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Optical follow up of the GRB 990123 sources from UPSO, Naini Tal

dc.contributor.authorSagar, R
dc.contributor.authorPandey, A K
dc.contributor.authorMohan, V
dc.contributor.authorYadav, R K S
dc.contributor.authorNilakshi
dc.contributor.authorBhattacharya, D
dc.contributor.authorCastro-Tirado, A J
dc.date.accessioned2006-06-09T06:46:29Z
dc.date.available2006-06-09T06:46:29Z
dc.date.issued1999
dc.description.abstractThe CCD magnitudes in Johnson $BV$ and Cousins R photometric passbands are determined for the optical transient of GRB 990123. These observations have been taken approximately 12 hours after trigger of the gamma-ray burst. BVR photometric light curves are obtained by combining the published data with the present measurements. They indicate that the flux decay constants in BV and R passbands are almost the same. Its value is $1.1\pm 0.06$. Such decay is quite consistent with the fireball models for the optical transient.en
dc.format.extent393064 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationBulletin of the Astronomical Society of India, 1999, Vol.27, p3-7en
dc.identifier.issn0304-9523
dc.identifier.urihttp://hdl.handle.net/2289/1336
dc.language.isoenen
dc.publisherThe Astronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1999BASI...27....3Sen
dc.rights(1999) by the Astronomical Society of India. Scanned images provided by the NASA ADS Data System.en
dc.titleOptical follow up of the GRB 990123 sources from UPSO, Naini Talen
dc.typeArticleen

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