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Further Progress in CCD Photometry

Published online by Cambridge University Press:  12 April 2016

Peter B. Stetson
Peter B. Stetson*
Affiliation:
Dominion Astrophysical Observatory, Canada

Abstract

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I comment on some of the steps required to convert raw instrumental magnitudes, derived by profile-fitting or synthetic-aperture photometry from CCD images, to final calibrated photometry on a standard system. The status of the DAO program to obtain homogeneous BV photometry for star clusters and nearby galaxies will also be discussed.

Information

Type
Session 6 Photometry with CCDs
Information
International Astronomical Union Colloquium , Volume 136: Stellar Photometry – Current Techniques and Future Developments , 1993, pp. 291 - 303
Copyright
Copyright © C.J. Butler and I. Elliottt 1993

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