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COSETI Papers

 

These papers will be provided in HTML and Adobe's Portable Document Format (PDF) form for viewing with Acrobat Reader 3.0.

U.S. Site

U.K. Site

 

Summary

Detailed two page summary sheet comparing the relative efficacy of the Microwave, Infrared and Visible approaches to SETI.
Heterodyne detection of CW beacons signals is assumed.  Results are normalized to a 1 kW transmitter power.

 

Paper 1

Kingsley, S.A., "The search for extraterrestrial intelligence (SETI) in the optical spectrum: a review", Proc. of SPIE's Los Angeles Symposium, OE LASE '93, Vol. 1867, The Search for Extraterrestrial Intelligence (SETI) in the Optical Spectrum, Los Angeles, California, January 21-22, 1993, pp. 75-113.

 

Paper 2

Kingsley, S.A., "Amateur Optical SETI", Proc. of SPIE's Los Angeles Symposium, OE LASE '93, Vol. 1867, The Search for Extraterrestrial Intelligence (SETI) in the Optical Spectrum, Los Angeles, California, January 21-22, 1993, pp. 178-208.

 

Paper 3

Kingsley, S.A., "The Columbus Optical SETI Observatory", Progress in the Search for Extraterrestrial Life, Commission 51 Symposium, Santa Cruz, August 16-20, 1993, Astronomical Society of the Pacific, Vol. 74, pp. 387-396, 1995.

 

Paper 4

Kingsley, S.A., "Design for an Optical SETI Observatory", 45th International Astronautical Conference, 23rd Review Meeting of the Search for Extraterrestrial Intelligence (SETI), SETI: Science and Technology, Jerusalem, 9-14 October 1994.

 

Paper 5

Kingsley, S.A., "A Prototype Optical SETI Observatory", Proc. of SPIE's 1996 Symposium on Lasers and Integrated Optoelectronics, The Search for Extraterrestrial Intelligence (SETI) in the Optical Spectrum II, San Jose, California, January 27-February 2, 1996, pp. 102-116.

 

Paper 6

Kingsley, S.A., "First Monochromatic and High-Resolution Pulsed Targeted Search Data from The Columbus Optical SETI Observatory".  Submitted for the Bioastronomy 99 Meeting in Kona, Hawaii, August 1999.

 

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