Hostname: page-component-cd9895bd7-hc48f Total loading time: 0 Render date: 2024-12-23T18:03:46.609Z Has data issue: false hasContentIssue false
  • English
  • Français

Stellar Photometry by a Perfect CCD

Published online by Cambridge University Press:  07 August 2017

Bjarne Thomsen  and
Frank Grundahl Jensen
Bjarne Thomsen
Affiliation:
Institute of Physics and Astronomy, Aarhus University
Frank Grundahl Jensen
Affiliation:
Institute of Physics and Astronomy, Aarhus University

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
Symposium - International Astronomical Union , Volume 167: New Developments in Array Technology and Applications , 1995 , pp. 369 - 370
Copyright
Copyright © Kluwer 1995 

References

Bergbush, P. and VandenBerg, D. A. 1992 ApJS 81, 163.Google Scholar
Janes, K. A. and Heasley, J. N. 1993 PASP 105, 527.Google Scholar
Parker, J. Wm. 1991 PASP 103, 243.Google Scholar
Schechter, P. L., Mateo, M. and Saha, A. 1993 PASP 105, 1342.Google Scholar
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
Stetson, P. B. 1994 PASP 106, 250.Google Scholar
Thomsen, B. and Frandsen, S. 1983 AJ 88, 789.Google Scholar