Table of contents
Correlation Status
| Project Code | Block Code | Sources | DOYS | UT | Freq | Stations | Status | PI | Comment |
|---|---|---|---|---|---|---|---|---|---|
| f231a | 123 | ||||||||
| c231a | 124 | ||||||||
| c231b | |||||||||
| c231c | |||||||||
| c231d |
General comments
- ALMA scheduled, will have 3 MHz frequency offset
- LMT runs off Oscilloquartz xtal without H-maser/Rb
- LMT is linear polarized, has a feed rotator active during calibration scans that ought to return to 'origin' for VLBI scans avoiding any per-scan instrumental polarization angle offsets
- MOPRA is linear polarized
- TAMNA is not observing due to broken maser
- Draft schedules: https://cloud.mpifr-bonn.mpg.de/index.php/s/J6SYRbxWJ8zMRF2
Recording media
See the media distribution plan
