| 1. | Very high spectral resolution astrophysics in the visible and infrared. |
| 2. | Very Large Array (VLA) adaptive optical heterodyne telescope interfero-meters for extremely high angular resolutions (< 10-4 arcsecond). |
| 3. | Direct detection of extra-solar planets. |
|
The Columbus Optical SETI Observatory |
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Web Site: www.stuartkingsley.com |
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