! Started logfile: J2134-0153_X_2003_06_18_pus_uvs.log on Wed Jan 17 18:20:32 2007 obs J2134-0153_X_2003_06_18_pus_uva.fits ! Reading UV FITS file: J2134-0153_X_2003_06_18_pus_uva.fits ! AN table 1: 21 integrations on 153 of 153 possible baselines. ! AN table 2: 38 integrations on 153 of 153 possible baselines. ! AN table 3: 33 integrations on 153 of 153 possible baselines. ! AN table 4: 58 integrations on 153 of 153 possible baselines. ! AN table 5: Unused. ! AN table 6: 45 integrations on 153 of 153 possible baselines. ! AN table 7: 202 integrations on 153 of 153 possible baselines. ! AN table 8: Unused. ! AN table 9: 111 integrations on 153 of 153 possible baselines. ! Apparent sampling: 0.18585 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J2134-0153 ! ! There are 4 IFs, and a total of 4 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.40997e+09 8e+06 1 8e+06 ! 02 2 8.47997e+09 8e+06 1 8e+06 ! 03 3 8.79497e+09 8e+06 1 8e+06 ! 04 4 8.89997e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 2231 lines of history. ! ! Reading 57780 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 378 telescope corrections were flagged in sub-array 1. ! A total of 684 telescope corrections were flagged in sub-array 2. ! A total of 594 telescope corrections were flagged in sub-array 3. ! A total of 797 telescope corrections were flagged in sub-array 4. ! A total of 753 telescope corrections were flagged in sub-array 5. ! A total of 2710 telescope corrections were flagged in sub-array 6. ! A total of 1385 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 2. ! A total of 378 telescope corrections were flagged in sub-array 1. ! A total of 612 telescope corrections were flagged in sub-array 2. ! A total of 594 telescope corrections were flagged in sub-array 3. ! A total of 766 telescope corrections were flagged in sub-array 4. ! A total of 733 telescope corrections were flagged in sub-array 5. ! A total of 2710 telescope corrections were flagged in sub-array 6. ! A total of 1385 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 3. ! A total of 378 telescope corrections were flagged in sub-array 1. ! A total of 612 telescope corrections were flagged in sub-array 2. ! A total of 594 telescope corrections were flagged in sub-array 3. ! A total of 766 telescope corrections were flagged in sub-array 4. ! A total of 733 telescope corrections were flagged in sub-array 5. ! A total of 2710 telescope corrections were flagged in sub-array 6. ! A total of 1385 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 4. ! A total of 378 telescope corrections were flagged in sub-array 1. ! A total of 612 telescope corrections were flagged in sub-array 2. ! A total of 594 telescope corrections were flagged in sub-array 3. ! A total of 766 telescope corrections were flagged in sub-array 4. ! A total of 733 telescope corrections were flagged in sub-array 5. ! A total of 2710 telescope corrections were flagged in sub-array 6. ! A total of 1385 telescope corrections were flagged in sub-array 7. ! ! Fit before self-cal, rms=1.374996Jy sigma=0.018808 ! Fit after self-cal, rms=0.784078Jy sigma=0.010354 ! 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 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! Estimated beam: bmin=0.5909 mas, bmaj=1.82 mas, bpa=-3.361 degrees ! Estimated noise=628.784 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.864849 Jy ! Component: 100 - total flux cleaned = 1.24313 Jy ! Total flux subtracted in 100 components = 1.24313 Jy ! Clean residual min=-0.094106 max=0.291187 Jy/beam ! Clean residual mean=0.000461 rms=0.026919 Jy/beam ! Combined flux in latest and established models = 1.24313 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 8 components and 1.24313 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.585846Jy sigma=0.007859 ! Fit after self-cal, rms=0.576770Jy sigma=0.007801 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! Added new window around map position (0.8, -0.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.292649 Jy ! Component: 100 - total flux cleaned = 0.440427 Jy ! Total flux subtracted in 100 components = 0.440427 Jy ! Clean residual min=-0.042187 max=0.107632 Jy/beam ! Clean residual mean=0.000119 rms=0.012915 Jy/beam ! Combined flux in latest and established models = 1.68355 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 16 components and 1.68355 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.331310Jy sigma=0.004135 ! Fit after self-cal, rms=0.317082Jy sigma=0.004008 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.106807 Jy ! Component: 100 - total flux cleaned = 0.16502 Jy ! Total flux subtracted in 100 components = 0.16502 Jy ! Clean residual min=-0.028496 max=0.060181 Jy/beam ! Clean residual mean=-0.000008 rms=0.007799 Jy/beam ! Combined flux in latest and established models = 1.84857 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 20 components and 1.84857 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.254509Jy sigma=0.002959 ! Fit after self-cal, rms=0.251165Jy sigma=0.002927 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! Added new window around map position (1.4, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.058026 Jy ! Component: 100 - total flux cleaned = 0.092658 Jy ! Total flux subtracted in 100 components = 0.092658 Jy ! Clean residual min=-0.021912 max=0.035189 Jy/beam ! Clean residual mean=-0.000102 rms=0.005756 Jy/beam ! Combined flux in latest and established models = 1.94123 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 27 components and 1.94123 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.228853Jy sigma=0.002531 ! Fit after self-cal, rms=0.227123Jy sigma=0.002508 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! Added new window around map position (2.2, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0375995 Jy ! Component: 100 - total flux cleaned = 0.0593323 Jy ! Total flux subtracted in 100 components = 0.0593323 Jy ! Clean residual min=-0.017210 max=0.018847 Jy/beam ! Clean residual mean=-0.000175 rms=0.004637 Jy/beam ! Combined flux in latest and established models = 2.00056 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 33 components and 2.00056 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.218599Jy sigma=0.002354 ! Fit after self-cal, rms=0.217540Jy sigma=0.002339 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1829 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 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! Estimated beam: bmin=0.8238 mas, bmaj=2.441 mas, bpa=-5.093 degrees ! Estimated noise=339.785 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 = 0.0367393 Jy ! Component: 100 - total flux cleaned = 0.0568521 Jy ! Component: 150 - total flux cleaned = 0.0692448 Jy ! Component: 200 - total flux cleaned = 0.0734058 Jy ! Total flux subtracted in 200 components = 0.0734058 Jy ! Clean residual min=-0.013926 max=0.015494 Jy/beam ! Clean residual mean=-0.000492 rms=0.004103 Jy/beam ! Combined flux in latest and established models = 2.07397 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 47 components and 2.07397 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.212230Jy sigma=0.002229 ! Fit after self-cal, rms=0.211926Jy sigma=0.002225 ! Inverting map ! Your choice of large map pixels excluded 1.27% of the data. ! The x-axis pixel size should ideally be below 0.1829 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* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! 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* ! ! Telescope amplitude corrections in sub-array 3: ! 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 30 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.05 FD 0.98 GG 1.00* HN 0.99 ! KK 1.00* KP 1.03 LA 1.02 MA 1.00* ! MK 1.00* NL 1.07 ON 1.00* OV 1.01 ! PT 1.00 SC 0.96 TC 1.00* TS 1.00* ! WF 1.01 WZ 1.06 ! ! A total of 57 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* ON 0.00* OV 0.00* ! PT 0.00* SC 0.00* TC 0.00* TS 0.00* ! WF 0.00* WZ 0.00* ! ! A total of 102 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.97 FD 0.96 GG 1.00* HN 0.98 ! KK 1.03 KP 1.00 LA 0.97 MA 1.00* ! MK 1.01 NL 1.02 ON 1.00* OV 0.97 ! PT 0.96 SC 0.98 TC 1.00* TS 1.00* ! WF 0.93 WZ 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.01 FD 0.99 GG 1.00* HN 0.99 ! KK 1.02 KP 1.01 LA 1.01 MA 1.00* ! MK 1.02 NL 1.09 ON 1.00* OV 1.01 ! PT 0.99 SC 1.09 TC 1.00* TS 0.97 ! WF 1.11 WZ 1.00* ! ! ! Correcting IF 2. ! 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 72 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! 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* ! ! Telescope amplitude corrections in sub-array 3: ! 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 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.05 FD 0.97 GG 1.00* HN 1.00 ! KK 1.00* KP 0.98 LA 1.02 MA 1.12 ! MK 1.00* NL 1.05 ON 1.00* OV 1.00 ! PT 1.04 SC 0.93 TC 1.00* TS 1.00* ! WF 1.04 WZ 1.05 ! ! A total of 9 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 0.99 ! KK 1.00* KP 1.00* LA 1.00* MA 1.08 ! MK 1.00* NL 1.05 ON 1.27 OV 1.00* ! PT 1.00* SC 1.00* TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! A total of 102 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.99 FD 0.96 GG 1.00* HN 0.99 ! KK 1.03 KP 0.95 LA 0.97 MA 1.00* ! MK 1.01 NL 0.98 ON 1.00* OV 0.96 ! PT 1.01 SC 0.95 TC 1.00* TS 1.00* ! WF 0.95 WZ 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.02 FD 0.98 GG 1.00* HN 1.01 ! KK 1.01 KP 0.96 LA 1.01 MA 1.00* ! MK 1.02 NL 1.05 ON 1.00* OV 1.00 ! PT 1.04 SC 1.03 TC 1.00* TS 0.96 ! WF 1.13 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 72 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! 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* ! ! Telescope amplitude corrections in sub-array 3: ! 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 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.10 FD 0.97 GG 1.00* HN 0.98 ! KK 1.00* KP 1.03 LA 1.04 MA 1.27 ! MK 1.00* NL 1.02 ON 1.00* OV 1.05 ! PT 1.08 SC 0.96 TC 1.00* TS 1.00* ! WF 1.02 WZ 1.02 ! ! A total of 9 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 0.95 ! KK 1.00* KP 1.00* LA 1.00* MA 1.26 ! MK 1.00* NL 1.03 ON 1.02 OV 1.00* ! PT 1.00* SC 1.00* TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! A total of 102 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.03 FD 0.95 GG 1.00* HN 0.98 ! KK 1.09 KP 0.99 LA 0.98 MA 1.00* ! MK 1.01 NL 0.97 ON 1.00* OV 1.01 ! PT 1.04 SC 0.97 TC 1.00* TS 1.00* ! WF 0.93 WZ 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.07 FD 0.98 GG 1.00* HN 0.99 ! KK 1.09 KP 1.00 LA 1.02 MA 1.00* ! MK 1.03 NL 1.03 ON 1.00* OV 1.04 ! PT 1.07 SC 1.06 TC 1.00* TS 0.92 ! WF 1.08 WZ 1.00* ! ! ! Correcting IF 4. ! 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 72 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! 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* ! ! Telescope amplitude corrections in sub-array 3: ! 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 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.07 FD 0.96 GG 1.00* HN 1.01 ! KK 1.00* KP 0.98 LA 1.01 MA 1.25 ! MK 1.00* NL 1.03 ON 1.00* OV 1.04 ! PT 1.09 SC 1.01 TC 1.00* TS 1.00* ! WF 0.99 WZ 1.02 ! ! A total of 9 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 1.03 ! KK 1.00* KP 1.00* LA 1.00* MA 1.23 ! MK 1.00* NL 1.02 ON 1.24 OV 1.00* ! PT 1.00* SC 1.00* TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! A total of 102 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 FD 0.94 GG 1.00* HN 1.01 ! KK 1.05 KP 0.95 LA 0.96 MA 1.00* ! MK 1.04 NL 0.98 ON 1.00* OV 0.99 ! PT 1.04 SC 1.03 TC 1.00* TS 1.00* ! WF 0.90 WZ 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.03 FD 0.97 GG 1.00* HN 1.03 ! KK 1.02 KP 0.96 LA 1.00 MA 1.00* ! MK 1.06 NL 1.04 ON 1.00* OV 1.03 ! PT 1.08 SC 1.10 TC 1.00* TS 0.92 ! WF 1.07 WZ 1.00* ! ! ! Fit before self-cal, rms=0.211926Jy sigma=0.002225 ! Fit after self-cal, rms=0.194573Jy sigma=0.001919 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! Estimated beam: bmin=0.8352 mas, bmaj=2.429 mas, bpa=-5.069 degrees ! Estimated noise=342.752 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 = 0.00421761 Jy ! Component: 100 - total flux cleaned = 0.00446858 Jy ! Component: 150 - total flux cleaned = 0.00427748 Jy ! Component: 200 - total flux cleaned = 0.00412966 Jy ! Total flux subtracted in 200 components = 0.00412966 Jy ! Clean residual min=-0.008038 max=0.006574 Jy/beam ! Clean residual mean=0.000473 rms=0.001800 Jy/beam ! Combined flux in latest and established models = 2.0781 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 65 components and 2.0781 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.193834Jy sigma=0.001911 ! Fit after self-cal, rms=0.194042Jy sigma=0.001910 ! Inverting map ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 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=0.194042Jy sigma=0.001910 ! Fit after self-cal, rms=0.191489Jy sigma=0.001858 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! Estimated beam: bmin=0.8338 mas, bmaj=2.427 mas, bpa=-5.077 degrees ! Estimated noise=342.965 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0050364 Jy ! Component: 100 - total flux cleaned = 0.00519952 Jy ! Component: 150 - total flux cleaned = 0.00494312 Jy ! Component: 200 - total flux cleaned = 0.00494896 Jy ! Total flux subtracted in 200 components = 0.00494896 Jy ! Clean residual min=-0.007603 max=0.005768 Jy/beam ! Clean residual mean=0.000553 rms=0.001496 Jy/beam ! Combined flux in latest and established models = 2.08305 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 68 components and 2.08305 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.191070Jy sigma=0.001854 ! Fit after self-cal, rms=0.191002Jy sigma=0.001853 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 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 = 0.00110366 Jy ! Component: 100 - total flux cleaned = 0.000983849 Jy ! Component: 150 - total flux cleaned = 0.000782553 Jy ! Component: 200 - total flux cleaned = 0.000595861 Jy ! Total flux subtracted in 200 components = 0.000595861 Jy ! Clean residual min=-0.006645 max=0.005795 Jy/beam ! Clean residual mean=0.000543 rms=0.001448 Jy/beam ! Combined flux in latest and established models = 2.08364 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 73 components and 2.08364 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.190800Jy sigma=0.001852 ! Fit after self-cal, rms=0.190761Jy sigma=0.001851 ! Inverting map ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 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=0.190761Jy sigma=0.001851 ! Fit after self-cal, rms=0.187807Jy sigma=0.001808 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! Estimated beam: bmin=0.8327 mas, bmaj=2.423 mas, bpa=-5.092 degrees ! Estimated noise=342.458 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00301458 Jy ! Component: 100 - total flux cleaned = 0.00361247 Jy ! Component: 150 - total flux cleaned = 0.00380104 Jy ! Component: 200 - total flux cleaned = 0.00388446 Jy ! Total flux subtracted in 200 components = 0.00388446 Jy ! Clean residual min=-0.004525 max=0.003968 Jy/beam ! Clean residual mean=0.000490 rms=0.001039 Jy/beam ! Combined flux in latest and established models = 2.08753 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 80 components and 2.08753 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.187603Jy sigma=0.001806 ! Fit after self-cal, rms=0.187551Jy sigma=0.001805 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 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 = 0.000864846 Jy ! Component: 100 - total flux cleaned = 0.000953696 Jy ! Component: 150 - total flux cleaned = 0.000953674 Jy ! Component: 200 - total flux cleaned = 0.00102809 Jy ! Total flux subtracted in 200 components = 0.00102809 Jy ! Clean residual min=-0.004191 max=0.003947 Jy/beam ! Clean residual mean=0.000473 rms=0.001018 Jy/beam ! Combined flux in latest and established models = 2.08856 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 83 components and 2.08856 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.187429Jy sigma=0.001804 ! Fit after self-cal, rms=0.187407Jy sigma=0.001804 ! Inverting map ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 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=0.187407Jy sigma=0.001804 ! Fit after self-cal, rms=0.187335Jy sigma=0.001803 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! Estimated beam: bmin=2.254 mas, bmaj=3.778 mas, bpa=-9.285 degrees ! Estimated noise=417.977 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0029865 Jy ! Component: 100 - total flux cleaned = 0.00360031 Jy ! Component: 150 - total flux cleaned = 0.00375516 Jy ! Component: 200 - total flux cleaned = 0.00382632 Jy ! Total flux subtracted in 200 components = 0.00382632 Jy ! Clean residual min=-0.002871 max=0.004496 Jy/beam ! Clean residual mean=0.000875 rms=0.001275 Jy/beam ! Combined flux in latest and established models = 2.09238 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 92 components and 2.09238 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.187295Jy sigma=0.001803 ! Fit after self-cal, rms=0.187286Jy sigma=0.001803 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 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 = 0.000413049 Jy ! Component: 100 - total flux cleaned = 0.000484639 Jy ! Component: 150 - total flux cleaned = 0.000542067 Jy ! Component: 200 - total flux cleaned = 0.000566968 Jy ! Total flux subtracted in 200 components = 0.000566968 Jy ! Clean residual min=-0.002895 max=0.004508 Jy/beam ! Clean residual mean=0.000856 rms=0.001288 Jy/beam ! Combined flux in latest and established models = 2.09295 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 97 components and 2.09295 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.187283Jy sigma=0.001803 ! Fit after self-cal, rms=0.187268Jy sigma=0.001803 ! Inverting map ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 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 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! Estimated beam: bmin=0.833 mas, bmaj=2.422 mas, bpa=-5.093 degrees ! Estimated noise=342.548 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.833 x 2.422 at -5.093 degrees (North through East) ! Clean map min=-0.0031094 max=1.2277 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=0.187268Jy sigma=0.001803 ! Fit after self-cal, rms=0.178020Jy sigma=0.001591 ! Inverting map and beam ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! Estimated beam: bmin=0.832 mas, bmaj=2.422 mas, bpa=-5.11 degrees ! Estimated noise=342.275 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00100355 Jy ! Component: 100 - total flux cleaned = 0.0010926 Jy ! Component: 150 - total flux cleaned = 0.00109671 Jy ! Component: 200 - total flux cleaned = 0.00109905 Jy ! Total flux subtracted in 200 components = 0.00109905 Jy ! Clean residual min=-0.003127 max=0.003464 Jy/beam ! Clean residual mean=0.000452 rms=0.000940 Jy/beam ! Combined flux in latest and established models = 2.09405 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 99 components and 2.09405 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.177917Jy sigma=0.001589 ! Fit after self-cal, rms=0.177893Jy sigma=0.001589 ! Inverting map ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000341094 Jy ! Component: 100 - total flux cleaned = 0.000410903 Jy ! Component: 150 - total flux cleaned = 0.000410637 Jy ! Component: 200 - total flux cleaned = 0.000409169 Jy ! Total flux subtracted in 200 components = 0.000409169 Jy ! Clean residual min=-0.003070 max=0.003401 Jy/beam ! Clean residual mean=0.000445 rms=0.000929 Jy/beam ! Combined flux in latest and established models = 2.09446 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 101 components and 2.09446 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.177823Jy sigma=0.001588 ! Fit after self-cal, rms=0.177801Jy sigma=0.001588 ! Inverting map ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.177801Jy sigma=0.001588 ! Fit after self-cal, rms=0.178124Jy sigma=0.001588 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 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! Estimated beam: bmin=0.5922 mas, bmaj=1.815 mas, bpa=-3.061 degrees ! Estimated noise=638.471 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.905306 Jy ! Component: 100 - total flux cleaned = 1.33369 Jy ! Component: 150 - total flux cleaned = 1.5711 Jy ! Component: 200 - total flux cleaned = 1.71831 Jy ! Total flux subtracted in 200 components = 1.71831 Jy ! Clean residual min=-0.026212 max=0.077081 Jy/beam ! Clean residual mean=0.000318 rms=0.010094 Jy/beam ! Combined flux in latest and established models = 1.71831 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 16 model components to the UV plane model. ! The established model now contains 16 components and 1.71831 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! Estimated beam: bmin=0.8322 mas, bmaj=2.422 mas, bpa=-5.107 degrees ! Estimated noise=342.239 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 = 0.164774 Jy ! Component: 100 - total flux cleaned = 0.251594 Jy ! Component: 150 - total flux cleaned = 0.299221 Jy ! Component: 200 - total flux cleaned = 0.326834 Jy ! Total flux subtracted in 200 components = 0.326834 Jy ! Clean residual min=-0.004811 max=0.023295 Jy/beam ! Clean residual mean=0.001223 rms=0.002956 Jy/beam ! Combined flux in latest and established models = 2.04515 Jy ! Adding 40 model components to the UV plane model. ! The established model now contains 42 components and 2.04515 Jy ! Inverting map ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! Added new window around map position (-0.8, 0). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0209871 Jy ! Component: 100 - total flux cleaned = 0.0328064 Jy ! Component: 150 - total flux cleaned = 0.0404158 Jy ! Component: 200 - total flux cleaned = 0.0449396 Jy ! Total flux subtracted in 200 components = 0.0449396 Jy ! Clean residual min=-0.002988 max=0.003792 Jy/beam ! Clean residual mean=0.000519 rms=0.000958 Jy/beam ! Combined flux in latest and established models = 2.09008 Jy ! Adding 23 model components to the UV plane model. ! The established model now contains 62 components and 2.09008 Jy ! Inverting map ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 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 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! Estimated beam: bmin=2.252 mas, bmaj=3.777 mas, bpa=-9.299 degrees ! Estimated noise=418.03 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00380276 Jy ! Component: 100 - total flux cleaned = 0.00552957 Jy ! Component: 150 - total flux cleaned = 0.0058579 Jy ! Component: 200 - total flux cleaned = 0.00615018 Jy ! Total flux subtracted in 200 components = 0.00615018 Jy ! Clean residual min=-0.002695 max=0.003924 Jy/beam ! Clean residual mean=0.000888 rms=0.001219 Jy/beam ! Combined flux in latest and established models = 2.09623 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 = 9.0201e-05 Jy ! Component: 100 - total flux cleaned = 0.000140631 Jy ! Component: 150 - total flux cleaned = 0.000162761 Jy ! Component: 200 - total flux cleaned = 0.000142253 Jy ! Total flux subtracted in 200 components = 0.000142253 Jy ! Clean residual min=-0.002691 max=0.003909 Jy/beam ! Clean residual mean=0.000883 rms=0.001217 Jy/beam ! Combined flux in latest and established models = 2.09638 Jy ! Adding 45 model components to the UV plane model. ! The established model now contains 104 components and 2.09638 Jy ! Inverting map ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! Estimated beam: bmin=0.8322 mas, bmaj=2.422 mas, bpa=-5.107 degrees ! Estimated noise=342.239 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000814125 Jy ! Component: 100 - total flux cleaned = -0.000816705 Jy ! Component: 150 - total flux cleaned = -0.000712117 Jy ! Component: 200 - total flux cleaned = -0.000619315 Jy ! Total flux subtracted in 200 components = -0.000619315 Jy ! Clean residual min=-0.002501 max=0.003534 Jy/beam ! Clean residual mean=0.000426 rms=0.000871 Jy/beam ! Combined flux in latest and established models = 2.09576 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 115 components and 2.09576 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.178787Jy sigma=0.001589 ! Fit after self-cal, rms=0.177547Jy sigma=0.001582 wmodel J2134-0153_X_2003_06_18_pus_map.mod ! Writing 115 model components to file: J2134-0153_X_2003_06_18_pus_map.mod wobs J2134-0153_X_2003_06_18_pus_uvs.fits ! Writing UV FITS file: J2134-0153_X_2003_06_18_pus_uvs.fits wwins J2134-0153_X_2003_06_18_pus_map.win ! wwins: Wrote 5 windows to J2134-0153_X_2003_06_18_pus_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.00152018 Jy ! Component: 100 - total flux cleaned = 0.00289808 Jy ! Component: 150 - total flux cleaned = 0.00419325 Jy ! Component: 200 - total flux cleaned = 0.00541471 Jy ! Component: 250 - total flux cleaned = 0.00648214 Jy ! Component: 300 - total flux cleaned = 0.00724113 Jy ! Component: 350 - total flux cleaned = 0.00789044 Jy ! Component: 400 - total flux cleaned = 0.0085637 Jy ! Component: 450 - total flux cleaned = 0.0092603 Jy ! Component: 500 - total flux cleaned = 0.0098999 Jy ! Component: 550 - total flux cleaned = 0.0105652 Jy ! Component: 600 - total flux cleaned = 0.0112553 Jy ! Component: 650 - total flux cleaned = 0.0118941 Jy ! Component: 700 - total flux cleaned = 0.0124838 Jy ! Component: 750 - total flux cleaned = 0.0131354 Jy ! Component: 800 - total flux cleaned = 0.0136689 Jy ! Component: 850 - total flux cleaned = 0.0142641 Jy ! Component: 900 - total flux cleaned = 0.0148495 Jy ! Component: 950 - total flux cleaned = 0.0153918 Jy ! Component: 1000 - total flux cleaned = 0.0158593 Jy ! Total flux subtracted in 1024 components = 0.0161566 Jy ! Clean residual min=-0.001919 max=0.001937 Jy/beam ! Clean residual mean=0.000263 rms=0.000665 Jy/beam ! Combined flux in latest and established models = 2.11191 Jy keep ! Adding 59 model components to the UV plane model. ! The established model now contains 172 components and 2.11191 Jy wmap "J2134-0153_X_2003_06_18_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8322 x 2.422 at -5.107 degrees (North through East) ! Clean map min=-0.0029926 max=1.2234 Jy/beam ! Writing clean map to FITS file: J2134-0153_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 1.22336 invert ! Inverting map ! Your choice of large map pixels excluded 1.31% of the data. ! The x-axis pixel size should ideally be below 0.1829 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000662733 device "J2134-0153_X_2003_06_18_pus\_map.eps/VPS" ! Attempting to open device: 'J2134-0153_X_2003_06_18_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.16252 0.16252 0.32504 0.650081 1.30016 2.60032 5.20064 10.4013 20.8026 41.6052 83.2103 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0019 print "peak=",int(1000*peak_flux)/1000 ! peak= 1.223 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8322 x 2.422 at -5.107 degrees (North through East) ! Clean map min=-0.0029926 max=1.2234 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J2134-0153_X_2003_06_18_pus\_map.gif/vgif" ! Attempting to open device: 'J2134-0153_X_2003_06_18_pus_map.gif/vgif' mapplot cln quit ! Quitting program ! Log file J2134-0153_X_2003_06_18_pus_uvs.log closed on Wed Jan 17 18:22:32 2007