! Started logfile: J1949+2421_X_2017_07_09_pus_uvs.log on Wed May 8 15:30:43 2019 obs J1949+2421_X_2017_07_09_pus_uva.fits ! Reading UV FITS file: J1949+2421_X_2017_07_09_pus_uva.fits ! AN table 1: 114 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.903899 visibilities/baseline/integration-bin. ! Found source: J1949+2421 ! ! 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 979 lines of history. ! ! Reading 55644 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 J1949+2421_X_2017_07_09_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 57 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 57 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 57 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 57 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 5. ! A total of 57 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 6. ! A total of 57 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 7. ! A total of 57 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 8. ! A total of 57 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 9. ! A total of 57 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 10. ! A total of 57 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 11. ! A total of 57 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 12. ! A total of 57 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.861088Jy sigma=0.007240 ! Fit after self-cal, rms=0.849003Jy sigma=0.007142 ! 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 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec ! Estimated beam: bmin=0.7172 mas, bmaj=1.476 mas, bpa=-5.004 degrees ! Estimated noise=714.848 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 = 0.108772 Jy ! Component: 100 - total flux cleaned = 0.14989 Jy ! Total flux subtracted in 100 components = 0.14989 Jy ! Clean residual min=-0.006495 max=0.021081 Jy/beam ! Clean residual mean=-0.000042 rms=0.002159 Jy/beam ! Combined flux in latest and established models = 0.14989 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 8 components and 0.14989 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=0.095194Jy sigma=0.000769 ! Fit after self-cal, rms=0.095084Jy sigma=0.000768 ! Inverting map ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec ! Added new window around map position (0.8, 0.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0241026 Jy ! Component: 100 - total flux cleaned = 0.0387228 Jy ! Total flux subtracted in 100 components = 0.0387228 Jy ! Clean residual min=-0.005438 max=0.011211 Jy/beam ! Clean residual mean=-0.000021 rms=0.001251 Jy/beam ! Combined flux in latest and established models = 0.188613 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 18 components and 0.188613 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=0.085722Jy sigma=0.000684 ! Fit after self-cal, rms=0.085501Jy sigma=0.000682 ! Inverting map ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0110068 Jy ! Component: 100 - total flux cleaned = 0.0177833 Jy ! Total flux subtracted in 100 components = 0.0177833 Jy ! Clean residual min=-0.004325 max=0.006968 Jy/beam ! Clean residual mean=-0.000012 rms=0.000892 Jy/beam ! Combined flux in latest and established models = 0.206396 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 29 components and 0.206396 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=0.083356Jy sigma=0.000662 ! Fit after self-cal, rms=0.083262Jy sigma=0.000662 ! Inverting map ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00586066 Jy ! Component: 100 - total flux cleaned = 0.00959305 Jy ! Total flux subtracted in 100 components = 0.00959305 Jy ! Clean residual min=-0.004031 max=0.004805 Jy/beam ! Clean residual mean=-0.000007 rms=0.000745 Jy/beam ! Combined flux in latest and established models = 0.215989 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 36 components and 0.215989 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=0.082647Jy sigma=0.000656 ! Fit after self-cal, rms=0.082603Jy sigma=0.000656 ! Inverting map ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 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 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec ! Estimated beam: bmin=0.9253 mas, bmaj=1.757 mas, bpa=-4.162 degrees ! Estimated noise=360.056 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 = 0.00459034 Jy ! Component: 100 - total flux cleaned = 0.00694465 Jy ! Component: 150 - total flux cleaned = 0.00846262 Jy ! Component: 200 - total flux cleaned = 0.00946885 Jy ! Total flux subtracted in 200 components = 0.00946885 Jy ! Clean residual min=-0.003019 max=0.003143 Jy/beam ! Clean residual mean=-0.000001 rms=0.000629 Jy/beam ! Combined flux in latest and established models = 0.225458 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 50 components and 0.225458 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=0.082351Jy sigma=0.000653 ! Fit after self-cal, rms=0.082320Jy sigma=0.000653 ! Inverting map ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 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 1.00 FD 0.97 HN 1.00 KP 1.04 ! LA 0.96 MK 1.03 NL 0.96 OV 0.98 ! PT 1.01 SC 1.06 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.99 HN 1.04 KP 1.05 ! LA 0.98 MK 0.96 NL 0.95 OV 1.00 ! PT 1.05 SC 1.05 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.99 HN 1.01 KP 1.03 ! LA 1.00 MK 1.01 NL 0.94 OV 0.99 ! PT 1.01 SC 1.04 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.97 HN 1.04 KP 1.04 ! LA 1.00 MK 1.04 NL 0.96 OV 0.99 ! PT 1.02 SC 1.05 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.97 HN 0.98 KP 1.03 ! LA 0.98 MK 1.04 NL 0.96 OV 0.98 ! PT 1.00 SC 1.02 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.98 HN 1.03 KP 1.02 ! LA 0.99 MK 0.99 NL 0.97 OV 0.99 ! PT 1.00 SC 1.02 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 1.00 HN 1.00 KP 1.02 ! LA 1.01 MK 1.00 NL 0.97 OV 0.99 ! PT 1.02 SC 1.02 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 1.03 HN 1.03 KP 1.03 ! LA 0.99 MK 1.00 NL 0.97 OV 1.00 ! PT 1.01 SC 1.06 ! ! ! Correcting IF 9. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.98 HN 1.06 KP 1.02 ! LA 1.00 MK 0.98 NL 0.96 OV 0.98 ! PT 1.03 SC 1.01 ! ! ! Correcting IF 10. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.98 HN 1.06 KP 1.04 ! LA 1.02 MK 0.99 NL 0.97 OV 0.99 ! PT 1.02 SC 0.98 ! ! ! Correcting IF 11. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 1.02 HN 1.05 KP 1.02 ! LA 1.00 MK 0.92 NL 0.98 OV 1.00 ! PT 1.04 SC 1.03 ! ! ! Correcting IF 12. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 1.01 HN 1.04 KP 1.00 ! LA 0.99 MK 0.91 NL 0.97 OV 1.00 ! PT 1.01 SC 1.02 ! ! ! Fit before self-cal, rms=0.082320Jy sigma=0.000653 ! Fit after self-cal, rms=0.083054Jy sigma=0.000651 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec ! Estimated beam: bmin=0.9278 mas, bmaj=1.765 mas, bpa=-4.535 degrees ! Estimated noise=360.986 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 (9.2, 4.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00288174 Jy ! Component: 100 - total flux cleaned = 0.0046527 Jy ! Component: 150 - total flux cleaned = 0.00587335 Jy ! Component: 200 - total flux cleaned = 0.00626831 Jy ! Total flux subtracted in 200 components = 0.00626831 Jy ! Clean residual min=-0.001738 max=0.002379 Jy/beam ! Clean residual mean=-0.000007 rms=0.000470 Jy/beam ! Combined flux in latest and established models = 0.231726 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 66 components and 0.231726 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=0.082944Jy sigma=0.000650 ! Fit after self-cal, rms=0.082964Jy sigma=0.000650 ! Inverting map ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec ! Added new window around map position (15.2, 6.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00231874 Jy ! Component: 100 - total flux cleaned = 0.0035901 Jy ! Component: 150 - total flux cleaned = 0.00427496 Jy ! Component: 200 - total flux cleaned = 0.0049121 Jy ! Total flux subtracted in 200 components = 0.0049121 Jy ! Clean residual min=-0.001557 max=0.001993 Jy/beam ! Clean residual mean=-0.000009 rms=0.000411 Jy/beam ! Combined flux in latest and established models = 0.236638 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 86 components and 0.236638 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=0.082895Jy sigma=0.000649 ! Fit after self-cal, rms=0.082887Jy sigma=0.000649 ! Inverting map ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 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=0.082887Jy sigma=0.000649 ! Fit after self-cal, rms=0.082497Jy sigma=0.000648 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec ! Estimated beam: bmin=0.927 mas, bmaj=1.762 mas, bpa=-4.499 degrees ! Estimated noise=360.966 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00033379 Jy ! Component: 100 - total flux cleaned = 0.00070795 Jy ! Component: 150 - total flux cleaned = 0.000990235 Jy ! Component: 200 - total flux cleaned = 0.00117745 Jy ! Total flux subtracted in 200 components = 0.00117745 Jy ! Clean residual min=-0.001384 max=0.001658 Jy/beam ! Clean residual mean=-0.000004 rms=0.000330 Jy/beam ! Combined flux in latest and established models = 0.237816 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 96 components and 0.237816 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=0.082480Jy sigma=0.000648 ! Fit after self-cal, rms=0.082472Jy sigma=0.000648 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 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 (4.2, 1.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00146927 Jy ! Component: 100 - total flux cleaned = 0.00180387 Jy ! Component: 150 - total flux cleaned = 0.00193725 Jy ! Component: 200 - total flux cleaned = 0.00202024 Jy ! Total flux subtracted in 200 components = 0.00202024 Jy ! Clean residual min=-0.001283 max=0.001207 Jy/beam ! Clean residual mean=-0.000001 rms=0.000300 Jy/beam ! Combined flux in latest and established models = 0.239836 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 112 components and 0.239836 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=0.082437Jy sigma=0.000647 ! Fit after self-cal, rms=0.082434Jy sigma=0.000647 ! Inverting map ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 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=0.082434Jy sigma=0.000647 ! Fit after self-cal, rms=0.082479Jy sigma=0.000647 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec ! Estimated beam: bmin=0.9273 mas, bmaj=1.762 mas, bpa=-4.434 degrees ! Estimated noise=361.097 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000548919 Jy ! Component: 100 - total flux cleaned = 0.000879495 Jy ! Component: 150 - total flux cleaned = 0.00102187 Jy ! Component: 200 - total flux cleaned = 0.00112944 Jy ! Total flux subtracted in 200 components = 0.00112944 Jy ! Clean residual min=-0.001263 max=0.001163 Jy/beam ! Clean residual mean=-0.000000 rms=0.000285 Jy/beam ! Combined flux in latest and established models = 0.240965 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 118 components and 0.240965 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=0.082465Jy sigma=0.000647 ! Fit after self-cal, rms=0.082462Jy sigma=0.000647 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 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 = 9.34027e-05 Jy ! Component: 100 - total flux cleaned = 0.000300003 Jy ! Component: 150 - total flux cleaned = 0.000431549 Jy ! Component: 200 - total flux cleaned = 0.000537011 Jy ! Total flux subtracted in 200 components = 0.000537011 Jy ! Clean residual min=-0.001232 max=0.001115 Jy/beam ! Clean residual mean=0.000000 rms=0.000278 Jy/beam ! Combined flux in latest and established models = 0.241502 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 123 components and 0.241502 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=0.082454Jy sigma=0.000647 ! Fit after self-cal, rms=0.082452Jy sigma=0.000647 ! Inverting map ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 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=0.082452Jy sigma=0.000647 ! Fit after self-cal, rms=0.082494Jy sigma=0.000647 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec ! Estimated beam: bmin=2.163 mas, bmaj=2.741 mas, bpa=-3.855 degrees ! Estimated noise=458.972 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000323265 Jy ! Component: 100 - total flux cleaned = 0.000715211 Jy ! Component: 150 - total flux cleaned = 0.00107074 Jy ! Component: 200 - total flux cleaned = 0.00135739 Jy ! Total flux subtracted in 200 components = 0.00135739 Jy ! Clean residual min=-0.001099 max=0.000956 Jy/beam ! Clean residual mean=-0.000002 rms=0.000327 Jy/beam ! Combined flux in latest and established models = 0.24286 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 133 components and 0.24286 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=0.082489Jy sigma=0.000647 ! Fit after self-cal, rms=0.082487Jy sigma=0.000647 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 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 = 4.68618e-05 Jy ! Component: 100 - total flux cleaned = 0.000282088 Jy ! Component: 150 - total flux cleaned = 0.000516323 Jy ! Component: 200 - total flux cleaned = 0.000736414 Jy ! Total flux subtracted in 200 components = 0.000736414 Jy ! Clean residual min=-0.001098 max=0.000944 Jy/beam ! Clean residual mean=-0.000001 rms=0.000322 Jy/beam ! Combined flux in latest and established models = 0.243596 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 139 components and 0.243596 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=0.082484Jy sigma=0.000647 ! Fit after self-cal, rms=0.082483Jy sigma=0.000647 ! Inverting map ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 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 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec ! Estimated beam: bmin=0.9279 mas, bmaj=1.762 mas, bpa=-4.4 degrees ! Estimated noise=361.285 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9279 x 1.762 at -4.4 degrees (North through East) ! Clean map min=-0.0010061 max=0.14436 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 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 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec ! Estimated beam: bmin=0.7182 mas, bmaj=1.481 mas, bpa=-5.34 degrees ! Estimated noise=717.291 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.109682 Jy ! Component: 100 - total flux cleaned = 0.153183 Jy ! Component: 150 - total flux cleaned = 0.177409 Jy ! Component: 200 - total flux cleaned = 0.192065 Jy ! Total flux subtracted in 200 components = 0.192065 Jy ! Clean residual min=-0.002903 max=0.007762 Jy/beam ! Clean residual mean=-0.000019 rms=0.000969 Jy/beam ! Combined flux in latest and established models = 0.192065 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 22 model components to the UV plane model. ! The established model now contains 22 components and 0.192065 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec ! Estimated beam: bmin=0.9279 mas, bmaj=1.762 mas, bpa=-4.4 degrees ! Estimated noise=361.285 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 = 0.0142719 Jy ! Component: 100 - total flux cleaned = 0.0220427 Jy ! Component: 150 - total flux cleaned = 0.0267427 Jy ! Component: 200 - total flux cleaned = 0.0300368 Jy ! Total flux subtracted in 200 components = 0.0300368 Jy ! Clean residual min=-0.001725 max=0.002914 Jy/beam ! Clean residual mean=-0.000010 rms=0.000513 Jy/beam ! Combined flux in latest and established models = 0.222102 Jy ! Adding 40 model components to the UV plane model. ! The established model now contains 50 components and 0.222102 Jy ! Inverting map ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec ! Added new window around map position (-1, -0.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00295306 Jy ! Component: 100 - total flux cleaned = 0.00501283 Jy ! Component: 150 - total flux cleaned = 0.00672167 Jy ! Component: 200 - total flux cleaned = 0.008224 Jy ! Total flux subtracted in 200 components = 0.008224 Jy ! Clean residual min=-0.001364 max=0.001545 Jy/beam ! Clean residual mean=-0.000005 rms=0.000370 Jy/beam ! Combined flux in latest and established models = 0.230326 Jy ! Adding 30 model components to the UV plane model. ! The established model now contains 74 components and 0.230326 Jy ! Inverting map ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 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 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec ! Estimated beam: bmin=2.163 mas, bmaj=2.741 mas, bpa=-3.855 degrees ! Estimated noise=458.972 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00258962 Jy ! Component: 100 - total flux cleaned = 0.00452201 Jy ! Component: 150 - total flux cleaned = 0.00604374 Jy ! Component: 200 - total flux cleaned = 0.00727405 Jy ! Total flux subtracted in 200 components = 0.00727405 Jy ! Clean residual min=-0.001336 max=0.001021 Jy/beam ! Clean residual mean=-0.000006 rms=0.000388 Jy/beam ! Combined flux in latest and established models = 0.2376 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 = 0.00101049 Jy ! Component: 100 - total flux cleaned = 0.00185929 Jy ! Component: 150 - total flux cleaned = 0.00258578 Jy ! Component: 200 - total flux cleaned = 0.00316751 Jy ! Total flux subtracted in 200 components = 0.00316751 Jy ! Clean residual min=-0.001155 max=0.000934 Jy/beam ! Clean residual mean=-0.000004 rms=0.000335 Jy/beam ! Combined flux in latest and established models = 0.240768 Jy ! Adding 87 model components to the UV plane model. ! The established model now contains 143 components and 0.240768 Jy ! Inverting map ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec ! Estimated beam: bmin=0.9279 mas, bmaj=1.762 mas, bpa=-4.4 degrees ! Estimated noise=361.285 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000162367 Jy ! Component: 100 - total flux cleaned = 9.64346e-05 Jy ! Component: 150 - total flux cleaned = 0.000260412 Jy ! Component: 200 - total flux cleaned = 0.00040866 Jy ! Total flux subtracted in 200 components = 0.00040866 Jy ! Clean residual min=-0.000986 max=0.000981 Jy/beam ! Clean residual mean=-0.000002 rms=0.000260 Jy/beam ! Combined flux in latest and established models = 0.241176 Jy selfcal ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 163 components and 0.241176 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=0.082472Jy sigma=0.000647 ! Fit after self-cal, rms=0.082466Jy sigma=0.000647 wmodel J1949+2421_X_2017_07_09_pus_map.mod ! Writing 163 model components to file: J1949+2421_X_2017_07_09_pus_map.mod wobs J1949+2421_X_2017_07_09_pus_uvs.fits ! Writing UV FITS file: J1949+2421_X_2017_07_09_pus_uvs.fits wwins J1949+2421_X_2017_07_09_pus_map.win ! wwins: Wrote 6 windows to J1949+2421_X_2017_07_09_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 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000150639 Jy ! Component: 100 - total flux cleaned = -0.000274716 Jy ! Component: 150 - total flux cleaned = -0.000308278 Jy ! Component: 200 - total flux cleaned = -0.000340191 Jy ! Component: 250 - total flux cleaned = -0.000370602 Jy ! Component: 300 - total flux cleaned = -0.000400311 Jy ! Component: 350 - total flux cleaned = -0.000400721 Jy ! Component: 400 - total flux cleaned = -0.000372607 Jy ! Component: 450 - total flux cleaned = -0.000317462 Jy ! Component: 500 - total flux cleaned = -0.000250188 Jy ! Component: 550 - total flux cleaned = -0.000171068 Jy ! Component: 600 - total flux cleaned = -8.07872e-05 Jy ! Component: 650 - total flux cleaned = 2.01131e-05 Jy ! Component: 700 - total flux cleaned = 8.18319e-05 Jy ! Component: 750 - total flux cleaned = 0.000190839 Jy ! Component: 800 - total flux cleaned = 0.000250383 Jy ! Component: 850 - total flux cleaned = 0.000332731 Jy ! Component: 900 - total flux cleaned = 0.000402 Jy ! Component: 950 - total flux cleaned = 0.000470177 Jy ! Component: 1000 - total flux cleaned = 0.000503795 Jy ! Component: 1050 - total flux cleaned = 0.000581101 Jy ! Component: 1100 - total flux cleaned = 0.000613873 Jy ! Component: 1150 - total flux cleaned = 0.000678348 Jy ! Component: 1200 - total flux cleaned = 0.000710258 Jy ! Component: 1250 - total flux cleaned = 0.000783439 Jy ! Component: 1300 - total flux cleaned = 0.000814133 Jy ! Component: 1350 - total flux cleaned = 0.000814216 Jy ! Component: 1400 - total flux cleaned = 0.000874642 Jy ! Component: 1450 - total flux cleaned = 0.000884688 Jy ! Component: 1500 - total flux cleaned = 0.000904258 Jy ! Component: 1550 - total flux cleaned = 0.000885012 Jy ! Component: 1600 - total flux cleaned = 0.000952132 Jy ! Component: 1650 - total flux cleaned = 0.000952088 Jy ! Component: 1700 - total flux cleaned = 0.000970693 Jy ! Component: 1750 - total flux cleaned = 0.000970699 Jy ! Component: 1800 - total flux cleaned = 0.00102563 Jy ! Component: 1850 - total flux cleaned = 0.00104382 Jy ! Component: 1900 - total flux cleaned = 0.00106173 Jy ! Component: 1950 - total flux cleaned = 0.001115 Jy ! Component: 2000 - total flux cleaned = 0.00110621 Jy ! Total flux subtracted in 2048 components = 0.00111505 Jy ! Clean residual min=-0.000471 max=0.000539 Jy/beam ! Clean residual mean=-0.000000 rms=0.000163 Jy/beam ! Combined flux in latest and established models = 0.242291 Jy keep ! Adding 160 model components to the UV plane model. ! The established model now contains 322 components and 0.242291 Jy ![Exited script file: muppet] wmap "J1949+2421_X_2017_07_09_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9279 x 1.762 at -4.4 degrees (North through East) ! Clean map min=-0.0011309 max=0.1447 Jy/beam ! Writing clean map to FITS file: J1949+2421_X_2017_07_09_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.144697 invert ! Inverting map ! Your choice of large map pixels excluded 0.133% of the data. ! The x-axis pixel size should ideally be below 0.1991 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000163232 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.338429 0.338429 0.676858 1.35372 2.70743 5.41486 10.8297 21.6595 43.3189 86.6378 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0004 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.144 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9279 x 1.762 at -4.4 degrees (North through East) ! Clean map min=-0.0011309 max=0.1447 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 J1949+2421_X_2017_07_09_pus_uvs.log closed on Wed May 8 15:30:47 2019