Cosmic ray effect on the X-ray Trigger Telescope of UFFO/Lomonosov using YSO scintillation crystal array in space

M. B. Kim, S. Jeong, H. M. Jeong, V. Leonov, J Lee, I.H. Park, A.M. Amelushkin, V. O. Barinova, A.V. Bogomolov, V. V. Bogomolov, Søren Brandt, Carl Budtz-Jørgensen, A. J. Castro-Tirado, P. Chen, P. Connell, G. Garipov, E. S. Gorbovskoy, N. L. Dzhioeva, C. Eyles, M.-H. A. Huang & 22 others A.F. Iyudin, V. V. Kalegaev, P. S. Kasarjan, J. E. Kim, V. G. Kornilov, E. A. Kuznetsova, H. Lim, V. M. Lipunov, T. -C. Liu, I. N. Myagkova, J. W. Nam, M. I. Panasyuk, M. I. Panchenko, V. L. Petrov, A. V. Prokhorov, V. Reglero, J. Ripa, J. M. Rodrigo, A. N. Shustova, S. I. Svertilov, N. V Tyurina, I. V. Yashin

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Abstract

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.
Original languageEnglish
Article number218
JournalP o S - Proceedings of Science
Number of pages8
ISSN1824-8039
Publication statusPublished - 2017
Event35th International Cosmic Ray Conference (ICRC2017) - Busan Exhibition & Convention Center, Busan, Korea, Republic of
Duration: 12 Jul 201720 Jul 2017

Conference

Conference35th International Cosmic Ray Conference (ICRC2017)
LocationBusan Exhibition & Convention Center
CountryKorea, Republic of
CityBusan
Period12/07/201720/07/2017

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

Kim, M. B., Jeong, S., Jeong, H. M., Leonov, V., Lee, J., Park, I. H., ... Yashin, I. V. (2017). Cosmic ray effect on the X-ray Trigger Telescope of UFFO/Lomonosov using YSO scintillation crystal array in space. P o S - Proceedings of Science, [218].
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. . / Cosmic ray effect on the X-ray Trigger Telescope of UFFO/Lomonosov using YSO scintillation crystal array in space. In: P o S - Proceedings of Science. 2017.
@inproceedings{db671af2b0c4402fa07031d0aa42e579,
title = "Cosmic ray effect on the X-ray Trigger Telescope of UFFO/Lomonosov using YSO scintillation crystal array in space",
abstract = "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.",
author = "Kim, {M. B.} and S. Jeong and Jeong, {H. M.} and V. Leonov and J Lee and I.H. Park and A.M. Amelushkin and Barinova, {V. O.} and A.V. Bogomolov and Bogomolov, {V. V.} and S{\o}ren Brandt and Carl Budtz-J{\o}rgensen and Castro-Tirado, {A. J.} and P. Chen and P. Connell and G. Garipov and Gorbovskoy, {E. S.} and Dzhioeva, {N. L.} and C. Eyles and Huang, {M.-H. A.} and A.F. Iyudin and Kalegaev, {V. V.} and Kasarjan, {P. S.} and Kim, {J. E.} and Kornilov, {V. G.} and Kuznetsova, {E. A.} and H. Lim and Lipunov, {V. M.} and Liu, {T. -C.} and Myagkova, {I. N.} and Nam, {J. W.} and Panasyuk, {M. I.} and Panchenko, {M. I.} and Petrov, {V. L.} and Prokhorov, {A. V.} and V. Reglero and J. Ripa and Rodrigo, {J. M.} and Shustova, {A. N.} and Svertilov, {S. I.} and Tyurina, {N. V} and Yashin, {I. V.}",
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)",
year = "2017",
language = "English",
journal = "P o S - Proceedings of Science",
issn = "1824-8039",
publisher = "SISSA",

}

Kim, MB, Jeong, S, Jeong, HM, Leonov, V, Lee, J, Park, IH, Amelushkin, AM, Barinova, VO, Bogomolov, AV, Bogomolov, VV, Brandt, S, Budtz-Jørgensen, C, Castro-Tirado, AJ, Chen, P, Connell, P, Garipov, G, Gorbovskoy, ES, Dzhioeva, NL, Eyles, C, Huang, M-HA, Iyudin, AF, Kalegaev, VV, Kasarjan, PS, Kim, JE, Kornilov, VG, Kuznetsova, EA, Lim, H, Lipunov, VM, Liu, T-C, Myagkova, IN, Nam, JW, Panasyuk, MI, Panchenko, MI, Petrov, VL, Prokhorov, AV, Reglero, V, Ripa, J, Rodrigo, JM, Shustova, AN, Svertilov, SI, Tyurina, NV & Yashin, IV 2017, 'Cosmic ray effect on the X-ray Trigger Telescope of UFFO/Lomonosov using YSO scintillation crystal array in space', P o S - Proceedings of Science.

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 journalConference articleResearchpeer-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 -