! Started logfile: J1852-2433_X_2005_05_12_yyk_uvs.log on Sat Oct 8 17:37:19 2005 obs J1852-2433_X_2005_05_12_yyk_uve.fits ! Reading UV FITS file: J1852-2433_X_2005_05_12_yyk_uve.fits ! AN table 1: 18 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.34321 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1852-2433 ! ! 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 1439 lines of history. ! ! Reading 1112 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 J1852-2433_X_2005_05_12_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)= 0.0926412 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=0.9111 mas, bmaj=3.575 mas, bpa=-22.81 degrees ! Estimated noise=3.24608 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 (0.2, -0.2). ! clean: niter=100 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0487077 Jy ! Component: 100 - total flux cleaned = 0.0601559 Jy ! Total flux subtracted in 100 components = 0.0601559 Jy ! Clean residual min=-0.010093 max=0.010167 Jy/beam ! Clean residual mean=-0.000030 rms=0.002720 Jy/beam ! Combined flux in latest and established models = 0.0601559 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 21 model components to the UV plane model. ! The established model now contains 21 components and 0.0601559 Jy ! ! Correcting IF 1. ! A total of 114 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 108 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 123 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 160 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.071040Jy sigma=1.036567 ! Fit after self-cal, rms=0.068319Jy sigma=1.000659 ! Inverting map and beam ! Estimated beam: bmin=0.9111 mas, bmaj=3.575 mas, bpa=-22.81 degrees ! Estimated noise=3.24608 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=1.41 mas, bmaj=4.864 mas, bpa=-23.61 degrees ! Estimated noise=1.86559 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 = 0.00843657 Jy ! Component: 100 - total flux cleaned = 0.0104301 Jy ! Component: 150 - total flux cleaned = 0.0105127 Jy ! Component: 200 - total flux cleaned = 0.010384 Jy ! Total flux subtracted in 200 components = 0.010384 Jy ! Clean residual min=-0.004828 max=0.006219 Jy/beam ! Clean residual mean=-0.000027 rms=0.001580 Jy/beam ! Combined flux in latest and established models = 0.0705398 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 13 model components to the UV plane model. ! The established model now contains 33 components and 0.0705398 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.067584Jy sigma=0.985712 ! Fit after self-cal, rms=0.067548Jy sigma=0.984764 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.41 x 4.864 at -23.61 degrees (North through East) ! Clean map min=-0.0046911 max=0.050225 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: 1.00175 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.07 HN 1.00* KP 0.98 ! LA 1.00* MK 0.89 NL 1.00* OV 1.10 ! PT 0.95 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=0.067548Jy sigma=0.984764 ! Fit after self-cal, rms=0.067447Jy sigma=0.983832 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=0.067447Jy sigma=0.983832 ! Fit after self-cal, rms=0.067440Jy sigma=0.983626 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=1.363 mas, bmaj=4.889 mas, bpa=-24.03 degrees ! Estimated noise=1.86638 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 = 0.00089413 Jy ! Component: 100 - total flux cleaned = 0.00082465 Jy ! Component: 150 - total flux cleaned = 0.000702403 Jy ! Component: 200 - total flux cleaned = 0.000643291 Jy ! Total flux subtracted in 200 components = 0.000643291 Jy ! Clean residual min=-0.004658 max=0.006402 Jy/beam ! Clean residual mean=-0.000021 rms=0.001510 Jy/beam ! Combined flux in latest and established models = 0.0711831 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 8 model components to the UV plane model. ! The established model now contains 37 components and 0.0711831 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.067332Jy sigma=0.981751 ! Fit after self-cal, rms=0.067331Jy sigma=0.981483 ! 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=0.067331Jy sigma=0.981483 ! Fit after self-cal, rms=0.061074Jy sigma=0.868760 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 = 0.00485869 Jy ! Component: 100 - total flux cleaned = 0.0049495 Jy ! Component: 150 - total flux cleaned = 0.00489625 Jy ! Component: 200 - total flux cleaned = 0.00484281 Jy ! Total flux subtracted in 200 components = 0.00484281 Jy ! Clean residual min=-0.004231 max=0.005883 Jy/beam ! Clean residual mean=-0.000011 rms=0.001449 Jy/beam ! Combined flux in latest and established models = 0.0760259 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 12 model components to the UV plane model. ! The established model now contains 45 components and 0.076026 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.060639Jy sigma=0.861585 ! Fit after self-cal, rms=0.060030Jy sigma=0.852215 ! 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: 1.363 x 4.889 at -24.03 degrees (North through East) ! Clean map min=-0.0042952 max=0.057285 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=3.605 mas, bmaj=8.077 mas, bpa=7.978 degrees ! Estimated noise=2.04084 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 = 0.000367555 Jy ! Component: 100 - total flux cleaned = 0.000335 Jy ! Component: 150 - total flux cleaned = 0.00020389 Jy ! Component: 200 - total flux cleaned = 0.000109649 Jy ! Total flux subtracted in 200 components = 0.000109649 Jy ! Clean residual min=-0.004627 max=0.005239 Jy/beam ! Clean residual mean=-0.000014 rms=0.001660 Jy/beam ! Combined flux in latest and established models = 0.0761356 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 49 components and 0.0761356 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.060008Jy sigma=0.851506 ! Fit after self-cal, rms=0.059942Jy sigma=0.850460 ! 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=0.9003 mas, bmaj=3.577 mas, bpa=-22.86 degrees ! Estimated noise=3.21834 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0567396 Jy ! Component: 100 - total flux cleaned = 0.0711206 Jy ! Component: 150 - total flux cleaned = 0.0777208 Jy ! Component: 200 - total flux cleaned = 0.0800456 Jy ! Total flux subtracted in 200 components = 0.0800456 Jy ! Clean residual min=-0.007629 max=0.007642 Jy/beam ! Clean residual mean=0.000003 rms=0.002116 Jy/beam ! Combined flux in latest and established models = 0.0800457 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 31 model components to the UV plane model. ! The established model now contains 31 components and 0.0800457 Jy ! Inverting map and beam ! Estimated beam: bmin=1.363 mas, bmaj=4.889 mas, bpa=-24.03 degrees ! Estimated noise=1.86638 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 = -0.00236341 Jy ! Component: 100 - total flux cleaned = -0.00262441 Jy ! Component: 150 - total flux cleaned = -0.00289304 Jy ! Component: 200 - total flux cleaned = -0.00304252 Jy ! Total flux subtracted in 200 components = -0.00304252 Jy ! Clean residual min=-0.004761 max=0.005785 Jy/beam ! Clean residual mean=-0.000005 rms=0.001532 Jy/beam ! Combined flux in latest and established models = 0.0770031 Jy ! Adding 13 model components to the UV plane model. ! The established model now contains 44 components and 0.0770032 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=3.605 mas, bmaj=8.077 mas, bpa=7.978 degrees ! Estimated noise=2.04084 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 = -0.000130188 Jy ! Component: 100 - total flux cleaned = -0.000248516 Jy ! Component: 150 - total flux cleaned = -0.000360867 Jy ! Component: 200 - total flux cleaned = -0.000469288 Jy ! Total flux subtracted in 200 components = -0.000469288 Jy ! Clean residual min=-0.004944 max=0.005309 Jy/beam ! Clean residual mean=-0.000011 rms=0.001715 Jy/beam ! Combined flux in latest and established models = 0.0765339 Jy ! Adding 6 model components to the UV plane model. ! The established model now contains 46 components and 0.0765339 Jy ! Inverting map uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=1.363 mas, bmaj=4.889 mas, bpa=-24.03 degrees ! Estimated noise=1.86638 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -4.38243e-05 Jy ! Component: 100 - total flux cleaned = -0.000236177 Jy ! Component: 150 - total flux cleaned = -0.000404427 Jy ! Component: 200 - total flux cleaned = -0.000562054 Jy ! Total flux subtracted in 200 components = -0.000562054 Jy ! Clean residual min=-0.004532 max=0.005584 Jy/beam ! Clean residual mean=-0.000008 rms=0.001475 Jy/beam ! Combined flux in latest and established models = 0.0759718 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 9 model components to the UV plane model. ! The established model now contains 51 components and 0.0759718 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.059878Jy sigma=0.849665 ! Fit after self-cal, rms=0.059871Jy sigma=0.849388 wmodel J1852-2433_X_2005_05_12_yyk\_map.mod ! Writing 51 model components to file: J1852-2433_X_2005_05_12_yyk_map.mod wobs J1852-2433_X_2005_05_12_yyk\_uvs.fits ! Writing UV FITS file: J1852-2433_X_2005_05_12_yyk_uvs.fits wwins J1852-2433_X_2005_05_12_yyk\_map.win ! wwins: Wrote 1 windows to J1852-2433_X_2005_05_12_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 = 0.000942285 Jy ! Component: 100 - total flux cleaned = 0.000796474 Jy ! Component: 150 - total flux cleaned = 0.000862838 Jy ! Component: 200 - total flux cleaned = 0.00123015 Jy ! Component: 250 - total flux cleaned = 0.00157821 Jy ! Component: 300 - total flux cleaned = 0.00174263 Jy ! Component: 350 - total flux cleaned = 0.0019505 Jy ! Component: 400 - total flux cleaned = 0.00229657 Jy ! Component: 450 - total flux cleaned = 0.0025338 Jy ! Component: 500 - total flux cleaned = 0.00266938 Jy ! Component: 550 - total flux cleaned = 0.00280048 Jy ! Component: 600 - total flux cleaned = 0.00296916 Jy ! Component: 650 - total flux cleaned = 0.00313152 Jy ! Component: 700 - total flux cleaned = 0.00332909 Jy ! Component: 750 - total flux cleaned = 0.00348139 Jy ! Component: 800 - total flux cleaned = 0.00362766 Jy ! Component: 850 - total flux cleaned = 0.00373287 Jy ! Component: 900 - total flux cleaned = 0.00376704 Jy ! Component: 950 - total flux cleaned = 0.00376708 Jy ! Component: 1000 - total flux cleaned = 0.00386341 Jy ! Component: 1050 - total flux cleaned = 0.00380119 Jy ! Component: 1100 - total flux cleaned = 0.00374166 Jy ! Component: 1150 - total flux cleaned = 0.00368329 Jy ! Component: 1200 - total flux cleaned = 0.00356851 Jy ! Component: 1250 - total flux cleaned = 0.00348437 Jy ! Component: 1300 - total flux cleaned = 0.00348425 Jy ! Component: 1350 - total flux cleaned = 0.00348405 Jy ! Component: 1400 - total flux cleaned = 0.00350991 Jy ! Component: 1450 - total flux cleaned = 0.00358733 Jy ! Component: 1500 - total flux cleaned = 0.00361264 Jy ! Component: 1550 - total flux cleaned = 0.00358761 Jy ! Component: 1600 - total flux cleaned = 0.00356318 Jy ! Component: 1650 - total flux cleaned = 0.00351567 Jy ! Component: 1700 - total flux cleaned = 0.0034457 Jy ! Component: 1750 - total flux cleaned = 0.00342233 Jy ! Component: 1800 - total flux cleaned = 0.00339933 Jy ! Component: 1850 - total flux cleaned = 0.0033093 Jy ! Component: 1900 - total flux cleaned = 0.00335369 Jy ! Component: 1950 - total flux cleaned = 0.00339771 Jy ! Component: 2000 - total flux cleaned = 0.00341989 Jy ! Total flux subtracted in 2048 components = 0.0035076 Jy ! Clean residual min=-0.001096 max=0.001191 Jy/beam ! Clean residual mean=-0.000025 rms=0.000439 Jy/beam ! Combined flux in latest and established models = 0.0794794 Jy keep ! Adding 89 model components to the UV plane model. ! The established model now contains 140 components and 0.0794794 Jy ![Exited script file: muppet] wmap "J1852-2433_X_2005_05_12_yyk\_map.fits" ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.363 x 4.889 at -24.03 degrees (North through East) ! Clean map min=-0.0036222 max=0.055319 Jy/beam ! Writing clean map to FITS file: J1852-2433_X_2005_05_12_yyk_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0553194 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000453212 device "J1852-2433_X_2005_05_12_yyk\_map.eps/VPS" ! Attempting to open device: 'J1852-2433_X_2005_05_12_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -2.45779 2.45779 4.91559 9.83118 19.6624 39.3247 78.6494 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0013 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.055 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.363 x 4.889 at -24.03 degrees (North through East) ! Clean map min=-0.0036222 max=0.055319 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1852-2433_X_2005_05_12_yyk\_map.gif/gif" ! Attempting to open device: 'J1852-2433_X_2005_05_12_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J1852-2433_X_2005_05_12_yyk_uvs.log closed on Sat Oct 8 17:37:23 2005