GRBs with optical afterglow and known redshift: a statistical study

Details GRBs with optical afterglow and known redshift: a statistical study GRBs with optical afterglow and known redshift: a statistical study

2007-01-10

arxiv.org/abs/astro-ph/0701306v1

Nuovo Cim.B121:1487-1488,2006

Astronomy and Astrophysics

Astrophysics

To be published in the proceedings of the conference "SWIFT and GRBs: Unveiling the Relativistic Universe", Venice, June 5-9,

Scientific paper

10.1393/ncb/i2007-10289-6

We present a correlation between two intrinsic parameters of GRB optical afterglows. These are the isotropic luminosity at the maximum of the light curve (Lpeak) and the time-integrated isotropic energy (Eiso) radiated after the observed maximum. We test the correlation between the logarithms of (Eiso) and (Lpeak) and finally we value the effect of the different samples of GRBs in according with the first optical observation reduced to proper time.

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