< edit: I forgot to stretch the JPEG before attaching it here... Fixed. >
Hopefully what I'm doing wrong or not doing at all will be evident to someone...
I am working on a 2x3 mosaic of the Heart Nebula area in OIII. I've already created a mosaic of the area for Ha, and the results were not only fairly easy to obtain (at least in PI terms

) but are pretty acceptable to my eye. But, the OIII set is not playing well at all for me for some reason.
Each OIII panel is an integration of six 10 minute subs. I've tried both ABE and DBE on each panel prior to using GradientMergeMosaic, but the mosaic area corresponding to one of the panels -- the IC1795 nebula region -- always ends up having a very different "look" than the other five. I wonder if this is because there's a lot more signal there? I've tried to process each panel's stack identically.
I should note that after many tries I was unable to get the OIII panels to co-register with Star Alignment; I didn't know about some of the more clever techniques (e.g. creating and using an artificial starfield as a reference) until today so I haven't tried any of those things yet, but what I've done instead is use my Ha mosaic as the reference image for alignment, and that seems to work just fine. But I'm not sure if this might be a factor in the problem I'm having.
I am also, courtesy of the PI tutorial videos about mosaics, aware that PixelMath can be used to address edge transition issues, but my problem is so drastic that I'm thinking that there must be a better way to address it.
A JPEG of the OIII mosaic is attached. The Ha equivalent is at
http://www.flickr.com/photos/46580576@N07/10046413393/.
thanks,
Dave B.