Powehi Black Hole Images Super Resolution Problems

摘要

The problem of Super-Resolution begins with evaluating the working discrete model of the Apparatus Function (AF) of the device or the Antenna Pattern (AP) of the telescope. With the evaluation of such AFs, APs, we associate the mathematical problem of the apodization choice of a reversible discrete AF, AP Os with the minimum norm Nor (R)=||R||, R=O-1. On the images of the Black Hole (BH) of Powehi, the presence of point objects allowed us to evaluate three versions of the APs for a complex of 8 telescopes and realize the corresponding Super-Resolutions according to these versions of the APs.