! Started logfile: J0604-4225_X_2002_01_31_yyk_uvs.log on Wed Jun 27 10:49:38 2007
obs J0604-4225_X_2002_01_31_yyk_uva.fits
! Reading UV FITS file: J0604-4225_X_2002_01_31_yyk_uva.fits
! AN table 1: 39 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.577208 visibilities/baseline/integration-bin.
! Found source: J0604-4225
! 
! 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 4052 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 J0604-4225_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)= 0.277639 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 1.13% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.6331 mas, bmaj=1.728 mas, bpa=2.339 degrees
! Estimated noise=3976.68 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 = 0.183802 Jy
! Component: 100  -  total flux cleaned = 0.226968 Jy
! Total flux subtracted in 100 components = 0.226968 Jy
! Clean residual min=-0.019052 max=0.021701 Jy/beam
! Clean residual mean=0.000160 rms=0.006485 Jy/beam
! Combined flux in latest and established models = 0.226968 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 6 model components to the UV plane model.
! The established model now contains 6 components and 0.226968 Jy
! 
! Correcting IF 1.
!  A total of 135 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 135 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 135 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 135 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.173559Jy  sigma=0.001285
! Fit after  self-cal, rms=0.173381Jy  sigma=0.001284
! Inverting map and beam 
! Your choice of large map pixels excluded 1.13% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.6331 mas, bmaj=1.728 mas, bpa=2.339 degrees
! Estimated noise=3977.08 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 1.13% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.7956 mas, bmaj=2.144 mas, bpa=2.165 degrees
! Estimated noise=1660.35 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 = 0.0148644 Jy
! Component: 100  -  total flux cleaned = 0.0161872 Jy
! Component: 150  -  total flux cleaned = 0.01626 Jy
! Component: 200  -  total flux cleaned = 0.0162601 Jy
! Total flux subtracted in 200 components = 0.0162601 Jy
! Clean residual min=-0.013877 max=0.012622 Jy/beam
! Clean residual mean=0.000325 rms=0.003842 Jy/beam
! Combined flux in latest and established models = 0.243228 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 14 model components to the UV plane model.
! The established model now contains 18 components and 0.243228 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.172575Jy  sigma=0.001277
! Fit after  self-cal, rms=0.172560Jy  sigma=0.001277
! Inverting map 
! Your choice of large map pixels excluded 1.13% 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 ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7956 x 2.144 at 2.165 degrees (North through East)
! Clean map  min=-0.012457  max=0.20376 Jy/beam
if(peak(flux) < thresh*2)
  selflims ampcor_selflim
  end if
gscale
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Amplitude normalization factor in sub-array 1: 1.00885
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.89     HN        1.00*    KP        1.03     
!   LA        1.13     MK        0.95     NL        1.00*    OV        0.94     
!   PT        0.99     SC        0.98     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 0.999739
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.88     HN        1.00*    KP        1.01     
!   LA        1.23     MK        0.99     NL        1.00*    OV        0.92     
!   PT        0.95     SC        1.03     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 0.998366
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.88     HN        1.00*    KP        0.97     
!   LA        1.11     MK        0.98     NL        1.00*    OV        0.98     
!   PT        1.08     SC        1.01     
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 0.975609
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.88     HN        1.00*    KP        1.16     
!   LA        1.10     MK        1.08     NL        1.00*    OV        0.95     
!   PT        1.13     SC        0.96     
! 
! 
! Fit before self-cal, rms=0.172560Jy  sigma=0.001277
! Fit after  self-cal, rms=0.171288Jy  sigma=0.001261
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=0.171288Jy  sigma=0.001261
! Fit after  self-cal, rms=0.171293Jy  sigma=0.001260
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 1.13% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.7925 mas, bmaj=2.147 mas, bpa=2.196 degrees
! Estimated noise=1634.3 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 = -0.00109887 Jy
! Component: 100  -  total flux cleaned = -0.00128319 Jy
! Component: 150  -  total flux cleaned = -0.00133595 Jy
! Component: 200  -  total flux cleaned = -0.00133891 Jy
! Total flux subtracted in 200 components = -0.00133891 Jy
! Clean residual min=-0.004970 max=0.007664 Jy/beam
! Clean residual mean=-0.000019 rms=0.001682 Jy/beam
! Combined flux in latest and established models = 0.241889 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 9 model components to the UV plane model.
! The established model now contains 24 components and 0.241889 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.171255Jy  sigma=0.001260
! Fit after  self-cal, rms=0.171245Jy  sigma=0.001260
! Inverting map 
! Your choice of large map pixels excluded 1.13% 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=0.171245Jy  sigma=0.001260
! Fit after  self-cal, rms=0.165556Jy  sigma=0.001220
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.13% 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 = 0.000307874 Jy
! Component: 100  -  total flux cleaned = 0.000125537 Jy
! Component: 150  -  total flux cleaned = 0.000151444 Jy
! Component: 200  -  total flux cleaned = 0.000162483 Jy
! Total flux subtracted in 200 components = 0.000162483 Jy
! Clean residual min=-0.005124 max=0.007208 Jy/beam
! Clean residual mean=-0.000021 rms=0.001647 Jy/beam
! Combined flux in latest and established models = 0.242052 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 11 model components to the UV plane model.
! The established model now contains 28 components and 0.242052 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.165304Jy  sigma=0.001218
! Fit after  self-cal, rms=0.164172Jy  sigma=0.001210
! Inverting map 
! Your choice of large map pixels excluded 1.13% 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: 0.7925 x 2.147 at 2.196 degrees (North through East)
! Clean map  min=-0.0047078  max=0.20945 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=0.164172Jy  sigma=0.001210
! Fit after  self-cal, rms=0.162784Jy  sigma=0.001209
! 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=0.162784Jy  sigma=0.001209
! Fit after  self-cal, rms=0.162539Jy  sigma=0.001208
! Inverting map and beam 
! Your choice of large map pixels excluded 1.13% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.7792 mas, bmaj=2.124 mas, bpa=2.884 degrees
! Estimated noise=1621.99 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000834622 Jy
! Component: 100  -  total flux cleaned = 0.000861134 Jy
! Component: 150  -  total flux cleaned = 0.00088067 Jy
! Component: 200  -  total flux cleaned = 0.000877994 Jy
! Total flux subtracted in 200 components = 0.000877994 Jy
! Clean residual min=-0.005101 max=0.006527 Jy/beam
! Clean residual mean=-0.000021 rms=0.001589 Jy/beam
! Combined flux in latest and established models = 0.24293 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 9 model components to the UV plane model.
! The established model now contains 31 components and 0.24293 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.162533Jy  sigma=0.001208
! Fit after  self-cal, rms=0.162467Jy  sigma=0.001207
! Inverting map 
! Your choice of large map pixels excluded 1.13% 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=0.162467Jy  sigma=0.001207
! Fit after  self-cal, rms=0.165020Jy  sigma=0.001202
! 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=0.165020Jy  sigma=0.001202
! Fit after  self-cal, rms=0.165026Jy  sigma=0.001202
! Inverting map and beam 
! Your choice of large map pixels excluded 1.13% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.7774 mas, bmaj=2.118 mas, bpa=2.92 degrees
! Estimated noise=1621.66 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00069259 Jy
! Component: 100  -  total flux cleaned = 0.000717698 Jy
! Component: 150  -  total flux cleaned = 0.000716984 Jy
! Component: 200  -  total flux cleaned = 0.000719282 Jy
! Total flux subtracted in 200 components = 0.000719282 Jy
! Clean residual min=-0.005069 max=0.006465 Jy/beam
! Clean residual mean=-0.000030 rms=0.001580 Jy/beam
! Combined flux in latest and established models = 0.243649 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 7 model components to the UV plane model.
! The established model now contains 31 components and 0.243649 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.165024Jy  sigma=0.001202
! Fit after  self-cal, rms=0.165020Jy  sigma=0.001202
! Inverting map 
! Your choice of large map pixels excluded 1.13% 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 1.13% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=2.924 mas, bmaj=10.9 mas, bpa=5.447 degrees
! Estimated noise=2190.41 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 = 0.000309386 Jy
! Component: 100  -  total flux cleaned = 0.000310113 Jy
! Component: 150  -  total flux cleaned = 0.000310669 Jy
! Component: 200  -  total flux cleaned = 0.000310949 Jy
! Total flux subtracted in 200 components = 0.000310949 Jy
! Clean residual min=-0.004453 max=0.007413 Jy/beam
! Clean residual mean=-0.000055 rms=0.002090 Jy/beam
! Combined flux in latest and established models = 0.24396 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 31 components and 0.24396 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.165017Jy  sigma=0.001202
! Fit after  self-cal, rms=0.165025Jy  sigma=0.001202
! Inverting map 
! Your choice of large map pixels excluded 1.13% of the data.
!  The x-axis pixel size should ideally be below 0.1988 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 1.13% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.6301 mas, bmaj=1.737 mas, bpa=2.183 degrees
! Estimated noise=3912.56 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.184257 Jy
! Component: 100  -  total flux cleaned = 0.224344 Jy
! Component: 150  -  total flux cleaned = 0.236006 Jy
! Component: 200  -  total flux cleaned = 0.240728 Jy
! Total flux subtracted in 200 components = 0.240728 Jy
! Clean residual min=-0.011209 max=0.011481 Jy/beam
! Clean residual mean=-0.000023 rms=0.003805 Jy/beam
! Combined flux in latest and established models = 0.240728 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 9 model components to the UV plane model.
! The established model now contains 9 components and 0.240728 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 1.13% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.7774 mas, bmaj=2.118 mas, bpa=2.92 degrees
! Estimated noise=1621.66 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 = 0.00347213 Jy
! Component: 100  -  total flux cleaned = 0.00345752 Jy
! Component: 150  -  total flux cleaned = 0.00335583 Jy
! Component: 200  -  total flux cleaned = 0.00329217 Jy
! Total flux subtracted in 200 components = 0.00329217 Jy
! Clean residual min=-0.005175 max=0.006946 Jy/beam
! Clean residual mean=-0.000029 rms=0.001609 Jy/beam
! Combined flux in latest and established models = 0.24402 Jy
! Adding 10 model components to the UV plane model.
! The established model now contains 15 components and 0.24402 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.13% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Added new window around map position (2.6, -9).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00641286 Jy
! Component: 100  -  total flux cleaned = 0.0085884 Jy
! Component: 150  -  total flux cleaned = 0.0093053 Jy
! Component: 200  -  total flux cleaned = 0.0096485 Jy
! Total flux subtracted in 200 components = 0.0096485 Jy
! Clean residual min=-0.004223 max=0.003954 Jy/beam
! Clean residual mean=0.000005 rms=0.001270 Jy/beam
! Combined flux in latest and established models = 0.253668 Jy
! Adding 16 model components to the UV plane model.
! The established model now contains 31 components and 0.253668 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.13% 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 1.13% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=2.924 mas, bmaj=10.9 mas, bpa=5.447 degrees
! Estimated noise=2190.41 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 = 0.000252864 Jy
! Component: 100  -  total flux cleaned = 0.000252086 Jy
! Component: 150  -  total flux cleaned = 0.000251042 Jy
! Component: 200  -  total flux cleaned = 0.000250043 Jy
! Total flux subtracted in 200 components = 0.000250043 Jy
! Clean residual min=-0.003705 max=0.003373 Jy/beam
! Clean residual mean=0.000015 rms=0.001393 Jy/beam
! Combined flux in latest and established models = 0.253918 Jy
! Adding 3 model components to the UV plane model.
! The established model now contains 33 components and 0.253918 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.13% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 1.13% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.7774 mas, bmaj=2.118 mas, bpa=2.92 degrees
! Estimated noise=1621.66 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -7.63961e-05 Jy
! Component: 100  -  total flux cleaned = -7.45435e-05 Jy
! Component: 150  -  total flux cleaned = -4.5762e-05 Jy
! Component: 200  -  total flux cleaned = -7.34844e-05 Jy
! Total flux subtracted in 200 components = -7.34844e-05 Jy
! Clean residual min=-0.004112 max=0.004050 Jy/beam
! Clean residual mean=0.000006 rms=0.001256 Jy/beam
! Combined flux in latest and established models = 0.253845 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 11 model components to the UV plane model.
! The established model now contains 40 components and 0.253845 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.164877Jy  sigma=0.001200
! Fit after  self-cal, rms=0.164847Jy  sigma=0.001200
wmodel J0604-4225_X_2002_01_31_yyk\_map.mod
! Writing 40 model components to file: J0604-4225_X_2002_01_31_yyk_map.mod
wobs J0604-4225_X_2002_01_31_yyk\_uvs.fits
! Applying 39 buffered edits.
! Writing UV FITS file: J0604-4225_X_2002_01_31_yyk_uvs.fits
wwins J0604-4225_X_2002_01_31_yyk\_map.win
! wwins: Wrote 2 windows to J0604-4225_X_2002_01_31_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 1.13% 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 = -7.60172e-05 Jy
! Component: 100  -  total flux cleaned = -0.000140194 Jy
! Component: 150  -  total flux cleaned = -0.000201805 Jy
! Component: 200  -  total flux cleaned = -0.000145909 Jy
! Component: 250  -  total flux cleaned = -3.81134e-05 Jy
! Component: 300  -  total flux cleaned = 1.27026e-05 Jy
! Component: 350  -  total flux cleaned = 1.28487e-05 Jy
! Component: 400  -  total flux cleaned = 6.00056e-05 Jy
! Component: 450  -  total flux cleaned = -7.84597e-05 Jy
! Component: 500  -  total flux cleaned = -0.000209075 Jy
! Component: 550  -  total flux cleaned = -0.000122968 Jy
! Component: 600  -  total flux cleaned = -0.000165698 Jy
! Component: 650  -  total flux cleaned = -0.000126341 Jy
! Component: 700  -  total flux cleaned = -0.000127316 Jy
! Component: 750  -  total flux cleaned = -0.000166038 Jy
! Component: 800  -  total flux cleaned = -9.22725e-05 Jy
! Component: 850  -  total flux cleaned = -9.21706e-05 Jy
! Component: 900  -  total flux cleaned = -5.65257e-05 Jy
! Component: 950  -  total flux cleaned = 1.29605e-05 Jy
! Component: 1000  -  total flux cleaned = -2.09436e-05 Jy
! Component: 1050  -  total flux cleaned = -2.13972e-05 Jy
! Component: 1100  -  total flux cleaned = -8.81662e-05 Jy
! Component: 1150  -  total flux cleaned = -8.82675e-05 Jy
! Component: 1200  -  total flux cleaned = -8.83507e-05 Jy
! Component: 1250  -  total flux cleaned = -5.5622e-05 Jy
! Component: 1300  -  total flux cleaned = -2.2882e-05 Jy
! Component: 1350  -  total flux cleaned = -5.53661e-05 Jy
! Component: 1400  -  total flux cleaned = -8.78227e-05 Jy
! Component: 1450  -  total flux cleaned = -5.54085e-05 Jy
! Component: 1500  -  total flux cleaned = -8.79545e-05 Jy
! Component: 1550  -  total flux cleaned = -5.46458e-05 Jy
! Component: 1600  -  total flux cleaned = -5.4667e-05 Jy
! Component: 1650  -  total flux cleaned = -2.10438e-05 Jy
! Component: 1700  -  total flux cleaned = -2.11208e-05 Jy
! Component: 1750  -  total flux cleaned = 4.66507e-05 Jy
! Component: 1800  -  total flux cleaned = 4.68356e-05 Jy
! Component: 1850  -  total flux cleaned = 0.000116053 Jy
! Component: 1900  -  total flux cleaned = 0.000151408 Jy
! Component: 1950  -  total flux cleaned = 0.000222086 Jy
! Component: 2000  -  total flux cleaned = 0.000293503 Jy
! Total flux subtracted in 2048 components = 0.000329875 Jy
! Clean residual min=-0.002078 max=0.002428 Jy/beam
! Clean residual mean=-0.000005 rms=0.000630 Jy/beam
! Combined flux in latest and established models = 0.254175 Jy
keep
! Adding 103 model components to the UV plane model.
! The established model now contains 143 components and 0.254175 Jy
![Exited script file: muppet]
wmap "J0604-4225_X_2002_01_31_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 1.13% 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: 0.7774 x 2.118 at 2.92 degrees (North through East)
! Clean map  min=-0.0036027  max=0.20655 Jy/beam
! Writing clean map to FITS file: J0604-4225_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 0.20655 
invert
! Inverting map 
! Your choice of large map pixels excluded 1.13% 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 0.000624038 
device "J0604-4225_X_2002_01_31_yyk\_map.eps/VPS"
! Attempting to open device: 'J0604-4225_X_2002_01_31_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.906372 0.906372 1.81274 3.62549 7.25098 14.502 29.0039 58.0078
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0018 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.206 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7774 x 2.118 at 2.92 degrees (North through East)
! Clean map  min=-0.0036027  max=0.20655 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0604-4225_X_2002_01_31_yyk\_map.gif/gif"
! Attempting to open device: 'J0604-4225_X_2002_01_31_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J0604-4225_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 10:49:44 2007