! Started logfile: J1147-3812_X_2017_02_24_pus_uvs.log on Sat May 4 10:02:16 2019 obs J1147-3812_X_2017_02_24_pus_uva.fits ! Reading UV FITS file: J1147-3812_X_2017_02_24_pus_uva.fits ! AN table 1: 24 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.617593 visibilities/baseline/integration-bin. ! Found source: J1147-3812 ! ! 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 1882 lines of history. ! ! Reading 8004 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 J1147-3812_X_2017_02_24_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 53 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 53 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 53 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 53 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 5. ! A total of 53 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 6. ! A total of 53 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 7. ! A total of 53 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 8. ! A total of 53 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 9. ! A total of 53 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 10. ! A total of 53 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 11. ! A total of 53 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 12. ! A total of 53 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.287450Jy sigma=0.001885 ! Fit after self-cal, rms=0.273005Jy sigma=0.001796 ! 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 0.0875% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=0.6126 mas, bmaj=1.84 mas, bpa=8.924 degrees ! Estimated noise=1868.89 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 = 0.761333 Jy ! Component: 100 - total flux cleaned = 0.979218 Jy ! Total flux subtracted in 100 components = 0.979218 Jy ! Clean residual min=-0.055093 max=0.095950 Jy/beam ! Clean residual mean=-0.000145 rms=0.012875 Jy/beam ! Combined flux in latest and established models = 0.979218 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.979218 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=0.258425Jy sigma=0.001742 ! Fit after self-cal, rms=0.258145Jy sigma=0.001741 ! Inverting map ! Your choice of large map pixels excluded 0.0875% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.106246 Jy ! Component: 100 - total flux cleaned = 0.164278 Jy ! Total flux subtracted in 100 components = 0.164278 Jy ! Clean residual min=-0.035554 max=0.055375 Jy/beam ! Clean residual mean=-0.000023 rms=0.008453 Jy/beam ! Combined flux in latest and established models = 1.1435 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 10 components and 1.1435 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=0.199067Jy sigma=0.001195 ! Fit after self-cal, rms=0.198996Jy sigma=0.001193 ! Inverting map ! Your choice of large map pixels excluded 0.0875% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Added new window around map position (1, -2.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0513662 Jy ! Component: 100 - total flux cleaned = 0.0842795 Jy ! Total flux subtracted in 100 components = 0.0842795 Jy ! Clean residual min=-0.030414 max=0.043170 Jy/beam ! Clean residual mean=0.000033 rms=0.007163 Jy/beam ! Combined flux in latest and established models = 1.22778 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 18 components and 1.22778 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=0.178782Jy sigma=0.001033 ! Fit after self-cal, rms=0.177588Jy sigma=0.001023 ! Inverting map ! Your choice of large map pixels excluded 0.0875% of the data. ! The x-axis pixel size should ideally be below 0.1994 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 0.0875% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=0.8071 mas, bmaj=2.295 mas, bpa=8.261 degrees ! Estimated noise=1245.99 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 = 0.0413476 Jy ! Component: 100 - total flux cleaned = 0.0644463 Jy ! Component: 150 - total flux cleaned = 0.078472 Jy ! Component: 200 - total flux cleaned = 0.0828184 Jy ! Total flux subtracted in 200 components = 0.0828184 Jy ! Clean residual min=-0.021958 max=0.029589 Jy/beam ! Clean residual mean=0.000027 rms=0.006759 Jy/beam ! Combined flux in latest and established models = 1.31059 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 34 components and 1.31059 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=0.168705Jy sigma=0.000940 ! Fit after self-cal, rms=0.168249Jy sigma=0.000934 ! Inverting map ! Your choice of large map pixels excluded 0.0875% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.19 FD 0.98 HN 1.39 KP 0.99 ! LA 1.01 MK 0.97 NL 1.07 OV 0.94 ! PT 0.95 SC 1.02 ! ! ! Correcting IF 2. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.19 FD 0.99 HN 1.41 KP 0.97 ! LA 1.02 MK 0.97 NL 1.05 OV 0.94 ! PT 0.96 SC 1.02 ! ! ! Correcting IF 3. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.19 FD 0.98 HN 1.33 KP 0.97 ! LA 1.00 MK 1.01 NL 1.07 OV 0.95 ! PT 0.95 SC 1.02 ! ! ! Correcting IF 4. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.20 FD 0.96 HN 1.33 KP 0.97 ! LA 1.00 MK 1.00 NL 1.07 OV 0.95 ! PT 0.95 SC 1.03 ! ! ! Correcting IF 5. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.22 FD 0.97 HN 1.34 KP 0.96 ! LA 0.98 MK 1.01 NL 1.05 OV 0.95 ! PT 0.95 SC 1.01 ! ! ! Correcting IF 6. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.21 FD 0.97 HN 1.41 KP 0.95 ! LA 1.03 MK 0.99 NL 1.07 OV 0.94 ! PT 0.94 SC 1.02 ! ! ! Correcting IF 7. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.20 FD 0.99 HN 1.23 KP 0.95 ! LA 1.00 MK 1.01 NL 1.10 OV 0.95 ! PT 0.96 SC 1.00 ! ! ! Correcting IF 8. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.19 FD 0.96 HN 1.31 KP 0.94 ! LA 1.03 MK 1.00 NL 1.08 OV 0.95 ! PT 0.94 SC 1.02 ! ! ! Correcting IF 9. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.23 FD 0.99 HN 1.39 KP 0.96 ! LA 1.00 MK 1.00 NL 1.07 OV 0.94 ! PT 0.95 SC 0.96 ! ! ! Correcting IF 10. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.20 FD 0.98 HN 1.38 KP 0.97 ! LA 1.00 MK 1.01 NL 1.10 OV 0.94 ! PT 0.94 SC 0.95 ! ! ! Correcting IF 11. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.27 FD 1.00 HN 1.33 KP 0.95 ! LA 0.99 MK 1.02 NL 1.08 OV 0.93 ! PT 0.95 SC 0.98 ! ! ! Correcting IF 12. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.25 FD 0.98 HN 1.34 KP 1.01 ! LA 0.99 MK 1.00 NL 1.06 OV 0.94 ! PT 0.96 SC 0.98 ! ! ! Fit before self-cal, rms=0.168249Jy sigma=0.000934 ! Fit after self-cal, rms=0.143046Jy sigma=0.000721 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=0.8073 mas, bmaj=2.297 mas, bpa=8.142 degrees ! Estimated noise=1258.23 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 = -0.0078521 Jy ! Component: 100 - total flux cleaned = -0.010553 Jy ! Component: 150 - total flux cleaned = -0.0120703 Jy ! Component: 200 - total flux cleaned = -0.0128698 Jy ! Total flux subtracted in 200 components = -0.0128698 Jy ! Clean residual min=-0.012556 max=0.011397 Jy/beam ! Clean residual mean=-0.000111 rms=0.002786 Jy/beam ! Combined flux in latest and established models = 1.29772 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 44 components and 1.29772 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=0.140818Jy sigma=0.000709 ! Fit after self-cal, rms=0.140954Jy sigma=0.000708 ! Inverting map ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 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=0.140954Jy sigma=0.000708 ! Fit after self-cal, rms=0.140190Jy sigma=0.000694 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=0.8076 mas, bmaj=2.297 mas, bpa=8.109 degrees ! Estimated noise=1257.28 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00539681 Jy ! Component: 100 - total flux cleaned = -0.0070644 Jy ! Component: 150 - total flux cleaned = -0.00825961 Jy ! Component: 200 - total flux cleaned = -0.00890339 Jy ! Total flux subtracted in 200 components = -0.00890339 Jy ! Clean residual min=-0.008786 max=0.010782 Jy/beam ! Clean residual mean=-0.000137 rms=0.002241 Jy/beam ! Combined flux in latest and established models = 1.28882 Jy selfcal ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 52 components and 1.28882 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=0.138937Jy sigma=0.000688 ! Fit after self-cal, rms=0.138920Jy sigma=0.000688 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 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) ! Added new window around map position (3.4, -3). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00726987 Jy ! Component: 100 - total flux cleaned = 0.00730861 Jy ! Component: 150 - total flux cleaned = 0.00685396 Jy ! Component: 200 - total flux cleaned = 0.00624256 Jy ! Total flux subtracted in 200 components = 0.00624256 Jy ! Clean residual min=-0.007505 max=0.006874 Jy/beam ! Clean residual mean=-0.000135 rms=0.001908 Jy/beam ! Combined flux in latest and established models = 1.29506 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 65 components and 1.29506 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=0.137752Jy sigma=0.000679 ! Fit after self-cal, rms=0.137764Jy sigma=0.000679 ! Inverting map ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 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=0.137764Jy sigma=0.000679 ! Fit after self-cal, rms=0.136778Jy sigma=0.000664 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=0.8073 mas, bmaj=2.298 mas, bpa=8.094 degrees ! Estimated noise=1255.65 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00367746 Jy ! Component: 100 - total flux cleaned = -0.00429911 Jy ! Component: 150 - total flux cleaned = -0.00484673 Jy ! Component: 200 - total flux cleaned = -0.00518926 Jy ! Total flux subtracted in 200 components = -0.00518926 Jy ! Clean residual min=-0.007210 max=0.005445 Jy/beam ! Clean residual mean=-0.000009 rms=0.001417 Jy/beam ! Combined flux in latest and established models = 1.28987 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 68 components and 1.28987 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=0.136026Jy sigma=0.000660 ! Fit after self-cal, rms=0.136031Jy sigma=0.000660 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 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 = -0.000709753 Jy ! Component: 100 - total flux cleaned = -0.00131391 Jy ! Component: 150 - total flux cleaned = -0.00158735 Jy ! Component: 200 - total flux cleaned = -0.0017161 Jy ! Total flux subtracted in 200 components = -0.0017161 Jy ! Clean residual min=-0.006663 max=0.005343 Jy/beam ! Clean residual mean=-0.000012 rms=0.001327 Jy/beam ! Combined flux in latest and established models = 1.28816 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 70 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=0.135644Jy sigma=0.000658 ! Fit after self-cal, rms=0.135659Jy sigma=0.000658 ! Inverting map ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 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=0.135659Jy sigma=0.000658 ! Fit after self-cal, rms=0.136183Jy sigma=0.000658 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=2.409 mas, bmaj=8.331 mas, bpa=7.22 degrees ! Estimated noise=1605.49 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00344626 Jy ! Component: 100 - total flux cleaned = -0.0036539 Jy ! Component: 150 - total flux cleaned = -0.00393175 Jy ! Component: 200 - total flux cleaned = -0.0040996 Jy ! Total flux subtracted in 200 components = -0.0040996 Jy ! Clean residual min=-0.006106 max=0.004929 Jy/beam ! Clean residual mean=-0.000024 rms=0.001587 Jy/beam ! Combined flux in latest and established models = 1.28406 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 75 components and 1.28406 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=0.135948Jy sigma=0.000657 ! Fit after self-cal, rms=0.135944Jy sigma=0.000657 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 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 = -1.15252e-05 Jy ! Component: 100 - total flux cleaned = -1.38502e-05 Jy ! Component: 150 - total flux cleaned = -8.19369e-05 Jy ! Component: 200 - total flux cleaned = -8.21911e-05 Jy ! Total flux subtracted in 200 components = -8.21911e-05 Jy ! Clean residual min=-0.006129 max=0.004906 Jy/beam ! Clean residual mean=-0.000025 rms=0.001556 Jy/beam ! Combined flux in latest and established models = 1.28398 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 79 components and 1.28398 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=0.135854Jy sigma=0.000656 ! Fit after self-cal, rms=0.135870Jy sigma=0.000656 ! Inverting map ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 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 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=0.8072 mas, bmaj=2.297 mas, bpa=8.077 degrees ! Estimated noise=1254.42 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8072 x 2.297 at 8.077 degrees (North through East) ! Clean map min=-0.0060057 max=1.0166 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=0.135870Jy sigma=0.000656 ! Fit after self-cal, rms=0.128634Jy sigma=0.000605 ! Inverting map and beam ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=0.8069 mas, bmaj=2.295 mas, bpa=8.012 degrees ! Estimated noise=1252.44 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00148228 Jy ! Component: 100 - total flux cleaned = -0.00148542 Jy ! Component: 150 - total flux cleaned = -0.00160264 Jy ! Component: 200 - total flux cleaned = -0.00171015 Jy ! Total flux subtracted in 200 components = -0.00171015 Jy ! Clean residual min=-0.005462 max=0.004252 Jy/beam ! Clean residual mean=-0.000009 rms=0.001141 Jy/beam ! Combined flux in latest and established models = 1.28227 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 84 components and 1.28227 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=0.128322Jy sigma=0.000603 ! Fit after self-cal, rms=0.128327Jy sigma=0.000603 ! Inverting map ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00049645 Jy ! Component: 100 - total flux cleaned = -0.000694598 Jy ! Component: 150 - total flux cleaned = -0.000788691 Jy ! Component: 200 - total flux cleaned = -0.000787728 Jy ! Total flux subtracted in 200 components = -0.000787728 Jy ! Clean residual min=-0.005124 max=0.004135 Jy/beam ! Clean residual mean=-0.000010 rms=0.001098 Jy/beam ! Combined flux in latest and established models = 1.28148 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 91 components and 1.28148 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=0.128144Jy sigma=0.000602 ! Fit after self-cal, rms=0.128152Jy sigma=0.000602 ! Inverting map ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 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=0.128152Jy sigma=0.000602 ! Fit after self-cal, rms=0.128408Jy sigma=0.000602 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 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=0.6104 mas, bmaj=1.838 mas, bpa=8.771 degrees ! Estimated noise=1889.54 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.768162 Jy ! Component: 100 - total flux cleaned = 0.99107 Jy ! Component: 150 - total flux cleaned = 1.09848 Jy ! Component: 200 - total flux cleaned = 1.15517 Jy ! Total flux subtracted in 200 components = 1.15517 Jy ! Clean residual min=-0.019829 max=0.029075 Jy/beam ! Clean residual mean=-0.000067 rms=0.004277 Jy/beam ! Combined flux in latest and established models = 1.15517 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 12 model components to the UV plane model. ! The established model now contains 12 components and 1.15517 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=0.8068 mas, bmaj=2.295 mas, bpa=8.011 degrees ! Estimated noise=1251.35 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 = 0.0469543 Jy ! Component: 100 - total flux cleaned = 0.0734875 Jy ! Component: 150 - total flux cleaned = 0.089456 Jy ! Component: 200 - total flux cleaned = 0.100005 Jy ! Total flux subtracted in 200 components = 0.100005 Jy ! Clean residual min=-0.006351 max=0.009667 Jy/beam ! Clean residual mean=-0.000034 rms=0.001761 Jy/beam ! Combined flux in latest and established models = 1.25518 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 32 components and 1.25518 Jy ! Inverting map ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Added new window around map position (1.2, -5.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00934929 Jy ! Component: 100 - total flux cleaned = 0.0136673 Jy ! Component: 150 - total flux cleaned = 0.0151736 Jy ! Component: 200 - total flux cleaned = 0.0158253 Jy ! Total flux subtracted in 200 components = 0.0158253 Jy ! Clean residual min=-0.004837 max=0.007311 Jy/beam ! Clean residual mean=-0.000018 rms=0.001326 Jy/beam ! Combined flux in latest and established models = 1.271 Jy ! Adding 20 model components to the UV plane model. ! The established model now contains 46 components and 1.271 Jy ! Inverting map ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Added new window around map position (-1.8, 0.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00446243 Jy ! Component: 100 - total flux cleaned = 0.00513602 Jy ! Component: 150 - total flux cleaned = 0.00528827 Jy ! Component: 200 - total flux cleaned = 0.00556471 Jy ! Total flux subtracted in 200 components = 0.00556471 Jy ! Clean residual min=-0.004565 max=0.004607 Jy/beam ! Clean residual mean=-0.000011 rms=0.001145 Jy/beam ! Combined flux in latest and established models = 1.27657 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 63 components and 1.27657 Jy ! Inverting map ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 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 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=2.41 mas, bmaj=8.328 mas, bpa=7.176 degrees ! Estimated noise=1602.34 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0028456 Jy ! Component: 100 - total flux cleaned = 0.00334399 Jy ! Component: 150 - total flux cleaned = 0.00362211 Jy ! Component: 200 - total flux cleaned = 0.00380546 Jy ! Total flux subtracted in 200 components = 0.00380546 Jy ! Clean residual min=-0.005529 max=0.004070 Jy/beam ! Clean residual mean=-0.000013 rms=0.001404 Jy/beam ! Combined flux in latest and established models = 1.28037 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 = 0.000113778 Jy ! Component: 100 - total flux cleaned = 0.000263401 Jy ! Component: 150 - total flux cleaned = 0.000350532 Jy ! Component: 200 - total flux cleaned = 0.000351607 Jy ! Total flux subtracted in 200 components = 0.000351607 Jy ! Clean residual min=-0.005508 max=0.004003 Jy/beam ! Clean residual mean=-0.000014 rms=0.001372 Jy/beam ! Combined flux in latest and established models = 1.28072 Jy ! Adding 19 model components to the UV plane model. ! The established model now contains 81 components and 1.28073 Jy ! Inverting map ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=0.8068 mas, bmaj=2.295 mas, bpa=8.011 degrees ! Estimated noise=1251.35 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00116945 Jy ! Component: 100 - total flux cleaned = -0.00141542 Jy ! Component: 150 - total flux cleaned = -0.00163279 Jy ! Component: 200 - total flux cleaned = -0.00163207 Jy ! Total flux subtracted in 200 components = -0.00163207 Jy ! Clean residual min=-0.004440 max=0.003867 Jy/beam ! Clean residual mean=-0.000011 rms=0.001026 Jy/beam ! Combined flux in latest and established models = 1.27909 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 95 components and 1.27909 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=0.128197Jy sigma=0.000602 ! Fit after self-cal, rms=0.128132Jy sigma=0.000601 wmodel J1147-3812_X_2017_02_24_pus_map.mod ! Writing 95 model components to file: J1147-3812_X_2017_02_24_pus_map.mod wobs J1147-3812_X_2017_02_24_pus_uvs.fits ! Writing UV FITS file: J1147-3812_X_2017_02_24_pus_uvs.fits wwins J1147-3812_X_2017_02_24_pus_map.win ! wwins: Wrote 5 windows to J1147-3812_X_2017_02_24_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 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000830029 Jy ! Component: 100 - total flux cleaned = -0.000766599 Jy ! Component: 150 - total flux cleaned = -0.00039917 Jy ! Component: 200 - total flux cleaned = 5.35525e-06 Jy ! Component: 250 - total flux cleaned = 0.000663489 Jy ! Component: 300 - total flux cleaned = 0.00108284 Jy ! Component: 350 - total flux cleaned = 0.0014901 Jy ! Component: 400 - total flux cleaned = 0.00168536 Jy ! Component: 450 - total flux cleaned = 0.00163738 Jy ! Component: 500 - total flux cleaned = 0.00159188 Jy ! Component: 550 - total flux cleaned = 0.00163817 Jy ! Component: 600 - total flux cleaned = 0.00163902 Jy ! Component: 650 - total flux cleaned = 0.0015518 Jy ! Component: 700 - total flux cleaned = 0.00168069 Jy ! Component: 750 - total flux cleaned = 0.00176408 Jy ! Component: 800 - total flux cleaned = 0.00188686 Jy ! Component: 850 - total flux cleaned = 0.0020886 Jy ! Component: 900 - total flux cleaned = 0.00220802 Jy ! Component: 950 - total flux cleaned = 0.00244307 Jy ! Component: 1000 - total flux cleaned = 0.00267351 Jy ! Component: 1050 - total flux cleaned = 0.00278719 Jy ! Component: 1100 - total flux cleaned = 0.00293687 Jy ! Component: 1150 - total flux cleaned = 0.00301064 Jy ! Component: 1200 - total flux cleaned = 0.00304709 Jy ! Component: 1250 - total flux cleaned = 0.00322586 Jy ! Component: 1300 - total flux cleaned = 0.00326052 Jy ! Component: 1350 - total flux cleaned = 0.00332958 Jy ! Component: 1400 - total flux cleaned = 0.00343226 Jy ! Component: 1450 - total flux cleaned = 0.00350031 Jy ! Component: 1500 - total flux cleaned = 0.00353412 Jy ! Component: 1550 - total flux cleaned = 0.00363394 Jy ! Component: 1600 - total flux cleaned = 0.0037983 Jy ! Component: 1650 - total flux cleaned = 0.00376551 Jy ! Component: 1700 - total flux cleaned = 0.00389381 Jy ! Component: 1750 - total flux cleaned = 0.00383059 Jy ! Component: 1800 - total flux cleaned = 0.00392471 Jy ! Component: 1850 - total flux cleaned = 0.00389363 Jy ! Component: 1900 - total flux cleaned = 0.00392491 Jy ! Component: 1950 - total flux cleaned = 0.0040167 Jy ! Component: 2000 - total flux cleaned = 0.00407727 Jy ! Total flux subtracted in 2048 components = 0.00416665 Jy ! Clean residual min=-0.001486 max=0.001659 Jy/beam ! Clean residual mean=-0.000005 rms=0.000566 Jy/beam ! Combined flux in latest and established models = 1.28326 Jy keep ! Adding 137 model components to the UV plane model. ! The established model now contains 232 components and 1.28326 Jy ![Exited script file: muppet] wmap "J1147-3812_X_2017_02_24_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8068 x 2.295 at 8.011 degrees (North through East) ! Clean map min=-0.0054407 max=1.0404 Jy/beam ! Writing clean map to FITS file: J1147-3812_X_2017_02_24_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 1.04044 invert ! Inverting map ! Your choice of large map pixels excluded 0.0879% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000561785 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.161985 0.161985 0.323969 0.647938 1.29588 2.59175 5.18351 10.367 20.734 41.468 82.9361 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0016 print "peak=",int(1000*peak_flux)/1000 ! peak= 1.04 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8068 x 2.295 at 8.011 degrees (North through East) ! Clean map min=-0.0054407 max=1.0404 Jy/beam ! Error occured in command: mapplot ! ! ! ! ! ! 4 consecutive EOF's on stdin - 10 will exit program ! ! 5 consecutive EOF's on stdin - 10 will exit program ! ! 6 consecutive EOF's on stdin - 10 will exit program ! ! 7 consecutive EOF's on stdin - 10 will exit program ! ! 8 consecutive EOF's on stdin - 10 will exit program ! ! 9 consecutive EOF's on stdin - 10 will exit program ! ! 10 consecutive EOF's on stdin - 10 will exit program ! Log file J1147-3812_X_2017_02_24_pus_uvs.log closed on Sat May 4 10:02:17 2019