Hi popo,
Thanks for that. This image has surprised me in a few ways. Firstly, the amount of structure that can be extracted from the brighter areas and secondly the extent of the fainter region. Of course, once you know it's there it is possible to find other images (e.g.
this APOD from five years ago) but the vast bulk of images revealed by
Googling give little hint that so much is going on. But the biggest surprise is the muted response over at Stargazer's and I'm forced to ask myself why? Have I overdone the processing in order to reveal the bright structure or was my colour choice for the faint bits a little off? Coincidentally, that choice isn't so far away from the APOD palette, which I hadn't seen until after my first draft was complete, so I'm a little doubtful it's the colour choice that is at fault.
I'm tempted to ask just why so few images out in the wild show the surrounding nebulosity. OK, I do use a large cooled CCD and yes, I was scratching around just above the noise floor of my data but heck, that was only 5 x 1,000 seconds (comfortably less than an hour and a half) of imaging through the blue filter and that at a comparatively dim f/7.
What's going on? Don't folk believe the data they see on their images or don't they want to show what's actually there? I'll ask that question at Stargazer's in about a week's time in a gentler fashion once I get, or don't get, a few more comments.
Bob.