! Started logfile: /scr/pima/rdv95_uvs/J0958+6533_X_uvs.log on Wed Nov 6 20:45:46 2013 obs /scr/pima/rdv95_uvs/J0958+6533_X_uva.fits ! Reading UV FITS file: /scr/pima/rdv95_uvs/J0958+6533_X_uva.fits ! AN table 1: 18 integrations on 78 of 78 possible baselines. ! AN table 2: 2 integrations on 36 of 36 possible baselines. ! AN table 3: 2 integrations on 45 of 45 possible baselines. ! AN table 4: 2 integrations on 3 of 3 possible baselines. ! AN table 5: 6 integrations on 15 of 15 possible baselines. ! Apparent sampling: 0.989771 visibilities/baseline/integration-bin. ! Found source: J0958+6533 ! ! 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 6580 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 /scr/pima/rdv95_uvs/J0958+6533_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:MA self-cal status=correctable weight=1 ! 1:MK self-cal status=correctable weight=1 ! 1:NL self-cal status=correctable weight=1 ! 1:NY self-cal status=correctable weight=1 ! 1:OV self-cal status=correctable weight=1 ! 1:PT self-cal status=correctable weight=1 ! 1:SC self-cal status=correctable weight=1 ! 1:WZ self-cal status=correctable weight=1 ! 2:BR self-cal status=correctable weight=1 ! 2:FD self-cal status=correctable weight=1 ! 2:HN self-cal status=correctable weight=1 ! 2:KP self-cal status=correctable weight=1 ! 2:LA self-cal status=correctable weight=1 ! 2:NL self-cal status=correctable weight=1 ! 2:NY self-cal status=correctable weight=1 ! 2:OV self-cal status=correctable weight=1 ! 2:PT 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:MA self-cal status=correctable weight=1 ! 3:NL self-cal status=correctable weight=1 ! 3:NY 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:MA self-cal status=correctable weight=1 ! 4:NY self-cal status=correctable weight=1 ! 4:WZ self-cal status=correctable weight=1 ! 5:BR self-cal status=correctable weight=1 ! 5:FT self-cal status=correctable weight=1 ! 5:MA self-cal status=correctable weight=1 ! 5:MK self-cal status=correctable weight=1 ! 5:NY self-cal status=correctable weight=1 ! 5:WZ 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 12 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 12 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 18 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 2 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 17 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 18 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 2 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 17 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=1.186619Jy sigma=11.128424 ! Fit after self-cal, rms=0.423669Jy sigma=2.801057 ! 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:MA ! Flagging baselines of antenna 1:MA 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:NY ! Flagging baselines of antenna 2:NY in the currently selected channels. flag 3:MA ! Flagging baselines of antenna 3:MA in the currently selected channels. flag 3:NY ! Flagging baselines of antenna 3:NY in the currently selected channels. flag 3:WZ ! Flagging baselines of antenna 3:WZ in the currently selected channels. flag 4:MA ! Flagging baselines of antenna 4:MA in the currently selected channels. flag 4:NY ! Flagging baselines of antenna 4:NY in the currently selected channels. flag 4:WZ ! Flagging baselines of antenna 4:WZ in the currently selected channels. flag 5:FT ! Flagging baselines of antenna 5:FT in the currently selected channels. flag 5:MA ! Flagging baselines of antenna 5:MA in the currently selected channels. flag 5:NY ! Flagging baselines of antenna 5:NY in the currently selected channels. flag 5:WZ ! Flagging baselines of antenna 5:WZ 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=0.7197 mas, bmaj=2.233 mas, bpa=-24.74 degrees ! Estimated noise=1.97836 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 = 0.553312 Jy ! Component: 100 - total flux cleaned = 0.682469 Jy ! Total flux subtracted in 100 components = 0.682469 Jy ! Clean residual min=-0.016973 max=0.043289 Jy/beam ! Clean residual mean=-0.000008 rms=0.005080 Jy/beam ! Combined flux in latest and established models = 0.682469 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 8 components and 0.682469 Jy ! ! Correcting IF 1. ! A total of 54 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 24 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 54 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 24 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 36 telescope corrections were flagged in sub-array 1. ! A total of 4 telescope corrections were flagged in sub-array 3. ! A total of 19 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 36 telescope corrections were flagged in sub-array 1. ! A total of 4 telescope corrections were flagged in sub-array 3. ! A total of 19 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=0.113188Jy sigma=1.335968 ! Fit after self-cal, rms=0.113259Jy sigma=1.337320 ! Inverting map and beam ! Estimated beam: bmin=0.7197 mas, bmaj=2.228 mas, bpa=-24.88 degrees ! Estimated noise=1.98959 mJy/beam. ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0442649 Jy ! Component: 100 - total flux cleaned = 0.0665464 Jy ! Total flux subtracted in 100 components = 0.0665464 Jy ! Clean residual min=-0.016818 max=0.019399 Jy/beam ! Clean residual mean=-0.000001 rms=0.003515 Jy/beam ! Combined flux in latest and established models = 0.749016 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 13 components and 0.749016 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.089376Jy sigma=0.971245 ! Fit after self-cal, rms=0.089110Jy sigma=0.969733 ! 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=0.8731 mas, bmaj=2.675 mas, bpa=-25.65 degrees ! Estimated noise=1.13579 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 = 0.0319026 Jy ! Component: 100 - total flux cleaned = 0.048631 Jy ! Component: 150 - total flux cleaned = 0.0593677 Jy ! Component: 200 - total flux cleaned = 0.0647446 Jy ! Total flux subtracted in 200 components = 0.0647446 Jy ! Clean residual min=-0.016018 max=0.014664 Jy/beam ! Clean residual mean=-0.000015 rms=0.003608 Jy/beam ! Combined flux in latest and established models = 0.81376 Jy ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 38 components and 0.81376 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081250Jy sigma=0.799078 ! Fit after self-cal, rms=0.081148Jy sigma=0.798430 ! 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 0.98 FD 1.01 HN 1.04 KP 0.99 ! LA 1.02 MA 1.00* MK 0.99 NL 0.95 ! NY 1.00* OV 1.00 PT 0.97 SC 1.00 ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 1.08 HN 1.08 KP 1.11 ! LA 1.12 NL 1.05 NY 1.00* OV 1.07 ! PT 1.06 ! ! Telescope amplitude corrections in sub-array 3: ! FD 1.03 HN 1.10 KP 1.07 LA 1.07 ! MA 1.00* NL 1.06 NY 1.00* PT 1.00 ! SC 1.01 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! MA 0.00* NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* FT 0.00* MA 0.00* MK 0.00* ! NY 0.00* WZ 0.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 1.01 HN 1.10 KP 0.95 ! LA 0.98 MA 1.00* MK 1.00 NL 0.96 ! NY 1.00* OV 0.98 PT 0.97 SC 1.02 ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 FD 1.09 HN 1.16 KP 1.04 ! LA 1.07 NL 1.03 NY 1.00* OV 1.04 ! PT 1.08 ! ! Telescope amplitude corrections in sub-array 3: ! FD 1.00 HN 1.28 KP 1.00 LA 1.04 ! MA 1.00* NL 1.05 NY 1.00* PT 1.05 ! SC 1.05 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! MA 0.00* NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* FT 0.00* MA 0.00* MK 0.00* ! NY 0.00* WZ 0.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 FD 1.00 HN 1.12 KP 0.85 ! LA 1.04 MA 1.00* MK 0.99 NL 0.98 ! NY 1.00* OV 1.03 PT 0.97 SC 1.00 ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.08 FD 1.07 HN 1.15 KP 0.96 ! LA 1.14 NL 1.05 NY 1.00* OV 1.12 ! PT 1.06 ! ! Telescope amplitude corrections in sub-array 3: ! FD 1.01 HN 1.20 KP 0.92 LA 1.08 ! MA 1.00* NL 1.09 NY 1.00* PT 1.01 ! SC 1.02 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! MA 0.00* NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* FT 0.00* MA 0.00* MK 0.00* ! NY 0.00* WZ 0.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 1.05 HN 1.14 KP 0.89 ! LA 1.02 MA 1.00* MK 1.02 NL 1.01 ! NY 1.00* OV 1.01 PT 1.00 SC 1.01 ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.07 FD 1.10 HN 1.17 KP 0.98 ! LA 1.15 NL 1.12 NY 1.00* OV 1.07 ! PT 1.10 ! ! Telescope amplitude corrections in sub-array 3: ! FD 1.08 HN 1.12 KP 0.96 LA 1.06 ! MA 1.00* NL 1.08 NY 1.00* PT 1.06 ! SC 1.07 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! MA 0.00* NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* FT 0.00* MA 0.00* MK 0.00* ! NY 0.00* WZ 0.00* ! ! ! Fit before self-cal, rms=0.081148Jy sigma=0.798430 ! Fit after self-cal, rms=0.059979Jy sigma=0.536803 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.876 mas, bmaj=2.709 mas, bpa=-25.51 degrees ! Estimated noise=1.13593 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 (-2, 2.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00522189 Jy ! Component: 100 - total flux cleaned = 0.00659836 Jy ! Component: 150 - total flux cleaned = 0.00724684 Jy ! Component: 200 - total flux cleaned = 0.00750955 Jy ! Total flux subtracted in 200 components = 0.00750955 Jy ! Clean residual min=-0.004036 max=0.003218 Jy/beam ! Clean residual mean=-0.000001 rms=0.000752 Jy/beam ! Combined flux in latest and established models = 0.82127 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 58 components and 0.82127 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.059386Jy sigma=0.529519 ! Fit after self-cal, rms=0.059366Jy sigma=0.529094 ! 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=0.059366Jy sigma=0.529094 ! Fit after self-cal, rms=0.059274Jy sigma=0.528596 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=0.8758 mas, bmaj=2.709 mas, bpa=-25.5 degrees ! Estimated noise=1.13505 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00175079 Jy ! Component: 100 - total flux cleaned = 0.00238617 Jy ! Component: 150 - total flux cleaned = 0.00277649 Jy ! Component: 200 - total flux cleaned = 0.00277596 Jy ! Total flux subtracted in 200 components = 0.00277596 Jy ! Clean residual min=-0.003539 max=0.002948 Jy/beam ! Clean residual mean=0.000000 rms=0.000669 Jy/beam ! Combined flux in latest and established models = 0.824046 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 67 components and 0.824046 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.059066Jy sigma=0.526359 ! Fit after self-cal, rms=0.059014Jy sigma=0.526150 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 = 0.000305794 Jy ! Component: 100 - total flux cleaned = 0.000463045 Jy ! Component: 150 - total flux cleaned = 0.000512634 Jy ! Component: 200 - total flux cleaned = 0.000470097 Jy ! Total flux subtracted in 200 components = 0.000470097 Jy ! Clean residual min=-0.003429 max=0.002816 Jy/beam ! Clean residual mean=0.000000 rms=0.000643 Jy/beam ! Combined flux in latest and established models = 0.824516 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 75 components and 0.824516 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.058920Jy sigma=0.525232 ! Fit after self-cal, rms=0.058894Jy sigma=0.525148 ! 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=0.058894Jy sigma=0.525148 ! Fit after self-cal, rms=0.058881Jy sigma=0.524815 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=0.8755 mas, bmaj=2.709 mas, bpa=-25.49 degrees ! Estimated noise=1.13456 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000712156 Jy ! Component: 100 - total flux cleaned = 0.00119165 Jy ! Component: 150 - total flux cleaned = 0.00119427 Jy ! Component: 200 - total flux cleaned = 0.00111883 Jy ! Total flux subtracted in 200 components = 0.00111883 Jy ! Clean residual min=-0.003037 max=0.002748 Jy/beam ! Clean residual mean=0.000001 rms=0.000605 Jy/beam ! Combined flux in latest and established models = 0.825634 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 85 components and 0.825634 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.058788Jy sigma=0.524020 ! Fit after self-cal, rms=0.058765Jy sigma=0.523949 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 = 0.000103948 Jy ! Component: 100 - total flux cleaned = 0.000176771 Jy ! Component: 150 - total flux cleaned = 0.000143271 Jy ! Component: 200 - total flux cleaned = 8.11366e-05 Jy ! Total flux subtracted in 200 components = 8.11366e-05 Jy ! Clean residual min=-0.002965 max=0.002662 Jy/beam ! Clean residual mean=0.000001 rms=0.000594 Jy/beam ! Combined flux in latest and established models = 0.825716 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 92 components and 0.825716 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.058713Jy sigma=0.523555 ! Fit after self-cal, rms=0.058699Jy sigma=0.523515 ! 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=0.058699Jy sigma=0.523515 ! Fit after self-cal, rms=0.058694Jy sigma=0.523356 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=2.232 mas, bmaj=3.182 mas, bpa=-27.29 degrees ! Estimated noise=1.32103 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000674529 Jy ! Component: 100 - total flux cleaned = -0.000734769 Jy ! Component: 150 - total flux cleaned = -0.000854075 Jy ! Component: 200 - total flux cleaned = -0.000933673 Jy ! Total flux subtracted in 200 components = -0.000933673 Jy ! Clean residual min=-0.002298 max=0.002531 Jy/beam ! Clean residual mean=0.000001 rms=0.000657 Jy/beam ! Combined flux in latest and established models = 0.824782 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 105 components and 0.824782 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.058695Jy sigma=0.523149 ! Fit after self-cal, rms=0.058673Jy sigma=0.522977 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 = -7.86628e-05 Jy ! Component: 100 - total flux cleaned = -0.000107731 Jy ! Component: 150 - total flux cleaned = -0.000152862 Jy ! Component: 200 - total flux cleaned = -0.000173431 Jy ! Total flux subtracted in 200 components = -0.000173431 Jy ! Clean residual min=-0.002263 max=0.002509 Jy/beam ! Clean residual mean=0.000001 rms=0.000643 Jy/beam ! Combined flux in latest and established models = 0.824609 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 115 components and 0.824608 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.058671Jy sigma=0.522959 ! Fit after self-cal, rms=0.058659Jy sigma=0.522865 ! 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] selfant 1:BR,true ! 1:BR self-cal status=fixed weight=1 selfant 1:FD,true ! 1:FD self-cal status=fixed weight=1 selfant 1:HN,true ! 1:HN self-cal status=fixed weight=1 selfant 1:KP,true ! 1:KP self-cal status=fixed weight=1 selfant 1:LA,true ! 1:LA self-cal status=fixed weight=1 selfant 1:MK,true ! 1:MK self-cal status=fixed weight=1 selfant 1:NL,true ! 1:NL self-cal status=fixed weight=1 selfant 1:OV,true ! 1:OV self-cal status=fixed weight=1 selfant 1:PT,true ! 1:PT self-cal status=fixed weight=1 selfant 1:SC,true ! 1:SC self-cal status=fixed weight=1 selfant 2:BR,true ! 2:BR self-cal status=fixed weight=1 selfant 2:FD,true ! 2:FD self-cal status=fixed weight=1 selfant 2:HN,true ! 2:HN self-cal status=fixed weight=1 selfant 2:KP,true ! 2:KP self-cal status=fixed weight=1 selfant 2:LA,true ! 2:LA self-cal status=fixed weight=1 selfant 2:NL,true ! 2:NL self-cal status=fixed weight=1 selfant 2:OV,true ! 2:OV self-cal status=fixed weight=1 selfant 2:PT,true ! 2:PT self-cal status=fixed weight=1 selfant 3:FD,true ! 3:FD self-cal status=fixed weight=1 selfant 3:HN,true ! 3:HN self-cal status=fixed weight=1 selfant 3:KP,true ! 3:KP self-cal status=fixed weight=1 selfant 3:LA,true ! 3:LA self-cal status=fixed weight=1 selfant 3:NL,true ! 3:NL self-cal status=fixed weight=1 selfant 3:PT,true ! 3:PT self-cal status=fixed weight=1 selfant 3:SC,true ! 3:SC self-cal status=fixed weight=1 selfant 5:BR,true ! 5:BR self-cal status=fixed weight=1 selfant 5:MK,true ! 5:MK self-cal status=fixed weight=1 ![Exited script file: /tmp/ff.ff] selfcal true, true, soltime1 ! Performing amp+phase self-cal over 800000 minute time intervals ! ! Correcting IF 1. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 9 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 9 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 18 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 2 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 16 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 18 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 2 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 16 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=0.106634Jy sigma=0.637035 ! Fit after self-cal, rms=0.090498Jy sigma=0.517756 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:MA self-cal status=correctable weight=1 ! 1:MK self-cal status=correctable weight=1 ! 1:NL self-cal status=correctable weight=1 ! 1:NY self-cal status=correctable weight=1 ! 1:OV self-cal status=correctable weight=1 ! 1:PT self-cal status=correctable weight=1 ! 1:SC self-cal status=correctable weight=1 ! 1:WZ self-cal status=correctable weight=1 ! 2:BR self-cal status=correctable weight=1 ! 2:FD self-cal status=correctable weight=1 ! 2:HN self-cal status=correctable weight=1 ! 2:KP self-cal status=correctable weight=1 ! 2:LA self-cal status=correctable weight=1 ! 2:NL self-cal status=correctable weight=1 ! 2:NY self-cal status=correctable weight=1 ! 2:OV self-cal status=correctable weight=1 ! 2:PT 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:MA self-cal status=correctable weight=1 ! 3:NL self-cal status=correctable weight=1 ! 3:NY 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:MA self-cal status=correctable weight=1 ! 4:NY self-cal status=correctable weight=1 ! 4:WZ self-cal status=correctable weight=1 ! 5:BR self-cal status=correctable weight=1 ! 5:FT self-cal status=correctable weight=1 ! 5:MA self-cal status=correctable weight=1 ! 5:MK self-cal status=correctable weight=1 ! 5:NY self-cal status=correctable weight=1 ! 5:WZ self-cal status=correctable weight=1 selfcal true, true, soltime1 ! Performing amp+phase self-cal over 800000 minute time intervals ! ! Correcting IF 1. ! A total of 3 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 3 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 4 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 4 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=0.090498Jy sigma=0.517756 ! Fit after self-cal, rms=0.089666Jy sigma=0.513823 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 ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! Estimated beam: bmin=0.6136 mas, bmaj=0.7573 mas, bpa=-51.67 degrees ! Estimated noise=2.17433 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 = 0.00405941 Jy ! Component: 100 - total flux cleaned = 0.00340277 Jy ! Component: 150 - total flux cleaned = 0.00390632 Jy ! Component: 200 - total flux cleaned = 0.00434888 Jy ! Total flux subtracted in 200 components = 0.00434888 Jy ! Clean residual min=-0.006700 max=0.008345 Jy/beam ! Clean residual mean=-0.000000 rms=0.001253 Jy/beam ! Combined flux in latest and established models = 0.828957 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 125 components and 0.828957 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081077Jy sigma=0.490172 ! Fit after self-cal, rms=0.080560Jy sigma=0.488093 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000819046 Jy ! Component: 100 - total flux cleaned = 0.00115291 Jy ! Component: 150 - total flux cleaned = 0.00175969 Jy ! Component: 200 - total flux cleaned = 0.00230143 Jy ! Total flux subtracted in 200 components = 0.00230143 Jy ! Clean residual min=-0.005726 max=0.007013 Jy/beam ! Clean residual mean=-0.000000 rms=0.001139 Jy/beam ! Combined flux in latest and established models = 0.831259 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 129 components and 0.831259 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.078328Jy sigma=0.482772 ! Fit after self-cal, rms=0.077999Jy sigma=0.481330 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! Added new window around map position (-0.6, -2.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00191922 Jy ! Component: 100 - total flux cleaned = 0.00214182 Jy ! Component: 150 - total flux cleaned = 0.00235526 Jy ! Component: 200 - total flux cleaned = 0.00235701 Jy ! Total flux subtracted in 200 components = 0.00235701 Jy ! Clean residual min=-0.004863 max=0.004857 Jy/beam ! Clean residual mean=-0.000000 rms=0.001061 Jy/beam ! Combined flux in latest and established models = 0.833616 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 138 components and 0.833616 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.076861Jy sigma=0.478531 ! Fit after self-cal, rms=0.076637Jy sigma=0.477395 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec 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 ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! Estimated beam: bmin=0.7645 mas, bmaj=1.021 mas, bpa=-60.41 degrees ! Estimated noise=1.14586 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 (29.4, 12.6). ! clean: niter=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00425913 Jy ! Component: 100 - total flux cleaned = 0.00633626 Jy ! Component: 150 - total flux cleaned = 0.0073167 Jy ! Component: 200 - total flux cleaned = 0.0080069 Jy ! Component: 250 - total flux cleaned = 0.00818935 Jy ! Component: 300 - total flux cleaned = 0.00845402 Jy ! Component: 350 - total flux cleaned = 0.00870655 Jy ! Component: 400 - total flux cleaned = 0.00894764 Jy ! Total flux subtracted in 400 components = 0.00894764 Jy ! Clean residual min=-0.003519 max=0.003870 Jy/beam ! Clean residual mean=0.000005 rms=0.000969 Jy/beam ! Combined flux in latest and established models = 0.842563 Jy ! Performing phase self-cal ! Adding 42 model components to the UV plane model. ! The established model now contains 170 components and 0.842563 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.075665Jy sigma=0.473957 ! Fit after self-cal, rms=0.075607Jy sigma=0.473722 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! Added new window around map position (-20.4, 23.4). ! clean: niter=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00341283 Jy ! Component: 100 - total flux cleaned = 0.00496805 Jy ! Component: 150 - total flux cleaned = 0.00651338 Jy ! Component: 200 - total flux cleaned = 0.00808793 Jy ! Component: 250 - total flux cleaned = 0.00904699 Jy ! Component: 300 - total flux cleaned = 0.00982261 Jy ! Component: 350 - total flux cleaned = 0.0102978 Jy ! Component: 400 - total flux cleaned = 0.0107564 Jy ! Total flux subtracted in 400 components = 0.0107564 Jy ! Clean residual min=-0.003200 max=0.003664 Jy/beam ! Clean residual mean=0.000004 rms=0.000923 Jy/beam ! Combined flux in latest and established models = 0.85332 Jy ! Performing phase self-cal ! Adding 59 model components to the UV plane model. ! The established model now contains 200 components and 0.85332 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.074970Jy sigma=0.471657 ! Fit after self-cal, rms=0.074914Jy sigma=0.471446 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! Added new window around map position (5.8, -0.8). ! clean: niter=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00371823 Jy ! Component: 100 - total flux cleaned = 0.00521028 Jy ! Component: 150 - total flux cleaned = 0.00624462 Jy ! Component: 200 - total flux cleaned = 0.00720283 Jy ! Component: 250 - total flux cleaned = 0.00830974 Jy ! Component: 300 - total flux cleaned = 0.00922534 Jy ! Component: 350 - total flux cleaned = 0.00997396 Jy ! Component: 400 - total flux cleaned = 0.0106334 Jy ! Total flux subtracted in 400 components = 0.0106334 Jy ! Clean residual min=-0.003156 max=0.003232 Jy/beam ! Clean residual mean=0.000004 rms=0.000886 Jy/beam ! Combined flux in latest and established models = 0.863953 Jy ! Performing phase self-cal ! Adding 55 model components to the UV plane model. ! The established model now contains 231 components and 0.863953 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.074324Jy sigma=0.469686 ! Fit after self-cal, rms=0.074303Jy sigma=0.469540 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam 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 (5.4, 17.4). ! clean: niter=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00327015 Jy ! Component: 100 - total flux cleaned = 0.00509877 Jy ! Component: 150 - total flux cleaned = 0.00640987 Jy ! Component: 200 - total flux cleaned = 0.00784331 Jy ! Component: 250 - total flux cleaned = 0.00914839 Jy ! Component: 300 - total flux cleaned = 0.0104626 Jy ! Component: 350 - total flux cleaned = 0.0116658 Jy ! Component: 400 - total flux cleaned = 0.0128264 Jy ! Total flux subtracted in 400 components = 0.0128264 Jy ! Clean residual min=-0.002976 max=0.003056 Jy/beam ! Clean residual mean=0.000004 rms=0.000810 Jy/beam ! Combined flux in latest and established models = 0.87678 Jy ! Performing phase self-cal ! Adding 62 model components to the UV plane model. ! The established model now contains 259 components and 0.87678 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.073861Jy sigma=0.467630 ! Fit after self-cal, rms=0.073847Jy sigma=0.467536 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! Added new window around map position (12.2, -37.4). ! clean: niter=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00298952 Jy ! Component: 100 - total flux cleaned = 0.0047008 Jy ! Component: 150 - total flux cleaned = 0.00612118 Jy ! Component: 200 - total flux cleaned = 0.00745878 Jy ! Component: 250 - total flux cleaned = 0.00868161 Jy ! Component: 300 - total flux cleaned = 0.00986049 Jy ! Component: 350 - total flux cleaned = 0.0110032 Jy ! Component: 400 - total flux cleaned = 0.0120607 Jy ! Total flux subtracted in 400 components = 0.0120607 Jy ! Clean residual min=-0.002977 max=0.002858 Jy/beam ! Clean residual mean=0.000003 rms=0.000762 Jy/beam ! Combined flux in latest and established models = 0.88884 Jy ! Performing phase self-cal ! Adding 74 model components to the UV plane model. ! The established model now contains 296 components and 0.88884 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.073489Jy sigma=0.466095 ! Fit after self-cal, rms=0.073477Jy sigma=0.465953 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec print "=== Finished natural weighting clean for al sites ===" ! === Finished natural weighting clean for al sites === 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. selfcal true, true, soltime1 ! Performing amp+phase self-cal over 800000 minute time intervals ! ! Correcting IF 1. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 12 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 12 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 18 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 2 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 20 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 18 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 2 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 20 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=0.080358Jy sigma=0.503914 ! Fit after self-cal, rms=0.072055Jy sigma=0.462336 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! Estimated beam: bmin=0.7606 mas, bmaj=1.017 mas, bpa=-61.48 degrees ! Estimated noise=1.14318 mJy/beam. ! clean: niter=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00129363 Jy ! Component: 100 - total flux cleaned = 0.00137654 Jy ! Component: 150 - total flux cleaned = 0.00129727 Jy ! Component: 200 - total flux cleaned = 0.000802646 Jy ! Component: 250 - total flux cleaned = 0.000469235 Jy ! Component: 300 - total flux cleaned = 0.0004687 Jy ! Component: 350 - total flux cleaned = 0.000516294 Jy ! Component: 400 - total flux cleaned = 0.000657498 Jy ! Total flux subtracted in 400 components = 0.000657498 Jy ! Clean residual min=-0.002545 max=0.002377 Jy/beam ! Clean residual mean=0.000002 rms=0.000561 Jy/beam ! Combined flux in latest and established models = 0.889498 Jy selfcal ! Performing phase self-cal ! Adding 37 model components to the UV plane model. ! The established model now contains 313 components and 0.889498 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.071485Jy sigma=0.460863 ! Fit after self-cal, rms=0.071469Jy sigma=0.460750 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec 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=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.51829e-06 Jy ! Component: 100 - total flux cleaned = 2.15561e-06 Jy ! Component: 150 - total flux cleaned = 0.000133143 Jy ! Component: 200 - total flux cleaned = 0.000261063 Jy ! Component: 250 - total flux cleaned = 0.000424986 Jy ! Component: 300 - total flux cleaned = 0.000584272 Jy ! Component: 350 - total flux cleaned = 0.000700243 Jy ! Component: 400 - total flux cleaned = 0.000738263 Jy ! Total flux subtracted in 400 components = 0.000738263 Jy ! Clean residual min=-0.002439 max=0.002303 Jy/beam ! Clean residual mean=0.000002 rms=0.000548 Jy/beam ! Combined flux in latest and established models = 0.890236 Jy ! Performing phase self-cal ! Adding 61 model components to the UV plane model. ! The established model now contains 334 components and 0.890236 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.071297Jy sigma=0.460155 ! Fit after self-cal, rms=0.071285Jy sigma=0.460112 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec 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=0.071285Jy sigma=0.460112 ! Fit after self-cal, rms=0.071068Jy sigma=0.459751 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! Estimated beam: bmin=0.7594 mas, bmaj=1.015 mas, bpa=-61.82 degrees ! Estimated noise=1.14274 mJy/beam. ! clean: niter=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000824171 Jy ! Component: 100 - total flux cleaned = 0.000282042 Jy ! Component: 150 - total flux cleaned = -0.000166639 Jy ! Component: 200 - total flux cleaned = -0.000546138 Jy ! Component: 250 - total flux cleaned = -0.000745692 Jy ! Component: 300 - total flux cleaned = -0.000860947 Jy ! Component: 350 - total flux cleaned = -0.00108442 Jy ! Component: 400 - total flux cleaned = -0.0011928 Jy ! Total flux subtracted in 400 components = -0.0011928 Jy ! Clean residual min=-0.002300 max=0.002151 Jy/beam ! Clean residual mean=0.000001 rms=0.000501 Jy/beam ! Combined flux in latest and established models = 0.889044 Jy selfcal ! Performing phase self-cal ! Adding 55 model components to the UV plane model. ! The established model now contains 352 components and 0.889043 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070866Jy sigma=0.459077 ! Fit after self-cal, rms=0.070858Jy sigma=0.459038 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec 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=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -7.94514e-05 Jy ! Component: 100 - total flux cleaned = -0.00018996 Jy ! Component: 150 - total flux cleaned = -0.00019092 Jy ! Component: 200 - total flux cleaned = -0.000293144 Jy ! Component: 250 - total flux cleaned = -0.000325953 Jy ! Component: 300 - total flux cleaned = -0.000424491 Jy ! Component: 350 - total flux cleaned = -0.000424699 Jy ! Component: 400 - total flux cleaned = -0.000519636 Jy ! Total flux subtracted in 400 components = -0.000519636 Jy ! Clean residual min=-0.002272 max=0.002076 Jy/beam ! Clean residual mean=0.000001 rms=0.000494 Jy/beam ! Combined flux in latest and established models = 0.888524 Jy ! Performing phase self-cal ! Adding 72 model components to the UV plane model. ! The established model now contains 366 components and 0.888524 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070752Jy sigma=0.458654 ! Fit after self-cal, rms=0.070744Jy sigma=0.458633 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec 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, soltime3 ! Performing amp+phase self-cal over 1 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070744Jy sigma=0.458633 ! Fit after self-cal, rms=0.070318Jy sigma=0.454063 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! Estimated beam: bmin=2.223 mas, bmaj=3.191 mas, bpa=-28.32 degrees ! Estimated noise=1.33887 mJy/beam. ! clean: niter=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000193634 Jy ! Component: 100 - total flux cleaned = -0.000370459 Jy ! Component: 150 - total flux cleaned = -0.000648347 Jy ! Component: 200 - total flux cleaned = -0.000704808 Jy ! Component: 250 - total flux cleaned = -0.000678947 Jy ! Component: 300 - total flux cleaned = -0.000702578 Jy ! Component: 350 - total flux cleaned = -0.000816221 Jy ! Component: 400 - total flux cleaned = -0.000903378 Jy ! Total flux subtracted in 400 components = -0.000903378 Jy ! Clean residual min=-0.002521 max=0.002562 Jy/beam ! Clean residual mean=0.000003 rms=0.000686 Jy/beam ! Combined flux in latest and established models = 0.88762 Jy selfcal ! Performing phase self-cal ! Adding 32 model components to the UV plane model. ! The established model now contains 388 components and 0.88762 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070330Jy sigma=0.453905 ! Fit after self-cal, rms=0.070320Jy sigma=0.453864 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec 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 (-48.8, 49). ! clean: niter=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00242293 Jy ! Component: 100 - total flux cleaned = 0.00293095 Jy ! Component: 150 - total flux cleaned = 0.00310975 Jy ! Component: 200 - total flux cleaned = 0.00299429 Jy ! Component: 250 - total flux cleaned = 0.00309917 Jy ! Component: 300 - total flux cleaned = 0.00313187 Jy ! Component: 350 - total flux cleaned = 0.00319374 Jy ! Component: 400 - total flux cleaned = 0.00310503 Jy ! Total flux subtracted in 400 components = 0.00310503 Jy ! Clean residual min=-0.001966 max=0.002022 Jy/beam ! Clean residual mean=0.000005 rms=0.000586 Jy/beam ! Combined flux in latest and established models = 0.890725 Jy ! Performing phase self-cal ! Adding 52 model components to the UV plane model. ! The established model now contains 431 components and 0.890725 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070243Jy sigma=0.452797 ! Fit after self-cal, rms=0.070234Jy sigma=0.452762 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! Added new window around map position (-45.4, -26.4). ! clean: niter=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00149529 Jy ! Component: 100 - total flux cleaned = 0.00234423 Jy ! Component: 150 - total flux cleaned = 0.00298195 Jy ! Component: 200 - total flux cleaned = 0.00329549 Jy ! Component: 250 - total flux cleaned = 0.00358688 Jy ! Component: 300 - total flux cleaned = 0.00382086 Jy ! Component: 350 - total flux cleaned = 0.0040079 Jy ! Component: 400 - total flux cleaned = 0.00418852 Jy ! Total flux subtracted in 400 components = 0.00418852 Jy ! Clean residual min=-0.001704 max=0.001740 Jy/beam ! Clean residual mean=0.000004 rms=0.000508 Jy/beam ! Combined flux in latest and established models = 0.894914 Jy ! Performing phase self-cal ! Adding 88 model components to the UV plane model. ! The established model now contains 511 components and 0.894914 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070162Jy sigma=0.452032 ! Fit after self-cal, rms=0.070154Jy sigma=0.451990 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "=== Finished amplitude self-cal for all stations ===" ! === Finished amplitude self-cal for all stations === restore ! Inverting map and beam ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! Estimated beam: bmin=0.7588 mas, bmaj=1.015 mas, bpa=-62 degrees ! Estimated noise=1.14283 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7588 x 1.015 at -62 degrees (North through East) ! Clean map min=-0.0068869 max=0.63174 Jy/beam if(peak(flux) > thresh) selfcal true, true clean clean_niter,clean_gain selfcal flux_cutoff = imstat(rms) * dynam 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) selfcal true, true end if ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070154Jy sigma=0.451990 ! Fit after self-cal, rms=0.068250Jy sigma=0.428888 ! Inverting map and beam ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! Estimated beam: bmin=0.759 mas, bmaj=1.015 mas, bpa=-61.94 degrees ! Estimated noise=1.14364 mJy/beam. ! clean: niter=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000648319 Jy ! Component: 100 - total flux cleaned = 0.00111971 Jy ! Component: 150 - total flux cleaned = 0.00160599 Jy ! Component: 200 - total flux cleaned = 0.00191271 Jy ! Component: 250 - total flux cleaned = 0.00225177 Jy ! Component: 300 - total flux cleaned = 0.00234508 Jy ! Component: 350 - total flux cleaned = 0.0024357 Jy ! Component: 400 - total flux cleaned = 0.00261236 Jy ! Total flux subtracted in 400 components = 0.00261236 Jy ! Clean residual min=-0.001872 max=0.001731 Jy/beam ! Clean residual mean=0.000001 rms=0.000396 Jy/beam ! Combined flux in latest and established models = 0.897526 Jy ! Performing phase self-cal ! Adding 71 model components to the UV plane model. ! The established model now contains 570 components and 0.897526 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.068038Jy sigma=0.427753 ! Fit after self-cal, rms=0.068033Jy sigma=0.427726 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! clean: niter=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.20434e-06 Jy ! Component: 100 - total flux cleaned = 0.00017374 Jy ! Component: 150 - total flux cleaned = 0.000298076 Jy ! Component: 200 - total flux cleaned = 0.000256417 Jy ! Component: 250 - total flux cleaned = 0.000417824 Jy ! Component: 300 - total flux cleaned = 0.000614738 Jy ! Component: 350 - total flux cleaned = 0.000690996 Jy ! Component: 400 - total flux cleaned = 0.000919701 Jy ! Total flux subtracted in 400 components = 0.000919701 Jy ! Clean residual min=-0.001843 max=0.001713 Jy/beam ! Clean residual mean=0.000001 rms=0.000388 Jy/beam ! Combined flux in latest and established models = 0.898446 Jy ! Performing phase self-cal ! Adding 102 model components to the UV plane model. ! The established model now contains 604 components and 0.898446 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.067901Jy sigma=0.427105 ! Fit after self-cal, rms=0.067897Jy sigma=0.427092 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.067897Jy sigma=0.427092 ! Fit after self-cal, rms=0.067913Jy sigma=0.427020 print "=== CLearing model and starting over ===" ! === CLearing model and starting over === clrmod true ! clrmod: Cleared the established and tentative models. 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. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! Estimated beam: bmin=0.6118 mas, bmaj=0.7519 mas, bpa=-53.59 degrees ! Estimated noise=2.16411 mJy/beam. ! clean: niter=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.509161 Jy ! Component: 100 - total flux cleaned = 0.657868 Jy ! Component: 150 - total flux cleaned = 0.717604 Jy ! Component: 200 - total flux cleaned = 0.749302 Jy ! Component: 250 - total flux cleaned = 0.770111 Jy ! Component: 300 - total flux cleaned = 0.784582 Jy ! Component: 350 - total flux cleaned = 0.795209 Jy ! Component: 400 - total flux cleaned = 0.803672 Jy ! Total flux subtracted in 400 components = 0.803672 Jy ! Clean residual min=-0.004842 max=0.005563 Jy/beam ! Clean residual mean=-0.000001 rms=0.001078 Jy/beam ! Combined flux in latest and established models = 0.803671 Jy 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. flux_cutoff = imstat(rms) * dynam ! Adding 39 model components to the UV plane model. ! The established model now contains 39 components and 0.803671 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! Estimated beam: bmin=0.759 mas, bmaj=1.015 mas, bpa=-61.95 degrees ! Estimated noise=1.14412 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0100212 Jy ! Component: 100 - total flux cleaned = 0.0166653 Jy ! Component: 150 - total flux cleaned = 0.0215541 Jy ! Component: 200 - total flux cleaned = 0.0256226 Jy ! Component: 250 - total flux cleaned = 0.0292529 Jy ! Component: 300 - total flux cleaned = 0.0325695 Jy ! Component: 350 - total flux cleaned = 0.0355126 Jy ! Component: 400 - total flux cleaned = 0.0382774 Jy ! Total flux subtracted in 400 components = 0.0382774 Jy ! Clean residual min=-0.003052 max=0.003000 Jy/beam ! Clean residual mean=0.000002 rms=0.000738 Jy/beam ! Combined flux in latest and established models = 0.841949 Jy ! Adding 84 model components to the UV plane model. ! The established model now contains 112 components and 0.841949 Jy ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! Estimated beam: bmin=2.223 mas, bmaj=3.191 mas, bpa=-28.31 degrees ! Estimated noise=1.34017 mJy/beam. ! clean: niter=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00367316 Jy ! Component: 100 - total flux cleaned = 0.00720971 Jy ! Component: 150 - total flux cleaned = 0.0104086 Jy ! Component: 200 - total flux cleaned = 0.0132166 Jy ! Component: 250 - total flux cleaned = 0.0157105 Jy ! Component: 300 - total flux cleaned = 0.0179359 Jy ! Component: 350 - total flux cleaned = 0.0200369 Jy ! Component: 400 - total flux cleaned = 0.0220308 Jy ! Total flux subtracted in 400 components = 0.0220308 Jy ! Clean residual min=-0.003478 max=0.003100 Jy/beam ! Clean residual mean=0.000007 rms=0.000981 Jy/beam ! Combined flux in latest and established models = 0.86398 Jy flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00189149 Jy ! Component: 100 - total flux cleaned = 0.00377548 Jy ! Component: 150 - total flux cleaned = 0.00548771 Jy ! Component: 200 - total flux cleaned = 0.00712469 Jy ! Component: 250 - total flux cleaned = 0.00869145 Jy ! Component: 300 - total flux cleaned = 0.0102623 Jy ! Component: 350 - total flux cleaned = 0.0116345 Jy ! Component: 400 - total flux cleaned = 0.012958 Jy ! Total flux subtracted in 400 components = 0.012958 Jy ! Clean residual min=-0.003142 max=0.002567 Jy/beam ! Clean residual mean=0.000007 rms=0.000803 Jy/beam ! Combined flux in latest and established models = 0.876938 Jy ! Adding 173 model components to the UV plane model. ! The established model now contains 267 components and 0.876937 Jy ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! Estimated beam: bmin=0.759 mas, bmaj=1.015 mas, bpa=-61.95 degrees ! Estimated noise=1.14412 mJy/beam. ! clean: niter=400 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000777646 Jy ! Component: 100 - total flux cleaned = 0.00157892 Jy ! Component: 150 - total flux cleaned = 0.00219242 Jy ! Component: 200 - total flux cleaned = 0.00285357 Jy ! Component: 250 - total flux cleaned = 0.00363214 Jy ! Component: 300 - total flux cleaned = 0.00424714 Jy ! Component: 350 - total flux cleaned = 0.00497828 Jy ! Component: 400 - total flux cleaned = 0.00588411 Jy ! Total flux subtracted in 400 components = 0.00588411 Jy ! Clean residual min=-0.002383 max=0.002107 Jy/beam ! Clean residual mean=0.000002 rms=0.000508 Jy/beam ! Combined flux in latest and established models = 0.882821 Jy selfcal ! Performing phase self-cal ! Adding 72 model components to the UV plane model. ! The established model now contains 318 components and 0.882821 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.068518Jy sigma=0.431128 ! Fit after self-cal, rms=0.068380Jy sigma=0.430518 wmodel /scr/pima/rdv95_uvs/J0958+6533_X_map.mod ! Writing 318 model components to file: /scr/pima/rdv95_uvs/J0958+6533_X_map.mod wobs /scr/pima/rdv95_uvs/J0958+6533_X_uvs.fits ! Applying 856 buffered edits. ! Writing UV FITS file: /scr/pima/rdv95_uvs/J0958+6533_X_uvs.fits wwins /scr/pima/rdv95_uvs/J0958+6533_X_map.win ! wwins: Wrote 10 windows to /scr/pima/rdv95_uvs/J0958+6533_X_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000680183 Jy ! Component: 100 - total flux cleaned = -0.00107134 Jy ! Component: 150 - total flux cleaned = -0.00151818 Jy ! Component: 200 - total flux cleaned = -0.00180543 Jy ! Component: 250 - total flux cleaned = -0.00208427 Jy ! Component: 300 - total flux cleaned = -0.00232165 Jy ! Component: 350 - total flux cleaned = -0.00261924 Jy ! Component: 400 - total flux cleaned = -0.00294399 Jy ! Component: 450 - total flux cleaned = -0.00319966 Jy ! Component: 500 - total flux cleaned = -0.00345157 Jy ! Component: 550 - total flux cleaned = -0.00363758 Jy ! Component: 600 - total flux cleaned = -0.00375963 Jy ! Component: 650 - total flux cleaned = -0.00381984 Jy ! Component: 700 - total flux cleaned = -0.00381944 Jy ! Component: 750 - total flux cleaned = -0.00384896 Jy ! Component: 800 - total flux cleaned = -0.0038196 Jy ! Component: 850 - total flux cleaned = -0.00387745 Jy ! Component: 900 - total flux cleaned = -0.00379238 Jy ! Component: 950 - total flux cleaned = -0.00384933 Jy ! Component: 1000 - total flux cleaned = -0.00376543 Jy ! Component: 1050 - total flux cleaned = -0.00382098 Jy ! Component: 1100 - total flux cleaned = -0.00387592 Jy ! Component: 1150 - total flux cleaned = -0.00393052 Jy ! Component: 1200 - total flux cleaned = -0.00406506 Jy ! Component: 1250 - total flux cleaned = -0.00409188 Jy ! Component: 1300 - total flux cleaned = -0.00414473 Jy ! Component: 1350 - total flux cleaned = -0.00419748 Jy ! Component: 1400 - total flux cleaned = -0.0042235 Jy ! Component: 1450 - total flux cleaned = -0.00437863 Jy ! Component: 1500 - total flux cleaned = -0.00435288 Jy ! Component: 1550 - total flux cleaned = -0.00445519 Jy ! Component: 1600 - total flux cleaned = -0.00455643 Jy ! Component: 1650 - total flux cleaned = -0.00453139 Jy ! Component: 1700 - total flux cleaned = -0.00458105 Jy ! Component: 1750 - total flux cleaned = -0.00458137 Jy ! Component: 1800 - total flux cleaned = -0.0046059 Jy ! Component: 1850 - total flux cleaned = -0.00463026 Jy ! Component: 1900 - total flux cleaned = -0.00458166 Jy ! Component: 1950 - total flux cleaned = -0.00458195 Jy ! Component: 2000 - total flux cleaned = -0.00467798 Jy ! Component: 2050 - total flux cleaned = -0.0045828 Jy ! Component: 2100 - total flux cleaned = -0.00460641 Jy ! Component: 2150 - total flux cleaned = -0.00462971 Jy ! Component: 2200 - total flux cleaned = -0.00458316 Jy ! Component: 2250 - total flux cleaned = -0.0045601 Jy ! Component: 2300 - total flux cleaned = -0.00442185 Jy ! Component: 2350 - total flux cleaned = -0.00437604 Jy ! Component: 2400 - total flux cleaned = -0.00428494 Jy ! Component: 2450 - total flux cleaned = -0.00426223 Jy ! Component: 2500 - total flux cleaned = -0.00423966 Jy ! Component: 2550 - total flux cleaned = -0.00414984 Jy ! Component: 2600 - total flux cleaned = -0.00410533 Jy ! Component: 2650 - total flux cleaned = -0.00403862 Jy ! Component: 2700 - total flux cleaned = -0.00401646 Jy ! Component: 2750 - total flux cleaned = -0.00397252 Jy ! Component: 2800 - total flux cleaned = -0.00384133 Jy ! Component: 2850 - total flux cleaned = -0.00384144 Jy ! Component: 2900 - total flux cleaned = -0.0037116 Jy ! Component: 2950 - total flux cleaned = -0.0037764 Jy ! Component: 3000 - total flux cleaned = -0.0036691 Jy ! Component: 3050 - total flux cleaned = -0.00358361 Jy ! Component: 3100 - total flux cleaned = -0.00360476 Jy ! Component: 3150 - total flux cleaned = -0.00351978 Jy ! Component: 3200 - total flux cleaned = -0.00354087 Jy ! Component: 3250 - total flux cleaned = -0.00345686 Jy ! Component: 3300 - total flux cleaned = -0.00343602 Jy ! Component: 3350 - total flux cleaned = -0.00341535 Jy ! Component: 3400 - total flux cleaned = -0.00335306 Jy ! Component: 3450 - total flux cleaned = -0.00335313 Jy ! Component: 3500 - total flux cleaned = -0.00318846 Jy ! Component: 3550 - total flux cleaned = -0.00325001 Jy ! Component: 3600 - total flux cleaned = -0.00329082 Jy ! Component: 3650 - total flux cleaned = -0.00331119 Jy ! Component: 3700 - total flux cleaned = -0.00337207 Jy ! Component: 3750 - total flux cleaned = -0.00335163 Jy ! Component: 3800 - total flux cleaned = -0.00343213 Jy ! Component: 3850 - total flux cleaned = -0.0033318 Jy ! Component: 3900 - total flux cleaned = -0.00333175 Jy ! Component: 3950 - total flux cleaned = -0.00335168 Jy ! Component: 4000 - total flux cleaned = -0.00337157 Jy ! Component: 4050 - total flux cleaned = -0.00335189 Jy ! Total flux subtracted in 4096 components = -0.00329269 Jy ! Clean residual min=-0.001121 max=0.001169 Jy/beam ! Clean residual mean=0.000000 rms=0.000321 Jy/beam ! Combined flux in latest and established models = 0.879529 Jy keep ! Adding 322 model components to the UV plane model. ! The established model now contains 640 components and 0.879529 Jy ![Exited script file: /home/lpetrov/bin/rdv_muppet] wmap "/scr/pima/rdv95_uvs/J0958+6533_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.759 x 1.015 at -61.95 degrees (North through East) ! Clean map min=-0.0018183 max=0.63266 Jy/beam ! Writing clean map to FITS file: /scr/pima/rdv95_uvs/J0958+6533_X_map.fits float peak_flux peak_flux = peak(flux,max) invert ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.194 milli-arcsec ! The y-axis pixel size should ideally be below 0.1747 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= 0.6326 rms= 0.00032 Jy quit ! Quitting program ! Log file /scr/pima/rdv95_uvs/J0958+6533_X_uvs.log closed on Wed Nov 6 20:45:54 2013