! Started logfile: /scr/pima/gb073_uvs/J0800+5010_X_uvs.log on Sat Dec 26 09:34:13 2015 obs /scr/pima/gb073_uvs/J0800+5010_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J0800+5010_X_uva.fits ! AN table 1: 29 integrations on 36 of 36 possible baselines. ! AN table 2: 29 integrations on 36 of 36 possible baselines. ! AN table 3: 58 integrations on 55 of 55 possible baselines. ! AN table 4: 29 integrations on 55 of 55 possible baselines. ! AN table 5: 29 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.876522 visibilities/baseline/integration-bin. ! Found source: J0800+5010 ! ! 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 61616 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/J0800+5010_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 66 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 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 66 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 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 66 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 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 66 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 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 124 telescope corrections were flagged in sub-array 3. ! A total of 58 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 58 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 124 telescope corrections were flagged in sub-array 3. ! A total of 58 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 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 66 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 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 66 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. ! ! Fit before self-cal, rms=1.005481Jy sigma=9.804230 ! Fit after self-cal, rms=0.940777Jy sigma=9.175006 ! 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 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 milli-arcsec ! Estimated beam: bmin=0.425 mas, bmaj=0.9303 mas, bpa=-20.09 degrees ! Estimated noise=0.726239 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 = 0.0480115 Jy ! Component: 100 - total flux cleaned = 0.0584812 Jy ! Total flux subtracted in 100 components = 0.0584812 Jy ! Clean residual min=-0.002608 max=0.002924 Jy/beam ! Clean residual mean=0.000003 rms=0.000556 Jy/beam ! Combined flux in latest and established models = 0.0584812 Jy ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 0.0584812 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=0.080677Jy sigma=0.678446 ! Fit after self-cal, rms=0.079522Jy sigma=0.667236 ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00361505 Jy ! Component: 100 - total flux cleaned = 0.00488847 Jy ! Total flux subtracted in 100 components = 0.00488847 Jy ! Clean residual min=-0.002640 max=0.002512 Jy/beam ! Clean residual mean=0.000002 rms=0.000552 Jy/beam ! Combined flux in latest and established models = 0.0633697 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 9 components and 0.0633697 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=0.079318Jy sigma=0.665163 ! Fit after self-cal, rms=0.079314Jy sigma=0.665075 ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 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 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 milli-arcsec ! Estimated beam: bmin=0.5703 mas, bmaj=1.162 mas, bpa=-16.13 degrees ! Estimated noise=0.334692 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 (1.8, 3). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00292772 Jy ! Component: 100 - total flux cleaned = 0.00459216 Jy ! Component: 150 - total flux cleaned = 0.00565676 Jy ! Component: 200 - total flux cleaned = 0.00611598 Jy ! Total flux subtracted in 200 components = 0.00611598 Jy ! Clean residual min=-0.001167 max=0.001275 Jy/beam ! Clean residual mean=-0.000002 rms=0.000271 Jy/beam ! Combined flux in latest and established models = 0.0694856 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 26 components and 0.0694856 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=0.079219Jy sigma=0.663920 ! Fit after self-cal, rms=0.079203Jy sigma=0.663676 ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5703 x 1.162 at -16.13 degrees (North through East) ! Clean map min=-0.00095355 max=0.06201 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.10 EF 1.00* FD 0.91 KP 1.03 ! LA 1.15 MK 1.00 NL 1.02 OV 1.02 ! PT 0.94 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 EF 1.00* LA 1.02 MC 1.05 ! NL 0.98 ON 0.98 PT 0.98 SC 0.95 ! ZC 0.76 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 EF 1.00* FD 1.00 KP 0.97 ! LA 0.99 MC 1.01 NL 0.99 ON 1.02 ! PT 1.04 SC 0.94 ZC 0.88 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 EF 1.00* FD 0.98 KP 1.03 ! LA 1.03 MK 1.01 NL 0.98 ON 1.01 ! PT 0.99 SC 0.99 ZC 0.88 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.94 EF 1.00* FD 0.96 KP 0.95 ! LA 1.08 MC 1.02 NL 0.91 ON 0.99 ! OV 1.04 PT 1.00 SC 0.91 ZC 0.88 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.94 EF 1.00* FD 0.96 KP 1.08 ! LA 1.11 MK 0.99 NL 1.05 OV 1.11 ! PT 1.04 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 EF 1.00* LA 1.11 MC 0.99 ! NL 0.97 ON 0.82 PT 1.00 SC 0.93 ! ZC 0.79 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 EF 1.00* FD 1.06 KP 1.01 ! LA 1.06 MC 0.97 NL 1.01 ON 1.06 ! PT 1.04 SC 0.95 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.09 EF 1.00* FD 1.05 KP 1.07 ! LA 1.03 MK 1.05 NL 1.05 ON 1.07 ! PT 1.00 SC 0.95 ZC 0.94 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 EF 1.00* FD 1.05 KP 1.09 ! LA 1.03 MC 0.97 NL 1.00 ON 0.87 ! OV 1.03 PT 1.00 SC 0.95 ZC 0.90 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 EF 1.00* FD 0.97 KP 1.06 ! LA 0.96 MK 0.97 NL 0.98 OV 0.94 ! PT 0.93 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 EF 1.00* LA 0.99 MC 0.94 ! NL 0.90 ON 0.76 PT 1.04 SC 0.93 ! ZC 0.90 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 EF 1.00* FD 1.00 KP 0.96 ! LA 0.97 MC 0.97 NL 0.95 ON 1.02 ! PT 0.98 SC 1.02 ZC 0.85 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.14 EF 1.00* FD 0.95 KP 0.95 ! LA 0.98 MK 0.90 NL 1.01 ON 1.11 ! PT 1.01 SC 1.12 ZC 0.90 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.96 EF 1.00* FD 1.06 KP 0.92 ! LA 1.11 MC 1.00 NL 0.98 ON 0.88 ! OV 1.03 PT 0.99 SC 1.04 ZC 0.81 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.14 EF 1.00* FD 0.94 KP 0.92 ! LA 1.00 MK 1.06 NL 1.08 OV 0.95 ! PT 1.05 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.14 EF 1.00* LA 1.04 MC 1.04 ! NL 0.95 ON 0.86 PT 0.88 SC 1.19 ! ZC 0.82 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.06 EF 1.00* FD 1.01 KP 1.00 ! LA 1.02 MC 0.96 NL 1.05 ON 1.00 ! PT 1.00 SC 1.07 ZC 0.86 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.07 EF 1.00* FD 1.04 KP 0.96 ! LA 1.06 MK 0.97 NL 0.99 ON 1.02 ! PT 1.01 SC 0.99 ZC 0.94 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 EF 1.00* FD 1.06 KP 0.95 ! LA 0.95 MC 1.12 NL 1.03 ON 0.98 ! OV 1.02 PT 1.05 SC 1.18 ZC 0.88 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.01 KP 0.92 ! LA 1.04 MK 0.95 NL 1.08 OV 0.96 ! PT 0.91 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* LA 0.95 MC 1.07 ! NL 1.06 ON 1.11 PT 0.87 SC 1.13 ! ZC 0.76 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.02 KP 0.85 ! LA 1.01 MC 1.23 NL 1.06 ON 1.26 ! PT 0.96 SC 1.03 ZC 0.80 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.97 KP 0.95 ! LA 0.97 MK 1.02 NL 1.10 ON 1.19 ! PT 0.95 SC 1.02 ZC 0.90 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.06 KP 0.92 ! LA 1.04 MC 1.24 NL 0.92 ON 1.15 ! OV 1.03 PT 1.09 SC 1.05 ZC 0.80 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.95 KP 0.86 ! LA 1.06 MK 1.00 NL 0.95 OV 1.09 ! PT 0.91 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* LA 1.05 MC 1.07 ! NL 0.93 ON 1.18 PT 0.91 SC 0.91 ! ZC 0.80 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.03 KP 0.84 ! LA 1.03 MC 1.19 NL 1.03 ON 1.24 ! PT 1.02 SC 1.02 ZC 0.86 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.99 KP 0.91 ! LA 0.96 MK 0.95 NL 0.97 ON 1.27 ! PT 0.98 SC 0.96 ZC 0.88 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 0.96 KP 0.96 ! LA 0.96 MC 1.32 NL 0.89 ON 1.25 ! OV 1.10 PT 0.97 SC 0.91 ZC 0.78 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.12 EF 1.00* FD 0.93 KP 0.94 ! LA 1.10 MK 1.08 NL 0.99 OV 1.04 ! PT 1.02 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.06 EF 1.00* LA 0.97 MC 1.28 ! NL 0.89 ON 1.16 PT 1.05 SC 0.85 ! ZC 0.66 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 EF 1.00* FD 1.00 KP 0.97 ! LA 1.09 MC 1.36 NL 0.97 ON 1.32 ! PT 0.98 SC 0.98 ZC 0.69 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 EF 1.00* FD 1.02 KP 0.98 ! LA 0.96 MK 1.17 NL 1.04 ON 1.35 ! PT 0.97 SC 0.97 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 EF 1.00* FD 1.08 KP 0.97 ! LA 1.06 MC 1.33 NL 0.95 ON 1.40 ! OV 0.99 PT 0.96 SC 0.97 ZC 0.61 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.06 EF 1.00* FD 0.94 KP 0.93 ! LA 1.08 MK 1.00 NL 1.01 OV 1.04 ! PT 0.96 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.90 EF 1.00* LA 0.97 MC 1.16 ! NL 1.02 ON 1.20 PT 0.90 SC 0.93 ! ZC 0.64 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 EF 1.00* FD 1.04 KP 0.96 ! LA 1.05 MC 1.19 NL 1.06 ON 1.26 ! PT 0.95 SC 1.03 ZC 0.64 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.06 EF 1.00* FD 1.02 KP 0.91 ! LA 1.05 MK 0.97 NL 1.05 ON 1.18 ! PT 0.99 SC 0.95 ZC 0.75 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 EF 1.00* FD 0.98 KP 0.83 ! LA 1.09 MC 1.18 NL 0.92 ON 1.25 ! OV 1.07 PT 1.08 SC 1.00 ZC 0.66 ! ! ! Fit before self-cal, rms=0.079203Jy sigma=0.663676 ! Fit after self-cal, rms=0.079456Jy sigma=0.658726 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 milli-arcsec ! Estimated beam: bmin=0.5676 mas, bmaj=1.152 mas, bpa=-17.04 degrees ! Estimated noise=0.33398 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 = 0.00113131 Jy ! Component: 100 - total flux cleaned = 0.00156935 Jy ! Component: 150 - total flux cleaned = 0.00165042 Jy ! Component: 200 - total flux cleaned = 0.00165021 Jy ! Total flux subtracted in 200 components = 0.00165021 Jy ! Clean residual min=-0.000971 max=0.000976 Jy/beam ! Clean residual mean=-0.000002 rms=0.000218 Jy/beam ! Combined flux in latest and established models = 0.0711359 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 38 components and 0.0711359 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=0.079439Jy sigma=0.658513 ! Fit after self-cal, rms=0.079579Jy sigma=0.657995 ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 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=0.079579Jy sigma=0.657995 ! Fit after self-cal, rms=0.080325Jy sigma=0.657674 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 milli-arcsec ! Estimated beam: bmin=0.567 mas, bmaj=1.149 mas, bpa=-17.15 degrees ! Estimated noise=0.33446 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000717326 Jy ! Component: 100 - total flux cleaned = 0.000879268 Jy ! Component: 150 - total flux cleaned = 0.000908539 Jy ! Component: 200 - total flux cleaned = 0.000921048 Jy ! Total flux subtracted in 200 components = 0.000921048 Jy ! Clean residual min=-0.000958 max=0.000924 Jy/beam ! Clean residual mean=-0.000002 rms=0.000213 Jy/beam ! Combined flux in latest and established models = 0.0720569 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 41 components and 0.0720569 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=0.080318Jy sigma=0.657587 ! Fit after self-cal, rms=0.080348Jy sigma=0.657542 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 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 = 0.000260651 Jy ! Component: 100 - total flux cleaned = 0.000272029 Jy ! Component: 150 - total flux cleaned = 0.000282291 Jy ! Component: 200 - total flux cleaned = 0.000301827 Jy ! Total flux subtracted in 200 components = 0.000301827 Jy ! Clean residual min=-0.000942 max=0.000901 Jy/beam ! Clean residual mean=-0.000002 rms=0.000212 Jy/beam ! Combined flux in latest and established models = 0.0723587 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 44 components and 0.0723587 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=0.080344Jy sigma=0.657513 ! Fit after self-cal, rms=0.080344Jy sigma=0.657503 ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 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=0.080344Jy sigma=0.657503 ! Fit after self-cal, rms=0.080688Jy sigma=0.657483 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 milli-arcsec ! Estimated beam: bmin=0.5667 mas, bmaj=1.148 mas, bpa=-17.23 degrees ! Estimated noise=0.335246 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000401509 Jy ! Component: 100 - total flux cleaned = 0.000459951 Jy ! Component: 150 - total flux cleaned = 0.000490958 Jy ! Component: 200 - total flux cleaned = 0.000519477 Jy ! Total flux subtracted in 200 components = 0.000519477 Jy ! Clean residual min=-0.000931 max=0.000892 Jy/beam ! Clean residual mean=-0.000001 rms=0.000211 Jy/beam ! Combined flux in latest and established models = 0.0728782 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 46 components and 0.0728782 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=0.080685Jy sigma=0.657451 ! Fit after self-cal, rms=0.080693Jy sigma=0.657447 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 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 = 9.21575e-05 Jy ! Component: 100 - total flux cleaned = 0.000119269 Jy ! Component: 150 - total flux cleaned = 0.000135849 Jy ! Component: 200 - total flux cleaned = 0.000151642 Jy ! Total flux subtracted in 200 components = 0.000151642 Jy ! Clean residual min=-0.000916 max=0.000894 Jy/beam ! Clean residual mean=-0.000002 rms=0.000211 Jy/beam ! Combined flux in latest and established models = 0.0730298 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 48 components and 0.0730298 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=0.080691Jy sigma=0.657428 ! Fit after self-cal, rms=0.080690Jy sigma=0.657427 ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 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=0.080690Jy sigma=0.657427 ! Fit after self-cal, rms=0.080835Jy sigma=0.657417 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 milli-arcsec ! Estimated beam: bmin=2.759 mas, bmaj=2.78 mas, bpa=48.64 degrees ! Estimated noise=0.449075 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000505931 Jy ! Component: 100 - total flux cleaned = 0.000641339 Jy ! Component: 150 - total flux cleaned = 0.0006822 Jy ! Component: 200 - total flux cleaned = 0.000705008 Jy ! Total flux subtracted in 200 components = 0.000705008 Jy ! Clean residual min=-0.001079 max=0.000974 Jy/beam ! Clean residual mean=-0.000005 rms=0.000268 Jy/beam ! Combined flux in latest and established models = 0.0737348 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 51 components and 0.0737348 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=0.080835Jy sigma=0.657434 ! Fit after self-cal, rms=0.080836Jy sigma=0.657426 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 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 = 0.000133866 Jy ! Component: 100 - total flux cleaned = 0.000139177 Jy ! Component: 150 - total flux cleaned = 0.000143638 Jy ! Component: 200 - total flux cleaned = 0.000147538 Jy ! Total flux subtracted in 200 components = 0.000147538 Jy ! Clean residual min=-0.001068 max=0.000976 Jy/beam ! Clean residual mean=-0.000006 rms=0.000267 Jy/beam ! Combined flux in latest and established models = 0.0738824 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 54 components and 0.0738824 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=0.080837Jy sigma=0.657443 ! Fit after self-cal, rms=0.080837Jy sigma=0.657441 ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 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 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 milli-arcsec ! Estimated beam: bmin=0.5663 mas, bmaj=1.146 mas, bpa=-17.29 degrees ! Estimated noise=0.335827 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5663 x 1.146 at -17.29 degrees (North through East) ! Clean map min=-0.00075711 max=0.062081 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 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 milli-arcsec ! Estimated beam: bmin=0.4199 mas, bmaj=0.9193 mas, bpa=-21.58 degrees ! Estimated noise=0.720528 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0483058 Jy ! Component: 100 - total flux cleaned = 0.0589132 Jy ! Component: 150 - total flux cleaned = 0.0625291 Jy ! Component: 200 - total flux cleaned = 0.0645491 Jy ! Total flux subtracted in 200 components = 0.0645491 Jy ! Clean residual min=-0.002747 max=0.002200 Jy/beam ! Clean residual mean=0.000003 rms=0.000501 Jy/beam ! Combined flux in latest and established models = 0.0645491 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 8 model components to the UV plane model. ! The established model now contains 8 components and 0.0645491 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 milli-arcsec ! Estimated beam: bmin=0.5663 mas, bmaj=1.146 mas, bpa=-17.29 degrees ! Estimated noise=0.335827 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 = 0.00296555 Jy ! Component: 100 - total flux cleaned = 0.00486243 Jy ! Component: 150 - total flux cleaned = 0.00618543 Jy ! Component: 200 - total flux cleaned = 0.00712662 Jy ! Total flux subtracted in 200 components = 0.00712662 Jy ! Clean residual min=-0.000955 max=0.000867 Jy/beam ! Clean residual mean=0.000002 rms=0.000219 Jy/beam ! Combined flux in latest and established models = 0.0716757 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 29 components and 0.0716757 Jy ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 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 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 milli-arcsec ! Estimated beam: bmin=2.759 mas, bmaj=2.78 mas, bpa=48.64 degrees ! Estimated noise=0.449075 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00119358 Jy ! Component: 100 - total flux cleaned = 0.00161421 Jy ! Component: 150 - total flux cleaned = 0.00174123 Jy ! Component: 200 - total flux cleaned = 0.00182652 Jy ! Total flux subtracted in 200 components = 0.00182652 Jy ! Clean residual min=-0.001050 max=0.000980 Jy/beam ! Clean residual mean=-0.000004 rms=0.000268 Jy/beam ! Combined flux in latest and established models = 0.0735023 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 = 7.87982e-05 Jy ! Component: 100 - total flux cleaned = 0.000132495 Jy ! Component: 150 - total flux cleaned = 0.000176017 Jy ! Component: 200 - total flux cleaned = 0.000212351 Jy ! Total flux subtracted in 200 components = 0.000212351 Jy ! Clean residual min=-0.001059 max=0.000966 Jy/beam ! Clean residual mean=-0.000005 rms=0.000267 Jy/beam ! Combined flux in latest and established models = 0.0737146 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 47 components and 0.0737146 Jy ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 milli-arcsec ! Estimated beam: bmin=0.5663 mas, bmaj=1.146 mas, bpa=-17.29 degrees ! Estimated noise=0.335827 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000254137 Jy ! Component: 100 - total flux cleaned = -0.000236348 Jy ! Component: 150 - total flux cleaned = -0.000191071 Jy ! Component: 200 - total flux cleaned = -0.000150733 Jy ! Total flux subtracted in 200 components = -0.000150733 Jy ! Clean residual min=-0.000892 max=0.000857 Jy/beam ! Clean residual mean=-0.000002 rms=0.000211 Jy/beam ! Combined flux in latest and established models = 0.0735639 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 53 components and 0.0735639 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=0.080836Jy sigma=0.657435 ! Fit after self-cal, rms=0.080830Jy sigma=0.657408 wmodel /scr/pima/gb073_uvs/J0800+5010_X_map.mod ! Writing 53 model components to file: /scr/pima/gb073_uvs/J0800+5010_X_map.mod wobs /scr/pima/gb073_uvs/J0800+5010_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J0800+5010_X_uvs.fits wwins /scr/pima/gb073_uvs/J0800+5010_X_map.win ! wwins: Wrote 2 windows to /scr/pima/gb073_uvs/J0800+5010_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 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000220872 Jy ! Component: 100 - total flux cleaned = -0.000334739 Jy ! Component: 150 - total flux cleaned = -0.000445332 Jy ! Component: 200 - total flux cleaned = -0.000522695 Jy ! Component: 250 - total flux cleaned = -0.000659191 Jy ! Component: 300 - total flux cleaned = -0.000748522 Jy ! Component: 350 - total flux cleaned = -0.000806974 Jy ! Component: 400 - total flux cleaned = -0.000806868 Jy ! Component: 450 - total flux cleaned = -0.000821012 Jy ! Component: 500 - total flux cleaned = -0.000764379 Jy ! Component: 550 - total flux cleaned = -0.000820579 Jy ! Component: 600 - total flux cleaned = -0.000792431 Jy ! Component: 650 - total flux cleaned = -0.000806156 Jy ! Component: 700 - total flux cleaned = -0.000819809 Jy ! Component: 750 - total flux cleaned = -0.000846763 Jy ! Component: 800 - total flux cleaned = -0.000887248 Jy ! Component: 850 - total flux cleaned = -0.000900565 Jy ! Component: 900 - total flux cleaned = -0.000940476 Jy ! Component: 950 - total flux cleaned = -0.000979922 Jy ! Component: 1000 - total flux cleaned = -0.00100602 Jy ! Component: 1050 - total flux cleaned = -0.00103189 Jy ! Component: 1100 - total flux cleaned = -0.000967639 Jy ! Component: 1150 - total flux cleaned = -0.00105711 Jy ! Component: 1200 - total flux cleaned = -0.00110802 Jy ! Component: 1250 - total flux cleaned = -0.0010828 Jy ! Component: 1300 - total flux cleaned = -0.00113299 Jy ! Component: 1350 - total flux cleaned = -0.00109564 Jy ! Component: 1400 - total flux cleaned = -0.0011081 Jy ! Component: 1450 - total flux cleaned = -0.00112057 Jy ! Component: 1500 - total flux cleaned = -0.00114507 Jy ! Component: 1550 - total flux cleaned = -0.00110846 Jy ! Component: 1600 - total flux cleaned = -0.00112063 Jy ! Component: 1650 - total flux cleaned = -0.00115679 Jy ! Component: 1700 - total flux cleaned = -0.00113271 Jy ! Component: 1750 - total flux cleaned = -0.0011566 Jy ! Component: 1800 - total flux cleaned = -0.0011209 Jy ! Component: 1850 - total flux cleaned = -0.00113272 Jy ! Component: 1900 - total flux cleaned = -0.00115629 Jy ! Component: 1950 - total flux cleaned = -0.00110928 Jy ! Component: 2000 - total flux cleaned = -0.0010392 Jy ! Component: 2050 - total flux cleaned = -0.00107426 Jy ! Component: 2100 - total flux cleaned = -0.00103954 Jy ! Component: 2150 - total flux cleaned = -0.0010165 Jy ! Component: 2200 - total flux cleaned = -0.00101643 Jy ! Component: 2250 - total flux cleaned = -0.00100502 Jy ! Component: 2300 - total flux cleaned = -0.0010278 Jy ! Component: 2350 - total flux cleaned = -0.000993713 Jy ! Component: 2400 - total flux cleaned = -0.000959786 Jy ! Component: 2450 - total flux cleaned = -0.00102728 Jy ! Component: 2500 - total flux cleaned = -0.00096002 Jy ! Component: 2550 - total flux cleaned = -0.0009488 Jy ! Component: 2600 - total flux cleaned = -0.000982093 Jy ! Component: 2650 - total flux cleaned = -0.00094892 Jy ! Component: 2700 - total flux cleaned = -0.000926951 Jy ! Component: 2750 - total flux cleaned = -0.000948887 Jy ! Component: 2800 - total flux cleaned = -0.000926968 Jy ! Component: 2850 - total flux cleaned = -0.000926999 Jy ! Component: 2900 - total flux cleaned = -0.000959691 Jy ! Component: 2950 - total flux cleaned = -0.00093803 Jy ! Component: 3000 - total flux cleaned = -0.000992048 Jy ! Component: 3050 - total flux cleaned = -0.00100271 Jy ! Component: 3100 - total flux cleaned = -0.00100264 Jy ! Component: 3150 - total flux cleaned = -0.00104538 Jy ! Component: 3200 - total flux cleaned = -0.00101332 Jy ! Component: 3250 - total flux cleaned = -0.000992125 Jy ! Component: 3300 - total flux cleaned = -0.00103445 Jy ! Component: 3350 - total flux cleaned = -0.00102383 Jy ! Component: 3400 - total flux cleaned = -0.000992258 Jy ! Component: 3450 - total flux cleaned = -0.00100273 Jy ! Component: 3500 - total flux cleaned = -0.00103411 Jy ! Component: 3550 - total flux cleaned = -0.00107581 Jy ! Component: 3600 - total flux cleaned = -0.00108621 Jy ! Component: 3650 - total flux cleaned = -0.00100337 Jy ! Component: 3700 - total flux cleaned = -0.00103432 Jy ! Component: 3750 - total flux cleaned = -0.00103436 Jy ! Component: 3800 - total flux cleaned = -0.0010549 Jy ! Component: 3850 - total flux cleaned = -0.0010549 Jy ! Component: 3900 - total flux cleaned = -0.00106515 Jy ! Component: 3950 - total flux cleaned = -0.00101431 Jy ! Component: 4000 - total flux cleaned = -0.00104474 Jy ! Component: 4050 - total flux cleaned = -0.00101436 Jy ! Total flux subtracted in 4096 components = -0.00102447 Jy ! Clean residual min=-0.000600 max=0.000549 Jy/beam ! Clean residual mean=-0.000000 rms=0.000165 Jy/beam ! Combined flux in latest and established models = 0.0725394 Jy keep ! Adding 345 model components to the UV plane model. ! The established model now contains 398 components and 0.0725394 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J0800+5010_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5663 x 1.146 at -17.29 degrees (North through East) ! Clean map min=-0.00077099 max=0.062375 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J0800+5010_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0623754 invert ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1802 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000164924 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.793215 0.793215 1.58643 3.17286 6.34572 12.6914 25.3829 50.7658 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0004 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.062 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 378.207 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J0800+5010_X_uvs.log closed on Sat Dec 26 09:34:19 2015