! Started logfile: J0102+5824_X_2009_04_21_pus_uvs.log on Sun Jan 23 18:04:45 2011
obs J0102+5824_X_2009_04_21_pus_uva.fits
! Reading UV FITS file: J0102+5824_X_2009_04_21_pus_uva.fits
! AN table 1: 74 integrations on 120 of 120 possible baselines.
! AN table 2: 292 integrations on 120 of 120 possible baselines.
! AN table 3: 36 integrations on 120 of 120 possible baselines.
! Apparent sampling: 0.127177 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J0102+5824
! 
! 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 2449 lines of history.
! 
! Reading 24540 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 J0102+5824_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 = 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 714 telescope corrections were flagged in sub-array 1.
!  A total of 3662 telescope corrections were flagged in sub-array 2.
!  A total of 382 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 711 telescope corrections were flagged in sub-array 1.
!  A total of 3662 telescope corrections were flagged in sub-array 2.
!  A total of 382 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 714 telescope corrections were flagged in sub-array 1.
!  A total of 3662 telescope corrections were flagged in sub-array 2.
!  A total of 382 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 711 telescope corrections were flagged in sub-array 1.
!  A total of 3662 telescope corrections were flagged in sub-array 2.
!  A total of 382 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=1.168897Jy  sigma=0.010079
! Fit after  self-cal, rms=0.807736Jy  sigma=0.007151
! 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 7.3% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! Estimated beam: bmin=0.5073 mas, bmaj=0.629 mas, bpa=38.65 degrees
! Estimated noise=938.368 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 = 1.34748 Jy
! Component: 100  -  total flux cleaned = 1.64132 Jy
! Total flux subtracted in 100 components = 1.64132 Jy
! Clean residual min=-0.023234 max=0.082002 Jy/beam
! Clean residual mean=0.001172 rms=0.008125 Jy/beam
! Combined flux in latest and established models = 1.64132 Jy
! Performing phase self-cal
! Adding 1 model components to the UV plane model.
! The established model now contains 1 components and 1.64132 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.304607Jy  sigma=0.002683
! Fit after  self-cal, rms=0.304606Jy  sigma=0.002683
! Inverting map 
! Your choice of large map pixels excluded 7.3% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0914847 Jy
! Component: 100  -  total flux cleaned = 0.145966 Jy
! Total flux subtracted in 100 components = 0.145966 Jy
! Clean residual min=-0.021705 max=0.052343 Jy/beam
! Clean residual mean=0.000836 rms=0.006648 Jy/beam
! Combined flux in latest and established models = 1.78729 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 9 components and 1.78729 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.265036Jy  sigma=0.002230
! Fit after  self-cal, rms=0.264967Jy  sigma=0.002229
! Inverting map 
! Your choice of large map pixels excluded 7.3% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! Added new window around map position (-0.6, -0.8).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0495293 Jy
! Component: 100  -  total flux cleaned = 0.0810423 Jy
! Total flux subtracted in 100 components = 0.0810423 Jy
! Clean residual min=-0.022866 max=0.037132 Jy/beam
! Clean residual mean=0.000654 rms=0.006105 Jy/beam
! Combined flux in latest and established models = 1.86833 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 16 components and 1.86833 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.252192Jy  sigma=0.002070
! Fit after  self-cal, rms=0.251560Jy  sigma=0.002065
! Inverting map 
! Your choice of large map pixels excluded 7.3% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! Added new window around map position (-1.4, -0.4).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0377829 Jy
! Component: 100  -  total flux cleaned = 0.0630616 Jy
! Total flux subtracted in 100 components = 0.0630616 Jy
! Clean residual min=-0.022156 max=0.031187 Jy/beam
! Clean residual mean=0.000518 rms=0.005734 Jy/beam
! Combined flux in latest and established models = 1.93139 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 20 components and 1.93139 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.243899Jy  sigma=0.001976
! Fit after  self-cal, rms=0.243386Jy  sigma=0.001971
! Inverting map 
! Your choice of large map pixels excluded 7.3% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 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 7.3% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! Estimated beam: bmin=0.5874 mas, bmaj=0.7228 mas, bpa=27.92 degrees
! Estimated noise=572.819 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 (0.2, -1.2).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.045588 Jy
! Component: 100  -  total flux cleaned = 0.073929 Jy
! Component: 150  -  total flux cleaned = 0.0939827 Jy
! Component: 200  -  total flux cleaned = 0.108593 Jy
! Total flux subtracted in 200 components = 0.108593 Jy
! Clean residual min=-0.022929 max=0.028948 Jy/beam
! Clean residual mean=0.002352 rms=0.005614 Jy/beam
! Combined flux in latest and established models = 2.03998 Jy
! Performing phase self-cal
! Adding 25 model components to the UV plane model.
! The established model now contains 38 components and 2.03998 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.236765Jy  sigma=0.001862
! Fit after  self-cal, rms=0.236162Jy  sigma=0.001856
! Inverting map 
! Your choice of large map pixels excluded 7.3% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 54 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.94     FD        0.94     HN        1.24     KB        1.00*    
!   KK        1.04     KP        0.96     LA        0.94     MK        1.00     
!   NL        0.95     NY        0.96     OV        0.99     PT        0.97     
!   SC        0.97     TS        1.10     WZ        1.08     ZC        1.11     
! 
!  A total of 186 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.95     FD        1.01     HN        1.02     KB        0.98     
!   KK        1.02     KP        1.01     LA        1.03     MK        0.95     
!   NL        0.98     NY        0.99     OV        1.01     PT        1.03     
!   SC        1.08     TS        0.98     WZ        1.07     ZC        1.05     
! 
!  A total of 24 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.03     FD        1.00*    HN        1.00     KB        0.94     
!   KK        1.00*    KP        1.00*    LA        1.08     MK        1.00*    
!   NL        1.00     NY        0.96     OV        1.07     PT        1.10     
!   SC        1.00*    TS        0.93     WZ        1.08     ZC        1.04     
! 
! 
! Correcting IF 2.
!  A total of 57 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.94     FD        0.94     HN        1.36     KB        1.00*    
!   KK        1.00     KP        0.95     LA        0.94     MK        1.00     
!   NL        0.93     NY        1.00     OV        0.97     PT        0.96     
!   SC        0.98     TS        1.10     WZ        1.02     ZC        1.10     
! 
!  A total of 186 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.95     FD        1.01     HN        1.02     KB        0.98     
!   KK        1.00     KP        1.00     LA        1.02     MK        0.95     
!   NL        0.97     NY        1.02     OV        0.99     PT        1.01     
!   SC        1.09     TS        0.98     WZ        1.02     ZC        1.04     
! 
!  A total of 24 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.99     FD        1.00*    HN        1.01     KB        0.94     
!   KK        1.00*    KP        1.00*    LA        1.08     MK        1.00*    
!   NL        0.99     NY        1.00     OV        1.04     PT        1.07     
!   SC        1.00*    TS        0.93     WZ        0.99     ZC        1.04     
! 
! 
! Correcting IF 3.
!  A total of 54 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.96     FD        0.94     HN        1.38     KB        1.00*    
!   KK        1.02     KP        0.95     LA        0.92     MK        1.01     
!   NL        0.95     NY        0.99     OV        0.99     PT        0.95     
!   SC        0.99     TS        1.09     WZ        0.98     ZC        1.10     
! 
!  A total of 186 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.97     FD        1.01     HN        1.02     KB        0.96     
!   KK        1.02     KP        1.01     LA        1.00     MK        0.94     
!   NL        0.98     NY        1.02     OV        1.01     PT        1.00     
!   SC        1.11     TS        0.97     WZ        0.98     ZC        1.03     
! 
!  A total of 24 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.01     FD        1.00*    HN        1.01     KB        0.92     
!   KK        1.00*    KP        1.00*    LA        1.06     MK        1.00*    
!   NL        1.03     NY        0.99     OV        1.07     PT        1.05     
!   SC        1.00*    TS        0.92     WZ        0.97     ZC        1.05     
! 
! 
! Correcting IF 4.
!  A total of 57 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.93     FD        0.95     HN        1.37     KB        1.00*    
!   KK        1.01     KP        0.94     LA        0.91     MK        1.02     
!   NL        0.95     NY        0.96     OV        0.98     PT        0.92     
!   SC        1.00     TS        1.09     WZ        1.01     ZC        1.11     
! 
!  A total of 186 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.94     FD        1.02     HN        1.02     KB        0.96     
!   KK        0.99     KP        0.99     LA        1.00     MK        0.97     
!   NL        0.99     NY        0.98     OV        1.00     PT        0.99     
!   SC        1.10     TS        0.97     WZ        1.00     ZC        1.03     
! 
!  A total of 24 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.98     FD        1.00*    HN        0.99     KB        0.92     
!   KK        1.00*    KP        1.00*    LA        1.04     MK        1.00*    
!   NL        1.02     NY        0.96     OV        1.04     PT        1.02     
!   SC        1.00*    TS        0.91     WZ        0.99     ZC        1.01     
! 
! 
! Fit before self-cal, rms=0.236162Jy  sigma=0.001856
! Fit after  self-cal, rms=0.199583Jy  sigma=0.001535
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! Estimated beam: bmin=0.5861 mas, bmaj=0.7316 mas, bpa=26.93 degrees
! Estimated noise=578.952 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 = -0.0162561 Jy
! Component: 100  -  total flux cleaned = -0.0213815 Jy
! Component: 150  -  total flux cleaned = -0.0226114 Jy
! Component: 200  -  total flux cleaned = -0.0236644 Jy
! Total flux subtracted in 200 components = -0.0236644 Jy
! Clean residual min=-0.013998 max=0.014285 Jy/beam
! Clean residual mean=0.000258 rms=0.003878 Jy/beam
! Combined flux in latest and established models = 2.01632 Jy
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 47 components and 2.01632 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.197945Jy  sigma=0.001521
! Fit after  self-cal, rms=0.197949Jy  sigma=0.001520
! Inverting map 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 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=0.197949Jy  sigma=0.001520
! Fit after  self-cal, rms=0.179844Jy  sigma=0.001253
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! Estimated beam: bmin=0.5878 mas, bmaj=0.7308 mas, bpa=26.66 degrees
! Estimated noise=578.8 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.0114873 Jy
! Component: 100  -  total flux cleaned = -0.0142838 Jy
! Component: 150  -  total flux cleaned = -0.0158283 Jy
! Component: 200  -  total flux cleaned = -0.0162634 Jy
! Total flux subtracted in 200 components = -0.0162634 Jy
! Clean residual min=-0.005020 max=0.008986 Jy/beam
! Clean residual mean=0.000407 rms=0.001338 Jy/beam
! Combined flux in latest and established models = 2.00006 Jy
selfcal
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 56 components and 2.00006 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.178596Jy  sigma=0.001244
! Fit after  self-cal, rms=0.178535Jy  sigma=0.001243
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 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 (-2.2, -0.4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00512779 Jy
! Component: 100  -  total flux cleaned = 0.00586194 Jy
! Component: 150  -  total flux cleaned = 0.00648717 Jy
! Component: 200  -  total flux cleaned = 0.0068499 Jy
! Total flux subtracted in 200 components = 0.0068499 Jy
! Clean residual min=-0.004639 max=0.004474 Jy/beam
! Clean residual mean=0.000201 rms=0.001190 Jy/beam
! Combined flux in latest and established models = 2.00691 Jy
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 63 components and 2.00691 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.177900Jy  sigma=0.001237
! Fit after  self-cal, rms=0.177858Jy  sigma=0.001237
! Inverting map 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 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=0.177858Jy  sigma=0.001237
! Fit after  self-cal, rms=0.177588Jy  sigma=0.001233
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! Estimated beam: bmin=0.5881 mas, bmaj=0.7312 mas, bpa=26.5 degrees
! Estimated noise=578.359 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00494323 Jy
! Component: 100  -  total flux cleaned = -0.00575312 Jy
! Component: 150  -  total flux cleaned = -0.00592914 Jy
! Component: 200  -  total flux cleaned = -0.00592772 Jy
! Total flux subtracted in 200 components = -0.00592772 Jy
! Clean residual min=-0.004319 max=0.003605 Jy/beam
! Clean residual mean=0.000249 rms=0.001044 Jy/beam
! Combined flux in latest and established models = 2.00098 Jy
selfcal
! Performing phase self-cal
! Adding 26 model components to the UV plane model.
! The established model now contains 67 components and 2.00098 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.177172Jy  sigma=0.001229
! Fit after  self-cal, rms=0.177158Jy  sigma=0.001229
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 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 = -0.000350348 Jy
! Component: 100  -  total flux cleaned = -0.000347039 Jy
! Component: 150  -  total flux cleaned = -9.24982e-05 Jy
! Component: 200  -  total flux cleaned = 2.02574e-05 Jy
! Total flux subtracted in 200 components = 2.02574e-05 Jy
! Clean residual min=-0.004185 max=0.003466 Jy/beam
! Clean residual mean=0.000249 rms=0.001008 Jy/beam
! Combined flux in latest and established models = 2.001 Jy
! Performing phase self-cal
! Adding 28 model components to the UV plane model.
! The established model now contains 71 components and 2.001 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.176975Jy  sigma=0.001227
! Fit after  self-cal, rms=0.176964Jy  sigma=0.001227
! Inverting map 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 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=0.176964Jy  sigma=0.001227
! Fit after  self-cal, rms=0.176904Jy  sigma=0.001227
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! Estimated beam: bmin=2.393 mas, bmaj=3.034 mas, bpa=-39.42 degrees
! Estimated noise=930.221 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00100488 Jy
! Component: 100  -  total flux cleaned = -0.0012265 Jy
! Component: 150  -  total flux cleaned = -0.00140111 Jy
! Component: 200  -  total flux cleaned = -0.00149808 Jy
! Total flux subtracted in 200 components = -0.00149808 Jy
! Clean residual min=-0.004408 max=0.004536 Jy/beam
! Clean residual mean=0.000575 rms=0.001465 Jy/beam
! Combined flux in latest and established models = 1.9995 Jy
selfcal
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 81 components and 1.9995 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.176943Jy  sigma=0.001227
! Fit after  self-cal, rms=0.176930Jy  sigma=0.001227
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 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 = 0.000157822 Jy
! Component: 100  -  total flux cleaned = 0.000157732 Jy
! Component: 150  -  total flux cleaned = 0.000192796 Jy
! Component: 200  -  total flux cleaned = 0.000193334 Jy
! Total flux subtracted in 200 components = 0.000193334 Jy
! Clean residual min=-0.004436 max=0.004546 Jy/beam
! Clean residual mean=0.000553 rms=0.001455 Jy/beam
! Combined flux in latest and established models = 1.99969 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 85 components and 1.99969 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.176947Jy  sigma=0.001227
! Fit after  self-cal, rms=0.176947Jy  sigma=0.001227
! Inverting map 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 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 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! Estimated beam: bmin=0.5882 mas, bmaj=0.7316 mas, bpa=26.36 degrees
! Estimated noise=578.061 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5882 x 0.7316 at 26.36 degrees (North through East)
! Clean map  min=-0.0052492  max=1.7473 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=0.176947Jy  sigma=0.001227
! Fit after  self-cal, rms=0.166610Jy  sigma=0.001122
! Inverting map and beam 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! Estimated beam: bmin=0.5883 mas, bmaj=0.7318 mas, bpa=26.41 degrees
! Estimated noise=577.344 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00315332 Jy
! Component: 100  -  total flux cleaned = -0.00412376 Jy
! Component: 150  -  total flux cleaned = -0.00460396 Jy
! Component: 200  -  total flux cleaned = -0.0046031 Jy
! Total flux subtracted in 200 components = -0.0046031 Jy
! Clean residual min=-0.003380 max=0.003077 Jy/beam
! Clean residual mean=0.000260 rms=0.000856 Jy/beam
! Combined flux in latest and established models = 1.99509 Jy
! Performing phase self-cal
! Adding 23 model components to the UV plane model.
! The established model now contains 87 components and 1.99509 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.166410Jy  sigma=0.001120
! Fit after  self-cal, rms=0.166398Jy  sigma=0.001120
! Inverting map 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000222994 Jy
! Component: 100  -  total flux cleaned = -0.000316526 Jy
! Component: 150  -  total flux cleaned = -0.000316671 Jy
! Component: 200  -  total flux cleaned = -0.000315139 Jy
! Total flux subtracted in 200 components = -0.000315139 Jy
! Clean residual min=-0.003287 max=0.002984 Jy/beam
! Clean residual mean=0.000269 rms=0.000836 Jy/beam
! Combined flux in latest and established models = 1.99478 Jy
! Performing phase self-cal
! Adding 23 model components to the UV plane model.
! The established model now contains 90 components and 1.99477 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.166300Jy  sigma=0.001119
! Fit after  self-cal, rms=0.166292Jy  sigma=0.001119
! Inverting map 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.166292Jy  sigma=0.001119
! Fit after  self-cal, rms=0.166257Jy  sigma=0.001119
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 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! Estimated beam: bmin=0.5097 mas, bmaj=0.6309 mas, bpa=36.64 degrees
! Estimated noise=952.215 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 1.35448 Jy
! Component: 100  -  total flux cleaned = 1.64985 Jy
! Component: 150  -  total flux cleaned = 1.73054 Jy
! Component: 200  -  total flux cleaned = 1.779 Jy
! Total flux subtracted in 200 components = 1.779 Jy
! Clean residual min=-0.007242 max=0.026248 Jy/beam
! Clean residual mean=0.000538 rms=0.002816 Jy/beam
! Combined flux in latest and established models = 1.779 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 13 model components to the UV plane model.
! The established model now contains 13 components and 1.779 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! Estimated beam: bmin=0.5883 mas, bmaj=0.7321 mas, bpa=26.28 degrees
! Estimated noise=577.126 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 = 0.0647958 Jy
! Component: 100  -  total flux cleaned = 0.106357 Jy
! Component: 150  -  total flux cleaned = 0.134923 Jy
! Component: 200  -  total flux cleaned = 0.155181 Jy
! Total flux subtracted in 200 components = 0.155181 Jy
! Clean residual min=-0.001871 max=0.011379 Jy/beam
! Clean residual mean=0.001987 rms=0.001565 Jy/beam
! Combined flux in latest and established models = 1.93418 Jy
! Adding 48 model components to the UV plane model.
! The established model now contains 49 components and 1.93418 Jy
! Inverting map 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! Added new window around map position (-0.6, 0).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0146619 Jy
! Component: 100  -  total flux cleaned = 0.0253808 Jy
! Component: 150  -  total flux cleaned = 0.0333488 Jy
! Component: 200  -  total flux cleaned = 0.0393846 Jy
! Total flux subtracted in 200 components = 0.0393846 Jy
! Clean residual min=-0.002144 max=0.004052 Jy/beam
! Clean residual mean=0.000791 rms=0.000863 Jy/beam
! Combined flux in latest and established models = 1.97356 Jy
! Adding 46 model components to the UV plane model.
! The established model now contains 78 components and 1.97356 Jy
! Inverting map 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! Added new window around map position (1.2, -0.8).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00479315 Jy
! Component: 100  -  total flux cleaned = 0.00853727 Jy
! Component: 150  -  total flux cleaned = 0.0115191 Jy
! Component: 200  -  total flux cleaned = 0.0139039 Jy
! Total flux subtracted in 200 components = 0.0139039 Jy
! Clean residual min=-0.002476 max=0.003124 Jy/beam
! Clean residual mean=0.000369 rms=0.000770 Jy/beam
! Combined flux in latest and established models = 1.98747 Jy
! Adding 51 model components to the UV plane model.
! The established model now contains 103 components and 1.98747 Jy
! Inverting map 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 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 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! Estimated beam: bmin=2.393 mas, bmaj=3.037 mas, bpa=-39.45 degrees
! Estimated noise=927.497 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00454402 Jy
! Component: 100  -  total flux cleaned = 0.00504672 Jy
! Component: 150  -  total flux cleaned = 0.00527639 Jy
! Component: 200  -  total flux cleaned = 0.00551479 Jy
! Total flux subtracted in 200 components = 0.00551479 Jy
! Clean residual min=-0.003760 max=0.004696 Jy/beam
! Clean residual mean=0.000764 rms=0.001282 Jy/beam
! Combined flux in latest and established models = 1.99298 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 = 4.82175e-05 Jy
! Component: 100  -  total flux cleaned = 4.97307e-05 Jy
! Component: 150  -  total flux cleaned = 8.8379e-05 Jy
! Component: 200  -  total flux cleaned = 8.98517e-05 Jy
! Total flux subtracted in 200 components = 8.98517e-05 Jy
! Clean residual min=-0.003749 max=0.004734 Jy/beam
! Clean residual mean=0.000756 rms=0.001269 Jy/beam
! Combined flux in latest and established models = 1.99307 Jy
! Adding 27 model components to the UV plane model.
! The established model now contains 114 components and 1.99307 Jy
! Inverting map 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! Estimated beam: bmin=0.5883 mas, bmaj=0.7321 mas, bpa=26.28 degrees
! Estimated noise=577.126 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000547564 Jy
! Component: 100  -  total flux cleaned = -0.000548473 Jy
! Component: 150  -  total flux cleaned = -0.000549448 Jy
! Component: 200  -  total flux cleaned = -0.000441881 Jy
! Total flux subtracted in 200 components = -0.000441881 Jy
! Clean residual min=-0.002686 max=0.003120 Jy/beam
! Clean residual mean=0.000215 rms=0.000757 Jy/beam
! Combined flux in latest and established models = 1.99263 Jy
selfcal
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 122 components and 1.99263 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.166108Jy  sigma=0.001119
! Fit after  self-cal, rms=0.166000Jy  sigma=0.001118
wmodel J0102+5824_X_2009_04_21_pus_map.mod
! Writing 122 model components to file: J0102+5824_X_2009_04_21_pus_map.mod
wobs J0102+5824_X_2009_04_21_pus_uvs.fits
! Writing UV FITS file: J0102+5824_X_2009_04_21_pus_uvs.fits
wwins J0102+5824_X_2009_04_21_pus_map.win
! wwins: Wrote 7 windows to J0102+5824_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 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.00120508 Jy
! Component: 100  -  total flux cleaned = 0.00170091 Jy
! Component: 150  -  total flux cleaned = 0.0018891 Jy
! Component: 200  -  total flux cleaned = 0.00202571 Jy
! Component: 250  -  total flux cleaned = 0.00229059 Jy
! Component: 300  -  total flux cleaned = 0.0024617 Jy
! Component: 350  -  total flux cleaned = 0.00262926 Jy
! Component: 400  -  total flux cleaned = 0.00283394 Jy
! Component: 450  -  total flux cleaned = 0.00299473 Jy
! Component: 500  -  total flux cleaned = 0.00323174 Jy
! Component: 550  -  total flux cleaned = 0.0033869 Jy
! Component: 600  -  total flux cleaned = 0.00361603 Jy
! Component: 650  -  total flux cleaned = 0.00376661 Jy
! Component: 700  -  total flux cleaned = 0.00398914 Jy
! Component: 750  -  total flux cleaned = 0.00417188 Jy
! Component: 800  -  total flux cleaned = 0.00438788 Jy
! Component: 850  -  total flux cleaned = 0.00456528 Jy
! Component: 900  -  total flux cleaned = 0.00470546 Jy
! Component: 950  -  total flux cleaned = 0.00484392 Jy
! Component: 1000  -  total flux cleaned = 0.00498088 Jy
! Total flux subtracted in 1024 components = 0.0050826 Jy
! Clean residual min=-0.002301 max=0.002037 Jy/beam
! Clean residual mean=0.000079 rms=0.000637 Jy/beam
! Combined flux in latest and established models = 1.99771 Jy
keep
! Adding 81 model components to the UV plane model.
! The established model now contains 203 components and 1.99771 Jy
![Exited script file: muppet]
wmap "J0102+5824_X_2009_04_21_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5883 x 0.7321 at 26.28 degrees (North through East)
! Clean map  min=-0.0025015  max=1.7501 Jy/beam
! Writing clean map to FITS file: J0102+5824_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 1.75014 
invert
! Inverting map 
! Your choice of large map pixels excluded 7.04% of the data.
!  The x-axis pixel size should ideally be below 0.1542 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1707 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000637649 
device "J0102+5824_X_2009_04_21_pus\_map.eps/VPS"
! Attempting to open device: 'J0102+5824_X_2009_04_21_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.109302 0.109302 0.218604 0.437209 0.874418 1.74884 3.49767 6.99534 13.9907 27.9814 55.9627
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0019 
print "peak=",int(1000*peak_flux)/1000
! peak= 1.75 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5883 x 0.7321 at 26.28 degrees (North through East)
! Clean map  min=-0.0025015  max=1.7501 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0102+5824_X_2009_04_21_pus\_map.gif/vgif"
! Attempting to open device: 'J0102+5824_X_2009_04_21_pus_map.gif/vgif'
mapplot cln