We refer the reader to Bertin and Arnouts (1996) for a detailed description of SExtractor software. Here we wish to focus on the determination of the best extraction parameters, based on the image quality and noise characteristic of our image data sample.
SExtractor gives the possibility of filtering images with a kernel so that the noise is decreased and the S/N increased: this kernel is chosen in such a way that it reproduces the PSF of the stars in the field. For the OACDF extraction, our choice has been for a Gaussian kernel, whose FWHM properly matches the seeing on the images. Detection is performed on the filtered image. The detection threshold was determined as the best compromise between limiting magnitude and percentage of spurious detection.