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Modified 15:11, 6 Apr 2022 by ubach | Page History
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    Version as of 23:22, 28 Apr 2024

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    1. All: 80 Hz continuous calibration. Update the table: https://deki.mpifr-bonn.mpg.de/Working_Groups/EVN_TOG/Continuous_calibration_%2880_Hz%29

    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.