! Started logfile: /scr/pima/gb073_uvs/J1247+3209_X_uvs.log on Sat Dec 26 09:38:59 2015 obs /scr/pima/gb073_uvs/J1247+3209_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1247+3209_X_uva.fits ! AN table 1: 29 integrations on 45 of 45 possible baselines. ! AN table 2: 29 integrations on 45 of 45 possible baselines. ! AN table 3: 29 integrations on 36 of 36 possible baselines. ! AN table 4: 29 integrations on 28 of 28 possible baselines. ! Apparent sampling: 0.918495 visibilities/baseline/integration-bin. ! Found source: J1247+3209 ! ! 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 32816 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/J1247+3209_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 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 30 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 30 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 30 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 30 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 5. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 30 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 6. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 30 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 7. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 30 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 8. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 30 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=1.004078Jy sigma=10.555826 ! Fit after self-cal, rms=0.949989Jy sigma=10.000262 ! 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 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec ! Estimated beam: bmin=0.5351 mas, bmaj=1.208 mas, bpa=-5.125 degrees ! Estimated noise=0.935489 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 = 0.0408677 Jy ! Component: 100 - total flux cleaned = 0.0497796 Jy ! Total flux subtracted in 100 components = 0.0497796 Jy ! Clean residual min=-0.002777 max=0.002954 Jy/beam ! Clean residual mean=-0.000001 rms=0.000670 Jy/beam ! Combined flux in latest and established models = 0.0497796 Jy ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 0.0497796 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=0.073567Jy sigma=0.678979 ! Fit after self-cal, rms=0.072011Jy sigma=0.659330 ! Inverting map ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00361426 Jy ! Component: 100 - total flux cleaned = 0.00434123 Jy ! Total flux subtracted in 100 components = 0.00434123 Jy ! Clean residual min=-0.002818 max=0.003235 Jy/beam ! Clean residual mean=-0.000001 rms=0.000669 Jy/beam ! Combined flux in latest and established models = 0.0541208 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.0541208 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=0.071827Jy sigma=0.657974 ! Fit after self-cal, rms=0.071817Jy sigma=0.657896 ! Inverting map ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 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 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec ! Estimated beam: bmin=0.7278 mas, bmaj=1.542 mas, bpa=-1.948 degrees ! Estimated noise=0.416271 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 (4.6, 4.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00410235 Jy ! Component: 100 - total flux cleaned = 0.00574744 Jy ! Component: 150 - total flux cleaned = 0.00671944 Jy ! Component: 200 - total flux cleaned = 0.00743709 Jy ! Total flux subtracted in 200 components = 0.00743709 Jy ! Clean residual min=-0.001246 max=0.001267 Jy/beam ! Clean residual mean=-0.000001 rms=0.000310 Jy/beam ! Combined flux in latest and established models = 0.0615579 Jy ! Performing phase self-cal ! Adding 37 model components to the UV plane model. ! The established model now contains 41 components and 0.0615579 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=0.071638Jy sigma=0.655172 ! Fit after self-cal, rms=0.071567Jy sigma=0.654515 ! Inverting map ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7278 x 1.542 at -1.948 degrees (North through East) ! Clean map min=-0.0011457 max=0.054011 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 0.96 EF 1.00* FD 0.88 KP 1.17 ! LA 1.04 MK 1.03 NL 1.03 OV 1.05 ! PT 0.93 SC 0.91 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 EF 1.00* FD 1.06 KP 1.04 ! LA 1.13 NL 0.91 ON 0.92 OV 1.00 ! PT 0.95 SC 0.95 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* FD 1.00* LA 1.00* MC 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* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* PT 1.00* SC 1.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.12 EF 1.00* FD 1.06 KP 1.03 ! LA 1.12 MK 0.97 NL 1.10 OV 1.05 ! PT 1.02 SC 0.87 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 EF 1.00* FD 1.07 KP 1.05 ! LA 1.07 NL 0.95 ON 0.88 OV 0.97 ! PT 1.07 SC 1.06 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* FD 1.00* LA 1.00* MC 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 FD 1.11 KP 0.98 LA 1.16 ! MK 1.01 NL 0.95 PT 1.00 SC 1.16 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 EF 1.00* FD 0.99 KP 1.03 ! LA 1.01 MK 1.05 NL 0.98 OV 0.88 ! PT 0.95 SC 0.94 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 EF 1.00* FD 0.93 KP 1.04 ! LA 1.05 NL 0.96 ON 0.91 OV 0.95 ! PT 0.95 SC 1.05 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* FD 1.00* LA 1.00* MC 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 1.01 FD 1.00 KP 0.95 LA 0.92 ! MK 1.04 NL 0.90 PT 1.10 SC 1.08 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 EF 1.00* FD 1.06 KP 0.94 ! LA 1.02 MK 1.00 NL 1.04 OV 1.01 ! PT 1.03 SC 1.01 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.92 EF 1.00* FD 1.16 KP 1.08 ! LA 1.02 NL 1.02 ON 1.03 OV 1.07 ! PT 1.01 SC 1.03 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* FD 1.00* LA 1.00* MC 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 0.97 FD 0.98 KP 0.94 LA 1.09 ! MK 0.95 NL 1.00 PT 1.03 SC 1.04 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.97 KP 0.92 ! LA 0.98 MK 1.07 NL 0.98 OV 0.99 ! PT 0.93 SC 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.03 KP 0.96 ! LA 0.85 NL 1.10 ON 1.17 OV 1.04 ! PT 0.95 SC 1.08 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* FD 1.00* LA 1.00* MC 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* FD 0.97 KP 0.93 LA 1.04 ! MK 1.15 NL 1.04 PT 0.91 SC 0.92 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.06 KP 0.91 ! LA 1.03 MK 1.10 NL 1.12 OV 1.05 ! PT 0.90 SC 0.86 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.02 KP 0.90 ! LA 1.03 NL 1.02 ON 1.07 OV 0.95 ! PT 0.95 SC 0.88 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* FD 1.17 LA 0.96 MC 0.95 ! NL 1.01 ON 1.05 PT 1.03 SC 0.86 ! ZC 0.85 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 0.98 KP 0.87 LA 0.87 ! MK 1.02 NL 1.08 PT 0.91 SC 1.04 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 0.94 EF 1.00* FD 0.90 KP 0.93 ! LA 1.15 MK 1.12 NL 1.00 OV 0.95 ! PT 0.99 SC 0.96 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 EF 1.00* FD 1.06 KP 1.00 ! LA 0.95 NL 1.04 ON 1.04 OV 1.04 ! PT 0.95 SC 1.00 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* FD 1.08 LA 1.13 MC 0.97 ! NL 0.88 ON 0.97 PT 1.01 SC 0.98 ! ZC 0.86 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* PT 1.00* SC 1.00* ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 0.94 EF 1.00* FD 0.97 KP 0.92 ! LA 1.13 MK 1.08 NL 1.00 OV 0.96 ! PT 0.92 SC 0.89 ! ! 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* ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* FD 1.00* LA 1.00* MC 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 0.98 FD 1.02 KP 0.98 LA 0.98 ! MK 1.08 NL 1.01 PT 1.03 SC 0.98 ! ! ! Fit before self-cal, rms=0.071567Jy sigma=0.654515 ! Fit after self-cal, rms=0.070974Jy sigma=0.652730 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec ! Estimated beam: bmin=0.7271 mas, bmaj=1.534 mas, bpa=-1.921 degrees ! Estimated noise=0.416264 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 = 0.00142499 Jy ! Component: 100 - total flux cleaned = 0.00219057 Jy ! Component: 150 - total flux cleaned = 0.00273955 Jy ! Component: 200 - total flux cleaned = 0.00301889 Jy ! Total flux subtracted in 200 components = 0.00301889 Jy ! Clean residual min=-0.001110 max=0.001351 Jy/beam ! Clean residual mean=-0.000000 rms=0.000273 Jy/beam ! Combined flux in latest and established models = 0.0645768 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 53 components and 0.0645768 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=0.070943Jy sigma=0.652388 ! Fit after self-cal, rms=0.070957Jy sigma=0.652110 ! Inverting map ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 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=0.070957Jy sigma=0.652110 ! Fit after self-cal, rms=0.071155Jy sigma=0.652064 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec ! Estimated beam: bmin=0.7261 mas, bmaj=1.531 mas, bpa=-1.914 degrees ! Estimated noise=0.417625 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000787023 Jy ! Component: 100 - total flux cleaned = 0.0012747 Jy ! Component: 150 - total flux cleaned = 0.00141999 Jy ! Component: 200 - total flux cleaned = 0.00147646 Jy ! Total flux subtracted in 200 components = 0.00147646 Jy ! Clean residual min=-0.001121 max=0.001336 Jy/beam ! Clean residual mean=-0.000000 rms=0.000270 Jy/beam ! Combined flux in latest and established models = 0.0660532 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 57 components and 0.0660532 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=0.071143Jy sigma=0.651963 ! Fit after self-cal, rms=0.071143Jy sigma=0.651935 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 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 (-2.8, 23.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00108248 Jy ! Component: 100 - total flux cleaned = 0.00139189 Jy ! Component: 150 - total flux cleaned = 0.00149664 Jy ! Component: 200 - total flux cleaned = 0.00157541 Jy ! Total flux subtracted in 200 components = 0.00157541 Jy ! Clean residual min=-0.001163 max=0.001172 Jy/beam ! Clean residual mean=-0.000001 rms=0.000263 Jy/beam ! Combined flux in latest and established models = 0.0676286 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 65 components and 0.0676286 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=0.071122Jy sigma=0.651751 ! Fit after self-cal, rms=0.071112Jy sigma=0.651692 ! Inverting map ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec ! Added new window around map position (24.8, 50). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00100896 Jy ! Component: 100 - total flux cleaned = 0.00128999 Jy ! Component: 150 - total flux cleaned = 0.00134613 Jy ! Component: 200 - total flux cleaned = 0.00139693 Jy ! Total flux subtracted in 200 components = 0.00139693 Jy ! Clean residual min=-0.001132 max=0.001047 Jy/beam ! Clean residual mean=-0.000001 rms=0.000260 Jy/beam ! Combined flux in latest and established models = 0.0690255 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 75 components and 0.0690255 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=0.071092Jy sigma=0.651538 ! Fit after self-cal, rms=0.071086Jy sigma=0.651509 ! Inverting map ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 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=0.071086Jy sigma=0.651509 ! Fit after self-cal, rms=0.071737Jy sigma=0.651470 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec ! Estimated beam: bmin=0.7266 mas, bmaj=1.532 mas, bpa=-1.896 degrees ! Estimated noise=0.419841 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000533717 Jy ! Component: 100 - total flux cleaned = 0.000773791 Jy ! Component: 150 - total flux cleaned = 0.000860983 Jy ! Component: 200 - total flux cleaned = 0.000877147 Jy ! Total flux subtracted in 200 components = 0.000877147 Jy ! Clean residual min=-0.001121 max=0.001100 Jy/beam ! Clean residual mean=-0.000001 rms=0.000260 Jy/beam ! Combined flux in latest and established models = 0.0699027 Jy selfcal ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 80 components and 0.0699027 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=0.071724Jy sigma=0.651395 ! Fit after self-cal, rms=0.071732Jy sigma=0.651290 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 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 = 9.46915e-05 Jy ! Component: 100 - total flux cleaned = 0.000126012 Jy ! Component: 150 - total flux cleaned = 0.000140975 Jy ! Component: 200 - total flux cleaned = 0.000168829 Jy ! Total flux subtracted in 200 components = 0.000168829 Jy ! Clean residual min=-0.001101 max=0.001097 Jy/beam ! Clean residual mean=-0.000001 rms=0.000258 Jy/beam ! Combined flux in latest and established models = 0.0700715 Jy ! Performing phase self-cal ! Adding 34 model components to the UV plane model. ! The established model now contains 83 components and 0.0700715 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=0.071725Jy sigma=0.651245 ! Fit after self-cal, rms=0.071724Jy sigma=0.651241 ! Inverting map ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 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=0.071724Jy sigma=0.651241 ! Fit after self-cal, rms=0.072108Jy sigma=0.651247 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec ! Estimated beam: bmin=2.45 mas, bmaj=3.134 mas, bpa=8.002 degrees ! Estimated noise=0.534563 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000325885 Jy ! Component: 100 - total flux cleaned = 0.000338723 Jy ! Component: 150 - total flux cleaned = 0.000319244 Jy ! Component: 200 - total flux cleaned = 0.000310586 Jy ! Total flux subtracted in 200 components = 0.000310586 Jy ! Clean residual min=-0.001138 max=0.001316 Jy/beam ! Clean residual mean=-0.000002 rms=0.000328 Jy/beam ! Combined flux in latest and established models = 0.0703821 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 99 components and 0.0703821 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=0.072104Jy sigma=0.651234 ! Fit after self-cal, rms=0.072110Jy sigma=0.651223 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 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 = 7.72795e-05 Jy ! Component: 100 - total flux cleaned = 6.1191e-05 Jy ! Component: 150 - total flux cleaned = 3.15905e-05 Jy ! Component: 200 - total flux cleaned = 1.12937e-05 Jy ! Total flux subtracted in 200 components = 1.12937e-05 Jy ! Clean residual min=-0.001127 max=0.001311 Jy/beam ! Clean residual mean=-0.000001 rms=0.000328 Jy/beam ! Combined flux in latest and established models = 0.0703934 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 107 components and 0.0703934 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=0.072109Jy sigma=0.651219 ! Fit after self-cal, rms=0.072109Jy sigma=0.651216 ! Inverting map ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 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 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec ! Estimated beam: bmin=0.7262 mas, bmaj=1.531 mas, bpa=-1.904 degrees ! Estimated noise=0.42174 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7262 x 1.531 at -1.904 degrees (North through East) ! Clean map min=-0.00094381 max=0.054515 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 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec ! Estimated beam: bmin=0.5342 mas, bmaj=1.199 mas, bpa=-5.216 degrees ! Estimated noise=0.943812 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0427827 Jy ! Component: 100 - total flux cleaned = 0.0524858 Jy ! Component: 150 - total flux cleaned = 0.0568521 Jy ! Component: 200 - total flux cleaned = 0.0596131 Jy ! Total flux subtracted in 200 components = 0.0596131 Jy ! Clean residual min=-0.002765 max=0.002957 Jy/beam ! Clean residual mean=-0.000001 rms=0.000636 Jy/beam ! Combined flux in latest and established models = 0.0596131 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 11 model components to the UV plane model. ! The established model now contains 11 components and 0.0596131 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec ! Estimated beam: bmin=0.7262 mas, bmaj=1.531 mas, bpa=-1.904 degrees ! Estimated noise=0.42174 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 = 0.00291811 Jy ! Component: 100 - total flux cleaned = 0.00487159 Jy ! Component: 150 - total flux cleaned = 0.00639033 Jy ! Component: 200 - total flux cleaned = 0.00761544 Jy ! Total flux subtracted in 200 components = 0.00761544 Jy ! Clean residual min=-0.001157 max=0.001239 Jy/beam ! Clean residual mean=-0.000001 rms=0.000282 Jy/beam ! Combined flux in latest and established models = 0.0672286 Jy ! Adding 29 model components to the UV plane model. ! The established model now contains 37 components and 0.0672286 Jy ! Inverting map ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec ! Added new window around map position (15.8, -20.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00123137 Jy ! Component: 100 - total flux cleaned = 0.00200175 Jy ! Component: 150 - total flux cleaned = 0.00230398 Jy ! Component: 200 - total flux cleaned = 0.00249739 Jy ! Total flux subtracted in 200 components = 0.00249739 Jy ! Clean residual min=-0.001092 max=0.001070 Jy/beam ! Clean residual mean=-0.000001 rms=0.000266 Jy/beam ! Combined flux in latest and established models = 0.069726 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 50 components and 0.069726 Jy ! Inverting map ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 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 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec ! Estimated beam: bmin=2.45 mas, bmaj=3.134 mas, bpa=8.002 degrees ! Estimated noise=0.534563 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000434124 Jy ! Component: 100 - total flux cleaned = 0.000518308 Jy ! Component: 150 - total flux cleaned = 0.000491374 Jy ! Component: 200 - total flux cleaned = 0.000454892 Jy ! Total flux subtracted in 200 components = 0.000454892 Jy ! Clean residual min=-0.001205 max=0.001325 Jy/beam ! Clean residual mean=-0.000001 rms=0.000330 Jy/beam ! Combined flux in latest and established models = 0.0701808 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 = -2.22135e-05 Jy ! Component: 100 - total flux cleaned = -3.24917e-05 Jy ! Component: 150 - total flux cleaned = -4.2731e-05 Jy ! Component: 200 - total flux cleaned = -5.20591e-05 Jy ! Total flux subtracted in 200 components = -5.20591e-05 Jy ! Clean residual min=-0.001191 max=0.001337 Jy/beam ! Clean residual mean=-0.000001 rms=0.000328 Jy/beam ! Combined flux in latest and established models = 0.0701288 Jy ! Adding 30 model components to the UV plane model. ! The established model now contains 76 components and 0.0701288 Jy ! Inverting map ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec ! Estimated beam: bmin=0.7262 mas, bmaj=1.531 mas, bpa=-1.904 degrees ! Estimated noise=0.42174 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 3.47071e-05 Jy ! Component: 100 - total flux cleaned = 1.26866e-05 Jy ! Component: 150 - total flux cleaned = 3.29978e-05 Jy ! Component: 200 - total flux cleaned = 7.18947e-05 Jy ! Total flux subtracted in 200 components = 7.18947e-05 Jy ! Clean residual min=-0.001080 max=0.001081 Jy/beam ! Clean residual mean=-0.000001 rms=0.000258 Jy/beam ! Combined flux in latest and established models = 0.0702007 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 85 components and 0.0702007 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=0.072104Jy sigma=0.651181 ! Fit after self-cal, rms=0.072096Jy sigma=0.651138 wmodel /scr/pima/gb073_uvs/J1247+3209_X_map.mod ! Writing 85 model components to file: /scr/pima/gb073_uvs/J1247+3209_X_map.mod wobs /scr/pima/gb073_uvs/J1247+3209_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1247+3209_X_uvs.fits wwins /scr/pima/gb073_uvs/J1247+3209_X_map.win ! wwins: Wrote 5 windows to /scr/pima/gb073_uvs/J1247+3209_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 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000104262 Jy ! Component: 100 - total flux cleaned = -6.6473e-05 Jy ! Component: 150 - total flux cleaned = -4.84063e-05 Jy ! Component: 200 - total flux cleaned = -3.09164e-05 Jy ! Component: 250 - total flux cleaned = -3.1184e-05 Jy ! Component: 300 - total flux cleaned = -6.48791e-05 Jy ! Component: 350 - total flux cleaned = -4.83447e-05 Jy ! Component: 400 - total flux cleaned = -6.46248e-05 Jy ! Component: 450 - total flux cleaned = -6.45424e-05 Jy ! Component: 500 - total flux cleaned = -8.02912e-05 Jy ! Component: 550 - total flux cleaned = -3.35334e-05 Jy ! Component: 600 - total flux cleaned = -3.32763e-05 Jy ! Component: 650 - total flux cleaned = 1.27509e-05 Jy ! Component: 700 - total flux cleaned = 2.81773e-05 Jy ! Component: 750 - total flux cleaned = 7.30594e-05 Jy ! Component: 800 - total flux cleaned = 0.000117423 Jy ! Component: 850 - total flux cleaned = 0.000132159 Jy ! Component: 900 - total flux cleaned = 0.000233677 Jy ! Component: 950 - total flux cleaned = 0.000290904 Jy ! Component: 1000 - total flux cleaned = 0.000319384 Jy ! Component: 1050 - total flux cleaned = 0.000390126 Jy ! Component: 1100 - total flux cleaned = 0.000403968 Jy ! Component: 1150 - total flux cleaned = 0.000459635 Jy ! Component: 1200 - total flux cleaned = 0.000487085 Jy ! Component: 1250 - total flux cleaned = 0.000596619 Jy ! Component: 1300 - total flux cleaned = 0.000596591 Jy ! Component: 1350 - total flux cleaned = 0.00067762 Jy ! Component: 1400 - total flux cleaned = 0.000690895 Jy ! Component: 1450 - total flux cleaned = 0.000757692 Jy ! Component: 1500 - total flux cleaned = 0.000837147 Jy ! Component: 1550 - total flux cleaned = 0.000902892 Jy ! Component: 1600 - total flux cleaned = 0.000955102 Jy ! Component: 1650 - total flux cleaned = 0.001046 Jy ! Component: 1700 - total flux cleaned = 0.00109756 Jy ! Component: 1750 - total flux cleaned = 0.00117444 Jy ! Component: 1800 - total flux cleaned = 0.00123819 Jy ! Component: 1850 - total flux cleaned = 0.00131422 Jy ! Component: 1900 - total flux cleaned = 0.00131449 Jy ! Component: 1950 - total flux cleaned = 0.00143959 Jy ! Component: 2000 - total flux cleaned = 0.00150183 Jy ! Component: 2050 - total flux cleaned = 0.00151427 Jy ! Component: 2100 - total flux cleaned = 0.00158812 Jy ! Component: 2150 - total flux cleaned = 0.00163697 Jy ! Component: 2200 - total flux cleaned = 0.00173412 Jy ! Component: 2250 - total flux cleaned = 0.00174613 Jy ! Component: 2300 - total flux cleaned = 0.00183026 Jy ! Component: 2350 - total flux cleaned = 0.00187803 Jy ! Component: 2400 - total flux cleaned = 0.00191373 Jy ! Component: 2450 - total flux cleaned = 0.00193749 Jy ! Component: 2500 - total flux cleaned = 0.00201985 Jy ! Component: 2550 - total flux cleaned = 0.00207835 Jy ! Component: 2600 - total flux cleaned = 0.00217145 Jy ! Component: 2650 - total flux cleaned = 0.00215989 Jy ! Component: 2700 - total flux cleaned = 0.00224059 Jy ! Component: 2750 - total flux cleaned = 0.00226348 Jy ! Component: 2800 - total flux cleaned = 0.00243455 Jy ! Component: 2850 - total flux cleaned = 0.00240053 Jy ! Component: 2900 - total flux cleaned = 0.00250212 Jy ! Component: 2950 - total flux cleaned = 0.00254704 Jy ! Component: 3000 - total flux cleaned = 0.00259183 Jy ! Component: 3050 - total flux cleaned = 0.00268081 Jy ! Component: 3100 - total flux cleaned = 0.0027141 Jy ! Component: 3150 - total flux cleaned = 0.00278023 Jy ! Component: 3200 - total flux cleaned = 0.00282412 Jy ! Component: 3250 - total flux cleaned = 0.00292244 Jy ! Component: 3300 - total flux cleaned = 0.00293324 Jy ! Component: 3350 - total flux cleaned = 0.00299823 Jy ! Component: 3400 - total flux cleaned = 0.00306297 Jy ! Component: 3450 - total flux cleaned = 0.0031489 Jy ! Component: 3500 - total flux cleaned = 0.00312742 Jy ! Component: 3550 - total flux cleaned = 0.00316999 Jy ! Component: 3600 - total flux cleaned = 0.0032124 Jy ! Component: 3650 - total flux cleaned = 0.00324413 Jy ! Component: 3700 - total flux cleaned = 0.00331774 Jy ! Component: 3750 - total flux cleaned = 0.00328634 Jy ! Component: 3800 - total flux cleaned = 0.00332802 Jy ! Component: 3850 - total flux cleaned = 0.00337997 Jy ! Component: 3900 - total flux cleaned = 0.00341101 Jy ! Component: 3950 - total flux cleaned = 0.00348311 Jy ! Component: 4000 - total flux cleaned = 0.00351391 Jy ! Component: 4050 - total flux cleaned = 0.00349343 Jy ! Total flux subtracted in 4096 components = 0.00352399 Jy ! Clean residual min=-0.000686 max=0.000781 Jy/beam ! Clean residual mean=-0.000000 rms=0.000169 Jy/beam ! Combined flux in latest and established models = 0.0737247 Jy keep ! Adding 329 model components to the UV plane model. ! The established model now contains 414 components and 0.0737247 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1247+3209_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7262 x 1.531 at -1.904 degrees (North through East) ! Clean map min=-0.00078507 max=0.054692 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1247+3209_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0546917 invert ! Inverting map ! Your choice of large map pixels excluded 2.49% of the data. ! The x-axis pixel size should ideally be below 0.1815 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000168528 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.924427 0.924427 1.84885 3.69771 7.39542 14.7908 29.5817 59.1633 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0005 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.054 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 324.525 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1247+3209_X_uvs.log closed on Sat Dec 26 09:39:05 2015