! Started logfile: 0104-408_X.log on Thu Feb 14 22:48:28 2008
observe 0104-408_X.edt
! Reading UV FITS file: 0104-408_X.edt
! AN table 1: 21 integrations on 136 of 136 possible baselines.
! AN table 2: 5 integrations on 136 of 136 possible baselines.
! AN table 3: 39 integrations on 136 of 136 possible baselines.
! Apparent sampling: 0.103281 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: 0104-408
! 
! 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 3652 visibilities.
![@gonzo6-0.1 0104-408_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 = 6.0
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 276 telescope corrections were flagged in sub-array 1.
!  A total of 85 telescope corrections were flagged in sub-array 2.
!  A total of 433 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 276 telescope corrections were flagged in sub-array 1.
!  A total of 85 telescope corrections were flagged in sub-array 2.
!  A total of 430 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 276 telescope corrections were flagged in sub-array 1.
!  A total of 85 telescope corrections were flagged in sub-array 2.
!  A total of 426 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 276 telescope corrections were flagged in sub-array 1.
!  A total of 85 telescope corrections were flagged in sub-array 2.
!  A total of 429 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=2.878060Jy  sigma=0.042295
! Fit after  self-cal, rms=2.878126Jy  sigma=0.042300
! 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=0.5916 mas, bmaj=2.178 mas, bpa=-5.29 degrees
! Estimated noise=1468.36 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 = 3.00795 Jy
! Total flux subtracted in 50 components = 3.00795 Jy
! Clean residual min=-0.247766 max=0.838915 Jy/beam
! Clean residual mean=-0.001619 rms=0.074051 Jy/beam
! Combined flux in latest and established models = 3.00795 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 3.00795 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.902482Jy  sigma=0.013597
! Fit after  self-cal, rms=0.902482Jy  sigma=0.013597
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.657709 Jy
! Total flux subtracted in 50 components = 0.657709 Jy
! Clean residual min=-0.077267 max=0.197893 Jy/beam
! Clean residual mean=-0.000690 rms=0.024640 Jy/beam
! Combined flux in latest and established models = 3.66566 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 5 model components to the UV plane model.
! The established model now contains 5 components and 3.66566 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.346201Jy  sigma=0.005012
! Fit after  self-cal, rms=0.346295Jy  sigma=0.005012
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.216641 Jy
! Total flux subtracted in 50 components = 0.216641 Jy
! Clean residual min=-0.045115 max=0.103130 Jy/beam
! Clean residual mean=-0.000399 rms=0.013664 Jy/beam
! Combined flux in latest and established models = 3.8823 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 6 model components to the UV plane model.
! The established model now contains 10 components and 3.8823 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.214915Jy  sigma=0.002894
! Fit after  self-cal, rms=0.215025Jy  sigma=0.002894
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.118673 Jy
! Total flux subtracted in 50 components = 0.118673 Jy
! Clean residual min=-0.029994 max=0.058603 Jy/beam
! Clean residual mean=-0.000243 rms=0.008170 Jy/beam
! Combined flux in latest and established models = 4.00097 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 5 model components to the UV plane model.
! The established model now contains 13 components and 4.00097 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.154213Jy  sigma=0.001885
! Fit after  self-cal, rms=0.154196Jy  sigma=0.001885
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0676204 Jy
! Total flux subtracted in 50 components = 0.0676204 Jy
! Clean residual min=-0.022978 max=0.033619 Jy/beam
! Clean residual mean=-0.000155 rms=0.005361 Jy/beam
! Combined flux in latest and established models = 4.06859 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 5 model components to the UV plane model.
! The established model now contains 15 components and 4.06859 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.128262Jy  sigma=0.001436
! Fit after  self-cal, rms=0.128242Jy  sigma=0.001436
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0393516 Jy
! Total flux subtracted in 50 components = 0.0393516 Jy
! Clean residual min=-0.021210 max=0.020114 Jy/beam
! Clean residual mean=-0.000105 rms=0.004076 Jy/beam
! Combined flux in latest and established models = 4.10795 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 20 components and 4.10795 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.118394Jy  sigma=0.001272
! Fit after  self-cal, rms=0.118386Jy  sigma=0.001271
! 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=0.6432 mas, bmaj=2.323 mas, bpa=-7.219 degrees
! Estimated noise=900.279 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 = 0.0197135 Jy
! Component: 100  -  total flux cleaned = 0.0236468 Jy
! Total flux subtracted in 100 components = 0.0236468 Jy
! Clean residual min=-0.011570 max=0.012272 Jy/beam
! Clean residual mean=-0.000180 rms=0.002585 Jy/beam
! Combined flux in latest and established models = 4.13159 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 30 components and 4.13159 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.112479Jy  sigma=0.001196
! Fit after  self-cal, rms=0.112435Jy  sigma=0.001195
! 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        1.00     GC        1.00*    HN        1.00*    
!   KK        1.00     KP        1.00     LA        1.00     MC        1.00*    
!   MK        1.00     NL        1.00*    NY        1.00*    ON        1.00*    
!   OV        1.00     PT        1.00     SC        1.00*    WF        1.00*    
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   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 3:
!   BR        1.00*    FD        1.00     GC        1.00*    HN        1.00*    
!   KK        1.00     KP        1.00     LA        1.00     MC        1.00*    
!   MK        1.00     NL        1.00     NY        1.00*    ON        1.00*    
!   OV        1.00     PT        1.00     SC        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*    HN        1.00*    
!   KK        1.00     KP        1.00     LA        1.00     MC        1.00*    
!   MK        1.00     NL        1.00*    NY        1.00*    ON        1.00*    
!   OV        1.00     PT        1.00     SC        1.00*    WF        1.00*    
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   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 3:
!   BR        1.00*    FD        1.00     GC        1.00*    HN        1.00*    
!   KK        1.00     KP        1.00     LA        1.00     MC        1.00*    
!   MK        1.00     NL        1.00     NY        1.00*    ON        1.00*    
!   OV        1.00     PT        1.00     SC        1.00     WF        1.00*    
!   WZ        1.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00     GC        1.00*    HN        1.00*    
!   KK        1.00     KP        1.00     LA        1.00     MC        1.00*    
!   MK        1.00     NL        1.00*    NY        1.00*    ON        1.00*    
!   OV        1.00     PT        1.00     SC        1.00*    WF        1.00*    
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   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*    
! 
!  A total of 3 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        1.00     GC        1.00*    HN        1.00*    
!   KK        1.00     KP        1.00     LA        1.00     MC        1.00*    
!   MK        1.00     NL        1.00     NY        1.00*    ON        1.00*    
!   OV        1.00     PT        1.00     SC        1.00     WF        1.00*    
!   WZ        1.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00     GC        1.00*    HN        1.00*    
!   KK        1.00     KP        1.00     LA        1.00     MC        1.00*    
!   MK        1.00     NL        1.00*    NY        1.00*    ON        1.00*    
!   OV        1.00     PT        1.00     SC        1.00*    WF        1.00*    
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   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 3:
!   BR        1.00*    FD        1.00     GC        1.00*    HN        1.00*    
!   KK        1.00     KP        1.00     LA        1.00     MC        1.00*    
!   MK        1.00     NL        1.00     NY        1.00*    ON        1.00*    
!   OV        1.00     PT        1.00     SC        1.00     WF        1.00*    
!   WZ        1.00*    
! 
! 
! Fit before self-cal, rms=0.112435Jy  sigma=0.001195
! Fit after  self-cal, rms=0.112323Jy  sigma=0.001192
dynam = dynam - 0.5
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=0.6432 mas, bmaj=2.325 mas, bpa=-7.237 degrees
! Estimated noise=900.071 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 (2.1, 4.1).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00438388 Jy
! Component: 100  -  total flux cleaned = 0.00654276 Jy
! Total flux subtracted in 100 components = 0.00654276 Jy
! Clean residual min=-0.007684 max=0.007576 Jy/beam
! Clean residual mean=-0.000163 rms=0.001983 Jy/beam
! Combined flux in latest and established models = 4.13814 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 48 components and 4.13814 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.109464Jy  sigma=0.001168
! Fit after  self-cal, rms=0.109419Jy  sigma=0.001168
! 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 = 0.002211 Jy
! Component: 100  -  total flux cleaned = 0.00338668 Jy
! Total flux subtracted in 100 components = 0.00338668 Jy
! Clean residual min=-0.006441 max=0.006835 Jy/beam
! Clean residual mean=-0.000169 rms=0.001816 Jy/beam
! Combined flux in latest and established models = 4.14152 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 18 model components to the UV plane model.
! The established model now contains 60 components and 4.14152 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.108085Jy  sigma=0.001159
! Fit after  self-cal, rms=0.107386Jy  sigma=0.001146
! Inverting map and beam 
! Estimated beam: bmin=0.643 mas, bmaj=2.326 mas, bpa=-7.259 degrees
! Estimated noise=900.511 mJy/beam.
! Added new window around map position (0.4, -3).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00359513 Jy
! Component: 100  -  total flux cleaned = 0.00520615 Jy
! Total flux subtracted in 100 components = 0.00520615 Jy
! Clean residual min=-0.005381 max=0.006154 Jy/beam
! Clean residual mean=-0.000146 rms=0.001593 Jy/beam
! Combined flux in latest and established models = 4.14673 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 71 components and 4.14673 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.106171Jy  sigma=0.001137
! Fit after  self-cal, rms=0.106032Jy  sigma=0.001133
! Inverting map and beam 
! Estimated beam: bmin=0.6429 mas, bmaj=2.327 mas, bpa=-7.271 degrees
! Estimated noise=900.778 mJy/beam.
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.003162 Jy
! Component: 100  -  total flux cleaned = 0.00444865 Jy
! Total flux subtracted in 100 components = 0.00444865 Jy
! Clean residual min=-0.004960 max=0.005476 Jy/beam
! Clean residual mean=-0.000131 rms=0.001464 Jy/beam
! Combined flux in latest and established models = 4.15118 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 75 components and 4.15118 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.105236Jy  sigma=0.001128
! Fit after  self-cal, rms=0.105201Jy  sigma=0.001126
! Inverting map and beam 
! Estimated beam: bmin=0.6428 mas, bmaj=2.327 mas, bpa=-7.281 degrees
! Estimated noise=900.99 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 = 0.00298895 Jy
! Component: 100  -  total flux cleaned = 0.00400401 Jy
! Total flux subtracted in 100 components = 0.00400401 Jy
! Clean residual min=-0.004631 max=0.005175 Jy/beam
! Clean residual mean=-0.000120 rms=0.001380 Jy/beam
! Combined flux in latest and established models = 4.15518 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 82 components and 4.15518 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.104661Jy  sigma=0.001122
! Fit after  self-cal, rms=0.104662Jy  sigma=0.001122
! Inverting map 
print "***********************************"
! *********************************** 
print "*** Finished Amplitude Self-Cal ***"
! *** Finished Amplitude Self-Cal *** 
print "***********************************"
! *********************************** 
save 0104-408_X
! Writing UV FITS file: 0104-408_X.uvf
! Writing 82 model components to file: 0104-408_X.mod
! wwins: Wrote 3 windows to 0104-408_X.win
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6428 x 2.327 at -7.281 degrees (North through East)
! Clean map  min=-0.0045484  max=3.8812 Jy/beam
! Writing clean map to FITS file: 0104-408_X.fits
! Writing difmap environment to: 0104-408_X.par
print "****************************"
! **************************** 
print "*** Now, make some plots ***"
! *** Now, make some plots *** 
print "****************************"
! **************************** 
![@gonzo_plot 0104-408_X]
device 0104-408_Xuv.ps/vps,1,2
! Attempting to open device: '0104-408_Xuv.ps/vps'
radplot
! Using default options string "m1"
uvplot
! Using default options string ""
device 0104-408_Xim.ps/vps
! Attempting to open device: '0104-408_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=0.6428 mas, bmaj=2.327 mas, bpa=-7.281 degrees
! Estimated noise=900.99 mJy/beam.
mappl cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6428 x 2.327 at -7.281 degrees (North through East)
! Clean map  min=-0.0045484  max=3.8812 Jy/beam
![Exited script file: gonzo_plot]
![Exited script file: gonzo6-0.1]
quit
! Quitting program
! Log file 0104-408_X.log closed on Thu Feb 14 22:48:35 2008