I am working with an F4 200m TS Photon with a skywatcher f4 aplanatic coma corrector, using an altair 269c for galaxy season and an ASI294mm for nebula season- so both effectively 4/3 sensors with approx 22mm diagonals. I have been working through a range of issues like accurate collimation, pinched optics and decent guiding and balance of my rig together with installation of a ring over the mirror clips. I am finally getting some almost decent results. the final stage is back focus distance so that the final smaller diffraction spikes on brighter stars aren't spread away from the centre of the image
I read that the stated backfocus distance is 55mm but ither people claim about 53mm. I guess that the optimum distance varies from setup to setup as the sensor distance in any camera has a manufacturing tolerance of 0.5mm.... Is there a diagram anywhere for newts and coma correctors that is similar to this one for refractors and field flatteners? - or is the field flattening element of the cc roughly equivalent to the field flattening element in a refractor reducer/flattener and so could this diagram be used for cc's?
Thanks
Paul
