In search of the coalsack loop...a large but very faint ring of HII emission thought to be a supernova remnant. It was noted in 1979 but only first imaged in 1997 (see https://www.atnf.csi...alker/paper.pdf ).
I have displayed this inverted to try to match the original photo in Figure 1 and help see where to go (panels were positioned using Telescopius around Jewel box).
This image is a mosaic of 4 (now 6*) panels: In total I managed 3 hours of 6 min guided subs- battling 50% moon, low sky position and neighbours' cars- although that time is split unevenly top-bottom. I used the Samyang 135mm lens and ASI533MC (& MFT very fiddly adaptor) shot at f/2 with a fast ratio astronomik Ha 5nm filter. Vignetting at this f stop was calibrated out having first tried 10 min at f/2.8 and saw no difference. For reference the original 1997 photo used 15 min subs at f/4.5 and 1.5 nm filter.
*Latest: Added two more 1 hr panels at the top of this image where the loop turns to the right plus stars for reference; https://www.cloudyni...635_5994994.jpg
Thanks mate...it was a lot of work and to be fair its not the best image but it was more about the curiosity of it.
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SIMPLE = T / file does conform to FITS standard
BITPIX = 20 / number of bits per data pixel
NAXIS = 3 / number of data axes
NAXIS1 = 4878 / length of data axis 1
NAXIS2 = 5001 / length of data axis 2
NAXIS3 = 3 / length of data axis 3
EXTEND = T / FITS dataset may contain extensions
COMMENT FITS (Flexible Image Transport System) format is defined in 'Astronomy
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BSCALE = 1 / default scaling factor
DATE = '2023-07-27T00:20:28' / UTC date that FITS file was created
INSTRUME= ' ' / instrument name
OBSERVER= ' ' / observer name
TELESCOP= ' ' / telescope used to acquire this image
ROWORDER= 'TOP-DOWN' / Order of the rows in image array
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YPIXSZ = 3.75 / Y pixel size microns
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The 0th row is at the visual top of the image, and the 0th column is the visual left-hand side
Incredible work! Haven't seen this image anywhere else on this site, so props for the unique choice!