! Started logfile: J2303-3030_X_2002_01_31_yyk_uvs.log on Wed Jun 27 11:05:33 2007 obs J2303-3030_X_2002_01_31_yyk_uva.fits ! Reading UV FITS file: J2303-3030_X_2002_01_31_yyk_uva.fits ! AN table 1: 69 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.679227 visibilities/baseline/integration-bin. ! Found source: J2303-3030 ! ! 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 8436 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 J2303-3030_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)= 0.242955 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=0.6298 mas, bmaj=1.535 mas, bpa=2.467 degrees ! Estimated noise=1851.56 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 = 0.0512318 Jy ! Component: 100 - total flux cleaned = 0.0752436 Jy ! Total flux subtracted in 100 components = 0.0752436 Jy ! Clean residual min=-0.017724 max=0.015594 Jy/beam ! Clean residual mean=0.000006 rms=0.004033 Jy/beam ! Combined flux in latest and established models = 0.0752436 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 17 model components to the UV plane model. ! The established model now contains 17 components and 0.0752436 Jy ! ! Correcting IF 1. ! A total of 151 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 151 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 176 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 151 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.230885Jy sigma=0.001502 ! Fit after self-cal, rms=0.229828Jy sigma=0.001491 ! Inverting map and beam ! Estimated beam: bmin=0.6298 mas, bmaj=1.535 mas, bpa=2.467 degrees ! Estimated noise=1851.56 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=0.8358 mas, bmaj=2.087 mas, bpa=3.551 degrees ! Estimated noise=1146.63 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 (-0.6, -0.4). ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0317316 Jy ! Component: 100 - total flux cleaned = 0.042571 Jy ! Component: 150 - total flux cleaned = 0.0434359 Jy ! Component: 200 - total flux cleaned = 0.0437649 Jy ! Total flux subtracted in 200 components = 0.0437649 Jy ! Clean residual min=-0.009857 max=0.009586 Jy/beam ! Clean residual mean=0.000125 rms=0.002564 Jy/beam ! Combined flux in latest and established models = 0.119009 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 30 model components to the UV plane model. ! The established model now contains 45 components and 0.119009 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.227670Jy sigma=0.001468 ! Fit after self-cal, rms=0.227662Jy sigma=0.001468 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8358 x 2.087 at 3.551 degrees (North through East) ! Clean map min=-0.0091482 max=0.06174 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=0.227662Jy sigma=0.001468 ! Fit after self-cal, rms=0.227662Jy sigma=0.001468 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=0.227662Jy sigma=0.001468 ! Fit after self-cal, rms=0.227662Jy sigma=0.001468 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.8358 mas, bmaj=2.087 mas, bpa=3.551 degrees ! Estimated noise=1146.63 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 = -0.000279761 Jy ! Component: 100 - total flux cleaned = -0.000625143 Jy ! Component: 150 - total flux cleaned = -0.000830736 Jy ! Component: 200 - total flux cleaned = -0.00109772 Jy ! Total flux subtracted in 200 components = -0.00109772 Jy ! Clean residual min=-0.009224 max=0.008963 Jy/beam ! Clean residual mean=0.000123 rms=0.002483 Jy/beam ! Combined flux in latest and established models = 0.117911 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 22 model components to the UV plane model. ! The established model now contains 56 components and 0.117911 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.227601Jy sigma=0.001467 ! Fit after self-cal, rms=0.227595Jy sigma=0.001467 ! 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=0.227595Jy sigma=0.001467 ! Fit after self-cal, rms=0.226453Jy sigma=0.001459 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 = 0.0018621 Jy ! Component: 100 - total flux cleaned = 0.00159352 Jy ! Component: 150 - total flux cleaned = 0.00125284 Jy ! Component: 200 - total flux cleaned = 0.0010554 Jy ! Total flux subtracted in 200 components = 0.0010554 Jy ! Clean residual min=-0.009430 max=0.009296 Jy/beam ! Clean residual mean=0.000109 rms=0.002371 Jy/beam ! Combined flux in latest and established models = 0.118966 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 17 model components to the UV plane model. ! The established model now contains 66 components and 0.118966 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.226362Jy sigma=0.001458 ! Fit after self-cal, rms=0.226063Jy sigma=0.001456 ! 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: 0.8358 x 2.087 at 3.551 degrees (North through East) ! Clean map min=-0.0092345 max=0.06586 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 mas, bmaj=7.99 mas, bpa=11.46 degrees ! Estimated noise=1490.48 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 = -0.000898229 Jy ! Component: 100 - total flux cleaned = -0.000898746 Jy ! Component: 150 - total flux cleaned = -0.000900798 Jy ! Component: 200 - total flux cleaned = -0.000986103 Jy ! Total flux subtracted in 200 components = -0.000986103 Jy ! Clean residual min=-0.011240 max=0.009581 Jy/beam ! Clean residual mean=0.000208 rms=0.003553 Jy/beam ! Combined flux in latest and established models = 0.11798 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 74 components and 0.11798 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.226110Jy sigma=0.001456 ! Fit after self-cal, rms=0.225935Jy sigma=0.001454 ! 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=0.6298 mas, bmaj=1.535 mas, bpa=2.467 degrees ! Estimated noise=1851.56 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0637986 Jy ! Component: 100 - total flux cleaned = 0.0936458 Jy ! Component: 150 - total flux cleaned = 0.109712 Jy ! Component: 200 - total flux cleaned = 0.114714 Jy ! Total flux subtracted in 200 components = 0.114714 Jy ! Clean residual min=-0.013217 max=0.013848 Jy/beam ! Clean residual mean=0.000050 rms=0.003500 Jy/beam ! Combined flux in latest and established models = 0.114714 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 36 model components to the UV plane model. ! The established model now contains 36 components and 0.114714 Jy ! Inverting map and beam ! Estimated beam: bmin=0.8358 mas, bmaj=2.087 mas, bpa=3.551 degrees ! Estimated noise=1146.63 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 = 0.00884035 Jy ! Component: 100 - total flux cleaned = 0.00937175 Jy ! Component: 150 - total flux cleaned = 0.0095363 Jy ! Component: 200 - total flux cleaned = 0.0090188 Jy ! Total flux subtracted in 200 components = 0.0090188 Jy ! Clean residual min=-0.009246 max=0.008769 Jy/beam ! Clean residual mean=0.000113 rms=0.002406 Jy/beam ! Combined flux in latest and established models = 0.123733 Jy ! Adding 17 model components to the UV plane model. ! The established model now contains 51 components and 0.123733 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 mas, bmaj=7.99 mas, bpa=11.46 degrees ! Estimated noise=1490.48 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 = -0.00160993 Jy ! Component: 100 - total flux cleaned = -0.00176687 Jy ! Component: 150 - total flux cleaned = -0.0019668 Jy ! Component: 200 - total flux cleaned = -0.0021394 Jy ! Total flux subtracted in 200 components = -0.0021394 Jy ! Clean residual min=-0.011034 max=0.010060 Jy/beam ! Clean residual mean=0.000212 rms=0.003610 Jy/beam ! Combined flux in latest and established models = 0.121593 Jy ! Adding 11 model components to the UV plane model. ! The established model now contains 60 components and 0.121593 Jy ! Inverting map uvtaper 0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=0.8358 mas, bmaj=2.087 mas, bpa=3.551 degrees ! Estimated noise=1146.63 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.00027595 Jy ! Component: 100 - total flux cleaned = -0.000673393 Jy ! Component: 150 - total flux cleaned = -0.00075298 Jy ! Component: 200 - total flux cleaned = -0.000891245 Jy ! Total flux subtracted in 200 components = -0.000891245 Jy ! Clean residual min=-0.008761 max=0.008065 Jy/beam ! Clean residual mean=0.000109 rms=0.002330 Jy/beam ! Combined flux in latest and established models = 0.120702 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 16 model components to the UV plane model. ! The established model now contains 70 components and 0.120702 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.225785Jy sigma=0.001453 ! Fit after self-cal, rms=0.225614Jy sigma=0.001452 wmodel J2303-3030_X_2002_01_31_yyk\_map.mod ! Writing 70 model components to file: J2303-3030_X_2002_01_31_yyk_map.mod wobs J2303-3030_X_2002_01_31_yyk\_uvs.fits ! Applying 69 buffered edits. ! Writing UV FITS file: J2303-3030_X_2002_01_31_yyk_uvs.fits wwins J2303-3030_X_2002_01_31_yyk\_map.win ! wwins: Wrote 2 windows to J2303-3030_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 = -0.00141615 Jy ! Component: 100 - total flux cleaned = -0.00209109 Jy ! Component: 150 - total flux cleaned = -0.00221914 Jy ! Component: 200 - total flux cleaned = -0.00210104 Jy ! Component: 250 - total flux cleaned = -0.0021002 Jy ! Component: 300 - total flux cleaned = -0.00241713 Jy ! Component: 350 - total flux cleaned = -0.0024197 Jy ! Component: 400 - total flux cleaned = -0.00213566 Jy ! Component: 450 - total flux cleaned = -0.00185949 Jy ! Component: 500 - total flux cleaned = -0.00132369 Jy ! Component: 550 - total flux cleaned = -0.000633637 Jy ! Component: 600 - total flux cleaned = -0.000133196 Jy ! Component: 650 - total flux cleaned = 0.000433626 Jy ! Component: 700 - total flux cleaned = 0.000747921 Jy ! Component: 750 - total flux cleaned = 0.000902869 Jy ! Component: 800 - total flux cleaned = 0.00127747 Jy ! Component: 850 - total flux cleaned = 0.00149613 Jy ! Component: 900 - total flux cleaned = 0.00163914 Jy ! Component: 950 - total flux cleaned = 0.0020544 Jy ! Component: 1000 - total flux cleaned = 0.00232376 Jy ! Component: 1050 - total flux cleaned = 0.00265569 Jy ! Component: 1100 - total flux cleaned = 0.00285095 Jy ! Component: 1150 - total flux cleaned = 0.00297864 Jy ! Component: 1200 - total flux cleaned = 0.00322828 Jy ! Component: 1250 - total flux cleaned = 0.00335016 Jy ! Component: 1300 - total flux cleaned = 0.00341033 Jy ! Component: 1350 - total flux cleaned = 0.0036446 Jy ! Component: 1400 - total flux cleaned = 0.0036447 Jy ! Component: 1450 - total flux cleaned = 0.0038715 Jy ! Component: 1500 - total flux cleaned = 0.00420354 Jy ! Component: 1550 - total flux cleaned = 0.00453063 Jy ! Component: 1600 - total flux cleaned = 0.00474466 Jy ! Component: 1650 - total flux cleaned = 0.00484884 Jy ! Component: 1700 - total flux cleaned = 0.0048477 Jy ! Component: 1750 - total flux cleaned = 0.00484699 Jy ! Component: 1800 - total flux cleaned = 0.00484665 Jy ! Component: 1850 - total flux cleaned = 0.00489653 Jy ! Component: 1900 - total flux cleaned = 0.0050426 Jy ! Component: 1950 - total flux cleaned = 0.00494687 Jy ! Component: 2000 - total flux cleaned = 0.00508982 Jy ! Total flux subtracted in 2048 components = 0.0052299 Jy ! Clean residual min=-0.002878 max=0.002366 Jy/beam ! Clean residual mean=0.000065 rms=0.000914 Jy/beam ! Combined flux in latest and established models = 0.125932 Jy keep ! Adding 127 model components to the UV plane model. ! The established model now contains 197 components and 0.125932 Jy ![Exited script file: muppet] wmap "J2303-3030_X_2002_01_31_yyk\_map.fits" ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8358 x 2.087 at 3.551 degrees (North through East) ! Clean map min=-0.0061223 max=0.059467 Jy/beam ! Writing clean map to FITS file: J2303-3030_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 0.0594671 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00089774 device "J2303-3030_X_2002_01_31_yyk\_map.eps/VPS" ! Attempting to open device: 'J2303-3030_X_2002_01_31_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -4.52893 4.52893 9.05786 18.1157 36.2314 72.4628 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0026 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.059 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8358 x 2.087 at 3.551 degrees (North through East) ! Clean map min=-0.0061223 max=0.059467 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J2303-3030_X_2002_01_31_yyk\_map.gif/gif" ! Attempting to open device: 'J2303-3030_X_2002_01_31_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J2303-3030_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 11:05:39 2007