! Started logfile: J1357+7643_X_1999_12_20_pus_uvs.log on Fri Dec 14 17:23:03 2007
obs J1357+7643_X_1999_12_20_pus_uva.fits
! Reading UV FITS file: J1357+7643_X_1999_12_20_pus_uva.fits
! AN table 1: 185 integrations on 190 of 190 possible baselines.
! AN table 2: 467 integrations on 190 of 190 possible baselines.
! AN table 3: 54 integrations on 190 of 190 possible baselines.
! Apparent sampling: 0.227419 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J1357+7643
! 
! 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 2418 lines of history.
! 
! Reading 122024 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 J1357+7643_X_1999_12_20_pus]
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.03
float dynam
dynam = 6.0
float soltime1
soltime1 = 120
float soltime2
soltime2 = 20
float thresh
thresh = 0.5
float win_mult
win_mult = 1.8
float time_av
time_av = 16
float old_peak
float new_peak
float flux_cutoff
mapsize field_size, field_cell
! Map grid = 256x256 pixels with 0.200x0.200 milli-arcsec cellsize.
startmod
! Applying default point source starting model.
! Performing phase self-cal
! Adding 1 model components to the UV plane model.
! The established model now contains 1 components and 1 Jy
! 
! Correcting IF 1.
!  A total of 2638 telescope corrections were flagged in sub-array 1.
!  A total of 5677 telescope corrections were flagged in sub-array 2.
!  A total of 617 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 2638 telescope corrections were flagged in sub-array 1.
!  A total of 5677 telescope corrections were flagged in sub-array 2.
!  A total of 617 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 2638 telescope corrections were flagged in sub-array 1.
!  A total of 5677 telescope corrections were flagged in sub-array 2.
!  A total of 617 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 2638 telescope corrections were flagged in sub-array 1.
!  A total of 5677 telescope corrections were flagged in sub-array 2.
!  A total of 617 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=0.801769Jy  sigma=0.006975
! Fit after  self-cal, rms=0.343537Jy  sigma=0.002789
! clrmod: Cleared the established, tentative and continuum models.
! Redundant starting model cleared.
uvw 2,-1
! Uniform weighting binwidth: 2 (pixels).
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 3.54% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! Estimated beam: bmin=0.5344 mas, bmaj=0.5576 mas, bpa=87.05 degrees
! Estimated noise=513.5 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 = 0.557044 Jy
! Component: 100  -  total flux cleaned = 0.678516 Jy
! Total flux subtracted in 100 components = 0.678516 Jy
! Clean residual min=-0.005985 max=0.033999 Jy/beam
! Clean residual mean=0.000064 rms=0.001775 Jy/beam
! Combined flux in latest and established models = 0.678516 Jy
! Performing phase self-cal
! Adding 1 model components to the UV plane model.
! The established model now contains 1 components and 0.678516 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.215880Jy  sigma=0.001463
! Fit after  self-cal, rms=0.215879Jy  sigma=0.001463
! Inverting map 
! Your choice of large map pixels excluded 3.54% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0321606 Jy
! Component: 100  -  total flux cleaned = 0.0491717 Jy
! Total flux subtracted in 100 components = 0.0491717 Jy
! Clean residual min=-0.005553 max=0.008752 Jy/beam
! Clean residual mean=0.000034 rms=0.001339 Jy/beam
! Combined flux in latest and established models = 0.727687 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 8 components and 0.727687 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.208487Jy  sigma=0.001344
! Fit after  self-cal, rms=0.208460Jy  sigma=0.001344
! Inverting map 
! Your choice of large map pixels excluded 3.54% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0109615 Jy
! Component: 100  -  total flux cleaned = 0.0186811 Jy
! Total flux subtracted in 100 components = 0.0186811 Jy
! Clean residual min=-0.005804 max=0.006638 Jy/beam
! Clean residual mean=0.000023 rms=0.001270 Jy/beam
! Combined flux in latest and established models = 0.746368 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 10 components and 0.746368 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.207179Jy  sigma=0.001320
! Fit after  self-cal, rms=0.207167Jy  sigma=0.001320
! Inverting map 
! Your choice of large map pixels excluded 3.54% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
print "************** FINISHED UNIFORM WEIGHTING CLEAN **************"
! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** 
! 
uvw 0,-1
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
win_mult = win_mult * 1.6
clean_niter = clean_niter * 2
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 3.54% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! Estimated beam: bmin=0.6708 mas, bmaj=0.7181 mas, bpa=-72.9 degrees
! Estimated noise=242.98 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 (-0.6, 0.2).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0172677 Jy
! Component: 100  -  total flux cleaned = 0.0277136 Jy
! Component: 150  -  total flux cleaned = 0.0344072 Jy
! Component: 200  -  total flux cleaned = 0.0388077 Jy
! Total flux subtracted in 200 components = 0.0388077 Jy
! Clean residual min=-0.005087 max=0.007754 Jy/beam
! Clean residual mean=0.000006 rms=0.001096 Jy/beam
! Combined flux in latest and established models = 0.785176 Jy
! Performing phase self-cal
! Adding 32 model components to the UV plane model.
! The established model now contains 36 components and 0.785176 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.206052Jy  sigma=0.001298
! Fit after  self-cal, rms=0.206017Jy  sigma=0.001297
! Inverting map 
! Your choice of large map pixels excluded 3.54% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! Added new window around map position (1, -0.4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00604682 Jy
! Component: 100  -  total flux cleaned = 0.00864574 Jy
! Component: 150  -  total flux cleaned = 0.00955101 Jy
! Component: 200  -  total flux cleaned = 0.0102147 Jy
! Total flux subtracted in 200 components = 0.0102147 Jy
! Clean residual min=-0.005538 max=0.004750 Jy/beam
! Clean residual mean=-0.000074 rms=0.001014 Jy/beam
! Combined flux in latest and established models = 0.795391 Jy
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 45 components and 0.795391 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.205828Jy  sigma=0.001295
! Fit after  self-cal, rms=0.205825Jy  sigma=0.001295
! Inverting map 
! Your choice of large map pixels excluded 3.54% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 144 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     FD        1.00     GC        0.97     HH        1.00*    
!   HN        0.92     KK        1.00     KP        1.02     LA        1.02     
!   MC        1.04     MK        0.99     NY        1.00     ON        0.99     
!   OV        0.99     PT        1.04     SC        1.10     TS        1.03     
!   WF        0.98     WZ        1.04     GN        0.96     NL        1.00*    
! 
!  A total of 333 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.97     FD        1.02     GC        1.00     HH        1.00*    
!   HN        1.03     KK        1.04     KP        1.02     LA        1.01     
!   MC        1.00     MK        1.06     NY        1.01     ON        0.98     
!   OV        1.00     PT        1.01     SC        1.15     TS        0.97     
!   WF        1.04     WZ        0.98     GN        1.00     NL        0.98     
! 
!  A total of 15 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.01     FD        1.03     GC        1.03     HH        1.00*    
!   HN        0.94     KK        1.09     KP        1.02     LA        1.02     
!   MC        0.97     MK        1.07     NY        0.99     ON        0.97     
!   OV        0.99     PT        1.00     SC        1.09     TS        1.02     
!   WF        1.00     WZ        0.98     GN        1.01     NL        0.99     
! 
! 
! Correcting IF 2.
!  A total of 144 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     FD        1.00     GC        0.93     HH        1.00*    
!   HN        0.91     KK        1.00     KP        0.97     LA        1.02     
!   MC        1.04     MK        1.00     NY        0.99     ON        0.98     
!   OV        1.00     PT        1.04     SC        1.04     TS        1.01     
!   WF        0.98     WZ        1.01     GN        0.99     NL        1.00*    
! 
!  A total of 333 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.97     FD        1.03     GC        0.96     HH        1.00*    
!   HN        1.02     KK        1.03     KP        0.97     LA        1.00     
!   MC        0.99     MK        1.09     NY        1.00     ON        0.95     
!   OV        1.00     PT        1.00     SC        1.10     TS        0.97     
!   WF        1.04     WZ        0.98     GN        1.00     NL        0.97     
! 
!  A total of 15 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00     FD        1.03     GC        0.99     HH        1.00*    
!   HN        0.94     KK        1.06     KP        0.97     LA        1.01     
!   MC        0.99     MK        1.05     NY        0.98     ON        0.95     
!   OV        1.00     PT        0.99     SC        1.04     TS        1.02     
!   WF        1.01     WZ        0.98     GN        1.01     NL        0.98     
! 
! 
! Correcting IF 3.
!  A total of 144 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.97     FD        1.01     GC        0.96     HH        1.00*    
!   HN        0.93     KK        1.01     KP        0.97     LA        1.01     
!   MC        1.02     MK        0.99     NY        0.97     ON        0.99     
!   OV        1.00     PT        1.03     SC        1.06     TS        1.01     
!   WF        0.97     WZ        1.02     GN        0.96     NL        1.00*    
! 
!  A total of 333 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.95     FD        1.02     GC        0.99     HH        1.00*    
!   HN        1.04     KK        1.04     KP        0.98     LA        1.00     
!   MC        0.98     MK        1.05     NY        0.98     ON        0.97     
!   OV        0.99     PT        1.01     SC        1.11     TS        0.97     
!   WF        1.04     WZ        0.98     GN        1.00     NL        0.97     
! 
!  A total of 15 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.98     FD        1.03     GC        1.02     HH        1.00*    
!   HN        0.96     KK        1.07     KP        0.99     LA        1.01     
!   MC        0.94     MK        1.03     NY        0.97     ON        0.97     
!   OV        1.00     PT        1.01     SC        1.07     TS        1.04     
!   WF        0.99     WZ        0.96     GN        1.02     NL        0.99     
! 
! 
! Correcting IF 4.
!  A total of 144 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        1.01     GC        0.95     HH        1.00*    
!   HN        0.93     KK        1.00     KP        0.97     LA        1.02     
!   MC        1.04     MK        0.97     NY        1.00     ON        1.02     
!   OV        0.99     PT        1.02     SC        1.07     TS        1.01     
!   WF        0.99     WZ        1.04     GN        0.97     NL        1.00*    
! 
!  A total of 333 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.98     FD        1.03     GC        1.00     HH        1.00*    
!   HN        1.07     KK        1.03     KP        0.97     LA        1.01     
!   MC        0.99     MK        1.04     NY        1.02     ON        0.97     
!   OV        0.99     PT        1.00     SC        1.11     TS        0.96     
!   WF        1.05     WZ        0.97     GN        1.00     NL        0.98     
! 
!  A total of 15 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00     FD        1.03     GC        1.02     HH        1.00*    
!   HN        0.94     KK        1.07     KP        0.99     LA        1.01     
!   MC        0.95     MK        1.02     NY        1.00     ON        0.98     
!   OV        0.99     PT        1.00     SC        1.05     TS        1.01     
!   WF        1.04     WZ        0.97     GN        0.99     NL        0.98     
! 
! 
! Fit before self-cal, rms=0.205825Jy  sigma=0.001295
! Fit after  self-cal, rms=0.205252Jy  sigma=0.001265
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! Estimated beam: bmin=0.6691 mas, bmaj=0.7193 mas, bpa=-72.5 degrees
! Estimated noise=244.398 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 (2.6, -2.6).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00055696 Jy
! Component: 100  -  total flux cleaned = 0.000790851 Jy
! Component: 150  -  total flux cleaned = 0.000984823 Jy
! Component: 200  -  total flux cleaned = 0.00132768 Jy
! Total flux subtracted in 200 components = 0.00132768 Jy
! Clean residual min=-0.002928 max=0.004140 Jy/beam
! Clean residual mean=-0.000036 rms=0.000725 Jy/beam
! Combined flux in latest and established models = 0.796718 Jy
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 59 components and 0.796718 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.205111Jy  sigma=0.001264
! Fit after  self-cal, rms=0.205145Jy  sigma=0.001264
! Inverting map 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! Added new window around map position (-2.6, 2.6).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00220767 Jy
! Component: 100  -  total flux cleaned = 0.00237523 Jy
! Component: 150  -  total flux cleaned = 0.00245164 Jy
! Component: 200  -  total flux cleaned = 0.00238242 Jy
! Total flux subtracted in 200 components = 0.00238242 Jy
! Clean residual min=-0.003023 max=0.003273 Jy/beam
! Clean residual mean=-0.000053 rms=0.000704 Jy/beam
! Combined flux in latest and established models = 0.799101 Jy
! Performing phase self-cal
! Adding 21 model components to the UV plane model.
! The established model now contains 67 components and 0.799101 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.205073Jy  sigma=0.001263
! Fit after  self-cal, rms=0.205067Jy  sigma=0.001263
! Inverting map 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 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=0.205067Jy  sigma=0.001263
! Fit after  self-cal, rms=0.204733Jy  sigma=0.001244
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! Estimated beam: bmin=0.6678 mas, bmaj=0.7207 mas, bpa=-73.07 degrees
! Estimated noise=244.612 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00111552 Jy
! Component: 100  -  total flux cleaned = -0.0015253 Jy
! Component: 150  -  total flux cleaned = -0.00185767 Jy
! Component: 200  -  total flux cleaned = -0.00234359 Jy
! Total flux subtracted in 200 components = -0.00234359 Jy
! Clean residual min=-0.001741 max=0.001559 Jy/beam
! Clean residual mean=-0.000015 rms=0.000385 Jy/beam
! Combined flux in latest and established models = 0.796757 Jy
selfcal
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 77 components and 0.796757 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.204643Jy  sigma=0.001242
! Fit after  self-cal, rms=0.204649Jy  sigma=0.001242
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 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 = -0.000242742 Jy
! Component: 100  -  total flux cleaned = -0.000296557 Jy
! Component: 150  -  total flux cleaned = -0.000298424 Jy
! Component: 200  -  total flux cleaned = -0.000386645 Jy
! Total flux subtracted in 200 components = -0.000386645 Jy
! Clean residual min=-0.001733 max=0.001444 Jy/beam
! Clean residual mean=-0.000013 rms=0.000375 Jy/beam
! Combined flux in latest and established models = 0.796371 Jy
! Performing phase self-cal
! Adding 27 model components to the UV plane model.
! The established model now contains 86 components and 0.796371 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.204626Jy  sigma=0.001242
! Fit after  self-cal, rms=0.204627Jy  sigma=0.001242
! Inverting map 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 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=0.204627Jy  sigma=0.001242
! Fit after  self-cal, rms=0.205293Jy  sigma=0.001241
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! Estimated beam: bmin=0.6672 mas, bmaj=0.7204 mas, bpa=-73.45 degrees
! Estimated noise=244.691 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00048486 Jy
! Component: 100  -  total flux cleaned = -0.00102135 Jy
! Component: 150  -  total flux cleaned = -0.00136276 Jy
! Component: 200  -  total flux cleaned = -0.00160932 Jy
! Total flux subtracted in 200 components = -0.00160932 Jy
! Clean residual min=-0.001556 max=0.001474 Jy/beam
! Clean residual mean=0.000002 rms=0.000342 Jy/beam
! Combined flux in latest and established models = 0.794761 Jy
selfcal
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 90 components and 0.794761 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.205259Jy  sigma=0.001240
! Fit after  self-cal, rms=0.205268Jy  sigma=0.001240
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 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 = -0.000179651 Jy
! Component: 100  -  total flux cleaned = -0.000299868 Jy
! Component: 150  -  total flux cleaned = -0.000336172 Jy
! Component: 200  -  total flux cleaned = -0.000336278 Jy
! Total flux subtracted in 200 components = -0.000336278 Jy
! Clean residual min=-0.001563 max=0.001369 Jy/beam
! Clean residual mean=0.000004 rms=0.000336 Jy/beam
! Combined flux in latest and established models = 0.794425 Jy
! Performing phase self-cal
! Adding 27 model components to the UV plane model.
! The established model now contains 96 components and 0.794425 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.205256Jy  sigma=0.001240
! Fit after  self-cal, rms=0.205256Jy  sigma=0.001240
! Inverting map 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 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=0.205256Jy  sigma=0.001240
! Fit after  self-cal, rms=0.205493Jy  sigma=0.001240
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! Estimated beam: bmin=2.323 mas, bmaj=2.679 mas, bpa=-40.74 degrees
! Estimated noise=369.442 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000506548 Jy
! Component: 100  -  total flux cleaned = 0.000381751 Jy
! Component: 150  -  total flux cleaned = 0.000302047 Jy
! Component: 200  -  total flux cleaned = 0.000233499 Jy
! Total flux subtracted in 200 components = 0.000233499 Jy
! Clean residual min=-0.001621 max=0.001865 Jy/beam
! Clean residual mean=0.000020 rms=0.000542 Jy/beam
! Combined flux in latest and established models = 0.794659 Jy
selfcal
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 101 components and 0.794659 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.205490Jy  sigma=0.001240
! Fit after  self-cal, rms=0.205493Jy  sigma=0.001240
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 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 = 0.00011795 Jy
! Component: 100  -  total flux cleaned = 7.52418e-05 Jy
! Component: 150  -  total flux cleaned = 5.69077e-05 Jy
! Component: 200  -  total flux cleaned = 7.54485e-05 Jy
! Total flux subtracted in 200 components = 7.54485e-05 Jy
! Clean residual min=-0.001596 max=0.001864 Jy/beam
! Clean residual mean=0.000018 rms=0.000538 Jy/beam
! Combined flux in latest and established models = 0.794734 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 104 components and 0.794734 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.205494Jy  sigma=0.001240
! Fit after  self-cal, rms=0.205494Jy  sigma=0.001240
! Inverting map 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
win_mult = win_mult / 1.2
print "************** FINISHED AMPLITUDE SELF-CAL **************"
! ************** FINISHED AMPLITUDE SELF-CAL ************** 
restore
! Inverting map and beam 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! Estimated beam: bmin=0.6668 mas, bmaj=0.7204 mas, bpa=-73.62 degrees
! Estimated noise=244.781 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6668 x 0.7204 at -73.62 degrees (North through East)
! Clean map  min=-0.0011492  max=0.7309 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=0.205494Jy  sigma=0.001240
! Fit after  self-cal, rms=0.199869Jy  sigma=0.001178
! Inverting map and beam 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! Estimated beam: bmin=0.667 mas, bmaj=0.7205 mas, bpa=-73.48 degrees
! Estimated noise=244.693 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00109576 Jy
! Component: 100  -  total flux cleaned = -0.00147634 Jy
! Component: 150  -  total flux cleaned = -0.00187816 Jy
! Component: 200  -  total flux cleaned = -0.0021362 Jy
! Total flux subtracted in 200 components = -0.0021362 Jy
! Clean residual min=-0.001248 max=0.001190 Jy/beam
! Clean residual mean=0.000011 rms=0.000309 Jy/beam
! Combined flux in latest and established models = 0.792598 Jy
! Performing phase self-cal
! Adding 27 model components to the UV plane model.
! The established model now contains 116 components and 0.792598 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.199854Jy  sigma=0.001178
! Fit after  self-cal, rms=0.199852Jy  sigma=0.001178
! Inverting map 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000179216 Jy
! Component: 100  -  total flux cleaned = -0.0003157 Jy
! Component: 150  -  total flux cleaned = -0.0004177 Jy
! Component: 200  -  total flux cleaned = -0.000465408 Jy
! Total flux subtracted in 200 components = -0.000465408 Jy
! Clean residual min=-0.001236 max=0.001178 Jy/beam
! Clean residual mean=0.000015 rms=0.000307 Jy/beam
! Combined flux in latest and established models = 0.792132 Jy
! Performing phase self-cal
! Adding 33 model components to the UV plane model.
! The established model now contains 121 components and 0.792132 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.199847Jy  sigma=0.001178
! Fit after  self-cal, rms=0.199847Jy  sigma=0.001178
! Inverting map 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.199847Jy  sigma=0.001178
! Fit after  self-cal, rms=0.199990Jy  sigma=0.001178
print "************** CLEARING MODEL AND STARTING OVER **********"
! ************** CLEARING MODEL AND STARTING OVER ********** 
clrmod true
! clrmod: Cleared the established and tentative models.
uvw 2,-1
! Uniform weighting binwidth: 2 (pixels).
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! Estimated beam: bmin=0.532 mas, bmaj=0.5566 mas, bpa=85.84 degrees
! Estimated noise=513.182 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.55748 Jy
! Component: 100  -  total flux cleaned = 0.679048 Jy
! Component: 150  -  total flux cleaned = 0.714244 Jy
! Component: 200  -  total flux cleaned = 0.733374 Jy
! Total flux subtracted in 200 components = 0.733374 Jy
! Clean residual min=-0.002788 max=0.009921 Jy/beam
! Clean residual mean=0.000035 rms=0.000806 Jy/beam
! Combined flux in latest and established models = 0.733374 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 8 model components to the UV plane model.
! The established model now contains 8 components and 0.733374 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! Estimated beam: bmin=0.6668 mas, bmaj=0.7205 mas, bpa=-73.54 degrees
! Estimated noise=244.699 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 = 0.0233069 Jy
! Component: 100  -  total flux cleaned = 0.0354958 Jy
! Component: 150  -  total flux cleaned = 0.0424011 Jy
! Component: 200  -  total flux cleaned = 0.0468159 Jy
! Total flux subtracted in 200 components = 0.0468159 Jy
! Clean residual min=-0.001069 max=0.002581 Jy/beam
! Clean residual mean=0.000108 rms=0.000437 Jy/beam
! Combined flux in latest and established models = 0.780189 Jy
! Adding 31 model components to the UV plane model.
! The established model now contains 32 components and 0.780189 Jy
! Inverting map 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! Added new window around map position (-0.6, -1).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00308838 Jy
! Component: 100  -  total flux cleaned = 0.00531879 Jy
! Component: 150  -  total flux cleaned = 0.00699445 Jy
! Component: 200  -  total flux cleaned = 0.00828122 Jy
! Total flux subtracted in 200 components = 0.00828122 Jy
! Clean residual min=-0.001137 max=0.001226 Jy/beam
! Clean residual mean=0.000041 rms=0.000315 Jy/beam
! Combined flux in latest and established models = 0.788471 Jy
! Adding 35 model components to the UV plane model.
! The established model now contains 56 components and 0.788471 Jy
! Inverting map 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! Estimated beam: bmin=2.324 mas, bmaj=2.682 mas, bpa=-40.89 degrees
! Estimated noise=368.835 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00214758 Jy
! Component: 100  -  total flux cleaned = 0.00320317 Jy
! Component: 150  -  total flux cleaned = 0.00343203 Jy
! Component: 200  -  total flux cleaned = 0.00354839 Jy
! Total flux subtracted in 200 components = 0.00354839 Jy
! Clean residual min=-0.001461 max=0.001630 Jy/beam
! Clean residual mean=0.000049 rms=0.000464 Jy/beam
! Combined flux in latest and established models = 0.792019 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 = 6.22481e-05 Jy
! Component: 100  -  total flux cleaned = 0.000114016 Jy
! Component: 150  -  total flux cleaned = 0.000146731 Jy
! Component: 200  -  total flux cleaned = 0.000165718 Jy
! Total flux subtracted in 200 components = 0.000165718 Jy
! Clean residual min=-0.001418 max=0.001620 Jy/beam
! Clean residual mean=0.000043 rms=0.000459 Jy/beam
! Combined flux in latest and established models = 0.792185 Jy
! Adding 35 model components to the UV plane model.
! The established model now contains 82 components and 0.792185 Jy
! Inverting map 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! Estimated beam: bmin=0.6668 mas, bmaj=0.7205 mas, bpa=-73.54 degrees
! Estimated noise=244.699 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00051544 Jy
! Component: 100  -  total flux cleaned = -0.000723833 Jy
! Component: 150  -  total flux cleaned = -0.000776801 Jy
! Component: 200  -  total flux cleaned = -0.000752892 Jy
! Total flux subtracted in 200 components = -0.000752892 Jy
! Clean residual min=-0.001181 max=0.001170 Jy/beam
! Clean residual mean=0.000017 rms=0.000298 Jy/beam
! Combined flux in latest and established models = 0.791432 Jy
selfcal
! Performing phase self-cal
! Adding 26 model components to the UV plane model.
! The established model now contains 101 components and 0.791432 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.199971Jy  sigma=0.001177
! Fit after  self-cal, rms=0.199969Jy  sigma=0.001177
wmodel J1357+7643_X_1999_12_20_pus_map.mod
! Writing 101 model components to file: J1357+7643_X_1999_12_20_pus_map.mod
wobs J1357+7643_X_1999_12_20_pus_uvs.fits
! Writing UV FITS file: J1357+7643_X_1999_12_20_pus_uvs.fits
wwins J1357+7643_X_1999_12_20_pus_map.win
! wwins: Wrote 6 windows to J1357+7643_X_1999_12_20_pus_map.win
x = (field_size-8) * field_cell / 4
addwin -x,x,-x,x
clean (field_size*4),0.01
! Inverting map 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 2.0997e-05 Jy
! Component: 100  -  total flux cleaned = -1.83939e-05 Jy
! Component: 150  -  total flux cleaned = 9.35478e-05 Jy
! Component: 200  -  total flux cleaned = 0.000201799 Jy
! Component: 250  -  total flux cleaned = 0.000376823 Jy
! Component: 300  -  total flux cleaned = 0.000530428 Jy
! Component: 350  -  total flux cleaned = 0.000730899 Jy
! Component: 400  -  total flux cleaned = 0.000861871 Jy
! Component: 450  -  total flux cleaned = 0.000958694 Jy
! Component: 500  -  total flux cleaned = 0.00102225 Jy
! Component: 550  -  total flux cleaned = 0.00106931 Jy
! Component: 600  -  total flux cleaned = 0.00111569 Jy
! Component: 650  -  total flux cleaned = 0.00111574 Jy
! Component: 700  -  total flux cleaned = 0.00114601 Jy
! Component: 750  -  total flux cleaned = 0.00114585 Jy
! Component: 800  -  total flux cleaned = 0.00114577 Jy
! Component: 850  -  total flux cleaned = 0.00113107 Jy
! Component: 900  -  total flux cleaned = 0.00117503 Jy
! Component: 950  -  total flux cleaned = 0.00117504 Jy
! Component: 1000  -  total flux cleaned = 0.00123269 Jy
! Total flux subtracted in 1024 components = 0.0012327 Jy
! Clean residual min=-0.000831 max=0.000831 Jy/beam
! Clean residual mean=0.000005 rms=0.000273 Jy/beam
! Combined flux in latest and established models = 0.792665 Jy
keep
! Adding 88 model components to the UV plane model.
! The established model now contains 189 components and 0.792665 Jy
![Exited script file: muppet]
wmap "J1357+7643_X_1999_12_20_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6668 x 0.7205 at -73.54 degrees (North through East)
! Clean map  min=-0.00092353  max=0.73161 Jy/beam
! Writing clean map to FITS file: J1357+7643_X_1999_12_20_pus_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.731605 
invert
! Inverting map 
! Your choice of large map pixels excluded 3.52% of the data.
!  The x-axis pixel size should ideally be below 0.1534 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1563 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000272462 
device "J1357+7643_X_1999_12_20_pus\_map.eps/VPS"
! Attempting to open device: 'J1357+7643_X_1999_12_20_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.111725 0.111725 0.22345 0.446901 0.893802 1.7876 3.57521 7.15041 14.3008 28.6016 57.2033
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0008 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.731 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6668 x 0.7205 at -73.54 degrees (North through East)
! Clean map  min=-0.00092353  max=0.73161 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1357+7643_X_1999_12_20_pus\_map.gif/vgif"
! Attempting to open device: 'J1357+7643_X_1999_12_20_pus_map.gif/vgif'
mapplot cln
quit
! Quitting program
! Log file J1357+7643_X_1999_12_20_pus_uvs.log closed on Fri Dec 14 17:23:39 2007