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; 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

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. HuangA.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 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/Territory	Korea, Republic of
City	Busan
Period	12/07/2017 → 20/07/2017

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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)

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UFFO: Ultra-Fast Flash Observatory, UFFO
Brandt, S. (Project Participant), Budtz-Jørgensen, C. (Project Participant) & Lund, N. (Project Participant)
01/01/2010 → …
Project: Research

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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, S., Budtz-Jørgensen, C., Castro-Tirado, A. J., Chen, P., Connell, P., Garipov, G., Gorbovskoy, E. S., Dzhioeva, N. L., Eyles, C., ... 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, Article 218.

@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); 35th International Cosmic Ray Conference (ICRC2017) ; Conference date: 12-07-2017 Through 20-07-2017",

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.

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

SN - 1824-8039

JO - P o S - Proceedings of Science

JF - P o S - Proceedings of Science

M1 - 218

T2 - 35th International Cosmic Ray Conference (ICRC2017)

Y2 - 12 July 2017 through 20 July 2017

ER -

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

Abstract

Conference

Bibliographical note

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Projects

UFFO: Ultra-Fast Flash Observatory, UFFO

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