! Started logfile: J1238-3825_X_2002_01_31_yyk_uvs.log on Wed Jun 27 10:57:10 2007 obs J1238-3825_X_2002_01_31_yyk_uva.fits ! Reading UV FITS file: J1238-3825_X_2002_01_31_yyk_uva.fits ! AN table 1: 37 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.728529 visibilities/baseline/integration-bin. ! Found source: J1238-3825 ! ! 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 8.40947e+09 8e+06 1 8e+06 ! 02 2 8.47947e+09 8e+06 1 8e+06 ! 03 3 8.79447e+09 8e+06 1 8e+06 ! 04 4 8.89947e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 1544 lines of history. ! ! Reading 4852 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 flag NL ! Flagging baselines of antenna 1:NL in the currently selected channels. ![@muppet J1238-3825_X_2002_01_31_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)= 0.203646 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=0.6915 mas, bmaj=1.86 mas, bpa=3.873 degrees ! Estimated noise=2261.58 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 = 0.0485002 Jy ! Component: 100 - total flux cleaned = 0.0642859 Jy ! Total flux subtracted in 100 components = 0.0642859 Jy ! Clean residual min=-0.013275 max=0.020650 Jy/beam ! Clean residual mean=0.000115 rms=0.004390 Jy/beam ! Combined flux in latest and established models = 0.0642859 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 18 model components to the UV plane model. ! The established model now contains 18 components and 0.0642859 Jy ! ! Correcting IF 1. ! A total of 122 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 89 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 89 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 121 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.194608Jy sigma=0.001397 ! Fit after self-cal, rms=0.194367Jy sigma=0.001395 ! Inverting map and beam ! Estimated beam: bmin=0.6915 mas, bmaj=1.86 mas, bpa=3.873 degrees ! Estimated noise=2261.58 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=0.9324 mas, bmaj=2.396 mas, bpa=-0.2372 degrees ! Estimated noise=1536.81 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 = 0.0153702 Jy ! Component: 100 - total flux cleaned = 0.0197969 Jy ! Component: 150 - total flux cleaned = 0.020064 Jy ! Component: 200 - total flux cleaned = 0.0203049 Jy ! Total flux subtracted in 200 components = 0.0203049 Jy ! Clean residual min=-0.012615 max=0.016861 Jy/beam ! Clean residual mean=0.000333 rms=0.004305 Jy/beam ! Combined flux in latest and established models = 0.0845907 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 24 model components to the UV plane model. ! The established model now contains 34 components and 0.0845907 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194233Jy sigma=0.001388 ! Fit after self-cal, rms=0.194242Jy sigma=0.001388 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9324 x 2.396 at -0.2372 degrees (North through East) ! Clean map min=-0.012236 max=0.054897 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=0.194242Jy sigma=0.001388 ! Fit after self-cal, rms=0.194242Jy sigma=0.001388 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=0.194242Jy sigma=0.001388 ! Fit after self-cal, rms=0.194243Jy sigma=0.001388 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.9324 mas, bmaj=2.396 mas, bpa=-0.2372 degrees ! Estimated noise=1536.81 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 = 0.000325481 Jy ! Component: 100 - total flux cleaned = 0.000477659 Jy ! Component: 150 - total flux cleaned = 0.000550315 Jy ! Component: 200 - total flux cleaned = 0.000614088 Jy ! Total flux subtracted in 200 components = 0.000614088 Jy ! Clean residual min=-0.012781 max=0.016617 Jy/beam ! Clean residual mean=0.000339 rms=0.004276 Jy/beam ! Combined flux in latest and established models = 0.0852048 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 6 model components to the UV plane model. ! The established model now contains 36 components and 0.0852048 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194209Jy sigma=0.001387 ! Fit after self-cal, rms=0.194206Jy sigma=0.001387 ! 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=0.194206Jy sigma=0.001387 ! Fit after self-cal, rms=0.192040Jy sigma=0.001372 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 = 0.00490286 Jy ! Component: 100 - total flux cleaned = 0.00498369 Jy ! Component: 150 - total flux cleaned = 0.00512498 Jy ! Component: 200 - total flux cleaned = 0.00518777 Jy ! Total flux subtracted in 200 components = 0.00518777 Jy ! Clean residual min=-0.011117 max=0.014877 Jy/beam ! Clean residual mean=0.000295 rms=0.003692 Jy/beam ! Combined flux in latest and established models = 0.0903926 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 11 model components to the UV plane model. ! The established model now contains 41 components and 0.0903926 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.192053Jy sigma=0.001371 ! Fit after self-cal, rms=0.191043Jy sigma=0.001365 ! 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: 0.9324 x 2.396 at -0.2372 degrees (North through East) ! Clean map min=-0.011058 max=0.059625 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=3.187 mas, bmaj=11.58 mas, bpa=5.896 degrees ! Estimated noise=1872.36 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 = 0.00338725 Jy ! Component: 100 - total flux cleaned = 0.00346861 Jy ! Component: 150 - total flux cleaned = 0.00362665 Jy ! Component: 200 - total flux cleaned = 0.00370367 Jy ! Total flux subtracted in 200 components = 0.00370367 Jy ! Clean residual min=-0.013391 max=0.014307 Jy/beam ! Clean residual mean=0.000447 rms=0.004444 Jy/beam ! Combined flux in latest and established models = 0.0940962 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 41 components and 0.0940963 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.191042Jy sigma=0.001365 ! Fit after self-cal, rms=0.190601Jy sigma=0.001361 ! 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=0.6915 mas, bmaj=1.86 mas, bpa=3.873 degrees ! Estimated noise=2261.58 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.056156 Jy ! Component: 100 - total flux cleaned = 0.072674 Jy ! Component: 150 - total flux cleaned = 0.0800198 Jy ! Component: 200 - total flux cleaned = 0.0826354 Jy ! Total flux subtracted in 200 components = 0.0826354 Jy ! Clean residual min=-0.014111 max=0.013428 Jy/beam ! Clean residual mean=0.000088 rms=0.003809 Jy/beam ! Combined flux in latest and established models = 0.0826354 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 28 model components to the UV plane model. ! The established model now contains 28 components and 0.0826354 Jy ! Inverting map and beam ! Estimated beam: bmin=0.9324 mas, bmaj=2.396 mas, bpa=-0.2372 degrees ! Estimated noise=1536.81 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) ! Added new window around map position (-6.4, 24). ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0169322 Jy ! Component: 100 - total flux cleaned = 0.0179512 Jy ! Component: 150 - total flux cleaned = 0.0177699 Jy ! Component: 200 - total flux cleaned = 0.0179225 Jy ! Total flux subtracted in 200 components = 0.0179225 Jy ! Clean residual min=-0.010731 max=0.009759 Jy/beam ! Clean residual mean=0.000096 rms=0.002673 Jy/beam ! Combined flux in latest and established models = 0.100558 Jy ! Adding 22 model components to the UV plane model. ! The established model now contains 49 components and 0.100558 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=3.187 mas, bmaj=11.58 mas, bpa=5.896 degrees ! Estimated noise=1872.36 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 = 0.000166234 Jy ! Component: 100 - total flux cleaned = 0.000277715 Jy ! Component: 150 - total flux cleaned = 0.0002732 Jy ! Component: 200 - total flux cleaned = 0.000267861 Jy ! Total flux subtracted in 200 components = 0.000267861 Jy ! Clean residual min=-0.012036 max=0.009425 Jy/beam ! Clean residual mean=0.000167 rms=0.003163 Jy/beam ! Combined flux in latest and established models = 0.100826 Jy ! Adding 7 model components to the UV plane model. ! The established model now contains 54 components and 0.100826 Jy ! Inverting map uvtaper 0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=0.9324 mas, bmaj=2.396 mas, bpa=-0.2372 degrees ! Estimated noise=1536.81 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.000559122 Jy ! Component: 100 - total flux cleaned = -0.000785234 Jy ! Component: 150 - total flux cleaned = -0.000881641 Jy ! Component: 200 - total flux cleaned = -0.000885839 Jy ! Total flux subtracted in 200 components = -0.000885839 Jy ! Clean residual min=-0.010895 max=0.008506 Jy/beam ! Clean residual mean=0.000096 rms=0.002488 Jy/beam ! Combined flux in latest and established models = 0.0999399 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 61 components and 0.0999399 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.189425Jy sigma=0.001354 ! Fit after self-cal, rms=0.189128Jy sigma=0.001351 wmodel J1238-3825_X_2002_01_31_yyk\_map.mod ! Writing 61 model components to file: J1238-3825_X_2002_01_31_yyk_map.mod wobs J1238-3825_X_2002_01_31_yyk\_uvs.fits ! Applying 37 buffered edits. ! Writing UV FITS file: J1238-3825_X_2002_01_31_yyk_uvs.fits wwins J1238-3825_X_2002_01_31_yyk\_map.win ! wwins: Wrote 2 windows to J1238-3825_X_2002_01_31_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 = -0.00423696 Jy ! Component: 100 - total flux cleaned = -0.00624541 Jy ! Component: 150 - total flux cleaned = -0.00636781 Jy ! Component: 200 - total flux cleaned = -0.00626171 Jy ! Component: 250 - total flux cleaned = -0.00606859 Jy ! Component: 300 - total flux cleaned = -0.00607564 Jy ! Component: 350 - total flux cleaned = -0.00591278 Jy ! Component: 400 - total flux cleaned = -0.00575585 Jy ! Component: 450 - total flux cleaned = -0.00568016 Jy ! Component: 500 - total flux cleaned = -0.0058228 Jy ! Component: 550 - total flux cleaned = -0.0058871 Jy ! Component: 600 - total flux cleaned = -0.00595197 Jy ! Component: 650 - total flux cleaned = -0.00601304 Jy ! Component: 700 - total flux cleaned = -0.0061344 Jy ! Component: 750 - total flux cleaned = -0.00619361 Jy ! Component: 800 - total flux cleaned = -0.00630988 Jy ! Component: 850 - total flux cleaned = -0.00642392 Jy ! Component: 900 - total flux cleaned = -0.00653591 Jy ! Component: 950 - total flux cleaned = -0.00653716 Jy ! Component: 1000 - total flux cleaned = -0.00670118 Jy ! Component: 1050 - total flux cleaned = -0.00659396 Jy ! Component: 1100 - total flux cleaned = -0.0064884 Jy ! Component: 1150 - total flux cleaned = -0.00643618 Jy ! Component: 1200 - total flux cleaned = -0.00633246 Jy ! Component: 1250 - total flux cleaned = -0.00633215 Jy ! Component: 1300 - total flux cleaned = -0.00638311 Jy ! Component: 1350 - total flux cleaned = -0.00643307 Jy ! Component: 1400 - total flux cleaned = -0.00653347 Jy ! Component: 1450 - total flux cleaned = -0.00668316 Jy ! Component: 1500 - total flux cleaned = -0.00688321 Jy ! Component: 1550 - total flux cleaned = -0.00703293 Jy ! Component: 1600 - total flux cleaned = -0.00728204 Jy ! Component: 1650 - total flux cleaned = -0.00738202 Jy ! Component: 1700 - total flux cleaned = -0.00763244 Jy ! Component: 1750 - total flux cleaned = -0.0077832 Jy ! Component: 1800 - total flux cleaned = -0.00798496 Jy ! Component: 1850 - total flux cleaned = -0.00808596 Jy ! Component: 1900 - total flux cleaned = -0.00823828 Jy ! Component: 1950 - total flux cleaned = -0.00828933 Jy ! Component: 2000 - total flux cleaned = -0.00849423 Jy ! Total flux subtracted in 2048 components = -0.0085976 Jy ! Clean residual min=-0.002738 max=0.002705 Jy/beam ! Clean residual mean=-0.000047 rms=0.000981 Jy/beam ! Combined flux in latest and established models = 0.0913423 Jy keep ! Adding 91 model components to the UV plane model. ! The established model now contains 152 components and 0.0913423 Jy ![Exited script file: muppet] wmap "J1238-3825_X_2002_01_31_yyk\_map.fits" ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9324 x 2.396 at -0.2372 degrees (North through East) ! Clean map min=-0.0067432 max=0.060177 Jy/beam ! Writing clean map to FITS file: J1238-3825_X_2002_01_31_yyk_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0601765 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00102316 device "J1238-3825_X_2002_01_31_yyk\_map.eps/VPS" ! Attempting to open device: 'J1238-3825_X_2002_01_31_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -5.10078 5.10078 10.2016 20.4031 40.8062 81.6125 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.003 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.06 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9324 x 2.396 at -0.2372 degrees (North through East) ! Clean map min=-0.0067432 max=0.060177 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1238-3825_X_2002_01_31_yyk\_map.gif/gif" ! Attempting to open device: 'J1238-3825_X_2002_01_31_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J1238-3825_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 10:57:16 2007