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19972026
most citedA very energetic supernova associated with the gamma-ray burst of 29 March 2003

1.5k citations · 15.4k across the 209 of their papers we have counts for

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Showing 2003 · astro-phShow all

17 papers · 2 filters

astro-ph2003

The polarization evolution of the optical afterglow of GRB 030329

J. Greiner, S. Klose, K. Reinsch +23

We report 31 polarimetric observations of the afterglow of GRB 030329 with high signal-to-noise and high sampling frequency. The data imply that the afterglow magnetic field has sm…

astro-ph2003★ 116 cited

Evolution of the polarization of the optical afterglow of the gamma-ray burst GRB 030329

J. Greiner, S. Klose, K. Reinsch +23

We report 31 polarimetric observations of the afterglow of GRB 030329 with high signal-to-noise and high sampling frequency. We establish the polarization light curve, detect susta…

astro-ph2003★ 28 cited

X-ray/optical observations of A0535+26/HDE 245770 in quiescence

M. Orlandini, C. Bartolini, S. Campana +10

We present the result of three BeppoSAX observations of the X-ray binary pulsar A0535+26 in its quiescent state. The source is quite well detected up to 200 keV (6 sigma detection…

astro-ph2003★ 19 cited

GRB 030227: the first multiwavelength afterglow of an INTEGRAL GRB

A. J. Castro-Tirado, J. Gorosabel, S. Guziy +39

We present multiwavelength observations of a gamma-ray burst detected by INTEGRAL (GRB 030227) between 5.3 hours and ~1.7 days after the event. Here we report the discovery of a di…

astro-ph2003★ 112 cited

Very high column density and small reddening towards GRB 020124 at z = 3.20

J. Hjorth, P. Møller, J. Gorosabel +27

We present optical and near-infrared observations of the dim afterglow of GRB 020124, obtained between 2 and 68 hours after the gamma-ray burst. The burst occurred in a very faint…

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-ph2003★ 58 cited

Variable polarization in the optical afterglow of GRB 021004

E. Rol, R. A. M. J. Wijers, J. P. U. Fynbo +19

We present polarimetric observations of the afterglow of gamma-ray burst (GRB) 021004, obtained with the Nordic Optical Telescope (NOT) and the Very Large Telescope (VLT) between 8…

astro-ph2003★ 1.5k cited

A very energetic supernova associated with the gamma-ray burst of 29 March 2003

Jens Hjorth, Jesper Sollerman, Palle Møller +24

Over the past five years evidence has mounted that long-duration (> 2 s) gamma-ray bursts (GRBs)--the most brilliant of all astronomical explosions--signal the collapse of massive…

astro-ph2003★ 25 cited

Yet another galaxy identification for an ultraluminous X-ray source

N. Masetti, L. Foschini, L. C. Ho +4

We report on the identification of the optical and infrared counterparts of the ultraluminous X-ray source (ULX) XMMU J121214.5+131248 (NGC4168-ULX1). The optical spectrum yields a…

astro-ph2003★ 10 cited

XMM-Newton Observations of the Field of Gamma-Ray Burst 980425

E. Pian, P. Giommi, L. Amati +12

The error box of GRB980425 has been observed by XMM-Newton in March 2002, with the aim of measuring the late epoch X-ray emission of the supernova 1998bw and of clarifying its supp…

astro-ph2003★ 34 cited

Spectral and Temporal Behavior of the Black Hole Candidate XTE J1118+480 as Observed with BeppoSAX

F. Frontera, L. Amati, A. A. Zdziarski +5

XTE J1118+480 is a well established black hole candidate with a mass estimate in the range from 7 to 10 solar masses. With BeppoSAX we observed the source 4 times, from April to De…

astro-ph2003★ 94 cited

Optical and near-infrared observations of the GRB020405 afterglow

N. Masetti, E. Palazzi, E. Pian +33

(Abridged) We report on observations of the optical and NIR afterglow of GRB020405. Ground-based optical observations started about 1 day after the GRB and spanned a period of ~10…

astro-ph2003

Optical and NIR monitoring of the GRB020405 afterglow

N. Masetti, E. Palazzi, E. Pian

Optical and near-infrared (NIR) observations of GRB020405 started about 1 day after the GRB and extended over ~70 days. Photometry shows that the early decay is consistent with a s…

astro-ph2003

Multiwavelength observations of the GRB000615 field

E. Maiorano, N. Masetti, E. Palazzi +6

We report on prompt and afterglow observations of GRB 000615 detected by BeppoSAX. The study of the high-energy prompt event is presented along with the search for its X-ray and op…

astro-ph2003★ 14 cited

The dark burst 010214 with BeppoSAX: possible variable absorption and jet X-ray emission

C. Guidorzi, F. Frontera, E. Montanari +12

We report on the prompt and afterglow emission observations of the dark burst GRB010214 with BeppoSAX. The prompt emission shows possible evidence of variable absorption from N_H =…

astro-ph2003

The optical/near-IR spectral energy distribution of the GRB 000210 host galaxy

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

We report on UBVRIZJsHKs-band photometry of the dark GRB 000210 host galaxy. Fitting a grid of spectral templates to its Spectral Energy Distribution (SED), we derived a photometri…

astro-ph2003★ 13 cited

BeppoSAX observations of two unclassified LMXBs: X1543-624 and X1556-605

R. Farinelli, F. Frontera, N. Masetti +8

Observations of two unclassified Low Mass X-ray Binaries, X1543-624 and X1556-605, are presented. In the 2-10 keV band the first of the two sources is a factor two stronger than th…