! Started logfile: J0003-1149_X_2004_05_08_yyk_uvs.log on Wed Dec 7 01:08:00 2005 obs J0003-1149_X_2004_05_08_yyk_uve.fits ! Reading UV FITS file: J0003-1149_X_2004_05_08_yyk_uve.fits ! AN table 1: 10 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.433333 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0003-1149 ! ! 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 1434 lines of history. ! ! Reading 780 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 J0003-1149_X_2004_05_08_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 = 256x256 pixels with 0.800x0.800 milli-arcsec cellsize. phase_soltime=phase_soltime1 print "uvstat(rms)=",uvstat(rms),"Jy" ! uvstat(rms)= 0.620117 Jy startmod ,phase_soltime ! Applying default point source starting model. ! Performing phase self-cal over 10 minute time intervals ! 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 54 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 53 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 53 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 53 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.413300Jy sigma=7.100203 ! Fit after self-cal, rms=0.411232Jy sigma=7.071846 ! 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 ! Estimated beam: bmin=3.172 mas, bmaj=13.7 mas, bpa=17.9 degrees ! Estimated noise=2.55044 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 = 0.518196 Jy ! Component: 100 - total flux cleaned = 0.589156 Jy ! Total flux subtracted in 100 components = 0.589156 Jy ! Clean residual min=-0.020594 max=0.020885 Jy/beam ! Clean residual mean=0.000046 rms=0.007854 Jy/beam ! Combined flux in latest and established models = 0.589156 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 15 model components to the UV plane model. ! The established model now contains 15 components and 0.589156 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.120669Jy sigma=1.781053 ! Fit after self-cal, rms=0.120464Jy sigma=1.774053 ! Inverting map 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=3.458 mas, bmaj=12.82 mas, bpa=19.15 degrees ! Estimated noise=2.23098 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 = 0.0244757 Jy ! Component: 100 - total flux cleaned = 0.0402058 Jy ! Component: 150 - total flux cleaned = 0.047786 Jy ! Component: 200 - total flux cleaned = 0.0541627 Jy ! Total flux subtracted in 200 components = 0.0541627 Jy ! Clean residual min=-0.010205 max=0.010188 Jy/beam ! Clean residual mean=0.000125 rms=0.003518 Jy/beam ! Combined flux in latest and established models = 0.643318 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 37 model components to the UV plane model. ! The established model now contains 49 components and 0.643319 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.109153Jy sigma=1.567153 ! Fit after self-cal, rms=0.108878Jy sigma=1.559780 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! selflims ampcor_selflim ! 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 6 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 1.00066 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.02 HN 1.00* KP 1.02 ! LA 0.98 MK 1.00* NL 1.00* OV 1.03 ! PT 0.94 SC 1.00* ! ! ! Correcting IF 2. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 1.00772 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00 HN 1.00* KP 0.96 ! LA 0.97 MK 1.00* NL 1.00* OV 0.99 ! PT 1.00 SC 1.00* ! ! ! Correcting IF 3. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 1.00078 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.04 HN 1.00* KP 0.95 ! LA 1.03 MK 1.00* NL 1.00* OV 0.98 ! PT 1.01 SC 1.00* ! ! ! Correcting IF 4. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 1.00142 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.98 HN 1.00* KP 0.99 ! LA 0.99 MK 1.00* NL 1.00* OV 0.98 ! PT 1.05 SC 1.00* ! ! ! Fit before self-cal, rms=0.108878Jy sigma=1.559780 ! Fit after self-cal, rms=0.105914Jy sigma=1.529104 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=0.105914Jy sigma=1.529104 ! Fit after self-cal, rms=0.105545Jy sigma=1.521939 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=3.476 mas, bmaj=12.66 mas, bpa=18.89 degrees ! Estimated noise=2.26907 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 = -0.00763977 Jy ! Component: 100 - total flux cleaned = -0.0106965 Jy ! Component: 150 - total flux cleaned = -0.012231 Jy ! Component: 200 - total flux cleaned = -0.0144238 Jy ! Total flux subtracted in 200 components = -0.0144238 Jy ! Clean residual min=-0.002525 max=0.002447 Jy/beam ! Clean residual mean=-0.000003 rms=0.000858 Jy/beam ! Combined flux in latest and established models = 0.628895 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 38 model components to the UV plane model. ! The established model now contains 86 components and 0.628895 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.104441Jy sigma=1.501248 ! Fit after self-cal, rms=0.104056Jy sigma=1.494583 ! 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=0.104056Jy sigma=1.494583 ! Fit after self-cal, rms=0.065257Jy sigma=0.910426 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 = -0.000315236 Jy ! Component: 100 - total flux cleaned = 0.00127791 Jy ! Component: 150 - total flux cleaned = 0.0024739 Jy ! Component: 200 - total flux cleaned = 0.00365769 Jy ! Total flux subtracted in 200 components = 0.00365769 Jy ! Clean residual min=-0.003009 max=0.002983 Jy/beam ! Clean residual mean=0.000003 rms=0.000980 Jy/beam ! Combined flux in latest and established models = 0.632552 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 20 model components to the UV plane model. ! The established model now contains 104 components and 0.632552 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.063984Jy sigma=0.892789 ! Fit after self-cal, rms=0.062979Jy sigma=0.876466 ! 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: 3.476 x 12.66 at 18.89 degrees (North through East) ! Clean map min=-0.01563 max=0.55504 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=0.062979Jy sigma=0.876466 ! Fit after self-cal, rms=0.061848Jy sigma=0.866981 ! 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=0.061848Jy sigma=0.866981 ! Fit after self-cal, rms=0.061800Jy sigma=0.865954 ! Inverting map and beam ! Estimated beam: bmin=3.472 mas, bmaj=12.64 mas, bpa=18.91 degrees ! Estimated noise=2.2639 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.000345699 Jy ! Component: 100 - total flux cleaned = -0.00072999 Jy ! Component: 150 - total flux cleaned = -0.00123373 Jy ! Component: 200 - total flux cleaned = -0.00191027 Jy ! Total flux subtracted in 200 components = -0.00191027 Jy ! Clean residual min=-0.000822 max=0.000818 Jy/beam ! Clean residual mean=0.000001 rms=0.000268 Jy/beam ! Combined flux in latest and established models = 0.630642 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 34 model components to the UV plane model. ! The established model now contains 137 components and 0.630642 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.061733Jy sigma=0.863139 ! Fit after self-cal, rms=0.061695Jy sigma=0.862957 ! 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=0.061695Jy sigma=0.862957 ! Fit after self-cal, rms=0.059270Jy sigma=0.810449 ! 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=0.059270Jy sigma=0.810449 ! Fit after self-cal, rms=0.059269Jy sigma=0.810421 ! Inverting map and beam ! Estimated beam: bmin=3.472 mas, bmaj=12.64 mas, bpa=18.9 degrees ! Estimated noise=2.26264 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000369708 Jy ! Component: 100 - total flux cleaned = 0.000158507 Jy ! Component: 150 - total flux cleaned = 0.000298393 Jy ! Component: 200 - total flux cleaned = 0.000527762 Jy ! Total flux subtracted in 200 components = 0.000527762 Jy ! Clean residual min=-0.000569 max=0.000567 Jy/beam ! Clean residual mean=0.000001 rms=0.000203 Jy/beam ! Combined flux in latest and established models = 0.63117 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 36 model components to the UV plane model. ! The established model now contains 173 components and 0.63117 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.059168Jy sigma=0.809230 ! Fit after self-cal, rms=0.059157Jy sigma=0.809193 ! Inverting map ! ************** FINISHED AMPLITUDE SELF-CAL ************** uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. win_mult = win_mult * 1.4 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=3.706 mas, bmaj=12.41 mas, bpa=18.88 degrees ! Estimated noise=2.27573 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 = -0.000432597 Jy ! Component: 100 - total flux cleaned = -0.000713185 Jy ! Component: 150 - total flux cleaned = -0.00080742 Jy ! Component: 200 - total flux cleaned = -0.000747819 Jy ! Total flux subtracted in 200 components = -0.000747819 Jy ! Clean residual min=-0.000756 max=0.000748 Jy/beam ! Clean residual mean=-0.000008 rms=0.000238 Jy/beam ! Combined flux in latest and established models = 0.630422 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 27 model components to the UV plane model. ! The established model now contains 194 components and 0.630422 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.059114Jy sigma=0.808382 ! Fit after self-cal, rms=0.059115Jy sigma=0.808289 ! Inverting map uvtaper 0,0 ! 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=3.154 mas, bmaj=13.66 mas, bpa=17.98 degrees ! Estimated noise=2.58865 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.520499 Jy ! Component: 100 - total flux cleaned = 0.597132 Jy ! Component: 150 - total flux cleaned = 0.609711 Jy ! Component: 200 - total flux cleaned = 0.61404 Jy ! Total flux subtracted in 200 components = 0.61404 Jy ! Clean residual min=-0.008758 max=0.008951 Jy/beam ! Clean residual mean=0.000025 rms=0.003608 Jy/beam ! Combined flux in latest and established models = 0.61404 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 39 model components to the UV plane model. ! The established model now contains 39 components and 0.61404 Jy ! Inverting map and beam ! Estimated beam: bmin=3.472 mas, bmaj=12.64 mas, bpa=18.9 degrees ! Estimated noise=2.26264 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 = 0.00801188 Jy ! Component: 100 - total flux cleaned = 0.0149065 Jy ! Component: 150 - total flux cleaned = 0.0181283 Jy ! Component: 200 - total flux cleaned = 0.0213665 Jy ! Total flux subtracted in 200 components = 0.0213665 Jy ! Clean residual min=-0.005116 max=0.005216 Jy/beam ! Clean residual mean=0.000045 rms=0.001738 Jy/beam ! Combined flux in latest and established models = 0.635407 Jy ! Adding 39 model components to the UV plane model. ! The established model now contains 74 components and 0.635407 Jy ! Inverting map uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=3.706 mas, bmaj=12.41 mas, bpa=18.88 degrees ! Estimated noise=2.27573 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 = -0.0020044 Jy ! Component: 100 - total flux cleaned = -0.000995148 Jy ! Component: 150 - total flux cleaned = 1.29192e-07 Jy ! Component: 200 - total flux cleaned = -0.000255033 Jy ! Total flux subtracted in 200 components = -0.000255033 Jy ! Clean residual min=-0.001558 max=0.001536 Jy/beam ! Clean residual mean=0.000001 rms=0.000610 Jy/beam ! Combined flux in latest and established models = 0.635152 Jy ! Adding 48 model components to the UV plane model. ! The established model now contains 119 components and 0.635152 Jy ! Inverting map uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=3.472 mas, bmaj=12.64 mas, bpa=18.9 degrees ! Estimated noise=2.26264 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000275306 Jy ! Component: 100 - total flux cleaned = 0.00104894 Jy ! Component: 150 - total flux cleaned = 0.00147461 Jy ! Component: 200 - total flux cleaned = 0.00162419 Jy ! Total flux subtracted in 200 components = 0.00162419 Jy ! Clean residual min=-0.000881 max=0.000876 Jy/beam ! Clean residual mean=-0.000003 rms=0.000324 Jy/beam ! Combined flux in latest and established models = 0.636776 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 40 model components to the UV plane model. ! The established model now contains 150 components and 0.636776 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.059164Jy sigma=0.810852 ! Fit after self-cal, rms=0.059131Jy sigma=0.810277 wmodel J0003-1149_X_2004_05_08_yyk\_map.mod ! Writing 150 model components to file: J0003-1149_X_2004_05_08_yyk_map.mod wobs J0003-1149_X_2004_05_08_yyk\_uvs.fits ! Writing UV FITS file: J0003-1149_X_2004_05_08_yyk_uvs.fits wwins J0003-1149_X_2004_05_08_yyk\_map.win ! wwins: No CLEAN windows to write. ! Error occured in command: wwins ![Exited script file: muppet] ! wmap "J0003-1149_X_2004_05_08_yyk\_map.fits" ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.472 x 12.64 at 18.9 degrees (North through East) ! Clean map min=-0.011434 max=0.55634 Jy/beam ! Writing clean map to FITS file: J0003-1149_X_2004_05_08_yyk_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.556337 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000280695 device "J0003-1149_X_2004_05_08_yyk\_map.eps/VPS" ! Attempting to open device: 'J0003-1149_X_2004_05_08_yyk_map.eps/VPS' loglevs 8*100*3*image_rms/peak_flux ! The new contour levels are: ! -1.2109 1.2109 2.4218 4.8436 9.6872 19.3744 38.7488 77.4976 print "clev=",int(8*3*image_rms*10000)/10000 ! clev= 0.0067 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.556 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.472 x 12.64 at 18.9 degrees (North through East) ! Clean map min=-0.011434 max=0.55634 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0003-1149_X_2004_05_08_yyk\_map.gif/gif" ! Attempting to open device: 'J0003-1149_X_2004_05_08_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J0003-1149_X_2004_05_08_yyk_uvs.log closed on Wed Dec 7 01:08:01 2005