RCW6 (HOO/Semi Starless)

RCW6 (HOO/Semi Starless)
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RCW6 (HOO/Semi Starless)

RCW 6 is an emission nebula in the southern hemisphere constellation Canis Major. Other names: Gum 5 and SH2-301. Over 8 hrs of LRGB data from Telescope Live remote observatory in Chile. Pre and Post processing done in Pixinsight with final touches using Paintshop pro.
SPECIFICATIONS
Telescope ..........................................................................................................................................................................................................................
Telescope
Planewave CDK24 (CHI-1)
Camera ..........................................................................................................................................................................................................................
Camera
QHY 600M (CMOS)
Location ..........................................................................................................................................................................................................................
Location
Chile
Date of observation ..........................................................................................................................................................................................................................
Date of observation
Nov. thru Dec. 2023
Filters ..........................................................................................................................................................................................................................
Filters
Lum, Red, Green, Blue
Processing ..........................................................................................................................................................................................................................
Processing
Pixinsight, Paintshop Pro, HOO norm. script, StarsXterminator
Credits ..........................................................................................................................................................................................................................
Credits
Dev (Dave) and Judith (Judy) Prana, using Telescope Live data
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