! Started logfile: J2115+2933_X_2007_12_05_pus_uvs.log on Wed Sep 8 21:28:15 2010 obs J2115+2933_X_2007_12_05_pus_uva.fits ! Reading UV FITS file: J2115+2933_X_2007_12_05_pus_uva.fits ! AN table 1: 183 integrations on 136 of 136 possible baselines. ! AN table 2: 135 integrations on 136 of 136 possible baselines. ! AN table 3: 29 integrations on 136 of 136 possible baselines. ! AN table 4: 18 integrations on 136 of 136 possible baselines. ! Apparent sampling: 0.134388 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J2115+2933 ! ! 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 1501 lines of history. ! ! Reading 26684 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 print "field_size =",field_size ! field_size = 512 print "field_cell =",field_cell ! field_cell = 0.2 print "taper_size =",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 = 512x512 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 1865 telescope corrections were flagged in sub-array 1. ! A total of 1641 telescope corrections were flagged in sub-array 2. ! A total of 400 telescope corrections were flagged in sub-array 3. ! A total of 251 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 1865 telescope corrections were flagged in sub-array 1. ! A total of 1641 telescope corrections were flagged in sub-array 2. ! A total of 400 telescope corrections were flagged in sub-array 3. ! A total of 251 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 1865 telescope corrections were flagged in sub-array 1. ! A total of 1641 telescope corrections were flagged in sub-array 2. ! A total of 400 telescope corrections were flagged in sub-array 3. ! A total of 251 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 1903 telescope corrections were flagged in sub-array 1. ! A total of 1660 telescope corrections were flagged in sub-array 2. ! A total of 400 telescope corrections were flagged in sub-array 3. ! A total of 251 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=0.739554Jy sigma=0.005631 ! Fit after self-cal, rms=0.552338Jy sigma=0.004066 ! 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 11.6% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1854 milli-arcsec ! Estimated beam: bmin=0.4433 mas, bmaj=1.155 mas, bpa=-7.57 degrees ! Estimated noise=1147.09 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.374673 Jy ! Component: 100 - total flux cleaned = 0.491304 Jy ! Total flux subtracted in 100 components = 0.491304 Jy ! Clean residual min=-0.017551 max=0.056428 Jy/beam ! Clean residual mean=0.000480 rms=0.005297 Jy/beam ! Combined flux in latest and established models = 0.491304 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.491304 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.300926Jy sigma=0.001658 ! Fit after self-cal, rms=0.300606Jy sigma=0.001657 ! Inverting map ! Your choice of large map pixels excluded 11.6% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1854 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0654789 Jy ! Component: 100 - total flux cleaned = 0.104763 Jy ! Total flux subtracted in 100 components = 0.104763 Jy ! Clean residual min=-0.010789 max=0.020768 Jy/beam ! Clean residual mean=0.000252 rms=0.003052 Jy/beam ! Combined flux in latest and established models = 0.596067 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 12 components and 0.596067 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.278222Jy sigma=0.001341 ! Fit after self-cal, rms=0.277727Jy sigma=0.001340 ! Inverting map ! Your choice of large map pixels excluded 11.6% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1854 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0261938 Jy ! Component: 100 - total flux cleaned = 0.0432863 Jy ! Total flux subtracted in 100 components = 0.0432863 Jy ! Clean residual min=-0.009528 max=0.012170 Jy/beam ! Clean residual mean=0.000158 rms=0.002463 Jy/beam ! Combined flux in latest and established models = 0.639353 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 18 components and 0.639353 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.273340Jy sigma=0.001273 ! Fit after self-cal, rms=0.273227Jy sigma=0.001272 ! Inverting map ! Your choice of large map pixels excluded 11.6% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1854 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 11.6% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1854 milli-arcsec ! Estimated beam: bmin=0.5614 mas, bmaj=1.274 mas, bpa=-2.675 degrees ! Estimated noise=595.194 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 = 0.0239705 Jy ! Component: 100 - total flux cleaned = 0.0356534 Jy ! Component: 150 - total flux cleaned = 0.0416311 Jy ! Component: 200 - total flux cleaned = 0.0446336 Jy ! Total flux subtracted in 200 components = 0.0446336 Jy ! Clean residual min=-0.006757 max=0.011381 Jy/beam ! Clean residual mean=0.000363 rms=0.001959 Jy/beam ! Combined flux in latest and established models = 0.683987 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 27 components and 0.683987 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.271440Jy sigma=0.001247 ! Fit after self-cal, rms=0.271290Jy sigma=0.001245 ! Inverting map ! Your choice of large map pixels excluded 11.6% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1854 milli-arcsec ! Added new window around map position (0.6, -2.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0102923 Jy ! Component: 100 - total flux cleaned = 0.012212 Jy ! Component: 150 - total flux cleaned = 0.0138519 Jy ! Component: 200 - total flux cleaned = 0.0143752 Jy ! Total flux subtracted in 200 components = 0.0143752 Jy ! Clean residual min=-0.007182 max=0.009068 Jy/beam ! Clean residual mean=0.000041 rms=0.001638 Jy/beam ! Combined flux in latest and established models = 0.698362 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 44 components and 0.698362 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.270793Jy sigma=0.001239 ! Fit after self-cal, rms=0.270684Jy sigma=0.001238 ! Inverting map ! Your choice of large map pixels excluded 11.6% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1854 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 117 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.95 FD 0.99 HH 0.96 HN 1.04 ! KB 1.00 KP 1.00 LA 0.99 MK 1.00* ! NL 1.01 NY 0.95 ON 1.01 OV 0.99 ! PT 0.98 SV 1.04 TS 1.00 WZ 1.00* ! ZC 0.97 ! ! A total of 87 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* HH 1.27 HN 1.00* ! KB 1.00 KP 1.00* LA 1.00* MK 1.00* ! NL 1.00* NY 0.93 ON 0.96 OV 1.00* ! PT 1.00* SV 1.06 TS 1.00 WZ 1.04 ! ZC 1.08 ! ! A total of 15 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 FD 1.00 HH 1.00* HN 1.00* ! KB 1.00* KP 1.01 LA 1.03 MK 1.00* ! NL 1.00* NY 1.00* ON 1.00* OV 1.02 ! PT 1.02 SV 1.00* TS 1.00* WZ 1.00* ! ZC 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* HH 1.00* HN 1.00* ! KB 1.02 KP 0.97 LA 1.00* MK 1.00* ! NL 1.00* NY 1.00* ON 1.00* OV 0.98 ! PT 1.00* SV 1.00* TS 0.94 WZ 1.00* ! ZC 1.00* ! ! ! Correcting IF 2. ! A total of 117 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 0.99 HH 0.98 HN 1.05 ! KB 1.02 KP 0.96 LA 0.97 MK 1.00* ! NL 0.98 NY 0.97 ON 1.02 OV 0.98 ! PT 1.03 SV 0.98 TS 0.99 WZ 1.00* ! ZC 1.03 ! ! A total of 87 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* HH 1.30 HN 1.00* ! KB 0.99 KP 1.00* LA 1.00* MK 1.00* ! NL 1.00* NY 0.97 ON 0.96 OV 1.00* ! PT 1.00* SV 1.01 TS 1.00 WZ 1.03 ! ZC 1.08 ! ! A total of 15 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 1.03 HH 1.00* HN 1.00* ! KB 1.00* KP 0.98 LA 0.94 MK 1.00* ! NL 1.00* NY 1.00* ON 1.00* OV 1.00 ! PT 1.07 SV 1.00* TS 1.00* WZ 1.00* ! ZC 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* HH 1.00* HN 1.00* ! KB 1.01 KP 0.92 LA 1.00* MK 1.00* ! NL 1.00* NY 1.00* ON 1.00* OV 0.97 ! PT 1.00* SV 1.00* TS 0.96 WZ 1.00* ! ZC 1.00* ! ! ! Correcting IF 3. ! A total of 117 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 1.00 HH 0.99 HN 1.03 ! KB 1.01 KP 1.00 LA 1.00 MK 1.00* ! NL 1.00 NY 0.98 ON 0.96 OV 1.03 ! PT 1.05 SV 0.96 TS 1.00 WZ 1.00* ! ZC 0.97 ! ! A total of 87 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* HH 1.28 HN 1.00* ! KB 1.01 KP 1.00* LA 1.00* MK 1.00* ! NL 1.00* NY 0.99 ON 0.90 OV 1.00* ! PT 1.00* SV 0.99 TS 1.03 WZ 1.00 ! ZC 1.11 ! ! A total of 15 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 1.02 HH 1.00* HN 1.00* ! KB 1.00* KP 1.00 LA 1.09 MK 1.00* ! NL 1.00* NY 1.00* ON 1.00* OV 1.03 ! PT 1.06 SV 1.00* TS 1.00* WZ 1.00* ! ZC 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* HH 1.00* HN 1.00* ! KB 1.00 KP 0.96 LA 1.00* MK 1.00* ! NL 1.00* NY 1.00* ON 1.00* OV 1.02 ! PT 1.00* SV 1.00* TS 0.97 WZ 1.00* ! ZC 1.00* ! ! ! Correcting IF 4. ! A total of 117 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 0.99 HH 0.95 HN 1.07 ! KB 1.01 KP 1.01 LA 1.00 MK 1.00* ! NL 1.00 NY 0.98 ON 0.99 OV 1.03 ! PT 1.03 SV 0.95 TS 1.03 WZ 1.00* ! ZC 1.00* ! ! A total of 87 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* HH 1.06 HN 1.00* ! KB 1.00 KP 1.00* LA 1.00* MK 1.00* ! NL 1.00* NY 1.00 ON 0.91 OV 1.00* ! PT 1.00* SV 1.00 TS 1.01 WZ 0.97 ! ZC 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 0.97 HH 1.00* HN 1.00* ! KB 1.00* KP 1.06 LA 0.98 MK 1.00* ! NL 1.00* NY 1.00* ON 1.00* OV 1.03 ! PT 1.05 SV 1.00* TS 1.00* WZ 1.00* ! ZC 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* HH 1.00* HN 1.00* ! KB 0.98 KP 0.98 LA 1.00* MK 1.00* ! NL 1.00* NY 1.00* ON 1.00* OV 1.00 ! PT 1.00* SV 1.00* TS 0.99 WZ 1.00* ! ZC 1.00* ! ! ! Fit before self-cal, rms=0.270684Jy sigma=0.001238 ! Fit after self-cal, rms=0.279100Jy sigma=0.001228 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 milli-arcsec ! Estimated beam: bmin=0.5569 mas, bmaj=1.323 mas, bpa=-2.553 degrees ! Estimated noise=597.359 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 = 0.00483318 Jy ! Component: 100 - total flux cleaned = 0.00570444 Jy ! Component: 150 - total flux cleaned = 0.00627722 Jy ! Component: 200 - total flux cleaned = 0.00637437 Jy ! Total flux subtracted in 200 components = 0.00637437 Jy ! Clean residual min=-0.003945 max=0.004821 Jy/beam ! Clean residual mean=-0.000018 rms=0.001121 Jy/beam ! Combined flux in latest and established models = 0.704736 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 56 components and 0.704736 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.278954Jy sigma=0.001226 ! Fit after self-cal, rms=0.278792Jy sigma=0.001226 ! Inverting map ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 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=0.278792Jy sigma=0.001226 ! Fit after self-cal, rms=0.278332Jy sigma=0.001221 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 milli-arcsec ! Estimated beam: bmin=0.5567 mas, bmaj=1.323 mas, bpa=-2.528 degrees ! Estimated noise=598.051 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.002163 Jy ! Component: 100 - total flux cleaned = 0.00244298 Jy ! Component: 150 - total flux cleaned = 0.00244211 Jy ! Component: 200 - total flux cleaned = 0.00237458 Jy ! Total flux subtracted in 200 components = 0.00237458 Jy ! Clean residual min=-0.003385 max=0.004037 Jy/beam ! Clean residual mean=-0.000081 rms=0.000912 Jy/beam ! Combined flux in latest and established models = 0.707111 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 59 components and 0.707111 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.278250Jy sigma=0.001220 ! Fit after self-cal, rms=0.278232Jy sigma=0.001219 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 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 (3, -5). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00312492 Jy ! Component: 100 - total flux cleaned = 0.00374718 Jy ! Component: 150 - total flux cleaned = 0.00383472 Jy ! Component: 200 - total flux cleaned = 0.00376072 Jy ! Total flux subtracted in 200 components = 0.00376072 Jy ! Clean residual min=-0.003214 max=0.003582 Jy/beam ! Clean residual mean=-0.000153 rms=0.000831 Jy/beam ! Combined flux in latest and established models = 0.710871 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 70 components and 0.710871 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.278141Jy sigma=0.001219 ! Fit after self-cal, rms=0.278115Jy sigma=0.001219 ! Inverting map ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 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=0.278115Jy sigma=0.001219 ! Fit after self-cal, rms=0.278634Jy sigma=0.001217 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 milli-arcsec ! Estimated beam: bmin=0.5564 mas, bmaj=1.324 mas, bpa=-2.568 degrees ! Estimated noise=598.432 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00190157 Jy ! Component: 100 - total flux cleaned = 0.00212984 Jy ! Component: 150 - total flux cleaned = 0.00226033 Jy ! Component: 200 - total flux cleaned = 0.00231932 Jy ! Total flux subtracted in 200 components = 0.00231932 Jy ! Clean residual min=-0.003276 max=0.003055 Jy/beam ! Clean residual mean=-0.000071 rms=0.000766 Jy/beam ! Combined flux in latest and established models = 0.713191 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 73 components and 0.713191 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.278586Jy sigma=0.001216 ! Fit after self-cal, rms=0.278575Jy sigma=0.001216 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 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 = 0.000116612 Jy ! Component: 100 - total flux cleaned = 0.000173796 Jy ! Component: 150 - total flux cleaned = 0.000175134 Jy ! Component: 200 - total flux cleaned = 0.000221449 Jy ! Total flux subtracted in 200 components = 0.000221449 Jy ! Clean residual min=-0.003171 max=0.003003 Jy/beam ! Clean residual mean=-0.000075 rms=0.000749 Jy/beam ! Combined flux in latest and established models = 0.713412 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 76 components and 0.713412 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.278545Jy sigma=0.001216 ! Fit after self-cal, rms=0.278530Jy sigma=0.001216 ! Inverting map ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 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=0.278530Jy sigma=0.001216 ! Fit after self-cal, rms=0.279277Jy sigma=0.001216 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 milli-arcsec ! Estimated beam: bmin=2.961 mas, bmaj=3.581 mas, bpa=-44.66 degrees ! Estimated noise=769.9 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00101516 Jy ! Component: 100 - total flux cleaned = 0.00114447 Jy ! Component: 150 - total flux cleaned = 0.00121824 Jy ! Component: 200 - total flux cleaned = 0.00125268 Jy ! Total flux subtracted in 200 components = 0.00125268 Jy ! Clean residual min=-0.002668 max=0.003229 Jy/beam ! Clean residual mean=-0.000102 rms=0.000910 Jy/beam ! Combined flux in latest and established models = 0.714665 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 82 components and 0.714665 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.279269Jy sigma=0.001216 ! Fit after self-cal, rms=0.279269Jy sigma=0.001216 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 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 = 0.00013992 Jy ! Component: 100 - total flux cleaned = 0.000213353 Jy ! Component: 150 - total flux cleaned = 0.000182953 Jy ! Component: 200 - total flux cleaned = 0.000182754 Jy ! Total flux subtracted in 200 components = 0.000182754 Jy ! Clean residual min=-0.002724 max=0.003080 Jy/beam ! Clean residual mean=-0.000110 rms=0.000895 Jy/beam ! Combined flux in latest and established models = 0.714847 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 84 components and 0.714847 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.279270Jy sigma=0.001216 ! Fit after self-cal, rms=0.279264Jy sigma=0.001216 ! Inverting map ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 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 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 milli-arcsec ! Estimated beam: bmin=0.5563 mas, bmaj=1.324 mas, bpa=-2.59 degrees ! Estimated noise=598.672 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5563 x 1.324 at -2.59 degrees (North through East) ! Clean map min=-0.0025007 max=0.52892 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=0.279264Jy sigma=0.001216 ! Fit after self-cal, rms=0.428157Jy sigma=0.001113 ! Inverting map and beam ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 milli-arcsec ! Estimated beam: bmin=0.5561 mas, bmaj=1.323 mas, bpa=-2.634 degrees ! Estimated noise=598.142 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000318603 Jy ! Component: 100 - total flux cleaned = -0.000154782 Jy ! Component: 150 - total flux cleaned = -0.000201614 Jy ! Component: 200 - total flux cleaned = -0.000287121 Jy ! Total flux subtracted in 200 components = -0.000287121 Jy ! Clean residual min=-0.002564 max=0.003172 Jy/beam ! Clean residual mean=0.000001 rms=0.000696 Jy/beam ! Combined flux in latest and established models = 0.71456 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 94 components and 0.71456 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.428140Jy sigma=0.001113 ! Fit after self-cal, rms=0.428179Jy sigma=0.001113 ! Inverting map ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 milli-arcsec ! Added new window around map position (-2.8, -14.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00285616 Jy ! Component: 100 - total flux cleaned = 0.00324164 Jy ! Component: 150 - total flux cleaned = 0.00315193 Jy ! Component: 200 - total flux cleaned = 0.00310918 Jy ! Total flux subtracted in 200 components = 0.00310918 Jy ! Clean residual min=-0.002503 max=0.002517 Jy/beam ! Clean residual mean=-0.000060 rms=0.000666 Jy/beam ! Combined flux in latest and established models = 0.717669 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 106 components and 0.717669 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.428160Jy sigma=0.001112 ! Fit after self-cal, rms=0.428130Jy sigma=0.001112 ! Inverting map ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.428130Jy sigma=0.001112 ! Fit after self-cal, rms=0.433433Jy sigma=0.001112 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 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 milli-arcsec ! Estimated beam: bmin=0.4403 mas, bmaj=1.189 mas, bpa=-6.723 degrees ! Estimated noise=1153.82 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.378685 Jy ! Component: 100 - total flux cleaned = 0.499815 Jy ! Component: 150 - total flux cleaned = 0.568594 Jy ! Component: 200 - total flux cleaned = 0.608932 Jy ! Total flux subtracted in 200 components = 0.608932 Jy ! Clean residual min=-0.007116 max=0.020551 Jy/beam ! Clean residual mean=0.000237 rms=0.002325 Jy/beam ! Combined flux in latest and established models = 0.608932 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 0.608932 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 milli-arcsec ! Estimated beam: bmin=0.5561 mas, bmaj=1.323 mas, bpa=-2.641 degrees ! Estimated noise=597.907 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 = 0.0409989 Jy ! Component: 100 - total flux cleaned = 0.0622519 Jy ! Component: 150 - total flux cleaned = 0.0755396 Jy ! Component: 200 - total flux cleaned = 0.0843309 Jy ! Total flux subtracted in 200 components = 0.0843309 Jy ! Clean residual min=-0.003327 max=0.005771 Jy/beam ! Clean residual mean=0.000461 rms=0.001098 Jy/beam ! Combined flux in latest and established models = 0.693263 Jy ! Adding 32 model components to the UV plane model. ! The established model now contains 38 components and 0.693263 Jy ! Inverting map ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 milli-arcsec ! Added new window around map position (-0.6, -3.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00658346 Jy ! Component: 100 - total flux cleaned = 0.0115073 Jy ! Component: 150 - total flux cleaned = 0.0153594 Jy ! Component: 200 - total flux cleaned = 0.0184411 Jy ! Total flux subtracted in 200 components = 0.0184411 Jy ! Clean residual min=-0.002663 max=0.002788 Jy/beam ! Clean residual mean=0.000103 rms=0.000736 Jy/beam ! Combined flux in latest and established models = 0.711704 Jy ! Adding 40 model components to the UV plane model. ! The established model now contains 68 components and 0.711704 Jy ! Inverting map ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 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 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 milli-arcsec ! Estimated beam: bmin=2.961 mas, bmaj=3.582 mas, bpa=-44.49 degrees ! Estimated noise=769.505 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00346638 Jy ! Component: 100 - total flux cleaned = 0.00542405 Jy ! Component: 150 - total flux cleaned = 0.0066461 Jy ! Component: 200 - total flux cleaned = 0.00697072 Jy ! Total flux subtracted in 200 components = 0.00697072 Jy ! Clean residual min=-0.002483 max=0.002537 Jy/beam ! Clean residual mean=-0.000072 rms=0.000791 Jy/beam ! Combined flux in latest and established models = 0.718675 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 = 0.000124692 Jy ! Component: 100 - total flux cleaned = 0.000154943 Jy ! Component: 150 - total flux cleaned = 0.000182771 Jy ! Component: 200 - total flux cleaned = 0.000182837 Jy ! Total flux subtracted in 200 components = 0.000182837 Jy ! Clean residual min=-0.002437 max=0.002465 Jy/beam ! Clean residual mean=-0.000081 rms=0.000778 Jy/beam ! Combined flux in latest and established models = 0.718858 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 88 components and 0.718857 Jy ! Inverting map ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 milli-arcsec ! Estimated beam: bmin=0.5561 mas, bmaj=1.323 mas, bpa=-2.641 degrees ! Estimated noise=597.907 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00104968 Jy ! Component: 100 - total flux cleaned = -0.00112865 Jy ! Component: 150 - total flux cleaned = -0.000991558 Jy ! Component: 200 - total flux cleaned = -0.000867776 Jy ! Total flux subtracted in 200 components = -0.000867776 Jy ! Clean residual min=-0.002461 max=0.002667 Jy/beam ! Clean residual mean=-0.000019 rms=0.000652 Jy/beam ! Combined flux in latest and established models = 0.71799 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 97 components and 0.71799 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.434157Jy sigma=0.001114 ! Fit after self-cal, rms=0.435159Jy sigma=0.001114 wmodel J2115+2933_X_2007_12_05_pus_map.mod ! Writing 97 model components to file: J2115+2933_X_2007_12_05_pus_map.mod wobs J2115+2933_X_2007_12_05_pus_uvs.fits ! Writing UV FITS file: J2115+2933_X_2007_12_05_pus_uvs.fits wwins J2115+2933_X_2007_12_05_pus_map.win ! wwins: Wrote 5 windows to J2115+2933_X_2007_12_05_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 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000147772 Jy ! Component: 100 - total flux cleaned = -0.000608182 Jy ! Component: 150 - total flux cleaned = -0.000652765 Jy ! Component: 200 - total flux cleaned = -0.000526679 Jy ! Component: 250 - total flux cleaned = -0.000485761 Jy ! Component: 300 - total flux cleaned = -0.00052503 Jy ! Component: 350 - total flux cleaned = -0.000485839 Jy ! Component: 400 - total flux cleaned = -0.000485907 Jy ! Component: 450 - total flux cleaned = -0.000485816 Jy ! Component: 500 - total flux cleaned = -0.000485862 Jy ! Component: 550 - total flux cleaned = -0.000341906 Jy ! Component: 600 - total flux cleaned = -0.000307031 Jy ! Component: 650 - total flux cleaned = -0.000272595 Jy ! Component: 700 - total flux cleaned = -0.000341554 Jy ! Component: 750 - total flux cleaned = -0.000273369 Jy ! Component: 800 - total flux cleaned = -0.000273445 Jy ! Component: 850 - total flux cleaned = -0.000273464 Jy ! Component: 900 - total flux cleaned = -0.000240835 Jy ! Component: 950 - total flux cleaned = -0.000241074 Jy ! Component: 1000 - total flux cleaned = -0.000209092 Jy ! Component: 1050 - total flux cleaned = -0.000240265 Jy ! Component: 1100 - total flux cleaned = -0.00017774 Jy ! Component: 1150 - total flux cleaned = -0.000177519 Jy ! Component: 1200 - total flux cleaned = -0.000146988 Jy ! Component: 1250 - total flux cleaned = -0.000117111 Jy ! Component: 1300 - total flux cleaned = -8.75373e-05 Jy ! Component: 1350 - total flux cleaned = -0.000117126 Jy ! Component: 1400 - total flux cleaned = -8.77404e-05 Jy ! Component: 1450 - total flux cleaned = -8.75841e-05 Jy ! Component: 1500 - total flux cleaned = -5.88158e-05 Jy ! Component: 1550 - total flux cleaned = -3.05608e-05 Jy ! Component: 1600 - total flux cleaned = -5.87064e-05 Jy ! Component: 1650 - total flux cleaned = -2.85849e-06 Jy ! Component: 1700 - total flux cleaned = 2.47841e-05 Jy ! Component: 1750 - total flux cleaned = -2.86181e-06 Jy ! Component: 1800 - total flux cleaned = -2.7116e-06 Jy ! Component: 1850 - total flux cleaned = 2.43342e-05 Jy ! Component: 1900 - total flux cleaned = 5.12549e-05 Jy ! Component: 1950 - total flux cleaned = 5.11976e-05 Jy ! Component: 2000 - total flux cleaned = 5.10998e-05 Jy ! Total flux subtracted in 2048 components = 5.11885e-05 Jy ! Clean residual min=-0.001528 max=0.001442 Jy/beam ! Clean residual mean=-0.000015 rms=0.000452 Jy/beam ! Combined flux in latest and established models = 0.718041 Jy keep ! Adding 144 model components to the UV plane model. ! The established model now contains 241 components and 0.718041 Jy wmap "J2115+2933_X_2007_12_05_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5561 x 1.323 at -2.641 degrees (North through East) ! Clean map min=-0.0020659 max=0.53292 Jy/beam ! Writing clean map to FITS file: J2115+2933_X_2007_12_05_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.532921 invert ! Inverting map ! Your choice of large map pixels excluded 11.4% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1856 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000452601 device "J2115+2933_X_2007_12_05_pus\_map.eps/VPS" ! Attempting to open device: 'J2115+2933_X_2007_12_05_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.254785 0.254785 0.50957 1.01914 2.03828 4.07656 8.15313 16.3063 32.6125 65.225 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0013 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.532 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5561 x 1.323 at -2.641 degrees (North through East) ! Clean map min=-0.0020659 max=0.53292 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J2115+2933_X_2007_12_05_pus\_map.gif/vgif" ! Attempting to open device: 'J2115+2933_X_2007_12_05_pus_map.gif/vgif' mapplot cln quit ! Quitting program ! Log file J2115+2933_X_2007_12_05_pus_uvs.log closed on Wed Sep 8 21:28:24 2010