! Started logfile: J1058+0133_X_2003_06_18_pus_uvs.log on Wed Jan 17 17:09:06 2007 obs J1058+0133_X_2003_06_18_pus_uva.fits ! Reading UV FITS file: J1058+0133_X_2003_06_18_pus_uva.fits ! AN table 1: 102 integrations on 153 of 153 possible baselines. ! AN table 2: 80 integrations on 153 of 153 possible baselines. ! AN table 3: 130 integrations on 153 of 153 possible baselines. ! AN table 4: 39 integrations on 153 of 153 possible baselines. ! AN table 5: 16 integrations on 153 of 153 possible baselines. ! AN table 6: 60 integrations on 153 of 153 possible baselines. ! AN table 7: 42 integrations on 153 of 153 possible baselines. ! AN table 8: Unused. ! AN table 9: Unused. ! Apparent sampling: 0.0674499 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1058+0133 ! ! 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 2231 lines of history. ! ! Reading 19360 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 1519 telescope corrections were flagged in sub-array 1. ! A total of 1330 telescope corrections were flagged in sub-array 2. ! A total of 2181 telescope corrections were flagged in sub-array 3. ! A total of 702 telescope corrections were flagged in sub-array 4. ! A total of 273 telescope corrections were flagged in sub-array 5. ! A total of 1041 telescope corrections were flagged in sub-array 6. ! A total of 625 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 2. ! A total of 1483 telescope corrections were flagged in sub-array 1. ! A total of 1287 telescope corrections were flagged in sub-array 2. ! A total of 2112 telescope corrections were flagged in sub-array 3. ! A total of 672 telescope corrections were flagged in sub-array 4. ! A total of 273 telescope corrections were flagged in sub-array 5. ! A total of 1041 telescope corrections were flagged in sub-array 6. ! A total of 625 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 3. ! A total of 1483 telescope corrections were flagged in sub-array 1. ! A total of 1300 telescope corrections were flagged in sub-array 2. ! A total of 2112 telescope corrections were flagged in sub-array 3. ! A total of 672 telescope corrections were flagged in sub-array 4. ! A total of 273 telescope corrections were flagged in sub-array 5. ! A total of 1041 telescope corrections were flagged in sub-array 6. ! A total of 626 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 4. ! A total of 1483 telescope corrections were flagged in sub-array 1. ! A total of 1287 telescope corrections were flagged in sub-array 2. ! A total of 2112 telescope corrections were flagged in sub-array 3. ! A total of 672 telescope corrections were flagged in sub-array 4. ! A total of 273 telescope corrections were flagged in sub-array 5. ! A total of 1041 telescope corrections were flagged in sub-array 6. ! A total of 625 telescope corrections were flagged in sub-array 7. ! ! Fit before self-cal, rms=1.649902Jy sigma=0.017880 ! Fit after self-cal, rms=1.190018Jy sigma=0.014903 ! 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 1.14% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.6196 mas, bmaj=1.58 mas, bpa=3.687 degrees ! Estimated noise=1254.76 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 = 1.60832 Jy ! Component: 100 - total flux cleaned = 1.99336 Jy ! Total flux subtracted in 100 components = 1.99336 Jy ! Clean residual min=-0.076165 max=0.156656 Jy/beam ! Clean residual mean=0.002221 rms=0.024885 Jy/beam ! Combined flux in latest and established models = 1.99336 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 1.99336 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.473419Jy sigma=0.004876 ! Fit after self-cal, rms=0.473121Jy sigma=0.004874 ! Inverting map ! Your choice of large map pixels excluded 1.14% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.166976 Jy ! Component: 100 - total flux cleaned = 0.250067 Jy ! Total flux subtracted in 100 components = 0.250067 Jy ! Clean residual min=-0.068745 max=0.083414 Jy/beam ! Clean residual mean=0.001469 rms=0.016976 Jy/beam ! Combined flux in latest and established models = 2.24343 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 14 components and 2.24343 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.413058Jy sigma=0.003654 ! Fit after self-cal, rms=0.412897Jy sigma=0.003653 ! Inverting map ! Your choice of large map pixels excluded 1.14% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 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 1.14% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.8025 mas, bmaj=1.809 mas, bpa=2.153 degrees ! Estimated noise=721.957 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 = 0.0589748 Jy ! Component: 100 - total flux cleaned = 0.0861459 Jy ! Component: 150 - total flux cleaned = 0.0990662 Jy ! Component: 200 - total flux cleaned = 0.100776 Jy ! Total flux subtracted in 200 components = 0.100776 Jy ! Clean residual min=-0.046890 max=0.084131 Jy/beam ! Clean residual mean=0.003979 rms=0.018915 Jy/beam ! Combined flux in latest and established models = 2.3442 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 19 components and 2.3442 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.407185Jy sigma=0.003497 ! Fit after self-cal, rms=0.407091Jy sigma=0.003497 ! Inverting map ! Your choice of large map pixels excluded 1.14% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 84 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 1.02 GG 1.00* HN 0.95 ! KK 1.28 KP 1.00 LA 0.96 MA 1.00* ! MK 0.92 NL 1.09 ON 1.00* OV 0.96 ! PT 0.96 SC 0.99 TC 1.00* TS 1.00* ! WF 1.14 WZ 1.00* ! ! A total of 78 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* GG 1.00* HN 0.92 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 1.01 ON 0.91 OV 1.00* ! PT 1.00* SC 1.00* TC 1.00* TS 1.00* ! WF 0.96 WZ 1.00* ! ! A total of 39 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.90 FD 1.05 GG 1.00* HN 1.00* ! KK 1.00* KP 0.97 LA 1.00* MA 1.00* ! MK 1.00* NL 1.00* ON 1.00* OV 1.00* ! PT 1.00* SC 1.00* TC 1.07 TS 1.00* ! WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 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 15 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 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 39 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* ! 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 51 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 1.07 GG 1.00* HN 1.00* ! KK 1.00* KP 1.01 LA 1.01 MA 1.00* ! MK 1.00* NL 1.00* ON 1.00* OV 1.05 ! PT 1.00* SC 1.03 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 2. ! A total of 84 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 1.00 GG 1.00* HN 0.96 ! KK 1.26 KP 0.95 LA 0.97 MA 1.13 ! MK 0.94 NL 1.05 ON 1.05 OV 0.97 ! PT 1.00 SC 0.95 TC 1.00* TS 1.11 ! WF 1.18 WZ 0.91 ! ! A total of 96 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* GG 1.00* HN 0.93 ! KK 1.00* KP 1.00* LA 1.00* MA 1.16 ! MK 1.00* NL 0.97 ON 0.96 OV 1.00* ! PT 1.00* SC 1.00* TC 1.00* TS 1.00* ! WF 1.03 WZ 1.00* ! ! A total of 108 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.91 FD 1.04 GG 1.00* HN 1.00* ! KK 1.00* KP 0.91 LA 1.00* MA 1.00* ! MK 1.00* NL 1.00* ON 1.00* OV 1.00* ! PT 1.00* SC 1.00* TC 1.15 TS 1.00* ! WF 1.00* WZ 1.00* ! ! A total of 30 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 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 15 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 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 39 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* ! 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 51 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 1.07 GG 1.00* HN 1.00* ! KK 1.00* KP 0.96 LA 1.02 MA 1.00* ! MK 1.00* NL 1.00* ON 1.00* OV 1.05 ! PT 1.00* SC 0.97 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 3. ! A total of 84 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 0.99 GG 1.00* HN 0.94 ! KK 1.35 KP 0.98 LA 0.97 MA 1.17 ! MK 0.93 NL 1.02 ON 1.08 OV 0.99 ! PT 1.02 SC 0.97 TC 1.00* TS 1.17 ! WF 1.11 WZ 0.88 ! ! A total of 108 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* GG 1.00* HN 0.88 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 0.99 ON 0.90 OV 1.00* ! PT 1.00* SC 1.00* TC 1.00* TS 1.00* ! WF 0.94 WZ 1.00* ! ! A total of 108 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 FD 1.00 GG 1.00* HN 1.00* ! KK 1.00* KP 0.95 LA 1.00* MA 1.00* ! MK 1.00* NL 1.00* ON 1.00* OV 1.00* ! PT 1.00* SC 1.00* TC 1.11 TS 1.00* ! WF 1.00* WZ 1.00* ! ! A total of 30 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 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 15 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 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 39 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* ! 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 54 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 1.05 GG 1.00* HN 1.00* ! KK 1.00* KP 1.01 LA 1.00 MA 1.00* ! MK 1.00* NL 1.00* ON 1.00* OV 1.08 ! PT 1.00* SC 0.97 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 4. ! A total of 84 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.97 GG 1.00* HN 0.96 ! KK 1.30 KP 0.94 LA 0.94 MA 1.08 ! MK 0.95 NL 1.02 ON 1.11 OV 0.99 ! PT 1.03 SC 1.01 TC 1.00* TS 1.10 ! WF 1.09 WZ 0.96 ! ! A total of 96 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* GG 1.00* HN 0.97 ! KK 1.00* KP 1.00* LA 1.00* MA 1.15 ! MK 1.00* NL 0.97 ON 0.90 OV 1.00* ! PT 1.00* SC 1.00* TC 1.00* TS 1.00* ! WF 0.90 WZ 1.00* ! ! A total of 108 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.92 FD 1.01 GG 1.00* HN 1.00* ! KK 1.00* KP 0.91 LA 1.00* MA 1.00* ! MK 1.00* NL 1.00* ON 1.00* OV 1.00* ! PT 1.00* SC 1.00* TC 1.08 TS 1.00* ! WF 1.00* WZ 1.00* ! ! A total of 30 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 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 15 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 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 39 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* ! 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 51 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 1.04 GG 1.00* HN 1.00* ! KK 1.00* KP 0.95 LA 0.99 MA 1.00* ! MK 1.00* NL 1.00* ON 1.00* OV 1.07 ! PT 1.00* SC 1.01 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! ! Fit before self-cal, rms=0.407091Jy sigma=0.003497 ! Fit after self-cal, rms=0.343296Jy sigma=0.002772 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.8495 mas, bmaj=1.768 mas, bpa=1.554 degrees ! Estimated noise=768.887 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 = -0.0113586 Jy ! Component: 100 - total flux cleaned = -0.0135412 Jy ! Component: 150 - total flux cleaned = -0.0150396 Jy ! Component: 200 - total flux cleaned = -0.0150395 Jy ! Total flux subtracted in 200 components = -0.0150395 Jy ! Clean residual min=-0.036863 max=0.067540 Jy/beam ! Clean residual mean=0.003319 rms=0.015093 Jy/beam ! Combined flux in latest and established models = 2.32916 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 23 components and 2.32916 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.342113Jy sigma=0.002758 ! Fit after self-cal, rms=0.342500Jy sigma=0.002757 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 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=0.342500Jy sigma=0.002757 ! Fit after self-cal, rms=0.343837Jy sigma=0.002753 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.8519 mas, bmaj=1.773 mas, bpa=1.643 degrees ! Estimated noise=768.356 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00968534 Jy ! Component: 100 - total flux cleaned = -0.0115628 Jy ! Component: 150 - total flux cleaned = -0.0122283 Jy ! Component: 200 - total flux cleaned = -0.0119297 Jy ! Total flux subtracted in 200 components = -0.0119297 Jy ! Clean residual min=-0.035064 max=0.066907 Jy/beam ! Clean residual mean=0.003419 rms=0.014958 Jy/beam ! Combined flux in latest and established models = 2.31723 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 24 components and 2.31723 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.342998Jy sigma=0.002742 ! Fit after self-cal, rms=0.342998Jy sigma=0.002742 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 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 (-2, 2.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0644515 Jy ! Component: 100 - total flux cleaned = 0.0993468 Jy ! Component: 150 - total flux cleaned = 0.120855 Jy ! Component: 200 - total flux cleaned = 0.12281 Jy ! Total flux subtracted in 200 components = 0.12281 Jy ! Clean residual min=-0.026264 max=0.048471 Jy/beam ! Clean residual mean=0.002329 rms=0.011855 Jy/beam ! Combined flux in latest and established models = 2.44004 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 48 components and 2.44004 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.331912Jy sigma=0.002467 ! Fit after self-cal, rms=0.329318Jy sigma=0.002438 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 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=0.329318Jy sigma=0.002438 ! Fit after self-cal, rms=0.328084Jy sigma=0.002416 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.8522 mas, bmaj=1.773 mas, bpa=1.61 degrees ! Estimated noise=766.41 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0234285 Jy ! Component: 100 - total flux cleaned = 0.0291353 Jy ! Component: 150 - total flux cleaned = 0.0336111 Jy ! Component: 200 - total flux cleaned = 0.0359157 Jy ! Total flux subtracted in 200 components = 0.0359157 Jy ! Clean residual min=-0.023410 max=0.045491 Jy/beam ! Clean residual mean=0.002110 rms=0.010796 Jy/beam ! Combined flux in latest and established models = 2.47596 Jy selfcal ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 64 components and 2.47596 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.325681Jy sigma=0.002352 ! Fit after self-cal, rms=0.325046Jy sigma=0.002345 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 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 = 0.00800492 Jy ! Component: 100 - total flux cleaned = 0.0104847 Jy ! Component: 150 - total flux cleaned = 0.011546 Jy ! Component: 200 - total flux cleaned = 0.0121963 Jy ! Total flux subtracted in 200 components = 0.0121963 Jy ! Clean residual min=-0.022197 max=0.044070 Jy/beam ! Clean residual mean=0.002003 rms=0.010557 Jy/beam ! Combined flux in latest and established models = 2.48815 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 73 components and 2.48815 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.324168Jy sigma=0.002324 ! Fit after self-cal, rms=0.323975Jy sigma=0.002323 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 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=0.323975Jy sigma=0.002323 ! Fit after self-cal, rms=0.324091Jy sigma=0.002313 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=2.209 mas, bmaj=3.2 mas, bpa=-11.64 degrees ! Estimated noise=956.236 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0254086 Jy ! Component: 100 - total flux cleaned = 0.0244738 Jy ! Component: 150 - total flux cleaned = 0.0237089 Jy ! Component: 200 - total flux cleaned = 0.0233741 Jy ! Total flux subtracted in 200 components = 0.0233741 Jy ! Clean residual min=-0.031689 max=0.070313 Jy/beam ! Clean residual mean=0.003898 rms=0.020074 Jy/beam ! Combined flux in latest and established models = 2.51153 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 84 components and 2.51153 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.324412Jy sigma=0.002299 ! Fit after self-cal, rms=0.324086Jy sigma=0.002295 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 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 = 0.00749789 Jy ! Component: 100 - total flux cleaned = 0.00718325 Jy ! Component: 150 - total flux cleaned = 0.00719134 Jy ! Component: 200 - total flux cleaned = 0.00690947 Jy ! Total flux subtracted in 200 components = 0.00690947 Jy ! Clean residual min=-0.030024 max=0.069140 Jy/beam ! Clean residual mean=0.003712 rms=0.019856 Jy/beam ! Combined flux in latest and established models = 2.51844 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 86 components and 2.51844 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.324247Jy sigma=0.002293 ! Fit after self-cal, rms=0.324116Jy sigma=0.002291 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 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 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.8528 mas, bmaj=1.774 mas, bpa=1.631 degrees ! Estimated noise=764.79 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8528 x 1.774 at 1.631 degrees (North through East) ! Clean map min=-0.020828 max=2.1236 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=0.324116Jy sigma=0.002291 ! Fit after self-cal, rms=0.297888Jy sigma=0.002027 ! Inverting map and beam ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.8534 mas, bmaj=1.775 mas, bpa=1.705 degrees ! Estimated noise=764.62 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0029917 Jy ! Component: 100 - total flux cleaned = -0.00425345 Jy ! Component: 150 - total flux cleaned = -0.00570271 Jy ! Component: 200 - total flux cleaned = -0.00668341 Jy ! Total flux subtracted in 200 components = -0.00668341 Jy ! Clean residual min=-0.020458 max=0.042316 Jy/beam ! Clean residual mean=0.001751 rms=0.009728 Jy/beam ! Combined flux in latest and established models = 2.51175 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 95 components and 2.51175 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.296821Jy sigma=0.002009 ! Fit after self-cal, rms=0.296902Jy sigma=0.002008 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec ! Added new window around map position (-5.2, 5.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0403167 Jy ! Component: 100 - total flux cleaned = 0.0636745 Jy ! Component: 150 - total flux cleaned = 0.0769386 Jy ! Component: 200 - total flux cleaned = 0.0832667 Jy ! Total flux subtracted in 200 components = 0.0832667 Jy ! Clean residual min=-0.019912 max=0.027438 Jy/beam ! Clean residual mean=0.000359 rms=0.007425 Jy/beam ! Combined flux in latest and established models = 2.59502 Jy ! Performing phase self-cal ! Adding 34 model components to the UV plane model. ! The established model now contains 127 components and 2.59502 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.291643Jy sigma=0.001840 ! Fit after self-cal, rms=0.291261Jy sigma=0.001831 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.291261Jy sigma=0.001831 ! Fit after self-cal, rms=0.290733Jy sigma=0.001813 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 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.643 mas, bmaj=1.614 mas, bpa=4.168 degrees ! Estimated noise=1325.82 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.63066 Jy ! Component: 100 - total flux cleaned = 2.00116 Jy ! Component: 150 - total flux cleaned = 2.14889 Jy ! Component: 200 - total flux cleaned = 2.23556 Jy ! Total flux subtracted in 200 components = 2.23556 Jy ! Clean residual min=-0.030241 max=0.045330 Jy/beam ! Clean residual mean=0.001929 rms=0.011470 Jy/beam ! Combined flux in latest and established models = 2.23556 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 17 model components to the UV plane model. ! The established model now contains 17 components and 2.23556 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.8544 mas, bmaj=1.778 mas, bpa=1.715 degrees ! Estimated noise=761.965 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 = 0.0739952 Jy ! Component: 100 - total flux cleaned = 0.12894 Jy ! Component: 150 - total flux cleaned = 0.173001 Jy ! Component: 200 - total flux cleaned = 0.209084 Jy ! Total flux subtracted in 200 components = 0.209084 Jy ! Clean residual min=-0.020530 max=0.028094 Jy/beam ! Clean residual mean=0.002417 rms=0.009176 Jy/beam ! Combined flux in latest and established models = 2.44464 Jy ! Adding 51 model components to the UV plane model. ! The established model now contains 59 components and 2.44464 Jy ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 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 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=2.21 mas, bmaj=3.206 mas, bpa=-11.53 degrees ! Estimated noise=950.377 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0606242 Jy ! Component: 100 - total flux cleaned = 0.101936 Jy ! Component: 150 - total flux cleaned = 0.131422 Jy ! Component: 200 - total flux cleaned = 0.152934 Jy ! Total flux subtracted in 200 components = 0.152934 Jy ! Clean residual min=-0.025583 max=0.037796 Jy/beam ! Clean residual mean=0.001500 rms=0.011854 Jy/beam ! Combined flux in latest and established models = 2.59758 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 = 0.0158324 Jy ! Component: 100 - total flux cleaned = 0.0275649 Jy ! Component: 150 - total flux cleaned = 0.0353663 Jy ! Component: 200 - total flux cleaned = 0.0390583 Jy ! Total flux subtracted in 200 components = 0.0390583 Jy ! Clean residual min=-0.024147 max=0.036262 Jy/beam ! Clean residual mean=0.000475 rms=0.011124 Jy/beam ! Combined flux in latest and established models = 2.63664 Jy ! Adding 51 model components to the UV plane model. ! The established model now contains 92 components and 2.63664 Jy ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.8544 mas, bmaj=1.778 mas, bpa=1.715 degrees ! Estimated noise=761.965 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00296452 Jy ! Component: 100 - total flux cleaned = -0.00300808 Jy ! Component: 150 - total flux cleaned = -0.00171647 Jy ! Component: 200 - total flux cleaned = -0.000576908 Jy ! Total flux subtracted in 200 components = -0.000576908 Jy ! Clean residual min=-0.016920 max=0.022110 Jy/beam ! Clean residual mean=0.000275 rms=0.005901 Jy/beam ! Combined flux in latest and established models = 2.63606 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 105 components and 2.63606 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.290319Jy sigma=0.001754 ! Fit after self-cal, rms=0.289966Jy sigma=0.001743 wmodel J1058+0133_X_2003_06_18_pus_map.mod ! Writing 105 model components to file: J1058+0133_X_2003_06_18_pus_map.mod wobs J1058+0133_X_2003_06_18_pus_uvs.fits ! Writing UV FITS file: J1058+0133_X_2003_06_18_pus_uvs.fits wwins J1058+0133_X_2003_06_18_pus_map.win ! wwins: Wrote 3 windows to J1058+0133_X_2003_06_18_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 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.00960982 Jy ! Component: 100 - total flux cleaned = 0.0164092 Jy ! Component: 150 - total flux cleaned = 0.0207291 Jy ! Component: 200 - total flux cleaned = 0.0230761 Jy ! Component: 250 - total flux cleaned = 0.0250062 Jy ! Component: 300 - total flux cleaned = 0.0259041 Jy ! Component: 350 - total flux cleaned = 0.0258961 Jy ! Component: 400 - total flux cleaned = 0.0256911 Jy ! Component: 450 - total flux cleaned = 0.0258874 Jy ! Component: 500 - total flux cleaned = 0.0255125 Jy ! Component: 550 - total flux cleaned = 0.0247903 Jy ! Component: 600 - total flux cleaned = 0.0242654 Jy ! Component: 650 - total flux cleaned = 0.0234233 Jy ! Component: 700 - total flux cleaned = 0.0227744 Jy ! Component: 750 - total flux cleaned = 0.0226202 Jy ! Component: 800 - total flux cleaned = 0.0223166 Jy ! Component: 850 - total flux cleaned = 0.0221714 Jy ! Component: 900 - total flux cleaned = 0.0228908 Jy ! Component: 950 - total flux cleaned = 0.0228888 Jy ! Component: 1000 - total flux cleaned = 0.0228907 Jy ! Total flux subtracted in 1024 components = 0.0230269 Jy ! Clean residual min=-0.010628 max=0.007341 Jy/beam ! Clean residual mean=-0.000071 rms=0.003109 Jy/beam ! Combined flux in latest and established models = 2.65909 Jy keep ! Adding 84 model components to the UV plane model. ! The established model now contains 188 components and 2.65909 Jy wmap "J1058+0133_X_2003_06_18_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8544 x 1.778 at 1.715 degrees (North through East) ! Clean map min=-0.011462 max=2.12 Jy/beam ! Writing clean map to FITS file: J1058+0133_X_2003_06_18_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 2.11999 invert ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1956 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00310068 device "J1058+0133_X_2003_06_18_pus\_map.eps/VPS" ! Attempting to open device: 'J1058+0133_X_2003_06_18_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.438776 0.438776 0.877553 1.75511 3.51021 7.02042 14.0408 28.0817 56.1634 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0093 print "peak=",int(1000*peak_flux)/1000 ! peak= 2.119 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8544 x 1.778 at 1.715 degrees (North through East) ! Clean map min=-0.011462 max=2.12 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1058+0133_X_2003_06_18_pus\_map.gif/vgif" ! Attempting to open device: 'J1058+0133_X_2003_06_18_pus_map.gif/vgif' mapplot cln quit ! Quitting program ! Log file J1058+0133_X_2003_06_18_pus_uvs.log closed on Wed Jan 17 17:10:36 2007