! Started logfile: /scr/pima/rv123_uvs/J2212+2355_X_dfm.log on Sun Dec 23 00:45:24 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/J2212+2355_X_uva.fits ! Reading UV FITS file: /scr/pima/rv123_uvs/J2212+2355_X_uva.fits ! AN table 1: 13 integrations on 15 of 15 possible baselines. ! AN table 2: 11 integrations on 15 of 15 possible baselines. ! AN table 3: 47 integrations on 36 of 36 possible baselines. ! AN table 4: 4 integrations on 6 of 6 possible baselines. ! AN table 5: 3 integrations on 15 of 15 possible baselines. ! AN table 6: 15 integrations on 21 of 21 possible baselines. ! AN table 7: 3 integrations on 28 of 28 possible baselines. ! AN table 8: 11 integrations on 45 of 45 possible baselines. ! AN table 9: 2 integrations on 3 of 3 possible baselines. ! AN table 10: 13 integrations on 28 of 28 possible baselines. ! AN table 11: 30 integrations on 21 of 21 possible baselines. ! Apparent sampling: 0.507597 visibilities/baseline/integration-bin. ! Found source: J2212+2355 ! ! 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 8152 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 J2212+2355_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 24 telescope corrections were flagged in sub-array 1. ! A total of 8 telescope corrections were flagged in sub-array 2. ! A total of 171 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 43 telescope corrections were flagged in sub-array 6. ! A total of 8 telescope corrections were flagged in sub-array 7. ! A total of 56 telescope corrections were flagged in sub-array 8. ! A total of 52 telescope corrections were flagged in sub-array 10. ! A total of 151 telescope corrections were flagged in sub-array 11. ! ! Correcting IF 2. ! A total of 24 telescope corrections were flagged in sub-array 1. ! A total of 8 telescope corrections were flagged in sub-array 2. ! A total of 171 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 43 telescope corrections were flagged in sub-array 6. ! A total of 8 telescope corrections were flagged in sub-array 7. ! A total of 56 telescope corrections were flagged in sub-array 8. ! A total of 52 telescope corrections were flagged in sub-array 10. ! A total of 151 telescope corrections were flagged in sub-array 11. ! ! Correcting IF 3. ! A total of 33 telescope corrections were flagged in sub-array 1. ! A total of 19 telescope corrections were flagged in sub-array 2. ! A total of 222 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 53 telescope corrections were flagged in sub-array 6. ! A total of 8 telescope corrections were flagged in sub-array 7. ! A total of 56 telescope corrections were flagged in sub-array 8. ! A total of 6 telescope corrections were flagged in sub-array 9. ! A total of 64 telescope corrections were flagged in sub-array 10. ! A total of 151 telescope corrections were flagged in sub-array 11. ! ! Correcting IF 4. ! A total of 33 telescope corrections were flagged in sub-array 1. ! A total of 19 telescope corrections were flagged in sub-array 2. ! A total of 222 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 53 telescope corrections were flagged in sub-array 6. ! A total of 8 telescope corrections were flagged in sub-array 7. ! A total of 56 telescope corrections were flagged in sub-array 8. ! A total of 6 telescope corrections were flagged in sub-array 9. ! A total of 64 telescope corrections were flagged in sub-array 10. ! A total of 151 telescope corrections were flagged in sub-array 11. ! ! Fit before self-cal, rms=1.155587Jy sigma=15.815690 ! Fit after self-cal, rms=0.527494Jy sigma=6.601163 ! 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 5.74% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.6412 mas, bmaj=0.8514 mas, bpa=-17.79 degrees ! Estimated noise=1.03041 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 = 0.422012 Jy ! Component: 100 - total flux cleaned = 0.576189 Jy ! Total flux subtracted in 100 components = 0.576189 Jy ! Clean residual min=-0.016790 max=0.069096 Jy/beam ! Clean residual mean=-0.000012 rms=0.004187 Jy/beam ! Combined flux in latest and established models = 0.576189 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 9 components and 0.576189 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.203365Jy sigma=2.404697 ! Fit after self-cal, rms=0.203089Jy sigma=2.402391 ! Inverting map ! Your choice of large map pixels excluded 5.74% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0736952 Jy ! Component: 100 - total flux cleaned = 0.108834 Jy ! Total flux subtracted in 100 components = 0.108834 Jy ! Clean residual min=-0.017536 max=0.042040 Jy/beam ! Clean residual mean=-0.000069 rms=0.003316 Jy/beam ! Combined flux in latest and established models = 0.685023 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 9 components and 0.685023 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.186765Jy sigma=2.111276 ! Fit after self-cal, rms=0.186746Jy sigma=2.110847 ! Inverting map ! Your choice of large map pixels excluded 5.74% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Added new window around map position (1, 1.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0355609 Jy ! Component: 100 - total flux cleaned = 0.0489623 Jy ! Total flux subtracted in 100 components = 0.0489623 Jy ! Clean residual min=-0.021531 max=0.026072 Jy/beam ! Clean residual mean=-0.000091 rms=0.003044 Jy/beam ! Combined flux in latest and established models = 0.733985 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 18 components and 0.733985 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.186283Jy sigma=2.075698 ! Fit after self-cal, rms=0.184924Jy sigma=2.059564 ! Inverting map ! Your choice of large map pixels excluded 5.74% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Added new window around map position (0.4, 2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0159517 Jy ! Component: 100 - total flux cleaned = 0.0201942 Jy ! Total flux subtracted in 100 components = 0.0201942 Jy ! Clean residual min=-0.021243 max=0.017936 Jy/beam ! Clean residual mean=-0.000100 rms=0.002891 Jy/beam ! Combined flux in latest and established models = 0.754179 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 24 components and 0.754179 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.185124Jy sigma=2.053363 ! Fit after self-cal, rms=0.184663Jy sigma=2.048921 ! Inverting map ! Your choice of large map pixels excluded 5.74% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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 5.74% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.7828 mas, bmaj=0.9459 mas, bpa=-11.33 degrees ! Estimated noise=0.762006 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 = -0.0315949 Jy ! Component: 100 - total flux cleaned = -0.0454958 Jy ! Component: 150 - total flux cleaned = -0.049087 Jy ! Component: 200 - total flux cleaned = -0.0496032 Jy ! Total flux subtracted in 200 components = -0.0496032 Jy ! Clean residual min=-0.025933 max=0.014342 Jy/beam ! Clean residual mean=-0.006717 rms=0.004634 Jy/beam ! Combined flux in latest and established models = 0.704576 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 35 components and 0.704576 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.177371Jy sigma=1.983553 ! Fit after self-cal, rms=0.177264Jy sigma=1.982476 ! Inverting map ! Your choice of large map pixels excluded 5.74% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7828 x 0.9459 at -11.33 degrees (North through East) ! Clean map min=-0.024996 max=0.534 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.79 NY 0.76 ON 0.96 WN 1.46 ! WZ 1.05 YG 0.91 ! ! Telescope amplitude corrections in sub-array 2: ! HH 0.79 MC 0.85 NY 0.87 ON 0.96 ! WZ 0.98 YG 0.96 ! ! A total of 9 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HH 0.75 HN 0.97 MC 0.86 NL 1.45 ! NY 0.81 ON 0.96 SC 0.88 WN 1.56 ! WZ 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! FD 0.97 HN 0.98 LA 0.94 WN 1.64 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.05 FD 0.86 KP 1.02 NL 0.98 ! ON 1.01 OV 0.94 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.03 MK 1.01 NY 0.78 ON 0.88 ! OV 0.90 WN 1.56 WZ 1.11 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.01 FD 0.82 KP 1.02 LA 0.97 ! MK 0.96 OV 0.93 PT 0.81 WN 2.76 ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.97 FD 0.80 HN 1.12 KP 1.06 ! LA 0.95 MK 1.03 NL 1.00 OV 0.93 ! PT 0.82 SC 0.88 ! ! A total of 6 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! BR 0.00* HN 0.00* NY 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! BR 0.97 FD 0.80 KP 1.02 LA 0.93 ! MK 0.99 NL 1.01 NY 0.89 OV 0.92 ! ! Telescope amplitude corrections in sub-array 11: ! BR 0.96 KP 1.04 LA 1.05 MK 1.10 ! OV 0.92 PT 0.85 YG 1.07 ! ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.83 NY 0.98 ON 0.92 WN 1.54 ! WZ 0.95 YG 0.85 ! ! Telescope amplitude corrections in sub-array 2: ! HH 0.76 MC 0.90 NY 0.96 ON 0.90 ! WZ 0.98 YG 0.80 ! ! A total of 9 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HH 0.75 HN 0.94 MC 0.93 NL 1.49 ! NY 0.95 ON 0.91 SC 0.89 WN 1.56 ! WZ 0.97 ! ! Telescope amplitude corrections in sub-array 4: ! FD 0.91 HN 1.04 LA 0.96 WN 1.57 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 FD 0.86 KP 1.10 NL 0.96 ! ON 0.81 OV 0.97 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.06 MK 1.01 NY 0.86 ON 0.90 ! OV 0.89 WN 1.65 WZ 1.08 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.03 FD 0.80 KP 1.04 LA 0.98 ! MK 0.90 OV 0.92 PT 0.84 WN 2.59 ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.96 FD 0.82 HN 1.11 KP 1.05 ! LA 0.95 MK 1.00 NL 1.01 OV 0.92 ! PT 0.84 SC 0.91 ! ! A total of 6 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! BR 0.00* HN 0.00* NY 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! BR 0.96 FD 0.81 KP 1.03 LA 0.95 ! MK 1.00 NL 1.01 NY 1.03 OV 0.93 ! ! Telescope amplitude corrections in sub-array 11: ! BR 0.94 KP 1.05 LA 1.09 MK 1.08 ! OV 0.94 PT 0.86 YG 0.87 ! ! ! Correcting IF 3. ! A total of 9 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.82 NY 1.00* ON 1.24 WN 1.47 ! WZ 1.09 YG 0.91 ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.86 MC 1.36 NY 1.00* ON 1.23 ! WZ 1.02 YG 0.94 ! ! A total of 21 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HH 0.85 HN 0.93 MC 1.34 NL 1.49 ! NY 1.00* ON 1.23 SC 0.91 WN 1.47 ! WZ 1.04 ! ! Telescope amplitude corrections in sub-array 4: ! FD 0.95 HN 0.93 LA 1.06 WN 1.43 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.07 FD 0.89 KP 1.08 NL 0.94 ! ON 1.25 OV 0.92 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.07 MK 1.07 NY 1.00* ON 1.23 ! OV 0.88 WN 1.59 WZ 1.22 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00 FD 0.81 KP 1.07 LA 0.95 ! MK 0.91 OV 0.93 PT 0.83 WN 2.32 ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.97 FD 0.83 HN 1.08 KP 1.07 ! LA 0.97 MK 1.01 NL 1.00 OV 0.93 ! PT 0.82 SC 0.93 ! ! Telescope amplitude corrections in sub-array 9: ! BR 0.00* HN 0.00* NY 0.00* ! ! Telescope amplitude corrections in sub-array 10: ! BR 0.96 FD 0.81 KP 1.03 LA 0.94 ! MK 1.02 NL 1.03 NY 1.00* OV 0.93 ! ! Telescope amplitude corrections in sub-array 11: ! BR 0.96 KP 1.04 LA 1.02 MK 1.09 ! OV 0.96 PT 0.87 YG 1.18 ! ! ! Correcting IF 4. ! A total of 9 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.94 NY 1.00* ON 1.23 WN 1.51 ! WZ 1.04 YG 1.12 ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.93 MC 1.28 NY 1.00* ON 1.25 ! WZ 1.07 YG 1.07 ! ! A total of 21 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HH 0.95 HN 0.98 MC 1.33 NL 1.43 ! NY 1.00* ON 1.20 SC 0.91 WN 1.37 ! WZ 1.05 ! ! Telescope amplitude corrections in sub-array 4: ! FD 0.98 HN 1.03 LA 0.96 WN 1.31 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 FD 0.86 KP 1.06 NL 0.95 ! ON 1.30 OV 0.96 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.04 MK 1.00 NY 1.00* ON 1.21 ! OV 0.89 WN 1.55 WZ 1.29 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.03 FD 0.79 KP 1.07 LA 0.96 ! MK 0.96 OV 0.92 PT 0.84 WN 2.59 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.00 FD 0.81 HN 1.12 KP 1.07 ! LA 0.97 MK 0.99 NL 1.03 OV 0.92 ! PT 0.83 SC 0.90 ! ! Telescope amplitude corrections in sub-array 9: ! BR 0.00* HN 0.00* NY 0.00* ! ! Telescope amplitude corrections in sub-array 10: ! BR 0.95 FD 0.82 KP 1.02 LA 0.95 ! MK 0.98 NL 1.04 NY 1.00* OV 0.95 ! ! Telescope amplitude corrections in sub-array 11: ! BR 0.97 KP 1.05 LA 1.05 MK 1.14 ! OV 0.94 PT 0.89 YG 1.17 ! ! ! Fit before self-cal, rms=0.177264Jy sigma=1.982476 ! Fit after self-cal, rms=0.119388Jy sigma=1.006378 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.8017 mas, bmaj=0.9241 mas, bpa=-13.95 degrees ! Estimated noise=0.770038 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 = 0.00556942 Jy ! Component: 100 - total flux cleaned = 0.00600078 Jy ! Component: 150 - total flux cleaned = 0.00611266 Jy ! Component: 200 - total flux cleaned = 0.00611261 Jy ! Total flux subtracted in 200 components = 0.00611261 Jy ! Clean residual min=-0.005618 max=0.005166 Jy/beam ! Clean residual mean=0.000259 rms=0.001022 Jy/beam ! Combined flux in latest and established models = 0.710689 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 41 components and 0.710689 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.118817Jy sigma=0.996595 ! Fit after self-cal, rms=0.118888Jy sigma=0.992999 ! Inverting map ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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=0.118888Jy sigma=0.992999 ! Fit after self-cal, rms=0.116662Jy sigma=0.960547 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.8017 mas, bmaj=0.9197 mas, bpa=-13.3 degrees ! Estimated noise=0.770052 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00502119 Jy ! Component: 100 - total flux cleaned = 0.00566953 Jy ! Component: 150 - total flux cleaned = 0.00567366 Jy ! Component: 200 - total flux cleaned = 0.00567257 Jy ! Total flux subtracted in 200 components = 0.00567257 Jy ! Clean residual min=-0.005304 max=0.004709 Jy/beam ! Clean residual mean=0.000315 rms=0.000895 Jy/beam ! Combined flux in latest and established models = 0.716361 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 44 components and 0.716361 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.116324Jy sigma=0.955378 ! Fit after self-cal, rms=0.116254Jy sigma=0.954254 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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 = 0.00104498 Jy ! Component: 100 - total flux cleaned = 0.00112539 Jy ! Component: 150 - total flux cleaned = 0.00105701 Jy ! Component: 200 - total flux cleaned = 0.000990048 Jy ! Total flux subtracted in 200 components = 0.000990048 Jy ! Clean residual min=-0.005693 max=0.004618 Jy/beam ! Clean residual mean=0.000298 rms=0.000886 Jy/beam ! Combined flux in latest and established models = 0.717351 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 45 components and 0.717351 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.116131Jy sigma=0.951858 ! Fit after self-cal, rms=0.116096Jy sigma=0.951549 ! Inverting map ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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=0.116096Jy sigma=0.951549 ! Fit after self-cal, rms=0.113678Jy sigma=0.930091 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.8017 mas, bmaj=0.9161 mas, bpa=-13.42 degrees ! Estimated noise=0.769881 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00355969 Jy ! Component: 100 - total flux cleaned = 0.00373696 Jy ! Component: 150 - total flux cleaned = 0.00373862 Jy ! Component: 200 - total flux cleaned = 0.00367637 Jy ! Total flux subtracted in 200 components = 0.00367637 Jy ! Clean residual min=-0.004997 max=0.003810 Jy/beam ! Clean residual mean=0.000236 rms=0.000760 Jy/beam ! Combined flux in latest and established models = 0.721028 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 46 components and 0.721028 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.113450Jy sigma=0.926647 ! Fit after self-cal, rms=0.113422Jy sigma=0.926098 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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 = 0.000680615 Jy ! Component: 100 - total flux cleaned = 0.000748889 Jy ! Component: 150 - total flux cleaned = 0.00068927 Jy ! Component: 200 - total flux cleaned = 0.000635826 Jy ! Total flux subtracted in 200 components = 0.000635826 Jy ! Clean residual min=-0.005202 max=0.003666 Jy/beam ! Clean residual mean=0.000226 rms=0.000754 Jy/beam ! Combined flux in latest and established models = 0.721664 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 46 components and 0.721664 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.113284Jy sigma=0.924185 ! Fit after self-cal, rms=0.113262Jy sigma=0.923991 ! Inverting map ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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=0.113262Jy sigma=0.923991 ! Fit after self-cal, rms=0.113366Jy sigma=0.922828 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=2.707 mas, bmaj=3.054 mas, bpa=-56.65 degrees ! Estimated noise=1.001 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00194987 Jy ! Component: 100 - total flux cleaned = 0.00194678 Jy ! Component: 150 - total flux cleaned = 0.00198793 Jy ! Component: 200 - total flux cleaned = 0.00201584 Jy ! Total flux subtracted in 200 components = 0.00201584 Jy ! Clean residual min=-0.002560 max=0.003977 Jy/beam ! Clean residual mean=0.000580 rms=0.000830 Jy/beam ! Combined flux in latest and established models = 0.723679 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 48 components and 0.723679 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.113349Jy sigma=0.922147 ! Fit after self-cal, rms=0.113308Jy sigma=0.921553 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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 (-25.8, -50). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00378521 Jy ! Component: 100 - total flux cleaned = 0.00524667 Jy ! Component: 150 - total flux cleaned = 0.00564718 Jy ! Component: 200 - total flux cleaned = 0.00593129 Jy ! Total flux subtracted in 200 components = 0.00593129 Jy ! Clean residual min=-0.002519 max=0.003304 Jy/beam ! Clean residual mean=0.000321 rms=0.000775 Jy/beam ! Combined flux in latest and established models = 0.729611 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 71 components and 0.729611 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.113167Jy sigma=0.920562 ! Fit after self-cal, rms=0.113161Jy sigma=0.920296 ! Inverting map ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Added new window around map position (18.2, -41.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00281425 Jy ! Component: 100 - total flux cleaned = 0.00336445 Jy ! Component: 150 - total flux cleaned = 0.00365927 Jy ! Component: 200 - total flux cleaned = 0.00387275 Jy ! Total flux subtracted in 200 components = 0.00387275 Jy ! Clean residual min=-0.002690 max=0.002936 Jy/beam ! Clean residual mean=0.000196 rms=0.000749 Jy/beam ! Combined flux in latest and established models = 0.733483 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 91 components and 0.733483 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.113056Jy sigma=0.919388 ! Fit after self-cal, rms=0.113050Jy sigma=0.919244 ! Inverting map ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.8016 mas, bmaj=0.9137 mas, bpa=-13.71 degrees ! Estimated noise=0.770259 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8016 x 0.9137 at -13.71 degrees (North through East) ! Clean map min=-0.0025606 max=0.53325 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=0.113050Jy sigma=0.919244 ! Fit after self-cal, rms=0.121629Jy sigma=0.817326 ! Inverting map and beam ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.8036 mas, bmaj=0.9134 mas, bpa=-13.62 degrees ! Estimated noise=0.770399 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00241397 Jy ! Component: 100 - total flux cleaned = 0.00407306 Jy ! Component: 150 - total flux cleaned = 0.00519211 Jy ! Component: 200 - total flux cleaned = 0.00596905 Jy ! Total flux subtracted in 200 components = 0.00596905 Jy ! Clean residual min=-0.004212 max=0.003149 Jy/beam ! Clean residual mean=0.000125 rms=0.000666 Jy/beam ! Combined flux in latest and established models = 0.739453 Jy ! Performing phase self-cal ! Adding 35 model components to the UV plane model. ! The established model now contains 123 components and 0.739452 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.121318Jy sigma=0.813904 ! Fit after self-cal, rms=0.121317Jy sigma=0.813708 ! Inverting map ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000990373 Jy ! Component: 100 - total flux cleaned = 0.00123426 Jy ! Component: 150 - total flux cleaned = 0.00138928 Jy ! Component: 200 - total flux cleaned = 0.00154129 Jy ! Total flux subtracted in 200 components = 0.00154129 Jy ! Clean residual min=-0.004447 max=0.003033 Jy/beam ! Clean residual mean=0.000105 rms=0.000659 Jy/beam ! Combined flux in latest and established models = 0.740994 Jy ! Performing phase self-cal ! Adding 55 model components to the UV plane model. ! The established model now contains 143 components and 0.740994 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.121168Jy sigma=0.811864 ! Fit after self-cal, rms=0.121166Jy sigma=0.811820 ! Inverting map ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.121166Jy sigma=0.811820 ! Fit after self-cal, rms=0.118564Jy sigma=0.811192 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 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.6693 mas, bmaj=0.8275 mas, bpa=-17.68 degrees ! Estimated noise=1.00808 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.405406 Jy ! Component: 100 - total flux cleaned = 0.544944 Jy ! Component: 150 - total flux cleaned = 0.617819 Jy ! Component: 200 - total flux cleaned = 0.662076 Jy ! Total flux subtracted in 200 components = 0.662076 Jy ! Clean residual min=-0.009927 max=0.023143 Jy/beam ! Clean residual mean=0.000027 rms=0.001682 Jy/beam ! Combined flux in latest and established models = 0.662076 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 0.662076 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.8028 mas, bmaj=0.9121 mas, bpa=-13.78 degrees ! Estimated noise=0.771609 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 = 0.034719 Jy ! Component: 100 - total flux cleaned = 0.0533361 Jy ! Component: 150 - total flux cleaned = 0.0634221 Jy ! Component: 200 - total flux cleaned = 0.0643213 Jy ! Total flux subtracted in 200 components = 0.0643213 Jy ! Clean residual min=-0.007176 max=0.006325 Jy/beam ! Clean residual mean=0.000427 rms=0.000873 Jy/beam ! Combined flux in latest and established models = 0.726397 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 31 components and 0.726397 Jy ! Inverting map ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 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 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=2.699 mas, bmaj=3.05 mas, bpa=-56.67 degrees ! Estimated noise=1.00505 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00766979 Jy ! Component: 100 - total flux cleaned = 0.010965 Jy ! Component: 150 - total flux cleaned = 0.0129424 Jy ! Component: 200 - total flux cleaned = 0.0143887 Jy ! Total flux subtracted in 200 components = 0.0143887 Jy ! Clean residual min=-0.002694 max=0.003477 Jy/beam ! Clean residual mean=0.000389 rms=0.000784 Jy/beam ! Combined flux in latest and established models = 0.740786 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) ! Added new window around map position (-41, -14.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00249002 Jy ! Component: 100 - total flux cleaned = 0.00337136 Jy ! Component: 150 - total flux cleaned = 0.00441354 Jy ! Component: 200 - total flux cleaned = 0.00534481 Jy ! Total flux subtracted in 200 components = 0.00534481 Jy ! Clean residual min=-0.002415 max=0.002745 Jy/beam ! Clean residual mean=0.000175 rms=0.000711 Jy/beam ! Combined flux in latest and established models = 0.746131 Jy ! Adding 67 model components to the UV plane model. ! The established model now contains 92 components and 0.74613 Jy ! Inverting map ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! Estimated beam: bmin=0.8028 mas, bmaj=0.9121 mas, bpa=-13.78 degrees ! Estimated noise=0.771609 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000670592 Jy ! Component: 100 - total flux cleaned = 0.000659118 Jy ! Component: 150 - total flux cleaned = 0.000667846 Jy ! Component: 200 - total flux cleaned = 0.000665164 Jy ! Total flux subtracted in 200 components = 0.000665164 Jy ! Clean residual min=-0.005723 max=0.003600 Jy/beam ! Clean residual mean=0.000094 rms=0.000728 Jy/beam ! Combined flux in latest and established models = 0.746796 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 93 components and 0.746796 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.120928Jy sigma=0.840684 ! Fit after self-cal, rms=0.120806Jy sigma=0.838665 wmodel J2212+2355_X_map.mod ! Writing 93 model components to file: J2212+2355_X_map.mod wobs J2212+2355_X_uvs.fits ! Writing UV FITS file: J2212+2355_X_uvs.fits wwins J2212+2355_X_map.win ! wwins: Wrote 6 windows to J2212+2355_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 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00165715 Jy ! Component: 100 - total flux cleaned = -0.00212926 Jy ! Component: 150 - total flux cleaned = -0.00234261 Jy ! Component: 200 - total flux cleaned = -0.00267183 Jy ! Component: 250 - total flux cleaned = -0.00260937 Jy ! Component: 300 - total flux cleaned = -0.00231128 Jy ! Component: 350 - total flux cleaned = -0.00202109 Jy ! Component: 400 - total flux cleaned = -0.00168137 Jy ! Component: 450 - total flux cleaned = -0.00129506 Jy ! Component: 500 - total flux cleaned = -0.0010254 Jy ! Component: 550 - total flux cleaned = -0.000549947 Jy ! Component: 600 - total flux cleaned = -0.000238968 Jy ! Component: 650 - total flux cleaned = 1.68078e-05 Jy ! Component: 700 - total flux cleaned = 0.000319464 Jy ! Component: 750 - total flux cleaned = 0.000567755 Jy ! Component: 800 - total flux cleaned = 0.000715489 Jy ! Component: 850 - total flux cleaned = 0.00095835 Jy ! Component: 900 - total flux cleaned = 0.00110302 Jy ! Component: 950 - total flux cleaned = 0.00124581 Jy ! Component: 1000 - total flux cleaned = 0.00148173 Jy ! Component: 1050 - total flux cleaned = 0.00162186 Jy ! Component: 1100 - total flux cleaned = 0.00176094 Jy ! Component: 1150 - total flux cleaned = 0.00189874 Jy ! Component: 1200 - total flux cleaned = 0.00198996 Jy ! Component: 1250 - total flux cleaned = 0.00217108 Jy ! Component: 1300 - total flux cleaned = 0.00226059 Jy ! Component: 1350 - total flux cleaned = 0.0023495 Jy ! Component: 1400 - total flux cleaned = 0.00239353 Jy ! Component: 1450 - total flux cleaned = 0.00252503 Jy ! Component: 1500 - total flux cleaned = 0.00252506 Jy ! Component: 1550 - total flux cleaned = 0.00261134 Jy ! Component: 1600 - total flux cleaned = 0.00269704 Jy ! Component: 1650 - total flux cleaned = 0.00282435 Jy ! Component: 1700 - total flux cleaned = 0.00278174 Jy ! Component: 1750 - total flux cleaned = 0.00286591 Jy ! Component: 1800 - total flux cleaned = 0.00286597 Jy ! Component: 1850 - total flux cleaned = 0.00290756 Jy ! Component: 1900 - total flux cleaned = 0.00299017 Jy ! Component: 1950 - total flux cleaned = 0.00294915 Jy ! Component: 2000 - total flux cleaned = 0.00303066 Jy ! Component: 2050 - total flux cleaned = 0.00307131 Jy ! Component: 2100 - total flux cleaned = 0.00311153 Jy ! Component: 2150 - total flux cleaned = 0.00311149 Jy ! Component: 2200 - total flux cleaned = 0.00319105 Jy ! Component: 2250 - total flux cleaned = 0.00315151 Jy ! Component: 2300 - total flux cleaned = 0.00323056 Jy ! Component: 2350 - total flux cleaned = 0.00326973 Jy ! Component: 2400 - total flux cleaned = 0.00330866 Jy ! Component: 2450 - total flux cleaned = 0.00330867 Jy ! Component: 2500 - total flux cleaned = 0.00330872 Jy ! Component: 2550 - total flux cleaned = 0.00338578 Jy ! Component: 2600 - total flux cleaned = 0.00342395 Jy ! Component: 2650 - total flux cleaned = 0.00346215 Jy ! Component: 2700 - total flux cleaned = 0.00342435 Jy ! Component: 2750 - total flux cleaned = 0.00349985 Jy ! Component: 2800 - total flux cleaned = 0.00346216 Jy ! Component: 2850 - total flux cleaned = 0.00357446 Jy ! Component: 2900 - total flux cleaned = 0.00357452 Jy ! Component: 2950 - total flux cleaned = 0.00361157 Jy ! Component: 3000 - total flux cleaned = 0.00361161 Jy ! Component: 3050 - total flux cleaned = 0.00368514 Jy ! Component: 3100 - total flux cleaned = 0.00368501 Jy ! Component: 3150 - total flux cleaned = 0.00372154 Jy ! Component: 3200 - total flux cleaned = 0.00379411 Jy ! Component: 3250 - total flux cleaned = 0.00379405 Jy ! Component: 3300 - total flux cleaned = 0.00383001 Jy ! Component: 3350 - total flux cleaned = 0.00379415 Jy ! Component: 3400 - total flux cleaned = 0.00382995 Jy ! Component: 3450 - total flux cleaned = 0.00390112 Jy ! Component: 3500 - total flux cleaned = 0.00393655 Jy ! Component: 3550 - total flux cleaned = 0.00390118 Jy ! Component: 3600 - total flux cleaned = 0.00393634 Jy ! Component: 3650 - total flux cleaned = 0.00393629 Jy ! Component: 3700 - total flux cleaned = 0.00400625 Jy ! Component: 3750 - total flux cleaned = 0.00404101 Jy ! Component: 3800 - total flux cleaned = 0.00404095 Jy ! Component: 3850 - total flux cleaned = 0.00400644 Jy ! Component: 3900 - total flux cleaned = 0.00407537 Jy ! Component: 3950 - total flux cleaned = 0.00407539 Jy ! Component: 4000 - total flux cleaned = 0.00410952 Jy ! Component: 4050 - total flux cleaned = 0.0041437 Jy ! Total flux subtracted in 4096 components = 0.00417759 Jy ! Clean residual min=-0.002054 max=0.002012 Jy/beam ! Clean residual mean=0.000019 rms=0.000537 Jy/beam ! Combined flux in latest and established models = 0.750973 Jy keep ! Adding 294 model components to the UV plane model. ! The established model now contains 382 components and 0.750973 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv123_uvs/J2212+2355_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8028 x 0.9121 at -13.78 degrees (North through East) ! Clean map min=-0.0022066 max=0.52975 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv123_uvs/J2212+2355_X_map.fits wmodel /scr/pima/rv123_uvs/J2212+2355_X_map.mod ! Writing 382 model components to file: /scr/pima/rv123_uvs/J2212+2355_X_map.mod wobs /scr/pima/rv123_uvs/J2212+2355_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv123_uvs/J2212+2355_X_uvs.fits wwins /scr/pima/rv123_uvs/J2212+2355_X_map.win ! wwins: Wrote 7 windows to /scr/pima/rv123_uvs/J2212+2355_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.529751 invert ! Inverting map ! Your choice of large map pixels excluded 5.58% of the data. ! The x-axis pixel size should ideally be below 0.1695 milli-arcsec ! The y-axis pixel size should ideally be below 0.1694 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000536679 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.303924 0.303924 0.607847 1.21569 2.43139 4.86278 9.72555 19.4511 38.9022 77.8044 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0016 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.529 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 987.09 quit ! Quitting program ! Log file /scr/pima/rv123_uvs/J2212+2355_X_dfm.log closed on Sun Dec 23 00:45:28 2018