! Started logfile: J0648+7756_S_2006_02_16_yyk_uvs.log on Wed Jul 5 11:37:17 2006 obs J0648+7756_S_2006_02_16_yyk_uva.fits ! Reading UV FITS file: J0648+7756_S_2006_02_16_yyk_uva.fits ! AN table 1: 858 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.132634 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0648+7756 ! ! 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 2.23697e+09 8e+06 1 8e+06 ! 02 2 2.26697e+09 8e+06 1 8e+06 ! 03 3 2.35697e+09 8e+06 1 8e+06 ! 04 4 2.37697e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 2424 lines of history. ! ! Reading 20484 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 J0648+7756_S_2006_02_16_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 0.500x0.500 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)= 0.0935243 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=21.6 mas, bmaj=40.35 mas, bpa=14.75 degrees ! Estimated noise=2.24533 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 = 0.0540585 Jy ! Component: 100 - total flux cleaned = 0.0600562 Jy ! Total flux subtracted in 100 components = 0.0600562 Jy ! Clean residual min=-0.007532 max=0.007501 Jy/beam ! Clean residual mean=0.000479 rms=0.004696 Jy/beam ! Combined flux in latest and established models = 0.0600562 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 58 model components to the UV plane model. ! The established model now contains 58 components and 0.0600562 Jy ! ! Correcting IF 1. ! A total of 96 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 96 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 112 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 112 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.060477Jy sigma=1.046804 ! Fit after self-cal, rms=0.059878Jy sigma=1.032423 ! Inverting map and beam ! Estimated beam: bmin=21.6 mas, bmaj=40.35 mas, bpa=14.75 degrees ! Estimated noise=2.24533 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=24.16 mas, bmaj=38.92 mas, bpa=3.036 degrees ! Estimated noise=2.03523 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 = 0.00199458 Jy ! Component: 100 - total flux cleaned = 0.00204209 Jy ! Component: 150 - total flux cleaned = 0.00137852 Jy ! Component: 200 - total flux cleaned = -0.000359622 Jy ! Total flux subtracted in 200 components = -0.000359622 Jy ! Clean residual min=-0.001422 max=0.001434 Jy/beam ! Clean residual mean=-0.000038 rms=0.000682 Jy/beam ! Combined flux in latest and established models = 0.0596966 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 90 model components to the UV plane model. ! The established model now contains 148 components and 0.0596966 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.057429Jy sigma=0.990643 ! Fit after self-cal, rms=0.057382Jy sigma=0.989667 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 24.16 x 38.92 at 3.036 degrees (North through East) ! Clean map min=-0.011797 max=0.049509 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: 0.982026 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.09 HN 1.00* KP 0.95 ! LA 0.98 MK 1.00* NL 1.00* OV 1.00* ! PT 1.16 SC 1.00* ! ! ! Correcting IF 2. ! Amplitude normalization factor in sub-array 1: 1.00281 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00 HN 1.00* KP 1.00 ! LA 0.99 MK 1.00* NL 1.00* OV 1.00* ! PT 0.99 SC 1.00* ! ! ! Correcting IF 3. ! A total of 48 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 1 ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* HN 0.00* KP 0.00* ! LA 0.00* MK 0.00* NL 0.00* OV 0.00* ! PT 0.00* SC 0.00* ! ! ! Correcting IF 4. ! A total of 48 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 1 ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* HN 0.00* KP 0.00* ! LA 0.00* MK 0.00* NL 0.00* OV 0.00* ! PT 0.00* SC 0.00* ! ! ! Fit before self-cal, rms=0.057382Jy sigma=0.989667 ! Fit after self-cal, rms=0.053190Jy sigma=0.993363 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=0.053190Jy sigma=0.993363 ! Fit after self-cal, rms=0.053155Jy sigma=0.992889 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=22.86 mas, bmaj=38.56 mas, bpa=2.44 degrees ! Estimated noise=2.41141 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 = 0.000761059 Jy ! Component: 100 - total flux cleaned = 0.000496613 Jy ! Component: 150 - total flux cleaned = -0.000377105 Jy ! Component: 200 - total flux cleaned = -0.000742468 Jy ! Total flux subtracted in 200 components = -0.000742468 Jy ! Clean residual min=-0.000418 max=0.000417 Jy/beam ! Clean residual mean=-0.000031 rms=0.000198 Jy/beam ! Combined flux in latest and established models = 0.0589541 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 74 model components to the UV plane model. ! The established model now contains 221 components and 0.0589541 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.053126Jy sigma=0.990934 ! Fit after self-cal, rms=0.053095Jy sigma=0.990532 ! 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=0.053095Jy sigma=0.990532 ! Fit after self-cal, rms=0.046778Jy sigma=0.844175 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 = 0.00348197 Jy ! Component: 100 - total flux cleaned = 0.00280474 Jy ! Component: 150 - total flux cleaned = 0.00182271 Jy ! Component: 200 - total flux cleaned = 0.00192861 Jy ! Total flux subtracted in 200 components = 0.00192861 Jy ! Clean residual min=-0.000655 max=0.000657 Jy/beam ! Clean residual mean=0.000025 rms=0.000247 Jy/beam ! Combined flux in latest and established models = 0.0608827 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 76 model components to the UV plane model. ! The established model now contains 296 components and 0.0608827 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.046374Jy sigma=0.837581 ! Fit after self-cal, rms=0.045704Jy sigma=0.826577 ! 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: 22.86 x 38.56 at 2.44 degrees (North through East) ! Clean map min=-0.012112 max=0.049679 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 = 20 mega-wavelengths. win_mult = win_mult * 1.4 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=23.13 mas, bmaj=38.56 mas, bpa=2.291 degrees ! Estimated noise=2.41224 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 = -0.000290675 Jy ! Component: 100 - total flux cleaned = -0.000532411 Jy ! Component: 150 - total flux cleaned = -0.000882128 Jy ! Component: 200 - total flux cleaned = -0.00108333 Jy ! Total flux subtracted in 200 components = -0.00108333 Jy ! Clean residual min=-0.000293 max=0.000291 Jy/beam ! Clean residual mean=-0.000006 rms=0.000138 Jy/beam ! Combined flux in latest and established models = 0.0597993 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 365 components and 0.0597993 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.045692Jy sigma=0.826167 ! Fit after self-cal, rms=0.045598Jy sigma=0.825048 ! 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=22.13 mas, bmaj=40.19 mas, bpa=14.11 degrees ! Estimated noise=2.56631 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0594902 Jy ! Component: 100 - total flux cleaned = 0.0624238 Jy ! Component: 150 - total flux cleaned = 0.0580636 Jy ! Component: 200 - total flux cleaned = 0.0584035 Jy ! Total flux subtracted in 200 components = 0.0584035 Jy ! Clean residual min=-0.004855 max=0.004820 Jy/beam ! Clean residual mean=-0.000120 rms=0.002219 Jy/beam ! Combined flux in latest and established models = 0.0584035 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 107 model components to the UV plane model. ! The established model now contains 107 components and 0.0584035 Jy ! Inverting map and beam ! Estimated beam: bmin=22.86 mas, bmaj=38.56 mas, bpa=2.44 degrees ! Estimated noise=2.41141 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 = -0.001356 Jy ! Component: 100 - total flux cleaned = -0.000537376 Jy ! Component: 150 - total flux cleaned = 0.000440238 Jy ! Component: 200 - total flux cleaned = 0.000668801 Jy ! Total flux subtracted in 200 components = 0.000668801 Jy ! Clean residual min=-0.000957 max=0.000979 Jy/beam ! Clean residual mean=-0.000057 rms=0.000430 Jy/beam ! Combined flux in latest and established models = 0.0590723 Jy ! Adding 63 model components to the UV plane model. ! The established model now contains 170 components and 0.0590723 Jy ! Inverting map uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 20 mega-wavelengths. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=23.13 mas, bmaj=38.56 mas, bpa=2.291 degrees ! Estimated noise=2.41224 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 = 0.00014704 Jy ! Component: 100 - total flux cleaned = 0.000265086 Jy ! Component: 150 - total flux cleaned = 0.000342384 Jy ! Component: 200 - total flux cleaned = 0.00026762 Jy ! Total flux subtracted in 200 components = 0.00026762 Jy ! Clean residual min=-0.000323 max=0.000315 Jy/beam ! Clean residual mean=-0.000003 rms=0.000139 Jy/beam ! Combined flux in latest and established models = 0.05934 Jy ! Adding 93 model components to the UV plane model. ! The established model now contains 263 components and 0.05934 Jy ! Inverting map uvtaper 0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=22.86 mas, bmaj=38.56 mas, bpa=2.44 degrees ! Estimated noise=2.41141 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00021315 Jy ! Component: 100 - total flux cleaned = 0.000299971 Jy ! Component: 150 - total flux cleaned = 0.000368167 Jy ! Component: 200 - total flux cleaned = 0.000436545 Jy ! Total flux subtracted in 200 components = 0.000436545 Jy ! Clean residual min=-0.000215 max=0.000218 Jy/beam ! Clean residual mean=0.000001 rms=0.000084 Jy/beam ! Combined flux in latest and established models = 0.0597765 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 48 model components to the UV plane model. ! The established model now contains 311 components and 0.0597765 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.045680Jy sigma=0.826361 ! Fit after self-cal, rms=0.045659Jy sigma=0.826116 wmodel J0648+7756_S_2006_02_16_yyk\_map.mod ! Writing 311 model components to file: J0648+7756_S_2006_02_16_yyk_map.mod wobs J0648+7756_S_2006_02_16_yyk\_uvs.fits ! Writing UV FITS file: J0648+7756_S_2006_02_16_yyk_uvs.fits wwins J0648+7756_S_2006_02_16_yyk\_map.win ! wwins: No CLEAN windows to write. ! Error occured in command: wwins ![Exited script file: muppet] ! wmap "J0648+7756_S_2006_02_16_yyk\_map.fits" ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 22.86 x 38.56 at 2.44 degrees (North through East) ! Clean map min=-0.010654 max=0.04402 Jy/beam ! Writing clean map to FITS file: J0648+7756_S_2006_02_16_yyk_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0440196 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000101616 device "J0648+7756_S_2006_02_16_yyk\_map.eps/VPS" ! Attempting to open device: 'J0648+7756_S_2006_02_16_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.692528 0.692528 1.38506 2.77011 5.54022 11.0804 22.1609 44.3218 88.6436 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0003 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.044 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 22.86 x 38.56 at 2.44 degrees (North through East) ! Clean map min=-0.010654 max=0.04402 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0648+7756_S_2006_02_16_yyk\_map.gif/gif" ! Attempting to open device: 'J0648+7756_S_2006_02_16_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J0648+7756_S_2006_02_16_yyk_uvs.log closed on Wed Jul 5 11:37:41 2006