! Started logfile: 0119+041_X.log on Tue May 13 18:12:43 2008 observe 0119+041_X.edt ! Reading UV FITS file: 0119+041_X.edt ! AN table 1: 10 integrations on 153 of 153 possible baselines. ! Apparent sampling: 0.0464052 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 0119+041 ! ! 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 938 lines of history. ! ! Reading 284 visibilities. ![@gonzo8-0.1 0119+041_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 162 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 162 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 159 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 165 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.169875Jy sigma=0.002314 ! Fit after self-cal, rms=0.169629Jy sigma=0.002320 ! 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=1.137 mas, bmaj=2.227 mas, bpa=-23.51 degrees ! Estimated noise=4833.46 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 = 0.737699 Jy ! Total flux subtracted in 50 components = 0.737699 Jy ! Clean residual min=-0.082365 max=0.205729 Jy/beam ! Clean residual mean=-0.001097 rms=0.032696 Jy/beam ! Combined flux in latest and established models = 0.737699 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 0.737699 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.277884Jy sigma=0.004001 ! Fit after self-cal, rms=0.277884Jy sigma=0.004001 ! 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=1.145 mas, bmaj=3.151 mas, bpa=-21.44 degrees ! Estimated noise=3736.77 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 = 0.200815 Jy ! Component: 100 - total flux cleaned = 0.285259 Jy ! Total flux subtracted in 100 components = 0.285259 Jy ! Clean residual min=-0.029964 max=0.044468 Jy/beam ! Clean residual mean=-0.000165 rms=0.010429 Jy/beam ! Combined flux in latest and established models = 1.02296 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 27 model components to the UV plane model. ! The established model now contains 27 components and 1.02296 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.110250Jy sigma=0.001502 ! Fit after self-cal, rms=0.110170Jy sigma=0.001501 ! 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 1.00* FD 0.90 GC 1.08 HH 1.00* ! HN 1.00* KK 1.00* KP 0.94 LA 1.05 ! MC 1.00* MK 1.08 NL 0.96 NY 1.00* ! ON 1.00* OV 0.92 PT 0.95 SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 2. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.92 GC 1.10 HH 1.00* ! HN 1.00* KK 1.00* KP 0.93 LA 1.04 ! MC 1.00* MK 1.04 NL 0.95 NY 1.00* ! ON 1.00* OV 0.95 PT 0.97 SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 3. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.92 GC 1.10 HH 1.00* ! HN 1.00* KK 1.00* KP 0.96 LA 1.01 ! MC 1.00* MK 1.06 NL 1.00 NY 1.00* ! ON 1.00* OV 0.97 PT 0.98 SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.96 GC 1.12 HH 1.00* ! HN 1.00* KK 1.00* KP 0.96 LA 1.07 ! MC 1.00* MK 1.04 NL 1.04 NY 1.00* ! ON 1.00* OV 0.94 PT 1.05 SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Fit before self-cal, rms=0.110170Jy sigma=0.001501 ! Fit after self-cal, rms=0.073522Jy sigma=0.000967 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=1.179 mas, bmaj=3.433 mas, bpa=-22.34 degrees ! Estimated noise=3703.13 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 = -0.000452255 Jy ! Component: 100 - total flux cleaned = 0.000240881 Jy ! Total flux subtracted in 100 components = 0.000240881 Jy ! Clean residual min=-0.012609 max=0.014986 Jy/beam ! Clean residual mean=0.000074 rms=0.003944 Jy/beam ! Combined flux in latest and established models = 1.0232 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 11 model components to the UV plane model. ! The established model now contains 38 components and 1.0232 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.071790Jy sigma=0.000938 ! Fit after self-cal, rms=0.071774Jy sigma=0.000937 ! 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 = -0.000367868 Jy ! Component: 100 - total flux cleaned = -0.000374177 Jy ! Total flux subtracted in 100 components = -0.000374177 Jy ! Clean residual min=-0.012024 max=0.014952 Jy/beam ! Clean residual mean=0.000073 rms=0.003768 Jy/beam ! Combined flux in latest and established models = 1.02282 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 12 model components to the UV plane model. ! The established model now contains 44 components and 1.02282 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.071066Jy sigma=0.000924 ! Fit after self-cal, rms=0.071018Jy sigma=0.000921 ! Inverting map and beam ! Estimated beam: bmin=1.181 mas, bmaj=3.428 mas, bpa=-22.35 degrees ! Estimated noise=3708.86 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 = -0.00107727 Jy ! Component: 100 - total flux cleaned = -0.000883718 Jy ! Total flux subtracted in 100 components = -0.000883718 Jy ! Clean residual min=-0.011392 max=0.014621 Jy/beam ! Clean residual mean=0.000074 rms=0.003632 Jy/beam ! Combined flux in latest and established models = 1.02194 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 48 components and 1.02194 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070459Jy sigma=0.000913 ! Fit after self-cal, rms=0.070472Jy sigma=0.000912 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 0119+041_X ! Writing UV FITS file: 0119+041_X.uvf ! Writing 48 model components to file: 0119+041_X.mod ! wwins: Wrote 1 windows to 0119+041_X.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.181 x 3.428 at -22.35 degrees (North through East) ! Clean map min=-0.011154 max=0.93841 Jy/beam ! Writing clean map to FITS file: 0119+041_X.fits ! Writing difmap environment to: 0119+041_X.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 0119+041_X] device 0119+041_Xuv.ps/vps,1,2 ! Attempting to open device: '0119+041_Xuv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 0119+041_Xim.ps/vps ! Attempting to open device: '0119+041_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=1.181 mas, bmaj=3.428 mas, bpa=-22.35 degrees ! Estimated noise=3708.86 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.181 x 3.428 at -22.35 degrees (North through East) ! Clean map min=-0.011154 max=0.93841 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo8-0.1] quit ! Quitting program ! Log file 0119+041_X.log closed on Tue May 13 18:12:50 2008