! Started logfile: /scr/pima/rdv72_uvs/J0102+5824_X_uvs.log on Sat Oct 5 08:43:49 2013 obs /scr/pima/rdv72_uvs/J0102+5824_X_uva.fits ! Reading UV FITS file: /scr/pima/rdv72_uvs/J0102+5824_X_uva.fits ! AN table 1: 5 integrations on 6 of 6 possible baselines. ! AN table 2: 5 integrations on 45 of 45 possible baselines. ! AN table 3: 6 integrations on 45 of 45 possible baselines. ! AN table 4: 5 integrations on 1 of 1 possible baselines. ! AN table 5: 14 integrations on 66 of 66 possible baselines. ! AN table 6: 10 integrations on 3 of 3 possible baselines. ! AN table 7: 4 integrations on 3 of 3 possible baselines. ! AN table 8: 2 integrations on 1 of 1 possible baselines. ! AN table 9: 6 integrations on 28 of 28 possible baselines. ! AN table 10: 6 integrations on 36 of 36 possible baselines. ! AN table 11: 6 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.852695 visibilities/baseline/integration-bin. ! Found source: J0102+5824 ! ! There are 4 IFs, and a total of 4 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.40599e+09 1.6e+07 1 1.6e+07 ! 02 2 8.47599e+09 1.6e+07 1 1.6e+07 ! 03 3 8.79099e+09 1.6e+07 1 1.6e+07 ! 04 4 8.89599e+09 1.6e+07 1 1.6e+07 ! ! Polarization(s): RR ! ! Read 0 lines of history. ! ! Reading 7340 visibilities. select RR ! Selecting polarization: RR, channels: 1..4 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 print "field_size =",field_size ! field_size = 1024 print "field_cell =",field_cell ! field_cell = 0.2 print "taper_size =",taper_size ! taper_size = 70 ![@/home/lpetrov/bin/01_muppet /scr/pima/rdv72_uvs/J0102+5824_X] 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 = 1024x1024 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 2 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 7 telescope corrections were flagged in sub-array 3. ! A total of 10 telescope corrections were flagged in sub-array 4. ! A total of 8 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 4 telescope corrections were flagged in sub-array 8. ! A total of 6 telescope corrections were flagged in sub-array 9. ! A total of 7 telescope corrections were flagged in sub-array 10. ! A total of 8 telescope corrections were flagged in sub-array 11. ! ! Correcting IF 2. ! A total of 2 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 7 telescope corrections were flagged in sub-array 3. ! A total of 10 telescope corrections were flagged in sub-array 4. ! A total of 8 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 4 telescope corrections were flagged in sub-array 8. ! A total of 6 telescope corrections were flagged in sub-array 9. ! A total of 7 telescope corrections were flagged in sub-array 10. ! A total of 8 telescope corrections were flagged in sub-array 11. ! ! Correcting IF 3. ! A total of 2 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 7 telescope corrections were flagged in sub-array 3. ! A total of 10 telescope corrections were flagged in sub-array 4. ! A total of 8 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 4 telescope corrections were flagged in sub-array 8. ! A total of 6 telescope corrections were flagged in sub-array 9. ! A total of 7 telescope corrections were flagged in sub-array 10. ! A total of 8 telescope corrections were flagged in sub-array 11. ! ! Correcting IF 4. ! A total of 2 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 7 telescope corrections were flagged in sub-array 3. ! A total of 10 telescope corrections were flagged in sub-array 4. ! A total of 8 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 4 telescope corrections were flagged in sub-array 8. ! A total of 6 telescope corrections were flagged in sub-array 9. ! A total of 7 telescope corrections were flagged in sub-array 10. ! A total of 8 telescope corrections were flagged in sub-array 11. ! ! Fit before self-cal, rms=1.680663Jy sigma=26.932829 ! Fit after self-cal, rms=0.556030Jy sigma=9.707583 ! 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 2.36% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Estimated beam: bmin=0.6083 mas, bmaj=0.7717 mas, bpa=57.85 degrees ! Estimated noise=0.875142 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 = 1.05235 Jy ! Component: 100 - total flux cleaned = 1.29906 Jy ! Total flux subtracted in 100 components = 1.29906 Jy ! Clean residual min=-0.044634 max=0.098006 Jy/beam ! Clean residual mean=0.000272 rms=0.010487 Jy/beam ! Combined flux in latest and established models = 1.29906 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 1.29906 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.453345Jy sigma=6.877446 ! Fit after self-cal, rms=0.452092Jy sigma=6.876269 ! Inverting map ! Your choice of large map pixels excluded 2.36% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.105761 Jy ! Component: 100 - total flux cleaned = 0.165095 Jy ! Total flux subtracted in 100 components = 0.165095 Jy ! Clean residual min=-0.044366 max=0.070795 Jy/beam ! Clean residual mean=0.000202 rms=0.009253 Jy/beam ! Combined flux in latest and established models = 1.46415 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 9 components and 1.46415 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.430996Jy sigma=5.959031 ! Fit after self-cal, rms=0.430801Jy sigma=5.956699 ! Inverting map ! Your choice of large map pixels excluded 2.36% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Added new window around map position (-0.4, -2.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0623084 Jy ! Component: 100 - total flux cleaned = 0.0961533 Jy ! Total flux subtracted in 100 components = 0.0961533 Jy ! Clean residual min=-0.045669 max=0.064346 Jy/beam ! Clean residual mean=0.000163 rms=0.008770 Jy/beam ! Combined flux in latest and established models = 1.5603 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 13 components and 1.5603 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.426928Jy sigma=5.640806 ! Fit after self-cal, rms=0.426112Jy sigma=5.621610 ! Inverting map ! Your choice of large map pixels excluded 2.36% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Added new window around map position (-1.6, -0.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0565929 Jy ! Component: 100 - total flux cleaned = 0.0917852 Jy ! Total flux subtracted in 100 components = 0.0917852 Jy ! Clean residual min=-0.042976 max=0.052566 Jy/beam ! Clean residual mean=0.000125 rms=0.008386 Jy/beam ! Combined flux in latest and established models = 1.65209 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 21 components and 1.65209 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.419151Jy sigma=5.379589 ! Fit after self-cal, rms=0.418229Jy sigma=5.362100 ! Inverting map ! Your choice of large map pixels excluded 2.36% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Added new window around map position (1.8, 1.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.047525 Jy ! Component: 100 - total flux cleaned = 0.0778468 Jy ! Total flux subtracted in 100 components = 0.0778468 Jy ! Clean residual min=-0.042110 max=0.045860 Jy/beam ! Clean residual mean=0.000094 rms=0.008081 Jy/beam ! Combined flux in latest and established models = 1.72994 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 31 components and 1.72994 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.413718Jy sigma=5.227159 ! Fit after self-cal, rms=0.413536Jy sigma=5.221644 ! Inverting map ! Your choice of large map pixels excluded 2.36% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 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 2.36% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Estimated beam: bmin=0.7259 mas, bmaj=0.8622 mas, bpa=73.32 degrees ! Estimated noise=0.608127 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 (-16.2, 24.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0677468 Jy ! Component: 100 - total flux cleaned = 0.106857 Jy ! Component: 150 - total flux cleaned = 0.137929 Jy ! Component: 200 - total flux cleaned = 0.156772 Jy ! Total flux subtracted in 200 components = 0.156772 Jy ! Clean residual min=-0.047478 max=0.057399 Jy/beam ! Clean residual mean=0.000116 rms=0.011212 Jy/beam ! Combined flux in latest and established models = 1.88671 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 49 components and 1.88671 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.408456Jy sigma=4.883798 ! Fit after self-cal, rms=0.407648Jy sigma=4.858022 ! Inverting map ! Your choice of large map pixels excluded 2.36% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! NY 1.19 SC 0.83 WZ 1.14 ZC 1.70 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.22 FD 0.79 KP 0.97 LA 0.91 ! NL 1.11 NY 1.09 OV 1.03 PT 0.91 ! SC 0.81 ZC 1.43 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.41 FD 0.78 KK 1.28 KP 0.98 ! LA 0.98 MK 0.98 NL 1.04 OV 0.99 ! PT 0.93 SC 0.80 ! ! Telescope amplitude corrections in sub-array 4: ! NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.16 FD 0.78 KK 1.17 KP 1.20 ! LA 0.93 MK 1.00 NL 0.98 NY 0.92 ! OV 0.96 SC 0.87 WZ 0.97 ZC 17.26 ! ! A total of 24 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! NY 0.00* WZ 0.00* ZC 0.00* ! ! A total of 12 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 0.00* NY 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.00* NY 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! BR 1.45 LA 1.01 NL 1.17 NY 1.13 ! OV 1.10 PT 1.07 WZ 1.13 ZC 1.12 ! ! A total of 3 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! BR 1.34 LA 1.03 NL 1.12 NY 1.07 ! OV 1.00 PT 0.98 SC 0.96 WZ 1.16 ! ZC 1.09 ! ! A total of 3 telescope corrections were flagged in sub-array 11. ! Telescope amplitude corrections in sub-array 11: ! FD 0.83 KP 1.85 LA 0.99 NL 1.14 ! NY 1.05 OV 0.99 PT 1.02 SC 0.83 ! WZ 1.15 ZC 1.16 ! ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! NY 1.18 SC 0.84 WZ 1.15 ZC 1.63 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.20 FD 0.79 KP 0.93 LA 0.89 ! NL 1.12 NY 1.12 OV 1.02 PT 0.97 ! SC 0.84 ZC 1.39 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.39 FD 0.79 KK 1.16 KP 0.94 ! LA 0.98 MK 1.01 NL 1.03 OV 0.97 ! PT 0.95 SC 0.82 ! ! Telescope amplitude corrections in sub-array 4: ! NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.14 FD 0.78 KK 1.12 KP 1.16 ! LA 0.91 MK 1.01 NL 0.97 NY 0.94 ! OV 0.95 SC 0.89 WZ 0.96 ZC 17.76 ! ! A total of 24 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! NY 0.00* WZ 0.00* ZC 0.00* ! ! A total of 12 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 0.00* NY 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.00* NY 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! BR 1.40 LA 1.01 NL 1.13 NY 1.16 ! OV 1.05 PT 1.13 WZ 1.10 ZC 1.13 ! ! A total of 3 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! BR 1.37 LA 1.03 NL 1.09 NY 1.10 ! OV 1.01 PT 1.03 SC 0.98 WZ 1.17 ! ZC 1.05 ! ! A total of 3 telescope corrections were flagged in sub-array 11. ! Telescope amplitude corrections in sub-array 11: ! FD 0.84 KP 1.75 LA 0.99 NL 1.11 ! NY 1.07 OV 1.00 PT 1.06 SC 0.86 ! WZ 1.14 ZC 1.15 ! ! ! Correcting IF 3. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! NY 1.26 SC 0.82 WZ 1.16 ZC 1.39 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.23 FD 0.77 KP 0.87 LA 0.92 ! NL 1.15 NY 1.15 OV 1.07 PT 0.97 ! SC 0.86 ZC 1.15 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.46 FD 0.79 KK 1.18 KP 0.84 ! LA 1.00 MK 0.99 NL 1.08 OV 1.00 ! PT 0.95 SC 0.84 ! ! Telescope amplitude corrections in sub-array 4: ! NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.21 FD 0.76 KK 1.17 KP 1.08 ! LA 0.95 MK 0.98 NL 1.02 NY 0.96 ! OV 0.98 SC 0.91 WZ 1.00 ZC 13.44 ! ! A total of 24 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! NY 0.00* WZ 0.00* ZC 0.00* ! ! A total of 12 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 0.00* NY 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.00* NY 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! BR 1.44 LA 1.06 NL 1.16 NY 1.20 ! OV 1.08 PT 1.13 WZ 1.15 ZC 0.94 ! ! A total of 3 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! BR 1.42 LA 1.04 NL 1.14 NY 1.13 ! OV 1.06 PT 1.02 SC 0.95 WZ 1.16 ! ZC 0.91 ! ! A total of 3 telescope corrections were flagged in sub-array 11. ! Telescope amplitude corrections in sub-array 11: ! FD 0.84 KP 1.70 LA 1.02 NL 1.20 ! NY 1.09 OV 1.03 PT 1.07 SC 0.88 ! WZ 1.18 ZC 0.94 ! ! ! Correcting IF 4. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! NY 1.32 SC 0.84 WZ 1.17 ZC 1.47 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.21 FD 0.82 KP 0.93 LA 0.93 ! NL 1.19 NY 1.12 OV 1.05 PT 0.97 ! SC 0.85 ZC 1.24 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.49 FD 0.82 KK 1.14 KP 0.91 ! LA 1.00 MK 1.02 NL 1.14 OV 1.00 ! PT 0.95 SC 0.83 ! ! Telescope amplitude corrections in sub-array 4: ! NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.23 FD 0.79 KK 1.14 KP 1.17 ! LA 0.95 MK 1.02 NL 1.05 NY 0.92 ! OV 0.96 SC 0.91 WZ 1.02 ZC 15.73 ! ! A total of 24 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! NY 0.00* WZ 0.00* ZC 0.00* ! ! A total of 12 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 0.00* NY 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.00* NY 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! BR 1.42 LA 1.05 NL 1.16 NY 1.20 ! OV 1.09 PT 1.16 WZ 1.17 ZC 0.97 ! ! A total of 3 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! BR 1.34 LA 1.03 NL 1.14 NY 1.10 ! OV 1.05 PT 1.02 SC 0.98 WZ 1.20 ! ZC 0.95 ! ! A total of 3 telescope corrections were flagged in sub-array 11. ! Telescope amplitude corrections in sub-array 11: ! FD 0.88 KP 1.75 LA 1.05 NL 1.23 ! NY 1.08 OV 1.02 PT 1.05 SC 0.90 ! WZ 1.19 ZC 0.95 ! ! ! Fit before self-cal, rms=0.407648Jy sigma=4.858022 ! Fit after self-cal, rms=0.378315Jy sigma=2.193001 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Estimated beam: bmin=0.7263 mas, bmaj=0.8659 mas, bpa=72.36 degrees ! Estimated noise=0.61232 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 = -0.0268165 Jy ! Component: 100 - total flux cleaned = -0.0431547 Jy ! Component: 150 - total flux cleaned = -0.05221 Jy ! Component: 200 - total flux cleaned = -0.05652 Jy ! Total flux subtracted in 200 components = -0.05652 Jy ! Clean residual min=-0.016323 max=0.020013 Jy/beam ! Clean residual mean=0.000033 rms=0.002798 Jy/beam ! Combined flux in latest and established models = 1.83019 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 68 components and 1.83019 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.376226Jy sigma=2.107752 ! Fit after self-cal, rms=0.376117Jy sigma=2.100259 ! Inverting map ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Added new window around map position (-0.4, -0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0101743 Jy ! Component: 100 - total flux cleaned = 0.00581775 Jy ! Component: 150 - total flux cleaned = 0.00121982 Jy ! Component: 200 - total flux cleaned = -0.0017762 Jy ! Total flux subtracted in 200 components = -0.0017762 Jy ! Clean residual min=-0.013967 max=0.012823 Jy/beam ! Clean residual mean=0.000030 rms=0.002537 Jy/beam ! Combined flux in latest and established models = 1.82841 Jy ! Performing phase self-cal ! Adding 32 model components to the UV plane model. ! The established model now contains 78 components and 1.82841 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.374926Jy sigma=2.047950 ! Fit after self-cal, rms=0.374800Jy sigma=2.044786 ! Inverting map ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 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. ! ! Fit before self-cal, rms=0.374800Jy sigma=2.044786 ! Fit after self-cal, rms=0.372808Jy sigma=1.986132 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Estimated beam: bmin=0.7276 mas, bmaj=0.8637 mas, bpa=72.55 degrees ! Estimated noise=0.610904 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0118558 Jy ! Component: 100 - total flux cleaned = -0.0188687 Jy ! Component: 150 - total flux cleaned = -0.0236322 Jy ! Component: 200 - total flux cleaned = -0.0271024 Jy ! Total flux subtracted in 200 components = -0.0271024 Jy ! Clean residual min=-0.012753 max=0.009256 Jy/beam ! Clean residual mean=0.000018 rms=0.002174 Jy/beam ! Combined flux in latest and established models = 1.80131 Jy selfcal ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 82 components and 1.80131 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.371821Jy sigma=1.945806 ! Fit after self-cal, rms=0.371715Jy sigma=1.943625 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 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 = -0.00357176 Jy ! Component: 100 - total flux cleaned = -0.00572697 Jy ! Component: 150 - total flux cleaned = -0.00825431 Jy ! Component: 200 - total flux cleaned = -0.0100647 Jy ! Total flux subtracted in 200 components = -0.0100647 Jy ! Clean residual min=-0.011681 max=0.009355 Jy/beam ! Clean residual mean=0.000019 rms=0.002093 Jy/beam ! Combined flux in latest and established models = 1.79124 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 85 components and 1.79124 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.371228Jy sigma=1.925374 ! Fit after self-cal, rms=0.371172Jy sigma=1.924653 ! Inverting map ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 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. ! ! Fit before self-cal, rms=0.371172Jy sigma=1.924653 ! Fit after self-cal, rms=0.371076Jy sigma=1.909516 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Estimated beam: bmin=0.7295 mas, bmaj=0.862 mas, bpa=72.75 degrees ! Estimated noise=0.609977 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0116081 Jy ! Component: 100 - total flux cleaned = -0.0171802 Jy ! Component: 150 - total flux cleaned = -0.019841 Jy ! Component: 200 - total flux cleaned = -0.0214432 Jy ! Total flux subtracted in 200 components = -0.0214432 Jy ! Clean residual min=-0.010895 max=0.008078 Jy/beam ! Clean residual mean=0.000015 rms=0.001907 Jy/beam ! Combined flux in latest and established models = 1.7698 Jy selfcal ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 87 components and 1.7698 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.370329Jy sigma=1.884568 ! Fit after self-cal, rms=0.370273Jy sigma=1.883548 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 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 = -0.00277049 Jy ! Component: 100 - total flux cleaned = -0.00443767 Jy ! Component: 150 - total flux cleaned = -0.00597362 Jy ! Component: 200 - total flux cleaned = -0.00760239 Jy ! Total flux subtracted in 200 components = -0.00760239 Jy ! Clean residual min=-0.010119 max=0.008232 Jy/beam ! Clean residual mean=0.000016 rms=0.001863 Jy/beam ! Combined flux in latest and established models = 1.7622 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 88 components and 1.7622 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.369912Jy sigma=1.872075 ! Fit after self-cal, rms=0.369878Jy sigma=1.871666 ! Inverting map ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 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. ! ! Fit before self-cal, rms=0.369878Jy sigma=1.871666 ! Fit after self-cal, rms=0.371036Jy sigma=1.861023 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Estimated beam: bmin=2.378 mas, bmaj=2.939 mas, bpa=-32.09 degrees ! Estimated noise=0.85903 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0123751 Jy ! Component: 100 - total flux cleaned = -0.0204027 Jy ! Component: 150 - total flux cleaned = -0.0258985 Jy ! Component: 200 - total flux cleaned = -0.028192 Jy ! Total flux subtracted in 200 components = -0.028192 Jy ! Clean residual min=-0.011650 max=0.009768 Jy/beam ! Clean residual mean=0.000040 rms=0.002665 Jy/beam ! Combined flux in latest and established models = 1.73401 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 101 components and 1.73401 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.371084Jy sigma=1.856332 ! Fit after self-cal, rms=0.371054Jy sigma=1.855008 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 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 = -0.00328256 Jy ! Component: 100 - total flux cleaned = -0.00436561 Jy ! Component: 150 - total flux cleaned = -0.00532787 Jy ! Component: 200 - total flux cleaned = -0.00607912 Jy ! Total flux subtracted in 200 components = -0.00607912 Jy ! Clean residual min=-0.011049 max=0.010193 Jy/beam ! Clean residual mean=0.000042 rms=0.002652 Jy/beam ! Combined flux in latest and established models = 1.72793 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 109 components and 1.72793 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.371115Jy sigma=1.857019 ! Fit after self-cal, rms=0.371108Jy sigma=1.856817 ! Inverting map ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 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 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Estimated beam: bmin=0.7317 mas, bmaj=0.8606 mas, bpa=72.94 degrees ! Estimated noise=0.609218 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7317 x 0.8606 at 72.94 degrees (North through East) ! Clean map min=-0.0082567 max=1.3646 Jy/beam if(peak(flux) > thresh) selfcal true, true clean clean_niter,clean_gain selfcal flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) selfcal true, true end if ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.371108Jy sigma=1.856817 ! Fit after self-cal, rms=0.526951Jy sigma=1.648759 ! Inverting map and beam ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Estimated beam: bmin=0.7323 mas, bmaj=0.8613 mas, bpa=73.04 degrees ! Estimated noise=0.608787 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00852569 Jy ! Component: 100 - total flux cleaned = -0.0109334 Jy ! Component: 150 - total flux cleaned = -0.0116324 Jy ! Component: 200 - total flux cleaned = -0.0122789 Jy ! Total flux subtracted in 200 components = -0.0122789 Jy ! Clean residual min=-0.007852 max=0.007219 Jy/beam ! Clean residual mean=0.000011 rms=0.001622 Jy/beam ! Combined flux in latest and established models = 1.71565 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 113 components and 1.71565 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.526620Jy sigma=1.631768 ! Fit after self-cal, rms=0.526629Jy sigma=1.631245 ! Inverting map ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00109347 Jy ! Component: 100 - total flux cleaned = -0.00166833 Jy ! Component: 150 - total flux cleaned = -0.00220679 Jy ! Component: 200 - total flux cleaned = -0.00270827 Jy ! Total flux subtracted in 200 components = -0.00270827 Jy ! Clean residual min=-0.007701 max=0.007004 Jy/beam ! Clean residual mean=0.000012 rms=0.001596 Jy/beam ! Combined flux in latest and established models = 1.71294 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 115 components and 1.71294 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.526483Jy sigma=1.623573 ! Fit after self-cal, rms=0.526478Jy sigma=1.623343 ! Inverting map ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.526478Jy sigma=1.623343 ! Fit after self-cal, rms=0.531782Jy sigma=1.616855 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 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Estimated beam: bmin=0.613 mas, bmaj=0.7721 mas, bpa=56.52 degrees ! Estimated noise=0.902139 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.07226 Jy ! Component: 100 - total flux cleaned = 1.31509 Jy ! Component: 150 - total flux cleaned = 1.40922 Jy ! Component: 200 - total flux cleaned = 1.46683 Jy ! Total flux subtracted in 200 components = 1.46683 Jy ! Clean residual min=-0.014046 max=0.031448 Jy/beam ! Clean residual mean=0.000108 rms=0.003106 Jy/beam ! Combined flux in latest and established models = 1.46683 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 18 model components to the UV plane model. ! The established model now contains 18 components and 1.46683 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Estimated beam: bmin=0.7344 mas, bmaj=0.8604 mas, bpa=73.25 degrees ! Estimated noise=0.607947 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 = 0.0634557 Jy ! Component: 100 - total flux cleaned = 0.103148 Jy ! Component: 150 - total flux cleaned = 0.13147 Jy ! Component: 200 - total flux cleaned = 0.152629 Jy ! Total flux subtracted in 200 components = 0.152629 Jy ! Clean residual min=-0.009466 max=0.014301 Jy/beam ! Clean residual mean=0.000041 rms=0.002376 Jy/beam ! Combined flux in latest and established models = 1.61945 Jy ! Adding 45 model components to the UV plane model. ! The established model now contains 53 components and 1.61945 Jy ! Inverting map ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Added new window around map position (-0.2, 0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.017017 Jy ! Component: 100 - total flux cleaned = 0.0305612 Jy ! Component: 150 - total flux cleaned = 0.0416149 Jy ! Component: 200 - total flux cleaned = 0.0506947 Jy ! Total flux subtracted in 200 components = 0.0506947 Jy ! Clean residual min=-0.007901 max=0.008028 Jy/beam ! Clean residual mean=0.000023 rms=0.001742 Jy/beam ! Combined flux in latest and established models = 1.67015 Jy ! Adding 42 model components to the UV plane model. ! The established model now contains 77 components and 1.67015 Jy ! Inverting map ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Added new window around map position (-11.2, -12.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00852975 Jy ! Component: 100 - total flux cleaned = 0.0149147 Jy ! Component: 150 - total flux cleaned = 0.0190418 Jy ! Component: 200 - total flux cleaned = 0.0226718 Jy ! Total flux subtracted in 200 components = 0.0226718 Jy ! Clean residual min=-0.007291 max=0.006746 Jy/beam ! Clean residual mean=0.000019 rms=0.001551 Jy/beam ! Combined flux in latest and established models = 1.69282 Jy ! Adding 37 model components to the UV plane model. ! The established model now contains 93 components and 1.69282 Jy ! Inverting map ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 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 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Estimated beam: bmin=2.384 mas, bmaj=2.948 mas, bpa=-32.15 degrees ! Estimated noise=0.853102 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00692803 Jy ! Component: 100 - total flux cleaned = 0.0087538 Jy ! Component: 150 - total flux cleaned = 0.0099252 Jy ! Component: 200 - total flux cleaned = 0.0102082 Jy ! Total flux subtracted in 200 components = 0.0102082 Jy ! Clean residual min=-0.009844 max=0.008769 Jy/beam ! Clean residual mean=0.000042 rms=0.002342 Jy/beam ! Combined flux in latest and established models = 1.70303 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 = 0.000139674 Jy ! Component: 100 - total flux cleaned = 0.000376933 Jy ! Component: 150 - total flux cleaned = 0.000482441 Jy ! Component: 200 - total flux cleaned = 0.00059326 Jy ! Total flux subtracted in 200 components = 0.00059326 Jy ! Clean residual min=-0.009692 max=0.008204 Jy/beam ! Clean residual mean=0.000040 rms=0.002298 Jy/beam ! Combined flux in latest and established models = 1.70362 Jy ! Adding 31 model components to the UV plane model. ! The established model now contains 121 components and 1.70362 Jy ! Inverting map ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! Estimated beam: bmin=0.7344 mas, bmaj=0.8604 mas, bpa=73.25 degrees ! Estimated noise=0.607947 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000346361 Jy ! Component: 100 - total flux cleaned = 0.00120018 Jy ! Component: 150 - total flux cleaned = 0.00168446 Jy ! Component: 200 - total flux cleaned = 0.0020213 Jy ! Total flux subtracted in 200 components = 0.0020213 Jy ! Clean residual min=-0.006861 max=0.006585 Jy/beam ! Clean residual mean=0.000014 rms=0.001446 Jy/beam ! Combined flux in latest and established models = 1.70564 Jy selfcal ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 137 components and 1.70564 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.530738Jy sigma=1.570804 ! Fit after self-cal, rms=0.530470Jy sigma=1.560054 wmodel /scr/pima/rdv72_uvs/J0102+5824_X_map.mod ! Writing 137 model components to file: /scr/pima/rdv72_uvs/J0102+5824_X_map.mod wobs /scr/pima/rdv72_uvs/J0102+5824_X_uvs.fits ! Writing UV FITS file: /scr/pima/rdv72_uvs/J0102+5824_X_uvs.fits wwins /scr/pima/rdv72_uvs/J0102+5824_X_map.win ! wwins: Wrote 8 windows to /scr/pima/rdv72_uvs/J0102+5824_X_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 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00210829 Jy ! Component: 100 - total flux cleaned = -0.00369983 Jy ! Component: 150 - total flux cleaned = -0.00500575 Jy ! Component: 200 - total flux cleaned = -0.00616044 Jy ! Component: 250 - total flux cleaned = -0.00656908 Jy ! Component: 300 - total flux cleaned = -0.00746505 Jy ! Component: 350 - total flux cleaned = -0.00804973 Jy ! Component: 400 - total flux cleaned = -0.00881629 Jy ! Component: 450 - total flux cleaned = -0.00975774 Jy ! Component: 500 - total flux cleaned = -0.010406 Jy ! Component: 550 - total flux cleaned = -0.0113142 Jy ! Component: 600 - total flux cleaned = -0.0118511 Jy ! Component: 650 - total flux cleaned = -0.0126463 Jy ! Component: 700 - total flux cleaned = -0.0133443 Jy ! Component: 750 - total flux cleaned = -0.0142898 Jy ! Component: 800 - total flux cleaned = -0.0145433 Jy ! Component: 850 - total flux cleaned = -0.0152996 Jy ! Component: 900 - total flux cleaned = -0.0157135 Jy ! Component: 950 - total flux cleaned = -0.0161246 Jy ! Component: 1000 - total flux cleaned = -0.0165313 Jy ! Component: 1050 - total flux cleaned = -0.0170943 Jy ! Component: 1100 - total flux cleaned = -0.0171733 Jy ! Component: 1150 - total flux cleaned = -0.0178836 Jy ! Component: 1200 - total flux cleaned = -0.0182739 Jy ! Component: 1250 - total flux cleaned = -0.0184285 Jy ! Component: 1300 - total flux cleaned = -0.0188883 Jy ! Component: 1350 - total flux cleaned = -0.0192674 Jy ! Component: 1400 - total flux cleaned = -0.0192682 Jy ! Component: 1450 - total flux cleaned = -0.0197156 Jy ! Component: 1500 - total flux cleaned = -0.0201593 Jy ! Component: 1550 - total flux cleaned = -0.0202325 Jy ! Component: 1600 - total flux cleaned = -0.0202332 Jy ! Component: 1650 - total flux cleaned = -0.020956 Jy ! Component: 1700 - total flux cleaned = -0.0208849 Jy ! Component: 1750 - total flux cleaned = -0.0209576 Jy ! Component: 1800 - total flux cleaned = -0.021311 Jy ! Component: 1850 - total flux cleaned = -0.0215224 Jy ! Component: 1900 - total flux cleaned = -0.0218007 Jy ! Component: 1950 - total flux cleaned = -0.0222846 Jy ! Component: 2000 - total flux cleaned = -0.0224901 Jy ! Component: 2050 - total flux cleaned = -0.0226253 Jy ! Component: 2100 - total flux cleaned = -0.0229644 Jy ! Component: 2150 - total flux cleaned = -0.0231664 Jy ! Component: 2200 - total flux cleaned = -0.023634 Jy ! Component: 2250 - total flux cleaned = -0.0239669 Jy ! Component: 2300 - total flux cleaned = -0.0242303 Jy ! Component: 2350 - total flux cleaned = -0.0240989 Jy ! Component: 2400 - total flux cleaned = -0.0246217 Jy ! Component: 2450 - total flux cleaned = -0.0246868 Jy ! Component: 2500 - total flux cleaned = -0.0249453 Jy ! Component: 2550 - total flux cleaned = -0.0251377 Jy ! Component: 2600 - total flux cleaned = -0.0255205 Jy ! Component: 2650 - total flux cleaned = -0.0258375 Jy ! Component: 2700 - total flux cleaned = -0.0258375 Jy ! Component: 2750 - total flux cleaned = -0.0260884 Jy ! Component: 2800 - total flux cleaned = -0.0263377 Jy ! Component: 2850 - total flux cleaned = -0.0264615 Jy ! Component: 2900 - total flux cleaned = -0.026708 Jy ! Component: 2950 - total flux cleaned = -0.0265846 Jy ! Component: 3000 - total flux cleaned = -0.0269513 Jy ! Component: 3050 - total flux cleaned = -0.0270724 Jy ! Component: 3100 - total flux cleaned = -0.0273141 Jy ! Component: 3150 - total flux cleaned = -0.0274948 Jy ! Component: 3200 - total flux cleaned = -0.0276743 Jy ! Component: 3250 - total flux cleaned = -0.0277928 Jy ! Component: 3300 - total flux cleaned = -0.0279117 Jy ! Component: 3350 - total flux cleaned = -0.0280885 Jy ! Component: 3400 - total flux cleaned = -0.0283231 Jy ! Component: 3450 - total flux cleaned = -0.0283814 Jy ! Component: 3500 - total flux cleaned = -0.028498 Jy ! Component: 3550 - total flux cleaned = -0.0287879 Jy ! Component: 3600 - total flux cleaned = -0.0289032 Jy ! Component: 3650 - total flux cleaned = -0.0289606 Jy ! Component: 3700 - total flux cleaned = -0.0290179 Jy ! Component: 3750 - total flux cleaned = -0.0294154 Jy ! Component: 3800 - total flux cleaned = -0.029698 Jy ! Component: 3850 - total flux cleaned = -0.0298103 Jy ! Component: 3900 - total flux cleaned = -0.0301469 Jy ! Component: 3950 - total flux cleaned = -0.0301467 Jy ! Component: 4000 - total flux cleaned = -0.0303129 Jy ! Component: 4050 - total flux cleaned = -0.0304236 Jy ! Total flux subtracted in 4096 components = -0.0304789 Jy ! Clean residual min=-0.003326 max=0.002868 Jy/beam ! Clean residual mean=0.000006 rms=0.000914 Jy/beam ! Combined flux in latest and established models = 1.67516 Jy keep ! Adding 376 model components to the UV plane model. ! The established model now contains 513 components and 1.67516 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/rdv72_uvs/J0102+5824_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7344 x 0.8604 at 73.25 degrees (North through East) ! Clean map min=-0.0052044 max=1.3729 Jy/beam ! Writing clean map to FITS file: /scr/pima/rdv72_uvs/J0102+5824_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 1.37289 invert ! Inverting map ! Your choice of large map pixels excluded 2.43% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! The y-axis pixel size should ideally be below 0.1707 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000913291 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.19957 0.19957 0.39914 0.79828 1.59656 3.19312 6.38624 12.7725 25.5449 51.0899 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0027 print "peak=",int(1000*peak_flux)/1000 ! peak= 1.372 quit ! Quitting program ! Log file /scr/pima/rdv72_uvs/J0102+5824_X_uvs.log closed on Sat Oct 5 08:43:53 2013