! Started logfile: J2331-3811_X_2009_04_21_pus_uvs.log on Sun Jan 23 16:50:14 2011
obs J2331-3811_X_2009_04_21_pus_uva.fits
! Reading UV FITS file: J2331-3811_X_2009_04_21_pus_uva.fits
! AN table 1: 117 integrations on 120 of 120 possible baselines.
! AN table 2: 74 integrations on 120 of 120 possible baselines.
! AN table 3: 34 integrations on 120 of 120 possible baselines.
! Apparent sampling: 0.108111 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J2331-3811
! 
! 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  8.40997e+09        8e+06          1        8e+06
!  02        2  8.47997e+09        8e+06          1        8e+06
!  03        3  8.79497e+09        8e+06          1        8e+06
!  04        4  8.89997e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 3297 lines of history.
! 
! Reading 11676 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 = 512 
print "field_cell =",field_cell
! field_cell = 0.2 
print "taper_size =",taper_size
! taper_size = 70 
![@muppet J2331-3811_X_2009_04_21_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 = 512x512 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 1490 telescope corrections were flagged in sub-array 1.
!  A total of 908 telescope corrections were flagged in sub-array 2.
!  A total of 305 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 1490 telescope corrections were flagged in sub-array 1.
!  A total of 908 telescope corrections were flagged in sub-array 2.
!  A total of 305 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 1490 telescope corrections were flagged in sub-array 1.
!  A total of 908 telescope corrections were flagged in sub-array 2.
!  A total of 305 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 1490 telescope corrections were flagged in sub-array 1.
!  A total of 908 telescope corrections were flagged in sub-array 2.
!  A total of 305 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=0.793346Jy  sigma=0.005560
! Fit after  self-cal, rms=0.513816Jy  sigma=0.003544
! 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 1.08% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
! Estimated beam: bmin=0.5986 mas, bmaj=1.898 mas, bpa=-0.1866 degrees
! Estimated noise=1642.21 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 = 0.389257 Jy
! Component: 100  -  total flux cleaned = 0.482474 Jy
! Total flux subtracted in 100 components = 0.482474 Jy
! Clean residual min=-0.022202 max=0.036600 Jy/beam
! Clean residual mean=0.000011 rms=0.005969 Jy/beam
! Combined flux in latest and established models = 0.482474 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 7 components and 0.482474 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.219491Jy  sigma=0.001451
! Fit after  self-cal, rms=0.219464Jy  sigma=0.001451
! Inverting map 
! Your choice of large map pixels excluded 1.08% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0403815 Jy
! Component: 100  -  total flux cleaned = 0.0632569 Jy
! Total flux subtracted in 100 components = 0.0632569 Jy
! Clean residual min=-0.020234 max=0.026508 Jy/beam
! Clean residual mean=-0.000069 rms=0.005022 Jy/beam
! Combined flux in latest and established models = 0.545731 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 19 components and 0.545731 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.206216Jy  sigma=0.001350
! Fit after  self-cal, rms=0.206202Jy  sigma=0.001350
! Inverting map 
! Your choice of large map pixels excluded 1.08% of the data.
!  The x-axis pixel size should ideally be below 0.1933 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 1.08% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
! Estimated beam: bmin=0.7491 mas, bmaj=2.213 mas, bpa=-2.34 degrees
! Estimated noise=968.638 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 = 0.0296288 Jy
! Component: 100  -  total flux cleaned = 0.0439083 Jy
! Component: 150  -  total flux cleaned = 0.0508992 Jy
! Component: 200  -  total flux cleaned = 0.0543251 Jy
! Total flux subtracted in 200 components = 0.0543251 Jy
! Clean residual min=-0.023826 max=0.024509 Jy/beam
! Clean residual mean=-0.000474 rms=0.005966 Jy/beam
! Combined flux in latest and established models = 0.600056 Jy
! Performing phase self-cal
! Adding 20 model components to the UV plane model.
! The established model now contains 34 components and 0.600056 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.202261Jy  sigma=0.001323
! Fit after  self-cal, rms=0.202267Jy  sigma=0.001322
! Inverting map 
! Your choice of large map pixels excluded 1.08% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 33 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.83     HN        1.00*    KB        1.00     
!   KK        1.09     KP        0.93     LA        1.07     MK        0.94     
!   NL        1.23     NY        1.00*    OV        1.04     PT        1.04     
!   SC        0.97     TS        1.12     WZ        1.00*    ZC        1.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00*    FD        0.80     HN        1.00*    KB        1.00*    
!   KK        1.00*    KP        0.91     LA        1.06     MK        1.00*    
!   NL        1.16     NY        1.00*    OV        1.04     PT        1.04     
!   SC        0.99     TS        1.00*    WZ        1.00*    ZC        1.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        0.82     HN        1.00*    KB        1.00*    
!   KK        1.16     KP        0.90     LA        1.06     MK        0.92     
!   NL        1.26     NY        1.00*    OV        1.02     PT        1.00     
!   SC        0.94     TS        1.00*    WZ        1.00*    ZC        1.00*    
! 
! 
! Correcting IF 2.
!  A total of 33 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.85     HN        1.00*    KB        1.11     
!   KK        1.06     KP        0.88     LA        1.06     MK        0.95     
!   NL        1.22     NY        1.00*    OV        1.01     PT        1.10     
!   SC        0.96     TS        1.10     WZ        1.00*    ZC        1.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00*    FD        0.81     HN        1.00*    KB        1.00*    
!   KK        1.00*    KP        0.87     LA        1.06     MK        1.00*    
!   NL        1.15     NY        1.00*    OV        0.99     PT        1.07     
!   SC        0.99     TS        1.00*    WZ        1.00*    ZC        1.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        0.85     HN        1.00*    KB        1.00*    
!   KK        1.08     KP        0.87     LA        1.03     MK        0.92     
!   NL        1.19     NY        1.00*    OV        0.97     PT        1.07     
!   SC        0.97     TS        1.00*    WZ        1.00*    ZC        1.00*    
! 
! 
! Correcting IF 3.
!  A total of 33 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.85     HN        1.00*    KB        1.03     
!   KK        1.10     KP        0.82     LA        1.05     MK        0.96     
!   NL        1.28     NY        1.00*    OV        1.05     PT        1.08     
!   SC        1.05     TS        1.10     WZ        1.00*    ZC        1.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00*    FD        0.82     HN        1.00*    KB        1.00*    
!   KK        1.00*    KP        0.80     LA        1.10     MK        1.00*    
!   NL        1.18     NY        1.00*    OV        1.03     PT        1.09     
!   SC        0.99     TS        1.00*    WZ        1.00*    ZC        1.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        0.85     HN        1.00*    KB        1.00*    
!   KK        1.11     KP        0.76     LA        1.10     MK        1.03     
!   NL        1.21     NY        1.00*    OV        1.00     PT        1.09     
!   SC        0.97     TS        1.00*    WZ        1.00*    ZC        1.00*    
! 
! 
! Correcting IF 4.
!  A total of 33 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.87     HN        1.00*    KB        1.11     
!   KK        1.08     KP        0.86     LA        1.06     MK        0.96     
!   NL        1.30     NY        1.00*    OV        1.05     PT        1.12     
!   SC        1.04     TS        1.14     WZ        1.00*    ZC        1.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00*    FD        0.85     HN        1.00*    KB        1.00*    
!   KK        1.00*    KP        0.83     LA        1.07     MK        1.00*    
!   NL        1.20     NY        1.00*    OV        1.05     PT        1.05     
!   SC        1.08     TS        1.00*    WZ        1.00*    ZC        1.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        0.85     HN        1.00*    KB        1.00*    
!   KK        1.10     KP        0.84     LA        1.11     MK        0.98     
!   NL        1.23     NY        1.00*    OV        1.01     PT        1.06     
!   SC        1.06     TS        1.00*    WZ        1.00*    ZC        1.00*    
! 
! 
! Fit before self-cal, rms=0.202267Jy  sigma=0.001322
! Fit after  self-cal, rms=0.189973Jy  sigma=0.001189
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
! Estimated beam: bmin=0.758 mas, bmaj=2.254 mas, bpa=-2.643 degrees
! Estimated noise=974.389 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 = -0.00383848 Jy
! Component: 100  -  total flux cleaned = -0.00391857 Jy
! Component: 150  -  total flux cleaned = -0.00391806 Jy
! Component: 200  -  total flux cleaned = -0.00396904 Jy
! Total flux subtracted in 200 components = -0.00396904 Jy
! Clean residual min=-0.005174 max=0.004972 Jy/beam
! Clean residual mean=0.000139 rms=0.001359 Jy/beam
! Combined flux in latest and established models = 0.596087 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 39 components and 0.596087 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.189837Jy  sigma=0.001188
! Fit after  self-cal, rms=0.190275Jy  sigma=0.001187
! Inverting map 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 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=0.190275Jy  sigma=0.001187
! Fit after  self-cal, rms=0.190067Jy  sigma=0.001183
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
! Estimated beam: bmin=0.7602 mas, bmaj=2.255 mas, bpa=-2.583 degrees
! Estimated noise=974.051 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00212372 Jy
! Component: 100  -  total flux cleaned = -0.00235701 Jy
! Component: 150  -  total flux cleaned = -0.00249365 Jy
! Component: 200  -  total flux cleaned = -0.00264526 Jy
! Total flux subtracted in 200 components = -0.00264526 Jy
! Clean residual min=-0.005230 max=0.004911 Jy/beam
! Clean residual mean=0.000185 rms=0.001303 Jy/beam
! Combined flux in latest and established models = 0.593442 Jy
selfcal
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 41 components and 0.593442 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.189995Jy  sigma=0.001182
! Fit after  self-cal, rms=0.190006Jy  sigma=0.001182
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 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 = -0.000116965 Jy
! Component: 100  -  total flux cleaned = -0.000174543 Jy
! Component: 150  -  total flux cleaned = -0.000223941 Jy
! Component: 200  -  total flux cleaned = -0.000223565 Jy
! Total flux subtracted in 200 components = -0.000223565 Jy
! Clean residual min=-0.005171 max=0.004922 Jy/beam
! Clean residual mean=0.000183 rms=0.001301 Jy/beam
! Combined flux in latest and established models = 0.593219 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 42 components and 0.593219 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.189990Jy  sigma=0.001182
! Fit after  self-cal, rms=0.189989Jy  sigma=0.001182
! Inverting map 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 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=0.189989Jy  sigma=0.001182
! Fit after  self-cal, rms=0.189711Jy  sigma=0.001174
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
! Estimated beam: bmin=0.7619 mas, bmaj=2.257 mas, bpa=-2.472 degrees
! Estimated noise=973.588 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00203525 Jy
! Component: 100  -  total flux cleaned = -0.0021304 Jy
! Component: 150  -  total flux cleaned = -0.0022328 Jy
! Component: 200  -  total flux cleaned = -0.00230854 Jy
! Total flux subtracted in 200 components = -0.00230854 Jy
! Clean residual min=-0.004096 max=0.004246 Jy/beam
! Clean residual mean=0.000020 rms=0.001011 Jy/beam
! Combined flux in latest and established models = 0.59091 Jy
selfcal
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 43 components and 0.59091 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.189659Jy  sigma=0.001174
! Fit after  self-cal, rms=0.189676Jy  sigma=0.001174
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 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 = -0.00016759 Jy
! Component: 100  -  total flux cleaned = -0.000239845 Jy
! Component: 150  -  total flux cleaned = -0.000254499 Jy
! Component: 200  -  total flux cleaned = -0.000254772 Jy
! Total flux subtracted in 200 components = -0.000254772 Jy
! Clean residual min=-0.004062 max=0.004225 Jy/beam
! Clean residual mean=0.000020 rms=0.001010 Jy/beam
! Combined flux in latest and established models = 0.590655 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 46 components and 0.590655 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.189668Jy  sigma=0.001174
! Fit after  self-cal, rms=0.189666Jy  sigma=0.001174
! Inverting map 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 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=0.189666Jy  sigma=0.001174
! Fit after  self-cal, rms=0.189894Jy  sigma=0.001173
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
! Estimated beam: bmin=2.616 mas, bmaj=8.798 mas, bpa=-3.888 degrees
! Estimated noise=1265.06 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00155944 Jy
! Component: 100  -  total flux cleaned = -0.001946 Jy
! Component: 150  -  total flux cleaned = -0.00195525 Jy
! Component: 200  -  total flux cleaned = -0.00196385 Jy
! Total flux subtracted in 200 components = -0.00196385 Jy
! Clean residual min=-0.003785 max=0.004157 Jy/beam
! Clean residual mean=0.000023 rms=0.001271 Jy/beam
! Combined flux in latest and established models = 0.588691 Jy
selfcal
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 46 components and 0.588691 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.189875Jy  sigma=0.001173
! Fit after  self-cal, rms=0.189880Jy  sigma=0.001173
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 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 = -4.32005e-05 Jy
! Component: 100  -  total flux cleaned = -4.34822e-05 Jy
! Component: 150  -  total flux cleaned = -4.376e-05 Jy
! Component: 200  -  total flux cleaned = -4.40074e-05 Jy
! Total flux subtracted in 200 components = -4.40074e-05 Jy
! Clean residual min=-0.003786 max=0.004178 Jy/beam
! Clean residual mean=0.000023 rms=0.001271 Jy/beam
! Combined flux in latest and established models = 0.588647 Jy
! Performing phase self-cal
! Adding 3 model components to the UV plane model.
! The established model now contains 46 components and 0.588647 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.189877Jy  sigma=0.001173
! Fit after  self-cal, rms=0.189876Jy  sigma=0.001173
! Inverting map 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 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 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
! Estimated beam: bmin=0.7634 mas, bmaj=2.26 mas, bpa=-2.391 degrees
! Estimated noise=973.255 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7634 x 2.26 at -2.391 degrees (North through East)
! Clean map  min=-0.003847  max=0.52026 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
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.189876Jy  sigma=0.001173
! Fit after  self-cal, rms=1.520714Jy  sigma=0.001062
! Inverting map and beam 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
! Estimated beam: bmin=0.7634 mas, bmaj=2.262 mas, bpa=-2.359 degrees
! Estimated noise=972.107 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000864154 Jy
! Component: 100  -  total flux cleaned = -0.000946902 Jy
! Component: 150  -  total flux cleaned = -0.00102625 Jy
! Component: 200  -  total flux cleaned = -0.00107146 Jy
! Total flux subtracted in 200 components = -0.00107146 Jy
! Clean residual min=-0.003857 max=0.004151 Jy/beam
! Clean residual mean=0.000026 rms=0.000995 Jy/beam
! Combined flux in latest and established models = 0.587576 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 48 components and 0.587576 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=1.520708Jy  sigma=0.001062
! Fit after  self-cal, rms=1.520720Jy  sigma=0.001062
! Inverting map 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -3.97177e-05 Jy
! Component: 100  -  total flux cleaned = -7.57185e-05 Jy
! Component: 150  -  total flux cleaned = -0.000112683 Jy
! Component: 200  -  total flux cleaned = -0.000120379 Jy
! Total flux subtracted in 200 components = -0.000120379 Jy
! Clean residual min=-0.003863 max=0.004149 Jy/beam
! Clean residual mean=0.000026 rms=0.000995 Jy/beam
! Combined flux in latest and established models = 0.587455 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 50 components and 0.587455 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=1.520715Jy  sigma=0.001062
! Fit after  self-cal, rms=1.520720Jy  sigma=0.001062
! Inverting map 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=1.520720Jy  sigma=0.001062
! Fit after  self-cal, rms=1.977944Jy  sigma=0.001062
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 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
! Estimated beam: bmin=0.602 mas, bmaj=1.92 mas, bpa=0.04159 degrees
! Estimated noise=1710.8 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.395746 Jy
! Component: 100  -  total flux cleaned = 0.492286 Jy
! Component: 150  -  total flux cleaned = 0.532408 Jy
! Component: 200  -  total flux cleaned = 0.55431 Jy
! Total flux subtracted in 200 components = 0.55431 Jy
! Clean residual min=-0.008143 max=0.011144 Jy/beam
! Clean residual mean=0.000038 rms=0.002169 Jy/beam
! Combined flux in latest and established models = 0.55431 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 19 model components to the UV plane model.
! The established model now contains 19 components and 0.55431 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
! Estimated beam: bmin=0.7641 mas, bmaj=2.264 mas, bpa=-2.318 degrees
! Estimated noise=972.13 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 = 0.0173617 Jy
! Component: 100  -  total flux cleaned = 0.0250804 Jy
! Component: 150  -  total flux cleaned = 0.028696 Jy
! Component: 200  -  total flux cleaned = 0.0304043 Jy
! Total flux subtracted in 200 components = 0.0304043 Jy
! Clean residual min=-0.004002 max=0.003960 Jy/beam
! Clean residual mean=0.000024 rms=0.000997 Jy/beam
! Combined flux in latest and established models = 0.584714 Jy
! Adding 18 model components to the UV plane model.
! The established model now contains 32 components and 0.584714 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 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 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
! Estimated beam: bmin=2.619 mas, bmaj=8.813 mas, bpa=-3.876 degrees
! Estimated noise=1260.95 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00085892 Jy
! Component: 100  -  total flux cleaned = 0.00103569 Jy
! Component: 150  -  total flux cleaned = 0.00104287 Jy
! Component: 200  -  total flux cleaned = 0.00105022 Jy
! Total flux subtracted in 200 components = 0.00105022 Jy
! Clean residual min=-0.003881 max=0.003731 Jy/beam
! Clean residual mean=0.000049 rms=0.001273 Jy/beam
! Combined flux in latest and established models = 0.585764 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 = 6.63995e-06 Jy
! Component: 100  -  total flux cleaned = 7.15184e-06 Jy
! Component: 150  -  total flux cleaned = 1.36589e-05 Jy
! Component: 200  -  total flux cleaned = 2.04518e-05 Jy
! Total flux subtracted in 200 components = 2.04518e-05 Jy
! Clean residual min=-0.003878 max=0.003727 Jy/beam
! Clean residual mean=0.000049 rms=0.001273 Jy/beam
! Combined flux in latest and established models = 0.585784 Jy
! Adding 5 model components to the UV plane model.
! The established model now contains 34 components and 0.585784 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
! Estimated beam: bmin=0.7641 mas, bmaj=2.264 mas, bpa=-2.318 degrees
! Estimated noise=972.13 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00062481 Jy
! Component: 100  -  total flux cleaned = -0.000528242 Jy
! Component: 150  -  total flux cleaned = -0.000443051 Jy
! Component: 200  -  total flux cleaned = -0.000368372 Jy
! Total flux subtracted in 200 components = -0.000368372 Jy
! Clean residual min=-0.004008 max=0.004020 Jy/beam
! Clean residual mean=0.000023 rms=0.000992 Jy/beam
! Combined flux in latest and established models = 0.585416 Jy
selfcal
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 38 components and 0.585416 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=1.977914Jy  sigma=0.001062
! Fit after  self-cal, rms=1.977934Jy  sigma=0.001062
wmodel J2331-3811_X_2009_04_21_pus_map.mod
! Writing 38 model components to file: J2331-3811_X_2009_04_21_pus_map.mod
wobs J2331-3811_X_2009_04_21_pus_uvs.fits
! Writing UV FITS file: J2331-3811_X_2009_04_21_pus_uvs.fits
wwins J2331-3811_X_2009_04_21_pus_map.win
! wwins: Wrote 1 windows to J2331-3811_X_2009_04_21_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 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000442218 Jy
! Component: 100  -  total flux cleaned = -0.000650147 Jy
! Component: 150  -  total flux cleaned = -0.000404812 Jy
! Component: 200  -  total flux cleaned = -5.08384e-05 Jy
! Component: 250  -  total flux cleaned = 6.5231e-06 Jy
! Component: 300  -  total flux cleaned = -0.000264058 Jy
! Component: 350  -  total flux cleaned = -0.000315681 Jy
! Component: 400  -  total flux cleaned = -0.000417289 Jy
! Component: 450  -  total flux cleaned = -0.000467529 Jy
! Component: 500  -  total flux cleaned = -0.000615024 Jy
! Component: 550  -  total flux cleaned = -0.000710655 Jy
! Component: 600  -  total flux cleaned = -0.00085061 Jy
! Component: 650  -  total flux cleaned = -0.000850459 Jy
! Component: 700  -  total flux cleaned = -0.000896131 Jy
! Component: 750  -  total flux cleaned = -0.00094053 Jy
! Component: 800  -  total flux cleaned = -0.000984439 Jy
! Component: 850  -  total flux cleaned = -0.00107009 Jy
! Component: 900  -  total flux cleaned = -0.00115388 Jy
! Component: 950  -  total flux cleaned = -0.00123702 Jy
! Component: 1000  -  total flux cleaned = -0.00131866 Jy
! Component: 1050  -  total flux cleaned = -0.00135854 Jy
! Component: 1100  -  total flux cleaned = -0.00139831 Jy
! Component: 1150  -  total flux cleaned = -0.00151643 Jy
! Component: 1200  -  total flux cleaned = -0.00159433 Jy
! Component: 1250  -  total flux cleaned = -0.00178662 Jy
! Component: 1300  -  total flux cleaned = -0.00186234 Jy
! Component: 1350  -  total flux cleaned = -0.00189965 Jy
! Component: 1400  -  total flux cleaned = -0.00193669 Jy
! Component: 1450  -  total flux cleaned = -0.00201034 Jy
! Component: 1500  -  total flux cleaned = -0.00208297 Jy
! Component: 1550  -  total flux cleaned = -0.00208266 Jy
! Component: 1600  -  total flux cleaned = -0.00211838 Jy
! Component: 1650  -  total flux cleaned = -0.00222412 Jy
! Component: 1700  -  total flux cleaned = -0.00222397 Jy
! Component: 1750  -  total flux cleaned = -0.00229301 Jy
! Component: 1800  -  total flux cleaned = -0.00232736 Jy
! Component: 1850  -  total flux cleaned = -0.00242928 Jy
! Component: 1900  -  total flux cleaned = -0.00242918 Jy
! Component: 1950  -  total flux cleaned = -0.00249613 Jy
! Component: 2000  -  total flux cleaned = -0.00256197 Jy
! Total flux subtracted in 2048 components = -0.00262726 Jy
! Clean residual min=-0.001702 max=0.001655 Jy/beam
! Clean residual mean=0.000034 rms=0.000621 Jy/beam
! Combined flux in latest and established models = 0.582789 Jy
keep
! Adding 126 model components to the UV plane model.
! The established model now contains 164 components and 0.582789 Jy
![Exited script file: muppet]
wmap "J2331-3811_X_2009_04_21_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7641 x 2.264 at -2.318 degrees (North through East)
! Clean map  min=-0.0035159  max=0.52228 Jy/beam
! Writing clean map to FITS file: J2331-3811_X_2009_04_21_pus_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.522282 
invert
! Inverting map 
! Your choice of large map pixels excluded 1.09% of the data.
!  The x-axis pixel size should ideally be below 0.1933 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000619702 
device "J2331-3811_X_2009_04_21_pus\_map.eps/VPS"
! Attempting to open device: 'J2331-3811_X_2009_04_21_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.355959 0.355959 0.711917 1.42383 2.84767 5.69534 11.3907 22.7814 45.5627 91.1254
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0018 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.522 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7641 x 2.264 at -2.318 degrees (North through East)
! Clean map  min=-0.0035159  max=0.52228 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J2331-3811_X_2009_04_21_pus\_map.gif/vgif"
! Attempting to open device: 'J2331-3811_X_2009_04_21_pus_map.gif/vgif'
mapplot cln