! Started logfile: J0102+5824_X_2003_06_18_pus_uvs.log on Thu Jan 18 13:09:10 2007 obs J0102+5824_X_2003_06_18_pus_uva.fits ! Reading UV FITS file: J0102+5824_X_2003_06_18_pus_uva.fits ! AN table 1: 31 integrations on 153 of 153 possible baselines. ! AN table 2: 32 integrations on 153 of 153 possible baselines. ! AN table 3: 20 integrations on 153 of 153 possible baselines. ! AN table 4: 149 integrations on 153 of 153 possible baselines. ! AN table 5: 83 integrations on 153 of 153 possible baselines. ! AN table 6: 58 integrations on 153 of 153 possible baselines. ! Apparent sampling: 0.161541 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0102+5824 ! ! 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 2235 lines of history. ! ! Reading 36876 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 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 558 telescope corrections were flagged in sub-array 1. ! A total of 520 telescope corrections were flagged in sub-array 2. ! A total of 255 telescope corrections were flagged in sub-array 3. ! A total of 2008 telescope corrections were flagged in sub-array 4. ! A total of 751 telescope corrections were flagged in sub-array 5. ! A total of 703 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 522 telescope corrections were flagged in sub-array 1. ! A total of 467 telescope corrections were flagged in sub-array 2. ! A total of 243 telescope corrections were flagged in sub-array 3. ! A total of 1965 telescope corrections were flagged in sub-array 4. ! A total of 727 telescope corrections were flagged in sub-array 5. ! A total of 651 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 558 telescope corrections were flagged in sub-array 1. ! A total of 520 telescope corrections were flagged in sub-array 2. ! A total of 243 telescope corrections were flagged in sub-array 3. ! A total of 1962 telescope corrections were flagged in sub-array 4. ! A total of 727 telescope corrections were flagged in sub-array 5. ! A total of 651 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 522 telescope corrections were flagged in sub-array 1. ! A total of 464 telescope corrections were flagged in sub-array 2. ! A total of 243 telescope corrections were flagged in sub-array 3. ! A total of 1964 telescope corrections were flagged in sub-array 4. ! A total of 727 telescope corrections were flagged in sub-array 5. ! A total of 651 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=2.815243Jy sigma=0.033712 ! Fit after self-cal, rms=2.411668Jy sigma=0.029478 ! 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 3.15% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! Estimated beam: bmin=0.4911 mas, bmaj=0.6881 mas, bpa=4.083 degrees ! Estimated noise=640.78 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 = 2.54637 Jy ! Component: 100 - total flux cleaned = 3.11602 Jy ! Total flux subtracted in 100 components = 3.11602 Jy ! Clean residual min=-0.066545 max=0.207602 Jy/beam ! Clean residual mean=0.000669 rms=0.017293 Jy/beam ! Combined flux in latest and established models = 3.11602 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 3.11602 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.588600Jy sigma=0.006524 ! Fit after self-cal, rms=0.588569Jy sigma=0.006524 ! Inverting map ! Your choice of large map pixels excluded 3.15% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.231028 Jy ! Component: 100 - total flux cleaned = 0.370195 Jy ! Total flux subtracted in 100 components = 0.370195 Jy ! Clean residual min=-0.050139 max=0.076112 Jy/beam ! Clean residual mean=0.000225 rms=0.011003 Jy/beam ! Combined flux in latest and established models = 3.48622 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 14 components and 3.48622 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.467325Jy sigma=0.004270 ! Fit after self-cal, rms=0.466086Jy sigma=0.004269 ! Inverting map ! Your choice of large map pixels excluded 3.15% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0954191 Jy ! Component: 100 - total flux cleaned = 0.161869 Jy ! Total flux subtracted in 100 components = 0.161869 Jy ! Clean residual min=-0.051926 max=0.042545 Jy/beam ! Clean residual mean=0.000036 rms=0.009502 Jy/beam ! Combined flux in latest and established models = 3.64809 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 17 components and 3.64809 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.446194Jy sigma=0.003801 ! Fit after self-cal, rms=0.446244Jy sigma=0.003801 ! Inverting map ! Your choice of large map pixels excluded 3.15% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 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 3.15% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! Estimated beam: bmin=0.6496 mas, bmaj=0.8464 mas, bpa=-5.273 degrees ! Estimated noise=351.946 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 = 0.0425633 Jy ! Component: 100 - total flux cleaned = 0.0547346 Jy ! Component: 150 - total flux cleaned = 0.0547523 Jy ! Component: 200 - total flux cleaned = 0.0548022 Jy ! Total flux subtracted in 200 components = 0.0548022 Jy ! Clean residual min=-0.060227 max=0.030667 Jy/beam ! Clean residual mean=0.000016 rms=0.009425 Jy/beam ! Combined flux in latest and established models = 3.70289 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 21 components and 3.70289 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.444480Jy sigma=0.003692 ! Fit after self-cal, rms=0.444400Jy sigma=0.003692 ! Inverting map ! Your choice of large map pixels excluded 3.15% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! 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 9 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 1.06 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 1.03 ON 1.03 OV 1.00* ! PT 1.00* SC 1.00 TC 1.00* TS 1.00* ! WF 1.10 WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.92 FD 1.00* GG 1.00* HN 0.95 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 1.03 ON 1.00* OV 1.00* ! PT 1.00* SC 0.98 TC 1.00* TS 1.12 ! WF 1.00 WZ 1.00* ! ! A total of 15 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 0.95 ! KK 0.98 KP 1.01 LA 0.98 MA 1.00* ! MK 0.96 NL 1.05 ON 1.06 OV 0.96 ! PT 0.96 SC 0.96 TC 1.00* TS 0.96 ! WF 1.02 WZ 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.95 FD 1.01 GG 1.00* HN 0.92 ! KK 1.00* KP 1.05 LA 1.00 MA 1.00* ! MK 1.00* NL 1.05 ON 0.98 OV 1.00 ! PT 0.99 SC 0.98 TC 1.00* TS 1.14 ! WF 0.98 WZ 1.04 ! ! A total of 6 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.93 FD 1.00* GG 1.00* HN 0.90 ! KK 1.00* KP 1.00* LA 1.13 MA 1.00* ! MK 1.00* NL 1.32 ON 1.06 OV 1.10 ! PT 1.00* SC 1.00* TC 1.00* TS 0.95 ! WF 1.08 WZ 1.00* ! ! ! Correcting IF 2. ! A total of 36 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! 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 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* GG 1.00* HN 1.10 ! KK 1.00* KP 1.00* LA 1.00* MA 1.20 ! MK 1.00* NL 1.01 ON 1.04 OV 1.00* ! PT 1.00* SC 0.93 TC 1.00* TS 1.00* ! WF 1.13 WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.94 FD 1.00* GG 1.00* HN 0.97 ! KK 1.00* KP 1.00* LA 1.00* MA 0.98 ! MK 1.00* NL 1.00 ON 1.00* OV 1.00* ! PT 1.00* SC 0.95 TC 1.00* TS 1.14 ! WF 1.01 WZ 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.96 FD 1.01 GG 1.00* HN 0.97 ! KK 0.96 KP 0.96 LA 0.98 MA 1.17 ! MK 0.97 NL 1.01 ON 1.08 OV 0.96 ! PT 1.00 SC 0.93 TC 1.00* TS 0.95 ! WF 1.03 WZ 0.94 ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.96 FD 1.00 GG 1.00* HN 0.93 ! KK 1.00* KP 1.00 LA 1.01 MA 0.95 ! MK 1.00* NL 1.01 ON 1.00 OV 0.99 ! PT 1.04 SC 0.94 TC 1.00* TS 1.15 ! WF 1.00 WZ 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.95 FD 1.00* GG 1.00* HN 0.91 ! KK 1.00* KP 1.00* LA 1.14 MA 1.04 ! MK 1.00* NL 1.29 ON 1.08 OV 1.09 ! PT 1.00* SC 1.00* TC 1.00* TS 0.95 ! WF 1.11 WZ 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! 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 9 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 1.11 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 1.00 ON 1.06 OV 1.00* ! PT 1.00* SC 1.00 TC 1.00* TS 1.00* ! WF 1.04 WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 1.00* GG 1.00* HN 0.95 ! KK 1.00* KP 1.00* LA 1.00* MA 0.95 ! MK 1.00* NL 0.98 ON 1.00* OV 1.00* ! PT 1.00* SC 0.99 TC 1.00* TS 1.12 ! WF 0.95 WZ 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 FD 1.01 GG 1.00* HN 0.96 ! KK 1.01 KP 1.00 LA 0.99 MA 1.24 ! MK 0.97 NL 0.99 ON 1.05 OV 1.00 ! PT 1.03 SC 0.96 TC 1.00* TS 0.95 ! WF 0.96 WZ 0.96 ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 0.99 GG 1.00* HN 0.93 ! KK 1.00* KP 1.04 LA 1.01 MA 0.94 ! MK 1.00* NL 0.99 ON 1.00 OV 1.04 ! PT 1.06 SC 0.98 TC 1.00* TS 1.14 ! WF 0.95 WZ 1.01 ! ! A total of 6 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.99 FD 1.00* GG 1.00* HN 0.91 ! KK 1.00* KP 1.00* LA 1.14 MA 1.03 ! MK 1.00* NL 1.27 ON 1.10 OV 1.14 ! PT 1.00* SC 1.00* TC 1.00* TS 0.94 ! WF 1.01 WZ 1.00* ! ! ! Correcting IF 4. ! A total of 36 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! 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 42 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 1.13 ! KK 1.00* KP 1.00* LA 1.00* MA 1.25 ! MK 1.00* NL 1.01 ON 1.07 OV 1.00* ! PT 1.00* SC 1.01 TC 1.00* TS 1.00* ! WF 1.04 WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.96 FD 1.00* GG 1.00* HN 0.98 ! KK 1.00* KP 1.00* LA 1.00* MA 0.95 ! MK 1.00* NL 0.98 ON 1.00* OV 1.00* ! PT 1.00* SC 1.03 TC 1.00* TS 1.12 ! WF 0.94 WZ 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 FD 0.99 GG 1.00* HN 0.99 ! KK 0.98 KP 0.96 LA 0.97 MA 1.22 ! MK 1.00 NL 1.00 ON 1.05 OV 0.99 ! PT 1.03 SC 1.01 TC 1.00* TS 0.96 ! WF 0.96 WZ 0.98 ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 FD 0.98 GG 1.00* HN 0.96 ! KK 1.00* KP 1.00 LA 0.99 MA 0.94 ! MK 1.00* NL 1.00 ON 1.05 OV 1.02 ! PT 1.07 SC 1.02 TC 1.00* TS 1.13 ! WF 0.94 WZ 1.02 ! ! A total of 6 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.97 FD 1.00* GG 1.00* HN 0.94 ! KK 1.00* KP 1.00* LA 1.12 MA 1.02 ! MK 1.00* NL 1.33 ON 1.19 OV 1.12 ! PT 1.00* SC 1.00* TC 1.00* TS 0.95 ! WF 1.01 WZ 1.00* ! ! ! Fit before self-cal, rms=0.444400Jy sigma=0.003692 ! Fit after self-cal, rms=0.353782Jy sigma=0.002427 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! Estimated beam: bmin=0.6567 mas, bmaj=0.8469 mas, bpa=-5.523 degrees ! Estimated noise=353 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 = -0.00978058 Jy ! Component: 100 - total flux cleaned = -0.0108205 Jy ! Component: 150 - total flux cleaned = -0.012177 Jy ! Component: 200 - total flux cleaned = -0.0129792 Jy ! Total flux subtracted in 200 components = -0.0129792 Jy ! Clean residual min=-0.016713 max=0.011678 Jy/beam ! Clean residual mean=0.000644 rms=0.003834 Jy/beam ! Combined flux in latest and established models = 3.68991 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 23 components and 3.68991 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.352061Jy sigma=0.002398 ! Fit after self-cal, rms=0.353765Jy sigma=0.002398 ! Inverting map ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 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=0.353765Jy sigma=0.002398 ! Fit after self-cal, rms=0.343907Jy sigma=0.002175 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! Estimated beam: bmin=0.6585 mas, bmaj=0.8475 mas, bpa=-5.776 degrees ! Estimated noise=352.525 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0140194 Jy ! Component: 100 - total flux cleaned = -0.0144068 Jy ! Component: 150 - total flux cleaned = -0.0150854 Jy ! Component: 200 - total flux cleaned = -0.0153753 Jy ! Total flux subtracted in 200 components = -0.0153753 Jy ! Clean residual min=-0.010055 max=0.011194 Jy/beam ! Clean residual mean=0.000624 rms=0.002462 Jy/beam ! Combined flux in latest and established models = 3.67454 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 26 components and 3.67454 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.342498Jy sigma=0.002160 ! Fit after self-cal, rms=0.341370Jy sigma=0.002160 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 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 (-3.2, -1.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0100622 Jy ! Component: 100 - total flux cleaned = 0.011178 Jy ! Component: 150 - total flux cleaned = 0.0119047 Jy ! Component: 200 - total flux cleaned = 0.0123529 Jy ! Total flux subtracted in 200 components = 0.0123529 Jy ! Clean residual min=-0.009849 max=0.007613 Jy/beam ! Clean residual mean=0.000341 rms=0.002362 Jy/beam ! Combined flux in latest and established models = 3.68689 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 33 components and 3.68689 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.340822Jy sigma=0.002151 ! Fit after self-cal, rms=0.340804Jy sigma=0.002151 ! Inverting map ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 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=0.340804Jy sigma=0.002151 ! Fit after self-cal, rms=0.335251Jy sigma=0.002044 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! Estimated beam: bmin=0.6596 mas, bmaj=0.8473 mas, bpa=-5.789 degrees ! Estimated noise=352.826 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000876041 Jy ! Component: 100 - total flux cleaned = 0.000176608 Jy ! Component: 150 - total flux cleaned = 0.00103869 Jy ! Component: 200 - total flux cleaned = 0.00159056 Jy ! Total flux subtracted in 200 components = 0.00159056 Jy ! Clean residual min=-0.004623 max=0.006700 Jy/beam ! Clean residual mean=0.000571 rms=0.001424 Jy/beam ! Combined flux in latest and established models = 3.68848 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 35 components and 3.68848 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.334686Jy sigma=0.002039 ! Fit after self-cal, rms=0.334438Jy sigma=0.002039 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 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 (-1.6, -0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00546508 Jy ! Component: 100 - total flux cleaned = 0.00528498 Jy ! Component: 150 - total flux cleaned = 0.00512913 Jy ! Component: 200 - total flux cleaned = 0.00526345 Jy ! Total flux subtracted in 200 components = 0.00526345 Jy ! Clean residual min=-0.004805 max=0.005932 Jy/beam ! Clean residual mean=0.000453 rms=0.001360 Jy/beam ! Combined flux in latest and established models = 3.69374 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 41 components and 3.69374 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.334130Jy sigma=0.002036 ! Fit after self-cal, rms=0.334123Jy sigma=0.002036 ! Inverting map ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! Added new window around map position (-2, 4.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00494682 Jy ! Component: 100 - total flux cleaned = 0.00537395 Jy ! Component: 150 - total flux cleaned = 0.00524964 Jy ! Component: 200 - total flux cleaned = 0.00513374 Jy ! Total flux subtracted in 200 components = 0.00513374 Jy ! Clean residual min=-0.005321 max=0.005500 Jy/beam ! Clean residual mean=0.000350 rms=0.001324 Jy/beam ! Combined flux in latest and established models = 3.69888 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 53 components and 3.69888 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.333858Jy sigma=0.002035 ! Fit after self-cal, rms=0.333880Jy sigma=0.002035 ! Inverting map ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 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=0.333880Jy sigma=0.002035 ! Fit after self-cal, rms=0.333219Jy sigma=0.002031 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! Estimated beam: bmin=2.273 mas, bmaj=3.072 mas, bpa=-74.51 degrees ! Estimated noise=488.497 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00215425 Jy ! Component: 100 - total flux cleaned = 0.00223608 Jy ! Component: 150 - total flux cleaned = 0.0023112 Jy ! Component: 200 - total flux cleaned = 0.00243845 Jy ! Total flux subtracted in 200 components = 0.00243845 Jy ! Clean residual min=-0.003708 max=0.007209 Jy/beam ! Clean residual mean=0.001055 rms=0.001892 Jy/beam ! Combined flux in latest and established models = 3.70131 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 67 components and 3.70131 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.333230Jy sigma=0.002031 ! Fit after self-cal, rms=0.333155Jy sigma=0.002031 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 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 = 0.000235602 Jy ! Component: 100 - total flux cleaned = 0.000291497 Jy ! Component: 150 - total flux cleaned = 0.000390697 Jy ! Component: 200 - total flux cleaned = 0.000436286 Jy ! Total flux subtracted in 200 components = 0.000436286 Jy ! Clean residual min=-0.003831 max=0.007110 Jy/beam ! Clean residual mean=0.001030 rms=0.001879 Jy/beam ! Combined flux in latest and established models = 3.70175 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 71 components and 3.70175 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.333183Jy sigma=0.002031 ! Fit after self-cal, rms=0.333182Jy sigma=0.002031 ! Inverting map ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 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 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! Estimated beam: bmin=0.6607 mas, bmaj=0.8467 mas, bpa=-5.814 degrees ! Estimated noise=353.008 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6607 x 0.8467 at -5.814 degrees (North through East) ! Clean map min=-0.0042843 max=3.3888 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=0.333182Jy sigma=0.002031 ! Fit after self-cal, rms=1.003529Jy sigma=0.001701 ! Inverting map and beam ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! Estimated beam: bmin=0.6607 mas, bmaj=0.8468 mas, bpa=-5.845 degrees ! Estimated noise=353.156 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00219286 Jy ! Component: 100 - total flux cleaned = 0.0025752 Jy ! Component: 150 - total flux cleaned = 0.00273082 Jy ! Component: 200 - total flux cleaned = 0.00247481 Jy ! Total flux subtracted in 200 components = 0.00247481 Jy ! Clean residual min=-0.003279 max=0.004122 Jy/beam ! Clean residual mean=0.000104 rms=0.000953 Jy/beam ! Combined flux in latest and established models = 3.70423 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 76 components and 3.70423 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.003406Jy sigma=0.001698 ! Fit after self-cal, rms=1.003565Jy sigma=0.001698 ! Inverting map ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000241992 Jy ! Component: 100 - total flux cleaned = 0.000243351 Jy ! Component: 150 - total flux cleaned = 0.000341613 Jy ! Component: 200 - total flux cleaned = 0.000337835 Jy ! Total flux subtracted in 200 components = 0.000337835 Jy ! Clean residual min=-0.003417 max=0.003649 Jy/beam ! Clean residual mean=0.000096 rms=0.000938 Jy/beam ! Combined flux in latest and established models = 3.70456 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 80 components and 3.70456 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.003522Jy sigma=0.001697 ! Fit after self-cal, rms=1.003556Jy sigma=0.001697 ! Inverting map ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.003556Jy sigma=0.001697 ! Fit after self-cal, rms=0.992108Jy sigma=0.001695 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 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! Estimated beam: bmin=0.498 mas, bmaj=0.6868 mas, bpa=3.869 degrees ! Estimated noise=642.625 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.55916 Jy ! Component: 100 - total flux cleaned = 3.12054 Jy ! Component: 150 - total flux cleaned = 3.31892 Jy ! Component: 200 - total flux cleaned = 3.44299 Jy ! Total flux subtracted in 200 components = 3.44299 Jy ! Clean residual min=-0.016447 max=0.066778 Jy/beam ! Clean residual mean=0.000329 rms=0.005702 Jy/beam ! Combined flux in latest and established models = 3.44299 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 14 model components to the UV plane model. ! The established model now contains 14 components and 3.44299 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! Estimated beam: bmin=0.6613 mas, bmaj=0.8463 mas, bpa=-5.861 degrees ! Estimated noise=353.432 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 = 0.127878 Jy ! Component: 100 - total flux cleaned = 0.188743 Jy ! Component: 150 - total flux cleaned = 0.219722 Jy ! Component: 200 - total flux cleaned = 0.237462 Jy ! Total flux subtracted in 200 components = 0.237462 Jy ! Clean residual min=-0.006435 max=0.009417 Jy/beam ! Clean residual mean=0.000695 rms=0.001441 Jy/beam ! Combined flux in latest and established models = 3.68045 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 28 components and 3.68045 Jy ! Inverting map ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0118012 Jy ! Component: 100 - total flux cleaned = 0.0200828 Jy ! Component: 150 - total flux cleaned = 0.0247738 Jy ! Component: 200 - total flux cleaned = 0.0265848 Jy ! Total flux subtracted in 200 components = 0.0265848 Jy ! Clean residual min=-0.008042 max=0.004077 Jy/beam ! Clean residual mean=0.000103 rms=0.001127 Jy/beam ! Combined flux in latest and established models = 3.70704 Jy ! Adding 22 model components to the UV plane model. ! The established model now contains 37 components and 3.70704 Jy ! Inverting map ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 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 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! Estimated beam: bmin=2.272 mas, bmaj=3.071 mas, bpa=-74.5 degrees ! Estimated noise=489.169 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000842267 Jy ! Component: 100 - total flux cleaned = 0.00136557 Jy ! Component: 150 - total flux cleaned = 0.00176329 Jy ! Component: 200 - total flux cleaned = 0.00187169 Jy ! Total flux subtracted in 200 components = 0.00187169 Jy ! Clean residual min=-0.003102 max=0.004039 Jy/beam ! Clean residual mean=0.000188 rms=0.001197 Jy/beam ! Combined flux in latest and established models = 3.70891 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 = 4.77822e-05 Jy ! Component: 100 - total flux cleaned = 8.79241e-05 Jy ! Component: 150 - total flux cleaned = 8.76856e-05 Jy ! Component: 200 - total flux cleaned = 8.76152e-05 Jy ! Total flux subtracted in 200 components = 8.76152e-05 Jy ! Clean residual min=-0.003054 max=0.004001 Jy/beam ! Clean residual mean=0.000182 rms=0.001182 Jy/beam ! Combined flux in latest and established models = 3.709 Jy ! Adding 25 model components to the UV plane model. ! The established model now contains 58 components and 3.709 Jy ! Inverting map ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! Estimated beam: bmin=0.6613 mas, bmaj=0.8463 mas, bpa=-5.861 degrees ! Estimated noise=353.432 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00202491 Jy ! Component: 100 - total flux cleaned = 0.00242105 Jy ! Component: 150 - total flux cleaned = 0.00278701 Jy ! Component: 200 - total flux cleaned = 0.00295518 Jy ! Total flux subtracted in 200 components = 0.00295518 Jy ! Clean residual min=-0.007020 max=0.003581 Jy/beam ! Clean residual mean=-0.000003 rms=0.001063 Jy/beam ! Combined flux in latest and established models = 3.71195 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 64 components and 3.71195 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.992690Jy sigma=0.001722 ! Fit after self-cal, rms=0.992962Jy sigma=0.001722 wmodel J0102+5824_X_2003_06_18_pus_map.mod ! Writing 64 model components to file: J0102+5824_X_2003_06_18_pus_map.mod wobs J0102+5824_X_2003_06_18_pus_uvs.fits ! Writing UV FITS file: J0102+5824_X_2003_06_18_pus_uvs.fits wwins J0102+5824_X_2003_06_18_pus_map.win ! wwins: Wrote 4 windows to J0102+5824_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 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00295651 Jy ! Component: 100 - total flux cleaned = -0.00507358 Jy ! Component: 150 - total flux cleaned = -0.00539881 Jy ! Component: 200 - total flux cleaned = -0.00562909 Jy ! Component: 250 - total flux cleaned = -0.00577563 Jy ! Component: 300 - total flux cleaned = -0.00549791 Jy ! Component: 350 - total flux cleaned = -0.00516267 Jy ! Component: 400 - total flux cleaned = -0.00490209 Jy ! Component: 450 - total flux cleaned = -0.0045842 Jy ! Component: 500 - total flux cleaned = -0.00439699 Jy ! Component: 550 - total flux cleaned = -0.00409226 Jy ! Component: 600 - total flux cleaned = -0.00391376 Jy ! Component: 650 - total flux cleaned = -0.00362092 Jy ! Component: 700 - total flux cleaned = -0.0033907 Jy ! Component: 750 - total flux cleaned = -0.0031646 Jy ! Component: 800 - total flux cleaned = -0.00299775 Jy ! Component: 850 - total flux cleaned = -0.0027792 Jy ! Component: 900 - total flux cleaned = -0.00267201 Jy ! Component: 950 - total flux cleaned = -0.00256579 Jy ! Component: 1000 - total flux cleaned = -0.00246122 Jy ! Total flux subtracted in 1024 components = -0.00240912 Jy ! Clean residual min=-0.002594 max=0.002707 Jy/beam ! Clean residual mean=0.000063 rms=0.000899 Jy/beam ! Combined flux in latest and established models = 3.70954 Jy keep ! Adding 49 model components to the UV plane model. ! The established model now contains 107 components and 3.70954 Jy wmap "J0102+5824_X_2003_06_18_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6613 x 0.8463 at -5.861 degrees (North through East) ! Clean map min=-0.0033024 max=3.3941 Jy/beam ! Writing clean map to FITS file: J0102+5824_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 3.3941 invert ! Inverting map ! Your choice of large map pixels excluded 3.06% of the data. ! The x-axis pixel size should ideally be below 0.1535 milli-arcsec ! The y-axis pixel size should ideally be below 0.1771 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000899024 device "J0102+5824_X_2003_06_18_pus\_map.eps/VPS" ! Attempting to open device: 'J0102+5824_X_2003_06_18_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.0794636 0.0794636 0.158927 0.317854 0.635709 1.27142 2.54283 5.08567 10.1713 20.3427 40.6854 81.3707 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0026 print "peak=",int(1000*peak_flux)/1000 ! peak= 3.394 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6613 x 0.8463 at -5.861 degrees (North through East) ! Clean map min=-0.0033024 max=3.3941 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0102+5824_X_2003_06_18_pus\_map.gif/vgif" ! Attempting to open device: 'J0102+5824_X_2003_06_18_pus_map.gif/vgif' mapplot cln quit ! Quitting program ! Log file J0102+5824_X_2003_06_18_pus_uvs.log closed on Thu Jan 18 13:10:57 2007