Description | SETI VLBI on GL 581 Earth-like planet |
---|---|
Antennas | At-Mp-Pa |
Start | 316 21:00:00 |
Stop | 317 04:20:00 |
PI | Tingay |
Channel 1 | DAS #1 IFP#1 RCP USB: SWITCH BETWEEN: 8093 - 8157, 8193 - 8257, 8293 - 8357, 8393 - 8457, 8493 - 8557 and 8543 - 8657 MHz |
Channel 2 | DAS #1 IFP#2 LCP USB: SWITCH BETWEEN: 8093 - 8157, 8193 - 8257, 8293 - 8357, 8393 - 8457, 8493 - 8557 and 8543 - 8657 MHz |
Channel 3 | DAS #2 IFP#1 RCP USB: SWITCH BETWEEN: 8143 - 8207, 8243 - 8307, 8343 - 8407, 8443 - 8507, 8543 - 8607 and 8643 - 8707 MHz |
Channel 4 | DAS #2 IFP#2 LSB USB: SWITCH BETWEEN: 8143 - 8207, 8243 - 8307, 8343 - 8407, 8443 - 8507, 8543 - 8607 and 8643 - 8707 MHz |
DAS 1 Skyfreq | SWITCH BETWEEN: 8125, 8225, 8325, 8425, 8525 and 8625 MHz |
DAS 2 Skyfreq | SWITCH BETWEEN: 8175, 8275, 8375, 8475, 8575 and 8675 MHz |
Bandwidth | 64 MHz |
DAS Mode | 64 MHz.pro |
Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/vx012/vx012b
This is in essence the same experiment as vx012a, but over a larger frequency range, at a higher frequency.
This experiment is set up to switch between six frequency setups, as listed in the table above. These setups cover a 600 MHz frequency range from 8.1 GHz to 8.7 GHz.
Frequency switch information for Parkes will be provided by Chris Phillips. Frequency switch information for ATCA and Mopra is contained in the observing schedules.
Connect VSIC directly to DAS, using the “BG3” cables for 1 Gbps recording.
ATCA: See comments for individual antennas below.