! Started logfile: /d2/scr/pima/rdv96_uvs/J1014+2301_X_uvs.log on Fri Dec 20 23:44:56 2013
obs /d2/scr/pima/rdv96_uvs/J1014+2301_X_uva.fits
! Reading UV FITS file: /d2/scr/pima/rdv96_uvs/J1014+2301_X_uva.fits
! AN table 1: 2 integrations on 10 of 10 possible baselines.
! AN table 2: 2 integrations on 21 of 21 possible baselines.
! AN table 3: 8 integrations on 45 of 45 possible baselines.
! AN table 4: 14 integrations on 45 of 45 possible baselines.
! AN table 5: 14 integrations on 55 of 55 possible baselines.
! Apparent sampling: 0.743688 visibilities/baseline/integration-bin.
! Found source: J1014+2301
! 
! 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 5420 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/J1014+2301_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: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:PT       self-cal  status=correctable  weight=1
! 2:BR       self-cal  status=correctable  weight=1
! 2:FD       self-cal  status=correctable  weight=1
! 2:KP       self-cal  status=correctable  weight=1
! 2:LA       self-cal  status=correctable  weight=1
! 2:NL       self-cal  status=correctable  weight=1
! 2:OV       self-cal  status=correctable  weight=1
! 2:PT       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: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:WZ       self-cal  status=correctable  weight=1
! 4:BR       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:OV       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:BR       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: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
! 5:WF       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 3 telescope corrections were flagged in sub-array 3.
!  A total of 10 telescope corrections were flagged in sub-array 4.
!  A total of 61 telescope corrections were flagged in sub-array 5.
! 
! Correcting IF 2.
!  A total of 3 telescope corrections were flagged in sub-array 3.
!  A total of 10 telescope corrections were flagged in sub-array 4.
!  A total of 61 telescope corrections were flagged in sub-array 5.
! 
! Correcting IF 3.
!  A total of 3 telescope corrections were flagged in sub-array 3.
!  A total of 10 telescope corrections were flagged in sub-array 4.
!  A total of 61 telescope corrections were flagged in sub-array 5.
! 
! Correcting IF 4.
!  A total of 3 telescope corrections were flagged in sub-array 3.
!  A total of 10 telescope corrections were flagged in sub-array 4.
!  A total of 61 telescope corrections were flagged in sub-array 5.
! 
! Fit before self-cal, rms=1.072905Jy  sigma=5.814297
! Fit after  self-cal, rms=0.689724Jy  sigma=3.263351
! 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 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.
![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=1.064 mas, bmaj=1.669 mas, bpa=16.09 degrees
! Estimated noise=3.14558 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 = 0.26534 Jy
! Component: 100  -  total flux cleaned = 0.345112 Jy
! Total flux subtracted in 100 components = 0.345112 Jy
! Clean residual min=-0.014152 max=0.053127 Jy/beam
! Clean residual mean=0.000031 rms=0.003759 Jy/beam
! Combined flux in latest and established models = 0.345112 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 8 components and 0.345112 Jy
! 
! Correcting IF 1.
!  A total of 8 telescope corrections were flagged in sub-array 3.
!  A total of 14 telescope corrections were flagged in sub-array 4.
!  A total of 10 telescope corrections were flagged in sub-array 5.
! 
! Correcting IF 2.
!  A total of 8 telescope corrections were flagged in sub-array 3.
!  A total of 14 telescope corrections were flagged in sub-array 4.
!  A total of 10 telescope corrections were flagged in sub-array 5.
! 
! Correcting IF 3.
!  A total of 8 telescope corrections were flagged in sub-array 3.
!  A total of 14 telescope corrections were flagged in sub-array 4.
!  A total of 10 telescope corrections were flagged in sub-array 5.
! 
! Correcting IF 4.
!  A total of 8 telescope corrections were flagged in sub-array 3.
!  A total of 14 telescope corrections were flagged in sub-array 4.
!  A total of 10 telescope corrections were flagged in sub-array 5.
! 
! Fit before self-cal, rms=0.100154Jy  sigma=0.630311
! Fit after  self-cal, rms=0.099013Jy  sigma=0.627108
! Inverting map and beam 
! Estimated beam: bmin=1.064 mas, bmaj=1.669 mas, bpa=16.09 degrees
! Estimated noise=3.14558 mJy/beam.
! Added new window around map position (1.8, -0.4).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.048517 Jy
! Component: 100  -  total flux cleaned = 0.0718305 Jy
! Total flux subtracted in 100 components = 0.0718305 Jy
! Clean residual min=-0.008279 max=0.022458 Jy/beam
! Clean residual mean=0.000019 rms=0.002121 Jy/beam
! Combined flux in latest and established models = 0.416943 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 22 components and 0.416943 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.071260Jy  sigma=0.406189
! Fit after  self-cal, rms=0.067488Jy  sigma=0.391906
! Inverting map 
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0182166 Jy
! Component: 100  -  total flux cleaned = 0.026448 Jy
! Total flux subtracted in 100 components = 0.026448 Jy
! Clean residual min=-0.006753 max=0.009610 Jy/beam
! Clean residual mean=0.000014 rms=0.001540 Jy/beam
! Combined flux in latest and established models = 0.443391 Jy
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 35 components and 0.443391 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.061984Jy  sigma=0.345616
! Fit after  self-cal, rms=0.060732Jy  sigma=0.341732
! 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=1.323 mas, bmaj=1.993 mas, bpa=14.86 degrees
! Estimated noise=1.94499 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 = 0.0111699 Jy
! Component: 100  -  total flux cleaned = 0.0164081 Jy
! Component: 150  -  total flux cleaned = 0.0195353 Jy
! Component: 200  -  total flux cleaned = 0.0207937 Jy
! Total flux subtracted in 200 components = 0.0207937 Jy
! Clean residual min=-0.005860 max=0.005626 Jy/beam
! Clean residual mean=0.000017 rms=0.001344 Jy/beam
! Combined flux in latest and established models = 0.464184 Jy
! Performing phase self-cal
! Adding 28 model components to the UV plane model.
! The established model now contains 53 components and 0.464184 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.059112Jy  sigma=0.327413
! Fit after  self-cal, rms=0.058668Jy  sigma=0.326174
! 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        1.06     FD        1.05     KP        1.13     LA        1.03     
!   PT        1.02     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.04     FD        1.03     KP        1.04     LA        1.08     
!   NL        1.02     OV        1.09     PT        1.01     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.98     FD        1.00     HN        1.01     KP        1.02     
!   LA        1.04     NL        0.99     OV        1.01     PT        1.00     
!   SC        0.97     WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        0.98     FD        1.01     HN        1.03     KP        1.03     
!   LA        1.03     NL        1.02     OV        1.02     PT        1.00     
!   SC        1.03     WF        1.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 5.
!  Telescope amplitude corrections in sub-array 5:
!   BR        0.98     FD        1.02     HN        1.04     KP        1.02     
!   LA        1.04     MK        0.99     NL        0.98     OV        1.01     
!   PT        0.99     SC        1.01     WF        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.08     FD        1.04     KP        0.97     LA        1.04     
!   PT        1.07     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.04     FD        1.03     KP        0.99     LA        1.05     
!   NL        1.01     OV        1.04     PT        1.03     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.97     FD        1.00     HN        1.02     KP        0.98     
!   LA        0.99     NL        0.99     OV        1.01     PT        0.98     
!   SC        1.03     WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        0.97     FD        1.01     HN        1.04     KP        0.97     
!   LA        1.00     NL        1.02     OV        1.00     PT        1.00     
!   SC        1.04     WF        1.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 5.
!  Telescope amplitude corrections in sub-array 5:
!   BR        0.99     FD        1.01     HN        1.03     KP        0.96     
!   LA        1.00     MK        0.96     NL        0.99     OV        1.01     
!   PT        0.98     SC        1.02     WF        1.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.13     FD        1.00     KP        0.86     LA        1.13     
!   PT        0.99     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.13     FD        1.01     KP        0.83     LA        1.09     
!   NL        1.08     OV        1.04     PT        1.06     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.06     FD        0.96     HN        1.08     KP        0.85     
!   LA        1.05     NL        0.99     OV        1.02     PT        0.98     
!   SC        0.96     WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.03     FD        0.98     HN        1.04     KP        0.85     
!   LA        1.06     NL        1.00     OV        1.04     PT        0.98     
!   SC        0.99     WF        1.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 5.
!  Telescope amplitude corrections in sub-array 5:
!   BR        1.01     FD        1.00     HN        1.04     KP        0.83     
!   LA        1.06     MK        0.97     NL        0.97     OV        1.05     
!   PT        0.97     SC        1.02     WF        1.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.26     FD        1.07     KP        0.96     LA        1.08     
!   PT        1.04     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.07     FD        1.05     KP        0.94     LA        1.11     
!   NL        1.08     OV        1.01     PT        1.03     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.02     FD        1.03     HN        1.03     KP        0.89     
!   LA        1.02     NL        0.99     OV        1.02     PT        1.00     
!   SC        0.96     WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00     FD        1.02     HN        1.01     KP        0.90     
!   LA        1.05     NL        1.03     OV        1.00     PT        1.03     
!   SC        1.00     WF        1.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 5.
!  Telescope amplitude corrections in sub-array 5:
!   BR        1.02     FD        1.02     HN        0.99     KP        0.90     
!   LA        1.02     MK        1.03     NL        1.01     OV        1.00     
!   PT        1.02     SC        0.97     WF        1.00*    
! 
! 
! Fit before self-cal, rms=0.058668Jy  sigma=0.326174
! Fit after  self-cal, rms=0.053387Jy  sigma=0.281691
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=1.33 mas, bmaj=1.994 mas, bpa=15.01 degrees
! Estimated noise=1.94412 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 (5.6, -2.4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00173409 Jy
! Component: 100  -  total flux cleaned = 0.0024759 Jy
! Component: 150  -  total flux cleaned = 0.00297611 Jy
! Component: 200  -  total flux cleaned = 0.00348308 Jy
! Total flux subtracted in 200 components = 0.00348308 Jy
! Clean residual min=-0.002969 max=0.002687 Jy/beam
! Clean residual mean=-0.000000 rms=0.000656 Jy/beam
! Combined flux in latest and established models = 0.467667 Jy
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 68 components and 0.467667 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.052759Jy  sigma=0.278450
! Fit after  self-cal, rms=0.052594Jy  sigma=0.277790
! 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=0.052594Jy  sigma=0.277790
! Fit after  self-cal, rms=0.052606Jy  sigma=0.277579
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=1.333 mas, bmaj=1.997 mas, bpa=15.09 degrees
! Estimated noise=1.94233 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000217327 Jy
! Component: 100  -  total flux cleaned = 0.000926327 Jy
! Component: 150  -  total flux cleaned = 0.00136615 Jy
! Component: 200  -  total flux cleaned = 0.00168139 Jy
! Total flux subtracted in 200 components = 0.00168139 Jy
! Clean residual min=-0.002684 max=0.002456 Jy/beam
! Clean residual mean=0.000000 rms=0.000597 Jy/beam
! Combined flux in latest and established models = 0.469349 Jy
selfcal
! Performing phase self-cal
! Adding 26 model components to the UV plane model.
! The established model now contains 82 components and 0.469349 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.052297Jy  sigma=0.276121
! Fit after  self-cal, rms=0.052164Jy  sigma=0.275787
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 = 0.000496984 Jy
! Component: 100  -  total flux cleaned = 0.00107994 Jy
! Component: 150  -  total flux cleaned = 0.00134711 Jy
! Component: 200  -  total flux cleaned = 0.00148805 Jy
! Total flux subtracted in 200 components = 0.00148805 Jy
! Clean residual min=-0.002541 max=0.002360 Jy/beam
! Clean residual mean=0.000000 rms=0.000571 Jy/beam
! Combined flux in latest and established models = 0.470837 Jy
! Performing phase self-cal
! Adding 25 model components to the UV plane model.
! The established model now contains 89 components and 0.470837 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.051991Jy  sigma=0.275010
! Fit after  self-cal, rms=0.051897Jy  sigma=0.274811
! 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=0.051897Jy  sigma=0.274811
! Fit after  self-cal, rms=0.051864Jy  sigma=0.273967
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=1.337 mas, bmaj=2 mas, bpa=15.17 degrees
! Estimated noise=1.94238 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -6.51755e-05 Jy
! Component: 100  -  total flux cleaned = 0.000341815 Jy
! Component: 150  -  total flux cleaned = 0.000532544 Jy
! Component: 200  -  total flux cleaned = 0.00070015 Jy
! Total flux subtracted in 200 components = 0.00070015 Jy
! Clean residual min=-0.002331 max=0.002184 Jy/beam
! Clean residual mean=0.000001 rms=0.000542 Jy/beam
! Combined flux in latest and established models = 0.471537 Jy
selfcal
! Performing phase self-cal
! Adding 23 model components to the UV plane model.
! The established model now contains 93 components and 0.471537 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.051726Jy  sigma=0.273360
! Fit after  self-cal, rms=0.051656Jy  sigma=0.273198
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 = 0.000215278 Jy
! Component: 100  -  total flux cleaned = 0.000528733 Jy
! Component: 150  -  total flux cleaned = 0.000678283 Jy
! Component: 200  -  total flux cleaned = 0.000711509 Jy
! Total flux subtracted in 200 components = 0.000711509 Jy
! Clean residual min=-0.002240 max=0.002138 Jy/beam
! Clean residual mean=0.000001 rms=0.000529 Jy/beam
! Combined flux in latest and established models = 0.472249 Jy
! Performing phase self-cal
! Adding 31 model components to the UV plane model.
! The established model now contains 102 components and 0.472249 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.051568Jy  sigma=0.272835
! Fit after  self-cal, rms=0.051516Jy  sigma=0.272731
! 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=0.051516Jy  sigma=0.272731
! Fit after  self-cal, rms=0.051566Jy  sigma=0.272669
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=2.933 mas, bmaj=3.209 mas, bpa=-49.35 degrees
! Estimated noise=1.97246 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -6.76496e-05 Jy
! Component: 100  -  total flux cleaned = -0.000191836 Jy
! Component: 150  -  total flux cleaned = -0.00022596 Jy
! Component: 200  -  total flux cleaned = -0.000198873 Jy
! Total flux subtracted in 200 components = -0.000198873 Jy
! Clean residual min=-0.002159 max=0.001895 Jy/beam
! Clean residual mean=0.000001 rms=0.000564 Jy/beam
! Combined flux in latest and established models = 0.47205 Jy
selfcal
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 113 components and 0.47205 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.051547Jy  sigma=0.272382
! Fit after  self-cal, rms=0.051509Jy  sigma=0.272297
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 = 3.5639e-05 Jy
! Component: 100  -  total flux cleaned = 6.99885e-05 Jy
! Component: 150  -  total flux cleaned = 9.315e-05 Jy
! Component: 200  -  total flux cleaned = 0.000114361 Jy
! Total flux subtracted in 200 components = 0.000114361 Jy
! Clean residual min=-0.002161 max=0.001867 Jy/beam
! Clean residual mean=0.000000 rms=0.000556 Jy/beam
! Combined flux in latest and established models = 0.472164 Jy
! Performing phase self-cal
! Adding 24 model components to the UV plane model.
! The established model now contains 117 components and 0.472164 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.051489Jy  sigma=0.272116
! Fit after  self-cal, rms=0.051457Jy  sigma=0.272051
! 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 "/d2/scr/pima/rdv96_uvs/J1014+2301_X\_map.fits"
! Inverting map and beam 
! Estimated beam: bmin=1.182 mas, bmaj=1.938 mas, bpa=5.451 degrees
! Estimated noise=1.9811 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 1.182 x 1.938 at 5.451 degrees (North through East)
! Clean map  min=-0.0029611  max=0.31451 Jy/beam
! Writing clean map to FITS file: /d2/scr/pima/rdv96_uvs/J1014+2301_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=  0.3145  rms=  0.0008  Jy 
quit
! Quitting program
! Log file /d2/scr/pima/rdv96_uvs/J1014+2301_X_uvs.log closed on Fri Dec 20 23:44:59 2013