! Started logfile: /d2/scr/pima/rdv96_uvs/J0106-4034_X_uvs.log on Fri Dec 20 23:43:31 2013
obs /d2/scr/pima/rdv96_uvs/J0106-4034_X_uva.fits
! Reading UV FITS file: /d2/scr/pima/rdv96_uvs/J0106-4034_X_uva.fits
! AN table 1: 17 integrations on 6 of 6 possible baselines.
! AN table 2: 4 integrations on 15 of 15 possible baselines.
! AN table 3: 2 integrations on 21 of 21 possible baselines.
! AN table 4: 2 integrations on 21 of 21 possible baselines.
! AN table 5: 2 integrations on 28 of 28 possible baselines.
! AN table 6: 2 integrations on 15 of 15 possible baselines.
! Apparent sampling: 0.849398 visibilities/baseline/integration-bin.
! Found source: J0106-4034
! 
! 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 1128 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/J0106-4034_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:FD       self-cal  status=correctable  weight=1
! 1:HH       self-cal  status=correctable  weight=1
! 1:SC       self-cal  status=correctable  weight=1
! 1:WF       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:PT       self-cal  status=correctable  weight=1
! 2:SC       self-cal  status=correctable  weight=1
! 2:WF       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:NL       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:FD       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:OV       self-cal  status=correctable  weight=1
! 4:PT       self-cal  status=correctable  weight=1
! 4:WF       self-cal  status=correctable  weight=1
! 5:FD       self-cal  status=correctable  weight=1
! 5:KP       self-cal  status=correctable  weight=1
! 5:LA       self-cal  status=correctable  weight=1
! 5:MK       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
! 6:FD       self-cal  status=correctable  weight=1
! 6:KP       self-cal  status=correctable  weight=1
! 6:LA       self-cal  status=correctable  weight=1
! 6:MK       self-cal  status=correctable  weight=1
! 6:OV       self-cal  status=correctable  weight=1
! 6:PT       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 26 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 26 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 26 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 26 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=1.324891Jy  sigma=13.502048
! Fit after  self-cal, rms=0.295786Jy  sigma=1.339201
! 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:WF
! Flagging baselines of antenna 1:WF in the currently selected channels.
flag 2:WF
! Flagging baselines of antenna 2:WF in the currently selected channels.
flag 3:WF
! Flagging baselines of antenna 3:WF in the currently selected channels.
flag 4:WF
! Flagging baselines of antenna 4: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=0.7954 mas, bmaj=2.884 mas, bpa=-2.43 degrees
! Estimated noise=2.97956 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 = 0.702133 Jy
! Component: 100  -  total flux cleaned = 0.856649 Jy
! Total flux subtracted in 100 components = 0.856649 Jy
! Clean residual min=-0.032715 max=0.054901 Jy/beam
! Clean residual mean=-0.000270 rms=0.007619 Jy/beam
! Combined flux in latest and established models = 0.856649 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 7 components and 0.856649 Jy
! 
! Correcting IF 1.
!  A total of 42 telescope corrections were flagged in sub-array 1.
!  A total of 4 telescope corrections were flagged in sub-array 2.
!  A total of 2 telescope corrections were flagged in sub-array 3.
!  A total of 2 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 2.
!  A total of 42 telescope corrections were flagged in sub-array 1.
!  A total of 4 telescope corrections were flagged in sub-array 2.
!  A total of 2 telescope corrections were flagged in sub-array 3.
!  A total of 2 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 3.
!  A total of 42 telescope corrections were flagged in sub-array 1.
!  A total of 4 telescope corrections were flagged in sub-array 2.
!  A total of 2 telescope corrections were flagged in sub-array 3.
!  A total of 2 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 4.
!  A total of 42 telescope corrections were flagged in sub-array 1.
!  A total of 4 telescope corrections were flagged in sub-array 2.
!  A total of 2 telescope corrections were flagged in sub-array 3.
!  A total of 2 telescope corrections were flagged in sub-array 4.
! 
! Fit before self-cal, rms=0.146635Jy  sigma=1.792846
! Fit after  self-cal, rms=0.147279Jy  sigma=1.802717
! Inverting map and beam 
! Estimated beam: bmin=0.7955 mas, bmaj=2.872 mas, bpa=-2.36 degrees
! Estimated noise=3.00187 mJy/beam.
! Added new window around map position (-1.6, -0.6).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.057216 Jy
! Component: 100  -  total flux cleaned = 0.0910067 Jy
! Total flux subtracted in 100 components = 0.0910067 Jy
! Clean residual min=-0.031652 max=0.042789 Jy/beam
! Clean residual mean=-0.000036 rms=0.005591 Jy/beam
! Combined flux in latest and established models = 0.947656 Jy
! Performing phase self-cal
! Adding 24 model components to the UV plane model.
! The established model now contains 31 components and 0.947656 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.118381Jy  sigma=1.344962
! Fit after  self-cal, rms=0.117030Jy  sigma=1.322813
! 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=1.047 mas, bmaj=3.849 mas, bpa=-2.245 degrees
! Estimated noise=2.30318 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 = 0.0335377 Jy
! Component: 100  -  total flux cleaned = 0.0489473 Jy
! Component: 150  -  total flux cleaned = 0.0547039 Jy
! Component: 200  -  total flux cleaned = 0.0556024 Jy
! Total flux subtracted in 200 components = 0.0556024 Jy
! Clean residual min=-0.036038 max=0.022482 Jy/beam
! Clean residual mean=0.000217 rms=0.005821 Jy/beam
! Combined flux in latest and established models = 1.00326 Jy
! Performing phase self-cal
! Adding 26 model components to the UV plane model.
! The established model now contains 48 components and 1.00326 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.110281Jy  sigma=1.189637
! Fit after  self-cal, rms=0.109945Jy  sigma=1.181753
! 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:
!   FD        0.00*    HH        0.00*    SC        0.00*    WF        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   FD        0.99     KP        1.00     LA        1.06     PT        1.03     
!   SC        0.97     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   FD        1.01     KP        0.99     LA        1.03     NL        1.12     
!   PT        1.00     SC        0.99     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   FD        0.98     KP        0.99     LA        1.02     NL        1.06     
!   OV        1.03     PT        0.98     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   FD        0.96     KP        0.99     LA        1.03     MK        1.03     
!   NL        1.20     OV        0.96     PT        1.03     SC        0.98     
! 
!  Telescope amplitude corrections in sub-array 6:
!   FD        0.99     KP        1.00     LA        1.06     MK        0.99     
!   OV        0.97     PT        1.00     
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   FD        0.00*    HH        0.00*    SC        0.00*    WF        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   FD        1.01     KP        0.94     LA        1.04     PT        1.01     
!   SC        0.98     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   FD        1.00     KP        0.95     LA        1.00     NL        1.13     
!   PT        1.02     SC        1.00     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   FD        0.95     KP        0.94     LA        0.99     NL        1.05     
!   OV        1.03     PT        0.99     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   FD        0.97     KP        0.94     LA        1.02     MK        1.01     
!   NL        1.23     OV        0.94     PT        1.03     SC        1.02     
! 
!  Telescope amplitude corrections in sub-array 6:
!   FD        0.97     KP        0.93     LA        0.99     MK        1.02     
!   OV        0.96     PT        1.03     
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   FD        0.00*    HH        0.00*    SC        0.00*    WF        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   FD        0.99     KP        0.84     LA        1.09     PT        1.02     
!   SC        0.99     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   FD        0.99     KP        0.83     LA        1.12     NL        1.11     
!   PT        1.01     SC        1.05     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   FD        0.94     KP        0.85     LA        1.06     NL        1.07     
!   OV        1.10     PT        0.97     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   FD        0.97     KP        0.85     LA        1.07     MK        0.99     
!   NL        1.28     OV        1.03     PT        1.03     SC        1.02     
! 
!  Telescope amplitude corrections in sub-array 6:
!   FD        0.97     KP        0.83     LA        1.04     MK        1.02     
!   OV        1.03     PT        0.99     
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   FD        0.00*    HH        0.00*    SC        0.00*    WF        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   FD        1.08     KP        0.88     LA        1.07     PT        1.06     
!   SC        0.97     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   FD        1.05     KP        0.85     LA        1.04     NL        1.14     
!   PT        1.07     SC        1.02     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   FD        1.00     KP        0.87     LA        1.04     NL        1.11     
!   OV        1.09     PT        1.01     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   FD        1.00     KP        0.87     LA        1.05     MK        1.07     
!   NL        1.27     OV        0.98     PT        1.10     SC        1.07     
! 
!  Telescope amplitude corrections in sub-array 6:
!   FD        1.00     KP        0.89     LA        1.06     MK        1.06     
!   OV        0.99     PT        1.07     
! 
! 
! Fit before self-cal, rms=0.109945Jy  sigma=1.181753
! Fit after  self-cal, rms=0.067507Jy  sigma=0.658044
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=1.053 mas, bmaj=3.9 mas, bpa=-2.191 degrees
! Estimated noise=2.30977 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 = -0.00526667 Jy
! Component: 100  -  total flux cleaned = -0.00526729 Jy
! Component: 150  -  total flux cleaned = -0.00527912 Jy
! Component: 200  -  total flux cleaned = -0.00517347 Jy
! Total flux subtracted in 200 components = -0.00517347 Jy
! Clean residual min=-0.008035 max=0.006127 Jy/beam
! Clean residual mean=0.000009 rms=0.001567 Jy/beam
! Combined flux in latest and established models = 0.998085 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 59 components and 0.998085 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066300Jy  sigma=0.650366
! Fit after  self-cal, rms=0.066112Jy  sigma=0.648093
! 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=0.066112Jy  sigma=0.648093
! Fit after  self-cal, rms=0.066113Jy  sigma=0.646518
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=1.054 mas, bmaj=3.909 mas, bpa=-2.201 degrees
! Estimated noise=2.30751 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00398358 Jy
! Component: 100  -  total flux cleaned = -0.00386716 Jy
! Component: 150  -  total flux cleaned = -0.00386694 Jy
! Component: 200  -  total flux cleaned = -0.00386681 Jy
! Total flux subtracted in 200 components = -0.00386681 Jy
! Clean residual min=-0.006865 max=0.006071 Jy/beam
! Clean residual mean=0.000008 rms=0.001499 Jy/beam
! Combined flux in latest and established models = 0.994218 Jy
selfcal
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 63 components and 0.994218 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.065260Jy  sigma=0.641848
! Fit after  self-cal, rms=0.065044Jy  sigma=0.640537
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 = -0.00112915 Jy
! Component: 100  -  total flux cleaned = -0.00103101 Jy
! Component: 150  -  total flux cleaned = -0.00103087 Jy
! Component: 200  -  total flux cleaned = -0.00103149 Jy
! Total flux subtracted in 200 components = -0.00103149 Jy
! Clean residual min=-0.006288 max=0.005769 Jy/beam
! Clean residual mean=0.000002 rms=0.001474 Jy/beam
! Combined flux in latest and established models = 0.993186 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 70 components and 0.993187 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.064630Jy  sigma=0.638470
! Fit after  self-cal, rms=0.064547Jy  sigma=0.638036
! 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=0.064547Jy  sigma=0.638036
! Fit after  self-cal, rms=0.063555Jy  sigma=0.622286
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=1.054 mas, bmaj=3.917 mas, bpa=-2.208 degrees
! Estimated noise=2.30636 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00245968 Jy
! Component: 100  -  total flux cleaned = -0.0024545 Jy
! Component: 150  -  total flux cleaned = -0.00244737 Jy
! Component: 200  -  total flux cleaned = -0.00237014 Jy
! Total flux subtracted in 200 components = -0.00237014 Jy
! Clean residual min=-0.005432 max=0.005772 Jy/beam
! Clean residual mean=0.000012 rms=0.001382 Jy/beam
! Combined flux in latest and established models = 0.990816 Jy
selfcal
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 72 components and 0.990816 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.063028Jy  sigma=0.619751
! Fit after  self-cal, rms=0.062928Jy  sigma=0.619106
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 = -0.000780396 Jy
! Component: 100  -  total flux cleaned = -0.00078239 Jy
! Component: 150  -  total flux cleaned = -0.000717129 Jy
! Component: 200  -  total flux cleaned = -0.00071554 Jy
! Total flux subtracted in 200 components = -0.00071554 Jy
! Clean residual min=-0.005361 max=0.005587 Jy/beam
! Clean residual mean=0.000008 rms=0.001369 Jy/beam
! Combined flux in latest and established models = 0.990101 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 75 components and 0.990101 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062639Jy  sigma=0.617869
! Fit after  self-cal, rms=0.062603Jy  sigma=0.617652
! 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=0.062603Jy  sigma=0.617652
! Fit after  self-cal, rms=0.062658Jy  sigma=0.616668
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=2.993 mas, bmaj=10.75 mas, bpa=-3.29 degrees
! Estimated noise=2.56151 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00261653 Jy
! Component: 100  -  total flux cleaned = -0.00261348 Jy
! Component: 150  -  total flux cleaned = -0.00261338 Jy
! Component: 200  -  total flux cleaned = -0.00261353 Jy
! Total flux subtracted in 200 components = -0.00261353 Jy
! Clean residual min=-0.004791 max=0.004595 Jy/beam
! Clean residual mean=0.000009 rms=0.001457 Jy/beam
! Combined flux in latest and established models = 0.987487 Jy
selfcal
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 80 components and 0.987487 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062620Jy  sigma=0.615915
! Fit after  self-cal, rms=0.062582Jy  sigma=0.615406
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 = -0.000408481 Jy
! Component: 100  -  total flux cleaned = -0.000474503 Jy
! Component: 150  -  total flux cleaned = -0.000494141 Jy
! Component: 200  -  total flux cleaned = -0.000509899 Jy
! Total flux subtracted in 200 components = -0.000509899 Jy
! Clean residual min=-0.004769 max=0.004892 Jy/beam
! Clean residual mean=0.000005 rms=0.001456 Jy/beam
! Combined flux in latest and established models = 0.986977 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 83 components and 0.986977 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062548Jy  sigma=0.615182
! Fit after  self-cal, rms=0.062526Jy  sigma=0.614953
! 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 "/d2/scr/pima/rdv96_uvs/J0106-4034_X\_map.fits"
! Inverting map and beam 
! Your choice of large map pixels excluded 4.61% of the data.
!  The x-axis pixel size should ideally be below 0.1769 milli-arcsec
! Estimated beam: bmin=0.9982 mas, bmaj=2.555 mas, bpa=-0.1309 degrees
! Estimated noise=2.36748 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9982 x 2.555 at -0.1309 degrees (North through East)
! Clean map  min=-0.01412  max=0.89197 Jy/beam
! Writing clean map to FITS file: /d2/scr/pima/rdv96_uvs/J0106-4034_X_map.fits
float peak_flux
peak_flux = peak(flux,max)
invert
! Inverting map 
! Your choice of large map pixels excluded 4.61% of the data.
!  The x-axis pixel size should ideally be below 0.1769 milli-arcsec
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=  0.8919  rms=  0.00329  Jy 
quit
! Quitting program
! Log file /d2/scr/pima/rdv96_uvs/J0106-4034_X_uvs.log closed on Fri Dec 20 23:43:33 2013