! Started logfile: /scr/pima/rdv96_uvs/J1522-2730_S_uvs.log on Sat Dec 21 00:24:33 2013
obs /scr/pima/rdv96_uvs/J1522-2730_S_uva.fits
! Reading UV FITS file: /scr/pima/rdv96_uvs/J1522-2730_S_uva.fits
! AN table 1: 2 integrations on 21 of 21 possible baselines.
! AN table 2: 2 integrations on 1 of 1 possible baselines.
! AN table 3: 15 integrations on 3 of 3 possible baselines.
! AN table 4: 2 integrations on 28 of 28 possible baselines.
! AN table 5: 2 integrations on 36 of 36 possible baselines.
! AN table 6: 2 integrations on 45 of 45 possible baselines.
! AN table 7: 2 integrations on 28 of 28 possible baselines.
! AN table 8: 2 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.975717 visibilities/baseline/integration-bin.
! Found source: J1522-2730
! 
! 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 1768 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/J1522-2730_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:KP       self-cal  status=correctable  weight=1
! 1:LA       self-cal  status=correctable  weight=1
! 1:MK       self-cal  status=correctable  weight=1
! 1:OV       self-cal  status=correctable  weight=1
! 1:PT       self-cal  status=correctable  weight=1
! 2:HH       self-cal  status=correctable  weight=1
! 2:WZ       self-cal  status=correctable  weight=1
! 3:HH       self-cal  status=correctable  weight=1
! 3:MA       self-cal  status=correctable  weight=1
! 3:WZ       self-cal  status=correctable  weight=1
! 4:FD       self-cal  status=correctable  weight=1
! 4:HN       self-cal  status=correctable  weight=1
! 4:KP       self-cal  status=correctable  weight=1
! 4:LA       self-cal  status=correctable  weight=1
! 4:NL       self-cal  status=correctable  weight=1
! 4:PT       self-cal  status=correctable  weight=1
! 4:SC       self-cal  status=correctable  weight=1
! 4:WF       self-cal  status=correctable  weight=1
! 5:FD       self-cal  status=correctable  weight=1
! 5:HN       self-cal  status=correctable  weight=1
! 5:KP       self-cal  status=correctable  weight=1
! 5:LA       self-cal  status=correctable  weight=1
! 5:NL       self-cal  status=correctable  weight=1
! 5:OV       self-cal  status=correctable  weight=1
! 5:PT       self-cal  status=correctable  weight=1
! 5:SC       self-cal  status=correctable  weight=1
! 5:WF       self-cal  status=correctable  weight=1
! 6:BR       self-cal  status=correctable  weight=1
! 6:FD       self-cal  status=correctable  weight=1
! 6:HN       self-cal  status=correctable  weight=1
! 6:KP       self-cal  status=correctable  weight=1
! 6:LA       self-cal  status=correctable  weight=1
! 6:NL       self-cal  status=correctable  weight=1
! 6:OV       self-cal  status=correctable  weight=1
! 6:PT       self-cal  status=correctable  weight=1
! 6:SC       self-cal  status=correctable  weight=1
! 6:WF       self-cal  status=correctable  weight=1
! 7:BR       self-cal  status=correctable  weight=1
! 7:FD       self-cal  status=correctable  weight=1
! 7:KP       self-cal  status=correctable  weight=1
! 7:LA       self-cal  status=correctable  weight=1
! 7:MK       self-cal  status=correctable  weight=1
! 7:NL       self-cal  status=correctable  weight=1
! 7:OV       self-cal  status=correctable  weight=1
! 7:PT       self-cal  status=correctable  weight=1
! 8:FD       self-cal  status=correctable  weight=1
! 8:HN       self-cal  status=correctable  weight=1
! 8:KP       self-cal  status=correctable  weight=1
! 8:LA       self-cal  status=correctable  weight=1
! 8:MK       self-cal  status=correctable  weight=1
! 8:NL       self-cal  status=correctable  weight=1
! 8:OV       self-cal  status=correctable  weight=1
! 8:PT       self-cal  status=correctable  weight=1
! 8:SC       self-cal  status=correctable  weight=1
! 8:WF       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 4 telescope corrections were flagged in sub-array 2.
!  A total of 45 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 4 telescope corrections were flagged in sub-array 2.
!  A total of 45 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 4 telescope corrections were flagged in sub-array 2.
!  A total of 45 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 4 telescope corrections were flagged in sub-array 2.
!  A total of 45 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=1.252200Jy  sigma=10.585490
! Fit after  self-cal, rms=0.334205Jy  sigma=2.419485
! 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 2:HH
! Flagging baselines of antenna 2:HH in the currently selected channels.
flag 2:WZ
! Flagging baselines of antenna 2:WZ in the currently selected channels.
flag 3:HH
! Flagging baselines of antenna 3:HH in the currently selected channels.
flag 3:MA
! Flagging baselines of antenna 3:MA in the currently selected channels.
flag 3:WZ
! Flagging baselines of antenna 3:WZ in the currently selected channels.
flag 4:WF
! Flagging baselines of antenna 4:WF in the currently selected channels.
flag 5:WF
! Flagging baselines of antenna 5:WF in the currently selected channels.
flag 6:WF
! Flagging baselines of antenna 6:WF in the currently selected channels.
flag 8:WF
! Flagging baselines of antenna 8: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=3.076 mas, bmaj=8.777 mas, bpa=-6.503 degrees
! Estimated noise=3.03222 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 = 0.575615 Jy
! Component: 100  -  total flux cleaned = 0.702425 Jy
! Total flux subtracted in 100 components = 0.702425 Jy
! Clean residual min=-0.016088 max=0.040106 Jy/beam
! Clean residual mean=0.000411 rms=0.005119 Jy/beam
! Combined flux in latest and established models = 0.702425 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 7 components and 0.702425 Jy
! 
! Correcting IF 1.
!  A total of 2 telescope corrections were flagged in sub-array 4.
!  A total of 2 telescope corrections were flagged in sub-array 5.
!  A total of 2 telescope corrections were flagged in sub-array 6.
!  A total of 2 telescope corrections were flagged in sub-array 8.
! 
! Correcting IF 2.
!  A total of 2 telescope corrections were flagged in sub-array 4.
!  A total of 2 telescope corrections were flagged in sub-array 5.
!  A total of 2 telescope corrections were flagged in sub-array 6.
!  A total of 2 telescope corrections were flagged in sub-array 8.
! 
! Correcting IF 3.
!  A total of 2 telescope corrections were flagged in sub-array 4.
!  A total of 2 telescope corrections were flagged in sub-array 5.
!  A total of 2 telescope corrections were flagged in sub-array 6.
!  A total of 2 telescope corrections were flagged in sub-array 8.
! 
! Correcting IF 4.
!  A total of 2 telescope corrections were flagged in sub-array 4.
!  A total of 2 telescope corrections were flagged in sub-array 5.
!  A total of 2 telescope corrections were flagged in sub-array 6.
!  A total of 2 telescope corrections were flagged in sub-array 8.
! 
! Fit before self-cal, rms=0.140773Jy  sigma=1.319553
! Fit after  self-cal, rms=0.140744Jy  sigma=1.319352
! Inverting map and beam 
! Estimated beam: bmin=3.076 mas, bmaj=8.777 mas, bpa=-6.503 degrees
! Estimated noise=3.03222 mJy/beam.
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0394275 Jy
! Component: 100  -  total flux cleaned = 0.0605434 Jy
! Total flux subtracted in 100 components = 0.0605434 Jy
! Clean residual min=-0.015290 max=0.013812 Jy/beam
! Clean residual mean=0.000247 rms=0.004016 Jy/beam
! Combined flux in latest and established models = 0.762968 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 16 components and 0.762968 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.126644Jy  sigma=1.158694
! Fit after  self-cal, rms=0.126621Jy  sigma=1.158544
! 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=3.989 mas, bmaj=11.17 mas, bpa=-6.791 degrees
! Estimated noise=2.22233 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 = 0.020913 Jy
! Component: 100  -  total flux cleaned = 0.0315416 Jy
! Component: 150  -  total flux cleaned = 0.0372447 Jy
! Component: 200  -  total flux cleaned = 0.0403228 Jy
! Total flux subtracted in 200 components = 0.0403228 Jy
! Clean residual min=-0.015238 max=0.013971 Jy/beam
! Clean residual mean=0.000487 rms=0.003551 Jy/beam
! Combined flux in latest and established models = 0.803291 Jy
! Performing phase self-cal
! Adding 27 model components to the UV plane model.
! The established model now contains 41 components and 0.803291 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.124074Jy  sigma=1.124281
! Fit after  self-cal, rms=0.124073Jy  sigma=1.124241
! 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        0.97     FD        0.96     KP        1.00     LA        1.14     
!   MK        0.91     OV        0.89     PT        1.02     
! 
!  Telescope amplitude corrections in sub-array 2:
!   HH        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   FD        1.03     HN        1.05     KP        1.00     LA        1.24     
!   NL        1.13     PT        1.04     SC        0.95     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   FD        0.99     HN        0.99     KP        1.02     LA        1.18     
!   NL        1.02     OV        1.03     PT        1.06     SC        0.95     
!   WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   BR        1.05     FD        1.01     HN        1.06     KP        1.03     
!   LA        1.17     NL        0.97     OV        1.00     PT        1.07     
!   SC        0.97     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 7:
!   BR        1.02     FD        1.02     KP        1.02     LA        1.16     
!   MK        0.93     NL        0.98     OV        0.99     PT        1.07     
! 
!  Telescope amplitude corrections in sub-array 8:
!   FD        0.98     HN        1.15     KP        1.05     LA        1.17     
!   MK        0.96     NL        0.99     OV        1.00     PT        1.08     
!   SC        1.00     WF        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.98     FD        1.01     KP        1.00     LA        1.03     
!   MK        0.96     OV        0.94     PT        1.02     
! 
!  Telescope amplitude corrections in sub-array 2:
!   HH        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   FD        1.03     HN        1.09     KP        1.01     LA        1.06     
!   NL        1.16     PT        1.03     SC        1.04     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   FD        1.08     HN        1.05     KP        1.03     LA        1.05     
!   NL        1.05     OV        1.04     PT        1.03     SC        1.07     
!   WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   BR        1.08     FD        1.08     HN        1.11     KP        1.02     
!   LA        1.08     NL        1.03     OV        1.05     PT        1.05     
!   SC        1.06     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 7:
!   BR        1.07     FD        1.08     KP        1.05     LA        1.05     
!   MK        1.00     NL        1.00     OV        1.03     PT        1.02     
! 
!  Telescope amplitude corrections in sub-array 8:
!   FD        1.07     HN        1.23     KP        1.02     LA        1.06     
!   MK        0.98     NL        1.03     OV        1.05     PT        1.06     
!   SC        1.07     WF        1.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.01     FD        1.05     KP        0.87     LA        0.92     
!   MK        0.97     OV        0.96     PT        1.01     
! 
!  Telescope amplitude corrections in sub-array 2:
!   HH        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   FD        1.04     HN        1.08     KP        0.88     LA        0.97     
!   NL        1.20     PT        1.05     SC        0.96     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   FD        1.07     HN        1.04     KP        0.90     LA        0.96     
!   NL        1.09     OV        1.01     PT        1.08     SC        0.94     
!   WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   BR        1.07     FD        1.08     HN        1.02     KP        0.90     
!   LA        0.99     NL        1.05     OV        1.00     PT        1.07     
!   SC        0.95     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 7:
!   BR        1.01     FD        1.07     KP        0.88     LA        0.94     
!   MK        0.99     NL        1.08     OV        1.01     PT        1.07     
! 
!  Telescope amplitude corrections in sub-array 8:
!   FD        1.08     HN        1.14     KP        0.86     LA        0.97     
!   MK        0.98     NL        1.04     OV        1.04     PT        1.09     
!   SC        1.00     WF        1.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.96     FD        1.00     KP        0.76     LA        0.79     
!   MK        1.09     OV        0.81     PT        0.92     
! 
!  Telescope amplitude corrections in sub-array 2:
!   HH        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   FD        1.08     HN        0.93     KP        0.81     LA        0.79     
!   NL        1.14     PT        0.95     SC        0.99     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   FD        1.11     HN        0.92     KP        0.83     LA        0.82     
!   NL        1.00     OV        0.87     PT        0.94     SC        0.99     
!   WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   BR        1.04     FD        1.08     HN        0.94     KP        0.81     
!   LA        0.82     NL        0.99     OV        0.87     PT        0.94     
!   SC        1.00     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 7:
!   BR        1.10     FD        1.09     KP        0.82     LA        0.80     
!   MK        1.10     NL        0.97     OV        0.87     PT        0.94     
! 
!  Telescope amplitude corrections in sub-array 8:
!   FD        1.10     HN        1.03     KP        0.83     LA        0.81     
!   MK        1.14     NL        0.98     OV        0.89     PT        0.97     
!   SC        1.01     WF        1.00*    
! 
! 
! Fit before self-cal, rms=0.124073Jy  sigma=1.124241
! Fit after  self-cal, rms=0.063409Jy  sigma=0.515369
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=3.999 mas, bmaj=11.22 mas, bpa=-6.637 degrees
! Estimated noise=2.22272 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 = -0.00232351 Jy
! Component: 100  -  total flux cleaned = -0.00247898 Jy
! Component: 150  -  total flux cleaned = -0.00261546 Jy
! Component: 200  -  total flux cleaned = -0.00279091 Jy
! Total flux subtracted in 200 components = -0.00279091 Jy
! Clean residual min=-0.004204 max=0.004517 Jy/beam
! Clean residual mean=0.000031 rms=0.001196 Jy/beam
! Combined flux in latest and established models = 0.8005 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 49 components and 0.8005 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.063171Jy  sigma=0.513858
! Fit after  self-cal, rms=0.063251Jy  sigma=0.513591
! 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=0.063251Jy  sigma=0.513591
! Fit after  self-cal, rms=0.063182Jy  sigma=0.513092
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=4 mas, bmaj=11.22 mas, bpa=-6.593 degrees
! Estimated noise=2.22136 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00184496 Jy
! Component: 100  -  total flux cleaned = -0.00204905 Jy
! Component: 150  -  total flux cleaned = -0.00216469 Jy
! Component: 200  -  total flux cleaned = -0.00226657 Jy
! Total flux subtracted in 200 components = -0.00226657 Jy
! Clean residual min=-0.004178 max=0.004377 Jy/beam
! Clean residual mean=0.000026 rms=0.001170 Jy/beam
! Combined flux in latest and established models = 0.798233 Jy
selfcal
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 51 components and 0.798233 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.063009Jy  sigma=0.512017
! Fit after  self-cal, rms=0.063006Jy  sigma=0.511997
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 = -0.0001841 Jy
! Component: 100  -  total flux cleaned = -0.000225474 Jy
! Component: 150  -  total flux cleaned = -0.00026408 Jy
! Component: 200  -  total flux cleaned = -0.000300644 Jy
! Total flux subtracted in 200 components = -0.000300644 Jy
! Clean residual min=-0.004181 max=0.004366 Jy/beam
! Clean residual mean=0.000028 rms=0.001167 Jy/beam
! Combined flux in latest and established models = 0.797933 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 60 components and 0.797933 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062941Jy  sigma=0.511659
! Fit after  self-cal, rms=0.062937Jy  sigma=0.511645
! 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=0.062937Jy  sigma=0.511645
! Fit after  self-cal, rms=0.062901Jy  sigma=0.511132
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=4.001 mas, bmaj=11.22 mas, bpa=-6.531 degrees
! Estimated noise=2.22084 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00147127 Jy
! Component: 100  -  total flux cleaned = -0.00163795 Jy
! Component: 150  -  total flux cleaned = -0.00173281 Jy
! Component: 200  -  total flux cleaned = -0.00185752 Jy
! Total flux subtracted in 200 components = -0.00185752 Jy
! Clean residual min=-0.004150 max=0.004252 Jy/beam
! Clean residual mean=0.000020 rms=0.001146 Jy/beam
! Combined flux in latest and established models = 0.796075 Jy
selfcal
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 61 components and 0.796075 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062787Jy  sigma=0.510442
! Fit after  self-cal, rms=0.062785Jy  sigma=0.510430
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 = -0.000139523 Jy
! Component: 100  -  total flux cleaned = -0.000136731 Jy
! Component: 150  -  total flux cleaned = -0.000168073 Jy
! Component: 200  -  total flux cleaned = -0.000198581 Jy
! Total flux subtracted in 200 components = -0.000198581 Jy
! Clean residual min=-0.004148 max=0.004241 Jy/beam
! Clean residual mean=0.000021 rms=0.001144 Jy/beam
! Combined flux in latest and established models = 0.795876 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 62 components and 0.795876 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062742Jy  sigma=0.510202
! Fit after  self-cal, rms=0.062740Jy  sigma=0.510193
! 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=0.062740Jy  sigma=0.510193
! Fit after  self-cal, rms=0.062726Jy  sigma=0.509866
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=8.38 mas, bmaj=20.06 mas, bpa=-6.631 degrees
! Estimated noise=2.46796 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000760943 Jy
! Component: 100  -  total flux cleaned = -0.00085049 Jy
! Component: 150  -  total flux cleaned = -0.000901425 Jy
! Component: 200  -  total flux cleaned = -0.000924061 Jy
! Total flux subtracted in 200 components = -0.000924061 Jy
! Clean residual min=-0.004600 max=0.004052 Jy/beam
! Clean residual mean=0.000024 rms=0.001327 Jy/beam
! Combined flux in latest and established models = 0.794952 Jy
selfcal
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 67 components and 0.794952 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062696Jy  sigma=0.509581
! Fit after  self-cal, rms=0.062689Jy  sigma=0.509557
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 = -6.79118e-05 Jy
! Component: 100  -  total flux cleaned = -2.27993e-05 Jy
! Component: 150  -  total flux cleaned = -2.26002e-05 Jy
! Component: 200  -  total flux cleaned = -2.26945e-05 Jy
! Total flux subtracted in 200 components = -2.26945e-05 Jy
! Clean residual min=-0.004623 max=0.004044 Jy/beam
! Clean residual mean=0.000025 rms=0.001325 Jy/beam
! Combined flux in latest and established models = 0.79493 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 72 components and 0.79493 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062689Jy  sigma=0.509507
! Fit after  self-cal, rms=0.062685Jy  sigma=0.509491
! 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/J1522-2730_S\_map.fits"
! Inverting map and beam 
! Estimated beam: bmin=3.934 mas, bmaj=8.069 mas, bpa=-7.15 degrees
! Estimated noise=2.18976 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 3.934 x 8.069 at -7.15 degrees (North through East)
! Clean map  min=-0.018539  max=0.71086 Jy/beam
! Writing clean map to FITS file: /scr/pima/rdv96_uvs/J1522-2730_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=  0.7108  rms=  0.00321  Jy 
quit
! Quitting program
! Log file /scr/pima/rdv96_uvs/J1522-2730_S_uvs.log closed on Sat Dec 21 00:24:35 2013