This is an old revision of the document!
In this page you can find the files and documents used by the EVN support scientists to post-process the EVN data after correlation and deliver them to the PI.
The EVN Support Scientists process the data from each EVN observation after correlation and until the data are delivered to the PI of the experiment.
There are some tools to help you summarised here.
Read about the current versions of j2ms2 and tConvert here
In cases where one or more VLBI station uses linear polarisations rather than the conventional circular polarisation - it is possible to convert linear signals to circular using PolConvert, which is a program written by Ivan Marti-Vidal. A guide to using PolConvert can be found here
Under construction (insert construction worker gif) guide can be found here
After an NME is post-processed, we need to write a report about all the issues observed on it. All NMEs are stored in this web.
Modify the page to include your new NME. You can also find there the LaTeX template to produce the NME Report. However, I recommend you to use this Python script to produce a more customized LaTeX template that will save you some editing time.
Download it to your computer. You can run it without arguments or with -h to see the required inputs. The script will create a LaTeX template where the table has already been adjusted to the stations that have participated in your NME.
Antenna-specific problems: this is a text page located here. Please update this when you find a problem. Will be replaced soonish with a fault tracker probably.
ANTAB-related problems: this is a page to keep track of 'all' issues concerning ANTAB files. The plan is also to keep track of the stations that do not upload ANTAB files at a given time.