! Started logfile: 1313-333_S.log on Wed Apr 30 00:05:43 2008 observe 1313-333_S.edt ! Reading UV FITS file: 1313-333_S.edt ! AN table 1: 15 integrations on 153 of 153 possible baselines. ! Apparent sampling: 0.123312 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 1313-333 ! ! 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 963 lines of history. ! ! Reading 1132 visibilities. ![@gonzo5-0.4 1313-333_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 = 5.0 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 189 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 190 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 190 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 222 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.435346Jy sigma=0.005349 ! Fit after self-cal, rms=0.434103Jy sigma=0.005350 ! 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=2.756 mas, bmaj=15.75 mas, bpa=-12.07 degrees ! Estimated noise=4282.16 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 = 0.402106 Jy ! Total flux subtracted in 50 components = 0.402106 Jy ! Clean residual min=-0.039131 max=0.112266 Jy/beam ! Clean residual mean=0.000561 rms=0.018089 Jy/beam ! Combined flux in latest and established models = 0.402106 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 0.402106 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.232580Jy sigma=0.002930 ! Fit after self-cal, rms=0.232578Jy sigma=0.002930 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.117886 Jy ! Total flux subtracted in 50 components = 0.117886 Jy ! Clean residual min=-0.023832 max=0.055259 Jy/beam ! Clean residual mean=0.000339 rms=0.010091 Jy/beam ! Combined flux in latest and established models = 0.519992 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 12 model components to the UV plane model. ! The established model now contains 13 components and 0.519992 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.146689Jy sigma=0.001845 ! Fit after self-cal, rms=0.146678Jy sigma=0.001845 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0617073 Jy ! Total flux subtracted in 50 components = 0.0617073 Jy ! Clean residual min=-0.018978 max=0.029189 Jy/beam ! Clean residual mean=0.000224 rms=0.006422 Jy/beam ! Combined flux in latest and established models = 0.581699 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 7 model components to the UV plane model. ! The established model now contains 15 components and 0.581699 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.109766Jy sigma=0.001370 ! Fit after self-cal, rms=0.109743Jy sigma=0.001370 ! 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=3.79 mas, bmaj=20.48 mas, bpa=-14.18 degrees ! Estimated noise=2456.05 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 = 0.0564975 Jy ! Component: 100 - total flux cleaned = 0.0818025 Jy ! Total flux subtracted in 100 components = 0.0818025 Jy ! Clean residual min=-0.013717 max=0.017806 Jy/beam ! Clean residual mean=0.000094 rms=0.004622 Jy/beam ! Combined flux in latest and established models = 0.663501 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 57 model components to the UV plane model. ! The established model now contains 69 components and 0.663502 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.082839Jy sigma=0.001010 ! Fit after self-cal, rms=0.082664Jy sigma=0.001009 ! 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 1.01 FD 1.00 GC 1.00* HH 1.00* ! HN 1.00* KK 0.99 KP 0.98 LA 1.00 ! MC 1.00* MK 0.99 NL 1.00* NY 1.00* ! ON 1.00* OV 0.99 PT 0.98 SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.99 GC 1.00* HH 1.00* ! HN 1.00* KK 0.95 KP 0.99 LA 0.98 ! MC 1.00* MK 1.02 NL 1.00* NY 1.00* ! ON 1.00* OV 0.99 PT 0.98 SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.99 GC 1.00* HH 1.00* ! HN 1.00* KK 1.02 KP 0.99 LA 0.98 ! MC 1.00* MK 1.02 NL 1.00* NY 1.00* ! ON 1.00* OV 0.99 PT 0.99 SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 0.99 GC 1.00* HH 1.00* ! HN 1.00* KK 0.97 KP 0.98 LA 1.00* ! MC 1.00* MK 1.01 NL 1.00* NY 1.00* ! ON 1.00* OV 0.99 PT 0.98 SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Fit before self-cal, rms=0.082664Jy sigma=0.001009 ! Fit after self-cal, rms=0.080241Jy sigma=0.000991 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=3.811 mas, bmaj=20.56 mas, bpa=-14.13 degrees ! Estimated noise=2413.67 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 (-15.2, -10). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0133878 Jy ! Component: 100 - total flux cleaned = 0.0132325 Jy ! Total flux subtracted in 100 components = 0.0132325 Jy ! Clean residual min=-0.009797 max=0.007430 Jy/beam ! Clean residual mean=0.000087 rms=0.002615 Jy/beam ! Combined flux in latest and established models = 0.676734 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 96 components and 0.676734 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.077237Jy sigma=0.000955 ! Fit after self-cal, rms=0.077030Jy sigma=0.000952 ! 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 = 0.00261857 Jy ! Component: 100 - total flux cleaned = 0.00154636 Jy ! Total flux subtracted in 100 components = 0.00154636 Jy ! Clean residual min=-0.008990 max=0.007100 Jy/beam ! Clean residual mean=0.000084 rms=0.002270 Jy/beam ! Combined flux in latest and established models = 0.67828 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 16 model components to the UV plane model. ! The established model now contains 109 components and 0.67828 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.076453Jy sigma=0.000946 ! Fit after self-cal, rms=0.075322Jy sigma=0.000933 ! Inverting map and beam ! Estimated beam: bmin=3.823 mas, bmaj=20.49 mas, bpa=-14.12 degrees ! Estimated noise=2411.11 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 = 0.00328218 Jy ! Component: 100 - total flux cleaned = 0.00253278 Jy ! Total flux subtracted in 100 components = 0.00253278 Jy ! Clean residual min=-0.007302 max=0.005410 Jy/beam ! Clean residual mean=0.000052 rms=0.001890 Jy/beam ! Combined flux in latest and established models = 0.680813 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 16 model components to the UV plane model. ! The established model now contains 124 components and 0.680813 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.074812Jy sigma=0.000927 ! Fit after self-cal, rms=0.074761Jy sigma=0.000926 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 1313-333_S ! Writing UV FITS file: 1313-333_S.uvf ! Writing 124 model components to file: 1313-333_S.mod ! wwins: Wrote 2 windows to 1313-333_S.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.823 x 20.49 at -14.12 degrees (North through East) ! Clean map min=-0.010607 max=0.568 Jy/beam ! Writing clean map to FITS file: 1313-333_S.fits ! Writing difmap environment to: 1313-333_S.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 1313-333_S] device 1313-333_Suv.ps/vps,1,2 ! Attempting to open device: '1313-333_Suv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 1313-333_Sim.ps/vps ! Attempting to open device: '1313-333_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=3.823 mas, bmaj=20.49 mas, bpa=-14.12 degrees ! Estimated noise=2411.11 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.823 x 20.49 at -14.12 degrees (North through East) ! Clean map min=-0.010607 max=0.568 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo5-0.4] quit ! Quitting program ! Log file 1313-333_S.log closed on Wed Apr 30 00:05:48 2008