! Started logfile: J0350-3232_X_2002_01_31_yyk_uvs.log on Wed Jun 27 10:47:30 2007 obs J0350-3232_X_2002_01_31_yyk_uva.fits ! Reading UV FITS file: J0350-3232_X_2002_01_31_yyk_uva.fits ! AN table 1: 96 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.721296 visibilities/baseline/integration-bin. ! Found source: J0350-3232 ! ! 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 12464 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 J0350-3232_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)= 0.189676 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=0.6568 mas, bmaj=1.707 mas, bpa=9.083 degrees ! Estimated noise=1849.85 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, -0.2). ! clean: niter=100 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0793401 Jy ! Component: 100 - total flux cleaned = 0.102147 Jy ! Total flux subtracted in 100 components = 0.102147 Jy ! Clean residual min=-0.010694 max=0.011488 Jy/beam ! Clean residual mean=0.000018 rms=0.002918 Jy/beam ! Combined flux in latest and established models = 0.102147 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 0.102147 Jy ! ! Correcting IF 1. ! A total of 237 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 237 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 305 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 264 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.160439Jy sigma=0.001257 ! Fit after self-cal, rms=0.160292Jy sigma=0.001256 ! Inverting map and beam ! Estimated beam: bmin=0.6568 mas, bmaj=1.707 mas, bpa=9.083 degrees ! Estimated noise=1849.85 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=0.9795 mas, bmaj=2.432 mas, bpa=11.31 degrees ! Estimated noise=878.077 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 = 0.0124367 Jy ! Component: 100 - total flux cleaned = 0.0148376 Jy ! Component: 150 - total flux cleaned = 0.0148459 Jy ! Component: 200 - total flux cleaned = 0.0147893 Jy ! Total flux subtracted in 200 components = 0.0147893 Jy ! Clean residual min=-0.005726 max=0.005636 Jy/beam ! Clean residual mean=0.000085 rms=0.001629 Jy/beam ! Combined flux in latest and established models = 0.116936 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 19 model components to the UV plane model. ! The established model now contains 29 components and 0.116936 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.159676Jy sigma=0.001250 ! Fit after self-cal, rms=0.159669Jy sigma=0.001250 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9795 x 2.432 at 11.31 degrees (North through East) ! Clean map min=-0.0056472 max=0.097194 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: 1.00452 ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 0.97 HN 1.00* KP 1.02 ! LA 1.11 MK 1.02 NL 1.00* OV 0.94 ! PT 0.96 SC 0.96 ! ! ! Correcting IF 2. ! Amplitude normalization factor in sub-array 1: 1.03767 ! Telescope amplitude corrections in sub-array 1: ! BR 0.91 FD 0.84 HN 1.00* KP 0.98 ! LA 1.05 MK 0.88 NL 1.00* OV 0.96 ! PT 1.05 SC 0.97 ! ! ! 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=0.159669Jy sigma=0.001250 ! Fit after self-cal, rms=0.158491Jy sigma=0.001249 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=0.158491Jy sigma=0.001249 ! Fit after self-cal, rms=0.158491Jy sigma=0.001249 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.9671 mas, bmaj=2.395 mas, bpa=10.88 degrees ! Estimated noise=871.743 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 = 0.000315178 Jy ! Component: 100 - total flux cleaned = 0.000351777 Jy ! Component: 150 - total flux cleaned = 0.000350558 Jy ! Component: 200 - total flux cleaned = 0.000324319 Jy ! Total flux subtracted in 200 components = 0.000324319 Jy ! Clean residual min=-0.004481 max=0.004106 Jy/beam ! Clean residual mean=0.000075 rms=0.001312 Jy/beam ! Combined flux in latest and established models = 0.11726 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 12 model components to the UV plane model. ! The established model now contains 37 components and 0.11726 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.158475Jy sigma=0.001249 ! Fit after self-cal, rms=0.158472Jy sigma=0.001249 ! 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=0.158472Jy sigma=0.001249 ! Fit after self-cal, rms=0.157341Jy sigma=0.001239 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 = 0.00134867 Jy ! Component: 100 - total flux cleaned = 0.0013466 Jy ! Component: 150 - total flux cleaned = 0.00130248 Jy ! Component: 200 - total flux cleaned = 0.00129988 Jy ! Total flux subtracted in 200 components = 0.00129988 Jy ! Clean residual min=-0.004696 max=0.003667 Jy/beam ! Clean residual mean=0.000075 rms=0.001259 Jy/beam ! Combined flux in latest and established models = 0.11856 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 8 model components to the UV plane model. ! The established model now contains 40 components and 0.11856 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.157303Jy sigma=0.001239 ! Fit after self-cal, rms=0.157099Jy sigma=0.001237 ! 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: 0.9671 x 2.395 at 10.88 degrees (North through East) ! Clean map min=-0.0043896 max=0.099644 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=3.045 mas, bmaj=9.752 mas, bpa=14.79 degrees ! Estimated noise=1050.23 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 = -0.000200971 Jy ! Component: 100 - total flux cleaned = -0.0002309 Jy ! Component: 150 - total flux cleaned = -0.000289168 Jy ! Component: 200 - total flux cleaned = -0.000343757 Jy ! Total flux subtracted in 200 components = -0.000343757 Jy ! Clean residual min=-0.005009 max=0.004003 Jy/beam ! Clean residual mean=0.000121 rms=0.001645 Jy/beam ! Combined flux in latest and established models = 0.118216 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 6 model components to the UV plane model. ! The established model now contains 44 components and 0.118216 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.157093Jy sigma=0.001237 ! Fit after self-cal, rms=0.157043Jy sigma=0.001237 ! 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=0.6551 mas, bmaj=1.704 mas, bpa=8.902 degrees ! Estimated noise=1833.31 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0812786 Jy ! Component: 100 - total flux cleaned = 0.104664 Jy ! Component: 150 - total flux cleaned = 0.114699 Jy ! Component: 200 - total flux cleaned = 0.116731 Jy ! Total flux subtracted in 200 components = 0.116731 Jy ! Clean residual min=-0.009980 max=0.010004 Jy/beam ! Clean residual mean=0.000031 rms=0.002516 Jy/beam ! Combined flux in latest and established models = 0.116731 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 18 model components to the UV plane model. ! The established model now contains 18 components and 0.116731 Jy ! Inverting map and beam ! Estimated beam: bmin=0.9671 mas, bmaj=2.395 mas, bpa=10.88 degrees ! Estimated noise=871.743 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 = 0.00260066 Jy ! Component: 100 - total flux cleaned = 0.00245431 Jy ! Component: 150 - total flux cleaned = 0.00228466 Jy ! Component: 200 - total flux cleaned = 0.00210412 Jy ! Total flux subtracted in 200 components = 0.00210412 Jy ! Clean residual min=-0.004518 max=0.003974 Jy/beam ! Clean residual mean=0.000075 rms=0.001237 Jy/beam ! Combined flux in latest and established models = 0.118835 Jy ! Adding 8 model components to the UV plane model. ! The established model now contains 25 components and 0.118835 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=3.045 mas, bmaj=9.752 mas, bpa=14.79 degrees ! Estimated noise=1050.23 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 = -0.000391277 Jy ! Component: 100 - total flux cleaned = -0.000452972 Jy ! Component: 150 - total flux cleaned = -0.00051124 Jy ! Component: 200 - total flux cleaned = -0.000565279 Jy ! Total flux subtracted in 200 components = -0.000565279 Jy ! Clean residual min=-0.005009 max=0.004009 Jy/beam ! Clean residual mean=0.000121 rms=0.001641 Jy/beam ! Combined flux in latest and established models = 0.118269 Jy ! Adding 5 model components to the UV plane model. ! The established model now contains 29 components and 0.118269 Jy ! Inverting map uvtaper 0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=0.9671 mas, bmaj=2.395 mas, bpa=10.88 degrees ! Estimated noise=871.743 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000173942 Jy ! Component: 100 - total flux cleaned = 0.000144448 Jy ! Component: 150 - total flux cleaned = 0.000119583 Jy ! Component: 200 - total flux cleaned = 0.000118575 Jy ! Total flux subtracted in 200 components = 0.000118575 Jy ! Clean residual min=-0.004439 max=0.003947 Jy/beam ! Clean residual mean=0.000074 rms=0.001227 Jy/beam ! Combined flux in latest and established models = 0.118388 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 13 model components to the UV plane model. ! The established model now contains 34 components and 0.118388 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.157012Jy sigma=0.001236 ! Fit after self-cal, rms=0.156996Jy sigma=0.001236 wmodel J0350-3232_X_2002_01_31_yyk\_map.mod ! Writing 34 model components to file: J0350-3232_X_2002_01_31_yyk_map.mod wobs J0350-3232_X_2002_01_31_yyk\_uvs.fits ! Applying 96 buffered edits. ! Writing UV FITS file: J0350-3232_X_2002_01_31_yyk_uvs.fits wwins J0350-3232_X_2002_01_31_yyk\_map.win ! wwins: Wrote 1 windows to J0350-3232_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 = -0.0011988 Jy ! Component: 100 - total flux cleaned = -0.00167263 Jy ! Component: 150 - total flux cleaned = -0.00192062 Jy ! Component: 200 - total flux cleaned = -0.00203813 Jy ! Component: 250 - total flux cleaned = -0.00182209 Jy ! Component: 300 - total flux cleaned = -0.00177085 Jy ! Component: 350 - total flux cleaned = -0.00157262 Jy ! Component: 400 - total flux cleaned = -0.00133356 Jy ! Component: 450 - total flux cleaned = -0.00101209 Jy ! Component: 500 - total flux cleaned = -0.000702517 Jy ! Component: 550 - total flux cleaned = -0.000615484 Jy ! Component: 600 - total flux cleaned = -0.000446336 Jy ! Component: 650 - total flux cleaned = -7.81063e-05 Jy ! Component: 700 - total flux cleaned = -3.99774e-05 Jy ! Component: 750 - total flux cleaned = 0.000115599 Jy ! Component: 800 - total flux cleaned = 0.000192506 Jy ! Component: 850 - total flux cleaned = 0.000419043 Jy ! Component: 900 - total flux cleaned = 0.000603519 Jy ! Component: 950 - total flux cleaned = 0.000965611 Jy ! Component: 1000 - total flux cleaned = 0.00121419 Jy ! Component: 1050 - total flux cleaned = 0.00152897 Jy ! Component: 1100 - total flux cleaned = 0.00176948 Jy ! Component: 1150 - total flux cleaned = 0.00193906 Jy ! Component: 1200 - total flux cleaned = 0.0022391 Jy ! Component: 1250 - total flux cleaned = 0.00243589 Jy ! Component: 1300 - total flux cleaned = 0.0026953 Jy ! Component: 1350 - total flux cleaned = 0.00304668 Jy ! Component: 1400 - total flux cleaned = 0.00329924 Jy ! Component: 1450 - total flux cleaned = 0.00361009 Jy ! Component: 1500 - total flux cleaned = 0.00388599 Jy ! Component: 1550 - total flux cleaned = 0.00421915 Jy ! Component: 1600 - total flux cleaned = 0.00448761 Jy ! Component: 1650 - total flux cleaned = 0.00469477 Jy ! Component: 1700 - total flux cleaned = 0.00504564 Jy ! Component: 1750 - total flux cleaned = 0.00530474 Jy ! Component: 1800 - total flux cleaned = 0.00553289 Jy ! Component: 1850 - total flux cleaned = 0.00570286 Jy ! Component: 1900 - total flux cleaned = 0.0059823 Jy ! Component: 1950 - total flux cleaned = 0.00612106 Jy ! Component: 2000 - total flux cleaned = 0.00628572 Jy ! Total flux subtracted in 2048 components = 0.00639441 Jy ! Clean residual min=-0.001419 max=0.001524 Jy/beam ! Clean residual mean=0.000048 rms=0.000538 Jy/beam ! Combined flux in latest and established models = 0.124782 Jy keep ! Adding 135 model components to the UV plane model. ! The established model now contains 169 components and 0.124782 Jy ![Exited script file: muppet] wmap "J0350-3232_X_2002_01_31_yyk\_map.fits" ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9671 x 2.395 at 10.88 degrees (North through East) ! Clean map min=-0.002631 max=0.099735 Jy/beam ! Writing clean map to FITS file: J0350-3232_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 0.0997354 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000520995 device "J0350-3232_X_2002_01_31_yyk\_map.eps/VPS" ! Attempting to open device: 'J0350-3232_X_2002_01_31_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.56713 1.56713 3.13426 6.26853 12.5371 25.0741 50.1482 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0015 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.099 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9671 x 2.395 at 10.88 degrees (North through East) ! Clean map min=-0.002631 max=0.099735 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0350-3232_X_2002_01_31_yyk\_map.gif/gif" ! Attempting to open device: 'J0350-3232_X_2002_01_31_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J0350-3232_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 10:47:37 2007