Effective area versus photon incidence angle to relative the longitudinal telescope axis (squares - no constraints on the angle a, triangles - a<0.5⁰, spectral index g=2). 

Angular resolution versus photon energy for normal incidence. Green and blue curves- CYGAM telescope (squares - no constraints on the angle a, triangles - a<0,5⁰); red curve - EGRET telescope. 

Angular resolution for normal to the axis X incidence versus source power law spectrum index (squares- no constraints on the angle a, triangles- a<0,5 ⁰). 

Angular resolution versus photon incidence angle relative to the longitudinal telescope axis (squares - no constraints on the angle a, triangles - a<0,5 ⁰, spectral index g=2). 

Minimum detectable flux of a compact source 
versus the source power law spectrum index (a<0,5 ⁰, one year of observation). 

Source location capability for a year of observation for a source with the flux 10 ⁸ cm^-2 s ¹ (Eg>1GeV) versus the source power law spectrum index. 

Relative accuracy of  spectral index estimation after a year of observation for a source  with the flux 10 ⁸ cm ^-2 s ¹ (Eg>1GeV)  versus the source power law 
spectrum index.