! Started logfile: J0958+4725_X_2000_12_04_pus_uvs.log on Fri Oct 12 15:20:21 2007
obs J0958+4725_X_2000_12_04_pus_uva.fits
! Reading UV FITS file: J0958+4725_X_2000_12_04_pus_uva.fits
! AN table 1: 73 integrations on 190 of 190 possible baselines.
! AN table 2: 29 integrations on 190 of 190 possible baselines.
! AN table 3: 347 integrations on 190 of 190 possible baselines.
! AN table 4: 11 integrations on 190 of 190 possible baselines.
! Apparent sampling: 0.213627 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J0958+4725
! 
! 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 2126 lines of history.
! 
! Reading 74684 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 J0958+4725_X_2000_12_04_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 795 telescope corrections were flagged in sub-array 1.
!  A total of 265 telescope corrections were flagged in sub-array 2.
!  A total of 4045 telescope corrections were flagged in sub-array 3.
!  A total of 178 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 2.
!  A total of 795 telescope corrections were flagged in sub-array 1.
!  A total of 265 telescope corrections were flagged in sub-array 2.
!  A total of 4045 telescope corrections were flagged in sub-array 3.
!  A total of 178 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 3.
!  A total of 795 telescope corrections were flagged in sub-array 1.
!  A total of 265 telescope corrections were flagged in sub-array 2.
!  A total of 4045 telescope corrections were flagged in sub-array 3.
!  A total of 178 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 4.
!  A total of 795 telescope corrections were flagged in sub-array 1.
!  A total of 265 telescope corrections were flagged in sub-array 2.
!  A total of 4045 telescope corrections were flagged in sub-array 3.
!  A total of 178 telescope corrections were flagged in sub-array 4.
! 
! Fit before self-cal, rms=0.764039Jy  sigma=0.007587
! Fit after  self-cal, rms=0.204701Jy  sigma=0.001933
! 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 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! Estimated beam: bmin=0.5591 mas, bmaj=0.6477 mas, bpa=-2.532 degrees
! Estimated noise=589.814 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 = 0.743514 Jy
! Component: 100  -  total flux cleaned = 0.913275 Jy
! Total flux subtracted in 100 components = 0.913275 Jy
! Clean residual min=-0.015575 max=0.064385 Jy/beam
! Clean residual mean=0.000233 rms=0.004355 Jy/beam
! Combined flux in latest and established models = 0.913275 Jy
! Performing phase self-cal
! Adding 3 model components to the UV plane model.
! The established model now contains 3 components and 0.913275 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.223870Jy  sigma=0.002267
! Fit after  self-cal, rms=0.223866Jy  sigma=0.002267
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0680755 Jy
! Component: 100  -  total flux cleaned = 0.109888 Jy
! Total flux subtracted in 100 components = 0.109888 Jy
! Clean residual min=-0.012676 max=0.023119 Jy/beam
! Clean residual mean=0.000089 rms=0.003055 Jy/beam
! Combined flux in latest and established models = 1.02316 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 11 components and 1.02316 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.186055Jy  sigma=0.001712
! Fit after  self-cal, rms=0.186047Jy  sigma=0.001712
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0295704 Jy
! Component: 100  -  total flux cleaned = 0.0506657 Jy
! Total flux subtracted in 100 components = 0.0506657 Jy
! Clean residual min=-0.011166 max=0.012938 Jy/beam
! Clean residual mean=0.000024 rms=0.002694 Jy/beam
! Combined flux in latest and established models = 1.07383 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 11 components and 1.07383 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.177736Jy  sigma=0.001566
! Fit after  self-cal, rms=0.177736Jy  sigma=0.001566
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 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 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! Estimated beam: bmin=0.7415 mas, bmaj=0.9009 mas, bpa=2.994 degrees
! Estimated noise=255.587 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 = 0.0259104 Jy
! Component: 100  -  total flux cleaned = 0.0375012 Jy
! Component: 150  -  total flux cleaned = 0.0430084 Jy
! Component: 200  -  total flux cleaned = 0.045503 Jy
! Total flux subtracted in 200 components = 0.045503 Jy
! Clean residual min=-0.009295 max=0.008167 Jy/beam
! Clean residual mean=-0.000034 rms=0.002145 Jy/beam
! Combined flux in latest and established models = 1.11933 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 15 components and 1.11933 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.175810Jy  sigma=0.001509
! Fit after  self-cal, rms=0.175806Jy  sigma=0.001509
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 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        0.99     FD        1.00     GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        1.02     KK        0.99     KP        1.00     
!   LA        1.03     MA        1.00*    MC        1.00*    MK        0.96     
!   NL        1.01     NY        1.02     OV        0.97     PT        1.01     
!   SC        1.00*    TS        0.97     WF        1.04     WZ        0.99     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.01     FD        0.99     GC        1.12     GG        1.00*    
!   HH        1.00*    HN        0.98     KK        0.94     KP        1.00     
!   LA        0.99     MA        1.00*    MC        1.00*    MK        0.95     
!   NL        0.97     NY        0.99     OV        0.98     PT        1.00     
!   SC        1.29     TS        0.94     WF        0.98     WZ        1.12     
! 
!  A total of 33 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.01     FD        0.97     GC        1.13     GG        1.00*    
!   HH        1.00*    HN        0.97     KK        0.76     KP        1.01     
!   LA        1.00     MA        1.05     MC        0.98     MK        1.01     
!   NL        1.02     NY        1.01     OV        1.01     PT        1.02     
!   SC        1.07     TS        1.04     WF        1.00     WZ        0.96     
! 
!  A total of 6 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        1.00*    GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        0.99     KK        1.00*    KP        1.00*    
!   LA        1.00*    MA        1.00*    MC        1.00*    MK        1.00*    
!   NL        1.00*    NY        1.01     OV        1.00*    PT        1.00*    
!   SC        1.20     TS        1.18     WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        1.01     GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        1.02     KK        0.95     KP        1.00     
!   LA        1.03     MA        1.00*    MC        1.00*    MK        0.96     
!   NL        0.97     NY        1.02     OV        0.97     PT        1.01     
!   SC        1.00*    TS        0.97     WF        1.05     WZ        0.98     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        0.99     GC        1.11     GG        1.00*    
!   HH        1.00*    HN        0.98     KK        0.92     KP        1.01     
!   LA        0.97     MA        1.00*    MC        1.00*    MK        0.95     
!   NL        0.93     NY        0.99     OV        0.97     PT        1.00     
!   SC        1.32     TS        0.93     WF        1.00     WZ        1.13     
! 
!  A total of 33 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.01     FD        0.97     GC        1.13     GG        1.00*    
!   HH        1.00*    HN        0.98     KK        0.83     KP        1.01     
!   LA        0.99     MA        1.06     MC        0.99     MK        1.01     
!   NL        0.97     NY        1.00     OV        1.01     PT        1.02     
!   SC        1.07     TS        1.04     WF        0.99     WZ        0.97     
! 
!  A total of 6 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        1.00*    GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        0.98     KK        1.00*    KP        1.00*    
!   LA        1.00*    MA        1.00*    MC        1.00*    MK        1.00*    
!   NL        1.00*    NY        1.02     OV        1.00*    PT        1.00*    
!   SC        1.29     TS        1.19     WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.96     FD        1.05     GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        1.03     KK        0.94     KP        0.99     
!   LA        1.04     MA        1.00*    MC        1.00*    MK        0.97     
!   NL        0.96     NY        1.03     OV        0.93     PT        0.97     
!   SC        1.00*    TS        1.03     WF        1.03     WZ        1.02     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.99     FD        1.02     GC        1.12     GG        1.00*    
!   HH        1.00*    HN        0.99     KK        0.91     KP        1.01     
!   LA        0.98     MA        1.00*    MC        1.00*    MK        0.96     
!   NL        0.92     NY        0.98     OV        0.94     PT        0.96     
!   SC        1.34     TS        0.96     WF        0.99     WZ        1.13     
! 
!  A total of 33 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.99     FD        1.01     GC        1.13     GG        1.00*    
!   HH        1.00*    HN        0.98     KK        0.98     KP        1.00     
!   LA        1.00     MA        1.05     MC        0.99     MK        1.01     
!   NL        0.97     NY        1.01     OV        0.97     PT        0.99     
!   SC        1.08     TS        1.08     WF        0.99     WZ        0.99     
! 
!  A total of 6 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        1.00*    GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        0.99     KK        1.00*    KP        1.00*    
!   LA        1.00*    MA        1.00*    MC        1.00*    MK        1.00*    
!   NL        1.00*    NY        1.03     OV        1.00*    PT        1.00*    
!   SC        1.30     TS        1.19     WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.01     FD        1.04     GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        0.99     KK        0.96     KP        1.00     
!   LA        1.02     MA        1.00*    MC        1.00*    MK        0.94     
!   NL        0.96     NY        1.03     OV        0.96     PT        0.96     
!   SC        1.00*    TS        1.04     WF        1.07     WZ        1.03     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.02     FD        1.01     GC        1.15     GG        1.00*    
!   HH        1.00*    HN        0.95     KK        0.94     KP        1.00     
!   LA        0.97     MA        1.00*    MC        1.00*    MK        0.94     
!   NL        0.93     NY        0.97     OV        0.96     PT        0.95     
!   SC        1.32     TS        0.97     WF        0.95     WZ        1.12     
! 
!  A total of 33 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.03     FD        1.00     GC        1.13     GG        1.00*    
!   HH        1.00*    HN        0.93     KK        1.00     KP        1.00     
!   LA        0.99     MA        1.06     MC        1.02     MK        0.98     
!   NL        0.98     NY        0.99     OV        1.00     PT        0.97     
!   SC        1.07     TS        1.08     WF        1.00     WZ        0.99     
! 
!  A total of 6 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        1.00*    GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        0.97     KK        1.00*    KP        1.00*    
!   LA        1.00*    MA        1.00*    MC        1.00*    MK        1.00*    
!   NL        1.00*    NY        1.01     OV        1.00*    PT        1.00*    
!   SC        1.23     TS        1.24     WF        1.00*    WZ        1.00*    
! 
! 
! Fit before self-cal, rms=0.175806Jy  sigma=0.001509
! Fit after  self-cal, rms=0.171059Jy  sigma=0.001402
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! Estimated beam: bmin=0.7434 mas, bmaj=0.9077 mas, bpa=1.992 degrees
! Estimated noise=256.048 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 = -0.00456551 Jy
! Component: 100  -  total flux cleaned = -0.00509858 Jy
! Component: 150  -  total flux cleaned = -0.00543683 Jy
! Component: 200  -  total flux cleaned = -0.00580304 Jy
! Total flux subtracted in 200 components = -0.00580304 Jy
! Clean residual min=-0.008753 max=0.006515 Jy/beam
! Clean residual mean=0.000049 rms=0.001785 Jy/beam
! Combined flux in latest and established models = 1.11353 Jy
! Performing phase self-cal
! Adding 3 model components to the UV plane model.
! The established model now contains 17 components and 1.11353 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.170797Jy  sigma=0.001401
! Fit after  self-cal, rms=0.170852Jy  sigma=0.001401
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 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=0.170852Jy  sigma=0.001401
! Fit after  self-cal, rms=0.166574Jy  sigma=0.001318
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! Estimated beam: bmin=0.7434 mas, bmaj=0.9101 mas, bpa=1.207 degrees
! Estimated noise=256.236 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00160124 Jy
! Component: 100  -  total flux cleaned = -0.00173959 Jy
! Component: 150  -  total flux cleaned = -0.00174404 Jy
! Component: 200  -  total flux cleaned = -0.00184327 Jy
! Total flux subtracted in 200 components = -0.00184327 Jy
! Clean residual min=-0.003474 max=0.003382 Jy/beam
! Clean residual mean=0.000061 rms=0.000554 Jy/beam
! Combined flux in latest and established models = 1.11169 Jy
selfcal
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 23 components and 1.11169 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.166392Jy  sigma=0.001316
! Fit after  self-cal, rms=0.166417Jy  sigma=0.001316
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 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 = -7.44509e-05 Jy
! Component: 100  -  total flux cleaned = -0.000147402 Jy
! Component: 150  -  total flux cleaned = -0.00014443 Jy
! Component: 200  -  total flux cleaned = -0.000202934 Jy
! Total flux subtracted in 200 components = -0.000202934 Jy
! Clean residual min=-0.003016 max=0.003447 Jy/beam
! Clean residual mean=0.000063 rms=0.000547 Jy/beam
! Combined flux in latest and established models = 1.11148 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 24 components and 1.11148 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.166365Jy  sigma=0.001315
! Fit after  self-cal, rms=0.166362Jy  sigma=0.001315
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! Added new window around map position (0.4, -1).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00224184 Jy
! Component: 100  -  total flux cleaned = 0.0022499 Jy
! Component: 150  -  total flux cleaned = 0.00217823 Jy
! Component: 200  -  total flux cleaned = 0.00217539 Jy
! Total flux subtracted in 200 components = 0.00217539 Jy
! Clean residual min=-0.002934 max=0.001908 Jy/beam
! Clean residual mean=0.000038 rms=0.000506 Jy/beam
! Combined flux in latest and established models = 1.11366 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 35 components and 1.11366 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.166241Jy  sigma=0.001314
! Fit after  self-cal, rms=0.166232Jy  sigma=0.001314
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 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=0.166232Jy  sigma=0.001314
! Fit after  self-cal, rms=0.166494Jy  sigma=0.001312
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! Estimated beam: bmin=0.7438 mas, bmaj=0.9114 mas, bpa=0.7466 degrees
! Estimated noise=256.389 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000962574 Jy
! Component: 100  -  total flux cleaned = -0.000876237 Jy
! Component: 150  -  total flux cleaned = -0.000714478 Jy
! Component: 200  -  total flux cleaned = -0.000643357 Jy
! Total flux subtracted in 200 components = -0.000643357 Jy
! Clean residual min=-0.003251 max=0.001737 Jy/beam
! Clean residual mean=0.000032 rms=0.000484 Jy/beam
! Combined flux in latest and established models = 1.11301 Jy
selfcal
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 37 components and 1.11301 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.166395Jy  sigma=0.001312
! Fit after  self-cal, rms=0.166394Jy  sigma=0.001312
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 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 = 0.000226319 Jy
! Component: 100  -  total flux cleaned = 0.00022394 Jy
! Component: 150  -  total flux cleaned = 0.000226849 Jy
! Component: 200  -  total flux cleaned = 0.000287384 Jy
! Total flux subtracted in 200 components = 0.000287384 Jy
! Clean residual min=-0.003037 max=0.001649 Jy/beam
! Clean residual mean=0.000029 rms=0.000474 Jy/beam
! Combined flux in latest and established models = 1.1133 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 37 components and 1.1133 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.166339Jy  sigma=0.001311
! Fit after  self-cal, rms=0.166338Jy  sigma=0.001311
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 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=0.166338Jy  sigma=0.001311
! Fit after  self-cal, rms=0.166520Jy  sigma=0.001311
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! Estimated beam: bmin=2.474 mas, bmaj=2.792 mas, bpa=42.52 degrees
! Estimated noise=345.598 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000709466 Jy
! Component: 100  -  total flux cleaned = -0.000711661 Jy
! Component: 150  -  total flux cleaned = -0.000713206 Jy
! Component: 200  -  total flux cleaned = -0.000713641 Jy
! Total flux subtracted in 200 components = -0.000713641 Jy
! Clean residual min=-0.001625 max=0.001929 Jy/beam
! Clean residual mean=0.000073 rms=0.000528 Jy/beam
! Combined flux in latest and established models = 1.11259 Jy
selfcal
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 40 components and 1.11259 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.166509Jy  sigma=0.001311
! Fit after  self-cal, rms=0.166506Jy  sigma=0.001311
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 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 = 0.000107204 Jy
! Component: 100  -  total flux cleaned = 0.000145686 Jy
! Component: 150  -  total flux cleaned = 0.000166112 Jy
! Component: 200  -  total flux cleaned = 0.000175209 Jy
! Total flux subtracted in 200 components = 0.000175209 Jy
! Clean residual min=-0.001643 max=0.001869 Jy/beam
! Clean residual mean=0.000068 rms=0.000526 Jy/beam
! Combined flux in latest and established models = 1.11276 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 44 components and 1.11276 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.166511Jy  sigma=0.001311
! Fit after  self-cal, rms=0.166511Jy  sigma=0.001311
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 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 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! Estimated beam: bmin=0.7444 mas, bmaj=0.9121 mas, bpa=0.5409 degrees
! Estimated noise=256.464 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7444 x 0.9121 at 0.5409 degrees (North through East)
! Clean map  min=-0.0018956  max=1.0145 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=0.166511Jy  sigma=0.001311
! Fit after  self-cal, rms=0.205128Jy  sigma=0.001184
! Inverting map and beam 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! Estimated beam: bmin=0.7438 mas, bmaj=0.9134 mas, bpa=0.5798 degrees
! Estimated noise=256.124 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 1.58509e-05 Jy
! Component: 100  -  total flux cleaned = -0.000186014 Jy
! Component: 150  -  total flux cleaned = -0.000248794 Jy
! Component: 200  -  total flux cleaned = -0.000362317 Jy
! Total flux subtracted in 200 components = -0.000362317 Jy
! Clean residual min=-0.002316 max=0.001499 Jy/beam
! Clean residual mean=0.000012 rms=0.000373 Jy/beam
! Combined flux in latest and established models = 1.1124 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 46 components and 1.1124 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.205070Jy  sigma=0.001183
! Fit after  self-cal, rms=0.205075Jy  sigma=0.001183
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -5.67581e-05 Jy
! Component: 100  -  total flux cleaned = -0.000105129 Jy
! Component: 150  -  total flux cleaned = -0.000104729 Jy
! Component: 200  -  total flux cleaned = -0.000106502 Jy
! Total flux subtracted in 200 components = -0.000106502 Jy
! Clean residual min=-0.002019 max=0.001431 Jy/beam
! Clean residual mean=0.000014 rms=0.000367 Jy/beam
! Combined flux in latest and established models = 1.11229 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 49 components and 1.11229 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.205046Jy  sigma=0.001183
! Fit after  self-cal, rms=0.205047Jy  sigma=0.001183
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.205047Jy  sigma=0.001183
! Fit after  self-cal, rms=0.204971Jy  sigma=0.001183
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 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! Estimated beam: bmin=0.5591 mas, bmaj=0.6576 mas, bpa=-7.129 degrees
! Estimated noise=601.98 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.757936 Jy
! Component: 100  -  total flux cleaned = 0.924972 Jy
! Component: 150  -  total flux cleaned = 0.984743 Jy
! Component: 200  -  total flux cleaned = 1.02095 Jy
! Total flux subtracted in 200 components = 1.02095 Jy
! Clean residual min=-0.004593 max=0.019761 Jy/beam
! Clean residual mean=0.000115 rms=0.001611 Jy/beam
! Combined flux in latest and established models = 1.02095 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 1.02095 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! Estimated beam: bmin=0.7435 mas, bmaj=0.914 mas, bpa=0.5115 degrees
! Estimated noise=256.109 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 = 0.0459638 Jy
! Component: 100  -  total flux cleaned = 0.0672685 Jy
! Component: 150  -  total flux cleaned = 0.0776794 Jy
! Component: 200  -  total flux cleaned = 0.0832143 Jy
! Total flux subtracted in 200 components = 0.0832143 Jy
! Clean residual min=-0.001654 max=0.002839 Jy/beam
! Clean residual mean=0.000103 rms=0.000494 Jy/beam
! Combined flux in latest and established models = 1.10417 Jy
! Adding 29 model components to the UV plane model.
! The established model now contains 33 components and 1.10417 Jy
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! Added new window around map position (0.2, 0.6).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00330179 Jy
! Component: 100  -  total flux cleaned = 0.00535289 Jy
! Component: 150  -  total flux cleaned = 0.00584059 Jy
! Component: 200  -  total flux cleaned = 0.00610533 Jy
! Total flux subtracted in 200 components = 0.00610533 Jy
! Clean residual min=-0.001702 max=0.001459 Jy/beam
! Clean residual mean=0.000031 rms=0.000366 Jy/beam
! Combined flux in latest and established models = 1.11027 Jy
! Adding 22 model components to the UV plane model.
! The established model now contains 42 components and 1.11027 Jy
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 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 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! Estimated beam: bmin=2.474 mas, bmaj=2.792 mas, bpa=42.49 degrees
! Estimated noise=345.274 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00119667 Jy
! Component: 100  -  total flux cleaned = 0.00162143 Jy
! Component: 150  -  total flux cleaned = 0.00169548 Jy
! Component: 200  -  total flux cleaned = 0.00173743 Jy
! Total flux subtracted in 200 components = 0.00173743 Jy
! Clean residual min=-0.001604 max=0.001478 Jy/beam
! Clean residual mean=0.000032 rms=0.000448 Jy/beam
! Combined flux in latest and established models = 1.11201 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 = 2.9694e-05 Jy
! Component: 100  -  total flux cleaned = 5.01215e-05 Jy
! Component: 150  -  total flux cleaned = 6.32262e-05 Jy
! Component: 200  -  total flux cleaned = 6.95595e-05 Jy
! Total flux subtracted in 200 components = 6.95595e-05 Jy
! Clean residual min=-0.001610 max=0.001470 Jy/beam
! Clean residual mean=0.000030 rms=0.000446 Jy/beam
! Combined flux in latest and established models = 1.11208 Jy
! Adding 14 model components to the UV plane model.
! The established model now contains 52 components and 1.11208 Jy
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! Estimated beam: bmin=0.7435 mas, bmaj=0.914 mas, bpa=0.5115 degrees
! Estimated noise=256.109 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000342793 Jy
! Component: 100  -  total flux cleaned = -0.000343826 Jy
! Component: 150  -  total flux cleaned = -0.000305046 Jy
! Component: 200  -  total flux cleaned = -0.00030495 Jy
! Total flux subtracted in 200 components = -0.00030495 Jy
! Clean residual min=-0.001684 max=0.001283 Jy/beam
! Clean residual mean=0.000014 rms=0.000348 Jy/beam
! Combined flux in latest and established models = 1.11177 Jy
selfcal
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 55 components and 1.11177 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.204910Jy  sigma=0.001183
! Fit after  self-cal, rms=0.204903Jy  sigma=0.001183
wmodel J0958+4725_X_2000_12_04_pus_map.mod
! Writing 55 model components to file: J0958+4725_X_2000_12_04_pus_map.mod
wobs J0958+4725_X_2000_12_04_pus_uvs.fits
! Writing UV FITS file: J0958+4725_X_2000_12_04_pus_uvs.fits
wwins J0958+4725_X_2000_12_04_pus_map.win
! wwins: Wrote 3 windows to J0958+4725_X_2000_12_04_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 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000279077 Jy
! Component: 100  -  total flux cleaned = -9.61914e-05 Jy
! Component: 150  -  total flux cleaned = 5.46563e-05 Jy
! Component: 200  -  total flux cleaned = 0.00020044 Jy
! Component: 250  -  total flux cleaned = 0.000341693 Jy
! Component: 300  -  total flux cleaned = 0.000498844 Jy
! Component: 350  -  total flux cleaned = 0.000633275 Jy
! Component: 400  -  total flux cleaned = 0.000727327 Jy
! Component: 450  -  total flux cleaned = 0.000820021 Jy
! Component: 500  -  total flux cleaned = 0.000929473 Jy
! Component: 550  -  total flux cleaned = 0.00100126 Jy
! Component: 600  -  total flux cleaned = 0.00105421 Jy
! Component: 650  -  total flux cleaned = 0.00112374 Jy
! Component: 700  -  total flux cleaned = 0.001141 Jy
! Component: 750  -  total flux cleaned = 0.00120908 Jy
! Component: 800  -  total flux cleaned = 0.00127628 Jy
! Component: 850  -  total flux cleaned = 0.00132622 Jy
! Component: 900  -  total flux cleaned = 0.0013922 Jy
! Component: 950  -  total flux cleaned = 0.00142474 Jy
! Component: 1000  -  total flux cleaned = 0.0014572 Jy
! Total flux subtracted in 1024 components = 0.00145722 Jy
! Clean residual min=-0.000840 max=0.000937 Jy/beam
! Clean residual mean=-0.000004 rms=0.000301 Jy/beam
! Combined flux in latest and established models = 1.11323 Jy
keep
! Adding 83 model components to the UV plane model.
! The established model now contains 136 components and 1.11323 Jy
![Exited script file: muppet]
wmap "J0958+4725_X_2000_12_04_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7435 x 0.914 at 0.5115 degrees (North through East)
! Clean map  min=-0.0015949  max=1.014 Jy/beam
! Writing clean map to FITS file: J0958+4725_X_2000_12_04_pus_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 1.01403 
invert
! Inverting map 
! Your choice of large map pixels excluded 2.56% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1823 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000300602 
device "J0958+4725_X_2000_12_04_pus\_map.eps/VPS"
! Attempting to open device: 'J0958+4725_X_2000_12_04_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.0889334 0.0889334 0.177867 0.355734 0.711468 1.42294 2.84587 5.69174 11.3835 22.767 45.5339 91.0678
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0009 
print "peak=",int(1000*peak_flux)/1000
! peak= 1.014 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7435 x 0.914 at 0.5115 degrees (North through East)
! Clean map  min=-0.0015949  max=1.014 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0958+4725_X_2000_12_04_pus\_map.gif/vgif"
! Attempting to open device: 'J0958+4725_X_2000_12_04_pus_map.gif/vgif'
mapplot cln
quit
! Quitting program
! Log file J0958+4725_X_2000_12_04_pus_uvs.log closed on Fri Oct 12 15:20:41 2007