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Dear designated AIP,</div>
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I am a PhD student at ASTRON and Radboud University, working with my supervisor, Dr. Pikky Atri (cc’ed), on reducing VLBA data using AIPS. However, I’ve encountered some issues related to flagging, and I would appreciate your advice.</div>
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In my data, there are sudden variations in the system temperature, which I have flagged using UVFLG (see figure
<b>BM500_SystemTemperatureSpikes.png</b> in the attachments). </div>
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When I run the task VLBAAMP, the output indicates that the subtask ACSCL is using the FG table I created. However, upon examining the CL table with the gain corrections produced by VLBAAMP, it does not seem like any areas have been flagged, i.e., the flagged
spikes still persist (see figure <b>BM500_PersistentAmplitudeSpikes</b> in the attachments).</div>
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To circumvent this, I attempted to flag the TY table directly using SNEDT. This created a new version of the TY table with the flagged areas removed. However, running VLBAAMP again results in the same outcome, with the flagged areas seemingly not being applied.</div>
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At this point, the only way forward I can see is to flag the CL table produced by VLBAAMP. However, this would mean the sudden variations in system temperature would have already influenced the amplitude calibration, which is not ideal.</div>
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Am I missing something in the procedure, or could this be a potential issue in AIPS?</div>
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Thank you for your time and for maintaining AIPS!</div>
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Kind regards,</div>
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Lieuwe de Regt</div>
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