Re: ST1.7 Decon and ST1.8 SV Decon
Posted: Mon Sep 12, 2022 5:31 am
I also forgot to mention that the red/yellow/green/yellow/red coloring is a sliding scale, so you may see shades of pure green, banana green, banana yellow, etc.Mike in Rancho wrote: ↑Sat Sep 10, 2022 7:51 pm Thanks Ivo. Yes I've read that in the docs and even quoted it (loosely) in my post. I'm just trying to dig deeper into the apod mask colors - and perhaps am looking for meaning that isn't there. Wouldn't be the first time.
If all you have is these, try picking the brightest ones.Panel 1 is your basic red ball. I assume these are not to be used for SVD (I've never tried, actually). Problem is, sometimes my entire apod mask is pretty much only stars just like this.
Also. consider whether a pure synthetic PSF might just be better, if good quality samples are not getting you where you want to be. This may well get you better results than chasing samples in crowded wide fields. At the very least, the Moffat models should quite effectively undo the effects atmospheric turbulence. Any other imperfections/distortions in the PSF (whether local or across the entire image) may not even be visible at some scales.
Usually, atmospheric influences are the biggest contributors to out-of-the-ordinary PSFs, if the rest of your gear is dialed in reasonably well.
Correct!Panel 2 has some yellow in the core, no green. Ostensibly then okay for a secondary choice if I have nothing else in the area?
Correct. This appears to be a good sample. You may even want to increase the apodization mask so that more of the stellar profile is included.Panel 3 has some green. Not a ton, but pretty close to the best that I typically see. Assume this should be selected.
Ideally not, but if you are quite sure that the star isn't over-exposing and your sensor's (and stack's!) response stays linear with stars this bright, then maybe.Panel 4, (if one ignores the adjoining star), is green but red pixeled in the center. Not to be used even if it was by itself.
Still OK. It looks like the center is just creeping into the (possibly) non-linear danger zone.Panel 5, (again ignore the double star for now), is starting to show a green center but there's a yellow pixel (though not gone red) in the very center. Still okay? I think the Features and Docs examples of green stars actually may have a central yellow dot themselves, if I am peeking at it correctly?
More about the "danger zone"; this danger zone is, as said, the brightness where linearity might be getting iffy. This can be due to CCD well saturation (e.g. photons don't get converted into electrons as much due to the wells becoming "full"). This can also be due to stacking data of variable quality. For example, a star under poor seeing will not saturate as quick, because its light is "smeared out" over multiple pixels. Under good seeing conditions, however, stars will over-expose quicker as the light gets concentrated into fewer photo sites. If you stack a mixture of these, you will get stars that have cores that have unreliable data (due to averaging over-exposing cores with non-over-exposing cores).
Does the above help?