! Started logfile: /scr/pima/gb073_uvs/J1619+5256_X_uvs.log on Sat Dec 26 09:42:29 2015 obs /scr/pima/gb073_uvs/J1619+5256_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1619+5256_X_uva.fits ! AN table 1: 11 integrations on 45 of 45 possible baselines. ! AN table 2: 15 integrations on 78 of 78 possible baselines. ! AN table 3: 10 integrations on 66 of 66 possible baselines. ! AN table 4: 8 integrations on 36 of 36 possible baselines. ! AN table 5: 11 integrations on 55 of 55 possible baselines. ! AN table 6: 14 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.840898 visibilities/baseline/integration-bin. ! Found source: J1619+5256 ! ! 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 27864 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/J1619+5256_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 15 telescope corrections were flagged in sub-array 1. ! A total of 25 telescope corrections were flagged in sub-array 2. ! A total of 13 telescope corrections were flagged in sub-array 3. ! A total of 8 telescope corrections were flagged in sub-array 4. ! A total of 15 telescope corrections were flagged in sub-array 5. ! A total of 19 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 15 telescope corrections were flagged in sub-array 1. ! A total of 25 telescope corrections were flagged in sub-array 2. ! A total of 13 telescope corrections were flagged in sub-array 3. ! A total of 8 telescope corrections were flagged in sub-array 4. ! A total of 15 telescope corrections were flagged in sub-array 5. ! A total of 19 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 15 telescope corrections were flagged in sub-array 1. ! A total of 25 telescope corrections were flagged in sub-array 2. ! A total of 13 telescope corrections were flagged in sub-array 3. ! A total of 8 telescope corrections were flagged in sub-array 4. ! A total of 15 telescope corrections were flagged in sub-array 5. ! A total of 19 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 15 telescope corrections were flagged in sub-array 1. ! A total of 25 telescope corrections were flagged in sub-array 2. ! A total of 13 telescope corrections were flagged in sub-array 3. ! A total of 8 telescope corrections were flagged in sub-array 4. ! A total of 15 telescope corrections were flagged in sub-array 5. ! A total of 19 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 5. ! A total of 26 telescope corrections were flagged in sub-array 1. ! A total of 39 telescope corrections were flagged in sub-array 2. ! A total of 23 telescope corrections were flagged in sub-array 3. ! A total of 16 telescope corrections were flagged in sub-array 4. ! A total of 26 telescope corrections were flagged in sub-array 5. ! A total of 33 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 6. ! A total of 26 telescope corrections were flagged in sub-array 1. ! A total of 39 telescope corrections were flagged in sub-array 2. ! A total of 23 telescope corrections were flagged in sub-array 3. ! A total of 16 telescope corrections were flagged in sub-array 4. ! A total of 26 telescope corrections were flagged in sub-array 5. ! A total of 33 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 7. ! A total of 15 telescope corrections were flagged in sub-array 1. ! A total of 25 telescope corrections were flagged in sub-array 2. ! A total of 13 telescope corrections were flagged in sub-array 3. ! A total of 8 telescope corrections were flagged in sub-array 4. ! A total of 15 telescope corrections were flagged in sub-array 5. ! A total of 19 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 8. ! A total of 15 telescope corrections were flagged in sub-array 1. ! A total of 25 telescope corrections were flagged in sub-array 2. ! A total of 13 telescope corrections were flagged in sub-array 3. ! A total of 8 telescope corrections were flagged in sub-array 4. ! A total of 15 telescope corrections were flagged in sub-array 5. ! A total of 19 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.014059Jy sigma=9.040123 ! Fit after self-cal, rms=0.894536Jy sigma=7.974071 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec ! Estimated beam: bmin=0.4622 mas, bmaj=0.8068 mas, bpa=21.82 degrees ! Estimated noise=1.14568 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 = 0.0834197 Jy ! Component: 100 - total flux cleaned = 0.102522 Jy ! Total flux subtracted in 100 components = 0.102522 Jy ! Clean residual min=-0.004056 max=0.007447 Jy/beam ! Clean residual mean=-0.000002 rms=0.000930 Jy/beam ! Combined flux in latest and established models = 0.102522 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.102522 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=0.103474Jy sigma=0.690238 ! Fit after self-cal, rms=0.103317Jy sigma=0.689306 ! Inverting map ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0085428 Jy ! Component: 100 - total flux cleaned = 0.013192 Jy ! Total flux subtracted in 100 components = 0.013192 Jy ! Clean residual min=-0.003889 max=0.004188 Jy/beam ! Clean residual mean=0.000000 rms=0.000868 Jy/beam ! Combined flux in latest and established models = 0.115714 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 8 components and 0.115714 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=0.102397Jy sigma=0.677536 ! Fit after self-cal, rms=0.102401Jy sigma=0.677420 ! Inverting map ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec print "************** FINISHED UNIFORM WEIGHTING CLEAN **************" ! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** ! uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. win_mult = win_mult * 1.6 clean_niter = clean_niter * 2 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec ! Estimated beam: bmin=0.6201 mas, bmaj=1.008 mas, bpa=23.75 degrees ! Estimated noise=0.555873 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, 2.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00684115 Jy ! Component: 100 - total flux cleaned = 0.0107393 Jy ! Component: 150 - total flux cleaned = 0.0132923 Jy ! Component: 200 - total flux cleaned = 0.0149939 Jy ! Total flux subtracted in 200 components = 0.0149939 Jy ! Clean residual min=-0.002347 max=0.003309 Jy/beam ! Clean residual mean=0.000001 rms=0.000492 Jy/beam ! Combined flux in latest and established models = 0.130708 Jy ! Performing phase self-cal ! Adding 36 model components to the UV plane model. ! The established model now contains 41 components and 0.130708 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=0.101983Jy sigma=0.671577 ! Fit after self-cal, rms=0.101931Jy sigma=0.670691 ! Inverting map ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6201 x 1.008 at 23.75 degrees (North through East) ! Clean map min=-0.0017327 max=0.10717 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 EF 1.00* FD 0.88 KP 0.98 ! LA 1.02 MC 0.96 NL 0.93 OV 1.06 ! PT 0.93 ZC 0.80 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.95 EF 1.00* FD 1.04 KP 0.98 ! LA 1.08 MC 0.94 MK 1.00 NL 1.00 ! ON 0.91 OV 1.02 PT 0.97 SC 1.04 ! ZC 0.80 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 EF 1.00* FD 1.03 KP 0.91 ! LA 1.12 MC 0.96 NL 0.96 ON 0.81 ! OV 0.90 PT 0.93 SC 0.98 ZC 0.83 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.84 EF 1.00* KP 1.09 LA 1.12 ! MC 0.86 NL 0.91 ON 0.93 PT 1.01 ! ZC 0.79 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.94 EF 1.00* FD 0.92 KP 1.04 ! LA 1.02 MC 0.98 NL 0.97 ON 0.96 ! PT 0.94 SC 0.95 ZC 0.74 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.94 EF 1.00* FD 1.01 KP 1.01 ! LA 1.07 MC 1.10 MK 0.90 NL 0.91 ! ON 0.77 OV 1.07 PT 0.92 ZC 0.83 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.08 EF 1.00* FD 1.01 KP 1.01 ! LA 1.03 MC 1.00 NL 0.93 OV 1.22 ! PT 0.99 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.91 EF 1.00* FD 1.03 KP 1.05 ! LA 1.08 MC 0.91 MK 1.08 NL 1.00 ! ON 0.83 OV 1.09 PT 1.01 SC 0.97 ! ZC 0.87 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 EF 1.00* FD 1.04 KP 1.00 ! LA 0.98 MC 0.87 NL 0.97 ON 1.07 ! OV 1.08 PT 0.99 SC 1.03 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 EF 1.00* KP 1.08 LA 1.09 ! MC 0.78 NL 1.00 ON 0.90 PT 1.04 ! ZC 0.91 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 EF 1.00* FD 1.04 KP 0.98 ! LA 1.04 MC 1.04 NL 0.98 ON 1.01 ! PT 1.10 SC 0.93 ZC 0.74 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.92 EF 1.00* FD 1.03 KP 0.97 ! LA 1.05 MC 1.01 MK 0.98 NL 1.04 ! ON 0.89 OV 1.07 PT 1.04 ZC 0.87 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 EF 1.00* FD 0.96 KP 0.99 ! LA 0.93 MC 1.12 NL 0.92 OV 1.02 ! PT 0.98 ZC 0.75 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.94 EF 1.00* FD 0.97 KP 0.94 ! LA 1.05 MC 1.11 MK 1.08 NL 1.05 ! ON 0.86 OV 1.02 PT 0.99 SC 1.08 ! ZC 0.80 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 EF 1.00* FD 1.01 KP 0.92 ! LA 0.96 MC 0.91 NL 0.94 ON 1.11 ! OV 1.03 PT 1.00 SC 1.10 ZC 0.79 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.94 EF 1.00* KP 0.90 LA 1.00 ! MC 0.87 NL 0.97 ON 0.80 PT 0.99 ! ZC 0.91 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 EF 1.00* FD 1.03 KP 0.90 ! LA 1.01 MC 0.92 NL 0.89 ON 1.08 ! PT 1.00 SC 1.02 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.99 EF 1.00* FD 0.94 KP 0.96 ! LA 1.05 MC 1.07 MK 0.91 NL 0.95 ! ON 0.78 OV 0.98 PT 0.96 ZC 0.96 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 EF 1.00* FD 1.08 KP 1.02 ! LA 1.02 MC 1.11 NL 0.97 OV 1.06 ! PT 0.99 ZC 0.82 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 EF 1.00* FD 1.01 KP 1.00 ! LA 0.98 MC 1.16 MK 1.02 NL 1.03 ! ON 1.02 OV 1.01 PT 1.02 SC 1.26 ! ZC 0.87 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 EF 1.00* FD 1.18 KP 0.97 ! LA 1.01 MC 1.05 NL 0.94 ON 1.02 ! OV 0.96 PT 1.02 SC 1.03 ZC 0.84 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.95 EF 1.00* KP 0.95 LA 1.03 ! MC 0.80 NL 0.96 ON 0.82 PT 1.06 ! ZC 0.99 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.93 EF 1.00* FD 1.06 KP 1.01 ! LA 1.02 MC 1.08 NL 0.93 ON 1.06 ! PT 1.05 SC 0.95 ZC 0.79 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.95 EF 1.00* FD 1.04 KP 0.96 ! LA 0.97 MC 1.03 MK 0.98 NL 0.95 ! ON 0.84 OV 1.00 PT 1.02 ZC 0.93 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.06 KP 0.78 ! LA 0.94 MC 1.13 NL 1.10 OV 1.16 ! PT 1.04 ZC 0.91 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.03 KP 0.90 ! LA 1.01 MC 1.28 MK 1.04 NL 1.16 ! ON 1.45 OV 1.09 PT 0.98 SC 0.98 ! ZC 0.83 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 0.97 KP 0.87 ! LA 1.08 MC 1.16 NL 0.97 ON 1.15 ! OV 1.17 PT 0.93 SC 0.96 ZC 0.91 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* KP 0.80 LA 1.20 ! MC 1.04 NL 0.96 ON 1.32 PT 0.87 ! ZC 0.87 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.01 KP 0.89 ! LA 0.90 MC 1.29 NL 0.95 ON 1.20 ! PT 0.98 SC 1.20 ZC 0.86 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 0.99 KP 0.84 ! LA 1.02 MC 1.51 MK 1.08 NL 0.96 ! ON 1.01 OV 1.04 PT 1.00 ZC 0.91 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.04 KP 0.94 ! LA 0.99 MC 1.21 NL 1.05 OV 1.15 ! PT 0.96 ZC 0.87 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 0.92 KP 0.90 ! LA 1.05 MC 1.19 MK 1.13 NL 1.10 ! ON 1.20 OV 1.07 PT 0.94 SC 1.12 ! ZC 0.88 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.06 KP 0.92 ! LA 0.94 MC 1.38 NL 0.92 ON 1.17 ! OV 1.03 PT 0.95 SC 1.07 ZC 0.83 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* KP 0.87 LA 1.01 ! MC 1.13 NL 1.00 ON 1.23 PT 0.93 ! ZC 0.94 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.12 KP 0.94 ! LA 0.93 MC 1.26 NL 0.93 ON 1.25 ! PT 0.96 SC 1.07 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 0.96 KP 0.88 ! LA 0.99 MC 1.58 MK 1.06 NL 1.02 ! ON 0.96 OV 1.01 PT 0.91 ZC 0.86 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 EF 1.00* FD 1.05 KP 0.91 ! LA 1.05 MC 1.62 NL 0.93 OV 0.98 ! PT 1.03 ZC 0.64 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 EF 1.00* FD 0.93 KP 0.88 ! LA 1.06 MC 1.35 MK 1.11 NL 1.24 ! ON 1.47 OV 1.02 PT 1.01 SC 1.17 ! ZC 0.71 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 EF 1.00* FD 1.13 KP 0.94 ! LA 1.05 MC 1.18 NL 1.08 ON 1.47 ! OV 1.04 PT 0.91 SC 1.06 ZC 0.72 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 EF 1.00* KP 0.94 LA 1.06 ! MC 1.25 NL 1.04 ON 1.24 PT 1.15 ! ZC 0.66 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 EF 1.00* FD 1.03 KP 1.03 ! LA 0.97 MC 1.44 NL 1.04 ON 1.20 ! PT 0.93 SC 1.08 ZC 0.63 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.95 EF 1.00* FD 1.01 KP 0.99 ! LA 1.04 MC 1.39 MK 1.01 NL 1.05 ! ON 1.04 OV 1.03 PT 0.99 ZC 0.72 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 0.95 EF 1.00* FD 1.04 KP 0.97 ! LA 1.23 MC 1.33 NL 1.00 OV 1.06 ! PT 0.99 ZC 0.54 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.08 EF 1.00* FD 1.00 KP 0.92 ! LA 1.01 MC 1.40 MK 1.13 NL 1.07 ! ON 1.35 OV 1.02 PT 1.00 SC 1.11 ! ZC 0.63 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 EF 1.00* FD 1.14 KP 0.93 ! LA 1.01 MC 1.14 NL 1.01 ON 0.99 ! OV 1.01 PT 1.01 SC 1.03 ZC 0.66 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.18 EF 1.00* KP 1.02 LA 1.12 ! MC 1.18 NL 1.00 ON 0.98 PT 1.04 ! ZC 0.74 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 EF 1.00* FD 0.90 KP 1.02 ! LA 1.12 MC 1.26 NL 0.97 ON 1.25 ! PT 1.01 SC 1.09 ZC 0.53 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.96 EF 1.00* FD 1.02 KP 0.91 ! LA 1.10 MC 1.19 MK 0.97 NL 1.06 ! ON 1.22 OV 1.00 PT 1.09 ZC 0.74 ! ! ! Fit before self-cal, rms=0.101931Jy sigma=0.670691 ! Fit after self-cal, rms=0.102514Jy sigma=0.657146 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec ! Estimated beam: bmin=0.6163 mas, bmaj=1.008 mas, bpa=23.1 degrees ! Estimated noise=0.555837 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 = 0.00175226 Jy ! Component: 100 - total flux cleaned = 0.00239222 Jy ! Component: 150 - total flux cleaned = 0.00247076 Jy ! Component: 200 - total flux cleaned = 0.00249233 Jy ! Total flux subtracted in 200 components = 0.00249233 Jy ! Clean residual min=-0.001690 max=0.001677 Jy/beam ! Clean residual mean=0.000000 rms=0.000366 Jy/beam ! Combined flux in latest and established models = 0.133201 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 59 components and 0.133201 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=0.102477Jy sigma=0.656821 ! Fit after self-cal, rms=0.102601Jy sigma=0.656385 ! Inverting map ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 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=0.102601Jy sigma=0.656385 ! Fit after self-cal, rms=0.102851Jy sigma=0.656312 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec ! Estimated beam: bmin=0.6154 mas, bmaj=1.007 mas, bpa=23.07 degrees ! Estimated noise=0.556826 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00110917 Jy ! Component: 100 - total flux cleaned = 0.00147647 Jy ! Component: 150 - total flux cleaned = 0.00159214 Jy ! Component: 200 - total flux cleaned = 0.00162543 Jy ! Total flux subtracted in 200 components = 0.00162543 Jy ! Clean residual min=-0.001647 max=0.001623 Jy/beam ! Clean residual mean=0.000000 rms=0.000359 Jy/beam ! Combined flux in latest and established models = 0.134826 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 64 components and 0.134826 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=0.102834Jy sigma=0.656191 ! Fit after self-cal, rms=0.102838Jy sigma=0.656163 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 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 = 0.00039741 Jy ! Component: 100 - total flux cleaned = 0.000430256 Jy ! Component: 150 - total flux cleaned = 0.000445314 Jy ! Component: 200 - total flux cleaned = 0.000445207 Jy ! Total flux subtracted in 200 components = 0.000445207 Jy ! Clean residual min=-0.001645 max=0.001592 Jy/beam ! Clean residual mean=0.000000 rms=0.000358 Jy/beam ! Combined flux in latest and established models = 0.135271 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 67 components and 0.135271 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=0.102832Jy sigma=0.656127 ! Fit after self-cal, rms=0.102832Jy sigma=0.656123 ! Inverting map ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 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=0.102832Jy sigma=0.656123 ! Fit after self-cal, rms=0.102883Jy sigma=0.656079 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec ! Estimated beam: bmin=0.6146 mas, bmaj=1.007 mas, bpa=23.07 degrees ! Estimated noise=0.55775 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000680407 Jy ! Component: 100 - total flux cleaned = 0.000919352 Jy ! Component: 150 - total flux cleaned = 0.000947382 Jy ! Component: 200 - total flux cleaned = 0.000960308 Jy ! Total flux subtracted in 200 components = 0.000960308 Jy ! Clean residual min=-0.001620 max=0.001566 Jy/beam ! Clean residual mean=0.000000 rms=0.000356 Jy/beam ! Combined flux in latest and established models = 0.136232 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 68 components and 0.136232 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=0.102876Jy sigma=0.656048 ! Fit after self-cal, rms=0.102876Jy sigma=0.656041 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 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 = 0.000178821 Jy ! Component: 100 - total flux cleaned = 0.000191788 Jy ! Component: 150 - total flux cleaned = 0.000203905 Jy ! Component: 200 - total flux cleaned = 0.000204083 Jy ! Total flux subtracted in 200 components = 0.000204083 Jy ! Clean residual min=-0.001620 max=0.001560 Jy/beam ! Clean residual mean=0.000000 rms=0.000355 Jy/beam ! Combined flux in latest and established models = 0.136436 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 69 components and 0.136436 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=0.102871Jy sigma=0.656019 ! Fit after self-cal, rms=0.102871Jy sigma=0.656018 ! Inverting map ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 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=0.102871Jy sigma=0.656018 ! Fit after self-cal, rms=0.102984Jy sigma=0.655998 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec ! Estimated beam: bmin=2.714 mas, bmaj=3.456 mas, bpa=-77.23 degrees ! Estimated noise=0.70386 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000530749 Jy ! Component: 100 - total flux cleaned = 0.000588483 Jy ! Component: 150 - total flux cleaned = 0.000595257 Jy ! Component: 200 - total flux cleaned = 0.000601373 Jy ! Total flux subtracted in 200 components = 0.000601373 Jy ! Clean residual min=-0.002063 max=0.001723 Jy/beam ! Clean residual mean=0.000000 rms=0.000468 Jy/beam ! Combined flux in latest and established models = 0.137037 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 73 components and 0.137037 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=0.102983Jy sigma=0.656009 ! Fit after self-cal, rms=0.102982Jy sigma=0.656006 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 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 = 9.97762e-05 Jy ! Component: 100 - total flux cleaned = 0.000115644 Jy ! Component: 150 - total flux cleaned = 0.000122626 Jy ! Component: 200 - total flux cleaned = 0.000134236 Jy ! Total flux subtracted in 200 components = 0.000134236 Jy ! Clean residual min=-0.002046 max=0.001710 Jy/beam ! Clean residual mean=0.000000 rms=0.000468 Jy/beam ! Combined flux in latest and established models = 0.137171 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 73 components and 0.137171 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=0.102983Jy sigma=0.656010 ! Fit after self-cal, rms=0.102984Jy sigma=0.656009 ! Inverting map ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "************** FINISHED AMPLITUDE SELF-CAL **************" ! ************** FINISHED AMPLITUDE SELF-CAL ************** restore ! Inverting map and beam ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec ! Estimated beam: bmin=0.6138 mas, bmaj=1.007 mas, bpa=23.07 degrees ! Estimated noise=0.558984 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6138 x 1.007 at 23.07 degrees (North through East) ! Clean map min=-0.0013723 max=0.10713 Jy/beam if(peak(flux) > thresh) selfcal true, true clean clean_niter,clean_gain selfcal flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) selfcal true, true end if print "************** CLEARING MODEL AND STARTING OVER **********" ! ************** CLEARING MODEL AND STARTING OVER ********** clrmod true ! clrmod: Cleared the established and tentative models. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec ! Estimated beam: bmin=0.4552 mas, bmaj=0.803 mas, bpa=21.29 degrees ! Estimated noise=1.14444 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0832114 Jy ! Component: 100 - total flux cleaned = 0.102758 Jy ! Component: 150 - total flux cleaned = 0.110738 Jy ! Component: 200 - total flux cleaned = 0.116005 Jy ! Total flux subtracted in 200 components = 0.116005 Jy ! Clean residual min=-0.003429 max=0.003396 Jy/beam ! Clean residual mean=-0.000001 rms=0.000765 Jy/beam ! Combined flux in latest and established models = 0.116005 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 20 model components to the UV plane model. ! The established model now contains 20 components and 0.116005 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec ! Estimated beam: bmin=0.6138 mas, bmaj=1.007 mas, bpa=23.07 degrees ! Estimated noise=0.558984 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 = 0.00765572 Jy ! Component: 100 - total flux cleaned = 0.0122562 Jy ! Component: 150 - total flux cleaned = 0.0152009 Jy ! Component: 200 - total flux cleaned = 0.0171383 Jy ! Total flux subtracted in 200 components = 0.0171383 Jy ! Clean residual min=-0.001759 max=0.001486 Jy/beam ! Clean residual mean=-0.000004 rms=0.000364 Jy/beam ! Combined flux in latest and established models = 0.133144 Jy ! Adding 34 model components to the UV plane model. ! The established model now contains 45 components and 0.133144 Jy ! Inverting map ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec ! Estimated beam: bmin=2.714 mas, bmaj=3.456 mas, bpa=-77.23 degrees ! Estimated noise=0.70386 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00195664 Jy ! Component: 100 - total flux cleaned = 0.00285202 Jy ! Component: 150 - total flux cleaned = 0.0033251 Jy ! Component: 200 - total flux cleaned = 0.00357971 Jy ! Total flux subtracted in 200 components = 0.00357971 Jy ! Clean residual min=-0.002058 max=0.001725 Jy/beam ! Clean residual mean=-0.000001 rms=0.000467 Jy/beam ! Combined flux in latest and established models = 0.136723 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 = 0.000137457 Jy ! Component: 100 - total flux cleaned = 0.000156467 Jy ! Component: 150 - total flux cleaned = 0.000174193 Jy ! Component: 200 - total flux cleaned = 0.000184272 Jy ! Total flux subtracted in 200 components = 0.000184272 Jy ! Clean residual min=-0.002053 max=0.001726 Jy/beam ! Clean residual mean=-0.000000 rms=0.000467 Jy/beam ! Combined flux in latest and established models = 0.136908 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 67 components and 0.136908 Jy ! Inverting map ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec ! Estimated beam: bmin=0.6138 mas, bmaj=1.007 mas, bpa=23.07 degrees ! Estimated noise=0.558984 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 5.37973e-05 Jy ! Component: 100 - total flux cleaned = 3.87489e-05 Jy ! Component: 150 - total flux cleaned = 3.91421e-05 Jy ! Component: 200 - total flux cleaned = 5.2795e-05 Jy ! Total flux subtracted in 200 components = 5.2795e-05 Jy ! Clean residual min=-0.001639 max=0.001582 Jy/beam ! Clean residual mean=-0.000000 rms=0.000353 Jy/beam ! Combined flux in latest and established models = 0.136961 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 75 components and 0.136961 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=0.102980Jy sigma=0.656042 ! Fit after self-cal, rms=0.102975Jy sigma=0.655994 wmodel /scr/pima/gb073_uvs/J1619+5256_X_map.mod ! Writing 75 model components to file: /scr/pima/gb073_uvs/J1619+5256_X_map.mod wobs /scr/pima/gb073_uvs/J1619+5256_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1619+5256_X_uvs.fits wwins /scr/pima/gb073_uvs/J1619+5256_X_map.win ! wwins: Wrote 2 windows to /scr/pima/gb073_uvs/J1619+5256_X_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000245995 Jy ! Component: 100 - total flux cleaned = -0.000217576 Jy ! Component: 150 - total flux cleaned = -8.26537e-05 Jy ! Component: 200 - total flux cleaned = 4.82112e-05 Jy ! Component: 250 - total flux cleaned = 0.000202421 Jy ! Component: 300 - total flux cleaned = 0.000253234 Jy ! Component: 350 - total flux cleaned = 0.000327785 Jy ! Component: 400 - total flux cleaned = 0.000376526 Jy ! Component: 450 - total flux cleaned = 0.000376446 Jy ! Component: 500 - total flux cleaned = 0.000281472 Jy ! Component: 550 - total flux cleaned = 0.000281877 Jy ! Component: 600 - total flux cleaned = 0.000258344 Jy ! Component: 650 - total flux cleaned = 0.000212424 Jy ! Component: 700 - total flux cleaned = 0.000257766 Jy ! Component: 750 - total flux cleaned = 0.00019054 Jy ! Component: 800 - total flux cleaned = 0.000146306 Jy ! Component: 850 - total flux cleaned = 0.000212353 Jy ! Component: 900 - total flux cleaned = 0.000124991 Jy ! Component: 950 - total flux cleaned = 0.000103297 Jy ! Component: 1000 - total flux cleaned = 8.19101e-05 Jy ! Component: 1050 - total flux cleaned = 0.000103421 Jy ! Component: 1100 - total flux cleaned = 0.000124484 Jy ! Component: 1150 - total flux cleaned = 0.000145419 Jy ! Component: 1200 - total flux cleaned = 0.000124512 Jy ! Component: 1250 - total flux cleaned = 0.00012431 Jy ! Component: 1300 - total flux cleaned = 8.3374e-05 Jy ! Component: 1350 - total flux cleaned = 6.29994e-05 Jy ! Component: 1400 - total flux cleaned = 0.000144135 Jy ! Component: 1450 - total flux cleaned = 0.000143927 Jy ! Component: 1500 - total flux cleaned = 0.000183704 Jy ! Component: 1550 - total flux cleaned = 0.00016382 Jy ! Component: 1600 - total flux cleaned = 0.000223034 Jy ! Component: 1650 - total flux cleaned = 0.000223057 Jy ! Component: 1700 - total flux cleaned = 0.000223045 Jy ! Component: 1750 - total flux cleaned = 0.000300802 Jy ! Component: 1800 - total flux cleaned = 0.000300715 Jy ! Component: 1850 - total flux cleaned = 0.000262306 Jy ! Component: 1900 - total flux cleaned = 0.000300746 Jy ! Component: 1950 - total flux cleaned = 0.00039602 Jy ! Component: 2000 - total flux cleaned = 0.00035817 Jy ! Component: 2050 - total flux cleaned = 0.000282488 Jy ! Component: 2100 - total flux cleaned = 0.00028243 Jy ! Component: 2150 - total flux cleaned = 0.000245075 Jy ! Component: 2200 - total flux cleaned = 0.000263747 Jy ! Component: 2250 - total flux cleaned = 0.000226747 Jy ! Component: 2300 - total flux cleaned = 0.000189611 Jy ! Component: 2350 - total flux cleaned = 0.000226342 Jy ! Component: 2400 - total flux cleaned = 0.000262998 Jy ! Component: 2450 - total flux cleaned = 0.000189939 Jy ! Component: 2500 - total flux cleaned = 0.00011709 Jy ! Component: 2550 - total flux cleaned = 0.000153397 Jy ! Component: 2600 - total flux cleaned = 9.92606e-05 Jy ! Component: 2650 - total flux cleaned = 6.33614e-05 Jy ! Component: 2700 - total flux cleaned = 0.00011715 Jy ! Component: 2750 - total flux cleaned = 9.94151e-05 Jy ! Component: 2800 - total flux cleaned = 9.93953e-05 Jy ! Component: 2850 - total flux cleaned = 1.10127e-05 Jy ! Component: 2900 - total flux cleaned = 9.91598e-05 Jy ! Component: 2950 - total flux cleaned = 9.91323e-05 Jy ! Component: 3000 - total flux cleaned = 0.000186639 Jy ! Component: 3050 - total flux cleaned = 0.000169232 Jy ! Component: 3100 - total flux cleaned = 0.000151905 Jy ! Component: 3150 - total flux cleaned = 8.24714e-05 Jy ! Component: 3200 - total flux cleaned = 0.000151443 Jy ! Component: 3250 - total flux cleaned = 0.000185827 Jy ! Component: 3300 - total flux cleaned = 0.000220081 Jy ! Component: 3350 - total flux cleaned = 0.000220005 Jy ! Component: 3400 - total flux cleaned = 0.000322108 Jy ! Component: 3450 - total flux cleaned = 0.000271245 Jy ! Component: 3500 - total flux cleaned = 0.000271143 Jy ! Component: 3550 - total flux cleaned = 0.000338513 Jy ! Component: 3600 - total flux cleaned = 0.000388894 Jy ! Component: 3650 - total flux cleaned = 0.000305298 Jy ! Component: 3700 - total flux cleaned = 0.000371976 Jy ! Component: 3750 - total flux cleaned = 0.000421787 Jy ! Component: 3800 - total flux cleaned = 0.000421743 Jy ! Component: 3850 - total flux cleaned = 0.000454796 Jy ! Component: 3900 - total flux cleaned = 0.000438331 Jy ! Component: 3950 - total flux cleaned = 0.000471179 Jy ! Component: 4000 - total flux cleaned = 0.000487555 Jy ! Component: 4050 - total flux cleaned = 0.000454877 Jy ! Total flux subtracted in 4096 components = 0.000454898 Jy ! Clean residual min=-0.000812 max=0.001024 Jy/beam ! Clean residual mean=-0.000000 rms=0.000264 Jy/beam ! Combined flux in latest and established models = 0.137415 Jy keep ! Adding 338 model components to the UV plane model. ! The established model now contains 413 components and 0.137415 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1619+5256_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6138 x 1.007 at 23.07 degrees (North through East) ! Clean map min=-0.0013138 max=0.10744 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1619+5256_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.107438 invert ! Inverting map ! Your choice of large map pixels excluded 5.06% of the data. ! The x-axis pixel size should ideally be below 0.1789 milli-arcsec ! The y-axis pixel size should ideally be below 0.1842 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000262867 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.734005 0.734005 1.46801 2.93602 5.87204 11.7441 23.4882 46.9763 93.9526 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0007 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.107 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 408.716 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1619+5256_X_uvs.log closed on Sat Dec 26 09:42:35 2015