! Started logfile: J1325-4301_X_2002_01_31_yyk_uvs.log on Wed Jun 27 10:57:57 2007
obs J1325-4301_X_2002_01_31_yyk_uva.fits
! Reading UV FITS file: J1325-4301_X_2002_01_31_yyk_uva.fits
! AN table 1: 33 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.589899 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 1544 lines of history.
! 
! Reading 3504 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
flag NL
! Flagging baselines of antenna 1:NL in the currently selected channels.
![@muppet J1325-4301_X_2002_01_31_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)= 1.60367 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 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.6578 mas, bmaj=1.766 mas, bpa=2.051 degrees
! Estimated noise=2820.9 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 = 1.02562 Jy
! Component: 100  -  total flux cleaned = 1.52558 Jy
! Total flux subtracted in 100 components = 1.52558 Jy
! Clean residual min=-0.107539 max=0.174619 Jy/beam
! Clean residual mean=-0.000694 rms=0.047926 Jy/beam
! Combined flux in latest and established models = 1.52558 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 31 model components to the UV plane model.
! The established model now contains 31 components and 1.52558 Jy
! 
! Correcting IF 1.
!  A total of 106 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 106 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 106 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 106 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.701211Jy  sigma=0.005176
! Fit after  self-cal, rms=0.694688Jy  sigma=0.005136
! Inverting map and beam 
! Your choice of large map pixels excluded 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.6578 mas, bmaj=1.766 mas, bpa=2.051 degrees
! Estimated noise=2820.9 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 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.7584 mas, bmaj=2.081 mas, bpa=1.554 degrees
! Estimated noise=1909.45 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 = 0.479533 Jy
! Component: 100  -  total flux cleaned = 0.733478 Jy
! Component: 150  -  total flux cleaned = 0.780807 Jy
! Component: 200  -  total flux cleaned = 0.805507 Jy
! Total flux subtracted in 200 components = 0.805507 Jy
! Clean residual min=-0.069422 max=0.069438 Jy/beam
! Clean residual mean=0.001482 rms=0.035530 Jy/beam
! Combined flux in latest and established models = 2.33108 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 134 model components to the UV plane model.
! The established model now contains 159 components and 2.33108 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.367527Jy  sigma=0.002588
! Fit after  self-cal, rms=0.365859Jy  sigma=0.002578
! Inverting map 
! Your choice of large map pixels excluded 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7584 x 2.081 at 1.554 degrees (North through East)
! Clean map  min=-0.10294  max=0.98978 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: 0.996923
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.91     HN        1.00*    KP        0.96     
!   LA        1.01     MK        1.05     NL        1.00*    OV        1.08     
!   PT        0.99     SC        1.03     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.0178
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.91     HN        1.00*    KP        0.90     
!   LA        0.97     MK        1.00     NL        1.00*    OV        1.04     
!   PT        1.03     SC        0.98     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 1.01835
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.83     HN        1.00*    KP        0.87     
!   LA        0.99     MK        1.01     NL        1.00*    OV        1.03     
!   PT        1.02     SC        1.07     
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 1.01646
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.82     HN        1.00*    KP        0.94     
!   LA        0.98     MK        0.97     NL        1.00*    OV        1.02     
!   PT        1.05     SC        1.06     
! 
! 
! Fit before self-cal, rms=0.365859Jy  sigma=0.002578
! Fit after  self-cal, rms=0.306831Jy  sigma=0.002220
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=0.306831Jy  sigma=0.002220
! Fit after  self-cal, rms=0.306791Jy  sigma=0.002220
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.7858 mas, bmaj=2.152 mas, bpa=0.9448 degrees
! Estimated noise=1876.92 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 = 0.0292123 Jy
! Component: 100  -  total flux cleaned = 0.0410007 Jy
! Component: 150  -  total flux cleaned = 0.0457637 Jy
! Component: 200  -  total flux cleaned = 0.0402653 Jy
! Total flux subtracted in 200 components = 0.0402653 Jy
! Clean residual min=-0.020634 max=0.020561 Jy/beam
! Clean residual mean=0.000209 rms=0.011331 Jy/beam
! Combined flux in latest and established models = 2.37135 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 130 model components to the UV plane model.
! The established model now contains 289 components and 2.37135 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.278852Jy  sigma=0.001964
! Fit after  self-cal, rms=0.278531Jy  sigma=0.001962
! Inverting map 
! Your choice of large map pixels excluded 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 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=0.278531Jy  sigma=0.001962
! Fit after  self-cal, rms=0.267191Jy  sigma=0.001868
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 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 = -0.00136909 Jy
! Component: 100  -  total flux cleaned = -0.0106283 Jy
! Component: 150  -  total flux cleaned = -0.0163038 Jy
! Component: 200  -  total flux cleaned = -0.0212768 Jy
! Total flux subtracted in 200 components = -0.0212768 Jy
! Clean residual min=-0.011630 max=0.011542 Jy/beam
! Clean residual mean=0.000007 rms=0.006357 Jy/beam
! Combined flux in latest and established models = 2.35007 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 98 model components to the UV plane model.
! The established model now contains 380 components and 2.35007 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.260238Jy  sigma=0.001805
! Fit after  self-cal, rms=0.258425Jy  sigma=0.001789
! Inverting map 
! Your choice of large map pixels excluded 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 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: 0.7858 x 2.152 at 0.9448 degrees (North through East)
! Clean map  min=-0.050918  max=0.96031 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=0.258425Jy  sigma=0.001789
! Fit after  self-cal, rms=0.251084Jy  sigma=0.001769
! 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=0.251084Jy  sigma=0.001769
! Fit after  self-cal, rms=0.246628Jy  sigma=0.001742
! Inverting map and beam 
! Your choice of large map pixels excluded 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.782 mas, bmaj=2.145 mas, bpa=1.605 degrees
! Estimated noise=1853.03 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0126206 Jy
! Component: 100  -  total flux cleaned = 0.0202232 Jy
! Component: 150  -  total flux cleaned = 0.0241684 Jy
! Component: 200  -  total flux cleaned = 0.0258581 Jy
! Total flux subtracted in 200 components = 0.0258581 Jy
! Clean residual min=-0.006571 max=0.006585 Jy/beam
! Clean residual mean=0.000066 rms=0.003224 Jy/beam
! Combined flux in latest and established models = 2.37593 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 73 model components to the UV plane model.
! The established model now contains 449 components and 2.37593 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.244227Jy  sigma=0.001720
! Fit after  self-cal, rms=0.245048Jy  sigma=0.001727
! Inverting map 
! Your choice of large map pixels excluded 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 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=0.245048Jy  sigma=0.001727
! Fit after  self-cal, rms=1.459512Jy  sigma=0.001703
! 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=1.459512Jy  sigma=0.001703
! Fit after  self-cal, rms=1.477433Jy  sigma=0.001708
! Inverting map and beam 
! Your choice of large map pixels excluded 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.8163 mas, bmaj=2.24 mas, bpa=-1.047 degrees
! Estimated noise=1902.44 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00252476 Jy
! Component: 100  -  total flux cleaned = 0.00497113 Jy
! Component: 150  -  total flux cleaned = 0.0059612 Jy
! Component: 200  -  total flux cleaned = 0.00858078 Jy
! Total flux subtracted in 200 components = 0.00858078 Jy
! Clean residual min=-0.005095 max=0.005095 Jy/beam
! Clean residual mean=0.000028 rms=0.002284 Jy/beam
! Combined flux in latest and established models = 2.38451 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 59 model components to the UV plane model.
! The established model now contains 502 components and 2.38451 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=1.477154Jy  sigma=0.001695
! Fit after  self-cal, rms=1.467672Jy  sigma=0.001694
! Inverting map 
! Your choice of large map pixels excluded 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 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 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=3.094 mas, bmaj=11.71 mas, bpa=4.624 degrees
! Estimated noise=2488.75 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 = 0.00675782 Jy
! Component: 100  -  total flux cleaned = 0.0109459 Jy
! Component: 150  -  total flux cleaned = 0.0121976 Jy
! Component: 200  -  total flux cleaned = 0.0146976 Jy
! Total flux subtracted in 200 components = 0.0146976 Jy
! Clean residual min=-0.003252 max=0.003334 Jy/beam
! Clean residual mean=0.000020 rms=0.001669 Jy/beam
! Combined flux in latest and established models = 2.39921 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 72 model components to the UV plane model.
! The established model now contains 572 components and 2.39921 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=1.467630Jy  sigma=0.001691
! Fit after  self-cal, rms=1.460332Jy  sigma=0.001689
! Inverting map 
! Your choice of large map pixels excluded 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 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 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.6861 mas, bmaj=1.853 mas, bpa=-1.574 degrees
! Estimated noise=3069.82 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 1.0789 Jy
! Component: 100  -  total flux cleaned = 1.56155 Jy
! Component: 150  -  total flux cleaned = 1.82032 Jy
! Component: 200  -  total flux cleaned = 1.97297 Jy
! Total flux subtracted in 200 components = 1.97297 Jy
! Clean residual min=-0.077360 max=0.078974 Jy/beam
! Clean residual mean=0.000414 rms=0.031396 Jy/beam
! Combined flux in latest and established models = 1.97297 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 56 model components to the UV plane model.
! The established model now contains 56 components and 1.97297 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.8163 mas, bmaj=2.24 mas, bpa=-1.047 degrees
! Estimated noise=1902.44 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 = 0.250939 Jy
! Component: 100  -  total flux cleaned = 0.333025 Jy
! Component: 150  -  total flux cleaned = 0.343525 Jy
! Component: 200  -  total flux cleaned = 0.32797 Jy
! Total flux subtracted in 200 components = 0.32797 Jy
! Clean residual min=-0.044093 max=0.044348 Jy/beam
! Clean residual mean=0.000483 rms=0.023389 Jy/beam
! Combined flux in latest and established models = 2.30094 Jy
! Adding 138 model components to the UV plane model.
! The established model now contains 192 components and 2.30094 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 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 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=3.094 mas, bmaj=11.71 mas, bpa=4.624 degrees
! Estimated noise=2488.75 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 = -0.0664294 Jy
! Component: 100  -  total flux cleaned = -0.0776836 Jy
! Component: 150  -  total flux cleaned = -0.069325 Jy
! Component: 200  -  total flux cleaned = -0.0544866 Jy
! Total flux subtracted in 200 components = -0.0544866 Jy
! Clean residual min=-0.030544 max=0.030406 Jy/beam
! Clean residual mean=0.000070 rms=0.014361 Jy/beam
! Combined flux in latest and established models = 2.24645 Jy
! Adding 104 model components to the UV plane model.
! The established model now contains 290 components and 2.24645 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.8163 mas, bmaj=2.24 mas, bpa=-1.047 degrees
! Estimated noise=1902.44 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.00867896 Jy
! Component: 100  -  total flux cleaned = -0.00304213 Jy
! Component: 150  -  total flux cleaned = 0.00448324 Jy
! Component: 200  -  total flux cleaned = 0.0109863 Jy
! Total flux subtracted in 200 components = 0.0109863 Jy
! Clean residual min=-0.009339 max=0.009386 Jy/beam
! Clean residual mean=0.000012 rms=0.004515 Jy/beam
! Combined flux in latest and established models = 2.25744 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 54 model components to the UV plane model.
! The established model now contains 343 components and 2.25744 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=1.458788Jy  sigma=0.001715
! Fit after  self-cal, rms=1.463010Jy  sigma=0.001715
wmodel J1325-4301_X_2002_01_31_yyk\_map.mod
! Writing 343 model components to file: J1325-4301_X_2002_01_31_yyk_map.mod
wobs J1325-4301_X_2002_01_31_yyk\_uvs.fits
! Applying 33 buffered edits.
! Writing UV FITS file: J1325-4301_X_2002_01_31_yyk_uvs.fits
wwins J1325-4301_X_2002_01_31_yyk\_map.win
! wwins: No CLEAN windows to write.
! Error occured in command: wwins
![Exited script file: muppet]
! 
wmap "J1325-4301_X_2002_01_31_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8163 x 2.24 at -1.047 degrees (North through East)
! Clean map  min=-0.050541  max=0.85325 Jy/beam
! Writing clean map to FITS file: J1325-4301_X_2002_01_31_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.853253 
invert
! Inverting map 
! Your choice of large map pixels excluded 1.27% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.004374 
device "J1325-4301_X_2002_01_31_yyk\_map.eps/VPS"
! Attempting to open device: 'J1325-4301_X_2002_01_31_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -1.53788 1.53788 3.07576 6.15152 12.303 24.6061 49.2122 98.4243
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0131 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.853 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8163 x 2.24 at -1.047 degrees (North through East)
! Clean map  min=-0.050541  max=0.85325 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1325-4301_X_2002_01_31_yyk\_map.gif/gif"
! Attempting to open device: 'J1325-4301_X_2002_01_31_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1325-4301_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 10:58:02 2007