Description | The 5 GHz Faint Radio Population at VLBI Resolutions |
---|---|
Antennas | At-Cd-Ho-Mp-Pa |
Start | 344 02:00:00 |
Stop | 344 14:02:30 |
PI | S.P. Ellingsen |
Setup lba6cm-2p-2IF-64MHz:
Station Modes | At Mp Pa |
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Channel 1 | IFP#1-LO 4784 - 4848 MHz USB RCP |
Channel 2 | IFP#1-HI 4784 - 4848 MHz USB LCP |
Channel 3 | IFP#2-LO 4848 - 4912 MHz USB RCP |
Channel 4 | IFP#2-HI 4848 - 4912 MHz USB LCP |
DAS 1 Skyfreq | 4816 MHz |
DAS 1 Skyfreq | 4880 MHz |
Bandwidth | 64 MHz |
DAS Mode | 64MHz_[nf].pro (telescope) |
Station Modes | Cd Ho |
---|---|
Channel 1 | IFP#1 4784 - 4848 MHz USB RCP |
Channel 2 | IFP#2 4784 - 4848 MHz USB LCP |
DAS 1 Skyfreq | 4816 MHz |
Bandwidth | 64 MHz |
DAS Mode | 64MHz_[nf].pro (telescope) |
Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v310/v310a
This project is aiming to test the feasibility of in-beam phase referencing with the LBA at 5 GHz. It involves cycling between the three strongest 5 GHz sources in the ATESP field and a nearby ICRF2 source. The ICRF2 source should (hopefully) be strong enough to be used as a real-time fringe checker if necessary.
Parkes onsource flagging
ATCA onsource flagging
Mopra onsource flagging
Mopra Tsys
(plot)
Parkes Tsys