! Started logfile: J2115+2933_X_2008_04_02_pus_uvs.log on Sun Feb 21 20:53:45 2010 obs J2115+2933_X_2008_04_02_pus_uva.fits ! Reading UV FITS file: J2115+2933_X_2008_04_02_pus_uva.fits ! AN table 1: 60 integrations on 120 of 120 possible baselines. ! AN table 2: 142 integrations on 120 of 120 possible baselines. ! AN table 3: 38 integrations on 120 of 120 possible baselines. ! AN table 4: 15 integrations on 120 of 120 possible baselines. ! AN table 5: 263 integrations on 120 of 120 possible baselines. ! Apparent sampling: 0.079778 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 2284 lines of history. ! ! Reading 19836 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 704 telescope corrections were flagged in sub-array 1. ! A total of 1618 telescope corrections were flagged in sub-array 2. ! A total of 482 telescope corrections were flagged in sub-array 3. ! A total of 135 telescope corrections were flagged in sub-array 4. ! A total of 3211 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 704 telescope corrections were flagged in sub-array 1. ! A total of 1624 telescope corrections were flagged in sub-array 2. ! A total of 500 telescope corrections were flagged in sub-array 3. ! A total of 135 telescope corrections were flagged in sub-array 4. ! A total of 3211 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 704 telescope corrections were flagged in sub-array 1. ! A total of 1618 telescope corrections were flagged in sub-array 2. ! A total of 482 telescope corrections were flagged in sub-array 3. ! A total of 135 telescope corrections were flagged in sub-array 4. ! A total of 3211 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 704 telescope corrections were flagged in sub-array 1. ! A total of 1641 telescope corrections were flagged in sub-array 2. ! A total of 482 telescope corrections were flagged in sub-array 3. ! A total of 135 telescope corrections were flagged in sub-array 4. ! A total of 3293 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=0.735923Jy sigma=0.003948 ! Fit after self-cal, rms=0.591255Jy sigma=0.003138 ! 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 8.13% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! Estimated beam: bmin=0.6413 mas, bmaj=1.301 mas, bpa=-3.729 degrees ! Estimated noise=1185 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 = 0.433248 Jy ! Component: 100 - total flux cleaned = 0.564772 Jy ! Total flux subtracted in 100 components = 0.564772 Jy ! Clean residual min=-0.015840 max=0.057086 Jy/beam ! Clean residual mean=-0.000296 rms=0.004633 Jy/beam ! Combined flux in latest and established models = 0.564772 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 10 components and 0.564772 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.355560Jy sigma=0.001441 ! Fit after self-cal, rms=0.355232Jy sigma=0.001438 ! Inverting map ! Your choice of large map pixels excluded 8.13% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0639963 Jy ! Component: 100 - total flux cleaned = 0.0984415 Jy ! Total flux subtracted in 100 components = 0.0984415 Jy ! Clean residual min=-0.009996 max=0.016971 Jy/beam ! Clean residual mean=-0.000176 rms=0.002510 Jy/beam ! Combined flux in latest and established models = 0.663213 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 21 components and 0.663213 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.349058Jy sigma=0.001245 ! Fit after self-cal, rms=0.348570Jy sigma=0.001243 ! Inverting map ! Your choice of large map pixels excluded 8.13% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0209283 Jy ! Component: 100 - total flux cleaned = 0.0328166 Jy ! Total flux subtracted in 100 components = 0.0328166 Jy ! Clean residual min=-0.009172 max=0.010275 Jy/beam ! Clean residual mean=-0.000135 rms=0.002138 Jy/beam ! Combined flux in latest and established models = 0.69603 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 26 components and 0.69603 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.348134Jy sigma=0.001219 ! Fit after self-cal, rms=0.347976Jy sigma=0.001218 ! Inverting map ! Your choice of large map pixels excluded 8.13% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 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 8.13% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! Estimated beam: bmin=0.8608 mas, bmaj=1.099 mas, bpa=-1.502 degrees ! Estimated noise=835.399 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 (-0.8, -3.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0186118 Jy ! Component: 100 - total flux cleaned = 0.0279946 Jy ! Component: 150 - total flux cleaned = 0.0310488 Jy ! Component: 200 - total flux cleaned = 0.0326383 Jy ! Total flux subtracted in 200 components = 0.0326383 Jy ! Clean residual min=-0.012266 max=0.013666 Jy/beam ! Clean residual mean=-0.000187 rms=0.002669 Jy/beam ! Combined flux in latest and established models = 0.728668 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 39 components and 0.728668 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.346161Jy sigma=0.001208 ! Fit after self-cal, rms=0.346079Jy sigma=0.001206 ! Inverting map ! Your choice of large map pixels excluded 8.13% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 21 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 0.98 HH 1.00* HN 0.98 ! KK 1.00 KP 1.01 LA 0.99 MK 1.01 ! NL 1.00 NY 1.00* ON 1.00* OV 0.98 ! PT 0.98 SC 1.06 WZ 1.00* ZC 1.00* ! ! A total of 60 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.94 FD 0.98 HH 0.89 HN 1.00* ! KK 1.00* KP 0.98 LA 0.99 MK 1.00* ! NL 1.01 NY 1.03 ON 0.97 OV 0.97 ! PT 0.98 SC 1.00* WZ 1.09 ZC 1.09 ! ! A total of 54 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* HH 1.00* HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MK 1.00* ! NL 1.00* NY 0.91 ON 1.00 OV 1.00* ! PT 1.00* SC 1.00* WZ 0.97 ZC 1.02 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.94 FD 0.98 HH 1.00* HN 0.98 ! KK 1.00* KP 1.01 LA 0.99 MK 1.02 ! NL 1.00 NY 1.00* ON 1.00* OV 1.00 ! PT 0.96 SC 1.00* WZ 1.00* ZC 1.00* ! ! A total of 114 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 FD 1.00* HH 1.00 HN 0.97 ! KK 1.00* KP 1.06 LA 0.99 MK 1.00* ! NL 0.99 NY 1.04 ON 0.99 OV 0.98 ! PT 1.05 SC 1.02 WZ 1.25 ZC 1.13 ! ! ! Correcting IF 2. ! A total of 21 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 0.97 HH 1.00* HN 1.01 ! KK 0.98 KP 0.95 LA 0.99 MK 1.00 ! NL 0.97 NY 1.00* ON 1.00* OV 0.98 ! PT 0.96 SC 1.08 WZ 1.00* ZC 1.00* ! ! A total of 60 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.93 FD 0.98 HH 0.90 HN 1.00* ! KK 1.00* KP 0.95 LA 0.97 MK 1.00* ! NL 0.97 NY 0.98 ON 1.18 OV 0.97 ! PT 0.96 SC 1.00* WZ 1.09 ZC 2.43 ! ! A total of 108 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MK 0.00* ! NL 0.00* NY 0.00* ON 0.00* OV 0.00* ! PT 0.00* SC 0.00* WZ 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.93 FD 0.97 HH 1.00* HN 0.97 ! KK 1.00* KP 0.97 LA 0.99 MK 1.01 ! NL 1.00 NY 1.00* ON 1.00* OV 0.97 ! PT 0.97 SC 1.00* WZ 1.00* ZC 1.00* ! ! A total of 114 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 FD 1.00* HH 1.05 HN 0.98 ! KK 1.00* KP 0.97 LA 1.05 MK 1.00* ! NL 0.96 NY 1.02 ON 0.99 OV 0.99 ! PT 1.02 SC 1.00 WZ 1.31 ZC 1.07 ! ! ! Correcting IF 3. ! A total of 21 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.99 HH 1.00* HN 1.00 ! KK 1.05 KP 1.02 LA 1.00 MK 1.02 ! NL 1.02 NY 1.00* ON 1.00* OV 1.01 ! PT 0.96 SC 1.20 WZ 1.00* ZC 1.00* ! ! A total of 60 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 0.99 HH 0.83 HN 1.00* ! KK 1.00* KP 0.98 LA 1.02 MK 1.00* ! NL 1.00 NY 1.02 ON 1.02 OV 1.01 ! PT 0.98 SC 1.00* WZ 1.09 ZC 1.14 ! ! A total of 54 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* HH 1.00* HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MK 1.00* ! NL 1.00* NY 1.17 ON 0.95 OV 1.00* ! PT 1.00* SC 1.00* WZ 0.86 ZC 1.10 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 FD 1.00 HH 1.00* HN 0.96 ! KK 1.00* KP 0.99 LA 1.01 MK 1.01 ! NL 1.00 NY 1.00* ON 1.00* OV 1.00 ! PT 0.97 SC 1.00* WZ 1.00* ZC 1.00* ! ! A total of 114 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.06 FD 1.00* HH 1.10 HN 1.00 ! KK 1.00* KP 1.01 LA 1.04 MK 1.00* ! NL 0.98 NY 1.02 ON 0.96 OV 1.04 ! PT 1.03 SC 1.03 WZ 1.23 ZC 1.14 ! ! ! Correcting IF 4. ! A total of 21 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.99 HH 1.00* HN 1.05 ! KK 1.03 KP 0.98 LA 0.99 MK 1.02 ! NL 1.02 NY 1.00* ON 1.00* OV 1.03 ! PT 0.96 SC 1.16 WZ 1.00* ZC 1.00* ! ! A total of 129 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.97 HH 0.78 HN 1.00* ! KK 1.00* KP 0.96 LA 1.01 MK 1.00* ! NL 1.01 NY 0.97 ON 1.07 OV 1.00 ! PT 0.98 SC 1.00* WZ 1.06 ZC 1.19 ! ! A total of 54 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* HH 1.00* HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MK 1.00* ! NL 1.00* NY 0.97 ON 0.87 OV 1.00* ! PT 1.00* SC 1.00* WZ 1.01 ZC 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.94 FD 0.98 HH 1.00* HN 1.02 ! KK 1.00* KP 1.00 LA 1.00 MK 1.06 ! NL 1.02 NY 1.00* ON 1.00* OV 0.99 ! PT 0.97 SC 1.00* WZ 1.00* ZC 1.00* ! ! A total of 114 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 1.00* HH 0.95 HN 1.00 ! KK 1.00* KP 1.02 LA 1.07 MK 1.00* ! NL 0.99 NY 0.99 ON 0.82 OV 1.00 ! PT 1.02 SC 1.03 WZ 1.04 ZC 1.14 ! ! ! Fit before self-cal, rms=0.346079Jy sigma=0.001206 ! Fit after self-cal, rms=0.365880Jy sigma=0.001182 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! Estimated beam: bmin=0.8796 mas, bmaj=1.097 mas, bpa=-1.555 degrees ! Estimated noise=860.648 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 = -0.00101989 Jy ! Component: 100 - total flux cleaned = -0.000490624 Jy ! Component: 150 - total flux cleaned = 7.73833e-05 Jy ! Component: 200 - total flux cleaned = 0.000204501 Jy ! Total flux subtracted in 200 components = 0.000204501 Jy ! Clean residual min=-0.006223 max=0.006589 Jy/beam ! Clean residual mean=-0.000011 rms=0.001481 Jy/beam ! Combined flux in latest and established models = 0.728873 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 48 components and 0.728873 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.365646Jy sigma=0.001181 ! Fit after self-cal, rms=0.366533Jy sigma=0.001180 ! Inverting map ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 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=0.366533Jy sigma=0.001180 ! Fit after self-cal, rms=0.402488Jy sigma=0.001172 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! Estimated beam: bmin=0.8725 mas, bmaj=1.099 mas, bpa=-1.989 degrees ! Estimated noise=859.249 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000973488 Jy ! Component: 100 - total flux cleaned = -0.00146411 Jy ! Component: 150 - total flux cleaned = -0.00166594 Jy ! Component: 200 - total flux cleaned = -0.00193404 Jy ! Total flux subtracted in 200 components = -0.00193404 Jy ! Clean residual min=-0.004766 max=0.004649 Jy/beam ! Clean residual mean=-0.000001 rms=0.001133 Jy/beam ! Combined flux in latest and established models = 0.726939 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 55 components and 0.726939 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.402444Jy sigma=0.001172 ! Fit after self-cal, rms=0.403922Jy sigma=0.001171 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 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 = -4.44585e-05 Jy ! Component: 100 - total flux cleaned = -3.69248e-05 Jy ! Component: 150 - total flux cleaned = -3.62301e-05 Jy ! Component: 200 - total flux cleaned = -3.61425e-05 Jy ! Total flux subtracted in 200 components = -3.61425e-05 Jy ! Clean residual min=-0.004783 max=0.004631 Jy/beam ! Clean residual mean=-0.000001 rms=0.001124 Jy/beam ! Combined flux in latest and established models = 0.726902 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 60 components and 0.726902 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.403891Jy sigma=0.001171 ! Fit after self-cal, rms=0.403919Jy sigma=0.001171 ! Inverting map ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 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=0.403919Jy sigma=0.001171 ! Fit after self-cal, rms=0.405215Jy sigma=0.001168 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! Estimated beam: bmin=0.8702 mas, bmaj=1.101 mas, bpa=-2.08 degrees ! Estimated noise=859.343 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000386109 Jy ! Component: 100 - total flux cleaned = -0.000843197 Jy ! Component: 150 - total flux cleaned = -0.000985326 Jy ! Component: 200 - total flux cleaned = -0.000987683 Jy ! Total flux subtracted in 200 components = -0.000987683 Jy ! Clean residual min=-0.004159 max=0.004089 Jy/beam ! Clean residual mean=0.000003 rms=0.001006 Jy/beam ! Combined flux in latest and established models = 0.725915 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 66 components and 0.725915 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.405183Jy sigma=0.001167 ! Fit after self-cal, rms=0.405116Jy sigma=0.001167 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 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 = -0.000180114 Jy ! Component: 100 - total flux cleaned = -0.000372901 Jy ! Component: 150 - total flux cleaned = -0.000370424 Jy ! Component: 200 - total flux cleaned = -0.000421933 Jy ! Total flux subtracted in 200 components = -0.000421933 Jy ! Clean residual min=-0.004157 max=0.004045 Jy/beam ! Clean residual mean=0.000003 rms=0.000999 Jy/beam ! Combined flux in latest and established models = 0.725493 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 70 components and 0.725493 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.405097Jy sigma=0.001167 ! Fit after self-cal, rms=0.405100Jy sigma=0.001167 ! Inverting map ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 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=0.405100Jy sigma=0.001167 ! Fit after self-cal, rms=0.405270Jy sigma=0.001167 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! Estimated beam: bmin=2.479 mas, bmaj=2.619 mas, bpa=-19.62 degrees ! Estimated noise=971.643 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000108574 Jy ! Component: 100 - total flux cleaned = 0.000200025 Jy ! Component: 150 - total flux cleaned = 0.000201064 Jy ! Component: 200 - total flux cleaned = 0.000239353 Jy ! Total flux subtracted in 200 components = 0.000239353 Jy ! Clean residual min=-0.003818 max=0.004151 Jy/beam ! Clean residual mean=0.000010 rms=0.001114 Jy/beam ! Combined flux in latest and established models = 0.725732 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 77 components and 0.725732 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.405257Jy sigma=0.001167 ! Fit after self-cal, rms=0.405169Jy sigma=0.001167 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 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 = -0.000127441 Jy ! Component: 100 - total flux cleaned = -1.81398e-05 Jy ! Component: 150 - total flux cleaned = 0.000211539 Jy ! Component: 200 - total flux cleaned = 0.000306836 Jy ! Total flux subtracted in 200 components = 0.000306836 Jy ! Clean residual min=-0.003810 max=0.004009 Jy/beam ! Clean residual mean=0.000009 rms=0.001103 Jy/beam ! Combined flux in latest and established models = 0.726039 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 78 components and 0.726039 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.405161Jy sigma=0.001167 ! Fit after self-cal, rms=0.405114Jy sigma=0.001167 ! Inverting map ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 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 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! Estimated beam: bmin=0.8697 mas, bmaj=1.101 mas, bpa=-2.223 degrees ! Estimated noise=859.184 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8697 x 1.101 at -2.223 degrees (North through East) ! Clean map min=-0.0033668 max=0.54465 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=0.405114Jy sigma=0.001167 ! Fit after self-cal, rms=3.115931Jy sigma=0.001004 ! Inverting map and beam ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! Estimated beam: bmin=0.8686 mas, bmaj=1.102 mas, bpa=-2.096 degrees ! Estimated noise=859.84 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000836355 Jy ! Component: 100 - total flux cleaned = -0.00126318 Jy ! Component: 150 - total flux cleaned = -0.00138684 Jy ! Component: 200 - total flux cleaned = -0.00149731 Jy ! Total flux subtracted in 200 components = -0.00149731 Jy ! Clean residual min=-0.003724 max=0.003752 Jy/beam ! Clean residual mean=0.000003 rms=0.000918 Jy/beam ! Combined flux in latest and established models = 0.724542 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 82 components and 0.724542 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=3.115892Jy sigma=0.001004 ! Fit after self-cal, rms=3.115987Jy sigma=0.001004 ! Inverting map ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000117307 Jy ! Component: 100 - total flux cleaned = -0.0002032 Jy ! Component: 150 - total flux cleaned = -0.000250696 Jy ! Component: 200 - total flux cleaned = -0.000375761 Jy ! Total flux subtracted in 200 components = -0.000375761 Jy ! Clean residual min=-0.003700 max=0.003754 Jy/beam ! Clean residual mean=0.000003 rms=0.000912 Jy/beam ! Combined flux in latest and established models = 0.724166 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 85 components and 0.724166 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=3.115958Jy sigma=0.001004 ! Fit after self-cal, rms=3.115969Jy sigma=0.001004 ! Inverting map ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=3.115969Jy sigma=0.001004 ! Fit after self-cal, rms=5.770265Jy sigma=0.001003 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 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! Estimated beam: bmin=0.6616 mas, bmaj=1.304 mas, bpa=-4.629 degrees ! Estimated noise=1193.04 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.434765 Jy ! Component: 100 - total flux cleaned = 0.567262 Jy ! Component: 150 - total flux cleaned = 0.626461 Jy ! Component: 200 - total flux cleaned = 0.657443 Jy ! Total flux subtracted in 200 components = 0.657443 Jy ! Clean residual min=-0.007243 max=0.014858 Jy/beam ! Clean residual mean=-0.000108 rms=0.001964 Jy/beam ! Combined flux in latest and established models = 0.657443 Jy uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 18 model components to the UV plane model. ! The established model now contains 18 components and 0.657443 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! Estimated beam: bmin=0.8697 mas, bmaj=1.099 mas, bpa=-2.311 degrees ! Estimated noise=859.007 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 = 0.022551 Jy ! Component: 100 - total flux cleaned = 0.0361842 Jy ! Component: 150 - total flux cleaned = 0.0454379 Jy ! Component: 200 - total flux cleaned = 0.0519953 Jy ! Total flux subtracted in 200 components = 0.0519953 Jy ! Clean residual min=-0.004559 max=0.005638 Jy/beam ! Clean residual mean=0.000006 rms=0.001086 Jy/beam ! Combined flux in latest and established models = 0.709438 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 42 components and 0.709438 Jy ! Inverting map ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! Added new window around map position (0.8, -2.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00565726 Jy ! Component: 100 - total flux cleaned = 0.00953845 Jy ! Component: 150 - total flux cleaned = 0.0119619 Jy ! Component: 200 - total flux cleaned = 0.0132866 Jy ! Total flux subtracted in 200 components = 0.0132866 Jy ! Clean residual min=-0.003839 max=0.003859 Jy/beam ! Clean residual mean=0.000003 rms=0.000943 Jy/beam ! Combined flux in latest and established models = 0.722725 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 55 components and 0.722725 Jy ! Inverting map ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 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 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! Estimated beam: bmin=2.48 mas, bmaj=2.621 mas, bpa=-20.85 degrees ! Estimated noise=970.989 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00294509 Jy ! Component: 100 - total flux cleaned = 0.00448957 Jy ! Component: 150 - total flux cleaned = 0.00492975 Jy ! Component: 200 - total flux cleaned = 0.00513554 Jy ! Total flux subtracted in 200 components = 0.00513554 Jy ! Clean residual min=-0.003801 max=0.003328 Jy/beam ! Clean residual mean=0.000003 rms=0.001033 Jy/beam ! Combined flux in latest and established models = 0.72786 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 = 0.000118535 Jy ! Component: 100 - total flux cleaned = 0.000224377 Jy ! Component: 150 - total flux cleaned = 0.000340629 Jy ! Component: 200 - total flux cleaned = 0.000362374 Jy ! Total flux subtracted in 200 components = 0.000362374 Jy ! Clean residual min=-0.003756 max=0.003309 Jy/beam ! Clean residual mean=0.000003 rms=0.001027 Jy/beam ! Combined flux in latest and established models = 0.728223 Jy ! Adding 22 model components to the UV plane model. ! The established model now contains 69 components and 0.728223 Jy ! Inverting map ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! Estimated beam: bmin=0.8697 mas, bmaj=1.099 mas, bpa=-2.311 degrees ! Estimated noise=859.007 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000408904 Jy ! Component: 100 - total flux cleaned = -0.000497726 Jy ! Component: 150 - total flux cleaned = -0.000498826 Jy ! Component: 200 - total flux cleaned = -0.000428007 Jy ! Total flux subtracted in 200 components = -0.000428007 Jy ! Clean residual min=-0.003738 max=0.003742 Jy/beam ! Clean residual mean=0.000001 rms=0.000909 Jy/beam ! Combined flux in latest and established models = 0.727795 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 76 components and 0.727795 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=5.769931Jy sigma=0.001006 ! Fit after self-cal, rms=5.769982Jy sigma=0.001005 wmodel J2115+2933_X_2008_04_02_pus_map.mod ! Writing 76 model components to file: J2115+2933_X_2008_04_02_pus_map.mod wobs J2115+2933_X_2008_04_02_pus_uvs.fits ! Writing UV FITS file: J2115+2933_X_2008_04_02_pus_uvs.fits wwins J2115+2933_X_2008_04_02_pus_map.win ! wwins: Wrote 3 windows to J2115+2933_X_2008_04_02_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 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000763008 Jy ! Component: 100 - total flux cleaned = -0.00101935 Jy ! Component: 150 - total flux cleaned = -0.00138811 Jy ! Component: 200 - total flux cleaned = -0.00144785 Jy ! Component: 250 - total flux cleaned = -0.00156352 Jy ! Component: 300 - total flux cleaned = -0.00156213 Jy ! Component: 350 - total flux cleaned = -0.00161795 Jy ! Component: 400 - total flux cleaned = -0.00167284 Jy ! Component: 450 - total flux cleaned = -0.00172606 Jy ! Component: 500 - total flux cleaned = -0.00161964 Jy ! Component: 550 - total flux cleaned = -0.00156768 Jy ! Component: 600 - total flux cleaned = -0.00151683 Jy ! Component: 650 - total flux cleaned = -0.00151747 Jy ! Component: 700 - total flux cleaned = -0.00151764 Jy ! Component: 750 - total flux cleaned = -0.00161526 Jy ! Component: 800 - total flux cleaned = -0.00156584 Jy ! Component: 850 - total flux cleaned = -0.00142262 Jy ! Component: 900 - total flux cleaned = -0.00137525 Jy ! Component: 950 - total flux cleaned = -0.00114298 Jy ! Component: 1000 - total flux cleaned = -0.00114366 Jy ! Component: 1050 - total flux cleaned = -0.00100694 Jy ! Component: 1100 - total flux cleaned = -0.00105248 Jy ! Component: 1150 - total flux cleaned = -0.00100767 Jy ! Component: 1200 - total flux cleaned = -0.000963232 Jy ! Component: 1250 - total flux cleaned = -0.000875845 Jy ! Component: 1300 - total flux cleaned = -0.000962996 Jy ! Component: 1350 - total flux cleaned = -0.00104906 Jy ! Component: 1400 - total flux cleaned = -0.00092035 Jy ! Component: 1450 - total flux cleaned = -0.000920729 Jy ! Component: 1500 - total flux cleaned = -0.000962625 Jy ! Component: 1550 - total flux cleaned = -0.00108734 Jy ! Component: 1600 - total flux cleaned = -0.000962826 Jy ! Component: 1650 - total flux cleaned = -0.000839451 Jy ! Component: 1700 - total flux cleaned = -0.00096225 Jy ! Component: 1750 - total flux cleaned = -0.00108374 Jy ! Component: 1800 - total flux cleaned = -0.00100273 Jy ! Component: 1850 - total flux cleaned = -0.00100305 Jy ! Component: 1900 - total flux cleaned = -0.00104237 Jy ! Component: 1950 - total flux cleaned = -0.000924495 Jy ! Component: 2000 - total flux cleaned = -0.00112056 Jy ! Total flux subtracted in 2048 components = -0.00108152 Jy ! Clean residual min=-0.001969 max=0.002285 Jy/beam ! Clean residual mean=0.000018 rms=0.000690 Jy/beam ! Combined flux in latest and established models = 0.726713 Jy keep ! Adding 166 model components to the UV plane model. ! The established model now contains 242 components and 0.726713 Jy wmap "J2115+2933_X_2008_04_02_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8697 x 1.099 at -2.311 degrees (North through East) ! Clean map min=-0.0028867 max=0.54476 Jy/beam ! Writing clean map to FITS file: J2115+2933_X_2008_04_02_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.544765 invert ! Inverting map ! Your choice of large map pixels excluded 7.99% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1695 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000690206 device "J2115+2933_X_2008_04_02_pus\_map.eps/VPS" ! Attempting to open device: 'J2115+2933_X_2008_04_02_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.380094 0.380094 0.760187 1.52037 3.04075 6.0815 12.163 24.326 48.652 97.304 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.002 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.544 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8697 x 1.099 at -2.311 degrees (North through East) ! Clean map min=-0.0028867 max=0.54476 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J2115+2933_X_2008_04_02_pus\_map.gif/vgif" ! Attempting to open device: 'J2115+2933_X_2008_04_02_pus_map.gif/vgif' mapplot cln quit ! Quitting program ! Log file J2115+2933_X_2008_04_02_pus_uvs.log closed on Sun Feb 21 20:53:53 2010