! Started logfile: J2005+7752_X_2006_02_14_yyk_uvs.log on Wed Jul  5 13:40:37 2006
obs J2005+7752_X_2006_02_14_yyk_uva.fits
! Reading UV FITS file: J2005+7752_X_2006_02_14_yyk_uva.fits
! AN table 1: 866 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.795843 visibilities/baseline/integration-bin.
! Found source: J2005+7752
! 
! 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 2301 lines of history.
! 
! Reading 124056 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
![@muppet J2005+7752_X_2006_02_14_yyk]
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.04
float dynam
dynam = 6.0
float amp_soltime1
amp_soltime1 = 10
float amp_soltime2
amp_soltime2 = 1
float phase_soltime1
phase_soltime1=10
float phase_soltime2
phase_soltime2=0.5
float phase_soltime
phase_soltime=phase_soltime1
float ampcor_selflim
ampcor_selflim=1.20
float thresh
thresh = 0.10
float win_mult
win_mult = 1.8
float time_av
time_av = 30
float old_peak
float new_peak
float flux_cutoff
mapsize field_size, field_cell
! Map grid = 512x512 pixels with 0.200x0.200 milli-arcsec cellsize.
uvav time_av, true
! Averaging into 30 second bins.
! 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
phase_soltime=phase_soltime1
print "uvstat(rms)=",uvstat(rms),"Jy"
! uvstat(rms)= 0.82365 Jy 
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 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.6159 mas, bmaj=2.724 mas, bpa=-6.395 degrees
! Estimated noise=1.42738 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (0, 0).
! clean: niter=100  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.612591 Jy
! Component: 100  -  total flux cleaned = 0.785174 Jy
! Total flux subtracted in 100 components = 0.785174 Jy
! Clean residual min=-0.068461 max=0.122735 Jy/beam
! Clean residual mean=-0.000303 rms=0.020448 Jy/beam
! Combined flux in latest and established models = 0.785174 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 8 model components to the UV plane model.
! The established model now contains 8 components and 0.785174 Jy
! 
! Correcting IF 1.
!  A total of 16 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 16 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 16 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 16 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.283979Jy  sigma=5.397771
! Fit after  self-cal, rms=0.276644Jy  sigma=5.247590
! Inverting map and beam 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.6159 mas, bmaj=2.724 mas, bpa=-6.395 degrees
! Estimated noise=1.42738 mJy/beam.
! Added new window around map position (-1.8, 0).
! clean: niter=100  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.14312 Jy
! Component: 100  -  total flux cleaned = 0.221474 Jy
! Total flux subtracted in 100 components = 0.221474 Jy
! Clean residual min=-0.047250 max=0.045488 Jy/beam
! Clean residual mean=-0.000170 rms=0.011438 Jy/beam
! Combined flux in latest and established models = 1.00665 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 8 model components to the UV plane model.
! The established model now contains 14 components and 1.00665 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.196861Jy  sigma=3.632187
! Fit after  self-cal, rms=0.189745Jy  sigma=3.466803
! Inverting map 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
print "************** FINISHED UNIFORM WEIGHTING CLEAN **************"
! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** 
! 
uvw 0,-2
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -2.
! 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 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.7878 mas, bmaj=2.779 mas, bpa=-6.466 degrees
! Estimated noise=0.774651 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0884385 Jy
! Component: 100  -  total flux cleaned = 0.135094 Jy
! Component: 150  -  total flux cleaned = 0.162338 Jy
! Component: 200  -  total flux cleaned = 0.179561 Jy
! Total flux subtracted in 200 components = 0.179561 Jy
! Clean residual min=-0.024278 max=0.024053 Jy/beam
! Clean residual mean=-0.000076 rms=0.006026 Jy/beam
! Combined flux in latest and established models = 1.18621 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 23 model components to the UV plane model.
! The established model now contains 31 components and 1.18621 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.157660Jy  sigma=2.808842
! Fit after  self-cal, rms=0.154702Jy  sigma=2.737579
! Inverting map 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7878 x 2.779 at -6.466 degrees (North through East)
! Clean map  min=-0.017493  max=0.74478 Jy/beam
if(peak(flux) < thresh*2)
  selflims ampcor_selflim
  end if
gscale
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Amplitude normalization factor in sub-array 1: 0.988314
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.96     FD        1.01     HN        1.07     KP        1.01     
!   LA        1.00     MK        1.00     NL        1.04     OV        0.98     
!   PT        1.00*    SC        1.05     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.01002
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.96     FD        1.01     HN        1.06     KP        0.95     
!   LA        0.96     MK        0.96     NL        1.02     OV        0.97     
!   PT        1.00*    SC        1.03     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 1.00891
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.08     FD        1.03     HN        0.95     KP        0.87     
!   LA        0.97     MK        1.02     NL        0.99     OV        0.99     
!   PT        1.00*    SC        1.01     
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 0.99374
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.02     FD        1.06     HN        0.99     KP        0.91     
!   LA        0.96     MK        1.04     NL        1.00     OV        1.04     
!   PT        1.00*    SC        1.06     
! 
! 
! Fit before self-cal, rms=0.154702Jy  sigma=2.737579
! Fit after  self-cal, rms=0.146134Jy  sigma=2.569765
selfcal false, false, phase_soltime
! Performing phase self-cal over 10 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.146134Jy  sigma=2.569765
! Fit after  self-cal, rms=0.146653Jy  sigma=2.575152
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.7987 mas, bmaj=2.786 mas, bpa=-6.396 degrees
! Estimated noise=0.771368 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00180953 Jy
! Component: 100  -  total flux cleaned = -0.00173731 Jy
! Component: 150  -  total flux cleaned = -0.00410458 Jy
! Component: 200  -  total flux cleaned = -0.00618577 Jy
! Total flux subtracted in 200 components = -0.00618577 Jy
! Clean residual min=-0.009511 max=0.016751 Jy/beam
! Clean residual mean=-0.000010 rms=0.002894 Jy/beam
! Combined flux in latest and established models = 1.18002 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 22 model components to the UV plane model.
! The established model now contains 50 components and 1.18002 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.145049Jy  sigma=2.543997
! Fit after  self-cal, rms=0.145262Jy  sigma=2.544553
! Inverting map 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Added new window around map position (-6.6, -0.4).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0150811 Jy
! Component: 100  -  total flux cleaned = 0.0189433 Jy
! Component: 150  -  total flux cleaned = 0.0207374 Jy
! Component: 200  -  total flux cleaned = 0.0222362 Jy
! Total flux subtracted in 200 components = 0.0222362 Jy
! Clean residual min=-0.006921 max=0.007315 Jy/beam
! Clean residual mean=-0.000013 rms=0.001947 Jy/beam
! Combined flux in latest and established models = 1.20226 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 32 model components to the UV plane model.
! The established model now contains 75 components and 1.20226 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.143738Jy  sigma=2.514684
! Fit after  self-cal, rms=0.144110Jy  sigma=2.518551
! Inverting map 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
print "************** FINISHED AMPLITUDE GSCALE SELF-CAL **************"
! ************** FINISHED AMPLITUDE GSCALE SELF-CAL ************** 
! 
phase_soltime=phase_soltime2
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.144110Jy  sigma=2.518551
! Fit after  self-cal, rms=0.060787Jy  sigma=1.079464
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00289485 Jy
! Component: 100  -  total flux cleaned = 0.00479004 Jy
! Component: 150  -  total flux cleaned = 0.00674387 Jy
! Component: 200  -  total flux cleaned = 0.00833355 Jy
! Total flux subtracted in 200 components = 0.00833355 Jy
! Clean residual min=-0.007457 max=0.006027 Jy/beam
! Clean residual mean=-0.000017 rms=0.001733 Jy/beam
! Combined flux in latest and established models = 1.21059 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 27 model components to the UV plane model.
! The established model now contains 94 components and 1.21059 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.058860Jy  sigma=1.046178
! Fit after  self-cal, rms=0.057448Jy  sigma=1.021575
! Inverting map 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
print "*** FINISHED NATURAL WEIGHTING CLEAN with shorter phase_soltime ***"
! *** FINISHED NATURAL WEIGHTING CLEAN with shorter phase_soltime *** 
! 
dynam = dynam - 0.25
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7987 x 2.786 at -6.396 degrees (North through East)
! Clean map  min=-0.0069766  max=0.74519 Jy/beam
if(peak(flux) > thresh)
  selfcal true, true, amp_soltime1
  selfcal false, false, phase_soltime
  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 false,false,phase_soltime
    new_peak = peak(flux)
    until(new_peak<=flux_cutoff)
  selfcal true, true, amp_soltime2
  selfcal false, false, phase_soltime
  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 false,false,phase_soltime
    new_peak = peak(flux)
    until(new_peak<=flux_cutoff)
  print "************** FINISHED AMPLITUDE SELF-CAL **************"
  end if
! Performing amp+phase self-cal over 10 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.057448Jy  sigma=1.021575
! Fit after  self-cal, rms=0.053950Jy  sigma=0.954192
! Performing phase self-cal over 0.5 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.053950Jy  sigma=0.954192
! Fit after  self-cal, rms=0.053873Jy  sigma=0.952727
! Inverting map and beam 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.7971 mas, bmaj=2.788 mas, bpa=-6.513 degrees
! Estimated noise=0.768369 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00579262 Jy
! Component: 100  -  total flux cleaned = 0.00775522 Jy
! Component: 150  -  total flux cleaned = 0.00957373 Jy
! Component: 200  -  total flux cleaned = 0.0102782 Jy
! Total flux subtracted in 200 components = 0.0102782 Jy
! Clean residual min=-0.004958 max=0.004566 Jy/beam
! Clean residual mean=-0.000003 rms=0.001289 Jy/beam
! Combined flux in latest and established models = 1.22087 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 34 model components to the UV plane model.
! The established model now contains 119 components and 1.22087 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.053211Jy  sigma=0.939519
! Fit after  self-cal, rms=0.053126Jy  sigma=0.938109
! Inverting map 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Performing amp+phase self-cal over 1 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.053126Jy  sigma=0.938109
! Fit after  self-cal, rms=0.051979Jy  sigma=0.915521
! Performing phase self-cal over 0.5 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.051979Jy  sigma=0.915521
! Fit after  self-cal, rms=0.051980Jy  sigma=0.915507
! Inverting map and beam 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.7962 mas, bmaj=2.789 mas, bpa=-6.525 degrees
! Estimated noise=0.768198 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00351819 Jy
! Component: 100  -  total flux cleaned = 0.0048106 Jy
! Component: 150  -  total flux cleaned = 0.00568781 Jy
! Component: 200  -  total flux cleaned = 0.00630718 Jy
! Total flux subtracted in 200 components = 0.00630718 Jy
! Clean residual min=-0.004288 max=0.003919 Jy/beam
! Clean residual mean=-0.000003 rms=0.001119 Jy/beam
! Combined flux in latest and established models = 1.22718 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 37 model components to the UV plane model.
! The established model now contains 142 components and 1.22718 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.051657Jy  sigma=0.908947
! Fit after  self-cal, rms=0.051619Jy  sigma=0.908334
! Inverting map 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! ************** FINISHED AMPLITUDE SELF-CAL ************** 
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
win_mult = win_mult * 1.4
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=1.893 mas, bmaj=3.043 mas, bpa=-9.615 degrees
! Estimated noise=1.0229 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00370904 Jy
! Component: 100  -  total flux cleaned = 0.00442044 Jy
! Component: 150  -  total flux cleaned = 0.00487662 Jy
! Component: 200  -  total flux cleaned = 0.00523512 Jy
! Total flux subtracted in 200 components = 0.00523512 Jy
! Clean residual min=-0.005407 max=0.005149 Jy/beam
! Clean residual mean=-0.000015 rms=0.001559 Jy/beam
! Combined flux in latest and established models = 1.23241 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 41 model components to the UV plane model.
! The established model now contains 169 components and 1.23241 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.051644Jy  sigma=0.907421
! Fit after  self-cal, rms=0.051628Jy  sigma=0.907188
! Inverting map 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
win_mult = win_mult / 1.4
print "************** FINISHED TAPERING SELF-CAL CLEAN **************"
! ************** FINISHED TAPERING SELF-CAL CLEAN ************** 
! 
print "************** CLEARING MODEL AND STARTING OVER **********"
! ************** CLEARING MODEL AND STARTING OVER ********** 
clrmod true,true,true
! clrmod: Cleared the established, tentative and continuum 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 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.6186 mas, bmaj=2.724 mas, bpa=-6.391 degrees
! Estimated noise=1.41959 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.623324 Jy
! Component: 100  -  total flux cleaned = 0.830727 Jy
! Component: 150  -  total flux cleaned = 0.952339 Jy
! Component: 200  -  total flux cleaned = 1.03184 Jy
! Total flux subtracted in 200 components = 1.03184 Jy
! Clean residual min=-0.024243 max=0.032315 Jy/beam
! Clean residual mean=-0.000105 rms=0.007146 Jy/beam
! Combined flux in latest and established models = 1.03184 Jy
uvw 0,-2
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -2.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Adding 17 model components to the UV plane model.
! The established model now contains 17 components and 1.03184 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.7962 mas, bmaj=2.789 mas, bpa=-6.525 degrees
! Estimated noise=0.768198 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=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0746791 Jy
! Component: 100  -  total flux cleaned = 0.115349 Jy
! Component: 150  -  total flux cleaned = 0.141764 Jy
! Component: 200  -  total flux cleaned = 0.157705 Jy
! Total flux subtracted in 200 components = 0.157705 Jy
! Clean residual min=-0.008733 max=0.008416 Jy/beam
! Clean residual mean=-0.000023 rms=0.002605 Jy/beam
! Combined flux in latest and established models = 1.18955 Jy
! Adding 24 model components to the UV plane model.
! The established model now contains 34 components and 1.18955 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=1.893 mas, bmaj=3.043 mas, bpa=-9.615 degrees
! Estimated noise=1.0229 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=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0177888 Jy
! Component: 100  -  total flux cleaned = 0.0233687 Jy
! Component: 150  -  total flux cleaned = 0.0267218 Jy
! Component: 200  -  total flux cleaned = 0.0295778 Jy
! Total flux subtracted in 200 components = 0.0295778 Jy
! Clean residual min=-0.008351 max=0.006264 Jy/beam
! Clean residual mean=-0.000025 rms=0.002289 Jy/beam
! Combined flux in latest and established models = 1.21912 Jy
! Adding 48 model components to the UV plane model.
! The established model now contains 76 components and 1.21912 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.7962 mas, bmaj=2.789 mas, bpa=-6.525 degrees
! Estimated noise=0.768198 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00226076 Jy
! Component: 100  -  total flux cleaned = 0.00397278 Jy
! Component: 150  -  total flux cleaned = 0.0059521 Jy
! Component: 200  -  total flux cleaned = 0.00764427 Jy
! Total flux subtracted in 200 components = 0.00764427 Jy
! Clean residual min=-0.005146 max=0.004602 Jy/beam
! Clean residual mean=-0.000007 rms=0.001257 Jy/beam
! Combined flux in latest and established models = 1.22677 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 27 model components to the UV plane model.
! The established model now contains 101 components and 1.22677 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.052287Jy  sigma=0.919630
! Fit after  self-cal, rms=0.052116Jy  sigma=0.916526
wmodel J2005+7752_X_2006_02_14_yyk\_map.mod
! Writing 101 model components to file: J2005+7752_X_2006_02_14_yyk_map.mod
wobs J2005+7752_X_2006_02_14_yyk\_uvs.fits
! Writing UV FITS file: J2005+7752_X_2006_02_14_yyk_uvs.fits
wwins J2005+7752_X_2006_02_14_yyk\_map.win
! wwins: Wrote 3 windows to J2005+7752_X_2006_02_14_yyk_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 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00153571 Jy
! Component: 100  -  total flux cleaned = -0.00237212 Jy
! Component: 150  -  total flux cleaned = -0.00251529 Jy
! Component: 200  -  total flux cleaned = -0.00225817 Jy
! Component: 250  -  total flux cleaned = -0.00189405 Jy
! Component: 300  -  total flux cleaned = -0.0016653 Jy
! Component: 350  -  total flux cleaned = -0.00166452 Jy
! Component: 400  -  total flux cleaned = -0.00171489 Jy
! Component: 450  -  total flux cleaned = -0.00166472 Jy
! Component: 500  -  total flux cleaned = -0.00180735 Jy
! Component: 550  -  total flux cleaned = -0.00180795 Jy
! Component: 600  -  total flux cleaned = -0.00189652 Jy
! Component: 650  -  total flux cleaned = -0.00189694 Jy
! Component: 700  -  total flux cleaned = -0.00189677 Jy
! Component: 750  -  total flux cleaned = -0.00181623 Jy
! Component: 800  -  total flux cleaned = -0.00173918 Jy
! Component: 850  -  total flux cleaned = -0.00170177 Jy
! Component: 900  -  total flux cleaned = -0.00166569 Jy
! Component: 950  -  total flux cleaned = -0.00177121 Jy
! Component: 1000  -  total flux cleaned = -0.00183912 Jy
! Component: 1050  -  total flux cleaned = -0.00193845 Jy
! Component: 1100  -  total flux cleaned = -0.00206762 Jy
! Component: 1150  -  total flux cleaned = -0.0021305 Jy
! Component: 1200  -  total flux cleaned = -0.00209904 Jy
! Component: 1250  -  total flux cleaned = -0.0021301 Jy
! Component: 1300  -  total flux cleaned = -0.0021303 Jy
! Component: 1350  -  total flux cleaned = -0.00227596 Jy
! Component: 1400  -  total flux cleaned = -0.00216088 Jy
! Component: 1450  -  total flux cleaned = -0.00227352 Jy
! Component: 1500  -  total flux cleaned = -0.00221844 Jy
! Component: 1550  -  total flux cleaned = -0.00235428 Jy
! Component: 1600  -  total flux cleaned = -0.00245982 Jy
! Component: 1650  -  total flux cleaned = -0.00248565 Jy
! Component: 1700  -  total flux cleaned = -0.00261301 Jy
! Component: 1750  -  total flux cleaned = -0.00273759 Jy
! Component: 1800  -  total flux cleaned = -0.00273711 Jy
! Component: 1850  -  total flux cleaned = -0.0027861 Jy
! Component: 1900  -  total flux cleaned = -0.00281004 Jy
! Component: 1950  -  total flux cleaned = -0.00278674 Jy
! Component: 2000  -  total flux cleaned = -0.00283328 Jy
! Total flux subtracted in 2048 components = -0.00287912 Jy
! Clean residual min=-0.001303 max=0.001186 Jy/beam
! Clean residual mean=-0.000002 rms=0.000433 Jy/beam
! Combined flux in latest and established models = 1.22389 Jy
keep
! Adding 153 model components to the UV plane model.
! The established model now contains 254 components and 1.22389 Jy
![Exited script file: muppet]
wmap "J2005+7752_X_2006_02_14_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7962 x 2.789 at -6.525 degrees (North through East)
! Clean map  min=-0.0028784  max=0.73826 Jy/beam
! Writing clean map to FITS file: J2005+7752_X_2006_02_14_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.738265 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.694% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000424414 
device "J2005+7752_X_2006_02_14_yyk\_map.eps/VPS"
! Attempting to open device: 'J2005+7752_X_2006_02_14_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.172464 0.172464 0.344928 0.689857 1.37971 2.75943 5.51886 11.0377 22.0754 44.1508 88.3017
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0012 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.738 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7962 x 2.789 at -6.525 degrees (North through East)
! Clean map  min=-0.0028784  max=0.73826 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J2005+7752_X_2006_02_14_yyk\_map.gif/gif"
! Attempting to open device: 'J2005+7752_X_2006_02_14_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J2005+7752_X_2006_02_14_yyk_uvs.log closed on Wed Jul  5 13:41:25 2006