! Started logfile: /scr/pima/rv118_uvs/J2145+1115_X_dfm.log on Sun Dec 10 00:11:41 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/rv118_uvs/J2145+1115_X_uva.fits
! Reading UV FITS file: /scr/pima/rv118_uvs/J2145+1115_X_uva.fits
! AN table 1: 58 integrations on 3 of 3 possible baselines.
! AN table 2: 84 integrations on 55 of 55 possible baselines.
! AN table 3: 26 integrations on 28 of 28 possible baselines.
! Apparent sampling: 0.390982 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J2145+1115
! 
! 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 8636 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 J2145+1115_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 36 telescope corrections were flagged in sub-array 1.
!  A total of 514 telescope corrections were flagged in sub-array 2.
!  A total of 63 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 36 telescope corrections were flagged in sub-array 1.
!  A total of 514 telescope corrections were flagged in sub-array 2.
!  A total of 63 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 36 telescope corrections were flagged in sub-array 1.
!  A total of 514 telescope corrections were flagged in sub-array 2.
!  A total of 63 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 36 telescope corrections were flagged in sub-array 1.
!  A total of 514 telescope corrections were flagged in sub-array 2.
!  A total of 63 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=1.027090Jy  sigma=15.669900
! Fit after  self-cal, rms=0.787996Jy  sigma=11.642039
! 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 8.44% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1804 milli-arcsec
! Estimated beam: bmin=0.521 mas, bmaj=0.8767 mas, bpa=3.296 degrees
! Estimated noise=0.954573 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 = 0.17863 Jy
! Component: 100  -  total flux cleaned = 0.226629 Jy
! Total flux subtracted in 100 components = 0.226629 Jy
! Clean residual min=-0.006944 max=0.017312 Jy/beam
! Clean residual mean=0.000011 rms=0.001662 Jy/beam
! Combined flux in latest and established models = 0.226629 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 8 components and 0.226629 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.083926Jy  sigma=1.055331
! Fit after  self-cal, rms=0.083981Jy  sigma=1.054633
! Inverting map 
! Your choice of large map pixels excluded 8.44% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1804 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0173768 Jy
! Component: 100  -  total flux cleaned = 0.0225406 Jy
! Total flux subtracted in 100 components = 0.0225406 Jy
! Clean residual min=-0.005392 max=0.008169 Jy/beam
! Clean residual mean=0.000007 rms=0.001293 Jy/beam
! Combined flux in latest and established models = 0.24917 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 12 components and 0.24917 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.080927Jy  sigma=0.975695
! Fit after  self-cal, rms=0.080857Jy  sigma=0.975284
! Inverting map 
! Your choice of large map pixels excluded 8.44% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1804 milli-arcsec
! Added new window around map position (0.4, -1.2).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00619111 Jy
! Component: 100  -  total flux cleaned = 0.00782482 Jy
! Total flux subtracted in 100 components = 0.00782482 Jy
! Clean residual min=-0.005217 max=0.006138 Jy/beam
! Clean residual mean=0.000005 rms=0.001227 Jy/beam
! Combined flux in latest and established models = 0.256995 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 19 components and 0.256995 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.080210Jy  sigma=0.959976
! Fit after  self-cal, rms=0.080114Jy  sigma=0.958758
! Inverting map 
! Your choice of large map pixels excluded 8.44% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1804 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 8.44% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1804 milli-arcsec
! Estimated beam: bmin=0.6254 mas, bmaj=1.002 mas, bpa=-0.6004 degrees
! Estimated noise=0.550302 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (0.6, -2.8).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0069035 Jy
! Component: 100  -  total flux cleaned = 0.0106574 Jy
! Component: 150  -  total flux cleaned = 0.0124695 Jy
! Component: 200  -  total flux cleaned = 0.012937 Jy
! Total flux subtracted in 200 components = 0.012937 Jy
! Clean residual min=-0.003718 max=0.004569 Jy/beam
! Clean residual mean=0.000005 rms=0.000929 Jy/beam
! Combined flux in latest and established models = 0.269932 Jy
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 32 components and 0.269932 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.079610Jy  sigma=0.946500
! Fit after  self-cal, rms=0.079524Jy  sigma=0.945003
! Inverting map 
! Your choice of large map pixels excluded 8.44% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1804 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6254 x 1.002 at -0.6004 degrees (North through East)
! Clean map  min=-0.0030411  max=0.22238 Jy/beam
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 138 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   HH        0.00*    NY        0.00*    WZ        0.00*    
! 
!  A total of 18 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.04     FD        0.99     HH        1.00     HN        1.04     
!   KP        1.00     LA        0.96     NL        1.01     ON        1.02     
!   PT        0.99     SC        0.98     WZ        0.99     
! 
!  A total of 33 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.03     FD        0.96     KK        0.98     KP        0.99     
!   LA        0.99     NL        0.97     OV        1.01     PT        1.00     
! 
! 
! Correcting IF 2.
!  A total of 138 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   HH        0.00*    NY        0.00*    WZ        0.00*    
! 
!  A total of 18 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.03     FD        1.00     HH        1.23     HN        1.02     
!   KP        1.02     LA        0.98     NL        0.99     ON        1.03     
!   PT        0.96     SC        1.01     WZ        0.99     
! 
!  A total of 33 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.99     FD        0.99     KK        1.00     KP        1.01     
!   LA        1.00     NL        0.99     OV        0.99     PT        0.97     
! 
! 
! Correcting IF 3.
!  A total of 138 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   HH        0.00*    NY        0.00*    WZ        0.00*    
! 
!  A total of 18 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.04     FD        0.95     HH        1.02     HN        1.06     
!   KP        1.00     LA        0.98     NL        1.01     ON        1.01     
!   PT        0.97     SC        1.00     WZ        0.98     
! 
!  A total of 33 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.97     FD        0.99     KK        0.96     KP        1.00     
!   LA        0.99     NL        1.00     OV        1.02     PT        0.95     
! 
! 
! Correcting IF 4.
!  A total of 138 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   HH        0.00*    NY        0.00*    WZ        0.00*    
! 
!  A total of 18 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.08     FD        0.98     HH        1.05     HN        0.99     
!   KP        0.99     LA        0.98     NL        0.99     ON        0.99     
!   PT        0.98     SC        0.98     WZ        0.99     
! 
!  A total of 33 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.95     FD        0.98     KK        1.00     KP        1.03     
!   LA        0.98     NL        0.99     OV        1.02     PT        0.98     
! 
! 
! Fit before self-cal, rms=0.079524Jy  sigma=0.945003
! Fit after  self-cal, rms=0.080421Jy  sigma=0.953492
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
! Estimated beam: bmin=0.61 mas, bmaj=1.139 mas, bpa=-0.793 degrees
! Estimated noise=0.563416 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 (4, -9.8).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00276756 Jy
! Component: 100  -  total flux cleaned = 0.00252007 Jy
! Component: 150  -  total flux cleaned = 0.00238331 Jy
! Component: 200  -  total flux cleaned = 0.00232096 Jy
! Total flux subtracted in 200 components = 0.00232096 Jy
! Clean residual min=-0.004343 max=0.003980 Jy/beam
! Clean residual mean=0.000001 rms=0.000818 Jy/beam
! Combined flux in latest and established models = 0.272253 Jy
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 51 components and 0.272253 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.080135Jy  sigma=0.951114
! Fit after  self-cal, rms=0.080154Jy  sigma=0.950894
! Inverting map 
! Your choice of large map pixels excluded 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 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=0.080154Jy  sigma=0.950894
! Fit after  self-cal, rms=0.081202Jy  sigma=0.935492
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
! Estimated beam: bmin=0.6107 mas, bmaj=1.137 mas, bpa=-0.9175 degrees
! Estimated noise=0.563454 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 5.06616e-05 Jy
! Component: 100  -  total flux cleaned = -0.000100333 Jy
! Component: 150  -  total flux cleaned = -0.000145571 Jy
! Component: 200  -  total flux cleaned = -0.000184603 Jy
! Total flux subtracted in 200 components = -0.000184603 Jy
! Clean residual min=-0.002472 max=0.002625 Jy/beam
! Clean residual mean=0.000001 rms=0.000581 Jy/beam
! Combined flux in latest and established models = 0.272068 Jy
selfcal
! Performing phase self-cal
! Adding 21 model components to the UV plane model.
! The established model now contains 66 components and 0.272068 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.081127Jy  sigma=0.934781
! Fit after  self-cal, rms=0.081237Jy  sigma=0.934661
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 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 (-21.4, 8.8).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00198571 Jy
! Component: 100  -  total flux cleaned = 0.0019853 Jy
! Component: 150  -  total flux cleaned = 0.00211249 Jy
! Component: 200  -  total flux cleaned = 0.00218936 Jy
! Total flux subtracted in 200 components = 0.00218936 Jy
! Clean residual min=-0.002384 max=0.002376 Jy/beam
! Clean residual mean=0.000001 rms=0.000566 Jy/beam
! Combined flux in latest and established models = 0.274258 Jy
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 77 components and 0.274258 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.081110Jy  sigma=0.933605
! Fit after  self-cal, rms=0.081098Jy  sigma=0.933555
! Inverting map 
! Your choice of large map pixels excluded 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 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=0.081098Jy  sigma=0.933555
! Fit after  self-cal, rms=0.083352Jy  sigma=0.930500
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
! Estimated beam: bmin=0.612 mas, bmaj=1.137 mas, bpa=-1.024 degrees
! Estimated noise=0.563137 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000534766 Jy
! Component: 100  -  total flux cleaned = -0.000440811 Jy
! Component: 150  -  total flux cleaned = -0.000356901 Jy
! Component: 200  -  total flux cleaned = -0.000317542 Jy
! Total flux subtracted in 200 components = -0.000317542 Jy
! Clean residual min=-0.001948 max=0.001991 Jy/beam
! Clean residual mean=0.000001 rms=0.000483 Jy/beam
! Combined flux in latest and established models = 0.27394 Jy
selfcal
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 88 components and 0.27394 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.083301Jy  sigma=0.929803
! Fit after  self-cal, rms=0.083398Jy  sigma=0.929756
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 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 = -7.82634e-05 Jy
! Component: 100  -  total flux cleaned = -0.00011259 Jy
! Component: 150  -  total flux cleaned = -0.000146713 Jy
! Component: 200  -  total flux cleaned = -0.000239152 Jy
! Total flux subtracted in 200 components = -0.000239152 Jy
! Clean residual min=-0.001919 max=0.001987 Jy/beam
! Clean residual mean=0.000001 rms=0.000480 Jy/beam
! Combined flux in latest and established models = 0.273701 Jy
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 89 components and 0.273701 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.083372Jy  sigma=0.929486
! Fit after  self-cal, rms=0.083368Jy  sigma=0.929482
! Inverting map 
! Your choice of large map pixels excluded 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 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=0.083368Jy  sigma=0.929482
! Fit after  self-cal, rms=0.083758Jy  sigma=0.929364
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
! Estimated beam: bmin=2.811 mas, bmaj=2.985 mas, bpa=-9.81 degrees
! Estimated noise=0.699452 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000196381 Jy
! Component: 100  -  total flux cleaned = 0.000426848 Jy
! Component: 150  -  total flux cleaned = 0.000443386 Jy
! Component: 200  -  total flux cleaned = 0.00041474 Jy
! Total flux subtracted in 200 components = 0.00041474 Jy
! Clean residual min=-0.002080 max=0.002077 Jy/beam
! Clean residual mean=0.000002 rms=0.000584 Jy/beam
! Combined flux in latest and established models = 0.274116 Jy
selfcal
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 100 components and 0.274116 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.083757Jy  sigma=0.929360
! Fit after  self-cal, rms=0.083767Jy  sigma=0.929350
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 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 = 7.02718e-05 Jy
! Component: 100  -  total flux cleaned = 8.42953e-05 Jy
! Component: 150  -  total flux cleaned = 9.69006e-05 Jy
! Component: 200  -  total flux cleaned = 0.000109054 Jy
! Total flux subtracted in 200 components = 0.000109054 Jy
! Clean residual min=-0.002095 max=0.002053 Jy/beam
! Clean residual mean=0.000002 rms=0.000582 Jy/beam
! Combined flux in latest and established models = 0.274225 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 103 components and 0.274225 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.083765Jy  sigma=0.929349
! Fit after  self-cal, rms=0.083765Jy  sigma=0.929347
! Inverting map 
! Your choice of large map pixels excluded 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 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 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
! Estimated beam: bmin=0.6126 mas, bmaj=1.138 mas, bpa=-1.078 degrees
! Estimated noise=0.562862 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6126 x 1.138 at -1.078 degrees (North through East)
! Clean map  min=-0.001858  max=0.22588 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 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
! Estimated beam: bmin=0.508 mas, bmaj=0.9575 mas, bpa=2.242 degrees
! Estimated noise=0.997044 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.179902 Jy
! Component: 100  -  total flux cleaned = 0.226877 Jy
! Component: 150  -  total flux cleaned = 0.243822 Jy
! Component: 200  -  total flux cleaned = 0.252767 Jy
! Total flux subtracted in 200 components = 0.252767 Jy
! Clean residual min=-0.004477 max=0.005191 Jy/beam
! Clean residual mean=0.000004 rms=0.001063 Jy/beam
! Combined flux in latest and established models = 0.252767 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 15 model components to the UV plane model.
! The established model now contains 15 components and 0.252767 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
! Estimated beam: bmin=0.6126 mas, bmaj=1.138 mas, bpa=-1.078 degrees
! Estimated noise=0.562862 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 = 0.00691289 Jy
! Component: 100  -  total flux cleaned = 0.0110584 Jy
! Component: 150  -  total flux cleaned = 0.0136833 Jy
! Component: 200  -  total flux cleaned = 0.0149466 Jy
! Total flux subtracted in 200 components = 0.0149466 Jy
! Clean residual min=-0.002246 max=0.002272 Jy/beam
! Clean residual mean=0.000002 rms=0.000536 Jy/beam
! Combined flux in latest and established models = 0.267714 Jy
! Adding 23 model components to the UV plane model.
! The established model now contains 32 components and 0.267714 Jy
! Inverting map 
! Your choice of large map pixels excluded 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 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 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
! Estimated beam: bmin=2.811 mas, bmaj=2.985 mas, bpa=-9.81 degrees
! Estimated noise=0.699452 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00254032 Jy
! Component: 100  -  total flux cleaned = 0.00397801 Jy
! Component: 150  -  total flux cleaned = 0.00498184 Jy
! Component: 200  -  total flux cleaned = 0.00571859 Jy
! Total flux subtracted in 200 components = 0.00571859 Jy
! Clean residual min=-0.002046 max=0.001911 Jy/beam
! Clean residual mean=0.000003 rms=0.000587 Jy/beam
! Combined flux in latest and established models = 0.273433 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 = 0.000555492 Jy
! Component: 100  -  total flux cleaned = 0.000952084 Jy
! Component: 150  -  total flux cleaned = 0.00105455 Jy
! Component: 200  -  total flux cleaned = 0.00109566 Jy
! Total flux subtracted in 200 components = 0.00109566 Jy
! Clean residual min=-0.002024 max=0.001941 Jy/beam
! Clean residual mean=0.000002 rms=0.000577 Jy/beam
! Combined flux in latest and established models = 0.274528 Jy
! Adding 20 model components to the UV plane model.
! The established model now contains 49 components and 0.274528 Jy
! Inverting map 
! Your choice of large map pixels excluded 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
! Estimated beam: bmin=0.6126 mas, bmaj=1.138 mas, bpa=-1.078 degrees
! Estimated noise=0.562862 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00109695 Jy
! Component: 100  -  total flux cleaned = -0.00139869 Jy
! Component: 150  -  total flux cleaned = -0.00155916 Jy
! Component: 200  -  total flux cleaned = -0.00160711 Jy
! Total flux subtracted in 200 components = -0.00160711 Jy
! Clean residual min=-0.002023 max=0.002190 Jy/beam
! Clean residual mean=0.000001 rms=0.000484 Jy/beam
! Combined flux in latest and established models = 0.272921 Jy
selfcal
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 59 components and 0.272921 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.084007Jy  sigma=0.930606
! Fit after  self-cal, rms=0.083964Jy  sigma=0.930417
wmodel J2145+1115_X_map.mod
! Writing 59 model components to file: J2145+1115_X_map.mod
wobs   J2145+1115_X_uvs.fits
! Writing UV FITS file: J2145+1115_X_uvs.fits
wwins  J2145+1115_X_map.win
! wwins: Wrote 5 windows to J2145+1115_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 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
! clean: niter=4096  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 4.94695e-05 Jy
! Component: 100  -  total flux cleaned = 1.27893e-05 Jy
! Component: 150  -  total flux cleaned = 0.000117945 Jy
! Component: 200  -  total flux cleaned = 0.000185079 Jy
! Component: 250  -  total flux cleaned = 0.000184676 Jy
! Component: 300  -  total flux cleaned = 5.70435e-05 Jy
! Component: 350  -  total flux cleaned = -5.7938e-06 Jy
! Component: 400  -  total flux cleaned = 2.49294e-05 Jy
! Component: 450  -  total flux cleaned = -9.55389e-05 Jy
! Component: 500  -  total flux cleaned = -6.90828e-06 Jy
! Component: 550  -  total flux cleaned = -3.62262e-05 Jy
! Component: 600  -  total flux cleaned = -6.5056e-05 Jy
! Component: 650  -  total flux cleaned = -6.51431e-05 Jy
! Component: 700  -  total flux cleaned = -9.08577e-06 Jy
! Component: 750  -  total flux cleaned = -3.70539e-05 Jy
! Component: 800  -  total flux cleaned = -9.18378e-05 Jy
! Component: 850  -  total flux cleaned = -6.47174e-05 Jy
! Component: 900  -  total flux cleaned = 4.20114e-05 Jy
! Component: 950  -  total flux cleaned = -1.07388e-05 Jy
! Component: 1000  -  total flux cleaned = 4.14932e-05 Jy
! Component: 1050  -  total flux cleaned = -8.81596e-05 Jy
! Component: 1100  -  total flux cleaned = -3.64935e-05 Jy
! Component: 1150  -  total flux cleaned = 1.43663e-05 Jy
! Component: 1200  -  total flux cleaned = -1.10959e-05 Jy
! Component: 1250  -  total flux cleaned = 1.38267e-05 Jy
! Component: 1300  -  total flux cleaned = 3.8288e-05 Jy
! Component: 1350  -  total flux cleaned = -6.01254e-05 Jy
! Component: 1400  -  total flux cleaned = -1.13313e-05 Jy
! Component: 1450  -  total flux cleaned = 1.29539e-05 Jy
! Component: 1500  -  total flux cleaned = -8.32965e-05 Jy
! Component: 1550  -  total flux cleaned = 6.0128e-05 Jy
! Component: 1600  -  total flux cleaned = -3.44811e-05 Jy
! Component: 1650  -  total flux cleaned = 3.60575e-05 Jy
! Component: 1700  -  total flux cleaned = -5.73523e-05 Jy
! Component: 1750  -  total flux cleaned = -3.41242e-05 Jy
! Component: 1800  -  total flux cleaned = -1.09348e-05 Jy
! Component: 1850  -  total flux cleaned = 1.20442e-05 Jy
! Component: 1900  -  total flux cleaned = 3.48677e-05 Jy
! Component: 1950  -  total flux cleaned = 3.46931e-05 Jy
! Component: 2000  -  total flux cleaned = -3.24018e-05 Jy
! Component: 2050  -  total flux cleaned = 1.24223e-05 Jy
! Component: 2100  -  total flux cleaned = 5.67468e-05 Jy
! Component: 2150  -  total flux cleaned = -7.54149e-05 Jy
! Component: 2200  -  total flux cleaned = 1.21928e-05 Jy
! Component: 2250  -  total flux cleaned = 3.41462e-05 Jy
! Component: 2300  -  total flux cleaned = 3.41741e-05 Jy
! Component: 2350  -  total flux cleaned = 7.74153e-05 Jy
! Component: 2400  -  total flux cleaned = 1.31705e-05 Jy
! Component: 2450  -  total flux cleaned = -9.33183e-05 Jy
! Component: 2500  -  total flux cleaned = -5.06284e-05 Jy
! Component: 2550  -  total flux cleaned = -8.32226e-06 Jy
! Component: 2600  -  total flux cleaned = 3.36148e-05 Jy
! Component: 2650  -  total flux cleaned = -8.13979e-06 Jy
! Component: 2700  -  total flux cleaned = 3.34971e-05 Jy
! Component: 2750  -  total flux cleaned = 3.35754e-05 Jy
! Component: 2800  -  total flux cleaned = 0.000136227 Jy
! Component: 2850  -  total flux cleaned = 0.000136272 Jy
! Component: 2900  -  total flux cleaned = 0.000136226 Jy
! Component: 2950  -  total flux cleaned = 0.00019684 Jy
! Component: 3000  -  total flux cleaned = 0.000176624 Jy
! Component: 3050  -  total flux cleaned = 0.000196686 Jy
! Component: 3100  -  total flux cleaned = 0.000216772 Jy
! Component: 3150  -  total flux cleaned = 0.000157118 Jy
! Component: 3200  -  total flux cleaned = 0.000196681 Jy
! Component: 3250  -  total flux cleaned = 0.000275601 Jy
! Component: 3300  -  total flux cleaned = 0.000334294 Jy
! Component: 3350  -  total flux cleaned = 0.000295329 Jy
! Component: 3400  -  total flux cleaned = 0.000314749 Jy
! Component: 3450  -  total flux cleaned = 0.00027599 Jy
! Component: 3500  -  total flux cleaned = 0.000256518 Jy
! Component: 3550  -  total flux cleaned = 0.000352432 Jy
! Component: 3600  -  total flux cleaned = 0.00033342 Jy
! Component: 3650  -  total flux cleaned = 0.000352481 Jy
! Component: 3700  -  total flux cleaned = 0.000276755 Jy
! Component: 3750  -  total flux cleaned = 0.000295663 Jy
! Component: 3800  -  total flux cleaned = 0.000389586 Jy
! Component: 3850  -  total flux cleaned = 0.000370853 Jy
! Component: 3900  -  total flux cleaned = 0.000426842 Jy
! Component: 3950  -  total flux cleaned = 0.00044527 Jy
! Component: 4000  -  total flux cleaned = 0.000426799 Jy
! Component: 4050  -  total flux cleaned = 0.000371657 Jy
! Total flux subtracted in 4096 components = 0.000353379 Jy
! Clean residual min=-0.001163 max=0.001240 Jy/beam
! Clean residual mean=0.000000 rms=0.000295 Jy/beam
! Combined flux in latest and established models = 0.273274 Jy
keep
! Adding 326 model components to the UV plane model.
! The established model now contains 385 components and 0.273275 Jy
![Exited script file: /opt64/bin/pima_mupet_01.dfm]
wmap   /scr/pima/rv118_uvs/J2145+1115_X_map.fits
! Inverting map 
! Your choice of large map pixels excluded 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6126 x 1.138 at -1.078 degrees (North through East)
! Clean map  min=-0.0014672  max=0.22591 Jy/beam
! Writing clean map to FITS file: /scr/pima/rv118_uvs/J2145+1115_X_map.fits
wmodel /scr/pima/rv118_uvs/J2145+1115_X_map.mod
! Writing 385 model components to file: /scr/pima/rv118_uvs/J2145+1115_X_map.mod
wobs   /scr/pima/rv118_uvs/J2145+1115_X_uvs.fits
! Writing UV FITS file: /scr/pima/rv118_uvs/J2145+1115_X_uvs.fits
wwins  /scr/pima/rv118_uvs/J2145+1115_X_map.win
! wwins: Wrote 6 windows to /scr/pima/rv118_uvs/J2145+1115_X_map.win
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is", peak_flux
! The peak flux is 0.225915 
invert
! Inverting map 
! Your choice of large map pixels excluded 6.81% of the data.
!  The x-axis pixel size should ideally be below 0.1666 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000295271 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.392101 0.392101 0.784201 1.5684 3.13681 6.27361 12.5472 25.0944 50.1889
print "clev=      ", int(3*image_rms*10000)/10000
! clev=       0.0008 
print "peak=      ", int(1000*peak_flux)/1000
! peak=       0.225 
print "dyn_range= ", int(1000*peak_flux/image_rms)/1000
! dyn_range=  765.109 
quit
! Quitting program
! Log file /scr/pima/rv118_uvs/J2145+1115_X_dfm.log closed on Sun Dec 10 00:11:45 2017