! Started logfile: 1342+663_X.log on Fri Jul 22 10:03:06 2005 observe 1342+663_X.edt ! Reading UV FITS file: 1342+663_X.edt ! AN table 1: 31 integrations on 171 of 171 possible baselines. ! AN table 2: 30 integrations on 171 of 171 possible baselines. ! AN table 3: 81 integrations on 171 of 171 possible baselines. ! AN table 4: 38 integrations on 171 of 171 possible baselines. ! Apparent sampling: 0.171767 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 1342+663 ! ! 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 1818 lines of history. ! ! Reading 21148 visibilities. ![@gonzo8-0.1 1342+663_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 = 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 0.100x0.100 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 376 telescope corrections were flagged in sub-array 1. ! A total of 423 telescope corrections were flagged in sub-array 2. ! A total of 979 telescope corrections were flagged in sub-array 3. ! A total of 517 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 376 telescope corrections were flagged in sub-array 1. ! A total of 423 telescope corrections were flagged in sub-array 2. ! A total of 979 telescope corrections were flagged in sub-array 3. ! A total of 517 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 377 telescope corrections were flagged in sub-array 1. ! A total of 423 telescope corrections were flagged in sub-array 2. ! A total of 979 telescope corrections were flagged in sub-array 3. ! A total of 518 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 376 telescope corrections were flagged in sub-array 1. ! A total of 424 telescope corrections were flagged in sub-array 2. ! A total of 979 telescope corrections were flagged in sub-array 3. ! A total of 517 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=0.454244Jy sigma=0.007746 ! Fit after self-cal, rms=0.454003Jy sigma=0.007744 ! 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=0.8216 mas, bmaj=0.9781 mas, bpa=21.41 degrees ! Estimated noise=624.05 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) ! Added new window around map position (0, 0). ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.402626 Jy ! Total flux subtracted in 50 components = 0.402626 Jy ! Clean residual min=-0.022364 max=0.128466 Jy/beam ! Clean residual mean=-0.000029 rms=0.007390 Jy/beam ! Combined flux in latest and established models = 0.402626 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 0.402626 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.232979Jy sigma=0.004254 ! Fit after self-cal, rms=0.232929Jy sigma=0.004254 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.129764 Jy ! Total flux subtracted in 50 components = 0.129764 Jy ! Clean residual min=-0.013309 max=0.053960 Jy/beam ! Clean residual mean=-0.000025 rms=0.004044 Jy/beam ! Combined flux in latest and established models = 0.532391 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 10 components and 0.532391 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.141873Jy sigma=0.002549 ! Fit after self-cal, rms=0.141392Jy sigma=0.002544 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0625079 Jy ! Total flux subtracted in 50 components = 0.0625079 Jy ! Clean residual min=-0.010448 max=0.031316 Jy/beam ! Clean residual mean=-0.000024 rms=0.002803 Jy/beam ! Combined flux in latest and established models = 0.594898 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 22 components and 0.594898 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.107845Jy sigma=0.001891 ! Fit after self-cal, rms=0.107581Jy sigma=0.001889 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0382324 Jy ! Total flux subtracted in 50 components = 0.0382323 Jy ! Clean residual min=-0.009492 max=0.019779 Jy/beam ! Clean residual mean=-0.000023 rms=0.002149 Jy/beam ! Combined flux in latest and established models = 0.633131 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 31 components and 0.633131 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.092419Jy sigma=0.001581 ! Fit after self-cal, rms=0.092217Jy sigma=0.001579 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0245849 Jy ! Total flux subtracted in 50 components = 0.0245849 Jy ! Clean residual min=-0.009029 max=0.012864 Jy/beam ! Clean residual mean=-0.000022 rms=0.001792 Jy/beam ! Combined flux in latest and established models = 0.657716 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 33 components and 0.657716 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.085627Jy sigma=0.001439 ! Fit after self-cal, rms=0.085458Jy sigma=0.001437 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0162081 Jy ! Total flux subtracted in 50 components = 0.0162081 Jy ! Clean residual min=-0.008596 max=0.008339 Jy/beam ! Clean residual mean=-0.000022 rms=0.001602 Jy/beam ! Combined flux in latest and established models = 0.673924 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 34 components and 0.673924 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.082717Jy sigma=0.001376 ! Fit after self-cal, rms=0.082606Jy sigma=0.001374 ! 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=1.115 mas, bmaj=1.276 mas, bpa=10.98 degrees ! Estimated noise=317.11 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 = 0.0123443 Jy ! Component: 100 - total flux cleaned = 0.0181037 Jy ! Total flux subtracted in 100 components = 0.0181037 Jy ! Clean residual min=-0.005743 max=0.005576 Jy/beam ! Clean residual mean=-0.000096 rms=0.001314 Jy/beam ! Combined flux in latest and established models = 0.692027 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 40 components and 0.692027 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081257Jy sigma=0.001340 ! Fit after self-cal, rms=0.081188Jy sigma=0.001340 ! 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 0.98 FD 0.97 GC 0.96 HH 1.00* ! HN 0.97 KK 1.00* KP 0.99 LA 1.06 ! MC 1.00* MK 1.00 NL 1.00 NY 0.96 ! ON 1.00* OV 1.00 PT 1.00 SC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 1.00* GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 1.01 LA 1.00 ! MC 1.00* MK 1.00 NL 1.00* NY 1.00* ! ON 1.00* OV 0.97 PT 0.97 SC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 1.01 GC 1.00* HH 1.00* ! HN 1.05 KK 1.00* KP 1.03 LA 1.02 ! MC 1.00* MK 1.01 NL 0.99 NY 1.00* ! ON 1.00* OV 1.00 PT 1.00 SC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 FD 0.95 GC 1.00* HH 1.00* ! HN 1.06 KK 1.03 KP 0.98 LA 0.89 ! MC 1.00* MK 1.02 NL 0.98 NY 1.00* ! ON 1.00* OV 0.97 PT 0.97 SC 1.02 ! TS 1.00* WF 1.00* WZ 1.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.96 GC 1.00 HH 1.00* ! HN 0.95 KK 1.00* KP 0.99 LA 1.06 ! MC 1.00* MK 0.98 NL 1.00 NY 0.93 ! ON 1.00* OV 1.01 PT 1.01 SC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 FD 1.00* GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 1.02 LA 1.03 ! MC 1.00* MK 1.01 NL 1.00* NY 1.00* ! ON 1.00* OV 0.97 PT 0.98 SC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.01 GC 1.00* HH 1.00* ! HN 1.04 KK 1.00* KP 1.01 LA 1.03 ! MC 1.00* MK 0.99 NL 0.99 NY 1.00* ! ON 1.00* OV 0.99 PT 1.01 SC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 FD 0.92 GC 1.00* HH 1.00* ! HN 1.06 KK 1.08 KP 0.99 LA 0.87 ! MC 1.00* MK 1.00 NL 0.99 NY 1.00* ! ON 1.00* OV 0.97 PT 0.99 SC 1.02 ! TS 1.00* WF 1.00* WZ 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.96 GC 0.97 HH 1.00* ! HN 0.96 KK 1.00* KP 1.00 LA 1.08 ! MC 1.00* MK 0.98 NL 1.00 NY 0.99 ! ON 1.00* OV 0.99 PT 0.99 SC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 1.00* GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 1.00 LA 1.02 ! MC 1.00* MK 1.03 NL 1.00* NY 1.00* ! ON 1.00* OV 0.98 PT 0.99 SC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 0.99 GC 1.00* HH 1.00* ! HN 1.01 KK 1.00* KP 1.01 LA 1.04 ! MC 1.00* MK 1.00 NL 0.98 NY 1.00* ! ON 1.00* OV 1.00 PT 1.02 SC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 FD 0.95 GC 1.00* HH 1.00* ! HN 1.07 KK 1.03 KP 0.98 LA 0.88 ! MC 1.00* MK 1.05 NL 0.98 NY 1.00* ! ON 1.00* OV 0.98 PT 0.98 SC 1.03 ! TS 1.00* WF 1.00* WZ 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.96 GC 1.02 HH 1.00* ! HN 0.96 KK 1.00* KP 0.98 LA 1.09 ! MC 1.00* MK 0.99 NL 1.00 NY 0.97 ! ON 1.00* OV 1.00 PT 0.99 SC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 FD 1.00* GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 1.01 LA 1.04 ! MC 1.00* MK 1.05 NL 1.00* NY 1.00* ! ON 1.00* OV 0.99 PT 0.98 SC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 FD 1.01 GC 1.00* HH 1.00* ! HN 1.11 KK 1.00* KP 1.01 LA 1.03 ! MC 1.00* MK 1.03 NL 1.01 NY 1.00* ! ON 1.00* OV 1.00 PT 1.01 SC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 FD 0.93 GC 1.00* HH 1.00* ! HN 1.07 KK 1.06 KP 0.99 LA 0.88 ! MC 1.00* MK 1.03 NL 0.97 NY 1.00* ! ON 1.00* OV 0.96 PT 0.99 SC 1.09 ! TS 1.00* WF 1.00* WZ 1.00* ! ! ! Fit before self-cal, rms=0.081188Jy sigma=0.001340 ! Fit after self-cal, rms=0.075864Jy sigma=0.001226 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=1.121 mas, bmaj=1.283 mas, bpa=10.78 degrees ! Estimated noise=317.147 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 = -0.000935268 Jy ! Component: 100 - total flux cleaned = -0.00102945 Jy ! Total flux subtracted in 100 components = -0.00102945 Jy ! Clean residual min=-0.002881 max=0.003074 Jy/beam ! Clean residual mean=-0.000039 rms=0.000761 Jy/beam ! Combined flux in latest and established models = 0.690998 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 46 components and 0.690998 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.075723Jy sigma=0.001224 ! Fit after self-cal, rms=0.075706Jy sigma=0.001223 ! 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 = -0.000314334 Jy ! Component: 100 - total flux cleaned = -0.000312125 Jy ! Total flux subtracted in 100 components = -0.000312125 Jy ! Clean residual min=-0.002874 max=0.003061 Jy/beam ! Clean residual mean=-0.000040 rms=0.000754 Jy/beam ! Combined flux in latest and established models = 0.690686 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 7 model components to the UV plane model. ! The established model now contains 46 components and 0.690686 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.075615Jy sigma=0.001222 ! Fit after self-cal, rms=0.072956Jy sigma=0.001172 ! Inverting map and beam ! Estimated beam: bmin=1.119 mas, bmaj=1.284 mas, bpa=10.19 degrees ! Estimated noise=317.252 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 = 0.00122372 Jy ! Component: 100 - total flux cleaned = 0.00121421 Jy ! Total flux subtracted in 100 components = 0.00121421 Jy ! Clean residual min=-0.001848 max=0.002162 Jy/beam ! Clean residual mean=-0.000003 rms=0.000450 Jy/beam ! Combined flux in latest and established models = 0.6919 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 4 model components to the UV plane model. ! The established model now contains 46 components and 0.6919 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.072859Jy sigma=0.001171 ! Fit after self-cal, rms=0.072848Jy sigma=0.001171 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 1342+663_X ! Writing UV FITS file: 1342+663_X.uvf ! Writing 46 model components to file: 1342+663_X.mod ! wwins: Wrote 1 windows to 1342+663_X.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.119 x 1.284 at 10.19 degrees (North through East) ! Clean map min=-0.0018357 max=0.56008 Jy/beam ! Writing clean map to FITS file: 1342+663_X.fits ! Writing difmap environment to: 1342+663_X.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 1342+663_X] device 1342+663_Xuv.ps/vps,1,2 ! Attempting to open device: '1342+663_Xuv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 1342+663_Xim.ps/vps ! Attempting to open device: '1342+663_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=1.119 mas, bmaj=1.284 mas, bpa=10.19 degrees ! Estimated noise=317.252 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.119 x 1.284 at 10.19 degrees (North through East) ! Clean map min=-0.0018357 max=0.56008 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo8-0.1] quit ! Quitting program ! Log file 1342+663_X.log closed on Fri Jul 22 10:04:13 2005