! Started logfile: J0402-3147_X_2010_06_23_pus_uvs.log on Thu Jan 27 23:38:51 2011
obs J0402-3147_X_2010_06_23_pus_uva.fits
! Reading UV FITS file: J0402-3147_X_2010_06_23_pus_uva.fits
! AN table 1: 92 integrations on 105 of 105 possible baselines.
! AN table 2: 91 integrations on 105 of 105 possible baselines.
! AN table 3: 53 integrations on 105 of 105 possible baselines.
! Apparent sampling: 0.241646 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J0402-3147
! 
! 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 23952 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 J0402-3147_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 759 telescope corrections were flagged in sub-array 1.
!  A total of 694 telescope corrections were flagged in sub-array 2.
!  A total of 499 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 759 telescope corrections were flagged in sub-array 1.
!  A total of 694 telescope corrections were flagged in sub-array 2.
!  A total of 499 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 759 telescope corrections were flagged in sub-array 1.
!  A total of 694 telescope corrections were flagged in sub-array 2.
!  A total of 499 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 759 telescope corrections were flagged in sub-array 1.
!  A total of 694 telescope corrections were flagged in sub-array 2.
!  A total of 505 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=0.633249Jy  sigma=0.005529
! Fit after  self-cal, rms=0.549685Jy  sigma=0.004760
! 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 1.04% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
! Estimated beam: bmin=0.6242 mas, bmaj=1.742 mas, bpa=-1.928 degrees
! Estimated noise=988.975 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 = 0.338651 Jy
! Component: 100  -  total flux cleaned = 0.428553 Jy
! Total flux subtracted in 100 components = 0.428553 Jy
! Clean residual min=-0.023810 max=0.089662 Jy/beam
! Clean residual mean=0.001205 rms=0.009036 Jy/beam
! Combined flux in latest and established models = 0.428553 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 8 components and 0.428553 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.274756Jy  sigma=0.002569
! Fit after  self-cal, rms=0.274712Jy  sigma=0.002568
! Inverting map 
! Your choice of large map pixels excluded 1.04% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
! Added new window around map position (-0.8, 0.8).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.079298 Jy
! Component: 100  -  total flux cleaned = 0.122492 Jy
! Total flux subtracted in 100 components = 0.122492 Jy
! Clean residual min=-0.021073 max=0.058958 Jy/beam
! Clean residual mean=0.000745 rms=0.006309 Jy/beam
! Combined flux in latest and established models = 0.551045 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 14 components and 0.551045 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.226878Jy  sigma=0.001969
! Fit after  self-cal, rms=0.223523Jy  sigma=0.001939
! Inverting map 
! Your choice of large map pixels excluded 1.04% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0371942 Jy
! Component: 100  -  total flux cleaned = 0.0566322 Jy
! Total flux subtracted in 100 components = 0.0566322 Jy
! Clean residual min=-0.015980 max=0.035542 Jy/beam
! Clean residual mean=0.000530 rms=0.004807 Jy/beam
! Combined flux in latest and established models = 0.607677 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 21 components and 0.607677 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.208392Jy  sigma=0.001728
! Fit after  self-cal, rms=0.207338Jy  sigma=0.001719
! Inverting map 
! Your choice of large map pixels excluded 1.04% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
! Added new window around map position (0.8, 1.8).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0271813 Jy
! Component: 100  -  total flux cleaned = 0.0427105 Jy
! Total flux subtracted in 100 components = 0.0427105 Jy
! Clean residual min=-0.012339 max=0.020576 Jy/beam
! Clean residual mean=0.000362 rms=0.004007 Jy/beam
! Combined flux in latest and established models = 0.650387 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 29 components and 0.650387 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.198976Jy  sigma=0.001602
! Fit after  self-cal, rms=0.198648Jy  sigma=0.001598
! Inverting map 
! Your choice of large map pixels excluded 1.04% of the data.
!  The x-axis pixel size should ideally be below 0.1911 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 1.04% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
! Estimated beam: bmin=0.8454 mas, bmaj=2.31 mas, bpa=-6.487 degrees
! Estimated noise=497.359 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 = 0.0420489 Jy
! Component: 100  -  total flux cleaned = 0.0644694 Jy
! Component: 150  -  total flux cleaned = 0.0777582 Jy
! Component: 200  -  total flux cleaned = 0.0858587 Jy
! Total flux subtracted in 200 components = 0.0858587 Jy
! Clean residual min=-0.008486 max=0.015064 Jy/beam
! Clean residual mean=0.000176 rms=0.003408 Jy/beam
! Combined flux in latest and established models = 0.736246 Jy
! Performing phase self-cal
! Adding 33 model components to the UV plane model.
! The established model now contains 51 components and 0.736246 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.191837Jy  sigma=0.001478
! Fit after  self-cal, rms=0.191679Jy  sigma=0.001477
! Inverting map 
! Your choice of large map pixels excluded 1.04% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 84 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.95     FD        0.99     HN        1.00*    KK        1.01     
!   KP        0.97     LA        0.94     MA        1.00*    MK        0.98     
!   NL        1.23     NY        1.00*    OV        0.97     PT        0.99     
!   SC        0.98     TS        1.00*    ZC        1.00*    
! 
!  A total of 21 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.99     FD        0.98     HN        1.22     KK        1.04     
!   KP        0.96     LA        0.96     MA        1.00*    MK        0.97     
!   NL        0.96     NY        1.00*    OV        0.97     PT        0.98     
!   SC        1.05     TS        1.00*    ZC        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        0.98     HN        1.45     KK        1.00*    
!   KP        1.00     LA        0.95     MA        1.00*    MK        1.00*    
!   NL        1.22     NY        1.00*    OV        1.02     PT        1.02     
!   SC        0.94     TS        1.00*    ZC        1.00*    
! 
! 
! Correcting IF 2.
!  A total of 84 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.01     FD        0.99     HN        1.00*    KK        1.03     
!   KP        0.97     LA        0.97     MA        1.00*    MK        0.99     
!   NL        1.27     NY        1.00*    OV        0.98     PT        0.98     
!   SC        0.99     TS        1.00*    ZC        1.00*    
! 
!  A total of 21 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.04     FD        0.98     HN        1.19     KK        1.08     
!   KP        0.95     LA        0.99     MA        1.00*    MK        0.97     
!   NL        1.00     NY        1.00*    OV        1.01     PT        0.98     
!   SC        1.13     TS        1.00*    ZC        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        0.96     HN        1.43     KK        1.00*    
!   KP        1.00     LA        1.00     MA        1.00*    MK        1.00*    
!   NL        1.30     NY        1.00*    OV        1.03     PT        1.00     
!   SC        0.94     TS        1.00*    ZC        1.00*    
! 
! 
! Correcting IF 3.
!  A total of 84 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.98     FD        0.99     HN        1.00*    KK        1.04     
!   KP        0.97     LA        0.97     MA        1.00*    MK        1.01     
!   NL        1.22     NY        1.00*    OV        0.97     PT        0.98     
!   SC        0.92     TS        1.00*    ZC        1.00*    
! 
!  A total of 21 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.01     FD        0.96     HN        1.24     KK        1.05     
!   KP        0.95     LA        0.98     MA        1.00*    MK        0.98     
!   NL        0.94     NY        1.00*    OV        0.99     PT        0.98     
!   SC        1.02     TS        1.00*    ZC        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        0.97     HN        1.44     KK        1.00*    
!   KP        0.99     LA        0.99     MA        1.00*    MK        1.00*    
!   NL        1.19     NY        1.00*    OV        1.02     PT        1.00     
!   SC        0.94     TS        1.00*    ZC        1.00*    
! 
! 
! Correcting IF 4.
!  A total of 84 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.04     FD        0.99     HN        1.00*    KK        0.95     
!   KP        0.97     LA        0.96     MA        1.00*    MK        0.99     
!   NL        1.25     NY        1.00*    OV        0.96     PT        0.98     
!   SC        0.96     TS        1.00*    ZC        1.00*    
! 
!  A total of 21 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.08     FD        0.99     HN        1.27     KK        1.01     
!   KP        0.96     LA        0.97     MA        1.00*    MK        0.98     
!   NL        0.95     NY        1.00*    OV        0.97     PT        1.00     
!   SC        1.03     TS        1.00*    ZC        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        0.98     HN        1.31     KK        1.00*    
!   KP        1.01     LA        0.98     MA        1.00*    MK        1.00*    
!   NL        1.21     NY        1.00*    OV        0.99     PT        1.03     
!   SC        0.93     TS        1.00*    ZC        1.00*    
! 
! 
! Fit before self-cal, rms=0.191679Jy  sigma=0.001477
! Fit after  self-cal, rms=0.206473Jy  sigma=0.001417
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
! Estimated beam: bmin=0.8633 mas, bmaj=2.329 mas, bpa=-7.199 degrees
! Estimated noise=503.509 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 = -0.00594066 Jy
! Component: 100  -  total flux cleaned = -0.00631997 Jy
! Component: 150  -  total flux cleaned = -0.00648498 Jy
! Component: 200  -  total flux cleaned = -0.00649165 Jy
! Total flux subtracted in 200 components = -0.00649165 Jy
! Clean residual min=-0.005733 max=0.006738 Jy/beam
! Clean residual mean=-0.000337 rms=0.001478 Jy/beam
! Combined flux in latest and established models = 0.729754 Jy
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 63 components and 0.729754 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.206048Jy  sigma=0.001413
! Fit after  self-cal, rms=0.206320Jy  sigma=0.001413
! Inverting map 
! Your choice of large map pixels excluded 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 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=0.206320Jy  sigma=0.001413
! Fit after  self-cal, rms=0.208088Jy  sigma=0.001405
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
! Estimated beam: bmin=0.8647 mas, bmaj=2.337 mas, bpa=-7.129 degrees
! Estimated noise=503.22 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00368143 Jy
! Component: 100  -  total flux cleaned = -0.00394086 Jy
! Component: 150  -  total flux cleaned = -0.00415871 Jy
! Component: 200  -  total flux cleaned = -0.00425935 Jy
! Total flux subtracted in 200 components = -0.00425935 Jy
! Clean residual min=-0.004820 max=0.005094 Jy/beam
! Clean residual mean=-0.000011 rms=0.001184 Jy/beam
! Combined flux in latest and established models = 0.725495 Jy
selfcal
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 69 components and 0.725495 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.207867Jy  sigma=0.001403
! Fit after  self-cal, rms=0.207827Jy  sigma=0.001403
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 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 (-2.4, 0.2).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00294803 Jy
! Component: 100  -  total flux cleaned = 0.00260233 Jy
! Component: 150  -  total flux cleaned = 0.00240385 Jy
! Component: 200  -  total flux cleaned = 0.0024039 Jy
! Total flux subtracted in 200 components = 0.0024039 Jy
! Clean residual min=-0.004633 max=0.003984 Jy/beam
! Clean residual mean=-0.000074 rms=0.001078 Jy/beam
! Combined flux in latest and established models = 0.727899 Jy
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 84 components and 0.727899 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.207616Jy  sigma=0.001401
! Fit after  self-cal, rms=0.207573Jy  sigma=0.001401
! Inverting map 
! Your choice of large map pixels excluded 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 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=0.207573Jy  sigma=0.001401
! Fit after  self-cal, rms=0.210676Jy  sigma=0.001390
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
! Estimated beam: bmin=0.8652 mas, bmaj=2.338 mas, bpa=-7.116 degrees
! Estimated noise=503.288 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00103465 Jy
! Component: 100  -  total flux cleaned = -0.000919589 Jy
! Component: 150  -  total flux cleaned = -0.000827833 Jy
! Component: 200  -  total flux cleaned = -0.000828533 Jy
! Total flux subtracted in 200 components = -0.000828533 Jy
! Clean residual min=-0.004161 max=0.003276 Jy/beam
! Clean residual mean=-0.000071 rms=0.000908 Jy/beam
! Combined flux in latest and established models = 0.72707 Jy
selfcal
! Performing phase self-cal
! Adding 24 model components to the UV plane model.
! The established model now contains 91 components and 0.72707 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.210531Jy  sigma=0.001389
! Fit after  self-cal, rms=0.210544Jy  sigma=0.001389
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 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 = 5.27908e-05 Jy
! Component: 100  -  total flux cleaned = 0.000136218 Jy
! Component: 150  -  total flux cleaned = 0.000138393 Jy
! Component: 200  -  total flux cleaned = 0.000140339 Jy
! Total flux subtracted in 200 components = 0.000140339 Jy
! Clean residual min=-0.003980 max=0.003228 Jy/beam
! Clean residual mean=-0.000074 rms=0.000882 Jy/beam
! Combined flux in latest and established models = 0.727211 Jy
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 95 components and 0.727211 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.210463Jy  sigma=0.001389
! Fit after  self-cal, rms=0.210437Jy  sigma=0.001389
! Inverting map 
! Your choice of large map pixels excluded 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 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=0.210437Jy  sigma=0.001389
! Fit after  self-cal, rms=0.211535Jy  sigma=0.001388
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
! Estimated beam: bmin=2.485 mas, bmaj=6.445 mas, bpa=0.1886 degrees
! Estimated noise=600.187 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00184909 Jy
! Component: 100  -  total flux cleaned = -0.00172356 Jy
! Component: 150  -  total flux cleaned = -0.00161943 Jy
! Component: 200  -  total flux cleaned = -0.00164761 Jy
! Total flux subtracted in 200 components = -0.00164761 Jy
! Clean residual min=-0.003364 max=0.003251 Jy/beam
! Clean residual mean=-0.000110 rms=0.000994 Jy/beam
! Combined flux in latest and established models = 0.725563 Jy
selfcal
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 106 components and 0.725563 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.211484Jy  sigma=0.001388
! Fit after  self-cal, rms=0.211465Jy  sigma=0.001388
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 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 = -0.000221303 Jy
! Component: 100  -  total flux cleaned = -0.000187031 Jy
! Component: 150  -  total flux cleaned = -0.000130048 Jy
! Component: 200  -  total flux cleaned = -0.000127892 Jy
! Total flux subtracted in 200 components = -0.000127892 Jy
! Clean residual min=-0.003274 max=0.003264 Jy/beam
! Clean residual mean=-0.000104 rms=0.000990 Jy/beam
! Combined flux in latest and established models = 0.725435 Jy
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 111 components and 0.725435 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.211440Jy  sigma=0.001388
! Fit after  self-cal, rms=0.211429Jy  sigma=0.001388
! Inverting map 
! Your choice of large map pixels excluded 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 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 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
! Estimated beam: bmin=0.8658 mas, bmaj=2.339 mas, bpa=-7.104 degrees
! Estimated noise=503.306 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8658 x 2.339 at -7.104 degrees (North through East)
! Clean map  min=-0.0034822  max=0.47874 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 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
! Estimated beam: bmin=0.6623 mas, bmaj=1.765 mas, bpa=-5.884 degrees
! Estimated noise=1060.89 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.359656 Jy
! Component: 100  -  total flux cleaned = 0.490959 Jy
! Component: 150  -  total flux cleaned = 0.563857 Jy
! Component: 200  -  total flux cleaned = 0.608502 Jy
! Total flux subtracted in 200 components = 0.608502 Jy
! Clean residual min=-0.008665 max=0.023846 Jy/beam
! Clean residual mean=0.000563 rms=0.003583 Jy/beam
! Combined flux in latest and established models = 0.608502 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 20 model components to the UV plane model.
! The established model now contains 20 components and 0.608502 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
! Estimated beam: bmin=0.8658 mas, bmaj=2.339 mas, bpa=-7.104 degrees
! Estimated noise=503.306 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 = 0.0535095 Jy
! Component: 100  -  total flux cleaned = 0.0794329 Jy
! Component: 150  -  total flux cleaned = 0.0931761 Jy
! Component: 200  -  total flux cleaned = 0.101212 Jy
! Total flux subtracted in 200 components = 0.101212 Jy
! Clean residual min=-0.003414 max=0.005856 Jy/beam
! Clean residual mean=0.000338 rms=0.001362 Jy/beam
! Combined flux in latest and established models = 0.709714 Jy
! Adding 46 model components to the UV plane model.
! The established model now contains 58 components and 0.709714 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
! Added new window around map position (-0.8, 4.6).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00558756 Jy
! Component: 100  -  total flux cleaned = 0.00916306 Jy
! Component: 150  -  total flux cleaned = 0.0111652 Jy
! Component: 200  -  total flux cleaned = 0.0121531 Jy
! Total flux subtracted in 200 components = 0.0121531 Jy
! Clean residual min=-0.003063 max=0.003540 Jy/beam
! Clean residual mean=0.000041 rms=0.000889 Jy/beam
! Combined flux in latest and established models = 0.721867 Jy
! Adding 26 model components to the UV plane model.
! The established model now contains 78 components and 0.721867 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 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 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
! Estimated beam: bmin=2.485 mas, bmaj=6.445 mas, bpa=0.1886 degrees
! Estimated noise=600.187 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00226705 Jy
! Component: 100  -  total flux cleaned = 0.00279203 Jy
! Component: 150  -  total flux cleaned = 0.0028626 Jy
! Component: 200  -  total flux cleaned = 0.00283217 Jy
! Total flux subtracted in 200 components = 0.00283217 Jy
! Clean residual min=-0.002754 max=0.003086 Jy/beam
! Clean residual mean=-0.000065 rms=0.000972 Jy/beam
! Combined flux in latest and established models = 0.724699 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 = 1.13416e-06 Jy
! Component: 100  -  total flux cleaned = 2.28719e-06 Jy
! Component: 150  -  total flux cleaned = 2.00541e-06 Jy
! Component: 200  -  total flux cleaned = 1.68476e-06 Jy
! Total flux subtracted in 200 components = 1.68476e-06 Jy
! Clean residual min=-0.002753 max=0.003116 Jy/beam
! Clean residual mean=-0.000066 rms=0.000962 Jy/beam
! Combined flux in latest and established models = 0.724701 Jy
! Adding 25 model components to the UV plane model.
! The established model now contains 102 components and 0.724701 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
! Estimated beam: bmin=0.8658 mas, bmaj=2.339 mas, bpa=-7.104 degrees
! Estimated noise=503.306 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00122397 Jy
! Component: 100  -  total flux cleaned = -0.0014288 Jy
! Component: 150  -  total flux cleaned = -0.00137556 Jy
! Component: 200  -  total flux cleaned = -0.00132404 Jy
! Total flux subtracted in 200 components = -0.00132404 Jy
! Clean residual min=-0.003096 max=0.003097 Jy/beam
! Clean residual mean=0.000001 rms=0.000843 Jy/beam
! Combined flux in latest and established models = 0.723377 Jy
selfcal
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 113 components and 0.723377 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.211444Jy  sigma=0.001388
! Fit after  self-cal, rms=0.211364Jy  sigma=0.001388
wmodel J0402-3147_X_2010_06_23_pus_map.mod
! Writing 113 model components to file: J0402-3147_X_2010_06_23_pus_map.mod
wobs J0402-3147_X_2010_06_23_pus_uvs.fits
! Writing UV FITS file: J0402-3147_X_2010_06_23_pus_uvs.fits
wwins J0402-3147_X_2010_06_23_pus_map.win
! wwins: Wrote 5 windows to J0402-3147_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 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000735648 Jy
! Component: 100  -  total flux cleaned = -0.000840095 Jy
! Component: 150  -  total flux cleaned = -0.000839476 Jy
! Component: 200  -  total flux cleaned = -0.000839434 Jy
! Component: 250  -  total flux cleaned = -0.00083944 Jy
! Component: 300  -  total flux cleaned = -0.000879828 Jy
! Component: 350  -  total flux cleaned = -0.00091937 Jy
! Component: 400  -  total flux cleaned = -0.00095828 Jy
! Component: 450  -  total flux cleaned = -0.00103321 Jy
! Component: 500  -  total flux cleaned = -0.00110539 Jy
! Component: 550  -  total flux cleaned = -0.00117566 Jy
! Component: 600  -  total flux cleaned = -0.00127862 Jy
! Component: 650  -  total flux cleaned = -0.00134534 Jy
! Component: 700  -  total flux cleaned = -0.00134492 Jy
! Component: 750  -  total flux cleaned = -0.0012154 Jy
! Component: 800  -  total flux cleaned = -0.00115163 Jy
! Component: 850  -  total flux cleaned = -0.00105776 Jy
! Component: 900  -  total flux cleaned = -0.00093483 Jy
! Component: 950  -  total flux cleaned = -0.000844179 Jy
! Component: 1000  -  total flux cleaned = -0.00078447 Jy
! Total flux subtracted in 1024 components = -0.000696165 Jy
! Clean residual min=-0.002024 max=0.001645 Jy/beam
! Clean residual mean=0.000027 rms=0.000600 Jy/beam
! Combined flux in latest and established models = 0.722681 Jy
keep
! Adding 52 model components to the UV plane model.
! The established model now contains 164 components and 0.722681 Jy
![Exited script file: muppet]
wmap "J0402-3147_X_2010_06_23_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8658 x 2.339 at -7.104 degrees (North through East)
! Clean map  min=-0.0025465  max=0.48981 Jy/beam
! Writing clean map to FITS file: J0402-3147_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 0.489813 
invert
! Inverting map 
! Your choice of large map pixels excluded 1.06% of the data.
!  The x-axis pixel size should ideally be below 0.1911 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000599653 
device "J0402-3147_X_2010_06_23_pus\_map.eps/VPS"
! Attempting to open device: 'J0402-3147_X_2010_06_23_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.367274 0.367274 0.734549 1.4691 2.93819 5.87639 11.7528 23.5056 47.0111 94.0222
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0017 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.489 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8658 x 2.339 at -7.104 degrees (North through East)
! Clean map  min=-0.0025465  max=0.48981 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0402-3147_X_2010_06_23_pus\_map.gif/vgif"
! Attempting to open device: 'J0402-3147_X_2010_06_23_pus_map.gif/vgif'
mapplot cln