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    1. All: 80 Hz continuous calibration. Update the table:

    2. Gonzáles: find atm binary or preferably source code for distribution, that can be used to calculate opacity from FS weather information and inject it into the log.

    3. Bach, Rottmann: look at EHT station set-up document and see if it could be modified for use in the EVN

    4. Bach: investigate how Tsys and opacity are determined at K band and higher at stations. Discussion continues on Mattermost.

    5. Marcote, Bach, Campbell: Improving the session feedback, how to provide a better feedback about the “success” of EVN observations in the feedback page and for future TOGs

    6. Paragi, Bach, Kettenis, Campbell: discuss reduction of number of BBCs/core board and impact on (future) calibration of wide bands.

    7. Bach compare gnplt opacity estimation versus WVR measurement.


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