! Started logfile: 0454-234_S.log on Thu Aug 11 16:13:27 2005 observe 0454-234_S.edt ! Reading UV FITS file: 0454-234_S.edt ! AN table 1: 23 integrations on 171 of 171 possible baselines. ! AN table 2: 9 integrations on 171 of 171 possible baselines. ! Apparent sampling: 0.259503 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 0454-234 ! ! 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 1565 lines of history. ! ! Reading 5680 visibilities. ![@gonzo7-0.4 0454-234_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 298 telescope corrections were flagged in sub-array 1. ! A total of 131 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 2. ! A total of 302 telescope corrections were flagged in sub-array 1. ! A total of 131 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 3. ! A total of 309 telescope corrections were flagged in sub-array 1. ! A total of 136 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 4. ! A total of 318 telescope corrections were flagged in sub-array 1. ! A total of 131 telescope corrections were flagged in sub-array 2. ! ! Fit before self-cal, rms=0.300249Jy sigma=0.003872 ! Fit after self-cal, rms=0.300956Jy sigma=0.003878 ! 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=2.234 mas, bmaj=8.706 mas, bpa=4.666 degrees ! Estimated noise=1809.81 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 = 0.935044 Jy ! Total flux subtracted in 50 components = 0.935044 Jy ! Clean residual min=-0.044375 max=0.260774 Jy/beam ! Clean residual mean=0.000714 rms=0.017591 Jy/beam ! Combined flux in latest and established models = 0.935044 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 0.935044 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.358539Jy sigma=0.004630 ! Fit after self-cal, rms=0.358539Jy sigma=0.004630 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.213168 Jy ! Total flux subtracted in 50 components = 0.213168 Jy ! Clean residual min=-0.024374 max=0.080085 Jy/beam ! Clean residual mean=0.000393 rms=0.008127 Jy/beam ! Combined flux in latest and established models = 1.14821 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 9 components and 1.14821 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.188175Jy sigma=0.002392 ! Fit after self-cal, rms=0.188160Jy sigma=0.002391 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0851585 Jy ! Total flux subtracted in 50 components = 0.0851585 Jy ! Clean residual min=-0.016644 max=0.038361 Jy/beam ! Clean residual mean=0.000265 rms=0.005351 Jy/beam ! Combined flux in latest and established models = 1.23337 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 11 components and 1.23337 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.140128Jy sigma=0.001732 ! Fit after self-cal, rms=0.140122Jy sigma=0.001732 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0436258 Jy ! Total flux subtracted in 50 components = 0.0436258 Jy ! Clean residual min=-0.014826 max=0.022000 Jy/beam ! Clean residual mean=0.000200 rms=0.004307 Jy/beam ! Combined flux in latest and established models = 1.277 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 13 model components to the UV plane model. ! The established model now contains 23 components and 1.277 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.122959Jy sigma=0.001490 ! Fit after self-cal, rms=0.122911Jy sigma=0.001489 ! 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=2.936 mas, bmaj=10.58 mas, bpa=7.312 degrees ! Estimated noise=1168.03 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 = 0.0417577 Jy ! Component: 100 - total flux cleaned = 0.0609242 Jy ! Total flux subtracted in 100 components = 0.0609242 Jy ! Clean residual min=-0.009226 max=0.012996 Jy/beam ! Clean residual mean=0.000910 rms=0.003038 Jy/beam ! Combined flux in latest and established models = 1.33792 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 49 components and 1.33792 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.110338Jy sigma=0.001310 ! Fit after self-cal, rms=0.110303Jy sigma=0.001309 ! 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 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 1.02 LA 1.00 ! MC 1.00* MK 1.01 NL 1.00 NY 1.00* ! ON 1.00* OV 0.98 PT 0.99 SC 0.93 ! TS 1.00* WF 1.02 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 0.98 GC 1.00* HH 1.00* ! HN 1.00* KK 1.00 KP 0.99 LA 0.98 ! MC 1.00* MK 1.03 NL 1.00* NY 1.00* ! ON 1.00* OV 0.93 PT 0.97 SC 1.00* ! TS 1.01 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 0.99 FD 1.00 GC 1.00* HH 1.00* ! HN 0.99 KK 1.00* KP 0.99 LA 1.00 ! MC 1.00* MK 1.01 NL 1.00 NY 1.00* ! ON 1.00* OV 0.99 PT 0.99 SC 0.99 ! TS 1.00* WF 1.00 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.97 GC 1.00* HH 1.00* ! HN 1.00* KK 1.02 KP 0.97 LA 0.96 ! MC 1.00* MK 1.04 NL 1.00* NY 1.00* ! ON 1.00* OV 0.97 PT 0.97 SC 1.00* ! TS 1.02 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 1.04 KK 1.00* KP 1.01 LA 1.01 ! MC 1.00* MK 1.01 NL 0.98 NY 1.00* ! ON 1.00* OV 1.00 PT 0.98 SC 1.04 ! TS 1.00* WF 1.04 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 FD 0.99 GC 1.00* HH 1.00* ! HN 1.00* KK 0.99 KP 0.98 LA 1.00* ! MC 1.00* MK 1.05 NL 1.00* NY 1.00* ! ON 1.00* OV 0.96 PT 0.95 SC 1.00* ! TS 1.03 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 1.01 GC 1.00* HH 1.00* ! HN 0.98 KK 1.00* KP 1.00 LA 0.99 ! MC 1.00* MK 1.01 NL 1.00 NY 1.00* ! ON 1.00* OV 0.98 PT 1.00 SC 1.07 ! TS 1.00* WF 1.03 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.97 GC 1.00* HH 1.00* ! HN 1.00* KK 0.97 KP 0.96 LA 0.99 ! MC 1.00* MK 1.04 NL 1.00* NY 1.00* ! ON 1.00* OV 0.98 PT 0.95 SC 1.00* ! TS 1.02 WF 1.00* WZ 1.00* ! ! ! Fit before self-cal, rms=0.110303Jy sigma=0.001309 ! Fit after self-cal, rms=0.100536Jy sigma=0.001190 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=2.938 mas, bmaj=10.61 mas, bpa=7.293 degrees ! Estimated noise=1161.87 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 = 0.00185394 Jy ! Component: 100 - total flux cleaned = 0.00220601 Jy ! Total flux subtracted in 100 components = 0.00220601 Jy ! Clean residual min=-0.006099 max=0.007169 Jy/beam ! Clean residual mean=0.000354 rms=0.001816 Jy/beam ! Combined flux in latest and established models = 1.34013 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 55 components and 1.34013 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100429Jy sigma=0.001190 ! Fit after self-cal, rms=0.100429Jy sigma=0.001190 ! 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 = 0.000194526 Jy ! Component: 100 - total flux cleaned = 0.000342103 Jy ! Total flux subtracted in 100 components = 0.000342103 Jy ! Clean residual min=-0.006096 max=0.007270 Jy/beam ! Clean residual mean=0.000350 rms=0.001814 Jy/beam ! Combined flux in latest and established models = 1.34047 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 15 model components to the UV plane model. ! The established model now contains 66 components and 1.34047 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100388Jy sigma=0.001189 ! Fit after self-cal, rms=0.096230Jy sigma=0.001136 ! Inverting map and beam ! Estimated beam: bmin=2.936 mas, bmaj=10.59 mas, bpa=7.299 degrees ! Estimated noise=1162.59 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 = 0.00167732 Jy ! Component: 100 - total flux cleaned = 0.00185482 Jy ! Total flux subtracted in 100 components = 0.00185482 Jy ! Clean residual min=-0.004895 max=0.006437 Jy/beam ! Clean residual mean=0.000337 rms=0.001474 Jy/beam ! Combined flux in latest and established models = 1.34232 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 73 components and 1.34232 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.096184Jy sigma=0.001135 ! Fit after self-cal, rms=0.096184Jy sigma=0.001135 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 0454-234_S ! Writing UV FITS file: 0454-234_S.uvf ! Writing 73 model components to file: 0454-234_S.mod ! wwins: Wrote 1 windows to 0454-234_S.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 2.936 x 10.59 at 7.299 degrees (North through East) ! Clean map min=-0.0047982 max=1.2354 Jy/beam ! Writing clean map to FITS file: 0454-234_S.fits ! Writing difmap environment to: 0454-234_S.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 0454-234_S] device 0454-234_Suv.ps/vps,1,2 ! Attempting to open device: '0454-234_Suv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 0454-234_Sim.ps/vps ! Attempting to open device: '0454-234_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=2.936 mas, bmaj=10.59 mas, bpa=7.299 degrees ! Estimated noise=1162.59 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 2.936 x 10.59 at 7.299 degrees (North through East) ! Clean map min=-0.0047982 max=1.2354 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo7-0.4] quit ! Quitting program ! Log file 0454-234_S.log closed on Thu Aug 11 16:13:43 2005