! Started logfile: /d2/scr/pima/rdv96_uvs/J0914+0245_X_uvs.log on Fri Dec 20 23:44:43 2013 obs /d2/scr/pima/rdv96_uvs/J0914+0245_X_uva.fits ! Reading UV FITS file: /d2/scr/pima/rdv96_uvs/J0914+0245_X_uva.fits ! AN table 1: 18 integrations on 3 of 3 possible baselines. ! AN table 2: 17 integrations on 6 of 6 possible baselines. ! AN table 3: 16 integrations on 3 of 3 possible baselines. ! AN table 4: 2 integrations on 3 of 3 possible baselines. ! AN table 5: 4 integrations on 28 of 28 possible baselines. ! AN table 6: 19 integrations on 91 of 91 possible baselines. ! AN table 7: 5 integrations on 45 of 45 possible baselines. ! AN table 8: 4 integrations on 15 of 15 possible baselines. ! AN table 9: 4 integrations on 28 of 28 possible baselines. ! AN table 10: 2 integrations on 10 of 10 possible baselines. ! Apparent sampling: 0.557942 visibilities/baseline/integration-bin. ! Found source: J0914+0245 ! ! 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 5508 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/J0914+0245_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:HH self-cal status=correctable weight=1 ! 1:NY self-cal status=correctable weight=1 ! 1:WZ self-cal status=correctable weight=1 ! 2:HH self-cal status=correctable weight=1 ! 2:MA self-cal status=correctable weight=1 ! 2:NY self-cal status=correctable weight=1 ! 2:WZ self-cal status=correctable weight=1 ! 3:HH self-cal status=correctable weight=1 ! 3:MA self-cal status=correctable weight=1 ! 3:WZ self-cal status=correctable weight=1 ! 4:HN self-cal status=correctable weight=1 ! 4:SC self-cal status=correctable weight=1 ! 4:WZ 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:PT self-cal status=correctable weight=1 ! 5:SC self-cal status=correctable weight=1 ! 5:WZ self-cal status=correctable weight=1 ! 6:BR self-cal status=correctable weight=1 ! 6:FD self-cal status=correctable weight=1 ! 6:HH 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:MA self-cal status=correctable weight=1 ! 6:NL self-cal status=correctable weight=1 ! 6:NY 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 ! 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:OV 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:HN self-cal status=correctable weight=1 ! 8:LA self-cal status=correctable weight=1 ! 8:NL self-cal status=correctable weight=1 ! 8:OV 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: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 ! 10:BR 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:OV 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 54 telescope corrections were flagged in sub-array 1. ! A total of 32 telescope corrections were flagged in sub-array 2. ! A total of 48 telescope corrections were flagged in sub-array 3. ! A total of 3 telescope corrections were flagged in sub-array 5. ! A total of 111 telescope corrections were flagged in sub-array 6. ! A total of 9 telescope corrections were flagged in sub-array 7. ! A total of 1 telescope corrections were flagged in sub-array 8. ! A total of 1 telescope corrections were flagged in sub-array 10. ! ! Correcting IF 2. ! A total of 54 telescope corrections were flagged in sub-array 1. ! A total of 32 telescope corrections were flagged in sub-array 2. ! A total of 48 telescope corrections were flagged in sub-array 3. ! A total of 3 telescope corrections were flagged in sub-array 5. ! A total of 111 telescope corrections were flagged in sub-array 6. ! A total of 9 telescope corrections were flagged in sub-array 7. ! A total of 1 telescope corrections were flagged in sub-array 8. ! A total of 1 telescope corrections were flagged in sub-array 10. ! ! Correcting IF 3. ! A total of 54 telescope corrections were flagged in sub-array 1. ! A total of 68 telescope corrections were flagged in sub-array 2. ! A total of 48 telescope corrections were flagged in sub-array 3. ! A total of 3 telescope corrections were flagged in sub-array 5. ! A total of 139 telescope corrections were flagged in sub-array 6. ! A total of 9 telescope corrections were flagged in sub-array 7. ! A total of 1 telescope corrections were flagged in sub-array 8. ! A total of 1 telescope corrections were flagged in sub-array 10. ! ! Correcting IF 4. ! A total of 54 telescope corrections were flagged in sub-array 1. ! A total of 68 telescope corrections were flagged in sub-array 2. ! A total of 48 telescope corrections were flagged in sub-array 3. ! A total of 3 telescope corrections were flagged in sub-array 5. ! A total of 139 telescope corrections were flagged in sub-array 6. ! A total of 9 telescope corrections were flagged in sub-array 7. ! A total of 1 telescope corrections were flagged in sub-array 8. ! A total of 1 telescope corrections were flagged in sub-array 10. ! ! Fit before self-cal, rms=1.091844Jy sigma=6.874961 ! Fit after self-cal, rms=0.605280Jy sigma=3.190459 ! 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:HH ! Flagging baselines of antenna 1:HH in the currently selected channels. flag 1:NY ! Flagging baselines of antenna 1:NY in the currently selected channels. flag 1:WZ ! Flagging baselines of antenna 1:WZ in the currently selected channels. flag 2:HH ! Flagging baselines of antenna 2:HH in the currently selected channels. flag 2:MA ! Flagging baselines of antenna 2:MA 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:HH ! Flagging baselines of antenna 3:HH in the currently selected channels. flag 3:MA ! Flagging baselines of antenna 3:MA in the currently selected channels. flag 3:WZ ! Flagging baselines of antenna 3:WZ in the currently selected channels. flag 4:WZ ! Flagging baselines of antenna 4:WZ in the currently selected channels. flag 5:WZ ! Flagging baselines of antenna 5:WZ in the currently selected channels. flag 6:HH ! Flagging baselines of antenna 6:HH in the currently selected channels. flag 6:MA ! Flagging baselines of antenna 6:MA in the currently selected channels. flag 6:NY ! Flagging baselines of antenna 6:NY 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:WF ! Flagging baselines of antenna 8: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=1.174 mas, bmaj=2.08 mas, bpa=0.5627 degrees ! Estimated noise=2.92457 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 = 0.355466 Jy ! Component: 100 - total flux cleaned = 0.451795 Jy ! Total flux subtracted in 100 components = 0.451795 Jy ! Clean residual min=-0.015109 max=0.042013 Jy/beam ! Clean residual mean=-0.000088 rms=0.003772 Jy/beam ! Combined flux in latest and established models = 0.451795 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 14 components and 0.451795 Jy ! ! Correcting IF 1. ! A total of 36 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 4 telescope corrections were flagged in sub-array 5. ! A total of 69 telescope corrections were flagged in sub-array 6. ! A total of 4 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 2. ! A total of 36 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 4 telescope corrections were flagged in sub-array 5. ! A total of 69 telescope corrections were flagged in sub-array 6. ! A total of 4 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 4 telescope corrections were flagged in sub-array 5. ! A total of 41 telescope corrections were flagged in sub-array 6. ! A total of 4 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 4. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 4 telescope corrections were flagged in sub-array 5. ! A total of 41 telescope corrections were flagged in sub-array 6. ! A total of 4 telescope corrections were flagged in sub-array 8. ! ! Fit before self-cal, rms=0.102511Jy sigma=0.847013 ! Fit after self-cal, rms=0.102552Jy sigma=0.847477 ! Inverting map and beam ! Estimated beam: bmin=1.172 mas, bmaj=2.091 mas, bpa=0.6865 degrees ! Estimated noise=2.92778 mJy/beam. ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0460044 Jy ! Component: 100 - total flux cleaned = 0.0691394 Jy ! Total flux subtracted in 100 components = 0.0691394 Jy ! Clean residual min=-0.010403 max=0.011091 Jy/beam ! Clean residual mean=-0.000049 rms=0.002300 Jy/beam ! Combined flux in latest and established models = 0.520934 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 21 components and 0.520934 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.073951Jy sigma=0.573101 ! Fit after self-cal, rms=0.073767Jy sigma=0.572175 ! 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=1.52 mas, bmaj=2.598 mas, bpa=4.827 degrees ! Estimated noise=1.77895 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 = 0.0248697 Jy ! Component: 100 - total flux cleaned = 0.0366392 Jy ! Component: 150 - total flux cleaned = 0.0431036 Jy ! Component: 200 - total flux cleaned = 0.0467738 Jy ! Total flux subtracted in 200 components = 0.0467738 Jy ! Clean residual min=-0.009471 max=0.009132 Jy/beam ! Clean residual mean=-0.000028 rms=0.002378 Jy/beam ! Combined flux in latest and established models = 0.567708 Jy ! Performing phase self-cal ! Adding 34 model components to the UV plane model. ! The established model now contains 46 components and 0.567708 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.067481Jy sigma=0.497348 ! Fit after self-cal, rms=0.067392Jy sigma=0.497036 ! 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: ! HH 0.00* NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! HH 0.00* MA 0.00* NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! HH 0.00* MA 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! HN 0.00* SC 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.02 HN 1.03 KP 1.03 LA 1.06 ! NL 1.01 PT 0.99 SC 1.03 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.98 FD 0.98 HH 1.00* HN 0.98 ! KP 0.99 LA 1.03 MA 1.00* NL 0.94 ! NY 1.00* OV 0.99 PT 0.97 SC 0.98 ! WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 0.96 FD 1.00 HN 1.03 KP 1.00 ! LA 1.04 NL 0.97 OV 1.00 PT 0.98 ! SC 1.04 WF 1.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.94 HN 1.03 LA 1.01 NL 1.00 ! OV 0.96 WF 1.00* ! ! Telescope amplitude corrections in sub-array 9: ! BR 0.97 FD 1.01 KP 1.03 LA 1.06 ! MK 0.99 NL 1.02 OV 0.99 PT 1.01 ! ! Telescope amplitude corrections in sub-array 10: ! BR 0.92 KP 1.52 LA 1.18 MK 0.98 ! OV 1.09 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! HH 0.00* NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! HH 0.00* MA 0.00* NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! HH 0.00* MA 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! HN 0.00* SC 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.00 HN 1.01 KP 0.95 LA 1.02 ! NL 1.01 PT 0.99 SC 1.01 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.99 FD 0.98 HH 1.00* HN 1.00 ! KP 0.93 LA 1.01 MA 1.00* NL 0.96 ! NY 1.00* OV 0.95 PT 0.97 SC 1.03 ! WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 0.97 FD 0.99 HN 1.01 KP 0.94 ! LA 1.01 NL 0.98 OV 0.97 PT 1.02 ! SC 1.05 WF 1.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.96 HN 1.03 LA 0.99 NL 0.97 ! OV 0.98 WF 1.00* ! ! Telescope amplitude corrections in sub-array 9: ! BR 0.96 FD 1.03 KP 0.96 LA 1.02 ! MK 1.01 NL 1.03 OV 1.00 PT 1.03 ! ! Telescope amplitude corrections in sub-array 10: ! BR 0.94 KP 1.42 LA 1.14 MK 0.96 ! OV 1.05 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! HH 0.00* NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! HH 0.00* MA 0.00* NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! HH 0.00* MA 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! HN 0.00* SC 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.04 HN 1.12 KP 0.83 LA 1.08 ! NL 1.05 PT 0.99 SC 1.06 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.05 FD 0.97 HH 1.00* HN 1.02 ! KP 0.83 LA 1.10 MA 1.00* NL 0.98 ! NY 1.00* OV 1.04 PT 0.99 SC 0.98 ! WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.04 FD 0.96 HN 1.08 KP 0.85 ! LA 1.09 NL 1.00 OV 1.06 PT 0.97 ! SC 1.02 WF 1.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.02 HN 1.10 LA 1.02 NL 1.00 ! OV 0.99 WF 1.00* ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.02 FD 0.99 KP 0.87 LA 1.09 ! MK 0.98 NL 1.09 OV 1.06 PT 1.02 ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.08 KP 1.34 LA 1.18 MK 0.95 ! OV 1.13 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! HH 0.00* NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! HH 0.00* MA 0.00* NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! HH 0.00* MA 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! HN 0.00* SC 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.05 HN 1.07 KP 0.90 LA 1.05 ! NL 1.11 PT 1.04 SC 1.06 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.04 FD 1.03 HH 1.00* HN 1.00 ! KP 0.87 LA 1.09 MA 1.00* NL 1.02 ! NY 1.00* OV 1.00 PT 1.05 SC 1.01 ! WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.01 FD 1.05 HN 1.06 KP 0.89 ! LA 1.07 NL 1.08 OV 0.99 PT 1.05 ! SC 1.09 WF 1.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.98 HN 1.05 LA 1.01 NL 1.05 ! OV 0.99 WF 1.00* ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.00 FD 1.05 KP 0.93 LA 1.08 ! MK 1.02 NL 1.10 OV 1.03 PT 1.04 ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.04 KP 1.28 LA 1.08 MK 1.12 ! OV 1.19 ! ! ! Fit before self-cal, rms=0.067392Jy sigma=0.497036 ! Fit after self-cal, rms=0.054835Jy sigma=0.383484 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=1.525 mas, bmaj=2.61 mas, bpa=4.585 degrees ! Estimated noise=1.77873 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 (1.8, 8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00514234 Jy ! Component: 100 - total flux cleaned = 0.00815803 Jy ! Component: 150 - total flux cleaned = 0.00987183 Jy ! Component: 200 - total flux cleaned = 0.010531 Jy ! Total flux subtracted in 200 components = 0.010531 Jy ! Clean residual min=-0.002553 max=0.003060 Jy/beam ! Clean residual mean=-0.000002 rms=0.000675 Jy/beam ! Combined flux in latest and established models = 0.578239 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 62 components and 0.578239 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.054256Jy sigma=0.378875 ! Fit after self-cal, rms=0.054227Jy sigma=0.378520 ! 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=0.054227Jy sigma=0.378520 ! Fit after self-cal, rms=0.054162Jy sigma=0.378343 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=1.525 mas, bmaj=2.61 mas, bpa=4.536 degrees ! Estimated noise=1.77709 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00114655 Jy ! Component: 100 - total flux cleaned = 0.0014739 Jy ! Component: 150 - total flux cleaned = 0.00169544 Jy ! Component: 200 - total flux cleaned = 0.00184416 Jy ! Total flux subtracted in 200 components = 0.00184416 Jy ! Clean residual min=-0.002486 max=0.002842 Jy/beam ! Clean residual mean=-0.000001 rms=0.000641 Jy/beam ! Combined flux in latest and established models = 0.580083 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 71 components and 0.580084 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.054000Jy sigma=0.377444 ! Fit after self-cal, rms=0.053980Jy sigma=0.377388 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 (10, 35.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00169031 Jy ! Component: 100 - total flux cleaned = 0.00205964 Jy ! Component: 150 - total flux cleaned = 0.00215725 Jy ! Component: 200 - total flux cleaned = 0.00215762 Jy ! Total flux subtracted in 200 components = 0.00215762 Jy ! Clean residual min=-0.002328 max=0.002568 Jy/beam ! Clean residual mean=-0.000001 rms=0.000616 Jy/beam ! Combined flux in latest and established models = 0.582241 Jy ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 95 components and 0.582241 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.053809Jy sigma=0.376347 ! Fit after self-cal, rms=0.053800Jy sigma=0.376281 ! 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=0.053800Jy sigma=0.376281 ! Fit after self-cal, rms=0.053013Jy sigma=0.371607 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=1.523 mas, bmaj=2.609 mas, bpa=4.463 degrees ! Estimated noise=1.77614 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000551754 Jy ! Component: 100 - total flux cleaned = 0.000598851 Jy ! Component: 150 - total flux cleaned = 0.000599211 Jy ! Component: 200 - total flux cleaned = 0.000682647 Jy ! Total flux subtracted in 200 components = 0.000682647 Jy ! Clean residual min=-0.002167 max=0.002494 Jy/beam ! Clean residual mean=0.000001 rms=0.000548 Jy/beam ! Combined flux in latest and established models = 0.582924 Jy selfcal ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 113 components and 0.582924 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.052924Jy sigma=0.371097 ! Fit after self-cal, rms=0.052924Jy sigma=0.371081 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 (49.4, -32.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00157797 Jy ! Component: 100 - total flux cleaned = 0.00182226 Jy ! Component: 150 - total flux cleaned = 0.00199219 Jy ! Component: 200 - total flux cleaned = 0.00211041 Jy ! Total flux subtracted in 200 components = 0.00211041 Jy ! Clean residual min=-0.002080 max=0.002344 Jy/beam ! Clean residual mean=0.000002 rms=0.000533 Jy/beam ! Combined flux in latest and established models = 0.585034 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 128 components and 0.585034 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.052788Jy sigma=0.370348 ! Fit after self-cal, rms=0.052783Jy sigma=0.370296 ! Inverting map ! Added new window around map position (-5.4, 31.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00146089 Jy ! Component: 100 - total flux cleaned = 0.0016942 Jy ! Component: 150 - total flux cleaned = 0.00202558 Jy ! Component: 200 - total flux cleaned = 0.0021787 Jy ! Total flux subtracted in 200 components = 0.0021787 Jy ! Clean residual min=-0.002124 max=0.002210 Jy/beam ! Clean residual mean=0.000001 rms=0.000517 Jy/beam ! Combined flux in latest and established models = 0.587213 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 141 components and 0.587213 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.052663Jy sigma=0.369658 ! Fit after self-cal, rms=0.052659Jy sigma=0.369640 ! Inverting map ! Added new window around map position (-32.6, -16.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00140369 Jy ! Component: 100 - total flux cleaned = 0.00140716 Jy ! Component: 150 - total flux cleaned = 0.00136183 Jy ! Component: 200 - total flux cleaned = 0.00131912 Jy ! Total flux subtracted in 200 components = 0.00131912 Jy ! Clean residual min=-0.002046 max=0.002072 Jy/beam ! Clean residual mean=0.000002 rms=0.000498 Jy/beam ! Combined flux in latest and established models = 0.588532 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 162 components and 0.588532 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.052526Jy sigma=0.368933 ! Fit after self-cal, rms=0.052521Jy sigma=0.368895 ! 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=0.052521Jy sigma=0.368895 ! Fit after self-cal, rms=0.052481Jy sigma=0.368756 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=2.565 mas, bmaj=3.739 mas, bpa=-10.71 degrees ! Estimated noise=1.85904 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00104096 Jy ! Component: 100 - total flux cleaned = 0.00118035 Jy ! Component: 150 - total flux cleaned = 0.00124018 Jy ! Component: 200 - total flux cleaned = 0.00129613 Jy ! Total flux subtracted in 200 components = 0.00129613 Jy ! Clean residual min=-0.001628 max=0.001597 Jy/beam ! Clean residual mean=0.000002 rms=0.000473 Jy/beam ! Combined flux in latest and established models = 0.589828 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 182 components and 0.589828 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.052454Jy sigma=0.368534 ! Fit after self-cal, rms=0.052449Jy sigma=0.368512 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 = 0.000176011 Jy ! Component: 100 - total flux cleaned = 0.000329523 Jy ! Component: 150 - total flux cleaned = 0.000377594 Jy ! Component: 200 - total flux cleaned = 0.000401543 Jy ! Total flux subtracted in 200 components = 0.000401543 Jy ! Clean residual min=-0.001613 max=0.001621 Jy/beam ! Clean residual mean=0.000002 rms=0.000466 Jy/beam ! Combined flux in latest and established models = 0.59023 Jy ! Performing phase self-cal ! Adding 34 model components to the UV plane model. ! The established model now contains 198 components and 0.59023 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.052431Jy sigma=0.368380 ! Fit after self-cal, rms=0.052427Jy sigma=0.368371 ! 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:HH ! Syntax error in line: ! 1:HH ! ^ ! 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/J0914+0245_X\_map.fits" ! Inverting map and beam ! Your choice of large map pixels excluded 3.64% of the data. ! The x-axis pixel size should ideally be below 0.1873 milli-arcsec ! The y-axis pixel size should ideally be below 0.1979 milli-arcsec ! Estimated beam: bmin=0.9494 mas, bmaj=2.29 mas, bpa=-4.701 degrees ! Estimated noise=1.87145 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9494 x 2.29 at -4.701 degrees (North through East) ! Clean map min=-0.0080136 max=0.45281 Jy/beam ! Writing clean map to FITS file: /d2/scr/pima/rdv96_uvs/J0914+0245_X_map.fits float peak_flux peak_flux = peak(flux,max) invert ! Inverting map ! Your choice of large map pixels excluded 3.64% of the data. ! The x-axis pixel size should ideally be below 0.1873 milli-arcsec ! The y-axis pixel size should ideally be below 0.1979 milli-arcsec 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= 0.4528 rms= 0.00209 Jy quit ! Quitting program ! Log file /d2/scr/pima/rdv96_uvs/J0914+0245_X_uvs.log closed on Fri Dec 20 23:44:46 2013