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Monday, October 24, 2011

Info Post










I made a test, how image resolution gets effected by a stacking algorithm. When images are registered, they are moved and rotated by a fraction of the pixel accuracy. Depending on used algorithm, there will be some level of blurring in a final stacked image. In this test, CCDStack software is used to calibrate, register and stack the raw-images. Two similar processing are made from the same material, one with normal workflow and the second with images scaled up 200%. 







This is a 100% animated crop from images, stacked from a 100% size and 200% size calibrated frames.



10 x 1200s H-alpha with a QHY9 camera and the Tokina AT-X 300mm camera lens at f2.8.


"Mitchell" algorithm is used for up scaling all of the 200% sized frames.





An animation from a single, cropped and 400% up scaled, 1200s H-alpha exposure.

One image is registered and second not. HWFM in none registered image is 1,6 and in registered 2,4.

Method of register is most commonly used Bicubic B-spline.








Specially, if image are undersampled, like in this example, the blurring effects gets stronger and there is a risk to loose some of the finer details.

Down side of up scaling images to 200% large, is the needed amount of computer power and memory! Images will be four times large in file size. In this case a single frame, saved as a 16bit TIFF, will be about 130 MB.

CCDStack will use much more memory per image since images are internally processed as a 32bit floating point image space. All post processing in PhotoShop is done to a 200% sized version.



I have reprocessed Sh2-119 images with a new method, original versions can be found here: http://astroanarchy.blogspot.com/2011/10/sharpless-119-sh2-119.html






Sharpless 119


In constellation Cygnus, Ra 21h 18m Dec +44 00'








Image is in Natural color palette from the emission of ionized elements, 





R=Hydrogen + Sulfur, G=Oxygen and B=Oxygen + Hydrogen.


(Looks much like a wide screen version of the "Rosette Nebula".)











HST-palette from an emission of ionized elements, R=Sulfur, G=Hydrogen and B=Oxygen.





















Technical details:





Processing work flow:


Image acquisition, MaxiDL v5.07.


Stacked and calibrated in CCDStack2.


Deconvolution with a CCDStack2 Positive Constraint, 33 iterations.


Levels, curves and color combine in PS CS3.





Optics, Tokina AT-X 300mm camera lens at f2.8


Camera, QHY9

Guiding, Meade LX200 GPS 12" and a Lodestar guider


Image Scale, 3,5 arcseconds/pixel


Exposures H-alpha 10x1200s, binned 1x1O-III 3x1200s, binned 3x3


S-II 3x1200s, binned 2x2


Total exposure time ~5h











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