! Started logfile: J0609-1542_X_2007_01_11_yyk_uvs.log on Mon Jun 16 19:20:06 2008
obs J0609-1542_X_2007_01_11_yyk_uve.fits
! Reading UV FITS file: J0609-1542_X_2007_01_11_yyk_uve.fits
! AN table 1: 6 integrations on 36 of 36 possible baselines.
! Apparent sampling: 0.388889 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J0609-1542
! 
! 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 2143 lines of history.
! 
! Reading 336 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 J0609-1542_X_2007_01_11_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)= 2.91321 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 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.5693 mas, bmaj=1.668 mas, bpa=-1.31 degrees
! Estimated noise=3.18355 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 = 2.43729 Jy
! Component: 100  -  total flux cleaned = 2.81828 Jy
! Total flux subtracted in 100 components = 2.81828 Jy
! Clean residual min=-0.091448 max=0.111911 Jy/beam
! Clean residual mean=-0.000549 rms=0.028304 Jy/beam
! Combined flux in latest and established models = 2.81828 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 6 model components to the UV plane model.
! The established model now contains 6 components and 2.81828 Jy
! 
! Correcting IF 1.
!  A total of 27 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 27 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 27 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.462821Jy  sigma=6.526300
! Fit after  self-cal, rms=0.462355Jy  sigma=6.501486
! Inverting map and beam 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.5693 mas, bmaj=1.668 mas, bpa=-1.31 degrees
! Estimated noise=3.18355 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 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.6561 mas, bmaj=1.781 mas, bpa=-2.602 degrees
! Estimated noise=2.74739 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 = 0.217045 Jy
! Component: 100  -  total flux cleaned = 0.314735 Jy
! Component: 150  -  total flux cleaned = 0.36335 Jy
! Component: 200  -  total flux cleaned = 0.388823 Jy
! Total flux subtracted in 200 components = 0.388823 Jy
! Clean residual min=-0.081887 max=0.078111 Jy/beam
! Clean residual mean=-0.000299 rms=0.020436 Jy/beam
! Combined flux in latest and established models = 3.2071 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 16 components and 3.2071 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.385400Jy  sigma=5.356980
! Fit after  self-cal, rms=0.384840Jy  sigma=5.351542
! Inverting map 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6561 x 1.781 at -2.602 degrees (North through East)
! Clean map  min=-0.074044  max=2.8757 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: 1.00668
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.97     FD        0.97     HN        1.06     KP        1.00*    
!   LA        0.97     MK        0.99     OV        1.00*    PT        0.97     
!   SC        1.01     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.01098
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.98     FD        0.98     HN        1.05     KP        1.00*    
!   LA        0.92     MK        0.97     OV        1.00*    PT        1.02     
!   SC        0.99     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 1.00015
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.04     FD        1.02     HN        0.95     KP        1.00*    
!   LA        0.94     MK        1.02     OV        1.00*    PT        1.04     
!   SC        0.99     
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 0.980813
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.05     FD        1.05     HN        0.98     KP        1.00*    
!   LA        0.93     MK        1.05     OV        1.00*    PT        1.10     
!   SC        1.03     
! 
! 
! Fit before self-cal, rms=0.384840Jy  sigma=5.351542
! Fit after  self-cal, rms=0.348725Jy  sigma=4.800152
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=0.348725Jy  sigma=4.800152
! Fit after  self-cal, rms=0.348674Jy  sigma=4.799998
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.6593 mas, bmaj=1.788 mas, bpa=-2.575 degrees
! Estimated noise=2.74896 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 = 5.92726e-06 Jy
! Component: 100  -  total flux cleaned = 2.16567e-05 Jy
! Component: 150  -  total flux cleaned = 3.81292e-05 Jy
! Component: 200  -  total flux cleaned = 0.000697247 Jy
! Total flux subtracted in 200 components = 0.000697247 Jy
! Clean residual min=-0.041429 max=0.064421 Jy/beam
! Clean residual mean=-0.000067 rms=0.013465 Jy/beam
! Combined flux in latest and established models = 3.2078 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 9 model components to the UV plane model.
! The established model now contains 20 components and 3.2078 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.348531Jy  sigma=4.787377
! Fit after  self-cal, rms=0.348041Jy  sigma=4.785622
! Inverting map 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 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=0.348041Jy  sigma=4.785622
! Fit after  self-cal, rms=0.167876Jy  sigma=2.333695
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 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)
! Added new window around map position (4.4, 2.8).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0673815 Jy
! Component: 100  -  total flux cleaned = 0.0847206 Jy
! Component: 150  -  total flux cleaned = 0.093247 Jy
! Component: 200  -  total flux cleaned = 0.0991689 Jy
! Total flux subtracted in 200 components = 0.0991689 Jy
! Clean residual min=-0.031433 max=0.032435 Jy/beam
! Clean residual mean=0.000073 rms=0.008595 Jy/beam
! Combined flux in latest and established models = 3.30697 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 32 model components to the UV plane model.
! The established model now contains 50 components and 3.30697 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.137173Jy  sigma=1.888880
! Fit after  self-cal, rms=0.112667Jy  sigma=1.581999
! Inverting map 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 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: 0.6593 x 1.788 at -2.575 degrees (North through East)
! Clean map  min=-0.032421  max=2.9017 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=0.112667Jy  sigma=1.581999
! Fit after  self-cal, rms=0.090300Jy  sigma=1.251439
! 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=0.090300Jy  sigma=1.251439
! Fit after  self-cal, rms=0.087973Jy  sigma=1.224533
! Inverting map and beam 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.6588 mas, bmaj=1.786 mas, bpa=-2.418 degrees
! Estimated noise=2.73741 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.019571 Jy
! Component: 100  -  total flux cleaned = 0.0251672 Jy
! Component: 150  -  total flux cleaned = 0.0280729 Jy
! Component: 200  -  total flux cleaned = 0.0300464 Jy
! Total flux subtracted in 200 components = 0.0300464 Jy
! Clean residual min=-0.023414 max=0.020938 Jy/beam
! Clean residual mean=0.000102 rms=0.006186 Jy/beam
! Combined flux in latest and established models = 3.33702 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 22 model components to the UV plane model.
! The established model now contains 63 components and 3.33701 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.080831Jy  sigma=1.124217
! Fit after  self-cal, rms=0.079716Jy  sigma=1.115489
! Inverting map 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 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=0.079716Jy  sigma=1.115489
! Fit after  self-cal, rms=0.076766Jy  sigma=1.069847
! 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=0.076766Jy  sigma=1.069847
! Fit after  self-cal, rms=0.076718Jy  sigma=1.069647
! Inverting map and beam 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.6586 mas, bmaj=1.786 mas, bpa=-2.472 degrees
! Estimated noise=2.73609 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.01066 Jy
! Component: 100  -  total flux cleaned = 0.0140554 Jy
! Component: 150  -  total flux cleaned = 0.0156897 Jy
! Component: 200  -  total flux cleaned = 0.0168583 Jy
! Total flux subtracted in 200 components = 0.0168583 Jy
! Clean residual min=-0.021318 max=0.019320 Jy/beam
! Clean residual mean=0.000099 rms=0.005681 Jy/beam
! Combined flux in latest and established models = 3.35387 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 17 model components to the UV plane model.
! The established model now contains 68 components and 3.35387 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.074642Jy  sigma=1.038520
! Fit after  self-cal, rms=0.074284Jy  sigma=1.036196
! Inverting map 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 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 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=1.833 mas, bmaj=3.893 mas, bpa=16.63 degrees
! Estimated noise=4.23726 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 = -0.00877016 Jy
! Component: 100  -  total flux cleaned = -0.00649113 Jy
! Component: 150  -  total flux cleaned = -0.00524896 Jy
! Component: 200  -  total flux cleaned = -0.00525311 Jy
! Total flux subtracted in 200 components = -0.00525311 Jy
! Clean residual min=-0.031127 max=0.032247 Jy/beam
! Clean residual mean=0.000278 rms=0.012092 Jy/beam
! Combined flux in latest and established models = 3.34862 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 76 components and 3.34862 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.075653Jy  sigma=1.058880
! Fit after  self-cal, rms=0.075039Jy  sigma=1.049913
! Inverting map 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 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 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.5702 mas, bmaj=1.67 mas, bpa=-1.194 degrees
! Estimated noise=3.16977 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 2.44168 Jy
! Component: 100  -  total flux cleaned = 2.82088 Jy
! Component: 150  -  total flux cleaned = 2.98093 Jy
! Component: 200  -  total flux cleaned = 3.07725 Jy
! Total flux subtracted in 200 components = 3.07725 Jy
! Clean residual min=-0.051941 max=0.054728 Jy/beam
! Clean residual mean=-0.000223 rms=0.013816 Jy/beam
! Combined flux in latest and established models = 3.07725 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 15 model components to the UV plane model.
! The established model now contains 15 components and 3.07725 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.6586 mas, bmaj=1.786 mas, bpa=-2.472 degrees
! Estimated noise=2.73609 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 = 0.104312 Jy
! Component: 100  -  total flux cleaned = 0.159717 Jy
! Component: 150  -  total flux cleaned = 0.190893 Jy
! Component: 200  -  total flux cleaned = 0.213931 Jy
! Total flux subtracted in 200 components = 0.213931 Jy
! Clean residual min=-0.031908 max=0.025839 Jy/beam
! Clean residual mean=-0.000037 rms=0.007817 Jy/beam
! Combined flux in latest and established models = 3.29118 Jy
! Adding 44 model components to the UV plane model.
! The established model now contains 53 components and 3.29118 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 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 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=1.833 mas, bmaj=3.893 mas, bpa=16.63 degrees
! Estimated noise=4.23726 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 = 0.0432894 Jy
! Component: 100  -  total flux cleaned = 0.0488482 Jy
! Component: 150  -  total flux cleaned = 0.0530611 Jy
! Component: 200  -  total flux cleaned = 0.0556596 Jy
! Total flux subtracted in 200 components = 0.0556596 Jy
! Clean residual min=-0.033696 max=0.029786 Jy/beam
! Clean residual mean=0.000219 rms=0.012224 Jy/beam
! Combined flux in latest and established models = 3.34684 Jy
! Adding 21 model components to the UV plane model.
! The established model now contains 65 components and 3.34684 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.6586 mas, bmaj=1.786 mas, bpa=-2.472 degrees
! Estimated noise=2.73609 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00275771 Jy
! Component: 100  -  total flux cleaned = 0.00338547 Jy
! Component: 150  -  total flux cleaned = 0.00388246 Jy
! Component: 200  -  total flux cleaned = 0.00538026 Jy
! Total flux subtracted in 200 components = 0.00538026 Jy
! Clean residual min=-0.023443 max=0.019972 Jy/beam
! Clean residual mean=0.000074 rms=0.005813 Jy/beam
! Combined flux in latest and established models = 3.35222 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 18 model components to the UV plane model.
! The established model now contains 79 components and 3.35222 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.076686Jy  sigma=1.071621
! Fit after  self-cal, rms=0.076475Jy  sigma=1.067420
wmodel J0609-1542_X_2007_01_11_yyk\_map.mod
! Writing 79 model components to file: J0609-1542_X_2007_01_11_yyk_map.mod
wobs J0609-1542_X_2007_01_11_yyk\_uvs.fits
! Writing UV FITS file: J0609-1542_X_2007_01_11_yyk_uvs.fits
wwins J0609-1542_X_2007_01_11_yyk\_map.win
! wwins: Wrote 2 windows to J0609-1542_X_2007_01_11_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 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00773264 Jy
! Component: 100  -  total flux cleaned = -0.0100501 Jy
! Component: 150  -  total flux cleaned = -0.0121222 Jy
! Component: 200  -  total flux cleaned = -0.0129254 Jy
! Component: 250  -  total flux cleaned = -0.0117327 Jy
! Component: 300  -  total flux cleaned = -0.0112922 Jy
! Component: 350  -  total flux cleaned = -0.0106806 Jy
! Component: 400  -  total flux cleaned = -0.0102962 Jy
! Component: 450  -  total flux cleaned = -0.00958172 Jy
! Component: 500  -  total flux cleaned = -0.00908369 Jy
! Component: 550  -  total flux cleaned = -0.0079883 Jy
! Component: 600  -  total flux cleaned = -0.00650943 Jy
! Component: 650  -  total flux cleaned = -0.00539756 Jy
! Component: 700  -  total flux cleaned = -0.00447364 Jy
! Component: 750  -  total flux cleaned = -0.00347065 Jy
! Component: 800  -  total flux cleaned = -0.00274955 Jy
! Component: 850  -  total flux cleaned = -0.00183553 Jy
! Component: 900  -  total flux cleaned = -0.00128428 Jy
! Component: 950  -  total flux cleaned = -0.000448729 Jy
! Component: 1000  -  total flux cleaned = -0.00015034 Jy
! Component: 1050  -  total flux cleaned = 0.000142365 Jy
! Component: 1100  -  total flux cleaned = 0.000424645 Jy
! Component: 1150  -  total flux cleaned = 0.000789021 Jy
! Component: 1200  -  total flux cleaned = 0.00123026 Jy
! Component: 1250  -  total flux cleaned = 0.00157287 Jy
! Component: 1300  -  total flux cleaned = 0.00198804 Jy
! Component: 1350  -  total flux cleaned = 0.0022305 Jy
! Component: 1400  -  total flux cleaned = 0.00262388 Jy
! Component: 1450  -  total flux cleaned = 0.00270001 Jy
! Component: 1500  -  total flux cleaned = 0.00285109 Jy
! Component: 1550  -  total flux cleaned = 0.0029987 Jy
! Component: 1600  -  total flux cleaned = 0.00314321 Jy
! Component: 1650  -  total flux cleaned = 0.00321485 Jy
! Component: 1700  -  total flux cleaned = 0.00328463 Jy
! Component: 1750  -  total flux cleaned = 0.00314507 Jy
! Component: 1800  -  total flux cleaned = 0.00300858 Jy
! Component: 1850  -  total flux cleaned = 0.0030763 Jy
! Component: 1900  -  total flux cleaned = 0.00307643 Jy
! Component: 1950  -  total flux cleaned = 0.0030769 Jy
! Component: 2000  -  total flux cleaned = 0.00320943 Jy
! Total flux subtracted in 2048 components = 0.00327512 Jy
! Clean residual min=-0.004303 max=0.004745 Jy/beam
! Clean residual mean=0.000020 rms=0.001118 Jy/beam
! Combined flux in latest and established models = 3.3555 Jy
keep
! Adding 117 model components to the UV plane model.
! The established model now contains 196 components and 3.3555 Jy
![Exited script file: muppet]
wmap "J0609-1542_X_2007_01_11_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6586 x 1.786 at -2.472 degrees (North through East)
! Clean map  min=-0.01904  max=2.8914 Jy/beam
! Writing clean map to FITS file: J0609-1542_X_2007_01_11_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 2.89143 
invert
! Inverting map 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.00106668 
device "J0609-1542_X_2007_01_11_yyk\_map.eps/VPS"
! Attempting to open device: 'J0609-1542_X_2007_01_11_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.110673 0.110673 0.221347 0.442693 0.885387 1.77077 3.54155 7.08309 14.1662 28.3324 56.6647
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0032 
print "peak=",int(peak_flux*1000)/1000
! peak= 2.891 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6586 x 1.786 at -2.472 degrees (North through East)
! Clean map  min=-0.01904  max=2.8914 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0609-1542_X_2007_01_11_yyk\_map.gif/gif"
! Attempting to open device: 'J0609-1542_X_2007_01_11_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J0609-1542_X_2007_01_11_yyk_uvs.log closed on Mon Jun 16 19:20:11 2008