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CCD Time-Series Photometry of Astronomical Sources
Published online by Cambridge University Press: 07 August 2017
Abstract
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CCDs are essentially the only instrument available today for photometry at most observatories; they are also becoming more readily available to amateurs as well. Thus, obtaining good photometric data with these two-dimensional devices is something we all need to understand. The history of and recent developments in CCD time-series photometry will be reviewed with some comments on future directions.
- Type
- Section I — Review Papers
- Information
- Copyright
- Copyright © Kluwer 1995
References
Granados, A. and Borucki, W.
1994 in Proceedings of the First FRESIP Workshop, Granados, A. and Borucki, W., eds., NASA Conference Publication 10148.Google Scholar
Howell, S. B.
1992 in Astronomical CCD Observing and Reduction Techniques, Howell, S. B., ed., ASP Conference Series, Vol. 23.Google Scholar
Kreidl, T. J.
1993 in IAU Colloquium No. 136, Stellar Photometry — Current Techniques and Future Developments, Butler, C. J. and Elliott, I., eds., Cambridge University Press, Cambridge, p. 311.Google Scholar
Miller, H. R., Noble, J. C., Carini, M. T., Urry, C. M., Sokoloski, J. and Howell, S. B.
1992 in Testing the AGN Paradigm, AIP Conf. Proceedings No. 254, Holt, S. S., Neff, S. G. and Urrey, C. M., eds., AIP, New York.Google Scholar