! Started logfile: J0958+4725_X_2000_03_13_pus_uvs.log on Wed Apr 3 19:50:50 2013 obs J0958+4725_X_2000_03_13_pus_uva.fits ! Reading UV FITS file: J0958+4725_X_2000_03_13_pus_uva.fits ! AN table 1: 217 integrations on 190 of 190 possible baselines. ! AN table 2: 80 integrations on 190 of 190 possible baselines. ! AN table 3: 122 integrations on 190 of 190 possible baselines. ! Apparent sampling: 0.2743 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0958+4725 ! ! 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 8.40997e+09 8e+06 1 8e+06 ! 02 2 8.47997e+09 8e+06 1 8e+06 ! 03 3 8.79497e+09 8e+06 1 8e+06 ! 04 4 8.89997e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 2386 lines of history. ! ! Reading 87348 visibilities. select I ! Polarization I is unavailable. ! 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 = 512 print "field_cell =",field_cell ! field_cell = 0.2 print "taper_size =",taper_size ! taper_size = 70 ![@muppet J0958+4725_X_2000_03_13_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 2196 telescope corrections were flagged in sub-array 1. ! A total of 900 telescope corrections were flagged in sub-array 2. ! A total of 1831 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 2194 telescope corrections were flagged in sub-array 1. ! A total of 901 telescope corrections were flagged in sub-array 2. ! A total of 1837 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 2195 telescope corrections were flagged in sub-array 1. ! A total of 897 telescope corrections were flagged in sub-array 2. ! A total of 1832 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 2205 telescope corrections were flagged in sub-array 1. ! A total of 893 telescope corrections were flagged in sub-array 2. ! A total of 1833 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=0.732217Jy sigma=0.006325 ! Fit after self-cal, rms=0.276481Jy sigma=0.002063 ! 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 6.05% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! Estimated beam: bmin=0.5171 mas, bmaj=0.6914 mas, bpa=6.8 degrees ! Estimated noise=680.952 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 = 0.639824 Jy ! Component: 100 - total flux cleaned = 0.789058 Jy ! Total flux subtracted in 100 components = 0.789058 Jy ! Clean residual min=-0.016455 max=0.059658 Jy/beam ! Clean residual mean=-0.000029 rms=0.003462 Jy/beam ! Combined flux in latest and established models = 0.789058 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.789058 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.234406Jy sigma=0.001878 ! Fit after self-cal, rms=0.234401Jy sigma=0.001878 ! Inverting map ! Your choice of large map pixels excluded 6.05% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0667829 Jy ! Component: 100 - total flux cleaned = 0.104958 Jy ! Total flux subtracted in 100 components = 0.104958 Jy ! Clean residual min=-0.011762 max=0.019661 Jy/beam ! Clean residual mean=-0.000020 rms=0.002435 Jy/beam ! Combined flux in latest and established models = 0.894016 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 11 components and 0.894016 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.208423Jy sigma=0.001491 ! Fit after self-cal, rms=0.208397Jy sigma=0.001491 ! Inverting map ! Your choice of large map pixels excluded 6.05% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0251158 Jy ! Component: 100 - total flux cleaned = 0.0430268 Jy ! Total flux subtracted in 100 components = 0.0430268 Jy ! Clean residual min=-0.011486 max=0.015017 Jy/beam ! Clean residual mean=-0.000017 rms=0.002205 Jy/beam ! Combined flux in latest and established models = 0.937043 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 14 components and 0.937043 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.203776Jy sigma=0.001401 ! Fit after self-cal, rms=0.203754Jy sigma=0.001401 ! Inverting map ! Your choice of large map pixels excluded 6.05% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! Added new window around map position (-0.6, -1.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0094489 Jy ! Component: 100 - total flux cleaned = 0.0167688 Jy ! Total flux subtracted in 100 components = 0.0167688 Jy ! Clean residual min=-0.010827 max=0.013404 Jy/beam ! Clean residual mean=-0.000015 rms=0.002104 Jy/beam ! Combined flux in latest and established models = 0.953812 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 18 components and 0.953812 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.202621Jy sigma=0.001377 ! Fit after self-cal, rms=0.202585Jy sigma=0.001376 ! Inverting map ! Your choice of large map pixels excluded 6.05% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 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 6.05% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! Estimated beam: bmin=0.5998 mas, bmaj=0.8826 mas, bpa=-0.4783 degrees ! Estimated noise=308.835 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 = 0.0200553 Jy ! Component: 100 - total flux cleaned = 0.0309763 Jy ! Component: 150 - total flux cleaned = 0.0376455 Jy ! Component: 200 - total flux cleaned = 0.041167 Jy ! Total flux subtracted in 200 components = 0.041167 Jy ! Clean residual min=-0.008208 max=0.010539 Jy/beam ! Clean residual mean=0.000034 rms=0.001884 Jy/beam ! Combined flux in latest and established models = 0.994979 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 30 components and 0.994979 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.201858Jy sigma=0.001343 ! Fit after self-cal, rms=0.201817Jy sigma=0.001342 ! Inverting map ! Your choice of large map pixels excluded 6.05% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! Added new window around map position (1.8, -0.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00958747 Jy ! Component: 100 - total flux cleaned = 0.0106311 Jy ! Component: 150 - total flux cleaned = 0.0104197 Jy ! Component: 200 - total flux cleaned = 0.0100329 Jy ! Total flux subtracted in 200 components = 0.0100329 Jy ! Clean residual min=-0.008060 max=0.008540 Jy/beam ! Clean residual mean=0.000056 rms=0.001790 Jy/beam ! Combined flux in latest and established models = 1.00501 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 50 components and 1.00501 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.201310Jy sigma=0.001334 ! Fit after self-cal, rms=0.201258Jy sigma=0.001334 ! Inverting map ! Your choice of large map pixels excluded 6.05% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 102 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 0.97 GC 1.00 KP 1.03 ! LA 1.02 NL 0.99 OV 0.98 PT 1.03 ! SC 0.94 WF 1.06 HH 1.00* KK 1.08 ! MA 0.98 MC 0.99 MK 1.01 NY 0.92 ! ON 0.98 TS 1.05 WZ 0.97 HN 1.07 ! ! A total of 45 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.96 GC 1.02 KP 1.01 ! LA 0.99 NL 0.98 OV 0.93 PT 1.02 ! SC 1.07 WF 1.08 HH 1.00* KK 0.93 ! MA 1.00* MC 1.00* MK 0.99 NY 0.93 ! ON 0.99 TS 0.97 WZ 1.23 HN 1.21 ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 1.03 GC 1.06 KP 1.07 ! LA 1.05 NL 1.08 OV 1.01 PT 1.05 ! SC 1.00* WF 1.00* HH 1.00* KK 0.99 ! MA 1.58 MC 1.16 MK 0.93 NY 0.95 ! ON 0.99 TS 1.01 WZ 1.08 HN 1.00* ! ! ! Correcting IF 2. ! A total of 99 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 0.96 GC 0.99 KP 1.00 ! LA 0.98 NL 1.02 OV 0.96 PT 0.99 ! SC 0.93 WF 1.06 HH 1.00* KK 1.08 ! MA 0.99 MC 1.01 MK 1.05 NY 0.96 ! ON 0.97 TS 1.05 WZ 0.96 HN 1.00 ! ! A total of 42 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.95 GC 0.99 KP 0.98 ! LA 0.95 NL 1.00 OV 0.91 PT 0.98 ! SC 1.05 WF 1.07 HH 1.00* KK 0.92 ! MA 1.00* MC 1.00* MK 1.03 NY 0.96 ! ON 0.99 TS 0.98 WZ 1.24 HN 1.07 ! ! A total of 21 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 1.01 GC 1.03 KP 1.03 ! LA 1.03 NL 1.10 OV 0.97 PT 1.01 ! SC 1.00* WF 1.00* HH 1.00* KK 0.99 ! MA 1.25 MC 1.18 MK 0.96 NY 0.98 ! ON 0.98 TS 1.02 WZ 1.08 HN 1.00* ! ! ! Correcting IF 3. ! A total of 93 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.99 GC 1.00 KP 1.01 ! LA 0.96 NL 0.97 OV 0.97 PT 1.01 ! SC 0.95 WF 1.07 HH 1.00* KK 1.07 ! MA 0.98 MC 0.99 MK 1.01 NY 1.01 ! ON 0.97 TS 1.10 WZ 1.00 HN 1.03 ! ! A total of 45 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 0.98 GC 1.02 KP 0.98 ! LA 0.94 NL 0.97 OV 0.92 PT 1.01 ! SC 1.11 WF 1.08 HH 1.00* KK 0.91 ! MA 1.00* MC 1.00* MK 1.00 NY 0.98 ! ON 1.01 TS 1.01 WZ 1.26 HN 1.02 ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 FD 1.07 GC 1.04 KP 1.06 ! LA 1.03 NL 1.03 OV 1.00 PT 1.03 ! SC 1.00* WF 1.00* HH 1.00* KK 0.97 ! MA 1.27 MC 1.16 MK 0.92 NY 1.02 ! ON 1.00 TS 1.06 WZ 1.09 HN 1.00* ! ! ! Correcting IF 4. ! A total of 96 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.97 GC 1.00 KP 0.99 ! LA 0.98 NL 0.99 OV 0.97 PT 1.03 ! SC 1.00 WF 1.07 HH 1.00* KK 1.07 ! MA 0.95 MC 0.99 MK 1.03 NY 0.99 ! ON 0.98 TS 1.11 WZ 1.01 HN 1.02 ! ! A total of 45 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.96 GC 1.04 KP 0.97 ! LA 0.95 NL 0.97 OV 0.92 PT 1.03 ! SC 1.16 WF 1.08 HH 1.00* KK 0.92 ! MA 1.00* MC 1.00* MK 1.03 NY 0.98 ! ON 0.97 TS 1.02 WZ 1.23 HN 1.04 ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 1.06 GC 1.05 KP 1.03 ! LA 1.04 NL 1.05 OV 1.00 PT 1.05 ! SC 1.00* WF 1.00* HH 1.00* KK 1.01 ! MA 1.22 MC 1.13 MK 0.93 NY 1.02 ! ON 0.99 TS 1.05 WZ 1.12 HN 1.00* ! ! ! Fit before self-cal, rms=0.201258Jy sigma=0.001334 ! Fit after self-cal, rms=0.194748Jy sigma=0.001233 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! Estimated beam: bmin=0.6016 mas, bmaj=0.8932 mas, bpa=-0.7295 degrees ! Estimated noise=309.536 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 = -0.00599954 Jy ! Component: 100 - total flux cleaned = -0.0068323 Jy ! Component: 150 - total flux cleaned = -0.00726173 Jy ! Component: 200 - total flux cleaned = -0.00751041 Jy ! Total flux subtracted in 200 components = -0.00751041 Jy ! Clean residual min=-0.003904 max=0.003728 Jy/beam ! Clean residual mean=-0.000015 rms=0.000832 Jy/beam ! Combined flux in latest and established models = 0.997501 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 59 components and 0.997501 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194435Jy sigma=0.001231 ! Fit after self-cal, rms=0.194470Jy sigma=0.001231 ! Inverting map ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 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=0.194470Jy sigma=0.001231 ! Fit after self-cal, rms=0.193959Jy sigma=0.001219 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! Estimated beam: bmin=0.602 mas, bmaj=0.8939 mas, bpa=-1.14 degrees ! Estimated noise=309.131 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00449167 Jy ! Component: 100 - total flux cleaned = -0.005405 Jy ! Component: 150 - total flux cleaned = -0.00552793 Jy ! Component: 200 - total flux cleaned = -0.00552788 Jy ! Total flux subtracted in 200 components = -0.00552788 Jy ! Clean residual min=-0.002240 max=0.001984 Jy/beam ! Clean residual mean=-0.000008 rms=0.000507 Jy/beam ! Combined flux in latest and established models = 0.991973 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 65 components and 0.991973 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.193693Jy sigma=0.001217 ! Fit after self-cal, rms=0.193700Jy sigma=0.001217 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 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 = -0.000307311 Jy ! Component: 100 - total flux cleaned = -0.00030675 Jy ! Component: 150 - total flux cleaned = -0.000226894 Jy ! Component: 200 - total flux cleaned = -0.000156367 Jy ! Total flux subtracted in 200 components = -0.000156367 Jy ! Clean residual min=-0.002146 max=0.001957 Jy/beam ! Clean residual mean=-0.000008 rms=0.000493 Jy/beam ! Combined flux in latest and established models = 0.991817 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 73 components and 0.991817 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.193639Jy sigma=0.001216 ! Fit after self-cal, rms=0.193634Jy sigma=0.001216 ! Inverting map ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 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=0.193634Jy sigma=0.001216 ! Fit after self-cal, rms=0.194023Jy sigma=0.001215 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! Estimated beam: bmin=0.6021 mas, bmaj=0.8959 mas, bpa=-1.393 degrees ! Estimated noise=309.073 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00270141 Jy ! Component: 100 - total flux cleaned = -0.00310358 Jy ! Component: 150 - total flux cleaned = -0.00343569 Jy ! Component: 200 - total flux cleaned = -0.00336302 Jy ! Total flux subtracted in 200 components = -0.00336302 Jy ! Clean residual min=-0.001994 max=0.001904 Jy/beam ! Clean residual mean=-0.000012 rms=0.000448 Jy/beam ! Combined flux in latest and established models = 0.988454 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 75 components and 0.988454 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.193904Jy sigma=0.001214 ! Fit after self-cal, rms=0.193909Jy sigma=0.001214 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 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 = -0.00029266 Jy ! Component: 100 - total flux cleaned = -0.000170217 Jy ! Component: 150 - total flux cleaned = -0.000114719 Jy ! Component: 200 - total flux cleaned = -6.42591e-05 Jy ! Total flux subtracted in 200 components = -6.42591e-05 Jy ! Clean residual min=-0.001976 max=0.001863 Jy/beam ! Clean residual mean=-0.000013 rms=0.000440 Jy/beam ! Combined flux in latest and established models = 0.988389 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 78 components and 0.988389 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.193876Jy sigma=0.001214 ! Fit after self-cal, rms=0.193873Jy sigma=0.001214 ! Inverting map ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 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=0.193873Jy sigma=0.001214 ! Fit after self-cal, rms=0.194108Jy sigma=0.001214 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! Estimated beam: bmin=2.356 mas, bmaj=2.777 mas, bpa=48.41 degrees ! Estimated noise=439.975 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00193666 Jy ! Component: 100 - total flux cleaned = -0.00236713 Jy ! Component: 150 - total flux cleaned = -0.0024634 Jy ! Component: 200 - total flux cleaned = -0.00250379 Jy ! Total flux subtracted in 200 components = -0.00250379 Jy ! Clean residual min=-0.002172 max=0.001885 Jy/beam ! Clean residual mean=-0.000044 rms=0.000630 Jy/beam ! Combined flux in latest and established models = 0.985886 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 88 components and 0.985886 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194086Jy sigma=0.001214 ! Fit after self-cal, rms=0.194090Jy sigma=0.001214 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 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 = -0.000118143 Jy ! Component: 100 - total flux cleaned = -0.000118655 Jy ! Component: 150 - total flux cleaned = -0.000132788 Jy ! Component: 200 - total flux cleaned = -0.000132311 Jy ! Total flux subtracted in 200 components = -0.000132311 Jy ! Clean residual min=-0.002147 max=0.001879 Jy/beam ! Clean residual mean=-0.000045 rms=0.000633 Jy/beam ! Combined flux in latest and established models = 0.985753 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 91 components and 0.985753 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194086Jy sigma=0.001214 ! Fit after self-cal, rms=0.194085Jy sigma=0.001214 ! Inverting map ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 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 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! Estimated beam: bmin=0.602 mas, bmaj=0.8972 mas, bpa=-1.549 degrees ! Estimated noise=308.944 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.602 x 0.8972 at -1.549 degrees (North through East) ! Clean map min=-0.0020413 max=0.86201 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=0.194085Jy sigma=0.001214 ! Fit after self-cal, rms=0.185292Jy sigma=0.001149 ! Inverting map and beam ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! Estimated beam: bmin=0.6025 mas, bmaj=0.8968 mas, bpa=-1.529 degrees ! Estimated noise=308.71 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00155446 Jy ! Component: 100 - total flux cleaned = -0.00167919 Jy ! Component: 150 - total flux cleaned = -0.00167882 Jy ! Component: 200 - total flux cleaned = -0.00158187 Jy ! Total flux subtracted in 200 components = -0.00158187 Jy ! Clean residual min=-0.001698 max=0.001677 Jy/beam ! Clean residual mean=-0.000013 rms=0.000397 Jy/beam ! Combined flux in latest and established models = 0.984172 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 95 components and 0.984172 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.185239Jy sigma=0.001149 ! Fit after self-cal, rms=0.185236Jy sigma=0.001149 ! Inverting map ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000164291 Jy ! Component: 100 - total flux cleaned = -3.88922e-05 Jy ! Component: 150 - total flux cleaned = 3.86896e-05 Jy ! Component: 200 - total flux cleaned = 0.000110082 Jy ! Total flux subtracted in 200 components = 0.000110082 Jy ! Clean residual min=-0.001671 max=0.001677 Jy/beam ! Clean residual mean=-0.000012 rms=0.000393 Jy/beam ! Combined flux in latest and established models = 0.984282 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 96 components and 0.984282 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.185216Jy sigma=0.001149 ! Fit after self-cal, rms=0.185213Jy sigma=0.001149 ! Inverting map ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.185213Jy sigma=0.001149 ! Fit after self-cal, rms=0.185281Jy sigma=0.001148 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 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! Estimated beam: bmin=0.5222 mas, bmaj=0.6952 mas, bpa=4.893 degrees ! Estimated noise=692.743 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.652276 Jy ! Component: 100 - total flux cleaned = 0.798548 Jy ! Component: 150 - total flux cleaned = 0.857611 Jy ! Component: 200 - total flux cleaned = 0.891725 Jy ! Total flux subtracted in 200 components = 0.891725 Jy ! Clean residual min=-0.005235 max=0.018010 Jy/beam ! Clean residual mean=-0.000012 rms=0.001338 Jy/beam ! Combined flux in latest and established models = 0.891725 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 10 model components to the UV plane model. ! The established model now contains 10 components and 0.891725 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! Estimated beam: bmin=0.6024 mas, bmaj=0.8974 mas, bpa=-1.626 degrees ! Estimated noise=308.523 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 = 0.0388536 Jy ! Component: 100 - total flux cleaned = 0.0590322 Jy ! Component: 150 - total flux cleaned = 0.0702293 Jy ! Component: 200 - total flux cleaned = 0.0771356 Jy ! Total flux subtracted in 200 components = 0.0771356 Jy ! Clean residual min=-0.001920 max=0.004303 Jy/beam ! Clean residual mean=-0.000041 rms=0.000559 Jy/beam ! Combined flux in latest and established models = 0.968861 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 32 components and 0.968861 Jy ! Inverting map ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! Added new window around map position (0.6, -1). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00477242 Jy ! Component: 100 - total flux cleaned = 0.00812174 Jy ! Component: 150 - total flux cleaned = 0.0105729 Jy ! Component: 200 - total flux cleaned = 0.0123804 Jy ! Total flux subtracted in 200 components = 0.0123804 Jy ! Clean residual min=-0.001627 max=0.001769 Jy/beam ! Clean residual mean=-0.000015 rms=0.000401 Jy/beam ! Combined flux in latest and established models = 0.981241 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 49 components and 0.981241 Jy ! Inverting map ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! Added new window around map position (-2.2, -0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000867248 Jy ! Component: 100 - total flux cleaned = 0.00103294 Jy ! Component: 150 - total flux cleaned = 0.00118631 Jy ! Component: 200 - total flux cleaned = 0.00132834 Jy ! Total flux subtracted in 200 components = 0.00132834 Jy ! Clean residual min=-0.001569 max=0.001593 Jy/beam ! Clean residual mean=-0.000013 rms=0.000390 Jy/beam ! Combined flux in latest and established models = 0.98257 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 59 components and 0.98257 Jy ! Inverting map ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 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 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! Estimated beam: bmin=2.357 mas, bmaj=2.778 mas, bpa=48.39 degrees ! Estimated noise=438.78 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000372577 Jy ! Component: 100 - total flux cleaned = 0.000439204 Jy ! Component: 150 - total flux cleaned = 0.000463693 Jy ! Component: 200 - total flux cleaned = 0.000503952 Jy ! Total flux subtracted in 200 components = 0.000503952 Jy ! Clean residual min=-0.002106 max=0.001669 Jy/beam ! Clean residual mean=-0.000039 rms=0.000595 Jy/beam ! Combined flux in latest and established models = 0.983074 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 = -3.56797e-05 Jy ! Component: 100 - total flux cleaned = -5.16679e-05 Jy ! Component: 150 - total flux cleaned = -8.08469e-05 Jy ! Component: 200 - total flux cleaned = -0.000107197 Jy ! Total flux subtracted in 200 components = -0.000107197 Jy ! Clean residual min=-0.002102 max=0.001642 Jy/beam ! Clean residual mean=-0.000040 rms=0.000593 Jy/beam ! Combined flux in latest and established models = 0.982966 Jy ! Adding 19 model components to the UV plane model. ! The established model now contains 71 components and 0.982966 Jy ! Inverting map ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! Estimated beam: bmin=0.6024 mas, bmaj=0.8974 mas, bpa=-1.626 degrees ! Estimated noise=308.523 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000266812 Jy ! Component: 100 - total flux cleaned = -0.000264813 Jy ! Component: 150 - total flux cleaned = -0.000264534 Jy ! Component: 200 - total flux cleaned = -0.0002653 Jy ! Total flux subtracted in 200 components = -0.0002653 Jy ! Clean residual min=-0.001625 max=0.001568 Jy/beam ! Clean residual mean=-0.000012 rms=0.000381 Jy/beam ! Combined flux in latest and established models = 0.982701 Jy selfcal ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 81 components and 0.982701 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.185362Jy sigma=0.001150 ! Fit after self-cal, rms=0.185338Jy sigma=0.001149 wmodel J0958+4725_X_2000_03_13_pus_map.mod ! Writing 81 model components to file: J0958+4725_X_2000_03_13_pus_map.mod wobs J0958+4725_X_2000_03_13_pus_uvs.fits ! Writing UV FITS file: J0958+4725_X_2000_03_13_pus_uvs.fits wwins J0958+4725_X_2000_03_13_pus_map.win ! wwins: Wrote 5 windows to J0958+4725_X_2000_03_13_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 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 1.92188e-05 Jy ! Component: 100 - total flux cleaned = 7.46163e-05 Jy ! Component: 150 - total flux cleaned = 4.91851e-05 Jy ! Component: 200 - total flux cleaned = -7.71134e-05 Jy ! Component: 250 - total flux cleaned = -0.000151231 Jy ! Component: 300 - total flux cleaned = -0.000272519 Jy ! Component: 350 - total flux cleaned = -0.000296194 Jy ! Component: 400 - total flux cleaned = -0.000342896 Jy ! Component: 450 - total flux cleaned = -0.000389321 Jy ! Component: 500 - total flux cleaned = -0.000412259 Jy ! Component: 550 - total flux cleaned = -0.000502385 Jy ! Component: 600 - total flux cleaned = -0.000502342 Jy ! Component: 650 - total flux cleaned = -0.000635042 Jy ! Component: 700 - total flux cleaned = -0.000656794 Jy ! Component: 750 - total flux cleaned = -0.000700636 Jy ! Component: 800 - total flux cleaned = -0.000722193 Jy ! Component: 850 - total flux cleaned = -0.000850124 Jy ! Component: 900 - total flux cleaned = -0.000892346 Jy ! Component: 950 - total flux cleaned = -0.000997202 Jy ! Component: 1000 - total flux cleaned = -0.00103878 Jy ! Component: 1050 - total flux cleaned = -0.00118318 Jy ! Component: 1100 - total flux cleaned = -0.00120355 Jy ! Component: 1150 - total flux cleaned = -0.00126442 Jy ! Component: 1200 - total flux cleaned = -0.00126455 Jy ! Component: 1250 - total flux cleaned = -0.00136494 Jy ! Component: 1300 - total flux cleaned = -0.00136501 Jy ! Component: 1350 - total flux cleaned = -0.0014642 Jy ! Component: 1400 - total flux cleaned = -0.0015037 Jy ! Component: 1450 - total flux cleaned = -0.00152329 Jy ! Component: 1500 - total flux cleaned = -0.00146488 Jy ! Component: 1550 - total flux cleaned = -0.00158129 Jy ! Component: 1600 - total flux cleaned = -0.00156195 Jy ! Component: 1650 - total flux cleaned = -0.00160045 Jy ! Component: 1700 - total flux cleaned = -0.00158126 Jy ! Component: 1750 - total flux cleaned = -0.0015622 Jy ! Component: 1800 - total flux cleaned = -0.00163794 Jy ! Component: 1850 - total flux cleaned = -0.00163786 Jy ! Component: 1900 - total flux cleaned = -0.00169409 Jy ! Component: 1950 - total flux cleaned = -0.00167531 Jy ! Component: 2000 - total flux cleaned = -0.0016753 Jy ! Total flux subtracted in 2048 components = -0.00174929 Jy ! Clean residual min=-0.001016 max=0.001179 Jy/beam ! Clean residual mean=-0.000007 rms=0.000329 Jy/beam ! Combined flux in latest and established models = 0.980951 Jy keep ! Adding 183 model components to the UV plane model. ! The established model now contains 264 components and 0.980951 Jy ![Exited script file: muppet] wmap "J0958+4725_X_2000_03_13_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6024 x 0.8974 at -1.626 degrees (North through East) ! Clean map min=-0.0013966 max=0.86436 Jy/beam ! Writing clean map to FITS file: J0958+4725_X_2000_03_13_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.864357 invert ! Inverting map ! Your choice of large map pixels excluded 6.02% of the data. ! The x-axis pixel size should ideally be below 0.1565 milli-arcsec ! The y-axis pixel size should ideally be below 0.1873 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00032877 device "J0958+4725_X_2000_03_13_pus\_map.eps/VPS" ! Attempting to open device: 'J0958+4725_X_2000_03_13_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.114109 0.114109 0.228219 0.456437 0.912875 1.82575 3.6515 7.303 14.606 29.212 58.424 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0009 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.864 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6024 x 0.8974 at -1.626 degrees (North through East) ! Clean map min=-0.0013966 max=0.86436 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. quit ! Quitting program ! Log file J0958+4725_X_2000_03_13_pus_uvs.log closed on Wed Apr 3 19:51:10 2013