! Started logfile: J0017+8135_X_2000_03_13_pus_uvs.log on Wed Apr 3 15:18:13 2013 obs J0017+8135_X_2000_03_13_pus_uva.fits ! Reading UV FITS file: J0017+8135_X_2000_03_13_pus_uva.fits ! AN table 1: 166 integrations on 190 of 190 possible baselines. ! AN table 2: 139 integrations on 190 of 190 possible baselines. ! AN table 3: 154 integrations on 190 of 190 possible baselines. ! Apparent sampling: 0.27928 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0017+8135 ! ! 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 97424 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 J0017+8135_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 2015 telescope corrections were flagged in sub-array 1. ! A total of 1475 telescope corrections were flagged in sub-array 2. ! A total of 1955 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 2066 telescope corrections were flagged in sub-array 1. ! A total of 1474 telescope corrections were flagged in sub-array 2. ! A total of 1958 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 2010 telescope corrections were flagged in sub-array 1. ! A total of 1469 telescope corrections were flagged in sub-array 2. ! A total of 1956 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 2021 telescope corrections were flagged in sub-array 1. ! A total of 1479 telescope corrections were flagged in sub-array 2. ! A total of 1965 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=0.891726Jy sigma=0.008009 ! Fit after self-cal, rms=0.625735Jy sigma=0.005324 ! 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 4.24% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=0.5068 mas, bmaj=0.5462 mas, bpa=81.14 degrees ! Estimated noise=578.32 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 = 0.287526 Jy ! Component: 100 - total flux cleaned = 0.403878 Jy ! Total flux subtracted in 100 components = 0.403878 Jy ! Clean residual min=-0.010542 max=0.056881 Jy/beam ! Clean residual mean=-0.000052 rms=0.003040 Jy/beam ! Combined flux in latest and established models = 0.403878 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.403878 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.234019Jy sigma=0.002028 ! Fit after self-cal, rms=0.233472Jy sigma=0.002025 ! Inverting map ! Your choice of large map pixels excluded 4.24% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.067252 Jy ! Component: 100 - total flux cleaned = 0.107871 Jy ! Total flux subtracted in 100 components = 0.107871 Jy ! Clean residual min=-0.006758 max=0.031873 Jy/beam ! Clean residual mean=-0.000036 rms=0.001931 Jy/beam ! Combined flux in latest and established models = 0.511749 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 11 components and 0.511749 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.197573Jy sigma=0.001579 ! Fit after self-cal, rms=0.197330Jy sigma=0.001578 ! Inverting map ! Your choice of large map pixels excluded 4.24% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Added new window around map position (0, -0.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0329212 Jy ! Component: 100 - total flux cleaned = 0.056087 Jy ! Total flux subtracted in 100 components = 0.056087 Jy ! Clean residual min=-0.005271 max=0.014930 Jy/beam ! Clean residual mean=-0.000027 rms=0.001513 Jy/beam ! Combined flux in latest and established models = 0.567836 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 17 components and 0.567836 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.186031Jy sigma=0.001416 ! Fit after self-cal, rms=0.185665Jy sigma=0.001413 ! Inverting map ! Your choice of large map pixels excluded 4.24% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0197315 Jy ! Component: 100 - total flux cleaned = 0.0352369 Jy ! Total flux subtracted in 100 components = 0.0352369 Jy ! Clean residual min=-0.004815 max=0.010125 Jy/beam ! Clean residual mean=-0.000021 rms=0.001270 Jy/beam ! Combined flux in latest and established models = 0.603073 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 21 components and 0.603073 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.180855Jy sigma=0.001337 ! Fit after self-cal, rms=0.180723Jy sigma=0.001336 ! Inverting map ! Your choice of large map pixels excluded 4.24% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0135222 Jy ! Component: 100 - total flux cleaned = 0.0244165 Jy ! Total flux subtracted in 100 components = 0.0244165 Jy ! Clean residual min=-0.004487 max=0.006931 Jy/beam ! Clean residual mean=-0.000018 rms=0.001137 Jy/beam ! Combined flux in latest and established models = 0.62749 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 24 components and 0.62749 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.178322Jy sigma=0.001295 ! Fit after self-cal, rms=0.178271Jy sigma=0.001295 ! Inverting map ! Your choice of large map pixels excluded 4.24% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00954039 Jy ! Component: 100 - total flux cleaned = 0.0173581 Jy ! Total flux subtracted in 100 components = 0.0173581 Jy ! Clean residual min=-0.004310 max=0.005674 Jy/beam ! Clean residual mean=-0.000015 rms=0.001063 Jy/beam ! Combined flux in latest and established models = 0.644848 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 26 components and 0.644847 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.177011Jy sigma=0.001272 ! Fit after self-cal, rms=0.176991Jy sigma=0.001272 ! Inverting map ! Your choice of large map pixels excluded 4.24% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 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 4.24% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=0.6291 mas, bmaj=0.6707 mas, bpa=89.67 degrees ! Estimated noise=283.354 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 = 0.0194842 Jy ! Component: 100 - total flux cleaned = 0.0322178 Jy ! Component: 150 - total flux cleaned = 0.0408616 Jy ! Component: 200 - total flux cleaned = 0.0467858 Jy ! Total flux subtracted in 200 components = 0.0467858 Jy ! Clean residual min=-0.004103 max=0.007812 Jy/beam ! Clean residual mean=-0.000017 rms=0.001130 Jy/beam ! Combined flux in latest and established models = 0.691633 Jy ! Performing phase self-cal ! Adding 32 model components to the UV plane model. ! The established model now contains 41 components and 0.691633 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.175382Jy sigma=0.001237 ! Fit after self-cal, rms=0.175337Jy sigma=0.001237 ! Inverting map ! Your choice of large map pixels excluded 4.24% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Added new window around map position (-1, -0.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00727605 Jy ! Component: 100 - total flux cleaned = 0.0113959 Jy ! Component: 150 - total flux cleaned = 0.0142258 Jy ! Component: 200 - total flux cleaned = 0.0156161 Jy ! Total flux subtracted in 200 components = 0.0156161 Jy ! Clean residual min=-0.004290 max=0.005767 Jy/beam ! Clean residual mean=-0.000005 rms=0.001043 Jy/beam ! Combined flux in latest and established models = 0.707249 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 55 components and 0.707249 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.175120Jy sigma=0.001232 ! Fit after self-cal, rms=0.175097Jy sigma=0.001232 ! Inverting map ! Your choice of large map pixels excluded 4.24% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 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: ! BR 0.95 FD 0.97 GC 1.06 KP 1.02 ! LA 1.01 NL 1.01 OV 0.97 PT 1.02 ! SC 1.09 WF 1.02 HH 1.00* KK 1.01 ! MA 0.99 MC 0.94 MK 0.96 NY 0.94 ! ON 1.00* TS 0.97 WZ 1.10 HN 0.86 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.95 FD 0.97 GC 1.03 KP 1.04 ! LA 1.02 NL 0.97 OV 0.98 PT 1.01 ! SC 1.08 WF 0.90 HH 1.00* KK 1.02 ! MA 0.98 MC 0.96 MK 0.98 NY 0.93 ! ON 1.00* TS 1.00 WZ 1.02 HN 0.85 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 FD 0.94 GC 1.12 KP 1.00 ! LA 0.98 NL 0.97 OV 0.92 PT 1.00* ! SC 1.03 WF 1.01 HH 1.00* KK 1.04 ! MA 1.02 MC 1.00* MK 1.11 NY 0.93 ! ON 1.00* TS 0.98 WZ 0.96 HN 1.00* ! ! ! Correcting IF 2. ! A total of 21 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.95 FD 0.96 GC 1.06 KP 0.99 ! LA 0.97 NL 1.04 OV 0.96 PT 0.99 ! SC 1.07 WF 1.05 HH 1.00* KK 1.03 ! MA 1.02 MC 0.96 MK 1.02 NY 0.97 ! ON 1.00* TS 0.95 WZ 1.16 HN 0.90 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.95 FD 0.96 GC 1.02 KP 1.01 ! LA 0.97 NL 1.00 OV 0.96 PT 0.98 ! SC 1.05 WF 0.92 HH 1.00* KK 1.01 ! MA 0.97 MC 1.00 MK 1.05 NY 0.97 ! ON 1.00* TS 1.01 WZ 1.03 HN 0.81 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 FD 0.93 GC 1.11 KP 0.98 ! LA 0.95 NL 1.00 OV 0.93 PT 1.00* ! SC 1.01 WF 1.02 HH 1.00* KK 1.05 ! MA 1.01 MC 1.00* MK 1.14 NY 0.97 ! ON 1.00* TS 0.99 WZ 0.97 HN 1.00* ! ! ! Correcting IF 3. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 1.01 GC 1.08 KP 1.02 ! LA 0.98 NL 0.99 OV 0.98 PT 1.01 ! SC 1.11 WF 1.04 HH 1.00* KK 1.02 ! MA 1.05 MC 0.96 MK 1.00 NY 0.98 ! ON 1.00* TS 1.01 WZ 1.12 HN 0.85 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 0.99 GC 1.04 KP 1.03 ! LA 0.97 NL 0.98 OV 0.98 PT 1.03 ! SC 1.11 WF 0.91 HH 1.00* KK 1.00 ! MA 0.93 MC 0.96 MK 1.00 NY 1.01 ! ON 1.00* TS 1.06 WZ 1.08 HN 0.92 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 0.99 GC 1.12 KP 0.98 ! LA 0.95 NL 0.97 OV 0.94 PT 1.00* ! SC 1.08 WF 1.02 HH 1.00* KK 1.05 ! MA 0.99 MC 1.00* MK 1.11 NY 1.02 ! ON 1.00* TS 1.02 WZ 0.99 HN 1.00* ! ! ! Correcting IF 4. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 1.00 GC 1.07 KP 1.00 ! LA 1.00 NL 1.00 OV 1.00 PT 1.02 ! SC 1.18 WF 1.05 HH 1.00* KK 1.02 ! MA 0.98 MC 0.97 MK 1.00 NY 1.02 ! ON 1.00* TS 1.03 WZ 1.19 HN 0.83 ! ! A total of 27 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 FD 0.98 GC 1.04 KP 1.02 ! LA 0.99 NL 0.99 OV 0.99 PT 1.03 ! SC 1.17 WF 0.96 HH 1.00* KK 1.05 ! MA 1.00 MC 0.92 MK 1.04 NY 1.03 ! ON 1.00* TS 1.06 WZ 1.12 HN 0.74 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 FD 0.96 GC 1.13 KP 0.99 ! LA 0.96 NL 0.99 OV 0.95 PT 1.00* ! SC 1.14 WF 1.06 HH 1.00* KK 1.05 ! MA 0.96 MC 1.00* MK 1.14 NY 1.01 ! ON 1.00* TS 1.01 WZ 1.01 HN 1.00* ! ! ! Fit before self-cal, rms=0.175097Jy sigma=0.001232 ! Fit after self-cal, rms=0.174413Jy sigma=0.001202 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=0.6316 mas, bmaj=0.6721 mas, bpa=88.15 degrees ! Estimated noise=285.325 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 = -0.00362052 Jy ! Component: 100 - total flux cleaned = -0.0047331 Jy ! Component: 150 - total flux cleaned = -0.00559732 Jy ! Component: 200 - total flux cleaned = -0.00627412 Jy ! Total flux subtracted in 200 components = -0.00627412 Jy ! Clean residual min=-0.001858 max=0.002416 Jy/beam ! Clean residual mean=0.000003 rms=0.000470 Jy/beam ! Combined flux in latest and established models = 0.700975 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 61 components and 0.700975 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.174281Jy sigma=0.001201 ! Fit after self-cal, rms=0.174325Jy sigma=0.001201 ! Inverting map ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Added new window around map position (-1.2, -4.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00139322 Jy ! Component: 100 - total flux cleaned = 0.00151198 Jy ! Component: 150 - total flux cleaned = 0.00161097 Jy ! Component: 200 - total flux cleaned = 0.00165333 Jy ! Total flux subtracted in 200 components = 0.00165333 Jy ! Clean residual min=-0.001794 max=0.001928 Jy/beam ! Clean residual mean=0.000003 rms=0.000453 Jy/beam ! Combined flux in latest and established models = 0.702628 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 73 components and 0.702628 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.174285Jy sigma=0.001201 ! Fit after self-cal, rms=0.174283Jy sigma=0.001201 ! Inverting map ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 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=0.174283Jy sigma=0.001201 ! Fit after self-cal, rms=0.175368Jy sigma=0.001200 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=0.6324 mas, bmaj=0.673 mas, bpa=87.1 degrees ! Estimated noise=285.97 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00188741 Jy ! Component: 100 - total flux cleaned = -0.00236735 Jy ! Component: 150 - total flux cleaned = -0.00242529 Jy ! Component: 200 - total flux cleaned = -0.0024277 Jy ! Total flux subtracted in 200 components = -0.0024277 Jy ! Clean residual min=-0.001842 max=0.001879 Jy/beam ! Clean residual mean=0.000002 rms=0.000425 Jy/beam ! Combined flux in latest and established models = 0.700201 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 75 components and 0.700201 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.175313Jy sigma=0.001200 ! Fit after self-cal, rms=0.175322Jy sigma=0.001200 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (21, -14). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00104435 Jy ! Component: 100 - total flux cleaned = 0.00121642 Jy ! Component: 150 - total flux cleaned = 0.0014048 Jy ! Component: 200 - total flux cleaned = 0.00150558 Jy ! Total flux subtracted in 200 components = 0.00150558 Jy ! Clean residual min=-0.001685 max=0.001754 Jy/beam ! Clean residual mean=0.000002 rms=0.000415 Jy/beam ! Combined flux in latest and established models = 0.701706 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 80 components and 0.701706 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.175296Jy sigma=0.001200 ! Fit after self-cal, rms=0.175294Jy sigma=0.001200 ! Inverting map ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 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=0.175294Jy sigma=0.001200 ! Fit after self-cal, rms=0.176139Jy sigma=0.001200 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=0.6333 mas, bmaj=0.6736 mas, bpa=86.37 degrees ! Estimated noise=286.56 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000963768 Jy ! Component: 100 - total flux cleaned = -0.00135323 Jy ! Component: 150 - total flux cleaned = -0.00143482 Jy ! Component: 200 - total flux cleaned = -0.00143425 Jy ! Total flux subtracted in 200 components = -0.00143425 Jy ! Clean residual min=-0.001794 max=0.001762 Jy/beam ! Clean residual mean=0.000001 rms=0.000403 Jy/beam ! Combined flux in latest and established models = 0.700272 Jy selfcal ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 82 components and 0.700272 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.176111Jy sigma=0.001199 ! Fit after self-cal, rms=0.176118Jy sigma=0.001199 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (-1.4, -10.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00172414 Jy ! Component: 100 - total flux cleaned = 0.00246253 Jy ! Component: 150 - total flux cleaned = 0.00256193 Jy ! Component: 200 - total flux cleaned = 0.00271223 Jy ! Total flux subtracted in 200 components = 0.00271223 Jy ! Clean residual min=-0.001589 max=0.001604 Jy/beam ! Clean residual mean=0.000001 rms=0.000391 Jy/beam ! Combined flux in latest and established models = 0.702984 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 92 components and 0.702984 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.176097Jy sigma=0.001199 ! Fit after self-cal, rms=0.176096Jy sigma=0.001199 ! Inverting map ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 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=0.176096Jy sigma=0.001199 ! Fit after self-cal, rms=0.176654Jy sigma=0.001199 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=2.231 mas, bmaj=2.615 mas, bpa=-42.8 degrees ! Estimated noise=443.017 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000909993 Jy ! Component: 100 - total flux cleaned = 0.00111808 Jy ! Component: 150 - total flux cleaned = 0.00143607 Jy ! Component: 200 - total flux cleaned = 0.00167551 Jy ! Total flux subtracted in 200 components = 0.00167551 Jy ! Clean residual min=-0.002489 max=0.002356 Jy/beam ! Clean residual mean=0.000003 rms=0.000738 Jy/beam ! Combined flux in latest and established models = 0.70466 Jy selfcal ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 111 components and 0.70466 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.176644Jy sigma=0.001199 ! Fit after self-cal, rms=0.176649Jy sigma=0.001199 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 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 = 0.000708336 Jy ! Component: 100 - total flux cleaned = 0.000895177 Jy ! Component: 150 - total flux cleaned = 0.000984918 Jy ! Component: 200 - total flux cleaned = 0.00106459 Jy ! Total flux subtracted in 200 components = 0.00106459 Jy ! Clean residual min=-0.002561 max=0.002185 Jy/beam ! Clean residual mean=0.000003 rms=0.000716 Jy/beam ! Combined flux in latest and established models = 0.705725 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 118 components and 0.705725 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.176654Jy sigma=0.001199 ! Fit after self-cal, rms=0.176655Jy sigma=0.001199 ! Inverting map ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 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 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=0.634 mas, bmaj=0.6741 mas, bpa=85.98 degrees ! Estimated noise=286.981 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.634 x 0.6741 at 85.98 degrees (North through East) ! Clean map min=-0.0012549 max=0.43053 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 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=0.5075 mas, bmaj=0.5471 mas, bpa=78.25 degrees ! Estimated noise=590.93 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.294105 Jy ! Component: 100 - total flux cleaned = 0.414251 Jy ! Component: 150 - total flux cleaned = 0.481592 Jy ! Component: 200 - total flux cleaned = 0.525295 Jy ! Total flux subtracted in 200 components = 0.525295 Jy ! Clean residual min=-0.005728 max=0.024870 Jy/beam ! Clean residual mean=-0.000029 rms=0.001714 Jy/beam ! Combined flux in latest and established models = 0.525295 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 13 model components to the UV plane model. ! The established model now contains 13 components and 0.525295 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=0.634 mas, bmaj=0.6741 mas, bpa=85.98 degrees ! Estimated noise=286.981 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 = 0.0626321 Jy ! Component: 100 - total flux cleaned = 0.0984997 Jy ! Component: 150 - total flux cleaned = 0.120974 Jy ! Component: 200 - total flux cleaned = 0.135306 Jy ! Total flux subtracted in 200 components = 0.135306 Jy ! Clean residual min=-0.002425 max=0.008018 Jy/beam ! Clean residual mean=-0.000025 rms=0.000813 Jy/beam ! Combined flux in latest and established models = 0.660601 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 27 components and 0.660601 Jy ! Inverting map ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Added new window around map position (0, 0.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00949916 Jy ! Component: 100 - total flux cleaned = 0.0158435 Jy ! Component: 150 - total flux cleaned = 0.0202785 Jy ! Component: 200 - total flux cleaned = 0.0236522 Jy ! Total flux subtracted in 200 components = 0.0236522 Jy ! Clean residual min=-0.001696 max=0.002436 Jy/beam ! Clean residual mean=-0.000008 rms=0.000461 Jy/beam ! Combined flux in latest and established models = 0.684254 Jy ! Adding 25 model components to the UV plane model. ! The established model now contains 44 components and 0.684254 Jy ! Inverting map ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Added new window around map position (-0.2, -6.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00287469 Jy ! Component: 100 - total flux cleaned = 0.00528973 Jy ! Component: 150 - total flux cleaned = 0.00738351 Jy ! Component: 200 - total flux cleaned = 0.00920884 Jy ! Total flux subtracted in 200 components = 0.00920884 Jy ! Clean residual min=-0.001563 max=0.001588 Jy/beam ! Clean residual mean=-0.000003 rms=0.000401 Jy/beam ! Combined flux in latest and established models = 0.693463 Jy ! Adding 41 model components to the UV plane model. ! The established model now contains 68 components and 0.693463 Jy ! Inverting map ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 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 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=2.231 mas, bmaj=2.615 mas, bpa=-42.8 degrees ! Estimated noise=443.017 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0039057 Jy ! Component: 100 - total flux cleaned = 0.00643148 Jy ! Component: 150 - total flux cleaned = 0.00822529 Jy ! Component: 200 - total flux cleaned = 0.00956332 Jy ! Total flux subtracted in 200 components = 0.00956332 Jy ! Clean residual min=-0.002474 max=0.002070 Jy/beam ! Clean residual mean=0.000000 rms=0.000693 Jy/beam ! Combined flux in latest and established models = 0.703026 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 = 0.00100994 Jy ! Component: 100 - total flux cleaned = 0.00146141 Jy ! Component: 150 - total flux cleaned = 0.00184227 Jy ! Component: 200 - total flux cleaned = 0.00214412 Jy ! Total flux subtracted in 200 components = 0.00214412 Jy ! Clean residual min=-0.002425 max=0.001988 Jy/beam ! Clean residual mean=0.000003 rms=0.000676 Jy/beam ! Combined flux in latest and established models = 0.70517 Jy ! Adding 50 model components to the UV plane model. ! The established model now contains 107 components and 0.70517 Jy ! Inverting map ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=0.634 mas, bmaj=0.6741 mas, bpa=85.98 degrees ! Estimated noise=286.981 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000709237 Jy ! Component: 100 - total flux cleaned = -0.000714002 Jy ! Component: 150 - total flux cleaned = -0.000606233 Jy ! Component: 200 - total flux cleaned = -0.000538921 Jy ! Total flux subtracted in 200 components = -0.000538921 Jy ! Clean residual min=-0.001573 max=0.001437 Jy/beam ! Clean residual mean=0.000001 rms=0.000370 Jy/beam ! Combined flux in latest and established models = 0.704631 Jy selfcal ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 123 components and 0.704631 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.176621Jy sigma=0.001199 ! Fit after self-cal, rms=0.176597Jy sigma=0.001199 wmodel J0017+8135_X_2000_03_13_pus_map.mod ! Writing 123 model components to file: J0017+8135_X_2000_03_13_pus_map.mod wobs J0017+8135_X_2000_03_13_pus_uvs.fits ! Writing UV FITS file: J0017+8135_X_2000_03_13_pus_uvs.fits wwins J0017+8135_X_2000_03_13_pus_map.win ! wwins: Wrote 8 windows to J0017+8135_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 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000342934 Jy ! Component: 100 - total flux cleaned = -0.00052574 Jy ! Component: 150 - total flux cleaned = -0.000600965 Jy ! Component: 200 - total flux cleaned = -0.000576178 Jy ! Component: 250 - total flux cleaned = -0.000504087 Jy ! Component: 300 - total flux cleaned = -0.00050402 Jy ! Component: 350 - total flux cleaned = -0.000410773 Jy ! Component: 400 - total flux cleaned = -0.000364944 Jy ! Component: 450 - total flux cleaned = -0.000319887 Jy ! Component: 500 - total flux cleaned = -0.000364505 Jy ! Component: 550 - total flux cleaned = -0.000386313 Jy ! Component: 600 - total flux cleaned = -0.000364215 Jy ! Component: 650 - total flux cleaned = -0.000364342 Jy ! Component: 700 - total flux cleaned = -0.000385891 Jy ! Component: 750 - total flux cleaned = -0.000407033 Jy ! Component: 800 - total flux cleaned = -0.000449476 Jy ! Component: 850 - total flux cleaned = -0.00053271 Jy ! Component: 900 - total flux cleaned = -0.000532761 Jy ! Component: 950 - total flux cleaned = -0.000594403 Jy ! Component: 1000 - total flux cleaned = -0.000614822 Jy ! Component: 1050 - total flux cleaned = -0.00069548 Jy ! Component: 1100 - total flux cleaned = -0.000635114 Jy ! Component: 1150 - total flux cleaned = -0.000655258 Jy ! Component: 1200 - total flux cleaned = -0.000675102 Jy ! Component: 1250 - total flux cleaned = -0.000694865 Jy ! Component: 1300 - total flux cleaned = -0.00071453 Jy ! Component: 1350 - total flux cleaned = -0.000714451 Jy ! Component: 1400 - total flux cleaned = -0.000714531 Jy ! Component: 1450 - total flux cleaned = -0.0006952 Jy ! Component: 1500 - total flux cleaned = -0.000733562 Jy ! Component: 1550 - total flux cleaned = -0.000791019 Jy ! Component: 1600 - total flux cleaned = -0.000828949 Jy ! Component: 1650 - total flux cleaned = -0.000923533 Jy ! Component: 1700 - total flux cleaned = -0.000867003 Jy ! Component: 1750 - total flux cleaned = -0.000923309 Jy ! Component: 1800 - total flux cleaned = -0.000942046 Jy ! Component: 1850 - total flux cleaned = -0.00099782 Jy ! Component: 1900 - total flux cleaned = -0.00099783 Jy ! Component: 1950 - total flux cleaned = -0.00105295 Jy ! Component: 2000 - total flux cleaned = -0.00107118 Jy ! Total flux subtracted in 2048 components = -0.00121736 Jy ! Clean residual min=-0.000956 max=0.001149 Jy/beam ! Clean residual mean=-0.000000 rms=0.000325 Jy/beam ! Combined flux in latest and established models = 0.703414 Jy keep ! Adding 196 model components to the UV plane model. ! The established model now contains 319 components and 0.703413 Jy ![Exited script file: muppet] wmap "J0017+8135_X_2000_03_13_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.634 x 0.6741 at 85.98 degrees (North through East) ! Clean map min=-0.0012837 max=0.43194 Jy/beam ! Writing clean map to FITS file: J0017+8135_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 0.431944 invert ! Inverting map ! Your choice of large map pixels excluded 4.18% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000325033 device "J0017+8135_X_2000_03_13_pus\_map.eps/VPS" ! Attempting to open device: 'J0017+8135_X_2000_03_13_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.225747 0.225747 0.451494 0.902988 1.80598 3.61195 7.2239 14.4478 28.8956 57.7912 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0009 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.431 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.634 x 0.6741 at 85.98 degrees (North through East) ! Clean map min=-0.0012837 max=0.43194 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. quit ! Quitting program ! Log file J0017+8135_X_2000_03_13_pus_uvs.log closed on Wed Apr 3 15:18:37 2013