Large Magellanic Cloud SHO V2

Large Magellanic Cloud SHO V2
0

Large Magellanic Cloud SHO V2

New version of the LMC mosaic, using Astro Pixel Processor's mosaic stacking. This allowed a final, higher resolution image. Each of the 8 panels was stacked using PixInsight and background modelled with GraXpert AI. After mosaic stacking with APP, PixInsight was used for post processing.
SPECIFICATIONS
Telescope ..........................................................................................................................................................................................................................
Telescope
Takahashi FSQ-106ED
Camera ..........................................................................................................................................................................................................................
Camera
QHY 600M
Location ..........................................................................................................................................................................................................................
Location
Heaven's Mirror Observatory, Australia
Date of observation ..........................................................................................................................................................................................................................
Date of observation
Observation Bundle
Filters ..........................................................................................................................................................................................................................
Filters
SHO
Processing ..........................................................................................................................................................................................................................
Processing
PixInsight WBPP GraXpert, APP Mosaic, GHS BXT NXT SXT
Credits ..........................................................................................................................................................................................................................
Credits
Ian Baber.
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