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Click the image for a 75% size view. (1460 x
1706 - 1.21 MB)
Instrument |
12.5" RCOS @
~ f/9 (2880 mm fl) at 0.64 arcsec/pixel. Shown at 0.85 and 1.94 arcsec/pixel. |
Mount |
Paramount ME |
Camera |
SBIG STL-11000 w/
FW8 filter wheel & AstroDon Gen-2 LRGB filters. |
Acquisition Data |
2/1/2017 to 3/30/2017 Chino Valley, AZ. with CCD Commander & CCDSoft. AOL
guided |
Exposure |
Lum |
1575 min (102 x
15 min) Bin 1x1 |
RGB |
540 min (12 x
15 min. each) Bin 2x2 |
eXcalibrator RGB ratios are 1.00,
0.97 & 1.28 |
Software & Processing Notes |
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CCDSoft, CCDStack,
PixInsight, Photoshop CS6.
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eXcalibrator
v5.0 for (g:r) color balancing, using
38 stars from the SDSS-DR9 database.
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CCDBand-Aid to repair
KAI-11000M vertical bars.
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CCDStack to
calibrate all sub exposures and create the RGB image.
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PixInsight to
register, normalize, data reject, combine the luminance sub exposures,
gradient removal, non-linear stretching with HistogramTransformation,
galaxy core detail enhancement with HDRMultiscaleTransform and to create the LRGB image.
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PhotoShop for the final touch-up.
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Comment |
North is to the top.
These two galaxies our
designated as Arp 94, in the catalog of peculiar galaxies. NGC 3227
is the larger spiral galaxy and NGC 3226 is the smaller elliptical.
The galaxies are located in the constellation Leo, at a distance of
about 66 and 73 million light-years respectively.
The multiple looping streams are probably created by several close
encounters as the galaxies continue their gravitational dance.
Interestingly, there is a faint and nearly straight, tidal stream
extending to the south. These galaxies may have already merged, but
it will be many million years before we will, if ever, know. |
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