! Started logfile: /scr/pima/rdv96_uvs/J0533+4822_S_uvs.log on Sat Dec 21 00:22:34 2013 obs /scr/pima/rdv96_uvs/J0533+4822_S_uva.fits ! Reading UV FITS file: /scr/pima/rdv96_uvs/J0533+4822_S_uva.fits ! AN table 1: 2 integrations on 3 of 3 possible baselines. ! AN table 2: 2 integrations on 10 of 10 possible baselines. ! AN table 3: 2 integrations on 1 of 1 possible baselines. ! AN table 4: 6 integrations on 3 of 3 possible baselines. ! AN table 5: 2 integrations on 15 of 15 possible baselines. ! AN table 6: 2 integrations on 15 of 15 possible baselines. ! AN table 7: 2 integrations on 36 of 36 possible baselines. ! AN table 8: 3 integrations on 6 of 6 possible baselines. ! AN table 9: 4 integrations on 55 of 55 possible baselines. ! AN table 10: 2 integrations on 28 of 28 possible baselines. ! Apparent sampling: 0.987288 visibilities/baseline/integration-bin. ! Found source: J0533+4822 ! ! 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 1864 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/J0533+4822_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:BR self-cal status=correctable weight=1 ! 1:HN self-cal status=correctable weight=1 ! 1:NY self-cal status=correctable weight=1 ! 2:BR self-cal status=correctable weight=1 ! 2:HN self-cal status=correctable weight=1 ! 2:NL self-cal status=correctable weight=1 ! 2:NY self-cal status=correctable weight=1 ! 2:WZ self-cal status=correctable weight=1 ! 3:BR self-cal status=correctable weight=1 ! 3:WZ self-cal status=correctable weight=1 ! 4:NY self-cal status=correctable weight=1 ! 4:WF self-cal status=correctable weight=1 ! 4:WZ self-cal status=correctable weight=1 ! 5:BR self-cal status=correctable weight=1 ! 5:HN self-cal status=correctable weight=1 ! 5:LA self-cal status=correctable weight=1 ! 5:NL 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:HN self-cal status=correctable weight=1 ! 6:NL self-cal status=correctable weight=1 ! 6:SC self-cal status=correctable weight=1 ! 6:WF self-cal status=correctable weight=1 ! 6:WZ 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:PT self-cal status=correctable weight=1 ! 7:SC self-cal status=correctable weight=1 ! 7:WF self-cal status=correctable weight=1 ! 8:BR self-cal status=correctable weight=1 ! 8:MK self-cal status=correctable weight=1 ! 8:NY self-cal status=correctable weight=1 ! 8:WF self-cal status=correctable weight=1 ! 9:BR self-cal status=correctable weight=1 ! 9:FD self-cal status=correctable weight=1 ! 9:HN 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:NL self-cal status=correctable weight=1 ! 9:OV self-cal status=correctable weight=1 ! 9:PT self-cal status=correctable weight=1 ! 9:SC self-cal status=correctable weight=1 ! 9:WF self-cal status=correctable weight=1 ! 10:BR self-cal status=correctable weight=1 ! 10:FD 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:PT 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 4 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 4 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 4 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 4 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.136690Jy sigma=8.900931 ! Fit after self-cal, rms=0.504316Jy sigma=3.314473 ! 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 1:NY ! Flagging baselines of antenna 1:NY in the currently selected channels. flag 2:NY ! Flagging baselines of antenna 2:NY in the currently selected channels. flag 2:WZ ! Flagging baselines of antenna 2:WZ in the currently selected channels. flag 3:WZ ! Flagging baselines of antenna 3:WZ in the currently selected channels. flag 4:NY ! Flagging baselines of antenna 4:NY in the currently selected channels. flag 4:WF ! Flagging baselines of antenna 4:WF in the currently selected channels. flag 4:WZ ! Flagging baselines of antenna 4:WZ in the currently selected channels. flag 5:WF ! Flagging baselines of antenna 5:WF in the currently selected channels. flag 6:WF ! Flagging baselines of antenna 6:WF in the currently selected channels. flag 6:WZ ! Flagging baselines of antenna 6:WZ in the currently selected channels. flag 7:WF ! Flagging baselines of antenna 7:WF in the currently selected channels. flag 8:NY ! Flagging baselines of antenna 8:NY in the currently selected channels. flag 8:WF ! Flagging baselines of antenna 8:WF in the currently selected channels. flag 9:WF ! Flagging baselines of antenna 9: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=3.923 mas, bmaj=4.427 mas, bpa=-10.81 degrees ! Estimated noise=2.95353 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 = 0.439907 Jy ! Component: 100 - total flux cleaned = 0.544159 Jy ! Total flux subtracted in 100 components = 0.544159 Jy ! Clean residual min=-0.014250 max=0.039442 Jy/beam ! Clean residual mean=0.000066 rms=0.004156 Jy/beam ! Combined flux in latest and established models = 0.544159 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 10 components and 0.544159 Jy ! ! Correcting IF 1. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 4 telescope corrections were flagged in sub-array 2. ! A total of 12 telescope corrections were flagged in sub-array 4. ! A total of 2 telescope corrections were flagged in sub-array 5. ! A total of 4 telescope corrections were flagged in sub-array 6. ! A total of 2 telescope corrections were flagged in sub-array 7. ! A total of 12 telescope corrections were flagged in sub-array 8. ! A total of 4 telescope corrections were flagged in sub-array 9. ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 4 telescope corrections were flagged in sub-array 2. ! A total of 12 telescope corrections were flagged in sub-array 4. ! A total of 2 telescope corrections were flagged in sub-array 5. ! A total of 4 telescope corrections were flagged in sub-array 6. ! A total of 2 telescope corrections were flagged in sub-array 7. ! A total of 12 telescope corrections were flagged in sub-array 8. ! A total of 4 telescope corrections were flagged in sub-array 9. ! ! Correcting IF 3. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 4 telescope corrections were flagged in sub-array 2. ! A total of 12 telescope corrections were flagged in sub-array 4. ! A total of 2 telescope corrections were flagged in sub-array 5. ! A total of 4 telescope corrections were flagged in sub-array 6. ! A total of 2 telescope corrections were flagged in sub-array 7. ! A total of 12 telescope corrections were flagged in sub-array 8. ! A total of 4 telescope corrections were flagged in sub-array 9. ! ! Correcting IF 4. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 4 telescope corrections were flagged in sub-array 2. ! A total of 12 telescope corrections were flagged in sub-array 4. ! A total of 2 telescope corrections were flagged in sub-array 5. ! A total of 4 telescope corrections were flagged in sub-array 6. ! A total of 2 telescope corrections were flagged in sub-array 7. ! A total of 12 telescope corrections were flagged in sub-array 8. ! A total of 4 telescope corrections were flagged in sub-array 9. ! ! Fit before self-cal, rms=0.111980Jy sigma=1.034740 ! Fit after self-cal, rms=0.112350Jy sigma=1.040262 ! Inverting map and beam ! Estimated beam: bmin=3.924 mas, bmaj=4.413 mas, bpa=-11.12 degrees ! Estimated noise=2.97094 mJy/beam. ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0408539 Jy ! Component: 100 - total flux cleaned = 0.0603904 Jy ! Total flux subtracted in 100 components = 0.0603904 Jy ! Clean residual min=-0.010956 max=0.018771 Jy/beam ! Clean residual mean=0.000016 rms=0.003042 Jy/beam ! Combined flux in latest and established models = 0.604549 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 23 components and 0.604549 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.096359Jy sigma=0.848542 ! Fit after self-cal, rms=0.096166Jy sigma=0.847147 ! Inverting map ! Added new window around map position (4.8, 5.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.018929 Jy ! Component: 100 - total flux cleaned = 0.0304986 Jy ! Total flux subtracted in 100 components = 0.0304986 Jy ! Clean residual min=-0.010235 max=0.011483 Jy/beam ! Clean residual mean=-0.000004 rms=0.002710 Jy/beam ! Combined flux in latest and established models = 0.635048 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 39 components and 0.635048 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.091376Jy sigma=0.794970 ! Fit after self-cal, rms=0.090786Jy sigma=0.791002 ! 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=4.819 mas, bmaj=5.25 mas, bpa=-27.54 degrees ! Estimated noise=2.38053 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 = 0.0147789 Jy ! Component: 100 - total flux cleaned = 0.0233871 Jy ! Component: 150 - total flux cleaned = 0.0289209 Jy ! Component: 200 - total flux cleaned = 0.0324972 Jy ! Total flux subtracted in 200 components = 0.0324972 Jy ! Clean residual min=-0.008582 max=0.010203 Jy/beam ! Clean residual mean=-0.000053 rms=0.002283 Jy/beam ! Combined flux in latest and established models = 0.667545 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 59 components and 0.667545 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.088696Jy sigma=0.764433 ! Fit after self-cal, rms=0.088421Jy sigma=0.762603 ! 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 0.00* HN 0.00* NY 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* HN 0.00* NL 0.00* NY 0.00* ! WZ 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! NY 0.00* WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 HN 1.07 LA 1.28 NL 1.00 ! SC 0.94 WF 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.07 HN 1.02 NL 0.97 SC 1.02 ! WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.02 FD 1.01 HN 1.02 KP 1.03 ! LA 1.17 NL 1.01 PT 1.05 SC 0.89 ! WF 1.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.00* MK 0.00* NY 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.00 FD 0.97 HN 1.00 KP 1.00 ! LA 1.16 MK 0.96 NL 0.96 OV 0.98 ! PT 1.04 SC 0.95 WF 1.00* ! ! Telescope amplitude corrections in sub-array 10: ! BR 0.98 FD 0.99 KP 1.04 LA 1.19 ! MK 0.97 NL 1.04 OV 1.00 PT 1.01 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* HN 0.00* NY 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* HN 0.00* NL 0.00* NY 0.00* ! WZ 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! NY 0.00* WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.05 HN 1.06 LA 1.18 NL 1.06 ! SC 1.09 WF 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.12 HN 1.06 NL 1.05 SC 1.00 ! WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.06 FD 1.06 HN 1.11 KP 1.08 ! LA 1.06 NL 1.04 PT 1.07 SC 1.00 ! WF 1.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.00* MK 0.00* NY 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.04 FD 1.03 HN 1.06 KP 1.03 ! LA 1.02 MK 1.08 NL 1.00 OV 1.03 ! PT 1.02 SC 1.04 WF 1.00* ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.09 FD 1.03 KP 1.04 LA 1.06 ! MK 0.98 NL 1.02 OV 1.03 PT 1.03 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* HN 0.00* NY 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* HN 0.00* NL 0.00* NY 0.00* ! WZ 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! NY 0.00* WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.18 HN 0.99 LA 1.06 NL 1.13 ! SC 0.99 WF 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.92 HN 1.02 NL 1.13 SC 1.03 ! WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.13 FD 1.09 HN 1.03 KP 0.93 ! LA 1.00 NL 1.05 PT 1.06 SC 0.91 ! WF 1.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.00* MK 0.00* NY 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.04 FD 1.06 HN 1.00 KP 0.88 ! LA 0.97 MK 1.03 NL 1.06 OV 1.03 ! PT 1.07 SC 0.95 WF 1.00* ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.04 FD 1.03 KP 0.90 LA 0.97 ! MK 1.00 NL 1.09 OV 1.05 PT 1.05 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* HN 0.00* NY 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* HN 0.00* NL 0.00* NY 0.00* ! WZ 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! NY 0.00* WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 HN 0.92 LA 0.97 NL 1.04 ! SC 0.97 WF 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.11 HN 0.96 NL 0.99 SC 0.95 ! WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.03 FD 1.18 HN 0.92 KP 0.85 ! LA 0.81 NL 0.98 PT 0.97 SC 0.98 ! WF 1.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.00* MK 0.00* NY 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.03 FD 1.07 HN 0.90 KP 0.82 ! LA 0.81 MK 1.18 NL 0.99 OV 0.89 ! PT 0.93 SC 0.99 WF 1.00* ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.04 FD 0.98 KP 0.86 LA 0.82 ! MK 1.08 NL 1.02 OV 0.86 PT 0.90 ! ! ! Fit before self-cal, rms=0.088421Jy sigma=0.762603 ! Fit after self-cal, rms=0.052996Jy sigma=0.389317 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=4.874 mas, bmaj=5.22 mas, bpa=-26.13 degrees ! Estimated noise=2.38623 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 = -0.000721741 Jy ! Component: 100 - total flux cleaned = -0.00102541 Jy ! Component: 150 - total flux cleaned = -0.00119199 Jy ! Component: 200 - total flux cleaned = -0.00119539 Jy ! Total flux subtracted in 200 components = -0.00119539 Jy ! Clean residual min=-0.003403 max=0.004343 Jy/beam ! Clean residual mean=0.000031 rms=0.000970 Jy/beam ! Combined flux in latest and established models = 0.66635 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 69 components and 0.66635 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.052622Jy sigma=0.386256 ! Fit after self-cal, rms=0.052615Jy sigma=0.385754 ! 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=0.052615Jy sigma=0.385754 ! Fit after self-cal, rms=0.052683Jy sigma=0.385601 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=4.878 mas, bmaj=5.225 mas, bpa=-25.74 degrees ! Estimated noise=2.38682 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000775641 Jy ! Component: 100 - total flux cleaned = -0.000992694 Jy ! Component: 150 - total flux cleaned = -0.000994926 Jy ! Component: 200 - total flux cleaned = -0.00105018 Jy ! Total flux subtracted in 200 components = -0.00105018 Jy ! Clean residual min=-0.003325 max=0.004152 Jy/beam ! Clean residual mean=0.000031 rms=0.000948 Jy/beam ! Combined flux in latest and established models = 0.665299 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 73 components and 0.665299 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.052481Jy sigma=0.384175 ! Fit after self-cal, rms=0.052449Jy sigma=0.383985 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 (-102, 26.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00337439 Jy ! Component: 100 - total flux cleaned = 0.00377472 Jy ! Component: 150 - total flux cleaned = 0.00398229 Jy ! Component: 200 - total flux cleaned = 0.00423481 Jy ! Total flux subtracted in 200 components = 0.00423481 Jy ! Clean residual min=-0.003273 max=0.003665 Jy/beam ! Clean residual mean=0.000017 rms=0.000925 Jy/beam ! Combined flux in latest and established models = 0.669534 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 83 components and 0.669534 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.052090Jy sigma=0.381612 ! Fit after self-cal, rms=0.052075Jy sigma=0.381384 ! 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=0.052075Jy sigma=0.381384 ! Fit after self-cal, rms=0.051672Jy sigma=0.375860 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=4.865 mas, bmaj=5.234 mas, bpa=-26.53 degrees ! Estimated noise=2.38601 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000773474 Jy ! Component: 100 - total flux cleaned = 0.00110718 Jy ! Component: 150 - total flux cleaned = 0.00122445 Jy ! Component: 200 - total flux cleaned = 0.00122637 Jy ! Total flux subtracted in 200 components = 0.00122637 Jy ! Clean residual min=-0.003312 max=0.003680 Jy/beam ! Clean residual mean=0.000021 rms=0.000869 Jy/beam ! Combined flux in latest and established models = 0.67076 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 95 components and 0.67076 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.051510Jy sigma=0.374658 ! Fit after self-cal, rms=0.051505Jy sigma=0.374590 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 (12, 19.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00299032 Jy ! Component: 100 - total flux cleaned = 0.00383364 Jy ! Component: 150 - total flux cleaned = 0.00428695 Jy ! Component: 200 - total flux cleaned = 0.00441205 Jy ! Total flux subtracted in 200 components = 0.00441205 Jy ! Clean residual min=-0.003354 max=0.003180 Jy/beam ! Clean residual mean=0.000008 rms=0.000821 Jy/beam ! Combined flux in latest and established models = 0.675173 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 110 components and 0.675172 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.051210Jy sigma=0.371025 ! Fit after self-cal, rms=0.051190Jy sigma=0.370845 ! 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=0.051190Jy sigma=0.370845 ! Fit after self-cal, rms=0.051232Jy sigma=0.370638 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=9.306 mas, bmaj=9.552 mas, bpa=-49.93 degrees ! Estimated noise=2.66478 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00111057 Jy ! Component: 100 - total flux cleaned = 0.00131092 Jy ! Component: 150 - total flux cleaned = 0.00135221 Jy ! Component: 200 - total flux cleaned = 0.00131561 Jy ! Total flux subtracted in 200 components = 0.00131561 Jy ! Clean residual min=-0.003014 max=0.003968 Jy/beam ! Clean residual mean=0.000022 rms=0.000914 Jy/beam ! Combined flux in latest and established models = 0.676488 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 127 components and 0.676488 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.051202Jy sigma=0.369874 ! Fit after self-cal, rms=0.051199Jy sigma=0.369737 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 (28, -4.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00340137 Jy ! Component: 100 - total flux cleaned = 0.00476597 Jy ! Component: 150 - total flux cleaned = 0.00520841 Jy ! Component: 200 - total flux cleaned = 0.00539185 Jy ! Total flux subtracted in 200 components = 0.00539185 Jy ! Clean residual min=-0.002592 max=0.003071 Jy/beam ! Clean residual mean=-0.000007 rms=0.000831 Jy/beam ! Combined flux in latest and established models = 0.68188 Jy ! Performing phase self-cal ! Adding 43 model components to the UV plane model. ! The established model now contains 168 components and 0.68188 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.051054Jy sigma=0.367961 ! Fit after self-cal, rms=0.051046Jy sigma=0.367885 ! 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: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 "/scr/pima/rdv96_uvs/J0533+4822_S\_map.fits" ! Inverting map and beam ! Estimated beam: bmin=4.559 mas, bmaj=4.861 mas, bpa=-12.76 degrees ! Estimated noise=2.35479 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 4.559 x 4.861 at -12.76 degrees (North through East) ! Clean map min=-0.012381 max=0.53682 Jy/beam ! Writing clean map to FITS file: /scr/pima/rdv96_uvs/J0533+4822_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= 0.5368 rms= 0.00233 Jy quit ! Quitting program ! Log file /scr/pima/rdv96_uvs/J0533+4822_S_uvs.log closed on Sat Dec 21 00:22:36 2013