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Click the image for a 75% size view. (2400 x
1600 - 0.99 MB)
Instrument |
12.5" RCOS @
~ f/9 (2880 mm fl) at 0.64 arcsec/pixel. Shown at 0.85 and 1.77 arcsec/pixel. |
Mount |
Paramount ME |
Camera |
SBIG STL-11000 w/
FW8 filter wheel & AstroDon Gen-2 LRGB filters. |
Acquisition Data |
11/8/2016 to 11/14/2016 Chino Valley, AZ. with CCD Commander & CCDSoft. AOL
guided |
Exposure |
RGB |
540 min (12 x
15 min. each) Bin 1x1 |
eXcalibrator RGB ratios are 1.00,
0.99 & 1.16 |
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
108 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, data reject and combine the sub exposures, create the RGB image
and apply a mild Positive Constraint deconvolution.
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PixInsight for
gradient removal, non-linear stretching with HistogramTransformation.
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PhotoShop for the final touch-up.
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Comment |
The cluster is shown
rotated 120° counter-clockwise.
M2 is a globular
cluster in the constellation of Aquarius. Its actual position in the
galactic halo places it in the southern galactic cap, almost
directly beneath the southern pole of our Galaxy, the Milky Way, and
at a distance from us of around 47,000 light-years.
M2 is a compact and fairly dense globular cluster. It is one of the
richer globulars, containing more than 100,000 stars and stretching
more than 150 light-years across. Like other globular clusters, M2
is made up of stars that are all the same age. These are amongst the
oldest stars in our Galaxy, at an age of about 13 billion years.
Source:
NOAO/AURA/NSF.
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