! Started logfile: J2201+5048_X_2017_02_19_pus_uvs.log on Sat May  4 21:47:28 2019
obs J2201+5048_X_2017_02_19_pus_uva.fits
! Reading UV FITS file: J2201+5048_X_2017_02_19_pus_uva.fits
! AN table 1: 113 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.774435 visibilities/baseline/integration-bin.
! Found source: J2201+5048
! 
! There are 12 IFs, and a total of 12 channels:
! 
!  IF  Channel    Frequency  Freq offset  Number of   Overall IF
!       origin    at origin  per channel   channels    bandwidth
!  ------------------------------------------------------------- (Hz)
!  01        1  8.44388e+09      3.2e+07          1      3.2e+07
!  02        2  8.47588e+09      3.2e+07          1      3.2e+07
!  03        3  8.50788e+09      3.2e+07          1      3.2e+07
!  04        4  8.53988e+09      3.2e+07          1      3.2e+07
!  05        5  8.60388e+09      3.2e+07          1      3.2e+07
!  06        6  8.63588e+09      3.2e+07          1      3.2e+07
!  07        7  8.69988e+09      3.2e+07          1      3.2e+07
!  08        8  8.73188e+09      3.2e+07          1      3.2e+07
!  09        9  8.79588e+09      3.2e+07          1      3.2e+07
!  10       10  8.82788e+09      3.2e+07          1      3.2e+07
!  11       11  8.85988e+09      3.2e+07          1      3.2e+07
!  12       12  8.89188e+09      3.2e+07          1      3.2e+07
! 
! Polarization(s): RR
! 
! Read 858 lines of history.
! 
! Reading 47256 visibilities.
select I
! Polarization I is unavailable.
! Selecting polarization: RR,  channels: 1..12
! 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: 5..5
! Reading IF 6 channels: 6..6
! Reading IF 7 channels: 7..7
! Reading IF 8 channels: 8..8
! Reading IF 9 channels: 9..9
! Reading IF 10 channels: 10..10
! Reading IF 11 channels: 11..11
! Reading IF 12 channels: 12..12
print "field_size =",field_size
! field_size = 512 
print "field_cell =",field_cell
! field_cell = 0.2 
print "taper_size =",taper_size
! taper_size = 70 
![@muppet J2201+5048_X_2017_02_19_pus]
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 = 512x512 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 132 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 132 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 132 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 132 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 5.
!  A total of 132 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 6.
!  A total of 132 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 7.
!  A total of 132 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 8.
!  A total of 132 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 9.
!  A total of 132 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 10.
!  A total of 132 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 11.
!  A total of 132 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 12.
!  A total of 132 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.561295Jy  sigma=0.004193
! Fit after  self-cal, rms=0.523334Jy  sigma=0.003914
! clrmod: Cleared the established, tentative and continuum models.
! Redundant starting model cleared.
uvw 2,-1
! Uniform weighting binwidth: 2 (pixels).
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.776 mas, bmaj=1.026 mas, bpa=-7.529 degrees
! Estimated noise=946.693 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 = 0.36744 Jy
! Component: 100  -  total flux cleaned = 0.468989 Jy
! Total flux subtracted in 100 components = 0.468989 Jy
! Clean residual min=-0.020807 max=0.043921 Jy/beam
! Clean residual mean=-0.000069 rms=0.006024 Jy/beam
! Combined flux in latest and established models = 0.468989 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 7 components and 0.468989 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Correcting IF 9.
! 
! Correcting IF 10.
! 
! Correcting IF 11.
! 
! Correcting IF 12.
! 
! Fit before self-cal, rms=0.143100Jy  sigma=0.001012
! Fit after  self-cal, rms=0.143018Jy  sigma=0.001012
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0475326 Jy
! Component: 100  -  total flux cleaned = 0.0716106 Jy
! Total flux subtracted in 100 components = 0.0716106 Jy
! Clean residual min=-0.016074 max=0.027648 Jy/beam
! Clean residual mean=-0.000037 rms=0.004341 Jy/beam
! Combined flux in latest and established models = 0.540599 Jy
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 9 components and 0.540599 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Correcting IF 9.
! 
! Correcting IF 10.
! 
! Correcting IF 11.
! 
! Correcting IF 12.
! 
! Fit before self-cal, rms=0.125670Jy  sigma=0.000863
! Fit after  self-cal, rms=0.125591Jy  sigma=0.000863
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Added new window around map position (-1.8, 0.6).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0238853 Jy
! Component: 100  -  total flux cleaned = 0.0369785 Jy
! Total flux subtracted in 100 components = 0.0369785 Jy
! Clean residual min=-0.014493 max=0.017034 Jy/beam
! Clean residual mean=-0.000026 rms=0.003755 Jy/beam
! Combined flux in latest and established models = 0.577578 Jy
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 18 components and 0.577578 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Correcting IF 9.
! 
! Correcting IF 10.
! 
! Correcting IF 11.
! 
! Correcting IF 12.
! 
! Fit before self-cal, rms=0.120631Jy  sigma=0.000821
! Fit after  self-cal, rms=0.120276Jy  sigma=0.000819
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
print "************** FINISHED UNIFORM WEIGHTING CLEAN **************"
! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** 
! 
uvw 0,-1
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
win_mult = win_mult * 1.6
clean_niter = clean_niter * 2
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.9339 mas, bmaj=1.222 mas, bpa=-5.388 degrees
! Estimated noise=444.803 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 = 0.0130209 Jy
! Component: 100  -  total flux cleaned = 0.020916 Jy
! Component: 150  -  total flux cleaned = 0.0254413 Jy
! Component: 200  -  total flux cleaned = 0.0268742 Jy
! Total flux subtracted in 200 components = 0.0268742 Jy
! Clean residual min=-0.012414 max=0.017665 Jy/beam
! Clean residual mean=-0.000020 rms=0.003866 Jy/beam
! Combined flux in latest and established models = 0.604452 Jy
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 28 components and 0.604452 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Correcting IF 9.
! 
! Correcting IF 10.
! 
! Correcting IF 11.
! 
! Correcting IF 12.
! 
! Fit before self-cal, rms=0.118840Jy  sigma=0.000805
! Fit after  self-cal, rms=0.118714Jy  sigma=0.000804
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.96     FD        0.99     HN        0.97     KP        0.98     
!   LA        0.98     MK        0.95     NL        1.05     OV        1.01     
!   PT        1.00*    SC        1.03     
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.96     FD        0.99     HN        1.00     KP        0.97     
!   LA        0.98     MK        0.96     NL        1.06     OV        1.02     
!   PT        1.00*    SC        0.99     
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.96     FD        0.99     HN        1.00     KP        0.99     
!   LA        1.01     MK        0.97     NL        1.06     OV        1.00     
!   PT        1.00*    SC        1.03     
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.96     FD        0.96     HN        0.98     KP        0.97     
!   LA        1.01     MK        0.98     NL        1.05     OV        1.00     
!   PT        1.00*    SC        1.03     
! 
! 
! Correcting IF 5.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.98     FD        0.97     HN        0.94     KP        0.97     
!   LA        1.00     MK        0.99     NL        1.05     OV        1.02     
!   PT        1.00*    SC        1.02     
! 
! 
! Correcting IF 6.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     FD        0.98     HN        0.97     KP        0.97     
!   LA        1.00     MK        0.97     NL        1.05     OV        0.98     
!   PT        1.00*    SC        1.03     
! 
! 
! Correcting IF 7.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.97     FD        0.99     HN        0.96     KP        0.97     
!   LA        0.97     MK        0.99     NL        1.06     OV        0.98     
!   PT        1.00*    SC        1.03     
! 
! 
! Correcting IF 8.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.94     FD        0.99     HN        0.96     KP        0.98     
!   LA        0.99     MK        0.97     NL        1.05     OV        0.99     
!   PT        1.00*    SC        1.03     
! 
! 
! Correcting IF 9.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.97     FD        0.99     HN        0.97     KP        0.98     
!   LA        1.01     MK        0.96     NL        1.04     OV        0.99     
!   PT        1.00*    SC        0.99     
! 
! 
! Correcting IF 10.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.97     FD        1.00     HN        1.01     KP        0.98     
!   LA        0.98     MK        0.99     NL        1.05     OV        1.03     
!   PT        1.00*    SC        0.98     
! 
! 
! Correcting IF 11.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.01     FD        1.00     HN        0.99     KP        0.98     
!   LA        0.97     MK        0.96     NL        1.04     OV        1.03     
!   PT        1.00*    SC        1.00     
! 
! 
! Correcting IF 12.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        0.99     HN        0.96     KP        1.01     
!   LA        1.01     MK        1.07     NL        1.07     OV        1.03     
!   PT        1.00*    SC        1.02     
! 
! 
! Fit before self-cal, rms=0.118714Jy  sigma=0.000804
! Fit after  self-cal, rms=0.116840Jy  sigma=0.000789
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.9316 mas, bmaj=1.221 mas, bpa=-5.811 degrees
! Estimated noise=440.989 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 = -0.0005629 Jy
! Component: 100  -  total flux cleaned = -0.00140554 Jy
! Component: 150  -  total flux cleaned = -0.0017887 Jy
! Component: 200  -  total flux cleaned = -0.0019514 Jy
! Total flux subtracted in 200 components = -0.0019514 Jy
! Clean residual min=-0.013937 max=0.017100 Jy/beam
! Clean residual mean=-0.000004 rms=0.003683 Jy/beam
! Combined flux in latest and established models = 0.602501 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 35 components and 0.602501 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Correcting IF 9.
! 
! Correcting IF 10.
! 
! Correcting IF 11.
! 
! Correcting IF 12.
! 
! Fit before self-cal, rms=0.116551Jy  sigma=0.000788
! Fit after  self-cal, rms=0.116508Jy  sigma=0.000787
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Correcting IF 9.
! 
! Correcting IF 10.
! 
! Correcting IF 11.
! 
! Correcting IF 12.
! 
! Fit before self-cal, rms=0.116508Jy  sigma=0.000787
! Fit after  self-cal, rms=0.109164Jy  sigma=0.000682
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.9373 mas, bmaj=1.219 mas, bpa=-6.44 degrees
! Estimated noise=442.829 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00136347 Jy
! Component: 100  -  total flux cleaned = 0.00177422 Jy
! Component: 150  -  total flux cleaned = 0.00176425 Jy
! Component: 200  -  total flux cleaned = 0.00202445 Jy
! Total flux subtracted in 200 components = 0.00202445 Jy
! Clean residual min=-0.004319 max=0.013976 Jy/beam
! Clean residual mean=0.000009 rms=0.001519 Jy/beam
! Combined flux in latest and established models = 0.604525 Jy
selfcal
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 46 components and 0.604525 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Correcting IF 9.
! 
! Correcting IF 10.
! 
! Correcting IF 11.
! 
! Correcting IF 12.
! 
! Fit before self-cal, rms=0.108812Jy  sigma=0.000679
! Fit after  self-cal, rms=0.108915Jy  sigma=0.000678
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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)
! Added new window around map position (-3.6, 1.6).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0130139 Jy
! Component: 100  -  total flux cleaned = 0.0193059 Jy
! Component: 150  -  total flux cleaned = 0.0231921 Jy
! Component: 200  -  total flux cleaned = 0.0252096 Jy
! Total flux subtracted in 200 components = 0.0252096 Jy
! Clean residual min=-0.002862 max=0.004967 Jy/beam
! Clean residual mean=0.000012 rms=0.000793 Jy/beam
! Combined flux in latest and established models = 0.629735 Jy
! Performing phase self-cal
! Adding 23 model components to the UV plane model.
! The established model now contains 66 components and 0.629735 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Correcting IF 9.
! 
! Correcting IF 10.
! 
! Correcting IF 11.
! 
! Correcting IF 12.
! 
! Fit before self-cal, rms=0.107416Jy  sigma=0.000664
! Fit after  self-cal, rms=0.107275Jy  sigma=0.000663
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Added new window around map position (-5.4, 2.8).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00460382 Jy
! Component: 100  -  total flux cleaned = 0.00749204 Jy
! Component: 150  -  total flux cleaned = 0.00901935 Jy
! Component: 200  -  total flux cleaned = 0.0103521 Jy
! Total flux subtracted in 200 components = 0.0103521 Jy
! Clean residual min=-0.002082 max=0.002771 Jy/beam
! Clean residual mean=0.000011 rms=0.000563 Jy/beam
! Combined flux in latest and established models = 0.640087 Jy
! Performing phase self-cal
! Adding 24 model components to the UV plane model.
! The established model now contains 80 components and 0.640087 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Correcting IF 9.
! 
! Correcting IF 10.
! 
! Correcting IF 11.
! 
! Correcting IF 12.
! 
! Fit before self-cal, rms=0.107004Jy  sigma=0.000661
! Fit after  self-cal, rms=0.106988Jy  sigma=0.000661
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Added new window around map position (-0.6, -22.6).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00252551 Jy
! Component: 100  -  total flux cleaned = 0.00334873 Jy
! Component: 150  -  total flux cleaned = 0.00407078 Jy
! Component: 200  -  total flux cleaned = 0.00448226 Jy
! Total flux subtracted in 200 components = 0.00448226 Jy
! Clean residual min=-0.002055 max=0.001757 Jy/beam
! Clean residual mean=0.000014 rms=0.000502 Jy/beam
! Combined flux in latest and established models = 0.644569 Jy
! Performing phase self-cal
! Adding 25 model components to the UV plane model.
! The established model now contains 86 components and 0.644569 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Correcting IF 9.
! 
! Correcting IF 10.
! 
! Correcting IF 11.
! 
! Correcting IF 12.
! 
! Fit before self-cal, rms=0.106883Jy  sigma=0.000660
! Fit after  self-cal, rms=0.106878Jy  sigma=0.000660
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Correcting IF 9.
! 
! Correcting IF 10.
! 
! Correcting IF 11.
! 
! Correcting IF 12.
! 
! Fit before self-cal, rms=0.106878Jy  sigma=0.000660
! Fit after  self-cal, rms=0.106579Jy  sigma=0.000659
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.9376 mas, bmaj=1.219 mas, bpa=-6.536 degrees
! Estimated noise=442.493 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000608966 Jy
! Component: 100  -  total flux cleaned = 0.00102715 Jy
! Component: 150  -  total flux cleaned = 0.0012362 Jy
! Component: 200  -  total flux cleaned = 0.00147572 Jy
! Total flux subtracted in 200 components = 0.00147572 Jy
! Clean residual min=-0.001802 max=0.001479 Jy/beam
! Clean residual mean=0.000006 rms=0.000396 Jy/beam
! Combined flux in latest and established models = 0.646045 Jy
selfcal
! Performing phase self-cal
! Adding 27 model components to the UV plane model.
! The established model now contains 99 components and 0.646045 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Correcting IF 9.
! 
! Correcting IF 10.
! 
! Correcting IF 11.
! 
! Correcting IF 12.
! 
! Fit before self-cal, rms=0.106519Jy  sigma=0.000659
! Fit after  self-cal, rms=0.106507Jy  sigma=0.000659
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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 = 0.000408112 Jy
! Component: 100  -  total flux cleaned = 0.000721285 Jy
! Component: 150  -  total flux cleaned = 0.00100989 Jy
! Component: 200  -  total flux cleaned = 0.00123987 Jy
! Total flux subtracted in 200 components = 0.00123987 Jy
! Clean residual min=-0.001656 max=0.001395 Jy/beam
! Clean residual mean=0.000006 rms=0.000370 Jy/beam
! Combined flux in latest and established models = 0.647284 Jy
! Performing phase self-cal
! Adding 30 model components to the UV plane model.
! The established model now contains 104 components and 0.647284 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Correcting IF 9.
! 
! Correcting IF 10.
! 
! Correcting IF 11.
! 
! Correcting IF 12.
! 
! Fit before self-cal, rms=0.106473Jy  sigma=0.000658
! Fit after  self-cal, rms=0.106471Jy  sigma=0.000658
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Correcting IF 9.
! 
! Correcting IF 10.
! 
! Correcting IF 11.
! 
! Correcting IF 12.
! 
! Fit before self-cal, rms=0.106471Jy  sigma=0.000658
! Fit after  self-cal, rms=0.106373Jy  sigma=0.000658
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=2.107 mas, bmaj=2.236 mas, bpa=6.582 degrees
! Estimated noise=588.188 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00087155 Jy
! Component: 100  -  total flux cleaned = 0.00109434 Jy
! Component: 150  -  total flux cleaned = 0.00127603 Jy
! Component: 200  -  total flux cleaned = 0.00137455 Jy
! Total flux subtracted in 200 components = 0.00137455 Jy
! Clean residual min=-0.001455 max=0.001429 Jy/beam
! Clean residual mean=0.000011 rms=0.000435 Jy/beam
! Combined flux in latest and established models = 0.648659 Jy
selfcal
! Performing phase self-cal
! Adding 24 model components to the UV plane model.
! The established model now contains 122 components and 0.648659 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Correcting IF 9.
! 
! Correcting IF 10.
! 
! Correcting IF 11.
! 
! Correcting IF 12.
! 
! Fit before self-cal, rms=0.106362Jy  sigma=0.000658
! Fit after  self-cal, rms=0.106359Jy  sigma=0.000658
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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 = 0.00022636 Jy
! Component: 100  -  total flux cleaned = 0.000332407 Jy
! Component: 150  -  total flux cleaned = 0.000411301 Jy
! Component: 200  -  total flux cleaned = 0.000469089 Jy
! Total flux subtracted in 200 components = 0.000469089 Jy
! Clean residual min=-0.001500 max=0.001428 Jy/beam
! Clean residual mean=0.000011 rms=0.000427 Jy/beam
! Combined flux in latest and established models = 0.649128 Jy
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 129 components and 0.649128 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Correcting IF 9.
! 
! Correcting IF 10.
! 
! Correcting IF 11.
! 
! Correcting IF 12.
! 
! Fit before self-cal, rms=0.106354Jy  sigma=0.000658
! Fit after  self-cal, rms=0.106353Jy  sigma=0.000658
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
win_mult = win_mult / 1.2
print "************** FINISHED AMPLITUDE SELF-CAL **************"
! ************** FINISHED AMPLITUDE SELF-CAL ************** 
restore
! Inverting map and beam 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.938 mas, bmaj=1.22 mas, bpa=-6.594 degrees
! Estimated noise=442.363 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.938 x 1.22 at -6.594 degrees (North through East)
! Clean map  min=-0.0013384  max=0.48889 Jy/beam
if(peak(flux) > thresh)
  selfcal true, true
  clean clean_niter,clean_gain
  selfcal
  flux_cutoff = imstat(rms) * dynam
  repeat
    if (peak(flux) > flux_cutoff) peakwin win_mult
    clean clean_niter,clean_gain
    flux_cutoff = imstat(rms) * dynam
    selfcal
    new_peak = peak(flux)
    until(new_peak<=flux_cutoff)
  selfcal true, true
  end if
print "************** CLEARING MODEL AND STARTING OVER **********"
! ************** CLEARING MODEL AND STARTING OVER ********** 
clrmod true
! clrmod: Cleared the established and tentative models.
uvw 2,-1
! Uniform weighting binwidth: 2 (pixels).
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.7801 mas, bmaj=1.023 mas, bpa=-9.105 degrees
! Estimated noise=948.753 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.367947 Jy
! Component: 100  -  total flux cleaned = 0.46686 Jy
! Component: 150  -  total flux cleaned = 0.514053 Jy
! Component: 200  -  total flux cleaned = 0.543121 Jy
! Total flux subtracted in 200 components = 0.543121 Jy
! Clean residual min=-0.008558 max=0.015579 Jy/beam
! Clean residual mean=-0.000024 rms=0.002566 Jy/beam
! Combined flux in latest and established models = 0.543122 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 17 model components to the UV plane model.
! The established model now contains 17 components and 0.543122 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.938 mas, bmaj=1.22 mas, bpa=-6.594 degrees
! Estimated noise=442.363 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 = 0.0242244 Jy
! Component: 100  -  total flux cleaned = 0.040915 Jy
! Component: 150  -  total flux cleaned = 0.0530569 Jy
! Component: 200  -  total flux cleaned = 0.0624301 Jy
! Total flux subtracted in 200 components = 0.0624301 Jy
! Clean residual min=-0.003741 max=0.005582 Jy/beam
! Clean residual mean=-0.000002 rms=0.001185 Jy/beam
! Combined flux in latest and established models = 0.605552 Jy
! Adding 30 model components to the UV plane model.
! The established model now contains 34 components and 0.605552 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00753048 Jy
! Component: 100  -  total flux cleaned = 0.0136353 Jy
! Component: 150  -  total flux cleaned = 0.0186194 Jy
! Component: 200  -  total flux cleaned = 0.0227616 Jy
! Total flux subtracted in 200 components = 0.0227616 Jy
! Clean residual min=-0.002557 max=0.002559 Jy/beam
! Clean residual mean=0.000002 rms=0.000668 Jy/beam
! Combined flux in latest and established models = 0.628313 Jy
! Adding 32 model components to the UV plane model.
! The established model now contains 52 components and 0.628313 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=2.107 mas, bmaj=2.236 mas, bpa=6.582 degrees
! Estimated noise=588.188 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00580466 Jy
! Component: 100  -  total flux cleaned = 0.00955509 Jy
! Component: 150  -  total flux cleaned = 0.0123205 Jy
! Component: 200  -  total flux cleaned = 0.0144433 Jy
! Total flux subtracted in 200 components = 0.0144433 Jy
! Clean residual min=-0.002063 max=0.002115 Jy/beam
! Clean residual mean=0.000011 rms=0.000584 Jy/beam
! Combined flux in latest and established models = 0.642756 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 = 0.00165476 Jy
! Component: 100  -  total flux cleaned = 0.00296788 Jy
! Component: 150  -  total flux cleaned = 0.0040317 Jy
! Component: 200  -  total flux cleaned = 0.00470434 Jy
! Total flux subtracted in 200 components = 0.00470434 Jy
! Clean residual min=-0.001606 max=0.001673 Jy/beam
! Clean residual mean=0.000012 rms=0.000470 Jy/beam
! Combined flux in latest and established models = 0.647461 Jy
! Adding 91 model components to the UV plane model.
! The established model now contains 131 components and 0.647461 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.938 mas, bmaj=1.22 mas, bpa=-6.594 degrees
! Estimated noise=442.363 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000359692 Jy
! Component: 100  -  total flux cleaned = 0.000506176 Jy
! Component: 150  -  total flux cleaned = 0.00084558 Jy
! Component: 200  -  total flux cleaned = 0.00107979 Jy
! Total flux subtracted in 200 components = 0.00107979 Jy
! Clean residual min=-0.001658 max=0.001652 Jy/beam
! Clean residual mean=0.000004 rms=0.000393 Jy/beam
! Combined flux in latest and established models = 0.64854 Jy
selfcal
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 139 components and 0.648541 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Correcting IF 9.
! 
! Correcting IF 10.
! 
! Correcting IF 11.
! 
! Correcting IF 12.
! 
! Fit before self-cal, rms=0.106432Jy  sigma=0.000659
! Fit after  self-cal, rms=0.106415Jy  sigma=0.000659
wmodel J2201+5048_X_2017_02_19_pus_map.mod
! Writing 139 model components to file: J2201+5048_X_2017_02_19_pus_map.mod
wobs J2201+5048_X_2017_02_19_pus_uvs.fits
! Writing UV FITS file: J2201+5048_X_2017_02_19_pus_uvs.fits
wwins J2201+5048_X_2017_02_19_pus_map.win
! wwins: Wrote 5 windows to J2201+5048_X_2017_02_19_pus_map.win
x = (field_size-8) * field_cell / 4
addwin -x,x,-x,x
clean (field_size*4),0.01
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000422835 Jy
! Component: 100  -  total flux cleaned = -0.000450761 Jy
! Component: 150  -  total flux cleaned = -0.00031895 Jy
! Component: 200  -  total flux cleaned = -0.000293652 Jy
! Component: 250  -  total flux cleaned = -0.000269173 Jy
! Component: 300  -  total flux cleaned = -0.000222878 Jy
! Component: 350  -  total flux cleaned = -0.000246324 Jy
! Component: 400  -  total flux cleaned = -0.000180739 Jy
! Component: 450  -  total flux cleaned = -0.000224168 Jy
! Component: 500  -  total flux cleaned = -0.000307723 Jy
! Component: 550  -  total flux cleaned = -0.000390401 Jy
! Component: 600  -  total flux cleaned = -0.000491125 Jy
! Component: 650  -  total flux cleaned = -0.000530195 Jy
! Component: 700  -  total flux cleaned = -0.000569211 Jy
! Component: 750  -  total flux cleaned = -0.00060742 Jy
! Component: 800  -  total flux cleaned = -0.000663541 Jy
! Component: 850  -  total flux cleaned = -0.000718698 Jy
! Component: 900  -  total flux cleaned = -0.000791065 Jy
! Component: 950  -  total flux cleaned = -0.000826942 Jy
! Component: 1000  -  total flux cleaned = -0.000897583 Jy
! Component: 1050  -  total flux cleaned = -0.00098438 Jy
! Component: 1100  -  total flux cleaned = -0.00103569 Jy
! Component: 1150  -  total flux cleaned = -0.00110347 Jy
! Component: 1200  -  total flux cleaned = -0.00112038 Jy
! Component: 1250  -  total flux cleaned = -0.00118615 Jy
! Component: 1300  -  total flux cleaned = -0.00120276 Jy
! Component: 1350  -  total flux cleaned = -0.00123537 Jy
! Component: 1400  -  total flux cleaned = -0.00134646 Jy
! Component: 1450  -  total flux cleaned = -0.00140892 Jy
! Component: 1500  -  total flux cleaned = -0.00150161 Jy
! Component: 1550  -  total flux cleaned = -0.00156266 Jy
! Component: 1600  -  total flux cleaned = -0.00160786 Jy
! Component: 1650  -  total flux cleaned = -0.00159305 Jy
! Component: 1700  -  total flux cleaned = -0.00163746 Jy
! Component: 1750  -  total flux cleaned = -0.00172492 Jy
! Component: 1800  -  total flux cleaned = -0.00176806 Jy
! Component: 1850  -  total flux cleaned = -0.00179645 Jy
! Component: 1900  -  total flux cleaned = -0.00183838 Jy
! Component: 1950  -  total flux cleaned = -0.00188017 Jy
! Component: 2000  -  total flux cleaned = -0.00188014 Jy
! Total flux subtracted in 2048 components = -0.0019481 Jy
! Clean residual min=-0.000727 max=0.000819 Jy/beam
! Clean residual mean=0.000001 rms=0.000238 Jy/beam
! Combined flux in latest and established models = 0.646592 Jy
keep
! Adding 151 model components to the UV plane model.
! The established model now contains 290 components and 0.646592 Jy
![Exited script file: muppet]
wmap "J2201+5048_X_2017_02_19_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.938 x 1.22 at -6.594 degrees (North through East)
! Clean map  min=-0.0010723  max=0.48948 Jy/beam
! Writing clean map to FITS file: J2201+5048_X_2017_02_19_pus_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.489482 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.152% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000237399 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.1455 0.1455 0.291 0.582 1.164 2.328 4.656 9.312 18.624 37.248 74.496
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0007 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.489 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.938 x 1.22 at -6.594 degrees (North through East)
! Clean map  min=-0.0010723  max=0.48948 Jy/beam
! Error occured in command: mapplot
! 
! <Aborted by EOF>
! <Aborted by EOF>
! <Aborted by EOF>
! <Aborted by EOF>
! 4 consecutive EOF's on stdin - 10 will exit program
! <Aborted by EOF>
! 5 consecutive EOF's on stdin - 10 will exit program
! <Aborted by EOF>
! 6 consecutive EOF's on stdin - 10 will exit program
! <Aborted by EOF>
! 7 consecutive EOF's on stdin - 10 will exit program
! <Aborted by EOF>
! 8 consecutive EOF's on stdin - 10 will exit program
! <Aborted by EOF>
! 9 consecutive EOF's on stdin - 10 will exit program
! <Aborted by EOF>
! 10 consecutive EOF's on stdin - 10 will exit program
! Log file J2201+5048_X_2017_02_19_pus_uvs.log closed on Sat May  4 21:47:32 2019