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
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”