! Started logfile: 0202+149_X.log on Thu Feb 14 23:23:11 2008
observe 0202+149_X.edt
! Reading UV FITS file: 0202+149_X.edt
! AN table 1: 30 integrations on 136 of 136 possible baselines.
! AN table 2: 57 integrations on 136 of 136 possible baselines.
! AN table 3: 23 integrations on 136 of 136 possible baselines.
! AN table 4: 48 integrations on 136 of 136 possible baselines.
! Apparent sampling: 0.234736 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: 0202+149
! 
! 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 20176 visibilities.
![@gonzo6-0.1 0202+149_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 326 telescope corrections were flagged in sub-array 1.
!  A total of 581 telescope corrections were flagged in sub-array 2.
!  A total of 230 telescope corrections were flagged in sub-array 3.
!  A total of 726 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 2.
!  A total of 326 telescope corrections were flagged in sub-array 1.
!  A total of 582 telescope corrections were flagged in sub-array 2.
!  A total of 230 telescope corrections were flagged in sub-array 3.
!  A total of 725 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 3.
!  A total of 326 telescope corrections were flagged in sub-array 1.
!  A total of 571 telescope corrections were flagged in sub-array 2.
!  A total of 231 telescope corrections were flagged in sub-array 3.
!  A total of 736 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 4.
!  A total of 327 telescope corrections were flagged in sub-array 1.
!  A total of 626 telescope corrections were flagged in sub-array 2.
!  A total of 230 telescope corrections were flagged in sub-array 3.
!  A total of 733 telescope corrections were flagged in sub-array 4.
! 
! Fit before self-cal, rms=0.517826Jy  sigma=0.009109
! Fit after  self-cal, rms=0.514688Jy  sigma=0.009008
! 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=0.5434 mas, bmaj=1.306 mas, bpa=-14.68 degrees
! Estimated noise=817.472 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 = 0.956696 Jy
! Total flux subtracted in 50 components = 0.956696 Jy
! Clean residual min=-0.061784 max=0.326241 Jy/beam
! Clean residual mean=-0.000392 rms=0.019512 Jy/beam
! Combined flux in latest and established models = 0.956696 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 6 components and 0.956696 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.546447Jy  sigma=0.009509
! Fit after  self-cal, rms=0.546361Jy  sigma=0.009508
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.348963 Jy
! Total flux subtracted in 50 components = 0.348963 Jy
! Clean residual min=-0.035987 max=0.157612 Jy/beam
! Clean residual mean=-0.000220 rms=0.010407 Jy/beam
! Combined flux in latest and established models = 1.30566 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 9 components and 1.30566 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.307370Jy  sigma=0.005397
! Fit after  self-cal, rms=0.306798Jy  sigma=0.005390
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.170351 Jy
! Total flux subtracted in 50 components = 0.170351 Jy
! Clean residual min=-0.023367 max=0.076940 Jy/beam
! Clean residual mean=-0.000137 rms=0.006459 Jy/beam
! Combined flux in latest and established models = 1.47601 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 10 components and 1.47601 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.206848Jy  sigma=0.003591
! Fit after  self-cal, rms=0.206150Jy  sigma=0.003580
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0896838 Jy
! Total flux subtracted in 50 components = 0.0896838 Jy
! Clean residual min=-0.016734 max=0.045625 Jy/beam
! Clean residual mean=-0.000093 rms=0.004757 Jy/beam
! Combined flux in latest and established models = 1.56569 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 18 components and 1.56569 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.166085Jy  sigma=0.002793
! Fit after  self-cal, rms=0.165599Jy  sigma=0.002786
! Inverting map 
! Added new window around map position (-0.7, 0.3).
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0563763 Jy
! Total flux subtracted in 50 components = 0.0563763 Jy
! Clean residual min=-0.013406 max=0.029439 Jy/beam
! Clean residual mean=-0.000065 rms=0.003917 Jy/beam
! Combined flux in latest and established models = 1.62207 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 29 components and 1.62207 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.146727Jy  sigma=0.002388
! Fit after  self-cal, rms=0.146339Jy  sigma=0.002384
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0382262 Jy
! Total flux subtracted in 50 components = 0.0382262 Jy
! Clean residual min=-0.012364 max=0.028546 Jy/beam
! Clean residual mean=-0.000046 rms=0.003483 Jy/beam
! Combined flux in latest and established models = 1.6603 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 11 model components to the UV plane model.
! The established model now contains 35 components and 1.6603 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.136711Jy  sigma=0.002169
! Fit after  self-cal, rms=0.136601Jy  sigma=0.002168
! Inverting map 
! Added new window around map position (-4.5, 2.6).
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.032067 Jy
! Total flux subtracted in 50 components = 0.032067 Jy
! Clean residual min=-0.011519 max=0.021504 Jy/beam
! Clean residual mean=-0.000038 rms=0.003141 Jy/beam
! Combined flux in latest and established models = 1.69236 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 42 components and 1.69236 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.129528Jy  sigma=0.001998
! Fit after  self-cal, rms=0.129310Jy  sigma=0.001997
! Inverting map 
! Added new window around map position (-3.3, 3.6).
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0266466 Jy
! Total flux subtracted in 50 components = 0.0266466 Jy
! Clean residual min=-0.010824 max=0.015884 Jy/beam
! Clean residual mean=-0.000033 rms=0.002864 Jy/beam
! Combined flux in latest and established models = 1.71901 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 54 components and 1.71901 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.124410Jy  sigma=0.001868
! Fit after  self-cal, rms=0.124193Jy  sigma=0.001867
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0223711 Jy
! Total flux subtracted in 50 components = 0.0223711 Jy
! Clean residual min=-0.010241 max=0.015082 Jy/beam
! Clean residual mean=-0.000027 rms=0.002650 Jy/beam
! Combined flux in latest and established models = 1.74138 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 56 components and 1.74138 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.120471Jy  sigma=0.001767
! Fit after  self-cal, rms=0.120348Jy  sigma=0.001766
! 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=0.6628 mas, bmaj=1.596 mas, bpa=-16.92 degrees
! Estimated noise=417.507 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 = 0.0329747 Jy
! Component: 100  -  total flux cleaned = 0.058031 Jy
! Total flux subtracted in 100 components = 0.058031 Jy
! Clean residual min=-0.011143 max=0.018205 Jy/beam
! Clean residual mean=-0.000096 rms=0.003396 Jy/beam
! Combined flux in latest and established models = 1.79941 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 50 model components to the UV plane model.
! The established model now contains 89 components and 1.79941 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.112986Jy  sigma=0.001544
! Fit after  self-cal, rms=0.112463Jy  sigma=0.001539
! 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        0.99     FD        0.99     GC        1.02     HN        0.99     
!   KK        1.00*    KP        0.99     LA        0.98     MC        1.10     
!   MK        1.00*    NL        0.99     NY        1.02     ON        1.07     
!   OV        0.99     PT        0.98     SC        1.01     WF        0.98     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.99     FD        0.99     GC        1.00*    HN        0.99     
!   KK        0.99     KP        0.99     LA        0.99     MC        1.04     
!   MK        1.00     NL        0.99     NY        1.02     ON        1.00*    
!   OV        0.99     PT        0.99     SC        0.99     WF        0.99     
!   WZ        1.03     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.99     FD        0.99     GC        1.00     HN        1.00     
!   KK        1.00     KP        0.99     LA        0.99     MC        1.00*    
!   MK        1.00     NL        0.99     NY        1.03     ON        1.00*    
!   OV        0.99     PT        1.00*    SC        0.99     WF        1.00     
!   WZ        1.00*    
! 
!  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*    HN        0.98     
!   KK        1.00*    KP        1.00*    LA        1.00*    MC        1.02     
!   MK        1.00*    NL        0.99     NY        1.00*    ON        1.00*    
!   OV        1.00*    PT        1.00*    SC        1.02     WF        0.98     
!   WZ        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     FD        0.99     GC        1.02     HN        0.99     
!   KK        1.00*    KP        0.99     LA        0.98     MC        1.11     
!   MK        1.00*    NL        0.99     NY        1.02     ON        1.09     
!   OV        0.99     PT        0.99     SC        1.01     WF        0.99     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.99     FD        0.99     GC        1.00*    HN        0.99     
!   KK        1.00     KP        0.99     LA        0.99     MC        1.05     
!   MK        1.00     NL        0.99     NY        1.02     ON        1.00*    
!   OV        0.99     PT        0.99     SC        0.99     WF        0.99     
!   WZ        1.03     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.99     FD        0.99     GC        1.01     HN        1.00     
!   KK        1.01     KP        0.99     LA        0.99     MC        1.00*    
!   MK        1.01     NL        0.99     NY        1.03     ON        1.00*    
!   OV        0.99     PT        1.00*    SC        0.98     WF        1.00     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        1.00*    GC        1.00*    HN        0.98     
!   KK        1.00*    KP        1.00*    LA        1.00*    MC        1.02     
!   MK        1.00*    NL        0.99     NY        1.00*    ON        1.00*    
!   OV        1.00*    PT        1.00*    SC        1.02     WF        0.98     
!   WZ        1.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        0.99     GC        1.03     HN        0.99     
!   KK        1.00*    KP        0.99     LA        0.98     MC        1.10     
!   MK        1.00*    NL        0.99     NY        1.02     ON        1.12     
!   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        0.99     
!   KK        1.00     KP        0.99     LA        0.99     MC        1.06     
!   MK        1.00     NL        0.99     NY        1.01     ON        1.03     
!   OV        0.99     PT        0.99     SC        0.99     WF        0.99     
!   WZ        1.03     
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.99     FD        0.99     GC        1.01     HN        1.00     
!   KK        1.00     KP        0.99     LA        0.99     MC        1.00*    
!   MK        1.01     NL        0.99     NY        1.03     ON        1.00*    
!   OV        0.99     PT        1.00*    SC        0.99     WF        1.00     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        1.00*    GC        1.00*    HN        0.97     
!   KK        1.00*    KP        1.00*    LA        1.00*    MC        1.03     
!   MK        1.00*    NL        1.00*    NY        1.00*    ON        1.00*    
!   OV        1.00*    PT        1.00*    SC        1.03     WF        0.97     
!   WZ        1.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     FD        0.99     GC        1.02     HN        0.99     
!   KK        1.00*    KP        0.99     LA        0.98     MC        1.10     
!   MK        1.00*    NL        0.99     NY        1.02     ON        1.11     
!   OV        0.99     PT        0.98     SC        1.01     WF        0.99     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.99     FD        0.99     GC        1.00*    HN        0.99     
!   KK        0.99     KP        0.99     LA        0.99     MC        1.05     
!   MK        1.00     NL        0.99     NY        1.02     ON        1.02     
!   OV        0.99     PT        0.99     SC        0.99     WF        0.99     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.99     FD        0.99     GC        1.01     HN        1.00     
!   KK        1.01     KP        0.99     LA        0.99     MC        1.00*    
!   MK        1.01     NL        0.99     NY        1.04     ON        1.00*    
!   OV        0.99     PT        1.00*    SC        0.99     WF        1.00     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        1.00*    GC        1.00*    HN        0.97     
!   KK        1.00*    KP        1.00*    LA        1.00*    MC        1.03     
!   MK        1.00*    NL        1.00     NY        1.00*    ON        1.00*    
!   OV        1.00*    PT        1.00*    SC        1.03     WF        0.96     
!   WZ        1.00*    
! 
! 
! Fit before self-cal, rms=0.112463Jy  sigma=0.001539
! Fit after  self-cal, rms=0.108445Jy  sigma=0.001449
dynam = dynam - 0.5
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=0.6712 mas, bmaj=1.604 mas, bpa=-16.95 degrees
! Estimated noise=415.566 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 = 0.0198543 Jy
! Component: 100  -  total flux cleaned = 0.0334077 Jy
! Total flux subtracted in 100 components = 0.0334077 Jy
! Clean residual min=-0.007631 max=0.012062 Jy/beam
! Clean residual mean=-0.000016 rms=0.002157 Jy/beam
! Combined flux in latest and established models = 1.83282 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 38 model components to the UV plane model.
! The established model now contains 123 components and 1.83282 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.105966Jy  sigma=0.001354
! Fit after  self-cal, rms=0.105571Jy  sigma=0.001349
! Inverting map 
! Added new window around map position (-3.2, 1.3).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0128856 Jy
! Component: 100  -  total flux cleaned = 0.0220765 Jy
! Total flux subtracted in 100 components = 0.0220765 Jy
! Clean residual min=-0.007372 max=0.010601 Jy/beam
! Clean residual mean=-0.000000 rms=0.001809 Jy/beam
! Combined flux in latest and established models = 1.8549 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 154 components and 1.8549 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.104358Jy  sigma=0.001308
! Fit after  self-cal, rms=0.104152Jy  sigma=0.001306
! Inverting map 
! Added new window around map position (-2.1, 4.7).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00988077 Jy
! Component: 100  -  total flux cleaned = 0.0160867 Jy
! Total flux subtracted in 100 components = 0.0160867 Jy
! Clean residual min=-0.007313 max=0.006547 Jy/beam
! Clean residual mean=0.000008 rms=0.001617 Jy/beam
! Combined flux in latest and established models = 1.87098 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 175 components and 1.87098 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.103435Jy  sigma=0.001281
! Fit after  self-cal, rms=0.103328Jy  sigma=0.001280
! 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 = 0.00453191 Jy
! Component: 100  -  total flux cleaned = 0.00675217 Jy
! Total flux subtracted in 100 components = 0.00675217 Jy
! Clean residual min=-0.007274 max=0.006151 Jy/beam
! Clean residual mean=0.000011 rms=0.001545 Jy/beam
! Combined flux in latest and established models = 1.87774 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 37 model components to the UV plane model.
! The established model now contains 200 components and 1.87774 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.102997Jy  sigma=0.001271
! Fit after  self-cal, rms=0.101184Jy  sigma=0.001242
! Inverting map and beam 
! Estimated beam: bmin=0.6722 mas, bmaj=1.602 mas, bpa=-16.93 degrees
! Estimated noise=415.222 mJy/beam.
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00807236 Jy
! Component: 100  -  total flux cleaned = 0.0128299 Jy
! Total flux subtracted in 100 components = 0.0128299 Jy
! Clean residual min=-0.005481 max=0.004870 Jy/beam
! Clean residual mean=-0.000007 rms=0.001228 Jy/beam
! Combined flux in latest and established models = 1.89057 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 31 model components to the UV plane model.
! The established model now contains 222 components and 1.89057 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.100627Jy  sigma=0.001224
! Fit after  self-cal, rms=0.100341Jy  sigma=0.001221
! Inverting map and beam 
! Estimated beam: bmin=0.6723 mas, bmaj=1.601 mas, bpa=-16.92 degrees
! Estimated noise=415.138 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 = 0.00559615 Jy
! Component: 100  -  total flux cleaned = 0.00910964 Jy
! Total flux subtracted in 100 components = 0.00910964 Jy
! Clean residual min=-0.005158 max=0.004325 Jy/beam
! Clean residual mean=-0.000008 rms=0.001107 Jy/beam
! Combined flux in latest and established models = 1.89968 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 41 model components to the UV plane model.
! The established model now contains 244 components and 1.89968 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.099977Jy  sigma=0.001210
! Fit after  self-cal, rms=0.099923Jy  sigma=0.001209
! Inverting map 
print "***********************************"
! *********************************** 
print "*** Finished Amplitude Self-Cal ***"
! *** Finished Amplitude Self-Cal *** 
print "***********************************"
! *********************************** 
save 0202+149_X
! Writing UV FITS file: 0202+149_X.uvf
! Writing 244 model components to file: 0202+149_X.mod
! wwins: Wrote 6 windows to 0202+149_X.win
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6723 x 1.601 at -16.92 degrees (North through East)
! Clean map  min=-0.0048956  max=1.326 Jy/beam
! Writing clean map to FITS file: 0202+149_X.fits
! Writing difmap environment to: 0202+149_X.par
print "****************************"
! **************************** 
print "*** Now, make some plots ***"
! *** Now, make some plots *** 
print "****************************"
! **************************** 
![@gonzo_plot 0202+149_X]
device 0202+149_Xuv.ps/vps,1,2
! Attempting to open device: '0202+149_Xuv.ps/vps'
radplot
! Using default options string "m1"
uvplot
! Using default options string ""
device 0202+149_Xim.ps/vps
! Attempting to open device: '0202+149_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=0.6723 mas, bmaj=1.601 mas, bpa=-16.92 degrees
! Estimated noise=415.138 mJy/beam.
mappl cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6723 x 1.601 at -16.92 degrees (North through East)
! Clean map  min=-0.0048956  max=1.326 Jy/beam
![Exited script file: gonzo_plot]
![Exited script file: gonzo6-0.1]
quit
! Quitting program
! Log file 0202+149_X.log closed on Thu Feb 14 23:23:22 2008