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Click the image for a 75%
size wide field view. (3006 x 1691 - 2.18 MB)
Instrument |
12.5" RCOS @
~ f/9 (2880 mm fl) at 0.64 arcsec/pixel. Shown at 0.64 and
0.85 arcsec/pixel. |
Mount |
Paramount ME |
Camera |
SBIG STL-11000 w/
FW8 filter wheel & AstroDon Gen-2 RGB filters. |
Acquisition Data |
8/6/2020 to
8/11/2020 Chino Valley, AZ. with CCD Commander & TheSkyX. AOL
guided |
Exposure |
RGB |
435 min (29 x
5 min. each) Bin 1x1 |
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Software & Processing Notes
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CCDStack,
PixInsight, Photoshop CS6.
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eXcalibrator
v6.2 for (g:r),(b:r)
color balancing, using 704 stars from the Pan-STARRS database.
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CCDBand-Aid to repair
KAI-11000M vertical bars.
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CCDStack to
calibrate and normalize the sub exposures and moderate
sharpening with Positive Constraint Deconvolution.
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PixInsight
processing includes
CosmeticCorrection,
data rejection, mean combining the sub-exposures, create the RGB
image,
gradient removal and non-linear stretching with HistogramTransformation.
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PhotoShop for additional background neutralization.
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Noiseware 5, a PhotoShop plug-in
for background smoothing.
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Comment
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The cluster is shown
rotated 80° clockwise.
NGC 6749 is a faint
globular cluster, at a distance of about 25,000 light years, in the
constellation Aquila. The cluster is a very loosely packed with a
surface brightness of only magnitude 21.8 and is located in a rich
star field. These three conditions combine to make NGC 6749 the most
difficult globular cluster to observe visually. Surprisingly, this
was the first globular discovered by John Herschel.
The cluster has a galactic latitude of only -2.2°. So, we view it
through much dust and nebulae. This scatters the blue light, making
the cluster appear red, like the Sun at sunset. |
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