! Started logfile: /d2/scr/pima/rdv96_uvs/J2337-0230_X_uvs.log on Fri Dec 20 23:47:18 2013
obs /d2/scr/pima/rdv96_uvs/J2337-0230_X_uva.fits
! Reading UV FITS file: /d2/scr/pima/rdv96_uvs/J2337-0230_X_uva.fits
! AN table 1: 33 integrations on 6 of 6 possible baselines.
! AN table 2: 3 integrations on 36 of 36 possible baselines.
! AN table 3: 5 integrations on 55 of 55 possible baselines.
! AN table 4: 60 integrations on 3 of 3 possible baselines.
! AN table 5: 15 integrations on 6 of 6 possible baselines.
! Apparent sampling: 0.688602 visibilities/baseline/integration-bin.
! Found source: J2337-0230
! 
! 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  8.40599e+09        8e+06          1        8e+06
!  02        2  8.47599e+09        8e+06          1        8e+06
!  03        3  8.79099e+09        8e+06          1        8e+06
!  04        4  8.89599e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 0 lines of history.
! 
! Reading 2344 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 = 0.2 
print "taper_size =",taper_size
! taper_size = 70 
![@/home/lpetrov/bin/rdv_muppet /d2/scr/pima/rdv96_uvs/J2337-0230_X]
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:HH       self-cal  status=correctable  weight=1
! 1:NY       self-cal  status=correctable  weight=1
! 1:WF       self-cal  status=correctable  weight=1
! 1:WZ       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:NL       self-cal  status=correctable  weight=1
! 2:OV       self-cal  status=correctable  weight=1
! 2:PT       self-cal  status=correctable  weight=1
! 2:WZ       self-cal  status=correctable  weight=1
! 3:BR       self-cal  status=correctable  weight=1
! 3:FD       self-cal  status=correctable  weight=1
! 3:HN       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
! 3:WF       self-cal  status=correctable  weight=1
! 4:HH       self-cal  status=correctable  weight=1
! 4:MA       self-cal  status=correctable  weight=1
! 4:WZ       self-cal  status=correctable  weight=1
! 5:HH       self-cal  status=correctable  weight=1
! 5:MA       self-cal  status=correctable  weight=1
! 5:SC       self-cal  status=correctable  weight=1
! 5:WZ       self-cal  status=correctable  weight=1
system "rm /tmp/ff.ff"
mapsize field_size, field_cell
! Map grid = 1024x1024 pixels with 0.200x0.200 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 44 telescope corrections were flagged in sub-array 1.
!  A total of 22 telescope corrections were flagged in sub-array 3.
!  A total of 75 telescope corrections were flagged in sub-array 4.
!  A total of 29 telescope corrections were flagged in sub-array 5.
! 
! Correcting IF 2.
!  A total of 44 telescope corrections were flagged in sub-array 1.
!  A total of 22 telescope corrections were flagged in sub-array 3.
!  A total of 75 telescope corrections were flagged in sub-array 4.
!  A total of 29 telescope corrections were flagged in sub-array 5.
! 
! Correcting IF 3.
!  A total of 84 telescope corrections were flagged in sub-array 1.
!  A total of 22 telescope corrections were flagged in sub-array 3.
!  A total of 75 telescope corrections were flagged in sub-array 4.
!  A total of 29 telescope corrections were flagged in sub-array 5.
! 
! Correcting IF 4.
!  A total of 84 telescope corrections were flagged in sub-array 1.
!  A total of 22 telescope corrections were flagged in sub-array 3.
!  A total of 75 telescope corrections were flagged in sub-array 4.
!  A total of 29 telescope corrections were flagged in sub-array 5.
! 
! Fit before self-cal, rms=1.045068Jy  sigma=3.996211
! Fit after  self-cal, rms=0.746044Jy  sigma=2.384743
! 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:HH
! Flagging baselines of antenna 1:HH in the currently selected channels.
flag 1:NY
! Flagging baselines of antenna 1:NY in the currently selected channels.
flag 1:WF
! Flagging baselines of antenna 1:WF in the currently selected channels.
flag 1:WZ
! Flagging baselines of antenna 1:WZ in the currently selected channels.
flag 2:WZ
! Flagging baselines of antenna 2:WZ in the currently selected channels.
flag 3:WF
! Flagging baselines of antenna 3:WF in the currently selected channels.
flag 4:HH
! Flagging baselines of antenna 4:HH in the currently selected channels.
flag 4:MA
! Flagging baselines of antenna 4:MA in the currently selected channels.
flag 4:WZ
! Flagging baselines of antenna 4:WZ in the currently selected channels.
flag 5:HH
! Flagging baselines of antenna 5:HH in the currently selected channels.
flag 5:MA
! Flagging baselines of antenna 5:MA in the currently selected channels.
flag 5:WZ
! Flagging baselines of antenna 5: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=1.007 mas, bmaj=2.289 mas, bpa=-4.582 degrees
! Estimated noise=6.02406 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 = 0.277032 Jy
! Component: 100  -  total flux cleaned = 0.373058 Jy
! Total flux subtracted in 100 components = 0.373058 Jy
! Clean residual min=-0.017293 max=0.041155 Jy/beam
! Clean residual mean=0.000069 rms=0.005374 Jy/beam
! Combined flux in latest and established models = 0.373058 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 9 components and 0.373058 Jy
! 
! Correcting IF 1.
!  A total of 88 telescope corrections were flagged in sub-array 1.
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  A total of 3 telescope corrections were flagged in sub-array 3.
!  A total of 105 telescope corrections were flagged in sub-array 4.
!  A total of 31 telescope corrections were flagged in sub-array 5.
! 
! Correcting IF 2.
!  A total of 88 telescope corrections were flagged in sub-array 1.
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  A total of 3 telescope corrections were flagged in sub-array 3.
!  A total of 105 telescope corrections were flagged in sub-array 4.
!  A total of 31 telescope corrections were flagged in sub-array 5.
! 
! Correcting IF 3.
!  A total of 48 telescope corrections were flagged in sub-array 1.
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  A total of 3 telescope corrections were flagged in sub-array 3.
!  A total of 105 telescope corrections were flagged in sub-array 4.
!  A total of 31 telescope corrections were flagged in sub-array 5.
! 
! Correcting IF 4.
!  A total of 48 telescope corrections were flagged in sub-array 1.
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  A total of 3 telescope corrections were flagged in sub-array 3.
!  A total of 105 telescope corrections were flagged in sub-array 4.
!  A total of 31 telescope corrections were flagged in sub-array 5.
! 
! Fit before self-cal, rms=0.088252Jy  sigma=0.515385
! Fit after  self-cal, rms=0.086201Jy  sigma=0.510933
! Inverting map and beam 
! Estimated beam: bmin=1.007 mas, bmaj=2.289 mas, bpa=-4.582 degrees
! Estimated noise=6.02406 mJy/beam.
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0436118 Jy
! Component: 100  -  total flux cleaned = 0.0634042 Jy
! Total flux subtracted in 100 components = 0.0634042 Jy
! Clean residual min=-0.012023 max=0.014293 Jy/beam
! Clean residual mean=0.000014 rms=0.002668 Jy/beam
! Combined flux in latest and established models = 0.436463 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 18 components and 0.436463 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066943Jy  sigma=0.344874
! Fit after  self-cal, rms=0.066765Jy  sigma=0.344518
! 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=1.257 mas, bmaj=2.777 mas, bpa=-7.079 degrees
! Estimated noise=4.60042 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 = 0.0113523 Jy
! Component: 100  -  total flux cleaned = 0.0167575 Jy
! Component: 150  -  total flux cleaned = 0.0187935 Jy
! Component: 200  -  total flux cleaned = 0.0192861 Jy
! Total flux subtracted in 200 components = 0.0192861 Jy
! Clean residual min=-0.010427 max=0.009824 Jy/beam
! Clean residual mean=-0.000005 rms=0.002459 Jy/beam
! Combined flux in latest and established models = 0.455749 Jy
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 31 components and 0.455749 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.065350Jy  sigma=0.330758
! Fit after  self-cal, rms=0.065315Jy  sigma=0.330731
! 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:
!   HH        0.00*    NY        0.00*    WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.99     FD        1.04     HN        0.97     KP        0.95     
!   LA        1.03     NL        0.96     OV        1.02     PT        1.04     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.94     FD        1.00     HN        1.03     KP        1.01     
!   LA        1.04     MK        0.94     NL        0.97     OV        1.03     
!   PT        0.98     SC        0.93     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   HH        0.00*    MA        0.00*    SC        0.00*    WZ        0.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   HH        0.00*    NY        0.00*    WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.06     FD        1.02     HN        0.98     KP        0.93     
!   LA        0.94     NL        1.05     OV        1.00     PT        1.02     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.96     FD        1.00     HN        1.05     KP        0.96     
!   LA        1.01     MK        1.01     NL        0.95     OV        0.98     
!   PT        0.96     SC        0.91     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   HH        0.00*    MA        0.00*    SC        0.00*    WZ        0.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   HH        0.00*    NY        0.00*    WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.16     FD        0.98     HN        1.06     KP        0.84     
!   LA        1.09     NL        1.01     OV        1.03     PT        1.04     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00     FD        0.98     HN        1.03     KP        0.85     
!   LA        1.05     MK        0.94     NL        0.98     OV        1.03     
!   PT        0.98     SC        1.06     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   HH        0.00*    MA        0.00*    SC        0.00*    WZ        0.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   HH        0.00*    NY        0.00*    WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.09     FD        1.04     HN        1.11     KP        0.90     
!   LA        1.04     NL        0.99     OV        1.07     PT        1.04     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.02     FD        1.07     HN        1.02     KP        0.90     
!   LA        1.04     MK        1.06     NL        1.05     OV        1.01     
!   PT        1.01     SC        0.99     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   HH        0.00*    MA        0.00*    SC        0.00*    WZ        0.00*    
! 
! 
! Fit before self-cal, rms=0.065315Jy  sigma=0.330731
! Fit after  self-cal, rms=0.059994Jy  sigma=0.281595
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=1.251 mas, bmaj=2.758 mas, bpa=-6.796 degrees
! Estimated noise=4.58331 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 = -0.000395117 Jy
! Component: 100  -  total flux cleaned = -0.000312824 Jy
! Component: 150  -  total flux cleaned = -0.000235483 Jy
! Component: 200  -  total flux cleaned = -0.000237422 Jy
! Total flux subtracted in 200 components = -0.000237422 Jy
! Clean residual min=-0.007815 max=0.007456 Jy/beam
! Clean residual mean=0.000008 rms=0.001540 Jy/beam
! Combined flux in latest and established models = 0.455511 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 41 components and 0.455511 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.059671Jy  sigma=0.280932
! Fit after  self-cal, rms=0.059627Jy  sigma=0.280853
! 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=0.059627Jy  sigma=0.280853
! Fit after  self-cal, rms=0.059684Jy  sigma=0.280798
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=1.253 mas, bmaj=2.753 mas, bpa=-6.599 degrees
! Estimated noise=4.58024 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000453765 Jy
! Component: 100  -  total flux cleaned = -0.000379296 Jy
! Component: 150  -  total flux cleaned = -0.000308028 Jy
! Component: 200  -  total flux cleaned = -0.000308575 Jy
! Total flux subtracted in 200 components = -0.000308575 Jy
! Clean residual min=-0.007670 max=0.007429 Jy/beam
! Clean residual mean=0.000008 rms=0.001528 Jy/beam
! Combined flux in latest and established models = 0.455203 Jy
selfcal
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 43 components and 0.455203 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.059443Jy  sigma=0.280230
! Fit after  self-cal, rms=0.059373Jy  sigma=0.280212
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 = -7.33558e-05 Jy
! Component: 100  -  total flux cleaned = -7.30055e-05 Jy
! Component: 150  -  total flux cleaned = -7.3561e-05 Jy
! Component: 200  -  total flux cleaned = -7.57945e-05 Jy
! Total flux subtracted in 200 components = -7.57945e-05 Jy
! Clean residual min=-0.007549 max=0.007372 Jy/beam
! Clean residual mean=0.000008 rms=0.001519 Jy/beam
! Combined flux in latest and established models = 0.455127 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 44 components and 0.455127 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.059227Jy  sigma=0.279723
! Fit after  self-cal, rms=0.059142Jy  sigma=0.279706
! 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=0.059142Jy  sigma=0.279706
! Fit after  self-cal, rms=0.059221Jy  sigma=0.279637
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=1.256 mas, bmaj=2.747 mas, bpa=-6.353 degrees
! Estimated noise=4.5772 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000496774 Jy
! Component: 100  -  total flux cleaned = -0.000439404 Jy
! Component: 150  -  total flux cleaned = -0.000322383 Jy
! Component: 200  -  total flux cleaned = -0.000322358 Jy
! Total flux subtracted in 200 components = -0.000322358 Jy
! Clean residual min=-0.007387 max=0.007296 Jy/beam
! Clean residual mean=0.000007 rms=0.001509 Jy/beam
! Combined flux in latest and established models = 0.454804 Jy
selfcal
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 44 components and 0.454805 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.059051Jy  sigma=0.279178
! Fit after  self-cal, rms=0.058971Jy  sigma=0.279160
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 = 5.71614e-05 Jy
! Component: 100  -  total flux cleaned = -8.38754e-08 Jy
! Component: 150  -  total flux cleaned = -2.26659e-06 Jy
! Component: 200  -  total flux cleaned = 5.04116e-05 Jy
! Total flux subtracted in 200 components = 5.04116e-05 Jy
! Clean residual min=-0.007302 max=0.007241 Jy/beam
! Clean residual mean=0.000007 rms=0.001501 Jy/beam
! Combined flux in latest and established models = 0.454855 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 46 components and 0.454855 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.058857Jy  sigma=0.278760
! Fit after  self-cal, rms=0.058770Jy  sigma=0.278742
! Inverting map 
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 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=0.058770Jy  sigma=0.278742
! Fit after  self-cal, rms=0.058841Jy  sigma=0.278689
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=2.637 mas, bmaj=4.048 mas, bpa=-18.27 degrees
! Estimated noise=4.46762 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000141236 Jy
! Component: 100  -  total flux cleaned = -6.67186e-05 Jy
! Component: 150  -  total flux cleaned = -7.16691e-05 Jy
! Component: 200  -  total flux cleaned = -6.96893e-05 Jy
! Total flux subtracted in 200 components = -6.96893e-05 Jy
! Clean residual min=-0.005179 max=0.007611 Jy/beam
! Clean residual mean=0.000011 rms=0.001672 Jy/beam
! Combined flux in latest and established models = 0.454785 Jy
selfcal
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 49 components and 0.454785 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.059053Jy  sigma=0.278174
! Fit after  self-cal, rms=0.058745Jy  sigma=0.277754
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)
! Added new window around map position (16.4, -43.8).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00660623 Jy
! Component: 100  -  total flux cleaned = 0.0102419 Jy
! Component: 150  -  total flux cleaned = 0.0120734 Jy
! Component: 200  -  total flux cleaned = 0.0136369 Jy
! Total flux subtracted in 200 components = 0.0136369 Jy
! Clean residual min=-0.004602 max=0.004289 Jy/beam
! Clean residual mean=0.000001 rms=0.001278 Jy/beam
! Combined flux in latest and established models = 0.468422 Jy
! Performing phase self-cal
! Adding 32 model components to the UV plane model.
! The established model now contains 80 components and 0.468422 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.057906Jy  sigma=0.272763
! Fit after  self-cal, rms=0.057784Jy  sigma=0.272448
! 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:HH
! Syntax error in line:
! 1:HH
! ^
! 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 "/d2/scr/pima/rdv96_uvs/J2337-0230_X\_map.fits"
! Inverting map and beam 
! Estimated beam: bmin=0.8207 mas, bmaj=0.9891 mas, bpa=58.15 degrees
! Estimated noise=5.15592 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8207 x 0.9891 at 58.15 degrees (North through East)
! Clean map  min=-0.018276  max=0.2761 Jy/beam
! Writing clean map to FITS file: /d2/scr/pima/rdv96_uvs/J2337-0230_X_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=  0.2761  rms=  0.00458  Jy 
quit
! Quitting program
! Log file /d2/scr/pima/rdv96_uvs/J2337-0230_X_uvs.log closed on Fri Dec 20 23:47:20 2013