Photometry with the ASTAP program

A demonstration how to do photometry with ASTAP. The images are calibrated with darks, flats and flat-darks, the green channel is extracted, the image are astrometric solved, the magnitude of variable star AD CMi is measured against the Gaia EDR3 database and the result is presented in a spreadsheet and an AAVSO extended report is generated. Website http://www.hnsky.org/