Description | 3 cm disk-based pulsar astrometry |
---|---|
Antennas | At-Mp-Pa-Ho-Cd |
Start | 133 22:00:00 |
Stop | 134 08:30:00 |
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/v190a
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 and using the huygens cable.
At Hobart and Ceduna, one DAS unit is used to give 1 x 256 Mbps recording over 4 x 16 MHz channels.
Details of disks to be used, disko setup, and telescope-specific comments appear under the links below.
Read these instructions in conjunction with the disk usage plans that were sent out to each telescope for far more information.
1. Schedule for the ATCA is in place on LEON
2. The .psn file for Parkes is on the ftp site.
3. The VEX file for Hobart and Ceduna is on the ftp site
4. The sched command file for Mopra is one the ftp site