! Started logfile: J1354-0206_X_2002_05_14_yyk_uvs.log on Tue Jun 26 22:52:15 2007
obs J1354-0206_X_2002_05_14_yyk_uva.fits
! Reading UV FITS file: J1354-0206_X_2002_05_14_yyk_uva.fits
! AN table 1: 176 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.756313 visibilities/baseline/integration-bin.
! Found source: J1354-0206
! 
! 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 1076 lines of history.
! 
! Reading 23960 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 J1354-0206_X_2002_05_14_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)= 0.713001 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 0.175% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.6836 mas, bmaj=1.832 mas, bpa=-2.59 degrees
! Estimated noise=816.103 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 = 0.570877 Jy
! Component: 100  -  total flux cleaned = 0.698566 Jy
! Total flux subtracted in 100 components = 0.698566 Jy
! Clean residual min=-0.021029 max=0.036901 Jy/beam
! Clean residual mean=-0.000062 rms=0.003874 Jy/beam
! Combined flux in latest and established models = 0.698566 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 12 model components to the UV plane model.
! The established model now contains 12 components and 0.698566 Jy
! 
! Correcting IF 1.
!  A total of 306 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 306 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 306 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 306 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.189900Jy  sigma=0.001590
! Fit after  self-cal, rms=0.188397Jy  sigma=0.001580
! Inverting map and beam 
! Your choice of large map pixels excluded 0.155% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.6837 mas, bmaj=1.832 mas, bpa=-2.59 degrees
! Estimated noise=817.222 mJy/beam.
! clean: niter=100  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0543541 Jy
! Component: 100  -  total flux cleaned = 0.0824317 Jy
! Total flux subtracted in 100 components = 0.0824317 Jy
! Clean residual min=-0.013025 max=0.013904 Jy/beam
! Clean residual mean=-0.000023 rms=0.002399 Jy/beam
! Combined flux in latest and established models = 0.780998 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 18 model components to the UV plane model.
! The established model now contains 25 components and 0.780998 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.172834Jy  sigma=0.001432
! Fit after  self-cal, rms=0.172768Jy  sigma=0.001431
! Inverting map 
! Your choice of large map pixels excluded 0.155% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Added new window around map position (1.2, -0.6).
! clean: niter=100  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0189518 Jy
! Component: 100  -  total flux cleaned = 0.0312208 Jy
! Total flux subtracted in 100 components = 0.0312208 Jy
! Clean residual min=-0.011016 max=0.010906 Jy/beam
! Clean residual mean=-0.000009 rms=0.002126 Jy/beam
! Combined flux in latest and established models = 0.812218 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 34 components and 0.812218 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.170303Jy  sigma=0.001411
! Fit after  self-cal, rms=0.170234Jy  sigma=0.001410
! Inverting map 
! Your choice of large map pixels excluded 0.155% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
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 0.155% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.8505 mas, bmaj=2.145 mas, bpa=-3.091 degrees
! Estimated noise=526.452 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 = 0.011468 Jy
! Component: 100  -  total flux cleaned = 0.0158624 Jy
! Component: 150  -  total flux cleaned = 0.0171522 Jy
! Component: 200  -  total flux cleaned = 0.0174989 Jy
! Total flux subtracted in 200 components = 0.0174989 Jy
! Clean residual min=-0.011885 max=0.013500 Jy/beam
! Clean residual mean=-0.000000 rms=0.002726 Jy/beam
! Combined flux in latest and established models = 0.829717 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 23 model components to the UV plane model.
! The established model now contains 52 components and 0.829717 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.169452Jy  sigma=0.001405
! Fit after  self-cal, rms=0.169419Jy  sigma=0.001405
! Inverting map 
! Your choice of large map pixels excluded 0.155% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8505 x 2.145 at -3.091 degrees (North through East)
! Clean map  min=-0.011067  max=0.67304 Jy/beam
if(peak(flux) < thresh*2)
  selflims ampcor_selflim
  end if
gscale
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 18 telescope corrections were flagged in sub-array 1.
!  Amplitude normalization factor in sub-array 1: 1.00122
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     FD        0.99     HN        1.02     KP        0.92     
!   LA        1.02     NL        1.01     OV        1.00     PT        1.01     
!   SC        1.00     MK        1.02     
! 
! 
! Correcting IF 2.
!  A total of 18 telescope corrections were flagged in sub-array 1.
!  Amplitude normalization factor in sub-array 1: 1.01622
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     FD        0.97     HN        1.00     KP        0.89     
!   LA        0.98     NL        0.98     OV        0.97     PT        1.05     
!   SC        0.98     MK        1.01     
! 
! 
! Correcting IF 3.
!  A total of 18 telescope corrections were flagged in sub-array 1.
!  Amplitude normalization factor in sub-array 1: 0.998636
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.06     FD        0.93     HN        1.00     KP        0.91     
!   LA        1.00     NL        0.97     OV        1.01     PT        1.07     
!   SC        1.00     MK        1.06     
! 
! 
! Correcting IF 4.
!  A total of 18 telescope corrections were flagged in sub-array 1.
!  Amplitude normalization factor in sub-array 1: 0.973323
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.08     FD        0.93     HN        0.98     KP        0.99     
!   LA        0.99     NL        1.01     OV        1.05     PT        1.16     
!   SC        1.04     MK        1.05     
! 
! 
! Fit before self-cal, rms=0.169419Jy  sigma=0.001405
! Fit after  self-cal, rms=0.162882Jy  sigma=0.001349
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=0.162882Jy  sigma=0.001349
! Fit after  self-cal, rms=0.162876Jy  sigma=0.001349
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.8643 mas, bmaj=2.169 mas, bpa=-2.753 degrees
! Estimated noise=527.541 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 (0.4, 13.4).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00280872 Jy
! Component: 100  -  total flux cleaned = 0.00281715 Jy
! Component: 150  -  total flux cleaned = 0.00295287 Jy
! Component: 200  -  total flux cleaned = 0.00284283 Jy
! Total flux subtracted in 200 components = 0.00284283 Jy
! Clean residual min=-0.003636 max=0.003862 Jy/beam
! Clean residual mean=0.000008 rms=0.000919 Jy/beam
! Combined flux in latest and established models = 0.83256 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 19 model components to the UV plane model.
! The established model now contains 70 components and 0.83256 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.162615Jy  sigma=0.001347
! Fit after  self-cal, rms=0.162604Jy  sigma=0.001346
! Inverting map 
! Your choice of large map pixels excluded 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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=0.162604Jy  sigma=0.001346
! Fit after  self-cal, rms=0.152004Jy  sigma=0.001258
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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 = 0.00174313 Jy
! Component: 100  -  total flux cleaned = 0.00114659 Jy
! Component: 150  -  total flux cleaned = 0.00088548 Jy
! Component: 200  -  total flux cleaned = 0.000728706 Jy
! Total flux subtracted in 200 components = 0.000728706 Jy
! Clean residual min=-0.002926 max=0.003630 Jy/beam
! Clean residual mean=0.000006 rms=0.000863 Jy/beam
! Combined flux in latest and established models = 0.833289 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 23 model components to the UV plane model.
! The established model now contains 87 components and 0.833289 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.151923Jy  sigma=0.001258
! Fit after  self-cal, rms=0.150331Jy  sigma=0.001244
! Inverting map 
! Your choice of large map pixels excluded 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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: 0.8643 x 2.169 at -2.753 degrees (North through East)
! Clean map  min=-0.0028236  max=0.6774 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=0.150331Jy  sigma=0.001244
! Fit after  self-cal, rms=0.149888Jy  sigma=0.001228
! 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=0.149888Jy  sigma=0.001228
! Fit after  self-cal, rms=0.149492Jy  sigma=0.001224
! Inverting map and beam 
! Your choice of large map pixels excluded 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.8619 mas, bmaj=2.169 mas, bpa=-2.664 degrees
! Estimated noise=526.442 mJy/beam.
! Added new window around map position (12.6, -9).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00204559 Jy
! Component: 100  -  total flux cleaned = 0.00231099 Jy
! Component: 150  -  total flux cleaned = 0.00253084 Jy
! Component: 200  -  total flux cleaned = 0.00265517 Jy
! Total flux subtracted in 200 components = 0.00265517 Jy
! Clean residual min=-0.002604 max=0.002380 Jy/beam
! Clean residual mean=0.000003 rms=0.000638 Jy/beam
! Combined flux in latest and established models = 0.835944 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 31 model components to the UV plane model.
! The established model now contains 112 components and 0.835944 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.149417Jy  sigma=0.001224
! Fit after  self-cal, rms=0.149263Jy  sigma=0.001222
! Inverting map 
! Your choice of large map pixels excluded 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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=0.149263Jy  sigma=0.001222
! Fit after  self-cal, rms=0.149165Jy  sigma=0.001220
! 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=0.149165Jy  sigma=0.001220
! Fit after  self-cal, rms=0.149105Jy  sigma=0.001220
! Inverting map and beam 
! Your choice of large map pixels excluded 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.8627 mas, bmaj=2.169 mas, bpa=-2.603 degrees
! Estimated noise=526.658 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000562271 Jy
! Component: 100  -  total flux cleaned = 0.000690613 Jy
! Component: 150  -  total flux cleaned = 0.000691256 Jy
! Component: 200  -  total flux cleaned = 0.000594338 Jy
! Total flux subtracted in 200 components = 0.000594338 Jy
! Clean residual min=-0.002512 max=0.002323 Jy/beam
! Clean residual mean=0.000003 rms=0.000618 Jy/beam
! Combined flux in latest and established models = 0.836539 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 30 model components to the UV plane model.
! The established model now contains 122 components and 0.836539 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.149074Jy  sigma=0.001219
! Fit after  self-cal, rms=0.149034Jy  sigma=0.001219
! Inverting map 
! Your choice of large map pixels excluded 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=2.137 mas, bmaj=3.783 mas, bpa=-3.016 degrees
! Estimated noise=679.371 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 = 0.000190671 Jy
! Component: 100  -  total flux cleaned = 0.000279187 Jy
! Component: 150  -  total flux cleaned = 0.000392129 Jy
! Component: 200  -  total flux cleaned = 0.000483364 Jy
! Total flux subtracted in 200 components = 0.000483364 Jy
! Clean residual min=-0.002485 max=0.002738 Jy/beam
! Clean residual mean=0.000002 rms=0.000791 Jy/beam
! Combined flux in latest and established models = 0.837022 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 19 model components to the UV plane model.
! The established model now contains 138 components and 0.837022 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.149033Jy  sigma=0.001219
! Fit after  self-cal, rms=0.149007Jy  sigma=0.001219
! Inverting map 
! Your choice of large map pixels excluded 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.6883 mas, bmaj=1.841 mas, bpa=-2.341 degrees
! Estimated noise=821.62 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.574508 Jy
! Component: 100  -  total flux cleaned = 0.699391 Jy
! Component: 150  -  total flux cleaned = 0.752439 Jy
! Component: 200  -  total flux cleaned = 0.779522 Jy
! Total flux subtracted in 200 components = 0.779522 Jy
! Clean residual min=-0.006856 max=0.010050 Jy/beam
! Clean residual mean=-0.000015 rms=0.001376 Jy/beam
! Combined flux in latest and established models = 0.779522 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 20 model components to the UV plane model.
! The established model now contains 20 components and 0.779522 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.8627 mas, bmaj=2.169 mas, bpa=-2.603 degrees
! Estimated noise=526.658 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 = 0.0232874 Jy
! Component: 100  -  total flux cleaned = 0.0340646 Jy
! Component: 150  -  total flux cleaned = 0.04045 Jy
! Component: 200  -  total flux cleaned = 0.0450577 Jy
! Total flux subtracted in 200 components = 0.0450577 Jy
! Clean residual min=-0.002656 max=0.002975 Jy/beam
! Clean residual mean=-0.000002 rms=0.000773 Jy/beam
! Combined flux in latest and established models = 0.82458 Jy
! Adding 45 model components to the UV plane model.
! The established model now contains 58 components and 0.82458 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 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 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=2.137 mas, bmaj=3.783 mas, bpa=-3.016 degrees
! Estimated noise=679.371 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 = 0.00478363 Jy
! Component: 100  -  total flux cleaned = 0.00781982 Jy
! Component: 150  -  total flux cleaned = 0.00988659 Jy
! Component: 200  -  total flux cleaned = 0.0113354 Jy
! Total flux subtracted in 200 components = 0.0113354 Jy
! Clean residual min=-0.002639 max=0.002587 Jy/beam
! Clean residual mean=0.000000 rms=0.000816 Jy/beam
! Combined flux in latest and established models = 0.835915 Jy
! Adding 31 model components to the UV plane model.
! The established model now contains 87 components and 0.835915 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.8627 mas, bmaj=2.169 mas, bpa=-2.603 degrees
! Estimated noise=526.658 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00023882 Jy
! Component: 100  -  total flux cleaned = 0.00023789 Jy
! Component: 150  -  total flux cleaned = 0.000311535 Jy
! Component: 200  -  total flux cleaned = 0.000378796 Jy
! Total flux subtracted in 200 components = 0.000378796 Jy
! Clean residual min=-0.002344 max=0.002558 Jy/beam
! Clean residual mean=0.000001 rms=0.000634 Jy/beam
! Combined flux in latest and established models = 0.836294 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 28 model components to the UV plane model.
! The established model now contains 111 components and 0.836294 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.149128Jy  sigma=0.001219
! Fit after  self-cal, rms=0.149101Jy  sigma=0.001219
wmodel J1354-0206_X_2002_05_14_yyk\_map.mod
! Writing 111 model components to file: J1354-0206_X_2002_05_14_yyk_map.mod
wobs J1354-0206_X_2002_05_14_yyk\_uvs.fits
! Writing UV FITS file: J1354-0206_X_2002_05_14_yyk_uvs.fits
wwins J1354-0206_X_2002_05_14_yyk\_map.win
! wwins: Wrote 4 windows to J1354-0206_X_2002_05_14_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 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.000645766 Jy
! Component: 100  -  total flux cleaned = 0.000605491 Jy
! Component: 150  -  total flux cleaned = 0.0005672 Jy
! Component: 200  -  total flux cleaned = 0.000789857 Jy
! Component: 250  -  total flux cleaned = 0.00089739 Jy
! Component: 300  -  total flux cleaned = 0.00100206 Jy
! Component: 350  -  total flux cleaned = 0.00103542 Jy
! Component: 400  -  total flux cleaned = 0.0011002 Jy
! Component: 450  -  total flux cleaned = 0.0011958 Jy
! Component: 500  -  total flux cleaned = 0.00135129 Jy
! Component: 550  -  total flux cleaned = 0.0014421 Jy
! Component: 600  -  total flux cleaned = 0.00150181 Jy
! Component: 650  -  total flux cleaned = 0.00153104 Jy
! Component: 700  -  total flux cleaned = 0.00164644 Jy
! Component: 750  -  total flux cleaned = 0.0016746 Jy
! Component: 800  -  total flux cleaned = 0.00170257 Jy
! Component: 850  -  total flux cleaned = 0.00170257 Jy
! Component: 900  -  total flux cleaned = 0.00170266 Jy
! Component: 950  -  total flux cleaned = 0.00186207 Jy
! Component: 1000  -  total flux cleaned = 0.00188823 Jy
! Component: 1050  -  total flux cleaned = 0.00191478 Jy
! Component: 1100  -  total flux cleaned = 0.00194038 Jy
! Component: 1150  -  total flux cleaned = 0.0018897 Jy
! Component: 1200  -  total flux cleaned = 0.00188994 Jy
! Component: 1250  -  total flux cleaned = 0.00184017 Jy
! Component: 1300  -  total flux cleaned = 0.00179072 Jy
! Component: 1350  -  total flux cleaned = 0.00181531 Jy
! Component: 1400  -  total flux cleaned = 0.00186366 Jy
! Component: 1450  -  total flux cleaned = 0.00179163 Jy
! Component: 1500  -  total flux cleaned = 0.00181551 Jy
! Component: 1550  -  total flux cleaned = 0.00179181 Jy
! Component: 1600  -  total flux cleaned = 0.00176851 Jy
! Component: 1650  -  total flux cleaned = 0.00183864 Jy
! Component: 1700  -  total flux cleaned = 0.00190752 Jy
! Component: 1750  -  total flux cleaned = 0.00186148 Jy
! Component: 1800  -  total flux cleaned = 0.00170245 Jy
! Component: 1850  -  total flux cleaned = 0.00177021 Jy
! Component: 1900  -  total flux cleaned = 0.00170311 Jy
! Component: 1950  -  total flux cleaned = 0.00165888 Jy
! Component: 2000  -  total flux cleaned = 0.00165887 Jy
! Total flux subtracted in 2048 components = 0.00157156 Jy
! Clean residual min=-0.001267 max=0.001808 Jy/beam
! Clean residual mean=0.000001 rms=0.000426 Jy/beam
! Combined flux in latest and established models = 0.837866 Jy
keep
! Adding 160 model components to the UV plane model.
! The established model now contains 271 components and 0.837866 Jy
![Exited script file: muppet]
wmap "J1354-0206_X_2002_05_14_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8627 x 2.169 at -2.603 degrees (North through East)
! Clean map  min=-0.0018827  max=0.67928 Jy/beam
! Writing clean map to FITS file: J1354-0206_X_2002_05_14_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.679278 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.147% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000425972 
device "J1354-0206_X_2002_05_14_yyk\_map.eps/VPS"
! Attempting to open device: 'J1354-0206_X_2002_05_14_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.188129 0.188129 0.376257 0.752514 1.50503 3.01006 6.02012 12.0402 24.0805 48.1609 96.3218
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0012 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.679 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8627 x 2.169 at -2.603 degrees (North through East)
! Clean map  min=-0.0018827  max=0.67928 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1354-0206_X_2002_05_14_yyk\_map.gif/gif"
! Attempting to open device: 'J1354-0206_X_2002_05_14_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1354-0206_X_2002_05_14_yyk_uvs.log closed on Tue Jun 26 22:52:25 2007