! Started logfile: 1435+638_X.log on Fri Jul 22 15:57:39 2005
observe 1435+638_X.edt
! Reading UV FITS file: 1435+638_X.edt
! AN table 1: 45 integrations on 171 of 171 possible baselines.
! AN table 2: 64 integrations on 171 of 171 possible baselines.
! AN table 3: 49 integrations on 171 of 171 possible baselines.
! Apparent sampling: 0.173847 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: 1435+638
! 
! There are 4 IFs, and a total of 4 channels:
! 
!  IF  Channel    Frequency  Freq offset  Number of   Overall IF
!       origin    at origin  per channel   channels    bandwidth
!  ------------------------------------------------------------- (Hz)
!  01        1  8.40997e+09        8e+06          1        8e+06
!  02        2  8.47997e+09        8e+06          1        8e+06
!  03        3  8.79497e+09        8e+06          1        8e+06
!  04        4  8.89997e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 1818 lines of history.
! 
! Reading 18788 visibilities.
![@gonzo7-0.4 1435+638_X]
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 520 telescope corrections were flagged in sub-array 1.
!  A total of 861 telescope corrections were flagged in sub-array 2.
!  A total of 678 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 516 telescope corrections were flagged in sub-array 1.
!  A total of 863 telescope corrections were flagged in sub-array 2.
!  A total of 678 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 511 telescope corrections were flagged in sub-array 1.
!  A total of 860 telescope corrections were flagged in sub-array 2.
!  A total of 678 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 515 telescope corrections were flagged in sub-array 1.
!  A total of 862 telescope corrections were flagged in sub-array 2.
!  A total of 678 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=0.663544Jy  sigma=0.010871
! Fit after  self-cal, rms=0.657333Jy  sigma=0.010763
! 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 
! Your choice of large map pixels excluded 21.7% of the data.
!  The x-axis pixel size should ideally be below 0.2001 milli-arcsec
!  The y-axis pixel size should ideally be below 0.3536 milli-arcsec
! Estimated beam: bmin=0.9964 mas, bmaj=1.482 mas, bpa=-12.96 degrees
! Estimated noise=725.204 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 = 0.297695 Jy
! Total flux subtracted in 50 components = 0.297695 Jy
! Clean residual min=-0.045916 max=0.121772 Jy/beam
! Clean residual mean=0.000002 rms=0.008327 Jy/beam
! Combined flux in latest and established models = 0.297695 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 4 model components to the UV plane model.
! The established model now contains 4 components and 0.297695 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.288895Jy  sigma=0.005340
! Fit after  self-cal, rms=0.288391Jy  sigma=0.005335
! Inverting map 
! Your choice of large map pixels excluded 21.7% of the data.
!  The x-axis pixel size should ideally be below 0.2001 milli-arcsec
!  The y-axis pixel size should ideally be below 0.3536 milli-arcsec
! Added new window around map position (1.2, 0.4).
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.147511 Jy
! Total flux subtracted in 50 components = 0.147511 Jy
! Clean residual min=-0.035034 max=0.092341 Jy/beam
! Clean residual mean=0.000002 rms=0.005899 Jy/beam
! Combined flux in latest and established models = 0.445206 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 7 model components to the UV plane model.
! The established model now contains 7 components and 0.445206 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.217147Jy  sigma=0.003874
! Fit after  self-cal, rms=0.215761Jy  sigma=0.003850
! Inverting map 
! Your choice of large map pixels excluded 21.7% of the data.
!  The x-axis pixel size should ideally be below 0.2001 milli-arcsec
!  The y-axis pixel size should ideally be below 0.3536 milli-arcsec
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0967177 Jy
! Total flux subtracted in 50 components = 0.0967177 Jy
! Clean residual min=-0.026890 max=0.064867 Jy/beam
! Clean residual mean=0.000002 rms=0.004389 Jy/beam
! Combined flux in latest and established models = 0.541924 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 6 model components to the UV plane model.
! The established model now contains 8 components and 0.541924 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.181571Jy  sigma=0.003061
! Fit after  self-cal, rms=0.180608Jy  sigma=0.003037
! Inverting map 
! Your choice of large map pixels excluded 21.7% of the data.
!  The x-axis pixel size should ideally be below 0.2001 milli-arcsec
!  The y-axis pixel size should ideally be below 0.3536 milli-arcsec
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0652933 Jy
! Total flux subtracted in 50 components = 0.0652933 Jy
! Clean residual min=-0.021157 max=0.046238 Jy/beam
! Clean residual mean=0.000002 rms=0.003483 Jy/beam
! Combined flux in latest and established models = 0.607217 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 7 model components to the UV plane model.
! The established model now contains 9 components and 0.607217 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.161312Jy  sigma=0.002580
! Fit after  self-cal, rms=0.160468Jy  sigma=0.002561
! Inverting map 
! Your choice of large map pixels excluded 21.7% of the data.
!  The x-axis pixel size should ideally be below 0.2001 milli-arcsec
!  The y-axis pixel size should ideally be below 0.3536 milli-arcsec
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0447971 Jy
! Total flux subtracted in 50 components = 0.0447971 Jy
! Clean residual min=-0.017247 max=0.034760 Jy/beam
! Clean residual mean=0.000002 rms=0.002934 Jy/beam
! Combined flux in latest and established models = 0.652014 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 7 model components to the UV plane model.
! The established model now contains 10 components and 0.652014 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.149599Jy  sigma=0.002297
! Fit after  self-cal, rms=0.148985Jy  sigma=0.002282
! Inverting map 
! Your choice of large map pixels excluded 21.7% of the data.
!  The x-axis pixel size should ideally be below 0.2001 milli-arcsec
!  The y-axis pixel size should ideally be below 0.3536 milli-arcsec
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0309919 Jy
! Total flux subtracted in 50 components = 0.0309919 Jy
! Clean residual min=-0.015230 max=0.027995 Jy/beam
! Clean residual mean=0.000002 rms=0.002618 Jy/beam
! Combined flux in latest and established models = 0.683006 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 9 model components to the UV plane model.
! The established model now contains 12 components and 0.683006 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.143474Jy  sigma=0.002140
! Fit after  self-cal, rms=0.143153Jy  sigma=0.002133
! Inverting map 
! Your choice of large map pixels excluded 21.7% of the data.
!  The x-axis pixel size should ideally be below 0.2001 milli-arcsec
!  The y-axis pixel size should ideally be below 0.3536 milli-arcsec
! Added new window around map position (-4.8, -7.2).
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0272814 Jy
! Total flux subtracted in 50 components = 0.0272814 Jy
! Clean residual min=-0.015499 max=0.023191 Jy/beam
! Clean residual mean=0.000002 rms=0.002353 Jy/beam
! Combined flux in latest and established models = 0.710287 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 8 model components to the UV plane model.
! The established model now contains 16 components and 0.710287 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.140388Jy  sigma=0.002032
! Fit after  self-cal, rms=0.140206Jy  sigma=0.002026
! Inverting map 
! Your choice of large map pixels excluded 21.7% of the data.
!  The x-axis pixel size should ideally be below 0.2001 milli-arcsec
!  The y-axis pixel size should ideally be below 0.3536 milli-arcsec
! Added new window around map position (-1.6, -1.2).
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0227928 Jy
! Total flux subtracted in 50 components = 0.0227928 Jy
! Clean residual min=-0.014715 max=0.017171 Jy/beam
! Clean residual mean=0.000002 rms=0.002139 Jy/beam
! Combined flux in latest and established models = 0.73308 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 9 model components to the UV plane model.
! The established model now contains 20 components and 0.73308 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.137870Jy  sigma=0.001957
! Fit after  self-cal, rms=0.137839Jy  sigma=0.001956
! Inverting map 
! Your choice of large map pixels excluded 21.7% of the data.
!  The x-axis pixel size should ideally be below 0.2001 milli-arcsec
!  The y-axis pixel size should ideally be below 0.3536 milli-arcsec
! Added new window around map position (3.6, 2).
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0182511 Jy
! Total flux subtracted in 50 components = 0.0182511 Jy
! Clean residual min=-0.013888 max=0.010841 Jy/beam
! Clean residual mean=0.000002 rms=0.002009 Jy/beam
! Combined flux in latest and established models = 0.751331 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 12 model components to the UV plane model.
! The established model now contains 24 components and 0.751331 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.136685Jy  sigma=0.001919
! Fit after  self-cal, rms=0.136640Jy  sigma=0.001918
! Inverting map 
! Your choice of large map pixels excluded 21.7% of the data.
!  The x-axis pixel size should ideally be below 0.2001 milli-arcsec
!  The y-axis pixel size should ideally be below 0.3536 milli-arcsec
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 
! Your choice of large map pixels excluded 21.7% of the data.
!  The x-axis pixel size should ideally be below 0.2001 milli-arcsec
!  The y-axis pixel size should ideally be below 0.3536 milli-arcsec
! Estimated beam: bmin=1.293 mas, bmaj=1.901 mas, bpa=-19.82 degrees
! Estimated noise=410.368 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 = 0.018663 Jy
! Component: 100  -  total flux cleaned = 0.0242734 Jy
! Total flux subtracted in 100 components = 0.0242734 Jy
! Clean residual min=-0.010487 max=0.011701 Jy/beam
! Clean residual mean=0.000006 rms=0.002372 Jy/beam
! Combined flux in latest and established models = 0.775605 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 32 components and 0.775605 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.135612Jy  sigma=0.001864
! Fit after  self-cal, rms=0.135519Jy  sigma=0.001860
! Inverting map 
! Your choice of large map pixels excluded 21.7% of the data.
!  The x-axis pixel size should ideally be below 0.2001 milli-arcsec
!  The y-axis pixel size should ideally be below 0.3536 milli-arcsec
print "****************************************"
! **************************************** 
print "*** Finished Natural Weighting CLEAN ***"
! *** Finished Natural Weighting CLEAN *** 
print "****************************************"
! **************************************** 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 6 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.03     FD        1.00*    GC        1.05     HH        1.00*    
!   HN        1.00*    KK        1.00*    KP        0.98     LA        1.13     
!   MC        1.54     MK        1.00*    NL        0.96     NY        2.03     
!   ON        0.84     OV        1.02     PT        0.98     SC        1.00*    
!   TS        1.00*    WF        1.00*    WZ        1.43     
! 
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        0.94     GC        1.00*    HH        1.00*    
!   HN        1.00     KK        1.00*    KP        1.01     LA        1.02     
!   MC        1.00*    MK        1.95     NL        0.98     NY        1.00*    
!   ON        1.00*    OV        0.94     PT        0.95     SC        0.98     
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.97     FD        0.97     GC        1.00*    HH        1.00*    
!   HN        1.15     KK        1.00*    KP        1.04     LA        0.99     
!   MC        1.00*    MK        1.00     NL        0.96     NY        1.00*    
!   ON        1.00*    OV        0.99     PT        0.99     SC        0.97     
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 2.
!  A total of 6 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.02     FD        1.00*    GC        0.96     HH        1.00*    
!   HN        1.00*    KK        1.00*    KP        0.97     LA        1.11     
!   MC        1.51     MK        1.00*    NL        0.95     NY        2.17     
!   ON        0.92     OV        1.03     PT        0.99     SC        1.00*    
!   TS        1.00*    WF        1.00*    WZ        1.38     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        0.94     GC        1.00*    HH        1.00*    
!   HN        0.98     KK        1.00*    KP        1.01     LA        1.03     
!   MC        1.00*    MK        1.61     NL        0.95     NY        1.00*    
!   ON        1.00*    OV        0.93     PT        0.95     SC        0.99     
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.98     FD        0.96     GC        1.00*    HH        1.00*    
!   HN        1.10     KK        1.00*    KP        1.01     LA        1.00     
!   MC        1.00*    MK        1.00     NL        0.96     NY        1.00*    
!   ON        1.00*    OV        1.00     PT        1.00     SC        1.00     
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 3.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.05     FD        1.00*    GC        1.02     HH        1.00*    
!   HN        1.00*    KK        1.00*    KP        0.99     LA        1.13     
!   MC        1.35     MK        1.00*    NL        0.96     NY        2.12     
!   ON        0.85     OV        1.00     PT        0.98     SC        1.00*    
!   TS        1.00*    WF        1.00*    WZ        1.34     
! 
!  A total of 3 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.02     FD        0.95     GC        1.00*    HH        1.00*    
!   HN        0.96     KK        1.00*    KP        0.98     LA        1.00     
!   MC        1.00*    MK        1.37     NL        0.94     NY        1.00*    
!   ON        1.00*    OV        0.95     PT        0.96     SC        0.97     
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.97     FD        0.95     GC        1.00*    HH        1.00*    
!   HN        1.01     KK        1.00*    KP        1.00     LA        1.01     
!   MC        1.00*    MK        1.08     NL        0.95     NY        1.00*    
!   ON        1.00*    OV        1.01     PT        1.03     SC        1.07     
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.03     FD        1.00*    GC        1.07     HH        1.00*    
!   HN        1.00*    KK        1.00*    KP        0.97     LA        1.13     
!   MC        1.33     MK        1.00*    NL        0.98     NY        1.91     
!   ON        0.83     OV        1.01     PT        0.98     SC        1.00*    
!   TS        1.00*    WF        1.00*    WZ        1.32     
! 
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.02     FD        0.96     GC        1.00*    HH        1.00*    
!   HN        0.98     KK        1.00*    KP        1.00     LA        1.02     
!   MC        1.00*    MK        1.50     NL        0.96     NY        1.00*    
!   ON        1.00*    OV        0.95     PT        0.96     SC        0.99     
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.95     FD        0.98     GC        1.00*    HH        1.00*    
!   HN        1.07     KK        1.00*    KP        1.01     LA        1.01     
!   MC        1.00*    MK        1.08     NL        1.01     NY        1.00*    
!   ON        1.00*    OV        1.00     PT        1.00     SC        1.07     
!   TS        1.00*    WF        1.00*    WZ        1.00*    
! 
! 
! Fit before self-cal, rms=0.135519Jy  sigma=0.001860
! Fit after  self-cal, rms=0.184054Jy  sigma=0.001601
dynam = dynam - 0.5
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 21.8% of the data.
!  The x-axis pixel size should ideally be below 0.2001 milli-arcsec
!  The y-axis pixel size should ideally be below 0.3536 milli-arcsec
! Estimated beam: bmin=1.31 mas, bmaj=1.982 mas, bpa=-22.86 degrees
! Estimated noise=416.872 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 (-3.2, -2.8).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0130179 Jy
! Component: 100  -  total flux cleaned = 0.018535 Jy
! Total flux subtracted in 100 components = 0.018535 Jy
! Clean residual min=-0.008769 max=0.008873 Jy/beam
! Clean residual mean=0.000004 rms=0.001929 Jy/beam
! Combined flux in latest and established models = 0.79414 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 45 components and 0.79414 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.181392Jy  sigma=0.001573
! Fit after  self-cal, rms=0.181851Jy  sigma=0.001571
! Inverting map 
! Your choice of large map pixels excluded 21.8% of the data.
!  The x-axis pixel size should ideally be below 0.2001 milli-arcsec
!  The y-axis pixel size should ideally be below 0.3536 milli-arcsec
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 = 0.00198371 Jy
! Component: 100  -  total flux cleaned = 0.0036501 Jy
! Total flux subtracted in 100 components = 0.0036501 Jy
! Clean residual min=-0.008559 max=0.008731 Jy/beam
! Clean residual mean=0.000004 rms=0.001881 Jy/beam
! Combined flux in latest and established models = 0.79779 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 20 model components to the UV plane model.
! The established model now contains 53 components and 0.79779 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.180489Jy  sigma=0.001557
! Fit after  self-cal, rms=0.184002Jy  sigma=0.001461
! Inverting map and beam 
! Your choice of large map pixels excluded 21.8% of the data.
!  The x-axis pixel size should ideally be below 0.2001 milli-arcsec
!  The y-axis pixel size should ideally be below 0.3536 milli-arcsec
! Estimated beam: bmin=1.315 mas, bmaj=1.975 mas, bpa=-23.03 degrees
! Estimated noise=419.649 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 = 0.00743323 Jy
! Component: 100  -  total flux cleaned = 0.00925384 Jy
! Total flux subtracted in 100 components = 0.00925384 Jy
! Clean residual min=-0.006676 max=0.007243 Jy/beam
! Clean residual mean=0.000003 rms=0.001431 Jy/beam
! Combined flux in latest and established models = 0.807044 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 58 components and 0.807044 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.183123Jy  sigma=0.001450
! Fit after  self-cal, rms=0.183057Jy  sigma=0.001448
! Inverting map 
! Your choice of large map pixels excluded 21.8% of the data.
!  The x-axis pixel size should ideally be below 0.2001 milli-arcsec
!  The y-axis pixel size should ideally be below 0.3536 milli-arcsec
print "***********************************"
! *********************************** 
print "*** Finished Amplitude Self-Cal ***"
! *** Finished Amplitude Self-Cal *** 
print "***********************************"
! *********************************** 
save 1435+638_X
! Writing UV FITS file: 1435+638_X.uvf
! Writing 58 model components to file: 1435+638_X.mod
! wwins: Wrote 6 windows to 1435+638_X.win
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 1.315 x 1.975 at -23.03 degrees (North through East)
! Clean map  min=-0.0056206  max=0.40711 Jy/beam
! Writing clean map to FITS file: 1435+638_X.fits
! Writing difmap environment to: 1435+638_X.par
print "****************************"
! **************************** 
print "*** Now, make some plots ***"
! *** Now, make some plots *** 
print "****************************"
! **************************** 
![@gonzo_plot 1435+638_X]
device 1435+638_Xuv.ps/vps,1,2
! Attempting to open device: '1435+638_Xuv.ps/vps'
radplot
! Using default options string "m1"
uvplot
! Using default options string ""
device 1435+638_Xim.ps/vps
! Attempting to open device: '1435+638_Xim.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 
! Your choice of large map pixels excluded 21.8% of the data.
!  The x-axis pixel size should ideally be below 0.2001 milli-arcsec
!  The y-axis pixel size should ideally be below 0.3536 milli-arcsec
! Estimated beam: bmin=1.315 mas, bmaj=1.975 mas, bpa=-23.03 degrees
! Estimated noise=419.649 mJy/beam.
mappl cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 1.315 x 1.975 at -23.03 degrees (North through East)
! Clean map  min=-0.0056206  max=0.40711 Jy/beam
![Exited script file: gonzo_plot]
![Exited script file: gonzo7-0.4]
quit
! Quitting program
! Log file 1435+638_X.log closed on Fri Jul 22 15:59:06 2005