! Started logfile: 2209+236_X.log on Tue Aug 2 16:28:19 2005 observe 2209+236_X.edt ! Reading UV FITS file: 2209+236_X.edt ! AN table 1: 58 integrations on 171 of 171 possible baselines. ! AN table 2: 49 integrations on 171 of 171 possible baselines. ! AN table 3: 47 integrations on 171 of 171 possible baselines. ! AN table 4: 18 integrations on 171 of 171 possible baselines. ! AN table 5: 23 integrations on 171 of 171 possible baselines. ! Apparent sampling: 0.14266 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 2209+236 ! ! 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 1818 lines of history. ! ! Reading 19028 visibilities. ![@gonzo8-0.1 2209+236_X] print "***********************************" ! *********************************** print "*** Using gonzo instruction set ***" ! *** Using gonzo instruction set *** print "***********************************" ! *********************************** float field_size field_size = 1024 float field_cell field_cell = 0.1 integer clean_niter clean_niter = 50 float clean_gain clean_gain = 0.03 float dynam dynam = 8.0 float win_mult win_mult = 1.8 float solint solint = 3.6/6.0 logical doflt doflt = true logical doamp float new_peak float flux_cutoff mapsize field_size,field_cell ! Map grid = 1024x1024 pixels with 0.100x0.100 milli-arcsec cellsize. select ! 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 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 831 telescope corrections were flagged in sub-array 1. ! A total of 651 telescope corrections were flagged in sub-array 2. ! A total of 795 telescope corrections were flagged in sub-array 3. ! A total of 262 telescope corrections were flagged in sub-array 4. ! A total of 317 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 832 telescope corrections were flagged in sub-array 1. ! A total of 651 telescope corrections were flagged in sub-array 2. ! A total of 795 telescope corrections were flagged in sub-array 3. ! A total of 262 telescope corrections were flagged in sub-array 4. ! A total of 317 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 833 telescope corrections were flagged in sub-array 1. ! A total of 651 telescope corrections were flagged in sub-array 2. ! A total of 789 telescope corrections were flagged in sub-array 3. ! A total of 259 telescope corrections were flagged in sub-array 4. ! A total of 317 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 832 telescope corrections were flagged in sub-array 1. ! A total of 651 telescope corrections were flagged in sub-array 2. ! A total of 801 telescope corrections were flagged in sub-array 3. ! A total of 259 telescope corrections were flagged in sub-array 4. ! A total of 317 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=0.109989Jy sigma=0.001956 ! Fit after self-cal, rms=0.109364Jy sigma=0.001951 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvweight 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. doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.8128 mas, bmaj=1.172 mas, bpa=7.052 degrees ! Estimated noise=670.338 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0, 0). ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.775704 Jy ! Total flux subtracted in 50 components = 0.775704 Jy ! Clean residual min=-0.029726 max=0.216390 Jy/beam ! Clean residual mean=0.000222 rms=0.009226 Jy/beam ! Combined flux in latest and established models = 0.775704 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 0.775704 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.271342Jy sigma=0.005146 ! Fit after self-cal, rms=0.271341Jy sigma=0.005146 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.169602 Jy ! Total flux subtracted in 50 components = 0.169602 Jy ! Clean residual min=-0.012298 max=0.050566 Jy/beam ! Clean residual mean=0.000077 rms=0.003682 Jy/beam ! Combined flux in latest and established models = 0.945306 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.945306 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.133246Jy sigma=0.002496 ! Fit after self-cal, rms=0.133249Jy sigma=0.002496 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.052173 Jy ! Total flux subtracted in 50 components = 0.052173 Jy ! Clean residual min=-0.009991 max=0.023901 Jy/beam ! Clean residual mean=0.000032 rms=0.002694 Jy/beam ! Combined flux in latest and established models = 0.997479 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 14 model components to the UV plane model. ! The established model now contains 20 components and 0.997479 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.107433Jy sigma=0.001941 ! Fit after self-cal, rms=0.107395Jy sigma=0.001941 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0283774 Jy ! Total flux subtracted in 50 components = 0.0283774 Jy ! Clean residual min=-0.008896 max=0.015752 Jy/beam ! Clean residual mean=0.000007 rms=0.002316 Jy/beam ! Combined flux in latest and established models = 1.02586 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 12 model components to the UV plane model. ! The established model now contains 30 components and 1.02586 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.098045Jy sigma=0.001722 ! Fit after self-cal, rms=0.097978Jy sigma=0.001721 ! Inverting map print "****************************************" ! **************************************** print "*** Finished Uniform Weighting CLEAN ***" ! *** Finished Uniform Weighting CLEAN *** print "****************************************" ! **************************************** uvweight 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 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=1.101 mas, bmaj=1.721 mas, bpa=4.841 degrees ! Estimated noise=376.175 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0320655 Jy ! Component: 100 - total flux cleaned = 0.0474841 Jy ! Total flux subtracted in 100 components = 0.0474841 Jy ! Clean residual min=-0.007477 max=0.011833 Jy/beam ! Clean residual mean=-0.000085 rms=0.002200 Jy/beam ! Combined flux in latest and established models = 1.07334 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 46 model components to the UV plane model. ! The established model now contains 71 components and 1.07334 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.090283Jy sigma=0.001515 ! Fit after self-cal, rms=0.090048Jy sigma=0.001511 ! Inverting map print "****************************************" ! **************************************** print "*** Finished Natural Weighting CLEAN ***" ! *** Finished Natural Weighting CLEAN *** print "****************************************" ! **************************************** gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.98 GC 1.00* HH 1.00* ! HN 1.00 KK 1.00* KP 1.01 LA 1.01 ! MC 1.00* MK 1.00 NL 1.02 NY 1.00 ! ON 1.00* OV 1.00 PT 1.00 SC 1.00* ! TS 1.00* WF 1.04 WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 1.03 GC 1.00* HH 1.00* ! HN 0.99 KK 1.00* KP 0.99 LA 0.97 ! MC 1.00* MK 1.03 NL 0.97 NY 1.00* ! ON 1.00* OV 0.98 PT 1.02 SC 1.01 ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 33 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.09 FD 1.05 GC 1.00* HH 1.00* ! HN 1.02 KK 1.00* KP 1.00* LA 1.05 ! MC 1.00* MK 1.00* NL 1.05 NY 1.00* ! ON 1.00* OV 1.00* PT 1.00 SC 1.01 ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.04 FD 1.01 GC 1.00* HH 1.00* ! HN 1.05 KK 1.00* KP 1.04 LA 1.02 ! MC 1.00* MK 1.00* NL 1.01 NY 1.00* ! ON 1.00* OV 1.00 PT 1.01 SC 0.96 ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 FD 0.97 GC 1.00* HH 1.00* ! HN 0.96 KK 1.00* KP 0.95 LA 0.96 ! MC 1.00* MK 1.00* NL 1.04 NY 1.00* ! ON 1.00* OV 0.95 PT 0.92 SC 1.00 ! TS 1.00* WF 1.00* WZ 1.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.99 GC 1.00* HH 1.00* ! HN 0.98 KK 1.00* KP 1.01 LA 1.00 ! MC 1.00* MK 0.99 NL 1.00 NY 1.02 ! ON 1.00* OV 1.00 PT 0.99 SC 1.00* ! TS 1.00* WF 1.05 WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 1.03 GC 1.00* HH 1.00* ! HN 0.99 KK 1.00* KP 0.99 LA 0.98 ! MC 1.00* MK 1.05 NL 0.97 NY 1.00* ! ON 1.00* OV 1.00 PT 1.02 SC 1.04 ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 33 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.09 FD 1.04 GC 1.00* HH 1.00* ! HN 1.01 KK 1.00* KP 1.00* LA 1.06 ! MC 1.00* MK 1.00* NL 1.00 NY 1.00* ! ON 1.00* OV 1.00* PT 1.02 SC 1.01 ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.04 FD 1.01 GC 1.00* HH 1.00* ! HN 1.04 KK 1.00* KP 1.04 LA 1.03 ! MC 1.00* MK 1.00* NL 0.99 NY 1.00* ! ON 1.00* OV 1.01 PT 1.01 SC 0.98 ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 FD 0.97 GC 1.00* HH 1.00* ! HN 0.96 KK 1.00* KP 0.97 LA 0.97 ! MC 1.00* MK 1.00* NL 1.01 NY 1.00* ! ON 1.00* OV 0.93 PT 0.95 SC 0.99 ! TS 1.00* WF 1.00* WZ 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 0.98 GC 1.00* HH 1.00* ! HN 1.00 KK 1.00* KP 1.00 LA 1.00 ! MC 1.00* MK 1.00 NL 1.02 NY 1.04 ! ON 1.00* OV 1.00 PT 0.98 SC 1.00* ! TS 1.00* WF 1.02 WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 1.03 GC 1.00* HH 1.00* ! HN 0.99 KK 1.00* KP 0.98 LA 0.96 ! MC 1.00* MK 1.01 NL 0.97 NY 1.00* ! ON 1.00* OV 0.99 PT 1.03 SC 1.04 ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 39 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.11 FD 1.02 GC 1.00* HH 1.00* ! HN 1.02 KK 1.00* KP 1.00* LA 1.03 ! MC 1.00* MK 1.00* NL 1.00 NY 1.00* ! ON 1.00* OV 1.00* PT 1.03 SC 1.00 ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 FD 0.99 GC 1.00* HH 1.00* ! HN 0.99 KK 1.00* KP 1.03 LA 1.03 ! MC 1.00* MK 1.00* NL 0.98 NY 1.00* ! ON 1.00* OV 1.02 PT 1.03 SC 1.02 ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 0.99 GC 1.00* HH 1.00* ! HN 0.97 KK 1.00* KP 0.98 LA 0.96 ! MC 1.00* MK 1.00* NL 1.00 NY 1.00* ! ON 1.00* OV 0.96 PT 0.97 SC 1.02 ! TS 1.00* WF 1.00* WZ 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.98 GC 1.00* HH 1.00* ! HN 1.00 KK 1.00* KP 0.98 LA 0.99 ! MC 1.00* MK 1.01 NL 1.02 NY 1.03 ! ON 1.00* OV 0.99 PT 0.98 SC 1.00* ! TS 1.00* WF 1.02 WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 1.03 GC 1.00* HH 1.00* ! HN 0.99 KK 1.00* KP 0.99 LA 0.96 ! MC 1.00* MK 1.01 NL 0.96 NY 1.00* ! ON 1.00* OV 0.98 PT 1.03 SC 1.07 ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.07 FD 1.05 GC 1.00* HH 1.00* ! HN 1.03 KK 1.00* KP 1.00* LA 1.02 ! MC 1.00* MK 1.00* NL 1.01 NY 1.00* ! ON 1.00* OV 1.00* PT 1.01 SC 1.01 ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 1.03 GC 1.00* HH 1.00* ! HN 1.09 KK 1.00* KP 1.02 LA 1.02 ! MC 1.00* MK 1.00* NL 1.00 NY 1.00* ! ON 1.00* OV 1.01 PT 1.00 SC 0.97 ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 FD 0.97 GC 1.00* HH 1.00* ! HN 0.97 KK 1.00* KP 0.96 LA 0.97 ! MC 1.00* MK 1.00* NL 1.00 NY 1.00* ! ON 1.00* OV 0.95 PT 0.99 SC 1.07 ! TS 1.00* WF 1.00* WZ 1.00* ! ! ! Fit before self-cal, rms=0.090048Jy sigma=0.001511 ! Fit after self-cal, rms=0.078777Jy sigma=0.001293 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=1.105 mas, bmaj=1.741 mas, bpa=4.717 degrees ! Estimated noise=375.243 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0.8, 2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00796132 Jy ! Component: 100 - total flux cleaned = 0.00777422 Jy ! Total flux subtracted in 100 components = 0.00777422 Jy ! Clean residual min=-0.004768 max=0.004834 Jy/beam ! Clean residual mean=0.000019 rms=0.001299 Jy/beam ! Combined flux in latest and established models = 1.08111 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 16 model components to the UV plane model. ! The established model now contains 84 components and 1.08111 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.077807Jy sigma=0.001272 ! Fit after self-cal, rms=0.077654Jy sigma=0.001270 ! Inverting map dynam = dynam - 1.0 doamp = true solint = solint * (6.0/3.6) 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 doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00119298 Jy ! Component: 100 - total flux cleaned = 0.000958377 Jy ! Total flux subtracted in 100 components = 0.000958377 Jy ! Clean residual min=-0.004589 max=0.004782 Jy/beam ! Clean residual mean=0.000021 rms=0.001275 Jy/beam ! Combined flux in latest and established models = 1.08207 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 20 model components to the UV plane model. ! The established model now contains 96 components and 1.08207 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.077423Jy sigma=0.001266 ! Fit after self-cal, rms=0.070673Jy sigma=0.001165 ! Inverting map and beam ! Estimated beam: bmin=1.103 mas, bmaj=1.738 mas, bpa=4.751 degrees ! Estimated noise=375.345 mJy/beam. doamp = false solint = solint / (6.0/3.6) 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 doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00328648 Jy ! Component: 100 - total flux cleaned = 0.00365084 Jy ! Total flux subtracted in 100 components = 0.00365084 Jy ! Clean residual min=-0.002349 max=0.002644 Jy/beam ! Clean residual mean=0.000022 rms=0.000577 Jy/beam ! Combined flux in latest and established models = 1.08572 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 18 model components to the UV plane model. ! The established model now contains 112 components and 1.08572 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070495Jy sigma=0.001161 ! Fit after self-cal, rms=0.070459Jy sigma=0.001160 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 2209+236_X ! Writing UV FITS file: 2209+236_X.uvf ! Writing 112 model components to file: 2209+236_X.mod ! wwins: Wrote 2 windows to 2209+236_X.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.103 x 1.738 at 4.751 degrees (North through East) ! Clean map min=-0.002382 max=1.0146 Jy/beam ! Writing clean map to FITS file: 2209+236_X.fits ! Writing difmap environment to: 2209+236_X.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 2209+236_X] device 2209+236_Xuv.ps/vps,1,2 ! Attempting to open device: '2209+236_Xuv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 2209+236_Xim.ps/vps ! Attempting to open device: '2209+236_Xim.ps/vps' uvweight 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. loglevs -1,2048,2 ! The new contour levels are: ! -1 1 2 4 8 16 32 64 128 256 512 1024 2048 cmul = imstat(rms)*3 ! Inverting map and beam ! Estimated beam: bmin=1.103 mas, bmaj=1.738 mas, bpa=4.751 degrees ! Estimated noise=375.345 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.103 x 1.738 at 4.751 degrees (North through East) ! Clean map min=-0.002382 max=1.0146 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo8-0.1] quit ! Quitting program ! Log file 2209+236_X.log closed on Tue Aug 2 16:28:47 2005