! Started logfile: J1121-0442_X_2005_07_09_yyk_uvs.log on Fri Jan 20 11:24:40 2006
obs J1121-0442_X_2005_07_09_yyk_uve.fits
! Reading UV FITS file: J1121-0442_X_2005_07_09_yyk_uve.fits
! AN table 1: 10 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.506667 visibilities/baseline/integration-bin.
! Found source: J1121-0442
! 
! 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 1480 lines of history.
! 
! Reading 912 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 J1121-0442_X_2005_07_09_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 = 256x256 pixels with 0.400x0.400 milli-arcsec cellsize.
phase_soltime=phase_soltime1
print "uvstat(rms)=",uvstat(rms),"Jy"
! uvstat(rms)= 0.112456 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 9.48% of the data.
!  The x-axis pixel size should ideally be below 0.3346 milli-arcsec
! Estimated beam: bmin=1.083 mas, bmaj=5.884 mas, bpa=25.22 degrees
! Estimated noise=2.92576 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 = 0.0515954 Jy
! Component: 100  -  total flux cleaned = 0.0702706 Jy
! Total flux subtracted in 100 components = 0.0702706 Jy
! Clean residual min=-0.009478 max=0.012132 Jy/beam
! Clean residual mean=-0.000028 rms=0.003094 Jy/beam
! Combined flux in latest and established models = 0.0702706 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 22 model components to the UV plane model.
! The established model now contains 22 components and 0.0702706 Jy
! 
! Correcting IF 1.
!  A total of 42 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 51 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 39 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=0.094403Jy  sigma=1.313589
! Fit after  self-cal, rms=0.088923Jy  sigma=1.207755
! Inverting map and beam 
! Your choice of large map pixels excluded 9.5% of the data.
!  The x-axis pixel size should ideally be below 0.3346 milli-arcsec
! Estimated beam: bmin=1.084 mas, bmaj=5.877 mas, bpa=25.22 degrees
! Estimated noise=2.92449 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 9.5% of the data.
!  The x-axis pixel size should ideally be below 0.3346 milli-arcsec
! Estimated beam: bmin=1.678 mas, bmaj=6.723 mas, bpa=24.99 degrees
! Estimated noise=1.86945 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 = 0.0220843 Jy
! Component: 100  -  total flux cleaned = 0.0287829 Jy
! Component: 150  -  total flux cleaned = 0.0312156 Jy
! Component: 200  -  total flux cleaned = 0.0320489 Jy
! Total flux subtracted in 200 components = 0.0320489 Jy
! Clean residual min=-0.007339 max=0.007772 Jy/beam
! Clean residual mean=-0.000028 rms=0.002218 Jy/beam
! Combined flux in latest and established models = 0.102319 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 31 model components to the UV plane model.
! The established model now contains 48 components and 0.102319 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.086362Jy  sigma=1.138937
! Fit after  self-cal, rms=0.086253Jy  sigma=1.138277
! Inverting map 
! Your choice of large map pixels excluded 9.5% of the data.
!  The x-axis pixel size should ideally be below 0.3346 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 1.678 x 6.723 at 24.99 degrees (North through East)
! Clean map  min=-0.0066224  max=0.074872 Jy/beam
if(peak(flux) < thresh*2)
  selflims ampcor_selflim
  end if
! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2.
! Selfcal phase corrections will not be limited.
gscale
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Amplitude normalization factor in sub-array 1: 1.06224
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.85     FD        0.89     HN        1.00*    KP        0.90     
!   LA        1.02     MK        1.00*    NL        1.00*    OV        0.91     
!   PT        0.92     SC        0.92     
! 
! 
! Correcting IF 2.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Amplitude normalization factor in sub-array 1: 1
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    OV        1.00*    
!   PT        1.00*    SC        1.00*    
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 1
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    OV        1.00*    
!   PT        1.00*    SC        1.00*    
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 1
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    OV        1.00*    
!   PT        1.00*    SC        1.00*    
! 
! 
! Fit before self-cal, rms=0.086253Jy  sigma=1.138277
! Fit after  self-cal, rms=0.085554Jy  sigma=1.136267
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=0.085554Jy  sigma=1.136267
! Fit after  self-cal, rms=0.085558Jy  sigma=1.136217
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 9.55% of the data.
!  The x-axis pixel size should ideally be below 0.3346 milli-arcsec
! Estimated beam: bmin=1.68 mas, bmaj=6.613 mas, bpa=25.22 degrees
! Estimated noise=1.84565 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 = 0.000914397 Jy
! Component: 100  -  total flux cleaned = 0.00139623 Jy
! Component: 150  -  total flux cleaned = 0.00156031 Jy
! Component: 200  -  total flux cleaned = 0.00178589 Jy
! Total flux subtracted in 200 components = 0.00178589 Jy
! Clean residual min=-0.006950 max=0.006650 Jy/beam
! Clean residual mean=-0.000024 rms=0.002027 Jy/beam
! Combined flux in latest and established models = 0.104105 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 53 components and 0.104105 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.085460Jy  sigma=1.133517
! Fit after  self-cal, rms=0.085430Jy  sigma=1.133371
! Inverting map 
! Your choice of large map pixels excluded 9.55% of the data.
!  The x-axis pixel size should ideally be below 0.3346 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=0.085430Jy  sigma=1.133371
! Fit after  self-cal, rms=0.076143Jy  sigma=0.979204
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 9.55% of the data.
!  The x-axis pixel size should ideally be below 0.3346 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 = 0.00566374 Jy
! Component: 100  -  total flux cleaned = 0.00590887 Jy
! Component: 150  -  total flux cleaned = 0.00599095 Jy
! Component: 200  -  total flux cleaned = 0.00606266 Jy
! Total flux subtracted in 200 components = 0.00606266 Jy
! Clean residual min=-0.006317 max=0.006105 Jy/beam
! Clean residual mean=-0.000016 rms=0.001746 Jy/beam
! Combined flux in latest and established models = 0.110168 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 65 components and 0.110168 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.075627Jy  sigma=0.967824
! Fit after  self-cal, rms=0.073645Jy  sigma=0.948061
! Inverting map 
! Your choice of large map pixels excluded 9.55% of the data.
!  The x-axis pixel size should ideally be below 0.3346 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: 1.68 x 6.613 at 25.22 degrees (North through East)
! Clean map  min=-0.0066512  max=0.081963 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
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 9.55% of the data.
!  The x-axis pixel size should ideally be below 0.3346 milli-arcsec
! Estimated beam: bmin=3.33 mas, bmaj=6.877 mas, bpa=31.08 degrees
! Estimated noise=1.95291 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 = 0.00129617 Jy
! Component: 100  -  total flux cleaned = 0.0014004 Jy
! Component: 150  -  total flux cleaned = 0.00149068 Jy
! Component: 200  -  total flux cleaned = 0.00160518 Jy
! Total flux subtracted in 200 components = 0.00160518 Jy
! Clean residual min=-0.005413 max=0.005388 Jy/beam
! Clean residual mean=-0.000013 rms=0.001802 Jy/beam
! Combined flux in latest and established models = 0.111773 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 76 components and 0.111773 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.073582Jy  sigma=0.947473
! Fit after  self-cal, rms=0.073117Jy  sigma=0.944036
! Inverting map 
! Your choice of large map pixels excluded 9.55% of the data.
!  The x-axis pixel size should ideally be below 0.3346 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 9.55% of the data.
!  The x-axis pixel size should ideally be below 0.3346 milli-arcsec
! Estimated beam: bmin=1.087 mas, bmaj=5.85 mas, bpa=25.25 degrees
! Estimated noise=2.886 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0662827 Jy
! Component: 100  -  total flux cleaned = 0.0874459 Jy
! Component: 150  -  total flux cleaned = 0.0979449 Jy
! Component: 200  -  total flux cleaned = 0.101323 Jy
! Total flux subtracted in 200 components = 0.101323 Jy
! Clean residual min=-0.007921 max=0.008241 Jy/beam
! Clean residual mean=-0.000015 rms=0.002313 Jy/beam
! Combined flux in latest and established models = 0.101323 Jy
uvw 0,-2
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -2.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Adding 24 model components to the UV plane model.
! The established model now contains 24 components and 0.101323 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 9.55% of the data.
!  The x-axis pixel size should ideally be below 0.3346 milli-arcsec
! Estimated beam: bmin=1.68 mas, bmaj=6.613 mas, bpa=25.22 degrees
! Estimated noise=1.84565 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 = 0.0067632 Jy
! Component: 100  -  total flux cleaned = 0.00827092 Jy
! Component: 150  -  total flux cleaned = 0.00852669 Jy
! Component: 200  -  total flux cleaned = 0.00863984 Jy
! Total flux subtracted in 200 components = 0.00863984 Jy
! Clean residual min=-0.005932 max=0.006231 Jy/beam
! Clean residual mean=-0.000020 rms=0.001825 Jy/beam
! Combined flux in latest and established models = 0.109963 Jy
! Adding 22 model components to the UV plane model.
! The established model now contains 40 components and 0.109963 Jy
! Inverting map 
! Your choice of large map pixels excluded 9.55% of the data.
!  The x-axis pixel size should ideally be below 0.3346 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 9.55% of the data.
!  The x-axis pixel size should ideally be below 0.3346 milli-arcsec
! Estimated beam: bmin=3.33 mas, bmaj=6.877 mas, bpa=31.08 degrees
! Estimated noise=1.95291 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 = 0.00127925 Jy
! Component: 100  -  total flux cleaned = 0.00145171 Jy
! Component: 150  -  total flux cleaned = 0.00167565 Jy
! Component: 200  -  total flux cleaned = 0.00186292 Jy
! Total flux subtracted in 200 components = 0.00186292 Jy
! Clean residual min=-0.005331 max=0.005481 Jy/beam
! Clean residual mean=-0.000015 rms=0.001830 Jy/beam
! Combined flux in latest and established models = 0.111826 Jy
! Adding 17 model components to the UV plane model.
! The established model now contains 55 components and 0.111826 Jy
! Inverting map 
! Your choice of large map pixels excluded 9.55% of the data.
!  The x-axis pixel size should ideally be below 0.3346 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 9.55% of the data.
!  The x-axis pixel size should ideally be below 0.3346 milli-arcsec
! Estimated beam: bmin=1.68 mas, bmaj=6.613 mas, bpa=25.22 degrees
! Estimated noise=1.84565 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.000528694 Jy
! Component: 100  -  total flux cleaned = -0.00053853 Jy
! Component: 150  -  total flux cleaned = -0.000539953 Jy
! Component: 200  -  total flux cleaned = -0.00054084 Jy
! Total flux subtracted in 200 components = -0.00054084 Jy
! Clean residual min=-0.006239 max=0.005862 Jy/beam
! Clean residual mean=-0.000013 rms=0.001727 Jy/beam
! Combined flux in latest and established models = 0.111285 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 11 model components to the UV plane model.
! The established model now contains 62 components and 0.111285 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.073674Jy  sigma=0.948508
! Fit after  self-cal, rms=0.073360Jy  sigma=0.946631
wmodel J1121-0442_X_2005_07_09_yyk\_map.mod
! Writing 62 model components to file: J1121-0442_X_2005_07_09_yyk_map.mod
wobs J1121-0442_X_2005_07_09_yyk\_uvs.fits
! Writing UV FITS file: J1121-0442_X_2005_07_09_yyk_uvs.fits
wwins J1121-0442_X_2005_07_09_yyk\_map.win
! wwins: Wrote 1 windows to J1121-0442_X_2005_07_09_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 9.55% of the data.
!  The x-axis pixel size should ideally be below 0.3346 milli-arcsec
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.00059852 Jy
! Component: 100  -  total flux cleaned = 0.00154511 Jy
! Component: 150  -  total flux cleaned = 0.00239395 Jy
! Component: 200  -  total flux cleaned = 0.00293745 Jy
! Component: 250  -  total flux cleaned = 0.00293676 Jy
! Component: 300  -  total flux cleaned = 0.00280161 Jy
! Component: 350  -  total flux cleaned = 0.00273762 Jy
! Component: 400  -  total flux cleaned = 0.00279816 Jy
! Component: 450  -  total flux cleaned = 0.00285833 Jy
! Component: 500  -  total flux cleaned = 0.00297632 Jy
! Component: 550  -  total flux cleaned = 0.00320224 Jy
! Component: 600  -  total flux cleaned = 0.00325713 Jy
! Component: 650  -  total flux cleaned = 0.00320446 Jy
! Component: 700  -  total flux cleaned = 0.00315402 Jy
! Component: 750  -  total flux cleaned = 0.00295399 Jy
! Component: 800  -  total flux cleaned = 0.00280747 Jy
! Component: 850  -  total flux cleaned = 0.00256902 Jy
! Component: 900  -  total flux cleaned = 0.00224324 Jy
! Component: 950  -  total flux cleaned = 0.00215204 Jy
! Component: 1000  -  total flux cleaned = 0.00188363 Jy
! Total flux subtracted in 1024 components = 0.00206095 Jy
! Clean residual min=-0.002537 max=0.002945 Jy/beam
! Clean residual mean=0.000002 rms=0.000937 Jy/beam
! Combined flux in latest and established models = 0.113346 Jy
keep
! Adding 63 model components to the UV plane model.
! The established model now contains 125 components and 0.113346 Jy
![Exited script file: muppet]
wmap "J1121-0442_X_2005_07_09_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 9.55% of the data.
!  The x-axis pixel size should ideally be below 0.3346 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 1.68 x 6.613 at 25.22 degrees (North through East)
! Clean map  min=-0.005426  max=0.082561 Jy/beam
! Writing clean map to FITS file: J1121-0442_X_2005_07_09_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.0825613 
invert
! Inverting map 
! Your choice of large map pixels excluded 9.55% of the data.
!  The x-axis pixel size should ideally be below 0.3346 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000909557 
device "J1121-0442_X_2005_07_09_yyk\_map.eps/VPS"
! Attempting to open device: 'J1121-0442_X_2005_07_09_yyk_map.eps/VPS'
loglevs 1*100*3*image_rms/peak_flux
! The new contour levels are:
!  -3.30502 3.30502 6.61005 13.2201 26.4402 52.8804
print "clev=",int(1*3*image_rms*10000)/10000
! clev= 0.0027 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.082 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 1.68 x 6.613 at 25.22 degrees (North through East)
! Clean map  min=-0.005426  max=0.082561 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1121-0442_X_2005_07_09_yyk\_map.gif/gif"
! Attempting to open device: 'J1121-0442_X_2005_07_09_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1121-0442_X_2005_07_09_yyk_uvs.log closed on Fri Jan 20 11:24:41 2006