Analysis of isoplanatic high resolution stellar fields by the StarFinder code
Analysis of isoplanatic high resolution stellar fields by the StarFinder code
We describe a new code for the deep analysis of stellar fields, designed for Adaptive Optics (AO) Nyquist-sampled images with high and low Strehl ratio. The Point Spread Function (PSF) is extracted directly from the image frame, to take into account the actual structure of the instrumental response and the …