• @lefty7283OPM
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    21 year ago

    A few years ago I shot just the core of NGC7822, and I’ve decided to reshoot it as a 2 panel mosaic to get some of the outer structures. The whole nebula is actually pretty big in the sky (over 3 degrees!), but I did not want to deal with processing another 8+ panel mosaic to fit the whole thing.

    Captured over 23 nights from September through November, 2023 from a Bortle 9 zone.

    Places where I host my other images:

    Flickr | Instagram


    Equipment:

    • TPO 6" F/4 Imaging Newtonian

    • Orion Sirius EQ-G

    • ZWO ASI1600MM-Pro

    • Skywatcher Quattro Coma Corrector

    • ZWO EFW 8x1.25"/31mm

    • Astronomik LRGB+CLS Filters- 31mm

    • Astrodon 31mm Ha 5nm, Oiii 3nm, Sii 5nm

    • Agena 50mm Deluxe Straight-Through Guide Scope

    • ZWO ASI-120mc for guiding

    • Moonlite Autofocuser

    Acquisition: 51 hours 30 minutes (Camera at -15°C)

    • Left panel:

    • Ha - 54x360"

    • Oiii - 130x360"

    • Sii - 101x360"

    • Right Panel:

    • Ha - 46x360"

    • Oiii - 94x360"

    • Sii - 90x360"

    • Darks- 30

    • Flats- 30 per filter

    Capture Software:

    • Captured using N.I.N.A. and PHD2 for guiding and dithering.

    PixInsight processing:

    Preprocessing

    • BatchPreProcessing

    • StarAlignment

    • Blink

    • ImageIntegration per channel per panel

    • DrizzleIntegration (2x, Var β=1.5) per panel per channel

    • StarAlignment in mosaic mode to align the two panels, then GradientMergeMosaic to combine them

    Linear:

    • DynamicBackground Extraction

    duplicated each image and removed stars via StarXterminator. Ran DBE with a shitload of points to generate background model. model subtracted from original pic using the following PixelMath (math courtesy of /u/jimmythechicken1)

    $T * med(model) / model

    • BlurXTerminator

    • NoiseXterminator

    • STF applied via HistogramTransformation to bring nonlinear

    Nonlinear:

    • PixelMath to combine stretched narrowband masters into color image

    SHO --> RGB (classic Hubble Palette)

    • removed stars and processed stars-only image separately with invert>SCNR and curve adjustments, to be added to starless image later.

    • HistogramTransformations to adjust channel intensities

    • Invert > SCNR > Invert to remove magentas

    • CurveTransformations for slight hue adjustments

    • LRGBCombination using stretched Ha as luminance

    • shitloads of CurveTransformations to adjust hue, lightness, saturation, etc. (some with lum masks)

    • MLT chrominance noise reduction

    • NoiseXTerminator

    • LocalHistogramEqualization

    Two round of this: one at kernel radius 16 for the finer ‘feathery’ details and one at 512+ for larger structures

    • More curves

    • Relinearized narrowband and stars images to add in the stars only image

    “unstretched” both images with histogramtransformation midtones set to 0.9999

    pixelmath to just add those two images together

    histogramtransformation to un-relinearize them by setting midtones to 0.0001

    • ColorSaturation

    • Even more curves

    • Extract L > LRGBCombination for some chrominance noise reduction

    • Slight SCNR to remove some greens from the bright parts of the nebula

    • DynamicCrop to remove a few artifacts around the edge where the panels overlap

    • Resample to 60%

    • annotation

  • @KingRandomGuy
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    21 year ago

    Amazing work!

    I was curious to know how you handle flats with this many nights of integration. Do you have separate flats for each night, or did you just take a total of 30 flats on a single night?

    • @lefty7283OPM
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      21 year ago

      I take flats maybe once a month or the few times a year I travel with my gear. I keep the entire imaging train together so not much changes night to night.