Gamma-Ray Bursts and their Host Environments

Details Gamma-Ray Bursts and their Host Environments Gamma-Ray Bursts and their Host Environments

Feb 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000noao.prop..406r&link_type=abstract

NOAO Proposal ID #2000A-0406

Computer Science

Scientific paper

We propose rapid near-infrared K' and J band followup observations of four gamma ray bursts from each hemisphere during the spring 2000 semester. These observations will help answer several open questions about GRBs and their afterglows: (1) Can present afterglow models stand up to detailed comparison with high precision spectral slopes and light curves measurements? (2) Are ``dark'' GRBs without detected optical afterglows a consequence of dust absorption in the GRB environment? (3) Are observed breaks in GRB light curves truly wavelength-independent, as predicted under models of beamed burst afterglows?

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