Comments (6)
I like your terminology :-)
While this is a good workaround, the real solution we are working towards is a prescriptive sensor as opposed to a descriptive one. We want to know what the telescope is supposed to do, and don't care what it's actually doing... This will introduce a subarray-level activity sensor (obs_activity
, most likely). Any antenna that disagrees with the plan can then be flagged as required.
The problem with the herd approach is that some experiments have the dishes legitimately doing different things - think holography.
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Yes . the idea being that the data is split into scans based on what the telescope was meant to do. but then the data is flagged based on what each telescope was doing. This should not be to hard to do since we already have activity flagging per antenna / per baseline .
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@ludwigschwardt yup that sounds even better :)
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Now that we have an obs_activity
sensor I'm going to base the scan boundaries on that instead. The dishes are already "quack-flagged" when they are not on target.
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Please test the latest katdal 0.12 and let me know if that solves your problem :-)
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Can we close this?
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