Description | 21 cm disk-based pulsar astrometry |
---|---|
Antennas | At-Mp-Pa-Ho |
Start | 135 09:00:00 |
Stop | 135 23:59:59 |
PI | Adam Deller |
Channel 1 | DAS #1 IFP#1-LO 1384 - 1400 MHz USB RCP |
Channel 2 | DAS #1 IFP#1-HI 1400 - 1416 MHz USB RCP |
Channel 3 | DAS #1 IFP#2-LO 1384 - 1400 MHz USB LCP |
Channel 4 | DAS #1 IFP#2-HI 1400 - 1416 MHz USB LCP |
Channel 5 | DAS #2 IFP#1-LO 1416 - 1432 MHz USB RCP |
Channel 6 | DAS #2 IFP#1-HI 1432 - 1448 MHz USB RCP |
Channel 7 | DAS #2 IFP#2-LO 1416 - 1432 MHz USB LCP |
Channel 8 | DAS #2 IFP#2-HI 1432 - 1448 MHz USB LCP |
DAS 1 Skyfreq | 1400.00 |
DAS 2 Skyfreq | 1432.00 |
Bandwidth | 16 MHz |
Recorder | Disk |
DAS Mode | vsop.pro (telescope) |
Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v190/v190b
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 Hyugens cable.
At Hobart, 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. Schedules for the ATCA and Mopra are in place on LEON and MOPRA
2. The .psn file for Parkes is on the ftp site.
3. The VEX file for Hobart is on the ftp site