! Started logfile: J0419-2132_X_2007_01_11_yyk_uvs.log on Mon Jun 16 19:15:04 2008
obs J0419-2132_X_2007_01_11_yyk_uve.fits
! Reading UV FITS file: J0419-2132_X_2007_01_11_yyk_uve.fits
! AN table 1: 17 integrations on 36 of 36 possible baselines.
! Apparent sampling: 0.736928 visibilities/baseline/integration-bin.
! Found source: J0419-2132
! 
! 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 2143 lines of history.
! 
! Reading 1804 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 J0419-2132_X_2007_01_11_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)= 0.117123 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 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.6412 mas, bmaj=1.726 mas, bpa=2.722 degrees
! Estimated noise=1.84874 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 = 0.0508308 Jy
! Component: 100  -  total flux cleaned = 0.0676255 Jy
! Total flux subtracted in 100 components = 0.0676255 Jy
! Clean residual min=-0.011750 max=0.012565 Jy/beam
! Clean residual mean=0.000004 rms=0.003292 Jy/beam
! Combined flux in latest and established models = 0.0676255 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 0.0676255 Jy
! 
! Correcting IF 1.
!  A total of 24 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 52 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 26 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 36 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.097339Jy  sigma=1.382713
! Fit after  self-cal, rms=0.089716Jy  sigma=1.224002
! Inverting map and beam 
! Your choice of large map pixels excluded 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.6413 mas, bmaj=1.726 mas, bpa=2.723 degrees
! Estimated noise=1.84818 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 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8237 mas, bmaj=2.076 mas, bpa=1.834 degrees
! Estimated noise=1.09416 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 = 0.0240519 Jy
! Component: 100  -  total flux cleaned = 0.0312952 Jy
! Component: 150  -  total flux cleaned = 0.0338757 Jy
! Component: 200  -  total flux cleaned = 0.0343616 Jy
! Total flux subtracted in 200 components = 0.0343616 Jy
! Clean residual min=-0.004489 max=0.004651 Jy/beam
! Clean residual mean=0.000042 rms=0.001271 Jy/beam
! Combined flux in latest and established models = 0.101987 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 22 model components to the UV plane model.
! The established model now contains 32 components and 0.101987 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.086789Jy  sigma=1.135135
! Fit after  self-cal, rms=0.086678Jy  sigma=1.133833
! Inverting map 
! Your choice of large map pixels excluded 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8237 x 2.076 at 1.834 degrees (North through East)
! Clean map  min=-0.0041273  max=0.076459 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: 1.00178
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.93     FD        0.95     HN        1.10     KP        1.03     
!   LA        1.01     MK        1.12     OV        0.94     PT        0.97     
!   SC        0.95     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.03411
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.10     FD        1.07     HN        0.91     KP        0.84     
!   LA        0.95     MK        0.96     OV        1.00*    PT        1.00     
!   SC        0.88     
! 
! 
! 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*    OV        1.00*    PT        1.00*    
!   SC        1.00*    
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 0.984498
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.88     FD        1.08     HN        1.00*    KP        0.99     
!   LA        1.06     MK        1.05     OV        1.02     PT        1.16     
!   SC        0.91     
! 
! 
! Fit before self-cal, rms=0.086678Jy  sigma=1.133833
! Fit after  self-cal, rms=0.086161Jy  sigma=1.126100
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=0.086161Jy  sigma=1.126100
! Fit after  self-cal, rms=0.086056Jy  sigma=1.124728
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8207 mas, bmaj=2.055 mas, bpa=4.024 degrees
! Estimated noise=1.09024 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 = 0.0010316 Jy
! Component: 100  -  total flux cleaned = 0.00115596 Jy
! Component: 150  -  total flux cleaned = 0.00115634 Jy
! Component: 200  -  total flux cleaned = 0.00112616 Jy
! Total flux subtracted in 200 components = 0.00112616 Jy
! Clean residual min=-0.004272 max=0.004524 Jy/beam
! Clean residual mean=0.000040 rms=0.001176 Jy/beam
! Combined flux in latest and established models = 0.103113 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 11 model components to the UV plane model.
! The established model now contains 36 components and 0.103113 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.085997Jy  sigma=1.124064
! Fit after  self-cal, rms=0.085910Jy  sigma=1.122972
! Inverting map 
! Your choice of large map pixels excluded 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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=0.085910Jy  sigma=1.122972
! Fit after  self-cal, rms=0.074886Jy  sigma=0.955909
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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 = 0.00477776 Jy
! Component: 100  -  total flux cleaned = 0.00396138 Jy
! Component: 150  -  total flux cleaned = 0.00355446 Jy
! Component: 200  -  total flux cleaned = 0.00318085 Jy
! Total flux subtracted in 200 components = 0.00318085 Jy
! Clean residual min=-0.003934 max=0.003867 Jy/beam
! Clean residual mean=0.000039 rms=0.001044 Jy/beam
! Combined flux in latest and established models = 0.106294 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 42 components and 0.106294 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.073955Jy  sigma=0.933140
! Fit after  self-cal, rms=0.071968Jy  sigma=0.918171
! Inverting map 
! Your choice of large map pixels excluded 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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: 0.8207 x 2.055 at 4.024 degrees (North through East)
! Clean map  min=-0.0040165  max=0.087345 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 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=2.378 mas, bmaj=5.646 mas, bpa=18.97 degrees
! Estimated noise=1.45012 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 = -0.000837965 Jy
! Component: 100  -  total flux cleaned = -0.000838743 Jy
! Component: 150  -  total flux cleaned = -0.000838362 Jy
! Component: 200  -  total flux cleaned = -0.000837879 Jy
! Total flux subtracted in 200 components = -0.000837879 Jy
! Clean residual min=-0.004254 max=0.003809 Jy/beam
! Clean residual mean=0.000077 rms=0.001363 Jy/beam
! Combined flux in latest and established models = 0.105456 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 44 components and 0.105456 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.071960Jy  sigma=0.917875
! Fit after  self-cal, rms=0.071119Jy  sigma=0.914087
! Inverting map 
! Your choice of large map pixels excluded 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.6412 mas, bmaj=1.717 mas, bpa=3.835 degrees
! Estimated noise=1.83344 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0747645 Jy
! Component: 100  -  total flux cleaned = 0.0900248 Jy
! Component: 150  -  total flux cleaned = 0.097361 Jy
! Component: 200  -  total flux cleaned = 0.101189 Jy
! Total flux subtracted in 200 components = 0.101189 Jy
! Clean residual min=-0.007915 max=0.007263 Jy/beam
! Clean residual mean=0.000019 rms=0.001871 Jy/beam
! Combined flux in latest and established models = 0.101189 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 18 model components to the UV plane model.
! The established model now contains 18 components and 0.101189 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8207 mas, bmaj=2.055 mas, bpa=4.024 degrees
! Estimated noise=1.09024 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 = 0.00318927 Jy
! Component: 100  -  total flux cleaned = 0.00383595 Jy
! Component: 150  -  total flux cleaned = 0.00399528 Jy
! Component: 200  -  total flux cleaned = 0.00404574 Jy
! Total flux subtracted in 200 components = 0.00404574 Jy
! Clean residual min=-0.004173 max=0.003711 Jy/beam
! Clean residual mean=0.000035 rms=0.001033 Jy/beam
! Combined flux in latest and established models = 0.105235 Jy
! Adding 14 model components to the UV plane model.
! The established model now contains 28 components and 0.105235 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=2.378 mas, bmaj=5.646 mas, bpa=18.97 degrees
! Estimated noise=1.45012 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 = 0.00012692 Jy
! Component: 100  -  total flux cleaned = 0.000129617 Jy
! Component: 150  -  total flux cleaned = 0.00012999 Jy
! Component: 200  -  total flux cleaned = 0.000129991 Jy
! Total flux subtracted in 200 components = 0.000129991 Jy
! Clean residual min=-0.004148 max=0.003893 Jy/beam
! Clean residual mean=0.000075 rms=0.001369 Jy/beam
! Combined flux in latest and established models = 0.105365 Jy
! Adding 6 model components to the UV plane model.
! The established model now contains 31 components and 0.105365 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8207 mas, bmaj=2.055 mas, bpa=4.024 degrees
! Estimated noise=1.09024 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -5.3303e-05 Jy
! Component: 100  -  total flux cleaned = -5.5401e-05 Jy
! Component: 150  -  total flux cleaned = -5.54786e-05 Jy
! Component: 200  -  total flux cleaned = -5.52523e-05 Jy
! Total flux subtracted in 200 components = -5.52523e-05 Jy
! Clean residual min=-0.004139 max=0.003738 Jy/beam
! Clean residual mean=0.000035 rms=0.001027 Jy/beam
! Combined flux in latest and established models = 0.105309 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 34 components and 0.105309 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.070985Jy  sigma=0.912303
! Fit after  self-cal, rms=0.070484Jy  sigma=0.910200
wmodel J0419-2132_X_2007_01_11_yyk\_map.mod
! Writing 34 model components to file: J0419-2132_X_2007_01_11_yyk_map.mod
wobs J0419-2132_X_2007_01_11_yyk\_uvs.fits
! Writing UV FITS file: J0419-2132_X_2007_01_11_yyk_uvs.fits
wwins J0419-2132_X_2007_01_11_yyk\_map.win
! wwins: Wrote 1 windows to J0419-2132_X_2007_01_11_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 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00105202 Jy
! Component: 100  -  total flux cleaned = -0.00117903 Jy
! Component: 150  -  total flux cleaned = -0.00136009 Jy
! Component: 200  -  total flux cleaned = -0.00170306 Jy
! Component: 250  -  total flux cleaned = -0.00208689 Jy
! Component: 300  -  total flux cleaned = -0.00239894 Jy
! Component: 350  -  total flux cleaned = -0.00264875 Jy
! Component: 400  -  total flux cleaned = -0.00294041 Jy
! Component: 450  -  total flux cleaned = -0.00308065 Jy
! Component: 500  -  total flux cleaned = -0.00303363 Jy
! Component: 550  -  total flux cleaned = -0.00290092 Jy
! Component: 600  -  total flux cleaned = -0.00277127 Jy
! Component: 650  -  total flux cleaned = -0.00277166 Jy
! Component: 700  -  total flux cleaned = -0.0027298 Jy
! Component: 750  -  total flux cleaned = -0.00276993 Jy
! Component: 800  -  total flux cleaned = -0.00276921 Jy
! Component: 850  -  total flux cleaned = -0.00280771 Jy
! Component: 900  -  total flux cleaned = -0.0028075 Jy
! Component: 950  -  total flux cleaned = -0.00288236 Jy
! Component: 1000  -  total flux cleaned = -0.00291857 Jy
! Component: 1050  -  total flux cleaned = -0.00299071 Jy
! Component: 1100  -  total flux cleaned = -0.00299056 Jy
! Component: 1150  -  total flux cleaned = -0.00302625 Jy
! Component: 1200  -  total flux cleaned = -0.0032346 Jy
! Component: 1250  -  total flux cleaned = -0.00326864 Jy
! Component: 1300  -  total flux cleaned = -0.00340356 Jy
! Component: 1350  -  total flux cleaned = -0.00343574 Jy
! Component: 1400  -  total flux cleaned = -0.00340256 Jy
! Component: 1450  -  total flux cleaned = -0.0034023 Jy
! Component: 1500  -  total flux cleaned = -0.00340243 Jy
! Component: 1550  -  total flux cleaned = -0.00343406 Jy
! Component: 1600  -  total flux cleaned = -0.00337226 Jy
! Component: 1650  -  total flux cleaned = -0.00340286 Jy
! Component: 1700  -  total flux cleaned = -0.00334252 Jy
! Component: 1750  -  total flux cleaned = -0.00328344 Jy
! Component: 1800  -  total flux cleaned = -0.00322476 Jy
! Component: 1850  -  total flux cleaned = -0.00316728 Jy
! Component: 1900  -  total flux cleaned = -0.0031678 Jy
! Component: 1950  -  total flux cleaned = -0.00311161 Jy
! Component: 2000  -  total flux cleaned = -0.00316726 Jy
! Total flux subtracted in 2048 components = -0.00311171 Jy
! Clean residual min=-0.001900 max=0.001485 Jy/beam
! Clean residual mean=0.000020 rms=0.000492 Jy/beam
! Combined flux in latest and established models = 0.102198 Jy
keep
! Adding 130 model components to the UV plane model.
! The established model now contains 164 components and 0.102198 Jy
![Exited script file: muppet]
wmap "J0419-2132_X_2007_01_11_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8207 x 2.055 at 4.024 degrees (North through East)
! Clean map  min=-0.0030145  max=0.088931 Jy/beam
! Writing clean map to FITS file: J0419-2132_X_2007_01_11_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.0889306 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.545% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000489226 
device "J0419-2132_X_2007_01_11_yyk\_map.eps/VPS"
! Attempting to open device: 'J0419-2132_X_2007_01_11_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -1.65036 1.65036 3.30073 6.60145 13.2029 26.4058 52.8116
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0014 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.088 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8207 x 2.055 at 4.024 degrees (North through East)
! Clean map  min=-0.0030145  max=0.088931 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0419-2132_X_2007_01_11_yyk\_map.gif/gif"
! Attempting to open device: 'J0419-2132_X_2007_01_11_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J0419-2132_X_2007_01_11_yyk_uvs.log closed on Mon Jun 16 19:15:10 2008