! Started logfile: J0509+1011_X_2010_06_23_pus_uvs.log on Thu Jan 27 23:39:04 2011
obs J0509+1011_X_2010_06_23_pus_uva.fits
! Reading UV FITS file: J0509+1011_X_2010_06_23_pus_uva.fits
! AN table 1: 79 integrations on 105 of 105 possible baselines.
! AN table 2: 21 integrations on 105 of 105 possible baselines.
! AN table 3: 183 integrations on 105 of 105 possible baselines.
! Apparent sampling: 0.311021 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J0509+1011
! 
! 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  8.40996e+09        8e+06          1        8e+06
!  02        2  8.47996e+09        8e+06          1        8e+06
!  03        3  8.79496e+09        8e+06          1        8e+06
!  04        4  8.89996e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 3588 lines of history.
! 
! Reading 36968 visibilities.
select I
! Polarization I is unavailable.
! 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
print "field_size =",field_size
! field_size = 256 
print "field_cell =",field_cell
! field_cell = 0.2 
print "taper_size =",taper_size
! taper_size = 70 
![@muppet J0509+1011_X_2010_06_23_pus]
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.03
float dynam
dynam = 6.0
float soltime1
soltime1 = 120
float soltime2
soltime2 = 20
float thresh
thresh = 0.5
float win_mult
win_mult = 1.8
float time_av
time_av = 16
float old_peak
float new_peak
float flux_cutoff
mapsize field_size, field_cell
! Map grid = 256x256 pixels with 0.200x0.200 milli-arcsec cellsize.
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 740 telescope corrections were flagged in sub-array 1.
!  A total of 149 telescope corrections were flagged in sub-array 2.
!  A total of 1144 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 740 telescope corrections were flagged in sub-array 1.
!  A total of 149 telescope corrections were flagged in sub-array 2.
!  A total of 1262 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 740 telescope corrections were flagged in sub-array 1.
!  A total of 149 telescope corrections were flagged in sub-array 2.
!  A total of 1144 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 740 telescope corrections were flagged in sub-array 1.
!  A total of 149 telescope corrections were flagged in sub-array 2.
!  A total of 1150 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=0.817840Jy  sigma=0.008698
! Fit after  self-cal, rms=0.780429Jy  sigma=0.008341
! clrmod: Cleared the established, tentative and continuum models.
! Redundant starting model cleared.
uvw 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.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
! Estimated beam: bmin=0.6072 mas, bmaj=1.436 mas, bpa=-8.424 degrees
! Estimated noise=783.096 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (0, 0).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.172709 Jy
! Component: 100  -  total flux cleaned = 0.225049 Jy
! Total flux subtracted in 100 components = 0.225049 Jy
! Clean residual min=-0.007700 max=0.022952 Jy/beam
! Clean residual mean=0.000110 rms=0.002754 Jy/beam
! Combined flux in latest and established models = 0.225049 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 8 components and 0.225049 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.161658Jy  sigma=0.001483
! Fit after  self-cal, rms=0.161391Jy  sigma=0.001482
! Inverting map 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0253633 Jy
! Component: 100  -  total flux cleaned = 0.0396076 Jy
! Total flux subtracted in 100 components = 0.0396076 Jy
! Clean residual min=-0.006214 max=0.007479 Jy/beam
! Clean residual mean=0.000077 rms=0.001770 Jy/beam
! Combined flux in latest and established models = 0.264657 Jy
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 23 components and 0.264657 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.155180Jy  sigma=0.001378
! Fit after  self-cal, rms=0.155039Jy  sigma=0.001377
! Inverting map 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
print "************** FINISHED UNIFORM WEIGHTING CLEAN **************"
! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** 
! 
uvw 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
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
! Estimated beam: bmin=0.7933 mas, bmaj=1.987 mas, bpa=-12.95 degrees
! Estimated noise=362.702 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0185873 Jy
! Component: 100  -  total flux cleaned = 0.0270103 Jy
! Component: 150  -  total flux cleaned = 0.0310904 Jy
! Component: 200  -  total flux cleaned = 0.0330945 Jy
! Total flux subtracted in 200 components = 0.0330945 Jy
! Clean residual min=-0.005009 max=0.007264 Jy/beam
! Clean residual mean=0.000139 rms=0.001577 Jy/beam
! Combined flux in latest and established models = 0.297751 Jy
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 36 components and 0.297751 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.153639Jy  sigma=0.001348
! Fit after  self-cal, rms=0.153564Jy  sigma=0.001348
! Inverting map 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.03     FD        1.05     HN        1.00*    KK        1.00     
!   KP        1.08     LA        1.03     MA        1.00*    MK        1.05     
!   NL        1.00*    NY        1.00*    OV        1.09     PT        1.09     
!   SC        1.00*    TS        0.96     ZC        1.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.06     FD        1.06     HN        1.00     KK        1.00*    
!   KP        0.97     LA        1.02     MA        1.00*    MK        1.12     
!   NL        1.07     NY        1.00*    OV        1.01     PT        1.02     
!   SC        1.00     TS        1.00*    ZC        1.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.95     FD        0.96     HN        1.06     KK        1.00*    
!   KP        0.96     LA        0.95     MA        1.36     MK        1.01     
!   NL        1.03     NY        1.04     OV        0.99     PT        0.97     
!   SC        0.94     TS        1.00*    ZC        1.03     
! 
! 
! Correcting IF 2.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.13     FD        1.04     HN        1.00*    KK        1.03     
!   KP        1.06     LA        1.08     MA        1.00*    MK        1.04     
!   NL        1.00*    NY        1.00*    OV        1.08     PT        1.05     
!   SC        1.00*    TS        0.92     ZC        1.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.06     FD        1.06     HN        1.13     KK        1.00*    
!   KP        1.02     LA        0.99     MA        1.00*    MK        1.12     
!   NL        1.09     NY        1.00*    OV        1.10     PT        0.98     
!   SC        1.04     TS        1.00*    ZC        1.00*    
! 
!  A total of 24 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00     FD        0.96     HN        1.09     KK        1.00*    
!   KP        0.96     LA        0.97     MA        1.00*    MK        1.02     
!   NL        1.02     NY        1.04     OV        1.04     PT        0.97     
!   SC        1.03     TS        1.00*    ZC        0.89     
! 
! 
! Correcting IF 3.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.08     FD        1.07     HN        1.00*    KK        0.99     
!   KP        1.05     LA        1.06     MA        1.00*    MK        1.05     
!   NL        1.00*    NY        1.00*    OV        1.06     PT        1.04     
!   SC        1.00*    TS        0.92     ZC        1.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.04     FD        1.00     HN        1.21     KK        1.00*    
!   KP        1.00     LA        1.02     MA        1.00*    MK        1.07     
!   NL        1.03     NY        1.00*    OV        1.04     PT        0.98     
!   SC        1.05     TS        1.00*    ZC        1.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.97     FD        0.94     HN        1.06     KK        1.00*    
!   KP        0.95     LA        0.95     MA        0.89     MK        0.99     
!   NL        0.97     NY        1.08     OV        1.01     PT        0.95     
!   SC        0.92     TS        1.00*    ZC        0.84     
! 
! 
! Correcting IF 4.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.10     FD        1.08     HN        1.00*    KK        1.00     
!   KP        1.07     LA        1.04     MA        1.00*    MK        0.99     
!   NL        1.00*    NY        1.00*    OV        1.05     PT        1.07     
!   SC        1.00*    TS        0.94     ZC        1.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.14     FD        1.02     HN        1.07     KK        1.00*    
!   KP        0.98     LA        1.00     MA        1.00*    MK        1.08     
!   NL        1.02     NY        1.00*    OV        1.09     PT        1.03     
!   SC        0.99     TS        1.00*    ZC        1.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.01     FD        0.94     HN        1.10     KK        1.00*    
!   KP        0.95     LA        0.96     MA        0.88     MK        0.95     
!   NL        0.98     NY        1.02     OV        0.99     PT        0.96     
!   SC        0.94     TS        1.00*    ZC        0.88     
! 
! 
! Fit before self-cal, rms=0.153564Jy  sigma=0.001348
! Fit after  self-cal, rms=0.156233Jy  sigma=0.001329
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
! Estimated beam: bmin=0.7968 mas, bmaj=1.992 mas, bpa=-12.64 degrees
! Estimated noise=362.776 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00182382 Jy
! Component: 100  -  total flux cleaned = -0.00202549 Jy
! Component: 150  -  total flux cleaned = -0.00214921 Jy
! Component: 200  -  total flux cleaned = -0.00219941 Jy
! Total flux subtracted in 200 components = -0.00219941 Jy
! Clean residual min=-0.002381 max=0.003190 Jy/beam
! Clean residual mean=0.000085 rms=0.000856 Jy/beam
! Combined flux in latest and established models = 0.295552 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 42 components and 0.295552 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.156199Jy  sigma=0.001329
! Fit after  self-cal, rms=0.156357Jy  sigma=0.001329
! Inverting map 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
selfcal true, true, soltime1
! Performing amp+phase self-cal over 120 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.156357Jy  sigma=0.001329
! Fit after  self-cal, rms=0.157617Jy  sigma=0.001325
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
! Estimated beam: bmin=0.7995 mas, bmaj=1.996 mas, bpa=-12.57 degrees
! Estimated noise=362.947 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000779172 Jy
! Component: 100  -  total flux cleaned = -0.000897593 Jy
! Component: 150  -  total flux cleaned = -0.000975652 Jy
! Component: 200  -  total flux cleaned = -0.00102293 Jy
! Total flux subtracted in 200 components = -0.00102293 Jy
! Clean residual min=-0.001810 max=0.002644 Jy/beam
! Clean residual mean=0.000078 rms=0.000680 Jy/beam
! Combined flux in latest and established models = 0.294529 Jy
selfcal
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 44 components and 0.294529 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.157601Jy  sigma=0.001325
! Fit after  self-cal, rms=0.157621Jy  sigma=0.001325
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -7.87838e-05 Jy
! Component: 100  -  total flux cleaned = -0.000141678 Jy
! Component: 150  -  total flux cleaned = -0.000179569 Jy
! Component: 200  -  total flux cleaned = -0.000214754 Jy
! Total flux subtracted in 200 components = -0.000214754 Jy
! Clean residual min=-0.001798 max=0.002707 Jy/beam
! Clean residual mean=0.000080 rms=0.000680 Jy/beam
! Combined flux in latest and established models = 0.294314 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 44 components and 0.294314 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.157614Jy  sigma=0.001325
! Fit after  self-cal, rms=0.157614Jy  sigma=0.001324
! Inverting map 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
selfcal true, true, soltime2
! Performing amp+phase self-cal over 20 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.157614Jy  sigma=0.001324
! Fit after  self-cal, rms=0.158263Jy  sigma=0.001324
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
! Estimated beam: bmin=0.8014 mas, bmaj=2.002 mas, bpa=-12.54 degrees
! Estimated noise=363.112 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000782173 Jy
! Component: 100  -  total flux cleaned = -0.000883615 Jy
! Component: 150  -  total flux cleaned = -0.000929261 Jy
! Component: 200  -  total flux cleaned = -0.000991694 Jy
! Total flux subtracted in 200 components = -0.000991694 Jy
! Clean residual min=-0.001766 max=0.002586 Jy/beam
! Clean residual mean=0.000080 rms=0.000665 Jy/beam
! Combined flux in latest and established models = 0.293322 Jy
selfcal
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 44 components and 0.293322 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.158252Jy  sigma=0.001324
! Fit after  self-cal, rms=0.158261Jy  sigma=0.001324
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -6.57007e-05 Jy
! Component: 100  -  total flux cleaned = -0.00010225 Jy
! Component: 150  -  total flux cleaned = -0.000136559 Jy
! Component: 200  -  total flux cleaned = -0.000168768 Jy
! Total flux subtracted in 200 components = -0.000168768 Jy
! Clean residual min=-0.001760 max=0.002621 Jy/beam
! Clean residual mean=0.000082 rms=0.000666 Jy/beam
! Combined flux in latest and established models = 0.293154 Jy
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 44 components and 0.293154 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.158256Jy  sigma=0.001324
! Fit after  self-cal, rms=0.158255Jy  sigma=0.001324
! Inverting map 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
win_mult = win_mult * 1.2
selfcal true, true, soltime2
! Performing amp+phase self-cal over 20 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.158255Jy  sigma=0.001324
! Fit after  self-cal, rms=0.158791Jy  sigma=0.001324
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
! Estimated beam: bmin=2.545 mas, bmaj=3.572 mas, bpa=-22.99 degrees
! Estimated noise=423.599 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -4.89467e-05 Jy
! Component: 100  -  total flux cleaned = -5.2137e-05 Jy
! Component: 150  -  total flux cleaned = -7.42747e-05 Jy
! Component: 200  -  total flux cleaned = -0.000112265 Jy
! Total flux subtracted in 200 components = -0.000112265 Jy
! Clean residual min=-0.002137 max=0.003100 Jy/beam
! Clean residual mean=0.000135 rms=0.000860 Jy/beam
! Combined flux in latest and established models = 0.293041 Jy
selfcal
! Performing phase self-cal
! Adding 5 model components to the UV plane model.
! The established model now contains 45 components and 0.293041 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.158790Jy  sigma=0.001324
! Fit after  self-cal, rms=0.158791Jy  sigma=0.001324
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -4.62639e-05 Jy
! Component: 100  -  total flux cleaned = -6.97227e-05 Jy
! Component: 150  -  total flux cleaned = -8.93263e-05 Jy
! Component: 200  -  total flux cleaned = -9.08891e-05 Jy
! Total flux subtracted in 200 components = -9.08891e-05 Jy
! Clean residual min=-0.002132 max=0.003090 Jy/beam
! Clean residual mean=0.000137 rms=0.000862 Jy/beam
! Combined flux in latest and established models = 0.292951 Jy
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 45 components and 0.292951 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.158793Jy  sigma=0.001324
! Fit after  self-cal, rms=0.158787Jy  sigma=0.001324
! Inverting map 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
win_mult = win_mult / 1.2
print "************** FINISHED AMPLITUDE SELF-CAL **************"
! ************** FINISHED AMPLITUDE SELF-CAL ************** 
restore
! Inverting map and beam 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
! Estimated beam: bmin=0.8031 mas, bmaj=2.008 mas, bpa=-12.51 degrees
! Estimated noise=363.242 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8031 x 2.008 at -12.51 degrees (North through East)
! Clean map  min=-0.0015911  max=0.24481 Jy/beam
if(peak(flux) > thresh)
  selfcal true, true
  clean clean_niter,clean_gain
  selfcal
  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
    new_peak = peak(flux)
    until(new_peak<=flux_cutoff)
  selfcal true, true
  end if
print "************** CLEARING MODEL AND STARTING OVER **********"
! ************** CLEARING MODEL AND STARTING OVER ********** 
clrmod true
! clrmod: Cleared the established and tentative models.
uvw 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.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
! Estimated beam: bmin=0.6074 mas, bmaj=1.447 mas, bpa=-7.947 degrees
! Estimated noise=801.769 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.176558 Jy
! Component: 100  -  total flux cleaned = 0.231142 Jy
! Component: 150  -  total flux cleaned = 0.255954 Jy
! Component: 200  -  total flux cleaned = 0.26904 Jy
! Total flux subtracted in 200 components = 0.26904 Jy
! Clean residual min=-0.004159 max=0.007094 Jy/beam
! Clean residual mean=0.000042 rms=0.001253 Jy/beam
! Combined flux in latest and established models = 0.26904 Jy
uvw 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.
flux_cutoff = imstat(rms) * dynam
! Adding 15 model components to the UV plane model.
! The established model now contains 15 components and 0.26904 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
! Estimated beam: bmin=0.8031 mas, bmaj=2.008 mas, bpa=-12.51 degrees
! Estimated noise=363.242 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  keep
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0127559 Jy
! Component: 100  -  total flux cleaned = 0.0182571 Jy
! Component: 150  -  total flux cleaned = 0.0208085 Jy
! Component: 200  -  total flux cleaned = 0.0220159 Jy
! Total flux subtracted in 200 components = 0.0220159 Jy
! Clean residual min=-0.001775 max=0.002973 Jy/beam
! Clean residual mean=0.000091 rms=0.000676 Jy/beam
! Combined flux in latest and established models = 0.291056 Jy
! Adding 21 model components to the UV plane model.
! The established model now contains 31 components and 0.291056 Jy
! Inverting map 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
! Added new window around map position (-1.6, 1.8).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00273666 Jy
! Component: 100  -  total flux cleaned = 0.00355891 Jy
! Component: 150  -  total flux cleaned = 0.00370613 Jy
! Component: 200  -  total flux cleaned = 0.00378994 Jy
! Total flux subtracted in 200 components = 0.00378994 Jy
! Clean residual min=-0.001678 max=0.002493 Jy/beam
! Clean residual mean=0.000054 rms=0.000565 Jy/beam
! Combined flux in latest and established models = 0.294846 Jy
! Adding 18 model components to the UV plane model.
! The established model now contains 48 components and 0.294846 Jy
! Inverting map 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
! Added new window around map position (-1, 8).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00200298 Jy
! Component: 100  -  total flux cleaned = 0.00229824 Jy
! Component: 150  -  total flux cleaned = 0.00239049 Jy
! Component: 200  -  total flux cleaned = 0.00260211 Jy
! Total flux subtracted in 200 components = 0.00260211 Jy
! Clean residual min=-0.001523 max=0.001738 Jy/beam
! Clean residual mean=0.000016 rms=0.000483 Jy/beam
! Combined flux in latest and established models = 0.297448 Jy
! Adding 23 model components to the UV plane model.
! The established model now contains 67 components and 0.297448 Jy
! Inverting map 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
! Estimated beam: bmin=2.545 mas, bmaj=3.572 mas, bpa=-22.99 degrees
! Estimated noise=423.599 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000684104 Jy
! Component: 100  -  total flux cleaned = 0.000774649 Jy
! Component: 150  -  total flux cleaned = 0.000813153 Jy
! Component: 200  -  total flux cleaned = 0.000831219 Jy
! Total flux subtracted in 200 components = 0.000831219 Jy
! Clean residual min=-0.001757 max=0.001349 Jy/beam
! Clean residual mean=-0.000003 rms=0.000517 Jy/beam
! Combined flux in latest and established models = 0.29828 Jy
flux_cutoff = imstat(rms) * dynam
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  keep
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 3.1844e-05 Jy
! Component: 100  -  total flux cleaned = 6.07374e-05 Jy
! Component: 150  -  total flux cleaned = 8.80389e-05 Jy
! Component: 200  -  total flux cleaned = 0.00012645 Jy
! Total flux subtracted in 200 components = 0.00012645 Jy
! Clean residual min=-0.001762 max=0.001260 Jy/beam
! Clean residual mean=-0.000007 rms=0.000511 Jy/beam
! Combined flux in latest and established models = 0.298406 Jy
! Adding 23 model components to the UV plane model.
! The established model now contains 86 components and 0.298406 Jy
! Inverting map 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
! Estimated beam: bmin=0.8031 mas, bmaj=2.008 mas, bpa=-12.51 degrees
! Estimated noise=363.242 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000145266 Jy
! Component: 100  -  total flux cleaned = -0.000180134 Jy
! Component: 150  -  total flux cleaned = -0.000179363 Jy
! Component: 200  -  total flux cleaned = -0.00014748 Jy
! Total flux subtracted in 200 components = -0.00014748 Jy
! Clean residual min=-0.001497 max=0.001662 Jy/beam
! Clean residual mean=0.000003 rms=0.000458 Jy/beam
! Combined flux in latest and established models = 0.298259 Jy
selfcal
! Performing phase self-cal
! Adding 25 model components to the UV plane model.
! The established model now contains 98 components and 0.298259 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.158643Jy  sigma=0.001323
! Fit after  self-cal, rms=0.158630Jy  sigma=0.001322
wmodel J0509+1011_X_2010_06_23_pus_map.mod
! Writing 98 model components to file: J0509+1011_X_2010_06_23_pus_map.mod
wobs J0509+1011_X_2010_06_23_pus_uvs.fits
! Writing UV FITS file: J0509+1011_X_2010_06_23_pus_uvs.fits
wwins J0509+1011_X_2010_06_23_pus_map.win
! wwins: Wrote 3 windows to J0509+1011_X_2010_06_23_pus_map.win
x = (field_size-8) * field_cell / 4
addwin -x,x,-x,x
clean (field_size*4),0.01
! Inverting map 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.000738235 Jy
! Component: 100  -  total flux cleaned = 0.00100798 Jy
! Component: 150  -  total flux cleaned = 0.0011105 Jy
! Component: 200  -  total flux cleaned = 0.00115909 Jy
! Component: 250  -  total flux cleaned = 0.00118362 Jy
! Component: 300  -  total flux cleaned = 0.00125212 Jy
! Component: 350  -  total flux cleaned = 0.00114223 Jy
! Component: 400  -  total flux cleaned = 0.00103546 Jy
! Component: 450  -  total flux cleaned = 0.000972595 Jy
! Component: 500  -  total flux cleaned = 0.00091056 Jy
! Component: 550  -  total flux cleaned = 0.000809723 Jy
! Component: 600  -  total flux cleaned = 0.000770024 Jy
! Component: 650  -  total flux cleaned = 0.000672579 Jy
! Component: 700  -  total flux cleaned = 0.000596468 Jy
! Component: 750  -  total flux cleaned = 0.000521452 Jy
! Component: 800  -  total flux cleaned = 0.000502947 Jy
! Component: 850  -  total flux cleaned = 0.000393836 Jy
! Component: 900  -  total flux cleaned = 0.000393699 Jy
! Component: 950  -  total flux cleaned = 0.000340722 Jy
! Component: 1000  -  total flux cleaned = 0.000340639 Jy
! Total flux subtracted in 1024 components = 0.000340708 Jy
! Clean residual min=-0.001074 max=0.001055 Jy/beam
! Clean residual mean=-0.000012 rms=0.000350 Jy/beam
! Combined flux in latest and established models = 0.298599 Jy
keep
! Adding 73 model components to the UV plane model.
! The established model now contains 171 components and 0.298599 Jy
![Exited script file: muppet]
wmap "J0509+1011_X_2010_06_23_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8031 x 2.008 at -12.51 degrees (North through East)
! Clean map  min=-0.0017567  max=0.24549 Jy/beam
! Writing clean map to FITS file: J0509+1011_X_2010_06_23_pus_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.245493 
invert
! Inverting map 
! Your choice of large map pixels excluded 7.37% of the data.
!  The x-axis pixel size should ideally be below 0.1735 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000350187 
device "J0509+1011_X_2010_06_23_pus\_map.eps/VPS"
! Attempting to open device: 'J0509+1011_X_2010_06_23_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.42794 0.42794 0.855881 1.71176 3.42352 6.84705 13.6941 27.3882 54.7764
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.001 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.245 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8031 x 2.008 at -12.51 degrees (North through East)
! Clean map  min=-0.0017567  max=0.24549 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0509+1011_X_2010_06_23_pus\_map.gif/vgif"
! Attempting to open device: 'J0509+1011_X_2010_06_23_pus_map.gif/vgif'
mapplot cln