Post Blood Moon M13
Posted: Tue May 17, 2022 5:01 am
There have been some really nice clusters posted here lately.
My Frankenglob will not be one of them.
So, I did not take advantage of a little darkness during the eclipse, but did get started shortly after it was fully bright again. M13 was a bit distant, but I still needed to strap my moonlight-blocking shield to the end of the Newt. Eh...that seems to still be a work-in-progress to get right.
Another change I made was to unmount my UV-IR cut filter and apply some ultra matte paint to a couple inner surfaces that were, sadly, quite glossy. I was super careful about situating the glass in a microfiber towel so that I knew the orientation. Right up until it slipped out and bounced on the carpet. 50/50 chance I got it right, I suppose.
I shot an hour with the D5300, then took direction matched flats right on the rig, before swapping over to the 2600MM for an hour of luminance. The Nikon data actually came out pretty well, with some of the gremlins I have been fighting seemingly improved. Alas, to balance that out I somehow really botched the L data. Could have been the moon blocker wasn't 100% blocking or even impinged on the view (I did seem to pick up an extra diffraction spike that shouldn't be there), or that I imaged through the meridian (at 88° alt) and flopped the mirror, or...that when I put the tracing pad box on the scope the clutches didn't hold the weight. Oops. That sure might have flopped the mirror.
So in the end I had such a bad gradient/anomaly that the L stack had to be separately and aggressively Wiped first and saved, in order to then be composed with the registered R, G, and B extracted mono files from the D5300.
All stacking was in ASTAP. Siril was used to split the RGB into the three 32-bit FITS files, and to resample the 2600MM FITS stack to match the pixel scale. ASTAP then created star aligned new files from those.
Normal glob processing of Crop, Bin, Wipe, AutoDev, Contrast, HDR with context of 5 and shadow to about 60 (in order to maintain some core brightness and not be too tamed), SVD, Color after sampling non-glob stars, and Denoise. There are some really great star colors in the neighborhood here.
I also composed this, third time around, as L+Synth L from the Nikon data. Things were not looking right when I only used the 2600 data for L. I think maybe there was just too much disconnect between the datasets here to use the L, RGB that I thought would be best.
I suppose I will have to break down and get some real LRGB filters. Sigh.
My Frankenglob will not be one of them.
So, I did not take advantage of a little darkness during the eclipse, but did get started shortly after it was fully bright again. M13 was a bit distant, but I still needed to strap my moonlight-blocking shield to the end of the Newt. Eh...that seems to still be a work-in-progress to get right.
Another change I made was to unmount my UV-IR cut filter and apply some ultra matte paint to a couple inner surfaces that were, sadly, quite glossy. I was super careful about situating the glass in a microfiber towel so that I knew the orientation. Right up until it slipped out and bounced on the carpet. 50/50 chance I got it right, I suppose.
I shot an hour with the D5300, then took direction matched flats right on the rig, before swapping over to the 2600MM for an hour of luminance. The Nikon data actually came out pretty well, with some of the gremlins I have been fighting seemingly improved. Alas, to balance that out I somehow really botched the L data. Could have been the moon blocker wasn't 100% blocking or even impinged on the view (I did seem to pick up an extra diffraction spike that shouldn't be there), or that I imaged through the meridian (at 88° alt) and flopped the mirror, or...that when I put the tracing pad box on the scope the clutches didn't hold the weight. Oops. That sure might have flopped the mirror.
So in the end I had such a bad gradient/anomaly that the L stack had to be separately and aggressively Wiped first and saved, in order to then be composed with the registered R, G, and B extracted mono files from the D5300.
All stacking was in ASTAP. Siril was used to split the RGB into the three 32-bit FITS files, and to resample the 2600MM FITS stack to match the pixel scale. ASTAP then created star aligned new files from those.
Normal glob processing of Crop, Bin, Wipe, AutoDev, Contrast, HDR with context of 5 and shadow to about 60 (in order to maintain some core brightness and not be too tamed), SVD, Color after sampling non-glob stars, and Denoise. There are some really great star colors in the neighborhood here.
I also composed this, third time around, as L+Synth L from the Nikon data. Things were not looking right when I only used the 2600 data for L. I think maybe there was just too much disconnect between the datasets here to use the L, RGB that I thought would be best.
I suppose I will have to break down and get some real LRGB filters. Sigh.