! Started logfile: J1037-2934_X_1999_05_10_pus_uvs.log on Tue Jan 15 12:33:51 2008
obs J1037-2934_X_1999_05_10_pus_uva.fits
! Reading UV FITS file: J1037-2934_X_1999_05_10_pus_uva.fits
! AN table 1: 120 integrations on 153 of 153 possible baselines.
! AN table 2: 11 integrations on 153 of 153 possible baselines.
! AN table 3: 30 integrations on 153 of 153 possible baselines.
! AN table 4: 20 integrations on 153 of 153 possible baselines.
! Apparent sampling: 0.150074 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J1037-2934
! 
! 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 1771 lines of history.
! 
! Reading 16624 visibilities.
select I
! Polarization I is unavailable.
! Selecting polarization: RR,  channels: 1..4
! Reading IF 1 channels: 1..1
! Reading IF 2 channels: 2..2
! Reading IF 3 channels: 3..3
! Reading IF 4 channels: 4..4
print "field_size =",field_size
! field_size = 256 
print "field_cell =",field_cell
! field_cell = 0.2 
print "taper_size =",taper_size
! taper_size = 70 
![@muppet J1037-2934_X_1999_05_10_pus]
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 = 256x256 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 1348 telescope corrections were flagged in sub-array 1.
!  A total of 198 telescope corrections were flagged in sub-array 2.
!  A total of 540 telescope corrections were flagged in sub-array 3.
!  A total of 200 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 2.
!  A total of 1340 telescope corrections were flagged in sub-array 1.
!  A total of 198 telescope corrections were flagged in sub-array 2.
!  A total of 540 telescope corrections were flagged in sub-array 3.
!  A total of 200 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 3.
!  A total of 1340 telescope corrections were flagged in sub-array 1.
!  A total of 198 telescope corrections were flagged in sub-array 2.
!  A total of 540 telescope corrections were flagged in sub-array 3.
!  A total of 200 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 4.
!  A total of 1340 telescope corrections were flagged in sub-array 1.
!  A total of 198 telescope corrections were flagged in sub-array 2.
!  A total of 540 telescope corrections were flagged in sub-array 3.
!  A total of 200 telescope corrections were flagged in sub-array 4.
! 
! Fit before self-cal, rms=0.247462Jy  sigma=0.002154
! Fit after  self-cal, rms=0.243556Jy  sigma=0.002115
! 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 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! Estimated beam: bmin=0.6299 mas, bmaj=1.778 mas, bpa=-3.81 degrees
! Estimated noise=1323.76 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 = 0.740498 Jy
! Component: 100  -  total flux cleaned = 0.94945 Jy
! Total flux subtracted in 100 components = 0.94945 Jy
! Clean residual min=-0.025586 max=0.084940 Jy/beam
! Clean residual mean=0.001352 rms=0.010161 Jy/beam
! Combined flux in latest and established models = 0.94945 Jy
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 6 components and 0.94945 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.235245Jy  sigma=0.002144
! Fit after  self-cal, rms=0.234751Jy  sigma=0.002142
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0915332 Jy
! Component: 100  -  total flux cleaned = 0.139768 Jy
! Total flux subtracted in 100 components = 0.139768 Jy
! Clean residual min=-0.011776 max=0.038235 Jy/beam
! Clean residual mean=0.000656 rms=0.004707 Jy/beam
! Combined flux in latest and established models = 1.08922 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 14 components and 1.08922 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.181381Jy  sigma=0.001400
! Fit after  self-cal, rms=0.181208Jy  sigma=0.001399
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! Added new window around map position (0.8, -0.4).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0372793 Jy
! Component: 100  -  total flux cleaned = 0.0591776 Jy
! Total flux subtracted in 100 components = 0.0591776 Jy
! Clean residual min=-0.009759 max=0.017415 Jy/beam
! Clean residual mean=0.000341 rms=0.002935 Jy/beam
! Combined flux in latest and established models = 1.1484 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 20 components and 1.1484 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.170353Jy  sigma=0.001226
! Fit after  self-cal, rms=0.169794Jy  sigma=0.001222
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 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 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! Estimated beam: bmin=0.7538 mas, bmaj=2.15 mas, bpa=-11.48 degrees
! Estimated noise=606.278 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 = 0.026306 Jy
! Component: 100  -  total flux cleaned = 0.0396689 Jy
! Component: 150  -  total flux cleaned = 0.0470753 Jy
! Component: 200  -  total flux cleaned = 0.0501546 Jy
! Total flux subtracted in 200 components = 0.0501546 Jy
! Clean residual min=-0.007223 max=0.009583 Jy/beam
! Clean residual mean=0.000144 rms=0.001787 Jy/beam
! Combined flux in latest and established models = 1.19855 Jy
! Performing phase self-cal
! Adding 20 model components to the UV plane model.
! The established model now contains 34 components and 1.19855 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.166531Jy  sigma=0.001163
! Fit after  self-cal, rms=0.166200Jy  sigma=0.001160
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        1.00     GC        1.00*    HH        1.00*    
!   HN        1.02     KK        1.00     KP        0.99     LA        0.99     
!   MC        1.00*    MK        1.00     NL        1.00     NY        1.00*    
!   ON        1.00*    OV        1.00     PT        0.99     SC        1.01     
!   WF        1.05     WZ        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*    
!   MC        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   ON        0.00*    OV        0.00*    PT        0.00*    SC        0.00*    
!   WF        0.00*    WZ        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*    
!   MC        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   ON        0.00*    OV        0.00*    PT        0.00*    SC        0.00*    
!   WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.01     FD        1.00     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.01     KP        1.00     LA        1.00     
!   MC        1.00*    MK        1.00     NL        1.00     NY        1.00*    
!   ON        1.00*    OV        1.00     PT        1.00     SC        1.01     
!   WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        1.00     GC        1.00*    HH        1.00*    
!   HN        1.02     KK        1.00     KP        0.99     LA        0.99     
!   MC        1.00*    MK        1.00     NL        1.00     NY        1.00*    
!   ON        1.00*    OV        1.00     PT        0.99     SC        1.00     
!   WF        1.02     WZ        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*    
!   MC        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   ON        0.00*    OV        0.00*    PT        0.00*    SC        0.00*    
!   WF        0.00*    WZ        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*    
!   MC        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   ON        0.00*    OV        0.00*    PT        0.00*    SC        0.00*    
!   WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.01     FD        1.00     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.01     KP        1.00     LA        1.00     
!   MC        1.00*    MK        1.00     NL        1.01     NY        1.00*    
!   ON        1.00*    OV        1.00     PT        1.00     SC        1.01     
!   WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.01     FD        1.00     GC        1.00*    HH        1.00*    
!   HN        1.02     KK        1.00     KP        0.99     LA        0.99     
!   MC        1.00*    MK        1.00     NL        1.01     NY        1.00*    
!   ON        1.00*    OV        1.00     PT        0.99     SC        1.00     
!   WF        1.02     WZ        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*    
!   MC        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   ON        0.00*    OV        0.00*    PT        0.00*    SC        0.00*    
!   WF        0.00*    WZ        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*    
!   MC        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   ON        0.00*    OV        0.00*    PT        0.00*    SC        0.00*    
!   WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.01     FD        1.00     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.01     KP        1.00     LA        1.00     
!   MC        1.00*    MK        1.01     NL        1.01     NY        1.00*    
!   ON        1.00*    OV        1.01     PT        1.00     SC        1.01     
!   WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.01     FD        1.00     GC        1.00*    HH        1.00*    
!   HN        1.02     KK        1.00     KP        0.99     LA        0.99     
!   MC        1.00*    MK        1.00     NL        1.00     NY        1.00*    
!   ON        1.00*    OV        1.00     PT        0.99     SC        1.00     
!   WF        1.02     WZ        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*    
!   MC        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   ON        0.00*    OV        0.00*    PT        0.00*    SC        0.00*    
!   WF        0.00*    WZ        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*    
!   MC        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   ON        0.00*    OV        0.00*    PT        0.00*    SC        0.00*    
!   WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.02     FD        1.00     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.01     KP        1.00     LA        1.00     
!   MC        1.00*    MK        1.01     NL        1.01     NY        1.00*    
!   ON        1.00*    OV        1.01     PT        1.00     SC        1.01     
!   WF        1.00*    WZ        1.00*    
! 
! 
! Fit before self-cal, rms=0.166200Jy  sigma=0.001160
! Fit after  self-cal, rms=0.168518Jy  sigma=0.001156
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! Estimated beam: bmin=0.7551 mas, bmaj=2.153 mas, bpa=-11.52 degrees
! Estimated noise=606.209 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 = -0.000486194 Jy
! Component: 100  -  total flux cleaned = -0.000697566 Jy
! Component: 150  -  total flux cleaned = -0.000878173 Jy
! Component: 200  -  total flux cleaned = -0.000799944 Jy
! Total flux subtracted in 200 components = -0.000799944 Jy
! Clean residual min=-0.006205 max=0.006928 Jy/beam
! Clean residual mean=-0.000047 rms=0.001291 Jy/beam
! Combined flux in latest and established models = 1.19775 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 40 components and 1.19775 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.168396Jy  sigma=0.001154
! Fit after  self-cal, rms=0.168423Jy  sigma=0.001154
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! Added new window around map position (2.8, -3.4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00629513 Jy
! Component: 100  -  total flux cleaned = 0.00670836 Jy
! Component: 150  -  total flux cleaned = 0.00671517 Jy
! Component: 200  -  total flux cleaned = 0.00671862 Jy
! Total flux subtracted in 200 components = 0.00671862 Jy
! Clean residual min=-0.005703 max=0.002751 Jy/beam
! Clean residual mean=-0.000184 rms=0.000999 Jy/beam
! Combined flux in latest and established models = 1.20447 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 53 components and 1.20447 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.168134Jy  sigma=0.001151
! Fit after  self-cal, rms=0.168102Jy  sigma=0.001151
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 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=0.168102Jy  sigma=0.001151
! Fit after  self-cal, rms=0.167774Jy  sigma=0.001151
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! Estimated beam: bmin=0.7551 mas, bmaj=2.153 mas, bpa=-11.51 degrees
! Estimated noise=605.366 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000726539 Jy
! Component: 100  -  total flux cleaned = 0.000917212 Jy
! Component: 150  -  total flux cleaned = 0.000845217 Jy
! Component: 200  -  total flux cleaned = 0.000847276 Jy
! Total flux subtracted in 200 components = 0.000847276 Jy
! Clean residual min=-0.004925 max=0.002666 Jy/beam
! Clean residual mean=-0.000181 rms=0.000916 Jy/beam
! Combined flux in latest and established models = 1.20532 Jy
selfcal
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 63 components and 1.20532 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.167674Jy  sigma=0.001150
! Fit after  self-cal, rms=0.167659Jy  sigma=0.001150
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 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 = 0.000402143 Jy
! Component: 100  -  total flux cleaned = 0.000340798 Jy
! Component: 150  -  total flux cleaned = 0.000342981 Jy
! Component: 200  -  total flux cleaned = 0.000344684 Jy
! Total flux subtracted in 200 components = 0.000344684 Jy
! Clean residual min=-0.004474 max=0.002403 Jy/beam
! Clean residual mean=-0.000189 rms=0.000885 Jy/beam
! Combined flux in latest and established models = 1.20566 Jy
! Performing phase self-cal
! Adding 20 model components to the UV plane model.
! The established model now contains 68 components and 1.20566 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.167606Jy  sigma=0.001149
! Fit after  self-cal, rms=0.167605Jy  sigma=0.001149
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 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=0.167605Jy  sigma=0.001149
! Fit after  self-cal, rms=0.167549Jy  sigma=0.001149
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! Estimated beam: bmin=0.7553 mas, bmaj=2.152 mas, bpa=-11.49 degrees
! Estimated noise=604.848 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000259013 Jy
! Component: 100  -  total flux cleaned = -0.000376187 Jy
! Component: 150  -  total flux cleaned = -0.000424301 Jy
! Component: 200  -  total flux cleaned = -0.000423776 Jy
! Total flux subtracted in 200 components = -0.000423776 Jy
! Clean residual min=-0.003946 max=0.002365 Jy/beam
! Clean residual mean=-0.000161 rms=0.000836 Jy/beam
! Combined flux in latest and established models = 1.20524 Jy
selfcal
! Performing phase self-cal
! Adding 20 model components to the UV plane model.
! The established model now contains 75 components and 1.20524 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.167506Jy  sigma=0.001149
! Fit after  self-cal, rms=0.167502Jy  sigma=0.001149
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 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 = 0.000156017 Jy
! Component: 100  -  total flux cleaned = 7.31593e-05 Jy
! Component: 150  -  total flux cleaned = 3.42238e-05 Jy
! Component: 200  -  total flux cleaned = -3.82465e-06 Jy
! Total flux subtracted in 200 components = -3.82465e-06 Jy
! Clean residual min=-0.003697 max=0.002268 Jy/beam
! Clean residual mean=-0.000162 rms=0.000823 Jy/beam
! Combined flux in latest and established models = 1.20523 Jy
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 77 components and 1.20523 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.167477Jy  sigma=0.001149
! Fit after  self-cal, rms=0.167477Jy  sigma=0.001149
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 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=0.167477Jy  sigma=0.001149
! Fit after  self-cal, rms=0.167410Jy  sigma=0.001149
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! Estimated beam: bmin=2.294 mas, bmaj=6.17 mas, bpa=-4.885 degrees
! Estimated noise=762.61 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00150177 Jy
! Component: 100  -  total flux cleaned = -0.00158141 Jy
! Component: 150  -  total flux cleaned = -0.00167716 Jy
! Component: 200  -  total flux cleaned = -0.00167838 Jy
! Total flux subtracted in 200 components = -0.00167838 Jy
! Clean residual min=-0.003376 max=0.002779 Jy/beam
! Clean residual mean=-0.000264 rms=0.001041 Jy/beam
! Combined flux in latest and established models = 1.20355 Jy
selfcal
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 86 components and 1.20355 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.167410Jy  sigma=0.001149
! Fit after  self-cal, rms=0.167389Jy  sigma=0.001148
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 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 = 0.000117986 Jy
! Component: 100  -  total flux cleaned = 5.4803e-05 Jy
! Component: 150  -  total flux cleaned = -2.08134e-06 Jy
! Component: 200  -  total flux cleaned = -2.78351e-05 Jy
! Total flux subtracted in 200 components = -2.78351e-05 Jy
! Clean residual min=-0.003360 max=0.002801 Jy/beam
! Clean residual mean=-0.000263 rms=0.001046 Jy/beam
! Combined flux in latest and established models = 1.20353 Jy
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 91 components and 1.20353 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.167393Jy  sigma=0.001148
! Fit after  self-cal, rms=0.167384Jy  sigma=0.001148
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 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 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! Estimated beam: bmin=0.7555 mas, bmaj=2.152 mas, bpa=-11.47 degrees
! Estimated noise=604.489 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7555 x 2.152 at -11.47 degrees (North through East)
! Clean map  min=-0.0030427  max=1.0133 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=0.167384Jy  sigma=0.001148
! Fit after  self-cal, rms=0.170105Jy  sigma=0.001146
! Inverting map and beam 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! Estimated beam: bmin=0.7559 mas, bmaj=2.152 mas, bpa=-11.44 degrees
! Estimated noise=604.036 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000266936 Jy
! Component: 100  -  total flux cleaned = -0.000264957 Jy
! Component: 150  -  total flux cleaned = -0.00032869 Jy
! Component: 200  -  total flux cleaned = -0.000358269 Jy
! Total flux subtracted in 200 components = -0.000358269 Jy
! Clean residual min=-0.003255 max=0.002416 Jy/beam
! Clean residual mean=-0.000074 rms=0.000775 Jy/beam
! Combined flux in latest and established models = 1.20317 Jy
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 100 components and 1.20317 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.170085Jy  sigma=0.001146
! Fit after  self-cal, rms=0.170086Jy  sigma=0.001146
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -2.93825e-05 Jy
! Component: 100  -  total flux cleaned = -5.66971e-05 Jy
! Component: 150  -  total flux cleaned = -5.5711e-05 Jy
! Component: 200  -  total flux cleaned = -5.54625e-05 Jy
! Total flux subtracted in 200 components = -5.54625e-05 Jy
! Clean residual min=-0.003239 max=0.002330 Jy/beam
! Clean residual mean=-0.000073 rms=0.000768 Jy/beam
! Combined flux in latest and established models = 1.20311 Jy
! Performing phase self-cal
! Adding 25 model components to the UV plane model.
! The established model now contains 106 components and 1.20311 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.170074Jy  sigma=0.001146
! Fit after  self-cal, rms=0.170074Jy  sigma=0.001146
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.170074Jy  sigma=0.001146
! Fit after  self-cal, rms=0.170052Jy  sigma=0.001146
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 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! Estimated beam: bmin=0.6315 mas, bmaj=1.78 mas, bpa=-3.773 degrees
! Estimated noise=1324.71 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.740831 Jy
! Component: 100  -  total flux cleaned = 0.952729 Jy
! Component: 150  -  total flux cleaned = 1.04362 Jy
! Component: 200  -  total flux cleaned = 1.09225 Jy
! Total flux subtracted in 200 components = 1.09225 Jy
! Clean residual min=-0.011264 max=0.025130 Jy/beam
! Clean residual mean=0.000583 rms=0.003934 Jy/beam
! Combined flux in latest and established models = 1.09225 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 16 model components to the UV plane model.
! The established model now contains 16 components and 1.09225 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! Estimated beam: bmin=0.7561 mas, bmaj=2.152 mas, bpa=-11.43 degrees
! Estimated noise=603.857 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 = 0.0485101 Jy
! Component: 100  -  total flux cleaned = 0.0732952 Jy
! Component: 150  -  total flux cleaned = 0.0873339 Jy
! Component: 200  -  total flux cleaned = 0.0960405 Jy
! Total flux subtracted in 200 components = 0.0960405 Jy
! Clean residual min=-0.004196 max=0.006202 Jy/beam
! Clean residual mean=0.000232 rms=0.001385 Jy/beam
! Combined flux in latest and established models = 1.18829 Jy
! Adding 32 model components to the UV plane model.
! The established model now contains 41 components and 1.18829 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! Added new window around map position (-0.4, -2).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00648646 Jy
! Component: 100  -  total flux cleaned = 0.00899232 Jy
! Component: 150  -  total flux cleaned = 0.0102546 Jy
! Component: 200  -  total flux cleaned = 0.0111921 Jy
! Total flux subtracted in 200 components = 0.0111921 Jy
! Clean residual min=-0.003391 max=0.002594 Jy/beam
! Clean residual mean=0.000012 rms=0.000878 Jy/beam
! Combined flux in latest and established models = 1.19948 Jy
! Adding 26 model components to the UV plane model.
! The established model now contains 62 components and 1.19948 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 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 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! Estimated beam: bmin=2.294 mas, bmaj=6.171 mas, bpa=-4.866 degrees
! Estimated noise=761.222 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00205146 Jy
! Component: 100  -  total flux cleaned = 0.00210369 Jy
! Component: 150  -  total flux cleaned = 0.00205653 Jy
! Component: 200  -  total flux cleaned = 0.0020144 Jy
! Total flux subtracted in 200 components = 0.0020144 Jy
! Clean residual min=-0.002929 max=0.002956 Jy/beam
! Clean residual mean=-0.000074 rms=0.000954 Jy/beam
! Combined flux in latest and established models = 1.20149 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 = -4.39546e-07 Jy
! Component: 100  -  total flux cleaned = -3.81809e-05 Jy
! Component: 150  -  total flux cleaned = -3.84811e-05 Jy
! Component: 200  -  total flux cleaned = -7.06909e-05 Jy
! Total flux subtracted in 200 components = -7.06909e-05 Jy
! Clean residual min=-0.002884 max=0.002905 Jy/beam
! Clean residual mean=-0.000070 rms=0.000937 Jy/beam
! Combined flux in latest and established models = 1.20142 Jy
! Adding 21 model components to the UV plane model.
! The established model now contains 78 components and 1.20142 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! Estimated beam: bmin=0.7561 mas, bmaj=2.152 mas, bpa=-11.43 degrees
! Estimated noise=603.857 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00118587 Jy
! Component: 100  -  total flux cleaned = -0.00118158 Jy
! Component: 150  -  total flux cleaned = -0.00109836 Jy
! Component: 200  -  total flux cleaned = -0.000950029 Jy
! Total flux subtracted in 200 components = -0.000950029 Jy
! Clean residual min=-0.003072 max=0.002278 Jy/beam
! Clean residual mean=-0.000008 rms=0.000787 Jy/beam
! Combined flux in latest and established models = 1.20047 Jy
selfcal
! Performing phase self-cal
! Adding 25 model components to the UV plane model.
! The established model now contains 95 components and 1.20047 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.170242Jy  sigma=0.001147
! Fit after  self-cal, rms=0.170193Jy  sigma=0.001147
wmodel J1037-2934_X_1999_05_10_pus_map.mod
! Writing 95 model components to file: J1037-2934_X_1999_05_10_pus_map.mod
wobs J1037-2934_X_1999_05_10_pus_uvs.fits
! Writing UV FITS file: J1037-2934_X_1999_05_10_pus_uvs.fits
wwins J1037-2934_X_1999_05_10_pus_map.win
! wwins: Wrote 4 windows to J1037-2934_X_1999_05_10_pus_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 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000811089 Jy
! Component: 100  -  total flux cleaned = -0.00114492 Jy
! Component: 150  -  total flux cleaned = -0.00145869 Jy
! Component: 200  -  total flux cleaned = -0.00157167 Jy
! Component: 250  -  total flux cleaned = -0.00175258 Jy
! Component: 300  -  total flux cleaned = -0.00185608 Jy
! Component: 350  -  total flux cleaned = -0.0018564 Jy
! Component: 400  -  total flux cleaned = -0.00192247 Jy
! Component: 450  -  total flux cleaned = -0.00188984 Jy
! Component: 500  -  total flux cleaned = -0.00195178 Jy
! Component: 550  -  total flux cleaned = -0.00198249 Jy
! Component: 600  -  total flux cleaned = -0.00201287 Jy
! Component: 650  -  total flux cleaned = -0.00210076 Jy
! Component: 700  -  total flux cleaned = -0.00212928 Jy
! Component: 750  -  total flux cleaned = -0.00212974 Jy
! Component: 800  -  total flux cleaned = -0.00218575 Jy
! Component: 850  -  total flux cleaned = -0.0021858 Jy
! Component: 900  -  total flux cleaned = -0.00213189 Jy
! Component: 950  -  total flux cleaned = -0.00207917 Jy
! Component: 1000  -  total flux cleaned = -0.00210553 Jy
! Total flux subtracted in 1024 components = -0.00207952 Jy
! Clean residual min=-0.001547 max=0.001533 Jy/beam
! Clean residual mean=0.000011 rms=0.000524 Jy/beam
! Combined flux in latest and established models = 1.19839 Jy
keep
! Adding 66 model components to the UV plane model.
! The established model now contains 161 components and 1.19839 Jy
![Exited script file: muppet]
wmap "J1037-2934_X_1999_05_10_pus\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7561 x 2.152 at -11.43 degrees (North through East)
! Clean map  min=-0.0021325  max=1.0106 Jy/beam
! Writing clean map to FITS file: J1037-2934_X_1999_05_10_pus_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 1.0106 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.246% of the data.
!  The x-axis pixel size should ideally be below 0.1923 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000524151 
device "J1037-2934_X_1999_05_10_pus\_map.eps/VPS"
! Attempting to open device: 'J1037-2934_X_1999_05_10_pus_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.155596 0.155596 0.311192 0.622385 1.24477 2.48954 4.97908 9.95816 19.9163 39.8326 79.6653
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0015 
print "peak=",int(1000*peak_flux)/1000
! peak= 1.01 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7561 x 2.152 at -11.43 degrees (North through East)
! Clean map  min=-0.0021325  max=1.0106 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1037-2934_X_1999_05_10_pus\_map.gif/vgif"
! Attempting to open device: 'J1037-2934_X_1999_05_10_pus_map.gif/vgif'
mapplot cln
quit
! Quitting program
! Log file J1037-2934_X_1999_05_10_pus_uvs.log closed on Tue Jan 15 12:33:59 2008