! Started logfile: J0725-2640_X_2005_07_20_yyk_uvs.log on Fri Jan 20 10:04:30 2006
obs J0725-2640_X_2005_07_20_yyk_uve.fits
! Reading UV FITS file: J0725-2640_X_2005_07_20_yyk_uve.fits
! AN table 1: 10 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.833333 visibilities/baseline/integration-bin.
! Found source: J0725-2640
! 
! 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 1488 lines of history.
! 
! Reading 1500 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 J0725-2640_X_2005_07_20_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)= 0.312208 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 0.339% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.6827 mas, bmaj=1.772 mas, bpa=-4.325 degrees
! Estimated noise=1.55254 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 = 0.250727 Jy
! Component: 100  -  total flux cleaned = 0.30991 Jy
! Total flux subtracted in 100 components = 0.30991 Jy
! Clean residual min=-0.011045 max=0.019125 Jy/beam
! Clean residual mean=-0.000006 rms=0.003438 Jy/beam
! Combined flux in latest and established models = 0.30991 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 10 model components to the UV plane model.
! The established model now contains 10 components and 0.30991 Jy
! 
! Correcting IF 1.
!  A total of 10 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 10 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 10 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 11 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.086129Jy  sigma=1.330457
! Fit after  self-cal, rms=0.085757Jy  sigma=1.325104
! Inverting map and beam 
! Your choice of large map pixels excluded 0.339% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.6825 mas, bmaj=1.772 mas, bpa=-4.338 degrees
! Estimated noise=1.55313 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 0.339% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8115 mas, bmaj=2.102 mas, bpa=-1.885 degrees
! Estimated noise=1.12441 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 = 0.0307765 Jy
! Component: 100  -  total flux cleaned = 0.0417299 Jy
! Component: 150  -  total flux cleaned = 0.0463501 Jy
! Component: 200  -  total flux cleaned = 0.0468175 Jy
! Total flux subtracted in 200 components = 0.0468175 Jy
! Clean residual min=-0.007747 max=0.013008 Jy/beam
! Clean residual mean=0.000191 rms=0.003044 Jy/beam
! Combined flux in latest and established models = 0.356728 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 14 model components to the UV plane model.
! The established model now contains 20 components and 0.356728 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.079605Jy  sigma=1.198095
! Fit after  self-cal, rms=0.079581Jy  sigma=1.197986
! Inverting map 
! Your choice of large map pixels excluded 0.339% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8115 x 2.102 at -1.885 degrees (North through East)
! Clean map  min=-0.0074963  max=0.29577 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: 1.00144
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.90     FD        0.97     HN        1.13     KP        0.93     
!   LA        0.98     MK        0.97     NL        1.01     OV        1.00     
!   PT        1.13     SC        0.98     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 0.991674
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.96     FD        0.95     HN        1.24     KP        0.89     
!   LA        0.94     MK        0.97     NL        0.96     OV        1.01     
!   PT        1.22     SC        0.94     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 0.989817
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.01     FD        0.97     HN        1.05     KP        0.83     
!   LA        0.97     MK        1.08     NL        1.01     OV        1.00     
!   PT        1.25     SC        0.93     
! 
! 
! Correcting IF 4.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Amplitude normalization factor in sub-array 1: 0.93436
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.05     FD        1.00     HN        1.17     KP        0.98     
!   LA        0.98     MK        0.98     NL        1.00     OV        1.02     
!   PT        1.34     SC        1.18     
! 
! 
! Fit before self-cal, rms=0.079581Jy  sigma=1.197986
! Fit after  self-cal, rms=0.071270Jy  sigma=1.054160
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=0.071270Jy  sigma=1.054160
! Fit after  self-cal, rms=0.071286Jy  sigma=1.054074
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8161 mas, bmaj=2.093 mas, bpa=-1.496 degrees
! Estimated noise=1.07959 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 = -0.00957649 Jy
! Component: 100  -  total flux cleaned = -0.0120057 Jy
! Component: 150  -  total flux cleaned = -0.0128783 Jy
! Component: 200  -  total flux cleaned = -0.0130525 Jy
! Total flux subtracted in 200 components = -0.0130525 Jy
! Clean residual min=-0.004521 max=0.004453 Jy/beam
! Clean residual mean=0.000005 rms=0.001155 Jy/beam
! Combined flux in latest and established models = 0.343675 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 11 model components to the UV plane model.
! The established model now contains 29 components and 0.343675 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.070036Jy  sigma=1.036686
! Fit after  self-cal, rms=0.070028Jy  sigma=1.036648
! Inverting map 
! Your choice of large map pixels excluded 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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=0.070028Jy  sigma=1.036648
! Fit after  self-cal, rms=0.066950Jy  sigma=0.992725
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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 = 0.000312125 Jy
! Component: 100  -  total flux cleaned = 0.000312285 Jy
! Component: 150  -  total flux cleaned = 0.000284634 Jy
! Component: 200  -  total flux cleaned = 0.000258694 Jy
! Total flux subtracted in 200 components = 0.000258694 Jy
! Clean residual min=-0.004515 max=0.004604 Jy/beam
! Clean residual mean=0.000005 rms=0.001152 Jy/beam
! Combined flux in latest and established models = 0.343934 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 12 model components to the UV plane model.
! The established model now contains 34 components and 0.343934 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066952Jy  sigma=0.992329
! Fit after  self-cal, rms=0.066599Jy  sigma=0.989072
! Inverting map 
! Your choice of large map pixels excluded 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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: 0.8161 x 2.093 at -1.496 degrees (North through East)
! Clean map  min=-0.0041198  max=0.28817 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=0.066599Jy  sigma=0.989072
! Fit after  self-cal, rms=0.065363Jy  sigma=0.941442
! 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=0.065363Jy  sigma=0.941442
! Fit after  self-cal, rms=0.065296Jy  sigma=0.940949
! Inverting map and beam 
! Your choice of large map pixels excluded 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8158 mas, bmaj=2.098 mas, bpa=-1.472 degrees
! Estimated noise=1.0774 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -9.18044e-05 Jy
! Component: 100  -  total flux cleaned = -6.31557e-05 Jy
! Component: 150  -  total flux cleaned = -6.40733e-05 Jy
! Component: 200  -  total flux cleaned = -6.48851e-05 Jy
! Total flux subtracted in 200 components = -6.48851e-05 Jy
! Clean residual min=-0.003948 max=0.003814 Jy/beam
! Clean residual mean=-0.000012 rms=0.000986 Jy/beam
! Combined flux in latest and established models = 0.343869 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 38 components and 0.343869 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.065270Jy  sigma=0.940631
! Fit after  self-cal, rms=0.065246Jy  sigma=0.940502
! Inverting map 
! Your choice of large map pixels excluded 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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=0.065246Jy  sigma=0.940502
! Fit after  self-cal, rms=0.063904Jy  sigma=0.912645
! 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=0.063904Jy  sigma=0.912645
! Fit after  self-cal, rms=0.063897Jy  sigma=0.912597
! Inverting map and beam 
! Your choice of large map pixels excluded 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8175 mas, bmaj=2.101 mas, bpa=-1.396 degrees
! Estimated noise=1.07839 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.00012445 Jy
! Component: 100  -  total flux cleaned = -0.000152008 Jy
! Component: 150  -  total flux cleaned = -0.000152155 Jy
! Component: 200  -  total flux cleaned = -0.000177059 Jy
! Total flux subtracted in 200 components = -0.000177059 Jy
! Clean residual min=-0.003991 max=0.003815 Jy/beam
! Clean residual mean=-0.000013 rms=0.000978 Jy/beam
! Combined flux in latest and established models = 0.343692 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 13 model components to the UV plane model.
! The established model now contains 42 components and 0.343692 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.063879Jy  sigma=0.912226
! Fit after  self-cal, rms=0.063875Jy  sigma=0.912205
! Inverting map 
! Your choice of large map pixels excluded 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=2.284 mas, bmaj=5.543 mas, bpa=2.704 degrees
! Estimated noise=1.42556 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 = 0.000550382 Jy
! Component: 100  -  total flux cleaned = 0.000548144 Jy
! Component: 150  -  total flux cleaned = 0.000545077 Jy
! Component: 200  -  total flux cleaned = 0.000540654 Jy
! Total flux subtracted in 200 components = 0.000540654 Jy
! Clean residual min=-0.004754 max=0.003825 Jy/beam
! Clean residual mean=-0.000024 rms=0.001273 Jy/beam
! Combined flux in latest and established models = 0.344233 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 45 components and 0.344233 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.063977Jy  sigma=0.913294
! Fit after  self-cal, rms=0.063910Jy  sigma=0.912569
! Inverting map 
! Your choice of large map pixels excluded 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.687 mas, bmaj=1.772 mas, bpa=-4.244 degrees
! Estimated noise=1.51377 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.244466 Jy
! Component: 100  -  total flux cleaned = 0.300281 Jy
! Component: 150  -  total flux cleaned = 0.323669 Jy
! Component: 200  -  total flux cleaned = 0.333846 Jy
! Total flux subtracted in 200 components = 0.333846 Jy
! Clean residual min=-0.006415 max=0.006128 Jy/beam
! Clean residual mean=-0.000009 rms=0.001452 Jy/beam
! Combined flux in latest and established models = 0.333846 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 12 model components to the UV plane model.
! The established model now contains 12 components and 0.333846 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8175 mas, bmaj=2.101 mas, bpa=-1.396 degrees
! Estimated noise=1.07839 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)
! Added new window around map position (-1.2, -1).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00835918 Jy
! Component: 100  -  total flux cleaned = 0.010517 Jy
! Component: 150  -  total flux cleaned = 0.0111667 Jy
! Component: 200  -  total flux cleaned = 0.0116728 Jy
! Total flux subtracted in 200 components = 0.0116728 Jy
! Clean residual min=-0.003915 max=0.003906 Jy/beam
! Clean residual mean=-0.000010 rms=0.000938 Jy/beam
! Combined flux in latest and established models = 0.345519 Jy
! Adding 17 model components to the UV plane model.
! The established model now contains 28 components and 0.345519 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=2.284 mas, bmaj=5.543 mas, bpa=2.704 degrees
! Estimated noise=1.42556 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 = 0.000387495 Jy
! Component: 100  -  total flux cleaned = 0.000322354 Jy
! Component: 150  -  total flux cleaned = 0.000263197 Jy
! Component: 200  -  total flux cleaned = 0.000178185 Jy
! Total flux subtracted in 200 components = 0.000178185 Jy
! Clean residual min=-0.004382 max=0.004166 Jy/beam
! Clean residual mean=-0.000020 rms=0.001240 Jy/beam
! Combined flux in latest and established models = 0.345697 Jy
! Adding 12 model components to the UV plane model.
! The established model now contains 40 components and 0.345697 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8175 mas, bmaj=2.101 mas, bpa=-1.396 degrees
! Estimated noise=1.07839 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.000364707 Jy
! Component: 100  -  total flux cleaned = -0.000364079 Jy
! Component: 150  -  total flux cleaned = -0.000365225 Jy
! Component: 200  -  total flux cleaned = -0.000411863 Jy
! Total flux subtracted in 200 components = -0.000411863 Jy
! Clean residual min=-0.003707 max=0.003882 Jy/beam
! Clean residual mean=-0.000010 rms=0.000922 Jy/beam
! Combined flux in latest and established models = 0.345285 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 22 model components to the UV plane model.
! The established model now contains 57 components and 0.345285 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.063558Jy  sigma=0.908403
! Fit after  self-cal, rms=0.063495Jy  sigma=0.907929
wmodel J0725-2640_X_2005_07_20_yyk\_map.mod
! Writing 57 model components to file: J0725-2640_X_2005_07_20_yyk_map.mod
wobs J0725-2640_X_2005_07_20_yyk\_uvs.fits
! Writing UV FITS file: J0725-2640_X_2005_07_20_yyk_uvs.fits
wwins J0725-2640_X_2005_07_20_yyk\_map.win
! wwins: Wrote 2 windows to J0725-2640_X_2005_07_20_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 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00025375 Jy
! Component: 100  -  total flux cleaned = -0.00103953 Jy
! Component: 150  -  total flux cleaned = -0.00171635 Jy
! Component: 200  -  total flux cleaned = -0.00219884 Jy
! Component: 250  -  total flux cleaned = -0.00281416 Jy
! Component: 300  -  total flux cleaned = -0.00325638 Jy
! Component: 350  -  total flux cleaned = -0.00349495 Jy
! Component: 400  -  total flux cleaned = -0.00368037 Jy
! Component: 450  -  total flux cleaned = -0.00372619 Jy
! Component: 500  -  total flux cleaned = -0.00377073 Jy
! Component: 550  -  total flux cleaned = -0.00377111 Jy
! Component: 600  -  total flux cleaned = -0.00389602 Jy
! Component: 650  -  total flux cleaned = -0.00401792 Jy
! Component: 700  -  total flux cleaned = -0.00401724 Jy
! Component: 750  -  total flux cleaned = -0.00413446 Jy
! Component: 800  -  total flux cleaned = -0.00409554 Jy
! Component: 850  -  total flux cleaned = -0.00417113 Jy
! Component: 900  -  total flux cleaned = -0.00435571 Jy
! Component: 950  -  total flux cleaned = -0.00446372 Jy
! Component: 1000  -  total flux cleaned = -0.00442718 Jy
! Component: 1050  -  total flux cleaned = -0.00449792 Jy
! Component: 1100  -  total flux cleaned = -0.00456753 Jy
! Component: 1150  -  total flux cleaned = -0.00466993 Jy
! Component: 1200  -  total flux cleaned = -0.00477017 Jy
! Component: 1250  -  total flux cleaned = -0.00483596 Jy
! Component: 1300  -  total flux cleaned = -0.00499824 Jy
! Component: 1350  -  total flux cleaned = -0.00499775 Jy
! Component: 1400  -  total flux cleaned = -0.00502927 Jy
! Component: 1450  -  total flux cleaned = -0.00499849 Jy
! Component: 1500  -  total flux cleaned = -0.00496826 Jy
! Component: 1550  -  total flux cleaned = -0.00499809 Jy
! Component: 1600  -  total flux cleaned = -0.00487818 Jy
! Component: 1650  -  total flux cleaned = -0.00478942 Jy
! Component: 1700  -  total flux cleaned = -0.00478901 Jy
! Component: 1750  -  total flux cleaned = -0.00470301 Jy
! Component: 1800  -  total flux cleaned = -0.00467471 Jy
! Component: 1850  -  total flux cleaned = -0.00464688 Jy
! Component: 1900  -  total flux cleaned = -0.00467469 Jy
! Component: 1950  -  total flux cleaned = -0.0045646 Jy
! Component: 2000  -  total flux cleaned = -0.00459141 Jy
! Total flux subtracted in 2048 components = -0.00464522 Jy
! Clean residual min=-0.001393 max=0.001497 Jy/beam
! Clean residual mean=-0.000004 rms=0.000500 Jy/beam
! Combined flux in latest and established models = 0.34064 Jy
keep
! Adding 143 model components to the UV plane model.
! The established model now contains 200 components and 0.34064 Jy
![Exited script file: muppet]
wmap "J0725-2640_X_2005_07_20_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8175 x 2.101 at -1.396 degrees (North through East)
! Clean map  min=-0.0025901  max=0.28863 Jy/beam
! Writing clean map to FITS file: J0725-2640_X_2005_07_20_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.288633 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.272% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000496955 
device "J0725-2640_X_2005_07_20_yyk\_map.eps/VPS"
! Attempting to open device: 'J0725-2640_X_2005_07_20_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.516527 0.516527 1.03305 2.06611 4.13222 8.26443 16.5289 33.0577 66.1155
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0014 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.288 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8175 x 2.101 at -1.396 degrees (North through East)
! Clean map  min=-0.0025901  max=0.28863 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0725-2640_X_2005_07_20_yyk\_map.gif/gif"
! Attempting to open device: 'J0725-2640_X_2005_07_20_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J0725-2640_X_2005_07_20_yyk_uvs.log closed on Fri Jan 20 10:04:34 2006