! Started logfile: 1656+348_X.log on Wed May 14 14:02:52 2008 observe 1656+348_X.edt ! Reading UV FITS file: 1656+348_X.edt ! AN table 1: 56 integrations on 153 of 153 possible baselines. ! Apparent sampling: 0.0701447 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 1656+348 ! ! 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 946 lines of history. ! ! Reading 2404 visibilities. ![@gonzo8-0.1 1656+348_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 = 8.0 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 931 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 940 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 940 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 955 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.846278Jy sigma=0.016867 ! Fit after self-cal, rms=0.843575Jy sigma=0.016896 ! 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=1.122 mas, bmaj=2.05 mas, bpa=-4.639 degrees ! Estimated noise=3562.46 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 = 0.108523 Jy ! Total flux subtracted in 50 components = 0.108523 Jy ! Clean residual min=-0.017041 max=0.035925 Jy/beam ! Clean residual mean=-0.000237 rms=0.005595 Jy/beam ! Combined flux in latest and established models = 0.108523 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 0.108523 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.064895Jy sigma=0.001298 ! Fit after self-cal, rms=0.064886Jy sigma=0.001298 ! 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=1.752 mas, bmaj=2.305 mas, bpa=6.737 degrees ! Estimated noise=1987.06 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 = 0.0439407 Jy ! Component: 100 - total flux cleaned = 0.0607638 Jy ! Total flux subtracted in 100 components = 0.0607638 Jy ! Clean residual min=-0.007755 max=0.009177 Jy/beam ! Clean residual mean=-0.000052 rms=0.002879 Jy/beam ! Combined flux in latest and established models = 0.169287 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 35 model components to the UV plane model. ! The established model now contains 38 components and 0.169287 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.032002Jy sigma=0.000617 ! Fit after self-cal, rms=0.031942Jy sigma=0.000616 ! 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 9 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.08 FD 0.92 GC 1.22 HH 1.00* ! HN 1.00* KK 1.00* KP 0.91 LA 0.99 ! MC 1.00* MK 0.89 NL 1.02 NY 1.00* ! ON 1.00* OV 1.06 PT 0.89 SC 1.00* ! WF 1.05 WZ 1.00* ! ! ! Correcting IF 2. ! A total of 21 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 0.94 GC 1.00* HH 1.00* ! HN 1.15 KK 1.00* KP 0.93 LA 0.94 ! MC 1.00* MK 1.01 NL 1.12 NY 1.00* ! ON 1.00* OV 0.94 PT 0.96 SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 3. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 0.96 GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 0.93 LA 0.95 ! MC 1.00* MK 0.95 NL 1.15 NY 1.00* ! ON 1.00* OV 1.02 PT 0.95 SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 4. ! A total of 15 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 0.98 LA 0.99 ! MC 1.00* MK 0.82 NL 1.00* NY 1.00* ! ON 1.00* OV 0.95 PT 0.92 SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Fit before self-cal, rms=0.031942Jy sigma=0.000616 ! Fit after self-cal, rms=0.028402Jy sigma=0.000560 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=1.826 mas, bmaj=2.346 mas, bpa=7.664 degrees ! Estimated noise=2070.39 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 = 0.000121148 Jy ! Component: 100 - total flux cleaned = 0.00031373 Jy ! Total flux subtracted in 100 components = 0.00031373 Jy ! Clean residual min=-0.004270 max=0.006389 Jy/beam ! Clean residual mean=-0.000020 rms=0.001519 Jy/beam ! Combined flux in latest and established models = 0.169601 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 0.169601 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.028229Jy sigma=0.000557 ! Fit after self-cal, rms=0.028265Jy sigma=0.000556 ! 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 = 9.13291e-05 Jy ! Component: 100 - total flux cleaned = 0.000192696 Jy ! Total flux subtracted in 100 components = 0.000192696 Jy ! Clean residual min=-0.004338 max=0.006252 Jy/beam ! Clean residual mean=-0.000019 rms=0.001488 Jy/beam ! Combined flux in latest and established models = 0.169793 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 7 model components to the UV plane model. ! The established model now contains 48 components and 0.169793 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.028154Jy sigma=0.000554 ! Fit after self-cal, rms=0.026354Jy sigma=0.000508 ! Inverting map and beam ! Estimated beam: bmin=1.821 mas, bmaj=2.347 mas, bpa=8.316 degrees ! Estimated noise=2082.96 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 = 0.00052963 Jy ! Component: 100 - total flux cleaned = 0.000772609 Jy ! Total flux subtracted in 100 components = 0.000772609 Jy ! Clean residual min=-0.004197 max=0.004913 Jy/beam ! Clean residual mean=0.000006 rms=0.001254 Jy/beam ! Combined flux in latest and established models = 0.170566 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 8 model components to the UV plane model. ! The established model now contains 51 components and 0.170566 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.026244Jy sigma=0.000506 ! Fit after self-cal, rms=0.026244Jy sigma=0.000506 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 1656+348_X ! Writing UV FITS file: 1656+348_X.uvf ! Writing 51 model components to file: 1656+348_X.mod ! wwins: Wrote 1 windows to 1656+348_X.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.821 x 2.347 at 8.316 degrees (North through East) ! Clean map min=-0.0041324 max=0.148 Jy/beam ! Writing clean map to FITS file: 1656+348_X.fits ! Writing difmap environment to: 1656+348_X.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 1656+348_X] device 1656+348_Xuv.ps/vps,1,2 ! Attempting to open device: '1656+348_Xuv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 1656+348_Xim.ps/vps ! Attempting to open device: '1656+348_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=1.821 mas, bmaj=2.347 mas, bpa=8.316 degrees ! Estimated noise=2082.96 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.821 x 2.347 at 8.316 degrees (North through East) ! Clean map min=-0.0041324 max=0.148 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo8-0.1] quit ! Quitting program ! Log file 1656+348_X.log closed on Wed May 14 14:02:59 2008