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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2719
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dc.contributor.authorBhargavi, S. G-
dc.date.accessioned2008-07-17T06:59:28Z-
dc.date.available2008-07-17T06:59:28Z-
dc.date.issued2002-06-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 23, No. 1- 2, pp. 123 - 127en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/2719-
dc.description.abstractThis talk focuses on the various aspects we learnt from multiband observations of GRBs both, before and during the afterglow era. A statistical analysis to estimate the probable redshifts of host galaxies using the luminosity function of GRBs compatible with both the afterglow redshift data as well as the overall population of GRBs is discussed. We then address the question whether the observed fields of GRBs with precise localizations from third Inter-Planetary Network (IPN3) contain suitable candidates for their host galaxies.en
dc.format.extent45841 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://www.ias.ac.in/jaa/marjun2002/absmarjun.htm#Jaa289en
dc.subjectGamma rays: burstsen
dc.subjectCCD: observationsen
dc.subjectMethods: statisticalen
dc.titleMulti-band Observations of Gamma Ray Burstsen
dc.typeArticleen
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