UBV CCD standards near 5C1 radio sources at intermediate galactic latitude – I

dc.contributor.author	Mohan, V.
dc.contributor.author	Ojha, D. K.
dc.contributor.author	Bienayme, O.
dc.contributor.author	Paliwal, D. C.
dc.contributor.author	Pandey, A. K.
dc.contributor.author	Robin, A. C.
dc.contributor.author	Chareton, M.
dc.contributor.author	Bhatt, B. C.
dc.contributor.author	Sanwal, B. B.
dc.contributor.author	Oblak, E.
dc.contributor.author	Haywood, M.
dc.contributor.author	Creze, M.
dc.date.accessioned	2010-01-05T09:45:11Z
dc.date.available	2010-01-05T09:45:11Z
dc.date.issued	1994
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/405
dc.description.abstract	Using CCD observations photometric magnitudes have been obtained in 18 sub-fields in a direction at intermediate galactic latitude (l = 170°, b = 45°) in a 14 deg² area. B and V magnitudes have been obtained for a total of 214 stars out of which for 73 stars U magnitude also have been obtained. The magnitude range covered is 11< V <21 and 0.18< B – V < 1.85.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi22-403
dc.subject	CCD photometry – calibration – stellar populations	en_US
dc.title	UBV CCD standards near 5C1 radio sources at intermediate galactic latitude – I	en_US
dc.type	Article	en_US