! Started logfile: J0008-2339_X_2017_05_27_pus_uvs.log on Fri May 3 10:27:30 2019 obs J0008-2339_X_2017_05_27_pus_uva.fits ! Reading UV FITS file: J0008-2339_X_2017_05_27_pus_uva.fits ! AN table 1: 116 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.985057 visibilities/baseline/integration-bin. ! Found source: J0008-2339 ! ! 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 1033 lines of history. ! ! Reading 61704 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 J0008-2339_X_2017_05_27_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 10 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 10 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 10 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 10 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 5. ! A total of 10 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 6. ! A total of 10 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 7. ! A total of 10 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 8. ! A total of 10 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 9. ! A total of 10 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 10. ! A total of 10 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 11. ! A total of 10 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 12. ! A total of 10 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.881771Jy sigma=0.006793 ! Fit after self-cal, rms=0.860782Jy sigma=0.006643 ! 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 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.6103 mas, bmaj=1.678 mas, bpa=-2.992 degrees ! Estimated noise=843.192 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 = 0.109724 Jy ! Component: 100 - total flux cleaned = 0.146409 Jy ! Total flux subtracted in 100 components = 0.146409 Jy ! Clean residual min=-0.017792 max=0.061472 Jy/beam ! Clean residual mean=-0.000162 rms=0.005961 Jy/beam ! Combined flux in latest and established models = 0.146409 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.146409 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=0.138636Jy sigma=0.001029 ! Fit after self-cal, rms=0.138578Jy sigma=0.001028 ! Inverting map ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Added new window around map position (1.8, -3.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.053082 Jy ! Component: 100 - total flux cleaned = 0.0761032 Jy ! Total flux subtracted in 100 components = 0.0761032 Jy ! Clean residual min=-0.011863 max=0.038446 Jy/beam ! Clean residual mean=-0.000098 rms=0.003891 Jy/beam ! Combined flux in latest and established models = 0.222512 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 11 components and 0.222512 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=0.115665Jy sigma=0.000830 ! Fit after self-cal, rms=0.107838Jy sigma=0.000770 ! Inverting map ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0281222 Jy ! Component: 100 - total flux cleaned = 0.0407564 Jy ! Total flux subtracted in 100 components = 0.0407564 Jy ! Clean residual min=-0.007110 max=0.017766 Jy/beam ! Clean residual mean=-0.000048 rms=0.002051 Jy/beam ! Combined flux in latest and established models = 0.263268 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 12 components and 0.263268 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=0.100076Jy sigma=0.000696 ! Fit after self-cal, rms=0.098498Jy sigma=0.000684 ! Inverting map ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Added new window around map position (1, -1.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0144741 Jy ! Component: 100 - total flux cleaned = 0.0205134 Jy ! Total flux subtracted in 100 components = 0.0205134 Jy ! Clean residual min=-0.005051 max=0.009603 Jy/beam ! Clean residual mean=-0.000016 rms=0.001252 Jy/beam ! Combined flux in latest and established models = 0.283782 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 21 components and 0.283782 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=0.096134Jy sigma=0.000662 ! Fit after self-cal, rms=0.095923Jy sigma=0.000660 ! Inverting map ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 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 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.7946 mas, bmaj=2.053 mas, bpa=-2.21 degrees ! Estimated noise=370.639 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 = 0.0073725 Jy ! Component: 100 - total flux cleaned = 0.00809041 Jy ! Component: 150 - total flux cleaned = 0.00860848 Jy ! Component: 200 - total flux cleaned = 0.00921627 Jy ! Total flux subtracted in 200 components = 0.00921627 Jy ! Clean residual min=-0.002824 max=0.005881 Jy/beam ! Clean residual mean=-0.000008 rms=0.000711 Jy/beam ! Combined flux in latest and established models = 0.292998 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 29 components and 0.292998 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=0.095296Jy sigma=0.000655 ! Fit after self-cal, rms=0.095214Jy sigma=0.000654 ! Inverting map ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 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 0.95 FD 0.97 HN 1.10 KP 0.99 ! LA 0.95 MK 0.98 NL 0.98 OV 0.98 ! PT 0.98 SC 1.02 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 0.99 HN 1.06 KP 0.97 ! LA 0.97 MK 0.97 NL 0.98 OV 0.99 ! PT 0.99 SC 1.00 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.99 HN 1.10 KP 0.98 ! LA 0.99 MK 0.99 NL 0.97 OV 0.99 ! PT 1.00 SC 0.99 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.98 HN 1.06 KP 0.97 ! LA 0.99 MK 1.01 NL 0.99 OV 0.98 ! PT 1.03 SC 1.00 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 0.94 FD 0.96 HN 1.44 KP 0.99 ! LA 0.97 MK 1.04 NL 0.99 OV 0.99 ! PT 1.03 SC 0.98 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.99 HN 1.03 KP 0.99 ! LA 0.98 MK 1.01 NL 0.99 OV 1.00 ! PT 1.02 SC 1.03 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.98 HN 1.46 KP 0.99 ! LA 1.01 MK 1.02 NL 1.00 OV 0.99 ! PT 1.03 SC 1.01 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 1.05 HN 1.07 KP 0.98 ! LA 0.98 MK 1.01 NL 0.99 OV 0.98 ! PT 1.02 SC 1.02 ! ! ! Correcting IF 9. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.99 HN 1.11 KP 0.99 ! LA 1.00 MK 0.98 NL 1.00 OV 1.01 ! PT 0.99 SC 0.96 ! ! ! Correcting IF 10. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 1.01 HN 1.54 KP 1.00 ! LA 1.02 MK 1.01 NL 1.00 OV 1.02 ! PT 1.04 SC 0.97 ! ! ! Correcting IF 11. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 1.02 HN 1.00 KP 1.00 ! LA 1.01 MK 1.02 NL 1.00 OV 1.00 ! PT 1.06 SC 0.99 ! ! ! Correcting IF 12. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 1.00 HN 1.04 KP 0.94 ! LA 1.01 MK 1.04 NL 1.04 OV 1.02 ! PT 1.06 SC 1.01 ! ! ! Fit before self-cal, rms=0.095214Jy sigma=0.000654 ! Fit after self-cal, rms=0.101833Jy sigma=0.000650 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.7989 mas, bmaj=2.05 mas, bpa=-1.97 degrees ! Estimated noise=372.066 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 = 0.000716135 Jy ! Component: 100 - total flux cleaned = 0.000247337 Jy ! Component: 150 - total flux cleaned = 9.02562e-05 Jy ! Component: 200 - total flux cleaned = 8.93928e-05 Jy ! Total flux subtracted in 200 components = 8.93928e-05 Jy ! Clean residual min=-0.001551 max=0.002283 Jy/beam ! Clean residual mean=-0.000009 rms=0.000460 Jy/beam ! Combined flux in latest and established models = 0.293087 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 36 components and 0.293087 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=0.101719Jy sigma=0.000649 ! Fit after self-cal, rms=0.101751Jy sigma=0.000649 ! Inverting map ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 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=0.101751Jy sigma=0.000649 ! Fit after self-cal, rms=0.102031Jy sigma=0.000649 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.7994 mas, bmaj=2.049 mas, bpa=-1.877 degrees ! Estimated noise=371.778 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 7.67114e-05 Jy ! Component: 100 - total flux cleaned = -4.35036e-06 Jy ! Component: 150 - total flux cleaned = -3.71693e-05 Jy ! Component: 200 - total flux cleaned = -7.44965e-06 Jy ! Total flux subtracted in 200 components = -7.44965e-06 Jy ! Clean residual min=-0.001396 max=0.001835 Jy/beam ! Clean residual mean=-0.000007 rms=0.000422 Jy/beam ! Combined flux in latest and established models = 0.29308 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 42 components and 0.29308 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=0.101991Jy sigma=0.000649 ! Fit after self-cal, rms=0.101988Jy sigma=0.000649 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 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 = 0.000154967 Jy ! Component: 100 - total flux cleaned = 9.80211e-05 Jy ! Component: 150 - total flux cleaned = 4.57404e-05 Jy ! Component: 200 - total flux cleaned = 2.20682e-05 Jy ! Total flux subtracted in 200 components = 2.20682e-05 Jy ! Clean residual min=-0.001388 max=0.001721 Jy/beam ! Clean residual mean=-0.000007 rms=0.000410 Jy/beam ! Combined flux in latest and established models = 0.293102 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 47 components and 0.293102 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=0.101969Jy sigma=0.000649 ! Fit after self-cal, rms=0.101967Jy sigma=0.000649 ! Inverting map ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 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=0.101967Jy sigma=0.000649 ! Fit after self-cal, rms=0.112007Jy sigma=0.000646 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.7993 mas, bmaj=2.048 mas, bpa=-1.795 degrees ! Estimated noise=371.361 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000105158 Jy ! Component: 100 - total flux cleaned = 3.23469e-05 Jy ! Component: 150 - total flux cleaned = -1.11661e-05 Jy ! Component: 200 - total flux cleaned = -2.99298e-05 Jy ! Total flux subtracted in 200 components = -2.99298e-05 Jy ! Clean residual min=-0.001167 max=0.001315 Jy/beam ! Clean residual mean=-0.000005 rms=0.000276 Jy/beam ! Combined flux in latest and established models = 0.293072 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 51 components and 0.293072 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=0.111996Jy sigma=0.000646 ! Fit after self-cal, rms=0.112042Jy sigma=0.000646 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 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 (20.2, -19). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000348021 Jy ! Component: 100 - total flux cleaned = 0.000458039 Jy ! Component: 150 - total flux cleaned = 0.000545482 Jy ! Component: 200 - total flux cleaned = 0.000507489 Jy ! Total flux subtracted in 200 components = 0.000507489 Jy ! Clean residual min=-0.001084 max=0.001180 Jy/beam ! Clean residual mean=-0.000004 rms=0.000259 Jy/beam ! Combined flux in latest and established models = 0.293579 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 66 components and 0.293579 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=0.112021Jy sigma=0.000646 ! Fit after self-cal, rms=0.112019Jy sigma=0.000646 ! Inverting map ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Added new window around map position (-2, 2.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00107751 Jy ! Component: 100 - total flux cleaned = 0.00132017 Jy ! Component: 150 - total flux cleaned = 0.00144736 Jy ! Component: 200 - total flux cleaned = 0.00152279 Jy ! Total flux subtracted in 200 components = 0.00152279 Jy ! Clean residual min=-0.000998 max=0.000953 Jy/beam ! Clean residual mean=-0.000000 rms=0.000239 Jy/beam ! Combined flux in latest and established models = 0.295102 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 81 components and 0.295102 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=0.112004Jy sigma=0.000646 ! Fit after self-cal, rms=0.112005Jy sigma=0.000646 ! Inverting map ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 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=0.112005Jy sigma=0.000646 ! Fit after self-cal, rms=0.112156Jy sigma=0.000646 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=2.216 mas, bmaj=5.178 mas, bpa=2.829 degrees ! Estimated noise=473.727 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000101966 Jy ! Component: 100 - total flux cleaned = 0.000182865 Jy ! Component: 150 - total flux cleaned = 0.000248046 Jy ! Component: 200 - total flux cleaned = 0.000266766 Jy ! Total flux subtracted in 200 components = 0.000266766 Jy ! Clean residual min=-0.000895 max=0.001078 Jy/beam ! Clean residual mean=-0.000003 rms=0.000255 Jy/beam ! Combined flux in latest and established models = 0.295369 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 93 components and 0.295369 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=0.112153Jy sigma=0.000646 ! Fit after self-cal, rms=0.112153Jy sigma=0.000646 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 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 = -1.00299e-05 Jy ! Component: 100 - total flux cleaned = 4.6159e-06 Jy ! Component: 150 - total flux cleaned = 2.57449e-05 Jy ! Component: 200 - total flux cleaned = 5.14503e-05 Jy ! Total flux subtracted in 200 components = 5.14503e-05 Jy ! Clean residual min=-0.000890 max=0.001046 Jy/beam ! Clean residual mean=-0.000002 rms=0.000250 Jy/beam ! Combined flux in latest and established models = 0.29542 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 104 components and 0.29542 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=0.112153Jy sigma=0.000646 ! Fit after self-cal, rms=0.112153Jy sigma=0.000646 ! Inverting map ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 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 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.7993 mas, bmaj=2.048 mas, bpa=-1.808 degrees ! Estimated noise=371.438 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7993 x 2.048 at -1.808 degrees (North through East) ! Clean map min=-0.00096329 max=0.13561 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 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.6133 mas, bmaj=1.671 mas, bpa=-2.621 degrees ! Estimated noise=844.342 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.121075 Jy ! Component: 100 - total flux cleaned = 0.18369 Jy ! Component: 150 - total flux cleaned = 0.222041 Jy ! Component: 200 - total flux cleaned = 0.24599 Jy ! Total flux subtracted in 200 components = 0.24599 Jy ! Clean residual min=-0.005533 max=0.012601 Jy/beam ! Clean residual mean=-0.000066 rms=0.001699 Jy/beam ! Combined flux in latest and established models = 0.24599 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 15 model components to the UV plane model. ! The established model now contains 15 components and 0.24599 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.7993 mas, bmaj=2.048 mas, bpa=-1.808 degrees ! Estimated noise=371.438 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 = 0.0198936 Jy ! Component: 100 - total flux cleaned = 0.0310664 Jy ! Component: 150 - total flux cleaned = 0.037757 Jy ! Component: 200 - total flux cleaned = 0.0420013 Jy ! Total flux subtracted in 200 components = 0.0420013 Jy ! Clean residual min=-0.001446 max=0.002587 Jy/beam ! Clean residual mean=-0.000023 rms=0.000429 Jy/beam ! Combined flux in latest and established models = 0.287991 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 32 components and 0.287991 Jy ! Inverting map ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Added new window around map position (-0.8, 1). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00282269 Jy ! Component: 100 - total flux cleaned = 0.00417476 Jy ! Component: 150 - total flux cleaned = 0.0048234 Jy ! Component: 200 - total flux cleaned = 0.00527673 Jy ! Total flux subtracted in 200 components = 0.00527673 Jy ! Clean residual min=-0.001182 max=0.001045 Jy/beam ! Clean residual mean=-0.000007 rms=0.000273 Jy/beam ! Combined flux in latest and established models = 0.293268 Jy ! Adding 23 model components to the UV plane model. ! The established model now contains 49 components and 0.293268 Jy ! Inverting map ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 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 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=2.216 mas, bmaj=5.178 mas, bpa=2.829 degrees ! Estimated noise=473.727 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000897693 Jy ! Component: 100 - total flux cleaned = 0.00130103 Jy ! Component: 150 - total flux cleaned = 0.00158118 Jy ! Component: 200 - total flux cleaned = 0.00170878 Jy ! Total flux subtracted in 200 components = 0.00170878 Jy ! Clean residual min=-0.000970 max=0.001094 Jy/beam ! Clean residual mean=-0.000005 rms=0.000269 Jy/beam ! Combined flux in latest and established models = 0.294977 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 = 0.000112964 Jy ! Component: 100 - total flux cleaned = 0.000213954 Jy ! Component: 150 - total flux cleaned = 0.000292822 Jy ! Component: 200 - total flux cleaned = 0.000365023 Jy ! Total flux subtracted in 200 components = 0.000365023 Jy ! Clean residual min=-0.000955 max=0.001097 Jy/beam ! Clean residual mean=-0.000003 rms=0.000261 Jy/beam ! Combined flux in latest and established models = 0.295342 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 68 components and 0.295342 Jy ! Inverting map ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.7993 mas, bmaj=2.048 mas, bpa=-1.808 degrees ! Estimated noise=371.438 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 8.01964e-05 Jy ! Component: 100 - total flux cleaned = 0.000144857 Jy ! Component: 150 - total flux cleaned = 0.000220793 Jy ! Component: 200 - total flux cleaned = 0.000219887 Jy ! Total flux subtracted in 200 components = 0.000219887 Jy ! Clean residual min=-0.001039 max=0.000983 Jy/beam ! Clean residual mean=-0.000002 rms=0.000232 Jy/beam ! Combined flux in latest and established models = 0.295562 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 83 components and 0.295562 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=0.112164Jy sigma=0.000646 ! Fit after self-cal, rms=0.112153Jy sigma=0.000645 wmodel J0008-2339_X_2017_05_27_pus_map.mod ! Writing 83 model components to file: J0008-2339_X_2017_05_27_pus_map.mod wobs J0008-2339_X_2017_05_27_pus_uvs.fits ! Writing UV FITS file: J0008-2339_X_2017_05_27_pus_uvs.fits wwins J0008-2339_X_2017_05_27_pus_map.win ! wwins: Wrote 6 windows to J0008-2339_X_2017_05_27_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 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000125664 Jy ! Component: 100 - total flux cleaned = -0.000233971 Jy ! Component: 150 - total flux cleaned = -0.000349686 Jy ! Component: 200 - total flux cleaned = -0.000418037 Jy ! Component: 250 - total flux cleaned = -0.000469993 Jy ! Component: 300 - total flux cleaned = -0.000545397 Jy ! Component: 350 - total flux cleaned = -0.000606249 Jy ! Component: 400 - total flux cleaned = -0.000665445 Jy ! Component: 450 - total flux cleaned = -0.000700671 Jy ! Component: 500 - total flux cleaned = -0.000791569 Jy ! Component: 550 - total flux cleaned = -0.000858545 Jy ! Component: 600 - total flux cleaned = -0.000946073 Jy ! Component: 650 - total flux cleaned = -0.00101087 Jy ! Component: 700 - total flux cleaned = -0.00111672 Jy ! Component: 750 - total flux cleaned = -0.0012209 Jy ! Component: 800 - total flux cleaned = -0.00131319 Jy ! Component: 850 - total flux cleaned = -0.00136363 Jy ! Component: 900 - total flux cleaned = -0.00142356 Jy ! Component: 950 - total flux cleaned = -0.00150236 Jy ! Component: 1000 - total flux cleaned = -0.00157987 Jy ! Component: 1050 - total flux cleaned = -0.00162779 Jy ! Component: 1100 - total flux cleaned = -0.00170349 Jy ! Component: 1150 - total flux cleaned = -0.00176904 Jy ! Component: 1200 - total flux cleaned = -0.00181546 Jy ! Component: 1250 - total flux cleaned = -0.00187047 Jy ! Component: 1300 - total flux cleaned = -0.00193369 Jy ! Component: 1350 - total flux cleaned = -0.00199607 Jy ! Component: 1400 - total flux cleaned = -0.00203127 Jy ! Component: 1450 - total flux cleaned = -0.00206613 Jy ! Component: 1500 - total flux cleaned = -0.0021348 Jy ! Component: 1550 - total flux cleaned = -0.00215155 Jy ! Component: 1600 - total flux cleaned = -0.00216002 Jy ! Component: 1650 - total flux cleaned = -0.00218507 Jy ! Component: 1700 - total flux cleaned = -0.00220159 Jy ! Component: 1750 - total flux cleaned = -0.00223403 Jy ! Component: 1800 - total flux cleaned = -0.00223407 Jy ! Component: 1850 - total flux cleaned = -0.00224209 Jy ! Component: 1900 - total flux cleaned = -0.00226568 Jy ! Component: 1950 - total flux cleaned = -0.00222658 Jy ! Component: 2000 - total flux cleaned = -0.00224215 Jy ! Total flux subtracted in 2048 components = -0.00224984 Jy ! Clean residual min=-0.000414 max=0.000492 Jy/beam ! Clean residual mean=-0.000000 rms=0.000142 Jy/beam ! Combined flux in latest and established models = 0.293312 Jy keep ! Adding 137 model components to the UV plane model. ! The established model now contains 220 components and 0.293312 Jy ![Exited script file: muppet] wmap "J0008-2339_X_2017_05_27_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7993 x 2.048 at -1.808 degrees (North through East) ! Clean map min=-0.0010907 max=0.13413 Jy/beam ! Writing clean map to FITS file: J0008-2339_X_2017_05_27_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.134132 invert ! Inverting map ! Your choice of large map pixels excluded 0.185% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000141773 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.31709 0.31709 0.634179 1.26836 2.53672 5.07343 10.1469 20.2937 40.5875 81.1749 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0004 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.134 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7993 x 2.048 at -1.808 degrees (North through East) ! Clean map min=-0.0010907 max=0.13413 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 J0008-2339_X_2017_05_27_pus_uvs.log closed on Fri May 3 10:27:33 2019