! Started logfile: 1749+096_S.log on Fri Aug 19 11:58:38 2005 observe 1749+096_S.edt ! Reading UV FITS file: 1749+096_S.edt ! AN table 1: 17 integrations on 171 of 171 possible baselines. ! AN table 2: 88 integrations on 171 of 171 possible baselines. ! AN table 3: 40 integrations on 171 of 171 possible baselines. ! Apparent sampling: 0.10002 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 1749+096 ! ! 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 9920 visibilities. ![@gonzo7-0.4 1749+096_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 323 telescope corrections were flagged in sub-array 1. ! A total of 1457 telescope corrections were flagged in sub-array 2. ! A total of 658 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 323 telescope corrections were flagged in sub-array 1. ! A total of 1457 telescope corrections were flagged in sub-array 2. ! A total of 654 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 323 telescope corrections were flagged in sub-array 1. ! A total of 1478 telescope corrections were flagged in sub-array 2. ! A total of 659 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 323 telescope corrections were flagged in sub-array 1. ! A total of 1472 telescope corrections were flagged in sub-array 2. ! A total of 654 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=0.589486Jy sigma=0.009409 ! Fit after self-cal, rms=0.591579Jy sigma=0.009459 ! 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=2.397 mas, bmaj=6.518 mas, bpa=-4.947 degrees ! Estimated noise=927.933 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 = 1.19574 Jy ! Total flux subtracted in 50 components = 1.19574 Jy ! Clean residual min=-0.053313 max=0.333497 Jy/beam ! Clean residual mean=-0.000366 rms=0.016519 Jy/beam ! Combined flux in latest and established models = 1.19574 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 1.19574 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.406912Jy sigma=0.006515 ! Fit after self-cal, rms=0.406912Jy sigma=0.006515 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.272781 Jy ! Total flux subtracted in 50 components = 0.272781 Jy ! Clean residual min=-0.021321 max=0.100542 Jy/beam ! Clean residual mean=-0.000183 rms=0.006998 Jy/beam ! Combined flux in latest and established models = 1.46852 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 1.46852 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.187183Jy sigma=0.002974 ! Fit after self-cal, rms=0.187104Jy sigma=0.002973 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.104026 Jy ! Total flux subtracted in 50 components = 0.104026 Jy ! Clean residual min=-0.014230 max=0.045474 Jy/beam ! Clean residual mean=-0.000111 rms=0.004314 Jy/beam ! Combined flux in latest and established models = 1.57255 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 1.57255 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.129988Jy sigma=0.002026 ! Fit after self-cal, rms=0.129760Jy sigma=0.002023 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0486897 Jy ! Total flux subtracted in 50 components = 0.0486897 Jy ! Clean residual min=-0.014509 max=0.027350 Jy/beam ! Clean residual mean=-0.000077 rms=0.003446 Jy/beam ! Combined flux in latest and established models = 1.62124 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 22 components and 1.62124 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.114023Jy sigma=0.001751 ! Fit after self-cal, rms=0.113853Jy sigma=0.001749 ! Inverting map ! Added new window around map position (4.4, 6). ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0294382 Jy ! Total flux subtracted in 50 components = 0.0294382 Jy ! Clean residual min=-0.013235 max=0.015439 Jy/beam ! Clean residual mean=-0.000057 rms=0.003085 Jy/beam ! Combined flux in latest and established models = 1.65068 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 30 components and 1.65068 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.107442Jy sigma=0.001637 ! Fit after self-cal, rms=0.107254Jy sigma=0.001634 ! 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=3.049 mas, bmaj=7.248 mas, bpa=-5.629 degrees ! Estimated noise=713.3 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 = 0.0244426 Jy ! Component: 100 - total flux cleaned = 0.0394533 Jy ! Total flux subtracted in 100 components = 0.0394533 Jy ! Clean residual min=-0.010300 max=0.012818 Jy/beam ! Clean residual mean=-0.000031 rms=0.002482 Jy/beam ! Combined flux in latest and established models = 1.69013 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 20 model components to the UV plane model. ! The established model now contains 48 components and 1.69013 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.102044Jy sigma=0.001545 ! Fit after self-cal, rms=0.101885Jy sigma=0.001543 ! 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* HH 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* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 9 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 1.01 GC 1.00* HH 1.00* ! HN 1.03 KK 1.00* KP 1.01 LA 1.01 ! MC 1.00* MK 0.97 NL 1.01 NY 1.00* ! ON 1.00* OV 0.99 PT 0.99 SC 0.98 ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 1.02 GC 1.00* HH 1.00* ! HN 0.99 KK 1.03 KP 1.02 LA 0.98 ! MC 1.00* MK 0.97 NL 1.00 NY 1.00* ! ON 1.00* OV 0.95 PT 1.00 SC 1.00* ! TS 1.01 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* HH 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* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 9 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 1.01 GC 1.00* HH 1.00* ! HN 1.03 KK 1.00* KP 1.01 LA 1.02 ! MC 1.00* MK 1.03 NL 1.00 NY 1.00* ! ON 1.00* OV 0.98 PT 0.97 SC 1.02 ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.01 GC 1.00* HH 1.00* ! HN 1.01 KK 1.00 KP 0.99 LA 0.97 ! MC 1.00* MK 1.02 NL 1.00 NY 1.00* ! ON 1.00* OV 0.99 PT 0.98 SC 1.00* ! TS 0.94 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* HH 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* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 9 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.91 FD 1.00 GC 1.00* HH 1.00* ! HN 1.01 KK 1.00* KP 1.01 LA 1.00* ! MC 1.00* MK 0.97 NL 1.00 NY 1.00* ! ON 1.00* OV 0.99 PT 0.97 SC 1.05 ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 FD 1.01 GC 1.00* HH 1.00* ! HN 1.00 KK 1.01 KP 0.98 LA 1.03 ! MC 1.00* MK 0.98 NL 1.01 NY 1.00* ! ON 1.00* OV 0.98 PT 0.98 SC 1.00* ! TS 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* HH 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* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 9 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.90 FD 0.97 GC 1.00* HH 1.00* ! HN 1.01 KK 1.00* KP 1.02 LA 1.00 ! MC 1.00* MK 0.96 NL 1.00 NY 1.00* ! ON 1.00* OV 0.86 PT 0.97 SC 1.05 ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 1.00 GC 1.00* HH 1.00* ! HN 1.03 KK 1.04 KP 0.97 LA 0.98 ! MC 1.00* MK 0.99 NL 0.99 NY 1.00* ! ON 1.00* OV 0.98 PT 1.02 SC 1.00* ! TS 1.03 WF 1.00* WZ 1.00* ! ! ! Fit before self-cal, rms=0.101885Jy sigma=0.001543 ! Fit after self-cal, rms=0.086662Jy sigma=0.001275 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=3.068 mas, bmaj=7.284 mas, bpa=-5.53 degrees ! Estimated noise=714.606 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 = 0.00730139 Jy ! Component: 100 - total flux cleaned = 0.00813097 Jy ! Total flux subtracted in 100 components = 0.00813097 Jy ! Clean residual min=-0.005357 max=0.005760 Jy/beam ! Clean residual mean=-0.000005 rms=0.001360 Jy/beam ! Combined flux in latest and established models = 1.69826 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 54 components and 1.69826 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.086120Jy sigma=0.001266 ! Fit after self-cal, rms=0.086081Jy sigma=0.001265 ! 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 = 0.000836451 Jy ! Component: 100 - total flux cleaned = 0.00092659 Jy ! Total flux subtracted in 100 components = 0.00092659 Jy ! Clean residual min=-0.005304 max=0.005814 Jy/beam ! Clean residual mean=-0.000005 rms=0.001350 Jy/beam ! Combined flux in latest and established models = 1.69919 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 9 model components to the UV plane model. ! The established model now contains 61 components and 1.69919 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.085965Jy sigma=0.001263 ! Fit after self-cal, rms=0.081279Jy sigma=0.001184 ! Inverting map and beam ! Estimated beam: bmin=3.071 mas, bmaj=7.28 mas, bpa=-5.542 degrees ! Estimated noise=715.047 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 = 0.0018712 Jy ! Component: 100 - total flux cleaned = 0.00220292 Jy ! Total flux subtracted in 100 components = 0.00220292 Jy ! Clean residual min=-0.004039 max=0.004736 Jy/beam ! Clean residual mean=0.000012 rms=0.000999 Jy/beam ! Combined flux in latest and established models = 1.70139 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 74 components and 1.70139 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081171Jy sigma=0.001183 ! Fit after self-cal, rms=0.081163Jy sigma=0.001182 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 1749+096_S ! Writing UV FITS file: 1749+096_S.uvf ! Writing 74 model components to file: 1749+096_S.mod ! wwins: Wrote 2 windows to 1749+096_S.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.071 x 7.28 at -5.542 degrees (North through East) ! Clean map min=-0.0038905 max=1.5497 Jy/beam ! Writing clean map to FITS file: 1749+096_S.fits ! Writing difmap environment to: 1749+096_S.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 1749+096_S] device 1749+096_Suv.ps/vps,1,2 ! Attempting to open device: '1749+096_Suv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 1749+096_Sim.ps/vps ! Attempting to open device: '1749+096_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=3.071 mas, bmaj=7.28 mas, bpa=-5.542 degrees ! Estimated noise=715.047 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.071 x 7.28 at -5.542 degrees (North through East) ! Clean map min=-0.0038905 max=1.5497 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo7-0.4] quit ! Quitting program ! Log file 1749+096_S.log closed on Fri Aug 19 11:59:37 2005