Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-25T13:36:49.256Z Has data issue: false hasContentIssue false
  • English
  • Français

Photometric Properties of the Hubble Space Telescope Fine Guidance Sensors

Published online by Cambridge University Press:  12 April 2016

K. Zwintz ,
R. Kuschnig ,
W. W. Weiss  and
A. Witeschnik
K. Zwintz
Affiliation:
Institute for Astronomy, University of Vienna, Türkenschanzstrasse 17, A-1180 Vienna, Austria
R. Kuschnig
Affiliation:
Institute for Astronomy, University of Vienna, Türkenschanzstrasse 17, A-1180 Vienna, Austria
W. W. Weiss
Affiliation:
Institute for Astronomy, University of Vienna, Türkenschanzstrasse 17, A-1180 Vienna, Austria
A. Witeschnik
Affiliation:
Institute for Astronomy, University of Vienna, Türkenschanzstrasse 17, A-1180 Vienna, Austria

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.

To reach lower noise levels with the Hubble Space Telescope Fine Guidance Sensors (FGS) the photometric properties as well as the systematic effects affecting the data have been investigated.

Type
Part 1. Large Scale Surveys: Present and Future
Information
International Astronomical Union Colloquium , Volume 176: The Impact of Large-Scale Surveys on Pulsating Star Research , 2000 , pp. 82
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Weiss, W.W., Zwintz, K., Kuschnig, R., & Witeschnik, A. 1999, Comm. Ast. No. 129 Google Scholar
Zwintz, K., Kuschnig, R., Weiss, W.W., Gray, R.O., & Jenkner, H. 1999, A&A, 343, 899 Google Scholar