most citedOutshining the quasars at reionisation: The X-ray spectrum and lightcurve of the redshift 6.29 Gamma-Ray Burst GRB050904

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astro-ph200537 cited

The soft X-ray blast in the apparently sub-luminous GRB 031203

D. Watson, S. A. Vaughan, R. Willingale +11

GRB031203 was a very low apparent luminosity gamma-ray burst (GRB). It was also the first GRB with a dust-scattered X-ray halo. The observation of the halo allowed us to infer the…

astro-ph200516 cited

Multi-Wavelength Studies of the Optically Dark Gamma-Ray Burst 001025A

K. Pedersen, K. Hurley, J. Hjorth +18

We identify the fading X-ray afterglow of GRB 001025A from XMM-Newton observations obtained 1.9-2.3 days, 2 years, and 2.5 years after the burst. The non-detection of an optical co…

astro-ph200517 cited

Plasma Diagnostics of Active Region Evolution and Implications for Coronal Heating

R. O. Milligan, P. T. Gallagher, M. Mathioudakis +2

A detailed study is presented of the decaying solar active region NOAA 10103 observed with the Coronal Diagnostic Spectrometer (CDS), the Michelson Doppler Imager (MDI) and the Ext…

astro-ph200550 cited

Outshining the quasars at reionisation: The X-ray spectrum and lightcurve of the redshift 6.29 Gamma-Ray Burst GRB050904

D. Watson, J. N. Reeves, J. Hjorth +7

Gamma-ray burst (GRB) 050904 is the most distant X-ray source known, at z=6.295, comparable to the farthest AGN and galaxies. Its X-ray flux decays, but not as a power-law; it is d…

astro-ph200537 cited

Climatic and Biogeochemical Effects of a Galactic Gamma-Ray Burst

Adrian L. Melott, Brian C. Thomas, Daniel P. Hogan +2

It is likely that one or more gamma-ray bursts within our galaxy have strongly irradiated the Earth in the last Gy. This produces significant atmospheric ionization and dissociatio…

astro-ph200526 cited

Discovery of the INTEGRAL X/Gamma-ray transient IGR J00291+5934: a Comptonised accreting ms pulsar ?

S. E. Shaw, N. Mowlavi, J. Rodriguez +8

We report the discovery of a high-energy transient with the IBIS/ISGRI detector on board the INTEGRAL observatory. The source, namely IGR J00291+5934, was first detected on 2nd Dec…