! Started logfile: J1913-3630_X_2005_06_30_yyk_uvs.log on Sat Oct 8 17:38:34 2005 obs J1913-3630_X_2005_06_30_yyk_uve.fits ! Reading UV FITS file: J1913-3630_X_2005_06_30_yyk_uve.fits ! AN table 1: 15 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.325926 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1913-3630 ! ! 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 1460 lines of history. ! ! Reading 880 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 J1913-3630_X_2005_06_30_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 0.200x0.200 milli-arcsec cellsize. phase_soltime=phase_soltime1 print "uvstat(rms)=",uvstat(rms),"Jy" ! uvstat(rms)= 0.0953758 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=0.6614 mas, bmaj=1.969 mas, bpa=9.585 degrees ! Estimated noise=3.6972 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) ! Added new window around map position (0, 0). ! clean: niter=100 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0572658 Jy ! Component: 100 - total flux cleaned = 0.066886 Jy ! Total flux subtracted in 100 components = 0.066886 Jy ! Clean residual min=-0.013685 max=0.014337 Jy/beam ! Clean residual mean=-0.000021 rms=0.003960 Jy/beam ! Combined flux in latest and established models = 0.066886 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 11 model components to the UV plane model. ! The established model now contains 11 components and 0.066886 Jy ! ! Correcting IF 1. ! A total of 80 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 96 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 98 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 106 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.068788Jy sigma=1.141211 ! Fit after self-cal, rms=0.068336Jy sigma=1.135429 ! Inverting map and beam ! Estimated beam: bmin=0.6616 mas, bmaj=1.969 mas, bpa=9.585 degrees ! Estimated noise=3.6955 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=0.979 mas, bmaj=2.935 mas, bpa=9.602 degrees ! Estimated noise=1.68083 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 = 0.00129861 Jy ! Component: 100 - total flux cleaned = 0.00124114 Jy ! Component: 150 - total flux cleaned = 0.00128826 Jy ! Component: 200 - total flux cleaned = 0.00128453 Jy ! Total flux subtracted in 200 components = 0.00128453 Jy ! Clean residual min=-0.005359 max=0.006044 Jy/beam ! Clean residual mean=-0.000069 rms=0.001829 Jy/beam ! Combined flux in latest and established models = 0.0681705 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 13 model components to the UV plane model. ! The established model now contains 22 components and 0.0681705 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.068282Jy sigma=1.133708 ! Fit after self-cal, rms=0.068276Jy sigma=1.133681 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.979 x 2.935 at 9.602 degrees (North through East) ! Clean map min=-0.0049721 max=0.06484 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. ! 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 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 4. ! 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* ! ! ! Fit before self-cal, rms=0.068276Jy sigma=1.133681 ! Fit after self-cal, rms=0.068276Jy sigma=1.133681 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=0.068276Jy sigma=1.133681 ! Fit after self-cal, rms=0.068276Jy sigma=1.133681 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.979 mas, bmaj=2.935 mas, bpa=9.602 degrees ! Estimated noise=1.68083 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 = -4.76031e-05 Jy ! Component: 100 - total flux cleaned = -1.65587e-05 Jy ! Component: 150 - total flux cleaned = -1.57112e-05 Jy ! Component: 200 - total flux cleaned = 1.23747e-05 Jy ! Total flux subtracted in 200 components = 1.23747e-05 Jy ! Clean residual min=-0.005336 max=0.005952 Jy/beam ! Clean residual mean=-0.000069 rms=0.001823 Jy/beam ! Combined flux in latest and established models = 0.0681829 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 29 components and 0.0681829 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.068260Jy sigma=1.133338 ! Fit after self-cal, rms=0.068257Jy sigma=1.133323 ! 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=0.068257Jy sigma=1.133323 ! Fit after self-cal, rms=0.059800Jy sigma=0.981135 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 = 0.00643492 Jy ! Component: 100 - total flux cleaned = 0.0066044 Jy ! Component: 150 - total flux cleaned = 0.00665193 Jy ! Component: 200 - total flux cleaned = 0.00668476 Jy ! Total flux subtracted in 200 components = 0.00668476 Jy ! Clean residual min=-0.004791 max=0.006294 Jy/beam ! Clean residual mean=-0.000038 rms=0.001633 Jy/beam ! Combined flux in latest and established models = 0.0748677 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 9 model components to the UV plane model. ! The established model now contains 32 components and 0.0748677 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.059347Jy sigma=0.971380 ! Fit after self-cal, rms=0.058257Jy sigma=0.962588 ! 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: 0.979 x 2.935 at 9.602 degrees (North through East) ! Clean map min=-0.0045774 max=0.070949 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 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=3.35 mas, bmaj=13.87 mas, bpa=6.128 degrees ! Estimated noise=1.99829 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 = 0.000844002 Jy ! Component: 100 - total flux cleaned = 0.000884097 Jy ! Component: 150 - total flux cleaned = 0.000903549 Jy ! Component: 200 - total flux cleaned = 0.000923607 Jy ! Total flux subtracted in 200 components = 0.000923607 Jy ! Clean residual min=-0.003905 max=0.006759 Jy/beam ! Clean residual mean=-0.000067 rms=0.001835 Jy/beam ! Combined flux in latest and established models = 0.0757913 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 3 model components to the UV plane model. ! The established model now contains 34 components and 0.0757913 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.058266Jy sigma=0.962586 ! Fit after self-cal, rms=0.057834Jy sigma=0.961129 ! 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=0.6616 mas, bmaj=1.969 mas, bpa=9.585 degrees ! Estimated noise=3.6955 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0665227 Jy ! Component: 100 - total flux cleaned = 0.0769662 Jy ! Component: 150 - total flux cleaned = 0.07737 Jy ! Component: 200 - total flux cleaned = 0.0775242 Jy ! Total flux subtracted in 200 components = 0.0775242 Jy ! Clean residual min=-0.008209 max=0.008088 Jy/beam ! Clean residual mean=-0.000004 rms=0.002455 Jy/beam ! Combined flux in latest and established models = 0.0775242 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 13 model components to the UV plane model. ! The established model now contains 13 components and 0.0775242 Jy ! Inverting map and beam ! Estimated beam: bmin=0.979 mas, bmaj=2.935 mas, bpa=9.602 degrees ! Estimated noise=1.68083 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 = -0.00215501 Jy ! Component: 100 - total flux cleaned = -0.00221336 Jy ! Component: 150 - total flux cleaned = -0.00224104 Jy ! Component: 200 - total flux cleaned = -0.00224576 Jy ! Total flux subtracted in 200 components = -0.00224576 Jy ! Clean residual min=-0.004595 max=0.006234 Jy/beam ! Clean residual mean=-0.000047 rms=0.001579 Jy/beam ! Combined flux in latest and established models = 0.0752784 Jy ! Adding 10 model components to the UV plane model. ! The established model now contains 23 components and 0.0752784 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=3.35 mas, bmaj=13.87 mas, bpa=6.128 degrees ! Estimated noise=1.99829 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 = 0.000425808 Jy ! Component: 100 - total flux cleaned = 0.000447004 Jy ! Component: 150 - total flux cleaned = 0.000466746 Jy ! Component: 200 - total flux cleaned = 0.000487263 Jy ! Total flux subtracted in 200 components = 0.000487263 Jy ! Clean residual min=-0.003956 max=0.006694 Jy/beam ! Clean residual mean=-0.000072 rms=0.001827 Jy/beam ! Combined flux in latest and established models = 0.0757657 Jy ! Adding 4 model components to the UV plane model. ! The established model now contains 27 components and 0.0757657 Jy ! Inverting map uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=0.979 mas, bmaj=2.935 mas, bpa=9.602 degrees ! Estimated noise=1.68083 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.000342882 Jy ! Component: 100 - total flux cleaned = -0.000380496 Jy ! Component: 150 - total flux cleaned = -0.000398236 Jy ! Component: 200 - total flux cleaned = -0.000398433 Jy ! Total flux subtracted in 200 components = -0.000398433 Jy ! Clean residual min=-0.004531 max=0.006223 Jy/beam ! Clean residual mean=-0.000046 rms=0.001569 Jy/beam ! Combined flux in latest and established models = 0.0753673 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 12 model components to the UV plane model. ! The established model now contains 36 components and 0.0753673 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.057810Jy sigma=0.960728 ! Fit after self-cal, rms=0.057590Jy sigma=0.960160 wmodel J1913-3630_X_2005_06_30_yyk\_map.mod ! Writing 36 model components to file: J1913-3630_X_2005_06_30_yyk_map.mod wobs J1913-3630_X_2005_06_30_yyk\_uvs.fits ! Writing UV FITS file: J1913-3630_X_2005_06_30_yyk_uvs.fits wwins J1913-3630_X_2005_06_30_yyk\_map.win ! wwins: Wrote 1 windows to J1913-3630_X_2005_06_30_yyk_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.00253201 Jy ! Component: 100 - total flux cleaned = 0.00319472 Jy ! Component: 150 - total flux cleaned = 0.00272256 Jy ! Component: 200 - total flux cleaned = 0.00240632 Jy ! Component: 250 - total flux cleaned = 0.00222703 Jy ! Component: 300 - total flux cleaned = 0.00200317 Jy ! Component: 350 - total flux cleaned = 0.00195026 Jy ! Component: 400 - total flux cleaned = 0.00184901 Jy ! Component: 450 - total flux cleaned = 0.00160751 Jy ! Component: 500 - total flux cleaned = 0.00123338 Jy ! Component: 550 - total flux cleaned = 0.00109697 Jy ! Component: 600 - total flux cleaned = 0.000829506 Jy ! Component: 650 - total flux cleaned = 0.00065621 Jy ! Component: 700 - total flux cleaned = 0.000486879 Jy ! Component: 750 - total flux cleaned = 0.000362905 Jy ! Component: 800 - total flux cleaned = 0.000160493 Jy ! Component: 850 - total flux cleaned = -3.74614e-05 Jy ! Component: 900 - total flux cleaned = -0.000231874 Jy ! Component: 950 - total flux cleaned = -0.000460838 Jy ! Component: 1000 - total flux cleaned = -0.000610417 Jy ! Component: 1050 - total flux cleaned = -0.000793904 Jy ! Component: 1100 - total flux cleaned = -0.000973849 Jy ! Component: 1150 - total flux cleaned = -0.00108005 Jy ! Component: 1200 - total flux cleaned = -0.00121966 Jy ! Component: 1250 - total flux cleaned = -0.00135729 Jy ! Component: 1300 - total flux cleaned = -0.00156082 Jy ! Component: 1350 - total flux cleaned = -0.00162785 Jy ! Component: 1400 - total flux cleaned = -0.00176067 Jy ! Component: 1450 - total flux cleaned = -0.00182666 Jy ! Component: 1500 - total flux cleaned = -0.00208728 Jy ! Component: 1550 - total flux cleaned = -0.00218412 Jy ! Component: 1600 - total flux cleaned = -0.00234442 Jy ! Component: 1650 - total flux cleaned = -0.0025039 Jy ! Component: 1700 - total flux cleaned = -0.0026626 Jy ! Component: 1750 - total flux cleaned = -0.00282117 Jy ! Component: 1800 - total flux cleaned = -0.00294815 Jy ! Component: 1850 - total flux cleaned = -0.00304366 Jy ! Component: 1900 - total flux cleaned = -0.00313979 Jy ! Component: 1950 - total flux cleaned = -0.00323604 Jy ! Component: 2000 - total flux cleaned = -0.00330103 Jy ! Total flux subtracted in 2048 components = -0.00343224 Jy ! Clean residual min=-0.001832 max=0.001939 Jy/beam ! Clean residual mean=-0.000012 rms=0.000586 Jy/beam ! Combined flux in latest and established models = 0.071935 Jy keep ! Adding 102 model components to the UV plane model. ! The established model now contains 138 components and 0.071935 Jy ![Exited script file: muppet] wmap "J1913-3630_X_2005_06_30_yyk\_map.fits" ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.979 x 2.935 at 9.602 degrees (North through East) ! Clean map min=-0.0048549 max=0.072256 Jy/beam ! Writing clean map to FITS file: J1913-3630_X_2005_06_30_yyk_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0722563 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00054 device "J1913-3630_X_2005_06_30_yyk\_map.eps/VPS" ! Attempting to open device: 'J1913-3630_X_2005_06_30_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -2.24202 2.24202 4.48404 8.96808 17.9362 35.8723 71.7446 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0016 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.072 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.979 x 2.935 at 9.602 degrees (North through East) ! Clean map min=-0.0048549 max=0.072256 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1913-3630_X_2005_06_30_yyk\_map.gif/gif" ! Attempting to open device: 'J1913-3630_X_2005_06_30_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J1913-3630_X_2005_06_30_yyk_uvs.log closed on Sat Oct 8 17:38:38 2005