! Started logfile: /scr/pima/bg219b_uvs/J1508-4953_S_uvs.log on Thu Apr  7 01:25:46 2016
obs /scr/pima/bg219b_uvs/J1508-4953_S_uva.fits
! Reading UV FITS file: /scr/pima/bg219b_uvs/J1508-4953_S_uva.fits
! AN table 1: 29 integrations on 6 of 6 possible baselines.
! Apparent sampling: 0.83908 visibilities/baseline/integration-bin.
! Found source: J1508-4953
! 
! 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 584 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/bg219b_uvs/J1508-4953_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 29 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 29 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 29 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 29 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=1.105317Jy  sigma=14.138865
! Fit after  self-cal, rms=0.393922Jy  sigma=5.101406
! 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=21.97 mas, bmaj=209 mas, bpa=10.2 degrees
! Estimated noise=2.65097 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 = 0.480317 Jy
! Component: 100  -  total flux cleaned = 0.585057 Jy
! Total flux subtracted in 100 components = 0.585057 Jy
! Clean residual min=-0.013835 max=0.029212 Jy/beam
! Clean residual mean=-0.000505 rms=0.008674 Jy/beam
! Combined flux in latest and established models = 0.585057 Jy
! Performing phase self-cal
! Adding 3 model components to the UV plane model.
! The established model now contains 3 components and 0.585057 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.096568Jy  sigma=1.203794
! Fit after  self-cal, rms=0.096567Jy  sigma=1.203779
! 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=21.4 mas, bmaj=217.4 mas, bpa=10.69 degrees
! Estimated noise=2.56066 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 = 0.0212221 Jy
! Component: 100  -  total flux cleaned = 0.0257048 Jy
! Component: 150  -  total flux cleaned = 0.0268234 Jy
! Component: 200  -  total flux cleaned = 0.0271909 Jy
! Total flux subtracted in 200 components = 0.0271909 Jy
! Clean residual min=-0.006285 max=0.006384 Jy/beam
! Clean residual mean=0.000066 rms=0.002228 Jy/beam
! Combined flux in latest and established models = 0.612248 Jy
! Performing phase self-cal
! Adding 54 model components to the UV plane model.
! The established model now contains 57 components and 0.612248 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.089855Jy  sigma=1.123059
! Fit after  self-cal, rms=0.089769Jy  sigma=1.122531
! Inverting map 
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 21.4 x 217.4 at 10.69 degrees (North through East)
! Clean map  min=-0.0062737  max=0.60998 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.
!  A total of 15 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   FD        1.01     KP        0.99     LA        1.01     PT        0.99     
! 
! 
! Correcting IF 2.
!  A total of 15 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   FD        1.01     KP        0.99     LA        1.02     PT        1.02     
! 
! 
! Correcting IF 3.
!  A total of 15 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   FD        0.99     KP        1.03     LA        1.02     PT        0.97     
! 
! 
! Correcting IF 4.
!  A total of 15 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   FD        1.01     KP        0.96     LA        0.97     PT        0.99     
! 
! 
! Fit before self-cal, rms=0.089769Jy  sigma=1.122531
! Fit after  self-cal, rms=0.088008Jy  sigma=1.111903
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=21.77 mas, bmaj=215.4 mas, bpa=10.64 degrees
! Estimated noise=2.72586 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 = 0.00292664 Jy
! Component: 100  -  total flux cleaned = 0.00263287 Jy
! Component: 150  -  total flux cleaned = 0.00294522 Jy
! Component: 200  -  total flux cleaned = 0.00317977 Jy
! Total flux subtracted in 200 components = 0.00317977 Jy
! Clean residual min=-0.002073 max=0.002098 Jy/beam
! Clean residual mean=-0.000036 rms=0.000783 Jy/beam
! Combined flux in latest and established models = 0.615428 Jy
! Performing phase self-cal
! Adding 87 model components to the UV plane model.
! The established model now contains 144 components and 0.615428 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087808Jy  sigma=1.108733
! Fit after  self-cal, rms=0.087837Jy  sigma=1.108418
! 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=0.087837Jy  sigma=1.108418
! Fit after  self-cal, rms=0.087607Jy  sigma=1.108130
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=21.77 mas, bmaj=215.4 mas, bpa=10.65 degrees
! Estimated noise=2.72054 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000415162 Jy
! Component: 100  -  total flux cleaned = 0.00012806 Jy
! Component: 150  -  total flux cleaned = -0.000178673 Jy
! Component: 200  -  total flux cleaned = -9.24902e-05 Jy
! Total flux subtracted in 200 components = -9.24902e-05 Jy
! Clean residual min=-0.001568 max=0.001522 Jy/beam
! Clean residual mean=0.000056 rms=0.000609 Jy/beam
! Combined flux in latest and established models = 0.615336 Jy
selfcal
! Performing phase self-cal
! Adding 46 model components to the UV plane model.
! The established model now contains 189 components and 0.615336 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087523Jy  sigma=1.107126
! Fit after  self-cal, rms=0.087504Jy  sigma=1.107023
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 = 0.000768725 Jy
! Component: 100  -  total flux cleaned = 0.00112068 Jy
! Component: 150  -  total flux cleaned = 0.0014235 Jy
! Component: 200  -  total flux cleaned = 0.00153373 Jy
! Total flux subtracted in 200 components = 0.00153373 Jy
! Clean residual min=-0.002015 max=0.002038 Jy/beam
! Clean residual mean=-0.000030 rms=0.000719 Jy/beam
! Combined flux in latest and established models = 0.61687 Jy
! Performing phase self-cal
! Adding 50 model components to the UV plane model.
! The established model now contains 229 components and 0.61687 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087466Jy  sigma=1.106203
! Fit after  self-cal, rms=0.087476Jy  sigma=1.105904
! 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=0.087476Jy  sigma=1.105904
! Fit after  self-cal, rms=0.087355Jy  sigma=1.105645
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=21.78 mas, bmaj=215.3 mas, bpa=10.64 degrees
! Estimated noise=2.71846 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000112813 Jy
! Component: 100  -  total flux cleaned = -0.000173365 Jy
! Component: 150  -  total flux cleaned = -0.000166853 Jy
! Component: 200  -  total flux cleaned = -7.37966e-05 Jy
! Total flux subtracted in 200 components = -7.37966e-05 Jy
! Clean residual min=-0.001570 max=0.001550 Jy/beam
! Clean residual mean=0.000040 rms=0.000598 Jy/beam
! Combined flux in latest and established models = 0.616796 Jy
selfcal
! Performing phase self-cal
! Adding 33 model components to the UV plane model.
! The established model now contains 254 components and 0.616796 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087300Jy  sigma=1.105284
! Fit after  self-cal, rms=0.087275Jy  sigma=1.105158
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 = -0.000208125 Jy
! Component: 100  -  total flux cleaned = 0.000123875 Jy
! Component: 150  -  total flux cleaned = 0.000496568 Jy
! Component: 200  -  total flux cleaned = 0.000833278 Jy
! Total flux subtracted in 200 components = 0.000833278 Jy
! Clean residual min=-0.001498 max=0.001515 Jy/beam
! Clean residual mean=-0.000032 rms=0.000554 Jy/beam
! Combined flux in latest and established models = 0.617629 Jy
! Performing phase self-cal
! Adding 61 model components to the UV plane model.
! The established model now contains 297 components and 0.617629 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087249Jy  sigma=1.104489
! Fit after  self-cal, rms=0.087259Jy  sigma=1.104398
! 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=0.087259Jy  sigma=1.104398
! Fit after  self-cal, rms=0.087202Jy  sigma=1.104263
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=22.09 mas, bmaj=214.3 mas, bpa=10.65 degrees
! Estimated noise=2.71887 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000723937 Jy
! Component: 100  -  total flux cleaned = 0.000630928 Jy
! Component: 150  -  total flux cleaned = 0.000686437 Jy
! Component: 200  -  total flux cleaned = 0.000752036 Jy
! Total flux subtracted in 200 components = 0.000752036 Jy
! Clean residual min=-0.001076 max=0.001042 Jy/beam
! Clean residual mean=0.000009 rms=0.000392 Jy/beam
! Combined flux in latest and established models = 0.618381 Jy
selfcal
! Performing phase self-cal
! Adding 52 model components to the UV plane model.
! The established model now contains 343 components and 0.618381 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087162Jy  sigma=1.104098
! Fit after  self-cal, rms=0.087148Jy  sigma=1.104049
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 = -6.55778e-05 Jy
! Component: 100  -  total flux cleaned = -2.25099e-05 Jy
! Component: 150  -  total flux cleaned = 6.90803e-05 Jy
! Component: 200  -  total flux cleaned = 6.73395e-05 Jy
! Total flux subtracted in 200 components = 6.73395e-05 Jy
! Clean residual min=-0.000962 max=0.000967 Jy/beam
! Clean residual mean=-0.000011 rms=0.000367 Jy/beam
! Combined flux in latest and established models = 0.618448 Jy
! Performing phase self-cal
! Adding 65 model components to the UV plane model.
! The established model now contains 395 components and 0.618449 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087133Jy  sigma=1.103766
! Fit after  self-cal, rms=0.087138Jy  sigma=1.103710
! 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=21.78 mas, bmaj=215.3 mas, bpa=10.64 degrees
! Estimated noise=2.71769 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 21.78 x 215.3 at 10.64 degrees (North through East)
! Clean map  min=-0.011631  max=0.60744 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
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087138Jy  sigma=1.103710
! Fit after  self-cal, rms=0.069178Jy  sigma=0.848268
! Inverting map and beam 
! Estimated beam: bmin=21.79 mas, bmaj=215.2 mas, bpa=10.63 degrees
! Estimated noise=2.70656 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00086567 Jy
! Component: 100  -  total flux cleaned = -0.00134786 Jy
! Component: 150  -  total flux cleaned = -0.00206128 Jy
! Component: 200  -  total flux cleaned = -0.00241542 Jy
! Total flux subtracted in 200 components = -0.00241542 Jy
! Clean residual min=-0.000608 max=0.000599 Jy/beam
! Clean residual mean=0.000006 rms=0.000278 Jy/beam
! Combined flux in latest and established models = 0.616033 Jy
! Performing phase self-cal
! Adding 100 model components to the UV plane model.
! The established model now contains 487 components and 0.616033 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.069076Jy  sigma=0.847248
! Fit after  self-cal, rms=0.069073Jy  sigma=0.847228
! Inverting map 
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000463461 Jy
! Component: 100  -  total flux cleaned = 0.000493872 Jy
! Component: 150  -  total flux cleaned = 0.000454477 Jy
! Component: 200  -  total flux cleaned = 0.000456345 Jy
! Total flux subtracted in 200 components = 0.000456345 Jy
! Clean residual min=-0.000782 max=0.000764 Jy/beam
! Clean residual mean=-0.000008 rms=0.000316 Jy/beam
! Combined flux in latest and established models = 0.616489 Jy
! Performing phase self-cal
! Adding 63 model components to the UV plane model.
! The established model now contains 535 components and 0.616489 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.069057Jy  sigma=0.846901
! Fit after  self-cal, rms=0.069062Jy  sigma=0.846878
! Inverting map 
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.069062Jy  sigma=0.846878
! Fit after  self-cal, rms=0.068412Jy  sigma=0.836026
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=21.79 mas, bmaj=209.9 mas, bpa=10.18 degrees
! Estimated noise=2.73825 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.474215 Jy
! Component: 100  -  total flux cleaned = 0.577647 Jy
! Component: 150  -  total flux cleaned = 0.592587 Jy
! Component: 200  -  total flux cleaned = 0.593374 Jy
! Total flux subtracted in 200 components = 0.593374 Jy
! Clean residual min=-0.006442 max=0.006528 Jy/beam
! Clean residual mean=-0.000087 rms=0.003278 Jy/beam
! Combined flux in latest and established models = 0.593374 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 40 model components to the UV plane model.
! The established model now contains 40 components and 0.593374 Jy
! Inverting map and beam 
! Estimated beam: bmin=21.81 mas, bmaj=215.2 mas, bpa=10.63 degrees
! Estimated noise=2.70078 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 = 0.00443753 Jy
! Component: 100  -  total flux cleaned = 0.006647 Jy
! Component: 150  -  total flux cleaned = 0.00795154 Jy
! Component: 200  -  total flux cleaned = 0.00797588 Jy
! Total flux subtracted in 200 components = 0.00797588 Jy
! Clean residual min=-0.006018 max=0.005889 Jy/beam
! Clean residual mean=0.000140 rms=0.002104 Jy/beam
! Combined flux in latest and established models = 0.60135 Jy
! Adding 49 model components to the UV plane model.
! The established model now contains 87 components and 0.60135 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=22.12 mas, bmaj=214.2 mas, bpa=10.63 degrees
! Estimated noise=2.70175 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00138642 Jy
! Component: 100  -  total flux cleaned = 0.00138682 Jy
! Component: 150  -  total flux cleaned = 0.00236291 Jy
! Component: 200  -  total flux cleaned = 0.00345164 Jy
! Total flux subtracted in 200 components = 0.00345164 Jy
! Clean residual min=-0.006459 max=0.006569 Jy/beam
! Clean residual mean=-0.000136 rms=0.002682 Jy/beam
! Combined flux in latest and established models = 0.604802 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 = -2.97319e-05 Jy
! Component: 100  -  total flux cleaned = -0.000545724 Jy
! Component: 150  -  total flux cleaned = -0.00116266 Jy
! Component: 200  -  total flux cleaned = -0.00190646 Jy
! Total flux subtracted in 200 components = -0.00190646 Jy
! Clean residual min=-0.012921 max=0.013138 Jy/beam
! Clean residual mean=-0.000259 rms=0.005676 Jy/beam
! Combined flux in latest and established models = 0.602895 Jy
! Adding 69 model components to the UV plane model.
! The established model now contains 156 components and 0.602895 Jy
! Inverting map 
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Estimated beam: bmin=21.81 mas, bmaj=215.2 mas, bpa=10.63 degrees
! Estimated noise=2.70078 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -3.93536e-05 Jy
! Component: 100  -  total flux cleaned = -2.92304e-05 Jy
! Component: 150  -  total flux cleaned = 5.18221e-05 Jy
! Component: 200  -  total flux cleaned = 0.000147507 Jy
! Total flux subtracted in 200 components = 0.000147507 Jy
! Clean residual min=-0.016503 max=0.015971 Jy/beam
! Clean residual mean=0.000086 rms=0.006082 Jy/beam
! Combined flux in latest and established models = 0.603043 Jy
selfcal
! Performing phase self-cal
! Adding 39 model components to the UV plane model.
! The established model now contains 171 components and 0.603043 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.073126Jy  sigma=0.909252
! Fit after  self-cal, rms=0.071863Jy  sigma=0.890918
wmodel /scr/pima/bg219b_uvs/J1508-4953_S_map.mod
! Writing 171 model components to file: /scr/pima/bg219b_uvs/J1508-4953_S_map.mod
wobs /scr/pima/bg219b_uvs/J1508-4953_S_uvs.fits
! Writing UV FITS file: /scr/pima/bg219b_uvs/J1508-4953_S_uvs.fits
wwins /scr/pima/bg219b_uvs/J1508-4953_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/bg219b_uvs/J1508-4953_S\_map.fits"
! Inverting map 
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 21.81 x 215.2 at 10.63 degrees (North through East)
! Clean map  min=-0.017548  max=0.59662 Jy/beam
! Writing clean map to FITS file: /scr/pima/bg219b_uvs/J1508-4953_S_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.596619 
invert
! Inverting map 
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.00647049 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -3.25358 3.25358 6.50716 13.0143 26.0287 52.0573
print "clev=      ", int(3*image_rms*10000)/10000
! clev=       0.0194 
print "peak=      ", int(1000*peak_flux)/1000
! peak=       0.596 
print "dyn_range= ", int(1000*peak_flux/image_rms)/1000
! dyn_range=  92.206 
quit
! Quitting program
! Log file /scr/pima/bg219b_uvs/J1508-4953_S_uvs.log closed on Thu Apr  7 01:25:51 2016