! Started logfile: J1625-2527_X_2003_05_07_pus_uvs.log on Thu Dec 14 16:07:09 2006 obs J1625-2527_X_2003_05_07_pus_uva.fits ! Reading UV FITS file: J1625-2527_X_2003_05_07_pus_uva.fits ! AN table 1: 120 integrations on 171 of 171 possible baselines. ! AN table 2: 196 integrations on 171 of 171 possible baselines. ! AN table 3: 9 integrations on 171 of 171 possible baselines. ! AN table 4: 160 integrations on 171 of 171 possible baselines. ! AN table 5: 84 integrations on 171 of 171 possible baselines. ! AN table 6: 131 integrations on 171 of 171 possible baselines. ! Apparent sampling: 0.0430159 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1625-2527 ! ! 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 20596 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 2024 telescope corrections were flagged in sub-array 1. ! A total of 3196 telescope corrections were flagged in sub-array 2. ! A total of 171 telescope corrections were flagged in sub-array 3. ! A total of 2834 telescope corrections were flagged in sub-array 4. ! A total of 1051 telescope corrections were flagged in sub-array 5. ! A total of 2129 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 2024 telescope corrections were flagged in sub-array 1. ! A total of 3196 telescope corrections were flagged in sub-array 2. ! A total of 171 telescope corrections were flagged in sub-array 3. ! A total of 2834 telescope corrections were flagged in sub-array 4. ! A total of 1051 telescope corrections were flagged in sub-array 5. ! A total of 2129 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 2024 telescope corrections were flagged in sub-array 1. ! A total of 3196 telescope corrections were flagged in sub-array 2. ! A total of 171 telescope corrections were flagged in sub-array 3. ! A total of 2834 telescope corrections were flagged in sub-array 4. ! A total of 1051 telescope corrections were flagged in sub-array 5. ! A total of 2129 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 2027 telescope corrections were flagged in sub-array 1. ! A total of 3196 telescope corrections were flagged in sub-array 2. ! A total of 171 telescope corrections were flagged in sub-array 3. ! A total of 2834 telescope corrections were flagged in sub-array 4. ! A total of 1051 telescope corrections were flagged in sub-array 5. ! A total of 2129 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.528885Jy sigma=0.010702 ! Fit after self-cal, rms=0.756744Jy sigma=0.005330 ! 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 4.09% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec ! Estimated beam: bmin=0.6143 mas, bmaj=0.8985 mas, bpa=-12.24 degrees ! Estimated noise=1909.04 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 = 1.18265 Jy ! Component: 100 - total flux cleaned = 1.45951 Jy ! Total flux subtracted in 100 components = 1.45951 Jy ! Clean residual min=-0.054970 max=0.098471 Jy/beam ! Clean residual mean=0.001590 rms=0.016547 Jy/beam ! Combined flux in latest and established models = 1.45951 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 1.45951 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.529519Jy sigma=0.002582 ! Fit after self-cal, rms=0.529922Jy sigma=0.002582 ! Inverting map ! Your choice of large map pixels excluded 4.09% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.101425 Jy ! Component: 100 - total flux cleaned = 0.147491 Jy ! Total flux subtracted in 100 components = 0.147491 Jy ! Clean residual min=-0.046399 max=0.047717 Jy/beam ! Clean residual mean=0.001002 rms=0.014323 Jy/beam ! Combined flux in latest and established models = 1.607 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 13 components and 1.607 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.505088Jy sigma=0.002057 ! Fit after self-cal, rms=0.505342Jy sigma=0.002057 ! Inverting map ! Your choice of large map pixels excluded 4.09% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 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 4.09% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec ! Estimated beam: bmin=0.9495 mas, bmaj=1.477 mas, bpa=-18.23 degrees ! Estimated noise=788.018 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 = 0.0689392 Jy ! Component: 100 - total flux cleaned = 0.0936455 Jy ! Component: 150 - total flux cleaned = 0.102677 Jy ! Component: 200 - total flux cleaned = 0.104273 Jy ! Total flux subtracted in 200 components = 0.104273 Jy ! Clean residual min=-0.025039 max=0.034006 Jy/beam ! Clean residual mean=-0.000859 rms=0.009479 Jy/beam ! Combined flux in latest and established models = 1.71127 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 19 components and 1.71128 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.502527Jy sigma=0.001906 ! Fit after self-cal, rms=0.502633Jy sigma=0.001906 ! Inverting map ! Your choice of large map pixels excluded 4.09% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 99 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 1.00* ! KK 0.93 KP 1.05 LA 0.98 MA 0.90 ! MC 1.08 MK 0.93 NL 1.31 ON 1.09 ! OV 0.95 PT 0.99 SC 1.00* TC 0.97 ! TS 1.00* WF 1.00* WZ 0.92 ! ! A total of 45 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.94 GG 1.00* HN 1.09 ! KK 1.02 KP 1.05 LA 0.93 MA 1.02 ! MC 1.00* MK 1.00 NL 1.14 ON 1.04 ! OV 1.03 PT 0.95 SC 0.89 TC 0.98 ! TS 1.00* WF 1.19 WZ 1.04 ! ! 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* ! 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* ! ! A total of 57 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* GG 1.00* HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.07 ! MC 1.14 MK 1.00* NL 1.00* ON 1.07 ! OV 1.00* PT 1.00* SC 1.00* TC 0.96 ! TS 1.00* WF 1.00* WZ 0.90 ! ! A total of 9 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 0.93 GG 1.00* HN 1.07 ! KK 1.00* KP 1.06 LA 0.93 MA 1.03 ! MC 1.14 MK 1.00* NL 1.06 ON 1.09 ! OV 0.94 PT 0.94 SC 0.92 TC 0.96 ! TS 1.00* WF 0.99 WZ 0.96 ! ! A total of 45 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 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.04 ! MC 1.23 MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 0.90 TC 0.93 ! TS 1.00* WF 1.03 WZ 0.99 ! ! ! Correcting IF 2. ! A total of 99 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 0.97 GG 1.00* HN 1.00* ! KK 0.92 KP 0.99 LA 0.99 MA 0.96 ! MC 1.07 MK 0.94 NL 1.27 ON 1.12 ! OV 0.95 PT 1.03 SC 1.00* TC 0.98 ! TS 1.00* WF 1.00* WZ 0.94 ! ! A total of 45 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 0.94 GG 1.00* HN 1.10 ! KK 1.03 KP 0.99 LA 0.94 MA 1.00 ! MC 1.00* MK 1.01 NL 1.09 ON 1.09 ! OV 1.02 PT 0.99 SC 0.87 TC 1.07 ! TS 1.00* WF 1.15 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* ! 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* ! ! A total of 57 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* GG 1.00* HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.10 ! MC 1.08 MK 1.00* NL 1.00* ON 1.03 ! OV 1.00* PT 1.00* SC 1.00* TC 1.07 ! TS 1.00* WF 1.00* WZ 0.94 ! ! A total of 9 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 0.93 GG 1.00* HN 1.09 ! KK 1.00* KP 0.99 LA 0.94 MA 1.02 ! MC 1.10 MK 1.00* NL 1.02 ON 1.07 ! OV 0.94 PT 0.98 SC 0.89 TC 1.01 ! TS 1.00* WF 1.02 WZ 0.99 ! ! A total of 45 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 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.05 ! MC 1.19 MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 0.84 TC 1.00 ! TS 1.00* WF 1.06 WZ 1.04 ! ! ! Correcting IF 3. ! A total of 99 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.07 FD 0.96 GG 1.00* HN 1.00* ! KK 0.97 KP 0.93 LA 1.00 MA 0.92 ! MC 1.41 MK 0.95 NL 1.24 ON 1.18 ! OV 1.00 PT 1.07 SC 1.00* TC 0.95 ! TS 1.00* WF 1.00* WZ 0.86 ! ! A total of 45 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 0.93 GG 1.00* HN 1.11 ! KK 1.06 KP 0.95 LA 0.94 MA 0.94 ! MC 1.00* MK 0.95 NL 1.06 ON 1.14 ! OV 0.99 PT 1.03 SC 0.88 TC 1.01 ! TS 1.00* WF 1.09 WZ 1.01 ! ! 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* ! 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* ! ! A total of 57 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* GG 1.00* HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.06 ! MC 1.14 MK 1.00* NL 1.00* ON 1.04 ! OV 1.00* PT 1.00* SC 1.00* TC 0.99 ! TS 1.00* WF 1.00* WZ 0.91 ! ! A total of 9 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.06 FD 0.92 GG 1.00* HN 1.08 ! KK 1.00* KP 0.92 LA 0.95 MA 1.01 ! MC 1.84 MK 1.00* NL 1.00 ON 1.09 ! OV 0.99 PT 1.01 SC 0.91 TC 0.98 ! TS 1.00* WF 1.01 WZ 0.94 ! ! A total of 45 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 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.06 ! MC 1.12 MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 0.87 TC 0.90 ! TS 1.00* WF 1.00 WZ 1.03 ! ! ! Correcting IF 4. ! A total of 96 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 FD 0.94 GG 1.00* HN 1.00* ! KK 0.95 KP 1.01 LA 0.95 MA 1.00 ! MC 2.11 MK 0.98 NL 1.25 ON 1.07 ! OV 0.99 PT 1.07 SC 1.00* TC 1.00 ! TS 1.00* WF 1.00* WZ 0.97 ! ! A total of 45 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.91 GG 1.00* HN 1.16 ! KK 0.98 KP 1.01 LA 0.93 MA 1.02 ! MC 1.00* MK 0.98 NL 1.08 ON 1.06 ! OV 0.99 PT 1.03 SC 0.92 TC 0.97 ! TS 1.00* WF 1.06 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* ! 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* ! ! A total of 57 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* GG 1.00* HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.12 ! MC 1.54 MK 1.00* NL 1.00* ON 1.05 ! OV 1.00* PT 1.00* SC 1.00* TC 0.91 ! TS 1.00* WF 1.00* WZ 0.97 ! ! A total of 9 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 FD 0.90 GG 1.00* HN 1.12 ! KK 1.00* KP 0.99 LA 0.93 MA 1.03 ! MC 1.67 MK 1.00* NL 1.01 ON 1.03 ! OV 0.97 PT 1.02 SC 0.97 TC 1.31 ! TS 1.00* WF 0.99 WZ 0.95 ! ! A total of 45 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 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.11 ! MC 1.91 MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 0.87 TC 0.95 ! TS 1.00* WF 1.04 WZ 1.00 ! ! ! Fit before self-cal, rms=0.502633Jy sigma=0.001906 ! Fit after self-cal, rms=0.483854Jy sigma=0.001372 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec ! Estimated beam: bmin=0.9752 mas, bmaj=1.514 mas, bpa=-17.52 degrees ! Estimated noise=787.687 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 = -0.00441145 Jy ! Component: 100 - total flux cleaned = -0.00491029 Jy ! Component: 150 - total flux cleaned = -0.00514601 Jy ! Component: 200 - total flux cleaned = -0.00555518 Jy ! Total flux subtracted in 200 components = -0.00555518 Jy ! Clean residual min=-0.007164 max=0.011722 Jy/beam ! Clean residual mean=0.000053 rms=0.002390 Jy/beam ! Combined flux in latest and established models = 1.70572 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 25 components and 1.70572 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.483417Jy sigma=0.001369 ! Fit after self-cal, rms=0.483497Jy sigma=0.001368 ! Inverting map ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 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=0.483497Jy sigma=0.001368 ! Fit after self-cal, rms=0.474755Jy sigma=0.001295 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec ! Estimated beam: bmin=0.9728 mas, bmaj=1.517 mas, bpa=-18.04 degrees ! Estimated noise=787.215 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00112143 Jy ! Component: 100 - total flux cleaned = -0.00136507 Jy ! Component: 150 - total flux cleaned = -0.00167981 Jy ! Component: 200 - total flux cleaned = -0.00185687 Jy ! Total flux subtracted in 200 components = -0.00185687 Jy ! Clean residual min=-0.005153 max=0.007501 Jy/beam ! Clean residual mean=0.000217 rms=0.001890 Jy/beam ! Combined flux in latest and established models = 1.70386 Jy selfcal ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 25 components and 1.70386 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.474587Jy sigma=0.001295 ! Fit after self-cal, rms=0.474572Jy sigma=0.001295 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 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 = -0.000161626 Jy ! Component: 100 - total flux cleaned = -0.000234397 Jy ! Component: 150 - total flux cleaned = -0.00036569 Jy ! Component: 200 - total flux cleaned = -0.000482256 Jy ! Total flux subtracted in 200 components = -0.000482256 Jy ! Clean residual min=-0.005206 max=0.007774 Jy/beam ! Clean residual mean=0.000236 rms=0.001912 Jy/beam ! Combined flux in latest and established models = 1.70338 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 25 components and 1.70338 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.474492Jy sigma=0.001295 ! Fit after self-cal, rms=0.474495Jy sigma=0.001295 ! Inverting map ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 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=0.474495Jy sigma=0.001295 ! Fit after self-cal, rms=0.472071Jy sigma=0.001216 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec ! Estimated beam: bmin=0.9743 mas, bmaj=1.519 mas, bpa=-18.1 degrees ! Estimated noise=787.044 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00263913 Jy ! Component: 100 - total flux cleaned = -0.00292424 Jy ! Component: 150 - total flux cleaned = -0.00308545 Jy ! Component: 200 - total flux cleaned = -0.00315666 Jy ! Total flux subtracted in 200 components = -0.00315666 Jy ! Clean residual min=-0.004976 max=0.006456 Jy/beam ! Clean residual mean=0.000039 rms=0.001433 Jy/beam ! Combined flux in latest and established models = 1.70022 Jy selfcal ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 25 components and 1.70022 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.471941Jy sigma=0.001216 ! Fit after self-cal, rms=0.472009Jy sigma=0.001216 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 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, 5.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00430176 Jy ! Component: 100 - total flux cleaned = 0.00471556 Jy ! Component: 150 - total flux cleaned = 0.00460359 Jy ! Component: 200 - total flux cleaned = 0.00460495 Jy ! Total flux subtracted in 200 components = 0.00460495 Jy ! Clean residual min=-0.004622 max=0.004334 Jy/beam ! Clean residual mean=-0.000111 rms=0.001249 Jy/beam ! Combined flux in latest and established models = 1.70483 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 33 components and 1.70483 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.471788Jy sigma=0.001215 ! Fit after self-cal, rms=0.471770Jy sigma=0.001215 ! Inverting map ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 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=0.471770Jy sigma=0.001215 ! Fit after self-cal, rms=0.471250Jy sigma=0.001215 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec ! Estimated beam: bmin=2.725 mas, bmaj=6.145 mas, bpa=-13.02 degrees ! Estimated noise=827.189 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000956701 Jy ! Component: 100 - total flux cleaned = 0.00103981 Jy ! Component: 150 - total flux cleaned = 0.0011624 Jy ! Component: 200 - total flux cleaned = 0.0012086 Jy ! Total flux subtracted in 200 components = 0.0012086 Jy ! Clean residual min=-0.003548 max=0.003390 Jy/beam ! Clean residual mean=-0.000222 rms=0.001339 Jy/beam ! Combined flux in latest and established models = 1.70604 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 38 components and 1.70604 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.471224Jy sigma=0.001214 ! Fit after self-cal, rms=0.471165Jy sigma=0.001214 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 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 = 0.000691416 Jy ! Component: 100 - total flux cleaned = 0.000792594 Jy ! Component: 150 - total flux cleaned = 0.000755148 Jy ! Component: 200 - total flux cleaned = 0.000718061 Jy ! Total flux subtracted in 200 components = 0.000718061 Jy ! Clean residual min=-0.003888 max=0.003316 Jy/beam ! Clean residual mean=-0.000262 rms=0.001363 Jy/beam ! Combined flux in latest and established models = 1.70676 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 44 components and 1.70676 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.471155Jy sigma=0.001214 ! Fit after self-cal, rms=0.471134Jy sigma=0.001214 ! Inverting map ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 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 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec ! Estimated beam: bmin=0.9754 mas, bmaj=1.521 mas, bpa=-18.11 degrees ! Estimated noise=786.812 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9754 x 1.521 at -18.11 degrees (North through East) ! Clean map min=-0.0043213 max=1.6039 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=0.471134Jy sigma=0.001214 ! Fit after self-cal, rms=0.583193Jy sigma=0.001055 ! Inverting map and beam ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec ! Estimated beam: bmin=0.974 mas, bmaj=1.52 mas, bpa=-18.04 degrees ! Estimated noise=786.192 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00081247 Jy ! Component: 100 - total flux cleaned = 0.00090467 Jy ! Component: 150 - total flux cleaned = 0.000903167 Jy ! Component: 200 - total flux cleaned = 0.000905417 Jy ! Total flux subtracted in 200 components = 0.000905416 Jy ! Clean residual min=-0.004185 max=0.003940 Jy/beam ! Clean residual mean=-0.000101 rms=0.001098 Jy/beam ! Combined flux in latest and established models = 1.70766 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 52 components and 1.70766 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.583102Jy sigma=0.001055 ! Fit after self-cal, rms=0.583109Jy sigma=0.001055 ! Inverting map ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000760902 Jy ! Component: 100 - total flux cleaned = 0.000762721 Jy ! Component: 150 - total flux cleaned = 0.00068959 Jy ! Component: 200 - total flux cleaned = 0.000691452 Jy ! Total flux subtracted in 200 components = 0.000691452 Jy ! Clean residual min=-0.004230 max=0.003861 Jy/beam ! Clean residual mean=-0.000123 rms=0.001101 Jy/beam ! Combined flux in latest and established models = 1.70835 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 53 components and 1.70835 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.583045Jy sigma=0.001055 ! Fit after self-cal, rms=0.583045Jy sigma=0.001055 ! Inverting map ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.583045Jy sigma=0.001055 ! Fit after self-cal, rms=0.636598Jy sigma=0.001055 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 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec ! Estimated beam: bmin=0.6149 mas, bmaj=0.9037 mas, bpa=-11.4 degrees ! Estimated noise=1970.72 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.20214 Jy ! Component: 100 - total flux cleaned = 1.48195 Jy ! Component: 150 - total flux cleaned = 1.58416 Jy ! Component: 200 - total flux cleaned = 1.63135 Jy ! Total flux subtracted in 200 components = 1.63135 Jy ! Clean residual min=-0.011139 max=0.023291 Jy/beam ! Clean residual mean=0.000343 rms=0.003241 Jy/beam ! Combined flux in latest and established models = 1.63135 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 12 model components to the UV plane model. ! The established model now contains 12 components and 1.63135 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec ! Estimated beam: bmin=0.9744 mas, bmaj=1.519 mas, bpa=-18.04 degrees ! Estimated noise=785.861 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 = 0.0438391 Jy ! Component: 100 - total flux cleaned = 0.0612074 Jy ! Component: 150 - total flux cleaned = 0.0697342 Jy ! Component: 200 - total flux cleaned = 0.0737424 Jy ! Total flux subtracted in 200 components = 0.0737424 Jy ! Clean residual min=-0.004147 max=0.004733 Jy/beam ! Clean residual mean=0.000030 rms=0.001209 Jy/beam ! Combined flux in latest and established models = 1.70509 Jy ! Adding 16 model components to the UV plane model. ! The established model now contains 23 components and 1.70509 Jy ! Inverting map ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 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 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec ! Estimated beam: bmin=2.723 mas, bmaj=6.142 mas, bpa=-13 degrees ! Estimated noise=826.858 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00300575 Jy ! Component: 100 - total flux cleaned = 0.00347898 Jy ! Component: 150 - total flux cleaned = 0.00342575 Jy ! Component: 200 - total flux cleaned = 0.00340122 Jy ! Total flux subtracted in 200 components = 0.00340122 Jy ! Clean residual min=-0.003365 max=0.002643 Jy/beam ! Clean residual mean=-0.000169 rms=0.001139 Jy/beam ! Combined flux in latest and established models = 1.70849 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 = -2.3036e-05 Jy ! Component: 100 - total flux cleaned = -6.51969e-05 Jy ! Component: 150 - total flux cleaned = -8.41876e-05 Jy ! Component: 200 - total flux cleaned = -8.47129e-05 Jy ! Total flux subtracted in 200 components = -8.47129e-05 Jy ! Clean residual min=-0.003352 max=0.002604 Jy/beam ! Clean residual mean=-0.000168 rms=0.001135 Jy/beam ! Combined flux in latest and established models = 1.70841 Jy ! Adding 16 model components to the UV plane model. ! The established model now contains 37 components and 1.70841 Jy ! Inverting map ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec ! Estimated beam: bmin=0.9744 mas, bmaj=1.519 mas, bpa=-18.04 degrees ! Estimated noise=785.861 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000256044 Jy ! Component: 100 - total flux cleaned = -0.000259634 Jy ! Component: 150 - total flux cleaned = -0.000172008 Jy ! Component: 200 - total flux cleaned = -9.18889e-05 Jy ! Total flux subtracted in 200 components = -9.18889e-05 Jy ! Clean residual min=-0.004067 max=0.004049 Jy/beam ! Clean residual mean=-0.000095 rms=0.001079 Jy/beam ! Combined flux in latest and established models = 1.70831 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 43 components and 1.70831 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.636572Jy sigma=0.001055 ! Fit after self-cal, rms=0.636570Jy sigma=0.001055 wmodel J1625-2527_X_2003_05_07_pus_map.mod ! Writing 43 model components to file: J1625-2527_X_2003_05_07_pus_map.mod wobs J1625-2527_X_2003_05_07_pus_uvs.fits ! Writing UV FITS file: J1625-2527_X_2003_05_07_pus_uvs.fits wwins J1625-2527_X_2003_05_07_pus_map.win ! wwins: Wrote 2 windows to J1625-2527_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 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000413026 Jy ! Component: 100 - total flux cleaned = 0.000410601 Jy ! Component: 150 - total flux cleaned = 0.000222434 Jy ! Component: 200 - total flux cleaned = 0.000223945 Jy ! Component: 250 - total flux cleaned = 0.000170664 Jy ! Component: 300 - total flux cleaned = 0.000222595 Jy ! Component: 350 - total flux cleaned = 0.000273318 Jy ! Component: 400 - total flux cleaned = 0.000369924 Jy ! Component: 450 - total flux cleaned = 0.000464045 Jy ! Component: 500 - total flux cleaned = 0.000556466 Jy ! Component: 550 - total flux cleaned = 0.000601331 Jy ! Component: 600 - total flux cleaned = 0.000600096 Jy ! Component: 650 - total flux cleaned = 0.000513498 Jy ! Component: 700 - total flux cleaned = 0.000471494 Jy ! Component: 750 - total flux cleaned = 0.000429726 Jy ! Component: 800 - total flux cleaned = 0.000388436 Jy ! Component: 850 - total flux cleaned = 0.000347924 Jy ! Component: 900 - total flux cleaned = 0.000228201 Jy ! Component: 950 - total flux cleaned = 0.000111085 Jy ! Component: 1000 - total flux cleaned = 7.33471e-05 Jy ! Total flux subtracted in 1024 components = 7.33665e-05 Jy ! Clean residual min=-0.002269 max=0.002226 Jy/beam ! Clean residual mean=-0.000099 rms=0.000692 Jy/beam ! Combined flux in latest and established models = 1.70839 Jy keep ! Adding 47 model components to the UV plane model. ! The established model now contains 90 components and 1.70839 Jy wmap "J1625-2527_X_2003_05_07_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9744 x 1.519 at -18.04 degrees (North through East) ! Clean map min=-0.0037636 max=1.602 Jy/beam ! Writing clean map to FITS file: J1625-2527_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 1.60203 invert ! Inverting map ! Your choice of large map pixels excluded 3.46% of the data. ! The x-axis pixel size should ideally be below 0.1959 milli-arcsec ! The y-axis pixel size should ideally be below 0.174 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000691877 device "J1625-2527_X_2003_05_07_pus\_map.eps/VPS" ! Attempting to open device: 'J1625-2527_X_2003_05_07_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.129562 0.129562 0.259125 0.51825 1.0365 2.073 4.146 8.292 16.584 33.168 66.336 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.002 print "peak=",int(1000*peak_flux)/1000 ! peak= 1.602 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9744 x 1.519 at -18.04 degrees (North through East) ! Clean map min=-0.0037636 max=1.602 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1625-2527_X_2003_05_07_pus\_map.gif/vgif" ! Attempting to open device: 'J1625-2527_X_2003_05_07_pus_map.gif/vgif' mapplot cln quit ! Quitting program ! Log file J1625-2527_X_2003_05_07_pus_uvs.log closed on Thu Dec 14 16:09:34 2006