Hobart/Ceduna LBA observers schedule for September 09 session;
LBA Wiki page for this session
Hobart
| Local Date & Time | Description | Observer |
|---|
| Thursday 12pm-Friday 8am | IVS APSG24 at Hobart with remote observing of VT11U at Ceduna. Followed by set up for VT02N for Ceduna and Hobart | Jay |
| Friday 8am-4pm | vt02N [Freq change?] vc090, v255f. v255f is likely to need changes in the back-end configuration during the experiment | Warren |
| Friday 4pm - Saturday 8 am | v255f [Freq change?] vc091 v316a | JD |
| Saturday 8am - Saturday 8 pm | v316a [Freq change?] vc092 v255g.v255g is likely to need changes in the back-end configuration during the experiment | Warren |
| Saturday 8pm - Sunday 8am | v255g [Rx Change 6.7 -> 8.4 GHz], vc093, v252n | Jim L. |
| Sunday 8am - Sunday 8pm | v252n | Jay |
| Sunday 8pm - Monday 8am | v252n | Warren |
All experiments are at 6.7 Ghz except for vc093 & v252n which are at 8.4 GHz. Details on the backend configurations required will be added when the LBA Wiki has the info. The v255f and V255g experiments will likely require changes to the backend being made during the observations, at both Hobart and Ceduna. Bev and Mark will be at the Ceduna observatory to do this.
Suggested Disk Usage
Setup Notes
NOTE: I think that these LO frequencies, DAS profiles are correct, however, please check coherence etc carefully at setup time ase mistakes are always possible.
Hobart
| Experiment | Agilent (GHz) | LO (SMY) | Tone (SML) | DAS Profile | Notes |
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Ceduna
| Experiment | Agilent (GHz) | LO (SMY) | Tone (SMY) | DAS Profile | Notes |
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