! Started logfile: 3C390.3_X.log on Wed May 14 16:59:19 2008 observe 3C390.3_X.edt ! Reading UV FITS file: 3C390.3_X.edt ! AN table 1: 123 integrations on 153 of 153 possible baselines. ! Apparent sampling: 0.185557 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 3C390.3 ! ! 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 8.40997e+09 8e+06 1 8e+06 ! 02 2 8.47997e+09 8e+06 1 8e+06 ! 03 3 8.79497e+09 8e+06 1 8e+06 ! 04 4 8.89997e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 946 lines of history. ! ! Reading 13968 visibilities. ![@gonzo7-0.1 3C390.3_X] print "***********************************" ! *********************************** print "*** Using gonzo instruction set ***" ! *** Using gonzo instruction set *** print "***********************************" ! *********************************** float field_size field_size = 1024 float field_cell field_cell = 0.1 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 0.100x0.100 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 1995 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 1998 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 2027 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 2013 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.793012Jy sigma=0.011787 ! Fit after self-cal, rms=0.792415Jy sigma=0.011838 ! 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=0.6536 mas, bmaj=0.8243 mas, bpa=-89.96 degrees ! Estimated noise=2334.52 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 = 0.153871 Jy ! Total flux subtracted in 50 components = 0.153871 Jy ! Clean residual min=-0.013496 max=0.045082 Jy/beam ! Clean residual mean=-0.000039 rms=0.003209 Jy/beam ! Combined flux in latest and established models = 0.153871 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.153871 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.082139Jy sigma=0.001254 ! Fit after self-cal, rms=0.082132Jy sigma=0.001254 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0433266 Jy ! Total flux subtracted in 50 components = 0.0433266 Jy ! Clean residual min=-0.008481 max=0.017005 Jy/beam ! Clean residual mean=0.000003 rms=0.001974 Jy/beam ! Combined flux in latest and established models = 0.197197 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 5 model components to the UV plane model. ! The established model now contains 8 components and 0.197197 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.059133Jy sigma=0.000858 ! Fit after self-cal, rms=0.059105Jy sigma=0.000858 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.016781 Jy ! Total flux subtracted in 50 components = 0.016781 Jy ! Clean residual min=-0.007337 max=0.009431 Jy/beam ! Clean residual mean=0.000019 rms=0.001722 Jy/beam ! Combined flux in latest and established models = 0.213978 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 9 model components to the UV plane model. ! The established model now contains 12 components and 0.213978 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.054792Jy sigma=0.000773 ! Fit after self-cal, rms=0.054787Jy sigma=0.000773 ! 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=0.9105 mas, bmaj=1.121 mas, bpa=-60.66 degrees ! Estimated noise=1327.98 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 = 0.0106339 Jy ! Component: 100 - total flux cleaned = 0.0158923 Jy ! Total flux subtracted in 100 components = 0.0158923 Jy ! Clean residual min=-0.005376 max=0.008476 Jy/beam ! Clean residual mean=-0.000043 rms=0.001595 Jy/beam ! Combined flux in latest and established models = 0.229871 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 17 model components to the UV plane model. ! The established model now contains 26 components and 0.229871 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.053370Jy sigma=0.000737 ! Fit after self-cal, rms=0.053355Jy sigma=0.000737 ! Inverting map print "****************************************" ! **************************************** print "*** Finished Natural Weighting CLEAN ***" ! *** Finished Natural Weighting CLEAN *** print "****************************************" ! **************************************** gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 9 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.08 FD 0.98 GC 1.05 HH 1.00* ! HN 1.01 KK 1.00 KP 0.98 LA 0.98 ! MC 1.00* MK 0.99 NL 1.02 NY 0.99 ! ON 1.00* OV 1.02 PT 0.95 SC 1.11 ! WF 0.99 WZ 1.03 ! ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.98 GC 1.03 HH 1.00* ! HN 1.04 KK 0.98 KP 0.99 LA 0.98 ! MC 1.02 MK 0.99 NL 1.01 NY 0.96 ! ON 1.00 OV 0.99 PT 0.98 SC 0.99 ! WF 1.01 WZ 0.97 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 0.98 GC 1.02 HH 1.00* ! HN 1.02 KK 1.00 KP 0.97 LA 0.98 ! MC 1.04 MK 1.00 NL 1.00 NY 0.94 ! ON 1.03 OV 1.01 PT 0.98 SC 1.01 ! WF 1.03 WZ 0.97 ! ! ! Correcting IF 4. ! A total of 9 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.99 GC 0.99 HH 1.00* ! HN 1.08 KK 0.98 KP 0.98 LA 0.97 ! MC 1.08 MK 1.01 NL 1.00 NY 1.03 ! ON 0.83 OV 0.99 PT 0.99 SC 0.96 ! WF 1.00 WZ 0.93 ! ! ! Fit before self-cal, rms=0.053355Jy sigma=0.000737 ! Fit after self-cal, rms=0.053320Jy sigma=0.000732 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.9162 mas, bmaj=1.131 mas, bpa=-59.75 degrees ! Estimated noise=1330.2 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 = -2.34154e-05 Jy ! Component: 100 - total flux cleaned = 0.000129774 Jy ! Total flux subtracted in 100 components = 0.000129774 Jy ! Clean residual min=-0.005319 max=0.008264 Jy/beam ! Clean residual mean=0.000017 rms=0.001455 Jy/beam ! Combined flux in latest and established models = 0.23 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 6 model components to the UV plane model. ! The established model now contains 30 components and 0.23 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.053272Jy sigma=0.000731 ! Fit after self-cal, rms=0.053263Jy sigma=0.000731 ! 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) ! Added new window around map position (-5.4, 7.1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00806685 Jy ! Component: 100 - total flux cleaned = 0.0118676 Jy ! Total flux subtracted in 100 components = 0.0118676 Jy ! Clean residual min=-0.004715 max=0.005234 Jy/beam ! Clean residual mean=0.000035 rms=0.001145 Jy/beam ! Combined flux in latest and established models = 0.241868 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 12 model components to the UV plane model. ! The established model now contains 42 components and 0.241868 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.052373Jy sigma=0.000711 ! Fit after self-cal, rms=0.051678Jy sigma=0.000692 ! Inverting map and beam ! Estimated beam: bmin=0.9202 mas, bmaj=1.138 mas, bpa=-59.02 degrees ! Estimated noise=1332.04 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 = 0.0036741 Jy ! Component: 100 - total flux cleaned = 0.00452332 Jy ! Total flux subtracted in 100 components = 0.00452332 Jy ! Clean residual min=-0.004345 max=0.004230 Jy/beam ! Clean residual mean=0.000023 rms=0.001016 Jy/beam ! Combined flux in latest and established models = 0.246391 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 18 model components to the UV plane model. ! The established model now contains 55 components and 0.246391 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.051501Jy sigma=0.000688 ! Fit after self-cal, rms=0.051367Jy sigma=0.000686 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 3C390.3_X ! Writing UV FITS file: 3C390.3_X.uvf ! Writing 55 model components to file: 3C390.3_X.mod ! wwins: Wrote 2 windows to 3C390.3_X.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9202 x 1.138 at -59.02 degrees (North through East) ! Clean map min=-0.0041124 max=0.20642 Jy/beam ! Writing clean map to FITS file: 3C390.3_X.fits ! Writing difmap environment to: 3C390.3_X.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 3C390.3_X] device 3C390.3_Xuv.ps/vps,1,2 ! Attempting to open device: '3C390.3_Xuv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 3C390.3_Xim.ps/vps ! Attempting to open device: '3C390.3_Xim.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=0.9202 mas, bmaj=1.138 mas, bpa=-59.02 degrees ! Estimated noise=1332.04 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9202 x 1.138 at -59.02 degrees (North through East) ! Clean map min=-0.0041124 max=0.20642 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo7-0.1] quit ! Quitting program ! Log file 3C390.3_X.log closed on Wed May 14 16:59:28 2008