The Semi-Automatic Variability Search Pipeline (SAVS.PL) is the easy-to-use software which was created for semi-automatic reduction and analysis of a big amount of sky CCD images and detecting new variable stars.

For more information about the software see section Software Pipeline. If you find it interesting and useful, you can download the newest version from there. In the package the exemplary CCD images and user's manual with a tutorial are included.