! Started logfile: /d2/scr/pima/rdv96_uvs/J1056+7011_X_uvs.log on Fri Dec 20 23:45:07 2013 obs /d2/scr/pima/rdv96_uvs/J1056+7011_X_uva.fits ! Reading UV FITS file: /d2/scr/pima/rdv96_uvs/J1056+7011_X_uva.fits ! AN table 1: 6 integrations on 36 of 36 possible baselines. ! AN table 2: 7 integrations on 6 of 6 possible baselines. ! AN table 3: 8 integrations on 21 of 21 possible baselines. ! AN table 4: 16 integrations on 15 of 15 possible baselines. ! AN table 5: 13 integrations on 36 of 36 possible baselines. ! AN table 6: 19 integrations on 45 of 45 possible baselines. ! AN table 7: 8 integrations on 45 of 45 possible baselines. ! AN table 8: 6 integrations on 45 of 45 possible baselines. ! AN table 9: 5 integrations on 15 of 15 possible baselines. ! AN table 10: 7 integrations on 36 of 36 possible baselines. ! Apparent sampling: 0.940258 visibilities/baseline/integration-bin. ! Found source: J1056+7011 ! ! 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 11080 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/J1056+7011_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:BR self-cal status=correctable weight=1 ! 1:FD self-cal status=correctable weight=1 ! 1:HN self-cal status=correctable weight=1 ! 1:KP self-cal status=correctable weight=1 ! 1:LA self-cal status=correctable weight=1 ! 1:MK self-cal status=correctable weight=1 ! 1:NL self-cal status=correctable weight=1 ! 1:OV self-cal status=correctable weight=1 ! 1:PT self-cal status=correctable weight=1 ! 2:KP self-cal status=correctable weight=1 ! 2:MK 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: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 ! 4:FD 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:NL self-cal status=correctable weight=1 ! 5:NY self-cal status=correctable weight=1 ! 5:OV self-cal status=correctable weight=1 ! 5:PT self-cal status=correctable weight=1 ! 6:BR self-cal status=correctable weight=1 ! 6:FD self-cal status=correctable weight=1 ! 6:HN self-cal status=correctable weight=1 ! 6:KP self-cal status=correctable weight=1 ! 6:LA 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 ! 6:WF self-cal status=correctable weight=1 ! 7:BR self-cal status=correctable weight=1 ! 7:FD self-cal status=correctable weight=1 ! 7:HN self-cal status=correctable weight=1 ! 7:KP self-cal status=correctable weight=1 ! 7:LA self-cal status=correctable weight=1 ! 7:NL self-cal status=correctable weight=1 ! 7:OV self-cal status=correctable weight=1 ! 7:PT self-cal status=correctable weight=1 ! 7:SC self-cal status=correctable weight=1 ! 7:WZ self-cal status=correctable weight=1 ! 8:BR self-cal status=correctable weight=1 ! 8:FD self-cal status=correctable weight=1 ! 8:HN self-cal status=correctable weight=1 ! 8:KP self-cal status=correctable weight=1 ! 8:LA self-cal status=correctable weight=1 ! 8:MK self-cal status=correctable weight=1 ! 8:NL self-cal status=correctable weight=1 ! 8:OV self-cal status=correctable weight=1 ! 8:PT self-cal status=correctable weight=1 ! 8:SC self-cal status=correctable weight=1 ! 9:BR self-cal status=correctable weight=1 ! 9:FD self-cal status=correctable weight=1 ! 9:KP self-cal status=correctable weight=1 ! 9:LA self-cal status=correctable weight=1 ! 9:MK self-cal status=correctable weight=1 ! 9:OV self-cal status=correctable weight=1 ! 10:BR self-cal status=correctable weight=1 ! 10:FD self-cal status=correctable weight=1 ! 10:HN self-cal status=correctable weight=1 ! 10:KP self-cal status=correctable weight=1 ! 10:LA self-cal status=correctable weight=1 ! 10:MK self-cal status=correctable weight=1 ! 10:NL self-cal status=correctable weight=1 ! 10:OV self-cal status=correctable weight=1 ! 10:SC 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. ! A total of 4 telescope corrections were flagged in sub-array 3. ! A total of 4 telescope corrections were flagged in sub-array 5. ! A total of 8 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 4 telescope corrections were flagged in sub-array 3. ! A total of 4 telescope corrections were flagged in sub-array 5. ! A total of 8 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 4 telescope corrections were flagged in sub-array 3. ! A total of 17 telescope corrections were flagged in sub-array 5. ! A total of 8 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 4 telescope corrections were flagged in sub-array 3. ! A total of 17 telescope corrections were flagged in sub-array 5. ! A total of 8 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.013720Jy sigma=2.063104 ! Fit after self-cal, rms=0.860176Jy sigma=1.739049 ! 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=0.9604 mas, bmaj=1.279 mas, bpa=-64.39 degrees ! Estimated noise=5.98357 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 = 0.108299 Jy ! Component: 100 - total flux cleaned = 0.133769 Jy ! Total flux subtracted in 100 components = 0.133769 Jy ! Clean residual min=-0.003770 max=0.009721 Jy/beam ! Clean residual mean=0.000016 rms=0.000835 Jy/beam ! Combined flux in latest and established models = 0.133769 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 8 components and 0.133769 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.063329Jy sigma=0.115380 ! Fit after self-cal, rms=0.063251Jy sigma=0.115343 ! Inverting map ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0103522 Jy ! Component: 100 - total flux cleaned = 0.0155365 Jy ! Total flux subtracted in 100 components = 0.0155365 Jy ! Clean residual min=-0.003040 max=0.003046 Jy/beam ! Clean residual mean=0.000007 rms=0.000698 Jy/beam ! Combined flux in latest and established models = 0.149305 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 16 components and 0.149305 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.061346Jy sigma=0.110238 ! Fit after self-cal, rms=0.061361Jy sigma=0.110228 ! 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=1.263 mas, bmaj=1.837 mas, bpa=-68.31 degrees ! Estimated noise=3.43964 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 (-0.2, -1). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00417698 Jy ! Component: 100 - total flux cleaned = 0.00673241 Jy ! Component: 150 - total flux cleaned = 0.00848734 Jy ! Component: 200 - total flux cleaned = 0.00972809 Jy ! Total flux subtracted in 200 components = 0.00972809 Jy ! Clean residual min=-0.002340 max=0.002016 Jy/beam ! Clean residual mean=0.000015 rms=0.000502 Jy/beam ! Combined flux in latest and established models = 0.159033 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 39 components and 0.159033 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.061035Jy sigma=0.109456 ! Fit after self-cal, rms=0.061025Jy sigma=0.109418 ! 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: ! BR 0.99 FD 1.02 HN 0.95 KP 0.97 ! LA 1.04 MK 1.05 NL 0.95 OV 0.99 ! PT 0.96 ! ! Telescope amplitude corrections in sub-array 2: ! KP 0.98 MK 0.91 OV 0.95 PT 0.99 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.02 KP 0.98 LA 1.07 ! NL 0.98 OV 0.97 PT 1.03 ! ! Telescope amplitude corrections in sub-array 4: ! FD 0.95 KP 0.99 LA 1.04 NL 0.96 ! OV 1.00 PT 1.02 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.94 FD 1.05 HN 1.01 KP 1.04 ! LA 1.02 NL 0.98 NY 0.89 OV 0.99 ! PT 1.01 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.97 FD 0.99 HN 1.03 KP 1.00 ! LA 1.04 NL 0.92 OV 0.97 PT 0.99 ! SC 1.00 WF 0.80 ! ! Telescope amplitude corrections in sub-array 7: ! BR 0.99 FD 0.95 HN 1.06 KP 1.01 ! LA 0.98 NL 0.98 OV 0.94 PT 0.99 ! SC 1.05 WZ 3.17 ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.98 FD 0.97 HN 0.95 KP 0.99 ! LA 1.05 MK 0.97 NL 0.99 OV 1.03 ! PT 0.96 SC 0.93 ! ! Telescope amplitude corrections in sub-array 9: ! BR 0.99 FD 1.00 KP 0.99 LA 1.00 ! MK 0.98 OV 0.98 ! ! Telescope amplitude corrections in sub-array 10: ! BR 0.99 FD 1.02 HN 1.01 KP 0.97 ! LA 1.03 MK 0.97 NL 1.02 OV 0.97 ! SC 1.04 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.95 FD 1.03 HN 0.99 KP 0.96 ! LA 1.00 MK 1.03 NL 0.99 OV 0.95 ! PT 1.03 ! ! Telescope amplitude corrections in sub-array 2: ! KP 1.06 MK 1.28 OV 0.88 PT 0.97 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 FD 1.11 KP 1.01 LA 0.99 ! NL 0.98 OV 1.05 PT 0.93 ! ! Telescope amplitude corrections in sub-array 4: ! FD 1.01 KP 0.98 LA 1.04 NL 0.97 ! OV 1.02 PT 1.01 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.95 FD 0.98 HN 0.95 KP 0.98 ! LA 1.00 NL 0.94 NY 0.92 OV 1.03 ! PT 0.98 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.97 FD 1.01 HN 1.02 KP 0.94 ! LA 0.98 NL 0.97 OV 1.02 PT 0.97 ! SC 0.97 WF 0.82 ! ! Telescope amplitude corrections in sub-array 7: ! BR 0.93 FD 0.99 HN 0.97 KP 1.03 ! LA 1.00 NL 1.01 OV 0.95 PT 0.98 ! SC 1.07 WZ 1.97 ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.92 FD 1.00 HN 0.97 KP 0.91 ! LA 0.96 MK 0.97 NL 0.97 OV 0.99 ! PT 1.00 SC 1.06 ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.01 FD 0.91 KP 0.93 LA 0.98 ! MK 1.03 OV 1.00 ! ! Telescope amplitude corrections in sub-array 10: ! BR 0.97 FD 0.95 HN 0.96 KP 0.97 ! LA 0.96 MK 1.01 NL 1.06 OV 0.97 ! SC 1.14 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 FD 0.98 HN 1.09 KP 0.85 ! LA 1.09 MK 1.00 NL 0.98 OV 1.04 ! PT 1.02 ! ! Telescope amplitude corrections in sub-array 2: ! KP 0.83 MK 1.06 OV 1.02 PT 1.04 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.09 FD 1.11 KP 0.80 LA 1.23 ! NL 1.01 OV 1.02 PT 1.08 ! ! Telescope amplitude corrections in sub-array 4: ! FD 0.98 KP 0.87 LA 1.11 NL 0.99 ! OV 1.10 PT 0.98 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 1.00 HN 1.04 KP 0.89 ! LA 1.09 NL 0.97 NY 1.00* OV 1.07 ! PT 0.99 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.03 FD 0.98 HN 1.09 KP 0.82 ! LA 1.08 NL 1.05 OV 1.06 PT 0.99 ! SC 0.93 WF 0.93 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.07 FD 0.97 HN 1.04 KP 0.83 ! LA 1.12 NL 1.00 OV 1.09 PT 1.01 ! SC 0.96 WZ 2.85 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.09 FD 0.97 HN 1.06 KP 0.86 ! LA 1.08 MK 0.99 NL 1.05 OV 1.06 ! PT 1.02 SC 0.97 ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.17 FD 1.05 KP 0.76 LA 1.10 ! MK 1.03 OV 1.08 ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.03 FD 1.04 HN 1.06 KP 0.82 ! LA 1.08 MK 1.05 NL 1.05 OV 1.08 ! SC 1.16 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.06 FD 1.03 HN 1.03 KP 0.86 ! LA 1.11 MK 1.03 NL 1.05 OV 0.96 ! PT 1.10 ! ! Telescope amplitude corrections in sub-array 2: ! KP 0.94 MK 0.90 OV 0.98 PT 1.10 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.07 FD 1.04 KP 0.88 LA 1.11 ! NL 0.99 OV 1.05 PT 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! FD 1.10 KP 0.95 LA 1.15 NL 1.04 ! OV 1.00 PT 0.99 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.96 FD 1.10 HN 1.04 KP 0.95 ! LA 1.05 NL 0.99 NY 1.00* OV 1.02 ! PT 1.07 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.10 FD 1.04 HN 1.06 KP 0.91 ! LA 1.00 NL 0.98 OV 1.01 PT 1.05 ! SC 1.06 WF 0.98 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.03 FD 1.14 HN 0.96 KP 0.91 ! LA 1.08 NL 1.12 OV 1.14 PT 1.03 ! SC 0.99 WZ 2.51 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.06 FD 1.04 HN 0.97 KP 0.90 ! LA 1.09 MK 1.01 NL 1.12 OV 1.01 ! PT 1.00 SC 1.03 ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.09 FD 1.13 KP 0.92 LA 1.08 ! MK 0.92 OV 1.04 ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.03 FD 1.04 HN 1.20 KP 0.87 ! LA 1.08 MK 1.00 NL 1.07 OV 1.12 ! SC 1.16 ! ! ! Fit before self-cal, rms=0.061025Jy sigma=0.109418 ! Fit after self-cal, rms=0.059442Jy sigma=0.106050 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=1.265 mas, bmaj=1.895 mas, bpa=-68.17 degrees ! Estimated noise=3.43154 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 = 0.000972972 Jy ! Component: 100 - total flux cleaned = 0.000913731 Jy ! Component: 150 - total flux cleaned = 0.0009387 Jy ! Component: 200 - total flux cleaned = 0.000919189 Jy ! Total flux subtracted in 200 components = 0.000919189 Jy ! Clean residual min=-0.001506 max=0.001406 Jy/beam ! Clean residual mean=0.000013 rms=0.000345 Jy/beam ! Combined flux in latest and established models = 0.159953 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 49 components and 0.159953 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.059411Jy sigma=0.105992 ! Fit after self-cal, rms=0.059449Jy sigma=0.105951 ! 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=0.059449Jy sigma=0.105951 ! Fit after self-cal, rms=0.059333Jy sigma=0.105944 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=1.263 mas, bmaj=1.894 mas, bpa=-68.2 degrees ! Estimated noise=3.42988 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000417041 Jy ! Component: 100 - total flux cleaned = 0.000440427 Jy ! Component: 150 - total flux cleaned = 0.000421638 Jy ! Component: 200 - total flux cleaned = 0.000422159 Jy ! Total flux subtracted in 200 components = 0.000422159 Jy ! Clean residual min=-0.001507 max=0.001396 Jy/beam ! Clean residual mean=0.000011 rms=0.000342 Jy/beam ! Combined flux in latest and established models = 0.160375 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 56 components and 0.160375 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.059315Jy sigma=0.105916 ! Fit after self-cal, rms=0.059314Jy sigma=0.105913 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 = 9.22522e-05 Jy ! Component: 100 - total flux cleaned = 9.3375e-05 Jy ! Component: 150 - total flux cleaned = 9.34694e-05 Jy ! Component: 200 - total flux cleaned = 9.30892e-05 Jy ! Total flux subtracted in 200 components = 9.30892e-05 Jy ! Clean residual min=-0.001516 max=0.001395 Jy/beam ! Clean residual mean=0.000011 rms=0.000341 Jy/beam ! Combined flux in latest and established models = 0.160468 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 62 components and 0.160468 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.059305Jy sigma=0.105901 ! Fit after self-cal, rms=0.059304Jy sigma=0.105900 ! 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=0.059304Jy sigma=0.105900 ! Fit after self-cal, rms=0.059123Jy sigma=0.105810 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=1.261 mas, bmaj=1.894 mas, bpa=-68.27 degrees ! Estimated noise=3.4262 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 7.75278e-05 Jy ! Component: 100 - total flux cleaned = 0.000108972 Jy ! Component: 150 - total flux cleaned = 0.000109967 Jy ! Component: 200 - total flux cleaned = 0.000122733 Jy ! Total flux subtracted in 200 components = 0.000122733 Jy ! Clean residual min=-0.001470 max=0.001326 Jy/beam ! Clean residual mean=0.000009 rms=0.000335 Jy/beam ! Combined flux in latest and established models = 0.160591 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 66 components and 0.160591 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.059113Jy sigma=0.105799 ! Fit after self-cal, rms=0.059114Jy sigma=0.105797 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 = 7.14632e-05 Jy ! Component: 100 - total flux cleaned = 6.0136e-05 Jy ! Component: 150 - total flux cleaned = 6.05586e-05 Jy ! Component: 200 - total flux cleaned = 6.06482e-05 Jy ! Total flux subtracted in 200 components = 6.06482e-05 Jy ! Clean residual min=-0.001478 max=0.001325 Jy/beam ! Clean residual mean=0.000009 rms=0.000334 Jy/beam ! Combined flux in latest and established models = 0.160651 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 71 components and 0.160651 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.059108Jy sigma=0.105791 ! Fit after self-cal, rms=0.059109Jy sigma=0.105791 ! 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=0.059109Jy sigma=0.105791 ! Fit after self-cal, rms=0.058985Jy sigma=0.105788 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=2.592 mas, bmaj=3.255 mas, bpa=-53.72 degrees ! Estimated noise=3.73371 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000349117 Jy ! Component: 100 - total flux cleaned = 0.000385256 Jy ! Component: 150 - total flux cleaned = 0.000392174 Jy ! Component: 200 - total flux cleaned = 0.000397875 Jy ! Total flux subtracted in 200 components = 0.000397875 Jy ! Clean residual min=-0.001284 max=0.001387 Jy/beam ! Clean residual mean=0.000013 rms=0.000373 Jy/beam ! Combined flux in latest and established models = 0.161049 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 81 components and 0.161049 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.058986Jy sigma=0.105784 ! Fit after self-cal, rms=0.058985Jy sigma=0.105783 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 = 7.24548e-05 Jy ! Component: 100 - total flux cleaned = 8.74921e-05 Jy ! Component: 150 - total flux cleaned = 9.48439e-05 Jy ! Component: 200 - total flux cleaned = 9.83361e-05 Jy ! Total flux subtracted in 200 components = 9.83361e-05 Jy ! Clean residual min=-0.001273 max=0.001385 Jy/beam ! Clean residual mean=0.000013 rms=0.000373 Jy/beam ! Combined flux in latest and established models = 0.161147 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 85 components and 0.161147 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.058985Jy sigma=0.105782 ! Fit after self-cal, rms=0.058985Jy sigma=0.105782 ! 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. ! Applying 2560 buffered edits. 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:BR ! Syntax error in line: ! 1:BR ! ^ ! 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/J1056+7011_X\_map.fits" ! Inverting map and beam ! Estimated beam: bmin=1.259 mas, bmaj=1.895 mas, bpa=-68.34 degrees ! Estimated noise=3.42231 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.259 x 1.895 at -68.34 degrees (North through East) ! Clean map min=-0.0013715 max=0.1409 Jy/beam ! Writing clean map to FITS file: /d2/scr/pima/rdv96_uvs/J1056+7011_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= 0.1408 rms= 0.00033 Jy quit ! Quitting program ! Log file /d2/scr/pima/rdv96_uvs/J1056+7011_X_uvs.log closed on Fri Dec 20 23:45:09 2013