Add to ORKGThe 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
International audienceAims. Long gamma-ray bursts (LGRBs) have been shown to be powerful probes of t...
Gamma-ray bursts (GRBs) and galaxies at high redshift represent complementary probes of the star for...
We use the BD2 sample of gamma-ray bursts (GRBs) based on 5.9 years of BATSE DISCLA data with a vari...
Theisotropic Luminosity Function (LF) and Formation Rate History (FRH) of long GRBs is by the first ...
International audienceWe derive, adopting a direct method, the luminosity function and the formation...
We study the luminosity function (LF), the comoving rate and the detection rate of long gamma-ray bu...
We attempt to constrain the luminosity function of Gamma Ray Bursts (GRBs) from the observed number...
Using 220 Gamma-Ray Burst (GRB) redshifts and luminosities derived from the luminosity-variability c...
Using the luminosity function and apparent GRB rate inferred from the spectral peak energy-luminosit...
We rederive the short GRBs luminosity function using the BATSE peak flux distribution and compare th...
Wee stimatetheluminosit y evolution and formation ratefor over a 900 BATSE GRBs by using redshift an...
The realization that the total energy of GRBs is correlated with their jet break angles motivates th...
We compute the luminosity function (LF) and the formation rate of long gamma ray bursts (GRBs) by fi...
The contemporary discoveries of galaxies and gamma ray bursts (GRBs) at high redshift have supplied ...
The cosmic formation rate of long Gamma Ray Bursts (LGRBs) encodes the evolution, across cosmic time...
International audienceAims. Long gamma-ray bursts (LGRBs) have been shown to be powerful probes of t...
Gamma-ray bursts (GRBs) and galaxies at high redshift represent complementary probes of the star for...
We use the BD2 sample of gamma-ray bursts (GRBs) based on 5.9 years of BATSE DISCLA data with a vari...
Theisotropic Luminosity Function (LF) and Formation Rate History (FRH) of long GRBs is by the first ...
International audienceWe derive, adopting a direct method, the luminosity function and the formation...
We study the luminosity function (LF), the comoving rate and the detection rate of long gamma-ray bu...
We attempt to constrain the luminosity function of Gamma Ray Bursts (GRBs) from the observed number...
Using 220 Gamma-Ray Burst (GRB) redshifts and luminosities derived from the luminosity-variability c...
Using the luminosity function and apparent GRB rate inferred from the spectral peak energy-luminosit...
We rederive the short GRBs luminosity function using the BATSE peak flux distribution and compare th...
Wee stimatetheluminosit y evolution and formation ratefor over a 900 BATSE GRBs by using redshift an...
The realization that the total energy of GRBs is correlated with their jet break angles motivates th...
We compute the luminosity function (LF) and the formation rate of long gamma ray bursts (GRBs) by fi...
The contemporary discoveries of galaxies and gamma ray bursts (GRBs) at high redshift have supplied ...
The cosmic formation rate of long Gamma Ray Bursts (LGRBs) encodes the evolution, across cosmic time...
International audienceAims. Long gamma-ray bursts (LGRBs) have been shown to be powerful probes of t...
Gamma-ray bursts (GRBs) and galaxies at high redshift represent complementary probes of the star for...
We use the BD2 sample of gamma-ray bursts (GRBs) based on 5.9 years of BATSE DISCLA data with a vari...