Table of contents
- 1. C231D Correlation Report
- 1.1. General information
- 1.2. Status
- 1.3. Fringes
- 1.4. Notes
- 1.5. Post-Correlation checks
- 1.5.1. Residuals
- 1.5.2. FITS completeness (pclist)
C231D Correlation Report
General information
- Session info: http://www3.mpifr-bonn.mpg.de/div/vlbi/globalmm/
- Station feedback: https://www3.mpifr-bonn.mpg.de/div/vlbi/globalmm/sessions/may23/feedback_may23.asc
- No fringes to LMT, no data from Hs.
- Kt (no maser) and Br did not observe.
Status
what | date |
---|---|
Preparing for correlation | 5 Dec 2023 |
Ready to start v1 correlation once A, B tracks finish, and copying ofMPI%8027 to /data/c231d/Mk/ has finished | 27 Dec 2023 |
Correlation v1 3mm preparing - todo fix wrong ATCA position, clock adjust | 15 Jan 2023 |
Correlation v1 3mm started with above fixes | 15 Jan 2023 |
Fringes
Station | Code | Fringes | Plots | Comments |
---|---|---|---|---|
ALMA | did not observe | |||
NOEMA | yes | |||
KVN Ku Ky | yes | |||
KVN-Mopra | yes | |||
Mopra-ATCA | yes | ATCA IF1 has a delay offset wrt IF2, and had refpad W104 rather than W110 | ||
Mopra-JCMT | yes | |||
GLT-NOEMA | yes | |||
EU | yes | |||
EU-VLBA | yes | |||
LMT | no | |||
Notes
During the preproduction correlation tests I noticed that the Gl polarisations seem to be swapped. The strong fringes to Ef are on LR and RL, so I commented out the polswap=True in the v2d, but only here.