Pacman (NGC281); Widefield (SHO)

Dev Prana

Starless

Pacman (NGC281); Widefield (SHO)

Narrowband data from summer of 2021, Almeria Spain observatory. Only used Sii, Ha, Oiii (no lum) 23 hrs of 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. Full details on Astrobin:

https://www.astrobin.com/ez4oq7/B/

SPECIFICATIONS

Telescope ..........................................................................................................................................................................................................................

SPA-1 Takahashi FSQ-106ED (106 mm) F3.6

Camera ..........................................................................................................................................................................................................................

FLI PL16803 (CCD)

Location ..........................................................................................................................................................................................................................

Almeria, Spain

Date of observation ..........................................................................................................................................................................................................................

Summer 2021

Filters ..........................................................................................................................................................................................................................

Sii, Ha, Oiii

Processing ..........................................................................................................................................................................................................................

Pixinsight, Paintshop Pro

Credits ..........................................................................................................................................................................................................................

Dev (Dave) & Judy Prana, using Telescope Live data