! Started logfile: J1325-4301_X_2002_05_14_yyk_uvs.log on Tue Jun 26 22:50:31 2007
obs J1325-4301_X_2002_05_14_yyk_uva.fits
! Reading UV FITS file: J1325-4301_X_2002_05_14_yyk_uva.fits
! AN table 1: 35 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.608889 visibilities/baseline/integration-bin.
! Found source: J1325-4301
! 
! 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  8.40947e+09        8e+06          1        8e+06
!  02        2  8.47947e+09        8e+06          1        8e+06
!  03        3  8.79447e+09        8e+06          1        8e+06
!  04        4  8.89947e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 1076 lines of history.
! 
! Reading 3836 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 J1325-4301_X_2002_05_14_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)= 1.81151 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 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.6449 mas, bmaj=1.801 mas, bpa=-1.129 degrees
! Estimated noise=3320.21 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=100  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 1.09178 Jy
! Component: 100  -  total flux cleaned = 1.71088 Jy
! Total flux subtracted in 100 components = 1.71088 Jy
! Clean residual min=-0.165971 max=0.257201 Jy/beam
! Clean residual mean=-0.002647 rms=0.070374 Jy/beam
! Combined flux in latest and established models = 1.71088 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 62 model components to the UV plane model.
! The established model now contains 62 components and 1.71088 Jy
! 
! Correcting IF 1.
!  A total of 73 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 73 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 73 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 73 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.967650Jy  sigma=0.006252
! Fit after  self-cal, rms=0.967198Jy  sigma=0.006250
! Inverting map and beam 
! Your choice of large map pixels excluded 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.6449 mas, bmaj=1.801 mas, bpa=-1.129 degrees
! Estimated noise=3320.21 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 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.7791 mas, bmaj=2.142 mas, bpa=0.2921 degrees
! Estimated noise=1893.4 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 = 0.704054 Jy
! Component: 100  -  total flux cleaned = 1.11522 Jy
! Component: 150  -  total flux cleaned = 1.28201 Jy
! Component: 200  -  total flux cleaned = 1.35137 Jy
! Total flux subtracted in 200 components = 1.35137 Jy
! Clean residual min=-0.097780 max=0.097341 Jy/beam
! Clean residual mean=0.000953 rms=0.048337 Jy/beam
! Combined flux in latest and established models = 3.06225 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 138 model components to the UV plane model.
! The established model now contains 188 components and 3.06225 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.520057Jy  sigma=0.003229
! Fit after  self-cal, rms=0.518384Jy  sigma=0.003222
! Inverting map 
! Your choice of large map pixels excluded 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7791 x 2.142 at 0.2921 degrees (North through East)
! Clean map  min=-0.12316  max=0.59183 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: 0.947034
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.90     HN        1.00*    KP        0.90     
!   LA        0.95     NL        1.63     OV        1.06     PT        1.02     
!   SC        1.06     MK        1.03     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 0.975232
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.90     HN        1.00*    KP        0.87     
!   LA        0.91     NL        1.54     OV        1.01     PT        1.05     
!   SC        0.99     MK        0.99     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 0.985402
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.83     HN        1.00*    KP        0.85     
!   LA        0.91     NL        1.51     OV        1.00     PT        1.01     
!   SC        1.01     MK        1.02     
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 0.955081
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.83     HN        1.00*    KP        0.93     
!   LA        0.88     NL        1.46     OV        1.00     PT        1.08     
!   SC        0.97     MK        1.31     
! 
! 
! Fit before self-cal, rms=0.518384Jy  sigma=0.003222
! Fit after  self-cal, rms=0.408354Jy  sigma=0.002837
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=0.408354Jy  sigma=0.002837
! Fit after  self-cal, rms=0.408210Jy  sigma=0.002835
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.8126 mas, bmaj=2.208 mas, bpa=1.577 degrees
! Estimated noise=1731.08 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 = 0.042355 Jy
! Component: 100  -  total flux cleaned = 0.120098 Jy
! Component: 150  -  total flux cleaned = 0.169031 Jy
! Component: 200  -  total flux cleaned = 0.204495 Jy
! Total flux subtracted in 200 components = 0.204495 Jy
! Clean residual min=-0.033776 max=0.034093 Jy/beam
! Clean residual mean=0.001342 rms=0.018741 Jy/beam
! Combined flux in latest and established models = 3.26675 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 125 model components to the UV plane model.
! The established model now contains 311 components and 3.26675 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.359277Jy  sigma=0.002424
! Fit after  self-cal, rms=0.358836Jy  sigma=0.002423
! Inverting map 
! Your choice of large map pixels excluded 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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=0.358836Jy  sigma=0.002423
! Fit after  self-cal, rms=0.305629Jy  sigma=0.001906
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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 = 0.0410434 Jy
! Component: 100  -  total flux cleaned = 0.0703448 Jy
! Component: 150  -  total flux cleaned = 0.0848308 Jy
! Component: 200  -  total flux cleaned = 0.0992603 Jy
! Total flux subtracted in 200 components = 0.0992603 Jy
! Clean residual min=-0.018893 max=0.018897 Jy/beam
! Clean residual mean=0.000323 rms=0.010744 Jy/beam
! Combined flux in latest and established models = 3.36601 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 110 model components to the UV plane model.
! The established model now contains 413 components and 3.36601 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.292469Jy  sigma=0.001790
! Fit after  self-cal, rms=0.283255Jy  sigma=0.001693
! Inverting map 
! Your choice of large map pixels excluded 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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: 0.8126 x 2.208 at 1.577 degrees (North through East)
! Clean map  min=-0.040022  max=0.48484 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=0.283255Jy  sigma=0.001693
! Fit after  self-cal, rms=0.279006Jy  sigma=0.001645
! 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=0.279006Jy  sigma=0.001645
! Fit after  self-cal, rms=0.276742Jy  sigma=0.001622
! Inverting map and beam 
! Your choice of large map pixels excluded 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.7933 mas, bmaj=2.168 mas, bpa=1.535 degrees
! Estimated noise=1722.64 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.0131947 Jy
! Component: 100  -  total flux cleaned = -0.0169611 Jy
! Component: 150  -  total flux cleaned = -0.0149196 Jy
! Component: 200  -  total flux cleaned = -0.00930687 Jy
! Total flux subtracted in 200 components = -0.00930687 Jy
! Clean residual min=-0.010849 max=0.010885 Jy/beam
! Clean residual mean=0.000006 rms=0.005991 Jy/beam
! Combined flux in latest and established models = 3.3567 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 112 model components to the UV plane model.
! The established model now contains 514 components and 3.3567 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.271462Jy  sigma=0.001576
! Fit after  self-cal, rms=0.270565Jy  sigma=0.001568
! Inverting map 
! Your choice of large map pixels excluded 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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=0.270565Jy  sigma=0.001568
! Fit after  self-cal, rms=0.269417Jy  sigma=0.001564
! 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=0.269417Jy  sigma=0.001564
! Fit after  self-cal, rms=0.269155Jy  sigma=0.001561
! Inverting map and beam 
! Your choice of large map pixels excluded 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.7874 mas, bmaj=2.153 mas, bpa=1.595 degrees
! Estimated noise=1716.74 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00254616 Jy
! Component: 100  -  total flux cleaned = 0.00027456 Jy
! Component: 150  -  total flux cleaned = 0.00276715 Jy
! Component: 200  -  total flux cleaned = 0.00666124 Jy
! Total flux subtracted in 200 components = 0.00666124 Jy
! Clean residual min=-0.006523 max=0.006557 Jy/beam
! Clean residual mean=-0.000004 rms=0.003524 Jy/beam
! Combined flux in latest and established models = 3.36336 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 101 model components to the UV plane model.
! The established model now contains 575 components and 3.36336 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.267168Jy  sigma=0.001545
! Fit after  self-cal, rms=0.267033Jy  sigma=0.001544
! Inverting map 
! Your choice of large map pixels excluded 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=2.949 mas, bmaj=11.18 mas, bpa=4.23 degrees
! Estimated noise=2291.33 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 = 0.0160642 Jy
! Component: 100  -  total flux cleaned = 0.0237933 Jy
! Component: 150  -  total flux cleaned = 0.0266749 Jy
! Component: 200  -  total flux cleaned = 0.0277334 Jy
! Total flux subtracted in 200 components = 0.0277334 Jy
! Clean residual min=-0.006365 max=0.006395 Jy/beam
! Clean residual mean=0.000037 rms=0.003062 Jy/beam
! Combined flux in latest and established models = 3.39109 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 67 model components to the UV plane model.
! The established model now contains 630 components and 3.39109 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.266193Jy  sigma=0.001538
! Fit after  self-cal, rms=0.266139Jy  sigma=0.001538
! Inverting map 
! Your choice of large map pixels excluded 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.6507 mas, bmaj=1.794 mas, bpa=0.3578 degrees
! Estimated noise=3154.29 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 1.04065 Jy
! Component: 100  -  total flux cleaned = 1.58819 Jy
! Component: 150  -  total flux cleaned = 1.94659 Jy
! Component: 200  -  total flux cleaned = 2.20245 Jy
! Total flux subtracted in 200 components = 2.20245 Jy
! Clean residual min=-0.090748 max=0.107661 Jy/beam
! Clean residual mean=-0.000352 rms=0.033769 Jy/beam
! Combined flux in latest and established models = 2.20245 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 83 model components to the UV plane model.
! The established model now contains 83 components and 2.20245 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.7874 mas, bmaj=2.153 mas, bpa=1.595 degrees
! Estimated noise=1716.74 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 = 0.288962 Jy
! Component: 100  -  total flux cleaned = 0.347576 Jy
! Component: 150  -  total flux cleaned = 0.373267 Jy
! Component: 200  -  total flux cleaned = 0.398372 Jy
! Total flux subtracted in 200 components = 0.398373 Jy
! Clean residual min=-0.058178 max=0.058767 Jy/beam
! Clean residual mean=0.000752 rms=0.031417 Jy/beam
! Combined flux in latest and established models = 2.60083 Jy
! Adding 156 model components to the UV plane model.
! The established model now contains 224 components and 2.60083 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=2.949 mas, bmaj=11.18 mas, bpa=4.23 degrees
! Estimated noise=2291.33 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 = -0.0133541 Jy
! Component: 100  -  total flux cleaned = -0.00796473 Jy
! Component: 150  -  total flux cleaned = 0.0255978 Jy
! Component: 200  -  total flux cleaned = 0.038746 Jy
! Total flux subtracted in 200 components = 0.038746 Jy
! Clean residual min=-0.035887 max=0.035885 Jy/beam
! Clean residual mean=0.000348 rms=0.021112 Jy/beam
! Combined flux in latest and established models = 2.63957 Jy
! Adding 122 model components to the UV plane model.
! The established model now contains 332 components and 2.63957 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.7874 mas, bmaj=2.153 mas, bpa=1.595 degrees
! Estimated noise=1716.74 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.028275 Jy
! Component: 100  -  total flux cleaned = 0.0271324 Jy
! Component: 150  -  total flux cleaned = 0.0311454 Jy
! Component: 200  -  total flux cleaned = 0.0300418 Jy
! Total flux subtracted in 200 components = 0.0300418 Jy
! Clean residual min=-0.013605 max=0.013606 Jy/beam
! Clean residual mean=0.000121 rms=0.006628 Jy/beam
! Combined flux in latest and established models = 2.66961 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 58 model components to the UV plane model.
! The established model now contains 387 components and 2.66961 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.275998Jy  sigma=0.001587
! Fit after  self-cal, rms=0.275002Jy  sigma=0.001583
wmodel J1325-4301_X_2002_05_14_yyk\_map.mod
! Writing 387 model components to file: J1325-4301_X_2002_05_14_yyk_map.mod
wobs J1325-4301_X_2002_05_14_yyk\_uvs.fits
! Writing UV FITS file: J1325-4301_X_2002_05_14_yyk_uvs.fits
wwins J1325-4301_X_2002_05_14_yyk\_map.win
! wwins: No CLEAN windows to write.
! Error occured in command: wwins
![Exited script file: muppet]
! 
wmap "J1325-4301_X_2002_05_14_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7874 x 2.153 at 1.595 degrees (North through East)
! Clean map  min=-0.05633  max=0.52322 Jy/beam
! Writing clean map to FITS file: J1325-4301_X_2002_05_14_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.523221 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.912% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.00637161 
device "J1325-4301_X_2002_05_14_yyk\_map.eps/VPS"
! Attempting to open device: 'J1325-4301_X_2002_05_14_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -3.6533 3.6533 7.3066 14.6132 29.2264 58.4528
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0191 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.523 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7874 x 2.153 at 1.595 degrees (North through East)
! Clean map  min=-0.05633  max=0.52322 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1325-4301_X_2002_05_14_yyk\_map.gif/gif"
! Attempting to open device: 'J1325-4301_X_2002_05_14_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1325-4301_X_2002_05_14_yyk_uvs.log closed on Tue Jun 26 22:50:37 2007