activity
20012005
most citedThe host of GRB 030323 at z=3.372: a very high column density DLA system with a low metallicity

210 citations · 434 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph2005★ 33 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-ph2004★ 210 cited

The host of GRB 030323 at z=3.372: a very high column density DLA system with a low metallicity

P. M. Vreeswijk, S. L. Ellison, C. Ledoux +29

We present photometry and spectroscopy of the afterglow of GRB 030323. VLT spectra of the afterglow show damped Lya (DLA) absorption and low- and high-ionization lines at a redshif…

astro-ph2003★ 77 cited

The formation of the double neutron star pulsar J0737--3039

J. D. M. Dewi, E. P. J. van den Heuvel

We find that the orbital period (2.4 hours), eccentricity (0.09), dipole magnetic field strength (6.9 x 10^9 Gauss) and spin period (22 ms) of the new highly relativistic double ne…

astro-ph2003★ 45 cited

The blue host galaxy of the red GRB 000418

J. Gorosabel, S. Klose, L. Christensen +25

We report on multi-band (UBVRIZJsKs) observations of the host galaxy of the April 18, 2000 gamma-ray burst. The Spectral Energy Distribution (SED) is analysed by fitting empirical…

astro-ph2002★ 63 cited

A multi-colour study of the dark GRB 000210 host galaxy and its environment

J. Gorosabel, L. Christensen, J. Hjorth +25

We present UBVRIZJsHKs broad band photometry of the host galaxy of the dark gamma-ray burst (GRB) of February 10, 2000. These observations represent the most exhaustive photometry…

astro-ph2001★ 6 cited

The bright optical afterglow of the long GRB 001007

J. M. Castro Cerón, A. J. Castro-Tirado, J. Gorosabel +35

We present optical follow up observations of the long GRB 001007 between 6.14 hours and ~468 days after the event. An unusually bright optical afterglow (OA) was seen to decline fo…