The astrometric coordinates and photometric data of tracklets of man-made objects may be calculated with very high accuracy. By taking into account possible time biases of the recorded observation times, refraction effects, optical aberrations of specific telescope used and distortion effects of CMOS cameras with rolling shutter you can push the astrometric accuracy of your system to the limits.
Please contact us for an offer. We can also consult for and develop bespoke solutions tailored to your requirements.