Very dim supernova remnant, Abell 85 in Oiii

 Abell 85 or CTB1 is a nearby supernova remnant with an apparent diameter of about a half a degree (about the same size as a Full Moon). Upon early discovery, Abell 85 was thought to be a planetary nebula, so Abell included it in his catalog of planetary nebulae as number 85. Further research showed that Abell 85 is, in fact, a supernova remnant. The deep red color that shows in white in the picture below, comes from light emitted by energized Hydrogen (Ha), but Abell 85 also has an area shining in blue/green light from energized Oxygen (Oiii) atoms. 

The surrounding Ha light has been shown to be related to CTB1 as well. CTB1 makes for a very challenging object to photograph, as it is quite faint. Without using Ha and OIII filters, the SNR is virtually invisible.

PixInsight Processing:

1. Blinked files to remove bright airplanes
2. "Subframe Selector to remove frames based on:
   PSF Signal Weight, Elongation, FWHM, # of Stars"
3. Weighted Batch Preprocessing of Lights, Darks, Dark Flats
4. WBPP Cosmetic Correction,
5. Auto Dynamic Crop from WBPP
6. AutomaticBackgroundExtraction
7. EZ processing; EZ Soft Stretch; 30%
8. StarXTerminator_NL
9. NoiseExterminator (Non-Linear)
10. Curves - Multple Slight S-Curves
11. LocalHistogramEqualization - Kernel Radius = 25
12. LocalHistogramEqualization - Kernel Radius = 75
13. LocalHistogramEqualization - Kernel Radius = 125
14. MultiscaleLinearTransform to sharpen
15. Added stars back in with PixelMath
16. Bill Blanshan's Pixel Math Star Reduction V3