| RIPA, J., G. GALGOCZI, Norbert WERNER, A. PAL, M. OHNO, L. MESZAROS, T. MIZUNO, N. TARCAI, K. TORIGOE, N. UCHIDA, Y. FUKAZAWA, H. TAKAHASHI, K. NAKAZAWA, N. HIRADE, K. HIROSE, S. HISADOMI, T. ENOTO, H. ODAKA, Y. ICHINOHE, Z. FREI a L. KISS. Estimation of the detected background by the future gamma ray transient mission CAMELOT. Astronomische Nachrichten. WEINHEIM: WILEY-V C H VERLAG GMBH, 2019, roč. 340, č. 7, s. 666-673. ISSN 0004-6337. Dostupné z: https://dx.doi.org/10.1002/asna.201913673. |
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@article{1586737,
author = {Ripa, J. and Galgoczi, G. and Werner, Norbert and Pal, A. and Ohno, M. and Meszaros, L. and Mizuno, T. and Tarcai, N. and Torigoe, K. and Uchida, N. and Fukazawa, Y. and Takahashi, H. and Nakazawa, K. and Hirade, N. and Hirose, K. and Hisadomi, S. and Enoto, T. and Odaka, H. and Ichinohe, Y. and Frei, Z. and Kiss, L.},
article_location = {WEINHEIM},
article_number = {7},
doi = {http://dx.doi.org/10.1002/asna.201913673},
keywords = {(ISM; ) cosmic rays; gamma rays; bursts; instrumentation; detectors; X-rays; diffuse background},
language = {eng},
issn = {0004-6337},
journal = {Astronomische Nachrichten},
title = {Estimation of the detected background by the future gamma ray transient mission CAMELOT},
url = {https://arxiv.org/pdf/1909.00339.pdf},
volume = {340},
year = {2019}
}
TY - JOUR
ID - 1586737
AU - Ripa, J. - Galgoczi, G. - Werner, Norbert - Pal, A. - Ohno, M. - Meszaros, L. - Mizuno, T. - Tarcai, N. - Torigoe, K. - Uchida, N. - Fukazawa, Y. - Takahashi, H. - Nakazawa, K. - Hirade, N. - Hirose, K. - Hisadomi, S. - Enoto, T. - Odaka, H. - Ichinohe, Y. - Frei, Z. - Kiss, L.
PY - 2019
TI - Estimation of the detected background by the future gamma ray transient mission CAMELOT
JF - Astronomische Nachrichten
VL - 340
IS - 7
SP - 666-673
EP - 666-673
PB - WILEY-V C H VERLAG GMBH
SN - 00046337
KW - (ISM
KW - ) cosmic rays
KW - gamma rays
KW - bursts
KW - instrumentation
KW - detectors
KW - X-rays
KW - diffuse background
UR - https://arxiv.org/pdf/1909.00339.pdf
N2 - This study presents a background estimation for the CubeSats Applied for MEasuring and LOcalising Transients (CAMELOT), which is a proposed fleet of nanosatellites for the all-sky monitoring and timing-based localization of gamma ray transients with precise localization capability at low Earth orbits. CAMELOT will allow us to observe and precisely localize short gamma ray bursts (GRBs) associated with kilonovae, long GRBs associated with core-collapse massive stars, magnetar outbursts, terrestrial gamma ray flashes, and gamma ray counterparts to gravitational wave sources. A fleet of at least nine 3U CubeSats is proposed to be equipped with large and thin CsI(Tl) scintillators read out by multipixel photon counters (MPPC). A careful study of the radiation environment in space is necessary to optimize the detector casing, estimate the duty cycle due to the crossing of the South Atlantic Anomaly and polar regions, and minimize the effect of the radiation damage of MPPCs.
ER -
RIPA, J., G. GALGOCZI, Norbert WERNER, A. PAL, M. OHNO, L. MESZAROS, T. MIZUNO, N. TARCAI, K. TORIGOE, N. UCHIDA, Y. FUKAZAWA, H. TAKAHASHI, K. NAKAZAWA, N. HIRADE, K. HIROSE, S. HISADOMI, T. ENOTO, H. ODAKA, Y. ICHINOHE, Z. FREI a L. KISS. Estimation of the detected background by the future gamma ray transient mission CAMELOT. \textit{Astronomische Nachrichten}. WEINHEIM: WILEY-V C H VERLAG GMBH, 2019, roč.~340, č.~7, s.~666-673. ISSN~0004-6337. Dostupné z: https://dx.doi.org/10.1002/asna.201913673.
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