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1. Starlight ExPress MX5-C single shot color camera.
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-510x290 or 510x585 pixels; 1x1, 2x2, 3x3 binning; 9.8x12.65 or 9.8x 6.3 micron pixels.
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2. SBIG ST237 w/ color filter wheel.
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-640x480 pixels; 1x1,2x2, 3x3 binning; 7.4x7.4 micron pixels.
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3. SBIG ST4 autoguider/imager
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-192x165 pixels; 13.75x16 micron pixels; binning 1x1.
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4. SBIG ST402me CCD camera
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765 x 510 pixels; 9 microns
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MX5C Camera- On the MX5 the general procedure is to expose a series of shots at 5 to 10 minutes duration
using the 510x290 resolution and StarExpress software to collect up enough time to get a well exposed
image in color. The images will be later added to produce the final result. Then a series of shots is
made using the 510x585 resolution obtained using Astroart sortware. From this a high resolution luminence(monochrome)
only extraction is made and co-added to the color images to produce the finished full resolution result.
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ST237 Camera- On the SBIG camera a series of images are made at the 640x480 resolution to obtain data
for the final luminence frame. These durations may be anywhere from 20 seconds to 10 minutes depending
on the object and other factors such as light pollution level, seeing and telescope tracking . Then a
set of color frames with red, green and blue filters is exposed, usually with a duration of 10 minutes
each . The color filtered frames are made at the 2x2 binned half resolution. This is done to allow a
quick accumulation of light through the filters since the color information does not need to be at high
resolution. Dark frames(no light in) are obtained to allow subtracting the camera's electronic noise
and flat field frames taken against a white background are obtained to allow subtraction of uneven response
of the CCD chip.
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ST402 Camera- This newer camera operates much like the ST237 model except it has greatly improved noise
and recording capability.
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Various SLR type film cameras are used including: Olympus OM-1, Pentax K1000, and Nikon Nikkormat.
The Om-1 has interchangeable focus screens and a Beattie Intenscreen is used for astro photos, a great
help in composing and focusing. The film used for much of the astrophotography was Fuji 400 and 800 speed.
The response of these films was good for the astro objects being imaged and were fairly fine grained.
Off the shelf fresh film was used with no hypersensitizing. An occasional use of Kodak 200 or 400 was
used for lunar or planetary shots. It appears that starting sometime in the year 2000 Fuji modified their
print film to reduce redness. The effect on astrophotos was to greatly reduce the recording of red nebulae.
Kodak E200 slide film push processed 2 stops to ASA 800 is a good choice today. The general procedure
for film astrophotos is to expose 2 or more frames of the object on the same nite one after the other.
For piggyback shots using 50mm lenses at f2 -f4 2 to 16 minutes exposures are made. 100mm to 350 mm
telephoto shots are made at f4 to f5.6 and are 15 to 45 minutes in duration. Prime focus shots on the
C8 telescope are made using an off axis guider system and are 20 to 45 minutes in duration. These limits
allow reasonable image depth on the film and some relaxation of polar alinement accuracy. The key to
all of this is digitizing the film into computer format using an HP scanner and overlaying the images
in software such as Picture Window Pro. This allows strengthing the image depth and reducing out some
of the grain effects.
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