! Started logfile: J0320-3837_S_2002_05_14_yyk_uvs.log on Tue Jun 26 22:06:21 2007 obs J0320-3837_S_2002_05_14_yyk_uva.fits ! Reading UV FITS file: J0320-3837_S_2002_05_14_yyk_uva.fits ! AN table 1: 39 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.446724 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0320-3837 ! ! 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 1153 lines of history. ! ! Reading 3136 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 J0320-3837_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)= 0.301558 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=2.877 mas, bmaj=24.56 mas, bpa=26.84 degrees ! Estimated noise=3384.53 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 = 0.0924903 Jy ! Component: 100 - total flux cleaned = 0.0932456 Jy ! Total flux subtracted in 100 components = 0.0932456 Jy ! Clean residual min=-0.013809 max=0.013764 Jy/beam ! Clean residual mean=0.000650 rms=0.005657 Jy/beam ! Combined flux in latest and established models = 0.0932456 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 27 model components to the UV plane model. ! The established model now contains 27 components and 0.0932456 Jy ! ! Correcting IF 1. ! A total of 127 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 127 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 140 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 127 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.278659Jy sigma=0.001279 ! Fit after self-cal, rms=0.278227Jy sigma=0.001276 ! Inverting map and beam ! Estimated beam: bmin=2.877 mas, bmaj=24.56 mas, bpa=26.84 degrees ! Estimated noise=3388.28 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=3.682 mas, bmaj=28.8 mas, bpa=26 degrees ! Estimated noise=2504.28 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 = 0.0184172 Jy ! Component: 100 - total flux cleaned = 0.0213404 Jy ! Component: 150 - total flux cleaned = 0.0229747 Jy ! Component: 200 - total flux cleaned = 0.0215591 Jy ! Total flux subtracted in 200 components = 0.0215591 Jy ! Clean residual min=-0.004109 max=0.004079 Jy/beam ! Clean residual mean=0.000223 rms=0.001904 Jy/beam ! Combined flux in latest and established models = 0.114805 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 71 model components to the UV plane model. ! The established model now contains 97 components and 0.114805 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.276506Jy sigma=0.001266 ! Fit after self-cal, rms=0.276503Jy sigma=0.001266 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.682 x 28.8 at 26 degrees (North through East) ! Clean map min=-0.0080469 max=0.10526 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* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* MK 1.00* ! ! ! Correcting IF 2. ! Amplitude normalization factor in sub-array 1: 1.03855 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.99 HN 1.00* KP 1.00* ! LA 1.00 NL 0.92 OV 0.95 PT 0.89 ! SC 0.88 MK 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* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* MK 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* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* MK 1.00* ! ! ! Fit before self-cal, rms=0.276503Jy sigma=0.001266 ! Fit after self-cal, rms=0.274387Jy sigma=0.001266 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=0.274387Jy sigma=0.001266 ! Fit after self-cal, rms=0.274387Jy sigma=0.001266 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=3.634 mas, bmaj=28.7 mas, bpa=26.08 degrees ! Estimated noise=2477.71 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 = 0.000638248 Jy ! Component: 100 - total flux cleaned = -0.000701712 Jy ! Component: 150 - total flux cleaned = -0.00144456 Jy ! Component: 200 - total flux cleaned = -0.00259096 Jy ! Total flux subtracted in 200 components = -0.00259096 Jy ! Clean residual min=-0.002762 max=0.002773 Jy/beam ! Clean residual mean=0.000139 rms=0.001241 Jy/beam ! Combined flux in latest and established models = 0.112214 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 58 model components to the UV plane model. ! The established model now contains 146 components and 0.112214 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.273955Jy sigma=0.001264 ! Fit after self-cal, rms=0.273960Jy sigma=0.001264 ! 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=0.273960Jy sigma=0.001264 ! Fit after self-cal, rms=0.272568Jy sigma=0.001256 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 = 0.00162549 Jy ! Component: 100 - total flux cleaned = 0.00338208 Jy ! Component: 150 - total flux cleaned = 0.00300995 Jy ! Component: 200 - total flux cleaned = 0.00333307 Jy ! Total flux subtracted in 200 components = 0.00333307 Jy ! Clean residual min=-0.001972 max=0.001976 Jy/beam ! Clean residual mean=0.000123 rms=0.000856 Jy/beam ! Combined flux in latest and established models = 0.115547 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 52 model components to the UV plane model. ! The established model now contains 189 components and 0.115547 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.272273Jy sigma=0.001255 ! Fit after self-cal, rms=0.271975Jy sigma=0.001253 ! 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: 3.634 x 28.7 at 26.08 degrees (North through East) ! Clean map min=-0.0061577 max=0.1062 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=0.271975Jy sigma=0.001253 ! Fit after self-cal, rms=0.268997Jy sigma=0.001253 ! 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=0.268997Jy sigma=0.001253 ! Fit after self-cal, rms=0.268860Jy sigma=0.001253 ! Inverting map and beam ! Estimated beam: bmin=3.646 mas, bmaj=28.42 mas, bpa=26.03 degrees ! Estimated noise=2427.64 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00175458 Jy ! Component: 100 - total flux cleaned = 0.0027817 Jy ! Component: 150 - total flux cleaned = 0.00340414 Jy ! Component: 200 - total flux cleaned = 0.0034037 Jy ! Total flux subtracted in 200 components = 0.0034037 Jy ! Clean residual min=-0.001825 max=0.001846 Jy/beam ! Clean residual mean=0.000094 rms=0.000762 Jy/beam ! Combined flux in latest and established models = 0.118951 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 57 model components to the UV plane model. ! The established model now contains 239 components and 0.118951 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.268690Jy sigma=0.001252 ! Fit after self-cal, rms=0.268638Jy sigma=0.001252 ! 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=0.268638Jy sigma=0.001252 ! Fit after self-cal, rms=0.261740Jy sigma=0.001251 ! 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=0.261740Jy sigma=0.001251 ! Fit after self-cal, rms=0.261828Jy sigma=0.001251 ! Inverting map and beam ! Estimated beam: bmin=3.596 mas, bmaj=28.15 mas, bpa=26.05 degrees ! Estimated noise=2309.23 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.00199403 Jy ! Component: 100 - total flux cleaned = -0.000695031 Jy ! Component: 150 - total flux cleaned = 0.000555188 Jy ! Component: 200 - total flux cleaned = 0.000983063 Jy ! Total flux subtracted in 200 components = 0.000983063 Jy ! Clean residual min=-0.001693 max=0.001709 Jy/beam ! Clean residual mean=0.000037 rms=0.000690 Jy/beam ! Combined flux in latest and established models = 0.119934 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 43 model components to the UV plane model. ! The established model now contains 279 components and 0.119934 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.261599Jy sigma=0.001250 ! Fit after self-cal, rms=0.261707Jy sigma=0.001250 ! 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=8.669 mas, bmaj=41.67 mas, bpa=14.2 degrees ! Estimated noise=2735.53 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 = -0.000148799 Jy ! Component: 100 - total flux cleaned = -0.000402296 Jy ! Component: 150 - total flux cleaned = -0.000488813 Jy ! Component: 200 - total flux cleaned = -0.000482649 Jy ! Total flux subtracted in 200 components = -0.000482649 Jy ! Clean residual min=-0.001239 max=0.001260 Jy/beam ! Clean residual mean=0.000060 rms=0.000483 Jy/beam ! Combined flux in latest and established models = 0.119451 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 32 model components to the UV plane model. ! The established model now contains 308 components and 0.119451 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.261663Jy sigma=0.001250 ! Fit after self-cal, rms=0.261541Jy sigma=0.001249 ! 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=2.865 mas, bmaj=24.41 mas, bpa=26.84 degrees ! Estimated noise=3121.55 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0918503 Jy ! Component: 100 - total flux cleaned = 0.10369 Jy ! Component: 150 - total flux cleaned = 0.105249 Jy ! Component: 200 - total flux cleaned = 0.106942 Jy ! Total flux subtracted in 200 components = 0.106942 Jy ! Clean residual min=-0.006669 max=0.006676 Jy/beam ! Clean residual mean=0.000399 rms=0.002881 Jy/beam ! Combined flux in latest and established models = 0.106942 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 55 model components to the UV plane model. ! The established model now contains 55 components and 0.106942 Jy ! Inverting map and beam ! Estimated beam: bmin=3.596 mas, bmaj=28.15 mas, bpa=26.05 degrees ! Estimated noise=2309.23 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 = 0.00664938 Jy ! Component: 100 - total flux cleaned = 0.00799066 Jy ! Component: 150 - total flux cleaned = 0.00831661 Jy ! Component: 200 - total flux cleaned = 0.00806051 Jy ! Total flux subtracted in 200 components = 0.00806051 Jy ! Clean residual min=-0.003057 max=0.003104 Jy/beam ! Clean residual mean=0.000235 rms=0.001348 Jy/beam ! Combined flux in latest and established models = 0.115002 Jy ! Adding 71 model components to the UV plane model. ! The established model now contains 123 components and 0.115002 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=8.669 mas, bmaj=41.67 mas, bpa=14.2 degrees ! Estimated noise=2735.53 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 = 0.00220881 Jy ! Component: 100 - total flux cleaned = 0.00251416 Jy ! Component: 150 - total flux cleaned = 0.00103252 Jy ! Component: 200 - total flux cleaned = 0.000908548 Jy ! Total flux subtracted in 200 components = 0.000908548 Jy ! Clean residual min=-0.001755 max=0.001776 Jy/beam ! Clean residual mean=0.000209 rms=0.000758 Jy/beam ! Combined flux in latest and established models = 0.115911 Jy ! Adding 54 model components to the UV plane model. ! The established model now contains 177 components and 0.115911 Jy ! Inverting map uvtaper 0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=3.596 mas, bmaj=28.15 mas, bpa=26.05 degrees ! Estimated noise=2309.23 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.000693131 Jy ! Component: 100 - total flux cleaned = -0.000340492 Jy ! Component: 150 - total flux cleaned = -0.000495007 Jy ! Component: 200 - total flux cleaned = -0.00126955 Jy ! Total flux subtracted in 200 components = -0.00126955 Jy ! Clean residual min=-0.001870 max=0.001882 Jy/beam ! Clean residual mean=0.000119 rms=0.000807 Jy/beam ! Combined flux in latest and established models = 0.114641 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 47 model components to the UV plane model. ! The established model now contains 216 components and 0.114641 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.261645Jy sigma=0.001250 ! Fit after self-cal, rms=0.261484Jy sigma=0.001250 wmodel J0320-3837_S_2002_05_14_yyk\_map.mod ! Writing 216 model components to file: J0320-3837_S_2002_05_14_yyk_map.mod wobs J0320-3837_S_2002_05_14_yyk\_uvs.fits ! Writing UV FITS file: J0320-3837_S_2002_05_14_yyk_uvs.fits wwins J0320-3837_S_2002_05_14_yyk\_map.win ! wwins: No CLEAN windows to write. ! Error occured in command: wwins ![Exited script file: muppet] ! wmap "J0320-3837_S_2002_05_14_yyk\_map.fits" ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.596 x 28.15 at 26.05 degrees (North through East) ! Clean map min=-0.0066837 max=0.10616 Jy/beam ! Writing clean map to FITS file: J0320-3837_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 0.106165 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00086721 device "J0320-3837_S_2002_05_14_yyk\_map.eps/VPS" ! Attempting to open device: 'J0320-3837_S_2002_05_14_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -2.45056 2.45056 4.90112 9.80225 19.6045 39.209 78.418 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0026 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.106 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.596 x 28.15 at 26.05 degrees (North through East) ! Clean map min=-0.0066837 max=0.10616 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0320-3837_S_2002_05_14_yyk\_map.gif/gif" ! Attempting to open device: 'J0320-3837_S_2002_05_14_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J0320-3837_S_2002_05_14_yyk_uvs.log closed on Tue Jun 26 22:06:27 2007