! Started logfile: 1144-379_S.log on Thu Aug 21 11:31:03 2008
observe 1144-379_S.edt
! Reading UV FITS file: 1144-379_S.edt
! AN table 1: 9 integrations on 171 of 171 possible baselines.
! AN table 2: 4 integrations on 171 of 171 possible baselines.
! AN table 3: 9 integrations on 171 of 171 possible baselines.
! AN table 4: 34 integrations on 171 of 171 possible baselines.
! Apparent sampling: 0.0474102 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: 1144-379
! 
! 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  2.22497e+09        8e+06          1        8e+06
!  02        2  2.24497e+09        8e+06          1        8e+06
!  03        3  2.33497e+09        8e+06          1        8e+06
!  04        4  2.36497e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 1615 lines of history.
! 
! Reading 1816 visibilities.
![@gonzo7-0.4 1144-379_S]
print "***********************************"
! *********************************** 
print "*** Using gonzo instruction set ***"
! *** Using gonzo instruction set *** 
print "***********************************"
! *********************************** 
float field_size
field_size = 1024
float field_cell
field_cell = 0.4
integer clean_niter
clean_niter = 50
float clean_gain
clean_gain = 0.03
float dynam
dynam = 7.0
float win_mult
win_mult = 1.8
float solint
solint = 3.6/6.0
logical doflt
doflt = true
logical doamp
float new_peak
float flux_cutoff
mapsize field_size,field_cell
! Map grid = 1024x1024 pixels with 0.400x0.400 milli-arcsec cellsize.
select
! 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
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 132 telescope corrections were flagged in sub-array 1.
!  A total of 76 telescope corrections were flagged in sub-array 2.
!  A total of 171 telescope corrections were flagged in sub-array 3.
!  A total of 534 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 2.
!  A total of 132 telescope corrections were flagged in sub-array 1.
!  A total of 76 telescope corrections were flagged in sub-array 2.
!  A total of 171 telescope corrections were flagged in sub-array 3.
!  A total of 534 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 3.
!  A total of 132 telescope corrections were flagged in sub-array 1.
!  A total of 76 telescope corrections were flagged in sub-array 2.
!  A total of 171 telescope corrections were flagged in sub-array 3.
!  A total of 534 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 4.
!  A total of 132 telescope corrections were flagged in sub-array 1.
!  A total of 76 telescope corrections were flagged in sub-array 2.
!  A total of 171 telescope corrections were flagged in sub-array 3.
!  A total of 534 telescope corrections were flagged in sub-array 4.
! 
! Fit before self-cal, rms=0.258551Jy  sigma=2.903708
! Fit after  self-cal, rms=0.258832Jy  sigma=2.906519
! clrmod: Cleared the established, tentative and continuum models.
! Redundant starting model cleared.
uvweight 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.
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=2.844 mas, bmaj=20.95 mas, bpa=-4.82 degrees
! Estimated noise=3.30923 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal doamp, doflt, solint
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (0, 0).
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.634245 Jy
! Total flux subtracted in 50 components = 0.634245 Jy
! Clean residual min=-0.053847 max=0.176948 Jy/beam
! Clean residual mean=0.000610 rms=0.023201 Jy/beam
! Combined flux in latest and established models = 0.634245 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 2 model components to the UV plane model.
! The established model now contains 2 components and 0.634245 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.344108Jy  sigma=3.640863
! Fit after  self-cal, rms=0.344114Jy  sigma=3.640622
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.144817 Jy
! Total flux subtracted in 50 components = 0.144817 Jy
! Clean residual min=-0.039807 max=0.078470 Jy/beam
! Clean residual mean=0.000475 rms=0.015237 Jy/beam
! Combined flux in latest and established models = 0.779062 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 19 model components to the UV plane model.
! The established model now contains 19 components and 0.779062 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.257970Jy  sigma=2.562958
! Fit after  self-cal, rms=0.257980Jy  sigma=2.562129
! Inverting map 
print "****************************************"
! **************************************** 
print "*** Finished Uniform Weighting CLEAN ***"
! *** Finished Uniform Weighting CLEAN *** 
print "****************************************"
! **************************************** 
uvweight 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
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=3.099 mas, bmaj=34.23 mas, bpa=-5.475 degrees
! Estimated noise=1.69079 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal doamp, doflt, solint
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.102416 Jy
! Component: 100  -  total flux cleaned = 0.155347 Jy
! Total flux subtracted in 100 components = 0.155347 Jy
! Clean residual min=-0.036500 max=0.037036 Jy/beam
! Clean residual mean=0.001312 rms=0.013026 Jy/beam
! Combined flux in latest and established models = 0.934408 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 43 model components to the UV plane model.
! The established model now contains 60 components and 0.934408 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.212012Jy  sigma=2.078854
! Fit after  self-cal, rms=0.212003Jy  sigma=2.078549
! Inverting map 
print "****************************************"
! **************************************** 
print "*** Finished Natural Weighting CLEAN ***"
! *** Finished Natural Weighting CLEAN *** 
print "****************************************"
! **************************************** 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.12     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.00*    KP        0.91     LA        1.11     
!   MA        1.00*    MK        1.00*    NL        1.06     NY        1.00*    
!   OV        1.00*    PT        1.04     SC        0.82     TS        1.00*    
!   WF        1.12     WZ        1.00*    GG        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    FD        0.00*    GC        0.00*    HH        0.00*    
!   HN        0.00*    KK        0.00*    KP        0.00*    LA        0.00*    
!   MA        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TS        0.00*    
!   WF        0.00*    WZ        0.00*    GG        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.00*    FD        0.00*    GC        0.00*    HH        0.00*    
!   HN        0.00*    KK        0.00*    KP        0.00*    LA        0.00*    
!   MA        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TS        0.00*    
!   WF        0.00*    WZ        0.00*    GG        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        1.14     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        0.83     KP        0.93     LA        1.13     
!   MA        1.00*    MK        0.98     NL        1.00*    NY        1.00*    
!   OV        0.99     PT        1.07     SC        1.00*    TS        1.00*    
!   WF        1.00*    WZ        1.00*    GG        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.06     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.00*    KP        1.03     LA        1.06     
!   MA        1.00*    MK        1.00*    NL        1.21     NY        1.00*    
!   OV        1.00*    PT        0.94     SC        1.04     TS        1.00*    
!   WF        1.07     WZ        1.00*    GG        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    FD        0.00*    GC        0.00*    HH        0.00*    
!   HN        0.00*    KK        0.00*    KP        0.00*    LA        0.00*    
!   MA        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TS        0.00*    
!   WF        0.00*    WZ        0.00*    GG        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.00*    FD        0.00*    GC        0.00*    HH        0.00*    
!   HN        0.00*    KK        0.00*    KP        0.00*    LA        0.00*    
!   MA        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TS        0.00*    
!   WF        0.00*    WZ        0.00*    GG        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        1.03     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        0.83     KP        1.05     LA        1.15     
!   MA        1.00*    MK        1.07     NL        1.00*    NY        1.00*    
!   OV        0.94     PT        0.88     SC        1.00*    TS        1.00*    
!   WF        1.00*    WZ        1.00*    GG        1.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.01     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.00*    KP        1.09     LA        0.90     
!   MA        1.00*    MK        1.00*    NL        1.00     NY        1.00*    
!   OV        1.00*    PT        1.02     SC        1.16     TS        1.00*    
!   WF        1.09     WZ        1.00*    GG        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    FD        0.00*    GC        0.00*    HH        0.00*    
!   HN        0.00*    KK        0.00*    KP        0.00*    LA        0.00*    
!   MA        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TS        0.00*    
!   WF        0.00*    WZ        0.00*    GG        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.00*    FD        0.00*    GC        0.00*    HH        0.00*    
!   HN        0.00*    KK        0.00*    KP        0.00*    LA        0.00*    
!   MA        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TS        0.00*    
!   WF        0.00*    WZ        0.00*    GG        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        1.02     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        0.81     KP        1.13     LA        0.96     
!   MA        1.00*    MK        1.07     NL        1.00*    NY        1.00*    
!   OV        1.02     PT        0.95     SC        1.00*    TS        1.00*    
!   WF        1.00*    WZ        1.00*    GG        1.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.87     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.00*    KP        1.08     LA        0.75     
!   MA        1.00*    MK        1.00*    NL        1.09     NY        1.00*    
!   OV        1.00*    PT        0.97     SC        1.17     TS        1.00*    
!   WF        1.21     WZ        1.00*    GG        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    FD        0.00*    GC        0.00*    HH        0.00*    
!   HN        0.00*    KK        0.00*    KP        0.00*    LA        0.00*    
!   MA        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TS        0.00*    
!   WF        0.00*    WZ        0.00*    GG        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.00*    FD        0.00*    GC        0.00*    HH        0.00*    
!   HN        0.00*    KK        0.00*    KP        0.00*    LA        0.00*    
!   MA        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TS        0.00*    
!   WF        0.00*    WZ        0.00*    GG        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        0.89     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        0.76     KP        1.10     LA        0.78     
!   MA        1.00*    MK        1.03     NL        1.00*    NY        1.00*    
!   OV        0.93     PT        0.90     SC        1.00*    TS        1.00*    
!   WF        1.00*    WZ        1.00*    GG        1.00*    
! 
! 
! Fit before self-cal, rms=0.212003Jy  sigma=2.078549
! Fit after  self-cal, rms=0.132445Jy  sigma=1.275049
dynam = dynam - 0.5
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=3.034 mas, bmaj=35.31 mas, bpa=-5.408 degrees
! Estimated noise=1.64899 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal doamp, doflt, solint
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0291051 Jy
! Component: 100  -  total flux cleaned = 0.0350095 Jy
! Total flux subtracted in 100 components = 0.0350095 Jy
! Clean residual min=-0.012856 max=0.015934 Jy/beam
! Clean residual mean=0.000728 rms=0.005036 Jy/beam
! Combined flux in latest and established models = 0.969418 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 24 model components to the UV plane model.
! The established model now contains 84 components and 0.969418 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.126562Jy  sigma=1.200156
! Fit after  self-cal, rms=0.126554Jy  sigma=1.198414
! Inverting map 
dynam = dynam - 1.0
doamp = true
solint = solint * (6.0/3.6)
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 doamp, doflt, solint
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00154383 Jy
! Component: 100  -  total flux cleaned = 0.00139179 Jy
! Total flux subtracted in 100 components = 0.00139179 Jy
! Clean residual min=-0.012584 max=0.015720 Jy/beam
! Clean residual mean=0.000714 rms=0.004910 Jy/beam
! Combined flux in latest and established models = 0.970809 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 19 model components to the UV plane model.
! The established model now contains 101 components and 0.970809 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.126216Jy  sigma=1.195949
! Fit after  self-cal, rms=0.120824Jy  sigma=1.119160
! Inverting map and beam 
! Estimated beam: bmin=3 mas, bmaj=35.31 mas, bpa=-5.413 degrees
! Estimated noise=1.64261 mJy/beam.
doamp = false
solint = solint / (6.0/3.6)
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 doamp, doflt, solint
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0143676 Jy
! Component: 100  -  total flux cleaned = 0.014654 Jy
! Total flux subtracted in 100 components = 0.014654 Jy
! Clean residual min=-0.008345 max=0.011418 Jy/beam
! Clean residual mean=0.000512 rms=0.002846 Jy/beam
! Combined flux in latest and established models = 0.985463 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 24 model components to the UV plane model.
! The established model now contains 109 components and 0.985463 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.119235Jy  sigma=1.097775
! Fit after  self-cal, rms=0.119275Jy  sigma=1.097590
! Inverting map 
print "***********************************"
! *********************************** 
print "*** Finished Amplitude Self-Cal ***"
! *** Finished Amplitude Self-Cal *** 
print "***********************************"
! *********************************** 
save 1144-379_S
! Writing UV FITS file: 1144-379_S.uvf
! Writing 109 model components to file: 1144-379_S.mod
! wwins: Wrote 1 windows to 1144-379_S.win
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 3 x 35.31 at -5.413 degrees (North through East)
! Clean map  min=-0.0084057  max=0.81866 Jy/beam
! Writing clean map to FITS file: 1144-379_S.fits
! Writing difmap environment to: 1144-379_S.par
print "****************************"
! **************************** 
print "*** Now, make some plots ***"
! *** Now, make some plots *** 
print "****************************"
! **************************** 
![@gonzo_plot 1144-379_S]
device 1144-379_Suv.ps/vps,1,2
! Attempting to open device: '1144-379_Suv.ps/vps'
radplot
! Using default options string "m1"
uvplot
! Using default options string ""
device 1144-379_Sim.ps/vps
! Attempting to open device: '1144-379_Sim.ps/vps'
uvweight 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.
loglevs -1,2048,2
! The new contour levels are:
!  -1 1 2 4 8 16 32 64 128 256 512 1024 2048
cmul = imstat(rms)*3
! Inverting map and beam 
! Estimated beam: bmin=3 mas, bmaj=35.31 mas, bpa=-5.413 degrees
! Estimated noise=1.64261 mJy/beam.
mappl cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 3 x 35.31 at -5.413 degrees (North through East)
! Clean map  min=-0.0084057  max=0.81866 Jy/beam
![Exited script file: gonzo_plot]
![Exited script file: gonzo7-0.4]
quit
! Quitting program
! Log file 1144-379_S.log closed on Thu Aug 21 11:31:16 2008