most citedLy-alpha and UV emission from high-redshift GRB hosts: To what extent do GRBs trace star formation?

95 citations · 320 across the 6 of their papers we have counts for

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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-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-ph200589 cited

The GRB 030329 host: a blue low metallicity subluminous galaxy with intense star formation

J. Gorosabel, D. Pérez-Ramírez, J. Sollerman +13

We present broad band photometry and spectroscopic observations of the host galaxy of GRB 030329. Analysis of the spectral emission lines shows that the host is likely a low metall…

astro-ph200595 cited

Ly-alpha and UV emission from high-redshift GRB hosts: To what extent do GRBs trace star formation?

P. Jakobsson, G. Bjornsson, J. P. U. Fynbo +9

We report the result of a search for Ly-alpha emission from the host galaxies of the gamma-ray bursts (GRBs) 030226 (z = 1.986), 021004 (z = 2.335) and 020124 (z = 3.198). We find…

astro-ph20058 cited

The red optical afterglow of GRB 030725

G. Pugliese, P. Møller, J. Gorosabel +6

We present a photometric study of the optical counterpart of the long-duration Gamma Ray Burst (GRB) 030725, which triggered the HETE FREGATE and WXM instruments on July 25th, 2003…

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…