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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4659
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dc.contributor.authorSethi, S. K-
dc.contributor.authorBhargavi, S. G-
dc.contributor.authorGreiner, J-
dc.date.accessioned2009-07-21T15:51:55Z-
dc.date.available2009-07-21T15:51:55Z-
dc.date.issued2000-09-
dc.identifier.citationR. Marc Kippen., Robert S. Mallozzi and Gerald J. Fishman., eds., Gamma-Ray Bursts: 5th Huntsville Symposium., AIP Conference Proceedings, Vol. 526, held in Huntsville, AL, October 18 - 22, 1999. pp. 107 - 111en
dc.identifier.isbn978-1563969478-
dc.identifier.urihttp://hdl.handle.net/2248/4659-
dc.description.abstractThe two-point correlation of the 4th (current) BATSE catalog (2494 objects) is calculated. It is shown to be consistent with zero at nearly all angular scales of interest. Assuming that GRBs trace the large scale structure in the universe we calculate the angular correlation function for the standard CDM (sCDM) model. It is shown to be <=10-4 at θ~=5° if the BATSE catalog is assumed to be a volume-limited sample up to z~=1. Combined with the error analysis on the BATSE catalog this suggests that nearly 105 GRBs will be needed to make a positive detection of the two-point angular correlation function at this angular scale.en
dc.language.isoenen
dc.publisherAmerican Institute of Physicsen
dc.relation.ispartofseriesAIP Conference Proceedings; Vol. 526-
dc.relation.urihttp://dx.doi.org/10.1063/1.1361517en
dc.relation.urihttp://arxiv.org/abs/astro-ph/0001006en
dc.rights© American Institute of Physicsen
dc.subjectGamma-Ray Sources (Astronomical)en
dc.subjectCosmic Ray Energy Spectraen
dc.subjectAstrophysical Radiation Mechanismsen
dc.subjectSky Brightnessen
dc.subjectCluster Emission Modelen
dc.subjectCosmologyen
dc.subjectRed Shiften
dc.subjectIntergalactic Matteren
dc.titleOn the clustering of GRBs on the skyen
dc.typeArticleen
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