! Started logfile: J1147-0724_X_2003_07_09_pus_uvs.log on Sun Apr  7 13:40:25 2013
obs J1147-0724_X_2003_07_09_pus_uva.fits
! Reading UV FITS file: J1147-0724_X_2003_07_09_pus_uva.fits
! AN table 1: 35 integrations on 171 of 171 possible baselines.
! AN table 2: 214 integrations on 171 of 171 possible baselines.
! AN table 3: 129 integrations on 171 of 171 possible baselines.
! Apparent sampling: 0.142331 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J1147-0724
! 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 1874 lines of history.
! 
! Reading 36800 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 J1147-0724_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 622 telescope corrections were flagged in sub-array 1.
!  A total of 2676 telescope corrections were flagged in sub-array 2.
!  A total of 1654 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 622 telescope corrections were flagged in sub-array 1.
!  A total of 2679 telescope corrections were flagged in sub-array 2.
!  A total of 1654 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 623 telescope corrections were flagged in sub-array 1.
!  A total of 2782 telescope corrections were flagged in sub-array 2.
!  A total of 1655 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 623 telescope corrections were flagged in sub-array 1.
!  A total of 2752 telescope corrections were flagged in sub-array 2.
!  A total of 1654 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=0.831086Jy  sigma=0.005872
! Fit after  self-cal, rms=0.476696Jy  sigma=0.002709
! 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 1.24% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.185 milli-arcsec
! Estimated beam: bmin=0.7117 mas, bmaj=1.093 mas, bpa=13.55 degrees
! Estimated noise=1143.21 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 = 0.526878 Jy
! Component: 100  -  total flux cleaned = 0.671572 Jy
! Total flux subtracted in 100 components = 0.671572 Jy
! Clean residual min=-0.035685 max=0.056531 Jy/beam
! Clean residual mean=-0.000228 rms=0.009666 Jy/beam
! Combined flux in latest and established models = 0.671572 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 10 components and 0.671572 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.321128Jy  sigma=0.001781
! Fit after  self-cal, rms=0.320978Jy  sigma=0.001781
! Inverting map 
! Your choice of large map pixels excluded 1.24% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.185 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0615835 Jy
! Component: 100  -  total flux cleaned = 0.0959724 Jy
! Total flux subtracted in 100 components = 0.0959724 Jy
! Clean residual min=-0.034120 max=0.041646 Jy/beam
! Clean residual mean=-0.000121 rms=0.007609 Jy/beam
! Combined flux in latest and established models = 0.767544 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 19 components and 0.767544 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.307430Jy  sigma=0.001549
! Fit after  self-cal, rms=0.307285Jy  sigma=0.001549
! Inverting map 
! Your choice of large map pixels excluded 1.24% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.185 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 1.24% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.185 milli-arcsec
! Estimated beam: bmin=0.9071 mas, bmaj=1.383 mas, bpa=9.798 degrees
! Estimated noise=485.863 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 (-1.8, 0.4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0527462 Jy
! Component: 100  -  total flux cleaned = 0.0814283 Jy
! Component: 150  -  total flux cleaned = 0.0996621 Jy
! Component: 200  -  total flux cleaned = 0.107521 Jy
! Total flux subtracted in 200 components = 0.107521 Jy
! Clean residual min=-0.022743 max=0.035312 Jy/beam
! Clean residual mean=-0.000058 rms=0.005841 Jy/beam
! Combined flux in latest and established models = 0.875065 Jy
! Performing phase self-cal
! Adding 29 model components to the UV plane model.
! The established model now contains 46 components and 0.875066 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.299458Jy  sigma=0.001417
! Fit after  self-cal, rms=0.298555Jy  sigma=0.001405
! Inverting map 
! Your choice of large map pixels excluded 1.24% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.185 milli-arcsec
! Added new window around map position (4.8, -9.2).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0236408 Jy
! Component: 100  -  total flux cleaned = 0.0294543 Jy
! Component: 150  -  total flux cleaned = 0.0339815 Jy
! Component: 200  -  total flux cleaned = 0.0375338 Jy
! Total flux subtracted in 200 components = 0.0375338 Jy
! Clean residual min=-0.020191 max=0.025622 Jy/beam
! Clean residual mean=0.000015 rms=0.004700 Jy/beam
! Combined flux in latest and established models = 0.912599 Jy
! Performing phase self-cal
! Adding 21 model components to the UV plane model.
! The established model now contains 62 components and 0.912599 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.295808Jy  sigma=0.001363
! Fit after  self-cal, rms=0.295483Jy  sigma=0.001358
! Inverting map 
! Your choice of large map pixels excluded 1.24% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.185 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    GC        1.00*    GG        1.00*    
!   HN        0.70     KP        1.00*    LA        1.00*    MA        1.15     
!   MK        1.00*    NL        1.00*    NY        1.00*    ON        1.21     
!   OV        1.00*    PT        1.00*    SC        0.95     TC        1.00*    
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  A total of 108 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.95     FD        1.12     GC        1.10     GG        1.00*    
!   HN        0.97     KP        0.95     LA        0.98     MA        1.00*    
!   MK        1.01     NL        1.07     NY        1.00*    ON        1.00*    
!   OV        0.99     PT        0.99     SC        0.92     TC        0.93     
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  A total of 24 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        1.00*    KP        0.96     LA        0.97     MA        1.00*    
!   MK        1.00*    NL        0.97     NY        1.00*    ON        1.00*    
!   OV        0.99     PT        0.99     SC        1.00*    TC        0.77     
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 2.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    GC        1.00*    GG        1.00*    
!   HN        0.72     KP        1.00*    LA        1.00*    MA        1.13     
!   MK        1.00*    NL        1.00*    NY        1.00*    ON        1.03     
!   OV        1.00*    PT        1.00*    SC        1.03     TC        1.00*    
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  A total of 105 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.97     FD        1.14     GC        1.15     GG        1.00*    
!   HN        0.97     KP        0.93     LA        0.98     MA        1.00*    
!   MK        1.03     NL        1.04     NY        1.00*    ON        1.00*    
!   OV        0.98     PT        1.02     SC        0.92     TC        1.14     
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  A total of 24 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.02     FD        0.97     GC        1.00*    GG        1.00*    
!   HN        1.00*    KP        0.92     LA        0.97     MA        1.00*    
!   MK        1.00*    NL        0.96     NY        1.00*    ON        1.00*    
!   OV        0.99     PT        1.03     SC        1.00*    TC        0.81     
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 3.
!  A total of 6 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    GC        1.00*    GG        1.00*    
!   HN        0.71     KP        1.00*    LA        1.00*    MA        1.28     
!   MK        1.00*    NL        1.00*    NY        1.00*    ON        1.19     
!   OV        1.00*    PT        1.00*    SC        1.05     TC        1.00*    
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.01     FD        1.13     GC        1.25     GG        1.00*    
!   HN        0.98     KP        0.88     LA        0.99     MA        1.00*    
!   MK        1.03     NL        1.04     NY        1.00*    ON        1.00*    
!   OV        1.03     PT        1.04     SC        0.92     TC        1.48     
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  A total of 24 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.05     FD        0.97     GC        1.00*    GG        1.00*    
!   HN        1.00*    KP        0.87     LA        0.99     MA        1.00*    
!   MK        1.00*    NL        0.97     NY        1.00*    ON        1.00*    
!   OV        1.03     PT        1.06     SC        1.00*    TC        1.19     
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 4.
!  A total of 6 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    GC        1.00*    GG        1.00*    
!   HN        0.69     KP        1.00*    LA        1.00*    MA        1.39     
!   MK        1.00*    NL        1.00*    NY        1.00*    ON        0.93     
!   OV        1.00*    PT        1.00*    SC        1.17     TC        1.00*    
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  A total of 33 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        1.15     GC        1.30     GG        1.00*    
!   HN        1.00     KP        0.92     LA        0.98     MA        1.00*    
!   MK        1.08     NL        1.05     NY        1.00*    ON        1.00*    
!   OV        1.02     PT        1.04     SC        0.97     TC        1.67     
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  A total of 24 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.01     FD        0.94     GC        1.00*    GG        1.00*    
!   HN        1.00*    KP        0.92     LA        0.98     MA        1.00*    
!   MK        1.00*    NL        0.95     NY        1.00*    ON        1.00*    
!   OV        1.03     PT        1.06     SC        1.00*    TC        1.37     
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
! 
! Fit before self-cal, rms=0.295483Jy  sigma=0.001358
! Fit after  self-cal, rms=0.336651Jy  sigma=0.001252
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 milli-arcsec
! Estimated beam: bmin=0.9101 mas, bmaj=1.432 mas, bpa=9.081 degrees
! Estimated noise=491.54 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 = -0.00234534 Jy
! Component: 100  -  total flux cleaned = -0.00387441 Jy
! Component: 150  -  total flux cleaned = -0.0043108 Jy
! Component: 200  -  total flux cleaned = -0.00450683 Jy
! Total flux subtracted in 200 components = -0.00450683 Jy
! Clean residual min=-0.008357 max=0.006468 Jy/beam
! Clean residual mean=0.000002 rms=0.001641 Jy/beam
! Combined flux in latest and established models = 0.908092 Jy
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 77 components and 0.908092 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.336322Jy  sigma=0.001246
! Fit after  self-cal, rms=0.336528Jy  sigma=0.001246
! Inverting map 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 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=0.336528Jy  sigma=0.001246
! Fit after  self-cal, rms=0.339006Jy  sigma=0.001245
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 milli-arcsec
! Estimated beam: bmin=0.9098 mas, bmaj=1.434 mas, bpa=9.067 degrees
! Estimated noise=490.934 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00334188 Jy
! Component: 100  -  total flux cleaned = -0.00390682 Jy
! Component: 150  -  total flux cleaned = -0.00390588 Jy
! Component: 200  -  total flux cleaned = -0.00391258 Jy
! Total flux subtracted in 200 components = -0.00391258 Jy
! Clean residual min=-0.006978 max=0.005667 Jy/beam
! Clean residual mean=0.000003 rms=0.001463 Jy/beam
! Combined flux in latest and established models = 0.90418 Jy
selfcal
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 81 components and 0.90418 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.338826Jy  sigma=0.001242
! Fit after  self-cal, rms=0.338821Jy  sigma=0.001242
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 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 = -0.000978475 Jy
! Component: 100  -  total flux cleaned = -0.000975814 Jy
! Component: 150  -  total flux cleaned = -0.000975497 Jy
! Component: 200  -  total flux cleaned = -0.000861062 Jy
! Total flux subtracted in 200 components = -0.000861062 Jy
! Clean residual min=-0.006217 max=0.005397 Jy/beam
! Clean residual mean=-0.000000 rms=0.001398 Jy/beam
! Combined flux in latest and established models = 0.903319 Jy
! Performing phase self-cal
! Adding 26 model components to the UV plane model.
! The established model now contains 89 components and 0.903319 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.338746Jy  sigma=0.001240
! Fit after  self-cal, rms=0.338741Jy  sigma=0.001240
! Inverting map 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 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=0.338741Jy  sigma=0.001240
! Fit after  self-cal, rms=0.340971Jy  sigma=0.001240
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 milli-arcsec
! Estimated beam: bmin=0.9096 mas, bmaj=1.437 mas, bpa=8.998 degrees
! Estimated noise=491.001 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00277644 Jy
! Component: 100  -  total flux cleaned = -0.00265075 Jy
! Component: 150  -  total flux cleaned = -0.00265412 Jy
! Component: 200  -  total flux cleaned = -0.00265086 Jy
! Total flux subtracted in 200 components = -0.00265086 Jy
! Clean residual min=-0.005450 max=0.004885 Jy/beam
! Clean residual mean=0.000004 rms=0.001281 Jy/beam
! Combined flux in latest and established models = 0.900668 Jy
selfcal
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 89 components and 0.900668 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.340865Jy  sigma=0.001238
! Fit after  self-cal, rms=0.340863Jy  sigma=0.001238
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 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 = -0.000505078 Jy
! Component: 100  -  total flux cleaned = -0.000602534 Jy
! Component: 150  -  total flux cleaned = -0.000602736 Jy
! Component: 200  -  total flux cleaned = -0.000690349 Jy
! Total flux subtracted in 200 components = -0.000690349 Jy
! Clean residual min=-0.005040 max=0.004721 Jy/beam
! Clean residual mean=0.000002 rms=0.001242 Jy/beam
! Combined flux in latest and established models = 0.899977 Jy
! Performing phase self-cal
! Adding 23 model components to the UV plane model.
! The established model now contains 93 components and 0.899978 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.340812Jy  sigma=0.001237
! Fit after  self-cal, rms=0.340805Jy  sigma=0.001237
! Inverting map 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 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=0.340805Jy  sigma=0.001237
! Fit after  self-cal, rms=0.342547Jy  sigma=0.001237
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 milli-arcsec
! Estimated beam: bmin=2.434 mas, bmaj=3.536 mas, bpa=3.894 degrees
! Estimated noise=574.853 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00197513 Jy
! Component: 100  -  total flux cleaned = -0.00231619 Jy
! Component: 150  -  total flux cleaned = -0.00258592 Jy
! Component: 200  -  total flux cleaned = -0.00268319 Jy
! Total flux subtracted in 200 components = -0.00268319 Jy
! Clean residual min=-0.004969 max=0.005600 Jy/beam
! Clean residual mean=0.000001 rms=0.001525 Jy/beam
! Combined flux in latest and established models = 0.897294 Jy
selfcal
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 97 components and 0.897294 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.342516Jy  sigma=0.001236
! Fit after  self-cal, rms=0.342522Jy  sigma=0.001236
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 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 = -0.000304279 Jy
! Component: 100  -  total flux cleaned = -0.000304722 Jy
! Component: 150  -  total flux cleaned = -0.000304016 Jy
! Component: 200  -  total flux cleaned = -0.000302557 Jy
! Total flux subtracted in 200 components = -0.000302557 Jy
! Clean residual min=-0.004888 max=0.005437 Jy/beam
! Clean residual mean=-0.000001 rms=0.001506 Jy/beam
! Combined flux in latest and established models = 0.896992 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 101 components and 0.896992 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.342513Jy  sigma=0.001236
! Fit after  self-cal, rms=0.342519Jy  sigma=0.001236
! Inverting map 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 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 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 milli-arcsec
! Estimated beam: bmin=0.9093 mas, bmaj=1.438 mas, bpa=8.916 degrees
! Estimated noise=491.119 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9093 x 1.438 at 8.916 degrees (North through East)
! Clean map  min=-0.0091436  max=0.69208 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=0.342519Jy  sigma=0.001236
! Fit after  self-cal, rms=0.580111Jy  sigma=0.001126
! Inverting map and beam 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 milli-arcsec
! Estimated beam: bmin=0.9095 mas, bmaj=1.439 mas, bpa=8.856 degrees
! Estimated noise=490.479 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00119736 Jy
! Component: 100  -  total flux cleaned = -0.00109563 Jy
! Component: 150  -  total flux cleaned = -0.00109563 Jy
! Component: 200  -  total flux cleaned = -0.00117997 Jy
! Total flux subtracted in 200 components = -0.00117997 Jy
! Clean residual min=-0.004232 max=0.004159 Jy/beam
! Clean residual mean=0.000014 rms=0.001071 Jy/beam
! Combined flux in latest and established models = 0.895812 Jy
! Performing phase self-cal
! Adding 20 model components to the UV plane model.
! The established model now contains 109 components and 0.895812 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.580076Jy  sigma=0.001125
! Fit after  self-cal, rms=0.580071Jy  sigma=0.001125
! Inverting map 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 milli-arcsec
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000103026 Jy
! Component: 100  -  total flux cleaned = -0.000255875 Jy
! Component: 150  -  total flux cleaned = -0.000328939 Jy
! Component: 200  -  total flux cleaned = -0.000397662 Jy
! Total flux subtracted in 200 components = -0.000397662 Jy
! Clean residual min=-0.003954 max=0.004009 Jy/beam
! Clean residual mean=0.000013 rms=0.001042 Jy/beam
! Combined flux in latest and established models = 0.895414 Jy
! Performing phase self-cal
! Adding 29 model components to the UV plane model.
! The established model now contains 114 components and 0.895414 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.580053Jy  sigma=0.001125
! Fit after  self-cal, rms=0.580041Jy  sigma=0.001125
! Inverting map 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 milli-arcsec
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.580041Jy  sigma=0.001125
! Fit after  self-cal, rms=0.627944Jy  sigma=0.001124
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 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 milli-arcsec
! Estimated beam: bmin=0.7165 mas, bmaj=1.146 mas, bpa=11.67 degrees
! Estimated noise=1170.24 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.537162 Jy
! Component: 100  -  total flux cleaned = 0.681114 Jy
! Component: 150  -  total flux cleaned = 0.742232 Jy
! Component: 200  -  total flux cleaned = 0.780417 Jy
! Total flux subtracted in 200 components = 0.780417 Jy
! Clean residual min=-0.014288 max=0.020860 Jy/beam
! Clean residual mean=-0.000083 rms=0.003849 Jy/beam
! Combined flux in latest and established models = 0.780417 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 26 model components to the UV plane model.
! The established model now contains 26 components and 0.780417 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 milli-arcsec
! Estimated beam: bmin=0.9092 mas, bmaj=1.439 mas, bpa=8.796 degrees
! Estimated noise=490.426 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 = 0.0390592 Jy
! Component: 100  -  total flux cleaned = 0.061754 Jy
! Component: 150  -  total flux cleaned = 0.076188 Jy
! Component: 200  -  total flux cleaned = 0.0861407 Jy
! Total flux subtracted in 200 components = 0.0861407 Jy
! Clean residual min=-0.004434 max=0.006762 Jy/beam
! Clean residual mean=-0.000022 rms=0.001526 Jy/beam
! Combined flux in latest and established models = 0.866557 Jy
! Adding 35 model components to the UV plane model.
! The established model now contains 49 components and 0.866557 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 milli-arcsec
! Added new window around map position (0.4, -1.6).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00747531 Jy
! Component: 100  -  total flux cleaned = 0.012833 Jy
! Component: 150  -  total flux cleaned = 0.0166238 Jy
! Component: 200  -  total flux cleaned = 0.0184995 Jy
! Total flux subtracted in 200 components = 0.0184995 Jy
! Clean residual min=-0.003484 max=0.004533 Jy/beam
! Clean residual mean=0.000003 rms=0.001047 Jy/beam
! Combined flux in latest and established models = 0.885057 Jy
! Adding 29 model components to the UV plane model.
! The established model now contains 70 components and 0.885057 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 milli-arcsec
! Added new window around map position (10, -13).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00356837 Jy
! Component: 100  -  total flux cleaned = 0.00478878 Jy
! Component: 150  -  total flux cleaned = 0.00548426 Jy
! Component: 200  -  total flux cleaned = 0.00603236 Jy
! Total flux subtracted in 200 components = 0.00603236 Jy
! Clean residual min=-0.003210 max=0.003455 Jy/beam
! Clean residual mean=0.000008 rms=0.000931 Jy/beam
! Combined flux in latest and established models = 0.891089 Jy
! Adding 31 model components to the UV plane model.
! The established model now contains 89 components and 0.891089 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 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 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 milli-arcsec
! Estimated beam: bmin=2.435 mas, bmaj=3.542 mas, bpa=3.608 degrees
! Estimated noise=573.673 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0017295 Jy
! Component: 100  -  total flux cleaned = 0.00226768 Jy
! Component: 150  -  total flux cleaned = 0.0027098 Jy
! Component: 200  -  total flux cleaned = 0.00307927 Jy
! Total flux subtracted in 200 components = 0.00307927 Jy
! Clean residual min=-0.003611 max=0.003773 Jy/beam
! Clean residual mean=0.000011 rms=0.001194 Jy/beam
! Combined flux in latest and established models = 0.894168 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 = 0.000324675 Jy
! Component: 100  -  total flux cleaned = 0.000708943 Jy
! Component: 150  -  total flux cleaned = 0.0010061 Jy
! Component: 200  -  total flux cleaned = 0.00127432 Jy
! Total flux subtracted in 200 components = 0.00127432 Jy
! Clean residual min=-0.003513 max=0.003880 Jy/beam
! Clean residual mean=0.000012 rms=0.001165 Jy/beam
! Combined flux in latest and established models = 0.895443 Jy
! Adding 30 model components to the UV plane model.
! The established model now contains 115 components and 0.895443 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 milli-arcsec
! Estimated beam: bmin=0.9092 mas, bmaj=1.439 mas, bpa=8.796 degrees
! Estimated noise=490.426 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000491027 Jy
! Component: 100  -  total flux cleaned = -0.000660796 Jy
! Component: 150  -  total flux cleaned = -0.000663438 Jy
! Component: 200  -  total flux cleaned = -0.00066236 Jy
! Total flux subtracted in 200 components = -0.00066236 Jy
! Clean residual min=-0.003345 max=0.003096 Jy/beam
! Clean residual mean=0.000007 rms=0.000854 Jy/beam
! Combined flux in latest and established models = 0.89478 Jy
selfcal
! Performing phase self-cal
! Adding 20 model components to the UV plane model.
! The established model now contains 126 components and 0.89478 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.627730Jy  sigma=0.001122
! Fit after  self-cal, rms=0.627529Jy  sigma=0.001121
wmodel J1147-0724_X_2003_07_09_pus_map.mod
! Writing 126 model components to file: J1147-0724_X_2003_07_09_pus_map.mod
wobs J1147-0724_X_2003_07_09_pus_uvs.fits
! Writing UV FITS file: J1147-0724_X_2003_07_09_pus_uvs.fits
wwins J1147-0724_X_2003_07_09_pus_map.win
! wwins: Wrote 5 windows to J1147-0724_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 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.000335546 Jy
! Component: 100  -  total flux cleaned = 0.000762089 Jy
! Component: 150  -  total flux cleaned = 0.0011171 Jy
! Component: 200  -  total flux cleaned = 0.00140934 Jy
! Component: 250  -  total flux cleaned = 0.00164406 Jy
! Component: 300  -  total flux cleaned = 0.00200983 Jy
! Component: 350  -  total flux cleaned = 0.0022761 Jy
! Component: 400  -  total flux cleaned = 0.00244938 Jy
! Component: 450  -  total flux cleaned = 0.00261926 Jy
! Component: 500  -  total flux cleaned = 0.00282646 Jy
! Component: 550  -  total flux cleaned = 0.00302815 Jy
! Component: 600  -  total flux cleaned = 0.00322448 Jy
! Component: 650  -  total flux cleaned = 0.00337862 Jy
! Component: 700  -  total flux cleaned = 0.00352936 Jy
! Component: 750  -  total flux cleaned = 0.00367722 Jy
! Component: 800  -  total flux cleaned = 0.00385811 Jy
! Component: 850  -  total flux cleaned = 0.00403608 Jy
! Component: 900  -  total flux cleaned = 0.00417658 Jy
! Component: 950  -  total flux cleaned = 0.00434782 Jy
! Component: 1000  -  total flux cleaned = 0.00438142 Jy
! Component: 1050  -  total flux cleaned = 0.00441505 Jy
! Component: 1100  -  total flux cleaned = 0.00441566 Jy
! Component: 1150  -  total flux cleaned = 0.00454345 Jy
! Component: 1200  -  total flux cleaned = 0.00454397 Jy
! Component: 1250  -  total flux cleaned = 0.00463752 Jy
! Component: 1300  -  total flux cleaned = 0.00472952 Jy
! Component: 1350  -  total flux cleaned = 0.00469919 Jy
! Component: 1400  -  total flux cleaned = 0.00473001 Jy
! Component: 1450  -  total flux cleaned = 0.00475979 Jy
! Component: 1500  -  total flux cleaned = 0.00481754 Jy
! Component: 1550  -  total flux cleaned = 0.004846 Jy
! Component: 1600  -  total flux cleaned = 0.00487416 Jy
! Component: 1650  -  total flux cleaned = 0.00487464 Jy
! Component: 1700  -  total flux cleaned = 0.00512373 Jy
! Component: 1750  -  total flux cleaned = 0.0050412 Jy
! Component: 1800  -  total flux cleaned = 0.00504142 Jy
! Component: 1850  -  total flux cleaned = 0.00501493 Jy
! Component: 1900  -  total flux cleaned = 0.0049883 Jy
! Component: 1950  -  total flux cleaned = 0.00506754 Jy
! Component: 2000  -  total flux cleaned = 0.00496371 Jy
! Total flux subtracted in 2048 components = 0.00506681 Jy
! Clean residual min=-0.001307 max=0.001421 Jy/beam
! Clean residual mean=0.000003 rms=0.000472 Jy/beam
! Combined flux in latest and established models = 0.899847 Jy
keep
! Adding 150 model components to the UV plane model.
! The established model now contains 276 components and 0.899847 Jy
![Exited script file: muppet]
wmap "J1147-0724_X_2003_07_09_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9092 x 1.439 at 8.796 degrees (North through East)
! Clean map  min=-0.0030074  max=0.70092 Jy/beam
! Writing clean map to FITS file: J1147-0724_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 0.700925 
invert
! Inverting map 
! Your choice of large map pixels excluded 1.03% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1852 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000470381 
device "J1147-0724_X_2003_07_09_pus\_map.eps/VPS"
! Attempting to open device: 'J1147-0724_X_2003_07_09_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.201326 0.201326 0.402652 0.805304 1.61061 3.22122 6.44243 12.8849 25.7697 51.5395
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0014 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.7 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9092 x 1.439 at 8.796 degrees (North through East)
! Clean map  min=-0.0030074  max=0.70092 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
quit
! Quitting program
! Log file J1147-0724_X_2003_07_09_pus_uvs.log closed on Sun Apr  7 13:40:38 2013