Astrokit -- an Efficient Program for High-Precision Differential CCD Photometry and Search for Variable Stars
Artem Y. Burdanov, Vadim V. Krushinsky, Alexander A. Popov

TL;DR
Astrokit is a software tool designed for high-precision differential CCD photometry, enabling efficient detection of variable stars and exoplanet transits in large astronomical datasets.
Contribution
The paper introduces Astrokit, a novel software that automates high-precision photometry and variable star detection using robust statistical methods, suitable for large-scale surveys.
Findings
Successfully applied to sky survey data in Cygnus
Detected low-amplitude variable stars and exoplanet transits
Achieved high-precision photometry for thousands of stars
Abstract
Having a need to perform differential photometry for tens of thousands stars in a several square degrees field, we developed Astrokit program. The software corrects the star brightness variations caused by variations of atmospheric transparency: to this end, the program selects for each star an individual ensemble of reference stars having similar magnitudes and positions in the frame. With ten or more reference stars in the ensemble, the differences between their spectral types and the spectral type of the object studied become unimportant. Astrokit searches for variable stars using Robust Median Statistics criterion, which allows candidate variables to be selected more efficiently than by analyzing the standard deviation of star magnitudes. The software allows very precise automatic analysis of long inhomogeneous sets of photometric observations of a large number of objects to be…
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