GRB 040403: a faint X-ray rich Gamma-ray Burst discovered by INTEGRAL
| dc.creator | Mereghetti, S. | |
| dc.creator | Gotz, D. | |
| dc.creator | Andersen, M. I. | |
| dc.creator | Castro-Tirado, A. | |
| dc.creator | Frontera, F. | |
| dc.creator | Gorosabel, J. | |
| dc.creator | Hartmann, D. H. | |
| dc.creator | Hjorth, J. | |
| dc.creator | Hudec, R. | |
| dc.creator | Hurley, K. | |
| dc.creator | Pizzichini, G. | |
| dc.creator | Produit, N. | |
| dc.creator | Tarana, A. | |
| dc.creator | Topinka, M. | |
| dc.creator | Ubertini, P. | |
| dc.creator | de Ugarte, A. | |
| dc.date | 2004-12-01 | |
| dc.date.accessioned | 2026-07-07T02:16:06Z | |
| dc.date.available | 2026-07-07T02:16:06Z | |
| dc.description | GRB 040403 is one of the faintest gamma-ray bursts for which a rapid and accurate localization has been obtained. Here we report on the gamma-ray properties of this burst, based on observations with the IBIS instrument aboard INTEGRAL, and the results of searches for its optical afterglow. The steep spectrum (power law photon index = 1.9 in the 20-200 keV range) implies that GRB 040403 is most likely an X-ray rich burst. Our optical limit of R > 24.2 at 16.5 hours after the burst, indicates a rather faint afterglow, similar to those seen in other relatively soft and faint bursts. | |
| dc.description | 5 pages, 3 figures, accepted for publication in Astronomy and Astrophysics Letters | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0412012 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0412012 | |
| dc.identifier | Astron.Astrophys. 433 (2005) 113-116 | |
| dc.identifier | doi:10.1051/0004-6361:20042030 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/8662 | |
| dc.subject | Astrophysics | |
| dc.title | GRB 040403: a faint X-ray rich Gamma-ray Burst discovered by INTEGRAL | |
| dc.type | text |