! Started logfile: J0800-3959_X_2002_01_31_yyk_uvs.log on Wed Jun 27 10:52:11 2007
obs J0800-3959_X_2002_01_31_yyk_uva.fits
! Reading UV FITS file: J0800-3959_X_2002_01_31_yyk_uva.fits
! AN table 1: 36 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.605556 visibilities/baseline/integration-bin.
! Found source: J0800-3959
! 
! 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 3924 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 J0800-3959_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)= 0.193026 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 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.6656 mas, bmaj=1.717 mas, bpa=5.035 degrees
! Estimated noise=2510.87 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 = 0.0690797 Jy
! Component: 100  -  total flux cleaned = 0.0938364 Jy
! Total flux subtracted in 100 components = 0.0938364 Jy
! Clean residual min=-0.011126 max=0.012346 Jy/beam
! Clean residual mean=-0.000025 rms=0.003363 Jy/beam
! Combined flux in latest and established models = 0.0938364 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 17 model components to the UV plane model.
! The established model now contains 17 components and 0.0938364 Jy
! 
! Correcting IF 1.
!  A total of 112 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 112 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 148 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 112 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.169282Jy  sigma=0.001327
! Fit after  self-cal, rms=0.169108Jy  sigma=0.001325
! Inverting map and beam 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.6656 mas, bmaj=1.717 mas, bpa=5.035 degrees
! Estimated noise=2510.87 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 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.847 mas, bmaj=2.227 mas, bpa=3.53 degrees
! Estimated noise=1652.89 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 = 0.0209503 Jy
! Component: 100  -  total flux cleaned = 0.0274152 Jy
! Component: 150  -  total flux cleaned = 0.0294285 Jy
! Component: 200  -  total flux cleaned = 0.0295274 Jy
! Total flux subtracted in 200 components = 0.0295274 Jy
! Clean residual min=-0.008687 max=0.007737 Jy/beam
! Clean residual mean=0.000028 rms=0.002538 Jy/beam
! Combined flux in latest and established models = 0.123364 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 21 model components to the UV plane model.
! The established model now contains 36 components and 0.123364 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.167690Jy  sigma=0.001312
! Fit after  self-cal, rms=0.167683Jy  sigma=0.001312
! Inverting map 
! Your choice of large map pixels excluded 1.21% 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: 0.847 x 2.227 at 3.53 degrees (North through East)
! Clean map  min=-0.0080383  max=0.078253 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.
!  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.
!  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=0.167683Jy  sigma=0.001312
! Fit after  self-cal, rms=0.167683Jy  sigma=0.001312
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=0.167683Jy  sigma=0.001312
! Fit after  self-cal, rms=0.167683Jy  sigma=0.001312
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.847 mas, bmaj=2.227 mas, bpa=3.53 degrees
! Estimated noise=1652.89 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 = 1.07562e-05 Jy
! Component: 100  -  total flux cleaned = 1.04556e-05 Jy
! Component: 150  -  total flux cleaned = 1.11053e-05 Jy
! Component: 200  -  total flux cleaned = -3.00409e-05 Jy
! Total flux subtracted in 200 components = -3.00409e-05 Jy
! Clean residual min=-0.008645 max=0.007555 Jy/beam
! Clean residual mean=0.000029 rms=0.002522 Jy/beam
! Combined flux in latest and established models = 0.123334 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 9 model components to the UV plane model.
! The established model now contains 39 components and 0.123334 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.167671Jy  sigma=0.001312
! Fit after  self-cal, rms=0.167670Jy  sigma=0.001312
! Inverting map 
! Your choice of large map pixels excluded 1.21% 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=0.167670Jy  sigma=0.001312
! Fit after  self-cal, rms=0.165702Jy  sigma=0.001296
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.21% 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 = 0.0014198 Jy
! Component: 100  -  total flux cleaned = 0.00122256 Jy
! Component: 150  -  total flux cleaned = 0.00109177 Jy
! Component: 200  -  total flux cleaned = 0.00101268 Jy
! Total flux subtracted in 200 components = 0.00101268 Jy
! Clean residual min=-0.008605 max=0.007955 Jy/beam
! Clean residual mean=0.000031 rms=0.002547 Jy/beam
! Combined flux in latest and established models = 0.124346 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 47 components and 0.124346 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.165468Jy  sigma=0.001294
! Fit after  self-cal, rms=0.164784Jy  sigma=0.001289
! Inverting map 
! Your choice of large map pixels excluded 1.21% 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: 0.847 x 2.227 at 3.53 degrees (North through East)
! Clean map  min=-0.0078674  max=0.085469 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 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=3.152 mas, bmaj=11.77 mas, bpa=5.595 degrees
! Estimated noise=2126.98 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 = 6.00417e-05 Jy
! Component: 100  -  total flux cleaned = 6.11496e-05 Jy
! Component: 150  -  total flux cleaned = 5.85935e-05 Jy
! Component: 200  -  total flux cleaned = 5.29758e-05 Jy
! Total flux subtracted in 200 components = 5.29758e-05 Jy
! Clean residual min=-0.009707 max=0.007037 Jy/beam
! Clean residual mean=0.000055 rms=0.003028 Jy/beam
! Combined flux in latest and established models = 0.124399 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 3 model components to the UV plane model.
! The established model now contains 49 components and 0.124399 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.164795Jy  sigma=0.001289
! Fit after  self-cal, rms=0.164686Jy  sigma=0.001289
! Inverting map 
! Your choice of large map pixels excluded 1.21% 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 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.6656 mas, bmaj=1.717 mas, bpa=5.035 degrees
! Estimated noise=2510.87 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0737935 Jy
! Component: 100  -  total flux cleaned = 0.09761 Jy
! Component: 150  -  total flux cleaned = 0.109967 Jy
! Component: 200  -  total flux cleaned = 0.116236 Jy
! Total flux subtracted in 200 components = 0.116236 Jy
! Clean residual min=-0.011543 max=0.013754 Jy/beam
! Clean residual mean=0.000032 rms=0.003826 Jy/beam
! Combined flux in latest and established models = 0.116236 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 24 model components to the UV plane model.
! The established model now contains 24 components and 0.116236 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.847 mas, bmaj=2.227 mas, bpa=3.53 degrees
! Estimated noise=1652.89 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 = 0.0076475 Jy
! Component: 100  -  total flux cleaned = 0.00818959 Jy
! Component: 150  -  total flux cleaned = 0.00847623 Jy
! Component: 200  -  total flux cleaned = 0.00847757 Jy
! Total flux subtracted in 200 components = 0.00847757 Jy
! Clean residual min=-0.008998 max=0.008711 Jy/beam
! Clean residual mean=0.000035 rms=0.002533 Jy/beam
! Combined flux in latest and established models = 0.124714 Jy
! Adding 10 model components to the UV plane model.
! The established model now contains 32 components and 0.124714 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.21% 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 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=3.152 mas, bmaj=11.77 mas, bpa=5.595 degrees
! Estimated noise=2126.98 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 = 0.00011719 Jy
! Component: 100  -  total flux cleaned = 0.000117908 Jy
! Component: 150  -  total flux cleaned = 0.000117605 Jy
! Component: 200  -  total flux cleaned = 0.00011718 Jy
! Total flux subtracted in 200 components = 0.00011718 Jy
! Clean residual min=-0.010192 max=0.006235 Jy/beam
! Clean residual mean=0.000061 rms=0.003007 Jy/beam
! Combined flux in latest and established models = 0.124831 Jy
! Adding 2 model components to the UV plane model.
! The established model now contains 34 components and 0.124831 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.21% 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 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.847 mas, bmaj=2.227 mas, bpa=3.53 degrees
! Estimated noise=1652.89 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.000115826 Jy
! Component: 100  -  total flux cleaned = -0.000115837 Jy
! Component: 150  -  total flux cleaned = -0.000113213 Jy
! Component: 200  -  total flux cleaned = -0.000110894 Jy
! Total flux subtracted in 200 components = -0.000110894 Jy
! Clean residual min=-0.008576 max=0.008611 Jy/beam
! Clean residual mean=0.000035 rms=0.002489 Jy/beam
! Combined flux in latest and established models = 0.12472 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 40 components and 0.12472 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.164677Jy  sigma=0.001289
! Fit after  self-cal, rms=0.164648Jy  sigma=0.001289
wmodel J0800-3959_X_2002_01_31_yyk\_map.mod
! Writing 40 model components to file: J0800-3959_X_2002_01_31_yyk_map.mod
wobs J0800-3959_X_2002_01_31_yyk\_uvs.fits
! Applying 36 buffered edits.
! Writing UV FITS file: J0800-3959_X_2002_01_31_yyk_uvs.fits
wwins J0800-3959_X_2002_01_31_yyk\_map.win
! wwins: Wrote 1 windows to J0800-3959_X_2002_01_31_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 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.000173269 Jy
! Component: 100  -  total flux cleaned = 0.000316145 Jy
! Component: 150  -  total flux cleaned = 7.42855e-05 Jy
! Component: 200  -  total flux cleaned = -0.000261427 Jy
! Component: 250  -  total flux cleaned = -0.000163077 Jy
! Component: 300  -  total flux cleaned = -0.000251134 Jy
! Component: 350  -  total flux cleaned = -0.000423951 Jy
! Component: 400  -  total flux cleaned = -0.000261437 Jy
! Component: 450  -  total flux cleaned = -0.000340138 Jy
! Component: 500  -  total flux cleaned = -0.000188171 Jy
! Component: 550  -  total flux cleaned = -3.67122e-05 Jy
! Component: 600  -  total flux cleaned = 0.000183163 Jy
! Component: 650  -  total flux cleaned = 0.000396596 Jy
! Component: 700  -  total flux cleaned = 0.00046642 Jy
! Component: 750  -  total flux cleaned = 0.000534359 Jy
! Component: 800  -  total flux cleaned = 0.000534099 Jy
! Component: 850  -  total flux cleaned = 0.000665807 Jy
! Component: 900  -  total flux cleaned = 0.000861581 Jy
! Component: 950  -  total flux cleaned = 0.00092616 Jy
! Component: 1000  -  total flux cleaned = 0.000990527 Jy
! Component: 1050  -  total flux cleaned = 0.00118159 Jy
! Component: 1100  -  total flux cleaned = 0.001245 Jy
! Component: 1150  -  total flux cleaned = 0.00143501 Jy
! Component: 1200  -  total flux cleaned = 0.00156123 Jy
! Component: 1250  -  total flux cleaned = 0.00162351 Jy
! Component: 1300  -  total flux cleaned = 0.00174916 Jy
! Component: 1350  -  total flux cleaned = 0.00181174 Jy
! Component: 1400  -  total flux cleaned = 0.00193723 Jy
! Component: 1450  -  total flux cleaned = 0.00199983 Jy
! Component: 1500  -  total flux cleaned = 0.00218705 Jy
! Component: 1550  -  total flux cleaned = 0.00212485 Jy
! Component: 1600  -  total flux cleaned = 0.00212519 Jy
! Component: 1650  -  total flux cleaned = 0.00206328 Jy
! Component: 1700  -  total flux cleaned = 0.00193785 Jy
! Component: 1750  -  total flux cleaned = 0.00187461 Jy
! Component: 1800  -  total flux cleaned = 0.00193825 Jy
! Component: 1850  -  total flux cleaned = 0.00200252 Jy
! Component: 1900  -  total flux cleaned = 0.00200252 Jy
! Component: 1950  -  total flux cleaned = 0.00200233 Jy
! Component: 2000  -  total flux cleaned = 0.00200276 Jy
! Total flux subtracted in 2048 components = 0.00200341 Jy
! Clean residual min=-0.004424 max=0.003707 Jy/beam
! Clean residual mean=-0.000023 rms=0.001150 Jy/beam
! Combined flux in latest and established models = 0.126724 Jy
keep
! Adding 88 model components to the UV plane model.
! The established model now contains 128 components and 0.126724 Jy
![Exited script file: muppet]
wmap "J0800-3959_X_2002_01_31_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 1.21% 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: 0.847 x 2.227 at 3.53 degrees (North through East)
! Clean map  min=-0.0078306  max=0.087158 Jy/beam
! Writing clean map to FITS file: J0800-3959_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 0.0871576 
invert
! Inverting map 
! Your choice of large map pixels excluded 1.21% 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 0.00107882 
device "J0800-3959_X_2002_01_31_yyk\_map.eps/VPS"
! Attempting to open device: 'J0800-3959_X_2002_01_31_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -3.71335 3.71335 7.42669 14.8534 29.7068 59.4135
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0032 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.087 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.847 x 2.227 at 3.53 degrees (North through East)
! Clean map  min=-0.0078306  max=0.087158 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0800-3959_X_2002_01_31_yyk\_map.gif/gif"
! Attempting to open device: 'J0800-3959_X_2002_01_31_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J0800-3959_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 10:52:17 2007