! Started logfile: J1239-1023_X_2004_05_27_yyk_uvs.log on Wed Dec  7 01:05:58 2005
obs J1239-1023_X_2004_05_27_yyk_uve.fits
! Reading UV FITS file: J1239-1023_X_2004_05_27_yyk_uve.fits
! AN table 1: 24 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.851852 visibilities/baseline/integration-bin.
! Found source: J1239-1023
! 
! 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 1380 lines of history.
! 
! Reading 3680 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 J1239-1023_X_2004_05_27_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)= 0.801436 Jy 
startmod ,phase_soltime
! Applying default point source starting model.
! Performing phase self-cal over 10 minute time intervals
! 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 40 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 40 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 40 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 40 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.408232Jy  sigma=7.140770
! Fit after  self-cal, rms=0.399596Jy  sigma=7.100975
! 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 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.6181 mas, bmaj=1.683 mas, bpa=-0.7725 degrees
! Estimated noise=0.992148 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 = 0.553396 Jy
! Component: 100  -  total flux cleaned = 0.715723 Jy
! Total flux subtracted in 100 components = 0.715723 Jy
! Clean residual min=-0.028210 max=0.089130 Jy/beam
! Clean residual mean=-0.000136 rms=0.007972 Jy/beam
! Combined flux in latest and established models = 0.715723 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 0.715723 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.267202Jy  sigma=5.228925
! Fit after  self-cal, rms=0.267353Jy  sigma=5.222446
! Inverting map 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Added new window around map position (0.8, -0.2).
! clean: niter=100  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.1047 Jy
! Component: 100  -  total flux cleaned = 0.1564 Jy
! Total flux subtracted in 100 components = 0.1564 Jy
! Clean residual min=-0.025943 max=0.085731 Jy/beam
! Clean residual mean=-0.000082 rms=0.006071 Jy/beam
! Combined flux in latest and established models = 0.872123 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 12 model components to the UV plane model.
! The established model now contains 20 components and 0.872123 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.206254Jy  sigma=3.932812
! Fit after  self-cal, rms=0.205859Jy  sigma=3.905638
! Inverting map 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Added new window around map position (-2.2, -0.6).
! clean: niter=100  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0872107 Jy
! Component: 100  -  total flux cleaned = 0.134237 Jy
! Total flux subtracted in 100 components = 0.134237 Jy
! Clean residual min=-0.016582 max=0.036937 Jy/beam
! Clean residual mean=-0.000059 rms=0.004107 Jy/beam
! Combined flux in latest and established models = 1.00636 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 14 model components to the UV plane model.
! The established model now contains 34 components and 1.00636 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.151734Jy  sigma=2.809621
! Fit after  self-cal, rms=0.147107Jy  sigma=2.730822
! Inverting map 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Added new window around map position (-1.4, 0).
! clean: niter=100  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0490282 Jy
! Component: 100  -  total flux cleaned = 0.0815259 Jy
! Total flux subtracted in 100 components = 0.0815259 Jy
! Clean residual min=-0.012583 max=0.017706 Jy/beam
! Clean residual mean=-0.000041 rms=0.002954 Jy/beam
! Combined flux in latest and established models = 1.08789 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 16 model components to the UV plane model.
! The established model now contains 49 components and 1.08789 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.119879Jy  sigma=2.151742
! Fit after  self-cal, rms=0.117600Jy  sigma=2.118920
! Inverting map 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! clean: niter=100  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.028899 Jy
! Component: 100  -  total flux cleaned = 0.0497026 Jy
! Total flux subtracted in 100 components = 0.0497026 Jy
! Clean residual min=-0.010102 max=0.015163 Jy/beam
! Clean residual mean=-0.000030 rms=0.002397 Jy/beam
! Combined flux in latest and established models = 1.13759 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 24 model components to the UV plane model.
! The established model now contains 62 components and 1.13759 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.104942Jy  sigma=1.835362
! Fit after  self-cal, rms=0.104199Jy  sigma=1.824881
! Inverting map 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8328 mas, bmaj=2.106 mas, bpa=0.5212 degrees
! Estimated noise=0.648758 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 = 0.0437739 Jy
! Component: 100  -  total flux cleaned = 0.0697967 Jy
! Component: 150  -  total flux cleaned = 0.0868995 Jy
! Component: 200  -  total flux cleaned = 0.0984698 Jy
! Total flux subtracted in 200 components = 0.0984698 Jy
! Clean residual min=-0.011395 max=0.010496 Jy/beam
! Clean residual mean=-0.000020 rms=0.003173 Jy/beam
! Combined flux in latest and established models = 1.23606 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 50 model components to the UV plane model.
! The established model now contains 93 components and 1.23606 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.090823Jy  sigma=1.509281
! Fit after  self-cal, rms=0.090347Jy  sigma=1.501754
! Inverting map 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
selflims ampcor_selflim
! 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: 1.01283
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.97     FD        0.99     HN        1.01     KP        0.99     
!   LA        0.98     MK        0.99     NL        1.02     OV        1.01     
!   PT        0.95     SC        0.98     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.01753
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        0.99     HN        1.01     KP        0.94     
!   LA        0.96     MK        1.00     NL        0.99     OV        0.99     
!   PT        1.00     SC        0.96     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 1.00044
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.05     FD        1.05     HN        0.93     KP        0.91     
!   LA        0.98     MK        1.03     NL        0.99     OV        1.03     
!   PT        1.03     SC        1.00     
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 0.975126
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.06     FD        1.05     HN        0.97     KP        0.95     
!   LA        0.98     MK        1.03     NL        1.02     OV        1.05     
!   PT        1.10     SC        1.04     
! 
! 
! Fit before self-cal, rms=0.090347Jy  sigma=1.501754
! Fit after  self-cal, rms=0.081126Jy  sigma=1.299497
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=0.081126Jy  sigma=1.299497
! Fit after  self-cal, rms=0.081120Jy  sigma=1.299464
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8347 mas, bmaj=2.114 mas, bpa=0.7223 degrees
! Estimated noise=0.648926 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 = 0.00795132 Jy
! Component: 100  -  total flux cleaned = 0.0105634 Jy
! Component: 150  -  total flux cleaned = 0.0114205 Jy
! Component: 200  -  total flux cleaned = 0.0119395 Jy
! Total flux subtracted in 200 components = 0.0119395 Jy
! Clean residual min=-0.005706 max=0.011441 Jy/beam
! Clean residual mean=0.000008 rms=0.002228 Jy/beam
! Combined flux in latest and established models = 1.248 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 21 model components to the UV plane model.
! The established model now contains 101 components and 1.248 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.080733Jy  sigma=1.286117
! Fit after  self-cal, rms=0.080650Jy  sigma=1.285049
! Inverting map 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Added new window around map position (0.8, -11.8).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.013211 Jy
! Component: 100  -  total flux cleaned = 0.0198658 Jy
! Component: 150  -  total flux cleaned = 0.0246122 Jy
! Component: 200  -  total flux cleaned = 0.0277645 Jy
! Total flux subtracted in 200 components = 0.0277645 Jy
! Clean residual min=-0.005088 max=0.007463 Jy/beam
! Clean residual mean=0.000008 rms=0.001424 Jy/beam
! Combined flux in latest and established models = 1.27576 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 43 model components to the UV plane model.
! The established model now contains 136 components and 1.27576 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.079398Jy  sigma=1.248721
! Fit after  self-cal, rms=0.079292Jy  sigma=1.247397
! Inverting map 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Added new window around map position (-11.2, 11.8).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00772461 Jy
! Component: 100  -  total flux cleaned = 0.0100511 Jy
! Component: 150  -  total flux cleaned = 0.0113303 Jy
! Component: 200  -  total flux cleaned = 0.0119396 Jy
! Total flux subtracted in 200 components = 0.0119396 Jy
! Clean residual min=-0.004798 max=0.005060 Jy/beam
! Clean residual mean=0.000011 rms=0.001208 Jy/beam
! Combined flux in latest and established models = 1.2877 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 36 model components to the UV plane model.
! The established model now contains 158 components and 1.2877 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.078521Jy  sigma=1.234348
! Fit after  self-cal, rms=0.078419Jy  sigma=1.232599
! Inverting map 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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=0.078419Jy  sigma=1.232599
! Fit after  self-cal, rms=0.076795Jy  sigma=1.194078
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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)
! Added new window around map position (4.4, -14.2).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00492331 Jy
! Component: 100  -  total flux cleaned = 0.00576574 Jy
! Component: 150  -  total flux cleaned = 0.00641147 Jy
! Component: 200  -  total flux cleaned = 0.00685817 Jy
! Total flux subtracted in 200 components = 0.00685817 Jy
! Clean residual min=-0.004611 max=0.004278 Jy/beam
! Clean residual mean=0.000015 rms=0.001114 Jy/beam
! Combined flux in latest and established models = 1.29456 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 33 model components to the UV plane model.
! The established model now contains 186 components and 1.29456 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.075968Jy  sigma=1.182588
! Fit after  self-cal, rms=0.075927Jy  sigma=1.178016
! Inverting map 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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: 0.8347 x 2.114 at 0.7223 degrees (North through East)
! Clean map  min=-0.0044537  max=0.71164 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=0.075927Jy  sigma=1.178016
! Fit after  self-cal, rms=0.069070Jy  sigma=1.036505
! 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=0.069070Jy  sigma=1.036505
! Fit after  self-cal, rms=0.069119Jy  sigma=1.035923
! Inverting map and beam 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8336 mas, bmaj=2.113 mas, bpa=0.6829 degrees
! Estimated noise=0.646015 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00192801 Jy
! Component: 100  -  total flux cleaned = 0.0032286 Jy
! Component: 150  -  total flux cleaned = 0.00435435 Jy
! Component: 200  -  total flux cleaned = 0.00491347 Jy
! Total flux subtracted in 200 components = 0.00491347 Jy
! Clean residual min=-0.003257 max=0.003290 Jy/beam
! Clean residual mean=-0.000006 rms=0.000809 Jy/beam
! Combined flux in latest and established models = 1.29947 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 38 model components to the UV plane model.
! The established model now contains 214 components and 1.29947 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.068776Jy  sigma=1.029946
! Fit after  self-cal, rms=0.068771Jy  sigma=1.029180
! Inverting map 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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=0.068771Jy  sigma=1.029180
! Fit after  self-cal, rms=0.066819Jy  sigma=1.000361
! 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=0.066819Jy  sigma=1.000361
! Fit after  self-cal, rms=0.066833Jy  sigma=1.000268
! Inverting map and beam 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8332 mas, bmaj=2.113 mas, bpa=0.7024 degrees
! Estimated noise=0.644664 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.000857333 Jy
! Component: 100  -  total flux cleaned = -7.88074e-05 Jy
! Component: 150  -  total flux cleaned = 0.000371049 Jy
! Component: 200  -  total flux cleaned = 0.00071131 Jy
! Total flux subtracted in 200 components = 0.00071131 Jy
! Clean residual min=-0.002957 max=0.003102 Jy/beam
! Clean residual mean=-0.000010 rms=0.000759 Jy/beam
! Combined flux in latest and established models = 1.30019 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 42 model components to the UV plane model.
! The established model now contains 229 components and 1.30019 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066635Jy  sigma=0.996725
! Fit after  self-cal, rms=0.066633Jy  sigma=0.996470
! Inverting map 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=2.233 mas, bmaj=4.292 mas, bpa=3.184 degrees
! Estimated noise=0.846061 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 = 0.00314853 Jy
! Component: 100  -  total flux cleaned = 0.00383152 Jy
! Component: 150  -  total flux cleaned = 0.00417769 Jy
! Component: 200  -  total flux cleaned = 0.00441336 Jy
! Total flux subtracted in 200 components = 0.00441336 Jy
! Clean residual min=-0.004081 max=0.003867 Jy/beam
! Clean residual mean=-0.000021 rms=0.000962 Jy/beam
! Combined flux in latest and established models = 1.3046 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 248 components and 1.3046 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066577Jy  sigma=0.995539
! Fit after  self-cal, rms=0.066590Jy  sigma=0.995287
! Inverting map 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
uvtaper 0,0
! 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 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.6182 mas, bmaj=1.688 mas, bpa=-0.8011 degrees
! Estimated noise=0.991943 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.552147 Jy
! Component: 100  -  total flux cleaned = 0.7355 Jy
! Component: 150  -  total flux cleaned = 0.847991 Jy
! Component: 200  -  total flux cleaned = 0.927192 Jy
! Total flux subtracted in 200 components = 0.927192 Jy
! Clean residual min=-0.015645 max=0.033571 Jy/beam
! Clean residual mean=-0.000084 rms=0.004475 Jy/beam
! Combined flux in latest and established models = 0.927192 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 26 model components to the UV plane model.
! The established model now contains 26 components and 0.927192 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8332 mas, bmaj=2.113 mas, bpa=0.7024 degrees
! Estimated noise=0.644664 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 (-0.6, 0).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.128461 Jy
! Component: 100  -  total flux cleaned = 0.20025 Jy
! Component: 150  -  total flux cleaned = 0.244136 Jy
! Component: 200  -  total flux cleaned = 0.271677 Jy
! Total flux subtracted in 200 components = 0.271677 Jy
! Clean residual min=-0.007639 max=0.011012 Jy/beam
! Clean residual mean=-0.000060 rms=0.003270 Jy/beam
! Combined flux in latest and established models = 1.19887 Jy
! Adding 66 model components to the UV plane model.
! The established model now contains 78 components and 1.19887 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=2.233 mas, bmaj=4.292 mas, bpa=3.184 degrees
! Estimated noise=0.846061 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 = 0.0311817 Jy
! Component: 100  -  total flux cleaned = 0.0500597 Jy
! Component: 150  -  total flux cleaned = 0.0632834 Jy
! Component: 200  -  total flux cleaned = 0.0731224 Jy
! Total flux subtracted in 200 components = 0.0731224 Jy
! Clean residual min=-0.004812 max=0.007135 Jy/beam
! Clean residual mean=-0.000043 rms=0.002171 Jy/beam
! Combined flux in latest and established models = 1.27199 Jy
! Adding 99 model components to the UV plane model.
! The established model now contains 167 components and 1.27199 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8332 mas, bmaj=2.113 mas, bpa=0.7024 degrees
! Estimated noise=0.644664 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00659718 Jy
! Component: 100  -  total flux cleaned = 0.0115154 Jy
! Component: 150  -  total flux cleaned = 0.0155243 Jy
! Component: 200  -  total flux cleaned = 0.0174666 Jy
! Total flux subtracted in 200 components = 0.0174666 Jy
! Clean residual min=-0.003760 max=0.003809 Jy/beam
! Clean residual mean=-0.000013 rms=0.000891 Jy/beam
! Combined flux in latest and established models = 1.28946 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 44 model components to the UV plane model.
! The established model now contains 206 components and 1.28946 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067387Jy  sigma=1.009434
! Fit after  self-cal, rms=0.067214Jy  sigma=1.006135
wmodel J1239-1023_X_2004_05_27_yyk\_map.mod
! Writing 206 model components to file: J1239-1023_X_2004_05_27_yyk_map.mod
wobs J1239-1023_X_2004_05_27_yyk\_uvs.fits
! Writing UV FITS file: J1239-1023_X_2004_05_27_yyk_uvs.fits
wwins J1239-1023_X_2004_05_27_yyk\_map.win
! wwins: Wrote 8 windows to J1239-1023_X_2004_05_27_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 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.00124311 Jy
! Component: 100  -  total flux cleaned = 0.00170765 Jy
! Component: 150  -  total flux cleaned = 0.00203222 Jy
! Component: 200  -  total flux cleaned = 0.00229053 Jy
! Component: 250  -  total flux cleaned = 0.00263758 Jy
! Component: 300  -  total flux cleaned = 0.00297066 Jy
! Component: 350  -  total flux cleaned = 0.0033396 Jy
! Component: 400  -  total flux cleaned = 0.00378626 Jy
! Component: 450  -  total flux cleaned = 0.0040901 Jy
! Component: 500  -  total flux cleaned = 0.00425941 Jy
! Component: 550  -  total flux cleaned = 0.00425945 Jy
! Component: 600  -  total flux cleaned = 0.00442277 Jy
! Component: 650  -  total flux cleaned = 0.00446189 Jy
! Component: 700  -  total flux cleaned = 0.00450093 Jy
! Component: 750  -  total flux cleaned = 0.0044623 Jy
! Component: 800  -  total flux cleaned = 0.00450053 Jy
! Component: 850  -  total flux cleaned = 0.00450092 Jy
! Component: 900  -  total flux cleaned = 0.00457438 Jy
! Component: 950  -  total flux cleaned = 0.00450147 Jy
! Component: 1000  -  total flux cleaned = 0.00450178 Jy
! Component: 1050  -  total flux cleaned = 0.00446672 Jy
! Component: 1100  -  total flux cleaned = 0.00460653 Jy
! Component: 1150  -  total flux cleaned = 0.00460648 Jy
! Component: 1200  -  total flux cleaned = 0.00450417 Jy
! Component: 1250  -  total flux cleaned = 0.00450445 Jy
! Component: 1300  -  total flux cleaned = 0.004438 Jy
! Component: 1350  -  total flux cleaned = 0.00440457 Jy
! Component: 1400  -  total flux cleaned = 0.00433896 Jy
! Component: 1450  -  total flux cleaned = 0.00417686 Jy
! Component: 1500  -  total flux cleaned = 0.00404876 Jy
! Component: 1550  -  total flux cleaned = 0.00398534 Jy
! Component: 1600  -  total flux cleaned = 0.00385993 Jy
! Component: 1650  -  total flux cleaned = 0.00379785 Jy
! Component: 1700  -  total flux cleaned = 0.00379777 Jy
! Component: 1750  -  total flux cleaned = 0.00370549 Jy
! Component: 1800  -  total flux cleaned = 0.00361455 Jy
! Component: 1850  -  total flux cleaned = 0.00355433 Jy
! Component: 1900  -  total flux cleaned = 0.00346481 Jy
! Component: 1950  -  total flux cleaned = 0.00328758 Jy
! Component: 2000  -  total flux cleaned = 0.00325844 Jy
! Total flux subtracted in 2048 components = 0.00308436 Jy
! Clean residual min=-0.001569 max=0.001642 Jy/beam
! Clean residual mean=-0.000011 rms=0.000561 Jy/beam
! Combined flux in latest and established models = 1.29254 Jy
keep
! Adding 137 model components to the UV plane model.
! The established model now contains 342 components and 1.29254 Jy
![Exited script file: muppet]
wmap "J1239-1023_X_2004_05_27_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8332 x 2.113 at 0.7024 degrees (North through East)
! Clean map  min=-0.0026904  max=0.70514 Jy/beam
! Writing clean map to FITS file: J1239-1023_X_2004_05_27_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.705143 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.203% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000558813 
device "J1239-1023_X_2004_05_27_yyk\_map.eps/VPS"
! Attempting to open device: 'J1239-1023_X_2004_05_27_yyk_map.eps/VPS'
loglevs 2*100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.475489 0.475489 0.950979 1.90196 3.80391 7.60783 15.2157 30.4313 60.8626
print "clev=",int(2*3*image_rms*10000)/10000
! clev= 0.0033 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.705 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8332 x 2.113 at 0.7024 degrees (North through East)
! Clean map  min=-0.0026904  max=0.70514 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1239-1023_X_2004_05_27_yyk\_map.gif/gif"
! Attempting to open device: 'J1239-1023_X_2004_05_27_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1239-1023_X_2004_05_27_yyk_uvs.log closed on Wed Dec  7 01:06:04 2005