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Because of the eery shape of NGC 246 being a little like a human skull, it has now become commonly known as the Skull Nebula, and categorised by Sir Patrick Moore as Caldwell 56. The object is in fact a planetary nebula, the remnants of a failed star many years past. You’ll find this object in the constellation of Cetus, with it being roughly 1,600 light-years away from Earth.
This image represents only 24% of the cameras full frame, composed of luminance, red, green, blue, oxygen 3, and hydrogen alpha filtered colour channels. Thanks for having a look.
Hi res link:
live.staticflickr.com/65535/50685844921_967b9026ea_o.jpg
Information about the image:
Center (RA, Dec):(11.840, -11.841)
Center (RA, hms):00h 47m 21.671s
Center (Dec, dms):-11° 50' 26.283"
Size:23.3 x 16.6 arcmin
Radius:0.239 deg
Pixel scale:0.732 arcsec/pixel
Orientation:Up is 206 degrees E of N
Instrument: Planewave CDK 12.5 | Focal Ratio: F8
Camera: STXL-11000 + AOX | Mount: AP900GTO
Camera Sensitivity: Lum, OIII & Ha: BIN 1x1, RGB: BIN 2x2
Exposure Details: Total: 61.0 hours | Lum: 64 x 1200 sec [21.33hr], OIII: 37 x 1200 sec [12.33hr], Ha: 64 x 1200 sec [21.33hr], RGB 16 x 450sec each [6.0hrs]
Viewing Location: Central Victoria, Australia.
Observatory: ScopeDome 3m
Date: June-November 2020
Software Enhancements: CCDStack2, CCDBand-Aid, PS, Pixinsight
Author: Steven Mohr
The Lower half of Orion from the Bogeyman to the WitchHead. 12 Panel mosaic. Samyang135ASI2600 for RGB Samyang135ASI1600mm for Ha. Processed in Pixinsight and Photoshop.
Imaged in Hydrogen Alpha and Oxygen III. Approximately 5.5 hours exposure time, the colour palette is made up from applying Hydrogen to red and Oxygen to both green and blue. A Luminance channel from a blend of both the Hydrogen and Oxygen data was applied over the top of the colour image in Pixinsight.
The Astrodon OIII filter has captured the outer Oxygen shock wave nicely.
Imaged with an Altair Astro 6" RC and Atik 314l+, processed in Pixinsight and CS5.
IC 4603
LUMINANCE: 150 MINUTES
RGB: 30 MINUTES EACH CHANNEL
TOTAL: 4 HOURS
WILLIAM OPTICS 80 ED II
ZWO ASI 1600 MONO COOLED
PROCESSING: PIXINSIGHT + PS6
New version with processing my friend Leandro Fornazieiro
Stack of 40 individual DSLR shots. Sky-Watcher 150P Newtonian. Prime focus, Baader Neodymium filter. PIPP > Registax > PixInsight > Photoshop with colour blend layer from individual raw frame.
Taken w/ William Optics Redcat 51, QHYCCD Polemaster, Skywatcher EQM-35, Nikon D7500.
150 x 90s lights @ ISO 800, ~45 dark, ~80 flat, ~100 bias, stacked in DSS and post-processed in Photoshop & PixInsight
A section of the constellation Cygnus, containing the North American and Pelican nebula.
Tec
Canon T5 Modded w CLS-CCD clip filter.
Canon 200mm Prime f2.8@3.2
Ioptron Skyguider
150 x 90s Stacked in Pixinsight
Processed in Pixinsight and Photoshop cc
Taken at Camden Lake
July 24th 2020
1st time out with my Askar FRA400 telescope.
Wouldn't quite fit the entire galaxy in to the field of view, so I went for a 2 panel mosaic.
M31 lies 2.5 million light years away from us and has two visible dwarf galaxies for companions. They are M32, just above and left of centre and M110, an elliptical galaxy to the bottom centre of the image.
Captured at www.astronomycentre.org.uk
Boring Techie bit:
Telescope: Askar FRA400
Mount: EQ6r pro
Camera: ZWO 533mc pro
Filter: Optolong L'eNhance.
Guided and controlled by the ZWO asiair+
The 2 panels each consisted of 60 lights frames at 120 seconds exposure each. Plus darks, flats, dark flats & bias calibration frames.
All stacked together in DeepSkyStacker and the resulting 2 images were then stitched together and processed further in PixInsight & Affinity Photo.
The North America Nebula NGC7000 captured earlier this year using the QHY367 Pro C full frame one shot color 36 Megapixel CMOS camera mounted on the Takahashi 130 FSQ.
Often ignored in images of The North America Nebula is the immense patch of shadows, the dark nebula LDN 935 appearing prominently (left of center) with the Cygnus Wall (at bottom left) and The Pelican Nebula IC 5070 (at center). The dust from this dark nebula obscures the emission nebula to form the region known as The Gulf of Mexico. This detailed image surely visualizes the nature of dust and gas clouds that populate the universe.
In this Hubble Palette version (SHO) the H-Alpha is mapped to green, SII is mapped to red and OIII is mapped to the blue channel. RGB data was used for the natural star color, while the colors in this image are not the true colors, the narrowband filters used in the making of this Hubble Palette image reveal much more of the hidden gasses not visible in a broadband image, covering an area over 3 x 2 degrees of sky.
Captured over 5 nights in May and June 2020 for a total acquisition time of 20.8 hours.
View High Resolution Astrobin: www.astrobin.com/hz7qvn/
Technical Details
Captured and processed by: Terry Hancock
Location: GrandMesaObservatory.com Purdy Mesa, Colorado
Dates of Capture May 21, 29, June 10, 12, 15 2020
RGB 290 min 29 x 600 sec
HA 495 min 33 x 900 sec
OIII 210 min 14 x 900 sec
SII 255 min 17 x 900 sec
Narrowband Filters by Chroma (5nm)
Camera: QHY367 ProC full frame one shot color CMOS
Filter Wheel: QHYCFW3 Large
Gain 2850, Offset 76
Calibrated with dark, Bias and Flat Frames
Optics: Walter Holloway's Takahashi FSQ 130 APO Refractor @ F5
Image Scale: 1.56 arcsec/pix
Field of View: 3d 7' 41.0" x 2d 3' 5.3 (127.3 x 190.1 arcmin)
EQ Mount: Paramount ME
Image Acquisition software Maxim DL6 Pre Processing in Pixinsight Post Processed in Photoshop CC and Starnet.
T:Takahashi FSQ 106ED
M: Astrophysics Mach1 GTO
C: QHY600M_L
G: Lodestar X2
F: Antlia HA, OIII, SII 3nm
Foc: Esatto 4" Primalucelab
CPU: Eagle-2 Primalucelab
Sw: Sequence Generator Pro - PHD2 - Pixinsight
Ha:OIII:SIIxT=25:25:25x600"
Dumbell nebula, Jul. 20, '25
Celestron Edge HD800, ASI Air Plus, ASI MC Pro
Light, Dark, Flat, Flat Dark
PixInsight, Photoshop
Struggling to get enough data with this awful weather in UK! 40x 300sec subs.
William Optics GT81 with ZWO533mc Pro, processed in pixinsight
ASI 294 MC PRO.
72 ED Skywatcher con reductor/aplanador 0.85.
Star Adventurer 2i.
Guiado Asi 120mm Mini.
Ganancia 123 Offset 5 -10ºc
109x120s
L-Pro
Bortle 8.
PixInsight.
NGC6520 LRGB
Planewave 17” CDK
Camera: FLI ML16803
Filter: Chroma L,R,G,B
Focuser: IRF90
Focal Length: 2939mm
Focal Ratio: f/6.8
Mount: 10 Micron GM3000
Location: Deep Sky West, Chile
8hh of LRGB data, combination in PixInsight done:
L: 24 x 300sec
R: 24 x 300sec
G: 24 x 300sec
B: 24 x 300sec
BlurXTerminator not used.
Andromeda Galaxy in Hydrogen Alpha. The brighter clumps in the spiral arms are star-forming regions similar to The Great Orion Nebula in our own Galaxy. A full color image of Andromeda would appear predominately white in a full color image without any Ha information being added. When added in processing, the Ha star forming regions will appear red.
ZWO ASI6200MM-Pro/EFW 2" x 7 (Ha)
Tele Vue NP101is/Large Field Corrector
Losmandy G11
Capture in NINA
Processing in PixInsight
Capture TelescopeLive AUS-2 north of Canberra. 15h RGBHS. Processing Jan Zettergren, PixInsight and LR
41P/Tuttle-Giacobini-Kresak in the body of Ursa Major. x27 10 sec exposures (ISO3200) stacked in DSS and processed in Pixinsight and Faststone. 6D + 85mm f1.4 lens.
NGC7380 or the Wizard Nebula as it is commonly known as, is an emmision nebula in the constelation of Cepheus
Image Details:
Acquisition Dates:Sept. 20, 2019, Sept. 21, 2019, Sept. 30, 2019, Dec. 6, 2019, Dec. 9, 2019, Dec. 20, 2019, Dec. 25, 2019, Dec. 31, 2019
Frames:
Astronomik Ha 6nm: 51x300" (gain: 11.00) -20C bin 1x1
Astronomik OIII 6nm: 51x300" (gain: 11.00) -20C bin 1x1
Astronomik SII 6nm: 51x300" (gain: 11.00) -20C bin 1x1
Integration: 12.8 hours
Darks: ~101
Flats: ~101
Flat darks: ~101
Avg. Moon age: 15.36 days
Avg. Moon phase: 43.95%
Bortle Dark-Sky Scale: 4.00
Equipment Details:
Imaging Scope: Sharpstar Optics 15028HNT Hyperboloid Astrograph Reflector
Imaging Camera: Qhyccd 183M Mono ColdMOS at -20C
Mount: Sky-Watcher EQ8 Pro
Guide Scope: Sky-Watcher Finder Scope
Guide Camera: Starlight Xpress Ltd Lodestar X2
Filters: Astronomik 36mm RGB F2.2 Certified
Filterwheel: Starlight Xpress Ltd 7x36mm EFW
Power and USB Control: Pegasus Astro Ultimate USB Hub
Focuser: Primalucelab Sesto Senso Auto Focuser
Image Acquisition Software: Main Sequence Software SGPro
Guide Software: PHD 2
Processing Software: PixInsight
Mu Cephei (μ Cep) is a red supergiant located in the constellation Cepheus. With an average apparent magnitude of 4.08, it is the 10th brightest star in the constellation. Also known as Herschel’s Garnet Star and notable for its striking red colour, Mu Cephei is a spectral standard for its class (M2). It is one of the largest known stars, with a radius 1,260 – 1,650 times that of the Sun, and one of the largest stars visible to the unaided eye. Located at an approximate distance of 2,840 light years from Earth, it is one of the most distant stars visible without binoculars.
Taken in Early October 2021 with Fujifilm X-T3, Nikkor 85mm F/1.4.
Equipment:
10" f/4 ONTC Newtonian Teleskope
ASI294mmPro
Astronomik L-2
Skywatcher EQ-8 Pro
135 x120s Luminanz
45 x 120s red
45 x 120s green
45 x 120s blue
total exposure time: 9 hours
march 2022
Processing: PixInsight/affinity photo
Weekend...Check! Clear night...Check! New moon...Check!
So far so good...starting new target...SH 2-101 the tulip nebula. Took some RGB data. Not that much, but almost an hour per channel.
The humidity was so high, my secondary mirror mist up over the night...I have no heater and never used one...I should have put the dewshield on at least.
I will take the h-alpha data later.
-- EQUIPMENT ---------------------------
Camera: SBIG STF-8300
Filterwheel: SBIG FW8 (8 x 36 mm)
Filters: Astrodon RGB
Telescope: 10" ONTC Newton w. 2.5" Wynne corr. (1140mm f/4.5)
Mount: Astro-Physics 1100 GTO CP4
Guiding: SBIG OAG with Starlight Xpress Lodestar X2
Software
Capturing: Sequence Generator Pro
Mount control: AP V2
Guiding: PHD2
Processing: Pixinsight
-- Details -----------------------------------
Date: 30. August 2019
Location: My backyard
Temp CCD: -15°C
Pixel size: 5.4 μm
Pixel scale: 0.93 Arcseconds per pixel
-- Exposures ------------------------------
Red: 5 x 10 min
Green: 5 x10 min
Blue: 5 x 10 min
Total integration time: 2 hours and 30 minutes.
47 Tucanae
LRGB data from TelescopeLive. Processed with PixInsight.
The whirlpool galaxy is actually two galaxies interacting with each other. The quite obvious spiral galaxy that is M51 and the much smaller galaxy catalogued as NGC 5195.
First discovered by Charles Messier in 1773, M51 is located 31 million light years away in the constellation Canes Venatici.
Data gathered at www.astronomycentre.org.uk/ on the 18/03/2025.
Boring Techie bit:
Telescope: Skywatcher Quattro 8"
Mount: EQ6r pro
Camera: ZWO 533mc pro
Filter: Optolong UV/IR.
Guided and controlled by the ZWO asiair+ using Altair Starwave 50mm & ZWO 120mm mini.
248 light frames 60 seconds each.
Stacked with darks using WBPP in PixInsight.
Processed using Graxpert, StarNet2, PixInsight & Affinity Photo.
Logiciels et plugin utilisés :
Lightroom, AstroPixelProcessor, BlurXTerminator (Merci @h.collis pour le passage dans le plugin de Pixinsight) , PhotoShop (Plugin HLVG, Topaz Denoise)
127 lights, 100 offsets, 100 flats, No Dark
There is over 11 hours of imaging time in this image which was captured 31st Dec, 7th Jan and 14th Jan 2016, using the following equipment and software.
TS APO65Q Telescope
Atik 490EX CCD Camera
QHY5L Guide Camera on 90x50 finder scope
Baader Ha, OIII and SII narrow band filters.
Artemis Capture.
PHD2 Guiding.
All processing Pixinsight incl stacking (image integration)
This image is blended from SII, OIII and Ha filters using the PixelMath component in Pixinsight. The mix is to suit my own taste.
The SII has added Ha
The Ha as some OIII added
The OIII is on it's own
Thanks to Kayron at www.lightvortexastronomy.com for the wonderful tutorials.
I am very pleased with the detail of the data but I feel the stars do overpower and I would welcome any constructive criticism as to what I may be doing wrong (over exposure?) or can do to correct this in processing.
Dusty emission in the Tadpole nebula, IC 410, lies about 12,000 light-years away in the northern constellation Auriga. The cloud of glowing gas is over 100 light-years across, sculpted by stellar winds and radiation from embedded open star cluster NGC 1893. Formed in the interstellar cloud a mere 4 million years ago, bright cluster stars are seen all around the star-forming nebula. Notable near the image center are two relatively dense streamers of material trailing away from the nebula's central regions. Potentially sites of ongoing star formation in IC 410, these cosmic tadpole shapes are about 10 light-years long.
Distance 30 Mio. Lj
Equipment:
TS 10" f/4 ONTC Newton
1000mm f4
ZWO ASI 1600mmc
Astrodon LRGB
Losmandy G11/LFE Photo
Guding:
Lodestar on TS Optics - ultra short 9mm Off Axis Guider
PHD2
RGB per 12x120s
Luminanz 60x120s
total exposure time: ca. 192 min
20.03.2018
Processing: PixInsight/CaptureOne
IC 405 - der Flaming Star Nebel mit seinem Nachbar IC 410 der Tadpole Nebula
Konnte kurz vor Saisonende noch knapp 8,7 Std. mit dem Epsilon 130D und der QHY268m drauf halten.
Leider kommen die Quallen nicht so toll raus wie gehofft, denke da hätte noch etwas zusätzliches Schmalband geholfen.
Equipment:
Takahashi Epsilon 130ED
QHY268m
CFW3M
Astronomik H-alpha MaxFR
Skywatcher EQ8
Februar 2022
Processing: PixInsight/affinity photo
120x180s H-alpha
23x120s red
30x120s green
30x120s blue
2,7 Std. RGB
6 Std. H-alpha
total: 8,7 hour
NGC7000
143h 25min of HSO data from Telescope Live. Processed in PixInsight. Grayscale variant.
Triplet 115/800
Flattener Reducer: 0.79
ZWO ASI 183 MM PRO
LHARGB #optolong
300 | 240 | 45 | 45 | 45
All frames Bin 1x1 - Gain 111
Total: 675 minutes
PixInsight + PS6
Horsehead and Flame Nebulae in Orion
Horsehead: Barnard 33 in emission nebula IC434 & Flame Nebula (NGC2024 and Sh2-277)
Acquisition Date: 12/28/2013
Camera: SBIG ST8300M @ -15°C
Telescope Stellarvue SV105T (f/7)
Mount: Astro-Physics AP1100
Guidescope: William Optics 50mm f/4 guiding/finderscope
Guide Camera: SBIG STi-M
Filters:(Astrodon)
-Hydrogen Alpha (3 nm Ha): 6 x 15min (90min)
Limiting Magnitude: 5.1
Comments: Stellarvue SFF7-21 field flattener.
Processed in PixInsight 1.8 and Adobe Photoshop CS5
Optics: Rokinon 135mm f/2
Camera: ASI 585MC
Filters: UV/IR: Baader
Mount: ZWO AM3
Observatory: Hertford, North Carolina, USA
starbase.insightobservatory.com/imageset/299
Integration Time: 11h 15m
Cocoon Nebula IC5146 Caldwell 19
Esprit 100ED
Canon 700d
CGEM DX
ISO800 11x360s (1hr 6mins)
PixInsight
Resolution ............... 1.592 arcsec/px
Rotation ................. 103.508 deg
Reference system ......... ICRS
Observation start time ... 2023-08-20 23:40:03 UTC
Observation end time ..... 2023-08-21 00:51:53 UTC
Focal distance ........... 557.08 mm
Pixel size ............... 4.30 um
Field of view ............ 2d 18' 11.7" x 1d 32' 14.2"
Image center ............. RA: 21 53 33.574 Dec: +47 17 54.12 ex: +0.019102 px ey: +0.006723 px
SSRO- RCOS 16", Alta U9, PlaneWave Ascension 200HR, PixInsight 1.8, ACP, MaxIm DL, FocusMax
Object description at www.billionsandbillions.com
Orion will be leaving us soon ☹ for another season and I’m Just getting around to processing the broadband data from Grand Mesa Observatory on the Horsehead (IC434) and The Flame Nebula (NGC 2024) using the QHY600M monochrome CMOS on the TAK130 and I was so impressed with the luminance data that I decided to share this image, “besides I just love black and white photos”. This is a 56% crop of the original and just 43 x 2 minutes exposures with no noise reduction whatsoever applied to the image for a total integration time of 86 minutes. Also visible in this image in quite good detail NGC2023, IC 435, IC 432, IC 431 and of course the triple star system of the blue supergiant Alnitak is also seen in all its glory with not so much of a halo.
We have the honor of testing the new QHY600 60 Megapixel Full Frame Monochrome CMOS camera for QHYCCD.
This setup is available immediately for people wanting to subscribe to Grand Mesa Observatory's system 1. grandmesaobservatory.com/equipment
View in High resolution
Astrobin: www.astrobin.com/wpebfr/
Technical Details
Captured and processed by: Terry Hancock
Location: GrandMesaObservatory.com Purdy Mesa, Colorado
Dates of Capture December 24th, Jan 6th, 9th 2021
LUM 86 min 43 x 120 sec
Broadband and Narrowband Filters by Chroma
Camera: QHY600 Monochrome CMOS Photographic version
Gain 60, Offset 76 in Read Mode Photographic 16 bit
Calibrated with Dark, Bias and Flat Frames
Optics: Walter Holloway's Takahashi FSQ 130 APO Refractor @ F5
Image Scale: 1.19 arcsec/pix
Field of View: Field of view 1d 47' 6.3" x 1d 13' 44.9"
EQ Mount: Paramount ME
Image Acquisition software Maxim DL6 Pre Processing and Starnet in Pixinsight Post Processed in Photoshop CC
Scope: Orion Optics VX6 with 1/10 PV upgraded optics
Guide Scope: Skywatcher ST80
Guide Cam: QHY 5 Mono
Mount: Skywatcher HQE5
Camera: Nikon D5100 Modded
Exposure: 18x5 Minute Subs, Darks, Bias & Flats
Technical: 750mm f/5
Software: DSS, Pixinsight, PHD, Nebulosity
This is a combination of 26 subs, one set from April 2020, of 10 x 10 minutes duration and another set of 16 x 5 minutes duration from 2018. All at ISO400. Taken with my 480mm f/6 refractor on a modified Canon 80D.
Technical card for 2020 session is in my Backyard Astrophotography Album.
I’ve not cropped this, so some background galaxies can be seen in the corners.
M81 is a large spiral galaxy in Ursa Major that is reasonably local to us at 12 million light years. Its companion, M82 has been disrupted by an encounter with M81 in the past.
M82 is a starburst galaxy with intense star formation triggered by the gravitational influence of M81. The red fan-like filaments at right angles to the axis of the galaxy are formed by a "superwind". The intense star formation has resulted in multiple supernovae explosions occurring about once every 10 years - the explosions power the super wind. The filaments are expanding outwards at about 600 miles a second and glow brightly in hydrogen alpha (red). They are also a very strong source of radio emission, listed as 3C 231 in the 3rd Cambridge catalogue of radio sources.
NGC3077 lies top left. It’s classified as a peculiar galaxy and may have interacted with M81 in the past and become disrupted. Some radial dust bands are just visible in this image - couldn’t see this detail before so nice to pick up in this longer integration.
The faint galaxy Holmberg IX lies just above M81, seen here as a faint triangular smudge contained in a trapezoid set of stars. It seems to be a companion dwarf galaxy to M81, a bit like our Magellanic Clouds.
The small galaxies bottom left and right are PGC28563 and PGC28225 respectively.
Image scale: 1.59 arcsecond/pixel
Field-of-view: 1d 37' 34.0" x 1d 9' 3.6"
Image centred on:
RA: 9hr 55min 25.931s
DEC: +67d 10min 05.69s
I tried a few new things in PixInsight processing to try and get the best integrated image. I used a custom expression in SubFrame Selector and graded all the subs based on that expression (using Eccentricity, SNR and FWHM). The integration then used the weighted images (via a FITS keyword) so that the best made the most contribution and the worst, least.
SSRO- RCOS 16", Alta U9, PlaneWave Ascension 200HR, PixInsight 1.8, ACP, MaxIm DL, FocusMax
Object description at www.billionsandbillions.com
IC1848
Vespera Pro 2269x10sec Dual filter from Thun, CH on 7-8 Nov. 2025. Processed with PixInsight.
Messier 78
TS 115/800
ASI ZWO 1600 Mono Cooled
Optolong: LRGB (180 - 35 - 24 - 24)
Processamento: PixInsight + PS6
Testaufnahme mit der Canon 6D
Trotz schlechter Transparenz, recht gutes Ergebnis dabei herausgekommen
distance 444 ly
Equipment:
Skywatcher ED80/600
Skywatcher Reducer x0,85
Canon 6D
Celestron AVX
Guiding:
i-Nova PLA-Mx on 9x50 Finderscope
PHD
30x300s ISO3200
19.01.2017
28.01.2017
total exposure time: 2:30
Processing: PixInsight/Lightroom
Esprit 80/400, ASI2600MM-Pro, Astronomik SHO en 6nm (5h/5h25/4h50 et par brutes de 300"). NINA et Pixinsight.
NGC 281, also known as IC 11, SH2-184, and more commonly known as the “Pacman Nebula,” is an emission nebula located 9,100 light-years away in the constellation of Cassiopeia.
This image results from 8 hours of narrowband data and is rendered in the SHO Hubble Palette.
The initial data was collected over two nights ending on October 22nd. That collection cycle was interrupted due to illness. Three of the projects whose data was collected on those nights had enough integration that I could process the images. However, this one was still pretty short for the S2 filter. So I waited until I had a chance to add to the data set. Finally, on November 23, we had a clear night, and I was able to add about 3 hours more data to this project.
This image was shot on my Astro-Physics 130mm f/8.35 APO telescope platform, which uses a ZWO ASI2600MM-Pro camera, and is supported by an IOptron CEM60 Mount.
When I looked at the data for this project, I discovered a very strange artifact that I have never seen on this platform before - in fact, I have not seen it on any platform. I ended up having a series of concentric circles located in the lower-left corner of the image and a strange mottled noise across the rest of the image field. This pattern was not seen in the flats or the darks and was evident in every sub and master regardless of filters. It was also constant across all three evenings where data was collected.
In dealing with this, I ended up having the background sky much darker than I would have preferred, but all is not bad, as I think it does add to the "Snap" and the drama of the image.
This is also the first image I tried using Bill Blanshan's new SHO Normalization script on.
All details are in the post below.
The full story behind this image, along with a detailed processing walkthrough, can be found at:
cosgrovescosmos.com/projects/ngc281-pacman-nebula-11-23-22
A video of the blink analysis for this data is also available if interested:
Finally, a video on my YouTube channel provides a high-level view of the processing strategy for this image:
Please consider liking and following my fledgling YouTube channel! ( If nothing else you can laugh at my attempts to learn the video side of things!)
Thanks for looking!
Pat