! Started logfile: J0335-0709_X_2005_07_08_yyk_uvs.log on Fri Jan 20 09:51:12 2006
obs J0335-0709_X_2005_07_08_yyk_uve.fits
! Reading UV FITS file: J0335-0709_X_2005_07_08_yyk_uve.fits
! AN table 1: 11 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.810101 visibilities/baseline/integration-bin.
! Found source: J0335-0709
! 
! 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 1407 lines of history.
! 
! Reading 1604 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 J0335-0709_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)= 0.0957887 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 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.7398 mas, bmaj=1.888 mas, bpa=-6.48 degrees
! Estimated noise=1.36329 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 = 0.0540541 Jy
! Component: 100  -  total flux cleaned = 0.0672502 Jy
! Total flux subtracted in 100 components = 0.0672502 Jy
! Clean residual min=-0.008405 max=0.010602 Jy/beam
! Clean residual mean=0.000039 rms=0.002286 Jy/beam
! Combined flux in latest and established models = 0.0672502 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 12 model components to the UV plane model.
! The established model now contains 12 components and 0.0672502 Jy
! 
! Correcting IF 1.
!  A total of 18 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 17 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 49 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 32 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.071255Jy  sigma=1.250778
! Fit after  self-cal, rms=0.068143Jy  sigma=1.201027
! Inverting map and beam 
! Your choice of large map pixels excluded 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.7398 mas, bmaj=1.888 mas, bpa=-6.48 degrees
! Estimated noise=1.36329 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 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.9108 mas, bmaj=2.269 mas, bpa=-6.572 degrees
! Estimated noise=1.017 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 = 0.0126618 Jy
! Component: 100  -  total flux cleaned = 0.0161629 Jy
! Component: 150  -  total flux cleaned = 0.0176955 Jy
! Component: 200  -  total flux cleaned = 0.0183249 Jy
! Total flux subtracted in 200 components = 0.0183249 Jy
! Clean residual min=-0.005401 max=0.007932 Jy/beam
! Clean residual mean=0.000020 rms=0.001555 Jy/beam
! Combined flux in latest and established models = 0.0855751 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 21 model components to the UV plane model.
! The established model now contains 29 components and 0.0855751 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067869Jy  sigma=1.167133
! Fit after  self-cal, rms=0.067840Jy  sigma=1.166489
! Inverting map 
! Your choice of large map pixels excluded 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9108 x 2.269 at -6.572 degrees (North through East)
! Clean map  min=-0.0049972  max=0.071967 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
!  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 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: 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: 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=0.067840Jy  sigma=1.166489
! Fit after  self-cal, rms=0.067840Jy  sigma=1.166489
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=0.067840Jy  sigma=1.166489
! Fit after  self-cal, rms=0.067813Jy  sigma=1.165970
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.9108 mas, bmaj=2.269 mas, bpa=-6.572 degrees
! Estimated noise=1.017 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 (-14.8, 23).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0074022 Jy
! Component: 100  -  total flux cleaned = 0.00756466 Jy
! Component: 150  -  total flux cleaned = 0.00768612 Jy
! Component: 200  -  total flux cleaned = 0.00768597 Jy
! Total flux subtracted in 200 components = 0.00768597 Jy
! Clean residual min=-0.004664 max=0.006463 Jy/beam
! Clean residual mean=0.000023 rms=0.001383 Jy/beam
! Combined flux in latest and established models = 0.0932611 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 22 model components to the UV plane model.
! The established model now contains 50 components and 0.0932611 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067144Jy  sigma=1.150527
! Fit after  self-cal, rms=0.067069Jy  sigma=1.148482
! Inverting map 
! Your choice of large map pixels excluded 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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=0.067069Jy  sigma=1.148482
! Fit after  self-cal, rms=0.060489Jy  sigma=1.040045
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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 = 0.00252889 Jy
! Component: 100  -  total flux cleaned = 0.00267207 Jy
! Component: 150  -  total flux cleaned = 0.00221625 Jy
! Component: 200  -  total flux cleaned = 0.0018342 Jy
! Total flux subtracted in 200 components = 0.0018342 Jy
! Clean residual min=-0.004537 max=0.005304 Jy/beam
! Clean residual mean=0.000020 rms=0.001283 Jy/beam
! Combined flux in latest and established models = 0.0950953 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 22 model components to the UV plane model.
! The established model now contains 67 components and 0.0950953 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.060265Jy  sigma=1.031391
! Fit after  self-cal, rms=0.059620Jy  sigma=1.023768
! Inverting map 
! Your choice of large map pixels excluded 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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: 0.9108 x 2.269 at -6.572 degrees (North through East)
! Clean map  min=-0.0042723  max=0.074049 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
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 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=2.268 mas, bmaj=3.986 mas, bpa=-5.844 degrees
! Estimated noise=1.29156 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 = 0.000491313 Jy
! Component: 100  -  total flux cleaned = 0.000825649 Jy
! Component: 150  -  total flux cleaned = 0.000918972 Jy
! Component: 200  -  total flux cleaned = 0.000994347 Jy
! Total flux subtracted in 200 components = 0.000994347 Jy
! Clean residual min=-0.005126 max=0.006616 Jy/beam
! Clean residual mean=0.000039 rms=0.001697 Jy/beam
! Combined flux in latest and established models = 0.0960896 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 12 model components to the UV plane model.
! The established model now contains 77 components and 0.0960896 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.059631Jy  sigma=1.023677
! Fit after  self-cal, rms=0.059495Jy  sigma=1.022464
! Inverting map 
! Your choice of large map pixels excluded 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.7398 mas, bmaj=1.888 mas, bpa=-6.48 degrees
! Estimated noise=1.36329 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0635081 Jy
! Component: 100  -  total flux cleaned = 0.0783604 Jy
! Component: 150  -  total flux cleaned = 0.0863928 Jy
! Component: 200  -  total flux cleaned = 0.0913956 Jy
! Total flux subtracted in 200 components = 0.0913956 Jy
! Clean residual min=-0.006502 max=0.006111 Jy/beam
! Clean residual mean=0.000019 rms=0.001599 Jy/beam
! Combined flux in latest and established models = 0.0913956 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 28 model components to the UV plane model.
! The established model now contains 28 components and 0.0913956 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.9108 mas, bmaj=2.269 mas, bpa=-6.572 degrees
! Estimated noise=1.017 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 = 0.00361063 Jy
! Component: 100  -  total flux cleaned = 0.00395347 Jy
! Component: 150  -  total flux cleaned = 0.00414063 Jy
! Component: 200  -  total flux cleaned = 0.00414164 Jy
! Total flux subtracted in 200 components = 0.00414165 Jy
! Clean residual min=-0.004534 max=0.004914 Jy/beam
! Clean residual mean=0.000023 rms=0.001278 Jy/beam
! Combined flux in latest and established models = 0.0955373 Jy
! Adding 18 model components to the UV plane model.
! The established model now contains 40 components and 0.0955373 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=2.268 mas, bmaj=3.986 mas, bpa=-5.844 degrees
! Estimated noise=1.29156 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 = 0.000581361 Jy
! Component: 100  -  total flux cleaned = 0.000650637 Jy
! Component: 150  -  total flux cleaned = 0.000650295 Jy
! Component: 200  -  total flux cleaned = 0.000695586 Jy
! Total flux subtracted in 200 components = 0.000695586 Jy
! Clean residual min=-0.005124 max=0.006598 Jy/beam
! Clean residual mean=0.000041 rms=0.001696 Jy/beam
! Combined flux in latest and established models = 0.0962328 Jy
! Adding 18 model components to the UV plane model.
! The established model now contains 52 components and 0.0962329 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.9108 mas, bmaj=2.269 mas, bpa=-6.572 degrees
! Estimated noise=1.017 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.00028741 Jy
! Component: 100  -  total flux cleaned = -0.000536355 Jy
! Component: 150  -  total flux cleaned = -0.000755319 Jy
! Component: 200  -  total flux cleaned = -0.000905608 Jy
! Total flux subtracted in 200 components = -0.000905608 Jy
! Clean residual min=-0.004526 max=0.004764 Jy/beam
! Clean residual mean=0.000024 rms=0.001263 Jy/beam
! Combined flux in latest and established models = 0.0953273 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 17 model components to the UV plane model.
! The established model now contains 63 components and 0.0953273 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.059330Jy  sigma=1.019951
! Fit after  self-cal, rms=0.059282Jy  sigma=1.019351
wmodel J0335-0709_X_2005_07_08_yyk\_map.mod
! Writing 63 model components to file: J0335-0709_X_2005_07_08_yyk_map.mod
wobs J0335-0709_X_2005_07_08_yyk\_uvs.fits
! Writing UV FITS file: J0335-0709_X_2005_07_08_yyk_uvs.fits
wwins J0335-0709_X_2005_07_08_yyk\_map.win
! wwins: Wrote 2 windows to J0335-0709_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 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.000697775 Jy
! Component: 100  -  total flux cleaned = 0.000697654 Jy
! Component: 150  -  total flux cleaned = 0.000556526 Jy
! Component: 200  -  total flux cleaned = 0.000830289 Jy
! Component: 250  -  total flux cleaned = 0.00116092 Jy
! Component: 300  -  total flux cleaned = 0.00135261 Jy
! Component: 350  -  total flux cleaned = 0.00129123 Jy
! Component: 400  -  total flux cleaned = 0.00135117 Jy
! Component: 450  -  total flux cleaned = 0.00135059 Jy
! Component: 500  -  total flux cleaned = 0.00129314 Jy
! Component: 550  -  total flux cleaned = 0.00134794 Jy
! Component: 600  -  total flux cleaned = 0.00118539 Jy
! Component: 650  -  total flux cleaned = 0.00134516 Jy
! Component: 700  -  total flux cleaned = 0.00144824 Jy
! Component: 750  -  total flux cleaned = 0.00129423 Jy
! Component: 800  -  total flux cleaned = 0.00134537 Jy
! Component: 850  -  total flux cleaned = 0.00144389 Jy
! Component: 900  -  total flux cleaned = 0.00139477 Jy
! Component: 950  -  total flux cleaned = 0.00144256 Jy
! Component: 1000  -  total flux cleaned = 0.00139523 Jy
! Component: 1050  -  total flux cleaned = 0.00139481 Jy
! Component: 1100  -  total flux cleaned = 0.00130361 Jy
! Component: 1150  -  total flux cleaned = 0.00139291 Jy
! Component: 1200  -  total flux cleaned = 0.0012605 Jy
! Component: 1250  -  total flux cleaned = 0.00126002 Jy
! Component: 1300  -  total flux cleaned = 0.00113223 Jy
! Component: 1350  -  total flux cleaned = 0.00121712 Jy
! Component: 1400  -  total flux cleaned = 0.00117595 Jy
! Component: 1450  -  total flux cleaned = 0.00121682 Jy
! Component: 1500  -  total flux cleaned = 0.00105509 Jy
! Component: 1550  -  total flux cleaned = 0.00121478 Jy
! Component: 1600  -  total flux cleaned = 0.00101606 Jy
! Component: 1650  -  total flux cleaned = 0.0010552 Jy
! Component: 1700  -  total flux cleaned = 0.0009387 Jy
! Component: 1750  -  total flux cleaned = 0.00074801 Jy
! Component: 1800  -  total flux cleaned = 0.000635078 Jy
! Component: 1850  -  total flux cleaned = 0.000784364 Jy
! Component: 1900  -  total flux cleaned = 0.000525875 Jy
! Component: 1950  -  total flux cleaned = 0.000599054 Jy
! Component: 2000  -  total flux cleaned = 0.000526621 Jy
! Total flux subtracted in 2048 components = 0.000562718 Jy
! Clean residual min=-0.002169 max=0.002258 Jy/beam
! Clean residual mean=0.000012 rms=0.000699 Jy/beam
! Combined flux in latest and established models = 0.09589 Jy
keep
! Adding 151 model components to the UV plane model.
! The established model now contains 214 components and 0.09589 Jy
![Exited script file: muppet]
wmap "J0335-0709_X_2005_07_08_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9108 x 2.269 at -6.572 degrees (North through East)
! Clean map  min=-0.003225  max=0.072873 Jy/beam
! Writing clean map to FITS file: J0335-0709_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 0.0728731 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.386% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.00070445 
device "J0335-0709_X_2005_07_08_yyk\_map.eps/VPS"
! Attempting to open device: 'J0335-0709_X_2005_07_08_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -2.90004 2.90004 5.80009 11.6002 23.2003 46.4007 92.8014
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0021 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.072 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9108 x 2.269 at -6.572 degrees (North through East)
! Clean map  min=-0.003225  max=0.072873 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0335-0709_X_2005_07_08_yyk\_map.gif/gif"
! Attempting to open device: 'J0335-0709_X_2005_07_08_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J0335-0709_X_2005_07_08_yyk_uvs.log closed on Fri Jan 20 09:51:16 2006