! Started logfile: J1743-0350_X_2003_05_07_pus_uvs.log on Tue Dec 12 21:55:32 2006 obs J1743-0350_X_2003_05_07_pus_uve.fits ! Reading UV FITS file: J1743-0350_X_2003_05_07_pus_uve.fits ! AN table 1: 8 integrations on 171 of 171 possible baselines. ! AN table 2: 32 integrations on 171 of 171 possible baselines. ! AN table 3: 21 integrations on 171 of 171 possible baselines. ! AN table 4: 9 integrations on 171 of 171 possible baselines. ! AN table 5: 2 integrations on 171 of 171 possible baselines. ! Apparent sampling: 0.107943 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 1739 lines of history. ! ! Reading 5316 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 130 telescope corrections were flagged in sub-array 1. ! A total of 392 telescope corrections were flagged in sub-array 2. ! A total of 320 telescope corrections were flagged in sub-array 3. ! A total of 159 telescope corrections were flagged in sub-array 4. ! A total of 38 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 130 telescope corrections were flagged in sub-array 1. ! A total of 393 telescope corrections were flagged in sub-array 2. ! A total of 320 telescope corrections were flagged in sub-array 3. ! A total of 159 telescope corrections were flagged in sub-array 4. ! A total of 38 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 130 telescope corrections were flagged in sub-array 1. ! A total of 393 telescope corrections were flagged in sub-array 2. ! A total of 320 telescope corrections were flagged in sub-array 3. ! A total of 159 telescope corrections were flagged in sub-array 4. ! A total of 38 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 130 telescope corrections were flagged in sub-array 1. ! A total of 392 telescope corrections were flagged in sub-array 2. ! A total of 320 telescope corrections were flagged in sub-array 3. ! A total of 159 telescope corrections were flagged in sub-array 4. ! A total of 38 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=3.552541Jy sigma=30.370617 ! Fit after self-cal, rms=3.238616Jy sigma=28.918058 ! 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 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! Estimated beam: bmin=0.5291 mas, bmaj=0.7848 mas, bpa=-11.5 degrees ! Estimated noise=2.51162 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 = 2.94734 Jy ! Component: 100 - total flux cleaned = 3.81904 Jy ! Total flux subtracted in 100 components = 3.81904 Jy ! Clean residual min=-0.119401 max=0.402373 Jy/beam ! Clean residual mean=0.000483 rms=0.041486 Jy/beam ! Combined flux in latest and established models = 3.81904 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 10 components and 3.81904 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.926693Jy sigma=8.297506 ! Fit after self-cal, rms=0.925237Jy sigma=8.292446 ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.467548 Jy ! Component: 100 - total flux cleaned = 0.746388 Jy ! Total flux subtracted in 100 components = 0.746388 Jy ! Clean residual min=-0.071283 max=0.144906 Jy/beam ! Clean residual mean=-0.000287 rms=0.020321 Jy/beam ! Combined flux in latest and established models = 4.56543 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 19 components and 4.56543 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.510899Jy sigma=4.238306 ! Fit after self-cal, rms=0.508194Jy sigma=4.228612 ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.176449 Jy ! Component: 100 - total flux cleaned = 0.287703 Jy ! Total flux subtracted in 100 components = 0.287703 Jy ! Clean residual min=-0.051739 max=0.069127 Jy/beam ! Clean residual mean=-0.000581 rms=0.014662 Jy/beam ! Combined flux in latest and established models = 4.85313 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 21 components and 4.85313 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.423404Jy sigma=3.212614 ! Fit after self-cal, rms=0.422015Jy sigma=3.204307 ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 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 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! Estimated beam: bmin=0.6682 mas, bmaj=1.084 mas, bpa=-7.901 degrees ! Estimated noise=1.5175 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 = 0.102352 Jy ! Component: 100 - total flux cleaned = 0.146836 Jy ! Component: 150 - total flux cleaned = 0.16788 Jy ! Component: 200 - total flux cleaned = 0.175878 Jy ! Total flux subtracted in 200 components = 0.175878 Jy ! Clean residual min=-0.052755 max=0.037416 Jy/beam ! Clean residual mean=-0.005657 rms=0.013408 Jy/beam ! Combined flux in latest and established models = 5.02901 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 30 components and 5.02901 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.409546Jy sigma=2.919128 ! Fit after self-cal, rms=0.408955Jy sigma=2.916954 ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* GG 1.00* HN 1.00* ! KK 1.00* KP 1.00* LA 1.05 MA 1.05 ! MC 1.10 MK 1.00* NL 1.07 ON 1.08 ! OV 1.00* PT 1.12 SC 1.00* TC 1.00* ! TS 1.00* WF 1.00* WZ 1.00 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.97 GG 1.00* HN 1.04 ! KK 1.00* KP 1.10 LA 0.96 MA 1.04 ! MC 1.16 MK 0.99 NL 0.99 ON 1.09 ! OV 0.97 PT 0.98 SC 1.01 TC 1.01 ! TS 1.00* WF 1.03 WZ 0.99 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00 GG 1.00* HN 0.95 ! KK 1.00* KP 1.13 LA 1.00 MA 1.02 ! MC 1.09 MK 1.00* NL 1.07 ON 1.05 ! OV 1.00* PT 1.03 SC 0.98 TC 1.03 ! TS 1.00* WF 0.99 WZ 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.94 FD 1.00* GG 1.00* HN 1.03 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MC 1.00* MK 1.00* NL 1.04 ON 1.00* ! OV 1.00* PT 1.00* SC 1.02 TC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! 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* ! MC 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. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* GG 1.00* HN 1.00* ! KK 1.00* KP 1.00* LA 1.05 MA 1.04 ! MC 1.10 MK 1.00* NL 1.02 ON 1.05 ! OV 1.00* PT 1.14 SC 1.00* TC 1.00* ! TS 1.00* WF 1.00* WZ 1.00 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 0.97 GG 1.00* HN 1.06 ! KK 1.00* KP 1.03 LA 0.97 MA 1.03 ! MC 1.09 MK 0.99 NL 0.95 ON 1.11 ! OV 0.95 PT 1.01 SC 0.97 TC 1.06 ! TS 1.00* WF 1.02 WZ 1.02 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.02 GG 1.00* HN 1.01 ! KK 1.00* KP 1.07 LA 0.99 MA 1.01 ! MC 1.06 MK 1.00* NL 1.02 ON 1.01 ! OV 1.00* PT 1.03 SC 0.95 TC 1.05 ! TS 1.00* WF 1.03 WZ 1.02 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.95 FD 1.00* GG 1.00* HN 1.06 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MC 1.00* MK 1.00* NL 0.98 ON 1.00* ! OV 1.00* PT 1.00* SC 1.00 TC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! 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* ! MC 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. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* GG 1.00* HN 1.00* ! KK 1.00* KP 1.00* LA 1.04 MA 1.06 ! MC 1.00 MK 1.00* NL 0.98 ON 1.07 ! OV 1.00* PT 1.17 SC 1.00* TC 1.00* ! TS 1.00* WF 1.00* WZ 0.98 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 0.95 GG 1.00* HN 1.06 ! KK 1.00* KP 0.96 LA 0.96 MA 1.01 ! MC 1.10 MK 0.96 NL 0.93 ON 1.10 ! OV 0.98 PT 1.04 SC 0.97 TC 0.96 ! TS 1.00* WF 1.03 WZ 0.95 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 0.98 GG 1.00* HN 0.95 ! KK 1.00* KP 0.98 LA 1.00 MA 1.02 ! MC 0.99 MK 1.00* NL 1.00 ON 1.01 ! OV 1.00* PT 1.07 SC 0.97 TC 0.95 ! TS 1.00* WF 1.01 WZ 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 FD 1.00* GG 1.00* HN 1.06 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MC 1.00* MK 1.00* NL 0.96 ON 1.00* ! OV 1.00* PT 1.00* SC 0.99 TC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! 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* ! MC 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. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* GG 1.00* HN 1.00* ! KK 1.00* KP 1.00* LA 1.04 MA 1.10 ! MC 0.98 MK 1.00* NL 0.98 ON 1.05 ! OV 1.00* PT 1.17 SC 1.00* TC 1.00* ! TS 1.00* WF 1.00* WZ 0.99 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.93 GG 1.00* HN 1.08 ! KK 1.00* KP 1.03 LA 0.94 MA 1.07 ! MC 1.37 MK 1.02 NL 0.92 ON 1.01 ! OV 0.98 PT 1.04 SC 1.03 TC 1.00 ! TS 1.00* WF 1.01 WZ 0.96 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 0.95 GG 1.00* HN 0.98 ! KK 1.00* KP 1.05 LA 0.96 MA 1.07 ! MC 1.33 MK 1.00* NL 1.00 ON 0.99 ! OV 1.00* PT 1.08 SC 1.01 TC 1.01 ! TS 1.00* WF 0.99 WZ 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 FD 1.00* GG 1.00* HN 1.10 ! KK 1.00* KP 1.00* LA 1.00* MA 1.00* ! MC 1.00* MK 1.00* NL 0.95 ON 1.00* ! OV 1.00* PT 1.00* SC 1.07 TC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! 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* ! MC 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=0.408955Jy sigma=2.916954 ! Fit after self-cal, rms=0.295970Jy sigma=1.683640 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! Estimated beam: bmin=0.6735 mas, bmaj=1.084 mas, bpa=-7.667 degrees ! Estimated noise=1.51563 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 = -0.0332094 Jy ! Component: 100 - total flux cleaned = -0.0378884 Jy ! Component: 150 - total flux cleaned = -0.0392519 Jy ! Component: 200 - total flux cleaned = -0.0402826 Jy ! Total flux subtracted in 200 components = -0.0402826 Jy ! Clean residual min=-0.031435 max=0.027601 Jy/beam ! Clean residual mean=-0.000368 rms=0.007157 Jy/beam ! Combined flux in latest and established models = 4.98873 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 32 components and 4.98873 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.290407Jy sigma=1.656482 ! Fit after self-cal, rms=0.289943Jy sigma=1.654100 ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 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=0.289943Jy sigma=1.654100 ! Fit after self-cal, rms=0.260170Jy sigma=1.308615 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! Estimated beam: bmin=0.6768 mas, bmaj=1.085 mas, bpa=-7.707 degrees ! Estimated noise=1.51196 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0232451 Jy ! Component: 100 - total flux cleaned = -0.0274362 Jy ! Component: 150 - total flux cleaned = -0.0284216 Jy ! Component: 200 - total flux cleaned = -0.0292479 Jy ! Total flux subtracted in 200 components = -0.0292479 Jy ! Clean residual min=-0.012771 max=0.017630 Jy/beam ! Clean residual mean=-0.000635 rms=0.003495 Jy/beam ! Combined flux in latest and established models = 4.95948 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 32 components and 4.95948 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.256528Jy sigma=1.293439 ! Fit after self-cal, rms=0.256175Jy sigma=1.291672 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 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 (0.2, -1.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0149305 Jy ! Component: 100 - total flux cleaned = 0.0134482 Jy ! Component: 150 - total flux cleaned = 0.0121742 Jy ! Component: 200 - total flux cleaned = 0.010616 Jy ! Total flux subtracted in 200 components = 0.010616 Jy ! Clean residual min=-0.012533 max=0.012340 Jy/beam ! Clean residual mean=-0.000798 rms=0.003232 Jy/beam ! Combined flux in latest and established models = 4.9701 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 41 components and 4.9701 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.253162Jy sigma=1.272762 ! Fit after self-cal, rms=0.252429Jy sigma=1.269297 ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! Added new window around map position (-0.6, -8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0115075 Jy ! Component: 100 - total flux cleaned = 0.0123366 Jy ! Component: 150 - total flux cleaned = 0.0123304 Jy ! Component: 200 - total flux cleaned = 0.0119949 Jy ! Total flux subtracted in 200 components = 0.0119949 Jy ! Clean residual min=-0.012190 max=0.011769 Jy/beam ! Clean residual mean=-0.001021 rms=0.003057 Jy/beam ! Combined flux in latest and established models = 4.98209 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 48 components and 4.98209 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.250587Jy sigma=1.260135 ! Fit after self-cal, rms=0.250225Jy sigma=1.258711 ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 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=0.250225Jy sigma=1.258711 ! Fit after self-cal, rms=0.246286Jy sigma=1.185025 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! Estimated beam: bmin=0.6783 mas, bmaj=1.088 mas, bpa=-7.681 degrees ! Estimated noise=1.51121 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0061979 Jy ! Component: 100 - total flux cleaned = -0.0067322 Jy ! Component: 150 - total flux cleaned = -0.00641076 Jy ! Component: 200 - total flux cleaned = -0.00581012 Jy ! Total flux subtracted in 200 components = -0.00581012 Jy ! Clean residual min=-0.008810 max=0.009789 Jy/beam ! Clean residual mean=0.000186 rms=0.002482 Jy/beam ! Combined flux in latest and established models = 4.97628 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 52 components and 4.97628 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.243558Jy sigma=1.176568 ! Fit after self-cal, rms=0.243208Jy sigma=1.175034 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 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 = 0.00305807 Jy ! Component: 100 - total flux cleaned = 0.00334151 Jy ! Component: 150 - total flux cleaned = 0.00361728 Jy ! Component: 200 - total flux cleaned = 0.00361115 Jy ! Total flux subtracted in 200 components = 0.00361115 Jy ! Clean residual min=-0.009071 max=0.008879 Jy/beam ! Clean residual mean=0.000121 rms=0.002419 Jy/beam ! Combined flux in latest and established models = 4.97989 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 54 components and 4.97989 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.242206Jy sigma=1.171381 ! Fit after self-cal, rms=0.242026Jy sigma=1.170899 ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 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=0.242026Jy sigma=1.170899 ! Fit after self-cal, rms=0.242664Jy sigma=1.164654 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! Estimated beam: bmin=2.229 mas, bmaj=3.432 mas, bpa=-11.33 degrees ! Estimated noise=1.97718 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00915161 Jy ! Component: 100 - total flux cleaned = -0.00993007 Jy ! Component: 150 - total flux cleaned = -0.0104229 Jy ! Component: 200 - total flux cleaned = -0.0107241 Jy ! Total flux subtracted in 200 components = -0.0107241 Jy ! Clean residual min=-0.007852 max=0.008869 Jy/beam ! Clean residual mean=0.000575 rms=0.003055 Jy/beam ! Combined flux in latest and established models = 4.96917 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 61 components and 4.96917 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.241564Jy sigma=1.168338 ! Fit after self-cal, rms=0.241453Jy sigma=1.167966 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 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 = 0.000667799 Jy ! Component: 100 - total flux cleaned = 0.000487886 Jy ! Component: 150 - total flux cleaned = 0.00033476 Jy ! Component: 200 - total flux cleaned = 0.000200082 Jy ! Total flux subtracted in 200 components = 0.000200082 Jy ! Clean residual min=-0.007611 max=0.008852 Jy/beam ! Clean residual mean=0.000557 rms=0.003043 Jy/beam ! Combined flux in latest and established models = 4.96937 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 64 components and 4.96937 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.241133Jy sigma=1.167952 ! Fit after self-cal, rms=0.241078Jy sigma=1.167791 ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 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 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! Estimated beam: bmin=0.6792 mas, bmaj=1.09 mas, bpa=-7.663 degrees ! Estimated noise=1.50952 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6792 x 1.09 at -7.663 degrees (North through East) ! Clean map min=-0.0076421 max=4.0357 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=0.241078Jy sigma=1.167791 ! Fit after self-cal, rms=0.205749Jy sigma=0.793119 ! Inverting map and beam ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! Estimated beam: bmin=0.6792 mas, bmaj=1.089 mas, bpa=-7.641 degrees ! Estimated noise=1.50831 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00510907 Jy ! Component: 100 - total flux cleaned = -0.00584812 Jy ! Component: 150 - total flux cleaned = -0.00671906 Jy ! Component: 200 - total flux cleaned = -0.0073244 Jy ! Total flux subtracted in 200 components = -0.0073244 Jy ! Clean residual min=-0.006535 max=0.007290 Jy/beam ! Clean residual mean=0.000187 rms=0.001769 Jy/beam ! Combined flux in latest and established models = 4.96204 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 66 components and 4.96204 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.204691Jy sigma=0.787213 ! Fit after self-cal, rms=0.204544Jy sigma=0.786667 ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000645191 Jy ! Component: 100 - total flux cleaned = 0.000258888 Jy ! Component: 150 - total flux cleaned = 7.81271e-05 Jy ! Component: 200 - total flux cleaned = -8.80183e-05 Jy ! Total flux subtracted in 200 components = -8.80183e-05 Jy ! Clean residual min=-0.006735 max=0.006274 Jy/beam ! Clean residual mean=0.000189 rms=0.001737 Jy/beam ! Combined flux in latest and established models = 4.96196 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 69 components and 4.96196 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.204039Jy sigma=0.783615 ! Fit after self-cal, rms=0.203951Jy sigma=0.783400 ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.203951Jy sigma=0.783400 ! Fit after self-cal, rms=0.203875Jy sigma=0.780841 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 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! Estimated beam: bmin=0.5381 mas, bmaj=0.787 mas, bpa=-11.31 degrees ! Estimated noise=2.52138 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.95754 Jy ! Component: 100 - total flux cleaned = 3.80738 Jy ! Component: 150 - total flux cleaned = 4.23681 Jy ! Component: 200 - total flux cleaned = 4.48782 Jy ! Total flux subtracted in 200 components = 4.48782 Jy ! Clean residual min=-0.035788 max=0.128287 Jy/beam ! Clean residual mean=0.000472 rms=0.013766 Jy/beam ! Combined flux in latest and established models = 4.48782 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 4.48783 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! Estimated beam: bmin=0.6799 mas, bmaj=1.09 mas, bpa=-7.627 degrees ! Estimated noise=1.508 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 = 0.242328 Jy ! Component: 100 - total flux cleaned = 0.350445 Jy ! Component: 150 - total flux cleaned = 0.404891 Jy ! Component: 200 - total flux cleaned = 0.434113 Jy ! Total flux subtracted in 200 components = 0.434113 Jy ! Clean residual min=-0.007437 max=0.020198 Jy/beam ! Clean residual mean=0.000794 rms=0.002552 Jy/beam ! Combined flux in latest and established models = 4.92194 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 35 components and 4.92194 Jy ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! Added new window around map position (0.2, 0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0197262 Jy ! Component: 100 - total flux cleaned = 0.0280248 Jy ! Component: 150 - total flux cleaned = 0.0317142 Jy ! Component: 200 - total flux cleaned = 0.0320824 Jy ! Total flux subtracted in 200 components = 0.0320824 Jy ! Clean residual min=-0.007555 max=0.006245 Jy/beam ! Clean residual mean=0.000277 rms=0.001867 Jy/beam ! Combined flux in latest and established models = 4.95402 Jy ! Adding 19 model components to the UV plane model. ! The established model now contains 50 components and 4.95402 Jy ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 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 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! Estimated beam: bmin=2.23 mas, bmaj=3.431 mas, bpa=-11.34 degrees ! Estimated noise=1.97242 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00191494 Jy ! Component: 100 - total flux cleaned = 0.00116769 Jy ! Component: 150 - total flux cleaned = 0.000919612 Jy ! Component: 200 - total flux cleaned = 0.000604283 Jy ! Total flux subtracted in 200 components = 0.000604283 Jy ! Clean residual min=-0.005378 max=0.006574 Jy/beam ! Clean residual mean=0.000609 rms=0.002183 Jy/beam ! Combined flux in latest and established models = 4.95463 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 = -0.000173829 Jy ! Component: 100 - total flux cleaned = -0.000322769 Jy ! Component: 150 - total flux cleaned = -0.000322551 Jy ! Component: 200 - total flux cleaned = -0.000381025 Jy ! Total flux subtracted in 200 components = -0.000381025 Jy ! Clean residual min=-0.005239 max=0.006403 Jy/beam ! Clean residual mean=0.000617 rms=0.002133 Jy/beam ! Combined flux in latest and established models = 4.95425 Jy ! Adding 19 model components to the UV plane model. ! The established model now contains 67 components and 4.95425 Jy ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! Estimated beam: bmin=0.6799 mas, bmaj=1.09 mas, bpa=-7.627 degrees ! Estimated noise=1.508 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0025808 Jy ! Component: 100 - total flux cleaned = 0.00260008 Jy ! Component: 150 - total flux cleaned = 0.00289626 Jy ! Component: 200 - total flux cleaned = 0.00263508 Jy ! Total flux subtracted in 200 components = 0.00263508 Jy ! Clean residual min=-0.006255 max=0.006244 Jy/beam ! Clean residual mean=0.000214 rms=0.001732 Jy/beam ! Combined flux in latest and established models = 4.95688 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 73 components and 4.95688 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.203403Jy sigma=0.788295 ! Fit after self-cal, rms=0.203301Jy sigma=0.783514 wmodel J1743-0350_X_2003_05_07_pus_map.mod ! Writing 73 model components to file: J1743-0350_X_2003_05_07_pus_map.mod wobs J1743-0350_X_2003_05_07_pus_uvs.fits ! Writing UV FITS file: J1743-0350_X_2003_05_07_pus_uvs.fits wwins J1743-0350_X_2003_05_07_pus_map.win ! wwins: Wrote 4 windows to J1743-0350_X_2003_05_07_pus_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000618039 Jy ! Component: 100 - total flux cleaned = 0.00115545 Jy ! Component: 150 - total flux cleaned = 0.00166468 Jy ! Component: 200 - total flux cleaned = 0.00195876 Jy ! Component: 250 - total flux cleaned = 0.00234132 Jy ! Component: 300 - total flux cleaned = 0.00243457 Jy ! Component: 350 - total flux cleaned = 0.00279833 Jy ! Component: 400 - total flux cleaned = 0.0028872 Jy ! Component: 450 - total flux cleaned = 0.00314995 Jy ! Component: 500 - total flux cleaned = 0.00332248 Jy ! Component: 550 - total flux cleaned = 0.00366248 Jy ! Component: 600 - total flux cleaned = 0.00399665 Jy ! Component: 650 - total flux cleaned = 0.00424364 Jy ! Component: 700 - total flux cleaned = 0.00440752 Jy ! Component: 750 - total flux cleaned = 0.00481166 Jy ! Component: 800 - total flux cleaned = 0.0051305 Jy ! Component: 850 - total flux cleaned = 0.00544614 Jy ! Component: 900 - total flux cleaned = 0.00560218 Jy ! Component: 950 - total flux cleaned = 0.00598851 Jy ! Component: 1000 - total flux cleaned = 0.00621826 Jy ! Total flux subtracted in 1024 components = 0.00637021 Jy ! Clean residual min=-0.003789 max=0.004302 Jy/beam ! Clean residual mean=0.000142 rms=0.001420 Jy/beam ! Combined flux in latest and established models = 4.96325 Jy keep ! Adding 72 model components to the UV plane model. ! The established model now contains 134 components and 4.96325 Jy wmap "J1743-0350_X_2003_05_07_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6799 x 1.09 at -7.627 degrees (North through East) ! Clean map min=-0.0062433 max=4.0272 Jy/beam ! Writing clean map to FITS file: J1743-0350_X_2003_05_07_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 4.02721 invert ! Inverting map ! Your choice of large map pixels excluded 3.1% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! The y-axis pixel size should ideally be below 0.1833 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00142097 device "J1743-0350_X_2003_05_07_pus\_map.eps/VPS" ! Attempting to open device: 'J1743-0350_X_2003_05_07_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.105853 0.105853 0.211705 0.42341 0.846821 1.69364 3.38728 6.77457 13.5491 27.0983 54.1965 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0042 print "peak=",int(1000*peak_flux)/1000 ! peak= 4.027 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6799 x 1.09 at -7.627 degrees (North through East) ! Clean map min=-0.0062433 max=4.0272 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1743-0350_X_2003_05_07_pus\_map.gif/vgif" ! Attempting to open device: 'J1743-0350_X_2003_05_07_pus_map.gif/vgif' mapplot cln quit ! Quitting program ! Log file J1743-0350_X_2003_05_07_pus_uvs.log closed on Tue Dec 12 21:56:04 2006