Sharpless 2-217 in Auriga

Bicolor Ha/OIII image, using Ha as luminance and RGB for stars. A starless version can be seen here.



Exposure: Total exposure time about 25.7 hours, 47 x 20mins Ha, 22 x 20 mins OIII, 23/23/30 x 2 mins RGB. All bin 1x1. Captured over 8 nights in October and November 2017.
Light pollution: Bortle 8 (white zone, NELM about 4.5)
Image scale at capture: 0.6 arcsecs/pixel = f/5.7
Scale of presentation: 1.2 arcsecs/pixel (50% reduction)

Equipment:
Scope: C11 (standard, not Edge) with Celestron 0.63 reducer
Mount: Paramount MX+, connected via ASCOM Telescope Driver 6.1 for TheSkyX, with MKS 5000 driver 6.0.0.0
Camera: SXVR-H694, connected via SX ASCOM driver 6.2.1.17140 (SX 1.2.2 also installed)
Filter wheel: Atik EFW2 with 7x1.25 carousel and Artemis 2.4.3.0 driver
Filters: Astrodon 5nm Ha/SII, 3nm OIII, Type IIe LRGB
Rotator: Optec Pyxis 2", connected via Andy Galasso's 0.4 driver (Optec Pyxis Rotator AG)
Focuser: Rigel Systems GCUSB_nStep with driver version 6.0.7
OAG: Orion Thin OAG
Guide cam: Lodestar (first generation). 4 second exposures
Automation SW: Sequence Generator Pro 3.0.0.4 beta
Guide SW: PHD2.6.3, connected to guide cam via native SXV driver
ASCOM: ASCOM 6.3.0.2831
Platesolving: PlateSolve 2, failover to local Astrometry.net 0.19 server
Collimation: Metaguide 3, using ASI120MM connected via ZWO Direct Show driver 3.0.0.2

Processing Workflow by Workspace in PixInsight 1.85

1. Calibration
BatchPreProcessing with flats, darks and bias, using Cosmetic Correction with master dark

2. Stack and Mure Denoise
Blink to preview and reject a few frames
Subframe Selector to confirm selections and weight by FWHM and SNR
Image Integration
Mure Denoise

3. Luminance Linear Processing
Dynamic Crop
Dynamic Background Extraction
Deconvolution with Dynamic PSF

4. Luminance Stretching
Histo Trans
Masked Stretch
Curves Trans
Noise Reduction with TGV Denoise and Multiscale Median (following David Ault’s Astro Imaging Channel tutorial).
Local Histogram Equalization to enhance contrast inside nebula
Deconvolution
Final TGV Denoise

5. RGB Linear Processing
LRGB Combination to merge RGB channels
Dynamic Crop (using the same icon as with luminance)
Dynamic Background Extraction
Photometric Color Calibration

6. RGB Stretching
Split luminance from RGB
Masked stretch on chrominance
Curves to boost saturation on chrominance
Histo Trans and Curves on luminance
LRGB Combination to merge luminance and chrominance
TGV Denoise

7. Color
Merged narrowband channels in PixelMath: mapped Ha to R, OIII to green, 85% OIII and 15% Ha to blue
LRGB Combination: used Ha as luminance

8. Combine
Star removal, following David Ault’s technique
With PixelMath, add starless nebula to RGB star field using range mask

9. Final
In Photoshop, clean up blue comatic halos on color layer with Radial Blur and save as TIFF
Downsize 50% and save as JPG