GRB 030227: the first multiwavelength afterglow of an INTEGRAL GRB
| dc.creator | Castro-Tirado, A. J. | |
| dc.creator | Gorosabel, J. | |
| dc.creator | Guziy, S. | |
| dc.creator | Reverte, D. | |
| dc.creator | Cerón, J. M. Castro | |
| dc.creator | Postigo, A. de Ugarte | |
| dc.creator | Tanvir, N. | |
| dc.creator | Mereghetti, S. | |
| dc.creator | Tiengo, A. | |
| dc.creator | Buckle, J. | |
| dc.creator | Sagar, R. | |
| dc.creator | Pandey, S. B. | |
| dc.creator | Mohan, V. | |
| dc.creator | Masetti, N. | |
| dc.creator | Mannucci, F. | |
| dc.creator | Feltzing, S. | |
| dc.creator | Lundstrom, I. | |
| dc.creator | Pedersen, H. | |
| dc.creator | Riess, C. | |
| dc.creator | Trushkin, S. | |
| dc.creator | Vilchez, J. | |
| dc.creator | Lund, N. | |
| dc.creator | Brandt, S. | |
| dc.creator | Nunez, S. Martinez | |
| dc.creator | Reglero, V. | |
| dc.creator | Perez-Ramirez, M. D. | |
| dc.creator | Klose, S. | |
| dc.creator | Greiner, J. | |
| dc.creator | Hjorth, J. | |
| dc.creator | Kaper, L. | |
| dc.creator | Pian, E. | |
| dc.creator | Palazzi, E. | |
| dc.creator | Andersen, M. I. | |
| dc.creator | Fruchter, A. | |
| dc.creator | Fynbo, J. P. U. | |
| dc.creator | Jensen, B. L. | |
| dc.creator | Kouveliotou, C. | |
| dc.creator | Rhoads, J. | |
| dc.creator | Rol, E. | |
| dc.creator | Vreeswijk, P. M. | |
| dc.creator | Wijers, R. A. M. J. | |
| dc.creator | Heuvel, E. van den | |
| dc.date | 2003-09-29 | |
| dc.date.accessioned | 2026-07-07T12:00:57Z | |
| dc.date.available | 2026-07-07T12:00:57Z | |
| dc.description | 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 dim optical afterglow (OA) that would not have been detected by many previous searches due to its faintess (R~23). This OA was seen to decline following a power law decay with index Alpha_R= -0.95 +/- 0.16. The spectral index Beta_opt/NIR yielded -1.25 +/- 0.14. These values may be explained by a relativistic expansion of a fireball (with p = 2.0) in the cooling regime. We also find evidence for inverse Compton scattering in X-rays. | |
| dc.description | 5 pages, 5 figures, accepted for publication in A&A | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0309804 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0309804 | |
| dc.identifier | Astron.Astrophys.411:L315-L319,2003 | |
| dc.identifier | doi:10.1051/0004-6361:20031393 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/206954 | |
| dc.subject | Astrophysics | |
| dc.title | GRB 030227: the first multiwavelength afterglow of an INTEGRAL GRB | |
| dc.type | text |