! Started logfile: J1337-1257_X_2003_06_18_pus_uvs.log on Wed Jan 17 17:26:03 2007 obs J1337-1257_X_2003_06_18_pus_uva.fits ! Reading UV FITS file: J1337-1257_X_2003_06_18_pus_uva.fits ! AN table 1: 45 integrations on 153 of 153 possible baselines. ! AN table 2: 81 integrations on 153 of 153 possible baselines. ! AN table 3: Unused. ! AN table 4: 11 integrations on 153 of 153 possible baselines. ! AN table 5: 15 integrations on 153 of 153 possible baselines. ! AN table 6: 32 integrations on 153 of 153 possible baselines. ! AN table 7: 71 integrations on 153 of 153 possible baselines. ! AN table 8: 39 integrations on 153 of 153 possible baselines. ! AN table 9: Unused. ! Apparent sampling: 0.118692 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1337-1257 ! ! 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 21356 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 569 telescope corrections were flagged in sub-array 1. ! A total of 1180 telescope corrections were flagged in sub-array 2. ! A total of 198 telescope corrections were flagged in sub-array 3. ! A total of 270 telescope corrections were flagged in sub-array 4. ! A total of 576 telescope corrections were flagged in sub-array 5. ! A total of 1050 telescope corrections were flagged in sub-array 6. ! A total of 559 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 2. ! A total of 569 telescope corrections were flagged in sub-array 1. ! A total of 1125 telescope corrections were flagged in sub-array 2. ! A total of 198 telescope corrections were flagged in sub-array 3. ! A total of 270 telescope corrections were flagged in sub-array 4. ! A total of 576 telescope corrections were flagged in sub-array 5. ! A total of 1050 telescope corrections were flagged in sub-array 6. ! A total of 559 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 3. ! A total of 569 telescope corrections were flagged in sub-array 1. ! A total of 1125 telescope corrections were flagged in sub-array 2. ! A total of 198 telescope corrections were flagged in sub-array 3. ! A total of 270 telescope corrections were flagged in sub-array 4. ! A total of 576 telescope corrections were flagged in sub-array 5. ! A total of 1050 telescope corrections were flagged in sub-array 6. ! A total of 559 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 4. ! A total of 569 telescope corrections were flagged in sub-array 1. ! A total of 1125 telescope corrections were flagged in sub-array 2. ! A total of 198 telescope corrections were flagged in sub-array 3. ! A total of 270 telescope corrections were flagged in sub-array 4. ! A total of 576 telescope corrections were flagged in sub-array 5. ! A total of 1050 telescope corrections were flagged in sub-array 6. ! A total of 559 telescope corrections were flagged in sub-array 7. ! ! Fit before self-cal, rms=2.061985Jy sigma=0.026045 ! Fit after self-cal, rms=1.591941Jy sigma=0.020684 ! 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 1.03% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! Estimated beam: bmin=0.625 mas, bmaj=2.208 mas, bpa=-7.154 degrees ! Estimated noise=986.927 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 = 1.92667 Jy ! Component: 100 - total flux cleaned = 2.40263 Jy ! Total flux subtracted in 100 components = 2.40263 Jy ! Clean residual min=-0.066036 max=0.181291 Jy/beam ! Clean residual mean=0.003333 rms=0.026110 Jy/beam ! Combined flux in latest and established models = 2.40263 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 8 components and 2.40263 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.498457Jy sigma=0.005952 ! Fit after self-cal, rms=0.498241Jy sigma=0.005945 ! Inverting map ! Your choice of large map pixels excluded 1.03% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.189896 Jy ! Component: 100 - total flux cleaned = 0.296932 Jy ! Total flux subtracted in 100 components = 0.296932 Jy ! Clean residual min=-0.052582 max=0.142270 Jy/beam ! Clean residual mean=0.001682 rms=0.018807 Jy/beam ! Combined flux in latest and established models = 2.69956 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 26 components and 2.69956 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.418905Jy sigma=0.004274 ! Fit after self-cal, rms=0.418501Jy sigma=0.004267 ! Inverting map ! Your choice of large map pixels excluded 1.03% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! Added new window around map position (1.2, -1.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.121187 Jy ! Component: 100 - total flux cleaned = 0.186098 Jy ! Total flux subtracted in 100 components = 0.186098 Jy ! Clean residual min=-0.048350 max=0.067100 Jy/beam ! Clean residual mean=0.000585 rms=0.014904 Jy/beam ! Combined flux in latest and established models = 2.88566 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 32 components and 2.88566 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.387024Jy sigma=0.003537 ! Fit after self-cal, rms=0.384426Jy sigma=0.003503 ! Inverting map ! Your choice of large map pixels excluded 1.03% of the data. ! The x-axis pixel size should ideally be below 0.1822 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 1.03% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! Estimated beam: bmin=0.8154 mas, bmaj=2.857 mas, bpa=-10.29 degrees ! Estimated noise=611.48 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 = 0.0636199 Jy ! Component: 100 - total flux cleaned = 0.0902758 Jy ! Component: 150 - total flux cleaned = 0.0986317 Jy ! Component: 200 - total flux cleaned = 0.10623 Jy ! Total flux subtracted in 200 components = 0.10623 Jy ! Clean residual min=-0.045470 max=0.041252 Jy/beam ! Clean residual mean=-0.000802 rms=0.014077 Jy/beam ! Combined flux in latest and established models = 2.99189 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 48 components and 2.99189 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.376466Jy sigma=0.003297 ! Fit after self-cal, rms=0.375706Jy sigma=0.003285 ! Inverting map ! Your choice of large map pixels excluded 1.03% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.98 GG 1.00* HN 0.94 ! KK 1.05 KP 1.02 LA 0.99 MA 1.00* ! MK 0.96 NL 1.07 ON 1.00* OV 0.98 ! PT 0.97 SC 1.00* TC 1.00* TS 1.00* ! WF 1.13 WZ 1.00* ! ! A total of 18 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.95 FD 0.98 GG 1.00* HN 0.99 ! KK 1.03 KP 1.03 LA 0.99 MA 1.00* ! MK 0.96 NL 1.11 ON 1.02 OV 0.98 ! PT 0.97 SC 0.96 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! 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* ! ! Telescope amplitude corrections in sub-array 4: ! 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 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 45 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.99 FD 1.00* GG 1.00* HN 0.91 ! KK 1.04 KP 1.04 LA 0.93 MA 1.00* ! MK 1.04 NL 0.92 ON 1.00* OV 0.96 ! PT 0.93 SC 1.00* TC 1.00* TS 0.92 ! WF 1.00* WZ 1.00* ! ! A total of 6 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 1.08 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 1.56 ON 1.11 OV 1.00* ! PT 1.00* SC 0.96 TC 1.00* TS 1.00* ! WF 1.17 WZ 1.00* ! ! ! Correcting IF 2. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.97 GG 1.00* HN 0.94 ! KK 1.02 KP 0.96 LA 0.99 MA 1.00* ! MK 0.97 NL 1.04 ON 1.00* OV 0.97 ! PT 1.01 SC 1.00* TC 1.00* TS 1.00* ! WF 1.14 WZ 1.00* ! ! A total of 54 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 FD 0.98 GG 1.00* HN 0.98 ! KK 1.03 KP 0.98 LA 0.99 MA 1.13 ! MK 0.97 NL 1.08 ON 1.07 OV 0.97 ! PT 1.01 SC 0.92 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! 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* ! ! Telescope amplitude corrections in sub-array 4: ! 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 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 45 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 FD 1.00* GG 1.00* HN 0.91 ! KK 1.03 KP 1.00 LA 0.94 MA 1.00* ! MK 1.04 NL 0.88 ON 1.00* OV 0.95 ! PT 0.97 SC 1.00* TC 1.00* TS 0.92 ! WF 1.00* WZ 1.00* ! ! A total of 6 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 1.10 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 1.47 ON 1.10 OV 1.00* ! PT 1.00* SC 0.92 TC 1.00* TS 1.00* ! WF 1.16 WZ 1.00* ! ! ! Correcting IF 3. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 0.96 GG 1.00* HN 0.94 ! KK 1.10 KP 1.01 LA 1.00 MA 1.00* ! MK 0.96 NL 1.02 ON 1.00* OV 1.01 ! PT 1.04 SC 1.00* TC 1.00* TS 1.00* ! WF 1.06 WZ 1.00* ! ! A total of 54 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.97 GG 1.00* HN 0.98 ! KK 1.07 KP 1.02 LA 1.01 MA 1.18 ! MK 0.98 NL 1.08 ON 1.04 OV 1.01 ! PT 1.04 SC 0.95 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! 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* ! ! Telescope amplitude corrections in sub-array 4: ! 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 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 45 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.04 FD 1.00* GG 1.00* HN 0.91 ! KK 1.08 KP 1.03 LA 0.95 MA 1.00* ! MK 1.05 NL 0.88 ON 1.00* OV 0.99 ! PT 0.99 SC 1.00* TC 1.00* TS 0.90 ! WF 1.00* WZ 1.00* ! ! A total of 6 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 1.07 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 1.46 ON 1.07 OV 1.00* ! PT 1.00* SC 0.95 TC 1.00* TS 1.00* ! WF 1.07 WZ 1.00* ! ! ! Correcting IF 4. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.94 GG 1.00* HN 0.96 ! KK 1.06 KP 0.96 LA 0.98 MA 1.00* ! MK 1.00 NL 1.03 ON 1.00* OV 1.00 ! PT 1.05 SC 1.00* TC 1.00* TS 1.00* ! WF 1.06 WZ 1.00* ! ! A total of 54 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.95 GG 1.00* HN 1.02 ! KK 1.04 KP 0.97 LA 0.98 MA 1.19 ! MK 1.00 NL 1.09 ON 1.35 OV 1.00 ! PT 1.05 SC 0.99 TC 1.00* TS 1.00* ! WF 1.00* WZ 1.00* ! ! 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* ! ! Telescope amplitude corrections in sub-array 4: ! 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 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 45 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.02 FD 1.00* GG 1.00* HN 0.94 ! KK 1.05 KP 0.99 LA 0.93 MA 1.00* ! MK 1.09 NL 0.89 ON 1.00* OV 0.99 ! PT 1.00 SC 1.00* TC 1.00* TS 0.92 ! WF 1.00* WZ 1.00* ! ! A total of 6 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 1.10 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 1.47 ON 1.05 OV 1.00* ! PT 1.00* SC 1.01 TC 1.00* TS 1.00* ! WF 1.07 WZ 1.00* ! ! ! Fit before self-cal, rms=0.375706Jy sigma=0.003285 ! Fit after self-cal, rms=0.261312Jy sigma=0.002198 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! Estimated beam: bmin=0.8233 mas, bmaj=3.071 mas, bpa=-11 degrees ! Estimated noise=617.621 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 = 0.022444 Jy ! Component: 100 - total flux cleaned = 0.019561 Jy ! Component: 150 - total flux cleaned = 0.0168144 Jy ! Component: 200 - total flux cleaned = 0.0167949 Jy ! Total flux subtracted in 200 components = 0.0167949 Jy ! Clean residual min=-0.018488 max=0.015551 Jy/beam ! Clean residual mean=0.000127 rms=0.004846 Jy/beam ! Combined flux in latest and established models = 3.00869 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 62 components and 3.00869 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.255354Jy sigma=0.002127 ! Fit after self-cal, rms=0.255745Jy sigma=0.002118 ! Inverting map ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 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=0.255745Jy sigma=0.002118 ! Fit after self-cal, rms=0.241728Jy sigma=0.001855 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! Estimated beam: bmin=0.8252 mas, bmaj=3.072 mas, bpa=-11.06 degrees ! Estimated noise=616.694 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00142967 Jy ! Component: 100 - total flux cleaned = -0.00293234 Jy ! Component: 150 - total flux cleaned = -0.00323148 Jy ! Component: 200 - total flux cleaned = -0.00350348 Jy ! Total flux subtracted in 200 components = -0.00350348 Jy ! Clean residual min=-0.010654 max=0.008061 Jy/beam ! Clean residual mean=0.000133 rms=0.002326 Jy/beam ! Combined flux in latest and established models = 3.00518 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 68 components and 3.00518 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.240112Jy sigma=0.001838 ! Fit after self-cal, rms=0.240047Jy sigma=0.001836 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 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 = -0.000512594 Jy ! Component: 100 - total flux cleaned = -0.000223849 Jy ! Component: 150 - total flux cleaned = -0.0002109 Jy ! Component: 200 - total flux cleaned = -0.000203269 Jy ! Total flux subtracted in 200 components = -0.000203269 Jy ! Clean residual min=-0.009150 max=0.007446 Jy/beam ! Clean residual mean=0.000137 rms=0.002174 Jy/beam ! Combined flux in latest and established models = 3.00498 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 69 components and 3.00498 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.239297Jy sigma=0.001829 ! Fit after self-cal, rms=0.239179Jy sigma=0.001828 ! Inverting map ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 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=0.239179Jy sigma=0.001828 ! Fit after self-cal, rms=0.240084Jy sigma=0.001826 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! Estimated beam: bmin=0.8263 mas, bmaj=3.073 mas, bpa=-11.06 degrees ! Estimated noise=616.297 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00491862 Jy ! Component: 100 - total flux cleaned = -0.00514064 Jy ! Component: 150 - total flux cleaned = -0.00493351 Jy ! Component: 200 - total flux cleaned = -0.00493767 Jy ! Total flux subtracted in 200 components = -0.00493767 Jy ! Clean residual min=-0.007390 max=0.006975 Jy/beam ! Clean residual mean=0.000159 rms=0.001961 Jy/beam ! Combined flux in latest and established models = 3.00004 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 72 components and 3.00004 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.239360Jy sigma=0.001819 ! Fit after self-cal, rms=0.239306Jy sigma=0.001818 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 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 = -0.000253921 Jy ! Component: 100 - total flux cleaned = 8.62738e-05 Jy ! Component: 150 - total flux cleaned = 0.000246973 Jy ! Component: 200 - total flux cleaned = 0.00024521 Jy ! Total flux subtracted in 200 components = 0.00024521 Jy ! Clean residual min=-0.006728 max=0.006606 Jy/beam ! Clean residual mean=0.000154 rms=0.001881 Jy/beam ! Combined flux in latest and established models = 3.00029 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 75 components and 3.00029 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.238893Jy sigma=0.001814 ! Fit after self-cal, rms=0.238815Jy sigma=0.001814 ! Inverting map ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 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=0.238815Jy sigma=0.001814 ! Fit after self-cal, rms=0.239514Jy sigma=0.001813 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! Estimated beam: bmin=2.198 mas, bmaj=3.902 mas, bpa=-5.201 degrees ! Estimated noise=725.97 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00638336 Jy ! Component: 100 - total flux cleaned = -0.00737105 Jy ! Component: 150 - total flux cleaned = -0.00757365 Jy ! Component: 200 - total flux cleaned = -0.0076662 Jy ! Total flux subtracted in 200 components = -0.0076662 Jy ! Clean residual min=-0.005148 max=0.006106 Jy/beam ! Clean residual mean=0.000528 rms=0.001973 Jy/beam ! Combined flux in latest and established models = 2.99262 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 80 components and 2.99262 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.239437Jy sigma=0.001812 ! Fit after self-cal, rms=0.239367Jy sigma=0.001811 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 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 = -0.000198222 Jy ! Component: 100 - total flux cleaned = -0.000194318 Jy ! Component: 150 - total flux cleaned = -0.000296935 Jy ! Component: 200 - total flux cleaned = -0.000343246 Jy ! Total flux subtracted in 200 components = -0.000343246 Jy ! Clean residual min=-0.004814 max=0.005986 Jy/beam ! Clean residual mean=0.000542 rms=0.001969 Jy/beam ! Combined flux in latest and established models = 2.99228 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 85 components and 2.99228 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.239383Jy sigma=0.001811 ! Fit after self-cal, rms=0.239326Jy sigma=0.001810 ! Inverting map ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 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 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! Estimated beam: bmin=0.8272 mas, bmaj=3.075 mas, bpa=-11.06 degrees ! Estimated noise=616.079 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8272 x 3.075 at -11.06 degrees (North through East) ! Clean map min=-0.0055854 max=2.5575 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=0.239326Jy sigma=0.001810 ! Fit after self-cal, rms=0.213835Jy sigma=0.001537 ! Inverting map and beam ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! Estimated beam: bmin=0.8267 mas, bmaj=3.079 mas, bpa=-11.07 degrees ! Estimated noise=615.138 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00465671 Jy ! Component: 100 - total flux cleaned = -0.00529957 Jy ! Component: 150 - total flux cleaned = -0.00544754 Jy ! Component: 200 - total flux cleaned = -0.00558812 Jy ! Total flux subtracted in 200 components = -0.00558812 Jy ! Clean residual min=-0.005255 max=0.005443 Jy/beam ! Clean residual mean=0.000123 rms=0.001464 Jy/beam ! Combined flux in latest and established models = 2.98669 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 86 components and 2.98669 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.213445Jy sigma=0.001534 ! Fit after self-cal, rms=0.213395Jy sigma=0.001534 ! Inverting map ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000287653 Jy ! Component: 100 - total flux cleaned = -0.000406338 Jy ! Component: 150 - total flux cleaned = -0.000520456 Jy ! Component: 200 - total flux cleaned = -0.000631451 Jy ! Total flux subtracted in 200 components = -0.000631451 Jy ! Clean residual min=-0.004970 max=0.005348 Jy/beam ! Clean residual mean=0.000136 rms=0.001425 Jy/beam ! Combined flux in latest and established models = 2.98606 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 87 components and 2.98606 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.213187Jy sigma=0.001532 ! Fit after self-cal, rms=0.213145Jy sigma=0.001531 ! Inverting map ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.213145Jy sigma=0.001531 ! Fit after self-cal, rms=0.213620Jy sigma=0.001531 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 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! Estimated beam: bmin=0.6366 mas, bmaj=2.419 mas, bpa=-8.501 degrees ! Estimated noise=998.983 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.93301 Jy ! Component: 100 - total flux cleaned = 2.40379 Jy ! Component: 150 - total flux cleaned = 2.61336 Jy ! Component: 200 - total flux cleaned = 2.73061 Jy ! Total flux subtracted in 200 components = 2.73061 Jy ! Clean residual min=-0.019589 max=0.060092 Jy/beam ! Clean residual mean=0.001480 rms=0.008658 Jy/beam ! Combined flux in latest and established models = 2.73061 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 18 model components to the UV plane model. ! The established model now contains 18 components and 2.73061 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! Estimated beam: bmin=0.8274 mas, bmaj=3.08 mas, bpa=-11.07 degrees ! Estimated noise=614.935 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 = 0.106192 Jy ! Component: 100 - total flux cleaned = 0.163247 Jy ! Component: 150 - total flux cleaned = 0.196328 Jy ! Component: 200 - total flux cleaned = 0.216365 Jy ! Total flux subtracted in 200 components = 0.216365 Jy ! Clean residual min=-0.005585 max=0.010437 Jy/beam ! Clean residual mean=0.000868 rms=0.002417 Jy/beam ! Combined flux in latest and established models = 2.94698 Jy ! Adding 38 model components to the UV plane model. ! The established model now contains 50 components and 2.94698 Jy ! Inverting map ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0125511 Jy ! Component: 100 - total flux cleaned = 0.0205559 Jy ! Component: 150 - total flux cleaned = 0.0228427 Jy ! Component: 200 - total flux cleaned = 0.024665 Jy ! Total flux subtracted in 200 components = 0.024665 Jy ! Clean residual min=-0.004637 max=0.005452 Jy/beam ! Clean residual mean=0.000353 rms=0.001485 Jy/beam ! Combined flux in latest and established models = 2.97164 Jy ! Adding 18 model components to the UV plane model. ! The established model now contains 60 components and 2.97164 Jy ! Inverting map ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 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 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! Estimated beam: bmin=2.199 mas, bmaj=3.908 mas, bpa=-5.226 degrees ! Estimated noise=724.187 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00275058 Jy ! Component: 100 - total flux cleaned = 0.00407186 Jy ! Component: 150 - total flux cleaned = 0.00424885 Jy ! Component: 200 - total flux cleaned = 0.00434554 Jy ! Total flux subtracted in 200 components = 0.00434554 Jy ! Clean residual min=-0.004175 max=0.005044 Jy/beam ! Clean residual mean=0.000542 rms=0.001742 Jy/beam ! Combined flux in latest and established models = 2.97599 Jy flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 8.87133e-05 Jy ! Component: 100 - total flux cleaned = 0.000196145 Jy ! Component: 150 - total flux cleaned = 0.000245647 Jy ! Component: 200 - total flux cleaned = 0.000292644 Jy ! Total flux subtracted in 200 components = 0.000292644 Jy ! Clean residual min=-0.004145 max=0.004998 Jy/beam ! Clean residual mean=0.000530 rms=0.001732 Jy/beam ! Combined flux in latest and established models = 2.97628 Jy ! Adding 16 model components to the UV plane model. ! The established model now contains 74 components and 2.97628 Jy ! Inverting map ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! Estimated beam: bmin=0.8274 mas, bmaj=3.08 mas, bpa=-11.07 degrees ! Estimated noise=614.935 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000689853 Jy ! Component: 100 - total flux cleaned = -0.00067465 Jy ! Component: 150 - total flux cleaned = -0.000451404 Jy ! Component: 200 - total flux cleaned = -0.000348554 Jy ! Total flux subtracted in 200 components = -0.000348554 Jy ! Clean residual min=-0.004611 max=0.005132 Jy/beam ! Clean residual mean=0.000264 rms=0.001400 Jy/beam ! Combined flux in latest and established models = 2.97593 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 79 components and 2.97593 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.213297Jy sigma=0.001529 ! Fit after self-cal, rms=0.213069Jy sigma=0.001526 wmodel J1337-1257_X_2003_06_18_pus_map.mod ! Writing 79 model components to file: J1337-1257_X_2003_06_18_pus_map.mod wobs J1337-1257_X_2003_06_18_pus_uvs.fits ! Writing UV FITS file: J1337-1257_X_2003_06_18_pus_uvs.fits wwins J1337-1257_X_2003_06_18_pus_map.win ! wwins: Wrote 2 windows to J1337-1257_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 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.00220657 Jy ! Component: 100 - total flux cleaned = 0.00283118 Jy ! Component: 150 - total flux cleaned = 0.00304988 Jy ! Component: 200 - total flux cleaned = 0.00311631 Jy ! Component: 250 - total flux cleaned = 0.00331342 Jy ! Component: 300 - total flux cleaned = 0.00363221 Jy ! Component: 350 - total flux cleaned = 0.00393774 Jy ! Component: 400 - total flux cleaned = 0.00399679 Jy ! Component: 450 - total flux cleaned = 0.00388083 Jy ! Component: 500 - total flux cleaned = 0.0039372 Jy ! Component: 550 - total flux cleaned = 0.00382582 Jy ! Component: 600 - total flux cleaned = 0.00382596 Jy ! Component: 650 - total flux cleaned = 0.00382597 Jy ! Component: 700 - total flux cleaned = 0.00372091 Jy ! Component: 750 - total flux cleaned = 0.00361816 Jy ! Component: 800 - total flux cleaned = 0.00356769 Jy ! Component: 850 - total flux cleaned = 0.00341808 Jy ! Component: 900 - total flux cleaned = 0.00336884 Jy ! Component: 950 - total flux cleaned = 0.00336877 Jy ! Component: 1000 - total flux cleaned = 0.00346413 Jy ! Total flux subtracted in 1024 components = 0.00332257 Jy ! Clean residual min=-0.002616 max=0.002620 Jy/beam ! Clean residual mean=0.000121 rms=0.001014 Jy/beam ! Combined flux in latest and established models = 2.97926 Jy keep ! Adding 63 model components to the UV plane model. ! The established model now contains 141 components and 2.97926 Jy wmap "J1337-1257_X_2003_06_18_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8274 x 3.08 at -11.07 degrees (North through East) ! Clean map min=-0.0036421 max=2.5579 Jy/beam ! Writing clean map to FITS file: J1337-1257_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 2.55789 invert ! Inverting map ! Your choice of large map pixels excluded 1.08% of the data. ! The x-axis pixel size should ideally be below 0.1822 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00102329 device "J1337-1257_X_2003_06_18_pus\_map.eps/VPS" ! Attempting to open device: 'J1337-1257_X_2003_06_18_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.120015 0.120015 0.24003 0.480061 0.960121 1.92024 3.84049 7.68097 15.3619 30.7239 61.4478 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.003 print "peak=",int(1000*peak_flux)/1000 ! peak= 2.557 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8274 x 3.08 at -11.07 degrees (North through East) ! Clean map min=-0.0036421 max=2.5579 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1337-1257_X_2003_06_18_pus\_map.gif/vgif" ! Attempting to open device: 'J1337-1257_X_2003_06_18_pus_map.gif/vgif' mapplot cln quit ! Quitting program ! Log file J1337-1257_X_2003_06_18_pus_uvs.log closed on Wed Jan 17 17:27:08 2007