! Started logfile: /scr/pima/gc030_uvs/J1520+7225_X_uvs.log on Fri Apr 22 08:50:02 2016
obs /scr/pima/gc030_uvs/J1520+7225_X_uva.fits
! Reading UV FITS file: /scr/pima/gc030_uvs/J1520+7225_X_uva.fits
! AN table 1: 70 integrations on 36 of 36 possible baselines.
! AN table 2: 140 integrations on 36 of 36 possible baselines.
! AN table 3: 140 integrations on 36 of 36 possible baselines.
! Apparent sampling: 0.760079 visibilities/baseline/integration-bin.
! Found source: J1520+7225
! 
! 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 76616 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/J1520+7225_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 5 telescope corrections were flagged in sub-array 1.
!  A total of 22 telescope corrections were flagged in sub-array 2.
!  A total of 80 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 5 telescope corrections were flagged in sub-array 1.
!  A total of 22 telescope corrections were flagged in sub-array 2.
!  A total of 80 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 5 telescope corrections were flagged in sub-array 1.
!  A total of 28 telescope corrections were flagged in sub-array 2.
!  A total of 80 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 5 telescope corrections were flagged in sub-array 1.
!  A total of 28 telescope corrections were flagged in sub-array 2.
!  A total of 80 telescope corrections were flagged in sub-array 3.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
!  A total of 75 telescope corrections were flagged in sub-array 1.
!  A total of 160 telescope corrections were flagged in sub-array 2.
!  A total of 220 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 7.
!  A total of 5 telescope corrections were flagged in sub-array 1.
!  A total of 22 telescope corrections were flagged in sub-array 2.
!  A total of 80 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 8.
!  A total of 5 telescope corrections were flagged in sub-array 1.
!  A total of 22 telescope corrections were flagged in sub-array 2.
!  A total of 80 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=1.006806Jy  sigma=15.927912
! Fit after  self-cal, rms=0.960650Jy  sigma=15.303632
! 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 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 milli-arcsec
! Estimated beam: bmin=0.475 mas, bmaj=0.6849 mas, bpa=24.24 degrees
! Estimated noise=0.464095 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 = 0.0326982 Jy
! Component: 100  -  total flux cleaned = 0.0411621 Jy
! Total flux subtracted in 100 components = 0.0411621 Jy
! Clean residual min=-0.003584 max=0.004056 Jy/beam
! Clean residual mean=0.000000 rms=0.000832 Jy/beam
! Combined flux in latest and established models = 0.0411621 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 7 components and 0.0411621 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=0.097852Jy  sigma=0.815608
! Fit after  self-cal, rms=0.096449Jy  sigma=0.799006
! Inverting map 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00615709 Jy
! Component: 100  -  total flux cleaned = 0.0103782 Jy
! Total flux subtracted in 100 components = 0.0103782 Jy
! Clean residual min=-0.003259 max=0.003316 Jy/beam
! Clean residual mean=-0.000001 rms=0.000782 Jy/beam
! Combined flux in latest and established models = 0.0515403 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 13 components and 0.0515403 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=0.096044Jy  sigma=0.794139
! Fit after  self-cal, rms=0.095605Jy  sigma=0.793591
! Inverting map 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 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 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 milli-arcsec
! Estimated beam: bmin=0.5736 mas, bmaj=0.8115 mas, bpa=21.75 degrees
! Estimated noise=0.22531 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (-0.6, 2).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00280644 Jy
! Component: 100  -  total flux cleaned = 0.00385675 Jy
! Component: 150  -  total flux cleaned = 0.00454541 Jy
! Component: 200  -  total flux cleaned = 0.00486178 Jy
! Total flux subtracted in 200 components = 0.00486178 Jy
! Clean residual min=-0.002483 max=0.002618 Jy/beam
! Clean residual mean=-0.000002 rms=0.000548 Jy/beam
! Combined flux in latest and established models = 0.0564021 Jy
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 28 components and 0.0564021 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=0.095417Jy  sigma=0.790042
! Fit after  self-cal, rms=0.095174Jy  sigma=0.789253
! Inverting map 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5736 x 0.8115 at 21.75 degrees (North through East)
! Clean map  min=-0.0026833  max=0.045164 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*    
! 
!  A total of 3 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*    
! 
!  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*    
! 
!  A total of 3 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*    
! 
!  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*    
! 
!  A total of 3 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*    
! 
!  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*    
! 
!  A total of 3 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*    
! 
!  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 3 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*    
! 
!  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*    
! 
!  A total of 3 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*    
! 
!  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*    
! 
!  A total of 3 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*    
! 
!  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=0.095174Jy  sigma=0.789253
! Fit after  self-cal, rms=0.095184Jy  sigma=0.789238
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 milli-arcsec
! Estimated beam: bmin=0.5736 mas, bmaj=0.8117 mas, bpa=21.82 degrees
! Estimated noise=0.225416 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 = 0.00137284 Jy
! Component: 100  -  total flux cleaned = 0.00199694 Jy
! Component: 150  -  total flux cleaned = 0.00222555 Jy
! Component: 200  -  total flux cleaned = 0.00246901 Jy
! Total flux subtracted in 200 components = 0.00246901 Jy
! Clean residual min=-0.002371 max=0.002408 Jy/beam
! Clean residual mean=-0.000003 rms=0.000519 Jy/beam
! Combined flux in latest and established models = 0.0588711 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 29 components and 0.0588711 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=0.095096Jy  sigma=0.787579
! Fit after  self-cal, rms=0.094946Jy  sigma=0.787243
! Inverting map 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 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=0.094946Jy  sigma=0.787243
! Fit after  self-cal, rms=0.095282Jy  sigma=0.786270
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 milli-arcsec
! Estimated beam: bmin=0.5771 mas, bmaj=0.8087 mas, bpa=21.12 degrees
! Estimated noise=0.227995 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00109551 Jy
! Component: 100  -  total flux cleaned = 0.0013374 Jy
! Component: 150  -  total flux cleaned = 0.00137795 Jy
! Component: 200  -  total flux cleaned = 0.00145044 Jy
! Total flux subtracted in 200 components = 0.00145044 Jy
! Clean residual min=-0.002383 max=0.002120 Jy/beam
! Clean residual mean=-0.000003 rms=0.000485 Jy/beam
! Combined flux in latest and established models = 0.0603215 Jy
selfcal
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 36 components and 0.0603215 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=0.095236Jy  sigma=0.785456
! Fit after  self-cal, rms=0.095127Jy  sigma=0.785152
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 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 = 0.000574778 Jy
! Component: 100  -  total flux cleaned = 0.000653893 Jy
! Component: 150  -  total flux cleaned = 0.000687239 Jy
! Component: 200  -  total flux cleaned = 0.000751496 Jy
! Total flux subtracted in 200 components = 0.000751496 Jy
! Clean residual min=-0.002330 max=0.002087 Jy/beam
! Clean residual mean=-0.000004 rms=0.000478 Jy/beam
! Combined flux in latest and established models = 0.061073 Jy
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 40 components and 0.061073 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=0.095097Jy  sigma=0.784634
! Fit after  self-cal, rms=0.095024Jy  sigma=0.784498
! Inverting map 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 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=0.095024Jy  sigma=0.784498
! Fit after  self-cal, rms=0.095573Jy  sigma=0.784193
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 milli-arcsec
! Estimated beam: bmin=0.578 mas, bmaj=0.808 mas, bpa=20.97 degrees
! Estimated noise=0.229259 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0003479 Jy
! Component: 100  -  total flux cleaned = 0.000382262 Jy
! Component: 150  -  total flux cleaned = 0.000411186 Jy
! Component: 200  -  total flux cleaned = 0.000465731 Jy
! Total flux subtracted in 200 components = 0.000465731 Jy
! Clean residual min=-0.002294 max=0.001921 Jy/beam
! Clean residual mean=-0.000004 rms=0.000461 Jy/beam
! Combined flux in latest and established models = 0.0615388 Jy
selfcal
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 40 components and 0.0615388 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=0.095552Jy  sigma=0.783845
! Fit after  self-cal, rms=0.095500Jy  sigma=0.783677
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 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 = 0.000214523 Jy
! Component: 100  -  total flux cleaned = 0.000213644 Jy
! Component: 150  -  total flux cleaned = 0.000238638 Jy
! Component: 200  -  total flux cleaned = 0.000286046 Jy
! Total flux subtracted in 200 components = 0.000286046 Jy
! Clean residual min=-0.002288 max=0.001905 Jy/beam
! Clean residual mean=-0.000004 rms=0.000460 Jy/beam
! Combined flux in latest and established models = 0.0618248 Jy
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 42 components and 0.0618248 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=0.095486Jy  sigma=0.783452
! Fit after  self-cal, rms=0.095445Jy  sigma=0.783404
! Inverting map 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 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=0.095445Jy  sigma=0.783404
! Fit after  self-cal, rms=0.095789Jy  sigma=0.783381
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 milli-arcsec
! Estimated beam: bmin=2.125 mas, bmaj=2.914 mas, bpa=48.92 degrees
! Estimated noise=0.462748 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000192821 Jy
! Component: 100  -  total flux cleaned = -0.000377707 Jy
! Component: 150  -  total flux cleaned = -0.000514368 Jy
! Component: 200  -  total flux cleaned = -0.0006155 Jy
! Total flux subtracted in 200 components = -0.0006155 Jy
! Clean residual min=-0.003857 max=0.003585 Jy/beam
! Clean residual mean=-0.000018 rms=0.001002 Jy/beam
! Combined flux in latest and established models = 0.0612093 Jy
selfcal
! Performing phase self-cal
! Adding 3 model components to the UV plane model.
! The established model now contains 44 components and 0.0612093 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=0.095787Jy  sigma=0.784111
! Fit after  self-cal, rms=0.095804Jy  sigma=0.783744
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 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 = 0.000135663 Jy
! Component: 100  -  total flux cleaned = 1.7408e-05 Jy
! Component: 150  -  total flux cleaned = -7.0002e-05 Jy
! Component: 200  -  total flux cleaned = -0.000134672 Jy
! Total flux subtracted in 200 components = -0.000134672 Jy
! Clean residual min=-0.003903 max=0.003696 Jy/beam
! Clean residual mean=-0.000018 rms=0.001006 Jy/beam
! Combined flux in latest and established models = 0.0610746 Jy
! Performing phase self-cal
! Adding 3 model components to the UV plane model.
! The established model now contains 44 components and 0.0610746 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=0.095812Jy  sigma=0.784716
! Fit after  self-cal, rms=0.095805Jy  sigma=0.784513
! Inverting map 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 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 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 milli-arcsec
! Estimated beam: bmin=0.5781 mas, bmaj=0.8074 mas, bpa=20.95 degrees
! Estimated noise=0.22972 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5781 x 0.8074 at 20.95 degrees (North through East)
! Clean map  min=-0.0059196  max=0.045956 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 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 milli-arcsec
! Estimated beam: bmin=0.4778 mas, bmaj=0.6805 mas, bpa=23.64 degrees
! Estimated noise=0.474341 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0343621 Jy
! Component: 100  -  total flux cleaned = 0.0445509 Jy
! Component: 150  -  total flux cleaned = 0.0492333 Jy
! Component: 200  -  total flux cleaned = 0.0531648 Jy
! Total flux subtracted in 200 components = 0.0531648 Jy
! Clean residual min=-0.003540 max=0.003413 Jy/beam
! Clean residual mean=-0.000000 rms=0.000816 Jy/beam
! Combined flux in latest and established models = 0.0531648 Jy
uvw 0,-1
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Adding 19 model components to the UV plane model.
! The established model now contains 19 components and 0.0531648 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 milli-arcsec
! Estimated beam: bmin=0.5781 mas, bmaj=0.8074 mas, bpa=20.95 degrees
! Estimated noise=0.22972 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 = 0.00419468 Jy
! Component: 100  -  total flux cleaned = 0.00557807 Jy
! Component: 150  -  total flux cleaned = 0.0062734 Jy
! Component: 200  -  total flux cleaned = 0.00685304 Jy
! Total flux subtracted in 200 components = 0.00685304 Jy
! Clean residual min=-0.002752 max=0.002311 Jy/beam
! Clean residual mean=-0.000004 rms=0.000515 Jy/beam
! Combined flux in latest and established models = 0.0600178 Jy
! Adding 16 model components to the UV plane model.
! The established model now contains 33 components and 0.0600178 Jy
! Inverting map 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 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 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 milli-arcsec
! Estimated beam: bmin=2.125 mas, bmaj=2.914 mas, bpa=48.92 degrees
! Estimated noise=0.462748 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00148914 Jy
! Component: 100  -  total flux cleaned = 0.00150066 Jy
! Component: 150  -  total flux cleaned = 0.00146928 Jy
! Component: 200  -  total flux cleaned = 0.00150228 Jy
! Total flux subtracted in 200 components = 0.00150228 Jy
! Clean residual min=-0.003886 max=0.003894 Jy/beam
! Clean residual mean=-0.000019 rms=0.001014 Jy/beam
! Combined flux in latest and established models = 0.0615201 Jy
flux_cutoff = imstat(rms) * dynam
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  keep
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 2.7351e-07 Jy
! Component: 100  -  total flux cleaned = -2.03509e-05 Jy
! Component: 150  -  total flux cleaned = -5.95615e-05 Jy
! Component: 200  -  total flux cleaned = -9.5032e-05 Jy
! Total flux subtracted in 200 components = -9.5032e-05 Jy
! Clean residual min=-0.003930 max=0.003833 Jy/beam
! Clean residual mean=-0.000019 rms=0.001010 Jy/beam
! Combined flux in latest and established models = 0.0614251 Jy
! Adding 9 model components to the UV plane model.
! The established model now contains 39 components and 0.0614251 Jy
! Inverting map 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 milli-arcsec
! Estimated beam: bmin=0.5781 mas, bmaj=0.8074 mas, bpa=20.95 degrees
! Estimated noise=0.22972 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000510065 Jy
! Component: 100  -  total flux cleaned = -0.000439311 Jy
! Component: 150  -  total flux cleaned = -0.000199135 Jy
! Component: 200  -  total flux cleaned = 4.37865e-05 Jy
! Total flux subtracted in 200 components = 4.37865e-05 Jy
! Clean residual min=-0.002482 max=0.002136 Jy/beam
! Clean residual mean=-0.000004 rms=0.000481 Jy/beam
! Combined flux in latest and established models = 0.0614689 Jy
selfcal
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 45 components and 0.0614689 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=0.095831Jy  sigma=0.784732
! Fit after  self-cal, rms=0.095868Jy  sigma=0.784441
wmodel /scr/pima/gc030_uvs/J1520+7225_X_map.mod
! Writing 45 model components to file: /scr/pima/gc030_uvs/J1520+7225_X_map.mod
wobs /scr/pima/gc030_uvs/J1520+7225_X_uvs.fits
! Writing UV FITS file: /scr/pima/gc030_uvs/J1520+7225_X_uvs.fits
wwins /scr/pima/gc030_uvs/J1520+7225_X_map.win
! wwins: Wrote 2 windows to /scr/pima/gc030_uvs/J1520+7225_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 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 milli-arcsec
! clean: niter=4096  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00102299 Jy
! Component: 100  -  total flux cleaned = -0.0014903 Jy
! Component: 150  -  total flux cleaned = -0.00178179 Jy
! Component: 200  -  total flux cleaned = -0.00195638 Jy
! Component: 250  -  total flux cleaned = -0.00215519 Jy
! Component: 300  -  total flux cleaned = -0.00237857 Jy
! Component: 350  -  total flux cleaned = -0.00253344 Jy
! Component: 400  -  total flux cleaned = -0.0026531 Jy
! Component: 450  -  total flux cleaned = -0.00282797 Jy
! Component: 500  -  total flux cleaned = -0.00302703 Jy
! Component: 550  -  total flux cleaned = -0.0031941 Jy
! Component: 600  -  total flux cleaned = -0.00338469 Jy
! Component: 650  -  total flux cleaned = -0.00357127 Jy
! Component: 700  -  total flux cleaned = -0.00383207 Jy
! Component: 750  -  total flux cleaned = -0.00403676 Jy
! Component: 800  -  total flux cleaned = -0.00418758 Jy
! Component: 850  -  total flux cleaned = -0.00438511 Jy
! Component: 900  -  total flux cleaned = -0.00453054 Jy
! Component: 950  -  total flux cleaned = -0.0046736 Jy
! Component: 1000  -  total flux cleaned = -0.00483775 Jy
! Component: 1050  -  total flux cleaned = -0.00492959 Jy
! Component: 1100  -  total flux cleaned = -0.00506583 Jy
! Component: 1150  -  total flux cleaned = -0.00519967 Jy
! Component: 1200  -  total flux cleaned = -0.00539702 Jy
! Component: 1250  -  total flux cleaned = -0.00554814 Jy
! Component: 1300  -  total flux cleaned = -0.00567589 Jy
! Component: 1350  -  total flux cleaned = -0.0057807 Jy
! Component: 1400  -  total flux cleaned = -0.00600818 Jy
! Component: 1450  -  total flux cleaned = -0.00610994 Jy
! Component: 1500  -  total flux cleaned = -0.00627097 Jy
! Component: 1550  -  total flux cleaned = -0.0063306 Jy
! Component: 1600  -  total flux cleaned = -0.00642912 Jy
! Component: 1650  -  total flux cleaned = -0.00656469 Jy
! Component: 1700  -  total flux cleaned = -0.00671732 Jy
! Component: 1750  -  total flux cleaned = -0.00683032 Jy
! Component: 1800  -  total flux cleaned = -0.00688631 Jy
! Component: 1850  -  total flux cleaned = -0.00703328 Jy
! Component: 1900  -  total flux cleaned = -0.00706972 Jy
! Component: 1950  -  total flux cleaned = -0.00714172 Jy
! Component: 2000  -  total flux cleaned = -0.00733648 Jy
! Component: 2050  -  total flux cleaned = -0.00737149 Jy
! Component: 2100  -  total flux cleaned = -0.00742356 Jy
! Component: 2150  -  total flux cleaned = -0.00756074 Jy
! Component: 2200  -  total flux cleaned = -0.00764546 Jy
! Component: 2250  -  total flux cleaned = -0.00771234 Jy
! Component: 2300  -  total flux cleaned = -0.00779526 Jy
! Component: 2350  -  total flux cleaned = -0.00787729 Jy
! Component: 2400  -  total flux cleaned = -0.0079259 Jy
! Component: 2450  -  total flux cleaned = -0.00803829 Jy
! Component: 2500  -  total flux cleaned = -0.00805387 Jy
! Component: 2550  -  total flux cleaned = -0.0081483 Jy
! Component: 2600  -  total flux cleaned = -0.00819491 Jy
! Component: 2650  -  total flux cleaned = -0.00824134 Jy
! Component: 2700  -  total flux cleaned = -0.00833303 Jy
! Component: 2750  -  total flux cleaned = -0.00837831 Jy
! Component: 2800  -  total flux cleaned = -0.00845317 Jy
! Component: 2850  -  total flux cleaned = -0.0085273 Jy
! Component: 2900  -  total flux cleaned = -0.00854205 Jy
! Component: 2950  -  total flux cleaned = -0.00862948 Jy
! Component: 3000  -  total flux cleaned = -0.00873066 Jy
! Component: 3050  -  total flux cleaned = -0.00875918 Jy
! Component: 3100  -  total flux cleaned = -0.00885846 Jy
! Component: 3150  -  total flux cleaned = -0.00897071 Jy
! Component: 3200  -  total flux cleaned = -0.00904034 Jy
! Component: 3250  -  total flux cleaned = -0.00916439 Jy
! Component: 3300  -  total flux cleaned = -0.00924637 Jy
! Component: 3350  -  total flux cleaned = -0.00931412 Jy
! Component: 3400  -  total flux cleaned = -0.00940804 Jy
! Component: 3450  -  total flux cleaned = -0.00951464 Jy
! Component: 3500  -  total flux cleaned = -0.00962014 Jy
! Component: 3550  -  total flux cleaned = -0.00965935 Jy
! Component: 3600  -  total flux cleaned = -0.00975024 Jy
! Component: 3650  -  total flux cleaned = -0.00985307 Jy
! Component: 3700  -  total flux cleaned = -0.00995506 Jy
! Component: 3750  -  total flux cleaned = -0.0100058 Jy
! Component: 3800  -  total flux cleaned = -0.0101187 Jy
! Component: 3850  -  total flux cleaned = -0.0101685 Jy
! Component: 3900  -  total flux cleaned = -0.0102548 Jy
! Component: 3950  -  total flux cleaned = -0.0103283 Jy
! Component: 4000  -  total flux cleaned = -0.0104616 Jy
! Component: 4050  -  total flux cleaned = -0.0105458 Jy
! Total flux subtracted in 4096 components = -0.0105697 Jy
! Clean residual min=-0.000690 max=0.000685 Jy/beam
! Clean residual mean=-0.000003 rms=0.000201 Jy/beam
! Combined flux in latest and established models = 0.0508991 Jy
keep
! Adding 349 model components to the UV plane model.
! The established model now contains 394 components and 0.0508991 Jy
![Exited script file: /home/lpetrov/bin/01_muppet]
wmap "/scr/pima/gc030_uvs/J1520+7225_X\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5781 x 0.8074 at 20.95 degrees (North through East)
! Clean map  min=-0.0049217  max=0.045357 Jy/beam
! Writing clean map to FITS file: /scr/pima/gc030_uvs/J1520+7225_X_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.0453568 
invert
! Inverting map 
! Your choice of large map pixels excluded 2.27% of the data.
!  The x-axis pixel size should ideally be below 0.1827 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1924 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000201013 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -1.32955 1.32955 2.65909 5.31819 10.6364 21.2728 42.5455 85.091
print "clev=      ", int(3*image_rms*10000)/10000
! clev=       0.0006 
print "peak=      ", int(1000*peak_flux)/1000
! peak=       0.045 
print "dyn_range= ", int(1000*peak_flux/image_rms)/1000
! dyn_range=  225.64 
quit
! Quitting program
! Log file /scr/pima/gc030_uvs/J1520+7225_X_uvs.log closed on Fri Apr 22 08:50:09 2016