GRB 050223: A faint gamma-ray burst discovered by Swift

  • K. L. Page
  • , E. Rol
  • , A. J. Levan
  • , B. Zhang
  • , J. P. Osborne
  • , P. T. O'Brien
  • , A. P. Beardmore
  • , D. N. Burrows
  • , S. Campana
  • , G. Chincharini
  • , J. R. Cummings
  • , G. Cusumano
  • , N. Gehrels
  • , P. Giommi
  • , M. R. Goad
  • , O. Godet
  • , V. Mangano
  • , G. Tagliaferri
  • , A. A. Wells

Research output: Contribution to journalLetterpeer-review

9 Scopus citations

Abstract

GRB 050223 was discovered by the Swift Gamma-Ray Burst Explorer on 2005 February 23 and was the first gamma-ray burst (GRB) to be observed by both Swift and XMM-Newton. At the time of writing (2005 May), it has one of the faintest GRB afterglows ever observed. The spacecraft could not slew immediately to the burst, so the first X-ray and optical observations occurred approximately 45 min after the trigger. Although no optical emission was found by any instrument, both Swift and XMM-Newton detected the fading X-ray afterglow. Combined data from both of these observatories show the afterglow to be fading monotonically as 0.99+0.15-0.12 over a time-frame between 45 min and 27 h post-burst. Spectral analysis, allowed largely by the higher throughput of XMM-Newton, implies a power law with a slope of Γ = 1.75+0.19-0.18and shows no evidence for absorption above the Galactic column of 7 × 1020 cm-2. From the X-ray decay and spectral slopes, a low electron power-law index of p = 1.3-1.9 is derived; the slopes also imply that a jet-break has not occurred up to 27 h after the burst. The faintness of GRB 050223 may be due to a large jet opening or viewing angle or a high redshift.

Original languageEnglish (US)
Pages (from-to)L76-L80
JournalMonthly Notices of the Royal Astronomical Society: Letters
Volume363
Issue number1
DOIs
StatePublished - Oct 2005

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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