Calculate various image quality statistics based on an input
catalogue _CALCULATE_IMAGE_STATISTICS_
This primitive calculates the mean axial ratio of bright sources, the average object diameter converted to K-band equivalent, the sky brightness, the limiting magnitude, and the instrumental zero point.
Files results with the Calibration system. FWHM is obtained with the fwhm() method, axial ratio is obtained with the axial_ratio() method, sky brightness is obtained with the sky_brightness() method, limiting magnitude is obtained with the limiting_mag() method, and the zero point is obtained with the zeropoint() method.