! Started logfile: J1522-2730_X_2014_05_31_pus_uvs.log on Sun Nov 27 18:08:45 2016 obs J1522-2730_X_2014_05_31_pus_uva.fits ! Reading UV FITS file: J1522-2730_X_2014_05_31_pus_uva.fits ! AN table 1: 54 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.832099 visibilities/baseline/integration-bin. ! Found source: J1522-2730 ! ! There are 12 IFs, and a total of 12 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.44388e+09 3.2e+07 1 3.2e+07 ! 02 2 8.47588e+09 3.2e+07 1 3.2e+07 ! 03 3 8.50788e+09 3.2e+07 1 3.2e+07 ! 04 4 8.53988e+09 3.2e+07 1 3.2e+07 ! 05 5 8.60388e+09 3.2e+07 1 3.2e+07 ! 06 6 8.63588e+09 3.2e+07 1 3.2e+07 ! 07 7 8.69988e+09 3.2e+07 1 3.2e+07 ! 08 8 8.73188e+09 3.2e+07 1 3.2e+07 ! 09 9 8.79588e+09 3.2e+07 1 3.2e+07 ! 10 10 8.82788e+09 3.2e+07 1 3.2e+07 ! 11 11 8.85988e+09 3.2e+07 1 3.2e+07 ! 12 12 8.89188e+09 3.2e+07 1 3.2e+07 ! ! Polarization(s): RR ! ! Read 344 lines of history. ! ! Reading 24264 visibilities. select I ! Polarization I is unavailable. ! Selecting polarization: RR, channels: 1..12 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 ! Reading IF 5 channels: 5..5 ! Reading IF 6 channels: 6..6 ! Reading IF 7 channels: 7..7 ! Reading IF 8 channels: 8..8 ! Reading IF 9 channels: 9..9 ! Reading IF 10 channels: 10..10 ! Reading IF 11 channels: 11..11 ! Reading IF 12 channels: 12..12 print "field_size =",field_size ! field_size = 512 print "field_cell =",field_cell ! field_cell = 0.2 print "taper_size =",taper_size ! taper_size = 70 ![@muppet J1522-2730_X_2014_05_31_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 = 512x512 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 50 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 50 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 50 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 50 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 5. ! A total of 50 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 6. ! A total of 50 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 7. ! A total of 50 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 8. ! A total of 50 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 9. ! A total of 50 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 10. ! A total of 50 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 11. ! A total of 50 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 12. ! A total of 50 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.375662Jy sigma=0.003588 ! Fit after self-cal, rms=0.337997Jy sigma=0.003163 ! 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 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.5886 mas, bmaj=1.643 mas, bpa=-1.017 degrees ! Estimated noise=890.624 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 = 0.770149 Jy ! Component: 100 - total flux cleaned = 0.988266 Jy ! Total flux subtracted in 100 components = 0.988266 Jy ! Clean residual min=-0.056493 max=0.107184 Jy/beam ! Clean residual mean=-0.000305 rms=0.014158 Jy/beam ! Combined flux in latest and established models = 0.988266 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.988266 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.324897Jy sigma=0.003142 ! Fit after self-cal, rms=0.324748Jy sigma=0.003140 ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Added new window around map position (0.8, -1.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.118771 Jy ! Component: 100 - total flux cleaned = 0.190686 Jy ! Total flux subtracted in 100 components = 0.190686 Jy ! Clean residual min=-0.045586 max=0.081595 Jy/beam ! Clean residual mean=-0.000104 rms=0.010472 Jy/beam ! Combined flux in latest and established models = 1.17895 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 10 components and 1.17895 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.265431Jy sigma=0.002346 ! Fit after self-cal, rms=0.263772Jy sigma=0.002322 ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Added new window around map position (1.4, 0.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0661818 Jy ! Component: 100 - total flux cleaned = 0.103535 Jy ! Total flux subtracted in 100 components = 0.103535 Jy ! Clean residual min=-0.048114 max=0.057676 Jy/beam ! Clean residual mean=-0.000013 rms=0.009063 Jy/beam ! Combined flux in latest and established models = 1.28249 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 16 components and 1.28249 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.242709Jy sigma=0.002094 ! Fit after self-cal, rms=0.241172Jy sigma=0.002063 ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 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 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.7744 mas, bmaj=2.011 mas, bpa=-0.5373 degrees ! Estimated noise=462.569 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 = 0.0423878 Jy ! Component: 100 - total flux cleaned = 0.0660558 Jy ! Component: 150 - total flux cleaned = 0.0774392 Jy ! Component: 200 - total flux cleaned = 0.0797149 Jy ! Total flux subtracted in 200 components = 0.0797149 Jy ! Clean residual min=-0.060261 max=0.052471 Jy/beam ! Clean residual mean=0.000128 rms=0.011557 Jy/beam ! Combined flux in latest and established models = 1.3622 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 31 components and 1.3622 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.232943Jy sigma=0.001984 ! Fit after self-cal, rms=0.232954Jy sigma=0.001977 ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.90 FD 1.09 HN 1.31 KP 0.92 ! LA 1.03 MK 0.99 NL 1.01 OV 0.97 ! PT 1.00 SC 0.99 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.90 FD 1.09 HN 1.34 KP 0.87 ! LA 1.04 MK 0.99 NL 1.01 OV 0.96 ! PT 0.95 SC 1.00 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.90 FD 1.10 HN 1.34 KP 0.82 ! LA 1.06 MK 1.00 NL 1.01 OV 0.97 ! PT 0.92 SC 0.99 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.90 FD 1.08 HN 1.33 KP 0.79 ! LA 1.07 MK 1.00 NL 1.01 OV 0.96 ! PT 0.93 SC 0.99 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 0.91 FD 1.09 HN 1.25 KP 0.75 ! LA 1.06 MK 1.03 NL 1.03 OV 0.98 ! PT 0.94 SC 0.99 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 0.93 FD 1.12 HN 1.32 KP 0.75 ! LA 1.07 MK 1.02 NL 1.03 OV 1.00 ! PT 0.94 SC 0.99 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 1.21 HN 1.48 KP 0.80 ! LA 1.14 MK 1.07 NL 1.08 OV 1.05 ! PT 1.02 SC 1.06 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 0.90 FD 1.14 HN 1.41 KP 0.75 ! LA 1.06 MK 1.02 NL 1.04 OV 1.01 ! PT 0.94 SC 1.01 ! ! ! Correcting IF 9. ! Telescope amplitude corrections in sub-array 1: ! BR 0.92 FD 1.11 HN 1.41 KP 0.77 ! LA 1.07 MK 1.02 NL 1.03 OV 1.02 ! PT 0.96 SC 0.99 ! ! ! Correcting IF 10. ! Telescope amplitude corrections in sub-array 1: ! BR 0.92 FD 1.11 HN 1.36 KP 0.80 ! LA 1.09 MK 1.04 NL 1.05 OV 1.01 ! PT 0.95 SC 0.97 ! ! ! Correcting IF 11. ! Telescope amplitude corrections in sub-array 1: ! BR 0.91 FD 1.12 HN 1.37 KP 0.83 ! LA 1.09 MK 1.06 NL 1.05 OV 0.99 ! PT 0.97 SC 1.01 ! ! ! Correcting IF 12. ! Telescope amplitude corrections in sub-array 1: ! BR 0.91 FD 1.12 HN 1.36 KP 0.87 ! LA 1.08 MK 1.04 NL 1.04 OV 1.00 ! PT 0.99 SC 1.01 ! ! ! Fit before self-cal, rms=0.232954Jy sigma=0.001977 ! Fit after self-cal, rms=0.157639Jy sigma=0.001122 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.7847 mas, bmaj=2.007 mas, bpa=0.0578 degrees ! Estimated noise=469.764 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 = -0.0208244 Jy ! Component: 100 - total flux cleaned = -0.0225175 Jy ! Component: 150 - total flux cleaned = -0.0229729 Jy ! Component: 200 - total flux cleaned = -0.0233677 Jy ! Total flux subtracted in 200 components = -0.0233677 Jy ! Clean residual min=-0.028343 max=0.019185 Jy/beam ! Clean residual mean=-0.000058 rms=0.004591 Jy/beam ! Combined flux in latest and established models = 1.33883 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 47 components and 1.33883 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.152264Jy sigma=0.001069 ! Fit after self-cal, rms=0.150734Jy sigma=0.001060 ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 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. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.150734Jy sigma=0.001060 ! Fit after self-cal, rms=0.132994Jy sigma=0.000938 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.7865 mas, bmaj=2.008 mas, bpa=0.04846 degrees ! Estimated noise=471.589 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0154657 Jy ! Component: 100 - total flux cleaned = -0.0158697 Jy ! Component: 150 - total flux cleaned = -0.0165805 Jy ! Component: 200 - total flux cleaned = -0.0174698 Jy ! Total flux subtracted in 200 components = -0.0174698 Jy ! Clean residual min=-0.018516 max=0.011483 Jy/beam ! Clean residual mean=-0.000050 rms=0.002838 Jy/beam ! Combined flux in latest and established models = 1.32136 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 58 components and 1.32136 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.128787Jy sigma=0.000901 ! Fit after self-cal, rms=0.127239Jy sigma=0.000892 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 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 = -0.00707043 Jy ! Component: 100 - total flux cleaned = -0.00761406 Jy ! Component: 150 - total flux cleaned = -0.00783772 Jy ! Component: 200 - total flux cleaned = -0.00860686 Jy ! Total flux subtracted in 200 components = -0.00860686 Jy ! Clean residual min=-0.015534 max=0.011712 Jy/beam ! Clean residual mean=-0.000068 rms=0.002614 Jy/beam ! Combined flux in latest and established models = 1.31276 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 67 components and 1.31276 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.125956Jy sigma=0.000877 ! Fit after self-cal, rms=0.125303Jy sigma=0.000875 ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 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. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.125303Jy sigma=0.000875 ! Fit after self-cal, rms=0.122902Jy sigma=0.000841 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.7876 mas, bmaj=2.008 mas, bpa=0.04774 degrees ! Estimated noise=471.481 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0100436 Jy ! Component: 100 - total flux cleaned = -0.010541 Jy ! Component: 150 - total flux cleaned = -0.0111448 Jy ! Component: 200 - total flux cleaned = -0.0116925 Jy ! Total flux subtracted in 200 components = -0.0116925 Jy ! Clean residual min=-0.009833 max=0.005863 Jy/beam ! Clean residual mean=-0.000056 rms=0.001776 Jy/beam ! Combined flux in latest and established models = 1.30107 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 70 components and 1.30107 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.121087Jy sigma=0.000828 ! Fit after self-cal, rms=0.120442Jy sigma=0.000825 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 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 = -0.0038636 Jy ! Component: 100 - total flux cleaned = -0.00403772 Jy ! Component: 150 - total flux cleaned = -0.00432385 Jy ! Component: 200 - total flux cleaned = -0.00471184 Jy ! Total flux subtracted in 200 components = -0.00471184 Jy ! Clean residual min=-0.008170 max=0.006932 Jy/beam ! Clean residual mean=-0.000067 rms=0.001660 Jy/beam ! Combined flux in latest and established models = 1.29635 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 76 components and 1.29635 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.119740Jy sigma=0.000820 ! Fit after self-cal, rms=0.119447Jy sigma=0.000818 ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Added new window around map position (-1.4, -1.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00605558 Jy ! Component: 100 - total flux cleaned = 0.00710587 Jy ! Component: 150 - total flux cleaned = 0.00678044 Jy ! Component: 200 - total flux cleaned = 0.00649765 Jy ! Total flux subtracted in 200 components = 0.00649765 Jy ! Clean residual min=-0.007647 max=0.005305 Jy/beam ! Clean residual mean=-0.000055 rms=0.001478 Jy/beam ! Combined flux in latest and established models = 1.30285 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 98 components and 1.30285 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.118419Jy sigma=0.000811 ! Fit after self-cal, rms=0.118083Jy sigma=0.000810 ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 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. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.118083Jy sigma=0.000810 ! Fit after self-cal, rms=0.118822Jy sigma=0.000806 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=2.241 mas, bmaj=5.717 mas, bpa=4.981 degrees ! Estimated noise=584.387 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00441364 Jy ! Component: 100 - total flux cleaned = -0.00448577 Jy ! Component: 150 - total flux cleaned = -0.00475855 Jy ! Component: 200 - total flux cleaned = -0.00499912 Jy ! Total flux subtracted in 200 components = -0.00499912 Jy ! Clean residual min=-0.005598 max=0.005349 Jy/beam ! Clean residual mean=-0.000090 rms=0.001661 Jy/beam ! Combined flux in latest and established models = 1.29785 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 111 components and 1.29785 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.118450Jy sigma=0.000805 ! Fit after self-cal, rms=0.118264Jy sigma=0.000804 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 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 = -0.000527913 Jy ! Component: 100 - total flux cleaned = -0.000383584 Jy ! Component: 150 - total flux cleaned = -0.000331263 Jy ! Component: 200 - total flux cleaned = -0.000292419 Jy ! Total flux subtracted in 200 components = -0.000292419 Jy ! Clean residual min=-0.004831 max=0.005228 Jy/beam ! Clean residual mean=-0.000092 rms=0.001600 Jy/beam ! Combined flux in latest and established models = 1.29756 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 124 components and 1.29756 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.118108Jy sigma=0.000803 ! Fit after self-cal, rms=0.118011Jy sigma=0.000803 ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 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 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.7875 mas, bmaj=2.006 mas, bpa=0.01878 degrees ! Estimated noise=471.231 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7875 x 2.006 at 0.01878 degrees (North through East) ! Clean map min=-0.0079254 max=1.0433 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. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.118011Jy sigma=0.000803 ! Fit after self-cal, rms=0.113011Jy sigma=0.000743 ! Inverting map and beam ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.7877 mas, bmaj=2.007 mas, bpa=0.0554 degrees ! Estimated noise=470.505 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00430079 Jy ! Component: 100 - total flux cleaned = -0.00486947 Jy ! Component: 150 - total flux cleaned = -0.00538314 Jy ! Component: 200 - total flux cleaned = -0.00562016 Jy ! Total flux subtracted in 200 components = -0.00562016 Jy ! Clean residual min=-0.005050 max=0.004680 Jy/beam ! Clean residual mean=-0.000023 rms=0.001050 Jy/beam ! Combined flux in latest and established models = 1.29194 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 128 components and 1.29194 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.112398Jy sigma=0.000738 ! Fit after self-cal, rms=0.112269Jy sigma=0.000738 ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000964507 Jy ! Component: 100 - total flux cleaned = -0.000741801 Jy ! Component: 150 - total flux cleaned = -0.000737176 Jy ! Component: 200 - total flux cleaned = -0.000741174 Jy ! Total flux subtracted in 200 components = -0.000741174 Jy ! Clean residual min=-0.004485 max=0.004581 Jy/beam ! Clean residual mean=-0.000025 rms=0.000998 Jy/beam ! Combined flux in latest and established models = 1.2912 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 130 components and 1.2912 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.111965Jy sigma=0.000735 ! Fit after self-cal, rms=0.111884Jy sigma=0.000735 ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Added new window around map position (5.8, -22.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00227348 Jy ! Component: 100 - total flux cleaned = 0.00279509 Jy ! Component: 150 - total flux cleaned = 0.00297773 Jy ! Component: 200 - total flux cleaned = 0.00298091 Jy ! Total flux subtracted in 200 components = 0.00298091 Jy ! Clean residual min=-0.004008 max=0.003732 Jy/beam ! Clean residual mean=-0.000022 rms=0.000911 Jy/beam ! Combined flux in latest and established models = 1.29418 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 137 components and 1.29418 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.111603Jy sigma=0.000733 ! Fit after self-cal, rms=0.111557Jy sigma=0.000733 ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.111557Jy sigma=0.000733 ! Fit after self-cal, rms=0.112206Jy sigma=0.000732 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 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.5957 mas, bmaj=1.625 mas, bpa=-0.2118 degrees ! Estimated noise=917.87 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.793475 Jy ! Component: 100 - total flux cleaned = 1.01069 Jy ! Component: 150 - total flux cleaned = 1.12039 Jy ! Component: 200 - total flux cleaned = 1.18136 Jy ! Total flux subtracted in 200 components = 1.18136 Jy ! Clean residual min=-0.017765 max=0.030679 Jy/beam ! Clean residual mean=-0.000114 rms=0.003941 Jy/beam ! Combined flux in latest and established models = 1.18136 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 14 model components to the UV plane model. ! The established model now contains 14 components and 1.18136 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.7879 mas, bmaj=2.006 mas, bpa=0.05884 degrees ! Estimated noise=470.254 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 = 0.0472 Jy ! Component: 100 - total flux cleaned = 0.0720426 Jy ! Component: 150 - total flux cleaned = 0.0865565 Jy ! Component: 200 - total flux cleaned = 0.0957712 Jy ! Total flux subtracted in 200 components = 0.0957712 Jy ! Clean residual min=-0.006488 max=0.006119 Jy/beam ! Clean residual mean=-0.000050 rms=0.001329 Jy/beam ! Combined flux in latest and established models = 1.27713 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 35 components and 1.27713 Jy ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 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 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=2.246 mas, bmaj=5.725 mas, bpa=4.981 degrees ! Estimated noise=582.233 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00646239 Jy ! Component: 100 - total flux cleaned = 0.0100119 Jy ! Component: 150 - total flux cleaned = 0.0120271 Jy ! Component: 200 - total flux cleaned = 0.0123669 Jy ! Total flux subtracted in 200 components = 0.0123669 Jy ! Clean residual min=-0.004256 max=0.003377 Jy/beam ! Clean residual mean=-0.000048 rms=0.001175 Jy/beam ! Combined flux in latest and established models = 1.2895 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 = 0.000235328 Jy ! Component: 100 - total flux cleaned = 0.000391359 Jy ! Component: 150 - total flux cleaned = 0.000439503 Jy ! Component: 200 - total flux cleaned = 0.000489238 Jy ! Total flux subtracted in 200 components = 0.000489238 Jy ! Clean residual min=-0.004098 max=0.003460 Jy/beam ! Clean residual mean=-0.000047 rms=0.001147 Jy/beam ! Combined flux in latest and established models = 1.28999 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 59 components and 1.28999 Jy ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.7879 mas, bmaj=2.006 mas, bpa=0.05884 degrees ! Estimated noise=470.254 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00163205 Jy ! Component: 100 - total flux cleaned = -0.00183278 Jy ! Component: 150 - total flux cleaned = -0.00182789 Jy ! Component: 200 - total flux cleaned = -0.00182647 Jy ! Total flux subtracted in 200 components = -0.00182647 Jy ! Clean residual min=-0.004967 max=0.003900 Jy/beam ! Clean residual mean=-0.000027 rms=0.001051 Jy/beam ! Combined flux in latest and established models = 1.28816 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 69 components and 1.28816 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.113192Jy sigma=0.000744 ! Fit after self-cal, rms=0.112725Jy sigma=0.000740 wmodel J1522-2730_X_2014_05_31_pus_map.mod ! Writing 69 model components to file: J1522-2730_X_2014_05_31_pus_map.mod wobs J1522-2730_X_2014_05_31_pus_uvs.fits ! Writing UV FITS file: J1522-2730_X_2014_05_31_pus_uvs.fits wwins J1522-2730_X_2014_05_31_pus_map.win ! wwins: Wrote 5 windows to J1522-2730_X_2014_05_31_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 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00102599 Jy ! Component: 100 - total flux cleaned = -0.00185129 Jy ! Component: 150 - total flux cleaned = -0.00226735 Jy ! Component: 200 - total flux cleaned = -0.00285503 Jy ! Component: 250 - total flux cleaned = -0.00372963 Jy ! Component: 300 - total flux cleaned = -0.00445279 Jy ! Component: 350 - total flux cleaned = -0.00474561 Jy ! Component: 400 - total flux cleaned = -0.00491676 Jy ! Component: 450 - total flux cleaned = -0.00491564 Jy ! Component: 500 - total flux cleaned = -0.00502431 Jy ! Component: 550 - total flux cleaned = -0.00502369 Jy ! Component: 600 - total flux cleaned = -0.00507565 Jy ! Component: 650 - total flux cleaned = -0.00522843 Jy ! Component: 700 - total flux cleaned = -0.00542755 Jy ! Component: 750 - total flux cleaned = -0.00552589 Jy ! Component: 800 - total flux cleaned = -0.0057201 Jy ! Component: 850 - total flux cleaned = -0.00591121 Jy ! Component: 900 - total flux cleaned = -0.00605177 Jy ! Component: 950 - total flux cleaned = -0.00619073 Jy ! Component: 1000 - total flux cleaned = -0.00641867 Jy ! Component: 1050 - total flux cleaned = -0.00655352 Jy ! Component: 1100 - total flux cleaned = -0.0067303 Jy ! Component: 1150 - total flux cleaned = -0.00694776 Jy ! Component: 1200 - total flux cleaned = -0.00707638 Jy ! Component: 1250 - total flux cleaned = -0.00716072 Jy ! Component: 1300 - total flux cleaned = -0.0072448 Jy ! Component: 1350 - total flux cleaned = -0.0074509 Jy ! Component: 1400 - total flux cleaned = -0.00745138 Jy ! Component: 1450 - total flux cleaned = -0.00765158 Jy ! Component: 1500 - total flux cleaned = -0.00784827 Jy ! Component: 1550 - total flux cleaned = -0.00788724 Jy ! Component: 1600 - total flux cleaned = -0.00811753 Jy ! Component: 1650 - total flux cleaned = -0.008079 Jy ! Component: 1700 - total flux cleaned = -0.00811723 Jy ! Component: 1750 - total flux cleaned = -0.00822802 Jy ! Component: 1800 - total flux cleaned = -0.00826463 Jy ! Component: 1850 - total flux cleaned = -0.00830083 Jy ! Component: 1900 - total flux cleaned = -0.00833693 Jy ! Component: 1950 - total flux cleaned = -0.00837252 Jy ! Component: 2000 - total flux cleaned = -0.00826723 Jy ! Total flux subtracted in 2048 components = -0.00830228 Jy ! Clean residual min=-0.001826 max=0.001728 Jy/beam ! Clean residual mean=-0.000019 rms=0.000619 Jy/beam ! Combined flux in latest and established models = 1.27986 Jy keep ! Adding 126 model components to the UV plane model. ! The established model now contains 190 components and 1.27986 Jy ![Exited script file: muppet] wmap "J1522-2730_X_2014_05_31_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7879 x 2.006 at 0.05884 degrees (North through East) ! Clean map min=-0.0026818 max=1.0664 Jy/beam ! Writing clean map to FITS file: J1522-2730_X_2014_05_31_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 1.06641 invert ! Inverting map ! Your choice of large map pixels excluded 0.0742% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000616647 device "J1522-2730_X_2014_05_31_pus\_map.eps/VPS" ! Attempting to open device: 'J1522-2730_X_2014_05_31_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.173473 0.173473 0.346946 0.693893 1.38779 2.77557 5.55114 11.1023 22.2046 44.4091 88.8183 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0018 print "peak=",int(1000*peak_flux)/1000 ! peak= 1.066 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7879 x 2.006 at 0.05884 degrees (North through East) ! Clean map min=-0.0026818 max=1.0664 Jy/beam quit ! Quitting program ! Log file J1522-2730_X_2014_05_31_pus_uvs.log closed on Sun Nov 27 18:08:48 2016