View allAll Photos Tagged Optolong

Camera: Moravian G2 8300

Filters: 31mm unmounted Optolong

Optic: Triplet Apo Tecnosky 80mm f/4.8

Mount: Ioptron CEM60 HP

Autoguider: camera Magzero 5m, SW 70/500, Phd guiding

Frames Ha 7nm: 18X600 sec - RGB: 6X600 sec each Bin 1

Processing: Pixinsight, Photoshop

Az Orion-köd (más néven Messier 42) a Tejútrendszerben elhelyezkedő fényes diffúz köd, amely az Orion övétől délre található. Ez a Földhöz legközelebb lévő masszív csillagkeletkezési régió. A Messier 42 az egyik legjobban ismert ilyen típusú mélyég-objektum. Sokat elárult a csillagászoknak arról, hogyan képződnek a csillagok és a bolygók az itt látható csodálatos por- és gázfelhőkből. Az Orion-ködtől északra található úgynevezett "Futó ember-köd" egy futásban lévő ember alakjára emlékeztet. Az objektum a csillagok fényét kékes színben veri vissza.

Setup:

Canon 600D Baader szűrővel

TAMRON SP 150-600mm f/5-6.3 Di VC USD G2

OPTOLONG L-eNhance CCD-szűrő (EOS clip APS-C)

SkyWatcher Star Adventurer mechanika

Manfrotto MT055XPRO3 alumínium állvány

32 mm-es 1,25" keresőtávcső

Lacerta MGEN-II Stand Alone AutoGuider

Dátum / idő: 2023-01-14 18:27:18

Expoziciós idő: 51x90 sec

F-szám: f/5.6

Érzékenység ISO-ban: ISO 1600

Fókusztávolság: 300 mm

First 4 panels of a 20 panel mosaic I'm constructing

 

QHY163

11" Celestron EdgeHD with Hyperstar

 

Each panel:

Optolong HA- 3x120

Optolong OIII-5x120

Optolong SII-5x120

In my opinion it's one of the most colorful targets in our night sky, the star forming region of Rho Ophiuchi lies only about 360 light years from us in the Constellations of Ophiuchus and Scorpius.

 

This collection of images making up a 4 panel Mosaic was Captured over 3 nights from grandmesaobservatory.com in Colorado, using the QHY367C One Shot Color CMOS Camera on Walter Holloway's Takahashi FSQ130

 

Panel 1. rho Oph Nebula IC4604, and IC4605

www.flickr.com/photos/terryhancock/35707565605/in/photost...

 

Panel 2. Globular Clusters M4 and NGC6144

www.flickr.com/photos/terryhancock/35538862302/in/photost...

 

Panel 3. IC4605 and Dark Nebulae of Rho Ophiuchi

www.flickr.com/photos/terryhancock/35667959956/in/photost...

 

Panel 4. IC4605 and Antares www.flickr.com/photos/terryhancock/35320386870/in/photost...

 

Rho Ophiuchi 4 panel mosaic consisting of the above 4 panels

www.flickr.com/photos/terryhancock/35667959596/in/datepos...

 

Total Integration Time 8 Hours (2 hours per panel)

 

Technical Information

Location: Grand Mesa, Whitewater Colorado

Captured June 2017

QHY367C Full Frame One Shot Color COLDMOS cooled to -20C

Size: 7376 x 4938 pixels each panel, Mosaic is 11736x8093 pixels

Pixel Size: 4.88um x 4.88um

Total integration Time 480 minutes

Gain 2850, Offset 76

Darks and Flats no Bias

120 x 240 sec @ 1x1

Optics: Takahashi FSQ-130 @ F5.0 650mm

Optolong Luminance Filter for IR Block

Paramount ME German Equatorial Mount

Image Acquisition Maxim DL

Pre Processing Deep Sky Stacker

Post Processing Pixinsight & CS6

 

Please check out the new observatory at Grand Mesa Colorado

www.grandmesaobservatory.com

 

Nébuleuse NGC7822 dans la constellation de Céphée

 

30x300s, Gain 120 + DOF

ASI294 MC PRO + Optolong L-eNhance filter

TS Optics Photon N200/800

EQ6-R PRO

Guidage ASIAIR+ASI120MM mini

 

traitement Pixinsight + Photoshop CC2018

EQUIPMENT

GSO Newtonian 150/610 mm HPS Newtonian

ZWO Optical ASI533MC Pro (CMOS)

Equatorial Losmandy GM8

Optolong Light pollution L-Pro Filter 2.00" 90%

Coma corrector Explore Scientific 2.00"

 

Lights41 x 300 sec

Darks4 x 300 sec

Flats50 x 0.4 sec

Dark Flats50 x 0.4 sec

Total lights integration time 3:25 hours

IC1396, a large region of ionised gas containing the Elephant's Trunk Nebula (top right of centre - a concentration of interstellar gas and dust) and the Garnet Star (large red star top left), located in the constellation Cepheus about 2400 light years away from Earth. The Garnet Star is 1000 times larger and 100000 times brighter than the Sun!

 

ZWO ASI 2600MC Pro, gain 100, cooled to -10degC

William Optics GT81 with Flat 6AIII

Optolong L-eXtreme filter

ASIAir Pro

HEQ5 Pro mount guided

ZWO EAF

 

82 x 180s lights

40 darks

80 flats

80 dark flats

Stacked in DSS, processed in Photoshop and finished in Lightroom

 

Bortle 4 skies

 

Camera: Moravian G2 8300

Filters: 31mm unmounted Optolong

Optic: Triplet Apo Tecnosky 80mm f/4.8

Mount: Ioptron CEM60 HP

Frames RGB: 9X60sec each Bin 1

Processing: Pixinsight, Photoshop

Pubblicazioni: Nuovo Orione marzo 2019

 

I decided to re-image NGC7380, this time with the FLT132 and FLAT8 reducer. I had imaged this one before with the FLT91 (see flic.kr/p/2oWf1hi) and I wanted to see the difference in detail with the larger aperture. As nights are short and only darkish where I live, I imaged this target over three separate nights, getting around 3.5 hours each night.

 

NGC 7380 is located in the constellation Cepheus about 7,000 light-years from Earth within the Milky Way Galaxy. The star cluster is embedded in a nebula, which spans some 110 light-years. The stars of NGC 7380 have emerged from this star-forming region in the last 5 million years or so, making it a relatively young cluster.

 

Equipment:

- William Optics FLT132 with FLAT8 0.72x reducer/flattener

- ZWO ASI2600MC Pro camera with Optolong L'Ultimate 3nm Ha & Oiii dualband filter

- AM5 mount with ASIAir plus

- Processed with PixInsight and Affinity Photo 2

 

Integration:

10 hours and 39 minutes in 3m, 5m and 10m subs.

Darks, Flats and Bias frames.

 

More integration details: astrob.in/7p7u6l/0/

 

Thanks for looking.

Clear Skies,

Eduardo

Redcat51

AZ-EQ5

ZWO ASI533MC + Optolong L-eXtreme

20x480" lights

No calibration frames

Nebulosity4

Guiding with ZWO ASI120MC-S + William Optics UniGuide 32mm + PHD2

PixInsight

Photoshop CC

Driveway, Cairns, Australia

Comet C/ 2017 K 2 Pan STARRS passing by the Blue Horsehead Nebula in Scorpius.

August 21, 2022

 

just over 3 hours of integration (190 minutes , 5 minutes subs)

 

Equipment

 

HEQ 5/ Samyang 135 mm/ ZWO ASI 183 MC/Optolong UV/IR filter/ ASIAIR

 

Software and processing Notes

 

ASIAIR for capture. Astro Pixel Processor for stacking - twice, once for the nebula and once for the comet, layered in Photoshop

 

Starnet ++ v2

Topaz AI Denoise

Photoshop CS6

 

Location;

 

Linden, Blue Mountains, NSW Australia

Technical Card

Imaging telescope or lens: Sky-Watcher 200/1000 mm Newton

Imaging camera: Canon EOS Rebel T6

Mounts: Sky-Watcher EQ5, Onstep

Guiding telescope or lens: Guidescope 50mm

Guiding camera: Zwo ASI120MC

Software: Adobe Phosotshop CC, Astrophotography Tool, Sequator 1.5.2, PHD Guiding, PhotoScape

Filter: Optolong L-eNhance

Dates: April 24, 2020

Frames:

Optolong L-eNhance: 2x210" ISO800

Optolong L-eNhance: 15x300" ISO800

Integration: 1.4 hours

Darks: ~7

Flats: ~20

Resolution: 2601x1732

Locations: Home observatory, Montenegro, Rio Grande do Sul, Brazil

Data source: Backyard

 

Os frames foram captados na mesma noite em que registrei a Nebulosa da Lagoa, mas eu ainda não havia podido processá-los.

 

"A grande nebulosa de Carina (Eta Carinae) é catalogada como NGC 3372, que abrange cerca de três graus do céu a uma distância de 10 000 anos-luz, o que corresponde a um diâmetro de 300 anos-luz. Esta é a jóia do hemisfério sul, tornando-se uma das maiores regiões de formação estelar em nossa galáxia. É também a região HII (região de hidrogênio ionizado), o mais brilhante da Via Láctea". Fonte: astronoo.com

 

Refletor Sky-Watcher 203mm F/5 EQ5 com Onstep, Canon T6 (foco primário) modificada, Filtro Optolong L-Enhance. Guidescope 50mm com ASI 120MC-S. 17 light frames (15x300" + 02x210"), 07 dark frames, 20 flat frames. ISO 800. Processamento: Sequator, Photoshop e PhotoScape.

 

@LopesCosmos

www.instagram.com/lopescosmos/

www.astrobin.com/users/lopescosmos/

Technical Information:

 

Telescope: AIRY APO 130T

Mount: NEQ6-Pro

Camera : QHY9

Filter: Optolong H-a 7nm, OIII 6.5nm, SII 6.5nm

Frames: H-a: 32x900s -- OIII: 32x900s -- SII:32x900s

Total Integration: 24 Hours

Software: SGP – PHD2 – DSS -PixInsight – CS6

Location: Noventa di Piave (Venice) 4 meter above sea level – ITALY

 

Environment Temperature: About 15°C

 

Relative Humidity: 85%

 

Date: 11.09.19 - 12.09.19 - 13.09.19 - 14.09.19

  

NOTE: The image was acquired from a very polluted sky ( Red Zone - where I live ).

This is an especially faint nebula.

Even after 4+ hours of exposure, my stacked image was very noisy.

 

---Photo details----

Stacks Ha: 133x2min

 

Darks : 100

 

Exposure Time : ~4h26m

Stack program : PixInsight

 

---Photo scope---

Camera : ZWO ASI6200MM PRO

CCD Temperature : -10C

Filter(s) used: Optolong Ha3nm,

Tube : Takahashi FSQ-106 EDX4

Field flattener / Reducer : -

Effective focal length : 530 mm

Effective aperture : F/5

 

---Guide scope---

Camera : ASI Mini guider

Guide exposure : 3 sec

 

---Mount and other stuff---

Mount : Skywatcher AZ-EQ-6 GT

 

---Processing details----

NINA for acquisition, controlling the following:

- ASTAP (plate solving)

- PHD2 (guiding)

- Stellarium

 

PixInsight : stacking, alignment, background extraction, histogram manipulation

 

Lightroom for final touchups

 

StarNet2 for allowing different processing on nebula vs stars

 

Topaz Denoise for a processing step

This is the California Nebula (aka NGC 1499) in Perseus, a classic red emission nebula emitting mostly at the red wavelength of hydrogen-alpha light but also with a strong hydrogen-beta emission line in the blue-green part of the spectrum.

 

By contrast, below is the small blue reflection nebula known only as IC 348, a cloud of dust surrounding hot blue stars and reflecting their light. But the region also contains some dim red emission nebulosity.

 

Also throughout the field are patches of yellow-brown dust that form obscuring dark nebulas. The main dark nebulas are Barnard 5 (above IC 348) and Barnard 4 below.

 

This is a stack of 8 x 8 minute unfiltered exposures at ISO 800 blended with a stack of 9 x 15-minute exposures through an Optolong L-Enhance narrowband filter, to bring out the emission nebulas. All were with the Canon EOS Ra camera through the William Optics RedCat 51mm astrograph at f/4.9, equipped with the Starizona filter drawer. Autoguiding was with the Lacerta MGEN3 stand-alone autoguider on the Astro-Physics Mach 1 mount. All stacking, alignment and blending was with Photoshop. Luminosity masks applied with Lumenzia to do selective curves adjustments to various tonal ranges.

 

Shot from home November 15, 2020.

Before the clouds came in last night with the snow, I got another few hours of clear, crisp skies and a chance to image another deep sky object. This is the Christmas Tree Cluster and the Cone Nebula (NGC2264) located in the constellation of Monocerous. The red Christmas tree shape is clear, adorned with its blue tinged open star cluster masquerading as the baubles. The Cone Nebula sits at the top of the 'tree' but is inverted in this shot. Deep within the clouds of gas and dust are the ingredients for producing new stars, which burn a fiercely hot bright blue. The red hue in the image is a result of gas clouds glowing as they are hit by ultra-violet light emanating from the newborn stars. The region is about 30 lightyears across and sits 2600 lightyears from Earth, not far in the sky from the Orion constellation.

 

William Optics GT81

William Optics Flat 6AIII

ZWO ASI2600MC Pro

ZWO ASI Air Pro

Skywatcher HEQ 5 Pro

Optolong L-eNhance filter

 

48 x 300s lights, 40 darks, 50 flats and 50 dark flats at gain 100 and -10C.

 

Stacked in DSS, processed with PS and LR.

75 exposures (5-minutes each) on Caldwell 9, the Cave Nebula.

 

This was a fun project I shot in June/July, collecting as much data as possible over the course of 3 nights.

 

This image was created using a color camera and a dual bandpass filter (Optolong L-eNhance: bit.ly/2ZcEyKG)

 

I'm pretty obsessed with shooting in color with multi-bandpass filters these days, it's a great way to maximize your time under the stars!

 

My ASI294MC Pro camera was connected to a Sky-Watcher Esprit 100 telescope, riding on an EQ6-R Pro mount.

 

More Info: astrobackyard.com/cave-nebula/

 

Clear skies!

 

Camera:ASI294MC Pro

Scope: Askar FMA180Pro

Mount: SW EQ6r Pro

Filter RGB: Optolong L-Pro

Expo RGB: 40 x 180s (2h) + Dark, Flat, Bias

Controlled by AsiAir Mini

Processed in PixInsight and Photoshop LR

2023.07.09, Varpalota, Hungary

Took this picture Saturday night, NGC 7635 & M52

Orion 80mm ED refractor, Zwo 294MC Pro cooled color camera

Optolong L eNhanced filter

#SharpCap Pro

Ioptron i45 Pro EQ mount PHD2 guiding

Orion 60mm guidescope SSAG

220 Gain offset 10 0c cooling, 1 minute exposure, was 2 hours and 30 minutes

50 darks 50 flats and 50 bias frames

Astro Pixel Processor and PS

  

May 2021 data reprocessed 6/05/2023

 

NGC 3247- aka the Whirling Dervish

 

can you see the whirling dervish- the flowing skirt, the arms upstretched, the turban?

 

or is just an extreme case of pareidolia?

 

ED 80/W. O 0.8 FR/ EQ6

16 hours of total exposure- 10 minute subs

NINA/PHD2

8 hours with QHY 183 MM and Baader 7nm H alpha Filter

 

8 hours with ZWO ASI 183 MC and Optolong L Extreme filter

 

Bortle 6 Location- lots of moon about

  

PS I actually named this object in May 2009, way back when I first imaged it and found no amateur photos on the internet. And I still think the name is apt!

 

Processing notes

 

stacked and registered in Astro Pixel Processor

 

Ha and RGB data processed separately and combined using the Astrobackyard haRGB technique

Referred to as Bode's Nebula, it is however, a spiral galaxy located close to the Big Dipper or Plough asterism in Ursa Major. It has a close companion galaxy M82 the Cigar galaxy, so close together, they are often imaged as a pair.

 

Lying about 12 million light years from Earth and about 90,000 light years across. Binoculars will pick up M81 as a faint fuzzy patch of light under reasonable sky conditions.

First discovered by a German astronomer by the name of Johann Elert Bode in 1774, hence Bode's Nebula. At the time no one had any clue it was a whole other galaxy.

 

Boring techie bit:

Skywatcher Quattro 8" Newtonian Reflector steel tube with the f4 aplanatic coma corrector, Skywatcher EQ6 R pro mount, Altair Starwave 50mm guide scope, ZWO asi120mm guide camera mini, ZWO asi533mc pro cooled to -20c gain 110, Optolong L'enhance 2" filter, ZWO asiair plus.

Darks, Flats & Bias.

Stacked with DeepSkyStacker and processed in StarTools.

  

These filaments are remnants of a supernova that include SH2-96, SH2-94 and SH2-91. The field of view of the FLT132 (even with the 0.72x FLAT8 reducer) doesn't cover the full region, but it offers a closer look at SH2-96, which is rich in Ha (red) and Oiii (blue).

 

I used my William Optics FLT132, ASI2600MC Pro camera, Optolong L-Ultimate 3nm narrowband filter, on a ZWO AM5 mount. In these short summer nights, I needed two nights and up to 10 minute subs to get some decent signal for a total of just over 7 hours integration time.

 

More acquisition details as well as other versions (e.g. starless) in astrobin: astrob.in/myebzs/0/

 

Thanks for looking and Clear Skies!

 

Technical card

Imaging telescope or lens: Sky-Watcher 200/1000 mm Newton

Imaging camera: Canon EOS Rebel T6

Mounts: Onstep, Sky-Watcher EQ5

Guiding telescope or lens: Guidescope 50mm

Guiding camera: ZWO ASI120MC

Software: Pixinsight 1.8, Astrophotography Tool, Sequator 1.5.2, PHD Guiding

Filter: Optolong L-eNhance

Dates: May 27, 2020, May 28, 2020

Frames:

62x300" ISO800

Optolong L-eNhance: 42x300" ISO1600

Integration: 8.7 hours

Darks: ~80

Resolution: 2918x2067

Locations: Home observatory, Montenegro, Rio Grande do Sul, Brazil

Data source: Backyard

 

Meu primeiro registro da galáxia Centaurus A. No processamento dessa galáxia, utilizei muito o software PixInsight. Estou em fase inicial no aprendizado para o uso desse software, havendo ainda muito a aprender e a melhorar, inclusive para maior aproveitamento dos tempos totais de exposição realizados em cada alvo. No caso desse registro, os frames empilhados, captados em dois dias consecutivos, somam 8 horas e 40 minutos totais de exposição.

 

"Centaurus A é uma galáxia peculiar localizada na constelação Centaurus. É a quinta galáxia mais brilhante do céu noturno, a galáxia gigante mais próxima da Via Láctea e uma das rádio-galáxias mais próximas da Terra. Seu tipo exato é incerto, mas geralmente é classificada como uma galáxia elíptica gigante ou lenticular. A distância exata da galáxia à Terra também é incerta, mas as estimativas geralmente variam de 10 a 16 milhões de anos-luz". Fonte: constellation-guide.com

 

Refletor Sky-Watcher 203mm F/5 EQ5 com Onstep, Canon T6 (foco primário) modificada, Filtro Optolong L-eNhance (em parte dos frames). Guidescope 50mm com ASI 120MC-S. 104 light frames (62x300" ISO 800 + L-eNhance: 42x300" ISO 1600), 80 dark frames. Processamento: Sequator e PixInsight.

 

@LopesCosmos

www.instagram.com/lopescosmos/

www.astrobin.com/users/lopescosmos/

Equipment used :

 

Canon 6D mod & WO SpaceCat 51

 

RGB 25 x 600" ISO 3200 - Optolong L-Pro

H-Alpha & OIII 20 x 1500" ISO 3200 - Optolong L-eXtreme

 

Sky Watcher EQ6 Mount

Guide camera QHY5

Flats, Darks & Bias

 

I took this from my small pier last weekend. 2 panel mosaic of the center of the Milky Way

 

QHY23M & 50MM Canon Lens @ F/2.4 w/Optolong HA filter

 

10x300sec per panel

 

For fun I combined the HA data with an older Milky Way shot for color

Color data: flic.kr/p/WUeXq1

Equipment:

William Optics Redcat511 🔭

ZWO ASI2600MC Pro

ZWO ASI290MM Pro guide 📷

Skywatcher EQM-35 Pro mount

Optolong L-Extreme Filter

 

The Heart Nebula

The Heart Nebula (IC 1805), lies some 7500 light years away from Earth and is located in the Perseus Arm of the Galaxy in the constellation Cassiopeia. It was discovered by William Herschel on 3 November 1787. It is an emission nebula showing glowing ionized hydrogen gas and darker dust lanes.

The brightest part of the nebula (a knot at its western edge) is separately classified as NGC 896, because it was the first part of the nebula to be discovered. The nebula's intense red output and its morphology are driven by the radiation emanating from a small group of stars near the nebula's center. This open cluster of stars, known as Collinder 26 or Melotte 15, contains a few bright stars nearly 50 times the mass of our Sun, and many more dim stars that are only a fraction of our Sun's mass.

 

William Optics GT81

William Optics Flat 6AIII

ZWO ASI2600MC Pro

ZWO ASI Air Pro

Skywatcher HEQ 5 Pro

Optolong L-eXtreme filter

ZWO EAF

 

70 lights of 180sec at gain 100 and -10degC, 40 darks, 40 flats and 40 dark flats

Bortle 4 skies

 

Stacked and processing in PixInsight with final processing in Lightroom and Photoshop

 

This is a complex of faint nebulas and star clusters in Cepheus:

 

While this exposure shows the field as one large nebula, the arc-shaped region at top is catalogued as NGC 7822. The region below with dark lanes through it is Cederblad 214. The loose open cluster at right is NGC 7762, with the small yellowish cluster (dimmed by interstellar dust) is King 11. A small, sparse cluster at the centre of Ced214 is Berkeley 59.

 

The field of view is about 8° by 5.5° with the 250mm focal length RedCat astrograph.

 

This is a stack of 8 x 8-minute exposures through the William Optics RedCat 51mm f/4.9 astrographic refractor with the red-sensitive Canon EOS Ra camera at ISO 800, and blended with a stack of 8 x 15-minute exposures through the Optolong L-Enhance narrowband filter, with the EOS Ra at ISO 3200, to make up for the nearly 3 stops loss of light from the filter. But it really pops out all the faint nebulosity.

 

All images stacked, aligned and blended with Photoshop.

 

Guiding was with the Lacerta MGEN 3 stand-alone autoguider, which also controlled the camera shutter and applied dithering of 10 pixels between each frame to reduce thermal noise without having to apply LENR in camera or dark frames. This was on the Astro-Physics Mach1 mount.

* Setup:

Telescope: Refractor Orion ED80

Focal Length: 600mm

Camera: QHY163M

Mount: HEQ5 Pro

Filters: LRGB Optolong and H-Alpha 7nm Baader

Location: Silvânia / GO / Brazil

 

*Exposure:

Ha: 1.8 hour (subs 300s) bin1x1

R: 0.5 hour (subs 180s) bin1x1

G: 0.5 hour (subs 180s) bin1x1

B: 0.5 hour (subs 180s) bin1x1

Core: 10s subs

Total: 3.3 hours

Reprocess of www.flickr.com/photos/stormlv/52257579490/in/dateposted/

 

I'm trying a new flow in which the noise reduction happens on the nebula only instead of the stars.

 

This leaves them untouched, as well as not introducing any artefacts like when applying denoising globally

 

---Photo details----

Stacks RGB: 18x2min

Darks : 100

Flats: 100

Exposure Time : 36min

Stack program : PixInsight

 

---Photo scope---

Camera : ZWO ASI2600MC PRO

CCD Temperature : -10C

Filter(s) used: Optolong L-Pro

Tube : Takahashi FSQ-106 EDX4

Field flattener / Reducer : -

Effective focal length : 530 mm

Effective aperture : F/5

 

---Guide scope---

Camera : ASI Mini guider

Guide exposure : 2 sec

 

---Mount and other stuff---

Mount : Skywatcher AZ-EQ-6 GT

 

---Processing details----

NINA for acquisition, controlling the following:

- ASTAP (plate solving)

- PHD2 (guiding)

- Stellarium

 

PixInsight : stacking, alignment, background extraction, histogram manipulation

 

Lightroom for final touchups

 

Topaz Denoise for a last processing step

Here is the Seagull Nebula captured using a ZWO ASI533MC Pro camera and Starizona APEX ED 0.65x Reducer.

 

This image was featured in my latest video, that highlights the benefits of using a focal reducer for astrophotography: youtu.be/46WoTDhuAZc

 

The final image includes 14 x 4-minute exposures using a broadband light pollution filter (Optolong L-Pro).

 

Thanks for looking!

cave-242x30-g42-o42_-20C-13x240-g20-o42_-15C--qhy183c-lenh-85f5_6-v3b

 

Nearly 3 hours of sub-images are in this updated version of the Cave. Metro LP conditions, but an Optolong L-eNhance filter was used to cut through it. The first session had 52 minutes in 4 minute subs and the most recent data was 2hrs and 2 minutes in 30 second subs, QHY183c camera, Televue TV-85 at F/5.6.

 

NGC 672 es una galaxia espiral en la constelación de Triangulum , ubicada alrededor de 2 ° al suroeste de la estrella Alpha Trianguli . El objeto ahora identificado como NGC 672 fue descubierto por John Herschel el 11 de noviembre de 1827.

 

Esta galaxia está ubicada a una distancia de aproximadamente 23,4 mega-luz-años de la Vía Láctea , donde forma un par que interactúa con la galaxia irregular IC 1727.

 

110 x90' = (2h45') - Gain 1800, Offset 10, -10ºC

 

Equipo:

Telescopio/Telescope: TS RC 6" reductor 0,67 - Focal 919mm

Montura/Mount: Ioptron ieq45 PRO

Seguimiento/Guiding: tubo SV106+QHY5IILM

Camara/Camera: QHY294C

Control: Astroberry

Procesado: Pixinsight+PS

FIltro:Optolong L-pro

 

23/10/2020- Markinez ,Álava

   

Elaborazione difficile!

Non immaginavo che con oltre 13h di integrazione elaborare il complesso della nebulosa Velo (trattasi del resto di una supernova esplosa alcuni millenni fa) nella costellazione del Cigno fosse cosi ostico e complicato.

Forse alcuni fattori hanno complicato le cose: acquisizione con la presenza della luna quasi piena, trasparenza del cielo spesso non buona, inquinamento Bortle 6-7.

Probabilmente anche la debole luminosità della nebulosa insieme all'uso di un filtro a Banda-Stretta e ai fattori anzidetti hanno reso insufficienti i 300s di posa.

Ad ogni modo ho cercato di fare del mio meglio, anche se sono ancora principiante con i recenti programmi di elaborazione estetica GraXpert e SIRIL. Molto difficile è stato riuscire ad evidenziare le tenui nebulosità Halfa esterne alle nebulose NGC6960 e NGC6992.

Questa elaborazione ha evedenziato 2-3 criticità ottiche del teleobiettivo Zenit Giove 11-A soprattutto quando si utilizzano più filtri ottici contemporaneamente. Spero di trovare un buon compromesso quando utilizzerò questo obiettivo in futuro.

_____________

Difficult processing!

I didn't think that with over 13 hours of integration, processing the complex of the Veil nebula (the remnant of a supernova that exploded a few millennia ago) in the constellation of Cygnus would be so difficult and complicated.

Perhaps some factors complicated things: acquisition with the presence of an almost full moon, often poor transparency of the sky, Bortle 6-7 pollution.

Probably also the weak brightness of the nebula together with the use of a narrow-band filter and the aforementioned factors made the 300s exposure insufficient.

However, I tried to do my best, even though I am still a beginner with the recent aesthetic processing programs GraXpert and SIRIL. It was very difficult to highlight the faint Halfa nebulosities outside the NGC6960 and NGC6992 nebulae.

This processing also highlighted 2-3 optical critical issues of the Zenit Giove 11-A telephoto lens, especially when using multiple optical filters at the same time. I hope to find a good compromise when I use this lens in the future.

 

_____________

Lens : ZENIT Jupiter-11A 135mm f/4 flic.kr/p/MekcC7

Camera: ZWO ASI533MC-Pro

Filter: Optolong L-eNhance + SVbony UV-IR cut

Mount: Sky Watcher HEQ5 Synscan

Seeing: 3-4 (scala Antoniadi inversa)

104X300s / 121 gain / 18 dark/ 22 flat/ 22 darkflat/ 100bias

57x300s / 300gain / 12 dark / 22 flat / 22 darkflat/ 40bias

Date: 17-19-24-29-30-31/07/2024

Integration: 13h 25min

Temperature sensor: -5°C

Location: Biancavilla (CT) -Sicily- Italy 520m slm

acquisition: NINA

Processing: DSS +GraXpert+SIRIL+ PSCC.

astrometric resolution: nova.astrometry.net/annotated_full/11199844

 

Technical Information:

 

Telescope: AIRY APO 130T

Mount: NEQ6-Pro

Camera : QHY168C -- GAIN:10 ; OFFSET:50 -- -20°C

Filter: Optolong 2" L-eNhance

Frames: RGGB: 66 x 600s

Total Integration: 11 Hours

Software: SGP – PHD2 – PixInsight – CS6

Location: Noventa di Piave (Venice) 4 meter above sea level – ITALY

Environment Temperature: About 15°C

Relative Humidity: 88%

Date: 14.09.19 - 15.09.19 - 20.09.19 - 21.09.19

 

NOTE: The image was acquired from a very polluted sky (Red Zone - where I live).

The North America & the Pelican Nebulaes.

 

The North America Nebula (NGC 7000) is an emission nebula found in the Cygnus constellation, glowing due to the ionisation of interstellar gas caused by radiation being emitted by hot, young stars.

To the right of the North America Nebula, is a less luminous nebula nicknamed the Pelican Nebula (IC 5070). The two emission nebulaes measure about 50 light-years across, are located about 1500 light-years away from us.

The North America Nebula was discovered by William Herschel in October 1786. It was first photographed by Max Wolf in December 1890.

 

At first I was supposed to shoot only the North America Nebula. On the second day, the sky was clear, so I decided to shoot the Pelican too with the goal to make a mosaic.

As the nights are short, I just have +/- 3 hours of total exposure for each panel.

 

Now, the only thing to do is waiting for clear skies !

 

This picture was shoot during a waxing gibbous moon.

 

Setup :

Camera : ZWO ASI 533 MC

Main Scope : William Optics Redcat 51

Guide Camera : ZWO ASI 120MM Mini

Guide Scope : ZWO Mini Guide Scope

Mount : Skywatcher AZ GTI

Filter : Optolong L-Extreme

Others : ZWO ASIAIR PRO

 

Panel 1(left)

 

Lights : 41 x 300 sec

Darks : 60 ~ Offset: 100 ~ Flats: 100

 

Panel 2(Right)

 

Lights : 39 x 300 sec

Darks : 60 ~ Offset: 100 ~ Flats: 100

 

Efix: ASI1600MM-pro + SW Esprit 100 + NEQ6pro rowan mod + optolong LRGB filters. Guide: guidescope 60mm and QHY5L II M – 68 x 3 min L, 20 x 3 min R, 20 x 3 min G, 19 x 3 min B. 100 flats per filter, 100 darks, gain 100. Edit: PIX and PS.

The Sadr region, or IC 1318, is the diffuse emission nebula surrounding Sadr (γ Cygni) at the center of Cygnus's cross. The Sadr region is one of the surrounding nebulous regions; others include the Butterfly Nebula and the Crescent Nebula. It contains many dark nebulae in addition to the emission diffuse nebulae.

 

Camera: Moravian G2 8300

Filters: 31mm unmounted Optolong

Optic: Samyang telephoto lens 135mm

Mount: Vixen Sphinx

Autoguider: camera Magzero 5m, finder 8X50, Phd guiding

Frames: Ha 7nm 6X600 sec - RGB: 3X600 sec each Bin1 -20°

Processing: Pixinsight, PS

 

Pubblicazioni: Coelum ottobre '19

Captured in the early hours of June 15 using the QHY367C One Shot Color CMOS Camera with the Optolong L-Pro under a waning moon-lit sky (71%) from the Grand Mesa Observatory Colorado, on Walter Holloway's Takahashi FSQ130

 

Total Integration Time 2 hours and 6 mins

 

For comparison here is an earlier image from 2014 captured using a QHY11 Mono CCD

www.flickr.com/photos/terryhancock/13519138553/in/photost...

 

Technical Information

Location: Grand Mesa, Whitewater Colorado

Captured June 15 2017

QHY367C Full Frame One Shot Color COLDMOS cooled to -20C

Size: 7376 x 4938 pixels

Pixel Size: 4.88um x 4.88um

Total integration Time 126 minutes

Gain 2850, Offset 76

Darks and Flats no Bias

63 x 120 sec @ 1x1

Optics: Takahashi FSQ-130 @ F5.0 650mm

Optolong Luminance Filter for IR Block

Paramount ME German Equatorial Mount

Image Acquisition Maxim DL

Pre Processing Deep Sky Stacker

Post Processing Pixinsight & CS6

 

Please check out the new observatory at Grand Mesa Colorado www.grandmesaobservatory.com

IC405 94X600SS SOIT 15H40 filtre l'extreme optolong camera 2600 zwo azeq6 lunette fsq85 takahashi, système aziair sous pleine lune à 100%

The Carina Nebula (catalogued as NGC 3372) is a large, complex area of bright and dark nebulosity in the constellation Carina, located in the Carina–Sagittarius Arm of the Milky Way galaxy. The nebula is approximately 8,500 light-years from Earth. The nebula has within its boundaries the large Carina OB1 association and several related open clusters. The nebula is one of the largest diffuse nebulae in our skies. Although it is four times as large as and even brighter than the famous Orion Nebula, the Carina Nebula is much less well known due to its location in the southern sky. It was discovered by Nicolas-Louis de Lacaille in 1752 from the Cape of Good Hope.

 

Camera: CCD Moravian G2 8300

Optic: 135mm Samyang lens f/2 @f/3.5

Frames: Ha 7nm 11X600sec - RGB 4X600sec each - Bin1 -25°

Filters: 31mm unmounted Optolong

Autoguider: ZWO ASI290MM mini on ZWO 30 F/4, Phd guiding

Mount: Celestron CGE PRO

Processing: Pixinsight, PS

APT automation

SQM 21.88

Rho Ophiuchi "Fireworks from our Milky Way"

 

The star forming region of Rho Ophiuchi lies only about 360 light years from us in the Constellations of Ophiuchus and Scorpius.

 

This collection of images making up a 4 panel Mosaic was Captured over 3 nights from grandmesaobservatory.com in Colorado, using the QHY367C One Shot Color CMOS Camera on Walter Holloway's Takahashi FSQ130

 

Panel 1. rho Oph Nebula IC4604, and IC4605

www.flickr.com/photos/terryhancock/35707565605/in/photost...

 

Panel 2. Globular Clusters M4 and NGC6144

www.flickr.com/photos/terryhancock/35538862302/in/photost...

 

Panel 3. IC4605 and Dark Nebulae of Rho Ophiuchi

www.flickr.com/photos/terryhancock/35667959956/in/photost...

 

Panel 4. IC4605 and Antares www.flickr.com/photos/terryhancock/35320386870/in/photost...

 

Rho Ophiuchi 4 panel mosaic consisting of the above 4 panels

 

Total Integration Time 8 Hours (2 hours per panel)

 

Technical Information

Location: Grand Mesa, Whitewater Colorado

Captured June 2017

QHY367C Full Frame One Shot Color COLDMOS cooled to -20C

Size: 7376 x 4938 pixels each panel, Mosaic is 11736x8093 pixels

Pixel Size: 4.88um x 4.88um

Total integration Time 480 minutes

Gain 2850, Offset 76

Darks and Flats no Bias

120 x 240 sec @ 1x1

Optics: Takahashi FSQ-130 @ F5.0 650mm

Optolong Luminance Filter for IR Block

Paramount ME German Equatorial Mount

Image Acquisition Maxim DL

Pre Processing Deep Sky Stacker

Post Processing Pixinsight & CS6

 

Please check out the new observatory at Grand Mesa Colorado

www.grandmesaobservatory.com

 

La Galassia di Bode, (nota anche come M 81 o NGC 3031) è una galassia a spirale situata a circa 12 milioni di anni luce dalla Terra, nella costellazione boreale dell'Orsa Maggiore;

 

La Galassia Sigaro (nota anche come M 82 o NGC 3034) è una galassia attiva nella costellazione dell'Orsa Maggiore; si trova a circa 12 milioni di anni luce ed è associata alla più grande e famosa M81. Si tratta di un ottimo esempio di galassia starburst.

  

Fusione finale di scatti ripresi con 3 strumenti e camere diverse per un totale di 34ore.

 

FSQ106EDXIII e QSI683

Filter Astrodon

L: 39 x 900s

RGB: (19, 14, 18) x 300s

 

ORION ASTROGRAPH e 294C pro

Filter Optolong

L-PRO: 120 x 240s

 

TS RC 12" TRUSS e MORAVIAN G2-8300 MARK II

Filter Astronomik

L: 49 x 300s

Ha: 21 x 600s

RGB: 21 x 240s bin 2

 

The Bode Galaxy, (also known as M 81 or NGC 3031) is a spiral galaxy located about 12 million light years from Earth, in the northern constellation of Ursa Major;

The Cigar Galaxy (also known as M 82 or NGC 3034) is an active galaxy in the constellation Ursa Major; it is located about 12 million light years away and is associated with the larger and more famous M81. This is a great example of a starburst galaxy.

 

Final fusion of shots taken with 3 different instruments and cameras for a total of 34 hours.

 

FSQ106EDXIII and QSI683 Filter Astrodon

L: 39 x 900s

RGB: (19, 14, 18) x 300s

 

ORION ASTROGRAPH and 294C pro Filter Optolong

L-PRO: 120 x 240s

 

TS RC 12" TRUSS and MORAVIAN G2-8300 MARK II Filter Astronomy

 

L: 49 x 300s Has: 21 x 600s

RGB: 21 x 240s bin 2

This diffuse emission nebula also designated SH2-86 in the Sharpless catalogue is the home of the young open star cluster NGC 6823, visible in the centre of the image.

The nebula is estimated to be just under 6,000 light years from us and can be found in the constellation Vulpecula.

Data gathered at www.astronomycentre.org.uk

 

Boring techie bit:

Skywatcher Quattro 8" Newtonian Reflector steel tube with the f4 aplanatic coma corrector, Skywatcher EQ6 R pro mount, Altair Starwave 50mm guide scope, ZWO asi120mm guide camera mini, ZWO asi533mc pro cooled to -20c gain 101, Optolong L'enhance 2" filter, ZWO filter drawer, ZWO asiair plus.

120s exposures.

Best 80% of 57 light frames.

Darks, Flats & Bias.

Stacked with DeepSkyStacker and processed in PixInsight & Affinity Photo.

ccd: Moravian G3-11000 with IFW + OAG

filters: Optolong LRGB and Astrodon 5-nm Ha

telescope: DSI RC10C f/7.3

mount: 10Micron GM2000 QCI

guider: Lodestar

exposure: L 20x20min + RGB 6x12min (all 1x1)

location: Les Granges, 900 m

software: TheSkyX Pro, CCD Commander, Pixinsight, PS CS5

date: 29 Mar - 21 Apr 2017

Telescope: WO ZenithStar 81 Refractor

Mount: Losmandy GM811G

Imaging Camera: ZWO ASI 2600MC Pro

Filter: Optolong L-Extreme Filter

Site: Elk Grove, California, USA

Calibration Files: None

Guiding: ZWO ASI 174mm mini/Orion 60mm Guidescope/PHD2

Integration Time: 5h 33m

No of Frames: 111

Sub Exposure Time: 180 sec

Bortle Zone: Class 6

Date Taken: Aug 22 & 24, 2021

camera: ZWO ASI6200MM Pro with EFW 7x2"

filters: Optolong LRGB and Chroma 3-nm Ha/O3

telescope: TEC 140 f/7

mount: 10Micron GM2000 QCI

guider: ZWO ASI120 mini on 50-mm f/4 guidescope

exposure: L 31x10min (1x1) + RGB 20x5min (all 2x2)

location: Les Granges, 900 m (Hautes Alpes, France)

software: TheSkyX Pro, CCD Commander, Pixinsight, PS CC

date: 2 Jan - 6 Mar 2022

A compact group of galaxies about 35 million light-years away in the constellation Leo. NGC 3189, 3187, 3185 and SAO 81279.

 

Telescope: WO ZenithStar 81 Refractor

Mount: Losmandy GM811G

Imaging Camera: ZWO ASI 2600MC Pro

Filter: Optolong L-Pro Filter

Site: Elk Grove, California, USA

Calibration Files: None

Guiding: ZWO ASI 174mm mini/Orion 60mm Guidescope/PHD2

Integration Time: 3h 24m

No of Frames: 68

Sub Exposure Time: 180 seconds

Bortle Zone: Class 6

Date Taken: April 4, 2021

Technical Information:

 

Telescope: AIRY APO 130T PrimaLuceLab

Mount: Paramount MyT - Software Bisque

Camera: QHY168C -- Gain:10 ; Offset:50 -- -20°C with Dark and Flat Frames

Filter: Optolong 2" L-Pro, Optolong 2" L-eNhance

Frames: RGGB:

L-Pro: 150 x 240s -- L-eNhance: 21 x 600s

Total Integration: 12,5 Hours

Software: SGP – TheSkyX – PHD2 – PixInsight – CS6

Location: Noventa di Piave (Venice) 4 meter above sea level – ITALY

Environment Temperature: About 6°C

Relative Humidity: 88%

Date: 19.02.20 - 20.02.20 - 04.03.20

 

NOTE: The image was acquired from a very polluted sky (Red Zone)

Unfortunately, the seeing was not very good but I am quite happy of this result.

The image has been cropped because the field was larger and this helped ti hiligh more the galaxy.

Flaming Star - IC 405/IC 410 in the constellation Auriga.

 

Cam: Canon EOS 6Da

Scope: Lacerta ED72/432

Astromount: HEQ5 Pro

Autoguider: Lacerta M-GEN plus Finderscope 9x50

17x 1200sec plus 14x 1500sec | ISO400

Exceptionally from my lightpolluted garden with Optolong L-Pro 2" filter

 

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© Claus Steindl

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