! Started logfile: /scr/pima/bg219g_uvs/J1751-1950_S_uvs.log on Thu Apr  7 07:22:06 2016
obs /scr/pima/bg219g_uvs/J1751-1950_S_uva.fits
! Reading UV FITS file: /scr/pima/bg219g_uvs/J1751-1950_S_uva.fits
! AN table 1: 31 integrations on 15 of 15 possible baselines.
! Apparent sampling: 0.675269 visibilities/baseline/integration-bin.
! Found source: J1751-1950
! 
! 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     2.22e+09      3.2e+07          1      3.2e+07
!  02        2    2.252e+09      3.2e+07          1      3.2e+07
!  03        3    2.284e+09      3.2e+07          1      3.2e+07
!  04        4    2.348e+09      3.2e+07          1      3.2e+07
! 
! Polarization(s): RR
! 
! Read 54 lines of history.
! 
! Reading 1256 visibilities.
select rr, 1,2,3,4,6,7,8 
! 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 = 0.5 
print "taper_size =", taper_size
! taper_size = 20 
![@/home/lpetrov/bin/01_muppet /scr/pima/bg219g_uvs/J1751-1950_S]
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 0.500x0.500 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 46 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 46 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 46 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 46 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=1.010623Jy  sigma=19.417914
! Fit after  self-cal, rms=0.937427Jy  sigma=17.922052
! 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 
! Estimated beam: bmin=16.36 mas, bmaj=23.73 mas, bpa=27.21 degrees
! Estimated noise=1.59211 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=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0539883 Jy
! Component: 100  -  total flux cleaned = 0.0635256 Jy
! Total flux subtracted in 100 components = 0.0635256 Jy
! Clean residual min=-0.005912 max=0.006022 Jy/beam
! Clean residual mean=0.000007 rms=0.002656 Jy/beam
! Combined flux in latest and established models = 0.0635256 Jy
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 19 components and 0.0635256 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.070662Jy  sigma=1.212844
! Fit after  self-cal, rms=0.069464Jy  sigma=1.195404
! Inverting map 
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 
! Estimated beam: bmin=17.34 mas, bmaj=23.46 mas, bpa=19.6 degrees
! Estimated noise=1.17333 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 = 0.00137696 Jy
! Component: 100  -  total flux cleaned = 0.0016098 Jy
! Component: 150  -  total flux cleaned = 0.00172115 Jy
! Component: 200  -  total flux cleaned = 0.00180892 Jy
! Total flux subtracted in 200 components = 0.00180892 Jy
! Clean residual min=-0.001360 max=0.001363 Jy/beam
! Clean residual mean=0.000014 rms=0.000562 Jy/beam
! Combined flux in latest and established models = 0.0653346 Jy
! Performing phase self-cal
! Adding 86 model components to the UV plane model.
! The established model now contains 105 components and 0.0653345 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.069056Jy  sigma=1.188353
! Fit after  self-cal, rms=0.069003Jy  sigma=1.187749
! Inverting map 
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 17.34 x 23.46 at 19.6 degrees (North through East)
! Clean map  min=-0.0036428  max=0.060986 Jy/beam
if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val
! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2.
! Selfcal phase corrections will not be limited.
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    KP        1.00*    LA        1.00*    NL        1.00*    
!   OV        1.00*    PT        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.93     KP        0.93     LA        0.98     NL        1.00*    
!   OV        1.01     PT        1.07     
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.06     KP        1.00     LA        1.08     NL        1.00*    
!   OV        0.96     PT        1.00     
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.96     KP        0.90     LA        1.05     NL        1.00*    
!   OV        1.05     PT        0.93     
! 
! 
! Fit before self-cal, rms=0.069003Jy  sigma=1.187749
! Fit after  self-cal, rms=0.067914Jy  sigma=1.185425
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=17.4 mas, bmaj=23.34 mas, bpa=20.63 degrees
! Estimated noise=1.15708 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 = -0.000850975 Jy
! Component: 100  -  total flux cleaned = -0.000696419 Jy
! Component: 150  -  total flux cleaned = -0.000486863 Jy
! Component: 200  -  total flux cleaned = -0.000305541 Jy
! Total flux subtracted in 200 components = -0.000305541 Jy
! Clean residual min=-0.000954 max=0.000945 Jy/beam
! Clean residual mean=0.000008 rms=0.000367 Jy/beam
! Combined flux in latest and established models = 0.065029 Jy
! Performing phase self-cal
! Adding 71 model components to the UV plane model.
! The established model now contains 170 components and 0.065029 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067721Jy  sigma=1.182600
! Fit after  self-cal, rms=0.067753Jy  sigma=1.182053
! Inverting map 
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=0.067753Jy  sigma=1.182053
! Fit after  self-cal, rms=0.067398Jy  sigma=1.179104
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=17.4 mas, bmaj=23.34 mas, bpa=20.75 degrees
! Estimated noise=1.14533 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000555735 Jy
! Component: 100  -  total flux cleaned = 0.000970516 Jy
! Component: 150  -  total flux cleaned = 0.00141715 Jy
! Component: 200  -  total flux cleaned = 0.00171723 Jy
! Total flux subtracted in 200 components = 0.00171723 Jy
! Clean residual min=-0.000608 max=0.000610 Jy/beam
! Clean residual mean=0.000003 rms=0.000207 Jy/beam
! Combined flux in latest and established models = 0.0667462 Jy
selfcal
! Performing phase self-cal
! Adding 45 model components to the UV plane model.
! The established model now contains 214 components and 0.0667462 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067323Jy  sigma=1.178504
! Fit after  self-cal, rms=0.067438Jy  sigma=1.177429
flux_cutoff = imstat(rms) * dynam
! Inverting map 
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 = -0.00029806 Jy
! Component: 100  -  total flux cleaned = -0.000371555 Jy
! Component: 150  -  total flux cleaned = -0.000275239 Jy
! Component: 200  -  total flux cleaned = -0.000180627 Jy
! Total flux subtracted in 200 components = -0.000180627 Jy
! Clean residual min=-0.000522 max=0.000518 Jy/beam
! Clean residual mean=0.000001 rms=0.000187 Jy/beam
! Combined flux in latest and established models = 0.0665656 Jy
! Performing phase self-cal
! Adding 67 model components to the UV plane model.
! The established model now contains 278 components and 0.0665655 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067393Jy  sigma=1.176927
! Fit after  self-cal, rms=0.067415Jy  sigma=1.176838
! Inverting map 
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=0.067415Jy  sigma=1.176838
! Fit after  self-cal, rms=0.067520Jy  sigma=1.176569
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=17.39 mas, bmaj=23.31 mas, bpa=21.01 degrees
! Estimated noise=1.14047 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000146198 Jy
! Component: 100  -  total flux cleaned = 0.000177122 Jy
! Component: 150  -  total flux cleaned = 0.000292452 Jy
! Component: 200  -  total flux cleaned = 0.00026387 Jy
! Total flux subtracted in 200 components = 0.00026387 Jy
! Clean residual min=-0.000465 max=0.000465 Jy/beam
! Clean residual mean=0.000000 rms=0.000165 Jy/beam
! Combined flux in latest and established models = 0.0668294 Jy
selfcal
! Performing phase self-cal
! Adding 51 model components to the UV plane model.
! The established model now contains 324 components and 0.0668294 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067484Jy  sigma=1.176257
! Fit after  self-cal, rms=0.067551Jy  sigma=1.176189
flux_cutoff = imstat(rms) * dynam
! Inverting map 
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 = 0.00013525 Jy
! Component: 100  -  total flux cleaned = 0.000212907 Jy
! Component: 150  -  total flux cleaned = 0.000237242 Jy
! Component: 200  -  total flux cleaned = 0.000211268 Jy
! Total flux subtracted in 200 components = 0.000211268 Jy
! Clean residual min=-0.000453 max=0.000448 Jy/beam
! Clean residual mean=0.000001 rms=0.000159 Jy/beam
! Combined flux in latest and established models = 0.0670407 Jy
! Performing phase self-cal
! Adding 70 model components to the UV plane model.
! The established model now contains 379 components and 0.0670407 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067522Jy  sigma=1.175978
! Fit after  self-cal, rms=0.067540Jy  sigma=1.175957
! Inverting map 
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 20 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=0.067540Jy  sigma=1.175957
! Fit after  self-cal, rms=0.067651Jy  sigma=1.175891
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=17.67 mas, bmaj=23.43 mas, bpa=20.84 degrees
! Estimated noise=1.13941 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000395717 Jy
! Component: 100  -  total flux cleaned = 0.000625057 Jy
! Component: 150  -  total flux cleaned = 0.000823124 Jy
! Component: 200  -  total flux cleaned = 0.00087221 Jy
! Total flux subtracted in 200 components = 0.00087221 Jy
! Clean residual min=-0.000409 max=0.000411 Jy/beam
! Clean residual mean=0.000000 rms=0.000151 Jy/beam
! Combined flux in latest and established models = 0.0679129 Jy
selfcal
! Performing phase self-cal
! Adding 63 model components to the UV plane model.
! The established model now contains 427 components and 0.0679129 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067621Jy  sigma=1.175688
! Fit after  self-cal, rms=0.067655Jy  sigma=1.175667
flux_cutoff = imstat(rms) * dynam
! Inverting map 
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 = 0.00019662 Jy
! Component: 100  -  total flux cleaned = 0.000150302 Jy
! Component: 150  -  total flux cleaned = 0.000104272 Jy
! Component: 200  -  total flux cleaned = 7.55271e-05 Jy
! Total flux subtracted in 200 components = 7.55271e-05 Jy
! Clean residual min=-0.000422 max=0.000424 Jy/beam
! Clean residual mean=0.000000 rms=0.000151 Jy/beam
! Combined flux in latest and established models = 0.0679884 Jy
! Performing phase self-cal
! Adding 61 model components to the UV plane model.
! The established model now contains 472 components and 0.0679885 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067631Jy  sigma=1.175492
! Fit after  self-cal, rms=0.067646Jy  sigma=1.175475
! Inverting map 
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 
! Estimated beam: bmin=17.39 mas, bmaj=23.27 mas, bpa=21.38 degrees
! Estimated noise=1.13976 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 17.39 x 23.27 at 21.38 degrees (North through East)
! Clean map  min=-0.0034734  max=0.059864 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 
! Estimated beam: bmin=16.4 mas, bmaj=23.64 mas, bpa=27.75 degrees
! Estimated noise=1.5616 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0535809 Jy
! Component: 100  -  total flux cleaned = 0.0631064 Jy
! Component: 150  -  total flux cleaned = 0.0640067 Jy
! Component: 200  -  total flux cleaned = 0.0639781 Jy
! Total flux subtracted in 200 components = 0.0639781 Jy
! Clean residual min=-0.003853 max=0.003754 Jy/beam
! Clean residual mean=0.000020 rms=0.001537 Jy/beam
! Combined flux in latest and established models = 0.0639781 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 46 model components to the UV plane model.
! The established model now contains 46 components and 0.0639781 Jy
! Inverting map and beam 
! Estimated beam: bmin=17.39 mas, bmaj=23.27 mas, bpa=21.38 degrees
! Estimated noise=1.13976 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 = -0.00365569 Jy
! Component: 100  -  total flux cleaned = -0.00390684 Jy
! Component: 150  -  total flux cleaned = -0.00410998 Jy
! Component: 200  -  total flux cleaned = -0.00504825 Jy
! Total flux subtracted in 200 components = -0.00504825 Jy
! Clean residual min=-0.001337 max=0.001333 Jy/beam
! Clean residual mean=0.000008 rms=0.000483 Jy/beam
! Combined flux in latest and established models = 0.0589299 Jy
! Adding 62 model components to the UV plane model.
! The established model now contains 108 components and 0.0589299 Jy
! Inverting map 
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 20 mega-wavelengths.
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=17.67 mas, bmaj=23.43 mas, bpa=20.84 degrees
! Estimated noise=1.13941 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000586985 Jy
! Component: 100  -  total flux cleaned = 0.000535452 Jy
! Component: 150  -  total flux cleaned = 0.000578691 Jy
! Component: 200  -  total flux cleaned = 0.000373904 Jy
! Total flux subtracted in 200 components = 0.000373904 Jy
! Clean residual min=-0.000683 max=0.000685 Jy/beam
! Clean residual mean=0.000005 rms=0.000243 Jy/beam
! Combined flux in latest and established models = 0.0593038 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 = -0.000206302 Jy
! Component: 100  -  total flux cleaned = -0.000425604 Jy
! Component: 150  -  total flux cleaned = -0.000611494 Jy
! Component: 200  -  total flux cleaned = -0.00076349 Jy
! Total flux subtracted in 200 components = -0.00076349 Jy
! Clean residual min=-0.000895 max=0.000895 Jy/beam
! Clean residual mean=0.000004 rms=0.000297 Jy/beam
! Combined flux in latest and established models = 0.0585403 Jy
! Adding 90 model components to the UV plane model.
! The established model now contains 198 components and 0.0585403 Jy
! Inverting map 
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Estimated beam: bmin=17.39 mas, bmaj=23.27 mas, bpa=21.38 degrees
! Estimated noise=1.13976 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000161094 Jy
! Component: 100  -  total flux cleaned = 6.17213e-05 Jy
! Component: 150  -  total flux cleaned = 0.000153234 Jy
! Component: 200  -  total flux cleaned = 0.000212691 Jy
! Total flux subtracted in 200 components = 0.000212691 Jy
! Clean residual min=-0.000490 max=0.000490 Jy/beam
! Clean residual mean=0.000002 rms=0.000193 Jy/beam
! Combined flux in latest and established models = 0.058753 Jy
selfcal
! Performing phase self-cal
! Adding 72 model components to the UV plane model.
! The established model now contains 269 components and 0.058753 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067666Jy  sigma=1.176012
! Fit after  self-cal, rms=0.067685Jy  sigma=1.175820
wmodel /scr/pima/bg219g_uvs/J1751-1950_S_map.mod
! Writing 269 model components to file: /scr/pima/bg219g_uvs/J1751-1950_S_map.mod
wobs /scr/pima/bg219g_uvs/J1751-1950_S_uvs.fits
! Writing UV FITS file: /scr/pima/bg219g_uvs/J1751-1950_S_uvs.fits
wwins /scr/pima/bg219g_uvs/J1751-1950_S_map.win
! wwins: No CLEAN windows to write.
! Error occured in command: wwins
![Exited script file: /home/lpetrov/bin/01_muppet]
! 
wmap "/scr/pima/bg219g_uvs/J1751-1950_S\_map.fits"
! Inverting map 
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 17.39 x 23.27 at 21.38 degrees (North through East)
! Clean map  min=-0.0056462  max=0.057452 Jy/beam
! Writing clean map to FITS file: /scr/pima/bg219g_uvs/J1751-1950_S_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.0574517 
invert
! Inverting map 
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000178968 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.934532 0.934532 1.86906 3.73813 7.47626 14.9525 29.905 59.8101
print "clev=      ", int(3*image_rms*10000)/10000
! clev=       0.0005 
print "peak=      ", int(1000*peak_flux)/1000
! peak=       0.057 
print "dyn_range= ", int(1000*peak_flux/image_rms)/1000
! dyn_range=  321.016 
quit
! Quitting program
! Log file /scr/pima/bg219g_uvs/J1751-1950_S_uvs.log closed on Thu Apr  7 07:22:08 2016