! Started logfile: /d2/scr/pima/rdv96_uvs/J1006-5018_X_uvs.log on Fri Dec 20 23:44:50 2013 obs /d2/scr/pima/rdv96_uvs/J1006-5018_X_uva.fits ! Reading UV FITS file: /d2/scr/pima/rdv96_uvs/J1006-5018_X_uva.fits ! AN table 1: 2 integrations on 3 of 3 possible baselines. ! AN table 2: 2 integrations on 6 of 6 possible baselines. ! Apparent sampling: 1 visibilities/baseline/integration-bin. ! Found source: J1006-5018 ! ! 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 8.40599e+09 8e+06 1 8e+06 ! 02 2 8.47599e+09 8e+06 1 8e+06 ! 03 3 8.79099e+09 8e+06 1 8e+06 ! 04 4 8.89599e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 0 lines of history. ! ! Reading 72 visibilities. select RR ! 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 print "field_size =",field_size ! field_size = 1024 print "field_cell =",field_cell ! field_cell = 0.2 print "taper_size =",taper_size ! taper_size = 70 ![@/home/lpetrov/bin/rdv_muppet /d2/scr/pima/rdv96_uvs/J1006-5018_X] integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.03 float dynam dynam = 6.0 float soltime1 soltime1 = 800000 float soltime2 soltime2 = 15 float soltime3 soltime3 = 1 float thresh thresh = 0.5 float win_mult win_mult = 1.8 float old_peak float new_peak float flux_cutoff selfant "",false ! 1:FD self-cal status=correctable weight=1 ! 1:KP self-cal status=correctable weight=1 ! 1:PT self-cal status=correctable weight=1 ! 2:FD self-cal status=correctable weight=1 ! 2:KP self-cal status=correctable weight=1 ! 2:LA self-cal status=correctable weight=1 ! 2:PT self-cal status=correctable weight=1 system "rm /tmp/ff.ff" mapsize field_size, field_cell ! Map grid = 1024x1024 pixels with 0.200x0.200 milli-arcsec cellsize. 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. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.267319Jy sigma=10.510123 ! Fit after self-cal, rms=0.298463Jy sigma=2.228394 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. print "=== Flag out IVS stations" ! === Flag out IVS stations integer lun string cfg_file lun = outfile ( "/tmp/ff.ff" ) do i=1,nsub do j=1,ntel(i) fprintf lun, "%s\n", telname(j,i) end do end do close ( lun ) system "/home/lpetrov/bin/dimap_flag_process.csh /tmp/ff.ff" ![@/tmp/ff.ff \] ![Exited script file: /tmp/ff.ff] uvw 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. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=4.86 mas, bmaj=40.42 mas, bpa=3.743 degrees ! Estimated noise=11.4246 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.583448 Jy ! Component: 100 - total flux cleaned = 0.726866 Jy ! Total flux subtracted in 100 components = 0.726866 Jy ! Clean residual min=-0.058306 max=0.058804 Jy/beam ! Clean residual mean=0.001076 rms=0.023115 Jy/beam ! Combined flux in latest and established models = 0.726866 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 11 components and 0.726866 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.104566Jy sigma=0.885406 ! Fit after self-cal, rms=0.104561Jy sigma=0.885178 ! Inverting map print "=== Finished uniform weighting clean ===" ! === Finished uniform weighting clean === uvw 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 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=5.277 mas, bmaj=41.68 mas, bpa=3.73 degrees ! Estimated noise=10.3097 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0239225 Jy ! Component: 100 - total flux cleaned = 0.0242113 Jy ! Component: 150 - total flux cleaned = 0.0176314 Jy ! Component: 200 - total flux cleaned = 0.00956116 Jy ! Total flux subtracted in 200 components = 0.00956116 Jy ! Clean residual min=-0.010356 max=0.010096 Jy/beam ! Clean residual mean=0.000214 rms=0.004607 Jy/beam ! Combined flux in latest and established models = 0.736427 Jy ! Performing phase self-cal ! Adding 107 model components to the UV plane model. ! The established model now contains 116 components and 0.736427 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.069728Jy sigma=0.561327 ! Fit after self-cal, rms=0.069739Jy sigma=0.560863 ! Inverting map print "=== Finished natural weighting clean for VLBI sites ===" ! === Finished natural weighting clean for VLBI sites === 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: ! FD 0.00* KP 0.00* PT 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! FD 0.95 KP 1.04 LA 1.06 PT 1.02 ! ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! FD 0.00* KP 0.00* PT 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! FD 0.94 KP 1.03 LA 0.96 PT 0.98 ! ! ! Correcting IF 3. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! FD 0.00* KP 0.00* PT 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! FD 1.04 KP 0.87 LA 1.08 PT 0.96 ! ! ! Correcting IF 4. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! FD 0.00* KP 0.00* PT 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! FD 1.03 KP 1.02 LA 1.02 PT 0.97 ! ! ! Fit before self-cal, rms=0.069739Jy sigma=0.560863 ! Fit after self-cal, rms=0.054511Jy sigma=0.413132 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=5.497 mas, bmaj=57.54 mas, bpa=8.161 degrees ! Estimated noise=13.0931 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00399311 Jy ! Component: 100 - total flux cleaned = -0.00496549 Jy ! Component: 150 - total flux cleaned = -0.00470049 Jy ! Component: 200 - total flux cleaned = -0.00345068 Jy ! Total flux subtracted in 200 components = -0.00345068 Jy ! Clean residual min=-0.005706 max=0.005716 Jy/beam ! Clean residual mean=0.000036 rms=0.001980 Jy/beam ! Combined flux in latest and established models = 0.732977 Jy ! Performing phase self-cal ! Adding 63 model components to the UV plane model. ! The established model now contains 179 components and 0.732977 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.053131Jy sigma=0.404256 ! Fit after self-cal, rms=0.053124Jy sigma=0.403653 ! Inverting map selfcal true, true, soltime1 ! Performing amp+phase self-cal over 800000 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.053124Jy sigma=0.403653 ! Fit after self-cal, rms=0.053127Jy sigma=0.402730 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=5.499 mas, bmaj=57.53 mas, bpa=8.142 degrees ! Estimated noise=13.1161 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00361079 Jy ! Component: 100 - total flux cleaned = -0.00362261 Jy ! Component: 150 - total flux cleaned = -0.00341181 Jy ! Component: 200 - total flux cleaned = -0.00317012 Jy ! Total flux subtracted in 200 components = -0.00317012 Jy ! Clean residual min=-0.003939 max=0.004007 Jy/beam ! Clean residual mean=-0.000008 rms=0.001332 Jy/beam ! Combined flux in latest and established models = 0.729807 Jy selfcal ! Performing phase self-cal ! Adding 62 model components to the UV plane model. ! The established model now contains 241 components and 0.729807 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.052128Jy sigma=0.396370 ! Fit after self-cal, rms=0.052077Jy sigma=0.395384 flux_cutoff = imstat(rms) * dynam ! Inverting map repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00217271 Jy ! Component: 100 - total flux cleaned = -0.00291742 Jy ! Component: 150 - total flux cleaned = -0.00320619 Jy ! Component: 200 - total flux cleaned = -0.00348414 Jy ! Total flux subtracted in 200 components = -0.00348414 Jy ! Clean residual min=-0.002443 max=0.002444 Jy/beam ! Clean residual mean=-0.000012 rms=0.001024 Jy/beam ! Combined flux in latest and established models = 0.726322 Jy ! Performing phase self-cal ! Adding 82 model components to the UV plane model. ! The established model now contains 319 components and 0.726322 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.051386Jy sigma=0.391023 ! Fit after self-cal, rms=0.051357Jy sigma=0.390588 ! Inverting map selfcal true, true, soltime2 ! Performing amp+phase self-cal over 15 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.051357Jy sigma=0.390588 ! Fit after self-cal, rms=0.051469Jy sigma=0.390292 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=5.498 mas, bmaj=57.53 mas, bpa=8.14 degrees ! Estimated noise=13.1238 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000693311 Jy ! Component: 100 - total flux cleaned = -0.00106002 Jy ! Component: 150 - total flux cleaned = -0.00118019 Jy ! Component: 200 - total flux cleaned = -0.00083537 Jy ! Total flux subtracted in 200 components = -0.00083537 Jy ! Clean residual min=-0.001933 max=0.001962 Jy/beam ! Clean residual mean=-0.000018 rms=0.000841 Jy/beam ! Combined flux in latest and established models = 0.725487 Jy selfcal ! Performing phase self-cal ! Adding 69 model components to the UV plane model. ! The established model now contains 379 components and 0.725487 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.050950Jy sigma=0.387134 ! Fit after self-cal, rms=0.050952Jy sigma=0.386985 flux_cutoff = imstat(rms) * dynam ! Inverting map repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.62799e-05 Jy ! Component: 100 - total flux cleaned = 0.000134514 Jy ! Component: 150 - total flux cleaned = 0.000237537 Jy ! Component: 200 - total flux cleaned = 0.000438888 Jy ! Total flux subtracted in 200 components = 0.000438888 Jy ! Clean residual min=-0.001671 max=0.001689 Jy/beam ! Clean residual mean=-0.000024 rms=0.000731 Jy/beam ! Combined flux in latest and established models = 0.725926 Jy ! Performing phase self-cal ! Adding 67 model components to the UV plane model. ! The established model now contains 433 components and 0.725926 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.050552Jy sigma=0.384499 ! Fit after self-cal, rms=0.050561Jy sigma=0.384410 ! Inverting map uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. win_mult = win_mult * 1.2 selfcal true, true, soltime2 ! Performing amp+phase self-cal over 15 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.050561Jy sigma=0.384410 ! Fit after self-cal, rms=0.050603Jy sigma=0.384316 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=5.586 mas, bmaj=57.17 mas, bpa=8.129 degrees ! Estimated noise=13.1879 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00035252 Jy ! Component: 100 - total flux cleaned = -0.00064464 Jy ! Component: 150 - total flux cleaned = -0.000644718 Jy ! Component: 200 - total flux cleaned = -0.000270206 Jy ! Total flux subtracted in 200 components = -0.000270206 Jy ! Clean residual min=-0.001552 max=0.001537 Jy/beam ! Clean residual mean=-0.000010 rms=0.000662 Jy/beam ! Combined flux in latest and established models = 0.725656 Jy selfcal ! Performing phase self-cal ! Adding 74 model components to the UV plane model. ! The established model now contains 479 components and 0.725655 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.050252Jy sigma=0.382224 ! Fit after self-cal, rms=0.050260Jy sigma=0.382159 flux_cutoff = imstat(rms) * dynam ! Inverting map repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000108247 Jy ! Component: 100 - total flux cleaned = 0.00019584 Jy ! Component: 150 - total flux cleaned = 0.000366756 Jy ! Component: 200 - total flux cleaned = 0.000699275 Jy ! Total flux subtracted in 200 components = 0.000699275 Jy ! Clean residual min=-0.001379 max=0.001391 Jy/beam ! Clean residual mean=-0.000020 rms=0.000587 Jy/beam ! Combined flux in latest and established models = 0.726355 Jy ! Performing phase self-cal ! Adding 62 model components to the UV plane model. ! The established model now contains 519 components and 0.726355 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.049988Jy sigma=0.380529 ! Fit after self-cal, rms=0.049999Jy sigma=0.380468 ! Inverting map uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "=== Finished amplitude self-cal for VLBA stations ===" ! === Finished amplitude self-cal for VLBA stations === unflag * ! Unflagging all baselines in the currently selected channels. uncalib false, false, true ! uncal: All telescope correction flags have been un-done. integer lun lun = outfile ( "/tmp/ff.ff" ) do i=1,nsub do j=1,ntel(i) fprintf lun, "%s\n", telname(j,i) end do end do close ( lun ) system "/home/lpetrov/bin/dimap_selfant_process.csh /tmp/ff.ff" ![@/tmp/ff.ff] 1:FD ! Syntax error in line: ! 1:FD ! ^ ! Found constant: 1.000 ! Where a command or assignment expression was expected. ![Exited script file: /tmp/ff.ff] ![Exited script file: /home/lpetrov/bin/rdv_muppet] ! wmap "/d2/scr/pima/rdv96_uvs/J1006-5018_X\_map.fits" ! Inverting map and beam ! Estimated beam: bmin=5.269 mas, bmaj=41.74 mas, bpa=3.762 degrees ! Estimated noise=10.2463 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 5.269 x 41.74 at 3.762 degrees (North through East) ! Clean map min=-0.028568 max=0.67494 Jy/beam ! Writing clean map to FITS file: /d2/scr/pima/rdv96_uvs/J1006-5018_X_map.fits float peak_flux peak_flux = peak(flux,max) invert ! Inverting map float image_peak image_peak = int(10000*peak_flux)/10000 float image_rms image_rms = int(100000*imstat(rms))/100000 print "=========================================" ! ========================================= print "The image peak= ", image_peak, " rms= ", image_rms, " Jy" ! The image peak= 0.6749 rms= 0.00497 Jy quit ! Quitting program ! Log file /d2/scr/pima/rdv96_uvs/J1006-5018_X_uvs.log closed on Fri Dec 20 23:44:56 2013