! Started logfile: J2037-2438_X_2005_07_08_yyk_uvs.log on Fri Jan 20 10:59:56 2006
obs J2037-2438_X_2005_07_08_yyk_uve.fits
! Reading UV FITS file: J2037-2438_X_2005_07_08_yyk_uve.fits
! AN table 1: 10 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.96 visibilities/baseline/integration-bin.
! Found source: J2037-2438
! 
! 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 1406 lines of history.
! 
! Reading 1728 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 J2037-2438_X_2005_07_08_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)= 0.186193 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 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.6445 mas, bmaj=1.759 mas, bpa=5.061 degrees
! Estimated noise=1.73446 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 = 0.138442 Jy
! Component: 100  -  total flux cleaned = 0.166675 Jy
! Total flux subtracted in 100 components = 0.166675 Jy
! Clean residual min=-0.007775 max=0.010540 Jy/beam
! Clean residual mean=-0.000021 rms=0.002448 Jy/beam
! Combined flux in latest and established models = 0.166675 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 15 components and 0.166675 Jy
! 
! Correcting IF 1.
!  A total of 10 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 10 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 10 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 10 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.077682Jy  sigma=1.155351
! Fit after  self-cal, rms=0.077462Jy  sigma=1.149826
! Inverting map and beam 
! Your choice of large map pixels excluded 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.6445 mas, bmaj=1.759 mas, bpa=5.061 degrees
! Estimated noise=1.73446 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 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.878 mas, bmaj=2.187 mas, bpa=1.598 degrees
! Estimated noise=1.06342 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 = 0.0195544 Jy
! Component: 100  -  total flux cleaned = 0.0255137 Jy
! Component: 150  -  total flux cleaned = 0.0274336 Jy
! Component: 200  -  total flux cleaned = 0.0278627 Jy
! Total flux subtracted in 200 components = 0.0278627 Jy
! Clean residual min=-0.006199 max=0.005697 Jy/beam
! Clean residual mean=0.000029 rms=0.001483 Jy/beam
! Combined flux in latest and established models = 0.194537 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 13 model components to the UV plane model.
! The established model now contains 23 components and 0.194537 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.075200Jy  sigma=1.085016
! Fit after  self-cal, rms=0.075179Jy  sigma=1.084865
! Inverting map 
! Your choice of large map pixels excluded 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.878 x 2.187 at 1.598 degrees (North through East)
! Clean map  min=-0.0057259  max=0.16896 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: 1.0226
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.98     FD        0.96     HN        1.00*    KP        0.95     
!   LA        0.97     MK        0.92     NL        1.07     OV        1.01     
!   PT        0.94     SC        0.99     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.03097
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.04     FD        0.95     HN        1.00*    KP        0.86     
!   LA        0.99     MK        0.90     NL        1.02     OV        0.97     
!   PT        0.99     SC        0.96     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 0.99796
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.05     FD        1.04     HN        1.00*    KP        0.87     
!   LA        1.00     MK        0.95     NL        1.08     OV        1.02     
!   PT        1.07     SC        0.95     
! 
! 
! 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=0.075179Jy  sigma=1.084865
! Fit after  self-cal, rms=0.073902Jy  sigma=1.063644
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=0.073902Jy  sigma=1.063644
! Fit after  self-cal, rms=0.073905Jy  sigma=1.063624
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.8571 mas, bmaj=2.162 mas, bpa=0.777 degrees
! Estimated noise=1.05465 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 = 0.00119568 Jy
! Component: 100  -  total flux cleaned = 0.00119631 Jy
! Component: 150  -  total flux cleaned = 0.00124201 Jy
! Component: 200  -  total flux cleaned = 0.00123804 Jy
! Total flux subtracted in 200 components = 0.00123804 Jy
! Clean residual min=-0.004634 max=0.004667 Jy/beam
! Clean residual mean=0.000025 rms=0.001190 Jy/beam
! Combined flux in latest and established models = 0.195775 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 10 model components to the UV plane model.
! The established model now contains 28 components and 0.195775 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.073824Jy  sigma=1.062201
! Fit after  self-cal, rms=0.073811Jy  sigma=1.062141
! Inverting map 
! Your choice of large map pixels excluded 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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=0.073811Jy  sigma=1.062141
! Fit after  self-cal, rms=0.070734Jy  sigma=1.017179
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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 = 0.000592304 Jy
! Component: 100  -  total flux cleaned = 0.000641434 Jy
! Component: 150  -  total flux cleaned = 0.000616661 Jy
! Component: 200  -  total flux cleaned = 0.000616276 Jy
! Total flux subtracted in 200 components = 0.000616276 Jy
! Clean residual min=-0.004408 max=0.004710 Jy/beam
! Clean residual mean=0.000026 rms=0.001165 Jy/beam
! Combined flux in latest and established models = 0.196392 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 31 components and 0.196392 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.070731Jy  sigma=1.016880
! Fit after  self-cal, rms=0.070489Jy  sigma=1.012569
! Inverting map 
! Your choice of large map pixels excluded 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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: 0.8571 x 2.162 at 0.777 degrees (North through East)
! Clean map  min=-0.003973  max=0.16833 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=0.070489Jy  sigma=1.012569
! Fit after  self-cal, rms=0.068283Jy  sigma=0.995433
! 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=0.068283Jy  sigma=0.995433
! Fit after  self-cal, rms=0.068304Jy  sigma=0.994862
! Inverting map and beam 
! Your choice of large map pixels excluded 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.8438 mas, bmaj=2.142 mas, bpa=0.1077 degrees
! Estimated noise=1.0179 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.00437572 Jy
! Component: 100  -  total flux cleaned = -0.0046036 Jy
! Component: 150  -  total flux cleaned = -0.00466623 Jy
! Component: 200  -  total flux cleaned = -0.00471708 Jy
! Total flux subtracted in 200 components = -0.00471708 Jy
! Clean residual min=-0.004111 max=0.003786 Jy/beam
! Clean residual mean=0.000016 rms=0.001030 Jy/beam
! Combined flux in latest and established models = 0.191675 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 33 components and 0.191675 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067984Jy  sigma=0.990297
! Fit after  self-cal, rms=0.067999Jy  sigma=0.990219
! Inverting map 
! Your choice of large map pixels excluded 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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=0.067999Jy  sigma=0.990219
! Fit after  self-cal, rms=0.066747Jy  sigma=0.978870
! 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=0.066747Jy  sigma=0.978870
! Fit after  self-cal, rms=0.066765Jy  sigma=0.978836
! Inverting map and beam 
! Your choice of large map pixels excluded 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.8355 mas, bmaj=2.132 mas, bpa=-0.1502 degrees
! Estimated noise=0.992457 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.00337317 Jy
! Component: 100  -  total flux cleaned = -0.0035301 Jy
! Component: 150  -  total flux cleaned = -0.00352974 Jy
! Component: 200  -  total flux cleaned = -0.00350564 Jy
! Total flux subtracted in 200 components = -0.00350564 Jy
! Clean residual min=-0.003861 max=0.003569 Jy/beam
! Clean residual mean=0.000015 rms=0.000979 Jy/beam
! Combined flux in latest and established models = 0.188169 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 36 components and 0.188169 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066564Jy  sigma=0.975910
! Fit after  self-cal, rms=0.066568Jy  sigma=0.975897
! Inverting map 
! Your choice of large map pixels excluded 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=2.547 mas, bmaj=6.162 mas, bpa=8.248 degrees
! Estimated noise=1.28232 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 = 8.40796e-05 Jy
! Component: 100  -  total flux cleaned = 8.20276e-05 Jy
! Component: 150  -  total flux cleaned = 8.06177e-05 Jy
! Component: 200  -  total flux cleaned = 8.0103e-05 Jy
! Total flux subtracted in 200 components = 8.0103e-05 Jy
! Clean residual min=-0.003818 max=0.003509 Jy/beam
! Clean residual mean=0.000028 rms=0.001081 Jy/beam
! Combined flux in latest and established models = 0.188249 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 40 components and 0.188249 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066567Jy  sigma=0.976155
! Fit after  self-cal, rms=0.066565Jy  sigma=0.976068
! Inverting map 
! Your choice of large map pixels excluded 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.6311 mas, bmaj=1.743 mas, bpa=4.344 degrees
! Estimated noise=1.60546 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.130356 Jy
! Component: 100  -  total flux cleaned = 0.159228 Jy
! Component: 150  -  total flux cleaned = 0.17286 Jy
! Component: 200  -  total flux cleaned = 0.179724 Jy
! Total flux subtracted in 200 components = 0.179724 Jy
! Clean residual min=-0.005936 max=0.006103 Jy/beam
! Clean residual mean=-0.000009 rms=0.001719 Jy/beam
! Combined flux in latest and established models = 0.179724 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 21 model components to the UV plane model.
! The established model now contains 21 components and 0.179724 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.8355 mas, bmaj=2.132 mas, bpa=-0.1502 degrees
! Estimated noise=0.992457 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)
! Added new window around map position (-0.2, -2.6).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00774284 Jy
! Component: 100  -  total flux cleaned = 0.0097265 Jy
! Component: 150  -  total flux cleaned = 0.00972561 Jy
! Component: 200  -  total flux cleaned = 0.00979356 Jy
! Total flux subtracted in 200 components = 0.00979356 Jy
! Clean residual min=-0.004016 max=0.003197 Jy/beam
! Clean residual mean=0.000015 rms=0.000930 Jy/beam
! Combined flux in latest and established models = 0.189518 Jy
! Adding 24 model components to the UV plane model.
! The established model now contains 43 components and 0.189518 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=2.547 mas, bmaj=6.162 mas, bpa=8.248 degrees
! Estimated noise=1.28232 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 = 0.000435375 Jy
! Component: 100  -  total flux cleaned = 0.000471857 Jy
! Component: 150  -  total flux cleaned = 0.000446034 Jy
! Component: 200  -  total flux cleaned = 0.000422207 Jy
! Total flux subtracted in 200 components = 0.000422207 Jy
! Clean residual min=-0.003874 max=0.003580 Jy/beam
! Clean residual mean=0.000030 rms=0.001000 Jy/beam
! Combined flux in latest and established models = 0.18994 Jy
! Adding 12 model components to the UV plane model.
! The established model now contains 52 components and 0.18994 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.8355 mas, bmaj=2.132 mas, bpa=-0.1502 degrees
! Estimated noise=0.992457 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 7.60777e-05 Jy
! Component: 100  -  total flux cleaned = 0.000124909 Jy
! Component: 150  -  total flux cleaned = 7.73156e-05 Jy
! Component: 200  -  total flux cleaned = 3.51585e-05 Jy
! Total flux subtracted in 200 components = 3.51585e-05 Jy
! Clean residual min=-0.004077 max=0.003223 Jy/beam
! Clean residual mean=0.000016 rms=0.000919 Jy/beam
! Combined flux in latest and established models = 0.189975 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 64 components and 0.189975 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066258Jy  sigma=0.970970
! Fit after  self-cal, rms=0.066243Jy  sigma=0.970706
wmodel J2037-2438_X_2005_07_08_yyk\_map.mod
! Writing 64 model components to file: J2037-2438_X_2005_07_08_yyk_map.mod
wobs J2037-2438_X_2005_07_08_yyk\_uvs.fits
! Writing UV FITS file: J2037-2438_X_2005_07_08_yyk_uvs.fits
wwins J2037-2438_X_2005_07_08_yyk\_map.win
! wwins: Wrote 2 windows to J2037-2438_X_2005_07_08_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 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00173512 Jy
! Component: 100  -  total flux cleaned = -0.00265385 Jy
! Component: 150  -  total flux cleaned = -0.00305322 Jy
! Component: 200  -  total flux cleaned = -0.00326852 Jy
! Component: 250  -  total flux cleaned = -0.00342416 Jy
! Component: 300  -  total flux cleaned = -0.00347209 Jy
! Component: 350  -  total flux cleaned = -0.00352058 Jy
! Component: 400  -  total flux cleaned = -0.0035675 Jy
! Component: 450  -  total flux cleaned = -0.00361197 Jy
! Component: 500  -  total flux cleaned = -0.0036106 Jy
! Component: 550  -  total flux cleaned = -0.00382958 Jy
! Component: 600  -  total flux cleaned = -0.00404434 Jy
! Component: 650  -  total flux cleaned = -0.00433799 Jy
! Component: 700  -  total flux cleaned = -0.0045844 Jy
! Component: 750  -  total flux cleaned = -0.00474534 Jy
! Component: 800  -  total flux cleaned = -0.00494289 Jy
! Component: 850  -  total flux cleaned = -0.00517659 Jy
! Component: 900  -  total flux cleaned = -0.00540625 Jy
! Component: 950  -  total flux cleaned = -0.00563183 Jy
! Component: 1000  -  total flux cleaned = -0.00588962 Jy
! Component: 1050  -  total flux cleaned = -0.00614406 Jy
! Component: 1100  -  total flux cleaned = -0.00635863 Jy
! Component: 1150  -  total flux cleaned = -0.00667591 Jy
! Component: 1200  -  total flux cleaned = -0.00688392 Jy
! Component: 1250  -  total flux cleaned = -0.00698728 Jy
! Component: 1300  -  total flux cleaned = -0.00732659 Jy
! Component: 1350  -  total flux cleaned = -0.00759406 Jy
! Component: 1400  -  total flux cleaned = -0.00775943 Jy
! Component: 1450  -  total flux cleaned = -0.00802036 Jy
! Component: 1500  -  total flux cleaned = -0.00821361 Jy
! Component: 1550  -  total flux cleaned = -0.00846862 Jy
! Component: 1600  -  total flux cleaned = -0.00862659 Jy
! Component: 1650  -  total flux cleaned = -0.00884537 Jy
! Component: 1700  -  total flux cleaned = -0.00903084 Jy
! Component: 1750  -  total flux cleaned = -0.009245 Jy
! Component: 1800  -  total flux cleaned = -0.00933502 Jy
! Component: 1850  -  total flux cleaned = -0.00951543 Jy
! Component: 1900  -  total flux cleaned = -0.0096045 Jy
! Component: 1950  -  total flux cleaned = -0.00981083 Jy
! Component: 2000  -  total flux cleaned = -0.00989815 Jy
! Total flux subtracted in 2048 components = -0.0100716 Jy
! Clean residual min=-0.001767 max=0.001513 Jy/beam
! Clean residual mean=0.000012 rms=0.000536 Jy/beam
! Combined flux in latest and established models = 0.179903 Jy
keep
! Adding 144 model components to the UV plane model.
! The established model now contains 208 components and 0.179903 Jy
![Exited script file: muppet]
wmap "J2037-2438_X_2005_07_08_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8355 x 2.132 at -0.1502 degrees (North through East)
! Clean map  min=-0.0038136  max=0.15934 Jy/beam
! Writing clean map to FITS file: J2037-2438_X_2005_07_08_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.159337 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.348% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000532374 
device "J2037-2438_X_2005_07_08_yyk\_map.eps/VPS"
! Attempting to open device: 'J2037-2438_X_2005_07_08_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -1.00235 1.00235 2.00471 4.00942 8.01883 16.0377 32.0753 64.1507
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0015 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.159 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8355 x 2.132 at -0.1502 degrees (North through East)
! Clean map  min=-0.0038136  max=0.15934 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J2037-2438_X_2005_07_08_yyk\_map.gif/gif"
! Attempting to open device: 'J2037-2438_X_2005_07_08_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J2037-2438_X_2005_07_08_yyk_uvs.log closed on Fri Jan 20 11:00:00 2006