! Started logfile: J0433+0521_X_2003_07_09_pus_uvs.log on Sun Apr 7 11:45:31 2013 obs J0433+0521_X_2003_07_09_pus_uva.fits ! Reading UV FITS file: J0433+0521_X_2003_07_09_pus_uva.fits ! AN table 1: 26 integrations on 171 of 171 possible baselines. ! AN table 2: 214 integrations on 171 of 171 possible baselines. ! AN table 3: 14 integrations on 171 of 171 possible baselines. ! Apparent sampling: 0.0985173 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0433+0521 ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! ! 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 1874 lines of history. ! ! Reading 17116 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 J0433+0521_X_2003_07_09_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 440 telescope corrections were flagged in sub-array 1. ! A total of 3100 telescope corrections were flagged in sub-array 2. ! A total of 266 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 444 telescope corrections were flagged in sub-array 1. ! A total of 3097 telescope corrections were flagged in sub-array 2. ! A total of 266 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 440 telescope corrections were flagged in sub-array 1. ! A total of 3094 telescope corrections were flagged in sub-array 2. ! A total of 266 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 440 telescope corrections were flagged in sub-array 1. ! A total of 3105 telescope corrections were flagged in sub-array 2. ! A total of 266 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=0.893937Jy sigma=0.006659 ! Fit after self-cal, rms=0.595715Jy sigma=0.004449 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Estimated beam: bmin=0.6818 mas, bmaj=1.248 mas, bpa=2.275 degrees ! Estimated noise=1185.39 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 = 0.618703 Jy ! Component: 100 - total flux cleaned = 0.845337 Jy ! Total flux subtracted in 100 components = 0.845337 Jy ! Clean residual min=-0.066596 max=0.224072 Jy/beam ! Clean residual mean=0.000523 rms=0.022762 Jy/beam ! Combined flux in latest and established models = 0.845337 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.845337 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.543664Jy sigma=0.004158 ! Fit after self-cal, rms=0.542761Jy sigma=0.004152 ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Added new window around map position (-6.6, -3.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.207352 Jy ! Component: 100 - total flux cleaned = 0.337268 Jy ! Total flux subtracted in 100 components = 0.337268 Jy ! Clean residual min=-0.048060 max=0.111817 Jy/beam ! Clean residual mean=0.000281 rms=0.015619 Jy/beam ! Combined flux in latest and established models = 1.1826 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 29 components and 1.1826 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.442490Jy sigma=0.003059 ! Fit after self-cal, rms=0.438198Jy sigma=0.003032 ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Added new window around map position (-4.8, -2.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.117658 Jy ! Component: 100 - total flux cleaned = 0.205318 Jy ! Total flux subtracted in 100 components = 0.205318 Jy ! Clean residual min=-0.035847 max=0.087167 Jy/beam ! Clean residual mean=0.000178 rms=0.012077 Jy/beam ! Combined flux in latest and established models = 1.38792 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 40 components and 1.38792 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.393155Jy sigma=0.002509 ! Fit after self-cal, rms=0.391595Jy sigma=0.002501 ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Added new window around map position (-1.6, -1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0862823 Jy ! Component: 100 - total flux cleaned = 0.150877 Jy ! Total flux subtracted in 100 components = 0.150877 Jy ! Clean residual min=-0.030071 max=0.052798 Jy/beam ! Clean residual mean=0.000133 rms=0.009889 Jy/beam ! Combined flux in latest and established models = 1.5388 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 54 components and 1.5388 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.362930Jy sigma=0.002133 ! Fit after self-cal, rms=0.361850Jy sigma=0.002125 ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec print "************** FINISHED UNIFORM WEIGHTING CLEAN **************" ! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** ! uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. win_mult = win_mult * 1.6 clean_niter = clean_niter * 2 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Estimated beam: bmin=0.9057 mas, bmaj=1.368 mas, bpa=6.587 degrees ! Estimated noise=773.99 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 = 0.0938255 Jy ! Component: 100 - total flux cleaned = 0.16177 Jy ! Component: 150 - total flux cleaned = 0.214475 Jy ! Component: 200 - total flux cleaned = 0.256393 Jy ! Total flux subtracted in 200 components = 0.256393 Jy ! Clean residual min=-0.023667 max=0.048812 Jy/beam ! Clean residual mean=0.002653 rms=0.009890 Jy/beam ! Combined flux in latest and established models = 1.79519 Jy ! Performing phase self-cal ! Adding 41 model components to the UV plane model. ! The established model now contains 74 components and 1.79519 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.334383Jy sigma=0.001709 ! Fit after self-cal, rms=0.333326Jy sigma=0.001698 ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 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 1.00* FD 1.00* GC 1.05 GG 1.00* ! HN 1.08 KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 1.03 NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* TC 1.00* ! TS 1.09 WF 1.00* WZ 1.00* ! ! A total of 33 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.95 FD 0.98 GC 0.97 GG 1.00* ! HN 0.97 KP 0.92 LA 0.92 MA 1.00* ! MK 1.01 NL 1.10 NY 1.00* ON 1.00* ! OV 1.01 PT 0.96 SC 1.44 TC 1.12 ! TS 0.98 WF 0.97 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* GC 1.09 GG 1.00* ! HN 1.22 KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 0.87 NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* TC 1.00* ! TS 1.25 WF 1.00* WZ 1.00* ! ! A total of 30 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 FD 0.97 GC 1.02 GG 1.00* ! HN 0.98 KP 0.89 LA 0.92 MA 1.00* ! MK 1.05 NL 1.07 NY 1.00* ON 1.00* ! OV 1.00 PT 1.01 SC 1.47 TC 1.09 ! TS 1.01 WF 1.00 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! ! 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 1.00* GC 1.13 GG 1.00* ! HN 1.30 KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 0.80 NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* TC 1.00* ! TS 1.01 WF 1.00* WZ 1.00* ! ! A total of 30 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.97 GC 1.12 GG 1.00* ! HN 0.97 KP 0.86 LA 0.92 MA 1.00* ! MK 1.02 NL 1.06 NY 1.00* ON 1.00* ! OV 1.02 PT 0.98 SC 1.46 TC 1.01 ! TS 1.07 WF 1.10 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! ! Correcting IF 4. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* GC 1.08 GG 1.00* ! HN 1.36 KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 0.77 NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* TC 1.00* ! TS 1.05 WF 1.00* WZ 1.00* ! ! A total of 33 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 FD 0.96 GC 1.12 GG 1.00* ! HN 0.98 KP 0.88 LA 0.92 MA 1.00* ! MK 1.03 NL 1.03 NY 1.00* ON 1.00* ! OV 1.01 PT 0.98 SC 1.37 TC 0.97 ! TS 1.06 WF 1.07 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! ! Fit before self-cal, rms=0.333326Jy sigma=0.001698 ! Fit after self-cal, rms=0.353529Jy sigma=0.001532 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Estimated beam: bmin=0.926 mas, bmaj=1.401 mas, bpa=5.962 degrees ! Estimated noise=759.477 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 (-3.4, -1.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0358557 Jy ! Component: 100 - total flux cleaned = 0.0466862 Jy ! Component: 150 - total flux cleaned = 0.0513593 Jy ! Component: 200 - total flux cleaned = 0.0542921 Jy ! Total flux subtracted in 200 components = 0.0542921 Jy ! Clean residual min=-0.016269 max=0.041161 Jy/beam ! Clean residual mean=0.002276 rms=0.006672 Jy/beam ! Combined flux in latest and established models = 1.84948 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 96 components and 1.84948 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.349464Jy sigma=0.001474 ! Fit after self-cal, rms=0.349460Jy sigma=0.001471 ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Added new window around map position (-10.8, -4.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0418925 Jy ! Component: 100 - total flux cleaned = 0.0670365 Jy ! Component: 150 - total flux cleaned = 0.084515 Jy ! Component: 200 - total flux cleaned = 0.0956225 Jy ! Total flux subtracted in 200 components = 0.0956225 Jy ! Clean residual min=-0.013092 max=0.031261 Jy/beam ! Clean residual mean=0.001346 rms=0.004728 Jy/beam ! Combined flux in latest and established models = 1.94511 Jy ! Performing phase self-cal ! Adding 36 model components to the UV plane model. ! The established model now contains 128 components and 1.94511 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.344814Jy sigma=0.001372 ! Fit after self-cal, rms=0.344344Jy sigma=0.001365 ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Added new window around map position (-8.2, -3.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0278096 Jy ! Component: 100 - total flux cleaned = 0.0426161 Jy ! Component: 150 - total flux cleaned = 0.0491338 Jy ! Component: 200 - total flux cleaned = 0.053947 Jy ! Total flux subtracted in 200 components = 0.053947 Jy ! Clean residual min=-0.011254 max=0.021491 Jy/beam ! Clean residual mean=0.000773 rms=0.003683 Jy/beam ! Combined flux in latest and established models = 1.99905 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 152 components and 1.99905 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.342054Jy sigma=0.001321 ! Fit after self-cal, rms=0.341864Jy sigma=0.001319 ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Added new window around map position (-13.4, -3.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0201444 Jy ! Component: 100 - total flux cleaned = 0.031126 Jy ! Component: 150 - total flux cleaned = 0.0359472 Jy ! Component: 200 - total flux cleaned = 0.038901 Jy ! Total flux subtracted in 200 components = 0.038901 Jy ! Clean residual min=-0.011580 max=0.012361 Jy/beam ! Clean residual mean=0.000411 rms=0.003049 Jy/beam ! Combined flux in latest and established models = 2.03795 Jy ! Performing phase self-cal ! Adding 32 model components to the UV plane model. ! The established model now contains 177 components and 2.03796 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.340701Jy sigma=0.001296 ! Fit after self-cal, rms=0.340613Jy sigma=0.001294 ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 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=0.340613Jy sigma=0.001294 ! Fit after self-cal, rms=0.338996Jy sigma=0.001262 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Estimated beam: bmin=0.9276 mas, bmaj=1.402 mas, bpa=5.809 degrees ! Estimated noise=758.719 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0105849 Jy ! Component: 100 - total flux cleaned = 0.0181733 Jy ! Component: 150 - total flux cleaned = 0.0238071 Jy ! Component: 200 - total flux cleaned = 0.0282495 Jy ! Total flux subtracted in 200 components = 0.0282495 Jy ! Clean residual min=-0.007588 max=0.008336 Jy/beam ! Clean residual mean=0.000342 rms=0.002138 Jy/beam ! Combined flux in latest and established models = 2.06621 Jy selfcal ! Performing phase self-cal ! Adding 36 model components to the UV plane model. ! The established model now contains 198 components and 2.06621 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.338424Jy sigma=0.001252 ! Fit after self-cal, rms=0.338457Jy sigma=0.001251 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 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 = 0.0050183 Jy ! Component: 100 - total flux cleaned = 0.00892838 Jy ! Component: 150 - total flux cleaned = 0.0122065 Jy ! Component: 200 - total flux cleaned = 0.0144354 Jy ! Total flux subtracted in 200 components = 0.0144354 Jy ! Clean residual min=-0.007402 max=0.007909 Jy/beam ! Clean residual mean=0.000196 rms=0.001996 Jy/beam ! Combined flux in latest and established models = 2.08064 Jy ! Performing phase self-cal ! Adding 37 model components to the UV plane model. ! The established model now contains 208 components and 2.08064 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.338174Jy sigma=0.001247 ! Fit after self-cal, rms=0.338142Jy sigma=0.001247 ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 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=0.338142Jy sigma=0.001247 ! Fit after self-cal, rms=0.338566Jy sigma=0.001229 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Estimated beam: bmin=0.9268 mas, bmaj=1.403 mas, bpa=5.688 degrees ! Estimated noise=758.142 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00790902 Jy ! Component: 100 - total flux cleaned = 0.0124417 Jy ! Component: 150 - total flux cleaned = 0.0151483 Jy ! Component: 200 - total flux cleaned = 0.0168862 Jy ! Total flux subtracted in 200 components = 0.0168862 Jy ! Clean residual min=-0.006051 max=0.006918 Jy/beam ! Clean residual mean=0.000113 rms=0.001684 Jy/beam ! Combined flux in latest and established models = 2.09753 Jy selfcal ! Performing phase self-cal ! Adding 36 model components to the UV plane model. ! The established model now contains 230 components and 2.09753 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.338275Jy sigma=0.001224 ! Fit after self-cal, rms=0.338273Jy sigma=0.001223 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 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 = 0.00275066 Jy ! Component: 100 - total flux cleaned = 0.00438214 Jy ! Component: 150 - total flux cleaned = 0.00574947 Jy ! Component: 200 - total flux cleaned = 0.00717209 Jy ! Total flux subtracted in 200 components = 0.00717209 Jy ! Clean residual min=-0.005747 max=0.006425 Jy/beam ! Clean residual mean=0.000040 rms=0.001607 Jy/beam ! Combined flux in latest and established models = 2.1047 Jy ! Performing phase self-cal ! Adding 41 model components to the UV plane model. ! The established model now contains 238 components and 2.1047 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.338118Jy sigma=0.001221 ! Fit after self-cal, rms=0.338099Jy sigma=0.001221 ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 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=0.338099Jy sigma=0.001221 ! Fit after self-cal, rms=0.339562Jy sigma=0.001220 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Estimated beam: bmin=2.061 mas, bmaj=3.081 mas, bpa=6.758 degrees ! Estimated noise=861.448 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00740768 Jy ! Component: 100 - total flux cleaned = 0.0124535 Jy ! Component: 150 - total flux cleaned = 0.0154676 Jy ! Component: 200 - total flux cleaned = 0.0167867 Jy ! Total flux subtracted in 200 components = 0.0167867 Jy ! Clean residual min=-0.005935 max=0.007078 Jy/beam ! Clean residual mean=0.000075 rms=0.001914 Jy/beam ! Combined flux in latest and established models = 2.12149 Jy selfcal ! Performing phase self-cal ! Adding 51 model components to the UV plane model. ! The established model now contains 274 components and 2.12149 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.339486Jy sigma=0.001218 ! Fit after self-cal, rms=0.339455Jy sigma=0.001218 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 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 = 0.00169314 Jy ! Component: 100 - total flux cleaned = 0.00319656 Jy ! Component: 150 - total flux cleaned = 0.0039792 Jy ! Component: 200 - total flux cleaned = 0.00458155 Jy ! Total flux subtracted in 200 components = 0.00458155 Jy ! Clean residual min=-0.005736 max=0.006900 Jy/beam ! Clean residual mean=-0.000035 rms=0.001855 Jy/beam ! Combined flux in latest and established models = 2.12607 Jy ! Performing phase self-cal ! Adding 38 model components to the UV plane model. ! The established model now contains 297 components and 2.12607 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.339431Jy sigma=0.001217 ! Fit after self-cal, rms=0.339410Jy sigma=0.001217 ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "************** FINISHED AMPLITUDE SELF-CAL **************" ! ************** FINISHED AMPLITUDE SELF-CAL ************** restore ! Inverting map and beam ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Estimated beam: bmin=0.9263 mas, bmaj=1.405 mas, bpa=5.568 degrees ! Estimated noise=757.968 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9263 x 1.405 at 5.568 degrees (North through East) ! Clean map min=-0.006085 max=0.81196 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=0.339410Jy sigma=0.001217 ! Fit after self-cal, rms=0.324328Jy sigma=0.001123 ! Inverting map and beam ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Estimated beam: bmin=0.926 mas, bmaj=1.405 mas, bpa=5.569 degrees ! Estimated noise=758.005 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00241309 Jy ! Component: 100 - total flux cleaned = 0.00339726 Jy ! Component: 150 - total flux cleaned = 0.00404431 Jy ! Component: 200 - total flux cleaned = 0.00477239 Jy ! Total flux subtracted in 200 components = 0.00477239 Jy ! Clean residual min=-0.005702 max=0.005373 Jy/beam ! Clean residual mean=-0.000007 rms=0.001339 Jy/beam ! Combined flux in latest and established models = 2.13084 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 311 components and 2.13084 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.324204Jy sigma=0.001122 ! Fit after self-cal, rms=0.324188Jy sigma=0.001121 ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000956535 Jy ! Component: 100 - total flux cleaned = 0.00164799 Jy ! Component: 150 - total flux cleaned = 0.00219547 Jy ! Component: 200 - total flux cleaned = 0.00250612 Jy ! Total flux subtracted in 200 components = 0.00250612 Jy ! Clean residual min=-0.005725 max=0.005129 Jy/beam ! Clean residual mean=-0.000032 rms=0.001306 Jy/beam ! Combined flux in latest and established models = 2.13335 Jy ! Performing phase self-cal ! Adding 36 model components to the UV plane model. ! The established model now contains 318 components and 2.13335 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.324109Jy sigma=0.001120 ! Fit after self-cal, rms=0.324094Jy sigma=0.001120 ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.324094Jy sigma=0.001120 ! Fit after self-cal, rms=0.324824Jy sigma=0.001120 print "************** CLEARING MODEL AND STARTING OVER **********" ! ************** CLEARING MODEL AND STARTING OVER ********** clrmod true ! clrmod: Cleared the established and tentative models. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Estimated beam: bmin=0.6892 mas, bmaj=1.272 mas, bpa=1.654 degrees ! Estimated noise=1193.36 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.620417 Jy ! Component: 100 - total flux cleaned = 0.88745 Jy ! Component: 150 - total flux cleaned = 1.06306 Jy ! Component: 200 - total flux cleaned = 1.19526 Jy ! Total flux subtracted in 200 components = 1.19526 Jy ! Clean residual min=-0.041618 max=0.077383 Jy/beam ! Clean residual mean=0.000414 rms=0.013027 Jy/beam ! Combined flux in latest and established models = 1.19526 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 25 model components to the UV plane model. ! The established model now contains 25 components and 1.19526 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Estimated beam: bmin=0.9264 mas, bmaj=1.405 mas, bpa=5.575 degrees ! Estimated noise=757.955 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 = 0.156943 Jy ! Component: 100 - total flux cleaned = 0.273108 Jy ! Component: 150 - total flux cleaned = 0.361856 Jy ! Component: 200 - total flux cleaned = 0.431762 Jy ! Total flux subtracted in 200 components = 0.431762 Jy ! Clean residual min=-0.020536 max=0.043155 Jy/beam ! Clean residual mean=0.005043 rms=0.010405 Jy/beam ! Combined flux in latest and established models = 1.62703 Jy ! Adding 61 model components to the UV plane model. ! The established model now contains 72 components and 1.62703 Jy ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Estimated beam: bmin=2.062 mas, bmaj=3.082 mas, bpa=6.797 degrees ! Estimated noise=860.647 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.109503 Jy ! Component: 100 - total flux cleaned = 0.191117 Jy ! Component: 150 - total flux cleaned = 0.253988 Jy ! Component: 200 - total flux cleaned = 0.302997 Jy ! Total flux subtracted in 200 components = 0.302997 Jy ! Clean residual min=-0.014135 max=0.033581 Jy/beam ! Clean residual mean=0.004769 rms=0.008225 Jy/beam ! Combined flux in latest and established models = 1.93002 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 = 0.0385976 Jy ! Component: 100 - total flux cleaned = 0.0693097 Jy ! Component: 150 - total flux cleaned = 0.0940289 Jy ! Component: 200 - total flux cleaned = 0.114085 Jy ! Total flux subtracted in 200 components = 0.114085 Jy ! Clean residual min=-0.007437 max=0.015371 Jy/beam ! Clean residual mean=0.002228 rms=0.003930 Jy/beam ! Combined flux in latest and established models = 2.04411 Jy ! Adding 138 model components to the UV plane model. ! The established model now contains 186 components and 2.04411 Jy ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! Estimated beam: bmin=0.9264 mas, bmaj=1.405 mas, bpa=5.575 degrees ! Estimated noise=757.955 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0133829 Jy ! Component: 100 - total flux cleaned = 0.0241447 Jy ! Component: 150 - total flux cleaned = 0.0308889 Jy ! Component: 200 - total flux cleaned = 0.0373649 Jy ! Total flux subtracted in 200 components = 0.0373649 Jy ! Clean residual min=-0.007201 max=0.012532 Jy/beam ! Clean residual mean=0.000563 rms=0.001971 Jy/beam ! Combined flux in latest and established models = 2.08147 Jy selfcal ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 212 components and 2.08147 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.327992Jy sigma=0.001150 ! Fit after self-cal, rms=0.326947Jy sigma=0.001132 wmodel J0433+0521_X_2003_07_09_pus_map.mod ! Writing 212 model components to file: J0433+0521_X_2003_07_09_pus_map.mod wobs J0433+0521_X_2003_07_09_pus_uvs.fits ! Writing UV FITS file: J0433+0521_X_2003_07_09_pus_uvs.fits wwins J0433+0521_X_2003_07_09_pus_map.win ! wwins: Wrote 8 windows to J0433+0521_X_2003_07_09_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 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.00357333 Jy ! Component: 100 - total flux cleaned = 0.00673979 Jy ! Component: 150 - total flux cleaned = 0.0096766 Jy ! Component: 200 - total flux cleaned = 0.0124504 Jy ! Component: 250 - total flux cleaned = 0.0146796 Jy ! Component: 300 - total flux cleaned = 0.0167294 Jy ! Component: 350 - total flux cleaned = 0.0184225 Jy ! Component: 400 - total flux cleaned = 0.0196843 Jy ! Component: 450 - total flux cleaned = 0.0207266 Jy ! Component: 500 - total flux cleaned = 0.0215621 Jy ! Component: 550 - total flux cleaned = 0.0225614 Jy ! Component: 600 - total flux cleaned = 0.0232741 Jy ! Component: 650 - total flux cleaned = 0.0241473 Jy ! Component: 700 - total flux cleaned = 0.0248331 Jy ! Component: 750 - total flux cleaned = 0.0255903 Jy ! Component: 800 - total flux cleaned = 0.0263349 Jy ! Component: 850 - total flux cleaned = 0.0273084 Jy ! Component: 900 - total flux cleaned = 0.027946 Jy ! Component: 950 - total flux cleaned = 0.0285738 Jy ! Component: 1000 - total flux cleaned = 0.029424 Jy ! Component: 1050 - total flux cleaned = 0.0301084 Jy ! Component: 1100 - total flux cleaned = 0.0307826 Jy ! Component: 1150 - total flux cleaned = 0.031226 Jy ! Component: 1200 - total flux cleaned = 0.0318821 Jy ! Component: 1250 - total flux cleaned = 0.0326002 Jy ! Component: 1300 - total flux cleaned = 0.0333084 Jy ! Component: 1350 - total flux cleaned = 0.0339375 Jy ! Component: 1400 - total flux cleaned = 0.0345588 Jy ! Component: 1450 - total flux cleaned = 0.0351726 Jy ! Component: 1500 - total flux cleaned = 0.0358455 Jy ! Component: 1550 - total flux cleaned = 0.0363769 Jy ! Component: 1600 - total flux cleaned = 0.0369026 Jy ! Component: 1650 - total flux cleaned = 0.0374228 Jy ! Component: 1700 - total flux cleaned = 0.0378086 Jy ! Component: 1750 - total flux cleaned = 0.0384438 Jy ! Component: 1800 - total flux cleaned = 0.0388208 Jy ! Component: 1850 - total flux cleaned = 0.0391934 Jy ! Component: 1900 - total flux cleaned = 0.0396851 Jy ! Component: 1950 - total flux cleaned = 0.039928 Jy ! Component: 2000 - total flux cleaned = 0.0403495 Jy ! Total flux subtracted in 2048 components = 0.0407073 Jy ! Clean residual min=-0.003939 max=0.002969 Jy/beam ! Clean residual mean=0.000178 rms=0.001035 Jy/beam ! Combined flux in latest and established models = 2.12218 Jy keep ! Adding 147 model components to the UV plane model. ! The established model now contains 352 components and 2.12218 Jy ![Exited script file: muppet] wmap "J0433+0521_X_2003_07_09_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9264 x 1.405 at 5.575 degrees (North through East) ! Clean map min=-0.0051251 max=0.81488 Jy/beam ! Writing clean map to FITS file: J0433+0521_X_2003_07_09_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.814881 invert ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1761 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00103999 device "J0433+0521_X_2003_07_09_pus\_map.eps/VPS" ! Attempting to open device: 'J0433+0521_X_2003_07_09_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.382874 0.382874 0.765749 1.5315 3.06299 6.12599 12.252 24.504 49.0079 98.0158 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0031 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.814 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9264 x 1.405 at 5.575 degrees (North through East) ! Clean map min=-0.0051251 max=0.81488 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. quit ! Quitting program ! Log file J0433+0521_X_2003_07_09_pus_uvs.log closed on Sun Apr 7 11:45:41 2013