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; S. Brandt; C. 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

doi:10.22323/1.301.0218

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
, S. Brandt
, C. 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

^*Corresponding author for this work

Department of Electrophysics

Research output: Contribution to journal › Conference article › peer-review

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
Journal	Proceedings of Science
DOIs	https://doi.org/10.22323/1.301.0218
State	Published - 2017
Event	35th International Cosmic Ray Conference, ICRC 2017 - Bexco, Busan, Korea, Republic of Duration: 10 Jul 2017 → 20 Jul 2017

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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. Proceedings of Science. https://doi.org/10.22323/1.301.0218

@article{a455e7fec058404cafa28726d9ee10bf,

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 Park, \{I. H.\} and Amelushkin, \{A. M.\} and Barinova, \{V. O.\} and Bogomolov, \{A. V.\} and Bogomolov, \{V. V.\} and S. Brandt and C. 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 Iyudin, \{A. F.\} 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 = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons Attribution-Non Commercial-No Derivatives 4.0 International License (CC BY-NC-ND 4.0).; 35th International Cosmic Ray Conference, ICRC 2017 ; Conference date: 10-07-2017 Through 20-07-2017",

year = "2017",

doi = "10.22323/1.301.0218",

language = "English",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

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, MHA, Iyudin, AF, Kalegaev, VV, Kasarjan, PS, Kim, JE, Kornilov, VG, Kuznetsova, EA, Lim, H, Lipunov, VM, Liu, TC, 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', Proceedings of Science. https://doi.org/10.22323/1.301.0218

TY - JOUR

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, S.

AU - Budtz-Jørgensen, C.

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 - Publisher Copyright: © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-Non Commercial-No Derivatives 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.

UR - https://www.scopus.com/pages/publications/85046054078

U2 - 10.22323/1.301.0218

DO - 10.22323/1.301.0218

M3 - Conference article

AN - SCOPUS:85046054078

SN - 1824-8039

JO - Proceedings of Science

JF - Proceedings of Science

T2 - 35th International Cosmic Ray Conference, ICRC 2017

Y2 - 10 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

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