Monday, October 31, 2011
Veil Nebula as an anaglyph Red/Cyan 3D
3D-NOTE!
You'll need Red/Cyan Eyeglasses to be able to see images as 3D.If you have a Red and Blue filters, you can use them! Red goes to Left eye.
Original 2D:
Sunday, October 30, 2011
Veil Nebula, a supernova remnant
Veil Nebula
Supernova remnant in constellation Cygnus
Note. Image is updated at 27.03.2012 with a new data, it was buried in my hard disk.
R=Hydrogen + Sulfur, G=Oxygen and B=Oxygen + Hydrogen.
Image is not as deep as I wanted but the weather has been working against me for a long time now...
Veil Nebula is a cloud of ionized gas and dust, leftovers from an exploded star. The star exploded some 5000-8000 years ago at distance of about 1470 light years. This, relatively faint target, is difficult to image due the large angular diameter, about three degrees, and a dense star field.
This is a second version of this object, older version can be seen Here. I have made a 3D-animation about the possible shape of this SNR, it can be seen Here.
HST-palette, from the emission of ionized elements,
R=Sulfur, G=Hydrogen and B=Oxygen.
1:1 cropped image to show the resolution.
Not a bad one for the 200mm camera lens...
Technical details:
Processing work flow:
Image acquisition, MaxiDL v5.07.
Stacked and calibrated in CCDStack2.
Deconvolution with a CCDStack2 Positive Constraint, 33 iterations, added at 50% weight
Levels, curves and color combine in PS CS3.
Optics, Canon EF 200mm camera lens at f1.8
Camera, QHY9
Guiding, Meade LX200 GPS 12" and a Lodestar guider
Image Scale, ~5 arcseconds/pixel
New exposures H-alpha 13x1200s,
S-II and O-III information are from an older image
Monday, October 24, 2011
Image processing test with Sharpless 119
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%.
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.
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.
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.
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
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
Wednesday, October 19, 2011
IC 1396 as a Stereo Pair 3D
Parallel vision 3D
Cross vision 3D
Other 3D-formats:
Original 2D:
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