! Started logfile: J1712-1820_X_2005_07_09_yyk_uvs.log on Fri Jan 20 10:47:28 2006
obs J1712-1820_X_2005_07_09_yyk_uve.fits
! Reading UV FITS file: J1712-1820_X_2005_07_09_yyk_uve.fits
! AN table 1: 11 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.965657 visibilities/baseline/integration-bin.
! Found source: J1712-1820
! 
! 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  8.40997e+09        8e+06          1        8e+06
!  02        2  8.47997e+09        8e+06          1        8e+06
!  03        3  8.79497e+09        8e+06          1        8e+06
!  04        4  8.89997e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 1480 lines of history.
! 
! Reading 1912 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 J1712-1820_X_2005_07_09_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)= 0.117689 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 0.288% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.7 mas, bmaj=1.695 mas, bpa=3.756 degrees
! Estimated noise=1.47957 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 = 0.0787935 Jy
! Component: 100  -  total flux cleaned = 0.0979653 Jy
! Total flux subtracted in 100 components = 0.0979653 Jy
! Clean residual min=-0.007157 max=0.008430 Jy/beam
! Clean residual mean=-0.000019 rms=0.002254 Jy/beam
! Combined flux in latest and established models = 0.0979654 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 12 model components to the UV plane model.
! The established model now contains 12 components and 0.0979654 Jy
! 
! Correcting IF 1.
!  A total of 21 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 21 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 21 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 21 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.068177Jy  sigma=1.101937
! Fit after  self-cal, rms=0.067677Jy  sigma=1.094776
! Inverting map and beam 
! Your choice of large map pixels excluded 0.288% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.7 mas, bmaj=1.695 mas, bpa=3.756 degrees
! Estimated noise=1.47957 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 0.288% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.9045 mas, bmaj=2.202 mas, bpa=-0.2993 degrees
! Estimated noise=1.00192 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 = 0.0112446 Jy
! Component: 100  -  total flux cleaned = 0.01487 Jy
! Component: 150  -  total flux cleaned = 0.016236 Jy
! Component: 200  -  total flux cleaned = 0.0166112 Jy
! Total flux subtracted in 200 components = 0.0166112 Jy
! Clean residual min=-0.004434 max=0.004283 Jy/beam
! Clean residual mean=-0.000003 rms=0.001199 Jy/beam
! Combined flux in latest and established models = 0.114577 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 18 model components to the UV plane model.
! The established model now contains 25 components and 0.114577 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066618Jy  sigma=1.069098
! Fit after  self-cal, rms=0.066573Jy  sigma=1.068895
! Inverting map 
! Your choice of large map pixels excluded 0.288% 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: 0.9045 x 2.202 at -0.2993 degrees (North through East)
! Clean map  min=-0.0040147  max=0.095793 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: 1.05007
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.91     FD        0.99     HN        1.00*    KP        0.93     
!   LA        0.99     MK        0.95     NL        0.98     OV        0.98     
!   PT        0.92     SC        0.87     
! 
! 
! 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=0.066573Jy  sigma=1.068895
! Fit after  self-cal, rms=0.066376Jy  sigma=1.067838
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=0.066376Jy  sigma=1.067838
! Fit after  self-cal, rms=0.066373Jy  sigma=1.067837
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.288% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8949 mas, bmaj=2.172 mas, bpa=0.4648 degrees
! Estimated noise=0.998693 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 = 0.000439163 Jy
! Component: 100  -  total flux cleaned = 0.000498232 Jy
! Component: 150  -  total flux cleaned = 0.000523516 Jy
! Component: 200  -  total flux cleaned = 0.000545231 Jy
! Total flux subtracted in 200 components = 0.000545231 Jy
! Clean residual min=-0.004372 max=0.004225 Jy/beam
! Clean residual mean=-0.000003 rms=0.001189 Jy/beam
! Combined flux in latest and established models = 0.115122 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 14 model components to the UV plane model.
! The established model now contains 28 components and 0.115122 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066355Jy  sigma=1.067437
! Fit after  self-cal, rms=0.066338Jy  sigma=1.067374
! Inverting map 
! Your choice of large map pixels excluded 0.288% 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=0.066338Jy  sigma=1.067374
! Fit after  self-cal, rms=0.062675Jy  sigma=1.012467
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.288% 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 = 0.00125147 Jy
! Component: 100  -  total flux cleaned = 0.00116651 Jy
! Component: 150  -  total flux cleaned = 0.00120027 Jy
! Component: 200  -  total flux cleaned = 0.00122881 Jy
! Total flux subtracted in 200 components = 0.00122881 Jy
! Clean residual min=-0.004261 max=0.004236 Jy/beam
! Clean residual mean=-0.000002 rms=0.001136 Jy/beam
! Combined flux in latest and established models = 0.116351 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 35 components and 0.116351 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062682Jy  sigma=1.011435
! Fit after  self-cal, rms=0.062402Jy  sigma=1.007553
! Inverting map 
! Your choice of large map pixels excluded 0.288% 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: 0.8949 x 2.172 at 0.4648 degrees (North through East)
! Clean map  min=-0.0038565  max=0.096623 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 0.288% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=2.486 mas, bmaj=5.249 mas, bpa=10.29 degrees
! Estimated noise=1.2467 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 = -4.13479e-05 Jy
! Component: 100  -  total flux cleaned = -0.000112218 Jy
! Component: 150  -  total flux cleaned = -0.000171253 Jy
! Component: 200  -  total flux cleaned = -0.000194246 Jy
! Total flux subtracted in 200 components = -0.000194246 Jy
! Clean residual min=-0.004189 max=0.003825 Jy/beam
! Clean residual mean=-0.000001 rms=0.001267 Jy/beam
! Combined flux in latest and established models = 0.116156 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 8 model components to the UV plane model.
! The established model now contains 40 components and 0.116156 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062413Jy  sigma=1.007546
! Fit after  self-cal, rms=0.062387Jy  sigma=1.007127
! Inverting map 
! Your choice of large map pixels excluded 0.288% 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 0.288% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.6978 mas, bmaj=1.69 mas, bpa=4.052 degrees
! Estimated noise=1.46913 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0812741 Jy
! Component: 100  -  total flux cleaned = 0.100412 Jy
! Component: 150  -  total flux cleaned = 0.109064 Jy
! Component: 200  -  total flux cleaned = 0.113539 Jy
! Total flux subtracted in 200 components = 0.113539 Jy
! Clean residual min=-0.006308 max=0.007744 Jy/beam
! Clean residual mean=-0.000007 rms=0.001830 Jy/beam
! Combined flux in latest and established models = 0.113539 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 22 model components to the UV plane model.
! The established model now contains 22 components and 0.113539 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.288% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8949 mas, bmaj=2.172 mas, bpa=0.4648 degrees
! Estimated noise=0.998693 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 = 0.00229927 Jy
! Component: 100  -  total flux cleaned = 0.00252892 Jy
! Component: 150  -  total flux cleaned = 0.00266269 Jy
! Component: 200  -  total flux cleaned = 0.00276427 Jy
! Total flux subtracted in 200 components = 0.00276427 Jy
! Clean residual min=-0.004347 max=0.004275 Jy/beam
! Clean residual mean=-0.000001 rms=0.001123 Jy/beam
! Combined flux in latest and established models = 0.116303 Jy
! Adding 8 model components to the UV plane model.
! The established model now contains 28 components and 0.116303 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.288% 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 0.288% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=2.486 mas, bmaj=5.249 mas, bpa=10.29 degrees
! Estimated noise=1.2467 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 = -0.00015626 Jy
! Component: 100  -  total flux cleaned = -0.000124828 Jy
! Component: 150  -  total flux cleaned = -0.000124241 Jy
! Component: 200  -  total flux cleaned = -0.000126022 Jy
! Total flux subtracted in 200 components = -0.000126022 Jy
! Clean residual min=-0.004160 max=0.003797 Jy/beam
! Clean residual mean=-0.000000 rms=0.001266 Jy/beam
! Combined flux in latest and established models = 0.116177 Jy
! Adding 8 model components to the UV plane model.
! The established model now contains 33 components and 0.116177 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.288% 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 0.288% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8949 mas, bmaj=2.172 mas, bpa=0.4648 degrees
! Estimated noise=0.998693 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000107653 Jy
! Component: 100  -  total flux cleaned = 0.000133354 Jy
! Component: 150  -  total flux cleaned = 0.000179093 Jy
! Component: 200  -  total flux cleaned = 0.000199577 Jy
! Total flux subtracted in 200 components = 0.000199577 Jy
! Clean residual min=-0.004378 max=0.004292 Jy/beam
! Clean residual mean=-0.000001 rms=0.001118 Jy/beam
! Combined flux in latest and established models = 0.116377 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 17 model components to the UV plane model.
! The established model now contains 41 components and 0.116377 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062374Jy  sigma=1.006623
! Fit after  self-cal, rms=0.062352Jy  sigma=1.006430
wmodel J1712-1820_X_2005_07_09_yyk\_map.mod
! Writing 41 model components to file: J1712-1820_X_2005_07_09_yyk_map.mod
wobs J1712-1820_X_2005_07_09_yyk\_uvs.fits
! Writing UV FITS file: J1712-1820_X_2005_07_09_yyk_uvs.fits
wwins J1712-1820_X_2005_07_09_yyk\_map.win
! wwins: Wrote 1 windows to J1712-1820_X_2005_07_09_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 0.288% 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 = -0.000936144 Jy
! Component: 100  -  total flux cleaned = -0.00179923 Jy
! Component: 150  -  total flux cleaned = -0.00247511 Jy
! Component: 200  -  total flux cleaned = -0.00254291 Jy
! Component: 250  -  total flux cleaned = -0.00260643 Jy
! Component: 300  -  total flux cleaned = -0.00236645 Jy
! Component: 350  -  total flux cleaned = -0.00207543 Jy
! Component: 400  -  total flux cleaned = -0.00173701 Jy
! Component: 450  -  total flux cleaned = -0.00151612 Jy
! Component: 500  -  total flux cleaned = -0.00113845 Jy
! Component: 550  -  total flux cleaned = -0.000821984 Jy
! Component: 600  -  total flux cleaned = -0.000564919 Jy
! Component: 650  -  total flux cleaned = -0.000213603 Jy
! Component: 700  -  total flux cleaned = 3.1443e-05 Jy
! Component: 750  -  total flux cleaned = 0.000367516 Jy
! Component: 800  -  total flux cleaned = 0.000555443 Jy
! Component: 850  -  total flux cleaned = 0.000877891 Jy
! Component: 900  -  total flux cleaned = 0.00110324 Jy
! Component: 950  -  total flux cleaned = 0.00128012 Jy
! Component: 1000  -  total flux cleaned = 0.00158271 Jy
! Component: 1050  -  total flux cleaned = 0.0017095 Jy
! Component: 1100  -  total flux cleaned = 0.00187561 Jy
! Component: 1150  -  total flux cleaned = 0.00199869 Jy
! Component: 1200  -  total flux cleaned = 0.00232095 Jy
! Component: 1250  -  total flux cleaned = 0.00235946 Jy
! Component: 1300  -  total flux cleaned = 0.00232 Jy
! Component: 1350  -  total flux cleaned = 0.00262756 Jy
! Component: 1400  -  total flux cleaned = 0.00262687 Jy
! Component: 1450  -  total flux cleaned = 0.00273845 Jy
! Component: 1500  -  total flux cleaned = 0.00277435 Jy
! Component: 1550  -  total flux cleaned = 0.00281025 Jy
! Component: 1600  -  total flux cleaned = 0.00280995 Jy
! Component: 1650  -  total flux cleaned = 0.00280944 Jy
! Component: 1700  -  total flux cleaned = 0.00287913 Jy
! Component: 1750  -  total flux cleaned = 0.00294744 Jy
! Component: 1800  -  total flux cleaned = 0.00287976 Jy
! Component: 1850  -  total flux cleaned = 0.00281365 Jy
! Component: 1900  -  total flux cleaned = 0.00281375 Jy
! Component: 1950  -  total flux cleaned = 0.00271602 Jy
! Component: 2000  -  total flux cleaned = 0.0026522 Jy
! Total flux subtracted in 2048 components = 0.00265246 Jy
! Clean residual min=-0.001785 max=0.001669 Jy/beam
! Clean residual mean=0.000004 rms=0.000589 Jy/beam
! Combined flux in latest and established models = 0.119029 Jy
keep
! Adding 135 model components to the UV plane model.
! The established model now contains 176 components and 0.119029 Jy
![Exited script file: muppet]
wmap "J1712-1820_X_2005_07_09_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.288% 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: 0.8949 x 2.172 at 0.4648 degrees (North through East)
! Clean map  min=-0.0030584  max=0.095376 Jy/beam
! Writing clean map to FITS file: J1712-1820_X_2005_07_09_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.0953761 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.288% 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 0.00058324 
device "J1712-1820_X_2005_07_09_yyk\_map.eps/VPS"
! Attempting to open device: 'J1712-1820_X_2005_07_09_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -1.83455 1.83455 3.66909 7.33818 14.6764 29.3527 58.7055
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0017 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.095 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8949 x 2.172 at 0.4648 degrees (North through East)
! Clean map  min=-0.0030584  max=0.095376 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1712-1820_X_2005_07_09_yyk\_map.gif/gif"
! Attempting to open device: 'J1712-1820_X_2005_07_09_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1712-1820_X_2005_07_09_yyk_uvs.log closed on Fri Jan 20 10:47:31 2006