! Started logfile: /scr/pima/gc030_uvs/J1148+3154_X_uvs.log on Fri Apr 22 08:47:35 2016
obs /scr/pima/gc030_uvs/J1148+3154_X_uva.fits
! Reading UV FITS file: /scr/pima/gc030_uvs/J1148+3154_X_uva.fits
! AN table 1: 278 integrations on 36 of 36 possible baselines.
! Apparent sampling: 0.582934 visibilities/baseline/integration-bin.
! Found source: J1148+3154
! 
! 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 46672 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/J1148+3154_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 629 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 629 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 629 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 629 telescope corrections were flagged in sub-array 1.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
!  A total of 1034 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 7.
!  A total of 629 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 8.
!  A total of 629 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=1.007955Jy  sigma=14.823715
! Fit after  self-cal, rms=0.932181Jy  sigma=13.806821
! 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 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1833 milli-arcsec
! Estimated beam: bmin=0.4686 mas, bmaj=1.165 mas, bpa=-5.503 degrees
! Estimated noise=0.651473 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 = 0.0510991 Jy
! Component: 100  -  total flux cleaned = 0.0642708 Jy
! Total flux subtracted in 100 components = 0.0642708 Jy
! Clean residual min=-0.005057 max=0.006321 Jy/beam
! Clean residual mean=-0.000002 rms=0.001180 Jy/beam
! Combined flux in latest and established models = 0.0642708 Jy
! Performing phase self-cal
! Adding 4 model components to the UV plane model.
! The established model now contains 4 components and 0.0642708 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=0.116429Jy  sigma=0.770634
! Fit after  self-cal, rms=0.115817Jy  sigma=0.767699
! Inverting map 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1833 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00833387 Jy
! Component: 100  -  total flux cleaned = 0.0136503 Jy
! Total flux subtracted in 100 components = 0.0136503 Jy
! Clean residual min=-0.003793 max=0.004233 Jy/beam
! Clean residual mean=-0.000003 rms=0.000955 Jy/beam
! Combined flux in latest and established models = 0.0779211 Jy
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 7 components and 0.0779211 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=0.114770Jy  sigma=0.756775
! Fit after  self-cal, rms=0.114300Jy  sigma=0.755777
! Inverting map 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1833 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 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1833 milli-arcsec
! Estimated beam: bmin=0.5424 mas, bmaj=1.239 mas, bpa=-5.367 degrees
! Estimated noise=0.314734 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 = 0.00334977 Jy
! Component: 100  -  total flux cleaned = 0.00517428 Jy
! Component: 150  -  total flux cleaned = 0.00631932 Jy
! Component: 200  -  total flux cleaned = 0.00667093 Jy
! Total flux subtracted in 200 components = 0.00667093 Jy
! Clean residual min=-0.003024 max=0.003219 Jy/beam
! Clean residual mean=-0.000029 rms=0.000738 Jy/beam
! Combined flux in latest and established models = 0.084592 Jy
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 19 components and 0.084592 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=0.114119Jy  sigma=0.754073
! Fit after  self-cal, rms=0.113951Jy  sigma=0.753925
! Inverting map 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1833 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5424 x 1.239 at -5.367 degrees (North through East)
! Clean map  min=-0.0027433  max=0.070614 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.
!  A total of 201 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   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.
!  A total of 201 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   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.
!  A total of 201 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.03     EB        1.00     HN        0.88     KP        1.01     
!   LA        0.86     MK        0.90     NL        1.08     PT        1.06     
!   SC        1.05     
! 
! 
! Correcting IF 4.
!  A total of 201 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   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.
!  A total of 9 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   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.
!  A total of 201 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.06     EB        0.99     HN        0.84     KP        0.99     
!   LA        0.91     MK        0.99     NL        1.12     PT        1.07     
!   SC        1.07     
! 
! 
! Correcting IF 8.
!  A total of 201 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.04     EB        0.99     HN        0.84     KP        1.03     
!   LA        0.87     MK        0.87     NL        1.11     PT        1.05     
!   SC        1.08     
! 
! 
! Fit before self-cal, rms=0.113951Jy  sigma=0.753925
! Fit after  self-cal, rms=0.110121Jy  sigma=0.743979
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 milli-arcsec
! Estimated beam: bmin=0.5387 mas, bmaj=1.227 mas, bpa=-5.784 degrees
! Estimated noise=0.332565 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 = 0.00043017 Jy
! Component: 100  -  total flux cleaned = 0.000283946 Jy
! Component: 150  -  total flux cleaned = 0.000251809 Jy
! Component: 200  -  total flux cleaned = 0.000221696 Jy
! Total flux subtracted in 200 components = 0.000221696 Jy
! Clean residual min=-0.002479 max=0.002076 Jy/beam
! Clean residual mean=-0.000022 rms=0.000576 Jy/beam
! Combined flux in latest and established models = 0.0848137 Jy
! Performing phase self-cal
! Adding 5 model components to the UV plane model.
! The established model now contains 22 components and 0.0848137 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=0.110111Jy  sigma=0.743914
! Fit after  self-cal, rms=0.110085Jy  sigma=0.743734
! Inverting map 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 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=0.110085Jy  sigma=0.743734
! Fit after  self-cal, rms=0.109639Jy  sigma=0.742506
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 milli-arcsec
! Estimated beam: bmin=0.5378 mas, bmaj=1.228 mas, bpa=-5.965 degrees
! Estimated noise=0.333138 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00032125 Jy
! Component: 100  -  total flux cleaned = 0.000401844 Jy
! Component: 150  -  total flux cleaned = 0.00044092 Jy
! Component: 200  -  total flux cleaned = 0.000440709 Jy
! Total flux subtracted in 200 components = 0.000440709 Jy
! Clean residual min=-0.002299 max=0.001873 Jy/beam
! Clean residual mean=-0.000016 rms=0.000540 Jy/beam
! Combined flux in latest and established models = 0.0852544 Jy
selfcal
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 29 components and 0.0852544 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=0.109630Jy  sigma=0.742521
! Fit after  self-cal, rms=0.109651Jy  sigma=0.742425
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 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 = 1.84836e-05 Jy
! Component: 100  -  total flux cleaned = -5.65504e-06 Jy
! Component: 150  -  total flux cleaned = -1.64973e-05 Jy
! Component: 200  -  total flux cleaned = -2.71757e-05 Jy
! Total flux subtracted in 200 components = -2.71757e-05 Jy
! Clean residual min=-0.002305 max=0.001882 Jy/beam
! Clean residual mean=-0.000017 rms=0.000545 Jy/beam
! Combined flux in latest and established models = 0.0852272 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 29 components and 0.0852272 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=0.109647Jy  sigma=0.742409
! Fit after  self-cal, rms=0.109652Jy  sigma=0.742384
! Inverting map 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 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=0.109652Jy  sigma=0.742384
! Fit after  self-cal, rms=0.109300Jy  sigma=0.741977
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 milli-arcsec
! Estimated beam: bmin=0.5372 mas, bmaj=1.228 mas, bpa=-6.049 degrees
! Estimated noise=0.332862 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000178591 Jy
! Component: 100  -  total flux cleaned = 0.000191614 Jy
! Component: 150  -  total flux cleaned = 0.000181117 Jy
! Component: 200  -  total flux cleaned = 0.000160839 Jy
! Total flux subtracted in 200 components = 0.000160839 Jy
! Clean residual min=-0.002137 max=0.001833 Jy/beam
! Clean residual mean=-0.000013 rms=0.000520 Jy/beam
! Combined flux in latest and established models = 0.085388 Jy
selfcal
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 29 components and 0.085388 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=0.109296Jy  sigma=0.741975
! Fit after  self-cal, rms=0.109299Jy  sigma=0.741946
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 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 = 4.27654e-05 Jy
! Component: 100  -  total flux cleaned = 2.26362e-05 Jy
! Component: 150  -  total flux cleaned = 3.85572e-06 Jy
! Component: 200  -  total flux cleaned = 3.77679e-06 Jy
! Total flux subtracted in 200 components = 3.77679e-06 Jy
! Clean residual min=-0.002140 max=0.001848 Jy/beam
! Clean residual mean=-0.000013 rms=0.000520 Jy/beam
! Combined flux in latest and established models = 0.0853918 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 29 components and 0.0853918 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=0.109296Jy  sigma=0.741933
! Fit after  self-cal, rms=0.109295Jy  sigma=0.741929
! Inverting map 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 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=0.109295Jy  sigma=0.741929
! Fit after  self-cal, rms=0.109366Jy  sigma=0.741923
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 milli-arcsec
! Estimated beam: bmin=2.43 mas, bmaj=2.497 mas, bpa=53.48 degrees
! Estimated noise=0.692129 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000728088 Jy
! Component: 100  -  total flux cleaned = -0.000804658 Jy
! Component: 150  -  total flux cleaned = -0.00087256 Jy
! Component: 200  -  total flux cleaned = -0.000932466 Jy
! Total flux subtracted in 200 components = -0.000932466 Jy
! Clean residual min=-0.003256 max=0.003547 Jy/beam
! Clean residual mean=-0.000057 rms=0.000992 Jy/beam
! Combined flux in latest and established models = 0.0844593 Jy
selfcal
! Performing phase self-cal
! Adding 4 model components to the UV plane model.
! The established model now contains 29 components and 0.0844593 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=0.109371Jy  sigma=0.742695
! Fit after  self-cal, rms=0.109346Jy  sigma=0.742494
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 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 = -9.81743e-05 Jy
! Component: 100  -  total flux cleaned = -0.000153981 Jy
! Component: 150  -  total flux cleaned = -0.000202483 Jy
! Component: 200  -  total flux cleaned = -0.000245948 Jy
! Total flux subtracted in 200 components = -0.000245948 Jy
! Clean residual min=-0.003321 max=0.003523 Jy/beam
! Clean residual mean=-0.000056 rms=0.000994 Jy/beam
! Combined flux in latest and established models = 0.0842134 Jy
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 30 components and 0.0842134 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=0.109360Jy  sigma=0.743497
! Fit after  self-cal, rms=0.109337Jy  sigma=0.743376
! Inverting map 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 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 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 milli-arcsec
! Estimated beam: bmin=0.537 mas, bmaj=1.227 mas, bpa=-6.099 degrees
! Estimated noise=0.332768 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.537 x 1.227 at -6.099 degrees (North through East)
! Clean map  min=-0.0021659  max=0.069864 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 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 milli-arcsec
! Estimated beam: bmin=0.46 mas, bmaj=1.152 mas, bpa=-6.333 degrees
! Estimated noise=0.689626 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.050088 Jy
! Component: 100  -  total flux cleaned = 0.0641861 Jy
! Component: 150  -  total flux cleaned = 0.0726349 Jy
! Component: 200  -  total flux cleaned = 0.0781615 Jy
! Total flux subtracted in 200 components = 0.0781615 Jy
! Clean residual min=-0.002919 max=0.003710 Jy/beam
! Clean residual mean=-0.000001 rms=0.000741 Jy/beam
! Combined flux in latest and established models = 0.0781614 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 5 model components to the UV plane model.
! The established model now contains 5 components and 0.0781614 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 milli-arcsec
! Estimated beam: bmin=0.537 mas, bmaj=1.227 mas, bpa=-6.099 degrees
! Estimated noise=0.332768 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 = 0.00363561 Jy
! Component: 100  -  total flux cleaned = 0.0055006 Jy
! Component: 150  -  total flux cleaned = 0.00603162 Jy
! Component: 200  -  total flux cleaned = 0.00632634 Jy
! Total flux subtracted in 200 components = 0.00632634 Jy
! Clean residual min=-0.002133 max=0.002179 Jy/beam
! Clean residual mean=-0.000013 rms=0.000547 Jy/beam
! Combined flux in latest and established models = 0.0844878 Jy
! Adding 12 model components to the UV plane model.
! The established model now contains 13 components and 0.0844878 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 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 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 milli-arcsec
! Estimated beam: bmin=2.43 mas, bmaj=2.497 mas, bpa=53.48 degrees
! Estimated noise=0.692129 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000144496 Jy
! Component: 100  -  total flux cleaned = 0.000144138 Jy
! Component: 150  -  total flux cleaned = 0.000101241 Jy
! Component: 200  -  total flux cleaned = 2.25062e-05 Jy
! Total flux subtracted in 200 components = 2.25062e-05 Jy
! Clean residual min=-0.003280 max=0.003782 Jy/beam
! Clean residual mean=-0.000054 rms=0.001014 Jy/beam
! Combined flux in latest and established models = 0.0845103 Jy
flux_cutoff = imstat(rms) * dynam
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  keep
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000100884 Jy
! Component: 100  -  total flux cleaned = -0.000157442 Jy
! Component: 150  -  total flux cleaned = -0.000183882 Jy
! Component: 200  -  total flux cleaned = -0.000230489 Jy
! Total flux subtracted in 200 components = -0.000230489 Jy
! Clean residual min=-0.003325 max=0.003621 Jy/beam
! Clean residual mean=-0.000055 rms=0.001003 Jy/beam
! Combined flux in latest and established models = 0.0842798 Jy
! Adding 8 model components to the UV plane model.
! The established model now contains 17 components and 0.0842798 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 milli-arcsec
! Estimated beam: bmin=0.537 mas, bmaj=1.227 mas, bpa=-6.099 degrees
! Estimated noise=0.332768 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00023321 Jy
! Component: 100  -  total flux cleaned = 0.000495814 Jy
! Component: 150  -  total flux cleaned = 0.000666263 Jy
! Component: 200  -  total flux cleaned = 0.000755286 Jy
! Total flux subtracted in 200 components = 0.000755286 Jy
! Clean residual min=-0.002266 max=0.001972 Jy/beam
! Clean residual mean=-0.000013 rms=0.000538 Jy/beam
! Combined flux in latest and established models = 0.0850351 Jy
selfcal
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 23 components and 0.0850351 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=0.109324Jy  sigma=0.742355
! Fit after  self-cal, rms=0.109336Jy  sigma=0.742182
wmodel /scr/pima/gc030_uvs/J1148+3154_X_map.mod
! Writing 23 model components to file: /scr/pima/gc030_uvs/J1148+3154_X_map.mod
wobs /scr/pima/gc030_uvs/J1148+3154_X_uvs.fits
! Writing UV FITS file: /scr/pima/gc030_uvs/J1148+3154_X_uvs.fits
wwins /scr/pima/gc030_uvs/J1148+3154_X_map.win
! wwins: Wrote 1 windows to /scr/pima/gc030_uvs/J1148+3154_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 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 milli-arcsec
! clean: niter=4096  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000962824 Jy
! Component: 100  -  total flux cleaned = -0.00146595 Jy
! Component: 150  -  total flux cleaned = -0.00177176 Jy
! Component: 200  -  total flux cleaned = -0.00199805 Jy
! Component: 250  -  total flux cleaned = -0.00221455 Jy
! Component: 300  -  total flux cleaned = -0.00224409 Jy
! Component: 350  -  total flux cleaned = -0.00224389 Jy
! Component: 400  -  total flux cleaned = -0.00224364 Jy
! Component: 450  -  total flux cleaned = -0.00221613 Jy
! Component: 500  -  total flux cleaned = -0.0022162 Jy
! Component: 550  -  total flux cleaned = -0.00218998 Jy
! Component: 600  -  total flux cleaned = -0.0021393 Jy
! Component: 650  -  total flux cleaned = -0.00211406 Jy
! Component: 700  -  total flux cleaned = -0.00199296 Jy
! Component: 750  -  total flux cleaned = -0.00196966 Jy
! Component: 800  -  total flux cleaned = -0.00196967 Jy
! Component: 850  -  total flux cleaned = -0.00190108 Jy
! Component: 900  -  total flux cleaned = -0.00187875 Jy
! Component: 950  -  total flux cleaned = -0.00187861 Jy
! Component: 1000  -  total flux cleaned = -0.00189969 Jy
! Component: 1050  -  total flux cleaned = -0.00187793 Jy
! Component: 1100  -  total flux cleaned = -0.00183638 Jy
! Component: 1150  -  total flux cleaned = -0.00187725 Jy
! Component: 1200  -  total flux cleaned = -0.00183699 Jy
! Component: 1250  -  total flux cleaned = -0.00181714 Jy
! Component: 1300  -  total flux cleaned = -0.00181738 Jy
! Component: 1350  -  total flux cleaned = -0.00181749 Jy
! Component: 1400  -  total flux cleaned = -0.00179889 Jy
! Component: 1450  -  total flux cleaned = -0.00179883 Jy
! Component: 1500  -  total flux cleaned = -0.0018355 Jy
! Component: 1550  -  total flux cleaned = -0.00188993 Jy
! Component: 1600  -  total flux cleaned = -0.00185347 Jy
! Component: 1650  -  total flux cleaned = -0.00185308 Jy
! Component: 1700  -  total flux cleaned = -0.00188795 Jy
! Component: 1750  -  total flux cleaned = -0.00188773 Jy
! Component: 1800  -  total flux cleaned = -0.00180264 Jy
! Component: 1850  -  total flux cleaned = -0.00183589 Jy
! Component: 1900  -  total flux cleaned = -0.001836 Jy
! Component: 1950  -  total flux cleaned = -0.00186849 Jy
! Component: 2000  -  total flux cleaned = -0.00185229 Jy
! Component: 2050  -  total flux cleaned = -0.00186829 Jy
! Component: 2100  -  total flux cleaned = -0.00186837 Jy
! Component: 2150  -  total flux cleaned = -0.00185264 Jy
! Component: 2200  -  total flux cleaned = -0.00183722 Jy
! Component: 2250  -  total flux cleaned = -0.00185245 Jy
! Component: 2300  -  total flux cleaned = -0.00188281 Jy
! Component: 2350  -  total flux cleaned = -0.00188273 Jy
! Component: 2400  -  total flux cleaned = -0.00186787 Jy
! Component: 2450  -  total flux cleaned = -0.00188245 Jy
! Component: 2500  -  total flux cleaned = -0.001868 Jy
! Component: 2550  -  total flux cleaned = -0.00185362 Jy
! Component: 2600  -  total flux cleaned = -0.0018679 Jy
! Component: 2650  -  total flux cleaned = -0.00185382 Jy
! Component: 2700  -  total flux cleaned = -0.00186786 Jy
! Component: 2750  -  total flux cleaned = -0.00185381 Jy
! Component: 2800  -  total flux cleaned = -0.00185372 Jy
! Component: 2850  -  total flux cleaned = -0.00182657 Jy
! Component: 2900  -  total flux cleaned = -0.00183999 Jy
! Component: 2950  -  total flux cleaned = -0.0018399 Jy
! Component: 3000  -  total flux cleaned = -0.00182671 Jy
! Component: 3050  -  total flux cleaned = -0.00181361 Jy
! Component: 3100  -  total flux cleaned = -0.00185242 Jy
! Component: 3150  -  total flux cleaned = -0.0018395 Jy
! Component: 3200  -  total flux cleaned = -0.00181395 Jy
! Component: 3250  -  total flux cleaned = -0.0018521 Jy
! Component: 3300  -  total flux cleaned = -0.00183956 Jy
! Component: 3350  -  total flux cleaned = -0.0018645 Jy
! Component: 3400  -  total flux cleaned = -0.00186455 Jy
! Component: 3450  -  total flux cleaned = -0.00190122 Jy
! Component: 3500  -  total flux cleaned = -0.00192544 Jy
! Component: 3550  -  total flux cleaned = -0.00191342 Jy
! Component: 3600  -  total flux cleaned = -0.00194943 Jy
! Component: 3650  -  total flux cleaned = -0.00193752 Jy
! Component: 3700  -  total flux cleaned = -0.00197304 Jy
! Component: 3750  -  total flux cleaned = -0.00204299 Jy
! Component: 3800  -  total flux cleaned = -0.00200824 Jy
! Component: 3850  -  total flux cleaned = -0.00206582 Jy
! Component: 3900  -  total flux cleaned = -0.0020659 Jy
! Component: 3950  -  total flux cleaned = -0.00206595 Jy
! Component: 4000  -  total flux cleaned = -0.00203215 Jy
! Component: 4050  -  total flux cleaned = -0.00204342 Jy
! Total flux subtracted in 4096 components = -0.00205458 Jy
! Clean residual min=-0.000719 max=0.000595 Jy/beam
! Clean residual mean=-0.000004 rms=0.000232 Jy/beam
! Combined flux in latest and established models = 0.0829805 Jy
keep
! Adding 358 model components to the UV plane model.
! The established model now contains 381 components and 0.0829806 Jy
![Exited script file: /home/lpetrov/bin/01_muppet]
wmap "/scr/pima/gc030_uvs/J1148+3154_X\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.537 x 1.227 at -6.099 degrees (North through East)
! Clean map  min=-0.0016546  max=0.070115 Jy/beam
! Writing clean map to FITS file: /scr/pima/gc030_uvs/J1148+3154_X_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.0701154 
invert
! Inverting map 
! Your choice of large map pixels excluded 1.21% of the data.
!  The x-axis pixel size should ideally be below 0.1833 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000231757 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.99161 0.99161 1.98322 3.96644 7.93288 15.8658 31.7315 63.4631
print "clev=      ", int(3*image_rms*10000)/10000
! clev=       0.0006 
print "peak=      ", int(1000*peak_flux)/1000
! peak=       0.07 
print "dyn_range= ", int(1000*peak_flux/image_rms)/1000
! dyn_range=  302.538 
quit
! Quitting program
! Log file /scr/pima/gc030_uvs/J1148+3154_X_uvs.log closed on Fri Apr 22 08:47:40 2016