! Started logfile: 1424-418_X.log on Mon Sep 17 22:33:13 2007
observe 1424-418_X.edt
! Reading UV FITS file: 1424-418_X.edt
! AN table 1: 7 integrations on 171 of 171 possible baselines.
! AN table 2: 5 integrations on 171 of 171 possible baselines.
! AN table 3: 13 integrations on 171 of 171 possible baselines.
! AN table 4: 22 integrations on 171 of 171 possible baselines.
! Apparent sampling: 0.0525072 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: 1424-418
! 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.
! 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 2132 lines of history.
! 
! Reading 1688 visibilities.
![@gonzo5-0.1 1424-418_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 = 5.0
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 105 telescope corrections were flagged in sub-array 1.
!  A total of 95 telescope corrections were flagged in sub-array 2.
!  A total of 247 telescope corrections were flagged in sub-array 3.
!  A total of 370 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 2.
!  A total of 108 telescope corrections were flagged in sub-array 1.
!  A total of 95 telescope corrections were flagged in sub-array 2.
!  A total of 247 telescope corrections were flagged in sub-array 3.
!  A total of 367 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 3.
!  A total of 110 telescope corrections were flagged in sub-array 1.
!  A total of 95 telescope corrections were flagged in sub-array 2.
!  A total of 247 telescope corrections were flagged in sub-array 3.
!  A total of 367 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 4.
!  A total of 108 telescope corrections were flagged in sub-array 1.
!  A total of 95 telescope corrections were flagged in sub-array 2.
!  A total of 247 telescope corrections were flagged in sub-array 3.
!  A total of 367 telescope corrections were flagged in sub-array 4.
! 
! Fit before self-cal, rms=1.308494Jy  sigma=0.017883
! Fit after  self-cal, rms=1.310488Jy  sigma=0.017984
! 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=0.7711 mas, bmaj=5.159 mas, bpa=-3.095 degrees
! Estimated noise=3521.96 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 = 1.7704 Jy
! Total flux subtracted in 50 components = 1.7704 Jy
! Clean residual min=-0.144546 max=0.493734 Jy/beam
! Clean residual mean=0.002590 rms=0.052029 Jy/beam
! Combined flux in latest and established models = 1.7704 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 1.7704 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.548362Jy  sigma=0.007557
! Fit after  self-cal, rms=0.548362Jy  sigma=0.007557
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.386063 Jy
! Total flux subtracted in 50 components = 0.386063 Jy
! Clean residual min=-0.039241 max=0.107666 Jy/beam
! Clean residual mean=0.001227 rms=0.014886 Jy/beam
! Combined flux in latest and established models = 2.15646 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 2.15646 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.192979Jy  sigma=0.002648
! Fit after  self-cal, rms=0.192979Jy  sigma=0.002648
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0989803 Jy
! Total flux subtracted in 50 components = 0.0989803 Jy
! Clean residual min=-0.023062 max=0.043917 Jy/beam
! Clean residual mean=0.000877 rms=0.008801 Jy/beam
! Combined flux in latest and established models = 2.25544 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 17 components and 2.25544 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.129963Jy  sigma=0.001746
! Fit after  self-cal, rms=0.129523Jy  sigma=0.001739
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0507206 Jy
! Total flux subtracted in 50 components = 0.0507206 Jy
! Clean residual min=-0.017164 max=0.031350 Jy/beam
! Clean residual mean=0.000702 rms=0.006444 Jy/beam
! Combined flux in latest and established models = 2.30616 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 35 model components to the UV plane model.
! The established model now contains 45 components and 2.30616 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.105344Jy  sigma=0.001384
! Fit after  self-cal, rms=0.105012Jy  sigma=0.001379
! 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=1.034 mas, bmaj=6.28 mas, bpa=-2.781 degrees
! Estimated noise=2286.32 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 = 0.0461089 Jy
! Component: 100  -  total flux cleaned = 0.070348 Jy
! Total flux subtracted in 100 components = 0.070348 Jy
! Clean residual min=-0.015121 max=0.021988 Jy/beam
! Clean residual mean=0.001167 rms=0.005933 Jy/beam
! Combined flux in latest and established models = 2.37651 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 65 model components to the UV plane model.
! The established model now contains 102 components and 2.37651 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.086166Jy  sigma=0.001094
! Fit after  self-cal, rms=0.086003Jy  sigma=0.001091
! 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        1.00*    GG        1.00*    
!   HN        1.00*    KP        1.00     LA        1.00     MA        1.00*    
!   MK        1.00*    NL        1.04     NY        1.00*    ON        1.00*    
!   OV        1.00*    PT        0.99     SC        0.99     TC        1.00*    
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HN        0.00*    KP        0.00*    LA        0.00*    MA        0.00*    
!   MK        0.00*    NL        0.00*    NY        0.00*    ON        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TC        0.00*    
!   TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HN        0.00*    KP        0.00*    LA        0.00*    MA        0.00*    
!   MK        0.00*    NL        0.00*    NY        0.00*    ON        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TC        0.00*    
!   TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        1.00     GC        1.00*    GG        1.00*    
!   HN        1.00*    KP        0.99     LA        0.99     MA        1.00*    
!   MK        1.01     NL        1.00*    NY        1.00*    ON        1.00*    
!   OV        1.01     PT        0.99     SC        1.00*    TC        1.00*    
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00     GC        1.00*    GG        1.00*    
!   HN        1.00*    KP        1.01     LA        0.99     MA        1.00*    
!   MK        1.00*    NL        1.04     NY        1.00*    ON        1.00*    
!   OV        1.00*    PT        0.99     SC        0.99     TC        1.00*    
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HN        0.00*    KP        0.00*    LA        0.00*    MA        0.00*    
!   MK        0.00*    NL        0.00*    NY        0.00*    ON        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TC        0.00*    
!   TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HN        0.00*    KP        0.00*    LA        0.00*    MA        0.00*    
!   MK        0.00*    NL        0.00*    NY        0.00*    ON        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TC        0.00*    
!   TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        1.00     GC        1.00*    GG        1.00*    
!   HN        1.00*    KP        1.00     LA        0.99     MA        1.00*    
!   MK        1.00     NL        1.00*    NY        1.00*    ON        1.00*    
!   OV        1.00     PT        1.00     SC        1.00*    TC        1.00*    
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 3.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.99     GC        1.00*    GG        1.00*    
!   HN        1.00*    KP        1.00     LA        1.00     MA        1.00*    
!   MK        1.00*    NL        1.00     NY        1.00*    ON        1.00*    
!   OV        1.00*    PT        0.99     SC        1.00     TC        1.00*    
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HN        0.00*    KP        0.00*    LA        0.00*    MA        0.00*    
!   MK        0.00*    NL        0.00*    NY        0.00*    ON        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TC        0.00*    
!   TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HN        0.00*    KP        0.00*    LA        0.00*    MA        0.00*    
!   MK        0.00*    NL        0.00*    NY        0.00*    ON        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TC        0.00*    
!   TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        1.00     GC        1.00*    GG        1.00*    
!   HN        1.00*    KP        0.99     LA        0.99     MA        1.00*    
!   MK        1.01     NL        1.00*    NY        1.00*    ON        1.00*    
!   OV        1.00     PT        0.99     SC        1.00*    TC        1.00*    
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 4.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.99     GC        1.00*    GG        1.00*    
!   HN        1.00*    KP        1.00     LA        0.99     MA        1.00*    
!   MK        1.00*    NL        1.02     NY        1.00*    ON        1.00*    
!   OV        1.00*    PT        0.99     SC        1.00     TC        1.00*    
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HN        0.00*    KP        0.00*    LA        0.00*    MA        0.00*    
!   MK        0.00*    NL        0.00*    NY        0.00*    ON        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TC        0.00*    
!   TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.00*    FD        0.00*    GC        0.00*    GG        0.00*    
!   HN        0.00*    KP        0.00*    LA        0.00*    MA        0.00*    
!   MK        0.00*    NL        0.00*    NY        0.00*    ON        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TC        0.00*    
!   TS        0.00*    WF        0.00*    WZ        0.00*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        1.01     GC        1.00*    GG        1.00*    
!   HN        1.00*    KP        1.00     LA        0.99     MA        1.00*    
!   MK        1.00     NL        1.00*    NY        1.00*    ON        1.00*    
!   OV        1.00     PT        0.99     SC        1.00*    TC        1.00*    
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
! 
! Fit before self-cal, rms=0.086003Jy  sigma=0.001091
! Fit after  self-cal, rms=0.081222Jy  sigma=0.001051
dynam = dynam - 0.5
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=1.034 mas, bmaj=6.301 mas, bpa=-2.631 degrees
! Estimated noise=2294.68 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 = 0.004335 Jy
! Component: 100  -  total flux cleaned = 0.00451176 Jy
! Total flux subtracted in 100 components = 0.00451176 Jy
! Clean residual min=-0.012232 max=0.016929 Jy/beam
! Clean residual mean=0.000811 rms=0.004865 Jy/beam
! Combined flux in latest and established models = 2.38102 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 116 components and 2.38102 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.080680Jy  sigma=0.001044
! Fit after  self-cal, rms=0.080573Jy  sigma=0.001043
! 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 (4, -0.2).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0143781 Jy
! Component: 100  -  total flux cleaned = 0.0198719 Jy
! Total flux subtracted in 100 components = 0.0198719 Jy
! Clean residual min=-0.009214 max=0.015688 Jy/beam
! Clean residual mean=0.000626 rms=0.004305 Jy/beam
! Combined flux in latest and established models = 2.40089 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 17 model components to the UV plane model.
! The established model now contains 133 components and 2.40089 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.078276Jy  sigma=0.001012
! Fit after  self-cal, rms=0.076988Jy  sigma=0.000989
! Inverting map and beam 
! Estimated beam: bmin=1.034 mas, bmaj=6.297 mas, bpa=-2.627 degrees
! Estimated noise=2295.11 mJy/beam.
! Added new window around map position (12.8, -16).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0132349 Jy
! Component: 100  -  total flux cleaned = 0.020949 Jy
! Total flux subtracted in 100 components = 0.020949 Jy
! Clean residual min=-0.009940 max=0.008843 Jy/beam
! Clean residual mean=0.000431 rms=0.003174 Jy/beam
! Combined flux in latest and established models = 2.42184 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 43 model components to the UV plane model.
! The established model now contains 176 components and 2.42184 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.074641Jy  sigma=0.000960
! Fit after  self-cal, rms=0.073955Jy  sigma=0.000953
! Inverting map and beam 
! Estimated beam: bmin=1.034 mas, bmaj=6.299 mas, bpa=-2.624 degrees
! Estimated noise=2293.62 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 = 0.00725343 Jy
! Component: 100  -  total flux cleaned = 0.0123368 Jy
! Total flux subtracted in 100 components = 0.0123368 Jy
! Clean residual min=-0.009185 max=0.007836 Jy/beam
! Clean residual mean=0.000215 rms=0.002757 Jy/beam
! Combined flux in latest and established models = 2.43418 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 39 model components to the UV plane model.
! The established model now contains 206 components and 2.43418 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.073138Jy  sigma=0.000944
! Fit after  self-cal, rms=0.073060Jy  sigma=0.000943
! Inverting map 
print "***********************************"
! *********************************** 
print "*** Finished Amplitude Self-Cal ***"
! *** Finished Amplitude Self-Cal *** 
print "***********************************"
! *********************************** 
save 1424-418_X
! Writing UV FITS file: 1424-418_X.uvf
! Writing 206 model components to file: 1424-418_X.mod
! wwins: Wrote 3 windows to 1424-418_X.win
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 1.034 x 6.299 at -2.624 degrees (North through East)
! Clean map  min=-0.0093272  max=2.2597 Jy/beam
! Writing clean map to FITS file: 1424-418_X.fits
! Writing difmap environment to: 1424-418_X.par
print "****************************"
! **************************** 
print "*** Now, make some plots ***"
! *** Now, make some plots *** 
print "****************************"
! **************************** 
![@gonzo_plot 1424-418_X]
device 1424-418_Xuv.ps/vps,1,2
! Attempting to open device: '1424-418_Xuv.ps/vps'
radplot
! Using default options string "m1"
uvplot
! Using default options string ""
device 1424-418_Xim.ps/vps
! Attempting to open device: '1424-418_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=1.034 mas, bmaj=6.299 mas, bpa=-2.624 degrees
! Estimated noise=2293.62 mJy/beam.
mappl cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 1.034 x 6.299 at -2.624 degrees (North through East)
! Clean map  min=-0.0093272  max=2.2597 Jy/beam
![Exited script file: gonzo_plot]
![Exited script file: gonzo5-0.1]
quit
! Quitting program
! Log file 1424-418_X.log closed on Mon Sep 17 22:33:20 2007