! Started logfile: J0206-1150_X_2007_01_11_yyk_uvs.log on Mon Jun 16 19:07:44 2008
obs J0206-1150_X_2007_01_11_yyk_uve.fits
! Reading UV FITS file: J0206-1150_X_2007_01_11_yyk_uve.fits
! AN table 1: 15 integrations on 36 of 36 possible baselines.
! Apparent sampling: 0.764815 visibilities/baseline/integration-bin.
! Found source: J0206-1150
! 
! 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 2143 lines of history.
! 
! Reading 1652 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 J0206-1150_X_2007_01_11_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)= 0.255742 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 0.431% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.6268 mas, bmaj=1.695 mas, bpa=0.6755 degrees
! Estimated noise=1.41903 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 = 0.204317 Jy
! Component: 100  -  total flux cleaned = 0.236418 Jy
! Total flux subtracted in 100 components = 0.236418 Jy
! Clean residual min=-0.007185 max=0.009082 Jy/beam
! Clean residual mean=-0.000019 rms=0.002113 Jy/beam
! Combined flux in latest and established models = 0.236418 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 12 model components to the UV plane model.
! The established model now contains 12 components and 0.236418 Jy
! 
! Correcting IF 1.
!  A total of 16 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 16 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 17 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 17 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.080448Jy  sigma=1.387078
! Fit after  self-cal, rms=0.080379Jy  sigma=1.383884
! Inverting map and beam 
! Your choice of large map pixels excluded 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.6269 mas, bmaj=1.696 mas, bpa=0.6765 degrees
! Estimated noise=1.41876 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 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.7837 mas, bmaj=2.022 mas, bpa=-0.1371 degrees
! Estimated noise=0.952694 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 = 0.0182912 Jy
! Component: 100  -  total flux cleaned = 0.0257481 Jy
! Component: 150  -  total flux cleaned = 0.0290013 Jy
! Component: 200  -  total flux cleaned = 0.0305105 Jy
! Total flux subtracted in 200 components = 0.0305105 Jy
! Clean residual min=-0.005827 max=0.004685 Jy/beam
! Clean residual mean=0.000014 rms=0.001355 Jy/beam
! Combined flux in latest and established models = 0.266928 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 28 model components to the UV plane model.
! The established model now contains 35 components and 0.266928 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.077671Jy  sigma=1.330444
! Fit after  self-cal, rms=0.077638Jy  sigma=1.330276
! Inverting map 
! Your choice of large map pixels excluded 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7837 x 2.022 at -0.1371 degrees (North through East)
! Clean map  min=-0.0053979  max=0.24125 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: 1.00273
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.98     FD        0.99     HN        1.00     KP        0.99     
!   LA        0.97     MK        1.03     OV        1.01     PT        0.97     
!   SC        1.03     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.01715
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     FD        0.99     HN        1.02     KP        0.93     
!   LA        0.95     MK        0.96     OV        0.98     PT        1.05     
!   SC        0.98     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 1.00381
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.01     FD        1.00     HN        0.95     KP        0.84     
!   LA        0.99     MK        1.04     OV        1.07     PT        1.04     
!   SC        1.02     
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 0.985843
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.03     FD        1.08     HN        0.94     KP        0.89     
!   LA        0.97     MK        1.02     OV        1.08     PT        1.11     
!   SC        1.00     
! 
! 
! Fit before self-cal, rms=0.077638Jy  sigma=1.330276
! Fit after  self-cal, rms=0.076180Jy  sigma=1.301003
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=0.076180Jy  sigma=1.301003
! Fit after  self-cal, rms=0.076174Jy  sigma=1.300992
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.7888 mas, bmaj=2.032 mas, bpa=-0.1216 degrees
! Estimated noise=0.958529 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 = 0.00157928 Jy
! Component: 100  -  total flux cleaned = 0.0015789 Jy
! Component: 150  -  total flux cleaned = 0.00163441 Jy
! Component: 200  -  total flux cleaned = 0.00163719 Jy
! Total flux subtracted in 200 components = 0.00163719 Jy
! Clean residual min=-0.003946 max=0.003553 Jy/beam
! Clean residual mean=0.000004 rms=0.000933 Jy/beam
! Combined flux in latest and established models = 0.268566 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 9 model components to the UV plane model.
! The established model now contains 38 components and 0.268566 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.076146Jy  sigma=1.300311
! Fit after  self-cal, rms=0.076132Jy  sigma=1.300256
! Inverting map 
! Your choice of large map pixels excluded 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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=0.076132Jy  sigma=1.300256
! Fit after  self-cal, rms=0.055757Jy  sigma=0.948309
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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 = 0.00274616 Jy
! Component: 100  -  total flux cleaned = 0.00253249 Jy
! Component: 150  -  total flux cleaned = 0.00221409 Jy
! Component: 200  -  total flux cleaned = 0.00204637 Jy
! Total flux subtracted in 200 components = 0.00204637 Jy
! Clean residual min=-0.003952 max=0.002969 Jy/beam
! Clean residual mean=0.000002 rms=0.000916 Jy/beam
! Combined flux in latest and established models = 0.270612 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 41 components and 0.270612 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.055253Jy  sigma=0.940040
! Fit after  self-cal, rms=0.054430Jy  sigma=0.927558
! Inverting map 
! Your choice of large map pixels excluded 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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: 0.7888 x 2.032 at -0.1216 degrees (North through East)
! Clean map  min=-0.003579  max=0.24868 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=0.054430Jy  sigma=0.927558
! Fit after  self-cal, rms=0.053974Jy  sigma=0.916321
! 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=0.053974Jy  sigma=0.916321
! Fit after  self-cal, rms=0.053915Jy  sigma=0.915518
! Inverting map and beam 
! Your choice of large map pixels excluded 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.7858 mas, bmaj=2.023 mas, bpa=0.1415 degrees
! Estimated noise=0.955131 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 4.7128e-05 Jy
! Component: 100  -  total flux cleaned = 0.000164241 Jy
! Component: 150  -  total flux cleaned = 0.000211597 Jy
! Component: 200  -  total flux cleaned = 0.000211804 Jy
! Total flux subtracted in 200 components = 0.000211804 Jy
! Clean residual min=-0.003940 max=0.002758 Jy/beam
! Clean residual mean=-0.000005 rms=0.000842 Jy/beam
! Combined flux in latest and established models = 0.270824 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 45 components and 0.270824 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.053898Jy  sigma=0.915131
! Fit after  self-cal, rms=0.053886Jy  sigma=0.915003
! Inverting map 
! Your choice of large map pixels excluded 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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=0.053886Jy  sigma=0.915003
! Fit after  self-cal, rms=0.052422Jy  sigma=0.885866
! 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=0.052422Jy  sigma=0.885866
! Fit after  self-cal, rms=0.052426Jy  sigma=0.885836
! Inverting map and beam 
! Your choice of large map pixels excluded 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.7853 mas, bmaj=2.022 mas, bpa=0.06673 degrees
! Estimated noise=0.955855 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000463404 Jy
! Component: 100  -  total flux cleaned = 0.000538986 Jy
! Component: 150  -  total flux cleaned = 0.000603528 Jy
! Component: 200  -  total flux cleaned = 0.000658303 Jy
! Total flux subtracted in 200 components = 0.000658303 Jy
! Clean residual min=-0.003831 max=0.002795 Jy/beam
! Clean residual mean=-0.000004 rms=0.000835 Jy/beam
! Combined flux in latest and established models = 0.271482 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 10 model components to the UV plane model.
! The established model now contains 46 components and 0.271482 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.052409Jy  sigma=0.885526
! Fit after  self-cal, rms=0.052407Jy  sigma=0.885496
! Inverting map 
! Your choice of large map pixels excluded 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=2.154 mas, bmaj=4.256 mas, bpa=14.21 degrees
! Estimated noise=1.30946 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 = 0.000533249 Jy
! Component: 100  -  total flux cleaned = 0.000602047 Jy
! Component: 150  -  total flux cleaned = 0.000642047 Jy
! Component: 200  -  total flux cleaned = 0.000695048 Jy
! Total flux subtracted in 200 components = 0.000695048 Jy
! Clean residual min=-0.003870 max=0.003428 Jy/beam
! Clean residual mean=-0.000006 rms=0.001108 Jy/beam
! Combined flux in latest and established models = 0.272177 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 5 model components to the UV plane model.
! The established model now contains 47 components and 0.272177 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.052402Jy  sigma=0.885465
! Fit after  self-cal, rms=0.052399Jy  sigma=0.885411
! Inverting map 
! Your choice of large map pixels excluded 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.6281 mas, bmaj=1.696 mas, bpa=0.7132 degrees
! Estimated noise=1.42407 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.211119 Jy
! Component: 100  -  total flux cleaned = 0.242286 Jy
! Component: 150  -  total flux cleaned = 0.254118 Jy
! Component: 200  -  total flux cleaned = 0.260915 Jy
! Total flux subtracted in 200 components = 0.260915 Jy
! Clean residual min=-0.005411 max=0.005161 Jy/beam
! Clean residual mean=-0.000011 rms=0.001284 Jy/beam
! Combined flux in latest and established models = 0.260915 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 0.260915 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.7853 mas, bmaj=2.022 mas, bpa=0.06673 degrees
! Estimated noise=0.955855 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 = 0.00634861 Jy
! Component: 100  -  total flux cleaned = 0.00894378 Jy
! Component: 150  -  total flux cleaned = 0.0101682 Jy
! Component: 200  -  total flux cleaned = 0.0107187 Jy
! Total flux subtracted in 200 components = 0.0107187 Jy
! Clean residual min=-0.003814 max=0.002782 Jy/beam
! Clean residual mean=-0.000004 rms=0.000832 Jy/beam
! Combined flux in latest and established models = 0.271634 Jy
! Adding 18 model components to the UV plane model.
! The established model now contains 41 components and 0.271634 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=2.154 mas, bmaj=4.256 mas, bpa=14.21 degrees
! Estimated noise=1.30946 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 = 0.000543772 Jy
! Component: 100  -  total flux cleaned = 0.000580815 Jy
! Component: 150  -  total flux cleaned = 0.000614419 Jy
! Component: 200  -  total flux cleaned = 0.000645092 Jy
! Total flux subtracted in 200 components = 0.000645092 Jy
! Clean residual min=-0.003857 max=0.003414 Jy/beam
! Clean residual mean=-0.000005 rms=0.001106 Jy/beam
! Combined flux in latest and established models = 0.272279 Jy
! Adding 7 model components to the UV plane model.
! The established model now contains 43 components and 0.272279 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.7853 mas, bmaj=2.022 mas, bpa=0.06673 degrees
! Estimated noise=0.955855 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.000214304 Jy
! Component: 100  -  total flux cleaned = -0.000296241 Jy
! Component: 150  -  total flux cleaned = -0.000279724 Jy
! Component: 200  -  total flux cleaned = -0.00028061 Jy
! Total flux subtracted in 200 components = -0.00028061 Jy
! Clean residual min=-0.003806 max=0.002825 Jy/beam
! Clean residual mean=-0.000004 rms=0.000830 Jy/beam
! Combined flux in latest and established models = 0.271998 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 50 components and 0.271998 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.052375Jy  sigma=0.885020
! Fit after  self-cal, rms=0.052369Jy  sigma=0.884968
wmodel J0206-1150_X_2007_01_11_yyk\_map.mod
! Writing 50 model components to file: J0206-1150_X_2007_01_11_yyk_map.mod
wobs J0206-1150_X_2007_01_11_yyk\_uvs.fits
! Writing UV FITS file: J0206-1150_X_2007_01_11_yyk_uvs.fits
wwins J0206-1150_X_2007_01_11_yyk\_map.win
! wwins: Wrote 1 windows to J0206-1150_X_2007_01_11_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 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00167944 Jy
! Component: 100  -  total flux cleaned = -0.00313471 Jy
! Component: 150  -  total flux cleaned = -0.00435616 Jy
! Component: 200  -  total flux cleaned = -0.00528495 Jy
! Component: 250  -  total flux cleaned = -0.0061954 Jy
! Component: 300  -  total flux cleaned = -0.00658302 Jy
! Component: 350  -  total flux cleaned = -0.00682857 Jy
! Component: 400  -  total flux cleaned = -0.00702415 Jy
! Component: 450  -  total flux cleaned = -0.00713687 Jy
! Component: 500  -  total flux cleaned = -0.00724537 Jy
! Component: 550  -  total flux cleaned = -0.00731652 Jy
! Component: 600  -  total flux cleaned = -0.00741885 Jy
! Component: 650  -  total flux cleaned = -0.00738539 Jy
! Component: 700  -  total flux cleaned = -0.00751542 Jy
! Component: 750  -  total flux cleaned = -0.00757867 Jy
! Component: 800  -  total flux cleaned = -0.00767125 Jy
! Component: 850  -  total flux cleaned = -0.00779174 Jy
! Component: 900  -  total flux cleaned = -0.00776175 Jy
! Component: 950  -  total flux cleaned = -0.00779066 Jy
! Component: 1000  -  total flux cleaned = -0.00767703 Jy
! Component: 1050  -  total flux cleaned = -0.00756546 Jy
! Component: 1100  -  total flux cleaned = -0.0075651 Jy
! Component: 1150  -  total flux cleaned = -0.00737532 Jy
! Component: 1200  -  total flux cleaned = -0.00721554 Jy
! Component: 1250  -  total flux cleaned = -0.00708421 Jy
! Component: 1300  -  total flux cleaned = -0.00700706 Jy
! Component: 1350  -  total flux cleaned = -0.00693013 Jy
! Component: 1400  -  total flux cleaned = -0.00680375 Jy
! Component: 1450  -  total flux cleaned = -0.00667973 Jy
! Component: 1500  -  total flux cleaned = -0.00658136 Jy
! Component: 1550  -  total flux cleaned = -0.00648406 Jy
! Component: 1600  -  total flux cleaned = -0.00641214 Jy
! Component: 1650  -  total flux cleaned = -0.00617549 Jy
! Component: 1700  -  total flux cleaned = -0.00608224 Jy
! Component: 1750  -  total flux cleaned = -0.0059899 Jy
! Component: 1800  -  total flux cleaned = -0.00580715 Jy
! Component: 1850  -  total flux cleaned = -0.00571709 Jy
! Component: 1900  -  total flux cleaned = -0.00562769 Jy
! Component: 1950  -  total flux cleaned = -0.00547319 Jy
! Component: 2000  -  total flux cleaned = -0.00536412 Jy
! Total flux subtracted in 2048 components = -0.00527799 Jy
! Clean residual min=-0.001341 max=0.001099 Jy/beam
! Clean residual mean=0.000001 rms=0.000395 Jy/beam
! Combined flux in latest and established models = 0.26672 Jy
keep
! Adding 145 model components to the UV plane model.
! The established model now contains 195 components and 0.26672 Jy
![Exited script file: muppet]
wmap "J0206-1150_X_2007_01_11_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7853 x 2.022 at 0.06673 degrees (North through East)
! Clean map  min=-0.0026146  max=0.24747 Jy/beam
! Writing clean map to FITS file: J0206-1150_X_2007_01_11_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.247474 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.432% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000392165 
device "J0206-1150_X_2007_01_11_yyk\_map.eps/VPS"
! Attempting to open device: 'J0206-1150_X_2007_01_11_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.475401 0.475401 0.950802 1.9016 3.80321 7.60642 15.2128 30.4257 60.8513
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0011 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.247 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7853 x 2.022 at 0.06673 degrees (North through East)
! Clean map  min=-0.0026146  max=0.24747 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0206-1150_X_2007_01_11_yyk\_map.gif/gif"
! Attempting to open device: 'J0206-1150_X_2007_01_11_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J0206-1150_X_2007_01_11_yyk_uvs.log closed on Mon Jun 16 19:07:50 2008