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cf https://redmine.astron.nl/lofar_issuetracker/issues/6598
For any given image/observation, we pull in important items of metadata like central frequency, bandwidth, time of observation, etc.
Howe…
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cf https://redmine.astron.nl/lofar_issuetracker/issues/3721
Although source association is well-tested for single-band data, we could use some quality assurance on multi-band datasets (although no pr…
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It would be nice to be able to use awimager via the 'im' module in pyxis - it would be useful for imaging Lofar data, for example.
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cf. https://support.astron.nl/lofar_issuetracker/issues/5228
@bartscheers wrote:
During a Trap run the runcat positions are updated every time. The intermediate results are not stored, we only have th…
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Hi everyone,
I'm using the `lofar-vlbi` pipeline for the first time. Thanks for all lthe effort, the documentation is great!
I installed the sigularity image, cloned the relevant repos, edited `…
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Hi,
I am trying to create MODEL_DATA column with Predict Mode using DDF inside pipeline.
I get this error and DDF dies, but memory is not full.
- 13:49:39 - ClassMS | P…
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Hi,
I'm having trouble with a rather non-descriptive error thrown during the pre_average step by python_plugin which I have copied below. It only occurs during some facets. My dataset is multi-epoc…
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We need to have a way to deal with position errors in AARTFAAC when using pyse.py/TraP. There are two options for this:
- convert extremes of the positions to position error
- assume zero error to beg…
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CF https://redmine.astron.nl/lofar_issuetracker/issues/6605,
https://redmine.astron.nl/lofar_issuetracker/issues/6606
Currently we display values for the band with highest flux in the most recent tim…
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This could be quite tricky, but is crucial to stand a chance of supporting optical and/or mosaic image data. (cf https://redmine.astron.nl/lofar_issuetracker/issues/6577).
Possible options include ba…