The Wizard Nebula is an emission nebula that surrounds the open star cluster NGC 7380 in the constellation Cepheus. The nebula is known for its unique shape, resembling the appearance of a medieval sorcerer. The active star forming region lies at a distance of 7,200 light years from Earth and has an apparent magnitude of 7.2. It has a radius of 100 light years and occupies 25 arc minutes of the apparent sky. It has the designation Sh2-142 in the Sharpless catalog of H II regions.

Taken 23 June 2020 and 8,9,10 July 2020. Moon was minimal, early setting and low in the sky on these dates.

I was having trouble with movement in the optical train, now fixed with a better focuser, so framing not so good as I didn’t want to rotate the camera and filter wheel to one side. Will do next time around. Also, my focal length has walked during collimation so focus is not optimal and focal plane is tilted. Currently working on that issue to optimise the whole setup. Will invest in a Howie Glater laser collimator to help with that.

300s light frames totalling 8.6 hours SHO Narrowband, blended with a Foraxx pallet 50:50 mix using Pixelmath in Pixinsight.

Astromiks 36mm SHO 6nm Filters

30 x Darks, Flats (for each filter) and Dark Flats

ZWO ASI294MM Pro 120 gain, -10C

ZWO 7x36mm EFW

ZWO EAF

Stellalyra 8” Ritchey-Chrétien Carbon

HEQ6

ASIAIR Plus

Astro Pixel Processor

Pixinsight

Photoshop 2022

Orion Nebula. D5300 Nikon 500mm Catadioptric Mirror Lens. 30sec f/8 ISO 400.

Captured in Astro Photography Tool. 140 Lights, 30 Darks, 30 Flats, 30 Bias frames. LR, AstroPixelProcessor, PS. Sky-Watcher Star Tracker.

The Veil Nebula is a cloud of heated and ionized gas and dust in the constellation Cygnus. It constitutes the visible portions of the Cygnus Loop (radio source W78, or Sharpless 103), a large but relatively faint supernova remnant. The source supernova exploded circa 3,000 BC to 6,000 BC, and the remnants have since expanded to cover an area roughly 3 degrees in diameter. The distance to the nebula is not precisely known, but Far Ultraviolet Spectroscopic Explorer (FUSE) data supports a distance of about 1,470 light-years. (en.wikipedia.org/wiki/Veil_Nebula)

22 hrs RGB captured for this 2 panel Mosaic between 17 april and 18 June 2018 with Esprit 100 refractor/QHY16200 @-20C. Stacking/mosaic in AstroPixelProcessor, further processing in Pixinsight.

Knight Observatory, Tomar

[Explore 20180703]

29-04-2017 - 04:00 aprox. GMT -3

Star Adventurer

Canon 6D - Canon 50mm f/1.4 USM @ f/4

ISO 1600 - 5150K - 120s - DF 50mm

46 lights, 17 darks, 29 flats y 300 bias

Procesado: AstroPixelProcessor y Lightroom

M101

Planewave - CDK 431mm - FLI

L = 22*300s

RGB = 10 * 300s bin2

Ha = 13 * 600s

AstroPixelProcessor

Pixinsight

Affinity Photo

Dati: 17 x 480 sec ( 2.27ore) gain 5 @ -10° c + 36 dark + 30 flat e darkflat

Filtro: Astronomik UV/IR Block L2

Montatura: EQ6 pro

Ottica: Takahashi FSQ106

Sensore: QHY168C

Cam guida e tele: asi120mm su Scopos 62/520

Software acquisizione: nina e phd2

Software sviluppo: AstroPixelProcessor e Photoshop

Temperatura esterna: 10 ° C - Umidità 45%

53x6-min.

The red emission Nebula called Cygnus Wall is the part of the North America Nebula (NGC7000) that resembles Mexico/Central America. The region is characterized by dark nebulas and dust lanes that give the scenery a dramatic attitude.

The image was made with a standard unmodified Pentax K3ii on a TS 130/910 refractor with 0.79x reducer. The blue/ red colors were generated by separating magenta and red in postprocessing and shifting the magenta more and more to light blue. The now blue colors should represent OIII emission regions while the red colors come from Hydrogen alpha emissions.

39 x 300 s exposures @ ISO 200.

Astropixelprocessor and Photoshop CC2018

This is a panorama of the wonderful "Heart and Soul Nebula". The session was split in three separate panels, recording about two hours data with the RASA 8 for each. Captured with the IDAS NBZ Duo-Narrowband-Filter (Ha & OIII), processed as a bicolor image. RGB stars were recorded in a seperate session. I tried to bring out as much detail and structure as possible (especially in the area around the heart nebula) and to make the colors "pop"! Hope you like it!

Celestron RASA 8

Celestron Motorfocus

IDAS NBZ Filter

EQ6-R Pro

ZWO ASI 2600 MC Pro (Gain 100, Offset 18, -10°)

30 x 240 secs pro Panel

N.I.N.A., Guiding: ZWO ASI 462MC and PHD2

Astropixelprocessor, Photoshop, Pixinsight

Dati: 102 x 300 sec ( 8,5 ore) gain 5 @ -15° c

Filtro: Astronomik UV/IR Block L2

Montatura: EQ6 pro

Ottica: Takahashi FSQ106

Sensore: QHY168C

Cam guida e tele: magzero Mz5m su Scopos 62/520

Software acquisizione: nina e phd2

Software sviluppo: AstroPixelProcessor e Photoshop

Temperatura esterna: 16 ° C - Umidità 60%

The Great Orion Nebula is an enormous cloud of dust and gas where large numbers of new stars are being formed. It's bright central region, the Trapezium cluster, is home to four massive young stars that help shape the nebula.

Orion is estimated to be around 24 light years across and has a mass of about 2,000 times that of our Sun. It lies about 1,350 light years away from Earth.

🌀🌠🌌🌟

Image Information

Telescope: Tele Vue NP127fli Refractor | f5.6

Camera: FLI Proline 16803 CCD

Mount: 10Micron 2000 HPS

Exposure Details: L 6 x 300 sec, RGB 13 x 300 sec, Ha 6 x 600 sec

Observatory: Siding Spring, NSW, Australia

Date Taken: October - December 2018

Post-Processing: AstroPixelProcessor, PS

Thank you to Tele Vue Optics for featuring this image in their recent blog: bit.ly/2V8CgiC

This image shows the extended nebulosity around IC59/IC63. This nebulosity is very rarely found on imagery, and as far as I know only a handful of images showing this nebulosity can be found, where most of them only show a very weak impression of the nebulosity. With this image I hope to challenge people to image this beautiful region and maybe even bring out more details. It's really worth it!

The image was processed with astropixelprocessor and after that the starnet++ script in pixinsight was used to separate the stars from the nebulosity. Using Niktools the nebulosity was sharpened and stretched to show more detail in the final image.

Telescope: tmb92ss

Camera: qsi583ws

Exposure: 183x900s (46 h) with an astrodon 5 nm H-a filter

Here is the continuation of my large summer-2018 project.

I had imaged this region for about 13 nights altogether between July and October 2018. You can call me crazy, using so many nights for just one object, in a region where clear nights are rare :) But I really wanted to see if I could catch this beautiful Supernova remnant, and I'm glad it succeeded :)

Recently Pixinsight was supplied with the new Starnet++ module, which you can use to completely separate the stars from the background. I used this software to enhance the very weak nebulosity and was astonished to see how much more could be drawn from the background compared to the processing I did last year. All other processing was performed using Astropixelprocessor and photoshop.

Supernova remnants (SNR) are formed when a large star ends its life in a supernova explosion. About 300 of these remnants are currently known in our galaxy. One of the most famous remnants, the Veil Nebula, is located in the constellation of Cygnus. Although this is the most famous one in this constellation, it’s not the only SNR. Cygnus contains several obscure SNR’s, among which SNR 65.3+5.7 (also known as SNR 65.2+5.7).

SNR G65.3+5.7 was discovered by Gull et al. (1977) during an OIII survey of the Milky Way. Some parts of this SNR were already catalogued by Stewart Sharpless in his SH2 catalog as SH2-91, SH2-94 and SH2-96, but they were not recognized as being part of a bigger structure at that time. The idea that they could be part of a larger SNR was postulated by Sidney van den Bergh in 1960, but it took until 1977 for this to be confirmed.

This is one of the larger SNR in the sky spanning a region of roughly 4.0x3.3 degrees. Mavromatakis et al. (2002) determined the age of the SNR to be 20.000-25.000 years and the distance about 2.600 – 3.200 lightyears. The shell has a diameter of roughly 230 lightyears! This SNR is a predominantly OIII shell with also some H-alpha signal.

This supernova shell is quite weak and there are hardly any high-resolution images of this region. In the internet maybe 5-10 deep images of this shell can be found and, in most cases, they don’t cover the entire shell or the resolution is quite low because it was done by using photo lenses at short focal lengths. That’s why I decided to see if I could try to image the entire shell using my equipment, a TMB92 refractor in combination with a QSI583ws ccd camera. Because of its large size I needed to make a 3x3 mosaic to cover the whole region.

As so many nights were already necessary to cover the region in OIII I didn’t succeed in grabbing the H-alpha data, but on the internet I found the MDWsurvey (mdwskysurvey.org) initiated by David Mittelman (†), Dennis di Cicco, and Sean Walker (MDW). This is a marvelous project with the goal to image the entire northern sky in H-alpha at a resolution of 3.17”/pixel. I contacted them and told them of my effort to grab imagery of this SNR and they were very kind to provide me with the H-alpha imagery of this region, so that the entire SNR could be brought into view in reasonable high resolution.

This bicolor image shows a combination of about 53h of OIII data (made by myself) and 20 hours of Ha-data (made by the MDW survey) in a single image. In this way the full span of the shell can be seen in all its glory.

Image info:

H-alpha (astrodon 3nm, mdwskysurvey.org):

Telescope: Astro-physics AP130mm starfire

Camera: Fli Proline 16803

5 frames of 12x1200s each

OIII (astrodon 3nm):

Telescope: TMB92SS

Camera: QSI583ws

9 frames, 158 x 1200s total

After many months of struggling to get my equipment to work remotely, I think the system is now working reliably, unfortunately, the Moon was hanging nearby for my test subject on 26/02.

I'm not 100% with this image of M42 yet, still getting used to Astropixel Processor and post-production with my own images but I thought I would post anyway.

Images:

50 x 12 sec Red

50 x 12 sec Green

50 x 12 sec Blue

Total integration time: 30 minutes

Calibration files

100 darks

100 bias

100 flats

Stacked in AstroPixelProcessor

Processing in AstroPixelProcessor

Equipment:

Telescope: Skywatcher 120ED Pro

Focal reducer: Skywatcher 0.85x reducer/field flattener

Mount: Skywatcher HEQ5 Pro

Camera: Atik 314L+ Mono cooled to Temp degrees

Focuser: PrimaLuceLab ESATTO2

Guidescope: PrimaLuceLab 60mm

Guide camera: ZWO 120mm mono

Controller: PrimaLuceLab Eagle 2

Sequencing software: N.I.N.A.

The constellation Orion is beginning its winter trek across the sky. One of many gems in that area of the sky is the amazing complex near the bright star Zeta Orionis, one of the three stars in Orion's belt. Here are the Horsehead Nebula, a.k.a. Barnard 33, and the Flame Nebula, a.k.a. NGC 2024, among other, smaller features.

November 12, 2021. 1x3 mosaic, each panel 8 6-minute exposures (2.4 hours total). Explore Scientific FCD-100 102mm telescope, ASI294MC camera, dual narrow-band filter (H-alpha, [O III]), iOptron CEM25P mount, ASIAir controller, processed in Astro Pixel Processor and Lightroom.

Comet C/2023 P1 (Nishimura) September 3, 2023. This comet is bright enough to photograph with a small telescope and should be visible in binoculars (I didn't try until the sky was too bright so didn't see it), but not naked eye. The nice, long, straight tail stretches nearly to the corner of this frame.

Composite of 20 exposures, 2 minutes each. Explore Scientific ED102 102mm f/7 apochromat, ZWO ASI294MC Pro cooled CMOS camera, ZWO UV/IR cutoff filter, Losmandy GM811G mount, ASIAir Pro controller, autoguided. Processed in Astro Pixel Processor, Lightroom, Photoshop

45x240s, 200-500mm f/5.6 @500mm

25x 600 seconds Ha+14x 300seconds Red, 13x 300 seconds Green and 13x 300 seconds Blue (total integration 7.5 hrs). Processed with APP and Pixinsight with minimal steps. (NBRGB Combination,Histogram+Curves). 17,18,19 and 20 November 2017.

Esprit 100 f5.5/QHY16200CCD @ -20

Knight Observatory, Tomar

The Hyades star cluster is the head of the bull in the Taurus constellation; Aldebaran, the brightest yellow star, is the eye. Quite a few dark nebulae are also present in this extent, as well as star cluster NGC 1647 in the upper left.

I normally wouldn't have astrophotographed on a night forecast to have only a small window of clear skies, but it had been a couple months since I had been able to image, so I went for it. I only managed 20 minutes of data without high, thin cloud cover despite shooting for well over an hour, but you have to take what you can get during winter in north Idaho. I'm going to shoot this one again sometime.

Fujifilm X-T10, Samyang 135mm f/2.0 ED UMC @ f2.0, ISO 1600, 20 x 60 sec, tracking with iOptron SkyTracker Pro, stacking with DeepSkyStacker, editing with Astro Pixel Processor and GIMP, taken on Jan. 21, 2020 under Bortle 3 skies.

The Cygnus Loop (a.k.a. Veil Nebula) in the constellation Cygnus, the remnants of a supernova explosion in which a star blew itself apart after exhausting its primary nuclear fuels.

A mosaic of 150 exposures, 300 sec. each in two overlapping fields in the light emitted by hydrogen, oxygen, and sulfur gas, rendered in red, blue, and green, respectively. Explore Scientific ED102 0.1m f/7 refractor, Stellarvue 0.8x reducer/flattener, ZWO ASI294MC camera, 7nm H-alpha, 7nm [O III], 6.5nm [S II] filters, iOptron CEM25P mount, ASIAir controller, autoguided. Processed in Astro Pixel Processor and Lightroom.

This is the full Messier 42 (etc) view also showing the NGC1999 region at lower right.

High Dynamic Range (HDR) techniques have been used to compress the dynamic range. 3 stacks made with 30, 120 and 600 second exposures (488 in total) with a total integration time of 24.6 hours. The stacks have been combined using HDRCombination in Pixinsight and further processsed with HDRMultiscaletransform and other processing steps.

Esprit 100 f5.5/ QHY16200 CCD @ -20C

Image dates:11,12,13,15,16,17,18 & 19 dec 2017 and 14,15,17,18& 19 jan 2018

25x600 seconds, Esprit 100 f5.5/QHY16200 @-20C. (This is a detail from a 72 panel Orion Mosaic i am working on.)

Knight Observatory, Tomar

Part of the supernova remnant known as the Veil Nebula or Cygnus Loop. The result of a star that blew itself apart in a gigantic explosion several thousand years ago.

60 300 sec. exposures (5 hours total exposure), Celestron C5 with f/6.3 focal reducer/corrector (900mm focal length), ZWO ASI294MC Pro camera, dual narrow-band filter (H-alpha+[O III]), ZWO ASIAir controller, iOptron CEM25P mount, processed in AstroPixelProcessor and Adobe Lightroom.

What a joy to capture the spectacular "Jellyfish Nebula" in Gemini with the 2600MC and the RASA 8! I just love the nebula's shape, color and structure! I spent two nights on capturing Ha and OIII with the IDAS NBZ dualband filter and RGB stars without filter. Hope you like it!

Celestron RASA 8

Celestron Motorfocuser

EQ6-R Pro

ZWO ASI 2600 MC Pro (Gain 100, Offset 18, -10°)

RGB: 53 x 120" (1h 46')

Ha & OIII: 73 x 240" (4h 52')

Darks, Flats, Darkflats, Dithering

Guiding: ZWO ASI 120MM & PHD2

N.I.N.A., Astropixelprocessor, Photoshop, Pixinsight

A stereo pair of Comet C/2021 A1 (Leonard) as it moves through the sky. Early this morning (3 December) it passed in front of the nice globular cluster M3. From suburban Bloomington, Indiana, with no Moonlight but plenty of light pollution.

75 frames, each 90 sec. (nearly 2 hours total exposure), processed in Astro Pixel Processor, once to register on the comet, again to register on the stars, processed in Lightroom and composited in Photoshop.

Explore Scientific 102mm f/7 refractor, ZWO ASI294MC camera, UV/IR cut fillter, iOptron CEM25P mount, ASIAir Pro controller.

M 81 and M 82 are truly „iconic“ deep sky objects! I spent more than 17 hours on capturing this widefield, comprising „Bode’s Galaxy“, the „Cigar Galaxy“, some smaller galaxies nearby (like NGC 3077 and NGC 2976) and the galactical cirrus, that consists of dust within our own galaxy's disk.

To create a picture from RGB, H-Alpha and Luminance data and keep the balance between both, the bright galaxies and the faint cirrus, was a real challenge and took me many, many hours. Hope you like it!

Celestron RASA 8 f/2

Celestron Motorfocuser

EQ6-R Pro

ZWO ASI 2600 MC Pro (Gain 100, Offset 18, -10°):

RGB (no Filter): 420 x 60 (7h)

TS 2600 MP (Gain 100, Offset 50, -10°):

Ha (Baader H-alpha Highspeed Ultra-Narrowband 3.5nm Filter): 100 × 120 secs (3h 20')

Luminance (Baader Baader UV/IR Cut Filter): 475 × 30 secs (3h 57′ 30″) & 182 × 60 secs (3h 2')

Total: 17h 19′ 30″

Flats, Darkflats, Dithering

N.I.N.A., Guiding with ZWO ASI 120MM and PHD2

Astropixelprocessor, Photoshop, Pixinsight

D5300 Nikon 500mm Catadioptric Mirror Lens. 30sec f/8 ISO 400.

Captured in Astro Photography Tool. 140 Lights, 30 Darks, 30 Flats, 30 Bias frames. LR, AstroPixelProcessor, PS. Sky-Watcher Star Tracker. (The D5300 is used vs the D610 for the smaller pixel size- 3.89 microns vs 5.97 microns- to avoid undersampling.)

The Hercules Globular Cluster is composed of several hundred thousand stars and is about 24,000 light years away from Earth. The stars are so densely packed together they sometimes collide to form new stars called ‘blue stragglers’ which can clearly be seen in the image (zooming in helps!).

A globular cluster is a spherical collection of stars bound by gravity. Globular clusters in spiral galaxies like the Milky Way are found in the galactic halo which is the outer spheroidal part of the galaxy rather than found in the galaxy’s disc. Globular clusters tend to have older more massive stars and are composed of fewer heavy elements than open clusters. There are more than 150 Globular Clusters in the Milky Way. [Wikipedia]

Imaged from my UK back garden, Bortle 5, in Nautical dark (no Astro dark :-( ) on 31st May 2021 with:

- C925 Edge HD on CGX mount

- ASI 533MC Pro OSC camera

- ASI 120MM guidecam

Stack of 48 x 180s bin 2x2 with camera at 139 gain and -15degC

Processed with AstroPixelProcessor, StarTools and Affinity

Matériel :

* Samyang 135mm f2 @samyangfrance

* Filtre Nisi Natural Night @nisifrance

* Monture équatoriale StarAdventurer

-

-

Prise de vue :

* 200 lights soit 3h20, une minute par light

* 100 bias

* 100 flats

* No Dark

* Bortle 2,5 - 3

-

-

Traitement :

* Lightroom,

* AstroPixelProcessor,

* Photoshop (HLVG/Topaz Denoise)

6 hours total on M81 and M82

Stacked in AstroPixelProcessor and processed in PixInsight

QHY163m camera

With one of the more spectacular views in the night sky, Thor's Helmet Nebula (NGC 2359) features a bubble shaped emission nebula. This bubble (containing hundreds of solar masses of ionized material) appears to be getting blown by solar wind coming from the central star. This is a rare type of central star known as a Wolf-Rayet star which runs extremely hot and is thought to be in a pre-supernova stage.

Calibrated images of Thor's Helmet Nebula were provided by iTelescope.net. In addition to providing access to their telescopes, iTelescope.net provides subscribing members with a combination of premium image sets (with the rights to use & post them) and webinars that show how to process them. Itelescope.net captured the images and I did the post-processing with Astro Pixel Processor, Photoshop and Topaz Sharpen AI. Star spikes are natural.

Exposure Settings

• 27 images (9 red, 9 green & 9 blue)

• Exposure Time: 10 minutes (each image)

• Total Exposure Time: 270 minutes

Galaxy IC342 at 10.7 Million lightyears distance is seen here obscured by the dust and gas in the plane of our Milky way Galaxy. That is why IC342 has a reddish color.

LRGB data (11.6 hrs Luminance+12.5hrs RGB) shot on 15,16,17,18,19 and 20 November 2017. Esprit 100 refractor with QHY16200 Mono CCD camera @-20 Celcius.

Processed with AstroPixelProcessor and Pixinsight.

Wikipedia: en.wikipedia.org/wiki/IC_342

Knight Observatory, Tomar

In Explore 20180401

First narrowband mosaic for me.

M: Pegasus NYX-101

T: WO GTF81 Refractor

C: ZWO ASI533MM-Cooled

G: OAG and PHD2

GC: ZWO ASI120MC

RAW16; FITs

Temp: -10 DegC

Mosaic: 4 x Panels of:

Ha: Gain 100; Exp: 6 x 300s

Oiii: Gain 100; Exp: 6 x 300s

Sii: Gain 100; Exp: 6 x 300s

Frames: 72 Lights; Darks/DarkFlats/Flats

95% Crop

Capture: NINA

Processed: APP [HOS-1]; PS.

Sky: 50% moon, slight breeze, no cloud.

30-04-2017 - 01:00 aprox. GMT -3

Star Adventurer

Canon 6D - Sigma AF 70-300mm f/4-5.6 APO DG Macro @ f/5,6

ISO 1600 - 5150K - 120 segundos - DF 190mm

16 lights, 19 darks y 300 bias

AstroPixelProcessor, Photoshop y Lightroom

Easily the largest Seagull ever seen, by light years ;-)

The Seagull Nebula (Sh2-296) lies just on the border between the constellations of Monoceros (The Unicorn) and Canis Major (The Great Dog) and is close to Sirius, the brightest star in the night sky. The nebula lies more than four hundred times further away than the famous star.

The complex of gas and dust that forms the head of the seagull glows brightly in the sky due to the strong ultraviolet radiation coming mostly from one brilliant young star HD 53367.

The radiation from the young stars causes the surrounding hydrogen gas to glow. Light from the hot blue-white stars is also scattered off the tiny dust particles in the nebula to create a contrasting blue haze in some parts of the picture.

Spanning about 100 light-years from one wingtip to the other, Sh2-296 displays glowing material and dark dust lanes weaving amid bright stars.

It is a beautiful example of an emission nebula, in this case an HII region, indicating active formation of new stars, which can be seen peppering this image.

The Seagull Nebula complex was observed for the first time by the German-British astronomer Sir William Herschel back in 1785.

SHO Taken between 22 and 27 February 2022 (65% - 13% Moon), RGB stars taken 7 March 2022 (22% Moon). Last chance to capture this target for me in my location for 2022, but also my first attempt. I could have squeezed in Thor’s Helmet if I had rotated the camera but I didn’t want to change the optics at this point. I could only manage 2.5 hours a night due to the target getting lower by this time of year, and crashing into a neighbours tree.

I spent far too many hours processing and reprocessing using new and different Pixinsight work flows to get the best from the data, and of course I would like to start over again, but time to let this big bird free until I capture it again next time around.

Sky Quality 19.67 Magnitude Class 5 Bortle.

Astromiks 50mm SHO 6nm Filters

Sii=26 x 300s + 19 x 180s

Ha=27 x 300s + 18 x 180s

Oiii=14 x 300s + 17 x 180s

RGB Stars 46 x 60s x 3

10 hours 10 minutes total

30 x Darks, Flats and Bias

ZWO ASI6200MM Pro

ZWO 7x2" EFW

ZWO EAF

Williams Optics GT81 IV

WO 6A III Field Flattener 0.8

HEQ5 Pro Rowan

ASIAIR Pro

Astro Pixel Processor

Pixinsight

Photoshop 2022

A portion of the star-forming nebula IC 1396, or the Elephant Trunk Nebula in the constellation Cepheus. 3-panel mosaic, each 20 300 sec. exposures (5 hours total exposure). Explore Scientific 102mm f/7 refractor, ZWO ASI294MC camera, dual narrow-band fillter (H-alpha and [O III]), iOptron CEM25P mount, ASIAir Pro controller, processed in Astro Pixel Processor and Lightroom.

im Sternbild Schwan. Ein Supernova Überrest.

Je 9x3min in RGB, 81min Gesamtbelichtungszeit. Bearbeitet mit AstroPixelProcessor, Photoshop , Starnet. Datensatz von iTelescope.net: Takahashi FSQ-ED APO 106mm, f/5, SBIG STL-11000M CCD Kamera.

I made this image with the Esprit 100 APO refractor and QHY16200 CCD. R,G and B filters, 64x120 seconds each. Ha (6nm) filter 17x900 seconds (total integration: 10.6 hrs.). 10,11,12,13,14 and 15 November 2017.

Stacks made with AstroPixelProcessor and further processing with Pixinsight (Histogram, RGB+ NBRGBCombination, Curves)

Knight Observatory, Tomar.

This HII complex on the border of Monoceros and Canis Major. Covers about 3 degrees of sky, The nebula lies in one of the farthest arms of our Milky Way galaxy and is about 100 light years across.

The head of the Seagull is Vdb 93. Also contained within the nebula are the open clusters - NGC 2343, NGC 2335, Collinder 465, and Collinder 466.

This is a HaRGB Combination from the Canon 6Da RGB data from march 8, 10 &11 2016 and Ha data shot with QHY16200 on november 17,18,19 &20 2017. (3 hrs RGB+7 hrs Ha)

telescope: Esprit 100 f5.5.

Knight Observatory, Tomar

I wanted to include the Perseus molecular cloud in the same extent as the California Nebula, but it didn't quite fit in the 1.5x-crop-factor field of view of my Fuji + Samyang 135mm lens, so I shot a mosaic of 4 panels. I thought snct astro did a great job framing the extent here (flic.kr/p/2kcoAZu), so I imitated their framing.

Panels were 26, 30, 22, and 37 x 1 min integrations and overlapped substantially, so most areas were covered by more than one panel. I also added 50 x 1 min of imagery of the Perseus Molecular Cloud from Nov. 20, 2019 (flic.kr/p/2hNZ6iA). So in total this is 165 minutes worth of data.

Fujifilm X-T10, Samyang 135mm f/2.0 ED UMC @ f2.0, ISO 1600, tracking with iOptron SkyTracker Pro, stacking of individual panels done with DeepSkyStacker, flattening of individual panels and mosaicking done with Astro Pixel Processor, editing in GIMP.

Skies were Bortle 3/4 for the 4 panels shot on Dec. 5, 2020, and Bortle 2/3 for the 50 exposures from Nov. 20, 2019.

It was fun discovering the planetary nebula NGC 1514 below the California Nebula as I processed this. Even though it's tiny at 135mm, it was very apparent that it was a planetary nebula rather than a star.

A starless process of the Elephant's Trunk nebula captured in narrowband (Ha, S2 and O3) then processed in the Hubble Palette (SHO)

Stacked in AstroPixelProcessor

Processed in PixInsight and Photoshop

This was a two panel mosaic but i sstill managed to somehow get the framing wrong and not capture all of the LMC!

Samyang 135/ZWO ASI183MC/AM3/L pro/ASIAIR

Bortle 4.6

1 and a quarter hours for each panel- 5 minute subs/

processed in AstroPixelProcessor/Photoshop CS6 and Affinity Photo

M: iOptron EQ45-Pro

T: William Optics GTF81

C: ZWO ASI1600MC-Cooled

F: No Filter

G: PHD2

GC: ZWO ASI120mini [OAG]

RAW16; FITs

Temp: -15 DegC

Gain 200;

25 x Exp 15s

Frames: 25 Lights; 50 Darks; 50 Flats

60% Crop

Capture: SharpCap

Processed: APP; PS

Sky: No moon, calm, 30%cloud, mild, good seeing.

Perchée à près de 1000 mètres d’altitude (913 mètres exactement), la majestueuse Tour de Peyrebrune veille fièrement sur les contreforts du Lévézou. Nichée au sommet d'Alrance, elle offre une vue imprenable sur le lac de Panat, dans un cadre naturel à couper le souffle. Jadis, au Moyen Âge, cet endroit abritait un château fort et un ensemble de fortifications, témoins d’un passé riche en histoire.

—

Mon objectif était simple : jamais je n’avais vu de photo de la tour prise en astrophoto, un vide qu’il me fallait impérativement combler. La plus grande difficulté résidait dans la recherche du point de vue parfait, suffisamment dégagé pour laisser apparaître, sous un ciel étoilé, Orion, les Pléiades et la splendide nébuleuse de la Californie.

__________________________

——

Ciel : 25min (25x60sec)

Sol : un seul cliché de 30sec sur le lever de lune

—

Logiciel utilisé : AstroPixelProcessor, GraXpert, Starnet++, Photoshop & Lightroom

10 hours RGB plus 3 hours dual band data over 3 nights 4-6th April 2021

Skywatcher 200pds

Altair Astro 294c

Optolong L-eXtreme dual band filter

Stacked in Astropixelprocessor

Processed in PixInsight and Photoshop

M81 (Bodes Galaxy) Spiral Galaxy found in the constellation of Ursa Major.

M: iOptron iEQ45-Pro

T: Celestron C8 SCT

C: ZWO ASI1600MC-Cooled

G: OAG and PHD2

GC: ZWO ASI220MM

RAW16; FITs

Temp: -10 DegC

Filter: No Filter

Gain 139; Exp: 32 x 120s

Frames: 32 Lights

Cal Frames: DarkFlats/Flats

Total Exposure: ~64 mins

95% Crop

Capture: NINA

Processed: APP; PS.

Sky: No moon, no breeze, no cloud.

The Pleiades star cluster in the constellation Taurus. Stars and dust gravitationally bound to each other.

1x3 mosaic, each tile 30 300 second exposures frames (7.5 hours total exposure). Explore Scientific 102mm f/7 refractor, ZWO ASI294MC camera, UV/IR cut fillter, iOptron CEM25P mount, ASIAir Pro controller.

SN2020ue was discovered on 12 january 2020. It is a type 1a supernova in elliptical Galaxy NGC4636 at 55 Million Lightyears. I made this image on 20 jan 2020 (02:00-04:00), 21 x 300 seconds luminance. Stacked in Astropixelprocessor with 2 x drizzle and processed/annotated in Pixinsight.

Asteroid 1989 Tatry moved through the narrow field of view (Identified with the Minor planet center MPC checker) It is an inner main belt Asteroid with 17km diameter.

www.rochesterastronomy.org/supernova.html#2020ue

en.wikipedia.org/wiki/1989_Tatry

en.wikipedia.org/wiki/Type_Ia_supernova

Dati: 57 x 300 sec ( 4.75ore) gain 5 @ -20° c + 38 dark + 30 flat e darkflat

Filtro: Astronomik UV/IR Block L2

Montatura: EQ6 pro

Ottica: Takahashi FSQ106

Sensore: QHY168C

Cam guida e tele: asi120mm su Scopos 62/520

Software acquisizione: nina e phd2

Software sviluppo: AstroPixelProcessor e Photoshop

Temperatura esterna: 5 ° C - Umidità 50%

note: PRESENZA DI VELATURE IN CIELO