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I totally forgot to upload this image to Flickr, but also this is a re-processed image after learning some new techniques in post processing, but this is NGC1893 / IC410 or most commonly referred to as The Tadpoles, at a distance of over 12,000 light years from earth in the constellation of Auriga

 

Image Details:

Red 51x150S in SII 6nm Filter

Green: 51x150S in Ha 6nm Filter

Blue: 51x150S in OIII 6nm Filter

Darks, Flats and Flat Darks were applied in the image stacking process

 

Total Capture time: 12.8 Hours

 

Acquisition Dates: Nov. 19, 2019 , Dec. 30, 2019 , Jan. 3, 2020 , Jan. 17, 2020 , Jan. 18, 2020 , Jan. 19, 2020 , Jan. 21, 2020 , Jan. 28, 2020 , Feb. 1, 2020

 

Equipment Details:

Imaging Camera: Qhyccd 183M Mono ColdMOS Camera at -20C

Imaging Scope: SharpStar 15028HNT Hyperboloid Astrograph

Guide Camera: StarlightXpress Lodestar X2

Guide Scope: Sky-Watcher Finder Scope

Mount: Sky-Watcher EQ8 Pro

Focuser: Primalucelab ROBO Focuser

Filterwheel: Starlight Xpress Ltd 7x36mm EFW

Filters: Astronomik 6nm Ha, OIII and SII 36mm

Power and USB Control: Pegasus Astro USB Ultimate Hub Pro

Acquisition Software: Main Sequence Software. Sequence Generator Pro

Calibration and Stacking: Astro Pixel Processor

Processing Software: PixInsight 1.8.6

I noviluni di questa estate non sono stati molto favorevoli. Spesso sereno ma con il cielo veramente poco trasparente. Inoltre anche la temperatura ambiente ha contribuito a complicare le cose per chi utilizza le DSLR non raffreddate.

Infatti in questa circostanza pur essendo a 1600 metri slm la temperatura non è mai scesa sotto i 20°C facendo lavorare il sensore della mia 550D intorno ai 26°-27°C e file.raw con rumore termico.

Ad ogni modo ho tentato di ottenere il massimo dall'immagine combinata con DSS.

Persino il gradiente da inquinamento luminoso ha voluto complicarmi la vita, ma spero che il risultato sia comunque gradevole.

 

The new moon this summer were not very favorable. Often without clouds but with very little transparent sky. Also, the ambient temperature has contributed to complicate matters for those who use DSLR uncooled.

In fact, on this occasion despite being at 1600 meters above sea level, the temperature never dropped below 20 ° C making the sensor work in my 550D around 26 ° -27 ° C and file.raw with thermal noise.

Anyway I tried to get the most from the image combined with DSS.

Even from light pollution gradient wanted complicate my life, but I hope that the result is still pleasant

 

____________________

 

Lens: Zenit Giove-11A 135mm f/4

Camera: Canon EOS 550D (Rebel T2i) mod. Baader BCF

Mount: Sky Watcher HEQ5 Synscan

Seeing 2 (scala Antoniadi inversa)

29x300s 1600iso / 21 dark / 21 flat / 21 bias

date 09/07/2016

temperature 22°C (media)

Temperature sensor: 26°C (media)

Integration 2h 25min

Location: monti Nebrodi, (Sicily-Italy) 1550m slm

Elaborazione DSS + PSCS3.

 

Canon EOS Ra

Raptor 61 APO

Radian Triad Ultra

 

I am really excited about this telescope. Expect a reveal/review video on Wednesday!

An emission nebula (Westerhout 5, Sharpless 2-199, LBN 667) located in the constellation Cassiopeia. The star cluster known as IC 1848 is in the body of the nebula. The solar winds from the largest stars creates the voids in the nebula and result in gases being compressed into star forming regions.

 

Takahashi FSQ-106

Software Bisque MyT

QSI 683WSG-8

Ha 22x30min

Sii 30x30min

Oiii 16x30min

Total Integration Time = 34hrs

Data from Deepskywest Remote Observatory

Galaxien Trio im Haar der Berenike

NGC4725, NGC4712, NGC4747

  

Processing: PixInsight

total exposure time: 6,4 hours

 

119x120s Luminanz

25x120s red

25x120s green

25x120s blue

 

Equipment:

10" f/4 ONTC Newtonian

ASI294mmPro

Astronomik Filter

Skywatcher EQ-8 Pro

The most famous and brightest edge-on galaxy from Coma Berenices constellation.

42 million light years from earth

 

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• Sky-Watcher BK P2001 with TS Optics 2" Dual Speed Focuser

• EQ6-R Pro

• ZWO ASI1600MM-Pro

 

• ZWO L: 112x120s

• ZWO R, G, B: 90x120s bin2

(total integration 6.7h)

• -20° sensor temp., Gain 0 (HDR)

 

• Baader MPCC Mark III coma corrector

• 60x240 guide scope, ZWO ASI290Mini guide cam

 

Captured with ZWO EFW, ZWO EAF, ZWO ASIAIR, Pegasus Astro Powerbox

 

Saint Petersburg, Russia. Red light pollution zone, balcony

Nikon D810a, 300mm nikkor,

f/7.1, iso 3200, mount: astrotrac, 120x60sec light frames, 12x60sec dark frames, 10 bias. Stacked in DSS, edited in PS/LR.

NGC 5128 or Centaurus A is one of the closest radio galaxies to Earth at a distance of approximately 12 million light-years. It has a distinctive central dust lane and an active galactic nucleus containing a supermassive black hole creating a relativistic jet which emits in visual, radio and X-ray wavelengths. The inner and outer filaments of the optical jet are visible here as the red streaks between 2 and 3 o'clock. It is an unusual galaxy, possibly the result of a merger between an elliptical galaxy and a smaller spiral galaxy.

 

Scope: Planewave CDK17 @ f/6.8 = 2939mm FL

Mount: Paramount ME

Camera: SBIG STXL-11002/AOX

Filters: Astrodon LRGB gen II, 3nm NB

Image scale: 0.63 arcsec/pixel

Exposures: 15x1200s R, 15x1200s G, 15x1200s B, 22x1200s L, 11x1800s Ha (27.83 hours)

Processing: PixInsight 1.8.5

 

Acquisition: Martin Pugh

Processing: Rick Stevenson

Imaged from Seven Skies Observatory 2022-09-21 thru 2022-10-04.

 

The second of 3 images captured during our 'test run' with the new observatory.

 

Sh2-114 is a very faint and rarely imaged emission nebula in the Cygnus constellation. It is known as the Flying Dragon Nebula, as its wispy twisted shapes resemble a flying dragon with outstretched bat-like wings. It is an unusual emission nebula that is thought to be sculpted by a combination of intense stellar winds emitted by massive stars interacting with magnetic fields within the interstellar medium.

 

Image captured over 8 nights; 2022-09-21, 24, 25, 26, 27 & 30, 2022-10-01, & 03

36.5 hours total integration

Ha subs 68 * 1,200 sec = 22 hours 40 min

OIII subs 15 * 1,200 sec = 5 hours

SII subs 22 * 1,200 sec = 7 hours 20 min

R subs 15 * 120sec = 30 min

G subs 15 * 120sec = 30 min

B subs 15 * 120sec = 30 min

 

Imaging Equipment:

SharpStar 94EDPH with reducer at 414mm focal length,

Rainbow Astro RST-135,

ZWOASI2600MM Pro camera

SHO 3.0nm filters & RGB filters

www.astrobin.com/gjlue5/

 

M86 lies in the heart of the Virgo Cluster of galaxies.

The Virgo Cluster is a cluster of galaxies whose center is 53.8 ± 0.3 Million light years away in the constellation Virgo. Comprising approximately 1300 (and possibly up to 2000) member galaxies, the cluster forms the heart of the larger Virgo Supercluster, of which the Local Group (containing our Milky Way galaxy) is a member.

 

On my picture you could see M86 as the largest galaxy but you could observe more than a hundred galaxies more, on the annotated version you could find all the information (please, see comments).

 

Technical card

Imaging telescope or lens:Teleskop Service TS Photoline 107mm f/6.5 Super-Apo

 

Imaging camera:ZWO ASI183MM-Cool

 

Mount:Skywatcher AZ EQ-6 GT

 

Guiding telescope or lens:Teleskop Service TSOAG9 Off-Axis Guider

 

Guiding camera:ZWO ASI290 Mini

 

Focal reducer:Telescope-Service TS 2" Flattener

 

Software:Pleiades Astrophoto PixInsight , Seqence Generator Pro

 

Filters:Optolong Green 36mm , Optolong Blue 36mm , Optolong Red 36mm , Optolong Lum 36mm

 

Accessories:ZWO EFW , TALON6 R.O.R , MoonLite CSL 2.5" Focuser with High Res Stepper Motor

 

Dates:Jan. 29, 2020 , Feb. 2, 2020 , Feb. 19, 2020 , Feb. 20, 2020

 

Frames:

Optolong Blue 36mm: 70x120" (gain: 183.00) -15C bin 1x1

Optolong Green 36mm: 70x120" (gain: 183.00) -15C bin 1x1

Astrodon L Gen.2 E-series 36mm: 307x120" (gain: 183.00) -15C bin 1x1

Optolong Red 36mm: 70x120" (gain: 183.00) -15C bin 1x1

 

Integration: 17.2 hours

 

Avg. Moon age: 16.07 days

 

Avg. Moon phase: 24.47%

 

Astrometry.net job: 3343099

 

RA center: 12h 26' 44"

 

DEC center: +12° 49' 30"

 

Pixel scale: 2.090 arcsec/pixel

 

Orientation: 83.513 degrees

 

Field radius: 0.639 degrees

 

Resolution: 2716x1836

 

Locations: AAS Montsec, Àger, Lleida, Spain

 

Data source: Own remote observatory

 

Remote source: Non-commercial independent facility

Lagoon & Trifid nebulae, 9 shots tracked & stacked

Imaged over 25 nights in November and December 2024 at the Los Coloraos complex in Gorafe, Spain.

 

This Galaxy doesn't rise very high from Spain so multiple nights were required to capture over 40 hours of integration. Most of the data was imaged with the UV/IR cut filter for maximum detail with Red Green and Blue for colour and a few hours of Ha, were added to highlight the Nebula regions in the galaxy.

 

A challenging project to undertake with so many nights and over 1500 frames of data to process but I am happy with the end result.

 

Many thanks for viewing and clear skies!

 

Full resolution and capture details available at

astrob.in/9pghp0/0/

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• Sky-Watcher Quattro 250P

• Sky-Watcher EQ8-R Pro

• ZWO ASI294MM-Pro

 

• Astronomik L: 40x300s bin1 gain 0

• Astronomik RGB: 29x300s bin2 gain 125

(total integration 5.75h)

 

• ZWO OAG & ASI290Mini guide cam

• TS GPU coma corrector

• ZWO EFW, ZWO EAF & Pegasus Astro Ultimate Powerbox 2

 

Trevinca, Valding, Spain

Bortle 3, SQM 21.8

 

processed with Pixinsight

So what you read next is not going to make sense, for the last four day in the morning I get the data. I have edited as per I know the shot as a colour sensor looks. After looking at it on the fouth days edit I did not like it so I thought time to try some thing new. Glass of red wine and Pink Floyd "Wish you where here" playing on the computer "Shine on you crazy Diamond", edit how I see the data not some thing else.

I hope there is a few out there understand the madness and like the edit.... for those of you like me never found the chicken once starless the chicken stood out. Bottom left corner on the rim of the light patch looking into the middle of the shot. 100% looking at The lioness profile on the other side of the nebula. This is 27 hours worth of data.

  

QHY268M -10c 110 Odd shots 5 min each filter over 4 nights .. 30 shots each RGB 1 min exposure.

QHYCFW3 and 7 Antlia filters LRGBSHaO

MeLE Mini PC

Pegasus Astro Pocket Mini power box

Starpoint Australis SP3 Focuser Rotated 90 degrees

Skywatcher 200 F4 PREMIUM PHOTO QUATTRO REFLECTOR OTA

Skywatcher F4 Aplanatic Coma Corrector

Skywatcher NEQ 6 Pro Hypertuned

SVbony 50MM Guide scope

QHY5L-II-M Guide camera

Guided PHD2, Nina

Pixinsight, Ps, Lr

No Photoshop manipulations - other than to resize.

  

eruptions on a remote moon?

IC 405 - der Flaming Star Nebel mit seinem Nachbar IC 410 der Tadpole Nebula

 

Konnte kurz vor Saisonende noch knapp 8,7 Std. mit dem Epsilon 130D und der QHY268m drauf halten.

Leider kommen die Quallen nicht so toll raus wie gehofft, denke da hätte noch etwas zusätzliches Schmalband geholfen.

 

Equipment:

Takahashi Epsilon 130ED

QHY268m

CFW3M

Astronomik H-alpha MaxFR

Skywatcher EQ8

 

Februar 2022

Processing: PixInsight/affinity photo

 

120x180s H-alpha

23x120s red

30x120s green

30x120s blue

 

2,7 Std. RGB

6 Std. H-alpha

 

total: 8,7 hour

www.astrobin.com/hnbyi1/

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• Sky-Watcher Quattro 250P

• Sky-Watcher EQ8-R Pro

• ZWO ASI294MM-Pro

 

• ZWO Hα 7nm: 57x900s bin1 gain 200

• ZWO OIII 7nm: 54x900s bin2 gain 200

• ZWO SII 7nm: 41x900s bin2 gain 200

(total integration 38h)

 

• ZWO OAG & ASI290Mini guide cam

• TS GPU coma corrector

• ZWO EFW, ZWO EAF & Pegasus Astro Ultimate Powerbox 2

 

Trevinca, Valding, Spain

Bortle 3, SQM 21.8

 

processed with Pixinsight

M 92 Globular Cluster in Hercules LRGB

 

Messier 92 is a globular cluster in the constellation of Hercules. So Hercules has a pair of spectacular clusters!

 

M 92 is about 26,000 light years from Earth, only a little farther away than M 13 The Great Hercules Cluster.

 

It is one of the bright globular clusters in the northern hemisphere, but it is often overlooked because of its proximity to the spectacular M 13 Hercules Cluster that I imaged a few days prior to this image.

 

I would recommend looking at this cluster in a telescope if possible as it truly shines bright light diamonds in the sky.

 

It’s interesting to note that M 92 is approaching us at 112 km per second!

 

A single night of imaging in May 2023 from my home in Gérgal, Spain. Taken during almost a full Moon at 96%.

 

A higher resolution image with imaging details can be found on my Astrobin page at: astrob.in/full/otud5v/0/

 

Thank you for looking.

 

Technical summary:

Captured: 7-05-2023

Imaging Sessions: 1

Location: Gérgal, Andalucía, Spain

Bortle Class: 4

 

Total Integration: 2h 8m

Filters:

Red 23x 60s 23m BIN 2 Gain 100 0C SQM 20.1

Green 21x 60s 21m BIN 2 Gain 100 0C SQM 20.1

Blue 19x 60s 19m BIN 2 Gain 100 0C SQM 20.1

UV/IR 65x 60s 1h 5m BIN 2 Gain 100 0C SQM 20.1

Pixel Scale: 0.55 arcsec/pixel

 

Telescope: Celestron C11 Edge HD f/10 2800mm

Imaging Camera: ZWO ASI 6200MM Pro

Guiding: ZWO OAG-L - ZWO ASI120MM Mini

Filters: Astronomik R, G, B, UV/IR

Mount: iOptron CEM120 EC

Computer: Minix NUC

 

Capture software: NINA, PHD2

Editing software: PixInsight, Adobe Lightroom

www.astrobin.com/ha3yjd/

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• Sky-Watcher Quattro 250P

• Sky-Watcher EQ8-R Pro

• ZWO ASI294MM-Pro

 

• Astronomik L: 263x300s bin1 gain 0

• Astronomik RGB: 98x300s bin2 gain 125

(total integration 30h)

 

• ZWO OAG & ASI290Mini guide cam

• TS GPU coma corrector

• ZWO EFW, ZWO EAF & Pegasus Astro Ultimate Powerbox 2

 

Trevinca, Valding, Spain

Bortle 3, SQM 21.8

 

processed with Pixinsight

Distance: ca.52 Mio. Lj

 

Equipment:

TS 10" f/4 ONTC Newton

1000mm f4

ZWO ASI 1600mmc

Astrodon LRGB

Skywatcher EQ8

 

Guding:

Lodestar on TS Optics - ultra short 9mm Off Axis Guider

PHD2

 

April 2018

 

Processing: PixInsight

IC404 Flaming Star Nebula in Hydrogen-alpha. 90m

www.astrobin.com/zs53kj/

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• Sky-Watcher Quattro 250P

• Sky-Watcher EQ8-R Pro

• ZWO ASI294MM-Pro

 

• Astronomik L: 170x300s bin1 gain 0

• Astronomik RGB: 75x300s bin2 gain 125

(total integration 20.4h)

 

• ZWO OAG & ASI290Mini guide cam

• TS GPU coma corrector

• ZWO EFW, ZWO EAF & Pegasus Astro Ultimate Powerbox 2

 

Trevinca, Valding, Spain

Bortle 3, SQM 21.8

 

processed with Pixinsight

Canon eos 600D modified and cooled.

Baader Bcf filter.

Skywatcher 150/750 pds.

Skywatcher Neq6 pro2 guided with phd2, zwo asi 290mc and refractor orion 50/162mm

Here are the Lagoon and Trifid Nebulae in the constellation Sagittarius.

 

From my backyard, these targets sit SO low on the horizon, that they JUST clear the treeline and my neighbor's roof.

 

They're also directly over the light dome of the city, so, needless to say, a challenging image from my location.

 

However, I am SUPER happy with the results I am getting from the system I mentioned in my last video. The Triad ultra filter and RedCat are a match made in heaven if you like these types of images.

 

Not to rush galaxy season. but seriously, I can't wait to dig into Cygnus over the next 2 months.

 

Canon EOS 60Da

William Optics RedCat 51

Sky-Watcher HEQ5

OPT Triad Ultra

 

28 x 5-minutes

ISO 1600

 

Stacked in DSS with Darks and Flats.

 

Topaz DeNoise AI for noise reduction

 

Processed in Adobe Photoshop

   

Explanation: The globular cluster M22, contains over 100,000 stars. These stars formed together and are gravitationally bound. Stars orbit the center of the cluster, and the cluster orbits the center of our Galaxy. So far, about 140 globular clusters are known to exist in a roughly spherical halo around the Galactic center. Globular clusters do not appear spherically distributed as viewed from the Earth, and this fact was a key point in the determination that our Sun is not at the center of our Galaxy. Globular clusters are very old. There is a straightforward method of determining their age, and this nearly matches the 13.7 billion-year age of our entire universe. (Text: apod.nasa.gov/apod/ap050627.html)

 

This picture was photographed June, 13, 2015 in Rozhen observatory, Bulgaria.

 

Equipment: home assembled reflector 10 in., f/3.8

Mount WhiteSwan-180 with a control system «Eqdrive Standart», camera QSI-583wsg, Tevevue Paracorr-2. Off-axis guidecamera QHY5L-II.

RGB filter set Baader Planetarium.

RGB= 8*100 sec. each filter, bin.1.

40 minutes total.

 

FWHM 2.25″-2.56″

Altitude from 23° to 24°

 

Processed Pixinsight 1.8 and Photoshop CS6

-#265 in Explore 29/10/2017 (verificato 01/11/2017 )

 

Star Party del Gruppo Astrofili Catanesi presso Rifugio Margio Salice 18-20/08/2017

 

Speravo in qualcosa di più da questa immagine, ma in questa circostanza penso di aver raggiunto veramente i limiti strumentali e i miei limiti elaborativi.

La piccola nebulosa a riflessione, denominata "Iris" (NGC7023) di colore azzurro-ciano è certamente un oggetto facile da fotografare, ma il mio vero interesse erano le interessanti nubi molecolari che la circondano insieme a quelle oscure come la VdB141 denominata "nebulosa Fantasma" e che farebbero parte del complesso nebuloso molecolare di Cefeo

Sapevo che queste nubi molecolari, molto deboli e di natura oscura erano difficili da fotografare, ma contavo su una integrazione su 6h e 25min acquisita in 3 notti consecutive.

Purtroppo questa non è bastata perchè due parametri critici hanno rovinato la maggioranza dei frame: la temperatura del sensore direttamente influenzata dalla temperatura ambientale e la non ottima trasparenza del cielo. LA temperatura ambiente media notturna è stata di circa 18-19° C e quindi quella del sensore intorno ai 26° C. Troppo rumore termico (che potete vedere qui Frame grezzo singolo dell'immagine ) che ha cancellato il debole segnale delle nubi molecolari. In minor misura ha influito la non ottima trasparenza del cielo che ha permesso all'Inquinamento Luminoso delle vicine città di rendere il cielo lattiginoso.

Per evidenziare le nubi molecolari occorre agire con molti strech successivi che in questo caso hanno evidenziato soprattutto il rumore. Ho dovuto quindi trovare un compromesso rendendo morbida l'immagine.

L'elaborazione forzata ha evidenziato anche la vignettatura anche se trattata con i flat; quindi ho dovuto croppare del 10% entrambi i lati dell'immagine.

Mi auguro che questa condivisione possa aiutare gli amici astrofili come confronto e a fare le scelte migliori in base al setup posseduto e ad altri parametri esterni.

_________________________

-#265 on Explore 10.29.2017 (checked on 11.01.2017)

 

Star Party of Gruppo Astrofili Catanesi at Rifugio Margio Salice August 18-20, 2017

 

I was hoping for something more from this image, but in this circumstance I think I have really reached the instrumental limits and my elaborate limits.

The little reflection nebula, called "Iris" (NGC7023) of blue-cyan color is certainly an easy-to-photograph object, but my real interest was the interesting molecular clouds that surround it along with the obscure ones like the VdB141 called "Ghost Nebula "and that would be part of the Cepheus Molecular Cloud Complex .

I knew these molecular clouds, poorly lit and dark nature were difficult to photograph, but I expected on an integration of 6h 25min acquired in 3 consecutive nights.

Unfortunately this was not enough because two critical parameters have ruined the majority of frames: the temperature of the sensor directly affected by the ambient temperature and the poor transparency of the sky. The average nighttime ambient temperature was around 18-19 ° C and therefore the sensor temperature around 26 ° C. Too much thermal noise (you can see here single raw frame ) that cleared the little signal of molecular clouds. The unobtrusive transparency of the sky has adversely affected to a lesser extent; in fact it has made the bright sky caused by the light pollution coming from nearby cities

To highlight the molecular clouds, it is necessary to act with many successive strechs which in this case have highlighted the noise above. I had to find a compromise, making the image softer.

Forced processing also highlighted the vignetting even if treated with the flat; so I had to cut 10% on both sides of the image.

I hope this sharing can help amateur astronomers friends how to compare and make the best choices based on their setup and other external parameters.

__________________________

 

Optic: Rifrattore APO Scopos TL805 80mm/f7 + WO 0.8X

Camera: Canon EOS 550D (Rebel T2i) mod. Baader BCF

Mount: Sky Watcher HEQ5 Synscan

Seeing: 3 (scala Antoniadi inversa)

55x420s 1600iso / 17 dark /21 flat / 21 bias

Date: 18-19-20/08/2017

Integration: 6h 25min

Temperature: 19°C (media)

Temperature sensor: 26°C (media)

Location: Rifugio Margio Salice, monti Nebrodi (Sicily-Italy) 1250m slm

Elaborazione DSS + PSCS3.

 

This deep image of the Helix Nebula reveals the full extent of the series of ejecta blown off by this dying star. The deep exposure reveals a long history of stellar eruptions by a once Sun like star in Aquarius. In this image the Helix Nebula is shown to actually cover several full moons worth of sky area!

 

AP152 F7.5 Starfire APO refractor with 4" field flattener

FLI ProLine11002 CCD & CFW-2-7

L SII Ha OIII: 1hr, 7hrs, 10hrs, 9hrs = Total 27hrs (all bin 1X1) Astronomik filters

AstroHandy LightRing used for flats

FOV = 1.0deg X 0.8deg at 1.4"/pix

Guide Camera: Starlightxpress SXVH9

Astroart4 use for camera control and processing

Orion Nebula - Stock DSLR, Sigma Lens and star adventurer tracker.

 

Sh2-155 is a diffuse nebula in the constellation Cepheus, within a larger nebula complex containing emission, reflection, and dark nebulosity. The Cave nebula is about 2,400 light-years away from Earth.

 

Image captured over 4 nights; 2021-10-01 to 2021-10-07.

17 hours and 20 min total integration

Ha subs 24 * 1,200sec = 8 hours

OIII subs 13 * 1,200sec = 4 hours 20 minutes

SII subs 15 * 1,200sec = 5 hours

Imaging Equipment:

SharpStar 140PH Triplet 910mm focal length

Mesu 200 MKII,

ZWOASI2600MM Pro camera

3nm Ha, OIII & SII filters

NGC7380 or the Wizard Nebula as it is commonly known as, is an emmision nebula in the constelation of Cepheus

 

Image Details:

Acquisition Dates:Sept. 20, 2019, Sept. 21, 2019, Sept. 30, 2019, Dec. 6, 2019, Dec. 9, 2019, Dec. 20, 2019, Dec. 25, 2019, Dec. 31, 2019

 

Frames:

Astronomik Ha 6nm: 51x300" (gain: 11.00) -20C bin 1x1

Astronomik OIII 6nm: 51x300" (gain: 11.00) -20C bin 1x1

Astronomik SII 6nm: 51x300" (gain: 11.00) -20C bin 1x1

 

Integration: 12.8 hours

Darks: ~101

Flats: ~101

Flat darks: ~101

Avg. Moon age: 15.36 days

Avg. Moon phase: 43.95%

Bortle Dark-Sky Scale: 4.00

 

Equipment Details:

Imaging Scope: Sharpstar Optics 15028HNT Hyperboloid Astrograph Reflector

Imaging Camera: Qhyccd 183M Mono ColdMOS at -20C

Mount: Sky-Watcher EQ8 Pro

Guide Scope: Sky-Watcher Finder Scope

Guide Camera: Starlight Xpress Ltd Lodestar X2

Filters: Astronomik 36mm RGB F2.2 Certified

Filterwheel: Starlight Xpress Ltd 7x36mm EFW

Power and USB Control: Pegasus Astro Ultimate USB Hub

Focuser: Primalucelab Sesto Senso Auto Focuser

Image Acquisition Software: Main Sequence Software SGPro

Guide Software: PHD 2

Processing Software: PixInsight

  

This nebula region of gas and dust is brilliantly colorful and often photographed. The star that is yellow is the named star Antares.

 

L 10mx39

R 10mx38

G 10mx34

B 10mx28

Total Integration = 23.2h

 

Data from Telescope.Live

 

PI: CC/RGB Comb/DC/Curves/LRGB Comb

PS: ColorEfex Detail Extractor/Curves/Smart Sharpen

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• Sky-Watcher BK P2001 with TS Optics 2" Dual Speed Focuser

• EQ6-R Pro

• ZWO ASI1600MM-Pro

 

• Baader Hα 7nm: 15x600s

• Baader OIII 8.5nm: 15x600s

(total integration 5h)

• -20° sensor temp., Gain 139 (UG)

 

• Baader MPCC Mark III coma corrector

• 60x240 guide scope, ZWO ASI290Mini guide cam

 

Captured with ZWO EFW, ZWO EAF, ZWO ASIAIR, Pegasus Astro Powerbox

 

Saint Petersburg, Russia. Red light pollution zone, balcony

www.astrobin.com/u1ip0r/

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• Sky-Watcher Quattro 250P

• Sky-Watcher EQ8-R Pro

• ZWO ASI294MM-Pro

 

• Astronomik L: 101x300s bin1 gain 0

• Astronomik RGB: 44x300s bin2 gain 125

• ZWO Hα 7nm: 29x300s bin1 gain 200

(total integration 14.5h)

 

• ZWO OAG & ASI290Mini guide cam

• TS GPU coma corrector

• ZWO EFW, ZWO EAF & Pegasus Astro Ultimate Powerbox 2

 

Trevinca, Valding, Spain

Bortle 3, SQM 21.8

 

processed with Pixinsight

Rosette Nebula Narrow Band Image" Image time 30 Hrs with 10 min subs using Ha S2 O3 filters. Imaged from my backyard in Whittier CA USA Using a TOA-130f @ 1004mm Mounted on a AP1200 Note: Image start date 1-1-08 Thru 2-10-08

Using warp drive from it's powerful anti-matter engine, the Hullbull Remote Space Telescope has rapidly approached the distant City of Light, Metropolis 1, to capture images from the incredible light show heralding the opening of the light city, some thousand light years distant. Here, one of the first images from the mission shows the first stages of a powerful series of explosions where matter was created by use of an advanced dimensional oscillator, similar to a miniature and controlled "Big Bang". Stellar fireworks, if you will. This is from the start of the light show which was produced a safe distance from Metropolis 1, several astronomical units, but yet close enough for the residents to see it develop in real time. The scale of the light show as viewed from Metropolis 1 would be similar to about 20 times the size of the full moon in our own sky. Additional images from the light show will be posted as more data are received from the Hullbull Telescope.

The Cocoon Nebula (IC1396) in the constellation of Cygnus. My third attempt at this very faint object. This image combines data from 2013 and 2016. All data was collected from the Tacoma Astronomical Society's site for their annual star party in Goldendale, Washington. Total exposure time is 9.4 hours.

This is M78/NGC2068, a 5 light-year wide nebula about 1350LY away in the constellation Orion.

 

Imaged using a 8" SCT at f6.3 (1280mm focal length), with a QHY268M camera for a total integration time of 12 hours through LRGB and H-Alpha filters.

The Cygnus Wall complex is part of the more recognisable North American nebula.

 

This ridge is approximately 20 light years long and is a huge star forming region. You can see where it is in a larger picture below.

 

This is a 4 pane mosaic as the field of view was too small to fit in the Cygnus Wall itself.

 

Details

M: Mesu 200

T: ODK10

C: QSI683 with 3nm Astrodon Ha filter

 

18x1800s in each pane

Total exposure 36 hours

www.astrobin.com/385914/

 

Very faint nebulosa in Auriga.

That's the most complicated object I never did and my first integration from new really dark location at Montsec, Lleida (Spain). Integration of 29.5 hours.

 

A really proof for remote operations that I started one month ago.

 

Technical card

Imaging telescope or lens:Teleskop Service TS Photoline 107mm f/6.5 Super-Apo

 

Imaging camera:ZWO ASI1600MM-Cool

 

Mount:Astro-Physics Mach-1 GTO CP4

 

Guiding telescope or lens:Celestron OAG Deluxe

 

Guiding camera:QHYCCD QHY5III174

 

Focal reducer:Riccardi Reducer/Flattener 0.75x

 

Software:Main Sequence Software Seqence Generator Pro, Astro-Physics AAPC, Pleiades Astrophoto PixInsight

 

Filters:Astrodon HA 36mm - 5nm, Astrodon B Gen.2 E-series 36mm, Astrodon G Gen.2 E-series 36mm, Astrodon R Gen.2 E-series 36mm, Astrodon S-II 36mm - 5nm, Astrodon O-III 36mm - 5nm

 

Accessories:ZWO EFW, MoonLite NiteCrawler WR30

 

Resolution: 2328x1760

 

Dates:Jan. 9, 2019

 

Frames:

Astrodon B Gen.2 E-series 36mm: 45x10" (gain: 200.00) -20C bin 1x1

Astrodon G Gen.2 E-series 36mm: 45x10" (gain: 200.00) -20C bin 1x1

Astrodon HA 36mm - 5nm: 104x600" (gain: 200.00) -20C bin 1x1

Astrodon O-III 36mm - 5nm: 36x600" (gain: 200.00) -20C bin 1x1

Astrodon R Gen.2 E-series 36mm: 45x10" (gain: 200.00) -20C bin 1x1

Astrodon S-II 36mm - 5nm: 35x600" (gain: 200.00) -20C bin 1x1

 

Integration: 29.5 hours

 

Avg. Moon age: 3.07 days

 

Avg. Moon phase: 10.31%

 

Astrometry.net job: 2466785

 

RA center: 81.629 degrees

 

DEC center: 42.932 degrees

 

Pixel scale: 2.936 arcsec/pixel

 

Orientation: 89.771 degrees

 

Field radius: 1.190 degrees

 

Locations: AAS Montsec, Àger, Lleida, Spain

 

Data source: Own remote observatory

 

Remote source: Non-commercial independent facility

My previous attempt at this was a failure so I moved to a faster scope.

My intent with this image is to show the subtly of this faint structure.

Acquisition details: www.astrobin.com/prmon5/

Here is my first and only attempt at Comet Leonard!

It was from the end of November that I was looking for the ideal weather conditions, but unfortunately it never stopped raining and the sky was always overcast.

I had almost lost hope, but this morning (Friday 10 December) after I woke up at 3.45 AM, I was finally able to take the shot I so wanted to do.

Miraculously the conditions were optimal and Leonard's magnitude was 4.85 (considering the air masses).

I was able to shoot until around 6 AM and eventually I also captured a small thunderstorm along with the twilight lights of dawn.

 

Nikon D750 modded, AF-S NIKKOR 70-200mm f/2.8G ED VR II

 

Panorama 3 blocks @ 70mm: landscape (1x13sec, ISO 2540, f/5.6), sky (1x20sec, ISO 3200, f/2.8), Leonard (200mm scaled at 70, 85x20sec, ISO 3200, f/2.8 + 45 dark frames, bias, flats)

A close up of the prominence in the Cygnus Wall part of NGC 7000 North America Nebula

 

Imaged using the Celestron C14 EdgeHD telescope at f/11 and ZWO 6200MM cooled camera.

Imaged over 8 nights in September 2024 at Los Coloraos, Gorafe, Granada, Spain.

47 Hours of integration in Ha, Oiii, Sii, Red, Green and Blue filters.

 

A full resolution image and technical details are available at astrob.in/nkb6qp/0/

 

Deep Space Antenna 1 is ESA’s first 35-m deep dish, staring out to space to communicate with missions far from home.

 

Located 140 kilometres north of Perth, Western Australia, close to the village of New Norcia, this giant antenna is in the perfect spot to observe the skies.

 

“The Wadjarri people from the Murchison region refer to much of the milky way as the emu, as it resembles an emu stretched across the sky,” says Suzy Jackson, Maintenance & Operations Manager for the ground station.

 

“I’m told that when the emu’s nose reaches the horizon, that’s the best time to collect emu eggs. Having our antenna in the foreground just makes it all the better. I am amazed at how beautiful our workplace here is.”

 

The New Norcia antenna provides routine support to missions orbiting Mars like Mars Express and Exomars TGO as well as the Gaia space observatory, in the process of making the world's most precise map of the stars in our Milky Way galaxy and BepiColombo on its way to Mercury.

 

With the launch of ESA’s ESTRACK now 'dashboard’, you can find out exactly which missions are communicating with which antennas at any moment, and discover more about what individual missions are up to - what is their mission and how far away are they?

 

Explore the ESTRACK network in real time.

 

Check out our guide to using the dashboard, here.

 

This processed image was taken by local astrophotographer Jim Longbottom. Find more of his work on his Flickr page.

 

Credits: Jim Longbottom

 

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