!
OVERWRITE
autotape = 2
!
! SCHED file for 22 GHz water/12.2 GHz methanol observations of CEP A
! total 4x10 hours at LST 23.0. 
! This is the version for the H2O masers, 5 hours at LST 20.5
! 4 epochs 
! 
! ================================================================
!   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   r   r   r   r   r   o   o
!       Minimum number of stations [9 (6 for 3mm)]: 8
!       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
!                                         d          d
! 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 [none]:
!    Excluded dates plus reason [none]:
!    Preferred interval between segments in days [none]: 120
!    Special conditions (e.g., a series with different
!       spacings in time) [none]: preferably within 14 days of methanol obs.
! ================================================================
!
VERSION = 2.0
EXPT = 'Co-evolution of Methanol and Water maser filaments (CEP A HW2)'
EXPCODE = 'BV059aa'
OBSTYPE = 'VLBA'
OBSMODE = 'VLBA'
STATIONS = VLBA_SC, VLBA_HN, VLBA_NL, VLBA_FD, VLBA_LA,
           VLBA_PT, VLBA_KP, VLBA_OV, VLBA_BR, VLBA_MK
PINAME   = 'Wouter Vlemmings'
ADDRESS1 = 'Jodrell Bank Observatory'
ADDRESS2 = 'The University of Manchester'
ADDRESS3 = 'Macclesfield, Cheshire SK11 9DL'
ADDRESS4 = 'United Kingdom'
PHONE    = '+44 - 1477 572635'
OBSPHONE = ''
FAX      = '+44 - 1477 572649'
EMAIL    = 'wouter@jb.man.ac.uk'
NOTE1    = 'Make sure Pulse CAl is Off'
NOTE2    = 'This is mixed bandwidth observing'
NOTE3    = '22 GHz with 4 MHz/1 MHz'
!
correl   = 'Socorro'
coravg   = 2
corchan  = 128
cornant  = 10
corpol   = 'on'
corwtfn  = 'uniform'
corsrcs  = 'standard'
cortape  = DAT
corship1 = 'Wouter Vlemmings'
corship2 = 'Jodrell Bank Observatory, The University of Manchester'
corship3 = 'Macclesfield, Cheshire SK11 9DL'
corship4 = 'United Kingdom'
cornote1 = 'mixed bandwidth'
!
!
SRCCAT /
SOURCE='CEPAHW2'  RA=22:56:18.104 DEC= 62:01:49.419 EQUINOX='J2000
    vel = -11.0 /
!SOURCE='J2232+6249' RA=22:32:22.8655 DEC= 62:49:36.436 EQUINOX='J2000' /
!SOURCE='J2302+6405' RA=23:02:41.315002 DEC= 64:05:52.84927 EQUINOX='J2000' /
ENDCAT /
!
! ==========================================================
! ==============  Spectral line rest frequecies  ===========
! ==========================================================
! H2O restfreq 22235.081
! CH3OH restfreq 12178.595
!
lineinit /
lineset='H2O'  restfreq= 22232.081, 22232.081, 22234.581, 22234.581,
                          22235.581, 22235.581, 22238.081, 22238.081  /
endlines /
!
setinit = bv059h2o.set /                                 
! 
nchan = 8  samprate = 8.0  bits = 2  ! 128 Mbps 
format = 'VLBA1:2'  
! 
freqref  = 22230.08,22230.08,22234.08,22234.08,22235.08,22235.08,22236.08,22236.08
bbfilter =     4.0,    4.0,    1.0,    1.0,    1.0,    1.0,    4.0,    4.0
pol      =     rcp,    lcp,    rcp,    lcp,    rcp,    lcp,    rcp,    lcp
pcal     = 'off'
station  = VLBA  /
!
endset /
!
!
LST = VLBA_PT
!
DAY = 60552
!
START = 18:00:00
!
setup = 'bv059h2o.set'
!
doppler linename='h2o'
!
SOURCE = '3C345'        prescan = 00:02:00 dur = 00:11:00 dopsrc 'CEPAHW2' /
!
source = 'J2232+6249'	prescan = 00:02:00 dur = 00:02:30 dopsrc 'CEPAHW2'/
source = 'J2302+6405'	prescan = 00:00:00 dur = 00:02:30 dopsrc 'CEPAHW2'/
!
group 3 rep 16
source = 'J2232+6249'	prescan = 00:00:00 dur = 00:00:45 dopsrc 'CEPAHW2'/
SOURCE = 'CEPAHW2' 	prescan = 00:00:00 dur = 00:00:45 dopsrc 'CEPAHW2' /
source = 'J2302+6405'	prescan = 00:00:00 dur = 00:00:45 dopsrc 'CEPAHW2'/
!
source = 'J2202+4216'	prescan = 00:01:00 dur = 00:11:00 dopsrc 'CEPAHW2'/
!
source = 'J2232+6249'	prescan = 00:01:00 dur = 00:02:30 dopsrc 'CEPAHW2'/
source = 'J2302+6405'	prescan = 00:00:00 dur = 00:02:30 dopsrc 'CEPAHW2'/
!
group 3 rep 16
source = 'J2232+6249'	prescan = 00:00:00 dur = 00:00:45 dopsrc 'CEPAHW2'/
SOURCE = 'CEPAHW2' 	prescan = 00:00:00 dur = 00:00:45 dopsrc 'CEPAHW2' /
source = 'J2302+6405'	prescan = 00:00:00 dur = 00:00:45 dopsrc 'CEPAHW2'/
!
SOURCE = '3C48'         prescan = 00:02:00 dur = 00:11:00 dopsrc 'CEPAHW2' /
!
group 4 rep 4
source = 'J2202+4216'	prescan = 00:01:00 dur = 00:11:00 dopsrc 'CEPAHW2'/
SOURCE = 'CEPAHW2' 	prescan = 00:01:00 dur = 00:11:00 dopsrc 'CEPAHW2' /
SOURCE = 'CEPAHW2' 	prescan = 00:00:00 dur = 00:11:00 dopsrc 'CEPAHW2'/
SOURCE = 'CEPAHW2' 	prescan = 00:00:00 dur = 00:11:00 dopsrc 'CEPAHW2'/
!
SOURCE = '3C48'         prescan = 00:02:00 dur = 00:11:00 dopsrc 'CEPAHW2' /
!