! Started logfile: J1832-2039_S_1997_07_02_yyk_uvs.log on Sun Jan 7 19:31:56 2007 obs J1832-2039_S_1997_07_02_yyk_uva.fits ! Reading UV FITS file: J1832-2039_S_1997_07_02_yyk_uva.fits ! AN table 1: 139 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.973141 visibilities/baseline/integration-bin. ! Found source: J1832-2039 ! ! 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 2.22447e+09 8e+06 1 8e+06 ! 02 2 2.23447e+09 8e+06 1 8e+06 ! 03 3 2.29447e+09 8e+06 1 8e+06 ! 04 4 2.32447e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 755 lines of history. ! ! Reading 24348 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 ![@muppet J1832-2039_S_1997_07_02_yyk] integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.04 float dynam dynam = 6.0 float amp_soltime1 amp_soltime1 = 10 float amp_soltime2 amp_soltime2 = 1 float phase_soltime1 phase_soltime1=10 float phase_soltime2 phase_soltime2=0.5 float phase_soltime phase_soltime=phase_soltime1 float ampcor_selflim ampcor_selflim=1.20 float thresh thresh = 0.10 float win_mult win_mult = 1.8 float time_av time_av = 30 float old_peak float new_peak float flux_cutoff mapsize field_size, field_cell ! Map grid = 512x512 pixels with 0.500x0.500 milli-arcsec cellsize. phase_soltime=phase_soltime1 print "uvstat(rms)=",uvstat(rms),"Jy" ! uvstat(rms)= 0.649943 Jy 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 ! Estimated beam: bmin=2.619 mas, bmaj=6.717 mas, bpa=-1.491 degrees ! Estimated noise=1808.02 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=100 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.253246 Jy ! Component: 100 - total flux cleaned = 0.420572 Jy ! Total flux subtracted in 100 components = 0.420572 Jy ! Clean residual min=-0.045251 max=0.073883 Jy/beam ! Clean residual mean=0.000742 rms=0.021782 Jy/beam ! Combined flux in latest and established models = 0.420572 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 71 model components to the UV plane model. ! The established model now contains 71 components and 0.420572 Jy ! ! Correcting IF 1. ! A total of 197 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 63 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 28 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 28 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.521415Jy sigma=0.002094 ! Fit after self-cal, rms=0.518822Jy sigma=0.002084 ! Inverting map and beam ! Estimated beam: bmin=2.619 mas, bmaj=6.717 mas, bpa=-1.491 degrees ! Estimated noise=1808.26 mJy/beam. print "************** FINISHED UNIFORM WEIGHTING CLEAN **************" ! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** ! uvw 0,-2 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -2. ! 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 ! Estimated beam: bmin=3.466 mas, bmaj=8.944 mas, bpa=-3.84 degrees ! Estimated noise=1171.1 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.27408 Jy ! Component: 100 - total flux cleaned = 0.450775 Jy ! Component: 150 - total flux cleaned = 0.57234 Jy ! Component: 200 - total flux cleaned = 0.658028 Jy ! Total flux subtracted in 200 components = 0.658028 Jy ! Clean residual min=-0.023220 max=0.036085 Jy/beam ! Clean residual mean=0.001455 rms=0.013449 Jy/beam ! Combined flux in latest and established models = 1.0786 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 140 model components to the UV plane model. ! The established model now contains 191 components and 1.0786 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.413902Jy sigma=0.001508 ! Fit after self-cal, rms=0.410547Jy sigma=0.001499 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.466 x 8.944 at -3.84 degrees (North through East) ! Clean map min=-0.021262 max=0.2546 Jy/beam if(peak(flux) < thresh*2) selflims ampcor_selflim end if gscale ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 0.766232 ! Telescope amplitude corrections in sub-array 1: ! BR 0.91 FD 1.00 HN 1.01 KP 0.87 ! LA 0.92 MK 3.53 NL 1.00* OV 1.03 ! PT 0.87 SC 1.91 ! ! ! Correcting IF 2. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 0.883615 ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 1.05 HN 1.30 KP 0.92 ! LA 1.01 MK 0.41 NL 1.00 OV 0.97 ! PT 0.87 SC 2.80 ! ! ! Correcting IF 3. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 0.998603 ! Telescope amplitude corrections in sub-array 1: ! BR 0.92 FD 0.99 HN 0.89 KP 0.90 ! LA 0.75 MK 1.12 NL 0.97 OV 0.88 ! PT 1.00 SC 1.60 ! ! ! Correcting IF 4. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 0.822612 ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 1.03 HN 1.49 KP 0.92 ! LA 0.84 MK 1.46 NL 1.07 OV 0.88 ! PT 0.86 SC 2.61 ! ! ! Fit before self-cal, rms=0.410547Jy sigma=0.001499 ! Fit after self-cal, rms=0.545958Jy sigma=0.001792 selfcal false, false, phase_soltime ! Performing phase self-cal over 10 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.545958Jy sigma=0.001792 ! Fit after self-cal, rms=0.546875Jy sigma=0.001791 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=3.676 mas, bmaj=12.01 mas, bpa=-15.74 degrees ! Estimated noise=791.626 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.14014 Jy ! Component: 100 - total flux cleaned = -0.203571 Jy ! Component: 150 - total flux cleaned = -0.240953 Jy ! Component: 200 - total flux cleaned = -0.264168 Jy ! Total flux subtracted in 200 components = -0.264168 Jy ! Clean residual min=-0.009768 max=0.009643 Jy/beam ! Clean residual mean=-0.000323 rms=0.003634 Jy/beam ! Combined flux in latest and established models = 0.814432 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 117 model components to the UV plane model. ! The established model now contains 277 components and 0.814432 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.536305Jy sigma=0.001500 ! Fit after self-cal, rms=0.534829Jy sigma=0.001498 ! Inverting map print "************** FINISHED AMPLITUDE GSCALE SELF-CAL **************" ! ************** FINISHED AMPLITUDE GSCALE SELF-CAL ************** ! phase_soltime=phase_soltime2 selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.534829Jy sigma=0.001498 ! Fit after self-cal, rms=0.533419Jy sigma=0.001491 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.0171134 Jy ! Component: 100 - total flux cleaned = -0.0209777 Jy ! Component: 150 - total flux cleaned = -0.0243853 Jy ! Component: 200 - total flux cleaned = -0.0249791 Jy ! Total flux subtracted in 200 components = -0.0249791 Jy ! Clean residual min=-0.003929 max=0.003921 Jy/beam ! Clean residual mean=-0.000110 rms=0.001611 Jy/beam ! Combined flux in latest and established models = 0.789452 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 65 model components to the UV plane model. ! The established model now contains 340 components and 0.789452 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.533268Jy sigma=0.001483 ! Fit after self-cal, rms=0.533029Jy sigma=0.001482 ! Inverting map print "*** FINISHED NATURAL WEIGHTING CLEAN with shorter phase_soltime ***" ! *** FINISHED NATURAL WEIGHTING CLEAN with shorter phase_soltime *** ! dynam = dynam - 0.25 restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.676 x 12.01 at -15.74 degrees (North through East) ! Clean map min=-0.0094229 max=0.16811 Jy/beam if(peak(flux) > thresh) selfcal true, true, amp_soltime1 selfcal false, false, phase_soltime 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 false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) selfcal true, true, amp_soltime2 selfcal false, false, phase_soltime 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 false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) print "************** FINISHED AMPLITUDE SELF-CAL **************" end if ! Performing amp+phase self-cal over 10 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.533029Jy sigma=0.001482 ! Fit after self-cal, rms=0.542824Jy sigma=0.001414 ! Performing phase self-cal over 0.5 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.542824Jy sigma=0.001414 ! Fit after self-cal, rms=0.542383Jy sigma=0.001414 ! Inverting map and beam ! Estimated beam: bmin=3.242 mas, bmaj=11.27 mas, bpa=-17.71 degrees ! Estimated noise=722.109 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000761988 Jy ! Component: 100 - total flux cleaned = 0.00172026 Jy ! Component: 150 - total flux cleaned = 0.00232793 Jy ! Component: 200 - total flux cleaned = 0.00287268 Jy ! Total flux subtracted in 200 components = 0.00287268 Jy ! Clean residual min=-0.002223 max=0.002206 Jy/beam ! Clean residual mean=0.000007 rms=0.000866 Jy/beam ! Combined flux in latest and established models = 0.792325 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 63 model components to the UV plane model. ! The established model now contains 400 components and 0.792325 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.542154Jy sigma=0.001412 ! Fit after self-cal, rms=0.541945Jy sigma=0.001412 ! Inverting map ! Performing amp+phase self-cal over 1 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.541945Jy sigma=0.001412 ! Fit after self-cal, rms=0.602870Jy sigma=0.001411 ! Performing phase self-cal over 0.5 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.602870Jy sigma=0.001411 ! Fit after self-cal, rms=0.602863Jy sigma=0.001411 ! Inverting map and beam ! Estimated beam: bmin=3.126 mas, bmaj=10.95 mas, bpa=-18.67 degrees ! Estimated noise=698.785 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00106042 Jy ! Component: 100 - total flux cleaned = 0.00249234 Jy ! Component: 150 - total flux cleaned = 0.00312885 Jy ! Component: 200 - total flux cleaned = 0.00312527 Jy ! Total flux subtracted in 200 components = 0.00312527 Jy ! Clean residual min=-0.001833 max=0.001835 Jy/beam ! Clean residual mean=0.000023 rms=0.000710 Jy/beam ! Combined flux in latest and established models = 0.79545 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 61 model components to the UV plane model. ! The established model now contains 443 components and 0.79545 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.602717Jy sigma=0.001410 ! Fit after self-cal, rms=0.602734Jy sigma=0.001410 ! Inverting map ! ************** FINISHED AMPLITUDE SELF-CAL ************** uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 20 mega-wavelengths. win_mult = win_mult * 1.4 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=8.3 mas, bmaj=17.85 mas, bpa=-4.075 degrees ! Estimated noise=918.737 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000676945 Jy ! Component: 100 - total flux cleaned = 0.00182001 Jy ! Component: 150 - total flux cleaned = 0.00297645 Jy ! Component: 200 - total flux cleaned = 0.00340644 Jy ! Total flux subtracted in 200 components = 0.00340644 Jy ! Clean residual min=-0.001292 max=0.001282 Jy/beam ! Clean residual mean=0.000019 rms=0.000578 Jy/beam ! Combined flux in latest and established models = 0.798856 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 70 model components to the UV plane model. ! The established model now contains 512 components and 0.798856 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.602661Jy sigma=0.001409 ! Fit after self-cal, rms=0.602815Jy sigma=0.001409 ! Inverting map uvtaper 0 ! No UV-taper is currently set. win_mult = win_mult / 1.4 print "************** FINISHED TAPERING SELF-CAL CLEAN **************" ! ************** FINISHED TAPERING SELF-CAL CLEAN ************** ! print "************** CLEARING MODEL AND STARTING OVER **********" ! ************** CLEARING MODEL AND STARTING OVER ********** clrmod true,true,true ! clrmod: Cleared the established, tentative and continuum 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 ! Estimated beam: bmin=2.698 mas, bmaj=7.285 mas, bpa=-8.865 degrees ! Estimated noise=1310.19 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.184146 Jy ! Component: 100 - total flux cleaned = 0.310347 Jy ! Component: 150 - total flux cleaned = 0.405935 Jy ! Component: 200 - total flux cleaned = 0.480116 Jy ! Total flux subtracted in 200 components = 0.480116 Jy ! Clean residual min=-0.021304 max=0.032729 Jy/beam ! Clean residual mean=0.000335 rms=0.009096 Jy/beam ! Combined flux in latest and established models = 0.480116 Jy uvw 0,-2 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -2. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 103 model components to the UV plane model. ! The established model now contains 103 components and 0.480116 Jy ! Inverting map and beam ! Estimated beam: bmin=3.126 mas, bmaj=10.95 mas, bpa=-18.67 degrees ! Estimated noise=698.785 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=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0936209 Jy ! Component: 100 - total flux cleaned = 0.155526 Jy ! Component: 150 - total flux cleaned = 0.198903 Jy ! Component: 200 - total flux cleaned = 0.230082 Jy ! Total flux subtracted in 200 components = 0.230082 Jy ! Clean residual min=-0.008930 max=0.013182 Jy/beam ! Clean residual mean=0.000388 rms=0.004306 Jy/beam ! Combined flux in latest and established models = 0.710197 Jy ! Adding 127 model components to the UV plane model. ! The established model now contains 204 components and 0.710197 Jy ! Inverting map uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 20 mega-wavelengths. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=8.3 mas, bmaj=17.85 mas, bpa=-4.075 degrees ! Estimated noise=918.737 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=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0378067 Jy ! Component: 100 - total flux cleaned = 0.0558869 Jy ! Component: 150 - total flux cleaned = 0.0633016 Jy ! Component: 200 - total flux cleaned = 0.0672403 Jy ! Total flux subtracted in 200 components = 0.0672403 Jy ! Clean residual min=-0.003862 max=0.003872 Jy/beam ! Clean residual mean=0.000126 rms=0.001715 Jy/beam ! Combined flux in latest and established models = 0.777438 Jy ! Adding 109 model components to the UV plane model. ! The established model now contains 291 components and 0.777438 Jy ! Inverting map uvtaper 0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=3.126 mas, bmaj=10.95 mas, bpa=-18.67 degrees ! Estimated noise=698.785 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00188237 Jy ! Component: 100 - total flux cleaned = 0.002405 Jy ! Component: 150 - total flux cleaned = 0.00284102 Jy ! Component: 200 - total flux cleaned = 0.00304557 Jy ! Total flux subtracted in 200 components = 0.00304557 Jy ! Clean residual min=-0.002552 max=0.002559 Jy/beam ! Clean residual mean=0.000039 rms=0.000978 Jy/beam ! Combined flux in latest and established models = 0.780483 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 57 model components to the UV plane model. ! The established model now contains 348 components and 0.780483 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.603340Jy sigma=0.001412 ! Fit after self-cal, rms=0.602147Jy sigma=0.001410 wmodel J1832-2039_S_1997_07_02_yyk\_map.mod ! Writing 348 model components to file: J1832-2039_S_1997_07_02_yyk_map.mod wobs J1832-2039_S_1997_07_02_yyk\_uvs.fits ! Writing UV FITS file: J1832-2039_S_1997_07_02_yyk_uvs.fits wwins J1832-2039_S_1997_07_02_yyk\_map.win ! wwins: No CLEAN windows to write. ! Error occured in command: wwins ![Exited script file: muppet] ! wmap "J1832-2039_S_1997_07_02_yyk\_map.fits" ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.126 x 10.95 at -18.67 degrees (North through East) ! Clean map min=-0.0041034 max=0.14028 Jy/beam ! Writing clean map to FITS file: J1832-2039_S_1997_07_02_yyk_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.140278 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000879847 device "J1832-2039_S_1997_07_02_yyk\_map.eps/VPS" ! Attempting to open device: 'J1832-2039_S_1997_07_02_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.88165 1.88165 3.7633 7.52661 15.0532 30.1064 60.2129 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0026 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.14 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.126 x 10.95 at -18.67 degrees (North through East) ! Clean map min=-0.0041034 max=0.14028 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1832-2039_S_1997_07_02_yyk\_map.gif/gif" ! Attempting to open device: 'J1832-2039_S_1997_07_02_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J1832-2039_S_1997_07_02_yyk_uvs.log closed on Sun Jan 7 19:32:05 2007