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Technology: [ Rigel Telescope | Iowa Robotic Telescope | Control Software | Rigel Telescope Tests | Rigel May 2002 Tests ] |
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Rigel Acceptance TestsResults of the June 2002 acceptance tests are now available. Design CriteriaThe Rigel robotic observatory system design was driven by six criteria:
After considerable discussion of these design criteria with the telescope design group at Torus Precision Optics and the chief software engineer at Clear Sky Institute, as well as extensive experience with existing automated telescopes at the University of Iowa, we have designed a system that meets the above criteria. The complete system, called Rigel, can be produced in quantity at reasonable cost and with proven components and materials
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SubSystem |
Vendor, Model |
Item |
Specification |
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Optics |
Torus Precision Optics modified CC-04 design |
Optical Tube Assembly |
Open Truss |
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Primary Mirror |
37 cm (14.5in) diameter 1/16 wave RMS |
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Overall Focal Ratio |
f/14 |
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Optical Design |
Classical Cassegrain |
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Mount design |
Fork-mount Equatorial |
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| Mount |
Torus Precision Optics modified CC-04 |
Motors and Electronics |
Steppers, CSI motion control |
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FLI with SITe-003 sensor |
Camera assembly |
1024x1024 24m sensor TE cooled, back-side illuminated, AR coated |
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Filter
Wheel |
Torus Precision Optics |
Wheel assembly |
Twelve position, stepper motor |
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Filters |
Johnson-Cousins CBVRI, narrow band optional |
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Control
Software |
Torus |
Talon observatory control software |
Fully automated control of focus, mount, camera, filter wheel, dome, weather monitor, communication |
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Enclosure |
Winer Observatory |
Roll-off roof |
Controlled by Talon software |
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Weather
System |
Davis Instruments |
Weather Monitoring Equipment |
Full local weather monitoring |
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Time
Standard |
- |
NTP |
<1 msec synchronization with UTC |
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Control
Computer |
Dell |
Pentium 4 1.8 GHz, 512 MB RAM, 40 GB disk |
Linux O/S |
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Server
Compurter |
Dell |
PIII 700 MHz 2 x 27 GB disks 256 MB RAM |
Linux O/S |
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Subsystem |
Specification |
Value |
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Mount
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Pointing error |
30 arcsec RMS full sky |
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Tracking error |
<0.01 arcsec per second |
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Optics
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Surface Error |
<0.2l wave peak to valley <0.06l RMS |
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Point Spread Function |
>88% of stellar photons within one pixel (24m) at sensor edge (6.1mm) |
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Imaging |
Field of View |
17.1 arcmin |
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Pixel Resolution |
0.98 arcsec |
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Sensitivity |
>10:1 SNR 19th magnitude star with clear filter in 60 seconds |
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Spectroscopy |
Spectral Resolution |
1.5 nm |
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Total Spectrum Coverage |
400 – 750 nm continuous |
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Sensitivity |
>100:1 SNR on 6th magnitude star in 10 sec. |
| Item |
Date |
Comment |
| Mount base: Front view, Side view | 6 Oct 2000 | Series II design, same as CC04-CC05 |
| Isometric of complete telescope, Front view, Side view | 6 Oct 2000 |
Contact: rigel@phobos.physics.uiowa.edu
Last updated December 2, 2003