! ================================================================
!   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   o   o   r   r   r   r
!       Minimum number of stations [8 (6 for 3mm)]: 9
!       May we swap PT for a single VLA antenna? [yes] 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
!     minimum number of stations] 9
! Date constraints:
!    Preferred date (Fixed) 2008 Feb 29, UT 23 - Mar 01, UT 07

! ================================================================
overwrit
autotape = 2
version  = 1
expt     = 'Y27 Test'
expcode  = ty007a
obstype  = VLBA

piname   = 'Michael Rupen'
address1 = 'NRAO AOC'
address2 = 'Socorro, NM '
address3 = 'U.S.A.'
phone    = '505 835-7248'
obsphone = '505 232-6710'
email    = 'mrupen@nrao.edu'
fax      = '505 835-7027'
obsmode  = '3.6cm, 6cm'
note1    = ' '
! ==============  Correlator Information  ==================                    
!                                                                               
correl   = 'Socorro'
coravg   = 2.0
corchan  = 16 
cornant  = 12
corpol   = on 
corwtfn  = 'uniform'
corsrcs  = 'standard'
cortape  = 'DAT'
corship1 = 'Michael Rupen'
corship2 = 'AOC'
corship3 = 'Socorro'

! ==================== Setup Information ===================                    

srccat /

  ! taken from bd105e
  source='CYGX1' ra=19:58:21.6744 dec=+35:12:05.758  equinox='J2000' /

  ! taken from BD117J
  source='N0239+6005' RA=02:39:37.95235    DEC=+60:05:41.9112    equinox='J2000' /

endcat /

! ==================== Scan Information ===================
minpause   300
year = 2008
month = 04
day = 03
start = 19:00:00

stations = SC, HN, NL, FD, LA, PT, KP, OV, BR, MK, VLA27
setup = $SCHED/setups/v4cm-256-8-2.set 

source='J0136+4751'     dur= 600 vlamode='VA' /
source='J0137+3309'     dur= 200 vlamode='VA' / ! 3C48


! Check very faint sources
source='J1957+3338' dur= 300 vlamode='VA' / Vivek's calibrator for CygX-1
  source='CYGX1'      dur= 100 vlamode='VA' / 
  source='J1957+3338' dur=  80 vlamode='VA' / Vivek's calibrator for CygX-1

source='N0239+6005' dur= 240 vlamode='VA' / ! 0.12 Jy @ X -- LSI calibrator

! Check different DS:
! - 4 groups (10, 3.3, 1.7, 0.4 sec)
! - 5 fs scans in each
! - Interleave with VA scans on our 2ndary source, each 3 mins, DS=10 as a check
! --> 4 x (5x160+80+120)= 4 x 16.7mins= 66.7 mins

! 10s integrations, all VA, enough time on-source to allow for VA
!  ...note that VA mode means you ALWAYS lose the 1st 30s of the VA scan!!!
!  boy is that annoying...
group 2 rep=4
  source='J0136+4751'     dur=  90 vlamode='VA' /
  source='J0154+4743'     dur=  90 vlamode='VA' /
source='J0136+4751'     dur=  90 vlamode='VA' /

! 10s integrations
group 2 rep=4
  source='J0136+4751'     dur=  90 vlamode='VA' /
  source='J0154+4743'     dur=  90 vlamode='VX' /
source='J0136+4751'     dur=  90 vlamode='VA' /

source='J0154+4743'     dur= 120 vlamode='VA' /

! 3.3s integrations
group 2 rep=4
  source='J0136+4751'     dur=  90 vlamode='VA' /
  source='J0154+4743'     dur=  90 vlamode='VX' /
source='J0136+4751'     dur=  90 vlamode='VA' /

source='J0154+4743'     dur= 120 vlamode='VA' /

! 1.7s integrations
group 2 rep=4
  source='J0136+4751'     dur=  90 vlamode='VA' /
  source='J0154+4743'     dur=  90 vlamode='VX' /
source='J0136+4751'     dur=  90 vlamode='VA' /

source='J0154+4743'     dur= 120 vlamode='VA' /

! Check shorter switching times
! 10s integrations ; OBSERVE claims ~45s to switch sources
!
group 2 rep=4
  source='J0136+4751'     dur=  70 vlamode='VA' /
  source='J0154+4743'     dur=  70 vlamode='VX' /
source='J0136+4751'     dur=  70 vlamode='VA' /

source='J0154+4743'     dur= 120 vlamode='VA' /

group 2 rep=4
  source='J0136+4751'     dur=  60 vlamode='VA' /
  source='J0154+4743'     dur=  60 vlamode='VX' /
source='J0136+4751'     dur=  60 vlamode='VA' /

! group 2 rep=4
!   source='J0136+4751'     dur=  55 vlamode='VA' /
!   source='J0154+4743'     dur=  55 vlamode='VX' /
! source='J0136+4751'     dur=  55 vlamode='VA' /

group 2 rep=4
  source='J0136+4751'     dur=  50 vlamode='VA' /
  source='J0154+4743'     dur=  50 vlamode='VX' /
source='J0136+4751'     dur=  50 vlamode='VA' /

! Check fainter & VLA-only sources
source='J0136+4751' dur=  90 vlamode='VA' /
source='J0128+4901' dur= 120 vlamode='VA' / ! 0.24 Jy; not VLA cal.
source='J0132+4325' dur= 120 vlamode='VA' / ! 0.24 Jy; W VLA cal. at 7mm; C-VCS1 says 0.17-0.13 Jy @ X
source='J0125+4718' dur= 120 vlamode='VA' / ! 0.20-0.18 Jy @ X C-VCS1
source='J0140+4658' dur= 120 vlamode='VA' / ! 0.08-0.09 Jy; not VLA cal.
source='J0136+4751' dur=  90 vlamode='VA' /