! Started logfile: J1924-2914_X_2003_05_07_pus_uvs.log on Thu Dec 14 17:13:04 2006 obs J1924-2914_X_2003_05_07_pus_uva.fits ! Reading UV FITS file: J1924-2914_X_2003_05_07_pus_uva.fits ! AN table 1: 148 integrations on 171 of 171 possible baselines. ! AN table 2: 88 integrations on 171 of 171 possible baselines. ! AN table 3: 74 integrations on 171 of 171 possible baselines. ! AN table 4: 140 integrations on 171 of 171 possible baselines. ! AN table 5: 167 integrations on 171 of 171 possible baselines. ! AN table 6: 24 integrations on 171 of 171 possible baselines. ! Apparent sampling: 0.0407258 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1924-2914 ! ! There are 4 IFs, and a total of 4 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.40997e+09 8e+06 1 8e+06 ! 02 2 8.47997e+09 8e+06 1 8e+06 ! 03 3 8.79497e+09 8e+06 1 8e+06 ! 04 4 8.89997e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 1739 lines of history. ! ! Reading 17856 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 2321 telescope corrections were flagged in sub-array 1. ! A total of 1401 telescope corrections were flagged in sub-array 2. ! A total of 1110 telescope corrections were flagged in sub-array 3. ! A total of 2093 telescope corrections were flagged in sub-array 4. ! A total of 2629 telescope corrections were flagged in sub-array 5. ! A total of 413 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 2321 telescope corrections were flagged in sub-array 1. ! A total of 1401 telescope corrections were flagged in sub-array 2. ! A total of 1110 telescope corrections were flagged in sub-array 3. ! A total of 2093 telescope corrections were flagged in sub-array 4. ! A total of 2629 telescope corrections were flagged in sub-array 5. ! A total of 413 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 2321 telescope corrections were flagged in sub-array 1. ! A total of 1401 telescope corrections were flagged in sub-array 2. ! A total of 1110 telescope corrections were flagged in sub-array 3. ! A total of 2093 telescope corrections were flagged in sub-array 4. ! A total of 2629 telescope corrections were flagged in sub-array 5. ! A total of 413 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 2321 telescope corrections were flagged in sub-array 1. ! A total of 1401 telescope corrections were flagged in sub-array 2. ! A total of 1110 telescope corrections were flagged in sub-array 3. ! A total of 2090 telescope corrections were flagged in sub-array 4. ! A total of 2629 telescope corrections were flagged in sub-array 5. ! A total of 413 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=4.613982Jy sigma=0.035475 ! Fit after self-cal, rms=4.241675Jy sigma=0.033712 ! 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 1.21% of the data. ! The x-axis pixel size should ideally be below 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.5963 mas, bmaj=0.8897 mas, bpa=-10.43 degrees ! Estimated noise=1785.76 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 = 3.89588 Jy ! Component: 100 - total flux cleaned = 4.91296 Jy ! Total flux subtracted in 100 components = 4.91296 Jy ! Clean residual min=-0.172693 max=0.381654 Jy/beam ! Clean residual mean=0.006316 rms=0.054150 Jy/beam ! Combined flux in latest and established models = 4.91296 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 4.91296 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.244239Jy sigma=0.010035 ! Fit after self-cal, rms=1.244825Jy sigma=0.010035 ! Inverting map ! Your choice of large map pixels excluded 1.21% of the data. ! The x-axis pixel size should ideally be below 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.397665 Jy ! Component: 100 - total flux cleaned = 0.588272 Jy ! Total flux subtracted in 100 components = 0.588272 Jy ! Clean residual min=-0.150232 max=0.208584 Jy/beam ! Clean residual mean=0.003732 rms=0.041672 Jy/beam ! Combined flux in latest and established models = 5.50124 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 14 components and 5.50124 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.095124Jy sigma=0.008023 ! Fit after self-cal, rms=1.095572Jy sigma=0.008023 ! Inverting map ! Your choice of large map pixels excluded 1.21% of the data. ! The x-axis pixel size should ideally be below 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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 1.21% of the data. ! The x-axis pixel size should ideally be below 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.8498 mas, bmaj=1.394 mas, bpa=-16.35 degrees ! Estimated noise=891.032 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 = 0.291068 Jy ! Component: 100 - total flux cleaned = 0.409965 Jy ! Component: 150 - total flux cleaned = 0.46098 Jy ! Component: 200 - total flux cleaned = 0.482953 Jy ! Total flux subtracted in 200 components = 0.482953 Jy ! Clean residual min=-0.197782 max=0.262321 Jy/beam ! Clean residual mean=-0.003663 rms=0.080230 Jy/beam ! Combined flux in latest and established models = 5.98419 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 22 components and 5.98419 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.083255Jy sigma=0.007202 ! Fit after self-cal, rms=1.083166Jy sigma=0.007201 ! Inverting map ! Your choice of large map pixels excluded 1.21% of the data. ! The x-axis pixel size should ideally be below 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 150 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.89 GG 1.00* HN 1.25 ! KK 1.02 KP 1.12 LA 0.94 MA 0.99 ! MC 1.09 MK 0.93 NL 1.08 ON 1.00* ! OV 0.98 PT 0.92 SC 0.97 TC 1.00 ! TS 1.00* WF 1.11 WZ 0.91 ! ! A total of 54 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 1.17 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MC 1.00* MK 1.00* NL 1.50 ON 1.00* ! OV 1.00* PT 1.00* SC 1.05 TC 0.88 ! 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 0.99 FD 0.88 GG 1.00* HN 1.35 ! KK 1.00* KP 1.06 LA 0.91 MA 1.00* ! MC 1.00* MK 0.96 NL 1.11 ON 1.00* ! OV 0.97 PT 0.88 SC 0.99 TC 1.00* ! TS 1.00* WF 1.16 WZ 1.00* ! ! A total of 117 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 0.89 GG 1.00* HN 1.21 ! KK 1.00* KP 1.00* LA 0.96 MA 1.00* ! MC 1.00* MK 1.00* NL 1.43 ON 1.00* ! OV 1.08 PT 0.88 SC 1.05 TC 0.97 ! TS 1.00* WF 1.06 WZ 1.00* ! ! A total of 327 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 1.00* GG 1.00* HN 1.00* ! KK 0.87 KP 1.00* LA 1.00* MA 0.99 ! MC 1.10 MK 0.88 NL 1.00* ON 1.00* ! OV 1.09 PT 1.00* SC 0.99 TC 0.99 ! TS 1.29 WF 1.00* WZ 1.04 ! ! A total of 3 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* FD 1.00* GG 1.00* HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.01 ! MC 1.18 MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.02 TC 1.41 ! TS 1.00* WF 1.00* WZ 1.00* ! ! ! Correcting IF 2. ! A total of 150 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.89 GG 1.00* HN 1.26 ! KK 1.00 KP 1.04 LA 0.95 MA 0.97 ! MC 1.07 MK 0.94 NL 1.03 ON 1.00* ! OV 0.97 PT 0.95 SC 0.93 TC 1.06 ! TS 1.00* WF 1.13 WZ 0.93 ! ! A total of 54 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 1.20 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MC 1.00* MK 1.00* NL 1.43 ON 1.00* ! OV 1.00* PT 1.00* SC 1.01 TC 0.92 ! TS 1.00* WF 1.00 WZ 1.00* ! ! A total of 39 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 0.88 GG 1.00* HN 1.36 ! KK 1.00* KP 1.00 LA 0.92 MA 1.00* ! MC 1.00* MK 0.96 NL 1.06 ON 1.00* ! OV 0.96 PT 0.92 SC 0.95 TC 1.00* ! TS 1.00* WF 1.18 WZ 1.00* ! ! A total of 117 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 0.89 GG 1.00* HN 1.25 ! KK 1.00* KP 1.00* LA 0.97 MA 1.00* ! MC 1.00* MK 1.00* NL 1.35 ON 1.00* ! OV 1.07 PT 0.91 SC 1.00 TC 1.01 ! TS 1.00* WF 1.08 WZ 1.00* ! ! A total of 327 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 1.00* GG 1.00* HN 1.00* ! KK 0.87 KP 1.00* LA 1.00* MA 0.98 ! MC 1.07 MK 0.88 NL 1.00* ON 1.00* ! OV 1.07 PT 1.00* SC 0.95 TC 1.10 ! TS 1.28 WF 1.00* WZ 1.06 ! ! A total of 3 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* FD 1.00* GG 1.00* HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 0.99 ! MC 1.13 MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00 TC 1.54 ! TS 1.00* WF 1.00* WZ 1.00* ! ! ! Correcting IF 3. ! A total of 150 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 FD 0.88 GG 1.00* HN 1.24 ! KK 1.05 KP 0.97 LA 0.96 MA 0.98 ! MC 1.10 MK 0.93 NL 0.99 ON 1.00* ! OV 0.99 PT 0.98 SC 0.93 TC 1.00 ! TS 1.00* WF 1.08 WZ 0.93 ! ! A total of 54 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 1.18 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MC 1.00* MK 1.00* NL 1.39 ON 1.00* ! OV 1.00* PT 1.00* SC 1.02 TC 0.87 ! TS 1.00* WF 0.93 WZ 1.00* ! ! A total of 39 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 FD 0.87 GG 1.00* HN 1.34 ! KK 1.00* KP 0.93 LA 0.92 MA 1.00* ! MC 1.00* MK 0.96 NL 1.02 ON 1.00* ! OV 0.99 PT 0.94 SC 0.95 TC 1.00* ! TS 1.00* WF 1.12 WZ 1.00* ! ! A total of 117 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 0.88 GG 1.00* HN 1.23 ! KK 1.00* KP 1.00* LA 0.97 MA 1.00* ! MC 1.00* MK 1.00* NL 1.31 ON 1.00* ! OV 1.11 PT 0.94 SC 1.01 TC 0.94 ! TS 1.00* WF 1.03 WZ 1.00* ! ! A total of 327 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 1.00* GG 1.00* HN 1.00* ! KK 0.93 KP 1.00* LA 1.00* MA 1.01 ! MC 1.25 MK 0.89 NL 1.00* ON 1.00* ! OV 1.10 PT 1.00* SC 0.93 TC 1.03 ! TS 1.26 WF 1.00* WZ 1.04 ! ! A total of 3 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* FD 1.00* GG 1.00* HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.03 ! MC 0.98 MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.03 TC 1.52 ! TS 1.00* WF 1.00* WZ 1.00* ! ! ! Correcting IF 4. ! A total of 150 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.86 GG 1.00* HN 1.28 ! KK 1.01 KP 1.04 LA 0.93 MA 1.03 ! MC 1.68 MK 0.95 NL 1.00 ON 1.00* ! OV 0.99 PT 0.98 SC 0.97 TC 1.03 ! TS 1.00* WF 1.08 WZ 0.95 ! ! A total of 54 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 1.24 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MC 1.00* MK 1.00* NL 1.39 ON 1.00* ! OV 1.00* PT 1.00* SC 1.08 TC 0.87 ! TS 1.00* WF 0.92 WZ 1.00* ! ! A total of 39 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 0.85 GG 1.00* HN 1.36 ! KK 1.00* KP 0.99 LA 0.90 MA 1.00* ! MC 1.00* MK 0.98 NL 1.03 ON 1.00* ! OV 0.98 PT 0.94 SC 1.00 TC 1.00* ! TS 1.00* WF 1.09 WZ 1.00* ! ! A total of 120 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 0.86 GG 1.00* HN 1.27 ! KK 1.00* KP 1.00* LA 0.95 MA 1.00* ! MC 1.00* MK 1.00* NL 1.33 ON 1.00* ! OV 1.10 PT 0.94 SC 1.05 TC 0.98 ! TS 1.00* WF 1.03 WZ 1.00* ! ! A total of 327 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 1.00* GG 1.00* HN 1.00* ! KK 0.88 KP 1.00* LA 1.00* MA 1.05 ! MC 1.76 MK 0.92 NL 1.00* ON 1.00* ! OV 1.09 PT 1.00* SC 0.96 TC 1.08 ! TS 1.26 WF 1.00* WZ 1.04 ! ! A total of 3 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* FD 1.00* GG 1.00* HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.05 ! MC 2.15 MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.08 TC 1.61 ! TS 1.00* WF 1.00* WZ 1.00* ! ! ! Fit before self-cal, rms=1.083166Jy sigma=0.007201 ! Fit after self-cal, rms=0.821553Jy sigma=0.004109 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 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.834 mas, bmaj=1.35 mas, bpa=-15.41 degrees ! Estimated noise=957.581 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 = 0.00335348 Jy ! Component: 100 - total flux cleaned = 0.00340619 Jy ! Component: 150 - total flux cleaned = 0.00384467 Jy ! Component: 200 - total flux cleaned = 0.00387865 Jy ! Total flux subtracted in 200 components = 0.00387865 Jy ! Clean residual min=-0.062293 max=0.215985 Jy/beam ! Clean residual mean=0.022782 rms=0.046422 Jy/beam ! Combined flux in latest and established models = 5.98807 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 23 components and 5.98807 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.820801Jy sigma=0.004101 ! Fit after self-cal, rms=0.822490Jy sigma=0.004099 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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=0.822490Jy sigma=0.004099 ! Fit after self-cal, rms=0.796217Jy sigma=0.003946 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 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.8325 mas, bmaj=1.353 mas, bpa=-15.66 degrees ! Estimated noise=958.06 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00756203 Jy ! Component: 100 - total flux cleaned = 0.00827787 Jy ! Component: 150 - total flux cleaned = 0.00829774 Jy ! Component: 200 - total flux cleaned = 0.0086257 Jy ! Total flux subtracted in 200 components = 0.0086257 Jy ! Clean residual min=-0.056202 max=0.211360 Jy/beam ! Clean residual mean=0.022163 rms=0.044118 Jy/beam ! Combined flux in latest and established models = 5.99669 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 24 components and 5.99669 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.795713Jy sigma=0.003943 ! Fit after self-cal, rms=0.795694Jy sigma=0.003943 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 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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 (3.4, 8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.211161 Jy ! Component: 100 - total flux cleaned = 0.325633 Jy ! Component: 150 - total flux cleaned = 0.380828 Jy ! Component: 200 - total flux cleaned = 0.399165 Jy ! Total flux subtracted in 200 components = 0.399165 Jy ! Clean residual min=-0.058082 max=0.122202 Jy/beam ! Clean residual mean=0.012251 rms=0.023019 Jy/beam ! Combined flux in latest and established models = 6.39586 Jy ! Performing phase self-cal ! Adding 35 model components to the UV plane model. ! The established model now contains 58 components and 6.39586 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.745663Jy sigma=0.003211 ! Fit after self-cal, rms=0.734136Jy sigma=0.003082 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Added new window around map position (1, 6.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.123093 Jy ! Component: 100 - total flux cleaned = 0.157615 Jy ! Component: 150 - total flux cleaned = 0.173834 Jy ! Component: 200 - total flux cleaned = 0.185279 Jy ! Total flux subtracted in 200 components = 0.185279 Jy ! Clean residual min=-0.054096 max=0.074883 Jy/beam ! Clean residual mean=0.006535 rms=0.018257 Jy/beam ! Combined flux in latest and established models = 6.58114 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 76 components and 6.58114 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.712454Jy sigma=0.002787 ! Fit after self-cal, rms=0.707225Jy sigma=0.002736 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Added new window around map position (3.4, 1.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0723136 Jy ! Component: 100 - total flux cleaned = 0.0900743 Jy ! Component: 150 - total flux cleaned = 0.098635 Jy ! Component: 200 - total flux cleaned = 0.107341 Jy ! Total flux subtracted in 200 components = 0.107341 Jy ! Clean residual min=-0.050292 max=0.050021 Jy/beam ! Clean residual mean=0.002942 rms=0.015464 Jy/beam ! Combined flux in latest and established models = 6.68848 Jy ! Performing phase self-cal ! Adding 37 model components to the UV plane model. ! The established model now contains 99 components and 6.68848 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.697077Jy sigma=0.002617 ! Fit after self-cal, rms=0.694946Jy sigma=0.002599 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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=0.694946Jy sigma=0.002599 ! Fit after self-cal, rms=0.654032Jy sigma=0.002068 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 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.8314 mas, bmaj=1.356 mas, bpa=-15.42 degrees ! Estimated noise=958.395 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.071782 Jy ! Component: 100 - total flux cleaned = 0.118978 Jy ! Component: 150 - total flux cleaned = 0.149846 Jy ! Component: 200 - total flux cleaned = 0.165319 Jy ! Total flux subtracted in 200 components = 0.165319 Jy ! Clean residual min=-0.027031 max=0.045400 Jy/beam ! Clean residual mean=0.004366 rms=0.010454 Jy/beam ! Combined flux in latest and established models = 6.8538 Jy selfcal ! Performing phase self-cal ! Adding 36 model components to the UV plane model. ! The established model now contains 123 components and 6.8538 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.643808Jy sigma=0.001898 ! Fit after self-cal, rms=0.642197Jy sigma=0.001875 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 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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 = 0.0263885 Jy ! Component: 100 - total flux cleaned = 0.0354625 Jy ! Component: 150 - total flux cleaned = 0.040619 Jy ! Component: 200 - total flux cleaned = 0.0450571 Jy ! Total flux subtracted in 200 components = 0.0450571 Jy ! Clean residual min=-0.029106 max=0.038992 Jy/beam ! Clean residual mean=0.003000 rms=0.009528 Jy/beam ! Combined flux in latest and established models = 6.89885 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 127 components and 6.89885 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.639251Jy sigma=0.001832 ! Fit after self-cal, rms=0.638820Jy sigma=0.001827 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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=0.638820Jy sigma=0.001827 ! Fit after self-cal, rms=0.636852Jy sigma=0.001776 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 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=2.416 mas, bmaj=4.857 mas, bpa=-3.633 degrees ! Estimated noise=1096.73 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.064142 Jy ! Component: 100 - total flux cleaned = 0.0974183 Jy ! Component: 150 - total flux cleaned = 0.102636 Jy ! Component: 200 - total flux cleaned = 0.104714 Jy ! Total flux subtracted in 200 components = 0.104714 Jy ! Clean residual min=-0.027263 max=0.045506 Jy/beam ! Clean residual mean=0.006364 rms=0.012772 Jy/beam ! Combined flux in latest and established models = 7.00357 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 134 components and 7.00357 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.634966Jy sigma=0.001743 ! Fit after self-cal, rms=0.633957Jy sigma=0.001730 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 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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 = 0.0142534 Jy ! Component: 100 - total flux cleaned = 0.0183346 Jy ! Component: 150 - total flux cleaned = 0.0199988 Jy ! Component: 200 - total flux cleaned = 0.0195103 Jy ! Total flux subtracted in 200 components = 0.0195103 Jy ! Clean residual min=-0.031784 max=0.042870 Jy/beam ! Clean residual mean=0.004993 rms=0.012663 Jy/beam ! Combined flux in latest and established models = 7.02308 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 140 components and 7.02308 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.633875Jy sigma=0.001727 ! Fit after self-cal, rms=0.633619Jy sigma=0.001725 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.8313 mas, bmaj=1.355 mas, bpa=-15.35 degrees ! Estimated noise=958.933 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8313 x 1.355 at -15.35 degrees (North through East) ! Clean map min=-0.041285 max=5.2845 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=0.633619Jy sigma=0.001725 ! Fit after self-cal, rms=1.107396Jy sigma=0.001403 ! 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 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.8308 mas, bmaj=1.357 mas, bpa=-15.32 degrees ! Estimated noise=959.041 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0128473 Jy ! Component: 100 - total flux cleaned = 0.0158614 Jy ! Component: 150 - total flux cleaned = 0.0171802 Jy ! Component: 200 - total flux cleaned = 0.0188881 Jy ! Total flux subtracted in 200 components = 0.0188881 Jy ! Clean residual min=-0.025376 max=0.033823 Jy/beam ! Clean residual mean=0.002110 rms=0.007836 Jy/beam ! Combined flux in latest and established models = 7.04197 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 154 components and 7.04197 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.106510Jy sigma=0.001369 ! Fit after self-cal, rms=1.106442Jy sigma=0.001365 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Added new window around map position (6.4, 4.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0331625 Jy ! Component: 100 - total flux cleaned = 0.0402185 Jy ! Component: 150 - total flux cleaned = 0.0433811 Jy ! Component: 200 - total flux cleaned = 0.0439103 Jy ! Total flux subtracted in 200 components = 0.0439103 Jy ! Clean residual min=-0.022235 max=0.019185 Jy/beam ! Clean residual mean=0.000914 rms=0.006256 Jy/beam ! Combined flux in latest and established models = 7.08588 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 173 components and 7.08588 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.105316Jy sigma=0.001315 ! Fit after self-cal, rms=1.104956Jy sigma=0.001311 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.104956Jy sigma=0.001311 ! Fit after self-cal, rms=1.134584Jy sigma=0.001301 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 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.6048 mas, bmaj=0.9058 mas, bpa=-7.655 degrees ! Estimated noise=1875.75 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 3.91637 Jy ! Component: 100 - total flux cleaned = 4.90328 Jy ! Component: 150 - total flux cleaned = 5.26967 Jy ! Component: 200 - total flux cleaned = 5.47659 Jy ! Total flux subtracted in 200 components = 5.47659 Jy ! Clean residual min=-0.061736 max=0.114636 Jy/beam ! Clean residual mean=0.004898 rms=0.025704 Jy/beam ! Combined flux in latest and established models = 5.47659 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 22 model components to the UV plane model. ! The established model now contains 22 components and 5.47659 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 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.831 mas, bmaj=1.357 mas, bpa=-15.3 degrees ! Estimated noise=959.568 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 = 0.440668 Jy ! Component: 100 - total flux cleaned = 0.725342 Jy ! Component: 150 - total flux cleaned = 0.925605 Jy ! Component: 200 - total flux cleaned = 1.07274 Jy ! Total flux subtracted in 200 components = 1.07274 Jy ! Clean residual min=-0.034695 max=0.105665 Jy/beam ! Clean residual mean=0.017992 rms=0.027307 Jy/beam ! Combined flux in latest and established models = 6.54932 Jy ! Adding 81 model components to the UV plane model. ! The established model now contains 92 components and 6.54932 Jy ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=2.413 mas, bmaj=4.85 mas, bpa=-3.628 degrees ! Estimated noise=1098.55 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.197205 Jy ! Component: 100 - total flux cleaned = 0.317659 Jy ! Component: 150 - total flux cleaned = 0.396017 Jy ! Component: 200 - total flux cleaned = 0.447962 Jy ! Total flux subtracted in 200 components = 0.447962 Jy ! Clean residual min=-0.021274 max=0.038836 Jy/beam ! Clean residual mean=0.009484 rms=0.011699 Jy/beam ! Combined flux in latest and established models = 6.99728 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 = 0.0356442 Jy ! Component: 100 - total flux cleaned = 0.0562942 Jy ! Component: 150 - total flux cleaned = 0.0653841 Jy ! Component: 200 - total flux cleaned = 0.0724449 Jy ! Total flux subtracted in 200 components = 0.0724449 Jy ! Clean residual min=-0.020527 max=0.031113 Jy/beam ! Clean residual mean=0.005048 rms=0.008082 Jy/beam ! Combined flux in latest and established models = 7.06973 Jy ! Adding 69 model components to the UV plane model. ! The established model now contains 148 components and 7.06973 Jy ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.831 mas, bmaj=1.357 mas, bpa=-15.3 degrees ! Estimated noise=959.568 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00373498 Jy ! Component: 100 - total flux cleaned = 0.00761813 Jy ! Component: 150 - total flux cleaned = 0.0110446 Jy ! Component: 200 - total flux cleaned = 0.0118348 Jy ! Total flux subtracted in 200 components = 0.0118348 Jy ! Clean residual min=-0.021370 max=0.028958 Jy/beam ! Clean residual mean=0.002110 rms=0.006817 Jy/beam ! Combined flux in latest and established models = 7.08156 Jy selfcal ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 169 components and 7.08156 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.135116Jy sigma=0.001341 ! Fit after self-cal, rms=1.133581Jy sigma=0.001303 wmodel J1924-2914_X_2003_05_07_pus_map.mod ! Writing 169 model components to file: J1924-2914_X_2003_05_07_pus_map.mod wobs J1924-2914_X_2003_05_07_pus_uvs.fits ! Writing UV FITS file: J1924-2914_X_2003_05_07_pus_uvs.fits wwins J1924-2914_X_2003_05_07_pus_map.win ! wwins: Wrote 5 windows to J1924-2914_X_2003_05_07_pus_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.0105697 Jy ! Component: 100 - total flux cleaned = 0.0160012 Jy ! Component: 150 - total flux cleaned = 0.0213997 Jy ! Component: 200 - total flux cleaned = 0.0247989 Jy ! Component: 250 - total flux cleaned = 0.0277243 Jy ! Component: 300 - total flux cleaned = 0.0302302 Jy ! Component: 350 - total flux cleaned = 0.0323462 Jy ! Component: 400 - total flux cleaned = 0.0338174 Jy ! Component: 450 - total flux cleaned = 0.0352513 Jy ! Component: 500 - total flux cleaned = 0.0366536 Jy ! Component: 550 - total flux cleaned = 0.0380254 Jy ! Component: 600 - total flux cleaned = 0.0393679 Jy ! Component: 650 - total flux cleaned = 0.0406795 Jy ! Component: 700 - total flux cleaned = 0.0417103 Jy ! Component: 750 - total flux cleaned = 0.0432249 Jy ! Component: 800 - total flux cleaned = 0.0442148 Jy ! Component: 850 - total flux cleaned = 0.04519 Jy ! Component: 900 - total flux cleaned = 0.0461464 Jy ! Component: 950 - total flux cleaned = 0.0468532 Jy ! Component: 1000 - total flux cleaned = 0.047551 Jy ! Total flux subtracted in 1024 components = 0.0480091 Jy ! Clean residual min=-0.011397 max=0.013032 Jy/beam ! Clean residual mean=0.000688 rms=0.004471 Jy/beam ! Combined flux in latest and established models = 7.12957 Jy keep ! Adding 67 model components to the UV plane model. ! The established model now contains 229 components and 7.12957 Jy wmap "J1924-2914_X_2003_05_07_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 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.831 x 1.357 at -15.3 degrees (North through East) ! Clean map min=-0.029905 max=5.2464 Jy/beam ! Writing clean map to FITS file: J1924-2914_X_2003_05_07_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 5.24643 invert ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1828 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00448106 device "J1924-2914_X_2003_05_07_pus\_map.eps/VPS" ! Attempting to open device: 'J1924-2914_X_2003_05_07_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.256235 0.256235 0.51247 1.02494 2.04988 4.09976 8.19952 16.399 32.7981 65.5961 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0134 print "peak=",int(1000*peak_flux)/1000 ! peak= 5.246 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.831 x 1.357 at -15.3 degrees (North through East) ! Clean map min=-0.029905 max=5.2464 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1924-2914_X_2003_05_07_pus\_map.gif/vgif" ! Attempting to open device: 'J1924-2914_X_2003_05_07_pus_map.gif/vgif' mapplot cln quit ! Quitting program ! Log file J1924-2914_X_2003_05_07_pus_uvs.log closed on Thu Dec 14 17:15:33 2006