Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2528
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dc.contributor.authorMayya, Y. D-
dc.date.accessioned2008-06-27T10:02:20Z-
dc.date.available2008-06-27T10:02:20Z-
dc.date.issued1991-12-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 12, No. 4, pp. 319 - 331en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/2528-
dc.description.abstractCalibration of the CCD camera of the 1-m telescope at the Vainu Bappu Observatory, Kavalur, to the BVR system is reported here based on the observations of stars in the 'dipper asterism' in the open cluster M 67 (NGC 2682). Transformations involving B and V have negligible color terms, while those involving R are slightly color dependent. The possibility of using scaled-down R band fluxes to estimate the continuum flux at H-alpha is investigated by comparing the counts in R band with those through an interference filter center at H-alpha. The scaling factor is found to remain constant over a wide range of colors. The sensitivity of the telescope-filter-CCD combination is estimated to be 2.0 percent, 8.3 percent and 9.7 percent in B, V and R bands, respectively. The star F117 appears to be a small-amplitude (about 0.05 mag) variableen
dc.format.extent1093216 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/1991JApA...12..319Men
dc.subjectAstronomical Photometryen
dc.subjectAtmospheric Effectsen
dc.subjectCharge Coupled Devicesen
dc.subjectInstrument Compensationen
dc.subjectOpen Clustersen
dc.subjectAstronomical Observatoriesen
dc.subjectH Alpha Lineen
dc.subjectMultispectral Band Camerasen
dc.subjectTelescopesen
dc.titlePhotometric calibration of the CCD camera of 1-m telescope at VBOen
dc.typeArticleen
Appears in Collections:IIAP Publications

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