Ultra-fast flash observatory for observation of early photons from gamma ray bursts

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

doi:10.1117/12.926104

Ultra-fast flash observatory for observation of early photons from gamma ray bursts

I. H. Park^*, S. Ahmad, P. Barrillon, S. Brandt, C. Budtz-Jorgensen, A. J. Castro-Tirado, P. Chen, Y. J. Choi, P. Connell, S. Dagoret-Campagne, C. Eyles, B. Grossan, M. H.A. Huang, S. Jeong, A. Jung, J. E. Kim, M. B. Kima, S. W. Kim, Y. W. Kim, A. S. KrasnovJ. Lee, H. Lim, E. V. Linder, T. C. Liu, N. Lund, K. W. Min, G. W. Na, J. W. Nam, M. I. Panasyuk, J. Ripa, V. Reglero, 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: Conference contribution › 同行評審

4 引文斯高帕斯（Scopus）

摘要

We describe the space project of Ultra-Fast Flash Observatory (UFFO) which will observe early optical photons from gamma-ray bursts (GRBs) with a sub-second optical response, for the first time. The UFFO will probe the early optical rise of GRBs, opening a completely new frontier in GRB and transient studies, using a fast response Slewing Mirror Telescope (SMT) that redirects optical path to telescope instead of slewing of telescopes or spacecraft. In our small UFFO-Pathfinder experiment, scheduled to launch aboard the Lomonosov satellite in 2012, we use a motorized mirror in our Slewing Mirror Telescope instrument to achieve less than one second optical response after X-ray trigger. We describe the science and the mission of the UFFO project, including a next version called UFFO-100. With our program of ultra-fast optical response GRB observatories, we aim to gain a deeper understanding of GRB mechanisms, and potentially open up the z>10 universe to study via GRB as point source emission probes.

原文	English
主出版物標題	Space Telescopes and Instrumentation 2012
主出版物子標題	Ultraviolet to Gamma Ray
DOIs	https://doi.org/10.1117/12.926104
出版狀態	Published - 2012
事件	Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray - Amsterdam, 荷蘭持續時間: 1 7月 2012 → 6 7月 2012

出版系列

名字	Proceedings of SPIE - The International Society for Optical Engineering
卷	8443
ISSN（列印）	0277-786X

Conference

Conference	Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray
國家/地區	荷蘭
城市	Amsterdam
期間	1/07/12 → 6/07/12

存取文件

10.1117/12.926104

其它文件與鏈接

Link to publication in Scopus

引用此

Park, I. H., Ahmad, S., Barrillon, P., Brandt, S., Budtz-Jorgensen, C., Castro-Tirado, A. J., Chen, P., Choi, Y. J., Connell, P., Dagoret-Campagne, S., Eyles, C., Grossan, B., Huang, M. H. A., Jeong, S., Jung, A., Kim, J. E., Kima, M. B., Kim, S. W., Kim, Y. W., ... Yashin, I. (2012). Ultra-fast flash observatory for observation of early photons from gamma ray bursts. 於 Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray 文章 84430I (Proceedings of SPIE - The International Society for Optical Engineering; 卷 8443). https://doi.org/10.1117/12.926104

@inproceedings{a1bb96c2fc5c4a48a565f406482205fe,

title = "Ultra-fast flash observatory for observation of early photons from gamma ray bursts",

abstract = "We describe the space project of Ultra-Fast Flash Observatory (UFFO) which will observe early optical photons from gamma-ray bursts (GRBs) with a sub-second optical response, for the first time. The UFFO will probe the early optical rise of GRBs, opening a completely new frontier in GRB and transient studies, using a fast response Slewing Mirror Telescope (SMT) that redirects optical path to telescope instead of slewing of telescopes or spacecraft. In our small UFFO-Pathfinder experiment, scheduled to launch aboard the Lomonosov satellite in 2012, we use a motorized mirror in our Slewing Mirror Telescope instrument to achieve less than one second optical response after X-ray trigger. We describe the science and the mission of the UFFO project, including a next version called UFFO-100. With our program of ultra-fast optical response GRB observatories, we aim to gain a deeper understanding of GRB mechanisms, and potentially open up the z>10 universe to study via GRB as point source emission probes.",

keywords = "Gamma Ray Bursts, Lomonosov spacecraft, Optical Light Curve, Slewing Mirror Telescope, UV/Optical afterglows, Ultra-Fast Flash Observatory",

author = "Park, {I. H.} and S. Ahmad and P. Barrillon and S. Brandt and C. Budtz-Jorgensen and Castro-Tirado, {A. J.} and P. Chen and Choi, {Y. J.} and P. Connell and S. Dagoret-Campagne and C. Eyles and B. Grossan and Huang, {M. H.A.} and S. Jeong and A. Jung and Kim, {J. E.} and Kima, {M. B.} and Kim, {S. W.} and Kim, {Y. W.} and Krasnov, {A. S.} and J. Lee and H. Lim and Linder, {E. V.} and Liu, {T. C.} and N. Lund and Min, {K. W.} and Na, {G. W.} and Nam, {J. W.} and Panasyuk, {M. I.} and J. Ripa and V. Reglero 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 = "2012",

doi = "10.1117/12.926104",

language = "English",

isbn = "9780819491442",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

booktitle = "Space Telescopes and Instrumentation 2012",

note = "Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray ; Conference date: 01-07-2012 Through 06-07-2012",

}

Park, IH, Ahmad, S, Barrillon, P, Brandt, S, Budtz-Jorgensen, C, Castro-Tirado, AJ, Chen, P, Choi, YJ, Connell, P, Dagoret-Campagne, S, Eyles, C, Grossan, B, Huang, MHA, Jeong, S, Jung, A, Kim, JE, Kima, MB, Kim, SW, Kim, YW, Krasnov, AS, Lee, J, Lim, H, Linder, EV, Liu, TC, Lund, N, Min, KW, Na, GW, Nam, JW, Panasyuk, MI, Ripa, J, Reglero, V, Rodrigo, JM, Smoot, GF, Suh, JE, Svertilov, S, Vedenkin, N, Wang, MZ & Yashin, I 2012, Ultra-fast flash observatory for observation of early photons from gamma ray bursts. 於 Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray., 84430I, Proceedings of SPIE - The International Society for Optical Engineering, 卷 8443, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray, Amsterdam, 荷蘭, 1/07/12. https://doi.org/10.1117/12.926104

TY - GEN

T1 - Ultra-fast flash observatory for observation of early photons from gamma ray bursts

AU - Park, I. H.

AU - Ahmad, S.

AU - Barrillon, P.

AU - Brandt, S.

AU - Budtz-Jorgensen, C.

AU - Castro-Tirado, A. J.

AU - Chen, P.

AU - Choi, Y. J.

AU - Connell, P.

AU - Dagoret-Campagne, S.

AU - Eyles, C.

AU - Grossan, B.

AU - Huang, M. H.A.

AU - Jeong, S.

AU - Jung, A.

AU - Kim, J. E.

AU - Kima, M. B.

AU - Kim, S. W.

AU - Kim, Y. W.

AU - Krasnov, A. S.

AU - Lee, J.

AU - Lim, H.

AU - Linder, E. V.

AU - Liu, T. C.

AU - Lund, N.

AU - Min, K. W.

AU - Na, G. W.

AU - Nam, J. W.

AU - Panasyuk, M. I.

AU - Ripa, J.

AU - Reglero, V.

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 - 2012

Y1 - 2012

N2 - We describe the space project of Ultra-Fast Flash Observatory (UFFO) which will observe early optical photons from gamma-ray bursts (GRBs) with a sub-second optical response, for the first time. The UFFO will probe the early optical rise of GRBs, opening a completely new frontier in GRB and transient studies, using a fast response Slewing Mirror Telescope (SMT) that redirects optical path to telescope instead of slewing of telescopes or spacecraft. In our small UFFO-Pathfinder experiment, scheduled to launch aboard the Lomonosov satellite in 2012, we use a motorized mirror in our Slewing Mirror Telescope instrument to achieve less than one second optical response after X-ray trigger. We describe the science and the mission of the UFFO project, including a next version called UFFO-100. With our program of ultra-fast optical response GRB observatories, we aim to gain a deeper understanding of GRB mechanisms, and potentially open up the z>10 universe to study via GRB as point source emission probes.

AB - We describe the space project of Ultra-Fast Flash Observatory (UFFO) which will observe early optical photons from gamma-ray bursts (GRBs) with a sub-second optical response, for the first time. The UFFO will probe the early optical rise of GRBs, opening a completely new frontier in GRB and transient studies, using a fast response Slewing Mirror Telescope (SMT) that redirects optical path to telescope instead of slewing of telescopes or spacecraft. In our small UFFO-Pathfinder experiment, scheduled to launch aboard the Lomonosov satellite in 2012, we use a motorized mirror in our Slewing Mirror Telescope instrument to achieve less than one second optical response after X-ray trigger. We describe the science and the mission of the UFFO project, including a next version called UFFO-100. With our program of ultra-fast optical response GRB observatories, we aim to gain a deeper understanding of GRB mechanisms, and potentially open up the z>10 universe to study via GRB as point source emission probes.

KW - Gamma Ray Bursts

KW - Lomonosov spacecraft

KW - Optical Light Curve

KW - Slewing Mirror Telescope

KW - UV/Optical afterglows

KW - Ultra-Fast Flash Observatory

UR - http://www.scopus.com/inward/record.url?scp=84871765531&partnerID=8YFLogxK

U2 - 10.1117/12.926104

DO - 10.1117/12.926104

M3 - Conference contribution

AN - SCOPUS:84871765531

SN - 9780819491442

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Space Telescopes and Instrumentation 2012

T2 - Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray

Y2 - 1 July 2012 through 6 July 2012

ER -

Ultra-fast flash observatory for observation of early photons from gamma ray bursts

摘要

出版系列

Conference

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其它文件與鏈接

指紋

引用此