! Started logfile: J0852-1528_X_2005_07_20_yyk_uvs.log on Fri Jan 20 10:10:11 2006
obs J0852-1528_X_2005_07_20_yyk_uve.fits
! Reading UV FITS file: J0852-1528_X_2005_07_20_yyk_uve.fits
! AN table 1: 10 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.98 visibilities/baseline/integration-bin.
! Found source: J0852-1528
! 
! There are 4 IFs, and a total of 4 channels:
! 
!  IF  Channel    Frequency  Freq offset  Number of   Overall IF
!       origin    at origin  per channel   channels    bandwidth
!  ------------------------------------------------------------- (Hz)
!  01        1  8.40997e+09        8e+06          1        8e+06
!  02        2  8.47997e+09        8e+06          1        8e+06
!  03        3  8.79497e+09        8e+06          1        8e+06
!  04        4  8.89997e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 1488 lines of history.
! 
! Reading 1764 visibilities.
select I
! Polarization I is unavailable.
! 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
![@muppet J0852-1528_X_2005_07_20_yyk]
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.04
float dynam
dynam = 6.0
float amp_soltime1
amp_soltime1 = 10
float amp_soltime2
amp_soltime2 = 1
float phase_soltime1
phase_soltime1=10
float phase_soltime2
phase_soltime2=0.5
float phase_soltime
phase_soltime=phase_soltime1
float ampcor_selflim
ampcor_selflim=1.20
float thresh
thresh = 0.10
float win_mult
win_mult = 1.8
float time_av
time_av = 30
float old_peak
float new_peak
float flux_cutoff
mapsize field_size, field_cell
! Map grid = 512x512 pixels with 0.200x0.200 milli-arcsec cellsize.
phase_soltime=phase_soltime1
print "uvstat(rms)=",uvstat(rms),"Jy"
! uvstat(rms)= 0.14499 Jy 
uvw 2,-1
! Uniform weighting binwidth: 2 (pixels).
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.692 mas, bmaj=1.763 mas, bpa=-3.955 degrees
! Estimated noise=1.34069 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (0, 0).
! clean: niter=100  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.108291 Jy
! Component: 100  -  total flux cleaned = 0.12404 Jy
! Total flux subtracted in 100 components = 0.12404 Jy
! Clean residual min=-0.006527 max=0.007563 Jy/beam
! Clean residual mean=0.000043 rms=0.001648 Jy/beam
! Combined flux in latest and established models = 0.12404 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 10 model components to the UV plane model.
! The established model now contains 10 components and 0.12404 Jy
! 
! Correcting IF 1.
!  A total of 1 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 1 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 1 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 1 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.068779Jy  sigma=1.090671
! Fit after  self-cal, rms=0.068293Jy  sigma=1.082478
! Inverting map and beam 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.692 mas, bmaj=1.763 mas, bpa=-3.955 degrees
! Estimated noise=1.34069 mJy/beam.
print "************** FINISHED UNIFORM WEIGHTING CLEAN **************"
! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** 
! 
uvw 0,-2
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -2.
! Radial weighting is not currently selected.
win_mult = win_mult * 1.6
clean_niter = clean_niter * 2
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.8657 mas, bmaj=2.127 mas, bpa=-3.135 degrees
! Estimated noise=0.953593 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00617658 Jy
! Component: 100  -  total flux cleaned = 0.00776874 Jy
! Component: 150  -  total flux cleaned = 0.00776925 Jy
! Component: 200  -  total flux cleaned = 0.00768763 Jy
! Total flux subtracted in 200 components = 0.00768763 Jy
! Clean residual min=-0.004585 max=0.005872 Jy/beam
! Clean residual mean=0.000059 rms=0.001314 Jy/beam
! Combined flux in latest and established models = 0.131728 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 10 model components to the UV plane model.
! The established model now contains 17 components and 0.131728 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067823Jy  sigma=1.075232
! Fit after  self-cal, rms=0.067826Jy  sigma=1.075180
! Inverting map 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8657 x 2.127 at -3.135 degrees (North through East)
! Clean map  min=-0.0043819  max=0.12732 Jy/beam
if(peak(flux) < thresh*2)
  selflims ampcor_selflim
  end if
! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2.
! Selfcal phase corrections will not be limited.
gscale
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Amplitude normalization factor in sub-array 1: 1.0315
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.93     FD        0.95     HN        0.96     KP        0.88     
!   LA        0.93     MK        0.98     NL        0.98     OV        0.98     
!   PT        1.11     SC        1.01     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.02744
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.01     FD        0.96     HN        1.03     KP        0.89     
!   LA        0.96     MK        0.98     NL        0.96     OV        0.95     
!   PT        1.09     SC        0.90     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 1.00624
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.08     FD        1.01     HN        0.97     KP        0.88     
!   LA        0.99     MK        1.07     NL        0.93     OV        0.96     
!   PT        1.19     SC        0.86     
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 1
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    OV        1.00*    
!   PT        1.00*    SC        1.00*    
! 
! 
! Fit before self-cal, rms=0.067826Jy  sigma=1.075180
! Fit after  self-cal, rms=0.066800Jy  sigma=1.056025
selfcal false, false, phase_soltime
! Performing phase self-cal over 10 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066800Jy  sigma=1.056025
! Fit after  self-cal, rms=0.066795Jy  sigma=1.055991
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.8593 mas, bmaj=2.109 mas, bpa=-1.833 degrees
! Estimated noise=0.950577 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00108881 Jy
! Component: 100  -  total flux cleaned = 0.00122234 Jy
! Component: 150  -  total flux cleaned = 0.00122038 Jy
! Component: 200  -  total flux cleaned = 0.00121963 Jy
! Total flux subtracted in 200 components = 0.00121963 Jy
! Clean residual min=-0.004395 max=0.003956 Jy/beam
! Clean residual mean=0.000028 rms=0.001030 Jy/beam
! Combined flux in latest and established models = 0.132947 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 18 model components to the UV plane model.
! The established model now contains 28 components and 0.132947 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066699Jy  sigma=1.055123
! Fit after  self-cal, rms=0.066703Jy  sigma=1.055088
! Inverting map 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
print "************** FINISHED AMPLITUDE GSCALE SELF-CAL **************"
! ************** FINISHED AMPLITUDE GSCALE SELF-CAL ************** 
! 
phase_soltime=phase_soltime2
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066703Jy  sigma=1.055088
! Fit after  self-cal, rms=0.063526Jy  sigma=1.000953
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00101109 Jy
! Component: 100  -  total flux cleaned = 0.00103917 Jy
! Component: 150  -  total flux cleaned = 0.00103885 Jy
! Component: 200  -  total flux cleaned = 0.00103798 Jy
! Total flux subtracted in 200 components = 0.00103797 Jy
! Clean residual min=-0.004216 max=0.003559 Jy/beam
! Clean residual mean=0.000034 rms=0.000994 Jy/beam
! Combined flux in latest and established models = 0.133985 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 11 model components to the UV plane model.
! The established model now contains 33 components and 0.133985 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.063485Jy  sigma=1.000418
! Fit after  self-cal, rms=0.063334Jy  sigma=0.994767
! Inverting map 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
print "*** FINISHED NATURAL WEIGHTING CLEAN with shorter phase_soltime ***"
! *** FINISHED NATURAL WEIGHTING CLEAN with shorter phase_soltime *** 
! 
dynam = dynam - 0.25
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8593 x 2.109 at -1.833 degrees (North through East)
! Clean map  min=-0.0039355  max=0.12874 Jy/beam
if(peak(flux) > thresh)
  selfcal true, true, amp_soltime1
  selfcal false, false, phase_soltime
  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 false,false,phase_soltime
    new_peak = peak(flux)
    until(new_peak<=flux_cutoff)
  selfcal true, true, amp_soltime2
  selfcal false, false, phase_soltime
  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 false,false,phase_soltime
    new_peak = peak(flux)
    until(new_peak<=flux_cutoff)
  print "************** FINISHED AMPLITUDE SELF-CAL **************"
  end if
! Performing amp+phase self-cal over 10 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.063334Jy  sigma=0.994767
! Fit after  self-cal, rms=0.061228Jy  sigma=0.983894
! Performing phase self-cal over 0.5 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.061228Jy  sigma=0.983894
! Fit after  self-cal, rms=0.061291Jy  sigma=0.982905
! Inverting map and beam 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.8548 mas, bmaj=2.107 mas, bpa=-1.373 degrees
! Estimated noise=0.917531 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.00340378 Jy
! Component: 100  -  total flux cleaned = -0.00349183 Jy
! Component: 150  -  total flux cleaned = -0.00343227 Jy
! Component: 200  -  total flux cleaned = -0.00340922 Jy
! Total flux subtracted in 200 components = -0.00340922 Jy
! Clean residual min=-0.003665 max=0.003194 Jy/beam
! Clean residual mean=0.000019 rms=0.000890 Jy/beam
! Combined flux in latest and established models = 0.130576 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 11 model components to the UV plane model.
! The established model now contains 37 components and 0.130576 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.061150Jy  sigma=0.979997
! Fit after  self-cal, rms=0.061198Jy  sigma=0.979720
! Inverting map 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Performing amp+phase self-cal over 1 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.061198Jy  sigma=0.979720
! Fit after  self-cal, rms=0.060053Jy  sigma=0.972442
! Performing phase self-cal over 0.5 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.060053Jy  sigma=0.972442
! Fit after  self-cal, rms=0.060096Jy  sigma=0.972314
! Inverting map and beam 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.8524 mas, bmaj=2.106 mas, bpa=-0.7847 degrees
! Estimated noise=0.896159 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.00246028 Jy
! Component: 100  -  total flux cleaned = -0.00246491 Jy
! Component: 150  -  total flux cleaned = -0.00238486 Jy
! Component: 200  -  total flux cleaned = -0.00234398 Jy
! Total flux subtracted in 200 components = -0.00234398 Jy
! Clean residual min=-0.003566 max=0.003139 Jy/beam
! Clean residual mean=0.000014 rms=0.000841 Jy/beam
! Combined flux in latest and established models = 0.128232 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 40 components and 0.128232 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.059998Jy  sigma=0.970356
! Fit after  self-cal, rms=0.060013Jy  sigma=0.970287
! Inverting map 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! ************** FINISHED AMPLITUDE SELF-CAL ************** 
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
win_mult = win_mult * 1.4
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=2.232 mas, bmaj=4.264 mas, bpa=-0.3334 degrees
! Estimated noise=1.17617 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.000159899 Jy
! Component: 100  -  total flux cleaned = -0.000158545 Jy
! Component: 150  -  total flux cleaned = -0.000157818 Jy
! Component: 200  -  total flux cleaned = -0.000168812 Jy
! Total flux subtracted in 200 components = -0.000168812 Jy
! Clean residual min=-0.004419 max=0.003393 Jy/beam
! Clean residual mean=0.000029 rms=0.001108 Jy/beam
! Combined flux in latest and established models = 0.128063 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 13 model components to the UV plane model.
! The established model now contains 47 components and 0.128063 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.060023Jy  sigma=0.970433
! Fit after  self-cal, rms=0.060027Jy  sigma=0.970350
! Inverting map 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
win_mult = win_mult / 1.4
print "************** FINISHED TAPERING SELF-CAL CLEAN **************"
! ************** FINISHED TAPERING SELF-CAL CLEAN ************** 
! 
print "************** CLEARING MODEL AND STARTING OVER **********"
! ************** CLEARING MODEL AND STARTING OVER ********** 
clrmod true,true,true
! clrmod: Cleared the established, tentative and continuum models.
uvw 2,-1
! Uniform weighting binwidth: 2 (pixels).
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
clean clean_niter, clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.6907 mas, bmaj=1.759 mas, bpa=-2.854 degrees
! Estimated noise=1.2598 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.10356 Jy
! Component: 100  -  total flux cleaned = 0.120296 Jy
! Component: 150  -  total flux cleaned = 0.126172 Jy
! Component: 200  -  total flux cleaned = 0.127993 Jy
! Total flux subtracted in 200 components = 0.127993 Jy
! Clean residual min=-0.005301 max=0.004573 Jy/beam
! Clean residual mean=0.000010 rms=0.001219 Jy/beam
! Combined flux in latest and established models = 0.127993 Jy
uvw 0,-2
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -2.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Adding 11 model components to the UV plane model.
! The established model now contains 11 components and 0.127993 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.8524 mas, bmaj=2.106 mas, bpa=-0.7847 degrees
! Estimated noise=0.896159 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=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000738442 Jy
! Component: 100  -  total flux cleaned = 0.000809203 Jy
! Component: 150  -  total flux cleaned = 0.000770247 Jy
! Component: 200  -  total flux cleaned = 0.000768895 Jy
! Total flux subtracted in 200 components = 0.000768895 Jy
! Clean residual min=-0.003519 max=0.003126 Jy/beam
! Clean residual mean=0.000015 rms=0.000853 Jy/beam
! Combined flux in latest and established models = 0.128762 Jy
! Adding 9 model components to the UV plane model.
! The established model now contains 19 components and 0.128762 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=2.232 mas, bmaj=4.264 mas, bpa=-0.3334 degrees
! Estimated noise=1.17617 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=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.000281655 Jy
! Component: 100  -  total flux cleaned = -0.000299482 Jy
! Component: 150  -  total flux cleaned = -0.000331656 Jy
! Component: 200  -  total flux cleaned = -0.000375595 Jy
! Total flux subtracted in 200 components = -0.000375595 Jy
! Clean residual min=-0.004377 max=0.003417 Jy/beam
! Clean residual mean=0.000030 rms=0.001112 Jy/beam
! Combined flux in latest and established models = 0.128386 Jy
! Adding 8 model components to the UV plane model.
! The established model now contains 26 components and 0.128386 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! Estimated beam: bmin=0.8524 mas, bmaj=2.106 mas, bpa=-0.7847 degrees
! Estimated noise=0.896159 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000102682 Jy
! Component: 100  -  total flux cleaned = 4.67083e-05 Jy
! Component: 150  -  total flux cleaned = 2.33455e-05 Jy
! Component: 200  -  total flux cleaned = 2.13983e-05 Jy
! Total flux subtracted in 200 components = 2.13983e-05 Jy
! Clean residual min=-0.003532 max=0.003106 Jy/beam
! Clean residual mean=0.000014 rms=0.000846 Jy/beam
! Combined flux in latest and established models = 0.128408 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 9 model components to the UV plane model.
! The established model now contains 33 components and 0.128408 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.060003Jy  sigma=0.970384
! Fit after  self-cal, rms=0.060004Jy  sigma=0.970338
wmodel J0852-1528_X_2005_07_20_yyk\_map.mod
! Writing 33 model components to file: J0852-1528_X_2005_07_20_yyk_map.mod
wobs J0852-1528_X_2005_07_20_yyk\_uvs.fits
! Writing UV FITS file: J0852-1528_X_2005_07_20_yyk_uvs.fits
wwins J0852-1528_X_2005_07_20_yyk\_map.win
! wwins: Wrote 1 windows to J0852-1528_X_2005_07_20_yyk_map.win
x = (field_size-8) * field_cell / 4
addwin -x,x,-x,x
clean (field_size*4),0.01
! Inverting map 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00089394 Jy
! Component: 100  -  total flux cleaned = -0.00101279 Jy
! Component: 150  -  total flux cleaned = -0.000856935 Jy
! Component: 200  -  total flux cleaned = -0.000515347 Jy
! Component: 250  -  total flux cleaned = -0.000467803 Jy
! Component: 300  -  total flux cleaned = -0.000286414 Jy
! Component: 350  -  total flux cleaned = -0.000198856 Jy
! Component: 400  -  total flux cleaned = -0.000284375 Jy
! Component: 450  -  total flux cleaned = -0.000158792 Jy
! Component: 500  -  total flux cleaned = -0.000117965 Jy
! Component: 550  -  total flux cleaned = -0.000117669 Jy
! Component: 600  -  total flux cleaned = -7.9562e-05 Jy
! Component: 650  -  total flux cleaned = -0.000117939 Jy
! Component: 700  -  total flux cleaned = 0.000105558 Jy
! Component: 750  -  total flux cleaned = 0.000215471 Jy
! Component: 800  -  total flux cleaned = 0.000359186 Jy
! Component: 850  -  total flux cleaned = 0.000359468 Jy
! Component: 900  -  total flux cleaned = 0.000430358 Jy
! Component: 950  -  total flux cleaned = 0.000568573 Jy
! Component: 1000  -  total flux cleaned = 0.000568222 Jy
! Component: 1050  -  total flux cleaned = 0.000502205 Jy
! Component: 1100  -  total flux cleaned = 0.000700565 Jy
! Component: 1150  -  total flux cleaned = 0.000635405 Jy
! Component: 1200  -  total flux cleaned = 0.000635948 Jy
! Component: 1250  -  total flux cleaned = 0.000667681 Jy
! Component: 1300  -  total flux cleaned = 0.00066772 Jy
! Component: 1350  -  total flux cleaned = 0.000667942 Jy
! Component: 1400  -  total flux cleaned = 0.000606987 Jy
! Component: 1450  -  total flux cleaned = 0.000637336 Jy
! Component: 1500  -  total flux cleaned = 0.000607183 Jy
! Component: 1550  -  total flux cleaned = 0.000577929 Jy
! Component: 1600  -  total flux cleaned = 0.000461892 Jy
! Component: 1650  -  total flux cleaned = 0.000433443 Jy
! Component: 1700  -  total flux cleaned = 0.00037691 Jy
! Component: 1750  -  total flux cleaned = 0.000432926 Jy
! Component: 1800  -  total flux cleaned = 0.000348895 Jy
! Component: 1850  -  total flux cleaned = 0.000239303 Jy
! Component: 1900  -  total flux cleaned = 0.000185055 Jy
! Component: 1950  -  total flux cleaned = 0.000131198 Jy
! Component: 2000  -  total flux cleaned = 7.76747e-05 Jy
! Total flux subtracted in 2048 components = -5.40997e-05 Jy
! Clean residual min=-0.001550 max=0.001565 Jy/beam
! Clean residual mean=0.000004 rms=0.000508 Jy/beam
! Combined flux in latest and established models = 0.128354 Jy
keep
! Adding 142 model components to the UV plane model.
! The established model now contains 175 components and 0.128354 Jy
![Exited script file: muppet]
wmap "J0852-1528_X_2005_07_20_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8524 x 2.106 at -0.7847 degrees (North through East)
! Clean map  min=-0.0027112  max=0.12071 Jy/beam
! Writing clean map to FITS file: J0852-1528_X_2005_07_20_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.120713 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.297% of the data.
!  The x-axis pixel size should ideally be below 0.1986 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000508425 
device "J0852-1528_X_2005_07_20_yyk\_map.eps/VPS"
! Attempting to open device: 'J0852-1528_X_2005_07_20_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -1.26356 1.26356 2.52711 5.05423 10.1085 20.2169 40.4338 80.8677
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0015 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.12 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8524 x 2.106 at -0.7847 degrees (North through East)
! Clean map  min=-0.0027112  max=0.12071 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0852-1528_X_2005_07_20_yyk\_map.gif/gif"
! Attempting to open device: 'J0852-1528_X_2005_07_20_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J0852-1528_X_2005_07_20_yyk_uvs.log closed on Fri Jan 20 10:10:16 2006