! Started logfile: /scr/pima/gc030_uvs/J1316+7226_X_uvs.log on Fri Apr 22 08:49:03 2016
obs /scr/pima/gc030_uvs/J1316+7226_X_uva.fits
! Reading UV FITS file: /scr/pima/gc030_uvs/J1316+7226_X_uva.fits
! AN table 1: 70 integrations on 36 of 36 possible baselines.
! AN table 2: 70 integrations on 36 of 36 possible baselines.
! AN table 3: 209 integrations on 36 of 36 possible baselines.
! Apparent sampling: 0.640322 visibilities/baseline/integration-bin.
! Found source: J1316+7226
! 
! There are 8 IFs, and a total of 8 channels:
! 
!  IF  Channel    Frequency  Freq offset  Number of   Overall IF
!       origin    at origin  per channel   channels    bandwidth
!  ------------------------------------------------------------- (Hz)
!  01        1  8.37724e+09        8e+06          1        8e+06
!  02        2  8.38499e+09        8e+06          1        8e+06
!  03        3  8.39324e+09        8e+06          1        8e+06
!  04        4  8.40099e+09        8e+06          1        8e+06
!  05        5  8.40924e+09        8e+06          1        8e+06
!  06        6  8.41699e+09        8e+06          1        8e+06
!  07        7  8.42524e+09        8e+06          1        8e+06
!  08        8  8.43299e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 139 lines of history.
! 
! Reading 64360 visibilities.
select rr, 1,2,3,4,6,7,8 
! Selecting polarization: RR,  channels: 1..4 6..8
! Reading IF 1 channels: 1..1
! Reading IF 2 channels: 2..2
! Reading IF 3 channels: 3..3
! Reading IF 4 channels: 4..4
! Reading IF 5 channels: (none)
! Reading IF 6 channels: 6..6
! Reading IF 7 channels: 7..7
! Reading IF 8 channels: 8..8
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/gc030_uvs/J1316+7226_X]
float lim_self
lim_self = 120.0
float lim_val
lim_va   = 1.2
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 1 telescope corrections were flagged in sub-array 1.
!  A total of 20 telescope corrections were flagged in sub-array 2.
!  A total of 635 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 1 telescope corrections were flagged in sub-array 1.
!  A total of 20 telescope corrections were flagged in sub-array 2.
!  A total of 635 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 1 telescope corrections were flagged in sub-array 1.
!  A total of 20 telescope corrections were flagged in sub-array 2.
!  A total of 635 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 1 telescope corrections were flagged in sub-array 1.
!  A total of 20 telescope corrections were flagged in sub-array 2.
!  A total of 635 telescope corrections were flagged in sub-array 3.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
!  A total of 71 telescope corrections were flagged in sub-array 1.
!  A total of 90 telescope corrections were flagged in sub-array 2.
!  A total of 705 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 7.
!  A total of 1 telescope corrections were flagged in sub-array 1.
!  A total of 20 telescope corrections were flagged in sub-array 2.
!  A total of 635 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 8.
!  A total of 1 telescope corrections were flagged in sub-array 1.
!  A total of 20 telescope corrections were flagged in sub-array 2.
!  A total of 635 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=1.006438Jy  sigma=16.500483
! Fit after  self-cal, rms=0.950510Jy  sigma=15.853795
! 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 0.848% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
! Estimated beam: bmin=0.4626 mas, bmaj=0.7346 mas, bpa=-33.48 degrees
! Estimated noise=0.501599 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 = 0.0324186 Jy
! Component: 100  -  total flux cleaned = 0.0438725 Jy
! Total flux subtracted in 100 components = 0.0438725 Jy
! Clean residual min=-0.003886 max=0.005889 Jy/beam
! Clean residual mean=0.000006 rms=0.000792 Jy/beam
! Combined flux in latest and established models = 0.0438725 Jy
! Performing phase self-cal
! Adding 4 model components to the UV plane model.
! The established model now contains 4 components and 0.0438725 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.106996Jy  sigma=0.848065
! Fit after  self-cal, rms=0.105311Jy  sigma=0.832351
! Inverting map 
! Your choice of large map pixels excluded 0.848% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00911589 Jy
! Component: 100  -  total flux cleaned = 0.0148168 Jy
! Total flux subtracted in 100 components = 0.0148168 Jy
! Clean residual min=-0.003262 max=0.003299 Jy/beam
! Clean residual mean=0.000004 rms=0.000635 Jy/beam
! Combined flux in latest and established models = 0.0586893 Jy
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 6 components and 0.0586893 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.103665Jy  sigma=0.816752
! Fit after  self-cal, rms=0.103076Jy  sigma=0.815854
! Inverting map 
! Your choice of large map pixels excluded 0.848% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00435306 Jy
! Component: 100  -  total flux cleaned = 0.00708071 Jy
! Total flux subtracted in 100 components = 0.00708071 Jy
! Clean residual min=-0.002750 max=0.002447 Jy/beam
! Clean residual mean=0.000002 rms=0.000584 Jy/beam
! Combined flux in latest and established models = 0.06577 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 7 components and 0.06577 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.102744Jy  sigma=0.812892
! Fit after  self-cal, rms=0.102449Jy  sigma=0.812584
! Inverting map 
! Your choice of large map pixels excluded 0.848% of the data.
!  The x-axis pixel size should ideally be below 0.1881 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 0.848% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
! Estimated beam: bmin=0.5813 mas, bmaj=0.8354 mas, bpa=-34.35 degrees
! Estimated noise=0.251306 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 = 0.00183908 Jy
! Component: 100  -  total flux cleaned = 0.00227307 Jy
! Component: 150  -  total flux cleaned = 0.00233218 Jy
! Component: 200  -  total flux cleaned = 0.00233161 Jy
! Total flux subtracted in 200 components = 0.00233161 Jy
! Clean residual min=-0.003012 max=0.002725 Jy/beam
! Clean residual mean=0.000017 rms=0.000667 Jy/beam
! Combined flux in latest and established models = 0.0681017 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 10 components and 0.0681017 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.102381Jy  sigma=0.812298
! Fit after  self-cal, rms=0.102256Jy  sigma=0.812223
! Inverting map 
! Your choice of large map pixels excluded 0.848% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5813 x 0.8354 at -34.35 degrees (North through East)
! Clean map  min=-0.0028539  max=0.050549 Jy/beam
if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val
! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2.
! Selfcal phase corrections will not be limited.
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    HN        1.00*    KP        1.00*    LA        1.00*    
!   MK        1.00*    NL        1.00*    OV        1.00*    PT        1.00*    
!   SC        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.10     EB        1.01     HN        0.84     KP        0.97     
!   LA        0.92     MK        0.85     NL        1.09     OV        1.07     
!   PT        1.10     
! 
!  A total of 6 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    EB        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    PT        1.00*    
!   SC        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    HN        1.00*    KP        1.00*    LA        1.00*    
!   MK        1.00*    NL        1.00*    OV        1.00*    PT        1.00*    
!   SC        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.13     EB        1.00     HN        0.84     KP        1.05     
!   LA        0.94     MK        0.92     NL        1.01     OV        1.08     
!   PT        0.99     
! 
!  A total of 6 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    EB        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    PT        1.00*    
!   SC        1.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    HN        1.00*    KP        1.00*    LA        1.00*    
!   MK        1.00*    NL        1.00*    OV        1.00*    PT        1.00*    
!   SC        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00*    EB        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    OV        1.00*    
!   PT        1.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    EB        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    PT        1.00*    
!   SC        1.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    HN        1.00*    KP        1.00*    LA        1.00*    
!   MK        1.00*    NL        1.00*    OV        1.00*    PT        1.00*    
!   SC        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00*    EB        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    OV        1.00*    
!   PT        1.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    EB        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    PT        1.00*    
!   SC        1.00*    
! 
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    HN        1.00*    KP        1.00*    LA        1.00*    
!   MK        1.00*    NL        1.00*    OV        1.00*    PT        1.00*    
!   SC        1.00*    
! 
!  A total of 9 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00*    EB        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    OV        1.00*    
!   PT        1.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    EB        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    PT        1.00*    
!   SC        1.00*    
! 
! 
! Correcting IF 7.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    HN        1.00*    KP        1.00*    LA        1.00*    
!   MK        1.00*    NL        1.00*    OV        1.00*    PT        1.00*    
!   SC        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00*    EB        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    OV        1.00*    
!   PT        1.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    EB        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    PT        1.00*    
!   SC        1.00*    
! 
! 
! Correcting IF 8.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    HN        1.00*    KP        1.00*    LA        1.00*    
!   MK        1.00*    NL        1.00*    OV        1.00*    PT        1.00*    
!   SC        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00*    EB        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    OV        1.00*    
!   PT        1.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00*    EB        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    PT        1.00*    
!   SC        1.00*    
! 
! 
! Fit before self-cal, rms=0.102256Jy  sigma=0.812223
! Fit after  self-cal, rms=0.101323Jy  sigma=0.810634
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
! Estimated beam: bmin=0.5821 mas, bmaj=0.8339 mas, bpa=-34.64 degrees
! Estimated noise=0.251482 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 = 6.83355e-05 Jy
! Component: 100  -  total flux cleaned = 5.19759e-05 Jy
! Component: 150  -  total flux cleaned = 3.68149e-05 Jy
! Component: 200  -  total flux cleaned = 2.30193e-05 Jy
! Total flux subtracted in 200 components = 2.30193e-05 Jy
! Clean residual min=-0.002926 max=0.002619 Jy/beam
! Clean residual mean=0.000017 rms=0.000645 Jy/beam
! Combined flux in latest and established models = 0.0681247 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 13 components and 0.0681247 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.101310Jy  sigma=0.810655
! Fit after  self-cal, rms=0.101261Jy  sigma=0.810580
! Inverting map 
! Your choice of large map pixels excluded 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 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.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.101261Jy  sigma=0.810580
! Fit after  self-cal, rms=0.101106Jy  sigma=0.810012
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
! Estimated beam: bmin=0.5806 mas, bmaj=0.834 mas, bpa=-34.55 degrees
! Estimated noise=0.252446 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000286902 Jy
! Component: 100  -  total flux cleaned = 0.000345012 Jy
! Component: 150  -  total flux cleaned = 0.000332979 Jy
! Component: 200  -  total flux cleaned = 0.000321679 Jy
! Total flux subtracted in 200 components = 0.000321679 Jy
! Clean residual min=-0.002751 max=0.002500 Jy/beam
! Clean residual mean=0.000016 rms=0.000625 Jy/beam
! Combined flux in latest and established models = 0.0684464 Jy
selfcal
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 13 components and 0.0684464 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.101096Jy  sigma=0.810050
! Fit after  self-cal, rms=0.101100Jy  sigma=0.809999
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 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 = -7.39396e-05 Jy
! Component: 100  -  total flux cleaned = -9.49878e-05 Jy
! Component: 150  -  total flux cleaned = -0.000104709 Jy
! Component: 200  -  total flux cleaned = -0.00012275 Jy
! Total flux subtracted in 200 components = -0.00012275 Jy
! Clean residual min=-0.002763 max=0.002530 Jy/beam
! Clean residual mean=0.000016 rms=0.000628 Jy/beam
! Combined flux in latest and established models = 0.0683236 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 15 components and 0.0683236 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.101095Jy  sigma=0.810018
! Fit after  self-cal, rms=0.101090Jy  sigma=0.810012
! Inverting map 
! Your choice of large map pixels excluded 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 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.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.101090Jy  sigma=0.810012
! Fit after  self-cal, rms=0.101307Jy  sigma=0.809642
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
! Estimated beam: bmin=0.5791 mas, bmaj=0.8345 mas, bpa=-34.41 degrees
! Estimated noise=0.253334 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00026874 Jy
! Component: 100  -  total flux cleaned = 0.000289998 Jy
! Component: 150  -  total flux cleaned = 0.000289633 Jy
! Component: 200  -  total flux cleaned = 0.000281467 Jy
! Total flux subtracted in 200 components = 0.000281467 Jy
! Clean residual min=-0.002655 max=0.002456 Jy/beam
! Clean residual mean=0.000016 rms=0.000620 Jy/beam
! Combined flux in latest and established models = 0.0686051 Jy
selfcal
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 15 components and 0.0686051 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.101302Jy  sigma=0.809680
! Fit after  self-cal, rms=0.101312Jy  sigma=0.809650
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -6.17372e-05 Jy
! Component: 100  -  total flux cleaned = -7.75094e-05 Jy
! Component: 150  -  total flux cleaned = -9.20496e-05 Jy
! Component: 200  -  total flux cleaned = -0.000105835 Jy
! Total flux subtracted in 200 components = -0.000105835 Jy
! Clean residual min=-0.002661 max=0.002472 Jy/beam
! Clean residual mean=0.000016 rms=0.000621 Jy/beam
! Combined flux in latest and established models = 0.0684992 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 15 components and 0.0684992 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.101310Jy  sigma=0.809672
! Fit after  self-cal, rms=0.101308Jy  sigma=0.809669
! Inverting map 
! Your choice of large map pixels excluded 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 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.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.101308Jy  sigma=0.809669
! Fit after  self-cal, rms=0.101506Jy  sigma=0.809657
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
! Estimated beam: bmin=2.239 mas, bmaj=3.022 mas, bpa=26.71 degrees
! Estimated noise=0.492931 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000184765 Jy
! Component: 100  -  total flux cleaned = 0.000184296 Jy
! Component: 150  -  total flux cleaned = 0.00019418 Jy
! Component: 200  -  total flux cleaned = 0.000203891 Jy
! Total flux subtracted in 200 components = 0.000203891 Jy
! Clean residual min=-0.005878 max=0.005237 Jy/beam
! Clean residual mean=0.000061 rms=0.001702 Jy/beam
! Combined flux in latest and established models = 0.0687031 Jy
selfcal
! Performing phase self-cal
! Adding 4 model components to the UV plane model.
! The established model now contains 16 components and 0.0687031 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.101509Jy  sigma=0.809686
! Fit after  self-cal, rms=0.101485Jy  sigma=0.809651
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 9.09827e-05 Jy
! Component: 100  -  total flux cleaned = 0.00010052 Jy
! Component: 150  -  total flux cleaned = 0.000110002 Jy
! Component: 200  -  total flux cleaned = 0.00011936 Jy
! Total flux subtracted in 200 components = 0.00011936 Jy
! Clean residual min=-0.005882 max=0.005217 Jy/beam
! Clean residual mean=0.000061 rms=0.001699 Jy/beam
! Combined flux in latest and established models = 0.0688225 Jy
! Performing phase self-cal
! Adding 4 model components to the UV plane model.
! The established model now contains 16 components and 0.0688225 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.101488Jy  sigma=0.809778
! Fit after  self-cal, rms=0.101456Jy  sigma=0.809749
! Inverting map 
! Your choice of large map pixels excluded 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 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 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
! Estimated beam: bmin=0.5789 mas, bmaj=0.835 mas, bpa=-34.26 degrees
! Estimated noise=0.253765 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5789 x 0.835 at -34.26 degrees (North through East)
! Clean map  min=-0.002456  max=0.050815 Jy/beam
if(peak(flux) > thresh)
  selfcal true, true
  clean clean_niter,clean_gain
  selfcal
  flux_cutoff = imstat(rms) * dynam
  repeat
    if (peak(flux) > flux_cutoff) peakwin win_mult
    clean clean_niter,clean_gain
    flux_cutoff = imstat(rms) * dynam
    selfcal
    new_peak = peak(flux)
    until(new_peak<=flux_cutoff)
  selfcal true, true
  end if
print "************** CLEARING MODEL AND STARTING OVER **********"
! ************** CLEARING MODEL AND STARTING OVER ********** 
clrmod true
! clrmod: Cleared the established and tentative models.
uvw 2,-1
! Uniform weighting binwidth: 2 (pixels).
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
! Estimated beam: bmin=0.4612 mas, bmaj=0.737 mas, bpa=-33.42 degrees
! Estimated noise=0.504821 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0344627 Jy
! Component: 100  -  total flux cleaned = 0.0486878 Jy
! Component: 150  -  total flux cleaned = 0.0574464 Jy
! Component: 200  -  total flux cleaned = 0.0628869 Jy
! Total flux subtracted in 200 components = 0.0628869 Jy
! Clean residual min=-0.002725 max=0.002854 Jy/beam
! Clean residual mean=0.000003 rms=0.000591 Jy/beam
! Combined flux in latest and established models = 0.0628869 Jy
uvw 0,-1
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Adding 7 model components to the UV plane model.
! The established model now contains 7 components and 0.0628869 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
! Estimated beam: bmin=0.5789 mas, bmaj=0.835 mas, bpa=-34.26 degrees
! Estimated noise=0.253765 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 = 0.00385592 Jy
! Component: 100  -  total flux cleaned = 0.00561746 Jy
! Component: 150  -  total flux cleaned = 0.00588662 Jy
! Component: 200  -  total flux cleaned = 0.00608946 Jy
! Total flux subtracted in 200 components = 0.00608946 Jy
! Clean residual min=-0.002650 max=0.002408 Jy/beam
! Clean residual mean=0.000016 rms=0.000623 Jy/beam
! Combined flux in latest and established models = 0.0689763 Jy
! Adding 10 model components to the UV plane model.
! The established model now contains 11 components and 0.0689763 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 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 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
! Estimated beam: bmin=2.239 mas, bmaj=3.022 mas, bpa=26.71 degrees
! Estimated noise=0.492931 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -5.34434e-05 Jy
! Component: 100  -  total flux cleaned = -5.38076e-05 Jy
! Component: 150  -  total flux cleaned = -4.15579e-05 Jy
! Component: 200  -  total flux cleaned = -3.00196e-05 Jy
! Total flux subtracted in 200 components = -3.00196e-05 Jy
! Clean residual min=-0.005920 max=0.005204 Jy/beam
! Clean residual mean=0.000060 rms=0.001697 Jy/beam
! Combined flux in latest and established models = 0.0689463 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 = 1.08666e-05 Jy
! Component: 100  -  total flux cleaned = 2.10064e-05 Jy
! Component: 150  -  total flux cleaned = 3.08643e-05 Jy
! Component: 200  -  total flux cleaned = 4.11721e-05 Jy
! Total flux subtracted in 200 components = 4.11721e-05 Jy
! Clean residual min=-0.005921 max=0.005201 Jy/beam
! Clean residual mean=0.000060 rms=0.001696 Jy/beam
! Combined flux in latest and established models = 0.0689875 Jy
! Adding 4 model components to the UV plane model.
! The established model now contains 13 components and 0.0689875 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
! Estimated beam: bmin=0.5789 mas, bmaj=0.835 mas, bpa=-34.26 degrees
! Estimated noise=0.253765 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000109253 Jy
! Component: 100  -  total flux cleaned = 8.7541e-05 Jy
! Component: 150  -  total flux cleaned = -2.22994e-05 Jy
! Component: 200  -  total flux cleaned = -0.000126487 Jy
! Total flux subtracted in 200 components = -0.000126487 Jy
! Clean residual min=-0.002653 max=0.002453 Jy/beam
! Clean residual mean=0.000016 rms=0.000621 Jy/beam
! Combined flux in latest and established models = 0.068861 Jy
selfcal
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 17 components and 0.068861 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.101459Jy  sigma=0.809681
! Fit after  self-cal, rms=0.101510Jy  sigma=0.809602
wmodel /scr/pima/gc030_uvs/J1316+7226_X_map.mod
! Writing 17 model components to file: /scr/pima/gc030_uvs/J1316+7226_X_map.mod
wobs /scr/pima/gc030_uvs/J1316+7226_X_uvs.fits
! Writing UV FITS file: /scr/pima/gc030_uvs/J1316+7226_X_uvs.fits
wwins /scr/pima/gc030_uvs/J1316+7226_X_map.win
! wwins: Wrote 1 windows to /scr/pima/gc030_uvs/J1316+7226_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 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
! clean: niter=4096  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000727055 Jy
! Component: 100  -  total flux cleaned = -0.00119616 Jy
! Component: 150  -  total flux cleaned = -0.00167165 Jy
! Component: 200  -  total flux cleaned = -0.00224061 Jy
! Component: 250  -  total flux cleaned = -0.00264455 Jy
! Component: 300  -  total flux cleaned = -0.00289495 Jy
! Component: 350  -  total flux cleaned = -0.00313753 Jy
! Component: 400  -  total flux cleaned = -0.0032394 Jy
! Component: 450  -  total flux cleaned = -0.00330525 Jy
! Component: 500  -  total flux cleaned = -0.00327302 Jy
! Component: 550  -  total flux cleaned = -0.00327356 Jy
! Component: 600  -  total flux cleaned = -0.00330473 Jy
! Component: 650  -  total flux cleaned = -0.0032744 Jy
! Component: 700  -  total flux cleaned = -0.00321434 Jy
! Component: 750  -  total flux cleaned = -0.00315599 Jy
! Component: 800  -  total flux cleaned = -0.00315665 Jy
! Component: 850  -  total flux cleaned = -0.00321382 Jy
! Component: 900  -  total flux cleaned = -0.00326933 Jy
! Component: 950  -  total flux cleaned = -0.0032969 Jy
! Component: 1000  -  total flux cleaned = -0.00335074 Jy
! Component: 1050  -  total flux cleaned = -0.00329734 Jy
! Component: 1100  -  total flux cleaned = -0.00337578 Jy
! Component: 1150  -  total flux cleaned = -0.00337591 Jy
! Component: 1200  -  total flux cleaned = -0.00350248 Jy
! Component: 1250  -  total flux cleaned = -0.00347758 Jy
! Component: 1300  -  total flux cleaned = -0.0035268 Jy
! Component: 1350  -  total flux cleaned = -0.00362329 Jy
! Component: 1400  -  total flux cleaned = -0.00362354 Jy
! Component: 1450  -  total flux cleaned = -0.00364672 Jy
! Component: 1500  -  total flux cleaned = -0.0037391 Jy
! Component: 1550  -  total flux cleaned = -0.00380731 Jy
! Component: 1600  -  total flux cleaned = -0.00387465 Jy
! Component: 1650  -  total flux cleaned = -0.00389686 Jy
! Component: 1700  -  total flux cleaned = -0.00396233 Jy
! Component: 1750  -  total flux cleaned = -0.0039406 Jy
! Component: 1800  -  total flux cleaned = -0.00398308 Jy
! Component: 1850  -  total flux cleaned = -0.00402533 Jy
! Component: 1900  -  total flux cleaned = -0.00406688 Jy
! Component: 1950  -  total flux cleaned = -0.00406657 Jy
! Component: 2000  -  total flux cleaned = -0.00406683 Jy
! Component: 2050  -  total flux cleaned = -0.0041072 Jy
! Component: 2100  -  total flux cleaned = -0.00406797 Jy
! Component: 2150  -  total flux cleaned = -0.00412697 Jy
! Component: 2200  -  total flux cleaned = -0.00410723 Jy
! Component: 2250  -  total flux cleaned = -0.00403071 Jy
! Component: 2300  -  total flux cleaned = -0.00399294 Jy
! Component: 2350  -  total flux cleaned = -0.00391806 Jy
! Component: 2400  -  total flux cleaned = -0.00393637 Jy
! Component: 2450  -  total flux cleaned = -0.00388153 Jy
! Component: 2500  -  total flux cleaned = -0.00382719 Jy
! Component: 2550  -  total flux cleaned = -0.00382718 Jy
! Component: 2600  -  total flux cleaned = -0.00382687 Jy
! Component: 2650  -  total flux cleaned = -0.00375664 Jy
! Component: 2700  -  total flux cleaned = -0.00380876 Jy
! Component: 2750  -  total flux cleaned = -0.00374023 Jy
! Component: 2800  -  total flux cleaned = -0.00372304 Jy
! Component: 2850  -  total flux cleaned = -0.00373968 Jy
! Component: 2900  -  total flux cleaned = -0.00367312 Jy
! Component: 2950  -  total flux cleaned = -0.00362377 Jy
! Component: 3000  -  total flux cleaned = -0.0036402 Jy
! Component: 3050  -  total flux cleaned = -0.00365616 Jy
! Component: 3100  -  total flux cleaned = -0.00370397 Jy
! Component: 3150  -  total flux cleaned = -0.00360883 Jy
! Component: 3200  -  total flux cleaned = -0.00360904 Jy
! Component: 3250  -  total flux cleaned = -0.00359354 Jy
! Component: 3300  -  total flux cleaned = -0.00359341 Jy
! Component: 3350  -  total flux cleaned = -0.00357802 Jy
! Component: 3400  -  total flux cleaned = -0.00354763 Jy
! Component: 3450  -  total flux cleaned = -0.00353275 Jy
! Component: 3500  -  total flux cleaned = -0.00345864 Jy
! Component: 3550  -  total flux cleaned = -0.00348844 Jy
! Component: 3600  -  total flux cleaned = -0.00348838 Jy
! Component: 3650  -  total flux cleaned = -0.00345963 Jy
! Component: 3700  -  total flux cleaned = -0.00343101 Jy
! Component: 3750  -  total flux cleaned = -0.00344512 Jy
! Component: 3800  -  total flux cleaned = -0.00334648 Jy
! Component: 3850  -  total flux cleaned = -0.00333256 Jy
! Component: 3900  -  total flux cleaned = -0.00334648 Jy
! Component: 3950  -  total flux cleaned = -0.00329141 Jy
! Component: 4000  -  total flux cleaned = -0.00329151 Jy
! Component: 4050  -  total flux cleaned = -0.00330498 Jy
! Total flux subtracted in 4096 components = -0.00321131 Jy
! Clean residual min=-0.000841 max=0.000897 Jy/beam
! Clean residual mean=0.000005 rms=0.000238 Jy/beam
! Combined flux in latest and established models = 0.0656497 Jy
keep
! Adding 417 model components to the UV plane model.
! The established model now contains 434 components and 0.0656497 Jy
![Exited script file: /home/lpetrov/bin/01_muppet]
wmap "/scr/pima/gc030_uvs/J1316+7226_X\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5789 x 0.835 at -34.26 degrees (North through East)
! Clean map  min=-0.0015131  max=0.051049 Jy/beam
! Writing clean map to FITS file: /scr/pima/gc030_uvs/J1316+7226_X_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.0510491 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.849% of the data.
!  The x-axis pixel size should ideally be below 0.1881 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000233435 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -1.37183 1.37183 2.74366 5.48731 10.9746 21.9492 43.8985 87.797
print "clev=      ", int(3*image_rms*10000)/10000
! clev=       0.0007 
print "peak=      ", int(1000*peak_flux)/1000
! peak=       0.051 
print "dyn_range= ", int(1000*peak_flux/image_rms)/1000
! dyn_range=  218.686 
quit
! Quitting program
! Log file /scr/pima/gc030_uvs/J1316+7226_X_uvs.log closed on Fri Apr 22 08:49:10 2016