! Started logfile: J0637-3536_X_2002_01_31_yyk_uvs.log on Wed Jun 27 10:50:19 2007
obs J0637-3536_X_2002_01_31_yyk_uva.fits
! Reading UV FITS file: J0637-3536_X_2002_01_31_yyk_uva.fits
! AN table 1: 38 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.737427 visibilities/baseline/integration-bin.
! Found source: J0637-3536
! 
! 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 5044 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 J0637-3536_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)= 0.244842 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 1.37% of the data.
!  The x-axis pixel size should ideally be below 0.1993 milli-arcsec
! Estimated beam: bmin=0.6845 mas, bmaj=1.724 mas, bpa=4.004 degrees
! Estimated noise=2877.77 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 = 0.0263547 Jy
! Component: 100  -  total flux cleaned = 0.0216821 Jy
! Total flux subtracted in 100 components = 0.0216821 Jy
! Clean residual min=-0.010146 max=0.010115 Jy/beam
! Clean residual mean=0.000024 rms=0.003666 Jy/beam
! Combined flux in latest and established models = 0.0216821 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 34 model components to the UV plane model.
! The established model now contains 34 components and 0.0216821 Jy
! 
! Correcting IF 1.
!  A total of 380 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 89 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 161 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 89 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.240832Jy  sigma=0.001813
! Fit after  self-cal, rms=0.240679Jy  sigma=0.001811
! Inverting map and beam 
! Your choice of large map pixels excluded 1.37% of the data.
!  The x-axis pixel size should ideally be below 0.1993 milli-arcsec
! Estimated beam: bmin=0.6845 mas, bmaj=1.724 mas, bpa=4.003 degrees
! Estimated noise=2883.89 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 1.37% of the data.
!  The x-axis pixel size should ideally be below 0.1993 milli-arcsec
! Estimated beam: bmin=0.8817 mas, bmaj=2.264 mas, bpa=-1.743 degrees
! Estimated noise=1746.5 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 = -0.00291482 Jy
! Component: 100  -  total flux cleaned = -0.00713738 Jy
! Component: 150  -  total flux cleaned = -0.0102864 Jy
! Component: 200  -  total flux cleaned = -0.0112961 Jy
! Total flux subtracted in 200 components = -0.0112961 Jy
! Clean residual min=-0.003967 max=0.003964 Jy/beam
! Clean residual mean=0.000006 rms=0.001549 Jy/beam
! Combined flux in latest and established models = 0.0103859 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 51 model components to the UV plane model.
! The established model now contains 83 components and 0.0103859 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.239304Jy  sigma=0.001801
! Fit after  self-cal, rms=0.239224Jy  sigma=0.001801
! Inverting map 
! Your choice of large map pixels excluded 1.37% of the data.
!  The x-axis pixel size should ideally be below 0.1993 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8817 x 2.264 at -1.743 degrees (North through East)
! Clean map  min=-0.0080878  max=0.015546 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        0.00*    FD        0.00*    HN        0.00*    KP        0.00*    
!   LA        0.00*    MK        0.00*    NL        0.00*    OV        0.00*    
!   PT        0.00*    SC        0.00*    
! 
! 
! 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.
!  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.
!  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=0.239224Jy  sigma=0.001801
! Fit after  self-cal, rms=0.239268Jy  sigma=0.001801
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=0.239268Jy  sigma=0.001801
! Fit after  self-cal, rms=0.239266Jy  sigma=0.001801
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 1.37% of the data.
!  The x-axis pixel size should ideally be below 0.1993 milli-arcsec
! Estimated beam: bmin=0.8812 mas, bmaj=2.263 mas, bpa=-1.745 degrees
! Estimated noise=1747.62 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 = -0.00188786 Jy
! Component: 100  -  total flux cleaned = -0.00182948 Jy
! Component: 150  -  total flux cleaned = -0.00107817 Jy
! Component: 200  -  total flux cleaned = -0.000645498 Jy
! Total flux subtracted in 200 components = -0.000645498 Jy
! Clean residual min=-0.002578 max=0.002572 Jy/beam
! Clean residual mean=0.000021 rms=0.001028 Jy/beam
! Combined flux in latest and established models = 0.00974044 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 56 model components to the UV plane model.
! The established model now contains 129 components and 0.00974044 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.238745Jy  sigma=0.001798
! Fit after  self-cal, rms=0.238727Jy  sigma=0.001798
! Inverting map 
! Your choice of large map pixels excluded 1.37% of the data.
!  The x-axis pixel size should ideally be below 0.1993 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=0.238727Jy  sigma=0.001798
! Fit after  self-cal, rms=0.237715Jy  sigma=0.001788
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.37% of the data.
!  The x-axis pixel size should ideally be below 0.1993 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 = -0.000540072 Jy
! Component: 100  -  total flux cleaned = 0.000553093 Jy
! Component: 150  -  total flux cleaned = 0.00116305 Jy
! Component: 200  -  total flux cleaned = 0.00115459 Jy
! Total flux subtracted in 200 components = 0.00115459 Jy
! Clean residual min=-0.003251 max=0.003266 Jy/beam
! Clean residual mean=-0.000019 rms=0.001392 Jy/beam
! Combined flux in latest and established models = 0.010895 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 60 model components to the UV plane model.
! The established model now contains 186 components and 0.010895 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.236890Jy  sigma=0.001782
! Fit after  self-cal, rms=0.236596Jy  sigma=0.001779
! Inverting map 
! Your choice of large map pixels excluded 1.37% of the data.
!  The x-axis pixel size should ideally be below 0.1993 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: 0.8812 x 2.263 at -1.745 degrees (North through East)
! Clean map  min=-0.0092753  max=0.015508 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 1.37% of the data.
!  The x-axis pixel size should ideally be below 0.1993 milli-arcsec
! Estimated beam: bmin=3.065 mas, bmaj=9.934 mas, bpa=9.913 degrees
! Estimated noise=2201.86 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 = 0.00320515 Jy
! Component: 100  -  total flux cleaned = 0.00034606 Jy
! Component: 150  -  total flux cleaned = -0.00186276 Jy
! Component: 200  -  total flux cleaned = -0.00481321 Jy
! Total flux subtracted in 200 components = -0.00481321 Jy
! Clean residual min=-0.002957 max=0.002960 Jy/beam
! Clean residual mean=-0.000031 rms=0.001445 Jy/beam
! Combined flux in latest and established models = 0.00608183 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 56 model components to the UV plane model.
! The established model now contains 240 components and 0.00608183 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.236213Jy  sigma=0.001776
! Fit after  self-cal, rms=0.236012Jy  sigma=0.001775
! Inverting map 
! Your choice of large map pixels excluded 1.37% of the data.
!  The x-axis pixel size should ideally be below 0.1993 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 1.37% of the data.
!  The x-axis pixel size should ideally be below 0.1993 milli-arcsec
! Estimated beam: bmin=0.6845 mas, bmaj=1.724 mas, bpa=4.003 degrees
! Estimated noise=2884.07 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0191393 Jy
! Component: 100  -  total flux cleaned = 0.0211611 Jy
! Component: 150  -  total flux cleaned = 0.020425 Jy
! Component: 200  -  total flux cleaned = 0.0149518 Jy
! Total flux subtracted in 200 components = 0.0149518 Jy
! Clean residual min=-0.008069 max=0.008026 Jy/beam
! Clean residual mean=-0.000007 rms=0.003029 Jy/beam
! Combined flux in latest and established models = 0.0149519 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 65 model components to the UV plane model.
! The established model now contains 65 components and 0.0149519 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 1.37% of the data.
!  The x-axis pixel size should ideally be below 0.1993 milli-arcsec
! Estimated beam: bmin=0.8812 mas, bmaj=2.263 mas, bpa=-1.745 degrees
! Estimated noise=1747.62 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 = -0.00108595 Jy
! Component: 100  -  total flux cleaned = -0.00484303 Jy
! Component: 150  -  total flux cleaned = -0.00830763 Jy
! Component: 200  -  total flux cleaned = -0.0113399 Jy
! Total flux subtracted in 200 components = -0.0113399 Jy
! Clean residual min=-0.003994 max=0.003950 Jy/beam
! Clean residual mean=-0.000046 rms=0.001738 Jy/beam
! Combined flux in latest and established models = 0.00361191 Jy
! Adding 76 model components to the UV plane model.
! The established model now contains 141 components and 0.0036119 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.37% of the data.
!  The x-axis pixel size should ideally be below 0.1993 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 1.37% of the data.
!  The x-axis pixel size should ideally be below 0.1993 milli-arcsec
! Estimated beam: bmin=3.065 mas, bmaj=9.934 mas, bpa=9.913 degrees
! Estimated noise=2201.86 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 = -0.00447712 Jy
! Component: 100  -  total flux cleaned = -0.00670542 Jy
! Component: 150  -  total flux cleaned = -0.00809498 Jy
! Component: 200  -  total flux cleaned = -0.00965748 Jy
! Total flux subtracted in 200 components = -0.00965748 Jy
! Clean residual min=-0.003149 max=0.003087 Jy/beam
! Clean residual mean=-0.000012 rms=0.001537 Jy/beam
! Combined flux in latest and established models = -0.00604557 Jy
! Adding 53 model components to the UV plane model.
! The established model now contains 193 components and -0.00604558 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.37% of the data.
!  The x-axis pixel size should ideally be below 0.1993 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 1.37% of the data.
!  The x-axis pixel size should ideally be below 0.1993 milli-arcsec
! Estimated beam: bmin=0.8812 mas, bmaj=2.263 mas, bpa=-1.745 degrees
! Estimated noise=1747.62 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.00216917 Jy
! Component: 100  -  total flux cleaned = -0.00195716 Jy
! Component: 150  -  total flux cleaned = -0.00195374 Jy
! Component: 200  -  total flux cleaned = -0.00177663 Jy
! Total flux subtracted in 200 components = -0.00177663 Jy
! Clean residual min=-0.002113 max=0.002118 Jy/beam
! Clean residual mean=0.000008 rms=0.000829 Jy/beam
! Combined flux in latest and established models = -0.0078222 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 52 model components to the UV plane model.
! The established model now contains 243 components and -0.0078222 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.235801Jy  sigma=0.001772
! Fit after  self-cal, rms=0.235617Jy  sigma=0.001772
wmodel J0637-3536_X_2002_01_31_yyk\_map.mod
! Writing 243 model components to file: J0637-3536_X_2002_01_31_yyk_map.mod
wobs J0637-3536_X_2002_01_31_yyk\_uvs.fits
! Applying 38 buffered edits.
! Writing UV FITS file: J0637-3536_X_2002_01_31_yyk_uvs.fits
wwins J0637-3536_X_2002_01_31_yyk\_map.win
! wwins: No CLEAN windows to write.
! Error occured in command: wwins
![Exited script file: muppet]
! 
wmap "J0637-3536_X_2002_01_31_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 1.37% of the data.
!  The x-axis pixel size should ideally be below 0.1993 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8812 x 2.263 at -1.745 degrees (North through East)
! Clean map  min=-0.0071862  max=0.014407 Jy/beam
! Writing clean map to FITS file: J0637-3536_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 0.0144068 
invert
! Inverting map 
! Your choice of large map pixels excluded 1.37% of the data.
!  The x-axis pixel size should ideally be below 0.1993 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.00115723 
device "J0637-3536_X_2002_01_31_yyk\_map.eps/VPS"
! Attempting to open device: 'J0637-3536_X_2002_01_31_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -24.0977 24.0977 48.1954 96.3909
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0034 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.014 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8812 x 2.263 at -1.745 degrees (North through East)
! Clean map  min=-0.0071862  max=0.014407 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0637-3536_X_2002_01_31_yyk\_map.gif/gif"
! Attempting to open device: 'J0637-3536_X_2002_01_31_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J0637-3536_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 10:50:23 2007