Scan Timing
The scan timing determines the length of the scan, either in LST (sidereal) or in UT. The difference is about ten seconds in an hour. It is probably best for everyone to leave keep your schedule in LST when observing with the EVLA only. Options are to set the exact time the scan has to end ("Stop Time", only useful for fixed date schedules), the total (maximum) time the scan may take from the end of the previous scan including telescope slewing time ("Duration"), or the time the telescopes should track the source regardless of telescope slewing time ("On Source", previously known as "Dwell"). Dynamically allocated observing time schedules must be in "Duration (LST)". Note that in the end, the duration of the SB should be an integer multiple of 30 LST minutes (or slightly less).

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