Implementation of the readout system in the UFFO Slewing Mirror Telescope

J. E. Kim; H. Lim; A. Jung; K. B. Ahn; H. S. Choi; Y. J. Choi; B. Grossan; I. Hermann; S. Jeong; S. W. Kim; Y. W. Kim; J. Lee; E. V. Linder; K. W. Min; G. W. Na; J. W. Nam; K. H. Nam; M. I. Panasyuk; I. H. Park; G. F. Smoot; Y. D. Suh; S. Svertilov; N. Vedenkin; I. Yashin; M. H. Zhao

doi:10.7529/ICRC2011/V09/1263

Implementation of the readout system in the UFFO Slewing Mirror Telescope

J. E. Kim, H. Lim, A. Jung, K. B. Ahn, H. S. Choi, Y. J. Choi, B. Grossan, I. Hermann, S. Jeong, S. W. Kim, Y. W. Kim, J. Lee, E. V. Linder, K. W. Min, G. W. Na, J. W. Nam, K. H. Nam, M. I. Panasyuk, I. H. Park, G. F. SmootY. D. Suh, S. Svertilov, N. Vedenkin, I. Yashin, M. H. Zhao

Institute of Earth·Atmosphere·Astronomy(BK21+)

Research output: Contribution to conference › Paper › peer-review

3 Citations (Scopus)

Abstract

The Ultra-Fast Flash Observatory (UFFO) is a new space-based experiment to observe Gamma-Ray Bursts (GRBs). GRBs are the most luminous electromagnetic events in the universe and occur randomly in any direction. Therefore the UFFO consists of two telescopes; UFFO Burst Alert & Trigger Telescope (UBAT) to detect GRBs using a wide field-of-view (FOV), and a Slewing Mirror Telescope (SMT) to observe UV/optical events rapidly within the narrow, targeted FOV. The SMT is a Ritchey-Chretien telescope that uses a motorized mirror system and an Intensified Charge-Coupled Device (ICCD). When the GRB is triggered by the UBAT, the SMT receives the position information and rapidly tilts the mirror to the target. The ICCD start to take the data within a second after GRB is triggered. Here we give the details about the SMT readout electronics that deliver the data.

Original language	English
Pages	239-242
Number of pages	4
DOIs	https://doi.org/10.7529/ICRC2011/V09/1263
Publication status	Published - 2011
Event	32nd International Cosmic Ray Conference, ICRC 2011 - Beijing, China Duration: 2011 Aug 11 → 2011 Aug 18

Other

Other	32nd International Cosmic Ray Conference, ICRC 2011
Country/Territory	China
City	Beijing
Period	11/8/11 → 11/8/18

All Science Journal Classification (ASJC) codes

Nuclear and High Energy Physics

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10.7529/ICRC2011/V09/1263

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Kim, J. E., Lim, H., Jung, A., Ahn, K. B., Choi, H. S., Choi, Y. J., Grossan, B., Hermann, I., Jeong, S., Kim, S. W., Kim, Y. W., Lee, J., Linder, E. V., Min, K. W., Na, G. W., Nam, J. W., Nam, K. H., Panasyuk, M. I., Park, I. H., ... Zhao, M. H. (2011). Implementation of the readout system in the UFFO Slewing Mirror Telescope. 239-242. Paper presented at 32nd International Cosmic Ray Conference, ICRC 2011, Beijing, China. https://doi.org/10.7529/ICRC2011/V09/1263

@conference{61b0fbec350d4e3cb0fe381ef5f48b6d,

title = "Implementation of the readout system in the UFFO Slewing Mirror Telescope",

abstract = "The Ultra-Fast Flash Observatory (UFFO) is a new space-based experiment to observe Gamma-Ray Bursts (GRBs). GRBs are the most luminous electromagnetic events in the universe and occur randomly in any direction. Therefore the UFFO consists of two telescopes; UFFO Burst Alert & Trigger Telescope (UBAT) to detect GRBs using a wide field-of-view (FOV), and a Slewing Mirror Telescope (SMT) to observe UV/optical events rapidly within the narrow, targeted FOV. The SMT is a Ritchey-Chretien telescope that uses a motorized mirror system and an Intensified Charge-Coupled Device (ICCD). When the GRB is triggered by the UBAT, the SMT receives the position information and rapidly tilts the mirror to the target. The ICCD start to take the data within a second after GRB is triggered. Here we give the details about the SMT readout electronics that deliver the data.",

author = "Kim, {J. E.} and H. Lim and A. Jung and Ahn, {K. B.} and Choi, {H. S.} and Choi, {Y. J.} and B. Grossan and I. Hermann and S. Jeong and Kim, {S. W.} and Kim, {Y. W.} and J. Lee and Linder, {E. V.} and Min, {K. W.} and Na, {G. W.} and Nam, {J. W.} and Nam, {K. H.} and Panasyuk, {M. I.} and Park, {I. H.} and Smoot, {G. F.} and Suh, {Y. D.} and S. Svertilov and N. Vedenkin and I. Yashin and Zhao, {M. H.}",

year = "2011",

doi = "10.7529/ICRC2011/V09/1263",

language = "English",

pages = "239--242",

note = "32nd International Cosmic Ray Conference, ICRC 2011 ; Conference date: 11-08-2011 Through 18-08-2011",

}

Kim, JE, Lim, H, Jung, A, Ahn, KB, Choi, HS, Choi, YJ, Grossan, B, Hermann, I, Jeong, S, Kim, SW, Kim, YW, Lee, J, Linder, EV, Min, KW, Na, GW, Nam, JW, Nam, KH, Panasyuk, MI, Park, IH, Smoot, GF, Suh, YD, Svertilov, S, Vedenkin, N, Yashin, I & Zhao, MH 2011, 'Implementation of the readout system in the UFFO Slewing Mirror Telescope', Paper presented at 32nd International Cosmic Ray Conference, ICRC 2011, Beijing, China, 11/8/11 - 11/8/18 pp. 239-242. https://doi.org/10.7529/ICRC2011/V09/1263

TY - CONF

T1 - Implementation of the readout system in the UFFO Slewing Mirror Telescope

AU - Kim, J. E.

AU - Lim, H.

AU - Jung, A.

AU - Ahn, K. B.

AU - Choi, H. S.

AU - Choi, Y. J.

AU - Grossan, B.

AU - Hermann, I.

AU - Jeong, S.

AU - Kim, S. W.

AU - Kim, Y. W.

AU - Lee, J.

AU - Linder, E. V.

AU - Min, K. W.

AU - Na, G. W.

AU - Nam, J. W.

AU - Nam, K. H.

AU - Panasyuk, M. I.

AU - Park, I. H.

AU - Smoot, G. F.

AU - Suh, Y. D.

AU - Svertilov, S.

AU - Vedenkin, N.

AU - Yashin, I.

AU - Zhao, M. H.

PY - 2011

Y1 - 2011

N2 - The Ultra-Fast Flash Observatory (UFFO) is a new space-based experiment to observe Gamma-Ray Bursts (GRBs). GRBs are the most luminous electromagnetic events in the universe and occur randomly in any direction. Therefore the UFFO consists of two telescopes; UFFO Burst Alert & Trigger Telescope (UBAT) to detect GRBs using a wide field-of-view (FOV), and a Slewing Mirror Telescope (SMT) to observe UV/optical events rapidly within the narrow, targeted FOV. The SMT is a Ritchey-Chretien telescope that uses a motorized mirror system and an Intensified Charge-Coupled Device (ICCD). When the GRB is triggered by the UBAT, the SMT receives the position information and rapidly tilts the mirror to the target. The ICCD start to take the data within a second after GRB is triggered. Here we give the details about the SMT readout electronics that deliver the data.

AB - The Ultra-Fast Flash Observatory (UFFO) is a new space-based experiment to observe Gamma-Ray Bursts (GRBs). GRBs are the most luminous electromagnetic events in the universe and occur randomly in any direction. Therefore the UFFO consists of two telescopes; UFFO Burst Alert & Trigger Telescope (UBAT) to detect GRBs using a wide field-of-view (FOV), and a Slewing Mirror Telescope (SMT) to observe UV/optical events rapidly within the narrow, targeted FOV. The SMT is a Ritchey-Chretien telescope that uses a motorized mirror system and an Intensified Charge-Coupled Device (ICCD). When the GRB is triggered by the UBAT, the SMT receives the position information and rapidly tilts the mirror to the target. The ICCD start to take the data within a second after GRB is triggered. Here we give the details about the SMT readout electronics that deliver the data.

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UR - http://www.scopus.com/inward/citedby.url?scp=84899552322&partnerID=8YFLogxK

U2 - 10.7529/ICRC2011/V09/1263

DO - 10.7529/ICRC2011/V09/1263

M3 - Paper

AN - SCOPUS:84899552322

SP - 239

EP - 242

T2 - 32nd International Cosmic Ray Conference, ICRC 2011

Y2 - 11 August 2011 through 18 August 2011

ER -

Implementation of the readout system in the UFFO Slewing Mirror Telescope

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