Hostname: page-component-8448b6f56d-dnltx Total loading time: 0 Render date: 2024-04-25T03:50:27.026Z Has data issue: false hasContentIssue false
  • English
  • Français

Applications of a Realistic Model for CCD Imaging

Published online by Cambridge University Press:  07 August 2017

Steve B. Howell  and
William J. Merline
Steve B. Howell
Affiliation:
Planetary Science Institute
William J. Merline
Affiliation:
Planetary Science Institute

Extract

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.

We have constructed a computer model for simulation of point sources imaged on CCDs. An attempt has been made to ensure that the model produces “data” that mimic real data taken with two-D detectors. To be realistic, such simulations must include randomly generated noise of the appropriate type from all sources. The synthetic data are output as simple one-D integrations, as two-D radial slices, and as three-D intensity plots. Each noise source can be turned on or off so they can be studied independently as well as in combination to provide insight into the image components.

Type
Section II — Poster Papers
Information
Symposium - International Astronomical Union , Volume 167: New Developments in Array Technology and Applications , 1995 , pp. 371 - 372
Copyright
Copyright © Kluwer 1995 

References

Howell, S. B. 1995, in Proc. IAU Symposium No. 167, New Developments in Array Technology and Applications, Philip, A. G. D., Janes, K. A. and Upgren, A. R., eds., Kluwer Academic Pub., p. 167.Google Scholar
Merline, W. J. and Howell, S. B. 1992 in Astronomical Data Analysis Software and Systems I, Worrall, D., Biemesderfer, C., and Barnes, J., eds., ASP Conf. Series, Vol 25, San Francisco, p. 316.Google Scholar
Merline, W. J. and Howell, S. B. 1995 Experimental Astronomy, in press.Google Scholar