! Started logfile: J1513-1012_X_2003_05_07_pus_uvs.log on Thu Dec 14 15:58:05 2006 obs J1513-1012_X_2003_05_07_pus_uva.fits ! Reading UV FITS file: J1513-1012_X_2003_05_07_pus_uva.fits ! AN table 1: 57 integrations on 171 of 171 possible baselines. ! AN table 2: 19 integrations on 171 of 171 possible baselines. ! AN table 3: 130 integrations on 171 of 171 possible baselines. ! AN table 4: 62 integrations on 171 of 171 possible baselines. ! AN table 5: 89 integrations on 171 of 171 possible baselines. ! AN table 6: 38 integrations on 171 of 171 possible baselines. ! AN table 7: 106 integrations on 171 of 171 possible baselines. ! AN table 8: 271 integrations on 171 of 171 possible baselines. ! Apparent sampling: 0.0440112 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1513-1012 ! ! 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 1739 lines of history. ! ! Reading 23240 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 float field_size field_size = 256 float field_cell field_cell = 0.2 float taper_size taper_size = 70. 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 = 256x256 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 1015 telescope corrections were flagged in sub-array 1. ! A total of 361 telescope corrections were flagged in sub-array 2. ! A total of 2134 telescope corrections were flagged in sub-array 3. ! A total of 881 telescope corrections were flagged in sub-array 4. ! A total of 1449 telescope corrections were flagged in sub-array 5. ! A total of 656 telescope corrections were flagged in sub-array 6. ! A total of 1393 telescope corrections were flagged in sub-array 7. ! A total of 4693 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 2. ! A total of 1015 telescope corrections were flagged in sub-array 1. ! A total of 361 telescope corrections were flagged in sub-array 2. ! A total of 2134 telescope corrections were flagged in sub-array 3. ! A total of 881 telescope corrections were flagged in sub-array 4. ! A total of 1449 telescope corrections were flagged in sub-array 5. ! A total of 656 telescope corrections were flagged in sub-array 6. ! A total of 1393 telescope corrections were flagged in sub-array 7. ! A total of 4693 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 3. ! A total of 1015 telescope corrections were flagged in sub-array 1. ! A total of 361 telescope corrections were flagged in sub-array 2. ! A total of 2136 telescope corrections were flagged in sub-array 3. ! A total of 881 telescope corrections were flagged in sub-array 4. ! A total of 1449 telescope corrections were flagged in sub-array 5. ! A total of 656 telescope corrections were flagged in sub-array 6. ! A total of 1393 telescope corrections were flagged in sub-array 7. ! A total of 4693 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 4. ! A total of 1015 telescope corrections were flagged in sub-array 1. ! A total of 361 telescope corrections were flagged in sub-array 2. ! A total of 2142 telescope corrections were flagged in sub-array 3. ! A total of 881 telescope corrections were flagged in sub-array 4. ! A total of 1449 telescope corrections were flagged in sub-array 5. ! A total of 656 telescope corrections were flagged in sub-array 6. ! A total of 1393 telescope corrections were flagged in sub-array 7. ! A total of 4693 telescope corrections were flagged in sub-array 8. ! ! Fit before self-cal, rms=0.906756Jy sigma=0.006620 ! Fit after self-cal, rms=0.643811Jy sigma=0.004669 ! 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 3.95% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=0.503 mas, bmaj=1.864 mas, bpa=-8.01 degrees ! Estimated noise=1158.21 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 = 0.267945 Jy ! Component: 100 - total flux cleaned = 0.376539 Jy ! Total flux subtracted in 100 components = 0.376539 Jy ! Clean residual min=-0.023931 max=0.079919 Jy/beam ! Clean residual mean=0.001586 rms=0.008750 Jy/beam ! Combined flux in latest and established models = 0.376539 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.376539 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.320904Jy sigma=0.001952 ! Fit after self-cal, rms=0.319844Jy sigma=0.001949 ! Inverting map ! Your choice of large map pixels excluded 3.95% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec ! Added new window around map position (0.8, 0.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0795554 Jy ! Component: 100 - total flux cleaned = 0.126577 Jy ! Total flux subtracted in 100 components = 0.126577 Jy ! Clean residual min=-0.019295 max=0.062075 Jy/beam ! Clean residual mean=0.000857 rms=0.005652 Jy/beam ! Combined flux in latest and established models = 0.503116 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 14 components and 0.503116 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.283345Jy sigma=0.001518 ! Fit after self-cal, rms=0.281166Jy sigma=0.001496 ! Inverting map ! Your choice of large map pixels excluded 3.95% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0407223 Jy ! Component: 100 - total flux cleaned = 0.0611887 Jy ! Total flux subtracted in 100 components = 0.0611887 Jy ! Clean residual min=-0.015562 max=0.036935 Jy/beam ! Clean residual mean=0.000505 rms=0.004013 Jy/beam ! Combined flux in latest and established models = 0.564305 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 18 components and 0.564305 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.271481Jy sigma=0.001372 ! Fit after self-cal, rms=0.270564Jy sigma=0.001363 ! Inverting map ! Your choice of large map pixels excluded 3.95% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0215998 Jy ! Component: 100 - total flux cleaned = 0.0271967 Jy ! Total flux subtracted in 100 components = 0.0271967 Jy ! Clean residual min=-0.013375 max=0.023588 Jy/beam ! Clean residual mean=0.000348 rms=0.003288 Jy/beam ! Combined flux in latest and established models = 0.591501 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 26 components and 0.591501 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.268112Jy sigma=0.001332 ! Fit after self-cal, rms=0.267729Jy sigma=0.001329 ! Inverting map ! Your choice of large map pixels excluded 3.95% of the data. ! The x-axis pixel size should ideally be below 0.1835 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 3.95% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=0.6452 mas, bmaj=2.635 mas, bpa=-8.828 degrees ! Estimated noise=656.174 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 = 0.0186886 Jy ! Component: 100 - total flux cleaned = 0.0268758 Jy ! Component: 150 - total flux cleaned = 0.0299583 Jy ! Component: 200 - total flux cleaned = 0.030213 Jy ! Total flux subtracted in 200 components = 0.030213 Jy ! Clean residual min=-0.007137 max=0.011894 Jy/beam ! Clean residual mean=0.000895 rms=0.002462 Jy/beam ! Combined flux in latest and established models = 0.621714 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 30 components and 0.621714 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.266452Jy sigma=0.001314 ! Fit after self-cal, rms=0.266266Jy sigma=0.001312 ! Inverting map ! Your choice of large map pixels excluded 3.95% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 48 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.87 GG 1.00* HN 0.88 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MC 1.00* MK 1.00* NL 1.28 ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* TC 1.00* ! TS 1.00* WF 1.02 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* GG 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* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 129 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 FD 0.96 GG 1.00* HN 1.11 ! KK 0.86 KP 1.07 LA 0.93 MA 1.08 ! MC 1.01 MK 1.04 NL 1.02 ON 1.04 ! OV 1.00 PT 0.95 SC 1.00* TC 1.00* ! TS 1.00* WF 1.00* WZ 1.14 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.94 FD 1.01 GG 1.00* HN 1.00* ! KK 1.00* KP 1.07 LA 0.95 MA 1.00* ! MC 1.00* MK 1.00* NL 1.27 ON 1.00* ! OV 0.95 PT 0.97 SC 1.00* TC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 105 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 1.00* GG 1.00* HN 1.00* ! KK 1.03 KP 1.38 LA 1.00* MA 1.00* ! MC 1.00* MK 0.88 NL 1.00* ON 1.00* ! OV 1.02 PT 1.00* SC 1.00* TC 1.00* ! TS 1.18 WF 1.00* WZ 1.00* ! ! A total of 66 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.00* FD 0.00* GG 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* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 9 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 0.96 GG 1.00* HN 0.96 ! KK 1.00* KP 1.14 LA 0.99 MA 1.05 ! MC 1.10 MK 1.00* NL 1.06 ON 1.07 ! OV 1.00* PT 1.01 SC 0.95 TC 1.00* ! TS 1.00* WF 1.00 WZ 1.03 ! ! A total of 201 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! BR 1.00* FD 1.00* GG 1.00* HN 1.37 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00 ! MC 1.03 MK 1.00* NL 1.00* ON 1.09 ! OV 1.00* PT 1.00* SC 0.87 TC 1.00* ! TS 1.00* WF 1.00* WZ 0.88 ! ! ! Correcting IF 2. ! A total of 48 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.07 GG 1.00* HN 1.02 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MC 1.00* MK 1.00* NL 1.07 ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* TC 1.00* ! TS 1.00* WF 1.02 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* GG 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* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 129 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.96 FD 0.96 GG 1.00* HN 1.26 ! KK 0.90 KP 1.01 LA 0.95 MA 0.93 ! MC 1.02 MK 1.06 NL 0.99 ON 1.10 ! OV 0.99 PT 0.97 SC 1.00* TC 1.00* ! TS 1.00* WF 1.00* WZ 0.96 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.95 FD 1.02 GG 1.00* HN 1.00* ! KK 1.00* KP 0.98 LA 0.95 MA 1.00* ! MC 1.00* MK 1.00* NL 1.19 ON 1.00* ! OV 0.95 PT 1.00 SC 1.00* TC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 105 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 1.00* GG 1.00* HN 1.00* ! KK 0.97 KP 1.24 LA 1.00* MA 1.00* ! MC 1.00* MK 0.93 NL 1.00* ON 1.00* ! OV 1.04 PT 1.00* SC 1.00* TC 1.00* ! TS 1.20 WF 1.00* WZ 1.00* ! ! A total of 66 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.00* FD 0.00* GG 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* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 9 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 0.95 GG 1.00* HN 0.95 ! KK 1.00* KP 1.05 LA 1.01 MA 1.01 ! MC 1.07 MK 1.00* NL 1.01 ON 1.05 ! OV 1.00* PT 1.05 SC 0.93 TC 1.00* ! TS 1.00* WF 0.95 WZ 1.05 ! ! A total of 201 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! BR 1.00* FD 1.00* GG 1.00* HN 1.20 ! KK 1.00* KP 1.00* LA 1.00* MA 1.02 ! MC 0.99 MK 1.00* NL 1.00* ON 1.05 ! OV 1.00* PT 1.00* SC 0.88 TC 1.00* ! TS 1.00* WF 1.00* WZ 0.91 ! ! ! Correcting IF 3. ! A total of 48 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.97 GG 1.00* HN 0.98 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MC 1.00* MK 1.00* NL 1.06 ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* TC 1.00* ! TS 1.00* WF 1.07 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* GG 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* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 126 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 FD 0.95 GG 1.00* HN 1.22 ! KK 1.17 KP 0.93 LA 0.95 MA 0.88 ! MC 1.05 MK 1.15 NL 0.95 ON 0.87 ! OV 1.01 PT 1.00 SC 1.00* TC 1.00* ! TS 1.00* WF 1.00* WZ 1.06 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 1.02 GG 1.00* HN 1.00* ! KK 1.00* KP 0.92 LA 0.95 MA 1.00* ! MC 1.00* MK 1.00* NL 1.16 ON 1.00* ! OV 0.99 PT 1.02 SC 1.00* TC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 105 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 FD 1.00* GG 1.00* HN 1.00* ! KK 1.08 KP 1.20 LA 1.00* MA 1.00* ! MC 1.00* MK 0.92 NL 1.00* ON 1.00* ! OV 1.07 PT 1.00* SC 1.00* TC 1.00* ! TS 1.10 WF 1.00* WZ 1.00* ! ! A total of 66 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.00* FD 0.00* GG 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* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 9 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 0.94 GG 1.00* HN 0.94 ! KK 1.00* KP 0.96 LA 1.00 MA 0.99 ! MC 1.15 MK 1.00* NL 1.00 ON 0.99 ! OV 1.00* PT 1.10 SC 0.93 TC 1.00* ! TS 1.00* WF 0.92 WZ 1.01 ! ! A total of 201 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! BR 1.00* FD 1.00* GG 1.00* HN 1.19 ! KK 1.00* KP 1.00* LA 1.00* MA 0.99 ! MC 1.08 MK 1.00* NL 1.00* ON 1.09 ! OV 1.00* PT 1.00* SC 0.98 TC 1.00* ! TS 1.00* WF 1.00* WZ 0.90 ! ! ! Correcting IF 4. ! A total of 48 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.90 GG 1.00* HN 1.04 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MC 1.00* MK 1.00* NL 1.09 ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* TC 1.00* ! TS 1.00* WF 0.97 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* GG 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* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 120 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 0.92 GG 1.00* HN 1.32 ! KK 1.19 KP 1.01 LA 0.92 MA 0.93 ! MC 1.16 MK 1.17 NL 0.96 ON 0.87 ! OV 1.02 PT 1.01 SC 1.00* TC 1.00* ! TS 1.00* WF 1.00* WZ 1.09 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 FD 0.98 GG 1.00* HN 1.00* ! KK 1.00* KP 0.97 LA 0.92 MA 1.00* ! MC 1.00* MK 1.00* NL 1.19 ON 1.00* ! OV 0.98 PT 1.03 SC 1.00* TC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 105 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 1.00* GG 1.00* HN 1.00* ! KK 1.02 KP 1.24 LA 1.00* MA 1.00* ! MC 1.00* MK 0.92 NL 1.00* ON 1.00* ! OV 1.05 PT 1.00* SC 1.00* TC 1.00* ! TS 1.03 WF 1.00* WZ 1.00* ! ! A total of 66 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.00* FD 0.00* GG 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* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 9 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 0.94 GG 1.00* HN 0.96 ! KK 1.00* KP 1.05 LA 0.98 MA 1.03 ! MC 1.58 MK 1.00* NL 1.01 ON 0.99 ! OV 1.00* PT 1.08 SC 0.99 TC 1.00* ! TS 1.00* WF 0.89 WZ 1.04 ! ! A total of 201 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! BR 1.00* FD 1.00* GG 1.00* HN 1.24 ! KK 1.00* KP 1.00* LA 1.00* MA 1.02 ! MC 0.87 MK 1.00* NL 1.00* ON 1.02 ! OV 1.00* PT 1.00* SC 0.90 TC 1.00* ! TS 1.00* WF 1.00* WZ 0.94 ! ! ! Fit before self-cal, rms=0.266266Jy sigma=0.001312 ! Fit after self-cal, rms=0.262752Jy sigma=0.001279 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=0.653 mas, bmaj=2.903 mas, bpa=-9.821 degrees ! Estimated noise=682.745 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 = -0.00102903 Jy ! Component: 100 - total flux cleaned = -0.00165802 Jy ! Component: 150 - total flux cleaned = -0.00227197 Jy ! Component: 200 - total flux cleaned = -0.00239431 Jy ! Total flux subtracted in 200 components = -0.00239431 Jy ! Clean residual min=-0.005148 max=0.009089 Jy/beam ! Clean residual mean=0.000404 rms=0.001725 Jy/beam ! Combined flux in latest and established models = 0.61932 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 36 components and 0.61932 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.262390Jy sigma=0.001276 ! Fit after self-cal, rms=0.262631Jy sigma=0.001275 ! Inverting map ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 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=0.262631Jy sigma=0.001275 ! Fit after self-cal, rms=0.263275Jy sigma=0.001274 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=0.6562 mas, bmaj=2.902 mas, bpa=-9.929 degrees ! Estimated noise=683.288 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00023752 Jy ! Component: 100 - total flux cleaned = -0.000705352 Jy ! Component: 150 - total flux cleaned = -0.00093821 Jy ! Component: 200 - total flux cleaned = -0.000838285 Jy ! Total flux subtracted in 200 components = -0.000838285 Jy ! Clean residual min=-0.004859 max=0.007986 Jy/beam ! Clean residual mean=0.000346 rms=0.001660 Jy/beam ! Combined flux in latest and established models = 0.618482 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 39 components and 0.618482 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.263058Jy sigma=0.001272 ! Fit after self-cal, rms=0.263042Jy sigma=0.001271 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 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 = 0.000739369 Jy ! Component: 100 - total flux cleaned = 0.000867347 Jy ! Component: 150 - total flux cleaned = 0.000689714 Jy ! Component: 200 - total flux cleaned = 0.000541538 Jy ! Total flux subtracted in 200 components = 0.000541538 Jy ! Clean residual min=-0.004844 max=0.006580 Jy/beam ! Clean residual mean=0.000323 rms=0.001600 Jy/beam ! Combined flux in latest and established models = 0.619023 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 42 components and 0.619023 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.262916Jy sigma=0.001271 ! Fit after self-cal, rms=0.262868Jy sigma=0.001270 ! Inverting map ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 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=0.262868Jy sigma=0.001270 ! Fit after self-cal, rms=0.263754Jy sigma=0.001265 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=0.6593 mas, bmaj=2.901 mas, bpa=-10.05 degrees ! Estimated noise=684.567 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000613336 Jy ! Component: 100 - total flux cleaned = 0.000739955 Jy ! Component: 150 - total flux cleaned = 0.00065295 Jy ! Component: 200 - total flux cleaned = 0.000727689 Jy ! Total flux subtracted in 200 components = 0.000727689 Jy ! Clean residual min=-0.004338 max=0.006532 Jy/beam ! Clean residual mean=0.000326 rms=0.001439 Jy/beam ! Combined flux in latest and established models = 0.619751 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 43 components and 0.619751 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.263634Jy sigma=0.001264 ! Fit after self-cal, rms=0.263624Jy sigma=0.001263 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 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 (3, -0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0053833 Jy ! Component: 100 - total flux cleaned = 0.00627816 Jy ! Component: 150 - total flux cleaned = 0.00641681 Jy ! Component: 200 - total flux cleaned = 0.00641393 Jy ! Total flux subtracted in 200 components = 0.00641393 Jy ! Clean residual min=-0.004337 max=0.004095 Jy/beam ! Clean residual mean=0.000045 rms=0.001211 Jy/beam ! Combined flux in latest and established models = 0.626165 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 58 components and 0.626165 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.263367Jy sigma=0.001261 ! Fit after self-cal, rms=0.263384Jy sigma=0.001261 ! Inverting map ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 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=0.263384Jy sigma=0.001261 ! Fit after self-cal, rms=0.264680Jy sigma=0.001260 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=2.625 mas, bmaj=3.84 mas, bpa=-9.455 degrees ! Estimated noise=827.243 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00526061 Jy ! Component: 100 - total flux cleaned = 0.00527566 Jy ! Component: 150 - total flux cleaned = 0.00498508 Jy ! Component: 200 - total flux cleaned = 0.00480308 Jy ! Total flux subtracted in 200 components = 0.00480308 Jy ! Clean residual min=-0.003136 max=0.003898 Jy/beam ! Clean residual mean=0.000070 rms=0.001239 Jy/beam ! Combined flux in latest and established models = 0.630968 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 70 components and 0.630968 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.264598Jy sigma=0.001260 ! Fit after self-cal, rms=0.264651Jy sigma=0.001259 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 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 = 0.000495193 Jy ! Component: 100 - total flux cleaned = 0.000512493 Jy ! Component: 150 - total flux cleaned = 0.000332259 Jy ! Component: 200 - total flux cleaned = 0.000121206 Jy ! Total flux subtracted in 200 components = 0.000121206 Jy ! Clean residual min=-0.002945 max=0.003768 Jy/beam ! Clean residual mean=0.000058 rms=0.001247 Jy/beam ! Combined flux in latest and established models = 0.631089 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 76 components and 0.631089 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.264623Jy sigma=0.001259 ! Fit after self-cal, rms=0.264641Jy sigma=0.001259 ! Inverting map ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "************** FINISHED AMPLITUDE SELF-CAL **************" ! ************** FINISHED AMPLITUDE SELF-CAL ************** restore ! Inverting map and beam ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=0.6607 mas, bmaj=2.899 mas, bpa=-10.11 degrees ! Estimated noise=685.537 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6607 x 2.899 at -10.11 degrees (North through East) ! Clean map min=-0.0032822 max=0.36186 Jy/beam if(peak(flux) > thresh) selfcal true, true clean clean_niter,clean_gain selfcal flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) selfcal true, true end if print "************** CLEARING MODEL AND STARTING OVER **********" ! ************** CLEARING MODEL AND STARTING OVER ********** clrmod true ! clrmod: Cleared the established and tentative models. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=0.5165 mas, bmaj=2.334 mas, bpa=-10.64 degrees ! Estimated noise=1216.1 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.30138 Jy ! Component: 100 - total flux cleaned = 0.432768 Jy ! Component: 150 - total flux cleaned = 0.502012 Jy ! Component: 200 - total flux cleaned = 0.543591 Jy ! Total flux subtracted in 200 components = 0.543591 Jy ! Clean residual min=-0.008188 max=0.021321 Jy/beam ! Clean residual mean=0.000721 rms=0.003308 Jy/beam ! Combined flux in latest and established models = 0.543591 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 0.543591 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=0.6607 mas, bmaj=2.899 mas, bpa=-10.11 degrees ! Estimated noise=685.537 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 = 0.0407378 Jy ! Component: 100 - total flux cleaned = 0.0607354 Jy ! Component: 150 - total flux cleaned = 0.0720364 Jy ! Component: 200 - total flux cleaned = 0.0788743 Jy ! Total flux subtracted in 200 components = 0.0788743 Jy ! Clean residual min=-0.003529 max=0.007752 Jy/beam ! Clean residual mean=0.000415 rms=0.001287 Jy/beam ! Combined flux in latest and established models = 0.622466 Jy ! Adding 25 model components to the UV plane model. ! The established model now contains 31 components and 0.622466 Jy ! Inverting map ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 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 = 0.00582767 Jy ! Component: 100 - total flux cleaned = 0.00641028 Jy ! Component: 150 - total flux cleaned = 0.00653396 Jy ! Component: 200 - total flux cleaned = 0.00674594 Jy ! Total flux subtracted in 200 components = 0.00674594 Jy ! Clean residual min=-0.003242 max=0.004125 Jy/beam ! Clean residual mean=0.000105 rms=0.001020 Jy/beam ! Combined flux in latest and established models = 0.629212 Jy ! Adding 21 model components to the UV plane model. ! The established model now contains 47 components and 0.629212 Jy ! Inverting map ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=2.625 mas, bmaj=3.84 mas, bpa=-9.455 degrees ! Estimated noise=827.243 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00108643 Jy ! Component: 100 - total flux cleaned = 0.000892907 Jy ! Component: 150 - total flux cleaned = 0.000730186 Jy ! Component: 200 - total flux cleaned = 0.000538962 Jy ! Total flux subtracted in 200 components = 0.000538962 Jy ! Clean residual min=-0.002865 max=0.003715 Jy/beam ! Clean residual mean=0.000170 rms=0.001155 Jy/beam ! Combined flux in latest and established models = 0.629751 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 = -0.000127575 Jy ! Component: 100 - total flux cleaned = -0.000207523 Jy ! Component: 150 - total flux cleaned = -0.000282205 Jy ! Component: 200 - total flux cleaned = -0.000351558 Jy ! Total flux subtracted in 200 components = -0.000351558 Jy ! Clean residual min=-0.002753 max=0.003762 Jy/beam ! Clean residual mean=0.000197 rms=0.001138 Jy/beam ! Combined flux in latest and established models = 0.629399 Jy ! Adding 19 model components to the UV plane model. ! The established model now contains 64 components and 0.629399 Jy ! Inverting map ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=0.6607 mas, bmaj=2.899 mas, bpa=-10.11 degrees ! Estimated noise=685.537 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000463974 Jy ! Component: 100 - total flux cleaned = -0.000467155 Jy ! Component: 150 - total flux cleaned = -0.00033104 Jy ! Component: 200 - total flux cleaned = -0.000332866 Jy ! Total flux subtracted in 200 components = -0.000332866 Jy ! Clean residual min=-0.003057 max=0.003192 Jy/beam ! Clean residual mean=0.000114 rms=0.000920 Jy/beam ! Combined flux in latest and established models = 0.629066 Jy selfcal ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 80 components and 0.629066 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.264304Jy sigma=0.001257 ! Fit after self-cal, rms=0.264231Jy sigma=0.001257 wmodel J1513-1012_X_2003_05_07_pus_map.mod ! Writing 80 model components to file: J1513-1012_X_2003_05_07_pus_map.mod wobs J1513-1012_X_2003_05_07_pus_uvs.fits ! Writing UV FITS file: J1513-1012_X_2003_05_07_pus_uvs.fits wwins J1513-1012_X_2003_05_07_pus_map.win ! wwins: Wrote 4 windows to J1513-1012_X_2003_05_07_pus_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000548547 Jy ! Component: 100 - total flux cleaned = 0.00110495 Jy ! Component: 150 - total flux cleaned = 0.00162832 Jy ! Component: 200 - total flux cleaned = 0.00212513 Jy ! Component: 250 - total flux cleaned = 0.00255451 Jy ! Component: 300 - total flux cleaned = 0.0029227 Jy ! Component: 350 - total flux cleaned = 0.00318967 Jy ! Component: 400 - total flux cleaned = 0.00345025 Jy ! Component: 450 - total flux cleaned = 0.00370425 Jy ! Component: 500 - total flux cleaned = 0.00395232 Jy ! Component: 550 - total flux cleaned = 0.00403346 Jy ! Component: 600 - total flux cleaned = 0.00411293 Jy ! Component: 650 - total flux cleaned = 0.00419075 Jy ! Component: 700 - total flux cleaned = 0.00419018 Jy ! Component: 750 - total flux cleaned = 0.00422805 Jy ! Component: 800 - total flux cleaned = 0.00422823 Jy ! Component: 850 - total flux cleaned = 0.0042652 Jy ! Component: 900 - total flux cleaned = 0.00433777 Jy ! Component: 950 - total flux cleaned = 0.00433738 Jy ! Component: 1000 - total flux cleaned = 0.0043372 Jy ! Total flux subtracted in 1024 components = 0.00430207 Jy ! Clean residual min=-0.001748 max=0.001957 Jy/beam ! Clean residual mean=-0.000015 rms=0.000711 Jy/beam ! Combined flux in latest and established models = 0.633368 Jy keep ! Adding 50 model components to the UV plane model. ! The established model now contains 130 components and 0.633368 Jy wmap "J1513-1012_X_2003_05_07_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6607 x 2.899 at -10.11 degrees (North through East) ! Clean map min=-0.0040117 max=0.35954 Jy/beam ! Writing clean map to FITS file: J1513-1012_X_2003_05_07_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.359542 invert ! Inverting map ! Your choice of large map pixels excluded 4.41% of the data. ! The x-axis pixel size should ideally be below 0.1835 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000709499 device "J1513-1012_X_2003_05_07_pus\_map.eps/VPS" ! Attempting to open device: 'J1513-1012_X_2003_05_07_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.592003 0.592003 1.18401 2.36801 4.73602 9.47204 18.9441 37.8882 75.7764 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0021 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.359 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6607 x 2.899 at -10.11 degrees (North through East) ! Clean map min=-0.0040117 max=0.35954 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1513-1012_X_2003_05_07_pus\_map.gif/vgif" ! Attempting to open device: 'J1513-1012_X_2003_05_07_pus_map.gif/vgif' mapplot cln quit ! Quitting program ! Log file J1513-1012_X_2003_05_07_pus_uvs.log closed on Thu Dec 14 16:00:39 2006