! Started logfile: J1048-1909_X_2006_12_18_yyk_uvs.log on Mon Jun 16 19:32:06 2008
obs J1048-1909_X_2006_12_18_yyk_uve.fits
! Reading UV FITS file: J1048-1909_X_2006_12_18_yyk_uve.fits
! AN table 1: 6 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.581481 visibilities/baseline/integration-bin.
! Found source: J1048-1909
! 
! 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 2161 lines of history.
! 
! Reading 628 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 J1048-1909_X_2006_12_18_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)= 0.933518 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 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.6995 mas, bmaj=1.893 mas, bpa=0.7823 degrees
! Estimated noise=2.42391 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 = 0.788085 Jy
! Component: 100  -  total flux cleaned = 0.93133 Jy
! Total flux subtracted in 100 components = 0.93133 Jy
! Clean residual min=-0.030918 max=0.045684 Jy/beam
! Clean residual mean=-0.000247 rms=0.009552 Jy/beam
! Combined flux in latest and established models = 0.93133 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 14 model components to the UV plane model.
! The established model now contains 14 components and 0.93133 Jy
! 
! Correcting IF 1.
!  A total of 24 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 19 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 19 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 19 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.155340Jy  sigma=2.200497
! Fit after  self-cal, rms=0.154908Jy  sigma=2.193250
! Inverting map and beam 
! Your choice of large map pixels excluded 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.6995 mas, bmaj=1.893 mas, bpa=0.7823 degrees
! Estimated noise=2.42391 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 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8666 mas, bmaj=2.254 mas, bpa=7.197 degrees
! Estimated noise=1.92387 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 = 0.0688708 Jy
! Component: 100  -  total flux cleaned = 0.096788 Jy
! Component: 150  -  total flux cleaned = 0.109427 Jy
! Component: 200  -  total flux cleaned = 0.113022 Jy
! Total flux subtracted in 200 components = 0.113022 Jy
! Clean residual min=-0.028171 max=0.022189 Jy/beam
! Clean residual mean=-0.000072 rms=0.006586 Jy/beam
! Combined flux in latest and established models = 1.04435 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 25 model components to the UV plane model.
! The established model now contains 36 components and 1.04435 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.134971Jy  sigma=1.833100
! Fit after  self-cal, rms=0.134912Jy  sigma=1.831513
! Inverting map 
! Your choice of large map pixels excluded 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8666 x 2.254 at 7.197 degrees (North through East)
! Clean map  min=-0.026267  max=0.90903 Jy/beam
if(peak(flux) < thresh*2)
  selflims ampcor_selflim
  end if
gscale
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Amplitude normalization factor in sub-array 1: 0.994465
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.01     FD        1.00*    HN        1.04     KP        0.99     
!   LA        0.98     MK        1.00*    NL        1.03     OV        1.00     
!   PT        0.99     SC        1.01     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.0013
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.01     FD        1.00*    HN        1.05     KP        0.94     
!   LA        0.94     MK        1.01     NL        1.01     OV        0.98     
!   PT        1.05     SC        0.99     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 1.00334
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.07     FD        1.00*    HN        0.95     KP        0.86     
!   LA        0.95     MK        1.04     NL        0.99     OV        1.05     
!   PT        1.06     SC        0.99     
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 0.986824
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.09     FD        1.00*    HN        0.95     KP        0.90     
!   LA        0.95     MK        1.11     NL        0.98     OV        1.01     
!   PT        1.11     SC        1.02     
! 
! 
! Fit before self-cal, rms=0.134912Jy  sigma=1.831513
! Fit after  self-cal, rms=0.117455Jy  sigma=1.549147
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=0.117455Jy  sigma=1.549147
! Fit after  self-cal, rms=0.117470Jy  sigma=1.549094
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8776 mas, bmaj=2.305 mas, bpa=7.686 degrees
! Estimated noise=1.91662 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 (-3.8, 2.6).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0139523 Jy
! Component: 100  -  total flux cleaned = 0.0130093 Jy
! Component: 150  -  total flux cleaned = 0.0119453 Jy
! Component: 200  -  total flux cleaned = 0.0110595 Jy
! Total flux subtracted in 200 components = 0.0110595 Jy
! Clean residual min=-0.008965 max=0.009706 Jy/beam
! Clean residual mean=-0.000030 rms=0.002334 Jy/beam
! Combined flux in latest and established models = 1.05541 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 26 model components to the UV plane model.
! The established model now contains 60 components and 1.05541 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.114941Jy  sigma=1.512316
! Fit after  self-cal, rms=0.114988Jy  sigma=1.511759
! Inverting map 
! Your choice of large map pixels excluded 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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=0.114988Jy  sigma=1.511759
! Fit after  self-cal, rms=0.077786Jy  sigma=1.006760
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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 = -0.000776162 Jy
! Component: 100  -  total flux cleaned = -0.000378073 Jy
! Component: 150  -  total flux cleaned = 0.000147179 Jy
! Component: 200  -  total flux cleaned = 0.000475497 Jy
! Total flux subtracted in 200 components = 0.000475497 Jy
! Clean residual min=-0.008818 max=0.008914 Jy/beam
! Clean residual mean=-0.000034 rms=0.002191 Jy/beam
! Combined flux in latest and established models = 1.05589 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 27 model components to the UV plane model.
! The established model now contains 79 components and 1.05589 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.076997Jy  sigma=0.994569
! Fit after  self-cal, rms=0.074611Jy  sigma=0.963605
! Inverting map 
! Your choice of large map pixels excluded 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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: 0.8776 x 2.305 at 7.686 degrees (North through East)
! Clean map  min=-0.0082144  max=0.91339 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
! Performing amp+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=0.074611Jy  sigma=0.963605
! Fit after  self-cal, rms=0.073650Jy  sigma=0.945679
! 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=0.073650Jy  sigma=0.945679
! Fit after  self-cal, rms=0.073516Jy  sigma=0.943842
! Inverting map and beam 
! Your choice of large map pixels excluded 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8766 mas, bmaj=2.303 mas, bpa=7.555 degrees
! Estimated noise=1.91376 mJy/beam.
! Added new window around map position (3.6, -2.4).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00979952 Jy
! Component: 100  -  total flux cleaned = 0.0112486 Jy
! Component: 150  -  total flux cleaned = 0.0125996 Jy
! Component: 200  -  total flux cleaned = 0.0130913 Jy
! Total flux subtracted in 200 components = 0.0130913 Jy
! Clean residual min=-0.007563 max=0.006666 Jy/beam
! Clean residual mean=-0.000009 rms=0.001617 Jy/beam
! Combined flux in latest and established models = 1.06898 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 30 model components to the UV plane model.
! The established model now contains 104 components and 1.06898 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.071925Jy  sigma=0.916436
! Fit after  self-cal, rms=0.071887Jy  sigma=0.915800
! Inverting map 
! Your choice of large map pixels excluded 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Performing amp+phase self-cal over 1 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.071887Jy  sigma=0.915800
! Fit after  self-cal, rms=0.070818Jy  sigma=0.895773
! 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=0.070818Jy  sigma=0.895773
! Fit after  self-cal, rms=0.070828Jy  sigma=0.895748
! Inverting map and beam 
! Your choice of large map pixels excluded 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8762 mas, bmaj=2.302 mas, bpa=7.584 degrees
! Estimated noise=1.91349 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00175752 Jy
! Component: 100  -  total flux cleaned = 0.00218507 Jy
! Component: 150  -  total flux cleaned = 0.00219062 Jy
! Component: 200  -  total flux cleaned = 0.00230946 Jy
! Total flux subtracted in 200 components = 0.00230946 Jy
! Clean residual min=-0.007002 max=0.005945 Jy/beam
! Clean residual mean=-0.000012 rms=0.001503 Jy/beam
! Combined flux in latest and established models = 1.07129 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 24 model components to the UV plane model.
! The established model now contains 113 components and 1.07129 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.070426Jy  sigma=0.889126
! Fit after  self-cal, rms=0.070413Jy  sigma=0.888975
! Inverting map 
! Your choice of large map pixels excluded 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! ************** FINISHED AMPLITUDE SELF-CAL ************** 
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 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=2.047 mas, bmaj=4.914 mas, bpa=4.863 degrees
! Estimated noise=2.44135 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 = 0.000988261 Jy
! Component: 100  -  total flux cleaned = 0.00146612 Jy
! Component: 150  -  total flux cleaned = 0.00146347 Jy
! Component: 200  -  total flux cleaned = 0.00170202 Jy
! Total flux subtracted in 200 components = 0.00170202 Jy
! Clean residual min=-0.005980 max=0.004530 Jy/beam
! Clean residual mean=-0.000019 rms=0.001494 Jy/beam
! Combined flux in latest and established models = 1.07299 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 125 components and 1.07299 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.070402Jy  sigma=0.888169
! Fit after  self-cal, rms=0.070339Jy  sigma=0.886974
! Inverting map 
! Your choice of large map pixels excluded 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.7039 mas, bmaj=1.907 mas, bpa=1.182 degrees
! Estimated noise=2.41377 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.788083 Jy
! Component: 100  -  total flux cleaned = 0.928376 Jy
! Component: 150  -  total flux cleaned = 0.981004 Jy
! Component: 200  -  total flux cleaned = 1.00525 Jy
! Total flux subtracted in 200 components = 1.00525 Jy
! Clean residual min=-0.013991 max=0.014225 Jy/beam
! Clean residual mean=-0.000082 rms=0.003321 Jy/beam
! Combined flux in latest and established models = 1.00525 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 32 model components to the UV plane model.
! The established model now contains 32 components and 1.00525 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8762 mas, bmaj=2.302 mas, bpa=7.584 degrees
! Estimated noise=1.91349 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 (1, -1.4).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0237605 Jy
! Component: 100  -  total flux cleaned = 0.0384164 Jy
! Component: 150  -  total flux cleaned = 0.0491653 Jy
! Component: 200  -  total flux cleaned = 0.0564711 Jy
! Total flux subtracted in 200 components = 0.0564711 Jy
! Clean residual min=-0.008378 max=0.006950 Jy/beam
! Clean residual mean=-0.000039 rms=0.001868 Jy/beam
! Combined flux in latest and established models = 1.06172 Jy
! Adding 44 model components to the UV plane model.
! The established model now contains 73 components and 1.06172 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=2.047 mas, bmaj=4.914 mas, bpa=4.863 degrees
! Estimated noise=2.44135 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 = 0.00763815 Jy
! Component: 100  -  total flux cleaned = 0.0101116 Jy
! Component: 150  -  total flux cleaned = 0.0115621 Jy
! Component: 200  -  total flux cleaned = 0.012291 Jy
! Total flux subtracted in 200 components = 0.012291 Jy
! Clean residual min=-0.006177 max=0.005509 Jy/beam
! Clean residual mean=-0.000012 rms=0.001542 Jy/beam
! Combined flux in latest and established models = 1.07401 Jy
! Adding 35 model components to the UV plane model.
! The established model now contains 105 components and 1.07401 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8762 mas, bmaj=2.302 mas, bpa=7.584 degrees
! Estimated noise=1.91349 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000477242 Jy
! Component: 100  -  total flux cleaned = 0.00100332 Jy
! Component: 150  -  total flux cleaned = 0.00130553 Jy
! Component: 200  -  total flux cleaned = 0.00157602 Jy
! Total flux subtracted in 200 components = 0.00157602 Jy
! Clean residual min=-0.005765 max=0.005420 Jy/beam
! Clean residual mean=-0.000001 rms=0.001416 Jy/beam
! Combined flux in latest and established models = 1.07558 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 27 model components to the UV plane model.
! The established model now contains 122 components and 1.07558 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.070151Jy  sigma=0.886563
! Fit after  self-cal, rms=0.070059Jy  sigma=0.884949
wmodel J1048-1909_X_2006_12_18_yyk\_map.mod
! Writing 122 model components to file: J1048-1909_X_2006_12_18_yyk_map.mod
wobs J1048-1909_X_2006_12_18_yyk\_uvs.fits
! Writing UV FITS file: J1048-1909_X_2006_12_18_yyk_uvs.fits
wwins J1048-1909_X_2006_12_18_yyk\_map.win
! wwins: Wrote 4 windows to J1048-1909_X_2006_12_18_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 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00138197 Jy
! Component: 100  -  total flux cleaned = -0.00138157 Jy
! Component: 150  -  total flux cleaned = -0.00154513 Jy
! Component: 200  -  total flux cleaned = -0.00169984 Jy
! Component: 250  -  total flux cleaned = -0.0016259 Jy
! Component: 300  -  total flux cleaned = -0.00141523 Jy
! Component: 350  -  total flux cleaned = -0.00168385 Jy
! Component: 400  -  total flux cleaned = -0.00213702 Jy
! Component: 450  -  total flux cleaned = -0.00263594 Jy
! Component: 500  -  total flux cleaned = -0.00329834 Jy
! Component: 550  -  total flux cleaned = -0.0037071 Jy
! Component: 600  -  total flux cleaned = -0.00416272 Jy
! Component: 650  -  total flux cleaned = -0.00471366 Jy
! Component: 700  -  total flux cleaned = -0.00503509 Jy
! Component: 750  -  total flux cleaned = -0.00545251 Jy
! Component: 800  -  total flux cleaned = -0.00590872 Jy
! Component: 850  -  total flux cleaned = -0.0062054 Jy
! Component: 900  -  total flux cleaned = -0.00649433 Jy
! Component: 950  -  total flux cleaned = -0.00682239 Jy
! Component: 1000  -  total flux cleaned = -0.00709618 Jy
! Component: 1050  -  total flux cleaned = -0.00723012 Jy
! Component: 1100  -  total flux cleaned = -0.00749313 Jy
! Component: 1150  -  total flux cleaned = -0.00775058 Jy
! Component: 1200  -  total flux cleaned = -0.00796172 Jy
! Component: 1250  -  total flux cleaned = -0.00833384 Jy
! Component: 1300  -  total flux cleaned = -0.00849548 Jy
! Component: 1350  -  total flux cleaned = -0.00865567 Jy
! Component: 1400  -  total flux cleaned = -0.00889222 Jy
! Component: 1450  -  total flux cleaned = -0.00908659 Jy
! Component: 1500  -  total flux cleaned = -0.0092023 Jy
! Component: 1550  -  total flux cleaned = -0.00931539 Jy
! Component: 1600  -  total flux cleaned = -0.00935306 Jy
! Component: 1650  -  total flux cleaned = -0.00950172 Jy
! Component: 1700  -  total flux cleaned = -0.00961152 Jy
! Component: 1750  -  total flux cleaned = -0.00982792 Jy
! Component: 1800  -  total flux cleaned = -0.00986367 Jy
! Component: 1850  -  total flux cleaned = -0.0098992 Jy
! Component: 1900  -  total flux cleaned = -0.00996924 Jy
! Component: 1950  -  total flux cleaned = -0.00996935 Jy
! Component: 2000  -  total flux cleaned = -0.0100715 Jy
! Total flux subtracted in 2048 components = -0.00996956 Jy
! Clean residual min=-0.001863 max=0.002013 Jy/beam
! Clean residual mean=0.000000 rms=0.000620 Jy/beam
! Combined flux in latest and established models = 1.06561 Jy
keep
! Adding 115 model components to the UV plane model.
! The established model now contains 237 components and 1.06561 Jy
![Exited script file: muppet]
wmap "J1048-1909_X_2006_12_18_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8762 x 2.302 at 7.584 degrees (North through East)
! Clean map  min=-0.0041541  max=0.91873 Jy/beam
! Writing clean map to FITS file: J1048-1909_X_2006_12_18_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.918725 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.874% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000603121 
device "J1048-1909_X_2006_12_18_yyk\_map.eps/VPS"
! Attempting to open device: 'J1048-1909_X_2006_12_18_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.196943 0.196943 0.393886 0.787771 1.57554 3.15109 6.30217 12.6043 25.2087 50.4174
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0018 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.918 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8762 x 2.302 at 7.584 degrees (North through East)
! Clean map  min=-0.0041541  max=0.91873 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1048-1909_X_2006_12_18_yyk\_map.gif/gif"
! Attempting to open device: 'J1048-1909_X_2006_12_18_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1048-1909_X_2006_12_18_yyk_uvs.log closed on Mon Jun 16 19:32:12 2008