! Started logfile: /scr/pima/gc030_uvs/J1730+3714_X_uvs.log on Fri Apr 22 08:51:51 2016
obs /scr/pima/gc030_uvs/J1730+3714_X_uva.fits
! Reading UV FITS file: /scr/pima/gc030_uvs/J1730+3714_X_uva.fits
! AN table 1: 70 integrations on 21 of 21 possible baselines.
! AN table 2: 208 integrations on 36 of 36 possible baselines.
! Apparent sampling: 0.582273 visibilities/baseline/integration-bin.
! Found source: J1730+3714
! 
! 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 41728 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/J1730+3714_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 2 telescope corrections were flagged in sub-array 1.
!  A total of 513 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 2.
!  A total of 2 telescope corrections were flagged in sub-array 1.
!  A total of 513 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 3.
!  A total of 2 telescope corrections were flagged in sub-array 1.
!  A total of 513 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 4.
!  A total of 2 telescope corrections were flagged in sub-array 1.
!  A total of 513 telescope corrections were flagged in sub-array 2.
! 
! Not correcting unselected IF 5.
! 
! Correcting IF 6.
!  A total of 72 telescope corrections were flagged in sub-array 1.
!  A total of 583 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 7.
!  A total of 2 telescope corrections were flagged in sub-array 1.
!  A total of 513 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 8.
!  A total of 2 telescope corrections were flagged in sub-array 1.
!  A total of 513 telescope corrections were flagged in sub-array 2.
! 
! Fit before self-cal, rms=1.002681Jy  sigma=18.344686
! Fit after  self-cal, rms=0.957486Jy  sigma=17.735037
! 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 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 milli-arcsec
! Estimated beam: bmin=0.4712 mas, bmaj=1.082 mas, bpa=-13.22 degrees
! Estimated noise=0.671892 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 = 0.0270165 Jy
! Component: 100  -  total flux cleaned = 0.0361354 Jy
! Total flux subtracted in 100 components = 0.0361354 Jy
! Clean residual min=-0.003412 max=0.005273 Jy/beam
! Clean residual mean=-0.000004 rms=0.001002 Jy/beam
! Combined flux in latest and established models = 0.0361354 Jy
! Performing phase self-cal
! Adding 4 model components to the UV plane model.
! The established model now contains 4 components and 0.0361354 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=0.094875Jy  sigma=0.842571
! Fit after  self-cal, rms=0.093142Jy  sigma=0.824466
! Inverting map 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00807974 Jy
! Component: 100  -  total flux cleaned = 0.0131555 Jy
! Total flux subtracted in 100 components = 0.0131555 Jy
! Clean residual min=-0.003639 max=0.004789 Jy/beam
! Clean residual mean=-0.000002 rms=0.000958 Jy/beam
! Combined flux in latest and established models = 0.0492909 Jy
! Performing phase self-cal
! Adding 5 model components to the UV plane model.
! The established model now contains 6 components and 0.0492909 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=0.091421Jy  sigma=0.812208
! Fit after  self-cal, rms=0.090558Jy  sigma=0.810065
! Inverting map 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 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 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 milli-arcsec
! Estimated beam: bmin=0.563 mas, bmaj=1.164 mas, bpa=-10.75 degrees
! Estimated noise=0.278635 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 (-1.8, 0.4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00715044 Jy
! Component: 100  -  total flux cleaned = 0.0112789 Jy
! Component: 150  -  total flux cleaned = 0.0132206 Jy
! Component: 200  -  total flux cleaned = 0.0138548 Jy
! Total flux subtracted in 200 components = 0.0138548 Jy
! Clean residual min=-0.003177 max=0.003653 Jy/beam
! Clean residual mean=-0.000000 rms=0.000831 Jy/beam
! Combined flux in latest and established models = 0.0631457 Jy
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 20 components and 0.0631457 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=0.089650Jy  sigma=0.801571
! Fit after  self-cal, rms=0.088724Jy  sigma=0.799025
! Inverting map 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.563 x 1.164 at -10.75 degrees (North through East)
! Clean map  min=-0.003109  max=0.043182 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*    
!   NL        1.00*    OV        1.00*    PT        1.00*    
! 
!  A total of 12 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*    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*    
!   NL        1.00*    OV        1.00*    PT        1.00*    
! 
!  A total of 12 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*    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*    
!   NL        1.00*    OV        1.00*    PT        1.00*    
! 
!  A total of 12 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*    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*    
!   NL        1.00*    OV        1.00*    PT        1.00*    
! 
!  A total of 12 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*    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*    
!   NL        1.00*    OV        1.00*    PT        1.00*    
! 
!  A total of 12 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*    PT        1.00*    
!   SC        1.00*    
! 
! 
! Correcting IF 7.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.06     HN        0.84     KP        1.02     LA        0.99     
!   NL        1.15     OV        0.96     PT        0.91     
! 
!  A total of 12 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*    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*    
!   NL        1.00*    OV        1.00*    PT        1.00*    
! 
!  A total of 12 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*    PT        1.00*    
!   SC        1.00*    
! 
! 
! Fit before self-cal, rms=0.088724Jy  sigma=0.799025
! Fit after  self-cal, rms=0.088515Jy  sigma=0.798028
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 milli-arcsec
! Estimated beam: bmin=0.5634 mas, bmaj=1.165 mas, bpa=-10.77 degrees
! Estimated noise=0.279098 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 = 0.00340952 Jy
! Component: 100  -  total flux cleaned = 0.00438931 Jy
! Component: 150  -  total flux cleaned = 0.00475345 Jy
! Component: 200  -  total flux cleaned = 0.00514569 Jy
! Total flux subtracted in 200 components = 0.00514569 Jy
! Clean residual min=-0.003027 max=0.003281 Jy/beam
! Clean residual mean=0.000002 rms=0.000757 Jy/beam
! Combined flux in latest and established models = 0.0682914 Jy
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 25 components and 0.0682914 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=0.088267Jy  sigma=0.795286
! Fit after  self-cal, rms=0.087938Jy  sigma=0.794649
! Inverting map 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 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=0.087938Jy  sigma=0.794649
! Fit after  self-cal, rms=0.087571Jy  sigma=0.794167
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 milli-arcsec
! Estimated beam: bmin=0.5645 mas, bmaj=1.168 mas, bpa=-10.62 degrees
! Estimated noise=0.280558 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00193002 Jy
! Component: 100  -  total flux cleaned = 0.00236919 Jy
! Component: 150  -  total flux cleaned = 0.00269813 Jy
! Component: 200  -  total flux cleaned = 0.00304078 Jy
! Total flux subtracted in 200 components = 0.00304078 Jy
! Clean residual min=-0.002976 max=0.002907 Jy/beam
! Clean residual mean=0.000003 rms=0.000715 Jy/beam
! Combined flux in latest and established models = 0.0713322 Jy
selfcal
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 30 components and 0.0713322 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=0.087452Jy  sigma=0.793084
! Fit after  self-cal, rms=0.087273Jy  sigma=0.792734
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 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 = 0.000980254 Jy
! Component: 100  -  total flux cleaned = 0.00131582 Jy
! Component: 150  -  total flux cleaned = 0.00152943 Jy
! Component: 200  -  total flux cleaned = 0.00164842 Jy
! Total flux subtracted in 200 components = 0.00164842 Jy
! Clean residual min=-0.002999 max=0.002848 Jy/beam
! Clean residual mean=0.000004 rms=0.000710 Jy/beam
! Combined flux in latest and established models = 0.0729806 Jy
! Performing phase self-cal
! Adding 21 model components to the UV plane model.
! The established model now contains 33 components and 0.0729806 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=0.087202Jy  sigma=0.792104
! Fit after  self-cal, rms=0.087114Jy  sigma=0.791979
! Inverting map 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 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=0.087114Jy  sigma=0.791979
! Fit after  self-cal, rms=0.087517Jy  sigma=0.791691
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 milli-arcsec
! Estimated beam: bmin=0.5635 mas, bmaj=1.164 mas, bpa=-10.62 degrees
! Estimated noise=0.281619 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00108577 Jy
! Component: 100  -  total flux cleaned = 0.00140016 Jy
! Component: 150  -  total flux cleaned = 0.001506 Jy
! Component: 200  -  total flux cleaned = 0.00157198 Jy
! Total flux subtracted in 200 components = 0.00157198 Jy
! Clean residual min=-0.002907 max=0.002715 Jy/beam
! Clean residual mean=0.000004 rms=0.000695 Jy/beam
! Combined flux in latest and established models = 0.0745526 Jy
selfcal
! Performing phase self-cal
! Adding 20 model components to the UV plane model.
! The established model now contains 36 components and 0.0745526 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=0.087474Jy  sigma=0.791275
! Fit after  self-cal, rms=0.087429Jy  sigma=0.791141
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 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 = 0.000502635 Jy
! Component: 100  -  total flux cleaned = 0.000533446 Jy
! Component: 150  -  total flux cleaned = 0.00056295 Jy
! Component: 200  -  total flux cleaned = 0.000646924 Jy
! Total flux subtracted in 200 components = 0.000646924 Jy
! Clean residual min=-0.002898 max=0.002681 Jy/beam
! Clean residual mean=0.000005 rms=0.000692 Jy/beam
! Combined flux in latest and established models = 0.0751995 Jy
! Performing phase self-cal
! Adding 20 model components to the UV plane model.
! The established model now contains 38 components and 0.0751995 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=0.087399Jy  sigma=0.790841
! Fit after  self-cal, rms=0.087358Jy  sigma=0.790754
! Inverting map 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 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=0.087358Jy  sigma=0.790754
! Fit after  self-cal, rms=0.087554Jy  sigma=0.790711
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 milli-arcsec
! Estimated beam: bmin=2.347 mas, bmaj=2.708 mas, bpa=15.93 degrees
! Estimated noise=0.595858 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000777614 Jy
! Component: 100  -  total flux cleaned = 0.000694056 Jy
! Component: 150  -  total flux cleaned = 0.00064923 Jy
! Component: 200  -  total flux cleaned = 0.000611172 Jy
! Total flux subtracted in 200 components = 0.000611172 Jy
! Clean residual min=-0.004825 max=0.004794 Jy/beam
! Clean residual mean=0.000018 rms=0.001317 Jy/beam
! Combined flux in latest and established models = 0.0758107 Jy
selfcal
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 45 components and 0.0758107 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=0.087558Jy  sigma=0.791242
! Fit after  self-cal, rms=0.087524Jy  sigma=0.790766
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 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 = 0.000438796 Jy
! Component: 100  -  total flux cleaned = 0.00039497 Jy
! Component: 150  -  total flux cleaned = 0.000339041 Jy
! Component: 200  -  total flux cleaned = 0.000289863 Jy
! Total flux subtracted in 200 components = 0.000289863 Jy
! Clean residual min=-0.004815 max=0.004800 Jy/beam
! Clean residual mean=0.000017 rms=0.001316 Jy/beam
! Combined flux in latest and established models = 0.0761006 Jy
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 49 components and 0.0761006 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=0.087531Jy  sigma=0.791301
! Fit after  self-cal, rms=0.087537Jy  sigma=0.791078
! Inverting map 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 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 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 milli-arcsec
! Estimated beam: bmin=0.5631 mas, bmaj=1.161 mas, bpa=-10.65 degrees
! Estimated noise=0.281691 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5631 x 1.161 at -10.65 degrees (North through East)
! Clean map  min=-0.0033188  max=0.043034 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 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 milli-arcsec
! Estimated beam: bmin=0.4723 mas, bmaj=1.078 mas, bpa=-13.12 degrees
! Estimated noise=0.679147 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0293045 Jy
! Component: 100  -  total flux cleaned = 0.042522 Jy
! Component: 150  -  total flux cleaned = 0.0514729 Jy
! Component: 200  -  total flux cleaned = 0.0579859 Jy
! Total flux subtracted in 200 components = 0.0579859 Jy
! Clean residual min=-0.003917 max=0.004765 Jy/beam
! Clean residual mean=-0.000002 rms=0.000982 Jy/beam
! Combined flux in latest and established models = 0.057986 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 11 model components to the UV plane model.
! The established model now contains 11 components and 0.057986 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 milli-arcsec
! Estimated beam: bmin=0.5631 mas, bmaj=1.161 mas, bpa=-10.65 degrees
! Estimated noise=0.281691 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  keep
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (-0.6, 0).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0071399 Jy
! Component: 100  -  total flux cleaned = 0.0117882 Jy
! Component: 150  -  total flux cleaned = 0.0146097 Jy
! Component: 200  -  total flux cleaned = 0.0154631 Jy
! Total flux subtracted in 200 components = 0.0154631 Jy
! Clean residual min=-0.003021 max=0.003338 Jy/beam
! Clean residual mean=0.000003 rms=0.000753 Jy/beam
! Combined flux in latest and established models = 0.0734491 Jy
! Adding 19 model components to the UV plane model.
! The established model now contains 22 components and 0.0734491 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 milli-arcsec
! Added new window around map position (-9.4, -4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00298393 Jy
! Component: 100  -  total flux cleaned = 0.00411387 Jy
! Component: 150  -  total flux cleaned = 0.00458465 Jy
! Component: 200  -  total flux cleaned = 0.00515272 Jy
! Total flux subtracted in 200 components = 0.00515272 Jy
! Clean residual min=-0.002671 max=0.002783 Jy/beam
! Clean residual mean=0.000004 rms=0.000690 Jy/beam
! Combined flux in latest and established models = 0.0786018 Jy
! Adding 22 model components to the UV plane model.
! The established model now contains 35 components and 0.0786018 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 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 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 milli-arcsec
! Estimated beam: bmin=2.347 mas, bmaj=2.708 mas, bpa=15.93 degrees
! Estimated noise=0.595858 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00158785 Jy
! Component: 100  -  total flux cleaned = 0.00206534 Jy
! Component: 150  -  total flux cleaned = 0.0022557 Jy
! Component: 200  -  total flux cleaned = 0.00236474 Jy
! Total flux subtracted in 200 components = 0.00236474 Jy
! Clean residual min=-0.004406 max=0.004899 Jy/beam
! Clean residual mean=0.000019 rms=0.001288 Jy/beam
! Combined flux in latest and established models = 0.0809665 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 = 7.25843e-07 Jy
! Component: 100  -  total flux cleaned = -4.28439e-05 Jy
! Component: 150  -  total flux cleaned = -4.236e-05 Jy
! Component: 200  -  total flux cleaned = -6.20936e-05 Jy
! Total flux subtracted in 200 components = -6.20936e-05 Jy
! Clean residual min=-0.004401 max=0.004881 Jy/beam
! Clean residual mean=0.000019 rms=0.001281 Jy/beam
! Combined flux in latest and established models = 0.0809045 Jy
! Adding 21 model components to the UV plane model.
! The established model now contains 50 components and 0.0809045 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 milli-arcsec
! Estimated beam: bmin=0.5631 mas, bmaj=1.161 mas, bpa=-10.65 degrees
! Estimated noise=0.281691 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000312705 Jy
! Component: 100  -  total flux cleaned = -8.47832e-05 Jy
! Component: 150  -  total flux cleaned = -3.486e-05 Jy
! Component: 200  -  total flux cleaned = 1.19155e-05 Jy
! Total flux subtracted in 200 components = 1.19155e-05 Jy
! Clean residual min=-0.002562 max=0.002738 Jy/beam
! Clean residual mean=0.000005 rms=0.000659 Jy/beam
! Combined flux in latest and established models = 0.0809164 Jy
selfcal
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 58 components and 0.0809164 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=0.087382Jy  sigma=0.789740
! Fit after  self-cal, rms=0.087455Jy  sigma=0.787966
wmodel /scr/pima/gc030_uvs/J1730+3714_X_map.mod
! Writing 58 model components to file: /scr/pima/gc030_uvs/J1730+3714_X_map.mod
wobs /scr/pima/gc030_uvs/J1730+3714_X_uvs.fits
! Writing UV FITS file: /scr/pima/gc030_uvs/J1730+3714_X_uvs.fits
wwins /scr/pima/gc030_uvs/J1730+3714_X_map.win
! wwins: Wrote 4 windows to /scr/pima/gc030_uvs/J1730+3714_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 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 milli-arcsec
! clean: niter=4096  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -4.56511e-06 Jy
! Component: 100  -  total flux cleaned = 0.000129991 Jy
! Component: 150  -  total flux cleaned = 4.48213e-05 Jy
! Component: 200  -  total flux cleaned = 0.0001253 Jy
! Component: 250  -  total flux cleaned = 0.000203574 Jy
! Component: 300  -  total flux cleaned = 0.000279275 Jy
! Component: 350  -  total flux cleaned = 0.000389841 Jy
! Component: 400  -  total flux cleaned = 0.000460967 Jy
! Component: 450  -  total flux cleaned = 0.000497078 Jy
! Component: 500  -  total flux cleaned = 0.000600801 Jy
! Component: 550  -  total flux cleaned = 0.000767987 Jy
! Component: 600  -  total flux cleaned = 0.000897508 Jy
! Component: 650  -  total flux cleaned = 0.000992301 Jy
! Component: 700  -  total flux cleaned = 0.000992069 Jy
! Component: 750  -  total flux cleaned = 0.00117499 Jy
! Component: 800  -  total flux cleaned = 0.00120469 Jy
! Component: 850  -  total flux cleaned = 0.00129247 Jy
! Component: 900  -  total flux cleaned = 0.00132089 Jy
! Component: 950  -  total flux cleaned = 0.00129254 Jy
! Component: 1000  -  total flux cleaned = 0.00132019 Jy
! Component: 1050  -  total flux cleaned = 0.00129276 Jy
! Component: 1100  -  total flux cleaned = 0.00126589 Jy
! Component: 1150  -  total flux cleaned = 0.00129202 Jy
! Component: 1200  -  total flux cleaned = 0.00136882 Jy
! Component: 1250  -  total flux cleaned = 0.00134298 Jy
! Component: 1300  -  total flux cleaned = 0.00136706 Jy
! Component: 1350  -  total flux cleaned = 0.00139114 Jy
! Component: 1400  -  total flux cleaned = 0.0014392 Jy
! Component: 1450  -  total flux cleaned = 0.00148627 Jy
! Component: 1500  -  total flux cleaned = 0.00150945 Jy
! Component: 1550  -  total flux cleaned = 0.00155561 Jy
! Component: 1600  -  total flux cleaned = 0.00157792 Jy
! Component: 1650  -  total flux cleaned = 0.00162323 Jy
! Component: 1700  -  total flux cleaned = 0.0016675 Jy
! Component: 1750  -  total flux cleaned = 0.00173268 Jy
! Component: 1800  -  total flux cleaned = 0.00177547 Jy
! Component: 1850  -  total flux cleaned = 0.00183906 Jy
! Component: 1900  -  total flux cleaned = 0.00190125 Jy
! Component: 1950  -  total flux cleaned = 0.00190092 Jy
! Component: 2000  -  total flux cleaned = 0.00198182 Jy
! Component: 2050  -  total flux cleaned = 0.00202161 Jy
! Component: 2100  -  total flux cleaned = 0.00200192 Jy
! Component: 2150  -  total flux cleaned = 0.00209903 Jy
! Component: 2200  -  total flux cleaned = 0.00208002 Jy
! Component: 2250  -  total flux cleaned = 0.0021369 Jy
! Component: 2300  -  total flux cleaned = 0.00215554 Jy
! Component: 2350  -  total flux cleaned = 0.00222911 Jy
! Component: 2400  -  total flux cleaned = 0.00222921 Jy
! Component: 2450  -  total flux cleaned = 0.00230146 Jy
! Component: 2500  -  total flux cleaned = 0.00235447 Jy
! Component: 2550  -  total flux cleaned = 0.00240697 Jy
! Component: 2600  -  total flux cleaned = 0.00249318 Jy
! Component: 2650  -  total flux cleaned = 0.00249283 Jy
! Component: 2700  -  total flux cleaned = 0.0025603 Jy
! Component: 2750  -  total flux cleaned = 0.00261047 Jy
! Component: 2800  -  total flux cleaned = 0.00265997 Jy
! Component: 2850  -  total flux cleaned = 0.00269247 Jy
! Component: 2900  -  total flux cleaned = 0.00272465 Jy
! Component: 2950  -  total flux cleaned = 0.00278851 Jy
! Component: 3000  -  total flux cleaned = 0.00280426 Jy
! Component: 3050  -  total flux cleaned = 0.0027884 Jy
! Component: 3100  -  total flux cleaned = 0.00286587 Jy
! Component: 3150  -  total flux cleaned = 0.00288107 Jy
! Component: 3200  -  total flux cleaned = 0.00291129 Jy
! Component: 3250  -  total flux cleaned = 0.00297114 Jy
! Component: 3300  -  total flux cleaned = 0.00298588 Jy
! Component: 3350  -  total flux cleaned = 0.00301523 Jy
! Component: 3400  -  total flux cleaned = 0.0030587 Jy
! Component: 3450  -  total flux cleaned = 0.00310155 Jy
! Component: 3500  -  total flux cleaned = 0.0030873 Jy
! Component: 3550  -  total flux cleaned = 0.00311574 Jy
! Component: 3600  -  total flux cleaned = 0.00314394 Jy
! Component: 3650  -  total flux cleaned = 0.00321334 Jy
! Component: 3700  -  total flux cleaned = 0.00326846 Jy
! Component: 3750  -  total flux cleaned = 0.0033228 Jy
! Component: 3800  -  total flux cleaned = 0.00336327 Jy
! Component: 3850  -  total flux cleaned = 0.00334977 Jy
! Component: 3900  -  total flux cleaned = 0.00340286 Jy
! Component: 3950  -  total flux cleaned = 0.00342911 Jy
! Component: 4000  -  total flux cleaned = 0.00344216 Jy
! Component: 4050  -  total flux cleaned = 0.00348096 Jy
! Total flux subtracted in 4096 components = 0.00353241 Jy
! Clean residual min=-0.000751 max=0.000711 Jy/beam
! Clean residual mean=0.000002 rms=0.000245 Jy/beam
! Combined flux in latest and established models = 0.0844488 Jy
keep
! Adding 340 model components to the UV plane model.
! The established model now contains 398 components and 0.0844488 Jy
![Exited script file: /home/lpetrov/bin/01_muppet]
wmap "/scr/pima/gc030_uvs/J1730+3714_X\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5631 x 1.161 at -10.65 degrees (North through East)
! Clean map  min=-0.0021484  max=0.04199 Jy/beam
! Writing clean map to FITS file: /scr/pima/gc030_uvs/J1730+3714_X_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.0419896 
invert
! Inverting map 
! Your choice of large map pixels excluded 1.33% of the data.
!  The x-axis pixel size should ideally be below 0.1832 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000238764 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -1.70588 1.70588 3.41176 6.82353 13.6471 27.2941 54.5882
print "clev=      ", int(3*image_rms*10000)/10000
! clev=       0.0007 
print "peak=      ", int(1000*peak_flux)/1000
! peak=       0.041 
print "dyn_range= ", int(1000*peak_flux/image_rms)/1000
! dyn_range=  175.862 
quit
! Quitting program
! Log file /scr/pima/gc030_uvs/J1730+3714_X_uvs.log closed on Fri Apr 22 08:51:57 2016