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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2701
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dc.contributor.authorAnupama, G. C-
dc.contributor.authorKembhavi, A. K-
dc.contributor.authorPrabhu, T. P-
dc.contributor.authorSingh, K. P-
dc.contributor.authorBhat, P. N-
dc.date.accessioned2008-07-16T06:12:42Z-
dc.date.available2008-07-16T06:12:42Z-
dc.date.issued1995-02-
dc.identifier.citationAstronomy and Astrophysics Supplement Series, Vol. 103, No. 2, pp. 315 - 320en
dc.identifier.issn0365-0138-
dc.identifier.urihttp://hdl.handle.net/2248/2701-
dc.description.abstractWe present Cousins BVRI magnitudes for stars in the M 67 `dipper asterism' region, based on observations carried out at the prime focus of the 2.3 m Vainu Bappu Telescope of the Vainu Bappu Observatory, Kavalur. The photometric system is calibrated using the photometric standards in the field and linear transformation relations are derived. Photometric results are reported for 37 stars in BVRI bands. Results are also presented for an additional set of 35 stars in only two or three of these bands. The photometric accuracy is better than 3% for magnitudes B<16, V,R<17 and I<14, and is slightly poorer for the results presented beyond this limit.en
dc.format.extent657737 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherEuropean Southern Observatoryen
dc.relation.urihttp://adsabs.harvard.edu/abs/1994A%26AS..103..315Aen
dc.subjectCluster:openen
dc.subjectCluster:M 67en
dc.subjectCCD Photometryen
dc.subjectPhotometric calibrationen
dc.titleBVRI photometry of the Dipper Asterism region in M 67en
dc.typeArticleen
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