ATNF VLBI Wiki

vt02jb Setup:

Description	vt02jb fringe check observation
Antennas	At-Mp-Pa-Ho-Cd-Ti
Start	169 07:00:00
Stop	169 12:00:00
PI	Tingay
Channel 1	`DAS #1 IFP#1-LO 2268 - 2284 MHz USB RCP`
Channel 2	`DAS #1 IFP#1-HI 2284 - 2300 MHz USB RCP`
Channel 3	`DAS #1 IFP#2-LO 2268 - 2284 MHz USB LCP`
Channel 4	`DAS #1 IFP#2-HI 2284 - 2300 MHz USB LCP`
Channel 5	`DAS #2 IFP#1-LO 2300 - 2316 MHz USB RCP`
Channel 6	`DAS #2 IFP#1-HI 2316 - 2332 MHz USB RCP`
Channel 7	`DAS #2 IFP#2-LO 2300 - 2316 MHz USB LCP`
Channel 8	`DAS #2 IFP#2-HI 2316 - 2332 MHz USB LCP`
DAS 1 Skyfreq	2284.00 MHz
DAS 2 Skyfreq	2316.00 MHz
Bandwidth	16 MHz
DAS Mode	vsop.pro (telescope)

Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/vt02/vt02j/vt02jb

Schedule starts at 05:00 UT. Please start vt02jb once vt02ja fringe test is complete.

This is a disk based experiment. Do NOT delete the data after recording!!!!

DO NOT RECORD TO XRAIDS. RECORD TO REMOVABLES IF POSSIBLE, PLEASE;
IF REMOVABLES ARE NOT AVAILABLE, DON'T WORRY ABOUT RECORDING AT ALL.

Connect DAS directly to VSIC

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 Huygens cable.

At Hobart, Ceduna, and Tidbinbilla, one DAS unit is used to give 1 x 256 Mbps recording over 4 x 16 MHz channels. At Hobart, Ceduna, and Tidbinbilla the recorded data will match the frequencies/polarisations listed in the table for DAS1 .

Further antenna-based instructions as per v210a.