This is an old revision of the document!
|Description||The 5 GHz Faint Radio Population at VLBI Resolutions|
|Station Modes||At Mp Pa - Chris please fix this mode!|
|DAS 1 Skyfreq||4848 MHz|
|DAS Mode||64MHz_[nf].pro (telescope)|
|Station Modes||Cd Ho|
|DAS 1 Skyfreq||4816 MHz|
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.