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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1969
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dc.contributor.authorNilakshi-
dc.contributor.authorYadav, R. K. S-
dc.contributor.authorMohan, V-
dc.contributor.authorPandey, A. K-
dc.contributor.authorSagar, R-
dc.date.accessioned2007-11-15T10:18:56Z-
dc.date.available2007-11-15T10:18:56Z-
dc.date.issued1999-
dc.identifier.citationBASI, Vol. 27, No. 3, pp. 405 - 410en
dc.identifier.urihttp://hdl.handle.net/2248/1969-
dc.description.abstractThe CCD magnitudes in Johnson BV and Cousins RI photometric passbands are determined for 18 stars in the field of GRB 990123. These mesurements can be used in carrying out precise CCD photometry of the optical transient of GRB 990123 using differential photometric techniques during non-photometric sky conditions. A comparison with previous photometry indicates that the present photometry is more precise.en
dc.format.extent410002 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1999BASI...27..405Nen
dc.subjectPhotometryen
dc.subjectGRBen
dc.titleBVRI CCD photometric standards in the field of GRB 990123en
dc.typeArticleen
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