! Started logfile: J0423+4150_X_2001_03_12_pus_uvs.log on Wed Jan 2 19:50:34 2013 obs J0423+4150_X_2001_03_12_pus_uva.fits ! Reading UV FITS file: J0423+4150_X_2001_03_12_pus_uva.fits ! AN table 1: 147 integrations on 136 of 136 possible baselines. ! AN table 2: 209 integrations on 136 of 136 possible baselines. ! AN table 3: 68 integrations on 136 of 136 possible baselines. ! Apparent sampling: 0.160291 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0423+4150 ! ! 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 1745 lines of history. ! ! Reading 36972 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 J0423+4150_X_2001_03_12_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 1531 telescope corrections were flagged in sub-array 1. ! A total of 2723 telescope corrections were flagged in sub-array 2. ! A total of 616 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 1531 telescope corrections were flagged in sub-array 1. ! A total of 2723 telescope corrections were flagged in sub-array 2. ! A total of 616 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 1531 telescope corrections were flagged in sub-array 1. ! A total of 2723 telescope corrections were flagged in sub-array 2. ! A total of 619 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 1531 telescope corrections were flagged in sub-array 1. ! A total of 2723 telescope corrections were flagged in sub-array 2. ! A total of 619 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=0.570716Jy sigma=0.004063 ! Fit after self-cal, rms=0.418565Jy sigma=0.003062 ! 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 7.04% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! Estimated beam: bmin=0.5098 mas, bmaj=0.7081 mas, bpa=-14.48 degrees ! Estimated noise=921.689 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 = 0.584263 Jy ! Component: 100 - total flux cleaned = 0.74625 Jy ! Total flux subtracted in 100 components = 0.74625 Jy ! Clean residual min=-0.027921 max=0.068520 Jy/beam ! Clean residual mean=-0.000166 rms=0.008201 Jy/beam ! Combined flux in latest and established models = 0.74625 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.74625 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.356244Jy sigma=0.002401 ! Fit after self-cal, rms=0.356373Jy sigma=0.002400 ! Inverting map ! Your choice of large map pixels excluded 7.04% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.075102 Jy ! Component: 100 - total flux cleaned = 0.121444 Jy ! Total flux subtracted in 100 components = 0.121444 Jy ! Clean residual min=-0.026170 max=0.054690 Jy/beam ! Clean residual mean=-0.000116 rms=0.007128 Jy/beam ! Combined flux in latest and established models = 0.867694 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 13 components and 0.867694 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.334358Jy sigma=0.002065 ! Fit after self-cal, rms=0.334366Jy sigma=0.002064 ! Inverting map ! Your choice of large map pixels excluded 7.04% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! Added new window around map position (-1, -0.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0490788 Jy ! Component: 100 - total flux cleaned = 0.0795628 Jy ! Total flux subtracted in 100 components = 0.0795628 Jy ! Clean residual min=-0.023881 max=0.035668 Jy/beam ! Clean residual mean=-0.000086 rms=0.006479 Jy/beam ! Combined flux in latest and established models = 0.947257 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 22 components and 0.947257 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.325929Jy sigma=0.001915 ! Fit after self-cal, rms=0.325144Jy sigma=0.001908 ! Inverting map ! Your choice of large map pixels excluded 7.04% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 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 7.04% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! Estimated beam: bmin=0.6072 mas, bmaj=0.8887 mas, bpa=-19.83 degrees ! Estimated noise=470.342 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 (-3.8, -0.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.064743 Jy ! Component: 100 - total flux cleaned = 0.109964 Jy ! Component: 150 - total flux cleaned = 0.145054 Jy ! Component: 200 - total flux cleaned = 0.17276 Jy ! Total flux subtracted in 200 components = 0.17276 Jy ! Clean residual min=-0.021781 max=0.035430 Jy/beam ! Clean residual mean=-0.000156 rms=0.005980 Jy/beam ! Combined flux in latest and established models = 1.12002 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 46 components and 1.12002 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.310539Jy sigma=0.001667 ! Fit after self-cal, rms=0.308257Jy sigma=0.001650 ! Inverting map ! Your choice of large map pixels excluded 7.04% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! Added new window around map position (-5.8, -0.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.041167 Jy ! Component: 100 - total flux cleaned = 0.0687805 Jy ! Component: 150 - total flux cleaned = 0.0904706 Jy ! Component: 200 - total flux cleaned = 0.107769 Jy ! Total flux subtracted in 200 components = 0.107769 Jy ! Clean residual min=-0.017532 max=0.021739 Jy/beam ! Clean residual mean=-0.000062 rms=0.004684 Jy/beam ! Combined flux in latest and established models = 1.22779 Jy ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 66 components and 1.22779 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.301775Jy sigma=0.001552 ! Fit after self-cal, rms=0.301037Jy sigma=0.001544 ! Inverting map ! Your choice of large map pixels excluded 7.04% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 33 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 1.00 HH 1.00* HN 0.99 ! KK 0.96 KP 0.98 LA 0.93 MA 1.00* ! MC 1.20 MK 0.98 NL 1.00 ON 1.12 ! OV 0.96 PT 0.95 SC 0.96 TS 1.39 ! WZ 0.79 ! ! A total of 72 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 1.00* HH 1.00* HN 1.00* ! KK 1.08 KP 1.00* LA 1.00* MA 1.03 ! MC 1.04 MK 1.00* NL 1.00* ON 1.10 ! OV 1.00* PT 1.00* SC 1.00* TS 0.82 ! WZ 1.03 ! ! A total of 9 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.00 HH 1.00* HN 0.99 ! KK 0.90 KP 1.01 LA 0.95 MA 1.00* ! MC 1.00* MK 0.95 NL 0.99 ON 0.93 ! OV 1.00* PT 0.96 SC 1.15 TS 0.85 ! WZ 1.00* ! ! ! Correcting IF 2. ! A total of 33 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.98 HH 1.00* HN 0.98 ! KK 0.95 KP 0.93 LA 0.93 MA 1.00* ! MC 1.21 MK 0.97 NL 0.97 ON 1.22 ! OV 0.95 PT 1.00 SC 0.94 TS 1.41 ! WZ 0.76 ! ! A total of 72 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 1.00* HH 1.00* HN 1.00* ! KK 1.05 KP 1.00* LA 1.00* MA 0.98 ! MC 1.05 MK 1.00* NL 1.00* ON 1.07 ! OV 1.00* PT 1.00* SC 1.00* TS 0.83 ! WZ 1.05 ! ! A total of 9 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 0.99 HH 1.00* HN 0.99 ! KK 0.89 KP 0.97 LA 0.95 MA 1.00* ! MC 1.00* MK 0.95 NL 0.95 ON 0.95 ! OV 1.00* PT 0.99 SC 1.12 TS 0.86 ! WZ 1.00* ! ! ! Correcting IF 3. ! A total of 33 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 0.97 HH 1.00* HN 1.00 ! KK 1.01 KP 0.92 LA 0.95 MA 1.00* ! MC 1.30 MK 0.98 NL 1.01 ON 1.28 ! OV 0.99 PT 1.02 SC 0.94 TS 1.41 ! WZ 0.80 ! ! A total of 72 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.05 FD 1.00* HH 1.00* HN 1.00* ! KK 1.16 KP 1.00* LA 1.00* MA 1.06 ! MC 1.14 MK 1.00* NL 1.00* ON 1.10 ! OV 1.00* PT 1.00* SC 1.00* TS 0.82 ! WZ 1.08 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 FD 0.98 HH 1.00* HN 1.01 ! KK 0.97 KP 0.95 LA 0.96 MA 1.00* ! MC 1.00* MK 0.96 NL 1.00 ON 1.04 ! OV 1.00* PT 1.02 SC 1.18 TS 0.83 ! WZ 1.00* ! ! ! Correcting IF 4. ! A total of 33 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.95 HH 1.00* HN 1.00 ! KK 0.97 KP 0.94 LA 0.93 MA 1.00* ! MC 1.25 MK 1.01 NL 1.02 ON 1.22 ! OV 0.97 PT 1.02 SC 1.02 TS 1.41 ! WZ 0.81 ! ! A total of 72 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 1.00* HH 1.00* HN 1.00* ! KK 1.11 KP 1.00* LA 1.00* MA 1.03 ! MC 1.06 MK 1.00* NL 1.00* ON 1.21 ! OV 1.00* PT 1.00* SC 1.00* TS 0.82 ! WZ 1.10 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 0.97 HH 1.00* HN 1.02 ! KK 0.91 KP 0.98 LA 0.95 MA 1.00* ! MC 1.00* MK 1.00 NL 1.00 ON 1.05 ! OV 1.00* PT 1.01 SC 1.23 TS 0.84 ! WZ 1.00* ! ! ! Fit before self-cal, rms=0.301037Jy sigma=0.001544 ! Fit after self-cal, rms=0.287241Jy sigma=0.001298 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! Estimated beam: bmin=0.6139 mas, bmaj=0.9133 mas, bpa=-20.97 degrees ! Estimated noise=470.891 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 (-2.2, -1). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0184486 Jy ! Component: 100 - total flux cleaned = 0.0259105 Jy ! Component: 150 - total flux cleaned = 0.0300495 Jy ! Component: 200 - total flux cleaned = 0.0338707 Jy ! Total flux subtracted in 200 components = 0.0338707 Jy ! Clean residual min=-0.010735 max=0.013235 Jy/beam ! Clean residual mean=0.000005 rms=0.002004 Jy/beam ! Combined flux in latest and established models = 1.26166 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 90 components and 1.26166 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.285370Jy sigma=0.001265 ! Fit after self-cal, rms=0.285010Jy sigma=0.001262 ! Inverting map ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! Added new window around map position (-5.6, -2.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.01415 Jy ! Component: 100 - total flux cleaned = 0.0199317 Jy ! Component: 150 - total flux cleaned = 0.0237629 Jy ! Component: 200 - total flux cleaned = 0.0265466 Jy ! Total flux subtracted in 200 components = 0.0265466 Jy ! Clean residual min=-0.009386 max=0.006952 Jy/beam ! Clean residual mean=0.000028 rms=0.001659 Jy/beam ! Combined flux in latest and established models = 1.2882 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 104 components and 1.2882 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.284047Jy sigma=0.001246 ! Fit after self-cal, rms=0.283991Jy sigma=0.001245 ! Inverting map ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 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=0.283991Jy sigma=0.001245 ! Fit after self-cal, rms=0.281506Jy sigma=0.001241 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! Estimated beam: bmin=0.6143 mas, bmaj=0.918 mas, bpa=-21.19 degrees ! Estimated noise=469.621 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000897494 Jy ! Component: 100 - total flux cleaned = 0.0026808 Jy ! Component: 150 - total flux cleaned = 0.00527332 Jy ! Component: 200 - total flux cleaned = 0.00691024 Jy ! Total flux subtracted in 200 components = 0.00691024 Jy ! Clean residual min=-0.007978 max=0.005799 Jy/beam ! Clean residual mean=-0.000000 rms=0.001395 Jy/beam ! Combined flux in latest and established models = 1.29511 Jy selfcal ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 111 components and 1.29511 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.280897Jy sigma=0.001232 ! Fit after self-cal, rms=0.280832Jy sigma=0.001232 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 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 = 0.00311066 Jy ! Component: 100 - total flux cleaned = 0.00457623 Jy ! Component: 150 - total flux cleaned = 0.00554624 Jy ! Component: 200 - total flux cleaned = 0.00627966 Jy ! Total flux subtracted in 200 components = 0.00627966 Jy ! Clean residual min=-0.007552 max=0.005203 Jy/beam ! Clean residual mean=0.000005 rms=0.001324 Jy/beam ! Combined flux in latest and established models = 1.30139 Jy ! Performing phase self-cal ! Adding 34 model components to the UV plane model. ! The established model now contains 115 components and 1.30139 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.280530Jy sigma=0.001228 ! Fit after self-cal, rms=0.280513Jy sigma=0.001228 ! Inverting map ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 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=0.280513Jy sigma=0.001228 ! Fit after self-cal, rms=0.280185Jy sigma=0.001227 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! Estimated beam: bmin=0.615 mas, bmaj=0.9221 mas, bpa=-21.44 degrees ! Estimated noise=469.239 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00373886 Jy ! Component: 100 - total flux cleaned = -0.00314867 Jy ! Component: 150 - total flux cleaned = -0.00241222 Jy ! Component: 200 - total flux cleaned = -0.00188691 Jy ! Total flux subtracted in 200 components = -0.00188691 Jy ! Clean residual min=-0.006551 max=0.004807 Jy/beam ! Clean residual mean=-0.000008 rms=0.001206 Jy/beam ! Combined flux in latest and established models = 1.29951 Jy selfcal ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 116 components and 1.29951 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.279833Jy sigma=0.001223 ! Fit after self-cal, rms=0.279792Jy sigma=0.001223 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 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 = 0.00121265 Jy ! Component: 100 - total flux cleaned = 0.00184705 Jy ! Component: 150 - total flux cleaned = 0.00244505 Jy ! Component: 200 - total flux cleaned = 0.0030087 Jy ! Total flux subtracted in 200 components = 0.0030087 Jy ! Clean residual min=-0.006205 max=0.004539 Jy/beam ! Clean residual mean=-0.000005 rms=0.001166 Jy/beam ! Combined flux in latest and established models = 1.30252 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 117 components and 1.30251 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.279619Jy sigma=0.001221 ! Fit after self-cal, rms=0.279609Jy sigma=0.001221 ! Inverting map ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 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=0.279609Jy sigma=0.001221 ! Fit after self-cal, rms=0.279942Jy sigma=0.001220 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! Estimated beam: bmin=2.264 mas, bmaj=2.671 mas, bpa=-31.44 degrees ! Estimated noise=730.989 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000895447 Jy ! Component: 100 - total flux cleaned = 4.90316e-05 Jy ! Component: 150 - total flux cleaned = 0.000731952 Jy ! Component: 200 - total flux cleaned = 0.00089344 Jy ! Total flux subtracted in 200 components = 0.00089344 Jy ! Clean residual min=-0.006693 max=0.006208 Jy/beam ! Clean residual mean=-0.000035 rms=0.001907 Jy/beam ! Combined flux in latest and established models = 1.30341 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 127 components and 1.30341 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.279869Jy sigma=0.001220 ! Fit after self-cal, rms=0.279855Jy sigma=0.001220 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 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 = 0.000594741 Jy ! Component: 100 - total flux cleaned = 0.000990935 Jy ! Component: 150 - total flux cleaned = 0.00105859 Jy ! Component: 200 - total flux cleaned = 0.001179 Jy ! Total flux subtracted in 200 components = 0.001179 Jy ! Clean residual min=-0.006698 max=0.006298 Jy/beam ! Clean residual mean=-0.000031 rms=0.001907 Jy/beam ! Combined flux in latest and established models = 1.30459 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 130 components and 1.30459 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.279832Jy sigma=0.001219 ! Fit after self-cal, rms=0.279834Jy sigma=0.001219 ! Inverting map ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 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 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! Estimated beam: bmin=0.6158 mas, bmaj=0.9257 mas, bpa=-21.69 degrees ! Estimated noise=469.256 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6158 x 0.9257 at -21.69 degrees (North through East) ! Clean map min=-0.0045245 max=0.79014 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=0.279834Jy sigma=0.001219 ! Fit after self-cal, rms=0.304974Jy sigma=0.001133 ! Inverting map and beam ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! Estimated beam: bmin=0.6164 mas, bmaj=0.9255 mas, bpa=-21.57 degrees ! Estimated noise=468.409 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00383952 Jy ! Component: 100 - total flux cleaned = -0.00399246 Jy ! Component: 150 - total flux cleaned = -0.00399103 Jy ! Component: 200 - total flux cleaned = -0.00385977 Jy ! Total flux subtracted in 200 components = -0.00385977 Jy ! Clean residual min=-0.005176 max=0.004128 Jy/beam ! Clean residual mean=-0.000014 rms=0.000981 Jy/beam ! Combined flux in latest and established models = 1.30073 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 134 components and 1.30073 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.304830Jy sigma=0.001131 ! Fit after self-cal, rms=0.304819Jy sigma=0.001131 ! Inverting map ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000144358 Jy ! Component: 100 - total flux cleaned = -0.000146161 Jy ! Component: 150 - total flux cleaned = -3.3241e-05 Jy ! Component: 200 - total flux cleaned = 7.54721e-05 Jy ! Total flux subtracted in 200 components = 7.54721e-05 Jy ! Clean residual min=-0.004892 max=0.003965 Jy/beam ! Clean residual mean=-0.000014 rms=0.000955 Jy/beam ! Combined flux in latest and established models = 1.3008 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 137 components and 1.3008 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.304729Jy sigma=0.001130 ! Fit after self-cal, rms=0.304723Jy sigma=0.001130 ! Inverting map ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.304723Jy sigma=0.001130 ! Fit after self-cal, rms=0.308712Jy sigma=0.001130 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 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! Estimated beam: bmin=0.5128 mas, bmaj=0.7344 mas, bpa=-17.02 degrees ! Estimated noise=938.248 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.593039 Jy ! Component: 100 - total flux cleaned = 0.738574 Jy ! Component: 150 - total flux cleaned = 0.810777 Jy ! Component: 200 - total flux cleaned = 0.858013 Jy ! Total flux subtracted in 200 components = 0.858013 Jy ! Clean residual min=-0.012704 max=0.026645 Jy/beam ! Clean residual mean=-0.000116 rms=0.003857 Jy/beam ! Combined flux in latest and established models = 0.858013 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 14 model components to the UV plane model. ! The established model now contains 14 components and 0.858013 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! Estimated beam: bmin=0.617 mas, bmaj=0.9279 mas, bpa=-21.72 degrees ! Estimated noise=468.554 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 = 0.0741134 Jy ! Component: 100 - total flux cleaned = 0.131442 Jy ! Component: 150 - total flux cleaned = 0.178241 Jy ! Component: 200 - total flux cleaned = 0.216908 Jy ! Total flux subtracted in 200 components = 0.216908 Jy ! Clean residual min=-0.011327 max=0.023563 Jy/beam ! Clean residual mean=-0.000230 rms=0.004626 Jy/beam ! Combined flux in latest and established models = 1.07492 Jy ! Adding 72 model components to the UV plane model. ! The established model now contains 75 components and 1.07492 Jy ! Inverting map ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0322635 Jy ! Component: 100 - total flux cleaned = 0.059337 Jy ! Component: 150 - total flux cleaned = 0.0822176 Jy ! Component: 200 - total flux cleaned = 0.101673 Jy ! Total flux subtracted in 200 components = 0.101673 Jy ! Clean residual min=-0.006631 max=0.012368 Jy/beam ! Clean residual mean=-0.000133 rms=0.002543 Jy/beam ! Combined flux in latest and established models = 1.17659 Jy ! Adding 78 model components to the UV plane model. ! The established model now contains 125 components and 1.17659 Jy ! Inverting map ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! Added new window around map position (-4, -3). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0167051 Jy ! Component: 100 - total flux cleaned = 0.0310521 Jy ! Component: 150 - total flux cleaned = 0.0434056 Jy ! Component: 200 - total flux cleaned = 0.0540772 Jy ! Total flux subtracted in 200 components = 0.0540772 Jy ! Clean residual min=-0.005069 max=0.007080 Jy/beam ! Clean residual mean=-0.000081 rms=0.001553 Jy/beam ! Combined flux in latest and established models = 1.23067 Jy ! Adding 66 model components to the UV plane model. ! The established model now contains 152 components and 1.23067 Jy ! Inverting map ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! Added new window around map position (-6.8, -1.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00931282 Jy ! Component: 100 - total flux cleaned = 0.0173856 Jy ! Component: 150 - total flux cleaned = 0.0244062 Jy ! Component: 200 - total flux cleaned = 0.0305242 Jy ! Total flux subtracted in 200 components = 0.0305242 Jy ! Clean residual min=-0.004529 max=0.004370 Jy/beam ! Clean residual mean=-0.000052 rms=0.001082 Jy/beam ! Combined flux in latest and established models = 1.26119 Jy ! Adding 69 model components to the UV plane model. ! The established model now contains 177 components and 1.26119 Jy ! Inverting map ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 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 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! Estimated beam: bmin=2.262 mas, bmaj=2.67 mas, bpa=-31.39 degrees ! Estimated noise=727.536 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0138551 Jy ! Component: 100 - total flux cleaned = 0.0222791 Jy ! Component: 150 - total flux cleaned = 0.027819 Jy ! Component: 200 - total flux cleaned = 0.0316273 Jy ! Total flux subtracted in 200 components = 0.0316273 Jy ! Clean residual min=-0.005788 max=0.004332 Jy/beam ! Clean residual mean=-0.000082 rms=0.001551 Jy/beam ! Combined flux in latest and established models = 1.29282 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 = 0.00271198 Jy ! Component: 100 - total flux cleaned = 0.00468638 Jy ! Component: 150 - total flux cleaned = 0.00613884 Jy ! Component: 200 - total flux cleaned = 0.00721575 Jy ! Total flux subtracted in 200 components = 0.00721575 Jy ! Clean residual min=-0.005789 max=0.004665 Jy/beam ! Clean residual mean=-0.000056 rms=0.001491 Jy/beam ! Combined flux in latest and established models = 1.30004 Jy ! Adding 123 model components to the UV plane model. ! The established model now contains 271 components and 1.30004 Jy ! Inverting map ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! Estimated beam: bmin=0.617 mas, bmaj=0.9279 mas, bpa=-21.72 degrees ! Estimated noise=468.554 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00127552 Jy ! Component: 100 - total flux cleaned = 0.00156734 Jy ! Component: 150 - total flux cleaned = 0.00183086 Jy ! Component: 200 - total flux cleaned = 0.00201026 Jy ! Total flux subtracted in 200 components = 0.00201026 Jy ! Clean residual min=-0.003774 max=0.003253 Jy/beam ! Clean residual mean=-0.000012 rms=0.000782 Jy/beam ! Combined flux in latest and established models = 1.30205 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 280 components and 1.30205 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.308100Jy sigma=0.001123 ! Fit after self-cal, rms=0.307902Jy sigma=0.001122 wmodel J0423+4150_X_2001_03_12_pus_map.mod ! Writing 280 model components to file: J0423+4150_X_2001_03_12_pus_map.mod wobs J0423+4150_X_2001_03_12_pus_uvs.fits ! Writing UV FITS file: J0423+4150_X_2001_03_12_pus_uvs.fits wwins J0423+4150_X_2001_03_12_pus_map.win ! wwins: Wrote 8 windows to J0423+4150_X_2001_03_12_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 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000727323 Jy ! Component: 100 - total flux cleaned = -0.000894011 Jy ! Component: 150 - total flux cleaned = -0.00105241 Jy ! Component: 200 - total flux cleaned = -0.0010525 Jy ! Component: 250 - total flux cleaned = -0.00110114 Jy ! Component: 300 - total flux cleaned = -0.00100543 Jy ! Component: 350 - total flux cleaned = -0.00109689 Jy ! Component: 400 - total flux cleaned = -0.00132126 Jy ! Component: 450 - total flux cleaned = -0.00123351 Jy ! Component: 500 - total flux cleaned = -0.00136395 Jy ! Component: 550 - total flux cleaned = -0.00132189 Jy ! Component: 600 - total flux cleaned = -0.00128065 Jy ! Component: 650 - total flux cleaned = -0.00115759 Jy ! Component: 700 - total flux cleaned = -0.0010772 Jy ! Component: 750 - total flux cleaned = -0.00107751 Jy ! Component: 800 - total flux cleaned = -0.000881259 Jy ! Component: 850 - total flux cleaned = -0.000958973 Jy ! Component: 900 - total flux cleaned = -0.000767564 Jy ! Component: 950 - total flux cleaned = -0.000768728 Jy ! Component: 1000 - total flux cleaned = -0.00080675 Jy ! Component: 1050 - total flux cleaned = -0.000732395 Jy ! Component: 1100 - total flux cleaned = -0.000732817 Jy ! Component: 1150 - total flux cleaned = -0.000696379 Jy ! Component: 1200 - total flux cleaned = -0.000588791 Jy ! Component: 1250 - total flux cleaned = -0.000624526 Jy ! Component: 1300 - total flux cleaned = -0.00048312 Jy ! Component: 1350 - total flux cleaned = -0.000552811 Jy ! Component: 1400 - total flux cleaned = -0.000275491 Jy ! Component: 1450 - total flux cleaned = -0.000275625 Jy ! Component: 1500 - total flux cleaned = -0.000241903 Jy ! Component: 1550 - total flux cleaned = -0.000140003 Jy ! Component: 1600 - total flux cleaned = -0.000106327 Jy ! Component: 1650 - total flux cleaned = 9.39971e-05 Jy ! Component: 1700 - total flux cleaned = 0.000193042 Jy ! Component: 1750 - total flux cleaned = 0.000291725 Jy ! Component: 1800 - total flux cleaned = 0.00042248 Jy ! Component: 1850 - total flux cleaned = 0.000454507 Jy ! Component: 1900 - total flux cleaned = 0.000486747 Jy ! Component: 1950 - total flux cleaned = 0.000422896 Jy ! Component: 2000 - total flux cleaned = 0.000645087 Jy ! Total flux subtracted in 2048 components = 0.000361395 Jy ! Clean residual min=-0.001641 max=0.002025 Jy/beam ! Clean residual mean=-0.000010 rms=0.000550 Jy/beam ! Combined flux in latest and established models = 1.30241 Jy keep ! Adding 171 model components to the UV plane model. ! The established model now contains 451 components and 1.30241 Jy ![Exited script file: muppet] wmap "J0423+4150_X_2001_03_12_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.617 x 0.9279 at -21.72 degrees (North through East) ! Clean map min=-0.0027744 max=0.79236 Jy/beam ! Writing clean map to FITS file: J0423+4150_X_2001_03_12_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.792362 invert ! Inverting map ! Your choice of large map pixels excluded 6.83% of the data. ! The x-axis pixel size should ideally be below 0.1595 milli-arcsec ! The y-axis pixel size should ideally be below 0.1976 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00055043 device "J0423+4150_X_2001_03_12_pus\_map.eps/VPS" ! Attempting to open device: 'J0423+4150_X_2001_03_12_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.208401 0.208401 0.416802 0.833604 1.66721 3.33442 6.66883 13.3377 26.6753 53.3507 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0016 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.792 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.617 x 0.9279 at -21.72 degrees (North through East) ! Clean map min=-0.0027744 max=0.79236 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. quit ! Quitting program ! Log file J0423+4150_X_2001_03_12_pus_uvs.log closed on Wed Jan 2 19:50:49 2013