! Started logfile: J2319-3656_X_2010_06_23_pus_uvs.log on Thu Jan 27 23:45:02 2011
obs J2319-3656_X_2010_06_23_pus_uva.fits
! Reading UV FITS file: J2319-3656_X_2010_06_23_pus_uva.fits
! AN table 1: 188 integrations on 105 of 105 possible baselines.
! Apparent sampling: 0.188602 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J2319-3656
! 
! 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  8.40996e+09        8e+06          1        8e+06
!  02        2  8.47996e+09        8e+06          1        8e+06
!  03        3  8.79496e+09        8e+06          1        8e+06
!  04        4  8.89996e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 3588 lines of history.
! 
! Reading 14892 visibilities.
select I
! Polarization I is unavailable.
! 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 = 256 
print "field_cell =",field_cell
! field_cell = 0.2 
print "taper_size =",taper_size
! taper_size = 70 
![@muppet J2319-3656_X_2010_06_23_pus]
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.03
float dynam
dynam = 6.0
float soltime1
soltime1 = 120
float soltime2
soltime2 = 20
float thresh
thresh = 0.5
float win_mult
win_mult = 1.8
float time_av
time_av = 16
float old_peak
float new_peak
float flux_cutoff
mapsize field_size, field_cell
! Map grid = 256x256 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 1682 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 1689 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 1720 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 1822 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.981380Jy  sigma=0.010505
! Fit after  self-cal, rms=0.925102Jy  sigma=0.009973
! clrmod: Cleared the established, tentative and continuum models.
! Redundant starting model cleared.
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 
! Your choice of large map pixels excluded 0.886% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
! Estimated beam: bmin=0.6758 mas, bmaj=1.971 mas, bpa=3.659 degrees
! Estimated noise=1226.74 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 = 0.0612438 Jy
! Component: 100  -  total flux cleaned = 0.0765104 Jy
! Total flux subtracted in 100 components = 0.0765104 Jy
! Clean residual min=-0.004810 max=0.006998 Jy/beam
! Clean residual mean=0.000124 rms=0.001715 Jy/beam
! Combined flux in latest and established models = 0.0765104 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 7 components and 0.0765104 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.139244Jy  sigma=0.001244
! Fit after  self-cal, rms=0.138534Jy  sigma=0.001238
! Inverting map 
! Your choice of large map pixels excluded 0.886% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
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 
! Your choice of large map pixels excluded 0.886% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
! Estimated beam: bmin=0.8685 mas, bmaj=2.479 mas, bpa=-1.25 degrees
! Estimated noise=583.96 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 = 0.00908083 Jy
! Component: 100  -  total flux cleaned = 0.0124407 Jy
! Component: 150  -  total flux cleaned = 0.0138216 Jy
! Component: 200  -  total flux cleaned = 0.0138206 Jy
! Total flux subtracted in 200 components = 0.0138206 Jy
! Clean residual min=-0.002698 max=0.002922 Jy/beam
! Clean residual mean=-0.000104 rms=0.000877 Jy/beam
! Combined flux in latest and established models = 0.0903311 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 18 components and 0.090331 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.137874Jy  sigma=0.001233
! Fit after  self-cal, rms=0.137782Jy  sigma=0.001232
! Inverting map 
! Your choice of large map pixels excluded 0.886% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.02     HN        0.66     KK        1.00*    
!   KP        1.03     LA        0.98     MA        1.00*    MK        1.07     
!   NL        0.97     NY        1.00*    OV        0.99     PT        1.02     
!   SC        1.09     TS        1.00*    ZC        1.00*    
! 
! 
! Correcting IF 2.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00     HN        0.68     KK        1.00*    
!   KP        0.97     LA        1.03     MA        1.00*    MK        1.12     
!   NL        1.06     NY        1.00*    OV        1.03     PT        1.04     
!   SC        1.06     TS        1.00*    ZC        1.00*    
! 
! 
! Correcting IF 3.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.95     HN        0.60     KK        1.00*    
!   KP        0.97     LA        1.03     MA        1.00*    MK        0.99     
!   NL        1.03     NY        1.00*    OV        1.00     PT        1.03     
!   SC        1.02     TS        1.00*    ZC        1.00*    
! 
! 
! Correcting IF 4.
!  A total of 111 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.91     HN        0.68     KK        1.00*    
!   KP        1.02     LA        1.01     MA        1.00*    MK        0.92     
!   NL        1.01     NY        1.00*    OV        0.97     PT        1.00     
!   SC        0.87     TS        1.00*    ZC        1.00*    
! 
! 
! Fit before self-cal, rms=0.137782Jy  sigma=0.001232
! Fit after  self-cal, rms=0.124340Jy  sigma=0.001231
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
! Estimated beam: bmin=0.8716 mas, bmaj=2.479 mas, bpa=-1.372 degrees
! Estimated noise=584.986 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 = 0.000830199 Jy
! Component: 100  -  total flux cleaned = 0.000829562 Jy
! Component: 150  -  total flux cleaned = 0.000829739 Jy
! Component: 200  -  total flux cleaned = 0.000807703 Jy
! Total flux subtracted in 200 components = 0.000807703 Jy
! Clean residual min=-0.002654 max=0.002833 Jy/beam
! Clean residual mean=-0.000052 rms=0.000805 Jy/beam
! Combined flux in latest and established models = 0.0911388 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 24 components and 0.0911388 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.124328Jy  sigma=0.001231
! Fit after  self-cal, rms=0.124120Jy  sigma=0.001230
! Inverting map 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
selfcal true, true, soltime1
! Performing amp+phase self-cal over 120 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.124120Jy  sigma=0.001230
! Fit after  self-cal, rms=0.122985Jy  sigma=0.001229
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
! Estimated beam: bmin=0.867 mas, bmaj=2.469 mas, bpa=-1.395 degrees
! Estimated noise=584.08 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000756815 Jy
! Component: 100  -  total flux cleaned = 0.000779296 Jy
! Component: 150  -  total flux cleaned = 0.000779839 Jy
! Component: 200  -  total flux cleaned = 0.000779894 Jy
! Total flux subtracted in 200 components = 0.000779894 Jy
! Clean residual min=-0.002606 max=0.002277 Jy/beam
! Clean residual mean=-0.000089 rms=0.000724 Jy/beam
! Combined flux in latest and established models = 0.0919187 Jy
selfcal
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 29 components and 0.0919186 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.122975Jy  sigma=0.001229
! Fit after  self-cal, rms=0.122976Jy  sigma=0.001229
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
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 = 1.98899e-05 Jy
! Component: 100  -  total flux cleaned = 3.8173e-05 Jy
! Component: 150  -  total flux cleaned = 2.24334e-05 Jy
! Component: 200  -  total flux cleaned = 2.25553e-05 Jy
! Total flux subtracted in 200 components = 2.25553e-05 Jy
! Clean residual min=-0.002598 max=0.002321 Jy/beam
! Clean residual mean=-0.000099 rms=0.000727 Jy/beam
! Combined flux in latest and established models = 0.0919412 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 30 components and 0.0919412 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.122972Jy  sigma=0.001229
! Fit after  self-cal, rms=0.122969Jy  sigma=0.001229
! Inverting map 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
selfcal true, true, soltime2
! Performing amp+phase self-cal over 20 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.122969Jy  sigma=0.001229
! Fit after  self-cal, rms=0.122949Jy  sigma=0.001229
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
! Estimated beam: bmin=0.8611 mas, bmaj=2.454 mas, bpa=-1.467 degrees
! Estimated noise=583.837 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000793008 Jy
! Component: 100  -  total flux cleaned = 0.000836481 Jy
! Component: 150  -  total flux cleaned = 0.00085142 Jy
! Component: 200  -  total flux cleaned = 0.00083761 Jy
! Total flux subtracted in 200 components = 0.00083761 Jy
! Clean residual min=-0.002581 max=0.002345 Jy/beam
! Clean residual mean=-0.000086 rms=0.000729 Jy/beam
! Combined flux in latest and established models = 0.0927788 Jy
selfcal
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 32 components and 0.0927788 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.122940Jy  sigma=0.001229
! Fit after  self-cal, rms=0.122943Jy  sigma=0.001229
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
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 = 3.80139e-05 Jy
! Component: 100  -  total flux cleaned = 2.30395e-05 Jy
! Component: 150  -  total flux cleaned = 2.31703e-05 Jy
! Component: 200  -  total flux cleaned = 9.30745e-06 Jy
! Total flux subtracted in 200 components = 9.30745e-06 Jy
! Clean residual min=-0.002600 max=0.002356 Jy/beam
! Clean residual mean=-0.000089 rms=0.000731 Jy/beam
! Combined flux in latest and established models = 0.0927881 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 33 components and 0.0927881 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.122940Jy  sigma=0.001229
! Fit after  self-cal, rms=0.122937Jy  sigma=0.001229
! Inverting map 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
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 20 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.122937Jy  sigma=0.001229
! Fit after  self-cal, rms=0.122751Jy  sigma=0.001229
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
! Estimated beam: bmin=2.607 mas, bmaj=8.093 mas, bpa=-1.465 degrees
! Estimated noise=753.31 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000853239 Jy
! Component: 100  -  total flux cleaned = 0.000916172 Jy
! Component: 150  -  total flux cleaned = 0.000915662 Jy
! Component: 200  -  total flux cleaned = 0.00091609 Jy
! Total flux subtracted in 200 components = 0.00091609 Jy
! Clean residual min=-0.003120 max=0.002893 Jy/beam
! Clean residual mean=-0.000163 rms=0.000977 Jy/beam
! Combined flux in latest and established models = 0.0937042 Jy
selfcal
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 38 components and 0.0937042 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.122747Jy  sigma=0.001229
! Fit after  self-cal, rms=0.122738Jy  sigma=0.001229
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
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 = 4.06298e-05 Jy
! Component: 100  -  total flux cleaned = 4.08677e-05 Jy
! Component: 150  -  total flux cleaned = 2.93428e-05 Jy
! Component: 200  -  total flux cleaned = 1.95784e-05 Jy
! Total flux subtracted in 200 components = 1.95784e-05 Jy
! Clean residual min=-0.003105 max=0.002911 Jy/beam
! Clean residual mean=-0.000166 rms=0.000970 Jy/beam
! Combined flux in latest and established models = 0.0937238 Jy
! Performing phase self-cal
! Adding 3 model components to the UV plane model.
! The established model now contains 39 components and 0.0937238 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.122738Jy  sigma=0.001229
! Fit after  self-cal, rms=0.122731Jy  sigma=0.001229
! Inverting map 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
win_mult = win_mult / 1.2
print "************** FINISHED AMPLITUDE SELF-CAL **************"
! ************** FINISHED AMPLITUDE SELF-CAL ************** 
restore
! Inverting map and beam 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
! Estimated beam: bmin=0.8549 mas, bmaj=2.438 mas, bpa=-1.529 degrees
! Estimated noise=582.908 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8549 x 2.438 at -1.529 degrees (North through East)
! Clean map  min=-0.0025174  max=0.082231 Jy/beam
if(peak(flux) > thresh)
  selfcal true, true
  clean clean_niter,clean_gain
  selfcal
  flux_cutoff = imstat(rms) * dynam
  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)
  selfcal true, true
  end if
print "************** CLEARING MODEL AND STARTING OVER **********"
! ************** CLEARING MODEL AND STARTING OVER ********** 
clrmod true
! clrmod: Cleared the established and tentative models.
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.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
! Estimated beam: bmin=0.6758 mas, bmaj=1.966 mas, bpa=3.109 degrees
! Estimated noise=1176.55 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0589256 Jy
! Component: 100  -  total flux cleaned = 0.07394 Jy
! Component: 150  -  total flux cleaned = 0.0808098 Jy
! Component: 200  -  total flux cleaned = 0.0850397 Jy
! Total flux subtracted in 200 components = 0.0850397 Jy
! Clean residual min=-0.003842 max=0.003764 Jy/beam
! Clean residual mean=0.000040 rms=0.001214 Jy/beam
! Combined flux in latest and established models = 0.0850398 Jy
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.
flux_cutoff = imstat(rms) * dynam
! Adding 16 model components to the UV plane model.
! The established model now contains 16 components and 0.0850398 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
! Estimated beam: bmin=0.8549 mas, bmaj=2.438 mas, bpa=-1.529 degrees
! Estimated noise=582.908 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  keep
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00538807 Jy
! Component: 100  -  total flux cleaned = 0.00762167 Jy
! Component: 150  -  total flux cleaned = 0.00862243 Jy
! Component: 200  -  total flux cleaned = 0.00878619 Jy
! Total flux subtracted in 200 components = 0.00878619 Jy
! Clean residual min=-0.002684 max=0.002240 Jy/beam
! Clean residual mean=-0.000091 rms=0.000747 Jy/beam
! Combined flux in latest and established models = 0.093826 Jy
! Adding 15 model components to the UV plane model.
! The established model now contains 28 components and 0.093826 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
! Estimated beam: bmin=2.607 mas, bmaj=8.093 mas, bpa=-1.465 degrees
! Estimated noise=753.31 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000107532 Jy
! Component: 100  -  total flux cleaned = 0.000107723 Jy
! Component: 150  -  total flux cleaned = 0.000119662 Jy
! Component: 200  -  total flux cleaned = 0.000130857 Jy
! Total flux subtracted in 200 components = 0.000130857 Jy
! Clean residual min=-0.003106 max=0.002944 Jy/beam
! Clean residual mean=-0.000174 rms=0.000976 Jy/beam
! Combined flux in latest and established models = 0.0939568 Jy
flux_cutoff = imstat(rms) * dynam
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  keep
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 1.05938e-06 Jy
! Component: 100  -  total flux cleaned = 1.20585e-06 Jy
! Component: 150  -  total flux cleaned = 2.08026e-07 Jy
! Component: 200  -  total flux cleaned = -6.29506e-07 Jy
! Total flux subtracted in 200 components = -6.29506e-07 Jy
! Clean residual min=-0.003102 max=0.002932 Jy/beam
! Clean residual mean=-0.000174 rms=0.000976 Jy/beam
! Combined flux in latest and established models = 0.0939562 Jy
! Adding 7 model components to the UV plane model.
! The established model now contains 32 components and 0.0939562 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
! Estimated beam: bmin=0.8549 mas, bmaj=2.438 mas, bpa=-1.529 degrees
! Estimated noise=582.908 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000198115 Jy
! Component: 100  -  total flux cleaned = -0.00014781 Jy
! Component: 150  -  total flux cleaned = -0.000128481 Jy
! Component: 200  -  total flux cleaned = -0.000128757 Jy
! Total flux subtracted in 200 components = -0.000128757 Jy
! Clean residual min=-0.002686 max=0.002264 Jy/beam
! Clean residual mean=-0.000091 rms=0.000739 Jy/beam
! Combined flux in latest and established models = 0.0938274 Jy
selfcal
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 36 components and 0.0938274 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.122744Jy  sigma=0.001229
! Fit after  self-cal, rms=0.122747Jy  sigma=0.001229
wmodel J2319-3656_X_2010_06_23_pus_map.mod
! Writing 36 model components to file: J2319-3656_X_2010_06_23_pus_map.mod
wobs J2319-3656_X_2010_06_23_pus_uvs.fits
! Writing UV FITS file: J2319-3656_X_2010_06_23_pus_uvs.fits
wwins J2319-3656_X_2010_06_23_pus_map.win
! wwins: Wrote 1 windows to J2319-3656_X_2010_06_23_pus_map.win
x = (field_size-8) * field_cell / 4
addwin -x,x,-x,x
clean (field_size*4),0.01
! Inverting map 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000491444 Jy
! Component: 100  -  total flux cleaned = -0.000450339 Jy
! Component: 150  -  total flux cleaned = -0.000522835 Jy
! Component: 200  -  total flux cleaned = -0.00052258 Jy
! Component: 250  -  total flux cleaned = -0.000583742 Jy
! Component: 300  -  total flux cleaned = -0.000582255 Jy
! Component: 350  -  total flux cleaned = -0.000720208 Jy
! Component: 400  -  total flux cleaned = -0.000904274 Jy
! Component: 450  -  total flux cleaned = -0.00108175 Jy
! Component: 500  -  total flux cleaned = -0.00127586 Jy
! Component: 550  -  total flux cleaned = -0.00143978 Jy
! Component: 600  -  total flux cleaned = -0.00159691 Jy
! Component: 650  -  total flux cleaned = -0.00174834 Jy
! Component: 700  -  total flux cleaned = -0.0018537 Jy
! Component: 750  -  total flux cleaned = -0.00191459 Jy
! Component: 800  -  total flux cleaned = -0.00195426 Jy
! Component: 850  -  total flux cleaned = -0.00199279 Jy
! Component: 900  -  total flux cleaned = -0.00210422 Jy
! Component: 950  -  total flux cleaned = -0.00214011 Jy
! Component: 1000  -  total flux cleaned = -0.00221108 Jy
! Total flux subtracted in 1024 components = -0.00224613 Jy
! Clean residual min=-0.001069 max=0.001172 Jy/beam
! Clean residual mean=-0.000024 rms=0.000376 Jy/beam
! Combined flux in latest and established models = 0.0915813 Jy
keep
! Adding 73 model components to the UV plane model.
! The established model now contains 109 components and 0.0915813 Jy
![Exited script file: muppet]
wmap "J2319-3656_X_2010_06_23_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8549 x 2.438 at -1.529 degrees (North through East)
! Clean map  min=-0.0018833  max=0.080824 Jy/beam
! Writing clean map to FITS file: J2319-3656_X_2010_06_23_pus_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.0808243 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.894% of the data.
!  The x-axis pixel size should ideally be below 0.1961 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000379496 
device "J2319-3656_X_2010_06_23_pus\_map.eps/VPS"
! Attempting to open device: 'J2319-3656_X_2010_06_23_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -1.4086 1.4086 2.81719 5.63439 11.2688 22.5375 45.0751 90.1502
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0011 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.08 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8549 x 2.438 at -1.529 degrees (North through East)
! Clean map  min=-0.0018833  max=0.080824 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J2319-3656_X_2010_06_23_pus\_map.gif/vgif"
! Attempting to open device: 'J2319-3656_X_2010_06_23_pus_map.gif/vgif'
mapplot cln