! Started logfile: J0555+3948_X_2008_04_02_pus_uvs.log on Sun Feb 21 20:45:59 2010 obs J0555+3948_X_2008_04_02_pus_uva.fits ! Reading UV FITS file: J0555+3948_X_2008_04_02_pus_uva.fits ! AN table 1: 27 integrations on 120 of 120 possible baselines. ! AN table 2: 41 integrations on 120 of 120 possible baselines. ! AN table 3: 108 integrations on 120 of 120 possible baselines. ! AN table 4: 95 integrations on 120 of 120 possible baselines. ! Apparent sampling: 0.168173 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0555+3948 ! ! 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 2288 lines of history. ! ! Reading 21876 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 342 telescope corrections were flagged in sub-array 1. ! A total of 343 telescope corrections were flagged in sub-array 2. ! A total of 1213 telescope corrections were flagged in sub-array 3. ! A total of 809 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 342 telescope corrections were flagged in sub-array 1. ! A total of 343 telescope corrections were flagged in sub-array 2. ! A total of 1216 telescope corrections were flagged in sub-array 3. ! A total of 809 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 342 telescope corrections were flagged in sub-array 1. ! A total of 343 telescope corrections were flagged in sub-array 2. ! A total of 1202 telescope corrections were flagged in sub-array 3. ! A total of 809 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 342 telescope corrections were flagged in sub-array 1. ! A total of 343 telescope corrections were flagged in sub-array 2. ! A total of 1199 telescope corrections were flagged in sub-array 3. ! A total of 809 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=2.454410Jy sigma=0.023184 ! Fit after self-cal, rms=2.219067Jy sigma=0.021568 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.21% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! Estimated beam: bmin=0.6601 mas, bmaj=0.9206 mas, bpa=-1.805 degrees ! Estimated noise=1289.05 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.07616 Jy ! Component: 100 - total flux cleaned = 2.81529 Jy ! Total flux subtracted in 100 components = 2.81529 Jy ! Clean residual min=-0.084202 max=0.382683 Jy/beam ! Clean residual mean=-0.000227 rms=0.029767 Jy/beam ! Combined flux in latest and established models = 2.81529 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 13 components and 2.81529 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.867716Jy sigma=0.008438 ! Fit after self-cal, rms=0.863787Jy sigma=0.008423 ! Inverting map ! Your choice of large map pixels excluded 3.21% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! Added new window around map position (-0.6, 0.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.434139 Jy ! Component: 100 - total flux cleaned = 0.700316 Jy ! Total flux subtracted in 100 components = 0.700316 Jy ! Clean residual min=-0.050743 max=0.151686 Jy/beam ! Clean residual mean=-0.000139 rms=0.015633 Jy/beam ! Combined flux in latest and established models = 3.51561 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 26 components and 3.51561 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.475800Jy sigma=0.004326 ! Fit after self-cal, rms=0.468474Jy sigma=0.004288 ! Inverting map ! Your choice of large map pixels excluded 3.21% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.183974 Jy ! Component: 100 - total flux cleaned = 0.304569 Jy ! Total flux subtracted in 100 components = 0.304569 Jy ! Clean residual min=-0.037696 max=0.072021 Jy/beam ! Clean residual mean=-0.000100 rms=0.010637 Jy/beam ! Combined flux in latest and established models = 3.82018 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 32 components and 3.82018 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.353546Jy sigma=0.002899 ! Fit after self-cal, rms=0.350563Jy sigma=0.002880 ! Inverting map ! Your choice of large map pixels excluded 3.21% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0886027 Jy ! Component: 100 - total flux cleaned = 0.14764 Jy ! Total flux subtracted in 100 components = 0.14764 Jy ! Clean residual min=-0.035650 max=0.038995 Jy/beam ! Clean residual mean=-0.000081 rms=0.008981 Jy/beam ! Combined flux in latest and established models = 3.96782 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 39 components and 3.96782 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.320856Jy sigma=0.002454 ! Fit after self-cal, rms=0.319433Jy sigma=0.002445 ! Inverting map ! Your choice of large map pixels excluded 3.21% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec print "************** FINISHED UNIFORM WEIGHTING CLEAN **************" ! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** ! uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. win_mult = win_mult * 1.6 clean_niter = clean_niter * 2 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.21% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! Estimated beam: bmin=0.8485 mas, bmaj=1.47 mas, bpa=-3.975 degrees ! Estimated noise=558.963 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 = 0.0641231 Jy ! Component: 100 - total flux cleaned = 0.0936577 Jy ! Component: 150 - total flux cleaned = 0.108801 Jy ! Component: 200 - total flux cleaned = 0.116814 Jy ! Total flux subtracted in 200 components = 0.116814 Jy ! Clean residual min=-0.032477 max=0.033588 Jy/beam ! Clean residual mean=-0.000467 rms=0.008813 Jy/beam ! Combined flux in latest and established models = 4.08463 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 44 components and 4.08463 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.310171Jy sigma=0.002290 ! Fit after self-cal, rms=0.309418Jy sigma=0.002285 ! Inverting map ! Your choice of large map pixels excluded 3.21% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* HH 0.93 HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MK 1.00* ! NL 1.00* NY 1.06 ON 0.97 OV 1.00* ! PT 1.00* SC 1.00* WZ 1.01 ZC 0.89 ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.94 FD 0.98 HH 1.00* HN 0.99 ! KK 1.00* KP 0.99 LA 0.98 MK 1.07 ! NL 0.92 NY 1.02 ON 1.05 OV 1.01 ! PT 0.98 SC 0.95 WZ 1.00* ZC 1.00* ! ! A total of 60 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 1.05 HH 1.23 HN 1.04 ! KK 1.00* KP 1.06 LA 1.04 MK 1.00* ! NL 0.96 NY 1.01 ON 0.96 OV 1.05 ! PT 1.05 SC 1.17 WZ 1.00 ZC 1.12 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.94 FD 0.99 HH 1.00* HN 1.00 ! KK 0.96 KP 1.02 LA 0.99 MK 0.99 ! NL 0.98 NY 1.02 ON 1.00* OV 1.00 ! PT 0.98 SC 0.99 WZ 1.00* ZC 1.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* HH 0.93 HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MK 1.00* ! NL 1.00* NY 1.04 ON 0.98 OV 1.00* ! PT 1.00* SC 1.00* WZ 1.05 ZC 0.92 ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.95 FD 0.97 HH 1.00* HN 0.99 ! KK 1.00* KP 0.94 LA 0.97 MK 1.08 ! NL 0.90 NY 1.05 ON 1.04 OV 0.98 ! PT 0.97 SC 0.95 WZ 1.00* ZC 1.00* ! ! A total of 51 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.05 HH 1.17 HN 0.99 ! KK 1.00* KP 0.99 LA 1.03 MK 1.00* ! NL 0.95 NY 1.01 ON 0.96 OV 1.03 ! PT 1.03 SC 0.96 WZ 1.04 ZC 1.19 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.95 FD 0.98 HH 1.00* HN 1.00 ! KK 0.95 KP 0.97 LA 0.98 MK 0.99 ! NL 0.95 NY 1.05 ON 1.00* OV 0.98 ! PT 0.97 SC 1.00 WZ 1.00* ZC 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* HH 0.94 HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MK 1.00* ! NL 1.00* NY 1.10 ON 0.95 OV 1.00* ! PT 1.00* SC 1.00* WZ 1.00 ZC 0.94 ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 1.00 HH 1.00* HN 1.00 ! KK 1.00* KP 0.98 LA 1.01 MK 1.10 ! NL 0.93 NY 1.03 ON 1.01 OV 1.03 ! PT 0.98 SC 0.99 WZ 1.00* ZC 1.00* ! ! A total of 57 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 FD 1.07 HH 1.27 HN 0.99 ! KK 1.00* KP 1.05 LA 1.07 MK 1.00* ! NL 0.99 NY 0.99 ON 0.99 OV 1.08 ! PT 1.04 SC 1.00 WZ 0.99 ZC 1.18 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 1.01 HH 1.00* HN 1.01 ! KK 1.01 KP 1.01 LA 1.02 MK 1.00 ! NL 0.99 NY 1.05 ON 1.00* OV 1.03 ! PT 0.98 SC 1.03 WZ 1.00* ZC 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* HH 0.95 HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MK 1.00* ! NL 1.00* NY 1.07 ON 1.01 OV 1.00* ! PT 1.00* SC 1.00* WZ 1.00 ZC 0.98 ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 FD 1.00 HH 1.00* HN 1.00 ! KK 1.00* KP 0.98 LA 0.99 MK 1.11 ! NL 0.94 NY 1.06 ON 1.02 OV 1.03 ! PT 0.98 SC 1.00 WZ 1.00* ZC 1.00* ! ! A total of 60 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 1.07 HH 1.32 HN 1.00 ! KK 1.00* KP 1.04 LA 1.06 MK 1.00* ! NL 1.01 NY 1.02 ON 1.01 OV 1.07 ! PT 1.04 SC 1.02 WZ 1.00 ZC 1.17 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 FD 1.00 HH 1.00* HN 1.02 ! KK 1.00 KP 1.01 LA 1.01 MK 1.02 ! NL 1.00 NY 1.10 ON 1.00* OV 1.02 ! PT 0.97 SC 1.04 WZ 1.00* ZC 1.00* ! ! ! Fit before self-cal, rms=0.309418Jy sigma=0.002285 ! Fit after self-cal, rms=0.252054Jy sigma=0.001574 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! Estimated beam: bmin=0.8542 mas, bmaj=1.493 mas, bpa=-4.331 degrees ! Estimated noise=560.36 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 (-1.2, 0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0117326 Jy ! Component: 100 - total flux cleaned = 0.0113285 Jy ! Component: 150 - total flux cleaned = 0.0106185 Jy ! Component: 200 - total flux cleaned = 0.00968729 Jy ! Total flux subtracted in 200 components = 0.00968729 Jy ! Clean residual min=-0.012201 max=0.013188 Jy/beam ! Clean residual mean=0.000175 rms=0.002982 Jy/beam ! Combined flux in latest and established models = 4.09432 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 58 components and 4.09432 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.250468Jy sigma=0.001559 ! Fit after self-cal, rms=0.250277Jy sigma=0.001556 ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 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=0.250277Jy sigma=0.001556 ! Fit after self-cal, rms=0.235054Jy sigma=0.001445 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! Estimated beam: bmin=0.8528 mas, bmaj=1.495 mas, bpa=-4.318 degrees ! Estimated noise=560.424 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00555766 Jy ! Component: 100 - total flux cleaned = 0.00431391 Jy ! Component: 150 - total flux cleaned = 0.00353869 Jy ! Component: 200 - total flux cleaned = 0.00330565 Jy ! Total flux subtracted in 200 components = 0.00330565 Jy ! Clean residual min=-0.008731 max=0.006666 Jy/beam ! Clean residual mean=0.000020 rms=0.001713 Jy/beam ! Combined flux in latest and established models = 4.09762 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 63 components and 4.09762 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.234122Jy sigma=0.001437 ! Fit after self-cal, rms=0.233949Jy sigma=0.001436 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 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 = 0.00102468 Jy ! Component: 100 - total flux cleaned = 0.00102306 Jy ! Component: 150 - total flux cleaned = 0.0010123 Jy ! Component: 200 - total flux cleaned = 0.000829745 Jy ! Total flux subtracted in 200 components = 0.000829745 Jy ! Clean residual min=-0.007641 max=0.006271 Jy/beam ! Clean residual mean=0.000019 rms=0.001616 Jy/beam ! Combined flux in latest and established models = 4.09845 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 67 components and 4.09845 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.233391Jy sigma=0.001431 ! Fit after self-cal, rms=0.233276Jy sigma=0.001431 ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 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=0.233276Jy sigma=0.001431 ! Fit after self-cal, rms=0.225758Jy sigma=0.001395 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! Estimated beam: bmin=0.8522 mas, bmaj=1.496 mas, bpa=-4.301 degrees ! Estimated noise=560.322 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0031819 Jy ! Component: 100 - total flux cleaned = 0.00379788 Jy ! Component: 150 - total flux cleaned = 0.00362387 Jy ! Component: 200 - total flux cleaned = 0.00362815 Jy ! Total flux subtracted in 200 components = 0.00362815 Jy ! Clean residual min=-0.006153 max=0.004953 Jy/beam ! Clean residual mean=0.000021 rms=0.001262 Jy/beam ! Combined flux in latest and established models = 4.10208 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 71 components and 4.10208 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.225145Jy sigma=0.001392 ! Fit after self-cal, rms=0.225038Jy sigma=0.001391 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 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 = 0.000563448 Jy ! Component: 100 - total flux cleaned = 0.000736234 Jy ! Component: 150 - total flux cleaned = 0.000579923 Jy ! Component: 200 - total flux cleaned = 0.000434927 Jy ! Total flux subtracted in 200 components = 0.000434927 Jy ! Clean residual min=-0.006037 max=0.004700 Jy/beam ! Clean residual mean=0.000020 rms=0.001197 Jy/beam ! Combined flux in latest and established models = 4.10252 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 73 components and 4.10252 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.224580Jy sigma=0.001388 ! Fit after self-cal, rms=0.224494Jy sigma=0.001388 ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 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=0.224494Jy sigma=0.001388 ! Fit after self-cal, rms=0.224477Jy sigma=0.001388 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! Estimated beam: bmin=2.516 mas, bmaj=3.005 mas, bpa=-6.165 degrees ! Estimated noise=697.956 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0029311 Jy ! Component: 100 - total flux cleaned = 0.00319172 Jy ! Component: 150 - total flux cleaned = 0.00338372 Jy ! Component: 200 - total flux cleaned = 0.0034849 Jy ! Total flux subtracted in 200 components = 0.0034849 Jy ! Clean residual min=-0.003405 max=0.003778 Jy/beam ! Clean residual mean=0.000047 rms=0.000937 Jy/beam ! Combined flux in latest and established models = 4.106 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 79 components and 4.106 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.224411Jy sigma=0.001387 ! Fit after self-cal, rms=0.224347Jy sigma=0.001387 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 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 = 0.000153007 Jy ! Component: 100 - total flux cleaned = 0.000224975 Jy ! Component: 150 - total flux cleaned = 0.000385727 Jy ! Component: 200 - total flux cleaned = 0.00046936 Jy ! Total flux subtracted in 200 components = 0.00046936 Jy ! Clean residual min=-0.003264 max=0.003703 Jy/beam ! Clean residual mean=0.000046 rms=0.000922 Jy/beam ! Combined flux in latest and established models = 4.10647 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 80 components and 4.10647 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.224320Jy sigma=0.001386 ! Fit after self-cal, rms=0.224266Jy sigma=0.001386 ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 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 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! Estimated beam: bmin=0.852 mas, bmaj=1.496 mas, bpa=-4.291 degrees ! Estimated noise=560.415 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.852 x 1.496 at -4.291 degrees (North through East) ! Clean map min=-0.0044627 max=2.9451 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=0.224266Jy sigma=0.001386 ! Fit after self-cal, rms=0.196591Jy sigma=0.001134 ! Inverting map and beam ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! Estimated beam: bmin=0.8516 mas, bmaj=1.494 mas, bpa=-4.255 degrees ! Estimated noise=560.015 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000264557 Jy ! Component: 100 - total flux cleaned = -6.29815e-05 Jy ! Component: 150 - total flux cleaned = -0.000343529 Jy ! Component: 200 - total flux cleaned = -0.000470263 Jy ! Total flux subtracted in 200 components = -0.000470263 Jy ! Clean residual min=-0.004782 max=0.004523 Jy/beam ! Clean residual mean=0.000022 rms=0.001017 Jy/beam ! Combined flux in latest and established models = 4.106 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 82 components and 4.106 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.196294Jy sigma=0.001132 ! Fit after self-cal, rms=0.196258Jy sigma=0.001132 ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000399569 Jy ! Component: 100 - total flux cleaned = 0.000272537 Jy ! Component: 150 - total flux cleaned = 0.000275641 Jy ! Component: 200 - total flux cleaned = 0.000281374 Jy ! Total flux subtracted in 200 components = 0.000281374 Jy ! Clean residual min=-0.004697 max=0.004150 Jy/beam ! Clean residual mean=0.000021 rms=0.000984 Jy/beam ! Combined flux in latest and established models = 4.10629 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 84 components and 4.10629 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.196008Jy sigma=0.001130 ! Fit after self-cal, rms=0.195971Jy sigma=0.001130 ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.195971Jy sigma=0.001130 ! Fit after self-cal, rms=0.195973Jy sigma=0.001130 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 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! Estimated beam: bmin=0.6649 mas, bmaj=0.9492 mas, bpa=-3.924 degrees ! Estimated noise=1278.95 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.10568 Jy ! Component: 100 - total flux cleaned = 2.87396 Jy ! Component: 150 - total flux cleaned = 3.29043 Jy ! Component: 200 - total flux cleaned = 3.55493 Jy ! Total flux subtracted in 200 components = 3.55493 Jy ! Clean residual min=-0.036625 max=0.141455 Jy/beam ! Clean residual mean=-0.000081 rms=0.012044 Jy/beam ! Combined flux in latest and established models = 3.55493 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 27 model components to the UV plane model. ! The established model now contains 27 components and 3.55493 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! Estimated beam: bmin=0.8518 mas, bmaj=1.494 mas, bpa=-4.244 degrees ! Estimated noise=560.143 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 = 0.265885 Jy ! Component: 100 - total flux cleaned = 0.398261 Jy ! Component: 150 - total flux cleaned = 0.467285 Jy ! Component: 200 - total flux cleaned = 0.5047 Jy ! Total flux subtracted in 200 components = 0.5047 Jy ! Clean residual min=-0.007343 max=0.020981 Jy/beam ! Clean residual mean=0.000020 rms=0.002493 Jy/beam ! Combined flux in latest and established models = 4.05963 Jy ! Adding 39 model components to the UV plane model. ! The established model now contains 52 components and 4.05963 Jy ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! Added new window around map position (0.8, 0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.021851 Jy ! Component: 100 - total flux cleaned = 0.0332229 Jy ! Component: 150 - total flux cleaned = 0.0355219 Jy ! Component: 200 - total flux cleaned = 0.0372498 Jy ! Total flux subtracted in 200 components = 0.0372498 Jy ! Clean residual min=-0.005312 max=0.006274 Jy/beam ! Clean residual mean=0.000023 rms=0.001206 Jy/beam ! Combined flux in latest and established models = 4.09688 Jy ! Adding 22 model components to the UV plane model. ! The established model now contains 63 components and 4.09688 Jy ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! Added new window around map position (-2, -3). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00229862 Jy ! Component: 100 - total flux cleaned = 0.00403977 Jy ! Component: 150 - total flux cleaned = 0.00537289 Jy ! Component: 200 - total flux cleaned = 0.00660793 Jy ! Total flux subtracted in 200 components = 0.00660793 Jy ! Clean residual min=-0.004489 max=0.004507 Jy/beam ! Clean residual mean=0.000023 rms=0.001076 Jy/beam ! Combined flux in latest and established models = 4.10349 Jy ! Adding 17 model components to the UV plane model. ! The established model now contains 69 components and 4.10348 Jy ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 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 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! Estimated beam: bmin=2.515 mas, bmaj=3.006 mas, bpa=-6.081 degrees ! Estimated noise=697.906 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00329834 Jy ! Component: 100 - total flux cleaned = 0.00402304 Jy ! Component: 150 - total flux cleaned = 0.00436461 Jy ! Component: 200 - total flux cleaned = 0.00460379 Jy ! Total flux subtracted in 200 components = 0.00460379 Jy ! Clean residual min=-0.002418 max=0.002758 Jy/beam ! Clean residual mean=0.000050 rms=0.000769 Jy/beam ! Combined flux in latest and established models = 4.10809 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 = 6.83714e-05 Jy ! Component: 100 - total flux cleaned = 0.000101435 Jy ! Component: 150 - total flux cleaned = 0.000131322 Jy ! Component: 200 - total flux cleaned = 0.000157826 Jy ! Total flux subtracted in 200 components = 0.000157826 Jy ! Clean residual min=-0.002352 max=0.002697 Jy/beam ! Clean residual mean=0.000050 rms=0.000747 Jy/beam ! Combined flux in latest and established models = 4.10825 Jy ! Adding 31 model components to the UV plane model. ! The established model now contains 93 components and 4.10825 Jy ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! Estimated beam: bmin=0.8518 mas, bmaj=1.494 mas, bpa=-4.244 degrees ! Estimated noise=560.143 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00222399 Jy ! Component: 100 - total flux cleaned = -0.0020055 Jy ! Component: 150 - total flux cleaned = -0.00160724 Jy ! Component: 200 - total flux cleaned = -0.00142015 Jy ! Total flux subtracted in 200 components = -0.00142015 Jy ! Clean residual min=-0.004333 max=0.004480 Jy/beam ! Clean residual mean=0.000021 rms=0.001015 Jy/beam ! Combined flux in latest and established models = 4.10683 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 97 components and 4.10683 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.208706Jy sigma=0.001162 ! Fit after self-cal, rms=0.207530Jy sigma=0.001156 wmodel J0555+3948_X_2008_04_02_pus_map.mod ! Writing 97 model components to file: J0555+3948_X_2008_04_02_pus_map.mod wobs J0555+3948_X_2008_04_02_pus_uvs.fits ! Writing UV FITS file: J0555+3948_X_2008_04_02_pus_uvs.fits wwins J0555+3948_X_2008_04_02_pus_map.win ! wwins: Wrote 5 windows to J0555+3948_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 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000722395 Jy ! Component: 100 - total flux cleaned = 0.000646021 Jy ! Component: 150 - total flux cleaned = 0.00057271 Jy ! Component: 200 - total flux cleaned = 0.000717921 Jy ! Component: 250 - total flux cleaned = 0.000859232 Jy ! Component: 300 - total flux cleaned = 0.000788483 Jy ! Component: 350 - total flux cleaned = 0.000518292 Jy ! Component: 400 - total flux cleaned = 0.000451123 Jy ! Component: 450 - total flux cleaned = 0.000255543 Jy ! Component: 500 - total flux cleaned = 0.000126973 Jy ! Component: 550 - total flux cleaned = 1.4235e-07 Jy ! Component: 600 - total flux cleaned = -0.000124712 Jy ! Component: 650 - total flux cleaned = -0.000124292 Jy ! Component: 700 - total flux cleaned = -0.000185182 Jy ! Component: 750 - total flux cleaned = -0.00012554 Jy ! Component: 800 - total flux cleaned = -0.000362537 Jy ! Component: 850 - total flux cleaned = -0.000246207 Jy ! Component: 900 - total flux cleaned = -0.000421036 Jy ! Component: 950 - total flux cleaned = -0.000421205 Jy ! Component: 1000 - total flux cleaned = -0.000420554 Jy ! Component: 1050 - total flux cleaned = -0.000307492 Jy ! Component: 1100 - total flux cleaned = -0.000476307 Jy ! Component: 1150 - total flux cleaned = -0.000532648 Jy ! Component: 1200 - total flux cleaned = -0.000587383 Jy ! Component: 1250 - total flux cleaned = -0.00053214 Jy ! Component: 1300 - total flux cleaned = -0.00064198 Jy ! Component: 1350 - total flux cleaned = -0.000696107 Jy ! Component: 1400 - total flux cleaned = -0.000696034 Jy ! Component: 1450 - total flux cleaned = -0.000749216 Jy ! Component: 1500 - total flux cleaned = -0.000643019 Jy ! Component: 1550 - total flux cleaned = -0.000695565 Jy ! Component: 1600 - total flux cleaned = -0.00059023 Jy ! Component: 1650 - total flux cleaned = -0.000590038 Jy ! Component: 1700 - total flux cleaned = -0.00053867 Jy ! Component: 1750 - total flux cleaned = -0.000641372 Jy ! Component: 1800 - total flux cleaned = -0.000590004 Jy ! Component: 1850 - total flux cleaned = -0.000692493 Jy ! Component: 1900 - total flux cleaned = -0.00074294 Jy ! Component: 1950 - total flux cleaned = -0.000743156 Jy ! Component: 2000 - total flux cleaned = -0.000592523 Jy ! Total flux subtracted in 2048 components = -0.000692503 Jy ! Clean residual min=-0.003011 max=0.002585 Jy/beam ! Clean residual mean=0.000022 rms=0.000804 Jy/beam ! Combined flux in latest and established models = 4.10613 Jy keep ! Adding 109 model components to the UV plane model. ! The established model now contains 198 components and 4.10613 Jy wmap "J0555+3948_X_2008_04_02_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8518 x 1.494 at -4.244 degrees (North through East) ! Clean map min=-0.0032805 max=2.9442 Jy/beam ! Writing clean map to FITS file: J0555+3948_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 2.94423 invert ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1801 milli-arcsec ! The y-axis pixel size should ideally be below 0.153 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000803504 device "J0555+3948_X_2008_04_02_pus\_map.eps/VPS" ! Attempting to open device: 'J0555+3948_X_2008_04_02_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.0818725 0.0818725 0.163745 0.32749 0.65498 1.30996 2.61992 5.23984 10.4797 20.9594 41.9187 83.8374 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0024 print "peak=",int(1000*peak_flux)/1000 ! peak= 2.944 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8518 x 1.494 at -4.244 degrees (North through East) ! Clean map min=-0.0032805 max=2.9442 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0555+3948_X_2008_04_02_pus\_map.gif/vgif" ! Attempting to open device: 'J0555+3948_X_2008_04_02_pus_map.gif/vgif' mapplot cln quit ! Quitting program ! Log file J0555+3948_X_2008_04_02_pus_uvs.log closed on Sun Feb 21 20:46:06 2010