! Started logfile: J1415-3705_X_2002_01_31_yyk_uvs.log on Wed Jun 27 10:58:31 2007
obs J1415-3705_X_2002_01_31_yyk_uva.fits
! Reading UV FITS file: J1415-3705_X_2002_01_31_yyk_uva.fits
! AN table 1: 40 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.713889 visibilities/baseline/integration-bin.
! Found source: J1415-3705
! 
! 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  8.40947e+09        8e+06          1        8e+06
!  02        2  8.47947e+09        8e+06          1        8e+06
!  03        3  8.79447e+09        8e+06          1        8e+06
!  04        4  8.89947e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 1544 lines of history.
! 
! Reading 5140 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
flag NL
! Flagging baselines of antenna 1:NL in the currently selected channels.
![@muppet J1415-3705_X_2002_01_31_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)= 0.282817 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 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.6678 mas, bmaj=1.74 mas, bpa=5.36 degrees
! Estimated noise=3478.82 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 = 0.193787 Jy
! Component: 100  -  total flux cleaned = 0.243141 Jy
! Total flux subtracted in 100 components = 0.243141 Jy
! Clean residual min=-0.018651 max=0.016027 Jy/beam
! Clean residual mean=-0.000506 rms=0.005230 Jy/beam
! Combined flux in latest and established models = 0.243142 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 15 components and 0.243142 Jy
! 
! Correcting IF 1.
!  A total of 99 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 99 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 99 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 99 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.161481Jy  sigma=0.001235
! Fit after  self-cal, rms=0.161394Jy  sigma=0.001233
! Inverting map and beam 
! Your choice of large map pixels excluded 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.6678 mas, bmaj=1.74 mas, bpa=5.36 degrees
! Estimated noise=3478.82 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 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.8246 mas, bmaj=2.141 mas, bpa=2.283 degrees
! Estimated noise=1376.24 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 = 0.0240923 Jy
! Component: 100  -  total flux cleaned = 0.0318997 Jy
! Component: 150  -  total flux cleaned = 0.0345741 Jy
! Component: 200  -  total flux cleaned = 0.0347426 Jy
! Total flux subtracted in 200 components = 0.0347426 Jy
! Clean residual min=-0.011857 max=0.013059 Jy/beam
! Clean residual mean=0.000063 rms=0.003767 Jy/beam
! Combined flux in latest and established models = 0.277884 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 26 model components to the UV plane model.
! The established model now contains 31 components and 0.277884 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.159376Jy  sigma=0.001214
! Fit after  self-cal, rms=0.159367Jy  sigma=0.001214
! Inverting map 
! Your choice of large map pixels excluded 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8246 x 2.141 at 2.283 degrees (North through East)
! Clean map  min=-0.011224  max=0.21914 Jy/beam
if(peak(flux) < thresh*2)
  selflims ampcor_selflim
  end if
gscale
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Amplitude normalization factor in sub-array 1: 0.996004
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.95     FD        0.92     HN        1.00*    KP        1.00     
!   LA        1.19     MK        0.98     NL        1.00*    OV        0.92     
!   PT        0.99     SC        1.10     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.02069
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.01     FD        0.90     HN        1.00*    KP        0.92     
!   LA        1.09     MK        0.97     NL        1.00*    OV        0.92     
!   PT        1.01     SC        0.98     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 0.993831
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.03     FD        0.88     HN        1.00*    KP        0.96     
!   LA        1.19     MK        1.07     NL        1.00*    OV        0.94     
!   PT        1.06     SC        0.96     
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 0.971108
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        0.89     HN        1.00*    KP        1.14     
!   LA        1.19     MK        1.00     NL        1.00*    OV        0.92     
!   PT        1.14     SC        1.02     
! 
! 
! Fit before self-cal, rms=0.159367Jy  sigma=0.001214
! Fit after  self-cal, rms=0.157315Jy  sigma=0.001194
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=0.157315Jy  sigma=0.001194
! Fit after  self-cal, rms=0.157312Jy  sigma=0.001194
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.8313 mas, bmaj=2.159 mas, bpa=2.265 degrees
! Estimated noise=1359.19 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 = -0.000851704 Jy
! Component: 100  -  total flux cleaned = -0.000807195 Jy
! Component: 150  -  total flux cleaned = -0.000724426 Jy
! Component: 200  -  total flux cleaned = -0.00064643 Jy
! Total flux subtracted in 200 components = -0.00064643 Jy
! Clean residual min=-0.005678 max=0.005584 Jy/beam
! Clean residual mean=-0.000059 rms=0.001507 Jy/beam
! Combined flux in latest and established models = 0.277238 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 7 model components to the UV plane model.
! The established model now contains 37 components and 0.277238 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.157282Jy  sigma=0.001194
! Fit after  self-cal, rms=0.157279Jy  sigma=0.001194
! Inverting map 
! Your choice of large map pixels excluded 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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=0.157279Jy  sigma=0.001194
! Fit after  self-cal, rms=0.154374Jy  sigma=0.001172
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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 = 0.00128225 Jy
! Component: 100  -  total flux cleaned = 0.00151218 Jy
! Component: 150  -  total flux cleaned = 0.00162852 Jy
! Component: 200  -  total flux cleaned = 0.00173152 Jy
! Total flux subtracted in 200 components = 0.00173152 Jy
! Clean residual min=-0.005532 max=0.005602 Jy/beam
! Clean residual mean=-0.000074 rms=0.001477 Jy/beam
! Combined flux in latest and established models = 0.278969 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 9 model components to the UV plane model.
! The established model now contains 40 components and 0.278969 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.154339Jy  sigma=0.001172
! Fit after  self-cal, rms=0.153953Jy  sigma=0.001169
! Inverting map 
! Your choice of large map pixels excluded 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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: 0.8313 x 2.159 at 2.265 degrees (North through East)
! Clean map  min=-0.0050054  max=0.21758 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=0.153953Jy  sigma=0.001169
! Fit after  self-cal, rms=0.153647Jy  sigma=0.001167
! 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=0.153647Jy  sigma=0.001167
! Fit after  self-cal, rms=0.153559Jy  sigma=0.001166
! Inverting map and beam 
! Your choice of large map pixels excluded 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.8223 mas, bmaj=2.142 mas, bpa=2.909 degrees
! Estimated noise=1350.44 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000498436 Jy
! Component: 100  -  total flux cleaned = 0.000527002 Jy
! Component: 150  -  total flux cleaned = 0.000583009 Jy
! Component: 200  -  total flux cleaned = 0.000636273 Jy
! Total flux subtracted in 200 components = 0.000636273 Jy
! Clean residual min=-0.005453 max=0.005036 Jy/beam
! Clean residual mean=-0.000064 rms=0.001370 Jy/beam
! Combined flux in latest and established models = 0.279605 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 9 model components to the UV plane model.
! The established model now contains 45 components and 0.279605 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.153544Jy  sigma=0.001166
! Fit after  self-cal, rms=0.153512Jy  sigma=0.001166
! Inverting map 
! Your choice of large map pixels excluded 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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=0.153512Jy  sigma=0.001166
! Fit after  self-cal, rms=0.154869Jy  sigma=0.001162
! 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=0.154869Jy  sigma=0.001162
! Fit after  self-cal, rms=0.154870Jy  sigma=0.001162
! Inverting map and beam 
! Your choice of large map pixels excluded 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.8195 mas, bmaj=2.137 mas, bpa=3.053 degrees
! Estimated noise=1351.5 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00101953 Jy
! Component: 100  -  total flux cleaned = 0.00112761 Jy
! Component: 150  -  total flux cleaned = 0.00115261 Jy
! Component: 200  -  total flux cleaned = 0.00120047 Jy
! Total flux subtracted in 200 components = 0.00120047 Jy
! Clean residual min=-0.005399 max=0.005108 Jy/beam
! Clean residual mean=-0.000063 rms=0.001350 Jy/beam
! Combined flux in latest and established models = 0.280806 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 9 model components to the UV plane model.
! The established model now contains 48 components and 0.280806 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.154860Jy  sigma=0.001161
! Fit after  self-cal, rms=0.154858Jy  sigma=0.001161
! Inverting map 
! Your choice of large map pixels excluded 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=2.757 mas, bmaj=9.372 mas, bpa=9.725 degrees
! Estimated noise=1766.39 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 = 0.000593139 Jy
! Component: 100  -  total flux cleaned = 0.000596539 Jy
! Component: 150  -  total flux cleaned = 0.000597696 Jy
! Component: 200  -  total flux cleaned = 0.000598373 Jy
! Total flux subtracted in 200 components = 0.000598373 Jy
! Clean residual min=-0.004663 max=0.005862 Jy/beam
! Clean residual mean=-0.000116 rms=0.001927 Jy/beam
! Combined flux in latest and established models = 0.281404 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 7 model components to the UV plane model.
! The established model now contains 50 components and 0.281404 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.154855Jy  sigma=0.001161
! Fit after  self-cal, rms=0.154848Jy  sigma=0.001161
! Inverting map 
! Your choice of large map pixels excluded 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.666 mas, bmaj=1.743 mas, bpa=5.764 degrees
! Estimated noise=3429.82 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.193301 Jy
! Component: 100  -  total flux cleaned = 0.242247 Jy
! Component: 150  -  total flux cleaned = 0.26231 Jy
! Component: 200  -  total flux cleaned = 0.272886 Jy
! Total flux subtracted in 200 components = 0.272886 Jy
! Clean residual min=-0.011444 max=0.009920 Jy/beam
! Clean residual mean=-0.000107 rms=0.003283 Jy/beam
! Combined flux in latest and established models = 0.272886 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 24 model components to the UV plane model.
! The established model now contains 24 components and 0.272886 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.8195 mas, bmaj=2.137 mas, bpa=3.053 degrees
! Estimated noise=1351.5 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)
! Added new window around map position (0.2, -4.6).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0106754 Jy
! Component: 100  -  total flux cleaned = 0.0119111 Jy
! Component: 150  -  total flux cleaned = 0.0122585 Jy
! Component: 200  -  total flux cleaned = 0.0121897 Jy
! Total flux subtracted in 200 components = 0.0121897 Jy
! Clean residual min=-0.005396 max=0.005391 Jy/beam
! Clean residual mean=-0.000049 rms=0.001371 Jy/beam
! Combined flux in latest and established models = 0.285076 Jy
! Adding 19 model components to the UV plane model.
! The established model now contains 42 components and 0.285076 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=2.757 mas, bmaj=9.372 mas, bpa=9.725 degrees
! Estimated noise=1766.39 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 = 6.72768e-06 Jy
! Component: 100  -  total flux cleaned = 4.15425e-05 Jy
! Component: 150  -  total flux cleaned = 4.37727e-05 Jy
! Component: 200  -  total flux cleaned = 4.23193e-05 Jy
! Total flux subtracted in 200 components = 4.23193e-05 Jy
! Clean residual min=-0.004477 max=0.006442 Jy/beam
! Clean residual mean=-0.000096 rms=0.001929 Jy/beam
! Combined flux in latest and established models = 0.285118 Jy
! Adding 17 model components to the UV plane model.
! The established model now contains 56 components and 0.285118 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.8195 mas, bmaj=2.137 mas, bpa=3.053 degrees
! Estimated noise=1351.5 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00027829 Jy
! Component: 100  -  total flux cleaned = 0.000370877 Jy
! Component: 150  -  total flux cleaned = 0.000339095 Jy
! Component: 200  -  total flux cleaned = 0.00028143 Jy
! Total flux subtracted in 200 components = 0.00028143 Jy
! Clean residual min=-0.005282 max=0.005337 Jy/beam
! Clean residual mean=-0.000048 rms=0.001331 Jy/beam
! Combined flux in latest and established models = 0.285399 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 65 components and 0.285399 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.154768Jy  sigma=0.001161
! Fit after  self-cal, rms=0.154771Jy  sigma=0.001161
wmodel J1415-3705_X_2002_01_31_yyk\_map.mod
! Writing 65 model components to file: J1415-3705_X_2002_01_31_yyk_map.mod
wobs J1415-3705_X_2002_01_31_yyk\_uvs.fits
! Applying 40 buffered edits.
! Writing UV FITS file: J1415-3705_X_2002_01_31_yyk_uvs.fits
wwins J1415-3705_X_2002_01_31_yyk\_map.win
! wwins: Wrote 2 windows to J1415-3705_X_2002_01_31_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 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.000188386 Jy
! Component: 100  -  total flux cleaned = 0.000174059 Jy
! Component: 150  -  total flux cleaned = 0.000170039 Jy
! Component: 200  -  total flux cleaned = -1.43813e-05 Jy
! Component: 250  -  total flux cleaned = -0.000248409 Jy
! Component: 300  -  total flux cleaned = -0.000304987 Jy
! Component: 350  -  total flux cleaned = -0.000512881 Jy
! Component: 400  -  total flux cleaned = -0.000809532 Jy
! Component: 450  -  total flux cleaned = -0.00113755 Jy
! Component: 500  -  total flux cleaned = -0.00136054 Jy
! Component: 550  -  total flux cleaned = -0.00157603 Jy
! Component: 600  -  total flux cleaned = -0.00182497 Jy
! Component: 650  -  total flux cleaned = -0.00202348 Jy
! Component: 700  -  total flux cleaned = -0.00217664 Jy
! Component: 750  -  total flux cleaned = -0.00228614 Jy
! Component: 800  -  total flux cleaned = -0.00235585 Jy
! Component: 850  -  total flux cleaned = -0.00235526 Jy
! Component: 900  -  total flux cleaned = -0.00245583 Jy
! Component: 950  -  total flux cleaned = -0.00245672 Jy
! Component: 1000  -  total flux cleaned = -0.00245752 Jy
! Component: 1050  -  total flux cleaned = -0.00248923 Jy
! Component: 1100  -  total flux cleaned = -0.00261055 Jy
! Component: 1150  -  total flux cleaned = -0.00264026 Jy
! Component: 1200  -  total flux cleaned = -0.0026111 Jy
! Component: 1250  -  total flux cleaned = -0.00264018 Jy
! Component: 1300  -  total flux cleaned = -0.00272475 Jy
! Component: 1350  -  total flux cleaned = -0.00266916 Jy
! Component: 1400  -  total flux cleaned = -0.00266911 Jy
! Component: 1450  -  total flux cleaned = -0.00258751 Jy
! Component: 1500  -  total flux cleaned = -0.00256053 Jy
! Component: 1550  -  total flux cleaned = -0.00256075 Jy
! Component: 1600  -  total flux cleaned = -0.00266597 Jy
! Component: 1650  -  total flux cleaned = -0.00261342 Jy
! Component: 1700  -  total flux cleaned = -0.00263932 Jy
! Component: 1750  -  total flux cleaned = -0.00269046 Jy
! Component: 1800  -  total flux cleaned = -0.00263907 Jy
! Component: 1850  -  total flux cleaned = -0.00263899 Jy
! Component: 1900  -  total flux cleaned = -0.00261366 Jy
! Component: 1950  -  total flux cleaned = -0.00253803 Jy
! Component: 2000  -  total flux cleaned = -0.0025128 Jy
! Total flux subtracted in 2048 components = -0.00246272 Jy
! Clean residual min=-0.001383 max=0.001338 Jy/beam
! Clean residual mean=-0.000009 rms=0.000464 Jy/beam
! Combined flux in latest and established models = 0.282937 Jy
keep
! Adding 107 model components to the UV plane model.
! The established model now contains 172 components and 0.282937 Jy
![Exited script file: muppet]
wmap "J1415-3705_X_2002_01_31_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8195 x 2.137 at 3.053 degrees (North through East)
! Clean map  min=-0.0036026  max=0.20492 Jy/beam
! Writing clean map to FITS file: J1415-3705_X_2002_01_31_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.204917 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.872% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000465928 
device "J1415-3705_X_2002_01_31_yyk\_map.eps/VPS"
! Attempting to open device: 'J1415-3705_X_2002_01_31_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.682124 0.682124 1.36425 2.72849 5.45699 10.914 21.828 43.6559 87.3118
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0013 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.204 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8195 x 2.137 at 3.053 degrees (North through East)
! Clean map  min=-0.0036026  max=0.20492 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1415-3705_X_2002_01_31_yyk\_map.gif/gif"
! Attempting to open device: 'J1415-3705_X_2002_01_31_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1415-3705_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 10:58:37 2007