! Started logfile: /scr/pima/gb073_uvs/J1221+3010_X_uvs.log on Sat Dec 26 09:38:15 2015 obs /scr/pima/gb073_uvs/J1221+3010_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1221+3010_X_uva.fits ! AN table 1: 29 integrations on 36 of 36 possible baselines. ! AN table 2: 29 integrations on 55 of 55 possible baselines. ! AN table 3: 29 integrations on 45 of 45 possible baselines. ! AN table 4: 29 integrations on 36 of 36 possible baselines. ! AN table 5: 29 integrations on 36 of 36 possible baselines. ! Apparent sampling: 0.838362 visibilities/baseline/integration-bin. ! Found source: J1221+3010 ! ! 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 40456 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/J1221+3010_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 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 5. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 87 telescope corrections were flagged in sub-array 4. ! A total of 58 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 6. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 87 telescope corrections were flagged in sub-array 4. ! A total of 58 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 7. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 8. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=1.002877Jy sigma=10.883238 ! Fit after self-cal, rms=0.955530Jy sigma=10.431218 ! 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 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 milli-arcsec ! Estimated beam: bmin=0.546 mas, bmaj=1.195 mas, bpa=-9.068 degrees ! Estimated noise=0.882516 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 = 0.0349237 Jy ! Component: 100 - total flux cleaned = 0.0425488 Jy ! Total flux subtracted in 100 components = 0.0425488 Jy ! Clean residual min=-0.003257 max=0.003121 Jy/beam ! Clean residual mean=-0.000002 rms=0.000605 Jy/beam ! Combined flux in latest and established models = 0.0425488 Jy ! Performing phase self-cal ! Adding 3 model components to the UV plane model. ! The established model now contains 3 components and 0.0425488 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=0.068361Jy sigma=0.667790 ! Fit after self-cal, rms=0.066889Jy sigma=0.651153 ! Inverting map ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00379687 Jy ! Component: 100 - total flux cleaned = 0.00431108 Jy ! Total flux subtracted in 100 components = 0.00431108 Jy ! Clean residual min=-0.002699 max=0.002790 Jy/beam ! Clean residual mean=-0.000002 rms=0.000584 Jy/beam ! Combined flux in latest and established models = 0.0468599 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 8 components and 0.0468599 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=0.066593Jy sigma=0.648640 ! Fit after self-cal, rms=0.066592Jy sigma=0.648628 ! Inverting map ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 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 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 milli-arcsec ! Estimated beam: bmin=0.7803 mas, bmaj=1.557 mas, bpa=-4.281 degrees ! Estimated noise=0.368653 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (1, 0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00297132 Jy ! Component: 100 - total flux cleaned = 0.00457089 Jy ! Component: 150 - total flux cleaned = 0.00560118 Jy ! Component: 200 - total flux cleaned = 0.00629581 Jy ! Total flux subtracted in 200 components = 0.00629581 Jy ! Clean residual min=-0.001320 max=0.001497 Jy/beam ! Clean residual mean=-0.000005 rms=0.000341 Jy/beam ! Combined flux in latest and established models = 0.0531557 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 23 components and 0.0531557 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=0.066444Jy sigma=0.647176 ! Fit after self-cal, rms=0.066423Jy sigma=0.646775 ! Inverting map ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7803 x 1.557 at -4.281 degrees (North through East) ! Clean map min=-0.0012451 max=0.04708 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* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 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* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 EF 1.00* FD 0.97 KP 1.02 ! LA 1.01 NL 0.99 ON 0.84 OV 1.02 ! PT 1.00 SC 1.02 ZC 0.92 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.95 FD 1.07 KP 0.99 LA 1.05 ! MK 1.17 NL 1.06 ON 1.00* PT 1.00 ! SC 0.96 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 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* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.15 FD 0.94 KP 0.96 LA 0.97 ! MK 1.13 NL 1.03 ON 1.00* PT 1.05 ! SC 1.05 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.07 FD 0.98 KP 0.91 LA 0.99 ! MK 1.16 NL 1.13 OV 1.12 PT 0.98 ! SC 1.02 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 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* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.96 FD 0.99 KP 1.02 LA 0.90 ! MK 1.18 NL 1.04 ON 1.00* PT 1.02 ! SC 1.15 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.06 KP 0.94 LA 0.94 ! MK 1.08 NL 1.12 OV 1.12 PT 0.93 ! SC 0.92 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 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* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 0.87 KP 1.00 LA 0.90 ! MK 1.02 NL 1.05 ON 1.00* PT 1.00 ! SC 1.04 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 0.90 KP 0.90 ! LA 1.01 NL 1.17 ON 0.84 OV 1.05 ! PT 0.86 SC 0.91 ZC 1.15 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.09 KP 0.98 ! LA 1.18 NL 1.02 ON 1.00* PT 0.91 ! SC 0.97 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 1.05 KP 0.94 LA 0.88 ! MK 1.15 NL 1.02 ON 1.00* PT 0.98 ! SC 0.97 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 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* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.95 FD 1.10 KP 0.93 LA 1.01 ! MK 1.14 NL 1.15 ON 1.00* PT 0.99 ! SC 1.00 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 1.06 KP 0.91 LA 0.96 ! MK 1.14 NL 1.10 OV 1.03 PT 0.98 ! SC 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.87 EF 1.00* FD 0.91 KP 0.87 ! LA 1.00 NL 1.07 ON 1.02 OV 1.01 ! PT 0.98 SC 1.05 ZC 0.88 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 FD 0.91 KP 0.93 LA 1.04 ! MK 1.10 NL 1.10 ON 1.00* PT 0.90 ! SC 1.05 ! ! ! Fit before self-cal, rms=0.066423Jy sigma=0.646775 ! Fit after self-cal, rms=0.066552Jy sigma=0.645948 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 milli-arcsec ! Estimated beam: bmin=0.7841 mas, bmaj=1.554 mas, bpa=-4.338 degrees ! Estimated noise=0.370421 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 = 0.00101016 Jy ! Component: 100 - total flux cleaned = 0.00121267 Jy ! Component: 150 - total flux cleaned = 0.00127982 Jy ! Component: 200 - total flux cleaned = 0.00129329 Jy ! Total flux subtracted in 200 components = 0.00129329 Jy ! Clean residual min=-0.001273 max=0.001334 Jy/beam ! Clean residual mean=-0.000005 rms=0.000311 Jy/beam ! Combined flux in latest and established models = 0.054449 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 34 components and 0.054449 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=0.066534Jy sigma=0.645796 ! Fit after self-cal, rms=0.066561Jy sigma=0.645589 ! Inverting map ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 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=0.066561Jy sigma=0.645589 ! Fit after self-cal, rms=0.066748Jy sigma=0.645563 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 milli-arcsec ! Estimated beam: bmin=0.784 mas, bmaj=1.552 mas, bpa=-4.325 degrees ! Estimated noise=0.371074 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000547571 Jy ! Component: 100 - total flux cleaned = 0.000613404 Jy ! Component: 150 - total flux cleaned = 0.000612733 Jy ! Component: 200 - total flux cleaned = 0.000648184 Jy ! Total flux subtracted in 200 components = 0.000648184 Jy ! Clean residual min=-0.001264 max=0.001361 Jy/beam ! Clean residual mean=-0.000005 rms=0.000309 Jy/beam ! Combined flux in latest and established models = 0.0550972 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 37 components and 0.0550972 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=0.066741Jy sigma=0.645497 ! Fit after self-cal, rms=0.066749Jy sigma=0.645470 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 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 (-40.4, 42). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00111953 Jy ! Component: 100 - total flux cleaned = 0.00136274 Jy ! Component: 150 - total flux cleaned = 0.00147013 Jy ! Component: 200 - total flux cleaned = 0.00151726 Jy ! Total flux subtracted in 200 components = 0.00151726 Jy ! Clean residual min=-0.001242 max=0.001213 Jy/beam ! Clean residual mean=-0.000005 rms=0.000301 Jy/beam ! Combined flux in latest and established models = 0.0566144 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 49 components and 0.0566144 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=0.066730Jy sigma=0.645254 ! Fit after self-cal, rms=0.066725Jy sigma=0.645196 ! Inverting map ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 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=0.066725Jy sigma=0.645196 ! Fit after self-cal, rms=0.066717Jy sigma=0.645144 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 milli-arcsec ! Estimated beam: bmin=0.7829 mas, bmaj=1.55 mas, bpa=-4.292 degrees ! Estimated noise=0.371357 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000652644 Jy ! Component: 100 - total flux cleaned = 0.000803541 Jy ! Component: 150 - total flux cleaned = 0.000832468 Jy ! Component: 200 - total flux cleaned = 0.000832297 Jy ! Total flux subtracted in 200 components = 0.000832297 Jy ! Clean residual min=-0.001258 max=0.001194 Jy/beam ! Clean residual mean=-0.000005 rms=0.000298 Jy/beam ! Combined flux in latest and established models = 0.0574467 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 52 components and 0.0574467 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=0.066708Jy sigma=0.645067 ! Fit after self-cal, rms=0.066705Jy sigma=0.645044 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 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 = 0.000265206 Jy ! Component: 100 - total flux cleaned = 0.000293184 Jy ! Component: 150 - total flux cleaned = 0.000280667 Jy ! Component: 200 - total flux cleaned = 0.00026894 Jy ! Total flux subtracted in 200 components = 0.00026894 Jy ! Clean residual min=-0.001248 max=0.001183 Jy/beam ! Clean residual mean=-0.000005 rms=0.000298 Jy/beam ! Combined flux in latest and established models = 0.0577157 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 54 components and 0.0577157 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=0.066701Jy sigma=0.644997 ! Fit after self-cal, rms=0.066700Jy sigma=0.644992 ! Inverting map ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 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=0.066700Jy sigma=0.644992 ! Fit after self-cal, rms=0.066806Jy sigma=0.644829 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 milli-arcsec ! Estimated beam: bmin=2.658 mas, bmaj=3.006 mas, bpa=-1.799 degrees ! Estimated noise=0.460203 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000355516 Jy ! Component: 100 - total flux cleaned = 0.000467143 Jy ! Component: 150 - total flux cleaned = 0.000555021 Jy ! Component: 200 - total flux cleaned = 0.000618745 Jy ! Total flux subtracted in 200 components = 0.000618745 Jy ! Clean residual min=-0.001643 max=0.001310 Jy/beam ! Clean residual mean=-0.000010 rms=0.000428 Jy/beam ! Combined flux in latest and established models = 0.0583344 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 64 components and 0.0583344 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=0.066805Jy sigma=0.644820 ! Fit after self-cal, rms=0.066805Jy sigma=0.644806 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 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 = 0.000145907 Jy ! Component: 100 - total flux cleaned = 0.000198365 Jy ! Component: 150 - total flux cleaned = 0.000209665 Jy ! Component: 200 - total flux cleaned = 0.000209793 Jy ! Total flux subtracted in 200 components = 0.000209793 Jy ! Clean residual min=-0.001629 max=0.001306 Jy/beam ! Clean residual mean=-0.000010 rms=0.000427 Jy/beam ! Combined flux in latest and established models = 0.0585442 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 68 components and 0.0585442 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=0.066806Jy sigma=0.644804 ! Fit after self-cal, rms=0.066806Jy sigma=0.644802 ! Inverting map ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 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 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 milli-arcsec ! Estimated beam: bmin=0.7819 mas, bmaj=1.548 mas, bpa=-4.245 degrees ! Estimated noise=0.372826 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7819 x 1.548 at -4.245 degrees (North through East) ! Clean map min=-0.0011795 max=0.046932 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 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 milli-arcsec ! Estimated beam: bmin=0.545 mas, bmaj=1.186 mas, bpa=-9.208 degrees ! Estimated noise=0.892621 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0371374 Jy ! Component: 100 - total flux cleaned = 0.0459671 Jy ! Component: 150 - total flux cleaned = 0.049984 Jy ! Component: 200 - total flux cleaned = 0.0519778 Jy ! Total flux subtracted in 200 components = 0.0519778 Jy ! Clean residual min=-0.002665 max=0.002415 Jy/beam ! Clean residual mean=-0.000002 rms=0.000557 Jy/beam ! Combined flux in latest and established models = 0.0519778 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 10 model components to the UV plane model. ! The established model now contains 10 components and 0.0519778 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 milli-arcsec ! Estimated beam: bmin=0.7819 mas, bmaj=1.548 mas, bpa=-4.245 degrees ! Estimated noise=0.372826 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 = 0.00210901 Jy ! Component: 100 - total flux cleaned = 0.00343147 Jy ! Component: 150 - total flux cleaned = 0.00438768 Jy ! Component: 200 - total flux cleaned = 0.00507042 Jy ! Total flux subtracted in 200 components = 0.00507042 Jy ! Clean residual min=-0.001256 max=0.001193 Jy/beam ! Clean residual mean=-0.000005 rms=0.000307 Jy/beam ! Combined flux in latest and established models = 0.0570482 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 32 components and 0.0570482 Jy ! Inverting map ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 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 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 milli-arcsec ! Estimated beam: bmin=2.658 mas, bmaj=3.006 mas, bpa=-1.799 degrees ! Estimated noise=0.460203 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000806015 Jy ! Component: 100 - total flux cleaned = 0.00120966 Jy ! Component: 150 - total flux cleaned = 0.00128678 Jy ! Component: 200 - total flux cleaned = 0.00130806 Jy ! Total flux subtracted in 200 components = 0.00130806 Jy ! Clean residual min=-0.001665 max=0.001345 Jy/beam ! Clean residual mean=-0.000010 rms=0.000432 Jy/beam ! Combined flux in latest and established models = 0.0583563 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 = 1.94061e-05 Jy ! Component: 100 - total flux cleaned = 3.69413e-05 Jy ! Component: 150 - total flux cleaned = 3.73615e-05 Jy ! Component: 200 - total flux cleaned = 4.48523e-05 Jy ! Total flux subtracted in 200 components = 4.48523e-05 Jy ! Clean residual min=-0.001649 max=0.001334 Jy/beam ! Clean residual mean=-0.000010 rms=0.000429 Jy/beam ! Combined flux in latest and established models = 0.0584011 Jy ! Adding 21 model components to the UV plane model. ! The established model now contains 51 components and 0.0584011 Jy ! Inverting map ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 milli-arcsec ! Estimated beam: bmin=0.7819 mas, bmaj=1.548 mas, bpa=-4.245 degrees ! Estimated noise=0.372826 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000235195 Jy ! Component: 100 - total flux cleaned = -0.000161358 Jy ! Component: 150 - total flux cleaned = -9.61377e-05 Jy ! Component: 200 - total flux cleaned = -6.60517e-05 Jy ! Total flux subtracted in 200 components = -6.60517e-05 Jy ! Clean residual min=-0.001243 max=0.001134 Jy/beam ! Clean residual mean=-0.000005 rms=0.000297 Jy/beam ! Combined flux in latest and established models = 0.0583351 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 64 components and 0.0583351 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=0.066817Jy sigma=0.644858 ! Fit after self-cal, rms=0.066813Jy sigma=0.644822 wmodel /scr/pima/gb073_uvs/J1221+3010_X_map.mod ! Writing 64 model components to file: /scr/pima/gb073_uvs/J1221+3010_X_map.mod wobs /scr/pima/gb073_uvs/J1221+3010_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1221+3010_X_uvs.fits wwins /scr/pima/gb073_uvs/J1221+3010_X_map.win ! wwins: Wrote 3 windows to /scr/pima/gb073_uvs/J1221+3010_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 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000542146 Jy ! Component: 100 - total flux cleaned = -0.000857627 Jy ! Component: 150 - total flux cleaned = -0.00114211 Jy ! Component: 200 - total flux cleaned = -0.00134008 Jy ! Component: 250 - total flux cleaned = -0.00151438 Jy ! Component: 300 - total flux cleaned = -0.00170363 Jy ! Component: 350 - total flux cleaned = -0.00190765 Jy ! Component: 400 - total flux cleaned = -0.00210795 Jy ! Component: 450 - total flux cleaned = -0.00226911 Jy ! Component: 500 - total flux cleaned = -0.00242777 Jy ! Component: 550 - total flux cleaned = -0.00261813 Jy ! Component: 600 - total flux cleaned = -0.0027202 Jy ! Component: 650 - total flux cleaned = -0.00283791 Jy ! Component: 700 - total flux cleaned = -0.00297069 Jy ! Component: 750 - total flux cleaned = -0.00313478 Jy ! Component: 800 - total flux cleaned = -0.00318353 Jy ! Component: 850 - total flux cleaned = -0.00334408 Jy ! Component: 900 - total flux cleaned = -0.00348653 Jy ! Component: 950 - total flux cleaned = -0.00353358 Jy ! Component: 1000 - total flux cleaned = -0.00368845 Jy ! Component: 1050 - total flux cleaned = -0.00374952 Jy ! Component: 1100 - total flux cleaned = -0.00391622 Jy ! Component: 1150 - total flux cleaned = -0.00394596 Jy ! Component: 1200 - total flux cleaned = -0.00403495 Jy ! Component: 1250 - total flux cleaned = -0.00407902 Jy ! Component: 1300 - total flux cleaned = -0.00418092 Jy ! Component: 1350 - total flux cleaned = -0.00426733 Jy ! Component: 1400 - total flux cleaned = -0.00439573 Jy ! Component: 1450 - total flux cleaned = -0.00445227 Jy ! Component: 1500 - total flux cleaned = -0.00449451 Jy ! Component: 1550 - total flux cleaned = -0.00466184 Jy ! Component: 1600 - total flux cleaned = -0.00474494 Jy ! Component: 1650 - total flux cleaned = -0.00484087 Jy ! Component: 1700 - total flux cleaned = -0.00493621 Jy ! Component: 1750 - total flux cleaned = -0.00509793 Jy ! Component: 1800 - total flux cleaned = -0.00515145 Jy ! Component: 1850 - total flux cleaned = -0.00523117 Jy ! Component: 1900 - total flux cleaned = -0.00528394 Jy ! Component: 1950 - total flux cleaned = -0.00538859 Jy ! Component: 2000 - total flux cleaned = -0.00544056 Jy ! Component: 2050 - total flux cleaned = -0.00546639 Jy ! Component: 2100 - total flux cleaned = -0.00560732 Jy ! Component: 2150 - total flux cleaned = -0.00563273 Jy ! Component: 2200 - total flux cleaned = -0.0056329 Jy ! Component: 2250 - total flux cleaned = -0.00569574 Jy ! Component: 2300 - total flux cleaned = -0.00577065 Jy ! Component: 2350 - total flux cleaned = -0.00580795 Jy ! Component: 2400 - total flux cleaned = -0.00591895 Jy ! Component: 2450 - total flux cleaned = -0.00600455 Jy ! Component: 2500 - total flux cleaned = -0.00605301 Jy ! Component: 2550 - total flux cleaned = -0.00616175 Jy ! Component: 2600 - total flux cleaned = -0.00620967 Jy ! Component: 2650 - total flux cleaned = -0.00624549 Jy ! Component: 2700 - total flux cleaned = -0.00632849 Jy ! Component: 2750 - total flux cleaned = -0.00641102 Jy ! Component: 2800 - total flux cleaned = -0.006411 Jy ! Component: 2850 - total flux cleaned = -0.00642262 Jy ! Component: 2900 - total flux cleaned = -0.00648065 Jy ! Component: 2950 - total flux cleaned = -0.00650361 Jy ! Component: 3000 - total flux cleaned = -0.00654942 Jy ! Component: 3050 - total flux cleaned = -0.00658349 Jy ! Component: 3100 - total flux cleaned = -0.00658345 Jy ! Component: 3150 - total flux cleaned = -0.00657227 Jy ! Component: 3200 - total flux cleaned = -0.00662831 Jy ! Component: 3250 - total flux cleaned = -0.00663941 Jy ! Component: 3300 - total flux cleaned = -0.00663937 Jy ! Component: 3350 - total flux cleaned = -0.00666135 Jy ! Component: 3400 - total flux cleaned = -0.00665035 Jy ! Component: 3450 - total flux cleaned = -0.00671587 Jy ! Component: 3500 - total flux cleaned = -0.00674841 Jy ! Component: 3550 - total flux cleaned = -0.00670525 Jy ! Component: 3600 - total flux cleaned = -0.00678038 Jy ! Component: 3650 - total flux cleaned = -0.00679104 Jy ! Component: 3700 - total flux cleaned = -0.00681232 Jy ! Component: 3750 - total flux cleaned = -0.00680185 Jy ! Component: 3800 - total flux cleaned = -0.00685438 Jy ! Component: 3850 - total flux cleaned = -0.00685435 Jy ! Component: 3900 - total flux cleaned = -0.00692743 Jy ! Component: 3950 - total flux cleaned = -0.00696886 Jy ! Component: 4000 - total flux cleaned = -0.00690691 Jy ! Component: 4050 - total flux cleaned = -0.00697882 Jy ! Total flux subtracted in 4096 components = -0.00702997 Jy ! Clean residual min=-0.000536 max=0.000772 Jy/beam ! Clean residual mean=-0.000001 rms=0.000174 Jy/beam ! Combined flux in latest and established models = 0.0513051 Jy keep ! Adding 334 model components to the UV plane model. ! The established model now contains 398 components and 0.0513051 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1221+3010_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7819 x 1.548 at -4.245 degrees (North through East) ! Clean map min=-0.00083691 max=0.046742 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1221+3010_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0467417 invert ! Inverting map ! Your choice of large map pixels excluded 2.4% of the data. ! The x-axis pixel size should ideally be below 0.1867 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000174792 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.12186 1.12186 2.24372 4.48745 8.97489 17.9498 35.8996 71.7991 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0005 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.046 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 267.412 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1221+3010_X_uvs.log closed on Sat Dec 26 09:38:20 2015