No CrossRef data available.
Article contents
Stellar Photometry by a Perfect CCD
Published online by Cambridge University Press: 07 August 2017
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 developed algorithms for the construction of a simulated globular cluster, as it would appear on a frame obtained with a perfect CCD. This has allowed us to compare the absolute errors in the photometry of two different programs, DAOPHOT II (Stetson 1991, 1994) and SPS (Janes and Heasley 1993), with a special emphasis on criteria for selecting stars with the best photometry.
- Type
- Section II — Poster Papers
- Information
- Copyright
- Copyright © Kluwer 1995
References
Stetson, P. B.
1991 in Proceedings of the 3rd ESO/ST-ECF Data Analysis Workshop, Grosbol, P. J. and Warmels, R. H., eds., ESO, Garching, p. 187.Google Scholar