! Started logfile: J1743-0350_X_2003_06_18_pus_uvs.log on Wed Jan 17 17:58:50 2007 obs J1743-0350_X_2003_06_18_pus_uva.fits ! Reading UV FITS file: J1743-0350_X_2003_06_18_pus_uva.fits ! AN table 1: 121 integrations on 153 of 153 possible baselines. ! AN table 2: 63 integrations on 153 of 153 possible baselines. ! AN table 3: 146 integrations on 153 of 153 possible baselines. ! AN table 4: 100 integrations on 153 of 153 possible baselines. ! AN table 5: 13 integrations on 153 of 153 possible baselines. ! AN table 6: 131 integrations on 153 of 153 possible baselines. ! AN table 7: 17 integrations on 153 of 153 possible baselines. ! AN table 8: 17 integrations on 153 of 153 possible baselines. ! AN table 9: Unused. ! Apparent sampling: 0.164183 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1743-0350 ! ! 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 61092 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 1713 telescope corrections were flagged in sub-array 1. ! A total of 1021 telescope corrections were flagged in sub-array 2. ! A total of 2035 telescope corrections were flagged in sub-array 3. ! A total of 1529 telescope corrections were flagged in sub-array 4. ! A total of 158 telescope corrections were flagged in sub-array 5. ! A total of 1612 telescope corrections were flagged in sub-array 6. ! A total of 267 telescope corrections were flagged in sub-array 7. ! A total of 306 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 2. ! A total of 1713 telescope corrections were flagged in sub-array 1. ! A total of 1021 telescope corrections were flagged in sub-array 2. ! A total of 2035 telescope corrections were flagged in sub-array 3. ! A total of 1584 telescope corrections were flagged in sub-array 4. ! A total of 158 telescope corrections were flagged in sub-array 5. ! A total of 1612 telescope corrections were flagged in sub-array 6. ! A total of 255 telescope corrections were flagged in sub-array 7. ! A total of 306 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 3. ! A total of 1713 telescope corrections were flagged in sub-array 1. ! A total of 1021 telescope corrections were flagged in sub-array 2. ! A total of 2035 telescope corrections were flagged in sub-array 3. ! A total of 1584 telescope corrections were flagged in sub-array 4. ! A total of 158 telescope corrections were flagged in sub-array 5. ! A total of 1612 telescope corrections were flagged in sub-array 6. ! A total of 255 telescope corrections were flagged in sub-array 7. ! A total of 306 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 4. ! A total of 1713 telescope corrections were flagged in sub-array 1. ! A total of 1021 telescope corrections were flagged in sub-array 2. ! A total of 2035 telescope corrections were flagged in sub-array 3. ! A total of 1584 telescope corrections were flagged in sub-array 4. ! A total of 158 telescope corrections were flagged in sub-array 5. ! A total of 1612 telescope corrections were flagged in sub-array 6. ! A total of 255 telescope corrections were flagged in sub-array 7. ! A total of 306 telescope corrections were flagged in sub-array 8. ! ! Fit before self-cal, rms=3.980378Jy sigma=0.051435 ! Fit after self-cal, rms=3.550977Jy sigma=0.047175 ! 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 0.245% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.7423 mas, bmaj=1.098 mas, bpa=10.07 degrees ! Estimated noise=760.103 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 = 3.47868 Jy ! Component: 100 - total flux cleaned = 4.40198 Jy ! Total flux subtracted in 100 components = 4.40198 Jy ! Clean residual min=-0.123429 max=0.361575 Jy/beam ! Clean residual mean=0.000024 rms=0.048285 Jy/beam ! Combined flux in latest and established models = 4.40198 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 13 components and 4.40198 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.010361Jy sigma=0.010320 ! Fit after self-cal, rms=1.009663Jy sigma=0.010319 ! Inverting map ! Your choice of large map pixels excluded 0.245% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1987 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.395784 Jy ! Component: 100 - total flux cleaned = 0.620473 Jy ! Total flux subtracted in 100 components = 0.620473 Jy ! Clean residual min=-0.122284 max=0.127131 Jy/beam ! Clean residual mean=-0.000462 rms=0.032713 Jy/beam ! Combined flux in latest and established models = 5.02245 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 27 components and 5.02245 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.858108Jy sigma=0.007001 ! Fit after self-cal, rms=0.857935Jy sigma=0.006997 ! Inverting map ! Your choice of large map pixels excluded 0.245% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1987 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 0.245% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=1.034 mas, bmaj=1.445 mas, bpa=2.525 degrees ! Estimated noise=379.658 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 = 0.133984 Jy ! Component: 100 - total flux cleaned = 0.190222 Jy ! Component: 150 - total flux cleaned = 0.205964 Jy ! Component: 200 - total flux cleaned = 0.209769 Jy ! Total flux subtracted in 200 components = 0.209769 Jy ! Clean residual min=-0.095231 max=0.087120 Jy/beam ! Clean residual mean=-0.002208 rms=0.022689 Jy/beam ! Combined flux in latest and established models = 5.23222 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 34 components and 5.23222 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.833121Jy sigma=0.006748 ! Fit after self-cal, rms=0.833130Jy sigma=0.006746 ! Inverting map ! Your choice of large map pixels excluded 0.245% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1987 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 45 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 1.01 GG 1.00* HN 0.97 ! KK 1.00* KP 1.04 LA 1.00 MA 1.00* ! MK 1.00* NL 1.09 ON 1.00* OV 1.00 ! PT 1.01 SC 0.92 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.04 GG 1.00* HN 1.00* ! KK 1.00* KP 1.11 LA 1.05 MA 1.00* ! MK 1.00* NL 1.00* ON 1.00* OV 1.00* ! PT 1.05 SC 1.00* TC 0.93 TS 1.00* ! WF 1.00* WZ 1.00* ! ! A total of 96 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.86 FD 0.98 GG 1.00* HN 0.95 ! KK 1.03 KP 0.98 LA 0.97 MA 1.00* ! MK 1.04 NL 1.05 ON 1.00* OV 0.93 ! PT 0.96 SC 0.93 TC 1.04 TS 1.00* ! WF 1.01 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 0.90 GG 1.00* HN 1.00* ! KK 1.00* KP 0.90 LA 0.87 MA 1.00* ! MK 1.00* NL 0.87 ON 1.00* OV 0.98 ! PT 0.87 SC 1.00* TC 8.80 TS 1.00* ! WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 1.00* GG 1.00* HN 1.00* ! KK 1.04 KP 1.18 LA 1.00* MA 1.00* ! MK 1.01 NL 1.00* ON 1.00* OV 1.04 ! PT 1.15 SC 1.00* TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! A total of 66 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.98 FD 1.00 GG 1.00* HN 0.96 ! KK 1.00* KP 1.05 LA 1.01 MA 1.00* ! MK 1.00* NL 1.07 ON 1.00* OV 1.02 ! PT 1.01 SC 2.59 TC 0.99 TS 1.00* ! WF 1.11 WZ 1.00* ! ! A total of 39 telescope corrections were flagged in sub-array 7. ! 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* ! ! Telescope amplitude corrections in sub-array 8: ! 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 45 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.99 GG 1.00* HN 0.99 ! KK 1.00* KP 0.99 LA 1.00 MA 1.00* ! MK 1.00* NL 1.06 ON 1.00* OV 0.99 ! PT 1.04 SC 0.88 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.02 GG 1.00* HN 1.00* ! KK 1.00* KP 1.05 LA 1.06 MA 1.00* ! MK 1.00* NL 1.00* ON 1.00* OV 1.00* ! PT 1.10 SC 1.00* TC 1.02 TS 1.00* ! WF 1.00* WZ 1.00* ! ! A total of 96 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.88 FD 0.96 GG 1.00* HN 0.96 ! KK 1.02 KP 0.93 LA 0.97 MA 1.00* ! MK 1.05 NL 1.01 ON 1.00* OV 0.92 ! PT 1.00 SC 0.89 TC 1.10 TS 1.00* ! WF 1.04 WZ 1.00* ! ! A total of 96 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 1.00* ! KK 1.00* KP 0.86 LA 0.87 MA 1.00* ! MK 1.00* NL 0.83 ON 1.00* OV 0.97 ! PT 0.91 SC 1.00* TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 1.00* GG 1.00* HN 1.00* ! KK 1.01 KP 1.13 LA 1.00* MA 1.00* ! MK 1.02 NL 1.00* ON 1.00* OV 1.02 ! PT 1.19 SC 1.00* TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! A total of 66 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 0.96 ! KK 1.00* KP 1.00 LA 1.01 MA 1.00* ! MK 1.00* NL 1.04 ON 1.00* OV 1.01 ! PT 1.04 SC 2.96 TC 1.04 TS 1.00* ! WF 1.13 WZ 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 1.00* GG 1.00* HN 1.42 ! KK 1.00* KP 1.00* LA 1.00* MA 1.04 ! MK 1.00* NL 1.00* ON 1.01 OV 1.00* ! PT 1.00* SC 1.00* TC 1.00* TS 1.00* ! WF 1.22 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 8: ! 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 45 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 0.98 GG 1.00* HN 0.97 ! KK 1.00* KP 1.02 LA 1.00 MA 1.00* ! MK 1.00* NL 1.03 ON 1.00* OV 1.02 ! PT 1.06 SC 0.90 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.01 GG 1.00* HN 1.00* ! KK 1.00* KP 1.08 LA 1.06 MA 1.00* ! MK 1.00* NL 1.00* ON 1.00* OV 1.00* ! PT 1.12 SC 1.00* TC 0.94 TS 1.00* ! WF 1.00* WZ 1.00* ! ! A total of 96 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.92 FD 0.94 GG 1.00* HN 0.94 ! KK 1.08 KP 0.97 LA 0.97 MA 1.00* ! MK 1.04 NL 0.99 ON 1.00* OV 0.95 ! PT 1.02 SC 0.91 TC 1.00 TS 1.00* ! WF 0.98 WZ 1.00* ! ! A total of 96 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 1.00* ! KK 1.00* KP 0.89 LA 0.87 MA 1.00* ! MK 1.00* NL 0.82 ON 1.00* OV 1.00 ! PT 0.92 SC 1.00* TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.05 FD 1.00* GG 1.00* HN 1.00* ! KK 1.07 KP 1.16 LA 1.00* MA 1.00* ! MK 1.02 NL 1.00* ON 1.00* OV 1.06 ! PT 1.22 SC 1.00* TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! A total of 66 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.02 FD 0.97 GG 1.00* HN 0.94 ! KK 1.00* KP 1.03 LA 1.02 MA 1.00* ! MK 1.00* NL 1.01 ON 1.00* OV 1.05 ! PT 1.06 SC 3.17 TC 0.97 TS 1.00* ! WF 1.05 WZ 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 1.00* GG 1.00* HN 1.33 ! KK 1.00* KP 1.00* LA 1.00* MA 1.07 ! MK 1.00* NL 1.00* ON 1.03 OV 1.00* ! PT 1.00* SC 1.00* TC 1.00* TS 1.00* ! WF 1.09 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 8: ! 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 45 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.96 GG 1.00* HN 0.99 ! KK 1.00* KP 0.98 LA 0.98 MA 1.00* ! MK 1.00* NL 1.04 ON 1.00* OV 1.01 ! PT 1.07 SC 0.94 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 0.99 GG 1.00* HN 1.00* ! KK 1.00* KP 1.04 LA 1.03 MA 1.00* ! MK 1.00* NL 1.00* ON 1.00* OV 1.00* ! PT 1.13 SC 1.00* TC 0.87 TS 1.00* ! WF 1.00* WZ 1.00* ! ! A total of 96 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.90 FD 0.93 GG 1.00* HN 0.97 ! KK 1.03 KP 0.92 LA 0.95 MA 1.00* ! MK 1.07 NL 0.99 ON 1.00* OV 0.94 ! PT 1.02 SC 0.95 TC 1.00 TS 1.00* ! WF 0.97 WZ 1.00* ! ! A total of 96 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 0.87 GG 1.00* HN 1.00* ! KK 1.00* KP 0.86 LA 0.85 MA 1.00* ! MK 1.00* NL 0.84 ON 1.00* OV 0.98 ! PT 0.93 SC 1.00* TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 1.00* GG 1.00* HN 1.00* ! KK 1.04 KP 1.10 LA 1.00* MA 1.00* ! MK 1.04 NL 1.00* ON 1.00* OV 1.04 ! PT 1.23 SC 1.00* TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! A total of 66 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.00 FD 0.95 GG 1.00* HN 0.97 ! KK 1.00* KP 0.99 LA 0.99 MA 1.00* ! MK 1.00* NL 1.02 ON 1.00* OV 1.04 ! PT 1.06 SC 3.60 TC 0.94 TS 1.00* ! WF 1.04 WZ 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 1.00* GG 1.00* HN 1.38 ! KK 1.00* KP 1.00* LA 1.00* MA 1.10 ! MK 1.00* NL 1.00* ON 1.07 OV 1.00* ! PT 1.00* SC 1.00* TC 1.00* TS 1.00* ! WF 1.05 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 8: ! 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=0.833130Jy sigma=0.006746 ! Fit after self-cal, rms=0.603230Jy sigma=0.002244 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=1.056 mas, bmaj=1.522 mas, bpa=0.4248 degrees ! Estimated noise=382.924 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 (-0.2, -1.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0038146 Jy ! Component: 100 - total flux cleaned = 0.00376222 Jy ! Component: 150 - total flux cleaned = 0.00440106 Jy ! Component: 200 - total flux cleaned = 0.00441154 Jy ! Total flux subtracted in 200 components = 0.00441154 Jy ! Clean residual min=-0.012720 max=0.013043 Jy/beam ! Clean residual mean=-0.000117 rms=0.003174 Jy/beam ! Combined flux in latest and established models = 5.23664 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 43 components and 5.23663 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.600795Jy sigma=0.002197 ! Fit after self-cal, rms=0.600956Jy sigma=0.002193 ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 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=0.600956Jy sigma=0.002193 ! Fit after self-cal, rms=0.600118Jy sigma=0.002152 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=1.056 mas, bmaj=1.521 mas, bpa=0.4438 degrees ! Estimated noise=383.113 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00216756 Jy ! Component: 100 - total flux cleaned = 0.00167027 Jy ! Component: 150 - total flux cleaned = 0.00123946 Jy ! Component: 200 - total flux cleaned = 0.00124304 Jy ! Total flux subtracted in 200 components = 0.00124304 Jy ! Clean residual min=-0.009482 max=0.011696 Jy/beam ! Clean residual mean=-0.000051 rms=0.002547 Jy/beam ! Combined flux in latest and established models = 5.23788 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 44 components and 5.23788 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.598784Jy sigma=0.002129 ! Fit after self-cal, rms=0.598676Jy sigma=0.002127 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 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 (2, -1.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00478154 Jy ! Component: 100 - total flux cleaned = 0.00393541 Jy ! Component: 150 - total flux cleaned = 0.00316759 Jy ! Component: 200 - total flux cleaned = 0.00317896 Jy ! Total flux subtracted in 200 components = 0.00317896 Jy ! Clean residual min=-0.008107 max=0.009231 Jy/beam ! Clean residual mean=-0.000106 rms=0.002217 Jy/beam ! Combined flux in latest and established models = 5.24106 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 52 components and 5.24106 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.597718Jy sigma=0.002112 ! Fit after self-cal, rms=0.597613Jy sigma=0.002111 ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 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=0.597613Jy sigma=0.002111 ! Fit after self-cal, rms=0.599182Jy sigma=0.002109 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=1.057 mas, bmaj=1.521 mas, bpa=0.4072 degrees ! Estimated noise=383.322 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00163283 Jy ! Component: 100 - total flux cleaned = 0.00126131 Jy ! Component: 150 - total flux cleaned = 0.0009389 Jy ! Component: 200 - total flux cleaned = 0.00123389 Jy ! Total flux subtracted in 200 components = 0.00123389 Jy ! Clean residual min=-0.007578 max=0.008538 Jy/beam ! Clean residual mean=0.000054 rms=0.002032 Jy/beam ! Combined flux in latest and established models = 5.24229 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 56 components and 5.24229 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.598505Jy sigma=0.002098 ! Fit after self-cal, rms=0.598439Jy sigma=0.002097 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 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 = 0.00127652 Jy ! Component: 100 - total flux cleaned = 0.00071987 Jy ! Component: 150 - total flux cleaned = 0.000717714 Jy ! Component: 200 - total flux cleaned = 0.000712468 Jy ! Total flux subtracted in 200 components = 0.000712468 Jy ! Clean residual min=-0.007284 max=0.007821 Jy/beam ! Clean residual mean=0.000042 rms=0.001909 Jy/beam ! Combined flux in latest and established models = 5.243 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 57 components and 5.243 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.598000Jy sigma=0.002090 ! Fit after self-cal, rms=0.597951Jy sigma=0.002090 ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 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=0.597951Jy sigma=0.002090 ! Fit after self-cal, rms=0.599682Jy sigma=0.002089 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=2.318 mas, bmaj=4.212 mas, bpa=-9.634 degrees ! Estimated noise=414.089 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0037454 Jy ! Component: 100 - total flux cleaned = 0.00416214 Jy ! Component: 150 - total flux cleaned = 0.00423083 Jy ! Component: 200 - total flux cleaned = 0.00423064 Jy ! Total flux subtracted in 200 components = 0.00423064 Jy ! Clean residual min=-0.004561 max=0.004840 Jy/beam ! Clean residual mean=0.000171 rms=0.001532 Jy/beam ! Combined flux in latest and established models = 5.24723 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 66 components and 5.24723 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.599626Jy sigma=0.002087 ! Fit after self-cal, rms=0.599617Jy sigma=0.002087 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 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 = 0.000501282 Jy ! Component: 100 - total flux cleaned = 0.00057875 Jy ! Component: 150 - total flux cleaned = 0.000519193 Jy ! Component: 200 - total flux cleaned = 0.000520746 Jy ! Total flux subtracted in 200 components = 0.000520746 Jy ! Clean residual min=-0.004640 max=0.004731 Jy/beam ! Clean residual mean=0.000146 rms=0.001538 Jy/beam ! Combined flux in latest and established models = 5.24775 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 72 components and 5.24775 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.599591Jy sigma=0.002086 ! Fit after self-cal, rms=0.599573Jy sigma=0.002086 ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 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 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=1.057 mas, bmaj=1.521 mas, bpa=0.3713 degrees ! Estimated noise=383.574 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.057 x 1.521 at 0.3713 degrees (North through East) ! Clean map min=-0.013849 max=4.5594 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=0.599573Jy sigma=0.002086 ! Fit after self-cal, rms=0.840594Jy sigma=0.001594 ! Inverting map and beam ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=1.057 mas, bmaj=1.52 mas, bpa=0.362 degrees ! Estimated noise=383.508 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00032607 Jy ! Component: 100 - total flux cleaned = -0.0010027 Jy ! Component: 150 - total flux cleaned = -0.00120131 Jy ! Component: 200 - total flux cleaned = -0.00137678 Jy ! Total flux subtracted in 200 components = -0.00137678 Jy ! Clean residual min=-0.006716 max=0.005488 Jy/beam ! Clean residual mean=-0.000043 rms=0.001441 Jy/beam ! Combined flux in latest and established models = 5.24638 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 74 components and 5.24638 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.840410Jy sigma=0.001588 ! Fit after self-cal, rms=0.840399Jy sigma=0.001588 ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00016882 Jy ! Component: 100 - total flux cleaned = -0.000171254 Jy ! Component: 150 - total flux cleaned = -0.000327888 Jy ! Component: 200 - total flux cleaned = -0.000324234 Jy ! Total flux subtracted in 200 components = -0.000324234 Jy ! Clean residual min=-0.006592 max=0.005245 Jy/beam ! Clean residual mean=-0.000037 rms=0.001404 Jy/beam ! Combined flux in latest and established models = 5.24605 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 77 components and 5.24605 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.840279Jy sigma=0.001585 ! Fit after self-cal, rms=0.840277Jy sigma=0.001585 ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.840277Jy sigma=0.001585 ! Fit after self-cal, rms=0.842565Jy sigma=0.001584 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 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.7743 mas, bmaj=1.134 mas, bpa=7.565 degrees ! Estimated noise=766.011 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 3.49248 Jy ! Component: 100 - total flux cleaned = 4.40221 Jy ! Component: 150 - total flux cleaned = 4.77189 Jy ! Component: 200 - total flux cleaned = 4.96045 Jy ! Total flux subtracted in 200 components = 4.96045 Jy ! Clean residual min=-0.034498 max=0.093912 Jy/beam ! Clean residual mean=0.000285 rms=0.011776 Jy/beam ! Combined flux in latest and established models = 4.96045 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 25 model components to the UV plane model. ! The established model now contains 25 components and 4.96045 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=1.057 mas, bmaj=1.52 mas, bpa=0.3334 degrees ! Estimated noise=383.652 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 = 0.151801 Jy ! Component: 100 - total flux cleaned = 0.219114 Jy ! Component: 150 - total flux cleaned = 0.250988 Jy ! Component: 200 - total flux cleaned = 0.268877 Jy ! Total flux subtracted in 200 components = 0.268877 Jy ! Clean residual min=-0.010520 max=0.016592 Jy/beam ! Clean residual mean=0.000310 rms=0.002447 Jy/beam ! Combined flux in latest and established models = 5.22933 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 43 components and 5.22933 Jy ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 milli-arcsec ! Added new window around map position (-0.2, 1.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00753425 Jy ! Component: 100 - total flux cleaned = 0.00893866 Jy ! Component: 150 - total flux cleaned = 0.00976392 Jy ! Component: 200 - total flux cleaned = 0.0101374 Jy ! Total flux subtracted in 200 components = 0.0101374 Jy ! Clean residual min=-0.010032 max=0.008939 Jy/beam ! Clean residual mean=0.000140 rms=0.001789 Jy/beam ! Combined flux in latest and established models = 5.23947 Jy ! Adding 13 model components to the UV plane model. ! The established model now contains 53 components and 5.23947 Jy ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 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 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=2.319 mas, bmaj=4.214 mas, bpa=-9.655 degrees ! Estimated noise=414.137 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00414587 Jy ! Component: 100 - total flux cleaned = 0.00465366 Jy ! Component: 150 - total flux cleaned = 0.00482732 Jy ! Component: 200 - total flux cleaned = 0.00498599 Jy ! Total flux subtracted in 200 components = 0.00498599 Jy ! Clean residual min=-0.004339 max=0.003306 Jy/beam ! Clean residual mean=0.000102 rms=0.001220 Jy/beam ! Combined flux in latest and established models = 5.24445 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 = 0.000149405 Jy ! Component: 100 - total flux cleaned = 0.00029316 Jy ! Component: 150 - total flux cleaned = 0.000425489 Jy ! Component: 200 - total flux cleaned = 0.000555443 Jy ! Total flux subtracted in 200 components = 0.000555443 Jy ! Clean residual min=-0.004295 max=0.003223 Jy/beam ! Clean residual mean=0.000080 rms=0.001211 Jy/beam ! Combined flux in latest and established models = 5.24501 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 76 components and 5.24501 Jy ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=1.057 mas, bmaj=1.52 mas, bpa=0.3334 degrees ! Estimated noise=383.652 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00365003 Jy ! Component: 100 - total flux cleaned = -0.00396652 Jy ! Component: 150 - total flux cleaned = -0.00396575 Jy ! Component: 200 - total flux cleaned = -0.0042432 Jy ! Total flux subtracted in 200 components = -0.0042432 Jy ! Clean residual min=-0.009018 max=0.007589 Jy/beam ! Clean residual mean=0.000125 rms=0.001579 Jy/beam ! Combined flux in latest and established models = 5.24076 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 85 components and 5.24076 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.845390Jy sigma=0.001599 ! Fit after self-cal, rms=0.844824Jy sigma=0.001596 wmodel J1743-0350_X_2003_06_18_pus_map.mod ! Writing 85 model components to file: J1743-0350_X_2003_06_18_pus_map.mod wobs J1743-0350_X_2003_06_18_pus_uvs.fits ! Writing UV FITS file: J1743-0350_X_2003_06_18_pus_uvs.fits wwins J1743-0350_X_2003_06_18_pus_map.win ! wwins: Wrote 4 windows to J1743-0350_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 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000748465 Jy ! Component: 100 - total flux cleaned = -0.00169754 Jy ! Component: 150 - total flux cleaned = -0.00202133 Jy ! Component: 200 - total flux cleaned = -0.00201858 Jy ! Component: 250 - total flux cleaned = -0.00241212 Jy ! Component: 300 - total flux cleaned = -0.00269792 Jy ! Component: 350 - total flux cleaned = -0.00297779 Jy ! Component: 400 - total flux cleaned = -0.0031614 Jy ! Component: 450 - total flux cleaned = -0.00351647 Jy ! Component: 500 - total flux cleaned = -0.00351665 Jy ! Component: 550 - total flux cleaned = -0.00334542 Jy ! Component: 600 - total flux cleaned = -0.00326233 Jy ! Component: 650 - total flux cleaned = -0.00309754 Jy ! Component: 700 - total flux cleaned = -0.00301732 Jy ! Component: 750 - total flux cleaned = -0.00293738 Jy ! Component: 800 - total flux cleaned = -0.00293671 Jy ! Component: 850 - total flux cleaned = -0.00278022 Jy ! Component: 900 - total flux cleaned = -0.00270302 Jy ! Component: 950 - total flux cleaned = -0.00255222 Jy ! Component: 1000 - total flux cleaned = -0.00240226 Jy ! Total flux subtracted in 1024 components = -0.00232833 Jy ! Clean residual min=-0.003685 max=0.003687 Jy/beam ! Clean residual mean=0.000186 rms=0.001212 Jy/beam ! Combined flux in latest and established models = 5.23843 Jy keep ! Adding 38 model components to the UV plane model. ! The established model now contains 113 components and 5.23844 Jy wmap "J1743-0350_X_2003_06_18_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.057 x 1.52 at 0.3334 degrees (North through East) ! Clean map min=-0.0083957 max=4.586 Jy/beam ! Writing clean map to FITS file: J1743-0350_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 4.586 invert ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1977 milli-arcsec ! The y-axis pixel size should ideally be below 0.1988 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00121339 device "J1743-0350_X_2003_06_18_pus\_map.eps/VPS" ! Attempting to open device: 'J1743-0350_X_2003_06_18_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.079376 0.079376 0.158752 0.317504 0.635008 1.27002 2.54003 5.08007 10.1601 20.3203 40.6405 81.2811 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0036 print "peak=",int(1000*peak_flux)/1000 ! peak= 4.585 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.057 x 1.52 at 0.3334 degrees (North through East) ! Clean map min=-0.0083957 max=4.586 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1743-0350_X_2003_06_18_pus\_map.gif/vgif" ! Attempting to open device: 'J1743-0350_X_2003_06_18_pus_map.gif/vgif' mapplot cln quit ! Quitting program ! Log file J1743-0350_X_2003_06_18_pus_uvs.log closed on Wed Jan 17 18:00:58 2007