! Started logfile: 1451-400_S.log on Thu Aug 21 15:29:10 2008 observe 1451-400_S.edt ! Reading UV FITS file: 1451-400_S.edt ! AN table 1: 6 integrations on 171 of 171 possible baselines. ! Apparent sampling: 0.130604 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 1451-400 ! ! 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 2.22497e+09 8e+06 1 8e+06 ! 02 2 2.24497e+09 8e+06 1 8e+06 ! 03 3 2.33497e+09 8e+06 1 8e+06 ! 04 4 2.36497e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 1615 lines of history. ! ! Reading 536 visibilities. ![@gonzo7-0.4 1451-400_S] print "***********************************" ! *********************************** print "*** Using gonzo instruction set ***" ! *** Using gonzo instruction set *** print "***********************************" ! *********************************** float field_size field_size = 1024 float field_cell field_cell = 0.4 integer clean_niter clean_niter = 50 float clean_gain clean_gain = 0.03 float dynam dynam = 7.0 float win_mult win_mult = 1.8 float solint solint = 3.6/6.0 logical doflt doflt = true logical doamp float new_peak float flux_cutoff mapsize field_size,field_cell ! Map grid = 1024x1024 pixels with 0.400x0.400 milli-arcsec cellsize. select ! 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 startmod ! Applying default point source starting model. ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 1 Jy ! ! Correcting IF 1. ! A total of 82 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 79 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 79 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 79 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.640875Jy sigma=15.540957 ! Fit after self-cal, rms=0.640251Jy sigma=15.572887 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvweight 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. doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=2.322 mas, bmaj=6.789 mas, bpa=-8.909 degrees ! Estimated noise=2.7295 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0, 0). ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.280859 Jy ! Total flux subtracted in 50 components = 0.280859 Jy ! Clean residual min=-0.050690 max=0.089881 Jy/beam ! Clean residual mean=-0.001416 rms=0.017265 Jy/beam ! Combined flux in latest and established models = 0.280859 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 2 model components to the UV plane model. ! The established model now contains 2 components and 0.280859 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.239079Jy sigma=3.585821 ! Fit after self-cal, rms=0.239009Jy sigma=3.585589 ! Inverting map print "****************************************" ! **************************************** print "*** Finished Uniform Weighting CLEAN ***" ! *** Finished Uniform Weighting CLEAN *** print "****************************************" ! **************************************** uvweight 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. win_mult = win_mult * 1.6 clean_niter = clean_niter * 2 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=2.731 mas, bmaj=7.68 mas, bpa=-6.447 degrees ! Estimated noise=2.29499 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.118793 Jy ! Component: 100 - total flux cleaned = 0.181256 Jy ! Total flux subtracted in 100 components = 0.181256 Jy ! Clean residual min=-0.037504 max=0.089017 Jy/beam ! Clean residual mean=-0.001092 rms=0.014652 Jy/beam ! Combined flux in latest and established models = 0.462116 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 27 model components to the UV plane model. ! The established model now contains 29 components and 0.462116 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.183367Jy sigma=2.722054 ! Fit after self-cal, rms=0.183730Jy sigma=2.693301 ! Inverting map print "****************************************" ! **************************************** print "*** Finished Natural Weighting CLEAN ***" ! *** Finished Natural Weighting CLEAN *** print "****************************************" ! **************************************** gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.87 GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 0.86 LA 0.88 ! MA 1.00* MK 1.22 NL 2.03 NY 1.00* ! OV 1.01 PT 0.80 SC 1.05 TS 1.00* ! WF 1.00* WZ 1.00* GG 1.00* ! ! ! Correcting IF 2. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.88 GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 0.84 LA 0.90 ! MA 1.00* MK 1.02 NL 1.46 NY 1.00* ! OV 0.98 PT 0.79 SC 1.21 TS 1.00* ! WF 1.00* WZ 1.00* GG 1.00* ! ! ! Correcting IF 3. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.85 GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 0.83 LA 0.93 ! MA 1.00* MK 1.00 NL 1.47 NY 1.00* ! OV 1.11 PT 0.82 SC 0.95 TS 1.00* ! WF 1.00* WZ 1.00* GG 1.00* ! ! ! Correcting IF 4. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.87 GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 0.89 LA 0.84 ! MA 1.00* MK 1.11 NL 1.70 NY 1.00* ! OV 1.19 PT 0.75 SC 1.07 TS 1.00* ! WF 1.00* WZ 1.00* GG 1.00* ! ! ! Fit before self-cal, rms=0.183730Jy sigma=2.693301 ! Fit after self-cal, rms=0.177566Jy sigma=1.770818 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=2.914 mas, bmaj=8.275 mas, bpa=-8.871 degrees ! Estimated noise=2.32014 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (-9.6, -0.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0467768 Jy ! Component: 100 - total flux cleaned = 0.0486756 Jy ! Total flux subtracted in 100 components = 0.0486756 Jy ! Clean residual min=-0.021780 max=0.029341 Jy/beam ! Clean residual mean=0.000199 rms=0.005984 Jy/beam ! Combined flux in latest and established models = 0.510791 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 15 model components to the UV plane model. ! The established model now contains 44 components and 0.510792 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.159245Jy sigma=1.581045 ! Fit after self-cal, rms=0.155636Jy sigma=1.538176 ! Inverting map dynam = dynam - 1.0 doamp = true solint = solint * (6.0/3.6) 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 doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00400588 Jy ! Component: 100 - total flux cleaned = 0.00132447 Jy ! Total flux subtracted in 100 components = 0.00132447 Jy ! Clean residual min=-0.019790 max=0.023724 Jy/beam ! Clean residual mean=0.000212 rms=0.005483 Jy/beam ! Combined flux in latest and established models = 0.512116 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 13 model components to the UV plane model. ! The established model now contains 53 components and 0.512116 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.150528Jy sigma=1.515765 ! Fit after self-cal, rms=0.127372Jy sigma=1.423310 ! Inverting map and beam ! Estimated beam: bmin=2.878 mas, bmaj=8.195 mas, bpa=-8.287 degrees ! Estimated noise=2.25397 mJy/beam. doamp = false solint = solint / (6.0/3.6) 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 doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.017482 Jy ! Component: 100 - total flux cleaned = 0.0187105 Jy ! Total flux subtracted in 100 components = 0.0187105 Jy ! Clean residual min=-0.015013 max=0.016344 Jy/beam ! Clean residual mean=0.000146 rms=0.004074 Jy/beam ! Combined flux in latest and established models = 0.530827 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 20 model components to the UV plane model. ! The established model now contains 69 components and 0.530827 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.122715Jy sigma=1.398586 ! Fit after self-cal, rms=0.121209Jy sigma=1.379844 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 1451-400_S ! Writing UV FITS file: 1451-400_S.uvf ! Writing 69 model components to file: 1451-400_S.mod ! wwins: Wrote 2 windows to 1451-400_S.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 2.878 x 8.195 at -8.287 degrees (North through East) ! Clean map min=-0.014347 max=0.32355 Jy/beam ! Writing clean map to FITS file: 1451-400_S.fits ! Writing difmap environment to: 1451-400_S.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 1451-400_S] device 1451-400_Suv.ps/vps,1,2 ! Attempting to open device: '1451-400_Suv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 1451-400_Sim.ps/vps ! Attempting to open device: '1451-400_Sim.ps/vps' uvweight 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. loglevs -1,2048,2 ! The new contour levels are: ! -1 1 2 4 8 16 32 64 128 256 512 1024 2048 cmul = imstat(rms)*3 ! Inverting map and beam ! Estimated beam: bmin=2.878 mas, bmaj=8.195 mas, bpa=-8.287 degrees ! Estimated noise=2.25397 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 2.878 x 8.195 at -8.287 degrees (North through East) ! Clean map min=-0.014347 max=0.32355 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo7-0.4] quit ! Quitting program ! Log file 1451-400_S.log closed on Thu Aug 21 15:29:16 2008