Unfortunately I don't have a normal mount, but a German one. So I'm forced to lose precious hours when the object to be photographed is in the best position, on the meridian. I have neighbors and I can't make too much noise, so I have to reverse the side by hand, with huge problems in sync and solvin plate. But that's another discussion. The problem is that I also have to remember to enter in to the indi drivers of the two ccd cameras (120mm and 533mc) and manually invert Hflip and Vflip (I certainly don't start rotating them 180 degrees every time). And I have to remember which light and dark are flipped, because it is not recorded in the header of the FIT file (or at least I think). Is it possible to automate all these operations? you know that if you debayerise a flipped image the red and blue channel are inverted (for normal, RGGB or auto, for flipped BGGR), so this process is very important. And how about to have flip information inside the file?

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