! Started logfile: J1521+4336_X_2009_04_21_pus_uvs.log on Sun Jan 23 00:36:16 2011
obs J1521+4336_X_2009_04_21_pus_uva.fits
! Reading UV FITS file: J1521+4336_X_2009_04_21_pus_uva.fits
! AN table 1: 124 integrations on 120 of 120 possible baselines.
! AN table 2: 307 integrations on 120 of 120 possible baselines.
! AN table 3: 183 integrations on 120 of 120 possible baselines.
! Apparent sampling: 0.160898 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J1521+4336
! 
! 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 2445 lines of history.
! 
! Reading 47420 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 = 512 
print "field_cell =",field_cell
! field_cell = 0.2 
print "taper_size =",taper_size
! taper_size = 70 
![@muppet J1521+4336_X_2009_04_21_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 = 512x512 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 1486 telescope corrections were flagged in sub-array 1.
!  A total of 3319 telescope corrections were flagged in sub-array 2.
!  A total of 1856 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 1486 telescope corrections were flagged in sub-array 1.
!  A total of 3319 telescope corrections were flagged in sub-array 2.
!  A total of 1856 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 1486 telescope corrections were flagged in sub-array 1.
!  A total of 3320 telescope corrections were flagged in sub-array 2.
!  A total of 1856 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 1486 telescope corrections were flagged in sub-array 1.
!  A total of 3319 telescope corrections were flagged in sub-array 2.
!  A total of 1856 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=0.758510Jy  sigma=0.006008
! Fit after  self-cal, rms=0.619511Jy  sigma=0.004967
! 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 4.52% of the data.
!  The x-axis pixel size should ideally be below 0.16 milli-arcsec
! Estimated beam: bmin=0.4734 mas, bmaj=0.8019 mas, bpa=-6.204 degrees
! Estimated noise=859.619 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 = 0.312604 Jy
! Component: 100  -  total flux cleaned = 0.382818 Jy
! Total flux subtracted in 100 components = 0.382818 Jy
! Clean residual min=-0.009867 max=0.024959 Jy/beam
! Clean residual mean=0.000101 rms=0.002510 Jy/beam
! Combined flux in latest and established models = 0.382818 Jy
! Performing phase self-cal
! Adding 4 model components to the UV plane model.
! The established model now contains 4 components and 0.382818 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.181252Jy  sigma=0.001327
! Fit after  self-cal, rms=0.181228Jy  sigma=0.001326
! Inverting map 
! Your choice of large map pixels excluded 4.52% of the data.
!  The x-axis pixel size should ideally be below 0.16 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0277971 Jy
! Component: 100  -  total flux cleaned = 0.0434679 Jy
! Total flux subtracted in 100 components = 0.0434679 Jy
! Clean residual min=-0.009615 max=0.016118 Jy/beam
! Clean residual mean=0.000031 rms=0.002124 Jy/beam
! Combined flux in latest and established models = 0.426286 Jy
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 9 components and 0.426286 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.176703Jy  sigma=0.001270
! Fit after  self-cal, rms=0.176619Jy  sigma=0.001270
! Inverting map 
! Your choice of large map pixels excluded 4.52% of the data.
!  The x-axis pixel size should ideally be below 0.16 milli-arcsec
! Added new window around map position (0, 1.2).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0147662 Jy
! Component: 100  -  total flux cleaned = 0.0232521 Jy
! Total flux subtracted in 100 components = 0.0232521 Jy
! Clean residual min=-0.009107 max=0.010248 Jy/beam
! Clean residual mean=-0.000004 rms=0.001991 Jy/beam
! Combined flux in latest and established models = 0.449538 Jy
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 16 components and 0.449538 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.175491Jy  sigma=0.001253
! Fit after  self-cal, rms=0.175399Jy  sigma=0.001253
! Inverting map 
! Your choice of large map pixels excluded 4.52% of the data.
!  The x-axis pixel size should ideally be below 0.16 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 4.52% of the data.
!  The x-axis pixel size should ideally be below 0.16 milli-arcsec
! Estimated beam: bmin=0.5864 mas, bmaj=0.9348 mas, bpa=-2.276 degrees
! Estimated noise=420.511 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 (-7, 24.8).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0101011 Jy
! Component: 100  -  total flux cleaned = 0.0164026 Jy
! Component: 150  -  total flux cleaned = 0.0192025 Jy
! Component: 200  -  total flux cleaned = 0.0211362 Jy
! Total flux subtracted in 200 components = 0.0211362 Jy
! Clean residual min=-0.006047 max=0.007642 Jy/beam
! Clean residual mean=0.000141 rms=0.001585 Jy/beam
! Combined flux in latest and established models = 0.470674 Jy
! Performing phase self-cal
! Adding 20 model components to the UV plane model.
! The established model now contains 30 components and 0.470674 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.174872Jy  sigma=0.001245
! Fit after  self-cal, rms=0.174819Jy  sigma=0.001245
! Inverting map 
! Your choice of large map pixels excluded 4.52% of the data.
!  The x-axis pixel size should ideally be below 0.16 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 105 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        0.99     HN        1.02     KB        0.93     
!   KK        0.96     KP        1.00     LA        1.00     MK        0.98     
!   NL        1.01     NY        1.00*    OV        1.01     PT        1.02     
!   SC        0.98     TS        0.92     WZ        1.00*    ZC        1.03     
! 
!  A total of 255 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.93     FD        0.98     HN        1.03     KB        1.07     
!   KK        1.02     KP        0.97     LA        0.99     MK        1.02     
!   NL        0.93     NY        0.95     OV        0.97     PT        0.96     
!   SC        0.99     TS        0.94     WZ        1.15     ZC        0.99     
! 
!  A total of 81 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.99     FD        0.99     HN        1.04     KB        0.93     
!   KK        1.00*    KP        1.07     LA        1.01     MK        1.00*    
!   NL        1.01     NY        0.95     OV        1.00*    PT        1.06     
!   SC        1.06     TS        0.90     WZ        1.05     ZC        1.04     
! 
! 
! Correcting IF 2.
!  A total of 105 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     FD        1.01     HN        1.03     KB        0.96     
!   KK        0.95     KP        0.98     LA        1.01     MK        0.93     
!   NL        0.93     NY        1.00*    OV        0.97     PT        0.98     
!   SC        0.95     TS        0.99     WZ        1.00*    ZC        1.06     
! 
!  A total of 255 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.92     FD        0.98     HN        1.03     KB        1.08     
!   KK        1.00     KP        0.96     LA        0.97     MK        1.02     
!   NL        0.91     NY        0.97     OV        0.95     PT        0.96     
!   SC        1.00     TS        0.95     WZ        1.07     ZC        1.00     
! 
!  A total of 81 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.96     FD        1.01     HN        1.02     KB        0.90     
!   KK        1.00*    KP        1.11     LA        1.01     MK        1.00*    
!   NL        0.98     NY        0.97     OV        1.00*    PT        1.05     
!   SC        1.06     TS        0.94     WZ        1.03     ZC        1.04     
! 
! 
! Correcting IF 3.
!  A total of 105 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.98     FD        1.05     HN        1.02     KB        0.96     
!   KK        1.00     KP        0.98     LA        1.00     MK        0.98     
!   NL        0.96     NY        1.00*    OV        1.03     PT        0.99     
!   SC        0.95     TS        0.95     WZ        1.00*    ZC        1.06     
! 
!  A total of 255 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.96     FD        0.98     HN        1.04     KB        1.08     
!   KK        1.02     KP        0.97     LA        0.98     MK        1.01     
!   NL        0.96     NY        0.98     OV        0.98     PT        0.95     
!   SC        1.02     TS        0.95     WZ        1.06     ZC        1.00     
! 
!  A total of 81 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.01     FD        1.00     HN        1.08     KB        0.96     
!   KK        1.00*    KP        1.08     LA        0.99     MK        1.00*    
!   NL        1.01     NY        1.02     OV        1.00*    PT        1.02     
!   SC        1.06     TS        0.89     WZ        0.98     ZC        1.07     
! 
! 
! Correcting IF 4.
!  A total of 105 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.94     FD        1.05     HN        1.04     KB        0.92     
!   KK        0.99     KP        1.00     LA        0.99     MK        1.00     
!   NL        1.03     NY        1.00*    OV        0.99     PT        0.95     
!   SC        1.00     TS        0.98     WZ        1.00*    ZC        1.04     
! 
!  A total of 255 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.94     FD        0.98     HN        1.07     KB        1.05     
!   KK        1.00     KP        0.97     LA        0.95     MK        1.02     
!   NL        0.95     NY        0.94     OV        0.97     PT        0.93     
!   SC        1.02     TS        0.99     WZ        1.08     ZC        1.01     
! 
!  A total of 81 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.96     FD        1.05     HN        1.10     KB        0.99     
!   KK        1.00*    KP        1.08     LA        1.00     MK        1.00*    
!   NL        1.03     NY        0.98     OV        1.00*    PT        1.01     
!   SC        1.06     TS        0.91     WZ        1.03     ZC        1.02     
! 
! 
! Fit before self-cal, rms=0.174819Jy  sigma=0.001245
! Fit after  self-cal, rms=0.173910Jy  sigma=0.001226
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 milli-arcsec
! Estimated beam: bmin=0.5896 mas, bmaj=0.9525 mas, bpa=-2.493 degrees
! Estimated noise=425.749 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 = -0.00379844 Jy
! Component: 100  -  total flux cleaned = -0.00506718 Jy
! Component: 150  -  total flux cleaned = -0.00601244 Jy
! Component: 200  -  total flux cleaned = -0.00641913 Jy
! Total flux subtracted in 200 components = -0.00641913 Jy
! Clean residual min=-0.003314 max=0.003912 Jy/beam
! Clean residual mean=0.000036 rms=0.000934 Jy/beam
! Combined flux in latest and established models = 0.464255 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 44 components and 0.464255 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.173785Jy  sigma=0.001225
! Fit after  self-cal, rms=0.173749Jy  sigma=0.001225
! Inverting map 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 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=0.173749Jy  sigma=0.001225
! Fit after  self-cal, rms=0.177767Jy  sigma=0.001204
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 milli-arcsec
! Estimated beam: bmin=0.5893 mas, bmaj=0.9579 mas, bpa=-2.033 degrees
! Estimated noise=425.158 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000508716 Jy
! Component: 100  -  total flux cleaned = -0.00104631 Jy
! Component: 150  -  total flux cleaned = -0.00146014 Jy
! Component: 200  -  total flux cleaned = -0.00165382 Jy
! Total flux subtracted in 200 components = -0.00165382 Jy
! Clean residual min=-0.002183 max=0.002113 Jy/beam
! Clean residual mean=-0.000002 rms=0.000536 Jy/beam
! Combined flux in latest and established models = 0.462602 Jy
selfcal
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 54 components and 0.462601 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.177702Jy  sigma=0.001203
! Fit after  self-cal, rms=0.178207Jy  sigma=0.001203
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 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 = -0.000184492 Jy
! Component: 100  -  total flux cleaned = -0.000582752 Jy
! Component: 150  -  total flux cleaned = -0.00066633 Jy
! Component: 200  -  total flux cleaned = -0.000742848 Jy
! Total flux subtracted in 200 components = -0.000742848 Jy
! Clean residual min=-0.002140 max=0.001978 Jy/beam
! Clean residual mean=0.000002 rms=0.000522 Jy/beam
! Combined flux in latest and established models = 0.461859 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 58 components and 0.461859 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.178182Jy  sigma=0.001203
! Fit after  self-cal, rms=0.178176Jy  sigma=0.001203
! Inverting map 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 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=0.178176Jy  sigma=0.001203
! Fit after  self-cal, rms=0.177933Jy  sigma=0.001202
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 milli-arcsec
! Estimated beam: bmin=0.5896 mas, bmaj=0.9578 mas, bpa=-2.063 degrees
! Estimated noise=424.859 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000707419 Jy
! Component: 100  -  total flux cleaned = -0.000884566 Jy
! Component: 150  -  total flux cleaned = -0.00102397 Jy
! Component: 200  -  total flux cleaned = -0.00108692 Jy
! Total flux subtracted in 200 components = -0.00108692 Jy
! Clean residual min=-0.002176 max=0.001915 Jy/beam
! Clean residual mean=-0.000011 rms=0.000506 Jy/beam
! Combined flux in latest and established models = 0.460772 Jy
selfcal
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 62 components and 0.460772 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.177915Jy  sigma=0.001202
! Fit after  self-cal, rms=0.177830Jy  sigma=0.001202
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 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 = -0.000122919 Jy
! Component: 100  -  total flux cleaned = -0.000187202 Jy
! Component: 150  -  total flux cleaned = -0.000216248 Jy
! Component: 200  -  total flux cleaned = -0.000296654 Jy
! Total flux subtracted in 200 components = -0.000296654 Jy
! Clean residual min=-0.002174 max=0.001876 Jy/beam
! Clean residual mean=-0.000010 rms=0.000502 Jy/beam
! Combined flux in latest and established models = 0.460475 Jy
! Performing phase self-cal
! Adding 24 model components to the UV plane model.
! The established model now contains 67 components and 0.460475 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.177819Jy  sigma=0.001202
! Fit after  self-cal, rms=0.177816Jy  sigma=0.001202
! Inverting map 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 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=0.177816Jy  sigma=0.001202
! Fit after  self-cal, rms=0.177844Jy  sigma=0.001202
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 milli-arcsec
! Estimated beam: bmin=2.423 mas, bmaj=2.664 mas, bpa=48.61 degrees
! Estimated noise=648.227 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.001154 Jy
! Component: 100  -  total flux cleaned = -0.00123691 Jy
! Component: 150  -  total flux cleaned = -0.00123715 Jy
! Component: 200  -  total flux cleaned = -0.00125572 Jy
! Total flux subtracted in 200 components = -0.00125572 Jy
! Clean residual min=-0.002080 max=0.002325 Jy/beam
! Clean residual mean=-0.000017 rms=0.000679 Jy/beam
! Combined flux in latest and established models = 0.459219 Jy
selfcal
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 72 components and 0.459219 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.177844Jy  sigma=0.001202
! Fit after  self-cal, rms=0.177839Jy  sigma=0.001202
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 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 = -0.000277717 Jy
! Component: 100  -  total flux cleaned = -0.00029322 Jy
! Component: 150  -  total flux cleaned = -0.000323765 Jy
! Component: 200  -  total flux cleaned = -0.00035288 Jy
! Total flux subtracted in 200 components = -0.00035288 Jy
! Clean residual min=-0.002046 max=0.002357 Jy/beam
! Clean residual mean=-0.000010 rms=0.000675 Jy/beam
! Combined flux in latest and established models = 0.458866 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 73 components and 0.458866 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.177841Jy  sigma=0.001202
! Fit after  self-cal, rms=0.177845Jy  sigma=0.001202
! Inverting map 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 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 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 milli-arcsec
! Estimated beam: bmin=0.5897 mas, bmaj=0.958 mas, bpa=-2.071 degrees
! Estimated noise=424.689 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5897 x 0.958 at -2.071 degrees (North through East)
! Clean map  min=-0.0018942  max=0.40758 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 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 milli-arcsec
! Estimated beam: bmin=0.4755 mas, bmaj=0.8169 mas, bpa=-5.636 degrees
! Estimated noise=868.986 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.311351 Jy
! Component: 100  -  total flux cleaned = 0.380878 Jy
! Component: 150  -  total flux cleaned = 0.409136 Jy
! Component: 200  -  total flux cleaned = 0.425571 Jy
! Total flux subtracted in 200 components = 0.425571 Jy
! Clean residual min=-0.004878 max=0.008405 Jy/beam
! Clean residual mean=0.000041 rms=0.001201 Jy/beam
! Combined flux in latest and established models = 0.425571 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 9 model components to the UV plane model.
! The established model now contains 9 components and 0.425571 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 milli-arcsec
! Estimated beam: bmin=0.5897 mas, bmaj=0.958 mas, bpa=-2.071 degrees
! Estimated noise=424.689 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 = 0.0146167 Jy
! Component: 100  -  total flux cleaned = 0.0224081 Jy
! Component: 150  -  total flux cleaned = 0.0268389 Jy
! Component: 200  -  total flux cleaned = 0.0296187 Jy
! Total flux subtracted in 200 components = 0.0296187 Jy
! Clean residual min=-0.002346 max=0.002078 Jy/beam
! Clean residual mean=0.000075 rms=0.000527 Jy/beam
! Combined flux in latest and established models = 0.45519 Jy
! Adding 29 model components to the UV plane model.
! The established model now contains 31 components and 0.45519 Jy
! Inverting map 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 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 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 milli-arcsec
! Estimated beam: bmin=2.423 mas, bmaj=2.664 mas, bpa=48.61 degrees
! Estimated noise=648.227 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0027844 Jy
! Component: 100  -  total flux cleaned = 0.00300741 Jy
! Component: 150  -  total flux cleaned = 0.00317907 Jy
! Component: 200  -  total flux cleaned = 0.00331523 Jy
! Total flux subtracted in 200 components = 0.00331523 Jy
! Clean residual min=-0.002093 max=0.002335 Jy/beam
! Clean residual mean=0.000005 rms=0.000675 Jy/beam
! Combined flux in latest and established models = 0.458505 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 = 8.90287e-05 Jy
! Component: 100  -  total flux cleaned = 0.000126791 Jy
! Component: 150  -  total flux cleaned = 0.000127023 Jy
! Component: 200  -  total flux cleaned = 0.000126424 Jy
! Total flux subtracted in 200 components = 0.000126424 Jy
! Clean residual min=-0.002069 max=0.002336 Jy/beam
! Clean residual mean=-0.000004 rms=0.000668 Jy/beam
! Combined flux in latest and established models = 0.458631 Jy
! Adding 21 model components to the UV plane model.
! The established model now contains 44 components and 0.458631 Jy
! Inverting map 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 milli-arcsec
! Estimated beam: bmin=0.5897 mas, bmaj=0.958 mas, bpa=-2.071 degrees
! Estimated noise=424.689 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000427162 Jy
! Component: 100  -  total flux cleaned = -0.000173304 Jy
! Component: 150  -  total flux cleaned = -6.37179e-05 Jy
! Component: 200  -  total flux cleaned = 3.31781e-05 Jy
! Total flux subtracted in 200 components = 3.31781e-05 Jy
! Clean residual min=-0.002317 max=0.001869 Jy/beam
! Clean residual mean=0.000001 rms=0.000501 Jy/beam
! Combined flux in latest and established models = 0.458664 Jy
selfcal
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 53 components and 0.458664 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.177888Jy  sigma=0.001202
! Fit after  self-cal, rms=0.177806Jy  sigma=0.001202
wmodel J1521+4336_X_2009_04_21_pus_map.mod
! Writing 53 model components to file: J1521+4336_X_2009_04_21_pus_map.mod
wobs J1521+4336_X_2009_04_21_pus_uvs.fits
! Writing UV FITS file: J1521+4336_X_2009_04_21_pus_uvs.fits
wwins J1521+4336_X_2009_04_21_pus_map.win
! wwins: Wrote 3 windows to J1521+4336_X_2009_04_21_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 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000599375 Jy
! Component: 100  -  total flux cleaned = -0.000633953 Jy
! Component: 150  -  total flux cleaned = -0.000601277 Jy
! Component: 200  -  total flux cleaned = -0.000537745 Jy
! Component: 250  -  total flux cleaned = -0.000351145 Jy
! Component: 300  -  total flux cleaned = -0.000198651 Jy
! Component: 350  -  total flux cleaned = -7.82338e-05 Jy
! Component: 400  -  total flux cleaned = 0.000128814 Jy
! Component: 450  -  total flux cleaned = 0.000245452 Jy
! Component: 500  -  total flux cleaned = 0.000388896 Jy
! Component: 550  -  total flux cleaned = 0.000502161 Jy
! Component: 600  -  total flux cleaned = 0.000613894 Jy
! Component: 650  -  total flux cleaned = 0.000724167 Jy
! Component: 700  -  total flux cleaned = 0.000751587 Jy
! Component: 750  -  total flux cleaned = 0.000832946 Jy
! Component: 800  -  total flux cleaned = 0.000966712 Jy
! Component: 850  -  total flux cleaned = 0.00101941 Jy
! Component: 900  -  total flux cleaned = 0.00104567 Jy
! Component: 950  -  total flux cleaned = 0.00112356 Jy
! Component: 1000  -  total flux cleaned = 0.00112358 Jy
! Component: 1050  -  total flux cleaned = 0.0011493 Jy
! Component: 1100  -  total flux cleaned = 0.00120006 Jy
! Component: 1150  -  total flux cleaned = 0.00125026 Jy
! Component: 1200  -  total flux cleaned = 0.00125027 Jy
! Component: 1250  -  total flux cleaned = 0.00127499 Jy
! Component: 1300  -  total flux cleaned = 0.00129942 Jy
! Component: 1350  -  total flux cleaned = 0.00129939 Jy
! Component: 1400  -  total flux cleaned = 0.0013719 Jy
! Component: 1450  -  total flux cleaned = 0.00137196 Jy
! Component: 1500  -  total flux cleaned = 0.00139583 Jy
! Component: 1550  -  total flux cleaned = 0.00146677 Jy
! Component: 1600  -  total flux cleaned = 0.0014668 Jy
! Component: 1650  -  total flux cleaned = 0.00149016 Jy
! Component: 1700  -  total flux cleaned = 0.00153652 Jy
! Component: 1750  -  total flux cleaned = 0.00153649 Jy
! Component: 1800  -  total flux cleaned = 0.00155943 Jy
! Component: 1850  -  total flux cleaned = 0.0015594 Jy
! Component: 1900  -  total flux cleaned = 0.00155945 Jy
! Component: 1950  -  total flux cleaned = 0.00158182 Jy
! Component: 2000  -  total flux cleaned = 0.00160424 Jy
! Total flux subtracted in 2048 components = 0.00155978 Jy
! Clean residual min=-0.001420 max=0.001113 Jy/beam
! Clean residual mean=-0.000002 rms=0.000395 Jy/beam
! Combined flux in latest and established models = 0.460224 Jy
keep
! Adding 178 model components to the UV plane model.
! The established model now contains 231 components and 0.460224 Jy
![Exited script file: muppet]
wmap "J1521+4336_X_2009_04_21_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5897 x 0.958 at -2.071 degrees (North through East)
! Clean map  min=-0.0015284  max=0.40744 Jy/beam
! Writing clean map to FITS file: J1521+4336_X_2009_04_21_pus_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.407439 
invert
! Inverting map 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.16 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000396022 
device "J1521+4336_X_2009_04_21_pus\_map.eps/VPS"
! Attempting to open device: 'J1521+4336_X_2009_04_21_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.291593 0.291593 0.583186 1.16637 2.33274 4.66549 9.33097 18.6619 37.3239 74.6478
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0011 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.407 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5897 x 0.958 at -2.071 degrees (North through East)
! Clean map  min=-0.0015284  max=0.40744 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1521+4336_X_2009_04_21_pus\_map.gif/vgif"
! Attempting to open device: 'J1521+4336_X_2009_04_21_pus_map.gif/vgif'
mapplot cln