! Started logfile: J0555+3948_X_2003_07_09_pus_uvs.log on Sun Apr  7 11:55:26 2013
obs J0555+3948_X_2003_07_09_pus_uva.fits
! Reading UV FITS file: J0555+3948_X_2003_07_09_pus_uva.fits
! AN table 1: 80 integrations on 171 of 171 possible baselines.
! AN table 2: 34 integrations on 171 of 171 possible baselines.
! AN table 3: 189 integrations on 171 of 171 possible baselines.
! Apparent sampling: 0.208712 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J0555+3948
! Warning: Unknown AN-table MNTSTA value (3).
!          Will assume that it is ground-based.
! Warning: Unknown AN-table MNTSTA value (3).
!          Will assume that it is ground-based.
! Warning: Unknown AN-table MNTSTA value (3).
!          Will assume that it is ground-based.
! 
! 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 1875 lines of history.
! 
! Reading 43256 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 J0555+3948_X_2003_07_09_pus]
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.03
float dynam
dynam = 6.0
float soltime1
soltime1 = 120
float soltime2
soltime2 = 20
float thresh
thresh = 0.5
float win_mult
win_mult = 1.8
float time_av
time_av = 16
float old_peak
float new_peak
float flux_cutoff
mapsize field_size, field_cell
! Map grid = 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 686 telescope corrections were flagged in sub-array 1.
!  A total of 252 telescope corrections were flagged in sub-array 2.
!  A total of 2674 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 686 telescope corrections were flagged in sub-array 1.
!  A total of 252 telescope corrections were flagged in sub-array 2.
!  A total of 2674 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 686 telescope corrections were flagged in sub-array 1.
!  A total of 253 telescope corrections were flagged in sub-array 2.
!  A total of 2674 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 686 telescope corrections were flagged in sub-array 1.
!  A total of 252 telescope corrections were flagged in sub-array 2.
!  A total of 2677 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=2.534637Jy  sigma=0.023713
! Fit after  self-cal, rms=2.290659Jy  sigma=0.021682
! 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 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! Estimated beam: bmin=0.6235 mas, bmaj=1.087 mas, bpa=2.645 degrees
! Estimated noise=985.275 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 = 2.10244 Jy
! Component: 100  -  total flux cleaned = 2.8628 Jy
! Total flux subtracted in 100 components = 2.8628 Jy
! Clean residual min=-0.113641 max=0.443901 Jy/beam
! Clean residual mean=0.000790 rms=0.037140 Jy/beam
! Combined flux in latest and established models = 2.8628 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 10 components and 2.8628 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.942302Jy  sigma=0.009120
! Fit after  self-cal, rms=0.938879Jy  sigma=0.009095
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! Added new window around map position (-0.8, 0.2).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.482035 Jy
! Component: 100  -  total flux cleaned = 0.781048 Jy
! Total flux subtracted in 100 components = 0.781048 Jy
! Clean residual min=-0.068355 max=0.167349 Jy/beam
! Clean residual mean=0.000335 rms=0.019467 Jy/beam
! Combined flux in latest and established models = 3.64385 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 19 components and 3.64385 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.529899Jy  sigma=0.004992
! Fit after  self-cal, rms=0.521430Jy  sigma=0.004934
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.205898 Jy
! Component: 100  -  total flux cleaned = 0.3448 Jy
! Total flux subtracted in 100 components = 0.3448 Jy
! Clean residual min=-0.055358 max=0.080907 Jy/beam
! Clean residual mean=0.000144 rms=0.013142 Jy/beam
! Combined flux in latest and established models = 3.98865 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 29 components and 3.98865 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.395651Jy  sigma=0.003495
! Fit after  self-cal, rms=0.393340Jy  sigma=0.003478
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.104634 Jy
! Component: 100  -  total flux cleaned = 0.17993 Jy
! Total flux subtracted in 100 components = 0.17993 Jy
! Clean residual min=-0.048356 max=0.053251 Jy/beam
! Clean residual mean=0.000050 rms=0.010939 Jy/beam
! Combined flux in latest and established models = 4.16858 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 36 components and 4.16858 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.353387Jy  sigma=0.002951
! Fit after  self-cal, rms=0.351886Jy  sigma=0.002938
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 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 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! Estimated beam: bmin=0.7682 mas, bmaj=1.601 mas, bpa=-2.114 degrees
! Estimated noise=407.265 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 = 0.0961539 Jy
! Component: 100  -  total flux cleaned = 0.152868 Jy
! Component: 150  -  total flux cleaned = 0.189138 Jy
! Component: 200  -  total flux cleaned = 0.213003 Jy
! Total flux subtracted in 200 components = 0.213003 Jy
! Clean residual min=-0.059593 max=0.055394 Jy/beam
! Clean residual mean=-0.002960 rms=0.013113 Jy/beam
! Combined flux in latest and established models = 4.38158 Jy
! Performing phase self-cal
! Adding 30 model components to the UV plane model.
! The established model now contains 50 components and 4.38158 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.333392Jy  sigma=0.002610
! Fit after  self-cal, rms=0.332165Jy  sigma=0.002595
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 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        0.98     FD        0.98     GC        1.00*    GG        1.00*    
!   HN        1.07     KP        0.99     LA        0.96     MA        1.00*    
!   MK        0.99     NL        1.02     NY        1.00*    ON        1.00*    
!   OV        0.99     PT        0.98     SC        1.00     TC        1.00*    
!   TS        1.00*    WF        1.13     WZ        1.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.97     FD        0.97     GC        0.96     GG        1.00*    
!   HN        0.98     KP        0.90     LA        0.98     MA        1.00*    
!   MK        0.97     NL        1.09     NY        0.95     ON        1.09     
!   OV        0.98     PT        0.97     SC        1.07     TC        1.00*    
!   TS        0.96     WF        1.02     WZ        1.00*    
! 
!  A total of 12 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.97     FD        0.97     GC        1.00*    GG        1.00*    
!   HN        0.94     KP        0.92     LA        0.97     MA        1.00*    
!   MK        0.97     NL        1.08     NY        1.00*    ON        1.00*    
!   OV        0.99     PT        0.99     SC        0.99     TC        1.00*    
!   TS        1.00*    WF        1.02     WZ        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        0.98     GC        1.00*    GG        1.00*    
!   HN        1.09     KP        0.99     LA        0.96     MA        1.00*    
!   MK        1.00     NL        1.02     NY        1.00*    ON        1.00*    
!   OV        0.98     PT        1.03     SC        1.02     TC        1.00*    
!   TS        1.00*    WF        1.15     WZ        1.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.99     FD        0.97     GC        1.00     GG        1.00*    
!   HN        0.99     KP        0.86     LA        0.97     MA        1.00*    
!   MK        0.99     NL        1.06     NY        0.98     ON        1.09     
!   OV        0.98     PT        1.02     SC        1.04     TC        1.00*    
!   TS        0.97     WF        1.05     WZ        1.00*    
! 
!  A total of 12 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.99     FD        0.97     GC        1.00*    GG        1.00*    
!   HN        0.95     KP        0.89     LA        0.97     MA        1.00*    
!   MK        0.98     NL        1.06     NY        1.00*    ON        1.00*    
!   OV        0.98     PT        1.03     SC        0.97     TC        1.00*    
!   TS        1.00*    WF        1.05     WZ        1.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.04     FD        0.98     GC        1.00*    GG        1.00*    
!   HN        1.10     KP        1.00     LA        0.98     MA        1.00*    
!   MK        1.01     NL        1.07     NY        1.00*    ON        1.00*    
!   OV        1.03     PT        1.00     SC        1.00     TC        1.00*    
!   TS        1.00*    WF        1.12     WZ        1.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.03     FD        0.98     GC        1.15     GG        1.00*    
!   HN        0.99     KP        0.80     LA        1.00     MA        1.00*    
!   MK        0.99     NL        1.05     NY        1.01     ON        1.37     
!   OV        1.03     PT        1.06     SC        1.08     TC        1.00*    
!   TS        0.96     WF        1.12     WZ        1.00*    
! 
!  A total of 12 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.03     FD        0.97     GC        1.00*    GG        1.00*    
!   HN        0.95     KP        0.84     LA        0.98     MA        1.00*    
!   MK        0.99     NL        1.05     NY        1.00*    ON        1.00*    
!   OV        1.03     PT        1.05     SC        0.99     TC        1.00*    
!   TS        1.00*    WF        1.14     WZ        1.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.03     FD        0.97     GC        1.00*    GG        1.00*    
!   HN        1.14     KP        1.00     LA        0.97     MA        1.00*    
!   MK        1.03     NL        1.03     NY        1.00*    ON        1.00*    
!   OV        1.03     PT        1.01     SC        1.05     TC        1.00*    
!   TS        1.00*    WF        1.13     WZ        1.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.02     FD        0.97     GC        1.19     GG        1.00*    
!   HN        1.02     KP        0.87     LA        0.98     MA        1.00*    
!   MK        1.03     NL        1.05     NY        0.99     ON        1.48     
!   OV        1.02     PT        1.06     SC        1.14     TC        1.00*    
!   TS        0.99     WF        1.11     WZ        1.00*    
! 
!  A total of 9 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.01     FD        0.96     GC        1.00*    GG        1.00*    
!   HN        0.98     KP        0.89     LA        0.97     MA        1.00*    
!   MK        1.01     NL        1.05     NY        1.00*    ON        1.00*    
!   OV        1.03     PT        1.06     SC        1.05     TC        1.00*    
!   TS        1.00*    WF        1.13     WZ        1.00*    
! 
! 
! Fit before self-cal, rms=0.332165Jy  sigma=0.002595
! Fit after  self-cal, rms=0.199250Jy  sigma=0.001385
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! Estimated beam: bmin=0.7695 mas, bmaj=1.618 mas, bpa=-2.063 degrees
! Estimated noise=408.77 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 = -0.012506 Jy
! Component: 100  -  total flux cleaned = -0.0131983 Jy
! Component: 150  -  total flux cleaned = -0.0129386 Jy
! Component: 200  -  total flux cleaned = -0.0122289 Jy
! Total flux subtracted in 200 components = -0.0122289 Jy
! Clean residual min=-0.007261 max=0.009661 Jy/beam
! Clean residual mean=-0.000413 rms=0.001679 Jy/beam
! Combined flux in latest and established models = 4.36935 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 51 components and 4.36935 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.197302Jy  sigma=0.001371
! Fit after  self-cal, rms=0.197229Jy  sigma=0.001369
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! Added new window around map position (-2.2, 0.8).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00355432 Jy
! Component: 100  -  total flux cleaned = 0.00493435 Jy
! Component: 150  -  total flux cleaned = 0.00608581 Jy
! Component: 200  -  total flux cleaned = 0.00629095 Jy
! Total flux subtracted in 200 components = 0.00629095 Jy
! Clean residual min=-0.006941 max=0.006935 Jy/beam
! Clean residual mean=-0.000453 rms=0.001472 Jy/beam
! Combined flux in latest and established models = 4.37565 Jy
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 59 components and 4.37564 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.196387Jy  sigma=0.001363
! Fit after  self-cal, rms=0.196344Jy  sigma=0.001362
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 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=0.196344Jy  sigma=0.001362
! Fit after  self-cal, rms=0.196632Jy  sigma=0.001360
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! Estimated beam: bmin=0.7702 mas, bmaj=1.62 mas, bpa=-2.041 degrees
! Estimated noise=409.12 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00333882 Jy
! Component: 100  -  total flux cleaned = -0.0040304 Jy
! Component: 150  -  total flux cleaned = -0.00383241 Jy
! Component: 200  -  total flux cleaned = -0.00365093 Jy
! Total flux subtracted in 200 components = -0.00365093 Jy
! Clean residual min=-0.006383 max=0.006026 Jy/beam
! Clean residual mean=-0.000179 rms=0.001257 Jy/beam
! Combined flux in latest and established models = 4.37199 Jy
selfcal
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 64 components and 4.37199 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.195995Jy  sigma=0.001355
! Fit after  self-cal, rms=0.195955Jy  sigma=0.001355
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 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 = 0.00042149 Jy
! Component: 100  -  total flux cleaned = 0.000758251 Jy
! Component: 150  -  total flux cleaned = 0.00108532 Jy
! Component: 200  -  total flux cleaned = 0.00155332 Jy
! Total flux subtracted in 200 components = 0.00155332 Jy
! Clean residual min=-0.005908 max=0.005632 Jy/beam
! Clean residual mean=-0.000189 rms=0.001214 Jy/beam
! Combined flux in latest and established models = 4.37355 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 68 components and 4.37355 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.195621Jy  sigma=0.001353
! Fit after  self-cal, rms=0.195602Jy  sigma=0.001353
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 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=0.195602Jy  sigma=0.001353
! Fit after  self-cal, rms=0.195743Jy  sigma=0.001351
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! Estimated beam: bmin=0.7705 mas, bmaj=1.621 mas, bpa=-2.027 degrees
! Estimated noise=409.269 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00147948 Jy
! Component: 100  -  total flux cleaned = -0.0014795 Jy
! Component: 150  -  total flux cleaned = -0.00132499 Jy
! Component: 200  -  total flux cleaned = -0.00103618 Jy
! Total flux subtracted in 200 components = -0.00103618 Jy
! Clean residual min=-0.006166 max=0.005126 Jy/beam
! Clean residual mean=-0.000076 rms=0.001154 Jy/beam
! Combined flux in latest and established models = 4.37251 Jy
selfcal
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 69 components and 4.37251 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.195397Jy  sigma=0.001349
! Fit after  self-cal, rms=0.195374Jy  sigma=0.001349
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 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 = 0.000285457 Jy
! Component: 100  -  total flux cleaned = 0.000421649 Jy
! Component: 150  -  total flux cleaned = 0.000421876 Jy
! Component: 200  -  total flux cleaned = 0.000423761 Jy
! Total flux subtracted in 200 components = 0.000423761 Jy
! Clean residual min=-0.005628 max=0.004831 Jy/beam
! Clean residual mean=-0.000078 rms=0.001126 Jy/beam
! Combined flux in latest and established models = 4.37294 Jy
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 71 components and 4.37293 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.195154Jy  sigma=0.001347
! Fit after  self-cal, rms=0.195144Jy  sigma=0.001347
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 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=0.195144Jy  sigma=0.001347
! Fit after  self-cal, rms=0.195144Jy  sigma=0.001346
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! Estimated beam: bmin=2.074 mas, bmaj=2.635 mas, bpa=-10.51 degrees
! Estimated noise=536.594 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000144362 Jy
! Component: 100  -  total flux cleaned = 0.000305821 Jy
! Component: 150  -  total flux cleaned = 0.000554795 Jy
! Component: 200  -  total flux cleaned = 0.000747402 Jy
! Total flux subtracted in 200 components = 0.000747402 Jy
! Clean residual min=-0.004381 max=0.005425 Jy/beam
! Clean residual mean=-0.000112 rms=0.001190 Jy/beam
! Combined flux in latest and established models = 4.37368 Jy
selfcal
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 77 components and 4.37368 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.195101Jy  sigma=0.001346
! Fit after  self-cal, rms=0.195094Jy  sigma=0.001346
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 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 (-9, 8).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00140473 Jy
! Component: 100  -  total flux cleaned = 0.000402765 Jy
! Component: 150  -  total flux cleaned = -0.000279298 Jy
! Component: 200  -  total flux cleaned = -0.000644307 Jy
! Total flux subtracted in 200 components = -0.000644307 Jy
! Clean residual min=-0.003377 max=0.003638 Jy/beam
! Clean residual mean=-0.000100 rms=0.000954 Jy/beam
! Combined flux in latest and established models = 4.37304 Jy
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 94 components and 4.37304 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.195000Jy  sigma=0.001345
! Fit after  self-cal, rms=0.194996Jy  sigma=0.001345
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 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 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! Estimated beam: bmin=0.7706 mas, bmaj=1.622 mas, bpa=-2.023 degrees
! Estimated noise=409.373 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7706 x 1.622 at -2.023 degrees (North through East)
! Clean map  min=-0.0041642  max=3.011 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=0.194996Jy  sigma=0.001345
! Fit after  self-cal, rms=0.172472Jy  sigma=0.001164
! Inverting map and beam 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! Estimated beam: bmin=0.7707 mas, bmaj=1.622 mas, bpa=-2.027 degrees
! Estimated noise=409.095 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00240647 Jy
! Component: 100  -  total flux cleaned = -0.00268513 Jy
! Component: 150  -  total flux cleaned = -0.00294996 Jy
! Component: 200  -  total flux cleaned = -0.00307415 Jy
! Total flux subtracted in 200 components = -0.00307415 Jy
! Clean residual min=-0.005037 max=0.003220 Jy/beam
! Clean residual mean=-0.000162 rms=0.000873 Jy/beam
! Combined flux in latest and established models = 4.36996 Jy
! Performing phase self-cal
! Adding 24 model components to the UV plane model.
! The established model now contains 113 components and 4.36996 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.172232Jy  sigma=0.001162
! Fit after  self-cal, rms=0.172222Jy  sigma=0.001162
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000287583 Jy
! Component: 100  -  total flux cleaned = -0.000290371 Jy
! Component: 150  -  total flux cleaned = -0.00040022 Jy
! Component: 200  -  total flux cleaned = -0.000506666 Jy
! Total flux subtracted in 200 components = -0.000506666 Jy
! Clean residual min=-0.004599 max=0.003114 Jy/beam
! Clean residual mean=-0.000159 rms=0.000846 Jy/beam
! Combined flux in latest and established models = 4.36946 Jy
! Performing phase self-cal
! Adding 32 model components to the UV plane model.
! The established model now contains 121 components and 4.36946 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.172063Jy  sigma=0.001161
! Fit after  self-cal, rms=0.172056Jy  sigma=0.001161
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.172056Jy  sigma=0.001161
! Fit after  self-cal, rms=0.172100Jy  sigma=0.001161
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 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! Estimated beam: bmin=0.6213 mas, bmaj=1.11 mas, bpa=2.376 degrees
! Estimated noise=1005.57 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 2.13531 Jy
! Component: 100  -  total flux cleaned = 2.93756 Jy
! Component: 150  -  total flux cleaned = 3.38518 Jy
! Component: 200  -  total flux cleaned = 3.6754 Jy
! Total flux subtracted in 200 components = 3.6754 Jy
! Clean residual min=-0.041681 max=0.155793 Jy/beam
! Clean residual mean=0.000356 rms=0.015157 Jy/beam
! Combined flux in latest and established models = 3.6754 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 17 model components to the UV plane model.
! The established model now contains 17 components and 3.6754 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! Estimated beam: bmin=0.7709 mas, bmaj=1.622 mas, bpa=-2.022 degrees
! Estimated noise=409.125 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 = 0.279296 Jy
! Component: 100  -  total flux cleaned = 0.428146 Jy
! Component: 150  -  total flux cleaned = 0.514148 Jy
! Component: 200  -  total flux cleaned = 0.567961 Jy
! Total flux subtracted in 200 components = 0.567961 Jy
! Clean residual min=-0.011783 max=0.030776 Jy/beam
! Clean residual mean=0.000680 rms=0.004680 Jy/beam
! Combined flux in latest and established models = 4.24336 Jy
! Adding 40 model components to the UV plane model.
! The established model now contains 43 components and 4.24336 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! Added new window around map position (-0.8, 1.4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.035767 Jy
! Component: 100  -  total flux cleaned = 0.0600964 Jy
! Component: 150  -  total flux cleaned = 0.0771971 Jy
! Component: 200  -  total flux cleaned = 0.0859357 Jy
! Total flux subtracted in 200 components = 0.0859357 Jy
! Clean residual min=-0.007664 max=0.012951 Jy/beam
! Clean residual mean=0.000115 rms=0.001892 Jy/beam
! Combined flux in latest and established models = 4.32929 Jy
! Adding 28 model components to the UV plane model.
! The established model now contains 62 components and 4.32929 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! Added new window around map position (0.8, -0.2).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00884216 Jy
! Component: 100  -  total flux cleaned = 0.0121527 Jy
! Component: 150  -  total flux cleaned = 0.0155524 Jy
! Component: 200  -  total flux cleaned = 0.019327 Jy
! Total flux subtracted in 200 components = 0.019327 Jy
! Clean residual min=-0.006342 max=0.006626 Jy/beam
! Clean residual mean=-0.000009 rms=0.001433 Jy/beam
! Combined flux in latest and established models = 4.34862 Jy
! Adding 22 model components to the UV plane model.
! The established model now contains 78 components and 4.34862 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! Added new window around map position (-0.6, -1.4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00363266 Jy
! Component: 100  -  total flux cleaned = 0.00624877 Jy
! Component: 150  -  total flux cleaned = 0.00869129 Jy
! Component: 200  -  total flux cleaned = 0.0104755 Jy
! Total flux subtracted in 200 components = 0.0104755 Jy
! Clean residual min=-0.005466 max=0.004671 Jy/beam
! Clean residual mean=-0.000073 rms=0.001241 Jy/beam
! Combined flux in latest and established models = 4.35909 Jy
! Adding 29 model components to the UV plane model.
! The established model now contains 91 components and 4.35909 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 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 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! Estimated beam: bmin=2.074 mas, bmaj=2.635 mas, bpa=-10.46 degrees
! Estimated noise=536.081 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0058671 Jy
! Component: 100  -  total flux cleaned = 0.00752906 Jy
! Component: 150  -  total flux cleaned = 0.00764916 Jy
! Component: 200  -  total flux cleaned = 0.00754796 Jy
! Total flux subtracted in 200 components = 0.00754796 Jy
! Clean residual min=-0.003494 max=0.002947 Jy/beam
! Clean residual mean=-0.000340 rms=0.000933 Jy/beam
! Combined flux in latest and established models = 4.36664 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 = 2.84765e-06 Jy
! Component: 100  -  total flux cleaned = -0.000147591 Jy
! Component: 150  -  total flux cleaned = -0.00041962 Jy
! Component: 200  -  total flux cleaned = -0.000481887 Jy
! Total flux subtracted in 200 components = -0.000481887 Jy
! Clean residual min=-0.003209 max=0.002591 Jy/beam
! Clean residual mean=-0.000335 rms=0.000848 Jy/beam
! Combined flux in latest and established models = 4.36616 Jy
! Adding 56 model components to the UV plane model.
! The established model now contains 141 components and 4.36616 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! Estimated beam: bmin=0.7709 mas, bmaj=1.622 mas, bpa=-2.022 degrees
! Estimated noise=409.125 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00199196 Jy
! Component: 100  -  total flux cleaned = -0.00177609 Jy
! Component: 150  -  total flux cleaned = -0.00177707 Jy
! Component: 200  -  total flux cleaned = -0.00157374 Jy
! Total flux subtracted in 200 components = -0.00157374 Jy
! Clean residual min=-0.004628 max=0.003780 Jy/beam
! Clean residual mean=-0.000110 rms=0.001055 Jy/beam
! Combined flux in latest and established models = 4.36458 Jy
selfcal
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 150 components and 4.36459 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.178874Jy  sigma=0.001196
! Fit after  self-cal, rms=0.178321Jy  sigma=0.001191
wmodel J0555+3948_X_2003_07_09_pus_map.mod
! Writing 150 model components to file: J0555+3948_X_2003_07_09_pus_map.mod
wobs J0555+3948_X_2003_07_09_pus_uvs.fits
! Writing UV FITS file: J0555+3948_X_2003_07_09_pus_uvs.fits
wwins J0555+3948_X_2003_07_09_pus_map.win
! wwins: Wrote 7 windows to J0555+3948_X_2003_07_09_pus_map.win
x = (field_size-8) * field_cell / 4
addwin -x,x,-x,x
clean (field_size*4),0.01
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00210857 Jy
! Component: 100  -  total flux cleaned = -0.00336351 Jy
! Component: 150  -  total flux cleaned = -0.00434659 Jy
! Component: 200  -  total flux cleaned = -0.00522954 Jy
! Component: 250  -  total flux cleaned = -0.0058752 Jy
! Component: 300  -  total flux cleaned = -0.00671723 Jy
! Component: 350  -  total flux cleaned = -0.00726832 Jy
! Component: 400  -  total flux cleaned = -0.00774384 Jy
! Component: 450  -  total flux cleaned = -0.00821248 Jy
! Component: 500  -  total flux cleaned = -0.0087403 Jy
! Component: 550  -  total flux cleaned = -0.00906607 Jy
! Component: 600  -  total flux cleaned = -0.00945136 Jy
! Component: 650  -  total flux cleaned = -0.00964271 Jy
! Component: 700  -  total flux cleaned = -0.00995771 Jy
! Component: 750  -  total flux cleaned = -0.0102082 Jy
! Component: 800  -  total flux cleaned = -0.0104568 Jy
! Component: 850  -  total flux cleaned = -0.0107636 Jy
! Component: 900  -  total flux cleaned = -0.0111292 Jy
! Component: 950  -  total flux cleaned = -0.0113102 Jy
! Component: 1000  -  total flux cleaned = -0.0115502 Jy
! Component: 1050  -  total flux cleaned = -0.01167 Jy
! Component: 1100  -  total flux cleaned = -0.0119664 Jy
! Component: 1150  -  total flux cleaned = -0.0122024 Jy
! Component: 1200  -  total flux cleaned = -0.012554 Jy
! Component: 1250  -  total flux cleaned = -0.012786 Jy
! Component: 1300  -  total flux cleaned = -0.0130175 Jy
! Component: 1350  -  total flux cleaned = -0.0133627 Jy
! Component: 1400  -  total flux cleaned = -0.0134769 Jy
! Component: 1450  -  total flux cleaned = -0.0137611 Jy
! Component: 1500  -  total flux cleaned = -0.0139872 Jy
! Component: 1550  -  total flux cleaned = -0.0140996 Jy
! Component: 1600  -  total flux cleaned = -0.0144353 Jy
! Component: 1650  -  total flux cleaned = -0.0146019 Jy
! Component: 1700  -  total flux cleaned = -0.0147676 Jy
! Component: 1750  -  total flux cleaned = -0.0149324 Jy
! Component: 1800  -  total flux cleaned = -0.0150973 Jy
! Component: 1850  -  total flux cleaned = -0.0152606 Jy
! Component: 1900  -  total flux cleaned = -0.0155323 Jy
! Component: 1950  -  total flux cleaned = -0.0156941 Jy
! Component: 2000  -  total flux cleaned = -0.0158554 Jy
! Total flux subtracted in 2048 components = -0.0161233 Jy
! Clean residual min=-0.003112 max=0.002688 Jy/beam
! Clean residual mean=-0.000023 rms=0.000880 Jy/beam
! Combined flux in latest and established models = 4.34846 Jy
keep
! Adding 115 model components to the UV plane model.
! The established model now contains 250 components and 4.34846 Jy
![Exited script file: muppet]
wmap "J0555+3948_X_2003_07_09_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7709 x 1.622 at -2.022 degrees (North through East)
! Clean map  min=-0.0038186  max=3.0159 Jy/beam
! Writing clean map to FITS file: J0555+3948_X_2003_07_09_pus_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 3.0159 
invert
! Inverting map 
! Your choice of large map pixels excluded 1.52% of the data.
!  The x-axis pixel size should ideally be below 0.1633 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000880139 
device "J0555+3948_X_2003_07_09_pus\_map.eps/VPS"
! Attempting to open device: 'J0555+3948_X_2003_07_09_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.0875498 0.0875498 0.1751 0.350199 0.700399 1.4008 2.80159 5.60319 11.2064 22.4128 44.8255 89.651
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0026 
print "peak=",int(1000*peak_flux)/1000
! peak= 3.015 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7709 x 1.622 at -2.022 degrees (North through East)
! Clean map  min=-0.0038186  max=3.0159 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
quit
! Quitting program
! Log file J0555+3948_X_2003_07_09_pus_uvs.log closed on Sun Apr  7 11:55:40 2013