! Started logfile: 0809+483_X_2010_10_13_pus_uvs.log on Mon Feb 28 17:57:20 2011
obs 0809+483_X_2010_10_13_pus_uva.fits
! Reading UV FITS file: 0809+483_X_2010_10_13_pus_uva.fits
! AN table 1: 119 integrations on 105 of 105 possible baselines.
! AN table 2: Unused.
! AN table 3: Unused.
! AN table 4: Unused.
! AN table 5: Unused.
! Apparent sampling: 0.262585 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: 0809+483
! 
! 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  8.40996e+09        8e+06          1        8e+06
!  02        2  8.47996e+09        8e+06          1        8e+06
!  03        3  8.79496e+09        8e+06          1        8e+06
!  04        4  8.89996e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 5974 lines of history.
! 
! Reading 13124 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
print "field_size =",field_size
! field_size = 256 
print "field_cell =",field_cell
! field_cell = 0.2 
print "taper_size =",taper_size
! taper_size = 70 
![@muppet 0809+483_X_2010_10_13_pus]
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.03
float dynam
dynam = 6.0
float soltime1
soltime1 = 120
float soltime2
soltime2 = 20
float thresh
thresh = 0.5
float win_mult
win_mult = 1.8
float time_av
time_av = 16
float old_peak
float new_peak
float flux_cutoff
mapsize field_size, field_cell
! Map grid = 256x256 pixels with 0.200x0.200 milli-arcsec cellsize.
startmod
! Applying default point source starting model.
! Performing phase self-cal
! Adding 1 model components to the UV plane model.
! The established model now contains 1 components and 1 Jy
! 
! Correcting IF 1.
!  A total of 1078 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 1078 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 1102 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 1102 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=1.005942Jy  sigma=0.013471
! Fit after  self-cal, rms=0.958380Jy  sigma=0.012797
! clrmod: Cleared the established, tentative and continuum models.
! Redundant starting model cleared.
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 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
! Estimated beam: bmin=0.6216 mas, bmaj=1.005 mas, bpa=-12.17 degrees
! Estimated noise=939.525 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (0, 0).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.039214 Jy
! Component: 100  -  total flux cleaned = 0.0487337 Jy
! Total flux subtracted in 100 components = 0.0487337 Jy
! Clean residual min=-0.006616 max=0.005863 Jy/beam
! Clean residual mean=0.000049 rms=0.001590 Jy/beam
! Combined flux in latest and established models = 0.0487337 Jy
! Performing phase self-cal
! Adding 4 model components to the UV plane model.
! The established model now contains 4 components and 0.0487337 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.114897Jy  sigma=0.001254
! Fit after  self-cal, rms=0.113006Jy  sigma=0.001229
! Inverting map 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
print "************** FINISHED UNIFORM WEIGHTING CLEAN **************"
! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** 
! 
uvw 0,-1
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -1.
! 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 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
! Estimated beam: bmin=0.6867 mas, bmaj=1.197 mas, bpa=-8.864 degrees
! Estimated noise=533.389 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00418035 Jy
! Component: 100  -  total flux cleaned = 0.00452585 Jy
! Component: 150  -  total flux cleaned = 0.0044136 Jy
! Component: 200  -  total flux cleaned = 0.00427386 Jy
! Total flux subtracted in 200 components = 0.00427386 Jy
! Clean residual min=-0.003710 max=0.003391 Jy/beam
! Clean residual mean=0.000144 rms=0.000902 Jy/beam
! Combined flux in latest and established models = 0.0530076 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 11 components and 0.0530076 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.112798Jy  sigma=0.001228
! Fit after  self-cal, rms=0.112678Jy  sigma=0.001228
! Inverting map 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.06     FD        0.88     HH        1.00*    HN        0.77     
!   KB        1.14     KK        1.00*    KP        1.13     LA        1.06     
!   MK        1.13     NL        1.09     NY        1.00*    OV        1.01     
!   PT        1.11     SC        0.84     TS        0.99     
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.10     FD        1.06     HH        1.00*    HN        0.73     
!   KB        1.17     KK        1.00*    KP        1.05     LA        1.08     
!   MK        1.00     NL        1.13     NY        1.00*    OV        1.24     
!   PT        1.18     SC        0.86     TS        0.93     
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.86     FD        0.94     HH        1.00*    HN        0.75     
!   KB        1.14     KK        1.00*    KP        1.04     LA        0.87     
!   MK        1.08     NL        1.02     NY        1.00*    OV        1.02     
!   PT        1.23     SC        0.88     TS        0.94     
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.93     FD        0.94     HH        1.00*    HN        0.65     
!   KB        1.16     KK        1.00*    KP        0.96     LA        1.08     
!   MK        0.85     NL        1.00     NY        1.00*    OV        0.98     
!   PT        1.16     SC        0.73     TS        0.88     
! 
! 
! Fit before self-cal, rms=0.112678Jy  sigma=0.001228
! Fit after  self-cal, rms=0.098316Jy  sigma=0.001222
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
! Estimated beam: bmin=0.702 mas, bmaj=1.163 mas, bpa=-10.41 degrees
! Estimated noise=526.589 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000803981 Jy
! Component: 100  -  total flux cleaned = 0.00095439 Jy
! Component: 150  -  total flux cleaned = 0.000996317 Jy
! Component: 200  -  total flux cleaned = 0.00100916 Jy
! Total flux subtracted in 200 components = 0.00100916 Jy
! Clean residual min=-0.001844 max=0.002520 Jy/beam
! Clean residual mean=0.000245 rms=0.000633 Jy/beam
! Combined flux in latest and established models = 0.0540168 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 17 components and 0.0540168 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.098312Jy  sigma=0.001222
! Fit after  self-cal, rms=0.098101Jy  sigma=0.001220
! Inverting map 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
selfcal true, true, soltime1
! Performing amp+phase self-cal over 120 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.098101Jy  sigma=0.001220
! Fit after  self-cal, rms=0.097500Jy  sigma=0.001219
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
! Estimated beam: bmin=0.7035 mas, bmaj=1.159 mas, bpa=-10.03 degrees
! Estimated noise=525.48 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000190718 Jy
! Component: 100  -  total flux cleaned = 0.000174008 Jy
! Component: 150  -  total flux cleaned = 0.000174373 Jy
! Component: 200  -  total flux cleaned = 0.000174874 Jy
! Total flux subtracted in 200 components = 0.000174874 Jy
! Clean residual min=-0.002014 max=0.002285 Jy/beam
! Clean residual mean=0.000219 rms=0.000614 Jy/beam
! Combined flux in latest and established models = 0.0541916 Jy
selfcal
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 21 components and 0.0541916 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.097496Jy  sigma=0.001218
! Fit after  self-cal, rms=0.097539Jy  sigma=0.001218
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000111336 Jy
! Component: 100  -  total flux cleaned = -0.000135419 Jy
! Component: 150  -  total flux cleaned = -0.000156318 Jy
! Component: 200  -  total flux cleaned = -0.000175509 Jy
! Total flux subtracted in 200 components = -0.000175509 Jy
! Clean residual min=-0.002094 max=0.002235 Jy/beam
! Clean residual mean=0.000232 rms=0.000625 Jy/beam
! Combined flux in latest and established models = 0.0540161 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 24 components and 0.0540161 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.097538Jy  sigma=0.001218
! Fit after  self-cal, rms=0.097537Jy  sigma=0.001218
! Inverting map 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
selfcal true, true, soltime2
! Performing amp+phase self-cal over 20 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.097537Jy  sigma=0.001218
! Fit after  self-cal, rms=0.098345Jy  sigma=0.001218
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
! Estimated beam: bmin=0.7016 mas, bmaj=1.159 mas, bpa=-9.621 degrees
! Estimated noise=527.342 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000230853 Jy
! Component: 100  -  total flux cleaned = 0.000216597 Jy
! Component: 150  -  total flux cleaned = 0.000227385 Jy
! Component: 200  -  total flux cleaned = 0.000236963 Jy
! Total flux subtracted in 200 components = 0.000236963 Jy
! Clean residual min=-0.002219 max=0.002244 Jy/beam
! Clean residual mean=0.000208 rms=0.000623 Jy/beam
! Combined flux in latest and established models = 0.0542531 Jy
selfcal
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 24 components and 0.0542531 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.098342Jy  sigma=0.001218
! Fit after  self-cal, rms=0.098380Jy  sigma=0.001217
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -6.49263e-05 Jy
! Component: 100  -  total flux cleaned = -8.66204e-05 Jy
! Component: 150  -  total flux cleaned = -9.63251e-05 Jy
! Component: 200  -  total flux cleaned = -9.65576e-05 Jy
! Total flux subtracted in 200 components = -9.65576e-05 Jy
! Clean residual min=-0.002317 max=0.002275 Jy/beam
! Clean residual mean=0.000231 rms=0.000631 Jy/beam
! Combined flux in latest and established models = 0.0541565 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 26 components and 0.0541565 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.098380Jy  sigma=0.001217
! Fit after  self-cal, rms=0.098386Jy  sigma=0.001217
! Inverting map 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
win_mult = win_mult * 1.2
selfcal true, true, soltime2
! Performing amp+phase self-cal over 20 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.098386Jy  sigma=0.001217
! Fit after  self-cal, rms=0.099151Jy  sigma=0.001217
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
! Estimated beam: bmin=2.223 mas, bmaj=2.608 mas, bpa=-89.84 degrees
! Estimated noise=750.865 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000252814 Jy
! Component: 100  -  total flux cleaned = -0.000261494 Jy
! Component: 150  -  total flux cleaned = -0.000282794 Jy
! Component: 200  -  total flux cleaned = -0.000295312 Jy
! Total flux subtracted in 200 components = -0.000295312 Jy
! Clean residual min=-0.002181 max=0.003713 Jy/beam
! Clean residual mean=0.000577 rms=0.000944 Jy/beam
! Combined flux in latest and established models = 0.0538612 Jy
selfcal
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 28 components and 0.0538612 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.099150Jy  sigma=0.001217
! Fit after  self-cal, rms=0.099179Jy  sigma=0.001217
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000253516 Jy
! Component: 100  -  total flux cleaned = -0.000268891 Jy
! Component: 150  -  total flux cleaned = -0.000275784 Jy
! Component: 200  -  total flux cleaned = -0.00028766 Jy
! Total flux subtracted in 200 components = -0.00028766 Jy
! Clean residual min=-0.002216 max=0.003873 Jy/beam
! Clean residual mean=0.000594 rms=0.000951 Jy/beam
! Combined flux in latest and established models = 0.0535736 Jy
! Performing phase self-cal
! Adding 5 model components to the UV plane model.
! The established model now contains 28 components and 0.0535736 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.099180Jy  sigma=0.001217
! Fit after  self-cal, rms=0.099182Jy  sigma=0.001217
! Inverting map 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
win_mult = win_mult / 1.2
print "************** FINISHED AMPLITUDE SELF-CAL **************"
! ************** FINISHED AMPLITUDE SELF-CAL ************** 
restore
! Inverting map and beam 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
! Estimated beam: bmin=0.6991 mas, bmaj=1.159 mas, bpa=-9.198 degrees
! Estimated noise=529.267 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6991 x 1.159 at -9.198 degrees (North through East)
! Clean map  min=-0.0020486  max=0.051029 Jy/beam
if(peak(flux) > thresh)
  selfcal true, true
  clean clean_niter,clean_gain
  selfcal
  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
    new_peak = peak(flux)
    until(new_peak<=flux_cutoff)
  selfcal true, true
  end if
print "************** CLEARING MODEL AND STARTING OVER **********"
! ************** CLEARING MODEL AND STARTING OVER ********** 
clrmod true
! clrmod: Cleared the established and tentative 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 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
! Estimated beam: bmin=0.6363 mas, bmaj=0.9741 mas, bpa=-12.8 degrees
! Estimated noise=866.146 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0395273 Jy
! Component: 100  -  total flux cleaned = 0.0502048 Jy
! Component: 150  -  total flux cleaned = 0.0540219 Jy
! Component: 200  -  total flux cleaned = 0.0544476 Jy
! Total flux subtracted in 200 components = 0.0544476 Jy
! Clean residual min=-0.003247 max=0.003654 Jy/beam
! Clean residual mean=0.000043 rms=0.001017 Jy/beam
! Combined flux in latest and established models = 0.0544476 Jy
uvw 0,-1
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Adding 7 model components to the UV plane model.
! The established model now contains 7 components and 0.0544476 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
! Estimated beam: bmin=0.6991 mas, bmaj=1.159 mas, bpa=-9.198 degrees
! Estimated noise=529.267 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=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000277551 Jy
! Component: 100  -  total flux cleaned = 0.000154377 Jy
! Component: 150  -  total flux cleaned = 1.466e-05 Jy
! Component: 200  -  total flux cleaned = -0.000103159 Jy
! Total flux subtracted in 200 components = -0.000103159 Jy
! Clean residual min=-0.002466 max=0.002347 Jy/beam
! Clean residual mean=0.000198 rms=0.000645 Jy/beam
! Combined flux in latest and established models = 0.0543445 Jy
! Adding 9 model components to the UV plane model.
! The established model now contains 15 components and 0.0543444 Jy
! Inverting map 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
! Estimated beam: bmin=2.223 mas, bmaj=2.608 mas, bpa=-89.84 degrees
! Estimated noise=750.865 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000720541 Jy
! Component: 100  -  total flux cleaned = -0.000752034 Jy
! Component: 150  -  total flux cleaned = -0.000765767 Jy
! Component: 200  -  total flux cleaned = -0.00079114 Jy
! Total flux subtracted in 200 components = -0.00079114 Jy
! Clean residual min=-0.002247 max=0.003870 Jy/beam
! Clean residual mean=0.000586 rms=0.000952 Jy/beam
! Combined flux in latest and established models = 0.0535533 Jy
flux_cutoff = imstat(rms) * dynam
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=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -2.20576e-05 Jy
! Component: 100  -  total flux cleaned = -4.15019e-05 Jy
! Component: 150  -  total flux cleaned = -5.84908e-05 Jy
! Component: 200  -  total flux cleaned = -7.3159e-05 Jy
! Total flux subtracted in 200 components = -7.3159e-05 Jy
! Clean residual min=-0.002214 max=0.003882 Jy/beam
! Clean residual mean=0.000590 rms=0.000949 Jy/beam
! Combined flux in latest and established models = 0.0534802 Jy
! Adding 4 model components to the UV plane model.
! The established model now contains 16 components and 0.0534801 Jy
! Inverting map 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
! Estimated beam: bmin=0.6991 mas, bmaj=1.159 mas, bpa=-9.198 degrees
! Estimated noise=529.267 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000187325 Jy
! Component: 100  -  total flux cleaned = 0.000221074 Jy
! Component: 150  -  total flux cleaned = 0.000206623 Jy
! Component: 200  -  total flux cleaned = 0.000194665 Jy
! Total flux subtracted in 200 components = 0.000194665 Jy
! Clean residual min=-0.002441 max=0.002377 Jy/beam
! Clean residual mean=0.000213 rms=0.000637 Jy/beam
! Combined flux in latest and established models = 0.0536748 Jy
selfcal
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 21 components and 0.0536748 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.099181Jy  sigma=0.001217
! Fit after  self-cal, rms=0.099155Jy  sigma=0.001217
wmodel 0809+483_X_2010_10_13_pus_map.mod
! Writing 21 model components to file: 0809+483_X_2010_10_13_pus_map.mod
wobs 0809+483_X_2010_10_13_pus_uvs.fits
! Writing UV FITS file: 0809+483_X_2010_10_13_pus_uvs.fits
wwins 0809+483_X_2010_10_13_pus_map.win
! wwins: Wrote 1 windows to 0809+483_X_2010_10_13_pus_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 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.000326276 Jy
! Component: 100  -  total flux cleaned = 0.000824972 Jy
! Component: 150  -  total flux cleaned = 0.00131872 Jy
! Component: 200  -  total flux cleaned = 0.00181671 Jy
! Component: 250  -  total flux cleaned = 0.00225788 Jy
! Component: 300  -  total flux cleaned = 0.00255955 Jy
! Component: 350  -  total flux cleaned = 0.0029085 Jy
! Component: 400  -  total flux cleaned = 0.00321753 Jy
! Component: 450  -  total flux cleaned = 0.00354379 Jy
! Component: 500  -  total flux cleaned = 0.00378033 Jy
! Component: 550  -  total flux cleaned = 0.00395939 Jy
! Component: 600  -  total flux cleaned = 0.0041346 Jy
! Component: 650  -  total flux cleaned = 0.00430569 Jy
! Component: 700  -  total flux cleaned = 0.00449646 Jy
! Component: 750  -  total flux cleaned = 0.00465947 Jy
! Component: 800  -  total flux cleaned = 0.00481846 Jy
! Component: 850  -  total flux cleaned = 0.00492985 Jy
! Component: 900  -  total flux cleaned = 0.00508309 Jy
! Component: 950  -  total flux cleaned = 0.0052117 Jy
! Component: 1000  -  total flux cleaned = 0.00535916 Jy
! Total flux subtracted in 1024 components = 0.00542152 Jy
! Clean residual min=-0.001034 max=0.001080 Jy/beam
! Clean residual mean=0.000094 rms=0.000421 Jy/beam
! Combined flux in latest and established models = 0.0590963 Jy
keep
! Adding 85 model components to the UV plane model.
! The established model now contains 106 components and 0.0590963 Jy
![Exited script file: muppet]
wmap "0809+483_X_2010_10_13_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6991 x 1.159 at -9.198 degrees (North through East)
! Clean map  min=-0.0019029  max=0.051012 Jy/beam
! Writing clean map to FITS file: 0809+483_X_2010_10_13_pus_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.0510123 
invert
! Inverting map 
! Your choice of large map pixels excluded 13% of the data.
!  The x-axis pixel size should ideally be below 0.1646 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000415746 
device "0809+483_X_2010_10_13_pus\_map.eps/VPS"
! Attempting to open device: '0809+483_X_2010_10_13_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -2.44498 2.44498 4.88996 9.77992 19.5598 39.1197 78.2393
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0012 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.051 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6991 x 1.159 at -9.198 degrees (North through East)
! Clean map  min=-0.0019029  max=0.051012 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "0809+483_X_2010_10_13_pus\_map.gif/vgif"
! Attempting to open device: '0809+483_X_2010_10_13_pus_map.gif/vgif'
mapplot cln