The Reduction of CCD Images for Stellar Photometry on the Vatt
Janusz R., Boyle R. P., Philip A. G. Davis
Open Astronomy · 2003
doi:10.1515/astro-2017-0068 (opens in a new tab)
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Abstract
We briefly describe a method of organizing all the star field exposures taken in a complete CCD observational run. By a “CommandLog” (to be published in J. Astron. Data) one can organize all the observations and process them within IRAF in an orderly, automated manner to arrive at stellar photometry calibrated into a standard photometric system (in our case, Strömvil). During the course of this processing we determine the error of the flat and try to correct it.
Abstract licence: CC BY
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