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Horsehead Nebula in natural color emulated Narrowband


MarsG76

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Hi Astronomers,

Sharing with you another of my images... another image of one of the most popular objects imaged by astroimagers... The Horsehead Nebula/Barnard 33 with Alnitak and the Flame Nebula, but exposed mainly through narrowband filters, but emulating natural colors of the object.

I was planning to combine H-Alpha as red, OIII as green and H-Beta as blue channels to create a natural colour image through CCD narrowband filters, eliminating any light pollution or moon sky-glow in the process.
Unfortunately, the last night when I was able to do any imaging, to expose subs of this object was on the 20th February before it was cloudy every day and night with constant rain.
Having the H-Alpha and RGB data in the can, I set my exposure plan to alternate between OIII and H-Beta subs because during that night, which is luck because I only had a short window of a few hours and it turned out to be my final night of imaging for the forseeable future. I managed to get only 3 x 30 minute H-Beta and 4 x 20 minute OIII narrowband signal.

After waiting for a couple of weeks, I figured that I'm not going to get much decent time on Barnard 33 before it become obscured by landmarks so I decided to combine my currently exposed subs, H-Alpha into red, OIII into green and H-Beta into blue, as planned, and added 25% intensity from my RGB subs.

This image total exposure time was 9 hours and 32 minutes, consisting of 16 x 600 second 7nm narrowband H-Alpha, 4 x 1200 second 7nm narrowband OIII and 3 x 1800 second 7nm H-Beta with only 25% intensity added from the 14 subs each through red (180s), green (300s) and blue (600s) filters.

Taken through a 80mm Refractor @ f6.25, on a hypertuned CGEM mount with QHY268M camera.

I think that my narrowband imaging imitating natural color experiment is (once again) successful... the first time I tried this filter to channel alignment was on the Trifid nebula last August.

The advantages of exposing images through this narrowband filter to channel alignment is that most of (if not all) light pollution is rejected, imaging is possible during moon light (within reason), colors look natural, I find that more detail is captured through narrowband compared to broadband filters and narrowband filtered subs are much less susceptible to lens flares/internal reflections when there are bright stars near by or near the objects.

The only disadvantage I can think of is that the subs exposure times are a lot longer, resulting in much longer total exposure times needed to be spend on each image... although I'm starting to doubt this fact now after seeing how clean my H-Beta and OIII stack ended up being when they consisted only of 3 and 4 subs and perhaps shorter exposure time per channel will suffice?

Clear Skies,
Mariusz
 

HorseheadNebIC434 HaO3HbRGB 20Feb2022 FrmSGL.jpg

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