CCD Measurements of Visual Double Stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

The CCD-imaging equipment that many amateur astronomers use for astrophotography and photometry can also be used to measure the separation, position angle, and magnitude difference of visual double stars. There are a few imaging and data analysis procedures that are unique to this project. I describe a simple PSF-model that provides good accuracy and repeatability in measurements of pairs which -- due to their close spacing and/or large magnitude difference -- would be beyond the reach of standard astrometric software. This project has some conceptual similarities to asteroid lightcurve determination: in both cases, we are presented with a huge number of potential targets that need observation; repeated observation at different epochs adds value to the initial observations; there are very few professional astronomers pursuing these studies; and there exists a Journal devoted to publication of these observations so that they will be available to the professional community. Hence, double star measurement may be a fruitful area for amateur contributions.

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