! Started logfile: /scr/pima/gb073_uvs/J1742+5945_X_uvs.log on Sat Dec 26 09:43:09 2015 obs /scr/pima/gb073_uvs/J1742+5945_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1742+5945_X_uva.fits ! AN table 1: 9 integrations on 45 of 45 possible baselines. ! AN table 2: 5 integrations on 15 of 15 possible baselines. ! AN table 3: 7 integrations on 78 of 78 possible baselines. ! AN table 4: 7 integrations on 66 of 66 possible baselines. ! AN table 5: 7 integrations on 45 of 45 possible baselines. ! AN table 6: 8 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.856285 visibilities/baseline/integration-bin. ! Found source: J1742+5945 ! ! There are 8 IFs, and a total of 8 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.39799e+09 8e+06 1 8e+06 ! 02 2 8.40599e+09 8e+06 1 8e+06 ! 03 3 8.46799e+09 8e+06 1 8e+06 ! 04 4 8.47599e+09 8e+06 1 8e+06 ! 05 5 8.78299e+09 8e+06 1 8e+06 ! 06 6 8.79099e+09 8e+06 1 8e+06 ! 07 7 8.88799e+09 8e+06 1 8e+06 ! 08 8 8.89599e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 0 lines of history. ! ! Reading 15968 visibilities. select RR ! Selecting polarization: RR, channels: 1..8 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 ! Reading IF 5 channels: 5..5 ! Reading IF 6 channels: 6..6 ! Reading IF 7 channels: 7..7 ! Reading IF 8 channels: 8..8 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 ![@/home/lpetrov/bin/01_muppet /scr/pima/gb073_uvs/J1742+5945_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 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 3 telescope corrections were flagged in sub-array 1. ! A total of 7 telescope corrections were flagged in sub-array 3. ! A total of 7 telescope corrections were flagged in sub-array 4. ! A total of 8 telescope corrections were flagged in sub-array 5. ! A total of 8 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 3 telescope corrections were flagged in sub-array 1. ! A total of 7 telescope corrections were flagged in sub-array 3. ! A total of 7 telescope corrections were flagged in sub-array 4. ! A total of 8 telescope corrections were flagged in sub-array 5. ! A total of 8 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 3 telescope corrections were flagged in sub-array 1. ! A total of 7 telescope corrections were flagged in sub-array 3. ! A total of 7 telescope corrections were flagged in sub-array 4. ! A total of 8 telescope corrections were flagged in sub-array 5. ! A total of 8 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 3 telescope corrections were flagged in sub-array 1. ! A total of 7 telescope corrections were flagged in sub-array 3. ! A total of 7 telescope corrections were flagged in sub-array 4. ! A total of 8 telescope corrections were flagged in sub-array 5. ! A total of 8 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 5. ! A total of 12 telescope corrections were flagged in sub-array 1. ! A total of 5 telescope corrections were flagged in sub-array 2. ! A total of 14 telescope corrections were flagged in sub-array 3. ! A total of 14 telescope corrections were flagged in sub-array 4. ! A total of 14 telescope corrections were flagged in sub-array 5. ! A total of 16 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 6. ! A total of 12 telescope corrections were flagged in sub-array 1. ! A total of 5 telescope corrections were flagged in sub-array 2. ! A total of 14 telescope corrections were flagged in sub-array 3. ! A total of 14 telescope corrections were flagged in sub-array 4. ! A total of 14 telescope corrections were flagged in sub-array 5. ! A total of 16 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 7. ! A total of 3 telescope corrections were flagged in sub-array 1. ! A total of 7 telescope corrections were flagged in sub-array 3. ! A total of 7 telescope corrections were flagged in sub-array 4. ! A total of 8 telescope corrections were flagged in sub-array 5. ! A total of 8 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 8. ! A total of 3 telescope corrections were flagged in sub-array 1. ! A total of 7 telescope corrections were flagged in sub-array 3. ! A total of 7 telescope corrections were flagged in sub-array 4. ! A total of 8 telescope corrections were flagged in sub-array 5. ! A total of 8 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.007725Jy sigma=8.997508 ! Fit after self-cal, rms=0.907777Jy sigma=8.107725 ! 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 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.5248 mas, bmaj=0.6993 mas, bpa=45.33 degrees ! Estimated noise=1.2854 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 = 0.072265 Jy ! Component: 100 - total flux cleaned = 0.0889086 Jy ! Total flux subtracted in 100 components = 0.0889086 Jy ! Clean residual min=-0.004518 max=0.006784 Jy/beam ! Clean residual mean=-0.000007 rms=0.000984 Jy/beam ! Combined flux in latest and established models = 0.0889086 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.0889086 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.095527Jy sigma=0.672659 ! Fit after self-cal, rms=0.095224Jy sigma=0.671062 ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0070725 Jy ! Component: 100 - total flux cleaned = 0.0108995 Jy ! Total flux subtracted in 100 components = 0.0108995 Jy ! Clean residual min=-0.004258 max=0.004462 Jy/beam ! Clean residual mean=-0.000004 rms=0.000933 Jy/beam ! Combined flux in latest and established models = 0.0998081 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 9 components and 0.0998081 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.094399Jy sigma=0.661214 ! Fit after self-cal, rms=0.094369Jy sigma=0.660997 ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 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 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.6817 mas, bmaj=0.8812 mas, bpa=46.73 degrees ! Estimated noise=0.744856 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 (1.2, -0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00631133 Jy ! Component: 100 - total flux cleaned = 0.00916021 Jy ! Component: 150 - total flux cleaned = 0.0108359 Jy ! Component: 200 - total flux cleaned = 0.0115576 Jy ! Total flux subtracted in 200 components = 0.0115576 Jy ! Clean residual min=-0.002688 max=0.003422 Jy/beam ! Clean residual mean=0.000002 rms=0.000581 Jy/beam ! Combined flux in latest and established models = 0.111366 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 27 components and 0.111366 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.093981Jy sigma=0.656849 ! Fit after self-cal, rms=0.093916Jy sigma=0.656227 ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Added new window around map position (4.4, -0.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00324977 Jy ! Component: 100 - total flux cleaned = 0.0050622 Jy ! Component: 150 - total flux cleaned = 0.00563311 Jy ! Component: 200 - total flux cleaned = 0.0057209 Jy ! Total flux subtracted in 200 components = 0.0057209 Jy ! Clean residual min=-0.002477 max=0.002666 Jy/beam ! Clean residual mean=0.000006 rms=0.000547 Jy/beam ! Combined flux in latest and established models = 0.117087 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 39 components and 0.117087 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.093788Jy sigma=0.655102 ! Fit after self-cal, rms=0.093767Jy sigma=0.654912 ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6817 x 0.8812 at 46.73 degrees (North through East) ! Clean map min=-0.0020291 max=0.09297 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.93 FD 0.95 KP 0.93 LA 1.19 ! MC 0.98 NL 0.95 OV 1.00 PT 0.97 ! SC 0.66 ZC 0.93 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.91 KP 1.03 MK 1.09 ON 1.19 ! OV 0.81 PT 1.02 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.92 EF 1.00* FD 0.99 KP 0.98 ! LA 1.08 MC 0.86 MK 0.96 NL 1.04 ! ON 0.87 OV 0.98 PT 0.92 SC 0.92 ! ZC 0.90 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.90 EF 1.00* FD 0.96 KP 0.99 ! LA 1.10 MC 0.91 NL 1.00 ON 0.87 ! OV 1.19 PT 0.96 SC 0.93 ZC 0.90 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.07 EF 1.00* FD 0.96 KP 0.99 ! LA 1.03 MC 0.60 MK 1.17 NL 1.01 ! PT 0.96 ZC 0.85 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.95 EF 1.00* FD 0.99 KP 1.04 ! LA 1.02 MC 0.90 MK 0.97 NL 0.93 ! ON 1.09 PT 1.07 SC 0.94 ZC 0.98 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 1.14 KP 1.12 LA 1.12 ! MC 0.88 NL 0.98 OV 1.06 PT 1.10 ! SC 0.71 ZC 1.16 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 KP 1.11 MK 0.97 ON 0.92 ! OV 0.90 PT 1.13 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 EF 1.00* FD 1.08 KP 1.10 ! LA 1.12 MC 0.90 MK 0.99 NL 1.09 ! ON 0.91 OV 1.11 PT 0.94 SC 1.05 ! ZC 0.90 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.87 EF 1.00* FD 1.01 KP 1.15 ! LA 1.18 MC 0.86 NL 0.95 ON 1.00 ! OV 1.11 PT 1.20 SC 0.94 ZC 0.97 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.86 EF 1.00* FD 1.00 KP 1.01 ! LA 1.08 MC 0.55 MK 0.99 NL 0.98 ! PT 0.98 ZC 1.16 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.96 EF 1.00* FD 1.00 KP 1.08 ! LA 1.12 MC 1.19 MK 0.99 NL 1.01 ! ON 1.06 PT 1.04 SC 0.97 ZC 0.91 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 1.09 KP 0.95 LA 1.00 ! MC 1.00 NL 0.99 OV 1.10 PT 1.08 ! SC 0.82 ZC 1.28 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.93 KP 1.13 MK 0.91 ON 0.73 ! OV 0.93 PT 1.18 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 EF 1.00* FD 0.97 KP 1.01 ! LA 1.01 MC 1.12 MK 0.99 NL 0.98 ! ON 0.92 OV 0.99 PT 0.92 SC 1.10 ! ZC 0.92 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.13 EF 1.00* FD 1.02 KP 0.94 ! LA 0.96 MC 0.92 NL 0.87 ON 0.92 ! OV 0.99 PT 1.04 SC 1.07 ZC 1.04 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.94 EF 1.00* FD 1.07 KP 0.86 ! LA 0.95 MC 0.89 MK 0.93 NL 1.14 ! PT 0.98 ZC 1.02 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.92 EF 1.00* FD 0.96 KP 1.04 ! LA 0.95 MC 1.02 MK 0.92 NL 1.01 ! ON 0.94 PT 1.01 SC 1.06 ZC 0.85 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 1.18 KP 1.00 LA 1.14 ! MC 1.22 NL 0.91 OV 1.09 PT 0.97 ! SC 0.67 ZC 0.90 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.06 KP 0.90 MK 1.14 ON 0.92 ! OV 1.06 PT 1.02 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 EF 1.00* FD 1.04 KP 1.01 ! LA 1.02 MC 0.86 MK 1.01 NL 1.20 ! ON 0.77 OV 0.97 PT 0.91 SC 1.07 ! ZC 0.95 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.94 EF 1.00* FD 1.09 KP 0.94 ! LA 1.00 MC 1.13 NL 0.98 ON 0.96 ! OV 0.97 PT 1.21 SC 0.99 ZC 1.06 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.05 EF 1.00* FD 0.92 KP 1.01 ! LA 0.95 MC 0.77 MK 1.08 NL 1.02 ! PT 0.97 ZC 1.09 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.95 EF 1.00* FD 0.99 KP 1.07 ! LA 1.02 MC 0.94 MK 1.12 NL 1.03 ! ON 0.99 PT 0.92 SC 1.13 ZC 0.81 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.19 KP 0.98 LA 0.94 ! MC 1.19 NL 1.02 OV 1.24 PT 0.99 ! SC 0.80 ZC 1.13 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* KP 1.07 MK 0.95 ON 1.71 ! OV 0.93 PT 0.96 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.06 KP 0.91 ! LA 0.98 MC 1.62 MK 0.96 NL 1.05 ! ON 1.16 OV 1.11 PT 0.93 SC 0.87 ! ZC 0.90 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.12 KP 0.97 ! LA 0.93 MC 1.17 NL 0.92 ON 1.29 ! OV 1.04 PT 1.06 SC 1.07 ZC 0.98 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.03 KP 0.84 ! LA 1.06 MC 0.94 MK 0.84 NL 0.98 ! PT 0.94 ZC 1.09 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.03 KP 1.06 ! LA 0.97 MC 1.50 MK 1.15 NL 0.96 ! ON 1.29 PT 0.94 SC 1.03 ZC 0.89 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.14 KP 1.09 LA 0.94 ! MC 1.17 NL 0.90 OV 1.04 PT 1.03 ! SC 0.67 ZC 0.98 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* KP 0.65 MK 1.09 ON 1.02 ! OV 1.09 PT 0.92 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.01 KP 0.86 ! LA 1.06 MC 1.24 MK 0.99 NL 1.18 ! ON 0.98 OV 1.01 PT 0.86 SC 1.07 ! ZC 0.89 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.01 KP 0.77 ! LA 0.99 MC 0.91 NL 1.10 ON 1.00 ! OV 1.04 PT 1.00 SC 1.10 ZC 0.98 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.03 KP 0.92 ! LA 0.86 MC 0.72 MK 1.12 NL 0.94 ! PT 1.02 ZC 1.02 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.11 KP 0.83 ! LA 0.93 MC 1.22 MK 1.00 NL 1.07 ! ON 1.17 PT 1.02 SC 0.88 ZC 0.86 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 1.18 KP 0.92 LA 0.99 ! MC 1.43 NL 0.85 OV 1.02 PT 1.02 ! SC 0.80 ZC 0.86 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.31 KP 0.83 MK 1.09 ON 1.41 ! OV 1.10 PT 0.88 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 EF 1.00* FD 1.25 KP 0.88 ! LA 0.97 MC 1.08 MK 1.06 NL 1.06 ! ON 1.30 OV 1.10 PT 0.99 SC 1.04 ! ZC 0.66 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.93 EF 1.00* FD 1.02 KP 0.84 ! LA 1.00 MC 1.31 NL 1.08 ON 0.99 ! OV 1.10 PT 1.14 SC 0.94 ZC 0.87 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 EF 1.00* FD 1.06 KP 0.90 ! LA 1.09 MC 0.78 MK 0.98 NL 0.94 ! PT 0.95 ZC 0.79 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.20 EF 1.00* FD 0.96 KP 0.83 ! LA 1.15 MC 1.43 MK 1.01 NL 1.02 ! ON 1.22 PT 0.91 SC 0.94 ZC 0.74 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.24 FD 0.99 KP 0.88 LA 1.01 ! MC 1.16 NL 1.04 OV 1.06 PT 1.12 ! SC 0.57 ZC 0.92 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.14 KP 1.00 MK 1.10 ON 1.16 ! OV 0.86 PT 1.04 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.08 EF 1.00* FD 0.93 KP 0.94 ! LA 1.05 MC 1.18 MK 1.08 NL 1.11 ! ON 1.55 OV 1.01 PT 1.03 SC 1.11 ! ZC 0.77 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.04 EF 1.00* FD 1.01 KP 1.12 ! LA 1.02 MC 1.41 NL 1.06 ON 1.06 ! OV 1.02 PT 0.94 SC 1.05 ZC 0.92 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.92 EF 1.00* FD 0.99 KP 1.00 ! LA 1.10 MC 1.31 MK 1.07 NL 0.97 ! PT 0.93 ZC 0.74 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.98 EF 1.00* FD 0.97 KP 1.02 ! LA 1.02 MC 1.26 MK 1.03 NL 1.11 ! ON 1.37 PT 0.92 SC 1.10 ZC 0.66 ! ! ! Fit before self-cal, rms=0.093767Jy sigma=0.654912 ! Fit after self-cal, rms=0.093894Jy sigma=0.644023 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.6787 mas, bmaj=0.8844 mas, bpa=47.18 degrees ! Estimated noise=0.750968 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 (-40.6, 24). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00214992 Jy ! Component: 100 - total flux cleaned = 0.00326623 Jy ! Component: 150 - total flux cleaned = 0.00364341 Jy ! Component: 200 - total flux cleaned = 0.00378961 Jy ! Total flux subtracted in 200 components = 0.00378961 Jy ! Clean residual min=-0.002057 max=0.001929 Jy/beam ! Clean residual mean=-0.000001 rms=0.000450 Jy/beam ! Combined flux in latest and established models = 0.120876 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 56 components and 0.120876 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.093827Jy sigma=0.643595 ! Fit after self-cal, rms=0.093927Jy sigma=0.643139 ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 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. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.093927Jy sigma=0.643139 ! Fit after self-cal, rms=0.094298Jy sigma=0.643048 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.6771 mas, bmaj=0.8832 mas, bpa=47.1 degrees ! Estimated noise=0.753126 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00138148 Jy ! Component: 100 - total flux cleaned = 0.00192972 Jy ! Component: 150 - total flux cleaned = 0.00202727 Jy ! Component: 200 - total flux cleaned = 0.00208779 Jy ! Total flux subtracted in 200 components = 0.00208779 Jy ! Clean residual min=-0.002003 max=0.001974 Jy/beam ! Clean residual mean=-0.000001 rms=0.000448 Jy/beam ! Combined flux in latest and established models = 0.122964 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 59 components and 0.122964 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.094263Jy sigma=0.642874 ! Fit after self-cal, rms=0.094267Jy sigma=0.642847 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 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 (7.2, -2.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00179652 Jy ! Component: 100 - total flux cleaned = 0.0019025 Jy ! Component: 150 - total flux cleaned = 0.00190277 Jy ! Component: 200 - total flux cleaned = 0.00187481 Jy ! Total flux subtracted in 200 components = 0.00187481 Jy ! Clean residual min=-0.002051 max=0.001868 Jy/beam ! Clean residual mean=0.000000 rms=0.000439 Jy/beam ! Combined flux in latest and established models = 0.124839 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 70 components and 0.124839 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.094225Jy sigma=0.642539 ! Fit after self-cal, rms=0.094216Jy sigma=0.642489 ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 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. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.094216Jy sigma=0.642489 ! Fit after self-cal, rms=0.094379Jy sigma=0.642389 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.6752 mas, bmaj=0.8818 mas, bpa=46.89 degrees ! Estimated noise=0.755171 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00127497 Jy ! Component: 100 - total flux cleaned = 0.00191363 Jy ! Component: 150 - total flux cleaned = 0.00196937 Jy ! Component: 200 - total flux cleaned = 0.00202116 Jy ! Total flux subtracted in 200 components = 0.00202116 Jy ! Clean residual min=-0.002021 max=0.001869 Jy/beam ! Clean residual mean=-0.000000 rms=0.000435 Jy/beam ! Combined flux in latest and established models = 0.12686 Jy selfcal ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 73 components and 0.12686 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.094351Jy sigma=0.642244 ! Fit after self-cal, rms=0.094343Jy sigma=0.642219 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 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 = 0.000364692 Jy ! Component: 100 - total flux cleaned = 0.000414792 Jy ! Component: 150 - total flux cleaned = 0.000438787 Jy ! Component: 200 - total flux cleaned = 0.000461207 Jy ! Total flux subtracted in 200 components = 0.000461207 Jy ! Clean residual min=-0.002001 max=0.001889 Jy/beam ! Clean residual mean=-0.000000 rms=0.000435 Jy/beam ! Combined flux in latest and established models = 0.127321 Jy ! Performing phase self-cal ! Adding 36 model components to the UV plane model. ! The established model now contains 78 components and 0.127321 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.094329Jy sigma=0.642165 ! Fit after self-cal, rms=0.094325Jy sigma=0.642158 ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 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. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.094325Jy sigma=0.642158 ! Fit after self-cal, rms=0.094577Jy sigma=0.642098 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=2.678 mas, bmaj=3.159 mas, bpa=-60.11 degrees ! Estimated noise=1.00717 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000953699 Jy ! Component: 100 - total flux cleaned = 0.0011636 Jy ! Component: 150 - total flux cleaned = 0.00116315 Jy ! Component: 200 - total flux cleaned = 0.00117811 Jy ! Total flux subtracted in 200 components = 0.00117811 Jy ! Clean residual min=-0.002482 max=0.001952 Jy/beam ! Clean residual mean=-0.000002 rms=0.000561 Jy/beam ! Combined flux in latest and established models = 0.128499 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 92 components and 0.128499 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.094566Jy sigma=0.642058 ! Fit after self-cal, rms=0.094561Jy sigma=0.642040 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 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 = 7.00043e-05 Jy ! Component: 100 - total flux cleaned = 0.000152597 Jy ! Component: 150 - total flux cleaned = 0.000165392 Jy ! Component: 200 - total flux cleaned = 0.000164801 Jy ! Total flux subtracted in 200 components = 0.000164801 Jy ! Clean residual min=-0.002495 max=0.001954 Jy/beam ! Clean residual mean=-0.000002 rms=0.000561 Jy/beam ! Combined flux in latest and established models = 0.128664 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 93 components and 0.128664 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.094556Jy sigma=0.642049 ! Fit after self-cal, rms=0.094553Jy sigma=0.642038 ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 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 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.6735 mas, bmaj=0.881 mas, bpa=46.75 degrees ! Estimated noise=0.757888 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6735 x 0.881 at 46.75 degrees (North through East) ! Clean map min=-0.0017559 max=0.093074 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 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.5169 mas, bmaj=0.7048 mas, bpa=45.28 degrees ! Estimated noise=1.29894 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.072753 Jy ! Component: 100 - total flux cleaned = 0.0906472 Jy ! Component: 150 - total flux cleaned = 0.0991719 Jy ! Component: 200 - total flux cleaned = 0.10489 Jy ! Total flux subtracted in 200 components = 0.10489 Jy ! Clean residual min=-0.003674 max=0.003386 Jy/beam ! Clean residual mean=-0.000006 rms=0.000837 Jy/beam ! Combined flux in latest and established models = 0.10489 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 19 model components to the UV plane model. ! The established model now contains 19 components and 0.10489 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.6735 mas, bmaj=0.881 mas, bpa=46.75 degrees ! Estimated noise=0.757888 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 = 0.00725445 Jy ! Component: 100 - total flux cleaned = 0.0116395 Jy ! Component: 150 - total flux cleaned = 0.0148169 Jy ! Component: 200 - total flux cleaned = 0.017257 Jy ! Total flux subtracted in 200 components = 0.017257 Jy ! Clean residual min=-0.002134 max=0.001815 Jy/beam ! Clean residual mean=-0.000003 rms=0.000460 Jy/beam ! Combined flux in latest and established models = 0.122147 Jy ! Adding 39 model components to the UV plane model. ! The established model now contains 48 components and 0.122147 Jy ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 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 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=2.678 mas, bmaj=3.159 mas, bpa=-60.11 degrees ! Estimated noise=1.00717 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00279479 Jy ! Component: 100 - total flux cleaned = 0.00432375 Jy ! Component: 150 - total flux cleaned = 0.0052969 Jy ! Component: 200 - total flux cleaned = 0.00573708 Jy ! Total flux subtracted in 200 components = 0.00573708 Jy ! Clean residual min=-0.002520 max=0.001930 Jy/beam ! Clean residual mean=-0.000002 rms=0.000561 Jy/beam ! Combined flux in latest and established models = 0.127884 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 = 0.00023408 Jy ! Component: 100 - total flux cleaned = 0.000423393 Jy ! Component: 150 - total flux cleaned = 0.000496501 Jy ! Component: 200 - total flux cleaned = 0.000535621 Jy ! Total flux subtracted in 200 components = 0.000535621 Jy ! Clean residual min=-0.002515 max=0.001936 Jy/beam ! Clean residual mean=-0.000001 rms=0.000560 Jy/beam ! Combined flux in latest and established models = 0.12842 Jy ! Adding 45 model components to the UV plane model. ! The established model now contains 87 components and 0.12842 Jy ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.6735 mas, bmaj=0.881 mas, bpa=46.75 degrees ! Estimated noise=0.757888 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 5.86104e-05 Jy ! Component: 100 - total flux cleaned = 2.02706e-05 Jy ! Component: 150 - total flux cleaned = 9.30177e-05 Jy ! Component: 200 - total flux cleaned = 0.000158615 Jy ! Total flux subtracted in 200 components = 0.000158615 Jy ! Clean residual min=-0.002022 max=0.001918 Jy/beam ! Clean residual mean=-0.000001 rms=0.000438 Jy/beam ! Combined flux in latest and established models = 0.128578 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 97 components and 0.128578 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.094590Jy sigma=0.642316 ! Fit after self-cal, rms=0.094571Jy sigma=0.642204 wmodel /scr/pima/gb073_uvs/J1742+5945_X_map.mod ! Writing 97 model components to file: /scr/pima/gb073_uvs/J1742+5945_X_map.mod wobs /scr/pima/gb073_uvs/J1742+5945_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1742+5945_X_uvs.fits wwins /scr/pima/gb073_uvs/J1742+5945_X_map.win ! wwins: Wrote 5 windows to /scr/pima/gb073_uvs/J1742+5945_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 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000492027 Jy ! Component: 100 - total flux cleaned = -0.000702575 Jy ! Component: 150 - total flux cleaned = -0.000937078 Jy ! Component: 200 - total flux cleaned = -0.00122821 Jy ! Component: 250 - total flux cleaned = -0.00151144 Jy ! Component: 300 - total flux cleaned = -0.00178867 Jy ! Component: 350 - total flux cleaned = -0.00202982 Jy ! Component: 400 - total flux cleaned = -0.00229728 Jy ! Component: 450 - total flux cleaned = -0.00247288 Jy ! Component: 500 - total flux cleaned = -0.00264575 Jy ! Component: 550 - total flux cleaned = -0.00264532 Jy ! Component: 600 - total flux cleaned = -0.00278622 Jy ! Component: 650 - total flux cleaned = -0.00278573 Jy ! Component: 700 - total flux cleaned = -0.0028133 Jy ! Component: 750 - total flux cleaned = -0.00300466 Jy ! Component: 800 - total flux cleaned = -0.00292321 Jy ! Component: 850 - total flux cleaned = -0.00295037 Jy ! Component: 900 - total flux cleaned = -0.00300345 Jy ! Component: 950 - total flux cleaned = -0.00300332 Jy ! Component: 1000 - total flux cleaned = -0.00292471 Jy ! Component: 1050 - total flux cleaned = -0.00284667 Jy ! Component: 1100 - total flux cleaned = -0.00282099 Jy ! Component: 1150 - total flux cleaned = -0.00282102 Jy ! Component: 1200 - total flux cleaned = -0.00266824 Jy ! Component: 1250 - total flux cleaned = -0.00269364 Jy ! Component: 1300 - total flux cleaned = -0.00254326 Jy ! Component: 1350 - total flux cleaned = -0.00266777 Jy ! Component: 1400 - total flux cleaned = -0.00246932 Jy ! Component: 1450 - total flux cleaned = -0.00249397 Jy ! Component: 1500 - total flux cleaned = -0.00239632 Jy ! Component: 1550 - total flux cleaned = -0.00232344 Jy ! Component: 1600 - total flux cleaned = -0.00229937 Jy ! Component: 1650 - total flux cleaned = -0.00234738 Jy ! Component: 1700 - total flux cleaned = -0.00232334 Jy ! Component: 1750 - total flux cleaned = -0.00225217 Jy ! Component: 1800 - total flux cleaned = -0.00237033 Jy ! Component: 1850 - total flux cleaned = -0.00222928 Jy ! Component: 1900 - total flux cleaned = -0.00229936 Jy ! Component: 1950 - total flux cleaned = -0.00234585 Jy ! Component: 2000 - total flux cleaned = -0.00223046 Jy ! Component: 2050 - total flux cleaned = -0.00227636 Jy ! Component: 2100 - total flux cleaned = -0.00229919 Jy ! Component: 2150 - total flux cleaned = -0.00227637 Jy ! Component: 2200 - total flux cleaned = -0.00229913 Jy ! Component: 2250 - total flux cleaned = -0.0022992 Jy ! Component: 2300 - total flux cleaned = -0.00234413 Jy ! Component: 2350 - total flux cleaned = -0.00241086 Jy ! Component: 2400 - total flux cleaned = -0.00238875 Jy ! Component: 2450 - total flux cleaned = -0.00247679 Jy ! Component: 2500 - total flux cleaned = -0.00247677 Jy ! Component: 2550 - total flux cleaned = -0.00243301 Jy ! Component: 2600 - total flux cleaned = -0.00254182 Jy ! Component: 2650 - total flux cleaned = -0.00243361 Jy ! Component: 2700 - total flux cleaned = -0.00256311 Jy ! Component: 2750 - total flux cleaned = -0.00260625 Jy ! Component: 2800 - total flux cleaned = -0.00273446 Jy ! Component: 2850 - total flux cleaned = -0.00275569 Jy ! Component: 2900 - total flux cleaned = -0.0028191 Jy ! Component: 2950 - total flux cleaned = -0.00288245 Jy ! Component: 3000 - total flux cleaned = -0.00305027 Jy ! Component: 3050 - total flux cleaned = -0.0029876 Jy ! Component: 3100 - total flux cleaned = -0.00307078 Jy ! Component: 3150 - total flux cleaned = -0.00311211 Jy ! Component: 3200 - total flux cleaned = -0.00317396 Jy ! Component: 3250 - total flux cleaned = -0.00317395 Jy ! Component: 3300 - total flux cleaned = -0.00317396 Jy ! Component: 3350 - total flux cleaned = -0.00325557 Jy ! Component: 3400 - total flux cleaned = -0.00335697 Jy ! Component: 3450 - total flux cleaned = -0.00333673 Jy ! Component: 3500 - total flux cleaned = -0.00351819 Jy ! Component: 3550 - total flux cleaned = -0.00349798 Jy ! Component: 3600 - total flux cleaned = -0.00353794 Jy ! Component: 3650 - total flux cleaned = -0.00367747 Jy ! Component: 3700 - total flux cleaned = -0.00373706 Jy ! Component: 3750 - total flux cleaned = -0.00381623 Jy ! Component: 3800 - total flux cleaned = -0.0038162 Jy ! Component: 3850 - total flux cleaned = -0.00381608 Jy ! Component: 3900 - total flux cleaned = -0.00385539 Jy ! Component: 3950 - total flux cleaned = -0.0039333 Jy ! Component: 4000 - total flux cleaned = -0.00395281 Jy ! Component: 4050 - total flux cleaned = -0.00397226 Jy ! Total flux subtracted in 4096 components = -0.00404965 Jy ! Clean residual min=-0.001221 max=0.001266 Jy/beam ! Clean residual mean=-0.000002 rms=0.000314 Jy/beam ! Combined flux in latest and established models = 0.124529 Jy keep ! Adding 351 model components to the UV plane model. ! The established model now contains 448 components and 0.124529 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1742+5945_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6735 x 0.881 at 46.75 degrees (North through East) ! Clean map min=-0.0017054 max=0.092849 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1742+5945_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0928488 invert ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1689 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000313279 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.01222 1.01222 2.02445 4.0489 8.0978 16.1956 32.3912 64.7824 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0009 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.092 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 296.376 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1742+5945_X_uvs.log closed on Sat Dec 26 09:43:14 2015