! Started logfile: J0339-0146_X_2001_03_12_pus_uvs.log on Wed Jan 2 19:50:22 2013 obs J0339-0146_X_2001_03_12_pus_uva.fits ! Reading UV FITS file: J0339-0146_X_2001_03_12_pus_uva.fits ! AN table 1: 30 integrations on 136 of 136 possible baselines. ! AN table 2: 9 integrations on 136 of 136 possible baselines. ! AN table 3: 52 integrations on 136 of 136 possible baselines. ! AN table 4: 36 integrations on 136 of 136 possible baselines. ! AN table 5: 17 integrations on 136 of 136 possible baselines. ! Apparent sampling: 0.130106 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0339-0146 ! ! 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 1749 lines of history. ! ! Reading 10192 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 J0339-0146_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 380 telescope corrections were flagged in sub-array 1. ! A total of 141 telescope corrections were flagged in sub-array 2. ! A total of 510 telescope corrections were flagged in sub-array 3. ! A total of 579 telescope corrections were flagged in sub-array 4. ! A total of 140 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 380 telescope corrections were flagged in sub-array 1. ! A total of 141 telescope corrections were flagged in sub-array 2. ! A total of 510 telescope corrections were flagged in sub-array 3. ! A total of 579 telescope corrections were flagged in sub-array 4. ! A total of 140 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 380 telescope corrections were flagged in sub-array 1. ! A total of 141 telescope corrections were flagged in sub-array 2. ! A total of 510 telescope corrections were flagged in sub-array 3. ! A total of 579 telescope corrections were flagged in sub-array 4. ! A total of 140 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 380 telescope corrections were flagged in sub-array 1. ! A total of 141 telescope corrections were flagged in sub-array 2. ! A total of 510 telescope corrections were flagged in sub-array 3. ! A total of 579 telescope corrections were flagged in sub-array 4. ! A total of 140 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=0.958530Jy sigma=0.008818 ! Fit after self-cal, rms=0.585240Jy sigma=0.005456 ! 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 2.29% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! Estimated beam: bmin=0.5952 mas, bmaj=1.612 mas, bpa=-2.915 degrees ! Estimated noise=1166.56 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 = 0.964761 Jy ! Component: 100 - total flux cleaned = 1.2847 Jy ! Total flux subtracted in 100 components = 1.2847 Jy ! Clean residual min=-0.042242 max=0.141721 Jy/beam ! Clean residual mean=-0.000109 rms=0.014786 Jy/beam ! Combined flux in latest and established models = 1.2847 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 1.2847 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.410030Jy sigma=0.003658 ! Fit after self-cal, rms=0.404829Jy sigma=0.003629 ! Inverting map ! Your choice of large map pixels excluded 2.29% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! Added new window around map position (0.6, 0.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.166075 Jy ! Component: 100 - total flux cleaned = 0.256299 Jy ! Total flux subtracted in 100 components = 0.256299 Jy ! Clean residual min=-0.034449 max=0.070166 Jy/beam ! Clean residual mean=-0.000082 rms=0.008935 Jy/beam ! Combined flux in latest and established models = 1.541 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 20 components and 1.541 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.289666Jy sigma=0.002360 ! Fit after self-cal, rms=0.286016Jy sigma=0.002336 ! Inverting map ! Your choice of large map pixels excluded 2.29% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! Added new window around map position (1.4, 1.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.073591 Jy ! Component: 100 - total flux cleaned = 0.121427 Jy ! Total flux subtracted in 100 components = 0.121427 Jy ! Clean residual min=-0.029519 max=0.042003 Jy/beam ! Clean residual mean=-0.000075 rms=0.006796 Jy/beam ! Combined flux in latest and established models = 1.66242 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 30 components and 1.66242 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.251844Jy sigma=0.001920 ! Fit after self-cal, rms=0.249662Jy sigma=0.001901 ! Inverting map ! Your choice of large map pixels excluded 2.29% of the data. ! The x-axis pixel size should ideally be below 0.1708 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 2.29% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! Estimated beam: bmin=0.7883 mas, bmaj=2.057 mas, bpa=-5.283 degrees ! Estimated noise=811.597 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 = 0.0761449 Jy ! Component: 100 - total flux cleaned = 0.119915 Jy ! Component: 150 - total flux cleaned = 0.148398 Jy ! Component: 200 - total flux cleaned = 0.167372 Jy ! Total flux subtracted in 200 components = 0.167372 Jy ! Clean residual min=-0.020462 max=0.039428 Jy/beam ! Clean residual mean=-0.000151 rms=0.005692 Jy/beam ! Combined flux in latest and established models = 1.8298 Jy ! Performing phase self-cal ! Adding 43 model components to the UV plane model. ! The established model now contains 63 components and 1.8298 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.227941Jy sigma=0.001603 ! Fit after self-cal, rms=0.226282Jy sigma=0.001588 ! Inverting map ! Your choice of large map pixels excluded 2.29% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! Added new window around map position (3, 1.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0399406 Jy ! Component: 100 - total flux cleaned = 0.0528333 Jy ! Component: 150 - total flux cleaned = 0.0584952 Jy ! Component: 200 - total flux cleaned = 0.0633018 Jy ! Total flux subtracted in 200 components = 0.0633018 Jy ! Clean residual min=-0.016500 max=0.016519 Jy/beam ! Clean residual mean=-0.000123 rms=0.004411 Jy/beam ! Combined flux in latest and established models = 1.8931 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 83 components and 1.8931 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.220170Jy sigma=0.001509 ! Fit after self-cal, rms=0.219044Jy sigma=0.001496 ! Inverting map ! Your choice of large map pixels excluded 2.29% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 39 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.09 HH 0.95 HN 1.02 ! KK 1.00* KP 1.00* LA 1.16 MA 0.81 ! MC 1.00* MK 1.00* NL 1.07 ON 1.00* ! OV 1.00* PT 1.08 SC 1.03 TS 1.00* ! WZ 1.00* ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 FD 1.01 HH 1.00* HN 1.02 ! KK 1.04 KP 0.97 LA 0.99 MA 1.00* ! MC 1.00* MK 0.93 NL 1.01 ON 1.00* ! OV 0.98 PT 0.96 SC 1.00 TS 1.00* ! WZ 1.07 ! ! A total of 33 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 FD 1.05 HH 1.00* HN 1.00* ! KK 0.96 KP 1.02 LA 1.01 MA 1.00* ! MC 1.00* MK 1.02 NL 1.04 ON 1.00* ! OV 0.98 PT 0.96 SC 1.00* TS 1.06 ! WZ 1.00* ! ! ! Correcting IF 2. ! A total of 39 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.06 HH 0.95 HN 1.04 ! KK 1.00* KP 1.00* LA 1.15 MA 0.82 ! MC 1.00* MK 1.00* NL 1.05 ON 1.00* ! OV 1.00* PT 1.12 SC 1.00 TS 1.00* ! WZ 1.00* ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 1.00 HH 1.00* HN 1.01 ! KK 1.02 KP 0.93 LA 0.99 MA 1.00* ! MC 1.00* MK 0.95 NL 0.98 ON 1.00* ! OV 0.99 PT 1.00 SC 0.97 TS 1.00* ! WZ 1.07 ! ! A total of 33 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.98 FD 1.03 HH 1.00* HN 1.00* ! KK 0.94 KP 0.98 LA 1.00 MA 1.00* ! MC 1.00* MK 1.00 NL 0.99 ON 1.00* ! OV 0.98 PT 1.01 SC 1.00* TS 1.07 ! WZ 1.00* ! ! ! Correcting IF 3. ! A total of 39 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.06 HH 0.98 HN 1.05 ! KK 1.00* KP 1.00* LA 1.21 MA 0.80 ! MC 1.00* MK 1.00* NL 1.09 ON 1.00* ! OV 1.00* PT 1.15 SC 1.01 TS 1.00* ! WZ 1.00* ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 0.99 HH 1.00* HN 1.03 ! KK 1.09 KP 0.92 LA 1.01 MA 1.00* ! MC 1.00* MK 0.95 NL 1.00 ON 1.00* ! OV 1.02 PT 1.02 SC 0.99 TS 1.00* ! WZ 1.09 ! ! A total of 33 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 FD 1.03 HH 1.00* HN 1.00* ! KK 1.03 KP 0.96 LA 1.02 MA 1.00* ! MC 1.00* MK 1.01 NL 1.02 ON 1.00* ! OV 1.02 PT 1.04 SC 1.00* TS 1.02 ! WZ 1.00* ! ! ! Correcting IF 4. ! A total of 39 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.04 HH 0.99 HN 1.07 ! KK 1.00* KP 1.00* LA 1.17 MA 0.85 ! MC 1.00* MK 1.00* NL 1.09 ON 1.00* ! OV 1.00* PT 1.15 SC 1.08 TS 1.00* ! WZ 1.00* ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 0.97 HH 1.00* HN 1.02 ! KK 1.05 KP 0.93 LA 0.98 MA 1.00* ! MC 1.00* MK 0.96 NL 1.01 ON 1.00* ! OV 1.00 PT 1.01 SC 1.04 TS 1.00* ! WZ 1.09 ! ! A total of 33 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.98 FD 1.02 HH 1.00* HN 1.00* ! KK 0.97 KP 0.97 LA 1.00 MA 1.00* ! MC 1.00* MK 1.05 NL 1.05 ON 1.00* ! OV 1.00 PT 1.03 SC 1.00* TS 1.02 ! WZ 1.00* ! ! ! Fit before self-cal, rms=0.219044Jy sigma=0.001496 ! Fit after self-cal, rms=0.177186Jy sigma=0.001309 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! Estimated beam: bmin=0.7967 mas, bmaj=2.177 mas, bpa=-5.388 degrees ! Estimated noise=811.674 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 (4.8, 3.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00877893 Jy ! Component: 100 - total flux cleaned = 0.0133612 Jy ! Component: 150 - total flux cleaned = 0.0165973 Jy ! Component: 200 - total flux cleaned = 0.0172514 Jy ! Total flux subtracted in 200 components = 0.0172514 Jy ! Clean residual min=-0.006835 max=0.006362 Jy/beam ! Clean residual mean=0.000010 rms=0.001834 Jy/beam ! Combined flux in latest and established models = 1.91035 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 98 components and 1.91035 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.175790Jy sigma=0.001295 ! Fit after self-cal, rms=0.175509Jy sigma=0.001293 ! Inverting map ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 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=0.175509Jy sigma=0.001293 ! Fit after self-cal, rms=0.175175Jy sigma=0.001284 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! Estimated beam: bmin=0.7977 mas, bmaj=2.177 mas, bpa=-5.38 degrees ! Estimated noise=812.273 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00267485 Jy ! Component: 100 - total flux cleaned = 0.0054758 Jy ! Component: 150 - total flux cleaned = 0.00711027 Jy ! Component: 200 - total flux cleaned = 0.00726654 Jy ! Total flux subtracted in 200 components = 0.00726654 Jy ! Clean residual min=-0.005731 max=0.005351 Jy/beam ! Clean residual mean=0.000007 rms=0.001377 Jy/beam ! Combined flux in latest and established models = 1.91762 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 107 components and 1.91762 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.174519Jy sigma=0.001279 ! Fit after self-cal, rms=0.174373Jy sigma=0.001278 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 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 = 0.000995352 Jy ! Component: 100 - total flux cleaned = 0.00244169 Jy ! Component: 150 - total flux cleaned = 0.0027015 Jy ! Component: 200 - total flux cleaned = 0.00270031 Jy ! Total flux subtracted in 200 components = 0.00270031 Jy ! Clean residual min=-0.005265 max=0.004931 Jy/beam ! Clean residual mean=0.000007 rms=0.001302 Jy/beam ! Combined flux in latest and established models = 1.92032 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 112 components and 1.92032 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.174000Jy sigma=0.001275 ! Fit after self-cal, rms=0.173930Jy sigma=0.001274 ! Inverting map ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 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=0.173930Jy sigma=0.001274 ! Fit after self-cal, rms=0.174457Jy sigma=0.001274 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! Estimated beam: bmin=0.7991 mas, bmaj=2.177 mas, bpa=-5.383 degrees ! Estimated noise=812.99 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00205542 Jy ! Component: 100 - total flux cleaned = 0.00340592 Jy ! Component: 150 - total flux cleaned = 0.00400682 Jy ! Component: 200 - total flux cleaned = 0.00400778 Jy ! Total flux subtracted in 200 components = 0.00400778 Jy ! Clean residual min=-0.004749 max=0.004676 Jy/beam ! Clean residual mean=0.000003 rms=0.001221 Jy/beam ! Combined flux in latest and established models = 1.92432 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 117 components and 1.92432 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.174145Jy sigma=0.001272 ! Fit after self-cal, rms=0.174084Jy sigma=0.001271 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 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 = 0.000532897 Jy ! Component: 100 - total flux cleaned = 0.00133822 Jy ! Component: 150 - total flux cleaned = 0.0014335 Jy ! Component: 200 - total flux cleaned = 0.00152521 Jy ! Total flux subtracted in 200 components = 0.00152521 Jy ! Clean residual min=-0.004648 max=0.004510 Jy/beam ! Clean residual mean=0.000003 rms=0.001188 Jy/beam ! Combined flux in latest and established models = 1.92585 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 120 components and 1.92585 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.173884Jy sigma=0.001270 ! Fit after self-cal, rms=0.173844Jy sigma=0.001270 ! Inverting map ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 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=0.173844Jy sigma=0.001270 ! Fit after self-cal, rms=0.174205Jy sigma=0.001269 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! Estimated beam: bmin=2.311 mas, bmaj=3.577 mas, bpa=-5.526 degrees ! Estimated noise=983.498 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00311704 Jy ! Component: 100 - total flux cleaned = 0.00319571 Jy ! Component: 150 - total flux cleaned = 0.00314078 Jy ! Component: 200 - total flux cleaned = 0.00314163 Jy ! Total flux subtracted in 200 components = 0.00314163 Jy ! Clean residual min=-0.004834 max=0.004212 Jy/beam ! Clean residual mean=0.000000 rms=0.001354 Jy/beam ! Combined flux in latest and established models = 1.92899 Jy selfcal ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 137 components and 1.92899 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.174138Jy sigma=0.001269 ! Fit after self-cal, rms=0.174120Jy sigma=0.001268 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 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 = 0.00061119 Jy ! Component: 100 - total flux cleaned = 0.000778419 Jy ! Component: 150 - total flux cleaned = 0.000732526 Jy ! Component: 200 - total flux cleaned = 0.000651172 Jy ! Total flux subtracted in 200 components = 0.000651172 Jy ! Clean residual min=-0.004794 max=0.004161 Jy/beam ! Clean residual mean=0.000000 rms=0.001346 Jy/beam ! Combined flux in latest and established models = 1.92964 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 145 components and 1.92964 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.174077Jy sigma=0.001268 ! Fit after self-cal, rms=0.174063Jy sigma=0.001268 ! Inverting map ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 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 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! Estimated beam: bmin=0.8001 mas, bmaj=2.177 mas, bpa=-5.385 degrees ! Estimated noise=813.559 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8001 x 2.177 at -5.385 degrees (North through East) ! Clean map min=-0.0071588 max=1.2993 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=0.174063Jy sigma=0.001268 ! Fit after self-cal, rms=0.161397Jy sigma=0.001121 ! Inverting map and beam ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! Estimated beam: bmin=0.8004 mas, bmaj=2.179 mas, bpa=-5.417 degrees ! Estimated noise=812.789 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000411397 Jy ! Component: 100 - total flux cleaned = 0.000208496 Jy ! Component: 150 - total flux cleaned = 0.000112506 Jy ! Component: 200 - total flux cleaned = 0.000193658 Jy ! Total flux subtracted in 200 components = 0.000193658 Jy ! Clean residual min=-0.004531 max=0.004251 Jy/beam ! Clean residual mean=-0.000002 rms=0.001057 Jy/beam ! Combined flux in latest and established models = 1.92984 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 154 components and 1.92984 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.161206Jy sigma=0.001120 ! Fit after self-cal, rms=0.161172Jy sigma=0.001119 ! Inverting map ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 7.45654e-05 Jy ! Component: 100 - total flux cleaned = 0.000505008 Jy ! Component: 150 - total flux cleaned = 0.000507422 Jy ! Component: 200 - total flux cleaned = 0.0005076 Jy ! Total flux subtracted in 200 components = 0.0005076 Jy ! Clean residual min=-0.004429 max=0.004134 Jy/beam ! Clean residual mean=-0.000002 rms=0.001043 Jy/beam ! Combined flux in latest and established models = 1.93034 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 158 components and 1.93034 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.161040Jy sigma=0.001119 ! Fit after self-cal, rms=0.161013Jy sigma=0.001118 ! Inverting map ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.161013Jy sigma=0.001118 ! Fit after self-cal, rms=0.161298Jy sigma=0.001118 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 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! Estimated beam: bmin=0.6006 mas, bmaj=1.722 mas, bpa=-3.414 degrees ! Estimated noise=1180.18 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.976208 Jy ! Component: 100 - total flux cleaned = 1.32533 Jy ! Component: 150 - total flux cleaned = 1.4955 Jy ! Component: 200 - total flux cleaned = 1.59469 Jy ! Total flux subtracted in 200 components = 1.59469 Jy ! Clean residual min=-0.018076 max=0.052954 Jy/beam ! Clean residual mean=0.000001 rms=0.006522 Jy/beam ! Combined flux in latest and established models = 1.59469 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 15 model components to the UV plane model. ! The established model now contains 15 components and 1.59469 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! Estimated beam: bmin=0.8012 mas, bmaj=2.18 mas, bpa=-5.437 degrees ! Estimated noise=812.63 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 = 0.111968 Jy ! Component: 100 - total flux cleaned = 0.178181 Jy ! Component: 150 - total flux cleaned = 0.22162 Jy ! Component: 200 - total flux cleaned = 0.251486 Jy ! Total flux subtracted in 200 components = 0.251486 Jy ! Clean residual min=-0.008803 max=0.017088 Jy/beam ! Clean residual mean=-0.000040 rms=0.003004 Jy/beam ! Combined flux in latest and established models = 1.84618 Jy ! Adding 74 model components to the UV plane model. ! The established model now contains 77 components and 1.84618 Jy ! Inverting map ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! Added new window around map position (0, 1.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0215083 Jy ! Component: 100 - total flux cleaned = 0.0373093 Jy ! Component: 150 - total flux cleaned = 0.0491296 Jy ! Component: 200 - total flux cleaned = 0.0582241 Jy ! Total flux subtracted in 200 components = 0.0582241 Jy ! Clean residual min=-0.004993 max=0.007073 Jy/beam ! Clean residual mean=-0.000011 rms=0.001401 Jy/beam ! Combined flux in latest and established models = 1.9044 Jy ! Adding 43 model components to the UV plane model. ! The established model now contains 110 components and 1.9044 Jy ! Inverting map ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! Added new window around map position (1.6, -1). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00753526 Jy ! Component: 100 - total flux cleaned = 0.0132223 Jy ! Component: 150 - total flux cleaned = 0.0162165 Jy ! Component: 200 - total flux cleaned = 0.0184684 Jy ! Total flux subtracted in 200 components = 0.0184684 Jy ! Clean residual min=-0.004821 max=0.004311 Jy/beam ! Clean residual mean=-0.000004 rms=0.001131 Jy/beam ! Combined flux in latest and established models = 1.92287 Jy ! Adding 30 model components to the UV plane model. ! The established model now contains 123 components and 1.92287 Jy ! Inverting map ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 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 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! Estimated beam: bmin=2.309 mas, bmaj=3.577 mas, bpa=-5.567 degrees ! Estimated noise=982.424 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00403928 Jy ! Component: 100 - total flux cleaned = 0.00642077 Jy ! Component: 150 - total flux cleaned = 0.00677945 Jy ! Component: 200 - total flux cleaned = 0.00702967 Jy ! Total flux subtracted in 200 components = 0.00702967 Jy ! Clean residual min=-0.004416 max=0.004449 Jy/beam ! Clean residual mean=-0.000005 rms=0.001157 Jy/beam ! Combined flux in latest and established models = 1.9299 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 = 0.000114364 Jy ! Component: 100 - total flux cleaned = 0.000220486 Jy ! Component: 150 - total flux cleaned = 0.000220101 Jy ! Component: 200 - total flux cleaned = 0.000311183 Jy ! Total flux subtracted in 200 components = 0.000311183 Jy ! Clean residual min=-0.004366 max=0.004320 Jy/beam ! Clean residual mean=-0.000006 rms=0.001142 Jy/beam ! Combined flux in latest and established models = 1.93021 Jy ! Adding 48 model components to the UV plane model. ! The established model now contains 166 components and 1.93021 Jy ! Inverting map ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! Estimated beam: bmin=0.8012 mas, bmaj=2.18 mas, bpa=-5.437 degrees ! Estimated noise=812.63 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000868487 Jy ! Component: 100 - total flux cleaned = -0.000640229 Jy ! Component: 150 - total flux cleaned = -0.000537549 Jy ! Component: 200 - total flux cleaned = -0.000345215 Jy ! Total flux subtracted in 200 components = -0.000345215 Jy ! Clean residual min=-0.004495 max=0.003921 Jy/beam ! Clean residual mean=-0.000003 rms=0.001044 Jy/beam ! Combined flux in latest and established models = 1.92987 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 177 components and 1.92987 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.161554Jy sigma=0.001120 ! Fit after self-cal, rms=0.161375Jy sigma=0.001118 wmodel J0339-0146_X_2001_03_12_pus_map.mod ! Writing 177 model components to file: J0339-0146_X_2001_03_12_pus_map.mod wobs J0339-0146_X_2001_03_12_pus_uvs.fits ! Writing UV FITS file: J0339-0146_X_2001_03_12_pus_uvs.fits wwins J0339-0146_X_2001_03_12_pus_map.win ! wwins: Wrote 7 windows to J0339-0146_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 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000361412 Jy ! Component: 100 - total flux cleaned = -0.000562646 Jy ! Component: 150 - total flux cleaned = -0.000432616 Jy ! Component: 200 - total flux cleaned = -0.000188499 Jy ! Component: 250 - total flux cleaned = -0.000248062 Jy ! Component: 300 - total flux cleaned = -0.000132511 Jy ! Component: 350 - total flux cleaned = -2.00236e-05 Jy ! Component: 400 - total flux cleaned = 9.12891e-05 Jy ! Component: 450 - total flux cleaned = 0.000310049 Jy ! Component: 500 - total flux cleaned = 0.00057788 Jy ! Component: 550 - total flux cleaned = 0.000841523 Jy ! Component: 600 - total flux cleaned = 0.000946808 Jy ! Component: 650 - total flux cleaned = 0.00135877 Jy ! Component: 700 - total flux cleaned = 0.00140955 Jy ! Component: 750 - total flux cleaned = 0.00146046 Jy ! Component: 800 - total flux cleaned = 0.00160999 Jy ! Component: 850 - total flux cleaned = 0.00170863 Jy ! Component: 900 - total flux cleaned = 0.00185357 Jy ! Component: 950 - total flux cleaned = 0.0017576 Jy ! Component: 1000 - total flux cleaned = 0.00180561 Jy ! Component: 1050 - total flux cleaned = 0.00190044 Jy ! Component: 1100 - total flux cleaned = 0.00185352 Jy ! Component: 1150 - total flux cleaned = 0.00208619 Jy ! Component: 1200 - total flux cleaned = 0.00222392 Jy ! Component: 1250 - total flux cleaned = 0.00231473 Jy ! Component: 1300 - total flux cleaned = 0.00258613 Jy ! Component: 1350 - total flux cleaned = 0.0024963 Jy ! Component: 1400 - total flux cleaned = 0.0025411 Jy ! Component: 1450 - total flux cleaned = 0.0027186 Jy ! Component: 1500 - total flux cleaned = 0.00280676 Jy ! Component: 1550 - total flux cleaned = 0.00293782 Jy ! Component: 1600 - total flux cleaned = 0.00319791 Jy ! Component: 1650 - total flux cleaned = 0.00332745 Jy ! Component: 1700 - total flux cleaned = 0.00354056 Jy ! Component: 1750 - total flux cleaned = 0.00366789 Jy ! Component: 1800 - total flux cleaned = 0.00366755 Jy ! Component: 1850 - total flux cleaned = 0.0040437 Jy ! Component: 1900 - total flux cleaned = 0.00421013 Jy ! Component: 1950 - total flux cleaned = 0.00420989 Jy ! Component: 2000 - total flux cleaned = 0.00449732 Jy ! Total flux subtracted in 2048 components = 0.00441615 Jy ! Clean residual min=-0.002377 max=0.002428 Jy/beam ! Clean residual mean=-0.000006 rms=0.000756 Jy/beam ! Combined flux in latest and established models = 1.93428 Jy keep ! Adding 156 model components to the UV plane model. ! The established model now contains 332 components and 1.93428 Jy ![Exited script file: muppet] wmap "J0339-0146_X_2001_03_12_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8012 x 2.18 at -5.437 degrees (North through East) ! Clean map min=-0.0040167 max=1.2978 Jy/beam ! Writing clean map to FITS file: J0339-0146_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 1.2978 invert ! Inverting map ! Your choice of large map pixels excluded 2.37% of the data. ! The x-axis pixel size should ideally be below 0.1708 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000756855 device "J0339-0146_X_2001_03_12_pus\_map.eps/VPS" ! Attempting to open device: 'J0339-0146_X_2001_03_12_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.174955 0.174955 0.34991 0.699819 1.39964 2.79928 5.59855 11.1971 22.3942 44.7884 89.5769 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0022 print "peak=",int(1000*peak_flux)/1000 ! peak= 1.297 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8012 x 2.18 at -5.437 degrees (North through East) ! Clean map min=-0.0040167 max=1.2978 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. quit ! Quitting program ! Log file J0339-0146_X_2001_03_12_pus_uvs.log closed on Wed Jan 2 19:50:28 2013