The Dolphin Head Nebula (SH 2-308) - 2025-01-31 - HOO Palette - Winter Star Party (Reprocessed)
Image published in the September 2025 edition of Sky and Telescope magazine.
Image:
This image is comprised of Ha and OIII band data, and for the first time I have a target where the OIII signal is far stronger than the Ha signal. In my rendering of this image that I posted a week ago, I could barely, if at all, see any evidence of the Ha in the image.
I altered my PixInsight workflow three ways to improve the original image and obtain this result. Before mapping the Ha and OIII to the RGB channels, I applied LinearFit to increase the intensity of the Ha data to match the OIII. After mapping Ha and OIII to the RGB channels, I applied SPCC, this time with Ideal QE Curve selected, and using Photon Flux for the Whte Reference. And lastly, I selected OIII as luminance when I mixed the colors in NarrowbandNormalization.
As a result of the alternate processing, I can see Ha depicted as a goldish color in the outlying wispy areas, and within the target object.
Equipment:
ZWO ASI6200MM-P/EFW 2" x 7 (HO)
TeleVue NP101is (4" f/4.3)
Losmandy G11
Software:
Captured in NINA
Processed in PixInsight
Finished in Affinity Photo
Integration:
Ha 20 x 600s = 3:20
OIII 26 x 600s = 4:20
Total integration: 7:40
The Dolphin Head Nebula (SH 2-308) - 2025-01-31 - HOO Palette - Winter Star Party (Reprocessed)
Image published in the September 2025 edition of Sky and Telescope magazine.
Image:
This image is comprised of Ha and OIII band data, and for the first time I have a target where the OIII signal is far stronger than the Ha signal. In my rendering of this image that I posted a week ago, I could barely, if at all, see any evidence of the Ha in the image.
I altered my PixInsight workflow three ways to improve the original image and obtain this result. Before mapping the Ha and OIII to the RGB channels, I applied LinearFit to increase the intensity of the Ha data to match the OIII. After mapping Ha and OIII to the RGB channels, I applied SPCC, this time with Ideal QE Curve selected, and using Photon Flux for the Whte Reference. And lastly, I selected OIII as luminance when I mixed the colors in NarrowbandNormalization.
As a result of the alternate processing, I can see Ha depicted as a goldish color in the outlying wispy areas, and within the target object.
Equipment:
ZWO ASI6200MM-P/EFW 2" x 7 (HO)
TeleVue NP101is (4" f/4.3)
Losmandy G11
Software:
Captured in NINA
Processed in PixInsight
Finished in Affinity Photo
Integration:
Ha 20 x 600s = 3:20
OIII 26 x 600s = 4:20
Total integration: 7:40