! Started logfile: 2155-304_S.log on Wed May 7 16:12:56 2008 observe 2155-304_S.edt ! Reading UV FITS file: 2155-304_S.edt ! AN table 1: 22 integrations on 153 of 153 possible baselines. ! Apparent sampling: 0.0246583 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 2155-304 ! ! 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 955 lines of history. ! ! Reading 332 visibilities. ![@gonzo6-0.4-pw 2155-304_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 = 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 0.400x0.400 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 379 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 385 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 387 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 379 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.666357Jy sigma=0.006116 ! Fit after self-cal, rms=0.659303Jy sigma=0.006328 ! 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 peakw win_mult ! Inverting map and beam ! Estimated beam: bmin=3.713 mas, bmaj=11.92 mas, bpa=4.879 degrees ! Estimated noise=11970.4 mJy/beam. ! Added new window around map position (0, 0). 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=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.269286 Jy ! Total flux subtracted in 50 components = 0.269286 Jy ! Clean residual min=-0.051815 max=0.075218 Jy/beam ! Clean residual mean=-0.000009 rms=0.017067 Jy/beam ! Combined flux in latest and established models = 0.269286 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 2 model components to the UV plane model. ! The established model now contains 2 components and 0.269286 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.109208Jy sigma=0.001037 ! Fit after self-cal, rms=0.109204Jy sigma=0.001037 ! 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=4.28 mas, bmaj=13.71 mas, bpa=4.7 degrees ! Estimated noise=9349.73 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 = 0.0619047 Jy ! Component: 100 - total flux cleaned = 0.0883287 Jy ! Total flux subtracted in 100 components = 0.0883287 Jy ! Clean residual min=-0.021831 max=0.023406 Jy/beam ! Clean residual mean=-0.000040 rms=0.006992 Jy/beam ! Combined flux in latest and established models = 0.357615 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 11 components and 0.357615 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.072235Jy sigma=0.000673 ! Fit after self-cal, rms=0.072194Jy sigma=0.000673 ! 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 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 1.00* GC 1.00* HH 1.00* ! HN 1.02 KK 1.00* KP 0.91 LA 1.10 ! MC 1.00* MK 1.00* NL 0.87 NY 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 0.92 ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.08 FD 1.00* GC 1.00* HH 1.00* ! HN 1.07 KK 1.00* KP 0.94 LA 1.05 ! MC 1.00* MK 1.00* NL 0.75 NY 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.79 FD 1.00* GC 1.00* HH 1.00* ! HN 1.20 KK 1.00* KP 0.94 LA 1.08 ! MC 1.00* MK 1.00* NL 0.97 NY 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 4. ! A total of 9 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 1.00* GC 1.00* HH 1.00* ! HN 1.08 KK 1.00* KP 0.95 LA 1.00* ! MC 1.00* MK 1.00* NL 0.98 NY 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Fit before self-cal, rms=0.072194Jy sigma=0.000673 ! Fit after self-cal, rms=0.059564Jy sigma=0.000570 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=4.407 mas, bmaj=18.97 mas, bpa=-0.9314 degrees ! Estimated noise=10659.8 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 = 0.0062324 Jy ! Component: 100 - total flux cleaned = 0.00641649 Jy ! Total flux subtracted in 100 components = 0.00641649 Jy ! Clean residual min=-0.017737 max=0.016182 Jy/beam ! Clean residual mean=-0.000005 rms=0.005482 Jy/beam ! Combined flux in latest and established models = 0.364031 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 21 components and 0.364031 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.058693Jy sigma=0.000564 ! Fit after self-cal, rms=0.058940Jy sigma=0.000562 ! 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 = 0.000639083 Jy ! Component: 100 - total flux cleaned = 0.000641682 Jy ! Total flux subtracted in 100 components = 0.000641682 Jy ! Clean residual min=-0.017383 max=0.015872 Jy/beam ! Clean residual mean=-0.000005 rms=0.005341 Jy/beam ! Combined flux in latest and established models = 0.364673 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 11 model components to the UV plane model. ! The established model now contains 27 components and 0.364673 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.058544Jy sigma=0.000559 ! Fit after self-cal, rms=0.056895Jy sigma=0.000541 ! Inverting map and beam ! Estimated beam: bmin=4.391 mas, bmaj=19 mas, bpa=-0.9808 degrees ! Estimated noise=10637.7 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 = 0.00357156 Jy ! Component: 100 - total flux cleaned = 0.00370536 Jy ! Total flux subtracted in 100 components = 0.00370536 Jy ! Clean residual min=-0.016502 max=0.015725 Jy/beam ! Clean residual mean=0.000002 rms=0.005102 Jy/beam ! Combined flux in latest and established models = 0.368378 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 28 components and 0.368378 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.056498Jy sigma=0.000538 ! Fit after self-cal, rms=0.056556Jy sigma=0.000538 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 2155-304_S ! Writing UV FITS file: 2155-304_S.uvf ! Writing 28 model components to file: 2155-304_S.mod ! wwins: Wrote 1 windows to 2155-304_S.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 4.391 x 19 at -0.9808 degrees (North through East) ! Clean map min=-0.016187 max=0.33007 Jy/beam ! Writing clean map to FITS file: 2155-304_S.fits ! Writing difmap environment to: 2155-304_S.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 2155-304_S] device 2155-304_Suv.ps/vps,1,2 ! Attempting to open device: '2155-304_Suv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 2155-304_Sim.ps/vps ! Attempting to open device: '2155-304_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=4.391 mas, bmaj=19 mas, bpa=-0.9808 degrees ! Estimated noise=10637.7 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 4.391 x 19 at -0.9808 degrees (North through East) ! Clean map min=-0.016187 max=0.33007 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo6-0.4-pw] quit ! Quitting program ! Log file 2155-304_S.log closed on Wed May 7 16:13:00 2008