! Started logfile: J0423-0120_X_2010_10_13_pus_uvs.log on Mon Feb 28 17:14:51 2011
obs J0423-0120_X_2010_10_13_pus_uva.fits
! Reading UV FITS file: J0423-0120_X_2010_10_13_pus_uva.fits
! AN table 1: 64 integrations on 105 of 105 possible baselines.
! AN table 2: 40 integrations on 105 of 105 possible baselines.
! AN table 3: 68 integrations on 105 of 105 possible baselines.
! AN table 4: 31 integrations on 105 of 105 possible baselines.
! Apparent sampling: 0.120525 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J0423-0120
! 
! 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 5978 lines of history.
! 
! Reading 10276 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 J0423-0120_X_2010_10_13_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 767 telescope corrections were flagged in sub-array 1.
!  A total of 318 telescope corrections were flagged in sub-array 2.
!  A total of 761 telescope corrections were flagged in sub-array 3.
!  A total of 300 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 2.
!  A total of 767 telescope corrections were flagged in sub-array 1.
!  A total of 318 telescope corrections were flagged in sub-array 2.
!  A total of 761 telescope corrections were flagged in sub-array 3.
!  A total of 300 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 3.
!  A total of 767 telescope corrections were flagged in sub-array 1.
!  A total of 318 telescope corrections were flagged in sub-array 2.
!  A total of 761 telescope corrections were flagged in sub-array 3.
!  A total of 300 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 4.
!  A total of 767 telescope corrections were flagged in sub-array 1.
!  A total of 318 telescope corrections were flagged in sub-array 2.
!  A total of 761 telescope corrections were flagged in sub-array 3.
!  A total of 300 telescope corrections were flagged in sub-array 4.
! 
! Fit before self-cal, rms=3.479492Jy  sigma=0.041682
! Fit after  self-cal, rms=3.475037Jy  sigma=0.041584
! 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 10.7% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! Estimated beam: bmin=0.5804 mas, bmaj=1.095 mas, bpa=-2.839 degrees
! Estimated noise=1021.55 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 = 3.23497 Jy
! Component: 100  -  total flux cleaned = 4.23889 Jy
! Total flux subtracted in 100 components = 4.23889 Jy
! Clean residual min=-0.133430 max=0.434626 Jy/beam
! Clean residual mean=0.003494 rms=0.048401 Jy/beam
! Combined flux in latest and established models = 4.23889 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 10 components and 4.23889 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.874923Jy  sigma=0.010268
! Fit after  self-cal, rms=0.874367Jy  sigma=0.010263
! Inverting map 
! Your choice of large map pixels excluded 10.7% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.463531 Jy
! Component: 100  -  total flux cleaned = 0.689568 Jy
! Total flux subtracted in 100 components = 0.689568 Jy
! Clean residual min=-0.085268 max=0.124831 Jy/beam
! Clean residual mean=-0.000257 rms=0.023331 Jy/beam
! Combined flux in latest and established models = 4.92846 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 18 components and 4.92846 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.533355Jy  sigma=0.005628
! Fit after  self-cal, rms=0.532803Jy  sigma=0.005624
! Inverting map 
! Your choice of large map pixels excluded 10.7% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 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 10.7% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! Estimated beam: bmin=0.8226 mas, bmaj=1.59 mas, bpa=-8.788 degrees
! Estimated noise=677.731 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 = 0.177876 Jy
! Component: 100  -  total flux cleaned = 0.256331 Jy
! Component: 150  -  total flux cleaned = 0.29302 Jy
! Component: 200  -  total flux cleaned = 0.308772 Jy
! Total flux subtracted in 200 components = 0.308772 Jy
! Clean residual min=-0.068339 max=0.122736 Jy/beam
! Clean residual mean=-0.013200 rms=0.021154 Jy/beam
! Combined flux in latest and established models = 5.23723 Jy
! Performing phase self-cal
! Adding 21 model components to the UV plane model.
! The established model now contains 30 components and 5.23723 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.503075Jy  sigma=0.004964
! Fit after  self-cal, rms=0.502225Jy  sigma=0.004961
! Inverting map 
! Your choice of large map pixels excluded 10.7% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! Added new window around map position (-1.4, -1.6).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.105257 Jy
! Component: 100  -  total flux cleaned = 0.11913 Jy
! Component: 150  -  total flux cleaned = 0.119097 Jy
! Component: 200  -  total flux cleaned = 0.117851 Jy
! Total flux subtracted in 200 components = 0.117851 Jy
! Clean residual min=-0.065744 max=0.070850 Jy/beam
! Clean residual mean=-0.018433 rms=0.015466 Jy/beam
! Combined flux in latest and established models = 5.35508 Jy
! Performing phase self-cal
! Adding 21 model components to the UV plane model.
! The established model now contains 51 components and 5.35508 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.473297Jy  sigma=0.004746
! Fit after  self-cal, rms=0.470202Jy  sigma=0.004712
! Inverting map 
! Your choice of large map pixels excluded 10.7% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 69 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    HH        1.04     HN        1.16     
!   KB        1.00*    KK        1.00*    KP        1.00*    LA        0.98     
!   MK        1.00*    NL        0.99     NY        1.03     OV        1.00*    
!   PT        0.97     SC        1.01     TS        1.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.01     FD        0.84     HH        1.39     HN        1.07     
!   KB        1.00*    KK        1.00*    KP        0.99     LA        1.01     
!   MK        1.00*    NL        0.99     NY        1.00*    OV        1.00     
!   PT        0.98     SC        0.96     TS        1.00*    
! 
!  A total of 111 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.95     FD        0.85     HH        0.92     HN        1.09     
!   KB        1.21     KK        0.99     KP        0.99     LA        0.98     
!   MK        0.99     NL        0.97     NY        1.10     OV        0.97     
!   PT        0.95     SC        1.00*    TS        1.18     
! 
!  A total of 12 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        0.97     FD        0.84     HH        1.00*    HN        1.00*    
!   KB        1.00     KK        0.95     KP        0.99     LA        1.02     
!   MK        1.01     NL        1.00*    NY        1.00*    OV        0.97     
!   PT        0.98     SC        1.00*    TS        1.00*    
! 
! 
! Correcting IF 2.
!  A total of 69 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    HH        1.07     HN        1.16     
!   KB        1.00*    KK        1.00*    KP        1.00*    LA        0.96     
!   MK        1.00*    NL        1.02     NY        1.05     OV        1.00*    
!   PT        0.99     SC        1.02     TS        1.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.06     FD        0.98     HH        1.43     HN        1.09     
!   KB        1.00*    KK        1.00*    KP        0.99     LA        0.98     
!   MK        1.00*    NL        1.03     NY        1.00*    OV        1.02     
!   PT        1.00     SC        0.98     TS        1.00*    
! 
!  A total of 111 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00     FD        1.00     HH        0.91     HN        1.11     
!   KB        1.25     KK        1.03     KP        0.98     LA        0.94     
!   MK        0.94     NL        1.01     NY        1.08     OV        0.99     
!   PT        0.97     SC        1.00*    TS        1.21     
! 
!  A total of 12 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.01     FD        0.99     HH        1.00*    HN        1.00*    
!   KB        1.02     KK        0.99     KP        0.98     LA        0.98     
!   MK        0.96     NL        1.00*    NY        1.00*    OV        1.00     
!   PT        1.00     SC        1.00*    TS        1.00*    
! 
! 
! Correcting IF 3.
!  A total of 69 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    HH        1.09     HN        1.19     
!   KB        1.00*    KK        1.00*    KP        1.00*    LA        0.94     
!   MK        1.00*    NL        0.98     NY        1.11     OV        1.00*    
!   PT        1.04     SC        1.04     TS        1.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.04     FD        0.99     HH        1.72     HN        1.14     
!   KB        1.00*    KK        1.00*    KP        0.99     LA        0.96     
!   MK        1.00*    NL        0.98     NY        1.00*    OV        1.01     
!   PT        1.04     SC        0.99     TS        1.00*    
! 
!  A total of 111 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.98     FD        1.00     HH        0.87     HN        1.13     
!   KB        1.20     KK        1.00     KP        0.99     LA        0.94     
!   MK        0.99     NL        0.96     NY        1.16     OV        0.98     
!   PT        1.01     SC        1.00*    TS        1.20     
! 
!  A total of 12 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        0.99     FD        0.99     HH        1.00*    HN        1.00*    
!   KB        1.01     KK        0.94     KP        1.00     LA        0.97     
!   MK        1.02     NL        1.00*    NY        1.00*    OV        0.99     
!   PT        1.04     SC        1.00*    TS        1.00*    
! 
! 
! Correcting IF 4.
!  A total of 69 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    HH        1.08     HN        1.17     
!   KB        1.00*    KK        1.00*    KP        1.00*    LA        1.02     
!   MK        1.00*    NL        1.01     NY        1.07     OV        1.00*    
!   PT        0.99     SC        1.03     TS        1.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.09     FD        1.01     HH        1.85     HN        1.09     
!   KB        1.00*    KK        1.00*    KP        0.99     LA        1.04     
!   MK        1.00*    NL        1.00     NY        1.00*    OV        1.06     
!   PT        1.00     SC        1.00     TS        1.00*    
! 
!  A total of 111 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.03     FD        1.00     HH        0.87     HN        1.10     
!   KB        1.21     KK        1.01     KP        0.99     LA        1.00     
!   MK        0.98     NL        0.99     NY        1.11     OV        1.02     
!   PT        0.96     SC        1.00*    TS        1.07     
! 
!  A total of 12 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.04     FD        1.01     HH        1.00*    HN        1.00*    
!   KB        1.02     KK        0.98     KP        0.99     LA        1.04     
!   MK        1.00     NL        1.00*    NY        1.00*    OV        1.03     
!   PT        0.99     SC        1.00*    TS        1.00*    
! 
! 
! Fit before self-cal, rms=0.470202Jy  sigma=0.004712
! Fit after  self-cal, rms=0.304974Jy  sigma=0.002248
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! Estimated beam: bmin=0.8799 mas, bmaj=1.825 mas, bpa=-7.585 degrees
! Estimated noise=704.137 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 = 0.0146347 Jy
! Component: 100  -  total flux cleaned = 0.0128216 Jy
! Component: 150  -  total flux cleaned = 0.0127938 Jy
! Component: 200  -  total flux cleaned = 0.0121026 Jy
! Total flux subtracted in 200 components = 0.0121026 Jy
! Clean residual min=-0.030620 max=0.033088 Jy/beam
! Clean residual mean=-0.000812 rms=0.006966 Jy/beam
! Combined flux in latest and established models = 5.36718 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 61 components and 5.36718 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.297614Jy  sigma=0.002181
! Fit after  self-cal, rms=0.297408Jy  sigma=0.002177
! Inverting map 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 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=0.297408Jy  sigma=0.002177
! Fit after  self-cal, rms=0.279792Jy  sigma=0.001966
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! Estimated beam: bmin=0.8804 mas, bmaj=1.825 mas, bpa=-7.658 degrees
! Estimated noise=703.066 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.002066 Jy
! Component: 100  -  total flux cleaned = 0.00207041 Jy
! Component: 150  -  total flux cleaned = 0.00324199 Jy
! Component: 200  -  total flux cleaned = 0.0043055 Jy
! Total flux subtracted in 200 components = 0.0043055 Jy
! Clean residual min=-0.022030 max=0.022475 Jy/beam
! Clean residual mean=-0.000156 rms=0.005319 Jy/beam
! Combined flux in latest and established models = 5.37149 Jy
selfcal
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 67 components and 5.37149 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.275740Jy  sigma=0.001931
! Fit after  self-cal, rms=0.275515Jy  sigma=0.001928
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 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 = 0.00171581 Jy
! Component: 100  -  total flux cleaned = 0.00224491 Jy
! Component: 150  -  total flux cleaned = 0.00272402 Jy
! Component: 200  -  total flux cleaned = 0.00270462 Jy
! Total flux subtracted in 200 components = 0.00270462 Jy
! Clean residual min=-0.022612 max=0.021161 Jy/beam
! Clean residual mean=-0.000210 rms=0.005180 Jy/beam
! Combined flux in latest and established models = 5.37419 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 68 components and 5.37419 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.273079Jy  sigma=0.001914
! Fit after  self-cal, rms=0.273022Jy  sigma=0.001913
! Inverting map 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 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=0.273022Jy  sigma=0.001913
! Fit after  self-cal, rms=0.246978Jy  sigma=0.001698
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! Estimated beam: bmin=0.8817 mas, bmaj=1.829 mas, bpa=-7.544 degrees
! Estimated noise=703.538 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00602007 Jy
! Component: 100  -  total flux cleaned = 0.0065633 Jy
! Component: 150  -  total flux cleaned = 0.00656537 Jy
! Component: 200  -  total flux cleaned = 0.00657803 Jy
! Total flux subtracted in 200 components = 0.00657803 Jy
! Clean residual min=-0.016694 max=0.017549 Jy/beam
! Clean residual mean=-0.000040 rms=0.003408 Jy/beam
! Combined flux in latest and established models = 5.38077 Jy
selfcal
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 74 components and 5.38077 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.244561Jy  sigma=0.001676
! Fit after  self-cal, rms=0.244562Jy  sigma=0.001675
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 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)
! Added new window around map position (0.6, -5.2).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0128951 Jy
! Component: 100  -  total flux cleaned = 0.0133423 Jy
! Component: 150  -  total flux cleaned = 0.0137478 Jy
! Component: 200  -  total flux cleaned = 0.0133645 Jy
! Total flux subtracted in 200 components = 0.0133645 Jy
! Clean residual min=-0.015282 max=0.009902 Jy/beam
! Clean residual mean=-0.000327 rms=0.002787 Jy/beam
! Combined flux in latest and established models = 5.39413 Jy
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 82 components and 5.39413 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.242585Jy  sigma=0.001654
! Fit after  self-cal, rms=0.242408Jy  sigma=0.001652
! Inverting map 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 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=0.242408Jy  sigma=0.001652
! Fit after  self-cal, rms=0.246756Jy  sigma=0.001647
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! Estimated beam: bmin=2.444 mas, bmaj=3.554 mas, bpa=-16.14 degrees
! Estimated noise=820.873 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00386029 Jy
! Component: 100  -  total flux cleaned = 0.00537341 Jy
! Component: 150  -  total flux cleaned = 0.00580931 Jy
! Component: 200  -  total flux cleaned = 0.00618236 Jy
! Total flux subtracted in 200 components = 0.00618236 Jy
! Clean residual min=-0.008535 max=0.006293 Jy/beam
! Clean residual mean=-0.000479 rms=0.002268 Jy/beam
! Combined flux in latest and established models = 5.40031 Jy
selfcal
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 93 components and 5.40031 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.246484Jy  sigma=0.001639
! Fit after  self-cal, rms=0.246321Jy  sigma=0.001638
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 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 = 0.000947152 Jy
! Component: 100  -  total flux cleaned = 0.00167127 Jy
! Component: 150  -  total flux cleaned = 0.00205351 Jy
! Component: 200  -  total flux cleaned = 0.00213158 Jy
! Total flux subtracted in 200 components = 0.00213158 Jy
! Clean residual min=-0.008434 max=0.005737 Jy/beam
! Clean residual mean=-0.000570 rms=0.002195 Jy/beam
! Combined flux in latest and established models = 5.40245 Jy
! Performing phase self-cal
! Adding 20 model components to the UV plane model.
! The established model now contains 105 components and 5.40245 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.246034Jy  sigma=0.001636
! Fit after  self-cal, rms=0.245916Jy  sigma=0.001635
! Inverting map 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 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 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! Estimated beam: bmin=0.8837 mas, bmaj=1.835 mas, bpa=-7.594 degrees
! Estimated noise=704.158 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8837 x 1.835 at -7.594 degrees (North through East)
! Clean map  min=-0.011122  max=4.5483 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=0.245916Jy  sigma=0.001635
! Fit after  self-cal, rms=0.221940Jy  sigma=0.001357
! Inverting map and beam 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! Estimated beam: bmin=0.8841 mas, bmaj=1.834 mas, bpa=-7.57 degrees
! Estimated noise=703.599 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00157589 Jy
! Component: 100  -  total flux cleaned = -0.000783215 Jy
! Component: 150  -  total flux cleaned = -0.00039937 Jy
! Component: 200  -  total flux cleaned = -4.22718e-05 Jy
! Total flux subtracted in 200 components = -4.22718e-05 Jy
! Clean residual min=-0.012586 max=0.007332 Jy/beam
! Clean residual mean=-0.000206 rms=0.002317 Jy/beam
! Combined flux in latest and established models = 5.4024 Jy
! Performing phase self-cal
! Adding 20 model components to the UV plane model.
! The established model now contains 109 components and 5.4024 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.220015Jy  sigma=0.001349
! Fit after  self-cal, rms=0.219994Jy  sigma=0.001348
! Inverting map 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00027693 Jy
! Component: 100  -  total flux cleaned = 0.000615579 Jy
! Component: 150  -  total flux cleaned = 0.000616015 Jy
! Component: 200  -  total flux cleaned = 0.000603423 Jy
! Total flux subtracted in 200 components = 0.000603423 Jy
! Clean residual min=-0.012039 max=0.007000 Jy/beam
! Clean residual mean=-0.000217 rms=0.002233 Jy/beam
! Combined flux in latest and established models = 5.40301 Jy
! Performing phase self-cal
! Adding 24 model components to the UV plane model.
! The established model now contains 115 components and 5.40301 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.218482Jy  sigma=0.001342
! Fit after  self-cal, rms=0.218426Jy  sigma=0.001341
! Inverting map 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.218426Jy  sigma=0.001341
! Fit after  self-cal, rms=0.220880Jy  sigma=0.001337
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 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! Estimated beam: bmin=0.6138 mas, bmaj=1.247 mas, bpa=-4.459 degrees
! Estimated noise=1058.73 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 3.33806 Jy
! Component: 100  -  total flux cleaned = 4.2921 Jy
! Component: 150  -  total flux cleaned = 4.71562 Jy
! Component: 200  -  total flux cleaned = 4.91917 Jy
! Total flux subtracted in 200 components = 4.91917 Jy
! Clean residual min=-0.044536 max=0.097997 Jy/beam
! Clean residual mean=0.001946 rms=0.014911 Jy/beam
! Combined flux in latest and established models = 4.91917 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 4.91917 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! Estimated beam: bmin=0.8858 mas, bmaj=1.839 mas, bpa=-7.609 degrees
! Estimated noise=704.111 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 = 0.190906 Jy
! Component: 100  -  total flux cleaned = 0.297369 Jy
! Component: 150  -  total flux cleaned = 0.362134 Jy
! Component: 200  -  total flux cleaned = 0.403783 Jy
! Total flux subtracted in 200 components = 0.403783 Jy
! Clean residual min=-0.012434 max=0.028211 Jy/beam
! Clean residual mean=0.001280 rms=0.005149 Jy/beam
! Combined flux in latest and established models = 5.32295 Jy
! Adding 36 model components to the UV plane model.
! The established model now contains 42 components and 5.32295 Jy
! Inverting map 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! Added new window around map position (0.2, -1.6).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0293454 Jy
! Component: 100  -  total flux cleaned = 0.0486299 Jy
! Component: 150  -  total flux cleaned = 0.0620839 Jy
! Component: 200  -  total flux cleaned = 0.0698939 Jy
! Total flux subtracted in 200 components = 0.0698939 Jy
! Clean residual min=-0.008384 max=0.007798 Jy/beam
! Clean residual mean=0.000025 rms=0.002175 Jy/beam
! Combined flux in latest and established models = 5.39285 Jy
! Adding 26 model components to the UV plane model.
! The established model now contains 62 components and 5.39285 Jy
! Inverting map 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 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 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! Estimated beam: bmin=2.445 mas, bmaj=3.552 mas, bpa=-16.13 degrees
! Estimated noise=819.86 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00481437 Jy
! Component: 100  -  total flux cleaned = 0.00678874 Jy
! Component: 150  -  total flux cleaned = 0.0082942 Jy
! Component: 200  -  total flux cleaned = 0.00923966 Jy
! Total flux subtracted in 200 components = 0.00923966 Jy
! Clean residual min=-0.005478 max=0.004983 Jy/beam
! Clean residual mean=-0.000300 rms=0.001679 Jy/beam
! Combined flux in latest and established models = 5.40209 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 = 0.000294119 Jy
! Component: 100  -  total flux cleaned = 0.000631151 Jy
! Component: 150  -  total flux cleaned = 0.000777995 Jy
! Component: 200  -  total flux cleaned = 0.000840787 Jy
! Total flux subtracted in 200 components = 0.000840787 Jy
! Clean residual min=-0.005331 max=0.004620 Jy/beam
! Clean residual mean=-0.000338 rms=0.001605 Jy/beam
! Combined flux in latest and established models = 5.40293 Jy
! Adding 21 model components to the UV plane model.
! The established model now contains 80 components and 5.40293 Jy
! Inverting map 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! Estimated beam: bmin=0.8858 mas, bmaj=1.839 mas, bpa=-7.609 degrees
! Estimated noise=704.111 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000256928 Jy
! Component: 100  -  total flux cleaned = -1.3084e-05 Jy
! Component: 150  -  total flux cleaned = -0.000240084 Jy
! Component: 200  -  total flux cleaned = -0.000451356 Jy
! Total flux subtracted in 200 components = -0.000451356 Jy
! Clean residual min=-0.007857 max=0.006240 Jy/beam
! Clean residual mean=-0.000174 rms=0.001868 Jy/beam
! Combined flux in latest and established models = 5.40248 Jy
selfcal
! Performing phase self-cal
! Adding 23 model components to the UV plane model.
! The established model now contains 93 components and 5.40247 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.318457Jy  sigma=0.001786
! Fit after  self-cal, rms=0.317543Jy  sigma=0.001778
wmodel J0423-0120_X_2010_10_13_pus_map.mod
! Writing 93 model components to file: J0423-0120_X_2010_10_13_pus_map.mod
wobs J0423-0120_X_2010_10_13_pus_uvs.fits
! Writing UV FITS file: J0423-0120_X_2010_10_13_pus_uvs.fits
wwins J0423-0120_X_2010_10_13_pus_map.win
! wwins: Wrote 4 windows to J0423-0120_X_2010_10_13_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 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00356275 Jy
! Component: 100  -  total flux cleaned = -0.00670155 Jy
! Component: 150  -  total flux cleaned = -0.00786451 Jy
! Component: 200  -  total flux cleaned = -0.00874035 Jy
! Component: 250  -  total flux cleaned = -0.00905504 Jy
! Component: 300  -  total flux cleaned = -0.00925843 Jy
! Component: 350  -  total flux cleaned = -0.00965425 Jy
! Component: 400  -  total flux cleaned = -0.00994529 Jy
! Component: 450  -  total flux cleaned = -0.0102294 Jy
! Component: 500  -  total flux cleaned = -0.0103239 Jy
! Component: 550  -  total flux cleaned = -0.0106915 Jy
! Component: 600  -  total flux cleaned = -0.010872 Jy
! Component: 650  -  total flux cleaned = -0.0112287 Jy
! Component: 700  -  total flux cleaned = -0.0115814 Jy
! Component: 750  -  total flux cleaned = -0.011929 Jy
! Component: 800  -  total flux cleaned = -0.0122727 Jy
! Component: 850  -  total flux cleaned = -0.0126978 Jy
! Component: 900  -  total flux cleaned = -0.0129504 Jy
! Component: 950  -  total flux cleaned = -0.0133649 Jy
! Component: 1000  -  total flux cleaned = -0.0132827 Jy
! Total flux subtracted in 1024 components = -0.0135275 Jy
! Clean residual min=-0.004935 max=0.004066 Jy/beam
! Clean residual mean=-0.000018 rms=0.001497 Jy/beam
! Combined flux in latest and established models = 5.38895 Jy
keep
! Adding 61 model components to the UV plane model.
! The established model now contains 152 components and 5.38895 Jy
![Exited script file: muppet]
wmap "J0423-0120_X_2010_10_13_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8858 x 1.839 at -7.609 degrees (North through East)
! Clean map  min=-0.0058352  max=4.5625 Jy/beam
! Writing clean map to FITS file: J0423-0120_X_2010_10_13_pus_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 4.5625 
invert
! Inverting map 
! Your choice of large map pixels excluded 8.97% of the data.
!  The x-axis pixel size should ideally be below 0.1607 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1886 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.00149474 
device "J0423-0120_X_2010_10_13_pus\_map.eps/VPS"
! Attempting to open device: 'J0423-0120_X_2010_10_13_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.0982841 0.0982841 0.196568 0.393137 0.786273 1.57255 3.14509 6.29018 12.5804 25.1607 50.3215
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0044 
print "peak=",int(1000*peak_flux)/1000
! peak= 4.562 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8858 x 1.839 at -7.609 degrees (North through East)
! Clean map  min=-0.0058352  max=4.5625 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0423-0120_X_2010_10_13_pus\_map.gif/vgif"
! Attempting to open device: 'J0423-0120_X_2010_10_13_pus_map.gif/vgif'
mapplot cln