Chapeau!

LRGB GxC Crop-2 (Large)

 

I always had a general interest in astronomy but was eventually sparked into action after viewing Saturn through the Thompson 26 inch refractor at Herstmonceaux observatory in 2014.  The beauty of the planet and its unique rings is captivating and like many others it remains my favourite planet to this day.  One year on and looking further afield at Joan Genebriera’s Tacande Observatory on the island of La Palma, I discovered what is now  one of my very favourite Deep Sky Objects – M104 or the Sombrero Galaxy; until recently I used the resulting picture obtained whilst at La Palma as the main banner image for this website.  Though perhaps not as spectacular as the Orion Nebula or certain spiral galaxies, the sombrero-like galaxy (with a passing resemblance of a flying saucer too), is beguiling in its own unique way and ever since then I’ve been eager to return to The Hat and image it myself from home.

Chart_1.cdc3

However, imaging the Sombrero from the UK and especially at my location just south of London is quite another matter to La Palma.  Aside from light pollution, being at 51o north compared to 28o in La Palma, M104 is considerably lower in the sky when viewed from Fairvale Observatory in Redhill; at the time of imaging in early May it was about 26o above the southern horizon.  Furthermore, my sight lines are obscured on three sides by 15-foot hedges and directly south by two 45-foot conifers – see below SE to SW view of M104 imaging track at Fairvale Observatory.

M104 Track crop

As a result, only after it emerges from behind the western edge of the aforesaid conifers can M104 (just) be imaged, as it moves along the top of the hedge for just over an hour before disappearing from view once again.  Of course this is far from ideal but with my enthusiasm for the Sombrero, a high-resolution ZWO1600M-Cool camera and newly acquired ability to plate solve, I gave it a try over three consecutive nights.

 

RGB GxC crop (Large)

 

An unbarred spiral galaxy, the hallmark of M104 is its bright bulbous centre encircled by dark dust lanes, which when viewed from Earth tilted at just 6-degrees above the equatorial plane creates the appearance of a sombrero hat (see cropped image above).  With the much higher resolution of the Hubble telescope some 2,000 globular clusters have been identified with M104, ten-times that of the Milky Way.  In 1912 the galaxy was found to be moving away from Earth at 700 miles per second, providing an early indication that the Universe was in fact expanding in all directions.

All-in-all the Sombrero galaxy is a fascinating and unusual object, though small and all-in-all a challenging imaging target, especially seen from Fairvale Observatory.  Notwithstanding, at last I am very pleased to obtain my own exciting image of the Sombrero – chapeau!

M104 Location

IMAGING DETAILS
Object Sombrero Galaxy  M104     
Constellation Virgo
Distance 29 million light-years
Size 9’ x 4’  or  50,000 light-years
Apparent Magnitude +8.0
 
Scope  William Optics GT81 + Focal Reducer FL 382mm  f4.72
Mount SW AZ-EQ6 GT + EQASCOM computer control
Guiding William Optics 50mm guide scope
  + Starlight Xpress Lodestar X2 guide camera & PHD2 control
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 + PS2,  Deep Sky Stacker & Photoshop CS2
Image Position Centre  RA 12:39:59    DEC -11:37:20  
Exposures 25 x 180 sec L + 3x5x180 sec RGB  (Total time: 120 minutes)   
  @ 139 Gain   21  Offset @ -20oC    
Calibration 10 x 180sec Darks  20 x 1/4000 sec Bias  10 x Flats LRGB  @ ADU 25,000  
Location & Darkness Fairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5
Date & Time 5h + 6th + 7th  May 2018 @ 23.30h  approx.

 

 

Spinning Plates

65 Comp Lgx Crop

Much of life is about meeting and dealing with challenges. Who hasn’t put off a task in the hope either that it will go away, somebody else will deal with it or an easier solution might be found?  Whatever anybody says to the contrary, astrophotography is not easy and throws up many such challenges from the very beginning, which will usually have to be dealt with if progress is to be made.  Amongst such challenges a few have the potential to transform the process and / or outcome of imaging but can also irrationally at first appear as a stumbling block rather than an opportunity and, as a result, get put aside until another day.

My list of such obstacles so far confronted consists of:

I have experienced many other challenges but excluding processing itself – which is another story – overcoming these four tasks has each time had a material positive impact on my astrophotography.

It’s fair to say that with technology, problems and life in general, wherever possible I like to adopt the KISS principle (Keep It Simple Stupid).  Unfortunately such a philosophy is often difficult, if not impossible to follow with astrophotography and most of the time there is just no alternative but to work through the unavoidable difficulties step-by-step in every excruciating detail, which usually requires lots of patience, perseverance and time.  In understanding and finding a solution the almost endless and invaluable online help from others should not be overlooked, without which I would probably still be back at the proverbial square one.  The availability of such friendly help and the extensive free but still excellent software is surely one of the defining characteristics of astronomy and astrophotography, which not only makes it easier but more enjoyable.

Notwithstanding, when I look back at the aforementioned list of tasks which took me months or even years to address and solve, I wonder now why I had been so daunted beforehand.  Once I found the courage to work through the problems, I discovered that I too was able to set-up and carry out such techniques that hitherto I’d thought beyond my abilities.  It was very satisfying but, more to the point, each such breakthrough took me to another level of imaging.

Ever since moving on from DSLR to using the ZWO1600mm-Cool mono camera and EFW, I realised that if I was ever going to truly master astrophotography I would need to achieve much longer integration times, which could only mean one thing – the apparently black art of plate solving.  I had read about plate solving and understood the principle but at first was too busy learning the new camera and then either just kept putting it off or, with so much bad weather, used the rare clear night just to enjoy imaging.  Notwithstanding, an all too brief warm and clear spell recently occurred and I decided to give it a try.

Aside from the innate underlying complexity of such techniques I am first put off by the instructions. I do read them but as always with technical items they appear to have been written by an alien – poorly written, idiosyncratic and altogether difficult to understand.  In this case I chose to use PlaneWave’s PlateSolve2 software incorporated within the excellent image capture software Astro Photography Tool (APT) as Point Craft and to be fair, the author’s (Ivo from Hungary) instructions are comprehensive but still difficult to understand; thankfully the related APT Forum helps enormously to resolve resulting difficulties and misunderstandings. However, like riding a bike you will not learn by reading a book but need to get on and do it!

Having installed the necessary software and star catalogues for plate solving my first night was for various reasons a disaster, thankfully the good weather continued for the subsequent two evenings and I was therefore able to continue.  To learn the technique I needed a suitable target and at this time of the year the Leo Triplet formed an easily recognisable composition that met the bill, though the detail of each galaxy remains difficult to resolve with my set-up.  My approach was first to verify I could Solve an image i.e. identify the exact RA and DEC position of the image (location and orientation) using the plate solving software and then using this image and solved data:

  1. Re-position the camera exactly over the target in the same part of the sky
  2. Do the same but after a Meridian flip, and finally…
  3. Do the same using the original image but over two nights
PoinCraft

APT PointCraft input screen: After connecting the scope, solving the image (upper box) and framing the image (lower box), the GoTo++ function can be used to return the scope and imaging location to the originally solved and framed position in order to resume imaging.

I’m not going to say I’ve cracked it but I did achieve all the above tasks and am now confident that I’m on my way to obtaining longer integration times with the help of plate solving.  After some failures I was finally able to realign the camera to within 2 pixels, which is quite amazing accuracy achieved by the software.   I was even pleased with the resulting test images, which however emphasised the aforementioned need for much greater integration times; top-of-the page image from separate image sets on 19th April, image below from image sets on 20th April.  Of course increased times will also require clear skies and a return to more suitable targets.

Picture saved with settings embedded.Despite my aversion towards much of the so-called modern world I am not a technophobe, I embrace and often enjoy many of today’s technical developments.  However, I am of the opinion that many of the problems with such technology arise at the interface between the technology and mankind – technology is now (mostly) digital and we are analogue i.e. incompatible. Furthermore, such difficulties are often compounded by the lack of intuitive operation and inability of those creating such devices or software to explain to normal human beings how to use them – surely altogether a limiting factor for the ultimate development of the modern world itself? Notwithstanding and somewhat ironically, my experience indicates astrophotography may also be a metaphor for life.  Often working in the unknown, difficult, complex and frustrating but at times very rewarding – a bit like spinning plates really? And so on to my next plate – watch this space!

Leo

IMAGING DETAILS
Object The Leo Triplet   M65 + M66 + NGC 3628     
Constellation Leo
Distance 35 million light-years
Size M65 8.7’ x 2.45’      M66 9.1’ x4.2’      NGC 3628  15.1’ x 3.6’
Apparent Magnitude M65 +10.25              M66 + 8.9             NGC 3628  + 10.2
 
Scope  William Optics GT81 + Focal Reducer FL 382mm  f4.72
Mount SW AZ-EQ6 GT + EQASCOM computer control
Guiding William Optics 50mm guide scope
  + Starlight Xpress Lodestar X2 guide camera & PHD2 control
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 + PS2,  Deep Sky Stacker & Photoshop CS2
Image Location Centre  RA 11:19:59    DEC 13:31:01  
Exposures 1.Main image  60 sec x35* LRGB  (Total time: 100 minutes)  *15 East & 10 West

2. Second image  180 sec x 5 LRGB (Total time: 60 minutes)

  @ 300 Gain  50  Offset @ -20oC    
Calibration 1.   15 x 60 sec Darks  20 x 1/4000 sec Bias  10 x Flats LRGB  @ ADU 25,000  

2.   10 x 60 sec Darks  20 x 1/4000 sec Bias  10 x Flats LRGB  @ ADU25,000

Location & Darkness Fairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5
Date & Time 19th & 20th February 2018 @ 22.00h approx.

Playing With Fire

RGB (Large)

When possible my current repertoire has continued with DSO targets previously imaged with a modded DSLR and now revisited using the ZWO1600MM-Cool camera.  In general I’ve found the outcome with the new camera has been noticeably better in detail and colour but I’m still learning and know I can do better in time.  Last imaged in December 2015 with a DSRL camera, the larger FOV comfortably encompassed both the Tadpole (IC410) and adjacent Flaming Star (IC405) nebulae, resulting in an exciting composition. However, this time the ZWO CMOS sensor could only accommodate the latter in the image but with improved resolution.

fn3

Picture saved with settings embedded.

IC 405 (right) The Flaming Star Nebula & IC 410 The Tadpole Nebula: WO GT81 & modded Canon 550D + FF | 15 x 180 sec @ ISO 1,600 & full calibration | 8th December 2015

The Flaming Star is an emission / reflection nebula, which surrounds the bright blue variable star AE Aurigae.  Imaging in narrowband produced decent Ha data but was very weak in OIII and SII wavelengths and even with 2-hours integration time is somewhat lacking in colour both in SHO (top-of-the-page) & HOO (below).  Notwithstanding, it’s an exciting object that at some point in the future will obviously require much longer imaging time and perhaps even a mosaic  in order to include its neighbour the Tadpole once again.

HOO (Large)

FN

IMAGING DETAILS
Object The Flaming Star Nebula   IC405     
Constellation Auriga
Distance 1,500 light-years
Size 37’ x 19’  
Apparent Magnitude +6.0
 
Scope  William Optics GT81 + Focal Reducer FL 382mm  f4.72
Mount SW AZ-EQ6 GT + EQASCOM computer control
Guiding William Optics 50mm guide scope
  + Starlight Xpress Lodestar X2 guide camera & PHD2 control
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,  Deep Sky Stacker & Photoshop CS2
Exposures 300 sec x12 Ha, x6 SII & x6 OIII (Total time: 120 minutes)
  @ 139 Gain  21 Offset @ -20oC  
Calibration 5 x 300 sec Darks  20 x 1/4000 sec Bias  10 x Flats Ha, OIII & SII @ ADU 25,000  
Location & Darkness Fairvale Observatory – Redhill – Surrey – UK        Typically Bortle 5
Date & Time 24th February 2018 @ 20.30h approx.