! Started logfile: J2245+0500_X_2009_04_21_pus_uvs.log on Sun Jan 23 00:40:18 2011
obs J2245+0500_X_2009_04_21_pus_uva.fits
! Reading UV FITS file: J2245+0500_X_2009_04_21_pus_uva.fits
! AN table 1: 190 integrations on 120 of 120 possible baselines.
! AN table 2: 40 integrations on 120 of 120 possible baselines.
! AN table 3: 44 integrations on 120 of 120 possible baselines.
! Apparent sampling: 0.119191 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J2245+0500
! 
! 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 2445 lines of history.
! 
! Reading 15676 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 = 512 
print "field_cell =",field_cell
! field_cell = 0.2 
print "taper_size =",taper_size
! taper_size = 70 
![@muppet J2245+0500_X_2009_04_21_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 = 512x512 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 2356 telescope corrections were flagged in sub-array 1.
!  A total of 409 telescope corrections were flagged in sub-array 2.
!  A total of 617 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 2356 telescope corrections were flagged in sub-array 1.
!  A total of 409 telescope corrections were flagged in sub-array 2.
!  A total of 617 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 2356 telescope corrections were flagged in sub-array 1.
!  A total of 409 telescope corrections were flagged in sub-array 2.
!  A total of 617 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 2356 telescope corrections were flagged in sub-array 1.
!  A total of 409 telescope corrections were flagged in sub-array 2.
!  A total of 617 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=0.757680Jy  sigma=0.006732
! Fit after  self-cal, rms=0.720707Jy  sigma=0.006452
! 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 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.1893 milli-arcsec
! Estimated beam: bmin=0.6081 mas, bmaj=1.768 mas, bpa=0.9409 degrees
! Estimated noise=948.983 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 = 0.224346 Jy
! Component: 100  -  total flux cleaned = 0.274107 Jy
! Total flux subtracted in 100 components = 0.274107 Jy
! Clean residual min=-0.006614 max=0.016767 Jy/beam
! Clean residual mean=0.000057 rms=0.001660 Jy/beam
! Combined flux in latest and established models = 0.274107 Jy
! Performing phase self-cal
! Adding 4 model components to the UV plane model.
! The established model now contains 4 components and 0.274107 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.159563Jy  sigma=0.001241
! Fit after  self-cal, rms=0.159561Jy  sigma=0.001241
! Inverting map 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.1893 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0186522 Jy
! Component: 100  -  total flux cleaned = 0.0295927 Jy
! Total flux subtracted in 100 components = 0.0295927 Jy
! Clean residual min=-0.004948 max=0.005806 Jy/beam
! Clean residual mean=0.000039 rms=0.001245 Jy/beam
! Combined flux in latest and established models = 0.3037 Jy
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 20 components and 0.3037 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.156683Jy  sigma=0.001205
! Fit after  self-cal, rms=0.156685Jy  sigma=0.001205
! Inverting map 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.1893 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 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.1893 milli-arcsec
! Estimated beam: bmin=0.7423 mas, bmaj=2.091 mas, bpa=-0.03616 degrees
! Estimated noise=658.107 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 = 0.0103831 Jy
! Component: 100  -  total flux cleaned = 0.0158552 Jy
! Component: 150  -  total flux cleaned = 0.0189625 Jy
! Component: 200  -  total flux cleaned = 0.0207635 Jy
! Total flux subtracted in 200 components = 0.0207635 Jy
! Clean residual min=-0.003385 max=0.004315 Jy/beam
! Clean residual mean=0.000311 rms=0.000896 Jy/beam
! Combined flux in latest and established models = 0.324463 Jy
! Performing phase self-cal
! Adding 31 model components to the UV plane model.
! The established model now contains 39 components and 0.324463 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.156097Jy  sigma=0.001197
! Fit after  self-cal, rms=0.156110Jy  sigma=0.001197
! Inverting map 
! Your choice of large map pixels excluded 1.31% of the data.
!  The x-axis pixel size should ideally be below 0.1893 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 63 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     FD        1.01     HN        1.01     KB        0.95     
!   KK        1.05     KP        1.00     LA        0.97     MK        0.97     
!   NL        0.98     NY        1.00*    OV        1.01     PT        1.02     
!   SC        0.96     TS        1.10     WZ        1.00*    ZC        1.00*    
! 
!  A total of 42 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.98     FD        0.97     HN        0.96     KB        1.00*    
!   KK        1.00     KP        0.97     LA        1.04     MK        0.98     
!   NL        0.94     NY        1.00*    OV        1.01     PT        0.99     
!   SC        0.95     TS        1.00*    WZ        1.00*    ZC        1.00*    
! 
!  A total of 51 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        1.00*    HN        1.00*    KB        0.90     
!   KK        0.96     KP        1.00*    LA        1.00*    MK        0.98     
!   NL        1.00*    NY        1.00*    OV        1.00*    PT        1.00*    
!   SC        1.00*    TS        0.96     WZ        1.00*    ZC        1.00*    
! 
! 
! Correcting IF 2.
!  A total of 63 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     FD        0.97     HN        1.02     KB        0.97     
!   KK        1.01     KP        1.00     LA        0.99     MK        1.02     
!   NL        1.00     NY        1.00*    OV        1.00     PT        0.98     
!   SC        1.01     TS        1.16     WZ        1.00*    ZC        1.00*    
! 
!  A total of 42 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.98     FD        0.98     HN        1.01     KB        1.00*    
!   KK        0.93     KP        1.00     LA        1.05     MK        0.99     
!   NL        0.97     NY        1.00*    OV        0.96     PT        0.95     
!   SC        1.01     TS        1.00*    WZ        1.00*    ZC        1.00*    
! 
!  A total of 51 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        1.00*    HN        1.00*    KB        0.80     
!   KK        0.96     KP        1.00*    LA        1.00*    MK        1.16     
!   NL        1.00*    NY        1.00*    OV        1.00*    PT        1.00*    
!   SC        1.00*    TS        0.97     WZ        1.00*    ZC        1.00*    
! 
! 
! Correcting IF 3.
!  A total of 63 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.01     FD        0.99     HN        1.00     KB        1.01     
!   KK        1.02     KP        0.99     LA        0.98     MK        1.01     
!   NL        1.02     NY        1.00*    OV        1.04     PT        1.00     
!   SC        1.08     TS        1.06     WZ        1.00*    ZC        1.00*    
! 
!  A total of 42 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        1.00     HN        1.10     KB        1.00*    
!   KK        0.98     KP        1.00     LA        1.01     MK        0.99     
!   NL        1.02     NY        1.00*    OV        0.97     PT        0.94     
!   SC        1.04     TS        1.00*    WZ        1.00*    ZC        1.00*    
! 
!  A total of 51 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        1.00*    HN        1.00*    KB        1.02     
!   KK        0.99     KP        1.00*    LA        1.00*    MK        0.92     
!   NL        1.00*    NY        1.00*    OV        1.00*    PT        1.00*    
!   SC        1.00*    TS        0.85     WZ        1.00*    ZC        1.00*    
! 
! 
! Correcting IF 4.
!  A total of 63 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.02     FD        0.98     HN        0.99     KB        0.93     
!   KK        1.06     KP        0.98     LA        1.00     MK        1.03     
!   NL        1.04     NY        1.00*    OV        1.02     PT        1.02     
!   SC        1.06     TS        1.16     WZ        1.00*    ZC        1.00*    
! 
!  A total of 42 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.01     FD        0.99     HN        1.03     KB        1.00*    
!   KK        1.05     KP        1.04     LA        1.05     MK        1.01     
!   NL        1.01     NY        1.00*    OV        1.03     PT        0.95     
!   SC        0.97     TS        1.00*    WZ        1.00*    ZC        1.00*    
! 
!  A total of 51 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    FD        1.00*    HN        1.00*    KB        0.92     
!   KK        0.83     KP        1.00*    LA        1.00*    MK        1.02     
!   NL        1.00*    NY        1.00*    OV        1.00*    PT        1.00*    
!   SC        1.00*    TS        0.92     WZ        1.00*    ZC        1.00*    
! 
! 
! Fit before self-cal, rms=0.156110Jy  sigma=0.001197
! Fit after  self-cal, rms=0.158065Jy  sigma=0.001197
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 milli-arcsec
! Estimated beam: bmin=0.7691 mas, bmaj=2.078 mas, bpa=-0.9346 degrees
! Estimated noise=675.439 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 = -0.000694516 Jy
! Component: 100  -  total flux cleaned = -0.000750642 Jy
! Component: 150  -  total flux cleaned = -0.000774741 Jy
! Component: 200  -  total flux cleaned = -0.000796628 Jy
! Total flux subtracted in 200 components = -0.000796628 Jy
! Clean residual min=-0.003678 max=0.003518 Jy/beam
! Clean residual mean=-0.000005 rms=0.000836 Jy/beam
! Combined flux in latest and established models = 0.323666 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 44 components and 0.323666 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.158055Jy  sigma=0.001197
! Fit after  self-cal, rms=0.158104Jy  sigma=0.001197
! Inverting map 
! Your choice of large map pixels excluded 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 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=0.158104Jy  sigma=0.001197
! Fit after  self-cal, rms=0.158506Jy  sigma=0.001193
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 milli-arcsec
! Estimated beam: bmin=0.7692 mas, bmaj=2.08 mas, bpa=-0.9358 degrees
! Estimated noise=675.507 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000258006 Jy
! Component: 100  -  total flux cleaned = -0.000303924 Jy
! Component: 150  -  total flux cleaned = -0.000345619 Jy
! Component: 200  -  total flux cleaned = -0.000383627 Jy
! Total flux subtracted in 200 components = -0.000383627 Jy
! Clean residual min=-0.003297 max=0.003074 Jy/beam
! Clean residual mean=-0.000006 rms=0.000791 Jy/beam
! Combined flux in latest and established models = 0.323283 Jy
selfcal
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 49 components and 0.323283 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.158503Jy  sigma=0.001193
! Fit after  self-cal, rms=0.158514Jy  sigma=0.001193
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 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 = -6.64939e-05 Jy
! Component: 100  -  total flux cleaned = -8.93838e-05 Jy
! Component: 150  -  total flux cleaned = -0.000111485 Jy
! Component: 200  -  total flux cleaned = -0.000132747 Jy
! Total flux subtracted in 200 components = -0.000132747 Jy
! Clean residual min=-0.003306 max=0.003087 Jy/beam
! Clean residual mean=-0.000006 rms=0.000791 Jy/beam
! Combined flux in latest and established models = 0.32315 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 49 components and 0.32315 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.158513Jy  sigma=0.001193
! Fit after  self-cal, rms=0.158512Jy  sigma=0.001193
! Inverting map 
! Your choice of large map pixels excluded 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 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=0.158512Jy  sigma=0.001193
! Fit after  self-cal, rms=0.158700Jy  sigma=0.001193
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 milli-arcsec
! Estimated beam: bmin=0.7698 mas, bmaj=2.08 mas, bpa=-0.9378 degrees
! Estimated noise=675.932 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -6.01416e-05 Jy
! Component: 100  -  total flux cleaned = -0.000111404 Jy
! Component: 150  -  total flux cleaned = -0.000147276 Jy
! Component: 200  -  total flux cleaned = -0.000181116 Jy
! Total flux subtracted in 200 components = -0.000181116 Jy
! Clean residual min=-0.003286 max=0.003057 Jy/beam
! Clean residual mean=0.000002 rms=0.000788 Jy/beam
! Combined flux in latest and established models = 0.322969 Jy
selfcal
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 49 components and 0.322969 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.158698Jy  sigma=0.001192
! Fit after  self-cal, rms=0.158702Jy  sigma=0.001192
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 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 = -3.38354e-05 Jy
! Component: 100  -  total flux cleaned = -5.46132e-05 Jy
! Component: 150  -  total flux cleaned = -7.44958e-05 Jy
! Component: 200  -  total flux cleaned = -8.43173e-05 Jy
! Total flux subtracted in 200 components = -8.43173e-05 Jy
! Clean residual min=-0.003290 max=0.003067 Jy/beam
! Clean residual mean=0.000002 rms=0.000787 Jy/beam
! Combined flux in latest and established models = 0.322885 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 49 components and 0.322885 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.158701Jy  sigma=0.001192
! Fit after  self-cal, rms=0.158700Jy  sigma=0.001192
! Inverting map 
! Your choice of large map pixels excluded 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 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=0.158700Jy  sigma=0.001192
! Fit after  self-cal, rms=0.158859Jy  sigma=0.001192
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 milli-arcsec
! Estimated beam: bmin=2.208 mas, bmaj=3.274 mas, bpa=-4.852 degrees
! Estimated noise=871.118 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000249872 Jy
! Component: 100  -  total flux cleaned = -0.000268581 Jy
! Component: 150  -  total flux cleaned = -0.000322271 Jy
! Component: 200  -  total flux cleaned = -0.000371152 Jy
! Total flux subtracted in 200 components = -0.000371152 Jy
! Clean residual min=-0.003056 max=0.003846 Jy/beam
! Clean residual mean=0.000026 rms=0.001033 Jy/beam
! Combined flux in latest and established models = 0.322514 Jy
selfcal
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 52 components and 0.322514 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.158861Jy  sigma=0.001192
! Fit after  self-cal, rms=0.158863Jy  sigma=0.001192
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 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 = -9.2419e-05 Jy
! Component: 100  -  total flux cleaned = -0.000106524 Jy
! Component: 150  -  total flux cleaned = -0.000145592 Jy
! Component: 200  -  total flux cleaned = -0.000180932 Jy
! Total flux subtracted in 200 components = -0.000180932 Jy
! Clean residual min=-0.003067 max=0.003844 Jy/beam
! Clean residual mean=0.000028 rms=0.001032 Jy/beam
! Combined flux in latest and established models = 0.322333 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 54 components and 0.322333 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.158865Jy  sigma=0.001193
! Fit after  self-cal, rms=0.158867Jy  sigma=0.001192
! Inverting map 
! Your choice of large map pixels excluded 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 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 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 milli-arcsec
! Estimated beam: bmin=0.7702 mas, bmaj=2.081 mas, bpa=-0.9409 degrees
! Estimated noise=676.383 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7702 x 2.081 at -0.9409 degrees (North through East)
! Clean map  min=-0.0029189  max=0.29709 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 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 milli-arcsec
! Estimated beam: bmin=0.6382 mas, bmaj=1.749 mas, bpa=-0.2506 degrees
! Estimated noise=986.573 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.228208 Jy
! Component: 100  -  total flux cleaned = 0.278505 Jy
! Component: 150  -  total flux cleaned = 0.296259 Jy
! Component: 200  -  total flux cleaned = 0.306458 Jy
! Total flux subtracted in 200 components = 0.306458 Jy
! Clean residual min=-0.004298 max=0.005244 Jy/beam
! Clean residual mean=0.000006 rms=0.001108 Jy/beam
! Combined flux in latest and established models = 0.306458 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 19 model components to the UV plane model.
! The established model now contains 19 components and 0.306458 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 milli-arcsec
! Estimated beam: bmin=0.7702 mas, bmaj=2.081 mas, bpa=-0.9409 degrees
! Estimated noise=676.383 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 = 0.00774917 Jy
! Component: 100  -  total flux cleaned = 0.0117729 Jy
! Component: 150  -  total flux cleaned = 0.0140236 Jy
! Component: 200  -  total flux cleaned = 0.0153172 Jy
! Total flux subtracted in 200 components = 0.0153172 Jy
! Clean residual min=-0.003391 max=0.003160 Jy/beam
! Clean residual mean=0.000012 rms=0.000791 Jy/beam
! Combined flux in latest and established models = 0.321775 Jy
! Adding 29 model components to the UV plane model.
! The established model now contains 41 components and 0.321775 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 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 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 milli-arcsec
! Estimated beam: bmin=2.208 mas, bmaj=3.274 mas, bpa=-4.852 degrees
! Estimated noise=871.118 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000774758 Jy
! Component: 100  -  total flux cleaned = 0.000775 Jy
! Component: 150  -  total flux cleaned = 0.000760727 Jy
! Component: 200  -  total flux cleaned = 0.000718258 Jy
! Total flux subtracted in 200 components = 0.000718258 Jy
! Clean residual min=-0.003068 max=0.003845 Jy/beam
! Clean residual mean=0.000026 rms=0.001033 Jy/beam
! Combined flux in latest and established models = 0.322493 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 = -2.56721e-05 Jy
! Component: 100  -  total flux cleaned = -6.12418e-05 Jy
! Component: 150  -  total flux cleaned = -9.36401e-05 Jy
! Component: 200  -  total flux cleaned = -0.000113386 Jy
! Total flux subtracted in 200 components = -0.000113386 Jy
! Clean residual min=-0.003072 max=0.003843 Jy/beam
! Clean residual mean=0.000027 rms=0.001032 Jy/beam
! Combined flux in latest and established models = 0.32238 Jy
! Adding 10 model components to the UV plane model.
! The established model now contains 47 components and 0.32238 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 milli-arcsec
! Estimated beam: bmin=0.7702 mas, bmaj=2.081 mas, bpa=-0.9409 degrees
! Estimated noise=676.383 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -4.41901e-05 Jy
! Component: 100  -  total flux cleaned = 9.15742e-05 Jy
! Component: 150  -  total flux cleaned = 0.000203399 Jy
! Component: 200  -  total flux cleaned = 0.000297617 Jy
! Total flux subtracted in 200 components = 0.000297617 Jy
! Clean residual min=-0.003339 max=0.003150 Jy/beam
! Clean residual mean=0.000008 rms=0.000790 Jy/beam
! Combined flux in latest and established models = 0.322677 Jy
selfcal
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 50 components and 0.322677 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.158875Jy  sigma=0.001193
! Fit after  self-cal, rms=0.158872Jy  sigma=0.001193
wmodel J2245+0500_X_2009_04_21_pus_map.mod
! Writing 50 model components to file: J2245+0500_X_2009_04_21_pus_map.mod
wobs J2245+0500_X_2009_04_21_pus_uvs.fits
! Writing UV FITS file: J2245+0500_X_2009_04_21_pus_uvs.fits
wwins J2245+0500_X_2009_04_21_pus_map.win
! wwins: Wrote 1 windows to J2245+0500_X_2009_04_21_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 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000429737 Jy
! Component: 100  -  total flux cleaned = -0.00016433 Jy
! Component: 150  -  total flux cleaned = 8.61098e-05 Jy
! Component: 200  -  total flux cleaned = 0.000327359 Jy
! Component: 250  -  total flux cleaned = 0.000609716 Jy
! Component: 300  -  total flux cleaned = 0.000884336 Jy
! Component: 350  -  total flux cleaned = 0.00119558 Jy
! Component: 400  -  total flux cleaned = 0.00119568 Jy
! Component: 450  -  total flux cleaned = 0.00140886 Jy
! Component: 500  -  total flux cleaned = 0.00149253 Jy
! Component: 550  -  total flux cleaned = 0.0016572 Jy
! Component: 600  -  total flux cleaned = 0.00181911 Jy
! Component: 650  -  total flux cleaned = 0.00181948 Jy
! Component: 700  -  total flux cleaned = 0.00185896 Jy
! Component: 750  -  total flux cleaned = 0.0018594 Jy
! Component: 800  -  total flux cleaned = 0.00182146 Jy
! Component: 850  -  total flux cleaned = 0.00189721 Jy
! Component: 900  -  total flux cleaned = 0.00185933 Jy
! Component: 950  -  total flux cleaned = 0.00174837 Jy
! Component: 1000  -  total flux cleaned = 0.00185887 Jy
! Component: 1050  -  total flux cleaned = 0.00189493 Jy
! Component: 1100  -  total flux cleaned = 0.00196646 Jy
! Component: 1150  -  total flux cleaned = 0.00189483 Jy
! Component: 1200  -  total flux cleaned = 0.00185987 Jy
! Component: 1250  -  total flux cleaned = 0.00199976 Jy
! Component: 1300  -  total flux cleaned = 0.00193004 Jy
! Component: 1350  -  total flux cleaned = 0.00196463 Jy
! Component: 1400  -  total flux cleaned = 0.0019307 Jy
! Component: 1450  -  total flux cleaned = 0.00196466 Jy
! Component: 1500  -  total flux cleaned = 0.00199792 Jy
! Component: 1550  -  total flux cleaned = 0.00193157 Jy
! Component: 1600  -  total flux cleaned = 0.00196467 Jy
! Component: 1650  -  total flux cleaned = 0.00196489 Jy
! Component: 1700  -  total flux cleaned = 0.00202951 Jy
! Component: 1750  -  total flux cleaned = 0.00206172 Jy
! Component: 1800  -  total flux cleaned = 0.00202991 Jy
! Component: 1850  -  total flux cleaned = 0.00202986 Jy
! Component: 1900  -  total flux cleaned = 0.00206147 Jy
! Component: 1950  -  total flux cleaned = 0.00215457 Jy
! Component: 2000  -  total flux cleaned = 0.00215458 Jy
! Total flux subtracted in 2048 components = 0.00212388 Jy
! Clean residual min=-0.001859 max=0.001719 Jy/beam
! Clean residual mean=0.000001 rms=0.000582 Jy/beam
! Combined flux in latest and established models = 0.324801 Jy
keep
! Adding 145 model components to the UV plane model.
! The established model now contains 195 components and 0.324801 Jy
![Exited script file: muppet]
wmap "J2245+0500_X_2009_04_21_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7702 x 2.081 at -0.9409 degrees (North through East)
! Clean map  min=-0.0026318  max=0.29738 Jy/beam
! Writing clean map to FITS file: J2245+0500_X_2009_04_21_pus_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.297379 
invert
! Inverting map 
! Your choice of large map pixels excluded 1.36% of the data.
!  The x-axis pixel size should ideally be below 0.1893 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000580816 
device "J2245+0500_X_2009_04_21_pus\_map.eps/VPS"
! Attempting to open device: 'J2245+0500_X_2009_04_21_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.585935 0.585935 1.17187 2.34374 4.68748 9.37497 18.7499 37.4999 74.9997
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0017 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.297 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7702 x 2.081 at -0.9409 degrees (North through East)
! Clean map  min=-0.0026318  max=0.29738 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J2245+0500_X_2009_04_21_pus\_map.gif/vgif"
! Attempting to open device: 'J2245+0500_X_2009_04_21_pus_map.gif/vgif'
mapplot cln