Ceduna-Hobart diagnostic VLBI
4816 MHz sky freq
Ceduna used Agilent & Wiltron for first LO (at 9 dBm), replacing fixed oscillator. SMY01 and SML were used as second LOs at 436 MHz for Ch1 and Ch2 respectively. DAS profile VSOP_HO.PRO
Ceduna used Agilent instead of fixed 4.1 GHz oscillator between ~17:40 and 18:20:40
Wiltron used as first LO between 18:21:50 and 18:52:10
Ceduna recorded to Fermi disks 17 & 18
Hobart data on external eSATA Fermi disks. Fermi 7 & 8.