On Gamma-Ray Bursts at Very High Redshifts

Details On Gamma-Ray Bursts at Very High Redshifts On Gamma-Ray Bursts at Very High Redshifts

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..312..118m&link_type=abstract

Third Rome Workshop on Gamma-Ray Bursts in the Afterglow Era ASP Conference Series, Volume 312, Proceedings of the conference he

Astronomy and Astrophysics

Astronomy

Scientific paper

Several independent studies suggest that an essential fraction (a few or a few tens of %) of the long gamma-ray bursts - collected in the BATSE Catalog - should be at very high redshifts; i.e. at z > 5. In this contribution, first, these studies are surveyed; then, second, it is shown by a statistical argument that the non-detection of the corresponding population of high-z afterglows should be an observational bias.

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