I have studied a number of the great pics, and apart from their use of specialized line filters and the NASA colormapping, which places H-alpha in the green channel, I have wondered how they manage to get such smooth backgrounds. Sure, integrating for a long time helps a lot. But I did some example regions, like IC1396 (Elephant Trunk) with my OSC and it is mostly Red channel, which I take to mean H-alpha and S-II, for an equal duration exposure to what the great pics have done, and my images still show a grainy appearance. (e.g., 2-4 hours total integration at F/2)
I just stumbled on a technique, which make a lot of sense in retrospect, whereby the MMT is used to slightly enhance the 256 scale, (bias = +0.1 to +0.2), and lo and behold, my images have lost that grainy appearance, and show the same smooth background in the nebular regions as the great pics show. (Do the MMT in the linear image)
Makes sense in hindsight, since adding a very low-pass filtered image simply adds some of the local mean. If you add an amount equal to the local mean, the SNR increases by 2x, since you haven't increased the standard deviation in the local neighborhood. Hence it appears less grainy, and survives the nonlinear stretch to visibility much more robustly.
So I wonder if I have just rediscovered what the authors of those fabulous images have known all along?