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Genova, Italy (12 Aug 2021 - 02:39 GMT+2)

 

Orange vintage C8 (203 F10 SC Telescope) on EQ5 Mount

 

QHY5L-II Color Camera @ F25 (Barlow APO 2.5x)

 

Recording: SharpCap 4.0 (800x480 @ 44fps - 2min)

 

Jupiter:

Best 3685 frames of 5276 (80%)

Stacking+Wavelets: AstroSurface REDSHIFT-1

 

Europa and Ganimede:

Best 1741 frames of 5276 (33%)

Stacking: AutoStakkert! 3.1.4

Wavelets: Registax 6.1

 

Final: GIMP 2.10.8

Sol Región Activa 2741 - Barlow Powermate 2'5X

 

Telescopio: Skywatcher Refractor AP 120/900 f7.5 EvoStar ED

Cámara: ZWO ASI178MM

Montura: EQ5 Bresser EXOS2 motorizada sin goto

Filtros: - Baader Neutral Density Filter 1¼" (ND 0.6, T=25%)

- Baader Solar Continuum Filter 1¼" (540nm)

Accesorios: - Baader 2" Cool-Ceramic Safety Herschel Prism

- TeleVue Lente de Barlow 2,5x Powermate 1,25"

Software: SharpCap, Pipp, AutoStakkert, Registax y Photoshop

Fecha: 2019-05-10

Hora: 16:59 T.U.

Lugar: 42.615 N -6.417 W (Bembibre Spain)

Vídeo: 2 minutos

Resolución: 1024 x 768

Gain: 100

Exposure: 0,000049

Frames: 14662

Frames apilados: 10%

FPS: 121.95

IC434 Horsehead and Flame Nebula, and M42 Orion and Running Man Nebula - Test FOV ASI6200MC, 6th February 2020. ASI6200MC Pro. Optolong L-eNhance. TSAPO65Q. SkyWatcher EQ6-R Pro / 6R StellarDrive. 8 x 10 Mins with SharpCap Pro. Processed in NINA. Some artefacts remain - issues processing.

M51 with the Rokinon lens 135mm

Zwo ASI071MC Pro cooled color camera

Had clear skies last night, but windy

Pegasus Power Box and EAF

Zwo IR/cut filter 2"

#SharpCap Pro, PoleMaster

Orion Skyview Pro EQ mount

100 Gain offset 20, 0c cooling,

M51 was 55 minutes, 30 seconds exposure each

50 darks 50 flats and 50 bias frames

Astro Pixel Processor and PS

Plus the moon, Orion 102mm Mak-Cass telescope Zwo 290MC camera AS3 RegiStax6 and PS

Taken on 6 April 2018 at just after midnight (utc), with Celestron NexStar 6se SCT and ZWO ASI224 mc camera. Video was captured in SharpCap and processed in Autostakkert and PSP8.

Equipo Principal: ZWO ASI183MC-pro + Askar ACL200 + EQ6-R-Pro + ZWO EAF

 

Equipo guía: Hercules 32/130 mini guidescope, Player One Neptunce C-II

 

ASI183MC-pro:

*Gain 111, -15 º C, Optolong L-QEF 2", 106x180"

 

Tiempo Total de Integración: 5.3 h

 

100 Darks

50 Flats / 50 Darkflats por filtro

 

Polar alignment: Sharpcap 4

Adquisición: SGP 3.2

Guiado: Phd2

Procesado: Pixinsight 1.8.9, PS

O Mare Crisium possui 556 km de diâmetro e 176.000 km² de área. Tem um piso muito plano, com um anel de cristas rugosas (dorsa) em direção aos seus limites externos.

A bacia é do período pré-imbriano, há 4,55 a 3,85 bilhões de anos.

Mare Crisium foi batizado por Giovanni Riccioli, cujo sistema de nomenclatura de 1651 foi padronizado.

 

📆 24-08-2021 / 02:39 UTC

🔭 Sky-Watcher 150mm - f/8

📷 ZWO ASI 120MC-S + Barlow 2x + UV/IR Cut

Capture Area: 1280x960 pixels

2500 frames stacked

👨‍💻 SharpCap + PIPP + AS!3 + Astrosurface

🇧🇷 Porto Real-Brazil

Bortle 4/5 Sky

Sinus Iridum (Latin: "Rainbow Bay") is a basaltic lava plain located on the northwestern extent of Mare Imbrium on the Moon. It is surrounded, in a northeast-southwest direction, by the Jura Mountains range. The protruding portion to the southwest is called Promontorium Heraclides and the northeast is called Promontorium Laplace.[2] This plain and the underlying mountain ranges are considered to be one of the most beautiful spots on the Moon and are a favorite observation point among astronomers.

 

The bay-shaped plain does not contain any relevant impact points but includes the craters Heraclides E to the south, Laplace A along its eastern boundary and Bianchini G to the north. The surface is flat but is marked by a small amount of back.

Sinus Iridum (latim: "Baía do Arco-íris") é uma planície da lava basáltica localizada na extensão noroeste do Mare Imbrium, na Lua. É cercada, na direção nordeste–sudoeste, pela cadeia de Montes Jura. A parte saliente a sudoeste é chamada de Promontorium Heraclides e a nordeste é chamada de Promontorium Laplace.[2] Esta planície e as cadeias de montanhas subjacentes são considerados um dos mais bonitos pontos da Lua e é um ponto favorito de observação entre os astrônomos.

 

A planície, em forma de baía, não contém nenhum ponto relevante de impacto mas inclui as crateras Heraclides E ao sul, Laplace A ao longo de seu limite oriental e Bianchini G ao norte. A superfície é plana mas é marcada por pequena quantidade de dorsa.

 

Sky-Watcher 150mm - f/8

ZWO ASI 120MC-S + Barlow 2x + UV/IR Cut

SharpCap + PIPP + AS!3 + Astrosurface

Porto Real-Brazil

Bortle 4/5 Sky

Veil Nebula (redone in Siril)

Eastern Vail (NGC6992)

Pickering Triangle

Witches Broom (NGC6960)

 

ISO1600

31x245 sec (2h06'35")

16 light

32 bias

12 dark

33 flat

 

GT81

CEM25P

Nikon Z6

L-Enhance

asi224mc guide

 

PHD2 2.6.9

Sharpcap polar alignment 3.2

Digicamcontrol 2.1.2.0

 

Siril 1.2.0-beta2

GIMP 2.10.34

 

32*30 second subs, 16 minutes total capture time

Photographed at Curramore, QLD, Bortle Class 2

Acquisition software: SharpCap

Unguided

ASI294MC Pro temp = 0

Gain 120.

Processed in AstroPixel Processor, light only

The front element of the RASA8 had started to dew up. Bummer !!

NGC2237 Rosette Nebula

 

Integration 2h02'

Lights 122x60"

Darks 40x

Bias 55x

Flats 55x

 

GT81

CEM25P

ASI533mc

L-Enhance

ASI224mc guide

 

PHD2 v2.6.9dev4

Sharpcap 3.2

DSS 4.2.5

GIMP 2.10.20

  

[ZWO ASI533MC Pro]

Debayer Preview=On

Pan=0

Tilt=0

Output Format=FITS files (*.fits)

Binning=1

Capture Area=3008x3008

Colour Space=RAW16

Hardware Binning=Off

Turbo USB=100(Auto)

Flip=None

Frame Rate Limit=Maximum

Gain=101

Exposure=60

Timestamp Frames=Off

White Bal (B)=95

White Bal (R)=52

Brightness=5

Temperature=-7

Cooler Power=4

Target Temperature=-10

Cooler=On

Auto Exp Max Gain=300

Auto Exp Max Exp M S=30000

Auto Exp Target Brightness=100

Mono Bin=Off

Banding Threshold=35

Banding Suppression=0

Apply Flat=None

Subtract Dark=None

#Black Point

Display Black Point=0

#MidTone Point

Display MidTone Point=0,5

#White Point

Display White Point=1

Notes=

TimeStamp=2021-03-02T21:50:48.9938812Z

SharpCapVersion=3.2.6433.0

 

Data - 24/04/2021

Hora - 20:54 ~ 21:45 local (-3 UTC)

Lat - 7,13S

Log - 34,83W

Local - João Pessoa, PB - Brasil

Bortle - Class 8

Câmera - ZWO ASI 120MC-S

Telescópio - SW 150mm F8

Montagem - EQ5

Motorização - OnStep Brasil

Light - filme de 2000 frames (empilhados 50%)

Software Captura - SharpCap

Softwares Processamento - PS/Registax

Seeing 2/5

Transparency 2.5/5.

 

5 images derotated. 1.5X drizzle

 

C9.25 EDGEHD (F=2350mm)

ZWO120MC

SharpCap

Winjupos

AutoStakkert

PixInsight

Object Details: The attached composite shows the huge sunspot groups AR2993 & AR2994 as they were just rotating on back on April 18th. Having previously posted images showing them near mid-disk (attached here - www.flickr.com/photos/homcavobservatory/52034939249/

), as a result of a 4 day blackout due to a snow storm that week, I just had the opportunity to process this data).

 

During their passage across the Earth-facing side, they threw a variety of flares including two X-class. Large enough to be seen 'naked-eye' (with a proper solar filter of course), helioseismic imaging is currently tracking a large active region on the non-Earth facing side of the Sun which may be AR2994. If it remains intact it should rotate on the eastern limb in approximately a week.

 

Image Details: The images making up this composite were taken by Jay Edwards on the early morning hours of April 18, 2022 under high clouds of varying opacity from the RoR observatory I built at my home here in upstate, NY using:

 

At left: An Orion ED80T CF (i.e. an 80MM, f/6 triplet, carbon-fiber refractor) with a 0.8x Televue field flattener / focal reducer, Kendrick film solar filter and an unmodded Canon 700D DSLR controlled by APT, meant simply as a reference it is a single-frame taken at ISO 100 and with a 1/2500 second exposure;

 

At right: a vintage 1970, 8-inch, f/7 Criterion newtonian reflector with a home-made Baader (visual grade material) off-axis solar filter and a ZWO ASI290MC planetary camera / auto-guider. They are stacks of several hundred frames, in this case at various exposures, selected from short video clips consisting of several thousand.

 

The ASI290MC was placed at prime focus and was controlled by SharpCap Pro and all scopes were tracked using a Losmandy G-11 goto mount running a Gemini 2 control system. The images also utilized a set of specialized planetary filters (Infrared, Ultraviolet & Methane) in addition to the over-the-aperture solar filter. As shown here the entire composite has been resized down to HD (one-third of it's original resolution).

 

I'm looking forward to seeing AR2994 survives it's trip around the Sun !

 

Similar composites or various solar system objects, many using additional wavelengths, can be found at the links attached below:

 

Solar:

 

www.flickr.com/photos/homcavobservatory/51992208177/

 

www.flickr.com/photos/homcavobservatory/51948806640/

 

www.flickr.com/photos/homcavobservatory/51747214403/

 

www.flickr.com/photos/homcavobservatory/50815383151/

 

www.flickr.com/photos/homcavobservatory/50657578913/

 

www.flickr.com/photos/homcavobservatory/51027134346/

 

www.flickr.com/photos/homcavobservatory/51295865404/

 

Saturn:

 

www.flickr.com/photos/homcavobservatory/51489515877/

 

www.flickr.com/photos/homcavobservatory/51345118465/

 

www.flickr.com/photos/homcavobservatory/51007634042/

 

www.flickr.com/photos/homcavobservatory/51316298333/

 

www.flickr.com/photos/homcavobservatory/50347485511/

 

www.flickr.com/photos/homcavobservatory/50088602376/

 

Jupiter:

 

www.flickr.com/photos/homcavobservatory/51405393195/

 

www.flickr.com/photos/homcavobservatory/51679394534/

 

www.flickr.com/photos/homcavobservatory/51307264271/

 

www.flickr.com/photos/homcavobservatory/50303645602/

 

www.flickr.com/photos/homcavobservatory/50052655691/

 

www.flickr.com/photos/homcavobservatory/50123276377/

 

www.flickr.com/photos/homcavobservatory/50185470067/

 

www.flickr.com/photos/homcavobservatory/50993968018/

 

www.flickr.com/photos/homcavobservatory/51090643939/

 

Mars:

 

www.flickr.com/photos/homcavobservatory/50425593297/

 

www.flickr.com/photos/homcavobservatory/50594729106/

 

www.flickr.com/photos/homcavobservatory/50069773341/

 

www.flickr.com/photos/homcavobservatory/50223682613/

Jones-Emberson 1 (PK 164 + 31.1) est une nébuleuse planétaire de magnitude 14 située dans la constellation du Lynx, à une distance de 1600 années-lumière. C'est une nébuleuse planétaire avec une faible luminosité de surface. L'étoile centrale d'une magnitude de 16,8 est une naine blanche très bleue de la taille de la Terre

matériel :

FSQ-106ED, extender x1.6

monture NEQ6 pro goto

caméra ZWO 1600MC-C avec filtre IDAS-LPS-D1

logiciel acquisition : Sharpcap 3.2

logiciel guidage : phd2

traitement avec deepskystacker, PSS

 

Image issue de 40poses de 300s

  

Very tricky to process this one. Lots of dusty goodness, but making it stand out is hard work. This is my 15th iteration, and it'll do. I may get some more data next month with longer exposures.

 

The Iris Nebula (NGC 7023, Caldwell 4) is a blue, flower-shaped reflection nebula in the constellation Cepheus, about 1,400 light-years from Earth. It glows blue because dust grains scatter light from its central star, HD 200775, and some red light comes from photoluminescence where dust converts ultraviolet radiation to visible red light.

 

Image Details:

- Imaging Scope: William Optics 61mm ZenithStar APO

- Imaging Camera: ZWO ASI183MC Color with IR Cut filter

- Guiding Equipment: Celestron Starsense Autoguider

- Acquisition Software: Sharpcap

- Guiding Software: Celestron

- Light Frames: 25*4 mins @ 100 Gain, Temp -20C

- Dark Frames: 10*4 mins

- Stacked in Deep Sky Stacker

- Processed in PixInsight, Adobe Lightroom and Topaz Denoise

 

This is a composite shot of Saturn with a few of its moons. Saturn reached opposition on the night of July 9th and this shot was taken six nights later when the sky was (slightly) less cloudy. It would have been nice to have taken the shot closer to when it reached opposition but this was the first opportunity. However it still looks quite big and bright with plenty of detail visible. The predicted distance of Saturn at opposition was 1,351,000,000 km with its disk measuring 18.4 arcseconds in diameter. We measured Saturn's disk to be 18.1 arcseconds (an expected reduction in size after nearly a week of receding again) and giving us a distance of 1,352,364,750 km. So the calculations seem reasonably accurate.

 

Captured with SharpCap

Processed in PIPP, AutoStakkert and Registax

Post processed and composited Photoshop

 

For planet:

4,784 frames of video

Gain 100%

Exposure 0.052728 seconds

 

For moons:

284 frames of video

Gain 100%

Exposure 0.640857 seconds

 

Equipment:

Sky-Watcher Explorer-150PDS

Sky-Watcher EQ5 Mount

ZWO ASI120 MC camera

x2 Barlow with extension tube (equivalent to x3.3)

Telescopio: Refractor Bresser Messier Acro 102/460 f4.5

Cámara: ZWO ASI178MM

Montura: EQ5 Bresser EXOS2 motorizada sin goto

Filtros: Baader UV/IR Cut / L-Filter

Software: SharpCap, AutoStakkert, Registax y Photoshop

Fecha: 2019-03-20

Hora: 02:40 T.U.

Fase lunar: 98.8% 13.5 días Creciente

Lugar: 42.615 N -6.417 W (Bembibre Spain)

Vídeo: 2 minutos

Resolución: 3096 x 2080

Gain: 100

Exposure: 0,000451

Frames: 732

Frames apilados: 22%

FPS: 6.09

Taken from Oxfordshire, UK with a William Optics 70mm refractor, on an EQ5 Pro mount on a permanent pier. Camera used was a ZWO ASI120MC with a 5x Powermate Barlow attached to the camera nose.

 

4,000 frame video shot in Sharpcap, best 75% of those frames were stacked using Autostakkert! 3, then processed in Lightroom and Fast Stone Image Viewer.

Tránsito de Mercurio

 

Telescopio: Skywatcher Refractor AP 120/900 f7.5 EvoStar ED

Cámara: ZWO ASI178MM

Montura: iOptron CEM40

Filtros: - Baader Neutral Density Filter 1¼" (ND 0.9, T=12.5%)

- Baader Solar Continuum Filter 1¼" (540nm)

Accesorio: Baader 2" Cool-Ceramic Safety Herschel Prism

Software: SharpCap, AutoStakkert, Registax y Photoshop

Fecha: 2019-11-11

Hora: 12:47 T.U. (Tiempo universal)

Lugar: 42.615 N -6.417 W (Bembibre Spain)

Vídeo: 60 segundos

Resolución: 800 x 600

Gain: 72

Exposure: 0,000032

Frames: 6044

Frames apilados: 10%

FPS: 100.60

On the morning of Friday 13th May my friend Stuart tipped me off that there was a huge looping prominence visible on the Sun. It was cloudy at the time but I could see a few gaps possibly heading my way so I set up the solar telescope just in case. What followed was a hugely frustrating imaging session, with strong gusts of wind and lots of cloud scudding past the Sun every time I started to capture video. My laptop screen also hadn't been fixed yet so it was incredibly difficult to get focus and exposure right. By the time I got a clear look at the Sun the large prominence in question had lifted off and vanished! However, I manage to get some ok shots out of the imaging session.

 

Coronado PST and ASI120MC fitted with a 2 x Barlow. I shot either 500 or 1000 frame videos with SharpCap and stacked the best 50% of the frames using Autostakkert! 3. Processing was done in Lightroom, Photoshop CS2 and Fast Stone Image Viewer.

The moon passed in front of Mars on Monday night. This brief timelapse of the moment of "occultation" and re-emergence shows the view through a small but powerful backyard telescope married with contemporary imaging gear. I am pleased to see sufficient detail on the surface of Mars to note how much the planet rotated during the hour and a quarter it was hidden by the moon.

 

Tech Stuff:

Questar 3.5"/TV 2.5X PowerMate/QHY 5iii 178 camera. Captured in SharpCap, processed with PIPP, AstroSurface, and Luxea Pro video editor. From my yard in Westchester County NY.

Markarian's Chain in Virgo Cluster of Galaxies. Just as galaxies are communities of hundreds of billions of stars, Unimaginably large clusters of galaxies exist containing thousands of them. The Virgo Galaxy Cluster is one such cluster. Within this galaxy cluster is an smaller grouping we call Markarian's Chain. It has the shape almost of a ball and chain. The field of view of larger aperture telescopes are not wide enough to fit in the galaxies that comprise both the "ball" and the "chain" in that shape. So, this image is only wide enough to contain the "ball", or the grouping of galaxies that are distributed in a round fashion. While 10 to 12 galaxies in this image may be readily seen, others are smaller and fainter appearing. In fact, a careful eye, and a magnified view, can find more than 20 galaxies. Look for small elongated smudges that are not round and crisp like stars are. And don't forget the tiny, distant galaxy hiding behind the "halo" of the bright M86 galaxy. Three of the galaxies can be found along the bottom of the image near the center of the picture's border.

 

This image is the result of one and a half hours of 5 minute exposures on the Ritchey-Chretien 6 inch telescope with a Canon T7i DSLR at the prime focus. The exposures were all 300 seconds at ISO 800. The auto guiding work was done with a Skywatcher 50ED Evoguide guide scope and a ZWO ASI183MC camera connected to PHD2 auto-guiding software. Polar alignment was done with Sharpcap Pro software. Note: The thin straight line through the image was made by a satellite passing overhead during one of the frames.

2 minutes video recording - de-rotated

Seeing 3/5

Transparency 3/5

 

C9.25 EDGEHD

ZWO120MC

SharpCap

Winjupos

AutoStakkert

PixInsight

Tonight's Moon, Waxing Gibbous 65% illuminated

 

Altair Astro 72EDF

AA IMX178C Hypercam

AZ-GTI mount

 

Best 100 frames stacked with AS3! of 2000 captured with SharpCap 3.2 Pro.

Post processed with Adobe Photoshop CC2019

NGC 7380, ou nébuleuse du Sorcier, est un amas ouvert situé à environ 8000 années-lumière de la Terre dans la constellation de Céphée.

Les vents stellaires y ont façonné les gaz et la poussière, ce qui a engendré une forme qui pour certains évoque la silhouette d’un sorcier médiéval. Cette région de formation d’étoiles s’étend environ sur 100 années-lumière, ce qui dans notre ciel, lui donne une taille apparente légèrement plus grande que celle de la pleine Lune.

 

Matériel

lunette FSQ-106ED équipée Extender x1.6 sur monture NEQ6 pro goto

Caméra ZWO ASI1600MC-C équipée filtre IDAS-LPS-D1

autoguidage avec caméra ZWO ASI120MM sur lunette APM 50*240

70 poses de 240s

 

logiciels :

acquisition : Sharpcap 3.2

guidage : PHD2

prétraitement : Deepskysticker

Traitement : Photoshop CS6

Cadre : Gimp

Data - 14/08/2021

Hora - 18:15 local (-3 UTC)

Lat - 7,13S

Log - 34,83W

Local - João Pessoa, PB - Brasil

Bortle - Class 8

Telescopio - SW 1200mm F8

Câmera - ZWO ASI 120 Color

Método - Projeção positiva

Ocular - 9mm Plossi GSO

Montagem - Dobsoniana manual

Ligth - 1032 frames (50%)

Software Captura - SharpCap

Softwares Processamento - PIPP/AS3/Registax/PS

#astfotbr

The Sun's chromosphere is the layer just above the photosphere. This is what you are seeing. The photosphere is the layer we see when you directly look at the Sun. Don't do that!

The chromosphere is not visible to us without a Hydrogen-alpha filter on your telescope. Around the edge of the Sun you see prominences. On the disc itself, the dark lines are filaments, the bright areas are are plages, and the dots are sunspots.

 

The image was captured using:

This picture was capture using a 60mm Lunt Hα telescope in the double stack configuration.

Camera: ZWO ASI294MC Pro

Capture software: SharpCap

 

Processing was done using:

Autostakkert

Adobe Light Room Classic

Adobe Photoshop

Perseus Double Cluster

 

The Double Cluster (also known as Caldwell 14) consists of the open clusters NGC869 and NGC 884 (often designated h Persei and χ (chi) Persei, respectively), which are close together in the constellation Perseus.

 

This was shot in RGB over the course of several nights after my first target was behind out trees

.

Total Integration: 5 hours 35

 

Minutes

Equipment:

Skywatcher Evostar 100 ED, Flattener

ZWO ASI533MM, ZWO AM5, EAF, EFW, ASI120 guide cam

Stellarvue 50mm Guide Scope F050G

Chroma 3nm Red, Green, Blue Filters

 

Acquisition: NINA, Sharpcap for PA

 

Stacked PI, bias, flats, flatdarks

Processed/edited in PI, very minor editing in PS/LR

 

High Resolution Image: www.astrobin.com/z57dhd/

 

IG: jlratino

FB: JL Ratino

Waning Gibbous/85.1%

Moon Age 19.02 out of 29.39 days

 

I recently obtained a used set of planetary imaging filters containing Wratten no. 25 (red), no. 21 (orange), no. 12 (yellow), no. 58A (green), and no. 80A (blue). I used the first three filters to see if I could distinguish any differences. I think the red filter produced the better results although it was difficult to tell. Yellow came in a close second. The orange was a bit soft in comparison.

 

The moon was just past meridian when I started imaging but was about 31 degrees above the southern horizon. The seeing was quite bad. According to the experts, a red filter can reduce seeing effects. That seems consistent with my findings. We must live in the same universe.

 

TMB 80mm f/6.3 refractor; ASI585MC, ROI of about 2000 x 2000; UV/IR cut filter; No.25 red filter; SharpCap; best 500 frames out of 5000. Shutter speed 1 ms; Gain 300, AutoStakkert. Photoshop (for exposure and color adjustment.)

Plato é uma das mais famosas e observadas crateras de impacto da Lua. Está situada na margem norte do Mare Imbrium e foi formada a cerca de 3,84 bilhões de anos atrás. Sua região é uma das mais lindas e fotografadas da superfície lunar.

 

Plato é uma cratera de impacto que teve seu fundo coberto por lava produzida por erupções provenientes de falhas do subsolo interno da cratera causadas pelo impacto. A inundação de lava ocorrida há 3,5 bilhões de anos soterrou um provável pico central e criou um aspecto plano e liso, com uma aparência escura, tornando-a uma cratera rasa com apenas 1 Km de profundidade e sem picos no centro. Antes de ser inundada por lava, provavelmente Plato tinha 4 Km de profundidade, com as bordas das paredes parecendo degraus ou curvas de nível (como em Copernicus) e montanhas no centro.

 

27-08-2021 / 06:22 UTC

Sky-Watcher 150mm - f/8

ZWO ASI 120MC-S + Barlow 2x + UV/IR Cut

SharpCap + PIPP + AS!3 + Astrosurface

Porto Real-Brazil

Bortle 4/5 Sky

My first image after polar aligning with Sharpcap, a great piece of software IMHO. Got my guiding almost to the limits of local "seeing" conditions.

 

Imaging telescope or lens:Meade Starfinder 8

 

Imaging camera:Canon T1i Full Spectrum

 

Mount:Losmandy GM-8

 

Guiding telescope or lens:MEADE 50mm Finder Guidescope

 

Guiding camera:ZWO ASI120MM

 

Software:Open Guiding PHD2 Guiding, DeepSky Stacker (DSS) DSS 3.3.2, Auriga Imaging RegiStar, Adobe Photoshop CS4 Photoshop CS4 , Stark Labs Nebulosity Nebulosity 2.1.2

 

Filter:Orion SkyGlow Imaging Filter

 

Accessory:Baader MPCC coma corrector

 

Resolution: 5683x3778

 

Dates:June 30, 2016, June 1, 2019

 

Frames:

41x45"

Orion SkyGlow Imaging Filter: 54x180" ISO1600

 

Integration: 3.2 hours

 

Darks: ~50

 

Bias: ~50

 

Avg. Moon age: 26.34 days

 

Avg. Moon phase: 12.34%

 

Bortle Dark-Sky Scale: 4.00

 

Data source: Backyard

Jupiter and 3 of its moons. Two small dots are Io and Ganymede. The small dot over the planet is Europa in transit. Europa's diameter is 3,121.6 km and Earth's is 12,742 km so no you can imagine how small is Earth compared to Jupiter.

 

Imaged on June 26th 2020.

Tech details:

1000 frames of Sun, 23% gain, 28ms exposure

Equipment:

Scope: Skywatcher 150/750 F5 Newtonian

Mount: NEQ6

Imaging camera: ZWO ASI120MM

Software: SharpCap 3.2, AutoStakkert, Registax, Lightroom, Photoshop

Object Details: The attached composite shows Jupiter during a transit of it's Great Red Spot and the shadow of it's largest moon Ganymede (the largest satellite in the solar system, being larger than Mercury or Pluto & only slightly smaller than Mars). Ganymede itself can be seen on the right as it moves away from the planet while another Jovian moon (Io) can been seen on the left as it begins to transit.

 

Jupiter set below my horizon prior to Io's shadow transit, however a similar event showing both shadows in transit last year in a time-lapse can be shown at the link attached here: www.flickr.com/photos/homcavobservatory/48059027006/in/al...

 

Although the eye professionals in my family would probably admonish me for saying this ;) , if you cross your eyes to form a single merged image, given the slightly different a viewing angels due to the elapsed time, the image takes on a 3-D effect with Ganymede's shadow appearing to 'float' above Jupiter. Another example of this effect can be accomplished using a set of the image from 2016 attached here - www.flickr.com/photos/homcavobservatory/27109906411/in/al... .

 

I have had the pleasure of witnessing & imaging a few 'double shadow transits' on Jupiter, and although the transparency & seeing conditions were terrible at the time, I did have the opportunity once (in 2013) to image an extremely rare triple shadow transit - a (terribly noisy & low res.) shot of which can be found at the link here:

www.flickr.com/photos/homcavobservatory/10619712624/in/al...

 

Image Details: Taken by Jay Edwards on the of the evening of August 14, 2020 (UT date Aug. 15, 2020) at the HomCav Observatory using a (vintage 1970) 8-inch, f/7 Criterion newtonian reflector, 3X Televue barlow and an ASI290MC 'planetary camera / autoguider'. The scope was mounted on and tracked with a Losmandy G-11 running a Gemini 2 control system. The camera was controlled by SharpCap and used in 'full frame' mode.

 

Due to the thick, nearly solid cloud deck in my area that evening, I had to constantly adjust the imaging parameters to compensate for the varying thickness of the cloud deck during these briefs times of 'thinning' and attempted to match their appearance, w.r.t contrast, brightness, saturation, etc., via post processing.

 

Processed using a combination of AS3, Reistax & PSP, as presented here the images have been resized down so the entire composite is half HD resolution.

 

Given the challenging conditions at the time I was fairly pleased with the results, and hope others are getting a chance to witness these fascinating events.

Composite image made by combining two separate output from different exposure videos.

 

Taken on 21 June 2019 at 23.43 UTC, with Celestron NexStar 6se SCT and ZWO asi224mc Camera. Video captured in SharpCap, stacked in AutoStakkert, then processed in PSP8, Registax 6 and LR.

Now this really was one heck of a challenge! There was an International Space Station daytime lunar transit visible from our garden at 11:55:26. The Moon was only a 15% Waxing Crescent and on a bright sunny day with patches of cloud, even getting the Moon in shot was a challenge. I had my laptop in a box but still it was incredibly difficult to see the Moon on the screen so it was really hard to focus. The seeing was terrible and the gusts of wind were bouncing the telescope around.

I honestly didn't think I had a hope in hell of capturing this, so I was astonished when I was watching the screen and saw the ISS zoom past. Knowing how bad the seeing was, I didn't have high hopes of getting anything top quality, so I'm really pleased with this result.

 

William Optics 70mm refractor and ASI120MC camera with a 2x Barlow. 1,500 frames captured with Sharpcap. I debayered the video using PIPP then used Movie Maker to create the video. I also extracted all of the individual frames from the original video then processed the 30 frames that contained the ISS, then stacked them using StarStaX then made final tweaks in Fast Stone Image Viewer

ISS Solar Transit

July 4th, 08:39:10 MST, 0.6 seconds

Composite of best 150 of 1595 frames with 17 of ISS

 

Celestron 6se with solar filter and f/6.3 reducer

Celestron AVX

Zwo ASI1600MC-C

 

Sharpcap, Autostakkert!, PixInsight, Photoshop

21:50BST 96% illuminated, bright but hazy sky with poor transparency, not too bad, but details couldn't be sharpened much more.

 

Altair Astro Lightwave 72EDR f/6

AA IMX178C Hypercam

SkyWatcher AZ-GTI mount

 

Exp = 1.85ms

Gain= 250

 

Best 10% stacked with Autostakkert 3, of 3000 frames captured with SharpCap Pro 3.2

 

Post processed with Registax 6 and Photoshop CC2019 with Astra Image plugins for deconvolution, and sharpening.

 

www.backyardastro.org

Processed as 'LRGBHSO' in APP.

In the constellation of Auriga.

 

M: iOptron EQ45-Pro

T: William Optics GTF81

C: ZWO ASI533MM-Cooled

F: L,R,G,B,Ha,Oiii & Sii

G: PHD2 & Baader FlipMirror

GC: ZWO ASI120mini

RAW16; FITs

Temp: -10 DegC

Gain 101;

L 5 x Exp 200s

R 5 x Exp 200s

G 5 x Exp 200s

B 5 x Exp 200s

Ha 5 x Exp 400s

Oiii 5 x Exp 400s

Sii 5 x Exp 400s

Frames: 30 Lights; 0 Darks; 6 flats

100% Crop

Capture: SharpCap

Processed: APP; PS

Sky: 80% Gibbous moon, breezy, minimal cloud, cold, fair seeing.

 

3.477 light years distant.

 

Managed to capture a CME (Coronal Mass Ejection) on Friday July 28th 2023 starting from 15:42UT to 16:13UT.

 

Location:

Botkyrka, Stockholm, SE

 

This is by far the best solar I have ever captured in my entire time as an amateur solar photographer, a journey I started back in early 2022.

 

Equipment in use:

Lunt Solar Systems LS50THa/B600

Player One Astronomy Neptune-M (IMX178), 6 MP mono

iOptron GEM28 GoTo

 

Software in use:

SharpCap for capturing

Autostakkert! 3 for stacking

ImPPG for deconvolution

Photoshop CC for colorization and creating the video with

 

EXIF (Metadata):

1000 frames each, MONO16, 30 fps, SER format, 4 ms Exposure, 0 Gain, 0 Offset

40% stacked with Resample 2x

Moon mosaic taken with SkyWatcher Esprit 100ED, ZWO ASI224MC, Sharpcap, PIPP, Autostakkert and Microsoft ICE.

My first ever photo of Uranus, captured last night (2024-01-26)

 

This was captured using my newly purchased ZWO 715MC. This camera has amazingly small pixels that allows a telescope often used for deep sky to overcome its small focal length with densely packed small 1.45 micron pixels.

 

This is a perfect match for my 8" newtonian which has a native focal length of 1000mm. Typically you'd need an SCT or a big dobsonian with a camera with larger pixels. Up until now, basically all planetary cameras have had a pixel size of 2.9 microns.

 

This photo shows 4 of Uranus' moons. They're incredibly faint even on a relatively fast aperture setup for planetary. At magnitude 15, they're as faint as many deep sky targets requiring long exposures to reveal them. Long exposures and planetary are not something you hear very often.

 

The setup:

 

- ZWO ASI 715MC

- ZWO ADC

- ZWO EAF

- Skywatcher 200P (modified)

- Skywatcher EQ6R

- SharpCap

- AutoStakkert

- Registax

- Photoshop

 

10,000 frames captured at 112FPS, Moons 5s x 20 (max gain of 600)

The "Pinwheel Galaxy" M101 is about the same size as our Milky Way but 21 million light years distant. It's one of the faintest but most distinctive Messier galaxies.

This image has a different look from my prior attempt, see www.flickr.com/photos/124244349@N07/33239260336/in/photos... . The biggest differences likely stem from the switch from a CCD camera to a more responsive CMOS camera; a different light pollution filter; and another two years of improvements in my own technique.

Tech Stuff: Borg 71FL with 1.08X multi flattener; ZWO ASI1600MC; IDAS LPS-D2S filter, on Ioptron CubePro 8200 mount guided with SBIG ST-i guider. 140 minutes of 15 second exposures livestacked every 10 minutes by SharpCap 3.2; processed with PixInsight; finished with GIMP and ACDSee. Imaged over 4 nights in early June 2019 from my yard 10 miles north of New York City.

Jupiter on 26th October 2023. 8 images derotated. Each image was a stack of 50% of 30k frames. Captured using SharpCap Pro, stacked using Autostakkert, wavelet sharpening in Registax, derotated using WinJupos. Celestron C11 XLT, Altair 385c camera, 2x Barlow. Mounted on Skywatcher AZEQ6-GT.

The giant gas planet Saturn, located to the East of Jupiter, low in the late August sky.

 

Saturn last night. Celestron 8SE, Alt/Az mount, and TeleVue 3x Barlow. Using a ZWO ASI120MC camera ('Best' of 1K frames), SER movie file captured with SharpCap.

Images processed with PIPP then stacked with AS!2 / Registax-6 finally tweaked in PS.

Reprocessed data using new tricks in PixInsight!

 

The Leo Triplet (also known as the M66 Group) is a small group of galaxies about 35 million light-years away in the constellation Leo. This galaxy group consists of the spiral galaxies M65, M66, and NGC 3628.

 

Image Details:

- Imaging Scope: Astrotelescopes ED 80mm Refractor

- Imaging Camera: ZWO ASI183MC Color with UV/IR Blocking filter

- Guiding Scope: William Optics 66mm Petzval

- Guiding Camera: Orion Starshoot Auto Guider

- Acquisition Software: Sharpcap

- Guiding Software: PHD2

- Light Frames: 12*3 mins @ 50 Gain, Temp -16C

- Stacked in Deep Sky Stacker

- Processed in PixInsight and Adobe Lightroom

12"dobsonian, ZWO ASI 2600MC (first light!) Baader MPCC, Autostakkert 3, Sharpcap 3.2

 

2021-08-19-0939_3_AS_P35_lapl5_ap137_conv

 

Sadr region bicolor

 

Canon 200mm f/2.8 @ f/2.8

ASI 1600MM-C -20C gain 139

ZWO filters

 

2 minutes

 

14x Ha

14x Oxygen

 

Sharpcap

Sequence Generator Pro

Cartes Du Ciel

Pixinsight 1.8

6 images - de-rotated

Seeing 2.5/5

Transparency 3/5

 

Collimation slightly off.

 

C9.25 EDGEHD

ZWO120MC

SharpCap

Winjupos

AutoStakkert

PixInsight

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