! Started logfile: J0005-3445_X_2002_01_31_yyk_uvs.log on Wed Jun 27 10:41:51 2007 obs J0005-3445_X_2002_01_31_yyk_uva.fits ! Reading UV FITS file: J0005-3445_X_2002_01_31_yyk_uva.fits ! AN table 1: 73 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.675495 visibilities/baseline/integration-bin. ! Found source: J0005-3445 ! ! 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 8876 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 J0005-3445_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)= 0.245023 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=0.6492 mas, bmaj=1.575 mas, bpa=4.364 degrees ! Estimated noise=2225.4 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 = 0.0684911 Jy ! Component: 100 - total flux cleaned = 0.0854666 Jy ! Total flux subtracted in 100 components = 0.0854666 Jy ! Clean residual min=-0.016201 max=0.016743 Jy/beam ! Clean residual mean=0.000026 rms=0.003951 Jy/beam ! Combined flux in latest and established models = 0.0854666 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 12 model components to the UV plane model. ! The established model now contains 12 components and 0.0854666 Jy ! ! Correcting IF 1. ! A total of 165 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 165 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 165 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 165 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.231630Jy sigma=0.001448 ! Fit after self-cal, rms=0.230694Jy sigma=0.001441 ! Inverting map and beam ! Estimated beam: bmin=0.6492 mas, bmaj=1.575 mas, bpa=4.364 degrees ! Estimated noise=2225.4 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=0.8542 mas, bmaj=2.128 mas, bpa=4.122 degrees ! Estimated noise=1117.35 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 = 0.00988955 Jy ! Component: 100 - total flux cleaned = 0.0105801 Jy ! Component: 150 - total flux cleaned = 0.0105809 Jy ! Component: 200 - total flux cleaned = 0.0104968 Jy ! Total flux subtracted in 200 components = 0.0104968 Jy ! Clean residual min=-0.007038 max=0.008455 Jy/beam ! Clean residual mean=0.000044 rms=0.001987 Jy/beam ! Combined flux in latest and established models = 0.0959634 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 14 model components to the UV plane model. ! The established model now contains 23 components and 0.0959634 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.230556Jy sigma=0.001439 ! Fit after self-cal, rms=0.230547Jy sigma=0.001439 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8542 x 2.128 at 4.122 degrees (North through East) ! Clean map min=-0.0062421 max=0.084024 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=0.230547Jy sigma=0.001439 ! Fit after self-cal, rms=0.230547Jy sigma=0.001439 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=0.230547Jy sigma=0.001439 ! Fit after self-cal, rms=0.230547Jy sigma=0.001439 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.8542 mas, bmaj=2.128 mas, bpa=4.122 degrees ! Estimated noise=1117.35 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 = 0.000141415 Jy ! Component: 100 - total flux cleaned = 6.29062e-05 Jy ! Component: 150 - total flux cleaned = -5.98486e-06 Jy ! Component: 200 - total flux cleaned = -6.97625e-05 Jy ! Total flux subtracted in 200 components = -6.97625e-05 Jy ! Clean residual min=-0.006856 max=0.008296 Jy/beam ! Clean residual mean=0.000044 rms=0.001970 Jy/beam ! Combined flux in latest and established models = 0.0958937 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 7 model components to the UV plane model. ! The established model now contains 25 components and 0.0958937 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.230515Jy sigma=0.001438 ! Fit after self-cal, rms=0.230510Jy sigma=0.001438 ! 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=0.230510Jy sigma=0.001438 ! Fit after self-cal, rms=0.227899Jy sigma=0.001422 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) ! Added new window around map position (-7.4, -24.2). ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0088461 Jy ! Component: 100 - total flux cleaned = 0.00882683 Jy ! Component: 150 - total flux cleaned = 0.00882232 Jy ! Component: 200 - total flux cleaned = 0.00861168 Jy ! Total flux subtracted in 200 components = 0.00861168 Jy ! Clean residual min=-0.005402 max=0.006794 Jy/beam ! Clean residual mean=0.000030 rms=0.001729 Jy/beam ! Combined flux in latest and established models = 0.104505 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 22 model components to the UV plane model. ! The established model now contains 45 components and 0.104505 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.227634Jy sigma=0.001420 ! Fit after self-cal, rms=0.227228Jy sigma=0.001417 ! 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: 0.8542 x 2.128 at 4.122 degrees (North through East) ! Clean map min=-0.0053602 max=0.089561 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=2.942 mas, bmaj=9.088 mas, bpa=11.27 degrees ! Estimated noise=1425.84 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 = 0.000262885 Jy ! Component: 100 - total flux cleaned = 0.000261363 Jy ! Component: 150 - total flux cleaned = 0.000187771 Jy ! Component: 200 - total flux cleaned = 8.26881e-05 Jy ! Total flux subtracted in 200 components = 8.26881e-05 Jy ! Clean residual min=-0.006243 max=0.006469 Jy/beam ! Clean residual mean=0.000053 rms=0.002163 Jy/beam ! Combined flux in latest and established models = 0.104588 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 16 model components to the UV plane model. ! The established model now contains 60 components and 0.104588 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.227214Jy sigma=0.001417 ! Fit after self-cal, rms=0.227143Jy sigma=0.001417 ! 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=0.6492 mas, bmaj=1.575 mas, bpa=4.364 degrees ! Estimated noise=2225.4 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0773164 Jy ! Component: 100 - total flux cleaned = 0.0940935 Jy ! Component: 150 - total flux cleaned = 0.0992907 Jy ! Component: 200 - total flux cleaned = 0.101896 Jy ! Total flux subtracted in 200 components = 0.101896 Jy ! Clean residual min=-0.011604 max=0.012509 Jy/beam ! Clean residual mean=0.000005 rms=0.003483 Jy/beam ! Combined flux in latest and established models = 0.101896 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 19 model components to the UV plane model. ! The established model now contains 19 components and 0.101896 Jy ! Inverting map and beam ! Estimated beam: bmin=0.8542 mas, bmaj=2.128 mas, bpa=4.122 degrees ! Estimated noise=1117.35 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 = 0.00587885 Jy ! Component: 100 - total flux cleaned = 0.0063383 Jy ! Component: 150 - total flux cleaned = 0.00601614 Jy ! Component: 200 - total flux cleaned = 0.00561253 Jy ! Total flux subtracted in 200 components = 0.00561253 Jy ! Clean residual min=-0.006233 max=0.006379 Jy/beam ! Clean residual mean=0.000028 rms=0.001739 Jy/beam ! Combined flux in latest and established models = 0.107508 Jy ! Adding 13 model components to the UV plane model. ! The established model now contains 32 components and 0.107508 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=2.942 mas, bmaj=9.088 mas, bpa=11.27 degrees ! Estimated noise=1425.84 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 = -0.00168817 Jy ! Component: 100 - total flux cleaned = -0.00191501 Jy ! Component: 150 - total flux cleaned = -0.00210808 Jy ! Component: 200 - total flux cleaned = -0.00223729 Jy ! Total flux subtracted in 200 components = -0.00223729 Jy ! Clean residual min=-0.006570 max=0.006526 Jy/beam ! Clean residual mean=0.000054 rms=0.002217 Jy/beam ! Combined flux in latest and established models = 0.105271 Jy ! Adding 8 model components to the UV plane model. ! The established model now contains 40 components and 0.105271 Jy ! Inverting map uvtaper 0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=0.8542 mas, bmaj=2.128 mas, bpa=4.122 degrees ! Estimated noise=1117.35 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000815773 Jy ! Component: 100 - total flux cleaned = 0.000914318 Jy ! Component: 150 - total flux cleaned = 0.000833562 Jy ! Component: 200 - total flux cleaned = 0.000831766 Jy ! Total flux subtracted in 200 components = 0.000831766 Jy ! Clean residual min=-0.006111 max=0.006233 Jy/beam ! Clean residual mean=0.000028 rms=0.001705 Jy/beam ! Combined flux in latest and established models = 0.106103 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 49 components and 0.106103 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.227080Jy sigma=0.001417 ! Fit after self-cal, rms=0.227004Jy sigma=0.001416 wmodel J0005-3445_X_2002_01_31_yyk\_map.mod ! Writing 49 model components to file: J0005-3445_X_2002_01_31_yyk_map.mod wobs J0005-3445_X_2002_01_31_yyk\_uvs.fits ! Applying 73 buffered edits. ! Writing UV FITS file: J0005-3445_X_2002_01_31_yyk_uvs.fits wwins J0005-3445_X_2002_01_31_yyk\_map.win ! wwins: Wrote 2 windows to J0005-3445_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 = 0.00119365 Jy ! Component: 100 - total flux cleaned = 0.00191017 Jy ! Component: 150 - total flux cleaned = 0.00287118 Jy ! Component: 200 - total flux cleaned = 0.00360045 Jy ! Component: 250 - total flux cleaned = 0.00421066 Jy ! Component: 300 - total flux cleaned = 0.0047118 Jy ! Component: 350 - total flux cleaned = 0.00519719 Jy ! Component: 400 - total flux cleaned = 0.00582343 Jy ! Component: 450 - total flux cleaned = 0.00620089 Jy ! Component: 500 - total flux cleaned = 0.00656722 Jy ! Component: 550 - total flux cleaned = 0.00671176 Jy ! Component: 600 - total flux cleaned = 0.00705993 Jy ! Component: 650 - total flux cleaned = 0.00733131 Jy ! Component: 700 - total flux cleaned = 0.00766215 Jy ! Component: 750 - total flux cleaned = 0.00785335 Jy ! Component: 800 - total flux cleaned = 0.00810499 Jy ! Component: 850 - total flux cleaned = 0.00816676 Jy ! Component: 900 - total flux cleaned = 0.00834766 Jy ! Component: 950 - total flux cleaned = 0.00834653 Jy ! Component: 1000 - total flux cleaned = 0.00834641 Jy ! Component: 1050 - total flux cleaned = 0.00840265 Jy ! Component: 1100 - total flux cleaned = 0.00845805 Jy ! Component: 1150 - total flux cleaned = 0.00834896 Jy ! Component: 1200 - total flux cleaned = 0.00845799 Jy ! Component: 1250 - total flux cleaned = 0.00861547 Jy ! Component: 1300 - total flux cleaned = 0.00856164 Jy ! Component: 1350 - total flux cleaned = 0.00861251 Jy ! Component: 1400 - total flux cleaned = 0.00876423 Jy ! Component: 1450 - total flux cleaned = 0.0088637 Jy ! Component: 1500 - total flux cleaned = 0.00891323 Jy ! Component: 1550 - total flux cleaned = 0.00905881 Jy ! Component: 1600 - total flux cleaned = 0.00915449 Jy ! Component: 1650 - total flux cleaned = 0.00929517 Jy ! Component: 1700 - total flux cleaned = 0.00938716 Jy ! Component: 1750 - total flux cleaned = 0.00934123 Jy ! Component: 1800 - total flux cleaned = 0.00929601 Jy ! Component: 1850 - total flux cleaned = 0.00938597 Jy ! Component: 1900 - total flux cleaned = 0.00938579 Jy ! Component: 1950 - total flux cleaned = 0.0092987 Jy ! Component: 2000 - total flux cleaned = 0.0093848 Jy ! Total flux subtracted in 2048 components = 0.00929911 Jy ! Clean residual min=-0.002684 max=0.003047 Jy/beam ! Clean residual mean=0.000007 rms=0.000806 Jy/beam ! Combined flux in latest and established models = 0.115402 Jy keep ! Adding 121 model components to the UV plane model. ! The established model now contains 170 components and 0.115402 Jy ![Exited script file: muppet] wmap "J0005-3445_X_2002_01_31_yyk\_map.fits" ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8542 x 2.128 at 4.122 degrees (North through East) ! Clean map min=-0.0058718 max=0.086425 Jy/beam ! Writing clean map to FITS file: J0005-3445_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 0.0864246 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00080129 device "J0005-3445_X_2002_01_31_yyk\_map.eps/VPS" ! Attempting to open device: 'J0005-3445_X_2002_01_31_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -2.78147 2.78147 5.56293 11.1259 22.2517 44.5035 89.0069 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0024 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.086 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8542 x 2.128 at 4.122 degrees (North through East) ! Clean map min=-0.0058718 max=0.086425 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0005-3445_X_2002_01_31_yyk\_map.gif/gif" ! Attempting to open device: 'J0005-3445_X_2002_01_31_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J0005-3445_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 10:41:58 2007