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Stellar Photometry by a Perfect CCD
Published online by Cambridge University Press: 07 August 2017
Extract
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.
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- Section II — Poster Papers
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- Copyright © Kluwer 1995