*RGB color, Lab color and LRGB composit
*Drastic reduction of Exposure time by LRGB
1) Galaxies, Nebulae
Exposure time ; about 1/4 or more
2) Planets
One good monochrome + poor RGB = Best color image
The most important point is:
The human's eye is very
insensitive to the resolution in coloring data. The resolution of color image is determined by the
resolution of the L-image only. This is true either for nebulae and
planets.
Drastic Reduction of Exposure Time
In Most CCD camera, the 2x2 or 3x3 binning mode, where the sensitibity is improved in stead for deterioration in resolution, is available. By taking advantage of the binning mode in RGB image, the total exposure time can be reduced without any deterioration of the final LRGB image. This is the first merit of LRGB composite.
Example:
|
RGB system |
LRGB system |
Red |
9 min |
1 min (1/9 of R) |
Green |
18 min |
2 min (1/9 of G) |
Blue |
27 min |
3 min (1/9 of B) |
Luminosity |
|
6 min (2/3 of R) |
Total Exposure |
54 min |
12 min (1/4.5) |
In order improve the final S/N and resolution, extending the L-exposure is most effective.
Example: M101 R=G=B=20 min, L=175 min
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1) Ideal RGB filters (broad band)
2) Ideal Dichroic RGB (no gap, sharp cut and
3) Worst case of dichroic RGB filters, with a large gap
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HPC-1 |
SBIG |
SBIG |
SBIG |
SBIG |
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HPC-1 |
SBIG |
SBIG |
SBIG |
SBIG |
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HPC-1 |
SBIG |
SBIG |
SBIG |
SBIG/ |
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ST-5 |
KenkoR60 |
Kenko |
Edmund |
Edmund |
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ST-7 |
SBIG |
SBIG |
SBIG |
Edmund |
1)L images of galaxies and clusters are taken without IR-B.
2)L-images of nebulae and planets are taken with IR-B
3)Thickness of Kenko R60, PO1 and Edmund-B is same (2mm)
L-image is taken with Kenko MC-protector (2mm)
4)IR-B is always used for the ST-7 + C8/C5 system