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Click the image for a higher
resolution
view. (1800 x 1200 - 1.26 MB)
Instrument |
12.5" RCOS @
~f/9 (2880 mm fl) at 1.28 arcsec/pixel. Shown at 1.23 and 2.95 arcsec/pixel. |
Mount |
Paramount ME |
Camera |
SBIG STL-11000 w/
FW8 filter wheel, AstroDon Gen-2 Filters |
Acquisition Data |
9/4/2010 to 11/12/2010 Chino Valley, AZ... with CCDAutoPilot3
& CCDSoft. AOL guided |
Exposure |
Lum (no
filter) |
420 min (28 x 15 min,
bin 1x1) |
Ha |
600 min (20 x 30 min,
bin 1x1) |
RGB |
225 min ( 5 x 15 min
each, bin 2x2) |
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Software & Processing Notes |
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CCDSoft, CCDStack,
Photoshop CS6, PixInsight and Noel Carboni's actions
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CCDBand-Aid to repair
KAI-11000M vertical bars.
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eXcalibrator for (b-v), (v-r) color calibration, using 32 stars
from the NOMAD1 database.
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PixFix32 (pre-beta) to
repair column defects.
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CCDStack to calibrate,
register, normalize, data reject, combining the sub exposures
and RGB creation.
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PixInsight processing
includes gradient removal, the initial non-linear stretching with
HistogramTransformation. HDRMultiscaleTransform was used to enhance
the detail.
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PhotoShop for
the LRGB combine, adding Ha data to the red channel and final touch
up.
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Comment |
The nebula is shown
with north to the top.
Also catalogued as NGC
2099, M37 is in the constellation Auriga at a distance of about
4,500 light years. The age of the cluster is estimated as between
350 and 550 million years. M37 contains about 150 stars brighter
than magnitude 12.5 and at least 12 red giants.
Giovanni Battista Hodierna discovered the cluster sometime before
1654. Charles Messier independently rediscovered it in 1764 as
object number 37 in his catalog. |
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