! Started logfile: /scr/pima/rdv72_uvs/J1625-2527_X_uvs.log on Sat Oct 5 08:48:53 2013 obs /scr/pima/rdv72_uvs/J1625-2527_X_uva.fits ! Reading UV FITS file: /scr/pima/rdv72_uvs/J1625-2527_X_uva.fits ! AN table 1: 8 integrations on 10 of 10 possible baselines. ! AN table 2: 11 integrations on 3 of 3 possible baselines. ! AN table 3: 6 integrations on 1 of 1 possible baselines. ! AN table 4: 2 integrations on 1 of 1 possible baselines. ! AN table 5: 12 integrations on 1 of 1 possible baselines. ! AN table 6: 3 integrations on 10 of 10 possible baselines. ! AN table 7: 6 integrations on 15 of 15 possible baselines. ! AN table 8: 6 integrations on 21 of 21 possible baselines. ! AN table 9: 4 integrations on 28 of 28 possible baselines. ! AN table 10: 3 integrations on 36 of 36 possible baselines. ! AN table 11: 3 integrations on 36 of 36 possible baselines. ! Apparent sampling: 0.841584 visibilities/baseline/integration-bin. ! Found source: J1625-2527 ! ! 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 1.6e+07 1 1.6e+07 ! 02 2 8.47599e+09 1.6e+07 1 1.6e+07 ! 03 3 8.79099e+09 1.6e+07 1 1.6e+07 ! 04 4 8.89599e+09 1.6e+07 1 1.6e+07 ! ! Polarization(s): RR ! ! Read 0 lines of history. ! ! Reading 2380 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/01_muppet /scr/pima/rdv72_uvs/J1625-2527_X] integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.03 float dynam dynam = 6.0 float soltime1 soltime1 = 120 float soltime2 soltime2 = 20 float thresh thresh = 0.5 float win_mult win_mult = 1.8 float time_av time_av = 16 float old_peak float new_peak float flux_cutoff 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 1. ! A total of 27 telescope corrections were flagged in sub-array 2. ! A total of 12 telescope corrections were flagged in sub-array 3. ! A total of 4 telescope corrections were flagged in sub-array 4. ! A total of 24 telescope corrections were flagged in sub-array 5. ! A total of 3 telescope corrections were flagged in sub-array 6. ! A total of 8 telescope corrections were flagged in sub-array 9. ! A total of 4 telescope corrections were flagged in sub-array 10. ! ! Correcting IF 2. ! A total of 12 telescope corrections were flagged in sub-array 1. ! A total of 27 telescope corrections were flagged in sub-array 2. ! A total of 12 telescope corrections were flagged in sub-array 3. ! A total of 4 telescope corrections were flagged in sub-array 4. ! A total of 24 telescope corrections were flagged in sub-array 5. ! A total of 3 telescope corrections were flagged in sub-array 6. ! A total of 8 telescope corrections were flagged in sub-array 9. ! A total of 4 telescope corrections were flagged in sub-array 10. ! ! Correcting IF 3. ! A total of 12 telescope corrections were flagged in sub-array 1. ! A total of 27 telescope corrections were flagged in sub-array 2. ! A total of 12 telescope corrections were flagged in sub-array 3. ! A total of 4 telescope corrections were flagged in sub-array 4. ! A total of 24 telescope corrections were flagged in sub-array 5. ! A total of 3 telescope corrections were flagged in sub-array 6. ! A total of 8 telescope corrections were flagged in sub-array 9. ! A total of 4 telescope corrections were flagged in sub-array 10. ! ! Correcting IF 4. ! A total of 12 telescope corrections were flagged in sub-array 1. ! A total of 27 telescope corrections were flagged in sub-array 2. ! A total of 12 telescope corrections were flagged in sub-array 3. ! A total of 4 telescope corrections were flagged in sub-array 4. ! A total of 24 telescope corrections were flagged in sub-array 5. ! A total of 3 telescope corrections were flagged in sub-array 6. ! A total of 8 telescope corrections were flagged in sub-array 9. ! A total of 4 telescope corrections were flagged in sub-array 10. ! ! Fit before self-cal, rms=1.748708Jy sigma=27.898249 ! Fit after self-cal, rms=0.627143Jy sigma=11.369871 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. 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 0.136% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! Estimated beam: bmin=0.7365 mas, bmaj=1.482 mas, bpa=-11.48 degrees ! Estimated noise=1.4373 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 = 1.16259 Jy ! Component: 100 - total flux cleaned = 1.46419 Jy ! Total flux subtracted in 100 components = 1.46419 Jy ! Clean residual min=-0.084110 max=0.126049 Jy/beam ! Clean residual mean=-0.000588 rms=0.016600 Jy/beam ! Combined flux in latest and established models = 1.46419 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 12 components and 1.46419 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.450786Jy sigma=6.796808 ! Fit after self-cal, rms=0.450776Jy sigma=6.796504 ! Inverting map ! Your choice of large map pixels excluded 0.136% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! Added new window around map position (-0.6, -2.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.131463 Jy ! Component: 100 - total flux cleaned = 0.15324 Jy ! Total flux subtracted in 100 components = 0.15324 Jy ! Clean residual min=-0.077063 max=0.078537 Jy/beam ! Clean residual mean=-0.000510 rms=0.014166 Jy/beam ! Combined flux in latest and established models = 1.61743 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 22 components and 1.61743 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.437014Jy sigma=5.869271 ! Fit after self-cal, rms=0.436326Jy sigma=5.858021 ! Inverting map ! Your choice of large map pixels excluded 0.136% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec 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 ! Your choice of large map pixels excluded 0.136% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! Estimated beam: bmin=0.8991 mas, bmaj=1.796 mas, bpa=-13.91 degrees ! Estimated noise=1.12578 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 = 0.0662536 Jy ! Component: 100 - total flux cleaned = 0.0839674 Jy ! Component: 150 - total flux cleaned = 0.0870552 Jy ! Component: 200 - total flux cleaned = 0.0896971 Jy ! Total flux subtracted in 200 components = 0.0896971 Jy ! Clean residual min=-0.064903 max=0.083932 Jy/beam ! Clean residual mean=-0.000834 rms=0.017514 Jy/beam ! Combined flux in latest and established models = 1.70713 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 32 components and 1.70713 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.440458Jy sigma=5.495694 ! Fit after self-cal, rms=0.440320Jy sigma=5.491342 ! Inverting map ! Your choice of large map pixels excluded 0.136% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 9 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HO 0.82 KK 1.26 KP 0.93 MK 0.91 ! OV 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HO 0.00* KK 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! HO 0.00* KK 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! KK 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! WZ 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! FD 1.00* LA 0.97 NL 1.23 PT 1.13 ! SC 0.85 ! ! Telescope amplitude corrections in sub-array 7: ! FD 0.78 KP 1.63 LA 0.95 NL 1.06 ! PT 0.96 SC 0.89 ! ! Telescope amplitude corrections in sub-array 8: ! FD 0.76 KP 1.69 LA 0.95 NL 1.05 ! OV 1.03 PT 1.03 SC 0.93 ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.47 FD 0.77 KP 1.53 LA 0.94 ! NL 0.99 OV 1.02 PT 0.89 SC 0.97 ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.42 FD 0.81 KP 1.82 LA 0.89 ! MK 0.94 NL 1.02 OV 1.04 PT 0.88 ! SC 1.01 ! ! Telescope amplitude corrections in sub-array 11: ! FD 0.76 KK 1.33 KP 1.86 LA 0.97 ! MK 0.92 NL 1.11 OV 1.02 PT 0.88 ! SC 0.91 ! ! ! Correcting IF 2. ! A total of 9 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HO 0.90 KK 1.13 KP 0.88 MK 0.92 ! OV 0.95 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HO 0.00* KK 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! HO 0.00* KK 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! KK 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! WZ 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! FD 1.00* LA 0.99 NL 1.21 PT 1.16 ! SC 0.90 ! ! Telescope amplitude corrections in sub-array 7: ! FD 0.78 KP 1.63 LA 0.93 NL 1.08 ! PT 1.00 SC 0.92 ! ! Telescope amplitude corrections in sub-array 8: ! FD 0.77 KP 1.59 LA 0.93 NL 1.04 ! OV 1.02 PT 1.14 SC 0.97 ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.44 FD 0.77 KP 1.45 LA 0.92 ! NL 1.01 OV 1.01 PT 0.93 SC 1.00 ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.40 FD 0.82 KP 1.81 LA 0.90 ! MK 0.94 NL 1.05 OV 1.01 PT 0.95 ! SC 1.05 ! ! Telescope amplitude corrections in sub-array 11: ! FD 0.77 KK 1.21 KP 1.79 LA 0.97 ! MK 0.91 NL 1.10 OV 1.02 PT 0.93 ! SC 0.94 ! ! ! Correcting IF 3. ! A total of 9 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HO 1.08 KK 1.16 KP 0.81 MK 0.92 ! OV 1.01 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HO 0.00* KK 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! HO 0.00* KK 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! KK 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! WZ 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! FD 1.00* LA 1.01 NL 1.31 PT 1.26 ! SC 0.91 ! ! Telescope amplitude corrections in sub-array 7: ! FD 0.77 KP 1.52 LA 1.00 NL 1.13 ! PT 1.02 SC 0.92 ! ! Telescope amplitude corrections in sub-array 8: ! FD 0.77 KP 1.57 LA 0.98 NL 1.09 ! OV 1.09 PT 1.11 SC 0.99 ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.56 FD 0.76 KP 1.39 LA 0.95 ! NL 1.01 OV 1.05 PT 0.99 SC 1.03 ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.54 FD 0.81 KP 1.74 LA 0.93 ! MK 0.95 NL 1.08 OV 1.05 PT 0.95 ! SC 1.05 ! ! Telescope amplitude corrections in sub-array 11: ! FD 0.78 KK 1.29 KP 1.69 LA 1.02 ! MK 0.93 NL 1.15 OV 1.05 PT 0.94 ! SC 0.95 ! ! ! Correcting IF 4. ! A total of 9 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HO 1.10 KK 1.20 KP 0.83 MK 0.95 ! OV 1.04 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HO 0.00* KK 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! HO 0.00* KK 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! KK 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! WZ 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! FD 1.00* LA 1.01 NL 1.51 PT 1.25 ! SC 0.91 ! ! Telescope amplitude corrections in sub-array 7: ! FD 0.81 KP 1.63 LA 1.04 NL 1.16 ! PT 1.03 SC 0.94 ! ! Telescope amplitude corrections in sub-array 8: ! FD 0.80 KP 1.66 LA 1.01 NL 1.14 ! OV 1.06 PT 1.14 SC 1.02 ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.56 FD 0.80 KP 1.51 LA 0.97 ! NL 1.05 OV 1.06 PT 0.99 SC 1.05 ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.53 FD 0.85 KP 1.83 LA 0.95 ! MK 0.95 NL 1.12 OV 1.04 PT 0.95 ! SC 1.06 ! ! Telescope amplitude corrections in sub-array 11: ! FD 0.82 KK 1.31 KP 1.84 LA 1.04 ! MK 0.96 NL 1.20 OV 1.05 PT 0.94 ! SC 0.93 ! ! ! Fit before self-cal, rms=0.440320Jy sigma=5.491342 ! Fit after self-cal, rms=0.243601Jy sigma=2.316088 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! Estimated beam: bmin=0.9137 mas, bmaj=1.929 mas, bpa=-10.05 degrees ! Estimated noise=1.12578 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 = -0.020266 Jy ! Component: 100 - total flux cleaned = -0.0223974 Jy ! Component: 150 - total flux cleaned = -0.0237353 Jy ! Component: 200 - total flux cleaned = -0.0241954 Jy ! Total flux subtracted in 200 components = -0.0241954 Jy ! Clean residual min=-0.017662 max=0.017870 Jy/beam ! Clean residual mean=0.000175 rms=0.003234 Jy/beam ! Combined flux in latest and established models = 1.68294 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 38 components and 1.68294 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.240886Jy sigma=2.287882 ! Fit after self-cal, rms=0.242036Jy sigma=2.283154 ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! Added new window around map position (0.4, 3.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0154938 Jy ! Component: 100 - total flux cleaned = 0.0151188 Jy ! Component: 150 - total flux cleaned = 0.0147854 Jy ! Component: 200 - total flux cleaned = 0.013564 Jy ! Total flux subtracted in 200 components = 0.013564 Jy ! Clean residual min=-0.015692 max=0.011048 Jy/beam ! Clean residual mean=0.000197 rms=0.002972 Jy/beam ! Combined flux in latest and established models = 1.6965 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 50 components and 1.6965 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.240090Jy sigma=2.243850 ! Fit after self-cal, rms=0.239819Jy sigma=2.237207 ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec selfcal true, true, soltime1 ! Performing amp+phase self-cal over 120 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.239819Jy sigma=2.237207 ! Fit after self-cal, rms=0.239012Jy sigma=2.229689 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! Estimated beam: bmin=0.9144 mas, bmaj=1.931 mas, bpa=-9.967 degrees ! Estimated noise=1.12395 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00683175 Jy ! Component: 100 - total flux cleaned = -0.00781368 Jy ! Component: 150 - total flux cleaned = -0.00832961 Jy ! Component: 200 - total flux cleaned = -0.00896912 Jy ! Total flux subtracted in 200 components = -0.00896912 Jy ! Clean residual min=-0.013947 max=0.010436 Jy/beam ! Clean residual mean=0.000189 rms=0.002814 Jy/beam ! Combined flux in latest and established models = 1.68753 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 57 components and 1.68753 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.237661Jy sigma=2.216217 ! Fit after self-cal, rms=0.237612Jy sigma=2.213117 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 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=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000755751 Jy ! Component: 100 - total flux cleaned = 0.000969199 Jy ! Component: 150 - total flux cleaned = 0.000975824 Jy ! Component: 200 - total flux cleaned = 0.00081187 Jy ! Total flux subtracted in 200 components = 0.00081187 Jy ! Clean residual min=-0.012823 max=0.010153 Jy/beam ! Clean residual mean=0.000190 rms=0.002765 Jy/beam ! Combined flux in latest and established models = 1.68834 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 68 components and 1.68834 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.237115Jy sigma=2.206645 ! Fit after self-cal, rms=0.237137Jy sigma=2.205239 ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec selfcal true, true, soltime2 ! Performing amp+phase self-cal over 20 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.237137Jy sigma=2.205239 ! Fit after self-cal, rms=0.230584Jy sigma=2.119928 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! Estimated beam: bmin=0.9151 mas, bmaj=1.932 mas, bpa=-9.907 degrees ! Estimated noise=1.12234 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00617431 Jy ! Component: 100 - total flux cleaned = -0.00637754 Jy ! Component: 150 - total flux cleaned = -0.00654169 Jy ! Component: 200 - total flux cleaned = -0.00654386 Jy ! Total flux subtracted in 200 components = -0.00654386 Jy ! Clean residual min=-0.011409 max=0.009346 Jy/beam ! Clean residual mean=0.000101 rms=0.002429 Jy/beam ! Combined flux in latest and established models = 1.6818 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 71 components and 1.6818 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.230000Jy sigma=2.115171 ! Fit after self-cal, rms=0.230077Jy sigma=2.114430 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 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=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000588925 Jy ! Component: 100 - total flux cleaned = 0.000442479 Jy ! Component: 150 - total flux cleaned = 0.000316879 Jy ! Component: 200 - total flux cleaned = 0.00019907 Jy ! Total flux subtracted in 200 components = 0.00019907 Jy ! Clean residual min=-0.010951 max=0.009451 Jy/beam ! Clean residual mean=0.000101 rms=0.002414 Jy/beam ! Combined flux in latest and established models = 1.682 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 72 components and 1.682 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.229818Jy sigma=2.111953 ! Fit after self-cal, rms=0.229874Jy sigma=2.111498 ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 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, soltime2 ! Performing amp+phase self-cal over 20 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.229874Jy sigma=2.111498 ! Fit after self-cal, rms=0.229817Jy sigma=2.108434 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! Estimated beam: bmin=2.321 mas, bmaj=5.67 mas, bpa=-5.714 degrees ! Estimated noise=1.42537 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00416241 Jy ! Component: 100 - total flux cleaned = -0.00463847 Jy ! Component: 150 - total flux cleaned = -0.0048503 Jy ! Component: 200 - total flux cleaned = -0.0051526 Jy ! Total flux subtracted in 200 components = -0.0051526 Jy ! Clean residual min=-0.013486 max=0.010075 Jy/beam ! Clean residual mean=0.000190 rms=0.003095 Jy/beam ! Combined flux in latest and established models = 1.67684 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 82 components and 1.67684 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.229578Jy sigma=2.106867 ! Fit after self-cal, rms=0.229612Jy sigma=2.106338 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 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=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000266303 Jy ! Component: 100 - total flux cleaned = -0.00015127 Jy ! Component: 150 - total flux cleaned = -0.00042301 Jy ! Component: 200 - total flux cleaned = -0.000592709 Jy ! Total flux subtracted in 200 components = -0.000592709 Jy ! Clean residual min=-0.013185 max=0.010014 Jy/beam ! Clean residual mean=0.000190 rms=0.003075 Jy/beam ! Combined flux in latest and established models = 1.67625 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 86 components and 1.67625 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.229523Jy sigma=2.105945 ! Fit after self-cal, rms=0.229549Jy sigma=2.105717 ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "************** FINISHED AMPLITUDE SELF-CAL **************" ! ************** FINISHED AMPLITUDE SELF-CAL ************** restore ! Inverting map and beam ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! Estimated beam: bmin=0.9157 mas, bmaj=1.933 mas, bpa=-9.87 degrees ! Estimated noise=1.12119 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9157 x 1.933 at -9.87 degrees (North through East) ! Clean map min=-0.019074 max=1.3984 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=0.229549Jy sigma=2.105717 ! Fit after self-cal, rms=0.269399Jy sigma=1.438453 ! Inverting map and beam ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! Estimated beam: bmin=0.9152 mas, bmaj=1.935 mas, bpa=-9.801 degrees ! Estimated noise=1.12183 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00346082 Jy ! Component: 100 - total flux cleaned = -0.00438597 Jy ! Component: 150 - total flux cleaned = -0.00500669 Jy ! Component: 200 - total flux cleaned = -0.00532895 Jy ! Total flux subtracted in 200 components = -0.00532895 Jy ! Clean residual min=-0.008563 max=0.007268 Jy/beam ! Clean residual mean=0.000102 rms=0.001941 Jy/beam ! Combined flux in latest and established models = 1.67092 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 94 components and 1.67092 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.269047Jy sigma=1.434416 ! Fit after self-cal, rms=0.269055Jy sigma=1.433987 ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -4.65274e-05 Jy ! Component: 100 - total flux cleaned = -4.42032e-05 Jy ! Component: 150 - total flux cleaned = -0.000143026 Jy ! Component: 200 - total flux cleaned = -0.000229861 Jy ! Total flux subtracted in 200 components = -0.000229861 Jy ! Clean residual min=-0.008492 max=0.007304 Jy/beam ! Clean residual mean=0.000102 rms=0.001931 Jy/beam ! Combined flux in latest and established models = 1.67069 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 98 components and 1.67069 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.268907Jy sigma=1.432325 ! Fit after self-cal, rms=0.268931Jy sigma=1.432149 ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.268931Jy sigma=1.432149 ! Fit after self-cal, rms=0.270087Jy sigma=1.429874 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 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! Estimated beam: bmin=0.7356 mas, bmaj=1.546 mas, bpa=-9.285 degrees ! Estimated noise=1.43508 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.16974 Jy ! Component: 100 - total flux cleaned = 1.46296 Jy ! Component: 150 - total flux cleaned = 1.57227 Jy ! Component: 200 - total flux cleaned = 1.62869 Jy ! Total flux subtracted in 200 components = 1.62869 Jy ! Clean residual min=-0.028123 max=0.028602 Jy/beam ! Clean residual mean=0.000008 rms=0.003663 Jy/beam ! Combined flux in latest and established models = 1.62869 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 22 model components to the UV plane model. ! The established model now contains 22 components and 1.62869 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! Estimated beam: bmin=0.915 mas, bmaj=1.935 mas, bpa=-9.755 degrees ! Estimated noise=1.12189 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=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0295037 Jy ! Component: 100 - total flux cleaned = 0.0344622 Jy ! Component: 150 - total flux cleaned = 0.0363404 Jy ! Component: 200 - total flux cleaned = 0.0383435 Jy ! Total flux subtracted in 200 components = 0.0383435 Jy ! Clean residual min=-0.010622 max=0.013144 Jy/beam ! Clean residual mean=0.000097 rms=0.002120 Jy/beam ! Combined flux in latest and established models = 1.66704 Jy ! Adding 20 model components to the UV plane model. ! The established model now contains 35 components and 1.66704 Jy ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! Added new window around map position (2.2, 2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00514067 Jy ! Component: 100 - total flux cleaned = 0.00481987 Jy ! Component: 150 - total flux cleaned = 0.00482434 Jy ! Component: 200 - total flux cleaned = 0.00507816 Jy ! Total flux subtracted in 200 components = 0.00507816 Jy ! Clean residual min=-0.008936 max=0.008462 Jy/beam ! Clean residual mean=0.000107 rms=0.001962 Jy/beam ! Combined flux in latest and established models = 1.67211 Jy ! Adding 18 model components to the UV plane model. ! The established model now contains 48 components and 1.67211 Jy ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 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 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! Estimated beam: bmin=2.324 mas, bmaj=5.684 mas, bpa=-5.55 degrees ! Estimated noise=1.42623 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000219992 Jy ! Component: 100 - total flux cleaned = -0.000984838 Jy ! Component: 150 - total flux cleaned = -0.00165687 Jy ! Component: 200 - total flux cleaned = -0.00226041 Jy ! Total flux subtracted in 200 components = -0.00226041 Jy ! Clean residual min=-0.009183 max=0.008212 Jy/beam ! Clean residual mean=0.000208 rms=0.002541 Jy/beam ! Combined flux in latest and established models = 1.66985 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=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000555164 Jy ! Component: 100 - total flux cleaned = -0.00106135 Jy ! Component: 150 - total flux cleaned = -0.00134497 Jy ! Component: 200 - total flux cleaned = -0.00161753 Jy ! Total flux subtracted in 200 components = -0.00161753 Jy ! Clean residual min=-0.008893 max=0.008016 Jy/beam ! Clean residual mean=0.000205 rms=0.002529 Jy/beam ! Combined flux in latest and established models = 1.66824 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 70 components and 1.66824 Jy ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! Estimated beam: bmin=0.915 mas, bmaj=1.935 mas, bpa=-9.755 degrees ! Estimated noise=1.12189 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.91859e-05 Jy ! Component: 100 - total flux cleaned = 1.07309e-05 Jy ! Component: 150 - total flux cleaned = 0.000210929 Jy ! Component: 200 - total flux cleaned = 4.0076e-05 Jy ! Total flux subtracted in 200 components = 4.0076e-05 Jy ! Clean residual min=-0.009085 max=0.008279 Jy/beam ! Clean residual mean=0.000106 rms=0.001900 Jy/beam ! Combined flux in latest and established models = 1.66828 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 77 components and 1.66828 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.269786Jy sigma=1.431305 ! Fit after self-cal, rms=0.269715Jy sigma=1.425098 wmodel /scr/pima/rdv72_uvs/J1625-2527_X_map.mod ! Writing 77 model components to file: /scr/pima/rdv72_uvs/J1625-2527_X_map.mod wobs /scr/pima/rdv72_uvs/J1625-2527_X_uvs.fits ! Writing UV FITS file: /scr/pima/rdv72_uvs/J1625-2527_X_uvs.fits wwins /scr/pima/rdv72_uvs/J1625-2527_X_map.win ! wwins: Wrote 4 windows to /scr/pima/rdv72_uvs/J1625-2527_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 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00265244 Jy ! Component: 100 - total flux cleaned = -0.00389166 Jy ! Component: 150 - total flux cleaned = -0.00454587 Jy ! Component: 200 - total flux cleaned = -0.00517599 Jy ! Component: 250 - total flux cleaned = -0.00554365 Jy ! Component: 300 - total flux cleaned = -0.00566037 Jy ! Component: 350 - total flux cleaned = -0.00542943 Jy ! Component: 400 - total flux cleaned = -0.00542776 Jy ! Component: 450 - total flux cleaned = -0.00498512 Jy ! Component: 500 - total flux cleaned = -0.00433926 Jy ! Component: 550 - total flux cleaned = -0.00391792 Jy ! Component: 600 - total flux cleaned = -0.00329636 Jy ! Component: 650 - total flux cleaned = -0.00238152 Jy ! Component: 700 - total flux cleaned = -0.0019844 Jy ! Component: 750 - total flux cleaned = -0.00178765 Jy ! Component: 800 - total flux cleaned = -0.00110485 Jy ! Component: 850 - total flux cleaned = -0.000529457 Jy ! Component: 900 - total flux cleaned = -0.000149652 Jy ! Component: 950 - total flux cleaned = 0.000412014 Jy ! Component: 1000 - total flux cleaned = 0.000689805 Jy ! Component: 1050 - total flux cleaned = 0.00114529 Jy ! Component: 1100 - total flux cleaned = 0.00105525 Jy ! Component: 1150 - total flux cleaned = 0.00141163 Jy ! Component: 1200 - total flux cleaned = 0.00149972 Jy ! Component: 1250 - total flux cleaned = 0.0014116 Jy ! Component: 1300 - total flux cleaned = 0.0019294 Jy ! Component: 1350 - total flux cleaned = 0.00210056 Jy ! Component: 1400 - total flux cleaned = 0.00260874 Jy ! Component: 1450 - total flux cleaned = 0.00277561 Jy ! Component: 1500 - total flux cleaned = 0.00310714 Jy ! Component: 1550 - total flux cleaned = 0.00310762 Jy ! Component: 1600 - total flux cleaned = 0.00351586 Jy ! Component: 1650 - total flux cleaned = 0.00367828 Jy ! Component: 1700 - total flux cleaned = 0.00415998 Jy ! Component: 1750 - total flux cleaned = 0.00392035 Jy ! Component: 1800 - total flux cleaned = 0.00423657 Jy ! Component: 1850 - total flux cleaned = 0.00439285 Jy ! Component: 1900 - total flux cleaned = 0.00478034 Jy ! Component: 1950 - total flux cleaned = 0.00485738 Jy ! Component: 2000 - total flux cleaned = 0.00478092 Jy ! Component: 2050 - total flux cleaned = 0.00531188 Jy ! Component: 2100 - total flux cleaned = 0.00508651 Jy ! Component: 2150 - total flux cleaned = 0.00501147 Jy ! Component: 2200 - total flux cleaned = 0.00516029 Jy ! Component: 2250 - total flux cleaned = 0.00515947 Jy ! Component: 2300 - total flux cleaned = 0.00567114 Jy ! Component: 2350 - total flux cleaned = 0.00588875 Jy ! Component: 2400 - total flux cleaned = 0.005745 Jy ! Component: 2450 - total flux cleaned = 0.00595998 Jy ! Component: 2500 - total flux cleaned = 0.00617352 Jy ! Component: 2550 - total flux cleaned = 0.00617299 Jy ! Component: 2600 - total flux cleaned = 0.00652458 Jy ! Component: 2650 - total flux cleaned = 0.00631499 Jy ! Component: 2700 - total flux cleaned = 0.00659218 Jy ! Component: 2750 - total flux cleaned = 0.00659096 Jy ! Component: 2800 - total flux cleaned = 0.00652248 Jy ! Component: 2850 - total flux cleaned = 0.0068638 Jy ! Component: 2900 - total flux cleaned = 0.00679567 Jy ! Component: 2950 - total flux cleaned = 0.00672939 Jy ! Component: 3000 - total flux cleaned = 0.00706368 Jy ! Component: 3050 - total flux cleaned = 0.00712998 Jy ! Component: 3100 - total flux cleaned = 0.00712973 Jy ! Component: 3150 - total flux cleaned = 0.0072611 Jy ! Component: 3200 - total flux cleaned = 0.00706581 Jy ! Component: 3250 - total flux cleaned = 0.00719576 Jy ! Component: 3300 - total flux cleaned = 0.00713156 Jy ! Component: 3350 - total flux cleaned = 0.00764586 Jy ! Component: 3400 - total flux cleaned = 0.00726249 Jy ! Component: 3450 - total flux cleaned = 0.00770717 Jy ! Component: 3500 - total flux cleaned = 0.00739051 Jy ! Component: 3550 - total flux cleaned = 0.00751655 Jy ! Component: 3600 - total flux cleaned = 0.00751637 Jy ! Component: 3650 - total flux cleaned = 0.00776525 Jy ! Component: 3700 - total flux cleaned = 0.0078268 Jy ! Component: 3750 - total flux cleaned = 0.00764206 Jy ! Component: 3800 - total flux cleaned = 0.00776448 Jy ! Component: 3850 - total flux cleaned = 0.00776393 Jy ! Component: 3900 - total flux cleaned = 0.0075216 Jy ! Component: 3950 - total flux cleaned = 0.00824551 Jy ! Component: 4000 - total flux cleaned = 0.00812523 Jy ! Component: 4050 - total flux cleaned = 0.00818489 Jy ! Total flux subtracted in 4096 components = 0.00824439 Jy ! Clean residual min=-0.003265 max=0.003081 Jy/beam ! Clean residual mean=0.000054 rms=0.001065 Jy/beam ! Combined flux in latest and established models = 1.67652 Jy keep ! Adding 320 model components to the UV plane model. ! The established model now contains 397 components and 1.67652 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/rdv72_uvs/J1625-2527_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.915 x 1.935 at -9.755 degrees (North through East) ! Clean map min=-0.0068247 max=1.4267 Jy/beam ! Writing clean map to FITS file: /scr/pima/rdv72_uvs/J1625-2527_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 1.42667 invert ! Inverting map ! Your choice of large map pixels excluded 0.139% of the data. ! The x-axis pixel size should ideally be below 0.1996 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00105768 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.222409 0.222409 0.444818 0.889636 1.77927 3.55854 7.11709 14.2342 28.4683 56.9367 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0031 print "peak=",int(1000*peak_flux)/1000 ! peak= 1.426 quit ! Quitting program ! Log file /scr/pima/rdv72_uvs/J1625-2527_X_uvs.log closed on Sat Oct 5 08:48:57 2013