! Started logfile: /scr/pima/rdv96_uvs/J2211-1328_S_uvs.log on Sat Dec 21 00:25:55 2013
obs /scr/pima/rdv96_uvs/J2211-1328_S_uva.fits
! Reading UV FITS file: /scr/pima/rdv96_uvs/J2211-1328_S_uva.fits
! AN table 1: 12 integrations on 45 of 45 possible baselines.
! AN table 2: 5 integrations on 36 of 36 possible baselines.
! AN table 3: 4 integrations on 36 of 36 possible baselines.
! AN table 4: 3 integrations on 6 of 6 possible baselines.
! AN table 5: 4 integrations on 6 of 6 possible baselines.
! AN table 6: 19 integrations on 3 of 3 possible baselines.
! AN table 7: 29 integrations on 6 of 6 possible baselines.
! Apparent sampling: 0.854881 visibilities/baseline/integration-bin.
! Found source: J2211-1328
! 
! 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 3888 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/J2211-1328_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:BR       self-cal  status=correctable  weight=1
! 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:OV       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:HN       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: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
! 3:SC       self-cal  status=correctable  weight=1
! 4:BR       self-cal  status=correctable  weight=1
! 4:LA       self-cal  status=correctable  weight=1
! 4:OV       self-cal  status=correctable  weight=1
! 4:PT       self-cal  status=correctable  weight=1
! 5:BR       self-cal  status=correctable  weight=1
! 5:KP       self-cal  status=correctable  weight=1
! 5:MK       self-cal  status=correctable  weight=1
! 5:OV       self-cal  status=correctable  weight=1
! 6:HH       self-cal  status=correctable  weight=1
! 6:MA       self-cal  status=correctable  weight=1
! 6:WZ       self-cal  status=correctable  weight=1
! 7:HH       self-cal  status=correctable  weight=1
! 7:MA       self-cal  status=correctable  weight=1
! 7:SC       self-cal  status=correctable  weight=1
! 7:WZ       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 9 telescope corrections were flagged in sub-array 1.
!  A total of 57 telescope corrections were flagged in sub-array 6.
!  A total of 116 telescope corrections were flagged in sub-array 7.
! 
! Correcting IF 2.
!  A total of 9 telescope corrections were flagged in sub-array 1.
!  A total of 57 telescope corrections were flagged in sub-array 6.
!  A total of 116 telescope corrections were flagged in sub-array 7.
! 
! Correcting IF 3.
!  A total of 9 telescope corrections were flagged in sub-array 1.
!  A total of 57 telescope corrections were flagged in sub-array 6.
!  A total of 116 telescope corrections were flagged in sub-array 7.
! 
! Correcting IF 4.
!  A total of 9 telescope corrections were flagged in sub-array 1.
!  A total of 57 telescope corrections were flagged in sub-array 6.
!  A total of 116 telescope corrections were flagged in sub-array 7.
! 
! Fit before self-cal, rms=1.049779Jy  sigma=4.036534
! Fit after  self-cal, rms=0.699301Jy  sigma=2.669384
! 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.
flag 6:HH
! Flagging baselines of antenna 6:HH in the currently selected channels.
flag 6:MA
! Flagging baselines of antenna 6:MA in the currently selected channels.
flag 6:WZ
! Flagging baselines of antenna 6:WZ in the currently selected channels.
flag 7:HH
! Flagging baselines of antenna 7:HH in the currently selected channels.
flag 7:MA
! Flagging baselines of antenna 7:MA in the currently selected channels.
flag 7:WZ
! Flagging baselines of antenna 7:WZ 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=3.251 mas, bmaj=7.617 mas, bpa=-2.79 degrees
! Estimated noise=4.95907 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 = 0.240529 Jy
! Component: 100  -  total flux cleaned = 0.297945 Jy
! Total flux subtracted in 100 components = 0.297945 Jy
! Clean residual min=-0.009262 max=0.022508 Jy/beam
! Clean residual mean=0.000047 rms=0.003051 Jy/beam
! Combined flux in latest and established models = 0.297945 Jy
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 15 components and 0.297945 Jy
! 
! Correcting IF 1.
!  A total of 12 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 12 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 12 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 12 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.091552Jy  sigma=0.389998
! Fit after  self-cal, rms=0.091524Jy  sigma=0.389874
! Inverting map and beam 
! Estimated beam: bmin=3.251 mas, bmaj=7.617 mas, bpa=-2.79 degrees
! Estimated noise=4.95907 mJy/beam.
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0238751 Jy
! Component: 100  -  total flux cleaned = 0.0353959 Jy
! Total flux subtracted in 100 components = 0.0353959 Jy
! Clean residual min=-0.008888 max=0.014622 Jy/beam
! Clean residual mean=0.000019 rms=0.002287 Jy/beam
! Combined flux in latest and established models = 0.333341 Jy
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 31 components and 0.333341 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.083616Jy  sigma=0.343666
! Fit after  self-cal, rms=0.083544Jy  sigma=0.343448
! Inverting map 
! Added new window around map position (3.2, -16.8).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.014846 Jy
! Component: 100  -  total flux cleaned = 0.0232637 Jy
! Total flux subtracted in 100 components = 0.0232637 Jy
! Clean residual min=-0.007618 max=0.008148 Jy/beam
! Clean residual mean=0.000016 rms=0.001920 Jy/beam
! Combined flux in latest and established models = 0.356605 Jy
! Performing phase self-cal
! Adding 26 model components to the UV plane model.
! The established model now contains 56 components and 0.356605 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.080061Jy  sigma=0.324252
! Fit after  self-cal, rms=0.079642Jy  sigma=0.322690
! 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=4.301 mas, bmaj=9.784 mas, bpa=-3.029 degrees
! Estimated noise=3.24033 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 = 0.0124779 Jy
! Component: 100  -  total flux cleaned = 0.0197546 Jy
! Component: 150  -  total flux cleaned = 0.0243913 Jy
! Component: 200  -  total flux cleaned = 0.0274082 Jy
! Total flux subtracted in 200 components = 0.0274082 Jy
! Clean residual min=-0.007527 max=0.007004 Jy/beam
! Clean residual mean=0.000059 rms=0.001847 Jy/beam
! Combined flux in latest and established models = 0.384013 Jy
! Performing phase self-cal
! Adding 43 model components to the UV plane model.
! The established model now contains 91 components and 0.384013 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.077918Jy  sigma=0.312560
! Fit after  self-cal, rms=0.077807Jy  sigma=0.311999
! 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.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.04     FD        0.98     HN        0.98     KP        1.00     
!   LA        1.16     NL        0.99     OV        0.99     PT        1.01     
!   SC        0.95     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.02     FD        1.01     HN        1.01     KP        1.00     
!   LA        1.15     MK        0.83     NL        1.01     PT        1.01     
!   SC        0.93     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.02     FD        1.00     KP        1.01     LA        1.17     
!   MK        0.98     NL        0.97     OV        0.97     PT        1.06     
!   SC        1.01     
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.02     LA        1.11     OV        1.08     PT        1.06     
! 
!  Telescope amplitude corrections in sub-array 5:
!   BR        1.00     KP        1.03     MK        0.91     OV        1.01     
! 
!  Telescope amplitude corrections in sub-array 6:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 7:
!   HH        0.00*    MA        0.00*    SC        0.00*    WZ        0.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.06     FD        1.04     HN        1.04     KP        1.03     
!   LA        1.07     NL        1.04     OV        1.01     PT        1.04     
!   SC        1.03     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.06     FD        1.07     HN        1.06     KP        1.00     
!   LA        1.08     MK        1.07     NL        0.98     PT        1.05     
!   SC        1.09     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.04     FD        1.09     KP        1.06     LA        1.08     
!   MK        1.03     NL        1.08     OV        1.01     PT        1.03     
!   SC        1.08     
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.01     LA        1.02     OV        1.07     PT        1.12     
! 
!  Telescope amplitude corrections in sub-array 5:
!   BR        1.09     KP        0.99     MK        1.05     OV        1.00     
! 
!  Telescope amplitude corrections in sub-array 6:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 7:
!   HH        0.00*    MA        0.00*    SC        0.00*    WZ        0.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.07     FD        1.08     HN        0.97     KP        0.90     
!   LA        0.99     NL        1.05     OV        1.03     PT        1.04     
!   SC        0.93     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.09     FD        1.11     HN        1.02     KP        0.91     
!   LA        0.97     MK        0.96     NL        1.09     PT        1.05     
!   SC        0.98     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.09     FD        1.06     KP        0.89     LA        0.97     
!   MK        1.00     NL        1.08     OV        1.02     PT        1.10     
!   SC        0.97     
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.07     LA        1.06     OV        1.12     PT        1.06     
! 
!  Telescope amplitude corrections in sub-array 5:
!   BR        0.90     KP        0.90     MK        1.08     OV        1.09     
! 
!  Telescope amplitude corrections in sub-array 6:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 7:
!   HH        0.00*    MA        0.00*    SC        0.00*    WZ        0.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        1.07     HN        0.88     KP        0.81     
!   LA        0.82     NL        0.99     OV        0.87     PT        0.94     
!   SC        1.01     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        1.07     HN        0.92     KP        0.81     
!   LA        0.85     MK        1.15     NL        1.07     PT        0.97     
!   SC        1.02     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.98     FD        1.08     KP        0.82     LA        0.85     
!   MK        1.19     NL        1.00     OV        0.87     PT        0.91     
!   SC        1.09     
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        0.99     LA        0.84     OV        0.91     PT        0.96     
! 
!  Telescope amplitude corrections in sub-array 5:
!   BR        1.06     KP        0.84     MK        1.18     OV        0.83     
! 
!  Telescope amplitude corrections in sub-array 6:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 7:
!   HH        0.00*    MA        0.00*    SC        0.00*    WZ        0.00*    
! 
! 
! Fit before self-cal, rms=0.077807Jy  sigma=0.311999
! Fit after  self-cal, rms=0.065342Jy  sigma=0.250231
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=4.306 mas, bmaj=9.839 mas, bpa=-3.089 degrees
! Estimated noise=3.23184 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 = 0.000747236 Jy
! Component: 100  -  total flux cleaned = 0.00104709 Jy
! Component: 150  -  total flux cleaned = 0.00119447 Jy
! Component: 200  -  total flux cleaned = 0.00132449 Jy
! Total flux subtracted in 200 components = 0.00132449 Jy
! Clean residual min=-0.003052 max=0.003172 Jy/beam
! Clean residual mean=-0.000006 rms=0.000800 Jy/beam
! Combined flux in latest and established models = 0.385337 Jy
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 108 components and 0.385337 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.065238Jy  sigma=0.249821
! Fit after  self-cal, rms=0.065303Jy  sigma=0.249713
! 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=0.065303Jy  sigma=0.249713
! Fit after  self-cal, rms=0.065367Jy  sigma=0.249676
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=4.305 mas, bmaj=9.843 mas, bpa=-3.124 degrees
! Estimated noise=3.23422 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 9.34543e-05 Jy
! Component: 100  -  total flux cleaned = 0.000217313 Jy
! Component: 150  -  total flux cleaned = 0.000324336 Jy
! Component: 200  -  total flux cleaned = 0.000386887 Jy
! Total flux subtracted in 200 components = 0.000386887 Jy
! Clean residual min=-0.002955 max=0.002895 Jy/beam
! Clean residual mean=-0.000008 rms=0.000782 Jy/beam
! Combined flux in latest and established models = 0.385724 Jy
selfcal
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 115 components and 0.385724 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.065314Jy  sigma=0.249501
! Fit after  self-cal, rms=0.065313Jy  sigma=0.249487
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 = -2.49507e-05 Jy
! Component: 100  -  total flux cleaned = 8.44858e-07 Jy
! Component: 150  -  total flux cleaned = 1.16528e-06 Jy
! Component: 200  -  total flux cleaned = 2.32657e-05 Jy
! Total flux subtracted in 200 components = 2.32657e-05 Jy
! Clean residual min=-0.002923 max=0.002814 Jy/beam
! Clean residual mean=-0.000008 rms=0.000777 Jy/beam
! Combined flux in latest and established models = 0.385748 Jy
! Performing phase self-cal
! Adding 20 model components to the UV plane model.
! The established model now contains 127 components and 0.385748 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.065288Jy  sigma=0.249420
! Fit after  self-cal, rms=0.065288Jy  sigma=0.249414
! 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=0.065288Jy  sigma=0.249414
! Fit after  self-cal, rms=0.065343Jy  sigma=0.249366
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=4.304 mas, bmaj=9.846 mas, bpa=-3.168 degrees
! Estimated noise=3.23591 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 8.21915e-05 Jy
! Component: 100  -  total flux cleaned = 8.10619e-05 Jy
! Component: 150  -  total flux cleaned = 0.000103975 Jy
! Component: 200  -  total flux cleaned = 0.000125559 Jy
! Total flux subtracted in 200 components = 0.000125559 Jy
! Clean residual min=-0.002850 max=0.002798 Jy/beam
! Clean residual mean=-0.000009 rms=0.000768 Jy/beam
! Combined flux in latest and established models = 0.385873 Jy
selfcal
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 135 components and 0.385873 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.065317Jy  sigma=0.249294
! Fit after  self-cal, rms=0.065318Jy  sigma=0.249287
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 = -0.000107682 Jy
! Component: 100  -  total flux cleaned = -8.9149e-05 Jy
! Component: 150  -  total flux cleaned = -8.91449e-05 Jy
! Component: 200  -  total flux cleaned = -8.83577e-05 Jy
! Total flux subtracted in 200 components = -8.83577e-05 Jy
! Clean residual min=-0.002829 max=0.002757 Jy/beam
! Clean residual mean=-0.000009 rms=0.000766 Jy/beam
! Combined flux in latest and established models = 0.385785 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 139 components and 0.385785 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.065303Jy  sigma=0.249258
! Fit after  self-cal, rms=0.065304Jy  sigma=0.249255
! 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=0.065304Jy  sigma=0.249255
! Fit after  self-cal, rms=0.065332Jy  sigma=0.249225
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=8.472 mas, bmaj=15.09 mas, bpa=-10.21 degrees
! Estimated noise=3.54652 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000191024 Jy
! Component: 100  -  total flux cleaned = 0.000244184 Jy
! Component: 150  -  total flux cleaned = 0.000243279 Jy
! Component: 200  -  total flux cleaned = 0.000242836 Jy
! Total flux subtracted in 200 components = 0.000242836 Jy
! Clean residual min=-0.003234 max=0.002981 Jy/beam
! Clean residual mean=-0.000013 rms=0.000905 Jy/beam
! Combined flux in latest and established models = 0.386028 Jy
selfcal
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 143 components and 0.386028 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.065332Jy  sigma=0.249191
! Fit after  self-cal, rms=0.065329Jy  sigma=0.249180
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 = -7.54971e-06 Jy
! Component: 100  -  total flux cleaned = -6.44078e-06 Jy
! Component: 150  -  total flux cleaned = -6.34914e-06 Jy
! Component: 200  -  total flux cleaned = -7.00519e-06 Jy
! Total flux subtracted in 200 components = -7.00519e-06 Jy
! Clean residual min=-0.003220 max=0.002954 Jy/beam
! Clean residual mean=-0.000013 rms=0.000903 Jy/beam
! Combined flux in latest and established models = 0.386021 Jy
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 152 components and 0.386021 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.065331Jy  sigma=0.249176
! Fit after  self-cal, rms=0.065329Jy  sigma=0.249171
! 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:BR
! Syntax error in line:
! 1:BR
! ^
! 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/J2211-1328_S\_map.fits"
! Inverting map and beam 
! Estimated beam: bmin=4.163 mas, bmaj=7.997 mas, bpa=-5.656 degrees
! Estimated noise=3.26011 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 4.163 x 7.997 at -5.656 degrees (North through East)
! Clean map  min=-0.0070294  max=0.3032 Jy/beam
! Writing clean map to FITS file: /scr/pima/rdv96_uvs/J2211-1328_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=  0.3031  rms=  0.00166  Jy 
quit
! Quitting program
! Log file /scr/pima/rdv96_uvs/J2211-1328_S_uvs.log closed on Sat Dec 21 00:25:58 2013