The next-generation of adaptive optics for our SBIG large-format cameras. Requires a SBIG StarChaser SC-4 Off-Axis Guider Camera (or an older self-guiding system).
The SBIG AO-X is a large aperture AO designed to be compatible with all large format SBIG cameras. It requires an off-axis guide camera behind the AO; typically the SBIG StarChaser SC-4 is used.
The AO-X is compatible with the Aluma AC4040, Aluma AC2020, and Aluma AC455 cameras, when used with a StarChaser SC-4.
AO-X is also compatible with older STX-16803, STXL-16200, STXL-11000, and STXL-6303 cameras. Guiding can be performed via a StarChaser SC-4, or through older guide systems including STX Guider, FW8G-STXL self-guided filter wheels, the built-in guide sensor on some STX cameras, or a Remote Guide Head with an off-axis guider behind the AO-X.
Note: When using with StarChaser with AO, you will need a StarChaser to AO-X/AO-8T Adapter Cable.
AccessoriesAluma AC, STX, and STXL cameras have a standard mounting bolt pattern (four 6-32 threaded holes on a 4″ diameter). We have a variety of bolt-on adapters available for different telescope interfaces. Optionen: Aluma AC Adapter Plate
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Power: Supplied through Camera’s I2C Port |
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OS Compatibility: Windows 7, 8, 10 x86/x64. Contact us for Linux support. |
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Computer Interface: I2C |
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Dimensions: 6 x 7 x 1.2 in. |
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Weight: 2.2 lbs (1 kg) |
User’s Manual
Installation and operation instructions for your AO-X adaptive optics unit.
AO Results
The images below are actual star images showing the effect of image wander corrected at 1 Hz and 10 Hz:
1 Hz Corrections 10 Hz Corrections
And the resulting size of the star image in a long exposure:
1 Hz Corrections 10 Hz Corrections
Other data gathered by Brad Wallis of JPL (Brad Wallis and Benoit Schillings developed the prototype for the original AO-7) show the the effect of rapid corrections on poor seeing. At 1 Hz the larger, slower component is reduced, but the amplitude of the jitter remains about the same:
However, at a 5Hz correction rate, the faster jitter is reduced:
And at a 10 Hz correction rate, significant improvement is seen:
The improvement in stellar profiles can also be seen at corrections above 1 Hz. First by looking at the non-AO guided image:
Copyright 1995-2000 Brad D Wallis
And comparing the non-AO guided image to the AO guided image there is again significant improvement in the FWHM of the star profile:
elescope mounts cannot correct faster than about once per second. The 10Hz rate of the AO-X will clearly result in improved resolution under the right conditions.