C241A

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Session info: http://www3.mpifr-bonn.mpg.de/div/vlbi/globalmm/
Station feedback: Gl late due to storm (https://docs.google.com/spreadsheets/d/1SZ46_WttmTxk33a252ZKkd4-dkudvW65pTLRk0f7-wc/edit#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, no KT

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This revision modified by gfparaschos (Ban)

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This revision modified by gfparaschos (Ban)

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Session info: http://www3.mpifr-bonn.mpg.de/div/vlbi/globalmm/
Station feedback: Gl late due to storm (https://docs.google.com/spreadsheets/d/1SZ46_WttmTxk33a252ZKkd4-dkudvW65pTLRk0f7-wc/edit#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, no KT

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