! Started logfile: J0854+2006_X_2011_06_28_pus_uvs.log on Sun Apr 22 11:10:44 2012
obs J0854+2006_X_2011_06_28_pus_uva.fits
! Reading UV FITS file: J0854+2006_X_2011_06_28_pus_uva.fits
! AN table 1: 76 integrations on 153 of 153 possible baselines.
! AN table 2: 61 integrations on 153 of 153 possible baselines.
! AN table 3: 95 integrations on 153 of 153 possible baselines.
! AN table 4: 55 integrations on 153 of 153 possible baselines.
! Apparent sampling: 0.0815058 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J0854+2006
! 
! 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 5253 lines of history.
! 
! Reading 14316 visibilities.
select I
! Polarization I is unavailable.
! Selecting polarization: RR,  channels: 1..4
! Reading IF 1 channels: 1..1
! Reading IF 2 channels: 2..2
! Reading IF 3 channels: 3..3
! Reading IF 4 channels: 4..4
print "field_size =",field_size
! field_size = 512 
print "field_cell =",field_cell
! field_cell = 0.2 
print "taper_size =",taper_size
! taper_size = 70 
![@muppet J0854+2006_X_2011_06_28_pus]
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.03
float dynam
dynam = 6.0
float soltime1
soltime1 = 120
float soltime2
soltime2 = 20
float thresh
thresh = 0.5
float win_mult
win_mult = 1.8
float time_av
time_av = 16
float old_peak
float new_peak
float flux_cutoff
mapsize field_size, field_cell
! Map grid = 512x512 pixels with 0.200x0.200 milli-arcsec cellsize.
startmod
! Applying default point source starting model.
! Performing phase self-cal
! Adding 1 model components to the UV plane model.
! The established model now contains 1 components and 1 Jy
! 
! Correcting IF 1.
!  A total of 1139 telescope corrections were flagged in sub-array 1.
!  A total of 853 telescope corrections were flagged in sub-array 2.
!  A total of 1367 telescope corrections were flagged in sub-array 3.
!  A total of 633 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 2.
!  A total of 1139 telescope corrections were flagged in sub-array 1.
!  A total of 853 telescope corrections were flagged in sub-array 2.
!  A total of 1367 telescope corrections were flagged in sub-array 3.
!  A total of 633 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 3.
!  A total of 1139 telescope corrections were flagged in sub-array 1.
!  A total of 853 telescope corrections were flagged in sub-array 2.
!  A total of 1367 telescope corrections were flagged in sub-array 3.
!  A total of 633 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 4.
!  A total of 1139 telescope corrections were flagged in sub-array 1.
!  A total of 853 telescope corrections were flagged in sub-array 2.
!  A total of 1367 telescope corrections were flagged in sub-array 3.
!  A total of 633 telescope corrections were flagged in sub-array 4.
! 
! Fit before self-cal, rms=4.233625Jy  sigma=0.039257
! Fit after  self-cal, rms=4.198080Jy  sigma=0.039180
! 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 4.55% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! Estimated beam: bmin=0.5193 mas, bmaj=0.816 mas, bpa=8.615 degrees
! Estimated noise=994.966 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 = 3.79533 Jy
! Component: 100  -  total flux cleaned = 4.91625 Jy
! Total flux subtracted in 100 components = 4.91625 Jy
! Clean residual min=-0.129717 max=0.523902 Jy/beam
! Clean residual mean=0.000411 rms=0.034274 Jy/beam
! Combined flux in latest and established models = 4.91625 Jy
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 6 components and 4.91625 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=1.124857Jy  sigma=0.011081
! Fit after  self-cal, rms=1.118406Jy  sigma=0.011057
! Inverting map 
! Your choice of large map pixels excluded 4.55% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.596392 Jy
! Component: 100  -  total flux cleaned = 0.936493 Jy
! Total flux subtracted in 100 components = 0.936493 Jy
! Clean residual min=-0.081792 max=0.213950 Jy/beam
! Clean residual mean=0.000226 rms=0.019500 Jy/beam
! Combined flux in latest and established models = 5.85274 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 10 components and 5.85274 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.679500Jy  sigma=0.006412
! Fit after  self-cal, rms=0.670850Jy  sigma=0.006377
! Inverting map 
! Your choice of large map pixels excluded 4.55% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! Added new window around map position (-0.6, -1).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.242076 Jy
! Component: 100  -  total flux cleaned = 0.407528 Jy
! Total flux subtracted in 100 components = 0.407528 Jy
! Clean residual min=-0.065021 max=0.115507 Jy/beam
! Clean residual mean=0.000146 rms=0.014982 Jy/beam
! Combined flux in latest and established models = 6.26027 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 16 components and 6.26027 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.554687Jy  sigma=0.004976
! Fit after  self-cal, rms=0.546981Jy  sigma=0.004931
! Inverting map 
! Your choice of large map pixels excluded 4.55% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.137168 Jy
! Component: 100  -  total flux cleaned = 0.236653 Jy
! Total flux subtracted in 100 components = 0.236653 Jy
! Clean residual min=-0.060464 max=0.078557 Jy/beam
! Clean residual mean=0.000099 rms=0.012935 Jy/beam
! Combined flux in latest and established models = 6.49692 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 20 components and 6.49692 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.502238Jy  sigma=0.004329
! Fit after  self-cal, rms=0.498521Jy  sigma=0.004307
! Inverting map 
! Your choice of large map pixels excluded 4.55% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 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 4.55% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! Estimated beam: bmin=0.5933 mas, bmaj=0.9215 mas, bpa=8.364 degrees
! Estimated noise=743.706 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 = 0.124619 Jy
! Component: 100  -  total flux cleaned = 0.204505 Jy
! Component: 150  -  total flux cleaned = 0.258572 Jy
! Component: 200  -  total flux cleaned = 0.295449 Jy
! Total flux subtracted in 200 components = 0.295449 Jy
! Clean residual min=-0.052176 max=0.065009 Jy/beam
! Clean residual mean=-0.000256 rms=0.012092 Jy/beam
! Combined flux in latest and established models = 6.79237 Jy
! Performing phase self-cal
! Adding 20 model components to the UV plane model.
! The established model now contains 30 components and 6.79237 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.475209Jy  sigma=0.003888
! Fit after  self-cal, rms=0.471776Jy  sigma=0.003864
! Inverting map 
! Your choice of large map pixels excluded 4.55% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 9 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    FT        1.00*    HH        0.96     
!   HN        0.99     KK        0.96     KP        1.00*    MC        1.04     
!   MK        1.04     NL        1.00     NY        1.05     OV        1.00*    
!   PT        1.00*    SC        0.98     SH        0.97     TS        1.11     
!   WF        1.00     WZ        1.00     
! 
!  A total of 54 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.93     FD        0.94     FT        1.00*    HH        1.00*    
!   HN        0.97     KK        0.98     KP        0.96     MC        1.04     
!   MK        1.02     NL        0.98     NY        1.04     OV        0.95     
!   PT        0.92     SC        0.95     SH        0.95     TS        0.97     
!   WF        1.00     WZ        1.00*    
! 
!  A total of 96 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.93     FD        1.02     FT        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.00     KP        1.00     MC        1.02     
!   MK        1.02     NL        1.06     NY        1.04     OV        0.96     
!   PT        0.97     SC        1.00*    SH        0.95     TS        1.04     
!   WF        1.00*    WZ        0.99     
! 
!  A total of 24 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        0.96     FD        1.01     FT        1.00*    HH        1.06     
!   HN        0.98     KK        1.00*    KP        1.03     MC        1.02     
!   MK        1.00*    NL        1.01     NY        1.05     OV        0.98     
!   PT        0.99     SC        0.98     SH        1.00*    TS        1.00*    
!   WF        1.02     WZ        0.97     
! 
! 
! Correcting IF 2.
!  A total of 9 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    FT        1.00*    HH        0.97     
!   HN        0.99     KK        0.93     KP        1.00*    MC        1.04     
!   MK        1.03     NL        1.04     NY        1.02     OV        1.00*    
!   PT        1.00*    SC        1.01     SH        0.99     TS        1.14     
!   WF        0.97     WZ        1.00     
! 
!  A total of 54 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.97     FD        0.91     FT        1.00*    HH        1.00*    
!   HN        0.99     KK        0.96     KP        0.94     MC        1.04     
!   MK        1.00     NL        1.02     NY        1.01     OV        0.98     
!   PT        0.94     SC        0.98     SH        0.97     TS        0.99     
!   WF        0.99     WZ        1.00*    
! 
!  A total of 96 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.97     FD        0.98     FT        1.00*    HH        1.00*    
!   HN        1.00*    KK        0.97     KP        0.98     MC        1.00     
!   MK        0.99     NL        1.10     NY        1.01     OV        0.98     
!   PT        0.98     SC        1.00*    SH        0.97     TS        1.06     
!   WF        1.00*    WZ        1.00     
! 
!  A total of 24 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00     FD        0.98     FT        1.00*    HH        1.05     
!   HN        1.00     KK        1.00*    KP        1.01     MC        1.02     
!   MK        1.00*    NL        1.04     NY        1.02     OV        1.01     
!   PT        1.01     SC        1.01     SH        1.00*    TS        1.00*    
!   WF        1.01     WZ        0.96     
! 
! 
! Correcting IF 3.
!  A total of 9 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    FT        1.00*    HH        0.99     
!   HN        0.99     KK        1.00     KP        1.00*    MC        1.04     
!   MK        1.01     NL        0.99     NY        1.04     OV        1.00*    
!   PT        1.00*    SC        1.01     SH        1.04     TS        1.14     
!   WF        1.05     WZ        0.98     
! 
!  A total of 54 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.95     FD        0.94     FT        1.00*    HH        1.00*    
!   HN        0.98     KK        1.02     KP        0.95     MC        1.05     
!   MK        0.97     NL        0.96     NY        1.03     OV        0.97     
!   PT        0.92     SC        0.99     SH        1.00     TS        1.01     
!   WF        1.07     WZ        1.00*    
! 
!  A total of 96 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.95     FD        1.02     FT        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.02     KP        0.98     MC        1.04     
!   MK        0.97     NL        1.04     NY        1.04     OV        0.97     
!   PT        0.97     SC        1.00*    SH        1.02     TS        1.07     
!   WF        1.00*    WZ        0.98     
! 
!  A total of 24 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        0.98     FD        1.02     FT        1.00*    HH        1.12     
!   HN        0.99     KK        1.00*    KP        1.01     MC        1.01     
!   MK        1.00*    NL        0.99     NY        1.01     OV        1.00     
!   PT        0.99     SC        1.01     SH        1.00*    TS        1.00*    
!   WF        1.06     WZ        0.95     
! 
! 
! Correcting IF 4.
!  A total of 9 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    FT        1.00*    HH        0.97     
!   HN        0.99     KK        0.99     KP        1.00*    MC        1.05     
!   MK        1.06     NL        1.01     NY        1.03     OV        1.00*    
!   PT        1.00*    SC        1.03     SH        0.98     TS        1.12     
!   WF        1.00     WZ        1.04     
! 
!  A total of 54 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        0.96     FT        1.00*    HH        1.00*    
!   HN        0.98     KK        0.99     KP        0.91     MC        1.06     
!   MK        1.03     NL        0.99     NY        1.02     OV        1.00     
!   PT        0.94     SC        0.99     SH        0.95     TS        1.01     
!   WF        1.04     WZ        1.00*    
! 
!  A total of 96 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00     FD        1.03     FT        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.00     KP        0.95     MC        1.00     
!   MK        1.03     NL        1.07     NY        1.02     OV        1.00     
!   PT        0.98     SC        1.00*    SH        0.96     TS        1.07     
!   WF        1.00*    WZ        1.04     
! 
!  A total of 24 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.03     FD        1.02     FT        1.00*    HH        1.06     
!   HN        0.99     KK        1.00*    KP        0.98     MC        1.01     
!   MK        1.00*    NL        1.02     NY        1.03     OV        1.04     
!   PT        1.00     SC        1.02     SH        1.00*    TS        1.00*    
!   WF        1.03     WZ        1.02     
! 
! 
! Fit before self-cal, rms=0.471776Jy  sigma=0.003864
! Fit after  self-cal, rms=0.397845Jy  sigma=0.002836
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! Estimated beam: bmin=0.6063 mas, bmaj=0.964 mas, bpa=3.922 degrees
! Estimated noise=756.155 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 = 9.89002e-05 Jy
! Component: 100  -  total flux cleaned = -0.00710808 Jy
! Component: 150  -  total flux cleaned = -0.0102025 Jy
! Component: 200  -  total flux cleaned = -0.0120834 Jy
! Total flux subtracted in 200 components = -0.0120834 Jy
! Clean residual min=-0.039777 max=0.042641 Jy/beam
! Clean residual mean=0.000190 rms=0.008445 Jy/beam
! Combined flux in latest and established models = 6.78029 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 37 components and 6.78029 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.393108Jy  sigma=0.002794
! Fit after  self-cal, rms=0.392294Jy  sigma=0.002788
! Inverting map 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 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=0.392294Jy  sigma=0.002788
! Fit after  self-cal, rms=0.281270Jy  sigma=0.001973
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! Estimated beam: bmin=0.6067 mas, bmaj=0.9648 mas, bpa=3.758 degrees
! Estimated noise=755.842 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.0118417 Jy
! Component: 100  -  total flux cleaned = -0.0118184 Jy
! Component: 150  -  total flux cleaned = -0.011843 Jy
! Component: 200  -  total flux cleaned = -0.0118268 Jy
! Total flux subtracted in 200 components = -0.0118268 Jy
! Clean residual min=-0.022239 max=0.021868 Jy/beam
! Clean residual mean=0.000115 rms=0.004213 Jy/beam
! Combined flux in latest and established models = 6.76846 Jy
selfcal
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 43 components and 6.76846 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.278354Jy  sigma=0.001950
! Fit after  self-cal, rms=0.277891Jy  sigma=0.001948
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 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 (-1.2, -1).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0133224 Jy
! Component: 100  -  total flux cleaned = 0.0122372 Jy
! Component: 150  -  total flux cleaned = 0.0112973 Jy
! Component: 200  -  total flux cleaned = 0.0108832 Jy
! Total flux subtracted in 200 components = 0.0108832 Jy
! Clean residual min=-0.021875 max=0.018466 Jy/beam
! Clean residual mean=0.000021 rms=0.004066 Jy/beam
! Combined flux in latest and established models = 6.77934 Jy
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 54 components and 6.77934 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.275867Jy  sigma=0.001926
! Fit after  self-cal, rms=0.275441Jy  sigma=0.001923
! Inverting map 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 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=0.275441Jy  sigma=0.001923
! Fit after  self-cal, rms=0.241723Jy  sigma=0.001667
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! Estimated beam: bmin=0.6066 mas, bmaj=0.9662 mas, bpa=3.668 degrees
! Estimated noise=755.804 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00570896 Jy
! Component: 100  -  total flux cleaned = 0.00517184 Jy
! Component: 150  -  total flux cleaned = 0.00552892 Jy
! Component: 200  -  total flux cleaned = 0.00518446 Jy
! Total flux subtracted in 200 components = 0.00518446 Jy
! Clean residual min=-0.012911 max=0.009380 Jy/beam
! Clean residual mean=0.000023 rms=0.002022 Jy/beam
! Combined flux in latest and established models = 6.78453 Jy
selfcal
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 60 components and 6.78453 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.239645Jy  sigma=0.001649
! Fit after  self-cal, rms=0.239186Jy  sigma=0.001647
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 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 = 0.000451212 Jy
! Component: 100  -  total flux cleaned = 0.00182843 Jy
! Component: 150  -  total flux cleaned = 0.00212817 Jy
! Component: 200  -  total flux cleaned = 0.0021249 Jy
! Total flux subtracted in 200 components = 0.0021249 Jy
! Clean residual min=-0.011727 max=0.008360 Jy/beam
! Clean residual mean=0.000005 rms=0.001934 Jy/beam
! Combined flux in latest and established models = 6.78665 Jy
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 62 components and 6.78665 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.238393Jy  sigma=0.001640
! Fit after  self-cal, rms=0.238097Jy  sigma=0.001639
! Inverting map 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 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=0.238097Jy  sigma=0.001639
! Fit after  self-cal, rms=0.238014Jy  sigma=0.001635
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! Estimated beam: bmin=2.245 mas, bmaj=2.446 mas, bpa=9.959 degrees
! Estimated noise=1134.15 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.0038251 Jy
! Component: 100  -  total flux cleaned = -0.00352148 Jy
! Component: 150  -  total flux cleaned = -0.00330977 Jy
! Component: 200  -  total flux cleaned = -0.00330446 Jy
! Total flux subtracted in 200 components = -0.00330446 Jy
! Clean residual min=-0.009367 max=0.009068 Jy/beam
! Clean residual mean=-0.000288 rms=0.002810 Jy/beam
! Combined flux in latest and established models = 6.78335 Jy
selfcal
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 69 components and 6.78335 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.237429Jy  sigma=0.001630
! Fit after  self-cal, rms=0.237152Jy  sigma=0.001629
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 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 = 0.000440264 Jy
! Component: 100  -  total flux cleaned = 0.000623126 Jy
! Component: 150  -  total flux cleaned = 0.000771791 Jy
! Component: 200  -  total flux cleaned = 0.000783688 Jy
! Total flux subtracted in 200 components = 0.000783688 Jy
! Clean residual min=-0.009108 max=0.008874 Jy/beam
! Clean residual mean=-0.000314 rms=0.002785 Jy/beam
! Combined flux in latest and established models = 6.78413 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 73 components and 6.78413 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.237008Jy  sigma=0.001628
! Fit after  self-cal, rms=0.236808Jy  sigma=0.001627
! Inverting map 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 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 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! Estimated beam: bmin=0.6067 mas, bmaj=0.9674 mas, bpa=3.585 degrees
! Estimated noise=756.054 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6067 x 0.9674 at 3.585 degrees (North through East)
! Clean map  min=-0.0068953  max=5.0919 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=0.236808Jy  sigma=0.001627
! Fit after  self-cal, rms=0.205295Jy  sigma=0.001346
! Inverting map and beam 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! Estimated beam: bmin=0.607 mas, bmaj=0.9677 mas, bpa=3.624 degrees
! Estimated noise=755.731 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00383331 Jy
! Component: 100  -  total flux cleaned = -0.00385106 Jy
! Component: 150  -  total flux cleaned = -0.00445966 Jy
! Component: 200  -  total flux cleaned = -0.00446376 Jy
! Total flux subtracted in 200 components = -0.00446376 Jy
! Clean residual min=-0.009737 max=0.007058 Jy/beam
! Clean residual mean=-0.000179 rms=0.001706 Jy/beam
! Combined flux in latest and established models = 6.77967 Jy
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 76 components and 6.77967 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.204158Jy  sigma=0.001338
! Fit after  self-cal, rms=0.203987Jy  sigma=0.001337
! Inverting map 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000865976 Jy
! Component: 100  -  total flux cleaned = -0.000591591 Jy
! Component: 150  -  total flux cleaned = -0.000591285 Jy
! Component: 200  -  total flux cleaned = -0.000588736 Jy
! Total flux subtracted in 200 components = -0.000588736 Jy
! Clean residual min=-0.008817 max=0.006735 Jy/beam
! Clean residual mean=-0.000174 rms=0.001656 Jy/beam
! Combined flux in latest and established models = 6.77908 Jy
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 79 components and 6.77908 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.203402Jy  sigma=0.001333
! Fit after  self-cal, rms=0.203247Jy  sigma=0.001332
! Inverting map 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.203247Jy  sigma=0.001332
! Fit after  self-cal, rms=0.203253Jy  sigma=0.001329
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 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! Estimated beam: bmin=0.5316 mas, bmaj=0.8628 mas, bpa=3.025 degrees
! Estimated noise=1010.67 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 3.84499 Jy
! Component: 100  -  total flux cleaned = 4.94899 Jy
! Component: 150  -  total flux cleaned = 5.51915 Jy
! Component: 200  -  total flux cleaned = 5.86202 Jy
! Total flux subtracted in 200 components = 5.86202 Jy
! Clean residual min=-0.042206 max=0.181256 Jy/beam
! Clean residual mean=0.000193 rms=0.014293 Jy/beam
! Combined flux in latest and established models = 5.86202 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 11 model components to the UV plane model.
! The established model now contains 11 components and 5.86202 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! Estimated beam: bmin=0.6071 mas, bmaj=0.9689 mas, bpa=3.529 degrees
! Estimated noise=756.021 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 = 0.324823 Jy
! Component: 100  -  total flux cleaned = 0.523937 Jy
! Component: 150  -  total flux cleaned = 0.6527 Jy
! Component: 200  -  total flux cleaned = 0.73706 Jy
! Total flux subtracted in 200 components = 0.73706 Jy
! Clean residual min=-0.011249 max=0.045370 Jy/beam
! Clean residual mean=0.001335 rms=0.004492 Jy/beam
! Combined flux in latest and established models = 6.59908 Jy
! Adding 25 model components to the UV plane model.
! The established model now contains 28 components and 6.59907 Jy
! Inverting map 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0556008 Jy
! Component: 100  -  total flux cleaned = 0.0932395 Jy
! Component: 150  -  total flux cleaned = 0.119384 Jy
! Component: 200  -  total flux cleaned = 0.13794 Jy
! Total flux subtracted in 200 components = 0.13794 Jy
! Clean residual min=-0.007194 max=0.013337 Jy/beam
! Clean residual mean=0.000151 rms=0.001935 Jy/beam
! Combined flux in latest and established models = 6.73701 Jy
! Adding 22 model components to the UV plane model.
! The established model now contains 38 components and 6.73701 Jy
! Inverting map 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! Added new window around map position (0.2, -1).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0141296 Jy
! Component: 100  -  total flux cleaned = 0.0192733 Jy
! Component: 150  -  total flux cleaned = 0.0211017 Jy
! Component: 200  -  total flux cleaned = 0.0227315 Jy
! Total flux subtracted in 200 components = 0.0227315 Jy
! Clean residual min=-0.006967 max=0.008897 Jy/beam
! Clean residual mean=-0.000044 rms=0.001680 Jy/beam
! Combined flux in latest and established models = 6.75975 Jy
! Adding 25 model components to the UV plane model.
! The established model now contains 46 components and 6.75975 Jy
! Inverting map 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! Added new window around map position (-2.2, -2.6).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00272946 Jy
! Component: 100  -  total flux cleaned = 0.00331425 Jy
! Component: 150  -  total flux cleaned = 0.00386391 Jy
! Component: 200  -  total flux cleaned = 0.00438098 Jy
! Total flux subtracted in 200 components = 0.00438098 Jy
! Clean residual min=-0.006658 max=0.008061 Jy/beam
! Clean residual mean=-0.000082 rms=0.001609 Jy/beam
! Combined flux in latest and established models = 6.76413 Jy
! Adding 31 model components to the UV plane model.
! The established model now contains 58 components and 6.76413 Jy
! Inverting map 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! Added new window around map position (-3.6, -1).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00560762 Jy
! Component: 100  -  total flux cleaned = 0.00585414 Jy
! Component: 150  -  total flux cleaned = 0.00610135 Jy
! Component: 200  -  total flux cleaned = 0.00633521 Jy
! Total flux subtracted in 200 components = 0.00633521 Jy
! Clean residual min=-0.006312 max=0.006278 Jy/beam
! Clean residual mean=-0.000137 rms=0.001551 Jy/beam
! Combined flux in latest and established models = 6.77046 Jy
! Adding 26 model components to the UV plane model.
! The established model now contains 66 components and 6.77046 Jy
! Inverting map 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
uvw 0,2
! Uniform weighting is not currently selected.
! Amplitude error weighting is not currently selected.
! Radial weighting is not currently selected.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! Estimated beam: bmin=0.5842 mas, bmaj=0.8728 mas, bpa=8.23 degrees
! Estimated noise=935.125 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00472967 Jy
! Component: 100  -  total flux cleaned = -0.00503906 Jy
! Component: 150  -  total flux cleaned = -0.00503127 Jy
! Component: 200  -  total flux cleaned = -0.00529948 Jy
! Total flux subtracted in 200 components = -0.00529948 Jy
! Clean residual min=-0.008207 max=0.007304 Jy/beam
! Clean residual mean=-0.000257 rms=0.001870 Jy/beam
! Combined flux in latest and established models = 6.76516 Jy
clean
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -4.23765e-06 Jy
! Component: 100  -  total flux cleaned = -0.000258689 Jy
! Component: 150  -  total flux cleaned = -0.000252849 Jy
! Component: 200  -  total flux cleaned = -0.00048121 Jy
! Total flux subtracted in 200 components = -0.00048121 Jy
! Clean residual min=-0.007825 max=0.007206 Jy/beam
! Clean residual mean=-0.000251 rms=0.001832 Jy/beam
! Combined flux in latest and established models = 6.76468 Jy
selfcal
! Performing phase self-cal
! Adding 33 model components to the UV plane model.
! The established model now contains 79 components and 6.76468 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.217209Jy  sigma=0.001407
! Fit after  self-cal, rms=0.216149Jy  sigma=0.001402
wmodel J0854+2006_X_2011_06_28_pus_map.mod
! Writing 79 model components to file: J0854+2006_X_2011_06_28_pus_map.mod
wobs J0854+2006_X_2011_06_28_pus_uvs.fits
! Writing UV FITS file: J0854+2006_X_2011_06_28_pus_uvs.fits
wwins J0854+2006_X_2011_06_28_pus_map.win
! wwins: Wrote 6 windows to J0854+2006_X_2011_06_28_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 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00368438 Jy
! Component: 100  -  total flux cleaned = -0.00679947 Jy
! Component: 150  -  total flux cleaned = -0.00783435 Jy
! Component: 200  -  total flux cleaned = -0.00858778 Jy
! Component: 250  -  total flux cleaned = -0.00895728 Jy
! Component: 300  -  total flux cleaned = -0.00956268 Jy
! Component: 350  -  total flux cleaned = -0.0100374 Jy
! Component: 400  -  total flux cleaned = -0.0105046 Jy
! Component: 450  -  total flux cleaned = -0.0107331 Jy
! Component: 500  -  total flux cleaned = -0.0108463 Jy
! Component: 550  -  total flux cleaned = -0.0112937 Jy
! Component: 600  -  total flux cleaned = -0.0116226 Jy
! Component: 650  -  total flux cleaned = -0.0117311 Jy
! Component: 700  -  total flux cleaned = -0.0119467 Jy
! Component: 750  -  total flux cleaned = -0.0120533 Jy
! Component: 800  -  total flux cleaned = -0.0123696 Jy
! Component: 850  -  total flux cleaned = -0.0124738 Jy
! Component: 900  -  total flux cleaned = -0.0126807 Jy
! Component: 950  -  total flux cleaned = -0.0127825 Jy
! Component: 1000  -  total flux cleaned = -0.0130873 Jy
! Component: 1050  -  total flux cleaned = -0.0130867 Jy
! Component: 1100  -  total flux cleaned = -0.0132865 Jy
! Component: 1150  -  total flux cleaned = -0.0133861 Jy
! Component: 1200  -  total flux cleaned = -0.0136814 Jy
! Component: 1250  -  total flux cleaned = -0.0138766 Jy
! Component: 1300  -  total flux cleaned = -0.0141673 Jy
! Component: 1350  -  total flux cleaned = -0.0141674 Jy
! Component: 1400  -  total flux cleaned = -0.0143587 Jy
! Component: 1450  -  total flux cleaned = -0.0145486 Jy
! Component: 1500  -  total flux cleaned = -0.0145485 Jy
! Component: 1550  -  total flux cleaned = -0.0146423 Jy
! Component: 1600  -  total flux cleaned = -0.0148287 Jy
! Component: 1650  -  total flux cleaned = -0.0150131 Jy
! Component: 1700  -  total flux cleaned = -0.0151052 Jy
! Component: 1750  -  total flux cleaned = -0.015014 Jy
! Component: 1800  -  total flux cleaned = -0.0151047 Jy
! Component: 1850  -  total flux cleaned = -0.0154654 Jy
! Component: 1900  -  total flux cleaned = -0.0154653 Jy
! Component: 1950  -  total flux cleaned = -0.0156431 Jy
! Component: 2000  -  total flux cleaned = -0.0154662 Jy
! Total flux subtracted in 2048 components = -0.0156431 Jy
! Clean residual min=-0.004393 max=0.005384 Jy/beam
! Clean residual mean=-0.000061 rms=0.001517 Jy/beam
! Combined flux in latest and established models = 6.74904 Jy
keep
! Adding 182 model components to the UV plane model.
! The established model now contains 256 components and 6.74903 Jy
![Exited script file: muppet]
wmap "J0854+2006_X_2011_06_28_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5842 x 0.8728 at 8.23 degrees (North through East)
! Clean map  min=-0.0068028  max=5.0344 Jy/beam
! Writing clean map to FITS file: J0854+2006_X_2011_06_28_pus_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 5.03442 
invert
! Inverting map 
! Your choice of large map pixels excluded 4.25% of the data.
!  The x-axis pixel size should ideally be below 0.164 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1706 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.00151555 
device "J0854+2006_X_2011_06_28_pus\_map.eps/VPS"
! Attempting to open device: 'J0854+2006_X_2011_06_28_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.0903114 0.0903114 0.180623 0.361246 0.722491 1.44498 2.88996 5.77993 11.5599 23.1197 46.2394 92.4789
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0045 
print "peak=",int(1000*peak_flux)/1000
! peak= 5.034 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5842 x 0.8728 at 8.23 degrees (North through East)
! Clean map  min=-0.0068028  max=5.0344 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0854+2006_X_2011_06_28_pus\_map.gif/vgif"
! Attempting to open device: 'J0854+2006_X_2011_06_28_pus_map.gif/vgif'
mapplot cln