! Started logfile: /scr/pima/rdv72_uvs/J1354-0206_X_uvs.log on Sat Oct  5 08:47:56 2013
obs /scr/pima/rdv72_uvs/J1354-0206_X_uva.fits
! Reading UV FITS file: /scr/pima/rdv72_uvs/J1354-0206_X_uva.fits
! AN table 1: 3 integrations on 10 of 10 possible baselines.
! AN table 2: 2 integrations on 1 of 1 possible baselines.
! AN table 3: 6 integrations on 1 of 1 possible baselines.
! AN table 4: 12 integrations on 1 of 1 possible baselines.
! AN table 5: 3 integrations on 10 of 10 possible baselines.
! AN table 6: 15 integrations on 36 of 36 possible baselines.
! AN table 7: 4 integrations on 28 of 28 possible baselines.
! AN table 8: 6 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.701597 visibilities/baseline/integration-bin.
! Found source: J1354-0206
! 
! 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  8.40599e+09      1.6e+07          1      1.6e+07
!  02        2  8.47599e+09      1.6e+07          1      1.6e+07
!  03        3  8.79099e+09      1.6e+07          1      1.6e+07
!  04        4  8.89599e+09      1.6e+07          1      1.6e+07
! 
! Polarization(s): RR
! 
! Read 0 lines of history.
! 
! Reading 2812 visibilities.
select RR
! 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 = 1024 
print "field_cell =",field_cell
! field_cell = 0.2 
print "taper_size =",taper_size
! taper_size = 70 
![@/home/lpetrov/bin/01_muppet /scr/pima/rdv72_uvs/J1354-0206_X]
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 = 1024x1024 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 2 telescope corrections were flagged in sub-array 1.
!  A total of 4 telescope corrections were flagged in sub-array 2.
!  A total of 12 telescope corrections were flagged in sub-array 3.
!  A total of 24 telescope corrections were flagged in sub-array 4.
!  A total of 21 telescope corrections were flagged in sub-array 6.
!  A total of 4 telescope corrections were flagged in sub-array 7.
!  A total of 14 telescope corrections were flagged in sub-array 8.
! 
! Correcting IF 2.
!  A total of 2 telescope corrections were flagged in sub-array 1.
!  A total of 4 telescope corrections were flagged in sub-array 2.
!  A total of 12 telescope corrections were flagged in sub-array 3.
!  A total of 24 telescope corrections were flagged in sub-array 4.
!  A total of 21 telescope corrections were flagged in sub-array 6.
!  A total of 4 telescope corrections were flagged in sub-array 7.
!  A total of 14 telescope corrections were flagged in sub-array 8.
! 
! Correcting IF 3.
!  A total of 2 telescope corrections were flagged in sub-array 1.
!  A total of 4 telescope corrections were flagged in sub-array 2.
!  A total of 12 telescope corrections were flagged in sub-array 3.
!  A total of 24 telescope corrections were flagged in sub-array 4.
!  A total of 21 telescope corrections were flagged in sub-array 6.
!  A total of 4 telescope corrections were flagged in sub-array 7.
!  A total of 14 telescope corrections were flagged in sub-array 8.
! 
! Correcting IF 4.
!  A total of 2 telescope corrections were flagged in sub-array 1.
!  A total of 4 telescope corrections were flagged in sub-array 2.
!  A total of 12 telescope corrections were flagged in sub-array 3.
!  A total of 24 telescope corrections were flagged in sub-array 4.
!  A total of 21 telescope corrections were flagged in sub-array 6.
!  A total of 4 telescope corrections were flagged in sub-array 7.
!  A total of 14 telescope corrections were flagged in sub-array 8.
! 
! Fit before self-cal, rms=1.158817Jy  sigma=8.113645
! Fit after  self-cal, rms=0.501227Jy  sigma=2.549224
! 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 0.222% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.7733 mas, bmaj=1.853 mas, bpa=2.945 degrees
! Estimated noise=3.06543 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 = 0.460003 Jy
! Component: 100  -  total flux cleaned = 0.591953 Jy
! Total flux subtracted in 100 components = 0.591953 Jy
! Clean residual min=-0.031195 max=0.056737 Jy/beam
! Clean residual mean=0.000159 rms=0.008024 Jy/beam
! Combined flux in latest and established models = 0.591953 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 9 components and 0.591953 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.231429Jy  sigma=1.548499
! Fit after  self-cal, rms=0.231383Jy  sigma=1.548242
! Inverting map 
! Your choice of large map pixels excluded 0.222% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Added new window around map position (1, 2.2).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0599406 Jy
! Component: 100  -  total flux cleaned = 0.0939833 Jy
! Total flux subtracted in 100 components = 0.0939833 Jy
! Clean residual min=-0.030372 max=0.032524 Jy/beam
! Clean residual mean=0.000117 rms=0.006516 Jy/beam
! Combined flux in latest and established models = 0.685936 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 23 components and 0.685936 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.223222Jy  sigma=1.298976
! Fit after  self-cal, rms=0.223086Jy  sigma=1.296205
! Inverting map 
! Your choice of large map pixels excluded 0.222% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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 0.222% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.9187 mas, bmaj=2.231 mas, bpa=2.536 degrees
! Estimated noise=2.21574 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 = 0.040998 Jy
! Component: 100  -  total flux cleaned = 0.0614857 Jy
! Component: 150  -  total flux cleaned = 0.0728903 Jy
! Component: 200  -  total flux cleaned = 0.0754139 Jy
! Total flux subtracted in 200 components = 0.0754139 Jy
! Clean residual min=-0.033641 max=0.039096 Jy/beam
! Clean residual mean=0.000239 rms=0.008112 Jy/beam
! Combined flux in latest and established models = 0.76135 Jy
! Performing phase self-cal
! Adding 28 model components to the UV plane model.
! The established model now contains 39 components and 0.76135 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.228306Jy  sigma=1.176938
! Fit after  self-cal, rms=0.228335Jy  sigma=1.176414
! Inverting map 
! Your choice of large map pixels excluded 0.222% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.34     KK        1.33     KP        0.97     MK        0.88     
!   OV        1.09     
! 
!  Telescope amplitude corrections in sub-array 2:
!   KK        0.00*    MK        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   WZ        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   NY        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   FD        0.77     KP        1.86     LA        0.93     NL        0.98     
!   PT        0.96     
! 
!  Telescope amplitude corrections in sub-array 6:
!   BR        1.24     FD        0.78     KP        1.54     LA        0.96     
!   NL        1.04     OV        1.03     PT        0.91     SC        0.94     
!   WZ        1.06     
! 
!  Telescope amplitude corrections in sub-array 7:
!   BR        1.28     FD        0.84     KP        1.78     LA        1.01     
!   NL        0.97     OV        1.03     PT        0.89     SC        1.02     
! 
!  Telescope amplitude corrections in sub-array 8:
!   BR        1.47     FD        0.82     KK        1.28     KP        1.79     
!   LA        0.97     MK        0.85     NL        0.96     OV        1.00     
!   PT        0.89     SC        0.99     
! 
! 
! Correcting IF 2.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.27     KK        1.31     KP        0.95     MK        0.88     
!   OV        1.05     
! 
!  Telescope amplitude corrections in sub-array 2:
!   KK        0.00*    MK        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   WZ        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   NY        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   FD        0.79     KP        1.70     LA        0.98     NL        0.95     
!   PT        1.05     
! 
!  Telescope amplitude corrections in sub-array 6:
!   BR        1.27     FD        0.78     KP        1.38     LA        0.93     
!   NL        1.04     OV        1.04     PT        0.96     SC        0.98     
!   WZ        1.04     
! 
!  Telescope amplitude corrections in sub-array 7:
!   BR        1.26     FD        0.84     KP        1.43     LA        0.99     
!   NL        0.97     OV        1.00     PT        0.93     SC        1.05     
! 
!  Telescope amplitude corrections in sub-array 8:
!   BR        1.46     FD        0.84     KK        1.24     KP        1.95     
!   LA        0.92     MK        0.94     NL        0.98     OV        0.98     
!   PT        0.95     SC        0.97     
! 
! 
! Correcting IF 3.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.53     KK        1.30     KP        0.89     MK        0.87     
!   OV        1.19     
! 
!  Telescope amplitude corrections in sub-array 2:
!   KK        0.00*    MK        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   WZ        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   NY        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   FD        0.83     KP        1.79     LA        1.05     NL        1.07     
!   PT        0.99     
! 
!  Telescope amplitude corrections in sub-array 6:
!   BR        1.40     FD        0.79     KP        1.40     LA        0.97     
!   NL        1.05     OV        1.07     PT        0.97     SC        1.02     
!   WZ        1.16     
! 
!  Telescope amplitude corrections in sub-array 7:
!   BR        1.31     FD        0.84     KP        1.63     LA        1.00     
!   NL        1.02     OV        1.06     PT        0.97     SC        1.12     
! 
!  Telescope amplitude corrections in sub-array 8:
!   BR        1.55     FD        0.86     KK        1.36     KP        1.84     
!   LA        1.01     MK        0.90     NL        1.00     OV        1.07     
!   PT        0.98     SC        0.99     
! 
! 
! Correcting IF 4.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.39     KK        1.24     KP        0.89     MK        0.97     
!   OV        1.23     
! 
!  Telescope amplitude corrections in sub-array 2:
!   KK        0.00*    MK        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   WZ        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   NY        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   FD        0.79     KP        2.18     LA        1.03     NL        1.15     
!   PT        0.99     
! 
!  Telescope amplitude corrections in sub-array 6:
!   BR        1.34     FD        0.81     KP        1.52     LA        1.00     
!   NL        1.09     OV        1.10     PT        0.98     SC        1.03     
!   WZ        1.17     
! 
!  Telescope amplitude corrections in sub-array 7:
!   BR        1.35     FD        0.89     KP        1.76     LA        1.04     
!   NL        1.07     OV        1.06     PT        0.98     SC        1.09     
! 
!  Telescope amplitude corrections in sub-array 8:
!   BR        1.46     FD        0.89     KK        1.12     KP        2.12     
!   LA        1.07     MK        0.98     NL        1.09     OV        1.07     
!   PT        0.96     SC        1.02     
! 
! 
! Fit before self-cal, rms=0.228335Jy  sigma=1.176414
! Fit after  self-cal, rms=0.216506Jy  sigma=0.787514
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.9308 mas, bmaj=2.298 mas, bpa=2.577 degrees
! Estimated noise=2.23792 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 = -0.0146981 Jy
! Component: 100  -  total flux cleaned = -0.0167889 Jy
! Component: 150  -  total flux cleaned = -0.0173562 Jy
! Component: 200  -  total flux cleaned = -0.018052 Jy
! Total flux subtracted in 200 components = -0.018052 Jy
! Clean residual min=-0.009175 max=0.009011 Jy/beam
! Clean residual mean=-0.000024 rms=0.002240 Jy/beam
! Combined flux in latest and established models = 0.743298 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 46 components and 0.743298 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.214349Jy  sigma=0.778292
! Fit after  self-cal, rms=0.215265Jy  sigma=0.777098
! Inverting map 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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=0.215265Jy  sigma=0.777098
! Fit after  self-cal, rms=0.213998Jy  sigma=0.772900
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.9365 mas, bmaj=2.31 mas, bpa=2.747 degrees
! Estimated noise=2.23606 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.010082 Jy
! Component: 100  -  total flux cleaned = -0.0117226 Jy
! Component: 150  -  total flux cleaned = -0.0121079 Jy
! Component: 200  -  total flux cleaned = -0.0127477 Jy
! Total flux subtracted in 200 components = -0.0127477 Jy
! Clean residual min=-0.008568 max=0.008454 Jy/beam
! Clean residual mean=-0.000032 rms=0.002067 Jy/beam
! Combined flux in latest and established models = 0.730551 Jy
selfcal
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 55 components and 0.730551 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.212820Jy  sigma=0.769123
! Fit after  self-cal, rms=0.212705Jy  sigma=0.768825
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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 = -0.000562187 Jy
! Component: 100  -  total flux cleaned = -0.000833443 Jy
! Component: 150  -  total flux cleaned = -0.00119789 Jy
! Component: 200  -  total flux cleaned = -0.00152014 Jy
! Total flux subtracted in 200 components = -0.00152014 Jy
! Clean residual min=-0.008658 max=0.008713 Jy/beam
! Clean residual mean=-0.000032 rms=0.002050 Jy/beam
! Combined flux in latest and established models = 0.72903 Jy
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 57 components and 0.729031 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.212444Jy  sigma=0.767809
! Fit after  self-cal, rms=0.212356Jy  sigma=0.767662
! Inverting map 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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=0.212356Jy  sigma=0.767662
! Fit after  self-cal, rms=0.224729Jy  sigma=0.758648
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.9405 mas, bmaj=2.318 mas, bpa=2.893 degrees
! Estimated noise=2.24275 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00377759 Jy
! Component: 100  -  total flux cleaned = -0.00473471 Jy
! Component: 150  -  total flux cleaned = -0.00512561 Jy
! Component: 200  -  total flux cleaned = -0.00544692 Jy
! Total flux subtracted in 200 components = -0.00544692 Jy
! Clean residual min=-0.007074 max=0.006741 Jy/beam
! Clean residual mean=-0.000013 rms=0.001674 Jy/beam
! Combined flux in latest and established models = 0.723584 Jy
selfcal
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 62 components and 0.723584 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.224391Jy  sigma=0.757098
! Fit after  self-cal, rms=0.224370Jy  sigma=0.756947
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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 = -0.000614355 Jy
! Component: 100  -  total flux cleaned = -0.000798685 Jy
! Component: 150  -  total flux cleaned = -0.000967598 Jy
! Component: 200  -  total flux cleaned = -0.00104585 Jy
! Total flux subtracted in 200 components = -0.00104585 Jy
! Clean residual min=-0.007065 max=0.006666 Jy/beam
! Clean residual mean=-0.000013 rms=0.001666 Jy/beam
! Combined flux in latest and established models = 0.722538 Jy
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 63 components and 0.722538 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.224256Jy  sigma=0.756558
! Fit after  self-cal, rms=0.224216Jy  sigma=0.756513
! Inverting map 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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=0.224216Jy  sigma=0.756513
! Fit after  self-cal, rms=0.224087Jy  sigma=0.755290
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=2.837 mas, bmaj=3.835 mas, bpa=5.679 degrees
! Estimated noise=2.57949 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.0031749 Jy
! Component: 100  -  total flux cleaned = -0.00323162 Jy
! Component: 150  -  total flux cleaned = -0.00343503 Jy
! Component: 200  -  total flux cleaned = -0.00343491 Jy
! Total flux subtracted in 200 components = -0.00343491 Jy
! Clean residual min=-0.006556 max=0.007349 Jy/beam
! Clean residual mean=-0.000028 rms=0.001975 Jy/beam
! Combined flux in latest and established models = 0.719103 Jy
selfcal
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 69 components and 0.719103 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.224017Jy  sigma=0.754816
! Fit after  self-cal, rms=0.223972Jy  sigma=0.754672
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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 = -0.000386516 Jy
! Component: 100  -  total flux cleaned = -0.000429704 Jy
! Component: 150  -  total flux cleaned = -0.000461595 Jy
! Component: 200  -  total flux cleaned = -0.000460922 Jy
! Total flux subtracted in 200 components = -0.000460922 Jy
! Clean residual min=-0.006675 max=0.007372 Jy/beam
! Clean residual mean=-0.000027 rms=0.001951 Jy/beam
! Combined flux in latest and established models = 0.718642 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 71 components and 0.718642 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.223968Jy  sigma=0.754663
! Fit after  self-cal, rms=0.223946Jy  sigma=0.754638
! Inverting map 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.9422 mas, bmaj=2.324 mas, bpa=2.983 degrees
! Estimated noise=2.24802 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9422 x 2.324 at 2.983 degrees (North through East)
! Clean map  min=-0.0060823  max=0.61535 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=0.223946Jy  sigma=0.754638
! Fit after  self-cal, rms=0.259407Jy  sigma=0.611339
! Inverting map and beam 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.9389 mas, bmaj=2.322 mas, bpa=3.07 degrees
! Estimated noise=2.24313 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00312442 Jy
! Component: 100  -  total flux cleaned = -0.00312649 Jy
! Component: 150  -  total flux cleaned = -0.00312781 Jy
! Component: 200  -  total flux cleaned = -0.0032018 Jy
! Total flux subtracted in 200 components = -0.0032018 Jy
! Clean residual min=-0.006441 max=0.006069 Jy/beam
! Clean residual mean=0.000001 rms=0.001467 Jy/beam
! Combined flux in latest and established models = 0.71544 Jy
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 77 components and 0.71544 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.259233Jy  sigma=0.610740
! Fit after  self-cal, rms=0.259249Jy  sigma=0.610615
! Inverting map 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000407822 Jy
! Component: 100  -  total flux cleaned = -0.000481506 Jy
! Component: 150  -  total flux cleaned = -0.000545518 Jy
! Component: 200  -  total flux cleaned = -0.000545756 Jy
! Total flux subtracted in 200 components = -0.000545756 Jy
! Clean residual min=-0.006546 max=0.005895 Jy/beam
! Clean residual mean=0.000002 rms=0.001458 Jy/beam
! Combined flux in latest and established models = 0.714894 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 78 components and 0.714894 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.259174Jy  sigma=0.610412
! Fit after  self-cal, rms=0.259168Jy  sigma=0.610359
! Inverting map 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.259168Jy  sigma=0.610359
! Fit after  self-cal, rms=0.273634Jy  sigma=0.609778
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 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.7763 mas, bmaj=1.913 mas, bpa=3.346 degrees
! Estimated noise=3.27518 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.488382 Jy
! Component: 100  -  total flux cleaned = 0.620143 Jy
! Component: 150  -  total flux cleaned = 0.666021 Jy
! Component: 200  -  total flux cleaned = 0.686988 Jy
! Total flux subtracted in 200 components = 0.686988 Jy
! Clean residual min=-0.012546 max=0.011397 Jy/beam
! Clean residual mean=0.000016 rms=0.002423 Jy/beam
! Combined flux in latest and established models = 0.686988 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 15 model components to the UV plane model.
! The established model now contains 15 components and 0.686988 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.9408 mas, bmaj=2.325 mas, bpa=3.176 degrees
! Estimated noise=2.24375 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)
! Added new window around map position (0.8, -1).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0143632 Jy
! Component: 100  -  total flux cleaned = 0.0196051 Jy
! Component: 150  -  total flux cleaned = 0.0217279 Jy
! Component: 200  -  total flux cleaned = 0.0228712 Jy
! Total flux subtracted in 200 components = 0.0228712 Jy
! Clean residual min=-0.007228 max=0.005861 Jy/beam
! Clean residual mean=0.000004 rms=0.001496 Jy/beam
! Combined flux in latest and established models = 0.709859 Jy
! Adding 28 model components to the UV plane model.
! The established model now contains 39 components and 0.709859 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 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 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=2.84 mas, bmaj=3.847 mas, bpa=6.5 degrees
! Estimated noise=2.5744 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00213169 Jy
! Component: 100  -  total flux cleaned = 0.00258074 Jy
! Component: 150  -  total flux cleaned = 0.00270075 Jy
! Component: 200  -  total flux cleaned = 0.00270329 Jy
! Total flux subtracted in 200 components = 0.00270329 Jy
! Clean residual min=-0.006560 max=0.006308 Jy/beam
! Clean residual mean=0.000000 rms=0.001668 Jy/beam
! Combined flux in latest and established models = 0.712562 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 = 4.96791e-05 Jy
! Component: 100  -  total flux cleaned = 5.03343e-05 Jy
! Component: 150  -  total flux cleaned = 8.95698e-05 Jy
! Component: 200  -  total flux cleaned = 5.28531e-05 Jy
! Total flux subtracted in 200 components = 5.28531e-05 Jy
! Clean residual min=-0.006502 max=0.006189 Jy/beam
! Clean residual mean=-0.000000 rms=0.001659 Jy/beam
! Combined flux in latest and established models = 0.712615 Jy
! Adding 22 model components to the UV plane model.
! The established model now contains 59 components and 0.712615 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.9408 mas, bmaj=2.325 mas, bpa=3.176 degrees
! Estimated noise=2.24375 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000438876 Jy
! Component: 100  -  total flux cleaned = -0.000445243 Jy
! Component: 150  -  total flux cleaned = -0.000448259 Jy
! Component: 200  -  total flux cleaned = -0.000449023 Jy
! Total flux subtracted in 200 components = -0.000449023 Jy
! Clean residual min=-0.006478 max=0.005771 Jy/beam
! Clean residual mean=0.000000 rms=0.001441 Jy/beam
! Combined flux in latest and established models = 0.712166 Jy
selfcal
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 65 components and 0.712166 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.273440Jy  sigma=0.609773
! Fit after  self-cal, rms=0.273389Jy  sigma=0.609195
wmodel /scr/pima/rdv72_uvs/J1354-0206_X_map.mod
! Writing 65 model components to file: /scr/pima/rdv72_uvs/J1354-0206_X_map.mod
wobs /scr/pima/rdv72_uvs/J1354-0206_X_uvs.fits
! Writing UV FITS file: /scr/pima/rdv72_uvs/J1354-0206_X_uvs.fits
wwins /scr/pima/rdv72_uvs/J1354-0206_X_map.win
! wwins: Wrote 3 windows to /scr/pima/rdv72_uvs/J1354-0206_X_map.win
x = (field_size-8) * field_cell / 4
addwin -x,x,-x,x
clean (field_size*4),0.01
! Inverting map 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! clean: niter=4096  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00119543 Jy
! Component: 100  -  total flux cleaned = -0.00150319 Jy
! Component: 150  -  total flux cleaned = -0.00150588 Jy
! Component: 200  -  total flux cleaned = -0.00160345 Jy
! Component: 250  -  total flux cleaned = -0.00142399 Jy
! Component: 300  -  total flux cleaned = -0.000988142 Jy
! Component: 350  -  total flux cleaned = -0.00064762 Jy
! Component: 400  -  total flux cleaned = -0.000646023 Jy
! Component: 450  -  total flux cleaned = -0.000562829 Jy
! Component: 500  -  total flux cleaned = -0.000642192 Jy
! Component: 550  -  total flux cleaned = -0.000641147 Jy
! Component: 600  -  total flux cleaned = -0.000720028 Jy
! Component: 650  -  total flux cleaned = -0.000873757 Jy
! Component: 700  -  total flux cleaned = -0.000799704 Jy
! Component: 750  -  total flux cleaned = -0.00109898 Jy
! Component: 800  -  total flux cleaned = -0.00102353 Jy
! Component: 850  -  total flux cleaned = -0.000951374 Jy
! Component: 900  -  total flux cleaned = -0.00102225 Jy
! Component: 950  -  total flux cleaned = -0.00102182 Jy
! Component: 1000  -  total flux cleaned = -0.000740018 Jy
! Component: 1050  -  total flux cleaned = -0.000739402 Jy
! Component: 1100  -  total flux cleaned = -0.000532309 Jy
! Component: 1150  -  total flux cleaned = -0.000191147 Jy
! Component: 1200  -  total flux cleaned = -0.000123422 Jy
! Component: 1250  -  total flux cleaned = 0.000344215 Jy
! Component: 1300  -  total flux cleaned = 0.00047524 Jy
! Component: 1350  -  total flux cleaned = 0.000542035 Jy
! Component: 1400  -  total flux cleaned = 0.000672022 Jy
! Component: 1450  -  total flux cleaned = 0.00112254 Jy
! Component: 1500  -  total flux cleaned = 0.00118632 Jy
! Component: 1550  -  total flux cleaned = 0.00162939 Jy
! Component: 1600  -  total flux cleaned = 0.00194436 Jy
! Component: 1650  -  total flux cleaned = 0.00200729 Jy
! Component: 1700  -  total flux cleaned = 0.00243946 Jy
! Component: 1750  -  total flux cleaned = 0.00231721 Jy
! Component: 1800  -  total flux cleaned = 0.00249964 Jy
! Component: 1850  -  total flux cleaned = 0.00243992 Jy
! Component: 1900  -  total flux cleaned = 0.00303958 Jy
! Component: 1950  -  total flux cleaned = 0.00292013 Jy
! Component: 2000  -  total flux cleaned = 0.00286053 Jy
! Component: 2050  -  total flux cleaned = 0.00291922 Jy
! Component: 2100  -  total flux cleaned = 0.002861 Jy
! Component: 2150  -  total flux cleaned = 0.00297691 Jy
! Component: 2200  -  total flux cleaned = 0.00303431 Jy
! Component: 2250  -  total flux cleaned = 0.00309134 Jy
! Component: 2300  -  total flux cleaned = 0.00326197 Jy
! Component: 2350  -  total flux cleaned = 0.00309185 Jy
! Component: 2400  -  total flux cleaned = 0.00337326 Jy
! Component: 2450  -  total flux cleaned = 0.00337339 Jy
! Component: 2500  -  total flux cleaned = 0.00342829 Jy
! Component: 2550  -  total flux cleaned = 0.00342853 Jy
! Component: 2600  -  total flux cleaned = 0.00342863 Jy
! Component: 2650  -  total flux cleaned = 0.00359276 Jy
! Component: 2700  -  total flux cleaned = 0.00348399 Jy
! Component: 2750  -  total flux cleaned = 0.00369965 Jy
! Component: 2800  -  total flux cleaned = 0.00375338 Jy
! Component: 2850  -  total flux cleaned = 0.00353926 Jy
! Component: 2900  -  total flux cleaned = 0.00369908 Jy
! Component: 2950  -  total flux cleaned = 0.00364637 Jy
! Component: 3000  -  total flux cleaned = 0.00364622 Jy
! Component: 3050  -  total flux cleaned = 0.00375095 Jy
! Component: 3100  -  total flux cleaned = 0.00364683 Jy
! Component: 3150  -  total flux cleaned = 0.00380199 Jy
! Component: 3200  -  total flux cleaned = 0.00395639 Jy
! Component: 3250  -  total flux cleaned = 0.00380245 Jy
! Component: 3300  -  total flux cleaned = 0.00385346 Jy
! Component: 3350  -  total flux cleaned = 0.00390429 Jy
! Component: 3400  -  total flux cleaned = 0.00410659 Jy
! Component: 3450  -  total flux cleaned = 0.00405593 Jy
! Component: 3500  -  total flux cleaned = 0.00415556 Jy
! Component: 3550  -  total flux cleaned = 0.00405625 Jy
! Component: 3600  -  total flux cleaned = 0.00400718 Jy
! Component: 3650  -  total flux cleaned = 0.00420411 Jy
! Component: 3700  -  total flux cleaned = 0.00420425 Jy
! Component: 3750  -  total flux cleaned = 0.00425315 Jy
! Component: 3800  -  total flux cleaned = 0.00449578 Jy
! Component: 3850  -  total flux cleaned = 0.00454375 Jy
! Component: 3900  -  total flux cleaned = 0.00463977 Jy
! Component: 3950  -  total flux cleaned = 0.00459181 Jy
! Component: 4000  -  total flux cleaned = 0.00459202 Jy
! Component: 4050  -  total flux cleaned = 0.00459186 Jy
! Total flux subtracted in 4096 components = 0.00440273 Jy
! Clean residual min=-0.003001 max=0.003039 Jy/beam
! Clean residual mean=0.000001 rms=0.000818 Jy/beam
! Combined flux in latest and established models = 0.716569 Jy
keep
! Adding 274 model components to the UV plane model.
! The established model now contains 339 components and 0.716569 Jy
![Exited script file: /home/lpetrov/bin/01_muppet]
wmap "/scr/pima/rdv72_uvs/J1354-0206_X\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9408 x 2.325 at 3.176 degrees (North through East)
! Clean map  min=-0.0046457  max=0.62194 Jy/beam
! Writing clean map to FITS file: /scr/pima/rdv72_uvs/J1354-0206_X_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.621943 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.223% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000812773 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.392049 0.392049 0.784097 1.56819 3.13639 6.27278 12.5456 25.0911 50.1822
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0024 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.621 
quit
! Quitting program
! Log file /scr/pima/rdv72_uvs/J1354-0206_X_uvs.log closed on Sat Oct  5 08:48:00 2013