! Started logfile: J1154-3505_X_2002_01_31_yyk_uvs.log on Wed Jun 27 10:56:39 2007 obs J1154-3505_X_2002_01_31_yyk_uva.fits ! Reading UV FITS file: J1154-3505_X_2002_01_31_yyk_uva.fits ! AN table 1: 37 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.768168 visibilities/baseline/integration-bin. ! Found source: J1154-3505 ! ! 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 5116 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 J1154-3505_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)= 0.305211 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=0.7257 mas, bmaj=1.777 mas, bpa=4.161 degrees ! Estimated noise=2441.82 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 = 0.137822 Jy ! Component: 100 - total flux cleaned = 0.214554 Jy ! Total flux subtracted in 100 components = 0.214554 Jy ! Clean residual min=-0.022261 max=0.032545 Jy/beam ! Clean residual mean=-0.001219 rms=0.011864 Jy/beam ! Combined flux in latest and established models = 0.214554 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 55 model components to the UV plane model. ! The established model now contains 55 components and 0.214554 Jy ! ! Correcting IF 1. ! A total of 115 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 114 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 81 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 115 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.221638Jy sigma=0.001965 ! Fit after self-cal, rms=0.221600Jy sigma=0.001964 ! Inverting map and beam ! Estimated beam: bmin=0.7257 mas, bmaj=1.777 mas, bpa=4.161 degrees ! Estimated noise=2441.82 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=1.029 mas, bmaj=2.599 mas, bpa=-1.034 degrees ! Estimated noise=1459.09 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 = 0.111261 Jy ! Component: 100 - total flux cleaned = 0.170844 Jy ! Component: 150 - total flux cleaned = 0.200001 Jy ! Component: 200 - total flux cleaned = 0.222697 Jy ! Total flux subtracted in 200 components = 0.222697 Jy ! Clean residual min=-0.021464 max=0.021591 Jy/beam ! Clean residual mean=-0.001544 rms=0.013294 Jy/beam ! Combined flux in latest and established models = 0.437251 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 124 model components to the UV plane model. ! The established model now contains 170 components and 0.437251 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.184108Jy sigma=0.001516 ! Fit after self-cal, rms=0.183808Jy sigma=0.001514 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.029 x 2.599 at -1.034 degrees (North through East) ! Clean map min=-0.023259 max=0.13362 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=0.183808Jy sigma=0.001514 ! Fit after self-cal, rms=0.183808Jy sigma=0.001514 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=0.183808Jy sigma=0.001514 ! Fit after self-cal, rms=0.183808Jy sigma=0.001514 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=1.029 mas, bmaj=2.599 mas, bpa=-1.034 degrees ! Estimated noise=1459.09 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 = 0.0127467 Jy ! Component: 100 - total flux cleaned = 0.018859 Jy ! Component: 150 - total flux cleaned = 0.0199819 Jy ! Component: 200 - total flux cleaned = 0.0211068 Jy ! Total flux subtracted in 200 components = 0.0211068 Jy ! Clean residual min=-0.012686 max=0.012703 Jy/beam ! Clean residual mean=-0.000805 rms=0.007772 Jy/beam ! Combined flux in latest and established models = 0.458358 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 106 model components to the UV plane model. ! The established model now contains 274 components and 0.458358 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.177021Jy sigma=0.001430 ! Fit after self-cal, rms=0.176918Jy sigma=0.001429 ! 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=0.176918Jy sigma=0.001429 ! Fit after self-cal, rms=0.175958Jy sigma=0.001421 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 = 0.00521129 Jy ! Component: 100 - total flux cleaned = 0.0114243 Jy ! Component: 150 - total flux cleaned = 0.014113 Jy ! Component: 200 - total flux cleaned = 0.0153537 Jy ! Total flux subtracted in 200 components = 0.0153537 Jy ! Clean residual min=-0.007374 max=0.007443 Jy/beam ! Clean residual mean=-0.000500 rms=0.004559 Jy/beam ! Combined flux in latest and established models = 0.473711 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 81 model components to the UV plane model. ! The established model now contains 352 components and 0.473711 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.173158Jy sigma=0.001388 ! Fit after self-cal, rms=0.172901Jy sigma=0.001386 ! 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: 1.029 x 2.599 at -1.034 degrees (North through East) ! Clean map min=-0.020114 max=0.12704 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=0.172901Jy sigma=0.001386 ! Fit after self-cal, rms=0.177986Jy sigma=0.001385 ! 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=0.177986Jy sigma=0.001385 ! Fit after self-cal, rms=0.177963Jy sigma=0.001385 ! Inverting map and beam ! Estimated beam: bmin=1.047 mas, bmaj=2.626 mas, bpa=-0.6949 degrees ! Estimated noise=1473.85 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00388649 Jy ! Component: 100 - total flux cleaned = 0.0077323 Jy ! Component: 150 - total flux cleaned = 0.0105818 Jy ! Component: 200 - total flux cleaned = 0.0112747 Jy ! Total flux subtracted in 200 components = 0.0112747 Jy ! Clean residual min=-0.004203 max=0.004160 Jy/beam ! Clean residual mean=-0.000278 rms=0.002640 Jy/beam ! Combined flux in latest and established models = 0.484986 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 87 model components to the UV plane model. ! The established model now contains 429 components and 0.484986 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.176823Jy sigma=0.001373 ! Fit after self-cal, rms=0.176821Jy sigma=0.001373 ! 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=0.176821Jy sigma=0.001373 ! Fit after self-cal, rms=0.165279Jy sigma=0.001351 ! 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=0.165279Jy sigma=0.001351 ! Fit after self-cal, rms=0.165293Jy sigma=0.001351 ! Inverting map and beam ! Estimated beam: bmin=0.9994 mas, bmaj=2.523 mas, bpa=0.2699 degrees ! Estimated noise=1402.68 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.00233215 Jy ! Component: 100 - total flux cleaned = -0.00430178 Jy ! Component: 150 - total flux cleaned = -0.00432962 Jy ! Component: 200 - total flux cleaned = -0.0025213 Jy ! Total flux subtracted in 200 components = -0.0025213 Jy ! Clean residual min=-0.001978 max=0.001962 Jy/beam ! Clean residual mean=-0.000030 rms=0.000802 Jy/beam ! Combined flux in latest and established models = 0.482465 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 62 model components to the UV plane model. ! The established model now contains 488 components and 0.482465 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.164837Jy sigma=0.001347 ! Fit after self-cal, rms=0.164853Jy sigma=0.001347 ! 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=3.122 mas, bmaj=11.15 mas, bpa=10.65 degrees ! Estimated noise=1661.82 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 = 0.00211819 Jy ! Component: 100 - total flux cleaned = 0.0028717 Jy ! Component: 150 - total flux cleaned = 0.003145 Jy ! Component: 200 - total flux cleaned = 0.00275465 Jy ! Total flux subtracted in 200 components = 0.00275465 Jy ! Clean residual min=-0.001578 max=0.001575 Jy/beam ! Clean residual mean=-0.000058 rms=0.000741 Jy/beam ! Combined flux in latest and established models = 0.48522 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 70 model components to the UV plane model. ! The established model now contains 558 components and 0.48522 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.164711Jy sigma=0.001346 ! Fit after self-cal, rms=0.164721Jy sigma=0.001346 ! 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=0.716 mas, bmaj=1.767 mas, bpa=4.857 degrees ! Estimated noise=2335.64 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.134221 Jy ! Component: 100 - total flux cleaned = 0.208347 Jy ! Component: 150 - total flux cleaned = 0.263498 Jy ! Component: 200 - total flux cleaned = 0.299446 Jy ! Total flux subtracted in 200 components = 0.299446 Jy ! Clean residual min=-0.018555 max=0.018956 Jy/beam ! Clean residual mean=-0.000997 rms=0.008663 Jy/beam ! Combined flux in latest and established models = 0.299446 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 90 model components to the UV plane model. ! The established model now contains 90 components and 0.299446 Jy ! Inverting map and beam ! Estimated beam: bmin=0.9994 mas, bmaj=2.523 mas, bpa=0.2699 degrees ! Estimated noise=1402.68 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 = 0.068252 Jy ! Component: 100 - total flux cleaned = 0.107518 Jy ! Component: 150 - total flux cleaned = 0.128972 Jy ! Component: 200 - total flux cleaned = 0.13832 Jy ! Total flux subtracted in 200 components = 0.13832 Jy ! Clean residual min=-0.017434 max=0.017677 Jy/beam ! Clean residual mean=-0.001339 rms=0.010808 Jy/beam ! Combined flux in latest and established models = 0.437766 Jy ! Adding 120 model components to the UV plane model. ! The established model now contains 201 components and 0.437766 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=3.122 mas, bmaj=11.15 mas, bpa=10.65 degrees ! Estimated noise=1661.82 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 = 0.00612801 Jy ! Component: 100 - total flux cleaned = 0.00472824 Jy ! Component: 150 - total flux cleaned = 0.00354804 Jy ! Component: 200 - total flux cleaned = 0.00130511 Jy ! Total flux subtracted in 200 components = 0.00130511 Jy ! Clean residual min=-0.013670 max=0.013570 Jy/beam ! Clean residual mean=-0.000832 rms=0.007757 Jy/beam ! Combined flux in latest and established models = 0.439071 Jy ! Adding 96 model components to the UV plane model. ! The established model now contains 294 components and 0.439071 Jy ! Inverting map uvtaper 0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=0.9994 mas, bmaj=2.523 mas, bpa=0.2699 degrees ! Estimated noise=1402.68 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000981045 Jy ! Component: 100 - total flux cleaned = 0.0021546 Jy ! Component: 150 - total flux cleaned = 0.00110548 Jy ! Component: 200 - total flux cleaned = 0.0015621 Jy ! Total flux subtracted in 200 components = 0.0015621 Jy ! Clean residual min=-0.005328 max=0.005370 Jy/beam ! Clean residual mean=-0.000284 rms=0.002335 Jy/beam ! Combined flux in latest and established models = 0.440633 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 61 model components to the UV plane model. ! The established model now contains 355 components and 0.440633 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.165974Jy sigma=0.001357 ! Fit after self-cal, rms=0.165915Jy sigma=0.001356 wmodel J1154-3505_X_2002_01_31_yyk\_map.mod ! Writing 355 model components to file: J1154-3505_X_2002_01_31_yyk_map.mod wobs J1154-3505_X_2002_01_31_yyk\_uvs.fits ! Applying 37 buffered edits. ! Writing UV FITS file: J1154-3505_X_2002_01_31_yyk_uvs.fits wwins J1154-3505_X_2002_01_31_yyk\_map.win ! wwins: No CLEAN windows to write. ! Error occured in command: wwins ![Exited script file: muppet] ! wmap "J1154-3505_X_2002_01_31_yyk\_map.fits" ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9994 x 2.523 at 0.2699 degrees (North through East) ! Clean map min=-0.018977 max=0.10117 Jy/beam ! Writing clean map to FITS file: J1154-3505_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 0.101166 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00215221 device "J1154-3505_X_2002_01_31_yyk\_map.eps/VPS" ! Attempting to open device: 'J1154-3505_X_2002_01_31_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -6.38223 6.38223 12.7645 25.5289 51.0578 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0064 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.101 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9994 x 2.523 at 0.2699 degrees (North through East) ! Clean map min=-0.018977 max=0.10117 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1154-3505_X_2002_01_31_yyk\_map.gif/gif" ! Attempting to open device: 'J1154-3505_X_2002_01_31_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J1154-3505_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 10:56:44 2007