! Started logfile: J1238-3825_X_2002_05_14_yyk_uvs.log on Tue Jun 26 22:46:28 2007
obs J1238-3825_X_2002_05_14_yyk_uva.fits
! Reading UV FITS file: J1238-3825_X_2002_05_14_yyk_uva.fits
! AN table 1: 38 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.768421 visibilities/baseline/integration-bin.
! Found source: J1238-3825
! 
! 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 5256 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 J1238-3825_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)= 0.339536 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 0.958% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.6849 mas, bmaj=1.822 mas, bpa=-1.081 degrees
! Estimated noise=2678.01 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 = 0.0638332 Jy
! Component: 100  -  total flux cleaned = 0.0856098 Jy
! Total flux subtracted in 100 components = 0.0856098 Jy
! Clean residual min=-0.021167 max=0.026348 Jy/beam
! Clean residual mean=0.000026 rms=0.006610 Jy/beam
! Combined flux in latest and established models = 0.0856098 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 20 model components to the UV plane model.
! The established model now contains 20 components and 0.0856098 Jy
! 
! Correcting IF 1.
!  A total of 380 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 46 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 83 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 46 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.329971Jy  sigma=0.001794
! Fit after  self-cal, rms=0.328729Jy  sigma=0.001787
! Inverting map and beam 
! Your choice of large map pixels excluded 0.958% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.6849 mas, bmaj=1.822 mas, bpa=-1.081 degrees
! Estimated noise=2678.01 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 0.958% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.8369 mas, bmaj=2.201 mas, bpa=-0.3132 degrees
! Estimated noise=1773.14 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 = 0.02503 Jy
! Component: 100  -  total flux cleaned = 0.0325972 Jy
! Component: 150  -  total flux cleaned = 0.0350356 Jy
! Component: 200  -  total flux cleaned = 0.0354701 Jy
! Total flux subtracted in 200 components = 0.0354701 Jy
! Clean residual min=-0.012200 max=0.014527 Jy/beam
! Clean residual mean=-0.000042 rms=0.004200 Jy/beam
! Combined flux in latest and established models = 0.12108 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 23 model components to the UV plane model.
! The established model now contains 38 components and 0.12108 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.328143Jy  sigma=0.001778
! Fit after  self-cal, rms=0.328157Jy  sigma=0.001778
! Inverting map 
! Your choice of large map pixels excluded 0.958% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8369 x 2.201 at -0.3132 degrees (North through East)
! Clean map  min=-0.011822  max=0.081968 Jy/beam
if(peak(flux) < thresh*2)
  selflims ampcor_selflim
  end if
! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2.
! Selfcal phase corrections will not be limited.
gscale
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Amplitude normalization factor in sub-array 1: 1
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.00*    FD        0.00*    HN        0.00*    KP        0.00*    
!   LA        0.00*    NL        0.00*    OV        0.00*    PT        0.00*    
!   SC        0.00*    MK        0.00*    
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    NL        1.00*    OV        1.00*    PT        1.00*    
!   SC        1.00*    MK        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*    NL        1.00*    OV        1.00*    PT        1.00*    
!   SC        1.00*    MK        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*    NL        1.00*    OV        1.00*    PT        1.00*    
!   SC        1.00*    MK        1.00*    
! 
! 
! Fit before self-cal, rms=0.328157Jy  sigma=0.001778
! Fit after  self-cal, rms=0.328273Jy  sigma=0.001778
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=0.328273Jy  sigma=0.001778
! Fit after  self-cal, rms=0.328273Jy  sigma=0.001778
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.959% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.8369 mas, bmaj=2.202 mas, bpa=-0.2739 degrees
! Estimated noise=1774.21 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 = 0.000435998 Jy
! Component: 100  -  total flux cleaned = 0.000386648 Jy
! Component: 150  -  total flux cleaned = 0.000385578 Jy
! Component: 200  -  total flux cleaned = 0.00038593 Jy
! Total flux subtracted in 200 components = 0.00038593 Jy
! Clean residual min=-0.012172 max=0.014361 Jy/beam
! Clean residual mean=-0.000009 rms=0.004208 Jy/beam
! Combined flux in latest and established models = 0.121466 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 10 model components to the UV plane model.
! The established model now contains 43 components and 0.121466 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.328265Jy  sigma=0.001778
! Fit after  self-cal, rms=0.328282Jy  sigma=0.001778
! Inverting map 
! Your choice of large map pixels excluded 0.959% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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=0.328282Jy  sigma=0.001778
! Fit after  self-cal, rms=0.325357Jy  sigma=0.001762
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.959% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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 = 0.00703707 Jy
! Component: 100  -  total flux cleaned = 0.00706563 Jy
! Component: 150  -  total flux cleaned = 0.00699139 Jy
! Component: 200  -  total flux cleaned = 0.0068584 Jy
! Total flux subtracted in 200 components = 0.0068584 Jy
! Clean residual min=-0.009852 max=0.011857 Jy/beam
! Clean residual mean=-0.000031 rms=0.003606 Jy/beam
! Combined flux in latest and established models = 0.128324 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 48 components and 0.128324 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.325296Jy  sigma=0.001761
! Fit after  self-cal, rms=0.324641Jy  sigma=0.001758
! Inverting map 
! Your choice of large map pixels excluded 0.959% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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: 0.8369 x 2.202 at -0.2739 degrees (North through East)
! Clean map  min=-0.0098355  max=0.090344 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 0.959% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=2.655 mas, bmaj=10.29 mas, bpa=3.565 degrees
! Estimated noise=2280.22 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 = 0.00269318 Jy
! Component: 100  -  total flux cleaned = 0.00269262 Jy
! Component: 150  -  total flux cleaned = 0.00269321 Jy
! Component: 200  -  total flux cleaned = 0.00269424 Jy
! Total flux subtracted in 200 components = 0.00269424 Jy
! Clean residual min=-0.012907 max=0.013640 Jy/beam
! Clean residual mean=-0.000187 rms=0.004817 Jy/beam
! Combined flux in latest and established models = 0.131018 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 48 components and 0.131018 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.324641Jy  sigma=0.001758
! Fit after  self-cal, rms=0.324241Jy  sigma=0.001756
! Inverting map 
! Your choice of large map pixels excluded 0.959% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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 0.959% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.6849 mas, bmaj=1.822 mas, bpa=-1.08 degrees
! Estimated noise=2678.38 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0811909 Jy
! Component: 100  -  total flux cleaned = 0.107559 Jy
! Component: 150  -  total flux cleaned = 0.119651 Jy
! Component: 200  -  total flux cleaned = 0.125299 Jy
! Total flux subtracted in 200 components = 0.125299 Jy
! Clean residual min=-0.015280 max=0.016661 Jy/beam
! Clean residual mean=-0.000073 rms=0.004603 Jy/beam
! Combined flux in latest and established models = 0.125299 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 19 model components to the UV plane model.
! The established model now contains 19 components and 0.125299 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.959% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.8369 mas, bmaj=2.202 mas, bpa=-0.2739 degrees
! Estimated noise=1774.21 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 = 0.00587876 Jy
! Component: 100  -  total flux cleaned = 0.00663537 Jy
! Component: 150  -  total flux cleaned = 0.00669495 Jy
! Component: 200  -  total flux cleaned = 0.00669492 Jy
! Total flux subtracted in 200 components = 0.00669492 Jy
! Clean residual min=-0.011301 max=0.012546 Jy/beam
! Clean residual mean=-0.000123 rms=0.003594 Jy/beam
! Combined flux in latest and established models = 0.131994 Jy
! Adding 8 model components to the UV plane model.
! The established model now contains 27 components and 0.131994 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.959% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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 0.959% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=2.655 mas, bmaj=10.29 mas, bpa=3.565 degrees
! Estimated noise=2280.22 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 = 0.000781373 Jy
! Component: 100  -  total flux cleaned = 0.000779275 Jy
! Component: 150  -  total flux cleaned = 0.000820985 Jy
! Component: 200  -  total flux cleaned = 0.000856105 Jy
! Total flux subtracted in 200 components = 0.000856105 Jy
! Clean residual min=-0.014315 max=0.014120 Jy/beam
! Clean residual mean=-0.000254 rms=0.004849 Jy/beam
! Combined flux in latest and established models = 0.13285 Jy
! Adding 4 model components to the UV plane model.
! The established model now contains 29 components and 0.13285 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.959% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.959% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.8369 mas, bmaj=2.202 mas, bpa=-0.2739 degrees
! Estimated noise=1774.21 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.00059957 Jy
! Component: 100  -  total flux cleaned = -0.000653708 Jy
! Component: 150  -  total flux cleaned = -0.000689729 Jy
! Component: 200  -  total flux cleaned = -0.000757385 Jy
! Total flux subtracted in 200 components = -0.000757385 Jy
! Clean residual min=-0.011293 max=0.012474 Jy/beam
! Clean residual mean=-0.000123 rms=0.003585 Jy/beam
! Combined flux in latest and established models = 0.132093 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 10 model components to the UV plane model.
! The established model now contains 35 components and 0.132093 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.324177Jy  sigma=0.001756
! Fit after  self-cal, rms=0.323968Jy  sigma=0.001755
wmodel J1238-3825_X_2002_05_14_yyk\_map.mod
! Writing 35 model components to file: J1238-3825_X_2002_05_14_yyk_map.mod
wobs J1238-3825_X_2002_05_14_yyk\_uvs.fits
! Writing UV FITS file: J1238-3825_X_2002_05_14_yyk_uvs.fits
wwins J1238-3825_X_2002_05_14_yyk\_map.win
! wwins: Wrote 1 windows to J1238-3825_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 0.959% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.00492227 Jy
! Component: 100  -  total flux cleaned = 0.00866788 Jy
! Component: 150  -  total flux cleaned = 0.0121269 Jy
! Component: 200  -  total flux cleaned = 0.0141511 Jy
! Component: 250  -  total flux cleaned = 0.014148 Jy
! Component: 300  -  total flux cleaned = 0.0138473 Jy
! Component: 350  -  total flux cleaned = 0.013558 Jy
! Component: 400  -  total flux cleaned = 0.0129968 Jy
! Component: 450  -  total flux cleaned = 0.0125918 Jy
! Component: 500  -  total flux cleaned = 0.0118084 Jy
! Component: 550  -  total flux cleaned = 0.0113037 Jy
! Component: 600  -  total flux cleaned = 0.0105669 Jy
! Component: 650  -  total flux cleaned = 0.0103284 Jy
! Component: 700  -  total flux cleaned = 0.00950963 Jy
! Component: 750  -  total flux cleaned = 0.00905567 Jy
! Component: 800  -  total flux cleaned = 0.00860858 Jy
! Component: 850  -  total flux cleaned = 0.00784454 Jy
! Component: 900  -  total flux cleaned = 0.00731167 Jy
! Component: 950  -  total flux cleaned = 0.00679024 Jy
! Component: 1000  -  total flux cleaned = 0.00628078 Jy
! Component: 1050  -  total flux cleaned = 0.00588096 Jy
! Component: 1100  -  total flux cleaned = 0.00519685 Jy
! Component: 1150  -  total flux cleaned = 0.00481324 Jy
! Component: 1200  -  total flux cleaned = 0.00443731 Jy
! Component: 1250  -  total flux cleaned = 0.00397673 Jy
! Component: 1300  -  total flux cleaned = 0.00379651 Jy
! Component: 1350  -  total flux cleaned = 0.00335187 Jy
! Component: 1400  -  total flux cleaned = 0.00317723 Jy
! Component: 1450  -  total flux cleaned = 0.00292051 Jy
! Component: 1500  -  total flux cleaned = 0.00275175 Jy
! Component: 1550  -  total flux cleaned = 0.00250489 Jy
! Component: 1600  -  total flux cleaned = 0.00242481 Jy
! Component: 1650  -  total flux cleaned = 0.00226512 Jy
! Component: 1700  -  total flux cleaned = 0.002344 Jy
! Component: 1750  -  total flux cleaned = 0.00226529 Jy
! Component: 1800  -  total flux cleaned = 0.00257011 Jy
! Component: 1850  -  total flux cleaned = 0.00287276 Jy
! Component: 1900  -  total flux cleaned = 0.00332264 Jy
! Component: 1950  -  total flux cleaned = 0.00376842 Jy
! Component: 2000  -  total flux cleaned = 0.00420978 Jy
! Total flux subtracted in 2048 components = 0.00464589 Jy
! Clean residual min=-0.003793 max=0.003671 Jy/beam
! Clean residual mean=-0.000100 rms=0.001457 Jy/beam
! Combined flux in latest and established models = 0.136739 Jy
keep
! Adding 121 model components to the UV plane model.
! The established model now contains 156 components and 0.136739 Jy
![Exited script file: muppet]
wmap "J1238-3825_X_2002_05_14_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.959% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8369 x 2.202 at -0.2739 degrees (North through East)
! Clean map  min=-0.0082112  max=0.082159 Jy/beam
! Writing clean map to FITS file: J1238-3825_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 0.0821586 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.959% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.00142886 
device "J1238-3825_X_2002_05_14_yyk\_map.eps/VPS"
! Attempting to open device: 'J1238-3825_X_2002_05_14_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -5.21746 5.21746 10.4349 20.8698 41.7396 83.4793
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0042 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.082 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8369 x 2.202 at -0.2739 degrees (North through East)
! Clean map  min=-0.0082112  max=0.082159 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1238-3825_X_2002_05_14_yyk\_map.gif/gif"
! Attempting to open device: 'J1238-3825_X_2002_05_14_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1238-3825_X_2002_05_14_yyk_uvs.log closed on Tue Jun 26 22:46:33 2007