Southwest of Sadr

Southwest of SadrClick image for full size version

October 28, 2018

This image shows a part of the large cloud of nebulosity that surrounds Sadr (gamma-Cygni), about 1,800 light years away. I’ve been unable to find a specific catalogue entry for this object. It contains a few catalogued dark nebulae and vdB 130 (right of centre), but for now, I’m just calling this image “Southwest of Sadr.”  It is not far from IC 1318, and is visible at lower right in this image

Tekkies:

Sky-Watcher Esprit 150 f/7 refractor, QHY 16200-A camera, Optolong Ha, L, R, G and B filters, Paramount MX. Acquisition with TheSkyX unguided. Focused with FocusMax 4. Automation with CCDCommander. All pre-processing and processing in PixInsight. Acquired from my SkyShed in Guelph. No Moon for L, moderate moonlight for Ha, minimal moonlight for RGB, average to excellent transparency and fair to average seeing. Data acquired October 13-24, 2018.

24x10m Ha and 15x15m R, G and B (Total = 7hr45m).

Data Reduction and Cleanup
The BatchPreProcessing script was used to perform calibration, cosmetic correction and registration of all frames. LocalNormalization was applied to each filter set’s subs. ImageIntegration was used to make the Ha, R, G and B masters. DynamicCrop was used to crop all the masters identically. AutomaticBackgroundExtraction was applied to each master using default settings except box spacing of 25 and Function Degree of 2.

RGB:
Creation and cleanup:  The R, G and B were combined to make an RGB image which was processed with PhotometricColorCalibration.

Linear Noise Reduction:  MultiscaleLinearTransform was used to reduce noise in the RGB image. Layer settings for threshold and strength: Layer 1: 3.0 0.8   Layer 2: 2.5, 0.7  Layer 3: 2., 0.6  Layer 4: 1.0, 0.2  Layer 5: 0.5, 0.1.

Stretching: HistogramTransformation was applied to make a pleasing, bright image.

H-alpha:
Deconvolution:  A star mask was made to use as a Local Deringing Support image. A copy of the image was stretched to use as a range mask. Deconvolution was applied (80 iterations, regularized Richardson-Lucy, external PSF made using DynamicPSF tool with about 20 stars).

Linear Noise Reduction:  MultiscaleLinearTransform was used to reduce noise in the background areas of the Ha image. Layer settings for threshold and strength: Layer 1: 3.0 0.9   Layer 2: 2.0, 0.75  Layer 3: 1.0, 0.6  Layer 4: 0.5, 0.2.

Stretching:  HistogramTransformation was applied to the Ha to make a pleasing, bright image. 

Combining RGB and Ha:
PixelMath was used to add Ha to the RGB, using the following expressions for the R, G and B channels:
     R:  max(0.9*$T[0], 1.7*Ha)
     G:  $T[1]
     B:   iif($T[0]<Ha, $T[2] + 0.16*Ha, $T[2])

Additional Processing
Nonlinear Noise Reduction: TGVDenoise was used in L*a*b* mode to reduce noise in the background areas. A mask was used to protect low signal areas.

Sharpening: Using a mask to protect stars, background and dim nebulosity, MultiscaleLinearTransform was used to sharpen Layers 2 and 3 (strengths of 0.1 for both layers).

Contrast Enhancement: LocalHistogramEqualization was applied twice. The initial pass used a scale of 50 (max contrast 1.5, strength 0.25, 1 iteration). This was followed by a second pass using a scale of 150 (max contrast 1.5, strength 0.25, 1 iteration).

Final Steps: Background, nebula and star brightness, contrast and saturation were adjusted in several iterations using Curves with masks as required. The DarkStructureEnhance script was applied with 8 layers and a strength of 0.4. 

Image scale is about 1.15 arcsec per pixel for this camera/telescope combination.

By |2018-10-29T12:20:53+00:00October 28th, 2018|Nebulae|0 Comments

About the Author:

An avid astrophotographer who has been hunting deep sky treasures with his camera and telescope for many years now. He enjoys sharing the amazing cosmos with others.

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