IC410, Tadpole Nebula - HOO, SHO, Ha
Posted: Sat Nov 22, 2025 9:22 pm
Captured 16th & 19th November 2025. Processed as HOO, SHO, Ha - 7.8h integration for the SHO image.
HOO - Ha 15x450s, OIII 30x450s
SHO - SII 18x450s, Ha 15x450s, OIII 30x450s
Ha 15x450s
Equipment: Vixen 81s refractor, Celestron AVX mount, Vixen 0.67x reducer/flattener, Atik 314L+, Atik EFW2 9-slot filter wheel, Altair Ha (7nm), OIII (6.5nm), SII 6.5nm) filters, QHY miniguider.
Software: SharpCap, Pixinsight (Starnet++, NarrowbandNormalisation & StarReducer scripts).
Data: SII 18x450s, Ha 15x450s, OIII 30x450s; bias 100; darks 50, flats 50 each filter.
Capture: dithering used (3 pixels every frame with 10s settling time).
The exposures came from Brian's (@oopfan) minimum exposure calculations and are 1.5X minimum exposure. No over-saturated stars were observed. See viewtopic.php?t=9054
The frames were processed using drizzle_2x. This enabled the under sampled optics (camera has 6.45µm pixels, scope/reducer is F5.5) to deliver a pixel scale of 1.55 arcsec/pixel rather than a pixel scale of 3.11 arcsec/pixel thus avoiding 'square stars'.
The last couple of days have been spent in PixInsight experimenting with workflows to reduce noise - very much a work in progress.
As always, more data would improve the images.
Dave
HOO - Ha 15x450s, OIII 30x450s
SHO - SII 18x450s, Ha 15x450s, OIII 30x450s
Ha 15x450s
Equipment: Vixen 81s refractor, Celestron AVX mount, Vixen 0.67x reducer/flattener, Atik 314L+, Atik EFW2 9-slot filter wheel, Altair Ha (7nm), OIII (6.5nm), SII 6.5nm) filters, QHY miniguider.
Software: SharpCap, Pixinsight (Starnet++, NarrowbandNormalisation & StarReducer scripts).
Data: SII 18x450s, Ha 15x450s, OIII 30x450s; bias 100; darks 50, flats 50 each filter.
Capture: dithering used (3 pixels every frame with 10s settling time).
The exposures came from Brian's (@oopfan) minimum exposure calculations and are 1.5X minimum exposure. No over-saturated stars were observed. See viewtopic.php?t=9054
The frames were processed using drizzle_2x. This enabled the under sampled optics (camera has 6.45µm pixels, scope/reducer is F5.5) to deliver a pixel scale of 1.55 arcsec/pixel rather than a pixel scale of 3.11 arcsec/pixel thus avoiding 'square stars'.
The last couple of days have been spent in PixInsight experimenting with workflows to reduce noise - very much a work in progress.
As always, more data would improve the images.
Dave