! Started logfile: J2010+3322_X_2017_06_10_pus_uvs.log on Mon May 6 12:52:31 2019 obs J2010+3322_X_2017_06_10_pus_uva.fits ! Reading UV FITS file: J2010+3322_X_2017_06_10_pus_uva.fits ! AN table 1: 173 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.959666 visibilities/baseline/integration-bin. ! Found source: J2010+3322 ! ! 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 1309 lines of history. ! ! Reading 89652 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 J2010+3322_X_2017_06_10_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 38 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 79 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 52 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 38 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 5. ! A total of 38 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 6. ! A total of 52 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 7. ! A total of 79 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 8. ! A total of 38 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 9. ! A total of 52 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 10. ! A total of 52 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 11. ! A total of 52 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 12. ! A total of 52 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.881298Jy sigma=0.008236 ! Fit after self-cal, rms=0.852802Jy sigma=0.007979 ! 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 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.7717 mas, bmaj=1.335 mas, bpa=-3.294 degrees ! Estimated noise=601.669 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 = 0.114635 Jy ! Component: 100 - total flux cleaned = 0.174965 Jy ! Total flux subtracted in 100 components = 0.174965 Jy ! Clean residual min=-0.021675 max=0.057108 Jy/beam ! Clean residual mean=-0.000058 rms=0.006984 Jy/beam ! Combined flux in latest and established models = 0.174965 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 18 components and 0.174965 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=0.190262Jy sigma=0.001834 ! Fit after self-cal, rms=0.189421Jy sigma=0.001826 ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Added new window around map position (-5.4, 0.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0580078 Jy ! Component: 100 - total flux cleaned = 0.0964999 Jy ! Total flux subtracted in 100 components = 0.0964999 Jy ! Clean residual min=-0.016942 max=0.038897 Jy/beam ! Clean residual mean=-0.000055 rms=0.005429 Jy/beam ! Combined flux in latest and established models = 0.271465 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 39 components and 0.271465 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=0.160155Jy sigma=0.001531 ! Fit after self-cal, rms=0.155993Jy sigma=0.001491 ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Added new window around map position (1.2, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0436636 Jy ! Component: 100 - total flux cleaned = 0.0749593 Jy ! Total flux subtracted in 100 components = 0.0749593 Jy ! Clean residual min=-0.012598 max=0.030623 Jy/beam ! Clean residual mean=-0.000064 rms=0.004189 Jy/beam ! Combined flux in latest and established models = 0.346425 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 53 components and 0.346425 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=0.134519Jy sigma=0.001272 ! Fit after self-cal, rms=0.133232Jy sigma=0.001260 ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Added new window around map position (-1.2, 0.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0310674 Jy ! Component: 100 - total flux cleaned = 0.0551972 Jy ! Total flux subtracted in 100 components = 0.0551972 Jy ! Clean residual min=-0.010787 max=0.020366 Jy/beam ! Clean residual mean=-0.000064 rms=0.003395 Jy/beam ! Combined flux in latest and established models = 0.401622 Jy ! Performing phase self-cal ! Adding 38 model components to the UV plane model. ! The established model now contains 80 components and 0.401622 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=0.119197Jy sigma=0.001116 ! Fit after self-cal, rms=0.118886Jy sigma=0.001113 ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec print "************** FINISHED UNIFORM WEIGHTING CLEAN **************" ! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** ! uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. win_mult = win_mult * 1.6 clean_niter = clean_niter * 2 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.989 mas, bmaj=1.622 mas, bpa=-2.176 degrees ! Estimated noise=255.515 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 = 0.0394885 Jy ! Component: 100 - total flux cleaned = 0.0715212 Jy ! Component: 150 - total flux cleaned = 0.098201 Jy ! Component: 200 - total flux cleaned = 0.120606 Jy ! Total flux subtracted in 200 components = 0.120606 Jy ! Clean residual min=-0.010595 max=0.021478 Jy/beam ! Clean residual mean=-0.000174 rms=0.003615 Jy/beam ! Combined flux in latest and established models = 0.522228 Jy ! Performing phase self-cal ! Adding 74 model components to the UV plane model. ! The established model now contains 133 components and 0.522228 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=0.096598Jy sigma=0.000884 ! Fit after self-cal, rms=0.096058Jy sigma=0.000879 ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Added new window around map position (2.6, -0.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0229316 Jy ! Component: 100 - total flux cleaned = 0.0406983 Jy ! Component: 150 - total flux cleaned = 0.0558759 Jy ! Component: 200 - total flux cleaned = 0.068979 Jy ! Total flux subtracted in 200 components = 0.068979 Jy ! Clean residual min=-0.007943 max=0.017013 Jy/beam ! Clean residual mean=-0.000112 rms=0.002502 Jy/beam ! Combined flux in latest and established models = 0.591207 Jy ! Performing phase self-cal ! Adding 54 model components to the UV plane model. ! The established model now contains 173 components and 0.591207 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=0.087429Jy sigma=0.000789 ! Fit after self-cal, rms=0.087016Jy sigma=0.000785 ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Added new window around map position (-6.8, 1.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0153404 Jy ! Component: 100 - total flux cleaned = 0.0263394 Jy ! Component: 150 - total flux cleaned = 0.0359225 Jy ! Component: 200 - total flux cleaned = 0.0433744 Jy ! Total flux subtracted in 200 components = 0.0433744 Jy ! Clean residual min=-0.005686 max=0.014837 Jy/beam ! Clean residual mean=-0.000068 rms=0.001853 Jy/beam ! Combined flux in latest and established models = 0.634582 Jy ! Performing phase self-cal ! Adding 49 model components to the UV plane model. ! The established model now contains 203 components and 0.634582 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=0.083001Jy sigma=0.000744 ! Fit after self-cal, rms=0.082794Jy sigma=0.000742 ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Added new window around map position (-4, 0.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0114921 Jy ! Component: 100 - total flux cleaned = 0.0171811 Jy ! Component: 150 - total flux cleaned = 0.0224374 Jy ! Component: 200 - total flux cleaned = 0.0269343 Jy ! Total flux subtracted in 200 components = 0.0269343 Jy ! Clean residual min=-0.004584 max=0.005846 Jy/beam ! Clean residual mean=-0.000045 rms=0.001331 Jy/beam ! Combined flux in latest and established models = 0.661516 Jy ! Performing phase self-cal ! Adding 58 model components to the UV plane model. ! The established model now contains 236 components and 0.661516 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=0.080112Jy sigma=0.000714 ! Fit after self-cal, rms=0.079952Jy sigma=0.000713 ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.08 FD 0.97 HN 1.23 KP 1.00 ! LA 0.93 MK 1.35 NL 1.01 OV 0.98 ! PT 0.95 SC 1.25 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.08 FD 0.99 HN 1.03 KP 0.97 ! LA 0.93 MK 1.42 NL 1.00 OV 0.97 ! PT 0.99 SC 1.33 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.08 FD 0.98 HN 1.20 KP 0.99 ! LA 0.95 MK 1.32 NL 1.01 OV 0.99 ! PT 0.95 SC 1.30 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.07 FD 0.96 HN 1.04 KP 0.99 ! LA 0.96 MK 1.33 NL 0.98 OV 0.99 ! PT 0.98 SC 1.28 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.07 FD 0.97 HN 1.14 KP 0.99 ! LA 0.95 MK 1.26 NL 1.00 OV 0.99 ! PT 0.98 SC 1.22 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.08 FD 0.97 HN 1.04 KP 1.01 ! LA 0.96 MK 1.24 NL 0.98 OV 0.99 ! PT 0.96 SC 1.28 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.07 FD 0.99 HN 1.05 KP 1.01 ! LA 0.98 MK 1.23 NL 0.99 OV 0.99 ! PT 0.98 SC 1.21 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 1.03 HN 1.01 KP 1.01 ! LA 0.95 MK 1.19 NL 0.98 OV 1.00 ! PT 0.99 SC 1.23 ! ! ! Correcting IF 9. ! Telescope amplitude corrections in sub-array 1: ! BR 1.06 FD 1.00 HN 1.01 KP 1.02 ! LA 0.97 MK 1.05 NL 0.97 OV 0.99 ! PT 0.99 SC 1.18 ! ! ! Correcting IF 10. ! Telescope amplitude corrections in sub-array 1: ! BR 1.07 FD 0.99 HN 1.01 KP 1.01 ! LA 1.00 MK 1.12 NL 0.96 OV 0.99 ! PT 0.99 SC 1.08 ! ! ! Correcting IF 11. ! Telescope amplitude corrections in sub-array 1: ! BR 1.06 FD 1.01 HN 1.21 KP 1.02 ! LA 0.99 MK 0.97 NL 0.98 OV 0.99 ! PT 1.00 SC 1.09 ! ! ! Correcting IF 12. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 FD 1.00 HN 1.01 KP 0.97 ! LA 0.97 MK 0.96 NL 0.96 OV 1.00 ! PT 1.01 SC 1.15 ! ! ! Fit before self-cal, rms=0.079952Jy sigma=0.000713 ! Fit after self-cal, rms=0.087097Jy sigma=0.000694 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=1.045 mas, bmaj=1.692 mas, bpa=-2.967 degrees ! Estimated noise=273.24 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 = 0.000518912 Jy ! Component: 100 - total flux cleaned = 0.00281056 Jy ! Component: 150 - total flux cleaned = 0.00454484 Jy ! Component: 200 - total flux cleaned = 0.00583531 Jy ! Total flux subtracted in 200 components = 0.00583531 Jy ! Clean residual min=-0.003576 max=0.003427 Jy/beam ! Clean residual mean=0.000026 rms=0.000932 Jy/beam ! Combined flux in latest and established models = 0.667351 Jy ! Performing phase self-cal ! Adding 34 model components to the UV plane model. ! The established model now contains 248 components and 0.667351 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=0.086591Jy sigma=0.000689 ! Fit after self-cal, rms=0.086594Jy sigma=0.000689 ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec selfcal true, true, soltime1 ! Performing amp+phase self-cal over 120 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.086594Jy sigma=0.000689 ! Fit after self-cal, rms=0.097067Jy sigma=0.000675 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=1.05 mas, bmaj=1.728 mas, bpa=-2.727 degrees ! Estimated noise=274.548 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00103776 Jy ! Component: 100 - total flux cleaned = 0.00230304 Jy ! Component: 150 - total flux cleaned = 0.00342085 Jy ! Component: 200 - total flux cleaned = 0.00434295 Jy ! Total flux subtracted in 200 components = 0.00434295 Jy ! Clean residual min=-0.002100 max=0.002737 Jy/beam ! Clean residual mean=0.000006 rms=0.000655 Jy/beam ! Combined flux in latest and established models = 0.671694 Jy selfcal ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 261 components and 0.671694 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=0.096843Jy sigma=0.000673 ! Fit after self-cal, rms=0.097008Jy sigma=0.000672 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000878228 Jy ! Component: 100 - total flux cleaned = 0.00172941 Jy ! Component: 150 - total flux cleaned = 0.00227677 Jy ! Component: 200 - total flux cleaned = 0.00278122 Jy ! Total flux subtracted in 200 components = 0.00278122 Jy ! Clean residual min=-0.002065 max=0.002460 Jy/beam ! Clean residual mean=0.000009 rms=0.000593 Jy/beam ! Combined flux in latest and established models = 0.674475 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 266 components and 0.674475 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=0.096889Jy sigma=0.000671 ! Fit after self-cal, rms=0.096884Jy sigma=0.000671 ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec selfcal true, true, soltime2 ! Performing amp+phase self-cal over 20 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.096884Jy sigma=0.000671 ! Fit after self-cal, rms=0.096899Jy sigma=0.000670 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=1.043 mas, bmaj=1.721 mas, bpa=-2.309 degrees ! Estimated noise=271.757 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000696235 Jy ! Component: 100 - total flux cleaned = 0.00167283 Jy ! Component: 150 - total flux cleaned = 0.00248423 Jy ! Component: 200 - total flux cleaned = 0.00322551 Jy ! Total flux subtracted in 200 components = 0.00322551 Jy ! Clean residual min=-0.001646 max=0.002041 Jy/beam ! Clean residual mean=0.000003 rms=0.000500 Jy/beam ! Combined flux in latest and established models = 0.677701 Jy selfcal ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 272 components and 0.677701 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=0.096793Jy sigma=0.000669 ! Fit after self-cal, rms=0.096790Jy sigma=0.000669 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000597008 Jy ! Component: 100 - total flux cleaned = 0.00114301 Jy ! Component: 150 - total flux cleaned = 0.00159328 Jy ! Component: 200 - total flux cleaned = 0.00201337 Jy ! Total flux subtracted in 200 components = 0.00201337 Jy ! Clean residual min=-0.001578 max=0.001845 Jy/beam ! Clean residual mean=0.000006 rms=0.000463 Jy/beam ! Combined flux in latest and established models = 0.679714 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 273 components and 0.679714 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=0.096730Jy sigma=0.000668 ! Fit after self-cal, rms=0.096726Jy sigma=0.000668 ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. win_mult = win_mult * 1.2 selfcal true, true, soltime2 ! Performing amp+phase self-cal over 20 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Correcting IF 9. ! ! Correcting IF 10. ! ! Correcting IF 11. ! ! Correcting IF 12. ! ! Fit before self-cal, rms=0.096726Jy sigma=0.000668 ! Fit after self-cal, rms=0.096200Jy sigma=0.000668 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=2.235 mas, bmaj=2.67 mas, bpa=-1.954 degrees ! Estimated noise=315.297 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00181941 Jy ! Component: 100 - total flux cleaned = 0.00265863 Jy ! Component: 150 - total flux cleaned = 0.00319746 Jy ! Component: 200 - total flux cleaned = 0.00368189 Jy ! Total flux subtracted in 200 components = 0.00368189 Jy ! Clean residual min=-0.001433 max=0.001757 Jy/beam ! Clean residual mean=0.000004 rms=0.000486 Jy/beam ! Combined flux in latest and established models = 0.683396 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 285 components and 0.683396 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=0.096159Jy sigma=0.000668 ! Fit after self-cal, rms=0.096155Jy sigma=0.000668 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000428654 Jy ! Component: 100 - total flux cleaned = 0.00073034 Jy ! Component: 150 - total flux cleaned = 0.000941348 Jy ! Component: 200 - total flux cleaned = 0.00113823 Jy ! Total flux subtracted in 200 components = 0.00113823 Jy ! Clean residual min=-0.001377 max=0.001606 Jy/beam ! Clean residual mean=0.000008 rms=0.000465 Jy/beam ! Combined flux in latest and established models = 0.684534 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 295 components and 0.684534 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=0.096133Jy sigma=0.000667 ! Fit after self-cal, rms=0.096130Jy sigma=0.000667 ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "************** FINISHED AMPLITUDE SELF-CAL **************" ! ************** FINISHED AMPLITUDE SELF-CAL ************** restore ! Inverting map and beam ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=1.041 mas, bmaj=1.714 mas, bpa=-1.839 degrees ! Estimated noise=269.836 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.041 x 1.714 at -1.839 degrees (North through East) ! Clean map min=-0.0011885 max=0.12046 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 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.8039 mas, bmaj=1.405 mas, bpa=-3.371 degrees ! Estimated noise=659.048 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.12442 Jy ! Component: 100 - total flux cleaned = 0.2066 Jy ! Component: 150 - total flux cleaned = 0.265903 Jy ! Component: 200 - total flux cleaned = 0.311769 Jy ! Total flux subtracted in 200 components = 0.311769 Jy ! Clean residual min=-0.012940 max=0.027353 Jy/beam ! Clean residual mean=-0.000078 rms=0.004714 Jy/beam ! Combined flux in latest and established models = 0.311769 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 49 model components to the UV plane model. ! The established model now contains 49 components and 0.311769 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=1.041 mas, bmaj=1.714 mas, bpa=-1.839 degrees ! Estimated noise=269.836 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 = 0.0609778 Jy ! Component: 100 - total flux cleaned = 0.107133 Jy ! Component: 150 - total flux cleaned = 0.144501 Jy ! Component: 200 - total flux cleaned = 0.175632 Jy ! Total flux subtracted in 200 components = 0.175632 Jy ! Clean residual min=-0.009449 max=0.019085 Jy/beam ! Clean residual mean=-0.000210 rms=0.003937 Jy/beam ! Combined flux in latest and established models = 0.4874 Jy ! Adding 113 model components to the UV plane model. ! The established model now contains 140 components and 0.4874 Jy ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0263103 Jy ! Component: 100 - total flux cleaned = 0.048668 Jy ! Component: 150 - total flux cleaned = 0.0678013 Jy ! Component: 200 - total flux cleaned = 0.0842615 Jy ! Total flux subtracted in 200 components = 0.0842615 Jy ! Clean residual min=-0.005652 max=0.010515 Jy/beam ! Clean residual mean=-0.000122 rms=0.002229 Jy/beam ! Combined flux in latest and established models = 0.571662 Jy ! Adding 77 model components to the UV plane model. ! The established model now contains 199 components and 0.571662 Jy ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Added new window around map position (0.4, -1.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0142826 Jy ! Component: 100 - total flux cleaned = 0.0266781 Jy ! Component: 150 - total flux cleaned = 0.0374926 Jy ! Component: 200 - total flux cleaned = 0.0469537 Jy ! Total flux subtracted in 200 components = 0.0469537 Jy ! Clean residual min=-0.003809 max=0.006277 Jy/beam ! Clean residual mean=-0.000071 rms=0.001344 Jy/beam ! Combined flux in latest and established models = 0.618615 Jy ! Adding 74 model components to the UV plane model. ! The established model now contains 250 components and 0.618615 Jy ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Added new window around map position (-2.2, -0.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00834559 Jy ! Component: 100 - total flux cleaned = 0.015653 Jy ! Component: 150 - total flux cleaned = 0.0220766 Jy ! Component: 200 - total flux cleaned = 0.0277342 Jy ! Total flux subtracted in 200 components = 0.0277342 Jy ! Clean residual min=-0.002727 max=0.003737 Jy/beam ! Clean residual mean=-0.000040 rms=0.000860 Jy/beam ! Combined flux in latest and established models = 0.646349 Jy ! Adding 70 model components to the UV plane model. ! The established model now contains 289 components and 0.646349 Jy ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Added new window around map position (0, 1.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00501331 Jy ! Component: 100 - total flux cleaned = 0.0094298 Jy ! Component: 150 - total flux cleaned = 0.0133398 Jy ! Component: 200 - total flux cleaned = 0.0168031 Jy ! Total flux subtracted in 200 components = 0.0168031 Jy ! Clean residual min=-0.002026 max=0.002358 Jy/beam ! Clean residual mean=-0.000021 rms=0.000602 Jy/beam ! Combined flux in latest and established models = 0.663152 Jy ! Adding 71 model components to the UV plane model. ! The established model now contains 319 components and 0.663152 Jy ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=2.235 mas, bmaj=2.67 mas, bpa=-1.954 degrees ! Estimated noise=315.297 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00503082 Jy ! Component: 100 - total flux cleaned = 0.00883855 Jy ! Component: 150 - total flux cleaned = 0.0118617 Jy ! Component: 200 - total flux cleaned = 0.014298 Jy ! Total flux subtracted in 200 components = 0.014298 Jy ! Clean residual min=-0.001423 max=0.001805 Jy/beam ! Clean residual mean=-0.000012 rms=0.000537 Jy/beam ! Combined flux in latest and established models = 0.67745 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 = 0.00153157 Jy ! Component: 100 - total flux cleaned = 0.00281378 Jy ! Component: 150 - total flux cleaned = 0.00356365 Jy ! Component: 200 - total flux cleaned = 0.00411805 Jy ! Total flux subtracted in 200 components = 0.00411805 Jy ! Clean residual min=-0.001279 max=0.001509 Jy/beam ! Clean residual mean=-0.000002 rms=0.000458 Jy/beam ! Combined flux in latest and established models = 0.681568 Jy ! Adding 103 model components to the UV plane model. ! The established model now contains 390 components and 0.681568 Jy ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=1.041 mas, bmaj=1.714 mas, bpa=-1.839 degrees ! Estimated noise=269.836 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000859634 Jy ! Component: 100 - total flux cleaned = -0.000491186 Jy ! Component: 150 - total flux cleaned = -0.000224735 Jy ! Component: 200 - total flux cleaned = -2.79666e-05 Jy ! Total flux subtracted in 200 components = -2.79666e-05 Jy ! Clean residual min=-0.001320 max=0.001324 Jy/beam ! Clean residual mean=0.000001 rms=0.000366 Jy/beam ! Combined flux in latest and established models = 0.68154 Jy selfcal ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 400 components and 0.68154 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=0.096163Jy sigma=0.000667 ! Fit after self-cal, rms=0.096064Jy sigma=0.000667 wmodel J2010+3322_X_2017_06_10_pus_map.mod ! Writing 400 model components to file: J2010+3322_X_2017_06_10_pus_map.mod wobs J2010+3322_X_2017_06_10_pus_uvs.fits ! Writing UV FITS file: J2010+3322_X_2017_06_10_pus_uvs.fits wwins J2010+3322_X_2017_06_10_pus_map.win ! wwins: Wrote 10 windows to J2010+3322_X_2017_06_10_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 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000502994 Jy ! Component: 100 - total flux cleaned = 0.000745974 Jy ! Component: 150 - total flux cleaned = 0.000936491 Jy ! Component: 200 - total flux cleaned = 0.00107974 Jy ! Component: 250 - total flux cleaned = 0.00125803 Jy ! Component: 300 - total flux cleaned = 0.00139243 Jy ! Component: 350 - total flux cleaned = 0.00148571 Jy ! Component: 400 - total flux cleaned = 0.00159489 Jy ! Component: 450 - total flux cleaned = 0.00166589 Jy ! Component: 500 - total flux cleaned = 0.00173578 Jy ! Component: 550 - total flux cleaned = 0.00178737 Jy ! Component: 600 - total flux cleaned = 0.00185483 Jy ! Component: 650 - total flux cleaned = 0.00187146 Jy ! Component: 700 - total flux cleaned = 0.00192052 Jy ! Component: 750 - total flux cleaned = 0.00195259 Jy ! Component: 800 - total flux cleaned = 0.0019997 Jy ! Component: 850 - total flux cleaned = 0.00201531 Jy ! Component: 900 - total flux cleaned = 0.00206133 Jy ! Component: 950 - total flux cleaned = 0.00215191 Jy ! Component: 1000 - total flux cleaned = 0.00213717 Jy ! Component: 1050 - total flux cleaned = 0.00221101 Jy ! Component: 1100 - total flux cleaned = 0.00226917 Jy ! Component: 1150 - total flux cleaned = 0.00234128 Jy ! Component: 1200 - total flux cleaned = 0.00239804 Jy ! Component: 1250 - total flux cleaned = 0.00248233 Jy ! Component: 1300 - total flux cleaned = 0.00249597 Jy ! Component: 1350 - total flux cleaned = 0.00256456 Jy ! Component: 1400 - total flux cleaned = 0.00260532 Jy ! Component: 1450 - total flux cleaned = 0.00265937 Jy ! Component: 1500 - total flux cleaned = 0.00272579 Jy ! Component: 1550 - total flux cleaned = 0.00273911 Jy ! Component: 1600 - total flux cleaned = 0.00284348 Jy ! Component: 1650 - total flux cleaned = 0.00286918 Jy ! Component: 1700 - total flux cleaned = 0.00285633 Jy ! Component: 1750 - total flux cleaned = 0.00288188 Jy ! Component: 1800 - total flux cleaned = 0.00296963 Jy ! Component: 1850 - total flux cleaned = 0.00296976 Jy ! Component: 1900 - total flux cleaned = 0.00301892 Jy ! Component: 1950 - total flux cleaned = 0.00295803 Jy ! Component: 2000 - total flux cleaned = 0.00297032 Jy ! Total flux subtracted in 2048 components = 0.0029703 Jy ! Clean residual min=-0.000617 max=0.000638 Jy/beam ! Clean residual mean=-0.000000 rms=0.000237 Jy/beam ! Combined flux in latest and established models = 0.684511 Jy keep ! Adding 157 model components to the UV plane model. ! The established model now contains 554 components and 0.68451 Jy ![Exited script file: muppet] wmap "J2010+3322_X_2017_06_10_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.041 x 1.714 at -1.839 degrees (North through East) ! Clean map min=-0.0011247 max=0.12144 Jy/beam ! Writing clean map to FITS file: J2010+3322_X_2017_06_10_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.121444 invert ! Inverting map ! Your choice of large map pixels excluded 0.0476% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000236648 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.584586 0.584586 1.16917 2.33835 4.67669 9.35338 18.7068 37.4135 74.8271 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0007 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.121 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.041 x 1.714 at -1.839 degrees (North through East) ! Clean map min=-0.0011247 max=0.12144 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 J2010+3322_X_2017_06_10_pus_uvs.log closed on Mon May 6 12:52:40 2019