BVRI photometry of the Dipper Asterism region in M 67

dc.contributor.author	Anupama, G. C
dc.contributor.author	Kembhavi, A. K
dc.contributor.author	Prabhu, T. P
dc.contributor.author	Singh, K. P
dc.contributor.author	Bhat, P. N
dc.date.accessioned	2008-07-16T06:12:42Z
dc.date.available	2008-07-16T06:12:42Z
dc.date.issued	1995-02
dc.identifier.citation	Astronomy and Astrophysics Supplement Series, Vol. 103, No. 2, pp. 315 - 320	en
dc.identifier.issn	0365-0138
dc.identifier.uri	http://hdl.handle.net/2248/2701
dc.description.abstract	We 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.extent	657737 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	European Southern Observatory	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1994A%26AS..103..315A	en
dc.subject	Cluster:open	en
dc.subject	Cluster:M 67	en
dc.subject	CCD Photometry	en
dc.subject	Photometric calibration	en
dc.title	BVRI photometry of the Dipper Asterism region in M 67	en
dc.type	Article	en