! Started logfile: /scr/pima/rv120_uvs/J1254+1141_X_dfm.log on Fri Dec 22 22:42:17 2017 float field_size field_size = 1024 float field_cell field_cell = 0.2000 float taper_size taper_size = 70.0 float freq freq = 8.36575 obs /scr/pima/rv120_uvs/J1254+1141_X_uva.fits ! Reading UV FITS file: /scr/pima/rv120_uvs/J1254+1141_X_uva.fits ! AN table 1: 7 integrations on 28 of 28 possible baselines. ! AN table 2: 11 integrations on 3 of 3 possible baselines. ! AN table 3: 17 integrations on 3 of 3 possible baselines. ! AN table 4: 220 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.160676 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1254+1141 ! ! There are 4 IFs, and a total of 4 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.36575e+09 8e+06 1 8e+06 ! 02 2 8.44575e+09 8e+06 1 8e+06 ! 03 3 8.80575e+09 8e+06 1 8e+06 ! 04 4 8.92575e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 79 lines of history. ! ! Reading 9512 visibilities. select rr, 1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16 ! Restricting channel ranges to the available 4 channels. ! Selecting polarization: RR, channels: 1..4 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 print "field_size =", field_size ! field_size = 1024 print "field_cell =", field_cell ! field_cell = 0.2 print "taper_size =", taper_size ! taper_size = 70 ![@/opt64/bin/pima_mupet_01.dfm J1254+1141_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 8 telescope corrections were flagged in sub-array 1. ! A total of 3 telescope corrections were flagged in sub-array 2. ! A total of 9 telescope corrections were flagged in sub-array 3. ! A total of 1761 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 8 telescope corrections were flagged in sub-array 1. ! A total of 3 telescope corrections were flagged in sub-array 2. ! A total of 9 telescope corrections were flagged in sub-array 3. ! A total of 1761 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 8 telescope corrections were flagged in sub-array 1. ! A total of 3 telescope corrections were flagged in sub-array 2. ! A total of 9 telescope corrections were flagged in sub-array 3. ! A total of 1761 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 8 telescope corrections were flagged in sub-array 1. ! A total of 3 telescope corrections were flagged in sub-array 2. ! A total of 9 telescope corrections were flagged in sub-array 3. ! A total of 1761 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.112779Jy sigma=15.168238 ! Fit after self-cal, rms=0.555408Jy sigma=7.847682 ! 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 10.9% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! Estimated beam: bmin=0.542 mas, bmaj=0.8294 mas, bpa=-9.167 degrees ! Estimated noise=0.847425 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 = 0.332481 Jy ! Component: 100 - total flux cleaned = 0.436263 Jy ! Total flux subtracted in 100 components = 0.436263 Jy ! Clean residual min=-0.016602 max=0.046920 Jy/beam ! Clean residual mean=0.000008 rms=0.003530 Jy/beam ! Combined flux in latest and established models = 0.436263 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.436263 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.174291Jy sigma=1.812318 ! Fit after self-cal, rms=0.173511Jy sigma=1.803742 ! Inverting map ! Your choice of large map pixels excluded 10.9% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! Added new window around map position (-0.6, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0494895 Jy ! Component: 100 - total flux cleaned = 0.0507898 Jy ! Total flux subtracted in 100 components = 0.0507898 Jy ! Clean residual min=-0.019024 max=0.032885 Jy/beam ! Clean residual mean=0.000008 rms=0.002730 Jy/beam ! Combined flux in latest and established models = 0.487053 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 9 components and 0.487053 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.148796Jy sigma=1.492211 ! Fit after self-cal, rms=0.148007Jy sigma=1.483797 ! Inverting map ! Your choice of large map pixels excluded 10.9% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! Added new window around map position (-1.8, -0.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0193299 Jy ! Component: 100 - total flux cleaned = 0.0243047 Jy ! Total flux subtracted in 100 components = 0.0243047 Jy ! Clean residual min=-0.014929 max=0.021086 Jy/beam ! Clean residual mean=0.000007 rms=0.002270 Jy/beam ! Combined flux in latest and established models = 0.511358 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 13 components and 0.511358 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.135582Jy sigma=1.330721 ! Fit after self-cal, rms=0.134386Jy sigma=1.317801 ! Inverting map ! Your choice of large map pixels excluded 10.9% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00892328 Jy ! Component: 100 - total flux cleaned = 0.01121 Jy ! Total flux subtracted in 100 components = 0.01121 Jy ! Clean residual min=-0.011536 max=0.016769 Jy/beam ! Clean residual mean=0.000006 rms=0.002005 Jy/beam ! Combined flux in latest and established models = 0.522568 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 14 components and 0.522568 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.126580Jy sigma=1.237166 ! Fit after self-cal, rms=0.126155Jy sigma=1.233612 ! Inverting map ! Your choice of large map pixels excluded 10.9% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! Added new window around map position (0, -1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00893425 Jy ! Component: 100 - total flux cleaned = 0.0128343 Jy ! Total flux subtracted in 100 components = 0.0128343 Jy ! Clean residual min=-0.009731 max=0.014585 Jy/beam ! Clean residual mean=0.000006 rms=0.001814 Jy/beam ! Combined flux in latest and established models = 0.535402 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 19 components and 0.535402 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.120795Jy sigma=1.175361 ! Fit after self-cal, rms=0.120538Jy sigma=1.172613 ! Inverting map ! Your choice of large map pixels excluded 10.9% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! Added new window around map position (0.6, 2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00782436 Jy ! Component: 100 - total flux cleaned = 0.0099211 Jy ! Total flux subtracted in 100 components = 0.0099211 Jy ! Clean residual min=-0.008863 max=0.011660 Jy/beam ! Clean residual mean=0.000006 rms=0.001671 Jy/beam ! Combined flux in latest and established models = 0.545323 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 23 components and 0.545323 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.117199Jy sigma=1.135933 ! Fit after self-cal, rms=0.117113Jy sigma=1.135016 ! Inverting map ! Your choice of large map pixels excluded 10.9% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! Added new window around map position (-1.2, -1.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00605651 Jy ! Component: 100 - total flux cleaned = 0.00778538 Jy ! Total flux subtracted in 100 components = 0.00778538 Jy ! Clean residual min=-0.008476 max=0.009875 Jy/beam ! Clean residual mean=0.000006 rms=0.001567 Jy/beam ! Combined flux in latest and established models = 0.553109 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 26 components and 0.553109 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.114664Jy sigma=1.107848 ! Fit after self-cal, rms=0.114588Jy sigma=1.107277 ! Inverting map ! Your choice of large map pixels excluded 10.9% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! Added new window around map position (-2.6, 0.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00434581 Jy ! Component: 100 - total flux cleaned = 0.00582103 Jy ! Total flux subtracted in 100 components = 0.00582103 Jy ! Clean residual min=-0.008131 max=0.008407 Jy/beam ! Clean residual mean=0.000005 rms=0.001491 Jy/beam ! Combined flux in latest and established models = 0.55893 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 30 components and 0.55893 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.112985Jy sigma=1.089687 ! Fit after self-cal, rms=0.112951Jy sigma=1.089035 ! Inverting map ! Your choice of large map pixels excluded 10.9% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 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 10.9% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! Estimated beam: bmin=0.6558 mas, bmaj=0.8452 mas, bpa=-9.769 degrees ! Estimated noise=0.607176 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 = 0.00954365 Jy ! Component: 100 - total flux cleaned = 0.0105603 Jy ! Component: 150 - total flux cleaned = 0.0108617 Jy ! Component: 200 - total flux cleaned = 0.0111554 Jy ! Total flux subtracted in 200 components = 0.0111554 Jy ! Clean residual min=-0.007619 max=0.007542 Jy/beam ! Clean residual mean=-0.000001 rms=0.001459 Jy/beam ! Combined flux in latest and established models = 0.570085 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 37 components and 0.570085 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.110486Jy sigma=1.064744 ! Fit after self-cal, rms=0.110291Jy sigma=1.063101 ! Inverting map ! Your choice of large map pixels excluded 10.9% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6558 x 0.8452 at -9.769 degrees (North through East) ! Clean map min=-0.0063852 max=0.41932 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 1.00 KP 0.99 LA 1.01 ! MK 0.92 NL 1.07 OV 1.01 PT 1.02 ! ! A total of 30 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* KK 0.00* MK 0.00* ! ! A total of 42 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! KK 0.00* MK 0.00* NY 0.00* ! ! A total of 195 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 FD 1.02 HH 0.96 HN 1.10 ! KP 1.05 LA 0.99 NL 0.99 NY 0.98 ! ON 1.00 PT 1.01 SC 1.02 WZ 0.97 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 1.02 KP 0.99 LA 1.01 ! MK 0.90 NL 1.04 OV 1.02 PT 1.03 ! ! A total of 30 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* KK 0.00* MK 0.00* ! ! A total of 42 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! KK 0.00* MK 0.00* NY 0.00* ! ! A total of 195 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 1.03 HH 0.95 HN 1.10 ! KP 1.04 LA 1.00 NL 0.99 NY 1.02 ! ON 1.02 PT 1.00 SC 1.05 WZ 0.93 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.99 KP 0.98 LA 1.00 ! MK 0.93 NL 1.06 OV 0.98 PT 1.04 ! ! A total of 30 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* KK 0.00* MK 0.00* ! ! A total of 42 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! KK 0.00* MK 0.00* NY 0.00* ! ! A total of 195 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 FD 1.02 HH 0.94 HN 1.08 ! KP 1.02 LA 0.99 NL 0.98 NY 0.98 ! ON 1.03 PT 1.00 SC 1.06 WZ 0.95 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.98 KP 0.99 LA 0.99 ! MK 0.90 NL 1.06 OV 1.01 PT 1.02 ! ! A total of 30 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* KK 0.00* MK 0.00* ! ! A total of 42 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! KK 0.00* MK 0.00* NY 0.00* ! ! A total of 195 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 1.01 HH 0.94 HN 1.07 ! KP 1.04 LA 0.97 NL 0.98 NY 0.98 ! ON 1.03 PT 1.01 SC 1.10 WZ 0.94 ! ! ! Fit before self-cal, rms=0.110291Jy sigma=1.063101 ! Fit after self-cal, rms=0.104819Jy sigma=1.014162 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! Estimated beam: bmin=0.6333 mas, bmaj=0.8319 mas, bpa=-12.19 degrees ! Estimated noise=0.630277 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 (-2.6, -1.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00239082 Jy ! Component: 100 - total flux cleaned = 0.00275889 Jy ! Component: 150 - total flux cleaned = 0.00320282 Jy ! Component: 200 - total flux cleaned = 0.00333603 Jy ! Total flux subtracted in 200 components = 0.00333603 Jy ! Clean residual min=-0.005320 max=0.005075 Jy/beam ! Clean residual mean=0.000004 rms=0.001076 Jy/beam ! Combined flux in latest and established models = 0.573421 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 51 components and 0.573421 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.104392Jy sigma=1.009570 ! Fit after self-cal, rms=0.104369Jy sigma=1.008795 ! Inverting map ! Your choice of large map pixels excluded 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec selfcal true, true, soltime1 ! Performing amp+phase self-cal over 120 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.104369Jy sigma=1.008795 ! Fit after self-cal, rms=0.101137Jy sigma=0.978299 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! Estimated beam: bmin=0.6324 mas, bmaj=0.8318 mas, bpa=-11.55 degrees ! Estimated noise=0.630468 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00335302 Jy ! Component: 100 - total flux cleaned = 0.00371629 Jy ! Component: 150 - total flux cleaned = 0.00387295 Jy ! Component: 200 - total flux cleaned = 0.00400947 Jy ! Total flux subtracted in 200 components = 0.00400947 Jy ! Clean residual min=-0.004149 max=0.004609 Jy/beam ! Clean residual mean=0.000006 rms=0.000882 Jy/beam ! Combined flux in latest and established models = 0.57743 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 62 components and 0.57743 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.101017Jy sigma=0.977063 ! Fit after self-cal, rms=0.101027Jy sigma=0.976741 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 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 (-7.8, -0.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00423273 Jy ! Component: 100 - total flux cleaned = 0.00552303 Jy ! Component: 150 - total flux cleaned = 0.0058849 Jy ! Component: 200 - total flux cleaned = 0.00614901 Jy ! Total flux subtracted in 200 components = 0.00614901 Jy ! Clean residual min=-0.003980 max=0.004304 Jy/beam ! Clean residual mean=0.000003 rms=0.000868 Jy/beam ! Combined flux in latest and established models = 0.583579 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 74 components and 0.58358 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100860Jy sigma=0.974740 ! Fit after self-cal, rms=0.100801Jy sigma=0.974184 ! Inverting map ! Your choice of large map pixels excluded 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! Added new window around map position (34.8, 0.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00363966 Jy ! Component: 100 - total flux cleaned = 0.00520857 Jy ! Component: 150 - total flux cleaned = 0.0060312 Jy ! Component: 200 - total flux cleaned = 0.00658715 Jy ! Total flux subtracted in 200 components = 0.00658715 Jy ! Clean residual min=-0.003854 max=0.003796 Jy/beam ! Clean residual mean=0.000003 rms=0.000843 Jy/beam ! Combined flux in latest and established models = 0.590167 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 81 components and 0.590167 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100647Jy sigma=0.972671 ! Fit after self-cal, rms=0.100603Jy sigma=0.972374 ! Inverting map ! Your choice of large map pixels excluded 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec selfcal true, true, soltime2 ! Performing amp+phase self-cal over 20 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100603Jy sigma=0.972374 ! Fit after self-cal, rms=0.099021Jy sigma=0.954427 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! Estimated beam: bmin=0.6318 mas, bmaj=0.8322 mas, bpa=-11.5 degrees ! Estimated noise=0.630051 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00110864 Jy ! Component: 100 - total flux cleaned = 0.00151172 Jy ! Component: 150 - total flux cleaned = 0.0016949 Jy ! Component: 200 - total flux cleaned = 0.00191403 Jy ! Total flux subtracted in 200 components = 0.00191403 Jy ! Clean residual min=-0.002700 max=0.002589 Jy/beam ! Clean residual mean=0.000009 rms=0.000590 Jy/beam ! Combined flux in latest and established models = 0.592081 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 89 components and 0.592081 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.098995Jy sigma=0.953623 ! Fit after self-cal, rms=0.098948Jy sigma=0.953429 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 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 = 0.000113866 Jy ! Component: 100 - total flux cleaned = 0.000377051 Jy ! Component: 150 - total flux cleaned = 0.00052262 Jy ! Component: 200 - total flux cleaned = 0.000697693 Jy ! Total flux subtracted in 200 components = 0.000697693 Jy ! Clean residual min=-0.002691 max=0.002570 Jy/beam ! Clean residual mean=0.000008 rms=0.000584 Jy/beam ! Combined flux in latest and established models = 0.592778 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 96 components and 0.592778 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.098937Jy sigma=0.952965 ! Fit after self-cal, rms=0.098891Jy sigma=0.952839 ! Inverting map ! Your choice of large map pixels excluded 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. win_mult = win_mult * 1.2 selfcal true, true, soltime2 ! Performing amp+phase self-cal over 20 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.098891Jy sigma=0.952839 ! Fit after self-cal, rms=0.098748Jy sigma=0.952620 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! Estimated beam: bmin=2.566 mas, bmaj=2.888 mas, bpa=-35.96 degrees ! Estimated noise=0.838225 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00149936 Jy ! Component: 100 - total flux cleaned = 0.00183173 Jy ! Component: 150 - total flux cleaned = 0.00204376 Jy ! Component: 200 - total flux cleaned = 0.00222638 Jy ! Total flux subtracted in 200 components = 0.00222638 Jy ! Clean residual min=-0.003197 max=0.002858 Jy/beam ! Clean residual mean=0.000021 rms=0.000774 Jy/beam ! Combined flux in latest and established models = 0.595005 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 107 components and 0.595005 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.098733Jy sigma=0.952659 ! Fit after self-cal, rms=0.098711Jy sigma=0.952563 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 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 = 0.00026428 Jy ! Component: 100 - total flux cleaned = 0.000523069 Jy ! Component: 150 - total flux cleaned = 0.000681143 Jy ! Component: 200 - total flux cleaned = 0.000873212 Jy ! Total flux subtracted in 200 components = 0.000873212 Jy ! Clean residual min=-0.003133 max=0.002822 Jy/beam ! Clean residual mean=0.000020 rms=0.000768 Jy/beam ! Combined flux in latest and established models = 0.595878 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 113 components and 0.595878 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.098739Jy sigma=0.952988 ! Fit after self-cal, rms=0.098715Jy sigma=0.952906 ! Inverting map ! Your choice of large map pixels excluded 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 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 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! Estimated beam: bmin=0.6317 mas, bmaj=0.8317 mas, bpa=-11.45 degrees ! Estimated noise=0.629809 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6317 x 0.8317 at -11.45 degrees (North through East) ! Clean map min=-0.0026531 max=0.41263 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 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! Estimated beam: bmin=0.5333 mas, bmaj=0.8211 mas, bpa=-10.54 degrees ! Estimated noise=0.876101 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.32814 Jy ! Component: 100 - total flux cleaned = 0.438519 Jy ! Component: 150 - total flux cleaned = 0.493971 Jy ! Component: 200 - total flux cleaned = 0.521631 Jy ! Total flux subtracted in 200 components = 0.521631 Jy ! Clean residual min=-0.020011 max=0.020247 Jy/beam ! Clean residual mean=0.000019 rms=0.002081 Jy/beam ! Combined flux in latest and established models = 0.521631 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 14 model components to the UV plane model. ! The established model now contains 14 components and 0.521631 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! Estimated beam: bmin=0.6317 mas, bmaj=0.8317 mas, bpa=-11.45 degrees ! Estimated noise=0.629809 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 = 0.0236811 Jy ! Component: 100 - total flux cleaned = 0.0286874 Jy ! Component: 150 - total flux cleaned = 0.0328993 Jy ! Component: 200 - total flux cleaned = 0.036431 Jy ! Total flux subtracted in 200 components = 0.036431 Jy ! Clean residual min=-0.010962 max=0.010922 Jy/beam ! Clean residual mean=0.000018 rms=0.001369 Jy/beam ! Combined flux in latest and established models = 0.558062 Jy ! Adding 17 model components to the UV plane model. ! The established model now contains 23 components and 0.558062 Jy ! Inverting map ! Your choice of large map pixels excluded 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 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 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! Estimated beam: bmin=2.566 mas, bmaj=2.888 mas, bpa=-35.96 degrees ! Estimated noise=0.838225 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0131103 Jy ! Component: 100 - total flux cleaned = 0.0202009 Jy ! Component: 150 - total flux cleaned = 0.0248839 Jy ! Component: 200 - total flux cleaned = 0.0283057 Jy ! Total flux subtracted in 200 components = 0.0283057 Jy ! Clean residual min=-0.003809 max=0.003626 Jy/beam ! Clean residual mean=0.000025 rms=0.000850 Jy/beam ! Combined flux in latest and established models = 0.586367 Jy flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00265587 Jy ! Component: 100 - total flux cleaned = 0.0047345 Jy ! Component: 150 - total flux cleaned = 0.00637493 Jy ! Component: 200 - total flux cleaned = 0.00733914 Jy ! Total flux subtracted in 200 components = 0.00733914 Jy ! Clean residual min=-0.003401 max=0.002859 Jy/beam ! Clean residual mean=0.000021 rms=0.000780 Jy/beam ! Combined flux in latest and established models = 0.593707 Jy ! Adding 47 model components to the UV plane model. ! The established model now contains 69 components and 0.593707 Jy ! Inverting map ! Your choice of large map pixels excluded 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! Estimated beam: bmin=0.6317 mas, bmaj=0.8317 mas, bpa=-11.45 degrees ! Estimated noise=0.629809 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00227408 Jy ! Component: 100 - total flux cleaned = -0.00225137 Jy ! Component: 150 - total flux cleaned = -0.00180539 Jy ! Component: 200 - total flux cleaned = -0.0014413 Jy ! Total flux subtracted in 200 components = -0.0014413 Jy ! Clean residual min=-0.006027 max=0.006855 Jy/beam ! Clean residual mean=0.000008 rms=0.000903 Jy/beam ! Combined flux in latest and established models = 0.592266 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 73 components and 0.592266 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.102406Jy sigma=0.992854 ! Fit after self-cal, rms=0.101918Jy sigma=0.988339 wmodel J1254+1141_X_map.mod ! Writing 73 model components to file: J1254+1141_X_map.mod wobs J1254+1141_X_uvs.fits ! Writing UV FITS file: J1254+1141_X_uvs.fits wwins J1254+1141_X_map.win ! wwins: Wrote 10 windows to J1254+1141_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 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000590515 Jy ! Component: 100 - total flux cleaned = 0.000236325 Jy ! Component: 150 - total flux cleaned = 0.000236135 Jy ! Component: 200 - total flux cleaned = 0.000233522 Jy ! Component: 250 - total flux cleaned = 0.00032961 Jy ! Component: 300 - total flux cleaned = 0.000328426 Jy ! Component: 350 - total flux cleaned = 0.000511298 Jy ! Component: 400 - total flux cleaned = 0.000596669 Jy ! Component: 450 - total flux cleaned = 0.000595162 Jy ! Component: 500 - total flux cleaned = 0.000674166 Jy ! Component: 550 - total flux cleaned = 0.000750396 Jy ! Component: 600 - total flux cleaned = 0.000898176 Jy ! Component: 650 - total flux cleaned = 0.00103919 Jy ! Component: 700 - total flux cleaned = 0.00124314 Jy ! Component: 750 - total flux cleaned = 0.00150501 Jy ! Component: 800 - total flux cleaned = 0.0017582 Jy ! Component: 850 - total flux cleaned = 0.00206529 Jy ! Component: 900 - total flux cleaned = 0.00218445 Jy ! Component: 950 - total flux cleaned = 0.00224275 Jy ! Component: 1000 - total flux cleaned = 0.00235639 Jy ! Component: 1050 - total flux cleaned = 0.0024663 Jy ! Component: 1100 - total flux cleaned = 0.00262771 Jy ! Component: 1150 - total flux cleaned = 0.00268165 Jy ! Component: 1200 - total flux cleaned = 0.00283773 Jy ! Component: 1250 - total flux cleaned = 0.00278676 Jy ! Component: 1300 - total flux cleaned = 0.0028365 Jy ! Component: 1350 - total flux cleaned = 0.00273647 Jy ! Component: 1400 - total flux cleaned = 0.00259132 Jy ! Component: 1450 - total flux cleaned = 0.00259138 Jy ! Component: 1500 - total flux cleaned = 0.00254427 Jy ! Component: 1550 - total flux cleaned = 0.00249809 Jy ! Component: 1600 - total flux cleaned = 0.00245199 Jy ! Component: 1650 - total flux cleaned = 0.00236134 Jy ! Component: 1700 - total flux cleaned = 0.00222707 Jy ! Component: 1750 - total flux cleaned = 0.00218343 Jy ! Component: 1800 - total flux cleaned = 0.0021405 Jy ! Component: 1850 - total flux cleaned = 0.00205364 Jy ! Component: 1900 - total flux cleaned = 0.00188337 Jy ! Component: 1950 - total flux cleaned = 0.00205212 Jy ! Component: 2000 - total flux cleaned = 0.00180145 Jy ! Component: 2050 - total flux cleaned = 0.00200793 Jy ! Component: 2100 - total flux cleaned = 0.00204875 Jy ! Component: 2150 - total flux cleaned = 0.00212881 Jy ! Component: 2200 - total flux cleaned = 0.00216859 Jy ! Component: 2250 - total flux cleaned = 0.00220823 Jy ! Component: 2300 - total flux cleaned = 0.0021692 Jy ! Component: 2350 - total flux cleaned = 0.0022864 Jy ! Component: 2400 - total flux cleaned = 0.00224761 Jy ! Component: 2450 - total flux cleaned = 0.00236243 Jy ! Component: 2500 - total flux cleaned = 0.00243841 Jy ! Component: 2550 - total flux cleaned = 0.00247559 Jy ! Component: 2600 - total flux cleaned = 0.00243817 Jy ! Component: 2650 - total flux cleaned = 0.00240198 Jy ! Component: 2700 - total flux cleaned = 0.00247585 Jy ! Component: 2750 - total flux cleaned = 0.00251207 Jy ! Component: 2800 - total flux cleaned = 0.00236742 Jy ! Component: 2850 - total flux cleaned = 0.00240388 Jy ! Component: 2900 - total flux cleaned = 0.00254628 Jy ! Component: 2950 - total flux cleaned = 0.00244025 Jy ! Component: 3000 - total flux cleaned = 0.0024753 Jy ! Component: 3050 - total flux cleaned = 0.00247508 Jy ! Component: 3100 - total flux cleaned = 0.00257858 Jy ! Component: 3150 - total flux cleaned = 0.00257847 Jy ! Component: 3200 - total flux cleaned = 0.00261267 Jy ! Component: 3250 - total flux cleaned = 0.00261264 Jy ! Component: 3300 - total flux cleaned = 0.00257888 Jy ! Component: 3350 - total flux cleaned = 0.00271266 Jy ! Component: 3400 - total flux cleaned = 0.00271276 Jy ! Component: 3450 - total flux cleaned = 0.00261353 Jy ! Component: 3500 - total flux cleaned = 0.00261392 Jy ! Component: 3550 - total flux cleaned = 0.00267938 Jy ! Component: 3600 - total flux cleaned = 0.00284175 Jy ! Component: 3650 - total flux cleaned = 0.0029063 Jy ! Component: 3700 - total flux cleaned = 0.00300265 Jy ! Component: 3750 - total flux cleaned = 0.0030664 Jy ! Component: 3800 - total flux cleaned = 0.00316166 Jy ! Component: 3850 - total flux cleaned = 0.00322428 Jy ! Component: 3900 - total flux cleaned = 0.00338105 Jy ! Component: 3950 - total flux cleaned = 0.00334988 Jy ! Component: 4000 - total flux cleaned = 0.0034737 Jy ! Component: 4050 - total flux cleaned = 0.00344276 Jy ! Total flux subtracted in 4096 components = 0.00362666 Jy ! Clean residual min=-0.001816 max=0.001597 Jy/beam ! Clean residual mean=0.000007 rms=0.000478 Jy/beam ! Combined flux in latest and established models = 0.595892 Jy keep ! Adding 279 model components to the UV plane model. ! The established model now contains 342 components and 0.595892 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv120_uvs/J1254+1141_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6317 x 0.8317 at -11.45 degrees (North through East) ! Clean map min=-0.0023198 max=0.41203 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv120_uvs/J1254+1141_X_map.fits wmodel /scr/pima/rv120_uvs/J1254+1141_X_map.mod ! Writing 342 model components to file: /scr/pima/rv120_uvs/J1254+1141_X_map.mod wobs /scr/pima/rv120_uvs/J1254+1141_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv120_uvs/J1254+1141_X_uvs.fits wwins /scr/pima/rv120_uvs/J1254+1141_X_map.win ! wwins: Wrote 11 windows to /scr/pima/rv120_uvs/J1254+1141_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.412025 invert ! Inverting map ! Your choice of large map pixels excluded 10.7% of the data. ! The x-axis pixel size should ideally be below 0.1663 milli-arcsec ! The y-axis pixel size should ideally be below 0.1765 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000478184 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.348171 0.348171 0.696343 1.39269 2.78537 5.57074 11.1415 22.283 44.5659 89.1319 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0014 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.412 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 861.644 quit ! Quitting program ! Log file /scr/pima/rv120_uvs/J1254+1141_X_dfm.log closed on Fri Dec 22 22:42:22 2017