Redshift and spatial distribution of the intermediate gamma-ray bursts

Details Redshift and spatial distribution of the intermediate gamma-ray bursts Redshift and spatial distribution of the intermediate gamma-ray bursts

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aipc.1358..235h&link_type=abstract

GAMMA RAY BURSTS 2010. AIP Conference Proceedings, Volume 1358, pp. 235-238 (2011).

Physics

Redshift, Gamma-Rays, Data Acquisition, Explosions, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies, Gamma-Ray, Data Acquisition: Hardware And Software, Energetic Particles

Scientific paper

One of the most important task of the Gamma-Ray Burst field is the calssification of the bursts. Many researches have proven the existence of the third kind (intermediate duration) of GRBs in the BATSE data. Recent works have analyzed BeppoSax and Swift observations and can also identify three types of GRBs in the data sets. However, the class memberships are probabilistic we have enough observed redshifts to calculate the redshift and spatial distribution of the intermediate GRBs. They are significantly farther than the short bursts and seems to be closer than the long ones.

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