! Started logfile: /scr/pima/rv102_uvs/J0224+0659_X_dfm.log on Sat Nov 9 10:15:56 2019 float field_size field_size = 1024 float field_cell field_cell = 0.2000 float taper_size taper_size = 70.0 float freq freq = 8.40599 obs /scr/pima/rv102_uvs/J0224+0659_X_uva.fits ! Reading UV FITS file: /scr/pima/rv102_uvs/J0224+0659_X_uva.fits ! AN table 1: 19 integrations on 3 of 3 possible baselines. ! AN table 2: 238 integrations on 10 of 10 possible baselines. ! AN table 3: 119 integrations on 55 of 55 possible baselines. ! AN table 4: 13 integrations on 1 of 1 possible baselines. ! AN table 5: 19 integrations on 1 of 1 possible baselines. ! AN table 6: 25 integrations on 36 of 36 possible baselines. ! Apparent sampling: 0.600565 visibilities/baseline/integration-bin. ! Found source: J0224+0659 ! ! 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 8.40599e+09 8e+06 1 8e+06 ! 02 2 8.47599e+09 8e+06 1 8e+06 ! 03 3 8.79099e+09 8e+06 1 8e+06 ! 04 4 8.89599e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 79 lines of history. ! ! Reading 23816 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 J0224+0659_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 12 telescope corrections were flagged in sub-array 1. ! A total of 127 telescope corrections were flagged in sub-array 2. ! A total of 484 telescope corrections were flagged in sub-array 3. ! A total of 26 telescope corrections were flagged in sub-array 4. ! A total of 38 telescope corrections were flagged in sub-array 5. ! A total of 95 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 12 telescope corrections were flagged in sub-array 1. ! A total of 127 telescope corrections were flagged in sub-array 2. ! A total of 484 telescope corrections were flagged in sub-array 3. ! A total of 26 telescope corrections were flagged in sub-array 4. ! A total of 38 telescope corrections were flagged in sub-array 5. ! A total of 95 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 12 telescope corrections were flagged in sub-array 1. ! A total of 362 telescope corrections were flagged in sub-array 2. ! A total of 615 telescope corrections were flagged in sub-array 3. ! A total of 26 telescope corrections were flagged in sub-array 4. ! A total of 38 telescope corrections were flagged in sub-array 5. ! A total of 95 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 12 telescope corrections were flagged in sub-array 1. ! A total of 362 telescope corrections were flagged in sub-array 2. ! A total of 615 telescope corrections were flagged in sub-array 3. ! A total of 26 telescope corrections were flagged in sub-array 4. ! A total of 38 telescope corrections were flagged in sub-array 5. ! A total of 95 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.202659Jy sigma=14.044713 ! Fit after self-cal, rms=0.452724Jy sigma=5.169953 ! 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 1.52% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.4938 mas, bmaj=1.885 mas, bpa=-10.63 degrees ! Estimated noise=0.741974 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 = 0.455016 Jy ! Component: 100 - total flux cleaned = 0.566483 Jy ! Total flux subtracted in 100 components = 0.566483 Jy ! Clean residual min=-0.016121 max=0.047806 Jy/beam ! Clean residual mean=0.000489 rms=0.004750 Jy/beam ! Combined flux in latest and established models = 0.566483 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.566483 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.235272Jy sigma=2.354250 ! Fit after self-cal, rms=0.235302Jy sigma=2.353367 ! Inverting map ! Your choice of large map pixels excluded 1.52% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0535884 Jy ! Component: 100 - total flux cleaned = 0.0823028 Jy ! Total flux subtracted in 100 components = 0.0823028 Jy ! Clean residual min=-0.013733 max=0.033493 Jy/beam ! Clean residual mean=0.000365 rms=0.003281 Jy/beam ! Combined flux in latest and established models = 0.648786 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 13 components and 0.648786 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.220920Jy sigma=2.137964 ! Fit after self-cal, rms=0.221017Jy sigma=2.136810 ! Inverting map ! Your choice of large map pixels excluded 1.52% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Added new window around map position (-1.4, 0.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0302924 Jy ! Component: 100 - total flux cleaned = 0.048537 Jy ! Total flux subtracted in 100 components = 0.048537 Jy ! Clean residual min=-0.011960 max=0.019262 Jy/beam ! Clean residual mean=0.000293 rms=0.002641 Jy/beam ! Combined flux in latest and established models = 0.697323 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 18 components and 0.697323 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.215628Jy sigma=2.058808 ! Fit after self-cal, rms=0.214955Jy sigma=2.053165 ! Inverting map ! Your choice of large map pixels excluded 1.52% of the data. ! The x-axis pixel size should ideally be below 0.1918 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 1.52% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.5727 mas, bmaj=1.951 mas, bpa=-9.466 degrees ! Estimated noise=0.46826 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 = 0.0220523 Jy ! Component: 100 - total flux cleaned = 0.0338784 Jy ! Component: 150 - total flux cleaned = 0.0374963 Jy ! Component: 200 - total flux cleaned = 0.0391545 Jy ! Total flux subtracted in 200 components = 0.0391545 Jy ! Clean residual min=-0.008346 max=0.013729 Jy/beam ! Clean residual mean=0.001353 rms=0.002012 Jy/beam ! Combined flux in latest and established models = 0.736477 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 31 components and 0.736477 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.211979Jy sigma=2.021782 ! Fit after self-cal, rms=0.211640Jy sigma=2.018823 ! Inverting map ! Your choice of large map pixels excluded 1.52% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Added new window around map position (0.8, -5.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.011596 Jy ! Component: 100 - total flux cleaned = 0.0170743 Jy ! Component: 150 - total flux cleaned = 0.0197444 Jy ! Component: 200 - total flux cleaned = 0.0218474 Jy ! Total flux subtracted in 200 components = 0.0218474 Jy ! Clean residual min=-0.006808 max=0.009524 Jy/beam ! Clean residual mean=0.001180 rms=0.001749 Jy/beam ! Combined flux in latest and established models = 0.758325 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 42 components and 0.758325 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.210532Jy sigma=2.009253 ! Fit after self-cal, rms=0.210359Jy sigma=2.008335 ! Inverting map ! Your choice of large map pixels excluded 1.52% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5727 x 1.951 at -9.466 degrees (North through East) ! Clean map min=-0.0064306 max=0.60397 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 45 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HN 0.00* SC 0.00* WF 0.00* ! ! A total of 45 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! MA 0.99 NY 1.01 ON 1.02 WF 0.97 ! WZ 0.96 ! ! A total of 18 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! FD 1.01 HN 1.00 KP 1.00 LA 1.02 ! MA 1.01 NY 1.04 ON 1.01 PT 1.03 ! SC 1.00 WF 0.95 WZ 1.00 ! ! Telescope amplitude corrections in sub-array 4: ! HN 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! MK 0.00* WF 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! FD 0.98 HN 0.99 KP 1.02 LA 0.99 ! MK 1.08 NL 1.01 PT 1.00 SC 1.05 ! WF 0.92 ! ! ! Correcting IF 2. ! A total of 45 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HN 0.00* SC 0.00* WF 0.00* ! ! A total of 45 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! MA 0.97 NY 1.03 ON 1.02 WF 0.97 ! WZ 1.00 ! ! A total of 18 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! FD 0.99 HN 1.01 KP 1.00 LA 1.02 ! MA 0.97 NY 1.03 ON 1.02 PT 1.04 ! SC 0.99 WF 0.93 WZ 1.05 ! ! Telescope amplitude corrections in sub-array 4: ! HN 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! MK 0.00* WF 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! FD 0.99 HN 1.00 KP 1.01 LA 0.99 ! MK 1.05 NL 1.03 PT 1.02 SC 1.02 ! WF 0.91 ! ! ! Correcting IF 3. ! A total of 45 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HN 0.00* SC 0.00* WF 0.00* ! ! A total of 228 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! MA 0.98 NY 1.00* ON 0.99 WF 0.95 ! WZ 1.00 ! ! A total of 102 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! FD 0.97 HN 1.00 KP 0.99 LA 1.00 ! MA 1.04 NY 1.00* ON 1.02 PT 1.00 ! SC 0.97 WF 0.92 WZ 1.04 ! ! Telescope amplitude corrections in sub-array 4: ! HN 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! MK 0.00* WF 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! FD 0.97 HN 0.93 KP 1.00 LA 0.99 ! MK 1.04 NL 1.00 PT 1.03 SC 1.03 ! WF 0.87 ! ! ! Correcting IF 4. ! A total of 45 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HN 0.00* SC 0.00* WF 0.00* ! ! A total of 228 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! MA 1.03 NY 1.00* ON 1.02 WF 0.93 ! WZ 0.99 ! ! A total of 102 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! FD 1.26 HN 0.99 KP 0.98 LA 1.00 ! MA 1.10 NY 1.00* ON 1.01 PT 1.00 ! SC 0.96 WF 0.93 WZ 1.02 ! ! Telescope amplitude corrections in sub-array 4: ! HN 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! MK 0.00* WF 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! FD 1.01 HN 0.96 KP 0.99 LA 0.97 ! MK 1.03 NL 1.03 PT 1.01 SC 1.03 ! WF 0.87 ! ! ! Fit before self-cal, rms=0.210359Jy sigma=2.008335 ! Fit after self-cal, rms=0.202191Jy sigma=1.972225 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.5735 mas, bmaj=1.957 mas, bpa=-9.523 degrees ! Estimated noise=0.475081 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, 0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00801937 Jy ! Component: 100 - total flux cleaned = 0.0109279 Jy ! Component: 150 - total flux cleaned = 0.0126279 Jy ! Component: 200 - total flux cleaned = 0.0139272 Jy ! Total flux subtracted in 200 components = 0.0139272 Jy ! Clean residual min=-0.003835 max=0.005409 Jy/beam ! Clean residual mean=0.000505 rms=0.001077 Jy/beam ! Combined flux in latest and established models = 0.772252 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 62 components and 0.772252 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.201796Jy sigma=1.967732 ! Fit after self-cal, rms=0.201732Jy sigma=1.967345 ! Inverting map ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 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=0.201732Jy sigma=1.967345 ! Fit after self-cal, rms=0.200995Jy sigma=1.966204 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.5731 mas, bmaj=1.956 mas, bpa=-9.517 degrees ! Estimated noise=0.475198 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00441743 Jy ! Component: 100 - total flux cleaned = 0.00666123 Jy ! Component: 150 - total flux cleaned = 0.00723554 Jy ! Component: 200 - total flux cleaned = 0.0075719 Jy ! Total flux subtracted in 200 components = 0.0075719 Jy ! Clean residual min=-0.003666 max=0.004769 Jy/beam ! Clean residual mean=0.000351 rms=0.000967 Jy/beam ! Combined flux in latest and established models = 0.779824 Jy selfcal ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 76 components and 0.779824 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.200859Jy sigma=1.964559 ! Fit after self-cal, rms=0.200849Jy sigma=1.964496 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 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 (-18.6, -18.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0042071 Jy ! Component: 100 - total flux cleaned = 0.00663307 Jy ! Component: 150 - total flux cleaned = 0.00774314 Jy ! Component: 200 - total flux cleaned = 0.00837949 Jy ! Total flux subtracted in 200 components = 0.00837949 Jy ! Clean residual min=-0.003683 max=0.004125 Jy/beam ! Clean residual mean=0.000290 rms=0.000893 Jy/beam ! Combined flux in latest and established models = 0.788203 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 89 components and 0.788203 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.200732Jy sigma=1.963161 ! Fit after self-cal, rms=0.200722Jy sigma=1.963048 ! Inverting map ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Added new window around map position (-43, 21). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00364192 Jy ! Component: 100 - total flux cleaned = 0.00523812 Jy ! Component: 150 - total flux cleaned = 0.00615487 Jy ! Component: 200 - total flux cleaned = 0.00699374 Jy ! Total flux subtracted in 200 components = 0.00699374 Jy ! Clean residual min=-0.003740 max=0.003657 Jy/beam ! Clean residual mean=0.000265 rms=0.000830 Jy/beam ! Combined flux in latest and established models = 0.795197 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 105 components and 0.795197 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.200637Jy sigma=1.962020 ! Fit after self-cal, rms=0.200632Jy sigma=1.961957 ! Inverting map ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 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=0.200632Jy sigma=1.961957 ! Fit after self-cal, rms=0.200368Jy sigma=1.961103 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.5731 mas, bmaj=1.957 mas, bpa=-9.509 degrees ! Estimated noise=0.475737 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00203614 Jy ! Component: 100 - total flux cleaned = 0.00261065 Jy ! Component: 150 - total flux cleaned = 0.00336863 Jy ! Component: 200 - total flux cleaned = 0.00383087 Jy ! Total flux subtracted in 200 components = 0.00383087 Jy ! Clean residual min=-0.003301 max=0.003711 Jy/beam ! Clean residual mean=0.000192 rms=0.000775 Jy/beam ! Combined flux in latest and established models = 0.799028 Jy selfcal ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 116 components and 0.799028 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.200321Jy sigma=1.960515 ! Fit after self-cal, rms=0.200314Jy sigma=1.960493 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 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 (-10.8, 43.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00245319 Jy ! Component: 100 - total flux cleaned = 0.00315763 Jy ! Component: 150 - total flux cleaned = 0.00338182 Jy ! Component: 200 - total flux cleaned = 0.00369852 Jy ! Total flux subtracted in 200 components = 0.00369852 Jy ! Clean residual min=-0.003407 max=0.002887 Jy/beam ! Clean residual mean=0.000186 rms=0.000735 Jy/beam ! Combined flux in latest and established models = 0.802727 Jy ! Performing phase self-cal ! Adding 35 model components to the UV plane model. ! The established model now contains 131 components and 0.802727 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.200240Jy sigma=1.959879 ! Fit after self-cal, rms=0.200236Jy sigma=1.959836 ! Inverting map ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 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=0.200236Jy sigma=1.959836 ! Fit after self-cal, rms=0.200178Jy sigma=1.959703 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=2.157 mas, bmaj=3.101 mas, bpa=33.21 degrees ! Estimated noise=0.672036 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0025899 Jy ! Component: 100 - total flux cleaned = 0.00415391 Jy ! Component: 150 - total flux cleaned = 0.00505165 Jy ! Component: 200 - total flux cleaned = 0.00559519 Jy ! Total flux subtracted in 200 components = 0.00559519 Jy ! Clean residual min=-0.003715 max=0.003902 Jy/beam ! Clean residual mean=0.000396 rms=0.000962 Jy/beam ! Combined flux in latest and established models = 0.808322 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 150 components and 0.808322 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.200158Jy sigma=1.959529 ! Fit after self-cal, rms=0.200155Jy sigma=1.959464 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 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 = 0.00119469 Jy ! Component: 100 - total flux cleaned = 0.00148689 Jy ! Component: 150 - total flux cleaned = 0.00175107 Jy ! Component: 200 - total flux cleaned = 0.00203464 Jy ! Total flux subtracted in 200 components = 0.00203464 Jy ! Clean residual min=-0.003827 max=0.003935 Jy/beam ! Clean residual mean=0.000366 rms=0.000967 Jy/beam ! Combined flux in latest and established models = 0.810357 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 161 components and 0.810357 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.200154Jy sigma=1.959401 ! Fit after self-cal, rms=0.200155Jy sigma=1.959388 ! Inverting map ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 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 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.5729 mas, bmaj=1.957 mas, bpa=-9.506 degrees ! Estimated noise=0.475999 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5729 x 1.957 at -9.506 degrees (North through East) ! Clean map min=-0.0026666 max=0.60247 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=0.200155Jy sigma=1.959388 ! Fit after self-cal, rms=0.194990Jy sigma=1.696703 ! Inverting map and beam ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.5733 mas, bmaj=1.958 mas, bpa=-9.521 degrees ! Estimated noise=0.477062 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000370084 Jy ! Component: 100 - total flux cleaned = 0.000258063 Jy ! Component: 150 - total flux cleaned = 0.000454983 Jy ! Component: 200 - total flux cleaned = 0.00058762 Jy ! Total flux subtracted in 200 components = 0.00058762 Jy ! Clean residual min=-0.002804 max=0.002807 Jy/beam ! Clean residual mean=0.000102 rms=0.000670 Jy/beam ! Combined flux in latest and established models = 0.810944 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 176 components and 0.810944 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194954Jy sigma=1.696354 ! Fit after self-cal, rms=0.194950Jy sigma=1.696340 ! Inverting map ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -5.41067e-06 Jy ! Component: 100 - total flux cleaned = 0.000115266 Jy ! Component: 150 - total flux cleaned = 0.000306026 Jy ! Component: 200 - total flux cleaned = 0.000415073 Jy ! Total flux subtracted in 200 components = 0.000415073 Jy ! Clean residual min=-0.002787 max=0.002765 Jy/beam ! Clean residual mean=0.000100 rms=0.000664 Jy/beam ! Combined flux in latest and established models = 0.811359 Jy ! Performing phase self-cal ! Adding 36 model components to the UV plane model. ! The established model now contains 184 components and 0.811359 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194933Jy sigma=1.696164 ! Fit after self-cal, rms=0.194932Jy sigma=1.696164 ! Inverting map ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194932Jy sigma=1.696164 ! Fit after self-cal, rms=0.195133Jy sigma=1.696105 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 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.4956 mas, bmaj=1.897 mas, bpa=-10.62 degrees ! Estimated noise=0.768179 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.460939 Jy ! Component: 100 - total flux cleaned = 0.571789 Jy ! Component: 150 - total flux cleaned = 0.627309 Jy ! Component: 200 - total flux cleaned = 0.662718 Jy ! Total flux subtracted in 200 components = 0.662718 Jy ! Clean residual min=-0.009878 max=0.019776 Jy/beam ! Clean residual mean=0.000237 rms=0.002651 Jy/beam ! Combined flux in latest and established models = 0.662718 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 0.662718 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.5732 mas, bmaj=1.959 mas, bpa=-9.52 degrees ! Estimated noise=0.477245 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 = 0.0355227 Jy ! Component: 100 - total flux cleaned = 0.058101 Jy ! Component: 150 - total flux cleaned = 0.0729378 Jy ! Component: 200 - total flux cleaned = 0.0835205 Jy ! Total flux subtracted in 200 components = 0.0835205 Jy ! Clean residual min=-0.004266 max=0.006896 Jy/beam ! Clean residual mean=0.000523 rms=0.001304 Jy/beam ! Combined flux in latest and established models = 0.746238 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 32 components and 0.746239 Jy ! Inverting map ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Added new window around map position (-0.8, 2.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00830315 Jy ! Component: 100 - total flux cleaned = 0.0147735 Jy ! Component: 150 - total flux cleaned = 0.0202174 Jy ! Component: 200 - total flux cleaned = 0.0250068 Jy ! Total flux subtracted in 200 components = 0.0250068 Jy ! Clean residual min=-0.003511 max=0.004764 Jy/beam ! Clean residual mean=0.000343 rms=0.000970 Jy/beam ! Combined flux in latest and established models = 0.771245 Jy ! Adding 35 model components to the UV plane model. ! The established model now contains 58 components and 0.771245 Jy ! Inverting map ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Added new window around map position (-23, 22.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00476237 Jy ! Component: 100 - total flux cleaned = 0.00844415 Jy ! Component: 150 - total flux cleaned = 0.0114661 Jy ! Component: 200 - total flux cleaned = 0.014204 Jy ! Total flux subtracted in 200 components = 0.014204 Jy ! Clean residual min=-0.003174 max=0.004036 Jy/beam ! Clean residual mean=0.000253 rms=0.000833 Jy/beam ! Combined flux in latest and established models = 0.785449 Jy ! Adding 36 model components to the UV plane model. ! The established model now contains 72 components and 0.785449 Jy ! Inverting map ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Added new window around map position (16.6, -18.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00325926 Jy ! Component: 100 - total flux cleaned = 0.0053801 Jy ! Component: 150 - total flux cleaned = 0.00703587 Jy ! Component: 200 - total flux cleaned = 0.00839539 Jy ! Total flux subtracted in 200 components = 0.00839539 Jy ! Clean residual min=-0.002927 max=0.003216 Jy/beam ! Clean residual mean=0.000202 rms=0.000764 Jy/beam ! Combined flux in latest and established models = 0.793845 Jy ! Adding 49 model components to the UV plane model. ! The established model now contains 98 components and 0.793845 Jy ! Inverting map ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 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 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=2.158 mas, bmaj=3.099 mas, bpa=33.14 degrees ! Estimated noise=0.673036 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0040562 Jy ! Component: 100 - total flux cleaned = 0.0072578 Jy ! Component: 150 - total flux cleaned = 0.00992382 Jy ! Component: 200 - total flux cleaned = 0.0121815 Jy ! Total flux subtracted in 200 components = 0.0121815 Jy ! Clean residual min=-0.003452 max=0.003723 Jy/beam ! Clean residual mean=0.000395 rms=0.000967 Jy/beam ! Combined flux in latest and established models = 0.806026 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 = 0.00126174 Jy ! Component: 100 - total flux cleaned = 0.00183218 Jy ! Component: 150 - total flux cleaned = 0.0021612 Jy ! Component: 200 - total flux cleaned = 0.00246808 Jy ! Total flux subtracted in 200 components = 0.00246808 Jy ! Clean residual min=-0.003224 max=0.003562 Jy/beam ! Clean residual mean=0.000341 rms=0.000908 Jy/beam ! Combined flux in latest and established models = 0.808494 Jy ! Adding 63 model components to the UV plane model. ! The established model now contains 153 components and 0.808494 Jy ! Inverting map ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.5732 mas, bmaj=1.959 mas, bpa=-9.52 degrees ! Estimated noise=0.477245 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000334346 Jy ! Component: 100 - total flux cleaned = -0.000266941 Jy ! Component: 150 - total flux cleaned = -0.000201729 Jy ! Component: 200 - total flux cleaned = -0.000143533 Jy ! Total flux subtracted in 200 components = -0.000143533 Jy ! Clean residual min=-0.002900 max=0.002703 Jy/beam ! Clean residual mean=0.000113 rms=0.000682 Jy/beam ! Combined flux in latest and established models = 0.808351 Jy selfcal ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 175 components and 0.808351 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.195136Jy sigma=1.696677 ! Fit after self-cal, rms=0.195106Jy sigma=1.696424 wmodel J0224+0659_X_map.mod ! Writing 175 model components to file: J0224+0659_X_map.mod wobs J0224+0659_X_uvs.fits ! Writing UV FITS file: J0224+0659_X_uvs.fits wwins J0224+0659_X_map.win ! wwins: Wrote 10 windows to J0224+0659_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 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000311068 Jy ! Component: 100 - total flux cleaned = -2.69926e-05 Jy ! Component: 150 - total flux cleaned = 0.000338178 Jy ! Component: 200 - total flux cleaned = 0.000737448 Jy ! Component: 250 - total flux cleaned = 0.00116903 Jy ! Component: 300 - total flux cleaned = 0.00154928 Jy ! Component: 350 - total flux cleaned = 0.00192237 Jy ! Component: 400 - total flux cleaned = 0.00236987 Jy ! Component: 450 - total flux cleaned = 0.00281025 Jy ! Component: 500 - total flux cleaned = 0.00324372 Jy ! Component: 550 - total flux cleaned = 0.00363156 Jy ! Component: 600 - total flux cleaned = 0.00401352 Jy ! Component: 650 - total flux cleaned = 0.00439047 Jy ! Component: 700 - total flux cleaned = 0.00476283 Jy ! Component: 750 - total flux cleaned = 0.00516724 Jy ! Component: 800 - total flux cleaned = 0.00560293 Jy ! Component: 850 - total flux cleaned = 0.00596159 Jy ! Component: 900 - total flux cleaned = 0.00628142 Jy ! Component: 950 - total flux cleaned = 0.00673789 Jy ! Component: 1000 - total flux cleaned = 0.00705055 Jy ! Component: 1050 - total flux cleaned = 0.00732583 Jy ! Component: 1100 - total flux cleaned = 0.00759876 Jy ! Component: 1150 - total flux cleaned = 0.00800408 Jy ! Component: 1200 - total flux cleaned = 0.00840468 Jy ! Component: 1250 - total flux cleaned = 0.00866923 Jy ! Component: 1300 - total flux cleaned = 0.00896454 Jy ! Component: 1350 - total flux cleaned = 0.00932225 Jy ! Component: 1400 - total flux cleaned = 0.00957966 Jy ! Component: 1450 - total flux cleaned = 0.00993091 Jy ! Component: 1500 - total flux cleaned = 0.0102788 Jy ! Component: 1550 - total flux cleaned = 0.0104354 Jy ! Component: 1600 - total flux cleaned = 0.0106845 Jy ! Component: 1650 - total flux cleaned = 0.0109621 Jy ! Component: 1700 - total flux cleaned = 0.0111454 Jy ! Component: 1750 - total flux cleaned = 0.0113579 Jy ! Component: 1800 - total flux cleaned = 0.0115685 Jy ! Component: 1850 - total flux cleaned = 0.0117178 Jy ! Component: 1900 - total flux cleaned = 0.0118069 Jy ! Component: 1950 - total flux cleaned = 0.0120132 Jy ! Component: 2000 - total flux cleaned = 0.0121591 Jy ! Component: 2050 - total flux cleaned = 0.0122461 Jy ! Component: 2100 - total flux cleaned = 0.0124478 Jy ! Component: 2150 - total flux cleaned = 0.012505 Jy ! Component: 2200 - total flux cleaned = 0.0126749 Jy ! Component: 2250 - total flux cleaned = 0.0127311 Jy ! Component: 2300 - total flux cleaned = 0.0128708 Jy ! Component: 2350 - total flux cleaned = 0.0128434 Jy ! Component: 2400 - total flux cleaned = 0.0129814 Jy ! Component: 2450 - total flux cleaned = 0.0129541 Jy ! Component: 2500 - total flux cleaned = 0.0131445 Jy ! Component: 2550 - total flux cleaned = 0.0132255 Jy ! Component: 2600 - total flux cleaned = 0.0133867 Jy ! Component: 2650 - total flux cleaned = 0.0134135 Jy ! Component: 2700 - total flux cleaned = 0.0135458 Jy ! Component: 2750 - total flux cleaned = 0.0135986 Jy ! Component: 2800 - total flux cleaned = 0.0136509 Jy ! Component: 2850 - total flux cleaned = 0.0137029 Jy ! Component: 2900 - total flux cleaned = 0.0138323 Jy ! Component: 2950 - total flux cleaned = 0.0139092 Jy ! Component: 3000 - total flux cleaned = 0.0141131 Jy ! Component: 3050 - total flux cleaned = 0.0141384 Jy ! Component: 3100 - total flux cleaned = 0.014264 Jy ! Component: 3150 - total flux cleaned = 0.014364 Jy ! Component: 3200 - total flux cleaned = 0.0144634 Jy ! Component: 3250 - total flux cleaned = 0.0145125 Jy ! Component: 3300 - total flux cleaned = 0.0147582 Jy ! Component: 3350 - total flux cleaned = 0.0146359 Jy ! Component: 3400 - total flux cleaned = 0.0148546 Jy ! Component: 3450 - total flux cleaned = 0.0148786 Jy ! Component: 3500 - total flux cleaned = 0.0149026 Jy ! Component: 3550 - total flux cleaned = 0.0149744 Jy ! Component: 3600 - total flux cleaned = 0.0150932 Jy ! Component: 3650 - total flux cleaned = 0.0151876 Jy ! Component: 3700 - total flux cleaned = 0.0152815 Jy ! Component: 3750 - total flux cleaned = 0.015375 Jy ! Component: 3800 - total flux cleaned = 0.0155144 Jy ! Component: 3850 - total flux cleaned = 0.0155143 Jy ! Component: 3900 - total flux cleaned = 0.0155832 Jy ! Component: 3950 - total flux cleaned = 0.0156289 Jy ! Component: 4000 - total flux cleaned = 0.0156974 Jy ! Component: 4050 - total flux cleaned = 0.0157427 Jy ! Total flux subtracted in 4096 components = 0.0158101 Jy ! Clean residual min=-0.001444 max=0.001520 Jy/beam ! Clean residual mean=0.000056 rms=0.000381 Jy/beam ! Combined flux in latest and established models = 0.824161 Jy keep ! Adding 328 model components to the UV plane model. ! The established model now contains 503 components and 0.824161 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv102_uvs/J0224+0659_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5732 x 1.959 at -9.52 degrees (North through East) ! Clean map min=-0.0017278 max=0.60319 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv102_uvs/J0224+0659_X_map.fits wmodel /scr/pima/rv102_uvs/J0224+0659_X_map.mod ! Writing 503 model components to file: /scr/pima/rv102_uvs/J0224+0659_X_map.mod wobs /scr/pima/rv102_uvs/J0224+0659_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv102_uvs/J0224+0659_X_uvs.fits wwins /scr/pima/rv102_uvs/J0224+0659_X_map.win ! wwins: Wrote 11 windows to /scr/pima/rv102_uvs/J0224+0659_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.603194 invert ! Inverting map ! Your choice of large map pixels excluded 1.6% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000381636 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.189808 0.189808 0.379616 0.759231 1.51846 3.03692 6.07385 12.1477 24.2954 48.5908 97.1816 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0011 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.603 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1580.55 quit ! Quitting program ! Log file /scr/pima/rv102_uvs/J0224+0659_X_dfm.log closed on Sat Nov 9 10:16:02 2019