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2004ApJ...613..484B - Astrophys. J., 613, 484-491 (2004/September-3)

Gamma-ray burst intensity distributions.

BAND D.L., NORRIS J.P. and BONNELL J.T.

Abstract (from CDS):

We use the lag-luminosity relation to calculate self-consistently the redshifts, apparent peak bolometric luminosities LB, and isotropic energies Eisofor a large sample of BATSE gamma-ray bursts. We consider two different forms of the lag-luminosity relation; for both forms the median redshift for our burst database is 1.6. We model the resulting Eisosample with power-law and Gaussian probability distributions without redshift evolution, both of which are reasonable models. The power-law model has an index of αE=1.76±0.05 (95% confidence), where p(Eiso)∝E–αEiso. The simple universal jet profile model suggested but did not require αE=2, and subsequent physically reasonable refinements to this model permit greater diversity in αE, as well as deviations from a power law; therefore, our observed Eisoprobability distribution does not disprove the universal jet model.

Abstract Copyright:

Journal keyword(s): Gamma Rays: Bursts

Simbad objects: 1

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