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Click the image for a 70%
size, 4.96
arcsec/pixel display (2700 x 1800)
Instrument |
Takahashi FSQ-106ED @
f/5.0 (530 mm FL) Captured at 3.5 arcsec/pixel. Shown resampled to 17.9 arcsec/pixel. |
Mount |
Paramount ME |
Camera |
SBIG STL-11000 w/
internal filter wheel, AstroDon Filters |
Acquisition Data |
12/27/2008
to 1/8/2009 Chino Valley... with CCDAutoPilot3 |
Exposure |
Lum 230
min. (23 x 10 min. bin 1x1)
Ha 300
min. (10 x 30 min. bin 1x1, 6 nm filter)
RGB 240
min. ( 8 x 10 min. each bin 1x1)
50-50 blend of LRGB &
HaGB + an additional overlay of star colors.
Click
here for an Ha B&W version
Click here for a narrow band color
mapped version |
Software |
CCDSoft,
CCDStack, Photoshop CS w/ the Fits Liberator plugin, Noel Carboni's actions
and Russell Croman's GradientXTerminator.
CCDStack to calibrate, register,
normalize, data reject & combine sub exposures.
PhotoShop for
non-linear stretching and color combine. |
Comment |
North is to the top.
The Rosette Nebula is
a large, circular hydrogen region located near one end of a giant
molecular cloud in the Monoceros region of the Milky Way Galaxy. The
open cluster, NGC 2244, is closely associated with the nebulosity,
the stars having been formed from the nebula's matter. The Nebula is
about 100 light-years across and is about 5000 light-years away. The
nebula can be seen with a small telescope using low power. With
binoculars the wisps of the nebula become clearly visible, if
observed under very dark skies. |
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