! Started logfile: J0102+5824_X_2003_07_09_pus_uvs.log on Sat Apr 6 23:14:25 2013 obs J0102+5824_X_2003_07_09_pus_uva.fits ! Reading UV FITS file: J0102+5824_X_2003_07_09_pus_uva.fits ! AN table 1: 11 integrations on 171 of 171 possible baselines. ! AN table 2: 29 integrations on 171 of 171 possible baselines. ! AN table 3: 68 integrations on 171 of 171 possible baselines. ! AN table 4: 67 integrations on 171 of 171 possible baselines. ! AN table 5: 158 integrations on 171 of 171 possible baselines. ! Apparent sampling: 0.282862 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0102+5824 ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! ! 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 1874 lines of history. ! ! Reading 64428 visibilities. select I ! Polarization I is unavailable. ! Selecting polarization: RR, channels: 1..4 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 print "field_size =",field_size ! field_size = 512 print "field_cell =",field_cell ! field_cell = 0.2 print "taper_size =",taper_size ! taper_size = 70 ![@muppet J0102+5824_X_2003_07_09_pus] integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.03 float dynam dynam = 6.0 float soltime1 soltime1 = 120 float soltime2 soltime2 = 20 float thresh thresh = 0.5 float win_mult win_mult = 1.8 float time_av time_av = 16 float old_peak float new_peak float flux_cutoff mapsize field_size, field_cell ! Map grid = 512x512 pixels with 0.200x0.200 milli-arcsec cellsize. startmod ! Applying default point source starting model. ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 1 Jy ! ! Correcting IF 1. ! A total of 185 telescope corrections were flagged in sub-array 1. ! A total of 184 telescope corrections were flagged in sub-array 2. ! A total of 767 telescope corrections were flagged in sub-array 3. ! A total of 703 telescope corrections were flagged in sub-array 4. ! A total of 1403 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 185 telescope corrections were flagged in sub-array 1. ! A total of 184 telescope corrections were flagged in sub-array 2. ! A total of 766 telescope corrections were flagged in sub-array 3. ! A total of 703 telescope corrections were flagged in sub-array 4. ! A total of 1403 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 185 telescope corrections were flagged in sub-array 1. ! A total of 184 telescope corrections were flagged in sub-array 2. ! A total of 766 telescope corrections were flagged in sub-array 3. ! A total of 703 telescope corrections were flagged in sub-array 4. ! A total of 1403 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 185 telescope corrections were flagged in sub-array 1. ! A total of 184 telescope corrections were flagged in sub-array 2. ! A total of 767 telescope corrections were flagged in sub-array 3. ! A total of 703 telescope corrections were flagged in sub-array 4. ! A total of 1403 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=2.787555Jy sigma=0.022579 ! Fit after self-cal, rms=2.418923Jy sigma=0.019950 ! 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 1.49% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! Estimated beam: bmin=0.5517 mas, bmaj=0.6434 mas, bpa=2.552 degrees ! Estimated noise=711.592 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 = 2.43542 Jy ! Component: 100 - total flux cleaned = 2.99619 Jy ! Total flux subtracted in 100 components = 2.99619 Jy ! Clean residual min=-0.077501 max=0.221229 Jy/beam ! Clean residual mean=0.000329 rms=0.017130 Jy/beam ! Combined flux in latest and established models = 2.99618 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 2.99618 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.797666Jy sigma=0.006794 ! Fit after self-cal, rms=0.797660Jy sigma=0.006794 ! Inverting map ! Your choice of large map pixels excluded 1.49% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.269888 Jy ! Component: 100 - total flux cleaned = 0.451954 Jy ! Total flux subtracted in 100 components = 0.451954 Jy ! Clean residual min=-0.067674 max=0.103464 Jy/beam ! Clean residual mean=0.000104 rms=0.014277 Jy/beam ! Combined flux in latest and established models = 3.44814 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 10 components and 3.44814 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.637257Jy sigma=0.005133 ! Fit after self-cal, rms=0.637224Jy sigma=0.005133 ! Inverting map ! Your choice of large map pixels excluded 1.49% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! Added new window around map position (0.6, -0.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.126797 Jy ! Component: 100 - total flux cleaned = 0.219462 Jy ! Total flux subtracted in 100 components = 0.219462 Jy ! Clean residual min=-0.062465 max=0.083517 Jy/beam ! Clean residual mean=-0.000004 rms=0.013501 Jy/beam ! Combined flux in latest and established models = 3.6676 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 17 components and 3.6676 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.594948Jy sigma=0.004603 ! Fit after self-cal, rms=0.594571Jy sigma=0.004599 ! Inverting map ! Your choice of large map pixels excluded 1.49% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 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 1.49% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! Estimated beam: bmin=0.702 mas, bmaj=0.7797 mas, bpa=12.7 degrees ! Estimated noise=377.95 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 = 0.15266 Jy ! Component: 100 - total flux cleaned = 0.242952 Jy ! Component: 150 - total flux cleaned = 0.299859 Jy ! Component: 200 - total flux cleaned = 0.336033 Jy ! Total flux subtracted in 200 components = 0.336033 Jy ! Clean residual min=-0.053909 max=0.067202 Jy/beam ! Clean residual mean=-0.001800 rms=0.011963 Jy/beam ! Combined flux in latest and established models = 4.00363 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 30 components and 4.00363 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.568549Jy sigma=0.004159 ! Fit after self-cal, rms=0.568230Jy sigma=0.004155 ! Inverting map ! Your choice of large map pixels excluded 1.49% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 24 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 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* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.94 FD 0.97 GC 1.03 GG 1.00* ! HN 1.02 KP 0.91 LA 0.99 MA 1.03 ! MK 0.90 NL 1.07 NY 0.89 ON 0.87 ! OV 0.98 PT 0.98 SC 1.00* TC 1.00* ! TS 0.84 WF 1.02 WZ 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.96 FD 1.00* GC 1.15 GG 1.00* ! HN 0.92 KP 1.00* LA 1.04 MA 1.00 ! MK 1.00* NL 1.09 NY 0.98 ON 1.03 ! OV 1.03 PT 1.00* SC 1.00* TC 1.00* ! TS 1.20 WF 1.00* WZ 1.06 ! ! A total of 12 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.96 FD 0.97 GC 0.95 GG 1.00* ! HN 0.91 KP 0.93 LA 0.98 MA 1.07 ! MK 1.00* NL 1.09 NY 1.02 ON 0.87 ! OV 0.97 PT 0.98 SC 1.00* TC 1.00* ! TS 1.18 WF 1.10 WZ 0.87 ! ! A total of 9 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.95 FD 0.97 GC 1.07 GG 1.00* ! HN 0.93 KP 0.92 LA 0.97 MA 0.94 ! MK 0.89 NL 1.08 NY 0.94 ON 0.92 ! OV 0.97 PT 0.98 SC 1.00 TC 1.00* ! TS 1.03 WF 1.00 WZ 1.03 ! ! ! Correcting IF 2. ! A total of 24 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 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* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 FD 0.97 GC 1.08 GG 1.00* ! HN 1.03 KP 0.86 LA 0.98 MA 1.01 ! MK 0.90 NL 1.03 NY 0.92 ON 0.89 ! OV 0.98 PT 1.03 SC 1.00* TC 1.00* ! TS 0.84 WF 1.03 WZ 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 1.00* GC 1.21 GG 1.00* ! HN 0.93 KP 1.00* LA 1.04 MA 0.97 ! MK 1.00* NL 1.05 NY 1.02 ON 1.06 ! OV 1.03 PT 1.00* SC 1.00* TC 1.00* ! TS 1.20 WF 1.00* WZ 1.10 ! ! A total of 12 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 FD 0.96 GC 1.00 GG 1.00* ! HN 0.91 KP 0.88 LA 0.98 MA 1.05 ! MK 1.00* NL 1.05 NY 1.05 ON 0.88 ! OV 0.96 PT 1.02 SC 1.00* TC 1.00* ! TS 1.19 WF 1.12 WZ 0.91 ! ! A total of 9 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 FD 0.97 GC 1.12 GG 1.00* ! HN 0.94 KP 0.88 LA 0.97 MA 0.92 ! MK 0.90 NL 1.05 NY 0.97 ON 0.93 ! OV 0.96 PT 1.02 SC 0.97 TC 1.00* ! TS 1.04 WF 1.02 WZ 1.06 ! ! ! Correcting IF 3. ! A total of 24 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 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* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.97 GC 1.21 GG 1.00* ! HN 1.02 KP 0.80 LA 0.99 MA 1.13 ! MK 0.91 NL 1.01 NY 0.94 ON 1.11 ! OV 1.01 PT 1.06 SC 1.00* TC 1.00* ! TS 0.83 WF 1.10 WZ 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 1.00* GC 1.35 GG 1.00* ! HN 0.92 KP 1.00* LA 1.05 MA 1.07 ! MK 1.00* NL 1.03 NY 1.04 ON 1.32 ! OV 1.06 PT 1.00* SC 1.00* TC 1.00* ! TS 1.22 WF 1.00* WZ 1.13 ! ! A total of 12 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 FD 0.96 GC 1.10 GG 1.00* ! HN 0.91 KP 0.81 LA 0.98 MA 1.16 ! MK 1.00* NL 1.03 NY 1.08 ON 1.20 ! OV 1.00 PT 1.05 SC 1.00* TC 1.00* ! TS 1.18 WF 1.22 WZ 0.93 ! ! A total of 9 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 FD 0.96 GC 1.21 GG 1.00* ! HN 0.93 KP 0.82 LA 0.98 MA 0.95 ! MK 0.90 NL 1.04 NY 1.00 ON 1.23 ! OV 1.00 PT 1.05 SC 1.00 TC 1.00* ! TS 1.04 WF 1.10 WZ 1.07 ! ! ! Correcting IF 4. ! A total of 24 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 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* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 FD 0.96 GC 1.25 GG 1.00* ! HN 1.06 KP 0.86 LA 0.98 MA 1.16 ! MK 0.94 NL 1.02 NY 0.93 ON 1.12 ! OV 1.00 PT 1.06 SC 1.00* TC 1.00* ! TS 0.85 WF 1.08 WZ 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 1.00* GC 1.39 GG 1.00* ! HN 0.95 KP 1.00* LA 1.04 MA 1.12 ! MK 1.00* NL 1.04 NY 1.03 ON 1.43 ! OV 1.05 PT 1.00* SC 1.00* TC 1.00* ! TS 1.23 WF 1.00* WZ 1.15 ! ! A total of 12 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 FD 0.94 GC 1.13 GG 1.00* ! HN 0.93 KP 0.87 LA 0.97 MA 1.22 ! MK 1.00* NL 1.03 NY 1.06 ON 1.34 ! OV 0.99 PT 1.05 SC 1.00* TC 1.00* ! TS 1.19 WF 1.23 WZ 0.93 ! ! A total of 9 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.98 FD 0.95 GC 1.24 GG 1.00* ! HN 0.96 KP 0.88 LA 0.97 MA 1.01 ! MK 0.93 NL 1.04 NY 0.98 ON 1.39 ! OV 0.99 PT 1.05 SC 1.05 TC 1.00* ! TS 1.04 WF 1.09 WZ 1.07 ! ! ! Fit before self-cal, rms=0.568230Jy sigma=0.004155 ! Fit after self-cal, rms=0.376252Jy sigma=0.002571 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! Estimated beam: bmin=0.7135 mas, bmaj=0.7833 mas, bpa=4.819 degrees ! Estimated noise=379.626 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 = -0.0543158 Jy ! Component: 100 - total flux cleaned = -0.0629975 Jy ! Component: 150 - total flux cleaned = -0.069816 Jy ! Component: 200 - total flux cleaned = -0.073471 Jy ! Total flux subtracted in 200 components = -0.073471 Jy ! Clean residual min=-0.026917 max=0.028750 Jy/beam ! Clean residual mean=-0.001142 rms=0.004793 Jy/beam ! Combined flux in latest and established models = 3.93016 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 33 components and 3.93016 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.364405Jy sigma=0.002487 ! Fit after self-cal, rms=0.364204Jy sigma=0.002485 ! Inverting map ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 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=0.364204Jy sigma=0.002485 ! Fit after self-cal, rms=0.294737Jy sigma=0.001756 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! Estimated beam: bmin=0.7138 mas, bmaj=0.7882 mas, bpa=6.813 degrees ! Estimated noise=379.58 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0277776 Jy ! Component: 100 - total flux cleaned = -0.0341811 Jy ! Component: 150 - total flux cleaned = -0.0392713 Jy ! Component: 200 - total flux cleaned = -0.0429031 Jy ! Total flux subtracted in 200 components = -0.0429031 Jy ! Clean residual min=-0.013330 max=0.009347 Jy/beam ! Clean residual mean=-0.000913 rms=0.002171 Jy/beam ! Combined flux in latest and established models = 3.88726 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 34 components and 3.88726 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.289338Jy sigma=0.001720 ! Fit after self-cal, rms=0.288806Jy sigma=0.001716 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 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 = -0.0079538 Jy ! Component: 100 - total flux cleaned = -0.0106112 Jy ! Component: 150 - total flux cleaned = -0.0130634 Jy ! Component: 200 - total flux cleaned = -0.0148579 Jy ! Total flux subtracted in 200 components = -0.0148579 Jy ! Clean residual min=-0.009469 max=0.010518 Jy/beam ! Clean residual mean=-0.000838 rms=0.002114 Jy/beam ! Combined flux in latest and established models = 3.8724 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 34 components and 3.8724 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.287542Jy sigma=0.001710 ! Fit after self-cal, rms=0.287415Jy sigma=0.001709 ! Inverting map ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! Added new window around map position (-2.2, -0.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00871467 Jy ! Component: 100 - total flux cleaned = 0.00875007 Jy ! Component: 150 - total flux cleaned = 0.00877118 Jy ! Component: 200 - total flux cleaned = 0.00854761 Jy ! Total flux subtracted in 200 components = 0.00854761 Jy ! Clean residual min=-0.009408 max=0.008224 Jy/beam ! Clean residual mean=-0.000881 rms=0.002011 Jy/beam ! Combined flux in latest and established models = 3.88095 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 46 components and 3.88095 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.286734Jy sigma=0.001703 ! Fit after self-cal, rms=0.286637Jy sigma=0.001703 ! Inverting map ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 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=0.286637Jy sigma=0.001703 ! Fit after self-cal, rms=0.284620Jy sigma=0.001680 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! Estimated beam: bmin=0.7159 mas, bmaj=0.7899 mas, bpa=6.242 degrees ! Estimated noise=380.457 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0117613 Jy ! Component: 100 - total flux cleaned = -0.0160476 Jy ! Component: 150 - total flux cleaned = -0.019424 Jy ! Component: 200 - total flux cleaned = -0.0215062 Jy ! Total flux subtracted in 200 components = -0.0215062 Jy ! Clean residual min=-0.011580 max=0.007669 Jy/beam ! Clean residual mean=-0.000686 rms=0.001716 Jy/beam ! Combined flux in latest and established models = 3.85944 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 46 components and 3.85944 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.282491Jy sigma=0.001668 ! Fit after self-cal, rms=0.282398Jy sigma=0.001667 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 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 = -0.00348368 Jy ! Component: 100 - total flux cleaned = -0.00400923 Jy ! Component: 150 - total flux cleaned = -0.00469811 Jy ! Component: 200 - total flux cleaned = -0.00509953 Jy ! Total flux subtracted in 200 components = -0.00509953 Jy ! Clean residual min=-0.008559 max=0.007438 Jy/beam ! Clean residual mean=-0.000660 rms=0.001675 Jy/beam ! Combined flux in latest and established models = 3.85434 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 49 components and 3.85434 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.281807Jy sigma=0.001664 ! Fit after self-cal, rms=0.281780Jy sigma=0.001664 ! Inverting map ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 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=0.281780Jy sigma=0.001664 ! Fit after self-cal, rms=0.280995Jy sigma=0.001653 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! Estimated beam: bmin=2.287 mas, bmaj=2.563 mas, bpa=-65.8 degrees ! Estimated noise=537.099 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0137526 Jy ! Component: 100 - total flux cleaned = -0.0145011 Jy ! Component: 150 - total flux cleaned = -0.0146924 Jy ! Component: 200 - total flux cleaned = -0.0148125 Jy ! Total flux subtracted in 200 components = -0.0148125 Jy ! Clean residual min=-0.009280 max=0.007690 Jy/beam ! Clean residual mean=-0.001858 rms=0.002816 Jy/beam ! Combined flux in latest and established models = 3.83953 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 55 components and 3.83953 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.280443Jy sigma=0.001651 ! Fit after self-cal, rms=0.280391Jy sigma=0.001650 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 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 = -0.000289676 Jy ! Component: 100 - total flux cleaned = 5.68802e-06 Jy ! Component: 150 - total flux cleaned = -4.6616e-05 Jy ! Component: 200 - total flux cleaned = -9.69868e-05 Jy ! Total flux subtracted in 200 components = -9.69868e-05 Jy ! Clean residual min=-0.009504 max=0.007122 Jy/beam ! Clean residual mean=-0.001856 rms=0.002809 Jy/beam ! Combined flux in latest and established models = 3.83943 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 58 components and 3.83943 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.280339Jy sigma=0.001650 ! Fit after self-cal, rms=0.280330Jy sigma=0.001650 ! Inverting map ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 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 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! Estimated beam: bmin=0.7177 mas, bmaj=0.791 mas, bpa=5.964 degrees ! Estimated noise=381.178 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7177 x 0.791 at 5.964 degrees (North through East) ! Clean map min=-0.0066941 max=3.3508 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=0.280330Jy sigma=0.001650 ! Fit after self-cal, rms=0.223748Jy sigma=0.001194 ! Inverting map and beam ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! Estimated beam: bmin=0.7191 mas, bmaj=0.7917 mas, bpa=5.848 degrees ! Estimated noise=379.955 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0115248 Jy ! Component: 100 - total flux cleaned = -0.0143403 Jy ! Component: 150 - total flux cleaned = -0.017029 Jy ! Component: 200 - total flux cleaned = -0.0193356 Jy ! Total flux subtracted in 200 components = -0.0193356 Jy ! Clean residual min=-0.010222 max=0.004721 Jy/beam ! Clean residual mean=-0.000368 rms=0.001085 Jy/beam ! Combined flux in latest and established models = 3.8201 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 58 components and 3.8201 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.222410Jy sigma=0.001186 ! Fit after self-cal, rms=0.222399Jy sigma=0.001186 ! Inverting map ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00243382 Jy ! Component: 100 - total flux cleaned = -0.00406097 Jy ! Component: 150 - total flux cleaned = -0.00547403 Jy ! Component: 200 - total flux cleaned = -0.00609427 Jy ! Total flux subtracted in 200 components = -0.00609427 Jy ! Clean residual min=-0.007743 max=0.004814 Jy/beam ! Clean residual mean=-0.000338 rms=0.001065 Jy/beam ! Combined flux in latest and established models = 3.814 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 60 components and 3.814 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.222023Jy sigma=0.001184 ! Fit after self-cal, rms=0.222015Jy sigma=0.001184 ! Inverting map ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.222015Jy sigma=0.001184 ! Fit after self-cal, rms=0.221452Jy sigma=0.001177 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 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! Estimated beam: bmin=0.5556 mas, bmaj=0.6523 mas, bpa=-0.05708 degrees ! Estimated noise=735.423 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.51336 Jy ! Component: 100 - total flux cleaned = 3.07103 Jy ! Component: 150 - total flux cleaned = 3.29738 Jy ! Component: 200 - total flux cleaned = 3.44681 Jy ! Total flux subtracted in 200 components = 3.44681 Jy ! Clean residual min=-0.017052 max=0.080312 Jy/beam ! Clean residual mean=0.000168 rms=0.004378 Jy/beam ! Combined flux in latest and established models = 3.44681 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 12 model components to the UV plane model. ! The established model now contains 12 components and 3.44681 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! Estimated beam: bmin=0.7207 mas, bmaj=0.7929 mas, bpa=5.875 degrees ! Estimated noise=380.137 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 = 0.157479 Jy ! Component: 100 - total flux cleaned = 0.237209 Jy ! Component: 150 - total flux cleaned = 0.27974 Jy ! Component: 200 - total flux cleaned = 0.304067 Jy ! Total flux subtracted in 200 components = 0.304067 Jy ! Clean residual min=-0.005637 max=0.014860 Jy/beam ! Clean residual mean=-0.000026 rms=0.001500 Jy/beam ! Combined flux in latest and established models = 3.75087 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 26 components and 3.75087 Jy ! Inverting map ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! Added new window around map position (0, -0.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0161241 Jy ! Component: 100 - total flux cleaned = 0.0256288 Jy ! Component: 150 - total flux cleaned = 0.028011 Jy ! Component: 200 - total flux cleaned = 0.0298108 Jy ! Total flux subtracted in 200 components = 0.0298108 Jy ! Clean residual min=-0.004757 max=0.006393 Jy/beam ! Clean residual mean=-0.000174 rms=0.001102 Jy/beam ! Combined flux in latest and established models = 3.78068 Jy ! Adding 25 model components to the UV plane model. ! The established model now contains 40 components and 3.78068 Jy ! Inverting map ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! Added new window around map position (-1.2, -2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00335889 Jy ! Component: 100 - total flux cleaned = 0.0045949 Jy ! Component: 150 - total flux cleaned = 0.00572405 Jy ! Component: 200 - total flux cleaned = 0.00696762 Jy ! Total flux subtracted in 200 components = 0.00696762 Jy ! Clean residual min=-0.004746 max=0.005482 Jy/beam ! Clean residual mean=-0.000209 rms=0.001018 Jy/beam ! Combined flux in latest and established models = 3.78765 Jy ! Adding 25 model components to the UV plane model. ! The established model now contains 49 components and 3.78765 Jy ! Inverting map ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! Added new window around map position (1.4, 0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00179953 Jy ! Component: 100 - total flux cleaned = 0.00218316 Jy ! Component: 150 - total flux cleaned = 0.00271292 Jy ! Component: 200 - total flux cleaned = 0.00320937 Jy ! Total flux subtracted in 200 components = 0.00320937 Jy ! Clean residual min=-0.004603 max=0.004316 Jy/beam ! Clean residual mean=-0.000225 rms=0.000977 Jy/beam ! Combined flux in latest and established models = 3.79086 Jy ! Adding 29 model components to the UV plane model. ! The established model now contains 59 components and 3.79086 Jy ! Inverting map ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 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 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! Estimated beam: bmin=2.291 mas, bmaj=2.567 mas, bpa=-65.91 degrees ! Estimated noise=531.864 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00455592 Jy ! Component: 100 - total flux cleaned = 0.00509109 Jy ! Component: 150 - total flux cleaned = 0.00514939 Jy ! Component: 200 - total flux cleaned = 0.00520054 Jy ! Total flux subtracted in 200 components = 0.00520054 Jy ! Clean residual min=-0.005190 max=0.003702 Jy/beam ! Clean residual mean=-0.000852 rms=0.001396 Jy/beam ! Combined flux in latest and established models = 3.79606 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 = 8.88738e-05 Jy ! Component: 100 - total flux cleaned = 0.000168341 Jy ! Component: 150 - total flux cleaned = 0.000241574 Jy ! Component: 200 - total flux cleaned = 0.000273878 Jy ! Total flux subtracted in 200 components = 0.000273878 Jy ! Clean residual min=-0.005246 max=0.003667 Jy/beam ! Clean residual mean=-0.000857 rms=0.001386 Jy/beam ! Combined flux in latest and established models = 3.79633 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 85 components and 3.79633 Jy ! Inverting map ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! Estimated beam: bmin=0.7207 mas, bmaj=0.7929 mas, bpa=5.875 degrees ! Estimated noise=380.137 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000547711 Jy ! Component: 100 - total flux cleaned = -0.000268102 Jy ! Component: 150 - total flux cleaned = -0.000135265 Jy ! Component: 200 - total flux cleaned = -0.000138403 Jy ! Total flux subtracted in 200 components = -0.000138403 Jy ! Clean residual min=-0.004542 max=0.003936 Jy/beam ! Clean residual mean=-0.000251 rms=0.000933 Jy/beam ! Combined flux in latest and established models = 3.7962 Jy selfcal ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 90 components and 3.7962 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.220195Jy sigma=0.001171 ! Fit after self-cal, rms=0.220078Jy sigma=0.001170 wmodel J0102+5824_X_2003_07_09_pus_map.mod ! Writing 90 model components to file: J0102+5824_X_2003_07_09_pus_map.mod wobs J0102+5824_X_2003_07_09_pus_uvs.fits ! Writing UV FITS file: J0102+5824_X_2003_07_09_pus_uvs.fits wwins J0102+5824_X_2003_07_09_pus_map.win ! wwins: Wrote 6 windows to J0102+5824_X_2003_07_09_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 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000452086 Jy ! Component: 100 - total flux cleaned = -0.00145272 Jy ! Component: 150 - total flux cleaned = -0.00241139 Jy ! Component: 200 - total flux cleaned = -0.00320596 Jy ! Component: 250 - total flux cleaned = -0.00398171 Jy ! Component: 300 - total flux cleaned = -0.00467799 Jy ! Component: 350 - total flux cleaned = -0.00542257 Jy ! Component: 400 - total flux cleaned = -0.00609179 Jy ! Component: 450 - total flux cleaned = -0.00669112 Jy ! Component: 500 - total flux cleaned = -0.00740058 Jy ! Component: 550 - total flux cleaned = -0.00804265 Jy ! Component: 600 - total flux cleaned = -0.00850401 Jy ! Component: 650 - total flux cleaned = -0.00907467 Jy ! Component: 700 - total flux cleaned = -0.00958275 Jy ! Component: 750 - total flux cleaned = -0.0100299 Jy ! Component: 800 - total flux cleaned = -0.0104731 Jy ! Component: 850 - total flux cleaned = -0.0110221 Jy ! Component: 900 - total flux cleaned = -0.0114028 Jy ! Component: 950 - total flux cleaned = -0.0119966 Jy ! Component: 1000 - total flux cleaned = -0.0124776 Jy ! Component: 1050 - total flux cleaned = -0.0129556 Jy ! Component: 1100 - total flux cleaned = -0.0134821 Jy ! Component: 1150 - total flux cleaned = -0.0141084 Jy ! Component: 1200 - total flux cleaned = -0.0146259 Jy ! Component: 1250 - total flux cleaned = -0.0151393 Jy ! Component: 1300 - total flux cleaned = -0.0154964 Jy ! Component: 1350 - total flux cleaned = -0.0160534 Jy ! Component: 1400 - total flux cleaned = -0.0165055 Jy ! Component: 1450 - total flux cleaned = -0.0170048 Jy ! Component: 1500 - total flux cleaned = -0.0175007 Jy ! Component: 1550 - total flux cleaned = -0.017993 Jy ! Component: 1600 - total flux cleaned = -0.0185314 Jy ! Component: 1650 - total flux cleaned = -0.0188231 Jy ! Component: 1700 - total flux cleaned = -0.0193066 Jy ! Component: 1750 - total flux cleaned = -0.0198356 Jy ! Component: 1800 - total flux cleaned = -0.0201703 Jy ! Component: 1850 - total flux cleaned = -0.0205978 Jy ! Component: 1900 - total flux cleaned = -0.0208816 Jy ! Component: 1950 - total flux cleaned = -0.0213987 Jy ! Component: 2000 - total flux cleaned = -0.021726 Jy ! Total flux subtracted in 2048 components = -0.0221446 Jy ! Clean residual min=-0.002324 max=0.002373 Jy/beam ! Clean residual mean=-0.000142 rms=0.000802 Jy/beam ! Combined flux in latest and established models = 3.77405 Jy keep ! Adding 162 model components to the UV plane model. ! The established model now contains 249 components and 3.77405 Jy ![Exited script file: muppet] wmap "J0102+5824_X_2003_07_09_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7207 x 0.7929 at 5.875 degrees (North through East) ! Clean map min=-0.0047931 max=3.3543 Jy/beam ! Writing clean map to FITS file: J0102+5824_X_2003_07_09_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 3.35425 invert ! Inverting map ! Your choice of large map pixels excluded 1.48% of the data. ! The x-axis pixel size should ideally be below 0.1574 milli-arcsec ! The y-axis pixel size should ideally be below 0.1851 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000802093 device "J0102+5824_X_2003_07_09_pus\_map.eps/VPS" ! Attempting to open device: 'J0102+5824_X_2003_07_09_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.0717382 0.0717382 0.143476 0.286953 0.573906 1.14781 2.29562 4.59124 9.18249 18.365 36.73 73.4599 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0024 print "peak=",int(1000*peak_flux)/1000 ! peak= 3.354 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7207 x 0.7929 at 5.875 degrees (North through East) ! Clean map min=-0.0047931 max=3.3543 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. quit ! Quitting program ! Log file J0102+5824_X_2003_07_09_pus_uvs.log closed on Sat Apr 6 23:14:41 2013