An online repository of Swift/XRT light curves of γ-ray bursts

P. A. Evans, A. P. Beardmore, K. L. Page, L. G. Tyler, J. P. Osborne, M. R. Goad, P. T. O'Brien, L. Vetere, J. Racusin, D. Morris, D. N. Burrows, M. Capalbi, M. Perri, N. Gehrels, P. Romano

Research output: Contribution to journalArticlepeer-review

463 Scopus citations

Abstract

Context. Swift data are revolutionising our understanding of Gamma Ray Bursts. Since bursts fade rapidly, it is desirable to create and disseminate accurate light curves rapidly. Aims. To provide the community with an online repository of X-ray light curves obtained with Swift. The light curves should be of the quality expected of published data, but automatically created and updated so as to be self-consistent and rapidly available. Methods. We have produced a suite of programs which automatically generates Swift/XRT light curves of GRBs. Effects of the damage to the CCD, automatic readout-mode switching and pile-up are appropriately handled, and the data are binned with variable bin durations, as necessary for a fading source. Results. The light curve repository website* contains light curves, hardness ratios and deep images for every GRB which Swift's XRT has observed. When new GRBs are detected, light curves are created and updated within minutes of the data arriving at the UK Swift Science Data Centre.

Original languageEnglish (US)
Pages (from-to)379-385
Number of pages7
JournalAstronomy and Astrophysics
Volume469
Issue number1
DOIs
StatePublished - Jul 2007

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'An online repository of Swift/XRT light curves of γ-ray bursts'. Together they form a unique fingerprint.

Cite this