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/


Horsehead Nebula

The Horse head Nebula


Horsehead Nebula
The Horsehead Nebula in HaRGB

A famous, indeed iconic nebula in the constellation Orion, The Horsehead was not even discovered until 1888 with the advent of astro photography.  It is very faint to see visually with a telescope.

The image above was captured with my TEC 140 refractor and Atik 460 CCD camera with Astrodon RGB and Ha(3nm) filters. It contains a total of 120 minutes of Ha data and 45 minutes each of RGB data, everything binned 1x1 with 5 minutes exposures.


M97 The Owl Nebula

M97 - The Owl Nebula TEC 140


M97 The Owl Nebula
The Owl Nebula

The Owl Nebula is a planetary nebula in the constellation of Ursa Major, one of three planetary nebulae in the Messier catalogue.  It is visible as a faint smudge in amateur telescopes but the colours are not evident visually.  It is called The Owl Nebula because of the resemblance to the face of an owl.  6 hours and 30 minutes of LRGB in this image


M97 The Owl Nebula Annotated
M97 Annotated Version

The annotated version above shows many distant galaxies in the same field of view as M97, although obviously these are very much more distant.


M97 Inverted
Annotated Version

M97 The Owl Nebula HOO Palette
HOO Version

The HOO version above shows the Owl Nebula with Hydrogen Alpha mapped as Red channel and OIII mapped to Green and Blue to create the HOO palette colours. 3 hours and 30 minutes of HaOIII.  This HOO image could really do with more data added to it in the Ha and OIII channels and I hope to do this next spring hopefully.

Image Technical Data

This image was captured with TEC 140 refractor and Atik 460 CCD with Astrodon LRGBHaOIII (3nm) filters during Spring 2020 (during the coronavirus lockdown in the UK) from my backyard in Nottingham.  Mount is my MESU 200 guided with OAG.  There is a quite a lot of data in these images as follows.  Everything binned 1x1:

Lum 20 x 600s;  Red 13 x 30s;  Green 12 x 300s;  Blue 13 x 300s;  Ha 12 x 600s; OIII 9 x 600s


M97 The Owl Nebula

M97 - The Owl Nebula TEC 140


M97 The Owl Nebula
The Owl Nebula

The Owl Nebula is a planetary nebula in the constellation of Ursa Major, one of three planetary nebulae in the Messier catalogue.  It is visible as a faint smudge in amateur telescopes but the colours are not evident visually.  It is called The Owl Nebula because of the resemblance to the face of an owl.  6 hours and 30 minutes of LRGB in this image


M97 The Owl Nebula Annotated
M97 Annotated Version

The annotated version above shows many distant galaxies in the same field of view as M97, although obviously these are very much more distant.


M97 Inverted
Annotated Version

M97 The Owl Nebula HOO Palette
HOO Version

The HOO version above shows the Owl Nebula with Hydrogen Alpha mapped as Red channel and OIII mapped to Green and Blue to create the HOO palette colours. 3 hours and 30 minutes of HaOIII.  This HOO image could really do with more data added to it in the Ha and OIII channels and I hope to do this next spring hopefully.

Image Technical Data

This image was captured with TEC 140 refractor and Atik 460 CCD with Astrodon LRGBHaOIII (3nm) filters during Spring 2020 (during the coronavirus lockdown in the UK) from my backyard in Nottingham.  Mount is my MESU 200 guided with OAG.  There is a quite a lot of data in these images as follows.  Everything binned 1x1:

Lum 20 x 600s;  Red 13 x 30s;  Green 12 x 300s;  Blue 13 x 300s;  Ha 12 x 600s; OIII 9 x 600s


NGC 4565 - The Needle Galaxy

NGC4565 - The Needle Galaxy TEC 140

Located in the constellation of Coma Berenices, The Needle Galaxy is an almost edge on galaxy about 40 million light years away.  Much detail can be seen in the dusty lanes of the edge-on spiral arms.

This picture is a two year project, off and on.  I acquired the luminance data in May 2019 with a view to completing the image then.  However, cloudy weather then plagued the UK for weeks, and when it eventually cleared the object had vanished behind neighbouring roofs!  So I had to park this image and wait a year to collect the RGB colour data in April 2020 (whilst my country [UK] was in lockdown due to the coronavirus).


NGC4565 - The Needle Galaxy

Data used to build the image collected with TEC140 refractor and Atik460 CCD camera with Astrodon LRGB Gen 2 E-series filters.  I used Off-Axis guiding on my Mesu 200 mount.

Data set is 20 x ten minute luminance (1x1) and 60 minutes each in R, G and B (2x2).  Processed in PixInsight and Photoshop.

Lots of very faint background galaxies visible the image above and detailed in the annotated version below.


Annotated Version

Inverted Version

The North American Nebula with Samyang 135mm


North American Nebula Ha
Hydrogen Alpha North American and Pelican Nebulae

Above is 120 minutes worth of Hydrogen Alpha data captured in five minute exposures with an Astrodon Ha 3nm filter and a Samyang 135mm camera lens on a Moravian Instruments G2-8300 CCD camera.


Completed in RGB NAN
RGB data

I then captured one hour in each of the Astrodon R,G and B filters with the same rig as detailed for the Ha image, again in five minute exposures.   However, use of the superb Astrodon E series RGB filters produce a nice image and the colours are brought out quite nicely although it lacks a bit of punch and vibrancy. 

The bright star to the right is Deneb.


HaRGB image

In Photoshop I broke out the red channel and then blended it as a 50:50 mix with the Ha image (at the top of this page) before recombining back into RGB.  I also saved a copy of this HaR constituent and then used that as a luminance layer to really make the image pop.  I then used a series of high pass filters to reveal finer structures in the image.


Alternate Version HaRGB

M81_Galaxy

M81 - Bode's Galaxy in Ursa Major with TEC 140


M81 in Ursa Major

M81 is a face on spiral galaxy in the constellation of Ursa Major and it (and nearby M82) are the most northerly of the Messier objects.  It is easily visible in binoculars as a faint smudge.  Its open spiral arms and red HII star forming regions make it a popular target for amateur and professional astronomers alike.  In this picture note at the four o'clock position the very faint satellite galaxy Holmberg II.

It is located about 12 million light years away, placing it outside of the local group and it is steadily receding from us.

I have imaged M81 in several settings.  This picture was taken with my TEC140 refractor and Atik 460 CCD camera with Baader LRGBHa filters.  It contains five hours of luminance of 900s exposure, two hours of Ha data and 90 minutes in each of RGB to give a total integration time of about twelve hours.

M81 HaLRGB Annotated
M81 HaLRGB Inverted


M13_Complete_After_PS

M13 - The Great Globular Cluster in Hercules

M13 is arguably the greatest of the Northern hemisphere globular clusters and, after Omega Centauri, the greatest globular cluster in the sky.

It is a located about 26000 light years away and has a diameter of about 120 light years.  It is one of about 250 globular clusters that surround the nucleus of our galaxy.  Most galaxies have globular clusters in orbit around them and the reason why is still unclear.  What is clear is that the clusters and the stars within them are extremely old, in the region of ten billion years old or twice the age of the sun. 

M13 is visible with the naked eye on a dark night as a fuzzy star.  A telescope reveals its starry nature and a scope over 8 inches will show many stars and is an amazing  site to behold.


M13 - The Great Globular Cluster in Hercules

The above image is a composite of LRGB data with one hour of data in each of the RGB channels and two hours in the luminance, everything binned 1x1, giving a total of five hours imaging time.  TEC 140 refractor and Atik 460 camera CCD camera with Baader LRGB filters. on MESU 200 mount.  The data was collected in 2018 and processed in PixInsight.  HDR tool makes a big impact in bringing out the detail in the core of the cluster.

TIP:  In this picture look for the "Propeller".  Can you see it? :)


M13 Annotated
M13 Annotated Version

M13 Inverted Version

NGC5982 Group

Three Galaxies in Draco


NGC5982 Group
The Draco Trio

The Draco Trio is a group of three galaxies in the constellation of Draco, The Dragon.  They are located about 120-130 million light years away.

This image was captured over the winter 2019-2020.  I used my TEC140 refractor with Atik 460 CCD and Astrodon LRGB filters.  The luminance is four hours of 15 minute exposures binned 1x1 and the RGB one hour in each filter binned 2x2. Mount is MESU200 guided with OAG with a QHY5.


Draco Trio Annotated
Draco Trio Annotated

Draco Trio Inverted
Draco Trio Inverted

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