! Started logfile: 1156+295_X.log on Wed May 14 12:45:09 2008 observe 1156+295_X.edt ! Reading UV FITS file: 1156+295_X.edt ! AN table 1: 39 integrations on 153 of 153 possible baselines. ! Apparent sampling: 0.0514496 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 1156+295 ! ! 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 1228 visibilities. ![@gonzo8-0.1 1156+295_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 584 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 591 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 588 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 562 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=1.249893Jy sigma=0.015704 ! Fit after self-cal, rms=1.237848Jy sigma=0.015635 ! 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=0.5859 mas, bmaj=1.19 mas, bpa=51.53 degrees ! Estimated noise=3246.23 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 = 1.70533 Jy ! Total flux subtracted in 50 components = 1.70533 Jy ! Clean residual min=-0.178535 max=0.475586 Jy/beam ! Clean residual mean=0.000572 rms=0.062368 Jy/beam ! Combined flux in latest and established models = 1.70533 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 1.70533 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.556680Jy sigma=0.007229 ! Fit after self-cal, rms=0.556680Jy sigma=0.007229 ! 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=0.5721 mas, bmaj=1.326 mas, bpa=52.74 degrees ! Estimated noise=2141.98 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 = 0.421157 Jy ! Component: 100 - total flux cleaned = 0.553544 Jy ! Total flux subtracted in 100 components = 0.553544 Jy ! Clean residual min=-0.073537 max=0.073651 Jy/beam ! Clean residual mean=0.002125 rms=0.032612 Jy/beam ! Combined flux in latest and established models = 2.25887 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 16 model components to the UV plane model. ! The established model now contains 16 components and 2.25887 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.177137Jy sigma=0.002178 ! Fit after self-cal, rms=0.177125Jy sigma=0.002178 ! 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 18 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 1.08 GC 1.01 HH 1.00* ! HN 1.00* KK 0.94 KP 0.97 LA 1.00* ! MC 1.00* MK 0.98 NL 1.00* NY 1.01 ! ON 1.00* OV 0.97 PT 1.00* SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 2. ! A total of 27 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 1.07 GC 1.00* HH 1.00* ! HN 1.00* KK 0.97 KP 1.00* LA 1.00* ! MC 1.00* MK 0.96 NL 1.00* NY 1.01 ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 3. ! A total of 18 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 1.11 GC 1.10 HH 1.00* ! HN 1.00* KK 0.95 KP 1.00 LA 1.00* ! MC 1.00* MK 0.96 NL 1.00* NY 1.02 ! ON 1.00* OV 0.95 PT 1.00* SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Correcting IF 4. ! A total of 21 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 1.08 GC 1.11 HH 1.00* ! HN 1.00* KK 0.96 KP 0.96 LA 1.00* ! MC 1.00* MK 0.93 NL 1.00* NY 1.03 ! ON 1.00* OV 1.00 PT 1.04 SC 1.00* ! WF 1.00* WZ 1.00* ! ! ! Fit before self-cal, rms=0.177125Jy sigma=0.002178 ! Fit after self-cal, rms=0.133335Jy sigma=0.001523 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.5809 mas, bmaj=1.27 mas, bpa=53.64 degrees ! Estimated noise=2239.21 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 = 0.0576152 Jy ! Component: 100 - total flux cleaned = 0.0781142 Jy ! Total flux subtracted in 100 components = 0.0781142 Jy ! Clean residual min=-0.025606 max=0.020562 Jy/beam ! Clean residual mean=0.000264 rms=0.006365 Jy/beam ! Combined flux in latest and established models = 2.33699 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 6 model components to the UV plane model. ! The established model now contains 22 components and 2.33699 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.109554Jy sigma=0.001253 ! Fit after self-cal, rms=0.109609Jy sigma=0.001252 ! 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 = 0.00931332 Jy ! Component: 100 - total flux cleaned = 0.0147395 Jy ! Total flux subtracted in 100 components = 0.0147395 Jy ! Clean residual min=-0.024907 max=0.021066 Jy/beam ! Clean residual mean=0.000172 rms=0.005703 Jy/beam ! Combined flux in latest and established models = 2.35173 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 2.35173 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.108799Jy sigma=0.001245 ! Fit after self-cal, rms=0.099714Jy sigma=0.001090 ! Inverting map and beam ! Estimated beam: bmin=0.5799 mas, bmaj=1.272 mas, bpa=53.67 degrees ! Estimated noise=2236.15 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 = 0.0056409 Jy ! Component: 100 - total flux cleaned = 0.00561867 Jy ! Total flux subtracted in 100 components = 0.00561867 Jy ! Clean residual min=-0.010122 max=0.011231 Jy/beam ! Clean residual mean=0.000068 rms=0.002629 Jy/beam ! Combined flux in latest and established models = 2.35734 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 6 model components to the UV plane model. ! The established model now contains 31 components and 2.35734 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.099151Jy sigma=0.001084 ! Fit after self-cal, rms=0.099163Jy sigma=0.001083 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 1156+295_X ! Writing UV FITS file: 1156+295_X.uvf ! Writing 31 model components to file: 1156+295_X.mod ! wwins: Wrote 1 windows to 1156+295_X.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5799 x 1.272 at 53.67 degrees (North through East) ! Clean map min=-0.0096206 max=2.1915 Jy/beam ! Writing clean map to FITS file: 1156+295_X.fits ! Writing difmap environment to: 1156+295_X.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 1156+295_X] device 1156+295_Xuv.ps/vps,1,2 ! Attempting to open device: '1156+295_Xuv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 1156+295_Xim.ps/vps ! Attempting to open device: '1156+295_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=0.5799 mas, bmaj=1.272 mas, bpa=53.67 degrees ! Estimated noise=2236.15 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5799 x 1.272 at 53.67 degrees (North through East) ! Clean map min=-0.0096206 max=2.1915 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo8-0.1] quit ! Quitting program ! Log file 1156+295_X.log closed on Wed May 14 12:45:16 2008