DATE |
2000 - ON |
| OBSERVER(S) |
BHATHAL AND DARCY |
| SITE |
CAMPBELLTOWN ROTARY OBSERVATORY, OZ OSETI |
| INSTR. SIZE (M) |
0.4 AND 0.3 |
| SEARCH FREQ. (MHz) |
550 nm |
| FREQ. RES. (Hz) |
NONE |
| OBJECTS |
200 SOLAR-TYPE STARS AND 25 GLOBULAR CLUSTERS |
| FLUX LIMITS (W/m
2
) |
6 x 10
-9
PEAK DURING 1ns PULSE |
| TOTAL HOURS |
ONGOING |
| REFERENCE |
73 |
| COMMENTS |
Dedicated telescope built for SETI. Uses high time resolution photodiodes in coincidence to search for laser pulses, and coincidence between two telescopes separated by 20 m to bring down false alarm rate. Soon to be teamed with microwave search of same objects. |
|
| DATE |
2000 - ON |
| OBSERVER(S) |
MONTEBUGNOLI (SETItalia) |
| SITE |
MEDICINA |
| INSTR. SIZE (M) |
32 |
| SEARCH FREQ. (MHz) |
1415-1425 and 4255-4265 |
| FREQ. RES. (Hz) |
0.6 |
| OBJECTS |
NORTHERN SKY |
| FLUX LIMITS (W/m
2
) |
|
| TOTAL HOURS |
ONGOING |
| REFERENCE |
69 |
| COMMENTS |
Commensal sky survey using Medicina telescope and SERENDIP signal processing boards. |
|
| DATE |
2001 - ON |
| OBSERVER(S) |
DRAKE ET AL., LICK OPTICAL SETI |
| SITE |
LICK OBSERVATORY, UC SANTA CRUZ |
| INSTR. SIZE (M) |
1 (NICKEL REFLECTOR) |
| SEARCH FREQ. (MHz) |
550nm |
| FREQ. RES. (Hz) |
NONE |
| OBJECTS |
5039 SOLAR-TYPE STARS PLANNED |
| FLUX LIMITS (W/m
2
) |
1 x 10
-9 PEAK DURING 1ns PULSE, OR 1 x 10-20 AVERAGE PER 100 SECOND OBSERVATION
|
| TOTAL HOURS |
ONGOING, APPROXIMATELY 1 NIGHT PER WEEK |
| REFERENCE |
77 |
| COMMENTS |
Uses three photodiodes in coincidence to eliminate background events. |
|
| DATE |
JUNE 01, 2001 |
| OBSERVER(S) |
SHIRAI, OYAMA, IMAI, AND ABE |
| SITE |
VLA |
| INSTR. SIZE (M) |
|
| SEARCH FREQ. (MHz) |
22.235 GHz |
| FREQ. RES. (Hz) |
6.104 KHz |
| OBJECTS |
13 |
| FLUX LIMITS (W/m
2
) |
20 mJy |
| TOTAL HOURS |
|
| REFERENCE |
|
| COMMENTS |
Observed each star for 10 min. |
|