I've had good results with ADUs in the range 14,000 to 30,000. I don't think that it's mega-critical as long as you are well out of the noise floor and not saturating the sensor. Flat field corrections in software are multiplictive so, in theory at least, as long as you are not clipped at the black or white ends the corrected results should be the same as long as the sensor is linear. The KAF 8300 is, apparently, quite linear and is used for scientific work. With regards to the back focus distance, you'll have a fun time sourcing all the spacers that you'll need to get it exact. I found Telescop-Express to be a very useful resource. The third screw in the eyepiece holder is an absolutely must with the weight of the coma corrector, filter wheel and camera hanging off of the PDS focuser if you want any kind of orthogonality at your chip! I used an M6 allen-head bolt that I have in abundance. There's plenty of metal in the eyepiece holder to take the bolt. Taps and dies are cheap and you just need to find a buddy with a pillar drill (every astronomer should have access to a pillar drill! ). You can see the bolt in this close up: You might also consider tightening up the focuser a bit too. See here: http://www.teleskop-shop.at/testphotos/w-erbung/Crayford_adjustment_Synta_microfoc.pdf I found that the weight of the imaging gear would slowly unwind the focuser over the evening until I had "corrected" the tension in mine.