! Started logfile: 0048-097_X.log on Fri Oct 27 17:09:01 2006 observe 0048-097_X.edt ! Reading UV FITS file: 0048-097_X.edt ! AN table 1: 2 integrations on 153 of 153 possible baselines. ! AN table 2: 24 integrations on 153 of 153 possible baselines. ! AN table 3: 15 integrations on 153 of 153 possible baselines. ! AN table 4: 45 integrations on 153 of 153 possible baselines. ! AN table 5: 23 integrations on 153 of 153 possible baselines. ! Apparent sampling: 0.0639204 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 0048-097 ! ! 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 1304 lines of history. ! ! Reading 4264 visibilities. ![@gonzo8-0.1 0048-097_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 36 telescope corrections were flagged in sub-array 1. ! A total of 321 telescope corrections were flagged in sub-array 2. ! A total of 270 telescope corrections were flagged in sub-array 3. ! A total of 761 telescope corrections were flagged in sub-array 4. ! A total of 338 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 36 telescope corrections were flagged in sub-array 1. ! A total of 321 telescope corrections were flagged in sub-array 2. ! A total of 270 telescope corrections were flagged in sub-array 3. ! A total of 761 telescope corrections were flagged in sub-array 4. ! A total of 340 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 36 telescope corrections were flagged in sub-array 1. ! A total of 321 telescope corrections were flagged in sub-array 2. ! A total of 270 telescope corrections were flagged in sub-array 3. ! A total of 764 telescope corrections were flagged in sub-array 4. ! A total of 357 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 36 telescope corrections were flagged in sub-array 1. ! A total of 321 telescope corrections were flagged in sub-array 2. ! A total of 270 telescope corrections were flagged in sub-array 3. ! A total of 764 telescope corrections were flagged in sub-array 4. ! A total of 346 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=0.128268Jy sigma=0.001570 ! Fit after self-cal, rms=0.125753Jy sigma=0.001571 ! 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=0.5491 mas, bmaj=2.353 mas, bpa=-7.707 degrees ! Estimated noise=1562.06 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) ! Added new window around map position (0, 0). ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.725938 Jy ! Total flux subtracted in 50 components = 0.725938 Jy ! Clean residual min=-0.047558 max=0.202458 Jy/beam ! Clean residual mean=0.000711 rms=0.015281 Jy/beam ! Combined flux in latest and established models = 0.725938 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 0.725938 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.240996Jy sigma=0.003662 ! Fit after self-cal, rms=0.240997Jy sigma=0.003662 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.158703 Jy ! Total flux subtracted in 50 components = 0.158703 Jy ! Clean residual min=-0.019402 max=0.048042 Jy/beam ! Clean residual mean=0.000206 rms=0.005999 Jy/beam ! Combined flux in latest and established models = 0.884641 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 5 components and 0.884641 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.123612Jy sigma=0.001769 ! Fit after self-cal, rms=0.123613Jy sigma=0.001769 ! 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=0.6993 mas, bmaj=2.952 mas, bpa=-10.42 degrees ! Estimated noise=1017.95 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 = 0.0625276 Jy ! Component: 100 - total flux cleaned = 0.0887163 Jy ! Total flux subtracted in 100 components = 0.0887163 Jy ! Clean residual min=-0.011500 max=0.016153 Jy/beam ! Clean residual mean=-0.000191 rms=0.003335 Jy/beam ! Combined flux in latest and established models = 0.973357 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 31 components and 0.973357 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.097329Jy sigma=0.001276 ! Fit after self-cal, rms=0.097308Jy sigma=0.001275 ! Inverting map print "****************************************" ! **************************************** print "*** Finished Natural Weighting CLEAN ***" ! *** Finished Natural Weighting CLEAN *** print "****************************************" ! **************************************** gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! FD 0.00* GC 0.00* HH 0.00* HN 0.00* ! LA 0.00* MC 0.00* MK 0.00* NY 0.00* ! ON 0.00* OV 0.00* PT 0.00* SC 0.00* ! TS 0.00* WF 0.00* BR 0.00* KK 0.00* ! KP 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! FD 0.96 GC 1.00* HH 1.00* HN 0.99 ! LA 0.98 MC 1.00* MK 0.97 NY 1.00* ! ON 1.00* OV 0.96 PT 0.98 SC 1.00* ! TS 1.00* WF 1.01 BR 0.99 KK 0.99 ! KP 0.98 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 0.00* GC 0.00* HH 0.00* HN 0.00* ! LA 0.00* MC 0.00* MK 0.00* NY 0.00* ! ON 0.00* OV 0.00* PT 0.00* SC 0.00* ! TS 0.00* WF 0.00* BR 0.00* KK 0.00* ! KP 0.00* WZ 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! FD 0.95 GC 1.08 HH 1.00* HN 1.00* ! LA 0.98 MC 1.00* MK 0.98 NY 1.00* ! ON 1.00* OV 0.97 PT 0.98 SC 1.00* ! TS 1.01 WF 1.00* BR 0.99 KK 1.00* ! KP 1.00* WZ 1.00* ! ! A total of 12 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! FD 1.00* GC 1.00* HH 1.00* HN 1.02 ! LA 1.00 MC 1.00* MK 1.00* NY 1.00* ! ON 1.10 OV 1.00* PT 1.00* SC 1.00* ! TS 1.00* WF 1.00* BR 1.00* KK 1.00* ! KP 1.03 WZ 1.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! FD 0.00* GC 0.00* HH 0.00* HN 0.00* ! LA 0.00* MC 0.00* MK 0.00* NY 0.00* ! ON 0.00* OV 0.00* PT 0.00* SC 0.00* ! TS 0.00* WF 0.00* BR 0.00* KK 0.00* ! KP 0.00* WZ 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! FD 0.97 GC 1.00* HH 1.00* HN 0.99 ! LA 0.98 MC 1.00* MK 0.97 NY 1.00* ! ON 1.00* OV 0.97 PT 1.02 SC 1.00* ! TS 1.00* WF 1.03 BR 0.98 KK 1.01 ! KP 0.93 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 0.00* GC 0.00* HH 0.00* HN 0.00* ! LA 0.00* MC 0.00* MK 0.00* NY 0.00* ! ON 0.00* OV 0.00* PT 0.00* SC 0.00* ! TS 0.00* WF 0.00* BR 0.00* KK 0.00* ! KP 0.00* WZ 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! FD 0.97 GC 1.10 HH 1.00* HN 1.00* ! LA 0.98 MC 1.00* MK 0.98 NY 1.00* ! ON 1.00* OV 0.97 PT 1.00 SC 1.00* ! TS 1.00 WF 1.00* BR 0.99 KK 1.00* ! KP 1.00* WZ 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! FD 1.00* GC 1.00* HH 1.00* HN 1.00 ! LA 1.00 MC 1.00* MK 1.00* NY 1.00* ! ON 1.07 OV 1.00* PT 1.00* SC 1.00* ! TS 1.00* WF 1.00* BR 1.00* KK 1.00* ! KP 0.99 WZ 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! FD 0.00* GC 0.00* HH 0.00* HN 0.00* ! LA 0.00* MC 0.00* MK 0.00* NY 0.00* ! ON 0.00* OV 0.00* PT 0.00* SC 0.00* ! TS 0.00* WF 0.00* BR 0.00* KK 0.00* ! KP 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! FD 0.95 GC 1.00* HH 1.00* HN 1.02 ! LA 1.00 MC 1.00* MK 1.00 NY 1.00* ! ON 1.00* OV 1.00 PT 1.04 SC 1.00* ! TS 1.00* WF 1.15 BR 1.02 KK 1.00 ! KP 0.93 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 0.00* GC 0.00* HH 0.00* HN 0.00* ! LA 0.00* MC 0.00* MK 0.00* NY 0.00* ! ON 0.00* OV 0.00* PT 0.00* SC 0.00* ! TS 0.00* WF 0.00* BR 0.00* KK 0.00* ! KP 0.00* WZ 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! FD 0.95 GC 1.09 HH 1.00* HN 1.00* ! LA 0.99 MC 1.00* MK 0.98 NY 1.00* ! ON 1.00* OV 1.00 PT 1.03 SC 1.00* ! TS 1.01 WF 1.00* BR 1.03 KK 1.00* ! KP 1.00* WZ 1.00* ! ! A total of 9 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! FD 1.00* GC 1.00* HH 1.00* HN 1.12 ! LA 0.98 MC 1.00* MK 1.00* NY 1.00* ! ON 1.11 OV 1.00* PT 1.00* SC 1.00* ! TS 1.00* WF 1.00* BR 1.00* KK 1.00* ! KP 1.00 WZ 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! FD 0.00* GC 0.00* HH 0.00* HN 0.00* ! LA 0.00* MC 0.00* MK 0.00* NY 0.00* ! ON 0.00* OV 0.00* PT 0.00* SC 0.00* ! TS 0.00* WF 0.00* BR 0.00* KK 0.00* ! KP 0.00* WZ 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! FD 0.95 GC 1.00* HH 1.00* HN 1.01 ! LA 0.98 MC 1.00* MK 1.03 NY 1.00* ! ON 1.00* OV 0.99 PT 1.04 SC 1.00* ! TS 1.00* WF 1.12 BR 1.00 KK 0.99 ! KP 0.95 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 0.00* GC 0.00* HH 0.00* HN 0.00* ! LA 0.00* MC 0.00* MK 0.00* NY 0.00* ! ON 0.00* OV 0.00* PT 0.00* SC 0.00* ! TS 0.00* WF 0.00* BR 0.00* KK 0.00* ! KP 0.00* WZ 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! FD 0.94 GC 1.13 HH 1.00* HN 1.00* ! LA 0.98 MC 1.00* MK 1.03 NY 1.00* ! ON 1.00* OV 0.97 PT 1.03 SC 1.00* ! TS 1.01 WF 1.00* BR 1.01 KK 1.00* ! KP 1.00* WZ 1.00* ! ! A total of 12 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! FD 1.00* GC 1.00* HH 1.00* HN 1.05 ! LA 1.00 MC 1.00* MK 1.00* NY 1.00* ! ON 1.05 OV 1.00* PT 1.00* SC 1.00* ! TS 1.00* WF 1.00* BR 1.00* KK 1.00* ! KP 0.98 WZ 1.00* ! ! ! Fit before self-cal, rms=0.097308Jy sigma=0.001275 ! Fit after self-cal, rms=0.084822Jy sigma=0.001077 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.7015 mas, bmaj=2.963 mas, bpa=-10.28 degrees ! Estimated noise=1018.33 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 = 0.00157519 Jy ! Component: 100 - total flux cleaned = 0.0017296 Jy ! Total flux subtracted in 100 components = 0.0017296 Jy ! Clean residual min=-0.004333 max=0.004681 Jy/beam ! Clean residual mean=-0.000022 rms=0.001104 Jy/beam ! Combined flux in latest and established models = 0.975087 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 39 components and 0.975087 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084733Jy sigma=0.001075 ! Fit after self-cal, rms=0.084718Jy sigma=0.001074 ! 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 = 0.000111441 Jy ! Component: 100 - total flux cleaned = 0.0001714 Jy ! Total flux subtracted in 100 components = 0.0001714 Jy ! Clean residual min=-0.004203 max=0.004484 Jy/beam ! Clean residual mean=-0.000024 rms=0.001090 Jy/beam ! Combined flux in latest and established models = 0.975258 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 8 model components to the UV plane model. ! The established model now contains 41 components and 0.975258 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084676Jy sigma=0.001073 ! Fit after self-cal, rms=0.083409Jy sigma=0.001056 ! Inverting map and beam ! Estimated beam: bmin=0.7018 mas, bmaj=2.961 mas, bpa=-10.28 degrees ! Estimated noise=1018.98 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 = 0.00118222 Jy ! Component: 100 - total flux cleaned = 0.00134723 Jy ! Total flux subtracted in 100 components = 0.00134723 Jy ! Clean residual min=-0.004106 max=0.004454 Jy/beam ! Clean residual mean=-0.000002 rms=0.001068 Jy/beam ! Combined flux in latest and established models = 0.976606 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 43 components and 0.976606 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.083367Jy sigma=0.001055 ! Fit after self-cal, rms=0.083356Jy sigma=0.001055 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 0048-097_X ! Writing UV FITS file: 0048-097_X.uvf ! Writing 43 model components to file: 0048-097_X.mod ! wwins: Wrote 1 windows to 0048-097_X.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7018 x 2.961 at -10.28 degrees (North through East) ! Clean map min=-0.0040043 max=0.93585 Jy/beam ! Writing clean map to FITS file: 0048-097_X.fits ! Writing difmap environment to: 0048-097_X.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 0048-097_X] device 0048-097_Xuv.ps/vps,1,2 ! Attempting to open device: '0048-097_Xuv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 0048-097_Xim.ps/vps ! Attempting to open device: '0048-097_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=0.7018 mas, bmaj=2.961 mas, bpa=-10.28 degrees ! Estimated noise=1018.98 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7018 x 2.961 at -10.28 degrees (North through East) ! Clean map min=-0.0040043 max=0.93585 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo8-0.1] quit ! Quitting program ! Log file 0048-097_X.log closed on Fri Oct 27 17:09:18 2006