! Started logfile: /scr/pima/rv125_uvs/J1848+3219_X_dfm.log on Sun Dec 23 02:53:16 2018 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/rv125_uvs/J1848+3219_X_uva.fits ! Reading UV FITS file: /scr/pima/rv125_uvs/J1848+3219_X_uva.fits ! AN table 1: 50 integrations on 55 of 55 possible baselines. ! AN table 2: 37 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.277237 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1848+3219 ! ! 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 69 lines of history. ! ! Reading 4896 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 J1848+3219_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 print "===============================================================" ! =============================================================== ! print "=== Difmap script: pima_mupet_01.dvm version of 2016.05.19 === " ! === Difmap script: pima_mupet_01.dvm version of 2016.05.19 === ! 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 370 telescope corrections were flagged in sub-array 1. ! A total of 184 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 2. ! A total of 370 telescope corrections were flagged in sub-array 1. ! A total of 184 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 3. ! A total of 442 telescope corrections were flagged in sub-array 1. ! A total of 194 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 4. ! A total of 442 telescope corrections were flagged in sub-array 1. ! A total of 194 telescope corrections were flagged in sub-array 2. ! ! Fit before self-cal, rms=1.128201Jy sigma=17.255349 ! Fit after self-cal, rms=0.484755Jy sigma=7.223192 ! 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 3.6% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! Estimated beam: bmin=0.7048 mas, bmaj=0.9097 mas, bpa=23.5 degrees ! Estimated noise=1.07372 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 = 0.408464 Jy ! Component: 100 - total flux cleaned = 0.504669 Jy ! Total flux subtracted in 100 components = 0.504669 Jy ! Clean residual min=-0.014472 max=0.037741 Jy/beam ! Clean residual mean=-0.000041 rms=0.003365 Jy/beam ! Combined flux in latest and established models = 0.504669 Jy ! Performing phase self-cal ! Adding 3 model components to the UV plane model. ! The established model now contains 3 components and 0.504669 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.133031Jy sigma=1.791951 ! Fit after self-cal, rms=0.132963Jy sigma=1.791378 ! Inverting map ! Your choice of large map pixels excluded 3.6% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0395089 Jy ! Component: 100 - total flux cleaned = 0.0588213 Jy ! Total flux subtracted in 100 components = 0.0588213 Jy ! Clean residual min=-0.013535 max=0.016709 Jy/beam ! Clean residual mean=-0.000031 rms=0.002760 Jy/beam ! Combined flux in latest and established models = 0.56349 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 8 components and 0.56349 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.123401Jy sigma=1.557590 ! Fit after self-cal, rms=0.123341Jy sigma=1.556913 ! Inverting map ! Your choice of large map pixels excluded 3.6% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 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 3.6% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! Estimated beam: bmin=0.8512 mas, bmaj=1.079 mas, bpa=12.77 degrees ! Estimated noise=0.811913 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 = 0.00824398 Jy ! Component: 100 - total flux cleaned = 0.00825695 Jy ! Component: 150 - total flux cleaned = 0.00826624 Jy ! Component: 200 - total flux cleaned = 0.00827414 Jy ! Total flux subtracted in 200 components = 0.00827414 Jy ! Clean residual min=-0.013659 max=0.018758 Jy/beam ! Clean residual mean=-0.000083 rms=0.003667 Jy/beam ! Combined flux in latest and established models = 0.571764 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 12 components and 0.571764 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.122618Jy sigma=1.539863 ! Fit after self-cal, rms=0.122563Jy sigma=1.539346 ! Inverting map ! Your choice of large map pixels excluded 3.6% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8512 x 1.079 at 12.77 degrees (North through East) ! Clean map min=-0.012889 max=0.51981 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 60 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 HH 0.83 HN 1.04 KP 1.13 ! LA 0.99 MC 0.84 NL 1.10 NY 0.83 ! PT 0.85 SC 0.95 WN 1.35 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 HN 1.06 KP 1.06 LA 1.00 ! MK 1.00 NL 1.04 NY 0.87 OV 0.94 ! PT 0.85 SC 0.94 ! ! ! Correcting IF 2. ! A total of 60 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 HH 0.81 HN 1.02 KP 1.07 ! LA 1.00 MC 0.89 NL 1.13 NY 0.94 ! PT 0.89 SC 0.98 WN 1.37 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 HN 1.05 KP 1.05 LA 1.01 ! MK 0.99 NL 1.03 NY 0.94 OV 0.95 ! PT 0.84 SC 0.95 ! ! ! Correcting IF 3. ! A total of 36 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 HH 0.91 HN 1.01 KP 1.14 ! LA 0.99 MC 1.26 NL 1.11 NY 1.00* ! PT 0.92 SC 1.01 WN 1.31 ! ! A total of 18 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 HN 1.07 KP 1.07 LA 1.02 ! MK 1.00 NL 1.05 NY 1.00* OV 0.96 ! PT 0.83 SC 0.97 ! ! ! Correcting IF 4. ! A total of 36 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 HH 1.14 HN 1.00 KP 1.13 ! LA 1.01 MC 1.25 NL 1.10 NY 1.00* ! PT 0.91 SC 1.00 WN 1.25 ! ! A total of 18 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 HN 1.08 KP 1.07 LA 1.02 ! MK 1.01 NL 1.05 NY 1.00* OV 0.96 ! PT 0.84 SC 0.94 ! ! ! Fit before self-cal, rms=0.122563Jy sigma=1.539346 ! Fit after self-cal, rms=0.092209Jy sigma=1.054364 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! Estimated beam: bmin=0.8514 mas, bmaj=1.102 mas, bpa=12.5 degrees ! Estimated noise=0.826328 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, 1.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00173095 Jy ! Component: 100 - total flux cleaned = 0.00198736 Jy ! Component: 150 - total flux cleaned = 0.00217936 Jy ! Component: 200 - total flux cleaned = 0.0026951 Jy ! Total flux subtracted in 200 components = 0.0026951 Jy ! Clean residual min=-0.005949 max=0.006590 Jy/beam ! Clean residual mean=-0.000001 rms=0.001287 Jy/beam ! Combined flux in latest and established models = 0.574459 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 23 components and 0.574459 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.090317Jy sigma=1.032693 ! Fit after self-cal, rms=0.090304Jy sigma=1.030019 ! Inverting map ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 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=0.090304Jy sigma=1.030019 ! Fit after self-cal, rms=0.081060Jy sigma=0.915067 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! Estimated beam: bmin=0.8497 mas, bmaj=1.103 mas, bpa=12.59 degrees ! Estimated noise=0.823583 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00129915 Jy ! Component: 100 - total flux cleaned = 0.00104618 Jy ! Component: 150 - total flux cleaned = 0.000844559 Jy ! Component: 200 - total flux cleaned = 0.000928623 Jy ! Total flux subtracted in 200 components = 0.000928623 Jy ! Clean residual min=-0.003307 max=0.003908 Jy/beam ! Clean residual mean=-0.000006 rms=0.000807 Jy/beam ! Combined flux in latest and established models = 0.575388 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 30 components and 0.575388 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080557Jy sigma=0.908882 ! Fit after self-cal, rms=0.080526Jy sigma=0.908101 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 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 (-14.6, -33.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00229579 Jy ! Component: 100 - total flux cleaned = 0.00269051 Jy ! Component: 150 - total flux cleaned = 0.0026894 Jy ! Component: 200 - total flux cleaned = 0.00284368 Jy ! Total flux subtracted in 200 components = 0.00284368 Jy ! Clean residual min=-0.003207 max=0.003371 Jy/beam ! Clean residual mean=-0.000003 rms=0.000789 Jy/beam ! Combined flux in latest and established models = 0.578232 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 39 components and 0.578232 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080192Jy sigma=0.904325 ! Fit after self-cal, rms=0.080169Jy sigma=0.903935 ! Inverting map ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! Added new window around map position (-18.2, -4.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00234264 Jy ! Component: 100 - total flux cleaned = 0.00324189 Jy ! Component: 150 - total flux cleaned = 0.00360889 Jy ! Component: 200 - total flux cleaned = 0.00381581 Jy ! Total flux subtracted in 200 components = 0.00381581 Jy ! Clean residual min=-0.003082 max=0.003404 Jy/beam ! Clean residual mean=0.000000 rms=0.000772 Jy/beam ! Combined flux in latest and established models = 0.582047 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 47 components and 0.582048 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.079893Jy sigma=0.901143 ! Fit after self-cal, rms=0.079874Jy sigma=0.900931 ! Inverting map ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! Added new window around map position (24, -32.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00239335 Jy ! Component: 100 - total flux cleaned = 0.00299742 Jy ! Component: 150 - total flux cleaned = 0.00327262 Jy ! Component: 200 - total flux cleaned = 0.00346726 Jy ! Total flux subtracted in 200 components = 0.00346726 Jy ! Clean residual min=-0.003101 max=0.003130 Jy/beam ! Clean residual mean=0.000001 rms=0.000759 Jy/beam ! Combined flux in latest and established models = 0.585515 Jy ! Performing phase self-cal ! Adding 33 model components to the UV plane model. ! The established model now contains 59 components and 0.585515 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.079668Jy sigma=0.898410 ! Fit after self-cal, rms=0.079658Jy sigma=0.898215 ! Inverting map ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 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=0.079658Jy sigma=0.898215 ! Fit after self-cal, rms=0.079672Jy sigma=0.881583 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! Estimated beam: bmin=0.8497 mas, bmaj=1.103 mas, bpa=12.59 degrees ! Estimated noise=0.823256 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000160068 Jy ! Component: 100 - total flux cleaned = -0.000290171 Jy ! Component: 150 - total flux cleaned = -0.000288895 Jy ! Component: 200 - total flux cleaned = -0.000288201 Jy ! Total flux subtracted in 200 components = -0.000288201 Jy ! Clean residual min=-0.002849 max=0.003166 Jy/beam ! Clean residual mean=0.000003 rms=0.000686 Jy/beam ! Combined flux in latest and established models = 0.585227 Jy selfcal ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 69 components and 0.585226 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.079523Jy sigma=0.879744 ! Fit after self-cal, rms=0.079535Jy sigma=0.879565 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 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 (-35.4, 43.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0022812 Jy ! Component: 100 - total flux cleaned = 0.00263165 Jy ! Component: 150 - total flux cleaned = 0.00275676 Jy ! Component: 200 - total flux cleaned = 0.00293209 Jy ! Total flux subtracted in 200 components = 0.00293209 Jy ! Clean residual min=-0.002829 max=0.003034 Jy/beam ! Clean residual mean=0.000001 rms=0.000676 Jy/beam ! Combined flux in latest and established models = 0.588158 Jy ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 82 components and 0.588158 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.079349Jy sigma=0.877313 ! Fit after self-cal, rms=0.079343Jy sigma=0.877104 ! Inverting map ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! Added new window around map position (-30.6, -12.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00229261 Jy ! Component: 100 - total flux cleaned = 0.00269701 Jy ! Component: 150 - total flux cleaned = 0.0028738 Jy ! Component: 200 - total flux cleaned = 0.00287488 Jy ! Total flux subtracted in 200 components = 0.00287488 Jy ! Clean residual min=-0.002888 max=0.002978 Jy/beam ! Clean residual mean=-0.000002 rms=0.000665 Jy/beam ! Combined flux in latest and established models = 0.591033 Jy ! Performing phase self-cal ! Adding 36 model components to the UV plane model. ! The established model now contains 97 components and 0.591033 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.079172Jy sigma=0.875216 ! Fit after self-cal, rms=0.079155Jy sigma=0.875062 ! Inverting map ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! Added new window around map position (-26.2, 21.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00212508 Jy ! Component: 100 - total flux cleaned = 0.00247601 Jy ! Component: 150 - total flux cleaned = 0.00266631 Jy ! Component: 200 - total flux cleaned = 0.00272376 Jy ! Total flux subtracted in 200 components = 0.00272376 Jy ! Clean residual min=-0.002778 max=0.002639 Jy/beam ! Clean residual mean=-0.000001 rms=0.000650 Jy/beam ! Combined flux in latest and established models = 0.593757 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 106 components and 0.593757 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.078998Jy sigma=0.872573 ! Fit after self-cal, rms=0.078979Jy sigma=0.872456 ! Inverting map ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 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=0.078979Jy sigma=0.872456 ! Fit after self-cal, rms=0.078915Jy sigma=0.871824 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! Estimated beam: bmin=2.447 mas, bmaj=2.558 mas, bpa=39.05 degrees ! Estimated noise=1.03845 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00153706 Jy ! Component: 100 - total flux cleaned = 0.00198643 Jy ! Component: 150 - total flux cleaned = 0.00205881 Jy ! Component: 200 - total flux cleaned = 0.00212376 Jy ! Total flux subtracted in 200 components = 0.00212376 Jy ! Clean residual min=-0.002982 max=0.002640 Jy/beam ! Clean residual mean=-0.000003 rms=0.000745 Jy/beam ! Combined flux in latest and established models = 0.595881 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 125 components and 0.595881 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.078907Jy sigma=0.871497 ! Fit after self-cal, rms=0.078905Jy sigma=0.871443 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 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 = 0.000281409 Jy ! Component: 100 - total flux cleaned = 0.000403376 Jy ! Component: 150 - total flux cleaned = 0.000487351 Jy ! Component: 200 - total flux cleaned = 0.000565261 Jy ! Total flux subtracted in 200 components = 0.000565261 Jy ! Clean residual min=-0.002975 max=0.002650 Jy/beam ! Clean residual mean=-0.000004 rms=0.000740 Jy/beam ! Combined flux in latest and established models = 0.596446 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 138 components and 0.596446 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.078906Jy sigma=0.871296 ! Fit after self-cal, rms=0.078904Jy sigma=0.871272 ! Inverting map ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 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 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! Estimated beam: bmin=0.8496 mas, bmaj=1.103 mas, bpa=12.59 degrees ! Estimated noise=0.822889 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8496 x 1.103 at 12.59 degrees (North through East) ! Clean map min=-0.0025737 max=0.51691 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 ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.078904Jy sigma=0.871272 ! Fit after self-cal, rms=0.074871Jy sigma=0.806671 ! Inverting map and beam ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! Estimated beam: bmin=0.8496 mas, bmaj=1.103 mas, bpa=12.54 degrees ! Estimated noise=0.822658 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -5.16543e-05 Jy ! Component: 100 - total flux cleaned = 0.000127947 Jy ! Component: 150 - total flux cleaned = 0.000238647 Jy ! Component: 200 - total flux cleaned = 0.000344518 Jy ! Total flux subtracted in 200 components = 0.000344518 Jy ! Clean residual min=-0.002741 max=0.002562 Jy/beam ! Clean residual mean=-0.000002 rms=0.000632 Jy/beam ! Combined flux in latest and established models = 0.59679 Jy ! Performing phase self-cal ! Adding 36 model components to the UV plane model. ! The established model now contains 144 components and 0.596791 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.074756Jy sigma=0.805298 ! Fit after self-cal, rms=0.074744Jy sigma=0.805240 ! Inverting map ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -1.49732e-05 Jy ! Component: 100 - total flux cleaned = 9.01675e-05 Jy ! Component: 150 - total flux cleaned = 0.000191736 Jy ! Component: 200 - total flux cleaned = 0.000340264 Jy ! Total flux subtracted in 200 components = 0.000340264 Jy ! Clean residual min=-0.002725 max=0.002527 Jy/beam ! Clean residual mean=-0.000002 rms=0.000628 Jy/beam ! Combined flux in latest and established models = 0.597131 Jy ! Performing phase self-cal ! Adding 46 model components to the UV plane model. ! The established model now contains 150 components and 0.597131 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.074655Jy sigma=0.804239 ! Fit after self-cal, rms=0.074645Jy sigma=0.804195 ! Inverting map ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.074645Jy sigma=0.804195 ! Fit after self-cal, rms=0.074637Jy sigma=0.804120 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 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! Estimated beam: bmin=0.6978 mas, bmaj=0.9272 mas, bpa=23.9 degrees ! Estimated noise=1.09273 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.405752 Jy ! Component: 100 - total flux cleaned = 0.500271 Jy ! Component: 150 - total flux cleaned = 0.534039 Jy ! Component: 200 - total flux cleaned = 0.550346 Jy ! Total flux subtracted in 200 components = 0.550346 Jy ! Clean residual min=-0.004985 max=0.008149 Jy/beam ! Clean residual mean=-0.000008 rms=0.001154 Jy/beam ! Combined flux in latest and established models = 0.550346 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 0.550346 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! Estimated beam: bmin=0.8497 mas, bmaj=1.103 mas, bpa=12.52 degrees ! Estimated noise=0.822464 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 = 0.012005 Jy ! Component: 100 - total flux cleaned = 0.0190712 Jy ! Component: 150 - total flux cleaned = 0.0242693 Jy ! Component: 200 - total flux cleaned = 0.0285302 Jy ! Total flux subtracted in 200 components = 0.0285302 Jy ! Clean residual min=-0.003449 max=0.003036 Jy/beam ! Clean residual mean=-0.000007 rms=0.000725 Jy/beam ! Combined flux in latest and established models = 0.578876 Jy ! Adding 22 model components to the UV plane model. ! The established model now contains 30 components and 0.578876 Jy ! Inverting map ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 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 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! Estimated beam: bmin=2.446 mas, bmaj=2.558 mas, bpa=38.72 degrees ! Estimated noise=1.03788 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00400295 Jy ! Component: 100 - total flux cleaned = 0.00687405 Jy ! Component: 150 - total flux cleaned = 0.00925418 Jy ! Component: 200 - total flux cleaned = 0.0112595 Jy ! Total flux subtracted in 200 components = 0.0112595 Jy ! Clean residual min=-0.003138 max=0.002733 Jy/beam ! Clean residual mean=-0.000011 rms=0.000768 Jy/beam ! Combined flux in latest and established models = 0.590135 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 = 0.00156963 Jy ! Component: 100 - total flux cleaned = 0.00268768 Jy ! Component: 150 - total flux cleaned = 0.00366951 Jy ! Component: 200 - total flux cleaned = 0.0045334 Jy ! Total flux subtracted in 200 components = 0.0045334 Jy ! Clean residual min=-0.003005 max=0.002803 Jy/beam ! Clean residual mean=-0.000007 rms=0.000748 Jy/beam ! Combined flux in latest and established models = 0.594669 Jy ! Adding 40 model components to the UV plane model. ! The established model now contains 67 components and 0.594669 Jy ! Inverting map ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! Estimated beam: bmin=0.8497 mas, bmaj=1.103 mas, bpa=12.52 degrees ! Estimated noise=0.822464 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000112628 Jy ! Component: 100 - total flux cleaned = 0.000742345 Jy ! Component: 150 - total flux cleaned = 0.00142775 Jy ! Component: 200 - total flux cleaned = 0.00170295 Jy ! Total flux subtracted in 200 components = 0.00170295 Jy ! Clean residual min=-0.002908 max=0.002760 Jy/beam ! Clean residual mean=-0.000004 rms=0.000666 Jy/beam ! Combined flux in latest and established models = 0.596372 Jy selfcal ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 83 components and 0.596372 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.075045Jy sigma=0.813929 ! Fit after self-cal, rms=0.074978Jy sigma=0.812839 wmodel J1848+3219_X_map.mod ! Writing 83 model components to file: J1848+3219_X_map.mod wobs J1848+3219_X_uvs.fits ! Writing UV FITS file: J1848+3219_X_uvs.fits wwins J1848+3219_X_map.win ! wwins: Wrote 8 windows to J1848+3219_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 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00037554 Jy ! Component: 100 - total flux cleaned = -0.000526583 Jy ! Component: 150 - total flux cleaned = -0.000527897 Jy ! Component: 200 - total flux cleaned = -0.000622473 Jy ! Component: 250 - total flux cleaned = -0.000761906 Jy ! Component: 300 - total flux cleaned = -0.000944114 Jy ! Component: 350 - total flux cleaned = -0.000944255 Jy ! Component: 400 - total flux cleaned = -0.000988198 Jy ! Component: 450 - total flux cleaned = -0.00111954 Jy ! Component: 500 - total flux cleaned = -0.00120554 Jy ! Component: 550 - total flux cleaned = -0.00141908 Jy ! Component: 600 - total flux cleaned = -0.00146136 Jy ! Component: 650 - total flux cleaned = -0.00162884 Jy ! Component: 700 - total flux cleaned = -0.00183614 Jy ! Component: 750 - total flux cleaned = -0.00200061 Jy ! Component: 800 - total flux cleaned = -0.00208234 Jy ! Component: 850 - total flux cleaned = -0.00216308 Jy ! Component: 900 - total flux cleaned = -0.0022431 Jy ! Component: 950 - total flux cleaned = -0.00244269 Jy ! Component: 1000 - total flux cleaned = -0.00260051 Jy ! Component: 1050 - total flux cleaned = -0.00295273 Jy ! Component: 1100 - total flux cleaned = -0.00302999 Jy ! Component: 1150 - total flux cleaned = -0.00302992 Jy ! Component: 1200 - total flux cleaned = -0.00322154 Jy ! Component: 1250 - total flux cleaned = -0.00344926 Jy ! Component: 1300 - total flux cleaned = -0.0033363 Jy ! Component: 1350 - total flux cleaned = -0.00352408 Jy ! Component: 1400 - total flux cleaned = -0.00371059 Jy ! Component: 1450 - total flux cleaned = -0.0037841 Jy ! Component: 1500 - total flux cleaned = -0.00396879 Jy ! Component: 1550 - total flux cleaned = -0.00400523 Jy ! Component: 1600 - total flux cleaned = -0.00396893 Jy ! Component: 1650 - total flux cleaned = -0.00425862 Jy ! Component: 1700 - total flux cleaned = -0.0045461 Jy ! Component: 1750 - total flux cleaned = -0.00465325 Jy ! Component: 1800 - total flux cleaned = -0.00468855 Jy ! Component: 1850 - total flux cleaned = -0.00483021 Jy ! Component: 1900 - total flux cleaned = -0.0048657 Jy ! Component: 1950 - total flux cleaned = -0.00500534 Jy ! Component: 2000 - total flux cleaned = -0.0050405 Jy ! Component: 2050 - total flux cleaned = -0.00514444 Jy ! Component: 2100 - total flux cleaned = -0.00524774 Jy ! Component: 2150 - total flux cleaned = -0.00548739 Jy ! Component: 2200 - total flux cleaned = -0.00548728 Jy ! Component: 2250 - total flux cleaned = -0.00555481 Jy ! Component: 2300 - total flux cleaned = -0.00575697 Jy ! Component: 2350 - total flux cleaned = -0.00575747 Jy ! Component: 2400 - total flux cleaned = -0.00575766 Jy ! Component: 2450 - total flux cleaned = -0.00589023 Jy ! Component: 2500 - total flux cleaned = -0.00595642 Jy ! Component: 2550 - total flux cleaned = -0.00612078 Jy ! Component: 2600 - total flux cleaned = -0.00615335 Jy ! Component: 2650 - total flux cleaned = -0.0060882 Jy ! Component: 2700 - total flux cleaned = -0.0063151 Jy ! Component: 2750 - total flux cleaned = -0.00625027 Jy ! Component: 2800 - total flux cleaned = -0.00650746 Jy ! Component: 2850 - total flux cleaned = -0.00647537 Jy ! Component: 2900 - total flux cleaned = -0.00644365 Jy ! Component: 2950 - total flux cleaned = -0.00638035 Jy ! Component: 3000 - total flux cleaned = -0.00641188 Jy ! Component: 3050 - total flux cleaned = -0.00653781 Jy ! Component: 3100 - total flux cleaned = -0.0065377 Jy ! Component: 3150 - total flux cleaned = -0.00659978 Jy ! Component: 3200 - total flux cleaned = -0.00653794 Jy ! Component: 3250 - total flux cleaned = -0.0065692 Jy ! Component: 3300 - total flux cleaned = -0.00672304 Jy ! Component: 3350 - total flux cleaned = -0.0066312 Jy ! Component: 3400 - total flux cleaned = -0.00660058 Jy ! Component: 3450 - total flux cleaned = -0.00653998 Jy ! Component: 3500 - total flux cleaned = -0.00660041 Jy ! Component: 3550 - total flux cleaned = -0.00669111 Jy ! Component: 3600 - total flux cleaned = -0.00672122 Jy ! Component: 3650 - total flux cleaned = -0.00681098 Jy ! Component: 3700 - total flux cleaned = -0.00672128 Jy ! Component: 3750 - total flux cleaned = -0.00675084 Jy ! Component: 3800 - total flux cleaned = -0.0067804 Jy ! Component: 3850 - total flux cleaned = -0.00686892 Jy ! Component: 3900 - total flux cleaned = -0.00689841 Jy ! Component: 3950 - total flux cleaned = -0.00698614 Jy ! Component: 4000 - total flux cleaned = -0.00692788 Jy ! Component: 4050 - total flux cleaned = -0.00692796 Jy ! Total flux subtracted in 4096 components = -0.00689895 Jy ! Clean residual min=-0.001772 max=0.001817 Jy/beam ! Clean residual mean=-0.000001 rms=0.000476 Jy/beam ! Combined flux in latest and established models = 0.589473 Jy keep ! Adding 335 model components to the UV plane model. ! The established model now contains 417 components and 0.589473 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv125_uvs/J1848+3219_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8497 x 1.103 at 12.52 degrees (North through East) ! Clean map min=-0.0024372 max=0.51727 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv125_uvs/J1848+3219_X_map.fits wmodel /scr/pima/rv125_uvs/J1848+3219_X_map.mod ! Writing 417 model components to file: /scr/pima/rv125_uvs/J1848+3219_X_map.mod wobs /scr/pima/rv125_uvs/J1848+3219_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv125_uvs/J1848+3219_X_uvs.fits wwins /scr/pima/rv125_uvs/J1848+3219_X_map.win ! wwins: Wrote 9 windows to /scr/pima/rv125_uvs/J1848+3219_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.517271 invert ! Inverting map ! Your choice of large map pixels excluded 3.37% of the data. ! The x-axis pixel size should ideally be below 0.1926 milli-arcsec ! The y-axis pixel size should ideally be below 0.1713 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000475365 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.275696 0.275696 0.551392 1.10278 2.20557 4.41113 8.82227 17.6445 35.2891 70.5782 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0014 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.517 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1088.16 quit ! Quitting program ! Log file /scr/pima/rv125_uvs/J1848+3219_X_dfm.log closed on Sun Dec 23 02:53:20 2018