! Started logfile: J1354-0206_S_1996_05_15_yyk_uvs.log on Sun Jan 7 18:26:35 2007 obs J1354-0206_S_1996_05_15_yyk_uva.fits ! Reading UV FITS file: J1354-0206_S_1996_05_15_yyk_uva.fits ! AN table 1: 53 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.376939 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1354-0206 ! ! 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 2.22049e+09 8e+06 1 8e+06 ! 02 2 2.23424e+09 8e+06 1 8e+06 ! 03 3 2.29424e+09 8e+06 1 8e+06 ! 04 4 2.32424e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 617 lines of history. ! ! Reading 3596 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 J1354-0206_S_1996_05_15_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)= 3.26354 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=2.669 mas, bmaj=8.708 mas, bpa=-12.7 degrees ! Estimated noise=7206.5 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 = 0.321255 Jy ! Component: 100 - total flux cleaned = 0.269809 Jy ! Total flux subtracted in 100 components = 0.269809 Jy ! Clean residual min=-0.101080 max=0.099939 Jy/beam ! Clean residual mean=-0.000311 rms=0.039774 Jy/beam ! Combined flux in latest and established models = 0.269809 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 35 model components to the UV plane model. ! The established model now contains 35 components and 0.269809 Jy ! ! Correcting IF 1. ! A total of 256 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 245 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 530 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 530 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=3.216800Jy sigma=0.004941 ! Fit after self-cal, rms=3.223737Jy sigma=0.004941 ! Inverting map and beam ! Estimated beam: bmin=2.669 mas, bmaj=8.708 mas, bpa=-12.7 degrees ! Estimated noise=7211.67 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=2.825 mas, bmaj=11.55 mas, bpa=-15.15 degrees ! Estimated noise=5299.84 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 = -0.0152661 Jy ! Component: 100 - total flux cleaned = -0.0413285 Jy ! Component: 150 - total flux cleaned = -0.0716134 Jy ! Component: 200 - total flux cleaned = -0.0952577 Jy ! Total flux subtracted in 200 components = -0.0952577 Jy ! Clean residual min=-0.043270 max=0.044639 Jy/beam ! Clean residual mean=-0.000348 rms=0.013480 Jy/beam ! Combined flux in latest and established models = 0.174551 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 39 model components to the UV plane model. ! The established model now contains 74 components and 0.174551 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=3.216204Jy sigma=0.004900 ! Fit after self-cal, rms=3.217818Jy sigma=0.004895 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 2.825 x 11.55 at -15.15 degrees (North through East) ! Clean map min=-0.066917 max=0.11743 Jy/beam if(peak(flux) < thresh*2) selflims ampcor_selflim end if ! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2. ! Selfcal phase corrections will not be limited. 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: 1 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* HN 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ! ! ! Correcting IF 2. ! Amplitude normalization factor in sub-array 1: 1 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* HN 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ! ! ! Correcting IF 3. ! Amplitude normalization factor in sub-array 1: 1 ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* HN 0.00* KP 0.00* ! LA 0.00* MK 0.00* NL 0.00* OV 0.00* ! PT 0.00* SC 0.00* ! ! ! Correcting IF 4. ! Amplitude normalization factor in sub-array 1: 1 ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* HN 0.00* KP 0.00* ! LA 0.00* MK 0.00* NL 0.00* OV 0.00* ! PT 0.00* SC 0.00* ! ! ! Fit before self-cal, rms=3.217818Jy sigma=0.004895 ! Fit after self-cal, rms=3.221360Jy sigma=0.004899 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=3.221360Jy sigma=0.004899 ! Fit after self-cal, rms=3.221160Jy sigma=0.004899 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=2.823 mas, bmaj=11.54 mas, bpa=-15.15 degrees ! Estimated noise=5304.16 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 = -0.0161972 Jy ! Component: 100 - total flux cleaned = -0.02 Jy ! Component: 150 - total flux cleaned = -0.0167468 Jy ! Component: 200 - total flux cleaned = -0.0149297 Jy ! Total flux subtracted in 200 components = -0.0149297 Jy ! Clean residual min=-0.020224 max=0.020612 Jy/beam ! Clean residual mean=0.000037 rms=0.006746 Jy/beam ! Combined flux in latest and established models = 0.159621 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 42 model components to the UV plane model. ! The established model now contains 115 components and 0.159621 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=3.218570Jy sigma=0.004888 ! Fit after self-cal, rms=3.217751Jy sigma=0.004888 ! 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=3.217751Jy sigma=0.004888 ! Fit after self-cal, rms=3.217484Jy sigma=0.004878 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 = 0.0288556 Jy ! Component: 100 - total flux cleaned = 0.0233448 Jy ! Component: 150 - total flux cleaned = 0.0175256 Jy ! Component: 200 - total flux cleaned = 0.0140828 Jy ! Total flux subtracted in 200 components = 0.0140828 Jy ! Clean residual min=-0.010518 max=0.010763 Jy/beam ! Clean residual mean=-0.000071 rms=0.004001 Jy/beam ! Combined flux in latest and established models = 0.173704 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 48 model components to the UV plane model. ! The established model now contains 161 components and 0.173704 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=3.215523Jy sigma=0.004872 ! Fit after self-cal, rms=3.214206Jy sigma=0.004866 ! 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: 2.823 x 11.54 at -15.15 degrees (North through East) ! Clean map min=-0.056567 max=0.11641 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=3.214206Jy sigma=0.004866 ! Fit after self-cal, rms=3.214206Jy sigma=0.004866 ! 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=3.214206Jy sigma=0.004866 ! Fit after self-cal, rms=3.213586Jy sigma=0.004868 ! Inverting map and beam ! Estimated beam: bmin=2.823 mas, bmaj=11.54 mas, bpa=-15.15 degrees ! Estimated noise=5304.16 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000119537 Jy ! Component: 100 - total flux cleaned = -0.00209579 Jy ! Component: 150 - total flux cleaned = -0.00473434 Jy ! Component: 200 - total flux cleaned = -0.00459515 Jy ! Total flux subtracted in 200 components = -0.00459515 Jy ! Clean residual min=-0.008326 max=0.008304 Jy/beam ! Clean residual mean=-0.000064 rms=0.002906 Jy/beam ! Combined flux in latest and established models = 0.169109 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 40 model components to the UV plane model. ! The established model now contains 197 components and 0.169109 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=3.212594Jy sigma=0.004866 ! Fit after self-cal, rms=3.213848Jy sigma=0.004865 ! 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=3.213848Jy sigma=0.004865 ! Fit after self-cal, rms=3.213848Jy sigma=0.004865 ! 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=3.213848Jy sigma=0.004865 ! Fit after self-cal, rms=3.213718Jy sigma=0.004865 ! Inverting map and beam ! Estimated beam: bmin=2.823 mas, bmaj=11.54 mas, bpa=-15.15 degrees ! Estimated noise=5304.16 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.001581 Jy ! Component: 100 - total flux cleaned = 0.00406304 Jy ! Component: 150 - total flux cleaned = 0.00702218 Jy ! Component: 200 - total flux cleaned = 0.0104809 Jy ! Total flux subtracted in 200 components = 0.0104809 Jy ! Clean residual min=-0.007229 max=0.007223 Jy/beam ! Clean residual mean=-0.000124 rms=0.002546 Jy/beam ! Combined flux in latest and established models = 0.17959 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 54 model components to the UV plane model. ! The established model now contains 250 components and 0.17959 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=3.212433Jy sigma=0.004864 ! Fit after self-cal, rms=3.213604Jy sigma=0.004864 ! 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=7.129 mas, bmaj=19.63 mas, bpa=-10.88 degrees ! Estimated noise=6953.32 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 = -0.00250959 Jy ! Component: 100 - total flux cleaned = -0.00164432 Jy ! Component: 150 - total flux cleaned = -0.00133188 Jy ! Component: 200 - total flux cleaned = -0.0023557 Jy ! Total flux subtracted in 200 components = -0.0023557 Jy ! Clean residual min=-0.016706 max=0.016605 Jy/beam ! Clean residual mean=0.000215 rms=0.004594 Jy/beam ! Combined flux in latest and established models = 0.177234 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 35 model components to the UV plane model. ! The established model now contains 283 components and 0.177234 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=3.212407Jy sigma=0.004863 ! Fit after self-cal, rms=3.212808Jy sigma=0.004863 ! 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=2.67 mas, bmaj=8.71 mas, bpa=-12.7 degrees ! Estimated noise=7210.3 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.145182 Jy ! Component: 100 - total flux cleaned = -0.0822753 Jy ! Component: 150 - total flux cleaned = -0.210882 Jy ! Component: 200 - total flux cleaned = -0.289574 Jy ! Total flux subtracted in 200 components = -0.289574 Jy ! Clean residual min=-0.126931 max=0.127058 Jy/beam ! Clean residual mean=-0.001243 rms=0.038252 Jy/beam ! Combined flux in latest and established models = -0.289574 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 45 model components to the UV plane model. ! The established model now contains 45 components and -0.289574 Jy ! Inverting map and beam ! Estimated beam: bmin=2.823 mas, bmaj=11.54 mas, bpa=-15.15 degrees ! Estimated noise=5304.16 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 = 0.0758945 Jy ! Component: 100 - total flux cleaned = 0.0791165 Jy ! Component: 150 - total flux cleaned = 0.0740195 Jy ! Component: 200 - total flux cleaned = 0.0837187 Jy ! Total flux subtracted in 200 components = 0.0837187 Jy ! Clean residual min=-0.029741 max=0.030627 Jy/beam ! Clean residual mean=0.000402 rms=0.010293 Jy/beam ! Combined flux in latest and established models = -0.205855 Jy ! Adding 41 model components to the UV plane model. ! The established model now contains 86 components and -0.205855 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=7.129 mas, bmaj=19.63 mas, bpa=-10.88 degrees ! Estimated noise=6953.32 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 = 0.00264824 Jy ! Component: 100 - total flux cleaned = 0.00145531 Jy ! Component: 150 - total flux cleaned = 0.00152907 Jy ! Component: 200 - total flux cleaned = 0.00393657 Jy ! Total flux subtracted in 200 components = 0.00393657 Jy ! Clean residual min=-0.015440 max=0.015245 Jy/beam ! Clean residual mean=0.000220 rms=0.004863 Jy/beam ! Combined flux in latest and established models = -0.201919 Jy ! Adding 48 model components to the UV plane model. ! The established model now contains 133 components and -0.201918 Jy ! Inverting map uvtaper 0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=2.823 mas, bmaj=11.54 mas, bpa=-15.15 degrees ! Estimated noise=5304.16 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00727146 Jy ! Component: 100 - total flux cleaned = 0.0126904 Jy ! Component: 150 - total flux cleaned = 0.0136579 Jy ! Component: 200 - total flux cleaned = 0.0178637 Jy ! Total flux subtracted in 200 components = 0.0178637 Jy ! Clean residual min=-0.013626 max=0.013344 Jy/beam ! Clean residual mean=0.000057 rms=0.004436 Jy/beam ! Combined flux in latest and established models = -0.184055 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 38 model components to the UV plane model. ! The established model now contains 166 components and -0.184055 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=3.208121Jy sigma=0.004865 ! Fit after self-cal, rms=3.202265Jy sigma=0.004864 wmodel J1354-0206_S_1996_05_15_yyk\_map.mod ! Writing 166 model components to file: J1354-0206_S_1996_05_15_yyk_map.mod wobs J1354-0206_S_1996_05_15_yyk\_uvs.fits ! Writing UV FITS file: J1354-0206_S_1996_05_15_yyk_uvs.fits wwins J1354-0206_S_1996_05_15_yyk\_map.win ! wwins: No CLEAN windows to write. ! Error occured in command: wwins ![Exited script file: muppet] ! wmap "J1354-0206_S_1996_05_15_yyk\_map.fits" ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 2.823 x 11.54 at -15.15 degrees (North through East) ! Clean map min=-0.21856 max=0.073691 Jy/beam ! Writing clean map to FITS file: J1354-0206_S_1996_05_15_yyk_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0736909 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00444291 device "J1354-0206_S_1996_05_15_yyk\_map.eps/VPS" ! Attempting to open device: 'J1354-0206_S_1996_05_15_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -18.0873 18.0873 36.1747 72.3494 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0133 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.073 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 2.823 x 11.54 at -15.15 degrees (North through East) ! Clean map min=-0.21856 max=0.073691 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1354-0206_S_1996_05_15_yyk\_map.gif/gif" ! Attempting to open device: 'J1354-0206_S_1996_05_15_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J1354-0206_S_1996_05_15_yyk_uvs.log closed on Sun Jan 7 18:26:39 2007