! ================================================================ ! Preferred Dynamic Contraints. Alter [defaults] as desired. ! ================================================================ ! Equipment constraints: ! Stations. Below each station code, the "o" indicates an ! [optional] station that is to be used if it is available. ! Change "o" to "r" if the station is required or change ! "o" to "n" if the station is not to be used. ! SC HN NL FD LA PT KP OV BR MK ! r r r r r r r r r r ! Minimum number of stations: 10 ! May we swap PT for a single VLA antenna? No ! Bands and polarizations. Below each band code, insert "R" ! if the righthand polarization is to be used, "L" if the ! lefthand polarization is to be used, "d" if dual ! polarizations are to be used, or "o" if the band is in ! your setups but scheduling should not be constrained by ! its availability. ! 90cm 50cm 20cm 13cm 6cm 4cm 2cm 1cm 7mm 3mm ! R ! Weather constraints: ! [appropriate for bands marked "L", "R", or "d" above ! and for at least the minimum number of stations] ! Date constraints: ! Preferred date(s), usually a series start: within the period ! 15-30 Jan. 2003 or 20 Feb. - 10 March 2003. ! Excluded dates plus reason: After March 10, 2003 (see ! special conditions below) ! Preferred interval between segments in days [none]: ! Special conditions (e.g., a series with different ! spacings in time): Experiment GC023B should be carried ! out 10-30 days apart from global VLBI experiment GC023A ! (currently scheduled for Feb. 10, 2003). ! ================================================================ ! ! file gc023b.key ! ! ================================================================ ! Control Information ! ================================================================ overwrite ! Prevents need to clean out old files on restart. autotape = 2 ! Automatic tape allocation on 2 drive stations. sumitem = early, dwell, el1, az1 ! Control items in summary file. ! ================================================================ ! Cover information (PI, experiment ...) ! ================================================================ version = 1 expt = 'Phase-reference astrometry of Compact Symmetric Objects' expcode = 'gc023b' obstype = 'VLBA' piname = 'Patrick Charlot' address1 = 'Observatoire de Bordeaux - CNRS' address2 = 'BP 89' address3 = '33270 Floirac' address4 = 'France' email = 'charlot@observ.u-bordeaux.fr' phone = '+33 5 57 77 61 41 (w) / +33 5 56 20 12 80 (h)' obsphone = '+33 5 57 77 61 41 (w) / +33 5 56 20 12 80 (h)' fax = '+33 5 57 77 61 10' obsmode = '128-4-2' note1 = 'fringe finders: DA193 and 3C454.3' note2 = 'amplitude check source: 1739+522' note3 = ' ' note4 = ' ' ! ================================================================ ! Correlator section ! ================================================================ correl = 'Socorro' coravg = 2 corchan = 16 cornant = 10 corpol = 'off' corwtfn = 'uniform' corsrcs = 'standard' cortape = 'dat' corship1 = 'Patrick Charlot' corship2 = 'Observatoire de Bordeaux - CNRS' corship3 = 'BP 89' corship4 = '33270 Floirac - France' ! ================================================================ ! Catalogs. These are the standard ones and are the defaults. ! ================================================================ srcfile = '$SCHED/catalogs/sources.vlba' stafile = '$SCHED/catalogs/stations.dat' ! ================================================================ ! Setup. ! ================================================================ setup = '$SCHED/setups/v4cm-128-4-2-R.set' ! ================================================================ ! The schedule ! ================================================================ ! Time intervals (dur, gap, dwell - but not prescan) are in ! sidereal units - shorter than UT units by ~1.0027. ! Start and stop times are in LST for the specified station, ! which is VLBA_PT for VLBI dynamic scheduling projects. ! The start day can be specified as the "local sidereal day", ! which is sort of like MJD, but for sidereal time. These days ! are listed on VLA schedules. The regular UT date can also be ! used (new feature). lst = VLBA_PT day = 59379 ! local sidereal day !year = 2003 month = 2 day = 10 start = 14:00:20 ! This is a phase referencing schedule with a lot of short scans. ! For dynamic scheduling, the key calibration scans should be ! toward the middle. Some time could be lost off either end. ! Drive antennas to phase calibrator then start nodding stations = SC, HN, NL, FD, LA, PT, KP, OV, BR, MK source = 'J1421+4645' dur = 60 gap = 120 / group = 2 repeat = 6 source = 'J1414+4554' dur = 240 gap = 0 / source = 'J1421+4645' dur = 60 gap = 0 / source = 'J1936+7131' dur = 90 gap = 60 / group = 2 repeat = 6 source = 'J1945+7055' dur = 240 gap = 0 / source = 'J1936+7131' dur = 60 gap = 0 / source = 'J2010+6116' dur = 80 gap = 0 / group = 2 repeat = 10 source = 'J2022+6136' dur = 60 gap = 0 / source = 'J2010+6116' dur = 60 gap = 0 / ! gap of 2 min for readback test source = 'J1421+4645' dur = 80 gap = 120 / group = 2 repeat = 6 source = 'J1414+4554' dur = 240 gap = 0 / source = 'J1421+4645' dur = 60 gap = 0 / ! amplitude calibrator source = '1739+522' dur = 110 gap = 60 / source = 'J1936+7131' dur = 110 gap = 0 / group = 2 repeat = 6 source = 'J1945+7055' dur = 240 gap = 0 / source = 'J1936+7131' dur = 60 gap = 0 / source = 'J2010+6116' dur = 80 gap = 0 / group = 2 repeat = 10 source = 'J2022+6136' dur = 60 gap = 0 / source = 'J2010+6116' dur = 60 gap = 0 / ! gap of 2 min for readback test source = 'J2125+0441' dur = 150 gap = 120 / group = 2 repeat = 6 source = 'J2130+0502' dur = 240 gap = 0 / source = 'J2125+0441' dur = 60 gap = 0 / source = 'J2217+0220' dur = 90 gap = 0 / group = 2 repeat = 6 source = 'J2212+0152' dur = 240 gap = 0 / source = 'J2217+0220' dur = 60 gap = 0 / source = 'J2125+0441' dur = 90 gap = 0 / group = 2 repeat = 6 source = 'J2130+0502' dur = 240 gap = 0 / source = 'J2125+0441' dur = 60 gap = 0 / source = 'J2217+0220' dur = 90 gap = 0 / group = 2 repeat = 6 source = 'J2212+0152' dur = 240 gap = 0 / source = 'J2217+0220' dur = 60 gap = 0 / source = 'J0004+4615' dur = 150 gap = 0 / group = 2 repeat = 6 source = 'J0003+4807' dur = 240 gap = 0 / source = 'J0004+4615' dur = 60 gap = 0 / ! gap of 2 min for readback test source = 'J1421+4645' dur = 60 gap = 120 / group = 2 repeat = 6 source = 'J1414+4554' dur = 240 gap = 0 / source = 'J1421+4645' dur = 60 gap = 0 / ! amplitude check source source = '1739+522' dur = 130 gap = 0 / source = 'J1936+7131' dur = 110 gap = 0 / group = 2 repeat = 6 source = 'J1945+7055' dur = 240 gap = 0 / source = 'J1936+7131' dur = 60 gap = 0 / source = 'J2010+6116' dur = 90 gap = 0 / group = 2 repeat = 10 source = 'J2022+6136' dur = 60 gap = 0 / source = 'J2010+6116' dur = 60 gap = 0 / ! gap of 2 min for readback test source = 'J2125+0441' dur = 130 gap = 120 / group = 2 repeat = 6 source = 'J2130+0502' dur = 240 gap = 0 / source = 'J2125+0441' dur = 60 gap = 0 / source = 'J2217+0220' dur = 90 gap = 0 / group = 2 repeat = 6 source = 'J2212+0152' dur = 240 gap = 0 / source = 'J2217+0220' dur = 60 gap = 0 / ! fringe finder source = '3C454.3' dur = 280 gap = 0 / source = 'J0004+4615' dur = 150 gap = 0 / group = 2 repeat = 6 source = 'J0003+4807' dur = 240 gap = 0 / source = 'J0004+4615' dur = 60 gap = 0 / source = 'J0419+3955' dur = 70 gap = 90 / group = 2 repeat = 10 source = 'J0427+4133' dur = 60 gap = 0 / source = 'J0419+3955' dur = 60 gap = 0 / source = 'J1936+7131' dur = 80 gap = 60 / group = 2 repeat = 6 source = 'J1945+7055' dur = 240 gap = 0 / source = 'J1936+7131' dur = 60 gap = 0 / ! amplitude check source source = '1739+522' dur = 110 gap = 0 / source = 'J2010+6116' dur = 110 gap = 0 / group = 2 repeat = 10 source = 'J2022+6136' dur = 60 gap = 0 / source = 'J2010+6116' dur = 60 gap = 0 / ! gap of 2 min for readback test source = 'J2125+0441' dur = 140 gap = 120 / group = 2 repeat = 6 source = 'J2130+0502' dur = 240 gap = 0 / source = 'J2125+0441' dur = 60 gap = 0 / source = 'J2217+0220' dur = 90 gap = 0 / group = 2 repeat = 6 source = 'J2212+0152' dur = 240 gap = 0 / source = 'J2217+0220' dur = 60 gap = 0 / source = 'J0004+4615' dur = 100 gap = 60 / group = 2 repeat = 6 source = 'J0003+4807' dur = 240 gap = 0 / source = 'J0004+4615' dur = 60 gap = 0 / source = 'J0419+3955' dur = 100 gap = 80 / group = 2 repeat = 10 source = 'J0427+4133' dur = 60 gap = 0 / source = 'J0419+3955' dur = 60 gap = 0 / ! gap of 2 min for readback test source = 'J0753+5352' dur = 60 gap = 120 / group = 2 repeat = 6 source = 'J0754+5324' dur = 240 gap = 0 / source = 'J0753+5352' dur = 60 gap = 0 / source = 'J1936+7131' dur = 130 gap = 0 / group = 2 repeat = 6 source = 'J1945+7055' dur = 240 gap = 0 / source = 'J1936+7131' dur = 60 gap = 0 / source = 'J2010+6116' dur = 80 gap = 0 / group = 2 repeat = 10 source = 'J2022+6136' dur = 60 gap = 0 / source = 'J2010+6116' dur = 60 gap = 0 / source = 'J0004+4615' dur = 130 gap = 0 / group = 2 repeat = 6 source = 'J0003+4807' dur = 240 gap = 0 / source = 'J0004+4615' dur = 60 gap = 0 / ! gap of 2 min for readback test source = 'J0419+3955' dur = 160 gap = 120 / group = 2 repeat = 10 source = 'J0427+4133' dur = 60 gap = 0 / source = 'J0419+3955' dur = 60 gap = 0 / source = 'J0753+5352' dur = 100 gap = 60 / group = 2 repeat = 6 source = 'J0754+5324' dur = 240 gap = 0 / source = 'J0753+5352' dur = 60 gap = 0 / source = 'J0004+4615' dur = 120 gap = 60 / group = 2 repeat = 6 source = 'J0003+4807' dur = 240 gap = 0 / source = 'J0004+4615' dur = 60 gap = 0 / ! fringe finder source = '0552+398' dur = 300 gap = 60 / source = 'J0419+3955' dur = 160 gap = 0 / group = 2 repeat = 10 source = 'J0427+4133' dur = 60 gap = 0 / source = 'J0419+3955' dur = 60 gap = 0 / ! gap of 2 min for readback test source = 'J0753+5352' dur = 60 gap = 120 / group = 2 repeat = 12 source = 'J0754+5324' dur = 240 gap = 0 / source = 'J0753+5352' dur = 60 gap = 0 / source = 'J0419+3955' dur = 140 gap = 60 / group = 2 repeat = 20 source = 'J0427+4133' dur = 60 gap = 0 / source = 'J0419+3955' dur = 60 gap = 0 / source = 'J0753+5352' dur = 90 gap = 60 / group = 2 repeat = 6 source = 'J0754+5324' dur = 240 gap = 0 / source = 'J0753+5352' dur = 60 gap = 0 / ! gap of 2 min for readback test source = 'J1421+4645' dur = 60 gap = 120 / group = 2 repeat = 12 source = 'J1414+4554' dur = 240 gap = 0 / source = 'J1421+4645' dur = 60 gap = 0 / source = 'J0753+5352' dur = 90 gap = 60 / group = 2 repeat = 6 source = 'J0754+5324' dur = 240 gap = 0 / source = 'J0753+5352' dur = 60 gap = 0 / ! gap of 2 min for readback test source = 'J1421+4645' dur = 60 gap = 120 / group = 2 repeat = 6 source = 'J1414+4554' dur = 240 gap = 0 / source = 'J1421+4645' dur = 60 gap = 0 / source = 'J1936+7131' dur = 150 gap = 0 / group = 2 repeat = 12 source = 'J1945+7055' dur = 240 gap = 0 / source = 'J1936+7131' dur = 60 gap = 0 / ! amplitude check source source = '1739+522' dur = 100 gap = 0 / source = 'J0753+5352' dur = 70 gap = 60 / group = 2 repeat = 5 source = 'J0754+5324' dur = 240 gap = 0 / source = 'J0753+5352' dur = 60 gap = 0 / ! end file gc023b.key source = 'J1421+4645' dur = 60 gap = 0 record / group = 2 repeat = 6 source = 'J1414+4554' dur = 240 gap = 0 / source = 'J1421+4645' dur = 60 gap = 0 / ! amplitude check source source = '1739+522' dur = 80 gap = 60 / source = 'J1936+7131' dur = 100 gap = 0 / group = 2 repeat = 6 source = 'J1945+7055' dur = 240 gap = 0 / source = 'J1936+7131' dur = 60 gap = 0 / source = 'J2010+6116' dur = 80 gap = 0 / group = 2 repeat = 10 source = 'J2022+6136' dur = 60 gap = 0 / source = 'J2010+6116' dur = 60 gap = 0 / source = 'J0753+5352' dur = 60 gap = 60 / group = 2 repeat = 6 source = 'J0754+5324' dur = 240 gap = 0 / source = 'J0753+5352' dur = 60 gap = 0 / ! gap of 2 min for readback test