! Started logfile: J2147+0929_X_2009_04_21_pus_uvs.log on Sun Jan 23 00:39:56 2011
obs J2147+0929_X_2009_04_21_pus_uva.fits
! Reading UV FITS file: J2147+0929_X_2009_04_21_pus_uva.fits
! AN table 1: 171 integrations on 120 of 120 possible baselines.
! AN table 2: 101 integrations on 120 of 120 possible baselines.
! AN table 3: 23 integrations on 120 of 120 possible baselines.
! Apparent sampling: 0.177684 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J2147+0929
! 
! 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 25160 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 J2147+0929_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 1886 telescope corrections were flagged in sub-array 1.
!  A total of 1082 telescope corrections were flagged in sub-array 2.
!  A total of 199 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 1886 telescope corrections were flagged in sub-array 1.
!  A total of 1082 telescope corrections were flagged in sub-array 2.
!  A total of 199 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 1886 telescope corrections were flagged in sub-array 1.
!  A total of 1082 telescope corrections were flagged in sub-array 2.
!  A total of 199 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 1886 telescope corrections were flagged in sub-array 1.
!  A total of 1082 telescope corrections were flagged in sub-array 2.
!  A total of 199 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=0.497842Jy  sigma=0.004384
! Fit after  self-cal, rms=0.232882Jy  sigma=0.002429
! 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 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
! Estimated beam: bmin=0.5289 mas, bmaj=1.57 mas, bpa=-5.226 degrees
! Estimated noise=767.231 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 = 0.689233 Jy
! Component: 100  -  total flux cleaned = 0.847083 Jy
! Total flux subtracted in 100 components = 0.847083 Jy
! Clean residual min=-0.017296 max=0.060302 Jy/beam
! Clean residual mean=-0.000311 rms=0.005308 Jy/beam
! Combined flux in latest and established models = 0.847083 Jy
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 6 components and 0.847083 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.214633Jy  sigma=0.002050
! Fit after  self-cal, rms=0.214544Jy  sigma=0.002050
! Inverting map 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0658115 Jy
! Component: 100  -  total flux cleaned = 0.100508 Jy
! Total flux subtracted in 100 components = 0.100508 Jy
! Clean residual min=-0.015860 max=0.020566 Jy/beam
! Clean residual mean=-0.000470 rms=0.004080 Jy/beam
! Combined flux in latest and established models = 0.947592 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 15 components and 0.947592 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.192441Jy  sigma=0.001832
! Fit after  self-cal, rms=0.192265Jy  sigma=0.001831
! Inverting map 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 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 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
! Estimated beam: bmin=0.594 mas, bmaj=1.713 mas, bpa=-6.032 degrees
! Estimated noise=513.15 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 (0.6, 0).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0250893 Jy
! Component: 100  -  total flux cleaned = 0.0397838 Jy
! Component: 150  -  total flux cleaned = 0.0456891 Jy
! Component: 200  -  total flux cleaned = 0.0465773 Jy
! Total flux subtracted in 200 components = 0.0465773 Jy
! Clean residual min=-0.014052 max=0.011881 Jy/beam
! Clean residual mean=-0.003024 rms=0.002808 Jy/beam
! Combined flux in latest and established models = 0.994169 Jy
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 34 components and 0.994169 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.188619Jy  sigma=0.001805
! Fit after  self-cal, rms=0.188504Jy  sigma=0.001804
! Inverting map 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 27 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     FD        0.99     HN        1.03     KB        2.74     
!   KK        1.05     KP        1.00     LA        0.98     MK        1.01     
!   NL        0.99     NY        1.02     OV        1.01     PT        1.01     
!   SC        1.00     TS        1.10     WZ        1.06     ZC        1.02     
! 
!  A total of 39 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.97     FD        0.99     HN        0.99     KB        1.00*    
!   KK        1.00*    KP        0.98     LA        1.03     MK        1.00*    
!   NL        1.00     NY        1.01     OV        1.00     PT        1.00     
!   SC        0.98     TS        1.00*    WZ        1.09     ZC        0.98     
! 
!  A total of 3 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.96     FD        0.91     HN        0.96     KB        1.01     
!   KK        1.03     KP        0.91     LA        0.88     MK        0.93     
!   NL        0.76     NY        1.00*    OV        0.94     PT        0.94     
!   SC        0.98     TS        0.95     WZ        1.00*    ZC        1.00*    
! 
! 
! Correcting IF 2.
!  A total of 27 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.98     FD        0.99     HN        1.03     KB        2.81     
!   KK        1.04     KP        0.99     LA        0.99     MK        1.01     
!   NL        0.97     NY        1.05     OV        1.00     PT        1.00     
!   SC        1.02     TS        1.12     WZ        0.99     ZC        1.02     
! 
!  A total of 39 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.96     FD        0.98     HN        0.99     KB        1.00*    
!   KK        1.00*    KP        0.99     LA        1.03     MK        1.00*    
!   NL        0.98     NY        1.05     OV        0.98     PT        0.99     
!   SC        0.98     TS        1.00*    WZ        1.01     ZC        0.99     
! 
!  A total of 3 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.95     FD        0.92     HN        0.98     KB        1.05     
!   KK        0.94     KP        0.92     LA        0.88     MK        0.94     
!   NL        0.76     NY        1.00*    OV        0.92     PT        0.90     
!   SC        0.99     TS        0.95     WZ        1.00*    ZC        1.00*    
! 
! 
! Correcting IF 3.
!  A total of 27 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.01     FD        0.98     HN        1.04     KB        1.03     
!   KK        1.03     KP        0.99     LA        0.97     MK        1.01     
!   NL        1.01     NY        1.06     OV        1.01     PT        1.00     
!   SC        1.04     TS        1.13     WZ        0.95     ZC        1.03     
! 
!  A total of 39 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.01     FD        0.99     HN        1.01     KB        1.00*    
!   KK        1.00*    KP        0.98     LA        1.02     MK        1.00*    
!   NL        1.03     NY        1.07     OV        0.99     PT        0.99     
!   SC        1.01     TS        1.00*    WZ        0.99     ZC        0.98     
! 
!  A total of 3 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.98     FD        0.93     HN        0.97     KB        1.03     
!   KK        0.98     KP        0.93     LA        0.89     MK        0.94     
!   NL        0.78     NY        1.00*    OV        0.94     PT        0.91     
!   SC        1.01     TS        0.93     WZ        1.00*    ZC        1.00*    
! 
! 
! Correcting IF 4.
!  A total of 27 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     FD        1.01     HN        1.04     KB        1.00     
!   KK        1.05     KP        0.99     LA        0.98     MK        1.03     
!   NL        1.02     NY        1.02     OV        1.00     PT        0.98     
!   SC        1.03     TS        1.12     WZ        0.98     ZC        1.02     
! 
!  A total of 39 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.98     FD        0.99     HN        0.99     KB        1.00*    
!   KK        1.00*    KP        0.98     LA        1.03     MK        1.00*    
!   NL        1.00     NY        1.04     OV        1.01     PT        0.98     
!   SC        1.00     TS        1.00*    WZ        1.00     ZC        0.97     
! 
!  A total of 3 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.97     FD        0.96     HN        0.97     KB        1.01     
!   KK        0.97     KP        0.91     LA        0.87     MK        0.97     
!   NL        0.79     NY        1.00*    OV        0.95     PT        0.90     
!   SC        1.01     TS        0.94     WZ        1.00*    ZC        1.00*    
! 
! 
! Fit before self-cal, rms=0.188504Jy  sigma=0.001804
! Fit after  self-cal, rms=0.167328Jy  sigma=0.001379
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
! Estimated beam: bmin=0.6025 mas, bmaj=1.728 mas, bpa=-6.277 degrees
! Estimated noise=514.793 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 = -0.0104859 Jy
! Component: 100  -  total flux cleaned = -0.00974598 Jy
! Component: 150  -  total flux cleaned = -0.00932273 Jy
! Component: 200  -  total flux cleaned = -0.0089562 Jy
! Total flux subtracted in 200 components = -0.0089562 Jy
! Clean residual min=-0.005462 max=0.006043 Jy/beam
! Clean residual mean=-0.000530 rms=0.001242 Jy/beam
! Combined flux in latest and established models = 0.985213 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 45 components and 0.985213 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.166436Jy  sigma=0.001370
! Fit after  self-cal, rms=0.166497Jy  sigma=0.001370
! Inverting map 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 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=0.166497Jy  sigma=0.001370
! Fit after  self-cal, rms=0.164086Jy  sigma=0.001350
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
! Estimated beam: bmin=0.6037 mas, bmaj=1.727 mas, bpa=-6.274 degrees
! Estimated noise=513.252 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00446121 Jy
! Component: 100  -  total flux cleaned = -0.004613 Jy
! Component: 150  -  total flux cleaned = -0.00472082 Jy
! Component: 200  -  total flux cleaned = -0.00471601 Jy
! Total flux subtracted in 200 components = -0.00471601 Jy
! Clean residual min=-0.004494 max=0.004460 Jy/beam
! Clean residual mean=-0.000301 rms=0.000951 Jy/beam
! Combined flux in latest and established models = 0.980497 Jy
selfcal
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 51 components and 0.980497 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.163843Jy  sigma=0.001347
! Fit after  self-cal, rms=0.163825Jy  sigma=0.001347
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 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)
! Added new window around map position (2.8, 1).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00444905 Jy
! Component: 100  -  total flux cleaned = 0.00511484 Jy
! Component: 150  -  total flux cleaned = 0.00520511 Jy
! Component: 200  -  total flux cleaned = 0.00528046 Jy
! Total flux subtracted in 200 components = 0.00528046 Jy
! Clean residual min=-0.004312 max=0.003729 Jy/beam
! Clean residual mean=-0.000334 rms=0.000872 Jy/beam
! Combined flux in latest and established models = 0.985777 Jy
! Performing phase self-cal
! Adding 31 model components to the UV plane model.
! The established model now contains 77 components and 0.985777 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.163683Jy  sigma=0.001346
! Fit after  self-cal, rms=0.163671Jy  sigma=0.001346
! Inverting map 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 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=0.163671Jy  sigma=0.001346
! Fit after  self-cal, rms=0.163241Jy  sigma=0.001344
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
! Estimated beam: bmin=0.6045 mas, bmaj=1.728 mas, bpa=-6.32 degrees
! Estimated noise=512.513 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00187919 Jy
! Component: 100  -  total flux cleaned = -0.00152046 Jy
! Component: 150  -  total flux cleaned = -0.00130392 Jy
! Component: 200  -  total flux cleaned = -0.00104777 Jy
! Total flux subtracted in 200 components = -0.00104777 Jy
! Clean residual min=-0.003717 max=0.003621 Jy/beam
! Clean residual mean=-0.000189 rms=0.000828 Jy/beam
! Combined flux in latest and established models = 0.984729 Jy
selfcal
! Performing phase self-cal
! Adding 27 model components to the UV plane model.
! The established model now contains 82 components and 0.984729 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.163148Jy  sigma=0.001343
! Fit after  self-cal, rms=0.163138Jy  sigma=0.001343
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 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 = 0.000440396 Jy
! Component: 100  -  total flux cleaned = 0.000664385 Jy
! Component: 150  -  total flux cleaned = 0.000764865 Jy
! Component: 200  -  total flux cleaned = 0.000856193 Jy
! Total flux subtracted in 200 components = 0.000856193 Jy
! Clean residual min=-0.003652 max=0.003612 Jy/beam
! Clean residual mean=-0.000194 rms=0.000817 Jy/beam
! Combined flux in latest and established models = 0.985586 Jy
! Performing phase self-cal
! Adding 28 model components to the UV plane model.
! The established model now contains 86 components and 0.985586 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.163104Jy  sigma=0.001343
! Fit after  self-cal, rms=0.163102Jy  sigma=0.001343
! Inverting map 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 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=0.163102Jy  sigma=0.001343
! Fit after  self-cal, rms=0.162936Jy  sigma=0.001342
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
! Estimated beam: bmin=2.378 mas, bmaj=2.911 mas, bpa=0.5925 degrees
! Estimated noise=694.265 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000240797 Jy
! Component: 100  -  total flux cleaned = 3.22428e-05 Jy
! Component: 150  -  total flux cleaned = 3.05766e-05 Jy
! Component: 200  -  total flux cleaned = 3.03905e-05 Jy
! Total flux subtracted in 200 components = 3.03905e-05 Jy
! Clean residual min=-0.004050 max=0.006682 Jy/beam
! Clean residual mean=-0.000327 rms=0.001351 Jy/beam
! Combined flux in latest and established models = 0.985616 Jy
selfcal
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 94 components and 0.985616 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.162928Jy  sigma=0.001343
! Fit after  self-cal, rms=0.162917Jy  sigma=0.001342
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 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)
! Added new window around map position (7.8, 2.2).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00629804 Jy
! Component: 100  -  total flux cleaned = 0.009626 Jy
! Component: 150  -  total flux cleaned = 0.0110564 Jy
! Component: 200  -  total flux cleaned = 0.0115974 Jy
! Total flux subtracted in 200 components = 0.0115974 Jy
! Clean residual min=-0.003957 max=0.002369 Jy/beam
! Clean residual mean=-0.000529 rms=0.000914 Jy/beam
! Combined flux in latest and established models = 0.997213 Jy
! Performing phase self-cal
! Adding 35 model components to the UV plane model.
! The established model now contains 129 components and 0.997213 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.162818Jy  sigma=0.001341
! Fit after  self-cal, rms=0.162808Jy  sigma=0.001341
! Inverting map 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 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 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
! Estimated beam: bmin=0.6051 mas, bmaj=1.729 mas, bpa=-6.345 degrees
! Estimated noise=512.004 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6051 x 1.729 at -6.345 degrees (North through East)
! Clean map  min=-0.0025861  max=0.88609 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
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.162808Jy  sigma=0.001341
! Fit after  self-cal, rms=0.152558Jy  sigma=0.001224
! Inverting map and beam 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
! Estimated beam: bmin=0.6051 mas, bmaj=1.729 mas, bpa=-6.345 degrees
! Estimated noise=511.293 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000618464 Jy
! Component: 100  -  total flux cleaned = 0.000625449 Jy
! Component: 150  -  total flux cleaned = 0.000629498 Jy
! Component: 200  -  total flux cleaned = 0.000564191 Jy
! Total flux subtracted in 200 components = 0.000564191 Jy
! Clean residual min=-0.003059 max=0.002467 Jy/beam
! Clean residual mean=-0.000120 rms=0.000649 Jy/beam
! Combined flux in latest and established models = 0.997777 Jy
! Performing phase self-cal
! Adding 40 model components to the UV plane model.
! The established model now contains 161 components and 0.997777 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.152490Jy  sigma=0.001224
! Fit after  self-cal, rms=0.152488Jy  sigma=0.001224
! Inverting map 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000216885 Jy
! Component: 100  -  total flux cleaned = 0.000216818 Jy
! Component: 150  -  total flux cleaned = 0.00021507 Jy
! Component: 200  -  total flux cleaned = 0.000101842 Jy
! Total flux subtracted in 200 components = 0.000101842 Jy
! Clean residual min=-0.002953 max=0.002457 Jy/beam
! Clean residual mean=-0.000121 rms=0.000638 Jy/beam
! Combined flux in latest and established models = 0.997879 Jy
! Performing phase self-cal
! Adding 51 model components to the UV plane model.
! The established model now contains 179 components and 0.997879 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.152451Jy  sigma=0.001223
! Fit after  self-cal, rms=0.152450Jy  sigma=0.001223
! Inverting map 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.152450Jy  sigma=0.001223
! Fit after  self-cal, rms=0.152416Jy  sigma=0.001223
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 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
! Estimated beam: bmin=0.5393 mas, bmaj=1.579 mas, bpa=-5.628 degrees
! Estimated noise=768.975 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.685242 Jy
! Component: 100  -  total flux cleaned = 0.83654 Jy
! Component: 150  -  total flux cleaned = 0.889712 Jy
! Component: 200  -  total flux cleaned = 0.916512 Jy
! Total flux subtracted in 200 components = 0.916512 Jy
! Clean residual min=-0.005663 max=0.012779 Jy/beam
! Clean residual mean=0.000057 rms=0.001458 Jy/beam
! Combined flux in latest and established models = 0.916512 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 9 model components to the UV plane model.
! The established model now contains 9 components and 0.916512 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
! Estimated beam: bmin=0.6053 mas, bmaj=1.73 mas, bpa=-6.354 degrees
! Estimated noise=511.08 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 = 0.0231099 Jy
! Component: 100  -  total flux cleaned = 0.035775 Jy
! Component: 150  -  total flux cleaned = 0.0440405 Jy
! Component: 200  -  total flux cleaned = 0.0502708 Jy
! Total flux subtracted in 200 components = 0.0502708 Jy
! Clean residual min=-0.003674 max=0.003784 Jy/beam
! Clean residual mean=0.000089 rms=0.000967 Jy/beam
! Combined flux in latest and established models = 0.966783 Jy
! Adding 44 model components to the UV plane model.
! The established model now contains 48 components and 0.966783 Jy
! Inverting map 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 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 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
! Estimated beam: bmin=2.379 mas, bmaj=2.912 mas, bpa=0.4829 degrees
! Estimated noise=692.568 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0100578 Jy
! Component: 100  -  total flux cleaned = 0.0163235 Jy
! Component: 150  -  total flux cleaned = 0.0206755 Jy
! Component: 200  -  total flux cleaned = 0.0234566 Jy
! Total flux subtracted in 200 components = 0.0234566 Jy
! Clean residual min=-0.003579 max=0.003063 Jy/beam
! Clean residual mean=-0.000145 rms=0.001012 Jy/beam
! Combined flux in latest and established models = 0.990239 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 = 0.00179547 Jy
! Component: 100  -  total flux cleaned = 0.0031002 Jy
! Component: 150  -  total flux cleaned = 0.0041187 Jy
! Component: 200  -  total flux cleaned = 0.00498046 Jy
! Total flux subtracted in 200 components = 0.00498046 Jy
! Clean residual min=-0.003387 max=0.002732 Jy/beam
! Clean residual mean=-0.000228 rms=0.000857 Jy/beam
! Combined flux in latest and established models = 0.99522 Jy
! Adding 117 model components to the UV plane model.
! The established model now contains 153 components and 0.99522 Jy
! Inverting map 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
! Estimated beam: bmin=0.6053 mas, bmaj=1.73 mas, bpa=-6.354 degrees
! Estimated noise=511.08 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00069641 Jy
! Component: 100  -  total flux cleaned = 0.0010651 Jy
! Component: 150  -  total flux cleaned = 0.00140538 Jy
! Component: 200  -  total flux cleaned = 0.00172308 Jy
! Total flux subtracted in 200 components = 0.00172308 Jy
! Clean residual min=-0.002910 max=0.002416 Jy/beam
! Clean residual mean=-0.000095 rms=0.000638 Jy/beam
! Combined flux in latest and established models = 0.996943 Jy
selfcal
! Performing phase self-cal
! Adding 30 model components to the UV plane model.
! The established model now contains 183 components and 0.996943 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.152571Jy  sigma=0.001225
! Fit after  self-cal, rms=0.152541Jy  sigma=0.001224
wmodel J2147+0929_X_2009_04_21_pus_map.mod
! Writing 183 model components to file: J2147+0929_X_2009_04_21_pus_map.mod
wobs J2147+0929_X_2009_04_21_pus_uvs.fits
! Writing UV FITS file: J2147+0929_X_2009_04_21_pus_uvs.fits
wwins J2147+0929_X_2009_04_21_pus_map.win
! wwins: Wrote 4 windows to J2147+0929_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 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00112574 Jy
! Component: 100  -  total flux cleaned = -0.0019591 Jy
! Component: 150  -  total flux cleaned = -0.00262359 Jy
! Component: 200  -  total flux cleaned = -0.0033504 Jy
! Component: 250  -  total flux cleaned = -0.00368188 Jy
! Component: 300  -  total flux cleaned = -0.00412621 Jy
! Component: 350  -  total flux cleaned = -0.0045604 Jy
! Component: 400  -  total flux cleaned = -0.00486987 Jy
! Component: 450  -  total flux cleaned = -0.0052869 Jy
! Component: 500  -  total flux cleaned = -0.00558444 Jy
! Component: 550  -  total flux cleaned = -0.00580458 Jy
! Component: 600  -  total flux cleaned = -0.0060935 Jy
! Component: 650  -  total flux cleaned = -0.00634229 Jy
! Component: 700  -  total flux cleaned = -0.0065528 Jy
! Component: 750  -  total flux cleaned = -0.00682922 Jy
! Component: 800  -  total flux cleaned = -0.00693106 Jy
! Component: 850  -  total flux cleaned = -0.00709959 Jy
! Component: 900  -  total flux cleaned = -0.00726623 Jy
! Component: 950  -  total flux cleaned = -0.00736515 Jy
! Component: 1000  -  total flux cleaned = -0.00749592 Jy
! Component: 1050  -  total flux cleaned = -0.00769006 Jy
! Component: 1100  -  total flux cleaned = -0.00775436 Jy
! Component: 1150  -  total flux cleaned = -0.00794491 Jy
! Component: 1200  -  total flux cleaned = -0.00800767 Jy
! Component: 1250  -  total flux cleaned = -0.00803909 Jy
! Component: 1300  -  total flux cleaned = -0.00825585 Jy
! Component: 1350  -  total flux cleaned = -0.00831719 Jy
! Component: 1400  -  total flux cleaned = -0.00840821 Jy
! Component: 1450  -  total flux cleaned = -0.00849865 Jy
! Component: 1500  -  total flux cleaned = -0.00858833 Jy
! Component: 1550  -  total flux cleaned = -0.0086777 Jy
! Component: 1600  -  total flux cleaned = -0.0087366 Jy
! Component: 1650  -  total flux cleaned = -0.00885373 Jy
! Component: 1700  -  total flux cleaned = -0.00894098 Jy
! Component: 1750  -  total flux cleaned = -0.00899862 Jy
! Component: 1800  -  total flux cleaned = -0.00911346 Jy
! Component: 1850  -  total flux cleaned = -0.00914197 Jy
! Component: 1900  -  total flux cleaned = -0.00917031 Jy
! Component: 1950  -  total flux cleaned = -0.00925457 Jy
! Component: 2000  -  total flux cleaned = -0.00931062 Jy
! Total flux subtracted in 2048 components = -0.00936632 Jy
! Clean residual min=-0.001588 max=0.001385 Jy/beam
! Clean residual mean=-0.000033 rms=0.000506 Jy/beam
! Combined flux in latest and established models = 0.987577 Jy
keep
! Adding 154 model components to the UV plane model.
! The established model now contains 337 components and 0.987577 Jy
![Exited script file: muppet]
wmap "J2147+0929_X_2009_04_21_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6053 x 1.73 at -6.354 degrees (North through East)
! Clean map  min=-0.0022209  max=0.88577 Jy/beam
! Writing clean map to FITS file: J2147+0929_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 0.885765 
invert
! Inverting map 
! Your choice of large map pixels excluded 4.34% of the data.
!  The x-axis pixel size should ideally be below 0.1564 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000506489 
device "J2147+0929_X_2009_04_21_pus\_map.eps/VPS"
! Attempting to open device: 'J2147+0929_X_2009_04_21_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.171543 0.171543 0.343086 0.686172 1.37234 2.74469 5.48937 10.9787 21.9575 43.915 87.83
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0015 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.885 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6053 x 1.73 at -6.354 degrees (North through East)
! Clean map  min=-0.0022209  max=0.88577 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J2147+0929_X_2009_04_21_pus\_map.gif/vgif"
! Attempting to open device: 'J2147+0929_X_2009_04_21_pus_map.gif/vgif'
mapplot cln