! Started logfile: 1320-407_X_2010_10_13_pus_uvs.log on Mon Feb 28 17:57:45 2011
obs 1320-407_X_2010_10_13_pus_uva.fits
! Reading UV FITS file: 1320-407_X_2010_10_13_pus_uva.fits
! AN table 1: 187 integrations on 105 of 105 possible baselines.
! AN table 2: Unused.
! AN table 3: Unused.
! AN table 4: Unused.
! AN table 5: Unused.
! Apparent sampling: 0.0771072 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: 1320-407
! 
! 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 5974 lines of history.
! 
! Reading 6056 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 1320-407_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 2331 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 2355 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 2331 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 2331 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=1.004083Jy  sigma=0.010942
! Fit after  self-cal, rms=0.934601Jy  sigma=0.010185
! 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 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 milli-arcsec
! Estimated beam: bmin=0.6682 mas, bmaj=2.038 mas, bpa=2.95 degrees
! Estimated noise=1687.13 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 = 0.055911 Jy
! Component: 100  -  total flux cleaned = 0.0676808 Jy
! Total flux subtracted in 100 components = 0.0676808 Jy
! Clean residual min=-0.006919 max=0.007642 Jy/beam
! Clean residual mean=0.000270 rms=0.002003 Jy/beam
! Combined flux in latest and established models = 0.0676808 Jy
! Performing phase self-cal
! Adding 3 model components to the UV plane model.
! The established model now contains 3 components and 0.0676808 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.111242Jy  sigma=0.001182
! Fit after  self-cal, rms=0.109682Jy  sigma=0.001166
! Inverting map 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 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 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 milli-arcsec
! Estimated beam: bmin=0.8927 mas, bmaj=2.911 mas, bpa=4.942 degrees
! Estimated noise=908.707 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 = 0.00502136 Jy
! Component: 100  -  total flux cleaned = 0.00551045 Jy
! Component: 150  -  total flux cleaned = 0.00558173 Jy
! Component: 200  -  total flux cleaned = 0.00569201 Jy
! Total flux subtracted in 200 components = 0.00569201 Jy
! Clean residual min=-0.004712 max=0.004318 Jy/beam
! Clean residual mean=0.000374 rms=0.001348 Jy/beam
! Combined flux in latest and established models = 0.0733729 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 11 components and 0.0733729 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.109415Jy  sigma=0.001163
! Fit after  self-cal, rms=0.109366Jy  sigma=0.001163
! Inverting map 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 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        0.83     HH        1.00*    HN        1.00*    
!   KB        1.00*    KK        1.00*    KP        1.02     LA        0.99     
!   MK        1.01     NL        1.09     NY        1.00*    OV        1.10     
!   PT        1.03     SC        1.02     TS        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.98     HH        1.00*    HN        1.00*    
!   KB        1.00*    KK        1.00*    KP        1.01     LA        0.93     
!   MK        0.91     NL        1.11     NY        1.00*    OV        1.17     
!   PT        1.05     SC        0.98     TS        1.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.91     HH        1.00*    HN        1.00*    
!   KB        1.00*    KK        1.00*    KP        0.97     LA        0.97     
!   MK        0.95     NL        1.13     NY        1.00*    OV        0.94     
!   PT        1.14     SC        0.95     TS        1.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.89     HH        1.00*    HN        1.00*    
!   KB        1.00*    KK        1.00*    KP        0.90     LA        1.05     
!   MK        0.99     NL        1.07     NY        1.00*    OV        1.17     
!   PT        1.04     SC        0.90     TS        1.00*    
! 
! 
! Fit before self-cal, rms=0.109366Jy  sigma=0.001163
! Fit after  self-cal, rms=0.107333Jy  sigma=0.001160
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 milli-arcsec
! Estimated beam: bmin=0.8816 mas, bmaj=2.876 mas, bpa=5.038 degrees
! Estimated noise=903.705 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 = 0.000442926 Jy
! Component: 100  -  total flux cleaned = 0.000444193 Jy
! Component: 150  -  total flux cleaned = 0.00048166 Jy
! Component: 200  -  total flux cleaned = 0.000483328 Jy
! Total flux subtracted in 200 components = 0.000483328 Jy
! Clean residual min=-0.003743 max=0.003264 Jy/beam
! Clean residual mean=0.000186 rms=0.001050 Jy/beam
! Combined flux in latest and established models = 0.0738562 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 17 components and 0.0738562 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.107307Jy  sigma=0.001160
! Fit after  self-cal, rms=0.107319Jy  sigma=0.001158
! Inverting map 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 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=0.107319Jy  sigma=0.001158
! Fit after  self-cal, rms=0.108056Jy  sigma=0.001157
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 milli-arcsec
! Estimated beam: bmin=0.876 mas, bmaj=2.873 mas, bpa=5.239 degrees
! Estimated noise=904.9 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000482848 Jy
! Component: 100  -  total flux cleaned = 0.000451867 Jy
! Component: 150  -  total flux cleaned = 0.000450166 Jy
! Component: 200  -  total flux cleaned = 0.000423141 Jy
! Total flux subtracted in 200 components = 0.000423141 Jy
! Clean residual min=-0.003778 max=0.003324 Jy/beam
! Clean residual mean=0.000164 rms=0.001103 Jy/beam
! Combined flux in latest and established models = 0.0742793 Jy
selfcal
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 18 components and 0.0742793 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.108037Jy  sigma=0.001157
! Fit after  self-cal, rms=0.108073Jy  sigma=0.001157
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 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 = -9.52164e-05 Jy
! Component: 100  -  total flux cleaned = -0.000121094 Jy
! Component: 150  -  total flux cleaned = -0.000165285 Jy
! Component: 200  -  total flux cleaned = -0.000183549 Jy
! Total flux subtracted in 200 components = -0.000183549 Jy
! Clean residual min=-0.003659 max=0.003242 Jy/beam
! Clean residual mean=0.000199 rms=0.001078 Jy/beam
! Combined flux in latest and established models = 0.0740958 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 22 components and 0.0740958 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.108062Jy  sigma=0.001157
! Fit after  self-cal, rms=0.108059Jy  sigma=0.001157
! Inverting map 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 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=0.108059Jy  sigma=0.001157
! Fit after  self-cal, rms=0.109271Jy  sigma=0.001155
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 milli-arcsec
! Estimated beam: bmin=0.8727 mas, bmaj=2.882 mas, bpa=5.415 degrees
! Estimated noise=906.549 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000138043 Jy
! Component: 100  -  total flux cleaned = 0.000119342 Jy
! Component: 150  -  total flux cleaned = 0.000117101 Jy
! Component: 200  -  total flux cleaned = 0.000102863 Jy
! Total flux subtracted in 200 components = 0.000102863 Jy
! Clean residual min=-0.003557 max=0.003234 Jy/beam
! Clean residual mean=0.000172 rms=0.001072 Jy/beam
! Combined flux in latest and established models = 0.0741986 Jy
selfcal
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 26 components and 0.0741986 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.109268Jy  sigma=0.001155
! Fit after  self-cal, rms=0.109395Jy  sigma=0.001155
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 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 = -4.46082e-05 Jy
! Component: 100  -  total flux cleaned = -7.62505e-05 Jy
! Component: 150  -  total flux cleaned = -0.000119307 Jy
! Component: 200  -  total flux cleaned = -0.000144923 Jy
! Total flux subtracted in 200 components = -0.000144923 Jy
! Clean residual min=-0.003463 max=0.003154 Jy/beam
! Clean residual mean=0.000182 rms=0.001050 Jy/beam
! Combined flux in latest and established models = 0.0740537 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 30 components and 0.0740537 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.109392Jy  sigma=0.001155
! Fit after  self-cal, rms=0.109393Jy  sigma=0.001155
! Inverting map 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 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=0.109393Jy  sigma=0.001155
! Fit after  self-cal, rms=0.110345Jy  sigma=0.001154
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 milli-arcsec
! Estimated beam: bmin=2.797 mas, bmaj=10.89 mas, bpa=-2.237 degrees
! Estimated noise=1150.02 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000362147 Jy
! Component: 100  -  total flux cleaned = 0.000361543 Jy
! Component: 150  -  total flux cleaned = 0.0003609 Jy
! Component: 200  -  total flux cleaned = 0.000360317 Jy
! Total flux subtracted in 200 components = 0.000360317 Jy
! Clean residual min=-0.003785 max=0.003348 Jy/beam
! Clean residual mean=0.000309 rms=0.001452 Jy/beam
! Combined flux in latest and established models = 0.074414 Jy
selfcal
! Performing phase self-cal
! Adding 4 model components to the UV plane model.
! The established model now contains 31 components and 0.074414 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.110348Jy  sigma=0.001154
! Fit after  self-cal, rms=0.110416Jy  sigma=0.001154
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 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 = -0.000133322 Jy
! Component: 100  -  total flux cleaned = -0.000134163 Jy
! Component: 150  -  total flux cleaned = -0.000134629 Jy
! Component: 200  -  total flux cleaned = -0.000134947 Jy
! Total flux subtracted in 200 components = -0.000134947 Jy
! Clean residual min=-0.003820 max=0.003318 Jy/beam
! Clean residual mean=0.000306 rms=0.001449 Jy/beam
! Combined flux in latest and established models = 0.0742791 Jy
! Performing phase self-cal
! Adding 5 model components to the UV plane model.
! The established model now contains 31 components and 0.0742791 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.110419Jy  sigma=0.001154
! Fit after  self-cal, rms=0.110418Jy  sigma=0.001154
! Inverting map 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 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 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 milli-arcsec
! Estimated beam: bmin=0.8716 mas, bmaj=2.888 mas, bpa=5.477 degrees
! Estimated noise=908.026 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8716 x 2.888 at 5.477 degrees (North through East)
! Clean map  min=-0.0032171  max=0.068062 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 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 milli-arcsec
! Estimated beam: bmin=0.6513 mas, bmaj=2.029 mas, bpa=3.907 degrees
! Estimated noise=1664.64 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0583493 Jy
! Component: 100  -  total flux cleaned = 0.0716441 Jy
! Component: 150  -  total flux cleaned = 0.0731803 Jy
! Component: 200  -  total flux cleaned = 0.0733032 Jy
! Total flux subtracted in 200 components = 0.0733032 Jy
! Clean residual min=-0.005993 max=0.005340 Jy/beam
! Clean residual mean=0.000141 rms=0.001827 Jy/beam
! Combined flux in latest and established models = 0.0733032 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 10 model components to the UV plane model.
! The established model now contains 10 components and 0.0733032 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 milli-arcsec
! Estimated beam: bmin=0.8716 mas, bmaj=2.888 mas, bpa=5.477 degrees
! Estimated noise=908.026 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 = 0.000221476 Jy
! Component: 100  -  total flux cleaned = 0.000222737 Jy
! Component: 150  -  total flux cleaned = 0.000224965 Jy
! Component: 200  -  total flux cleaned = 0.00031895 Jy
! Total flux subtracted in 200 components = 0.00031895 Jy
! Clean residual min=-0.003562 max=0.003163 Jy/beam
! Clean residual mean=0.000179 rms=0.001072 Jy/beam
! Combined flux in latest and established models = 0.0736222 Jy
! Adding 6 model components to the UV plane model.
! The established model now contains 14 components and 0.0736222 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 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 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 milli-arcsec
! Estimated beam: bmin=2.797 mas, bmaj=10.89 mas, bpa=-2.237 degrees
! Estimated noise=1150.02 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000430688 Jy
! Component: 100  -  total flux cleaned = 0.000431786 Jy
! Component: 150  -  total flux cleaned = 0.000432621 Jy
! Component: 200  -  total flux cleaned = 0.000433178 Jy
! Total flux subtracted in 200 components = 0.000433178 Jy
! Clean residual min=-0.003860 max=0.003336 Jy/beam
! Clean residual mean=0.000310 rms=0.001463 Jy/beam
! Combined flux in latest and established models = 0.0740553 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 = 3.80805e-07 Jy
! Component: 100  -  total flux cleaned = 6.88128e-07 Jy
! Component: 150  -  total flux cleaned = 9.19438e-07 Jy
! Component: 200  -  total flux cleaned = 1.37644e-06 Jy
! Total flux subtracted in 200 components = 1.37644e-06 Jy
! Clean residual min=-0.003847 max=0.003304 Jy/beam
! Clean residual mean=0.000310 rms=0.001449 Jy/beam
! Combined flux in latest and established models = 0.0740567 Jy
! Adding 8 model components to the UV plane model.
! The established model now contains 20 components and 0.0740567 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 milli-arcsec
! Estimated beam: bmin=0.8716 mas, bmaj=2.888 mas, bpa=5.477 degrees
! Estimated noise=908.026 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000254065 Jy
! Component: 100  -  total flux cleaned = -0.000198464 Jy
! Component: 150  -  total flux cleaned = -0.000198186 Jy
! Component: 200  -  total flux cleaned = -0.000176457 Jy
! Total flux subtracted in 200 components = -0.000176457 Jy
! Clean residual min=-0.003559 max=0.003141 Jy/beam
! Clean residual mean=0.000173 rms=0.001061 Jy/beam
! Combined flux in latest and established models = 0.0738802 Jy
selfcal
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 23 components and 0.0738802 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.110426Jy  sigma=0.001154
! Fit after  self-cal, rms=0.110427Jy  sigma=0.001154
wmodel 1320-407_X_2010_10_13_pus_map.mod
! Writing 23 model components to file: 1320-407_X_2010_10_13_pus_map.mod
wobs 1320-407_X_2010_10_13_pus_uvs.fits
! Writing UV FITS file: 1320-407_X_2010_10_13_pus_uvs.fits
wwins 1320-407_X_2010_10_13_pus_map.win
! wwins: Wrote 1 windows to 1320-407_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 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 milli-arcsec
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 8.30065e-05 Jy
! Component: 100  -  total flux cleaned = 0.000494098 Jy
! Component: 150  -  total flux cleaned = 0.0010306 Jy
! Component: 200  -  total flux cleaned = 0.00136265 Jy
! Component: 250  -  total flux cleaned = 0.00167279 Jy
! Component: 300  -  total flux cleaned = 0.00177977 Jy
! Component: 350  -  total flux cleaned = 0.0019166 Jy
! Component: 400  -  total flux cleaned = 0.00201443 Jy
! Component: 450  -  total flux cleaned = 0.00204585 Jy
! Component: 500  -  total flux cleaned = 0.00213563 Jy
! Component: 550  -  total flux cleaned = 0.00219326 Jy
! Component: 600  -  total flux cleaned = 0.00230223 Jy
! Component: 650  -  total flux cleaned = 0.00238155 Jy
! Component: 700  -  total flux cleaned = 0.00250943 Jy
! Component: 750  -  total flux cleaned = 0.00270771 Jy
! Component: 800  -  total flux cleaned = 0.00280373 Jy
! Component: 850  -  total flux cleaned = 0.00294478 Jy
! Component: 900  -  total flux cleaned = 0.00305894 Jy
! Component: 950  -  total flux cleaned = 0.00312568 Jy
! Component: 1000  -  total flux cleaned = 0.00321265 Jy
! Total flux subtracted in 1024 components = 0.00325505 Jy
! Clean residual min=-0.001534 max=0.001345 Jy/beam
! Clean residual mean=0.000034 rms=0.000464 Jy/beam
! Combined flux in latest and established models = 0.0771353 Jy
keep
! Adding 51 model components to the UV plane model.
! The established model now contains 74 components and 0.0771353 Jy
![Exited script file: muppet]
wmap "1320-407_X_2010_10_13_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8716 x 2.888 at 5.477 degrees (North through East)
! Clean map  min=-0.0023254  max=0.069105 Jy/beam
! Writing clean map to FITS file: 1320-407_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 0.0691052 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.922% of the data.
!  The x-axis pixel size should ideally be below 0.1956 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000463321 
device "1320-407_X_2010_10_13_pus\_map.eps/VPS"
! Attempting to open device: '1320-407_X_2010_10_13_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -2.01137 2.01137 4.02274 8.04549 16.091 32.182 64.3639
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0013 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.069 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8716 x 2.888 at 5.477 degrees (North through East)
! Clean map  min=-0.0023254  max=0.069105 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "1320-407_X_2010_10_13_pus\_map.gif/vgif"
! Attempting to open device: '1320-407_X_2010_10_13_pus_map.gif/vgif'
mapplot cln