LRGB_M1

M1 - The Crab Nebula TEC140

The Crab Nebula - M1 - is the expanding remains of a supernova that was seen in 1054 throughput medieval Europe, The Middle East and China.  The nebula is very distant at about 6500 light years and lies in the Perseus Arm of our galaxy, further out from The Galaxy's core than The Sun.  It is called The Crab because William Parsons from his Irish observatory who first viewed it in 1840 thought it resembled the outline of a crab and the name has stuck.  The object was first observed in the 1731 and was linked to the Supernova of 1054 as recently as 1913.  Earlier photographic plates from the 1950's and those taken today show a definite expansion in the nebula in the intervening 70 years.


LRGB_M1
M1 - The Crab Nebula

Image Technical Data

Imaged from my backyard in Nottingham, UK in the winter of 2017 with my TEC 140 refractor and Atik 460 cooled CCD camera and Baader LRGB filters.  I used a NEQ6 mount guided with OAG.

All images data binned 1x1:

Lum > 10 x 900s ; Red > 15 x 300s ; Green 15 x 300s ; Blue > 19 x 300s

Image capture with APT and processing in PixInsight and Photoshop CC.


LRGB_Annotated
M1 Annotated Version

LRGB_Inverted
M1 Inverted Version

NGC 7814

NGC 7814 - The Little Sombrero Galaxy - TEC 140

NGC 7814
NGC 7814 - The Little Sombrero Galaxy

NGC 7814 is an edge-on spiral galaxy 40 million light-years away in the constellation of Pegasus.  IT is nicknamed "The Little Sombrero" because of its likeness to The Sombrero Galaxy M104 in Virgo.  Close examination of the picture reveals many tiny galaxies, up to a billion light years away in the depths of The Universe.

The dust lanes of the edge-on spiral arms can be easily seen.

Image Technical Data

NGC 7814 is very remote and so needs a long integration (exposure) time.  This image was captured from my backyard observatory in Nottingham, UK over the course of three nights in October 2019 (a very wet period in the UK and the capture nights were 2,17 and 24).  It took significant dedication to capture the subframes for this image given the dreary weather circumstances  and I nearly gave up on several occasions!  I used my TEC 140 refractor with Atik 460 cooled CCD camera with Astrodon E Series Generation 2 filters on my OAG guided MESU 200 mount.

Integration is a total of nine hours comprised of:

Luminance > 22 x 900s binned 1x1 ; Red > 17 x 300s 2x2 ; Green > 14 x 300s 2x2 ; Blue > 14 x 300s 2x2

Image capture in Sequence Generator Pro and processing in PixInsight and Photoshop CC.  The bright star to the top centre is very difficult to control. This star is of course a foreground star in our own galaxy and is millions of times nearer to the Earth than the galaxy.


NGC 7814 Annotated
NGC 7814 Annotated

NGC 7814 Inverted
NGC 7814 Inverted

M39

M39 Open Cluster in Cygnus - TEC140 refractor

M39 is an open cluster, about 1100 light years distant, in the constellation of Cygnus, The Swan.  M39 is about 30 arc minutes in diameter, about the width of the full moon. The Cygnus constellation abounds in interesting objects and The Milky Way galaxy flows straight through it.


M39
M39 Open Cluster in Cygnus

ImageTechnical Data

Imaged from my backyard in Nottingham, UK on the 16th October 2019 when it was high overhead from my location.  I used my TEC 140 refractor and Atik 460 cooled CCD camera with Astrodon RGB E Series Generation 2 filters.  I used my MESU 200 mount guided with an off-Axis guider.

All exposures binned 1x1:

Red > 15 x 120s ; Green > 12 x 120s ; Blue > 15 x 120s


M39_Annotated
M39 Annotated

M39_Inverted
M39 Inverted

I hope you like it! :)


Fireworks_Galaxy_LRGBHa2

NGC 6946 - The Fireworks Galaxy - TEC 140


NGC6946 - The Fireworks Galaxy

NGC6946 is located on the border between Cygnus and Cepheus and is a fairly bright galaxy about 25 million light years away.  It is dubbed the "The Fireworks Galaxy" due to the unusually high number of supernovae that have occured here - ten - that have been observed during the last century.  Typically a galaxy would normally have one per century and it is not known why this galaxy has had ten times the average.

The galaxy is quite heavily obscured by dust within our own galaxy and this is probably the reason why it was not accorded the honour of a Messier catalogue number.

Image Technical Details

Imaged from my back yard in Nottingham, UK, during September 2020 whilst high overhead.  I used my TEC140 refractor with Atik 460 CCD camera and Astrodon LRGB Generation 2 E series filters and a Ha (3nm) filter.  Out in front of the filter wheel was an IDAS light pollution filter.  MESU 200 Mount was guided with an off-axis guider.  Transparency for the luminance was good but was poor for the RGB and Ha data.

Lum > 36 x 300s 1x1s ; RGB  > 14 in each x 300s 2x2 ; Ha > 14 x 300s 2x2

Image capture in SGP and processing in PixInsight and Photoshop CC.


LRGBHa_Annotated
Annotated Version

LRGBHa_Inverted
Colour Inverted Version

NGC 2403

NGC 2403 - TEC140

NGC 2403 is a spiral galaxy located about eight million light years away in the constellation of Camelopardalis in the Northern hemisphere.  It is an outlying member of the M81/M82 group.  You will note that it bares a striking resemblance to M33 and contains huge HII star forming regions.  NGC2403 is much smaller than our own galaxy, being only about 50000 light years in diameter as opposed to about 120000 light years for our own Milky Way galaxy.  It is not known why a smaller galaxy like this should have such huge HII regions that dwarf those of our own, larger galaxy.


NGC 2403
NGC 2403

Image Technical Data

Imaged from my backyard, March 2019, in Nottingham, UK.  I used my TEC 140 refractor with Atik 460 CCD camera and Astrodon LRGB filters.  Image acquisition data, everything binned 1x1

Luminance 29 x 600s; Red 12 x 300s; Green 12 x 300s;  Blue 12 x 300s


NGC 2403 Annotated
Annotated Version

NGC 2403 inverted
Inverted Version

M15

M15 The Globular Cluster in Pegasus

M15 is a magnificent Globular Cluster in the constellation of Pegasus, which after M13 and M92 is arguably the best one visible to Northern Hemisphere observers.

It is located about 34000 light years away and is about 125 light years in diameter with an age of 12 billion years, it is as old as the Milky Way itself.


M15 Globular Cluster

Image Technical Data

Imaged with my TEC 140 refractor and Atik 460 CCD camera September 24th 2018.  Mount is my MESU 200 guided with off-axis guiding.

Red 22 x 300s 1×1; Green 12 x 300s 1×1;  Blue 19 x 300s 1×1

Total Integration of the data set is about four and a half hours. Note that I did not use a separate luminance channel and instead I binned each of the RGB channels 1x1.  I remain to be convinced of the need to capture a separate luminance channel with either globular or open clusters.

Image processing is with PixInsight and data collected with Sequence Generator Pro.


M15 Annotated

NGC 7331 Completed_LRGB

NGC 7331 TEC 140 Refractor - The Deer Lick Group

NGC 7331 (Caldwell 30) is a spiral galaxy about 46 million light years away in the constellation of Pegasus.  It is a vibrant and colorful galaxy, often referred to as the Milky Way's "twin" due to it being of a similar size and mass to our own galaxy.  It is visible in amateur telescopes as a faint smudge if the sky is dark.

In the images below, the smaller galaxies to the left of the main galaxy are a chance line-of-sight alignment.  These four galaxies are much more distant than NGC 7331 (about 320 million light years) and are nothing to do with the main galaxy.  This collection of galaxies (NGC 7331 and the distant background galaxies are collectively referred to as the Deer Lick Group named after the Deer Lick gap in the mountains of North Carolina by astronomer Tomm Lorenzin who liked to observe from there.


NGC 7331 Completed_LRGB
NGC 7331

Image Technical Data

Imaged over two nights on the 21st and 22nd September 2019 with my TEC 140 refractor from my backyard in Nottingham, UK.  I used my Atik 460 CCD camera with Astrodon LRGB Generation 2 E-series 1.25" filters.  I used my MESU 200 mount that was guided via OAG.

Luminance 24 x 600s 1×1;  Red 12 x 300s 2×2; Green 12 x 300s 2×2;  Blue 12 x 300s 2×2

Total Integration of the data set is seven hours.  It would benefit from the addition of more data but I am quite content with it now as it is.

Image processing with PixInsight and data collected with Sequence Generator Pro.


NGC 7331 Completed_LRGB_Alternate
NGC 7331 Alternative Processing

In the second version I processed the data slightly differently with a bit more focus on the red spectrum of the galaxy in the absence of any Hydrogen Alpha data.  However, I think this is slightly too much and I prefer the first image as more natural.  However, I include it here as an interesting contrast in the different approaches that can be taken to astronomy image processing with the same data set with differing emphases that can be quite subjective.


NGC 7331 Annotated
Annotated Version

NGC 7331 Inverted
Inverted Version

Abell 1656 Complete

Abell 1656 TEC 140


Abell 1656 Complete
Abell 1656

Abell 1656 - The Coma Cluster - is a cluster of galaxies in the constellation of Coma Berenices, located about 320-330 million lights years away.  The cluster is dominated by two supergiant elliptical galaxies  NGC 4874 and NGC 4889 which are visible in this image in the centre below the bright blue star (which is local to our own galaxy).  NGC 4889 is the largest and most massive galaxy in the local universe and is vsoble in modest amateur telescopes despite the great distance.  It contains the most massive black hole yet discovered.  The galaxy itself is estimated to have more than 1000 times the mass of opur own Milky Way galaxy.

Image Technical Data

Image acquired spring 2020 (during the Coronavirus lockdown) in my backyard in Nottingham, UK.  It was acquired with TEC 140 refractor (with field flattener) with Atik460 CCD camera and Astrodon LRGB Gen2 E series filters on my MESU 200 mount.  Guiding was via off-axis guider.

Luminance 30 x 300s 1x1;  Red 14 x 300s 2x2; Green 15 x 300s 2x2;  Blue 14 x 300s 2x2

Data processed with PixInsight and Photoshop and data collected with SGP Pro and guided with PHD2.


Abell_1656_Annotated
Annotated Version of Abell 1656

M27 LRGB

M27 - My First LRGB CCD Picture

M27 is known as The Dumbbell Nebula and is a planetary nebula in the constellation of Vulpecula - The Fox.  It is located about 1250 light years away and represents the outer ejected gas envelope of a dying star. 

This is the first image I took with my CCD camera - Atik460 - on the 28th October 2013.  This is a lovely object in the summer and early autumn skies and is very pleasing visually in a pair of binoculars or a telescope.  Its brightness and vivid colour make it a perennial favourite object for astro imagers.  


M27 LRGB
M27 - The Dumbell Nebula

Image Technical Data

This is a small dataset taken with my  superb Skywatcher ED80 Black Diamond refractor and Atik 460 CCD camera with Baader LRGB filters on an NEQ6 mount, guided with a Skywatcher guidescope and QHY5 (I still have and use this guide setup).  This is a superb imaging setup and despite its modest cost is capable of great results.  I upgraded the ED80 to a Takahashi FSQ85 and sold the ED80.  Be assured though, the super ED80 is capable of 90% of what the FDSQ can do at 10% of the cost.  I kind of regret selling that ED80 now.

Luminance 8 x 300s 1x1;  Red 6x 180s 1x1; Green 7 x 180s 1x1;  Blue 7x 180s 1x1

Developed in PixInsight - first picture I ever developed with this software.

It looks quite nice for an early effort.

P.S.  This excellent Atik 460 CCD camera and EFW2 filter wheel is still going strong after seven years of use (writing this in August 2020).  I had to have a port repair on the EFW2's mini-USB port under Atik's fabulous customer service in 2019 but other than that no issues whatsoever with the camera or filter wheel.  I have since upgraded the filters to Astrodon E series Gen2 LRGBHaOIII filters.


M33 The Triangulum Galaxy

M33 With TEC140 Refractor

I have completed several images of the famous Triangulum Galaxy - M33, over the years.  This is one of the most photographed objects in the sky and with good reason; it is a beautiful face on spiral galaxy that is the second closest major galaxy after Andromeda.  It is bright and colourful and responds well to all types of imaging, whether with a DSLR or CCD, camera lens or telescope.  It is probably the second "go to" target to photograph for astro photography beginners after the Andromeda galaxy.

The image below is a version captured with the TEC 140 refractor and Atik 460 CCD camera and is the total of about 12 hours of LRGBHa data captured from my backyard observatory in Nottingham, UK in 2018.  You can see it fills the frame very nicely.


M33 The Triangulum Galaxy
M33 The Triangulum Galaxy

M33 Annotated
M33 Annotated

M33 Inverted
M33 Inverted

Image Technical Data

Image acquired spring 2018 and 2019 seasons over several capture sessions due to very wet and persistent cloudy weather) in my backyard in Nottingham, UK.  It was acquired with TEC 140 refractor  with Atik 460 CCD camera and Baader HaLRGB  filters on my MESU 200 mount.  Guiding was via off-axis guider.

A modest data set with everything binned 1x1 so as not to need so much luminance so a bit of an experiment!  Did it work?

Luminance 10 x 300s 1×1;  Red 9x 300s 1x1; Green 10x 300s 1×1;  Blue 9x 300s 1x1; Ha 12 x 900s 1x1

Data processed with PixInsight and Photoshop and data collected with SGP Pro and guided with PHD2.

Here is another version of M33 with a wider field FSQ85 refractor:

https://thekirkshouse.com/m33-the-triangulum-galaxy/


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