! Started logfile: J1323-4452_X_2002_01_31_yyk_uvs.log on Wed Jun 27 10:57:47 2007
obs J1323-4452_X_2002_01_31_yyk_uva.fits
! Reading UV FITS file: J1323-4452_X_2002_01_31_yyk_uva.fits
! AN table 1: 39 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.439886 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J1323-4452
! 
! 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 3088 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 J1323-4452_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)= 0.22755 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 1.19% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.6383 mas, bmaj=1.746 mas, bpa=2.399 degrees
! Estimated noise=3676.41 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=100  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0573728 Jy
! Component: 100  -  total flux cleaned = 0.0846852 Jy
! Total flux subtracted in 100 components = 0.0846852 Jy
! Clean residual min=-0.014880 max=0.015358 Jy/beam
! Clean residual mean=-0.000499 rms=0.005966 Jy/beam
! Combined flux in latest and established models = 0.0846852 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 41 model components to the UV plane model.
! The established model now contains 41 components and 0.0846852 Jy
! 
! Correcting IF 1.
!  A total of 167 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 126 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 126 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 126 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.212039Jy  sigma=0.001525
! Fit after  self-cal, rms=0.211580Jy  sigma=0.001522
! Inverting map and beam 
! Your choice of large map pixels excluded 1.19% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.6383 mas, bmaj=1.746 mas, bpa=2.399 degrees
! Estimated noise=3676.46 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 1.19% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.8239 mas, bmaj=2.244 mas, bpa=-1.004 degrees
! Estimated noise=1785.74 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 = 0.0402517 Jy
! Component: 100  -  total flux cleaned = 0.0527034 Jy
! Component: 150  -  total flux cleaned = 0.0600543 Jy
! Component: 200  -  total flux cleaned = 0.0636649 Jy
! Total flux subtracted in 200 components = 0.0636649 Jy
! Clean residual min=-0.006499 max=0.006572 Jy/beam
! Clean residual mean=0.000006 rms=0.003162 Jy/beam
! Combined flux in latest and established models = 0.14835 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 100 model components to the UV plane model.
! The established model now contains 141 components and 0.14835 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.204839Jy  sigma=0.001461
! Fit after  self-cal, rms=0.204754Jy  sigma=0.001460
! Inverting map 
! Your choice of large map pixels excluded 1.19% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8239 x 2.244 at -1.004 degrees (North through East)
! Clean map  min=-0.015574  max=0.033675 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.
!  A total of 3 telescope corrections were flagged in sub-array 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 3.
!  A total of 3 telescope corrections were flagged in sub-array 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 4.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Amplitude normalization factor in sub-array 1: 1.01168
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.03     HN        1.00*    KP        0.99     
!   LA        0.93     MK        0.94     NL        1.00*    OV        0.96     
!   PT        1.02     SC        1.00     
! 
! 
! Fit before self-cal, rms=0.204754Jy  sigma=0.001460
! Fit after  self-cal, rms=0.204441Jy  sigma=0.001461
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=0.204441Jy  sigma=0.001461
! Fit after  self-cal, rms=0.204441Jy  sigma=0.001461
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 1.19% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.8223 mas, bmaj=2.248 mas, bpa=-1.41 degrees
! Estimated noise=1785.07 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 = 0.0050642 Jy
! Component: 100  -  total flux cleaned = 0.00948234 Jy
! Component: 150  -  total flux cleaned = 0.0138839 Jy
! Component: 200  -  total flux cleaned = 0.0174447 Jy
! Total flux subtracted in 200 components = 0.0174447 Jy
! Clean residual min=-0.003476 max=0.003516 Jy/beam
! Clean residual mean=0.000049 rms=0.001630 Jy/beam
! Combined flux in latest and established models = 0.165795 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 76 model components to the UV plane model.
! The established model now contains 208 components and 0.165795 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.203486Jy  sigma=0.001453
! Fit after  self-cal, rms=0.203452Jy  sigma=0.001453
! Inverting map 
! Your choice of large map pixels excluded 1.19% of the data.
!  The x-axis pixel size should ideally be below 0.199 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=0.203452Jy  sigma=0.001453
! Fit after  self-cal, rms=0.201925Jy  sigma=0.001442
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.19% of the data.
!  The x-axis pixel size should ideally be below 0.199 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 = 0.00108318 Jy
! Component: 100  -  total flux cleaned = 0.0051099 Jy
! Component: 150  -  total flux cleaned = 0.00863063 Jy
! Component: 200  -  total flux cleaned = 0.0111188 Jy
! Total flux subtracted in 200 components = 0.0111188 Jy
! Clean residual min=-0.002700 max=0.002716 Jy/beam
! Clean residual mean=0.000023 rms=0.001128 Jy/beam
! Combined flux in latest and established models = 0.176914 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 58 model components to the UV plane model.
! The established model now contains 262 components and 0.176914 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.201395Jy  sigma=0.001438
! Fit after  self-cal, rms=0.201237Jy  sigma=0.001437
! Inverting map 
! Your choice of large map pixels excluded 1.19% of the data.
!  The x-axis pixel size should ideally be below 0.199 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: 0.8223 x 2.248 at -1.41 degrees (North through East)
! Clean map  min=-0.011741  max=0.030818 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 1.19% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=3.106 mas, bmaj=12.08 mas, bpa=3.02 degrees
! Estimated noise=2330.09 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 = 0.00481785 Jy
! Component: 100  -  total flux cleaned = 0.00609734 Jy
! Component: 150  -  total flux cleaned = 0.0064047 Jy
! Component: 200  -  total flux cleaned = 0.00706399 Jy
! Total flux subtracted in 200 components = 0.00706399 Jy
! Clean residual min=-0.003195 max=0.003067 Jy/beam
! Clean residual mean=0.000025 rms=0.000941 Jy/beam
! Combined flux in latest and established models = 0.183977 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 49 model components to the UV plane model.
! The established model now contains 309 components and 0.183978 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.201207Jy  sigma=0.001436
! Fit after  self-cal, rms=0.201173Jy  sigma=0.001436
! Inverting map 
! Your choice of large map pixels excluded 1.19% of the data.
!  The x-axis pixel size should ideally be below 0.199 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 1.19% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.6382 mas, bmaj=1.744 mas, bpa=2.227 degrees
! Estimated noise=3708.61 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0522147 Jy
! Component: 100  -  total flux cleaned = 0.0786937 Jy
! Component: 150  -  total flux cleaned = 0.0880845 Jy
! Component: 200  -  total flux cleaned = 0.0974028 Jy
! Total flux subtracted in 200 components = 0.0974028 Jy
! Clean residual min=-0.010649 max=0.010598 Jy/beam
! Clean residual mean=-0.000261 rms=0.004489 Jy/beam
! Combined flux in latest and established models = 0.0974028 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 66 model components to the UV plane model.
! The established model now contains 66 components and 0.0974028 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 1.19% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.8223 mas, bmaj=2.248 mas, bpa=-1.41 degrees
! Estimated noise=1785.07 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 = 0.0263752 Jy
! Component: 100  -  total flux cleaned = 0.0376731 Jy
! Component: 150  -  total flux cleaned = 0.0427034 Jy
! Component: 200  -  total flux cleaned = 0.045788 Jy
! Total flux subtracted in 200 components = 0.045788 Jy
! Clean residual min=-0.005872 max=0.005883 Jy/beam
! Clean residual mean=0.000050 rms=0.002806 Jy/beam
! Combined flux in latest and established models = 0.143191 Jy
! Adding 92 model components to the UV plane model.
! The established model now contains 156 components and 0.143191 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.19% of the data.
!  The x-axis pixel size should ideally be below 0.199 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 1.19% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=3.106 mas, bmaj=12.08 mas, bpa=3.02 degrees
! Estimated noise=2330.09 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 = 0.00797902 Jy
! Component: 100  -  total flux cleaned = 0.00941675 Jy
! Component: 150  -  total flux cleaned = 0.012239 Jy
! Component: 200  -  total flux cleaned = 0.0149149 Jy
! Total flux subtracted in 200 components = 0.0149149 Jy
! Clean residual min=-0.003406 max=0.003429 Jy/beam
! Clean residual mean=0.000065 rms=0.001893 Jy/beam
! Combined flux in latest and established models = 0.158106 Jy
! Adding 113 model components to the UV plane model.
! The established model now contains 263 components and 0.158106 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.19% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 1.19% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.8223 mas, bmaj=2.248 mas, bpa=-1.41 degrees
! Estimated noise=1785.07 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00220147 Jy
! Component: 100  -  total flux cleaned = 0.00316852 Jy
! Component: 150  -  total flux cleaned = 0.00505048 Jy
! Component: 200  -  total flux cleaned = 0.00522058 Jy
! Total flux subtracted in 200 components = 0.00522058 Jy
! Clean residual min=-0.002377 max=0.002378 Jy/beam
! Clean residual mean=-0.000002 rms=0.000931 Jy/beam
! Combined flux in latest and established models = 0.163326 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 40 model components to the UV plane model.
! The established model now contains 300 components and 0.163326 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.200912Jy  sigma=0.001434
! Fit after  self-cal, rms=0.200772Jy  sigma=0.001433
wmodel J1323-4452_X_2002_01_31_yyk\_map.mod
! Writing 300 model components to file: J1323-4452_X_2002_01_31_yyk_map.mod
wobs J1323-4452_X_2002_01_31_yyk\_uvs.fits
! Applying 39 buffered edits.
! Writing UV FITS file: J1323-4452_X_2002_01_31_yyk_uvs.fits
wwins J1323-4452_X_2002_01_31_yyk\_map.win
! wwins: No CLEAN windows to write.
! Error occured in command: wwins
![Exited script file: muppet]
! 
wmap "J1323-4452_X_2002_01_31_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 1.19% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8223 x 2.248 at -1.41 degrees (North through East)
! Clean map  min=-0.0088114  max=0.022803 Jy/beam
! Writing clean map to FITS file: J1323-4452_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 0.0228032 
invert
! Inverting map 
! Your choice of large map pixels excluded 1.19% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000977622 
device "J1323-4452_X_2002_01_31_yyk\_map.eps/VPS"
! Attempting to open device: 'J1323-4452_X_2002_01_31_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -12.8616 12.8616 25.7232 51.4465
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0029 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.022 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8223 x 2.248 at -1.41 degrees (North through East)
! Clean map  min=-0.0088114  max=0.022803 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1323-4452_X_2002_01_31_yyk\_map.gif/gif"
! Attempting to open device: 'J1323-4452_X_2002_01_31_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1323-4452_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 10:57:51 2007