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19952005
most citedThe redshift distribution of gamma-ray bursts revisited

78 citations · 126 across the 3 of their papers we have counts for

collaborators

12 papers

astro-ph200578 cited

The redshift distribution of gamma-ray bursts revisited

Priyamvada Natarajan, Badr Albanna, Jens Hjorth +3

In this letter, we calculate the redshift distribution of gamma-ray bursts assuming that they trace (i) the globally averaged star formation rate or (ii) the average metallicity in…

astro-ph20041 cited

Quantifying Substructure Using Galaxy-Galaxy Lensing in Distant Clusters

Priyamvada Natarajan, Jean-Paul Kneib, Ian Smail +1

We present high-resolution mass reconstructions for five massive cluster-lenses spanning a redshift range from z = 0.18 - 0.57 utilizing archival Hubble Space Telescope data and ap…

astro-ph200247 cited

The afterglow and complex environment of the optically dim burst GRB 980613

Jens Hjorth, Bjarne Thomsen, Svend R. Nielsen +15

We report the identification of the optical afterglow of GRB 980613 in R- and I-band images obtained between 16 and 48 hours after the gamma-ray burst. Early near-infrared (NIR) H…

astro-ph2002

An HST study of three very faint GRB host galaxies

A. O. Jaunsen, M. I. Andersen, J. Hjorth +8

As part of the HST/STIS GRB host survey program we present the detection of three faint gamma-ray burst (GRB) host galaxies based on an accurate localisation using ground-based dat…

astro-ph2001

The Host Galaxy and Optical Light Curve of the Gamma-Ray Burst GRB 980703

S. Holland, J. P. U. Fynbo, J. Hjorth +10

We present deep HST/STIS and ground-based photometry of the host galaxy of the gamma-ray burst GRB 980703 taken 17, 551, 710, and 716 days after the burst. We find that the host is…

astro-ph2000

HST/STIS Imaging of the Host Galaxy of GRB980425/SN1998bw

J. U. Fynbo, S. Holland, M. I. Andersen +6

We present HST/STIS observations of ESO 184-G82, the host galaxy of the gamma-ray burst GRB 980425 associated with the peculiar Type Ic supernova SN1998bw. ESO 184-G82 is found to…