! Started logfile: J1352-2745_X_2005_07_20_yyk_uvs.log on Fri Jan 20 10:32:10 2006
obs J1352-2745_X_2005_07_20_yyk_uve.fits
! Reading UV FITS file: J1352-2745_X_2005_07_20_yyk_uve.fits
! AN table 1: 10 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.864444 visibilities/baseline/integration-bin.
! Found source: J1352-2745
! 
! 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 1556 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 J1352-2745_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)= 0.137582 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 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.684 mas, bmaj=1.813 mas, bpa=-6.194 degrees
! Estimated noise=1.97437 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 = 0.0792952 Jy
! Component: 100  -  total flux cleaned = 0.0992012 Jy
! Total flux subtracted in 100 components = 0.0992012 Jy
! Clean residual min=-0.011476 max=0.013127 Jy/beam
! Clean residual mean=0.000010 rms=0.003043 Jy/beam
! Combined flux in latest and established models = 0.0992012 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 14 model components to the UV plane model.
! The established model now contains 14 components and 0.0992012 Jy
! 
! Correcting IF 1.
!  A total of 12 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 13 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 26 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 12 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.096090Jy  sigma=1.275451
! Fit after  self-cal, rms=0.091591Jy  sigma=1.218261
! Inverting map and beam 
! Your choice of large map pixels excluded 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.6842 mas, bmaj=1.814 mas, bpa=-6.192 degrees
! Estimated noise=1.97364 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 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.877 mas, bmaj=2.384 mas, bpa=-8.46 degrees
! Estimated noise=1.25811 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 = 0.0192817 Jy
! Component: 100  -  total flux cleaned = 0.0232545 Jy
! Component: 150  -  total flux cleaned = 0.0235834 Jy
! Component: 200  -  total flux cleaned = 0.0235807 Jy
! Total flux subtracted in 200 components = 0.0235807 Jy
! Clean residual min=-0.007511 max=0.007875 Jy/beam
! Clean residual mean=0.000101 rms=0.001981 Jy/beam
! Combined flux in latest and established models = 0.122782 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 26 components and 0.122782 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.090391Jy  sigma=1.165757
! Fit after  self-cal, rms=0.090398Jy  sigma=1.165707
! Inverting map 
! Your choice of large map pixels excluded 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.877 x 2.384 at -8.46 degrees (North through East)
! Clean map  min=-0.0070435  max=0.10489 Jy/beam
if(peak(flux) < thresh*2)
  selflims ampcor_selflim
  end if
! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2.
! Selfcal phase corrections will not be limited.
gscale
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Amplitude normalization factor in sub-array 1: 1.01836
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.95     FD        0.94     HN        1.07     KP        0.83     
!   LA        0.98     MK        0.93     NL        1.00     OV        1.09     
!   PT        1.07     SC        0.94     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    OV        1.00*    
!   PT        1.00*    SC        1.00*    
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 0.997708
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.03     FD        1.09     HN        1.00*    KP        0.85     
!   LA        0.95     MK        0.98     NL        1.01     OV        0.94     
!   PT        1.18     SC        1.00*    
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 1
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    OV        1.00*    
!   PT        1.00*    SC        1.00*    
! 
! 
! Fit before self-cal, rms=0.090398Jy  sigma=1.165707
! Fit after  self-cal, rms=0.089680Jy  sigma=1.154453
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=0.089680Jy  sigma=1.154453
! Fit after  self-cal, rms=0.089688Jy  sigma=1.154421
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.8695 mas, bmaj=2.375 mas, bpa=-8.598 degrees
! Estimated noise=1.23559 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 = -0.00103318 Jy
! Component: 100  -  total flux cleaned = -0.00103724 Jy
! Component: 150  -  total flux cleaned = -0.00107199 Jy
! Component: 200  -  total flux cleaned = -0.00110514 Jy
! Total flux subtracted in 200 components = -0.00110514 Jy
! Clean residual min=-0.006394 max=0.006356 Jy/beam
! Clean residual mean=0.000065 rms=0.001722 Jy/beam
! Combined flux in latest and established models = 0.121677 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 12 model components to the UV plane model.
! The established model now contains 35 components and 0.121677 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.089600Jy  sigma=1.153902
! Fit after  self-cal, rms=0.089611Jy  sigma=1.153883
! Inverting map 
! Your choice of large map pixels excluded 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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=0.089611Jy  sigma=1.153883
! Fit after  self-cal, rms=0.079368Jy  sigma=1.045388
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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 = 0.00350808 Jy
! Component: 100  -  total flux cleaned = 0.00376945 Jy
! Component: 150  -  total flux cleaned = 0.00369988 Jy
! Component: 200  -  total flux cleaned = 0.00363657 Jy
! Total flux subtracted in 200 components = 0.00363657 Jy
! Clean residual min=-0.005674 max=0.006165 Jy/beam
! Clean residual mean=0.000067 rms=0.001625 Jy/beam
! Combined flux in latest and established models = 0.125313 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 19 model components to the UV plane model.
! The established model now contains 44 components and 0.125313 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.079358Jy  sigma=1.043125
! Fit after  self-cal, rms=0.077898Jy  sigma=1.033133
! Inverting map 
! Your choice of large map pixels excluded 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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: 0.8695 x 2.375 at -8.598 degrees (North through East)
! Clean map  min=-0.0052796  max=0.10838 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=0.077898Jy  sigma=1.033133
! Fit after  self-cal, rms=0.076989Jy  sigma=1.028841
! 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=0.076989Jy  sigma=1.028841
! Fit after  self-cal, rms=0.076690Jy  sigma=1.027186
! Inverting map and beam 
! Your choice of large map pixels excluded 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.8744 mas, bmaj=2.373 mas, bpa=-7.931 degrees
! Estimated noise=1.22714 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.000515081 Jy
! Component: 100  -  total flux cleaned = -0.000615866 Jy
! Component: 150  -  total flux cleaned = -0.000696436 Jy
! Component: 200  -  total flux cleaned = -0.000720367 Jy
! Total flux subtracted in 200 components = -0.000720367 Jy
! Clean residual min=-0.005444 max=0.006052 Jy/beam
! Clean residual mean=0.000067 rms=0.001572 Jy/beam
! Combined flux in latest and established models = 0.124593 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 50 components and 0.124593 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.076704Jy  sigma=1.026772
! Fit after  self-cal, rms=0.076623Jy  sigma=1.026392
! Inverting map 
! Your choice of large map pixels excluded 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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=0.076623Jy  sigma=1.026392
! Fit after  self-cal, rms=0.077116Jy  sigma=1.030077
! 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=0.077116Jy  sigma=1.030077
! Fit after  self-cal, rms=0.077091Jy  sigma=1.029885
! Inverting map and beam 
! Your choice of large map pixels excluded 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.8823 mas, bmaj=2.359 mas, bpa=-6.731 degrees
! Estimated noise=1.22453 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.000721095 Jy
! Component: 100  -  total flux cleaned = -0.00072145 Jy
! Component: 150  -  total flux cleaned = -0.000789559 Jy
! Component: 200  -  total flux cleaned = -0.000841738 Jy
! Total flux subtracted in 200 components = -0.000841738 Jy
! Clean residual min=-0.005521 max=0.006151 Jy/beam
! Clean residual mean=0.000075 rms=0.001611 Jy/beam
! Combined flux in latest and established models = 0.123751 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 14 model components to the UV plane model.
! The established model now contains 55 components and 0.123751 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.077098Jy  sigma=1.029076
! Fit after  self-cal, rms=0.077092Jy  sigma=1.029021
! Inverting map 
! Your choice of large map pixels excluded 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=2.407 mas, bmaj=6.122 mas, bpa=2.701 degrees
! Estimated noise=1.5496 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 = -0.000209746 Jy
! Component: 100  -  total flux cleaned = -0.000235588 Jy
! Component: 150  -  total flux cleaned = -0.000236781 Jy
! Component: 200  -  total flux cleaned = -0.000259611 Jy
! Total flux subtracted in 200 components = -0.000259611 Jy
! Clean residual min=-0.005200 max=0.006272 Jy/beam
! Clean residual mean=0.000138 rms=0.002015 Jy/beam
! Combined flux in latest and established models = 0.123492 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 4 model components to the UV plane model.
! The established model now contains 56 components and 0.123492 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.077115Jy  sigma=1.029347
! Fit after  self-cal, rms=0.077094Jy  sigma=1.029309
! Inverting map 
! Your choice of large map pixels excluded 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.6872 mas, bmaj=1.808 mas, bpa=-5.3 degrees
! Estimated noise=1.93201 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0897651 Jy
! Component: 100  -  total flux cleaned = 0.109809 Jy
! Component: 150  -  total flux cleaned = 0.117532 Jy
! Component: 200  -  total flux cleaned = 0.119873 Jy
! Total flux subtracted in 200 components = 0.119873 Jy
! Clean residual min=-0.007117 max=0.006978 Jy/beam
! Clean residual mean=0.000020 rms=0.001864 Jy/beam
! Combined flux in latest and established models = 0.119873 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 20 model components to the UV plane model.
! The established model now contains 20 components and 0.119873 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.8823 mas, bmaj=2.359 mas, bpa=-6.731 degrees
! Estimated noise=1.22453 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 = 0.00438262 Jy
! Component: 100  -  total flux cleaned = 0.00451156 Jy
! Component: 150  -  total flux cleaned = 0.00446293 Jy
! Component: 200  -  total flux cleaned = 0.00441788 Jy
! Total flux subtracted in 200 components = 0.00441787 Jy
! Clean residual min=-0.005517 max=0.006103 Jy/beam
! Clean residual mean=0.000076 rms=0.001637 Jy/beam
! Combined flux in latest and established models = 0.124291 Jy
! Adding 17 model components to the UV plane model.
! The established model now contains 33 components and 0.124291 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=2.407 mas, bmaj=6.122 mas, bpa=2.701 degrees
! Estimated noise=1.5496 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 = -0.000521508 Jy
! Component: 100  -  total flux cleaned = -0.000465034 Jy
! Component: 150  -  total flux cleaned = -0.000488107 Jy
! Component: 200  -  total flux cleaned = -0.000532278 Jy
! Total flux subtracted in 200 components = -0.000532278 Jy
! Clean residual min=-0.005194 max=0.006292 Jy/beam
! Clean residual mean=0.000140 rms=0.002018 Jy/beam
! Combined flux in latest and established models = 0.123759 Jy
! Adding 11 model components to the UV plane model.
! The established model now contains 40 components and 0.123759 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.8823 mas, bmaj=2.359 mas, bpa=-6.731 degrees
! Estimated noise=1.22453 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 3.06698e-05 Jy
! Component: 100  -  total flux cleaned = -1.1747e-05 Jy
! Component: 150  -  total flux cleaned = -4.99521e-05 Jy
! Component: 200  -  total flux cleaned = -8.33726e-05 Jy
! Total flux subtracted in 200 components = -8.33726e-05 Jy
! Clean residual min=-0.005531 max=0.006086 Jy/beam
! Clean residual mean=0.000075 rms=0.001623 Jy/beam
! Combined flux in latest and established models = 0.123675 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 19 model components to the UV plane model.
! The established model now contains 48 components and 0.123675 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.077114Jy  sigma=1.029850
! Fit after  self-cal, rms=0.077098Jy  sigma=1.029829
wmodel J1352-2745_X_2005_07_20_yyk\_map.mod
! Writing 48 model components to file: J1352-2745_X_2005_07_20_yyk_map.mod
wobs J1352-2745_X_2005_07_20_yyk\_uvs.fits
! Writing UV FITS file: J1352-2745_X_2005_07_20_yyk_uvs.fits
wwins J1352-2745_X_2005_07_20_yyk\_map.win
! wwins: Wrote 1 windows to J1352-2745_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 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.00179342 Jy
! Component: 100  -  total flux cleaned = 0.00289559 Jy
! Component: 150  -  total flux cleaned = 0.00392896 Jy
! Component: 200  -  total flux cleaned = 0.00455122 Jy
! Component: 250  -  total flux cleaned = 0.0052313 Jy
! Component: 300  -  total flux cleaned = 0.00596055 Jy
! Component: 350  -  total flux cleaned = 0.0065036 Jy
! Component: 400  -  total flux cleaned = 0.00680546 Jy
! Component: 450  -  total flux cleaned = 0.00716705 Jy
! Component: 500  -  total flux cleaned = 0.00765388 Jy
! Component: 550  -  total flux cleaned = 0.00805653 Jy
! Component: 600  -  total flux cleaned = 0.00857785 Jy
! Component: 650  -  total flux cleaned = 0.00920916 Jy
! Component: 700  -  total flux cleaned = 0.00963696 Jy
! Component: 750  -  total flux cleaned = 0.00969483 Jy
! Component: 800  -  total flux cleaned = 0.00986932 Jy
! Component: 850  -  total flux cleaned = 0.0100965 Jy
! Component: 900  -  total flux cleaned = 0.0103156 Jy
! Component: 950  -  total flux cleaned = 0.0104233 Jy
! Component: 1000  -  total flux cleaned = 0.0106869 Jy
! Component: 1050  -  total flux cleaned = 0.0108939 Jy
! Component: 1100  -  total flux cleaned = 0.0107923 Jy
! Component: 1150  -  total flux cleaned = 0.0110904 Jy
! Component: 1200  -  total flux cleaned = 0.0113807 Jy
! Component: 1250  -  total flux cleaned = 0.0115702 Jy
! Component: 1300  -  total flux cleaned = 0.0117569 Jy
! Component: 1350  -  total flux cleaned = 0.0118023 Jy
! Component: 1400  -  total flux cleaned = 0.0119826 Jy
! Component: 1450  -  total flux cleaned = 0.0120275 Jy
! Component: 1500  -  total flux cleaned = 0.0120721 Jy
! Component: 1550  -  total flux cleaned = 0.0124161 Jy
! Component: 1600  -  total flux cleaned = 0.012669 Jy
! Component: 1650  -  total flux cleaned = 0.0129186 Jy
! Component: 1700  -  total flux cleaned = 0.0131637 Jy
! Component: 1750  -  total flux cleaned = 0.0133653 Jy
! Component: 1800  -  total flux cleaned = 0.0135651 Jy
! Component: 1850  -  total flux cleaned = 0.0138397 Jy
! Component: 1900  -  total flux cleaned = 0.0141497 Jy
! Component: 1950  -  total flux cleaned = 0.0144173 Jy
! Component: 2000  -  total flux cleaned = 0.0147565 Jy
! Total flux subtracted in 2048 components = 0.014943 Jy
! Clean residual min=-0.002229 max=0.001985 Jy/beam
! Clean residual mean=0.000028 rms=0.000706 Jy/beam
! Combined flux in latest and established models = 0.138618 Jy
keep
! Adding 143 model components to the UV plane model.
! The established model now contains 191 components and 0.138618 Jy
![Exited script file: muppet]
wmap "J1352-2745_X_2005_07_20_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8823 x 2.359 at -6.731 degrees (North through East)
! Clean map  min=-0.0036876  max=0.10746 Jy/beam
! Writing clean map to FITS file: J1352-2745_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 0.107458 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.243% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000700216 
device "J1352-2745_X_2005_07_20_yyk\_map.eps/VPS"
! Attempting to open device: 'J1352-2745_X_2005_07_20_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -1.95486 1.95486 3.90972 7.81944 15.6389 31.2778 62.5555
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0021 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.107 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8823 x 2.359 at -6.731 degrees (North through East)
! Clean map  min=-0.0036876  max=0.10746 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1352-2745_X_2005_07_20_yyk\_map.gif/gif"
! Attempting to open device: 'J1352-2745_X_2005_07_20_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1352-2745_X_2005_07_20_yyk_uvs.log closed on Fri Jan 20 10:32:14 2006