I'm going thru all your helpful DBE videos and trying to apply them to my latest image NGC 129 in Cassiopeia. As you point out in your videos the key thing is identifying what's going on. (ie. flat-field, gradient, dust donuts, etc.) I believe this is a flat-field error. That said, regardless of the settings I select for tolerance or shadows relaxation, I'm not able to remove the circular glow in the upper right of center. I've tried multiple tolerance levels from 5 to 10. I've tried both division and subtraction.
Can you advise as to what you think is going on? Inn link below is he original RGB image and the second is a more processed image. (ie. PCC, SCNR, HT, NoiseExt).
Thanks Much!
Comments
I totally agree that I should diagnose the underlying causes of these issues first as opposed to using PI to fix them. And I have been trying to do so for a while as I’ll describe below.
I’m using a 9.25” Celestron SCT, HyperStar with an Optolong LP filter, and ZWO294MC Pro on a Skywatcher mount. I don’t do anything particular with the cables other than just let them hang down (and I wonder if that could be an issue for diffraction). I use Asiair for capturing.
Additionally, I take all my frames from my Detroit-based condominium courtyard where there are a lot of lights so I use a flexible due shield on the scope to help block stray light. The LP Bortle rate where I am is 7.
Next week I’ll post some of the raw light frames: (calibrated, debayered) as well as some of the darks, flats, dark flats. I typically shoot either 30 sec or 60 sec frames for lights. I use master darks that correspond to those exposure rates (or in some cases I may do new darks after the session).
I have been struggling with making and diagnosing effectiveness on my flats. I use a light panel from Germany on top of the dew shield but I have to use light filters to get the ADUs down to the correct range even with low settings on the panel. My camera is the ZWO 294MC pro CMOS and they (and others) recommend using at least 3 sec exposures on the flats to account for the “flashing” that occurs in the corner. I have a library of dark flats that I’ll use either with 3 sec or whatever other exposure rates I’ll try on the flats. I’ve been doing a lot of trial and error by varying the levels of ADUs by changing the exposure rates of my camera and intensity levels on the panel. I wonder if there is a better way to access this so I don’t have to do so much darn trial and error.
I have also struggled to get the backfocus correct using some small-mm separators to get it as precise as possible and my focus has improved. I’ve also done analysis on collimation of my HyperStar and (I think) it’s ok. The only avenue I know to explore is alignment of the plate. Or other?
Appreciate any insight you (or anyone else) can provide but no reason to respond till I have posted the additional frames which may better pinpoint my issues.
Thanks much!
Richard (aka TheAstroTiger on Instagram).