! Started logfile: J1951-0509_X_2005_06_01_yyk_uvs.log on Sat Oct  8 17:41:14 2005
obs J1951-0509_X_2005_06_01_yyk_uve.fits
! Reading UV FITS file: J1951-0509_X_2005_06_01_yyk_uve.fits
! AN table 1: 10 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.78 visibilities/baseline/integration-bin.
! Found source: J1951-0509
! 
! 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 1617 lines of history.
! 
! Reading 1404 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 J1951-0509_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)= 0.223674 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 0.312% of the data.
!  The x-axis pixel size should ideally be below 0.1991 milli-arcsec
! Estimated beam: bmin=0.6957 mas, bmaj=1.758 mas, bpa=0.9107 degrees
! Estimated noise=1.27313 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 = 0.183119 Jy
! Component: 100  -  total flux cleaned = 0.212504 Jy
! Total flux subtracted in 100 components = 0.212504 Jy
! Clean residual min=-0.006637 max=0.008151 Jy/beam
! Clean residual mean=-0.000016 rms=0.001746 Jy/beam
! Combined flux in latest and established models = 0.212504 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 10 model components to the UV plane model.
! The established model now contains 10 components and 0.212504 Jy
! 
! Correcting IF 1.
!  A total of 26 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 26 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 26 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=0.059698Jy  sigma=1.157254
! Fit after  self-cal, rms=0.059461Jy  sigma=1.151110
! Inverting map and beam 
! Your choice of large map pixels excluded 0.313% of the data.
!  The x-axis pixel size should ideally be below 0.1991 milli-arcsec
! Estimated beam: bmin=0.6955 mas, bmaj=1.758 mas, bpa=0.888 degrees
! Estimated noise=1.27306 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 0.313% of the data.
!  The x-axis pixel size should ideally be below 0.1991 milli-arcsec
! Estimated beam: bmin=0.8655 mas, bmaj=2.116 mas, bpa=-0.1115 degrees
! Estimated noise=0.952348 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 = 0.0151431 Jy
! Component: 100  -  total flux cleaned = 0.0207612 Jy
! Component: 150  -  total flux cleaned = 0.023217 Jy
! Component: 200  -  total flux cleaned = 0.0240059 Jy
! Total flux subtracted in 200 components = 0.0240059 Jy
! Clean residual min=-0.004827 max=0.006976 Jy/beam
! Clean residual mean=0.000006 rms=0.001280 Jy/beam
! Combined flux in latest and established models = 0.23651 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 24 model components to the UV plane model.
! The established model now contains 30 components and 0.23651 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.057049Jy  sigma=1.096352
! Fit after  self-cal, rms=0.057026Jy  sigma=1.095764
! Inverting map 
! Your choice of large map pixels excluded 0.313% of the data.
!  The x-axis pixel size should ideally be below 0.1991 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8655 x 2.116 at -0.1115 degrees (North through East)
! Clean map  min=-0.0042277  max=0.21512 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: 0.996148
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.02     FD        1.00     HN        1.07     KP        1.01     
!   LA        0.99     MK        0.97     NL        1.03     OV        1.01     
!   PT        0.98     SC        0.96     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.01016
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.01     FD        0.94     HN        1.04     KP        0.94     
!   LA        1.00     MK        1.04     NL        0.99     OV        1.00     
!   PT        1.02     SC        0.92     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 1.01875
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.09     FD        1.01     HN        0.86     KP        0.86     
!   LA        0.99     MK        1.04     NL        0.99     OV        0.99     
!   PT        1.03     SC        0.96     
! 
! 
! Correcting IF 4.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Amplitude normalization factor in sub-array 1: 0.968178
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        1.04     HN        0.93     KP        0.96     
!   LA        1.01     MK        1.03     NL        0.99     OV        1.07     
!   PT        1.07     SC        1.23     
! 
! 
! Fit before self-cal, rms=0.057026Jy  sigma=1.095764
! Fit after  self-cal, rms=0.052895Jy  sigma=1.024676
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=0.052895Jy  sigma=1.024676
! Fit after  self-cal, rms=0.052898Jy  sigma=1.024597
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 milli-arcsec
! Estimated beam: bmin=0.8695 mas, bmaj=2.132 mas, bpa=0.04562 degrees
! Estimated noise=0.949338 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 (-0.8, -4.2).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00631117 Jy
! Component: 100  -  total flux cleaned = 0.00731999 Jy
! Component: 150  -  total flux cleaned = 0.00758082 Jy
! Component: 200  -  total flux cleaned = 0.00758405 Jy
! Total flux subtracted in 200 components = 0.00758405 Jy
! Clean residual min=-0.003860 max=0.003475 Jy/beam
! Clean residual mean=0.000007 rms=0.000914 Jy/beam
! Combined flux in latest and established models = 0.244094 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 22 model components to the UV plane model.
! The established model now contains 52 components and 0.244094 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.052390Jy  sigma=1.011621
! Fit after  self-cal, rms=0.052357Jy  sigma=1.011132
! Inverting map 
! Your choice of large map pixels excluded 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 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=0.052357Jy  sigma=1.011132
! Fit after  self-cal, rms=0.050941Jy  sigma=0.976474
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 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 = 0.00139097 Jy
! Component: 100  -  total flux cleaned = 0.00149704 Jy
! Component: 150  -  total flux cleaned = 0.00144856 Jy
! Component: 200  -  total flux cleaned = 0.00136338 Jy
! Total flux subtracted in 200 components = 0.00136338 Jy
! Clean residual min=-0.003803 max=0.003250 Jy/beam
! Clean residual mean=0.000007 rms=0.000869 Jy/beam
! Combined flux in latest and established models = 0.245457 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 21 model components to the UV plane model.
! The established model now contains 61 components and 0.245457 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.050861Jy  sigma=0.974714
! Fit after  self-cal, rms=0.050727Jy  sigma=0.972372
! Inverting map 
! Your choice of large map pixels excluded 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 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: 0.8695 x 2.132 at 0.04562 degrees (North through East)
! Clean map  min=-0.0033564  max=0.21562 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=0.050727Jy  sigma=0.972372
! Fit after  self-cal, rms=0.049803Jy  sigma=0.948359
! 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=0.049803Jy  sigma=0.948359
! Fit after  self-cal, rms=0.049770Jy  sigma=0.948104
! Inverting map and beam 
! Your choice of large map pixels excluded 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 milli-arcsec
! Estimated beam: bmin=0.8699 mas, bmaj=2.125 mas, bpa=0.1911 degrees
! Estimated noise=0.945894 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00121113 Jy
! Component: 100  -  total flux cleaned = 0.00121245 Jy
! Component: 150  -  total flux cleaned = 0.00117107 Jy
! Component: 200  -  total flux cleaned = 0.0011723 Jy
! Total flux subtracted in 200 components = 0.0011723 Jy
! Clean residual min=-0.003605 max=0.002906 Jy/beam
! Clean residual mean=0.000003 rms=0.000782 Jy/beam
! Combined flux in latest and established models = 0.246629 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 79 components and 0.246629 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.049694Jy  sigma=0.946408
! Fit after  self-cal, rms=0.049670Jy  sigma=0.946294
! Inverting map 
! Your choice of large map pixels excluded 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 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=0.049670Jy  sigma=0.946294
! Fit after  self-cal, rms=0.048703Jy  sigma=0.922279
! 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=0.048703Jy  sigma=0.922279
! Fit after  self-cal, rms=0.048692Jy  sigma=0.922244
! Inverting map and beam 
! Your choice of large map pixels excluded 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 milli-arcsec
! Estimated beam: bmin=0.8725 mas, bmaj=2.127 mas, bpa=0.1899 degrees
! Estimated noise=0.945241 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000590134 Jy
! Component: 100  -  total flux cleaned = 0.000592044 Jy
! Component: 150  -  total flux cleaned = 0.000557362 Jy
! Component: 200  -  total flux cleaned = 0.000525221 Jy
! Total flux subtracted in 200 components = 0.000525221 Jy
! Clean residual min=-0.003578 max=0.002767 Jy/beam
! Clean residual mean=0.000003 rms=0.000762 Jy/beam
! Combined flux in latest and established models = 0.247155 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 25 model components to the UV plane model.
! The established model now contains 88 components and 0.247155 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.048634Jy  sigma=0.921203
! Fit after  self-cal, rms=0.048624Jy  sigma=0.921141
! Inverting map 
! Your choice of large map pixels excluded 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 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 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 milli-arcsec
! Estimated beam: bmin=2.152 mas, bmaj=3.861 mas, bpa=4.875 degrees
! Estimated noise=1.21037 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 = 0.000669193 Jy
! Component: 100  -  total flux cleaned = 0.000789975 Jy
! Component: 150  -  total flux cleaned = 0.000770365 Jy
! Component: 200  -  total flux cleaned = 0.000769981 Jy
! Total flux subtracted in 200 components = 0.000769981 Jy
! Clean residual min=-0.003115 max=0.002973 Jy/beam
! Clean residual mean=0.000005 rms=0.000903 Jy/beam
! Combined flux in latest and established models = 0.247924 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 96 components and 0.247924 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.048619Jy  sigma=0.921088
! Fit after  self-cal, rms=0.048612Jy  sigma=0.921051
! Inverting map 
! Your choice of large map pixels excluded 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 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 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 milli-arcsec
! Estimated beam: bmin=0.6995 mas, bmaj=1.764 mas, bpa=0.8536 degrees
! Estimated noise=1.27371 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.183667 Jy
! Component: 100  -  total flux cleaned = 0.212647 Jy
! Component: 150  -  total flux cleaned = 0.223548 Jy
! Component: 200  -  total flux cleaned = 0.230237 Jy
! Total flux subtracted in 200 components = 0.230237 Jy
! Clean residual min=-0.004832 max=0.004226 Jy/beam
! Clean residual mean=-0.000006 rms=0.001209 Jy/beam
! Combined flux in latest and established models = 0.230237 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 21 model components to the UV plane model.
! The established model now contains 21 components and 0.230237 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 milli-arcsec
! Estimated beam: bmin=0.8725 mas, bmaj=2.127 mas, bpa=0.1899 degrees
! Estimated noise=0.945241 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 = 0.00727558 Jy
! Component: 100  -  total flux cleaned = 0.0114995 Jy
! Component: 150  -  total flux cleaned = 0.0139524 Jy
! Component: 200  -  total flux cleaned = 0.0150191 Jy
! Total flux subtracted in 200 components = 0.0150191 Jy
! Clean residual min=-0.003613 max=0.002746 Jy/beam
! Clean residual mean=0.000003 rms=0.000795 Jy/beam
! Combined flux in latest and established models = 0.245256 Jy
! Adding 36 model components to the UV plane model.
! The established model now contains 55 components and 0.245256 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 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 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 milli-arcsec
! Estimated beam: bmin=2.152 mas, bmaj=3.861 mas, bpa=4.875 degrees
! Estimated noise=1.21037 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 = 0.00151406 Jy
! Component: 100  -  total flux cleaned = 0.00201431 Jy
! Component: 150  -  total flux cleaned = 0.00233565 Jy
! Component: 200  -  total flux cleaned = 0.00250093 Jy
! Total flux subtracted in 200 components = 0.00250093 Jy
! Clean residual min=-0.003110 max=0.002983 Jy/beam
! Clean residual mean=0.000006 rms=0.000909 Jy/beam
! Combined flux in latest and established models = 0.247757 Jy
! Adding 22 model components to the UV plane model.
! The established model now contains 72 components and 0.247757 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 milli-arcsec
! Estimated beam: bmin=0.8725 mas, bmaj=2.127 mas, bpa=0.1899 degrees
! Estimated noise=0.945241 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.000587003 Jy
! Component: 100  -  total flux cleaned = -0.000485318 Jy
! Component: 150  -  total flux cleaned = -0.00040426 Jy
! Component: 200  -  total flux cleaned = -0.000443193 Jy
! Total flux subtracted in 200 components = -0.000443193 Jy
! Clean residual min=-0.003622 max=0.002794 Jy/beam
! Clean residual mean=0.000003 rms=0.000769 Jy/beam
! Combined flux in latest and established models = 0.247314 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 21 model components to the UV plane model.
! The established model now contains 87 components and 0.247314 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.048662Jy  sigma=0.922503
! Fit after  self-cal, rms=0.048656Jy  sigma=0.922454
wmodel J1951-0509_X_2005_06_01_yyk\_map.mod
! Writing 87 model components to file: J1951-0509_X_2005_06_01_yyk_map.mod
wobs J1951-0509_X_2005_06_01_yyk\_uvs.fits
! Writing UV FITS file: J1951-0509_X_2005_06_01_yyk_uvs.fits
wwins J1951-0509_X_2005_06_01_yyk\_map.win
! wwins: Wrote 2 windows to J1951-0509_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 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00139054 Jy
! Component: 100  -  total flux cleaned = -0.00164684 Jy
! Component: 150  -  total flux cleaned = -0.00169515 Jy
! Component: 200  -  total flux cleaned = -0.00165149 Jy
! Component: 250  -  total flux cleaned = -0.00169514 Jy
! Component: 300  -  total flux cleaned = -0.00186349 Jy
! Component: 350  -  total flux cleaned = -0.0019446 Jy
! Component: 400  -  total flux cleaned = -0.001945 Jy
! Component: 450  -  total flux cleaned = -0.0019456 Jy
! Component: 500  -  total flux cleaned = -0.00198448 Jy
! Component: 550  -  total flux cleaned = -0.00205955 Jy
! Component: 600  -  total flux cleaned = -0.00209604 Jy
! Component: 650  -  total flux cleaned = -0.00213168 Jy
! Component: 700  -  total flux cleaned = -0.00213199 Jy
! Component: 750  -  total flux cleaned = -0.00223605 Jy
! Component: 800  -  total flux cleaned = -0.0022017 Jy
! Component: 850  -  total flux cleaned = -0.00220166 Jy
! Component: 900  -  total flux cleaned = -0.00223439 Jy
! Component: 950  -  total flux cleaned = -0.00229902 Jy
! Component: 1000  -  total flux cleaned = -0.0022023 Jy
! Component: 1050  -  total flux cleaned = -0.0021389 Jy
! Component: 1100  -  total flux cleaned = -0.00207718 Jy
! Component: 1150  -  total flux cleaned = -0.00207839 Jy
! Component: 1200  -  total flux cleaned = -0.00207871 Jy
! Component: 1250  -  total flux cleaned = -0.00204774 Jy
! Component: 1300  -  total flux cleaned = -0.00204791 Jy
! Component: 1350  -  total flux cleaned = -0.00195962 Jy
! Component: 1400  -  total flux cleaned = -0.00193028 Jy
! Component: 1450  -  total flux cleaned = -0.00198773 Jy
! Component: 1500  -  total flux cleaned = -0.00195868 Jy
! Component: 1550  -  total flux cleaned = -0.00190197 Jy
! Component: 1600  -  total flux cleaned = -0.00192995 Jy
! Component: 1650  -  total flux cleaned = -0.00193021 Jy
! Component: 1700  -  total flux cleaned = -0.00190273 Jy
! Component: 1750  -  total flux cleaned = -0.00187544 Jy
! Component: 1800  -  total flux cleaned = -0.00187549 Jy
! Component: 1850  -  total flux cleaned = -0.0018487 Jy
! Component: 1900  -  total flux cleaned = -0.00184884 Jy
! Component: 1950  -  total flux cleaned = -0.00190119 Jy
! Component: 2000  -  total flux cleaned = -0.00179746 Jy
! Total flux subtracted in 2048 components = -0.00179728 Jy
! Clean residual min=-0.001556 max=0.001611 Jy/beam
! Clean residual mean=0.000004 rms=0.000481 Jy/beam
! Combined flux in latest and established models = 0.245516 Jy
keep
! Adding 139 model components to the UV plane model.
! The established model now contains 226 components and 0.245516 Jy
![Exited script file: muppet]
wmap "J1951-0509_X_2005_06_01_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8725 x 2.127 at 0.1899 degrees (North through East)
! Clean map  min=-0.0024762  max=0.21521 Jy/beam
! Writing clean map to FITS file: J1951-0509_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 0.215208 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.235% of the data.
!  The x-axis pixel size should ideally be below 0.1991 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000477802 
device "J1951-0509_X_2005_06_01_yyk\_map.eps/VPS"
! Attempting to open device: 'J1951-0509_X_2005_06_01_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.666056 0.666056 1.33211 2.66422 5.32844 10.6569 21.3138 42.6276 85.2551
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0014 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.215 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8725 x 2.127 at 0.1899 degrees (North through East)
! Clean map  min=-0.0024762  max=0.21521 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1951-0509_X_2005_06_01_yyk\_map.gif/gif"
! Attempting to open device: 'J1951-0509_X_2005_06_01_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1951-0509_X_2005_06_01_yyk_uvs.log closed on Sat Oct  8 17:41:18 2005