! Started logfile: J2109-4110_X_2002_01_31_yyk_uvs.log on Wed Jun 27 11:04:06 2007
obs J2109-4110_X_2002_01_31_yyk_uva.fits
! Reading UV FITS file: J2109-4110_X_2002_01_31_yyk_uva.fits
! AN table 1: 35 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.450159 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J2109-4110
! 
! 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 2836 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 J2109-4110_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)= 1.12436 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 1.16% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.6224 mas, bmaj=1.643 mas, bpa=0.03547 degrees
! Estimated noise=3335.87 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 = 0.85095 Jy
! Component: 100  -  total flux cleaned = 1.06736 Jy
! Total flux subtracted in 100 components = 1.06736 Jy
! Clean residual min=-0.114455 max=0.099976 Jy/beam
! Clean residual mean=0.000615 rms=0.030012 Jy/beam
! Combined flux in latest and established models = 1.06736 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 8 model components to the UV plane model.
! The established model now contains 8 components and 1.06736 Jy
! 
! Correcting IF 1.
!  A total of 113 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 113 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 113 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 113 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.386297Jy  sigma=0.002537
! Fit after  self-cal, rms=0.384794Jy  sigma=0.002528
! Inverting map and beam 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.6224 mas, bmaj=1.643 mas, bpa=0.036 degrees
! Estimated noise=3340.74 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 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.7604 mas, bmaj=2.078 mas, bpa=1.503 degrees
! Estimated noise=2114.76 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 = 0.188565 Jy
! Component: 100  -  total flux cleaned = 0.254983 Jy
! Component: 150  -  total flux cleaned = 0.278631 Jy
! Component: 200  -  total flux cleaned = 0.28017 Jy
! Total flux subtracted in 200 components = 0.28017 Jy
! Clean residual min=-0.088934 max=0.070029 Jy/beam
! Clean residual mean=0.001633 rms=0.025412 Jy/beam
! Combined flux in latest and established models = 1.34753 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 19 components and 1.34753 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.352248Jy  sigma=0.002159
! Fit after  self-cal, rms=0.352173Jy  sigma=0.002158
! Inverting map 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7604 x 2.078 at 1.503 degrees (North through East)
! Clean map  min=-0.084009  max=1.0887 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: 0.985527
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.88     HN        1.00*    KP        1.07     
!   LA        1.26     MK        0.99     NL        1.00*    OV        0.96     
!   PT        0.98     SC        1.01     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 0.99527
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.87     HN        1.00*    KP        1.01     
!   LA        1.24     MK        1.00     NL        1.00*    OV        0.94     
!   PT        1.01     SC        0.98     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 0.971752
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.84     HN        1.00*    KP        1.05     
!   LA        1.27     MK        1.02     NL        1.00*    OV        0.98     
!   PT        1.06     SC        1.07     
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 0.956993
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.83     HN        1.00*    KP        1.14     
!   LA        1.27     MK        1.06     NL        1.00*    OV        1.00     
!   PT        1.13     SC        1.02     
! 
! 
! Fit before self-cal, rms=0.352173Jy  sigma=0.002158
! Fit after  self-cal, rms=0.318188Jy  sigma=0.001936
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=0.318188Jy  sigma=0.001936
! Fit after  self-cal, rms=0.318199Jy  sigma=0.001936
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.7688 mas, bmaj=2.104 mas, bpa=1.343 degrees
! Estimated noise=2015.08 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 (3.2, 2).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0209932 Jy
! Component: 100  -  total flux cleaned = 0.0168509 Jy
! Component: 150  -  total flux cleaned = 0.0112998 Jy
! Component: 200  -  total flux cleaned = 0.00768239 Jy
! Total flux subtracted in 200 components = 0.00768239 Jy
! Clean residual min=-0.016599 max=0.017092 Jy/beam
! Clean residual mean=-0.000015 rms=0.005284 Jy/beam
! Combined flux in latest and established models = 1.35521 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 20 model components to the UV plane model.
! The established model now contains 38 components and 1.35521 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.307901Jy  sigma=0.001866
! Fit after  self-cal, rms=0.307792Jy  sigma=0.001865
! Inverting map 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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=0.307792Jy  sigma=0.001865
! Fit after  self-cal, rms=0.272601Jy  sigma=0.001559
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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 = 0.00760848 Jy
! Component: 100  -  total flux cleaned = 0.00688501 Jy
! Component: 150  -  total flux cleaned = 0.00606881 Jy
! Component: 200  -  total flux cleaned = 0.00606991 Jy
! Total flux subtracted in 200 components = 0.00606991 Jy
! Clean residual min=-0.014845 max=0.017362 Jy/beam
! Clean residual mean=0.000014 rms=0.004799 Jy/beam
! Combined flux in latest and established models = 1.36128 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 17 model components to the UV plane model.
! The established model now contains 48 components and 1.36128 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.272223Jy  sigma=0.001554
! Fit after  self-cal, rms=0.263425Jy  sigma=0.001482
! Inverting map 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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: 0.7688 x 2.104 at 1.343 degrees (North through East)
! Clean map  min=-0.015143  max=1.077 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=0.263425Jy  sigma=0.001482
! Fit after  self-cal, rms=0.262995Jy  sigma=0.001463
! 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=0.262995Jy  sigma=0.001463
! Fit after  self-cal, rms=0.260398Jy  sigma=0.001443
! Inverting map and beam 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.7633 mas, bmaj=2.101 mas, bpa=1.646 degrees
! Estimated noise=2001.4 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.010461 Jy
! Component: 100  -  total flux cleaned = 0.0128555 Jy
! Component: 150  -  total flux cleaned = 0.0134809 Jy
! Component: 200  -  total flux cleaned = 0.0134799 Jy
! Total flux subtracted in 200 components = 0.0134799 Jy
! Clean residual min=-0.010872 max=0.011007 Jy/beam
! Clean residual mean=-0.000095 rms=0.003289 Jy/beam
! Combined flux in latest and established models = 1.37476 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 17 model components to the UV plane model.
! The established model now contains 60 components and 1.37476 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.260187Jy  sigma=0.001441
! Fit after  self-cal, rms=0.259392Jy  sigma=0.001435
! Inverting map 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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=0.259392Jy  sigma=0.001435
! Fit after  self-cal, rms=0.259438Jy  sigma=0.001431
! 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=0.259438Jy  sigma=0.001431
! Fit after  self-cal, rms=0.259218Jy  sigma=0.001429
! Inverting map and beam 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.7628 mas, bmaj=2.1 mas, bpa=1.697 degrees
! Estimated noise=1999.71 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00563188 Jy
! Component: 100  -  total flux cleaned = 0.00634028 Jy
! Component: 150  -  total flux cleaned = 0.00624631 Jy
! Component: 200  -  total flux cleaned = 0.00632184 Jy
! Total flux subtracted in 200 components = 0.00632184 Jy
! Clean residual min=-0.009862 max=0.009738 Jy/beam
! Clean residual mean=-0.000112 rms=0.002902 Jy/beam
! Combined flux in latest and established models = 1.38108 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 18 model components to the UV plane model.
! The established model now contains 69 components and 1.38108 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.259145Jy  sigma=0.001429
! Fit after  self-cal, rms=0.259082Jy  sigma=0.001428
! Inverting map 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=2.719 mas, bmaj=10.55 mas, bpa=3.72 degrees
! Estimated noise=2736.39 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 = 0.000500381 Jy
! Component: 100  -  total flux cleaned = 6.96664e-05 Jy
! Component: 150  -  total flux cleaned = 7.22703e-05 Jy
! Component: 200  -  total flux cleaned = 6.92074e-05 Jy
! Total flux subtracted in 200 components = 6.92074e-05 Jy
! Clean residual min=-0.009012 max=0.013452 Jy/beam
! Clean residual mean=-0.000236 rms=0.004493 Jy/beam
! Combined flux in latest and established models = 1.38115 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 72 components and 1.38115 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.259099Jy  sigma=0.001428
! Fit after  self-cal, rms=0.259089Jy  sigma=0.001429
! Inverting map 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.6218 mas, bmaj=1.644 mas, bpa=0.3346 degrees
! Estimated noise=3219.1 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.837249 Jy
! Component: 100  -  total flux cleaned = 1.04994 Jy
! Component: 150  -  total flux cleaned = 1.1685 Jy
! Component: 200  -  total flux cleaned = 1.24397 Jy
! Total flux subtracted in 200 components = 1.24397 Jy
! Clean residual min=-0.029860 max=0.038026 Jy/beam
! Clean residual mean=-0.000114 rms=0.008990 Jy/beam
! Combined flux in latest and established models = 1.24397 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 17 model components to the UV plane model.
! The established model now contains 17 components and 1.24397 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.7628 mas, bmaj=2.1 mas, bpa=1.697 degrees
! Estimated noise=1999.71 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 = 0.0727641 Jy
! Component: 100  -  total flux cleaned = 0.103544 Jy
! Component: 150  -  total flux cleaned = 0.120712 Jy
! Component: 200  -  total flux cleaned = 0.130969 Jy
! Total flux subtracted in 200 components = 0.130969 Jy
! Clean residual min=-0.013765 max=0.009971 Jy/beam
! Clean residual mean=-0.000101 rms=0.003454 Jy/beam
! Combined flux in latest and established models = 1.37494 Jy
! Adding 24 model components to the UV plane model.
! The established model now contains 33 components and 1.37494 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=2.719 mas, bmaj=10.55 mas, bpa=3.72 degrees
! Estimated noise=2736.39 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 = 0.00912199 Jy
! Component: 100  -  total flux cleaned = 0.0124609 Jy
! Component: 150  -  total flux cleaned = 0.0131577 Jy
! Component: 200  -  total flux cleaned = 0.0134729 Jy
! Total flux subtracted in 200 components = 0.0134729 Jy
! Clean residual min=-0.012539 max=0.014267 Jy/beam
! Clean residual mean=-0.000199 rms=0.004718 Jy/beam
! Combined flux in latest and established models = 1.38841 Jy
! Adding 13 model components to the UV plane model.
! The established model now contains 44 components and 1.38841 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.7628 mas, bmaj=2.1 mas, bpa=1.697 degrees
! Estimated noise=1999.71 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.000409074 Jy
! Component: 100  -  total flux cleaned = 0.00013671 Jy
! Component: 150  -  total flux cleaned = 0.000258226 Jy
! Component: 200  -  total flux cleaned = 0.000485876 Jy
! Total flux subtracted in 200 components = 0.000485876 Jy
! Clean residual min=-0.011450 max=0.010290 Jy/beam
! Clean residual mean=-0.000095 rms=0.003104 Jy/beam
! Combined flux in latest and established models = 1.38889 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 17 model components to the UV plane model.
! The established model now contains 56 components and 1.38889 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.259313Jy  sigma=0.001430
! Fit after  self-cal, rms=0.259273Jy  sigma=0.001430
wmodel J2109-4110_X_2002_01_31_yyk\_map.mod
! Writing 56 model components to file: J2109-4110_X_2002_01_31_yyk_map.mod
wobs J2109-4110_X_2002_01_31_yyk\_uvs.fits
! Applying 35 buffered edits.
! Writing UV FITS file: J2109-4110_X_2002_01_31_yyk_uvs.fits
wwins J2109-4110_X_2002_01_31_yyk\_map.win
! wwins: Wrote 2 windows to J2109-4110_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 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00106204 Jy
! Component: 100  -  total flux cleaned = -0.00074467 Jy
! Component: 150  -  total flux cleaned = 1.21281e-05 Jy
! Component: 200  -  total flux cleaned = 0.00111032 Jy
! Component: 250  -  total flux cleaned = 0.00212485 Jy
! Component: 300  -  total flux cleaned = 0.00259597 Jy
! Component: 350  -  total flux cleaned = 0.003273 Jy
! Component: 400  -  total flux cleaned = 0.00392213 Jy
! Component: 450  -  total flux cleaned = 0.00486166 Jy
! Component: 500  -  total flux cleaned = 0.00576622 Jy
! Component: 550  -  total flux cleaned = 0.00663899 Jy
! Component: 600  -  total flux cleaned = 0.0076657 Jy
! Component: 650  -  total flux cleaned = 0.00820635 Jy
! Component: 700  -  total flux cleaned = 0.00873302 Jy
! Component: 750  -  total flux cleaned = 0.00907551 Jy
! Component: 800  -  total flux cleaned = 0.009496 Jy
! Component: 850  -  total flux cleaned = 0.00991107 Jy
! Component: 900  -  total flux cleaned = 0.0103205 Jy
! Component: 950  -  total flux cleaned = 0.0107249 Jy
! Component: 1000  -  total flux cleaned = 0.0112824 Jy
! Component: 1050  -  total flux cleaned = 0.0115181 Jy
! Component: 1100  -  total flux cleaned = 0.0116737 Jy
! Component: 1150  -  total flux cleaned = 0.0116741 Jy
! Component: 1200  -  total flux cleaned = 0.0116741 Jy
! Component: 1250  -  total flux cleaned = 0.0116734 Jy
! Component: 1300  -  total flux cleaned = 0.0117503 Jy
! Component: 1350  -  total flux cleaned = 0.0116729 Jy
! Component: 1400  -  total flux cleaned = 0.0115959 Jy
! Component: 1450  -  total flux cleaned = 0.0113613 Jy
! Component: 1500  -  total flux cleaned = 0.0112821 Jy
! Component: 1550  -  total flux cleaned = 0.0112026 Jy
! Component: 1600  -  total flux cleaned = 0.0111228 Jy
! Component: 1650  -  total flux cleaned = 0.0110427 Jy
! Component: 1700  -  total flux cleaned = 0.0109603 Jy
! Component: 1750  -  total flux cleaned = 0.0108776 Jy
! Component: 1800  -  total flux cleaned = 0.0107092 Jy
! Component: 1850  -  total flux cleaned = 0.0104523 Jy
! Component: 1900  -  total flux cleaned = 0.0101889 Jy
! Component: 1950  -  total flux cleaned = 0.0100111 Jy
! Component: 2000  -  total flux cleaned = 0.00973953 Jy
! Total flux subtracted in 2048 components = 0.00964547 Jy
! Clean residual min=-0.005161 max=0.005206 Jy/beam
! Clean residual mean=-0.000048 rms=0.001638 Jy/beam
! Combined flux in latest and established models = 1.39854 Jy
keep
! Adding 97 model components to the UV plane model.
! The established model now contains 153 components and 1.39854 Jy
![Exited script file: muppet]
wmap "J2109-4110_X_2002_01_31_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7628 x 2.1 at 1.697 degrees (North through East)
! Clean map  min=-0.0066449  max=1.0573 Jy/beam
! Writing clean map to FITS file: J2109-4110_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 1.05727 
invert
! Inverting map 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.0017413 
device "J2109-4110_X_2002_01_31_yyk\_map.eps/VPS"
! Attempting to open device: 'J2109-4110_X_2002_01_31_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.494094 0.494094 0.988188 1.97638 3.95275 7.9055 15.811 31.622 63.244
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0052 
print "peak=",int(peak_flux*1000)/1000
! peak= 1.057 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7628 x 2.1 at 1.697 degrees (North through East)
! Clean map  min=-0.0066449  max=1.0573 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J2109-4110_X_2002_01_31_yyk\_map.gif/gif"
! Attempting to open device: 'J2109-4110_X_2002_01_31_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J2109-4110_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 11:04:12 2007