! Started logfile: J0903-3117_X_2002_05_14_yyk_uvs.log on Tue Jun 26 22:35:04 2007
obs J0903-3117_X_2002_05_14_yyk_uva.fits
! Reading UV FITS file: J0903-3117_X_2002_05_14_yyk_uva.fits
! AN table 1: 77 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.870418 visibilities/baseline/integration-bin.
! Found source: J0903-3117
! 
! 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 1076 lines of history.
! 
! Reading 12064 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 J0903-3117_X_2002_05_14_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)= 0.310847 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 0.277% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.6501 mas, bmaj=1.776 mas, bpa=4.343 degrees
! Estimated noise=1820.12 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 = 0.059366 Jy
! Component: 100  -  total flux cleaned = 0.0812637 Jy
! Total flux subtracted in 100 components = 0.0812637 Jy
! Clean residual min=-0.016539 max=0.017957 Jy/beam
! Clean residual mean=-0.000013 rms=0.004631 Jy/beam
! Combined flux in latest and established models = 0.0812637 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 0.0812637 Jy
! 
! Correcting IF 1.
!  A total of 72 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 55 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 55 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 55 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.300727Jy  sigma=0.001511
! Fit after  self-cal, rms=0.299958Jy  sigma=0.001505
! Inverting map and beam 
! Your choice of large map pixels excluded 0.277% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.6501 mas, bmaj=1.776 mas, bpa=4.343 degrees
! Estimated noise=1820.12 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 0.277% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8717 mas, bmaj=2.284 mas, bpa=5.845 degrees
! Estimated noise=991.678 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 = 0.0289115 Jy
! Component: 100  -  total flux cleaned = 0.0370662 Jy
! Component: 150  -  total flux cleaned = 0.0391385 Jy
! Component: 200  -  total flux cleaned = 0.0394266 Jy
! Total flux subtracted in 200 components = 0.0394266 Jy
! Clean residual min=-0.008537 max=0.012749 Jy/beam
! Clean residual mean=-0.000054 rms=0.002445 Jy/beam
! Combined flux in latest and established models = 0.12069 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 14 model components to the UV plane model.
! The established model now contains 25 components and 0.12069 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.299359Jy  sigma=0.001490
! Fit after  self-cal, rms=0.299336Jy  sigma=0.001489
! Inverting map 
! Your choice of large map pixels excluded 0.277% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8717 x 2.284 at 5.845 degrees (North through East)
! Clean map  min=-0.0080079  max=0.08603 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.
!  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*    NL        1.00*    OV        1.00*    PT        1.00*    
!   SC        1.00*    MK        1.00*    
! 
! 
! Correcting IF 2.
!  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*    NL        1.00*    OV        1.00*    PT        1.00*    
!   SC        1.00*    MK        1.00*    
! 
! 
! Correcting IF 3.
!  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*    NL        1.00*    OV        1.00*    PT        1.00*    
!   SC        1.00*    MK        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*    NL        1.00*    OV        1.00*    PT        1.00*    
!   SC        1.00*    MK        1.00*    
! 
! 
! Fit before self-cal, rms=0.299336Jy  sigma=0.001489
! Fit after  self-cal, rms=0.299359Jy  sigma=0.001489
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=0.299359Jy  sigma=0.001489
! Fit after  self-cal, rms=0.299339Jy  sigma=0.001489
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.278% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8727 mas, bmaj=2.285 mas, bpa=5.849 degrees
! Estimated noise=992.401 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 (1, -5.6).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0120436 Jy
! Component: 100  -  total flux cleaned = 0.0125572 Jy
! Component: 150  -  total flux cleaned = 0.0131061 Jy
! Component: 200  -  total flux cleaned = 0.0135967 Jy
! Total flux subtracted in 200 components = 0.0135967 Jy
! Clean residual min=-0.008886 max=0.010533 Jy/beam
! Clean residual mean=-0.000049 rms=0.002106 Jy/beam
! Combined flux in latest and established models = 0.134287 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 20 model components to the UV plane model.
! The established model now contains 43 components and 0.134287 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.298644Jy  sigma=0.001486
! Fit after  self-cal, rms=0.298593Jy  sigma=0.001485
! Inverting map 
! Your choice of large map pixels excluded 0.278% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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=0.298593Jy  sigma=0.001485
! Fit after  self-cal, rms=0.296400Jy  sigma=0.001472
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.278% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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 = 0.00614111 Jy
! Component: 100  -  total flux cleaned = 0.00701417 Jy
! Component: 150  -  total flux cleaned = 0.00735695 Jy
! Component: 200  -  total flux cleaned = 0.00746146 Jy
! Total flux subtracted in 200 components = 0.00746146 Jy
! Clean residual min=-0.007571 max=0.006805 Jy/beam
! Clean residual mean=-0.000035 rms=0.001800 Jy/beam
! Combined flux in latest and established models = 0.141749 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 18 model components to the UV plane model.
! The established model now contains 55 components and 0.141749 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.296237Jy  sigma=0.001471
! Fit after  self-cal, rms=0.295888Jy  sigma=0.001469
! Inverting map 
! Your choice of large map pixels excluded 0.278% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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: 0.8727 x 2.285 at 5.849 degrees (North through East)
! Clean map  min=-0.0066082  max=0.084792 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 0.278% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=2.303 mas, bmaj=7.325 mas, bpa=8.925 degrees
! Estimated noise=1254.49 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 = 0.00305698 Jy
! Component: 100  -  total flux cleaned = 0.0031076 Jy
! Component: 150  -  total flux cleaned = 0.00310844 Jy
! Component: 200  -  total flux cleaned = 0.00306779 Jy
! Total flux subtracted in 200 components = 0.00306779 Jy
! Clean residual min=-0.007656 max=0.006347 Jy/beam
! Clean residual mean=-0.000060 rms=0.002126 Jy/beam
! Combined flux in latest and established models = 0.144816 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 10 model components to the UV plane model.
! The established model now contains 64 components and 0.144816 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.295889Jy  sigma=0.001469
! Fit after  self-cal, rms=0.295697Jy  sigma=0.001468
! Inverting map 
! Your choice of large map pixels excluded 0.278% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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 0.278% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.6501 mas, bmaj=1.776 mas, bpa=4.343 degrees
! Estimated noise=1820.99 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0771487 Jy
! Component: 100  -  total flux cleaned = 0.101718 Jy
! Component: 150  -  total flux cleaned = 0.11515 Jy
! Component: 200  -  total flux cleaned = 0.121824 Jy
! Total flux subtracted in 200 components = 0.121824 Jy
! Clean residual min=-0.013067 max=0.013657 Jy/beam
! Clean residual mean=-0.000005 rms=0.003754 Jy/beam
! Combined flux in latest and established models = 0.121824 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 26 model components to the UV plane model.
! The established model now contains 26 components and 0.121824 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.278% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8727 mas, bmaj=2.285 mas, bpa=5.849 degrees
! Estimated noise=992.401 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 = 0.0153958 Jy
! Component: 100  -  total flux cleaned = 0.0205094 Jy
! Component: 150  -  total flux cleaned = 0.0206519 Jy
! Component: 200  -  total flux cleaned = 0.0206554 Jy
! Total flux subtracted in 200 components = 0.0206554 Jy
! Clean residual min=-0.007049 max=0.006676 Jy/beam
! Clean residual mean=-0.000032 rms=0.001749 Jy/beam
! Combined flux in latest and established models = 0.14248 Jy
! Adding 26 model components to the UV plane model.
! The established model now contains 49 components and 0.14248 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.278% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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 0.278% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=2.303 mas, bmaj=7.325 mas, bpa=8.925 degrees
! Estimated noise=1254.49 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 = 0.00231222 Jy
! Component: 100  -  total flux cleaned = 0.00225513 Jy
! Component: 150  -  total flux cleaned = 0.00225476 Jy
! Component: 200  -  total flux cleaned = 0.00220432 Jy
! Total flux subtracted in 200 components = 0.00220432 Jy
! Clean residual min=-0.008080 max=0.006769 Jy/beam
! Clean residual mean=-0.000063 rms=0.002127 Jy/beam
! Combined flux in latest and established models = 0.144684 Jy
! Adding 9 model components to the UV plane model.
! The established model now contains 57 components and 0.144684 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.278% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.278% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8727 mas, bmaj=2.285 mas, bpa=5.849 degrees
! Estimated noise=992.401 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.000632868 Jy
! Component: 100  -  total flux cleaned = -0.000714237 Jy
! Component: 150  -  total flux cleaned = -0.000866891 Jy
! Component: 200  -  total flux cleaned = -0.00107402 Jy
! Total flux subtracted in 200 components = -0.00107402 Jy
! Clean residual min=-0.007457 max=0.006408 Jy/beam
! Clean residual mean=-0.000032 rms=0.001718 Jy/beam
! Combined flux in latest and established models = 0.14361 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 22 model components to the UV plane model.
! The established model now contains 69 components and 0.14361 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.295638Jy  sigma=0.001468
! Fit after  self-cal, rms=0.295433Jy  sigma=0.001467
wmodel J0903-3117_X_2002_05_14_yyk\_map.mod
! Writing 69 model components to file: J0903-3117_X_2002_05_14_yyk_map.mod
wobs J0903-3117_X_2002_05_14_yyk\_uvs.fits
! Writing UV FITS file: J0903-3117_X_2002_05_14_yyk_uvs.fits
wwins J0903-3117_X_2002_05_14_yyk\_map.win
! wwins: Wrote 2 windows to J0903-3117_X_2002_05_14_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 0.278% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.000405722 Jy
! Component: 100  -  total flux cleaned = 0.00147963 Jy
! Component: 150  -  total flux cleaned = 0.00198018 Jy
! Component: 200  -  total flux cleaned = 0.00207717 Jy
! Component: 250  -  total flux cleaned = 0.00226155 Jy
! Component: 300  -  total flux cleaned = 0.00287917 Jy
! Component: 350  -  total flux cleaned = 0.0034738 Jy
! Component: 400  -  total flux cleaned = 0.00405712 Jy
! Component: 450  -  total flux cleaned = 0.00470617 Jy
! Component: 500  -  total flux cleaned = 0.00509932 Jy
! Component: 550  -  total flux cleaned = 0.00517493 Jy
! Component: 600  -  total flux cleaned = 0.00540127 Jy
! Component: 650  -  total flux cleaned = 0.00569833 Jy
! Component: 700  -  total flux cleaned = 0.00591738 Jy
! Component: 750  -  total flux cleaned = 0.00641935 Jy
! Component: 800  -  total flux cleaned = 0.00670093 Jy
! Component: 850  -  total flux cleaned = 0.00697844 Jy
! Component: 900  -  total flux cleaned = 0.00718427 Jy
! Component: 950  -  total flux cleaned = 0.00765445 Jy
! Component: 1000  -  total flux cleaned = 0.00805049 Jy
! Component: 1050  -  total flux cleaned = 0.0082452 Jy
! Component: 1100  -  total flux cleaned = 0.00805191 Jy
! Component: 1150  -  total flux cleaned = 0.0085605 Jy
! Component: 1200  -  total flux cleaned = 0.00843552 Jy
! Component: 1250  -  total flux cleaned = 0.00862297 Jy
! Component: 1300  -  total flux cleaned = 0.00862288 Jy
! Component: 1350  -  total flux cleaned = 0.0088052 Jy
! Component: 1400  -  total flux cleaned = 0.0088642 Jy
! Component: 1450  -  total flux cleaned = 0.00880459 Jy
! Component: 1500  -  total flux cleaned = 0.00915393 Jy
! Component: 1550  -  total flux cleaned = 0.00903743 Jy
! Component: 1600  -  total flux cleaned = 0.0089807 Jy
! Component: 1650  -  total flux cleaned = 0.00926284 Jy
! Component: 1700  -  total flux cleaned = 0.00942982 Jy
! Component: 1750  -  total flux cleaned = 0.00948528 Jy
! Component: 1800  -  total flux cleaned = 0.00948585 Jy
! Component: 1850  -  total flux cleaned = 0.00980905 Jy
! Component: 1900  -  total flux cleaned = 0.00980895 Jy
! Component: 1950  -  total flux cleaned = 0.00991548 Jy
! Component: 2000  -  total flux cleaned = 0.00975902 Jy
! Total flux subtracted in 2048 components = 0.0101736 Jy
! Clean residual min=-0.003474 max=0.003680 Jy/beam
! Clean residual mean=-0.000017 rms=0.000994 Jy/beam
! Combined flux in latest and established models = 0.153784 Jy
keep
! Adding 145 model components to the UV plane model.
! The established model now contains 214 components and 0.153784 Jy
![Exited script file: muppet]
wmap "J0903-3117_X_2002_05_14_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.278% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8727 x 2.285 at 5.849 degrees (North through East)
! Clean map  min=-0.0049267  max=0.084305 Jy/beam
! Writing clean map to FITS file: J0903-3117_X_2002_05_14_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.0843046 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.278% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000991204 
device "J0903-3117_X_2002_05_14_yyk\_map.eps/VPS"
! Attempting to open device: 'J0903-3117_X_2002_05_14_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -3.52722 3.52722 7.05445 14.1089 28.2178 56.4356
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0029 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.084 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8727 x 2.285 at 5.849 degrees (North through East)
! Clean map  min=-0.0049267  max=0.084305 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0903-3117_X_2002_05_14_yyk\_map.gif/gif"
! Attempting to open device: 'J0903-3117_X_2002_05_14_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J0903-3117_X_2002_05_14_yyk_uvs.log closed on Tue Jun 26 22:35:10 2007