Detectability of Long GRB Afterglows From Very High Redshifts

Details Detectability of Long GRB Afterglows From Very High Redshifts Detectability of Long GRB Afterglows From Very High Redshifts

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..727..518g&link_type=abstract

GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP Conference Proceedings, Volume 727, pp. 518-521 (2004).

Physics

4

Gamma-Ray Sources, Gamma-Ray Bursts, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies, Ground-Based Ultraviolet, Optical And Infrared Telescopes

Scientific paper

Detectability of high redshift GRB afterglows are carefully discussed. Using standard assumptions, we find that Chandra, XMM and Swift XRT can potentially detect GRBs in the X-ray band out to very high redshifts z>~ 30. In the K and M bands, the JWST and ground-based telescopes are potentially able to detect GRBs even one day after the trigger out to z ~ 16 and 33.

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