! Started logfile: J0110-1648_S_2004_05_27_yyk_uvs.log on Wed Dec  7 01:02:49 2005
obs J0110-1648_S_2004_05_27_yyk_uve.fits
! Reading UV FITS file: J0110-1648_S_2004_05_27_yyk_uve.fits
! AN table 1: 22 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.430303 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J0110-1648
! 
! 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  2.23697e+09        8e+06          1        8e+06
!  02        2  2.26697e+09        8e+06          1        8e+06
!  03        3  2.35697e+09        8e+06          1        8e+06
!  04        4  2.37697e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 1388 lines of history.
! 
! Reading 1704 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 J0110-1648_S_2004_05_27_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 = 256x256 pixels with 1.00x1.00 milli-arcsec cellsize.
phase_soltime=phase_soltime1
print "uvstat(rms)=",uvstat(rms),"Jy"
! uvstat(rms)= 0.105788 Jy 
startmod ,phase_soltime
! Applying default point source starting model.
! Performing phase self-cal over 10 minute time intervals
! Adding 1 model components to the UV plane model.
! The established model now contains 1 components and 1 Jy
! 
! Correcting IF 1.
!  A total of 121 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 100 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 93 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 122 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.950186Jy  sigma=14.616661
! Fit after  self-cal, rms=0.947113Jy  sigma=14.588818
! clrmod: Cleared the established, tentative and continuum models.
! Redundant starting model cleared.
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 
! Estimated beam: bmin=6.038 mas, bmaj=18.49 mas, bpa=-5.08 degrees
! Estimated noise=2.69425 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 = 0.0485025 Jy
! Component: 100  -  total flux cleaned = 0.0591803 Jy
! Total flux subtracted in 100 components = 0.0591803 Jy
! Clean residual min=-0.008974 max=0.011161 Jy/beam
! Clean residual mean=-0.000040 rms=0.003031 Jy/beam
! Combined flux in latest and established models = 0.0591803 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 13 model components to the UV plane model.
! The established model now contains 13 components and 0.0591803 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.088743Jy  sigma=1.088376
! Fit after  self-cal, rms=0.088634Jy  sigma=1.086592
! Inverting map 
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 
! Estimated beam: bmin=9.101 mas, bmaj=20.63 mas, bpa=-4.077 degrees
! Estimated noise=1.38628 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 = 0.00943378 Jy
! Component: 100  -  total flux cleaned = 0.0129776 Jy
! Component: 150  -  total flux cleaned = 0.0144009 Jy
! Component: 200  -  total flux cleaned = 0.0145055 Jy
! Total flux subtracted in 200 components = 0.0145055 Jy
! Clean residual min=-0.005891 max=0.005085 Jy/beam
! Clean residual mean=-0.000108 rms=0.001620 Jy/beam
! Combined flux in latest and established models = 0.0736857 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 46 model components to the UV plane model.
! The established model now contains 57 components and 0.0736858 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.088284Jy  sigma=1.073641
! Fit after  self-cal, rms=0.088226Jy  sigma=1.072184
! Inverting map 
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
selflims ampcor_selflim
! 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.
!  A total of 9 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 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 6 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*    
! 
! 
! Fit before self-cal, rms=0.088226Jy  sigma=1.072184
! Fit after  self-cal, rms=0.088129Jy  sigma=1.075007
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=0.088129Jy  sigma=1.075007
! Fit after  self-cal, rms=0.088015Jy  sigma=1.073182
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=9.083 mas, bmaj=20.64 mas, bpa=-4.314 degrees
! Estimated noise=1.39465 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 = 0.000639891 Jy
! Component: 100  -  total flux cleaned = 0.000595445 Jy
! Component: 150  -  total flux cleaned = 0.000590436 Jy
! Component: 200  -  total flux cleaned = 0.000590107 Jy
! Total flux subtracted in 200 components = 0.000590107 Jy
! Clean residual min=-0.005428 max=0.004782 Jy/beam
! Clean residual mean=-0.000107 rms=0.001588 Jy/beam
! Combined flux in latest and established models = 0.0742759 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 14 model components to the UV plane model.
! The established model now contains 64 components and 0.0742758 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.088030Jy  sigma=1.072593
! Fit after  self-cal, rms=0.087973Jy  sigma=1.071534
! Inverting map 
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=0.087973Jy  sigma=1.071534
! Fit after  self-cal, rms=0.079919Jy  sigma=0.964548
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
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 = 0.00586407 Jy
! Component: 100  -  total flux cleaned = 0.00570117 Jy
! Component: 150  -  total flux cleaned = 0.00552201 Jy
! Component: 200  -  total flux cleaned = 0.00547719 Jy
! Total flux subtracted in 200 components = 0.00547719 Jy
! Clean residual min=-0.003921 max=0.004814 Jy/beam
! Clean residual mean=-0.000074 rms=0.001444 Jy/beam
! Combined flux in latest and established models = 0.079753 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 67 components and 0.079753 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.079402Jy  sigma=0.957051
! Fit after  self-cal, rms=0.078726Jy  sigma=0.950121
! Inverting map 
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: 9.083 x 20.64 at -4.314 degrees (North through East)
! Clean map  min=-0.0037496  max=0.068353 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 = 20 mega-wavelengths.
win_mult = win_mult * 1.4
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=11.14 mas, bmaj=21.47 mas, bpa=-0.2414 degrees
! Estimated noise=1.42687 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 = -0.00013662 Jy
! Component: 100  -  total flux cleaned = -0.00024215 Jy
! Component: 150  -  total flux cleaned = -0.000301035 Jy
! Component: 200  -  total flux cleaned = -0.000381883 Jy
! Total flux subtracted in 200 components = -0.000381883 Jy
! Clean residual min=-0.003675 max=0.004680 Jy/beam
! Clean residual mean=-0.000084 rms=0.001433 Jy/beam
! Combined flux in latest and established models = 0.0793712 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 17 model components to the UV plane model.
! The established model now contains 78 components and 0.0793711 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.078708Jy  sigma=0.949805
! Fit after  self-cal, rms=0.078687Jy  sigma=0.948998
! Inverting map 
uvtaper 0,0
! 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 
! Estimated beam: bmin=6.048 mas, bmaj=18.46 mas, bpa=-5.039 degrees
! Estimated noise=2.69213 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0587363 Jy
! Component: 100  -  total flux cleaned = 0.0696047 Jy
! Component: 150  -  total flux cleaned = 0.0738217 Jy
! Component: 200  -  total flux cleaned = 0.0749707 Jy
! Total flux subtracted in 200 components = 0.0749707 Jy
! Clean residual min=-0.006929 max=0.008522 Jy/beam
! Clean residual mean=0.000016 rms=0.002543 Jy/beam
! Combined flux in latest and established models = 0.0749707 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 15 model components to the UV plane model.
! The established model now contains 15 components and 0.0749707 Jy
! Inverting map and beam 
! Estimated beam: bmin=9.083 mas, bmaj=20.64 mas, bpa=-4.314 degrees
! Estimated noise=1.39465 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 = 0.00401179 Jy
! Component: 100  -  total flux cleaned = 0.00439726 Jy
! Component: 150  -  total flux cleaned = 0.00457292 Jy
! Component: 200  -  total flux cleaned = 0.00467195 Jy
! Total flux subtracted in 200 components = 0.00467195 Jy
! Clean residual min=-0.003726 max=0.004822 Jy/beam
! Clean residual mean=-0.000071 rms=0.001440 Jy/beam
! Combined flux in latest and established models = 0.0796427 Jy
! Adding 13 model components to the UV plane model.
! The established model now contains 28 components and 0.0796427 Jy
! Inverting map 
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 20 mega-wavelengths.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=11.14 mas, bmaj=21.47 mas, bpa=-0.2414 degrees
! Estimated noise=1.42687 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 = -0.00048194 Jy
! Component: 100  -  total flux cleaned = -0.000552011 Jy
! Component: 150  -  total flux cleaned = -0.000613494 Jy
! Component: 200  -  total flux cleaned = -0.000666059 Jy
! Total flux subtracted in 200 components = -0.000666059 Jy
! Clean residual min=-0.003549 max=0.004743 Jy/beam
! Clean residual mean=-0.000083 rms=0.001422 Jy/beam
! Combined flux in latest and established models = 0.0789766 Jy
! Adding 12 model components to the UV plane model.
! The established model now contains 36 components and 0.0789766 Jy
! Inverting map 
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Estimated beam: bmin=9.083 mas, bmaj=20.64 mas, bpa=-4.314 degrees
! Estimated noise=1.39465 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000272806 Jy
! Component: 100  -  total flux cleaned = 0.000402176 Jy
! Component: 150  -  total flux cleaned = 0.000520385 Jy
! Component: 200  -  total flux cleaned = 0.000626234 Jy
! Total flux subtracted in 200 components = 0.000626234 Jy
! Clean residual min=-0.003649 max=0.004758 Jy/beam
! Clean residual mean=-0.000069 rms=0.001396 Jy/beam
! Combined flux in latest and established models = 0.0796029 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 14 model components to the UV plane model.
! The established model now contains 43 components and 0.0796029 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.078661Jy  sigma=0.948837
! Fit after  self-cal, rms=0.078629Jy  sigma=0.948647
wmodel J0110-1648_S_2004_05_27_yyk\_map.mod
! Writing 43 model components to file: J0110-1648_S_2004_05_27_yyk_map.mod
wobs J0110-1648_S_2004_05_27_yyk\_uvs.fits
! Writing UV FITS file: J0110-1648_S_2004_05_27_yyk_uvs.fits
wwins J0110-1648_S_2004_05_27_yyk\_map.win
! wwins: Wrote 1 windows to J0110-1648_S_2004_05_27_yyk_map.win
x = (field_size-8) * field_cell / 4
addwin -x,x,-x,x
clean (field_size*4),0.01
! Inverting map 
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.00165776 Jy
! Component: 100  -  total flux cleaned = 0.00127994 Jy
! Component: 150  -  total flux cleaned = 0.00133392 Jy
! Component: 200  -  total flux cleaned = 0.00185239 Jy
! Component: 250  -  total flux cleaned = 0.00209624 Jy
! Component: 300  -  total flux cleaned = 0.0022366 Jy
! Component: 350  -  total flux cleaned = 0.00228149 Jy
! Component: 400  -  total flux cleaned = 0.00232611 Jy
! Component: 450  -  total flux cleaned = 0.00236831 Jy
! Component: 500  -  total flux cleaned = 0.00236912 Jy
! Component: 550  -  total flux cleaned = 0.00240879 Jy
! Component: 600  -  total flux cleaned = 0.00237123 Jy
! Component: 650  -  total flux cleaned = 0.00218917 Jy
! Component: 700  -  total flux cleaned = 0.00194177 Jy
! Component: 750  -  total flux cleaned = 0.00180325 Jy
! Component: 800  -  total flux cleaned = 0.00156611 Jy
! Component: 850  -  total flux cleaned = 0.00130242 Jy
! Component: 900  -  total flux cleaned = 0.00114138 Jy
! Component: 950  -  total flux cleaned = 0.00107737 Jy
! Component: 1000  -  total flux cleaned = 0.000859746 Jy
! Total flux subtracted in 1024 components = 0.000798589 Jy
! Clean residual min=-0.001956 max=0.002645 Jy/beam
! Clean residual mean=-0.000075 rms=0.000694 Jy/beam
! Combined flux in latest and established models = 0.0804014 Jy
keep
! Adding 53 model components to the UV plane model.
! The established model now contains 96 components and 0.0804015 Jy
![Exited script file: muppet]
wmap "J0110-1648_S_2004_05_27_yyk\_map.fits"
! Inverting map 
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 9.083 x 20.64 at -4.314 degrees (North through East)
! Clean map  min=-0.0032413  max=0.06879 Jy/beam
! Writing clean map to FITS file: J0110-1648_S_2004_05_27_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.0687899 
invert
! Inverting map 
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000671343 
device "J0110-1648_S_2004_05_27_yyk\_map.eps/VPS"
! Attempting to open device: 'J0110-1648_S_2004_05_27_yyk_map.eps/VPS'
loglevs 1*100*3*image_rms/peak_flux
! The new contour levels are:
!  -2.9278 2.9278 5.8556 11.7112 23.4224 46.8448 93.6896
print "clev=",int(1*3*image_rms*10000)/10000
! clev= 0.002 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.068 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 9.083 x 20.64 at -4.314 degrees (North through East)
! Clean map  min=-0.0032413  max=0.06879 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0110-1648_S_2004_05_27_yyk\_map.gif/gif"
! Attempting to open device: 'J0110-1648_S_2004_05_27_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J0110-1648_S_2004_05_27_yyk_uvs.log closed on Wed Dec  7 01:02:50 2005