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Article overview
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The Luminosity Function and Formation Rate History of GRBs | C. Firmani
; V. Avila-Reese
; G. Ghisellini
; A.V. Tutukov ;
; | Date: |
19 Apr 2005 | Subject: | astro-ph | Affiliation: | 1,2), V. Avila-Reese , G. Ghisellini , A.V. Tutukov ; ( Osserv. Astron. di Brera, Italy; Instituto de Astronomia, U.N.A.M., Mexico; Institute of Astronomy Moscow, Russia | Abstract: | The isotropic luminosity function (LF) and formation rate history (FRH) of long GRBs is by the first time constrained by using jointly both the observed GRB peak-flux and redshift distributions. Our results support an evolving LF and a FRH that keeps increasing after z=2. We discuss some interesting implications related to these results. | Source: | arXiv, astro-ph/0504417 | Services: | Forum | Review | PDF | Favorites |
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