The Reduction of CCD Images for Stellar Photometry on the Vatt

The Reduction of CCD Images for Stellar Photometry on the Vatt

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...

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Bibliographic Details
Main Authors: Janusz R., Boyle R. P., Philip A. G. Davis
Format: Article
Language:English
Published: De Gruyter 2003-12-01
Series:Open Astronomy
Subjects:
techniques
photometric
ccd photometry
reductions
Online Access:https://doi.org/10.1515/astro-2017-0068
Description
Summary: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.
ISSN:2543-6376

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