! Started logfile: J1639+8631_X_2006_02_14_yyk_uvs.log on Wed Jul 5 13:00:05 2006 obs J1639+8631_X_2006_02_14_yyk_uva.fits ! Reading UV FITS file: J1639+8631_X_2006_02_14_yyk_uva.fits ! AN table 1: 878 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.724196 visibilities/baseline/integration-bin. ! Found source: J1639+8631 ! ! 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 2310 lines of history. ! ! Reading 114452 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 J1639+8631_X_2006_02_14_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. uvav time_av, true ! Averaging into 30 second bins. ! 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 phase_soltime=phase_soltime1 print "uvstat(rms)=",uvstat(rms),"Jy" ! uvstat(rms)= 0.0861373 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=0.677 mas, bmaj=2.738 mas, bpa=11.6 degrees ! Estimated noise=1.46473 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 = 0.0484866 Jy ! Component: 100 - total flux cleaned = 0.0602885 Jy ! Total flux subtracted in 100 components = 0.0602885 Jy ! Clean residual min=-0.008449 max=0.008677 Jy/beam ! Clean residual mean=-0.000002 rms=0.002231 Jy/beam ! Combined flux in latest and established models = 0.0602885 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 10 components and 0.0602885 Jy ! ! Correcting IF 1. ! A total of 22 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 38 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 38 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 54 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.058714Jy sigma=1.143048 ! Fit after self-cal, rms=0.058702Jy sigma=1.142428 ! Inverting map and beam ! Estimated beam: bmin=0.677 mas, bmaj=2.738 mas, bpa=11.6 degrees ! Estimated noise=1.46473 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=0.8996 mas, bmaj=2.787 mas, bpa=9.622 degrees ! Estimated noise=0.863326 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 = 0.0114507 Jy ! Component: 100 - total flux cleaned = 0.0176711 Jy ! Component: 150 - total flux cleaned = 0.0216891 Jy ! Component: 200 - total flux cleaned = 0.0243662 Jy ! Total flux subtracted in 200 components = 0.0243662 Jy ! Clean residual min=-0.007478 max=0.008944 Jy/beam ! Clean residual mean=-0.000006 rms=0.002246 Jy/beam ! Combined flux in latest and established models = 0.0846547 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 46 model components to the UV plane model. ! The established model now contains 50 components and 0.0846547 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.056937Jy sigma=1.106626 ! Fit after self-cal, rms=0.056932Jy sigma=1.106259 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8996 x 2.787 at 9.622 degrees (North through East) ! Clean map min=-0.0072584 max=0.059648 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: 1.04092 ! Telescope amplitude corrections in sub-array 1: ! BR 0.85 FD 0.92 HN 0.89 KP 0.92 ! LA 0.90 MK 1.06 NL 1.15 OV 0.92 ! 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=0.056932Jy sigma=1.106259 ! Fit after self-cal, rms=0.056576Jy sigma=1.101903 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=0.056576Jy sigma=1.101903 ! Fit after self-cal, rms=0.056587Jy sigma=1.101837 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.9132 mas, bmaj=2.768 mas, bpa=9.177 degrees ! Estimated noise=0.854808 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 = 0.00206125 Jy ! Component: 100 - total flux cleaned = 0.00308187 Jy ! Component: 150 - total flux cleaned = 0.00336653 Jy ! Component: 200 - total flux cleaned = 0.00340015 Jy ! Total flux subtracted in 200 components = 0.00340015 Jy ! Clean residual min=-0.007218 max=0.008359 Jy/beam ! Clean residual mean=-0.000002 rms=0.002146 Jy/beam ! Combined flux in latest and established models = 0.0880548 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 16 model components to the UV plane model. ! The established model now contains 56 components and 0.0880548 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.056507Jy sigma=1.100463 ! Fit after self-cal, rms=0.056517Jy sigma=1.100458 ! 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=0.056517Jy sigma=1.100458 ! Fit after self-cal, rms=0.053350Jy sigma=1.032354 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 = 0.00230929 Jy ! Component: 100 - total flux cleaned = 0.00275879 Jy ! Component: 150 - total flux cleaned = 0.00285713 Jy ! Component: 200 - total flux cleaned = 0.00285777 Jy ! Total flux subtracted in 200 components = 0.00285777 Jy ! Clean residual min=-0.006912 max=0.007516 Jy/beam ! Clean residual mean=-0.000002 rms=0.002037 Jy/beam ! Combined flux in latest and established models = 0.0909126 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 60 components and 0.0909126 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.053111Jy sigma=1.030213 ! Fit after self-cal, rms=0.052963Jy sigma=1.026222 ! 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: 0.9132 x 2.768 at 9.177 degrees (North through East) ! Clean map min=-0.0066791 max=0.062232 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=1.925 mas, bmaj=3.225 mas, bpa=5.311 degrees ! Estimated noise=1.07352 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 = 0.00316282 Jy ! Component: 100 - total flux cleaned = 0.00291709 Jy ! Component: 150 - total flux cleaned = 0.00298736 Jy ! Component: 200 - total flux cleaned = 0.00304814 Jy ! Total flux subtracted in 200 components = 0.00304814 Jy ! Clean residual min=-0.008228 max=0.010745 Jy/beam ! Clean residual mean=-0.000002 rms=0.002729 Jy/beam ! Combined flux in latest and established models = 0.0939607 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 11 model components to the UV plane model. ! The established model now contains 65 components and 0.0939607 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.053156Jy sigma=1.030780 ! Fit after self-cal, rms=0.053071Jy sigma=1.028619 ! 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=0.6818 mas, bmaj=2.725 mas, bpa=11.37 degrees ! Estimated noise=1.46785 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0518706 Jy ! Component: 100 - total flux cleaned = 0.0630913 Jy ! Component: 150 - total flux cleaned = 0.0701559 Jy ! Component: 200 - total flux cleaned = 0.0750433 Jy ! Total flux subtracted in 200 components = 0.0750433 Jy ! Clean residual min=-0.006495 max=0.007737 Jy/beam ! Clean residual mean=-0.000001 rms=0.001869 Jy/beam ! Combined flux in latest and established models = 0.0750433 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 17 model components to the UV plane model. ! The established model now contains 17 components and 0.0750433 Jy ! Inverting map and beam ! Estimated beam: bmin=0.9132 mas, bmaj=2.768 mas, bpa=9.177 degrees ! Estimated noise=0.854808 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) ! Added new window around map position (-15.6, 13.8). ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0115622 Jy ! Component: 100 - total flux cleaned = 0.0148886 Jy ! Component: 150 - total flux cleaned = 0.0160953 Jy ! Component: 200 - total flux cleaned = 0.0166935 Jy ! Total flux subtracted in 200 components = 0.0166935 Jy ! Clean residual min=-0.005674 max=0.006358 Jy/beam ! Clean residual mean=-0.000001 rms=0.001665 Jy/beam ! Combined flux in latest and established models = 0.0917368 Jy ! Adding 29 model components to the UV plane model. ! The established model now contains 45 components and 0.0917368 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=1.925 mas, bmaj=3.225 mas, bpa=5.311 degrees ! Estimated noise=1.07352 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 = 0.00272194 Jy ! Component: 100 - total flux cleaned = 0.00301739 Jy ! Component: 150 - total flux cleaned = 0.00313604 Jy ! Component: 200 - total flux cleaned = 0.00314109 Jy ! Total flux subtracted in 200 components = 0.00314109 Jy ! Clean residual min=-0.006155 max=0.007468 Jy/beam ! Clean residual mean=-0.000001 rms=0.002060 Jy/beam ! Combined flux in latest and established models = 0.0948779 Jy ! Adding 19 model components to the UV plane model. ! The established model now contains 59 components and 0.0948779 Jy ! Inverting map uvtaper 0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=0.9132 mas, bmaj=2.768 mas, bpa=9.177 degrees ! Estimated noise=0.854808 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.00206573 Jy ! Component: 100 - total flux cleaned = -0.0019766 Jy ! Component: 150 - total flux cleaned = -0.00219301 Jy ! Component: 200 - total flux cleaned = -0.00225424 Jy ! Total flux subtracted in 200 components = -0.00225424 Jy ! Clean residual min=-0.005112 max=0.005503 Jy/beam ! Clean residual mean=0.000000 rms=0.001512 Jy/beam ! Combined flux in latest and established models = 0.0926236 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 25 model components to the UV plane model. ! The established model now contains 78 components and 0.0926236 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.051809Jy sigma=0.997063 ! Fit after self-cal, rms=0.051381Jy sigma=0.990121 wmodel J1639+8631_X_2006_02_14_yyk\_map.mod ! Writing 78 model components to file: J1639+8631_X_2006_02_14_yyk_map.mod wobs J1639+8631_X_2006_02_14_yyk\_uvs.fits ! Writing UV FITS file: J1639+8631_X_2006_02_14_yyk_uvs.fits wwins J1639+8631_X_2006_02_14_yyk\_map.win ! wwins: Wrote 2 windows to J1639+8631_X_2006_02_14_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 = 0.00175543 Jy ! Component: 100 - total flux cleaned = 0.00192632 Jy ! Component: 150 - total flux cleaned = 0.00216024 Jy ! Component: 200 - total flux cleaned = 0.00273507 Jy ! Component: 250 - total flux cleaned = 0.00321221 Jy ! Component: 300 - total flux cleaned = 0.00353509 Jy ! Component: 350 - total flux cleaned = 0.00378353 Jy ! Component: 400 - total flux cleaned = 0.00420179 Jy ! Component: 450 - total flux cleaned = 0.0044862 Jy ! Component: 500 - total flux cleaned = 0.0046517 Jy ! Component: 550 - total flux cleaned = 0.00470552 Jy ! Component: 600 - total flux cleaned = 0.00481125 Jy ! Component: 650 - total flux cleaned = 0.00486225 Jy ! Component: 700 - total flux cleaned = 0.00505807 Jy ! Component: 750 - total flux cleaned = 0.00524495 Jy ! Component: 800 - total flux cleaned = 0.00524367 Jy ! Component: 850 - total flux cleaned = 0.00533285 Jy ! Component: 900 - total flux cleaned = 0.00537783 Jy ! Component: 950 - total flux cleaned = 0.00546232 Jy ! Component: 1000 - total flux cleaned = 0.00562659 Jy ! Component: 1050 - total flux cleaned = 0.00574624 Jy ! Component: 1100 - total flux cleaned = 0.005864 Jy ! Component: 1150 - total flux cleaned = 0.00597866 Jy ! Component: 1200 - total flux cleaned = 0.00609129 Jy ! Component: 1250 - total flux cleaned = 0.0062388 Jy ! Component: 1300 - total flux cleaned = 0.00638322 Jy ! Component: 1350 - total flux cleaned = 0.00659496 Jy ! Component: 1400 - total flux cleaned = 0.00662905 Jy ! Component: 1450 - total flux cleaned = 0.00679892 Jy ! Component: 1500 - total flux cleaned = 0.00679908 Jy ! Component: 1550 - total flux cleaned = 0.0069643 Jy ! Component: 1600 - total flux cleaned = 0.00712628 Jy ! Component: 1650 - total flux cleaned = 0.0071895 Jy ! Component: 1700 - total flux cleaned = 0.00731436 Jy ! Component: 1750 - total flux cleaned = 0.00743715 Jy ! Component: 1800 - total flux cleaned = 0.00752789 Jy ! Component: 1850 - total flux cleaned = 0.00764717 Jy ! Component: 1900 - total flux cleaned = 0.0077356 Jy ! Component: 1950 - total flux cleaned = 0.00785215 Jy ! Component: 2000 - total flux cleaned = 0.00793835 Jy ! Total flux subtracted in 2048 components = 0.00816547 Jy ! Clean residual min=-0.001646 max=0.001533 Jy/beam ! Clean residual mean=0.000001 rms=0.000540 Jy/beam ! Combined flux in latest and established models = 0.100789 Jy keep ! Adding 152 model components to the UV plane model. ! The established model now contains 230 components and 0.100789 Jy ![Exited script file: muppet] wmap "J1639+8631_X_2006_02_14_yyk\_map.fits" ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9132 x 2.768 at 9.177 degrees (North through East) ! Clean map min=-0.0033254 max=0.059074 Jy/beam ! Writing clean map to FITS file: J1639+8631_X_2006_02_14_yyk_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0590743 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00052034 device "J1639+8631_X_2006_02_14_yyk\_map.eps/VPS" ! Attempting to open device: 'J1639+8631_X_2006_02_14_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -2.64247 2.64247 5.28495 10.5699 21.1398 42.2796 84.5591 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0015 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: 0.9132 x 2.768 at 9.177 degrees (North through East) ! Clean map min=-0.0033254 max=0.059074 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1639+8631_X_2006_02_14_yyk\_map.gif/gif" ! Attempting to open device: 'J1639+8631_X_2006_02_14_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J1639+8631_X_2006_02_14_yyk_uvs.log closed on Wed Jul 5 13:00:40 2006