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19982005
most citedThe line-of-sight towards GRB 030429 at z = 2.66: Probing the matter at stellar, galactic and intergalactic scales

129 citations · 408 across the 9 of their papers we have counts for

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astro-ph200579 cited

Gamma-Ray Burst Selected High Redshift Galaxies: Comparison to Field Galaxy Populations to z~3

C. J. Conselice, P. M. Vreeswijk, A. S. Fruchter +6

We study the internal structural properties of 37 long duration gamma-ray burst (GRB) host galaxies imaged with the Hubble Space Telescope. Fitting exponential disk and r^1/4 model…

astro-ph200511 cited

A Gamma-Ray Burst Mission to Investigate the Properties of Dark Energy

D. Q. Lamb, G. R. Ricker, D. Lazzati +26

[Abridged] Very recently, relations between the peak energy of Gamma-Ray Burst burst spectra, the isotropic-equivalent energy of the burst, and the radiated energy of the burst hav…

astro-ph2005126 cited

On the nature of nearby GRB/SN host galaxies

J. Sollerman, G. Ostlin, J. P. U. Fynbo +3

We present and discuss optical diagnostics of the low redshift (z<0.2) galaxies that are known to have hosted supernovae associated with gamma-ray bursts (GRBs). The three galaxies…

astro-ph200533 cited

Late-epoch optical and near-infrared observations of the GRB000911 afterglow and its host galaxy

N. Masetti, E. Palazzi, E. Pian +28

We present the results of an optical and near-infrared (NIR) monitoring campaign of the counterpart of Gamma-Ray Burst (GRB) 000911, located at redshift z=1.06, from 5 days to more…

astro-ph2004129 cited

The line-of-sight towards GRB 030429 at z = 2.66: Probing the matter at stellar, galactic and intergalactic scales

P. Jakobsson, J. Hjorth, J. P. U. Fynbo +21

We report the discovery of the optical afterglow (OA) of the long-duration gamma-ray burst GRB 030429, and present a comprehensive optical/near-infrared dataset used to probe the m…

astro-ph20043 cited

New Binary and Millisecond Pulsars from Arecibo Drift-Scan Searches

M. A. McLaughlin, D. R. Lorimer, D. J. Champion +6

We discuss four recycled pulsars found in Arecibo drift-scan searches. PSR J1944+0907 has a spin period of 5.2 ms and is isolated. The 5.8-ms pulsar J1453+19 may have a low-mass co…