Abstract
| Original language | English |
|---|---|
| Article number | 218 |
| Journal | P o S - Proceedings of Science |
| Number of pages | 8 |
| ISSN | 1824-8039 |
| Publication status | Published - 2017 |
| Event | 35th International Cosmic Ray Conference (ICRC2017) - Busan Exhibition & Convention Center, Busan, Korea, Republic of Duration: 12 Jul 2017 → 20 Jul 2017 |
Conference
| Conference | 35th International Cosmic Ray Conference (ICRC2017) |
|---|---|
| Location | Busan Exhibition & Convention Center |
| Country | Korea, Republic of |
| City | Busan |
| Period | 12/07/2017 → 20/07/2017 |
Bibliographical note
Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)Cite this
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Cosmic ray effect on the X-ray Trigger Telescope of UFFO/Lomonosov using YSO scintillation crystal array in space. / Kim, M. B. ; Jeong, S.; Jeong, H. M.; Leonov, V. ; Lee, J; Park, I.H.; Amelushkin, A.M.; Barinova, V. O. ; Bogomolov, A.V. ; Bogomolov, V. V.; Brandt, Søren; Budtz-Jørgensen, Carl; Castro-Tirado, A. J.; Chen, P.; Connell, P.; Garipov, G. ; Gorbovskoy, E. S. ; Dzhioeva, N. L.; Eyles, C. ; Huang, M.-H. A. ; Iyudin, A.F.; Kalegaev, V. V. ; Kasarjan, P. S. ; Kim, J. E.; Kornilov, V. G. ; Kuznetsova, E. A. ; Lim, H.; Lipunov, V. M.; Liu, T. -C.; Myagkova, I. N. ; Nam, J. W. ; Panasyuk, M. I. ; Panchenko, M. I. ; Petrov, V. L.; Prokhorov, A. V. ; Reglero, V. ; Ripa, J.; Rodrigo, J. M. ; Shustova, A. N. ; Svertilov, S. I.; Tyurina, N. V ; Yashin, I. V. .
In: P o S - Proceedings of Science, 2017.Research output: Contribution to journal › Conference article › Research › peer-review
TY - GEN
T1 - Cosmic ray effect on the X-ray Trigger Telescope of UFFO/Lomonosov using YSO scintillation crystal array in space
AU - Kim, M. B.
AU - Jeong, S.
AU - Jeong, H. M.
AU - Leonov, V.
AU - Lee, J
AU - Park, I.H.
AU - Amelushkin, A.M.
AU - Barinova, V. O.
AU - Bogomolov, A.V.
AU - Bogomolov, V. V.
AU - Brandt, Søren
AU - Budtz-Jørgensen, Carl
AU - Castro-Tirado, A. J.
AU - Chen, P.
AU - Connell, P.
AU - Garipov, G.
AU - Gorbovskoy, E. S.
AU - Dzhioeva, N. L.
AU - Eyles, C.
AU - Huang, M.-H. A.
AU - Iyudin, A.F.
AU - Kalegaev, V. V.
AU - Kasarjan, P. S.
AU - Kim, J. E.
AU - Kornilov, V. G.
AU - Kuznetsova, E. A.
AU - Lim, H.
AU - Lipunov, V. M.
AU - Liu, T. -C.
AU - Myagkova, I. N.
AU - Nam, J. W.
AU - Panasyuk, M. I.
AU - Panchenko, M. I.
AU - Petrov, V. L.
AU - Prokhorov, A. V.
AU - Reglero, V.
AU - Ripa, J.
AU - Rodrigo, J. M.
AU - Shustova, A. N.
AU - Svertilov, S. I.
AU - Tyurina, N. V
AU - Yashin, I. V.
N1 - Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)
PY - 2017
Y1 - 2017
N2 - UFFO Burst Alert and Trigger telescope (UBAT) is the X-ray trigger telescope of UFFO/Lomonosov to localize X-ray source with coded mask method and X-ray detector. Its X-ray detector is made up of 36 8×8 pixels Yttrium OxyorthoSilicate (Y2SiO5:Ce, YSO) scintillation crystal arrays and 36 64-channel Multi-Anode PhotoMultiplier Tubes (MAPMTs) for space mission. Its effective detection area is 161cm2 and energy range is several keV to 150 keV. It was successfully launched in April 28, 2016. In several calibration run, we got several X-ray background data. We already knew X-ray background flux is 2-3 counts/cm2/sec in space. However our X-ray background data shows approximately 7-8 times higher than what we know. There are many candidates to explain high X-ray background count in space. One of candidates is cosmic ray. We will report cosmic ray effect on the X-ray detector using YSO scintillation crystal arrays in space.
AB - UFFO Burst Alert and Trigger telescope (UBAT) is the X-ray trigger telescope of UFFO/Lomonosov to localize X-ray source with coded mask method and X-ray detector. Its X-ray detector is made up of 36 8×8 pixels Yttrium OxyorthoSilicate (Y2SiO5:Ce, YSO) scintillation crystal arrays and 36 64-channel Multi-Anode PhotoMultiplier Tubes (MAPMTs) for space mission. Its effective detection area is 161cm2 and energy range is several keV to 150 keV. It was successfully launched in April 28, 2016. In several calibration run, we got several X-ray background data. We already knew X-ray background flux is 2-3 counts/cm2/sec in space. However our X-ray background data shows approximately 7-8 times higher than what we know. There are many candidates to explain high X-ray background count in space. One of candidates is cosmic ray. We will report cosmic ray effect on the X-ray detector using YSO scintillation crystal arrays in space.
M3 - Conference article
JO - P o S - Proceedings of Science
JF - P o S - Proceedings of Science
SN - 1824-8039
M1 - 218
ER -