! SAMPLE SCHED INPUT FOR VLA SPECIFIC EXPERIMENT PLANNING ! ! This file is a close cousin to egplan.key with the main difference ! being in the station list. It is used to determine when sources ! are up, plot UV coverage, help find calibrators etc. ! This file shows how to use SCHED to determine times when sources ! are available, possible uv coverage, sky distribution etc. ! ! OPTMODE=UPTIME is used to generate a psuedo schedule in which ! each source has a day long string of scans, all on the same ! day. The summary file and the plotting capabilities can then ! be used to obtain the desired planning information. ! Note, SCHED will not make telescope control files when ! OPTMODE=UPTIME because the time order of scans is not enforced. ! ! Start SCHED interactively and specify the line (without the !): ! plot schedule=planvla.key / ! --------------------------------------------------------------- overwrit ! Prevents need to clean out old files expcode = yplan obstype = NONE version = 1 ! Optional cover stuff (with obstype=none) piname = 'Craig Walker' correl = 'Socorro' expt = ' Make uv plots' stafile = $SCHED/catalogs/stations_VLA.dat srcfile = $SCHED/catalogs/sources.vlba nosetup ! List the desired pads. Recall that SCHED has a 22 station limit ! as of April 1998. It is easy to change the limit so it can be ! increased if requests are sent to cwalker. "It's only memory". stations = E8,E16,E24,E32,E40,E48,E56,E64,E72, W8,W16,W24,W32,W40,W48,W56,W64,W72, N8,N16,N24,N32,N40,N48,N56,N64,N72 vlamode = VS ! VLA needs something. sumitem = el1, az1, ha1, pa1 ! Show these items in the summary. optmode = uptime ! Show source availability. All sources same day. opdur = 24:00:00 ! Total time range covered. opminant = 1 ! Source must be up at this many antennas. opminel = 15 ! Minimum elevation for source to be "up". year = 1997 month = 12 day = 10 start = 00:00:00 dur = 15:00 gap 0:00 ! Length and spacing of dummy scans. ! Give one scan per source for which information is desired. source = 3C84 / source = DA193 / source = 3C120 / source = 3C273 /