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v190g Setup:
| Description | 3 cm disk-based pulsar astrometry |
|---|---|
| Antennas | At-Mp-Pa-Ho-Cd-Ti |
| Start | 81 01:00:00 |
| Stop | 81 13:00:00 |
| PI | Adam Deller |
| Channel 1 | DAS #1 IFP#1-LO 8409 - 8425 MHz USB RCP |
| Channel 2 | DAS #1 IFP#1-HI 8425 - 8441 MHz USB RCP |
| Channel 3 | DAS #1 IFP#2-LO 8409 - 8425 MHz USB LCP |
| Channel 4 | DAS #1 IFP#2-HI 8425 - 8441 MHz USB LCP |
| Channel 5 | DAS #2 IFP#1-LO 8441 - 8457 MHz USB RCP |
| Channel 6 | DAS #2 IFP#1-HI 8457 - 8473 MHz USB RCP |
| Channel 7 | DAS #2 IFP#2-LO 8441 - 8457 MHz USB LCP |
| Channel 8 | DAS #2 IFP#2-HI 8457 - 8473 MHz USB LCP |
| DAS 1 Skyfreq | 8425.00 |
| DAS 2 Skyfreq | 8457.00 |
| Bandwidth | 16 MHz |
| Recorder | Disk |
| DAS Mode | vsop.pro (telescope) |
Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v190/v190g
Comments:
This is a disk based experiment. Do NOT delete the data after recording!!!!
Record on /data/removable or /data/xraid as appropriate. Disk allocations for each telescope are listed under the telescope specific notes, linked to below.
Parkes, ATCA & Mopra connect both DAS to single VSIC input using 'Huygens' cable. Use RecordMode “Chans 1-8”. DAS#2 should be configured to be the higher frequency and connected to input#2 (input with clock lines connected).
Hobart, Tidbinbilla, and Ceduna will use the standard flat cable, no jumper: this means that these three telescopes will match the 2 dual polarisation bands at the low centre frequency - 8425 MHz i.e. DAS1. Use RecordMode “Chans1-4”
Observing comments for each antenna:
Observing Logs
