! Started logfile: 0552+398_S.log on Fri Aug 12 12:57:00 2005 observe 0552+398_S.edt ! Reading UV FITS file: 0552+398_S.edt ! AN table 1: 55 integrations on 171 of 171 possible baselines. ! AN table 2: 14 integrations on 171 of 171 possible baselines. ! AN table 3: 13 integrations on 171 of 171 possible baselines. ! AN table 4: 25 integrations on 171 of 171 possible baselines. ! Apparent sampling: 0.251025 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 0552+398 ! ! 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 1565 lines of history. ! ! Reading 18372 visibilities. ![@gonzo7-0.4 0552+398_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 = 7.0 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 726 telescope corrections were flagged in sub-array 1. ! A total of 229 telescope corrections were flagged in sub-array 2. ! A total of 197 telescope corrections were flagged in sub-array 3. ! A total of 421 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 726 telescope corrections were flagged in sub-array 1. ! A total of 229 telescope corrections were flagged in sub-array 2. ! A total of 197 telescope corrections were flagged in sub-array 3. ! A total of 421 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 732 telescope corrections were flagged in sub-array 1. ! A total of 230 telescope corrections were flagged in sub-array 2. ! A total of 203 telescope corrections were flagged in sub-array 3. ! A total of 431 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 727 telescope corrections were flagged in sub-array 1. ! A total of 233 telescope corrections were flagged in sub-array 2. ! A total of 207 telescope corrections were flagged in sub-array 3. ! A total of 421 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.775820Jy sigma=0.025232 ! Fit after self-cal, rms=1.780674Jy sigma=0.025333 ! 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=2.694 mas, bmaj=3.089 mas, bpa=-8.566 degrees ! Estimated noise=1036.91 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 = 2.07592 Jy ! Total flux subtracted in 50 components = 2.07592 Jy ! Clean residual min=-0.070334 max=0.579060 Jy/beam ! Clean residual mean=-0.000286 rms=0.025232 Jy/beam ! Combined flux in latest and established models = 2.07592 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 2.07592 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.753886Jy sigma=0.011077 ! Fit after self-cal, rms=0.753886Jy sigma=0.011077 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.492124 Jy ! Total flux subtracted in 50 components = 0.492124 Jy ! Clean residual min=-0.032719 max=0.190437 Jy/beam ! Clean residual mean=-0.000151 rms=0.011578 Jy/beam ! Combined flux in latest and established models = 2.56804 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 9 components and 2.56804 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.369856Jy sigma=0.005336 ! Fit after self-cal, rms=0.369852Jy sigma=0.005336 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.206216 Jy ! Total flux subtracted in 50 components = 0.206216 Jy ! Clean residual min=-0.022571 max=0.099007 Jy/beam ! Clean residual mean=-0.000090 rms=0.007217 Jy/beam ! Combined flux in latest and established models = 2.77426 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 17 components and 2.77426 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.249815Jy sigma=0.003398 ! Fit after self-cal, rms=0.249790Jy sigma=0.003398 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.113284 Jy ! Total flux subtracted in 50 components = 0.113284 Jy ! Clean residual min=-0.018928 max=0.055679 Jy/beam ! Clean residual mean=-0.000055 rms=0.005281 Jy/beam ! Combined flux in latest and established models = 2.88754 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 22 components and 2.88754 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.201370Jy sigma=0.002566 ! Fit after self-cal, rms=0.201349Jy sigma=0.002566 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0646941 Jy ! Total flux subtracted in 50 components = 0.0646941 Jy ! Clean residual min=-0.017494 max=0.032185 Jy/beam ! Clean residual mean=-0.000035 rms=0.004486 Jy/beam ! Combined flux in latest and established models = 2.95224 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 23 components and 2.95224 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.183791Jy sigma=0.002240 ! Fit after self-cal, rms=0.183783Jy sigma=0.002240 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0372293 Jy ! Total flux subtracted in 50 components = 0.0372293 Jy ! Clean residual min=-0.016663 max=0.020522 Jy/beam ! Clean residual mean=-0.000023 rms=0.004193 Jy/beam ! Combined flux in latest and established models = 2.98947 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 24 components and 2.98947 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.178115Jy sigma=0.002124 ! Fit after self-cal, rms=0.178116Jy sigma=0.002124 ! 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=3.564 mas, bmaj=4.077 mas, bpa=20.39 degrees ! Estimated noise=612.726 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 = 0.0256134 Jy ! Component: 100 - total flux cleaned = 0.0356328 Jy ! Total flux subtracted in 100 components = 0.0356328 Jy ! Clean residual min=-0.013588 max=0.019024 Jy/beam ! Clean residual mean=0.000131 rms=0.003541 Jy/beam ! Combined flux in latest and established models = 3.0251 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 12 model components to the UV plane model. ! The established model now contains 32 components and 3.0251 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.175326Jy sigma=0.002069 ! Fit after self-cal, rms=0.175320Jy sigma=0.002069 ! 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 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 1.00 GC 1.03 HH 1.00* ! HN 0.98 KK 1.00* KP 1.03 LA 1.01 ! MC 0.99 MK 1.03 NL 1.00 NY 1.02 ! ON 1.02 OV 1.01 PT 1.01 SC 0.95 ! TS 1.00* WF 1.01 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 1.04 GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 1.01 LA 1.02 ! MC 1.00* MK 1.01 NL 1.01 NY 1.00* ! ON 1.00* OV 1.02 PT 1.02 SC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 1.03 GC 1.00* HH 1.00* ! HN 1.03 KK 1.00* KP 1.01 LA 1.00 ! MC 1.00* MK 1.00* NL 1.01 NY 1.00* ! ON 1.00* OV 0.99 PT 1.00 SC 0.97 ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 12 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 1.00* GC 1.01 HH 1.00* ! HN 1.00 KK 1.00* KP 1.00* LA 1.01 ! MC 1.00* MK 1.00* NL 1.01 NY 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00 ! TS 1.00* WF 1.02 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 1.00 FD 0.99 GC 1.03 HH 1.00* ! HN 0.98 KK 1.00* KP 1.01 LA 1.02 ! MC 0.94 MK 1.02 NL 1.00 NY 1.02 ! ON 1.09 OV 1.00 PT 1.01 SC 1.02 ! TS 1.00* WF 0.99 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 1.04 GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 1.03 LA 1.01 ! MC 1.00* MK 0.98 NL 1.02 NY 1.00* ! ON 1.00* OV 1.00 PT 1.02 SC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.01 GC 1.00* HH 1.00* ! HN 0.99 KK 1.00* KP 1.01 LA 0.99 ! MC 1.00* MK 1.00* NL 0.99 NY 1.00* ! ON 1.00* OV 0.98 PT 0.96 SC 1.00 ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 12 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 FD 1.00* GC 1.01 HH 1.00* ! HN 1.02 KK 1.00* KP 1.00* LA 0.99 ! MC 1.00* MK 1.00* NL 0.99 NY 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00 ! TS 1.00* WF 1.01 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 0.98 FD 0.99 GC 0.99 HH 1.00* ! HN 0.98 KK 1.00* KP 1.00 LA 1.13 ! MC 0.98 MK 1.00 NL 0.98 NY 1.01 ! ON 1.04 OV 0.99 PT 0.98 SC 1.08 ! TS 1.00* WF 1.01 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 1.00 GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 1.01 LA 1.05 ! MC 1.00* MK 0.99 NL 1.00 NY 1.00* ! ON 1.00* OV 0.99 PT 0.99 SC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.90 FD 1.00 GC 1.00* HH 1.00* ! HN 1.01 KK 1.00* KP 0.99 LA 1.00* ! MC 1.00* MK 1.00* NL 0.98 NY 1.00* ! ON 1.00* OV 0.97 PT 0.97 SC 0.99 ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 FD 1.00* GC 1.01 HH 1.00* ! HN 1.02 KK 1.00* KP 1.00* LA 1.07 ! MC 1.00* MK 1.00* NL 1.02 NY 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.05 ! TS 1.00* WF 1.00 WZ 1.00* ! ! ! Correcting IF 4. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.97 GC 0.99 HH 1.00* ! HN 0.96 KK 1.00* KP 0.98 LA 0.99 ! MC 1.17 MK 1.00 NL 0.97 NY 0.96 ! ON 1.05 OV 0.96 PT 0.99 SC 1.09 ! TS 1.00* WF 1.00 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 0.99 GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 1.00 LA 1.00 ! MC 1.00* MK 1.00* NL 0.98 NY 1.00* ! ON 1.00* OV 0.97 PT 0.99 SC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 0.96 GC 1.00* HH 1.00* ! HN 0.95 KK 1.00* KP 1.00 LA 0.96 ! MC 1.00* MK 1.00* NL 0.98 NY 1.00* ! ON 1.00* OV 1.00* PT 0.96 SC 1.02 ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 12 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 FD 1.00* GC 1.02 HH 1.00* ! HN 0.99 KK 1.00* KP 1.00* LA 1.01 ! MC 1.00* MK 1.00* NL 1.01 NY 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.03 ! TS 1.00* WF 1.00 WZ 1.00* ! ! ! Fit before self-cal, rms=0.175320Jy sigma=0.002069 ! Fit after self-cal, rms=0.136846Jy sigma=0.001402 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=3.591 mas, bmaj=4.105 mas, bpa=21.73 degrees ! Estimated noise=614.736 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 = -0.00922079 Jy ! Component: 100 - total flux cleaned = -0.010048 Jy ! Total flux subtracted in 100 components = -0.010048 Jy ! Clean residual min=-0.007441 max=0.006972 Jy/beam ! Clean residual mean=-0.000132 rms=0.001401 Jy/beam ! Combined flux in latest and established models = 3.01505 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 38 components and 3.01505 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.136317Jy sigma=0.001392 ! Fit after self-cal, rms=0.136329Jy sigma=0.001392 ! 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 = -0.00018649 Jy ! Component: 100 - total flux cleaned = -0.000331898 Jy ! Total flux subtracted in 100 components = -0.000331898 Jy ! Clean residual min=-0.007458 max=0.006829 Jy/beam ! Clean residual mean=-0.000131 rms=0.001394 Jy/beam ! Combined flux in latest and established models = 3.01472 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 6 model components to the UV plane model. ! The established model now contains 40 components and 3.01472 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.136142Jy sigma=0.001390 ! Fit after self-cal, rms=0.127708Jy sigma=0.001295 ! Inverting map and beam ! Estimated beam: bmin=3.593 mas, bmaj=4.103 mas, bpa=21.16 degrees ! Estimated noise=614.528 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 = -0.00215589 Jy ! Component: 100 - total flux cleaned = -0.00269349 Jy ! Total flux subtracted in 100 components = -0.00269349 Jy ! Clean residual min=-0.005360 max=0.003764 Jy/beam ! Clean residual mean=-0.000155 rms=0.000996 Jy/beam ! Combined flux in latest and established models = 3.01203 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 47 components and 3.01203 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.127547Jy sigma=0.001293 ! Fit after self-cal, rms=0.127545Jy sigma=0.001293 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 0552+398_S ! Writing UV FITS file: 0552+398_S.uvf ! Writing 47 model components to file: 0552+398_S.mod ! wwins: Wrote 1 windows to 0552+398_S.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.593 x 4.103 at 21.16 degrees (North through East) ! Clean map min=-0.004517 max=2.7684 Jy/beam ! Writing clean map to FITS file: 0552+398_S.fits ! Writing difmap environment to: 0552+398_S.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 0552+398_S] device 0552+398_Suv.ps/vps,1,2 ! Attempting to open device: '0552+398_Suv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 0552+398_Sim.ps/vps ! Attempting to open device: '0552+398_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=3.593 mas, bmaj=4.103 mas, bpa=21.16 degrees ! Estimated noise=614.528 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.593 x 4.103 at 21.16 degrees (North through East) ! Clean map min=-0.004517 max=2.7684 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo7-0.4] quit ! Quitting program ! Log file 0552+398_S.log closed on Fri Aug 12 12:57:32 2005