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Open AccessJournal ArticleDOI

An online repository of Swift/XRT light curves of GRBs.

TLDR
In this paper, the authors present a suite of programs that automatically generate Swift/XRT light curves of Gamma Ray Bursts (GRBs) from X-ray light curves obtained with the UK Swift Science Data Centre.
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.

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Journal ArticleDOI

The physics of gamma-ray bursts & relativistic jets

TL;DR: A comprehensive review of major developments in our understanding of gamma-ray bursts, with particular focus on the discoveries made within the last fifteen years when their true nature was uncovered, can be found in this paper.
Journal ArticleDOI

The Physics of Gamma-Ray Bursts and Relativistic Jets

TL;DR: A comprehensive review of major developments in the understanding of gamma-ray bursts can be found in this article, with particular focus on the discoveries made within the last fifteen years when their true nature was uncovered.
Journal ArticleDOI

Gamma-Ray Bursts in the Swift Era

TL;DR: The Swift satellite has transformed the physical understanding of γ-ray bursts (GRBs) by providing high-quality observations of hundreds of bursts, and facilitating a wide range of follow-up observations within seconds of each event as mentioned in this paper.
Journal ArticleDOI

A Decade of Short-duration Gamma-ray Burst Broadband Afterglows: Energetics, Circumburst Densities, and jet Opening Angles

TL;DR: In this article, the authors present a comprehensive catalog and analysis of broad-band afterglow observations for 103 short-duration gamma-ray bursts (GRBs), comprised of all short GRBs from November 2004 to March 2015 with prompt follow-up observations in the X-ray, optical, near-infrared and/or radio bands.
References
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Journal ArticleDOI

The Swift Gamma-Ray Burst Mission

Neil Gehrels, +77 more
TL;DR: The Swift mission as discussed by the authors is a multi-wavelength observatory for gamma-ray burst (GRB) astronomy, which is a first-of-its-kind autonomous rapid-slewing satellite for transient astronomy and pioneers the way for future rapid-reaction and multiwavelength missions.
Journal ArticleDOI

The Swift X-ray telescope

TL;DR: The Swift Gamma-Ray Explorer (XRT) as mentioned in this paper uses a mirror set built for JET-X and an XMM-Newton/EPIC MOS CCD detector to provide a sensitive broad-band (0.2-10 keV) X-ray imager with effective area of > 120 cm2 at 1.5 keV, field of view of 23.6 × 23. 6 arcminutes, and angular resolution of 18 arcseconds.
Journal ArticleDOI

The Swift X-ray Telescope

TL;DR: The Swift Gamma-Ray Explorer (XRT) as mentioned in this paper uses a mirror set built for JET-X and an XMM/EPIC MOS CCD detector to provide a sensitive broad-band (0.2-10 keV) X-ray imager with effective area of > 120 cm^2 at 1.5 keV, field of view of 23.6 x23.6 arcminutes, and angular resolution of 18 arcseconds (HPD).
Journal ArticleDOI

Determination of confidence limits for experiments with low numbers of counts

TL;DR: In this paper, two different methods, classical and Bayesian, for determining confidence intervals involving Poisson-distributed data are compared and reasons for preferring the Bayesian over the classical method are given.
Journal ArticleDOI

Studies in Astronomical Time Series Analysis. V. Bayesian Blocks, a New Method to Analyze Structure in Photon Counting Data*

TL;DR: A new time-domain algorithm for detecting localized structures (bursts), revealing pulse shapes, and generally characterizing intensity variations, based on Bayesian statistics, which is demonstrated by analyzing pulse structure in BATSE γ-ray data.
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