemental composition of incident Galactic cosmic rays from a few hundred GeV to PeV energies.Such large energy range sens...
Autores principales: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Lenguaje: | eng |
Publicado: |
SISSA
2017
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.22323/1.301.0247 http://cds.cern.ch/record/2676811 |
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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, L Eraud, L Hagenau, L Han, J H Huh, H G Hwang, Y S Hyun, H J Im, S Jeon, H B Jeon, J A Jeong, S Kang, S C Kim, H J 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, H Park, I H Park, J M 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, L Eraud, L Hagenau, L Han, J H Huh, H G Hwang, Y S Hyun, H J Im, S Jeon, H B Jeon, J A Jeong, S Kang, S C Kim, H J 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, H Park, I H Park, J M 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 Cosmic Ray Energetics And Mass experiment for the International Space Station (ISS-CREAM) is scheduled for launch in 2017. It is designed to directly measure and identify theelemental composition of incident Galactic cosmic rays from a few hundred GeV to PeV energies.Such large energy range sensitivity is reached by using an electromagnetic sampling calorimeter(CAL) which measures the energy deposit of particle-induced showers. The CAL is composedof twenty layers of tungsten plates interleaved with scintillating fibers, and glued together usingepoxy-coated fiberglass to comply with space launch requirements. In August 2015, beam testmeasurements were performed at CERN to verify the performance of the CAL using layers ofepoxy-coated fiberglass placed between tungsten plates. The CAL response to electron and pionbeams and its performance are reported and compared with previous beam test configurations. |
id | oai-inspirehep.net-1686196 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2017 |
publisher | SISSA |
record_format | invenio |
spelling | oai-inspirehep.net-16861962019-10-15T15:20:32Zdoi:10.22323/1.301.0247http://cds.cern.ch/record/2676811engPicot-Clémente, NicolasAmare, YAnderson, TAngelaszek, DAnthony, NCheryian, KChoi, G HCopley, MCoutu, SDerome, LEraud, LHagenau, LHan, J HHuh, H GHwang, Y SHyun, H JIm, SJeon, H BJeon, J AJeong, SKang, S CKim, H JKim, 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, HPark, I HPark, J MQuinn, RSeo, E SSmith, J RWalpole, PWeinmann, R PWu, JYoon, Y SPerformance of the ISS-CREAM CalorimeterDetectors and Experimental TechniquesThe Cosmic Ray Energetics And Mass experiment for the International Space Station (ISS-CREAM) is scheduled for launch in 2017. It is designed to directly measure and identify theelemental composition of incident Galactic cosmic rays from a few hundred GeV to PeV energies.Such large energy range sensitivity is reached by using an electromagnetic sampling calorimeter(CAL) which measures the energy deposit of particle-induced showers. The CAL is composedof twenty layers of tungsten plates interleaved with scintillating fibers, and glued together usingepoxy-coated fiberglass to comply with space launch requirements. In August 2015, beam testmeasurements were performed at CERN to verify the performance of the CAL using layers ofepoxy-coated fiberglass placed between tungsten plates. The CAL response to electron and pionbeams and its performance are reported and compared with previous beam test configurations.SISSAoai:inspirehep.net:16861962017 |
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, L Eraud, L Hagenau, L Han, J H Huh, H G Hwang, Y S Hyun, H J Im, S Jeon, H B Jeon, J A Jeong, S Kang, S C Kim, H J 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, H Park, I H Park, J M Quinn, R Seo, E S Smith, J R Walpole, P Weinmann, R P Wu, J Yoon, Y S Performance of the ISS-CREAM Calorimeter |
title | Performance of the ISS-CREAM Calorimeter |
title_full | Performance of the ISS-CREAM Calorimeter |
title_fullStr | Performance of the ISS-CREAM Calorimeter |
title_full_unstemmed | Performance of the ISS-CREAM Calorimeter |
title_short | Performance of the ISS-CREAM Calorimeter |
title_sort | performance of the iss-cream calorimeter |
topic | Detectors and Experimental Techniques |
url | https://dx.doi.org/10.22323/1.301.0247 http://cds.cern.ch/record/2676811 |
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