GLAST observation of high-redshift GRBs

Details GLAST observation of high-redshift GRBs GLAST observation of high-redshift GRBs

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..921..274b&link_type=abstract

THE FIRST GLAST SYMPOSIUM. AIP Conference Proceedings, Volume 921, pp. 274-276 (2007).

Mathematics

Logic

Gamma-Ray Sources, Gamma-Ray Bursts, Supernovae, Origin, Formation, Evolution, Age, And Star Formation, X- And Gamma-Ray Telescopes And Instrumentation

Scientific paper

We compare predicted Type Ib/c supernova (SNIb/c) rates with the observed long-duration Gamma-Ray-Burst (GRB) rates both locally and as a function of redshift, by assuming different star formation histories in galaxies of different morphological types. Due to the high star formation in spheroids at high redshift, we predict a large number of GRBs beyond z > 7. Moreover, based on our studies and on the current LAT performance, an estimate of the detection possibility of this burst population is presented.

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