Interstellar Maelstrom: M42

I get a warm feeling at the first view of the Orion constellation each year.  Just viewed with the naked eye, late at night against a clear black sky it is a wonderful sight that somehow seems strangely reassuring but for the astronomer and especially astrophotographers, there are many exciting targets that hold great promise, principal of which is M42 the Great Orion Nebula.  This winter my first view of Orion was last October, rising from the eastern horizon in the early morning, just as I was about to go to bed after a late-night imaging session. Unfortunately, it was more than two months before the weather relented and I was finally able to snatch an albeit brief image of the said Orion Nebula. 

M42 and other nearby diffuse & reflection nebula (M43 & NGC1975 AKA the Running Man Nebula) is one of the most famous star-forming regions, which being the brightest nebula in the northern hemisphere and just over 1,300 light years distance from Earth, can itself also been seen with the naked eye on a clear night.  To my surprise, I hadn’t imaged this beguiling object for 6-years, during which much had changed: a new mount, camera & filters + I had learned a few more processing tricks.

The Orion Nebula is a gigantic cosmic cloud of interstellar dust and gas, which is the basis for the birth of numerous new stars or a “star nursery” (see starless image below) .  Moreover, these powerful, young stars unleash vast streams of ultraviolet radiation that sculpt the nebula into a myriad of fantastic shapes, further highlighted by a red tint that arises due to the presence of hydrogen gas.  For astronomers, such activities reveal much about the processes of how stars and planetary systems are formed from collapsing clouds of gas and dust.

Known as the Trapezium, four stars tightly located at the centre of M42 are very difficult to image, because of the overpowering bright white light that obscures this area from sight.  However, for astrophotographers the elusive nature of the Triangulum is therefore considered to be the ultimate measure of a good Orion Nebula image.  To overcome this problem, the key is to image the nebula across a range of exposures, from very short to long, which can then be compiled into a single final photograph that equally captures details of bright and darker areas alike.

Although poor weather conditions limited the shoot to a relatively short integration time, I’m pleased to say that the subsequent application of various new processing techniques (*see footnote for details) has created an exciting final image, full of detail and colour, as well as the aforesaid Triangulum, that I believe does justice to this magnificent object that is surely the real star of the winter night sky. 

  • Blemish Blaster by Seti Astro – helps remove inevitable blemishes of the starless image created by StarXTerminator process, which I found much easier to use than PixInsight’s Clone Stamp mostly with better results too;
  • Star Stretch also by Seti Astro – Makes the often-tricky action of stretching star images from StarXTerminator a complete doddle;
  • Astro Image Detail by Hidden Light Photography – An excellent script that makes a great job of teasing out detail from the nebula, that results in a really exciting final image.     

 

  

 

Monkey Business

Constellation names mostly originated from ancient Middle Eastern, Greek, and Roman cultures, when they identified groups of stars and named them after their gods, goddesses, animals, and objects that were important to them.  Other world-wide groups and throughout time – Native American, Asian, and African – have also made and named similar pictures from star groups based on their cultures and related beliefs.  Given the number of stars observed when looking up into a clear dark sky, it is obviously helpful to ‘construct’ familiar patterns and adopt memorable names, which can then be used to identify areas of the sky in a way that can be easily identified by all.  I have no problem with this long and well-established convention, which despite their antiquity works just as well in the modern world but I do have an issue with nicknames.

I’ve smiled at some of the nicknames given to popular, usually deep sky objects that have been well established by astronomers, but despite the possible use of describing their form, I am increasingly finding them a distraction when considering the merit of astrophotography images: Seagull Nebula, Running Man Nebula, Pelican Nebula etc.  The problem is that they absolutely do look like the object they’re meant to depict but, like an earworm is to music, once seen they are difficult to view any other way.

With this partly in mind, for the first time in seven years I recently chose to image NGC 2174 again.  I previously used the William Optics GT81 with a modded Canon 550D DSLR camera, which resulted in an image that wasn’t too bad, except it looked like a monkey!  Given its nickname of the Monkey Head Nebula, this was to be expected but unfortunately, thereafter the picture of a monkey has remained with me ever since when I view NGC 2174 images.  The challenge on this occasion was therefore to limit the monkey’s impact on the image, thereby showing the object for what it really is – an emission nebula.

Using the same OTA but with a mono CMOS camera and a good set of filters, the new data set obtained was much improved, and with better processing experience it was time to see the monkey (or not) in a new light.  The first thing to do was present the image in an orientation that produces a more favourable perspective (less monkey like).  Using a basic SHO palette in PixInsight the initial image was promising (see below) but with an alternative PixelMath dynamic SHO palette* and then processing with autocolor script, color saturation, Russell Croman’s XT-suites and other tweaks, I was pleased to see that the monkey was nowhere to be seen in the final image (see image at the top-of-the-page), or at least to my eye.

At last, it is now possible to look at NGC 2147 and see the inherent features of this interesting emission nebula, where new stars are being born at a rapid rate. Moreover, the inner details can now be clearly viewed within, thus also showing the associated open star cluster NGC 2175 and more.  As a result of this monkey make-over, the NGC 2174 image now not only looks much better but critically, I no can longer see the ape!  Now where’s that Seagull?

 IMAGING DETAILS
ObjectNGC 2174
ConstellationOrion
Distance6,400 light-years
Size 40 arc secs
Apparent Magnitude+6.80  
  
Scope William Optics GT81 + Focal Reducer FL 382 mm f4.72
MountSW AZ-EQ6 GT + EQASCOM computer control & Cartes du Ciel
GuidingWilliam Optics 50mm guide scope
 + Starlight Xpress Lodestar X2 camera & PHD2 guiding
CameraZWO ASI294MM CMOS sensor
 FOV 2.87o x 1.96o Resolution 2.50”/pix  Max. image size 4,144 x 2,822 pix   
EFWZWOx8 EFW & 31mm Chroma HSO & LRGB filters 
Capture & ProcessingAstro Photography Tool + PHD2 + Deep Sky Stacker, PixInsight v1.8.9-1, Photoshop CS3
Image Location              & OrientationCentre = RA 6:09:39.801      DEC +20:29:12.851                         Right = North        Up = East     
*Image PI Processing: Dynamic Pixel Math  R = (O^~O)*S+~(O^~O)*H
G = ((O*H)^~(O*H))*H+~((O*H)^~(O*H))*O
B = O
ExposuresHa 36 x 300 sec (3hr), OIII 30 x 300 sec (2hr 30m), SII 32 x 300 sec (2hr 40m) Total Integration Time: 8hr 10 min     
 @ 120 Gain   30 Offset @ -15oC    
Calibration5 x 300 sec Darks  15 x  HSO Flats & Dark Flats         @ ADU 32,000
Location & DarknessFairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5-6
Date & Time25th + 26th February + 2nd March 2023 @ +19.00h  
WeatherApprox. < 3oC   RH >=65%                  🌙 +25 to +50%

Reach For The Stars

Preceding the arrival of what is for many astronomers the highlight of the year, the Orion constellation and all it’s objects, is the appearance of the majestic Pleiades open star cluster (Messier 45) in the constellation of Taurus.  The so-called Seven Sisters consists of hot blue luminous stars that formed during the past 100 million years, which are expected to last another 250 million years and can be easily observed with the naked eye even here at Fairvale Observatory (Bortle 5/6).  

I have imaged this exciting star cluster before but with astrophotography and especially iconic objects such as the Pleiades, one is always drawn back for another try.  Now armed with Chroma filters and a growing list of PixInsight skills acquired since last imaged late in 2018, I wanted to tease out more details of the fine wispy dust cloud through which the Sisters are passing and forms the signature of all good Pleiades’ images.  Furthermore, with longer exposures and total integration time greater than before, maybe I could also capture something of the abundant interstellar dust that is present across the wider background?  

I am therefore very pleased that the final image (top of the page + cropped version above) which has more than achieved these objectives and marks a significant improvement on my previous attempts – it’s always worth trying that little bit more.

 IMAGING DETAILS
ObjectM45 The Pleiades AKA Seven Sisters
ConstellationTaurus
Distance444 light-years
Size110’
Apparent Magnitude+1.6
  
Scope William Optics GT81 + Focal Reducer FL 382mm  f4.72
MountSW AZ-EQ6 GT + EQASCOM computer control
GuidingWilliam Optics 50mm guide scope
 + Starlight Xpress Lodestar X2 guide camera & PHD2 control
CameraZWO1600MM-Cool (mono)   CMOS sensor
 FOV 2.65o x 2.0o Resolution 2.05”/pix  Max. image size 4,656 x 3,520 pix   
EFWZWO x8 EFW & Chroma 31mm LRGB filters 
Capture & ProcessingAstro Photography Tool + Deep Sky Stacker PixInsight v 1.8.8-11,  Photoshop CS3, Topaz AI Denoise
Image Location & Orientation Centre: RA 03:47:03  DEC 24:03:08  Top = North   Right = West   
Exposures12 x 300 sec LRGB   Total time: 4 hours   
 @ 139 Gain   21  Offset @ -20oC    
Calibration5 x 300 sec Darks  15 x Flats & Dark Flats LRGB    @ ADU 25,000  
Location & DarknessFairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5
Date & Time6th  December 2021 @ +19.15h  
Weather & MoonApprox. <=4oC      RH >=85%          🌙 New Moon          

Reflections 2020

After starting astronomy in 2014, Watch This Space (Man) was launched shortly thereafter as a personal record of my then nascent astronomy journey.  Apart from the main blog about my progress or otherwise, links to other astrophotographers, astronomy tools, astronomy weather, scientific papers etc. can also be found on this website; I was suprised to see that to-date 152 items have been published on this site.

I always like to hear from others – comments, questions, help or just to say hello – and can be contacted via: graham.s.roberts@gmail.com  or just leave a comment at the end of any item if you prefer.

Vistor map 2020: In this most difficult of years for everyone, it’s especially heartening to see so much interest from all corner’s of the world and hope to see you and others again in 2021 – Clear Skies!

REFLECTIONS is a review of my astronomy and astrophotography during the past year, together with some thoughts on possible future developments.  

2020 Overview, Images & Goals for 2021

For the world 2020 was a year like no other.  Notwithstanding the obvious problems and dire consequences of Covid-19 for everyone, there have been surprising benefits for astronomy.  Although I am retired, under lockdown there was even more time available for hobbies.  Furthermore, as I live close to Gatwick and Heathrow airports + underneath numerous high altitude long-haul overflight paths, a massive reduction in air travel resulted in a very obvious improvement in seeing conditions, which was confirmed by guiding results.  Located in a Bortle 5 to 6 area I ordinarily achieve at best average RMS error guiding of 0.90” to 1.50”/pixel, guiding improved markedly during lockdown to between 0.50” to 0.75”/ pixel.  Of course such seeing conditions also resulted in better quality imaging itself and on a number of occasions I was able to achieve integration times of 10-hours or much more over a number of nights.  The result was better images but less of them and inevitably, a lot more cloud throughout the rest of the year!

Having previously got to grips with plate solving, using the new CdC planning function I intended to develop the use of mosaics this year.  However, such is the weather in the UK (see above) that it’s obvious to me that creating mosaics is probably not the best use of what imaging time we get.  Undeterred, during January I planned and shot a 15x panel mosaic of Barnard’s Loop in Ha-wavelength.  Unfortunately the unpredictable occurrence of patchy cloud invalidated some of the panels, though I was finally able to compile a 7x panel mosaic of the upper easterly section of Barnard’s Loop – see below.  Notwithstanding, there were lessons learned: (i) restrict mosaics to one or two panels and / or (ii) where wider view images are required use a wide FOV set-up rather than a large mosaic.

Most of my other objectives for 2020 turned out to be pipedreams e.g. a new observatory or perhaps a larger telescope or dual rig.  Despite this there were important developments on other fronts.

After eventually coming to the conclusion that mosaics were probably an unwise way to go considering UK conditions, it became clear that a suitable high-quality camera lens might produce similar coverage with less imaging time and hassle.  Thus also inspired by the images of others on the SGL Forum using such equipment, I set out to build a new rig based around the excellent Samyang 135 f2 lens.  This project remains work-in-progress but so far using the lens with a bespoke 3D printed rig and micro focuser made by Astrokraken and a modded DSLR, it’s apparent that this lens produces excellent widefield images in a relatively short time.

Initial Samyang 135 f2 set-up with modded DSLR

With the time and ‘opportunity’ afforded by lockdown throughout most of the year, I finally decided to do something about improving my processing, namely learning PixInsight.  Unfortunately the rumours were correct – it is a steep learning curve and altogether a less than user friendly software.  However, after many weeks of toil and expletives I’m pleased to say I can now process an entire image with PixInsight, the impact of which has been nothing less than profound.  However, whilst PixInsight is an excellent processing facility, I’ve come to the conclusion that it is often best used together with other process software where appropriate for specific tasks:

  • Deep Sky Stacker for calibration, alignment and stacking; the equivalent PixInsight process is just too complicated and time consuming;
  • Photoshop can be very helpful finessing colours and stretching (Levels & Curves);
  • Starnet++ is useful for creating starless images, which then help to get the best from processing nebula separately before re-combining with the stars;    
  • Topaz AI Denoise has been very effective and easy to use for noise reduction and sharpening at any point during the workflow.                      

This combination for processing has turned out to be something of a game changer and almost certainly was the most important astrophotography development of the year for me, which augurs well for 2021 and beyond. 

Favourite Images

Continuing with the theme of less is more, I imaged just 13 objects this year – of which three were experimental & three with a DSLR – but still with a total integration time of 80 hours (2019 17 objects & 65 hours, 2018: 25 objects & 43 hours).  Having worked through many of the astronomer’s favourites by now, images in 2020 consisted of: a new approach to old favourites, difficult / small objects for my equipment e.g. galaxies or less popular and widefield targets. 

I’m pleased to say that most of these images turned out well and it’s difficult to choose a favourite.  The so-called ‘favourites’ below therefore represent those images from this year that portray an important development in my astrophotography journey. More detailed reviews of these and all other images from 2020 can be found in specific articles that can be accessed using the links found below or via the Blog Index, located under the dropdown menu ABOUT.  

Heart Nebula: Although imaged in 2018, this version has been re-processed using mainly PixInsight, thus transforming the original SHO Hubble Palette image from something rather dull to one with warm, vibrant colours, as well as much great detail – demonstrating the significant impact of my new PixInsight based processing abilities.   

LBN 325: Numerous emission nebulae populate this small part of a very extensiveHII-Region, which forms an exciting LRGB image.  Processing was complex and difficult, in order to bring out exciting features that abound in this spectacular but less popular area of the Cygnus constellation. Integration time of 10-hours was obtained over three nights and is my first LRGB image processed using PixInsight.       

M63 Sunflower Galaxy:  At 12.6’ x 7.2’and apparent magnitude of +9.3,this small flocculent galaxy in the Canes Venatici constellation is a challenge for my equipment. However, with 8 hours 20 minutes exposure over three nights in April and careful processing, the all-important detail within the galactic disc is clear.  Topaz Denoise AI and Gigapixel software played an important role in maintaining the colour and delicate detail in this +50% cropped image.     

Taken from last year’s REFLECTIONS 2019:

“Although you never know, I don’t see any major breakthroughs in the coming year”.  Just goes to show what I know, fewer but better images were obtained in 2020:

RECORD CARD 2020

GoalSpecifics / ResultsOutcome
Improve image captureFurther Improvements in overall quality + much longer integration times + better guiding accuracy = less but better images.MUCH BETTER    
Better processingUsing PixInsight software combined with Photoshop, Starnet++ and Topaz Denoise AI has led to major processing improvements and much better final images.      MUCH MUCH BETTER  
Widefield ImagingInitial results from new imaging rig based around Samyang 135 f2 lens were very promising but there’s more to do.BETTER    

My main objectives for 2020 were largely fulfilled (see above), so what about 2021?

  • Imaging:  Other than maintaining the aforesaid improvements achieved over the past two years – guiding & longer integration times – two items that still need to be addressed are: (i) upgrade filters to remove star bloating and all round better images, (ii) improved focussing.   
  • Widefield: Complete Samyang-rig build and switch from DSLR to CMOS mono camera.  
  • Consolidate processing improvements: Whilst the move to PixInsight and other software was very successful in 2020, I’m still only scratching the surface of what’s possible.
  • Upgrade mono camera – there’s a new generation of colour CMOS cameras starting to appear, hopefully soon to be followed by their mono equivalents !

Hardly a year I and the rest of the world will want to remember, though more than ever astrophotography played a big role in providing relief from the trauma going on around us all. 

The major increase of integration times achieved and the use of PixInsight has proved transformative for my astrophotography and will justify returning to reimage some old favourites in future years.  I had often thought about upgrading my OTA to something bigger but given the lack of a permanent observatory here at Fairvale Observatory, combined with long periods of bad / cloudy weather, the penny finally dropped and I now have high hopes for the little wonder that is the Samyang 135 f2 lens when I complete its set-up in 2021.                

Looking back I have to be happy with my astrophotography in 2020 but more importantly, look forwards to an even better year which holds great promise building on the positive developments of the past 24-months.  Moreover, I hope for the sake of everyone that we will be able to deal with Covid-19 soon and return to something of a normal life once again.  These are big ambitions and I hope that WTSM’s Reflections 2021 will record such success.

Watch this space!

 

ASTROPHOTOGRAPHY INDEX OF 2020

To access each blog, click on the title required below highlighted in RED:

JANUARY & FEBRUARY – Jinxed: Barnard’s Loop Mosaic (+ NGC 1333 reflection nebula & LDN 1622 Bogeyman Nebula)

MARCH – Nice but Dim: Medusa planetary nebula / Abell 21

MARCH & APRIL – Return of the Lion: Leo Triplet M65, M66 & NGC 3628

MAY – Galactic Bloom: M63 Sunflower Galaxy

JUNE – Canine Capers: M51 Whirlpool Galaxy

AUGUST & SEPTEMBER – The Big Picture: First Light Samyang 135 f/2 NAN, Cygnus & Veil Nebula 

OCTOBER – Reach For The Sky: LBN 325 emission nebula

NOVEMBER – Swan Adventures: NGC 6914 reflection nebula

DECEMBER – Image Redux: HST re-processing – Pacman, Heart, Rosette, NAN & California Nebula

Image Redux

An astrophotography image is clearly the sum of its parts, which can broadly be defined as: Equipment – Image Capture – Processing.  Much attention and money is given to the first two items but it’s easy to overlook the importance of processing, I should know I’ve done it for years!  With time on my hands this year during Covid-19 & lockdown, I have at last turned my attention to this most critical of items to very good effect.  Hitherto I’ve used Deep Sky Stacker (DSS) for calibration & stacking, before moving to Photoshop for all other processing, which has usually produced satisfactory results.  However, I’ve often thought more might be obtained from the data by using more powerful software combined with an improvement of my overall skills.

On taking up astrophotography it’s a shock when first looking at the camera’s data, which will usually produce a dark almost featureless image, represented by a very narrow, steep image histogram – a graphical representation of the tone and light collected by the exposures.  This is because most of the image of the night sky will of course be dark, with precious few photons arriving from distant objects being photographed contained only within the said narrow histogram – the trick is to tease them out during processing in the so-called digital darkroom, thereby revealing the image within. 

In the right hands Photoshop is an excellent tool for post processing but it’s no coincidence that most accomplished astrophotographers are using PixInsight (PI), for good reason: it is dedicated to astrophotography, is very powerful, whilst at the same time being very flexible.  Unfortunately the learning curve for PixInsight is steep but from my recent experience very much worth the effort.  Metaphorically speaking, I’m in the foothills of using PixInsight but now with sufficient knowledge to process images from start to finish, I have already successfully tackled complex LRGB images LBN 325 and NGC 6194.  Subsequently I’ve turned my attention to re-processing old narrowband data, which first time round produced unsatisfactory results using Photoshop; this being as much the user as anything else.

Whilst PixInsight was the principal software for this re-processing, it was used in conjunction with Photoshop to achieve certain affects and other newly acquired dedicated software for specific tasks: Starnet++ to produce starless images and Topaz Denoise AI for noise reduction and sharpening. Using the HST palette in all cases, the workflow (see table at the end) was adapted for each image depending on the characteristics of the object.  Before (top) and after (below) images are shown beneath, together with links to the original blogs for more background and imaging information.

NGC 281 Pacman Nebula, August 2019:  Whilst the initial HaOO bicolour image looked good I struggled to do the same with the SHO version.  However, the transformation after re-processing with PI is, as they say – a whole new ballgame.  Vibrant colours have emerged from the previous somewhat gloomy image, together with detailed internal structures.  Although somewhat artistic in character, I particularly like the starless version which is shown at the top of the page.

IC 1805 Heart Nebula, August 2018:  Like Pacman the original bicolour processing was also successful but SHO much less so.  Re-processing has brought out warm colours and details around the inner edge of the heart-shaped nebulosity but it is the striking blue inner region which highlights Melotte-15 at the centre that steals the show.  Here fierce stellar forces associated with superhot, young open star clusters, model the adjacent dust clouds into features analogous to those of the Eagle Nebula’s Pillars of Creation.

NGC 2244 Rosette Nebula, February 2018: The Rosette was the most difficult data to re-process and therefore turned out to be the most satisfying.  Similar to the Heart Nebula, the rose-like dark nebulous outer region and bright inner edge frames the dramatic, somewhat translucent pale blue inner area.  Therein billowing, cloud-like blue nebulosity shows off various internal features, which include an open star cluster at the centre and the so-called Carnival of Animals marching across the lower right quadrant.  Altogether new processing has transformed this image into something rather special.        

NGC 7000 North America Nebula, August 2017:  Although very happy with the original SHO image processed using Photoshop, the revised version is not so much better but different.  Use of the SCNR function and subsequent PI and Photoshop colour adjustments have introduced greater detail overall, as well as produced more delicate colours, especially the diaphanous blue  nebulosity around the ‘Gulf of Mexico’

NGC 1499 California Nebula, October 2017:  In this case re-processing has brought out greater structure throughout the nebula and, to a lesser degree, improved the overall colour.  However, the nature of the object, limited integration time and relative lack of what is faint OIII and SII data has probably limited the final impact.    

Frankly I found PixInsight a complete pain to understand and use initially, however, with the help of online videos, tutorials and the recently published excellent Mastering PixInsight book, I believe the results more than justify the effort and speak for themselves; overall I’m very pleased with the outcome, which far exceeds my expectations.  Notwithstanding, going forwards I can’t see PixInsight being my only processing software (though it could be) but it almost certainly will now become my main choice for post processing, where necessary supplemented by Photoshop and other packages dedicated to specific tasks.  It’s a case of using the right tool for the job and the wider combination outlined provides much more flexibility, as well as producing excellent results.  All I need now are clear skies!

OUTLINE HST NARROWBAND WORKFLOW*

ACTIONCOMMENT
Alignment & StackingDeep Sky Stacker

NON-LINEAR PRE-PROCESSING
Dynamic Crop  All stacks
Dynamic Background Extraction (DBE)  Gradient removal
RGB Combination  SHO Hubble palette
Linear Fit   
Background Neutralisation   
Colour Calibration-1  
Deconvolution (sometimes)Not used here but can be if necessary
Noise ReductionUse ACDNR or Topaz DeNoise AI
Histogram TransformationNon-linear stretch

 LINEAR PROCESSING
Curves Transformation (CT)Preliminary to bring out colours but not too strong
Colour Calibration-2 
SCNRRemove Green Hue
Magenta star adjustmentIf present + use PixelMath script
Starnet++Separate Nebula & Stars  
(a) Curves Transformation & / or
(b) Colour Saturation
Colour punch Apply Range Mask to accentuate specific areas
Photoshop – selective coloursFurther specific colour adjustment
Re-combine starless & stars imagesPixelMath script + experiment with proportions  
Final adjustments where necessaryDBE + CT + ACDNR or DeNoise AI + Linear / Curves adjustment
 * PixInsight processing unless stated otherwise 

Reach For The Sky

In September I returned to the Cygnus constellation, popular for The North America and Veil Nebula at this time of the year but elsewhere often overlooked by astrophotographers.  In particular the vast HII-region that is located around the Deneb-Sadr area which contains an abundance of exciting imaging opportunities, this time my target was LBN325 which contains numerous Ha emission nebulae, a dark nebula and a supernova remnant. To capture these features at their best, I chose to shoot, process and then combine separate HaOO narrowband and RGB images for the first time.     

Integrating RGB data for better star colours and narrowband data for nebulosity turned out to be tricky but by removing the stars from the narrowband nebulosity and then processing the starless image before combining with RGB image manually eventually worked out well (see top-of-the-page image).  However, the narrowband and broadband data had respectively been taken either side of the Meridian without plate solving and unfortunately my manual alignment was on this occasion poor.  However, with careful cropping I was eventually able to able to align and combine each of the images, though at the cost of losing 25% of the overall field-of-view which did not overlap; see full size Ha-image below with interesting features along left and right edges which had to be cropped out to align the final narrowband and broadband images.

In addition to LBN325 there are a large number of other notable features (see Image Details table at the end & Nico Carver’s annotated image below – green outline delineates areas of my image).  In addition to the many Ha emission nebulae, the most noteworthy are the dark nebula Barnard 345 and a large section of the Supernova Remnant G082.2+53.  Some 100 light-years in total diameter, this OIII-rich feature is unfortunately too faint to be picked out in my image, which would require significantly more OIII data to be seen.  Looking further afield of the image the continuing richness of the adjoining area cannot be overstated, which is beautifully seen in Nico Carver’s accompanying image (Northwestern Cygnus by Nico Carver is licensed under a CC BY-SA 4.0 License) – an 8-pannel 46-hour mosaic!  I can only dream of such work but certainly hope to return to this area again when possible, in order to enjoy more of the exquisite objects that can be found across this truly exciting area of Cygnus.  But for now there’s another story about this image.

For some time I’ve known that I had to improve my processing skills and to this end purchased PixInsight software at the beginning of the year. Very few of the best astrophotographers do not use this processing software but PixInsight has a notoriously steep learning curve and no doubt like many others I gave up after a few days!  I can unequivocally say that PixInsight is by far the most user unfriendly software I’ve come across in nearly four decades; there’s no denying it’s abilities but the developers clearly gave very little thought to its users.  Nonetheless, spurred on by the need to improve my images and the ‘opportunity’ of more time that Covid-19 has provided us all recently, I returned to PixInsight a number of times over the summer and slowly made progress.

Cropped HaLRGB M101 practice image from scratch – using Pixel Math to add Ha has worked within the galaxy but unfortunately seems to have spread into other areas too!

Using my existing data for M101, I first spent many days working through the calibration and integration process, which can only be described as exhausting!  Undeterred and in an effort to speed up matters, I moved on to Batch Processing, which though helpful only partially assists the overall task of pre-processing and inevitably put PixInsight aside again in order to find renewed enthusiasm to continue.  From this initial experience I had already come to one conclusion – that I would not be using PixInsight for calibration and integration, continuing for now with Deep Sky Stacker and possibly later switching to either Astro Pixel Processor (APP) or Astro Art, both of which get good user reviews.

From the results of others it’s clear that PixInsight is a route to better images and there is no shortage of online tutorials and books but hitherto I’d not found one that worked well for me.    Online tutorials by Light Vortex Astronomy are an excellent learning aid but tricky to work with on screen and Harry’s Astro Shed video tutorials were also helpful but I needed a book on the matter to read, thumb through and casually refer to when needed.  Then I got lucky!

It was my good fortune that in May a new text by Rogelio Bernal Andreo (AKA ‘RBA’) Mastering PixInsight became first digitally available and then in September was published as a book. The work is divided into two well thought out and presented volumes:

  • A comprehensive, easy-to-follow and understand description of how to use PixInsight
  • A reference guide providing more in-depth information on specific PixInsight processes

The two volumes come as a boxed set, are well bound and illustrated and for the first time (from my point-of-view) form an accessible, easy to use and helpful text on PixInsight.  RBA deserves every success with this outstanding book(s) which I believe will transform the otherwise torrid experience of learning PixInsight.  Armed with RBA’s Mastering PixInsight, Light Vortex Astronomy online tutorials, Harry’s Astro Shed and a other online videos, I’m pleased to say that I am now at last able to use PixInsight for processing and LBN325 is my first image; I should also mention Shawn Nielsen’s excellent Visible Dark YouTube channel, which demonstrates a number of very useful techniques.

As my first attempt to use PixInsight for processing, I’m pleased with the outcome of LBN 325 but realise there’s still much more to learn and, aside from the framing error, it’s clear that even more integration time is needed to get the best of LBN325 and its companions.  Going forwards PixInsight and Photoshop both have their respective strengths and weaknesses and judicious use of various techniques from each is probably going to yield the best results.  For now, at least, I feel the considerable time put into learning PixInsight is starting to pay off and I’ve finally turned a corner with my processing.

 IMAGING DETAILS
ObjectLBN325 & 326 +  Barnard 345 &  SNR G082.2+5.3 DWB 156, 167, 165, 168, 170, 176,
ConstellationCygnus
Distance5,000 light-years?
Size>2o
Apparent MagnitudeNA
  
Scope William Optics GT81 + Focal Reducer FL 382mm  f4.72
MountSW AZ-EQ6 GT + EQASCOM computer control & Cartes du Ciel
GuidingWilliam Optics 50mm guide scope
 + Starlight Xpress Lodestar X2 camera & PHD2 guiding
CameraZWO1600MM-Cool mono  CMOS sensor
 FOV 2.65o x 2.0o Resolution 2.05”/pix  Max. image size 4,656 x 3,520 pix   
EFWZWO x8 + ZWO LRGB & Ha OIII SII 7nm filters 
Capture & ProcessingAPT + PHD2 +  DSS + PixInsight +  Photoshop CS3 + Topaz Denoise AI
Image Location            Centre  RA 20h 18’ 42.55”     DEC +46 25’ 03.12”        
ExposuresNB 300 sec x 53 Ha & x 38 OIII       BB 60 sec x 49 R, x 35 G & x 50 B Time: NB 7hr 58 min   BB 2hr 14 min  TOTAL 9hr  49 min   
 @ 139 Gain   21  Offset @ -20oC    
CalibrationDarks 5 x 300 sec & 10 X 60’    20 x 1/4000 sec Bias   5 x Ha & OIII Flats  10 x LRGB Flats     @ ADU 25,000
Location & DarknessFairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5-6
Date & Time9th 13th & 14th September 2020  @ +21.00h  
WeatherApprox. 15-20oC   RH <=60%                  🌙 20% waning

                             

              

Jinxed

Picture saved with settings embedded.

It seems the start of the year has been jinxed, resulting in something of a mixed bag for my astronomy but thankfully not without some positives.  A combination of illness, house decoration and some quite awful weather, really curtailed the possibility of any significant astrophotography projects.  Despite these difficulties, in the few moments that were available I have managed to carry out some useful experiments which hopefully lay the foundations for greater things the future – clear skies permitting!

Following the success of my first mosaic in 2019, I decided to undertake something more ambitious over the winter, inevitably returning to Orion – specifically Barnards’s Loop.  Unseen with the naked eye, the camera discloses the presence of this large arc of ionized gas that is approximately centered on the Orion Nebula, so large that only a conventional wide field camera lens can usually capture the entire Loop.  To obtain a higher quality image using a telescope it’s therefore necessary to create a mosaic.  With this in mind and keen to expand – physically and metaphorically – my use of the mosaic technique, Barnard’s Loop seemed a worthy object.

BLoop Mosaic PLan

I planned and compiled my previous mosaic of the Heart & Soul Nebula manually but following the recent addition of a mosaic tool to Cartes du Ciel (CdC), which importantly also integrates with my image capture software Astro Photography Tool (APT), this time I was able to plan a 14 (2×7) panel mosaic to image Barnard’s Loop (see accompanying CdC plan above) and the adjacent region.  With the ability to vary the overlap and mosaic size up to 10 x 10 panels, once constructed using the CdC mosaic planning the related data is saved to a file, which can then be imported as a series of custom objects into the Point Craft plate solving section of APT; each object is defined by its central RA and DEC co-ordinates.  Thereafter, using the plate solving function, the camera and scope are centered one-by-one on each panel for imaging, either manually or by writing a suitable script to automate imaging.

Given the size of the undertaking and difficulties with weather at this time of the year inevitably limiting imaging time, plus the strong Ha-nature of Barnard’s Loop, I chose to confine imaging to only Ha subs, which would pick-out the feature well and thus form a good basis for compiling the final mosaic.  The project started well on 3rd January when I was able to complete imaging the three panels covering the central sections of the large upper arm of the arc, unfortunately thereafter it all went downhill – mostly!

As Orion and therefore the Loop moved inexorably westwards, imaging time became increasingly restricted, further compounded by poor weather and when it was clear, poor seeing conditions.  Thus acquisition of the remaining panels became more and more difficult, with many of the resulting panels of only poor quality.  All-in all I managed to image twelve of the total 17 panels, adding three to the original plan to incorporate the lower ‘tail’ located between Saiph and Rigel.  Whilst the said panels covered the entire feature, such was the poor quality of many they could not be used to achieve the final aim of the project – a Ha-image of the entire Barnard’s Loop.

Using Microsoft’s ICE software, the upper section of the Loop came together well but I’ve not been able to incorporate the middle and lower sections which were of low-quality.  I’m quite pleased with the general outcome but consider the project has demonstrated that very large mosaics of this scale are an unlikely proposition at Fairvale Observatory given UK weather conditions and lack of a permanent a setup required to maximize imaging opportunities.  Notwithstanding, I believe up to four panel mosaics should be OK – we shall see.

Subsequently the weather was very bad and very, very wet, so unable to image I reprocessed NGC 1333 from last year, which at the time had not come out well.  I’d previously noticed that for some reason images had been exhibiting poor quality in the corners, where for no obvious reason stars showed trailing in the processed stacks – though not in the original subs. The solution, thankfully discovered via the Deep Sky Stacking Forum, was to change the Stacking Alignment setting from Automatic to Bilinear and bingo, all was well.

NGC 1333 LRGBx CropF2

NGC 1333 is a colorful reflection nebula located within the dark nebula Rho Ophiuchi, a vast area of gas and dust which is one of the closest star forming regions to the Solar System.  In order to evaluate its potential for my equipment I collected just over two hours of LRGB data in January 2019. As previously noted, at the time I was disappointed with the outcome but I now think the revised image processing indicates that with much greater integration time this object could work with more subs – watch this space.

As the bad weather continued throughout most of February there have been very few clear skies but on two such nights I managed brief imaging tests of two other January / February objects which I hope to return to in another year.  First of these was another dark nebula Barnard 22, illuminated from behind by the reflection nebula IC 2087. With total LRGB imaging time of just 1hr 24 minutes the processed image was extremely noisy but it was good to see the broad outline of B22 framed well within my FOV and suggests it too could be a viable object for another day.

Finally, with the daffodils already blooming, it was clear that winter was going to be a disappointing time for serious astrophotography, however, I was still able to attempt one final object before the winter night skies receded beyond the western horizon for another year.  Surprisingly I had hitherto overlooked this object, visually located just beyond the upper edge of Barnard’s Loop, which though difficult is fortunately also strong in the Ha-wavelength.  Lynds’ Dark Nebula (LDN) 1622 AKA the Bogeyman Nebula, describes the somewhat jinxed period I’ve experienced but this time fortuitously brought my earlier work together (x4 panel mosaic below: The Bogeyman – lower left + upper Barbard’s Loop + M78 – top right).

Picture saved with settings embedded.

Despite my best efforts I was unable to see the Bogeyman when framing the image in APT even after stretching but fortunately it still turned out well.  I noticed that most other successful images were mainly undertaken in HaRGB, however with limited time before the clouds again inevitably rolled, the few RGB subs obtained failed to add much colour to my image on this occasion.  Notwithstanding, with much greater integration time the final Ha-image holds great promise.  Furthermore, the said image could be incorporated into the upper main section of the Barnard’s Loop, together with the M78 reflection nebula, to finally make a complete and worthy mosaic image consisting of six panels – see main image at the top of the page and detailed x4 panel mosaic above.  Contrary to the name, on this occasion the Bogeyman completed the jigsaw and saved the day!

IMAGING DETAILS
Object Barnard’s Loop
Constellation Orion
Distance 1.434 light-years
Size 10o  ~300 light-years  
Apparent Magnitude 5
 
Scope  William Optics GT81 + Focal Reducer FL 382mm  f4.72
Mount SW AZ-EQ6 GT + EQASCOM computer control & Cartes du Ciel
Guiding William Optics 50mm guide scope
  + Starlight Xpress Lodestar X2 camera & PHD2 guiding
Camera ZWO1600MM-Cool mono  CMOS sensor
  FOV 2.65o x 2.0o Resolution 2.05”/pix  Max. image size 4,656 x 3,520 pix   
EFW ZWOx8 + ZWO LRGB & Ha OIII SII 7nm filters 
Capture & Processing Astro Photography Tool + PHD2 +  Deep Sky Stacker & Photoshop CS3
Image Location              & Orientation Various     
Exposures 10 x 5 x 300 sec  Ha

i.e. 25 minutes / panel or total time: 4hr 10 minutes   

  @ 139 Gain   21  Offset @ -20oC    
Calibration 5 x 300 sec Ha, OIII & SII  Darks,  20 x 1/4000 sec Bias  10 x  Ha, OIII & SII Flats               @ ADU 25,000
Location & Darkness Fairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5-6
Date & Time Panels 2, 3 & 4  January 3rd 2020  @ +21.00h

Panels 5, 6, 7, 8, 9 &14  January 18th 2020  @ +20.0h

Panels 15*,16 & 17* January 19th 2020  @ +19.45h  

*rejected

Weather Approx. 2oC   RH <=80%                  🌙 30% waning
IMAGING DETAILS
Object NGC 1333 refection nebula 
Constellation Orion
Distance 1,000 light-years
Size 6’ x 3’
Apparent Magnitude 5.6
 
Scope  William Optics GT81 + Focal Reducer FL 382mm  f4.72
Mount SW AZ-EQ6 GT + EQASCOM computer control & Cartes du Ciel
Guiding William Optics 50mm guide scope
  + Starlight Xpress Lodestar X2 camera & PHD2 guiding
Camera ZWO1600MM-Cool mono  CMOS sensor
  FOV 2.65o x 2.0o Resolution 2.05”/pix  Max. image size 4,656 x 3,520 pix   
EFW ZWOx8 + ZWO LRGB & Ha OIII SII 7nm filters 
Capture & Processing Astro Photography Tool + PHD2 +  Deep Sky Stacker & Photoshop CS3
Image Location              & Orientation Centre  RA 03:29:07 (23?)      DEC 31:28:14  @ +19.16h                     

Top = North     

Exposures 6 x 300 sec  L&B 7 x 300 sec R&G

Total Time: 2hr 10 min    

  @ 139 Gain   21  Offset @ -20oC    
Calibration 5 x 300 sec Ha + 10 X 300’ RGB  Darks,  20 x 1/4000 sec Bias  10 x  HaRGB Flats               @ ADU 25,000
Location & Darkness Fairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5-6
Date & Time 28th January 2020  @ +19.15h  
Weather Approx.?       RH <=?                 🌙 9% waxing
IMAGING DETAILS
Object Lynds’ Dark Nebula (LDN) 1622  AKA Bogeyman Nebula
Constellation Orion
Distance 500 light-years
Size 1o   ~10 light-years?
Apparent Magnitude ?
 
Scope  William Optics GT81 + Focal Reducer FL 382mm  f4.72
Mount SW AZ-EQ6 GT + EQASCOM computer control & Cartes du Ciel
Guiding William Optics 50mm guide scope
  + Starlight Xpress Lodestar X2 camera & PHD2 guiding
Camera ZWO1600MM-Cool mono  CMOS sensor
  FOV 2.65o x 2.0o Resolution 2.05”/pix  Max. image size 4,656 x 3,520 pix   
EFW ZWOx8 + ZWO LRGB & Ha OIII SII 7nm filters 
Capture & Processing Astro Photography Tool + PHD2 +  Deep Sky Stacker & Photoshop CS3
Image Location              & Orientation Centre  RA 05:55:38      DEC 01:59:40  @20.49h                     

Image rotated 180o for presentation Top = South     

Exposures 19 x 300 sec  Ha, 4 x 300 sec RGB

Time: Ha only 1hr 35 min   Total 2hr 35 min   

  @ 139 Gain   21  Offset @ -20oC    
Calibration 5 x 300 sec Ha + 10 X 300’ RGB  Darks,  20 x 1/4000 sec Bias  10 x  HaRGB Flats               @ ADU 25,000
Location & Darkness Fairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5-6
Date & Time 17th January 2020  @ +20.50h  
Weather Approx. 16oC   RH <=75%                  🌙 29% waning

 

 

Reflections 2019

The website Watch This Space (Man) began in 2015 as I started out in astronomy and is a record of my personal journey, comments and thoughts.  Apart from the main blog, the website also contains links to other astrophotographers, astronomy tools, astronomy weather, and scientific papers etc., which can be accessed from the top menu.

Whilst there is a photo gallery of my work in this website, an overview of the better images can be found in the My Astrophotography FLICKR album, which can be found in the GALLERY menu.  Furthermore, this year I took the plunge and joined the Astrobin community, where my images can be found using the appropriate link also in the GALLERY menu.

Heat Map 2019

During the past year the site was visited from 64 different countries, literally from every corner of the world.  I always like to hear from anybody out there – comments, questions, help or just to say hello  – and can be contacted via details given in the ABOUT menu section or just leave a comment on any item if you prefer.

Reflections 2019 BannerX

Reflections is compiled at the end of each year as a review of my astronomy and astrophotography during the previous twelve months, together with some thoughts on possible future developments.

Overview, Images & Goals for 2020

The past year’s plan was simple: build-on and experiment with developments from the previous year, in particular using Plate Solving to achieve longer integration times and explore further the north sky, which I could now see from the new Shed Observatory and operates during the spring and summer months.

By routinely using Plate Solving integration times, now obtained over a number of nights or even months, have increased by up to four-fold compared to previous years.  As a result I concentrated on less objects but for longer time, achieving between 6 to 8 hours of subs on some occasions, the limiting factor as ever being British weather.  Although quite modest compared to those able to use fixed observatories, or in clear, dry climates with Bortle 1 or 2 skies, I was very pleased with the positive impact this had on my images.

Starting astronomy and astrophotography somewhat late in the day a few years ago, like many others after retirement, the learning curve was steep and often frustrating.  There were times I’ve almost considered giving up but with perseverance I’ve made progress and often get great pleasure from some of the results, as well as just enjoying and learning about this wonderful subject.  For me it is just a hobby but recognising some of my achievements and abilities acquired since starting out in 2014, I was especially proud this year to be elected a Fellow of the Royal Astronomical Society.  For all the help in reaching this point, I’d like to thank all those who have helped me from the astronomy community, wherever they are.

RAS logo

Favourite Images

My weakness in astrophotography remains processing but having at last obtained some good integration times, this year I made a greater effort to improve these techniques – with some success.  Adopting the theme less is more, I imaged just 17 different objects this year – of which nine were full narrow or broadfband images, with the rest being  experimental or DSLR – with a total integration time of 65 hours (2018: 25 objects & 43 hours).  The resulting images turned out well, achieving Picture of the Week on the British Astronomical Association website on six occasions.  It’s therefore difficult to choose favourites from this select group based on merit alone, so this year’s favourites (see below) represent those good images that also mark a significant milestone in my astrophotography.  Detailed reviews of these and all other images from 2019 are discussed in dedicated articles that can be found via the Blog Index under the ABOUT dropdown menu.

SHO2 CompF (Large)

Horsehead & Flame Nebula: Usually imaged in LRGB broadband, this narrowband SHO version produced a very different affect and colours, whilst also showing the beauty of the accompanying clouds of interstellar gas and dust.  Taken over three nights, at nearly 7-hours, this image was also one of my longest integration times to date.     

M101 HaLRGB final Closeup

M101 Pinwheel Galaxy: Given Bortle 5-6 skies, being on the Gatwick Airport flightpath and a using a small refractor, I struggle to image galaxies and often LRGB images in general from Fairvale Observatory.  However, on this occasion the combination of 5-hours HaLRGB subs and new processing techniques to enhance the colours, M101 proved the exception and is perhaps my first decent classic spiral galaxy imaged from home.  Moreover, the HII regions light up along the spiral arms with the addition of Ha wavelength, producing a dazzling and dynamic image. 

Picture saved with settings embedded.

Heart & Soul Nebula:  Combining existing data from 2018 of the Heart Nebula and new 2019 data of the Soul Nebula + the intervening space, this is my first albeit modest mosaic, which promises to open up significant possibilities in the future. 

RECORD CARD – 2019
Goal Specifics / Results Outcome
Improve broadband and narrowband imaging

 

Achieved major increase of image integration times and overall quality. MUCH, MUCH BETTER

 

Improve processing Continuing to make slow improvements, with greater use of new Photoshop techniques. BETTER

 

Expand & Improve Widefield Imaging Despite some good images of the Milky Way in the USA, I never used the Vixen Polarie tracking mount and did not make it to any other dark sky sites  = disappointing. FAILED

 

My objectives in 2019 mostly went well in (see above), so here goes for 2020:

  • Imaging: There’s always scope to improve imaging techniques but probably most of all I still need to improve guiding quality and increase exposure and image integration times even further.
  • Mosaic: Expand the use of mosaic imaging using Plate Solving and new CdC planning software.
  • Improve processing: I expect this will continue to be something of a challenge for some time to come unless I go to the dark side and adopt software such as PixInsight & / or APP.
  • New Observatory: Unfortunately this will not be a fixed obsy whilst I continue to live here at Fairvale which is unsuitable.  However, I’m hopeful that another location between the Main (North) Observatory and the Shed Observatory might open up the north sky better and by getting away from the high hedges that surround the garden allow longer imaging sessions than can be currently obtained at the Shed.
  • Other: My mind is always thinking about larger telescopes or a dual rig and / or a new high-end encoded mount but probably not until I make further progress with the above goals and / or move to a better dark sky location – dreaming is part of astrophotography = watch this space!

Although you never know, I don’t see any major breakthroughs in the coming year but more of the same – revisiting familiar objects in order to obtain new image versions based on greater integration time and hopefully using mosaic techniques to build-out images in order to encompass wider areas of the sky.  This year I was surprised to discover objects that I had hitherto considered out of reach from my location (M101, M51 etc.), as well as exciting features that were completely new to me and still hold great promise e.g. DWB 111 AKA the Propeller Nebula.

Looking back I’m very happy to say 2019 was an excellent year for astronomy and astrophotography, almost certainly my best yet.  You can’t ask for more than that and I hope that WTSM’s Reflections 2020 will record further such success.

Watch this space!

wtsm logo

 

2019 CHRONICLE 

Below is a quarter by quarter summary of my astronomy and astrophotography for the year, followed by an imaging record.

JANUARY TO MARCH

Towards the end of 2018 I decided to undertake a project, with the prime objective to gather a much longer period of integration than hitherto achieved by using my newly developed skill of Plate Solving.  I’d previously imaged the Horsehead and Flame Nebula in the more traditional colour palette, either with a modded DSLR or by LRGB broadband.  However, I’d recently seen this iconic image undertaken using the Hubble Palette to great affect and was inspired to do the same myself. Thereafter, for more than 2-months the clouds rolled in and I thought my project would then be impossible, not least because by now Orion had crossed the Meridian in the early evening and imaging times were at best limited.  But as is often the case with astrophotography everything suddenly changed and it was game on!

The first evening of clear skies since 11th November 2018 coincided with the full lunar eclipse on 21st January, which I was therefore able to image once again.  Then six days later a very untypical clear and quite warm period of weather arrived and I was able to complete my intended project after all, with further time to image both the Great Orion Nebula and the reflection nebula M78 + Barnard’s Loop (see images below).

HaLRGB2FINALcrop (Large)

Combined +180 degrees 3+5min HaLRGB (Large)

Achieving much longer integration times of between 5 and nearly 8-hours, the impact on the resulting images was transformative.  I was especially pleased with the outcome of the Horsehead project in SHO (see Favourites Images section) but found the Ha-only starless version of the same scene (see below) particularly mesmerising, as the large HII structures throughout this region bring the image to life.

NGC 2024 Ha Starless2

By the end of February the night sky at 51o latitude has moved inexorably on to the so-called Galaxy Season, which provides something of a dearth of imaging opportunities for my 81mm telescope.  However, with a good patch of weather at the end of March, whilst experimenting with the Leo Group I noticed that small areas of Ursa Major region could be seen directly above for a couple of hours, which to my surprise opened up a whole new world of possibilities hitherto considered unavailable.  Shortly after I managed to obtain almost 5-hours of data on M101 the Pinwheel Galaxy, which is one of my best galaxy images taken from Fairvale Observatory (see Favourite Images section).

APRIL TO JUNE

Having discovered the albeit limited possibilities of seeing Ursa Major, I moved to the Shed Observatory early in April, which by then afforded slightly better views of the same area of sky and thereby to my great joy provided the possibility of imaging the wonderful Whirlpool Galaxy, M51.  Unfortunately time was somewhat limited but it was better than nothing and I was thrilled to obtain an image of this wonderful object for the first time.  Weather permitting I’ll be back for more data in 2020 with which to build on the promising result obtained this year.

LRGB Image FINALX2 (Large)

By the end of April just 8-weeks away from the summer solstice astronomical darkness is in short supply.  Fortunately having moved earlier to the Shed Observatory this year, I was in a good position to return to inaging the Bodes and Cigar Galaxies (see below), which had been my first ever image of north sky objects in 2018.

LRGBFinal (Large)

JULY TO SEPTEMBER

From May until late July the absence of Astronomical darkness makes astronomy difficult and frankly having progressed from the time of being a beginner, it is quite refreshing to take a break.  Therefore it was only after an evening viewing the partial eclipse on 16th July and a brief experiment with the Wizzard Nebula (something for the future) at the beginning of August, that much later I returned to astrophotography seriously.

SHO2SCcrop (Large)

Having messed up imaging the Soul Nebula with poor framing in 2018 and being at the Shed Observatory, I decided to re-image the Soul properly, together with some of the adjacent sky in order to combine the new data with last year’s adjacent Heart Nebula to form a mosaic of both objects.  I don’t know why but this was my first attempt at a mosaic.  Only very recently has integrated software for mosaic planning combining  Cartes de Ciel and Astrophotography Tool for image capture has been released.  However, on this occasion I planned and implemented the said mosaic imaging manually, with a satisfying outcome (see Favourite Images section) but with the new software now available I hope to embark on more extensive mosaic projects in the near future.

This year’s astrophotography has followed two themes, the aforementioned ‘less is more’ with the aim of producing better images using much greater integration times.  The second has been largely determined by chance, being the discovery of new objects that had hitherto either been unknown to me or considered to be out of view from Fairvale Observatory; the combination of my house, very high hedges + trees and adjacent houses obscures large swathes of the night sky.  Earlier in the year such chance had led me to the M101 and M51 galaxies and in the autumn it was first the iconic Pacman Nebula and then an exciting area of Cygnus constellation.

Pacman is not particularly large for my equipment but nevertheless produced a decent narrowband image, my last from the Shed Observatory for this year.  Not until late September did the clouds again relent for my next project that initially seemed something of a long shot but actually turned out very well.  The Propeller Nebula is located in a vast HII region of the Cygnus Constellation, which from my point-of-view was a complete surprise.  At some 25 arc seconds the nebula is again on the small side for my equipment but the complexity of the adjacent HII region transforms the wider image into something really spectacular (SHO version below), which I certainly intend to visit again next year to build on the current data and explore further afield the HII region which presents exciting possibilities.

SHO F HLVG (Large)

A subsequent long trip to the USA stopped all astronomy in Surrey but a couple of evenings out in Wyoming and Utah produced some incredible dark skies and DSLR Milky Way images (see below).  Despite the remoteness of Spilt Mountain in the UTAH section of the Dinosaur National Monument – designated a Dark Sky Area – whilst imaging at 20 second exposures only one-in-ten images were without a plane track, very sad.

IMG_2345 ComboX

OCTOBER TO DECEMBER

Prior to the arrival of Orion and other fun objects of the mid-winter night skies, imaging opportunities are sparse with my equipment but it’s been a couple of years since I last imaged M31 the Andromeda Galaxy and therefore for two evenings in late October it was time to give our neighbour the extended integration treatment.  At 7½ hours data acquisition went well but although the processed image is probably my best yet of this object, there’s room for improvement, which I suspect will require a move to more advanced processing software?

HaLRGBx5b (Large)

ASTROMINAGING RECORD 2019

No Date Type Object Name
       
1 21/01/19 DSLR Full Lunar Eclipse  
       
2 27/01/19* NB  Barnard-33 &

 NGC 2024

Horsehead & Flame Nebula
       
3 23/02/19* Combo M42 Great Orion Nebula
       
4 25/02/19* Combo M78 Reflection Nebula Orion
       
5 12/03/19 BB NGC443/444 Jellyfish Nebula
       
6 24/03/19 Combo M95/96/105 Leo-1 Group
       
7 29/03/19* Combo M101 Pinwheel Galaxy
       
8 10/04/19 Combo M51 Whirlpool Galaxy
       
9 13/04/19 BB M81 & m82 Bodes & Cigar Galaxies
       
10 16/07/19 DSLR Partial Lunar Eclipse  
       
11 02/08/19 NB NGC 7380 Wizzard Nebula
       
12 23/08/19* BB IC 1848 Soul Nebula +

Mosaic Link

       
13 26/08/19 NB NGC 281 PacMan Nebula
       
14 05/09/19* NB DWB 111 Propeller Nebula
       
15 Sept DSLR Milky Way Split Mountain Utah
       
16 22/10/19* Combo M31 Andromeda Galaxy
       
17 18/11/19 BB M74 Galaxy
       
18 18/11/18 NB SH2-240 Spaghetti Nebula
       

*multiple evenings        Combo = HaLRGB       Underlined = BAA published

POSTSCRIPT

The ones that got away – imaged but not seen in WTSM this year – warts and all

RHB_2ajelly (Medium)

I saw some wonderful narrowband versions of the supernova remnant IC 443 Jellyfish Nebula this year, in particular adopting a wider view to incoporate its sentinel-like parner stars Tejat (Mu Geminorum) left and the tripple star Propus (Eta Geminorum) right, together with the reflection nebula IC 444 in the background.  As an experiment I think it may hold promise but will require a lot more integration time to improve the quality, colour and bring out more of IC 444.

M95_96_105 (Medium)

I’ve tried the Leo-1 group (M95/96/105) before but, as they say, if you don’t succeed try again.  Unfortunately the passage of time didn’t help – I need a larger telescope to do these critters justice! 

IMG_2336 (Large)

Dinosaur National Monument – Split Mountain, Utah.  Even at this wonderfully remote location, which is one of the darkest places in the USA, passing planes still get in the way of a good image – just like at Fairvale Observatory

M74 LRGBx (Medium)

At <=10 arc minutes the spiral galaxy M74 is too much for my equipment.

SH2-240 AB combined Ha Stretch (Large)

Located between the constellations Auriga and Gemini, SH2-240, Simeis 147 AKA the Spaghetti Nebula is a very large (+3 degrees) supernova remnant but it’s very low brightness makes imaging extremely difficult.  In fact prior to and during capture in Ha-wavelength, I had no idea if it was even within the image frame.  Aggressive stretching shows that it was there but only much darker skies and probably longer exposure time is likely to produce a more viable picture. 

 

Reflections 2018

Reflections is a summary of my astronomy and astrophotography during the past year, plus some thoughts about what might happen in going forwards.  In some ways it’s a bit of a chore to compile but as it provides me with some perspective on what I’ve achieved year-to-year, I do find it to be a worthwhile exercise.

Watch This Space (Man) started in 2015 as a personal record of my astronomy journey. Notwithstanding, the blog has so far attracted 15,000 views from all over the world, including various locations in 64 countries over the past year (see map below for visitors in 2018).   I do like to hear from anybody out there – comments, questions, help or just to say hello  – and can be contacted via details in the ABOUT menu section or alternatively  just leave a comment on any item if you prefer.

 

WTSM Map 2018

 

I’m always tinkering with the website where apart from the main blog, there are also links to other astrophotographers, astronomy tools, astronomy weather, scientific papers etc.,  so even if you’re a regular visitor please take a look around from time-to-time.  Looking back I see I did not file any reports this year  under the new Astrobites section, on the other hand look out for more notable occasional image that now appears in the right-hand column under the heading Screenshot, which this year included: the Eskimo Nebula, Jupiter, the Moon & Jupiter in conjunction and Venus etc.         

Whilst there is a photo gallery of my work, for a more summary view of some of my better images there’s a FLICKR album link which is accessible from the GALLERY menu.  Following the change to mono imaging techniques in 2017, for reference each image is now accompanied by a detailed tabulation of the technical information; personally I find this information invaluable when looking at other astrophotographer’s images as a guide to settings and issues when imaging the same object myself for the first time.

Reflections Banner

Overview, Images & Goals for 2019

Since getting to grips with autoguiding in 2017, I’m pleased to say all the basic processes worked well throughout 2018, resulting in a marked improvement of individual image subs.  Long imaging times are difficult to achieve in the UK with poor skies being the norm but the successful adoption of Plate Solving this year marked a very significant breakthrough and holds great promise for ever longer integration times in the future.  Re-configuring the equipment and operating set-up in 2017 now enables operating from indoors most of the time, which apart from improving working conditions, has also made operating itself much more efficient.

I’m especially pleased that after more than 4-years astrophotography I finally manged to establish a new imaging location at the bottom of the garden this year, thereby for the first time enabling imaging of the north sky, literally opening up a new world!  For another perspective I was also fortunate to experience some excellent night skies in New Zealand, France and Cornwall during the year, which was great fun and led to some excellent images too (see 2018 CHRONICLE later in this blog).

Favourite Images

Apart from the odd DSLR shot of the night sky, my astrophotography at Fairvale Observatory in 2018 was entirely carried out with the ZWO1600MM-Cool mono CMOS sensor camera & EFW, combined with the William Optics GT81 scope, in both narrowband and broadband wavelengths.  The new camera has in every sense been a game changer and a lot more work but, in my opinion, the images this year show substantial improvement.  I also made progress using more complex processing techniques in Photoshop and improved colour and detail by combining Ha with LRGB or adding RGB and narrowband wavelengths.  With these advances I submitted a number of images to the British Astronomical Association which, I’m pleased to say, were chosen for publication on their website at various times throughout the year (see Astroimaging Record 2018 at end of blog for details).

A few of my personal favourites are shown below, in no particular order:

GR Final HaLRGB

M74 Phantom Galaxy (HaLRGB)

RGB HaOO XXX2

Rosette Nebula (HaOO) 

M13 LRGB Close-up

M13 Great Globular Cluster of Hercules (LRGB) 

Sombrero Galaxy

M104 Sombrero Galaxy (LRGB)

HHOO hlvg (Large)

Heart Nebula (HaOO)

RGB2 GxFinalX (Large)

M45 Pleiades (LRGB)

 

RECORD CARD – 2018
Goal Specifics / Results Outcome
Improve broadband and narrowband imaging

 

Improved understanding and use of the ZWO1600MM-Cool mono camera leading to better subs.  Major breakthrough with Plate Solving enabling a significant increase in image integration times and overall quality. MUCH BETTER

 

 

Improve processing Continuing to make improvements and achieving noticeably better narrowband images but with more work to do in broadband. Much greater use of various Photoshop techniques is improving detail, colours and final quality. BETTER

 

 

Expand & Improve Widefield Imaging Despite some good images of the Milky Way in the UK and NZ I barely used the Vixen Polarie tracking mount and did not make it to any dark sky sites in the UK. FAILED

 

 

I think it helps to set new goals each year, so here goes for 2019:

  • Imaging: (i) There’s lots of scope to improve imaging techniques but probably most of all I now need to improve guiding quality and then increase exposure and image integration times further. (ii) Start mosaic imaging using Plate Solving.
  • Improve processing: Despite progress, I expect this will continue to be a major challenge for some time to come. Working with Olly Penrice in France and using Steve Richards’ new book Dark Art or Magic Bullet provided lots of opportunities to learn more but I’m still considering a move to new software for pre- and post-processing – we shall see.
  • Other: (i) Widefield imaging – Since acquiring the Vixen Polarie two years ago I’ve done little more than dabble in the occasional night sky shot. Maybe just set my sights lower this year and just see what happens! (ii) Do more observing – I had been thinking of getting something bigger like a Dob for observing whilst imaging is underway but frankly now thinking just do a bit more when I can with what I’ve got.  (iii) Notwithstanding weather issues at Les Granges observatory in France, get back to at least one good dark sky site next year.

I’m very pleased to say 2018 was again very good year for astrophotography, almost certainly my best yet, which was especially defined by two positive developments that are already transforming my astrophotography and hold further promise in 2019 (I said the same last year but it’s true):

  • Starting to Plate Solve has opened up whole new possibilities, in particular: Meridian flips and multiple imaging over different nights; Mosaic imaging.
  • Fairvale Observatory South – The ability to see and image the north sky from the new location expands imaging possibilities very significantly – should have done it sooner.

You can’t ask for more than that and hope that WTSM’s Reflections 2019 will record further such success.

Watch this space!

wtsm logo

2018 CHRONICLE

Below is a quarter by quarter summary of my astronomy and astrophotography for the year 2018, followed by an imaging record.  It’s interesting but not surprising that I recorded about 50% less objects than in the previous year but, as explained, integration times have increased markedly – “never mind the width, feel the quality”!

JANUARY TO MARCH

The year started with a new perspective on astronomy – upside down!  A six week trip to New Zealand over the Christmas period produced some wonderful views of the night sky in the Southern Hemisphere. Using my basic DSLR and a GorillaPod, I was able to obtain some good images of the Milky Way, accompanied by the Large and Small Magellanic Clouds, which are unseen in the Northern Hemisphere.  New Zealand’s weather conditions and terrain also produced opportunities to see various noctilucent cloud formations, particularly on South Island (below).

IMG_9102 (Large)

Being Down Under for much of January I was unable to start astroimaging until February but it was worth the wait, which resulted in an excellent narrowband image of the Rosette Nebula with which to start the year .  From the experience and advice gained in 2017, in narrowband I now tend to stretch each Ha-OII-SII wavelength more aggressively prior to post-processing and, as a result, obtain better detail and contrast.  In this case the resulting HaOO version of the Rosette (see Favourite Images section above) was particularly good and for the first time was included on the British Astronomy Association’s website 🙂

BAA PotW

Since obtaining the ZWO1600MM-Cool mono camera narrowband imaging has been nothing less than a revelation to me.  Whilst tone mapping using the Hubble Palette produces quite spectacular and colourful results, applying the aforementioned stretching to the just the stacked Ha-wavelength subs can often result in equally exciting black and white (grey) images which show exquisite detail.  One such image taken in March was the Cone Nebula, which showed the more extensive nature of the HII-region as well as the Cone and Fox Fur Nebulae (below).

Picture saved with settings embedded.

With the passing of winter’s narrowband targets by the end of February, I moved on to broadband imaging in March.  Of all the DSO features, I am perhaps most fascinated by globular clusters but had previously obtained mixed results with a DSLR camera.  Using the CMOS based ZWO1600 mono camera, I was now able to obtain much noticeably better colour and detail of these exciting but enigmatic objects (see Favourite Images section for M13 & below for M3).

M3 LRGB Crop (Large)

I can be put-off by some of the more technical requirements associated with astrophotography and, I‘m ashamed to say, that my approach is first to – ignore it, then maybe undertake some research but do nothing, then consciously put it off again and then, when there’s absolutely no alternative – give it a try.  I am not a technophobe, quite the opposite, but often find technology and the people who design and write about it unclear to the point of making no sense sometimes or at least misleading; it seems  somewhat paradoxical that I even got onto astrophotography given these issues! Notwithstanding, when I eventually summon the courage to tackle such problems, almost always I get it to work, eventually.  Such has been the case with Plate Solving this year.

With sight lines limited by houses, hedges and tall trees to the east, south and west, I’ve hitherto had to make do with average imaging windows of up to 2-hours, either to the east or west of the Meridian and depending on the object’s declination – a lower levels  the Meridian view is itself hidden by two tall trees, obscuring up to 30o vertically and 10o either side.  Naturally these constraints limit the image integration times severely, with an inevitable impact on the quality of images, notably with higher noise, less colour and detail.  The answer of course is plate solving and during February this year I finally bit the proverbial bullet.

Since changing to the ZWO 1600MM-Cool camera I have used Astro Photography Tool (APT) for image capture and camera control, with great success.  The software is quite comprehensive and it is excellent to use, though like most software can be a little idiosyncratic in places.  This is the point where I either give-up, try other software or, as is the case with APT, turn to their excellent product Forum.  Armed with the APT manual and answers from the Forum, I soon managed to plate solve and obtain images of the Leo Triplet over two consecutive nights, which subsequently aligned and stacked well – at last!

APRIL TO JUNE

For the past year or more I’d been thinking about the possibility of moving the observatory to the end of the back garden during the spring and summer period, so as to provide a platform from which to view the northern sky, which as previously mentioned is otherwise completely obscured by my house.  The principal issue was how to operate the equipment some 30-metres away?  From the experience of others it seemed that both WiFi and Bluetooth can have big reliability issues and I am always keen to keep it simple, so for now I chose to try and use a long ethernet cable to link the operating / capture computer with a control computer indoors.

I had intended to set-up on the lawn but after I had recently extended the paving around a nearby shed in the corner of the garden, cut back some of the bushes and cleared out the shed it, was obvious that this was a preferable location; the paved base was more stable and provided a dry foundation on which to work but, furthermore, the adjacent shed could house the operating computer.  Despite successful tests indoors using an ethernet cable between the two computers and Teamviewer software, only when the equipment was set-up in position outside did I finally discover it no longer worked; I still don’t know why and the problem remains work in progress (when I can be bothered to look at it again).

Notwithstanding, it was obvious that I could instead comfortably operate the mount and camera myself from the shed and duly set about establishing what has now become Fairvale Observatory South or the Shed Observatory (see photos above); the principal observatory location by the house now becomes Fairvale Observatory North or Patio Observatory. Having established myself at the end of the garden with a not unreasonable view of the north sky over the roof of my house, I eagerly set about imaging some northern classics over the next few months.  Imaging in both narrowband and broadband I was pleased to obtain decent pictures of the Bode & Cigar galaxies and the Elephant’s Trunk Nebula before taking a break in June and July when there’s no astronomical darkness; I have imaged at this time of the year before but it’s sometimes good to take a break.

M81 B (Large)

My very first image of the northern sky M81 Bode & M82 Cigar Galaxies (LRGB)

Now I know the observatory works from this location, I plan to move there sooner in 2019 in order to spend more time with new set-up, hopefully improving on the aforementioned objects as well as trying new ones.  All-in-all the new location was a big success as well as being great fun.  Strangely I was surprised to find that the experience of guiding could be more demanding in the north sky but of course thinking about it more, as the views essentially centre on Polaris on which RA lines converge the tracking needs to be more extreme in order to move the same angular distance when compared to a southward view.  However, anxious not to upset the established settings too much, my set-up was shoddy and, as a result, guiding error was generally poor from this locality.  Next time I’ll pay more attention to this and hopefully achieve better guiding and subs.

JULY TO SEPTEMBER

After a break of nearly 8-weeks I was eager to get back to the ‘new’ observatory at the bottom of the garden.  Furthermore, much of the summer through into September was dominated by a heatwave which was accompanied by clear skies, night after night!  As a result I was able to get some very encouraging results of the Heart (see Favourite Images section above) and Soul Nebulae and finally, to my surprise, the unusual Bubble Nebula (see image below).

SHO2int3 (Large)

OCTOBER TO DECEMBER

Needless to say, once back at Fairvale Observatory North the clouds rolled in and, furthermore, suitable objects for my equipment are initially sparse at this time of the year.  Since obtaining the ZWO1600MM-Cool camera I’ve concentrated on nebulae and narrowband imaging.  Though I’ve managed a few decent LRGB images, it’s fair to say that there’s room for improvement here and therefore finished the year on M33 the Triangulum Galaxy (see below) and subsequently M45 the Pleiades.  Despite being a good size for my scope it’s become clear to me that M33 is actually a tricky object and I was not satisfied with the final image – again better guiding and longer integration next time will almost certainly help.  However, Pleiades subsequently came out well (see Favourite Images section above) but the delicate interplay of the blue star light and interstellar dust does require careful post-processing.

LRGB P2 CropXX

As it was my birthday and it’s been something of an overdue trip since first conceived in 2015, I travelled to Olly Penrice’s Les Granges Observatory at the beginning of November.  It’s a great set-up and Olly was a real pleasure to work and learn from.  As a somewhat remote location in the Hautes-Alpes region of Provence, when it’s clear the SQM values at Les Granges can exceed 22 and for the first two nights we were able to image M74 the Phantom galaxy in HaLRGB under such conditions using his TEC 140, though following some rain during the day seeing conditions were mixed on the first night.

HaLRGB mosaic (Large)

Unfortunately the clouds had followed me from the UK and for the rest of the time there we were unable to image, though it did allow me to spend some useful and enjoyable time processing with Olly.  Other than processing the M74 image and learning some new techniques, using data previously acquired by Olly and with his help, I was able to compile a wonderful 9-panel HaLRGB widefield mosaic image of the North America Nebula and surrounding region (see above).

 

Notwithstanding the mixed weather conditions, I was able to obtain my first good, face-on image of a spiral galaxy (see Favourite Images section above), which with some additional subs from Olly’s previous sessions using an 14″ ODK scope turned into a truly spectacular image (see below) of this less than popular object.

M74 ODK with TEC STARS HaLRGB Crop

 

ASTROIMAGING RECORD 2018

No Date Type Object Name
1 Jan 2018 DSLR New Zealand

 

Milky Way, Lenticular Clouds etc. 
2 09/02/18 NB NGC 2244 Rosette Nebula
       
3 11/02/18 NB NGC 2264 Cone Nebula
       
4 11/02/18 BB M44 Beehive Cluster
       
5 11/02/18 NB Abell 21 Medusa Nebula
       
6 11/02/18 BB NGC 2392 Eskimo Nebula
       
7 24/02/18 NB IC 405 Flaming Star Nebula
       
8 24/02/18 BB Moon  
       
9 19/04/18 BB M65 + M66 Leo Triplet
       
10 05/05/18 BB M3 Globular Cluster
       
11 06/05/18 BB M104 Sombrero Galaxy
       
12 06/05/18 BB M13 Globular Cluster
       
13 18/05/18 * BB M81 & M82 Bodes & Cigar Galaxies
       
14 20/05/18 NB NGC 7822 Nebula
       
15 22/05/18 NB IC 1396 Elephant’s Trunk Nebula
       
17 16/08/18 * NB IC 1805 Heart Nebula
       
18 02/09/18 NB IC 1848 Soul Nebula
       
19 03/09/18 NB NGC 7635 Bubble Nebula
       
20 09/10/18 BB M33 Triangulum Galaxy
       
21 28/10/18 BB M33 Triangulum Galaxy
       
22 2/11/18 BB M74 Phantom Galaxy
       
23 17/11/18 BB M45 Pleiades
       
24 18/11/18 BB IC 2118 Witch’s Head Nebula
       

*multiple evenings                                            Underlined = BAA published

 

Other Worlds

GR Final HaLRGB

Apart from the simple enjoyment of travel, it often opens the potential for new opportunities and experiences that more profoundly broadens one’s horizons; I’ve travelled extensively during my life which has been enriched accordingly.  Earlier this month I visited astrophotographer Oliver (Olly) Penrice at his Les Granges Observatory in the Hautes-Alps region of Provence in France, with the objectives of imaging with a more favourable dark sky and to learn from Olly’s experience.

Les Granges Location (Medium)

Situated deep in the mountains and very much off the beaten track, Les Granges is in the small (28 people) hamlet of Ètoile-Saint-Cyrice, some way from Peter Mayle’s better known Provence but nonetheless itself interesting and beautiful, with some wonderful geology to boot; after all my wife and I are also geologists.

IMG_1046 (Medium)

Area immediately north east of Etoile-Saint-Cyrice

IMG_1066 (Medium)

Spectacular monocline rock folding at Sisteron

Subject to time and conditions, I particularly wanted to image a target that could not be achieved at home, either because it cannot be seen from my location or is beyond the capabilities of my equipment. Before leaving for France I therefore researched the projected night sky at Les Granges and developed a short list of potential targets, number one of which was a spiral galaxy.  At the moment my equipment struggles with these faint fuzzies and I’ve long wished to bag a good image of a ‘proper’ galaxy.  With galaxy season still a few months off the choice was limited but it soon became clear that M74, the Phantom Galaxy would provide such a target: it is not commonly imaged, is somewhat faint and difficult to see but is a classic, face-on spiral galaxy – just right for Guy Fawkes Night on November 5th too!

M74 at les granges 051118 10pm

Olly’s imaging equipment consists of a Takahashi FSQ106Ns rig and a more suitable TEC 140 f/7 refractor, which when matched with an Atik 460 CCD camera was just the job for the proposed task.  Outstanding night skies at the Les Granges Observatory are commonplace, with SQM values in excess of 22 but it was raining when we arrived and the outlook seemed less than perfect.  Notwithstanding, the next two nights were clear in the early evening and so on the first night we managed to obtain 3-hours of RGB subs, followed by nearly 2.5 hours of Ha and Luminance data the following evening.  Whilst imaging we also spent time observing, in these conditions Andromeda Galaxy was clearly visible with the naked eye but using the 14″ Meade LX200 which Olly inherited from the late Alan Longstaff other objects such as M27 and M33 came to life in the eyepiece.

IMG_20181108_115731653 (Medium)

Does what it says on the tin – entrance to Les Granges observatory

Sadly the rain returned thereafter and this turned out to be the only window of opportunity for the rest of the week!  Thankfully Olly has a vast wealth of data that included some of M74, from which we were able to bolster our meagre data from the first two evenings of imaging the same object.

Since returning home I’ve worked on the recently acquired data again and am pleased with the resulting image, shown at the top of the page.  In particular, the addition of Ha-wavelength light has brought the galaxy to life where it highlights areas of star formation located within the spiral arms, in the form of distinctive areas of magenta coloured red spots – a characteristic sign of such activity within galaxies.  Olly also produced an alternative image by combining data from the aforesaid recent image with additional data previously taken with an ODK 14 inch scope.  This resulted in a total integration time of some 17-hours and produced a stunning image of M74 that I’m pleased to say I played a small part in (see below).

M74 ODK with TEC STARS HaLRGB Crop

It was disappointing that much of the time at Les Granges was spoilt by poor weather but I was able to use some of that time on processing techniques with Olly and just enjoying the wonderful ambiance that comes from being in such a location.  I hope to return again some time in order to enjoy the beauty of the area and the night sky that can be seen – when it’s not cloudy.  In the meantime, I’m more than pleased to catch some photons from another world of another world, which has resulted in stunning images of a spiral galaxy – at last.

  IMAGING DETAILS
Object M74 Phantom Galaxy
Constellation Pisces
Distance 30-million light-years
Size 10.5’ x 9.50’     
Apparent Magnitude +10.0
   
Scope  TEC 140   FL 980 mm   f7.00      (+ADK 14”)
Mount Mesu 200
Guiding PHD2 
Camera Atik 460 CCD  Pixels 4.50 ɥm
  FOV 43.80’ x 35.04’  Resolution 0.96”/ pixel     
Capture & Processing Atik software capture, Astroart pre-processing, PixInsight and Photoshop CS3 post processing
Image Location RA 01:36:41    DEC 15:47:01                       
Exposures 6 x 600sec RGB + 5×900 sec L & Ha  = 320 minutes  @ -20o
Location & Darkness Ètolie-Saint-Cyrice, Hautes-Alps Provence, France        SQM <=21.50 – 22.00
Date & Time 2nd & 3rd November 2018 @ +20.30h  
Weather <=8oC    RH% high