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Click the image for a 1.38 arcsec/pixel display (1800 x 1200)
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Instrument |
12.5" RCOS @
~f/9 (2880 mm fl) 1.28 arcsec / pixel. Shown resampled to 2.21
arcsec / pixel. |
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Mount |
Paramount ME |
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Camera |
SBIG STL-11000 w/
internal filter wheel, AstroDon Filters |
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Acquisition Data |
3/15/2009 to 3/24/2009
Chino Valley, AZ |
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Exposure |
Lum
400 min (40 x 10 min, bin 2x2)
RGB
360 min (12 x 10 min each, bin 2x2) |
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Software |
CCDSoft,
CCDStack, Photoshop CS w/ the Fits Liberator plugin,
Noel
Carboni's actions and Russ Croman's Gradient Exterminator
CCDStack to register,
normalize, data reject, combine and luminance sharpen.
PhotoShop for the
color combine. |
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Comment |
North is ~ to the top, the image is rotated 25 deg's CCW
The Coma Cluster (Abell
1656) is a large cluster of galaxies that contains over 1,000
identified galaxies. Abell 1656 and the Leo Cluster (Abell 1367) are
the major components of the Coma Supercluster. At a distance of 320
million light years, the apparent extent of the cluster is three
times larger than the Moon, half of which is shown in this image.
The central region is dominated by two giant elliptical galaxies...
NGC 4874 and 4889.
Notable Object:
QSO [HB89] 1256+280 With a red shift of 2.66, this quasar is at a
distance of about 10.3 to 12.3 Billion Light Years, depending on
who's redshift calculator you use. |
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