Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-27T04:52:59.687Z Has data issue: false hasContentIssue false
  • English
  • Français

Photometry from Space

Published online by Cambridge University Press:  12 April 2016

R.C. Bless  and
M. Taylor
R.C. Bless
Affiliation:
Astronomy Department, University of Wisconsin-Madison, U.S.A.
M. Taylor
Affiliation:
Astronomy Department, University of Wisconsin-Madison, U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

After a brief review of the traditional opportunities as well as the problems of doing photometry from space vehicles over a wide variety of wavelength regimes, several topics will be discussed. These include the factors associated with various types of spacecraft orbits (for example, near-earth, geosynchronous, planetary cruise) and with the different kinds of vehicles and platforms used (expendable, shuttle attached payloads, permanent stations, multi-purpose spacecraft, small and large projects). Since ground-based capabilities are constantly improving and expanding, it is necessary to assess those that might compete with space-based photometry. Finally, the present state of space observations as they pertain to “classical,” high precision, high speed and multi-object photometry will be reviewed; possibilities for the future will be addressed briefly.

Type
Session 7 Photometry from Space
Information
International Astronomical Union Colloquium , Volume 136: Stellar Photometry – Current Techniques and Future Developments , 1993 , pp. 336 - 345
Copyright
Copyright © C.J. Butler and I. Elliottt 1993

References

Boggess, A., Wilson, R., Barker, P.J., Meredith, L.M., 1987, in: Specific Accomplishments of the IUE, ed. Kondo, Y., p 3.Google Scholar
Bromage, G.E., 1992, these proceedings.Google Scholar
Clarke, J.T., Burrows, C., Crisp, D., Gallagher, J.S., Griffiths, R.E., Hester, J.J., Hoessel, J.G., Holtzman, J.A., Mould, J.R., Trauger, J.T., Westphal, J.A., 1992, White Paper for WF/PC 2 Far-Ultraviolet Science.Google Scholar
Code, A.D., Holm, A.V., Bottemiller, R.L., 1980, Astrohpys. J. 43, 501.Google Scholar
Dravins, D., Lindegren, L., Mezey, E., 1992, these proceedings.Google Scholar
Glass, I.S., 1992, these proceedings.Google Scholar
Großmann, V., 1992, these proceedings.Google Scholar
Harper, D.A., 1991, private communication.Google Scholar
Joyce, R.R., 1992 in: Astronomical CCD Observing and Reduction Techniques, ed. Howell, S., Astr. Soc. of Pacific Conf. Series 23, p 258.Google Scholar
McCammon, D., Juda, M., Zhang, J., Holt, S.S., Kelley, R.L., Moseley, S.H., Szymkowiak, A.E., 1987, Japanese Journal of Applied Physics 26, 2084.Google Scholar
Shearer, A., Redfern, R., Wouts, R., O’Kane, P., O’Byrne, C., Jordan, B.D., 1992, these proceedings.Google Scholar
Thompson, R., 1992, private communication.Google Scholar
Warner, B. 1988, in: High speed astronomical photometry, Cambridge University Press, Cambridge, p. 15.Google Scholar
Wesselius, P.R., van Duinen, R.J., Aalders, J.W.G., Kester, D., 1980, Astron. Astrophys. 85, 221.Google Scholar