! ================================================================ ! Preferred Dynamic Constraints. 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 o o o o o o o o r ! Minimum number of stations [9 (6 for 3mm)]: 9 ! May we swap PT for a single VLA antenna? NO ! Consult http://www.aoc.nrao.edu/~lsjouwer/y1gotcha.html ! to decide. If you adopt the default, then both PT and ! VLA1 must be in the stations list in the keyin file. ! 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 ! L L ! ! Weather constraints: ! Please observe following the proposed frequency of one ! observation every six weeks. This is crucial for the ! scientific success of the experiment ! ! RECONSIDERED FROM: ! Good weather at least at the middle of the continental US, ! for a low-declination source observed with phase-ref at 1cm and 7mm. ! We are aware of the recommendation of having better weather ! by the scheduling committee, but we want to have high-quality ! data at 1cm and 7mm even at the price of a sparser time sampling of ! the radio source. ! ! Date constraints: ! Preferred date(s), usually a series start [none]: ! Excluded dates plus reason [none]: ! Preferred interval between segments in days: ! 40 days (6 weeks requested), important for densely sampled source ! monitoring ! Special conditions (e.g., a series with different ! spacings in time) [none]: ! ================================================================ version = 2 expt = 'NGC1052, the Key to Explore the Disk-Jet Connection in AGN' expcode = br130d piname = 'Eduardo Ros' address1 = 'Max-Planck-Institut fuer Radioastronomie' address2 = 'Auf dem Huegel 69' address3 = 'D-53121 Bonn' address4 = ' Germany ' phone = '+49-228-525292' obsphone = '+49-228-7667213' email = ros@mpifr-bonn.mpg.de fax = '+49-228-525229' obsmode = '13 & 7mm 256-8-2-L-UL ' obstype = VLBA note1 = ' ' ! correl = Socorro coravg = 2 corchan = 16 cornant = 10 corpol = off corwtfn = uniform corsrcs = standard cortape = DAT corship1 = 'Eduardo Ros' corship2 = 'MPIfR, Auf dem Huegel 69' corship3 = 'D-53121 Bonn, Germany' cornote1 = ' ' ! overwrit ! autotape = 2 ! minpause = 30 ! Minimum playback tape stop duration. ! prestart = 20 ! Start tapes this long before scan start. sumitem = el1, dwell, tape1, tpstart stafile = $SCHED/catalogs/stations.dat srcfile = $SCHED/catalogs/sources.vlba freqfile = $SCHED/catalogs/freq.dat ! ! setup = '$SCHED/setups/v13m-256-8-2-L-UL.set' ! stations= VLBA_SC, VLBA_HN, VLBA_NL, VLBA_FD, VLBA_LA, VLBA_PT, VLBA_KP, VLBA_OV, VLBA_BR, VLBA_MK ! pcal='1MHz' LST='VLBA_PT' day = 60180 start=23:50:00 ! Bring antennas to fringe finder setup = '$SCHED/setups/v1cm-256-8-2-L-UL.set' source='IIIZW2' dwell = 05:00 / setup = '$SCHED/setups/v7mm-256-8-2-L-UL.set' source='IIIZW2' dwell = 05:00 / ! Start nodding group=10 repeat=19 setup = '$SCHED/setups/v1cm-256-8-2-L-UL.set' source='NGC1052' dur=60 gap=08:50 / source='J0243-0550' dur=30 gap=0 / source='NGC1052' dwell=60 / source='J0243-0550' dwell=30 / source='NGC1052' dwell=60 / setup = '$SCHED/setups/v7mm-256-8-2-L-UL.set' source='NGC1052' dwell=50 / source='J0243-0550' dwell=25 / source='NGC1052' dwell=50 / source='J0243-0550' dwell=25 / source='NGC1052' dwell=50 / source='J0243-0550' dwell=25 / source='NGC1052' dwell=50 / ! Another fringe finder setup = '$SCHED/setups/v1cm-256-8-2-L-UL.set' source='0420-014' dwell = 05:00 / setup = '$SCHED/setups/v7mm-256-8-2-L-UL.set' source='0420-014' dwell = 05:00 /