! Started logfile: 0552+398_S.log on Mon Jul 10 16:37:56 2006
observe 0552+398_S.edt
! Reading UV FITS file: 0552+398_S.edt
! AN table 1: 35 integrations on 190 of 190 possible baselines.
! AN table 2: 21 integrations on 190 of 190 possible baselines.
! AN table 3: 10 integrations on 190 of 190 possible baselines.
! AN table 4: 81 integrations on 190 of 190 possible baselines.
! Apparent sampling: 0.204117 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: 0552+398
! 
! 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  2.22497e+09        8e+06          1        8e+06
!  02        2  2.24497e+09        8e+06          1        8e+06
!  03        3  2.33497e+09        8e+06          1        8e+06
!  04        4  2.36497e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 1588 lines of history.
! 
! Reading 22804 visibilities.
![@gonzo7-0.4 0552+398_S]
print "***********************************"
! *********************************** 
print "*** Using gonzo instruction set ***"
! *** Using gonzo instruction set *** 
print "***********************************"
! *********************************** 
float field_size
field_size = 1024
float field_cell
field_cell = 0.4
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 0.400x0.400 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 450 telescope corrections were flagged in sub-array 1.
!  A total of 384 telescope corrections were flagged in sub-array 2.
!  A total of 133 telescope corrections were flagged in sub-array 3.
!  A total of 1099 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 2.
!  A total of 450 telescope corrections were flagged in sub-array 1.
!  A total of 383 telescope corrections were flagged in sub-array 2.
!  A total of 134 telescope corrections were flagged in sub-array 3.
!  A total of 1099 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 3.
!  A total of 450 telescope corrections were flagged in sub-array 1.
!  A total of 375 telescope corrections were flagged in sub-array 2.
!  A total of 134 telescope corrections were flagged in sub-array 3.
!  A total of 1106 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 4.
!  A total of 450 telescope corrections were flagged in sub-array 1.
!  A total of 384 telescope corrections were flagged in sub-array 2.
!  A total of 133 telescope corrections were flagged in sub-array 3.
!  A total of 1113 telescope corrections were flagged in sub-array 4.
! 
! Fit before self-cal, rms=2.098062Jy  sigma=0.030202
! Fit after  self-cal, rms=2.099211Jy  sigma=0.030233
! 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=2.635 mas, bmaj=3.734 mas, bpa=-19.45 degrees
! Estimated noise=875.989 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 = 2.29048 Jy
! Total flux subtracted in 50 components = 2.29048 Jy
! Clean residual min=-0.086583 max=0.639075 Jy/beam
! Clean residual mean=-0.000161 rms=0.026619 Jy/beam
! Combined flux in latest and established models = 2.29048 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 2.29048 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.842058Jy  sigma=0.012002
! Fit after  self-cal, rms=0.842058Jy  sigma=0.012002
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.51528 Jy
! Total flux subtracted in 50 components = 0.51528 Jy
! Clean residual min=-0.040118 max=0.180183 Jy/beam
! Clean residual mean=-0.000128 rms=0.011383 Jy/beam
! Combined flux in latest and established models = 2.80576 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 2.80576 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.408333Jy  sigma=0.005583
! Fit after  self-cal, rms=0.408278Jy  sigma=0.005582
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.183417 Jy
! Total flux subtracted in 50 components = 0.183417 Jy
! Clean residual min=-0.034935 max=0.080032 Jy/beam
! Clean residual mean=-0.000118 rms=0.007671 Jy/beam
! Combined flux in latest and established models = 2.98918 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 9 model components to the UV plane model.
! The established model now contains 12 components and 2.98918 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.305267Jy  sigma=0.003937
! Fit after  self-cal, rms=0.305251Jy  sigma=0.003937
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0907127 Jy
! Total flux subtracted in 50 components = 0.0907127 Jy
! Clean residual min=-0.033106 max=0.044526 Jy/beam
! Clean residual mean=-0.000112 rms=0.006452 Jy/beam
! Combined flux in latest and established models = 3.07989 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 3.07989 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.273003Jy  sigma=0.003406
! Fit after  self-cal, rms=0.272980Jy  sigma=0.003406
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0514638 Jy
! Total flux subtracted in 50 components = 0.0514638 Jy
! Clean residual min=-0.034378 max=0.025555 Jy/beam
! Clean residual mean=-0.000108 rms=0.005998 Jy/beam
! Combined flux in latest and established models = 3.13136 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 18 components and 3.13136 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.260500Jy  sigma=0.003208
! Fit after  self-cal, rms=0.260493Jy  sigma=0.003208
! 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=3.584 mas, bmaj=5.064 mas, bpa=-13.7 degrees
! Estimated noise=417.849 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 = 0.0546971 Jy
! Component: 100  -  total flux cleaned = 0.0680345 Jy
! Total flux subtracted in 100 components = 0.0680345 Jy
! Clean residual min=-0.024670 max=0.025792 Jy/beam
! Clean residual mean=0.000356 rms=0.004868 Jy/beam
! Combined flux in latest and established models = 3.19939 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 13 model components to the UV plane model.
! The established model now contains 25 components and 3.19939 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.248470Jy  sigma=0.003071
! Fit after  self-cal, rms=0.248469Jy  sigma=0.003071
! 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        0.95     FD        0.99     GC        0.95     HN        1.02     
!   LA        0.98     NL        1.01     OV        0.97     SC        0.90     
!   WF        0.98     GG        1.00*    HH        1.00*    KK        1.00*    
!   KP        1.00*    MA        1.00*    MC        1.00*    MK        1.00*    
!   NY        1.00*    TS        1.00*    WZ        1.00*    PT        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.05     FD        1.05     GC        1.00*    HN        1.00*    
!   LA        1.09     NL        1.04     OV        1.03     SC        1.07     
!   WF        1.00*    GG        1.00*    HH        1.00*    KK        1.00*    
!   KP        1.05     MA        1.00*    MC        1.00*    MK        1.00*    
!   NY        1.00*    TS        1.00*    WZ        1.00*    PT        1.03     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.03     FD        1.03     GC        1.03     HN        1.09     
!   LA        1.04     NL        1.06     OV        1.03     SC        1.00*    
!   WF        1.04     GG        1.00*    HH        1.00*    KK        1.09     
!   KP        0.96     MA        1.00*    MC        1.00*    MK        1.07     
!   NY        0.85     TS        0.98     WZ        1.00*    PT        1.00*    
! 
!  A total of 18 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.02     FD        1.01     GC        0.94     HN        1.01     
!   LA        1.00     NL        1.00     OV        1.01     SC        1.02     
!   WF        1.00     GG        1.00*    HH        1.00*    KK        0.99     
!   KP        1.01     MA        1.00*    MC        1.00*    MK        0.99     
!   NY        0.96     TS        1.00*    WZ        1.00*    PT        1.01     
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.93     FD        0.97     GC        0.90     HN        1.00     
!   LA        0.99     NL        1.02     OV        0.97     SC        1.04     
!   WF        0.96     GG        1.00*    HH        1.00*    KK        1.00*    
!   KP        1.00*    MA        1.00*    MC        1.00*    MK        1.00*    
!   NY        1.00*    TS        1.00*    WZ        1.00*    PT        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.02     FD        1.07     GC        1.00*    HN        1.00*    
!   LA        1.12     NL        1.04     OV        1.02     SC        1.07     
!   WF        1.00*    GG        1.00*    HH        1.00*    KK        1.00*    
!   KP        1.06     MA        1.00*    MC        1.00*    MK        1.00*    
!   NY        1.00*    TS        1.00*    WZ        1.00*    PT        0.99     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.04     FD        1.05     GC        1.03     HN        1.07     
!   LA        1.07     NL        1.06     OV        1.06     SC        1.00*    
!   WF        0.88     GG        1.00*    HH        1.00*    KK        1.08     
!   KP        1.04     MA        1.00*    MC        1.00*    MK        1.08     
!   NY        1.01     TS        1.08     WZ        1.00*    PT        1.00*    
! 
!  A total of 18 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.02     FD        1.01     GC        0.97     HN        1.01     
!   LA        1.00     NL        1.01     OV        1.01     SC        1.01     
!   WF        0.99     GG        1.00*    HH        1.00*    KK        1.00     
!   KP        1.00     MA        1.00*    MC        1.00*    MK        0.99     
!   NY        0.97     TS        1.00*    WZ        1.00*    PT        1.01     
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.96     FD        0.98     GC        1.00     HN        1.00     
!   LA        0.98     NL        1.02     OV        0.99     SC        0.94     
!   WF        0.85     GG        1.00*    HH        1.00*    KK        1.00*    
!   KP        1.00*    MA        1.00*    MC        1.00*    MK        1.00*    
!   NY        1.00*    TS        1.00*    WZ        1.00*    PT        1.00*    
! 
!  A total of 18 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.95     FD        0.97     GC        1.00*    HN        1.00*    
!   LA        1.27     NL        0.93     OV        0.99     SC        1.01     
!   WF        1.00*    GG        1.00*    HH        1.00*    KK        1.00*    
!   KP        1.05     MA        1.00*    MC        1.00*    MK        1.00*    
!   NY        1.00*    TS        1.00*    WZ        1.00*    PT        1.00     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.03     FD        1.03     GC        1.02     HN        1.09     
!   LA        0.99     NL        1.08     OV        1.01     SC        1.00*    
!   WF        0.99     GG        1.00*    HH        1.00*    KK        1.06     
!   KP        1.02     MA        1.00*    MC        1.00*    MK        1.04     
!   NY        1.09     TS        1.08     WZ        1.00*    PT        1.00*    
! 
!  A total of 15 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.01     FD        1.00     GC        0.97     HN        1.00     
!   LA        1.02     NL        1.02     OV        1.01     SC        1.01     
!   WF        1.00     GG        1.00*    HH        1.00*    KK        0.99     
!   KP        1.01     MA        1.00*    MC        1.00*    MK        0.99     
!   NY        0.95     TS        1.00*    WZ        1.00*    PT        1.00     
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.98     FD        1.00     GC        1.01     HN        0.99     
!   LA        0.98     NL        1.00     OV        0.95     SC        1.03     
!   WF        0.93     GG        1.00*    HH        1.00*    KK        1.00*    
!   KP        1.00*    MA        1.00*    MC        1.00*    MK        1.00*    
!   NY        1.00*    TS        1.00*    WZ        1.00*    PT        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        1.05     GC        1.00*    HN        1.00*    
!   LA        1.13     NL        1.05     OV        0.99     SC        1.03     
!   WF        1.00*    GG        1.00*    HH        1.00*    KK        1.00*    
!   KP        1.02     MA        1.00*    MC        1.00*    MK        1.00*    
!   NY        1.00*    TS        1.00*    WZ        1.00*    PT        0.99     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.02     FD        0.98     GC        1.03     HN        1.07     
!   LA        0.89     NL        1.05     OV        0.84     SC        1.00*    
!   WF        0.81     GG        1.00*    HH        1.00*    KK        1.04     
!   KP        1.02     MA        1.00*    MC        1.00*    MK        1.05     
!   NY        1.10     TS        1.05     WZ        1.00*    PT        1.00*    
! 
!  A total of 21 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.02     FD        1.01     GC        0.97     HN        1.00     
!   LA        1.00     NL        1.01     OV        1.01     SC        1.01     
!   WF        1.00     GG        1.00*    HH        1.00*    KK        1.01     
!   KP        1.01     MA        1.00*    MC        1.00*    MK        1.01     
!   NY        0.98     TS        1.00*    WZ        1.00*    PT        1.02     
! 
! 
! Fit before self-cal, rms=0.248469Jy  sigma=0.003071
! Fit after  self-cal, rms=0.180781Jy  sigma=0.002373
dynam = dynam - 0.5
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=3.586 mas, bmaj=5.067 mas, bpa=-13.05 degrees
! Estimated noise=417.607 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 (11.6, 0.8).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00884122 Jy
! Component: 100  -  total flux cleaned = 0.0101809 Jy
! Total flux subtracted in 100 components = 0.0101809 Jy
! Clean residual min=-0.007718 max=0.011763 Jy/beam
! Clean residual mean=-0.000554 rms=0.001802 Jy/beam
! Combined flux in latest and established models = 3.20957 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 32 components and 3.20957 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.179164Jy  sigma=0.002355
! Fit after  self-cal, rms=0.179143Jy  sigma=0.002355
! Inverting map 
! Added new window around map position (-11.6, -0.8).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00587688 Jy
! Component: 100  -  total flux cleaned = 0.00490643 Jy
! Total flux subtracted in 100 components = 0.00490643 Jy
! Clean residual min=-0.007231 max=0.008544 Jy/beam
! Clean residual mean=-0.000597 rms=0.001711 Jy/beam
! Combined flux in latest and established models = 3.21448 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 45 components and 3.21448 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.178290Jy  sigma=0.002347
! Fit after  self-cal, rms=0.178276Jy  sigma=0.002347
! 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 (-13.2, -24.8).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00204742 Jy
! Component: 100  -  total flux cleaned = 0.000914827 Jy
! Total flux subtracted in 100 components = 0.000914827 Jy
! Clean residual min=-0.007263 max=0.006808 Jy/beam
! Clean residual mean=-0.000608 rms=0.001663 Jy/beam
! Combined flux in latest and established models = 3.21539 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 28 model components to the UV plane model.
! The established model now contains 59 components and 3.21539 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.177699Jy  sigma=0.002341
! Fit after  self-cal, rms=0.163645Jy  sigma=0.002111
! Inverting map and beam 
! Estimated beam: bmin=3.584 mas, bmaj=5.064 mas, bpa=-12.92 degrees
! Estimated noise=418.06 mJy/beam.
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00772029 Jy
! Component: 100  -  total flux cleaned = 0.00799678 Jy
! Total flux subtracted in 100 components = 0.00799678 Jy
! Clean residual min=-0.006477 max=0.006544 Jy/beam
! Clean residual mean=-0.000342 rms=0.001313 Jy/beam
! Combined flux in latest and established models = 3.22339 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 14 model components to the UV plane model.
! The established model now contains 66 components and 3.22339 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.162876Jy  sigma=0.002104
! Fit after  self-cal, rms=0.161351Jy  sigma=0.002074
! Inverting map and beam 
! Estimated beam: bmin=3.581 mas, bmaj=5.062 mas, bpa=-12.86 degrees
! Estimated noise=418.456 mJy/beam.
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00639951 Jy
! Component: 100  -  total flux cleaned = 0.00565854 Jy
! Total flux subtracted in 100 components = 0.00565854 Jy
! Clean residual min=-0.006295 max=0.006235 Jy/beam
! Clean residual mean=-0.000292 rms=0.001242 Jy/beam
! Combined flux in latest and established models = 3.22905 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 16 model components to the UV plane model.
! The established model now contains 72 components and 3.22905 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.160737Jy  sigma=0.002068
! Fit after  self-cal, rms=0.160140Jy  sigma=0.002055
! Inverting map and beam 
! Estimated beam: bmin=3.578 mas, bmaj=5.059 mas, bpa=-12.82 degrees
! Estimated noise=418.805 mJy/beam.
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00526124 Jy
! Component: 100  -  total flux cleaned = 0.00459406 Jy
! Total flux subtracted in 100 components = 0.00459406 Jy
! Clean residual min=-0.006118 max=0.005958 Jy/beam
! Clean residual mean=-0.000257 rms=0.001182 Jy/beam
! Combined flux in latest and established models = 3.23364 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 14 model components to the UV plane model.
! The established model now contains 75 components and 3.23364 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.159622Jy  sigma=0.002051
! Fit after  self-cal, rms=0.159314Jy  sigma=0.002044
! Inverting map and beam 
! Estimated beam: bmin=3.576 mas, bmaj=5.057 mas, bpa=-12.78 degrees
! Estimated noise=419.136 mJy/beam.
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00476247 Jy
! Component: 100  -  total flux cleaned = 0.00455632 Jy
! Total flux subtracted in 100 components = 0.00455632 Jy
! Clean residual min=-0.005952 max=0.005673 Jy/beam
! Clean residual mean=-0.000238 rms=0.001131 Jy/beam
! Combined flux in latest and established models = 3.2382 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 14 model components to the UV plane model.
! The established model now contains 76 components and 3.2382 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.158871Jy  sigma=0.002040
! Fit after  self-cal, rms=0.158697Jy  sigma=0.002035
! Inverting map and beam 
! Estimated beam: bmin=3.574 mas, bmaj=5.054 mas, bpa=-12.74 degrees
! Estimated noise=419.453 mJy/beam.
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00436846 Jy
! Component: 100  -  total flux cleaned = 0.00436282 Jy
! Total flux subtracted in 100 components = 0.00436282 Jy
! Clean residual min=-0.005732 max=0.005402 Jy/beam
! Clean residual mean=-0.000223 rms=0.001088 Jy/beam
! Combined flux in latest and established models = 3.24256 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 13 model components to the UV plane model.
! The established model now contains 78 components and 3.24256 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.158311Jy  sigma=0.002032
! Fit after  self-cal, rms=0.158215Jy  sigma=0.002029
! Inverting map and beam 
! Estimated beam: bmin=3.573 mas, bmaj=5.052 mas, bpa=-12.71 degrees
! Estimated noise=419.759 mJy/beam.
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00384488 Jy
! Component: 100  -  total flux cleaned = 0.00384802 Jy
! Total flux subtracted in 100 components = 0.00384802 Jy
! Clean residual min=-0.005582 max=0.005152 Jy/beam
! Clean residual mean=-0.000212 rms=0.001050 Jy/beam
! Combined flux in latest and established models = 3.24641 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 80 components and 3.24641 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.157884Jy  sigma=0.002026
! Fit after  self-cal, rms=0.157828Jy  sigma=0.002024
! Inverting map and beam 
! Estimated beam: bmin=3.571 mas, bmaj=5.051 mas, bpa=-12.67 degrees
! Estimated noise=420.032 mJy/beam.
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0035518 Jy
! Component: 100  -  total flux cleaned = 0.0033817 Jy
! Total flux subtracted in 100 components = 0.0033817 Jy
! Clean residual min=-0.005467 max=0.004933 Jy/beam
! Clean residual mean=-0.000200 rms=0.001020 Jy/beam
! Combined flux in latest and established models = 3.24979 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 81 components and 3.24979 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.157542Jy  sigma=0.002022
! Fit after  self-cal, rms=0.157516Jy  sigma=0.002020
! Inverting map and beam 
! Estimated beam: bmin=3.57 mas, bmaj=5.049 mas, bpa=-12.65 degrees
! Estimated noise=420.292 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 = 0.00329296 Jy
! Component: 100  -  total flux cleaned = 0.0031347 Jy
! Total flux subtracted in 100 components = 0.0031347 Jy
! Clean residual min=-0.005325 max=0.004712 Jy/beam
! Clean residual mean=-0.000190 rms=0.000993 Jy/beam
! Combined flux in latest and established models = 3.25293 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 21 model components to the UV plane model.
! The established model now contains 85 components and 3.25293 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.157267Jy  sigma=0.002018
! Fit after  self-cal, rms=0.157267Jy  sigma=0.002018
! Inverting map 
print "***********************************"
! *********************************** 
print "*** Finished Amplitude Self-Cal ***"
! *** Finished Amplitude Self-Cal *** 
print "***********************************"
! *********************************** 
save 0552+398_S
! Writing UV FITS file: 0552+398_S.uvf
! Writing 85 model components to file: 0552+398_S.mod
! wwins: Wrote 4 windows to 0552+398_S.win
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 3.57 x 5.049 at -12.65 degrees (North through East)
! Clean map  min=-0.0040542  max=3.0662 Jy/beam
! Writing clean map to FITS file: 0552+398_S.fits
! Writing difmap environment to: 0552+398_S.par
print "****************************"
! **************************** 
print "*** Now, make some plots ***"
! *** Now, make some plots *** 
print "****************************"
! **************************** 
![@gonzo_plot 0552+398_S]
device 0552+398_Suv.ps/vps,1,2
! Attempting to open device: '0552+398_Suv.ps/vps'
radplot
! Using default options string "m1"
uvplot
! Using default options string ""
device 0552+398_Sim.ps/vps
! Attempting to open device: '0552+398_Sim.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=3.57 mas, bmaj=5.049 mas, bpa=-12.65 degrees
! Estimated noise=420.292 mJy/beam.
xyrange 0, 0, 0, 0
! The mapplot display area will be limited to:
!  Relative  RA: (The whole available range)
!  Relative DEC: (The whole available range)
mapcolor grey
! Mapplot colormap: grey, contrast: 1 brightness: 0.5.
docont=true
mappl cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 3.57 x 5.049 at -12.65 degrees (North through East)
! Clean map  min=-0.0040542  max=3.0662 Jy/beam
![Exited script file: gonzo_plot]
![Exited script file: gonzo7-0.4]
quit
! Quitting program
! Log file 0552+398_S.log closed on Mon Jul 10 16:39:05 2006