Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-23T21:09:39.941Z Has data issue: false hasContentIssue false

A Flexible Fast-Photometry System

Published online by Cambridge University Press:  25 April 2016

P. T. Rayner
Affiliation:
Department of Physics, University of Tasmania
R. D. Watson
Affiliation:
Department of Physics, University of Tasmania

Extract

A considerable amount of observational interest in short timescale phenomena has developed in optical astronomy in recent years. This interest has stemmed primarily from search efforts directed towards optical pulsars and the study of rapid fluctuations in cataclysmic variable and flare stars. Such studies have been made feasible by the development of the necessary photon pulse-counting technology required for rapid data sampling.

Type
Equipment
Copyright
Copyright © Astronomical Society of Australia 1974

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Beresford, I. R., Greenhill, J. G., Hamilton, P. A., and Watson, R. D., Nature, 241, 126 (1973).Google Scholar
Nather, R. E., Rev. Sci. Instrum. 43, 1012 (1972).CrossRefGoogle Scholar
Nather, R. E., and Warner, B., Mon. Not. R. Astron. Soc, 152, 209 (1971).CrossRefGoogle Scholar
Rayner, P. T., and Watson, R. D., Proc. Astron. Soc. Aust, 2, 5 (1974).Google Scholar
Rayner, P. T., and Watson, R. D., Proc. Astron. Soc. Aust., 2, 274 (1973).Google Scholar
Vaughan, A. E., Disney, M. J., and Nicholson, P., Mon. Not. R. Astron. Soc., (in press) (1974).Google Scholar