Useful links:
Observing Roster for Hobart March 2012:
Time (local; EST) | Experiment(s) | Band | Notes | Observer |
Tue 6 Mar 4:30 PM - Wed 7 Mar 8:30 AM | v252ac | 22 GHz | Ceduna & Hobart | Anita |
Wed 7 Mar 4:30 PM - Thu 8 Mar 8:30 AM | v255q | 6.7 GHz | Ceduna & Hobart | Simon |
Thu 8 Mar 11:30 PM - Fri 9 Mar 8:30 AM | vc163, v452a | 6.7 GHz (Hob), 6.0 GHz (Ced) | Ceduna & Hobart, initial setup, receiver change at Hobart (back to 6.7 GHz after 22 GHz tests) | Jay |
Fri 9 Mar 4:30 PM - Sat 10 Mar 7:00 AM | vc164, v256a | 1.6 GHz | Hobart only, initial setup, quad hybrid tuning same as VSIC tests immediately prior. BUT MAY NEED TO BE RETUNED POST-EXPERIMENT for Sat morning tests. (Awaiting confirmation). | JD |
Sat 10 Mar 11:30 PM - Sun 11 Mar 1:00 PM | vc165, v452b | 1.6 GHz | Hobart only, initial setup, experiment uses quadrature hybrid | Jo & Courtney |
Sun 11 Mar 7:30 PM - Sun 11 Mar 11:30 PM | vc166/vc167, vt19a/b | 1.6 GHz, 4.8 GHz | Hobart only, RadioAstron tests, experiment uses quadrature hybrid? | Brett & Jay |
During office hours both Ceduna and Hobart monitored and operated by Brett (on-site) & Jo, Simon & Jay at Sandy Bay.
Additional Tests & Scheduled Items
Tests are now marked on the block schedule. (Check the png version.)
All times given below are ADST. All tests use Hobart only (Ceduna idle).
Check the main VLBI wiki page for frequency setup. (No information available at time of writing.)
- Thursday ~10:00-12:30: ASKAP eVLBI X-band tests. Need to swap in BG3 cable.
- Thursday 12:30-13:30: JD & Jo configuring quad hybrid
- Thursday 14:30-15:30: 8 GHz student time (reconfigure for 22 GHz upon completion)
- Thursday 19:00-24:00: 22 GHz KVN eVLBI tests. Jo & JD to set up for these before going home. DAS profile is 16MHZ_UL_F.PRO.
- Friday 13:00-18:00: L-band VSIC. Same frequency as v256a.
- Saturday 11:00-15:00: ADST L-band GMRT tests. Jo to manage these from Sandy Bay. Quad hybrid may have to have been retuned from night before (JD). Data needs to be saved (data rate: 128 Mbps).
Setup Notes
Hobart
Experiment | Agilent | LO (SMY) | Tone (SML) | DAS Profile | Disks | Notes |
vc161 & v252ac | 16600 MHz | 636 MHz | 892.2 or 929.375 MHz | VSOP_HO.PRO | CURTV001B | |
vc162 & v255q | 12200 MHz | 810/468 MHz (LO1), 810 MHz (LO2) | 830.875, 630.5 MHz | VSOP.PRO | ATNFV009A | |
vc163 & v452a | 12200 MHz | 828 MHz | 666.5 MHz | VSOP.PRO | | |
vc164 & v256a | 4100 MHz | 602 MHz | 819.5 MHz | VSOP_HO.PRO | | |
vc165 & v452b | 4100 MHz | 578 MHz | 332.6 MHz | VSOP_HO.PRO | | |
vc166 & rafs16 | 4100 MHz | 584 MHz | 828.5 MHz | 16MHZ_UL.PRO, need to decide _F or _N | | |
vc167 & rafs16 | 10500 MHz | 680 MHz | 965.0 MHz | 16MHZ_UL.PRO, need to decide _F or _N | | |
Ceduna
Experiment | Agilent | LO (SMY01/03) | Tone (SMY02) | DAS Profile | Disks | Notes |
vc161 & v252ac | 17400 MHz | 336 MHz | 929.375 MHz | VSOP_HO.PRO | CURTV006B | |
vc162 & v255q | 11100 MHz | 810/468 MHz (LO1), 810 MHz (LO2) | 830.875, 630.5 MHz | VSOP.PRO | ATNFV015B | |
vc163 & v452a | 10600 | 694 MHz | 603.1 MHz | | | Source detection at 6042 MHz confirmed by Simon. |