! Started logfile: J0403-3605_X_2001_04_09_pus_uvs.log on Mon Oct  1 14:33:13 2007
obs J0403-3605_X_2001_04_09_pus_uva.fits
! Reading UV FITS file: J0403-3605_X_2001_04_09_pus_uva.fits
! AN table 1: 9 integrations on 190 of 190 possible baselines.
! AN table 2: 55 integrations on 190 of 190 possible baselines.
! AN table 3: 28 integrations on 190 of 190 possible baselines.
! AN table 4: 27 integrations on 190 of 190 possible baselines.
! AN table 5: 11 integrations on 190 of 190 possible baselines.
! AN table 6: 23 integrations on 190 of 190 possible baselines.
! Apparent sampling: 0.051978 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J0403-3605
! 
! 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 1926 lines of history.
! 
! Reading 6044 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 J0403-3605_X_2001_04_09_pus]
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.03
float dynam
dynam = 6.0
float soltime1
soltime1 = 120
float soltime2
soltime2 = 20
float thresh
thresh = 0.5
float win_mult
win_mult = 1.8
float time_av
time_av = 16
float old_peak
float new_peak
float flux_cutoff
mapsize field_size, field_cell
! Map grid = 256x256 pixels with 0.200x0.200 milli-arcsec cellsize.
startmod
! Applying default point source starting model.
! Performing phase self-cal
! Adding 1 model components to the UV plane model.
! The established model now contains 1 components and 1 Jy
! 
! Correcting IF 1.
!  A total of 180 telescope corrections were flagged in sub-array 1.
!  A total of 1073 telescope corrections were flagged in sub-array 2.
!  A total of 420 telescope corrections were flagged in sub-array 3.
!  A total of 382 telescope corrections were flagged in sub-array 4.
!  A total of 220 telescope corrections were flagged in sub-array 5.
!  A total of 314 telescope corrections were flagged in sub-array 6.
! 
! Correcting IF 2.
!  A total of 180 telescope corrections were flagged in sub-array 1.
!  A total of 1073 telescope corrections were flagged in sub-array 2.
!  A total of 420 telescope corrections were flagged in sub-array 3.
!  A total of 382 telescope corrections were flagged in sub-array 4.
!  A total of 220 telescope corrections were flagged in sub-array 5.
!  A total of 314 telescope corrections were flagged in sub-array 6.
! 
! Correcting IF 3.
!  A total of 180 telescope corrections were flagged in sub-array 1.
!  A total of 1073 telescope corrections were flagged in sub-array 2.
!  A total of 420 telescope corrections were flagged in sub-array 3.
!  A total of 382 telescope corrections were flagged in sub-array 4.
!  A total of 220 telescope corrections were flagged in sub-array 5.
!  A total of 314 telescope corrections were flagged in sub-array 6.
! 
! Correcting IF 4.
!  A total of 180 telescope corrections were flagged in sub-array 1.
!  A total of 1073 telescope corrections were flagged in sub-array 2.
!  A total of 420 telescope corrections were flagged in sub-array 3.
!  A total of 382 telescope corrections were flagged in sub-array 4.
!  A total of 220 telescope corrections were flagged in sub-array 5.
!  A total of 314 telescope corrections were flagged in sub-array 6.
! 
! Fit before self-cal, rms=0.822095Jy  sigma=0.006863
! Fit after  self-cal, rms=0.486583Jy  sigma=0.003589
! clrmod: Cleared the established, tentative and continuum models.
! Redundant starting model cleared.
uvw 2,-1
! Uniform weighting binwidth: 2 (pixels).
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.734% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
! Estimated beam: bmin=0.6656 mas, bmaj=1.474 mas, bpa=1.923 degrees
! Estimated noise=2116.21 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 = 0.443248 Jy
! Component: 100  -  total flux cleaned = 0.559688 Jy
! Total flux subtracted in 100 components = 0.559688 Jy
! Clean residual min=-0.019859 max=0.045792 Jy/beam
! Clean residual mean=0.001896 rms=0.007513 Jy/beam
! Combined flux in latest and established models = 0.559688 Jy
! Performing phase self-cal
! Adding 5 model components to the UV plane model.
! The established model now contains 5 components and 0.559688 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.243328Jy  sigma=0.001525
! Fit after  self-cal, rms=0.243348Jy  sigma=0.001525
! Inverting map 
! Your choice of large map pixels excluded 0.734% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0459018 Jy
! Component: 100  -  total flux cleaned = 0.0668352 Jy
! Total flux subtracted in 100 components = 0.0668352 Jy
! Clean residual min=-0.015152 max=0.021418 Jy/beam
! Clean residual mean=0.000702 rms=0.005156 Jy/beam
! Combined flux in latest and established models = 0.626523 Jy
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 15 components and 0.626523 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.233312Jy  sigma=0.001344
! Fit after  self-cal, rms=0.233284Jy  sigma=0.001343
! Inverting map 
! Your choice of large map pixels excluded 0.734% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
print "************** FINISHED UNIFORM WEIGHTING CLEAN **************"
! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** 
! 
uvw 0,-1
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
win_mult = win_mult * 1.6
clean_niter = clean_niter * 2
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.734% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
! Estimated beam: bmin=0.8587 mas, bmaj=2.379 mas, bpa=-7.837 degrees
! Estimated noise=1170.57 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 = 0.0272688 Jy
! Component: 100  -  total flux cleaned = 0.0400649 Jy
! Component: 150  -  total flux cleaned = 0.0462352 Jy
! Component: 200  -  total flux cleaned = 0.0487984 Jy
! Total flux subtracted in 200 components = 0.0487984 Jy
! Clean residual min=-0.014257 max=0.023579 Jy/beam
! Clean residual mean=-0.000151 rms=0.005305 Jy/beam
! Combined flux in latest and established models = 0.675322 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 26 components and 0.675322 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.231738Jy  sigma=0.001297
! Fit after  self-cal, rms=0.231659Jy  sigma=0.001297
! Inverting map 
! Your choice of large map pixels excluded 0.734% of the data.
!  The x-axis pixel size should ideally be below 0.1921 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        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HH        0.00*    HN        0.00*    KK        0.00*    KP        0.00*    
!   LA        0.00*    MA        0.00*    MC        0.00*    MK        0.00*    
!   NL        0.00*    NY        0.00*    OV        0.00*    PT        0.00*    
!   SC        0.00*    TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  A total of 27 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HH        0.00*    HN        0.00*    KK        0.00*    KP        0.00*    
!   LA        0.00*    MA        0.00*    MC        0.00*    MK        0.00*    
!   NL        0.00*    NY        0.00*    OV        0.00*    PT        0.00*    
!   SC        0.00*    TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  A total of 33 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        1.00     GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        1.00*    KK        0.96     KP        0.97     
!   LA        1.05     MA        1.00*    MC        1.00*    MK        0.87     
!   NL        1.00*    NY        1.00*    OV        1.01     PT        1.01     
!   SC        1.00*    TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        0.97     GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        1.00*    KK        1.04     KP        0.88     
!   LA        1.02     MA        1.00*    MC        1.00*    MK        0.94     
!   NL        1.17     NY        1.00*    OV        0.94     PT        0.98     
!   SC        1.03     TS        1.00*    WF        1.13     WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HH        0.00*    HN        0.00*    KK        0.00*    KP        0.00*    
!   LA        0.00*    MA        0.00*    MC        0.00*    MK        0.00*    
!   NL        0.00*    NY        0.00*    OV        0.00*    PT        0.00*    
!   SC        0.00*    TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 6.
!  Telescope amplitude corrections in sub-array 6:
!   BR        1.00*    FD        0.99     GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        1.32     KK        1.00*    KP        1.07     
!   LA        1.02     MA        1.00*    MC        1.00*    MK        1.00*    
!   NL        1.20     NY        1.00*    OV        1.00*    PT        0.99     
!   SC        0.96     TS        1.00*    WF        0.96     WZ        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HH        0.00*    HN        0.00*    KK        0.00*    KP        0.00*    
!   LA        0.00*    MA        0.00*    MC        0.00*    MK        0.00*    
!   NL        0.00*    NY        0.00*    OV        0.00*    PT        0.00*    
!   SC        0.00*    TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  A total of 27 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HH        0.00*    HN        0.00*    KK        0.00*    KP        0.00*    
!   LA        0.00*    MA        0.00*    MC        0.00*    MK        0.00*    
!   NL        0.00*    NY        0.00*    OV        0.00*    PT        0.00*    
!   SC        0.00*    TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  A total of 33 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        0.98     GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        1.00*    KK        0.96     KP        0.99     
!   LA        1.04     MA        1.00*    MC        1.00*    MK        0.97     
!   NL        1.00*    NY        1.00*    OV        1.00     PT        1.04     
!   SC        1.00*    TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        0.98     GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        1.00*    KK        1.08     KP        0.86     
!   LA        1.03     MA        1.00*    MC        1.00*    MK        1.04     
!   NL        1.11     NY        1.00*    OV        0.97     PT        0.97     
!   SC        1.05     TS        1.00*    WF        1.14     WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HH        0.00*    HN        0.00*    KK        0.00*    KP        0.00*    
!   LA        0.00*    MA        0.00*    MC        0.00*    MK        0.00*    
!   NL        0.00*    NY        0.00*    OV        0.00*    PT        0.00*    
!   SC        0.00*    TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 6.
!  Telescope amplitude corrections in sub-array 6:
!   BR        1.00*    FD        0.97     GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        1.23     KK        1.00*    KP        1.03     
!   LA        1.05     MA        1.00*    MC        1.00*    MK        1.00*    
!   NL        1.17     NY        1.00*    OV        1.00*    PT        1.03     
!   SC        1.01     TS        1.00*    WF        0.88     WZ        1.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HH        0.00*    HN        0.00*    KK        0.00*    KP        0.00*    
!   LA        0.00*    MA        0.00*    MC        0.00*    MK        0.00*    
!   NL        0.00*    NY        0.00*    OV        0.00*    PT        0.00*    
!   SC        0.00*    TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  A total of 27 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HH        0.00*    HN        0.00*    KK        0.00*    KP        0.00*    
!   LA        0.00*    MA        0.00*    MC        0.00*    MK        0.00*    
!   NL        0.00*    NY        0.00*    OV        0.00*    PT        0.00*    
!   SC        0.00*    TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  A total of 33 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        0.98     GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        1.00*    KK        1.01     KP        0.87     
!   LA        1.08     MA        1.00*    MC        1.00*    MK        0.89     
!   NL        1.00*    NY        1.00*    OV        0.97     PT        0.98     
!   SC        1.00*    TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        0.97     GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        1.00*    KK        1.03     KP        0.79     
!   LA        1.00     MA        1.00*    MC        1.00*    MK        0.95     
!   NL        1.13     NY        1.00*    OV        0.95     PT        0.92     
!   SC        1.04     TS        1.00*    WF        1.17     WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HH        0.00*    HN        0.00*    KK        0.00*    KP        0.00*    
!   LA        0.00*    MA        0.00*    MC        0.00*    MK        0.00*    
!   NL        0.00*    NY        0.00*    OV        0.00*    PT        0.00*    
!   SC        0.00*    TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 6.
!  Telescope amplitude corrections in sub-array 6:
!   BR        1.00*    FD        1.00     GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        1.34     KK        1.00*    KP        0.93     
!   LA        1.03     MA        1.00*    MC        1.00*    MK        1.00*    
!   NL        1.14     NY        1.00*    OV        1.00*    PT        0.93     
!   SC        1.00     TS        1.00*    WF        1.03     WZ        1.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HH        0.00*    HN        0.00*    KK        0.00*    KP        0.00*    
!   LA        0.00*    MA        0.00*    MC        0.00*    MK        0.00*    
!   NL        0.00*    NY        0.00*    OV        0.00*    PT        0.00*    
!   SC        0.00*    TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  A total of 27 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HH        0.00*    HN        0.00*    KK        0.00*    KP        0.00*    
!   LA        0.00*    MA        0.00*    MC        0.00*    MK        0.00*    
!   NL        0.00*    NY        0.00*    OV        0.00*    PT        0.00*    
!   SC        0.00*    TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  A total of 33 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        1.00     GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        1.00*    KK        0.97     KP        1.05     
!   LA        1.05     MA        1.00*    MC        1.00*    MK        0.92     
!   NL        1.00*    NY        1.00*    OV        0.94     PT        1.01     
!   SC        1.00*    TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        0.98     GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        1.00*    KK        1.06     KP        0.98     
!   LA        0.97     MA        1.00*    MC        1.00*    MK        0.96     
!   NL        1.12     NY        1.00*    OV        0.90     PT        0.96     
!   SC        1.06     TS        1.00*    WF        1.20     WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HH        0.00*    HN        0.00*    KK        0.00*    KP        0.00*    
!   LA        0.00*    MA        0.00*    MC        0.00*    MK        0.00*    
!   NL        0.00*    NY        0.00*    OV        0.00*    PT        0.00*    
!   SC        0.00*    TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 6.
!  Telescope amplitude corrections in sub-array 6:
!   BR        1.00*    FD        0.98     GC        1.00*    GG        1.00*    
!   HH        1.00*    HN        1.18     KK        1.00*    KP        1.14     
!   LA        1.00     MA        1.00*    MC        1.00*    MK        1.00*    
!   NL        1.16     NY        1.00*    OV        1.00*    PT        0.98     
!   SC        1.01     TS        1.00*    WF        1.00     WZ        1.00*    
! 
! 
! Fit before self-cal, rms=0.231659Jy  sigma=0.001297
! Fit after  self-cal, rms=0.252395Jy  sigma=0.001197
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
! Estimated beam: bmin=0.864 mas, bmaj=3.073 mas, bpa=-10.28 degrees
! Estimated noise=1188.83 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 = 0.00257145 Jy
! Component: 100  -  total flux cleaned = 0.00208384 Jy
! Component: 150  -  total flux cleaned = 0.00200037 Jy
! Component: 200  -  total flux cleaned = 0.00200066 Jy
! Total flux subtracted in 200 components = 0.00200066 Jy
! Clean residual min=-0.005275 max=0.007861 Jy/beam
! Clean residual mean=0.000517 rms=0.001946 Jy/beam
! Combined flux in latest and established models = 0.677322 Jy
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 29 components and 0.677322 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.252289Jy  sigma=0.001196
! Fit after  self-cal, rms=0.252610Jy  sigma=0.001195
! Inverting map 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 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=0.252610Jy  sigma=0.001195
! Fit after  self-cal, rms=0.251908Jy  sigma=0.001195
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
! Estimated beam: bmin=0.8625 mas, bmaj=3.071 mas, bpa=-10.31 degrees
! Estimated noise=1188.11 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00163168 Jy
! Component: 100  -  total flux cleaned = 0.00129901 Jy
! Component: 150  -  total flux cleaned = 0.00122749 Jy
! Component: 200  -  total flux cleaned = 0.00122987 Jy
! Total flux subtracted in 200 components = 0.00122987 Jy
! Clean residual min=-0.004852 max=0.007122 Jy/beam
! Clean residual mean=0.000506 rms=0.001884 Jy/beam
! Combined flux in latest and established models = 0.678552 Jy
selfcal
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 32 components and 0.678552 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.251841Jy  sigma=0.001194
! Fit after  self-cal, rms=0.251804Jy  sigma=0.001194
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 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 = 9.97716e-06 Jy
! Component: 100  -  total flux cleaned = -6.57201e-05 Jy
! Component: 150  -  total flux cleaned = -6.44019e-05 Jy
! Component: 200  -  total flux cleaned = -6.15161e-05 Jy
! Total flux subtracted in 200 components = -6.15161e-05 Jy
! Clean residual min=-0.004613 max=0.006908 Jy/beam
! Clean residual mean=0.000510 rms=0.001853 Jy/beam
! Combined flux in latest and established models = 0.678491 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 34 components and 0.67849 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.251761Jy  sigma=0.001194
! Fit after  self-cal, rms=0.251739Jy  sigma=0.001194
! Inverting map 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 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=0.251739Jy  sigma=0.001194
! Fit after  self-cal, rms=0.251364Jy  sigma=0.001194
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
! Estimated beam: bmin=0.8615 mas, bmaj=3.07 mas, bpa=-10.33 degrees
! Estimated noise=1187.53 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000854134 Jy
! Component: 100  -  total flux cleaned = 0.000671263 Jy
! Component: 150  -  total flux cleaned = 0.000670378 Jy
! Component: 200  -  total flux cleaned = 0.00066769 Jy
! Total flux subtracted in 200 components = 0.00066769 Jy
! Clean residual min=-0.004453 max=0.006608 Jy/beam
! Clean residual mean=0.000509 rms=0.001816 Jy/beam
! Combined flux in latest and established models = 0.679158 Jy
selfcal
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 35 components and 0.679158 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.251331Jy  sigma=0.001193
! Fit after  self-cal, rms=0.251308Jy  sigma=0.001193
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 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 = 5.10822e-06 Jy
! Component: 100  -  total flux cleaned = -5.14875e-05 Jy
! Component: 150  -  total flux cleaned = -5.35536e-05 Jy
! Component: 200  -  total flux cleaned = -5.75085e-05 Jy
! Total flux subtracted in 200 components = -5.75085e-05 Jy
! Clean residual min=-0.004311 max=0.006517 Jy/beam
! Clean residual mean=0.000512 rms=0.001795 Jy/beam
! Combined flux in latest and established models = 0.679101 Jy
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 35 components and 0.679101 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.251284Jy  sigma=0.001193
! Fit after  self-cal, rms=0.251268Jy  sigma=0.001193
! Inverting map 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 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=0.251268Jy  sigma=0.001193
! Fit after  self-cal, rms=0.251064Jy  sigma=0.001193
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
! Estimated beam: bmin=2.57 mas, bmaj=7.169 mas, bpa=-3.94 degrees
! Estimated noise=1399.75 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00062906 Jy
! Component: 100  -  total flux cleaned = 0.00062947 Jy
! Component: 150  -  total flux cleaned = 0.000632058 Jy
! Component: 200  -  total flux cleaned = 0.000634656 Jy
! Total flux subtracted in 200 components = 0.000634656 Jy
! Clean residual min=-0.003520 max=0.007243 Jy/beam
! Clean residual mean=0.000959 rms=0.002303 Jy/beam
! Combined flux in latest and established models = 0.679735 Jy
selfcal
! Performing phase self-cal
! Adding 2 model components to the UV plane model.
! The established model now contains 35 components and 0.679735 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.251083Jy  sigma=0.001193
! Fit after  self-cal, rms=0.251008Jy  sigma=0.001193
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 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 = -5.80359e-06 Jy
! Component: 100  -  total flux cleaned = -1.0484e-05 Jy
! Component: 150  -  total flux cleaned = -1.40787e-05 Jy
! Component: 200  -  total flux cleaned = -1.67909e-05 Jy
! Total flux subtracted in 200 components = -1.67909e-05 Jy
! Clean residual min=-0.003499 max=0.007216 Jy/beam
! Clean residual mean=0.000960 rms=0.002280 Jy/beam
! Combined flux in latest and established models = 0.679719 Jy
! Performing phase self-cal
! Adding 2 model components to the UV plane model.
! The established model now contains 35 components and 0.679719 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.251028Jy  sigma=0.001193
! Fit after  self-cal, rms=0.250967Jy  sigma=0.001192
! Inverting map 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
win_mult = win_mult / 1.2
print "************** FINISHED AMPLITUDE SELF-CAL **************"
! ************** FINISHED AMPLITUDE SELF-CAL ************** 
restore
! Inverting map and beam 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
! Estimated beam: bmin=0.8611 mas, bmaj=3.07 mas, bpa=-10.34 degrees
! Estimated noise=1187.4 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8611 x 3.07 at -10.34 degrees (North through East)
! Clean map  min=-0.0038274  max=0.58119 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=0.250967Jy  sigma=0.001192
! Fit after  self-cal, rms=0.283620Jy  sigma=0.001092
! Inverting map and beam 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
! Estimated beam: bmin=0.8608 mas, bmaj=3.071 mas, bpa=-10.33 degrees
! Estimated noise=1187.82 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000494811 Jy
! Component: 100  -  total flux cleaned = 0.000366345 Jy
! Component: 150  -  total flux cleaned = 0.000368438 Jy
! Component: 200  -  total flux cleaned = 0.000367859 Jy
! Total flux subtracted in 200 components = 0.000367859 Jy
! Clean residual min=-0.004274 max=0.006344 Jy/beam
! Clean residual mean=0.000572 rms=0.001727 Jy/beam
! Combined flux in latest and established models = 0.680086 Jy
! Performing phase self-cal
! Adding 5 model components to the UV plane model.
! The established model now contains 35 components and 0.680086 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.283601Jy  sigma=0.001092
! Fit after  self-cal, rms=0.283588Jy  sigma=0.001092
! Inverting map 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000128274 Jy
! Component: 100  -  total flux cleaned = 8.92349e-05 Jy
! Component: 150  -  total flux cleaned = 5.52815e-05 Jy
! Component: 200  -  total flux cleaned = 5.58692e-05 Jy
! Total flux subtracted in 200 components = 5.58692e-05 Jy
! Clean residual min=-0.004271 max=0.006270 Jy/beam
! Clean residual mean=0.000568 rms=0.001721 Jy/beam
! Combined flux in latest and established models = 0.680142 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 37 components and 0.680142 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.283578Jy  sigma=0.001092
! Fit after  self-cal, rms=0.283569Jy  sigma=0.001092
! Inverting map 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.283569Jy  sigma=0.001092
! Fit after  self-cal, rms=0.283206Jy  sigma=0.001092
print "************** CLEARING MODEL AND STARTING OVER **********"
! ************** CLEARING MODEL AND STARTING OVER ********** 
clrmod true
! clrmod: Cleared the established and tentative models.
uvw 2,-1
! Uniform weighting binwidth: 2 (pixels).
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
! Estimated beam: bmin=0.6823 mas, bmaj=2.37 mas, bpa=-6.296 degrees
! Estimated noise=2071.41 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.448902 Jy
! Component: 100  -  total flux cleaned = 0.570216 Jy
! Component: 150  -  total flux cleaned = 0.620642 Jy
! Component: 200  -  total flux cleaned = 0.645203 Jy
! Total flux subtracted in 200 components = 0.645203 Jy
! Clean residual min=-0.008938 max=0.012497 Jy/beam
! Clean residual mean=0.000900 rms=0.003141 Jy/beam
! Combined flux in latest and established models = 0.645203 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 20 model components to the UV plane model.
! The established model now contains 20 components and 0.645203 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
! Estimated beam: bmin=0.8605 mas, bmaj=3.071 mas, bpa=-10.32 degrees
! Estimated noise=1187.49 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 = 0.0195337 Jy
! Component: 100  -  total flux cleaned = 0.0282151 Jy
! Component: 150  -  total flux cleaned = 0.0321316 Jy
! Component: 200  -  total flux cleaned = 0.0333613 Jy
! Total flux subtracted in 200 components = 0.0333613 Jy
! Clean residual min=-0.004411 max=0.006067 Jy/beam
! Clean residual mean=0.000678 rms=0.001762 Jy/beam
! Combined flux in latest and established models = 0.678565 Jy
! Adding 18 model components to the UV plane model.
! The established model now contains 30 components and 0.678565 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
! Estimated beam: bmin=2.569 mas, bmaj=7.167 mas, bpa=-3.967 degrees
! Estimated noise=1401.35 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00218559 Jy
! Component: 100  -  total flux cleaned = 0.00218386 Jy
! Component: 150  -  total flux cleaned = 0.00212536 Jy
! Component: 200  -  total flux cleaned = 0.00212438 Jy
! Total flux subtracted in 200 components = 0.00212438 Jy
! Clean residual min=-0.003404 max=0.007723 Jy/beam
! Clean residual mean=0.001064 rms=0.002346 Jy/beam
! Combined flux in latest and established models = 0.680689 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 = -4.22876e-05 Jy
! Component: 100  -  total flux cleaned = -4.3701e-05 Jy
! Component: 150  -  total flux cleaned = -7.63706e-05 Jy
! Component: 200  -  total flux cleaned = -0.000101356 Jy
! Total flux subtracted in 200 components = -0.000101356 Jy
! Clean residual min=-0.003386 max=0.007516 Jy/beam
! Clean residual mean=0.001076 rms=0.002293 Jy/beam
! Combined flux in latest and established models = 0.680588 Jy
! Adding 5 model components to the UV plane model.
! The established model now contains 34 components and 0.680588 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
! Estimated beam: bmin=0.8605 mas, bmaj=3.071 mas, bpa=-10.32 degrees
! Estimated noise=1187.49 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00127128 Jy
! Component: 100  -  total flux cleaned = -0.00121669 Jy
! Component: 150  -  total flux cleaned = -0.00110996 Jy
! Component: 200  -  total flux cleaned = -0.00106831 Jy
! Total flux subtracted in 200 components = -0.00106831 Jy
! Clean residual min=-0.004400 max=0.006014 Jy/beam
! Clean residual mean=0.000624 rms=0.001705 Jy/beam
! Combined flux in latest and established models = 0.67952 Jy
selfcal
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 39 components and 0.679519 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.283187Jy  sigma=0.001091
! Fit after  self-cal, rms=0.283158Jy  sigma=0.001091
wmodel J0403-3605_X_2001_04_09_pus_map.mod
! Writing 39 model components to file: J0403-3605_X_2001_04_09_pus_map.mod
wobs J0403-3605_X_2001_04_09_pus_uvs.fits
! Writing UV FITS file: J0403-3605_X_2001_04_09_pus_uvs.fits
wwins J0403-3605_X_2001_04_09_pus_map.win
! wwins: Wrote 1 windows to J0403-3605_X_2001_04_09_pus_map.win
x = (field_size-8) * field_cell / 4
addwin -x,x,-x,x
clean (field_size*4),0.01
! Inverting map 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.00254925 Jy
! Component: 100  -  total flux cleaned = 0.00467405 Jy
! Component: 150  -  total flux cleaned = 0.00555632 Jy
! Component: 200  -  total flux cleaned = 0.00645228 Jy
! Component: 250  -  total flux cleaned = 0.00744389 Jy
! Component: 300  -  total flux cleaned = 0.00845628 Jy
! Component: 350  -  total flux cleaned = 0.00923382 Jy
! Component: 400  -  total flux cleaned = 0.0100455 Jy
! Component: 450  -  total flux cleaned = 0.0108269 Jy
! Component: 500  -  total flux cleaned = 0.0115808 Jy
! Component: 550  -  total flux cleaned = 0.012031 Jy
! Component: 600  -  total flux cleaned = 0.0124687 Jy
! Component: 650  -  total flux cleaned = 0.0128951 Jy
! Component: 700  -  total flux cleaned = 0.0132075 Jy
! Component: 750  -  total flux cleaned = 0.0135132 Jy
! Component: 800  -  total flux cleaned = 0.0138128 Jy
! Component: 850  -  total flux cleaned = 0.0139605 Jy
! Component: 900  -  total flux cleaned = 0.0142496 Jy
! Component: 950  -  total flux cleaned = 0.0144851 Jy
! Component: 1000  -  total flux cleaned = 0.0146702 Jy
! Total flux subtracted in 1024 components = 0.0147161 Jy
! Clean residual min=-0.002321 max=0.003094 Jy/beam
! Clean residual mean=0.000239 rms=0.000945 Jy/beam
! Combined flux in latest and established models = 0.694236 Jy
keep
! Adding 59 model components to the UV plane model.
! The established model now contains 98 components and 0.694236 Jy
![Exited script file: muppet]
wmap "J0403-3605_X_2001_04_09_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8605 x 3.071 at -10.32 degrees (North through East)
! Clean map  min=-0.0034926  max=0.58195 Jy/beam
! Writing clean map to FITS file: J0403-3605_X_2001_04_09_pus_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.581955 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.768% of the data.
!  The x-axis pixel size should ideally be below 0.1921 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000937671 
device "J0403-3605_X_2001_04_09_pus\_map.eps/VPS"
! Attempting to open device: 'J0403-3605_X_2001_04_09_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.483373 0.483373 0.966746 1.93349 3.86699 7.73397 15.4679 30.9359 61.8718
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0028 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.581 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8605 x 3.071 at -10.32 degrees (North through East)
! Clean map  min=-0.0034926  max=0.58195 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0403-3605_X_2001_04_09_pus\_map.gif/vgif"
! Attempting to open device: 'J0403-3605_X_2001_04_09_pus_map.gif/vgif'
mapplot cln
quit
! Quitting program
! Log file J0403-3605_X_2001_04_09_pus_uvs.log closed on Mon Oct  1 14:33:16 2007