Description | e-VLBI of nearby GPS candidates |
---|---|
Antennas | At-Mp-Pa |
Start | 85 04:00:00 |
Stop | 85 22:00:00 |
PI | Tingay |
Channel 1 | DAS #1 IFP#1-LO 4800 - 4816 MHz USB RCP |
Channel 2 | DAS #1 IFP#1-HI 4816 - 4832 MHz USB RCP |
Channel 3 | DAS #1 IFP#2-LO 4800 - 4816 MHz USB LCP |
Channel 4 | DAS #1 IFP#2-HI 4816 - 4832 MHz USB LCP |
Channel 5 | DAS #2 IFP#1-LO 4832 - 4848 MHz USB RCP |
Channel 6 | DAS #2 IFP#1-HI 4848 - 4864 MHz USB RCP |
Channel 7 | DAS #2 IFP#2-LO 4832 - 4848 MHz USB LCP |
Channel 8 | DAS #2 IFP#2-HI 4848 - 4864 MHz USB LCP |
DAS 1 Skyfreq | 4816.00 MHz |
DAS 2 Skyfreq | 4848.00 MHz |
Bandwidth | 16 MHz |
DAS Mode | vsop.pro (telescope) |
Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v251/v251a
This is a eVLBI experiment
Experiment needs to be split over both halves of CPSR2 cluster, using the following setup
Telescope | DAS | Pam Host | Port | TCP window |
---|---|---|---|---|
ATCA | DAS1 | pam2-ext2 | 52100 | 256 |
ATCA | DAS2 | pam1 | 52100 | 850 |
Mopra | DAS1 | pam2-ext2 | 52101 | 350 |
Mopra | DAS2 | pam1 | 52101 | 800 |
Parkes | DAS1 | pam3 | 52100 | 64 |
Parkes | DAS2 | pam4 | 52100 | 64 |
pam1 and pam4 are connected to the “odd” nodes. pam2 and pam3 are connected to even nodes.