Table of contents
- 1. C231A Correlation Report
- 1.1. General information
- 1.2. Status
- 1.3. Fringes
- 1.4. Notes
- 1.5. Post-Correlation checks
- 1.5.1. Polarizations
- 1.5.2. Residuals
- 1.5.3. FITS completeness (pclist)
C231A 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.
- Not observed: JCMT, Mopra, GBT, Kt (no maser), Br, Od (receiver selection problem at backend; On is fine).
Status
| what | date |
|---|---|
| Preparing correlation setup | 14 Dec 2023 |
| Correlation v1 running | 22 Dec 2023 |
| Correlation 3mm v1 finished | 28 Dec 2023 |
| Packaging done, but still pending PolConvert and PI project -based split | 09 Jan 2023 |
| Waiting for ALMA QA2 calibration tables |
Fringes
| Station | Code | Fringes | Plots | Comments |
|---|---|---|---|---|
| VLBA | yes | |||
| EU (Ef On Mh Ys) | yes | |||
| KVN (Ku Ky) | marginal | only 1 weak fringe, only intra-KVN, only 5 scans observed | ||
| ALMA | yes | ALMA-VLBA, ALMA-EU | ||
| NOEMA | yes | NOEMA-VLBA, NOEMA-EU | ||
Notes
- LMT, GLT, Br, Kt did not observe
- Onsala Od/L (DBBC3) IF input misconfigured to wrong receiver, but On/X (DBBC2) was fine
Post-Correlation checks
Polarizations
Polarization relative to NOEMA and prior to PolConvert, i.e., ALMA (A) and Mopra (W, not shown) still linear.
Residuals
