! Started logfile: J1603+6945_X_2013_01_09_pus_uvs.log on Mon Nov  3 15:55:08 2014
obs J1603+6945_X_2013_01_09_pus_uva.fits
! Reading UV FITS file: J1603+6945_X_2013_01_09_pus_uva.fits
! AN table 1: Unused.
! AN table 2: 176 integrations on 120 of 120 possible baselines.
! AN table 3: Unused.
! AN table 4: Unused.
! AN table 5: Unused.
! Apparent sampling: 0.454119 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J1603+6945
! 
! 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 2994 lines of history.
! 
! Reading 38364 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 J1603+6945_X_2013_01_09_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 889 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 889 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 889 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 889 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.891923Jy  sigma=0.010105
! Fit after  self-cal, rms=0.869421Jy  sigma=0.009888
! 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 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 milli-arcsec
! Estimated beam: bmin=0.4343 mas, bmaj=0.9431 mas, bpa=-42.94 degrees
! Estimated noise=834.384 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 = 0.089835 Jy
! Component: 100  -  total flux cleaned = 0.127769 Jy
! Total flux subtracted in 100 components = 0.127769 Jy
! Clean residual min=-0.007301 max=0.017818 Jy/beam
! Clean residual mean=0.000172 rms=0.002464 Jy/beam
! Combined flux in latest and established models = 0.127769 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 9 components and 0.127769 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.140513Jy  sigma=0.001265
! Fit after  self-cal, rms=0.140132Jy  sigma=0.001262
! Inverting map 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0209329 Jy
! Component: 100  -  total flux cleaned = 0.033767 Jy
! Total flux subtracted in 100 components = 0.033767 Jy
! Clean residual min=-0.005277 max=0.009132 Jy/beam
! Clean residual mean=0.000111 rms=0.001717 Jy/beam
! Combined flux in latest and established models = 0.161536 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 16 components and 0.161536 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.134664Jy  sigma=0.001193
! Fit after  self-cal, rms=0.134618Jy  sigma=0.001193
! Inverting map 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 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 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 milli-arcsec
! Estimated beam: bmin=0.5768 mas, bmaj=1.089 mas, bpa=-44 degrees
! Estimated noise=338.886 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 = 0.0144682 Jy
! Component: 100  -  total flux cleaned = 0.0221441 Jy
! Component: 150  -  total flux cleaned = 0.0264704 Jy
! Component: 200  -  total flux cleaned = 0.0289712 Jy
! Total flux subtracted in 200 components = 0.0289712 Jy
! Clean residual min=-0.007047 max=0.007032 Jy/beam
! Clean residual mean=0.000107 rms=0.001938 Jy/beam
! Combined flux in latest and established models = 0.190507 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 23 components and 0.190507 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.133139Jy  sigma=0.001173
! Fit after  self-cal, rms=0.133136Jy  sigma=0.001173
! Inverting map 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 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        1.06     FD        1.09     HH        1.00*    HN        1.07     
!   KP        0.76     LA        0.98     MC        1.00*    MK        0.95     
!   NL        0.83     NY        1.00*    OV        1.02     PT        1.01     
!   SC        0.99     TS        1.09     WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.16     FD        1.11     HH        1.00*    HN        1.13     
!   KP        0.74     LA        1.02     MC        1.00*    MK        1.00     
!   NL        0.98     NY        1.00*    OV        1.04     PT        1.06     
!   SC        1.06     TS        0.96     WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.17     FD        1.10     HH        1.00*    HN        1.07     
!   KP        0.64     LA        1.01     MC        1.00*    MK        0.96     
!   NL        0.94     NY        1.00*    OV        1.05     PT        1.02     
!   SC        1.02     TS        0.98     WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.21     FD        1.17     HH        1.00*    HN        1.09     
!   KP        0.71     LA        1.09     MC        1.00*    MK        1.01     
!   NL        0.97     NY        1.00*    OV        1.09     PT        1.12     
!   SC        1.12     TS        1.12     WF        1.00*    WZ        1.00*    
! 
! 
! Fit before self-cal, rms=0.133136Jy  sigma=0.001173
! Fit after  self-cal, rms=0.135874Jy  sigma=0.001136
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 milli-arcsec
! Estimated beam: bmin=0.5831 mas, bmaj=1.096 mas, bpa=-43.92 degrees
! Estimated noise=338.404 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 (-12, -9.4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00373196 Jy
! Component: 100  -  total flux cleaned = 0.00465537 Jy
! Component: 150  -  total flux cleaned = 0.00503736 Jy
! Component: 200  -  total flux cleaned = 0.00529184 Jy
! Total flux subtracted in 200 components = 0.00529184 Jy
! Clean residual min=-0.002129 max=0.002404 Jy/beam
! Clean residual mean=0.000110 rms=0.000597 Jy/beam
! Combined flux in latest and established models = 0.195799 Jy
! Performing phase self-cal
! Adding 26 model components to the UV plane model.
! The established model now contains 48 components and 0.195799 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.135753Jy  sigma=0.001134
! Fit after  self-cal, rms=0.135972Jy  sigma=0.001133
! Inverting map 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 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=0.135972Jy  sigma=0.001133
! Fit after  self-cal, rms=0.141386Jy  sigma=0.001131
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 milli-arcsec
! Estimated beam: bmin=0.5842 mas, bmaj=1.096 mas, bpa=-44.13 degrees
! Estimated noise=339.28 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000136655 Jy
! Component: 100  -  total flux cleaned = -5.50111e-07 Jy
! Component: 150  -  total flux cleaned = 2.63075e-05 Jy
! Component: 200  -  total flux cleaned = 2.52883e-05 Jy
! Total flux subtracted in 200 components = 2.52883e-05 Jy
! Clean residual min=-0.001564 max=0.002084 Jy/beam
! Clean residual mean=0.000058 rms=0.000459 Jy/beam
! Combined flux in latest and established models = 0.195824 Jy
selfcal
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 54 components and 0.195824 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.141370Jy  sigma=0.001131
! Fit after  self-cal, rms=0.141437Jy  sigma=0.001131
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 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 (1, 0.6).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00128116 Jy
! Component: 100  -  total flux cleaned = 0.00101527 Jy
! Component: 150  -  total flux cleaned = 0.000860227 Jy
! Component: 200  -  total flux cleaned = 0.000790486 Jy
! Total flux subtracted in 200 components = 0.000790486 Jy
! Clean residual min=-0.001466 max=0.001696 Jy/beam
! Clean residual mean=0.000052 rms=0.000429 Jy/beam
! Combined flux in latest and established models = 0.196615 Jy
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 61 components and 0.196615 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.141402Jy  sigma=0.001130
! Fit after  self-cal, rms=0.141403Jy  sigma=0.001130
! Inverting map 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 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=0.141403Jy  sigma=0.001130
! Fit after  self-cal, rms=0.141168Jy  sigma=0.001130
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 milli-arcsec
! Estimated beam: bmin=0.5819 mas, bmaj=1.097 mas, bpa=-43.95 degrees
! Estimated noise=338.174 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000349933 Jy
! Component: 100  -  total flux cleaned = 0.000162027 Jy
! Component: 150  -  total flux cleaned = 6.384e-05 Jy
! Component: 200  -  total flux cleaned = 5.32352e-06 Jy
! Total flux subtracted in 200 components = 5.32352e-06 Jy
! Clean residual min=-0.001492 max=0.001641 Jy/beam
! Clean residual mean=0.000051 rms=0.000409 Jy/beam
! Combined flux in latest and established models = 0.19662 Jy
selfcal
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 64 components and 0.19662 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.141147Jy  sigma=0.001130
! Fit after  self-cal, rms=0.141146Jy  sigma=0.001130
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 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 = 0.000112478 Jy
! Component: 100  -  total flux cleaned = 0.000111603 Jy
! Component: 150  -  total flux cleaned = 0.000137161 Jy
! Component: 200  -  total flux cleaned = 0.000114275 Jy
! Total flux subtracted in 200 components = 0.000114275 Jy
! Clean residual min=-0.001447 max=0.001592 Jy/beam
! Clean residual mean=0.000050 rms=0.000401 Jy/beam
! Combined flux in latest and established models = 0.196734 Jy
! Performing phase self-cal
! Adding 20 model components to the UV plane model.
! The established model now contains 70 components and 0.196734 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.141133Jy  sigma=0.001130
! Fit after  self-cal, rms=0.141134Jy  sigma=0.001130
! Inverting map 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 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=0.141134Jy  sigma=0.001130
! Fit after  self-cal, rms=0.140878Jy  sigma=0.001130
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 milli-arcsec
! Estimated beam: bmin=1.996 mas, bmaj=3.785 mas, bpa=85.13 degrees
! Estimated noise=515.245 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000636591 Jy
! Component: 100  -  total flux cleaned = 0.000810021 Jy
! Component: 150  -  total flux cleaned = 0.000830491 Jy
! Component: 200  -  total flux cleaned = 0.000849507 Jy
! Total flux subtracted in 200 components = 0.000849507 Jy
! Clean residual min=-0.001578 max=0.001919 Jy/beam
! Clean residual mean=0.000125 rms=0.000567 Jy/beam
! Combined flux in latest and established models = 0.197584 Jy
selfcal
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 77 components and 0.197584 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.140875Jy  sigma=0.001130
! Fit after  self-cal, rms=0.140872Jy  sigma=0.001130
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 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 = 0.000171899 Jy
! Component: 100  -  total flux cleaned = 0.000189436 Jy
! Component: 150  -  total flux cleaned = 0.000205455 Jy
! Component: 200  -  total flux cleaned = 0.000220424 Jy
! Total flux subtracted in 200 components = 0.000220424 Jy
! Clean residual min=-0.001592 max=0.001868 Jy/beam
! Clean residual mean=0.000119 rms=0.000565 Jy/beam
! Combined flux in latest and established models = 0.197804 Jy
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 82 components and 0.197804 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.140870Jy  sigma=0.001130
! Fit after  self-cal, rms=0.140871Jy  sigma=0.001130
! Inverting map 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 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 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 milli-arcsec
! Estimated beam: bmin=0.5799 mas, bmaj=1.097 mas, bpa=-43.74 degrees
! Estimated noise=337.405 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5799 x 1.097 at -43.74 degrees (North through East)
! Clean map  min=-0.0012963  max=0.12046 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 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 milli-arcsec
! Estimated beam: bmin=0.4359 mas, bmaj=0.947 mas, bpa=-42.53 degrees
! Estimated noise=842.25 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0903498 Jy
! Component: 100  -  total flux cleaned = 0.12916 Jy
! Component: 150  -  total flux cleaned = 0.150122 Jy
! Component: 200  -  total flux cleaned = 0.163326 Jy
! Total flux subtracted in 200 components = 0.163326 Jy
! Clean residual min=-0.003840 max=0.007802 Jy/beam
! Clean residual mean=0.000091 rms=0.001249 Jy/beam
! Combined flux in latest and established models = 0.163326 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 18 model components to the UV plane model.
! The established model now contains 18 components and 0.163326 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 milli-arcsec
! Estimated beam: bmin=0.5799 mas, bmaj=1.097 mas, bpa=-43.74 degrees
! Estimated noise=337.405 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 = 0.0128438 Jy
! Component: 100  -  total flux cleaned = 0.0196774 Jy
! Component: 150  -  total flux cleaned = 0.0241132 Jy
! Component: 200  -  total flux cleaned = 0.0270713 Jy
! Total flux subtracted in 200 components = 0.0270713 Jy
! Clean residual min=-0.001506 max=0.001985 Jy/beam
! Clean residual mean=0.000118 rms=0.000510 Jy/beam
! Combined flux in latest and established models = 0.190397 Jy
! Adding 26 model components to the UV plane model.
! The established model now contains 33 components and 0.190397 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 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 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 milli-arcsec
! Estimated beam: bmin=1.996 mas, bmaj=3.785 mas, bpa=85.13 degrees
! Estimated noise=515.245 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00366043 Jy
! Component: 100  -  total flux cleaned = 0.00544349 Jy
! Component: 150  -  total flux cleaned = 0.00622218 Jy
! Component: 200  -  total flux cleaned = 0.00655066 Jy
! Total flux subtracted in 200 components = 0.00655066 Jy
! Clean residual min=-0.001541 max=0.002071 Jy/beam
! Clean residual mean=0.000147 rms=0.000587 Jy/beam
! Combined flux in latest and established models = 0.196948 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 = 0.000229404 Jy
! Component: 100  -  total flux cleaned = 0.000293096 Jy
! Component: 150  -  total flux cleaned = 0.000350455 Jy
! Component: 200  -  total flux cleaned = 0.000402571 Jy
! Total flux subtracted in 200 components = 0.000402571 Jy
! Clean residual min=-0.001519 max=0.002110 Jy/beam
! Clean residual mean=0.000136 rms=0.000574 Jy/beam
! Combined flux in latest and established models = 0.197351 Jy
! Adding 33 model components to the UV plane model.
! The established model now contains 57 components and 0.197351 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 milli-arcsec
! Estimated beam: bmin=0.5799 mas, bmaj=1.097 mas, bpa=-43.74 degrees
! Estimated noise=337.405 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000144829 Jy
! Component: 100  -  total flux cleaned = -0.000317882 Jy
! Component: 150  -  total flux cleaned = -0.000433809 Jy
! Component: 200  -  total flux cleaned = -0.000536526 Jy
! Total flux subtracted in 200 components = -0.000536526 Jy
! Clean residual min=-0.001581 max=0.001369 Jy/beam
! Clean residual mean=0.000048 rms=0.000394 Jy/beam
! Combined flux in latest and established models = 0.196814 Jy
selfcal
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 68 components and 0.196814 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.140862Jy  sigma=0.001130
! Fit after  self-cal, rms=0.140856Jy  sigma=0.001129
wmodel J1603+6945_X_2013_01_09_pus_map.mod
! Writing 68 model components to file: J1603+6945_X_2013_01_09_pus_map.mod
wobs J1603+6945_X_2013_01_09_pus_uvs.fits
! Writing UV FITS file: J1603+6945_X_2013_01_09_pus_uvs.fits
wwins J1603+6945_X_2013_01_09_pus_map.win
! wwins: Wrote 3 windows to J1603+6945_X_2013_01_09_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 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 milli-arcsec
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -6.25345e-05 Jy
! Component: 100  -  total flux cleaned = -0.000109969 Jy
! Component: 150  -  total flux cleaned = -8.59931e-05 Jy
! Component: 200  -  total flux cleaned = -8.64244e-05 Jy
! Component: 250  -  total flux cleaned = -0.000108048 Jy
! Component: 300  -  total flux cleaned = -8.74051e-05 Jy
! Component: 350  -  total flux cleaned = -2.76983e-05 Jy
! Component: 400  -  total flux cleaned = 1.08695e-05 Jy
! Component: 450  -  total flux cleaned = 0.000122999 Jy
! Component: 500  -  total flux cleaned = 0.000177377 Jy
! Component: 550  -  total flux cleaned = 0.000249111 Jy
! Component: 600  -  total flux cleaned = 0.000372245 Jy
! Component: 650  -  total flux cleaned = 0.000493034 Jy
! Component: 700  -  total flux cleaned = 0.000594643 Jy
! Component: 750  -  total flux cleaned = 0.000744473 Jy
! Component: 800  -  total flux cleaned = 0.000875399 Jy
! Component: 850  -  total flux cleaned = 0.00103616 Jy
! Component: 900  -  total flux cleaned = 0.00114708 Jy
! Component: 950  -  total flux cleaned = 0.00131902 Jy
! Component: 1000  -  total flux cleaned = 0.00148836 Jy
! Total flux subtracted in 1024 components = 0.00157979 Jy
! Clean residual min=-0.000769 max=0.000896 Jy/beam
! Clean residual mean=0.000043 rms=0.000297 Jy/beam
! Combined flux in latest and established models = 0.198394 Jy
keep
! Adding 71 model components to the UV plane model.
! The established model now contains 139 components and 0.198394 Jy
![Exited script file: muppet]
wmap "J1603+6945_X_2013_01_09_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5799 x 1.097 at -43.74 degrees (North through East)
! Clean map  min=-0.0013406  max=0.12114 Jy/beam
! Writing clean map to FITS file: J1603+6945_X_2013_01_09_pus_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.121135 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.907% of the data.
!  The y-axis pixel size should ideally be below 0.176 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000296908 
device "J1603+6945_X_2013_01_09_pus\_map.eps/VPS"
! Attempting to open device: 'J1603+6945_X_2013_01_09_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.735314 0.735314 1.47063 2.94126 5.88251 11.765 23.53 47.0601 94.1202
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0008 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.121 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5799 x 1.097 at -43.74 degrees (North through East)
! Clean map  min=-0.0013406  max=0.12114 Jy/beam
quit
! Quitting program
! Log file J1603+6945_X_2013_01_09_pus_uvs.log closed on Mon Nov  3 15:55:12 2014