The History of Optical SETI Research on Planet Earth
9605-006
| Year |
Author(s) |
T/O |
Type |
Wavelength (m) |
Aperture (m) |
| 1961 |
Schwartz & Townes |
T |
CW |
0.50 |
5 |
| 1962 |
Bayley |
T |
CW |
0.55 |
5 |
| 1962 |
Oliver |
T |
P |
0.70 |
|
| 1965 |
Ross |
T |
P |
0.55 |
|
| 1971 |
Oliver |
T |
P |
1.06 |
100 |
| 1973 |
Wischnia |
O |
CW |
0.28 |
1 |
| 1973 |
Shavartsman |
O |
P |
0.55 |
0.6 |
| 1978 |
Shavratsman |
O |
P |
0.55 |
6 |
| 1979 |
Ross |
T |
P |
0.55 |
10 |
| 1983 |
Townes |
T |
CW |
few |
|
| 1983 |
Demming & Mumma |
T |
CW |
9.4 - 10.4 |
10 |
| 1985 |
Broderick |
T |
CW |
0.50 |
|
| 1985 |
Zuckerman |
T |
CW |
few |
|
| 1986 |
Betz |
O |
CW |
10 |
1.7 |
| 1988 |
Sherwood |
T |
CW |
10 |
|
| 1990 |
Kingsley |
T |
CW |
0.656 |
10 |
| 1991 |
Rather |
T |
CW |
0.55 |
10 |
| 1993 |
Lemarchand |
T |
P |
0.55 |
2.15 |
| 1996 |
Bliar |
O |
P |
0.573 |
0.64 |
| 1996 |
Kingsley |
O |
P |
0.55 |
0.254 |
This Table was constructed by Guillermo Lemarchand and presented at the OSETI II conference. It has been slightly modified by Stuart
Kingsley.
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