Table of contents
Correlation Status March 2017
| Project Code | Block Code | Sources | DOYS | UT | Frq | Stations | Status | PI | Comment |
| MN001 | C171A | 3C84 | 89-90 | 8:30-1:30 | 86 | Eb,Yb,On,Mh,KVN,GB,VLBA | Correlated, quality check | Nagai | |
| MA009 | M87 | 89-90 | 22-13 | 86 | Eb,Yb,On,Mh,Pv,KVN,GB,VLBA | Correlated, quality check | Asada | ||
| MB005 | C171B | NGC1052 | 90 | 9:30-24 | 86 | Eb,Yb,On,Mh,Pv,GB,VLBA,Nt(7mm) | Correlated quality check | Baczko | |
| MM07B | C171C | Fermi sources | 90-92 | 19-18:20 | 86 | Eb,Yb,On,Mh,Pv,KVN,GB,VLBA | Correlated quality check | Marscher | |
| MG002 | - | OJ287 | 92-93 | 17:20-07 | 86 | Eb,Yb,On,Mh,Pv,Aa,VLBA | Correlated | Gomez | ALMA mode |
| MB007 | - | Sgr* | 93 | 03-15:20 | 86 | Eb,Yb,Pv,GB,Aa,VLBA | Correlated | Brinkerink | ALMA mode |
| MA008 | - | 3C273 | 93-94 | 19-11 | 86 | Eb,Yb,Pv,On,Mh,Aa,VLBA | Correlated | Akiyama | ALMA mode |
General comments:
Whole session:
- Ys has (as usual) observed LCP only
- Pt has fringes only in parts of the experiment and only to a few stations
ALMA-mode:
- MH no fringes. Strange AC indicating error in setup of firmware. MH has a rare DBBC setup.
- Pv: used 32 MHz PFB by mistake. Not included in first run with 58 MHz sub-bands.
- Ys fringes in MB007. Seems to have used 32 MHz PFB in other 2 observations.
- ALMA: first time with GMVA and good fringes
- A 2nd correlation pass will be done to recover Pv and Ys: requires experimental zoom-mode and stitching of sub-bands to 58 MHz. More info under mg002.
