Design and implementation of electronics and data acquisition system for Ultra-Fast Flash Observatory

A. Jung; S. Ahmad; P. Barrillon; S. Brandt; C. Budtz-Jørgensen; A. J. Castro-Tirado; S. H. Chang; Y. Y. Chang; C. R. Chen; P. Chen; H. S. Choi; Y. J. Choi; P. Connell; S. Dagoret-Campagne; C. Eyles; B. Grossan; J. J. Huang; M. H.A. Huang; S. Jeong; J. E. Kim; M. Kim; S. W. Kim; Y. W. Kim; A. S. Krasnov; J. Lee; H. Lim; C. Y. Lin; E. V. Linder; T. C. Liu; N. Lund; J. W. Nam; K. W. Min; G. W. Na; M. I. Panasyuk; I. H. Park; V. Reglero; J. Ripa; J. M. Rodrigo; G. F. Smoot; J. E. Suh; S. Svertilov; N. Vedenkin; M. Z. Wang; I. Yashin

doi:10.1051/eas/1361091

Design and implementation of electronics and data acquisition system for Ultra-Fast Flash Observatory

A. Jung^*, S. Ahmad, P. Barrillon, S. Brandt, C. Budtz-Jørgensen, A. J. Castro-Tirado, S. H. Chang, Y. Y. Chang, C. R. Chen, P. Chen, H. S. Choi, Y. J. Choi, P. Connell, S. Dagoret-Campagne, C. Eyles, B. Grossan, J. J. Huang, M. H.A. Huang, S. Jeong, J. E. KimM. Kim, S. W. Kim, Y. W. Kim, A. S. Krasnov, J. Lee, H. Lim, C. Y. Lin, E. V. Linder, T. C. Liu, N. Lund, J. W. Nam, K. W. Min, G. W. Na, M. I. Panasyuk, I. H. Park, V. Reglero, J. Ripa, J. M. Rodrigo, G. F. Smoot, J. E. Suh, S. Svertilov, N. Vedenkin, M. Z. Wang, I. Yashin

^*此作品的通信作者

電子物理學系

研究成果 › 同行評審

摘要

The Ultra-Fast Flash Observatory (UFFO) Pathfinder for Gamma-Ray Bursts (GRBs) consists of two telescopes. The UFFO Burst Alert & Trigger Telescope (UBAT) handles the detection and localization of GRBs, and the Slewing Mirror Telescope (SMT) conducts the measurement of the UV/optical afterglow. UBAT is equipped with an X-ray detector, analog and digital signal readout electronics that detects X-rays from GRBs and determines the location. SMT is equipped with a stepping motor and the associated electronics to rotate the slewing mirror targeting the GRBs identified by UBAT. First the slewing mirror points to a GRB, then SMT obtains the optical image of the GRB using the intensified CCD and its readout electronics. The UFFO Data Acquisition system (UDAQ) is responsible for the overall function and operation of the observatory and the communication with the satellite main processor. In this paper we present the design and implementation of the electronics of UBAT and SMT as well as the architecture and implementation of UDAQ.

原文	English
頁（從 - 到）	567-571
頁數	5
期刊	EAS Publications Series
卷	61
DOIs	https://doi.org/10.1051/eas/1361091
出版狀態	Published - 2013
事件	2012 Gamma-Ray Burst Symposium, GRB 2012 - Malaga, 西班牙持續時間: 8 10月 2012 → 12 10月 2012

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10.1051/eas/1361091

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Jung, A., Ahmad, S., Barrillon, P., Brandt, S., Budtz-Jørgensen, C., Castro-Tirado, A. J., Chang, S. H., Chang, Y. Y., Chen, C. R., Chen, P., Choi, H. S., Choi, Y. J., Connell, P., Dagoret-Campagne, S., Eyles, C., Grossan, B., Huang, J. J., Huang, M. H. A., Jeong, S., ... Yashin, I. (2013). Design and implementation of electronics and data acquisition system for Ultra-Fast Flash Observatory. EAS Publications Series, 61, 567-571. https://doi.org/10.1051/eas/1361091

@article{025db0b4131e463ea786f8f2b9de5d2d,

title = "Design and implementation of electronics and data acquisition system for Ultra-Fast Flash Observatory",

abstract = "The Ultra-Fast Flash Observatory (UFFO) Pathfinder for Gamma-Ray Bursts (GRBs) consists of two telescopes. The UFFO Burst Alert & Trigger Telescope (UBAT) handles the detection and localization of GRBs, and the Slewing Mirror Telescope (SMT) conducts the measurement of the UV/optical afterglow. UBAT is equipped with an X-ray detector, analog and digital signal readout electronics that detects X-rays from GRBs and determines the location. SMT is equipped with a stepping motor and the associated electronics to rotate the slewing mirror targeting the GRBs identified by UBAT. First the slewing mirror points to a GRB, then SMT obtains the optical image of the GRB using the intensified CCD and its readout electronics. The UFFO Data Acquisition system (UDAQ) is responsible for the overall function and operation of the observatory and the communication with the satellite main processor. In this paper we present the design and implementation of the electronics of UBAT and SMT as well as the architecture and implementation of UDAQ.",

author = "A. Jung and S. Ahmad and P. Barrillon and S. Brandt and C. Budtz-J{\o}rgensen and Castro-Tirado, {A. J.} and Chang, {S. H.} and Chang, {Y. Y.} and Chen, {C. R.} and P. Chen and Choi, {H. S.} and Choi, {Y. J.} and P. Connell and S. Dagoret-Campagne and C. Eyles and B. Grossan and Huang, {J. J.} and Huang, {M. H.A.} and S. Jeong and Kim, {J. E.} and M. Kim and Kim, {S. W.} and Kim, {Y. W.} and Krasnov, {A. S.} and J. Lee and H. Lim and Lin, {C. Y.} and Linder, {E. V.} and Liu, {T. C.} and N. Lund and Nam, {J. W.} and Min, {K. W.} and Na, {G. W.} and Panasyuk, {M. I.} and Park, {I. H.} and V. Reglero and J. Ripa and Rodrigo, {J. M.} and Smoot, {G. F.} and Suh, {J. E.} and S. Svertilov and N. Vedenkin and Wang, {M. Z.} and I. Yashin",

year = "2013",

doi = "10.1051/eas/1361091",

language = "English",

volume = "61",

pages = "567--571",

journal = "EAS Publications Series",

issn = "1633-4760",

publisher = "EDP Sciences",

note = "2012 Gamma-Ray Burst Symposium, GRB 2012 ; Conference date: 08-10-2012 Through 12-10-2012",

}

Jung, A, Ahmad, S, Barrillon, P, Brandt, S, Budtz-Jørgensen, C, Castro-Tirado, AJ, Chang, SH, Chang, YY, Chen, CR, Chen, P, Choi, HS, Choi, YJ, Connell, P, Dagoret-Campagne, S, Eyles, C, Grossan, B, Huang, JJ, Huang, MHA, Jeong, S, Kim, JE, Kim, M, Kim, SW, Kim, YW, Krasnov, AS, Lee, J, Lim, H, Lin, CY, Linder, EV, Liu, TC, Lund, N, Nam, JW, Min, KW, Na, GW, Panasyuk, MI, Park, IH, Reglero, V, Ripa, J, Rodrigo, JM, Smoot, GF, Suh, JE, Svertilov, S, Vedenkin, N, Wang, MZ & Yashin, I 2013, 'Design and implementation of electronics and data acquisition system for Ultra-Fast Flash Observatory', EAS Publications Series, 卷 61, 頁 567-571. https://doi.org/10.1051/eas/1361091

TY - JOUR

T1 - Design and implementation of electronics and data acquisition system for Ultra-Fast Flash Observatory

AU - Jung, A.

AU - Ahmad, S.

AU - Barrillon, P.

AU - Brandt, S.

AU - Budtz-Jørgensen, C.

AU - Castro-Tirado, A. J.

AU - Chang, S. H.

AU - Chang, Y. Y.

AU - Chen, C. R.

AU - Chen, P.

AU - Choi, H. S.

AU - Choi, Y. J.

AU - Connell, P.

AU - Dagoret-Campagne, S.

AU - Eyles, C.

AU - Grossan, B.

AU - Huang, J. J.

AU - Huang, M. H.A.

AU - Jeong, S.

AU - Kim, J. E.

AU - Kim, M.

AU - Kim, S. W.

AU - Kim, Y. W.

AU - Krasnov, A. S.

AU - Lee, J.

AU - Lim, H.

AU - Lin, C. Y.

AU - Linder, E. V.

AU - Liu, T. C.

AU - Lund, N.

AU - Nam, J. W.

AU - Min, K. W.

AU - Na, G. W.

AU - Panasyuk, M. I.

AU - Park, I. H.

AU - Reglero, V.

AU - Ripa, J.

AU - Rodrigo, J. M.

AU - Smoot, G. F.

AU - Suh, J. E.

AU - Svertilov, S.

AU - Vedenkin, N.

AU - Wang, M. Z.

AU - Yashin, I.

PY - 2013

Y1 - 2013

N2 - The Ultra-Fast Flash Observatory (UFFO) Pathfinder for Gamma-Ray Bursts (GRBs) consists of two telescopes. The UFFO Burst Alert & Trigger Telescope (UBAT) handles the detection and localization of GRBs, and the Slewing Mirror Telescope (SMT) conducts the measurement of the UV/optical afterglow. UBAT is equipped with an X-ray detector, analog and digital signal readout electronics that detects X-rays from GRBs and determines the location. SMT is equipped with a stepping motor and the associated electronics to rotate the slewing mirror targeting the GRBs identified by UBAT. First the slewing mirror points to a GRB, then SMT obtains the optical image of the GRB using the intensified CCD and its readout electronics. The UFFO Data Acquisition system (UDAQ) is responsible for the overall function and operation of the observatory and the communication with the satellite main processor. In this paper we present the design and implementation of the electronics of UBAT and SMT as well as the architecture and implementation of UDAQ.

AB - The Ultra-Fast Flash Observatory (UFFO) Pathfinder for Gamma-Ray Bursts (GRBs) consists of two telescopes. The UFFO Burst Alert & Trigger Telescope (UBAT) handles the detection and localization of GRBs, and the Slewing Mirror Telescope (SMT) conducts the measurement of the UV/optical afterglow. UBAT is equipped with an X-ray detector, analog and digital signal readout electronics that detects X-rays from GRBs and determines the location. SMT is equipped with a stepping motor and the associated electronics to rotate the slewing mirror targeting the GRBs identified by UBAT. First the slewing mirror points to a GRB, then SMT obtains the optical image of the GRB using the intensified CCD and its readout electronics. The UFFO Data Acquisition system (UDAQ) is responsible for the overall function and operation of the observatory and the communication with the satellite main processor. In this paper we present the design and implementation of the electronics of UBAT and SMT as well as the architecture and implementation of UDAQ.

UR - http://www.scopus.com/inward/record.url?scp=84887108215&partnerID=8YFLogxK

U2 - 10.1051/eas/1361091

DO - 10.1051/eas/1361091

M3 - Conference article

AN - SCOPUS:84887108215

SN - 1633-4760

VL - 61

SP - 567

EP - 571

JO - EAS Publications Series

JF - EAS Publications Series

T2 - 2012 Gamma-Ray Burst Symposium, GRB 2012

Y2 - 8 October 2012 through 12 October 2012

ER -

Design and implementation of electronics and data acquisition system for Ultra-Fast Flash Observatory

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