activity
19962005
most citedThe line-of-sight towards GRB 030429 at z = 2.66: Probing the matter at stellar, galactic and intergalactic scales

129 citations · 395 across the 9 of their papers we have counts for

collaborators
Showing 2001Show all

6 papers · 1 filter

astro-ph2001

The BeppoSAX View on the 2001 Reactivation of SGR 1900+14

M. Feroci, S. Mereghetti, E. Costa +13

After a couple of years of quiescence, the soft gamma repeater SGR 1900+14 suddenly reactivated on 18 April 2001, with the emission of a very intense, long and modulated flare, onl…

astro-ph2001

Strategies for prompt searches for GRB afterglows: the discovery of the GRB 001011 optical/near-infrared counterpart using colour-colour selection

J. Gorosabel, J. U. Fynbo, J. Hjorth +25

We report the discovery of the optical and near-infrared counterparts to GRB 001011. The GRB 001011 error box determined by Beppo-SAX was simultaneously imaged in the near-infrared…

astro-ph2001

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…

astro-ph2001

The GLAST Burst Monitor (GBM)

G. G. Lichti, M. S. Briggs, R. Diehl +9

The selection of the GLAST burst monitor (GBM) by NASA will allow the investigation of the relation between the keV and the MeV-GeV emission from gamma-ray bursts. The GBM consists…

astro-ph2001

The extraordinarily bright optical afterglow of GRB 991208 and its host galaxy

A. J. Castro-Tirado, V. V. Sokolov, J. Gorosabel +50

Observations of the extraordinarily bright optical afterglow (OA) of GRB 991208 started 2.1 d after the event. The flux decay constant of the OA in the R-band is -2.30 +/- 0.07 up…

astro-ph2001

Discovery of a kHz QPO in 2S 0918-549

Peter G. Jonker, Michiel van der Klis, Jeroen Homan +6

We report the discovery of a kilohertz quasi-periodic oscillation (kHz QPO) in the low-mass X-ray binary (LMXB) 2S 0918-549. The kHz QPO has a frequency of 1156+-9 Hz, a FWHM of 70…