! Started logfile: /scr/pima/rdv96_uvs/J1409-2657_S_uvs.log on Sat Dec 21 00:24:26 2013
obs /scr/pima/rdv96_uvs/J1409-2657_S_uva.fits
! Reading UV FITS file: /scr/pima/rdv96_uvs/J1409-2657_S_uva.fits
! AN table 1: 13 integrations on 28 of 28 possible baselines.
! AN table 2: 13 integrations on 36 of 36 possible baselines.
! AN table 3: 5 integrations on 28 of 28 possible baselines.
! AN table 4: 5 integrations on 21 of 21 possible baselines.
! Apparent sampling: 0.871866 visibilities/baseline/integration-bin.
! Found source: J1409-2657
! 
! There are 4 IFs, and a total of 4 channels:
! 
!  IF  Channel    Frequency  Freq offset  Number of   Overall IF
!       origin    at origin  per channel   channels    bandwidth
!  ------------------------------------------------------------- (Hz)
!  01        1  2.23299e+09        8e+06          1        8e+06
!  02        2  2.26299e+09        8e+06          1        8e+06
!  03        3  2.35299e+09        8e+06          1        8e+06
!  04        4  2.37299e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 0 lines of history.
! 
! Reading 3756 visibilities.
select RR
! Selecting polarization: RR,  channels: 1..4
! Reading IF 1 channels: 1..1
! Reading IF 2 channels: 2..2
! Reading IF 3 channels: 3..3
! Reading IF 4 channels: 4..4
print "field_size =",field_size
! field_size = 1024 
print "field_cell =",field_cell
! field_cell = 0.4 
print "taper_size =",taper_size
! taper_size = 20 
![@/home/lpetrov/bin/rdv_muppet /scr/pima/rdv96_uvs/J1409-2657_S]
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.03
float dynam
dynam = 6.0
float soltime1
soltime1 = 800000
float soltime2
soltime2 = 15
float soltime3
soltime3 = 1
float thresh
thresh = 0.5
float win_mult
win_mult = 1.8
float old_peak
float new_peak
float flux_cutoff
selfant "",false
! 1:FD       self-cal  status=correctable  weight=1
! 1:HN       self-cal  status=correctable  weight=1
! 1:KP       self-cal  status=correctable  weight=1
! 1:LA       self-cal  status=correctable  weight=1
! 1:NL       self-cal  status=correctable  weight=1
! 1:PT       self-cal  status=correctable  weight=1
! 1:SC       self-cal  status=correctable  weight=1
! 1:WF       self-cal  status=correctable  weight=1
! 2:BR       self-cal  status=correctable  weight=1
! 2:FD       self-cal  status=correctable  weight=1
! 2:KP       self-cal  status=correctable  weight=1
! 2:LA       self-cal  status=correctable  weight=1
! 2:MK       self-cal  status=correctable  weight=1
! 2:NL       self-cal  status=correctable  weight=1
! 2:OV       self-cal  status=correctable  weight=1
! 2:PT       self-cal  status=correctable  weight=1
! 2:SC       self-cal  status=correctable  weight=1
! 3:BR       self-cal  status=correctable  weight=1
! 3:FD       self-cal  status=correctable  weight=1
! 3:KP       self-cal  status=correctable  weight=1
! 3:LA       self-cal  status=correctable  weight=1
! 3:MK       self-cal  status=correctable  weight=1
! 3:NL       self-cal  status=correctable  weight=1
! 3:OV       self-cal  status=correctable  weight=1
! 3:PT       self-cal  status=correctable  weight=1
! 4:BR       self-cal  status=correctable  weight=1
! 4:FD       self-cal  status=correctable  weight=1
! 4:KP       self-cal  status=correctable  weight=1
! 4:LA       self-cal  status=correctable  weight=1
! 4:MK       self-cal  status=correctable  weight=1
! 4:OV       self-cal  status=correctable  weight=1
! 4:PT       self-cal  status=correctable  weight=1
system "rm /tmp/ff.ff"
mapsize field_size, field_cell
! Map grid = 1024x1024 pixels with 0.400x0.400 milli-arcsec cellsize.
startmod
! Applying default point source starting model.
! Performing phase self-cal
! Adding 1 model components to the UV plane model.
! The established model now contains 1 components and 1 Jy
! 
! Correcting IF 1.
!  A total of 11 telescope corrections were flagged in sub-array 1.
!  A total of 11 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 2.
!  A total of 11 telescope corrections were flagged in sub-array 1.
!  A total of 11 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 3.
!  A total of 11 telescope corrections were flagged in sub-array 1.
!  A total of 11 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 4.
!  A total of 11 telescope corrections were flagged in sub-array 1.
!  A total of 11 telescope corrections were flagged in sub-array 2.
! 
! Fit before self-cal, rms=1.108522Jy  sigma=6.389273
! Fit after  self-cal, rms=0.535501Jy  sigma=2.915800
! clrmod: Cleared the established, tentative and continuum models.
! Redundant starting model cleared.
print "=== Flag out IVS stations"
! === Flag out IVS stations 
integer lun
string  cfg_file
lun = outfile ( "/tmp/ff.ff" ) 
do i=1,nsub
  do j=1,ntel(i)
    fprintf lun, "%s\n", telname(j,i)
    end do
  end do
close ( lun )
system "/home/lpetrov/bin/dimap_flag_process.csh /tmp/ff.ff"
![@/tmp/ff.ff \]
flag 1:WF
! Flagging baselines of antenna 1:WF in the currently selected channels.
![Exited script file: /tmp/ff.ff]
uvw 2,-1
! Uniform weighting binwidth: 2 (pixels).
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=2.906 mas, bmaj=7.793 mas, bpa=-9.225 degrees
! Estimated noise=3.30831 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (0, 0).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.372611 Jy
! Component: 100  -  total flux cleaned = 0.459117 Jy
! Total flux subtracted in 100 components = 0.459117 Jy
! Clean residual min=-0.010850 max=0.031475 Jy/beam
! Clean residual mean=0.000007 rms=0.003268 Jy/beam
! Combined flux in latest and established models = 0.459117 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 8 components and 0.459117 Jy
! 
! Correcting IF 1.
!  A total of 13 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 13 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 13 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 13 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.104722Jy  sigma=0.641730
! Fit after  self-cal, rms=0.104707Jy  sigma=0.641612
! Inverting map and beam 
! Estimated beam: bmin=2.906 mas, bmaj=7.793 mas, bpa=-9.225 degrees
! Estimated noise=3.30831 mJy/beam.
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0306269 Jy
! Component: 100  -  total flux cleaned = 0.0444992 Jy
! Total flux subtracted in 100 components = 0.0444992 Jy
! Clean residual min=-0.009943 max=0.009438 Jy/beam
! Clean residual mean=0.000052 rms=0.002328 Jy/beam
! Combined flux in latest and established models = 0.503616 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 21 components and 0.503616 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.093431Jy  sigma=0.557719
! Fit after  self-cal, rms=0.093439Jy  sigma=0.557682
! Inverting map 
print "=== Finished uniform weighting clean ==="
! === Finished uniform weighting clean === 
uvw 0,-1
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
win_mult = win_mult * 1.6
clean_niter = clean_niter * 2
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=3.933 mas, bmaj=10.35 mas, bpa=-9.308 degrees
! Estimated noise=2.08602 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0129018 Jy
! Component: 100  -  total flux cleaned = 0.0186532 Jy
! Component: 150  -  total flux cleaned = 0.0215057 Jy
! Component: 200  -  total flux cleaned = 0.0226847 Jy
! Total flux subtracted in 200 components = 0.0226847 Jy
! Clean residual min=-0.009432 max=0.008476 Jy/beam
! Clean residual mean=0.000039 rms=0.002212 Jy/beam
! Combined flux in latest and established models = 0.526301 Jy
! Performing phase self-cal
! Adding 28 model components to the UV plane model.
! The established model now contains 38 components and 0.526301 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.092188Jy  sigma=0.546235
! Fit after  self-cal, rms=0.092184Jy  sigma=0.546205
! Inverting map 
print "=== Finished natural weighting clean for VLBI sites ==="
! === Finished natural weighting clean for VLBI sites === 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   FD        0.97     HN        1.00     KP        1.04     LA        1.18     
!   NL        1.06     PT        1.02     SC        0.93     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.03     FD        1.00     KP        1.02     LA        1.20     
!   MK        0.92     NL        0.99     OV        1.00     PT        1.04     
!   SC        0.98     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.02     FD        1.00     KP        0.99     LA        1.19     
!   MK        0.93     NL        1.03     OV        1.00     PT        1.07     
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00     FD        1.00     KP        1.00     LA        1.17     
!   MK        0.90     OV        0.99     PT        1.07     
! 
! 
! Correcting IF 2.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   FD        1.06     HN        1.10     KP        1.02     LA        1.04     
!   NL        1.13     PT        1.05     SC        1.00     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.06     FD        1.04     KP        1.03     LA        1.07     
!   MK        1.01     NL        1.02     OV        1.05     PT        1.05     
!   SC        1.07     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.05     FD        1.05     KP        1.04     LA        1.05     
!   MK        1.00     NL        1.08     OV        1.05     PT        1.02     
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.07     FD        1.06     KP        1.00     LA        1.04     
!   MK        1.00     OV        1.03     PT        1.04     
! 
! 
! Correcting IF 3.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   FD        1.04     HN        1.02     KP        0.89     LA        0.98     
!   NL        1.16     PT        1.04     SC        0.95     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.96     FD        1.07     KP        0.90     LA        0.97     
!   MK        1.00     NL        1.05     OV        1.04     PT        1.06     
!   SC        0.97     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.06     FD        1.08     KP        0.89     LA        0.94     
!   MK        0.99     NL        1.07     OV        1.01     PT        1.06     
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.04     FD        1.06     KP        0.90     LA        0.97     
!   MK        1.01     OV        1.04     PT        1.02     
! 
! 
! Correcting IF 4.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   FD        1.05     HN        0.92     KP        0.84     LA        0.80     
!   NL        1.08     PT        0.94     SC        0.97     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.01     FD        1.09     KP        0.82     LA        0.83     
!   MK        1.09     NL        1.02     OV        0.90     PT        0.92     
!   SC        1.00     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.02     FD        1.08     KP        0.80     LA        0.85     
!   MK        1.11     NL        1.06     OV        0.88     PT        0.90     
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        0.98     FD        1.08     KP        0.86     LA        0.81     
!   MK        1.08     OV        0.84     PT        0.92     
! 
! 
! Fit before self-cal, rms=0.092184Jy  sigma=0.546205
! Fit after  self-cal, rms=0.067652Jy  sigma=0.372167
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=3.928 mas, bmaj=10.36 mas, bpa=-9.219 degrees
! Estimated noise=2.0911 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 1.88124e-05 Jy
! Component: 100  -  total flux cleaned = -0.000165349 Jy
! Component: 150  -  total flux cleaned = -0.00020617 Jy
! Component: 200  -  total flux cleaned = -0.000285547 Jy
! Total flux subtracted in 200 components = -0.000285547 Jy
! Clean residual min=-0.003429 max=0.003412 Jy/beam
! Clean residual mean=0.000006 rms=0.000751 Jy/beam
! Combined flux in latest and established models = 0.526015 Jy
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 50 components and 0.526015 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067573Jy  sigma=0.371934
! Fit after  self-cal, rms=0.067648Jy  sigma=0.371776
! Inverting map 
selfcal true, true, soltime1
! Performing amp+phase self-cal over 800000 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067648Jy  sigma=0.371776
! Fit after  self-cal, rms=0.067676Jy  sigma=0.371763
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=3.928 mas, bmaj=10.36 mas, bpa=-9.197 degrees
! Estimated noise=2.09115 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -2.53482e-05 Jy
! Component: 100  -  total flux cleaned = -0.000187427 Jy
! Component: 150  -  total flux cleaned = -0.000260529 Jy
! Component: 200  -  total flux cleaned = -0.000294676 Jy
! Total flux subtracted in 200 components = -0.000294676 Jy
! Clean residual min=-0.003450 max=0.003353 Jy/beam
! Clean residual mean=0.000006 rms=0.000743 Jy/beam
! Combined flux in latest and established models = 0.52572 Jy
selfcal
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 53 components and 0.52572 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067616Jy  sigma=0.371594
! Fit after  self-cal, rms=0.067611Jy  sigma=0.371580
flux_cutoff = imstat(rms) * dynam
! Inverting map 
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 7.78007e-05 Jy
! Component: 100  -  total flux cleaned = -8.34283e-05 Jy
! Component: 150  -  total flux cleaned = -0.000112781 Jy
! Component: 200  -  total flux cleaned = -0.000141001 Jy
! Total flux subtracted in 200 components = -0.000141001 Jy
! Clean residual min=-0.003459 max=0.003330 Jy/beam
! Clean residual mean=0.000006 rms=0.000739 Jy/beam
! Combined flux in latest and established models = 0.525579 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 60 components and 0.52558 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067569Jy  sigma=0.371475
! Fit after  self-cal, rms=0.067565Jy  sigma=0.371463
! Inverting map 
selfcal true, true, soltime2
! Performing amp+phase self-cal over 15 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067565Jy  sigma=0.371463
! Fit after  self-cal, rms=0.067439Jy  sigma=0.370398
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=3.929 mas, bmaj=10.36 mas, bpa=-9.16 degrees
! Estimated noise=2.09137 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -6.54247e-05 Jy
! Component: 100  -  total flux cleaned = -0.00022371 Jy
! Component: 150  -  total flux cleaned = -0.000252379 Jy
! Component: 200  -  total flux cleaned = -0.000279509 Jy
! Total flux subtracted in 200 components = -0.000279509 Jy
! Clean residual min=-0.003477 max=0.003027 Jy/beam
! Clean residual mean=0.000004 rms=0.000724 Jy/beam
! Combined flux in latest and established models = 0.5253 Jy
selfcal
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 63 components and 0.5253 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067400Jy  sigma=0.370299
! Fit after  self-cal, rms=0.067400Jy  sigma=0.370290
flux_cutoff = imstat(rms) * dynam
! Inverting map 
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 2.27862e-05 Jy
! Component: 100  -  total flux cleaned = -8.09097e-05 Jy
! Component: 150  -  total flux cleaned = -0.000104144 Jy
! Component: 200  -  total flux cleaned = -0.000127558 Jy
! Total flux subtracted in 200 components = -0.000127558 Jy
! Clean residual min=-0.003484 max=0.003012 Jy/beam
! Clean residual mean=0.000004 rms=0.000722 Jy/beam
! Combined flux in latest and established models = 0.525172 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 65 components and 0.525172 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067372Jy  sigma=0.370224
! Fit after  self-cal, rms=0.067370Jy  sigma=0.370217
! Inverting map 
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 20 mega-wavelengths.
win_mult = win_mult * 1.2
selfcal true, true, soltime2
! Performing amp+phase self-cal over 15 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067370Jy  sigma=0.370217
! Fit after  self-cal, rms=0.067406Jy  sigma=0.370201
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=9.224 mas, bmaj=20.58 mas, bpa=-4.479 degrees
! Estimated noise=2.29277 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000233897 Jy
! Component: 100  -  total flux cleaned = -0.000233543 Jy
! Component: 150  -  total flux cleaned = -0.000258563 Jy
! Component: 200  -  total flux cleaned = -0.000268733 Jy
! Total flux subtracted in 200 components = -0.000268733 Jy
! Clean residual min=-0.003771 max=0.003204 Jy/beam
! Clean residual mean=0.000005 rms=0.000852 Jy/beam
! Combined flux in latest and established models = 0.524904 Jy
selfcal
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 69 components and 0.524904 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067399Jy  sigma=0.370165
! Fit after  self-cal, rms=0.067395Jy  sigma=0.370149
flux_cutoff = imstat(rms) * dynam
! Inverting map 
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -1.92482e-06 Jy
! Component: 100  -  total flux cleaned = -2.01524e-06 Jy
! Component: 150  -  total flux cleaned = -2.37339e-05 Jy
! Component: 200  -  total flux cleaned = -4.32982e-05 Jy
! Total flux subtracted in 200 components = -4.32982e-05 Jy
! Clean residual min=-0.003769 max=0.003196 Jy/beam
! Clean residual mean=0.000004 rms=0.000851 Jy/beam
! Combined flux in latest and established models = 0.52486 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 74 components and 0.524861 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067395Jy  sigma=0.370136
! Fit after  self-cal, rms=0.067392Jy  sigma=0.370126
! Inverting map 
uvtaper 0,0
! No UV-taper is currently set.
win_mult = win_mult / 1.2
print "=== Finished amplitude self-cal for VLBA stations ==="
! === Finished amplitude self-cal for VLBA stations === 
unflag *
! Unflagging all baselines in the currently selected channels.
uncalib false, false, true
! uncal: All telescope correction flags have been un-done.
integer lun
lun = outfile ( "/tmp/ff.ff" )
do i=1,nsub
  do j=1,ntel(i)
    fprintf lun, "%s\n", telname(j,i)
    end do
  end do
close ( lun )
system "/home/lpetrov/bin/dimap_selfant_process.csh /tmp/ff.ff"
![@/tmp/ff.ff]
1:FD
! Syntax error in line:
! 1:FD
! ^
! Found constant: 1.000 
! Where a command or assignment expression was expected.
![Exited script file: /tmp/ff.ff]
![Exited script file: /home/lpetrov/bin/rdv_muppet]
! 
wmap "/scr/pima/rdv96_uvs/J1409-2657_S\_map.fits"
! Inverting map and beam 
! Estimated beam: bmin=3.919 mas, bmaj=10.42 mas, bpa=-10.01 degrees
! Estimated noise=2.08265 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 3.919 x 10.42 at -10.01 degrees (North through East)
! Clean map  min=-0.0064883  max=0.48347 Jy/beam
! Writing clean map to FITS file: /scr/pima/rdv96_uvs/J1409-2657_S_map.fits
float peak_flux
peak_flux = peak(flux,max)
invert
! Inverting map 
float image_peak
image_peak = int(10000*peak_flux)/10000
float image_rms
image_rms  = int(100000*imstat(rms))/100000
print "========================================="
! ========================================= 
print "The image peak= ", image_peak, " rms= ", image_rms, " Jy"
! The image peak=  0.4834  rms=  0.00143  Jy 
quit
! Quitting program
! Log file /scr/pima/rdv96_uvs/J1409-2657_S_uvs.log closed on Sat Dec 21 00:24:29 2013