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Paper detail

Cosmology with Gamma-Ray Bursts Using k-correction

In the case of Gamma-Ray Bursts with measured redshift, we can calculate the k-correction to get the fluence and energy that were actually produced in the comoving system of the GRB. To achieve this we have to use well-fitted parameters of a GRB spectrum, available in the GCN database. The output of the calculations is the comoving isotropic energy E_iso, but this is not the endpoint: this data can be useful for estimating the ΩM parameter of the Universe and for making a GRB Hubble diagram using Amati's relation.

preprint2012arXivOpen access
Andras KovacsZsolt BagolyLajos G. BalazsIstvan HorvathPeter Veres
astro-ph.HE
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Andras KovacsZsolt BagolyLajos G. BalazsIstvan HorvathPeter Veres

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