! Started logfile: J0102+5824_X_2001_03_12_pus_uvs.log on Wed Jan  2 19:48:04 2013
obs J0102+5824_X_2001_03_12_pus_uva.fits
! Reading UV FITS file: J0102+5824_X_2001_03_12_pus_uva.fits
! AN table 1: 315 integrations on 136 of 136 possible baselines.
! AN table 2: 113 integrations on 136 of 136 possible baselines.
! AN table 3: 215 integrations on 136 of 136 possible baselines.
! Apparent sampling: 0.166979 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J0102+5824
! 
! 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 1749 lines of history.
! 
! Reading 58408 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 J0102+5824_X_2001_03_12_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 3378 telescope corrections were flagged in sub-array 1.
!  A total of 1464 telescope corrections were flagged in sub-array 2.
!  A total of 2542 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 3378 telescope corrections were flagged in sub-array 1.
!  A total of 1464 telescope corrections were flagged in sub-array 2.
!  A total of 2542 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 3378 telescope corrections were flagged in sub-array 1.
!  A total of 1468 telescope corrections were flagged in sub-array 2.
!  A total of 2544 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 3378 telescope corrections were flagged in sub-array 1.
!  A total of 1468 telescope corrections were flagged in sub-array 2.
!  A total of 2565 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=0.854712Jy  sigma=0.006852
! Fit after  self-cal, rms=0.548695Jy  sigma=0.004466
! 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 5.32% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Estimated beam: bmin=0.544 mas, bmaj=0.6132 mas, bpa=14.33 degrees
! Estimated noise=675.893 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 = 1.0799 Jy
! Component: 100  -  total flux cleaned = 1.32259 Jy
! Total flux subtracted in 100 components = 1.32259 Jy
! Clean residual min=-0.028277 max=0.088575 Jy/beam
! Clean residual mean=-0.000064 rms=0.006749 Jy/beam
! Combined flux in latest and established models = 1.32259 Jy
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 6 components and 1.32259 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.374718Jy  sigma=0.002758
! Fit after  self-cal, rms=0.374718Jy  sigma=0.002758
! Inverting map 
! Your choice of large map pixels excluded 5.32% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.100493 Jy
! Component: 100  -  total flux cleaned = 0.166364 Jy
! Total flux subtracted in 100 components = 0.166364 Jy
! Clean residual min=-0.025021 max=0.036447 Jy/beam
! Clean residual mean=-0.000050 rms=0.005840 Jy/beam
! Combined flux in latest and established models = 1.48896 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 14 components and 1.48896 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.345355Jy  sigma=0.002285
! Fit after  self-cal, rms=0.345330Jy  sigma=0.002284
! Inverting map 
! Your choice of large map pixels excluded 5.32% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Added new window around map position (0.2, -0.6).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.04642 Jy
! Component: 100  -  total flux cleaned = 0.0793328 Jy
! Total flux subtracted in 100 components = 0.0793328 Jy
! Clean residual min=-0.024996 max=0.032278 Jy/beam
! Clean residual mean=-0.000043 rms=0.005580 Jy/beam
! Combined flux in latest and established models = 1.56829 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 16 components and 1.56829 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.342038Jy  sigma=0.002165
! Fit after  self-cal, rms=0.341982Jy  sigma=0.002164
! Inverting map 
! Your choice of large map pixels excluded 5.32% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 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 5.32% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Estimated beam: bmin=0.6657 mas, bmaj=0.7475 mas, bpa=7.302 degrees
! Estimated noise=384.249 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 (-0.8, -1.6).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0435288 Jy
! Component: 100  -  total flux cleaned = 0.0677267 Jy
! Component: 150  -  total flux cleaned = 0.0771369 Jy
! Component: 200  -  total flux cleaned = 0.0822783 Jy
! Total flux subtracted in 200 components = 0.0822783 Jy
! Clean residual min=-0.022635 max=0.030345 Jy/beam
! Clean residual mean=-0.000208 rms=0.004957 Jy/beam
! Combined flux in latest and established models = 1.65057 Jy
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 34 components and 1.65057 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.336779Jy  sigma=0.002090
! Fit after  self-cal, rms=0.336197Jy  sigma=0.002083
! Inverting map 
! Your choice of large map pixels excluded 5.32% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 51 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     FD        1.02     HH        1.00*    HN        1.16     
!   KK        0.97     KP        1.08     LA        1.01     MA        0.99     
!   MC        1.00*    MK        0.94     NL        1.02     ON        1.00*    
!   OV        1.00     PT        0.98     SC        1.07     TS        0.94     
!   WZ        1.07     
! 
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.95     FD        0.99     HH        1.00*    HN        0.95     
!   KK        0.93     KP        0.99     LA        0.97     MA        0.95     
!   MC        1.00*    MK        0.95     NL        0.96     ON        1.00*    
!   OV        0.94     PT        0.94     SC        1.00*    TS        1.10     
!   WZ        0.97     
! 
!  A total of 261 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.96     FD        0.99     HH        1.00*    HN        0.96     
!   KK        0.97     KP        0.97     LA        0.95     MA        0.91     
!   MC        1.00*    MK        0.93     NL        0.99     ON        1.00*    
!   OV        0.96     PT        0.96     SC        1.00     TS        1.28     
!   WZ        1.03     
! 
! 
! Correcting IF 2.
!  A total of 51 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        1.02     HH        1.00*    HN        1.15     
!   KK        0.96     KP        1.02     LA        1.01     MA        0.96     
!   MC        1.00*    MK        0.93     NL        0.98     ON        1.00*    
!   OV        1.00     PT        1.01     SC        1.06     TS        0.95     
!   WZ        1.07     
! 
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.95     FD        0.99     HH        1.00*    HN        0.95     
!   KK        0.92     KP        0.93     LA        0.95     MA        0.93     
!   MC        1.00*    MK        0.94     NL        0.92     ON        1.00*    
!   OV        0.93     PT        0.98     SC        1.00*    TS        1.10     
!   WZ        0.95     
! 
!  A total of 261 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.97     FD        0.98     HH        1.00*    HN        0.95     
!   KK        0.96     KP        0.92     LA        0.95     MA        0.90     
!   MC        1.00*    MK        0.93     NL        0.94     ON        1.00*    
!   OV        0.95     PT        0.99     SC        0.97     TS        1.29     
!   WZ        1.03     
! 
! 
! Correcting IF 3.
!  A total of 51 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.02     FD        0.99     HH        1.00*    HN        1.17     
!   KK        1.02     KP        1.00     LA        1.02     MA        1.00     
!   MC        1.00*    MK        0.94     NL        1.00     ON        1.00*    
!   OV        1.02     PT        1.04     SC        1.08     TS        0.93     
!   WZ        1.09     
! 
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.98     FD        0.96     HH        1.00*    HN        0.95     
!   KK        0.98     KP        0.91     LA        0.97     MA        0.99     
!   MC        1.00*    MK        0.94     NL        0.95     ON        1.00*    
!   OV        0.96     PT        0.99     SC        1.00*    TS        1.09     
!   WZ        0.98     
! 
!  A total of 261 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00     FD        0.95     HH        1.00*    HN        0.95     
!   KK        1.01     KP        0.89     LA        0.95     MA        0.93     
!   MC        1.00*    MK        0.93     NL        0.96     ON        1.00*    
!   OV        0.97     PT        1.01     SC        0.99     TS        1.26     
!   WZ        1.03     
! 
! 
! Correcting IF 4.
!  A total of 51 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        0.98     HH        1.00*    HN        1.18     
!   KK        0.97     KP        1.00     LA        1.00     MA        1.04     
!   MC        1.00*    MK        0.97     NL        1.02     ON        1.00*    
!   OV        1.00     PT        1.03     SC        1.14     TS        0.92     
!   WZ        1.09     
! 
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.94     FD        0.95     HH        1.00*    HN        0.96     
!   KK        0.93     KP        0.92     LA        0.94     MA        1.03     
!   MC        1.00*    MK        0.97     NL        0.97     ON        1.00*    
!   OV        0.94     PT        0.98     SC        1.00*    TS        1.10     
!   WZ        1.00     
! 
!  A total of 261 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.96     FD        0.93     HH        1.00*    HN        0.95     
!   KK        0.96     KP        0.90     LA        0.92     MA        0.96     
!   MC        1.00*    MK        0.95     NL        0.96     ON        1.00*    
!   OV        0.95     PT        1.00     SC        1.04     TS        1.26     
!   WZ        1.00     
! 
! 
! Fit before self-cal, rms=0.336197Jy  sigma=0.002083
! Fit after  self-cal, rms=0.310255Jy  sigma=0.001749
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Estimated beam: bmin=0.6691 mas, bmaj=0.7503 mas, bpa=3.849 degrees
! Estimated noise=390.049 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 = -0.0171128 Jy
! Component: 100  -  total flux cleaned = -0.020739 Jy
! Component: 150  -  total flux cleaned = -0.022257 Jy
! Component: 200  -  total flux cleaned = -0.02271 Jy
! Total flux subtracted in 200 components = -0.02271 Jy
! Clean residual min=-0.015599 max=0.016674 Jy/beam
! Clean residual mean=-0.000059 rms=0.003423 Jy/beam
! Combined flux in latest and established models = 1.62786 Jy
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 42 components and 1.62786 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.307520Jy  sigma=0.001730
! Fit after  self-cal, rms=0.307583Jy  sigma=0.001729
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 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=0.307583Jy  sigma=0.001729
! Fit after  self-cal, rms=0.266819Jy  sigma=0.001261
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Estimated beam: bmin=0.6715 mas, bmaj=0.7502 mas, bpa=6.799 degrees
! Estimated noise=390.075 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.0109997 Jy
! Component: 100  -  total flux cleaned = -0.0118727 Jy
! Component: 150  -  total flux cleaned = -0.0128253 Jy
! Component: 200  -  total flux cleaned = -0.0134387 Jy
! Total flux subtracted in 200 components = -0.0134387 Jy
! Clean residual min=-0.004275 max=0.005830 Jy/beam
! Clean residual mean=0.000024 rms=0.000853 Jy/beam
! Combined flux in latest and established models = 1.61442 Jy
selfcal
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 46 components and 1.61442 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.266107Jy  sigma=0.001253
! Fit after  self-cal, rms=0.266307Jy  sigma=0.001253
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 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)
! Added new window around map position (-0.8, -0.2).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000203732 Jy
! Component: 100  -  total flux cleaned = -0.000169506 Jy
! Component: 150  -  total flux cleaned = -0.000340362 Jy
! Component: 200  -  total flux cleaned = -0.000346096 Jy
! Total flux subtracted in 200 components = -0.000346096 Jy
! Clean residual min=-0.003503 max=0.004935 Jy/beam
! Clean residual mean=0.000025 rms=0.000814 Jy/beam
! Combined flux in latest and established models = 1.61407 Jy
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 50 components and 1.61407 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.266068Jy  sigma=0.001250
! Fit after  self-cal, rms=0.266058Jy  sigma=0.001250
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Added new window around map position (-3.4, -0.6).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00351957 Jy
! Component: 100  -  total flux cleaned = 0.00382758 Jy
! Component: 150  -  total flux cleaned = 0.00409791 Jy
! Component: 200  -  total flux cleaned = 0.00422147 Jy
! Total flux subtracted in 200 components = 0.00422147 Jy
! Clean residual min=-0.003160 max=0.003608 Jy/beam
! Clean residual mean=0.000024 rms=0.000764 Jy/beam
! Combined flux in latest and established models = 1.61829 Jy
! Performing phase self-cal
! Adding 28 model components to the UV plane model.
! The established model now contains 62 components and 1.61829 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.265900Jy  sigma=0.001248
! Fit after  self-cal, rms=0.265893Jy  sigma=0.001248
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Added new window around map position (-2.2, -1.8).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00179723 Jy
! Component: 100  -  total flux cleaned = 0.00192034 Jy
! Component: 150  -  total flux cleaned = 0.00213876 Jy
! Component: 200  -  total flux cleaned = 0.00224156 Jy
! Total flux subtracted in 200 components = 0.00224156 Jy
! Clean residual min=-0.003089 max=0.003292 Jy/beam
! Clean residual mean=0.000023 rms=0.000740 Jy/beam
! Combined flux in latest and established models = 1.62054 Jy
! Performing phase self-cal
! Adding 30 model components to the UV plane model.
! The established model now contains 72 components and 1.62054 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.265789Jy  sigma=0.001246
! Fit after  self-cal, rms=0.265787Jy  sigma=0.001246
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Added new window around map position (-3.8, 2.4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0017474 Jy
! Component: 100  -  total flux cleaned = 0.00184463 Jy
! Component: 150  -  total flux cleaned = 0.00212388 Jy
! Component: 200  -  total flux cleaned = 0.00229943 Jy
! Total flux subtracted in 200 components = 0.00229943 Jy
! Clean residual min=-0.003034 max=0.003266 Jy/beam
! Clean residual mean=0.000023 rms=0.000726 Jy/beam
! Combined flux in latest and established models = 1.62284 Jy
! Performing phase self-cal
! Adding 36 model components to the UV plane model.
! The established model now contains 80 components and 1.62284 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.265713Jy  sigma=0.001245
! Fit after  self-cal, rms=0.265709Jy  sigma=0.001245
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Added new window around map position (-12.8, -14.4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00229855 Jy
! Component: 100  -  total flux cleaned = 0.00265836 Jy
! Component: 150  -  total flux cleaned = 0.00307332 Jy
! Component: 200  -  total flux cleaned = 0.00330801 Jy
! Total flux subtracted in 200 components = 0.00330801 Jy
! Clean residual min=-0.002914 max=0.002928 Jy/beam
! Clean residual mean=0.000016 rms=0.000712 Jy/beam
! Combined flux in latest and established models = 1.62614 Jy
! Performing phase self-cal
! Adding 40 model components to the UV plane model.
! The established model now contains 88 components and 1.62614 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.265643Jy  sigma=0.001245
! Fit after  self-cal, rms=0.265639Jy  sigma=0.001245
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 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=0.265639Jy  sigma=0.001245
! Fit after  self-cal, rms=0.264748Jy  sigma=0.001238
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Estimated beam: bmin=0.6731 mas, bmaj=0.751 mas, bpa=6.802 degrees
! Estimated noise=390.198 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00546665 Jy
! Component: 100  -  total flux cleaned = -0.00658583 Jy
! Component: 150  -  total flux cleaned = -0.00724278 Jy
! Component: 200  -  total flux cleaned = -0.0073541 Jy
! Total flux subtracted in 200 components = -0.0073541 Jy
! Clean residual min=-0.002320 max=0.002304 Jy/beam
! Clean residual mean=0.000009 rms=0.000611 Jy/beam
! Combined flux in latest and established models = 1.61879 Jy
selfcal
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 90 components and 1.61879 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.264507Jy  sigma=0.001236
! Fit after  self-cal, rms=0.264493Jy  sigma=0.001236
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 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 = -0.000195708 Jy
! Component: 100  -  total flux cleaned = -0.0001095 Jy
! Component: 150  -  total flux cleaned = -2.7979e-05 Jy
! Component: 200  -  total flux cleaned = 0.000206289 Jy
! Total flux subtracted in 200 components = 0.000206289 Jy
! Clean residual min=-0.002301 max=0.002237 Jy/beam
! Clean residual mean=0.000009 rms=0.000599 Jy/beam
! Combined flux in latest and established models = 1.619 Jy
! Performing phase self-cal
! Adding 28 model components to the UV plane model.
! The established model now contains 94 components and 1.619 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.264433Jy  sigma=0.001235
! Fit after  self-cal, rms=0.264431Jy  sigma=0.001235
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 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=0.264431Jy  sigma=0.001235
! Fit after  self-cal, rms=0.264660Jy  sigma=0.001234
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Estimated beam: bmin=2.554 mas, bmaj=2.66 mas, bpa=-62.22 degrees
! Estimated noise=571.235 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00156041 Jy
! Component: 100  -  total flux cleaned = -0.00164052 Jy
! Component: 150  -  total flux cleaned = -0.00136503 Jy
! Component: 200  -  total flux cleaned = -0.00118053 Jy
! Total flux subtracted in 200 components = -0.00118053 Jy
! Clean residual min=-0.002736 max=0.003256 Jy/beam
! Clean residual mean=0.000016 rms=0.000897 Jy/beam
! Combined flux in latest and established models = 1.61782 Jy
selfcal
! Performing phase self-cal
! Adding 20 model components to the UV plane model.
! The established model now contains 107 components and 1.61782 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.264607Jy  sigma=0.001234
! Fit after  self-cal, rms=0.264602Jy  sigma=0.001234
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 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 = 0.000352076 Jy
! Component: 100  -  total flux cleaned = 0.000516154 Jy
! Component: 150  -  total flux cleaned = 0.000589752 Jy
! Component: 200  -  total flux cleaned = 0.000653834 Jy
! Total flux subtracted in 200 components = 0.000653834 Jy
! Clean residual min=-0.002702 max=0.003187 Jy/beam
! Clean residual mean=0.000015 rms=0.000887 Jy/beam
! Combined flux in latest and established models = 1.61847 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 112 components and 1.61847 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.264594Jy  sigma=0.001234
! Fit after  self-cal, rms=0.264595Jy  sigma=0.001234
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 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 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Estimated beam: bmin=0.6742 mas, bmaj=0.7517 mas, bpa=6.766 degrees
! Estimated noise=390.213 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6742 x 0.7517 at 6.766 degrees (North through East)
! Clean map  min=-0.0028507  max=1.4178 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
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.264595Jy  sigma=0.001234
! Fit after  self-cal, rms=0.249844Jy  sigma=0.001131
! Inverting map and beam 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Estimated beam: bmin=0.6746 mas, bmaj=0.752 mas, bpa=6.799 degrees
! Estimated noise=389.744 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00330018 Jy
! Component: 100  -  total flux cleaned = -0.00426349 Jy
! Component: 150  -  total flux cleaned = -0.00473642 Jy
! Component: 200  -  total flux cleaned = -0.00473554 Jy
! Total flux subtracted in 200 components = -0.00473554 Jy
! Clean residual min=-0.002097 max=0.002221 Jy/beam
! Clean residual mean=0.000004 rms=0.000522 Jy/beam
! Combined flux in latest and established models = 1.61373 Jy
! Performing phase self-cal
! Adding 20 model components to the UV plane model.
! The established model now contains 114 components and 1.61373 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.249732Jy  sigma=0.001130
! Fit after  self-cal, rms=0.249729Jy  sigma=0.001130
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Added new window around map position (-8, -0.8).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0013554 Jy
! Component: 100  -  total flux cleaned = 0.0015528 Jy
! Component: 150  -  total flux cleaned = 0.00167286 Jy
! Component: 200  -  total flux cleaned = 0.00172823 Jy
! Total flux subtracted in 200 components = 0.00172823 Jy
! Clean residual min=-0.002164 max=0.001921 Jy/beam
! Clean residual mean=0.000004 rms=0.000509 Jy/beam
! Combined flux in latest and established models = 1.61546 Jy
! Performing phase self-cal
! Adding 28 model components to the UV plane model.
! The established model now contains 122 components and 1.61546 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.249697Jy  sigma=0.001129
! Fit after  self-cal, rms=0.249694Jy  sigma=0.001129
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.249694Jy  sigma=0.001129
! Fit after  self-cal, rms=0.249765Jy  sigma=0.001129
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 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Estimated beam: bmin=0.5546 mas, bmaj=0.6167 mas, bpa=13.95 degrees
! Estimated noise=682.959 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 1.08776 Jy
! Component: 100  -  total flux cleaned = 1.32532 Jy
! Component: 150  -  total flux cleaned = 1.40248 Jy
! Component: 200  -  total flux cleaned = 1.44863 Jy
! Total flux subtracted in 200 components = 1.44863 Jy
! Clean residual min=-0.005476 max=0.025125 Jy/beam
! Clean residual mean=-0.000016 rms=0.001583 Jy/beam
! Combined flux in latest and established models = 1.44863 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 17 model components to the UV plane model.
! The established model now contains 17 components and 1.44863 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Estimated beam: bmin=0.6754 mas, bmaj=0.7524 mas, bpa=6.821 degrees
! Estimated noise=389.629 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 = 0.0556462 Jy
! Component: 100  -  total flux cleaned = 0.0872836 Jy
! Component: 150  -  total flux cleaned = 0.107089 Jy
! Component: 200  -  total flux cleaned = 0.120186 Jy
! Total flux subtracted in 200 components = 0.120186 Jy
! Clean residual min=-0.002658 max=0.007420 Jy/beam
! Clean residual mean=0.000026 rms=0.000883 Jy/beam
! Combined flux in latest and established models = 1.56881 Jy
! Adding 37 model components to the UV plane model.
! The established model now contains 41 components and 1.56881 Jy
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Added new window around map position (-1.8, -0.6).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00918309 Jy
! Component: 100  -  total flux cleaned = 0.0158746 Jy
! Component: 150  -  total flux cleaned = 0.0209863 Jy
! Component: 200  -  total flux cleaned = 0.0251159 Jy
! Total flux subtracted in 200 components = 0.0251159 Jy
! Clean residual min=-0.002177 max=0.002769 Jy/beam
! Clean residual mean=0.000014 rms=0.000591 Jy/beam
! Combined flux in latest and established models = 1.59393 Jy
! Adding 47 model components to the UV plane model.
! The established model now contains 74 components and 1.59393 Jy
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Added new window around map position (0.2, -1.4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0034447 Jy
! Component: 100  -  total flux cleaned = 0.00601274 Jy
! Component: 150  -  total flux cleaned = 0.00775074 Jy
! Component: 200  -  total flux cleaned = 0.00938753 Jy
! Total flux subtracted in 200 components = 0.00938753 Jy
! Clean residual min=-0.002052 max=0.002033 Jy/beam
! Clean residual mean=0.000009 rms=0.000530 Jy/beam
! Combined flux in latest and established models = 1.60332 Jy
! Adding 43 model components to the UV plane model.
! The established model now contains 87 components and 1.60332 Jy
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 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 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Estimated beam: bmin=2.555 mas, bmaj=2.661 mas, bpa=-61.93 degrees
! Estimated noise=568.845 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00387418 Jy
! Component: 100  -  total flux cleaned = 0.00617148 Jy
! Component: 150  -  total flux cleaned = 0.00781869 Jy
! Component: 200  -  total flux cleaned = 0.00877169 Jy
! Total flux subtracted in 200 components = 0.00877169 Jy
! Clean residual min=-0.002653 max=0.002303 Jy/beam
! Clean residual mean=0.000012 rms=0.000775 Jy/beam
! Combined flux in latest and established models = 1.61209 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 = 0.000530544 Jy
! Component: 100  -  total flux cleaned = 0.000947789 Jy
! Component: 150  -  total flux cleaned = 0.0011627 Jy
! Component: 200  -  total flux cleaned = 0.00135768 Jy
! Total flux subtracted in 200 components = 0.00135768 Jy
! Clean residual min=-0.002658 max=0.002281 Jy/beam
! Clean residual mean=0.000009 rms=0.000757 Jy/beam
! Combined flux in latest and established models = 1.61345 Jy
! Adding 49 model components to the UV plane model.
! The established model now contains 126 components and 1.61345 Jy
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! Estimated beam: bmin=0.6754 mas, bmaj=0.7524 mas, bpa=6.821 degrees
! Estimated noise=389.629 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000228422 Jy
! Component: 100  -  total flux cleaned = -0.000172675 Jy
! Component: 150  -  total flux cleaned = -7.32241e-05 Jy
! Component: 200  -  total flux cleaned = -2.85166e-05 Jy
! Total flux subtracted in 200 components = -2.85166e-05 Jy
! Clean residual min=-0.002029 max=0.001861 Jy/beam
! Clean residual mean=0.000003 rms=0.000491 Jy/beam
! Combined flux in latest and established models = 1.61342 Jy
selfcal
! Performing phase self-cal
! Adding 25 model components to the UV plane model.
! The established model now contains 141 components and 1.61342 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.249617Jy  sigma=0.001129
! Fit after  self-cal, rms=0.249595Jy  sigma=0.001129
wmodel J0102+5824_X_2001_03_12_pus_map.mod
! Writing 141 model components to file: J0102+5824_X_2001_03_12_pus_map.mod
wobs J0102+5824_X_2001_03_12_pus_uvs.fits
! Writing UV FITS file: J0102+5824_X_2001_03_12_pus_uvs.fits
wwins J0102+5824_X_2001_03_12_pus_map.win
! wwins: Wrote 11 windows to J0102+5824_X_2001_03_12_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 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000758943 Jy
! Component: 100  -  total flux cleaned = -0.00106295 Jy
! Component: 150  -  total flux cleaned = -0.00119355 Jy
! Component: 200  -  total flux cleaned = -0.00128947 Jy
! Component: 250  -  total flux cleaned = -0.00138403 Jy
! Component: 300  -  total flux cleaned = -0.00150779 Jy
! Component: 350  -  total flux cleaned = -0.00156874 Jy
! Component: 400  -  total flux cleaned = -0.00168952 Jy
! Component: 450  -  total flux cleaned = -0.00177924 Jy
! Component: 500  -  total flux cleaned = -0.00189708 Jy
! Component: 550  -  total flux cleaned = -0.0019842 Jy
! Component: 600  -  total flux cleaned = -0.00201286 Jy
! Component: 650  -  total flux cleaned = -0.00207019 Jy
! Component: 700  -  total flux cleaned = -0.00215536 Jy
! Component: 750  -  total flux cleaned = -0.00226786 Jy
! Component: 800  -  total flux cleaned = -0.00226769 Jy
! Component: 850  -  total flux cleaned = -0.00229571 Jy
! Component: 900  -  total flux cleaned = -0.00235073 Jy
! Component: 950  -  total flux cleaned = -0.00224127 Jy
! Component: 1000  -  total flux cleaned = -0.00218703 Jy
! Component: 1050  -  total flux cleaned = -0.00229537 Jy
! Component: 1100  -  total flux cleaned = -0.00221459 Jy
! Component: 1150  -  total flux cleaned = -0.00216126 Jy
! Component: 1200  -  total flux cleaned = -0.00224085 Jy
! Component: 1250  -  total flux cleaned = -0.00221432 Jy
! Component: 1300  -  total flux cleaned = -0.00224038 Jy
! Component: 1350  -  total flux cleaned = -0.0022404 Jy
! Component: 1400  -  total flux cleaned = -0.00224041 Jy
! Component: 1450  -  total flux cleaned = -0.00231814 Jy
! Component: 1500  -  total flux cleaned = -0.00236964 Jy
! Component: 1550  -  total flux cleaned = -0.00242091 Jy
! Component: 1600  -  total flux cleaned = -0.00244654 Jy
! Component: 1650  -  total flux cleaned = -0.00257329 Jy
! Component: 1700  -  total flux cleaned = -0.00257346 Jy
! Component: 1750  -  total flux cleaned = -0.00269913 Jy
! Component: 1800  -  total flux cleaned = -0.00272422 Jy
! Component: 1850  -  total flux cleaned = -0.00277402 Jy
! Component: 1900  -  total flux cleaned = -0.00287338 Jy
! Component: 1950  -  total flux cleaned = -0.00289807 Jy
! Component: 2000  -  total flux cleaned = -0.00292261 Jy
! Total flux subtracted in 2048 components = -0.00304519 Jy
! Clean residual min=-0.001600 max=0.001226 Jy/beam
! Clean residual mean=0.000007 rms=0.000435 Jy/beam
! Combined flux in latest and established models = 1.61037 Jy
keep
! Adding 196 model components to the UV plane model.
! The established model now contains 337 components and 1.61037 Jy
![Exited script file: muppet]
wmap "J0102+5824_X_2001_03_12_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6754 x 0.7524 at 6.821 degrees (North through East)
! Clean map  min=-0.0015801  max=1.4179 Jy/beam
! Writing clean map to FITS file: J0102+5824_X_2001_03_12_pus_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 1.41792 
invert
! Inverting map 
! Your choice of large map pixels excluded 5.26% of the data.
!  The x-axis pixel size should ideally be below 0.1612 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1672 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.00043576 
device "J0102+5824_X_2001_03_12_pus\_map.eps/VPS"
! Attempting to open device: 'J0102+5824_X_2001_03_12_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.0921971 0.0921971 0.184394 0.368789 0.737577 1.47515 2.95031 5.90062 11.8012 23.6025 47.2049 94.4099
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0013 
print "peak=",int(1000*peak_flux)/1000
! peak= 1.417 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6754 x 0.7524 at 6.821 degrees (North through East)
! Clean map  min=-0.0015801  max=1.4179 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
quit
! Quitting program
! Log file J0102+5824_X_2001_03_12_pus_uvs.log closed on Wed Jan  2 19:48:24 2013