5
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Click the image for ~ 55% size
view. (2100 x
1400 - 1.08 MB)
Instrument |
12.5" RCOS @
~ f/9 (2880 mm fl) at 0.64 arcsec/pixel. Shown at 1.15 & 3.22 arcsec/pixel. |
Mount |
Paramount ME |
Camera |
SBIG STL-11000 w/
FW8 filter wheel & AstroDon Gen-2 RGB filters. |
Acquisition Data |
10/5/2017 to 10/8/2015 Chino Valley, AZ. with CCD Commander & CCDSoft. AOL
guided |
Exposure |
RGB |
480 min (32 x
5 min. each) Bin 1x1 |
eXcalibrator RGB
ratios are 1.00, 1.05 & 1.20 |
Software & Processing Notes
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-
CCDSoft, CCDStack,
PixInsight, Photoshop CS6.
-
eXcalibrator
v6.1 for (g:r),(b:r) color balancing, using
360 stars from the SDSS-DR9 database.
-
CCDBand-Aid to repair
KAI-11000M vertical bars.
-
CCDStack to
calibrate the sub exposures.
-
PixInsight to
register, data reject, mean combine the sub exposures, create the RGB
image,
gradient removal, non-linear stretching with HistogramTransformation,
color saturation and green cast removal with SCNR.
-
PhotoShop for
additional background neutralization and JPEG
creation.
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Comment
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Shown rotated 155°
clockwise.
NGC 7686 is cataloged
as an open cluster in the constellation Andromeda. It is described
as poorly populated with 50 to 80 stars. Distance estimates range
from 900 to 3000 light years. William Herschel discovered it on
December 3, 1787.
Since its discovery, like Pluto, astronomers later demoted NGC 7686.
In 1961, Johnson et al. determined that it is not a cluster. Here is
the text from their presentation in the Lowell Observatory Bulletin
No. 113.
"Our color-magnitude
diagram shows merely a uniform scatter with no significant tendency
to show a cluster main sequence; we conclude that NGC 7686 is not a
cluster."
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