! Started logfile: J2236+2828_X_2003_06_18_pus_uvs.log on Wed Jan 17 18:31:04 2007 obs J2236+2828_X_2003_06_18_pus_uva.fits ! Reading UV FITS file: J2236+2828_X_2003_06_18_pus_uva.fits ! AN table 1: 206 integrations on 153 of 153 possible baselines. ! AN table 2: 107 integrations on 153 of 153 possible baselines. ! AN table 3: 97 integrations on 153 of 153 possible baselines. ! AN table 4: 73 integrations on 153 of 153 possible baselines. ! AN table 5: 90 integrations on 153 of 153 possible baselines. ! AN table 6: 12 integrations on 153 of 153 possible baselines. ! AN table 7: 94 integrations on 153 of 153 possible baselines. ! AN table 8: Unused. ! AN table 9: Unused. ! Apparent sampling: 0.113007 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J2236+2828 ! ! 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 46960 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 3105 telescope corrections were flagged in sub-array 1. ! A total of 1926 telescope corrections were flagged in sub-array 2. ! A total of 1238 telescope corrections were flagged in sub-array 3. ! A total of 935 telescope corrections were flagged in sub-array 4. ! A total of 1405 telescope corrections were flagged in sub-array 5. ! A total of 216 telescope corrections were flagged in sub-array 6. ! A total of 1692 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 2. ! A total of 3015 telescope corrections were flagged in sub-array 1. ! A total of 1869 telescope corrections were flagged in sub-array 2. ! A total of 1238 telescope corrections were flagged in sub-array 3. ! A total of 936 telescope corrections were flagged in sub-array 4. ! A total of 1405 telescope corrections were flagged in sub-array 5. ! A total of 216 telescope corrections were flagged in sub-array 6. ! A total of 1692 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 3. ! A total of 3023 telescope corrections were flagged in sub-array 1. ! A total of 1869 telescope corrections were flagged in sub-array 2. ! A total of 1238 telescope corrections were flagged in sub-array 3. ! A total of 936 telescope corrections were flagged in sub-array 4. ! A total of 1405 telescope corrections were flagged in sub-array 5. ! A total of 216 telescope corrections were flagged in sub-array 6. ! A total of 1692 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 4. ! A total of 3015 telescope corrections were flagged in sub-array 1. ! A total of 1869 telescope corrections were flagged in sub-array 2. ! A total of 1238 telescope corrections were flagged in sub-array 3. ! A total of 936 telescope corrections were flagged in sub-array 4. ! A total of 1405 telescope corrections were flagged in sub-array 5. ! A total of 216 telescope corrections were flagged in sub-array 6. ! A total of 1692 telescope corrections were flagged in sub-array 7. ! ! Fit before self-cal, rms=0.967009Jy sigma=0.011483 ! Fit after self-cal, rms=0.437251Jy sigma=0.003458 ! 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 0.139% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.663 mas, bmaj=1.195 mas, bpa=2.398 degrees ! Estimated noise=663.671 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 = 0.641177 Jy ! Component: 100 - total flux cleaned = 0.845245 Jy ! Total flux subtracted in 100 components = 0.845245 Jy ! Clean residual min=-0.022468 max=0.084286 Jy/beam ! Clean residual mean=0.000293 rms=0.009068 Jy/beam ! Combined flux in latest and established models = 0.845245 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.845245 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.407644Jy sigma=0.003248 ! Fit after self-cal, rms=0.406478Jy sigma=0.003233 ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0921426 Jy ! Component: 100 - total flux cleaned = 0.142859 Jy ! Total flux subtracted in 100 components = 0.142859 Jy ! Clean residual min=-0.017108 max=0.028900 Jy/beam ! Clean residual mean=0.000088 rms=0.005288 Jy/beam ! Combined flux in latest and established models = 0.988104 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 17 components and 0.988104 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.375432Jy sigma=0.002301 ! Fit after self-cal, rms=0.375049Jy sigma=0.002295 ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Added new window around map position (-0.6, -0.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0344606 Jy ! Component: 100 - total flux cleaned = 0.0544274 Jy ! Total flux subtracted in 100 components = 0.0544274 Jy ! Clean residual min=-0.014333 max=0.021367 Jy/beam ! Clean residual mean=0.000013 rms=0.004417 Jy/beam ! Combined flux in latest and established models = 1.04253 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 23 components and 1.04253 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.370634Jy sigma=0.002125 ! Fit after self-cal, rms=0.370466Jy sigma=0.002122 ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.199 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 0.139% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.9501 mas, bmaj=1.66 mas, bpa=-2.655 degrees ! Estimated noise=384.664 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 = 0.0241586 Jy ! Component: 100 - total flux cleaned = 0.0359362 Jy ! Component: 150 - total flux cleaned = 0.0418446 Jy ! Component: 200 - total flux cleaned = 0.04467 Jy ! Total flux subtracted in 200 components = 0.04467 Jy ! Clean residual min=-0.012849 max=0.015256 Jy/beam ! Clean residual mean=-0.000511 rms=0.004428 Jy/beam ! Combined flux in latest and established models = 1.0872 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 30 components and 1.0872 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.369399Jy sigma=0.002070 ! Fit after self-cal, rms=0.369457Jy sigma=0.002067 ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 90 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.98 GG 1.00* HN 0.96 ! KK 0.98 KP 0.97 LA 1.00 MA 1.00* ! MK 0.98 NL 1.05 ON 1.03 OV 0.93 ! PT 1.01 SC 0.90 TC 1.00* TS 1.00 ! WF 0.90 WZ 1.00* ! ! 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* ! ! A total of 42 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.96 FD 0.97 GG 1.00* HN 1.17 ! KK 1.00* KP 1.03 LA 0.97 MA 1.00* ! MK 1.00* NL 1.04 ON 1.00* OV 0.96 ! PT 1.00 SC 0.89 TC 1.00* TS 1.00* ! WF 1.05 WZ 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.94 FD 0.93 GG 1.00* HN 1.00* ! KK 1.17 KP 1.02 LA 0.92 MA 1.00* ! MK 1.02 NL 0.98 ON 1.00* OV 0.98 ! PT 0.98 SC 0.98 TC 1.00* TS 0.89 ! WF 1.00* WZ 1.00* ! ! A total of 75 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.95 FD 0.96 GG 1.00* HN 0.94 ! KK 1.00* KP 1.00* LA 0.97 MA 1.00* ! MK 1.00* NL 1.05 ON 1.00* OV 0.98 ! PT 0.96 SC 0.97 TC 1.00* TS 1.00* ! WF 0.94 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* ON 0.00* OV 0.00* ! PT 0.00* SC 0.00* TC 0.00* TS 0.00* ! WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! 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* ! ! ! Correcting IF 2. ! A total of 105 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.98 GG 1.00* HN 0.99 ! KK 0.98 KP 0.93 LA 1.00 MA 1.02 ! MK 0.98 NL 1.01 ON 1.04 OV 0.92 ! PT 1.05 SC 0.90 TC 1.00* TS 0.96 ! WF 0.98 WZ 1.00* ! ! A total of 57 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* ! ! A total of 42 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.96 FD 0.97 GG 1.00* HN 1.18 ! KK 1.00* KP 0.98 LA 0.98 MA 1.00* ! MK 1.00* NL 1.01 ON 1.00* OV 0.96 ! PT 1.03 SC 0.84 TC 1.00* TS 1.00* ! WF 1.14 WZ 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.96 FD 0.94 GG 1.00* HN 1.00* ! KK 1.16 KP 0.96 LA 0.92 MA 1.00* ! MK 1.04 NL 0.93 ON 1.00* OV 0.96 ! PT 1.03 SC 0.87 TC 1.00* TS 0.93 ! WF 1.00* WZ 1.00* ! ! A total of 75 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.95 FD 0.96 GG 1.00* HN 0.95 ! KK 1.00* KP 1.00* LA 0.97 MA 1.00* ! MK 1.00* NL 1.04 ON 1.00* OV 0.95 ! PT 1.02 SC 0.90 TC 1.00* TS 1.00* ! WF 0.93 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* ON 0.00* OV 0.00* ! PT 0.00* SC 0.00* TC 0.00* TS 0.00* ! WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! 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* ! ! ! Correcting IF 3. ! A total of 105 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 FD 0.99 GG 1.00* HN 0.96 ! KK 1.06 KP 0.97 LA 1.03 MA 0.95 ! MK 1.01 NL 1.00 ON 1.02 OV 0.96 ! PT 1.10 SC 0.96 TC 1.00* TS 0.98 ! WF 1.00* WZ 1.00* ! ! A total of 57 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* ! ! A total of 42 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 FD 0.96 GG 1.00* HN 1.16 ! KK 1.00* KP 1.03 LA 1.00 MA 1.00* ! MK 1.00* NL 0.99 ON 1.00* OV 1.01 ! PT 1.07 SC 0.90 TC 1.00* TS 1.00* ! WF 1.03 WZ 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 0.92 GG 1.00* HN 1.00* ! KK 1.24 KP 1.02 LA 0.94 MA 1.00* ! MK 1.06 NL 0.94 ON 1.00* OV 1.01 ! PT 1.06 SC 0.92 TC 1.00* TS 0.93 ! WF 1.00* WZ 1.00* ! ! A total of 75 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 FD 0.95 GG 1.00* HN 0.95 ! KK 1.00* KP 1.00* LA 0.99 MA 1.00* ! MK 1.00* NL 1.04 ON 1.00* OV 1.01 ! PT 1.05 SC 0.96 TC 1.00* TS 1.00* ! WF 0.93 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* ON 0.00* OV 0.00* ! PT 0.00* SC 0.00* TC 0.00* TS 0.00* ! WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! 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* ! ! ! Correcting IF 4. ! A total of 105 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.98 GG 1.00* HN 1.02 ! KK 1.04 KP 0.94 LA 1.01 MA 1.07 ! MK 1.03 NL 1.01 ON 1.03 OV 0.97 ! PT 1.11 SC 1.01 TC 1.00* TS 1.01 ! WF 1.17 WZ 1.00* ! ! A total of 57 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* ! ! A total of 42 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 0.96 GG 1.00* HN 1.20 ! KK 1.00* KP 0.99 LA 0.98 MA 1.00* ! MK 1.00* NL 1.01 ON 1.00* OV 1.01 ! PT 1.08 SC 0.97 TC 1.00* TS 1.00* ! WF 0.98 WZ 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 FD 0.92 GG 1.00* HN 1.00* ! KK 1.20 KP 0.97 LA 0.93 MA 1.00* ! MK 1.09 NL 0.96 ON 1.00* OV 1.01 ! PT 1.07 SC 0.99 TC 1.00* TS 0.99 ! WF 1.00* WZ 1.00* ! ! A total of 75 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.96 FD 0.94 GG 1.00* HN 1.02 ! KK 1.00* KP 1.00* LA 0.97 MA 1.00* ! MK 1.00* NL 1.03 ON 1.00* OV 1.00 ! PT 1.05 SC 1.02 TC 1.00* TS 1.00* ! WF 0.93 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.00* FD 0.00* GG 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* ON 0.00* OV 0.00* ! PT 0.00* SC 0.00* TC 0.00* TS 0.00* ! WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! 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* ! ! ! Fit before self-cal, rms=0.369457Jy sigma=0.002067 ! Fit after self-cal, rms=0.379236Jy sigma=0.001855 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.9597 mas, bmaj=1.681 mas, bpa=-2.918 degrees ! Estimated noise=389.746 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 = 0.00177687 Jy ! Component: 100 - total flux cleaned = 0.00202812 Jy ! Component: 150 - total flux cleaned = 0.00212669 Jy ! Component: 200 - total flux cleaned = 0.00243699 Jy ! Total flux subtracted in 200 components = 0.00243699 Jy ! Clean residual min=-0.006531 max=0.007089 Jy/beam ! Clean residual mean=-0.000592 rms=0.001782 Jy/beam ! Combined flux in latest and established models = 1.08964 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 37 components and 1.08964 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.379123Jy sigma=0.001853 ! Fit after self-cal, rms=0.379172Jy sigma=0.001852 ! Inverting map ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 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=0.379172Jy sigma=0.001852 ! Fit after self-cal, rms=0.449476Jy sigma=0.001780 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.9575 mas, bmaj=1.681 mas, bpa=-3.165 degrees ! Estimated noise=389.877 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000113381 Jy ! Component: 100 - total flux cleaned = -0.000368555 Jy ! Component: 150 - total flux cleaned = -0.000730267 Jy ! Component: 200 - total flux cleaned = -0.000967652 Jy ! Total flux subtracted in 200 components = -0.000967652 Jy ! Clean residual min=-0.003758 max=0.003373 Jy/beam ! Clean residual mean=-0.000204 rms=0.000870 Jy/beam ! Combined flux in latest and established models = 1.08867 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 42 components and 1.08867 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.449436Jy sigma=0.001778 ! Fit after self-cal, rms=0.449439Jy sigma=0.001777 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 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 = 6.05568e-05 Jy ! Component: 100 - total flux cleaned = -0.000175519 Jy ! Component: 150 - total flux cleaned = -0.000318868 Jy ! Component: 200 - total flux cleaned = -0.000516038 Jy ! Total flux subtracted in 200 components = -0.000516038 Jy ! Clean residual min=-0.003618 max=0.003073 Jy/beam ! Clean residual mean=-0.000188 rms=0.000856 Jy/beam ! Combined flux in latest and established models = 1.08815 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 45 components and 1.08815 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.449416Jy sigma=0.001776 ! Fit after self-cal, rms=0.449405Jy sigma=0.001776 ! Inverting map ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 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=0.449405Jy sigma=0.001776 ! Fit after self-cal, rms=0.450659Jy sigma=0.001776 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.9566 mas, bmaj=1.682 mas, bpa=-3.166 degrees ! Estimated noise=390.124 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000307671 Jy ! Component: 100 - total flux cleaned = -0.000108353 Jy ! Component: 150 - total flux cleaned = -0.000392297 Jy ! Component: 200 - total flux cleaned = -0.000580642 Jy ! Total flux subtracted in 200 components = -0.000580642 Jy ! Clean residual min=-0.003456 max=0.003112 Jy/beam ! Clean residual mean=-0.000183 rms=0.000823 Jy/beam ! Combined flux in latest and established models = 1.08757 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 45 components and 1.08757 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.450633Jy sigma=0.001775 ! Fit after self-cal, rms=0.450609Jy sigma=0.001774 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 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 = 0.000120416 Jy ! Component: 100 - total flux cleaned = -7.2371e-05 Jy ! Component: 150 - total flux cleaned = -0.000188045 Jy ! Component: 200 - total flux cleaned = -0.000347053 Jy ! Total flux subtracted in 200 components = -0.000347053 Jy ! Clean residual min=-0.003373 max=0.002995 Jy/beam ! Clean residual mean=-0.000179 rms=0.000813 Jy/beam ! Combined flux in latest and established models = 1.08723 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 45 components and 1.08723 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.450591Jy sigma=0.001774 ! Fit after self-cal, rms=0.450582Jy sigma=0.001774 ! Inverting map ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 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=0.450582Jy sigma=0.001774 ! Fit after self-cal, rms=0.451117Jy sigma=0.001774 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=2.794 mas, bmaj=3.16 mas, bpa=44.18 degrees ! Estimated noise=442.95 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000839411 Jy ! Component: 100 - total flux cleaned = 0.000662885 Jy ! Component: 150 - total flux cleaned = 0.000570133 Jy ! Component: 200 - total flux cleaned = 0.000461297 Jy ! Total flux subtracted in 200 components = 0.000461297 Jy ! Clean residual min=-0.002715 max=0.001953 Jy/beam ! Clean residual mean=-0.000340 rms=0.000752 Jy/beam ! Combined flux in latest and established models = 1.08769 Jy selfcal ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 47 components and 1.08769 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.451110Jy sigma=0.001773 ! Fit after self-cal, rms=0.451102Jy sigma=0.001773 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 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 = 0.000183981 Jy ! Component: 100 - total flux cleaned = 8.89343e-05 Jy ! Component: 150 - total flux cleaned = 1.34417e-05 Jy ! Component: 200 - total flux cleaned = -4.58651e-05 Jy ! Total flux subtracted in 200 components = -4.58651e-05 Jy ! Clean residual min=-0.002759 max=0.001983 Jy/beam ! Clean residual mean=-0.000339 rms=0.000754 Jy/beam ! Combined flux in latest and established models = 1.08764 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 48 components and 1.08764 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.451106Jy sigma=0.001773 ! Fit after self-cal, rms=0.451099Jy sigma=0.001773 ! Inverting map ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 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 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.9563 mas, bmaj=1.683 mas, bpa=-3.16 degrees ! Estimated noise=390.382 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9563 x 1.683 at -3.16 degrees (North through East) ! Clean map min=-0.0028584 max=0.87683 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=0.451099Jy sigma=0.001773 ! Fit after self-cal, rms=0.424770Jy sigma=0.001601 ! Inverting map and beam ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.9563 mas, bmaj=1.684 mas, bpa=-3.18 degrees ! Estimated noise=390.43 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -6.69368e-05 Jy ! Component: 100 - total flux cleaned = -0.000203629 Jy ! Component: 150 - total flux cleaned = -0.000323818 Jy ! Component: 200 - total flux cleaned = -0.000433977 Jy ! Total flux subtracted in 200 components = -0.000433977 Jy ! Clean residual min=-0.003054 max=0.002804 Jy/beam ! Clean residual mean=-0.000219 rms=0.000754 Jy/beam ! Combined flux in latest and established models = 1.08721 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 49 components and 1.08721 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.424753Jy sigma=0.001601 ! Fit after self-cal, rms=0.424741Jy sigma=0.001600 ! Inverting map ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.33169e-05 Jy ! Component: 100 - total flux cleaned = -9.07286e-05 Jy ! Component: 150 - total flux cleaned = -0.000184518 Jy ! Component: 200 - total flux cleaned = -0.000317832 Jy ! Total flux subtracted in 200 components = -0.000317832 Jy ! Clean residual min=-0.002975 max=0.002824 Jy/beam ! Clean residual mean=-0.000216 rms=0.000745 Jy/beam ! Combined flux in latest and established models = 1.08689 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 49 components and 1.08689 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.424730Jy sigma=0.001600 ! Fit after self-cal, rms=0.424722Jy sigma=0.001600 ! Inverting map ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.424722Jy sigma=0.001600 ! Fit after self-cal, rms=0.425641Jy sigma=0.001600 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 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.6695 mas, bmaj=1.216 mas, bpa=2.195 degrees ! Estimated noise=660.452 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.64208 Jy ! Component: 100 - total flux cleaned = 0.855492 Jy ! Component: 150 - total flux cleaned = 0.94418 Jy ! Component: 200 - total flux cleaned = 0.99273 Jy ! Total flux subtracted in 200 components = 0.99273 Jy ! Clean residual min=-0.007523 max=0.024958 Jy/beam ! Clean residual mean=0.000106 rms=0.002875 Jy/beam ! Combined flux in latest and established models = 0.99273 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 19 model components to the UV plane model. ! The established model now contains 19 components and 0.99273 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.9559 mas, bmaj=1.684 mas, bpa=-3.174 degrees ! Estimated noise=390.428 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 = 0.0501053 Jy ! Component: 100 - total flux cleaned = 0.0713258 Jy ! Component: 150 - total flux cleaned = 0.0815337 Jy ! Component: 200 - total flux cleaned = 0.0867395 Jy ! Total flux subtracted in 200 components = 0.0867395 Jy ! Clean residual min=-0.003037 max=0.005276 Jy/beam ! Clean residual mean=-0.000145 rms=0.000913 Jy/beam ! Combined flux in latest and established models = 1.07947 Jy ! Adding 34 model components to the UV plane model. ! The established model now contains 45 components and 1.07947 Jy ! Inverting map ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Added new window around map position (-1.8, -1.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00457338 Jy ! Component: 100 - total flux cleaned = 0.00593562 Jy ! Component: 150 - total flux cleaned = 0.00616399 Jy ! Component: 200 - total flux cleaned = 0.00636714 Jy ! Total flux subtracted in 200 components = 0.00636714 Jy ! Clean residual min=-0.002690 max=0.002057 Jy/beam ! Clean residual mean=-0.000208 rms=0.000688 Jy/beam ! Combined flux in latest and established models = 1.08584 Jy ! Adding 14 model components to the UV plane model. ! The established model now contains 55 components and 1.08584 Jy ! Inverting map ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 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 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=2.794 mas, bmaj=3.16 mas, bpa=43.6 degrees ! Estimated noise=443.039 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00102092 Jy ! Component: 100 - total flux cleaned = 0.00114323 Jy ! Component: 150 - total flux cleaned = 0.00116469 Jy ! Component: 200 - total flux cleaned = 0.00120329 Jy ! Total flux subtracted in 200 components = 0.00120329 Jy ! Clean residual min=-0.002348 max=0.001544 Jy/beam ! Clean residual mean=-0.000397 rms=0.000668 Jy/beam ! Combined flux in latest and established models = 1.08704 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 = 1.76033e-05 Jy ! Component: 100 - total flux cleaned = 5.00472e-05 Jy ! Component: 150 - total flux cleaned = 6.42856e-05 Jy ! Component: 200 - total flux cleaned = 7.8388e-05 Jy ! Total flux subtracted in 200 components = 7.8388e-05 Jy ! Clean residual min=-0.002343 max=0.001579 Jy/beam ! Clean residual mean=-0.000398 rms=0.000666 Jy/beam ! Combined flux in latest and established models = 1.08712 Jy ! Adding 15 model components to the UV plane model. ! The established model now contains 66 components and 1.08712 Jy ! Inverting map ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! Estimated beam: bmin=0.9559 mas, bmaj=1.684 mas, bpa=-3.174 degrees ! Estimated noise=390.428 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000384513 Jy ! Component: 100 - total flux cleaned = -0.000329905 Jy ! Component: 150 - total flux cleaned = -0.000278432 Jy ! Component: 200 - total flux cleaned = -0.000233986 Jy ! Total flux subtracted in 200 components = -0.000233986 Jy ! Clean residual min=-0.002668 max=0.002185 Jy/beam ! Clean residual mean=-0.000217 rms=0.000658 Jy/beam ! Combined flux in latest and established models = 1.08688 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 77 components and 1.08688 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.425516Jy sigma=0.001598 ! Fit after self-cal, rms=0.425445Jy sigma=0.001597 wmodel J2236+2828_X_2003_06_18_pus_map.mod ! Writing 77 model components to file: J2236+2828_X_2003_06_18_pus_map.mod wobs J2236+2828_X_2003_06_18_pus_uvs.fits ! Writing UV FITS file: J2236+2828_X_2003_06_18_pus_uvs.fits wwins J2236+2828_X_2003_06_18_pus_map.win ! wwins: Wrote 3 windows to J2236+2828_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 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.0012318 Jy ! Component: 100 - total flux cleaned = -0.00197405 Jy ! Component: 150 - total flux cleaned = -0.00266697 Jy ! Component: 200 - total flux cleaned = -0.00325446 Jy ! Component: 250 - total flux cleaned = -0.00375006 Jy ! Component: 300 - total flux cleaned = -0.00412744 Jy ! Component: 350 - total flux cleaned = -0.00452863 Jy ! Component: 400 - total flux cleaned = -0.00495286 Jy ! Component: 450 - total flux cleaned = -0.00542972 Jy ! Component: 500 - total flux cleaned = -0.00580266 Jy ! Component: 550 - total flux cleaned = -0.00619822 Jy ! Component: 600 - total flux cleaned = -0.00655615 Jy ! Component: 650 - total flux cleaned = -0.00687855 Jy ! Component: 700 - total flux cleaned = -0.00722353 Jy ! Component: 750 - total flux cleaned = -0.00750643 Jy ! Component: 800 - total flux cleaned = -0.00778534 Jy ! Component: 850 - total flux cleaned = -0.00808757 Jy ! Component: 900 - total flux cleaned = -0.00835869 Jy ! Component: 950 - total flux cleaned = -0.00862622 Jy ! Component: 1000 - total flux cleaned = -0.00889012 Jy ! Total flux subtracted in 1024 components = -0.00899472 Jy ! Clean residual min=-0.001635 max=0.001303 Jy/beam ! Clean residual mean=-0.000108 rms=0.000516 Jy/beam ! Combined flux in latest and established models = 1.07789 Jy keep ! Adding 61 model components to the UV plane model. ! The established model now contains 138 components and 1.07789 Jy wmap "J2236+2828_X_2003_06_18_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9559 x 1.684 at -3.174 degrees (North through East) ! Clean map min=-0.0024688 max=0.87841 Jy/beam ! Writing clean map to FITS file: J2236+2828_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 0.878411 invert ! Inverting map ! Your choice of large map pixels excluded 0.137% of the data. ! The x-axis pixel size should ideally be below 0.199 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000515997 device "J2236+2828_X_2003_06_18_pus\_map.eps/VPS" ! Attempting to open device: 'J2236+2828_X_2003_06_18_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.176226 0.176226 0.352453 0.704905 1.40981 2.81962 5.63924 11.2785 22.557 45.1139 90.2279 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0015 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.878 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9559 x 1.684 at -3.174 degrees (North through East) ! Clean map min=-0.0024688 max=0.87841 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J2236+2828_X_2003_06_18_pus\_map.gif/vgif" ! Attempting to open device: 'J2236+2828_X_2003_06_18_pus_map.gif/vgif' mapplot cln quit ! Quitting program ! Log file J2236+2828_X_2003_06_18_pus_uvs.log closed on Wed Jan 17 18:33:19 2007