! Started logfile: /scr/pima/gb073_uvs/J1431+2442_X_uvs.log on Sat Dec 26 09:40:38 2015 obs /scr/pima/gb073_uvs/J1431+2442_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1431+2442_X_uva.fits ! AN table 1: 29 integrations on 45 of 45 possible baselines. ! AN table 2: 29 integrations on 66 of 66 possible baselines. ! AN table 3: 29 integrations on 55 of 55 possible baselines. ! AN table 4: 29 integrations on 36 of 36 possible baselines. ! AN table 5: 29 integrations on 28 of 28 possible baselines. ! Apparent sampling: 0.922189 visibilities/baseline/integration-bin. ! Found source: J1431+2442 ! ! There are 8 IFs, and a total of 8 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.39799e+09 8e+06 1 8e+06 ! 02 2 8.40599e+09 8e+06 1 8e+06 ! 03 3 8.46799e+09 8e+06 1 8e+06 ! 04 4 8.47599e+09 8e+06 1 8e+06 ! 05 5 8.78299e+09 8e+06 1 8e+06 ! 06 6 8.79099e+09 8e+06 1 8e+06 ! 07 7 8.88799e+09 8e+06 1 8e+06 ! 08 8 8.89599e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 0 lines of history. ! ! Reading 49208 visibilities. select RR ! Selecting polarization: RR, channels: 1..8 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 ! Reading IF 5 channels: 5..5 ! Reading IF 6 channels: 6..6 ! Reading IF 7 channels: 7..7 ! Reading IF 8 channels: 8..8 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/gb073_uvs/J1431+2442_X] float lim_self lim_self = 120.0 float lim_val lim_va = 1.2 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 35 telescope corrections were flagged in sub-array 1. ! A total of 34 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 35 telescope corrections were flagged in sub-array 1. ! A total of 34 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 35 telescope corrections were flagged in sub-array 1. ! A total of 34 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 35 telescope corrections were flagged in sub-array 1. ! A total of 34 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 5. ! A total of 64 telescope corrections were flagged in sub-array 1. ! A total of 63 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 6. ! A total of 64 telescope corrections were flagged in sub-array 1. ! A total of 63 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 7. ! A total of 35 telescope corrections were flagged in sub-array 1. ! A total of 34 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 8. ! A total of 35 telescope corrections were flagged in sub-array 1. ! A total of 34 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=1.011122Jy sigma=10.120600 ! Fit after self-cal, rms=0.896246Jy sigma=8.953758 ! 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 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 milli-arcsec ! Estimated beam: bmin=0.4978 mas, bmaj=1.354 mas, bpa=-11.65 degrees ! Estimated noise=0.805751 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 = 0.0793103 Jy ! Component: 100 - total flux cleaned = 0.0979418 Jy ! Total flux subtracted in 100 components = 0.0979418 Jy ! Clean residual min=-0.003937 max=0.007416 Jy/beam ! Clean residual mean=0.000000 rms=0.000825 Jy/beam ! Combined flux in latest and established models = 0.0979418 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.0979418 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.080088Jy sigma=0.690833 ! Fit after self-cal, rms=0.079994Jy sigma=0.690294 ! Inverting map ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00802953 Jy ! Component: 100 - total flux cleaned = 0.0122275 Jy ! Total flux subtracted in 100 components = 0.0122275 Jy ! Clean residual min=-0.003606 max=0.003761 Jy/beam ! Clean residual mean=-0.000001 rms=0.000733 Jy/beam ! Combined flux in latest and established models = 0.110169 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 14 components and 0.110169 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.078999Jy sigma=0.676443 ! Fit after self-cal, rms=0.078994Jy sigma=0.676346 ! Inverting map ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 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 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 milli-arcsec ! Estimated beam: bmin=0.6964 mas, bmaj=1.684 mas, bpa=-10.77 degrees ! Estimated noise=0.35425 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 (-0.8, 0.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00467244 Jy ! Component: 100 - total flux cleaned = 0.00688333 Jy ! Component: 150 - total flux cleaned = 0.00789114 Jy ! Component: 200 - total flux cleaned = 0.00828628 Jy ! Total flux subtracted in 200 components = 0.00828628 Jy ! Clean residual min=-0.001809 max=0.001924 Jy/beam ! Clean residual mean=0.000001 rms=0.000357 Jy/beam ! Combined flux in latest and established models = 0.118456 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 34 components and 0.118456 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.078697Jy sigma=0.673202 ! Fit after self-cal, rms=0.078681Jy sigma=0.672967 ! Inverting map ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6964 x 1.684 at -10.77 degrees (North through East) ! Clean map min=-0.0013401 max=0.10439 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val ! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2. ! Selfcal phase corrections will not be limited. gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 EF 1.00* FD 0.96 KP 0.98 ! LA 1.04 MC 1.03 NL 0.94 ON 0.98 ! OV 1.00 PT 0.97 SC 0.95 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.95 FD 1.06 KP 0.99 LA 1.01 ! MK 0.97 NL 0.90 OV 1.05 PT 0.94 ! SC 1.04 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.94 FD 1.06 KP 0.99 LA 1.07 ! MK 0.95 NL 1.00 OV 1.01 PT 0.97 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.96 EF 1.00* FD 0.99 KP 1.00 ! LA 1.03 MC 0.94 NL 0.98 ON 1.06 ! OV 1.04 PT 1.04 SC 0.97 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 FD 1.06 KP 1.01 LA 1.07 ! MK 0.99 NL 0.98 OV 1.01 PT 0.98 ! SC 1.10 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.05 FD 1.07 KP 1.00 LA 1.03 ! MK 0.99 NL 0.99 OV 1.03 PT 1.03 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 EF 1.00* FD 1.03 KP 0.94 ! LA 0.99 MC 0.94 NL 0.96 ON 1.11 ! OV 0.97 PT 1.00 SC 1.05 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 FD 1.04 KP 0.96 LA 1.02 ! MK 0.93 NL 0.93 OV 1.03 PT 1.01 ! SC 1.11 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 FD 1.02 KP 0.93 LA 1.02 ! MK 0.95 NL 0.97 OV 0.95 PT 1.02 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.96 EF 1.00* FD 1.01 KP 0.97 ! LA 1.02 MC 1.02 NL 1.03 ON 1.03 ! OV 0.99 PT 1.02 SC 1.00 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 FD 1.03 KP 1.01 LA 1.00 ! MK 0.95 NL 0.97 OV 1.02 PT 1.03 ! SC 1.09 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 1.00 KP 1.02 LA 1.03 ! MK 0.95 NL 1.00 OV 0.96 PT 1.03 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 0.98 KP 0.84 LA 0.99 ! MK 1.03 NL 0.97 OV 1.07 PT 0.96 ! SC 1.09 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 1.01 KP 0.87 LA 1.05 ! MK 0.95 NL 1.02 OV 1.01 PT 1.00 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.04 KP 0.84 LA 0.99 ! MK 1.04 NL 0.93 OV 1.07 PT 0.99 ! SC 1.05 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 1.01 KP 0.87 LA 0.99 ! MK 0.91 NL 1.06 OV 1.03 PT 0.93 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 FD 1.03 KP 0.92 LA 1.02 ! MK 1.09 NL 0.98 OV 1.01 PT 1.07 ! SC 1.04 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.04 FD 0.99 KP 0.88 LA 1.03 ! MK 1.03 NL 1.09 OV 1.05 PT 1.04 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 FD 1.08 KP 0.87 LA 1.10 ! MK 1.06 NL 0.99 OV 1.00 PT 0.96 ! SC 1.05 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 FD 0.97 KP 0.94 LA 0.96 ! MK 0.98 NL 1.09 OV 1.02 PT 1.05 ! ! ! Fit before self-cal, rms=0.078681Jy sigma=0.672967 ! Fit after self-cal, rms=0.078786Jy sigma=0.670794 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 milli-arcsec ! Estimated beam: bmin=0.6972 mas, bmaj=1.68 mas, bpa=-10.83 degrees ! Estimated noise=0.353519 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 = 0.000613067 Jy ! Component: 100 - total flux cleaned = 0.000782805 Jy ! Component: 150 - total flux cleaned = 0.000901099 Jy ! Component: 200 - total flux cleaned = 0.000922375 Jy ! Total flux subtracted in 200 components = 0.000922375 Jy ! Clean residual min=-0.001731 max=0.001525 Jy/beam ! Clean residual mean=0.000001 rms=0.000317 Jy/beam ! Combined flux in latest and established models = 0.119378 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 48 components and 0.119378 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.078740Jy sigma=0.670494 ! Fit after self-cal, rms=0.078753Jy sigma=0.670426 ! Inverting map ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 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. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.078753Jy sigma=0.670426 ! Fit after self-cal, rms=0.078730Jy sigma=0.670414 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 milli-arcsec ! Estimated beam: bmin=0.6967 mas, bmaj=1.678 mas, bpa=-10.84 degrees ! Estimated noise=0.353773 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000309496 Jy ! Component: 100 - total flux cleaned = 0.00035354 Jy ! Component: 150 - total flux cleaned = 0.000372612 Jy ! Component: 200 - total flux cleaned = 0.000372547 Jy ! Total flux subtracted in 200 components = 0.000372547 Jy ! Clean residual min=-0.001719 max=0.001515 Jy/beam ! Clean residual mean=0.000001 rms=0.000316 Jy/beam ! Combined flux in latest and established models = 0.119751 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 54 components and 0.119751 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.078705Jy sigma=0.670264 ! Fit after self-cal, rms=0.078703Jy sigma=0.670248 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 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 = 5.46711e-05 Jy ! Component: 100 - total flux cleaned = 7.2023e-05 Jy ! Component: 150 - total flux cleaned = 7.16356e-05 Jy ! Component: 200 - total flux cleaned = 5.61912e-05 Jy ! Total flux subtracted in 200 components = 5.61912e-05 Jy ! Clean residual min=-0.001715 max=0.001507 Jy/beam ! Clean residual mean=0.000001 rms=0.000315 Jy/beam ! Combined flux in latest and established models = 0.119807 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 56 components and 0.119807 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.078685Jy sigma=0.670125 ! Fit after self-cal, rms=0.078684Jy sigma=0.670118 ! Inverting map ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 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. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.078684Jy sigma=0.670118 ! Fit after self-cal, rms=0.078634Jy sigma=0.670104 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 milli-arcsec ! Estimated beam: bmin=0.6961 mas, bmaj=1.677 mas, bpa=-10.84 degrees ! Estimated noise=0.353978 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000195167 Jy ! Component: 100 - total flux cleaned = 0.000225621 Jy ! Component: 150 - total flux cleaned = 0.000225412 Jy ! Component: 200 - total flux cleaned = 0.000225324 Jy ! Total flux subtracted in 200 components = 0.000225324 Jy ! Clean residual min=-0.001713 max=0.001494 Jy/beam ! Clean residual mean=0.000001 rms=0.000315 Jy/beam ! Combined flux in latest and established models = 0.120032 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 58 components and 0.120032 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.078618Jy sigma=0.670003 ! Fit after self-cal, rms=0.078616Jy sigma=0.670001 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 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 = 3.5453e-05 Jy ! Component: 100 - total flux cleaned = 3.53436e-05 Jy ! Component: 150 - total flux cleaned = 2.21349e-05 Jy ! Component: 200 - total flux cleaned = 2.21766e-05 Jy ! Total flux subtracted in 200 components = 2.21766e-05 Jy ! Clean residual min=-0.001712 max=0.001485 Jy/beam ! Clean residual mean=0.000001 rms=0.000315 Jy/beam ! Combined flux in latest and established models = 0.120054 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 60 components and 0.120054 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.078605Jy sigma=0.669923 ! Fit after self-cal, rms=0.078605Jy sigma=0.669921 ! Inverting map ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 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. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.078605Jy sigma=0.669921 ! Fit after self-cal, rms=0.078558Jy sigma=0.669912 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 milli-arcsec ! Estimated beam: bmin=3.004 mas, bmaj=3.049 mas, bpa=-0.3493 degrees ! Estimated noise=0.42678 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -6.7572e-06 Jy ! Component: 100 - total flux cleaned = -1.51445e-05 Jy ! Component: 150 - total flux cleaned = -2.30784e-05 Jy ! Component: 200 - total flux cleaned = -2.36874e-05 Jy ! Total flux subtracted in 200 components = -2.36874e-05 Jy ! Clean residual min=-0.001565 max=0.001299 Jy/beam ! Clean residual mean=0.000001 rms=0.000364 Jy/beam ! Combined flux in latest and established models = 0.120031 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 68 components and 0.120031 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.078559Jy sigma=0.669914 ! Fit after self-cal, rms=0.078557Jy sigma=0.669906 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 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 = -1.62951e-06 Jy ! Component: 100 - total flux cleaned = -8.32781e-06 Jy ! Component: 150 - total flux cleaned = -1.45468e-05 Jy ! Component: 200 - total flux cleaned = -9.56752e-06 Jy ! Total flux subtracted in 200 components = -9.56752e-06 Jy ! Clean residual min=-0.001554 max=0.001288 Jy/beam ! Clean residual mean=0.000001 rms=0.000364 Jy/beam ! Combined flux in latest and established models = 0.120021 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 70 components and 0.120021 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.078558Jy sigma=0.669919 ! Fit after self-cal, rms=0.078558Jy sigma=0.669916 ! Inverting map ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 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 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 milli-arcsec ! Estimated beam: bmin=0.6958 mas, bmaj=1.677 mas, bpa=-10.85 degrees ! Estimated noise=0.354021 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6958 x 1.677 at -10.85 degrees (North through East) ! Clean map min=-0.0013623 max=0.10392 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 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 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 milli-arcsec ! Estimated beam: bmin=0.4981 mas, bmaj=1.349 mas, bpa=-11.71 degrees ! Estimated noise=0.802818 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0789315 Jy ! Component: 100 - total flux cleaned = 0.0978923 Jy ! Component: 150 - total flux cleaned = 0.106159 Jy ! Component: 200 - total flux cleaned = 0.110937 Jy ! Total flux subtracted in 200 components = 0.110937 Jy ! Clean residual min=-0.003441 max=0.003744 Jy/beam ! Clean residual mean=-0.000001 rms=0.000712 Jy/beam ! Combined flux in latest and established models = 0.110937 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 20 model components to the UV plane model. ! The established model now contains 20 components and 0.110937 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 milli-arcsec ! Estimated beam: bmin=0.6958 mas, bmaj=1.677 mas, bpa=-10.85 degrees ! Estimated noise=0.354021 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 = 0.00464468 Jy ! Component: 100 - total flux cleaned = 0.006959 Jy ! Component: 150 - total flux cleaned = 0.00781263 Jy ! Component: 200 - total flux cleaned = 0.0080895 Jy ! Total flux subtracted in 200 components = 0.0080895 Jy ! Clean residual min=-0.001691 max=0.001499 Jy/beam ! Clean residual mean=0.000001 rms=0.000321 Jy/beam ! Combined flux in latest and established models = 0.119027 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 43 components and 0.119027 Jy ! Inverting map ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 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 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 milli-arcsec ! Estimated beam: bmin=3.004 mas, bmaj=3.049 mas, bpa=-0.3493 degrees ! Estimated noise=0.42678 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000539254 Jy ! Component: 100 - total flux cleaned = 0.000694946 Jy ! Component: 150 - total flux cleaned = 0.000810832 Jy ! Component: 200 - total flux cleaned = 0.000810742 Jy ! Total flux subtracted in 200 components = 0.000810742 Jy ! Clean residual min=-0.001596 max=0.001287 Jy/beam ! Clean residual mean=0.000001 rms=0.000365 Jy/beam ! Combined flux in latest and established models = 0.119837 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 = 1.53054e-05 Jy ! Component: 100 - total flux cleaned = 1.52757e-05 Jy ! Component: 150 - total flux cleaned = 1.54438e-05 Jy ! Component: 200 - total flux cleaned = 1.56835e-05 Jy ! Total flux subtracted in 200 components = 1.56835e-05 Jy ! Clean residual min=-0.001570 max=0.001290 Jy/beam ! Clean residual mean=0.000001 rms=0.000364 Jy/beam ! Combined flux in latest and established models = 0.119853 Jy ! Adding 17 model components to the UV plane model. ! The established model now contains 55 components and 0.119853 Jy ! Inverting map ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 milli-arcsec ! Estimated beam: bmin=0.6958 mas, bmaj=1.677 mas, bpa=-10.85 degrees ! Estimated noise=0.354021 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -3.83825e-05 Jy ! Component: 100 - total flux cleaned = -6.5352e-05 Jy ! Component: 150 - total flux cleaned = -8.77636e-05 Jy ! Component: 200 - total flux cleaned = -6.73081e-05 Jy ! Total flux subtracted in 200 components = -6.73081e-05 Jy ! Clean residual min=-0.001748 max=0.001562 Jy/beam ! Clean residual mean=0.000001 rms=0.000316 Jy/beam ! Combined flux in latest and established models = 0.119786 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 64 components and 0.119786 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.078604Jy sigma=0.670233 ! Fit after self-cal, rms=0.078598Jy sigma=0.670194 wmodel /scr/pima/gb073_uvs/J1431+2442_X_map.mod ! Writing 64 model components to file: /scr/pima/gb073_uvs/J1431+2442_X_map.mod wobs /scr/pima/gb073_uvs/J1431+2442_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1431+2442_X_uvs.fits wwins /scr/pima/gb073_uvs/J1431+2442_X_map.win ! wwins: Wrote 2 windows to /scr/pima/gb073_uvs/J1431+2442_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 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000457033 Jy ! Component: 100 - total flux cleaned = -0.0008399 Jy ! Component: 150 - total flux cleaned = -0.00125285 Jy ! Component: 200 - total flux cleaned = -0.00159776 Jy ! Component: 250 - total flux cleaned = -0.00193026 Jy ! Component: 300 - total flux cleaned = -0.00218408 Jy ! Component: 350 - total flux cleaned = -0.0024544 Jy ! Component: 400 - total flux cleaned = -0.00262994 Jy ! Component: 450 - total flux cleaned = -0.00275937 Jy ! Component: 500 - total flux cleaned = -0.0029707 Jy ! Component: 550 - total flux cleaned = -0.00315737 Jy ! Component: 600 - total flux cleaned = -0.00334132 Jy ! Component: 650 - total flux cleaned = -0.00348258 Jy ! Component: 700 - total flux cleaned = -0.00366161 Jy ! Component: 750 - total flux cleaned = -0.0038187 Jy ! Component: 800 - total flux cleaned = -0.00395517 Jy ! Component: 850 - total flux cleaned = -0.0041476 Jy ! Component: 900 - total flux cleaned = -0.00429995 Jy ! Component: 950 - total flux cleaned = -0.00445067 Jy ! Component: 1000 - total flux cleaned = -0.00461885 Jy ! Component: 1050 - total flux cleaned = -0.00478519 Jy ! Component: 1100 - total flux cleaned = -0.00498685 Jy ! Component: 1150 - total flux cleaned = -0.00504146 Jy ! Component: 1200 - total flux cleaned = -0.00515 Jy ! Component: 1250 - total flux cleaned = -0.00525778 Jy ! Component: 1300 - total flux cleaned = -0.00543582 Jy ! Component: 1350 - total flux cleaned = -0.00555938 Jy ! Component: 1400 - total flux cleaned = -0.00564724 Jy ! Component: 1450 - total flux cleaned = -0.00575191 Jy ! Component: 1500 - total flux cleaned = -0.00592523 Jy ! Component: 1550 - total flux cleaned = -0.00601128 Jy ! Component: 1600 - total flux cleaned = -0.00614814 Jy ! Component: 1650 - total flux cleaned = -0.00621619 Jy ! Component: 1700 - total flux cleaned = -0.00631755 Jy ! Component: 1750 - total flux cleaned = -0.00638476 Jy ! Component: 1800 - total flux cleaned = -0.00645141 Jy ! Component: 1850 - total flux cleaned = -0.00651784 Jy ! Component: 1900 - total flux cleaned = -0.00658354 Jy ! Component: 1950 - total flux cleaned = -0.00666558 Jy ! Component: 2000 - total flux cleaned = -0.00669816 Jy ! Component: 2050 - total flux cleaned = -0.00684386 Jy ! Component: 2100 - total flux cleaned = -0.00690828 Jy ! Component: 2150 - total flux cleaned = -0.00695628 Jy ! Component: 2200 - total flux cleaned = -0.00697214 Jy ! Component: 2250 - total flux cleaned = -0.00700388 Jy ! Component: 2300 - total flux cleaned = -0.00706689 Jy ! Component: 2350 - total flux cleaned = -0.00717676 Jy ! Component: 2400 - total flux cleaned = -0.00714563 Jy ! Component: 2450 - total flux cleaned = -0.00720788 Jy ! Component: 2500 - total flux cleaned = -0.00725429 Jy ! Component: 2550 - total flux cleaned = -0.00726966 Jy ! Component: 2600 - total flux cleaned = -0.00733094 Jy ! Component: 2650 - total flux cleaned = -0.00739163 Jy ! Component: 2700 - total flux cleaned = -0.00739147 Jy ! Component: 2750 - total flux cleaned = -0.00743657 Jy ! Component: 2800 - total flux cleaned = -0.00746666 Jy ! Component: 2850 - total flux cleaned = -0.00748163 Jy ! Component: 2900 - total flux cleaned = -0.00746684 Jy ! Component: 2950 - total flux cleaned = -0.0075853 Jy ! Component: 3000 - total flux cleaned = -0.00754115 Jy ! Component: 3050 - total flux cleaned = -0.00759988 Jy ! Component: 3100 - total flux cleaned = -0.00767284 Jy ! Component: 3150 - total flux cleaned = -0.00765823 Jy ! Component: 3200 - total flux cleaned = -0.0076727 Jy ! Component: 3250 - total flux cleaned = -0.0077591 Jy ! Component: 3300 - total flux cleaned = -0.00774465 Jy ! Component: 3350 - total flux cleaned = -0.00771616 Jy ! Component: 3400 - total flux cleaned = -0.00775902 Jy ! Component: 3450 - total flux cleaned = -0.0078441 Jy ! Component: 3500 - total flux cleaned = -0.00790065 Jy ! Component: 3550 - total flux cleaned = -0.00795684 Jy ! Component: 3600 - total flux cleaned = -0.0079847 Jy ! Component: 3650 - total flux cleaned = -0.00802652 Jy ! Component: 3700 - total flux cleaned = -0.00808205 Jy ! Component: 3750 - total flux cleaned = -0.00809573 Jy ! Component: 3800 - total flux cleaned = -0.00810953 Jy ! Component: 3850 - total flux cleaned = -0.00806839 Jy ! Component: 3900 - total flux cleaned = -0.00815046 Jy ! Component: 3950 - total flux cleaned = -0.00815046 Jy ! Component: 4000 - total flux cleaned = -0.00816406 Jy ! Component: 4050 - total flux cleaned = -0.00817765 Jy ! Total flux subtracted in 4096 components = -0.00816417 Jy ! Clean residual min=-0.000673 max=0.000699 Jy/beam ! Clean residual mean=-0.000000 rms=0.000225 Jy/beam ! Combined flux in latest and established models = 0.111622 Jy keep ! Adding 305 model components to the UV plane model. ! The established model now contains 369 components and 0.111622 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1431+2442_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6958 x 1.677 at -10.85 degrees (North through East) ! Clean map min=-0.0015683 max=0.1037 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1431+2442_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.103699 invert ! Inverting map ! Your choice of large map pixels excluded 4.62% of the data. ! The x-axis pixel size should ideally be below 0.1769 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000224913 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.650672 0.650672 1.30134 2.60269 5.20538 10.4108 20.8215 41.643 83.286 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0006 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.103 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 461.061 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1431+2442_X_uvs.log closed on Sat Dec 26 09:40:43 2015