! Started logfile: /scr/pima/rdv72_uvs/J0449+1121_X_uvs.log on Sat Oct  5 08:44:55 2013
obs /scr/pima/rdv72_uvs/J0449+1121_X_uva.fits
! Reading UV FITS file: /scr/pima/rdv72_uvs/J0449+1121_X_uva.fits
! AN table 1: 6 integrations on 3 of 3 possible baselines.
! AN table 2: 3 integrations on 1 of 1 possible baselines.
! AN table 3: 3 integrations on 1 of 1 possible baselines.
! AN table 4: 5 integrations on 6 of 6 possible baselines.
! AN table 5: 4 integrations on 1 of 1 possible baselines.
! AN table 6: 12 integrations on 28 of 28 possible baselines.
! AN table 7: 4 integrations on 3 of 3 possible baselines.
! AN table 8: 3 integrations on 45 of 45 possible baselines.
! AN table 9: 4 integrations on 36 of 36 possible baselines.
! AN table 10: 3 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.767073 visibilities/baseline/integration-bin.
! Found source: J0449+1121
! 
! 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  8.40599e+09      1.6e+07          1      1.6e+07
!  02        2  8.47599e+09      1.6e+07          1      1.6e+07
!  03        3  8.79099e+09      1.6e+07          1      1.6e+07
!  04        4  8.89599e+09      1.6e+07          1      1.6e+07
! 
! Polarization(s): RR
! 
! Read 0 lines of history.
! 
! Reading 2516 visibilities.
select RR
! 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
print "field_size =",field_size
! field_size = 1024 
print "field_cell =",field_cell
! field_cell = 0.2 
print "taper_size =",taper_size
! taper_size = 70 
![@/home/lpetrov/bin/01_muppet /scr/pima/rdv72_uvs/J0449+1121_X]
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.03
float dynam
dynam = 6.0
float soltime1
soltime1 = 120
float soltime2
soltime2 = 20
float thresh
thresh = 0.5
float win_mult
win_mult = 1.8
float time_av
time_av = 16
float old_peak
float new_peak
float flux_cutoff
mapsize field_size, field_cell
! Map grid = 1024x1024 pixels with 0.200x0.200 milli-arcsec cellsize.
startmod
! Applying default point source starting model.
! Performing phase self-cal
! 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 6 telescope corrections were flagged in sub-array 2.
!  A total of 6 telescope corrections were flagged in sub-array 3.
!  A total of 4 telescope corrections were flagged in sub-array 4.
!  A total of 8 telescope corrections were flagged in sub-array 5.
!  A total of 14 telescope corrections were flagged in sub-array 6.
!  A total of 10 telescope corrections were flagged in sub-array 8.
!  A total of 5 telescope corrections were flagged in sub-array 9.
!  A total of 2 telescope corrections were flagged in sub-array 10.
! 
! Correcting IF 2.
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  A total of 6 telescope corrections were flagged in sub-array 3.
!  A total of 4 telescope corrections were flagged in sub-array 4.
!  A total of 8 telescope corrections were flagged in sub-array 5.
!  A total of 14 telescope corrections were flagged in sub-array 6.
!  A total of 10 telescope corrections were flagged in sub-array 8.
!  A total of 5 telescope corrections were flagged in sub-array 9.
!  A total of 2 telescope corrections were flagged in sub-array 10.
! 
! Correcting IF 3.
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  A total of 6 telescope corrections were flagged in sub-array 3.
!  A total of 4 telescope corrections were flagged in sub-array 4.
!  A total of 8 telescope corrections were flagged in sub-array 5.
!  A total of 14 telescope corrections were flagged in sub-array 6.
!  A total of 10 telescope corrections were flagged in sub-array 8.
!  A total of 5 telescope corrections were flagged in sub-array 9.
!  A total of 2 telescope corrections were flagged in sub-array 10.
! 
! Correcting IF 4.
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  A total of 6 telescope corrections were flagged in sub-array 3.
!  A total of 4 telescope corrections were flagged in sub-array 4.
!  A total of 8 telescope corrections were flagged in sub-array 5.
!  A total of 14 telescope corrections were flagged in sub-array 6.
!  A total of 10 telescope corrections were flagged in sub-array 8.
!  A total of 5 telescope corrections were flagged in sub-array 9.
!  A total of 2 telescope corrections were flagged in sub-array 10.
! 
! Fit before self-cal, rms=1.141799Jy  sigma=7.406597
! Fit after  self-cal, rms=0.562473Jy  sigma=2.766831
! clrmod: Cleared the established, tentative and continuum models.
! Redundant starting model cleared.
uvw 2,-1
! Uniform weighting binwidth: 2 (pixels).
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
! Estimated beam: bmin=0.604 mas, bmaj=1.593 mas, bpa=-10.33 degrees
! Estimated noise=3.18491 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (0, 0).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.397444 Jy
! Component: 100  -  total flux cleaned = 0.521632 Jy
! Total flux subtracted in 100 components = 0.521632 Jy
! Clean residual min=-0.029626 max=0.064497 Jy/beam
! Clean residual mean=0.000062 rms=0.007267 Jy/beam
! Combined flux in latest and established models = 0.521632 Jy
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 6 components and 0.521632 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.209252Jy  sigma=1.494091
! Fit after  self-cal, rms=0.209049Jy  sigma=1.492408
! Inverting map 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
! Added new window around map position (0.8, 0).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0685686 Jy
! Component: 100  -  total flux cleaned = 0.109058 Jy
! Total flux subtracted in 100 components = 0.109058 Jy
! Clean residual min=-0.026816 max=0.034478 Jy/beam
! Clean residual mean=0.000032 rms=0.005679 Jy/beam
! Combined flux in latest and established models = 0.63069 Jy
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 17 components and 0.63069 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.186672Jy  sigma=1.194235
! Fit after  self-cal, rms=0.185930Jy  sigma=1.189239
! Inverting map 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
print "************** FINISHED UNIFORM WEIGHTING CLEAN **************"
! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** 
! 
uvw 0,-1
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -1.
! 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 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
! Estimated beam: bmin=0.6878 mas, bmaj=1.704 mas, bpa=-11.42 degrees
! Estimated noise=2.50931 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0544925 Jy
! Component: 100  -  total flux cleaned = 0.0861093 Jy
! Component: 150  -  total flux cleaned = 0.106499 Jy
! Component: 200  -  total flux cleaned = 0.11991 Jy
! Total flux subtracted in 200 components = 0.11991 Jy
! Clean residual min=-0.031429 max=0.038099 Jy/beam
! Clean residual mean=0.000066 rms=0.007009 Jy/beam
! Combined flux in latest and established models = 0.7506 Jy
! Performing phase self-cal
! Adding 25 model components to the UV plane model.
! The established model now contains 33 components and 0.7506 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.177968Jy  sigma=1.016044
! Fit after  self-cal, rms=0.177110Jy  sigma=1.007553
! Inverting map 
! Your choice of large map pixels excluded 4.38% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 18 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   NY        0.00*    WZ        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   WZ        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   NY        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   NY        1.16     SC        0.80     WZ        0.99     ZC        1.49     
! 
!  Telescope amplitude corrections in sub-array 5:
!   NL        0.00*    NY        0.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 6.
!  Telescope amplitude corrections in sub-array 6:
!   FD        0.79     LA        0.91     NL        1.10     NY        0.99     
!   PT        0.91     SC        0.83     WZ        1.20     ZC        1.52     
! 
!  A total of 12 telescope corrections were flagged in sub-array 7.
!  Telescope amplitude corrections in sub-array 7:
!   BR        0.00*    NY        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 8:
!   BR        1.45     FD        0.79     KK        1.32     KP        1.47     
!   LA        0.93     MK        0.92     NL        1.10     OV        1.00     
!   SC        0.91     WZ        1.03     
! 
!  Telescope amplitude corrections in sub-array 9:
!   BR        1.30     FD        0.79     KK        1.14     LA        0.93     
!   MK        0.94     NL        1.11     OV        1.00     PT        0.86     
!   SC        0.89     
! 
!  Telescope amplitude corrections in sub-array 10:
!   BR        1.37     FD        0.80     KK        1.15     KP        1.43     
!   LA        0.95     MK        0.90     NL        1.07     OV        0.99     
!   PT        0.87     SC        0.84     
! 
! 
! Correcting IF 2.
!  A total of 18 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   NY        0.00*    WZ        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   WZ        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   NY        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   NY        1.11     SC        0.81     WZ        1.15     ZC        1.41     
! 
!  Telescope amplitude corrections in sub-array 5:
!   NL        0.00*    NY        0.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 6.
!  Telescope amplitude corrections in sub-array 6:
!   FD        0.81     LA        0.90     NL        1.09     NY        1.11     
!   PT        0.93     SC        0.83     WZ        1.12     ZC        1.51     
! 
!  A total of 12 telescope corrections were flagged in sub-array 7.
!  Telescope amplitude corrections in sub-array 7:
!   BR        0.00*    NY        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 8:
!   BR        1.24     FD        0.77     KK        1.23     KP        1.29     
!   LA        0.93     MK        0.93     NL        1.09     OV        1.00     
!   SC        0.89     WZ        1.28     
! 
!  Telescope amplitude corrections in sub-array 9:
!   BR        1.27     FD        0.83     KK        1.16     LA        0.92     
!   MK        0.93     NL        1.10     OV        0.94     PT        0.89     
!   SC        0.93     
! 
!  Telescope amplitude corrections in sub-array 10:
!   BR        1.38     FD        0.82     KK        1.14     KP        1.43     
!   LA        0.92     MK        0.89     NL        1.11     OV        0.91     
!   PT        0.91     SC        0.89     
! 
! 
! Correcting IF 3.
!  A total of 18 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   NY        0.00*    WZ        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   WZ        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   NY        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   NY        1.23     SC        0.80     WZ        1.18     ZC        1.14     
! 
!  Telescope amplitude corrections in sub-array 5:
!   NL        0.00*    NY        0.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 6.
!  Telescope amplitude corrections in sub-array 6:
!   FD        0.78     LA        0.98     NL        1.23     NY        1.13     
!   PT        0.98     SC        0.86     WZ        1.22     ZC        1.18     
! 
!  A total of 12 telescope corrections were flagged in sub-array 7.
!  Telescope amplitude corrections in sub-array 7:
!   BR        0.00*    NY        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 8:
!   BR        1.40     FD        0.80     KK        1.19     KP        1.32     
!   LA        0.98     MK        0.97     NL        1.09     OV        1.04     
!   SC        0.93     WZ        1.12     
! 
!  Telescope amplitude corrections in sub-array 9:
!   BR        1.44     FD        0.82     KK        1.21     LA        0.94     
!   MK        0.94     NL        1.12     OV        0.99     PT        0.94     
!   SC        0.85     
! 
!  Telescope amplitude corrections in sub-array 10:
!   BR        1.50     FD        0.86     KK        1.19     KP        1.30     
!   LA        0.98     MK        0.90     NL        1.08     OV        1.01     
!   PT        0.92     SC        0.84     
! 
! 
! Correcting IF 4.
!  A total of 18 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   NY        0.00*    WZ        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   WZ        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   NY        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   NY        1.15     SC        0.79     WZ        1.14     ZC        1.26     
! 
!  Telescope amplitude corrections in sub-array 5:
!   NL        0.00*    NY        0.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 6.
!  Telescope amplitude corrections in sub-array 6:
!   FD        0.83     LA        0.95     NL        1.21     NY        1.12     
!   PT        0.98     SC        0.93     WZ        1.20     ZC        1.26     
! 
!  A total of 12 telescope corrections were flagged in sub-array 7.
!  Telescope amplitude corrections in sub-array 7:
!   BR        0.00*    NY        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 8:
!   BR        1.42     FD        0.78     KK        1.15     KP        1.44     
!   LA        0.95     MK        1.02     NL        1.19     OV        1.07     
!   SC        0.94     WZ        1.23     
! 
!  Telescope amplitude corrections in sub-array 9:
!   BR        1.36     FD        0.87     KK        1.13     LA        0.97     
!   MK        0.91     NL        1.27     OV        0.99     PT        0.90     
!   SC        0.96     
! 
!  Telescope amplitude corrections in sub-array 10:
!   BR        1.50     FD        0.87     KK        1.23     KP        1.73     
!   LA        0.94     MK        0.97     NL        1.16     OV        1.00     
!   PT        0.93     SC        0.88     
! 
! 
! Fit before self-cal, rms=0.177110Jy  sigma=1.007553
! Fit after  self-cal, rms=0.146536Jy  sigma=0.619088
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
! Estimated beam: bmin=0.6955 mas, bmaj=1.708 mas, bpa=-11.61 degrees
! Estimated noise=2.52196 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00481496 Jy
! Component: 100  -  total flux cleaned = -0.00557723 Jy
! Component: 150  -  total flux cleaned = -0.00579466 Jy
! Component: 200  -  total flux cleaned = -0.0061762 Jy
! Total flux subtracted in 200 components = -0.0061762 Jy
! Clean residual min=-0.007252 max=0.006477 Jy/beam
! Clean residual mean=0.000032 rms=0.001600 Jy/beam
! Combined flux in latest and established models = 0.744424 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 41 components and 0.744424 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.145287Jy  sigma=0.613664
! Fit after  self-cal, rms=0.145691Jy  sigma=0.612620
! Inverting map 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
selfcal true, true, soltime1
! Performing amp+phase self-cal over 120 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.145691Jy  sigma=0.612620
! Fit after  self-cal, rms=0.144753Jy  sigma=0.611632
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
! Estimated beam: bmin=0.6966 mas, bmaj=1.703 mas, bpa=-11.5 degrees
! Estimated noise=2.51452 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00285309 Jy
! Component: 100  -  total flux cleaned = -0.0032355 Jy
! Component: 150  -  total flux cleaned = -0.00355949 Jy
! Component: 200  -  total flux cleaned = -0.00383535 Jy
! Total flux subtracted in 200 components = -0.00383535 Jy
! Clean residual min=-0.006864 max=0.006232 Jy/beam
! Clean residual mean=0.000031 rms=0.001537 Jy/beam
! Combined flux in latest and established models = 0.740588 Jy
selfcal
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 41 components and 0.740588 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.144097Jy  sigma=0.608592
! Fit after  self-cal, rms=0.144036Jy  sigma=0.608315
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000666564 Jy
! Component: 100  -  total flux cleaned = -0.00092292 Jy
! Component: 150  -  total flux cleaned = -0.00115942 Jy
! Component: 200  -  total flux cleaned = -0.00137776 Jy
! Total flux subtracted in 200 components = -0.00137776 Jy
! Clean residual min=-0.006791 max=0.006173 Jy/beam
! Clean residual mean=0.000032 rms=0.001525 Jy/beam
! Combined flux in latest and established models = 0.739211 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 42 components and 0.73921 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.143747Jy  sigma=0.606971
! Fit after  self-cal, rms=0.143724Jy  sigma=0.606854
! Inverting map 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
selfcal true, true, soltime2
! Performing amp+phase self-cal over 20 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.143724Jy  sigma=0.606854
! Fit after  self-cal, rms=0.143150Jy  sigma=0.602152
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
! Estimated beam: bmin=0.6978 mas, bmaj=1.699 mas, bpa=-11.41 degrees
! Estimated noise=2.51197 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00128376 Jy
! Component: 100  -  total flux cleaned = -0.00139717 Jy
! Component: 150  -  total flux cleaned = -0.00158782 Jy
! Component: 200  -  total flux cleaned = -0.00176296 Jy
! Total flux subtracted in 200 components = -0.00176296 Jy
! Clean residual min=-0.006239 max=0.006338 Jy/beam
! Clean residual mean=0.000030 rms=0.001462 Jy/beam
! Combined flux in latest and established models = 0.737448 Jy
selfcal
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 46 components and 0.737448 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.142919Jy  sigma=0.600994
! Fit after  self-cal, rms=0.142905Jy  sigma=0.600878
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (25.4, 47.8).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00580496 Jy
! Component: 100  -  total flux cleaned = 0.00708443 Jy
! Component: 150  -  total flux cleaned = 0.00719486 Jy
! Component: 200  -  total flux cleaned = 0.00709951 Jy
! Total flux subtracted in 200 components = 0.00709951 Jy
! Clean residual min=-0.006042 max=0.005741 Jy/beam
! Clean residual mean=0.000021 rms=0.001407 Jy/beam
! Combined flux in latest and established models = 0.744547 Jy
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 58 components and 0.744547 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.142633Jy  sigma=0.598877
! Fit after  self-cal, rms=0.142624Jy  sigma=0.598671
! Inverting map 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
win_mult = win_mult * 1.2
selfcal true, true, soltime2
! Performing amp+phase self-cal over 20 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.142624Jy  sigma=0.598671
! Fit after  self-cal, rms=0.142429Jy  sigma=0.598152
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
! Estimated beam: bmin=2.529 mas, bmaj=3.003 mas, bpa=27.72 degrees
! Estimated noise=2.87789 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00274493 Jy
! Component: 100  -  total flux cleaned = 0.00312946 Jy
! Component: 150  -  total flux cleaned = 0.00323629 Jy
! Component: 200  -  total flux cleaned = 0.00342307 Jy
! Total flux subtracted in 200 components = 0.00342307 Jy
! Clean residual min=-0.006742 max=0.007178 Jy/beam
! Clean residual mean=0.000048 rms=0.001892 Jy/beam
! Combined flux in latest and established models = 0.74797 Jy
selfcal
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 67 components and 0.74797 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.142457Jy  sigma=0.597564
! Fit after  self-cal, rms=0.142467Jy  sigma=0.597491
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00057532 Jy
! Component: 100  -  total flux cleaned = 0.00073439 Jy
! Component: 150  -  total flux cleaned = 0.000838388 Jy
! Component: 200  -  total flux cleaned = 0.00086976 Jy
! Total flux subtracted in 200 components = 0.00086976 Jy
! Clean residual min=-0.006672 max=0.007013 Jy/beam
! Clean residual mean=0.000045 rms=0.001865 Jy/beam
! Combined flux in latest and established models = 0.74884 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 69 components and 0.74884 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.142484Jy  sigma=0.597516
! Fit after  self-cal, rms=0.142483Jy  sigma=0.597504
! Inverting map 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
win_mult = win_mult / 1.2
print "************** FINISHED AMPLITUDE SELF-CAL **************"
! ************** FINISHED AMPLITUDE SELF-CAL ************** 
restore
! Inverting map and beam 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
! Estimated beam: bmin=0.6983 mas, bmaj=1.696 mas, bpa=-11.37 degrees
! Estimated noise=2.5079 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6983 x 1.696 at -11.37 degrees (North through East)
! Clean map  min=-0.0048708  max=0.51868 Jy/beam
if(peak(flux) > thresh)
  selfcal true, true
  clean clean_niter,clean_gain
  selfcal
  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
    new_peak = peak(flux)
    until(new_peak<=flux_cutoff)
  selfcal true, true
  end if
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.142483Jy  sigma=0.597504
! Fit after  self-cal, rms=0.136564Jy  sigma=0.527626
! Inverting map and beam 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
! Estimated beam: bmin=0.6967 mas, bmaj=1.696 mas, bpa=-11.33 degrees
! Estimated noise=2.50515 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -7.80355e-05 Jy
! Component: 100  -  total flux cleaned = 2.10716e-05 Jy
! Component: 150  -  total flux cleaned = 0.000101936 Jy
! Component: 200  -  total flux cleaned = 0.000178949 Jy
! Total flux subtracted in 200 components = 0.000178949 Jy
! Clean residual min=-0.006177 max=0.005824 Jy/beam
! Clean residual mean=0.000020 rms=0.001332 Jy/beam
! Combined flux in latest and established models = 0.749019 Jy
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 77 components and 0.749019 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.136408Jy  sigma=0.526973
! Fit after  self-cal, rms=0.136403Jy  sigma=0.526923
! Inverting map 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00015491 Jy
! Component: 100  -  total flux cleaned = 0.000154961 Jy
! Component: 150  -  total flux cleaned = 0.000155854 Jy
! Component: 200  -  total flux cleaned = 3.26877e-05 Jy
! Total flux subtracted in 200 components = 3.26877e-05 Jy
! Clean residual min=-0.006109 max=0.005720 Jy/beam
! Clean residual mean=0.000020 rms=0.001328 Jy/beam
! Combined flux in latest and established models = 0.749052 Jy
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 81 components and 0.749052 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.136320Jy  sigma=0.526578
! Fit after  self-cal, rms=0.136321Jy  sigma=0.526553
! Inverting map 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.136321Jy  sigma=0.526553
! Fit after  self-cal, rms=0.136214Jy  sigma=0.526389
print "************** CLEARING MODEL AND STARTING OVER **********"
! ************** CLEARING MODEL AND STARTING OVER ********** 
clrmod true
! clrmod: Cleared the established and tentative 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 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
! Estimated beam: bmin=0.6065 mas, bmaj=1.564 mas, bpa=-9.804 degrees
! Estimated noise=3.27885 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.401753 Jy
! Component: 100  -  total flux cleaned = 0.535644 Jy
! Component: 150  -  total flux cleaned = 0.605448 Jy
! Component: 200  -  total flux cleaned = 0.646851 Jy
! Total flux subtracted in 200 components = 0.646851 Jy
! Clean residual min=-0.010811 max=0.021559 Jy/beam
! Clean residual mean=0.000039 rms=0.002497 Jy/beam
! Combined flux in latest and established models = 0.646851 Jy
uvw 0,-1
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Adding 23 model components to the UV plane model.
! The established model now contains 23 components and 0.646851 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
! Estimated beam: bmin=0.6971 mas, bmaj=1.694 mas, bpa=-11.3 degrees
! Estimated noise=2.50273 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=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0355531 Jy
! Component: 100  -  total flux cleaned = 0.054925 Jy
! Component: 150  -  total flux cleaned = 0.0663454 Jy
! Component: 200  -  total flux cleaned = 0.0742764 Jy
! Total flux subtracted in 200 components = 0.0742764 Jy
! Clean residual min=-0.006937 max=0.006750 Jy/beam
! Clean residual mean=0.000050 rms=0.001588 Jy/beam
! Combined flux in latest and established models = 0.721127 Jy
! Adding 42 model components to the UV plane model.
! The established model now contains 56 components and 0.721127 Jy
! Inverting map 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
! Estimated beam: bmin=2.53 mas, bmaj=3.004 mas, bpa=27.99 degrees
! Estimated noise=2.87212 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00948273 Jy
! Component: 100  -  total flux cleaned = 0.0152474 Jy
! Component: 150  -  total flux cleaned = 0.0186641 Jy
! Component: 200  -  total flux cleaned = 0.0201404 Jy
! Total flux subtracted in 200 components = 0.0201404 Jy
! Clean residual min=-0.006886 max=0.007473 Jy/beam
! Clean residual mean=0.000066 rms=0.002024 Jy/beam
! Combined flux in latest and established models = 0.741267 Jy
flux_cutoff = imstat(rms) * dynam
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=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00119323 Jy
! Component: 100  -  total flux cleaned = 0.00217049 Jy
! Component: 150  -  total flux cleaned = 0.00297025 Jy
! Component: 200  -  total flux cleaned = 0.0035775 Jy
! Total flux subtracted in 200 components = 0.0035775 Jy
! Clean residual min=-0.006671 max=0.007619 Jy/beam
! Clean residual mean=0.000056 rms=0.001935 Jy/beam
! Combined flux in latest and established models = 0.744845 Jy
! Adding 54 model components to the UV plane model.
! The established model now contains 95 components and 0.744845 Jy
! Inverting map 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
! Estimated beam: bmin=0.6971 mas, bmaj=1.694 mas, bpa=-11.3 degrees
! Estimated noise=2.50273 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000813767 Jy
! Component: 100  -  total flux cleaned = 0.000625008 Jy
! Component: 150  -  total flux cleaned = 0.000382651 Jy
! Component: 200  -  total flux cleaned = 0.000162584 Jy
! Total flux subtracted in 200 components = 0.000162584 Jy
! Clean residual min=-0.006068 max=0.005752 Jy/beam
! Clean residual mean=0.000024 rms=0.001332 Jy/beam
! Combined flux in latest and established models = 0.745007 Jy
selfcal
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 109 components and 0.745007 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.136156Jy  sigma=0.526271
! Fit after  self-cal, rms=0.136134Jy  sigma=0.525791
wmodel /scr/pima/rdv72_uvs/J0449+1121_X_map.mod
! Writing 109 model components to file: /scr/pima/rdv72_uvs/J0449+1121_X_map.mod
wobs /scr/pima/rdv72_uvs/J0449+1121_X_uvs.fits
! Writing UV FITS file: /scr/pima/rdv72_uvs/J0449+1121_X_uvs.fits
wwins /scr/pima/rdv72_uvs/J0449+1121_X_map.win
! wwins: Wrote 3 windows to /scr/pima/rdv72_uvs/J0449+1121_X_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 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
! clean: niter=4096  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00046078 Jy
! Component: 100  -  total flux cleaned = -5.88019e-05 Jy
! Component: 150  -  total flux cleaned = -5.9971e-05 Jy
! Component: 200  -  total flux cleaned = 0.00022109 Jy
! Component: 250  -  total flux cleaned = 0.000401643 Jy
! Component: 300  -  total flux cleaned = 0.000490129 Jy
! Component: 350  -  total flux cleaned = 0.000489733 Jy
! Component: 400  -  total flux cleaned = 0.000573319 Jy
! Component: 450  -  total flux cleaned = 0.000573937 Jy
! Component: 500  -  total flux cleaned = 0.000413328 Jy
! Component: 550  -  total flux cleaned = 0.000255888 Jy
! Component: 600  -  total flux cleaned = 0.000177735 Jy
! Component: 650  -  total flux cleaned = -5.23489e-05 Jy
! Component: 700  -  total flux cleaned = -0.00027609 Jy
! Component: 750  -  total flux cleaned = -0.000276001 Jy
! Component: 800  -  total flux cleaned = -0.000711863 Jy
! Component: 850  -  total flux cleaned = -0.00071167 Jy
! Component: 900  -  total flux cleaned = -0.000853991 Jy
! Component: 950  -  total flux cleaned = -0.00092487 Jy
! Component: 1000  -  total flux cleaned = -0.000924446 Jy
! Component: 1050  -  total flux cleaned = -0.000992477 Jy
! Component: 1100  -  total flux cleaned = -0.000923875 Jy
! Component: 1150  -  total flux cleaned = -0.000923476 Jy
! Component: 1200  -  total flux cleaned = -0.00092313 Jy
! Component: 1250  -  total flux cleaned = -0.00118608 Jy
! Component: 1300  -  total flux cleaned = -0.00112113 Jy
! Component: 1350  -  total flux cleaned = -0.00138025 Jy
! Component: 1400  -  total flux cleaned = -0.00157181 Jy
! Component: 1450  -  total flux cleaned = -0.00176215 Jy
! Component: 1500  -  total flux cleaned = -0.00195017 Jy
! Component: 1550  -  total flux cleaned = -0.00226138 Jy
! Component: 1600  -  total flux cleaned = -0.00244659 Jy
! Component: 1650  -  total flux cleaned = -0.00269207 Jy
! Component: 1700  -  total flux cleaned = -0.00293563 Jy
! Component: 1750  -  total flux cleaned = -0.00305678 Jy
! Component: 1800  -  total flux cleaned = -0.0032969 Jy
! Component: 1850  -  total flux cleaned = -0.00353494 Jy
! Component: 1900  -  total flux cleaned = -0.00383033 Jy
! Component: 1950  -  total flux cleaned = -0.0038296 Jy
! Component: 2000  -  total flux cleaned = -0.00371332 Jy
! Component: 2050  -  total flux cleaned = -0.00423541 Jy
! Component: 2100  -  total flux cleaned = -0.00423501 Jy
! Component: 2150  -  total flux cleaned = -0.00429249 Jy
! Component: 2200  -  total flux cleaned = -0.00440573 Jy
! Component: 2250  -  total flux cleaned = -0.00440623 Jy
! Component: 2300  -  total flux cleaned = -0.00463039 Jy
! Component: 2350  -  total flux cleaned = -0.00485375 Jy
! Component: 2400  -  total flux cleaned = -0.00474255 Jy
! Component: 2450  -  total flux cleaned = -0.00496332 Jy
! Component: 2500  -  total flux cleaned = -0.00501804 Jy
! Component: 2550  -  total flux cleaned = -0.00490882 Jy
! Component: 2600  -  total flux cleaned = -0.00501756 Jy
! Component: 2650  -  total flux cleaned = -0.00517941 Jy
! Component: 2700  -  total flux cleaned = -0.00507194 Jy
! Component: 2750  -  total flux cleaned = -0.00517879 Jy
! Component: 2800  -  total flux cleaned = -0.00533832 Jy
! Component: 2850  -  total flux cleaned = -0.00539076 Jy
! Component: 2900  -  total flux cleaned = -0.00554796 Jy
! Component: 2950  -  total flux cleaned = -0.00549557 Jy
! Component: 3000  -  total flux cleaned = -0.00565186 Jy
! Component: 3050  -  total flux cleaned = -0.00549613 Jy
! Component: 3100  -  total flux cleaned = -0.00575437 Jy
! Component: 3150  -  total flux cleaned = -0.0058574 Jy
! Component: 3200  -  total flux cleaned = -0.00560199 Jy
! Component: 3250  -  total flux cleaned = -0.00590769 Jy
! Component: 3300  -  total flux cleaned = -0.00600888 Jy
! Component: 3350  -  total flux cleaned = -0.00600875 Jy
! Component: 3400  -  total flux cleaned = -0.00610922 Jy
! Component: 3450  -  total flux cleaned = -0.00600905 Jy
! Component: 3500  -  total flux cleaned = -0.00615859 Jy
! Component: 3550  -  total flux cleaned = -0.00615896 Jy
! Component: 3600  -  total flux cleaned = -0.00606011 Jy
! Component: 3650  -  total flux cleaned = -0.00625698 Jy
! Component: 3700  -  total flux cleaned = -0.00645329 Jy
! Component: 3750  -  total flux cleaned = -0.00635547 Jy
! Component: 3800  -  total flux cleaned = -0.0064044 Jy
! Component: 3850  -  total flux cleaned = -0.00654994 Jy
! Component: 3900  -  total flux cleaned = -0.00650161 Jy
! Component: 3950  -  total flux cleaned = -0.00679021 Jy
! Component: 4000  -  total flux cleaned = -0.00688618 Jy
! Component: 4050  -  total flux cleaned = -0.00688634 Jy
! Total flux subtracted in 4096 components = -0.00707652 Jy
! Clean residual min=-0.002890 max=0.002867 Jy/beam
! Clean residual mean=0.000004 rms=0.000810 Jy/beam
! Combined flux in latest and established models = 0.737931 Jy
keep
! Adding 307 model components to the UV plane model.
! The established model now contains 416 components and 0.737931 Jy
![Exited script file: /home/lpetrov/bin/01_muppet]
wmap "/scr/pima/rdv72_uvs/J0449+1121_X\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6971 x 1.694 at -11.3 degrees (North through East)
! Clean map  min=-0.0047096  max=0.52197 Jy/beam
! Writing clean map to FITS file: /scr/pima/rdv72_uvs/J0449+1121_X_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.521967 
invert
! Inverting map 
! Your choice of large map pixels excluded 4.65% of the data.
!  The x-axis pixel size should ideally be below 0.1705 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000803725 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.46194 0.46194 0.92388 1.84776 3.69552 7.39104 14.7821 29.5642 59.1283
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0024 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.521 
quit
! Quitting program
! Log file /scr/pima/rdv72_uvs/J0449+1121_X_uvs.log closed on Sat Oct  5 08:44:59 2013