Abstract
Understanding the reasons for the faintness of the optical/near-infrared afterglows of the so-called dark bursts is essential to assess whether they form a subclass of GRBs, and hence for the use of GRBs in cosmology. With VLT and other ground-based telescopes, we searched for the afterglows of the INTEGRAL bursts GRB 040223, GRB 040422 and GRB 040624 in the first hours after the triggers. A detection of a faint afterglow and of the host galaxy in the K band was achieved for GRB 040422, while only upper limits were obtained for GRB 040223 and GRB 040624, although in the former case the X-ray afterglow was observed. A comparison with the magnitudes of a sample of afterglows clearly shows the faintness of these bursts, which are good examples of a population that an increasing usage of large diameter telescopes is beginning to unveil.
| Original language | English (US) |
|---|---|
| Title of host publication | GAMMA-RAY BURSTS IN THE SWIFT ERA |
| Subtitle of host publication | Sixteenth Maryland Astrophysics Conference |
| Pages | 467-470 |
| Number of pages | 4 |
| DOIs | |
| State | Published - May 19 2006 |
| Event | GAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference - Washington, D.C., United States Duration: Nov 29 2005 → Dec 2 2005 |
Publication series
| Name | AIP Conference Proceedings |
|---|---|
| Volume | 836 |
| ISSN (Print) | 0094-243X |
| ISSN (Electronic) | 1551-7616 |
Other
| Other | GAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference |
|---|---|
| Country/Territory | United States |
| City | Washington, D.C. |
| Period | 11/29/05 → 12/2/05 |
All Science Journal Classification (ASJC) codes
- General Physics and Astronomy
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