! Started logfile: /scr/pima/rv123_uvs/J2310+1055_X_dfm.log on Sun Dec 23 00:45:52 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/J2310+1055_X_uva.fits ! Reading UV FITS file: /scr/pima/rv123_uvs/J2310+1055_X_uva.fits ! AN table 1: 116 integrations on 15 of 15 possible baselines. ! AN table 2: 87 integrations on 15 of 15 possible baselines. ! AN table 3: 15 integrations on 10 of 10 possible baselines. ! AN table 4: 20 integrations on 45 of 45 possible baselines. ! AN table 5: 7 integrations on 3 of 3 possible baselines. ! AN table 6: 27 integrations on 36 of 36 possible baselines. ! Apparent sampling: 0.691234 visibilities/baseline/integration-bin. ! Found source: J2310+1055 ! ! 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 14068 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 J2310+1055_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 79 telescope corrections were flagged in sub-array 1. ! A total of 118 telescope corrections were flagged in sub-array 2. ! A total of 24 telescope corrections were flagged in sub-array 3. ! A total of 20 telescope corrections were flagged in sub-array 4. ! A total of 3 telescope corrections were flagged in sub-array 5. ! A total of 101 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 79 telescope corrections were flagged in sub-array 1. ! A total of 118 telescope corrections were flagged in sub-array 2. ! A total of 24 telescope corrections were flagged in sub-array 3. ! A total of 20 telescope corrections were flagged in sub-array 4. ! A total of 3 telescope corrections were flagged in sub-array 5. ! A total of 101 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 197 telescope corrections were flagged in sub-array 1. ! A total of 146 telescope corrections were flagged in sub-array 2. ! A total of 24 telescope corrections were flagged in sub-array 3. ! A total of 20 telescope corrections were flagged in sub-array 4. ! A total of 21 telescope corrections were flagged in sub-array 5. ! A total of 101 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 197 telescope corrections were flagged in sub-array 1. ! A total of 146 telescope corrections were flagged in sub-array 2. ! A total of 24 telescope corrections were flagged in sub-array 3. ! A total of 20 telescope corrections were flagged in sub-array 4. ! A total of 21 telescope corrections were flagged in sub-array 5. ! A total of 101 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.034402Jy sigma=14.844719 ! Fit after self-cal, rms=0.795812Jy sigma=10.964037 ! 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 5.63% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! Estimated beam: bmin=0.7743 mas, bmaj=0.8924 mas, bpa=29.32 degrees ! Estimated noise=0.710959 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 = 0.183287 Jy ! Component: 100 - total flux cleaned = 0.238583 Jy ! Total flux subtracted in 100 components = 0.238583 Jy ! Clean residual min=-0.007238 max=0.022700 Jy/beam ! Clean residual mean=-0.000005 rms=0.001565 Jy/beam ! Combined flux in latest and established models = 0.238583 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.238583 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.131164Jy sigma=1.193096 ! Fit after self-cal, rms=0.130616Jy sigma=1.192020 ! Inverting map ! Your choice of large map pixels excluded 5.63% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0231359 Jy ! Component: 100 - total flux cleaned = 0.0336288 Jy ! Total flux subtracted in 100 components = 0.0336288 Jy ! Clean residual min=-0.006223 max=0.007875 Jy/beam ! Clean residual mean=-0.000025 rms=0.001264 Jy/beam ! Combined flux in latest and established models = 0.272212 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 11 components and 0.272212 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.129476Jy sigma=1.180523 ! Fit after self-cal, rms=0.129376Jy sigma=1.180257 ! Inverting map ! Your choice of large map pixels excluded 5.63% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! Added new window around map position (-2.2, -0.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00561768 Jy ! Component: 100 - total flux cleaned = 0.00666639 Jy ! Total flux subtracted in 100 components = 0.00666639 Jy ! Clean residual min=-0.005761 max=0.007372 Jy/beam ! Clean residual mean=-0.000029 rms=0.001231 Jy/beam ! Combined flux in latest and established models = 0.278879 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 17 components and 0.278879 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.129535Jy sigma=1.187134 ! Fit after self-cal, rms=0.129444Jy sigma=1.186448 ! Inverting map ! Your choice of large map pixels excluded 5.63% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 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 5.63% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! Estimated beam: bmin=0.7196 mas, bmaj=1.029 mas, bpa=66.22 degrees ! Estimated noise=0.506339 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 = -0.0174235 Jy ! Component: 100 - total flux cleaned = -0.0255614 Jy ! Component: 150 - total flux cleaned = -0.0298428 Jy ! Component: 200 - total flux cleaned = -0.0305294 Jy ! Total flux subtracted in 200 components = -0.0305294 Jy ! Clean residual min=-0.014104 max=0.008680 Jy/beam ! Clean residual mean=-0.002374 rms=0.003184 Jy/beam ! Combined flux in latest and established models = 0.248349 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 29 components and 0.248349 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.126514Jy sigma=1.144731 ! Fit after self-cal, rms=0.125420Jy sigma=1.143768 ! Inverting map ! Your choice of large map pixels excluded 5.63% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7196 x 1.029 at 66.22 degrees (North through East) ! Clean map min=-0.013151 max=0.22769 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.73 MC 0.93 NY 0.82 WN 1.49 ! WZ 0.98 YG 1.24 ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.86 MC 0.82 NY 0.75 ON 0.92 ! WN 1.60 WZ 0.98 ! ! A total of 21 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HN 1.06 NL 1.05 SC 0.83 WN 1.77 ! WZ 1.07 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.95 FD 0.81 HN 1.06 KP 1.07 ! LA 0.96 MK 1.01 NL 1.03 OV 0.93 ! PT 0.83 SC 1.04 ! ! A total of 18 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* MK 0.00* NY 0.00* ! ! A total of 12 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.98 FD 0.86 KP 1.02 LA 0.94 ! MK 1.04 NL 1.02 OV 0.94 PT 0.82 ! YG 0.70 ! ! ! Correcting IF 2. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.75 MC 0.99 NY 0.92 WN 1.45 ! WZ 0.96 YG 1.02 ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.84 MC 0.90 NY 0.88 ON 0.91 ! WN 1.49 WZ 0.94 ! ! A total of 21 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HN 0.99 NL 1.09 SC 0.82 WN 1.81 ! WZ 1.00 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 FD 0.82 HN 1.03 KP 1.06 ! LA 0.96 MK 1.05 NL 1.04 OV 0.93 ! PT 0.84 SC 1.07 ! ! A total of 18 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* MK 0.00* NY 0.00* ! ! A total of 12 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.97 FD 0.88 KP 1.04 LA 0.96 ! MK 1.02 NL 1.06 OV 0.93 PT 0.82 ! YG 0.79 ! ! ! Correcting IF 3. ! A total of 111 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.89 MC 1.43 NY 1.00* WN 1.42 ! WZ 1.02 YG 1.12 ! ! A total of 39 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.97 MC 1.28 NY 1.00* ON 1.18 ! WN 1.49 WZ 1.03 ! ! A total of 21 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HN 1.21 NL 1.01 SC 0.79 WN 1.56 ! WZ 1.07 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 FD 0.81 HN 1.07 KP 1.07 ! LA 0.96 MK 1.02 NL 1.06 OV 0.93 ! PT 0.82 SC 1.06 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* MK 0.00* NY 0.00* ! ! A total of 12 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.97 FD 0.87 KP 1.05 LA 0.97 ! MK 1.06 NL 1.00 OV 0.94 PT 0.83 ! YG 0.83 ! ! ! Correcting IF 4. ! A total of 111 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.98 MC 1.42 NY 1.00* WN 1.37 ! WZ 1.01 YG 1.06 ! ! A total of 39 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 1.09 MC 1.19 NY 1.00* ON 1.17 ! WN 1.41 WZ 1.12 ! ! A total of 21 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HN 1.09 NL 1.09 SC 0.83 WN 1.46 ! WZ 0.98 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 FD 0.82 HN 1.07 KP 1.04 ! LA 0.97 MK 1.03 NL 1.07 OV 0.95 ! PT 0.83 SC 1.10 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* MK 0.00* NY 0.00* ! ! A total of 12 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.97 FD 0.86 KP 1.06 LA 0.99 ! MK 1.06 NL 1.04 OV 0.94 PT 0.84 ! YG 0.73 ! ! ! Fit before self-cal, rms=0.125420Jy sigma=1.143768 ! Fit after self-cal, rms=0.117886Jy sigma=0.884997 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! Estimated beam: bmin=0.7573 mas, bmaj=1.056 mas, bpa=70.18 degrees ! Estimated noise=0.51239 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (-2, 0.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0036843 Jy ! Component: 100 - total flux cleaned = 0.00425017 Jy ! Component: 150 - total flux cleaned = 0.00454074 Jy ! Component: 200 - total flux cleaned = 0.00460087 Jy ! Total flux subtracted in 200 components = 0.00460087 Jy ! Clean residual min=-0.002458 max=0.002639 Jy/beam ! Clean residual mean=0.000157 rms=0.000649 Jy/beam ! Combined flux in latest and established models = 0.25295 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 40 components and 0.25295 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.117707Jy sigma=0.880628 ! Fit after self-cal, rms=0.117534Jy sigma=0.878428 ! Inverting map ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 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=0.117534Jy sigma=0.878428 ! Fit after self-cal, rms=0.116884Jy sigma=0.865967 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! Estimated beam: bmin=0.7562 mas, bmaj=1.054 mas, bpa=70.71 degrees ! Estimated noise=0.513322 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00207705 Jy ! Component: 100 - total flux cleaned = 0.00234549 Jy ! Component: 150 - total flux cleaned = 0.00245715 Jy ! Component: 200 - total flux cleaned = 0.00246033 Jy ! Total flux subtracted in 200 components = 0.00246033 Jy ! Clean residual min=-0.001934 max=0.002323 Jy/beam ! Clean residual mean=0.000211 rms=0.000486 Jy/beam ! Combined flux in latest and established models = 0.25541 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 52 components and 0.25541 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.116773Jy sigma=0.864258 ! Fit after self-cal, rms=0.116634Jy sigma=0.863894 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 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 (-24.8, -50.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00193083 Jy ! Component: 100 - total flux cleaned = 0.00237867 Jy ! Component: 150 - total flux cleaned = 0.00251774 Jy ! Component: 200 - total flux cleaned = 0.00251666 Jy ! Total flux subtracted in 200 components = 0.00251666 Jy ! Clean residual min=-0.001953 max=0.002316 Jy/beam ! Clean residual mean=0.000146 rms=0.000481 Jy/beam ! Combined flux in latest and established models = 0.257927 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 59 components and 0.257927 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.116555Jy sigma=0.862884 ! Fit after self-cal, rms=0.116542Jy sigma=0.862741 ! Inverting map ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! Added new window around map position (-17.2, -27.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0010114 Jy ! Component: 100 - total flux cleaned = 0.00100174 Jy ! Component: 150 - total flux cleaned = 0.00109665 Jy ! Component: 200 - total flux cleaned = 0.00114012 Jy ! Total flux subtracted in 200 components = 0.00114012 Jy ! Clean residual min=-0.002080 max=0.002169 Jy/beam ! Clean residual mean=0.000126 rms=0.000471 Jy/beam ! Combined flux in latest and established models = 0.259067 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 68 components and 0.259067 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.116477Jy sigma=0.861796 ! Fit after self-cal, rms=0.116434Jy sigma=0.861680 ! Inverting map ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! Added new window around map position (18.2, 13.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00108882 Jy ! Component: 100 - total flux cleaned = 0.00120137 Jy ! Component: 150 - total flux cleaned = 0.00110408 Jy ! Component: 200 - total flux cleaned = 0.00110501 Jy ! Total flux subtracted in 200 components = 0.00110501 Jy ! Clean residual min=-0.002083 max=0.002026 Jy/beam ! Clean residual mean=0.000103 rms=0.000464 Jy/beam ! Combined flux in latest and established models = 0.260172 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 80 components and 0.260172 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.116358Jy sigma=0.860800 ! Fit after self-cal, rms=0.116341Jy sigma=0.860732 ! Inverting map ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 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=0.116341Jy sigma=0.860732 ! Fit after self-cal, rms=0.115761Jy sigma=0.853922 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! Estimated beam: bmin=0.7564 mas, bmaj=1.048 mas, bpa=70.79 degrees ! Estimated noise=0.513002 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00163872 Jy ! Component: 100 - total flux cleaned = 0.00174331 Jy ! Component: 150 - total flux cleaned = 0.00178782 Jy ! Component: 200 - total flux cleaned = 0.00187223 Jy ! Total flux subtracted in 200 components = 0.00187223 Jy ! Clean residual min=-0.001726 max=0.001985 Jy/beam ! Clean residual mean=0.000164 rms=0.000407 Jy/beam ! Combined flux in latest and established models = 0.262044 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 90 components and 0.262044 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.115685Jy sigma=0.853166 ! Fit after self-cal, rms=0.115593Jy sigma=0.853006 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 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 (25.2, 38.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0015125 Jy ! Component: 100 - total flux cleaned = 0.00188085 Jy ! Component: 150 - total flux cleaned = 0.00188074 Jy ! Component: 200 - total flux cleaned = 0.00196103 Jy ! Total flux subtracted in 200 components = 0.00196103 Jy ! Clean residual min=-0.001652 max=0.001835 Jy/beam ! Clean residual mean=0.000117 rms=0.000402 Jy/beam ! Combined flux in latest and established models = 0.264005 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 94 components and 0.264005 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.115523Jy sigma=0.852378 ! Fit after self-cal, rms=0.115520Jy sigma=0.852308 ! Inverting map ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! Added new window around map position (-32.2, 25.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00144036 Jy ! Component: 100 - total flux cleaned = 0.00140099 Jy ! Component: 150 - total flux cleaned = 0.00136257 Jy ! Component: 200 - total flux cleaned = 0.00139965 Jy ! Total flux subtracted in 200 components = 0.00139965 Jy ! Clean residual min=-0.001735 max=0.001766 Jy/beam ! Clean residual mean=0.000088 rms=0.000391 Jy/beam ! Combined flux in latest and established models = 0.265405 Jy ! Performing phase self-cal ! Adding 34 model components to the UV plane model. ! The established model now contains 104 components and 0.265405 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.115457Jy sigma=0.851812 ! Fit after self-cal, rms=0.115446Jy sigma=0.851758 ! Inverting map ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! Added new window around map position (0.2, -7). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0013092 Jy ! Component: 100 - total flux cleaned = 0.00142859 Jy ! Component: 150 - total flux cleaned = 0.00142962 Jy ! Component: 200 - total flux cleaned = 0.0014298 Jy ! Total flux subtracted in 200 components = 0.0014298 Jy ! Clean residual min=-0.001824 max=0.001612 Jy/beam ! Clean residual mean=0.000059 rms=0.000384 Jy/beam ! Combined flux in latest and established models = 0.266835 Jy ! Performing phase self-cal ! Adding 39 model components to the UV plane model. ! The established model now contains 115 components and 0.266835 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.115392Jy sigma=0.851193 ! Fit after self-cal, rms=0.115393Jy sigma=0.851150 ! Inverting map ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 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=0.115393Jy sigma=0.851150 ! Fit after self-cal, rms=0.114970Jy sigma=0.850640 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! Estimated beam: bmin=2.789 mas, bmaj=3.416 mas, bpa=-23.46 degrees ! Estimated noise=0.60873 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00144706 Jy ! Component: 100 - total flux cleaned = 0.00224936 Jy ! Component: 150 - total flux cleaned = 0.00247709 Jy ! Component: 200 - total flux cleaned = 0.00260586 Jy ! Total flux subtracted in 200 components = 0.00260586 Jy ! Clean residual min=-0.001458 max=0.001749 Jy/beam ! Clean residual mean=0.000132 rms=0.000425 Jy/beam ! Combined flux in latest and established models = 0.26944 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 135 components and 0.26944 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.114963Jy sigma=0.850308 ! Fit after self-cal, rms=0.114938Jy sigma=0.850238 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 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 = 0.000548759 Jy ! Component: 100 - total flux cleaned = 0.000650752 Jy ! Component: 150 - total flux cleaned = 0.00070513 Jy ! Component: 200 - total flux cleaned = 0.000754062 Jy ! Total flux subtracted in 200 components = 0.000754062 Jy ! Clean residual min=-0.001446 max=0.001715 Jy/beam ! Clean residual mean=0.000100 rms=0.000418 Jy/beam ! Combined flux in latest and established models = 0.270195 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 145 components and 0.270195 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.114940Jy sigma=0.850147 ! Fit after self-cal, rms=0.114941Jy sigma=0.850132 ! Inverting map ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 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 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! Estimated beam: bmin=0.7552 mas, bmaj=1.045 mas, bpa=70.72 degrees ! Estimated noise=0.512807 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7552 x 1.045 at 70.72 degrees (North through East) ! Clean map min=-0.0023066 max=0.22615 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 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! Estimated beam: bmin=0.8395 mas, bmaj=0.9243 mas, bpa=15.8 degrees ! Estimated noise=0.684255 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.174589 Jy ! Component: 100 - total flux cleaned = 0.223513 Jy ! Component: 150 - total flux cleaned = 0.243079 Jy ! Component: 200 - total flux cleaned = 0.253047 Jy ! Total flux subtracted in 200 components = 0.253047 Jy ! Clean residual min=-0.005030 max=0.005194 Jy/beam ! Clean residual mean=0.000007 rms=0.000736 Jy/beam ! Combined flux in latest and established models = 0.253047 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 13 model components to the UV plane model. ! The established model now contains 13 components and 0.253047 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! Estimated beam: bmin=0.7552 mas, bmaj=1.045 mas, bpa=70.72 degrees ! Estimated noise=0.512807 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 = 0.00415947 Jy ! Component: 100 - total flux cleaned = 0.00483014 Jy ! Component: 150 - total flux cleaned = 0.00519633 Jy ! Component: 200 - total flux cleaned = 0.00634069 Jy ! Total flux subtracted in 200 components = 0.00634069 Jy ! Clean residual min=-0.002823 max=0.002797 Jy/beam ! Clean residual mean=0.000288 rms=0.000563 Jy/beam ! Combined flux in latest and established models = 0.259388 Jy ! Adding 19 model components to the UV plane model. ! The established model now contains 30 components and 0.259388 Jy ! Inverting map ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 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 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! Estimated beam: bmin=2.789 mas, bmaj=3.416 mas, bpa=-23.46 degrees ! Estimated noise=0.60873 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00348472 Jy ! Component: 100 - total flux cleaned = 0.00582617 Jy ! Component: 150 - total flux cleaned = 0.00754849 Jy ! Component: 200 - total flux cleaned = 0.00855081 Jy ! Total flux subtracted in 200 components = 0.00855081 Jy ! Clean residual min=-0.001724 max=0.001884 Jy/beam ! Clean residual mean=0.000190 rms=0.000497 Jy/beam ! Combined flux in latest and established models = 0.267939 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 = 0.000337185 Jy ! Component: 100 - total flux cleaned = 0.000641532 Jy ! Component: 150 - total flux cleaned = 0.000921007 Jy ! Component: 200 - total flux cleaned = 0.00110612 Jy ! Total flux subtracted in 200 components = 0.00110612 Jy ! Clean residual min=-0.001603 max=0.001796 Jy/beam ! Clean residual mean=0.000137 rms=0.000459 Jy/beam ! Combined flux in latest and established models = 0.269045 Jy ! Adding 44 model components to the UV plane model. ! The established model now contains 74 components and 0.269045 Jy ! Inverting map ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! Estimated beam: bmin=0.7552 mas, bmaj=1.045 mas, bpa=70.72 degrees ! Estimated noise=0.512807 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000692907 Jy ! Component: 100 - total flux cleaned = -0.000569186 Jy ! Component: 150 - total flux cleaned = -0.000234107 Jy ! Component: 200 - total flux cleaned = 7.33612e-05 Jy ! Total flux subtracted in 200 components = 7.33612e-05 Jy ! Clean residual min=-0.002171 max=0.002100 Jy/beam ! Clean residual mean=0.000072 rms=0.000461 Jy/beam ! Combined flux in latest and established models = 0.269118 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 78 components and 0.269118 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.116292Jy sigma=0.858266 ! Fit after self-cal, rms=0.116442Jy sigma=0.857125 wmodel J2310+1055_X_map.mod ! Writing 78 model components to file: J2310+1055_X_map.mod wobs J2310+1055_X_uvs.fits ! Writing UV FITS file: J2310+1055_X_uvs.fits wwins J2310+1055_X_map.win ! wwins: Wrote 9 windows to J2310+1055_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 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000598306 Jy ! Component: 100 - total flux cleaned = 0.000738694 Jy ! Component: 150 - total flux cleaned = 0.000840019 Jy ! Component: 200 - total flux cleaned = 0.00100351 Jy ! Component: 250 - total flux cleaned = 0.00109899 Jy ! Component: 300 - total flux cleaned = 0.00119319 Jy ! Component: 350 - total flux cleaned = 0.00134705 Jy ! Component: 400 - total flux cleaned = 0.00143766 Jy ! Component: 450 - total flux cleaned = 0.00155673 Jy ! Component: 500 - total flux cleaned = 0.00170315 Jy ! Component: 550 - total flux cleaned = 0.00184729 Jy ! Component: 600 - total flux cleaned = 0.0019042 Jy ! Component: 650 - total flux cleaned = 0.00201651 Jy ! Component: 700 - total flux cleaned = 0.00207199 Jy ! Component: 750 - total flux cleaned = 0.00212706 Jy ! Component: 800 - total flux cleaned = 0.00215426 Jy ! Component: 850 - total flux cleaned = 0.00218133 Jy ! Component: 900 - total flux cleaned = 0.00226142 Jy ! Component: 950 - total flux cleaned = 0.00228768 Jy ! Component: 1000 - total flux cleaned = 0.00228777 Jy ! Component: 1050 - total flux cleaned = 0.00236581 Jy ! Component: 1100 - total flux cleaned = 0.00236583 Jy ! Component: 1150 - total flux cleaned = 0.00241691 Jy ! Component: 1200 - total flux cleaned = 0.00244229 Jy ! Component: 1250 - total flux cleaned = 0.00244241 Jy ! Component: 1300 - total flux cleaned = 0.00244253 Jy ! Component: 1350 - total flux cleaned = 0.00246744 Jy ! Component: 1400 - total flux cleaned = 0.00249205 Jy ! Component: 1450 - total flux cleaned = 0.00249197 Jy ! Component: 1500 - total flux cleaned = 0.00249196 Jy ! Component: 1550 - total flux cleaned = 0.00249205 Jy ! Component: 1600 - total flux cleaned = 0.00249208 Jy ! Component: 1650 - total flux cleaned = 0.00249215 Jy ! Component: 1700 - total flux cleaned = 0.00249216 Jy ! Component: 1750 - total flux cleaned = 0.00251582 Jy ! Component: 1800 - total flux cleaned = 0.00251578 Jy ! Component: 1850 - total flux cleaned = 0.00249234 Jy ! Component: 1900 - total flux cleaned = 0.00251557 Jy ! Component: 1950 - total flux cleaned = 0.00251551 Jy ! Component: 2000 - total flux cleaned = 0.0024694 Jy ! Component: 2050 - total flux cleaned = 0.00251534 Jy ! Component: 2100 - total flux cleaned = 0.00251539 Jy ! Component: 2150 - total flux cleaned = 0.00251541 Jy ! Component: 2200 - total flux cleaned = 0.00253802 Jy ! Component: 2250 - total flux cleaned = 0.00251549 Jy ! Component: 2300 - total flux cleaned = 0.00253789 Jy ! Component: 2350 - total flux cleaned = 0.00253777 Jy ! Component: 2400 - total flux cleaned = 0.00255992 Jy ! Component: 2450 - total flux cleaned = 0.00253774 Jy ! Component: 2500 - total flux cleaned = 0.00255974 Jy ! Component: 2550 - total flux cleaned = 0.00255969 Jy ! Component: 2600 - total flux cleaned = 0.00255964 Jy ! Component: 2650 - total flux cleaned = 0.00255966 Jy ! Component: 2700 - total flux cleaned = 0.00258124 Jy ! Component: 2750 - total flux cleaned = 0.00258114 Jy ! Component: 2800 - total flux cleaned = 0.00258112 Jy ! Component: 2850 - total flux cleaned = 0.00258104 Jy ! Component: 2900 - total flux cleaned = 0.00260229 Jy ! Component: 2950 - total flux cleaned = 0.00258111 Jy ! Component: 3000 - total flux cleaned = 0.00258121 Jy ! Component: 3050 - total flux cleaned = 0.00260219 Jy ! Component: 3100 - total flux cleaned = 0.00260213 Jy ! Component: 3150 - total flux cleaned = 0.0026229 Jy ! Component: 3200 - total flux cleaned = 0.00260213 Jy ! Component: 3250 - total flux cleaned = 0.00262281 Jy ! Component: 3300 - total flux cleaned = 0.00262277 Jy ! Component: 3350 - total flux cleaned = 0.00262283 Jy ! Component: 3400 - total flux cleaned = 0.00264322 Jy ! Component: 3450 - total flux cleaned = 0.00264317 Jy ! Component: 3500 - total flux cleaned = 0.00264319 Jy ! Component: 3550 - total flux cleaned = 0.00266339 Jy ! Component: 3600 - total flux cleaned = 0.00266341 Jy ! Component: 3650 - total flux cleaned = 0.00264335 Jy ! Component: 3700 - total flux cleaned = 0.00268335 Jy ! Component: 3750 - total flux cleaned = 0.00268331 Jy ! Component: 3800 - total flux cleaned = 0.00268332 Jy ! Component: 3850 - total flux cleaned = 0.00268331 Jy ! Component: 3900 - total flux cleaned = 0.00268329 Jy ! Component: 3950 - total flux cleaned = 0.00270297 Jy ! Component: 4000 - total flux cleaned = 0.00270297 Jy ! Component: 4050 - total flux cleaned = 0.00272249 Jy ! Total flux subtracted in 4096 components = 0.00272249 Jy ! Clean residual min=-0.001148 max=0.001045 Jy/beam ! Clean residual mean=0.000011 rms=0.000312 Jy/beam ! Combined flux in latest and established models = 0.271841 Jy keep ! Adding 317 model components to the UV plane model. ! The established model now contains 391 components and 0.271841 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv123_uvs/J2310+1055_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7552 x 1.045 at 70.72 degrees (North through East) ! Clean map min=-0.0017601 max=0.22317 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv123_uvs/J2310+1055_X_map.fits wmodel /scr/pima/rv123_uvs/J2310+1055_X_map.mod ! Writing 391 model components to file: /scr/pima/rv123_uvs/J2310+1055_X_map.mod wobs /scr/pima/rv123_uvs/J2310+1055_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv123_uvs/J2310+1055_X_uvs.fits wwins /scr/pima/rv123_uvs/J2310+1055_X_map.win ! wwins: Wrote 10 windows to /scr/pima/rv123_uvs/J2310+1055_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.223168 invert ! Inverting map ! Your choice of large map pixels excluded 5.76% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1789 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000310775 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.417769 0.417769 0.835538 1.67108 3.34215 6.6843 13.3686 26.7372 53.4744 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0009 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.223 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 718.1 quit ! Quitting program ! Log file /scr/pima/rv123_uvs/J2310+1055_X_dfm.log closed on Sun Dec 23 00:45:57 2018