! Started logfile: J1524-3012_X_2004_05_08_yyk_uvs.log on Wed Dec 7 00:33:30 2005 obs J1524-3012_X_2004_05_08_yyk_uve.fits ! Reading UV FITS file: J1524-3012_X_2004_05_08_yyk_uve.fits ! AN table 1: 9 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.74321 visibilities/baseline/integration-bin. ! Found source: J1524-3012 ! ! 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 1438 lines of history. ! ! Reading 1204 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 J1524-3012_X_2004_05_08_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. phase_soltime=phase_soltime1 print "uvstat(rms)=",uvstat(rms),"Jy" ! uvstat(rms)= 0.254694 Jy startmod ,phase_soltime ! Applying default point source starting model. ! Performing phase self-cal over 10 minute time intervals ! 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 12 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 12 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 12 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 12 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.772807Jy sigma=14.059696 ! Fit after self-cal, rms=0.772728Jy sigma=14.058486 ! 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 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 milli-arcsec ! Estimated beam: bmin=0.6784 mas, bmaj=1.826 mas, bpa=-0.5553 degrees ! Estimated noise=1.96868 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 = 0.207612 Jy ! Component: 100 - total flux cleaned = 0.258014 Jy ! Total flux subtracted in 100 components = 0.258014 Jy ! Clean residual min=-0.011327 max=0.015738 Jy/beam ! Clean residual mean=-0.000072 rms=0.003431 Jy/beam ! Combined flux in latest and established models = 0.258014 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 12 model components to the UV plane model. ! The established model now contains 12 components and 0.258014 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070630Jy sigma=1.176893 ! Fit after self-cal, rms=0.070554Jy sigma=1.175981 ! Inverting map ! Your choice of large map pixels excluded 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 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 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 milli-arcsec ! Estimated beam: bmin=0.8856 mas, bmaj=2.234 mas, bpa=-1.81 degrees ! Estimated noise=1.10843 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 = 0.0219263 Jy ! Component: 100 - total flux cleaned = 0.0289809 Jy ! Component: 150 - total flux cleaned = 0.0307707 Jy ! Component: 200 - total flux cleaned = 0.0310193 Jy ! Total flux subtracted in 200 components = 0.0310193 Jy ! Clean residual min=-0.008598 max=0.010603 Jy/beam ! Clean residual mean=-0.000052 rms=0.002534 Jy/beam ! Combined flux in latest and established models = 0.289033 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 17 model components to the UV plane model. ! The established model now contains 24 components and 0.289034 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.066854Jy sigma=1.087127 ! Fit after self-cal, rms=0.066794Jy sigma=1.086624 ! Inverting map ! Your choice of large map pixels excluded 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! selflims ampcor_selflim ! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2. ! Selfcal phase corrections will not be limited. gscale ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Amplitude normalization factor in sub-array 1: 1.00322 ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.97 HN 1.00* KP 0.96 ! LA 0.99 MK 0.92 NL 1.16 OV 1.00 ! PT 0.98 SC 0.97 ! ! ! Correcting IF 2. ! Amplitude normalization factor in sub-array 1: 1.00718 ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.98 HN 1.00* KP 0.92 ! LA 0.95 MK 0.97 NL 1.13 OV 0.98 ! PT 1.01 SC 0.99 ! ! ! Correcting IF 3. ! Amplitude normalization factor in sub-array 1: 0.987576 ! Telescope amplitude corrections in sub-array 1: ! BR 1.06 FD 1.01 HN 1.00* KP 0.89 ! LA 0.98 MK 1.03 NL 1.13 OV 1.00 ! PT 1.04 SC 0.99 ! ! ! Correcting IF 4. ! Amplitude normalization factor in sub-array 1: 0.976743 ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 1.03 HN 1.00* KP 0.88 ! LA 0.97 MK 1.00 NL 1.12 OV 1.01 ! PT 1.10 SC 1.10 ! ! ! Fit before self-cal, rms=0.066794Jy sigma=1.086624 ! Fit after self-cal, rms=0.064791Jy sigma=1.026519 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=0.064791Jy sigma=1.026519 ! Fit after self-cal, rms=0.064801Jy sigma=1.026500 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 milli-arcsec ! Estimated beam: bmin=0.8803 mas, bmaj=2.235 mas, bpa=-2.311 degrees ! Estimated noise=1.0933 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 = -0.00242022 Jy ! Component: 100 - total flux cleaned = -0.0026215 Jy ! Component: 150 - total flux cleaned = -0.00279716 Jy ! Component: 200 - total flux cleaned = -0.00285148 Jy ! Total flux subtracted in 200 components = -0.00285148 Jy ! Clean residual min=-0.004024 max=0.006931 Jy/beam ! Clean residual mean=-0.000024 rms=0.001479 Jy/beam ! Combined flux in latest and established models = 0.286182 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 11 model components to the UV plane model. ! The established model now contains 31 components and 0.286182 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.064640Jy sigma=1.023765 ! Fit after self-cal, rms=0.064623Jy sigma=1.023624 ! Inverting map ! Your choice of large map pixels excluded 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 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=0.064623Jy sigma=1.023624 ! Fit after self-cal, rms=0.062097Jy sigma=0.980276 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 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) ! Added new window around map position (-4.6, -13). ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00662287 Jy ! Component: 100 - total flux cleaned = 0.00638351 Jy ! Component: 150 - total flux cleaned = 0.00607483 Jy ! Component: 200 - total flux cleaned = 0.00606469 Jy ! Total flux subtracted in 200 components = 0.00606469 Jy ! Clean residual min=-0.003858 max=0.004580 Jy/beam ! Clean residual mean=-0.000003 rms=0.001224 Jy/beam ! Combined flux in latest and established models = 0.292247 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 21 model components to the UV plane model. ! The established model now contains 50 components and 0.292247 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.061498Jy sigma=0.966453 ! Fit after self-cal, rms=0.061346Jy sigma=0.963957 ! Inverting map ! Your choice of large map pixels excluded 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 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: 0.8803 x 2.235 at -2.311 degrees (North through East) ! Clean map min=-0.0036368 max=0.21971 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=0.061346Jy sigma=0.963957 ! Fit after self-cal, rms=0.061024Jy sigma=0.957043 ! 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=0.061024Jy sigma=0.957043 ! Fit after self-cal, rms=0.061021Jy sigma=0.956842 ! Inverting map and beam ! Your choice of large map pixels excluded 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 milli-arcsec ! Estimated beam: bmin=0.8739 mas, bmaj=2.227 mas, bpa=-2.703 degrees ! Estimated noise=1.08564 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00011539 Jy ! Component: 100 - total flux cleaned = -0.000116078 Jy ! Component: 150 - total flux cleaned = -0.000255782 Jy ! Component: 200 - total flux cleaned = -0.00044793 Jy ! Total flux subtracted in 200 components = -0.00044793 Jy ! Clean residual min=-0.003680 max=0.004213 Jy/beam ! Clean residual mean=-0.000002 rms=0.001149 Jy/beam ! Combined flux in latest and established models = 0.291799 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 16 model components to the UV plane model. ! The established model now contains 60 components and 0.291799 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.060902Jy sigma=0.954319 ! Fit after self-cal, rms=0.060892Jy sigma=0.954245 ! Inverting map ! Your choice of large map pixels excluded 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 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=0.060892Jy sigma=0.954245 ! Fit after self-cal, rms=0.060505Jy sigma=0.936593 ! 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=0.060505Jy sigma=0.936593 ! Fit after self-cal, rms=0.060517Jy sigma=0.936551 ! Inverting map and beam ! Your choice of large map pixels excluded 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 milli-arcsec ! Estimated beam: bmin=0.8667 mas, bmaj=2.219 mas, bpa=-2.891 degrees ! Estimated noise=1.08263 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 5.41095e-05 Jy ! Component: 100 - total flux cleaned = -6.53325e-05 Jy ! Component: 150 - total flux cleaned = -0.000175494 Jy ! Component: 200 - total flux cleaned = -0.000275606 Jy ! Total flux subtracted in 200 components = -0.000275606 Jy ! Clean residual min=-0.003515 max=0.003986 Jy/beam ! Clean residual mean=-0.000001 rms=0.001135 Jy/beam ! Combined flux in latest and established models = 0.291523 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 19 model components to the UV plane model. ! The established model now contains 63 components and 0.291523 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.060445Jy sigma=0.934978 ! Fit after self-cal, rms=0.060441Jy sigma=0.934942 ! Inverting map ! Your choice of large map pixels excluded 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 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 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 milli-arcsec ! Estimated beam: bmin=2.743 mas, bmaj=7.677 mas, bpa=4.244 degrees ! Estimated noise=1.36838 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 = -0.000542748 Jy ! Component: 100 - total flux cleaned = -0.000574918 Jy ! Component: 150 - total flux cleaned = -0.000636264 Jy ! Component: 200 - total flux cleaned = -0.000724559 Jy ! Total flux subtracted in 200 components = -0.000724559 Jy ! Clean residual min=-0.004088 max=0.004626 Jy/beam ! Clean residual mean=-0.000004 rms=0.001548 Jy/beam ! Combined flux in latest and established models = 0.290799 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 9 model components to the UV plane model. ! The established model now contains 68 components and 0.290799 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.060430Jy sigma=0.934602 ! Fit after self-cal, rms=0.060420Jy sigma=0.934556 ! Inverting map ! Your choice of large map pixels excluded 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 milli-arcsec uvtaper 0,0 ! 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 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 milli-arcsec ! Estimated beam: bmin=0.673 mas, bmaj=1.822 mas, bpa=-0.9313 degrees ! Estimated noise=1.9373 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.206354 Jy ! Component: 100 - total flux cleaned = 0.25737 Jy ! Component: 150 - total flux cleaned = 0.275077 Jy ! Component: 200 - total flux cleaned = 0.281261 Jy ! Total flux subtracted in 200 components = 0.281261 Jy ! Clean residual min=-0.007810 max=0.007612 Jy/beam ! Clean residual mean=-0.000009 rms=0.001972 Jy/beam ! Combined flux in latest and established models = 0.281261 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 20 model components to the UV plane model. ! The established model now contains 20 components and 0.281261 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 milli-arcsec ! Estimated beam: bmin=0.8667 mas, bmaj=2.219 mas, bpa=-2.891 degrees ! Estimated noise=1.08263 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 = 0.00735311 Jy ! Component: 100 - total flux cleaned = 0.00905186 Jy ! Component: 150 - total flux cleaned = 0.0100367 Jy ! Component: 200 - total flux cleaned = 0.01032 Jy ! Total flux subtracted in 200 components = 0.01032 Jy ! Clean residual min=-0.003733 max=0.004226 Jy/beam ! Clean residual mean=-0.000007 rms=0.001215 Jy/beam ! Combined flux in latest and established models = 0.291581 Jy ! Adding 23 model components to the UV plane model. ! The established model now contains 39 components and 0.291581 Jy ! Inverting map ! Your choice of large map pixels excluded 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 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 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 milli-arcsec ! Estimated beam: bmin=2.743 mas, bmaj=7.677 mas, bpa=4.244 degrees ! Estimated noise=1.36838 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 = 0.000509109 Jy ! Component: 100 - total flux cleaned = 0.00045715 Jy ! Component: 150 - total flux cleaned = 0.000317839 Jy ! Component: 200 - total flux cleaned = 0.000184118 Jy ! Total flux subtracted in 200 components = 0.000184118 Jy ! Clean residual min=-0.004394 max=0.004685 Jy/beam ! Clean residual mean=-0.000007 rms=0.001598 Jy/beam ! Combined flux in latest and established models = 0.291765 Jy ! Adding 12 model components to the UV plane model. ! The established model now contains 48 components and 0.291765 Jy ! Inverting map ! Your choice of large map pixels excluded 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 milli-arcsec ! Estimated beam: bmin=0.8667 mas, bmaj=2.219 mas, bpa=-2.891 degrees ! Estimated noise=1.08263 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 3.22525e-05 Jy ! Component: 100 - total flux cleaned = -0.000119759 Jy ! Component: 150 - total flux cleaned = -0.000381507 Jy ! Component: 200 - total flux cleaned = -0.000504058 Jy ! Total flux subtracted in 200 components = -0.000504058 Jy ! Clean residual min=-0.003619 max=0.004012 Jy/beam ! Clean residual mean=-0.000005 rms=0.001155 Jy/beam ! Combined flux in latest and established models = 0.291261 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 21 model components to the UV plane model. ! The established model now contains 61 components and 0.291261 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.060461Jy sigma=0.936012 ! Fit after self-cal, rms=0.060440Jy sigma=0.935701 wmodel J1524-3012_X_2004_05_08_yyk\_map.mod ! Writing 61 model components to file: J1524-3012_X_2004_05_08_yyk_map.mod wobs J1524-3012_X_2004_05_08_yyk\_uvs.fits ! Writing UV FITS file: J1524-3012_X_2004_05_08_yyk_uvs.fits wwins J1524-3012_X_2004_05_08_yyk\_map.win ! wwins: Wrote 2 windows to J1524-3012_X_2004_05_08_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 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000856069 Jy ! Component: 100 - total flux cleaned = 0.000542141 Jy ! Component: 150 - total flux cleaned = 0.000420757 Jy ! Component: 200 - total flux cleaned = 0.000418652 Jy ! Component: 250 - total flux cleaned = 0.000472684 Jy ! Component: 300 - total flux cleaned = 0.000472428 Jy ! Component: 350 - total flux cleaned = 0.00032898 Jy ! Component: 400 - total flux cleaned = 0.000374602 Jy ! Component: 450 - total flux cleaned = 0.000505527 Jy ! Component: 500 - total flux cleaned = 0.000631061 Jy ! Component: 550 - total flux cleaned = 0.000792405 Jy ! Component: 600 - total flux cleaned = 0.00079215 Jy ! Component: 650 - total flux cleaned = 0.000868298 Jy ! Component: 700 - total flux cleaned = 0.000831907 Jy ! Component: 750 - total flux cleaned = 0.000903328 Jy ! Component: 800 - total flux cleaned = 0.000799805 Jy ! Component: 850 - total flux cleaned = 0.000766344 Jy ! Component: 900 - total flux cleaned = 0.000603847 Jy ! Component: 950 - total flux cleaned = 0.000510029 Jy ! Component: 1000 - total flux cleaned = 0.000355996 Jy ! Component: 1050 - total flux cleaned = 0.000146241 Jy ! Component: 1100 - total flux cleaned = -2.85122e-05 Jy ! Component: 1150 - total flux cleaned = -0.000170844 Jy ! Component: 1200 - total flux cleaned = -0.000310252 Jy ! Component: 1250 - total flux cleaned = -0.000528128 Jy ! Component: 1300 - total flux cleaned = -0.000687582 Jy ! Component: 1350 - total flux cleaned = -0.000817708 Jy ! Component: 1400 - total flux cleaned = -0.000919536 Jy ! Component: 1450 - total flux cleaned = -0.00104429 Jy ! Component: 1500 - total flux cleaned = -0.00109389 Jy ! Component: 1550 - total flux cleaned = -0.00114278 Jy ! Component: 1600 - total flux cleaned = -0.0011908 Jy ! Component: 1650 - total flux cleaned = -0.00123741 Jy ! Component: 1700 - total flux cleaned = -0.00121452 Jy ! Component: 1750 - total flux cleaned = -0.00116967 Jy ! Component: 1800 - total flux cleaned = -0.00119209 Jy ! Component: 1850 - total flux cleaned = -0.00121425 Jy ! Component: 1900 - total flux cleaned = -0.00127862 Jy ! Component: 1950 - total flux cleaned = -0.00125763 Jy ! Component: 2000 - total flux cleaned = -0.00127844 Jy ! Total flux subtracted in 2048 components = -0.00117507 Jy ! Clean residual min=-0.001068 max=0.001454 Jy/beam ! Clean residual mean=0.000004 rms=0.000398 Jy/beam ! Combined flux in latest and established models = 0.290086 Jy keep ! Adding 131 model components to the UV plane model. ! The established model now contains 192 components and 0.290086 Jy ![Exited script file: muppet] wmap "J1524-3012_X_2004_05_08_yyk\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8667 x 2.219 at -2.891 degrees (North through East) ! Clean map min=-0.0027024 max=0.21983 Jy/beam ! Writing clean map to FITS file: J1524-3012_X_2004_05_08_yyk_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.219829 invert ! Inverting map ! Your choice of large map pixels excluded 0.582% of the data. ! The x-axis pixel size should ideally be below 0.1989 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000405416 device "J1524-3012_X_2004_05_08_yyk\_map.eps/VPS" ! Attempting to open device: 'J1524-3012_X_2004_05_08_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.553271 0.553271 1.10654 2.21308 4.42617 8.85233 17.7047 35.4093 70.8186 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0012 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.219 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8667 x 2.219 at -2.891 degrees (North through East) ! Clean map min=-0.0027024 max=0.21983 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1524-3012_X_2004_05_08_yyk\_map.gif/gif" ! Attempting to open device: 'J1524-3012_X_2004_05_08_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J1524-3012_X_2004_05_08_yyk_uvs.log closed on Wed Dec 7 00:33:34 2005