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most citedGlobal Properties of X-Ray Flashes and X-Ray-Rich Gamma-Ray Bursts Observed by Swift

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astro-ph200893 cited

Global Properties of X-Ray Flashes and X-Ray-Rich Gamma-Ray Bursts Observed by Swift

T. Sakamoto, D. Hullinger, G. Sato +14

We describe and discuss the spectral and temporal characteristics of the prompt emission and X-ray afterglow emission of X-ray flashes (XRFs) and X-ray-rich gamma-ray bursts (XRRs)…

astro-ph200613 cited

X-ray Flashes or soft Gamma-ray Bursts? The case of the likely distant XRF 040912

G. Stratta, S. Basa, N. Butler +49

In this work, we present a multi-wavelength study of XRF 040912, aimed at measuring its distance scale and the intrinsic burst properties. We performed a detailed spectral and temp…

astro-ph2005

High Resolution Gratings Spectroscopy of GRBs 030382 and 041006 with Chandra LETGS

N. R. Butler, G. R. Ricker, P. G. Ford +5

We present high resolution X-ray spectroscopy of two recent GRB afterglows observed with the Low Energy Transmission Gratings on Chandra. The afterglows to GRBs 030328 and 041006 a…

astro-ph2004

Global Characteristics of X-Ray Flashes and X-Ray-Rich GRBs Observed by HETE-2

T. Sakamoto, D. Q. Lamb, C. Graziani +35

We describe and discuss the global properties of 45 gamma-ray bursts (GRBs) observed by HETE-2 during the first three years of its mission, focusing on the properties of X-Ray Flas…

astro-ph2003

A Unified Jet Model of X-Ray Flashes, X-Ray-Rich Gamma-Ray Bursts, and Gamma-Ray Bursts: I. Power-Law-Shaped Universal and Top-Hat-Shaped Variable Opening-Angle Jet Models

D. Q. Lamb, T. Q. Donaghy, C. Graziani

HETE-2 has provided strong evidence that the properties of X-Ray Flashes (XRFs), X-ray-rich GRBs, and GRBs form a continuum, and therefore that these three kinds of bursts are the…

astro-ph2003

The X-ray Afterglows of GRB 020813 and GRB 021004 with Chandra HETGS: Possible Evidence for a Supernova Prior to GRB 020813

Nathaniel R. Butler, Herman L. Marshall, George R. Ricker +5

We report on the detection of an emission line near 1.3 keV, which we associate with blue-shifted hydrogen-like sulfur (S XVI), in a 76.8 ksec Chandra HETGS spectrum of the aftergl…