Introduction
This appendix does not directly relate to the OPT but does expect you are familiar with it and with its jargon.
Starting with the WIDAR observations in the spring of 2010, the majority of observing with the EVLA will be done by dynamically allocating observing time to the most appropriate SB in the observing queue. Here "most appropriate" typically depends on scientific priority, weather conditions and state of the array. This appendix describes some considerations and choices that might increase your chances to get more of your SBs observed successfully. This assumes that your scientific objectives can be met with a flexible approach while competing with other projects for the LST range to be observed.
Important note: for line observations currently (as of March 2010) there are restrictions on Doppler tracking. See section A.3.

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