! Started logfile: J1736-1944_S_2004_05_27_yyk_uvs.log on Wed Dec  7 01:04:33 2005
obs J1736-1944_S_2004_05_27_yyk_uve.fits
! Reading UV FITS file: J1736-1944_S_2004_05_27_yyk_uve.fits
! AN table 1: 15 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.380741 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J1736-1944
! 
! 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  2.23697e+09        8e+06          1        8e+06
!  02        2  2.26697e+09        8e+06          1        8e+06
!  03        3  2.35697e+09        8e+06          1        8e+06
!  04        4  2.37697e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 1383 lines of history.
! 
! Reading 1028 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 J1736-1944_S_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 = 256x256 pixels with 1.00x1.00 milli-arcsec cellsize.
phase_soltime=phase_soltime1
print "uvstat(rms)=",uvstat(rms),"Jy"
! uvstat(rms)= 0.109603 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 60 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 95 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 90 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 150 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.938083Jy  sigma=14.837549
! Fit after  self-cal, rms=0.930453Jy  sigma=14.774872
! 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 
! Estimated beam: bmin=8.096 mas, bmaj=19.38 mas, bpa=-0.5851 degrees
! Estimated noise=3.52409 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 = 0.0682795 Jy
! Component: 100  -  total flux cleaned = 0.0795988 Jy
! Total flux subtracted in 100 components = 0.0795988 Jy
! Clean residual min=-0.011510 max=0.011467 Jy/beam
! Clean residual mean=-0.000289 rms=0.003748 Jy/beam
! Combined flux in latest and established models = 0.0795988 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 15 components and 0.0795988 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.079559Jy  sigma=0.999481
! Fit after  self-cal, rms=0.079469Jy  sigma=0.995921
! Inverting map 
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 
! Estimated beam: bmin=8.888 mas, bmaj=23.58 mas, bpa=-4.301 degrees
! Estimated noise=2.14144 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 = -0.000449384 Jy
! Component: 100  -  total flux cleaned = -0.00118873 Jy
! Component: 150  -  total flux cleaned = -0.00147689 Jy
! Component: 200  -  total flux cleaned = -0.00173589 Jy
! Total flux subtracted in 200 components = -0.00173589 Jy
! Clean residual min=-0.005537 max=0.004474 Jy/beam
! Clean residual mean=-0.000152 rms=0.001525 Jy/beam
! Combined flux in latest and established models = 0.0778629 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 17 model components to the UV plane model.
! The established model now contains 31 components and 0.0778629 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.078931Jy  sigma=0.989469
! Fit after  self-cal, rms=0.078936Jy  sigma=0.989215
! Inverting map 
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
!  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 2.
!  Amplitude normalization factor in sub-array 1: 0.995525
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.94     HN        1.00*    KP        1.00     
!   LA        1.00*    MK        1.00*    NL        0.98     OV        1.14     
!   PT        0.99     SC        1.00*    
! 
! 
! Correcting IF 3.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Amplitude normalization factor in sub-array 1: 1.03083
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.84     FD        0.89     HN        1.00*    KP        1.00*    
!   LA        0.90     MK        1.00*    NL        0.96     OV        1.05     
!   PT        1.05     SC        1.00*    
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 1
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.00*    FD        0.00*    HN        0.00*    KP        0.00*    
!   LA        0.00*    MK        0.00*    NL        0.00*    OV        0.00*    
!   PT        0.00*    SC        0.00*    
! 
! 
! Fit before self-cal, rms=0.078936Jy  sigma=0.989215
! Fit after  self-cal, rms=0.076957Jy  sigma=0.987335
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=0.076957Jy  sigma=0.987335
! Fit after  self-cal, rms=0.076867Jy  sigma=0.986521
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=8.955 mas, bmaj=22.86 mas, bpa=-4.059 degrees
! Estimated noise=2.14609 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 = -0.000861211 Jy
! Component: 100  -  total flux cleaned = -0.00122616 Jy
! Component: 150  -  total flux cleaned = -0.00135422 Jy
! Component: 200  -  total flux cleaned = -0.00147016 Jy
! Total flux subtracted in 200 components = -0.00147016 Jy
! Clean residual min=-0.005773 max=0.004399 Jy/beam
! Clean residual mean=-0.000113 rms=0.001508 Jy/beam
! Combined flux in latest and established models = 0.0763927 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 18 model components to the UV plane model.
! The established model now contains 48 components and 0.0763927 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.076735Jy  sigma=0.984671
! Fit after  self-cal, rms=0.076741Jy  sigma=0.984614
! Inverting map 
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=0.076741Jy  sigma=0.984614
! Fit after  self-cal, rms=0.069435Jy  sigma=0.872127
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
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 = 0.00315866 Jy
! Component: 100  -  total flux cleaned = 0.00299661 Jy
! Component: 150  -  total flux cleaned = 0.00231824 Jy
! Component: 200  -  total flux cleaned = 0.0020147 Jy
! Total flux subtracted in 200 components = 0.0020147 Jy
! Clean residual min=-0.004541 max=0.004095 Jy/beam
! Clean residual mean=-0.000072 rms=0.001424 Jy/beam
! Combined flux in latest and established models = 0.0784074 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 58 components and 0.0784074 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.069039Jy  sigma=0.864521
! Fit after  self-cal, rms=0.068393Jy  sigma=0.855036
! Inverting map 
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: 8.955 x 22.86 at -4.059 degrees (North through East)
! Clean map  min=-0.0047461  max=0.082046 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 = 20 mega-wavelengths.
win_mult = win_mult * 1.4
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=10.21 mas, bmaj=23.96 mas, bpa=-2.515 degrees
! Estimated noise=2.18914 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 = 0.000267602 Jy
! Component: 100  -  total flux cleaned = 8.84682e-06 Jy
! Component: 150  -  total flux cleaned = -0.000170697 Jy
! Component: 200  -  total flux cleaned = -0.000337407 Jy
! Total flux subtracted in 200 components = -0.000337407 Jy
! Clean residual min=-0.004867 max=0.004160 Jy/beam
! Clean residual mean=-0.000079 rms=0.001456 Jy/beam
! Combined flux in latest and established models = 0.07807 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 19 model components to the UV plane model.
! The established model now contains 69 components and 0.07807 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.068285Jy  sigma=0.853703
! Fit after  self-cal, rms=0.068143Jy  sigma=0.852325
! Inverting map 
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 
! Estimated beam: bmin=8.076 mas, bmaj=18.96 mas, bpa=0.3339 degrees
! Estimated noise=3.35897 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.073834 Jy
! Component: 100  -  total flux cleaned = 0.0846287 Jy
! Component: 150  -  total flux cleaned = 0.0830567 Jy
! Component: 200  -  total flux cleaned = 0.0805843 Jy
! Total flux subtracted in 200 components = 0.0805843 Jy
! Clean residual min=-0.009591 max=0.010154 Jy/beam
! Clean residual mean=-0.000188 rms=0.002937 Jy/beam
! Combined flux in latest and established models = 0.0805843 Jy
uvw 0,-2
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -2.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Adding 20 model components to the UV plane model.
! The established model now contains 20 components and 0.0805843 Jy
! Inverting map and beam 
! Estimated beam: bmin=8.955 mas, bmaj=22.86 mas, bpa=-4.059 degrees
! Estimated noise=2.14609 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 = -0.00327904 Jy
! Component: 100  -  total flux cleaned = -0.00354711 Jy
! Component: 150  -  total flux cleaned = -0.00376998 Jy
! Component: 200  -  total flux cleaned = -0.00389437 Jy
! Total flux subtracted in 200 components = -0.00389437 Jy
! Clean residual min=-0.004337 max=0.004207 Jy/beam
! Clean residual mean=-0.000064 rms=0.001445 Jy/beam
! Combined flux in latest and established models = 0.07669 Jy
! Adding 17 model components to the UV plane model.
! The established model now contains 36 components and 0.07669 Jy
! Inverting map 
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 20 mega-wavelengths.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=10.21 mas, bmaj=23.96 mas, bpa=-2.515 degrees
! Estimated noise=2.18914 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 = 0.0002071 Jy
! Component: 100  -  total flux cleaned = 0.000167769 Jy
! Component: 150  -  total flux cleaned = 0.00020538 Jy
! Component: 200  -  total flux cleaned = 0.000206158 Jy
! Total flux subtracted in 200 components = 0.000206158 Jy
! Clean residual min=-0.004610 max=0.004092 Jy/beam
! Clean residual mean=-0.000071 rms=0.001481 Jy/beam
! Combined flux in latest and established models = 0.0768961 Jy
! Adding 10 model components to the UV plane model.
! The established model now contains 42 components and 0.0768961 Jy
! Inverting map 
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Estimated beam: bmin=8.955 mas, bmaj=22.86 mas, bpa=-4.059 degrees
! Estimated noise=2.14609 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.000102503 Jy
! Component: 100  -  total flux cleaned = -0.000271508 Jy
! Component: 150  -  total flux cleaned = -0.000270985 Jy
! Component: 200  -  total flux cleaned = -0.000345447 Jy
! Total flux subtracted in 200 components = -0.000345447 Jy
! Clean residual min=-0.004213 max=0.003877 Jy/beam
! Clean residual mean=-0.000061 rms=0.001420 Jy/beam
! Combined flux in latest and established models = 0.0765507 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 51 components and 0.0765507 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067897Jy  sigma=0.849621
! Fit after  self-cal, rms=0.067765Jy  sigma=0.848849
wmodel J1736-1944_S_2004_05_27_yyk\_map.mod
! Writing 51 model components to file: J1736-1944_S_2004_05_27_yyk_map.mod
wobs J1736-1944_S_2004_05_27_yyk\_uvs.fits
! Writing UV FITS file: J1736-1944_S_2004_05_27_yyk_uvs.fits
wwins J1736-1944_S_2004_05_27_yyk\_map.win
! wwins: Wrote 1 windows to J1736-1944_S_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 
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00195685 Jy
! Component: 100  -  total flux cleaned = -0.00290256 Jy
! Component: 150  -  total flux cleaned = -0.00302847 Jy
! Component: 200  -  total flux cleaned = -0.00314298 Jy
! Component: 250  -  total flux cleaned = -0.00319578 Jy
! Component: 300  -  total flux cleaned = -0.00348959 Jy
! Component: 350  -  total flux cleaned = -0.00371929 Jy
! Component: 400  -  total flux cleaned = -0.00406738 Jy
! Component: 450  -  total flux cleaned = -0.00431813 Jy
! Component: 500  -  total flux cleaned = -0.00427764 Jy
! Component: 550  -  total flux cleaned = -0.00435618 Jy
! Component: 600  -  total flux cleaned = -0.0043177 Jy
! Component: 650  -  total flux cleaned = -0.00424372 Jy
! Component: 700  -  total flux cleaned = -0.00417196 Jy
! Component: 750  -  total flux cleaned = -0.00417211 Jy
! Component: 800  -  total flux cleaned = -0.00410323 Jy
! Component: 850  -  total flux cleaned = -0.0041374 Jy
! Component: 900  -  total flux cleaned = -0.00413782 Jy
! Component: 950  -  total flux cleaned = -0.00423541 Jy
! Component: 1000  -  total flux cleaned = -0.00429901 Jy
! Total flux subtracted in 1024 components = -0.00429917 Jy
! Clean residual min=-0.001968 max=0.002072 Jy/beam
! Clean residual mean=-0.000062 rms=0.000748 Jy/beam
! Combined flux in latest and established models = 0.0722515 Jy
keep
! Adding 75 model components to the UV plane model.
! The established model now contains 126 components and 0.0722515 Jy
![Exited script file: muppet]
wmap "J1736-1944_S_2004_05_27_yyk\_map.fits"
! Inverting map 
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 8.955 x 22.86 at -4.059 degrees (North through East)
! Clean map  min=-0.0052598  max=0.081755 Jy/beam
! Writing clean map to FITS file: J1736-1944_S_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 0.0817554 
invert
! Inverting map 
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000745204 
device "J1736-1944_S_2004_05_27_yyk\_map.eps/VPS"
! Attempting to open device: 'J1736-1944_S_2004_05_27_yyk_map.eps/VPS'
loglevs 1*100*3*image_rms/peak_flux
! The new contour levels are:
!  -2.73451 2.73451 5.46903 10.9381 21.8761 43.7522 87.5044
print "clev=",int(1*3*image_rms*10000)/10000
! clev= 0.0022 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.081 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 8.955 x 22.86 at -4.059 degrees (North through East)
! Clean map  min=-0.0052598  max=0.081755 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1736-1944_S_2004_05_27_yyk\_map.gif/gif"
! Attempting to open device: 'J1736-1944_S_2004_05_27_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1736-1944_S_2004_05_27_yyk_uvs.log closed on Wed Dec  7 01:04:33 2005