! Started logfile: 0113-118_S.log on Thu Apr 10 00:03:49 2008 observe 0113-118_S.edt ! Reading UV FITS file: 0113-118_S.edt ! AN table 1: 23 integrations on 153 of 153 possible baselines. ! Apparent sampling: 0.067917 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 0113-118 ! ! 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 956 visibilities. ![@gonzo6-0.4-pw 0113-118_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 = 6.0 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 314 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 363 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 336 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 367 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.388771Jy sigma=0.004792 ! Fit after self-cal, rms=0.387497Jy sigma=0.004796 ! 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 peakw win_mult ! Inverting map and beam ! Estimated beam: bmin=8.57 mas, bmaj=27.3 mas, bpa=36.71 degrees ! Estimated noise=3772.1 mJy/beam. ! Added new window around map position (0, 0). 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=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.438822 Jy ! Total flux subtracted in 50 components = 0.438822 Jy ! Clean residual min=-0.058747 max=0.155985 Jy/beam ! Clean residual mean=0.005511 rms=0.040427 Jy/beam ! Combined flux in latest and established models = 0.438822 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 10 components and 0.438822 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.258880Jy sigma=0.003243 ! Fit after self-cal, rms=0.258632Jy sigma=0.003240 ! 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=14.23 mas, bmaj=26.65 mas, bpa=34.74 degrees ! Estimated noise=2805.27 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 = 0.194058 Jy ! Component: 100 - total flux cleaned = 0.257254 Jy ! Total flux subtracted in 100 components = 0.257254 Jy ! Clean residual min=-0.013364 max=0.024840 Jy/beam ! Clean residual mean=0.001078 rms=0.007747 Jy/beam ! Combined flux in latest and established models = 0.696076 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 41 model components to the UV plane model. ! The established model now contains 48 components and 0.696076 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081155Jy sigma=0.000973 ! Fit after self-cal, rms=0.080996Jy sigma=0.000971 ! 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 1.01 GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 0.96 LA 0.98 ! MC 1.00* MK 1.00* NL 0.97 NY 1.00* ! ON 1.00* OV 1.00* PT 0.99 SC 1.00* ! WF 1.00* WZ 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 1.00* GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 0.97 LA 0.97 ! MC 1.00* MK 1.00* NL 0.97 NY 1.00* ! ON 1.00* OV 1.00* PT 0.98 SC 1.00* ! WF 1.00* WZ 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 1.02 GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 0.97 LA 0.97 ! MC 1.00* MK 1.00* NL 0.97 NY 1.00* ! ON 1.00* OV 1.00* PT 0.98 SC 1.00* ! WF 1.00* WZ 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 1.02 GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 0.96 LA 1.00* ! MC 1.00* MK 1.00* NL 0.98 NY 1.00* ! ON 1.00* OV 1.00* PT 0.98 SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Fit before self-cal, rms=0.080996Jy sigma=0.000971 ! Fit after self-cal, rms=0.072771Jy sigma=0.000892 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=14.36 mas, bmaj=26.41 mas, bpa=34.46 degrees ! Estimated noise=2720.66 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 = 0.000904962 Jy ! Component: 100 - total flux cleaned = 0.000907581 Jy ! Total flux subtracted in 100 components = 0.000907581 Jy ! Clean residual min=-0.007208 max=0.007805 Jy/beam ! Clean residual mean=0.000005 rms=0.002171 Jy/beam ! Combined flux in latest and established models = 0.696984 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 14 model components to the UV plane model. ! The established model now contains 62 components and 0.696984 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.072401Jy sigma=0.000888 ! Fit after self-cal, rms=0.072396Jy sigma=0.000888 ! 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 = -4.10905e-06 Jy ! Component: 100 - total flux cleaned = 0.000126228 Jy ! Total flux subtracted in 100 components = 0.000126228 Jy ! Clean residual min=-0.006959 max=0.007784 Jy/beam ! Clean residual mean=0.000002 rms=0.002048 Jy/beam ! Combined flux in latest and established models = 0.69711 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 11 model components to the UV plane model. ! The established model now contains 67 components and 0.69711 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.072169Jy sigma=0.000885 ! Fit after self-cal, rms=0.071120Jy sigma=0.000874 ! Inverting map and beam ! Estimated beam: bmin=14.21 mas, bmaj=26.44 mas, bpa=34.57 degrees ! Estimated noise=2712.19 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 = -0.000104094 Jy ! Component: 100 - total flux cleaned = -0.000216192 Jy ! Total flux subtracted in 100 components = -0.000216192 Jy ! Clean residual min=-0.006660 max=0.007429 Jy/beam ! Clean residual mean=-0.000009 rms=0.001956 Jy/beam ! Combined flux in latest and established models = 0.696894 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 74 components and 0.696894 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070940Jy sigma=0.000871 ! Fit after self-cal, rms=0.070926Jy sigma=0.000871 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 0113-118_S ! Writing UV FITS file: 0113-118_S.uvf ! Writing 74 model components to file: 0113-118_S.mod ! wwins: Wrote 1 windows to 0113-118_S.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 14.21 x 26.44 at 34.57 degrees (North through East) ! Clean map min=-0.0066699 max=0.58707 Jy/beam ! Writing clean map to FITS file: 0113-118_S.fits ! Writing difmap environment to: 0113-118_S.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 0113-118_S] device 0113-118_Suv.ps/vps,1,2 ! Attempting to open device: '0113-118_Suv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 0113-118_Sim.ps/vps ! Attempting to open device: '0113-118_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=14.21 mas, bmaj=26.44 mas, bpa=34.57 degrees ! Estimated noise=2712.19 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 14.21 x 26.44 at 34.57 degrees (North through East) ! Clean map min=-0.0066699 max=0.58707 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo6-0.4-pw] quit ! Quitting program ! Log file 0113-118_S.log closed on Thu Apr 10 00:03:53 2008