! Started logfile: 3C446_S.log on Fri Apr 27 21:57:29 2007 observe 3C446_S.edt ! Reading UV FITS file: 3C446_S.edt ! AN table 1: 16 integrations on 153 of 153 possible baselines. ! AN table 2: 49 integrations on 153 of 153 possible baselines. ! AN table 3: 10 integrations on 153 of 153 possible baselines. ! Apparent sampling: 0.138475 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 3C446 ! ! 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 2.22997e+09 8e+06 1 8e+06 ! 02 2 2.25997e+09 8e+06 1 8e+06 ! 03 3 2.34997e+09 8e+06 1 8e+06 ! 04 4 2.36997e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 1912 lines of history. ! ! Reading 6356 visibilities. ![@gonzo7-0.4 3C446_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 198 telescope corrections were flagged in sub-array 1. ! A total of 525 telescope corrections were flagged in sub-array 2. ! A total of 156 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 198 telescope corrections were flagged in sub-array 1. ! A total of 527 telescope corrections were flagged in sub-array 2. ! A total of 156 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 198 telescope corrections were flagged in sub-array 1. ! A total of 525 telescope corrections were flagged in sub-array 2. ! A total of 160 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 199 telescope corrections were flagged in sub-array 1. ! A total of 525 telescope corrections were flagged in sub-array 2. ! A total of 156 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=1.658422Jy sigma=0.023853 ! Fit after self-cal, rms=1.658319Jy sigma=0.023859 ! 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=2.066 mas, bmaj=6.782 mas, bpa=0.9796 degrees ! Estimated noise=1297.17 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 = 1.85479 Jy ! Total flux subtracted in 50 components = 1.85479 Jy ! Clean residual min=-0.137992 max=0.517366 Jy/beam ! Clean residual mean=0.003234 rms=0.047973 Jy/beam ! Combined flux in latest and established models = 1.85479 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 1.85479 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.921074Jy sigma=0.013193 ! Fit after self-cal, rms=0.921073Jy sigma=0.013193 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.425205 Jy ! Total flux subtracted in 50 components = 0.425205 Jy ! Clean residual min=-0.099732 max=0.204256 Jy/beam ! Clean residual mean=0.002348 rms=0.029537 Jy/beam ! Combined flux in latest and established models = 2.27999 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 4 components and 2.27999 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.662492Jy sigma=0.009375 ! Fit after self-cal, rms=0.661035Jy sigma=0.009362 ! Inverting map ! Added new window around map position (2.8, -1.2). ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.211965 Jy ! Total flux subtracted in 50 components = 0.211965 Jy ! Clean residual min=-0.076467 max=0.156883 Jy/beam ! Clean residual mean=0.001920 rms=0.023266 Jy/beam ! Combined flux in latest and established models = 2.49196 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 11 components and 2.49196 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.560230Jy sigma=0.007958 ! Fit after self-cal, rms=0.556632Jy sigma=0.007907 ! 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=3.404 mas, bmaj=6.951 mas, bpa=6.116 degrees ! Estimated noise=656.676 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 = 0.265021 Jy ! Component: 100 - total flux cleaned = 0.407025 Jy ! Total flux subtracted in 100 components = 0.407025 Jy ! Clean residual min=-0.093670 max=0.167955 Jy/beam ! Clean residual mean=-0.001004 rms=0.046033 Jy/beam ! Combined flux in latest and established models = 2.89898 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 31 components and 2.89898 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.430188Jy sigma=0.006162 ! Fit after self-cal, rms=0.428757Jy sigma=0.006139 ! 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: ! FD 1.11 GC 1.01 HH 1.00* HN 1.00* ! LA 1.09 MC 1.00* MK 0.97 NY 1.00* ! ON 1.00* OV 1.08 PT 0.94 SC 1.00* ! TS 1.06 WF 1.00* BR 0.96 KK 1.00* ! KP 0.89 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! FD 1.14 GC 1.01 HH 1.00* HN 1.00* ! LA 0.99 MC 1.00* MK 0.98 NY 1.00* ! ON 1.00* OV 1.16 PT 0.87 SC 1.00* ! TS 1.00* WF 1.00* BR 0.98 KK 1.00* ! KP 0.86 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 1.14 GC 1.00* HH 1.00* HN 0.93 ! LA 1.10 MC 1.00* MK 1.00* NY 1.00* ! ON 1.00* OV 1.00* PT 1.07 SC 1.00* ! TS 1.00* WF 1.03 BR 1.00* KK 1.00* ! KP 0.95 WZ 1.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! FD 0.96 GC 1.00 HH 1.00* HN 1.00* ! LA 1.03 MC 1.00* MK 1.08 NY 1.00* ! ON 1.00* OV 1.10 PT 0.90 SC 1.00* ! TS 1.01 WF 1.00* BR 1.03 KK 1.00* ! KP 0.90 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! FD 0.99 GC 0.98 HH 1.00* HN 1.00* ! LA 0.96 MC 1.00* MK 1.08 NY 1.00* ! ON 1.00* OV 1.19 PT 0.86 SC 1.00* ! TS 1.00* WF 1.00* BR 1.05 KK 1.00* ! KP 0.89 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 1.00 GC 1.00* HH 1.00* HN 0.94 ! LA 1.08 MC 1.00* MK 1.00* NY 1.00* ! ON 1.00* OV 1.00* PT 1.06 SC 1.00* ! TS 1.00* WF 1.02 BR 1.00* KK 1.00* ! KP 1.02 WZ 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! FD 0.90 GC 1.02 HH 1.00* HN 1.00* ! LA 0.91 MC 1.00* MK 1.04 NY 1.00* ! ON 1.00* OV 1.06 PT 0.98 SC 1.00* ! TS 0.98 WF 1.00* BR 1.04 KK 1.00* ! KP 0.92 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! FD 0.97 GC 1.02 HH 1.00* HN 1.00* ! LA 0.87 MC 1.00* MK 1.03 NY 1.00* ! ON 1.00* OV 1.17 PT 0.96 SC 1.00* ! TS 1.00* WF 1.00* BR 1.07 KK 1.00* ! KP 0.93 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 0.94 GC 1.00* HH 1.00* HN 1.23 ! LA 0.94 MC 1.00* MK 1.00* NY 1.00* ! ON 1.00* OV 1.00* PT 1.20 SC 1.00* ! TS 1.00* WF 1.00* BR 1.00* KK 1.00* ! KP 1.00 WZ 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! FD 0.82 GC 1.13 HH 1.00* HN 1.00* ! LA 0.80 MC 1.00* MK 1.01 NY 1.00* ! ON 1.00* OV 0.97 PT 1.00 SC 1.00* ! TS 1.02 WF 1.00* BR 1.00 KK 1.00* ! KP 0.95 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! FD 0.83 GC 1.08 HH 1.00* HN 1.00* ! LA 0.78 MC 1.00* MK 0.98 NY 1.00* ! ON 1.00* OV 0.99 PT 0.97 SC 1.00* ! TS 1.00* WF 1.00* BR 1.00 KK 1.00* ! KP 0.95 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 0.80 GC 1.00* HH 1.00* HN 1.09 ! LA 0.74 MC 1.00* MK 1.00* NY 1.00* ! ON 1.00* OV 1.00* PT 1.09 SC 1.00* ! TS 1.00* WF 1.33 BR 1.00* KK 1.00* ! KP 1.03 WZ 1.00* ! ! ! Fit before self-cal, rms=0.428757Jy sigma=0.006139 ! Fit after self-cal, rms=0.271160Jy sigma=0.003944 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=3.415 mas, bmaj=7.048 mas, bpa=6.233 degrees ! Estimated noise=638.04 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 = 0.0416744 Jy ! Component: 100 - total flux cleaned = 0.0453749 Jy ! Total flux subtracted in 100 components = 0.0453749 Jy ! Clean residual min=-0.048516 max=0.145214 Jy/beam ! Clean residual mean=-0.000489 rms=0.025077 Jy/beam ! Combined flux in latest and established models = 2.94436 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 37 components and 2.94436 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.263787Jy sigma=0.003807 ! Fit after self-cal, rms=0.263349Jy sigma=0.003787 ! 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 (17.6, -14). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.11647 Jy ! Component: 100 - total flux cleaned = 0.16702 Jy ! Total flux subtracted in 100 components = 0.16702 Jy ! Clean residual min=-0.048662 max=0.064308 Jy/beam ! Clean residual mean=-0.000339 rms=0.015824 Jy/beam ! Combined flux in latest and established models = 3.11138 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 28 model components to the UV plane model. ! The established model now contains 65 components and 3.11138 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.214382Jy sigma=0.003027 ! Fit after self-cal, rms=0.197298Jy sigma=0.002752 ! Inverting map and beam ! Estimated beam: bmin=3.414 mas, bmaj=7.049 mas, bpa=6.194 degrees ! Estimated noise=635.058 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 = 0.0466758 Jy ! Component: 100 - total flux cleaned = 0.0710052 Jy ! Total flux subtracted in 100 components = 0.0710052 Jy ! Clean residual min=-0.040408 max=0.052881 Jy/beam ! Clean residual mean=-0.000169 rms=0.012926 Jy/beam ! Combined flux in latest and established models = 3.18238 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 28 model components to the UV plane model. ! The established model now contains 83 components and 3.18238 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.186518Jy sigma=0.002580 ! Fit after self-cal, rms=0.185560Jy sigma=0.002569 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 3C446_S ! Writing UV FITS file: 3C446_S.uvf ! Writing 83 model components to file: 3C446_S.mod ! wwins: Wrote 3 windows to 3C446_S.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.414 x 7.049 at 6.194 degrees (North through East) ! Clean map min=-0.037991 max=2.4462 Jy/beam ! Writing clean map to FITS file: 3C446_S.fits ! Writing difmap environment to: 3C446_S.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 3C446_S] device 3C446_Suv.ps/vps,1,2 ! Attempting to open device: '3C446_Suv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 3C446_Sim.ps/vps ! Attempting to open device: '3C446_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=3.414 mas, bmaj=7.049 mas, bpa=6.194 degrees ! Estimated noise=635.058 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.414 x 7.049 at 6.194 degrees (North through East) ! Clean map min=-0.037991 max=2.4462 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo7-0.4] quit ! Quitting program ! Log file 3C446_S.log closed on Fri Apr 27 21:57:48 2007