! Started logfile: 0727-115_X.log on Mon Mar  3 23:01:59 2008
observe 0727-115_X.edt
! Reading UV FITS file: 0727-115_X.edt
! AN table 1: 15 integrations on 136 of 136 possible baselines.
! AN table 2: 11 integrations on 136 of 136 possible baselines.
! AN table 3: 8 integrations on 136 of 136 possible baselines.
! AN table 4: 45 integrations on 136 of 136 possible baselines.
! Apparent sampling: 0.113273 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: 0727-115
! 
! 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 1230 lines of history.
! 
! Reading 4868 visibilities.
![@gonzo7-0.1 0727-115_X]
print "***********************************"
! *********************************** 
print "*** Using gonzo instruction set ***"
! *** Using gonzo instruction set *** 
print "***********************************"
! *********************************** 
float field_size
field_size = 1024
float field_cell
field_cell = 0.1
integer clean_niter
clean_niter = 50
float clean_gain
clean_gain = 0.03
float dynam
dynam = 7.0
float win_mult
win_mult = 1.8
float solint
solint = 3.6/6.0
logical doflt
doflt = true
logical doamp
float new_peak
float flux_cutoff
mapsize field_size,field_cell
! Map grid = 1024x1024 pixels with 0.100x0.100 milli-arcsec cellsize.
select
! 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
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 255 telescope corrections were flagged in sub-array 1.
!  A total of 106 telescope corrections were flagged in sub-array 2.
!  A total of 101 telescope corrections were flagged in sub-array 3.
!  A total of 644 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 2.
!  A total of 255 telescope corrections were flagged in sub-array 1.
!  A total of 105 telescope corrections were flagged in sub-array 2.
!  A total of 101 telescope corrections were flagged in sub-array 3.
!  A total of 644 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 3.
!  A total of 255 telescope corrections were flagged in sub-array 1.
!  A total of 105 telescope corrections were flagged in sub-array 2.
!  A total of 101 telescope corrections were flagged in sub-array 3.
!  A total of 644 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 4.
!  A total of 255 telescope corrections were flagged in sub-array 1.
!  A total of 105 telescope corrections were flagged in sub-array 2.
!  A total of 101 telescope corrections were flagged in sub-array 3.
!  A total of 645 telescope corrections were flagged in sub-array 4.
! 
! Fit before self-cal, rms=1.390499Jy  sigma=0.023188
! Fit after  self-cal, rms=1.390446Jy  sigma=0.023191
! clrmod: Cleared the established, tentative and continuum models.
! Redundant starting model cleared.
uvweight 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.
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=0.6751 mas, bmaj=1.929 mas, bpa=-4.684 degrees
! Estimated noise=1317.85 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal doamp, doflt, solint
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (0, 0).
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 1.75163 Jy
! Total flux subtracted in 50 components = 1.75163 Jy
! Clean residual min=-0.106763 max=0.488537 Jy/beam
! Clean residual mean=-0.000706 rms=0.035790 Jy/beam
! Combined flux in latest and established models = 1.75163 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 1 model components to the UV plane model.
! The established model now contains 1 components and 1.75163 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.687017Jy  sigma=0.011769
! Fit after  self-cal, rms=0.687015Jy  sigma=0.011769
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.436759 Jy
! Total flux subtracted in 50 components = 0.436759 Jy
! Clean residual min=-0.051444 max=0.184725 Jy/beam
! Clean residual mean=-0.000423 rms=0.017420 Jy/beam
! Combined flux in latest and established models = 2.18839 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 11 model components to the UV plane model.
! The established model now contains 11 components and 2.18839 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.347931Jy  sigma=0.006001
! Fit after  self-cal, rms=0.347987Jy  sigma=0.006000
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.200736 Jy
! Total flux subtracted in 50 components = 0.200736 Jy
! Clean residual min=-0.030326 max=0.093224 Jy/beam
! Clean residual mean=-0.000286 rms=0.010137 Jy/beam
! Combined flux in latest and established models = 2.38913 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 8 model components to the UV plane model.
! The established model now contains 17 components and 2.38913 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.214772Jy  sigma=0.003656
! Fit after  self-cal, rms=0.214531Jy  sigma=0.003655
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.106044 Jy
! Total flux subtracted in 50 components = 0.106044 Jy
! Clean residual min=-0.020599 max=0.052477 Jy/beam
! Clean residual mean=-0.000215 rms=0.006781 Jy/beam
! Combined flux in latest and established models = 2.49517 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 12 model components to the UV plane model.
! The established model now contains 24 components and 2.49517 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.157657Jy  sigma=0.002597
! Fit after  self-cal, rms=0.157622Jy  sigma=0.002596
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.061622 Jy
! Total flux subtracted in 50 components = 0.061622 Jy
! Clean residual min=-0.017328 max=0.042936 Jy/beam
! Clean residual mean=-0.000179 rms=0.005185 Jy/beam
! Combined flux in latest and established models = 2.55679 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 19 model components to the UV plane model.
! The established model now contains 39 components and 2.55679 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.132690Jy  sigma=0.002105
! Fit after  self-cal, rms=0.132673Jy  sigma=0.002104
! Inverting map 
! Added new window around map position (-1.9, 1.8).
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0448517 Jy
! Total flux subtracted in 50 components = 0.0448517 Jy
! Clean residual min=-0.015316 max=0.024094 Jy/beam
! Clean residual mean=-0.000140 rms=0.004123 Jy/beam
! Combined flux in latest and established models = 2.60164 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 18 model components to the UV plane model.
! The established model now contains 52 components and 2.60164 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.117434Jy  sigma=0.001783
! Fit after  self-cal, rms=0.116608Jy  sigma=0.001779
! Inverting map 
print "****************************************"
! **************************************** 
print "*** Finished Uniform Weighting CLEAN ***"
! *** Finished Uniform Weighting CLEAN *** 
print "****************************************"
! **************************************** 
uvweight 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
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=0.8571 mas, bmaj=2.686 mas, bpa=-8.107 degrees
! Estimated noise=754.244 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal doamp, doflt, solint
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0500505 Jy
! Component: 100  -  total flux cleaned = 0.0806542 Jy
! Total flux subtracted in 100 components = 0.0806542 Jy
! Clean residual min=-0.011114 max=0.019298 Jy/beam
! Clean residual mean=-0.000141 rms=0.003978 Jy/beam
! Combined flux in latest and established models = 2.6823 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 49 model components to the UV plane model.
! The established model now contains 95 components and 2.6823 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.098221Jy  sigma=0.001350
! Fit after  self-cal, rms=0.096690Jy  sigma=0.001333
! Inverting map 
print "****************************************"
! **************************************** 
print "*** Finished Natural Weighting CLEAN ***"
! *** Finished Natural Weighting CLEAN *** 
print "****************************************"
! **************************************** 
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*    HN        0.00*    
!   KK        0.00*    KP        0.00*    LA        0.00*    MC        0.00*    
!   MK        0.00*    NL        0.00*    NY        0.00*    ON        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    WF        0.00*    
!   WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        1.00     GC        1.00*    HN        1.00     
!   KK        1.01     KP        0.99     LA        0.99     MC        1.00*    
!   MK        1.00*    NL        1.00     NY        1.00*    ON        1.00*    
!   OV        1.00     PT        0.99     SC        1.01     WF        1.00     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        0.99     GC        1.00*    HN        1.00*    
!   KK        1.00*    KP        0.99     LA        0.99     MC        1.00*    
!   MK        1.00*    NL        1.00*    NY        1.00*    ON        1.00*    
!   OV        1.00*    PT        0.99     SC        1.00     WF        1.00*    
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00     FD        1.00     GC        1.00*    HN        1.00     
!   KK        1.00     KP        0.99     LA        0.99     MC        1.00*    
!   MK        1.00     NL        1.00     NY        1.00*    ON        1.00*    
!   OV        1.00     PT        0.99     SC        1.01     WF        1.00     
!   WZ        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.00*    FD        0.00*    GC        0.00*    HN        0.00*    
!   KK        0.00*    KP        0.00*    LA        0.00*    MC        0.00*    
!   MK        0.00*    NL        0.00*    NY        0.00*    ON        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    WF        0.00*    
!   WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        1.00     GC        1.00*    HN        1.00     
!   KK        1.00     KP        0.99     LA        0.99     MC        1.00*    
!   MK        1.00*    NL        1.00     NY        1.00*    ON        1.00*    
!   OV        1.00     PT        0.99     SC        1.01     WF        1.00     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        0.99     GC        1.00*    HN        1.00*    
!   KK        1.00*    KP        0.99     LA        0.99     MC        1.00*    
!   MK        1.00*    NL        1.00*    NY        1.00*    ON        1.00*    
!   OV        1.00*    PT        0.99     SC        1.00     WF        1.00*    
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00     FD        1.00     GC        1.00*    HN        1.00     
!   KK        1.00     KP        0.99     LA        0.99     MC        1.00*    
!   MK        1.00     NL        1.00     NY        1.00*    ON        1.00*    
!   OV        1.00     PT        0.99     SC        1.01     WF        1.00     
!   WZ        1.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.00*    FD        0.00*    GC        0.00*    HN        0.00*    
!   KK        0.00*    KP        0.00*    LA        0.00*    MC        0.00*    
!   MK        0.00*    NL        0.00*    NY        0.00*    ON        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    WF        0.00*    
!   WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        1.00     GC        1.00*    HN        1.00     
!   KK        1.00     KP        0.99     LA        0.99     MC        1.00*    
!   MK        1.00*    NL        1.00     NY        1.00*    ON        1.00*    
!   OV        1.00     PT        0.99     SC        1.01     WF        1.00     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        0.99     GC        1.00*    HN        1.00*    
!   KK        1.00*    KP        0.99     LA        0.99     MC        1.00*    
!   MK        1.00*    NL        1.00*    NY        1.00*    ON        1.00*    
!   OV        1.00*    PT        0.99     SC        1.01     WF        1.00*    
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00     FD        1.00     GC        1.00*    HN        1.00     
!   KK        1.00     KP        0.99     LA        0.99     MC        1.00*    
!   MK        1.00     NL        1.00     NY        1.00*    ON        1.00*    
!   OV        1.00     PT        0.99     SC        1.01     WF        1.00     
!   WZ        1.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.00*    FD        0.00*    GC        0.00*    HN        0.00*    
!   KK        0.00*    KP        0.00*    LA        0.00*    MC        0.00*    
!   MK        0.00*    NL        0.00*    NY        0.00*    ON        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    WF        0.00*    
!   WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        1.00     GC        1.00*    HN        1.00     
!   KK        1.00     KP        0.99     LA        0.99     MC        1.00*    
!   MK        1.00*    NL        1.00     NY        1.00*    ON        1.00*    
!   OV        1.00     PT        0.99     SC        1.01     WF        0.99     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        0.99     GC        1.00*    HN        1.00*    
!   KK        1.00*    KP        0.99     LA        0.99     MC        1.00*    
!   MK        1.00*    NL        1.00*    NY        1.00*    ON        1.00*    
!   OV        1.00*    PT        0.99     SC        1.00     WF        1.00*    
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00     FD        1.00     GC        1.00*    HN        1.00     
!   KK        1.00     KP        0.99     LA        0.99     MC        1.00*    
!   MK        1.00     NL        1.00     NY        1.00*    ON        1.00*    
!   OV        1.00     PT        0.99     SC        1.01     WF        1.00     
!   WZ        1.00*    
! 
! 
! Fit before self-cal, rms=0.096690Jy  sigma=0.001333
! Fit after  self-cal, rms=0.094347Jy  sigma=0.001277
dynam = dynam - 0.5
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=0.8591 mas, bmaj=2.698 mas, bpa=-8.15 degrees
! Estimated noise=749.853 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal doamp, doflt, solint
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0145772 Jy
! Component: 100  -  total flux cleaned = 0.0220523 Jy
! Total flux subtracted in 100 components = 0.0220523 Jy
! Clean residual min=-0.007872 max=0.012377 Jy/beam
! Clean residual mean=0.000011 rms=0.002397 Jy/beam
! Combined flux in latest and established models = 2.70435 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 26 model components to the UV plane model.
! The established model now contains 112 components and 2.70435 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.092748Jy  sigma=0.001233
! Fit after  self-cal, rms=0.092270Jy  sigma=0.001229
! Inverting map 
dynam = dynam - 1.0
doamp = true
solint = solint * (6.0/3.6)
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 doamp, doflt, solint
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (-0.6, 10.2).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0118033 Jy
! Component: 100  -  total flux cleaned = 0.0184857 Jy
! Total flux subtracted in 100 components = 0.0184857 Jy
! Clean residual min=-0.008261 max=0.010570 Jy/beam
! Clean residual mean=0.000021 rms=0.002090 Jy/beam
! Combined flux in latest and established models = 2.72283 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 24 model components to the UV plane model.
! The established model now contains 135 components and 2.72283 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.090897Jy  sigma=0.001203
! Fit after  self-cal, rms=0.090200Jy  sigma=0.001195
! Inverting map and beam 
! Estimated beam: bmin=0.8585 mas, bmaj=2.696 mas, bpa=-8.159 degrees
! Estimated noise=750.078 mJy/beam.
! Added new window around map position (-3.7, 0.8).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0106665 Jy
! Component: 100  -  total flux cleaned = 0.0161968 Jy
! Total flux subtracted in 100 components = 0.0161968 Jy
! Clean residual min=-0.006172 max=0.008017 Jy/beam
! Clean residual mean=0.000003 rms=0.001744 Jy/beam
! Combined flux in latest and established models = 2.73903 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 19 model components to the UV plane model.
! The established model now contains 152 components and 2.73903 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.089048Jy  sigma=0.001171
! Fit after  self-cal, rms=0.088700Jy  sigma=0.001167
! Inverting map and beam 
! Estimated beam: bmin=0.8582 mas, bmaj=2.696 mas, bpa=-8.165 degrees
! Estimated noise=749.948 mJy/beam.
doamp = false
solint = solint / (6.0/3.6)
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 doamp, doflt, solint
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00659703 Jy
! Component: 100  -  total flux cleaned = 0.0100911 Jy
! Total flux subtracted in 100 components = 0.0100911 Jy
! Clean residual min=-0.005612 max=0.007384 Jy/beam
! Clean residual mean=-0.000004 rms=0.001572 Jy/beam
! Combined flux in latest and established models = 2.74912 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 26 model components to the UV plane model.
! The established model now contains 168 components and 2.74912 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.088186Jy  sigma=0.001157
! Fit after  self-cal, rms=0.088103Jy  sigma=0.001157
! Inverting map 
print "***********************************"
! *********************************** 
print "*** Finished Amplitude Self-Cal ***"
! *** Finished Amplitude Self-Cal *** 
print "***********************************"
! *********************************** 
save 0727-115_X
! Writing UV FITS file: 0727-115_X.uvf
! Writing 168 model components to file: 0727-115_X.mod
! wwins: Wrote 4 windows to 0727-115_X.win
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8582 x 2.696 at -8.165 degrees (North through East)
! Clean map  min=-0.0054045  max=2.3381 Jy/beam
! Writing clean map to FITS file: 0727-115_X.fits
! Writing difmap environment to: 0727-115_X.par
print "****************************"
! **************************** 
print "*** Now, make some plots ***"
! *** Now, make some plots *** 
print "****************************"
! **************************** 
![@gonzo_plot 0727-115_X]
device 0727-115_Xuv.ps/vps,1,2
! Attempting to open device: '0727-115_Xuv.ps/vps'
radplot
! Using default options string "m1"
uvplot
! Using default options string ""
device 0727-115_Xim.ps/vps
! Attempting to open device: '0727-115_Xim.ps/vps'
uvweight 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.
loglevs -1,2048,2
! The new contour levels are:
!  -1 1 2 4 8 16 32 64 128 256 512 1024 2048
cmul = imstat(rms)*3
! Inverting map and beam 
! Estimated beam: bmin=0.8582 mas, bmaj=2.696 mas, bpa=-8.165 degrees
! Estimated noise=749.948 mJy/beam.
mappl cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8582 x 2.696 at -8.165 degrees (North through East)
! Clean map  min=-0.0054045  max=2.3381 Jy/beam
![Exited script file: gonzo_plot]
![Exited script file: gonzo7-0.1]
quit
! Quitting program
! Log file 0727-115_X.log closed on Mon Mar  3 23:02:06 2008