! Started logfile: J0116-2052_S_2002_05_14_yyk_uvs.log on Tue Jun 26 21:55:40 2007 obs J0116-2052_S_2002_05_14_yyk_uva.fits ! Reading UV FITS file: J0116-2052_S_2002_05_14_yyk_uva.fits ! AN table 1: 89 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.549064 visibilities/baseline/integration-bin. ! Found source: J0116-2052 ! ! 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 2.22947e+09 8e+06 1 8e+06 ! 02 2 2.25947e+09 8e+06 1 8e+06 ! 03 3 2.34947e+09 8e+06 1 8e+06 ! 04 4 2.36947e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 1154 lines of history. ! ! Reading 8796 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 J0116-2052_S_2002_05_14_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)= 0.515334 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=2.957 mas, bmaj=6.78 mas, bpa=4.183 degrees ! Estimated noise=2015.01 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 = 0.215678 Jy ! Component: 100 - total flux cleaned = 0.35491 Jy ! Total flux subtracted in 100 components = 0.35491 Jy ! Clean residual min=-0.049006 max=0.060559 Jy/beam ! Clean residual mean=0.004531 rms=0.022516 Jy/beam ! Combined flux in latest and established models = 0.35491 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 44 model components to the UV plane model. ! The established model now contains 44 components and 0.35491 Jy ! ! Correcting IF 1. ! A total of 296 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 303 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 306 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 296 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.412784Jy sigma=0.002648 ! Fit after self-cal, rms=0.411946Jy sigma=0.002642 ! Inverting map and beam ! Estimated beam: bmin=2.956 mas, bmaj=6.782 mas, bpa=4.172 degrees ! Estimated noise=2047.71 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=4.062 mas, bmaj=9.822 mas, bpa=5.503 degrees ! Estimated noise=1226.7 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 = 0.177701 Jy ! Component: 100 - total flux cleaned = 0.31158 Jy ! Component: 150 - total flux cleaned = 0.421315 Jy ! Component: 200 - total flux cleaned = 0.507681 Jy ! Total flux subtracted in 200 components = 0.507681 Jy ! Clean residual min=-0.042944 max=0.043713 Jy/beam ! Clean residual mean=0.005039 rms=0.022525 Jy/beam ! Combined flux in latest and established models = 0.862591 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 168 model components to the UV plane model. ! The established model now contains 205 components and 0.862591 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.334324Jy sigma=0.001998 ! Fit after self-cal, rms=0.332583Jy sigma=0.001984 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 4.062 x 9.822 at 5.503 degrees (North through East) ! Clean map min=-0.045411 max=0.21358 Jy/beam if(peak(flux) < thresh*2) selflims ampcor_selflim end if gscale ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 15 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 1.00677 ! Telescope amplitude corrections in sub-array 1: ! BR 0.90 FD 1.19 HN 0.92 KP 1.12 ! LA 0.70 NL 0.83 OV 0.89 PT 0.78 ! SC 1.61 MK 1.00* ! ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 0.996121 ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 1.10 HN 1.10 KP 1.00* ! LA 0.66 NL 1.00 OV 0.91 PT 0.78 ! SC 1.55 MK 0.96 ! ! ! Correcting IF 3. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 0.878141 ! Telescope amplitude corrections in sub-array 1: ! BR 1.16 FD 1.10 HN 2.18 KP 1.16 ! LA 0.73 NL 1.06 OV 1.07 PT 0.84 ! SC 0.94 MK 1.14 ! ! ! Correcting IF 4. ! A total of 15 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 1.08314 ! Telescope amplitude corrections in sub-array 1: ! BR 1.07 FD 0.94 HN 1.07 KP 1.28 ! LA 0.63 NL 1.07 OV 0.84 PT 0.78 ! SC 0.56 MK 1.00* ! ! ! Fit before self-cal, rms=0.332583Jy sigma=0.001984 ! Fit after self-cal, rms=0.300611Jy sigma=0.001694 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=0.300611Jy sigma=0.001694 ! Fit after self-cal, rms=0.301077Jy sigma=0.001691 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=4.413 mas, bmaj=10.49 mas, bpa=8.285 degrees ! Estimated noise=1025.31 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 = 0.0160205 Jy ! Component: 100 - total flux cleaned = 0.0259957 Jy ! Component: 150 - total flux cleaned = 0.0312487 Jy ! Component: 200 - total flux cleaned = 0.0321955 Jy ! Total flux subtracted in 200 components = 0.0321955 Jy ! Clean residual min=-0.010719 max=0.010831 Jy/beam ! Clean residual mean=-0.000496 rms=0.005265 Jy/beam ! Combined flux in latest and established models = 0.894786 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 107 model components to the UV plane model. ! The established model now contains 308 components and 0.894786 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.295349Jy sigma=0.001621 ! Fit after self-cal, rms=0.294943Jy sigma=0.001619 ! 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=0.294943Jy sigma=0.001619 ! Fit after self-cal, rms=0.292076Jy sigma=0.001593 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 = 0.00587303 Jy ! Component: 100 - total flux cleaned = 0.00662759 Jy ! Component: 150 - total flux cleaned = 0.0059555 Jy ! Component: 200 - total flux cleaned = 0.0112061 Jy ! Total flux subtracted in 200 components = 0.0112061 Jy ! Clean residual min=-0.007848 max=0.007826 Jy/beam ! Clean residual mean=-0.000439 rms=0.003994 Jy/beam ! Combined flux in latest and established models = 0.905992 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 100 model components to the UV plane model. ! The established model now contains 392 components and 0.905992 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.289294Jy sigma=0.001563 ! Fit after self-cal, rms=0.288488Jy sigma=0.001559 ! 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: 4.413 x 10.49 at 8.285 degrees (North through East) ! Clean map min=-0.020127 max=0.17787 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=0.288488Jy sigma=0.001559 ! Fit after self-cal, rms=0.319615Jy sigma=0.001498 ! 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=0.319615Jy sigma=0.001498 ! Fit after self-cal, rms=0.319454Jy sigma=0.001497 ! Inverting map and beam ! Estimated beam: bmin=3.943 mas, bmaj=9.668 mas, bpa=11.52 degrees ! Estimated noise=947.791 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00927024 Jy ! Component: 100 - total flux cleaned = 0.0148249 Jy ! Component: 150 - total flux cleaned = 0.0157761 Jy ! Component: 200 - total flux cleaned = 0.0188932 Jy ! Total flux subtracted in 200 components = 0.0188932 Jy ! Clean residual min=-0.005380 max=0.005346 Jy/beam ! Clean residual mean=-0.000144 rms=0.002757 Jy/beam ! Combined flux in latest and established models = 0.924885 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 96 model components to the UV plane model. ! The established model now contains 477 components and 0.924885 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.318154Jy sigma=0.001478 ! Fit after self-cal, rms=0.317966Jy sigma=0.001477 ! 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=0.317966Jy sigma=0.001477 ! Fit after self-cal, rms=0.367026Jy sigma=0.001472 ! 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=0.367026Jy sigma=0.001472 ! Fit after self-cal, rms=0.366976Jy sigma=0.001472 ! Inverting map and beam ! Estimated beam: bmin=3.779 mas, bmaj=9.797 mas, bpa=13.49 degrees ! Estimated noise=928.47 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00677493 Jy ! Component: 100 - total flux cleaned = 0.00928062 Jy ! Component: 150 - total flux cleaned = 0.0111313 Jy ! Component: 200 - total flux cleaned = 0.0121741 Jy ! Total flux subtracted in 200 components = 0.0121741 Jy ! Clean residual min=-0.004188 max=0.004187 Jy/beam ! Clean residual mean=-0.000080 rms=0.002167 Jy/beam ! Combined flux in latest and established models = 0.93706 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 105 model components to the UV plane model. ! The established model now contains 554 components and 0.93706 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.366342Jy sigma=0.001461 ! Fit after self-cal, rms=0.366231Jy sigma=0.001460 ! 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=8.443 mas, bmaj=20.54 mas, bpa=6.473 degrees ! Estimated noise=1110.95 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 = 0.000842321 Jy ! Component: 100 - total flux cleaned = 0.000865237 Jy ! Component: 150 - total flux cleaned = 0.00212399 Jy ! Component: 200 - total flux cleaned = 0.00250491 Jy ! Total flux subtracted in 200 components = 0.00250491 Jy ! Clean residual min=-0.004598 max=0.004547 Jy/beam ! Clean residual mean=-0.000210 rms=0.002505 Jy/beam ! Combined flux in latest and established models = 0.939564 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 107 model components to the UV plane model. ! The established model now contains 643 components and 0.939564 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.365684Jy sigma=0.001453 ! Fit after self-cal, rms=0.365616Jy sigma=0.001452 ! 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=2.908 mas, bmaj=6.836 mas, bpa=7.009 degrees ! Estimated noise=1791.19 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.173024 Jy ! Component: 100 - total flux cleaned = 0.28373 Jy ! Component: 150 - total flux cleaned = 0.372006 Jy ! Component: 200 - total flux cleaned = 0.445494 Jy ! Total flux subtracted in 200 components = 0.445494 Jy ! Clean residual min=-0.031320 max=0.033592 Jy/beam ! Clean residual mean=0.002148 rms=0.012980 Jy/beam ! Combined flux in latest and established models = 0.445494 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 96 model components to the UV plane model. ! The established model now contains 96 components and 0.445494 Jy ! Inverting map and beam ! Estimated beam: bmin=3.779 mas, bmaj=9.797 mas, bpa=13.49 degrees ! Estimated noise=928.47 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 = 0.107706 Jy ! Component: 100 - total flux cleaned = 0.187119 Jy ! Component: 150 - total flux cleaned = 0.2503 Jy ! Component: 200 - total flux cleaned = 0.301913 Jy ! Total flux subtracted in 200 components = 0.301913 Jy ! Clean residual min=-0.022995 max=0.023377 Jy/beam ! Clean residual mean=0.001826 rms=0.011375 Jy/beam ! Combined flux in latest and established models = 0.747407 Jy ! Adding 155 model components to the UV plane model. ! The established model now contains 239 components and 0.747407 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=8.443 mas, bmaj=20.54 mas, bpa=6.473 degrees ! Estimated noise=1110.95 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 = 0.0643944 Jy ! Component: 100 - total flux cleaned = 0.10218 Jy ! Component: 150 - total flux cleaned = 0.120547 Jy ! Component: 200 - total flux cleaned = 0.137561 Jy ! Total flux subtracted in 200 components = 0.137561 Jy ! Clean residual min=-0.013867 max=0.013675 Jy/beam ! Clean residual mean=0.000342 rms=0.007476 Jy/beam ! Combined flux in latest and established models = 0.884968 Jy ! Adding 133 model components to the UV plane model. ! The established model now contains 353 components and 0.884968 Jy ! Inverting map uvtaper 0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=3.779 mas, bmaj=9.797 mas, bpa=13.49 degrees ! Estimated noise=928.47 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00342322 Jy ! Component: 100 - total flux cleaned = 0.00608872 Jy ! Component: 150 - total flux cleaned = 0.00726485 Jy ! Component: 200 - total flux cleaned = 0.0100279 Jy ! Total flux subtracted in 200 components = 0.0100279 Jy ! Clean residual min=-0.006415 max=0.006447 Jy/beam ! Clean residual mean=0.000038 rms=0.003289 Jy/beam ! Combined flux in latest and established models = 0.894996 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 81 model components to the UV plane model. ! The established model now contains 432 components and 0.894996 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.367427Jy sigma=0.001478 ! Fit after self-cal, rms=0.366907Jy sigma=0.001475 wmodel J0116-2052_S_2002_05_14_yyk\_map.mod ! Writing 432 model components to file: J0116-2052_S_2002_05_14_yyk_map.mod wobs J0116-2052_S_2002_05_14_yyk\_uvs.fits ! Writing UV FITS file: J0116-2052_S_2002_05_14_yyk_uvs.fits wwins J0116-2052_S_2002_05_14_yyk\_map.win ! wwins: No CLEAN windows to write. ! Error occured in command: wwins ![Exited script file: muppet] ! wmap "J0116-2052_S_2002_05_14_yyk\_map.fits" ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.779 x 9.797 at 13.49 degrees (North through East) ! Clean map min=-0.018792 max=0.15147 Jy/beam ! Writing clean map to FITS file: J0116-2052_S_2002_05_14_yyk_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.151472 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00327793 device "J0116-2052_S_2002_05_14_yyk\_map.eps/VPS" ! Attempting to open device: 'J0116-2052_S_2002_05_14_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -6.49218 6.49218 12.9844 25.9687 51.9374 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0098 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.151 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.779 x 9.797 at 13.49 degrees (North through East) ! Clean map min=-0.018792 max=0.15147 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0116-2052_S_2002_05_14_yyk\_map.gif/gif" ! Attempting to open device: 'J0116-2052_S_2002_05_14_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J0116-2052_S_2002_05_14_yyk_uvs.log closed on Tue Jun 26 21:55:47 2007