! Started logfile: J0102+5824_X_1999_12_20_pus_uvs.log on Mon Dec 17 16:52:34 2007
obs J0102+5824_X_1999_12_20_pus_uva.fits
! Reading UV FITS file: J0102+5824_X_1999_12_20_pus_uva.fits
! AN table 1: 120 integrations on 190 of 190 possible baselines.
! AN table 2: 241 integrations on 190 of 190 possible baselines.
! AN table 3: 417 integrations on 190 of 190 possible baselines.
! AN table 4: 231 integrations on 190 of 190 possible baselines.
! Apparent sampling: 0.216567 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J0102+5824
! 
! 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 2514 lines of history.
! 
! Reading 166072 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 J0102+5824_X_1999_12_20_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 1149 telescope corrections were flagged in sub-array 1.
!  A total of 3091 telescope corrections were flagged in sub-array 2.
!  A total of 5747 telescope corrections were flagged in sub-array 3.
!  A total of 2987 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 2.
!  A total of 1149 telescope corrections were flagged in sub-array 1.
!  A total of 3091 telescope corrections were flagged in sub-array 2.
!  A total of 5727 telescope corrections were flagged in sub-array 3.
!  A total of 2979 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 3.
!  A total of 1149 telescope corrections were flagged in sub-array 1.
!  A total of 3087 telescope corrections were flagged in sub-array 2.
!  A total of 5737 telescope corrections were flagged in sub-array 3.
!  A total of 2987 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 4.
!  A total of 1149 telescope corrections were flagged in sub-array 1.
!  A total of 3087 telescope corrections were flagged in sub-array 2.
!  A total of 5737 telescope corrections were flagged in sub-array 3.
!  A total of 2980 telescope corrections were flagged in sub-array 4.
! 
! Fit before self-cal, rms=0.988790Jy  sigma=0.008974
! Fit after  self-cal, rms=0.744293Jy  sigma=0.006589
! 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 3.75% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! Estimated beam: bmin=0.5306 mas, bmaj=0.5784 mas, bpa=-9.366 degrees
! Estimated noise=400.153 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 = 0.205206 Jy
! Component: 100  -  total flux cleaned = 0.262081 Jy
! Total flux subtracted in 100 components = 0.262081 Jy
! Clean residual min=-0.004853 max=0.027203 Jy/beam
! Clean residual mean=0.000090 rms=0.001629 Jy/beam
! Combined flux in latest and established models = 0.26208 Jy
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 6 components and 0.26208 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.266866Jy  sigma=0.001599
! Fit after  self-cal, rms=0.266663Jy  sigma=0.001598
! Inverting map 
! Your choice of large map pixels excluded 3.75% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0328596 Jy
! Component: 100  -  total flux cleaned = 0.0541634 Jy
! Total flux subtracted in 100 components = 0.0541634 Jy
! Clean residual min=-0.004072 max=0.014360 Jy/beam
! Clean residual mean=0.000065 rms=0.001256 Jy/beam
! Combined flux in latest and established models = 0.316244 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 14 components and 0.316244 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.257299Jy  sigma=0.001437
! Fit after  self-cal, rms=0.257095Jy  sigma=0.001436
! Inverting map 
! Your choice of large map pixels excluded 3.75% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! Added new window around map position (-0.6, -0.6).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0179198 Jy
! Component: 100  -  total flux cleaned = 0.0317726 Jy
! Total flux subtracted in 100 components = 0.0317726 Jy
! Clean residual min=-0.003817 max=0.008312 Jy/beam
! Clean residual mean=0.000049 rms=0.001098 Jy/beam
! Combined flux in latest and established models = 0.348017 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 21 components and 0.348017 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.253626Jy  sigma=0.001370
! Fit after  self-cal, rms=0.253484Jy  sigma=0.001369
! Inverting map 
! Your choice of large map pixels excluded 3.75% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0120865 Jy
! Component: 100  -  total flux cleaned = 0.0217322 Jy
! Total flux subtracted in 100 components = 0.0217322 Jy
! Clean residual min=-0.003698 max=0.005818 Jy/beam
! Clean residual mean=0.000039 rms=0.001012 Jy/beam
! Combined flux in latest and established models = 0.369749 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 23 components and 0.369749 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.251758Jy  sigma=0.001334
! Fit after  self-cal, rms=0.251683Jy  sigma=0.001334
! Inverting map 
! Your choice of large map pixels excluded 3.75% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00854644 Jy
! Component: 100  -  total flux cleaned = 0.015437 Jy
! Total flux subtracted in 100 components = 0.015437 Jy
! Clean residual min=-0.003615 max=0.004717 Jy/beam
! Clean residual mean=0.000031 rms=0.000965 Jy/beam
! Combined flux in latest and established models = 0.385186 Jy
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 25 components and 0.385186 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.250763Jy  sigma=0.001315
! Fit after  self-cal, rms=0.250720Jy  sigma=0.001314
! Inverting map 
! Your choice of large map pixels excluded 3.75% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 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 3.75% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! Estimated beam: bmin=0.6588 mas, bmaj=0.7506 mas, bpa=8.336 degrees
! Estimated noise=207.952 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 = 0.0193363 Jy
! Component: 100  -  total flux cleaned = 0.0313408 Jy
! Component: 150  -  total flux cleaned = 0.0390765 Jy
! Component: 200  -  total flux cleaned = 0.0441313 Jy
! Total flux subtracted in 200 components = 0.0441313 Jy
! Clean residual min=-0.002243 max=0.008143 Jy/beam
! Clean residual mean=0.000385 rms=0.001013 Jy/beam
! Combined flux in latest and established models = 0.429317 Jy
! Performing phase self-cal
! Adding 26 model components to the UV plane model.
! The established model now contains 35 components and 0.429317 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.249465Jy  sigma=0.001285
! Fit after  self-cal, rms=0.249335Jy  sigma=0.001284
! Inverting map 
! Your choice of large map pixels excluded 3.75% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! Added new window around map position (-1.6, -1).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00847125 Jy
! Component: 100  -  total flux cleaned = 0.0134025 Jy
! Component: 150  -  total flux cleaned = 0.0167524 Jy
! Component: 200  -  total flux cleaned = 0.0191331 Jy
! Total flux subtracted in 200 components = 0.0191331 Jy
! Clean residual min=-0.002261 max=0.004056 Jy/beam
! Clean residual mean=0.000165 rms=0.000739 Jy/beam
! Combined flux in latest and established models = 0.44845 Jy
! Performing phase self-cal
! Adding 30 model components to the UV plane model.
! The established model now contains 64 components and 0.44845 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.249059Jy  sigma=0.001278
! Fit after  self-cal, rms=0.249011Jy  sigma=0.001277
! Inverting map 
! Your choice of large map pixels excluded 3.75% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 48 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.04     FD        1.01     GC        1.02     HH        1.00*    
!   HN        1.09     KK        0.96     KP        1.01     LA        1.00     
!   MC        1.20     MK        1.02     NY        1.00     ON        0.96     
!   OV        1.00     PT        1.00     SC        1.29     TS        0.99     
!   WF        1.04     WZ        1.10     GN        1.03     NL        1.00     
! 
!  A total of 48 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.20     FD        1.00     GC        1.03     HH        1.00*    
!   HN        1.06     KK        1.03     KP        0.99     LA        0.99     
!   MC        1.03     MK        1.03     NY        0.97     ON        0.98     
!   OV        1.01     PT        1.00     SC        1.08     TS        1.09     
!   WF        1.01     WZ        0.95     GN        1.01     NL        0.97     
! 
!  A total of 60 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.98     FD        1.00     GC        1.04     HH        1.00*    
!   HN        1.02     KK        1.05     KP        0.99     LA        0.99     
!   MC        1.05     MK        1.01     NY        0.98     ON        0.94     
!   OV        0.98     PT        0.99     SC        1.02     TS        1.01     
!   WF        1.02     WZ        0.99     GN        1.03     NL        1.00     
! 
!  A total of 48 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        0.97     FD        1.01     GC        0.92     HH        1.00*    
!   HN        0.94     KK        1.03     KP        1.06     LA        1.01     
!   MC        0.95     MK        1.04     NY        1.00     ON        0.97     
!   OV        1.02     PT        1.02     SC        1.11     TS        0.94     
!   WF        0.90     WZ        0.92     GN        1.04     NL        1.04     
! 
! 
! Correcting IF 2.
!  A total of 48 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.02     FD        1.01     GC        0.99     HH        1.00*    
!   HN        1.07     KK        0.99     KP        0.97     LA        1.01     
!   MC        1.17     MK        1.02     NY        0.98     ON        0.97     
!   OV        1.00     PT        0.99     SC        1.26     TS        0.99     
!   WF        1.05     WZ        1.04     GN        1.02     NL        1.00     
! 
!  A total of 48 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.20     FD        1.01     GC        0.98     HH        1.00*    
!   HN        1.04     KK        1.05     KP        0.96     LA        0.99     
!   MC        1.06     MK        1.02     NY        0.98     ON        0.95     
!   OV        1.00     PT        1.00     SC        1.02     TS        1.09     
!   WF        1.00     WZ        0.94     GN        0.98     NL        0.96     
! 
!  A total of 81 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.97     FD        1.00     GC        0.97     HH        1.00*    
!   HN        1.00     KK        1.21     KP        0.94     LA        1.00     
!   MC        1.04     MK        1.03     NY        0.98     ON        0.92     
!   OV        0.99     PT        0.99     SC        0.95     TS        1.11     
!   WF        1.01     WZ        0.96     GN        1.05     NL        0.98     
! 
!  A total of 45 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        0.96     FD        1.00     GC        0.96     HH        1.00*    
!   HN        0.92     KK        0.98     KP        1.02     LA        1.01     
!   MC        0.92     MK        1.02     NY        0.99     ON        0.93     
!   OV        1.01     PT        1.01     SC        1.04     TS        0.94     
!   WF        0.94     WZ        0.91     GN        1.05     NL        1.04     
! 
! 
! Correcting IF 3.
!  A total of 48 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.98     FD        1.01     GC        1.04     HH        1.00*    
!   HN        1.09     KK        0.99     KP        0.98     LA        1.01     
!   MC        1.14     MK        0.98     NY        0.91     ON        0.98     
!   OV        0.98     PT        1.00     SC        1.23     TS        0.96     
!   WF        1.04     WZ        1.02     GN        1.04     NL        0.98     
! 
!  A total of 42 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.96     FD        0.99     GC        1.03     HH        1.00*    
!   HN        1.07     KK        0.98     KP        0.96     LA        0.97     
!   MC        1.00     MK        1.00     NY        0.95     ON        0.97     
!   OV        0.99     PT        1.00     SC        0.99     TS        1.08     
!   WF        1.02     WZ        0.92     GN        0.98     NL        0.97     
! 
!  A total of 60 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.95     FD        1.00     GC        1.01     HH        1.00*    
!   HN        1.01     KK        1.04     KP        0.96     LA        0.98     
!   MC        1.00     MK        1.02     NY        0.94     ON        0.94     
!   OV        0.97     PT        0.99     SC        0.94     TS        0.92     
!   WF        0.97     WZ        0.98     GN        1.03     NL        0.99     
! 
!  A total of 48 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        0.94     FD        0.99     GC        0.93     HH        1.00*    
!   HN        0.92     KK        0.99     KP        1.05     LA        1.01     
!   MC        0.89     MK        1.03     NY        0.94     ON        0.98     
!   OV        1.01     PT        1.00     SC        0.99     TS        0.93     
!   WF        0.91     WZ        0.92     GN        1.04     NL        1.04     
! 
! 
! Correcting IF 4.
!  A total of 48 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.02     FD        1.00     GC        1.02     HH        1.00*    
!   HN        1.12     KK        0.94     KP        0.97     LA        1.00     
!   MC        1.18     MK        0.95     NY        0.98     ON        0.93     
!   OV        0.98     PT        1.00     SC        1.27     TS        0.95     
!   WF        1.04     WZ        1.05     GN        1.04     NL        0.98     
! 
!  A total of 42 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        0.98     GC        1.04     HH        1.00*    
!   HN        1.11     KK        0.98     KP        0.95     LA        0.99     
!   MC        1.05     MK        0.96     NY        0.96     ON        0.94     
!   OV        1.00     PT        1.00     SC        0.97     TS        1.06     
!   WF        1.00     WZ        0.91     GN        0.98     NL        0.98     
! 
!  A total of 60 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.97     FD        1.01     GC        1.02     HH        1.00*    
!   HN        1.04     KK        1.01     KP        0.94     LA        0.99     
!   MC        1.00     MK        0.99     NY        0.97     ON        0.92     
!   OV        0.98     PT        0.98     SC        0.94     TS        1.13     
!   WF        0.99     WZ        0.95     GN        1.03     NL        1.00     
! 
!  A total of 45 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        0.96     FD        0.98     GC        1.00     HH        1.00*    
!   HN        0.94     KK        0.93     KP        1.03     LA        1.02     
!   MC        0.89     MK        1.01     NY        0.99     ON        0.95     
!   OV        1.00     PT        0.99     SC        1.03     TS        0.90     
!   WF        0.93     WZ        0.89     GN        1.03     NL        1.02     
! 
! 
! Fit before self-cal, rms=0.249011Jy  sigma=0.001277
! Fit after  self-cal, rms=0.243985Jy  sigma=0.001262
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! Estimated beam: bmin=0.6575 mas, bmaj=0.754 mas, bpa=7.79 degrees
! Estimated noise=207.775 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 (-3, -1.8).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0032152 Jy
! Component: 100  -  total flux cleaned = 0.00455248 Jy
! Component: 150  -  total flux cleaned = 0.00561325 Jy
! Component: 200  -  total flux cleaned = 0.00624604 Jy
! Total flux subtracted in 200 components = 0.00624604 Jy
! Clean residual min=-0.001873 max=0.001995 Jy/beam
! Clean residual mean=-0.000003 rms=0.000520 Jy/beam
! Combined flux in latest and established models = 0.454696 Jy
! Performing phase self-cal
! Adding 21 model components to the UV plane model.
! The established model now contains 78 components and 0.454696 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.243915Jy  sigma=0.001261
! Fit after  self-cal, rms=0.243910Jy  sigma=0.001261
! Inverting map 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 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=0.243910Jy  sigma=0.001261
! Fit after  self-cal, rms=0.264149Jy  sigma=0.001241
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! Estimated beam: bmin=0.6593 mas, bmaj=0.7549 mas, bpa=9.374 degrees
! Estimated noise=209.004 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00175937 Jy
! Component: 100  -  total flux cleaned = 0.00218719 Jy
! Component: 150  -  total flux cleaned = 0.00249856 Jy
! Component: 200  -  total flux cleaned = 0.00272179 Jy
! Total flux subtracted in 200 components = 0.00272179 Jy
! Clean residual min=-0.001549 max=0.001129 Jy/beam
! Clean residual mean=0.000021 rms=0.000327 Jy/beam
! Combined flux in latest and established models = 0.457418 Jy
selfcal
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 89 components and 0.457418 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.264116Jy  sigma=0.001240
! Fit after  self-cal, rms=0.264336Jy  sigma=0.001240
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 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 = 0.000385121 Jy
! Component: 100  -  total flux cleaned = 0.000587594 Jy
! Component: 150  -  total flux cleaned = 0.000764017 Jy
! Component: 200  -  total flux cleaned = 0.000859147 Jy
! Total flux subtracted in 200 components = 0.000859147 Jy
! Clean residual min=-0.001559 max=0.001145 Jy/beam
! Clean residual mean=0.000009 rms=0.000323 Jy/beam
! Combined flux in latest and established models = 0.458277 Jy
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 91 components and 0.458277 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.264324Jy  sigma=0.001240
! Fit after  self-cal, rms=0.264323Jy  sigma=0.001240
! Inverting map 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 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=0.264323Jy  sigma=0.001240
! Fit after  self-cal, rms=0.268455Jy  sigma=0.001235
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! Estimated beam: bmin=0.6597 mas, bmaj=0.7549 mas, bpa=9.453 degrees
! Estimated noise=208.804 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -3.25513e-06 Jy
! Component: 100  -  total flux cleaned = 9.85735e-05 Jy
! Component: 150  -  total flux cleaned = 0.000188176 Jy
! Component: 200  -  total flux cleaned = 0.000295149 Jy
! Total flux subtracted in 200 components = 0.000295149 Jy
! Clean residual min=-0.001007 max=0.001124 Jy/beam
! Clean residual mean=0.000032 rms=0.000285 Jy/beam
! Combined flux in latest and established models = 0.458572 Jy
selfcal
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 92 components and 0.458572 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.268445Jy  sigma=0.001235
! Fit after  self-cal, rms=0.268461Jy  sigma=0.001235
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 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 = 6.26502e-06 Jy
! Component: 100  -  total flux cleaned = 0.000110529 Jy
! Component: 150  -  total flux cleaned = 0.000202327 Jy
! Component: 200  -  total flux cleaned = 0.000243791 Jy
! Total flux subtracted in 200 components = 0.000243791 Jy
! Clean residual min=-0.001030 max=0.001111 Jy/beam
! Clean residual mean=0.000029 rms=0.000283 Jy/beam
! Combined flux in latest and established models = 0.458816 Jy
! Performing phase self-cal
! Adding 21 model components to the UV plane model.
! The established model now contains 98 components and 0.458816 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.268457Jy  sigma=0.001235
! Fit after  self-cal, rms=0.268455Jy  sigma=0.001235
! Inverting map 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 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=0.268455Jy  sigma=0.001235
! Fit after  self-cal, rms=0.268368Jy  sigma=0.001235
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! Estimated beam: bmin=2.278 mas, bmaj=2.584 mas, bpa=82.33 degrees
! Estimated noise=329.295 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000462089 Jy
! Component: 100  -  total flux cleaned = 0.000570862 Jy
! Component: 150  -  total flux cleaned = 0.000648985 Jy
! Component: 200  -  total flux cleaned = 0.000685703 Jy
! Total flux subtracted in 200 components = 0.000685703 Jy
! Clean residual min=-0.000971 max=0.002210 Jy/beam
! Clean residual mean=0.000081 rms=0.000482 Jy/beam
! Combined flux in latest and established models = 0.459502 Jy
selfcal
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 104 components and 0.459502 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.268366Jy  sigma=0.001235
! Fit after  self-cal, rms=0.268366Jy  sigma=0.001235
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 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 (-7.2, -1.4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00204322 Jy
! Component: 100  -  total flux cleaned = 0.00263193 Jy
! Component: 150  -  total flux cleaned = 0.0028534 Jy
! Component: 200  -  total flux cleaned = 0.00287855 Jy
! Total flux subtracted in 200 components = 0.00287855 Jy
! Clean residual min=-0.000947 max=0.001351 Jy/beam
! Clean residual mean=-0.000050 rms=0.000371 Jy/beam
! Combined flux in latest and established models = 0.46238 Jy
! Performing phase self-cal
! Adding 42 model components to the UV plane model.
! The established model now contains 145 components and 0.46238 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.268357Jy  sigma=0.001235
! Fit after  self-cal, rms=0.268357Jy  sigma=0.001235
! Inverting map 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 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 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! Estimated beam: bmin=0.6598 mas, bmaj=0.7551 mas, bpa=9.643 degrees
! Estimated noise=208.759 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6598 x 0.7551 at 9.643 degrees (North through East)
! Clean map  min=-0.0007528  max=0.2943 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 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! Estimated beam: bmin=0.5326 mas, bmaj=0.5802 mas, bpa=-6.825 degrees
! Estimated noise=404.236 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.206078 Jy
! Component: 100  -  total flux cleaned = 0.267233 Jy
! Component: 150  -  total flux cleaned = 0.300586 Jy
! Component: 200  -  total flux cleaned = 0.324385 Jy
! Total flux subtracted in 200 components = 0.324385 Jy
! Clean residual min=-0.003044 max=0.013962 Jy/beam
! Clean residual mean=0.000066 rms=0.001011 Jy/beam
! Combined flux in latest and established models = 0.324385 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 13 model components to the UV plane model.
! The established model now contains 13 components and 0.324385 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! Estimated beam: bmin=0.6598 mas, bmaj=0.7551 mas, bpa=9.643 degrees
! Estimated noise=208.759 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 = 0.0433789 Jy
! Component: 100  -  total flux cleaned = 0.0692642 Jy
! Component: 150  -  total flux cleaned = 0.0861812 Jy
! Component: 200  -  total flux cleaned = 0.0979455 Jy
! Total flux subtracted in 200 components = 0.0979455 Jy
! Clean residual min=-0.001082 max=0.006795 Jy/beam
! Clean residual mean=0.000448 rms=0.000911 Jy/beam
! Combined flux in latest and established models = 0.42233 Jy
! Adding 45 model components to the UV plane model.
! The established model now contains 46 components and 0.42233 Jy
! Inverting map 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! Added new window around map position (0, -0.6).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00855592 Jy
! Component: 100  -  total flux cleaned = 0.0148673 Jy
! Component: 150  -  total flux cleaned = 0.0196148 Jy
! Component: 200  -  total flux cleaned = 0.0232602 Jy
! Total flux subtracted in 200 components = 0.0232602 Jy
! Clean residual min=-0.000846 max=0.002145 Jy/beam
! Clean residual mean=0.000180 rms=0.000429 Jy/beam
! Combined flux in latest and established models = 0.445591 Jy
! Adding 48 model components to the UV plane model.
! The established model now contains 80 components and 0.44559 Jy
! Inverting map 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00287308 Jy
! Component: 100  -  total flux cleaned = 0.005187 Jy
! Component: 150  -  total flux cleaned = 0.00710516 Jy
! Component: 200  -  total flux cleaned = 0.00872753 Jy
! Total flux subtracted in 200 components = 0.00872753 Jy
! Clean residual min=-0.000874 max=0.001081 Jy/beam
! Clean residual mean=0.000080 rms=0.000310 Jy/beam
! Combined flux in latest and established models = 0.454318 Jy
! Adding 59 model components to the UV plane model.
! The established model now contains 108 components and 0.454318 Jy
! Inverting map 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 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 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! Estimated beam: bmin=2.278 mas, bmaj=2.584 mas, bpa=82.33 degrees
! Estimated noise=329.295 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00347845 Jy
! Component: 100  -  total flux cleaned = 0.00536469 Jy
! Component: 150  -  total flux cleaned = 0.00654043 Jy
! Component: 200  -  total flux cleaned = 0.00716658 Jy
! Total flux subtracted in 200 components = 0.00716658 Jy
! Clean residual min=-0.001028 max=0.001354 Jy/beam
! Clean residual mean=-0.000008 rms=0.000394 Jy/beam
! Combined flux in latest and established models = 0.461484 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 = 0.000281507 Jy
! Component: 100  -  total flux cleaned = 0.000402984 Jy
! Component: 150  -  total flux cleaned = 0.000467801 Jy
! Component: 200  -  total flux cleaned = 0.000526163 Jy
! Total flux subtracted in 200 components = 0.000526163 Jy
! Clean residual min=-0.000997 max=0.001348 Jy/beam
! Clean residual mean=-0.000033 rms=0.000375 Jy/beam
! Combined flux in latest and established models = 0.462011 Jy
! Adding 95 model components to the UV plane model.
! The established model now contains 176 components and 0.462011 Jy
! Inverting map 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! Estimated beam: bmin=0.6598 mas, bmaj=0.7551 mas, bpa=9.643 degrees
! Estimated noise=208.759 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -1.26098e-06 Jy
! Component: 100  -  total flux cleaned = 9.81606e-05 Jy
! Component: 150  -  total flux cleaned = 0.000159171 Jy
! Component: 200  -  total flux cleaned = 0.000189036 Jy
! Total flux subtracted in 200 components = 0.000189036 Jy
! Clean residual min=-0.000864 max=0.001042 Jy/beam
! Clean residual mean=-0.000011 rms=0.000256 Jy/beam
! Combined flux in latest and established models = 0.4622 Jy
selfcal
! Performing phase self-cal
! Adding 33 model components to the UV plane model.
! The established model now contains 205 components and 0.4622 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.268341Jy  sigma=0.001235
! Fit after  self-cal, rms=0.268339Jy  sigma=0.001235
wmodel J0102+5824_X_1999_12_20_pus_map.mod
! Writing 205 model components to file: J0102+5824_X_1999_12_20_pus_map.mod
wobs J0102+5824_X_1999_12_20_pus_uvs.fits
! Writing UV FITS file: J0102+5824_X_1999_12_20_pus_uvs.fits
wwins J0102+5824_X_1999_12_20_pus_map.win
! wwins: Wrote 6 windows to J0102+5824_X_1999_12_20_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 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.000307778 Jy
! Component: 100  -  total flux cleaned = 0.00042117 Jy
! Component: 150  -  total flux cleaned = 0.000483397 Jy
! Component: 200  -  total flux cleaned = 0.000528908 Jy
! Component: 250  -  total flux cleaned = 0.000543875 Jy
! Component: 300  -  total flux cleaned = 0.000587997 Jy
! Component: 350  -  total flux cleaned = 0.000631323 Jy
! Component: 400  -  total flux cleaned = 0.000645542 Jy
! Component: 450  -  total flux cleaned = 0.000673681 Jy
! Component: 500  -  total flux cleaned = 0.000687511 Jy
! Component: 550  -  total flux cleaned = 0.000701256 Jy
! Component: 600  -  total flux cleaned = 0.000728417 Jy
! Component: 650  -  total flux cleaned = 0.000714899 Jy
! Component: 700  -  total flux cleaned = 0.00068831 Jy
! Component: 750  -  total flux cleaned = 0.000662031 Jy
! Component: 800  -  total flux cleaned = 0.000648998 Jy
! Component: 850  -  total flux cleaned = 0.000623111 Jy
! Component: 900  -  total flux cleaned = 0.000610257 Jy
! Component: 950  -  total flux cleaned = 0.000572092 Jy
! Component: 1000  -  total flux cleaned = 0.000559468 Jy
! Total flux subtracted in 1024 components = 0.000546898 Jy
! Clean residual min=-0.000693 max=0.000712 Jy/beam
! Clean residual mean=-0.000014 rms=0.000241 Jy/beam
! Combined flux in latest and established models = 0.462746 Jy
keep
! Adding 94 model components to the UV plane model.
! The established model now contains 298 components and 0.462746 Jy
![Exited script file: muppet]
wmap "J0102+5824_X_1999_12_20_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6598 x 0.7551 at 9.643 degrees (North through East)
! Clean map  min=-0.00075987  max=0.29504 Jy/beam
! Writing clean map to FITS file: J0102+5824_X_1999_12_20_pus_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.29504 
invert
! Inverting map 
! Your choice of large map pixels excluded 3.76% of the data.
!  The x-axis pixel size should ideally be below 0.1535 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1661 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000240613 
device "J0102+5824_X_1999_12_20_pus\_map.eps/VPS"
! Attempting to open device: 'J0102+5824_X_1999_12_20_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.244658 0.244658 0.489315 0.978631 1.95726 3.91452 7.82904 15.6581 31.3162 62.6324
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0007 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.295 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6598 x 0.7551 at 9.643 degrees (North through East)
! Clean map  min=-0.00075987  max=0.29504 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0102+5824_X_1999_12_20_pus\_map.gif/vgif"
! Attempting to open device: 'J0102+5824_X_1999_12_20_pus_map.gif/vgif'
mapplot cln
quit
! Quitting program
! Log file J0102+5824_X_1999_12_20_pus_uvs.log closed on Mon Dec 17 16:53:28 2007