Rosette nebula Core (HOO tri-color blend)

Rosette nebula Core (HOO tri-color blend)
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Rosette nebula Core (HOO tri-color blend)

NGC2237 - The Rosette nebula Core, enjoy!
Full equipment details and HD version on Astrobin:
https://www.astrobin.com/qq41ry/
https://www.astrobin.com/xktlu9/
SPECIFICATIONS
Telescope ..........................................................................................................................................................................................................................
Telescope
SPA-1 Takahashi FSQ-106ED (106 mm) F3.6; AUS-2 Takahashi FSQ-106ED
Camera ..........................................................................................................................................................................................................................
Camera
QHY 600M CMOS
Location ..........................................................................................................................................................................................................................
Location
Almería, Spain and Yass, NSW 2582, Australia
Date of observation ..........................................................................................................................................................................................................................
Date of observation
Sep. 2023 thru Feb. 2024
Filters ..........................................................................................................................................................................................................................
Filters
Sii, Ha, Oiii
Processing ..........................................................................................................................................................................................................................
Processing
Pixinsight, Paintshop Pro
Credits ..........................................................................................................................................................................................................................
Credits
Dev (Dave) Prana, using Telescope Live narrowband data
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