! Started logfile: J2222-1144_X_2005_05_12_yyk_uvs.log on Sat Oct 8 17:45:02 2005 obs J2222-1144_X_2005_05_12_yyk_uve.fits ! Reading UV FITS file: J2222-1144_X_2005_05_12_yyk_uve.fits ! AN table 1: 8 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.883333 visibilities/baseline/integration-bin. ! Found source: J2222-1144 ! ! 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 1272 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 J2222-1144_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)= 0.108493 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=0.8085 mas, bmaj=1.897 mas, bpa=3.266 degrees ! Estimated noise=2.45101 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 = 0.0612387 Jy ! Component: 100 - total flux cleaned = 0.0753353 Jy ! Total flux subtracted in 100 components = 0.0753353 Jy ! Clean residual min=-0.010191 max=0.010477 Jy/beam ! Clean residual mean=0.000035 rms=0.002921 Jy/beam ! Combined flux in latest and established models = 0.0753353 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 16 model components to the UV plane model. ! The established model now contains 16 components and 0.0753353 Jy ! ! Correcting IF 1. ! A total of 14 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 12 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 46 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 35 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.078282Jy sigma=1.224886 ! Fit after self-cal, rms=0.072856Jy sigma=1.137547 ! Inverting map and beam ! Estimated beam: bmin=0.8085 mas, bmaj=1.897 mas, bpa=3.266 degrees ! Estimated noise=2.45101 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=1.062 mas, bmaj=2.455 mas, bpa=8.089 degrees ! Estimated noise=1.53483 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 = 0.0150361 Jy ! Component: 100 - total flux cleaned = 0.0191851 Jy ! Component: 150 - total flux cleaned = 0.0200484 Jy ! Component: 200 - total flux cleaned = 0.0201862 Jy ! Total flux subtracted in 200 components = 0.0201862 Jy ! Clean residual min=-0.005158 max=0.005431 Jy/beam ! Clean residual mean=0.000036 rms=0.001537 Jy/beam ! Combined flux in latest and established models = 0.0955215 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 22 model components to the UV plane model. ! The established model now contains 35 components and 0.0955215 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.071696Jy sigma=1.094606 ! Fit after self-cal, rms=0.071673Jy sigma=1.094521 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.062 x 2.455 at 8.089 degrees (North through East) ! Clean map min=-0.0050262 max=0.081047 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=0.071673Jy sigma=1.094521 ! Fit after self-cal, rms=0.071673Jy sigma=1.094521 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=0.071673Jy sigma=1.094521 ! Fit after self-cal, rms=0.071674Jy sigma=1.094521 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=1.062 mas, bmaj=2.455 mas, bpa=8.089 degrees ! Estimated noise=1.53483 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 = 4.70957e-05 Jy ! Component: 100 - total flux cleaned = 9.00294e-05 Jy ! Component: 150 - total flux cleaned = 0.000164735 Jy ! Component: 200 - total flux cleaned = 0.000199576 Jy ! Total flux subtracted in 200 components = 0.000199576 Jy ! Clean residual min=-0.005196 max=0.005446 Jy/beam ! Clean residual mean=0.000036 rms=0.001524 Jy/beam ! Combined flux in latest and established models = 0.0957211 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 36 components and 0.0957211 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.071643Jy sigma=1.093871 ! Fit after self-cal, rms=0.071628Jy sigma=1.093773 ! 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=0.071628Jy sigma=1.093773 ! Fit after self-cal, rms=0.065496Jy sigma=1.008806 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 = 0.0029951 Jy ! Component: 100 - total flux cleaned = 0.0029303 Jy ! Component: 150 - total flux cleaned = 0.00287378 Jy ! Component: 200 - total flux cleaned = 0.00273544 Jy ! Total flux subtracted in 200 components = 0.00273544 Jy ! Clean residual min=-0.004743 max=0.005385 Jy/beam ! Clean residual mean=0.000027 rms=0.001447 Jy/beam ! Combined flux in latest and established models = 0.0984565 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 42 components and 0.0984565 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.065449Jy sigma=1.005709 ! Fit after self-cal, rms=0.064751Jy sigma=0.999951 ! 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: 1.062 x 2.455 at 8.089 degrees (North through East) ! Clean map min=-0.0046076 max=0.084653 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=2.55 mas, bmaj=5.135 mas, bpa=16.36 degrees ! Estimated noise=1.80076 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 = 0.000787104 Jy ! Component: 100 - total flux cleaned = 0.00094461 Jy ! Component: 150 - total flux cleaned = 0.00105301 Jy ! Component: 200 - total flux cleaned = 0.00110976 Jy ! Total flux subtracted in 200 components = 0.00110976 Jy ! Clean residual min=-0.004785 max=0.005078 Jy/beam ! Clean residual mean=0.000042 rms=0.001515 Jy/beam ! Combined flux in latest and established models = 0.0995663 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 5 model components to the UV plane model. ! The established model now contains 43 components and 0.0995663 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.064760Jy sigma=0.999933 ! Fit after self-cal, rms=0.064548Jy sigma=0.998804 ! 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=0.8085 mas, bmaj=1.897 mas, bpa=3.266 degrees ! Estimated noise=2.45101 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0713763 Jy ! Component: 100 - total flux cleaned = 0.0870909 Jy ! Component: 150 - total flux cleaned = 0.0939119 Jy ! Component: 200 - total flux cleaned = 0.0959002 Jy ! Total flux subtracted in 200 components = 0.0959002 Jy ! Clean residual min=-0.007962 max=0.008496 Jy/beam ! Clean residual mean=0.000009 rms=0.002156 Jy/beam ! Combined flux in latest and established models = 0.0959003 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 30 model components to the UV plane model. ! The established model now contains 30 components and 0.0959003 Jy ! Inverting map and beam ! Estimated beam: bmin=1.062 mas, bmaj=2.455 mas, bpa=8.089 degrees ! Estimated noise=1.53483 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 = 0.00250732 Jy ! Component: 100 - total flux cleaned = 0.00290913 Jy ! Component: 150 - total flux cleaned = 0.00291689 Jy ! Component: 200 - total flux cleaned = 0.00286806 Jy ! Total flux subtracted in 200 components = 0.00286806 Jy ! Clean residual min=-0.004653 max=0.005088 Jy/beam ! Clean residual mean=0.000026 rms=0.001432 Jy/beam ! Combined flux in latest and established models = 0.0987683 Jy ! Adding 9 model components to the UV plane model. ! The established model now contains 36 components and 0.0987683 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=2.55 mas, bmaj=5.135 mas, bpa=16.36 degrees ! Estimated noise=1.80076 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 = 0.000509324 Jy ! Component: 100 - total flux cleaned = 0.000664631 Jy ! Component: 150 - total flux cleaned = 0.000739841 Jy ! Component: 200 - total flux cleaned = 0.000799978 Jy ! Total flux subtracted in 200 components = 0.000799978 Jy ! Clean residual min=-0.004709 max=0.005036 Jy/beam ! Clean residual mean=0.000041 rms=0.001507 Jy/beam ! Combined flux in latest and established models = 0.0995683 Jy ! Adding 5 model components to the UV plane model. ! The established model now contains 39 components and 0.0995683 Jy ! Inverting map uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=1.062 mas, bmaj=2.455 mas, bpa=8.089 degrees ! Estimated noise=1.53483 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.000854643 Jy ! Component: 100 - total flux cleaned = -0.00095554 Jy ! Component: 150 - total flux cleaned = -0.000998897 Jy ! Component: 200 - total flux cleaned = -0.00103789 Jy ! Total flux subtracted in 200 components = -0.00103789 Jy ! Clean residual min=-0.004707 max=0.005104 Jy/beam ! Clean residual mean=0.000026 rms=0.001403 Jy/beam ! Combined flux in latest and established models = 0.0985304 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 43 components and 0.0985304 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.064522Jy sigma=0.997535 ! Fit after self-cal, rms=0.064414Jy sigma=0.997137 wmodel J2222-1144_X_2005_05_12_yyk\_map.mod ! Writing 43 model components to file: J2222-1144_X_2005_05_12_yyk_map.mod wobs J2222-1144_X_2005_05_12_yyk\_uvs.fits ! Writing UV FITS file: J2222-1144_X_2005_05_12_yyk_uvs.fits wwins J2222-1144_X_2005_05_12_yyk\_map.win ! wwins: Wrote 1 windows to J2222-1144_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 = 0.00203604 Jy ! Component: 100 - total flux cleaned = 0.00270586 Jy ! Component: 150 - total flux cleaned = 0.00309059 Jy ! Component: 200 - total flux cleaned = 0.00287807 Jy ! Component: 250 - total flux cleaned = 0.00267151 Jy ! Component: 300 - total flux cleaned = 0.00253579 Jy ! Component: 350 - total flux cleaned = 0.00253345 Jy ! Component: 400 - total flux cleaned = 0.00265651 Jy ! Component: 450 - total flux cleaned = 0.00265653 Jy ! Component: 500 - total flux cleaned = 0.00265728 Jy ! Component: 550 - total flux cleaned = 0.00282877 Jy ! Component: 600 - total flux cleaned = 0.00310697 Jy ! Component: 650 - total flux cleaned = 0.00337984 Jy ! Component: 700 - total flux cleaned = 0.00364546 Jy ! Component: 750 - total flux cleaned = 0.00369581 Jy ! Component: 800 - total flux cleaned = 0.00389972 Jy ! Component: 850 - total flux cleaned = 0.00379957 Jy ! Component: 900 - total flux cleaned = 0.00394728 Jy ! Component: 950 - total flux cleaned = 0.00404309 Jy ! Component: 1000 - total flux cleaned = 0.0041848 Jy ! Component: 1050 - total flux cleaned = 0.00437041 Jy ! Component: 1100 - total flux cleaned = 0.00464486 Jy ! Component: 1150 - total flux cleaned = 0.00482434 Jy ! Component: 1200 - total flux cleaned = 0.00500117 Jy ! Component: 1250 - total flux cleaned = 0.00500067 Jy ! Component: 1300 - total flux cleaned = 0.00513044 Jy ! Component: 1350 - total flux cleaned = 0.00534191 Jy ! Component: 1400 - total flux cleaned = 0.00542529 Jy ! Component: 1450 - total flux cleaned = 0.00563153 Jy ! Component: 1500 - total flux cleaned = 0.00571276 Jy ! Component: 1550 - total flux cleaned = 0.00591364 Jy ! Component: 1600 - total flux cleaned = 0.00611155 Jy ! Component: 1650 - total flux cleaned = 0.00615033 Jy ! Component: 1700 - total flux cleaned = 0.0062277 Jy ! Component: 1750 - total flux cleaned = 0.00638034 Jy ! Component: 1800 - total flux cleaned = 0.00645624 Jy ! Component: 1850 - total flux cleaned = 0.00660535 Jy ! Component: 1900 - total flux cleaned = 0.00664175 Jy ! Component: 1950 - total flux cleaned = 0.00667784 Jy ! Component: 2000 - total flux cleaned = 0.0066417 Jy ! Total flux subtracted in 2048 components = 0.00667762 Jy ! Clean residual min=-0.002037 max=0.002590 Jy/beam ! Clean residual mean=0.000007 rms=0.000681 Jy/beam ! Combined flux in latest and established models = 0.105208 Jy keep ! Adding 137 model components to the UV plane model. ! The established model now contains 180 components and 0.105208 Jy ![Exited script file: muppet] wmap "J2222-1144_X_2005_05_12_yyk\_map.fits" ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.062 x 2.455 at 8.089 degrees (North through East) ! Clean map min=-0.003167 max=0.084501 Jy/beam ! Writing clean map to FITS file: J2222-1144_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 0.0845008 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000668319 device "J2222-1144_X_2005_05_12_yyk\_map.eps/VPS" ! Attempting to open device: 'J2222-1144_X_2005_05_12_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -2.37271 2.37271 4.74542 9.49083 18.9817 37.9633 75.9267 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.002 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.084 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.062 x 2.455 at 8.089 degrees (North through East) ! Clean map min=-0.003167 max=0.084501 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J2222-1144_X_2005_05_12_yyk\_map.gif/gif" ! Attempting to open device: 'J2222-1144_X_2005_05_12_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J2222-1144_X_2005_05_12_yyk_uvs.log closed on Sat Oct 8 17:45:05 2005