! Started logfile: J2353-3037_X_2004_04_30_yyk_uvs.log on Wed Dec  7 01:00:40 2005
obs J2353-3037_X_2004_04_30_yyk_uve.fits
! Reading UV FITS file: J2353-3037_X_2004_04_30_yyk_uve.fits
! AN table 1: 5 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.693333 visibilities/baseline/integration-bin.
! Found source: J2353-3037
! 
! 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 1546 lines of history.
! 
! Reading 624 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 J2353-3037_X_2004_04_30_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)= 0.166202 Jy 
startmod ,phase_soltime
! Applying default point source starting model.
! Performing phase self-cal over 10 minute time intervals
! Adding 1 model components to the UV plane model.
! The established model now contains 1 components and 1 Jy
! 
! Correcting IF 1.
!  A total of 13 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 11 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 13 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 13 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.856727Jy  sigma=14.478863
! Fit after  self-cal, rms=0.856556Jy  sigma=14.474650
! clrmod: Cleared the established, tentative and continuum models.
! Redundant starting model cleared.
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 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.6902 mas, bmaj=1.768 mas, bpa=0.1466 degrees
! Estimated noise=2.46503 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 = 0.127755 Jy
! Component: 100  -  total flux cleaned = 0.154557 Jy
! Total flux subtracted in 100 components = 0.154557 Jy
! Clean residual min=-0.007988 max=0.009708 Jy/beam
! Clean residual mean=0.000040 rms=0.002503 Jy/beam
! Combined flux in latest and established models = 0.154557 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 18 model components to the UV plane model.
! The established model now contains 18 components and 0.154557 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.074813Jy  sigma=1.077864
! Fit after  self-cal, rms=0.074788Jy  sigma=1.077465
! Inverting map 
! Your choice of large map pixels excluded 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
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 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.7586 mas, bmaj=1.959 mas, bpa=1.027 degrees
! Estimated noise=1.86617 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 = 0.0116936 Jy
! Component: 100  -  total flux cleaned = 0.015957 Jy
! Component: 150  -  total flux cleaned = 0.0175471 Jy
! Component: 200  -  total flux cleaned = 0.017711 Jy
! Total flux subtracted in 200 components = 0.017711 Jy
! Clean residual min=-0.007018 max=0.008849 Jy/beam
! Clean residual mean=0.000171 rms=0.002154 Jy/beam
! Combined flux in latest and established models = 0.172268 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 19 model components to the UV plane model.
! The established model now contains 30 components and 0.172268 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.073801Jy  sigma=1.055199
! Fit after  self-cal, rms=0.073773Jy  sigma=1.054963
! Inverting map 
! Your choice of large map pixels excluded 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
selflims ampcor_selflim
! 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: 1.00046
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.96     FD        1.00*    HN        1.00*    KP        0.96     
!   LA        1.08     MK        0.99     NL        1.03     OV        1.00     
!   PT        1.00     SC        0.96     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.01741
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.01     FD        0.92     HN        1.00*    KP        0.89     
!   LA        0.97     MK        0.96     NL        1.01     OV        0.98     
!   PT        1.06     SC        1.03     
! 
! 
! Correcting IF 3.
!  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 4.
!  Amplitude normalization factor in sub-array 1: 0.982721
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.09     FD        1.00*    HN        1.00*    KP        0.92     
!   LA        0.94     MK        1.02     NL        1.01     OV        1.02     
!   PT        1.11     SC        1.06     
! 
! 
! Fit before self-cal, rms=0.073773Jy  sigma=1.054963
! Fit after  self-cal, rms=0.073517Jy  sigma=1.043314
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=0.073517Jy  sigma=1.043314
! Fit after  self-cal, rms=0.073509Jy  sigma=1.043122
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.7579 mas, bmaj=1.964 mas, bpa=0.6615 degrees
! Estimated noise=1.8654 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 = 0.000443829 Jy
! Component: 100  -  total flux cleaned = 0.000485179 Jy
! Component: 150  -  total flux cleaned = 0.000521066 Jy
! Component: 200  -  total flux cleaned = 0.000554187 Jy
! Total flux subtracted in 200 components = 0.000554187 Jy
! Clean residual min=-0.006085 max=0.007719 Jy/beam
! Clean residual mean=0.000126 rms=0.001779 Jy/beam
! Combined flux in latest and established models = 0.172822 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 42 components and 0.172822 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.073493Jy  sigma=1.042548
! Fit after  self-cal, rms=0.073469Jy  sigma=1.042335
! Inverting map 
! Your choice of large map pixels excluded 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 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=0.073469Jy  sigma=1.042335
! Fit after  self-cal, rms=0.070998Jy  sigma=1.003410
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 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 = 0.000379647 Jy
! Component: 100  -  total flux cleaned = 0.000495169 Jy
! Component: 150  -  total flux cleaned = 0.000590333 Jy
! Component: 200  -  total flux cleaned = 0.000621854 Jy
! Total flux subtracted in 200 components = 0.000621854 Jy
! Clean residual min=-0.005909 max=0.007570 Jy/beam
! Clean residual mean=0.000127 rms=0.001746 Jy/beam
! Combined flux in latest and established models = 0.173444 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 46 components and 0.173444 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.070997Jy  sigma=1.002941
! Fit after  self-cal, rms=0.070809Jy  sigma=1.000185
! Inverting map 
! Your choice of large map pixels excluded 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 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: 0.7579 x 1.964 at 0.6615 degrees (North through East)
! Clean map  min=-0.0054353  max=0.14918 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=0.070809Jy  sigma=1.000185
! Fit after  self-cal, rms=0.071574Jy  sigma=1.001562
! 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=0.071574Jy  sigma=1.001562
! Fit after  self-cal, rms=0.071561Jy  sigma=1.001221
! Inverting map and beam 
! Your choice of large map pixels excluded 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.7549 mas, bmaj=1.962 mas, bpa=0.2461 degrees
! Estimated noise=1.87084 mJy/beam.
! Added new window around map position (21.8, 15).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00790708 Jy
! Component: 100  -  total flux cleaned = 0.0104472 Jy
! Component: 150  -  total flux cleaned = 0.0111299 Jy
! Component: 200  -  total flux cleaned = 0.0114904 Jy
! Total flux subtracted in 200 components = 0.0114904 Jy
! Clean residual min=-0.005323 max=0.005987 Jy/beam
! Clean residual mean=0.000112 rms=0.001423 Jy/beam
! Combined flux in latest and established models = 0.184935 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 26 model components to the UV plane model.
! The established model now contains 68 components and 0.184935 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.071126Jy  sigma=0.989070
! Fit after  self-cal, rms=0.071065Jy  sigma=0.988128
! Inverting map 
! Your choice of large map pixels excluded 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 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=0.071065Jy  sigma=0.988128
! Fit after  self-cal, rms=0.072045Jy  sigma=0.981193
! 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=0.072045Jy  sigma=0.981193
! Fit after  self-cal, rms=0.072047Jy  sigma=0.981049
! Inverting map and beam 
! Your choice of large map pixels excluded 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.7557 mas, bmaj=1.96 mas, bpa=-0.6807 degrees
! Estimated noise=1.8742 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00314778 Jy
! Component: 100  -  total flux cleaned = 0.00409271 Jy
! Component: 150  -  total flux cleaned = 0.00426868 Jy
! Component: 200  -  total flux cleaned = 0.00432387 Jy
! Total flux subtracted in 200 components = 0.00432387 Jy
! Clean residual min=-0.004899 max=0.005803 Jy/beam
! Clean residual mean=0.000100 rms=0.001406 Jy/beam
! Combined flux in latest and established models = 0.189259 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 25 model components to the UV plane model.
! The established model now contains 85 components and 0.189259 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.071961Jy  sigma=0.978588
! Fit after  self-cal, rms=0.071947Jy  sigma=0.978369
! Inverting map 
! Your choice of large map pixels excluded 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 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 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=2.491 mas, bmaj=7.139 mas, bpa=1.106 degrees
! Estimated noise=2.58095 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 = 0.00233643 Jy
! Component: 100  -  total flux cleaned = 0.00271036 Jy
! Component: 150  -  total flux cleaned = 0.00275042 Jy
! Component: 200  -  total flux cleaned = 0.00282097 Jy
! Total flux subtracted in 200 components = 0.00282097 Jy
! Clean residual min=-0.006013 max=0.005836 Jy/beam
! Clean residual mean=0.000208 rms=0.001939 Jy/beam
! Combined flux in latest and established models = 0.19208 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 8 model components to the UV plane model.
! The established model now contains 90 components and 0.192079 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.071967Jy  sigma=0.978579
! Fit after  self-cal, rms=0.071962Jy  sigma=0.978468
! Inverting map 
! Your choice of large map pixels excluded 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
uvtaper 0,0
! 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 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.6883 mas, bmaj=1.767 mas, bpa=-0.7704 degrees
! Estimated noise=2.48605 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.129707 Jy
! Component: 100  -  total flux cleaned = 0.157037 Jy
! Component: 150  -  total flux cleaned = 0.170749 Jy
! Component: 200  -  total flux cleaned = 0.178975 Jy
! Total flux subtracted in 200 components = 0.178975 Jy
! Clean residual min=-0.008055 max=0.006511 Jy/beam
! Clean residual mean=0.000004 rms=0.001911 Jy/beam
! Combined flux in latest and established models = 0.178975 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 25 model components to the UV plane model.
! The established model now contains 25 components and 0.178975 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.7557 mas, bmaj=1.96 mas, bpa=-0.6807 degrees
! Estimated noise=1.8742 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 = 0.006277 Jy
! Component: 100  -  total flux cleaned = 0.00849314 Jy
! Component: 150  -  total flux cleaned = 0.00932003 Jy
! Component: 200  -  total flux cleaned = 0.009912 Jy
! Total flux subtracted in 200 components = 0.009912 Jy
! Clean residual min=-0.005024 max=0.005626 Jy/beam
! Clean residual mean=0.000100 rms=0.001426 Jy/beam
! Combined flux in latest and established models = 0.188887 Jy
! Adding 31 model components to the UV plane model.
! The established model now contains 51 components and 0.188887 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 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 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=2.491 mas, bmaj=7.139 mas, bpa=1.106 degrees
! Estimated noise=2.58095 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 = 0.00287493 Jy
! Component: 100  -  total flux cleaned = 0.00332914 Jy
! Component: 150  -  total flux cleaned = 0.00362887 Jy
! Component: 200  -  total flux cleaned = 0.00373404 Jy
! Total flux subtracted in 200 components = 0.00373404 Jy
! Clean residual min=-0.006192 max=0.005808 Jy/beam
! Clean residual mean=0.000208 rms=0.001935 Jy/beam
! Combined flux in latest and established models = 0.192621 Jy
! Adding 9 model components to the UV plane model.
! The established model now contains 59 components and 0.192621 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.7557 mas, bmaj=1.96 mas, bpa=-0.6807 degrees
! Estimated noise=1.8742 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.000388773 Jy
! Component: 100  -  total flux cleaned = -0.000507258 Jy
! Component: 150  -  total flux cleaned = -0.000557785 Jy
! Component: 200  -  total flux cleaned = -0.000607016 Jy
! Total flux subtracted in 200 components = -0.000607016 Jy
! Clean residual min=-0.004781 max=0.005544 Jy/beam
! Clean residual mean=0.000091 rms=0.001400 Jy/beam
! Combined flux in latest and established models = 0.192014 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 21 model components to the UV plane model.
! The established model now contains 77 components and 0.192014 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.071875Jy  sigma=0.978438
! Fit after  self-cal, rms=0.071854Jy  sigma=0.978307
wmodel J2353-3037_X_2004_04_30_yyk\_map.mod
! Writing 77 model components to file: J2353-3037_X_2004_04_30_yyk_map.mod
wobs J2353-3037_X_2004_04_30_yyk\_uvs.fits
! Writing UV FITS file: J2353-3037_X_2004_04_30_yyk_uvs.fits
wwins J2353-3037_X_2004_04_30_yyk\_map.win
! wwins: Wrote 2 windows to J2353-3037_X_2004_04_30_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 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.00102778 Jy
! Component: 100  -  total flux cleaned = 0.000707608 Jy
! Component: 150  -  total flux cleaned = 0.000560384 Jy
! Component: 200  -  total flux cleaned = 0.000559626 Jy
! Component: 250  -  total flux cleaned = 0.000686134 Jy
! Component: 300  -  total flux cleaned = 0.000747049 Jy
! Component: 350  -  total flux cleaned = 0.000923521 Jy
! Component: 400  -  total flux cleaned = 0.00114876 Jy
! Component: 450  -  total flux cleaned = 0.00125813 Jy
! Component: 500  -  total flux cleaned = 0.00131284 Jy
! Component: 550  -  total flux cleaned = 0.00151988 Jy
! Component: 600  -  total flux cleaned = 0.00172054 Jy
! Component: 650  -  total flux cleaned = 0.00171997 Jy
! Component: 700  -  total flux cleaned = 0.00167077 Jy
! Component: 750  -  total flux cleaned = 0.00143328 Jy
! Component: 800  -  total flux cleaned = 0.00133986 Jy
! Component: 850  -  total flux cleaned = 0.00101763 Jy
! Component: 900  -  total flux cleaned = 0.000836948 Jy
! Component: 950  -  total flux cleaned = 0.000615035 Jy
! Component: 1000  -  total flux cleaned = 0.000439908 Jy
! Component: 1050  -  total flux cleaned = 0.000266799 Jy
! Component: 1100  -  total flux cleaned = 9.70783e-05 Jy
! Component: 1150  -  total flux cleaned = -0.000154396 Jy
! Component: 1200  -  total flux cleaned = -0.000277857 Jy
! Component: 1250  -  total flux cleaned = -0.00044089 Jy
! Component: 1300  -  total flux cleaned = -0.000601606 Jy
! Component: 1350  -  total flux cleaned = -0.000879132 Jy
! Component: 1400  -  total flux cleaned = -0.00107463 Jy
! Component: 1450  -  total flux cleaned = -0.001384 Jy
! Component: 1500  -  total flux cleaned = -0.00157542 Jy
! Component: 1550  -  total flux cleaned = -0.00187806 Jy
! Component: 1600  -  total flux cleaned = -0.00210226 Jy
! Component: 1650  -  total flux cleaned = -0.00232426 Jy
! Component: 1700  -  total flux cleaned = -0.00261655 Jy
! Component: 1750  -  total flux cleaned = -0.00279762 Jy
! Component: 1800  -  total flux cleaned = -0.00304853 Jy
! Component: 1850  -  total flux cleaned = -0.00326153 Jy
! Component: 1900  -  total flux cleaned = -0.00347268 Jy
! Component: 1950  -  total flux cleaned = -0.00378632 Jy
! Component: 2000  -  total flux cleaned = -0.00409722 Jy
! Total flux subtracted in 2048 components = -0.00440497 Jy
! Clean residual min=-0.001999 max=0.001704 Jy/beam
! Clean residual mean=0.000023 rms=0.000619 Jy/beam
! Combined flux in latest and established models = 0.187609 Jy
keep
! Adding 103 model components to the UV plane model.
! The established model now contains 180 components and 0.187609 Jy
![Exited script file: muppet]
wmap "J2353-3037_X_2004_04_30_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7557 x 1.96 at -0.6807 degrees (North through East)
! Clean map  min=-0.0037234  max=0.1489 Jy/beam
! Writing clean map to FITS file: J2353-3037_X_2004_04_30_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.148898 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.996% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000618475 
device "J2353-3037_X_2004_04_30_yyk\_map.eps/VPS"
! Attempting to open device: 'J2353-3037_X_2004_04_30_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -1.24611 1.24611 2.49221 4.98442 9.96885 19.9377 39.8754 79.7508
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0018 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.148 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7557 x 1.96 at -0.6807 degrees (North through East)
! Clean map  min=-0.0037234  max=0.1489 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J2353-3037_X_2004_04_30_yyk\_map.gif/gif"
! Attempting to open device: 'J2353-3037_X_2004_04_30_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J2353-3037_X_2004_04_30_yyk_uvs.log closed on Wed Dec  7 01:00:44 2005