! Started logfile: 1606+106_X.log on Tue Mar 25 11:13:29 2008
observe 1606+106_X.edt
! Reading UV FITS file: 1606+106_X.edt
! AN table 1: 46 integrations on 136 of 136 possible baselines.
! AN table 2: 13 integrations on 136 of 136 possible baselines.
! AN table 3: 88 integrations on 136 of 136 possible baselines.
! Apparent sampling: 0.165416 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: 1606+106
! 
! 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 1222 lines of history.
! 
! Reading 13228 visibilities.
![@gonzo8-0.1 1606+106_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 = 8.0
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 607 telescope corrections were flagged in sub-array 1.
!  A total of 182 telescope corrections were flagged in sub-array 2.
!  A total of 1346 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 606 telescope corrections were flagged in sub-array 1.
!  A total of 181 telescope corrections were flagged in sub-array 2.
!  A total of 1340 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 607 telescope corrections were flagged in sub-array 1.
!  A total of 175 telescope corrections were flagged in sub-array 2.
!  A total of 1335 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 628 telescope corrections were flagged in sub-array 1.
!  A total of 175 telescope corrections were flagged in sub-array 2.
!  A total of 1340 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=0.347388Jy  sigma=0.005200
! Fit after  self-cal, rms=0.341992Jy  sigma=0.005053
! 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=0.557 mas, bmaj=1.37 mas, bpa=-8.629 degrees
! Estimated noise=1077.36 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 = 0.518572 Jy
! Total flux subtracted in 50 components = 0.518572 Jy
! Clean residual min=-0.023442 max=0.147044 Jy/beam
! Clean residual mean=-0.000038 rms=0.008316 Jy/beam
! Combined flux in latest and established models = 0.518572 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 2 model components to the UV plane model.
! The established model now contains 2 components and 0.518572 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.280121Jy  sigma=0.005116
! Fit after  self-cal, rms=0.280093Jy  sigma=0.005115
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.153417 Jy
! Total flux subtracted in 50 components = 0.153417 Jy
! Clean residual min=-0.014389 max=0.067621 Jy/beam
! Clean residual mean=-0.000012 rms=0.005052 Jy/beam
! Combined flux in latest and established models = 0.671988 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 7 model components to the UV plane model.
! The established model now contains 8 components and 0.671988 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.182727Jy  sigma=0.003304
! Fit after  self-cal, rms=0.181397Jy  sigma=0.003296
! Inverting map 
! Added new window around map position (-0.6, 0.3).
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0781073 Jy
! Total flux subtracted in 50 components = 0.0781073 Jy
! Clean residual min=-0.011260 max=0.039709 Jy/beam
! Clean residual mean=-0.000000 rms=0.003661 Jy/beam
! Combined flux in latest and established models = 0.750096 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 18 components and 0.750096 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.142444Jy  sigma=0.002499
! Fit after  self-cal, rms=0.141026Jy  sigma=0.002491
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0502178 Jy
! Total flux subtracted in 50 components = 0.0502178 Jy
! Clean residual min=-0.009487 max=0.029582 Jy/beam
! Clean residual mean=0.000007 rms=0.002869 Jy/beam
! Combined flux in latest and established models = 0.800313 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 20 model components to the UV plane model.
! The established model now contains 31 components and 0.800313 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.120063Jy  sigma=0.002029
! Fit after  self-cal, rms=0.119074Jy  sigma=0.002024
! Inverting map 
! Added new window around map position (-1.3, 0.9).
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.036305 Jy
! Total flux subtracted in 50 components = 0.036305 Jy
! Clean residual min=-0.007718 max=0.019574 Jy/beam
! Clean residual mean=0.000013 rms=0.002354 Jy/beam
! Combined flux in latest and established models = 0.836618 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 47 components and 0.836618 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.106185Jy  sigma=0.001724
! Fit after  self-cal, rms=0.105479Jy  sigma=0.001719
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0267419 Jy
! Total flux subtracted in 50 components = 0.0267419 Jy
! Clean residual min=-0.006742 max=0.015026 Jy/beam
! Clean residual mean=0.000017 rms=0.002007 Jy/beam
! Combined flux in latest and established models = 0.86336 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 28 model components to the UV plane model.
! The established model now contains 69 components and 0.86336 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.097468Jy  sigma=0.001521
! Fit after  self-cal, rms=0.097046Jy  sigma=0.001519
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0206703 Jy
! Total flux subtracted in 50 components = 0.0206703 Jy
! Clean residual min=-0.006081 max=0.011770 Jy/beam
! Clean residual mean=0.000020 rms=0.001769 Jy/beam
! Combined flux in latest and established models = 0.884031 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 25 model components to the UV plane model.
! The established model now contains 83 components and 0.884031 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.091828Jy  sigma=0.001384
! Fit after  self-cal, rms=0.091533Jy  sigma=0.001382
! 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=0.6924 mas, bmaj=1.684 mas, bpa=-9.768 degrees
! Estimated noise=637.027 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 = 0.0316928 Jy
! Component: 100  -  total flux cleaned = 0.0510857 Jy
! Total flux subtracted in 100 components = 0.0510857 Jy
! Clean residual min=-0.005354 max=0.011803 Jy/beam
! Clean residual mean=0.000312 rms=0.002021 Jy/beam
! Combined flux in latest and established models = 0.935116 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 57 model components to the UV plane model.
! The established model now contains 122 components and 0.935116 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.083127Jy  sigma=0.001142
! Fit after  self-cal, rms=0.082428Jy  sigma=0.001135
! 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        1.00     FD        0.99     GC        1.03     HN        1.01     
!   KK        1.00*    KP        0.98     LA        0.98     MC        1.01     
!   MK        1.00*    NL        0.99     NY        1.01     ON        1.01     
!   OV        0.99     PT        0.98     SC        1.02     WF        1.01     
!   WZ        1.01     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        0.98     GC        1.00     HN        1.00*    
!   KK        1.00*    KP        0.98     LA        0.98     MC        1.00*    
!   MK        1.00*    NL        1.00*    NY        1.00*    ON        1.00*    
!   OV        0.99     PT        0.99     SC        1.00*    WF        1.00*    
!   WZ        1.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.01     FD        1.00     GC        1.04     HN        1.00     
!   KK        1.02     KP        0.98     LA        0.98     MC        1.00*    
!   MK        1.02     NL        0.99     NY        1.02     ON        1.00*    
!   OV        0.99     PT        0.98     SC        1.02     WF        0.99     
!   WZ        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        0.99     GC        1.03     HN        1.01     
!   KK        1.00*    KP        0.98     LA        0.98     MC        1.01     
!   MK        1.00*    NL        0.99     NY        1.02     ON        0.99     
!   OV        0.99     PT        0.98     SC        1.02     WF        1.00     
!   WZ        1.00     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        0.98     GC        1.01     HN        1.00*    
!   KK        1.00*    KP        0.98     LA        0.98     MC        1.00*    
!   MK        1.00*    NL        1.00*    NY        1.00*    ON        1.00*    
!   OV        0.99     PT        0.99     SC        1.00*    WF        1.00*    
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00     FD        1.00     GC        1.03     HN        1.00     
!   KK        1.00     KP        0.98     LA        0.98     MC        0.99     
!   MK        1.02     NL        0.99     NY        1.02     ON        1.00     
!   OV        0.99     PT        0.98     SC        1.01     WF        0.99     
!   WZ        0.98     
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        1.00     GC        1.04     HN        1.01     
!   KK        1.00*    KP        0.98     LA        0.98     MC        1.00     
!   MK        1.00*    NL        1.00     NY        1.01     ON        1.02     
!   OV        0.99     PT        0.98     SC        1.01     WF        0.99     
!   WZ        1.00     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        0.99     GC        1.00     HN        1.00*    
!   KK        1.02     KP        0.98     LA        0.98     MC        1.00*    
!   MK        1.00*    NL        1.00*    NY        1.00*    ON        1.00*    
!   OV        0.99     PT        0.99     SC        1.00*    WF        1.00*    
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00     FD        1.00     GC        1.03     HN        1.00     
!   KK        1.00     KP        0.98     LA        0.98     MC        1.00     
!   MK        1.01     NL        1.00     NY        1.03     ON        0.98     
!   OV        0.99     PT        0.98     SC        1.02     WF        1.00     
!   WZ        0.98     
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        0.99     GC        1.03     HN        1.01     
!   KK        1.00*    KP        0.98     LA        0.98     MC        1.00     
!   MK        1.00*    NL        0.99     NY        1.01     ON        1.01     
!   OV        0.99     PT        0.98     SC        1.02     WF        1.03     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.98     FD        0.98     GC        1.01     HN        1.00*    
!   KK        1.02     KP        0.98     LA        0.99     MC        1.00*    
!   MK        1.00*    NL        1.00*    NY        1.00*    ON        1.00*    
!   OV        0.99     PT        0.98     SC        1.00*    WF        1.00*    
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00     FD        1.00     GC        1.03     HN        1.00     
!   KK        1.00     KP        0.98     LA        0.98     MC        1.00*    
!   MK        1.01     NL        1.00     NY        1.03     ON        1.00*    
!   OV        0.99     PT        0.98     SC        1.01     WF        1.00     
!   WZ        1.00*    
! 
! 
! Fit before self-cal, rms=0.082428Jy  sigma=0.001135
! Fit after  self-cal, rms=0.081677Jy  sigma=0.001091
dynam = dynam - 0.5
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=0.6951 mas, bmaj=1.701 mas, bpa=-9.75 degrees
! Estimated noise=631.168 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 (-1.6, 2.8).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00801657 Jy
! Component: 100  -  total flux cleaned = 0.0108912 Jy
! Total flux subtracted in 100 components = 0.0108912 Jy
! Clean residual min=-0.003192 max=0.007012 Jy/beam
! Clean residual mean=0.000353 rms=0.000964 Jy/beam
! Combined flux in latest and established models = 0.946008 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 17 model components to the UV plane model.
! The established model now contains 137 components and 0.946007 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.081124Jy  sigma=0.001075
! Fit after  self-cal, rms=0.080958Jy  sigma=0.001073
! Inverting map 
! Added new window around map position (-4.5, 5.8).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00603759 Jy
! Component: 100  -  total flux cleaned = 0.00828384 Jy
! Total flux subtracted in 100 components = 0.00828384 Jy
! Clean residual min=-0.002900 max=0.005309 Jy/beam
! Clean residual mean=0.000333 rms=0.000895 Jy/beam
! Combined flux in latest and established models = 0.954291 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 150 components and 0.954291 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.080469Jy  sigma=0.001066
! Fit after  self-cal, rms=0.080429Jy  sigma=0.001065
! 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)
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00151024 Jy
! Component: 100  -  total flux cleaned = 0.00214487 Jy
! Total flux subtracted in 100 components = 0.00214487 Jy
! Clean residual min=-0.002975 max=0.004968 Jy/beam
! Clean residual mean=0.000328 rms=0.000884 Jy/beam
! Combined flux in latest and established models = 0.956436 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 25 model components to the UV plane model.
! The established model now contains 159 components and 0.956436 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.080274Jy  sigma=0.001063
! Fit after  self-cal, rms=0.079299Jy  sigma=0.001055
! Inverting map and beam 
! Estimated beam: bmin=0.6949 mas, bmaj=1.7 mas, bpa=-9.738 degrees
! Estimated noise=631.365 mJy/beam.
! Added new window around map position (-3.3, 0.4).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00487039 Jy
! Component: 100  -  total flux cleaned = 0.00706871 Jy
! Total flux subtracted in 100 components = 0.00706871 Jy
! Clean residual min=-0.003064 max=0.004079 Jy/beam
! Clean residual mean=0.000242 rms=0.000805 Jy/beam
! Combined flux in latest and established models = 0.963505 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 20 model components to the UV plane model.
! The established model now contains 173 components and 0.963505 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.078996Jy  sigma=0.001049
! Fit after  self-cal, rms=0.078709Jy  sigma=0.001047
! Inverting map and beam 
! Estimated beam: bmin=0.695 mas, bmaj=1.7 mas, bpa=-9.747 degrees
! Estimated noise=631.952 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 = 0.00354738 Jy
! Component: 100  -  total flux cleaned = 0.00515946 Jy
! Total flux subtracted in 100 components = 0.00515946 Jy
! Clean residual min=-0.002996 max=0.003688 Jy/beam
! Clean residual mean=0.000218 rms=0.000774 Jy/beam
! Combined flux in latest and established models = 0.968664 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 25 model components to the UV plane model.
! The established model now contains 182 components and 0.968665 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.078540Jy  sigma=0.001044
! Fit after  self-cal, rms=0.078495Jy  sigma=0.001043
! Inverting map 
print "***********************************"
! *********************************** 
print "*** Finished Amplitude Self-Cal ***"
! *** Finished Amplitude Self-Cal *** 
print "***********************************"
! *********************************** 
save 1606+106_X
! Writing UV FITS file: 1606+106_X.uvf
! Writing 182 model components to file: 1606+106_X.mod
! wwins: Wrote 6 windows to 1606+106_X.win
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.695 x 1.7 at -9.747 degrees (North through East)
! Clean map  min=-0.0028671  max=0.69659 Jy/beam
! Writing clean map to FITS file: 1606+106_X.fits
! Writing difmap environment to: 1606+106_X.par
print "****************************"
! **************************** 
print "*** Now, make some plots ***"
! *** Now, make some plots *** 
print "****************************"
! **************************** 
![@gonzo_plot 1606+106_X]
device 1606+106_Xuv.ps/vps,1,2
! Attempting to open device: '1606+106_Xuv.ps/vps'
radplot
! Using default options string "m1"
uvplot
! Using default options string ""
device 1606+106_Xim.ps/vps
! Attempting to open device: '1606+106_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=0.695 mas, bmaj=1.7 mas, bpa=-9.747 degrees
! Estimated noise=631.952 mJy/beam.
mappl cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.695 x 1.7 at -9.747 degrees (North through East)
! Clean map  min=-0.0028671  max=0.69659 Jy/beam
![Exited script file: gonzo_plot]
![Exited script file: gonzo8-0.1]
quit
! Quitting program
! Log file 1606+106_X.log closed on Tue Mar 25 11:13:38 2008