UBV CCD standards in two galaactic directions – II

dc.contributor.author	Mohan, V.
dc.contributor.author	Sanwal, B. B.
dc.contributor.author	Paliwal, D. C.
dc.contributor.author	Pandey, A. K.
dc.contributor.author	Bhatt, B. C.
dc.contributor.author	Robin, A. C.
dc.date.accessioned	2009-12-17T09:11:37Z
dc.date.available	2009-12-17T09:11:37Z
dc.date.issued	1996
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/382
dc.description.abstract	Using CCD observations, photometric magnitudes have been obtained in two galactic directions at intermediate latitude. A total of 7 sub-fields in one direction (l = 3°, b = 47°) have been observed leading to photometric magnitudes for 52 stars. In the second direction (l = 278°, b = 47°) a total of 10 sub-fields have been observed yielding photometric magnitudes for 139 stars. The magnitude range covered is 13< V < 19.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi24-7
dc.subject	CCD photometry, Calibration, Star counts	en_US
dc.title	UBV CCD standards in two galaactic directions – II	en_US
dc.type	Article	en_US