Dear PI-Community,
as promised before, I did some further tests with the flat fields
![smile :)](http://pixinsight.com/forum/Smileys/default/smile.gif)
Well it may be not really surprising, but I found that really the "correct" exposure time of the flats is the
most important thing.
As some fellowers stated in this thread before, you really should avoid noise (from too short exposure times) or gradients
from bad flat field generators (or the sky itself)
For me I found the following rules suitable:
- for my Canon EOS 1100d and 450d (both modified for Ha) I use an ADU of 4000 for flats.
- for my ATIK 383L+ an ADU of 50% of max. ADU value (= about 32.000) gives the best results.
If I "underexpose" the flats, I also had some adverse effects, i.e. clipped black regions (from the OAG) become "pure" white
![tongue :tongue:](http://pixinsight.com/forum/Smileys/default/tongue.gif)
So this was very instructive for me.
Unfortunately, the "correct flat exposure times" were not that relevant in general astrofoto-literature, that I read before.
So testing and comparing the results was the best way to find out
![Wink ;)](http://pixinsight.com/forum/Smileys/default/wink.gif)