! Started logfile: J2107-1708_X_2005_06_01_yyk_uvs.log on Sat Oct  8 17:43:23 2005
obs J2107-1708_X_2005_06_01_yyk_uve.fits
! Reading UV FITS file: J2107-1708_X_2005_06_01_yyk_uve.fits
! AN table 1: 19 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.969591 visibilities/baseline/integration-bin.
! Found source: J2107-1708
! 
! 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 1618 lines of history.
! 
! Reading 3316 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 J2107-1708_X_2005_06_01_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)= 0.10434 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 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.6864 mas, bmaj=1.823 mas, bpa=1.559 degrees
! Estimated noise=1.14065 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 = 0.0610623 Jy
! Component: 100  -  total flux cleaned = 0.0751728 Jy
! Total flux subtracted in 100 components = 0.0751728 Jy
! Clean residual min=-0.005895 max=0.007551 Jy/beam
! Clean residual mean=-0.000006 rms=0.001530 Jy/beam
! Combined flux in latest and established models = 0.0751728 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 22 model components to the UV plane model.
! The established model now contains 22 components and 0.0751728 Jy
! 
! Correcting IF 1.
!  A total of 4 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 4 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 27 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 16 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.072157Jy  sigma=1.118519
! Fit after  self-cal, rms=0.069800Jy  sigma=1.089338
! Inverting map and beam 
! Your choice of large map pixels excluded 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.6864 mas, bmaj=1.823 mas, bpa=1.559 degrees
! Estimated noise=1.14065 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 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.9242 mas, bmaj=2.356 mas, bpa=0.2656 degrees
! Estimated noise=0.671126 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 = 0.011411 Jy
! Component: 100  -  total flux cleaned = 0.0147134 Jy
! Component: 150  -  total flux cleaned = 0.0159824 Jy
! Component: 200  -  total flux cleaned = 0.0160738 Jy
! Total flux subtracted in 200 components = 0.0160738 Jy
! Clean residual min=-0.002920 max=0.003141 Jy/beam
! Clean residual mean=0.000001 rms=0.000774 Jy/beam
! Combined flux in latest and established models = 0.0912466 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 24 model components to the UV plane model.
! The established model now contains 40 components and 0.0912466 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.069072Jy  sigma=1.059960
! Fit after  self-cal, rms=0.069067Jy  sigma=1.059916
! Inverting map 
! Your choice of large map pixels excluded 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9242 x 2.356 at 0.2656 degrees (North through East)
! Clean map  min=-0.0026619  max=0.079334 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: 1.02408
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     FD        0.96     HN        1.06     KP        0.99     
!   LA        1.00     MK        0.90     NL        0.98     OV        0.95     
!   PT        0.98     SC        0.96     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.01642
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.98     FD        1.00     HN        1.05     KP        0.91     
!   LA        0.95     MK        0.91     NL        1.01     OV        1.07     
!   PT        1.01     SC        0.94     
! 
! 
! 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=0.069067Jy  sigma=1.059916
! Fit after  self-cal, rms=0.068944Jy  sigma=1.057308
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=0.068944Jy  sigma=1.057308
! Fit after  self-cal, rms=0.068944Jy  sigma=1.057307
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.8998 mas, bmaj=2.307 mas, bpa=-0.2308 degrees
! Estimated noise=0.668575 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 = 0.000880686 Jy
! Component: 100  -  total flux cleaned = 0.000882026 Jy
! Component: 150  -  total flux cleaned = 0.000815999 Jy
! Component: 200  -  total flux cleaned = 0.000786158 Jy
! Total flux subtracted in 200 components = 0.000786158 Jy
! Clean residual min=-0.002824 max=0.002978 Jy/beam
! Clean residual mean=0.000003 rms=0.000741 Jy/beam
! Combined flux in latest and established models = 0.0920328 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 8 model components to the UV plane model.
! The established model now contains 43 components and 0.0920328 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.068863Jy  sigma=1.056570
! Fit after  self-cal, rms=0.068858Jy  sigma=1.056546
! Inverting map 
! Your choice of large map pixels excluded 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
print "************** FINISHED AMPLITUDE GSCALE SELF-CAL **************"
! ************** FINISHED AMPLITUDE GSCALE SELF-CAL ************** 
! 
phase_soltime=phase_soltime2
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.068858Jy  sigma=1.056546
! Fit after  self-cal, rms=0.065349Jy  sigma=1.006119
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00140708 Jy
! Component: 100  -  total flux cleaned = 0.00145896 Jy
! Component: 150  -  total flux cleaned = 0.0014587 Jy
! Component: 200  -  total flux cleaned = 0.00145915 Jy
! Total flux subtracted in 200 components = 0.00145915 Jy
! Clean residual min=-0.002796 max=0.003022 Jy/beam
! Clean residual mean=0.000002 rms=0.000738 Jy/beam
! Combined flux in latest and established models = 0.0934919 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 13 model components to the UV plane model.
! The established model now contains 49 components and 0.0934919 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.065340Jy  sigma=1.005490
! Fit after  self-cal, rms=0.064895Jy  sigma=1.001804
! Inverting map 
! Your choice of large map pixels excluded 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
print "*** FINISHED NATURAL WEIGHTING CLEAN with shorter phase_soltime ***"
! *** FINISHED NATURAL WEIGHTING CLEAN with shorter phase_soltime *** 
! 
dynam = dynam - 0.25
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8998 x 2.307 at -0.2308 degrees (North through East)
! Clean map  min=-0.0024926  max=0.080889 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 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=2.26 mas, bmaj=4.992 mas, bpa=7.506 degrees
! Estimated noise=0.835578 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 = -0.00022059 Jy
! Component: 100  -  total flux cleaned = -0.000179038 Jy
! Component: 150  -  total flux cleaned = -0.000179514 Jy
! Component: 200  -  total flux cleaned = -0.00017993 Jy
! Total flux subtracted in 200 components = -0.00017993 Jy
! Clean residual min=-0.002767 max=0.003283 Jy/beam
! Clean residual mean=0.000002 rms=0.000896 Jy/beam
! Combined flux in latest and established models = 0.093312 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 51 components and 0.093312 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.064905Jy  sigma=1.001804
! Fit after  self-cal, rms=0.064825Jy  sigma=1.001304
! Inverting map 
! Your choice of large map pixels excluded 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
uvtaper 0,0
! 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 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.6786 mas, bmaj=1.811 mas, bpa=1.393 degrees
! Estimated noise=1.13174 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0652479 Jy
! Component: 100  -  total flux cleaned = 0.0802979 Jy
! Component: 150  -  total flux cleaned = 0.0873446 Jy
! Component: 200  -  total flux cleaned = 0.0909152 Jy
! Total flux subtracted in 200 components = 0.0909152 Jy
! Clean residual min=-0.004533 max=0.004177 Jy/beam
! Clean residual mean=0.000000 rms=0.001094 Jy/beam
! Combined flux in latest and established models = 0.0909153 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 20 model components to the UV plane model.
! The established model now contains 20 components and 0.0909153 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.8998 mas, bmaj=2.307 mas, bpa=-0.2308 degrees
! Estimated noise=0.668575 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 = 0.00238281 Jy
! Component: 100  -  total flux cleaned = 0.00256434 Jy
! Component: 150  -  total flux cleaned = 0.00252792 Jy
! Component: 200  -  total flux cleaned = 0.00249695 Jy
! Total flux subtracted in 200 components = 0.00249695 Jy
! Clean residual min=-0.002809 max=0.002902 Jy/beam
! Clean residual mean=0.000002 rms=0.000742 Jy/beam
! Combined flux in latest and established models = 0.0934122 Jy
! Adding 12 model components to the UV plane model.
! The established model now contains 31 components and 0.0934122 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=2.26 mas, bmaj=4.992 mas, bpa=7.506 degrees
! Estimated noise=0.835578 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 = -3.51308e-05 Jy
! Component: 100  -  total flux cleaned = -3.42988e-05 Jy
! Component: 150  -  total flux cleaned = -3.18956e-05 Jy
! Component: 200  -  total flux cleaned = -2.9263e-05 Jy
! Total flux subtracted in 200 components = -2.9263e-05 Jy
! Clean residual min=-0.002764 max=0.003229 Jy/beam
! Clean residual mean=0.000003 rms=0.000899 Jy/beam
! Combined flux in latest and established models = 0.093383 Jy
! Adding 6 model components to the UV plane model.
! The established model now contains 34 components and 0.093383 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! Estimated beam: bmin=0.8998 mas, bmaj=2.307 mas, bpa=-0.2308 degrees
! Estimated noise=0.668575 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 9.00109e-05 Jy
! Component: 100  -  total flux cleaned = 4.00903e-05 Jy
! Component: 150  -  total flux cleaned = 1.94143e-07 Jy
! Component: 200  -  total flux cleaned = -3.19898e-05 Jy
! Total flux subtracted in 200 components = -3.19898e-05 Jy
! Clean residual min=-0.002748 max=0.002947 Jy/beam
! Clean residual mean=0.000002 rms=0.000736 Jy/beam
! Combined flux in latest and established models = 0.093351 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 7 model components to the UV plane model.
! The established model now contains 38 components and 0.093351 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.064782Jy  sigma=1.001075
! Fit after  self-cal, rms=0.064756Jy  sigma=1.000969
wmodel J2107-1708_X_2005_06_01_yyk\_map.mod
! Writing 38 model components to file: J2107-1708_X_2005_06_01_yyk_map.mod
wobs J2107-1708_X_2005_06_01_yyk\_uvs.fits
! Writing UV FITS file: J2107-1708_X_2005_06_01_yyk_uvs.fits
wwins J2107-1708_X_2005_06_01_yyk\_map.win
! wwins: Wrote 1 windows to J2107-1708_X_2005_06_01_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 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.000232417 Jy
! Component: 100  -  total flux cleaned = 0.000279164 Jy
! Component: 150  -  total flux cleaned = 0.000368096 Jy
! Component: 200  -  total flux cleaned = 0.000163158 Jy
! Component: 250  -  total flux cleaned = 4.66145e-06 Jy
! Component: 300  -  total flux cleaned = -0.000109082 Jy
! Component: 350  -  total flux cleaned = -7.25628e-05 Jy
! Component: 400  -  total flux cleaned = -0.000213934 Jy
! Component: 450  -  total flux cleaned = -0.000212914 Jy
! Component: 500  -  total flux cleaned = -0.000145476 Jy
! Component: 550  -  total flux cleaned = -0.000177346 Jy
! Component: 600  -  total flux cleaned = -8.17311e-05 Jy
! Component: 650  -  total flux cleaned = -0.000176156 Jy
! Component: 700  -  total flux cleaned = -0.000114819 Jy
! Component: 750  -  total flux cleaned = -8.44259e-05 Jy
! Component: 800  -  total flux cleaned = -2.44768e-05 Jy
! Component: 850  -  total flux cleaned = -5.3275e-05 Jy
! Component: 900  -  total flux cleaned = 6.14249e-05 Jy
! Component: 950  -  total flux cleaned = 0.000117368 Jy
! Component: 1000  -  total flux cleaned = 3.30647e-05 Jy
! Component: 1050  -  total flux cleaned = 8.80925e-05 Jy
! Component: 1100  -  total flux cleaned = 8.7694e-05 Jy
! Component: 1150  -  total flux cleaned = 3.52151e-05 Jy
! Component: 1200  -  total flux cleaned = 0.000140055 Jy
! Component: 1250  -  total flux cleaned = 0.000114321 Jy
! Component: 1300  -  total flux cleaned = 0.000190136 Jy
! Component: 1350  -  total flux cleaned = 0.000214465 Jy
! Component: 1400  -  total flux cleaned = 0.000263971 Jy
! Component: 1450  -  total flux cleaned = 0.000264034 Jy
! Component: 1500  -  total flux cleaned = 0.000360854 Jy
! Component: 1550  -  total flux cleaned = 0.000312652 Jy
! Component: 1600  -  total flux cleaned = 0.000430887 Jy
! Component: 1650  -  total flux cleaned = 0.000500857 Jy
! Component: 1700  -  total flux cleaned = 0.000638689 Jy
! Component: 1750  -  total flux cleaned = 0.00072988 Jy
! Component: 1800  -  total flux cleaned = 0.000842681 Jy
! Component: 1850  -  total flux cleaned = 0.000909768 Jy
! Component: 1900  -  total flux cleaned = 0.00102012 Jy
! Component: 1950  -  total flux cleaned = 0.00110722 Jy
! Component: 2000  -  total flux cleaned = 0.001194 Jy
! Total flux subtracted in 2048 components = 0.00130122 Jy
! Clean residual min=-0.001353 max=0.001083 Jy/beam
! Clean residual mean=-0.000001 rms=0.000410 Jy/beam
! Combined flux in latest and established models = 0.0946522 Jy
keep
! Adding 143 model components to the UV plane model.
! The established model now contains 181 components and 0.0946523 Jy
![Exited script file: muppet]
wmap "J2107-1708_X_2005_06_01_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8998 x 2.307 at -0.2308 degrees (North through East)
! Clean map  min=-0.0021782  max=0.080746 Jy/beam
! Writing clean map to FITS file: J2107-1708_X_2005_06_01_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.0807458 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.301% of the data.
!  The x-axis pixel size should ideally be below 0.1988 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000408342 
device "J2107-1708_X_2005_06_01_yyk\_map.eps/VPS"
! Attempting to open device: 'J2107-1708_X_2005_06_01_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -1.51714 1.51714 3.03428 6.06855 12.1371 24.2742 48.5484 97.0968
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0012 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.08 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8998 x 2.307 at -0.2308 degrees (North through East)
! Clean map  min=-0.0021782  max=0.080746 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J2107-1708_X_2005_06_01_yyk\_map.gif/gif"
! Attempting to open device: 'J2107-1708_X_2005_06_01_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J2107-1708_X_2005_06_01_yyk_uvs.log closed on Sat Oct  8 17:43:27 2005