! Started logfile: J0925-2027_X_2002_05_14_yyk_uvs.log on Tue Jun 26 22:37:11 2007
obs J0925-2027_X_2002_05_14_yyk_uva.fits
! Reading UV FITS file: J0925-2027_X_2002_05_14_yyk_uva.fits
! AN table 1: 109 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.65158 visibilities/baseline/integration-bin.
! Found source: J0925-2027
! 
! 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 1077 lines of history.
! 
! Reading 12784 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 J0925-2027_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)= 0.250343 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 0.311% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=0.6723 mas, bmaj=1.728 mas, bpa=6.242 degrees
! Estimated noise=1319.06 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 = 0.0487147 Jy
! Component: 100  -  total flux cleaned = 0.0693333 Jy
! Total flux subtracted in 100 components = 0.0693333 Jy
! Clean residual min=-0.008828 max=0.011555 Jy/beam
! Clean residual mean=0.000040 rms=0.002394 Jy/beam
! Combined flux in latest and established models = 0.0693333 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 23 model components to the UV plane model.
! The established model now contains 23 components and 0.0693333 Jy
! 
! Correcting IF 1.
!  A total of 306 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 303 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 328 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 303 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.241614Jy  sigma=0.001473
! Fit after  self-cal, rms=0.240239Jy  sigma=0.001469
! Inverting map and beam 
! Your choice of large map pixels excluded 0.312% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=0.6722 mas, bmaj=1.728 mas, bpa=6.242 degrees
! Estimated noise=1371.63 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 0.312% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=0.9142 mas, bmaj=2.251 mas, bpa=7.614 degrees
! Estimated noise=846.991 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 = 0.0242516 Jy
! Component: 100  -  total flux cleaned = 0.0332373 Jy
! Component: 150  -  total flux cleaned = 0.0370058 Jy
! Component: 200  -  total flux cleaned = 0.0385853 Jy
! Total flux subtracted in 200 components = 0.0385853 Jy
! Clean residual min=-0.005472 max=0.005606 Jy/beam
! Clean residual mean=0.000008 rms=0.001531 Jy/beam
! Combined flux in latest and established models = 0.107919 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 31 model components to the UV plane model.
! The established model now contains 43 components and 0.107919 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.239436Jy  sigma=0.001455
! Fit after  self-cal, rms=0.239405Jy  sigma=0.001455
! Inverting map 
! Your choice of large map pixels excluded 0.312% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9142 x 2.251 at 7.614 degrees (North through East)
! Clean map  min=-0.0050615  max=0.059268 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 30 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 33 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 33 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 33 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=0.239405Jy  sigma=0.001455
! Fit after  self-cal, rms=0.238612Jy  sigma=0.001454
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=0.238612Jy  sigma=0.001454
! Fit after  self-cal, rms=0.238595Jy  sigma=0.001453
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.315% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=0.9133 mas, bmaj=2.248 mas, bpa=7.525 degrees
! Estimated noise=849.689 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 = 0.000767933 Jy
! Component: 100  -  total flux cleaned = 0.000865545 Jy
! Component: 150  -  total flux cleaned = 0.0009091 Jy
! Component: 200  -  total flux cleaned = 0.000989645 Jy
! Total flux subtracted in 200 components = 0.000989645 Jy
! Clean residual min=-0.005581 max=0.005817 Jy/beam
! Clean residual mean=0.000008 rms=0.001515 Jy/beam
! Combined flux in latest and established models = 0.108908 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 11 model components to the UV plane model.
! The established model now contains 46 components and 0.108908 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.238590Jy  sigma=0.001453
! Fit after  self-cal, rms=0.238572Jy  sigma=0.001453
! Inverting map 
! Your choice of large map pixels excluded 0.315% of the data.
!  The x-axis pixel size should ideally be below 0.1994 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=0.238572Jy  sigma=0.001453
! Fit after  self-cal, rms=0.237180Jy  sigma=0.001443
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.315% of the data.
!  The x-axis pixel size should ideally be below 0.1994 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 = 0.00337928 Jy
! Component: 100  -  total flux cleaned = 0.00352596 Jy
! Component: 150  -  total flux cleaned = 0.00364201 Jy
! Component: 200  -  total flux cleaned = 0.00368758 Jy
! Total flux subtracted in 200 components = 0.00368758 Jy
! Clean residual min=-0.005193 max=0.004993 Jy/beam
! Clean residual mean=0.000002 rms=0.001392 Jy/beam
! Combined flux in latest and established models = 0.112596 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 50 components and 0.112596 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.237147Jy  sigma=0.001442
! Fit after  self-cal, rms=0.236759Jy  sigma=0.001440
! Inverting map 
! Your choice of large map pixels excluded 0.315% of the data.
!  The x-axis pixel size should ideally be below 0.1994 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: 0.9133 x 2.248 at 7.525 degrees (North through East)
! Clean map  min=-0.0044868  max=0.063813 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 0.315% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=2.276 mas, bmaj=5.636 mas, bpa=11.65 degrees
! Estimated noise=1060.23 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 = 0.00202846 Jy
! Component: 100  -  total flux cleaned = 0.00202427 Jy
! Component: 150  -  total flux cleaned = 0.00202445 Jy
! Component: 200  -  total flux cleaned = 0.00202729 Jy
! Total flux subtracted in 200 components = 0.00202729 Jy
! Clean residual min=-0.004984 max=0.005025 Jy/beam
! Clean residual mean=-0.000004 rms=0.001531 Jy/beam
! Combined flux in latest and established models = 0.114623 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 4 model components to the UV plane model.
! The established model now contains 52 components and 0.114623 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.236765Jy  sigma=0.001440
! Fit after  self-cal, rms=0.236674Jy  sigma=0.001440
! Inverting map 
! Your choice of large map pixels excluded 0.315% of the data.
!  The x-axis pixel size should ideally be below 0.1994 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 0.315% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=0.6721 mas, bmaj=1.726 mas, bpa=6.21 degrees
! Estimated noise=1327.88 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0563854 Jy
! Component: 100  -  total flux cleaned = 0.0772218 Jy
! Component: 150  -  total flux cleaned = 0.0890369 Jy
! Component: 200  -  total flux cleaned = 0.0961587 Jy
! Total flux subtracted in 200 components = 0.0961587 Jy
! Clean residual min=-0.008231 max=0.008086 Jy/beam
! Clean residual mean=0.000016 rms=0.002024 Jy/beam
! Combined flux in latest and established models = 0.0961587 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 30 model components to the UV plane model.
! The established model now contains 30 components and 0.0961587 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.315% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=0.9133 mas, bmaj=2.248 mas, bpa=7.525 degrees
! Estimated noise=849.689 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)
! Added new window around map position (0.8, 0.4).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0113041 Jy
! Component: 100  -  total flux cleaned = 0.0167701 Jy
! Component: 150  -  total flux cleaned = 0.0188439 Jy
! Component: 200  -  total flux cleaned = 0.0190456 Jy
! Total flux subtracted in 200 components = 0.0190456 Jy
! Clean residual min=-0.004774 max=0.004830 Jy/beam
! Clean residual mean=-0.000003 rms=0.001265 Jy/beam
! Combined flux in latest and established models = 0.115204 Jy
! Adding 26 model components to the UV plane model.
! The established model now contains 47 components and 0.115204 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.315% of the data.
!  The x-axis pixel size should ideally be below 0.1994 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 0.315% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=2.276 mas, bmaj=5.636 mas, bpa=11.65 degrees
! Estimated noise=1060.23 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 = 0.00172902 Jy
! Component: 100  -  total flux cleaned = 0.00172749 Jy
! Component: 150  -  total flux cleaned = 0.00178765 Jy
! Component: 200  -  total flux cleaned = 0.00189763 Jy
! Total flux subtracted in 200 components = 0.00189763 Jy
! Clean residual min=-0.004815 max=0.004605 Jy/beam
! Clean residual mean=-0.000009 rms=0.001417 Jy/beam
! Combined flux in latest and established models = 0.117102 Jy
! Adding 13 model components to the UV plane model.
! The established model now contains 59 components and 0.117102 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.315% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.315% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! Estimated beam: bmin=0.9133 mas, bmaj=2.248 mas, bpa=7.525 degrees
! Estimated noise=849.689 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.00104118 Jy
! Component: 100  -  total flux cleaned = -0.00103723 Jy
! Component: 150  -  total flux cleaned = -0.0011088 Jy
! Component: 200  -  total flux cleaned = -0.00117269 Jy
! Total flux subtracted in 200 components = -0.00117269 Jy
! Clean residual min=-0.004585 max=0.004564 Jy/beam
! Clean residual mean=-0.000004 rms=0.001229 Jy/beam
! Combined flux in latest and established models = 0.115929 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 21 model components to the UV plane model.
! The established model now contains 74 components and 0.115929 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.236481Jy  sigma=0.001438
! Fit after  self-cal, rms=0.236363Jy  sigma=0.001438
wmodel J0925-2027_X_2002_05_14_yyk\_map.mod
! Writing 74 model components to file: J0925-2027_X_2002_05_14_yyk_map.mod
wobs J0925-2027_X_2002_05_14_yyk\_uvs.fits
! Writing UV FITS file: J0925-2027_X_2002_05_14_yyk_uvs.fits
wwins J0925-2027_X_2002_05_14_yyk\_map.win
! wwins: Wrote 2 windows to J0925-2027_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 0.315% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.000925571 Jy
! Component: 100  -  total flux cleaned = 0.00100402 Jy
! Component: 150  -  total flux cleaned = 0.00114928 Jy
! Component: 200  -  total flux cleaned = 0.00101019 Jy
! Component: 250  -  total flux cleaned = 0.000676957 Jy
! Component: 300  -  total flux cleaned = 0.000291242 Jy
! Component: 350  -  total flux cleaned = 4.22789e-05 Jy
! Component: 400  -  total flux cleaned = -0.000263438 Jy
! Component: 450  -  total flux cleaned = -0.000619815 Jy
! Component: 500  -  total flux cleaned = -0.000795273 Jy
! Component: 550  -  total flux cleaned = -0.00114024 Jy
! Component: 600  -  total flux cleaned = -0.0015326 Jy
! Component: 650  -  total flux cleaned = -0.00158709 Jy
! Component: 700  -  total flux cleaned = -0.0017502 Jy
! Component: 750  -  total flux cleaned = -0.00180405 Jy
! Component: 800  -  total flux cleaned = -0.00196255 Jy
! Component: 850  -  total flux cleaned = -0.00211828 Jy
! Component: 900  -  total flux cleaned = -0.00237399 Jy
! Component: 950  -  total flux cleaned = -0.00237383 Jy
! Component: 1000  -  total flux cleaned = -0.00247309 Jy
! Component: 1050  -  total flux cleaned = -0.00247245 Jy
! Component: 1100  -  total flux cleaned = -0.00242427 Jy
! Component: 1150  -  total flux cleaned = -0.00242441 Jy
! Component: 1200  -  total flux cleaned = -0.00242395 Jy
! Component: 1250  -  total flux cleaned = -0.00237836 Jy
! Component: 1300  -  total flux cleaned = -0.00233317 Jy
! Component: 1350  -  total flux cleaned = -0.00224285 Jy
! Component: 1400  -  total flux cleaned = -0.00224351 Jy
! Component: 1450  -  total flux cleaned = -0.00219978 Jy
! Component: 1500  -  total flux cleaned = -0.00224373 Jy
! Component: 1550  -  total flux cleaned = -0.00224289 Jy
! Component: 1600  -  total flux cleaned = -0.00211428 Jy
! Component: 1650  -  total flux cleaned = -0.00190378 Jy
! Component: 1700  -  total flux cleaned = -0.00203029 Jy
! Component: 1750  -  total flux cleaned = -0.0020711 Jy
! Component: 1800  -  total flux cleaned = -0.00198892 Jy
! Component: 1850  -  total flux cleaned = -0.00194909 Jy
! Component: 1900  -  total flux cleaned = -0.00210903 Jy
! Component: 1950  -  total flux cleaned = -0.0020295 Jy
! Component: 2000  -  total flux cleaned = -0.00206871 Jy
! Total flux subtracted in 2048 components = -0.00203028 Jy
! Clean residual min=-0.002113 max=0.002181 Jy/beam
! Clean residual mean=-0.000006 rms=0.000741 Jy/beam
! Combined flux in latest and established models = 0.113899 Jy
keep
! Adding 138 model components to the UV plane model.
! The established model now contains 212 components and 0.113899 Jy
![Exited script file: muppet]
wmap "J0925-2027_X_2002_05_14_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.315% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9133 x 2.248 at 7.525 degrees (North through East)
! Clean map  min=-0.0037177  max=0.066755 Jy/beam
! Writing clean map to FITS file: J0925-2027_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 0.0667552 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.315% of the data.
!  The x-axis pixel size should ideally be below 0.1994 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000738814 
device "J0925-2027_X_2002_05_14_yyk\_map.eps/VPS"
! Attempting to open device: 'J0925-2027_X_2002_05_14_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -3.32026 3.32026 6.64051 13.281 26.562 53.1241
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0022 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.066 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9133 x 2.248 at 7.525 degrees (North through East)
! Clean map  min=-0.0037177  max=0.066755 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0925-2027_X_2002_05_14_yyk\_map.gif/gif"
! Attempting to open device: 'J0925-2027_X_2002_05_14_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J0925-2027_X_2002_05_14_yyk_uvs.log closed on Tue Jun 26 22:37:17 2007