Sidebar
Observer : Simon Ellingsen & Bev Bedson
Agilent : 13.04 GHz, 14.0 dBm
Signal from L1 is RCP (from vc134 fringe check at 06:54:40)
SMY01 into DAS IFP#1 637 MHz, 7 dBm
SMY03 into DAS IFP#2 669 MHz, 7 dBm
DAS Profile VSOP.PRO
Recording to ATNF V015B started at 07:00:00 UT (but telescope not onsource)
Telescope first onsource at 07:08:30 UT
Telescope Windstowed 07:14:21 - 12:03:27 UT & 22:18:21 - 22:46:15
Setup for Ceduna 4×16 MHz RCP :
Signal from L1 (RCP) into LHS amplifier, output to splitter above frequency translator
One splitter output into LHS splitter, which splits to LHS programmable attenuators (for Tsys etc) and to Frequency translator LHS
Other splitter output into RHS splitter, which splits into RHS programmable attenuators (for Tsys etc) and to Frequency translator RHS
