! Started logfile: /scr/pima/gb073_uvs/J1058+8114_X_uvs.log on Sat Dec 26 09:36:46 2015 obs /scr/pima/gb073_uvs/J1058+8114_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1058+8114_X_uva.fits ! AN table 1: 6 integrations on 55 of 55 possible baselines. ! AN table 2: 6 integrations on 78 of 78 possible baselines. ! AN table 3: 6 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.990787 visibilities/baseline/integration-bin. ! Found source: J1058+8114 ! ! 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 9464 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/J1058+8114_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 6 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 7 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 7 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 7 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 7 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 5. ! A total of 12 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! A total of 13 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 6. ! A total of 12 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! A total of 13 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 7. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 7 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 8. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 7 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=1.069986Jy sigma=9.878337 ! Fit after self-cal, rms=0.695584Jy sigma=6.084120 ! 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 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.527 mas, bmaj=0.5881 mas, bpa=83.51 degrees ! Estimated noise=1.51572 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 = 0.23848 Jy ! Component: 100 - total flux cleaned = 0.334585 Jy ! Total flux subtracted in 100 components = 0.334585 Jy ! Clean residual min=-0.017132 max=0.044799 Jy/beam ! Clean residual mean=-0.000017 rms=0.003708 Jy/beam ! Combined flux in latest and established models = 0.334585 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.334585 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=0.148919Jy sigma=1.276090 ! Fit after self-cal, rms=0.146090Jy sigma=1.257943 ! Inverting map ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec ! Added new window around map position (0, -0.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0531825 Jy ! Component: 100 - total flux cleaned = 0.0849085 Jy ! Total flux subtracted in 100 components = 0.0849085 Jy ! Clean residual min=-0.012415 max=0.024343 Jy/beam ! Clean residual mean=-0.000007 rms=0.002348 Jy/beam ! Combined flux in latest and established models = 0.419493 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 16 components and 0.419494 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=0.117975Jy sigma=0.911521 ! Fit after self-cal, rms=0.116672Jy sigma=0.901303 ! Inverting map ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0239964 Jy ! Component: 100 - total flux cleaned = 0.0377711 Jy ! Total flux subtracted in 100 components = 0.0377711 Jy ! Clean residual min=-0.010263 max=0.014358 Jy/beam ! Clean residual mean=-0.000002 rms=0.001929 Jy/beam ! Combined flux in latest and established models = 0.457265 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 17 components and 0.457265 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=0.110023Jy sigma=0.813961 ! Fit after self-cal, rms=0.109365Jy sigma=0.808971 ! Inverting map ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 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 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.649 mas, bmaj=0.721 mas, bpa=88.49 degrees ! Estimated noise=0.957527 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 = 0.0150201 Jy ! Component: 100 - total flux cleaned = 0.0215361 Jy ! Component: 150 - total flux cleaned = 0.0230713 Jy ! Component: 200 - total flux cleaned = 0.0235553 Jy ! Total flux subtracted in 200 components = 0.0235553 Jy ! Clean residual min=-0.007503 max=0.007805 Jy/beam ! Clean residual mean=0.000003 rms=0.001382 Jy/beam ! Combined flux in latest and established models = 0.48082 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 21 components and 0.48082 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=0.107420Jy sigma=0.783708 ! Fit after self-cal, rms=0.107142Jy sigma=0.781729 ! Inverting map ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec ! Added new window around map position (-12, -15). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00649546 Jy ! Component: 100 - total flux cleaned = 0.00766162 Jy ! Component: 150 - total flux cleaned = 0.00799125 Jy ! Component: 200 - total flux cleaned = 0.00828929 Jy ! Total flux subtracted in 200 components = 0.00828929 Jy ! Clean residual min=-0.007339 max=0.006125 Jy/beam ! Clean residual mean=0.000002 rms=0.001312 Jy/beam ! Combined flux in latest and established models = 0.489109 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 33 components and 0.489109 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=0.106114Jy sigma=0.772687 ! Fit after self-cal, rms=0.106051Jy sigma=0.772171 ! Inverting map ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.649 x 0.721 at 88.49 degrees (North through East) ! Clean map min=-0.0054246 max=0.30634 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 0.94 EF 1.00* FD 0.98 KP 0.99 ! LA 1.04 MC 0.96 MK 1.02 NL 0.93 ! OV 1.00 PT 0.95 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 EF 1.00* FD 0.98 KP 1.00 ! LA 1.02 MC 1.02 MK 0.98 NL 0.92 ! ON 1.12 OV 1.01 PT 0.98 SC 0.94 ! ZC 0.72 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 EF 1.00* FD 1.00 KP 0.99 ! LA 1.01 MC 1.04 MK 0.99 NL 0.95 ! ON 1.07 PT 0.97 SC 0.95 ZC 0.78 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 EF 1.00* FD 1.03 KP 1.00 ! LA 1.08 MC 0.97 MK 0.98 NL 0.98 ! OV 1.03 PT 1.00 ZC 0.82 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 EF 1.00* FD 1.04 KP 1.01 ! LA 1.05 MC 1.04 MK 0.99 NL 0.97 ! ON 1.01 OV 1.03 PT 1.04 SC 1.00 ! ZC 0.77 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 EF 1.00* FD 1.04 KP 1.01 ! LA 1.07 MC 1.00 MK 0.98 NL 0.97 ! ON 1.05 PT 1.02 SC 0.98 ZC 0.82 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 EF 1.00* FD 1.00 KP 0.97 ! LA 0.96 MC 1.04 MK 0.94 NL 0.94 ! OV 0.99 PT 0.98 ZC 0.73 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 EF 1.00* FD 1.02 KP 0.95 ! LA 1.01 MC 1.01 MK 0.95 NL 0.98 ! ON 1.09 OV 1.00 PT 1.00 SC 1.01 ! ZC 0.68 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 EF 1.00* FD 1.01 KP 0.95 ! LA 0.97 MC 1.03 MK 0.94 NL 0.99 ! ON 1.00 PT 1.02 SC 1.04 ZC 0.77 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 EF 1.00* FD 0.99 KP 1.01 ! LA 1.00 MC 1.01 MK 0.97 NL 0.96 ! OV 1.01 PT 1.01 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 EF 1.00* FD 1.04 KP 0.96 ! LA 1.01 MC 1.16 MK 0.96 NL 0.99 ! ON 1.11 OV 0.99 PT 1.02 SC 1.01 ! ZC 0.70 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 EF 1.00* FD 1.04 KP 1.00 ! LA 1.00 MC 1.07 MK 1.00 NL 0.95 ! ON 1.14 PT 1.04 SC 1.02 ZC 0.80 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.98 KP 0.89 ! LA 0.99 MC 1.48 MK 0.98 NL 1.01 ! OV 1.05 PT 1.00 ZC 0.74 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.03 KP 0.93 ! LA 0.99 MC 1.43 MK 0.98 NL 0.99 ! ON 1.35 OV 1.07 PT 1.01 SC 1.01 ! ZC 0.68 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00 KP 0.92 ! LA 0.97 MC 1.29 MK 0.99 NL 1.00 ! ON 1.33 PT 1.02 SC 1.03 ZC 0.80 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00 KP 0.89 ! LA 0.98 MC 1.42 MK 1.01 NL 1.06 ! OV 1.04 PT 0.95 ZC 0.74 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 0.98 KP 0.90 ! LA 1.00 MC 1.41 MK 1.00 NL 1.02 ! ON 1.46 OV 1.03 PT 0.97 SC 0.99 ! ZC 0.68 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.06 KP 0.93 ! LA 0.99 MC 1.32 MK 0.98 NL 1.02 ! ON 1.31 PT 0.91 SC 0.99 ZC 0.76 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 EF 1.00* FD 1.03 KP 0.92 ! LA 1.04 MC 1.55 MK 1.04 NL 1.02 ! OV 1.00 PT 1.00 ZC 0.62 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 EF 1.00* FD 1.06 KP 0.93 ! LA 1.00 MC 1.43 MK 1.05 NL 1.09 ! ON 1.48 OV 1.01 PT 1.02 SC 1.05 ! ZC 0.54 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 EF 1.00* FD 1.09 KP 0.92 ! LA 1.08 MC 1.31 MK 1.04 NL 1.03 ! ON 1.41 PT 1.01 SC 1.04 ZC 0.63 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 EF 1.00* FD 1.01 KP 0.93 ! LA 1.03 MC 1.74 MK 1.07 NL 1.04 ! OV 1.02 PT 1.03 ZC 0.60 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 EF 1.00* FD 1.02 KP 0.91 ! LA 1.06 MC 1.45 MK 1.04 NL 1.04 ! ON 1.64 OV 1.01 PT 1.02 SC 1.06 ! ZC 0.51 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 EF 1.00* FD 1.05 KP 0.94 ! LA 1.03 MC 1.40 MK 1.02 NL 1.03 ! ON 1.49 PT 1.06 SC 1.13 ZC 0.62 ! ! ! Fit before self-cal, rms=0.106051Jy sigma=0.772171 ! Fit after self-cal, rms=0.094153Jy sigma=0.654633 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.6413 mas, bmaj=0.7203 mas, bpa=81.24 degrees ! Estimated noise=0.959909 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 = -0.00127537 Jy ! Component: 100 - total flux cleaned = -0.00183658 Jy ! Component: 150 - total flux cleaned = -0.00201016 Jy ! Component: 200 - total flux cleaned = -0.00216608 Jy ! Total flux subtracted in 200 components = -0.00216608 Jy ! Clean residual min=-0.003115 max=0.002963 Jy/beam ! Clean residual mean=-0.000005 rms=0.000660 Jy/beam ! Combined flux in latest and established models = 0.486943 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 44 components and 0.486943 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=0.093865Jy sigma=0.652239 ! Fit after self-cal, rms=0.094097Jy sigma=0.651167 ! Inverting map ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 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=0.094097Jy sigma=0.651167 ! Fit after self-cal, rms=0.094343Jy sigma=0.650873 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.6409 mas, bmaj=0.7212 mas, bpa=80.12 degrees ! Estimated noise=0.959333 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000811427 Jy ! Component: 100 - total flux cleaned = -0.00116529 Jy ! Component: 150 - total flux cleaned = -0.00147081 Jy ! Component: 200 - total flux cleaned = -0.0016723 Jy ! Total flux subtracted in 200 components = -0.0016723 Jy ! Clean residual min=-0.002873 max=0.002804 Jy/beam ! Clean residual mean=-0.000005 rms=0.000637 Jy/beam ! Combined flux in latest and established models = 0.485271 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 45 components and 0.485271 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=0.094165Jy sigma=0.649285 ! Fit after self-cal, rms=0.094141Jy sigma=0.648979 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 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 = -3.67588e-05 Jy ! Component: 100 - total flux cleaned = -0.000226946 Jy ! Component: 150 - total flux cleaned = -0.000399852 Jy ! Component: 200 - total flux cleaned = -0.00050371 Jy ! Total flux subtracted in 200 components = -0.00050371 Jy ! Clean residual min=-0.002823 max=0.002692 Jy/beam ! Clean residual mean=-0.000005 rms=0.000625 Jy/beam ! Combined flux in latest and established models = 0.484767 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 47 components and 0.484767 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=0.094032Jy sigma=0.647955 ! Fit after self-cal, rms=0.094012Jy sigma=0.647744 ! Inverting map ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 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=0.094012Jy sigma=0.647744 ! Fit after self-cal, rms=0.094188Jy sigma=0.647558 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.6404 mas, bmaj=0.722 mas, bpa=79.57 degrees ! Estimated noise=0.9584 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000901233 Jy ! Component: 100 - total flux cleaned = -0.00121735 Jy ! Component: 150 - total flux cleaned = -0.00143498 Jy ! Component: 200 - total flux cleaned = -0.0015334 Jy ! Total flux subtracted in 200 components = -0.0015334 Jy ! Clean residual min=-0.002726 max=0.002594 Jy/beam ! Clean residual mean=-0.000005 rms=0.000613 Jy/beam ! Combined flux in latest and established models = 0.483234 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 47 components and 0.483234 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=0.094088Jy sigma=0.646709 ! Fit after self-cal, rms=0.094075Jy sigma=0.646553 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 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 = -3.99871e-05 Jy ! Component: 100 - total flux cleaned = -8.8078e-05 Jy ! Component: 150 - total flux cleaned = -0.000132724 Jy ! Component: 200 - total flux cleaned = -0.000175152 Jy ! Total flux subtracted in 200 components = -0.000175152 Jy ! Clean residual min=-0.002717 max=0.002575 Jy/beam ! Clean residual mean=-0.000005 rms=0.000607 Jy/beam ! Combined flux in latest and established models = 0.483059 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 51 components and 0.483059 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=0.094017Jy sigma=0.645991 ! Fit after self-cal, rms=0.094003Jy sigma=0.645865 ! Inverting map ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 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=0.094003Jy sigma=0.645865 ! Fit after self-cal, rms=0.094081Jy sigma=0.645799 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=2.707 mas, bmaj=2.734 mas, bpa=61.93 degrees ! Estimated noise=1.33168 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00033607 Jy ! Component: 100 - total flux cleaned = 0.000188826 Jy ! Component: 150 - total flux cleaned = 4.58183e-05 Jy ! Component: 200 - total flux cleaned = -5.62913e-05 Jy ! Total flux subtracted in 200 components = -5.62913e-05 Jy ! Clean residual min=-0.002623 max=0.003166 Jy/beam ! Clean residual mean=-0.000012 rms=0.000728 Jy/beam ! Combined flux in latest and established models = 0.483002 Jy selfcal ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 51 components and 0.483002 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=0.094085Jy sigma=0.645791 ! Fit after self-cal, rms=0.094073Jy sigma=0.645616 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 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 (10, 50.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00180757 Jy ! Component: 100 - total flux cleaned = 0.0023044 Jy ! Component: 150 - total flux cleaned = 0.00257964 Jy ! Component: 200 - total flux cleaned = 0.00277707 Jy ! Total flux subtracted in 200 components = 0.00277707 Jy ! Clean residual min=-0.002619 max=0.002453 Jy/beam ! Clean residual mean=-0.000013 rms=0.000685 Jy/beam ! Combined flux in latest and established models = 0.485779 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 73 components and 0.485779 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=0.094024Jy sigma=0.645323 ! Fit after self-cal, rms=0.094017Jy sigma=0.645258 ! Inverting map ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 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 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.6402 mas, bmaj=0.7224 mas, bpa=79.3 degrees ! Estimated noise=0.957638 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6402 x 0.7224 at 79.3 degrees (North through East) ! Clean map min=-0.0021057 max=0.30377 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 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.5133 mas, bmaj=0.5923 mas, bpa=72.85 degrees ! Estimated noise=1.51478 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.240906 Jy ! Component: 100 - total flux cleaned = 0.344981 Jy ! Component: 150 - total flux cleaned = 0.396595 Jy ! Component: 200 - total flux cleaned = 0.425658 Jy ! Total flux subtracted in 200 components = 0.425658 Jy ! Clean residual min=-0.006091 max=0.015096 Jy/beam ! Clean residual mean=-0.000008 rms=0.001441 Jy/beam ! Combined flux in latest and established models = 0.425658 Jy uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 12 model components to the UV plane model. ! The established model now contains 12 components and 0.425658 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.6402 mas, bmaj=0.7224 mas, bpa=79.3 degrees ! Estimated noise=0.957638 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 = 0.0265913 Jy ! Component: 100 - total flux cleaned = 0.0396478 Jy ! Component: 150 - total flux cleaned = 0.0463101 Jy ! Component: 200 - total flux cleaned = 0.0502429 Jy ! Total flux subtracted in 200 components = 0.0502429 Jy ! Clean residual min=-0.002882 max=0.004197 Jy/beam ! Clean residual mean=-0.000005 rms=0.000641 Jy/beam ! Combined flux in latest and established models = 0.475901 Jy ! Adding 22 model components to the UV plane model. ! The established model now contains 26 components and 0.475901 Jy ! Inverting map ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec ! Added new window around map position (-0.8, -0.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00347552 Jy ! Component: 100 - total flux cleaned = 0.00496796 Jy ! Component: 150 - total flux cleaned = 0.00601388 Jy ! Component: 200 - total flux cleaned = 0.00694659 Jy ! Total flux subtracted in 200 components = 0.00694659 Jy ! Clean residual min=-0.002651 max=0.002722 Jy/beam ! Clean residual mean=-0.000005 rms=0.000589 Jy/beam ! Combined flux in latest and established models = 0.482847 Jy ! Adding 29 model components to the UV plane model. ! The established model now contains 49 components and 0.482847 Jy ! Inverting map ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec ! Added new window around map position (37.6, 12.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00163046 Jy ! Component: 100 - total flux cleaned = 0.00234543 Jy ! Component: 150 - total flux cleaned = 0.00270741 Jy ! Component: 200 - total flux cleaned = 0.002766 Jy ! Total flux subtracted in 200 components = 0.002766 Jy ! Clean residual min=-0.002593 max=0.002498 Jy/beam ! Clean residual mean=-0.000005 rms=0.000573 Jy/beam ! Combined flux in latest and established models = 0.485613 Jy ! Adding 49 model components to the UV plane model. ! The established model now contains 79 components and 0.485613 Jy ! Inverting map ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 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 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=2.707 mas, bmaj=2.734 mas, bpa=61.93 degrees ! Estimated noise=1.33168 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00125273 Jy ! Component: 100 - total flux cleaned = 0.00189405 Jy ! Component: 150 - total flux cleaned = 0.00181233 Jy ! Component: 200 - total flux cleaned = 0.00181241 Jy ! Total flux subtracted in 200 components = 0.00181241 Jy ! Clean residual min=-0.002582 max=0.002371 Jy/beam ! Clean residual mean=-0.000012 rms=0.000665 Jy/beam ! Combined flux in latest and established models = 0.487426 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 = -0.000130254 Jy ! Component: 100 - total flux cleaned = -0.000190297 Jy ! Component: 150 - total flux cleaned = -0.000189836 Jy ! Component: 200 - total flux cleaned = -0.000217078 Jy ! Total flux subtracted in 200 components = -0.000217078 Jy ! Clean residual min=-0.002528 max=0.002378 Jy/beam ! Clean residual mean=-0.000012 rms=0.000657 Jy/beam ! Combined flux in latest and established models = 0.487209 Jy ! Adding 39 model components to the UV plane model. ! The established model now contains 114 components and 0.487209 Jy ! Inverting map ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.6402 mas, bmaj=0.7224 mas, bpa=79.3 degrees ! Estimated noise=0.957638 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000294795 Jy ! Component: 100 - total flux cleaned = -0.000401341 Jy ! Component: 150 - total flux cleaned = -0.000452587 Jy ! Component: 200 - total flux cleaned = -0.000550243 Jy ! Total flux subtracted in 200 components = -0.000550243 Jy ! Clean residual min=-0.002703 max=0.002480 Jy/beam ! Clean residual mean=-0.000004 rms=0.000557 Jy/beam ! Combined flux in latest and established models = 0.486658 Jy selfcal ! Performing phase self-cal ! Adding 40 model components to the UV plane model. ! The established model now contains 130 components and 0.486658 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=0.093887Jy sigma=0.645195 ! Fit after self-cal, rms=0.093747Jy sigma=0.643473 wmodel /scr/pima/gb073_uvs/J1058+8114_X_map.mod ! Writing 130 model components to file: /scr/pima/gb073_uvs/J1058+8114_X_map.mod wobs /scr/pima/gb073_uvs/J1058+8114_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1058+8114_X_uvs.fits wwins /scr/pima/gb073_uvs/J1058+8114_X_map.win ! wwins: Wrote 6 windows to /scr/pima/gb073_uvs/J1058+8114_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 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000269306 Jy ! Component: 100 - total flux cleaned = -0.000268127 Jy ! Component: 150 - total flux cleaned = -0.00022606 Jy ! Component: 200 - total flux cleaned = -0.000225988 Jy ! Component: 250 - total flux cleaned = -0.000305913 Jy ! Component: 300 - total flux cleaned = -0.000424199 Jy ! Component: 350 - total flux cleaned = -0.000502234 Jy ! Component: 400 - total flux cleaned = -0.00054075 Jy ! Component: 450 - total flux cleaned = -0.000578998 Jy ! Component: 500 - total flux cleaned = -0.000616154 Jy ! Component: 550 - total flux cleaned = -0.000616457 Jy ! Component: 600 - total flux cleaned = -0.000616118 Jy ! Component: 650 - total flux cleaned = -0.000438259 Jy ! Component: 700 - total flux cleaned = -0.000473581 Jy ! Component: 750 - total flux cleaned = -0.000403791 Jy ! Component: 800 - total flux cleaned = -0.000196823 Jy ! Component: 850 - total flux cleaned = -0.000162867 Jy ! Component: 900 - total flux cleaned = 3.93161e-05 Jy ! Component: 950 - total flux cleaned = -0.000128454 Jy ! Component: 1000 - total flux cleaned = -2.8967e-05 Jy ! Component: 1050 - total flux cleaned = 6.94435e-05 Jy ! Component: 1100 - total flux cleaned = 0.000167136 Jy ! Component: 1150 - total flux cleaned = 0.000198885 Jy ! Component: 1200 - total flux cleaned = 0.000262758 Jy ! Component: 1250 - total flux cleaned = 0.000230914 Jy ! Component: 1300 - total flux cleaned = 0.000294372 Jy ! Component: 1350 - total flux cleaned = 0.000294524 Jy ! Component: 1400 - total flux cleaned = 0.000356823 Jy ! Component: 1450 - total flux cleaned = 0.000387776 Jy ! Component: 1500 - total flux cleaned = 0.000295854 Jy ! Component: 1550 - total flux cleaned = 0.000509355 Jy ! Component: 1600 - total flux cleaned = 0.000569784 Jy ! Component: 1650 - total flux cleaned = 0.000418891 Jy ! Component: 1700 - total flux cleaned = 0.000538406 Jy ! Component: 1750 - total flux cleaned = 0.000597854 Jy ! Component: 1800 - total flux cleaned = 0.000509175 Jy ! Component: 1850 - total flux cleaned = 0.00065632 Jy ! Component: 1900 - total flux cleaned = 0.000743744 Jy ! Component: 1950 - total flux cleaned = 0.000685919 Jy ! Component: 2000 - total flux cleaned = 0.000801315 Jy ! Component: 2050 - total flux cleaned = 0.000772507 Jy ! Component: 2100 - total flux cleaned = 0.000886624 Jy ! Component: 2150 - total flux cleaned = 0.000915155 Jy ! Component: 2200 - total flux cleaned = 0.00100003 Jy ! Component: 2250 - total flux cleaned = 0.00105608 Jy ! Component: 2300 - total flux cleaned = 0.00119575 Jy ! Component: 2350 - total flux cleaned = 0.00136248 Jy ! Component: 2400 - total flux cleaned = 0.00136246 Jy ! Component: 2450 - total flux cleaned = 0.00136249 Jy ! Component: 2500 - total flux cleaned = 0.00133518 Jy ! Component: 2550 - total flux cleaned = 0.00147131 Jy ! Component: 2600 - total flux cleaned = 0.00155267 Jy ! Component: 2650 - total flux cleaned = 0.00155263 Jy ! Component: 2700 - total flux cleaned = 0.0016331 Jy ! Component: 2750 - total flux cleaned = 0.00181978 Jy ! Component: 2800 - total flux cleaned = 0.00168701 Jy ! Component: 2850 - total flux cleaned = 0.00184566 Jy ! Component: 2900 - total flux cleaned = 0.00187228 Jy ! Component: 2950 - total flux cleaned = 0.00202935 Jy ! Component: 3000 - total flux cleaned = 0.00202915 Jy ! Component: 3050 - total flux cleaned = 0.00213291 Jy ! Component: 3100 - total flux cleaned = 0.00226174 Jy ! Component: 3150 - total flux cleaned = 0.00213342 Jy ! Component: 3200 - total flux cleaned = 0.00221013 Jy ! Component: 3250 - total flux cleaned = 0.00233722 Jy ! Component: 3300 - total flux cleaned = 0.00228667 Jy ! Component: 3350 - total flux cleaned = 0.00243802 Jy ! Component: 3400 - total flux cleaned = 0.00241289 Jy ! Component: 3450 - total flux cleaned = 0.0024628 Jy ! Component: 3500 - total flux cleaned = 0.00258744 Jy ! Component: 3550 - total flux cleaned = 0.0025378 Jy ! Component: 3600 - total flux cleaned = 0.00256246 Jy ! Component: 3650 - total flux cleaned = 0.00253796 Jy ! Component: 3700 - total flux cleaned = 0.00256246 Jy ! Component: 3750 - total flux cleaned = 0.00263554 Jy ! Component: 3800 - total flux cleaned = 0.00261163 Jy ! Component: 3850 - total flux cleaned = 0.00270835 Jy ! Component: 3900 - total flux cleaned = 0.00280465 Jy ! Component: 3950 - total flux cleaned = 0.00278065 Jy ! Component: 4000 - total flux cleaned = 0.00280448 Jy ! Component: 4050 - total flux cleaned = 0.00275687 Jy ! Total flux subtracted in 4096 components = 0.00289894 Jy ! Clean residual min=-0.001399 max=0.001397 Jy/beam ! Clean residual mean=-0.000002 rms=0.000379 Jy/beam ! Combined flux in latest and established models = 0.489557 Jy keep ! Adding 332 model components to the UV plane model. ! The established model now contains 462 components and 0.489557 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1058+8114_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6402 x 0.7224 at 79.3 degrees (North through East) ! Clean map min=-0.0018596 max=0.3035 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1058+8114_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.303498 invert ! Inverting map ! Your choice of large map pixels excluded 9.14% of the data. ! The x-axis pixel size should ideally be below 0.1743 milli-arcsec ! The y-axis pixel size should ideally be below 0.1608 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000377883 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.373528 0.373528 0.747057 1.49411 2.98823 5.97646 11.9529 23.9058 47.8116 95.6233 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0011 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.303 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 803.151 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1058+8114_X_uvs.log closed on Sat Dec 26 09:36:51 2015