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Constelación en que se encuentra: Escorpión
Distancia: 5500 años luz
Según la NASA, es una nebulosa de emisión ubicada en la constelación de Escorpión, compuesta principalmente de hidrógeno. Es una región activa de formación de estrellas en la que en los últimos millones de años se han formado estrellas que tienen 10 veces la masa del sol.
Datos de la imagen:
Exposure: 1hr 55 min (23 x 5 min)
Telescope: Celestron C9.25 Edge - Hyperstar
Camera: ZWO ASI071MC Pro
Focal ratio: f2.3
Capturing software: NINA
Filter: IDAS NBZ
Mount: iOptron CEM60
Guiding: ASI462MC with PHD2 and Stellarvue F60M3
Dithering: Yes
Calibration: 75 darks, 100 flat darks, 100 flats
Processing: PixInsight
Date: 04-ago-2022
Location: Bogotá, Colombia
The distinctive Sombero galaxy sits at a distance of 29 millionLight years away from us.
This is an image taken as a 'test' in my backyard , It consists of 120sec X26 frames shot through the luminance filter of a highly sensitive CCD camera. The final picture was integrated and processed in Pixinsight.
Capture Software was Sequence Generator Pro, guided with PHD 2.6.1DEV.
Note this is a cropped version of the original (approx 25% of frame)
Wikipedia link here: en.wikipedia.org/wiki/Sombrero_Galaxy
First light for my new lens
1 stack of 19 images, Canon 800D at ISO 800, Takumar 135mm f2.5 lens at f4, 30s exposures, Omegon Lx2 tracking mount. 45 darks, 120 biases. Processed in PixInsight as below
***** Integration
lightvortexastronomy tutorial (www.lightvortexastronomy.com/tutorial-pre-processing-cali...)
* CC defect list + master dark
* weighing: (15*(1-(FWHM-FWHMMin)/(FWHMMax-FWHMMin)) + 15*(1-(Eccentricity-EccentricityMin)/(EccentricityMax-EccentricityMin)) + 20*(SNRWeight-SNRWeightMin)/(SNRWeightMax-SNRWeightMin))+50
* img 1135 reference
* star align - distortion relaxed to 0.3
* integration - winsorized sigma clipping
***** Linear processing
*** Crop
*** DBE, 0.5 tolerance
*** Color calibration
* SNCR 0.5
* Background neutralization (using small area under middle star as sample background - hard to find true neutrality in Orion flickr.com/photos/deepskycolors/16774216742/in/faves-1833...)
* Color calibration w/background and structure detection
*** Deconvolution
* Created star_mask_large - large scale structure 2, small scale 1, noise threshold 0.1, scale 8
* Created range mask - extracted luma, applied standard STF, then histogram shadow = 0.25 mids = 0.3 high = 1
* Deconvolve with range mask on, 100 interations, custom PSF, dark 0.01 bright 0.004, local deringing with star mask, wavelet regularization
*** Star reduction
Small star mask - noise 0.15, scale 4, small scale 3 comp 1, smoothness 8, binarize, midtones = 0.02
Range mask from that, 0.05-1
Apply, erosion operator 2 iterations 0.6 with shape oval
*** Linear noise reduction
jonrista.com/the-astrophotographers-guide/pixinsights/eff...
*TGV - small noise
Created TGV masks - extracted luminosity, standard stretch (luminance_mask), curved it with black point at ~0.2 and white at ~0.5, moved histogram point to middle (tgv_mask)
apply tgv mask inverted to the image, give luma mask as local support
TGV chroma str 7 edge protection 2E-4 smoothness 2 iterations 500
TGV luma str 5 edge protection 1E-5 smoothness 2 iterations 500
*MMT - larger noise and TGV artifacts
Created MMT mask - extract luminosity, standard stretch, move histogram point to 75%, apply low range -0.5. Apply inverted
MMT mask - 8 layers, threshold 10 10 7 5 5 2.5 2 2 on rgb
*****Nonlinear
***Initial stretch
*Autostretch, apply to hist
*Create full star mask, max(star_mask_large, star_mask_small)
* HDR transform, 8 layers, B3 spline, star mask applied inverted, preserve hue, lightness mask
***MLT stretch
www.stelleelettroniche.it/en/2014/09/astrophoto/m42-ngc19...
**Initial
* created a new multiscale linear transform, kept 4 layers using linear interpolation
* diffed from original image to create a "blurred" version of original image
* extracted luminance from original, used as mask on blurred version
* used curves to create s shape in luminance, inflection 3/4 up, and pump up saturation a lot
* pixelmath sum the 3, rescaled, back to original image
**Second
* new multiscale linear transform, keep 5 layers
* diff from original
* extract luminance from blurred image, to use as a mask
* masked blurred image with its own luminance, gave it s-shaped RGB curve, big boost in saturation
* pixelmath sum the 3, rescaled, back to original image
***Star and nebula mask:
Range select to catch nebulas, blur with 3 a troux wavelet iterations (removing first 5 layers), add to star mask to obtain star and nebula mask
***Local histogram equalization
kernel 32 contrast 1.5 amount 0.35, with star and nebula mask on
***Nonlinear NR
*Luminance mask, clipped shadows
*ACDNR stdev 4 chroma 2 luma, amount 0.9 chroma 0.7 luma
***Dark structure enhance
* 5x5, 3 iterations, amount 0.25
*** Sharpen
* Sharpen with multiscale linear transform, bias layers 2-6 (0.05, 0.05, 0.025, 0.012, 0.006)
The Iris nebula, NGC7023.
Camera: QHY23M
Scope: TS INED70mm apo with 0.8x reducer
Focal length: 336mm f/4.8
Exposures:
Luminance - 14 x 600s (bin 1)
R, G, B - 15 x 300s, 10 x 300s, 10 x 300s (all bin 2)
Exposures taken on 14th and 17th May 2018 from Cumbria (UK)
The Great Nebula in Orion (M42) and the Running Man Nebula (NGC 1977), photographed in Narrowband using the Hubble Palette (HST).
M42 is a diffuse nebula situated in the Milky Way, south of Orion's Belt in the constellation of Orion. It is one of the brightest nebulae, and is visible to the naked eye in the night sky. M42 is located at a distance of 1,344 light-years, and is the closest region of massive star formation to Earth.
Why image in Narrowband?
In short, different elements show up in different colors of the spectra in far more detail. See my link to ''A brief description of the Electromagnetic Spectrum of Light'' for more info.
Why go through all the trouble?
“That's the way to learn the most, that when you are doing something with such enjoyment that you don’t notice that the time passes.” - Albert Einstein.
Narrowband wavelengths of the light spectra in this image:
The Hubble Palette (HST)
Hydrogen-Alpha - 656.3nm
Oxygen-III - 500.7nm
Sulfur-II - 672.4nm
RGB Channel Mapping Ratio:
Red: 40% Ha + 60% SII
Green: 40% OIII + 30% Ha + 30% SII
Blue: 100% OIII
PixInsight PixelMath Formula Expression:
R/K: 0.4*Ha + 0.6*SII
G: 0.4*OIII + 0.3*Ha + 0.3*SII
B: OIII
Processing:
Pre-Processing and Linear workflow in PixInsight. PixelMath and Nebula Structure enhancement via Wavelets. Finished in Photoshop.
"Capturing Data is Science, but Processing it is Art".
Astrometry Info:
Annotated Sky Chart for this image.
RA, Dec center: 83.7624970537, -5.30247840247 degrees
Orientation: 1.2575903817 deg E of N
Pixel scale: 5.79732928062 arcsec/pixel
View this image in World Wide Telescope.
Hubble Palette explanation:
www.astronomymark.com/hubble_palette.htm
Narrowband explanation:
www.swagastro.com/narrowband-information.html
My brief description of the Electromagnetic Spectrum of Light:
www.flickr.com/photos/martin_heigan/22278042895
Martin
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M101 / NGC5457 or most commonly known as the Pinwheel Galaxy is a face on spiral galaxy in Ursa Major and has a distance of around 21 million light years from Earth.
The QHY183M picks up quite a lot of the Ha detail in this galaxy without me having to image separate Ha Filter data
Image Details:
101x150S in R
101x150S in G
101x150S in B
Total Capture time: 12.6 Hours
Acquisition Dates: Feb. 27, 2019, March 29, 2019, March 30, 2019, April 1, 2019, April 11, 2019, April 12, 2019, April 14, 2019
All frames had 101 Darks and Flats applied
Equipment Details:
Imaging Camera: Qhyccd 183M Mono ColdMOS Camera at -20C
Imaging Scope: Sky-Watcher Quattro 8" F4 Imaging Newtonian
Guide Camera: Qhyccd QHY5L-II
Guide Scope: Sky-Watcher Finder Scope
Mount: Sky-Watcher EQ8 Pro
Focuser: Primalucelab ROBO Focuser
FIlterwheel: Starlight Xpress Ltd 7x36mm EFW
Filters: Baader Planetarium RGB
Power and USB Control: Pegasus Astro USB Ultimate Hub Pro
Acquisition Software: Main-Sequence Software Inc. Sequence Generator Pro
Processing Software: PixInsight 1.8.6
View of the comet Lovejoy near the Seven Sisters last night. First attempt processing with PixInsight
M101 Pinwheel Galaxy at a distance of 23 million light years. Shot using the new RASA 8 with the trusty ASI071MC. I really enjoyed taking the time to process this deep sky object with PixInsight as the software can be quite challenging. 📷🌌✨
Camera: ASi071MC-Pro
Telescope: Celestron RASA 8
Aperture: f2.0
Focal Length: 400mm (cropped)
Mount: Celestron CGX
Filters: Astrodon RASA LPS
Frames: 29X60sec
Gain: 90 Offset: 20
Camera Temp: -15°C
Bias: 50 frames
Darks: 50 frames
Post Processing: Pixinsight, LR
The North American Nebula (NGC7000). Processed in Pixinsight and Lightroom CC. This is my first deep sky object processed in Pixinsight. Taken from the Rockies of Alberta. 📷🔭🌌
Camera: ASi071MC-Pro
Telescope: Williams Optics Z61, (fl360mm f5.9)
Mount: iOptron SkyGuiderPro
Stack: 33x60sec
Gain: 130 Offset: 50
Temp: -20°C
Darks: 50
Bias: 50
Processing: Pixinsight, LR .
This is one of my final projects for the 2020-2021 season before I take a break over the summer months where the skies don't go completely dark. I love imaging dark nebulae and this is by far my favourite, a target that I have imaged before, but wanted to see how far I could push the exposures when imaging North
RA: 21h59m18.57s
Dec: 71°58'57.40"
Constellation: Cepheus
Designation: LDN 1235
Image Details:
409x150S at Gain 100 - CLS-CCD Filter
Darks: 101 Frames
Flats: 101 Frames
Bias: 101 Frames
Acquisition Dates: March 7, 2021 , March 8, 2021 , March 17, 2021 , March 19, 2021 , April 12, 2021 , April 13, 2021 , April 14, 2021 , April 15, 2021 , April 16, 2021
Total Capture time: 17 Hours
Equipment Details:
Imaging Camera: ZWO ASI6200MC Pro 62mpx Full Frame OSC
Imaging Scope: SharpStar 15028HNT Hyperboloid Astrograph
Guide Camera: StarlightXpress Lodestar X2
Guide Scope: 365Astronomy 280mm Guide Scope
Mount: Sky-Watcher EQ8 Pro
Pier: Altair Astro Skyshed 8" Pier
Focuser: Primalucelab Sesto Senso V2
Filter: Astronomik CLS-CCD 2"
Power and USB Control: Pegasus Astro USB Ultimate Hub Pro
Acquisition Software: Main Sequence Software. Sequence Generator Pro 3.2
Calibration and Stacking: Astro Pixel Processor
Processing Software: PixInsight 1.8.8 and EZ Processing Suite for Star Reduction
IC405 with some additional colour data around AE Aurigae to show the blue reflection nebulosity better.
QHY23 data from previous image, plus:
Camera: QHY163M
Scope: MN190
Focal length: 1000mm f/5.2
Exposures:
19 x 300s H-alpha
8 x 300s Red
3 x 300s Green
5 x 300s Blue
Taken 31.12.2019 from Cumbria (UK)
The Lagoon Nebula (catalogued as Messier 8 or M8, NGC 6523, Sharpless 25, RCW 146, and Gum 72) is a giant interstellar cloud in the constellation Sagittarius. It is classified as an emission nebula and as an H II region. The Lagoon Nebula is estimated to be between 4,000–6,000 light-years away from the Earth. In the sky of Earth, it spans 90' by 40', which translates to an actual dimension of 110 by 50 light years. Like many nebulae, it appears pink in time-exposure color photos but is gray to the eye peering through binoculars or a telescope, human vision having poor color sensitivity at low light levels. The nebula contains a number of Bok globules (dark, collapsing clouds of protostellar material), the most prominent of which have been catalogued by E. E. Barnard as B88, B89 and B296. It also includes a funnel-like or tornado-like structure caused by a hot O-type star that emanates ultraviolet light, heating and ionizing gases on the surface of the nebula. The Lagoon Nebula also contains at its centre a structure known as the Hourglass Nebula (so named by John Herschel), which should not be confused with the better known Engraved Hourglass Nebula in the constellation of Musca. In 2006, four Herbig–Haro objects were detected within the Hourglass, providing direct evidence of active star formation by accretion within it. (Celestron EdgeHD 800, Antlia SHO 3nm, ZWO AM5, ASI2600MM-Pro, ASIAIR, Pixinsight, Photoshop).
2024-10-09
Harney, MD
The Bubble Nebula is an emissions nebula in the constellation Cassiopeia. The star cluster M52 is to the right and just below the Bubble Nebula.
Camera: ZWO ASI2600MC
Guide Camera: QHY5III462
Telescope: Vixen ED80SF F/7.5
Mount: Losmandy G11
Integration time:
91 x 240s =364m (6.06hrs)
No filters
Capture: NINA
Processing: Pixinsight, Affinity
The Elephant's Trunk Nebula or IC 1396 as it is otherwise known, but never with such a wide field of view, at a distance of around 2400 light years from earth and is mainly illuminated by a single bright star. It is thought that this region of space is home to a pretty young star forming region.
This image consists of the same data as the RGB Image but has been processed using my tutorial on creating SHO images from One Shot Colour Cameras which you can read here:
www.stastrophotography.com/creating-a-hubble-palette-imag...
RA: 21h39m00.01s
Dec: 57°29'24.00""
Constellation: Cepheus
Designation: IC1396
Image Details: 128x300S at Gain 100
Darks: 101 Frames
Flats: 101 Frames
Bias: 201 Frames
Acquisition Dates: Nov. 5, 2020 , Nov. 7, 2020 , Nov. 24, 2020 , Dec. 1, 2020 , Dec. 24, 2020 , Dec. 27, 2020
Total Capture time: 10.7 Hours
Equipment Details:
Imaging Camera: ZWO ASI6200MC Pro 62mpx Full Frame OSC
Imaging Scope: SharpStar 15028HNT Hyperboloid Astrograph
Guide Camera: StarlightXpress Lodestar X2
Guide Scope: 365Astronomy 280mm Guide Scope
Mount: Sky-Watcher EQ8 Pro
Focuser: Primalucelab Sesto Senso V2
Filter: Optolong L-eXtreme 2"
Power and USB Control: Pegasus Astro USB Ultimate Hub Pro
Acquisition Software: Main Sequence Software. Sequence Generator Pro 3.2
Calibration and Stacking: Astro Pixel Processor
Processing Software: PixInsight 1.8.8 and EZ Processing Suite for Star Reduction
A cropped narrowband image of the Elephant's Trunk Nebula, a concentration of interstellar gas and dust with-in the much larger ionized gas region IC 1396 (located in the constellation Cepheus), about 2,400 light-years away from Earth.
Gear:
GSO 6" f/4 Imaging Newtonian Reflector Telescope.
Baader Mark-III MPCC Coma Corrector.
Celestron SkySync GPS Accessory.
Orion Mini 50mm Guide Scope.
Orion StarShoot Autoguider.
Celestron AVX Mount.
QHYCCD PoleMaster.
Celestron StarSense.
Aurora Flatfield Panel.
Optolong 36mm SHO filters.
QHYCFW2-M-US Filterwheel (7 position).
QHY163M Cooled CMOS Monochrome Astronomy Camera.
Lights/Subs:
Ha = 24 x 420 sec.
SII = 24 x 420 sec.
OIII = 24 x 420 sec.
Camera Settings:
Gain = 17 (equivalent to 170 now)
Offset = 70
CMOS Cooled to -25°C
Calibration Frames:
50 x Bias/Offset.
25 x Darks.
20 x Flats and Dark Flats.
Image Acquisition:
Sequence Generator Pro via the Mosaic and Framing Wizard.
Plate Solving in SGP via the Astrometry.net ANSVR Solver.
Autoguiding via Open PHD Guiding.
Processing:
Pre-Processing and Linear workflow in PixInsight,
and finished in Photoshop.
Wavelengths of the Electromagnetic Spectrum of Light:
Hydrogen-Alpha (656.3nm)
Oxygen-III (500.7nm)
Sulfur-II (672.4nm)
PixelMath:
Mapped Color Channel Combinations.
R = (0.5*SII)+(0.5*Ha)
G = (0.2*Ha)+(0.8*OIII)
B = OIII
Astrometry Info:
View an Annotated Sky Chart for this image.
Center RA, Dec: 323.737, 57.633
Center RA, hms: 21h 34m 56.902s
Center Dec, dms: +57° 37' 59.929"
Size: 46.8 x 60.6 arcmin
Radius: 0.638 deg
Pixel scale: 2.02 arcsec/pixel
Orientation: Up is 268 degrees E of N
View in the World Wide Telescope.
Martin
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44 subs de 600s
101 darks
301 offsets
Pas de Flats
Calibration : PixInsight
Traitement : PixInsight et Photoshop
Askar 130mm f7.7 Quad refractor w/.8 reducer @700mm f/5.5. Zwo Asi 1600 Zwo EFW, Zwo filters. Zwo EFM. Zwo 120 guide cam. Ioptron 45pro mount. AsI Air. 4 frame mosaic total 36 hrs integration. RGB stars. Pixinsight RC Astro Photoshop.
This image is taken from the heavily light polluted sky of Stockholm. Bortle9. About 3 hours of data with my WO Magrez90 telescope and a ZWO ASI294MM pro camera.
The Coma Cluster of Galaxies is one of the densest clusters known - it contains thousands of galaxies. It lies about 330 million light-years away, about seven times farther than the Virgo cluster, in the direction of the constellation Coma Berenices. The main body of the Coma cluster has a diameter of about 25 million light-years, but enhancements above the background can be traced out to a supercluster of a diameter of about 200 million light-years.
Almost every object in photographs of this cluster is a galaxy. Each of these galaxies houses billions of stars - just as our own Milky Way Galaxy does. The Coma Cluster is one of the first places where observed gravitational anomalies were considered to be indicative of unobserved mass.
Pleiades wip - 122 minutes of subs ranging between 15 and 120s. C9.25, Hyperstar + QHY8L OSC CCD. Unguided. Processed in Pixinsight.
Here is my SHO version of the Bubble Nebula, I captured the final SII and OIII last night
Image Details: 20x600S in SII, HA and OIII
HA used as Luminance Layer
SII Mapped to Red
HA Mapped to Green
OIII Mapped to Blue
25 Darks and Flats applied to all frames
Data was catpured on the following dates:
Aug. 16, 2016
Aug. 17, 2016
Oct. 2, 2016
Dec. 22, 2016
Dec. 26, 2016
Dec. 28, 2016
Jan. 2, 2017
Jan. 19, 2017
Jan. 20, 2017
Equipment Details-
Mount: Sky-Watcher EQ8 Pro
Imaging Scope: Sky-Watcher Quattro 8-CF F4 Imagine Newtonian
Imaging Camera: Atik Cameras 383L+ Mono CCD Cooled to -20C
Guide Scope: Celestron Telescopes C80ED Refractor
Guide Camera: Qhyccd QHY5L-II
Filter Wheel: Starlight Xpress Ltd 7x36mm EFW
Filters: Baader Planetarium 7nm HA, OIII and SII 36mm Unmounted
Stacking and Combining: Maxim-DL
Processing: PixInsight
This is some existing data I had that I've reworked in Pixinsight using some different noise reduction methods which worked pretty well. Also took the opportunity to alter the RGB and Ha channels slightly to get a different effect.
Data taken in my back yard with the following equipment:-
Explore Scientific Triple ED80 - 80mm Refractor
ATIK 314L+ Mono CCD
Orion Star Shoot Auto Guide Camera
EQ5 Mount
LRGB & H-Alpha (7nm) Baader Filters (Auto SX Filter Wheel)
Capture Software: MaxImDL
Process Software: Pixinsight & Adobe Lightroom
Guide Software: PHD2
Camera was ZWO ASI120MC-S on my TS 65QAPO telescope. Avi video processed in PIPP Registax. ISS and starfield processed seperatly as different exposure. Pixinsight and PS used.
I have attempted this type of shot a few times now but always failed. There are so many things to get right and little margin for error. Most times I have ended up chasing the ISS with my eye in the finder. Hard do and doesn't give a stable platform. Add to that my capture software seems a bit hit and miss and keeps locking up I have felt like this target was my Nemisis. I have got a few DSLR long exposure trails but I wanted a single detail frame with some stars around if possible.
So I needed to think up a strategy. I then noticed that tonights pass would go close to M13 which is a very easy target to see. The app skyguide, gave me all the info I needed. I fast forwarded the app to 23:20 and could clearly see the ISS track almost clipped one of the two distinctive stars either side of M13. All I had to do was hide in wait at that location with telescope camera and laptop. Easy!
Well not really still a lot to get right. Based on other attempts I nudged the exposure down. My capture software showed about 45 frames per second (USB 3) so if that maintained it would be good. This was on a setting that gave me 1280 x 750 as I conceded a slower frame rate was better than missing the target with a smaller image but higher frame rate.. As it turned out, I had 16 frames with ISS in and I couldn't really have hoped for more. To focus I wanted the closest thing I could get. Moon wasn't available so my focus was on Jupiter. I set the software up to record x1 60 second clip. I had tried repeat clips previously but software didn't carry that out instead it locked up! All ready to go then. All I need is ISS. Sky was staying clear without a hint of cloud on any horizon.
First sight was just left of Jupiter. Here it comes I better get inside the obsy.
The way the track went I couldn't see the early part until it was clear of Leo. But my observatory slot is quite big and I saw it come into view well before it was close to Hercules where M13 is. Didn't want to click start on software to early as it would run for 1 minute.. I estimated about 30 seconds before it gets in my scope and I clicked start.. Horror! Nothing happend! Shit software let me down. Clicked again and it started. 😳 pheww!,
Nothing else I could do now.. So I picked up my binoculars and found M13 easily. Watched it! And there it was whizzing by. Just as predicted. So bright was the ISS that I momentarily lost sight of M13. Made me wonder if I had overdone the exposure.. After 1 minute the recording stopped. I now turned the exposure right up and did a clip of the star field as I wanted to put that into my picture later.. Here is the result. I hope you like it.
Funny to think that as I photographed this the crew were packing up ready for their departure in a couple of days. "safe trip back guys"
Processed in PIPP, Registax, Pixinsight and PS
If anybody has any tips on how I would achieve a better focus on the ISS itself please let me know. If I could just improve that I think my result would be a whole lot better. I think its trial and error time but happy to hear from you.
Sadr Star rises early in the morning on the back of the Milky Way. Early season wide field work on the portable SkyGuiderPro and trusty DSLR/135mm lens. I am really enjoying the reds hitting the camera sensor thanks to the modification I had done by LifePixel IR. ✨🔭
Camera: Nikon D5600a
Lens: Rokinon 135mm f/2 @ f3.2
Mount: iOptron SkyGuiderPro
Frames: 49 frames @ 60sec
ISO: 400”
OAT: 11°C
Bias: 30 frames
Darks: 50 frames
Post Processing: PixInsight, PS, LR
LDN 1235 or the Dark Shark Nebula is a patch of dark nebulosity in the constellation of Cepheus, the dark nebulosity spans across for around 15 Light years
The image consists of
51x300S in Red, Green and Blue totalling 12.8 Hours
Darks, Flats and Dark Flats have been applied
Acquisition Dates: Sept. 20, 2019, Sept. 27, 2019, Sept. 28, 2019, Sept. 29, 2019, Oct. 2, 2019, Oct. 27, 2019
Equipment Details:
Imaging Camera: Qhyccd 183M Mono ColdMOS Camera at -20C
Imaging Scope: SharpStar 15028HNT F2.2 Hyperboloid Astrograph
Guide Camera: StarlightXpress Lodestar X2
Guide Scope: Sky-Watcher Finder Scope
Mount: Sky-Watcher EQ8 Pro
Focuser: Primalucelab ROBO Focuser
FIlterwheel: Starlight Xpress Ltd 7x36mm EFW
Filters: Astronomik RGB Fast Focal Ratio 36mm Filters
Power and USB Control: Pegasus Astro USB Ultimate Hub Pro
Acquisition Software: Main Sequence Software. Sequence Generator Pro
Processing Software: PixInsight 1.8.6
2nd and possibly final colour version of M101. This image contains all the data from my previous process plus, another 2.5 hours of luminance shot with the IDAS light pollution filter in place. The IDAS makes a huge improvement in my LRGB subs and I would recommend trying one if you have urban light pollution like myself.
Imaging times;
Luminance 7.5 hours in 5 minute subs
RGB - 4.5 hours (total) in 5 minute subs
Total imaging time 12 hours.
Imaged with an Altair Astro 6" RC & Atik 314l+ processed in Pixinsight & CS5.
15x 120sec exposures
Stacked in DeepSkyStacker
Edited in Pixinsight and Lightroom
Shot with Nikon D600 and ioptron skytracker
NGC 7822 is a young star forming complex in the constellation of Cepheus.
The complex encompasses the emission region designated Sharpless 171, and the young cluster of stars named Berkeley 59.
The complex is believed to be some 800-1000 pc distant (3,000 light years), with the younger components aged no more than a few million years.
The complex also includes one of the hottest stars discovered within 1 kpc of the Sun, namely BD+66 1673, which is an eclipsing binary system consisting of an O5V that exhibits a surface temperature of nearly 45000 K and a luminosity ~100,000 times that of the Sun.
The star is one of the primary sources illuminating the nebula and shaping the complex's famed pillars of creation-type formations, the elephant trunks.
(Description credits: Wikipedia)
Technical card
Imaging telescope or lens:Teleskop Service TS Photoline 107mm f/6.5 Super-Apo
Imaging camera:ZWO ASI1600MM-Cool
Mounts:Skywatcher AZ EQ-6 GT, Astro-Physics Mach-1 GTO CP4
Guiding telescope or lens:Celestron OAG Deluxe
Guiding camera:QHYCCD QHY5III174
Focal reducer:Riccardi Reducer/Flattener 0.75x
Software:Main Sequence Software Seqence Generator Pro, Astro-Physics AAPC, Pleiades Astrophoto PixInsight
Filters:Astrodon HA 36mm - 5nm, Baader Planetarium Ha 1.25" 7nm, Astrodon S-II 36mm - 5nm, Astrodon O-III 36mm - 5nm, Astrodon B Gen.2 E-series 36mm, Astrodon G Gen.2 E-series 36mm, Astrodon R Gen.2 E-series 36mm, Baader Planetarium OIII 1.25" 8.5nm, Baader Planetarium SII 1.25" 8nm
Accessories:ZWO EFW, MoonLite NiteCrawler WR30
Resolution: 1696x2276
Dates: Oct. 13, 2017, Oct. 14, 2017, Sept. 20, 2018, Sept. 22, 2018, Sept. 23, 2018, Sept. 24, 2018
Frames:
Astrodon B Gen.2 E-series 36mm: 15x5" (gain: 200.00) -20C bin 1x1
Astrodon G Gen.2 E-series 36mm: 15x5" (gain: 200.00) -20C bin 1x1
Astrodon HA 36mm - 5nm: 56x300" (gain: 200.00) -20C bin 1x1
Baader Planetarium Ha 1.25" 7nm: 50x120" (gain: 200.00) -20C bin 1x1
Baader Planetarium Ha 1.25" 7nm: 25x180" (gain: 200.00) -20C bin 1x1
Astrodon O-III 36mm - 5nm: 21x300" (gain: 200.00) -20C bin 1x1
Baader Planetarium OIII 1.25" 8.5nm: 17x120" (gain: 200.00) -20C bin 1x1
Astrodon R Gen.2 E-series 36mm: 15x5" (gain: 200.00) -20C bin 1x1
Astrodon S-II 36mm - 5nm: 15x300" (gain: 200.00) -20C bin 1x1
Baader Planetarium SII 1.25" 8nm: 16x180" (gain: 200.00) -20C bin 1x1
Integration: 12.0 hours
Avg. Moon age: 16.28 days
Avg. Moon phase: 73.22%
Astrometry.net job: 2281894
RA center: 0.897 degrees
DEC center: 67.148 degrees
Pixel scale: 2.931 arcsec/pixel
Orientation: 1.157 degrees
Field radius: 1.155 degrees
Locations: Berga Resort, Berga, Barcelona, Spain
Data source: Backyard
Distance: ca. 2,000 Lj
Equipment:
TS 10" f/4 ONTC Newton
1000mm f4
ZWO ASI585MC
Skywatcher EQ8
Guding:
Lodestar on TS Optics - ultra short 9mm Off Axis Guider
PHD2
600x30s
Gain 252
5 hours total integration time
June 2023
Processing: PixInsight
In order to trial the famous Blur/Noise/Star-Xterminator plugins for PixInsight, I decided to look at images I captured in July 2020 while testing my newly-acquired Nikon 600mm F4 lens.
Needless to say that these 3 scripts take your images to the next level especially when this is only 6 subs (3x 3' + 3x 2') at 1020mm F6.7 and autoguiding was struggling to control my NEQ6 mount!
Here is the cropped starless version, then tweaked using the usual PixInsight tools + BlurX and NoiseX.
I don't usually like starless images where I find stars do add to the richness of the field of view, but for once I could not resist ... O:)
My first RGB Image from the Qhyccd 183M 20mpx Back Illuminated ColdMOS Camera, I will be writing part 2 of the review soon, so here's what I hope is one of many images taken with this awesome camera
Gear:
Imaging Scope: Sky-Watcher Quattro 8" F4 Imaging Newtonian
Imaging Camera: Qhyccd 183M 20mpx ColdMOS Camera at -20C and DSO Gain
Mount: Sky-Watcher EQ8 Pro
Guide Camera: Qhyccd QHY5L-II Mono
Guide Scope: Sky-Watcher 50x90 Finder Scope
Filter Wheel: Starlight Xpress Ltd 7x36mm EFW
Filters: Baader Planetarium 36mm RGB
Coma Corrector: Sky-Watcher Aplanatic Coma Corrector
Image Acquisition: Main Sequence Software SGPro
Image Processing: PixInsight
Image Details:
Target: IC434 - Horsehead Nebula
Constelation: Orion
Red: 19x300S
Green: 19x300S
Blue: 19x300S
Darks: 51x300S
Flats: 101
Bias: 251 converted to SuperBIAS and deducted from Flats
PixInsight Image processing workflow:
1. Calibrated against darks and Bias Subtracted Flats
2. Star Alignment
3. Least noise frame from each colour chosen as Normalization Frame and Dynamic Background Extraction Performed
4. Normalization of all frames
5. Stacking of frames and generation of drizle data (for larger quality image in future)
6. Performed LinearFit using Red stacked image as reference
7. Performed MultiMedianTransformation to reduce background noise
8. Performed SCNR to remove excessive green in image
9. Stretched the image using HistogramTransformation
10. Performed a CurvesTransformation to bring out the star colour
Right now I have not performed any Sharpening of the image, nor have I added the Ha data to this image, I'll post an updated image when I get round to doing that
Image from 2 March 2023
First steps with PixInsight and the fabulous plugin RC-Astro.
Stacked with Astro Pixel Processor (stack 95%)
Pictures combined with Astro Pixel Processor (SHO-3)
Image Processing:
Astro Pixel Processor (Removing light pollution)
PixInsight and plugin RC-Astro.
SHO: Blur Xterminator – Noise XTerminator – Star XTerminator
Ha: Blur Xterminator – Noise XTerminator
Fitswork combined HaSHO and Image stretching
ATIK 460EX
TS 80/560 F7 Reducer/Flattener 0,8x
Ha 97 x 5min
OIII 95 x 5min
SII 125 x 5min
Total exposure time 26h25min
Had yet another go at processing my ancient data. Slightly less aggressive crop than before and took a bit more time on curves adjustment in Pixinsight. Might have slightly overdone the star reduction as they look a bit sharper/more artificial than the nebula. Anyway I continue to be blown away with what can be dragged out of a mere four hours of integration on a 15 year old camera.
Constelación en que se encuentra: #Cassiopeia
Distancia: 9800 años luz
Sharpless 2-101 (Sh2-101) es una nebulosa que resultó como consecuencia de la explosión de una estrella como super nova, en la constelación de Cassiopeia.
Se piensa que un pulsar en el centro emite ondas de rayos X.
Datos de la imagen:
Exposure: 11hr 9min (223 x 3min)
Telescope: #Celestron #EdgeHD #C925 #Hyperstar
Camera: ZWO #ASI2600MC Pro
Focal ratio: f2.3
Capturing software: NINA
Filter: IDAS #NBZ
Mount: #iOptron #CEM60
Guiding: #ASI462MC with #PHD2 and Stellarvue F60M3
Dithering: Yes
Calibration: 30 darks, 30 flat darks, 50 flats
Processing: #PixInsight
Date: 14-sep-2024, 1-oct-2024
Location: #Bogotá, #Colombia
Re-edit of this mosaic using PixInsight 1.8
2-tile mosaic covering the Pipe Nebula and most of "The Kiwi", plus a bit of Sagittarius showing Messier 8 and 20. And as a bonus, Saturn is the bright one bottom centre. :-P
Later in the season I hope to shoot 2 more tiles above, below and to the left of this image, covering a nice big chunk of this amazing region of the sky.
Each tile is a stack of 10 x 180s images shot at 120mm focal length, F4.5 and 640ISO.
Humidity was very high, and for the last few shots I was in thickening fog moving down from the hills ...
CLICK ON THE IMAGE TO VIEW IT IN FULL RES
3x3 tiles mosaic ; every tile is composed by 9x1200" frames
Total exposure 27hrs.
T:Takahashi FSQ 106ED @f/3,65 w 0.73x focal reducer
M: Astrophysics Mach1 GTO
C: QSI 690ws-g8
G: QHY-MZ5m
F: Astronomik 6nm Ha.
Foc: Sharp Sky Pro foucser
CPU: Eagle Primalucelab
Sw: Sequence Generator Pro - PHD2 - Pixinsight 1.8
Ha:9x 1200"; 3x3 tiles mosaic
Bias: 31
Dark: 31
Flat: 50
This is the first time I have ever imaged this object, I will re-visit next year when I will image at F2.8 with a wider field of view using a keller reducer.
Since this object is in the southern area of sky, I am limited by trees and the house on the data I can capture in a single night
Image Details:
101x150S - Red
101x150S - Green
101x150S - Blue
101 Darks, Flats and Dark Flats
Image Acquisition Dates: Jan. 1, 2019, Jan. 2, 2019, Jan. 8, 2019, Jan. 9, 2019, Jan. 27, 2019, Jan. 28, 2019, Jan. 30, 2019, Feb. 10, 2019, Feb. 20, 2019, Feb. 23, 2019, Feb. 24, 2019, Feb. 25, 2019
Equipment Used:
Imaging Camera: Qhyccd 183M Mono ColdMOS Camera at -20C
Imaging Scope: Sky-Watcher Quattro 8" F4 Imaging Newtonian
Guide Camera: Qhyccd QHY5L-II
Guide Scope: Sky-Watcher Finder Scope
Mount: Sky-Watcher EQ8 Pro
Focuser: Primalucelab ROBO Focuser
FIlterwheel: Starlight Xpress Ltd 7x36mm EFW
Filters: Baader Planetarium RGB and Ha
Power and USB Control: Pegasus Astro USB Ultimate Hub Pro
Acquisition Software: Main-Sequence Software Inc. Sequence Generator Pro
Processing Software: PixInsight 1.8.6