! Started logfile: /scr/pima/rv119_uvs/J2216+3518_X_dfm.log on Sun Dec 17 11:38:23 2017
float field_size
field_size =  1024
float field_cell
field_cell =   0.2000
float taper_size
taper_size =   70.0
float freq
freq       =    8.36575
obs     /scr/pima/rv119_uvs/J2216+3518_X_uva.fits
! Reading UV FITS file: /scr/pima/rv119_uvs/J2216+3518_X_uva.fits
! AN table 1: 128 integrations on 10 of 10 possible baselines.
! AN table 2: 10 integrations on 3 of 3 possible baselines.
! AN table 3: 12 integrations on 6 of 6 possible baselines.
! AN table 4: 9 integrations on 36 of 36 possible baselines.
! AN table 5: 4 integrations on 36 of 36 possible baselines.
! AN table 6: 3 integrations on 3 of 3 possible baselines.
! AN table 7: 7 integrations on 36 of 36 possible baselines.
! AN table 8: 11 integrations on 21 of 21 possible baselines.
! Apparent sampling: 0.436806 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J2216+3518
! 
! There are 4 IFs, and a total of 4 channels:
! 
!  IF  Channel    Frequency  Freq offset  Number of   Overall IF
!       origin    at origin  per channel   channels    bandwidth
!  ------------------------------------------------------------- (Hz)
!  01        1  8.36575e+09        8e+06          1        8e+06
!  02        2  8.44575e+09        8e+06          1        8e+06
!  03        3  8.80575e+09        8e+06          1        8e+06
!  04        4  8.92575e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 79 lines of history.
! 
! Reading 4092 visibilities.
select rr, 1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16 
! Restricting channel ranges to the available 4 channels.
! Selecting polarization: RR,  channels: 1..4
! Reading IF 1 channels: 1..1
! Reading IF 2 channels: 2..2
! Reading IF 3 channels: 3..3
! Reading IF 4 channels: 4..4
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 
![@/opt64/bin/pima_mupet_01.dfm J2216+3518_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 396 telescope corrections were flagged in sub-array 1.
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  A total of 32 telescope corrections were flagged in sub-array 3.
!  A total of 30 telescope corrections were flagged in sub-array 4.
!  A total of 8 telescope corrections were flagged in sub-array 5.
!  A total of 3 telescope corrections were flagged in sub-array 6.
!  A total of 27 telescope corrections were flagged in sub-array 7.
!  A total of 45 telescope corrections were flagged in sub-array 8.
! 
! Correcting IF 2.
!  A total of 396 telescope corrections were flagged in sub-array 1.
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  A total of 32 telescope corrections were flagged in sub-array 3.
!  A total of 30 telescope corrections were flagged in sub-array 4.
!  A total of 8 telescope corrections were flagged in sub-array 5.
!  A total of 3 telescope corrections were flagged in sub-array 6.
!  A total of 27 telescope corrections were flagged in sub-array 7.
!  A total of 45 telescope corrections were flagged in sub-array 8.
! 
! Correcting IF 3.
!  A total of 396 telescope corrections were flagged in sub-array 1.
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  A total of 32 telescope corrections were flagged in sub-array 3.
!  A total of 30 telescope corrections were flagged in sub-array 4.
!  A total of 8 telescope corrections were flagged in sub-array 5.
!  A total of 3 telescope corrections were flagged in sub-array 6.
!  A total of 27 telescope corrections were flagged in sub-array 7.
!  A total of 45 telescope corrections were flagged in sub-array 8.
! 
! Correcting IF 4.
!  A total of 396 telescope corrections were flagged in sub-array 1.
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  A total of 32 telescope corrections were flagged in sub-array 3.
!  A total of 30 telescope corrections were flagged in sub-array 4.
!  A total of 8 telescope corrections were flagged in sub-array 5.
!  A total of 3 telescope corrections were flagged in sub-array 6.
!  A total of 27 telescope corrections were flagged in sub-array 7.
!  A total of 45 telescope corrections were flagged in sub-array 8.
! 
! Fit before self-cal, rms=1.036203Jy  sigma=14.733369
! Fit after  self-cal, rms=0.772246Jy  sigma=10.823007
! 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 7.32% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
! Estimated beam: bmin=0.8488 mas, bmaj=0.9857 mas, bpa=86.62 degrees
! Estimated noise=1.14965 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 = 0.182117 Jy
! Component: 100  -  total flux cleaned = 0.243585 Jy
! Total flux subtracted in 100 components = 0.243585 Jy
! Clean residual min=-0.007873 max=0.027355 Jy/beam
! Clean residual mean=-0.000036 rms=0.002060 Jy/beam
! Combined flux in latest and established models = 0.243585 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 10 components and 0.243585 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.100863Jy  sigma=1.230251
! Fit after  self-cal, rms=0.100646Jy  sigma=1.227685
! Inverting map 
! Your choice of large map pixels excluded 7.32% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0301621 Jy
! Component: 100  -  total flux cleaned = 0.0455951 Jy
! Total flux subtracted in 100 components = 0.0455951 Jy
! Clean residual min=-0.006287 max=0.010830 Jy/beam
! Clean residual mean=-0.000019 rms=0.001343 Jy/beam
! Combined flux in latest and established models = 0.289181 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 16 components and 0.289181 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.091457Jy  sigma=1.005427
! Fit after  self-cal, rms=0.091178Jy  sigma=1.004344
! Inverting map 
! Your choice of large map pixels excluded 7.32% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
! Added new window around map position (0, 0.8).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0106205 Jy
! Component: 100  -  total flux cleaned = 0.0165801 Jy
! Total flux subtracted in 100 components = 0.0165801 Jy
! Clean residual min=-0.005780 max=0.008943 Jy/beam
! Clean residual mean=-0.000013 rms=0.001221 Jy/beam
! Combined flux in latest and established models = 0.305761 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 22 components and 0.305761 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.089592Jy  sigma=0.970069
! Fit after  self-cal, rms=0.089493Jy  sigma=0.968456
! Inverting map 
! Your choice of large map pixels excluded 7.32% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
! Added new window around map position (0.8, -1).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00787057 Jy
! Component: 100  -  total flux cleaned = 0.01246 Jy
! Total flux subtracted in 100 components = 0.01246 Jy
! Clean residual min=-0.005573 max=0.004990 Jy/beam
! Clean residual mean=-0.000008 rms=0.001152 Jy/beam
! Combined flux in latest and established models = 0.318221 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 31 components and 0.318221 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.088564Jy  sigma=0.951952
! Fit after  self-cal, rms=0.088480Jy  sigma=0.950480
! Inverting map 
! Your choice of large map pixels excluded 7.32% of the data.
!  The y-axis pixel size should ideally be below 0.172 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 7.32% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
! Estimated beam: bmin=0.9066 mas, bmaj=1.104 mas, bpa=78.1 degrees
! Estimated noise=0.899932 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 = 0.00633863 Jy
! Component: 100  -  total flux cleaned = 0.00647561 Jy
! Component: 150  -  total flux cleaned = 0.00673151 Jy
! Component: 200  -  total flux cleaned = 0.00684634 Jy
! Total flux subtracted in 200 components = 0.00684634 Jy
! Clean residual min=-0.004707 max=0.004446 Jy/beam
! Clean residual mean=-0.000001 rms=0.001052 Jy/beam
! Combined flux in latest and established models = 0.325067 Jy
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 40 components and 0.325067 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087679Jy  sigma=0.942241
! Fit after  self-cal, rms=0.087671Jy  sigma=0.941604
! Inverting map 
! Your choice of large map pixels excluded 7.32% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9066 x 1.104 at 78.1 degrees (North through East)
! Clean map  min=-0.0041317  max=0.22889 Jy/beam
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 144 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   HH        0.88     HN        1.09     NY        1.00     ON        0.97     
!   WZ        0.93     
! 
!  A total of 24 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   HN        0.00*    ON        0.00*    SC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   HN        1.06     NY        0.86     SC        0.99     WZ        1.00     
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        0.99     FD        0.95     HN        1.01     KP        1.02     
!   LA        0.99     NL        0.99     NY        1.01     PT        0.98     
!   SC        1.00     
! 
!  Telescope amplitude corrections in sub-array 5:
!   BR        1.01     FD        0.94     HN        1.00     KP        1.02     
!   LA        1.06     NL        0.99     OV        1.04     PT        1.01     
!   SC        0.94     
! 
!  A total of 6 telescope corrections were flagged in sub-array 6.
!  Telescope amplitude corrections in sub-array 6:
!   BR        0.00*    HN        0.00*    MK        0.00*    
! 
!  Telescope amplitude corrections in sub-array 7:
!   BR        1.03     FD        1.02     HN        1.05     KP        1.00     
!   LA        0.96     NL        0.99     NY        0.88     OV        0.99     
!   PT        0.98     
! 
!  A total of 18 telescope corrections were flagged in sub-array 8.
!  Telescope amplitude corrections in sub-array 8:
!   BR        1.02     FD        1.06     KP        1.04     LA        0.96     
!   MK        1.01     OV        0.97     PT        1.05     
! 
! 
! Correcting IF 2.
!  A total of 144 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   HH        0.95     HN        1.04     NY        0.93     ON        0.97     
!   WZ        0.95     
! 
!  A total of 24 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   HN        0.00*    ON        0.00*    SC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   HN        0.96     NY        1.01     SC        0.94     WZ        0.98     
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.03     FD        0.99     HN        1.02     KP        0.95     
!   LA        0.97     NL        0.98     NY        0.98     PT        0.99     
!   SC        0.99     
! 
!  Telescope amplitude corrections in sub-array 5:
!   BR        0.96     FD        1.00     HN        1.04     KP        0.97     
!   LA        1.15     NL        0.98     OV        1.13     PT        0.94     
!   SC        0.96     
! 
!  A total of 6 telescope corrections were flagged in sub-array 6.
!  Telescope amplitude corrections in sub-array 6:
!   BR        0.00*    HN        0.00*    MK        0.00*    
! 
!  Telescope amplitude corrections in sub-array 7:
!   BR        1.00     FD        1.02     HN        1.03     KP        1.04     
!   LA        0.99     NL        0.99     NY        1.00     OV        1.00     
!   PT        0.98     
! 
!  A total of 18 telescope corrections were flagged in sub-array 8.
!  Telescope amplitude corrections in sub-array 8:
!   BR        1.01     FD        1.04     KP        0.95     LA        0.92     
!   MK        1.21     OV        0.98     PT        0.97     
! 
! 
! Correcting IF 3.
!  A total of 144 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   HH        1.08     HN        1.09     NY        1.07     ON        1.06     
!   WZ        0.87     
! 
!  A total of 24 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   HN        0.00*    ON        0.00*    SC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   HN        0.98     NY        0.88     SC        1.06     WZ        0.98     
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.03     FD        1.06     HN        1.01     KP        0.97     
!   LA        1.01     NL        1.02     NY        0.95     PT        1.00     
!   SC        1.01     
! 
!  Telescope amplitude corrections in sub-array 5:
!   BR        1.03     FD        0.86     HN        1.09     KP        0.99     
!   LA        1.20     NL        1.00     OV        1.04     PT        0.97     
!   SC        1.01     
! 
!  A total of 6 telescope corrections were flagged in sub-array 6.
!  Telescope amplitude corrections in sub-array 6:
!   BR        0.00*    HN        0.00*    MK        0.00*    
! 
!  Telescope amplitude corrections in sub-array 7:
!   BR        1.01     FD        1.08     HN        1.03     KP        0.99     
!   LA        1.02     NL        0.98     NY        1.05     OV        1.02     
!   PT        0.96     
! 
!  A total of 18 telescope corrections were flagged in sub-array 8.
!  Telescope amplitude corrections in sub-array 8:
!   BR        1.06     FD        1.12     KP        1.04     LA        0.97     
!   MK        1.10     OV        1.02     PT        1.10     
! 
! 
! Correcting IF 4.
!  A total of 144 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   HH        1.29     HN        1.07     NY        0.95     ON        1.08     
!   WZ        0.87     
! 
!  A total of 24 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   HN        0.00*    ON        0.00*    SC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   HN        0.93     NY        0.99     SC        0.96     WZ        0.97     
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        0.94     FD        1.02     HN        1.06     KP        1.02     
!   LA        1.02     NL        0.97     NY        1.02     PT        1.02     
!   SC        0.85     
! 
!  Telescope amplitude corrections in sub-array 5:
!   BR        1.10     FD        0.93     HN        1.04     KP        0.99     
!   LA        1.09     NL        1.01     OV        1.04     PT        0.97     
!   SC        1.02     
! 
!  A total of 6 telescope corrections were flagged in sub-array 6.
!  Telescope amplitude corrections in sub-array 6:
!   BR        0.00*    HN        0.00*    MK        0.00*    
! 
!  Telescope amplitude corrections in sub-array 7:
!   BR        1.07     FD        1.07     HN        1.11     KP        1.01     
!   LA        1.03     NL        1.06     NY        0.95     OV        0.96     
!   PT        0.97     
! 
!  A total of 18 telescope corrections were flagged in sub-array 8.
!  Telescope amplitude corrections in sub-array 8:
!   BR        1.15     FD        1.02     KP        1.01     LA        1.06     
!   MK        1.11     OV        0.98     PT        1.00     
! 
! 
! Fit before self-cal, rms=0.087671Jy  sigma=0.941604
! Fit after  self-cal, rms=0.084324Jy  sigma=0.936292
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
! Estimated beam: bmin=0.9221 mas, bmaj=1.136 mas, bpa=68.83 degrees
! Estimated noise=0.946599 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 = 0.000618316 Jy
! Component: 100  -  total flux cleaned = 0.00078609 Jy
! Component: 150  -  total flux cleaned = 0.000713729 Jy
! Component: 200  -  total flux cleaned = 0.00078248 Jy
! Total flux subtracted in 200 components = 0.00078248 Jy
! Clean residual min=-0.004190 max=0.003996 Jy/beam
! Clean residual mean=0.000027 rms=0.000860 Jy/beam
! Combined flux in latest and established models = 0.325849 Jy
! Performing phase self-cal
! Adding 21 model components to the UV plane model.
! The established model now contains 49 components and 0.325849 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.084154Jy  sigma=0.934299
! Fit after  self-cal, rms=0.084432Jy  sigma=0.933865
! Inverting map 
! Your choice of large map pixels excluded 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 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.
! 
! Fit before self-cal, rms=0.084432Jy  sigma=0.933865
! Fit after  self-cal, rms=0.085129Jy  sigma=0.931671
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
! Estimated beam: bmin=0.9241 mas, bmaj=1.134 mas, bpa=68.8 degrees
! Estimated noise=0.947548 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00078784 Jy
! Component: 100  -  total flux cleaned = 0.000855304 Jy
! Component: 150  -  total flux cleaned = 0.000855225 Jy
! Component: 200  -  total flux cleaned = 0.000917674 Jy
! Total flux subtracted in 200 components = 0.000917674 Jy
! Clean residual min=-0.004059 max=0.003832 Jy/beam
! Clean residual mean=0.000018 rms=0.000849 Jy/beam
! Combined flux in latest and established models = 0.326767 Jy
selfcal
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 50 components and 0.326767 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.085010Jy  sigma=0.930428
! Fit after  self-cal, rms=0.085047Jy  sigma=0.930354
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 6.09494e-05 Jy
! Component: 100  -  total flux cleaned = 0.000121777 Jy
! Component: 150  -  total flux cleaned = 0.000176076 Jy
! Component: 200  -  total flux cleaned = 0.000178849 Jy
! Total flux subtracted in 200 components = 0.000178849 Jy
! Clean residual min=-0.003978 max=0.003782 Jy/beam
! Clean residual mean=0.000019 rms=0.000842 Jy/beam
! Combined flux in latest and established models = 0.326946 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 51 components and 0.326946 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.084957Jy  sigma=0.929504
! Fit after  self-cal, rms=0.084977Jy  sigma=0.929456
! Inverting map 
! Your choice of large map pixels excluded 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 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.
! 
! Fit before self-cal, rms=0.084977Jy  sigma=0.929456
! Fit after  self-cal, rms=0.086424Jy  sigma=0.924740
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
! Estimated beam: bmin=0.927 mas, bmaj=1.132 mas, bpa=68.29 degrees
! Estimated noise=0.948652 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000569716 Jy
! Component: 100  -  total flux cleaned = 0.000688291 Jy
! Component: 150  -  total flux cleaned = 0.000797661 Jy
! Component: 200  -  total flux cleaned = 0.000848687 Jy
! Total flux subtracted in 200 components = 0.000848687 Jy
! Clean residual min=-0.003614 max=0.003416 Jy/beam
! Clean residual mean=-0.000001 rms=0.000809 Jy/beam
! Combined flux in latest and established models = 0.327795 Jy
selfcal
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 51 components and 0.327795 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.086334Jy  sigma=0.923965
! Fit after  self-cal, rms=0.086410Jy  sigma=0.923861
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 6.39797e-05 Jy
! Component: 100  -  total flux cleaned = 0.000113003 Jy
! Component: 150  -  total flux cleaned = 0.000113707 Jy
! Component: 200  -  total flux cleaned = 0.00015674 Jy
! Total flux subtracted in 200 components = 0.00015674 Jy
! Clean residual min=-0.003659 max=0.003326 Jy/beam
! Clean residual mean=-0.000000 rms=0.000804 Jy/beam
! Combined flux in latest and established models = 0.327951 Jy
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 51 components and 0.327951 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.086336Jy  sigma=0.923295
! Fit after  self-cal, rms=0.086355Jy  sigma=0.923265
! Inverting map 
! Your choice of large map pixels excluded 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 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.
! 
! Fit before self-cal, rms=0.086355Jy  sigma=0.923265
! Fit after  self-cal, rms=0.087617Jy  sigma=0.923071
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
! Estimated beam: bmin=2.306 mas, bmaj=3.106 mas, bpa=88.93 degrees
! Estimated noise=1.16639 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00108238 Jy
! Component: 100  -  total flux cleaned = 0.00126998 Jy
! Component: 150  -  total flux cleaned = 0.0013228 Jy
! Component: 200  -  total flux cleaned = 0.0013427 Jy
! Total flux subtracted in 200 components = 0.0013427 Jy
! Clean residual min=-0.004081 max=0.004042 Jy/beam
! Clean residual mean=-0.000000 rms=0.001020 Jy/beam
! Combined flux in latest and established models = 0.329294 Jy
selfcal
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 54 components and 0.329294 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087622Jy  sigma=0.923012
! Fit after  self-cal, rms=0.087621Jy  sigma=0.922922
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 7.20726e-05 Jy
! Component: 100  -  total flux cleaned = 8.85415e-05 Jy
! Component: 150  -  total flux cleaned = 0.00010131 Jy
! Component: 200  -  total flux cleaned = 0.000111174 Jy
! Total flux subtracted in 200 components = 0.000111174 Jy
! Clean residual min=-0.004085 max=0.004033 Jy/beam
! Clean residual mean=-0.000000 rms=0.001020 Jy/beam
! Combined flux in latest and established models = 0.329405 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 55 components and 0.329405 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087621Jy  sigma=0.922872
! Fit after  self-cal, rms=0.087612Jy  sigma=0.922823
! Inverting map 
! Your choice of large map pixels excluded 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 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 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
! Estimated beam: bmin=0.931 mas, bmaj=1.131 mas, bpa=68.02 degrees
! Estimated noise=0.950324 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.931 x 1.131 at 68.02 degrees (North through East)
! Clean map  min=-0.0034446  max=0.23178 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 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
! Estimated beam: bmin=0.8377 mas, bmaj=1.026 mas, bpa=74.03 degrees
! Estimated noise=1.22581 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.182785 Jy
! Component: 100  -  total flux cleaned = 0.247123 Jy
! Component: 150  -  total flux cleaned = 0.278299 Jy
! Component: 200  -  total flux cleaned = 0.296398 Jy
! Total flux subtracted in 200 components = 0.296398 Jy
! Clean residual min=-0.006133 max=0.009643 Jy/beam
! Clean residual mean=-0.000013 rms=0.001307 Jy/beam
! Combined flux in latest and established models = 0.296397 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 23 model components to the UV plane model.
! The established model now contains 23 components and 0.296397 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
! Estimated beam: bmin=0.931 mas, bmaj=1.131 mas, bpa=68.02 degrees
! Estimated noise=0.950324 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 = 0.0152246 Jy
! Component: 100  -  total flux cleaned = 0.0236955 Jy
! Component: 150  -  total flux cleaned = 0.0288722 Jy
! Component: 200  -  total flux cleaned = 0.0309859 Jy
! Total flux subtracted in 200 components = 0.0309859 Jy
! Clean residual min=-0.003913 max=0.003647 Jy/beam
! Clean residual mean=-0.000003 rms=0.000846 Jy/beam
! Combined flux in latest and established models = 0.327383 Jy
! Adding 19 model components to the UV plane model.
! The established model now contains 33 components and 0.327383 Jy
! Inverting map 
! Your choice of large map pixels excluded 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 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 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
! Estimated beam: bmin=2.306 mas, bmaj=3.106 mas, bpa=88.93 degrees
! Estimated noise=1.16639 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00156104 Jy
! Component: 100  -  total flux cleaned = 0.00202636 Jy
! Component: 150  -  total flux cleaned = 0.0020706 Jy
! Component: 200  -  total flux cleaned = 0.00207021 Jy
! Total flux subtracted in 200 components = 0.00207021 Jy
! Clean residual min=-0.004049 max=0.003999 Jy/beam
! Clean residual mean=0.000000 rms=0.001021 Jy/beam
! Combined flux in latest and established models = 0.329454 Jy
flux_cutoff = imstat(rms) * dynam
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  keep
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 1.20648e-05 Jy
! Component: 100  -  total flux cleaned = 2.3022e-05 Jy
! Component: 150  -  total flux cleaned = 2.35107e-05 Jy
! Component: 200  -  total flux cleaned = 3.37425e-05 Jy
! Total flux subtracted in 200 components = 3.37425e-05 Jy
! Clean residual min=-0.004054 max=0.004003 Jy/beam
! Clean residual mean=0.000000 rms=0.001020 Jy/beam
! Combined flux in latest and established models = 0.329487 Jy
! Adding 13 model components to the UV plane model.
! The established model now contains 43 components and 0.329487 Jy
! Inverting map 
! Your choice of large map pixels excluded 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
! Estimated beam: bmin=0.931 mas, bmaj=1.131 mas, bpa=68.02 degrees
! Estimated noise=0.950324 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000480714 Jy
! Component: 100  -  total flux cleaned = -0.000671092 Jy
! Component: 150  -  total flux cleaned = -0.000762698 Jy
! Component: 200  -  total flux cleaned = -0.000763802 Jy
! Total flux subtracted in 200 components = -0.000763802 Jy
! Clean residual min=-0.003792 max=0.003473 Jy/beam
! Clean residual mean=-0.000001 rms=0.000823 Jy/beam
! Combined flux in latest and established models = 0.328723 Jy
selfcal
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 50 components and 0.328723 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087878Jy  sigma=0.925416
! Fit after  self-cal, rms=0.087866Jy  sigma=0.924869
wmodel J2216+3518_X_map.mod
! Writing 50 model components to file: J2216+3518_X_map.mod
wobs   J2216+3518_X_uvs.fits
! Writing UV FITS file: J2216+3518_X_uvs.fits
wwins  J2216+3518_X_map.win
! wwins: Wrote 3 windows to J2216+3518_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 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
! clean: niter=4096  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000623871 Jy
! Component: 100  -  total flux cleaned = -0.00100572 Jy
! Component: 150  -  total flux cleaned = -0.00125027 Jy
! Component: 200  -  total flux cleaned = -0.00130923 Jy
! Component: 250  -  total flux cleaned = -0.00159694 Jy
! Component: 300  -  total flux cleaned = -0.00165295 Jy
! Component: 350  -  total flux cleaned = -0.00181875 Jy
! Component: 400  -  total flux cleaned = -0.00176492 Jy
! Component: 450  -  total flux cleaned = -0.0018179 Jy
! Component: 500  -  total flux cleaned = -0.00166021 Jy
! Component: 550  -  total flux cleaned = -0.00150552 Jy
! Component: 600  -  total flux cleaned = -0.00135319 Jy
! Component: 650  -  total flux cleaned = -0.00120177 Jy
! Component: 700  -  total flux cleaned = -0.00105257 Jy
! Component: 750  -  total flux cleaned = -0.000954338 Jy
! Component: 800  -  total flux cleaned = -0.000857937 Jy
! Component: 850  -  total flux cleaned = -0.000714773 Jy
! Component: 900  -  total flux cleaned = -0.000667496 Jy
! Component: 950  -  total flux cleaned = -0.000573756 Jy
! Component: 1000  -  total flux cleaned = -0.000389153 Jy
! Component: 1050  -  total flux cleaned = -0.000434457 Jy
! Component: 1100  -  total flux cleaned = -0.000343784 Jy
! Component: 1150  -  total flux cleaned = -0.00029909 Jy
! Component: 1200  -  total flux cleaned = -0.00029904 Jy
! Component: 1250  -  total flux cleaned = -0.000166946 Jy
! Component: 1300  -  total flux cleaned = -0.000167351 Jy
! Component: 1350  -  total flux cleaned = -0.00012409 Jy
! Component: 1400  -  total flux cleaned = 4.67957e-06 Jy
! Component: 1450  -  total flux cleaned = -3.81876e-05 Jy
! Component: 1500  -  total flux cleaned = -0.000164813 Jy
! Component: 1550  -  total flux cleaned = -3.8632e-05 Jy
! Component: 1600  -  total flux cleaned = -3.79855e-05 Jy
! Component: 1650  -  total flux cleaned = -3.81059e-05 Jy
! Component: 1700  -  total flux cleaned = -7.88743e-05 Jy
! Component: 1750  -  total flux cleaned = -7.88956e-05 Jy
! Component: 1800  -  total flux cleaned = -7.88092e-05 Jy
! Component: 1850  -  total flux cleaned = -3.90526e-05 Jy
! Component: 1900  -  total flux cleaned = 4.07352e-07 Jy
! Component: 1950  -  total flux cleaned = -0.000118078 Jy
! Component: 2000  -  total flux cleaned = -0.000157269 Jy
! Component: 2050  -  total flux cleaned = -0.000157604 Jy
! Component: 2100  -  total flux cleaned = -0.000196148 Jy
! Component: 2150  -  total flux cleaned = -0.000195782 Jy
! Component: 2200  -  total flux cleaned = -0.00015797 Jy
! Component: 2250  -  total flux cleaned = -4.48952e-05 Jy
! Component: 2300  -  total flux cleaned = -0.000157769 Jy
! Component: 2350  -  total flux cleaned = -0.000306899 Jy
! Component: 2400  -  total flux cleaned = -0.000269821 Jy
! Component: 2450  -  total flux cleaned = -0.000343443 Jy
! Component: 2500  -  total flux cleaned = -0.000160035 Jy
! Component: 2550  -  total flux cleaned = -0.000305572 Jy
! Component: 2600  -  total flux cleaned = -0.000160923 Jy
! Component: 2650  -  total flux cleaned = -0.000376563 Jy
! Component: 2700  -  total flux cleaned = -0.00030485 Jy
! Component: 2750  -  total flux cleaned = -0.000411631 Jy
! Component: 2800  -  total flux cleaned = -0.000411238 Jy
! Component: 2850  -  total flux cleaned = -0.000235561 Jy
! Component: 2900  -  total flux cleaned = -0.000340226 Jy
! Component: 2950  -  total flux cleaned = -0.000306101 Jy
! Component: 3000  -  total flux cleaned = -0.000340529 Jy
! Component: 3050  -  total flux cleaned = -0.00037474 Jy
! Component: 3100  -  total flux cleaned = -0.000545359 Jy
! Component: 3150  -  total flux cleaned = -0.000409601 Jy
! Component: 3200  -  total flux cleaned = -0.000476839 Jy
! Component: 3250  -  total flux cleaned = -0.000644403 Jy
! Component: 3300  -  total flux cleaned = -0.000477573 Jy
! Component: 3350  -  total flux cleaned = -0.000643601 Jy
! Component: 3400  -  total flux cleaned = -0.000610458 Jy
! Component: 3450  -  total flux cleaned = -0.000643584 Jy
! Component: 3500  -  total flux cleaned = -0.000578134 Jy
! Component: 3550  -  total flux cleaned = -0.000708054 Jy
! Component: 3600  -  total flux cleaned = -0.000805125 Jy
! Component: 3650  -  total flux cleaned = -0.000869582 Jy
! Component: 3700  -  total flux cleaned = -0.00086954 Jy
! Component: 3750  -  total flux cleaned = -0.000805762 Jy
! Component: 3800  -  total flux cleaned = -0.000964399 Jy
! Component: 3850  -  total flux cleaned = -0.00083804 Jy
! Component: 3900  -  total flux cleaned = -0.000838075 Jy
! Component: 3950  -  total flux cleaned = -0.000869328 Jy
! Component: 4000  -  total flux cleaned = -0.000900457 Jy
! Component: 4050  -  total flux cleaned = -0.000807563 Jy
! Total flux subtracted in 4096 components = -0.000961912 Jy
! Clean residual min=-0.001550 max=0.001670 Jy/beam
! Clean residual mean=0.000003 rms=0.000513 Jy/beam
! Combined flux in latest and established models = 0.327761 Jy
keep
! Adding 333 model components to the UV plane model.
! The established model now contains 383 components and 0.327762 Jy
![Exited script file: /opt64/bin/pima_mupet_01.dfm]
wmap   /scr/pima/rv119_uvs/J2216+3518_X_map.fits
! Inverting map 
! Your choice of large map pixels excluded 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.931 x 1.131 at 68.02 degrees (North through East)
! Clean map  min=-0.0029481  max=0.23142 Jy/beam
! Writing clean map to FITS file: /scr/pima/rv119_uvs/J2216+3518_X_map.fits
wmodel /scr/pima/rv119_uvs/J2216+3518_X_map.mod
! Writing 383 model components to file: /scr/pima/rv119_uvs/J2216+3518_X_map.mod
wobs   /scr/pima/rv119_uvs/J2216+3518_X_uvs.fits
! Writing UV FITS file: /scr/pima/rv119_uvs/J2216+3518_X_uvs.fits
wwins  /scr/pima/rv119_uvs/J2216+3518_X_map.win
! wwins: Wrote 4 windows to /scr/pima/rv119_uvs/J2216+3518_X_map.win
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is", peak_flux
! The peak flux is 0.231423 
invert
! Inverting map 
! Your choice of large map pixels excluded 4.6% of the data.
!  The y-axis pixel size should ideally be below 0.172 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000512452 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.664306 0.664306 1.32861 2.65722 5.31445 10.6289 21.2578 42.5156 85.0311
print "clev=      ", int(3*image_rms*10000)/10000
! clev=       0.0015 
print "peak=      ", int(1000*peak_flux)/1000
! peak=       0.231 
print "dyn_range= ", int(1000*peak_flux/image_rms)/1000
! dyn_range=  451.599 
quit
! Quitting program
! Log file /scr/pima/rv119_uvs/J2216+3518_X_dfm.log closed on Sun Dec 17 11:38:28 2017