! Started logfile: J1737-2251_X_2007_01_11_yyk_uvs.log on Mon Jun 16 20:14:56 2008
obs J1737-2251_X_2007_01_11_yyk_uve.fits
! Reading UV FITS file: J1737-2251_X_2007_01_11_yyk_uve.fits
! AN table 1: 15 integrations on 36 of 36 possible baselines.
! Apparent sampling: 0.516667 visibilities/baseline/integration-bin.
! Found source: J1737-2251
! 
! 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 2143 lines of history.
! 
! Reading 1116 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 J1737-2251_X_2007_01_11_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)= 0.118142 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 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 milli-arcsec
! Estimated beam: bmin=1.188 mas, bmaj=3.466 mas, bpa=-20.65 degrees
! Estimated noise=2.17977 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 = 0.0731622 Jy
! Component: 100  -  total flux cleaned = 0.0960734 Jy
! Total flux subtracted in 100 components = 0.0960734 Jy
! Clean residual min=-0.012015 max=0.013365 Jy/beam
! Clean residual mean=0.000048 rms=0.004017 Jy/beam
! Combined flux in latest and established models = 0.0960734 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 20 model components to the UV plane model.
! The established model now contains 20 components and 0.0960734 Jy
! 
! Correcting IF 1.
!  A total of 36 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 36 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 39 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.079008Jy  sigma=1.230041
! Fit after  self-cal, rms=0.074234Jy  sigma=1.185176
! Inverting map and beam 
! Your choice of large map pixels excluded 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 milli-arcsec
! Estimated beam: bmin=1.188 mas, bmaj=3.466 mas, bpa=-20.65 degrees
! Estimated noise=2.17977 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 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 milli-arcsec
! Estimated beam: bmin=1.929 mas, bmaj=3.814 mas, bpa=-9.194 degrees
! Estimated noise=1.33178 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 = 0.0244381 Jy
! Component: 100  -  total flux cleaned = 0.0353128 Jy
! Component: 150  -  total flux cleaned = 0.0407947 Jy
! Component: 200  -  total flux cleaned = 0.0423988 Jy
! Total flux subtracted in 200 components = 0.0423988 Jy
! Clean residual min=-0.006595 max=0.007575 Jy/beam
! Clean residual mean=0.000062 rms=0.002187 Jy/beam
! Combined flux in latest and established models = 0.138472 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 25 model components to the UV plane model.
! The established model now contains 35 components and 0.138472 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.070082Jy  sigma=1.087341
! Fit after  self-cal, rms=0.070040Jy  sigma=1.087150
! Inverting map 
! Your choice of large map pixels excluded 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 1.929 x 3.814 at -9.194 degrees (North through East)
! Clean map  min=-0.0061043  max=0.087761 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
!  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*    OV        1.00*    PT        1.00*    
!   SC        1.00*    
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.01527
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.93     FD        0.96     HN        1.00*    KP        0.98     
!   LA        0.99     MK        1.00*    OV        0.99     PT        1.01     
!   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*    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*    OV        1.00*    PT        1.00*    
!   SC        1.00*    
! 
! 
! Fit before self-cal, rms=0.070040Jy  sigma=1.087150
! Fit after  self-cal, rms=0.069871Jy  sigma=1.086594
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=0.069871Jy  sigma=1.086594
! Fit after  self-cal, rms=0.069870Jy  sigma=1.086593
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 milli-arcsec
! Estimated beam: bmin=1.931 mas, bmaj=3.791 mas, bpa=-8.829 degrees
! Estimated noise=1.32705 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 = 0.000870122 Jy
! Component: 100  -  total flux cleaned = 0.00107327 Jy
! Component: 150  -  total flux cleaned = 0.0013564 Jy
! Component: 200  -  total flux cleaned = 0.00162193 Jy
! Total flux subtracted in 200 components = 0.00162193 Jy
! Clean residual min=-0.006190 max=0.006817 Jy/beam
! Clean residual mean=0.000066 rms=0.002056 Jy/beam
! Combined flux in latest and established models = 0.140094 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 12 model components to the UV plane model.
! The established model now contains 38 components and 0.140094 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.069741Jy  sigma=1.083500
! Fit after  self-cal, rms=0.069733Jy  sigma=1.083473
! Inverting map 
! Your choice of large map pixels excluded 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 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=0.069733Jy  sigma=1.083473
! Fit after  self-cal, rms=0.063463Jy  sigma=0.961407
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 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 = 0.00540748 Jy
! Component: 100  -  total flux cleaned = 0.00651273 Jy
! Component: 150  -  total flux cleaned = 0.00669316 Jy
! Component: 200  -  total flux cleaned = 0.00685642 Jy
! Total flux subtracted in 200 components = 0.00685642 Jy
! Clean residual min=-0.005622 max=0.006137 Jy/beam
! Clean residual mean=0.000043 rms=0.001941 Jy/beam
! Combined flux in latest and established models = 0.146951 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 10 model components to the UV plane model.
! The established model now contains 40 components and 0.146951 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.063173Jy  sigma=0.954078
! Fit after  self-cal, rms=0.062771Jy  sigma=0.947294
! Inverting map 
! Your choice of large map pixels excluded 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 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: 1.931 x 3.791 at -8.829 degrees (North through East)
! Clean map  min=-0.0052534  max=0.08985 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 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 milli-arcsec
! Estimated beam: bmin=2.919 mas, bmaj=8.5 mas, bpa=23.94 degrees
! Estimated noise=1.39208 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 = 0.00140577 Jy
! Component: 100  -  total flux cleaned = 0.00164383 Jy
! Component: 150  -  total flux cleaned = 0.00179028 Jy
! Component: 200  -  total flux cleaned = 0.00193166 Jy
! Total flux subtracted in 200 components = 0.00193166 Jy
! Clean residual min=-0.005525 max=0.006112 Jy/beam
! Clean residual mean=0.000047 rms=0.002001 Jy/beam
! Combined flux in latest and established models = 0.148882 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 7 model components to the UV plane model.
! The established model now contains 41 components and 0.148882 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062793Jy  sigma=0.946493
! Fit after  self-cal, rms=0.062762Jy  sigma=0.945763
! Inverting map 
! Your choice of large map pixels excluded 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 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 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 milli-arcsec
! Estimated beam: bmin=1.19 mas, bmaj=3.456 mas, bpa=-20.61 degrees
! Estimated noise=2.17199 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0825899 Jy
! Component: 100  -  total flux cleaned = 0.109702 Jy
! Component: 150  -  total flux cleaned = 0.124016 Jy
! Component: 200  -  total flux cleaned = 0.132368 Jy
! Total flux subtracted in 200 components = 0.132368 Jy
! Clean residual min=-0.009763 max=0.009899 Jy/beam
! Clean residual mean=0.000032 rms=0.002790 Jy/beam
! Combined flux in latest and established models = 0.132368 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 22 model components to the UV plane model.
! The established model now contains 22 components and 0.132368 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 milli-arcsec
! Estimated beam: bmin=1.931 mas, bmaj=3.791 mas, bpa=-8.829 degrees
! Estimated noise=1.32705 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 = 0.00859753 Jy
! Component: 100  -  total flux cleaned = 0.0112245 Jy
! Component: 150  -  total flux cleaned = 0.0118868 Jy
! Component: 200  -  total flux cleaned = 0.0123407 Jy
! Total flux subtracted in 200 components = 0.0123407 Jy
! Clean residual min=-0.005736 max=0.007158 Jy/beam
! Clean residual mean=0.000042 rms=0.002101 Jy/beam
! Combined flux in latest and established models = 0.144709 Jy
! Adding 13 model components to the UV plane model.
! The established model now contains 30 components and 0.144709 Jy
! Inverting map 
! Your choice of large map pixels excluded 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 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 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 milli-arcsec
! Estimated beam: bmin=2.919 mas, bmaj=8.5 mas, bpa=23.94 degrees
! Estimated noise=1.39208 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 = 0.00190478 Jy
! Component: 100  -  total flux cleaned = 0.00220751 Jy
! Component: 150  -  total flux cleaned = 0.00239285 Jy
! Component: 200  -  total flux cleaned = 0.00257077 Jy
! Total flux subtracted in 200 components = 0.00257077 Jy
! Clean residual min=-0.005803 max=0.006430 Jy/beam
! Clean residual mean=0.000050 rms=0.002118 Jy/beam
! Combined flux in latest and established models = 0.147279 Jy
! Adding 7 model components to the UV plane model.
! The established model now contains 33 components and 0.147279 Jy
! Inverting map 
! Your choice of large map pixels excluded 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 milli-arcsec
! Estimated beam: bmin=1.931 mas, bmaj=3.791 mas, bpa=-8.829 degrees
! Estimated noise=1.32705 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.00052938 Jy
! Component: 100  -  total flux cleaned = -0.000532504 Jy
! Component: 150  -  total flux cleaned = -0.000540143 Jy
! Component: 200  -  total flux cleaned = -0.000467092 Jy
! Total flux subtracted in 200 components = -0.000467092 Jy
! Clean residual min=-0.005719 max=0.006237 Jy/beam
! Clean residual mean=0.000044 rms=0.001935 Jy/beam
! Combined flux in latest and established models = 0.146812 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 10 model components to the UV plane model.
! The established model now contains 39 components and 0.146812 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062834Jy  sigma=0.947623
! Fit after  self-cal, rms=0.062641Jy  sigma=0.945521
wmodel J1737-2251_X_2007_01_11_yyk\_map.mod
! Writing 39 model components to file: J1737-2251_X_2007_01_11_yyk_map.mod
wobs J1737-2251_X_2007_01_11_yyk\_uvs.fits
! Writing UV FITS file: J1737-2251_X_2007_01_11_yyk_uvs.fits
wwins J1737-2251_X_2007_01_11_yyk\_map.win
! wwins: Wrote 1 windows to J1737-2251_X_2007_01_11_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 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 milli-arcsec
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.0019171 Jy
! Component: 100  -  total flux cleaned = 0.00281237 Jy
! Component: 150  -  total flux cleaned = 0.00299712 Jy
! Component: 200  -  total flux cleaned = 0.00316376 Jy
! Component: 250  -  total flux cleaned = 0.00292975 Jy
! Component: 300  -  total flux cleaned = 0.00300011 Jy
! Component: 350  -  total flux cleaned = 0.00320841 Jy
! Component: 400  -  total flux cleaned = 0.00347357 Jy
! Component: 450  -  total flux cleaned = 0.00378968 Jy
! Component: 500  -  total flux cleaned = 0.0041519 Jy
! Component: 550  -  total flux cleaned = 0.00449952 Jy
! Component: 600  -  total flux cleaned = 0.00494275 Jy
! Component: 650  -  total flux cleaned = 0.00547142 Jy
! Component: 700  -  total flux cleaned = 0.00587469 Jy
! Component: 750  -  total flux cleaned = 0.0063102 Jy
! Component: 800  -  total flux cleaned = 0.00658815 Jy
! Component: 850  -  total flux cleaned = 0.00690002 Jy
! Component: 900  -  total flux cleaned = 0.00724239 Jy
! Component: 950  -  total flux cleaned = 0.00736627 Jy
! Component: 1000  -  total flux cleaned = 0.00760767 Jy
! Total flux subtracted in 1024 components = 0.00764708 Jy
! Clean residual min=-0.001933 max=0.002341 Jy/beam
! Clean residual mean=0.000030 rms=0.000825 Jy/beam
! Combined flux in latest and established models = 0.154459 Jy
keep
! Adding 56 model components to the UV plane model.
! The established model now contains 95 components and 0.154459 Jy
![Exited script file: muppet]
wmap "J1737-2251_X_2007_01_11_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 1.931 x 3.791 at -8.829 degrees (North through East)
! Clean map  min=-0.0039036  max=0.095344 Jy/beam
! Writing clean map to FITS file: J1737-2251_X_2007_01_11_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.0953443 
invert
! Inverting map 
! Your choice of large map pixels excluded 12% of the data.
!  The x-axis pixel size should ideally be below 0.3369 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000838258 
device "J1737-2251_X_2007_01_11_yyk\_map.eps/VPS"
! Attempting to open device: 'J1737-2251_X_2007_01_11_yyk_map.eps/VPS'
loglevs 1*100*3*image_rms/peak_flux
! The new contour levels are:
!  -2.63757 2.63757 5.27514 10.5503 21.1006 42.2011 84.4022
print "clev=",int(1*3*image_rms*10000)/10000
! clev= 0.0025 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.095 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 1.931 x 3.791 at -8.829 degrees (North through East)
! Clean map  min=-0.0039036  max=0.095344 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1737-2251_X_2007_01_11_yyk\_map.gif/gif"
! Attempting to open device: 'J1737-2251_X_2007_01_11_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1737-2251_X_2007_01_11_yyk_uvs.log closed on Mon Jun 16 20:14:57 2008