! Started logfile: 1125+596_S.log on Tue Apr 29 23:45:04 2008 observe 1125+596_S.edt ! Reading UV FITS file: 1125+596_S.edt ! AN table 1: 76 integrations on 153 of 153 possible baselines. ! Apparent sampling: 0.169161 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 1125+596 ! ! 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 963 lines of history. ! ! Reading 7868 visibilities. ![@gonzo6-0.4 1125+596_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 1236 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 1236 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 1220 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 1297 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.656786Jy sigma=0.008066 ! Fit after self-cal, rms=0.656431Jy sigma=0.008095 ! 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=2.848 mas, bmaj=3.702 mas, bpa=26.16 degrees ! Estimated noise=2840.23 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 = 0.270121 Jy ! Total flux subtracted in 50 components = 0.270121 Jy ! Clean residual min=-0.013341 max=0.075332 Jy/beam ! Clean residual mean=0.000067 rms=0.004109 Jy/beam ! Combined flux in latest and established models = 0.270121 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 0.270121 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.092924Jy sigma=0.001138 ! Fit after self-cal, rms=0.092925Jy sigma=0.001138 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.058907 Jy ! Total flux subtracted in 50 components = 0.058907 Jy ! Clean residual min=-0.007624 max=0.016481 Jy/beam ! Clean residual mean=0.000026 rms=0.001964 Jy/beam ! Combined flux in latest and established models = 0.329028 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 0.329028 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.056488Jy sigma=0.000661 ! Fit after self-cal, rms=0.056489Jy sigma=0.000661 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0150208 Jy ! Total flux subtracted in 50 components = 0.0150208 Jy ! Clean residual min=-0.007088 max=0.008220 Jy/beam ! Clean residual mean=0.000016 rms=0.001763 Jy/beam ! Combined flux in latest and established models = 0.344049 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 13 model components to the UV plane model. ! The established model now contains 13 components and 0.344049 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.053529Jy sigma=0.000619 ! Fit after self-cal, rms=0.053523Jy sigma=0.000619 ! 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=3.052 mas, bmaj=3.77 mas, bpa=25.76 degrees ! Estimated noise=2192.14 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 = 0.00876312 Jy ! Component: 100 - total flux cleaned = 0.0135923 Jy ! Total flux subtracted in 100 components = 0.0135923 Jy ! Clean residual min=-0.006213 max=0.005085 Jy/beam ! Clean residual mean=-0.000003 rms=0.001347 Jy/beam ! Combined flux in latest and established models = 0.357641 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 17 components and 0.357641 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.052281Jy sigma=0.000602 ! Fit after self-cal, rms=0.052286Jy sigma=0.000602 ! 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 1.00 FD 0.99 GC 1.00 HH 1.00* ! HN 0.99 KK 1.04 KP 0.97 LA 1.01 ! MC 1.00* MK 1.00 NL 0.99 NY 1.02 ! ON 1.00* OV 1.00 PT 1.00 SC 1.00 ! WF 1.00 WZ 0.96 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.99 GC 0.99 HH 1.00* ! HN 0.99 KK 1.04 KP 1.01 LA 1.00 ! MC 1.00* MK 1.00 NL 0.98 NY 1.01 ! ON 1.00* OV 1.00 PT 1.01 SC 1.02 ! WF 1.01 WZ 0.99 ! ! ! Correcting IF 3. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.99 GC 1.02 HH 1.00* ! HN 1.00 KK 1.01 KP 1.02 LA 1.01 ! MC 1.00* MK 1.01 NL 0.96 NY 0.98 ! ON 1.00* OV 1.00 PT 0.98 SC 1.02 ! WF 1.00* WZ 1.01 ! ! ! Correcting IF 4. ! A total of 9 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 1.00 GC 0.96 HH 1.00* ! HN 1.01 KK 1.00* KP 0.98 LA 1.00* ! MC 1.00* MK 1.00 NL 0.97 NY 0.94 ! ON 1.00* OV 0.99 PT 1.01 SC 1.03 ! WF 1.00* WZ 0.99 ! ! ! Fit before self-cal, rms=0.052286Jy sigma=0.000602 ! Fit after self-cal, rms=0.051976Jy sigma=0.000598 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=3.053 mas, bmaj=3.781 mas, bpa=26.16 degrees ! Estimated noise=2212.32 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 = 0.000428961 Jy ! Component: 100 - total flux cleaned = 0.000632967 Jy ! Total flux subtracted in 100 components = 0.000632967 Jy ! Clean residual min=-0.005587 max=0.005176 Jy/beam ! Clean residual mean=0.000005 rms=0.001304 Jy/beam ! Combined flux in latest and established models = 0.358274 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 21 components and 0.358274 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.051906Jy sigma=0.000598 ! Fit after self-cal, rms=0.051905Jy sigma=0.000598 ! 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 = 2.96827e-05 Jy ! Component: 100 - total flux cleaned = -1.11059e-05 Jy ! Total flux subtracted in 100 components = -1.11059e-05 Jy ! Clean residual min=-0.005527 max=0.005201 Jy/beam ! Clean residual mean=0.000005 rms=0.001302 Jy/beam ! Combined flux in latest and established models = 0.358263 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 9 model components to the UV plane model. ! The established model now contains 26 components and 0.358263 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.051868Jy sigma=0.000597 ! Fit after self-cal, rms=0.050890Jy sigma=0.000580 ! Inverting map and beam ! Estimated beam: bmin=3.051 mas, bmaj=3.783 mas, bpa=26.16 degrees ! Estimated noise=2218.32 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 = 0.00115508 Jy ! Component: 100 - total flux cleaned = 0.00119415 Jy ! Total flux subtracted in 100 components = 0.00119415 Jy ! Clean residual min=-0.005080 max=0.004968 Jy/beam ! Clean residual mean=-0.000010 rms=0.001271 Jy/beam ! Combined flux in latest and established models = 0.359457 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 30 components and 0.359457 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.050850Jy sigma=0.000580 ! Fit after self-cal, rms=0.050854Jy sigma=0.000580 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 1125+596_S ! Writing UV FITS file: 1125+596_S.uvf ! Writing 30 model components to file: 1125+596_S.mod ! wwins: Wrote 1 windows to 1125+596_S.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.051 x 3.783 at 26.16 degrees (North through East) ! Clean map min=-0.0049776 max=0.34389 Jy/beam ! Writing clean map to FITS file: 1125+596_S.fits ! Writing difmap environment to: 1125+596_S.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 1125+596_S] device 1125+596_Suv.ps/vps,1,2 ! Attempting to open device: '1125+596_Suv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 1125+596_Sim.ps/vps ! Attempting to open device: '1125+596_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=3.051 mas, bmaj=3.783 mas, bpa=26.16 degrees ! Estimated noise=2218.32 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.051 x 3.783 at 26.16 degrees (North through East) ! Clean map min=-0.0049776 max=0.34389 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo6-0.4] quit ! Quitting program ! Log file 1125+596_S.log closed on Tue Apr 29 23:45:09 2008