! Started logfile: /scr/pima/bg219a_uvs/J0026+3508_S_dfm.log on Thu May 19 23:44:43 2016
float field_size
field_size =  1024
float field_cell
field_cell =   0.5000
float taper_size
taper_size =   20.0
float freq
freq       =    2.22000
obs     /scr/pima/bg219a_uvs/J0026+3508_S_uva.fits
! Reading UV FITS file: /scr/pima/bg219a_uvs/J0026+3508_S_uva.fits
! AN table 1: 61 integrations on 21 of 21 possible baselines.
! Apparent sampling: 0.466823 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J0026+3508
! 
! 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 49 lines of history.
! 
! Reading 2392 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 = 0.5 
print "taper_size =", taper_size
! taper_size = 20 
![@/opt64/bin/pima_mupet_01.dfm J0026+3508_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 154 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 154 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 154 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 154 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=1.016273Jy  sigma=29.775045
! Fit after  self-cal, rms=0.916938Jy  sigma=27.646980
! 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=3.726 mas, bmaj=10.39 mas, bpa=-30.78 degrees
! Estimated noise=0.778702 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 = 0.0613553 Jy
! Component: 100  -  total flux cleaned = 0.0930377 Jy
! Total flux subtracted in 100 components = 0.0930377 Jy
! Clean residual min=-0.013684 max=0.016993 Jy/beam
! Clean residual mean=0.000044 rms=0.005185 Jy/beam
! Combined flux in latest and established models = 0.0930377 Jy
! Performing phase self-cal
! Adding 29 model components to the UV plane model.
! The established model now contains 29 components and 0.0930377 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.069033Jy  sigma=2.010584
! Fit after  self-cal, rms=0.067905Jy  sigma=1.973234
! 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=4.931 mas, bmaj=10.48 mas, bpa=-30.57 degrees
! Estimated noise=0.541723 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 = 0.0305004 Jy
! Component: 100  -  total flux cleaned = 0.0488065 Jy
! Component: 150  -  total flux cleaned = 0.0557055 Jy
! Component: 200  -  total flux cleaned = 0.0618758 Jy
! Total flux subtracted in 200 components = 0.0618758 Jy
! Clean residual min=-0.007104 max=0.007037 Jy/beam
! Clean residual mean=0.000033 rms=0.003096 Jy/beam
! Combined flux in latest and established models = 0.154913 Jy
! Performing phase self-cal
! Adding 88 model components to the UV plane model.
! The established model now contains 108 components and 0.154913 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.047312Jy  sigma=1.369453
! Fit after  self-cal, rms=0.046704Jy  sigma=1.351774
! Inverting map 
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 4.931 x 10.48 at -30.57 degrees (North through East)
! Clean map  min=-0.01087  max=0.073045 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 21 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.96     LA        0.88     MK        1.08     NL        1.08     
!   OV        1.09     PT        0.84     SC        1.00*    
! 
! 
! Correcting IF 2.
!  A total of 21 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    LA        1.00*    MK        1.00*    NL        1.00*    
!   OV        1.00*    PT        1.00*    SC        1.00*    
! 
! 
! Correcting IF 3.
!  A total of 21 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.91     LA        0.86     MK        1.05     NL        1.05     
!   OV        1.05     PT        0.88     SC        1.00*    
! 
! 
! Correcting IF 4.
!  A total of 21 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.04     LA        0.85     MK        1.02     NL        1.12     
!   OV        0.96     PT        0.85     SC        1.00*    
! 
! 
! Fit before self-cal, rms=0.046704Jy  sigma=1.351774
! Fit after  self-cal, rms=0.041634Jy  sigma=1.272272
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=4.909 mas, bmaj=10.56 mas, bpa=-29.74 degrees
! Estimated noise=0.518518 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 = 0.00356557 Jy
! Component: 100  -  total flux cleaned = 0.00520915 Jy
! Component: 150  -  total flux cleaned = 0.0055044 Jy
! Component: 200  -  total flux cleaned = 0.00564755 Jy
! Total flux subtracted in 200 components = 0.00564755 Jy
! Clean residual min=-0.001605 max=0.001618 Jy/beam
! Clean residual mean=-0.000001 rms=0.000622 Jy/beam
! Combined flux in latest and established models = 0.160561 Jy
! Performing phase self-cal
! Adding 56 model components to the UV plane model.
! The established model now contains 162 components and 0.160561 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.040348Jy  sigma=1.232543
! Fit after  self-cal, rms=0.040326Jy  sigma=1.229662
! 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=0.040326Jy  sigma=1.229662
! Fit after  self-cal, rms=0.039231Jy  sigma=1.206552
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=4.882 mas, bmaj=10.56 mas, bpa=-29.73 degrees
! Estimated noise=0.516415 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00213109 Jy
! Component: 100  -  total flux cleaned = 0.00281631 Jy
! Component: 150  -  total flux cleaned = 0.00368152 Jy
! Component: 200  -  total flux cleaned = 0.00436443 Jy
! Total flux subtracted in 200 components = 0.00436443 Jy
! Clean residual min=-0.000958 max=0.000970 Jy/beam
! Clean residual mean=0.000003 rms=0.000365 Jy/beam
! Combined flux in latest and established models = 0.164925 Jy
selfcal
! Performing phase self-cal
! Adding 59 model components to the UV plane model.
! The established model now contains 215 components and 0.164925 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.038891Jy  sigma=1.196829
! Fit after  self-cal, rms=0.038871Jy  sigma=1.195570
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 = 0.00116562 Jy
! Component: 100  -  total flux cleaned = 0.00183984 Jy
! Component: 150  -  total flux cleaned = 0.00238391 Jy
! Component: 200  -  total flux cleaned = 0.00287912 Jy
! Total flux subtracted in 200 components = 0.00287912 Jy
! Clean residual min=-0.000653 max=0.000658 Jy/beam
! Clean residual mean=0.000000 rms=0.000238 Jy/beam
! Combined flux in latest and established models = 0.167805 Jy
! Performing phase self-cal
! Adding 62 model components to the UV plane model.
! The established model now contains 263 components and 0.167805 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.038746Jy  sigma=1.192296
! Fit after  self-cal, rms=0.038735Jy  sigma=1.191849
! 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=0.038735Jy  sigma=1.191849
! Fit after  self-cal, rms=0.037947Jy  sigma=1.176675
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=4.878 mas, bmaj=10.61 mas, bpa=-29.64 degrees
! Estimated noise=0.511752 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000321122 Jy
! Component: 100  -  total flux cleaned = -0.000401165 Jy
! Component: 150  -  total flux cleaned = -0.000369116 Jy
! Component: 200  -  total flux cleaned = -0.000462804 Jy
! Total flux subtracted in 200 components = -0.000462804 Jy
! Clean residual min=-0.000497 max=0.000497 Jy/beam
! Clean residual mean=-0.000001 rms=0.000168 Jy/beam
! Combined flux in latest and established models = 0.167342 Jy
selfcal
! Performing phase self-cal
! Adding 59 model components to the UV plane model.
! The established model now contains 319 components and 0.167342 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.037887Jy  sigma=1.174769
! Fit after  self-cal, rms=0.037886Jy  sigma=1.174533
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 = -0.000162155 Jy
! Component: 100  -  total flux cleaned = -0.000250254 Jy
! Component: 150  -  total flux cleaned = -0.000304765 Jy
! Component: 200  -  total flux cleaned = -0.000410109 Jy
! Total flux subtracted in 200 components = -0.000410109 Jy
! Clean residual min=-0.000432 max=0.000432 Jy/beam
! Clean residual mean=0.000001 rms=0.000143 Jy/beam
! Combined flux in latest and established models = 0.166932 Jy
! Performing phase self-cal
! Adding 47 model components to the UV plane model.
! The established model now contains 345 components and 0.166932 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.037848Jy  sigma=1.173409
! Fit after  self-cal, rms=0.037847Jy  sigma=1.173323
! 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=0.037847Jy  sigma=1.173323
! Fit after  self-cal, rms=0.037666Jy  sigma=1.173000
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=10.23 mas, bmaj=10.8 mas, bpa=12.09 degrees
! Estimated noise=0.542732 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -9.43941e-05 Jy
! Component: 100  -  total flux cleaned = 3.15327e-05 Jy
! Component: 150  -  total flux cleaned = 0.000190122 Jy
! Component: 200  -  total flux cleaned = 0.000251498 Jy
! Total flux subtracted in 200 components = 0.000251498 Jy
! Clean residual min=-0.000333 max=0.000334 Jy/beam
! Clean residual mean=0.000001 rms=0.000119 Jy/beam
! Combined flux in latest and established models = 0.167183 Jy
selfcal
! Performing phase self-cal
! Adding 47 model components to the UV plane model.
! The established model now contains 387 components and 0.167183 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.037640Jy  sigma=1.172105
! Fit after  self-cal, rms=0.037647Jy  sigma=1.172028
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 = 4.07155e-05 Jy
! Component: 100  -  total flux cleaned = 8.05481e-05 Jy
! Component: 150  -  total flux cleaned = -6.42478e-05 Jy
! Component: 200  -  total flux cleaned = -0.000189751 Jy
! Total flux subtracted in 200 components = -0.000189751 Jy
! Clean residual min=-0.000298 max=0.000297 Jy/beam
! Clean residual mean=0.000002 rms=0.000105 Jy/beam
! Combined flux in latest and established models = 0.166993 Jy
! Performing phase self-cal
! Adding 53 model components to the UV plane model.
! The established model now contains 431 components and 0.166993 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.037631Jy  sigma=1.171573
! Fit after  self-cal, rms=0.037632Jy  sigma=1.171538
! 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=4.879 mas, bmaj=10.62 mas, bpa=-29.59 degrees
! Estimated noise=0.508442 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 4.879 x 10.62 at -29.59 degrees (North through East)
! Clean map  min=-0.0032368  max=0.06621 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=3.703 mas, bmaj=10.33 mas, bpa=-30.38 degrees
! Estimated noise=0.733207 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0574222 Jy
! Component: 100  -  total flux cleaned = 0.0893423 Jy
! Component: 150  -  total flux cleaned = 0.109453 Jy
! Component: 200  -  total flux cleaned = 0.120464 Jy
! Total flux subtracted in 200 components = 0.120464 Jy
! Clean residual min=-0.008613 max=0.008711 Jy/beam
! Clean residual mean=0.000024 rms=0.002907 Jy/beam
! Combined flux in latest and established models = 0.120464 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 63 model components to the UV plane model.
! The established model now contains 63 components and 0.120464 Jy
! Inverting map and beam 
! Estimated beam: bmin=4.879 mas, bmaj=10.62 mas, bpa=-29.59 degrees
! Estimated noise=0.508442 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 = 0.0156909 Jy
! Component: 100  -  total flux cleaned = 0.0241564 Jy
! Component: 150  -  total flux cleaned = 0.0276751 Jy
! Component: 200  -  total flux cleaned = 0.0289992 Jy
! Total flux subtracted in 200 components = 0.0289992 Jy
! Clean residual min=-0.003943 max=0.003945 Jy/beam
! Clean residual mean=0.000011 rms=0.001604 Jy/beam
! Combined flux in latest and established models = 0.149463 Jy
! Adding 89 model components to the UV plane model.
! The established model now contains 145 components and 0.149463 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=10.23 mas, bmaj=10.8 mas, bpa=12.09 degrees
! Estimated noise=0.542732 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00286565 Jy
! Component: 100  -  total flux cleaned = 0.00360766 Jy
! Component: 150  -  total flux cleaned = 0.00479358 Jy
! Component: 200  -  total flux cleaned = 0.00708253 Jy
! Total flux subtracted in 200 components = 0.00708253 Jy
! Clean residual min=-0.001821 max=0.001833 Jy/beam
! Clean residual mean=0.000011 rms=0.000909 Jy/beam
! Combined flux in latest and established models = 0.156546 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 = 0.00173048 Jy
! Component: 100  -  total flux cleaned = 0.00313285 Jy
! Component: 150  -  total flux cleaned = 0.00428167 Jy
! Component: 200  -  total flux cleaned = 0.00508869 Jy
! Total flux subtracted in 200 components = 0.00508869 Jy
! Clean residual min=-0.001077 max=0.001068 Jy/beam
! Clean residual mean=0.000015 rms=0.000488 Jy/beam
! Combined flux in latest and established models = 0.161634 Jy
! Adding 187 model components to the UV plane model.
! The established model now contains 323 components and 0.161634 Jy
! Inverting map 
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Estimated beam: bmin=4.879 mas, bmaj=10.62 mas, bpa=-29.59 degrees
! Estimated noise=0.508442 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00095488 Jy
! Component: 100  -  total flux cleaned = 0.00145071 Jy
! Component: 150  -  total flux cleaned = 0.00210438 Jy
! Component: 200  -  total flux cleaned = 0.00249552 Jy
! Total flux subtracted in 200 components = 0.00249552 Jy
! Clean residual min=-0.000777 max=0.000781 Jy/beam
! Clean residual mean=0.000001 rms=0.000270 Jy/beam
! Combined flux in latest and established models = 0.16413 Jy
selfcal
! Performing phase self-cal
! Adding 44 model components to the UV plane model.
! The established model now contains 367 components and 0.16413 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.037792Jy  sigma=1.175014
! Fit after  self-cal, rms=0.037777Jy  sigma=1.174324
wmodel /J0026+3508_S_map.mod
! wmodel: Unable to open new model file: /J0026+3508_S_map.mod
! Error occured in command: wmodel
![Exited script file: /opt64/bin/pima_mupet_01.dfm]
! 
wmap /scr/pima/bg219a_uvs/J0026+3508_S_map.fits
! Inverting map 
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 4.879 x 10.62 at -29.59 degrees (North through East)
! Clean map  min=-0.0023548  max=0.056175 Jy/beam
! Writing clean map to FITS file: /scr/pima/bg219a_uvs/J0026+3508_S_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is", peak_flux
! The peak flux is 0.0561746 
invert
! Inverting map 
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000247335 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -1.32089 1.32089 2.64178 5.28356 10.5671 21.1342 42.2685 84.5369
print "clev=      ", int(3*image_rms*10000)/10000
! clev=       0.0007 
print "peak=      ", int(1000*peak_flux)/1000
! peak=       0.056 
print "dyn_range= ", int(1000*peak_flux/image_rms)/1000
! dyn_range=  227.119 
quit
! Quitting program
! Log file /scr/pima/bg219a_uvs/J0026+3508_S_dfm.log closed on Thu May 19 23:44:46 2016