View allAll Photos Tagged tsoptics
Mal wieder ein kurzes Zeitfenster bis wieder die Wolken kamen.
12 x 600s
ASI 2600 MC Pro
TS65Q APO
IDAS LPS D2
ZWO OAG - ASI 120 MC-S
Asiair Pro
EQ5 Pro Synscan GoTo
Teleskop oder Objektiv (Aufnahme): TS Optics TS 65/420 Quadruplet
Aufnahmekamera: ZWO ASI 2600 MC Pro
Montierung: SkyWatcher EQ6 R Pro
Teleskop oder Objektiv (Nachführung): TS Optics TS 65/420 Quadruplet
Nachführkamera: ZWO ASI 120MM
Software: APF-R · Pleiades Astrophoto S.L. PixInsight 1.8.8 Ripley · Adobe Photoshop 2020 · AstroPixel Processor
Filter: Optolong L-eXtreme 2"
Zubehör: ZWO EAF Electronic Auto Focuser · ZWO ASIAir Pro · ZWO OAG · Baader Coma Corrector
Frames: 50x600" (8h 20')
Aufnahmedauer: 8h 20'
Learning Pixinsight a couple of weeks now, and here is my first Result.
A complete HOO Processing of Rosette Nebula.
NGC 4490 - Gemeinsam mit NGC 4485 bildet sie das wechselwirkende Galaxienpaar Arp 269 oder Holm 414, das durch einen sogenannten Gezeitenarm der rund 24.000 Lichtjahre ins All ragt, verbunden wird.
ASI 2600 MC Pro
TS UNC 10" f/5 - 254/1250
Idas LPS D2
Asiair Pro
EQ 6-R Pro
100 x 300s Belichtungszeit
NGC 2174/NGC2175
45 x 600s
ASi 2600 MC Pro - TS65Q APO
Optolong L-Extreme 2"
Zwo OAG - Asi 120 MC-S
Asiair Pro
Ha - OIII - Luminance Processing
Camera: ASI 2600 MC Pro
Scope: TS65Q APO 65/420
Guiding: Asiair & ASI 120 MC-S
Filter: Optolong L-Extreme
Integration Time: 34 x 600s
Nach Herz kommt Seele IC1848 - Seelennebel. Nächste Runde mit ASI 2600 MC und Asiair. Diesmal funktionierte fast alles... Polar Alignment - super. Ziel anfahren - super. Plate Solve - super. Guiding - erst super, im laufenden Betrieb dann nicht mehr so super. Andauernd ist die DEC Achse abgeschmiert. Im Endeffekt hat es mir wieder mal von 40 Bildern 12 versaut. Keine Ahnung woran es liegt. Also hier das technische:
ASI 2600 MC Pro - TS65Q APO - Asiair - Optolong L-Extreme
28 x 600s - Gain 100 - 1x1 - Flats, Darks, Bias
NGC 1499
11 x 600s
ASI 2600 MC Pro - TS65Q APO - Optolong LExtreme - ZWO OAG - ASI 120 MC-S - ASIAIR Pro
Prominent features in this shot:
Aristoteles and Eudoxus in the North, near the terminator.
Mare Serenitatis below them.
Mare Nectaris with Theophilus, Cyrillus and Catalina and the Rupes Altai, glowing brightly
Maurolycus, its rim glowing, its floor still steeped in darkness, further South on the terminator
TS-Optics TSAPO65Q Quadruplet apochromatic refractor, focal length: 420 mm focal length, aperture: 65 mm
Canon EOS 600D
40 x 600s
ASI 2600 MC Pro
TS65Q Apo
Antlia ALP-T 2" Dualband Filter
Asiair Pro
Skywatcher EQ6 R Pro
Processed with APP - PI - PS
Wünsche allen einen guten Rutsch und ein gesundes neues Jahr!
Happy new year!
ASI 2600 MC Pro
TS Optics 65/420 APO
ZWO OAG - EAF - Filterdrawer - Asiair Pro
Optolong L-Extreme 2"
6 x 600s
TS-Optics Photoline 140mm
Touptek ToupTek 571c
iOptron CEM70G
84 shots 300 sec each
Antlia Tri Band RGB Pro 2"
Elaboration with Pixinsight
Very wet weather, even if i used dew heaters for the telescope i realized too later that dew was present also in the flattener lens.....so Flats have not worked very well. I had to use sintetic flats to mitigate issues.
Teleskop Oder Objektiv (Aufnahme)
TS UNC 10" Newton UNC 10" F5
Aufnahmekamera
ZWO ASI 2600 MC Pro
Montierung
SkyWatcher EQ6 R Pro
Filter
Hutech IDAS LPS D2 2"
Zubehör
ZWO ASIAir Pro · ZWO EAF Electronic Auto Focuser · ZWO OAG · Baader Coma Corrector
Software
APF-R · Pleiades Astrophoto S.L. PixInsight 1.8.8 Ripley · Adobe Photoshop 2020 · AstroPixel Processor
Teleskop Oder Objektiv (Nachführung)
TS UNC 10" Newton UNC 10" F5
Nachführkamera
ZWO ASI 120 MINI
100 x 300s
Only 3 x 600s - Thanks to the cloudy Sky
But it´s the first for this Winter, so I have to show it :-))
Testlauf meines vorläufig kompletten ZWO Setups.
Hauptkamera: ZWO ASI2600 MC Pro
Guiding: ZWO OAG - ASI 120 MC-S
Optolong L-Extreme in ZWO Filterschublade
Fokus: ZWO EAF
Steuerung: ZWO Aisair Pro
Teleskop: TS65Q APO
Some weeks ago I published a “widefield” of the Andromeda Galaxy but then decided to take another rendition of it, this time with a smaller FOV and focusing in bringing out the hydrogen clouds (the pink spots) and the dust clouds (the brown filaments) close to the nucleus, which is not so common to see.
In the end I enjoyed it so much that took a crop and also publish as a separated image.
I hope you enjoy.
Shot at Barcarena, Portugal on Sep.28/29, Oct.4/18 of 2021 and Oct.18, Nov.1 2022
Technical details:
RGB: 472x180s (23h36)
Ha: 55x600s (9h10)
LUM: 199x120s (6h38)
Total integraton: 39h24m
RedCat 51 | QHYCCD 268C | Skywatcher EQ6-R Pro | TSOptics IV/IR 2’’ | TS Optics Triplet APO 800/115 | TS Optics TSFLAT2 0.79x | QHYCCD 268C | QHYCCD 268M | Omegon IV/IR Cut 2'' | Astronomik Ha 6nm | RBFocus Myrrdin 2.3 | RBFocus Gaius-S
Acquisition: N.I.N.A. | Processing: Pixinsight
In the constellation of Ursa Major, at about 25 million light years from us lies the Pinwheel Galaxy. This beautiful galaxy has 170,000 light years across, about twice of our Milky Way.
In the photo, two types of color clusters hint on the objects present: the red-pinkish ones are the hydrogen rich nebulas where star forming is taking place and the blue ones on the spiral arms are clusters of young and hot blue stars.
This photo is a cropped reprocessing of my previously published photo.
Shot at Santa Susana, Portugal on Mar.26th and Barcarena, Portugal on Apr.1st and Apr.28th 2022.
Technical details:
LUM: 129 x 180’’ (6h45)
RGB: 160 x 180’’ (8h00)
Ha: 82 x 300’’ (6h50)
Total integration: 21h35
TS Optics Triplet APO 800/115 | QHYCCD 268M | Skywatcher AZ EQ5-GT | Optolong RGB | Baader Ha 6nm TSOptics TSFLAT 3’ 0.79x
Acquisition: N.I.N.A. | Processing: Pixinsight
In the constellation of Canes Venatici but quite close to Ursa Major’s star Alkaid lies the Whirlpool Galaxy, a beautiful interacting grand-design spiral galaxy. It is located at about 31 million light years from us and can be seen during Spring even with binoculars if the sky is dark enough.
Very prominently, this galaxy is interacting with a smaller one - NGC 5195 - the yellowish one on the right. As a result, large tidal tails are formed - those are the faint yellow structures around both galaxies.
Looking closer to M51, dark lanes in the spiral arms can be seen; what are these? They are compressed gas and dust clouds - the raw material for stars. And these new stars being formed are what makes the blue patches seen nearby.
One of amateurs astrophotographers preferred targets, the Whirlpool galaxy is, for sure, an amazing view. I hope you enjoy.
Shot at Santa Susana, Portugal on the 29th and 30th of April, 2022.
IG: @the.cosmic.arena
Technical details:
LUM: 172 x 180s (8h60), BIN1
RGB: 3 x 40 x 180s (6h00), BIN2
Telescope: TS Optics Triplet APO 800/115
Camera: QHYCCD 268M
Mount: Skywatcher AZ EQ5-GT
Filters: Optolong LRGB
Reducer: TSOptics TSFLAT 3’ 0.79x
Acquisition: N.I.N.A.
Processing: Pixinsight, Photoshop
Optique: TSAPO 125-975 Photoline (x0.79)
Monture: HEQ-5
Imageur: Zwo ASI-2600MC-Pro
Guidage: Zwo ASI 120 MC
Prise de vue: ASI Air
Filtre: Optolong L-extreme
200 Brutes de 120s Gain:100 60 DOF
Pré-traitement: SIRIL
Traitement: PixInsight
The Andromeda Galaxy, with a diameter of 200 light years, is a spiral galaxy at approximately 2.5 million light years from Earth and it is the largest galaxy of the Local Group which also contains the Milky Way, the Triangulum Galaxy (M33) and about 44 other smaller galaxies.
The Andromeda Galaxy is approaching the Milky Way at about 100 kilometres per second. This makes Andromeda one of the few blueshifted galaxies that we observe. It is expected to directly collide with the Milky Way in about 4 billion years. Like the Milky Way, the Andromeda Galaxy has satellite galaxies, consisting of 14 known dwarf galaxies. The best known and most readily observed satellite galaxies are M32 and M110.
Canon EOS 60D (unmodded) and TS APO 80/480 Triplet on a HEQ5 guided mount (QHY5L-II + 60/200).
Photos were acquired with EOS Utility and PHD Guiding.
Calibration and stacking with MaximDL and post processing with Photoshop.
► IN THE FOV:
Galaxies: M31, M32, M110
____________________________________________
⚙️ TECHNICAL DETAILS:
480mm - f/6.0 - ISO800
Light Frames: 12x420''
Dark Frames: 9x420''
Bias & Flat Frames
____________________________________________
🙏 FOLLOW ME ON:
My Portfolio - Facebook - Instagram
🔭 ...OR JOIN THE BLUE JOURNEY PROJECT:
TS-Optics Photoline 140mm f/6.5 ToupTek 571c
iOptron CEM70G
Antlia Tri Band RGB Pro 2"
TS-Optics TSAPORed075
61 frames 300 sec
Pleiades Astrophoto PixInsight · Stefan Berg Nighttime Imaging 'N' Astronomy (N.I.N.A. / NINA)
TS-Optics 140mm
Touptek ToupTek 571c
Antlia Tri Band RGB Pro 2"
iOptron CEM70G
60 shots 300 sec each
Elaboration with Pixinsight
Canon EOS600D on a TS-Optics TSAPO65Q 420mm focal length, 65 mm aperture quadruplet refracting telescope
Not very good seeing tonight - turbulent air, strong wind, heat rising.
This nebula is located at around 7500 lights years from the Earth and extend over 165 lights years.
On the upper right part you can see the Fish Head Nebula (IC 1795).
On the left it is a part of the Heart Nebula (IC 1805) and you can see Melotte 15 in the middle of the Heart Nebula, a little star cluster with a lot of dust
Starless version: flic.kr/p/2mA2B1y
One exposure 300s : flic.kr/p/2mwYXX5
-Equipment-
Scope: TS-Optics 94/414 EPDH (414mm focal)
Camera: ZWO ASI533MC Pro at -15°C
Guiding: ZWO OAG
Guiding camera: ZWO ASI 120MM
Mount: Skywatcher NEQ5
Filter: Optrolong L-eXtreme
-Acquisition-
Light :218x300s ( 18h ) at Gain:101 Offset:49
Dark-100x300s Flat-50 Bias-100
Date : Take on 5 night 29, 30 september 2021
and 7, 8, 9 october 2021
Location : France-Alsace Bortle 4/5
-Software-
Carte du Ciel, N.I.N.A, Phd2 , PoleMaster and PixInsight
I use the ForaxX palette for HOO combination
ForaxX website : thecoldestnights.com
And the Ez Processing Suite from darkarcon
darkarcon website : darkarchon.internet-box.ch:8443/
-Pre Processing in PixInsight-
Image Calibration
Cosmetic Correction
Debayer
Subframe Selector
Star Alignement
Local Normalization
Drizzle x2
Dynamic crop
-Processing
Split the master_LRGB into L, R, G, B layer
DynamicBackgroundExtractor each layer
___RGB layer___
Split RGB channels for build Ha and Oiii
Ha=R Oiii= B*0.3+G*0.7
EZ_Soft Stretch
HOO combination with Foraxx formula
R=Ha
G=((Oiii*Ha)^~(Oiii*Ha))*Ha + ~((Oiii*Ha)^~(Oiii*Ha))*Oiii
B=Oiii
Starnet++ for remove stars and build a mask nebula
Color Saturation
Curves Tansformation (K,saturation,hue)
Saturate stars for push up stars color
SCNR with star Mask for remove green in stars (OSC camera)
Bring back the stars with PixelMath
___L layer___
Ez_Deconvolution
Ez_Denoise
Ez_Soft Stretch
Ez_HDR
Local Histogram Equalization with nebula mask
UnsharpedMask with nebula mask
___LRGB___
Final Curve Transformation
DarkStructureEnhance script
EZ_Star Reduction
Save as BMP 32bit file
Clear skies !
Imaging telescope or lens:GSO 8" f/5 Newton
Imaging camera:ZWO ASI 183 MM PRO
Mount:SkyWatcher NEQ6 Pro Goto
Guiding telescope or lens:GSO 8" f/5 Newton
Guiding camera:Astrolumina Alccd5L-IIc
Focal reducer:Pal Gyulai GPU Aplanatic Koma Korrector 4-element
Software:Main Sequence Software Seqence Generator Pro, Adobe PhotoShop CS5, FitsWork 4, DeepSky Stacker Deep Sky Stacker 3.3.4, PHD2 Guiding
Filters:Baader Ha 1.25" 7nm, Baader Planetarium SII 1.25" 8nm, Baader Planetarium O3 1.25" 8.5nm
Accessory:TSOptics TS Off Axis Guider - 9mm
Dates:Sept. 11, 2018, Sept. 19, 2018, Sept. 20, 2018
Frames:
Baader Ha 1.25" 7nm: 32x600" (gain: 200.00) -20C bin 1x1
Baader Planetarium O3 1.25" 8.5nm: 32x600" (gain: 200.00) -20C bin 1x1
Baader Planetarium SII 1.25" 8nm: 35x600" (gain: 200.00) -20C bin 1x1
Integration: 16.5 hours
Darks: 35
Flats: 27
TS-Optics TSED503 ED apochromatic refractor (not quite apochromatic, but with higher-quality glass that reduces CA noticeably compared to achromats. I don't see any CA here).
330 mm focal length, 50 mm aperture. Telescopes don't come any smaller than this.
Camera: Canon EOS600D
TS-Optics Photoline 140mm
Touptek ToupTek 571c
Antlia Tri Band RGB Pro 2"
iOptron CEM70G
38 shots 300 sec each
Elaboration with Pixinsight
Different elaboration from the past
Imaging telescope or lens:GSO 8" f/5 Newton
Imaging camera:ZWO ASI 183 MM PRO
Mount:SkyWatcher NEQ6 Pro Goto
Guiding telescope or lens:GSO 8" f/5 Newton
Guiding camera:Astrolumina Alccd5L-IIc
Focal reducer:Pal Gyulai GPU Aplanatic Koma Korrector 4-element
Software:Adobe PhotoShop CS5, FitsWork 4, CCDCiel, DeepSky Stacker Deep Sky Stacker 3.3.4, PHD2 Guiding
Filters:Baader Ha 1.25" 7nm, Baader Planetarium SII 1.25" 8nm, Baader Planetarium O3 1.25" 8.5nm
Accessory:TSOptics TS Off Axis Guider - 9mm
Dates:July 18, 2018, July 19, 2018, July 24, 2018
Frames:
Baader Ha 1.25" 7nm: 23x600" (gain: 200.00) -20C bin 1x1
Baader Planetarium O3 1.25" 8.5nm: 25x600" (gain: 200.00) -20C bin 1x1
Baader Planetarium SII 1.25" 8nm: 25x600" (gain: 200.00) -20C bin 1x1
Integration: 12.2 hours
Darks: 29
Flats: 29
Object description (wikipedia.org):
The Elephant's Trunk nebula is a concentration of interstellar gas and dust within the much larger ionized gas region IC 1396 located in the constellation Cepheus about 2,400 light years away from Earth. The piece of the nebula shown here is the dark, dense globule IC 1396A; it is commonly called the Elephant's Trunk nebula because of its appearance at visible light wavelengths, where there is a dark patch with a bright, sinuous rim. The bright rim is the surface of the dense cloud that is being illuminated and ionized by a very bright, massive star (HD 206267) that is just to the west of IC 1396A. (In the Figure above, the massive star is just to the left of the edge of the image.) The entire IC 1396 region is ionized by the massive star, except for dense globules that can protect themselves from the star's harsh ultraviolet rays.
The Elephant's Trunk nebula is now thought to be a site of star formation, containing several very young (less than 100,000 yr) stars that were discovered in infrared images in 2003. Two older (but still young, a couple of million years, by the standards of stars, which live for billions of years) stars are present in a small, circular cavity in the head of the globule. Winds from these young stars may have emptied the cavity.
The combined action of the light from the massive star ionizing and compressing the rim of the cloud, and the wind from the young stars shifting gas from the center outward lead to very high compression in the Elephant's Trunk nebula. This pressure has triggered the current generation of protostars.
Processed some old data from november last year.
Session Information :
* 51° N 3° E
* Torhout, Belgium
* Capture Date : 30.11.2019
Object Information
* Type : Solar edge with protuberances.
* Distance : 0.986 AU or roughly 147.5 million km
Hardware
* Mount : Celestron CGX
* Imaging Scope : TS Optics 152mm f/5.9 Achromat
* ERF : Baader 2" UV/IR Cut
* Filter : Daystar Quark Hydrogen-Alpha (Chromosphere)
* Imaging Camera : ZWO ASI 174MM
Exposure Settings
* Exposure : 6ms
* Gain : 0
* Gamma : 25
* Frames Surface : 4.000
* Frames Surface Stacked : 10% (400)
* Frames Protuberance : 4.000
* Frames Protuberance Stacked 10% (400)
Capture Software
* FireCapture
Processing Software
* AutoStakkert!
* RegiStax
* Adobe Photoshop
* Topaz GigaPixel AI
* Topaz Sharpen AI
* Topaz DeNoise AI
Commonly known as Gecko Nebula, LBN 437 is a molecular cloud in constellation Lacerta (“lizard”), located at about 1,200 light years from us. Notably, this nebula is paired with a much larger one - Sh2-126 - here seen as the red cloud permeating the image. In the densest region, here seen near the center, a star forming region exists and includes an Herbig Haro object associated with V375 Lacertae.
Shot at Santa Susana, Portugal on August 25th, 29th, 30th and September 1st 2022.
Technical details:
Lum: 250x180s
Ha: 62x300s
Red 18x180s
Green: 50x180
Blue: 51x180
Total integraton: 23h37m
TS Optics Triplet APO 800/115 | QHYCCD 268M | Skywatcher EQ6-R Pro | Optolong LRGB | Baader Ha 7nm | TSOptics TSFLAT 3’ 0.79x | RBFocus Gaius-S | USB_Foc Electronic Focuser
Acquisition: N.I.N.A. | Processing: Pixinsight
27 x 90sec f/6 360mm ISO1600
total exposure time 40 min 30sec
Star Adventurer Pro
TS Optics 60/360 FPL53 APO Refractor
Processed in Siril, Photoshop and Lightroom
Our version of Messier 106 galaxy with the whole AstroFleet team. The data were acquired with our setup (TS-Optics CF-APO 155mm & ASI2600MM Pro) hosted at PixelSkies, Spain.
Messier 106 is a barred spiral galaxy located in the constellation Canes Venatici, approximately 22 to 25 million light-years away from Earth. It was discovered by Pierre Méchain in 1781 and was later included in Charles Messier's catalog of nebulae and star clusters.
Galaxy’s dust lanes formed a spiral pattern which can be traced into its bright central core. The spiral arms end in bright blue knots, which are young star clusters dominated by very hot, luminous, massive stars which only have a lifetime of a few million years. Also conspicuous is the yellowish remnant of an older spiral arm, whose color indicates that its more massive stars ceased to shine long ago.
Since the 1950s, Messier 106 has been known as a source of radio emission, and appears much larger in radio emission than in visible light. It is also a Seyfert galaxy; due to unusual emission lines in its spectrum, discovered by Carl Seyfert in 1943, we now suspect that matter in the galaxy is falling into a supermassive black hole at its center.
Two supernovae were discovered in Messier 106: SN 1981K et SN 2014bc.
- SN 1981K: This supernova (type II) occured on November 3 1981 by swiss astronomer Paul Wild.
- SN 2014bc: This supernova (type II) were discovered by PS1 Science Consortium.
RA 12h 18m 04.4s
DEC +47° 29’ 16.0"
ORIENTATION Up is 273 degrees E of N
CONSTELLATION Canes Venatici
DISTANCE 23.7 million ly
Captured March 2023
Fiel Of view: 62.6 x 41.7 arcmin
Total integration time of 58.8 hours.
Technical Details
Data acquisition & processing: AstroFleet team
Location: PixelSkies, Castilléjar, Granada, Andalucia, SPAIN
Ha: 203*600s
L: 439*180s
R: 20*180s
G: 20*180s
B: 20*180s
Optics: TS-Optics CF-APO 155mm @ F/8
Mount: iOptron CEM70
CMOS: ZWO ASI2600MM Pro
Canon EOS600D on a TS-Optics TSAPO65Q 420mm focal length, 65 mm aperture quadruplet refracting telescope
Tonight the terminator has moved further west, revealing all of Mare Nectaris, the Rupes Altai and the famous three-crater group Theophilus, Cyrilllus and Catalina.
Within around 2 degrees of angular distance from the moon, in the upper right hand corner, is Regulus, the "little king" in constellation Leo.
Canon EOS600D on a TS-Optics TSAPO65Q 420mm focal length, 65 mm aperture quadruplet refracting telescope
Tonight the Mare Nectaris takes centre stage.
Sunspot AR2740 @ 6562.8Å
Processed some data I had given up on after seeing the quality graph in AutoStakkert. After several hours of messing with the data in several editors I'm actually very happy with this result !
Session Information :
* 51° N 3° E
* Torhout, Belgium
* Capture Date : 05.05.2019
* Surface Capture Start : 12:58:32 UTC
* Surface Capture Mid : 12:58:47 UTC
* Surface Capture End : 12:59:03 UTC
* Protuberance Capture Start : 13:00:03 UTC
* Protuberance Capture Mid : 13:00:15 UTC
* Protuberance Capture End : 13:00:27 UTC
Object Information
* Type : Sunspot
* Designation : AR2470
* Distance : 1.009 AU or roughly 150.9 million km
Hardware
* Mount : Celestron CGX
* Imaging Scope : TS Optics 152mm f/5.9 Achromat
* ERF : Baader 2" UV/IR Cut
* Filter : Daystar Quark Hydrogen-Alpha (Chromosphere)
* Imaging Camera : ZWO ASI 174MM
Exposure Settings
* Exposure : 6ms
* Gain : 0
* Gamma : 25
* Frames Surface : 4.000
* Frames Surface Stacked : 10% (400)
* Frames Protuberance : 3.000
* Frames Protuberance Stacked 10% (300)
Capture Software
* FireCapture
Processing Software
* AutoStakkert!
* RegiStax
* Adobe Photoshop
* Topaz DeNoise AI
Sharpless 101 (Sh2-101) is a H II region emission nebula located in the constellation Cygnus. It is sometimes also called the Tulip Nebula because it appears to resemble the outline of a tulip when imaged photographically. It was catalogued by astronomer Stewart Sharpless in his 1959 catalog of nebulae. It lies at a distance of about 6,000 light-years from Earth.
Sharpless 101 (Sh2-101) è una nebulosa ad emissione situata nella costellazione del Cigno. A volte viene anche chiamata Nebulosa Tulipano perché sembra assomigliare al contorno di un tulipano. Fu catalogata dall'astronomo Stewart Sharpless nel suo catalogo di nebulose del 1959. Si trova ad una distanza di circa 6.000 anni luce dalla Terra.
---------------------------
DATA
June 2017/August 2018
Location: Santa Cesarea Terme (LE)
Telescope: TSOptics apo 102/715 Photoline
Guide: refractor 80/400, camera QHYCCD Q5L-II-M
Camera: Moravian G2-8300FW mono
Mount: Ioptron ieq45-pro
Filters:
Baader Ha 7nm 36mm: 15x600" -20°C bin1
Baader OIII 8.5nm 36mm: 14x600" -15°C bin1
Baader SII 8nm 36mm: 16x600" -15°C bin1
Total exposure: 7.5 hours
Software: Pixinsight 1.8
This is a new elaboration from the same session as per
M31_20Sep2025 Andromeda Galaxy
TS-Optics Photoline 140mm f/6.5 ToupTek 571c
iOptron CEM70G
Antlia Tri Band RGB Pro 2"
TS-Optics TSAPORed075
61 frames 300 sec
Pleiades Astrophoto PixInsight · Stefan Berg Nighttime Imaging 'N' Astronomy (N.I.N.A. / NINA)
Canon EOS600D on a TS-Optics TSAPO65Q 420mm focal length, 65 mm aperture quadruplet refracting telescope
Near the zero meridian there is a long row of very large, interesting craters: Ptolemaeus, Alphonsus, Albategnius, Arzachel, Purbach, Regiomontanus, Walter, Nonius, Stöfler ...
Imaging telescope or lens:GSO 8" f/5 Newton
Imaging camera:Moravian G2-8300FW
Mount:SkyWatcher NEQ6 Pro Goto
Guiding telescope or lens:GSO 8" f/5 Newton
Guiding camera:Astrolumina Alccd5L-IIc
Focal reducer:Pal Gyulai GPU Aplanatic Koma Korrector 4-element
Software:Adobe PhotoShop CS5, FitsWork 4, DeepSky Stacker Deep Sky Stacker 3.3.4
Filters:Baader Ha 1.25" 7nm, Baader Planetarium SII 1.25" 8nm, Baader Planetarium O3 1.25" 8.5nm
Accessory:TSOptics TS Off Axis Guider - 9mm
Dates:Feb. 21, 2018, Feb. 23, 2018, Feb. 25, 2018
Frames:
Baader Ha 1.25" 7nm: 11x600" -20C bin 1x1
Baader Planetarium O3 1.25" 8.5nm: 13x600" -20C bin 1x1
Baader Planetarium SII 1.25" 8nm: 14x600" -20C
Integration: 6.3 hours
Darks: 35
Flats: 21
Bias: 100