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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4939
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dc.contributor.authorSethi, S.K.-
dc.contributor.authorBhargavi, S.G.-
dc.contributor.authorGreiner, Greiner-
dc.date.accessioned2012-07-14T10:45:18Z-
dc.date.available2012-07-14T10:45:18Z-
dc.date.issued2000-
dc.identifier.citationAIP Conference Proceedings, 2000, Vol.526, p107-111en
dc.identifier.urihttp://hdl.handle.net/2289/4939-
dc.descriptionRestricted Accessen
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.urihttp://adsabs.harvard.edu/abs/2000AIPC..526..107Sen
dc.relation.urihttp://arxiv.org/abs/astro-ph/0001006en
dc.relation.urihttp://dx.doi.org/10.1063/1.1361517en
dc.rights2000 by the American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics.en
dc.subjectgamma-ray sourcesen
dc.subjectgamma-ray burstsen
dc.subjectCosmic raysen
dc.subjectObservational cosmologyen
dc.titleOn the clustering of GRBs on the skyen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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