Table of contents
Combined revision comparison
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All: Beam-maps at L- and C-band and send them to Keimpema https://deki.mpifr-bonn.mpg.de/Working_Groups/EVN_TOG/Beam_maps
+ Bach investigate use of HOLOG for creating beam maps -
All: Upgrade to SDK9.4 first at the correlators then at the stations.
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All: 80 Hz continuous calibration. Update the table: https://deki.mpifr-bonn.mpg.de/Working_Groups/EVN_TOG/Continuous_calibration_%2880_Hz%29
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Vicente: 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.
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Bach, Rottmann: look at EHT station set-up document and see if it could be modified for use in the EVN
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Bach: to contact subgroup of interested/experts and to investigate how Tsys and opacity are determined at K band and higher at stations to improve K-band amplitude calibration.
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Rottmann and Leeuwinga: send emails to owners of 2 – 4 TB modules and ask what should be done with them.
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Rottmann: set up meeting with Verkouter, Kettenis, Alef, Rottmann and Wagner, to discuss the best format of VDIF packets.
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Marcote, Bach, Campbell: Better impact reporting discussion and/or implementation.
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Bach: invite group of interested/experts for working on DBBC3 support in the Field System.
Version from 15:11, 18 May 2020
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Version as of 15:13, 18 May 2020
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-
All: Beam-maps at L- and C-band and send them to Keimpema https://deki.mpifr-bonn.mpg.de/Working_Groups/EVN_TOG/Beam_maps
+ Bach investigate use of HOLOG for creating beam maps -
All: Upgrade to SDK9.4 first at the correlators then at the stations.
-
All: 80 Hz continuous calibration. Update the table: https://deki.mpifr-bonn.mpg.de/Working_Groups/EVN_TOG/Continuous_calibration_%2880_Hz%29
-
Vicente: 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.
-
Bach, Rottmann: look at EHT station set-up document and see if it could be modified for use in the EVN
-
Bach: to contact subgroup of interested/experts and to investigate how Tsys and opacity are determined at K band and higher at stations to improve K-band amplitude calibration.
-
Rottmann and Leeuwinga: send emails to owners of 2 – 4 TB modules and ask what should be done with them.
-
Rottmann: set up meeting with Verkouter, Kettenis, Alef, Rottmann and Wagner, to discuss the best format of VDIF packets.
-
Marcote, Bach, Campbell: Better impact reporting discussion and/or implementation.
-
Bach: invite group of interested/experts for working on DBBC3 support in the Field System.