Comparison cosmic ray irradiation simulation and particle beam test on UFFO Burst Alert & Trigger telescope(UBAT) detectors

H. M. Jeong; S. Jeong; M. B. Kim; 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; N. L. Dzhioeva; C. Eyles; G. Garipov; E. S. Gorbovskoy; 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

Comparison cosmic ray irradiation simulation and particle beam test on UFFO Burst Alert & Trigger telescope(UBAT) detectors

H. M. Jeong, S. Jeong, M. B. Kim, 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, N. L. Dzhioeva, C. Eyles, G. Garipov, E. S. Gorbovskoy, M. H. A. Huang, A. F. IyudinV. 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

Ultra-Fast Flash Observatory pathfinder(UFFO-p) was launched onboard Lomonosov on 28th of April, 2016, and now is under various types of calibration for detection of Gamma Ray Bursts (GRBs). Since last September UFFO-p has taken X-ray data in space with UFFO Burst Alert &Trigger telescope (UBAT), those X-rays are mostly diffused backgrounds however, the rate turns out to be higher than expected by a factor of three. We assumed cosmic rays can contribute by making the count rate higher. We did such a simulation to investigate the effect of cosmic rays. In December 2016, we irradiated fragmented high energy heavy ions at CERN on the UBAT detector. We will report the result of comparison between simulation and beam test.

Original language	English
Article number	219
Journal	P o S - Proceedings of Science
Number of pages	6
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

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).

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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

Cite this

Jeong, H. M., Jeong, S., Kim, M. B., 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., Dzhioeva, N. L., Eyles, C., Garipov, G., Gorbovskoy, E. S., Huang, M. H. A., ... Yashin, I. V. (2017). Comparison cosmic ray irradiation simulation and particle beam test on UFFO Burst Alert & Trigger telescope(UBAT) detectors. P o S - Proceedings of Science, Article 219.

@inproceedings{cfbc0443f0c84099a232891dfadb1e63,

title = "Comparison cosmic ray irradiation simulation and particle beam test on UFFO Burst Alert & Trigger telescope(UBAT) detectors",

abstract = "Ultra-Fast Flash Observatory pathfinder(UFFO-p) was launched onboard Lomonosov on 28th of April, 2016, and now is under various types of calibration for detection of Gamma Ray Bursts (GRBs). Since last September UFFO-p has taken X-ray data in space with UFFO Burst Alert &Trigger telescope (UBAT), those X-rays are mostly diffused backgrounds however, the rate turns out to be higher than expected by a factor of three. We assumed cosmic rays can contribute by making the count rate higher. We did such a simulation to investigate the effect of cosmic rays. In December 2016, we irradiated fragmented high energy heavy ions at CERN on the UBAT detector. We will report the result of comparison between simulation and beam test.",

author = "Jeong, {H. M.} and S. Jeong and Kim, {M. B.} 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{\o}ren Brandt and Carl Budtz-J{\o}rgensen and Castro-Tirado, {A. J.} and P. Chen and P. Connell and Dzhioeva, {N. L.} and C. Eyles and G. Garipov and Gorbovskoy, {E. S.} 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 = "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",

}

Jeong, HM, Jeong, S, Kim, MB, Lee, J, Park, IH, Amelushkin, AM, Barinova, VO, Bogomolov, AV, Bogomolov, VV, Brandt, S , Budtz-Jørgensen, C, Castro-Tirado, AJ, Chen, P, Connell, P, Dzhioeva, NL, Eyles, C, Garipov, G, Gorbovskoy, ES, 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, 'Comparison cosmic ray irradiation simulation and particle beam test on UFFO Burst Alert & Trigger telescope(UBAT) detectors', P o S - Proceedings of Science.

TY - GEN

T1 - Comparison cosmic ray irradiation simulation and particle beam test on UFFO Burst Alert & Trigger telescope(UBAT) detectors

AU - Jeong, H. M.

AU - Jeong, S.

AU - Kim, M. B.

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 - Dzhioeva, N. L.

AU - Eyles, C.

AU - Garipov, G.

AU - Gorbovskoy, E. S.

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 - Ultra-Fast Flash Observatory pathfinder(UFFO-p) was launched onboard Lomonosov on 28th of April, 2016, and now is under various types of calibration for detection of Gamma Ray Bursts (GRBs). Since last September UFFO-p has taken X-ray data in space with UFFO Burst Alert &Trigger telescope (UBAT), those X-rays are mostly diffused backgrounds however, the rate turns out to be higher than expected by a factor of three. We assumed cosmic rays can contribute by making the count rate higher. We did such a simulation to investigate the effect of cosmic rays. In December 2016, we irradiated fragmented high energy heavy ions at CERN on the UBAT detector. We will report the result of comparison between simulation and beam test.

AB - Ultra-Fast Flash Observatory pathfinder(UFFO-p) was launched onboard Lomonosov on 28th of April, 2016, and now is under various types of calibration for detection of Gamma Ray Bursts (GRBs). Since last September UFFO-p has taken X-ray data in space with UFFO Burst Alert &Trigger telescope (UBAT), those X-rays are mostly diffused backgrounds however, the rate turns out to be higher than expected by a factor of three. We assumed cosmic rays can contribute by making the count rate higher. We did such a simulation to investigate the effect of cosmic rays. In December 2016, we irradiated fragmented high energy heavy ions at CERN on the UBAT detector. We will report the result of comparison between simulation and beam test.

M3 - Conference article

SN - 1824-8039

JO - P o S - Proceedings of Science

JF - P o S - Proceedings of Science

M1 - 219

T2 - 35th International Cosmic Ray Conference (ICRC2017)

Y2 - 12 July 2017 through 20 July 2017

ER -

Comparison cosmic ray irradiation simulation and particle beam test on UFFO Burst Alert & Trigger telescope(UBAT) detectors

Abstract

Conference

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Projects

UFFO: Ultra-Fast Flash Observatory, UFFO

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