GRB 050117: Simultaneous gamma-ray and X-ray observations with the Swift satellite

J. E. Hill, D. C. Morris, T. Sakamoto, G. Sato, D. N. Burrows, L. Angelini, C. Pagani, A. Moretti, A. F. Abbey, S. Barthelmy, A. P. Beardmore, V. V. Biryukov, S. Campana, M. Capalbi, G. Cusumano, P. Giommi, M. A. Ibrahimov, J. A. Kennea, S. Kobayashi, K. IokaC. Markwardt, P. Meszaros, P. T. O'Brien, J. P. Osborne, A. S. Pozanenko, M. Perri, V. V. Rumyantsev, P. Schady, D. A. Sharapov, G. Tagliaferri, B. Zhang, G. Chincarini, N. Gehrels, A. Wells, J. A. Nousek

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The Swift Gamma-Ray Burst Explorer performed its first autonomous, X-ray follow-up to a newly detected GRB on 2005 January 17, within 193 seconds of the burst trigger by the Swift Burst Alert Telescope. While the burst was still in progress, the X-ray Telescope obtained a position and an image for an un-catalogued X-ray source; simultaneous with the gamma-ray observation. The XRT observed flux during the prompt emission was 1.1 × 10-8 ergs cm-2 s-1 in the 0.5-10 keV energy band. The emission in the X-ray band decreased by three orders of magnitude within 700 seconds, following the prompt emission. This is found to be consistent with the gamma-ray decay when extrapolated into the XRT energy band. During the following 6.3 hours, the XRT observed the afterglow in an automated sequence for an additional 947 seconds, until the burst became fully obscured by the Earth limb. A faint, extremely slowly decaying afterglow, α=-0.21, was detected. Finally, a break in the lightcurve occurred and the flux decayed with α<-1.2. The X-ray position triggered many follow-up observations: no optical afterglow could be confirmed, although a candidate was identified 3 arcsecs from the XRT position.

Original languageEnglish
Title of host publicationAIP Conference Proceedings
Pages289-292
Number of pages4
Volume836
DOIs
Publication statusPublished - 2006 May 19
EventGAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference - Washington, D.C.
Duration: 2005 Nov 292005 Dec 2

Other

OtherGAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference
CityWashington, D.C.
Period05/11/2905/12/2

Fingerprint

gamma rays
bursts
afterglows
x rays
energy bands
Earth limb
telescopes
gamma ray bursts
actuators
decay

Keywords

  • Gamma rays: bursts
  • General: gamma-rays, X-rays
  • Individual (GRB 050117)

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Hill, J. E., Morris, D. C., Sakamoto, T., Sato, G., Burrows, D. N., Angelini, L., ... Nousek, J. A. (2006). GRB 050117: Simultaneous gamma-ray and X-ray observations with the Swift satellite. In AIP Conference Proceedings (Vol. 836, pp. 289-292) https://doi.org/10.1063/1.2207904

GRB 050117 : Simultaneous gamma-ray and X-ray observations with the Swift satellite. / Hill, J. E.; Morris, D. C.; Sakamoto, T.; Sato, G.; Burrows, D. N.; Angelini, L.; Pagani, C.; Moretti, A.; Abbey, A. F.; Barthelmy, S.; Beardmore, A. P.; Biryukov, V. V.; Campana, S.; Capalbi, M.; Cusumano, G.; Giommi, P.; Ibrahimov, M. A.; Kennea, J. A.; Kobayashi, S.; Ioka, K.; Markwardt, C.; Meszaros, P.; O'Brien, P. T.; Osborne, J. P.; Pozanenko, A. S.; Perri, M.; Rumyantsev, V. V.; Schady, P.; Sharapov, D. A.; Tagliaferri, G.; Zhang, B.; Chincarini, G.; Gehrels, N.; Wells, A.; Nousek, J. A.

AIP Conference Proceedings. Vol. 836 2006. p. 289-292.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Hill, JE, Morris, DC, Sakamoto, T, Sato, G, Burrows, DN, Angelini, L, Pagani, C, Moretti, A, Abbey, AF, Barthelmy, S, Beardmore, AP, Biryukov, VV, Campana, S, Capalbi, M, Cusumano, G, Giommi, P, Ibrahimov, MA, Kennea, JA, Kobayashi, S, Ioka, K, Markwardt, C, Meszaros, P, O'Brien, PT, Osborne, JP, Pozanenko, AS, Perri, M, Rumyantsev, VV, Schady, P, Sharapov, DA, Tagliaferri, G, Zhang, B, Chincarini, G, Gehrels, N, Wells, A & Nousek, JA 2006, GRB 050117: Simultaneous gamma-ray and X-ray observations with the Swift satellite. in AIP Conference Proceedings. vol. 836, pp. 289-292, GAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference, Washington, D.C., 05/11/29. https://doi.org/10.1063/1.2207904
Hill JE, Morris DC, Sakamoto T, Sato G, Burrows DN, Angelini L et al. GRB 050117: Simultaneous gamma-ray and X-ray observations with the Swift satellite. In AIP Conference Proceedings. Vol. 836. 2006. p. 289-292 https://doi.org/10.1063/1.2207904
Hill, J. E. ; Morris, D. C. ; Sakamoto, T. ; Sato, G. ; Burrows, D. N. ; Angelini, L. ; Pagani, C. ; Moretti, A. ; Abbey, A. F. ; Barthelmy, S. ; Beardmore, A. P. ; Biryukov, V. V. ; Campana, S. ; Capalbi, M. ; Cusumano, G. ; Giommi, P. ; Ibrahimov, M. A. ; Kennea, J. A. ; Kobayashi, S. ; Ioka, K. ; Markwardt, C. ; Meszaros, P. ; O'Brien, P. T. ; Osborne, J. P. ; Pozanenko, A. S. ; Perri, M. ; Rumyantsev, V. V. ; Schady, P. ; Sharapov, D. A. ; Tagliaferri, G. ; Zhang, B. ; Chincarini, G. ; Gehrels, N. ; Wells, A. ; Nousek, J. A. / GRB 050117 : Simultaneous gamma-ray and X-ray observations with the Swift satellite. AIP Conference Proceedings. Vol. 836 2006. pp. 289-292
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abstract = "The Swift Gamma-Ray Burst Explorer performed its first autonomous, X-ray follow-up to a newly detected GRB on 2005 January 17, within 193 seconds of the burst trigger by the Swift Burst Alert Telescope. While the burst was still in progress, the X-ray Telescope obtained a position and an image for an un-catalogued X-ray source; simultaneous with the gamma-ray observation. The XRT observed flux during the prompt emission was 1.1 × 10-8 ergs cm-2 s-1 in the 0.5-10 keV energy band. The emission in the X-ray band decreased by three orders of magnitude within 700 seconds, following the prompt emission. This is found to be consistent with the gamma-ray decay when extrapolated into the XRT energy band. During the following 6.3 hours, the XRT observed the afterglow in an automated sequence for an additional 947 seconds, until the burst became fully obscured by the Earth limb. A faint, extremely slowly decaying afterglow, α=-0.21, was detected. Finally, a break in the lightcurve occurred and the flux decayed with α<-1.2. The X-ray position triggered many follow-up observations: no optical afterglow could be confirmed, although a candidate was identified 3 arcsecs from the XRT position.",
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AU - Hill, J. E.

AU - Morris, D. C.

AU - Sakamoto, T.

AU - Sato, G.

AU - Burrows, D. N.

AU - Angelini, L.

AU - Pagani, C.

AU - Moretti, A.

AU - Abbey, A. F.

AU - Barthelmy, S.

AU - Beardmore, A. P.

AU - Biryukov, V. V.

AU - Campana, S.

AU - Capalbi, M.

AU - Cusumano, G.

AU - Giommi, P.

AU - Ibrahimov, M. A.

AU - Kennea, J. A.

AU - Kobayashi, S.

AU - Ioka, K.

AU - Markwardt, C.

AU - Meszaros, P.

AU - O'Brien, P. T.

AU - Osborne, J. P.

AU - Pozanenko, A. S.

AU - Perri, M.

AU - Rumyantsev, V. V.

AU - Schady, P.

AU - Sharapov, D. A.

AU - Tagliaferri, G.

AU - Zhang, B.

AU - Chincarini, G.

AU - Gehrels, N.

AU - Wells, A.

AU - Nousek, J. A.

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N2 - The Swift Gamma-Ray Burst Explorer performed its first autonomous, X-ray follow-up to a newly detected GRB on 2005 January 17, within 193 seconds of the burst trigger by the Swift Burst Alert Telescope. While the burst was still in progress, the X-ray Telescope obtained a position and an image for an un-catalogued X-ray source; simultaneous with the gamma-ray observation. The XRT observed flux during the prompt emission was 1.1 × 10-8 ergs cm-2 s-1 in the 0.5-10 keV energy band. The emission in the X-ray band decreased by three orders of magnitude within 700 seconds, following the prompt emission. This is found to be consistent with the gamma-ray decay when extrapolated into the XRT energy band. During the following 6.3 hours, the XRT observed the afterglow in an automated sequence for an additional 947 seconds, until the burst became fully obscured by the Earth limb. A faint, extremely slowly decaying afterglow, α=-0.21, was detected. Finally, a break in the lightcurve occurred and the flux decayed with α<-1.2. The X-ray position triggered many follow-up observations: no optical afterglow could be confirmed, although a candidate was identified 3 arcsecs from the XRT position.

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