! Started logfile: J1924-2914_X_2000_03_13_pus_uvs.log on Mon Apr 1 13:07:33 2013 obs J1924-2914_X_2000_03_13_pus_uva.fits ! Reading UV FITS file: J1924-2914_X_2000_03_13_pus_uva.fits ! AN table 1: 41 integrations on 190 of 190 possible baselines. ! AN table 2: 60 integrations on 190 of 190 possible baselines. ! AN table 3: 58 integrations on 190 of 190 possible baselines. ! AN table 4: 28 integrations on 190 of 190 possible baselines. ! AN table 5: 54 integrations on 190 of 190 possible baselines. ! Apparent sampling: 0.0589212 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1924-2914 ! ! 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 2382 lines of history. ! ! Reading 10792 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 J1924-2914_X_2000_03_13_pus] integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.03 float dynam dynam = 6.0 float soltime1 soltime1 = 120 float soltime2 soltime2 = 20 float thresh thresh = 0.5 float win_mult win_mult = 1.8 float time_av time_av = 16 float old_peak float new_peak float flux_cutoff mapsize field_size, field_cell ! Map grid = 512x512 pixels with 0.200x0.200 milli-arcsec cellsize. startmod ! Applying default point source starting model. ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 1 Jy ! ! Correcting IF 1. ! A total of 805 telescope corrections were flagged in sub-array 1. ! A total of 862 telescope corrections were flagged in sub-array 2. ! A total of 900 telescope corrections were flagged in sub-array 3. ! A total of 503 telescope corrections were flagged in sub-array 4. ! A total of 857 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 805 telescope corrections were flagged in sub-array 1. ! A total of 862 telescope corrections were flagged in sub-array 2. ! A total of 900 telescope corrections were flagged in sub-array 3. ! A total of 503 telescope corrections were flagged in sub-array 4. ! A total of 857 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 805 telescope corrections were flagged in sub-array 1. ! A total of 862 telescope corrections were flagged in sub-array 2. ! A total of 900 telescope corrections were flagged in sub-array 3. ! A total of 503 telescope corrections were flagged in sub-array 4. ! A total of 857 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 805 telescope corrections were flagged in sub-array 1. ! A total of 862 telescope corrections were flagged in sub-array 2. ! A total of 900 telescope corrections were flagged in sub-array 3. ! A total of 503 telescope corrections were flagged in sub-array 4. ! A total of 857 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=6.322554Jy sigma=0.057210 ! Fit after self-cal, rms=5.838829Jy sigma=0.052974 ! 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 0.544% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.6321 mas, bmaj=1.485 mas, bpa=4.029 degrees ! Estimated noise=1477.2 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 = 4.68443 Jy ! Component: 100 - total flux cleaned = 6.03193 Jy ! Total flux subtracted in 100 components = 6.03193 Jy ! Clean residual min=-0.205998 max=0.558012 Jy/beam ! Clean residual mean=0.000925 rms=0.067892 Jy/beam ! Combined flux in latest and established models = 6.03193 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 10 components and 6.03193 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.727093Jy sigma=0.015817 ! Fit after self-cal, rms=1.727456Jy sigma=0.015814 ! Inverting map ! Your choice of large map pixels excluded 0.544% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.639376 Jy ! Component: 100 - total flux cleaned = 1.01141 Jy ! Total flux subtracted in 100 components = 1.01141 Jy ! Clean residual min=-0.139996 max=0.277246 Jy/beam ! Clean residual mean=0.000465 rms=0.043284 Jy/beam ! Combined flux in latest and established models = 7.04334 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 26 components and 7.04334 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.333630Jy sigma=0.010794 ! Fit after self-cal, rms=1.333888Jy sigma=0.010791 ! Inverting map ! Your choice of large map pixels excluded 0.544% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! Added new window around map position (1.4, 2.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.277341 Jy ! Component: 100 - total flux cleaned = 0.461682 Jy ! Total flux subtracted in 100 components = 0.461682 Jy ! Clean residual min=-0.139457 max=0.196926 Jy/beam ! Clean residual mean=0.000236 rms=0.036389 Jy/beam ! Combined flux in latest and established models = 7.50502 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 41 components and 7.50502 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.223732Jy sigma=0.009086 ! Fit after self-cal, rms=1.219261Jy sigma=0.009056 ! Inverting map ! Your choice of large map pixels excluded 0.544% of the data. ! The x-axis pixel size should ideally be below 0.1938 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 0.544% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.8964 mas, bmaj=2.217 mas, bpa=1.537 degrees ! Estimated noise=884.853 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 = 0.413143 Jy ! Component: 100 - total flux cleaned = 0.638105 Jy ! Component: 150 - total flux cleaned = 0.763777 Jy ! Component: 200 - total flux cleaned = 0.834126 Jy ! Total flux subtracted in 200 components = 0.834126 Jy ! Clean residual min=-0.130900 max=0.325182 Jy/beam ! Clean residual mean=0.004847 rms=0.055737 Jy/beam ! Combined flux in latest and established models = 8.33915 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 53 components and 8.33915 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.158835Jy sigma=0.007231 ! Fit after self-cal, rms=1.145970Jy sigma=0.007126 ! Inverting map ! Your choice of large map pixels excluded 0.544% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! Added new window around map position (2.6, 7.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.340243 Jy ! Component: 100 - total flux cleaned = 0.514013 Jy ! Component: 150 - total flux cleaned = 0.583639 Jy ! Component: 200 - total flux cleaned = 0.59654 Jy ! Total flux subtracted in 200 components = 0.59654 Jy ! Clean residual min=-0.113365 max=0.161578 Jy/beam ! Clean residual mean=0.001380 rms=0.037579 Jy/beam ! Combined flux in latest and established models = 8.93569 Jy ! Performing phase self-cal ! Adding 38 model components to the UV plane model. ! The established model now contains 88 components and 8.93569 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.076910Jy sigma=0.005594 ! Fit after self-cal, rms=1.056344Jy sigma=0.005341 ! Inverting map ! Your choice of large map pixels excluded 0.544% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 15 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* GC 0.00* KP 0.00* ! LA 0.00* NL 0.00* OV 0.00* PT 0.00* ! SC 0.00* WF 0.00* HH 0.00* KK 0.00* ! MA 0.00* MC 0.00* MK 0.00* NY 0.00* ! ON 0.00* TS 0.00* WZ 0.00* HN 0.00* ! ! A total of 57 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.07 FD 0.93 GC 1.00* KP 1.09 ! LA 1.01 NL 1.01 OV 1.03 PT 0.98 ! SC 1.01 WF 1.11 HH 0.93 KK 1.00* ! MA 1.00 MC 1.10 MK 1.00* NY 1.00* ! ON 1.00* TS 1.00* WZ 1.09 HN 1.54 ! ! A total of 63 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.07 FD 0.97 GC 1.00* KP 0.98 ! LA 1.00 NL 1.00* OV 1.03 PT 0.96 ! SC 1.00* WF 1.00* HH 1.11 KK 0.95 ! MA 1.02 MC 1.16 MK 1.00 NY 1.00* ! ON 1.00* TS 1.00* WZ 1.03 HN 1.00* ! ! A total of 57 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* GC 0.00* KP 0.00* ! LA 0.00* NL 0.00* OV 0.00* PT 0.00* ! SC 0.00* WF 0.00* HH 0.00* KK 0.00* ! MA 0.00* MC 0.00* MK 0.00* NY 0.00* ! ON 0.00* TS 0.00* WZ 0.00* HN 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 FD 0.95 GC 1.00* KP 1.03 ! LA 1.03 NL 0.98 OV 0.99 PT 1.00* ! SC 0.99 WF 1.04 HH 1.00* KK 1.03 ! MA 1.00* MC 1.00* MK 0.98 NY 1.00* ! ON 1.00* TS 1.00* WZ 1.00* HN 1.00* ! ! ! Correcting IF 2. ! A total of 15 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* GC 0.00* KP 0.00* ! LA 0.00* NL 0.00* OV 0.00* PT 0.00* ! SC 0.00* WF 0.00* HH 0.00* KK 0.00* ! MA 0.00* MC 0.00* MK 0.00* NY 0.00* ! ON 0.00* TS 0.00* WZ 0.00* HN 0.00* ! ! A total of 57 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.07 FD 0.92 GC 1.00* KP 1.06 ! LA 0.97 NL 1.04 OV 1.01 PT 0.94 ! SC 0.99 WF 1.11 HH 0.89 KK 1.00* ! MA 1.01 MC 1.10 MK 1.00* NY 1.00* ! ON 1.00* TS 1.00* WZ 1.10 HN 1.46 ! ! A total of 63 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.07 FD 0.96 GC 1.00* KP 0.95 ! LA 0.95 NL 1.00* OV 1.03 PT 0.92 ! SC 1.00* WF 1.00* HH 1.09 KK 0.96 ! MA 1.03 MC 1.17 MK 1.04 NY 1.00* ! ON 1.00* TS 1.00* WZ 1.03 HN 1.00* ! ! A total of 57 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* GC 0.00* KP 0.00* ! LA 0.00* NL 0.00* OV 0.00* PT 0.00* ! SC 0.00* WF 0.00* HH 0.00* KK 0.00* ! MA 0.00* MC 0.00* MK 0.00* NY 0.00* ! ON 0.00* TS 0.00* WZ 0.00* HN 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 0.94 GC 1.00* KP 1.00 ! LA 0.99 NL 1.01 OV 0.97 PT 1.00* ! SC 0.97 WF 1.05 HH 1.00* KK 1.03 ! MA 1.00* MC 1.00* MK 1.02 NY 1.00* ! ON 1.00* TS 1.00* WZ 1.00* HN 1.00* ! ! ! Correcting IF 3. ! A total of 15 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* GC 0.00* KP 0.00* ! LA 0.00* NL 0.00* OV 0.00* PT 0.00* ! SC 0.00* WF 0.00* HH 0.00* KK 0.00* ! MA 0.00* MC 0.00* MK 0.00* NY 0.00* ! ON 0.00* TS 0.00* WZ 0.00* HN 0.00* ! ! A total of 57 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.10 FD 0.95 GC 1.00* KP 1.06 ! LA 0.96 NL 0.98 OV 1.02 PT 0.97 ! SC 1.01 WF 1.11 HH 0.87 KK 1.00* ! MA 1.04 MC 1.10 MK 1.00* NY 1.00* ! ON 1.00* TS 1.00* WZ 1.13 HN 1.44 ! ! A total of 63 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.11 FD 0.99 GC 1.00* KP 0.96 ! LA 0.95 NL 1.00* OV 1.05 PT 0.95 ! SC 1.00* WF 1.00* HH 0.98 KK 0.92 ! MA 1.04 MC 1.18 MK 0.99 NY 1.00* ! ON 1.00* TS 1.00* WZ 1.06 HN 1.00* ! ! A total of 57 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* GC 0.00* KP 0.00* ! LA 0.00* NL 0.00* OV 0.00* PT 0.00* ! SC 0.00* WF 0.00* HH 0.00* KK 0.00* ! MA 0.00* MC 0.00* MK 0.00* NY 0.00* ! ON 0.00* TS 0.00* WZ 0.00* HN 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.05 FD 0.97 GC 1.00* KP 1.01 ! LA 0.98 NL 0.96 OV 0.99 PT 1.00* ! SC 0.98 WF 1.06 HH 1.00* KK 1.01 ! MA 1.00* MC 1.00* MK 0.98 NY 1.00* ! ON 1.00* TS 1.00* WZ 1.00* HN 1.00* ! ! ! Correcting IF 4. ! A total of 15 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* GC 0.00* KP 0.00* ! LA 0.00* NL 0.00* OV 0.00* PT 0.00* ! SC 0.00* WF 0.00* HH 0.00* KK 0.00* ! MA 0.00* MC 0.00* MK 0.00* NY 0.00* ! ON 0.00* TS 0.00* WZ 0.00* HN 0.00* ! ! A total of 57 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.07 FD 0.93 GC 1.00* KP 1.05 ! LA 0.97 NL 0.98 OV 1.02 PT 0.98 ! SC 1.07 WF 1.12 HH 0.91 KK 1.00* ! MA 1.00 MC 1.12 MK 1.00* NY 1.00* ! ON 1.00* TS 1.00* WZ 1.14 HN 1.54 ! ! A total of 63 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.07 FD 0.98 GC 1.00* KP 0.95 ! LA 0.96 NL 1.00* OV 1.04 PT 0.95 ! SC 1.00* WF 1.00* HH 0.99 KK 0.93 ! MA 1.01 MC 1.18 MK 1.00 NY 1.00* ! ON 1.00* TS 1.00* WZ 1.07 HN 1.00* ! ! A total of 57 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* GC 0.00* KP 0.00* ! LA 0.00* NL 0.00* OV 0.00* PT 0.00* ! SC 0.00* WF 0.00* HH 0.00* KK 0.00* ! MA 0.00* MC 0.00* MK 0.00* NY 0.00* ! ON 0.00* TS 0.00* WZ 0.00* HN 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 0.95 GC 1.00* KP 0.99 ! LA 0.99 NL 0.97 OV 0.98 PT 1.00* ! SC 1.03 WF 1.06 HH 1.00* KK 1.03 ! MA 1.00* MC 1.00* MK 0.99 NY 1.00* ! ON 1.00* TS 1.00* WZ 1.00* HN 1.00* ! ! ! Fit before self-cal, rms=1.056344Jy sigma=0.005341 ! Fit after self-cal, rms=0.945400Jy sigma=0.003332 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.9215 mas, bmaj=2.278 mas, bpa=-0.9715 degrees ! Estimated noise=911.766 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 (4.6, 5.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.142479 Jy ! Component: 100 - total flux cleaned = 0.204719 Jy ! Component: 150 - total flux cleaned = 0.231531 Jy ! Component: 200 - total flux cleaned = 0.251161 Jy ! Total flux subtracted in 200 components = 0.251161 Jy ! Clean residual min=-0.057765 max=0.061306 Jy/beam ! Clean residual mean=-0.000282 rms=0.016131 Jy/beam ! Combined flux in latest and established models = 9.18685 Jy ! Performing phase self-cal ! Adding 45 model components to the UV plane model. ! The established model now contains 132 components and 9.18685 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.920245Jy sigma=0.002769 ! Fit after self-cal, rms=0.918164Jy sigma=0.002722 ! Inverting map ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 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=0.918164Jy sigma=0.002722 ! Fit after self-cal, rms=0.911050Jy sigma=0.002643 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.9217 mas, bmaj=2.278 mas, bpa=-0.9283 degrees ! Estimated noise=912.446 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0738013 Jy ! Component: 100 - total flux cleaned = 0.102903 Jy ! Component: 150 - total flux cleaned = 0.112138 Jy ! Component: 200 - total flux cleaned = 0.120057 Jy ! Total flux subtracted in 200 components = 0.120057 Jy ! Clean residual min=-0.043483 max=0.053938 Jy/beam ! Clean residual mean=0.000110 rms=0.012596 Jy/beam ! Combined flux in latest and established models = 9.3069 Jy selfcal ! Performing phase self-cal ! Adding 37 model components to the UV plane model. ! The established model now contains 151 components and 9.3069 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.903541Jy sigma=0.002442 ! Fit after self-cal, rms=0.901955Jy sigma=0.002422 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0.4, 5.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0448647 Jy ! Component: 100 - total flux cleaned = 0.0587769 Jy ! Component: 150 - total flux cleaned = 0.0681007 Jy ! Component: 200 - total flux cleaned = 0.073943 Jy ! Total flux subtracted in 200 components = 0.073943 Jy ! Clean residual min=-0.039084 max=0.040354 Jy/beam ! Clean residual mean=-0.000228 rms=0.010831 Jy/beam ! Combined flux in latest and established models = 9.38085 Jy ! Performing phase self-cal ! Adding 32 model components to the UV plane model. ! The established model now contains 171 components and 9.38085 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.896835Jy sigma=0.002298 ! Fit after self-cal, rms=0.895735Jy sigma=0.002287 ! Inverting map ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 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=0.895735Jy sigma=0.002287 ! Fit after self-cal, rms=0.887898Jy sigma=0.002239 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.9223 mas, bmaj=2.275 mas, bpa=-0.8794 degrees ! Estimated noise=912.809 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0432721 Jy ! Component: 100 - total flux cleaned = 0.0578212 Jy ! Component: 150 - total flux cleaned = 0.0657541 Jy ! Component: 200 - total flux cleaned = 0.0717935 Jy ! Total flux subtracted in 200 components = 0.0717935 Jy ! Clean residual min=-0.033788 max=0.032962 Jy/beam ! Clean residual mean=0.000078 rms=0.009010 Jy/beam ! Combined flux in latest and established models = 9.45264 Jy selfcal ! Performing phase self-cal ! Adding 32 model components to the UV plane model. ! The established model now contains 184 components and 9.45264 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.884562Jy sigma=0.002146 ! Fit after self-cal, rms=0.883715Jy sigma=0.002137 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 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 = 0.0128782 Jy ! Component: 100 - total flux cleaned = 0.0175377 Jy ! Component: 150 - total flux cleaned = 0.0209471 Jy ! Component: 200 - total flux cleaned = 0.0232717 Jy ! Total flux subtracted in 200 components = 0.0232717 Jy ! Clean residual min=-0.031017 max=0.028658 Jy/beam ! Clean residual mean=-0.000035 rms=0.008233 Jy/beam ! Combined flux in latest and established models = 9.47591 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 191 components and 9.47591 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.882135Jy sigma=0.002092 ! Fit after self-cal, rms=0.881636Jy sigma=0.002088 ! Inverting map ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 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=0.881636Jy sigma=0.002088 ! Fit after self-cal, rms=0.877446Jy sigma=0.002072 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=2.432 mas, bmaj=5.955 mas, bpa=2.729 degrees ! Estimated noise=1046.32 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0163504 Jy ! Component: 100 - total flux cleaned = 0.0224767 Jy ! Component: 150 - total flux cleaned = 0.0244239 Jy ! Component: 200 - total flux cleaned = 0.0260247 Jy ! Total flux subtracted in 200 components = 0.0260247 Jy ! Clean residual min=-0.028268 max=0.031887 Jy/beam ! Clean residual mean=0.000206 rms=0.009656 Jy/beam ! Combined flux in latest and established models = 9.50194 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 204 components and 9.50194 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.877814Jy sigma=0.002042 ! Fit after self-cal, rms=0.876861Jy sigma=0.002031 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 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 = 0.0103944 Jy ! Component: 100 - total flux cleaned = 0.0112314 Jy ! Component: 150 - total flux cleaned = 0.0111908 Jy ! Component: 200 - total flux cleaned = 0.011211 Jy ! Total flux subtracted in 200 components = 0.011211 Jy ! Clean residual min=-0.024452 max=0.026450 Jy/beam ! Clean residual mean=0.000134 rms=0.008732 Jy/beam ! Combined flux in latest and established models = 9.51315 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 216 components and 9.51315 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.876754Jy sigma=0.002017 ! Fit after self-cal, rms=0.876283Jy sigma=0.002012 ! Inverting map ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 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 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.9229 mas, bmaj=2.273 mas, bpa=-0.8353 degrees ! Estimated noise=912.919 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9229 x 2.273 at -0.8353 degrees (North through East) ! Clean map min=-0.026659 max=6.46 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=0.876283Jy sigma=0.002012 ! Fit after self-cal, rms=0.838688Jy sigma=0.001500 ! Inverting map and beam ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.9237 mas, bmaj=2.273 mas, bpa=-0.9191 degrees ! Estimated noise=912.122 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0144843 Jy ! Component: 100 - total flux cleaned = 0.0197469 Jy ! Component: 150 - total flux cleaned = 0.0217554 Jy ! Component: 200 - total flux cleaned = 0.0235726 Jy ! Total flux subtracted in 200 components = 0.0235726 Jy ! Clean residual min=-0.026770 max=0.023306 Jy/beam ! Clean residual mean=0.000195 rms=0.006035 Jy/beam ! Combined flux in latest and established models = 9.53672 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 235 components and 9.53672 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.837677Jy sigma=0.001460 ! Fit after self-cal, rms=0.837347Jy sigma=0.001458 ! Inverting map ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00693397 Jy ! Component: 100 - total flux cleaned = 0.00750989 Jy ! Component: 150 - total flux cleaned = 0.00751877 Jy ! Component: 200 - total flux cleaned = 0.0075343 Jy ! Total flux subtracted in 200 components = 0.0075343 Jy ! Clean residual min=-0.027180 max=0.021530 Jy/beam ! Clean residual mean=0.000163 rms=0.005797 Jy/beam ! Combined flux in latest and established models = 9.54425 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 239 components and 9.54425 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.836628Jy sigma=0.001436 ! Fit after self-cal, rms=0.836428Jy sigma=0.001435 ! Inverting map ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.836428Jy sigma=0.001435 ! Fit after self-cal, rms=0.834901Jy sigma=0.001428 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 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.6831 mas, bmaj=1.608 mas, bpa=-2.068 degrees ! Estimated noise=1487.52 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 4.89177 Jy ! Component: 100 - total flux cleaned = 6.20146 Jy ! Component: 150 - total flux cleaned = 6.82098 Jy ! Component: 200 - total flux cleaned = 7.24722 Jy ! Total flux subtracted in 200 components = 7.24722 Jy ! Clean residual min=-0.105045 max=0.261066 Jy/beam ! Clean residual mean=0.000953 rms=0.042907 Jy/beam ! Combined flux in latest and established models = 7.24722 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 37 model components to the UV plane model. ! The established model now contains 37 components and 7.24722 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.9243 mas, bmaj=2.273 mas, bpa=-0.8932 degrees ! Estimated noise=912.057 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 = 0.665216 Jy ! Component: 100 - total flux cleaned = 1.08983 Jy ! Component: 150 - total flux cleaned = 1.38395 Jy ! Component: 200 - total flux cleaned = 1.59469 Jy ! Total flux subtracted in 200 components = 1.59469 Jy ! Clean residual min=-0.065039 max=0.124176 Jy/beam ! Clean residual mean=0.003738 rms=0.027772 Jy/beam ! Combined flux in latest and established models = 8.84191 Jy ! Adding 100 model components to the UV plane model. ! The established model now contains 123 components and 8.84191 Jy ! Inverting map ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! Added new window around map position (-0.8, 0.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.15592 Jy ! Component: 100 - total flux cleaned = 0.27199 Jy ! Component: 150 - total flux cleaned = 0.359585 Jy ! Component: 200 - total flux cleaned = 0.426491 Jy ! Total flux subtracted in 200 components = 0.426491 Jy ! Clean residual min=-0.029324 max=0.042743 Jy/beam ! Clean residual mean=0.001630 rms=0.011001 Jy/beam ! Combined flux in latest and established models = 9.2684 Jy ! Adding 78 model components to the UV plane model. ! The established model now contains 191 components and 9.2684 Jy ! Inverting map ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 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 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=2.431 mas, bmaj=5.953 mas, bpa=2.708 degrees ! Estimated noise=1044.54 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0817243 Jy ! Component: 100 - total flux cleaned = 0.13455 Jy ! Component: 150 - total flux cleaned = 0.171122 Jy ! Component: 200 - total flux cleaned = 0.197543 Jy ! Total flux subtracted in 200 components = 0.197543 Jy ! Clean residual min=-0.019032 max=0.026026 Jy/beam ! Clean residual mean=0.001182 rms=0.008048 Jy/beam ! Combined flux in latest and established models = 9.46594 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 = 0.019617 Jy ! Component: 100 - total flux cleaned = 0.0342906 Jy ! Component: 150 - total flux cleaned = 0.0453495 Jy ! Component: 200 - total flux cleaned = 0.0537621 Jy ! Total flux subtracted in 200 components = 0.0537621 Jy ! Clean residual min=-0.017865 max=0.020508 Jy/beam ! Clean residual mean=0.000664 rms=0.006630 Jy/beam ! Combined flux in latest and established models = 9.5197 Jy ! Adding 125 model components to the UV plane model. ! The established model now contains 307 components and 9.51971 Jy ! Inverting map ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.9243 mas, bmaj=2.273 mas, bpa=-0.8932 degrees ! Estimated noise=912.057 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0019867 Jy ! Component: 100 - total flux cleaned = 0.00307918 Jy ! Component: 150 - total flux cleaned = 0.00355557 Jy ! Component: 200 - total flux cleaned = 0.00314104 Jy ! Total flux subtracted in 200 components = 0.00314104 Jy ! Clean residual min=-0.018437 max=0.018543 Jy/beam ! Clean residual mean=0.000342 rms=0.004868 Jy/beam ! Combined flux in latest and established models = 9.52285 Jy selfcal ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 325 components and 9.52285 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.831198Jy sigma=0.001361 ! Fit after self-cal, rms=0.830058Jy sigma=0.001328 wmodel J1924-2914_X_2000_03_13_pus_map.mod ! Writing 325 model components to file: J1924-2914_X_2000_03_13_pus_map.mod wobs J1924-2914_X_2000_03_13_pus_uvs.fits ! Writing UV FITS file: J1924-2914_X_2000_03_13_pus_uvs.fits wwins J1924-2914_X_2000_03_13_pus_map.win ! wwins: Wrote 6 windows to J1924-2914_X_2000_03_13_pus_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00488894 Jy ! Component: 100 - total flux cleaned = -0.00518832 Jy ! Component: 150 - total flux cleaned = -0.00519198 Jy ! Component: 200 - total flux cleaned = -0.00544628 Jy ! Component: 250 - total flux cleaned = -0.00593775 Jy ! Component: 300 - total flux cleaned = -0.00640497 Jy ! Component: 350 - total flux cleaned = -0.00549335 Jy ! Component: 400 - total flux cleaned = -0.00527279 Jy ! Component: 450 - total flux cleaned = -0.00419652 Jy ! Component: 500 - total flux cleaned = -0.00335755 Jy ! Component: 550 - total flux cleaned = -0.00232618 Jy ! Component: 600 - total flux cleaned = -0.00171493 Jy ! Component: 650 - total flux cleaned = -0.000719887 Jy ! Component: 700 - total flux cleaned = -0.000326034 Jy ! Component: 750 - total flux cleaned = 0.000823348 Jy ! Component: 800 - total flux cleaned = 0.00157456 Jy ! Component: 850 - total flux cleaned = 0.00249858 Jy ! Component: 900 - total flux cleaned = 0.00340502 Jy ! Component: 950 - total flux cleaned = 0.00412046 Jy ! Component: 1000 - total flux cleaned = 0.0046463 Jy ! Component: 1050 - total flux cleaned = 0.00516563 Jy ! Component: 1100 - total flux cleaned = 0.00550722 Jy ! Component: 1150 - total flux cleaned = 0.00567591 Jy ! Component: 1200 - total flux cleaned = 0.00584188 Jy ! Component: 1250 - total flux cleaned = 0.00600655 Jy ! Component: 1300 - total flux cleaned = 0.00600606 Jy ! Component: 1350 - total flux cleaned = 0.00616521 Jy ! Component: 1400 - total flux cleaned = 0.0066365 Jy ! Component: 1450 - total flux cleaned = 0.0066355 Jy ! Component: 1500 - total flux cleaned = 0.00678872 Jy ! Component: 1550 - total flux cleaned = 0.00663599 Jy ! Component: 1600 - total flux cleaned = 0.00663633 Jy ! Component: 1650 - total flux cleaned = 0.00708217 Jy ! Component: 1700 - total flux cleaned = 0.0072272 Jy ! Component: 1750 - total flux cleaned = 0.0073721 Jy ! Component: 1800 - total flux cleaned = 0.00722933 Jy ! Component: 1850 - total flux cleaned = 0.00780008 Jy ! Component: 1900 - total flux cleaned = 0.00808241 Jy ! Component: 1950 - total flux cleaned = 0.00808212 Jy ! Component: 2000 - total flux cleaned = 0.00822195 Jy ! Total flux subtracted in 2048 components = 0.00836024 Jy ! Clean residual min=-0.009268 max=0.007904 Jy/beam ! Clean residual mean=0.000278 rms=0.002726 Jy/beam ! Combined flux in latest and established models = 9.53121 Jy keep ! Adding 141 model components to the UV plane model. ! The established model now contains 465 components and 9.53121 Jy ![Exited script file: muppet] wmap "J1924-2914_X_2000_03_13_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9243 x 2.273 at -0.8932 degrees (North through East) ! Clean map min=-0.012452 max=6.4627 Jy/beam ! Writing clean map to FITS file: J1924-2914_X_2000_03_13_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 6.46272 invert ! Inverting map ! Your choice of large map pixels excluded 0.588% of the data. ! The x-axis pixel size should ideally be below 0.1938 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00272166 device "J1924-2914_X_2000_03_13_pus\_map.eps/VPS" ! Attempting to open device: 'J1924-2914_X_2000_03_13_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.12634 0.12634 0.252679 0.505358 1.01072 2.02143 4.04286 8.08573 16.1715 32.3429 64.6858 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0081 print "peak=",int(1000*peak_flux)/1000 ! peak= 6.462 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9243 x 2.273 at -0.8932 degrees (North through East) ! Clean map min=-0.012452 max=6.4627 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. quit ! Quitting program ! Log file J1924-2914_X_2000_03_13_pus_uvs.log closed on Mon Apr 1 13:07:42 2013