! Started logfile: /scr/pima/rv118_uvs/J0854+2006_X_dfm.log on Sun Dec 10 00:08:41 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/rv118_uvs/J0854+2006_X_uva.fits ! Reading UV FITS file: /scr/pima/rv118_uvs/J0854+2006_X_uva.fits ! AN table 1: 2 integrations on 21 of 21 possible baselines. ! AN table 2: 6 integrations on 10 of 10 possible baselines. ! AN table 3: 8 integrations on 45 of 45 possible baselines. ! AN table 4: 3 integrations on 1 of 1 possible baselines. ! AN table 5: 16 integrations on 6 of 6 possible baselines. ! AN table 6: 2 integrations on 10 of 10 possible baselines. ! AN table 7: 2 integrations on 10 of 10 possible baselines. ! AN table 8: 2 integrations on 10 of 10 possible baselines. ! AN table 9: 4 integrations on 36 of 36 possible baselines. ! AN table 10: 6 integrations on 6 of 6 possible baselines. ! Apparent sampling: 0.625468 visibilities/baseline/integration-bin. ! Found source: J0854+2006 ! ! 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 2004 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 J0854+2006_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 20 telescope corrections were flagged in sub-array 2. ! A total of 30 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 24 telescope corrections were flagged in sub-array 5. ! A total of 12 telescope corrections were flagged in sub-array 9. ! A total of 10 telescope corrections were flagged in sub-array 10. ! ! Correcting IF 2. ! A total of 20 telescope corrections were flagged in sub-array 2. ! A total of 30 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 24 telescope corrections were flagged in sub-array 5. ! A total of 12 telescope corrections were flagged in sub-array 9. ! A total of 10 telescope corrections were flagged in sub-array 10. ! ! Correcting IF 3. ! A total of 20 telescope corrections were flagged in sub-array 2. ! A total of 30 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 24 telescope corrections were flagged in sub-array 5. ! A total of 12 telescope corrections were flagged in sub-array 9. ! A total of 10 telescope corrections were flagged in sub-array 10. ! ! Correcting IF 4. ! A total of 20 telescope corrections were flagged in sub-array 2. ! A total of 30 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 24 telescope corrections were flagged in sub-array 5. ! A total of 12 telescope corrections were flagged in sub-array 9. ! A total of 10 telescope corrections were flagged in sub-array 10. ! ! Fit before self-cal, rms=3.774193Jy sigma=30.092925 ! Fit after self-cal, rms=2.630782Jy sigma=20.578821 ! 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 3.83% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.6439 mas, bmaj=0.8856 mas, bpa=0.4821 degrees ! Estimated noise=2.60917 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 = 2.64694 Jy ! Component: 100 - total flux cleaned = 3.31111 Jy ! Total flux subtracted in 100 components = 3.31111 Jy ! Clean residual min=-0.095587 max=0.268449 Jy/beam ! Clean residual mean=-0.000046 rms=0.019885 Jy/beam ! Combined flux in latest and established models = 3.31111 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 3.31111 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.680957Jy sigma=5.042379 ! Fit after self-cal, rms=0.679504Jy sigma=5.036210 ! Inverting map ! Your choice of large map pixels excluded 3.83% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.280706 Jy ! Component: 100 - total flux cleaned = 0.410401 Jy ! Total flux subtracted in 100 components = 0.410401 Jy ! Clean residual min=-0.080197 max=0.158694 Jy/beam ! Clean residual mean=-0.000024 rms=0.015952 Jy/beam ! Combined flux in latest and established models = 3.72151 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 9 components and 3.72151 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.532815Jy sigma=3.828651 ! Fit after self-cal, rms=0.530033Jy sigma=3.815518 ! Inverting map ! Your choice of large map pixels excluded 3.83% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Added new window around map position (-0.8, 0.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.147597 Jy ! Component: 100 - total flux cleaned = 0.172613 Jy ! Total flux subtracted in 100 components = 0.172613 Jy ! Clean residual min=-0.086888 max=0.107039 Jy/beam ! Clean residual mean=-0.000013 rms=0.014633 Jy/beam ! Combined flux in latest and established models = 3.89413 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 14 components and 3.89413 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.490084Jy sigma=3.513829 ! Fit after self-cal, rms=0.483175Jy sigma=3.463333 ! Inverting map ! Your choice of large map pixels excluded 3.83% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Added new window around map position (1, 0.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0319193 Jy ! Component: 100 - total flux cleaned = 0.0384272 Jy ! Total flux subtracted in 100 components = 0.0384272 Jy ! Clean residual min=-0.073788 max=0.076439 Jy/beam ! Clean residual mean=-0.000011 rms=0.013611 Jy/beam ! Combined flux in latest and established models = 3.93255 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 17 components and 3.93255 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.465229Jy sigma=3.319176 ! Fit after self-cal, rms=0.464061Jy sigma=3.309148 ! Inverting map ! Your choice of large map pixels excluded 3.83% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 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 3.83% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.7474 mas, bmaj=1.021 mas, bpa=-0.9651 degrees ! Estimated noise=2.33506 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 (-2.4, -0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0717534 Jy ! Component: 100 - total flux cleaned = 0.083456 Jy ! Component: 150 - total flux cleaned = 0.0898939 Jy ! Component: 200 - total flux cleaned = 0.0918546 Jy ! Total flux subtracted in 200 components = 0.0918546 Jy ! Clean residual min=-0.054353 max=0.052413 Jy/beam ! Clean residual mean=-0.000007 rms=0.011435 Jy/beam ! Combined flux in latest and established models = 4.02441 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 33 components and 4.02441 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.442058Jy sigma=3.123747 ! Fit after self-cal, rms=0.441127Jy sigma=3.116567 ! Inverting map ! Your choice of large map pixels excluded 3.83% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7474 x 1.021 at -0.9651 degrees (North through East) ! Clean map min=-0.052195 max=3.3965 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 FD 0.96 LA 0.98 NL 1.00 ! NY 1.05 OV 1.00 PT 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 HN 1.03 KK 1.01 MK 1.01 ! NY 1.06 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 1.16 HN 1.00 KK 1.01 ! KP 1.00 LA 1.00 NL 1.00 OV 0.99 ! PT 0.98 SC 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! KK 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! HH 0.83 NY 0.99 ON 1.02 WZ 0.98 ! ! Telescope amplitude corrections in sub-array 6: ! HH 0.62 HN 1.00 NL 1.30 ON 1.03 ! SC 0.96 ! ! Telescope amplitude corrections in sub-array 7: ! HH 4.03 LA 1.04 ON 0.99 SC 1.04 ! WZ 0.98 ! ! Telescope amplitude corrections in sub-array 8: ! FD 0.98 HH 0.63 KP 1.03 LA 1.03 ! PT 1.03 ! ! A total of 6 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! BR 1.04 FD 0.98 HN 1.01 LA 1.01 ! NL 1.00 OV 0.98 PT 1.03 SC 1.00 ! WZ 1.00 ! ! A total of 6 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! HN 1.01 NY 1.02 ON 1.01 WZ 1.00 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 0.96 LA 0.98 NL 1.00 ! NY 1.04 OV 1.00 PT 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 HN 1.04 KK 0.99 MK 0.99 ! NY 1.05 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 1.15 HN 0.99 KK 1.00 ! KP 1.01 LA 0.99 NL 1.00 OV 0.99 ! PT 1.00 SC 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! KK 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! HH 0.88 NY 1.00 ON 1.03 WZ 0.98 ! ! Telescope amplitude corrections in sub-array 6: ! HH 0.66 HN 0.99 NL 1.31 ON 1.04 ! SC 0.96 ! ! Telescope amplitude corrections in sub-array 7: ! HH 4.99 LA 1.00 ON 0.99 SC 1.02 ! WZ 1.00 ! ! Telescope amplitude corrections in sub-array 8: ! FD 0.97 HH 0.65 KP 1.03 LA 1.02 ! PT 1.03 ! ! A total of 6 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! BR 1.03 FD 0.98 HN 0.99 LA 0.99 ! NL 1.00 OV 0.99 PT 1.02 SC 1.00 ! WZ 1.01 ! ! A total of 6 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! HN 1.01 NY 1.03 ON 1.04 WZ 0.99 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.94 LA 0.97 NL 0.97 ! NY 1.03 OV 0.98 PT 0.96 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 HN 0.99 KK 1.00 MK 0.99 ! NY 1.04 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 1.06 HN 0.98 KK 0.99 ! KP 0.97 LA 0.95 NL 0.99 OV 1.01 ! PT 0.97 SC 0.96 ! ! Telescope amplitude corrections in sub-array 4: ! KK 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! HH 0.81 NY 0.98 ON 1.03 WZ 0.94 ! ! Telescope amplitude corrections in sub-array 6: ! HH 0.62 HN 0.98 NL 1.31 ON 1.00 ! SC 0.96 ! ! Telescope amplitude corrections in sub-array 7: ! HH 4.01 LA 1.01 ON 1.01 SC 1.01 ! WZ 0.96 ! ! Telescope amplitude corrections in sub-array 8: ! FD 0.95 HH 0.63 KP 1.01 LA 1.02 ! PT 1.04 ! ! A total of 6 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! BR 1.03 FD 0.97 HN 1.00 LA 0.98 ! NL 0.98 OV 0.99 PT 1.04 SC 0.95 ! WZ 0.96 ! ! A total of 6 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! HN 1.00 NY 0.99 ON 1.03 WZ 0.98 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.94 LA 0.96 NL 0.96 ! NY 1.03 OV 0.98 PT 0.94 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 HN 0.98 KK 0.99 MK 0.99 ! NY 1.05 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 1.08 HN 0.97 KK 1.00 ! KP 0.96 LA 0.98 NL 0.97 OV 0.98 ! PT 0.97 SC 0.94 ! ! Telescope amplitude corrections in sub-array 4: ! KK 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! HH 0.83 NY 0.97 ON 1.02 WZ 0.96 ! ! Telescope amplitude corrections in sub-array 6: ! HH 0.64 HN 0.98 NL 1.28 ON 1.00 ! SC 0.93 ! ! Telescope amplitude corrections in sub-array 7: ! HH 7.48 LA 1.02 ON 1.00 SC 0.98 ! WZ 0.95 ! ! Telescope amplitude corrections in sub-array 8: ! FD 0.96 HH 0.66 KP 1.00 LA 1.02 ! PT 1.02 ! ! A total of 6 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! BR 1.02 FD 0.96 HN 0.99 LA 0.98 ! NL 0.97 OV 0.97 PT 1.00 SC 0.96 ! WZ 0.95 ! ! A total of 6 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! HN 0.98 NY 1.01 ON 1.02 WZ 0.98 ! ! ! Fit before self-cal, rms=0.441127Jy sigma=3.116567 ! Fit after self-cal, rms=0.227599Jy sigma=1.525710 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.7566 mas, bmaj=1.032 mas, bpa=-4.213 degrees ! Estimated noise=2.36955 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 = 0.0204332 Jy ! Component: 100 - total flux cleaned = 0.0217011 Jy ! Component: 150 - total flux cleaned = 0.0228259 Jy ! Component: 200 - total flux cleaned = 0.0238585 Jy ! Total flux subtracted in 200 components = 0.0238585 Jy ! Clean residual min=-0.025396 max=0.026253 Jy/beam ! Clean residual mean=0.000008 rms=0.006348 Jy/beam ! Combined flux in latest and established models = 4.04827 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 45 components and 4.04827 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.223371Jy sigma=1.501346 ! Fit after self-cal, rms=0.223229Jy sigma=1.498291 ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 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=0.223229Jy sigma=1.498291 ! Fit after self-cal, rms=0.150741Jy sigma=0.925619 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.7556 mas, bmaj=1.032 mas, bpa=-4.166 degrees ! Estimated noise=2.36978 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0156261 Jy ! Component: 100 - total flux cleaned = 0.0193029 Jy ! Component: 150 - total flux cleaned = 0.0210573 Jy ! Component: 200 - total flux cleaned = 0.0214558 Jy ! Total flux subtracted in 200 components = 0.0214558 Jy ! Clean residual min=-0.013330 max=0.015102 Jy/beam ! Clean residual mean=-0.000005 rms=0.002481 Jy/beam ! Combined flux in latest and established models = 4.06972 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 52 components and 4.06972 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.146645Jy sigma=0.900002 ! Fit after self-cal, rms=0.146121Jy sigma=0.895988 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 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 (-4.2, 0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00912827 Jy ! Component: 100 - total flux cleaned = 0.00913238 Jy ! Component: 150 - total flux cleaned = 0.00950181 Jy ! Component: 200 - total flux cleaned = 0.00917529 Jy ! Total flux subtracted in 200 components = 0.00917529 Jy ! Clean residual min=-0.012268 max=0.012344 Jy/beam ! Clean residual mean=-0.000003 rms=0.002376 Jy/beam ! Combined flux in latest and established models = 4.0789 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 59 components and 4.0789 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.143811Jy sigma=0.879389 ! Fit after self-cal, rms=0.143587Jy sigma=0.877310 ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Added new window around map position (-2.8, -2.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00654142 Jy ! Component: 100 - total flux cleaned = 0.00824603 Jy ! Component: 150 - total flux cleaned = 0.00856691 Jy ! Component: 200 - total flux cleaned = 0.00884756 Jy ! Total flux subtracted in 200 components = 0.00884756 Jy ! Clean residual min=-0.011332 max=0.009937 Jy/beam ! Clean residual mean=-0.000001 rms=0.002300 Jy/beam ! Combined flux in latest and established models = 4.08775 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 67 components and 4.08775 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.141815Jy sigma=0.866709 ! Fit after self-cal, rms=0.141530Jy sigma=0.865222 ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 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=0.141530Jy sigma=0.865222 ! Fit after self-cal, rms=0.134645Jy sigma=0.818663 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.7552 mas, bmaj=1.031 mas, bpa=-4.135 degrees ! Estimated noise=2.36692 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0055439 Jy ! Component: 100 - total flux cleaned = 0.0079925 Jy ! Component: 150 - total flux cleaned = 0.00983065 Jy ! Component: 200 - total flux cleaned = 0.010659 Jy ! Total flux subtracted in 200 components = 0.010659 Jy ! Clean residual min=-0.009649 max=0.008347 Jy/beam ! Clean residual mean=-0.000006 rms=0.001826 Jy/beam ! Combined flux in latest and established models = 4.0984 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 76 components and 4.0984 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.132712Jy sigma=0.807232 ! Fit after self-cal, rms=0.132518Jy sigma=0.806016 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 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 = 0.000497799 Jy ! Component: 100 - total flux cleaned = 0.00150506 Jy ! Component: 150 - total flux cleaned = 0.00243968 Jy ! Component: 200 - total flux cleaned = 0.00331712 Jy ! Total flux subtracted in 200 components = 0.00331712 Jy ! Clean residual min=-0.009281 max=0.008178 Jy/beam ! Clean residual mean=-0.000005 rms=0.001782 Jy/beam ! Combined flux in latest and established models = 4.10172 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 79 components and 4.10172 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.131562Jy sigma=0.799786 ! Fit after self-cal, rms=0.131440Jy sigma=0.799099 ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 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=0.131440Jy sigma=0.799099 ! Fit after self-cal, rms=0.131000Jy sigma=0.796424 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=2.282 mas, bmaj=2.557 mas, bpa=-13.18 degrees ! Estimated noise=3.33943 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00903899 Jy ! Component: 100 - total flux cleaned = 0.0129142 Jy ! Component: 150 - total flux cleaned = 0.0137838 Jy ! Component: 200 - total flux cleaned = 0.014313 Jy ! Total flux subtracted in 200 components = 0.014313 Jy ! Clean residual min=-0.009513 max=0.009432 Jy/beam ! Clean residual mean=-0.000013 rms=0.002364 Jy/beam ! Combined flux in latest and established models = 4.11603 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 95 components and 4.11603 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.130485Jy sigma=0.795614 ! Fit after self-cal, rms=0.130465Jy sigma=0.794898 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 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 = 0.00227624 Jy ! Component: 100 - total flux cleaned = 0.00257163 Jy ! Component: 150 - total flux cleaned = 0.00299567 Jy ! Component: 200 - total flux cleaned = 0.00328305 Jy ! Total flux subtracted in 200 components = 0.00328305 Jy ! Clean residual min=-0.009433 max=0.009741 Jy/beam ! Clean residual mean=-0.000011 rms=0.002380 Jy/beam ! Combined flux in latest and established models = 4.11932 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 104 components and 4.11932 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.130282Jy sigma=0.794578 ! Fit after self-cal, rms=0.130273Jy sigma=0.794377 ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 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 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.755 mas, bmaj=1.03 mas, bpa=-4.131 degrees ! Estimated noise=2.36556 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.755 x 1.03 at -4.131 degrees (North through East) ! Clean map min=-0.027301 max=3.3935 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=0.130273Jy sigma=0.794377 ! Fit after self-cal, rms=0.117756Jy sigma=0.578922 ! Inverting map and beam ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.755 mas, bmaj=1.03 mas, bpa=-4.107 degrees ! Estimated noise=2.36537 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0019267 Jy ! Component: 100 - total flux cleaned = 0.00265845 Jy ! Component: 150 - total flux cleaned = 0.00351612 Jy ! Component: 200 - total flux cleaned = 0.00412045 Jy ! Total flux subtracted in 200 components = 0.00412045 Jy ! Clean residual min=-0.008891 max=0.008305 Jy/beam ! Clean residual mean=-0.000006 rms=0.001682 Jy/beam ! Combined flux in latest and established models = 4.12344 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 109 components and 4.12344 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.116685Jy sigma=0.570613 ! Fit after self-cal, rms=0.116582Jy sigma=0.570019 ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00013182 Jy ! Component: 100 - total flux cleaned = 0.000902319 Jy ! Component: 150 - total flux cleaned = 0.00144535 Jy ! Component: 200 - total flux cleaned = 0.00179809 Jy ! Total flux subtracted in 200 components = 0.00179809 Jy ! Clean residual min=-0.008641 max=0.008226 Jy/beam ! Clean residual mean=-0.000005 rms=0.001656 Jy/beam ! Combined flux in latest and established models = 4.12524 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 113 components and 4.12524 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.116006Jy sigma=0.564670 ! Fit after self-cal, rms=0.115932Jy sigma=0.564300 ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.115932Jy sigma=0.564300 ! Fit after self-cal, rms=0.115717Jy sigma=0.562954 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 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.6502 mas, bmaj=0.8891 mas, bpa=-1.916 degrees ! Estimated noise=2.63594 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.64077 Jy ! Component: 100 - total flux cleaned = 3.29941 Jy ! Component: 150 - total flux cleaned = 3.58979 Jy ! Component: 200 - total flux cleaned = 3.75012 Jy ! Total flux subtracted in 200 components = 3.75012 Jy ! Clean residual min=-0.023487 max=0.081933 Jy/beam ! Clean residual mean=-0.000028 rms=0.005852 Jy/beam ! Combined flux in latest and established models = 3.75012 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 3.75012 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.7549 mas, bmaj=1.03 mas, bpa=-4.115 degrees ! Estimated noise=2.36443 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 = 0.129964 Jy ! Component: 100 - total flux cleaned = 0.203351 Jy ! Component: 150 - total flux cleaned = 0.253158 Jy ! Component: 200 - total flux cleaned = 0.28917 Jy ! Total flux subtracted in 200 components = 0.28917 Jy ! Clean residual min=-0.015810 max=0.020744 Jy/beam ! Clean residual mean=-0.000021 rms=0.002742 Jy/beam ! Combined flux in latest and established models = 4.03929 Jy ! Adding 31 model components to the UV plane model. ! The established model now contains 34 components and 4.03929 Jy ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0274149 Jy ! Component: 100 - total flux cleaned = 0.0477662 Jy ! Component: 150 - total flux cleaned = 0.0574165 Jy ! Component: 200 - total flux cleaned = 0.0661596 Jy ! Total flux subtracted in 200 components = 0.0661596 Jy ! Clean residual min=-0.014656 max=0.011989 Jy/beam ! Clean residual mean=-0.000010 rms=0.001984 Jy/beam ! Combined flux in latest and established models = 4.10545 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 43 components and 4.10545 Jy ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 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 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=2.28 mas, bmaj=2.556 mas, bpa=-13.25 degrees ! Estimated noise=3.34041 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0158697 Jy ! Component: 100 - total flux cleaned = 0.019851 Jy ! Component: 150 - total flux cleaned = 0.0231516 Jy ! Component: 200 - total flux cleaned = 0.0254934 Jy ! Total flux subtracted in 200 components = 0.0254934 Jy ! Clean residual min=-0.009266 max=0.009364 Jy/beam ! Clean residual mean=-0.000014 rms=0.002373 Jy/beam ! Combined flux in latest and established models = 4.13094 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 = 0.00187396 Jy ! Component: 100 - total flux cleaned = 0.00323717 Jy ! Component: 150 - total flux cleaned = 0.00436598 Jy ! Component: 200 - total flux cleaned = 0.00520233 Jy ! Total flux subtracted in 200 components = 0.00520233 Jy ! Clean residual min=-0.008930 max=0.009388 Jy/beam ! Clean residual mean=-0.000012 rms=0.002311 Jy/beam ! Combined flux in latest and established models = 4.13614 Jy ! Adding 47 model components to the UV plane model. ! The established model now contains 82 components and 4.13615 Jy ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.7549 mas, bmaj=1.03 mas, bpa=-4.115 degrees ! Estimated noise=2.36443 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00142297 Jy ! Component: 100 - total flux cleaned = -0.00105976 Jy ! Component: 150 - total flux cleaned = -0.00136471 Jy ! Component: 200 - total flux cleaned = -0.00136073 Jy ! Total flux subtracted in 200 components = -0.00136073 Jy ! Clean residual min=-0.010292 max=0.010329 Jy/beam ! Clean residual mean=-0.000004 rms=0.001759 Jy/beam ! Combined flux in latest and established models = 4.13478 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 92 components and 4.13478 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.137793Jy sigma=0.761171 ! Fit after self-cal, rms=0.134428Jy sigma=0.727819 wmodel J0854+2006_X_map.mod ! Writing 92 model components to file: J0854+2006_X_map.mod wobs J0854+2006_X_uvs.fits ! Writing UV FITS file: J0854+2006_X_uvs.fits wwins J0854+2006_X_map.win ! wwins: Wrote 6 windows to J0854+2006_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 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000752572 Jy ! Component: 100 - total flux cleaned = -0.0011966 Jy ! Component: 150 - total flux cleaned = -0.00120041 Jy ! Component: 200 - total flux cleaned = -0.00106665 Jy ! Component: 250 - total flux cleaned = -0.000409881 Jy ! Component: 300 - total flux cleaned = -0.000153807 Jy ! Component: 350 - total flux cleaned = -2.83115e-05 Jy ! Component: 400 - total flux cleaned = -0.00027517 Jy ! Component: 450 - total flux cleaned = -0.000395126 Jy ! Component: 500 - total flux cleaned = -0.000395739 Jy ! Component: 550 - total flux cleaned = -0.000629933 Jy ! Component: 600 - total flux cleaned = -0.000745018 Jy ! Component: 650 - total flux cleaned = -0.000629486 Jy ! Component: 700 - total flux cleaned = -0.000967183 Jy ! Component: 750 - total flux cleaned = -0.0010792 Jy ! Component: 800 - total flux cleaned = -0.000971765 Jy ! Component: 850 - total flux cleaned = -0.000865923 Jy ! Component: 900 - total flux cleaned = -0.00107993 Jy ! Component: 950 - total flux cleaned = -0.000761481 Jy ! Component: 1000 - total flux cleaned = -0.000657892 Jy ! Component: 1050 - total flux cleaned = -0.000760449 Jy ! Component: 1100 - total flux cleaned = -0.000656424 Jy ! Component: 1150 - total flux cleaned = -0.000859595 Jy ! Component: 1200 - total flux cleaned = -0.000657342 Jy ! Component: 1250 - total flux cleaned = -0.00105948 Jy ! Component: 1300 - total flux cleaned = -0.00155538 Jy ! Component: 1350 - total flux cleaned = -0.00125862 Jy ! Component: 1400 - total flux cleaned = -0.00135536 Jy ! Component: 1450 - total flux cleaned = -0.00106371 Jy ! Component: 1500 - total flux cleaned = -0.00115977 Jy ! Component: 1550 - total flux cleaned = -0.000874264 Jy ! Component: 1600 - total flux cleaned = -0.000873468 Jy ! Component: 1650 - total flux cleaned = -0.00106123 Jy ! Component: 1700 - total flux cleaned = -0.00124954 Jy ! Component: 1750 - total flux cleaned = -0.000971404 Jy ! Component: 1800 - total flux cleaned = -0.000878991 Jy ! Component: 1850 - total flux cleaned = -0.000971324 Jy ! Component: 1900 - total flux cleaned = -0.00106242 Jy ! Component: 1950 - total flux cleaned = -0.000792179 Jy ! Component: 2000 - total flux cleaned = -0.00088232 Jy ! Component: 2050 - total flux cleaned = -0.000613928 Jy ! Component: 2100 - total flux cleaned = -0.000703026 Jy ! Component: 2150 - total flux cleaned = -0.000879786 Jy ! Component: 2200 - total flux cleaned = -0.000528786 Jy ! Component: 2250 - total flux cleaned = -0.000354043 Jy ! Component: 2300 - total flux cleaned = -9.50855e-05 Jy ! Component: 2350 - total flux cleaned = -8.62262e-06 Jy ! Component: 2400 - total flux cleaned = 0.000162743 Jy ! Component: 2450 - total flux cleaned = 0.000331687 Jy ! Component: 2500 - total flux cleaned = 0.000753622 Jy ! Component: 2550 - total flux cleaned = 0.00100605 Jy ! Component: 2600 - total flux cleaned = 0.00108912 Jy ! Component: 2650 - total flux cleaned = 0.00150375 Jy ! Component: 2700 - total flux cleaned = 0.00166864 Jy ! Component: 2750 - total flux cleaned = 0.00174989 Jy ! Component: 2800 - total flux cleaned = 0.00215688 Jy ! Component: 2850 - total flux cleaned = 0.00207515 Jy ! Component: 2900 - total flux cleaned = 0.00215585 Jy ! Component: 2950 - total flux cleaned = 0.00231635 Jy ! Component: 3000 - total flux cleaned = 0.00271548 Jy ! Component: 3050 - total flux cleaned = 0.00303335 Jy ! Component: 3100 - total flux cleaned = 0.0030328 Jy ! Component: 3150 - total flux cleaned = 0.00326837 Jy ! Component: 3200 - total flux cleaned = 0.00373714 Jy ! Component: 3250 - total flux cleaned = 0.00373697 Jy ! Component: 3300 - total flux cleaned = 0.00396881 Jy ! Component: 3350 - total flux cleaned = 0.00443007 Jy ! Component: 3400 - total flux cleaned = 0.00458385 Jy ! Component: 3450 - total flux cleaned = 0.00519347 Jy ! Component: 3500 - total flux cleaned = 0.00504158 Jy ! Component: 3550 - total flux cleaned = 0.00473901 Jy ! Component: 3600 - total flux cleaned = 0.00534043 Jy ! Component: 3650 - total flux cleaned = 0.00548904 Jy ! Component: 3700 - total flux cleaned = 0.00578667 Jy ! Component: 3750 - total flux cleaned = 0.00615768 Jy ! Component: 3800 - total flux cleaned = 0.00623132 Jy ! Component: 3850 - total flux cleaned = 0.0065991 Jy ! Component: 3900 - total flux cleaned = 0.00689128 Jy ! Component: 3950 - total flux cleaned = 0.00681864 Jy ! Component: 4000 - total flux cleaned = 0.00710879 Jy ! Component: 4050 - total flux cleaned = 0.00768574 Jy ! Total flux subtracted in 4096 components = 0.00775726 Jy ! Clean residual min=-0.003891 max=0.003935 Jy/beam ! Clean residual mean=-0.000003 rms=0.001154 Jy/beam ! Combined flux in latest and established models = 4.14254 Jy keep ! Adding 320 model components to the UV plane model. ! The established model now contains 409 components and 4.14254 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv118_uvs/J0854+2006_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7549 x 1.03 at -4.115 degrees (North through East) ! Clean map min=-0.014814 max=3.3992 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv118_uvs/J0854+2006_X_map.fits wmodel /scr/pima/rv118_uvs/J0854+2006_X_map.mod ! Writing 409 model components to file: /scr/pima/rv118_uvs/J0854+2006_X_map.mod wobs /scr/pima/rv118_uvs/J0854+2006_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv118_uvs/J0854+2006_X_uvs.fits wwins /scr/pima/rv118_uvs/J0854+2006_X_map.win ! wwins: Wrote 7 windows to /scr/pima/rv118_uvs/J0854+2006_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 3.39923 invert ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00115361 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.101812 0.101812 0.203624 0.407248 0.814495 1.62899 3.25798 6.51596 13.0319 26.0638 52.1277 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0034 print "peak= ", int(1000*peak_flux)/1000 ! peak= 3.399 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 2946.61 quit ! Quitting program ! Log file /scr/pima/rv118_uvs/J0854+2006_X_dfm.log closed on Sun Dec 10 00:08:45 2017