! Started logfile: 1954-388_S.log on Tue Aug 26 14:59:25 2008 observe 1954-388_S.edt2 ! Reading UV FITS file: 1954-388_S.edt2 ! AN table 1: 18 integrations on 171 of 171 possible baselines. ! Apparent sampling: 0.103639 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 1954-388 ! ! 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 1615 lines of history. ! ! Reading 1276 visibilities. ![@gonzo5-0.4 1954-388_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 = 5.0 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 255 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 255 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 255 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 255 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.178503Jy sigma=3.019792 ! Fit after self-cal, rms=0.177386Jy sigma=3.013903 ! 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=2.467 mas, bmaj=6.908 mas, bpa=-12.03 degrees ! Estimated noise=3.6566 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 = 0.739724 Jy ! Total flux subtracted in 50 components = 0.739724 Jy ! Clean residual min=-0.070722 max=0.206296 Jy/beam ! Clean residual mean=-0.000323 rms=0.026506 Jy/beam ! Combined flux in latest and established models = 0.739724 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 0.739724 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.314197Jy sigma=4.426773 ! Fit after self-cal, rms=0.314197Jy sigma=4.426774 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.163786 Jy ! Total flux subtracted in 50 components = 0.163786 Jy ! Clean residual min=-0.048463 max=0.054883 Jy/beam ! Clean residual mean=-0.000261 rms=0.013821 Jy/beam ! Combined flux in latest and established models = 0.90351 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 7 components and 0.90351 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.201685Jy sigma=2.897275 ! Fit after self-cal, rms=0.201649Jy sigma=2.897082 ! 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=3.586 mas, bmaj=10.38 mas, bpa=3.162 degrees ! Estimated noise=1.89418 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 = 0.0749015 Jy ! Component: 100 - total flux cleaned = 0.104045 Jy ! Total flux subtracted in 100 components = 0.104045 Jy ! Clean residual min=-0.034191 max=0.036138 Jy/beam ! Clean residual mean=-0.000680 rms=0.010870 Jy/beam ! Combined flux in latest and established models = 1.00755 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 33 components and 1.00756 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.170668Jy sigma=2.936867 ! Fit after self-cal, rms=0.170622Jy sigma=2.936515 ! 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 1.09 GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 0.90 LA 1.08 ! MA 1.00* MK 1.00 NL 0.97 NY 1.00* ! OV 1.03 PT 1.01 SC 0.84 TS 1.00* ! WF 1.00* WZ 1.00* GG 1.00* ! ! ! Correcting IF 2. ! A total of 12 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.98 GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 1.11 LA 1.22 ! MA 1.00* MK 1.02 NL 1.07 NY 1.00* ! OV 0.97 PT 0.84 SC 0.99 TS 1.00* ! WF 1.00* WZ 1.00* GG 1.00* ! ! ! Correcting IF 3. ! A total of 12 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.97 GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 1.11 LA 0.91 ! MA 1.00* MK 1.10 NL 1.04 NY 1.00* ! OV 1.03 PT 0.93 SC 1.15 TS 1.00* ! WF 1.00* WZ 1.00* GG 1.00* ! ! ! Correcting IF 4. ! A total of 12 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.86 GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 1.10 LA 0.80 ! MA 1.00* MK 0.98 NL 1.06 NY 1.00* ! OV 1.00 PT 0.90 SC 1.13 TS 1.00* ! WF 1.00* WZ 1.00* GG 1.00* ! ! ! Fit before self-cal, rms=0.170622Jy sigma=2.936515 ! Fit after self-cal, rms=0.109844Jy sigma=1.291545 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=3.537 mas, bmaj=10.22 mas, bpa=3.442 degrees ! Estimated noise=1.93334 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 = 0.00603409 Jy ! Component: 100 - total flux cleaned = 0.00653731 Jy ! Total flux subtracted in 100 components = 0.00653731 Jy ! Clean residual min=-0.014779 max=0.012520 Jy/beam ! Clean residual mean=-0.000323 rms=0.003892 Jy/beam ! Combined flux in latest and established models = 1.01409 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 38 components and 1.01409 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.109231Jy sigma=1.292385 ! Fit after self-cal, rms=0.109192Jy sigma=1.291720 ! 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 = 0.000579167 Jy ! Component: 100 - total flux cleaned = 0.000709548 Jy ! Total flux subtracted in 100 components = 0.000709548 Jy ! Clean residual min=-0.014513 max=0.012355 Jy/beam ! Clean residual mean=-0.000319 rms=0.003856 Jy/beam ! Combined flux in latest and established models = 1.0148 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 4 model components to the UV plane model. ! The established model now contains 41 components and 1.0148 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.108891Jy sigma=1.290922 ! Fit after self-cal, rms=0.103236Jy sigma=1.166967 ! Inverting map and beam ! Estimated beam: bmin=3.532 mas, bmaj=10.22 mas, bpa=3.505 degrees ! Estimated noise=1.93777 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 = 0.004221 Jy ! Component: 100 - total flux cleaned = 0.00460439 Jy ! Total flux subtracted in 100 components = 0.00460439 Jy ! Clean residual min=-0.009940 max=0.010687 Jy/beam ! Clean residual mean=-0.000240 rms=0.002888 Jy/beam ! Combined flux in latest and established models = 1.01941 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 45 components and 1.01941 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.102870Jy sigma=1.165698 ! Fit after self-cal, rms=0.102807Jy sigma=1.165294 ! Inverting map ! Added new window around map position (-15.6, 8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0104076 Jy ! Component: 100 - total flux cleaned = 0.0157558 Jy ! Total flux subtracted in 100 components = 0.0157558 Jy ! Clean residual min=-0.009590 max=0.008611 Jy/beam ! Clean residual mean=-0.000149 rms=0.002495 Jy/beam ! Combined flux in latest and established models = 1.03516 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 54 components and 1.03516 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.101558Jy sigma=1.160119 ! Fit after self-cal, rms=0.101432Jy sigma=1.155085 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 1954-388_S ! Writing UV FITS file: 1954-388_S.uvf ! Writing 54 model components to file: 1954-388_S.mod ! wwins: Wrote 2 windows to 1954-388_S.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.532 x 10.22 at 3.505 degrees (North through East) ! Clean map min=-0.0089515 max=0.9607 Jy/beam ! Writing clean map to FITS file: 1954-388_S.fits ! Writing difmap environment to: 1954-388_S.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 1954-388_S] device 1954-388_Suv.ps/vps,1,2 ! Attempting to open device: '1954-388_Suv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 1954-388_Sim.ps/vps ! Attempting to open device: '1954-388_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=3.532 mas, bmaj=10.22 mas, bpa=3.505 degrees ! Estimated noise=1.93777 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.532 x 10.22 at 3.505 degrees (North through East) ! Clean map min=-0.0089515 max=0.9607 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo5-0.4] quit ! Quitting program ! Log file 1954-388_S.log closed on Tue Aug 26 14:59:32 2008