! Started logfile: /scr/pima/rv125_uvs/J2236+2828_X_dfm.log on Sun Dec 23 02:54:05 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/J2236+2828_X_uva.fits ! Reading UV FITS file: /scr/pima/rv125_uvs/J2236+2828_X_uva.fits ! AN table 1: 58 integrations on 6 of 6 possible baselines. ! AN table 2: 6 integrations on 6 of 6 possible baselines. ! AN table 3: 2 integrations on 6 of 6 possible baselines. ! AN table 4: 32 integrations on 36 of 36 possible baselines. ! AN table 5: 14 integrations on 36 of 36 possible baselines. ! Apparent sampling: 0.362573 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J2236+2828 ! ! 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 2976 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 J2236+2828_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 190 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 168 telescope corrections were flagged in sub-array 4. ! A total of 64 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 190 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 168 telescope corrections were flagged in sub-array 4. ! A total of 64 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 214 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 2 telescope corrections were flagged in sub-array 3. ! A total of 168 telescope corrections were flagged in sub-array 4. ! A total of 78 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 214 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 2 telescope corrections were flagged in sub-array 3. ! A total of 168 telescope corrections were flagged in sub-array 4. ! A total of 78 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=1.674193Jy sigma=19.966149 ! Fit after self-cal, rms=0.411916Jy sigma=5.097025 ! 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 2.26% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Estimated beam: bmin=0.922 mas, bmaj=1.054 mas, bpa=-19.02 degrees ! Estimated noise=1.71696 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 = 0.971497 Jy ! Component: 100 - total flux cleaned = 1.21906 Jy ! Total flux subtracted in 100 components = 1.21906 Jy ! Clean residual min=-0.035503 max=0.105205 Jy/beam ! Clean residual mean=-0.000130 rms=0.009318 Jy/beam ! Combined flux in latest and established models = 1.21906 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 1.21906 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.285498Jy sigma=3.415893 ! Fit after self-cal, rms=0.283454Jy sigma=3.390958 ! Inverting map ! Your choice of large map pixels excluded 2.26% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.122772 Jy ! Component: 100 - total flux cleaned = 0.187687 Jy ! Total flux subtracted in 100 components = 0.187687 Jy ! Clean residual min=-0.033841 max=0.037890 Jy/beam ! Clean residual mean=-0.000027 rms=0.006999 Jy/beam ! Combined flux in latest and established models = 1.40675 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 10 components and 1.40675 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.217652Jy sigma=2.462666 ! Fit after self-cal, rms=0.215845Jy sigma=2.433302 ! Inverting map ! Your choice of large map pixels excluded 2.26% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Added new window around map position (0.6, 1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0455315 Jy ! Component: 100 - total flux cleaned = 0.0488578 Jy ! Total flux subtracted in 100 components = 0.0488578 Jy ! Clean residual min=-0.033016 max=0.032889 Jy/beam ! Clean residual mean=-0.000001 rms=0.006509 Jy/beam ! Combined flux in latest and established models = 1.45561 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 14 components and 1.45561 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.205917Jy sigma=2.289070 ! Fit after self-cal, rms=0.205455Jy sigma=2.278293 ! Inverting map ! Your choice of large map pixels excluded 2.26% of the data. ! The y-axis pixel size should ideally be below 0.1827 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 2.26% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Estimated beam: bmin=1.116 mas, bmaj=1.212 mas, bpa=-36.78 degrees ! Estimated noise=1.38635 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 = 0.0297482 Jy ! Component: 100 - total flux cleaned = 0.0357707 Jy ! Component: 150 - total flux cleaned = 0.036865 Jy ! Component: 200 - total flux cleaned = 0.0383357 Jy ! Total flux subtracted in 200 components = 0.0383357 Jy ! Clean residual min=-0.033744 max=0.035178 Jy/beam ! Clean residual mean=-0.000028 rms=0.008782 Jy/beam ! Combined flux in latest and established models = 1.49394 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 21 components and 1.49394 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.199412Jy sigma=2.213856 ! Fit after self-cal, rms=0.199146Jy sigma=2.209099 ! Inverting map ! Your choice of large map pixels excluded 2.26% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.116 x 1.212 at -36.78 degrees (North through East) ! Clean map min=-0.032594 max=1.2518 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 18 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.79 MC 0.93 NY 0.85 WN 1.43 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.77 HN 0.96 NL 1.62 SC 0.99 ! ! Telescope amplitude corrections in sub-array 3: ! HN 1.04 NL 1.06 NY 0.85 SC 0.92 ! ! A total of 60 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 HN 1.04 KP 1.11 LA 1.00 ! MK 0.98 NL 1.04 OV 0.95 PT 0.85 ! SC 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 HN 1.02 KP 1.08 LA 0.99 ! MK 0.99 NL 1.04 NY 0.86 OV 0.95 ! PT 0.84 ! ! ! Correcting IF 2. ! A total of 18 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.79 MC 0.97 NY 0.98 WN 1.45 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.72 HN 1.00 NL 1.55 SC 1.04 ! ! Telescope amplitude corrections in sub-array 3: ! HN 1.02 NL 1.02 NY 0.97 SC 0.96 ! ! A total of 60 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 HN 1.04 KP 1.10 LA 1.02 ! MK 0.96 NL 1.03 OV 0.93 PT 0.86 ! SC 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 HN 1.02 KP 1.07 LA 1.01 ! MK 0.98 NL 1.03 NY 0.97 OV 0.93 ! PT 0.86 ! ! ! Correcting IF 3. ! A total of 18 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.00* MC 0.00* NY 0.00* WN 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.82 HN 1.01 NL 1.63 SC 1.01 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HN 0.00* NL 0.00* NY 0.00* SC 0.00* ! ! A total of 60 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 HN 1.04 KP 1.09 LA 1.02 ! MK 0.98 NL 1.05 OV 0.95 PT 0.85 ! SC 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 HN 1.03 KP 1.06 LA 1.01 ! MK 0.98 NL 1.05 NY 1.00* OV 0.95 ! PT 0.81 ! ! ! Correcting IF 4. ! A total of 18 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.00* MC 0.00* NY 0.00* WN 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.93 HN 1.00 NL 1.68 SC 1.12 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HN 0.00* NL 0.00* NY 0.00* SC 0.00* ! ! A total of 60 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 HN 1.05 KP 1.09 LA 1.02 ! MK 0.99 NL 1.05 OV 0.96 PT 0.84 ! SC 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 HN 1.03 KP 1.08 LA 1.01 ! MK 1.00 NL 1.06 NY 1.00* OV 0.95 ! PT 0.83 ! ! ! Fit before self-cal, rms=0.199146Jy sigma=2.209099 ! Fit after self-cal, rms=0.091401Jy sigma=1.002033 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Estimated beam: bmin=1.053 mas, bmaj=1.19 mas, bpa=-6.853 degrees ! Estimated noise=1.48913 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 = 0.00164802 Jy ! Component: 100 - total flux cleaned = 0.00038137 Jy ! Component: 150 - total flux cleaned = -0.000681759 Jy ! Component: 200 - total flux cleaned = -0.00184511 Jy ! Total flux subtracted in 200 components = -0.00184511 Jy ! Clean residual min=-0.012356 max=0.010429 Jy/beam ! Clean residual mean=0.000220 rms=0.002654 Jy/beam ! Combined flux in latest and established models = 1.4921 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 28 components and 1.4921 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.089215Jy sigma=0.974932 ! Fit after self-cal, rms=0.088465Jy sigma=0.969628 ! Inverting map ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 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=0.088465Jy sigma=0.969628 ! Fit after self-cal, rms=0.078657Jy sigma=0.817455 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Estimated beam: bmin=1.052 mas, bmaj=1.189 mas, bpa=-6.948 degrees ! Estimated noise=1.49089 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00580265 Jy ! Component: 100 - total flux cleaned = 0.00624143 Jy ! Component: 150 - total flux cleaned = 0.00623862 Jy ! Component: 200 - total flux cleaned = 0.00596324 Jy ! Total flux subtracted in 200 components = 0.00596324 Jy ! Clean residual min=-0.006487 max=0.008156 Jy/beam ! Clean residual mean=0.000012 rms=0.001455 Jy/beam ! Combined flux in latest and established models = 1.49806 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 36 components and 1.49806 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.077123Jy sigma=0.797961 ! Fit after self-cal, rms=0.076577Jy sigma=0.792517 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 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 (0.4, 2.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00269219 Jy ! Component: 100 - total flux cleaned = 0.00247853 Jy ! Component: 150 - total flux cleaned = 0.00248294 Jy ! Component: 200 - total flux cleaned = 0.00264682 Jy ! Total flux subtracted in 200 components = 0.00264682 Jy ! Clean residual min=-0.006159 max=0.006838 Jy/beam ! Clean residual mean=0.000016 rms=0.001365 Jy/beam ! Combined flux in latest and established models = 1.50071 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 50 components and 1.50071 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.075343Jy sigma=0.775202 ! Fit after self-cal, rms=0.075101Jy sigma=0.772645 ! Inverting map ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Added new window around map position (2.2, 20.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00184644 Jy ! Component: 100 - total flux cleaned = 0.00128555 Jy ! Component: 150 - total flux cleaned = 0.000976437 Jy ! Component: 200 - total flux cleaned = 0.000838741 Jy ! Total flux subtracted in 200 components = 0.000838741 Jy ! Clean residual min=-0.005946 max=0.006838 Jy/beam ! Clean residual mean=0.000016 rms=0.001304 Jy/beam ! Combined flux in latest and established models = 1.50155 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 56 components and 1.50155 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.074175Jy sigma=0.760265 ! Fit after self-cal, rms=0.073935Jy sigma=0.758549 ! Inverting map ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Added new window around map position (-36.2, 28.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00405432 Jy ! Component: 100 - total flux cleaned = 0.00597012 Jy ! Component: 150 - total flux cleaned = 0.00713631 Jy ! Component: 200 - total flux cleaned = 0.00816383 Jy ! Total flux subtracted in 200 components = 0.00816383 Jy ! Clean residual min=-0.005484 max=0.005390 Jy/beam ! Clean residual mean=0.000013 rms=0.001241 Jy/beam ! Combined flux in latest and established models = 1.50971 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 66 components and 1.50971 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.073012Jy sigma=0.748589 ! Fit after self-cal, rms=0.072856Jy sigma=0.747376 ! Inverting map ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 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=0.072856Jy sigma=0.747376 ! Fit after self-cal, rms=0.069695Jy sigma=0.725703 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Estimated beam: bmin=1.05 mas, bmaj=1.188 mas, bpa=-6.719 degrees ! Estimated noise=1.48991 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00356358 Jy ! Component: 100 - total flux cleaned = 0.00550196 Jy ! Component: 150 - total flux cleaned = 0.00640748 Jy ! Component: 200 - total flux cleaned = 0.00670966 Jy ! Total flux subtracted in 200 components = 0.00670966 Jy ! Clean residual min=-0.004776 max=0.005064 Jy/beam ! Clean residual mean=0.000009 rms=0.001091 Jy/beam ! Combined flux in latest and established models = 1.51642 Jy selfcal ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 77 components and 1.51642 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.069132Jy sigma=0.719212 ! Fit after self-cal, rms=0.068999Jy sigma=0.718235 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 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 (39.8, -19.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00150366 Jy ! Component: 100 - total flux cleaned = 0.00135418 Jy ! Component: 150 - total flux cleaned = 0.00144737 Jy ! Component: 200 - total flux cleaned = 0.00154776 Jy ! Total flux subtracted in 200 components = 0.00154776 Jy ! Clean residual min=-0.004611 max=0.004401 Jy/beam ! Clean residual mean=0.000008 rms=0.001058 Jy/beam ! Combined flux in latest and established models = 1.51797 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 92 components and 1.51797 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.068410Jy sigma=0.711421 ! Fit after self-cal, rms=0.068302Jy sigma=0.710690 ! Inverting map ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 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=0.068302Jy sigma=0.710690 ! Fit after self-cal, rms=0.068063Jy sigma=0.709436 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Estimated beam: bmin=2.3 mas, bmaj=2.545 mas, bpa=-40.82 degrees ! Estimated noise=1.88036 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00332033 Jy ! Component: 100 - total flux cleaned = 0.00408788 Jy ! Component: 150 - total flux cleaned = 0.00433878 Jy ! Component: 200 - total flux cleaned = 0.00461216 Jy ! Total flux subtracted in 200 components = 0.00461216 Jy ! Clean residual min=-0.005325 max=0.005239 Jy/beam ! Clean residual mean=0.000020 rms=0.001169 Jy/beam ! Combined flux in latest and established models = 1.52258 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 108 components and 1.52258 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.067983Jy sigma=0.707490 ! Fit after self-cal, rms=0.067940Jy sigma=0.707145 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 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 = 0.000135834 Jy ! Component: 100 - total flux cleaned = 0.000357566 Jy ! Component: 150 - total flux cleaned = 0.000556366 Jy ! Component: 200 - total flux cleaned = 0.000782854 Jy ! Total flux subtracted in 200 components = 0.000782854 Jy ! Clean residual min=-0.005245 max=0.005272 Jy/beam ! Clean residual mean=0.000020 rms=0.001166 Jy/beam ! Combined flux in latest and established models = 1.52336 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 113 components and 1.52336 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.067888Jy sigma=0.706190 ! Fit after self-cal, rms=0.067871Jy sigma=0.705959 ! Inverting map ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 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 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Estimated beam: bmin=1.049 mas, bmaj=1.187 mas, bpa=-6.667 degrees ! Estimated noise=1.49045 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.049 x 1.187 at -6.667 degrees (North through East) ! Clean map min=-0.0042632 max=1.2452 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=0.067871Jy sigma=0.705959 ! Fit after self-cal, rms=0.062859Jy sigma=0.642866 ! Inverting map and beam ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Estimated beam: bmin=1.048 mas, bmaj=1.187 mas, bpa=-6.763 degrees ! Estimated noise=1.49064 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00223708 Jy ! Component: 100 - total flux cleaned = 0.00261259 Jy ! Component: 150 - total flux cleaned = 0.0026155 Jy ! Component: 200 - total flux cleaned = 0.00269371 Jy ! Total flux subtracted in 200 components = 0.00269371 Jy ! Clean residual min=-0.004196 max=0.004270 Jy/beam ! Clean residual mean=0.000005 rms=0.001004 Jy/beam ! Combined flux in latest and established models = 1.52605 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 122 components and 1.52605 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.062508Jy sigma=0.639168 ! Fit after self-cal, rms=0.062443Jy sigma=0.638791 ! Inverting map ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Added new window around map position (-37.2, 7.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00307491 Jy ! Component: 100 - total flux cleaned = 0.00368368 Jy ! Component: 150 - total flux cleaned = 0.00393274 Jy ! Component: 200 - total flux cleaned = 0.00401076 Jy ! Total flux subtracted in 200 components = 0.00401076 Jy ! Clean residual min=-0.004210 max=0.004145 Jy/beam ! Clean residual mean=0.000001 rms=0.000982 Jy/beam ! Combined flux in latest and established models = 1.53007 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 134 components and 1.53007 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.062078Jy sigma=0.634464 ! Fit after self-cal, rms=0.062016Jy sigma=0.634077 ! Inverting map ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.062016Jy sigma=0.634077 ! Fit after self-cal, rms=0.061898Jy sigma=0.633456 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 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Estimated beam: bmin=0.9015 mas, bmaj=1.084 mas, bpa=-10.94 degrees ! Estimated noise=1.74198 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.961881 Jy ! Component: 100 - total flux cleaned = 1.23936 Jy ! Component: 150 - total flux cleaned = 1.36789 Jy ! Component: 200 - total flux cleaned = 1.42994 Jy ! Total flux subtracted in 200 components = 1.42994 Jy ! Clean residual min=-0.011088 max=0.029353 Jy/beam ! Clean residual mean=-0.000039 rms=0.002499 Jy/beam ! Combined flux in latest and established models = 1.42994 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 11 model components to the UV plane model. ! The established model now contains 11 components and 1.42994 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Estimated beam: bmin=1.048 mas, bmaj=1.187 mas, bpa=-6.697 degrees ! Estimated noise=1.49116 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 = 0.0409139 Jy ! Component: 100 - total flux cleaned = 0.0620915 Jy ! Component: 150 - total flux cleaned = 0.0743798 Jy ! Component: 200 - total flux cleaned = 0.0833708 Jy ! Total flux subtracted in 200 components = 0.0833708 Jy ! Clean residual min=-0.005717 max=0.007095 Jy/beam ! Clean residual mean=0.000004 rms=0.001306 Jy/beam ! Combined flux in latest and established models = 1.51331 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 28 components and 1.51331 Jy ! Inverting map ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Added new window around map position (-0.6, -1.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00604677 Jy ! Component: 100 - total flux cleaned = 0.00843336 Jy ! Component: 150 - total flux cleaned = 0.00990006 Jy ! Component: 200 - total flux cleaned = 0.0110476 Jy ! Total flux subtracted in 200 components = 0.0110476 Jy ! Clean residual min=-0.005176 max=0.005418 Jy/beam ! Clean residual mean=0.000007 rms=0.001192 Jy/beam ! Combined flux in latest and established models = 1.52436 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 43 components and 1.52436 Jy ! Inverting map ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Added new window around map position (-22, 4.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00251523 Jy ! Component: 100 - total flux cleaned = 0.00354016 Jy ! Component: 150 - total flux cleaned = 0.00450608 Jy ! Component: 200 - total flux cleaned = 0.005418 Jy ! Total flux subtracted in 200 components = 0.005418 Jy ! Clean residual min=-0.004774 max=0.004857 Jy/beam ! Clean residual mean=0.000006 rms=0.001122 Jy/beam ! Combined flux in latest and established models = 1.52978 Jy ! Adding 40 model components to the UV plane model. ! The established model now contains 58 components and 1.52978 Jy ! Inverting map ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Added new window around map position (-39.8, 3.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000954972 Jy ! Component: 100 - total flux cleaned = 0.00129413 Jy ! Component: 150 - total flux cleaned = 0.00113258 Jy ! Component: 200 - total flux cleaned = 0.00113625 Jy ! Total flux subtracted in 200 components = 0.00113625 Jy ! Clean residual min=-0.004716 max=0.004543 Jy/beam ! Clean residual mean=0.000005 rms=0.001072 Jy/beam ! Combined flux in latest and established models = 1.53091 Jy ! Adding 42 model components to the UV plane model. ! The established model now contains 70 components and 1.53091 Jy ! Inverting map ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 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 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Estimated beam: bmin=2.299 mas, bmaj=2.544 mas, bpa=-40.71 degrees ! Estimated noise=1.88346 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00350415 Jy ! Component: 100 - total flux cleaned = 0.00524862 Jy ! Component: 150 - total flux cleaned = 0.00599691 Jy ! Component: 200 - total flux cleaned = 0.00624818 Jy ! Total flux subtracted in 200 components = 0.00624818 Jy ! Clean residual min=-0.005363 max=0.004385 Jy/beam ! Clean residual mean=0.000008 rms=0.001081 Jy/beam ! Combined flux in latest and established models = 1.53716 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 = 0.000238853 Jy ! Component: 100 - total flux cleaned = 0.000678328 Jy ! Component: 150 - total flux cleaned = 0.0010878 Jy ! Component: 200 - total flux cleaned = 0.0013444 Jy ! Total flux subtracted in 200 components = 0.0013444 Jy ! Clean residual min=-0.005265 max=0.004324 Jy/beam ! Clean residual mean=0.000005 rms=0.001049 Jy/beam ! Combined flux in latest and established models = 1.5385 Jy ! Adding 44 model components to the UV plane model. ! The established model now contains 113 components and 1.5385 Jy ! Inverting map ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! Estimated beam: bmin=1.048 mas, bmaj=1.187 mas, bpa=-6.697 degrees ! Estimated noise=1.49116 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00162446 Jy ! Component: 100 - total flux cleaned = -0.00176742 Jy ! Component: 150 - total flux cleaned = -0.00177178 Jy ! Component: 200 - total flux cleaned = -0.00177636 Jy ! Total flux subtracted in 200 components = -0.00177636 Jy ! Clean residual min=-0.004388 max=0.004235 Jy/beam ! Clean residual mean=0.000001 rms=0.001007 Jy/beam ! Combined flux in latest and established models = 1.53673 Jy selfcal ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 117 components and 1.53673 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.064001Jy sigma=0.647217 ! Fit after self-cal, rms=0.063267Jy sigma=0.639557 wmodel J2236+2828_X_map.mod ! Writing 117 model components to file: J2236+2828_X_map.mod wobs J2236+2828_X_uvs.fits ! Writing UV FITS file: J2236+2828_X_uvs.fits wwins J2236+2828_X_map.win ! wwins: Wrote 10 windows to J2236+2828_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 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000166402 Jy ! Component: 100 - total flux cleaned = 0.000164609 Jy ! Component: 150 - total flux cleaned = -5.38352e-05 Jy ! Component: 200 - total flux cleaned = -0.000193701 Jy ! Component: 250 - total flux cleaned = -0.000193935 Jy ! Component: 300 - total flux cleaned = -0.000531988 Jy ! Component: 350 - total flux cleaned = -0.000597877 Jy ! Component: 400 - total flux cleaned = -0.00072887 Jy ! Component: 450 - total flux cleaned = -0.000793865 Jy ! Component: 500 - total flux cleaned = -0.00104875 Jy ! Component: 550 - total flux cleaned = -0.00136144 Jy ! Component: 600 - total flux cleaned = -0.00154687 Jy ! Component: 650 - total flux cleaned = -0.00160787 Jy ! Component: 700 - total flux cleaned = -0.00202795 Jy ! Component: 750 - total flux cleaned = -0.00220537 Jy ! Component: 800 - total flux cleaned = -0.00226433 Jy ! Component: 850 - total flux cleaned = -0.00267151 Jy ! Component: 900 - total flux cleaned = -0.00267218 Jy ! Component: 950 - total flux cleaned = -0.00318485 Jy ! Component: 1000 - total flux cleaned = -0.00324047 Jy ! Component: 1050 - total flux cleaned = -0.00351958 Jy ! Component: 1100 - total flux cleaned = -0.00368527 Jy ! Component: 1150 - total flux cleaned = -0.00379487 Jy ! Component: 1200 - total flux cleaned = -0.00390416 Jy ! Component: 1250 - total flux cleaned = -0.00411993 Jy ! Component: 1300 - total flux cleaned = -0.00433371 Jy ! Component: 1350 - total flux cleaned = -0.00428104 Jy ! Component: 1400 - total flux cleaned = -0.00443936 Jy ! Component: 1450 - total flux cleaned = -0.00475284 Jy ! Component: 1500 - total flux cleaned = -0.00480475 Jy ! Component: 1550 - total flux cleaned = -0.00501054 Jy ! Component: 1600 - total flux cleaned = -0.0051123 Jy ! Component: 1650 - total flux cleaned = -0.00516299 Jy ! Component: 1700 - total flux cleaned = -0.00526344 Jy ! Component: 1750 - total flux cleaned = -0.00531298 Jy ! Component: 1800 - total flux cleaned = -0.00531343 Jy ! Component: 1850 - total flux cleaned = -0.00555915 Jy ! Component: 1900 - total flux cleaned = -0.00555958 Jy ! Component: 1950 - total flux cleaned = -0.00580162 Jy ! Component: 2000 - total flux cleaned = -0.00575424 Jy ! Component: 2050 - total flux cleaned = -0.00608869 Jy ! Component: 2100 - total flux cleaned = -0.00627833 Jy ! Component: 2150 - total flux cleaned = -0.00632509 Jy ! Component: 2200 - total flux cleaned = -0.00655921 Jy ! Component: 2250 - total flux cleaned = -0.00655913 Jy ! Component: 2300 - total flux cleaned = -0.00674338 Jy ! Component: 2350 - total flux cleaned = -0.00674354 Jy ! Component: 2400 - total flux cleaned = -0.00701708 Jy ! Component: 2450 - total flux cleaned = -0.00692622 Jy ! Component: 2500 - total flux cleaned = -0.00701611 Jy ! Component: 2550 - total flux cleaned = -0.00715058 Jy ! Component: 2600 - total flux cleaned = -0.00706149 Jy ! Component: 2650 - total flux cleaned = -0.00710575 Jy ! Component: 2700 - total flux cleaned = -0.00715006 Jy ! Component: 2750 - total flux cleaned = -0.00728142 Jy ! Component: 2800 - total flux cleaned = -0.00723775 Jy ! Component: 2850 - total flux cleaned = -0.00732406 Jy ! Component: 2900 - total flux cleaned = -0.00749593 Jy ! Component: 2950 - total flux cleaned = -0.00753832 Jy ! Component: 3000 - total flux cleaned = -0.0075381 Jy ! Component: 3050 - total flux cleaned = -0.00762255 Jy ! Component: 3100 - total flux cleaned = -0.00766476 Jy ! Component: 3150 - total flux cleaned = -0.00795717 Jy ! Component: 3200 - total flux cleaned = -0.00799861 Jy ! Component: 3250 - total flux cleaned = -0.00791584 Jy ! Component: 3300 - total flux cleaned = -0.00808044 Jy ! Component: 3350 - total flux cleaned = -0.0081217 Jy ! Component: 3400 - total flux cleaned = -0.0081218 Jy ! Component: 3450 - total flux cleaned = -0.00820265 Jy ! Component: 3500 - total flux cleaned = -0.00844435 Jy ! Component: 3550 - total flux cleaned = -0.0084441 Jy ! Component: 3600 - total flux cleaned = -0.00848389 Jy ! Component: 3650 - total flux cleaned = -0.00832504 Jy ! Component: 3700 - total flux cleaned = -0.00860175 Jy ! Component: 3750 - total flux cleaned = -0.00856238 Jy ! Component: 3800 - total flux cleaned = -0.00848448 Jy ! Component: 3850 - total flux cleaned = -0.00840674 Jy ! Component: 3900 - total flux cleaned = -0.00848447 Jy ! Component: 3950 - total flux cleaned = -0.00852309 Jy ! Component: 4000 - total flux cleaned = -0.00848464 Jy ! Component: 4050 - total flux cleaned = -0.00856127 Jy ! Total flux subtracted in 4096 components = -0.00875136 Jy ! Clean residual min=-0.002470 max=0.002155 Jy/beam ! Clean residual mean=0.000004 rms=0.000631 Jy/beam ! Combined flux in latest and established models = 1.52798 Jy keep ! Adding 332 model components to the UV plane model. ! The established model now contains 448 components and 1.52798 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv125_uvs/J2236+2828_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.048 x 1.187 at -6.697 degrees (North through East) ! Clean map min=-0.0033667 max=1.2419 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv125_uvs/J2236+2828_X_map.fits wmodel /scr/pima/rv125_uvs/J2236+2828_X_map.mod ! Writing 448 model components to file: /scr/pima/rv125_uvs/J2236+2828_X_map.mod wobs /scr/pima/rv125_uvs/J2236+2828_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv125_uvs/J2236+2828_X_uvs.fits wwins /scr/pima/rv125_uvs/J2236+2828_X_map.win ! wwins: Wrote 11 windows to /scr/pima/rv125_uvs/J2236+2828_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 1.24192 invert ! Inverting map ! Your choice of large map pixels excluded 2.16% of the data. ! The y-axis pixel size should ideally be below 0.1827 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000631672 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.152587 0.152587 0.305174 0.610349 1.2207 2.44139 4.88279 9.76558 19.5312 39.0623 78.1246 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0018 print "peak= ", int(1000*peak_flux)/1000 ! peak= 1.241 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1966.09 quit ! Quitting program ! Log file /scr/pima/rv125_uvs/J2236+2828_X_dfm.log closed on Sun Dec 23 02:54:10 2018