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The report presents the application of the Mathematical Microscope (MM) in the analysis of point objects in astronomy from telescopes in different ranges. Main Purpose of MM (MPMM): We have a high-precision discrete image Y|A and a set of discrete reversible Antenna Pattern (AP) or Apparatus Functions (AF) {O}. It is required to find a solution to the set of systems of equations Y|A = {O} X. Note that we do not know the AP or AF A=ARGB = [AR, AG, AB], and the parametric set of discrete reversible AF {O} is our idea of how the unknown AF A is arranged in the data of discrete measurements Y|A. The solution Y|A = {O} X can be found in the following Physical Fundamental Assumption (PFA): there are separate point objects (stars) in Super-Resolved (SR) X.