Variability/Luminosity for the X-ray emission of long GRB as seen by the Wide Field Cameras on BeppoSAX

Details Variability/Luminosity for the X-ray emission of long GRB as seen by the Wide Field Cameras on BeppoSAX Variability/Luminosity for the X-ray emission of long GRB as seen by the Wide Field Cameras on BeppoSAX

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..312..142v&link_type=abstract

Third Rome Workshop on Gamma-Ray Bursts in the Afterglow Era ASP Conference Series, Volume 312, Proceedings of the conference he

Astronomy and Astrophysics

Astronomy

Scientific paper

Bursts that show maximum or exclusive emission in the X-ray may hide object at very high redshift. Measuring the redshift of bursts without optical counterparts would lead to a better comprehension of the nature and evolution of GRBs and probe the universe at high redshift. Previous studies have shown the existence of a relation between the complexity of the GRBs lightcurves and the Peak Luminosity in the gamma ray energy range. Here we define Variability in the X-ray energy range and we measure it using the BeppoSAX Wide Field Cameras data. We find a relation between the Variability in the energy range 2-26keV and the intrinsic peak luminosity of the bursts.

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