! Started logfile: 1908-201_S.log on Fri Apr 24 14:57:51 2009 observe 1908-201_S.edt2 ! Reading UV FITS file: 1908-201_S.edt2 ! AN table 1: 70 integrations on 190 of 190 possible baselines. ! AN table 2: 23 integrations on 190 of 190 possible baselines. ! AN table 3: 7 integrations on 190 of 190 possible baselines. ! AN table 4: 41 integrations on 190 of 190 possible baselines. ! Apparent sampling: 0.0992535 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 1908-201 ! ! 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 1481 lines of history. ! ! Reading 10636 visibilities. ![@gonzo8-0.4 1908-201_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 = 8.0 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 1208 telescope corrections were flagged in sub-array 1. ! A total of 406 telescope corrections were flagged in sub-array 2. ! A total of 140 telescope corrections were flagged in sub-array 3. ! A total of 704 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 1241 telescope corrections were flagged in sub-array 1. ! A total of 406 telescope corrections were flagged in sub-array 2. ! A total of 140 telescope corrections were flagged in sub-array 3. ! A total of 705 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 1205 telescope corrections were flagged in sub-array 1. ! A total of 406 telescope corrections were flagged in sub-array 2. ! A total of 140 telescope corrections were flagged in sub-array 3. ! A total of 720 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 1193 telescope corrections were flagged in sub-array 1. ! A total of 406 telescope corrections were flagged in sub-array 2. ! A total of 140 telescope corrections were flagged in sub-array 3. ! A total of 708 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=0.858260Jy sigma=4.883629 ! Fit after self-cal, rms=0.786130Jy sigma=4.817047 ! 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=1.784 mas, bmaj=3.692 mas, bpa=7.186 degrees ! Estimated noise=3.68876 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 = 0.851896 Jy ! Total flux subtracted in 50 components = 0.851896 Jy ! Clean residual min=-0.084512 max=0.331064 Jy/beam ! Clean residual mean=-0.000965 rms=0.029956 Jy/beam ! Combined flux in latest and established models = 0.851896 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 6 components and 0.851896 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.833419Jy sigma=5.133649 ! Fit after self-cal, rms=0.833332Jy sigma=5.133189 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.363581 Jy ! Total flux subtracted in 50 components = 0.363581 Jy ! Clean residual min=-0.062355 max=0.171939 Jy/beam ! Clean residual mean=-0.000733 rms=0.022270 Jy/beam ! Combined flux in latest and established models = 1.21548 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 17 components and 1.21548 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.660807Jy sigma=3.900004 ! Fit after self-cal, rms=0.660709Jy sigma=3.899294 ! 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=2.333 mas, bmaj=4.739 mas, bpa=4.199 degrees ! Estimated noise=2.43215 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 = 0.306453 Jy ! Component: 100 - total flux cleaned = 0.454512 Jy ! Total flux subtracted in 100 components = 0.454512 Jy ! Clean residual min=-0.078967 max=0.243893 Jy/beam ! Clean residual mean=0.011011 rms=0.029451 Jy/beam ! Combined flux in latest and established models = 1.66999 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 24 model components to the UV plane model. ! The established model now contains 41 components and 1.66999 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.551530Jy sigma=2.927943 ! Fit after self-cal, rms=0.551391Jy sigma=2.926733 ! Inverting map ! Added new window around map position (6.4, 2.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.222199 Jy ! Component: 100 - total flux cleaned = 0.334464 Jy ! Total flux subtracted in 100 components = 0.334464 Jy ! Clean residual min=-0.060936 max=0.167051 Jy/beam ! Clean residual mean=0.005085 rms=0.019859 Jy/beam ! Combined flux in latest and established models = 2.00445 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 30 model components to the UV plane model. ! The established model now contains 71 components and 2.00445 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.471295Jy sigma=2.342579 ! Fit after self-cal, rms=0.462191Jy sigma=2.267215 ! 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 12 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.95 GC 1.00* HH 0.82 ! HN 0.82 KK 1.00* KP 0.95 LA 1.02 ! MA 1.27 MC 0.87 MK 1.00* NL 1.32 ! NY 1.00* ON 1.05 OV 0.93 PT 0.87 ! SC 0.98 TS 1.00* WF 0.94 WZ 0.91 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.90 FD 1.00* GC 1.00* HH 1.00* ! HN 0.91 KK 1.00* KP 1.13 LA 1.83 ! MA 1.00* MC 1.00* MK 1.00* NL 1.00* ! NY 1.00* ON 1.00* OV 1.09 PT 0.83 ! SC 1.00* TS 1.00* WF 1.07 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* FD 0.00* GC 0.00* HH 0.00* ! HN 0.00* KK 0.00* KP 0.00* LA 0.00* ! MA 0.00* MC 0.00* MK 0.00* NL 0.00* ! NY 0.00* ON 0.00* OV 0.00* PT 0.00* ! SC 0.00* TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 54 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.85 FD 0.94 GC 1.00* HH 1.00* ! HN 0.84 KK 1.03 KP 0.99 LA 1.12 ! MA 1.00* MC 1.00* MK 0.89 NL 1.62 ! NY 1.00* ON 1.00* OV 0.90 PT 0.82 ! SC 1.10 TS 1.00* WF 0.96 WZ 1.00* ! ! ! 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 0.90 GC 1.00* HH 0.77 ! HN 0.88 KK 1.00* KP 1.01 LA 1.04 ! MA 1.03 MC 0.87 MK 1.00* NL 1.26 ! NY 1.00* ON 0.88 OV 0.89 PT 0.91 ! SC 0.86 TS 1.00* WF 0.92 WZ 0.98 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 1.00* GC 1.00* HH 1.00* ! HN 1.04 KK 1.00* KP 1.17 LA 1.78 ! MA 1.00* MC 1.00* MK 1.00* NL 1.00* ! NY 1.00* ON 1.00* OV 1.03 PT 0.94 ! SC 1.00* TS 1.00* WF 1.09 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* FD 0.00* GC 0.00* HH 0.00* ! HN 0.00* KK 0.00* KP 0.00* LA 0.00* ! MA 0.00* MC 0.00* MK 0.00* NL 0.00* ! NY 0.00* ON 0.00* OV 0.00* PT 0.00* ! SC 0.00* TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 54 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.85 FD 0.85 GC 1.00* HH 1.00* ! HN 0.88 KK 1.11 KP 1.04 LA 1.12 ! MA 1.00* MC 1.00* MK 0.91 NL 1.73 ! NY 1.00* ON 1.00* OV 0.83 PT 0.90 ! SC 0.92 TS 1.00* WF 0.96 WZ 1.00* ! ! ! Correcting IF 3. ! A total of 24 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 1.74 ! HN 1.09 KK 1.00* KP 1.03 LA 0.97 ! MA 1.10 MC 1.25 MK 1.00* NL 0.75 ! NY 1.00* ON 0.89 OV 1.00 PT 0.97 ! SC 1.02 TS 1.00* WF 0.95 WZ 0.91 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.91 FD 1.00* GC 1.00* HH 1.00* ! HN 1.67 KK 1.00* KP 1.31 LA 1.68 ! MA 1.00* MC 1.00* MK 1.00* NL 1.00* ! NY 1.00* ON 1.00* OV 0.93 PT 0.88 ! SC 1.00* TS 1.00* WF 1.66 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* FD 0.00* GC 0.00* HH 0.00* ! HN 0.00* KK 0.00* KP 0.00* LA 0.00* ! MA 0.00* MC 0.00* MK 0.00* NL 0.00* ! NY 0.00* ON 0.00* OV 0.00* PT 0.00* ! SC 0.00* TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 39 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.92 FD 0.85 GC 1.00* HH 1.00* ! HN 1.31 KK 1.05 KP 1.07 LA 1.07 ! MA 1.00* MC 1.00* MK 0.89 NL 1.65 ! NY 1.00* ON 1.00* OV 0.91 PT 0.93 ! SC 1.03 TS 1.00* WF 1.17 WZ 1.00* ! ! ! Correcting IF 4. ! A total of 18 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.77 GC 1.00* HH 0.79 ! HN 1.10 KK 1.00* KP 1.07 LA 0.85 ! MA 0.91 MC 1.02 MK 1.00* NL 1.16 ! NY 1.00* ON 0.99 OV 0.88 PT 0.91 ! SC 0.92 TS 1.00* WF 0.95 WZ 1.01 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 1.00* GC 1.00* HH 1.00* ! HN 1.16 KK 1.00* KP 1.27 LA 1.57 ! MA 1.00* MC 1.00* MK 1.00* NL 1.00* ! NY 1.00* ON 1.00* OV 1.07 PT 0.96 ! SC 1.00* TS 1.00* WF 1.03 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* FD 0.00* GC 0.00* HH 0.00* ! HN 0.00* KK 0.00* KP 0.00* LA 0.00* ! MA 0.00* MC 0.00* MK 0.00* NL 0.00* ! NY 0.00* ON 0.00* OV 0.00* PT 0.00* ! SC 0.00* TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 51 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.88 FD 0.77 GC 1.00* HH 1.00* ! HN 1.08 KK 0.93 KP 1.08 LA 0.82 ! MA 1.00* MC 1.00* MK 0.89 NL 1.86 ! NY 1.00* ON 1.00* OV 0.83 PT 0.91 ! SC 0.99 TS 1.00* WF 0.94 WZ 1.00* ! ! ! Fit before self-cal, rms=0.462191Jy sigma=2.267215 ! Fit after self-cal, rms=0.431461Jy sigma=1.572031 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=2.29 mas, bmaj=4.806 mas, bpa=2.806 degrees ! Estimated noise=2.45353 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 = 0.0254488 Jy ! Component: 100 - total flux cleaned = 0.0253134 Jy ! Total flux subtracted in 100 components = 0.0253134 Jy ! Clean residual min=-0.037177 max=0.047572 Jy/beam ! Clean residual mean=0.003047 rms=0.009488 Jy/beam ! Combined flux in latest and established models = 2.02977 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 84 components and 2.02977 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.425060Jy sigma=1.550317 ! Fit after self-cal, rms=0.424705Jy sigma=1.544278 ! 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 = 0.00421885 Jy ! Component: 100 - total flux cleaned = 0.00489735 Jy ! Total flux subtracted in 100 components = 0.00489735 Jy ! Clean residual min=-0.035869 max=0.039697 Jy/beam ! Clean residual mean=0.002981 rms=0.009344 Jy/beam ! Combined flux in latest and established models = 2.03466 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 14 model components to the UV plane model. ! The established model now contains 89 components and 2.03466 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.422616Jy sigma=1.538776 ! Fit after self-cal, rms=0.491362Jy sigma=0.995926 ! Inverting map and beam ! Estimated beam: bmin=2.356 mas, bmaj=4.845 mas, bpa=2.662 degrees ! Estimated noise=2.48723 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) ! Added new window around map position (-4, 0.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0108388 Jy ! Component: 100 - total flux cleaned = 0.0142188 Jy ! Total flux subtracted in 100 components = 0.0142188 Jy ! Clean residual min=-0.016964 max=0.024712 Jy/beam ! Clean residual mean=0.002002 rms=0.004182 Jy/beam ! Combined flux in latest and established models = 2.04888 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 11 model components to the UV plane model. ! The established model now contains 98 components and 2.04888 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.488564Jy sigma=0.966048 ! Fit after self-cal, rms=0.488422Jy sigma=0.959816 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 1908-201_S ! Writing UV FITS file: 1908-201_S.uvf ! Writing 98 model components to file: 1908-201_S.mod ! wwins: Wrote 3 windows to 1908-201_S.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 2.356 x 4.845 at 2.662 degrees (North through East) ! Clean map min=-0.016219 max=1.0947 Jy/beam ! Writing clean map to FITS file: 1908-201_S.fits ! Writing difmap environment to: 1908-201_S.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 1908-201_S] device 1908-201_Suv.ps/vps,1,2 ! Attempting to open device: '1908-201_Suv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 1908-201_Sim.ps/vps ! Attempting to open device: '1908-201_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=2.356 mas, bmaj=4.845 mas, bpa=2.662 degrees ! Estimated noise=2.48723 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 2.356 x 4.845 at 2.662 degrees (North through East) ! Clean map min=-0.016219 max=1.0947 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo8-0.4] quit ! Quitting program ! Log file 1908-201_S.log closed on Fri Apr 24 14:57:58 2009