! Started logfile: J2101-4219_X_2002_05_14_yyk_uvs.log on Tue Jun 26 23:15:28 2007 obs J2101-4219_X_2002_05_14_yyk_uva.fits ! Reading UV FITS file: J2101-4219_X_2002_05_14_yyk_uva.fits ! AN table 1: 24 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.422222 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J2101-4219 ! ! 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 1077 lines of history. ! ! Reading 1824 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 J2101-4219_X_2002_05_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. phase_soltime=phase_soltime1 print "uvstat(rms)=",uvstat(rms),"Jy" ! uvstat(rms)= 0.332856 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=0.793 mas, bmaj=7.155 mas, bpa=19.78 degrees ! Estimated noise=3695.15 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=100 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.105113 Jy ! Component: 100 - total flux cleaned = 0.134959 Jy ! Total flux subtracted in 100 components = 0.134959 Jy ! Clean residual min=-0.021161 max=0.020916 Jy/beam ! Clean residual mean=-0.000798 rms=0.008541 Jy/beam ! Combined flux in latest and established models = 0.134959 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 39 model components to the UV plane model. ! The established model now contains 39 components and 0.134959 Jy ! ! Correcting IF 1. ! A total of 96 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 88 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 104 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 128 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.301743Jy sigma=0.001778 ! Fit after self-cal, rms=0.300816Jy sigma=0.001773 ! Inverting map and beam ! Estimated beam: bmin=0.793 mas, bmaj=7.155 mas, bpa=19.78 degrees ! Estimated noise=3695.15 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=1.223 mas, bmaj=7.98 mas, bpa=18.08 degrees ! Estimated noise=2789.24 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 = 0.0592943 Jy ! Component: 100 - total flux cleaned = 0.0656596 Jy ! Component: 150 - total flux cleaned = 0.0676297 Jy ! Component: 200 - total flux cleaned = 0.0648689 Jy ! Total flux subtracted in 200 components = 0.0648689 Jy ! Clean residual min=-0.009918 max=0.009984 Jy/beam ! Clean residual mean=-0.000635 rms=0.004940 Jy/beam ! Combined flux in latest and established models = 0.199828 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 102 model components to the UV plane model. ! The established model now contains 139 components and 0.199828 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.292300Jy sigma=0.001692 ! Fit after self-cal, rms=0.292277Jy sigma=0.001691 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.223 x 7.98 at 18.08 degrees (North through East) ! Clean map min=-0.021834 max=0.12196 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* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* MK 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* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* MK 1.00* ! ! ! Correcting IF 3. ! A total of 24 telescope corrections were flagged in sub-array 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* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* MK 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* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* MK 1.00* ! ! ! Fit before self-cal, rms=0.292277Jy sigma=0.001691 ! Fit after self-cal, rms=0.292892Jy sigma=0.001692 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=0.292892Jy sigma=0.001692 ! Fit after self-cal, rms=0.292881Jy sigma=0.001691 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=1.215 mas, bmaj=7.972 mas, bpa=18.14 degrees ! Estimated noise=2812.65 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 = 0.00713184 Jy ! Component: 100 - total flux cleaned = 0.00898842 Jy ! Component: 150 - total flux cleaned = 0.00851276 Jy ! Component: 200 - total flux cleaned = 0.00950627 Jy ! Total flux subtracted in 200 components = 0.00950627 Jy ! Clean residual min=-0.005433 max=0.005450 Jy/beam ! Clean residual mean=-0.000246 rms=0.002475 Jy/beam ! Combined flux in latest and established models = 0.209334 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 63 model components to the UV plane model. ! The established model now contains 190 components and 0.209334 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.291322Jy sigma=0.001681 ! Fit after self-cal, rms=0.291302Jy sigma=0.001681 ! 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=0.291302Jy sigma=0.001681 ! Fit after self-cal, rms=0.288758Jy sigma=0.001659 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 = 1.51672e-05 Jy ! Component: 100 - total flux cleaned = 0.0047303 Jy ! Component: 150 - total flux cleaned = 0.00939308 Jy ! Component: 200 - total flux cleaned = 0.0113908 Jy ! Total flux subtracted in 200 components = 0.0113908 Jy ! Clean residual min=-0.004004 max=0.004023 Jy/beam ! Clean residual mean=-0.000037 rms=0.001667 Jy/beam ! Combined flux in latest and established models = 0.220725 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 54 model components to the UV plane model. ! The established model now contains 241 components and 0.220725 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.287623Jy sigma=0.001652 ! Fit after self-cal, rms=0.286790Jy sigma=0.001647 ! 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: 1.215 x 7.972 at 18.14 degrees (North through East) ! Clean map min=-0.016776 max=0.12008 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 ! Performing amp+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=0.286790Jy sigma=0.001647 ! Fit after self-cal, rms=0.286790Jy sigma=0.001647 ! 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=0.286790Jy sigma=0.001647 ! Fit after self-cal, rms=0.286466Jy sigma=0.001645 ! Inverting map and beam ! Estimated beam: bmin=1.215 mas, bmaj=7.972 mas, bpa=18.14 degrees ! Estimated noise=2812.65 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00158132 Jy ! Component: 100 - total flux cleaned = 0.000808253 Jy ! Component: 150 - total flux cleaned = 0.00270388 Jy ! Component: 200 - total flux cleaned = 0.00419545 Jy ! Total flux subtracted in 200 components = 0.00419545 Jy ! Clean residual min=-0.003626 max=0.003625 Jy/beam ! Clean residual mean=0.000037 rms=0.001487 Jy/beam ! Combined flux in latest and established models = 0.22492 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 50 model components to the UV plane model. ! The established model now contains 282 components and 0.22492 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.285650Jy sigma=0.001640 ! Fit after self-cal, rms=0.285505Jy sigma=0.001639 ! Inverting map ! Performing amp+phase self-cal over 1 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.285505Jy sigma=0.001639 ! Fit after self-cal, rms=0.285505Jy sigma=0.001639 ! 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=0.285505Jy sigma=0.001639 ! Fit after self-cal, rms=0.285426Jy sigma=0.001639 ! Inverting map and beam ! Estimated beam: bmin=1.215 mas, bmaj=7.972 mas, bpa=18.14 degrees ! Estimated noise=2812.65 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00134565 Jy ! Component: 100 - total flux cleaned = 0.00285838 Jy ! Component: 150 - total flux cleaned = 0.00371804 Jy ! Component: 200 - total flux cleaned = 0.00561122 Jy ! Total flux subtracted in 200 components = 0.00561122 Jy ! Clean residual min=-0.003298 max=0.003291 Jy/beam ! Clean residual mean=0.000059 rms=0.001335 Jy/beam ! Combined flux in latest and established models = 0.230531 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 39 model components to the UV plane model. ! The established model now contains 308 components and 0.230531 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.284813Jy sigma=0.001636 ! Fit after self-cal, rms=0.284814Jy sigma=0.001635 ! Inverting map ! ************** FINISHED AMPLITUDE SELF-CAL ************** 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=2.963 mas, bmaj=16.89 mas, bpa=2.2 degrees ! Estimated noise=3124.17 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 = 0.00390811 Jy ! Component: 100 - total flux cleaned = 0.00732849 Jy ! Component: 150 - total flux cleaned = 0.0103692 Jy ! Component: 200 - total flux cleaned = 0.0135754 Jy ! Total flux subtracted in 200 components = 0.0135754 Jy ! Clean residual min=-0.002649 max=0.002653 Jy/beam ! Clean residual mean=0.000071 rms=0.001224 Jy/beam ! Combined flux in latest and established models = 0.244107 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 36 model components to the UV plane model. ! The established model now contains 335 components and 0.244107 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.284517Jy sigma=0.001634 ! Fit after self-cal, rms=0.284521Jy sigma=0.001634 ! 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=0.7931 mas, bmaj=7.158 mas, bpa=19.78 degrees ! Estimated noise=3700.8 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.113045 Jy ! Component: 100 - total flux cleaned = 0.146377 Jy ! Component: 150 - total flux cleaned = 0.172289 Jy ! Component: 200 - total flux cleaned = 0.182021 Jy ! Total flux subtracted in 200 components = 0.182021 Jy ! Clean residual min=-0.014815 max=0.015092 Jy/beam ! Clean residual mean=-0.000485 rms=0.006225 Jy/beam ! Combined flux in latest and established models = 0.182021 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 47 model components to the UV plane model. ! The established model now contains 47 components and 0.182021 Jy ! Inverting map and beam ! Estimated beam: bmin=1.215 mas, bmaj=7.972 mas, bpa=18.14 degrees ! Estimated noise=2812.65 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 = 0.0351341 Jy ! Component: 100 - total flux cleaned = 0.0400043 Jy ! Component: 150 - total flux cleaned = 0.0372491 Jy ! Component: 200 - total flux cleaned = 0.0335679 Jy ! Total flux subtracted in 200 components = 0.0335679 Jy ! Clean residual min=-0.008227 max=0.008339 Jy/beam ! Clean residual mean=-0.000393 rms=0.004025 Jy/beam ! Combined flux in latest and established models = 0.215589 Jy ! Adding 86 model components to the UV plane model. ! The established model now contains 130 components and 0.215589 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=2.963 mas, bmaj=16.89 mas, bpa=2.2 degrees ! Estimated noise=3124.17 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 = 0.00347125 Jy ! Component: 100 - total flux cleaned = 0.00271547 Jy ! Component: 150 - total flux cleaned = 0.00476995 Jy ! Component: 200 - total flux cleaned = 0.0070601 Jy ! Total flux subtracted in 200 components = 0.0070601 Jy ! Clean residual min=-0.004429 max=0.004432 Jy/beam ! Clean residual mean=-0.000137 rms=0.002184 Jy/beam ! Combined flux in latest and established models = 0.222649 Jy ! Adding 97 model components to the UV plane model. ! The established model now contains 220 components and 0.222649 Jy ! Inverting map uvtaper 0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=1.215 mas, bmaj=7.972 mas, bpa=18.14 degrees ! Estimated noise=2812.65 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00174216 Jy ! Component: 100 - total flux cleaned = 0.00107724 Jy ! Component: 150 - total flux cleaned = 0.00167464 Jy ! Component: 200 - total flux cleaned = 0.00252565 Jy ! Total flux subtracted in 200 components = 0.00252565 Jy ! Clean residual min=-0.003491 max=0.003520 Jy/beam ! Clean residual mean=0.000008 rms=0.001486 Jy/beam ! Combined flux in latest and established models = 0.225174 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 42 model components to the UV plane model. ! The established model now contains 255 components and 0.225174 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.285039Jy sigma=0.001636 ! Fit after self-cal, rms=0.285037Jy sigma=0.001635 wmodel J2101-4219_X_2002_05_14_yyk\_map.mod ! Writing 255 model components to file: J2101-4219_X_2002_05_14_yyk_map.mod wobs J2101-4219_X_2002_05_14_yyk\_uvs.fits ! Writing UV FITS file: J2101-4219_X_2002_05_14_yyk_uvs.fits wwins J2101-4219_X_2002_05_14_yyk\_map.win ! wwins: No CLEAN windows to write. ! Error occured in command: wwins ![Exited script file: muppet] ! wmap "J2101-4219_X_2002_05_14_yyk\_map.fits" ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.215 x 7.972 at 18.14 degrees (North through East) ! Clean map min=-0.017674 max=0.12963 Jy/beam ! Writing clean map to FITS file: J2101-4219_X_2002_05_14_yyk_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.129626 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00152966 device "J2101-4219_X_2002_05_14_yyk\_map.eps/VPS" ! Attempting to open device: 'J2101-4219_X_2002_05_14_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -3.54018 3.54018 7.08036 14.1607 28.3214 56.6429 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0045 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.129 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.215 x 7.972 at 18.14 degrees (North through East) ! Clean map min=-0.017674 max=0.12963 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J2101-4219_X_2002_05_14_yyk\_map.gif/gif" ! Attempting to open device: 'J2101-4219_X_2002_05_14_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J2101-4219_X_2002_05_14_yyk_uvs.log closed on Tue Jun 26 23:15:33 2007