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v212a Setup:
| Description | SN2004ip |
|---|---|
| Antennas | At-Mp-Pa-Ti |
| Start | 159 09:00:00 |
| Stop | 159 20:58:00 |
| PI | Ryder |
| Channel 1 | DAS #1 IFP#1-LO 2226 - 2242 MHz USB RCP |
| Channel 2 | DAS #1 IFP#1-HI 2242 - 2258 MHz USB RCP |
| Channel 3 | DAS #1 IFP#2-LO 2226 - 2242 MHz USB LCP |
| Channel 4 | DAS #1 IFP#2-HI 2242 - 2258 MHz USB LCP |
| Channel 5 | DAS #2 IFP#1-LO 2258 - 2274 MHz USB RCP |
| Channel 6 | DAS #2 IFP#1-HI 2274 - 2290 MHz USB RCP |
| Channel 7 | DAS #2 IFP#2-LO 2258 - 2274 MHz USB LCP |
| Channel 8 | DAS #2 IFP#2-HI 2274 - 2290 MHz USB LCP |
| DAS 1 Skyfreq | 2242.00 MHz |
| DAS 2 Skyfreq | 2274.00 MHz |
| Bandwidth | 16 MHz |
| DAS Mode | vsop.pro (telescope) |
Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v212/v212a
This is a disk based experiment. Do NOT delete the data after recording!!!!
Please make sure that v212a gets recorded to its own set of xraid disks, as these data will be going to Curtin, not Swinburne. Please do not mix these data with data from other experiments
Connect DAS directly to VSIC
At the ATCA, Mopra, and Parkes, both DAS units are used to give 2 x 256 Mbps = 512 Mbps recording over 8 x 16 MHz channels, using the Huygens cable.
At Tidbinbilla, one DAS unit is used to give 1 x 256 Mbps recording over 4 x 16 MHz channels. These channels will match the frequencies listed at RCP for both DAS1 and DAS2 in the table above.
Details of disks to be used, disko setup, and telescope-specific comments appear under the links below.
Comments:
Observing comments for each antenna:
Observing Logs
