! Started logfile: /scr/pima/rv123_uvs/J2359+3850_X_dfm.log on Sun Dec 23 00:46:06 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/rv123_uvs/J2359+3850_X_uva.fits ! Reading UV FITS file: /scr/pima/rv123_uvs/J2359+3850_X_uva.fits ! AN table 1: 16 integrations on 28 of 28 possible baselines. ! AN table 2: 108 integrations on 21 of 21 possible baselines. ! AN table 3: 23 integrations on 28 of 28 possible baselines. ! AN table 4: 29 integrations on 55 of 55 possible baselines. ! AN table 5: 16 integrations on 28 of 28 possible baselines. ! AN table 6: 37 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.661856 visibilities/baseline/integration-bin. ! Found source: J2359+3850 ! ! 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 89 lines of history. ! ! Reading 18712 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 J2359+3850_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 16 telescope corrections were flagged in sub-array 1. ! A total of 205 telescope corrections were flagged in sub-array 2. ! A total of 82 telescope corrections were flagged in sub-array 3. ! A total of 8 telescope corrections were flagged in sub-array 4. ! A total of 104 telescope corrections were flagged in sub-array 5. ! A total of 136 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 16 telescope corrections were flagged in sub-array 1. ! A total of 205 telescope corrections were flagged in sub-array 2. ! A total of 82 telescope corrections were flagged in sub-array 3. ! A total of 8 telescope corrections were flagged in sub-array 4. ! A total of 104 telescope corrections were flagged in sub-array 5. ! A total of 136 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 30 telescope corrections were flagged in sub-array 1. ! A total of 351 telescope corrections were flagged in sub-array 2. ! A total of 82 telescope corrections were flagged in sub-array 3. ! A total of 39 telescope corrections were flagged in sub-array 4. ! A total of 104 telescope corrections were flagged in sub-array 5. ! A total of 147 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 30 telescope corrections were flagged in sub-array 1. ! A total of 351 telescope corrections were flagged in sub-array 2. ! A total of 82 telescope corrections were flagged in sub-array 3. ! A total of 39 telescope corrections were flagged in sub-array 4. ! A total of 104 telescope corrections were flagged in sub-array 5. ! A total of 147 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.023692Jy sigma=15.752621 ! Fit after self-cal, rms=0.789731Jy sigma=11.742245 ! 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 3.11% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=0.66 mas, bmaj=0.9132 mas, bpa=-4.875 degrees ! Estimated noise=0.6623 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 = 0.178259 Jy ! Component: 100 - total flux cleaned = 0.23311 Jy ! Total flux subtracted in 100 components = 0.23311 Jy ! Clean residual min=-0.006785 max=0.022650 Jy/beam ! Clean residual mean=-0.000029 rms=0.001537 Jy/beam ! Combined flux in latest and established models = 0.23311 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.23311 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.112513Jy sigma=1.304714 ! Fit after self-cal, rms=0.111843Jy sigma=1.303754 ! Inverting map ! Your choice of large map pixels excluded 3.11% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0237036 Jy ! Component: 100 - total flux cleaned = 0.0361519 Jy ! Total flux subtracted in 100 components = 0.0361519 Jy ! Clean residual min=-0.005975 max=0.010612 Jy/beam ! Clean residual mean=-0.000024 rms=0.001297 Jy/beam ! Combined flux in latest and established models = 0.269262 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 17 components and 0.269262 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.107698Jy sigma=1.178002 ! Fit after self-cal, rms=0.107740Jy sigma=1.177767 ! Inverting map ! Your choice of large map pixels excluded 3.11% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Added new window around map position (-0.6, -2.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.010293 Jy ! Component: 100 - total flux cleaned = 0.0169119 Jy ! Total flux subtracted in 100 components = 0.0169119 Jy ! Clean residual min=-0.005821 max=0.008401 Jy/beam ! Clean residual mean=-0.000022 rms=0.001231 Jy/beam ! Combined flux in latest and established models = 0.286174 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 25 components and 0.286174 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.107347Jy sigma=1.155079 ! Fit after self-cal, rms=0.107163Jy sigma=1.153021 ! Inverting map ! Your choice of large map pixels excluded 3.11% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Added new window around map position (5.6, 1.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00729748 Jy ! Component: 100 - total flux cleaned = 0.0105648 Jy ! Total flux subtracted in 100 components = 0.0105648 Jy ! Clean residual min=-0.005613 max=0.007375 Jy/beam ! Clean residual mean=-0.000022 rms=0.001190 Jy/beam ! Combined flux in latest and established models = 0.296739 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 31 components and 0.296739 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.106956Jy sigma=1.143853 ! Fit after self-cal, rms=0.106883Jy sigma=1.143029 ! Inverting map ! Your choice of large map pixels excluded 3.11% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 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 3.11% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=0.8156 mas, bmaj=1.049 mas, bpa=-1.39 degrees ! Estimated noise=0.393289 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 = 0.00180972 Jy ! Component: 100 - total flux cleaned = 0.00243134 Jy ! Component: 150 - total flux cleaned = 0.00263257 Jy ! Component: 200 - total flux cleaned = 0.00271762 Jy ! Total flux subtracted in 200 components = 0.00271762 Jy ! Clean residual min=-0.009231 max=0.007330 Jy/beam ! Clean residual mean=-0.000820 rms=0.002178 Jy/beam ! Combined flux in latest and established models = 0.299456 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 43 components and 0.299456 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.106648Jy sigma=1.138054 ! Fit after self-cal, rms=0.106619Jy sigma=1.137609 ! Inverting map ! Your choice of large map pixels excluded 3.11% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8156 x 1.049 at -1.39 degrees (North through East) ! Clean map min=-0.0088895 max=0.22341 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 KP 1.11 LA 1.10 MK 1.04 ! NL 1.23 NY 0.62 OV 0.97 YG 1.27 ! ! A total of 63 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.88 MC 0.90 NY 0.75 ON 0.93 ! WN 1.55 WZ 1.10 YG 1.05 ! ! A total of 18 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 0.88 HN 1.05 KP 1.08 ! NL 1.02 OV 0.92 SC 0.89 WN 1.45 ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 0.87 HN 1.03 KP 1.08 ! LA 0.99 NL 1.02 NY 0.77 ON 0.87 ! OV 0.94 PT 0.87 WN 1.53 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.06 FD 0.81 KP 1.14 LA 1.01 ! MK 0.95 OV 0.96 PT 0.89 WN 1.65 ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.00 FD 0.87 HN 1.06 KP 1.04 ! LA 1.01 MK 1.05 NL 1.02 NY 0.82 ! OV 0.95 PT 0.85 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 KP 1.08 LA 1.13 MK 1.07 ! NL 1.16 NY 0.76 OV 0.99 YG 1.24 ! ! A total of 63 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.91 MC 0.98 NY 0.89 ON 0.88 ! WN 1.49 WZ 1.04 YG 1.07 ! ! A total of 18 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 FD 0.86 HN 1.02 KP 1.08 ! NL 1.04 OV 0.90 SC 0.93 WN 1.28 ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 0.86 HN 1.03 KP 1.10 ! LA 1.01 NL 1.03 NY 0.90 ON 0.82 ! OV 0.95 PT 0.88 WN 1.43 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 FD 0.86 KP 1.04 LA 1.03 ! MK 0.95 OV 0.99 PT 0.89 WN 1.43 ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.00 FD 0.88 HN 1.10 KP 1.04 ! LA 1.02 MK 1.05 NL 1.02 NY 0.91 ! OV 0.94 PT 0.84 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 KP 1.10 LA 1.12 MK 1.06 ! NL 1.23 NY 1.00* OV 0.99 YG 1.50 ! ! A total of 87 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.97 MC 1.40 NY 1.00* ON 1.25 ! WN 1.44 WZ 1.18 YG 0.89 ! ! A total of 18 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 0.88 HN 1.04 KP 1.11 ! NL 1.05 OV 0.92 SC 0.93 WN 1.60 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 FD 0.87 HN 1.05 KP 1.12 ! LA 1.01 NL 1.03 NY 1.00* ON 1.04 ! OV 0.97 PT 0.89 WN 1.42 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 FD 0.90 KP 1.11 LA 0.95 ! MK 1.05 OV 0.94 PT 0.89 WN 1.77 ! ! A total of 21 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 FD 0.89 HN 1.08 KP 1.05 ! LA 1.02 MK 1.07 NL 1.05 NY 1.00* ! OV 0.94 PT 0.88 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 KP 1.05 LA 1.18 MK 1.07 ! NL 1.27 NY 1.00* OV 0.97 YG 1.50 ! ! A total of 87 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 1.07 MC 1.38 NY 1.00* ON 1.19 ! WN 1.38 WZ 1.17 YG 0.87 ! ! A total of 18 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.10 FD 0.87 HN 1.05 KP 1.10 ! NL 1.04 OV 0.97 SC 0.91 WN 1.25 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.05 FD 0.87 HN 1.05 KP 1.09 ! LA 1.02 NL 1.02 NY 1.00* ON 1.02 ! OV 0.95 PT 0.90 WN 1.41 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 FD 0.83 KP 1.12 LA 1.00 ! MK 0.96 OV 1.05 PT 0.82 WN 1.54 ! ! A total of 21 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 FD 0.87 HN 1.06 KP 1.06 ! LA 1.02 MK 1.05 NL 1.04 NY 1.00* ! OV 0.96 PT 0.88 ! ! ! Fit before self-cal, rms=0.106619Jy sigma=1.137609 ! Fit after self-cal, rms=0.107076Jy sigma=0.923776 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=0.8283 mas, bmaj=1.09 mas, bpa=-2.355 degrees ! Estimated noise=0.400184 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 = -0.00351354 Jy ! Component: 100 - total flux cleaned = -0.00404803 Jy ! Component: 150 - total flux cleaned = -0.0043717 Jy ! Component: 200 - total flux cleaned = -0.00460075 Jy ! Total flux subtracted in 200 components = -0.00460075 Jy ! Clean residual min=-0.002495 max=0.002559 Jy/beam ! Clean residual mean=-0.000005 rms=0.000601 Jy/beam ! Combined flux in latest and established models = 0.294856 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 49 components and 0.294856 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.106889Jy sigma=0.919988 ! Fit after self-cal, rms=0.106685Jy sigma=0.918688 ! Inverting map ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 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=0.106685Jy sigma=0.918688 ! Fit after self-cal, rms=0.106832Jy sigma=0.905367 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=0.8288 mas, bmaj=1.088 mas, bpa=-2.089 degrees ! Estimated noise=0.400042 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000850117 Jy ! Component: 100 - total flux cleaned = -0.00115926 Jy ! Component: 150 - total flux cleaned = -0.00143141 Jy ! Component: 200 - total flux cleaned = -0.00162576 Jy ! Total flux subtracted in 200 components = -0.00162576 Jy ! Clean residual min=-0.002045 max=0.002159 Jy/beam ! Clean residual mean=-0.000018 rms=0.000416 Jy/beam ! Combined flux in latest and established models = 0.29323 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 49 components and 0.29323 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.106732Jy sigma=0.904056 ! Fit after self-cal, rms=0.106829Jy sigma=0.903778 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 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 (-1.6, -1.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00100217 Jy ! Component: 100 - total flux cleaned = 0.000773126 Jy ! Component: 150 - total flux cleaned = 0.000570386 Jy ! Component: 200 - total flux cleaned = 0.00039378 Jy ! Total flux subtracted in 200 components = 0.00039378 Jy ! Clean residual min=-0.001887 max=0.001921 Jy/beam ! Clean residual mean=-0.000021 rms=0.000406 Jy/beam ! Combined flux in latest and established models = 0.293624 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 58 components and 0.293624 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.106757Jy sigma=0.902479 ! Fit after self-cal, rms=0.106720Jy sigma=0.902338 ! Inverting map ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Added new window around map position (-38.4, 11.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00133021 Jy ! Component: 100 - total flux cleaned = 0.00151865 Jy ! Component: 150 - total flux cleaned = 0.00155639 Jy ! Component: 200 - total flux cleaned = 0.00148085 Jy ! Total flux subtracted in 200 components = 0.00148085 Jy ! Clean residual min=-0.001848 max=0.001733 Jy/beam ! Clean residual mean=-0.000029 rms=0.000394 Jy/beam ! Combined flux in latest and established models = 0.295104 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 68 components and 0.295104 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.106663Jy sigma=0.901437 ! Fit after self-cal, rms=0.106642Jy sigma=0.901361 ! Inverting map ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 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=0.106642Jy sigma=0.901361 ! Fit after self-cal, rms=0.106197Jy sigma=0.898399 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=0.8327 mas, bmaj=1.082 mas, bpa=-1.745 degrees ! Estimated noise=0.399758 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -2.34206e-05 Jy ! Component: 100 - total flux cleaned = 8.13709e-05 Jy ! Component: 150 - total flux cleaned = 4.21297e-05 Jy ! Component: 200 - total flux cleaned = 4.57435e-06 Jy ! Total flux subtracted in 200 components = 4.57435e-06 Jy ! Clean residual min=-0.001679 max=0.001628 Jy/beam ! Clean residual mean=-0.000012 rms=0.000369 Jy/beam ! Combined flux in latest and established models = 0.295109 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 70 components and 0.295109 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.106136Jy sigma=0.897641 ! Fit after self-cal, rms=0.106080Jy sigma=0.897515 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 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 = -4.35792e-05 Jy ! Component: 100 - total flux cleaned = -7.47341e-06 Jy ! Component: 150 - total flux cleaned = -3.97962e-05 Jy ! Component: 200 - total flux cleaned = -4.00917e-05 Jy ! Total flux subtracted in 200 components = -4.00917e-05 Jy ! Clean residual min=-0.001680 max=0.001613 Jy/beam ! Clean residual mean=-0.000012 rms=0.000366 Jy/beam ! Combined flux in latest and established models = 0.295069 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 72 components and 0.295069 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.106038Jy sigma=0.897115 ! Fit after self-cal, rms=0.106002Jy sigma=0.897039 ! Inverting map ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 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=0.106002Jy sigma=0.897039 ! Fit after self-cal, rms=0.105755Jy sigma=0.896837 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=2.672 mas, bmaj=3.009 mas, bpa=87.93 degrees ! Estimated noise=0.460588 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000162072 Jy ! Component: 100 - total flux cleaned = -0.000141472 Jy ! Component: 150 - total flux cleaned = -0.000125966 Jy ! Component: 200 - total flux cleaned = -0.000112542 Jy ! Total flux subtracted in 200 components = -0.000112542 Jy ! Clean residual min=-0.001278 max=0.001561 Jy/beam ! Clean residual mean=-0.000014 rms=0.000385 Jy/beam ! Combined flux in latest and established models = 0.294956 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 81 components and 0.294956 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.105758Jy sigma=0.896702 ! Fit after self-cal, rms=0.105742Jy sigma=0.896628 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 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 = -6.47515e-05 Jy ! Component: 100 - total flux cleaned = -0.000104621 Jy ! Component: 150 - total flux cleaned = -6.67404e-05 Jy ! Component: 200 - total flux cleaned = -6.61329e-05 Jy ! Total flux subtracted in 200 components = -6.61329e-05 Jy ! Clean residual min=-0.001295 max=0.001547 Jy/beam ! Clean residual mean=-0.000013 rms=0.000383 Jy/beam ! Combined flux in latest and established models = 0.29489 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 84 components and 0.29489 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.105746Jy sigma=0.896612 ! Fit after self-cal, rms=0.105743Jy sigma=0.896571 ! Inverting map ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 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 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=0.8352 mas, bmaj=1.079 mas, bpa=-1.496 degrees ! Estimated noise=0.399603 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8352 x 1.079 at -1.496 degrees (North through East) ! Clean map min=-0.0015038 max=0.22605 Jy/beam if(peak(flux) > thresh) selfcal true, true clean clean_niter,clean_gain selfcal flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) selfcal true, true end if print "============== Clearing model and starting over ==========" ! ============== Clearing model and starting over ========== clrmod true ! clrmod: Cleared the established and tentative models. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=0.6867 mas, bmaj=0.9281 mas, bpa=-4.757 degrees ! Estimated noise=0.673066 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.178504 Jy ! Component: 100 - total flux cleaned = 0.231671 Jy ! Component: 150 - total flux cleaned = 0.252937 Jy ! Component: 200 - total flux cleaned = 0.264532 Jy ! Total flux subtracted in 200 components = 0.264532 Jy ! Clean residual min=-0.002989 max=0.006688 Jy/beam ! Clean residual mean=-0.000006 rms=0.000724 Jy/beam ! Combined flux in latest and established models = 0.264532 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 12 model components to the UV plane model. ! The established model now contains 12 components and 0.264532 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=0.8352 mas, bmaj=1.079 mas, bpa=-1.496 degrees ! Estimated noise=0.399603 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 = 0.0112353 Jy ! Component: 100 - total flux cleaned = 0.0175468 Jy ! Component: 150 - total flux cleaned = 0.021408 Jy ! Component: 200 - total flux cleaned = 0.0240061 Jy ! Total flux subtracted in 200 components = 0.0240061 Jy ! Clean residual min=-0.001716 max=0.002183 Jy/beam ! Clean residual mean=0.000017 rms=0.000390 Jy/beam ! Combined flux in latest and established models = 0.288538 Jy ! Adding 25 model components to the UV plane model. ! The established model now contains 29 components and 0.288538 Jy ! Inverting map ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Added new window around map position (0.2, -3.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00218926 Jy ! Component: 100 - total flux cleaned = 0.00377511 Jy ! Component: 150 - total flux cleaned = 0.00498711 Jy ! Component: 200 - total flux cleaned = 0.00550203 Jy ! Total flux subtracted in 200 components = 0.00550203 Jy ! Clean residual min=-0.001684 max=0.001532 Jy/beam ! Clean residual mean=-0.000003 rms=0.000357 Jy/beam ! Combined flux in latest and established models = 0.29404 Jy ! Adding 30 model components to the UV plane model. ! The established model now contains 48 components and 0.29404 Jy ! Inverting map ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 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 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=2.672 mas, bmaj=3.009 mas, bpa=87.93 degrees ! Estimated noise=0.460588 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000844348 Jy ! Component: 100 - total flux cleaned = 0.00113919 Jy ! Component: 150 - total flux cleaned = 0.00135406 Jy ! Component: 200 - total flux cleaned = 0.00144522 Jy ! Total flux subtracted in 200 components = 0.00144522 Jy ! Clean residual min=-0.001301 max=0.001584 Jy/beam ! Clean residual mean=-0.000018 rms=0.000383 Jy/beam ! Combined flux in latest and established models = 0.295485 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 = 5.52441e-05 Jy ! Component: 100 - total flux cleaned = 7.43611e-05 Jy ! Component: 150 - total flux cleaned = 7.52814e-05 Jy ! Component: 200 - total flux cleaned = 7.53855e-05 Jy ! Total flux subtracted in 200 components = 7.53855e-05 Jy ! Clean residual min=-0.001288 max=0.001584 Jy/beam ! Clean residual mean=-0.000018 rms=0.000382 Jy/beam ! Combined flux in latest and established models = 0.295561 Jy ! Adding 23 model components to the UV plane model. ! The established model now contains 67 components and 0.295561 Jy ! Inverting map ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! Estimated beam: bmin=0.8352 mas, bmaj=1.079 mas, bpa=-1.496 degrees ! Estimated noise=0.399603 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000279726 Jy ! Component: 100 - total flux cleaned = -0.000244184 Jy ! Component: 150 - total flux cleaned = -0.00017912 Jy ! Component: 200 - total flux cleaned = -0.000148634 Jy ! Total flux subtracted in 200 components = -0.000148634 Jy ! Clean residual min=-0.001657 max=0.001527 Jy/beam ! Clean residual mean=-0.000009 rms=0.000351 Jy/beam ! Combined flux in latest and established models = 0.295412 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 74 components and 0.295412 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.105539Jy sigma=0.895808 ! Fit after self-cal, rms=0.105429Jy sigma=0.895418 wmodel J2359+3850_X_map.mod ! Writing 74 model components to file: J2359+3850_X_map.mod wobs J2359+3850_X_uvs.fits ! Writing UV FITS file: J2359+3850_X_uvs.fits wwins J2359+3850_X_map.win ! wwins: Wrote 6 windows to J2359+3850_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 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 3.64704e-05 Jy ! Component: 100 - total flux cleaned = 0.000116145 Jy ! Component: 150 - total flux cleaned = 0.000243644 Jy ! Component: 200 - total flux cleaned = 0.000268928 Jy ! Component: 250 - total flux cleaned = 0.000268834 Jy ! Component: 300 - total flux cleaned = 0.000172981 Jy ! Component: 350 - total flux cleaned = 7.87055e-05 Jy ! Component: 400 - total flux cleaned = -1.43712e-05 Jy ! Component: 450 - total flux cleaned = -0.000129361 Jy ! Component: 500 - total flux cleaned = -0.000265692 Jy ! Component: 550 - total flux cleaned = -0.000333167 Jy ! Component: 600 - total flux cleaned = -0.000422365 Jy ! Component: 650 - total flux cleaned = -0.000422461 Jy ! Component: 700 - total flux cleaned = -0.000553735 Jy ! Component: 750 - total flux cleaned = -0.000510301 Jy ! Component: 800 - total flux cleaned = -0.000596524 Jy ! Component: 850 - total flux cleaned = -0.000596667 Jy ! Component: 900 - total flux cleaned = -0.000639354 Jy ! Component: 950 - total flux cleaned = -0.000702694 Jy ! Component: 1000 - total flux cleaned = -0.00074464 Jy ! Component: 1050 - total flux cleaned = -0.000744641 Jy ! Component: 1100 - total flux cleaned = -0.000765468 Jy ! Component: 1150 - total flux cleaned = -0.000868277 Jy ! Component: 1200 - total flux cleaned = -0.000888702 Jy ! Component: 1250 - total flux cleaned = -0.000969839 Jy ! Component: 1300 - total flux cleaned = -0.00094964 Jy ! Component: 1350 - total flux cleaned = -0.000969711 Jy ! Component: 1400 - total flux cleaned = -0.000989927 Jy ! Component: 1450 - total flux cleaned = -0.00106923 Jy ! Component: 1500 - total flux cleaned = -0.00104948 Jy ! Component: 1550 - total flux cleaned = -0.00106921 Jy ! Component: 1600 - total flux cleaned = -0.0011668 Jy ! Component: 1650 - total flux cleaned = -0.00112804 Jy ! Component: 1700 - total flux cleaned = -0.00120513 Jy ! Component: 1750 - total flux cleaned = -0.00124362 Jy ! Component: 1800 - total flux cleaned = -0.00126276 Jy ! Component: 1850 - total flux cleaned = -0.00128169 Jy ! Component: 1900 - total flux cleaned = -0.00130058 Jy ! Component: 1950 - total flux cleaned = -0.00128184 Jy ! Component: 2000 - total flux cleaned = -0.00126323 Jy ! Component: 2050 - total flux cleaned = -0.00137527 Jy ! Component: 2100 - total flux cleaned = -0.00139381 Jy ! Component: 2150 - total flux cleaned = -0.00135675 Jy ! Component: 2200 - total flux cleaned = -0.00141204 Jy ! Component: 2250 - total flux cleaned = -0.00141209 Jy ! Component: 2300 - total flux cleaned = -0.00143037 Jy ! Component: 2350 - total flux cleaned = -0.00146674 Jy ! Component: 2400 - total flux cleaned = -0.00148488 Jy ! Component: 2450 - total flux cleaned = -0.00148494 Jy ! Component: 2500 - total flux cleaned = -0.00152108 Jy ! Component: 2550 - total flux cleaned = -0.00155688 Jy ! Component: 2600 - total flux cleaned = -0.00155695 Jy ! Component: 2650 - total flux cleaned = -0.00161037 Jy ! Component: 2700 - total flux cleaned = -0.00159263 Jy ! Component: 2750 - total flux cleaned = -0.00166315 Jy ! Component: 2800 - total flux cleaned = -0.0016281 Jy ! Component: 2850 - total flux cleaned = -0.00169819 Jy ! Component: 2900 - total flux cleaned = -0.00169812 Jy ! Component: 2950 - total flux cleaned = -0.00169807 Jy ! Component: 3000 - total flux cleaned = -0.00171537 Jy ! Component: 3050 - total flux cleaned = -0.00168091 Jy ! Component: 3100 - total flux cleaned = -0.00173251 Jy ! Component: 3150 - total flux cleaned = -0.00176675 Jy ! Component: 3200 - total flux cleaned = -0.00178381 Jy ! Component: 3250 - total flux cleaned = -0.00173268 Jy ! Component: 3300 - total flux cleaned = -0.00180052 Jy ! Component: 3350 - total flux cleaned = -0.00185124 Jy ! Component: 3400 - total flux cleaned = -0.0018344 Jy ! Component: 3450 - total flux cleaned = -0.00181757 Jy ! Component: 3500 - total flux cleaned = -0.00185099 Jy ! Component: 3550 - total flux cleaned = -0.0018176 Jy ! Component: 3600 - total flux cleaned = -0.00185086 Jy ! Component: 3650 - total flux cleaned = -0.00188405 Jy ! Component: 3700 - total flux cleaned = -0.00188401 Jy ! Component: 3750 - total flux cleaned = -0.00191703 Jy ! Component: 3800 - total flux cleaned = -0.00190057 Jy ! Component: 3850 - total flux cleaned = -0.00194979 Jy ! Component: 3900 - total flux cleaned = -0.00191711 Jy ! Component: 3950 - total flux cleaned = -0.00191712 Jy ! Component: 4000 - total flux cleaned = -0.0019009 Jy ! Component: 4050 - total flux cleaned = -0.00196576 Jy ! Total flux subtracted in 4096 components = -0.00198194 Jy ! Clean residual min=-0.000849 max=0.001170 Jy/beam ! Clean residual mean=-0.000000 rms=0.000270 Jy/beam ! Combined flux in latest and established models = 0.29343 Jy keep ! Adding 339 model components to the UV plane model. ! The established model now contains 413 components and 0.29343 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv123_uvs/J2359+3850_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8352 x 1.079 at -1.496 degrees (North through East) ! Clean map min=-0.0013205 max=0.22713 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv123_uvs/J2359+3850_X_map.fits wmodel /scr/pima/rv123_uvs/J2359+3850_X_map.mod ! Writing 413 model components to file: /scr/pima/rv123_uvs/J2359+3850_X_map.mod wobs /scr/pima/rv123_uvs/J2359+3850_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv123_uvs/J2359+3850_X_uvs.fits wwins /scr/pima/rv123_uvs/J2359+3850_X_map.win ! wwins: Wrote 7 windows to /scr/pima/rv123_uvs/J2359+3850_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.227132 invert ! Inverting map ! Your choice of large map pixels excluded 3.2% of the data. ! The x-axis pixel size should ideally be below 0.1733 milli-arcsec ! The y-axis pixel size should ideally be below 0.1641 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000269776 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.356325 0.356325 0.712651 1.4253 2.8506 5.7012 11.4024 22.8048 45.6096 91.2193 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0008 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.227 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 841.927 quit ! Quitting program ! Log file /scr/pima/rv123_uvs/J2359+3850_X_dfm.log closed on Sun Dec 23 00:46:11 2018