! Started logfile: 1921-293_X.log on Mon Mar 31 22:54:28 2008 observe 1921-293_X.edt ! Reading UV FITS file: 1921-293_X.edt ! AN table 1: 14 integrations on 136 of 136 possible baselines. ! AN table 2: 39 integrations on 136 of 136 possible baselines. ! AN table 3: 11 integrations on 136 of 136 possible baselines. ! Apparent sampling: 0.0697381 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 1921-293 ! ! 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 1222 lines of history. ! ! Reading 2428 visibilities. ![@gonzo6-0.1 1921-293_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 = 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 0.100x0.100 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 238 telescope corrections were flagged in sub-array 1. ! A total of 511 telescope corrections were flagged in sub-array 2. ! A total of 134 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 238 telescope corrections were flagged in sub-array 1. ! A total of 511 telescope corrections were flagged in sub-array 2. ! A total of 134 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 238 telescope corrections were flagged in sub-array 1. ! A total of 510 telescope corrections were flagged in sub-array 2. ! A total of 127 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 238 telescope corrections were flagged in sub-array 1. ! A total of 510 telescope corrections were flagged in sub-array 2. ! A total of 127 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=7.602909Jy sigma=0.124983 ! Fit after self-cal, rms=7.604406Jy sigma=0.125013 ! 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=0.6393 mas, bmaj=3.052 mas, bpa=-9.365 degrees ! Estimated noise=1905.42 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 = 6.21571 Jy ! Total flux subtracted in 50 components = 6.21571 Jy ! Clean residual min=-0.505786 max=1.871602 Jy/beam ! Clean residual mean=0.012948 rms=0.240150 Jy/beam ! Combined flux in latest and established models = 6.21571 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 6.21571 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=2.813856Jy sigma=0.046828 ! Fit after self-cal, rms=2.814168Jy sigma=0.046816 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.79884 Jy ! Total flux subtracted in 50 components = 1.79884 Jy ! Clean residual min=-0.289938 max=0.801920 Jy/beam ! Clean residual mean=0.007290 rms=0.123193 Jy/beam ! Combined flux in latest and established models = 8.01455 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 19 model components to the UV plane model. ! The established model now contains 24 components and 8.01455 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.511710Jy sigma=0.024915 ! Fit after self-cal, rms=1.512240Jy sigma=0.024876 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.886755 Jy ! Total flux subtracted in 50 components = 0.886755 Jy ! Clean residual min=-0.205530 max=0.413106 Jy/beam ! Clean residual mean=0.004519 rms=0.072095 Jy/beam ! Combined flux in latest and established models = 8.9013 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 35 components and 8.9013 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.932999Jy sigma=0.015025 ! Fit after self-cal, rms=0.933823Jy sigma=0.014983 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.465555 Jy ! Total flux subtracted in 50 components = 0.465555 Jy ! Clean residual min=-0.165202 max=0.219562 Jy/beam ! Clean residual mean=0.003062 rms=0.050020 Jy/beam ! Combined flux in latest and established models = 9.36686 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 21 model components to the UV plane model. ! The established model now contains 49 components and 9.36686 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.672924Jy sigma=0.010485 ! Fit after self-cal, rms=0.674017Jy sigma=0.010439 ! 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=0.7847 mas, bmaj=3.931 mas, bpa=-12.38 degrees ! Estimated noise=1105.69 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 = 0.362454 Jy ! Component: 100 - total flux cleaned = 0.551651 Jy ! Total flux subtracted in 100 components = 0.551651 Jy ! Clean residual min=-0.126417 max=0.232239 Jy/beam ! Clean residual mean=0.003362 rms=0.053579 Jy/beam ! Combined flux in latest and established models = 9.91851 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 48 model components to the UV plane model. ! The established model now contains 88 components and 9.91851 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.478637Jy sigma=0.006948 ! Fit after self-cal, rms=0.479321Jy sigma=0.006937 ! 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 0.00* FD 0.00* GC 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 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* WF 0.00* ! WZ 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 1.01 GC 1.00* HN 1.00* ! KK 0.99 KP 0.99 LA 0.98 MC 1.00* ! MK 0.98 NL 0.99 NY 1.00* ON 1.00* ! OV 1.00 PT 0.99 SC 1.04 WF 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 1.00 GC 1.00* HN 1.00* ! KK 1.00* KP 0.98 LA 0.98 MC 1.00* ! MK 1.00* NL 0.97 NY 1.00* ON 1.00* ! OV 1.01 PT 1.00 SC 1.00* WF 1.00* ! WZ 1.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* GC 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 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* WF 0.00* ! WZ 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 1.01 GC 1.00* HN 1.00* ! KK 0.99 KP 0.99 LA 0.98 MC 1.00* ! MK 0.98 NL 0.99 NY 1.00* ON 1.00* ! OV 1.00 PT 0.99 SC 1.04 WF 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 1.00 GC 1.00* HN 1.00* ! KK 1.00* KP 0.98 LA 0.98 MC 1.00* ! MK 1.00* NL 0.97 NY 1.00* ON 1.00* ! OV 1.01 PT 1.00 SC 1.00* WF 1.00* ! WZ 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* GC 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 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* WF 0.00* ! WZ 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 1.01 GC 1.00* HN 1.00* ! KK 1.00 KP 0.99 LA 0.98 MC 1.00* ! MK 0.99 NL 0.99 NY 1.00* ON 1.00* ! OV 1.00 PT 0.99 SC 1.01 WF 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 1.00 GC 1.00* HN 1.00* ! KK 0.97 KP 0.98 LA 0.98 MC 1.00* ! MK 1.00* NL 0.96 NY 1.00* ON 1.00* ! OV 1.01 PT 1.00 SC 1.00* WF 1.00* ! WZ 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* GC 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 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* WF 0.00* ! WZ 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 1.01 GC 1.00* HN 1.00* ! KK 1.00 KP 0.99 LA 0.98 MC 1.00* ! MK 0.99 NL 0.99 NY 1.00* ON 1.00* ! OV 1.00 PT 0.99 SC 1.00 WF 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 1.00 GC 1.00* HN 1.00* ! KK 0.97 KP 0.98 LA 0.98 MC 1.00* ! MK 1.00* NL 0.96 NY 1.00* ON 1.00* ! OV 1.01 PT 1.00 SC 1.00* WF 1.00* ! WZ 1.00* ! ! ! Fit before self-cal, rms=0.479321Jy sigma=0.006937 ! Fit after self-cal, rms=0.445941Jy sigma=0.006513 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.7837 mas, bmaj=3.955 mas, bpa=-12.46 degrees ! Estimated noise=1092.12 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 = 0.0879805 Jy ! Component: 100 - total flux cleaned = 0.105098 Jy ! Total flux subtracted in 100 components = 0.105098 Jy ! Clean residual min=-0.105488 max=0.200165 Jy/beam ! Clean residual mean=0.002015 rms=0.039613 Jy/beam ! Combined flux in latest and established models = 10.0236 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 95 components and 10.0236 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.430857Jy sigma=0.006263 ! Fit after self-cal, rms=0.431315Jy sigma=0.006260 ! 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 (3.5, 1.7). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.175435 Jy ! Component: 100 - total flux cleaned = 0.255512 Jy ! Total flux subtracted in 100 components = 0.255512 Jy ! Clean residual min=-0.106437 max=0.104535 Jy/beam ! Clean residual mean=0.000898 rms=0.028626 Jy/beam ! Combined flux in latest and established models = 10.2791 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 26 model components to the UV plane model. ! The established model now contains 120 components and 10.2791 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.358325Jy sigma=0.005066 ! Fit after self-cal, rms=0.327527Jy sigma=0.004635 ! Inverting map and beam ! Estimated beam: bmin=0.7819 mas, bmaj=3.945 mas, bpa=-12.46 degrees ! Estimated noise=1091.87 mJy/beam. ! Added new window around map position (9.2, -6.7). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.111196 Jy ! Component: 100 - total flux cleaned = 0.17738 Jy ! Total flux subtracted in 100 components = 0.17738 Jy ! Clean residual min=-0.062822 max=0.077183 Jy/beam ! Clean residual mean=0.000916 rms=0.019992 Jy/beam ! Combined flux in latest and established models = 10.4565 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 25 model components to the UV plane model. ! The established model now contains 144 components and 10.4565 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.288601Jy sigma=0.003962 ! Fit after self-cal, rms=0.274164Jy sigma=0.003791 ! Inverting map and beam ! Estimated beam: bmin=0.7815 mas, bmaj=3.941 mas, bpa=-12.45 degrees ! Estimated noise=1092.16 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 = 0.0681587 Jy ! Component: 100 - total flux cleaned = 0.0989374 Jy ! Total flux subtracted in 100 components = 0.0989374 Jy ! Clean residual min=-0.053363 max=0.063511 Jy/beam ! Clean residual mean=0.000652 rms=0.016437 Jy/beam ! Combined flux in latest and established models = 10.5554 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 31 model components to the UV plane model. ! The established model now contains 170 components and 10.5554 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.256246Jy sigma=0.003482 ! Fit after self-cal, rms=0.252097Jy sigma=0.003439 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 1921-293_X ! Writing UV FITS file: 1921-293_X.uvf ! Writing 170 model components to file: 1921-293_X.mod ! wwins: Wrote 3 windows to 1921-293_X.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7815 x 3.941 at -12.45 degrees (North through East) ! Clean map min=-0.054066 max=8.1162 Jy/beam ! Writing clean map to FITS file: 1921-293_X.fits ! Writing difmap environment to: 1921-293_X.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 1921-293_X] device 1921-293_Xuv.ps/vps,1,2 ! Attempting to open device: '1921-293_Xuv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 1921-293_Xim.ps/vps ! Attempting to open device: '1921-293_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=0.7815 mas, bmaj=3.941 mas, bpa=-12.45 degrees ! Estimated noise=1092.16 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7815 x 3.941 at -12.45 degrees (North through East) ! Clean map min=-0.054066 max=8.1162 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo6-0.1] quit ! Quitting program ! Log file 1921-293_X.log closed on Mon Mar 31 22:54:34 2008