The status of the ultra fast flash observatory - pathfinder

J. W. Nam; S. Ahmad; K. B. Ahn; P. Barrillon; S. Brandt; C. Budtz-Jrgensen; A. J. Castro-Tirado; C. H. Chang; C. Y. Chang; Y. Y. Chang; C. R. Chen; P. Chen; M. Cho; H. S. Choi; Y. J. Choi; P. Connel; S. Dagoret-Campagne; C. Eyles; B. Grossan; J. J. Huang; M. H.A. Huang; S. Jeong; A. Jung; J. E. Kim; M. B. Kim; 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; 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:10.1016/j.nuclphysbps.2013.10.061

The status of the ultra fast flash observatory - pathfinder

J. W. Nam, S. Ahmad, K. B. Ahn, P. Barrillon, S. Brandt, C. Budtz-Jrgensen, A. J. Castro-Tirado, C. H. Chang, C. Y. Chang, Y. Y. Chang, C. R. Chen, P. Chen, M. Cho, H. S. Choi, Y. J. Choi, P. Connel, S. Dagoret-Campagne, C. Eyles, B. Grossan, J. J. HuangM. H.A. Huang, S. Jeong, A. Jung, J. E. Kim, M. B. Kim, 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, 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

Department of Astronomy

Research output: Contribution to journal › Article

2 Citations (Scopus)

Abstract

The Ultra Fast Flash Observatory (UFFO) is a project to study early optical emissions from Gamma Ray Bursts (GRBs). The primary scientific goal of UFFO is to see if GRBs can be calibrated with their rising times, so that they could be used as new standard candles. In order to minimize delay in optical follow-up measurements, which is now about 100 sec after trigger from the Swift experiment, we rotate a mirror to redirect light path so that optical measurement can be performed within a second after the trigger. We have developed a pathfinder mission, UFFO-pathfinder to launch on board the Lomonosov satellite in 2012. In this talk, I will present scientific motivations and descriptions of the design and development of UFFO-pathfinder.

Original language	English
Pages (from-to)	29-33
Number of pages	5
Journal	Nuclear Physics B - Proceedings Supplements
Volume	246-247
DOIs	https://doi.org/10.1016/j.nuclphysbps.2013.10.061
Publication status	Published - 2014 Jan 1

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All Science Journal Classification (ASJC) codes

Atomic and Molecular Physics, and Optics
Nuclear and High Energy Physics

Cite this

Nam, J. W., Ahmad, S., Ahn, K. B., Barrillon, P., Brandt, S., Budtz-Jrgensen, C., Castro-Tirado, A. J., Chang, C. H., Chang, C. Y., Chang, Y. Y., Chen, C. R., Chen, P., Cho, M., Choi, H. S., Choi, Y. J., Connel, P., Dagoret-Campagne, S., Eyles, C., Grossan, B., ... Yashin, I. (2014). The status of the ultra fast flash observatory - pathfinder. Nuclear Physics B - Proceedings Supplements, 246-247, 29-33. https://doi.org/10.1016/j.nuclphysbps.2013.10.061

Nam, J. W. ; Ahmad, S. ; Ahn, K. B. ; Barrillon, P. ; Brandt, S. ; Budtz-Jrgensen, C. ; Castro-Tirado, A. J. ; Chang, C. H. ; Chang, C. Y. ; Chang, Y. Y. ; Chen, C. R. ; Chen, P. ; Cho, M. ; Choi, H. S. ; Choi, Y. J. ; Connel, P. ; Dagoret-Campagne, S. ; Eyles, C. ; Grossan, B. ; Huang, J. J. ; Huang, M. H.A. ; Jeong, S. ; Jung, A. ; Kim, J. E. ; Kim, M. B. ; Kim, S. W. ; Kim, Y. W. ; Krasnov, A. S. ; Lee, J. ; Lim, H. ; Linder, E. V. ; Liu, T. C. ; Lund, N. ; Min, K. W. ; Na, G. W. ; Panasyuk, M. I. ; Park, I. H. ; Reglero, V. ; Ripa, J. ; Rodrigo, J. M. ; Smoot, G. F. ; Suh, J. E. ; Svertilov, S. ; Vedenkin, N. ; Wang, M. Z. ; Yashin, I. / The status of the ultra fast flash observatory - pathfinder. In: Nuclear Physics B - Proceedings Supplements. 2014 ; Vol. 246-247. pp. 29-33.

@article{c2b58fc5e68f4087ae0340c6deb60776,

title = "The status of the ultra fast flash observatory - pathfinder",

abstract = "The Ultra Fast Flash Observatory (UFFO) is a project to study early optical emissions from Gamma Ray Bursts (GRBs). The primary scientific goal of UFFO is to see if GRBs can be calibrated with their rising times, so that they could be used as new standard candles. In order to minimize delay in optical follow-up measurements, which is now about 100 sec after trigger from the Swift experiment, we rotate a mirror to redirect light path so that optical measurement can be performed within a second after the trigger. We have developed a pathfinder mission, UFFO-pathfinder to launch on board the Lomonosov satellite in 2012. In this talk, I will present scientific motivations and descriptions of the design and development of UFFO-pathfinder.",

author = "Nam, {J. W.} and S. Ahmad and Ahn, {K. B.} and P. Barrillon and S. Brandt and C. Budtz-Jrgensen and Castro-Tirado, {A. J.} and Chang, {C. H.} and Chang, {C. Y.} and Chang, {Y. Y.} and Chen, {C. R.} and P. Chen and M. Cho and Choi, {H. S.} and Choi, {Y. J.} and P. Connel and S. Dagoret-Campagne and C. Eyles and B. Grossan and Huang, {J. J.} and Huang, {M. H.A.} and S. Jeong and A. Jung and Kim, {J. E.} and Kim, {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 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 = "2014",

month = jan

day = "1",

doi = "10.1016/j.nuclphysbps.2013.10.061",

language = "English",

volume = "246-247",

pages = "29--33",

journal = "Nuclear and Particle Physics Proceedings",

issn = "2405-6014",

publisher = "Elsevier",

}

Nam, JW, Ahmad, S, Ahn, KB, Barrillon, P, Brandt, S, Budtz-Jrgensen, C, Castro-Tirado, AJ, Chang, CH, Chang, CY, Chang, YY, Chen, CR, Chen, P, Cho, M, Choi, HS, Choi, YJ, Connel, P, Dagoret-Campagne, S, Eyles, C, Grossan, B, Huang, JJ, Huang, MHA, Jeong, S, Jung, A, Kim, JE, Kim, MB, Kim, SW, Kim, YW, Krasnov, AS, Lee, J, Lim, H, Linder, EV, Liu, TC, Lund, N, 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 2014, 'The status of the ultra fast flash observatory - pathfinder', Nuclear Physics B - Proceedings Supplements, vol. 246-247, pp. 29-33. https://doi.org/10.1016/j.nuclphysbps.2013.10.061

The status of the ultra fast flash observatory - pathfinder. / Nam, J. W.; Ahmad, S.; Ahn, K. B.; Barrillon, P.; Brandt, S.; Budtz-Jrgensen, C.; Castro-Tirado, A. J.; Chang, C. H.; Chang, C. Y.; Chang, Y. Y.; Chen, C. R.; Chen, P.; Cho, M.; Choi, H. S.; Choi, Y. J.; Connel, P.; Dagoret-Campagne, S.; Eyles, C.; Grossan, B.; Huang, J. J.; Huang, M. H.A.; Jeong, S.; Jung, A.; Kim, J. E.; Kim, M. B.; Kim, S. W.; Kim, Y. W.; Krasnov, A. S.; Lee, J.; Lim, H.; Linder, E. V.; Liu, T. C.; Lund, N.; Min, K. W.; Na, G. W.; Panasyuk, M. I.; Park, I. H.; Reglero, V.; Ripa, J.; Rodrigo, J. M.; Smoot, G. F.; Suh, J. E.; Svertilov, S.; Vedenkin, N.; Wang, M. Z.; Yashin, I.

In: Nuclear Physics B - Proceedings Supplements, Vol. 246-247, 01.01.2014, p. 29-33.

Research output: Contribution to journal › Article

TY - JOUR

T1 - The status of the ultra fast flash observatory - pathfinder

AU - Nam, J. W.

AU - Ahmad, S.

AU - Ahn, K. B.

AU - Barrillon, P.

AU - Brandt, S.

AU - Budtz-Jrgensen, C.

AU - Castro-Tirado, A. J.

AU - Chang, C. H.

AU - Chang, C. Y.

AU - Chang, Y. Y.

AU - Chen, C. R.

AU - Chen, P.

AU - Cho, M.

AU - Choi, H. S.

AU - Choi, Y. J.

AU - Connel, P.

AU - Dagoret-Campagne, S.

AU - Eyles, C.

AU - Grossan, B.

AU - Huang, J. J.

AU - Huang, M. H.A.

AU - Jeong, S.

AU - Jung, A.

AU - Kim, J. E.

AU - Kim, 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 - 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 - 2014/1/1

Y1 - 2014/1/1

N2 - The Ultra Fast Flash Observatory (UFFO) is a project to study early optical emissions from Gamma Ray Bursts (GRBs). The primary scientific goal of UFFO is to see if GRBs can be calibrated with their rising times, so that they could be used as new standard candles. In order to minimize delay in optical follow-up measurements, which is now about 100 sec after trigger from the Swift experiment, we rotate a mirror to redirect light path so that optical measurement can be performed within a second after the trigger. We have developed a pathfinder mission, UFFO-pathfinder to launch on board the Lomonosov satellite in 2012. In this talk, I will present scientific motivations and descriptions of the design and development of UFFO-pathfinder.

AB - The Ultra Fast Flash Observatory (UFFO) is a project to study early optical emissions from Gamma Ray Bursts (GRBs). The primary scientific goal of UFFO is to see if GRBs can be calibrated with their rising times, so that they could be used as new standard candles. In order to minimize delay in optical follow-up measurements, which is now about 100 sec after trigger from the Swift experiment, we rotate a mirror to redirect light path so that optical measurement can be performed within a second after the trigger. We have developed a pathfinder mission, UFFO-pathfinder to launch on board the Lomonosov satellite in 2012. In this talk, I will present scientific motivations and descriptions of the design and development of UFFO-pathfinder.

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UR - http://www.scopus.com/inward/citedby.url?scp=84891931353&partnerID=8YFLogxK

U2 - 10.1016/j.nuclphysbps.2013.10.061

DO - 10.1016/j.nuclphysbps.2013.10.061

M3 - Article

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VL - 246-247

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EP - 33

JO - Nuclear and Particle Physics Proceedings

JF - Nuclear and Particle Physics Proceedings

SN - 2405-6014

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10.1016/j.nuclphysbps.2013.10.061