! Started logfile: /scr/pima/bg219a_uvs/J1845-2852_S_dfm.log on Fri May 20 00:18:01 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/J1845-2852_S_uva.fits
! Reading UV FITS file: /scr/pima/bg219a_uvs/J1845-2852_S_uva.fits
! AN table 1: 28 integrations on 15 of 15 possible baselines.
! Apparent sampling: 0.733333 visibilities/baseline/integration-bin.
! Found source: J1845-2852
! 
! 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 1232 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 J1845-2852_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 36 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 36 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 36 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 36 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=1.060914Jy  sigma=18.008453
! Fit after  self-cal, rms=0.699578Jy  sigma=11.581876
! 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=1.989 mas, bmaj=5.654 mas, bpa=-1.082 degrees
! Estimated noise=1.54235 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 = 0.231095 Jy
! Component: 100  -  total flux cleaned = 0.303395 Jy
! Total flux subtracted in 100 components = 0.303395 Jy
! Clean residual min=-0.021308 max=0.032864 Jy/beam
! Clean residual mean=-0.000126 rms=0.006255 Jy/beam
! Combined flux in latest and established models = 0.303395 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 9 components and 0.303395 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.096771Jy  sigma=1.625822
! Fit after  self-cal, rms=0.096820Jy  sigma=1.624911
! 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=2.216 mas, bmaj=6.088 mas, bpa=-2.175 degrees
! Estimated noise=1.30661 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 = 0.0453472 Jy
! Component: 100  -  total flux cleaned = 0.0694813 Jy
! Component: 150  -  total flux cleaned = 0.0838235 Jy
! Component: 200  -  total flux cleaned = 0.0931871 Jy
! Total flux subtracted in 200 components = 0.0931871 Jy
! Clean residual min=-0.008752 max=0.009694 Jy/beam
! Clean residual mean=-0.000049 rms=0.002217 Jy/beam
! Combined flux in latest and established models = 0.396582 Jy
! Performing phase self-cal
! Adding 30 model components to the UV plane model.
! The established model now contains 34 components and 0.396582 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.074542Jy  sigma=1.206245
! Fit after  self-cal, rms=0.074453Jy  sigma=1.205080
! Inverting map 
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 2.216 x 6.088 at -2.175 degrees (North through East)
! Clean map  min=-0.008125  max=0.31389 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:
!   LA        1.01     MK        1.05     NL        0.99     OV        0.97     
!   PT        1.01     SC        1.07     
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   LA        0.98     MK        1.04     NL        0.99     OV        0.98     
!   PT        0.98     SC        1.01     
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   LA        0.98     MK        1.01     NL        0.99     OV        0.95     
!   PT        0.95     SC        1.03     
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   LA        0.98     MK        1.00     NL        0.98     OV        0.94     
!   PT        0.99     SC        0.95     
! 
! 
! Fit before self-cal, rms=0.074453Jy  sigma=1.205080
! Fit after  self-cal, rms=0.072780Jy  sigma=1.179743
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=2.237 mas, bmaj=6.107 mas, bpa=-2.098 degrees
! Estimated noise=1.29157 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 = -0.000170611 Jy
! Component: 100  -  total flux cleaned = -1.43043e-05 Jy
! Component: 150  -  total flux cleaned = 9.6546e-05 Jy
! Component: 200  -  total flux cleaned = 0.000167726 Jy
! Total flux subtracted in 200 components = 0.000167726 Jy
! Clean residual min=-0.006402 max=0.006556 Jy/beam
! Clean residual mean=-0.000005 rms=0.001646 Jy/beam
! Combined flux in latest and established models = 0.39675 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 42 components and 0.39675 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.072746Jy  sigma=1.179100
! Fit after  self-cal, rms=0.072758Jy  sigma=1.179038
! 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=0.072758Jy  sigma=1.179038
! Fit after  self-cal, rms=0.072815Jy  sigma=1.179025
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=2.238 mas, bmaj=6.108 mas, bpa=-2.118 degrees
! Estimated noise=1.29238 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -1.14513e-05 Jy
! Component: 100  -  total flux cleaned = 8.83384e-05 Jy
! Component: 150  -  total flux cleaned = 0.000120203 Jy
! Component: 200  -  total flux cleaned = 0.000121028 Jy
! Total flux subtracted in 200 components = 0.000121028 Jy
! Clean residual min=-0.006347 max=0.006638 Jy/beam
! Clean residual mean=-0.000006 rms=0.001638 Jy/beam
! Combined flux in latest and established models = 0.396871 Jy
selfcal
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 43 components and 0.396871 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.072790Jy  sigma=1.178594
! Fit after  self-cal, rms=0.072789Jy  sigma=1.178587
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 = 7.647e-06 Jy
! Component: 100  -  total flux cleaned = 8.81598e-06 Jy
! Component: 150  -  total flux cleaned = 9.65989e-06 Jy
! Component: 200  -  total flux cleaned = 9.89673e-06 Jy
! Total flux subtracted in 200 components = 9.89673e-06 Jy
! Clean residual min=-0.006358 max=0.006655 Jy/beam
! Clean residual mean=-0.000005 rms=0.001633 Jy/beam
! Combined flux in latest and established models = 0.396881 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 46 components and 0.396881 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.072769Jy  sigma=1.178275
! Fit after  self-cal, rms=0.072770Jy  sigma=1.178269
! 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=0.072770Jy  sigma=1.178269
! Fit after  self-cal, rms=0.071831Jy  sigma=1.164225
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=2.232 mas, bmaj=6.098 mas, bpa=-2.068 degrees
! Estimated noise=1.29107 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000118604 Jy
! Component: 100  -  total flux cleaned = 0.000191829 Jy
! Component: 150  -  total flux cleaned = 0.000191629 Jy
! Component: 200  -  total flux cleaned = 0.000191602 Jy
! Total flux subtracted in 200 components = 0.000191602 Jy
! Clean residual min=-0.005714 max=0.005376 Jy/beam
! Clean residual mean=-0.000022 rms=0.001404 Jy/beam
! Combined flux in latest and established models = 0.397072 Jy
selfcal
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 53 components and 0.397072 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.071800Jy  sigma=1.163796
! Fit after  self-cal, rms=0.071810Jy  sigma=1.163691
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 = -0.000100555 Jy
! Component: 100  -  total flux cleaned = -5.60815e-05 Jy
! Component: 150  -  total flux cleaned = -7.64457e-05 Jy
! Component: 200  -  total flux cleaned = -9.51853e-05 Jy
! Total flux subtracted in 200 components = -9.51853e-05 Jy
! Clean residual min=-0.005679 max=0.005381 Jy/beam
! Clean residual mean=-0.000022 rms=0.001401 Jy/beam
! Combined flux in latest and established models = 0.396977 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 55 components and 0.396977 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.071797Jy  sigma=1.163533
! Fit after  self-cal, rms=0.071796Jy  sigma=1.163523
! 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=0.071796Jy  sigma=1.163523
! Fit after  self-cal, rms=0.071674Jy  sigma=1.163432
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=6.044 mas, bmaj=15.4 mas, bpa=-1.711 degrees
! Estimated noise=2.1122 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00171315 Jy
! Component: 100  -  total flux cleaned = 0.00177331 Jy
! Component: 150  -  total flux cleaned = 0.00179992 Jy
! Component: 200  -  total flux cleaned = 0.00184975 Jy
! Total flux subtracted in 200 components = 0.00184975 Jy
! Clean residual min=-0.005124 max=0.005732 Jy/beam
! Clean residual mean=-0.000069 rms=0.001870 Jy/beam
! Combined flux in latest and established models = 0.398827 Jy
selfcal
! Performing phase self-cal
! Adding 5 model components to the UV plane model.
! The established model now contains 57 components and 0.398827 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.071739Jy  sigma=1.164487
! Fit after  self-cal, rms=0.071714Jy  sigma=1.164369
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 = 0.000111976 Jy
! Component: 100  -  total flux cleaned = 0.00011086 Jy
! Component: 150  -  total flux cleaned = 0.000109941 Jy
! Component: 200  -  total flux cleaned = 0.000128436 Jy
! Total flux subtracted in 200 components = 0.000128436 Jy
! Clean residual min=-0.005069 max=0.005749 Jy/beam
! Clean residual mean=-0.000068 rms=0.001856 Jy/beam
! Combined flux in latest and established models = 0.398955 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 58 components and 0.398955 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.071768Jy  sigma=1.165183
! Fit after  self-cal, rms=0.071755Jy  sigma=1.165128
! 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=2.231 mas, bmaj=6.094 mas, bpa=-2.029 degrees
! Estimated noise=1.28996 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 2.231 x 6.094 at -2.029 degrees (North through East)
! Clean map  min=-0.0049427  max=0.31052 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=1.995 mas, bmaj=5.641 mas, bpa=-0.8702 degrees
! Estimated noise=1.51925 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.227619 Jy
! Component: 100  -  total flux cleaned = 0.29901 Jy
! Component: 150  -  total flux cleaned = 0.334545 Jy
! Component: 200  -  total flux cleaned = 0.354868 Jy
! Total flux subtracted in 200 components = 0.354868 Jy
! Clean residual min=-0.010419 max=0.011194 Jy/beam
! Clean residual mean=-0.000057 rms=0.002911 Jy/beam
! Combined flux in latest and established models = 0.354869 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 16 model components to the UV plane model.
! The established model now contains 16 components and 0.354869 Jy
! Inverting map and beam 
! Estimated beam: bmin=2.231 mas, bmaj=6.094 mas, bpa=-2.029 degrees
! Estimated noise=1.28996 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 = 0.0163162 Jy
! Component: 100  -  total flux cleaned = 0.0258445 Jy
! Component: 150  -  total flux cleaned = 0.0318879 Jy
! Component: 200  -  total flux cleaned = 0.0358043 Jy
! Total flux subtracted in 200 components = 0.0358043 Jy
! Clean residual min=-0.006460 max=0.005509 Jy/beam
! Clean residual mean=-0.000043 rms=0.001514 Jy/beam
! Combined flux in latest and established models = 0.390673 Jy
! Adding 28 model components to the UV plane model.
! The established model now contains 38 components and 0.390673 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=6.044 mas, bmaj=15.4 mas, bpa=-1.711 degrees
! Estimated noise=2.1122 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0058868 Jy
! Component: 100  -  total flux cleaned = 0.00765609 Jy
! Component: 150  -  total flux cleaned = 0.00807099 Jy
! Component: 200  -  total flux cleaned = 0.00811365 Jy
! Total flux subtracted in 200 components = 0.00811365 Jy
! Clean residual min=-0.005137 max=0.005750 Jy/beam
! Clean residual mean=-0.000070 rms=0.001873 Jy/beam
! Combined flux in latest and established models = 0.398787 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 = 2.03426e-05 Jy
! Component: 100  -  total flux cleaned = 5.86016e-05 Jy
! Component: 150  -  total flux cleaned = 9.43897e-05 Jy
! Component: 200  -  total flux cleaned = 0.000127985 Jy
! Total flux subtracted in 200 components = 0.000127985 Jy
! Clean residual min=-0.005071 max=0.005738 Jy/beam
! Clean residual mean=-0.000068 rms=0.001860 Jy/beam
! Combined flux in latest and established models = 0.398915 Jy
! Adding 26 model components to the UV plane model.
! The established model now contains 61 components and 0.398915 Jy
! Inverting map 
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Estimated beam: bmin=2.231 mas, bmaj=6.094 mas, bpa=-2.029 degrees
! Estimated noise=1.28996 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00194025 Jy
! Component: 100  -  total flux cleaned = -0.00181855 Jy
! Component: 150  -  total flux cleaned = -0.00172654 Jy
! Component: 200  -  total flux cleaned = -0.00169025 Jy
! Total flux subtracted in 200 components = -0.00169025 Jy
! Clean residual min=-0.005648 max=0.005588 Jy/beam
! Clean residual mean=-0.000022 rms=0.001412 Jy/beam
! Combined flux in latest and established models = 0.397224 Jy
selfcal
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 69 components and 0.397224 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.071706Jy  sigma=1.164316
! Fit after  self-cal, rms=0.071724Jy  sigma=1.164287
wmodel /J1845-2852_S_map.mod
! wmodel: Unable to open new model file: /J1845-2852_S_map.mod
! Error occured in command: wmodel
![Exited script file: /opt64/bin/pima_mupet_01.dfm]
! 
wmap /scr/pima/bg219a_uvs/J1845-2852_S_map.fits
! Inverting map 
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 2.231 x 6.094 at -2.029 degrees (North through East)
! Clean map  min=-0.0051676  max=0.30941 Jy/beam
! Writing clean map to FITS file: /scr/pima/bg219a_uvs/J1845-2852_S_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is", peak_flux
! The peak flux is 0.309408 
invert
! Inverting map 
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.00141243 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -1.36948 1.36948 2.73897 5.47793 10.9559 21.9117 43.8235 87.6469
print "clev=      ", int(3*image_rms*10000)/10000
! clev=       0.0042 
print "peak=      ", int(1000*peak_flux)/1000
! peak=       0.309 
print "dyn_range= ", int(1000*peak_flux/image_rms)/1000
! dyn_range=  219.06 
quit
! Quitting program
! Log file /scr/pima/bg219a_uvs/J1845-2852_S_dfm.log closed on Fri May 20 00:18:03 2016