! ================================================================
!   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
!           o   o   o   o   o   o   o   o   n   o
!       Minimum number of stations [9 (6 for 3mm)]: 8 but no more
!           than 2 out from SW array (FD, LA, PT, KP)
!       May we swap PT for a single VLA antenna? [yes] no
!          Consult http://www.aoc.nrao.edu/~gtaylor/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
! Weather constraints:
!    we'll take weather appropriate for 2cm rather than 1cm at
!    any station; the observation should NOT be limited
!    by weather at SC.
! Date constraints:
!    Preferred date(s), usually a series start [none]: as soon as possible
!    Excluded dates plus reason [none]:
!    Preferred interval between segments in days [none]:  30 days
!    Special conditions (e.g., a series with different
!       spacings in time) [none]:
! ================================================================
! BS102 H2O Masers in IRAS16342
overwrit
autotape=2
! ==========================================================
! =================  Cover Information  ====================
! ==========================================================
version  = 1 
expt     = 'H2O masers in IRAS16342-3814'
expcode  = bc184k 
obstype  = VLBA
piname   = 'Mark Claussen'    
address1 = 'National Radio Astronomy Observatory'  
address2 = 'P. O. Box O'                           
address3 = 'Socorro, New Mexico, 87801'
address4 = ' U.S.A. '
phone    = '505 835 7284 '    
obsphone = '505 835 7284 '     
email    = 'mclausse@aoc.nrao.edu'  
fax      = '505 835 7027 '   
obsmode  = 'Line'
correl   = 'Socorro'
obsmode  = '1.3 cm VLBA non-standard correlator setup' 
! ================================================================
!       In line source catalog.
! ================================================================
srccat /
equinox =J2000
! from proposal:
calcode=' '
source='IRAS16342' ra=16:37:39.958  dec=-38:20:17.165 
        vel=+176.0,+88.0,+1.0,-86.0 /

SOURCE='J1626-2951','1622-297','J1626-29'
     RA=16:26:06.0208473 DEC= -29:51:26.971308 CALCODE='N'
     REMARKS='USNO - Ref Frame 1998-6, Eubanks June 1998' /

SOURCE='J1733-1304','1730-130','J1733-13','NRAO530'
     RA=17:33:02.7057824 DEC= -13:04:49.548279 CALCODE='N'
     REMARKS='USNO - Ref Frame 1998-6, Eubanks June 1998' /

endcat /

! ==========================================================
! ==============  Correlator Information  ==================
! ==========================================================

correl   = 'Socorro'
coravg   = 1.6
corchan  = 512
cornant  = 9
corpol   = 'off'
corwtfn  = 'uniform'
corsrcs  = 'VLBA Data Base'
cortape  = DAT
corship1 = 'M. Claussen'
corship2 = 'P. O. Box O'
corship3 = 'Socorro NM 87801'
cornote1 = 'Positions from schedule for target '
!

! ==========================================================
! ==================== Setup Information ===================
! ==========================================================
!  These are bare minimum setup "files" that use defaults from
!  the frequency catalog.  
!  The first even defaults the BBC numbers and sidebands.
!  This still requires getting the frequencies right for the
!  scheme that SCHED chooses and is not really recommended.




lineinit /
lineset ='H2O'  restfreq=22235.08, 22235.08, 22235.08, 22235.08 /
endlines /

setinit = bc184.set /
   nchan    = 4   
   freqref  = 22235.08
   freqoff  = 0.0, 6.0, 12.0, 18.0
   bbfilter = 8.0, 8.0, 8.0, 8.0
   netside  = U, U, U, U
   bits     = 2  
   pol      = 'lcp'
   format   = VLBA
   /
endset /



! ==========================================================
! ========================  The Schedule  ==================
! ==========================================================
!year  = 2008 month = 02 
day = 61237
start = 13:30:00
lst = 'vlba_pt'
!
doppler
stations = SC, HN, NL, FD, LA, PT, KP, OV, MK
setup = bc184.set
linename='h2o'
bw = 8.0, 8.0, 8.0, 8.0
pcal = off
! minpause = 32
!
! Drive antennas to fringe finder
!
source = 'J1626-2951' dopsrc='iras16342' gap=0 dur=100 norecord /
!
! Start observing sources
        source = 'J1626-2951' dopsrc='IRAS16342' gap=0 dwell=300 record /

group = 1 repeat = 4
        source= 'IRAS16342' dwell = 900 /     

        source = 'J1733-1304' dopsrc='IRAS16342' gap=0 dwell=300 record /

group = 1 repeat = 4
        source= 'IRAS16342' dwell = 900 /     
	
! source = 'J1733-1304' dopsrc='IRAS16342' dwell=300 /

group = 1 repeat = 6
        source= 'IRAS16342' dwell = 900 /     

! 
!        source = 'J1733-1304' dopsrc='IRAS16342' gap=0 dwell=300 record /

group = 1 repeat = 4
        source= 'IRAS16342' dwell = 900 /     

source = 'J1733-1304' dopsrc='IRAS16342' dwell=300 /

group = 1 repeat = 4
        source= 'IRAS16342' dwell = 900 /     

source = 'J1733-1304' dopsrc='IRAS16342' dwell=300 /