! Started logfile: 2200+420_K.log_2 on Mon May  9 09:57:40 2005
observe 2200+420_K.edt
! Reading UV FITS file: 2200+420_K.edt
! AN table 1: 31 integrations on 55 of 55 possible baselines.
! AN table 2: 33 integrations on 55 of 55 possible baselines.
! Apparent sampling: 0.602557 visibilities/baseline/integration-bin.
! Found source: 2200+420
! 
! There are 8 IFs, and a total of 8 channels:
! 
!  IF  Channel    Frequency  Freq offset  Number of   Overall IF
!       origin    at origin  per channel   channels    bandwidth
!  ------------------------------------------------------------- (Hz)
!  01        1  2.37245e+10        8e+06          1        8e+06
!  02        2  2.37375e+10        8e+06          1        8e+06
!  03        3  2.37765e+10        8e+06          1        8e+06
!  04        4  2.38545e+10        8e+06          1        8e+06
!  05        5  2.39975e+10        8e+06          1        8e+06
!  06        6  2.41015e+10        8e+06          1        8e+06
!  07        7  2.41665e+10        8e+06          1        8e+06
!  08        8  2.41925e+10        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 784 lines of history.
! 
! Reading 16968 visibilities.
![@gonzo5-0.02 2200+420_K]
print "***********************************"
! *********************************** 
print "*** Using gonzo instruction set ***"
! *** Using gonzo instruction set *** 
print "***********************************"
! *********************************** 
float field_size
field_size = 1024
float field_cell
field_cell = 0.02
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.03
float dynam
dynam = 5.0
float win_mult
win_mult = 1.4
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 0.0200x0.0200 milli-arcsec cellsize.
select
! Selecting polarization: RR,  channels: 1..8
! Reading IF 1 channels: 1..1
! Reading IF 2 channels: 2..2
! Reading IF 3 channels: 3..3
! Reading IF 4 channels: 4..4
! Reading IF 5 channels: 5..5
! Reading IF 6 channels: 6..6
! Reading IF 7 channels: 7..7
! Reading IF 8 channels: 8..8
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 85 telescope corrections were flagged in sub-array 1.
!  A total of 77 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 2.
!  A total of 85 telescope corrections were flagged in sub-array 1.
!  A total of 77 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 3.
!  A total of 85 telescope corrections were flagged in sub-array 1.
!  A total of 77 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 4.
!  A total of 85 telescope corrections were flagged in sub-array 1.
!  A total of 77 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 5.
!  A total of 85 telescope corrections were flagged in sub-array 1.
!  A total of 77 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 6.
!  A total of 85 telescope corrections were flagged in sub-array 1.
!  A total of 77 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 7.
!  A total of 85 telescope corrections were flagged in sub-array 1.
!  A total of 77 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 8.
!  A total of 85 telescope corrections were flagged in sub-array 1.
!  A total of 78 telescope corrections were flagged in sub-array 2.
! 
! Fit before self-cal, rms=2.459474Jy  sigma=14.132357
! Fit after  self-cal, rms=2.459431Jy  sigma=14.132629
! 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=0.2942 mas, bmaj=0.5513 mas, bpa=15.52 degrees
! Estimated noise=1.48016 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=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 2.59177 Jy
! Component: 100  -  total flux cleaned = 3.18442 Jy
! Total flux subtracted in 100 components = 3.18442 Jy
! Clean residual min=-0.081759 max=0.217372 Jy/beam
! Clean residual mean=0.001716 rms=0.027173 Jy/beam
! Combined flux in latest and established models = 3.18442 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 17 model components to the UV plane model.
! The established model now contains 17 components and 3.18442 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.567537Jy  sigma=3.257707
! Fit after  self-cal, rms=0.567477Jy  sigma=3.257344
! Inverting map 
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.233478 Jy
! Component: 100  -  total flux cleaned = 0.366583 Jy
! Total flux subtracted in 100 components = 0.366583 Jy
! Clean residual min=-0.071320 max=0.078373 Jy/beam
! Clean residual mean=0.000838 rms=0.018531 Jy/beam
! Combined flux in latest and established models = 3.55101 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 22 model components to the UV plane model.
! The established model now contains 38 components and 3.55101 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.438749Jy  sigma=2.510679
! Fit after  self-cal, rms=0.438597Jy  sigma=2.509754
! 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 * 1.4
clean_niter = clean_niter * 2
dynam = dynam - 0.5
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=0.333 mas, bmaj=0.6212 mas, bpa=16.28 degrees
! Estimated noise=0.960195 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=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.105418 Jy
! Component: 100  -  total flux cleaned = 0.163393 Jy
! Component: 150  -  total flux cleaned = 0.196076 Jy
! Component: 200  -  total flux cleaned = 0.208408 Jy
! Total flux subtracted in 200 components = 0.208408 Jy
! Clean residual min=-0.069033 max=0.074837 Jy/beam
! Clean residual mean=0.001436 rms=0.017838 Jy/beam
! Combined flux in latest and established models = 3.75942 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 16 model components to the UV plane model.
! The established model now contains 52 components and 3.75942 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.413636Jy  sigma=2.361351
! Fit after  self-cal, rms=0.413511Jy  sigma=2.360603
! Inverting map 
print "****************************************"
! **************************************** 
print "*** Finished Natural Weighting CLEAN ***"
! *** Finished Natural Weighting CLEAN *** 
print "****************************************"
! **************************************** 
gscale false
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Amplitude normalization factor in sub-array 1: 0.992721
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.93     FD        1.05     HN        1.12     KP        1.07     
!   LA        0.97     MK        1.03     NL        1.02     OV        0.92     
!   PT        0.95     SC        1.02     TI        1.00*    
! 
!  Amplitude normalization factor in sub-array 2: 0.96497
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.99     FD        1.06     HN        1.08     KP        1.06     
!   LA        0.97     MK        1.10     NL        1.01     OV        0.96     
!   PT        1.12     SC        1.06     TI        1.00*    
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 0.997989
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.94     FD        1.00     HN        1.07     KP        1.07     
!   LA        0.99     MK        1.01     NL        1.01     OV        0.93     
!   PT        0.99     SC        1.02     TI        1.00*    
! 
!  Amplitude normalization factor in sub-array 2: 0.97151
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        1.01     HN        1.04     KP        1.06     
!   LA        0.99     MK        1.05     NL        0.99     OV        0.98     
!   PT        1.16     SC        1.04     TI        1.00*    
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 1.0164
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.95     FD        0.91     HN        1.06     KP        1.03     
!   LA        1.01     MK        0.99     NL        0.99     OV        0.96     
!   PT        0.95     SC        0.98     TI        1.00*    
! 
!  Amplitude normalization factor in sub-array 2: 0.988199
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        0.92     HN        1.03     KP        1.02     
!   LA        1.00     MK        1.04     NL        0.98     OV        0.99     
!   PT        1.12     SC        1.02     TI        1.00*    
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 1.01986
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.91     FD        0.95     HN        1.15     KP        0.97     
!   LA        0.98     MK        0.98     NL        1.06     OV        0.90     
!   PT        0.90     SC        0.99     TI        1.00*    
! 
!  Amplitude normalization factor in sub-array 2: 0.99309
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.96     FD        0.95     HN        1.12     KP        0.96     
!   LA        0.97     MK        1.04     NL        1.06     OV        0.93     
!   PT        1.06     SC        1.02     TI        1.00*    
! 
! 
! Correcting IF 5.
!  Amplitude normalization factor in sub-array 1: 1.01162
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.80     FD        1.05     HN        1.03     KP        1.00     
!   LA        0.98     MK        1.06     NL        1.03     OV        0.94     
!   PT        0.97     SC        1.01     TI        1.00*    
! 
!  Amplitude normalization factor in sub-array 2: 0.98393
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.84     FD        1.06     HN        1.00     KP        0.99     
!   LA        0.99     MK        1.12     NL        1.02     OV        0.98     
!   PT        1.14     SC        1.03     TI        1.00*    
! 
! 
! Correcting IF 6.
!  Amplitude normalization factor in sub-array 1: 1.00381
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.96     FD        0.99     HN        1.10     KP        1.01     
!   LA        1.00     MK        1.04     NL        1.08     OV        0.83     
!   PT        0.97     SC        0.98     TI        1.00*    
! 
!  Amplitude normalization factor in sub-array 2: 0.975351
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.02     FD        1.00     HN        1.07     KP        1.00     
!   LA        1.00     MK        1.12     NL        1.07     OV        0.86     
!   PT        1.12     SC        1.02     TI        1.00*    
! 
! 
! Correcting IF 7.
!  Amplitude normalization factor in sub-array 1: 1.02603
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.02     FD        0.90     HN        0.99     KP        1.03     
!   LA        1.02     MK        1.03     NL        1.08     OV        0.81     
!   PT        0.87     SC        0.97     TI        1.00*    
! 
!  Amplitude normalization factor in sub-array 2: 0.999063
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.08     FD        0.91     HN        0.97     KP        1.02     
!   LA        1.02     MK        1.09     NL        1.07     OV        0.83     
!   PT        1.02     SC        1.00     TI        1.00*    
! 
! 
! Correcting IF 8.
!  Amplitude normalization factor in sub-array 1: 1.01706
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     FD        0.92     HN        1.06     KP        1.04     
!   LA        1.01     MK        1.03     NL        1.10     OV        0.83     
!   PT        0.84     SC        1.00     TI        1.00*    
! 
!  Amplitude normalization factor in sub-array 2: 0.989257
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.06     FD        0.93     HN        1.04     KP        1.02     
!   LA        1.00     MK        1.10     NL        1.09     OV        0.85     
!   PT        0.97     SC        1.05     TI        1.00*    
! 
! 
! Fit before self-cal, rms=0.413511Jy  sigma=2.360603
! Fit after  self-cal, rms=0.275687Jy  sigma=1.566103
dynam = dynam - 0.5
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=0.3358 mas, bmaj=0.6269 mas, bpa=16.81 degrees
! Estimated noise=0.95714 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 (-0.44, -2.36).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0508279 Jy
! Component: 100  -  total flux cleaned = 0.0626597 Jy
! Component: 150  -  total flux cleaned = 0.0725097 Jy
! Component: 200  -  total flux cleaned = 0.0781484 Jy
! Total flux subtracted in 200 components = 0.0781484 Jy
! Clean residual min=-0.033712 max=0.043901 Jy/beam
! Clean residual mean=0.000416 rms=0.009369 Jy/beam
! Combined flux in latest and established models = 3.83756 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 42 model components to the UV plane model.
! The established model now contains 94 components and 3.83756 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.257561Jy  sigma=1.458645
! Fit after  self-cal, rms=0.256511Jy  sigma=1.452963
! Inverting map 
! Added new window around map position (-0.38, -1.26).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0364868 Jy
! Component: 100  -  total flux cleaned = 0.0381956 Jy
! Component: 150  -  total flux cleaned = 0.0396643 Jy
! Component: 200  -  total flux cleaned = 0.0409213 Jy
! Total flux subtracted in 200 components = 0.0409213 Jy
! Clean residual min=-0.030427 max=0.027665 Jy/beam
! Clean residual mean=0.000330 rms=0.008368 Jy/beam
! Combined flux in latest and established models = 3.87849 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 37 model components to the UV plane model.
! The established model now contains 124 components and 3.87849 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.249544Jy  sigma=1.411414
! Fit after  self-cal, rms=0.248923Jy  sigma=1.408041
! 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=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00861485 Jy
! Component: 100  -  total flux cleaned = 0.0103072 Jy
! Component: 150  -  total flux cleaned = 0.0103267 Jy
! Component: 200  -  total flux cleaned = 0.0107737 Jy
! Total flux subtracted in 200 components = 0.0107737 Jy
! Clean residual min=-0.029054 max=0.027549 Jy/beam
! Clean residual mean=0.000334 rms=0.008016 Jy/beam
! Combined flux in latest and established models = 3.88926 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 36 model components to the UV plane model.
! The established model now contains 143 components and 3.88926 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.246921Jy  sigma=1.395874
! Fit after  self-cal, rms=0.207802Jy  sigma=1.162330
! Inverting map and beam 
! Estimated beam: bmin=0.3355 mas, bmaj=0.6259 mas, bpa=16.73 degrees
! Estimated noise=0.956746 mJy/beam.
! Added new window around map position (-1.06, -3.58).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0281067 Jy
! Component: 100  -  total flux cleaned = 0.0452973 Jy
! Component: 150  -  total flux cleaned = 0.0570305 Jy
! Component: 200  -  total flux cleaned = 0.0647842 Jy
! Total flux subtracted in 200 components = 0.0647842 Jy
! Clean residual min=-0.013121 max=0.012441 Jy/beam
! Clean residual mean=0.000014 rms=0.003393 Jy/beam
! Combined flux in latest and established models = 3.95404 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 28 model components to the UV plane model.
! The established model now contains 171 components and 3.95404 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.203370Jy  sigma=1.134544
! Fit after  self-cal, rms=0.202335Jy  sigma=1.129218
! Inverting map and beam 
! Estimated beam: bmin=0.3356 mas, bmaj=0.6258 mas, bpa=16.73 degrees
! Estimated noise=0.956074 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=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00823379 Jy
! Component: 100  -  total flux cleaned = 0.0148074 Jy
! Component: 150  -  total flux cleaned = 0.0192214 Jy
! Component: 200  -  total flux cleaned = 0.021483 Jy
! Total flux subtracted in 200 components = 0.021483 Jy
! Clean residual min=-0.011737 max=0.010605 Jy/beam
! Clean residual mean=-0.000041 rms=0.002895 Jy/beam
! Combined flux in latest and established models = 3.97553 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 39 model components to the UV plane model.
! The established model now contains 205 components and 3.97553 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Correcting IF 5.
! 
! Correcting IF 6.
! 
! Correcting IF 7.
! 
! Correcting IF 8.
! 
! Fit before self-cal, rms=0.201305Jy  sigma=1.122757
! Fit after  self-cal, rms=0.201273Jy  sigma=1.122560
! Inverting map 
print "***********************************"
! *********************************** 
print "*** Finished Amplitude Self-Cal ***"
! *** Finished Amplitude Self-Cal *** 
print "***********************************"
! *********************************** 
save 2200+420_K
! Writing UV FITS file: 2200+420_K.uvf
! Writing 205 model components to file: 2200+420_K.mod
! wwins: Wrote 4 windows to 2200+420_K.win
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.3356 x 0.6258 at 16.73 degrees (North through East)
! Clean map  min=-0.010361  max=3.3707 Jy/beam
! Writing clean map to FITS file: 2200+420_K.fits
! Writing difmap environment to: 2200+420_K.par
print "****************************"
! **************************** 
print "*** Now, make some plots ***"
! *** Now, make some plots *** 
print "****************************"
! **************************** 
![@gonzo_plot 2200+420_K]
device 2200+420_Kuv.ps/vps,1,2
! Attempting to open device: '2200+420_Kuv.ps/vps'
radplot
! Using default options string "m1"
uvplot
! Using default options string ""
device 2200+420_Kim.ps/vps
! Attempting to open device: '2200+420_Kim.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=0.3356 mas, bmaj=0.6258 mas, bpa=16.73 degrees
! Estimated noise=0.956074 mJy/beam.
mappl cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.3356 x 0.6258 at 16.73 degrees (North through East)
! Clean map  min=-0.010361  max=3.3707 Jy/beam
![Exited script file: gonzo_plot]
![Exited script file: gonzo5-0.02]
quit
! Quitting program
! Log file 2200+420_K.log_2 closed on Mon May  9 09:59:09 2005