! Started logfile: /scr/pima/rdv96_uvs/J1113+1442_S_uvs.log on Sat Dec 21 00:23:41 2013 obs /scr/pima/rdv96_uvs/J1113+1442_S_uva.fits ! Reading UV FITS file: /scr/pima/rdv96_uvs/J1113+1442_S_uva.fits ! AN table 1: 6 integrations on 10 of 10 possible baselines. ! AN table 2: 3 integrations on 15 of 15 possible baselines. ! AN table 3: 7 integrations on 45 of 45 possible baselines. ! AN table 4: 3 integrations on 21 of 21 possible baselines. ! AN table 5: 14 integrations on 55 of 55 possible baselines. ! AN table 6: 4 integrations on 36 of 36 possible baselines. ! AN table 7: 6 integrations on 6 of 6 possible baselines. ! Apparent sampling: 0.831821 visibilities/baseline/integration-bin. ! Found source: J1113+1442 ! ! 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 2.23299e+09 8e+06 1 8e+06 ! 02 2 2.26299e+09 8e+06 1 8e+06 ! 03 3 2.35299e+09 8e+06 1 8e+06 ! 04 4 2.37299e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 0 lines of history. ! ! Reading 4768 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 = 0.4 print "taper_size =",taper_size ! taper_size = 20 ![@/home/lpetrov/bin/rdv_muppet /scr/pima/rdv96_uvs/J1113+1442_S] 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:HN self-cal status=correctable weight=1 ! 1:LA self-cal status=correctable weight=1 ! 1:NL self-cal status=correctable weight=1 ! 1:SC self-cal status=correctable weight=1 ! 2:BR 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:OV self-cal status=correctable weight=1 ! 2:PT self-cal status=correctable weight=1 ! 3:BR self-cal status=correctable weight=1 ! 3:FD self-cal status=correctable weight=1 ! 3:HN self-cal status=correctable weight=1 ! 3:KP self-cal status=correctable weight=1 ! 3:LA self-cal status=correctable weight=1 ! 3:NL self-cal status=correctable weight=1 ! 3:OV self-cal status=correctable weight=1 ! 3:PT self-cal status=correctable weight=1 ! 3:SC self-cal status=correctable weight=1 ! 3:WZ self-cal status=correctable weight=1 ! 4:BR self-cal status=correctable weight=1 ! 4:HN self-cal status=correctable weight=1 ! 4:KP self-cal status=correctable weight=1 ! 4:LA self-cal status=correctable weight=1 ! 4:NL self-cal status=correctable weight=1 ! 4:OV self-cal status=correctable weight=1 ! 4:PT self-cal status=correctable weight=1 ! 5:BR self-cal status=correctable weight=1 ! 5:FD self-cal status=correctable weight=1 ! 5:HN self-cal status=correctable weight=1 ! 5:KP self-cal status=correctable weight=1 ! 5:LA self-cal status=correctable weight=1 ! 5:MK self-cal status=correctable weight=1 ! 5:NL self-cal status=correctable weight=1 ! 5:OV self-cal status=correctable weight=1 ! 5:PT self-cal status=correctable weight=1 ! 5:SC self-cal status=correctable weight=1 ! 5:WF self-cal status=correctable weight=1 ! 6:BR self-cal status=correctable weight=1 ! 6:FD self-cal status=correctable weight=1 ! 6:KP self-cal status=correctable weight=1 ! 6:LA self-cal status=correctable weight=1 ! 6:MK self-cal status=correctable weight=1 ! 6:NL self-cal status=correctable weight=1 ! 6:OV self-cal status=correctable weight=1 ! 6:PT self-cal status=correctable weight=1 ! 6:SC self-cal status=correctable weight=1 ! 7:BR self-cal status=correctable weight=1 ! 7:HN self-cal status=correctable weight=1 ! 7:NL self-cal status=correctable weight=1 ! 7:WF self-cal status=correctable weight=1 system "rm /tmp/ff.ff" mapsize field_size, field_cell ! Map grid = 1024x1024 pixels with 0.400x0.400 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. ! A total of 5 telescope corrections were flagged in sub-array 1. ! A total of 35 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 5 telescope corrections were flagged in sub-array 1. ! A total of 35 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 5 telescope corrections were flagged in sub-array 1. ! A total of 35 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 5 telescope corrections were flagged in sub-array 1. ! A total of 35 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=1.075688Jy sigma=6.189581 ! Fit after self-cal, rms=0.632950Jy sigma=3.477707 ! 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 \] flag 3:WZ ! Flagging baselines of antenna 3:WZ in the currently selected channels. flag 5:WF ! Flagging baselines of antenna 5:WF in the currently selected channels. flag 7:WF ! Flagging baselines of antenna 7:WF in the currently selected channels. ![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=3.374 mas, bmaj=7.092 mas, bpa=6.104 degrees ! Estimated noise=2.86367 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) ! Added new window around map position (0, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.297306 Jy ! Component: 100 - total flux cleaned = 0.369529 Jy ! Total flux subtracted in 100 components = 0.369529 Jy ! Clean residual min=-0.009081 max=0.027339 Jy/beam ! Clean residual mean=-0.000003 rms=0.002629 Jy/beam ! Combined flux in latest and established models = 0.369529 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 11 components and 0.369529 Jy ! ! Correcting IF 1. ! A total of 7 telescope corrections were flagged in sub-array 3. ! A total of 12 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 2. ! A total of 7 telescope corrections were flagged in sub-array 3. ! A total of 12 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 3. ! A total of 7 telescope corrections were flagged in sub-array 3. ! A total of 12 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 4. ! A total of 7 telescope corrections were flagged in sub-array 3. ! A total of 12 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 7. ! ! Fit before self-cal, rms=0.083092Jy sigma=0.518933 ! Fit after self-cal, rms=0.082992Jy sigma=0.518445 ! Inverting map and beam ! Estimated beam: bmin=3.374 mas, bmaj=7.092 mas, bpa=6.104 degrees ! Estimated noise=2.86367 mJy/beam. ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0268288 Jy ! Component: 100 - total flux cleaned = 0.0386077 Jy ! Total flux subtracted in 100 components = 0.0386077 Jy ! Clean residual min=-0.007144 max=0.007939 Jy/beam ! Clean residual mean=0.000010 rms=0.001882 Jy/beam ! Combined flux in latest and established models = 0.408137 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 24 components and 0.408137 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.073536Jy sigma=0.445114 ! Fit after self-cal, rms=0.073512Jy sigma=0.444936 ! 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=4.193 mas, bmaj=8.352 mas, bpa=6.572 degrees ! Estimated noise=1.89939 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 = 0.0106588 Jy ! Component: 100 - total flux cleaned = 0.0156823 Jy ! Component: 150 - total flux cleaned = 0.0184589 Jy ! Component: 200 - total flux cleaned = 0.0192515 Jy ! Total flux subtracted in 200 components = 0.0192515 Jy ! Clean residual min=-0.006233 max=0.007468 Jy/beam ! Clean residual mean=0.000022 rms=0.001790 Jy/beam ! Combined flux in latest and established models = 0.427389 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 46 components and 0.427389 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.072483Jy sigma=0.433904 ! Fit after self-cal, rms=0.072454Jy sigma=0.433748 ! 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. ! Telescope amplitude corrections in sub-array 1: ! FD 1.04 HN 0.97 LA 1.21 NL 1.14 ! SC 0.85 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.07 FD 1.03 KP 1.09 LA 1.23 ! OV 1.02 PT 1.07 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 0.99 HN 0.99 KP 1.00 ! LA 1.17 NL 0.99 OV 1.01 PT 1.04 ! SC 0.91 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.04 HN 0.98 KP 1.02 LA 1.18 ! NL 1.02 OV 1.01 PT 1.07 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 FD 0.99 HN 0.98 KP 1.00 ! LA 1.15 MK 0.87 NL 1.00 OV 1.01 ! PT 1.03 SC 0.96 WF 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.99 FD 0.99 KP 1.00 LA 1.16 ! MK 0.97 NL 1.04 OV 0.98 PT 1.11 ! SC 0.95 ! ! A total of 18 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 0.00* HN 0.00* NL 0.00* WF 0.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! FD 1.09 HN 1.12 LA 1.05 NL 1.05 ! SC 0.96 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 1.09 KP 1.01 LA 1.10 ! OV 1.14 PT 1.07 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 FD 1.05 HN 1.02 KP 1.04 ! LA 1.02 NL 1.04 OV 1.01 PT 1.02 ! SC 1.01 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.05 HN 1.10 KP 1.04 LA 1.04 ! NL 1.07 OV 1.06 PT 1.06 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 1.05 HN 1.03 KP 1.00 ! LA 1.05 MK 1.02 NL 1.02 OV 1.04 ! PT 1.02 SC 1.06 WF 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.04 FD 1.05 KP 1.00 LA 1.03 ! MK 1.04 NL 1.07 OV 1.06 PT 1.04 ! SC 1.08 ! ! A total of 18 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 0.00* HN 0.00* NL 0.00* WF 0.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! FD 1.13 HN 1.04 LA 1.03 NL 1.06 ! SC 0.88 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.08 FD 1.09 KP 0.94 LA 1.02 ! OV 1.07 PT 1.08 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 FD 1.07 HN 0.99 KP 0.91 ! LA 0.99 NL 1.09 OV 1.03 PT 1.04 ! SC 0.96 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 HN 1.00 KP 0.90 LA 0.98 ! NL 1.17 OV 1.08 PT 1.11 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.05 FD 1.06 HN 1.01 KP 0.89 ! LA 0.96 MK 1.00 NL 1.06 OV 1.03 ! PT 1.07 SC 0.94 WF 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.07 FD 1.06 KP 0.90 LA 1.00 ! MK 1.05 NL 1.08 OV 1.06 PT 1.05 ! SC 1.00 ! ! A total of 18 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 0.00* HN 0.00* NL 0.00* WF 0.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! FD 1.18 HN 0.89 LA 0.80 NL 1.07 ! SC 1.02 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.10 FD 1.07 KP 0.87 LA 0.84 ! OV 0.86 PT 0.94 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.08 HN 0.90 KP 0.84 ! LA 0.83 NL 1.02 OV 0.90 PT 0.92 ! SC 1.02 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 HN 0.92 KP 0.83 LA 0.84 ! NL 1.04 OV 0.93 PT 0.95 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 FD 1.08 HN 0.90 KP 0.83 ! LA 0.81 MK 1.14 NL 1.01 OV 0.87 ! PT 0.92 SC 1.01 WF 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.02 FD 1.07 KP 0.83 LA 0.85 ! MK 1.15 NL 1.07 OV 0.89 PT 0.91 ! SC 1.02 ! ! A total of 18 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 0.00* HN 0.00* NL 0.00* WF 0.00* ! ! ! Fit before self-cal, rms=0.072454Jy sigma=0.433748 ! Fit after self-cal, rms=0.053577Jy sigma=0.293562 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=4.175 mas, bmaj=8.305 mas, bpa=6.93 degrees ! Estimated noise=1.91028 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 = -0.00109957 Jy ! Component: 100 - total flux cleaned = -0.00120812 Jy ! Component: 150 - total flux cleaned = -0.00134045 Jy ! Component: 200 - total flux cleaned = -0.0014567 Jy ! Total flux subtracted in 200 components = -0.0014567 Jy ! Clean residual min=-0.003120 max=0.003150 Jy/beam ! Clean residual mean=-0.000005 rms=0.000657 Jy/beam ! Combined flux in latest and established models = 0.425932 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 54 components and 0.425932 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.053426Jy sigma=0.293002 ! Fit after self-cal, rms=0.053447Jy sigma=0.292834 ! 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=0.053447Jy sigma=0.292834 ! Fit after self-cal, rms=0.053466Jy sigma=0.292743 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=4.174 mas, bmaj=8.315 mas, bpa=6.914 degrees ! Estimated noise=1.91063 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000838802 Jy ! Component: 100 - total flux cleaned = -0.000872659 Jy ! Component: 150 - total flux cleaned = -0.000941991 Jy ! Component: 200 - total flux cleaned = -0.00106383 Jy ! Total flux subtracted in 200 components = -0.00106383 Jy ! Clean residual min=-0.002854 max=0.003125 Jy/beam ! Clean residual mean=-0.000005 rms=0.000639 Jy/beam ! Combined flux in latest and established models = 0.424868 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 55 components and 0.424868 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.053372Jy sigma=0.292401 ! Fit after self-cal, rms=0.053356Jy sigma=0.292338 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) ! Added new window around map position (-22.4, 62). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00286331 Jy ! Component: 100 - total flux cleaned = 0.00369724 Jy ! Component: 150 - total flux cleaned = 0.00374849 Jy ! Component: 200 - total flux cleaned = 0.00383742 Jy ! Total flux subtracted in 200 components = 0.00383742 Jy ! Clean residual min=-0.002626 max=0.002168 Jy/beam ! Clean residual mean=-0.000001 rms=0.000566 Jy/beam ! Combined flux in latest and established models = 0.428705 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 79 components and 0.428706 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.053179Jy sigma=0.291185 ! Fit after self-cal, rms=0.053169Jy sigma=0.291127 ! 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=0.053169Jy sigma=0.291127 ! Fit after self-cal, rms=0.053227Jy sigma=0.290964 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=4.171 mas, bmaj=8.325 mas, bpa=6.88 degrees ! Estimated noise=1.91083 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000342013 Jy ! Component: 100 - total flux cleaned = 0.000470901 Jy ! Component: 150 - total flux cleaned = 0.000546786 Jy ! Component: 200 - total flux cleaned = 0.000547367 Jy ! Total flux subtracted in 200 components = 0.000547367 Jy ! Clean residual min=-0.002356 max=0.001999 Jy/beam ! Clean residual mean=-0.000001 rms=0.000539 Jy/beam ! Combined flux in latest and established models = 0.429253 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 85 components and 0.429253 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.053148Jy sigma=0.290602 ! Fit after self-cal, rms=0.053140Jy sigma=0.290576 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 = 6.42389e-05 Jy ! Component: 100 - total flux cleaned = 0.000130937 Jy ! Component: 150 - total flux cleaned = 0.00013034 Jy ! Component: 200 - total flux cleaned = 0.00013048 Jy ! Total flux subtracted in 200 components = 0.00013048 Jy ! Clean residual min=-0.002162 max=0.001976 Jy/beam ! Clean residual mean=-0.000001 rms=0.000532 Jy/beam ! Combined flux in latest and established models = 0.429383 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 89 components and 0.429383 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.053094Jy sigma=0.290395 ! Fit after self-cal, rms=0.053088Jy sigma=0.290382 ! Inverting map uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 20 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=0.053088Jy sigma=0.290382 ! Fit after self-cal, rms=0.053106Jy sigma=0.290308 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=8.781 mas, bmaj=11.58 mas, bpa=-6.302 degrees ! Estimated noise=2.11308 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00041399 Jy ! Component: 100 - total flux cleaned = -0.000391482 Jy ! Component: 150 - total flux cleaned = -0.000335522 Jy ! Component: 200 - total flux cleaned = -0.000318743 Jy ! Total flux subtracted in 200 components = -0.000318743 Jy ! Clean residual min=-0.001955 max=0.001901 Jy/beam ! Clean residual mean=-0.000003 rms=0.000567 Jy/beam ! Combined flux in latest and established models = 0.429065 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 103 components and 0.429065 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.053111Jy sigma=0.290183 ! Fit after self-cal, rms=0.053088Jy sigma=0.290115 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 = -1.74344e-06 Jy ! Component: 100 - total flux cleaned = 3.04312e-05 Jy ! Component: 150 - total flux cleaned = 3.05749e-05 Jy ! Component: 200 - total flux cleaned = 1.91099e-05 Jy ! Total flux subtracted in 200 components = 1.91099e-05 Jy ! Clean residual min=-0.001894 max=0.001825 Jy/beam ! Clean residual mean=-0.000003 rms=0.000558 Jy/beam ! Combined flux in latest and established models = 0.429084 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 108 components and 0.429084 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.053099Jy sigma=0.290046 ! Fit after self-cal, rms=0.053080Jy sigma=0.289996 ! 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 "/scr/pima/rdv96_uvs/J1113+1442_S\_map.fits" ! Inverting map and beam ! Estimated beam: bmin=3.514 mas, bmaj=8.117 mas, bpa=-0.5266 degrees ! Estimated noise=1.86937 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 3.514 x 8.117 at -0.5266 degrees (North through East) ! Clean map min=-0.0061764 max=0.37815 Jy/beam ! Writing clean map to FITS file: /scr/pima/rdv96_uvs/J1113+1442_S_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= 0.3781 rms= 0.00135 Jy quit ! Quitting program ! Log file /scr/pima/rdv96_uvs/J1113+1442_S_uvs.log closed on Sat Dec 21 00:23:43 2013