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Globular clusters, the ancient stellar cities of the universe, formed just after 'The Big Bang'. I can't remember where I read this but I was instantly hooked!
They are beautiful objects to photograph and observe. highly packed spherical agglomerations of stars, circular or oval in shape, they can look like spilt sugar on a black cotton table cloth; not that I have been many places where black tablecloths were de-rigours.
William Herschel used the name 'globular' first - from the latin globulus meaning small sphere apparently. The immense density of stars within globular clusters means that they remain bound together irrespective of whatever gravitational disturbances from the milky way or gaseous drag is occuring in the immediate galactic neighbourhood. This brightness and density means that globular clusters have a high surface brightness and so some can be easily seen through binoculars and small refractor scopes, even during moonlit nights!
Reading an article in an astronomy magazine recently, (I can't remember which one but it would have been either Astronomy Now or The Sky at Night - the only two I tend to read when I can), that globular clusters can be classified - The Shapley-Sawyer Concentration Class - a 12 step classification of the relative density of the core. I = high concentration of stars. XII = almost no concentration towards the centre!
I have been focused in recent weeks on imaging M13 in Hercules. 25,000 light years away, at a magnitude +5.8, if you are in a truly dark site like the Elan Valley, you have a good chance of seeing it with the naked eye on a moonless night. Edmond Halley who discovered it in 1714 said "this is but a little patch, but it shows itself to the naked eye when the sky is serene and the Moon absent".
How can you find M13?
M13 sits just outside the largest edge of the keystone asterism in the constellation Hercules. Use the stars Vega and Arcturus to lead your viewpoint to this keystone star pattern - a large uneven square of four stars, found about a third of the way from Vega to Arcturus. M13 will be a third of the way along the longest edge of the square between the stars Eta Herculis and Zeta Herculis.
What equipment have I been using to image M13?
- Zenithstar 61ii with field flattener
- Canon 800D astro-modded DSLR
- ASIair mini
- ZWO 120mm mini guide cam
- RVO 32mm guide scope
- EQM-35-Pro mount and tripod
- Celestron Lithium Pro power tank
- small power bank to power dummy battery for DSLR
- sharp images with pinpoint stars
- a good halo of stars around the core
- no blown out stars or oversaturated ones
- no blown out core
- Stacking of Lights and calibration frames in SIRIL to gain results file
- Siril - open results file - select 'histogram' on bottom menu - right click on image and CROP. Save as resultscrop.fits
- background extraction (at 15% in bottom menu and smoothing at 1.0 using AI
- save as 32 bit fits file resultscropBge or some such name
- image processing - star processing - click on cog icon
- now click on stars icon - tick amplitude box - enter new values into amplitude boxes (I use 0.1 to 0.7)
- click star icon - a list of stars should appear in the dialogue box - keep this box open - drag it to one side
- image processing (top menu) - deconvolution - PSF from stars - generate
- In the PSF box - the star should be within the box with black space around it - if the star is going outside the box alter the PSF values by increasing them - keep generating and altering the values until the star generated fits within the box with black around it.
- Close the PSF box that you dragged to one side
- On remaining dialogue box open (the deconvolution box), experiment with the iterations gradient settings - and when happy - click apply
- image processing - colour calibration - PCC
- image processing - green noise removal
- image processing - star processing - starnet++ removal
- load the starmask result image (for globular clusters ignore the starless image that has been generated - we don't need it)
- open new image - the starmsk image just generated in SIRIL
- now complete a denoise (using AI)
- save as 32 bits fits file
- Check that you have image in Linear mode on bottom menu.
- image processing - GHS histogram stretch - take the local stretch intensity slider across to max
- use mouse to zoom closer into the cluster on the image
- now move stretch factor slider on GHS box across to right until stars are just appearing - apply
- image processing - GHS histogram stretch 2 - Local intensity stretch slider 2/3rds way across to right - now apply tin amount of stretch slider - zoom into image to look for artifacts in surrounding stars - move slider back to eliminate these - ensure not blowing out the globular cluster core - click apply when happy
- you can apply a saturation stretch now - top right hand corner menu on this second GHS histogram dialogue box). Do very tiny adjustments to saturation
- save as tiff file if opening in affinity photo
- I open the image in camera raw editor and then make subtle edits. be prepared to mask the core so you can work on the background first; and then the reverse, masking the background to work on the core



