! Started logfile: /scr/pima/gb073_uvs/J1614+3746_X_uvs.log on Sat Dec 26 09:42:22 2015 obs /scr/pima/gb073_uvs/J1614+3746_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1614+3746_X_uva.fits ! AN table 1: 29 integrations on 55 of 55 possible baselines. ! AN table 2: 29 integrations on 28 of 28 possible baselines. ! AN table 3: 29 integrations on 78 of 78 possible baselines. ! AN table 4: 29 integrations on 55 of 55 possible baselines. ! AN table 5: 29 integrations on 55 of 55 possible baselines. ! Apparent sampling: 0.964627 visibilities/baseline/integration-bin. ! Found source: J1614+3746 ! ! 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 60648 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/J1614+3746_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 29 telescope corrections were flagged in sub-array 1. ! A total of 30 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 30 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 30 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 30 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 5. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 59 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 6. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 59 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 7. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 30 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 8. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 30 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.005939Jy sigma=9.811804 ! Fit after self-cal, rms=0.928845Jy sigma=9.030658 ! 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 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.467 mas, bmaj=0.948 mas, bpa=-18.54 degrees ! Estimated noise=0.768929 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 = 0.0552379 Jy ! Component: 100 - total flux cleaned = 0.0678805 Jy ! Total flux subtracted in 100 components = 0.0678805 Jy ! Clean residual min=-0.002774 max=0.004882 Jy/beam ! Clean residual mean=-0.000004 rms=0.000615 Jy/beam ! Combined flux in latest and established models = 0.0678805 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.0678805 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=0.082168Jy sigma=0.684873 ! Fit after self-cal, rms=0.081636Jy sigma=0.680381 ! Inverting map ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00587116 Jy ! Component: 100 - total flux cleaned = 0.00936334 Jy ! Total flux subtracted in 100 components = 0.00936334 Jy ! Clean residual min=-0.002663 max=0.002553 Jy/beam ! Clean residual mean=-0.000002 rms=0.000563 Jy/beam ! Combined flux in latest and established models = 0.0772438 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 9 components and 0.0772438 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=0.081001Jy sigma=0.671706 ! Fit after self-cal, rms=0.081006Jy sigma=0.671651 ! Inverting map ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 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 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.644 mas, bmaj=1.173 mas, bpa=-14.36 degrees ! Estimated noise=0.333102 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 = 0.00381474 Jy ! Component: 100 - total flux cleaned = 0.00551906 Jy ! Component: 150 - total flux cleaned = 0.00634598 Jy ! Component: 200 - total flux cleaned = 0.00676164 Jy ! Total flux subtracted in 200 components = 0.00676164 Jy ! Clean residual min=-0.001209 max=0.001127 Jy/beam ! Clean residual mean=0.000000 rms=0.000273 Jy/beam ! Combined flux in latest and established models = 0.0840055 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 20 components and 0.0840055 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=0.080860Jy sigma=0.669807 ! Fit after self-cal, rms=0.080855Jy sigma=0.669738 ! Inverting map ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.644 x 1.173 at -14.36 degrees (North through East) ! Clean map min=-0.00097809 max=0.074553 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 1.06 EF 1.00* FD 0.97 KP 0.95 ! LA 1.05 MC 0.97 NL 0.93 OV 0.99 ! PT 0.98 SC 0.96 ZC 0.86 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 0.95 KP 1.02 LA 1.08 ! MK 0.96 NL 0.95 OV 0.95 PT 0.97 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.93 EF 1.00* FD 0.97 KP 0.98 ! LA 1.05 MC 0.99 MK 1.04 NL 0.87 ! ON 1.05 OV 0.95 PT 0.95 SC 0.92 ! ZC 0.84 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 EF 1.00* FD 1.09 KP 0.95 ! LA 1.05 MC 0.97 NL 0.91 ON 1.16 ! PT 0.95 SC 0.92 ZC 0.73 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.93 FD 0.97 KP 0.97 LA 1.06 ! MC 0.95 MK 0.99 NL 0.93 ON 0.95 ! OV 0.98 PT 0.96 SC 0.98 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.08 EF 1.00* FD 1.00 KP 1.01 ! LA 1.04 MC 1.10 NL 0.98 OV 0.97 ! PT 1.03 SC 1.06 ZC 0.83 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.08 FD 1.07 KP 0.95 LA 1.06 ! MK 0.96 NL 0.98 OV 0.99 PT 1.06 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 EF 1.00* FD 1.03 KP 1.02 ! LA 1.07 MC 1.05 MK 1.06 NL 0.97 ! ON 0.98 OV 1.03 PT 1.02 SC 1.04 ! ZC 0.85 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 EF 1.00* FD 1.07 KP 1.03 ! LA 1.04 MC 1.01 NL 0.93 ON 0.87 ! PT 1.05 SC 0.99 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.08 FD 1.02 KP 1.01 LA 1.05 ! MC 1.06 MK 0.94 NL 0.97 ON 0.92 ! OV 1.02 PT 1.02 SC 0.96 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 EF 1.00* FD 0.98 KP 1.02 ! LA 0.98 MC 0.98 NL 0.92 OV 0.99 ! PT 1.02 SC 0.98 ZC 0.88 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 1.05 KP 0.92 LA 0.98 ! MK 0.93 NL 0.94 OV 0.94 PT 1.02 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 EF 1.00* FD 0.99 KP 0.94 ! LA 1.03 MC 1.01 MK 0.94 NL 0.93 ! ON 1.10 OV 1.01 PT 0.98 SC 1.06 ! ZC 0.76 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 EF 1.00* FD 1.08 KP 0.97 ! LA 1.01 MC 0.95 NL 0.95 ON 1.03 ! PT 0.96 SC 1.05 ZC 0.72 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 1.08 KP 1.03 LA 1.02 ! MC 0.88 MK 0.94 NL 0.91 ON 0.96 ! OV 0.99 PT 1.00 SC 0.95 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 EF 1.00* FD 1.03 KP 1.04 ! LA 0.97 MC 0.98 NL 0.99 OV 0.99 ! PT 1.06 SC 0.94 ZC 0.91 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.95 FD 1.01 KP 0.97 LA 1.01 ! MK 1.00 NL 1.03 OV 0.94 PT 1.08 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 EF 1.00* FD 1.03 KP 0.96 ! LA 0.98 MC 1.01 MK 1.01 NL 0.95 ! ON 0.99 OV 0.98 PT 1.00 SC 1.08 ! ZC 0.84 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 EF 1.00* FD 1.08 KP 1.09 ! LA 0.97 MC 1.00 NL 0.99 ON 0.88 ! PT 1.03 SC 1.07 ZC 0.76 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 1.06 KP 0.97 LA 0.98 ! MC 1.06 MK 0.96 NL 0.98 ON 1.02 ! OV 0.95 PT 0.98 SC 0.98 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.06 KP 0.92 ! LA 0.95 MC 1.17 NL 1.03 OV 1.04 ! PT 0.96 SC 1.06 ZC 0.86 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.05 KP 0.81 LA 0.97 ! MK 1.13 NL 1.07 OV 0.96 PT 1.00 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.05 KP 0.91 ! LA 0.99 MC 1.25 MK 1.10 NL 0.96 ! ON 1.18 OV 1.02 PT 0.94 SC 1.09 ! ZC 0.97 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.96 KP 0.92 ! LA 0.97 MC 1.22 NL 1.02 ON 1.10 ! PT 1.03 SC 1.01 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 1.07 KP 0.91 LA 1.01 ! MC 1.07 MK 0.97 NL 1.03 ON 1.09 ! OV 1.11 PT 1.00 SC 1.06 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.06 KP 0.95 ! LA 1.01 MC 1.08 NL 0.98 OV 1.12 ! PT 0.97 SC 0.95 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.11 KP 0.87 LA 0.98 ! MK 1.03 NL 0.96 OV 0.99 PT 1.00 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 0.99 KP 0.84 ! LA 0.94 MC 1.35 MK 1.02 NL 1.02 ! ON 1.25 OV 1.07 PT 0.99 SC 1.04 ! ZC 0.92 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.03 KP 0.92 ! LA 1.00 MC 1.23 NL 1.03 ON 1.26 ! PT 0.95 SC 1.03 ZC 0.75 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 1.01 KP 0.84 LA 1.08 ! MC 1.26 MK 1.00 NL 1.01 ON 1.14 ! OV 1.07 PT 0.95 SC 0.96 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 EF 1.00* FD 1.03 KP 0.91 ! LA 1.04 MC 1.26 NL 1.00 OV 1.08 ! PT 1.06 SC 0.97 ZC 0.78 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.07 FD 1.14 KP 0.91 LA 1.17 ! MK 1.07 NL 1.03 OV 0.98 PT 1.00 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.10 EF 1.00* FD 1.12 KP 0.89 ! LA 1.00 MC 1.41 MK 1.36 NL 1.00 ! ON 1.30 OV 1.06 PT 1.00 SC 0.99 ! ZC 0.69 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 EF 1.00* FD 1.15 KP 0.96 ! LA 1.12 MC 1.21 NL 0.94 ON 1.39 ! PT 1.10 SC 1.01 ZC 0.65 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 1.06 KP 1.01 LA 0.99 ! MC 1.12 MK 1.11 NL 1.01 ON 1.35 ! OV 1.01 PT 1.13 SC 0.98 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 EF 1.00* FD 1.02 KP 0.91 ! LA 1.01 MC 1.34 NL 1.03 OV 1.10 ! PT 1.06 SC 1.01 ZC 0.72 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 0.93 KP 0.91 LA 1.05 ! MK 1.00 NL 1.11 OV 0.96 PT 1.07 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 EF 1.00* FD 1.03 KP 0.96 ! LA 1.00 MC 1.13 MK 1.11 NL 0.96 ! ON 1.61 OV 1.04 PT 1.11 SC 0.97 ! ZC 0.70 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 EF 1.00* FD 0.96 KP 0.98 ! LA 1.11 MC 1.38 NL 1.02 ON 1.17 ! PT 0.94 SC 1.02 ZC 0.56 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.04 FD 0.94 KP 0.97 LA 1.03 ! MC 1.21 MK 1.02 NL 1.01 ON 1.15 ! OV 1.00 PT 1.08 SC 1.02 ! ! ! Fit before self-cal, rms=0.080855Jy sigma=0.669738 ! Fit after self-cal, rms=0.082659Jy sigma=0.663860 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6424 mas, bmaj=1.179 mas, bpa=-14.54 degrees ! Estimated noise=0.333725 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 = 0.000164572 Jy ! Component: 100 - total flux cleaned = 0.00013902 Jy ! Component: 150 - total flux cleaned = 0.00011812 Jy ! Component: 200 - total flux cleaned = 0.000109196 Jy ! Total flux subtracted in 200 components = 0.000109196 Jy ! Clean residual min=-0.000933 max=0.001009 Jy/beam ! Clean residual mean=-0.000002 rms=0.000209 Jy/beam ! Combined flux in latest and established models = 0.0841146 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 22 components and 0.0841147 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=0.082654Jy sigma=0.663823 ! Fit after self-cal, rms=0.082774Jy sigma=0.663496 ! Inverting map ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Added new window around map position (22.2, -43.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000894016 Jy ! Component: 100 - total flux cleaned = 0.00101855 Jy ! Component: 150 - total flux cleaned = 0.00103463 Jy ! Component: 200 - total flux cleaned = 0.0010347 Jy ! Total flux subtracted in 200 components = 0.0010347 Jy ! Clean residual min=-0.000924 max=0.000881 Jy/beam ! Clean residual mean=-0.000001 rms=0.000207 Jy/beam ! Combined flux in latest and established models = 0.0851494 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 35 components and 0.0851494 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=0.082762Jy sigma=0.663400 ! Fit after self-cal, rms=0.082763Jy sigma=0.663383 ! Inverting map ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 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=0.082763Jy sigma=0.663383 ! Fit after self-cal, rms=0.083241Jy sigma=0.663355 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6418 mas, bmaj=1.178 mas, bpa=-14.67 degrees ! Estimated noise=0.33457 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000419389 Jy ! Component: 100 - total flux cleaned = 0.000512813 Jy ! Component: 150 - total flux cleaned = 0.000535999 Jy ! Component: 200 - total flux cleaned = 0.000535693 Jy ! Total flux subtracted in 200 components = 0.000535693 Jy ! Clean residual min=-0.000902 max=0.000884 Jy/beam ! Clean residual mean=-0.000001 rms=0.000207 Jy/beam ! Combined flux in latest and established models = 0.0856851 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 37 components and 0.0856851 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=0.083235Jy sigma=0.663322 ! Fit after self-cal, rms=0.083244Jy sigma=0.663317 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 6.31859e-05 Jy ! Component: 100 - total flux cleaned = 7.42489e-05 Jy ! Component: 150 - total flux cleaned = 7.41719e-05 Jy ! Component: 200 - total flux cleaned = 7.39118e-05 Jy ! Total flux subtracted in 200 components = 7.39118e-05 Jy ! Clean residual min=-0.000901 max=0.000879 Jy/beam ! Clean residual mean=-0.000001 rms=0.000206 Jy/beam ! Combined flux in latest and established models = 0.085759 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 41 components and 0.085759 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=0.083241Jy sigma=0.663300 ! Fit after self-cal, rms=0.083241Jy sigma=0.663299 ! Inverting map ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 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=0.083241Jy sigma=0.663299 ! Fit after self-cal, rms=0.083318Jy sigma=0.663281 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6411 mas, bmaj=1.177 mas, bpa=-14.75 degrees ! Estimated noise=0.335285 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000296602 Jy ! Component: 100 - total flux cleaned = 0.000316173 Jy ! Component: 150 - total flux cleaned = 0.000316407 Jy ! Component: 200 - total flux cleaned = 0.000316635 Jy ! Total flux subtracted in 200 components = 0.000316635 Jy ! Clean residual min=-0.000895 max=0.000886 Jy/beam ! Clean residual mean=-0.000001 rms=0.000206 Jy/beam ! Combined flux in latest and established models = 0.0860756 Jy selfcal ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 46 components and 0.0860756 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=0.083315Jy sigma=0.663262 ! Fit after self-cal, rms=0.083313Jy sigma=0.663260 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 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 = 1.92882e-05 Jy ! Component: 100 - total flux cleaned = 1.09043e-05 Jy ! Component: 150 - total flux cleaned = 2.84358e-06 Jy ! Component: 200 - total flux cleaned = -4.88768e-06 Jy ! Total flux subtracted in 200 components = -4.88768e-06 Jy ! Clean residual min=-0.000894 max=0.000889 Jy/beam ! Clean residual mean=-0.000001 rms=0.000206 Jy/beam ! Combined flux in latest and established models = 0.0860707 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 49 components and 0.0860707 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=0.083311Jy sigma=0.663251 ! Fit after self-cal, rms=0.083311Jy sigma=0.663248 ! Inverting map ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 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=0.083311Jy sigma=0.663248 ! Fit after self-cal, rms=0.083411Jy sigma=0.663233 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=2.713 mas, bmaj=3.009 mas, bpa=33.63 degrees ! Estimated noise=0.440109 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000347786 Jy ! Component: 100 - total flux cleaned = 0.000473668 Jy ! Component: 150 - total flux cleaned = 0.000480404 Jy ! Component: 200 - total flux cleaned = 0.000483563 Jy ! Total flux subtracted in 200 components = 0.000483563 Jy ! Clean residual min=-0.000967 max=0.000868 Jy/beam ! Clean residual mean=-0.000003 rms=0.000255 Jy/beam ! Combined flux in latest and established models = 0.0865543 Jy selfcal ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 53 components and 0.0865543 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=0.083413Jy sigma=0.663245 ! Fit after self-cal, rms=0.083410Jy sigma=0.663240 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 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 = 8.13392e-06 Jy ! Component: 100 - total flux cleaned = 1.19728e-05 Jy ! Component: 150 - total flux cleaned = 2.2771e-05 Jy ! Component: 200 - total flux cleaned = 2.60309e-05 Jy ! Total flux subtracted in 200 components = 2.60309e-05 Jy ! Clean residual min=-0.000968 max=0.000868 Jy/beam ! Clean residual mean=-0.000003 rms=0.000255 Jy/beam ! Combined flux in latest and established models = 0.0865803 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 54 components and 0.0865803 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=0.083410Jy sigma=0.663243 ! Fit after self-cal, rms=0.083410Jy sigma=0.663239 ! Inverting map ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 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 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6405 mas, bmaj=1.177 mas, bpa=-14.82 degrees ! Estimated noise=0.33609 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6405 x 1.177 at -14.82 degrees (North through East) ! Clean map min=-0.00073973 max=0.074948 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 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.4627 mas, bmaj=0.9537 mas, bpa=-18.98 degrees ! Estimated noise=0.775559 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0558912 Jy ! Component: 100 - total flux cleaned = 0.0692121 Jy ! Component: 150 - total flux cleaned = 0.0751534 Jy ! Component: 200 - total flux cleaned = 0.0785244 Jy ! Total flux subtracted in 200 components = 0.0785244 Jy ! Clean residual min=-0.002320 max=0.002304 Jy/beam ! Clean residual mean=-0.000002 rms=0.000513 Jy/beam ! Combined flux in latest and established models = 0.0785244 Jy uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 11 model components to the UV plane model. ! The established model now contains 11 components and 0.0785244 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6405 mas, bmaj=1.177 mas, bpa=-14.82 degrees ! Estimated noise=0.33609 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 = 0.00374861 Jy ! Component: 100 - total flux cleaned = 0.00542855 Jy ! Component: 150 - total flux cleaned = 0.00642473 Jy ! Component: 200 - total flux cleaned = 0.00688332 Jy ! Total flux subtracted in 200 components = 0.00688332 Jy ! Clean residual min=-0.000932 max=0.000869 Jy/beam ! Clean residual mean=-0.000003 rms=0.000210 Jy/beam ! Combined flux in latest and established models = 0.0854077 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 29 components and 0.0854077 Jy ! Inverting map ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 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 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=2.713 mas, bmaj=3.009 mas, bpa=33.63 degrees ! Estimated noise=0.440109 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000692997 Jy ! Component: 100 - total flux cleaned = 0.000958787 Jy ! Component: 150 - total flux cleaned = 0.00101662 Jy ! Component: 200 - total flux cleaned = 0.0010631 Jy ! Total flux subtracted in 200 components = 0.0010631 Jy ! Clean residual min=-0.000970 max=0.000863 Jy/beam ! Clean residual mean=-0.000003 rms=0.000255 Jy/beam ! Combined flux in latest and established models = 0.0864708 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 = 3.75394e-05 Jy ! Component: 100 - total flux cleaned = 6.8249e-05 Jy ! Component: 150 - total flux cleaned = 8.66556e-05 Jy ! Component: 200 - total flux cleaned = 0.000102558 Jy ! Total flux subtracted in 200 components = 0.000102558 Jy ! Clean residual min=-0.000968 max=0.000873 Jy/beam ! Clean residual mean=-0.000003 rms=0.000255 Jy/beam ! Combined flux in latest and established models = 0.0865734 Jy ! Adding 15 model components to the UV plane model. ! The established model now contains 43 components and 0.0865734 Jy ! Inverting map ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6405 mas, bmaj=1.177 mas, bpa=-14.82 degrees ! Estimated noise=0.33609 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000222809 Jy ! Component: 100 - total flux cleaned = -0.000224061 Jy ! Component: 150 - total flux cleaned = -0.00019338 Jy ! Component: 200 - total flux cleaned = -0.000180208 Jy ! Total flux subtracted in 200 components = -0.000180208 Jy ! Clean residual min=-0.000907 max=0.000891 Jy/beam ! Clean residual mean=-0.000002 rms=0.000207 Jy/beam ! Combined flux in latest and established models = 0.0863932 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 50 components and 0.0863932 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=0.083409Jy sigma=0.663256 ! Fit after self-cal, rms=0.083406Jy sigma=0.663235 wmodel /scr/pima/gb073_uvs/J1614+3746_X_map.mod ! Writing 50 model components to file: /scr/pima/gb073_uvs/J1614+3746_X_map.mod wobs /scr/pima/gb073_uvs/J1614+3746_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1614+3746_X_uvs.fits wwins /scr/pima/gb073_uvs/J1614+3746_X_map.win ! wwins: Wrote 2 windows to /scr/pima/gb073_uvs/J1614+3746_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 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000207538 Jy ! Component: 100 - total flux cleaned = -0.000438102 Jy ! Component: 150 - total flux cleaned = -0.000596475 Jy ! Component: 200 - total flux cleaned = -0.000673786 Jy ! Component: 250 - total flux cleaned = -0.000779682 Jy ! Component: 300 - total flux cleaned = -0.00085373 Jy ! Component: 350 - total flux cleaned = -0.000926298 Jy ! Component: 400 - total flux cleaned = -0.00101212 Jy ! Component: 450 - total flux cleaned = -0.00108288 Jy ! Component: 500 - total flux cleaned = -0.00115266 Jy ! Component: 550 - total flux cleaned = -0.00122132 Jy ! Component: 600 - total flux cleaned = -0.00130307 Jy ! Component: 650 - total flux cleaned = -0.00135694 Jy ! Component: 700 - total flux cleaned = -0.00139681 Jy ! Component: 750 - total flux cleaned = -0.00143647 Jy ! Component: 800 - total flux cleaned = -0.00144963 Jy ! Component: 850 - total flux cleaned = -0.00150169 Jy ! Component: 900 - total flux cleaned = -0.00154029 Jy ! Component: 950 - total flux cleaned = -0.00161689 Jy ! Component: 1000 - total flux cleaned = -0.00157877 Jy ! Component: 1050 - total flux cleaned = -0.00164176 Jy ! Component: 1100 - total flux cleaned = -0.00166697 Jy ! Component: 1150 - total flux cleaned = -0.00170432 Jy ! Component: 1200 - total flux cleaned = -0.00174149 Jy ! Component: 1250 - total flux cleaned = -0.001803 Jy ! Component: 1300 - total flux cleaned = -0.00179065 Jy ! Component: 1350 - total flux cleaned = -0.00183942 Jy ! Component: 1400 - total flux cleaned = -0.00188786 Jy ! Component: 1450 - total flux cleaned = -0.00191199 Jy ! Component: 1500 - total flux cleaned = -0.00194787 Jy ! Component: 1550 - total flux cleaned = -0.00197162 Jy ! Component: 1600 - total flux cleaned = -0.00197172 Jy ! Component: 1650 - total flux cleaned = -0.00200705 Jy ! Component: 1700 - total flux cleaned = -0.00203039 Jy ! Component: 1750 - total flux cleaned = -0.00199545 Jy ! Component: 1800 - total flux cleaned = -0.0020303 Jy ! Component: 1850 - total flux cleaned = -0.00207656 Jy ! Component: 1900 - total flux cleaned = -0.00209952 Jy ! Component: 1950 - total flux cleaned = -0.00211095 Jy ! Component: 2000 - total flux cleaned = -0.00211095 Jy ! Component: 2050 - total flux cleaned = -0.00211092 Jy ! Component: 2100 - total flux cleaned = -0.00207713 Jy ! Component: 2150 - total flux cleaned = -0.0020884 Jy ! Component: 2200 - total flux cleaned = -0.00209968 Jy ! Component: 2250 - total flux cleaned = -0.002133 Jy ! Component: 2300 - total flux cleaned = -0.0021109 Jy ! Component: 2350 - total flux cleaned = -0.00209986 Jy ! Component: 2400 - total flux cleaned = -0.00209979 Jy ! Component: 2450 - total flux cleaned = -0.0020998 Jy ! Component: 2500 - total flux cleaned = -0.00209979 Jy ! Component: 2550 - total flux cleaned = -0.00209978 Jy ! Component: 2600 - total flux cleaned = -0.00212144 Jy ! Component: 2650 - total flux cleaned = -0.00215366 Jy ! Component: 2700 - total flux cleaned = -0.00212147 Jy ! Component: 2750 - total flux cleaned = -0.00208944 Jy ! Component: 2800 - total flux cleaned = -0.00208942 Jy ! Component: 2850 - total flux cleaned = -0.0021001 Jy ! Component: 2900 - total flux cleaned = -0.00212123 Jy ! Component: 2950 - total flux cleaned = -0.0021212 Jy ! Component: 3000 - total flux cleaned = -0.0021317 Jy ! Component: 3050 - total flux cleaned = -0.00211079 Jy ! Component: 3100 - total flux cleaned = -0.00209002 Jy ! Component: 3150 - total flux cleaned = -0.00211076 Jy ! Component: 3200 - total flux cleaned = -0.0021004 Jy ! Component: 3250 - total flux cleaned = -0.00211071 Jy ! Component: 3300 - total flux cleaned = -0.00215186 Jy ! Component: 3350 - total flux cleaned = -0.00222364 Jy ! Component: 3400 - total flux cleaned = -0.00218276 Jy ! Component: 3450 - total flux cleaned = -0.00216236 Jy ! Component: 3500 - total flux cleaned = -0.00213186 Jy ! Component: 3550 - total flux cleaned = -0.0021724 Jy ! Component: 3600 - total flux cleaned = -0.00215216 Jy ! Component: 3650 - total flux cleaned = -0.00215216 Jy ! Component: 3700 - total flux cleaned = -0.00214212 Jy ! Component: 3750 - total flux cleaned = -0.00218215 Jy ! Component: 3800 - total flux cleaned = -0.00216222 Jy ! Component: 3850 - total flux cleaned = -0.00213237 Jy ! Component: 3900 - total flux cleaned = -0.00214236 Jy ! Component: 3950 - total flux cleaned = -0.00216217 Jy ! Component: 4000 - total flux cleaned = -0.00213256 Jy ! Component: 4050 - total flux cleaned = -0.00213255 Jy ! Total flux subtracted in 4096 components = -0.00215216 Jy ! Clean residual min=-0.000535 max=0.000543 Jy/beam ! Clean residual mean=-0.000002 rms=0.000161 Jy/beam ! Combined flux in latest and established models = 0.084241 Jy keep ! Adding 341 model components to the UV plane model. ! The established model now contains 391 components and 0.084241 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1614+3746_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6405 x 1.177 at -14.82 degrees (North through East) ! Clean map min=-0.00068685 max=0.075178 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1614+3746_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0751781 invert ! Inverting map ! Your choice of large map pixels excluded 6.15% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000161158 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.643104 0.643104 1.28621 2.57242 5.14484 10.2897 20.5793 41.1587 82.3174 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0004 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.075 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 466.487 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1614+3746_X_uvs.log closed on Sat Dec 26 09:42:29 2015