! Started logfile: J2316-4337_X_2002_01_31_yyk_uvs.log on Wed Jun 27 11:05:52 2007
obs J2316-4337_X_2002_01_31_yyk_uva.fits
! Reading UV FITS file: J2316-4337_X_2002_01_31_yyk_uva.fits
! AN table 1: 37 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.446847 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J2316-4337
! 
! 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 2976 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 J2316-4337_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)= 0.27073 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 1.2% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.5978 mas, bmaj=1.784 mas, bpa=1.604 degrees
! Estimated noise=3245.73 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 = 0.0815593 Jy
! Component: 100  -  total flux cleaned = 0.110819 Jy
! Total flux subtracted in 100 components = 0.110819 Jy
! Clean residual min=-0.018351 max=0.018511 Jy/beam
! Clean residual mean=-0.000049 rms=0.005838 Jy/beam
! Combined flux in latest and established models = 0.110819 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 43 model components to the UV plane model.
! The established model now contains 43 components and 0.110819 Jy
! 
! Correcting IF 1.
!  A total of 117 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 154 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 117 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 117 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.239926Jy  sigma=0.001447
! Fit after  self-cal, rms=0.239567Jy  sigma=0.001445
! Inverting map and beam 
! Your choice of large map pixels excluded 1.2% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.5978 mas, bmaj=1.784 mas, bpa=1.604 degrees
! Estimated noise=3245.73 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 1.2% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.8138 mas, bmaj=2.208 mas, bpa=3.668 degrees
! Estimated noise=2078.26 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 = 0.0537264 Jy
! Component: 100  -  total flux cleaned = 0.08319 Jy
! Component: 150  -  total flux cleaned = 0.0910447 Jy
! Component: 200  -  total flux cleaned = 0.094563 Jy
! Total flux subtracted in 200 components = 0.094563 Jy
! Clean residual min=-0.006262 max=0.006253 Jy/beam
! Clean residual mean=-0.000059 rms=0.002646 Jy/beam
! Combined flux in latest and established models = 0.205383 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 94 model components to the UV plane model.
! The established model now contains 133 components and 0.205382 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.230690Jy  sigma=0.001378
! Fit after  self-cal, rms=0.230641Jy  sigma=0.001377
! Inverting map 
! Your choice of large map pixels excluded 1.2% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8138 x 2.208 at 3.668 degrees (North through East)
! Clean map  min=-0.010754  max=0.06723 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: 1.01595
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.88     HN        1.00*    KP        0.92     
!   LA        0.93     MK        1.00*    NL        1.00*    OV        1.04     
!   PT        0.98     SC        1.09     
! 
! 
! 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=0.230641Jy  sigma=0.001377
! Fit after  self-cal, rms=0.229999Jy  sigma=0.001376
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=0.229999Jy  sigma=0.001376
! Fit after  self-cal, rms=0.229997Jy  sigma=0.001376
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 1.2% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.8271 mas, bmaj=2.239 mas, bpa=3.273 degrees
! Estimated noise=2063.7 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 = -0.00501245 Jy
! Component: 100  -  total flux cleaned = -0.00801529 Jy
! Component: 150  -  total flux cleaned = -0.0103944 Jy
! Component: 200  -  total flux cleaned = -0.0133584 Jy
! Total flux subtracted in 200 components = -0.0133584 Jy
! Clean residual min=-0.003259 max=0.003297 Jy/beam
! Clean residual mean=-0.000010 rms=0.001367 Jy/beam
! Combined flux in latest and established models = 0.192024 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 58 model components to the UV plane model.
! The established model now contains 185 components and 0.192024 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.229357Jy  sigma=0.001372
! Fit after  self-cal, rms=0.229347Jy  sigma=0.001372
! Inverting map 
! Your choice of large map pixels excluded 1.2% of the data.
!  The x-axis pixel size should ideally be below 0.1988 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=0.229347Jy  sigma=0.001372
! Fit after  self-cal, rms=0.228289Jy  sigma=0.001365
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.2% of the data.
!  The x-axis pixel size should ideally be below 0.1988 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 = -0.00535567 Jy
! Component: 100  -  total flux cleaned = -0.0060168 Jy
! Component: 150  -  total flux cleaned = -0.00519109 Jy
! Component: 200  -  total flux cleaned = -0.00420803 Jy
! Total flux subtracted in 200 components = -0.00420803 Jy
! Clean residual min=-0.002946 max=0.002957 Jy/beam
! Clean residual mean=0.000017 rms=0.001115 Jy/beam
! Combined flux in latest and established models = 0.187816 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 45 model components to the UV plane model.
! The established model now contains 227 components and 0.187816 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.227692Jy  sigma=0.001361
! Fit after  self-cal, rms=0.227437Jy  sigma=0.001360
! Inverting map 
! Your choice of large map pixels excluded 1.2% of the data.
!  The x-axis pixel size should ideally be below 0.1988 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: 0.8271 x 2.239 at 3.273 degrees (North through East)
! Clean map  min=-0.010151  max=0.064723 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 1.2% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=3.057 mas, bmaj=12.29 mas, bpa=3.327 degrees
! Estimated noise=2680.61 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 = 0.00178612 Jy
! Component: 100  -  total flux cleaned = 0.00300218 Jy
! Component: 150  -  total flux cleaned = 0.00390598 Jy
! Component: 200  -  total flux cleaned = 0.00373602 Jy
! Total flux subtracted in 200 components = 0.00373602 Jy
! Clean residual min=-0.002144 max=0.002149 Jy/beam
! Clean residual mean=0.000037 rms=0.000812 Jy/beam
! Combined flux in latest and established models = 0.191552 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 41 model components to the UV plane model.
! The established model now contains 265 components and 0.191552 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.227393Jy  sigma=0.001359
! Fit after  self-cal, rms=0.227323Jy  sigma=0.001359
! Inverting map 
! Your choice of large map pixels excluded 1.2% of the data.
!  The x-axis pixel size should ideally be below 0.1988 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 1.2% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.5999 mas, bmaj=1.79 mas, bpa=1.345 degrees
! Estimated noise=3261.86 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0797447 Jy
! Component: 100  -  total flux cleaned = 0.105568 Jy
! Component: 150  -  total flux cleaned = 0.120175 Jy
! Component: 200  -  total flux cleaned = 0.129162 Jy
! Total flux subtracted in 200 components = 0.129162 Jy
! Clean residual min=-0.010929 max=0.010938 Jy/beam
! Clean residual mean=-0.000098 rms=0.004249 Jy/beam
! Combined flux in latest and established models = 0.129162 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 68 model components to the UV plane model.
! The established model now contains 68 components and 0.129162 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 1.2% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.8271 mas, bmaj=2.239 mas, bpa=3.273 degrees
! Estimated noise=2063.7 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 = 0.0352433 Jy
! Component: 100  -  total flux cleaned = 0.044339 Jy
! Component: 150  -  total flux cleaned = 0.0460703 Jy
! Component: 200  -  total flux cleaned = 0.0450984 Jy
! Total flux subtracted in 200 components = 0.0450984 Jy
! Clean residual min=-0.005366 max=0.005380 Jy/beam
! Clean residual mean=-0.000113 rms=0.002261 Jy/beam
! Combined flux in latest and established models = 0.17426 Jy
! Adding 78 model components to the UV plane model.
! The established model now contains 145 components and 0.17426 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.2% of the data.
!  The x-axis pixel size should ideally be below 0.1988 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 1.2% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=3.057 mas, bmaj=12.29 mas, bpa=3.327 degrees
! Estimated noise=2680.61 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 = 0.00827453 Jy
! Component: 100  -  total flux cleaned = 0.0106157 Jy
! Component: 150  -  total flux cleaned = 0.0115671 Jy
! Component: 200  -  total flux cleaned = 0.0119418 Jy
! Total flux subtracted in 200 components = 0.0119418 Jy
! Clean residual min=-0.002350 max=0.002389 Jy/beam
! Clean residual mean=-0.000023 rms=0.001136 Jy/beam
! Combined flux in latest and established models = 0.186202 Jy
! Adding 66 model components to the UV plane model.
! The established model now contains 205 components and 0.186202 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.2% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 1.2% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.8271 mas, bmaj=2.239 mas, bpa=3.273 degrees
! Estimated noise=2063.7 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000148714 Jy
! Component: 100  -  total flux cleaned = 0.000181379 Jy
! Component: 150  -  total flux cleaned = 0.0012494 Jy
! Component: 200  -  total flux cleaned = 0.00164938 Jy
! Total flux subtracted in 200 components = 0.00164938 Jy
! Clean residual min=-0.002396 max=0.002401 Jy/beam
! Clean residual mean=0.000028 rms=0.000851 Jy/beam
! Combined flux in latest and established models = 0.187852 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 47 model components to the UV plane model.
! The established model now contains 250 components and 0.187852 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.227156Jy  sigma=0.001357
! Fit after  self-cal, rms=0.227040Jy  sigma=0.001357
wmodel J2316-4337_X_2002_01_31_yyk\_map.mod
! Writing 250 model components to file: J2316-4337_X_2002_01_31_yyk_map.mod
wobs J2316-4337_X_2002_01_31_yyk\_uvs.fits
! Applying 37 buffered edits.
! Writing UV FITS file: J2316-4337_X_2002_01_31_yyk_uvs.fits
wwins J2316-4337_X_2002_01_31_yyk\_map.win
! wwins: No CLEAN windows to write.
! Error occured in command: wwins
![Exited script file: muppet]
! 
wmap "J2316-4337_X_2002_01_31_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 1.2% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8271 x 2.239 at 3.273 degrees (North through East)
! Clean map  min=-0.0082954  max=0.050975 Jy/beam
! Writing clean map to FITS file: J2316-4337_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 0.0509753 
invert
! Inverting map 
! Your choice of large map pixels excluded 1.2% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.00106639 
device "J2316-4337_X_2002_01_31_yyk\_map.eps/VPS"
! Attempting to open device: 'J2316-4337_X_2002_01_31_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -6.27592 6.27592 12.5518 25.1037 50.2073
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0031 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.05 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8271 x 2.239 at 3.273 degrees (North through East)
! Clean map  min=-0.0082954  max=0.050975 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J2316-4337_X_2002_01_31_yyk\_map.gif/gif"
! Attempting to open device: 'J2316-4337_X_2002_01_31_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J2316-4337_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 11:05:56 2007