I have just installed an Alnitak Flat-Man XL panel in my observatory and was wondering what approach people are using to create their master frames. Mainly interested in the number of bias frames used to make the master and why as well as for the darks and flats. In the past I've generally used 5 flats, 10 darks and 20 bias frames when creating my masters but now that I have a high quality EL panel taking flats using ACP has become quit painless as I can do them any evening regardless of weather so the number of frames isn't a time constraint. I also use a rotator so I take east side and west side flats although I intend to do some experimenting to see if they are different at all. The only way I know to do this is use a master east frame to flat a master west flat. If the doughnuts disappear that I think it may be safe to think this is a proper line of thought. Any suggestions or am I missing something here?
The darks and bias frames are also able to be done on nights not good for imaging and my thought here is to create a more update library. Taking lots of calibration frames shouldn't be an issue as you can make the masters and then delete the individual frames saving only master frames. I'd likely save these master frames with data they were used on such as the object they were used to calibrate in one folder with the folders of those nights data in sub folders. There might be some redundant master frames over time but at least not near as many frames as all the individual used to make them. Does this make sense or do you have a better solution?
Thanks,
Steve