|
Click the image for a 75%
size, 4.67
arcsec/pixel display (2550 x 1700)
Instrument |
Takahashi FSQ-106ED @
f/5.0 (530 mm FL) Captured at 3.5 arcsec/pixel. Shown resampled
to 16.8 arcsec/pixel. |
Mount |
Paramount ME |
Camera |
SBIG STL-11000 w/
internal filter wheel, AstroDon Filters |
Acquisition Data |
12/27/2008
to 1/3/2009 Chino Valley, AZ... with CCDAutoPilot3 |
Exposure |
Ha
300 min. (10 x 30 min. bin 1x1)
OIII 270 min. (9 x 30 min. bin 1x1)
RGB 150 min. (5
x 10 min. Each... bin 1x1)
Ha, OIII & OIII are mapped
to RGB respectivly. An RGB overlay was added for the star
colors.
Click
here for a BW Ha
version
Click
here for a narrowband 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
bottom, I think it looks better up side down.
The California Nebula
(NGC 1499) is located in the constellation Perseus at a distance of
about 1,000 light years from Earth. It is so named because it
appears to resemble the outline of the US State of California. NGC
1499 is a classic emission nebula, around 100 light-years long. It
glows with the red light characteristic of hydrogen atoms
recombining with long lost electrons, stripped away (ionized) by
energetic starlight.
Because of its very low surface brightness, it is extremely
difficult to observe visually and was discovered by E. E. Barnard in
1884. |
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