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Another object from this nice catalogue of faint nebula.
Long integration of 53 hours using two narrow band filters mainly, searching the limits of the equipment and my own process skills.
It's not a popular target probably because is difficult and usually is not showing so much detail due to the high dynamic range, the core is bright, really bright compare with the faint surroundings.
Sh2-235 is the most central and brightest nebula of an H II region known as G174+2.5; it is observed in the direction of the northern part of the Aur OB1 association and includes the nebulae catalogued as Sh2-231, Sh2-232, Sh2-233 and Sh2-235, identified as individual nebulae in the 1959 census of H II regions. Although in the optical images they appear as distinct nebulae, in reality they all belong to a single giant molecular cloud, of which some parts appear illuminated by young and hot stars. This cloud is located in Perseus' Arm at a galactic latitude that places it slightly off-center with respect to the center of the galactic disk; the distance measurements indicate a range between 1600 and 2000 parsec, so it is normally indicated as about 1800 parsec (5870 light years).
(descri. credits to wiki.it it.wikipedia.org/wiki/Sh2-235)
Technical card
Imaging telescope or lens:Altair Astro RC250-TT 10" RC Truss Tube
Imaging camera:ZWO ASI1600MM-Cool
Mounts:Mesu 200 Mk2, Astro-Physics Mach-1 GTO CP4
Guiding telescope or lens:Celestron OAG Deluxe
Guiding camera:ZWO ASI174 Mini
Focal reducer:Riccardi Reducer/Flattener 0.75x
Software:Pleiades Astrophoto PixInsight , Seqence Generator Pro
Filters:Astrodon O-III 36mm - 5nm, Astrodon S-II 36mm - 5nm, Astrodon R Gen.2 E-series 36mm, Astrodon G Gen.2 E-series 36mm, Astrodon B Gen.2 E-series 36mm, Astrodon HA 36mm - 5nm, Astrodon L Gen.2 E-series 36mm
Accessories:ZWO EFW, MoonLite NiteCrawler WR30
Resolution: 2328x1760
Dates:Dec. 25, 2019, Jan. 3, 2020, Jan. 12, 2020, Jan. 15, 2020
Frames:
Astrodon B Gen.2 E-series 36mm: 90x30" (gain: 75.00) -20C bin 1x1
Astrodon G Gen.2 E-series 36mm: 90x30" (gain: 75.00) -20C bin 1x1
Astrodon HA 36mm - 5nm: 186x600" (gain: 200.00) -20C bin 1x1
Astrodon R Gen.2 E-series 36mm: 90x30" (gain: 75.00) -20C bin 1x1
Optolong SII 6.5nm 36mm: 121x600" (gain: 113.00) -20C bin 1x1
Integration: 53.4 hours
Avg. Moon age: 18.25 days
Avg. Moon phase: 55.61%
Astrometry.net job: 3224550
RA center: 5h 41' 5"
DEC center: +35° 49' 58"
Pixel scale: 1.007 arcsec/pixel
Orientation: 90.283 degrees
Field radius: 0.408
Locations: AAS Montsec, Àger, Lleida, Spain
Data source: Own remote observatory
Remote source: Non-commercial independent facility
This is my first Post-Covid image but also my first Mosaic since switching back to a MONO imager, was so happy with the performance of my ASI6200MC Pro that I stuck with the same model but the MONO version, taken from Bortle 4 skies in the south east UK
RA: 05h23m06.99s
Dec: +33°58'17.2"
Constellation: Auriga
Designation: IC405, IC410 / NGC1893, IC417, NGC1907, NGC1931
Image Details:
Panel 1: 101x150S in 3nm Ha, 4.5nm OIII and 4.5nm SII
Panel 2: 101x150S in 3nm Ha, 4.5nm OIII and 4.5nm SII
Darks: 201 Frames
Flats: 201 Frames
Bias: 201 Frames
Acquisition Dates: Jan. 29, 2022 · Feb. 4, 2022 · Feb. 6, 2022 · Feb. 18, 2022 · Feb. 19, 2022 · Feb. 21, 2022 · Feb. 22, 2022 · Feb. 24, 2022 · Feb. 25, 2022 · Feb. 26, 2022 · Feb. 27, 2022
Total Capture time: 25h 15min
Equipment Details:
Imaging Camera: ZWO ASI6200MM Pro 62mpx Full Frame
Imaging Scope: SharpStar 15028HNT Hyperboloid Astrograph
Guide Camera: ZWO ASI260MC Pro
OAG: ZWO L-OAG
Mount: Sky-Watcher EQ8 Pro
Pier: Altair Astro Skyshed 8" Pier
Focuser: Primalucelab Sesto Senso V2
Filter: Baader Ultrafast F2 3nm Ha, 4.5nm OIII and 4.5nm SII
Power and USB Control: Primalucelab Eagle4 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
TS 115/800
ZWO ASI 1600 mono cooled
LRGB
L: 180 minutes
RGB: 240 minutes (DSLR)
Total: 7 hours
PixInsight + PS6
astrocamp.eu/en/messier-81-widefield-march-25/
In March 2025, I embarked on an astrophotography project focusing on Messier 81 and its neighboring galaxies. I captured the luminance data at the Hohen List observatory in the Eifel region, while the RGB channels were taken earlier from my home in Koblenz. Combining these, I achieved a total exposure time of 6 hours and 20 minutes. The resulting widefield image prominently features Messier 81 at the center, with Messier 82 to its left, the Garland Galaxy below, and NGC 2976 in the upper right. This project served as a testament to the capabilities of my telescope-camera setup, delivering impressive results even with a relatively short integration time.
Around 600 shots with 70-200mm exposure of 0,8 seconds.
Processed stacked in Pixinsight.
No equatorial or azimutal mount.
Using the MARS data in the latest PixInsight I got the best result I've gotten from M45.
15 hours
ASI 2600 mcpro/ASI 290 mono
AM5/AA+
StellarVue 90mm/Askar FMA180Pro
8 panel mosaic
view in full size ;)
Equipment:
TS 10" f/4 ONTC Newton
1000mm f4
ZWO AS183mmPro
2x Barlow
Skywatcher EQ8
The Lion Nebula.
Found in the constellation of Cepheus, the Lion Nebula when viewed from just the right perspective, actually does represent a lion. At approx 10,000 light years away
it is made up of an emission nebula and a reflection nebula.
Not bright enough for visual observation sadly, it does however make for a great imaging target.
Boring Techie bit:
Telescope: Askar FRA400
Mount: EQ6r pro
Camera: ZWO 533mc pro
Filter: Optolong L'eNhance.
Guided and controlled by the ZWO asiair+
Eighty 3 minute exposures
Stacked & processed in PixInsight with BlurXterminator, NoiseXterminator, Starnet++, Graxpert and Affinity Photo.
Nebulosa California (California nebula) #NGC1499
Constelación en que se encuentra: Perseus
Distancia: 1800 de años luz
De SkySafari:
NGC 1499 es una nebulosa de emisión en la constelación Perseo que recibe su nombre por el parecido con el mapa del estado de California de Estados Unidos. Fue descubierta en 1885.
Su brillo superficial es bajo. Está a unos 1800 años luz del sistema solar, en el brazo de Orión de la Vía Láctea. Es una región en la que, por su alto contenido de hidrógeno, se han formado muchas estrellas masivas y luminosas. La estrella luminosa es Menkib (Xi-Per), de color blanco azuloso, e ilumina la nebulosa.
Datos de la imagen:
Exposure: 4hr 09min (83 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: 24-nov-2024
Location: #Bogotá, #Colombia
45x40sec iso 800
Canon 6D + Canon 400mm f5.6 L @5.6
Skywatcher Star Adventurer
clip in Lpro Filter
stacked at pixinsight
post pixinsight + photoshop
M81/M82 - 20-05-2020 - Saucats
Lights: 300x30" (2h30)
Reprise du traitement avec PixInsight.
DOF: 50
Iso: 1600
Traitement: PixInsight / DxO PhotoLab
Nikon D3100 (Non Défiltré)
Skywatcher 80ED Equinox (80x500)
Skywatcher Az-Gti Equatorial Mode
6 heures (brutes de 60") au RC8 + réducteur x0.68 (1088 mm de focale) + ASI533MC + filtre Optolong L-Pro, Pixinsight.
Mi ultima toma de 2017
Nexstar 8Se
CGEM
QHY Img132e
Mosaico de 14 teselas.
Autostakkert
ICE
PixInsight
Ps Cs6
Ciudad de México, Coyoacan.
A Cluster of Pearls in the Southern Skies ( NGC 3766 " The Pearl Cluster" ) by Mike O'Day ( 500px.com/MikeODay )
Shimmering like a pearl to the naked eye, this open cluster of mostly young blue stars ( known as the "Pearl Cluster" ) is approximately 5500 light years from Earth and was discovered by Abbe Lacaille in 1752 from South Africa.
This HDR "true colour" image is constructed from 11 sets of exposures ranging from 1/4 sec ( to capture the centre of the brighter stars ) through to 240 seconds ( for the fainter stars of the Milky Way ). Total exposure time was around 5 hours.
12 April 2018
Image details:
Field of view ..... 58' 49.8" x 39' 36.4"
Image center ...... RA: 11 36 03.890 Dec: -61 35 30.17
Resolution ........ 0.586 arcsec/px ( full size image )
Orientation: North is up
Telescope: Orion Optics CT12 Newtonian ( mirror 300mm, fl 1200mm, f4 ).
Corrector: ASA 2" Coma Corrector Quattro 1.175x.
Effective Focal Length / Aperture : 1470mm f4.7
Mount: Skywatcher EQ8
Guiding: TSOAG9 Off-Axis-Guider, Starlight Xpress Lodestar X2, PHD2
Camera:
Nikon D5300 (unmodified) (sensor 23.5 x 15.6mm, 6016x4016 3.91um pixels)
Location:
Blue Mountains, Australia
Moderate light pollution ( pale green zone on darksitefinder.com map )
Capture ( 12 April 2018 ):
11 sets of sub-images with exposure duration for each set doubling ( 1/4s to 240s ) all at ISO250.
( 70 x 240sec + 10 each forthe other durations )
Processing:
Calibration: master bias, master flat and master dark
Integration in 11 sets
HDR combination
Pixinsight April 2018
Links:
A Hydrogen-Alpha + Oxygen III + Sulphur II Narrowband widefield image of the Cygnus Wall. The North America Nebula (NGC 7000 or Caldwell 20) is an emission nebula in the constellation Cygnus, close to the star Deneb. The remarkable shape of the nebula resembles that of the continent of North America, complete with a prominent Gulf of Mexico.
The Cygnus Wall:
The Cygnus Wall is a term for the "Mexico and Central America part" of the North America Nebula. The Cygnus Wall has the most concentrated star formation in the nebula. The North America Nebula and the nearby Pelican Nebula, (IC 5070) are in fact parts of the same interstellar cloud of ionized hydrogen (H II region). The nebula complex is estimated to be about 1,800 light-years from Earth.
Gear:
William Optics Star 71mm f/4.9 Imaging APO Refractor Telescope.
William Optics 50mm Finder Scope.
Celestron SkySync GPS Accessory.
Orion Mini 50mm Guide Scope.
Orion StarShoot Autoguider.
Celestron AVX Mount.
QHYCCD PoleMaster.
Celestron StarSense.
QHYCFW2-M-US Filterwheel (7 position x 36mm).
QHY163M Cooled CMOS Monochrome Astronomy Camera.
Tech:
Guiding in Open PHD 2.6.3.
Image acquisition in Sequence Generator Pro.
Lights/Subs:
2 Stage Cooled CMOS
Imaged at -25°C
Gain: 20
Offset: 80
Narrowband:
S = 12 x 600 sec. 16bit FITS.
H = 12 x 600 sec. 16bit FITS.
O = 12 x 600 sec. 16bit FITS.
Calibration Frames:
50 x Bias/Offset.
25 x Darks.
20 x Flats & Dark Flats.
PixelMath RGB Channel Combination:
PixInsight Expression:
R = SII
G = (Ha*OIII)*1.5
B = OIII
Image Acquisition:
Sequence Generator Pro with the Mosaic and Framing Wizard.
Plate Solving:
Astrometry.net ANSVR Solver via SGP.
Processing:
Pre-Processing and Linear workflow in PixInsight,
and finished in Photoshop.
Photographed in the following wavelengths of light:
Optolong SHO Narrowband filters:
OIII line 500.7nm (6.5nm bandwidth)
H-Alpha line 656nm (7nm bandwidth)
SII line 672nm (6.5nm bandwidth)
Astrometry Info:
View the Annotated Sky Chart for this image.
Center RA, Dec: 314.764, 44.279
Center RA, hms: 20h 59m 03.425s
Center Dec, dms: +44° 16' 43.955"
Size: 2.27 x 1.55 deg
Radius: 1.375 deg
Pixel scale: 5.11 arcsec/pixel
Orientation: Up is 97.9 degrees E of N
View this image in the World Wide Telescope.
Martin
-
[Home Page] [Photography Showcase] [My Free Photo App]
[Flickr Profile] [Facebook] [Twitter] [My Science & Physics Page]
A large stellar nursery in the constellation of Scorpius some 6,000 light years away from us.
The nebula is very faint, making it difficult to observe, despite it's size of around 250 light years.
The image consists of 19 data sets of 5 minute LRGB each.
Data was captured online using the Chile 2 telescope at Slooh.com
Mosaico 4 teselas.
Visionking 80mm Apo triplet ed
QHY Img132e
CGEM
Autostakkert, Pixinsight, LR, Ps Cs6
"M101 is a large galaxy, with a diameter of 170,000 light-years. By comparison, the Milky Way has a diameter of 258,000 light years. It has around a trillion stars, twice the number in the Milky Way. It has a disk mass on the order of 100 billion solar masses, along with a small central bulge of about 3 billion solar masses.
M101 is asymmetrical due to the tidal forces from interactions with its companion galaxies. These gravitational interactions compress interstellar hydrogen gas, which then triggers strong star formation activity in M101's spiral arms that can be detected in ultraviolet images. "
- Wikipedia
Shooting Location :
* 51° N 3° E
* bortle class 5 backyard
Object Information
* Type : Spiral Galaxy
* Magnitude : 7,86
* Location (J2000.0): RA 14h 03m 13s / DEC +58° 20' 56"
* Approximate distance : 6.400 parsecs / 20.877.000 lightyears
Hardware
* Mount : Celestron CGX
* Imaging Scope : Sky-Watcher Explorer 150PDS
* Imaging Camera : ZWO ASI 183MM
* Filter Wheel : ZWO EFW 7*36mm + Baader Ha 7nm, Baader OIII 8.5nm + Baader SII 8.5nm + Baader LRGB
* Coma Corrector : Baader MPCC III
* Guide Scope : Sky-Watcher StarTravel 80
* Guide Camera : ZWO ASI 120MM
Exposures
* Gain : 111
* Offset : 10
* Sensor Temperature : -20°C
* Light Frames :
> Baader Luminance : 49x 180sec
> Baader Red : 11x 180sec
> Baader Green : 11x 180sec
> Baader Blue : 11x 180sec
* Flat Frames :
> Baader L : 30x
> Baader R : 30x
> Baader G : 30x
> Baader B : 30x
* Dark Frames : 100x
* Bias Frames : 100x
* Total Integration Time : 4h06m
* Capture Date : 2019-04-10
Capture Software
* Sequence Generator Pro
* PHD2 Guiding
Processing Software
* PixInsight
* Noiseless
* Adobe Photoshop
207x180s h-alpha
369x180s OIII
163x180s SII
34x180s red
44x180s green
43x180s blue
total: 43 hour
Equipment:
Epsilon 130D dual rig
QHY268m + CFW3M
TS2600MP (Touptek IMX571) + ZWO EFW
Astronomik DeepSky RGB
Astronomik MaxFR
Pegasus NYX-101
August 2023
Location: french alps
The Trifid (M20) is a combination emission (red) and reflection (blue) nebula that is located in the constellation Sagittarius. It gets its name because the main section of the nebula is divided by dust lanes into roughly three parts.
Taken over two nights from a relatively dark site on the slopes of Palomar mountain, this image consists of 1022 sub-exposures that were each exposed for 5 seconds using an uncooled QHY5-III 178C camera and a Stellarvue SV80ST2 telescope (the latter operating at f/4.8 using a 0.8X reducer/corrector, total exposure integration time about 85 minutes). Using such short exposures greatly simplifies the image capture process since there was no need to guide the Celestron AVX mount that carried the scope and camera.
Image capture was done with SharpCap, image processing was done in PixInsight and Photoshop CC2015.
This photo is best seen against a dark background or in the Flickr light box at full size (1920 x 1242 pixels).
Here is a link to the full-sized image:
All rights reserved.
This is visible in Scorpius. At about 5,500 light years away the Cat's Paw is an emission nebula with a red colour that originates from an abundance of ionized hydrogen atoms.
Taken with iTelescope.net T12 (Takahashi FSQ-ED 106mm, SBIG STL-11000M / Siding Spring, Australia) in mid December.
60 minutes of data: 3 5 minutes exposures each of Luminance, Red, Green, Blue.
Processing in FixFits (remove bright rows), PixInsight (StarAlignment, ImageIntegration, ChannelCombination, STF / Histogram, LRGB), Lightroom (image enhancement and cropping).
Last nights clear spell wasn't actually as good as promised, but decent enough to capture 3 hours of OIII. The sky was milky and damp, but there was decent seeing towards the zenith. Rain has set in again and with the moon looming it may be a while before I can add any more OIII.
The colour mapping is pretty standard, Ha to red and OIII to blue and green.
Total exposure time 8 hours, shot using an Altair Astro 6" RC, Astrodon narrowband filters and an Atik 314l+. Processed using Pixinsight and CS5.
This is a very small part of the whole area as its end of season for this part of the sky no way I could do a whole panorama. The Blue is Oxygen that all part of the Super Nova remnant What you are looking at is in Gum 17 area also not far from the Pencil Nebula. This whole area has some great targets for next year, this was some thing I was looking forward to being able to do with the filters as I knew the blue stood out.
QHY268M -10c 120 Odd shots 5 min each filter over 6 nights .. 30 shots each RGB 1 min exposure.
QHYCFW3 and 7 Antlia filters LRGBSHaO
MeLE Mini PC
Pegasus Astro Pocket Mini power box
Starpoint Australis SP3 Focuser Rotated 22 degrees from last
Skywatcher 200 F4 PREMIUM PHOTO QUATTRO REFLECTOR OTA
Skywatcher F4 Aplanatic Coma Corrector
Skywatcher NEQ 6 Pro Hypertuned
SVbony 50MM Guide scope
QHY5L-II-M Guide camera
Guided PHD2, Nina
Pixinsight, Ps, Lr
A cropped Bi-Color processing test of Pickering's Triangle (or Pickering's Triangular Wisp) in the Veil Nebula (a Supernova Remnant).
NGC 6974 and NGC 6979 are luminous knots in a fainter patch of nebulosity on the northern rim between NGC 6992 and Pickering's Triangle.
Ha & OIII Bi-Color:
Photographed in the Hydrogen-Alpha and Oxygen III spectral wavelengths of light (Ha mapped to Red, OIII mapped to Blue, SynthGreen).
Narrowband filters:
H-Alpha
OIII
Processing:
Pre-Processing and Linear workflow in PixInsight, and finished in Photoshop (experimenting with Wavelets, Photoshop Actions and new bi-color processing techniques).
Astrometry Info:
nova.astrometry.net/user_images/1381741#annotated
RA, Dec center: 312.019287471, 31.6310735368 degrees
Orientation: 0.443881002562 deg E of N
Pixel scale: 2.4980010893 arcsec/pixel
Martin
-
[Home Page] [Photography Showcase] [eBook] [Twitter]
It is always fun to do a bit of astroimaging on a relatively warm December evening.
Central to this image is a dark cloud of dust and gas resembling a horse’s head, known as the Horsehead Nebula (B33). This nebula is further enhanced by a bright H alpha emission nebula, which is part of the Orion molecular cloud designated IC434. Adjacent to the Horsehead Nebula is the Flame Nebula (NGC 2024), an active star-forming region containing hundreds of low-mass stars. Approximately 86% of these stars have circumstellar disks, which are believed to be an early stage of planetary system formation. Notably, the bright star on the edge of the Flame Nebula is Alnitak, the easternmost star of Orion’s Belt.
The image was obtained with 30, 2 minute images using a RASA8 telescope, ASII2600MC Pro camera, and an IDAS NBZ II dual narrowband filter. Processing was with Pixinsight and PS.
Canon 6d
Montura Omegon
objetivo 85 mm f 3.5
20 fotos 65" ISO 1600 D/B
6 fotos 65" ISO 3200 D/B
PixInsight
Cabañeros
Junio 2019
What started out as a question became a small marathon. I was getting shadow /reflections of the filters in the shot. So it became full clean down mirrors and filters. once put together I did a NB night and a RGB night to see if all had gone, happy to say its all clear.
What better way to really see so I did 5 nights of NB in total about 130 shots per filter. This is a Hubble SHaO pallet. One thing that showed up in those 5 night 2 am in the morning mount would disconnect. It would restart straight away once I got the port recognized. Turns out the fitting for the EQMOD cable for the mount was not firm even if the screws where. Two small slithers of a wall plug on the screws the whole thing is a tight as a drum and ran all night.
Now who cant see the chicken running Bottom left cant miss it. Still cant get over the detail in the shot.
QHY268M -10c 130 Odd shots 5 min each filter over 5 nights .. 30 shots each RGB 1 min exposure.
QHYCFW3 and 7 Antlia filters LRGBSHaO
MeLE Mini PC
Pegasus Astro Pocket Mini power box
Starpoint Australis SP3 Focuser Rotated
Skywatcher 200 F4 PREMIUM PHOTO QUATTRO REFLECTOR OTA
Skywatcher F4 Aplanatic Coma Corrector
Skywatcher NEQ 6 Pro Hypertuned
SVbony 50MM Guide scope
QHY5L-II-M Guide camera
Guided PHD2, Nina
Pixinsight, Ps, Lr
ccd: QSI683wsg with Astrodon LRGBHaS2O3 filters
telescope: DSI RC10C f/7.3
mount: 10Micron GM2000 QCI
guider: Lodestar
exposure: L 20x15min (1x1) + RGB 8x8min (2x2)
location: Les Granges, 900 m
software: TheSkyX Pro, CCD Commander, Pixinsight, PS CS5
date: 3-8 Jul 2016
The Whirlpool Galaxy, also known as Messier 51a (M51a) or NGC 5194, in the constellation Canes Venatici. 31 million light-years from Earth.
Skywatcher Esprit 100ED
Canon 700d
Celestron CGEM
ISO800 35x120s (1hr 10mins)
Processed in PixInsight
Grantham UK
Resolution ............... 0.797 arcsec/px
Rotation ................. -90.985 deg
Observation start time ... 2023-04-07 19:36:20 UTC
Observation end time ..... 2023-04-07 23:51:56 UTC
Focal distance ........... 556.23 mm
Pixel size ............... 2.15 um
Field of view ............ 2d 9' 28.6" x 1d 24' 10.7"
Image center ............. RA: 13 29 52.534 Dec: +47 10 19.52 ex: -0.000050 px ey: -0.000120 px
Using 34x40s & 18x60s subs in PixInsight, I reduced most stars to better show the structure of this remarkable comet. Through 7x35mm binoculars, I was able to see about 1.5 degrees of Comet Lemmon. Yesterday with less moonlight, I could measure just over 2.5 degrees in Botle 5 skies.
2024-02-07 0840 UTC
Winter Star Party, Scout Key, Florida
Camera: ZWO ASI 2600MC
Guide Camera: ZWO ASI 290MM
Telescope: Vixen ED80 f/6.5
Mount: Losmandy G11
Integration: 80 minutes
Capture: NINA
Postprocessing: Pixinsight
The core of Carina with the 8" and QHY268M I am blown away the detail in the shot at 100% . I was taken back by the fact even at 200% there is still no noise and not one bit applied. I don't need to say much more other than enjoy the shots and editing.
QHY268M -10c 100 Odd shots 5 min each filter over 5 nights .. 30 shots each RGB 1 min exposure.
QHYCFW3 and 7 Antlia filters LRGBSHaO
MeLE Mini PC
Pegasus Astro Pocket Mini power box
Starpoint Australis SP3 Focuser Rotated 90 degrees
Skywatcher 200 F4 PREMIUM PHOTO QUATTRO REFLECTOR OTA
Skywatcher F4 Aplanatic Coma Corrector
Skywatcher NEQ 6 Pro Hypertuned
SVbony 50MM Guide scope
QHY5L-II-M Guide camera
Guided PHD2, Nina
Pixinsight, Ps, Lr
33 x 180s red
35 x 180s green
31 x 180s blue
192 x 180s Luminanz
254 x 180 H-Alpha
total 27 hours
Equipment:
Takahashi Epsilon 130D dual rig
QHY268m (IMX571)
QHYCFW3M-SR
TS2600MP (Touptek/RisingCam IMX571)
ZWO EFW
Astronomik Filter
Sywatcher EQ8
Altair 294c
60x60s, 45x120s
Stacked in AstroPixelProcessor
Processed in PixInsight
Finished in Photoshop
The Globular Cluster of Hercules or Messier 13 or even NGC 6205 is a globular cluster visible in the constellation of Hercules.
It is the brightest globular cluster in the northern hemisphere and is also visible to the naked eye
The estimated distance from the solar system is just over 25,000 a.l.
Acquisition details:
Giosi Amante & Alessandro Pensato acquisition
2xRC8"
2x QHYCCD 183M
2x StarPi (Stellarmate)
LRGB Baader
LRGB Optolong
N_EQ6
CEM70
Processing Giosi Amante exclusively with Pixinsight
L bin1 137x60s
L bin1 119x300s
R bin2 32x60s
G bin2 32x60s
B bin2 32x60s
R bin2 16x300s
G bin2 16x300s
B bin2 16x300s
Aquisizione totale 17 ore e 48'
The Orion Nebula, also known as M42, is a diffuse nebula located about 1,344 light-years away from Earth in the constellation Orion. It is a well-known stellar nursery, where new stars and planetary systems are forming from collapsing clouds of gas and dust. Spanning about 24 light-years in diameter, it is one of the closest and largest regions of massive star formation visible to us.
At the heart of M42 lies the Trapezium Cluster, a young open cluster of stars. This cluster consists of four main stars arranged in a trapezoid shape within a 1.5 light-year diameter. Two of these stars can be resolved into binaries, bringing the total to six visible stars in the cluster. These stars, along with many others in the nebula, are in the early stages of their evolution. The Trapezium Cluster is part of the larger Orion Nebula cluster, which includes about 2,800 stars spread over 20 light-years.
Near the top of the frame is Sh2-279, the Running Man reflection nebula.
All the surrounding dust and lanes of dark-nebulae are part of the Orion Molecular Cloud complex.
This was a moderately complicated image to make, being an HDR:
300 lights at 1s - for the stars, especially the trapezium cluster in the core
100 frames at 180s for the detail in the dust
20 frames at an intermediate 30s for a smooth blend
TI: 6.25hr
Processed in PixInsight: WBPP, BlurXterminator, ABE, SPCC, NoiseXterminator, HDRComposition, Seti Astro's Statistical Stretch; finished in Affinity (tonemapping, HSL, clarity).
Prints, cards and more: shiny.photo/photo/M42-and-De-Mairan-s-Nebula-905695a23bff...
My first wide field Galaxy photo, 6 months after getting my first Telescope (a small inexpensive GSO 6" Newtonian Reflector) .
Ancient light from a Galaxy far, far away (situated 11.42 million light years from Earth).
The Sculptor Galaxy, also known as the Silver Coin or Silver Dollar Galaxy (NGC 253), is an intermediate spiral galaxy in the constellation Sculptor. It is a Starburst galaxy, which means that it is undergoing a period of intense star formation (well it was 11.42 million years ago, as the light took that long to reach us).
Recent research suggests the presence in the centre of this Galaxy of a Supermassive Black Hole, with a mass estimated to be 5 million times that of our Sun.
Photographed at the West Rand Astronomy Club's Annual Star Party at Mountain Sanctuary Park (North-West Province, South Africa). A special thank you to Neil Viljoen from "The Telescope Shop" for his assistance.
Astrometry info:
Center RA, Dec: 11.885, -25.297
Center RA, hms: 00h 47m 32.295s
Center Dec, dms: -25° 17' 48.899"
Size: 74.4 x 56.8 arcmin
Radius: 0.780 deg
Pixel scale: 4.36 arcsec/pixel
Orientation: Up is 18.2 degrees E of N
View the Annotated Astrometry Sky Chart.
View in the World Wide Telescope.
Gear:
GSO 6" f/4 Imaging Newtonian Reflector Telescope (Astrograph).
Celestron Advanced VX Equatorial Mount.
Orion 50mm Guide Scope.
Orion StarShoot AutoGuider (Guiding in PHD2).
Image Acquisition via Sequence Generator Pro.
Canon 60Da DSLR (sensitive to IR light at 656.28 nm).
Astronomik CLS Light Pollution Filter.
Processed in PixInsight & Photoshop.
Lights/Subs:
30 x Stacked 5 min. RAW exposures at ISO 1600.
Calibration Frames:
30 x Darks (Dark frames)
30 x Flats (Flat-field frames)
40 x Bias (Offset frames)
Martin
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Date: 25:30-27:10JST May.7, 2019
Location: Amagi Highland, Shizuoka Pref., Japan
Cloud Coverage: 5 ~ 30%
Wind: 0.5 ~ 5 kt
Temperature: 3.1C ~ 4.1C
Humidity: 39 ~ 44%
Air pressure: 896hPa
Lens: SIGMA 135mm F1.8 DG HSM | Art (f/2.5)
Mount: SWAT-310 (single axis autoguiding)
Autoguider: QHY5L-II, LM75JC, PHD2
Camera: Canon EOS 6D (SEO-SP4)
ISO speed: 3200
Exposure: 27x150sec.+15x45sec.+13x20sec.
Processing: PixInsight
updated on Jan. 1, 2020
This is the Lion Nebula located in the constellation Cepheus, also cataloged as Sh2-132 in the Sharpless Catalog. It is a relatively faint emission nebula located approximately 10,000 lightyears away.
Tech Specs: William Optics REDCAT 51 Telescope, ZWO ASI071MC camera running at 0F and Optolong L-eXtreme 2” Filter, 4 Hours using 5-minute subs, Sky-Watcher EQ6R-Pro mount, ZWO EAF (ProAstroGear Black-CAT) and ASIAir Pro, guided using a ZWO 30mm f/4 mini guide scope and ZWO 120 mini, processed in PixInsight. Image Date: August 30, 2025. Location: The Dark Side Observatory (W59), Weatherly, PA, USA (Bortle Class 4).
Equipment:
Scope: Lacerta 72/432 F6 0.85x reduktorral (367mm F5.1)
Mount: Skywatcher EQ-5 Pro Synscan Goto
Guide scope: Orion 50mm mini
Guide camera: ZWO ASI120mm Mini
Main camera: ZWO ASI183MM-Pro cooled monochrome camera
Accessories:
ZWO ASIAIR Pro
ZWO EFW 8x1.25"
Lacerta Dew-heater 20cm
Lacerta Dew-heater 30cm
Programs:
PixInsight
Adobe Photoshop CC 2020
Details:
Camera temp: -15°C
Gain: 111
Astronomik 6nm Ha:
18x300s
10x60s