! Started logfile: J1135-0428_X_2005_07_08_yyk_uvs.log on Fri Jan 20 10:22:20 2006
obs J1135-0428_X_2005_07_08_yyk_uve.fits
! Reading UV FITS file: J1135-0428_X_2005_07_08_yyk_uve.fits
! AN table 1: 11 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.90303 visibilities/baseline/integration-bin.
! Found source: J1135-0428
! 
! 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 1407 lines of history.
! 
! Reading 1788 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
![@muppet J1135-0428_X_2005_07_08_yyk]
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.04
float dynam
dynam = 6.0
float amp_soltime1
amp_soltime1 = 10
float amp_soltime2
amp_soltime2 = 1
float phase_soltime1
phase_soltime1=10
float phase_soltime2
phase_soltime2=0.5
float phase_soltime
phase_soltime=phase_soltime1
float ampcor_selflim
ampcor_selflim=1.20
float thresh
thresh = 0.10
float win_mult
win_mult = 1.8
float time_av
time_av = 30
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.
phase_soltime=phase_soltime1
print "uvstat(rms)=",uvstat(rms),"Jy"
! uvstat(rms)= 0.373319 Jy 
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 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=0.7171 mas, bmaj=1.804 mas, bpa=-0.9797 degrees
! Estimated noise=1.24497 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (0, 0).
! clean: niter=100  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.315062 Jy
! Component: 100  -  total flux cleaned = 0.358003 Jy
! Total flux subtracted in 100 components = 0.358003 Jy
! Clean residual min=-0.008151 max=0.010385 Jy/beam
! Clean residual mean=-0.000023 rms=0.002243 Jy/beam
! Combined flux in latest and established models = 0.358003 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 7 model components to the UV plane model.
! The established model now contains 7 components and 0.358003 Jy
! 
! Correcting IF 1.
!  A total of 12 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 12 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 13 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 13 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.070895Jy  sigma=1.237306
! Fit after  self-cal, rms=0.070083Jy  sigma=1.184755
! Inverting map and beam 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=0.717 mas, bmaj=1.804 mas, bpa=-0.9783 degrees
! Estimated noise=1.24581 mJy/beam.
print "************** FINISHED UNIFORM WEIGHTING CLEAN **************"
! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** 
! 
uvw 0,-2
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -2.
! 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 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=0.8874 mas, bmaj=2.131 mas, bpa=-0.8175 degrees
! Estimated noise=0.928121 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.01733 Jy
! Component: 100  -  total flux cleaned = 0.024382 Jy
! Component: 150  -  total flux cleaned = 0.0277503 Jy
! Component: 200  -  total flux cleaned = 0.0291547 Jy
! Total flux subtracted in 200 components = 0.0291547 Jy
! Clean residual min=-0.007462 max=0.007234 Jy/beam
! Clean residual mean=-0.000006 rms=0.001633 Jy/beam
! Combined flux in latest and established models = 0.387158 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 33 model components to the UV plane model.
! The established model now contains 38 components and 0.387158 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067744Jy  sigma=1.126772
! Fit after  self-cal, rms=0.067749Jy  sigma=1.126738
! Inverting map 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8874 x 2.131 at -0.8175 degrees (North through East)
! Clean map  min=-0.0068673  max=0.36597 Jy/beam
if(peak(flux) < thresh*2)
  selflims ampcor_selflim
  end if
gscale
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Amplitude normalization factor in sub-array 1: 1.00539
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.98     FD        0.99     HN        1.09     KP        0.96     
!   LA        1.00     MK        0.98     NL        1.00     OV        1.02     
!   PT        0.98     SC        0.95     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.0108
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        0.99     HN        1.10     KP        0.91     
!   LA        0.98     MK        0.98     NL        0.96     OV        1.02     
!   PT        1.02     SC        0.94     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 1.00971
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.04     FD        1.01     HN        0.97     KP        0.84     
!   LA        0.98     MK        1.05     NL        0.96     OV        1.04     
!   PT        1.06     SC        0.95     
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 0.948338
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.09     FD        1.03     HN        1.05     KP        0.99     
!   LA        0.99     MK        1.04     NL        0.99     OV        1.05     
!   PT        1.11     SC        1.21     
! 
! 
! Fit before self-cal, rms=0.067749Jy  sigma=1.126738
! Fit after  self-cal, rms=0.063528Jy  sigma=1.036064
selfcal false, false, phase_soltime
! Performing phase self-cal over 10 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.063528Jy  sigma=1.036064
! Fit after  self-cal, rms=0.063533Jy  sigma=1.036040
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=0.8913 mas, bmaj=2.145 mas, bpa=-0.6312 degrees
! Estimated noise=0.919736 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.00316658 Jy
! Component: 100  -  total flux cleaned = -0.00407683 Jy
! Component: 150  -  total flux cleaned = -0.00417916 Jy
! Component: 200  -  total flux cleaned = -0.00420307 Jy
! Total flux subtracted in 200 components = -0.00420307 Jy
! Clean residual min=-0.003610 max=0.003532 Jy/beam
! Clean residual mean=-0.000003 rms=0.000952 Jy/beam
! Combined flux in latest and established models = 0.382955 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 19 model components to the UV plane model.
! The established model now contains 53 components and 0.382955 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.063406Jy  sigma=1.033907
! Fit after  self-cal, rms=0.063406Jy  sigma=1.033899
! Inverting map 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
print "************** FINISHED AMPLITUDE GSCALE SELF-CAL **************"
! ************** FINISHED AMPLITUDE GSCALE SELF-CAL ************** 
! 
phase_soltime=phase_soltime2
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.063406Jy  sigma=1.033899
! Fit after  self-cal, rms=0.060500Jy  sigma=0.993801
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000224096 Jy
! Component: 100  -  total flux cleaned = 0.000267603 Jy
! Component: 150  -  total flux cleaned = 0.00029582 Jy
! Component: 200  -  total flux cleaned = 0.000304388 Jy
! Total flux subtracted in 200 components = 0.000304388 Jy
! Clean residual min=-0.003574 max=0.003389 Jy/beam
! Clean residual mean=-0.000003 rms=0.000944 Jy/beam
! Combined flux in latest and established models = 0.383259 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 11 model components to the UV plane model.
! The established model now contains 55 components and 0.383259 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.060500Jy  sigma=0.993752
! Fit after  self-cal, rms=0.060265Jy  sigma=0.991062
! Inverting map 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
print "*** FINISHED NATURAL WEIGHTING CLEAN with shorter phase_soltime ***"
! *** FINISHED NATURAL WEIGHTING CLEAN with shorter phase_soltime *** 
! 
dynam = dynam - 0.25
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8913 x 2.145 at -0.6312 degrees (North through East)
! Clean map  min=-0.003418  max=0.36371 Jy/beam
if(peak(flux) > thresh)
  selfcal true, true, amp_soltime1
  selfcal false, false, phase_soltime
  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 false,false,phase_soltime
    new_peak = peak(flux)
    until(new_peak<=flux_cutoff)
  selfcal true, true, amp_soltime2
  selfcal false, false, phase_soltime
  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 false,false,phase_soltime
    new_peak = peak(flux)
    until(new_peak<=flux_cutoff)
  print "************** FINISHED AMPLITUDE SELF-CAL **************"
  end if
! Performing amp+phase self-cal over 10 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.060265Jy  sigma=0.991062
! Fit after  self-cal, rms=0.057429Jy  sigma=0.922830
! Performing phase self-cal over 0.5 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.057429Jy  sigma=0.922830
! Fit after  self-cal, rms=0.057406Jy  sigma=0.922515
! Inverting map and beam 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=0.8908 mas, bmaj=2.149 mas, bpa=-0.6547 degrees
! Estimated noise=0.918234 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 3.967e-05 Jy
! Component: 100  -  total flux cleaned = 3.85358e-05 Jy
! Component: 150  -  total flux cleaned = 8.10759e-05 Jy
! Component: 200  -  total flux cleaned = 0.000119967 Jy
! Total flux subtracted in 200 components = 0.000119967 Jy
! Clean residual min=-0.003137 max=0.002797 Jy/beam
! Clean residual mean=-0.000004 rms=0.000781 Jy/beam
! Combined flux in latest and established models = 0.383379 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 8 model components to the UV plane model.
! The established model now contains 58 components and 0.383379 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.057392Jy  sigma=0.922378
! Fit after  self-cal, rms=0.057393Jy  sigma=0.922315
! Inverting map 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Performing amp+phase self-cal over 1 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.057393Jy  sigma=0.922315
! Fit after  self-cal, rms=0.056138Jy  sigma=0.901191
! Performing phase self-cal over 0.5 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.056138Jy  sigma=0.901191
! Fit after  self-cal, rms=0.056140Jy  sigma=0.901175
! Inverting map and beam 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=0.8907 mas, bmaj=2.151 mas, bpa=-0.6682 degrees
! Estimated noise=0.918681 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000413976 Jy
! Component: 100  -  total flux cleaned = 0.000441444 Jy
! Component: 150  -  total flux cleaned = 0.000466825 Jy
! Component: 200  -  total flux cleaned = 0.000500249 Jy
! Total flux subtracted in 200 components = 0.000500249 Jy
! Clean residual min=-0.003198 max=0.002760 Jy/beam
! Clean residual mean=-0.000004 rms=0.000777 Jy/beam
! Combined flux in latest and established models = 0.383879 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 9 model components to the UV plane model.
! The established model now contains 58 components and 0.383879 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.056132Jy  sigma=0.901070
! Fit after  self-cal, rms=0.056135Jy  sigma=0.901060
! Inverting map 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! ************** FINISHED AMPLITUDE SELF-CAL ************** 
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
win_mult = win_mult * 1.4
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=2.317 mas, bmaj=3.865 mas, bpa=-3.93 degrees
! Estimated noise=1.17473 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -4.53461e-05 Jy
! Component: 100  -  total flux cleaned = -3.03051e-05 Jy
! Component: 150  -  total flux cleaned = -3.02459e-05 Jy
! Component: 200  -  total flux cleaned = -3.60111e-05 Jy
! Total flux subtracted in 200 components = -3.60111e-05 Jy
! Clean residual min=-0.003806 max=0.002895 Jy/beam
! Clean residual mean=-0.000007 rms=0.000933 Jy/beam
! Combined flux in latest and established models = 0.383843 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 7 model components to the UV plane model.
! The established model now contains 59 components and 0.383843 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.056136Jy  sigma=0.901100
! Fit after  self-cal, rms=0.056138Jy  sigma=0.901085
! Inverting map 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
win_mult = win_mult / 1.4
print "************** FINISHED TAPERING SELF-CAL CLEAN **************"
! ************** FINISHED TAPERING SELF-CAL CLEAN ************** 
! 
print "************** CLEARING MODEL AND STARTING OVER **********"
! ************** CLEARING MODEL AND STARTING OVER ********** 
clrmod true,true,true
! clrmod: Cleared the established, tentative and continuum 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 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=0.7203 mas, bmaj=1.816 mas, bpa=-1.114 degrees
! Estimated noise=1.24964 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.316767 Jy
! Component: 100  -  total flux cleaned = 0.35907 Jy
! Component: 150  -  total flux cleaned = 0.369641 Jy
! Component: 200  -  total flux cleaned = 0.375124 Jy
! Total flux subtracted in 200 components = 0.375124 Jy
! Clean residual min=-0.004272 max=0.004017 Jy/beam
! Clean residual mean=-0.000009 rms=0.001097 Jy/beam
! Combined flux in latest and established models = 0.375124 Jy
uvw 0,-2
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -2.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Adding 30 model components to the UV plane model.
! The established model now contains 30 components and 0.375124 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=0.8907 mas, bmaj=2.151 mas, bpa=-0.6682 degrees
! Estimated noise=0.918681 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=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00471529 Jy
! Component: 100  -  total flux cleaned = 0.00673097 Jy
! Component: 150  -  total flux cleaned = 0.00747997 Jy
! Component: 200  -  total flux cleaned = 0.00770098 Jy
! Total flux subtracted in 200 components = 0.00770098 Jy
! Clean residual min=-0.003157 max=0.002793 Jy/beam
! Clean residual mean=-0.000006 rms=0.000784 Jy/beam
! Combined flux in latest and established models = 0.382825 Jy
! Adding 18 model components to the UV plane model.
! The established model now contains 45 components and 0.382825 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=2.317 mas, bmaj=3.865 mas, bpa=-3.93 degrees
! Estimated noise=1.17473 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=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000462951 Jy
! Component: 100  -  total flux cleaned = 0.000508894 Jy
! Component: 150  -  total flux cleaned = 0.000536847 Jy
! Component: 200  -  total flux cleaned = 0.000562637 Jy
! Total flux subtracted in 200 components = 0.000562637 Jy
! Clean residual min=-0.003777 max=0.002880 Jy/beam
! Clean residual mean=-0.000008 rms=0.000935 Jy/beam
! Combined flux in latest and established models = 0.383388 Jy
! Adding 6 model components to the UV plane model.
! The established model now contains 48 components and 0.383388 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=0.8907 mas, bmaj=2.151 mas, bpa=-0.6682 degrees
! Estimated noise=0.918681 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.000154006 Jy
! Component: 100  -  total flux cleaned = -0.000134203 Jy
! Component: 150  -  total flux cleaned = -7.91623e-05 Jy
! Component: 200  -  total flux cleaned = -4.50656e-05 Jy
! Total flux subtracted in 200 components = -4.50656e-05 Jy
! Clean residual min=-0.003150 max=0.002801 Jy/beam
! Clean residual mean=-0.000005 rms=0.000782 Jy/beam
! Combined flux in latest and established models = 0.383343 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 12 model components to the UV plane model.
! The established model now contains 53 components and 0.383343 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.056143Jy  sigma=0.901266
! Fit after  self-cal, rms=0.056144Jy  sigma=0.901257
wmodel J1135-0428_X_2005_07_08_yyk\_map.mod
! Writing 53 model components to file: J1135-0428_X_2005_07_08_yyk_map.mod
wobs J1135-0428_X_2005_07_08_yyk\_uvs.fits
! Writing UV FITS file: J1135-0428_X_2005_07_08_yyk_uvs.fits
wwins J1135-0428_X_2005_07_08_yyk\_map.win
! wwins: Wrote 1 windows to J1135-0428_X_2005_07_08_yyk_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 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000974196 Jy
! Component: 100  -  total flux cleaned = -0.00138186 Jy
! Component: 150  -  total flux cleaned = -0.0018698 Jy
! Component: 200  -  total flux cleaned = -0.00224253 Jy
! Component: 250  -  total flux cleaned = -0.00264524 Jy
! Component: 300  -  total flux cleaned = -0.0029911 Jy
! Component: 350  -  total flux cleaned = -0.0031599 Jy
! Component: 400  -  total flux cleaned = -0.00332427 Jy
! Component: 450  -  total flux cleaned = -0.00340432 Jy
! Component: 500  -  total flux cleaned = -0.00352251 Jy
! Component: 550  -  total flux cleaned = -0.00375122 Jy
! Component: 600  -  total flux cleaned = -0.0038244 Jy
! Component: 650  -  total flux cleaned = -0.00378784 Jy
! Component: 700  -  total flux cleaned = -0.0039312 Jy
! Component: 750  -  total flux cleaned = -0.00389557 Jy
! Component: 800  -  total flux cleaned = -0.00386125 Jy
! Component: 850  -  total flux cleaned = -0.00396354 Jy
! Component: 900  -  total flux cleaned = -0.00399752 Jy
! Component: 950  -  total flux cleaned = -0.004031 Jy
! Component: 1000  -  total flux cleaned = -0.00403106 Jy
! Component: 1050  -  total flux cleaned = -0.00393525 Jy
! Component: 1100  -  total flux cleaned = -0.00393525 Jy
! Component: 1150  -  total flux cleaned = -0.00396586 Jy
! Component: 1200  -  total flux cleaned = -0.00393494 Jy
! Component: 1250  -  total flux cleaned = -0.00393515 Jy
! Component: 1300  -  total flux cleaned = -0.00390498 Jy
! Component: 1350  -  total flux cleaned = -0.00384593 Jy
! Component: 1400  -  total flux cleaned = -0.00381711 Jy
! Component: 1450  -  total flux cleaned = -0.00370229 Jy
! Component: 1500  -  total flux cleaned = -0.00367411 Jy
! Component: 1550  -  total flux cleaned = -0.00361862 Jy
! Component: 1600  -  total flux cleaned = -0.00370195 Jy
! Component: 1650  -  total flux cleaned = -0.00350999 Jy
! Component: 1700  -  total flux cleaned = -0.0035646 Jy
! Component: 1750  -  total flux cleaned = -0.00351076 Jy
! Component: 1800  -  total flux cleaned = -0.00348406 Jy
! Component: 1850  -  total flux cleaned = -0.00351021 Jy
! Component: 1900  -  total flux cleaned = -0.00351004 Jy
! Component: 1950  -  total flux cleaned = -0.00356164 Jy
! Component: 2000  -  total flux cleaned = -0.0036898 Jy
! Total flux subtracted in 2048 components = -0.00366454 Jy
! Clean residual min=-0.001561 max=0.001422 Jy/beam
! Clean residual mean=-0.000009 rms=0.000477 Jy/beam
! Combined flux in latest and established models = 0.379678 Jy
keep
! Adding 140 model components to the UV plane model.
! The established model now contains 193 components and 0.379678 Jy
![Exited script file: muppet]
wmap "J1135-0428_X_2005_07_08_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8907 x 2.151 at -0.6682 degrees (North through East)
! Clean map  min=-0.002398  max=0.3647 Jy/beam
! Writing clean map to FITS file: J1135-0428_X_2005_07_08_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.364697 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.299% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000471893 
device "J1135-0428_X_2005_07_08_yyk\_map.eps/VPS"
! Attempting to open device: 'J1135-0428_X_2005_07_08_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.388179 0.388179 0.776358 1.55272 3.10543 6.21087 12.4217 24.8435 49.6869 99.3738
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0014 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.364 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8907 x 2.151 at -0.6682 degrees (North through East)
! Clean map  min=-0.002398  max=0.3647 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1135-0428_X_2005_07_08_yyk\_map.gif/gif"
! Attempting to open device: 'J1135-0428_X_2005_07_08_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1135-0428_X_2005_07_08_yyk_uvs.log closed on Fri Jan 20 10:22:24 2006