with the clear but moonlit skies last night I decided to investigate plate solving with MaximDL - something I have been meaning to do for a while. Now - I am still in the early stage of using Maxim DL, and think that I will eventually switch over to using it for guiding as well.
I got it to solve frames from my QHY5 very nicely (couldn't believe how quick it was on my little netbook) - although I did need to reduce the magnitude stars it would try to use from 20 --> 12. Maxim also picked up the position of the mount without any issues, and I was able to use that for the rough position. I was also able to sync on the solved position, and also slew to other stars shown in the 'Zoom' tab (found the Helix for the first time, and snapped a couple of frames of that just for the hell of it - I think it needs more focal length than my FS-60 with a reducer though

)
First question is - when it has solved the image and gives you the position, it also gives you what it thinks is the focal length and image scale of your scope/camera etc. When I used the calculator it provides to figure out the image scale - it gave me 4.76 or something like that (355mm focal length FS-60 with 0.72x reducer = 255mm, then 5.2 micron square pixels in QHY5), but after solving it said the image scale was 3.03 or therabouts - can't remember the exact numbers. Why the difference, or is my focal length / pixel size wrong?
Second question: does syncing the mount with the solved position have the same effect as doing an alignment using the handset, or syncing stars with CdC? And if you sync multiple stars using MaximDL, does it build a model using all of the stars or does it only 'remember' the current one?
Third question: what other cool stuff can I do now I have the basics sorted out?
Cheers
Adam