Description | The Importance of Magnetic Fields in the Formation of Water Fountains |
---|---|
Antennas | Pa-At-Mp-Ho-Cd-Hh |
Start | 164 06:30:00 |
Stop | 164 06:59:00 |
PI | Ioannis Gonidakis |
Setup h2o_1:
Station Modes | Pa At Mp Ho Cd |
---|---|
Channel 1 | IFP#1-LO 22230 - 22246 MHz USB RCP |
Channel 2 | IFP#1-HI 22246 - 22262 MHz USB RCP |
Channel 3 | IFP#2-LO 22230 - 22246 MHz USB LCP |
Channel 4 | IFP#2-HI 22246 - 22262 MHz USB LCP |
DAS 1 Skyfreq | 22246 MHz |
Bandwidth | 16 MHz |
DAS Mode | vsop.pro (telescope) |
Station Modes | Hh |
---|---|
Channel 1 | 22230 - 22246 MHz USB RCP |
Channel 2 | 22230 - 22246 MHz USB LCP |
Channel 3 | 22246 - 22262 MHz USB RCP |
Channel 4 | 22246 - 22262 MHz USB LCP |
Bandwidth | 16 MHz |
DAS Mode | Mark5 |
Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/fringe-checks/vc205
Parkes onsource flagging
ATCA onsource flagging
Mopra onsource flagging
Mopra Tsys
(plot)
Parkes Tsys