Barnard 228

Barnard 228
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Barnard 228

Image of Barnard 228, also known as the Dark Wolf Nebula.
Barnard 228 is part of the Lupus Molecular Cloud, some 500 light-years distant.

Image acquired with AUS-2 (Takahashi FSQ-106ED). Data from 5 one-click observations.

Total integration time 300 minutes
LRGB 15 subs of 300s with each filter
SPECIFICATIONS
Telescope ..........................................................................................................................................................................................................................
Telescope
AUS2 Takahashi FSQ-106ED
Camera ..........................................................................................................................................................................................................................
Camera
FLI PL16803
Location ..........................................................................................................................................................................................................................
Location
Heaven's Mirror Observatory, Australia
Date of observation ..........................................................................................................................................................................................................................
Date of observation
2/05 (4x) and 25/05/2022
Filters ..........................................................................................................................................................................................................................
Filters
LRGB
Processing ..........................................................................................................................................................................................................................
Processing
Astro Pixel Processor, Photoshop CC with AstroPanel Pro, Astronomy Tools, Topaz Sharpen AI and Denoise Projects 3 plug-ins
Credits ..........................................................................................................................................................................................................................
Credits
One-click observations TL
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