C241A Correlation Report
General information
- Session info: http://www3.mpifr-bonn.mpg.de/div/vlbi/globalmm/
- Station feedback: Gl late due to storm (https://docs.google.com/spreadsheets...gid=1941489491), bad weather at Pv in the beginning and at Ef, Ys lost scans 0376, 0377, Mh was offline 2024-04-19 1228 to 1400 UTC, c241a was observed from 109-22:00 to 110-06:50 UT, 110-10:00 to 110-10:37 UT. Nn did not observe due to storm in the beginning, then due to a cabling error, we were on the "regular" 3mm band R&S SMA 100A synthesizer that was referenced to the maser (it should have sufficient quality for VLBI, however). We switched to the VLBI specific R&S SMA 100B just before starting c241b, and the following observations of c241b and c241c were done with it, Aa good
Status
| what | date |
| started e-transfer for PV(1/2), Ys, On, Mh, sent email to KVN/Mp (awaiting start), Ef will be started by Uwe | 22.4.2024 |
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Fringes
| Station | Fringes | Plots | Comments |
| Ef | | | |
| Nn | | | |
| Pv | | | |
| Ys | | | |
| Mh | | | |
| On | | | |
| Gl | | | |
| KVN (4?) | | | |
| VLBA(8) | | | |
Notes
Post-Correlation checks
Residuals
FITS completeness (pclist)
