Pacman (NGC281); Close-up (HOO tri-color)

Pacman (NGC281); Close-up (HOO tri-color)
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Pacman (NGC281); Close-up (HOO tri-color)

Narrowband data from summer of 2021, Almeria Spain observatory. Only used Sii, Ha, Oiii (no lum) data for the final image. NGC 281, IC 11 or Sh2-184 is a bright emission nebula and part of an H II region in the northern constellation of Cassiopeia and is part of the Milky Way's Perseus Spiral Arm.
SPECIFICATIONS
Telescope ..........................................................................................................................................................................................................................
Telescope
SPA-1 Takahashi FSQ-106ED (106 mm) F3.6
Camera ..........................................................................................................................................................................................................................
Camera
FLI PL16803 (CCD)
Location ..........................................................................................................................................................................................................................
Location
Almeria, Spain
Date of observation ..........................................................................................................................................................................................................................
Date of observation
Summer, Fall 2021
Filters ..........................................................................................................................................................................................................................
Filters
Sii, Ha, Oiii
Processing ..........................................................................................................................................................................................................................
Processing
Pixinsight, Paintshop Pro
Credits ..........................................................................................................................................................................................................................
Credits
Dev (Dave) & Judy Prana, using Telescope Live data
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