! Started logfile: /scr/pima/gb073_uvs/J1608+6018_X_uvs.log on Sat Dec 26 09:42:14 2015 obs /scr/pima/gb073_uvs/J1608+6018_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1608+6018_X_uva.fits ! AN table 1: 29 integrations on 55 of 55 possible baselines. ! AN table 2: 29 integrations on 66 of 66 possible baselines. ! AN table 3: 29 integrations on 66 of 66 possible baselines. ! AN table 4: 29 integrations on 45 of 45 possible baselines. ! AN table 5: 29 integrations on 55 of 55 possible baselines. ! AN table 6: 29 integrations on 55 of 55 possible baselines. ! Apparent sampling: 0.825166 visibilities/baseline/integration-bin. ! Found source: J1608+6018 ! ! 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 65472 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/J1608+6018_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 59 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 42 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 59 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 42 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 59 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 42 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 59 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 42 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 5. ! A total of 88 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! A total of 71 telescope corrections were flagged in sub-array 5. ! A total of 58 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 6. ! A total of 88 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! A total of 71 telescope corrections were flagged in sub-array 5. ! A total of 58 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 7. ! A total of 59 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 42 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 8. ! A total of 59 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 42 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.006163Jy sigma=9.400012 ! Fit after self-cal, rms=0.936883Jy sigma=8.758281 ! 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 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec ! Estimated beam: bmin=0.4083 mas, bmaj=0.9303 mas, bpa=24.32 degrees ! Estimated noise=0.789667 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 = 0.046221 Jy ! Component: 100 - total flux cleaned = 0.0608788 Jy ! Total flux subtracted in 100 components = 0.0608788 Jy ! Clean residual min=-0.003890 max=0.007165 Jy/beam ! Clean residual mean=-0.000005 rms=0.000695 Jy/beam ! Combined flux in latest and established models = 0.0608788 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.0608788 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=0.084743Jy sigma=0.691634 ! Fit after self-cal, rms=0.083437Jy sigma=0.681206 ! Inverting map ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0108806 Jy ! Component: 100 - total flux cleaned = 0.0169879 Jy ! Total flux subtracted in 100 components = 0.0169879 Jy ! Clean residual min=-0.003487 max=0.004076 Jy/beam ! Clean residual mean=-0.000001 rms=0.000609 Jy/beam ! Combined flux in latest and established models = 0.0778667 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 6 components and 0.0778667 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=0.081676Jy sigma=0.662529 ! Fit after self-cal, rms=0.081521Jy sigma=0.661689 ! Inverting map ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00525959 Jy ! Component: 100 - total flux cleaned = 0.00578059 Jy ! Total flux subtracted in 100 components = 0.00578059 Jy ! Clean residual min=-0.003635 max=0.002880 Jy/beam ! Clean residual mean=0.000000 rms=0.000591 Jy/beam ! Combined flux in latest and established models = 0.0836473 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 10 components and 0.0836473 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=0.081247Jy sigma=0.659492 ! Fit after self-cal, rms=0.081177Jy sigma=0.659169 ! Inverting map ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 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 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec ! Estimated beam: bmin=0.6091 mas, bmaj=1.149 mas, bpa=24.77 degrees ! Estimated noise=0.348962 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 (-1.4, -4.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00182773 Jy ! Component: 100 - total flux cleaned = 0.00220063 Jy ! Component: 150 - total flux cleaned = 0.00237583 Jy ! Component: 200 - total flux cleaned = 0.00249215 Jy ! Total flux subtracted in 200 components = 0.00249215 Jy ! Clean residual min=-0.001749 max=0.001391 Jy/beam ! Clean residual mean=0.000005 rms=0.000275 Jy/beam ! Combined flux in latest and established models = 0.0861394 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 21 components and 0.0861394 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=0.081090Jy sigma=0.658505 ! Fit after self-cal, rms=0.081067Jy sigma=0.658411 ! Inverting map ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6091 x 1.149 at 24.77 degrees (North through East) ! Clean map min=-0.0012951 max=0.065212 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 0.82 EF 1.00* FD 0.91 KP 1.01 ! LA 1.15 MC 0.85 NL 1.01 OV 1.03 ! PT 1.00 SC 1.00* ZC 0.92 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.92 EF 1.00* FD 1.04 KP 1.07 ! LA 1.02 MC 0.75 MK 1.20 NL 0.95 ! ON 0.82 OV 1.04 PT 0.94 ZC 0.95 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 EF 1.00* FD 1.00 KP 1.03 ! LA 1.03 MC 1.06 NL 0.96 ON 0.93 ! OV 1.03 PT 1.04 SC 0.93 ZC 0.91 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.89 FD 0.92 KP 1.02 LA 1.06 ! MC 0.98 MK 1.08 NL 0.99 ON 0.99 ! PT 1.02 ZC 0.80 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 EF 1.00* FD 0.99 KP 1.00 ! LA 1.06 MC 0.95 NL 0.93 ON 1.01 ! PT 0.91 SC 0.94 ZC 0.91 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.93 EF 1.00* FD 0.95 KP 1.02 ! LA 1.04 MC 0.87 MK 1.13 NL 0.97 ! OV 1.03 PT 0.94 ZC 0.80 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.07 EF 1.00* FD 1.09 KP 1.09 ! LA 1.10 MC 0.98 NL 1.04 OV 1.02 ! PT 1.01 SC 1.00* ZC 0.85 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 EF 1.00* FD 0.97 KP 1.06 ! LA 1.02 MC 0.88 MK 1.18 NL 1.00 ! ON 0.79 OV 0.98 PT 1.00 ZC 1.01 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.08 EF 1.00* FD 1.06 KP 1.15 ! LA 1.01 MC 1.02 NL 0.96 ON 0.96 ! OV 0.99 PT 1.06 SC 0.91 ZC 0.92 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 FD 1.03 KP 1.05 LA 1.03 ! MC 0.98 MK 1.07 NL 0.98 ON 1.07 ! PT 1.00 ZC 0.83 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 EF 1.00* FD 1.07 KP 1.08 ! LA 1.04 MC 0.93 NL 0.92 ON 0.94 ! PT 1.03 SC 0.95 ZC 0.86 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 EF 1.00* FD 0.97 KP 0.97 ! LA 0.99 MC 0.92 MK 1.35 NL 0.98 ! OV 1.00 PT 0.97 ZC 0.84 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 EF 1.00* FD 0.96 KP 0.93 ! LA 1.03 MC 0.76 NL 0.96 OV 1.06 ! PT 1.07 SC 1.00* ZC 0.88 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 EF 1.00* FD 1.02 KP 1.03 ! LA 0.98 MC 0.79 MK 1.07 NL 0.98 ! ON 0.66 OV 1.01 PT 0.98 ZC 0.98 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 EF 1.00* FD 1.05 KP 0.98 ! LA 0.98 MC 0.90 NL 0.96 ON 1.02 ! OV 1.05 PT 1.09 SC 1.03 ZC 0.87 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 FD 1.13 KP 0.99 LA 0.98 ! MC 1.12 MK 0.96 NL 0.97 ON 0.97 ! PT 1.01 ZC 0.84 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.04 EF 1.00* FD 1.04 KP 0.99 ! LA 1.02 MC 0.98 NL 0.94 ON 1.15 ! PT 1.04 SC 0.92 ZC 0.86 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.94 EF 1.00* FD 0.97 KP 0.94 ! LA 1.05 MC 0.86 MK 1.07 NL 0.93 ! OV 0.90 PT 1.02 ZC 0.83 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 EF 1.00* FD 1.00 KP 1.05 ! LA 1.09 MC 0.84 NL 1.09 OV 1.05 ! PT 1.06 SC 1.00* ZC 0.86 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 EF 1.00* FD 0.93 KP 1.02 ! LA 1.00 MC 0.88 MK 0.97 NL 1.01 ! ON 0.77 OV 1.02 PT 1.05 ZC 0.93 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 EF 1.00* FD 1.09 KP 1.02 ! LA 1.02 MC 1.10 NL 0.95 ON 0.97 ! OV 1.05 PT 1.07 SC 0.98 ZC 0.76 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 FD 1.02 KP 0.97 LA 0.96 ! MC 1.11 MK 1.15 NL 0.94 ON 1.01 ! PT 1.10 ZC 0.79 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.05 EF 1.00* FD 1.09 KP 1.06 ! LA 0.97 MC 1.00 NL 1.00 ON 0.84 ! PT 0.97 SC 0.97 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00 EF 1.00* FD 1.03 KP 1.02 ! LA 0.93 MC 1.05 MK 0.97 NL 0.95 ! OV 0.99 PT 1.09 ZC 0.81 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.07 KP 0.97 ! LA 1.11 MC 1.02 NL 1.02 OV 1.09 ! PT 0.97 SC 1.00* ZC 0.82 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.07 KP 0.88 ! LA 1.00 MC 0.98 MK 1.17 NL 0.89 ! ON 0.94 OV 1.02 PT 1.11 ZC 0.92 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.08 KP 0.87 ! LA 1.03 MC 1.15 NL 1.07 ON 1.10 ! OV 1.07 PT 1.06 SC 0.99 ZC 0.90 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.03 KP 1.00 LA 1.07 ! MC 1.10 MK 1.04 NL 0.95 ON 1.19 ! PT 1.00 ZC 0.78 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 0.99 KP 0.89 ! LA 0.96 MC 1.24 NL 1.11 ON 1.24 ! PT 1.01 SC 0.99 ZC 0.79 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.07 KP 0.92 ! LA 0.99 MC 1.18 MK 1.08 NL 0.96 ! OV 1.01 PT 1.08 ZC 0.80 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.95 KP 0.89 ! LA 1.08 MC 0.99 NL 1.21 OV 0.98 ! PT 0.87 SC 1.00* ZC 0.86 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 0.99 KP 0.96 ! LA 1.02 MC 0.95 MK 1.13 NL 1.00 ! ON 0.98 OV 1.04 PT 0.96 ZC 0.87 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 0.96 KP 0.88 ! LA 1.13 MC 1.21 NL 0.95 ON 1.14 ! OV 1.07 PT 1.03 SC 1.03 ZC 0.83 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.12 KP 0.82 LA 0.99 ! MC 1.07 MK 1.03 NL 0.98 ON 1.39 ! PT 0.93 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.03 KP 0.89 ! LA 1.09 MC 1.12 NL 1.01 ON 1.32 ! PT 0.89 SC 0.95 ZC 0.86 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.05 KP 0.90 ! LA 0.98 MC 1.12 MK 0.88 NL 0.92 ! OV 1.12 PT 0.90 ZC 0.82 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 EF 1.00* FD 1.05 KP 0.89 ! LA 1.03 MC 0.83 NL 1.02 OV 1.16 ! PT 0.97 SC 1.00* ZC 0.74 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 EF 1.00* FD 1.08 KP 0.87 ! LA 0.99 MC 1.01 MK 1.05 NL 1.03 ! ON 0.85 OV 1.14 PT 0.97 ZC 0.82 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.10 EF 1.00* FD 1.04 KP 0.98 ! LA 1.08 MC 1.04 NL 1.05 ON 1.25 ! OV 0.99 PT 1.04 SC 1.02 ZC 0.78 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.09 FD 1.09 KP 0.90 LA 1.06 ! MC 1.21 MK 0.99 NL 1.10 ON 1.15 ! PT 1.02 ZC 0.67 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.04 EF 1.00* FD 1.05 KP 0.95 ! LA 1.04 MC 1.12 NL 1.04 ON 1.10 ! PT 0.97 SC 0.91 ZC 0.68 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.99 EF 1.00* FD 1.03 KP 0.99 ! LA 0.99 MC 1.24 MK 0.93 NL 0.95 ! OV 1.06 PT 1.01 ZC 0.74 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 0.93 EF 1.00* FD 1.01 KP 0.99 ! LA 1.01 MC 1.04 NL 1.09 OV 0.97 ! PT 0.97 SC 1.00* ZC 0.61 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 EF 1.00* FD 0.96 KP 0.95 ! LA 1.12 MC 1.13 MK 1.10 NL 0.99 ! ON 0.93 OV 0.99 PT 1.07 ZC 0.72 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 EF 1.00* FD 1.17 KP 0.93 ! LA 1.01 MC 1.01 NL 0.99 ON 1.14 ! OV 1.06 PT 1.04 SC 1.08 ZC 0.74 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.85 FD 0.96 KP 0.91 LA 1.03 ! MC 1.37 MK 1.02 NL 0.99 ON 1.26 ! PT 0.99 ZC 0.66 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.89 EF 1.00* FD 1.05 KP 0.95 ! LA 1.01 MC 1.22 NL 1.12 ON 1.06 ! PT 0.98 SC 0.99 ZC 0.70 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.99 EF 1.00* FD 1.05 KP 0.91 ! LA 1.02 MC 1.03 MK 1.13 NL 1.01 ! OV 1.03 PT 1.00 ZC 0.63 ! ! ! Fit before self-cal, rms=0.081067Jy sigma=0.658411 ! Fit after self-cal, rms=0.079252Jy sigma=0.653224 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec ! Estimated beam: bmin=0.5991 mas, bmaj=1.144 mas, bpa=23.87 degrees ! Estimated noise=0.347758 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 = 0.000945759 Jy ! Component: 100 - total flux cleaned = 0.00130811 Jy ! Component: 150 - total flux cleaned = 0.00142145 Jy ! Component: 200 - total flux cleaned = 0.00148854 Jy ! Total flux subtracted in 200 components = 0.00148854 Jy ! Clean residual min=-0.000959 max=0.000908 Jy/beam ! Clean residual mean=0.000002 rms=0.000215 Jy/beam ! Combined flux in latest and established models = 0.087628 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 32 components and 0.087628 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=0.079233Jy sigma=0.653046 ! Fit after self-cal, rms=0.079343Jy sigma=0.652510 ! Inverting map ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 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=0.079343Jy sigma=0.652510 ! Fit after self-cal, rms=0.080077Jy sigma=0.652427 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec ! Estimated beam: bmin=0.597 mas, bmaj=1.145 mas, bpa=23.75 degrees ! Estimated noise=0.349751 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000833481 Jy ! Component: 100 - total flux cleaned = 0.000915955 Jy ! Component: 150 - total flux cleaned = 0.000950982 Jy ! Component: 200 - total flux cleaned = 0.000998066 Jy ! Total flux subtracted in 200 components = 0.000998066 Jy ! Clean residual min=-0.000934 max=0.000902 Jy/beam ! Clean residual mean=0.000002 rms=0.000214 Jy/beam ! Combined flux in latest and established models = 0.0886261 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 33 components and 0.0886261 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=0.080062Jy sigma=0.652285 ! Fit after self-cal, rms=0.080096Jy sigma=0.652243 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 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 = 0.000156971 Jy ! Component: 100 - total flux cleaned = 0.000140622 Jy ! Component: 150 - total flux cleaned = 0.000183914 Jy ! Component: 200 - total flux cleaned = 0.000210432 Jy ! Total flux subtracted in 200 components = 0.000210432 Jy ! Clean residual min=-0.000931 max=0.000926 Jy/beam ! Clean residual mean=0.000002 rms=0.000214 Jy/beam ! Combined flux in latest and established models = 0.0888365 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 37 components and 0.0888365 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=0.080089Jy sigma=0.652165 ! Fit after self-cal, rms=0.080091Jy sigma=0.652154 ! Inverting map ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 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=0.080091Jy sigma=0.652154 ! Fit after self-cal, rms=0.080499Jy sigma=0.652121 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec ! Estimated beam: bmin=0.5948 mas, bmaj=1.146 mas, bpa=23.69 degrees ! Estimated noise=0.351632 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000624051 Jy ! Component: 100 - total flux cleaned = 0.00077804 Jy ! Component: 150 - total flux cleaned = 0.000814268 Jy ! Component: 200 - total flux cleaned = 0.000837272 Jy ! Total flux subtracted in 200 components = 0.000837272 Jy ! Clean residual min=-0.000949 max=0.000907 Jy/beam ! Clean residual mean=0.000003 rms=0.000213 Jy/beam ! Combined flux in latest and established models = 0.0896738 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 37 components and 0.0896738 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=0.080490Jy sigma=0.652043 ! Fit after self-cal, rms=0.080498Jy sigma=0.652030 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 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 = 9.05308e-05 Jy ! Component: 100 - total flux cleaned = 0.000102375 Jy ! Component: 150 - total flux cleaned = 0.000102466 Jy ! Component: 200 - total flux cleaned = 0.000112679 Jy ! Total flux subtracted in 200 components = 0.000112679 Jy ! Clean residual min=-0.000947 max=0.000920 Jy/beam ! Clean residual mean=0.000003 rms=0.000213 Jy/beam ! Combined flux in latest and established models = 0.0897864 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 41 components and 0.0897865 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=0.080495Jy sigma=0.652001 ! Fit after self-cal, rms=0.080495Jy sigma=0.651998 ! Inverting map ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 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=0.080495Jy sigma=0.651998 ! Fit after self-cal, rms=0.080888Jy sigma=0.651975 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec ! Estimated beam: bmin=2.784 mas, bmaj=3.641 mas, bpa=-80.87 degrees ! Estimated noise=0.457485 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00050883 Jy ! Component: 100 - total flux cleaned = 0.000678734 Jy ! Component: 150 - total flux cleaned = 0.000732457 Jy ! Component: 200 - total flux cleaned = 0.0007646 Jy ! Total flux subtracted in 200 components = 0.0007646 Jy ! Clean residual min=-0.000986 max=0.000994 Jy/beam ! Clean residual mean=0.000006 rms=0.000262 Jy/beam ! Combined flux in latest and established models = 0.0905511 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 52 components and 0.090551 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=0.080887Jy sigma=0.651972 ! Fit after self-cal, rms=0.080891Jy sigma=0.651964 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 7.15314e-05 Jy ! Component: 100 - total flux cleaned = 8.27109e-05 Jy ! Component: 150 - total flux cleaned = 9.75416e-05 Jy ! Component: 200 - total flux cleaned = 0.000110521 Jy ! Total flux subtracted in 200 components = 0.000110521 Jy ! Clean residual min=-0.000970 max=0.000980 Jy/beam ! Clean residual mean=0.000007 rms=0.000261 Jy/beam ! Combined flux in latest and established models = 0.0906616 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 54 components and 0.0906616 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=0.080891Jy sigma=0.651972 ! Fit after self-cal, rms=0.080892Jy sigma=0.651972 ! Inverting map ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 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 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec ! Estimated beam: bmin=0.5933 mas, bmaj=1.146 mas, bpa=23.65 degrees ! Estimated noise=0.353491 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5933 x 1.146 at 23.65 degrees (North through East) ! Clean map min=-0.00096305 max=0.065287 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 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec ! Estimated beam: bmin=0.4016 mas, bmaj=0.9278 mas, bpa=23.21 degrees ! Estimated noise=0.779574 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0457193 Jy ! Component: 100 - total flux cleaned = 0.06501 Jy ! Component: 150 - total flux cleaned = 0.0757022 Jy ! Component: 200 - total flux cleaned = 0.0816601 Jy ! Total flux subtracted in 200 components = 0.0816601 Jy ! Clean residual min=-0.002438 max=0.003008 Jy/beam ! Clean residual mean=-0.000002 rms=0.000539 Jy/beam ! Combined flux in latest and established models = 0.0816601 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 5 model components to the UV plane model. ! The established model now contains 5 components and 0.0816601 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec ! Estimated beam: bmin=0.5933 mas, bmaj=1.146 mas, bpa=23.65 degrees ! Estimated noise=0.353491 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 = 0.00363367 Jy ! Component: 100 - total flux cleaned = 0.00560593 Jy ! Component: 150 - total flux cleaned = 0.00689373 Jy ! Component: 200 - total flux cleaned = 0.00731659 Jy ! Total flux subtracted in 200 components = 0.00731659 Jy ! Clean residual min=-0.000987 max=0.001024 Jy/beam ! Clean residual mean=0.000001 rms=0.000223 Jy/beam ! Combined flux in latest and established models = 0.0889767 Jy ! Adding 18 model components to the UV plane model. ! The established model now contains 18 components and 0.0889767 Jy ! Inverting map ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec ! Added new window around map position (1, -3.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000651217 Jy ! Component: 100 - total flux cleaned = 0.000944219 Jy ! Component: 150 - total flux cleaned = 0.00109689 Jy ! Component: 200 - total flux cleaned = 0.00116743 Jy ! Total flux subtracted in 200 components = 0.00116743 Jy ! Clean residual min=-0.000941 max=0.000881 Jy/beam ! Clean residual mean=0.000002 rms=0.000215 Jy/beam ! Combined flux in latest and established models = 0.0901441 Jy ! Adding 20 model components to the UV plane model. ! The established model now contains 30 components and 0.0901441 Jy ! Inverting map ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 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 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec ! Estimated beam: bmin=2.784 mas, bmaj=3.641 mas, bpa=-80.87 degrees ! Estimated noise=0.457485 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000530154 Jy ! Component: 100 - total flux cleaned = 0.000726166 Jy ! Component: 150 - total flux cleaned = 0.00076722 Jy ! Component: 200 - total flux cleaned = 0.000804567 Jy ! Total flux subtracted in 200 components = 0.000804567 Jy ! Clean residual min=-0.000945 max=0.000969 Jy/beam ! Clean residual mean=0.000007 rms=0.000257 Jy/beam ! Combined flux in latest and established models = 0.0909487 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 = 2.45422e-05 Jy ! Component: 100 - total flux cleaned = 3.08701e-05 Jy ! Component: 150 - total flux cleaned = 4.43636e-05 Jy ! Component: 200 - total flux cleaned = 5.0676e-05 Jy ! Total flux subtracted in 200 components = 5.0676e-05 Jy ! Clean residual min=-0.000942 max=0.000974 Jy/beam ! Clean residual mean=0.000007 rms=0.000256 Jy/beam ! Combined flux in latest and established models = 0.0909993 Jy ! Adding 14 model components to the UV plane model. ! The established model now contains 42 components and 0.0909993 Jy ! Inverting map ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec ! Estimated beam: bmin=0.5933 mas, bmaj=1.146 mas, bpa=23.65 degrees ! Estimated noise=0.353491 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000221737 Jy ! Component: 100 - total flux cleaned = -0.000242652 Jy ! Component: 150 - total flux cleaned = -0.000242325 Jy ! Component: 200 - total flux cleaned = -0.000224732 Jy ! Total flux subtracted in 200 components = -0.000224732 Jy ! Clean residual min=-0.000945 max=0.000923 Jy/beam ! Clean residual mean=0.000003 rms=0.000212 Jy/beam ! Combined flux in latest and established models = 0.0907746 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 47 components and 0.0907746 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=0.080902Jy sigma=0.652056 ! Fit after self-cal, rms=0.080898Jy sigma=0.652015 wmodel /scr/pima/gb073_uvs/J1608+6018_X_map.mod ! Writing 47 model components to file: /scr/pima/gb073_uvs/J1608+6018_X_map.mod wobs /scr/pima/gb073_uvs/J1608+6018_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1608+6018_X_uvs.fits wwins /scr/pima/gb073_uvs/J1608+6018_X_map.win ! wwins: Wrote 3 windows to /scr/pima/gb073_uvs/J1608+6018_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 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000156902 Jy ! Component: 100 - total flux cleaned = -0.000272967 Jy ! Component: 150 - total flux cleaned = -0.000273337 Jy ! Component: 200 - total flux cleaned = -0.000304406 Jy ! Component: 250 - total flux cleaned = -0.000289352 Jy ! Component: 300 - total flux cleaned = -0.000289376 Jy ! Component: 350 - total flux cleaned = -0.000275031 Jy ! Component: 400 - total flux cleaned = -0.000303819 Jy ! Component: 450 - total flux cleaned = -0.000247514 Jy ! Component: 500 - total flux cleaned = -0.000247335 Jy ! Component: 550 - total flux cleaned = -0.000219553 Jy ! Component: 600 - total flux cleaned = -0.000219566 Jy ! Component: 650 - total flux cleaned = -0.000219602 Jy ! Component: 700 - total flux cleaned = -0.000232846 Jy ! Component: 750 - total flux cleaned = -0.000193105 Jy ! Component: 800 - total flux cleaned = -0.000245869 Jy ! Component: 850 - total flux cleaned = -0.000272056 Jy ! Component: 900 - total flux cleaned = -0.000258924 Jy ! Component: 950 - total flux cleaned = -0.000258795 Jy ! Component: 1000 - total flux cleaned = -0.000220467 Jy ! Component: 1050 - total flux cleaned = -0.000245891 Jy ! Component: 1100 - total flux cleaned = -0.000220671 Jy ! Component: 1150 - total flux cleaned = -0.000296024 Jy ! Component: 1200 - total flux cleaned = -0.00033319 Jy ! Component: 1250 - total flux cleaned = -0.000333106 Jy ! Component: 1300 - total flux cleaned = -0.000345366 Jy ! Component: 1350 - total flux cleaned = -0.000369871 Jy ! Component: 1400 - total flux cleaned = -0.000357722 Jy ! Component: 1450 - total flux cleaned = -0.000369838 Jy ! Component: 1500 - total flux cleaned = -0.000405837 Jy ! Component: 1550 - total flux cleaned = -0.000405851 Jy ! Component: 1600 - total flux cleaned = -0.000393981 Jy ! Component: 1650 - total flux cleaned = -0.000382211 Jy ! Component: 1700 - total flux cleaned = -0.000464656 Jy ! Component: 1750 - total flux cleaned = -0.000382658 Jy ! Component: 1800 - total flux cleaned = -0.000452769 Jy ! Component: 1850 - total flux cleaned = -0.000487615 Jy ! Component: 1900 - total flux cleaned = -0.000452838 Jy ! Component: 1950 - total flux cleaned = -0.00047584 Jy ! Component: 2000 - total flux cleaned = -0.000487299 Jy ! Component: 2050 - total flux cleaned = -0.000510121 Jy ! Component: 2100 - total flux cleaned = -0.000487353 Jy ! Component: 2150 - total flux cleaned = -0.000498641 Jy ! Component: 2200 - total flux cleaned = -0.000555182 Jy ! Component: 2250 - total flux cleaned = -0.000543911 Jy ! Component: 2300 - total flux cleaned = -0.000543855 Jy ! Component: 2350 - total flux cleaned = -0.000555054 Jy ! Component: 2400 - total flux cleaned = -0.000577348 Jy ! Component: 2450 - total flux cleaned = -0.000532897 Jy ! Component: 2500 - total flux cleaned = -0.0005661 Jy ! Component: 2550 - total flux cleaned = -0.000588061 Jy ! Component: 2600 - total flux cleaned = -0.000555109 Jy ! Component: 2650 - total flux cleaned = -0.000587897 Jy ! Component: 2700 - total flux cleaned = -0.000577056 Jy ! Component: 2750 - total flux cleaned = -0.000544475 Jy ! Component: 2800 - total flux cleaned = -0.000587807 Jy ! Component: 2850 - total flux cleaned = -0.00052302 Jy ! Component: 2900 - total flux cleaned = -0.000587631 Jy ! Component: 2950 - total flux cleaned = -0.000609044 Jy ! Component: 3000 - total flux cleaned = -0.000576975 Jy ! Component: 3050 - total flux cleaned = -0.000587654 Jy ! Component: 3100 - total flux cleaned = -0.000577038 Jy ! Component: 3150 - total flux cleaned = -0.000577076 Jy ! Component: 3200 - total flux cleaned = -0.000534813 Jy ! Component: 3250 - total flux cleaned = -0.000513781 Jy ! Component: 3300 - total flux cleaned = -0.000513839 Jy ! Component: 3350 - total flux cleaned = -0.00054526 Jy ! Component: 3400 - total flux cleaned = -0.000440961 Jy ! Component: 3450 - total flux cleaned = -0.000482573 Jy ! Component: 3500 - total flux cleaned = -0.000513643 Jy ! Component: 3550 - total flux cleaned = -0.000513656 Jy ! Component: 3600 - total flux cleaned = -0.000451752 Jy ! Component: 3650 - total flux cleaned = -0.000441463 Jy ! Component: 3700 - total flux cleaned = -0.000420954 Jy ! Component: 3750 - total flux cleaned = -0.000431176 Jy ! Component: 3800 - total flux cleaned = -0.000421013 Jy ! Component: 3850 - total flux cleaned = -0.000431192 Jy ! Component: 3900 - total flux cleaned = -0.000441302 Jy ! Component: 3950 - total flux cleaned = -0.000390771 Jy ! Component: 4000 - total flux cleaned = -0.000390759 Jy ! Component: 4050 - total flux cleaned = -0.000400796 Jy ! Total flux subtracted in 4096 components = -0.000350621 Jy ! Clean residual min=-0.000786 max=0.000611 Jy/beam ! Clean residual mean=0.000002 rms=0.000167 Jy/beam ! Combined flux in latest and established models = 0.090424 Jy keep ! Adding 351 model components to the UV plane model. ! The established model now contains 398 components and 0.090424 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1608+6018_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5933 x 1.146 at 23.65 degrees (North through East) ! Clean map min=-0.00079787 max=0.065123 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1608+6018_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0651231 invert ! Inverting map ! Your choice of large map pixels excluded 9.04% of the data. ! The x-axis pixel size should ideally be below 0.1767 milli-arcsec ! The y-axis pixel size should ideally be below 0.1995 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000166446 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.766763 0.766763 1.53353 3.06705 6.1341 12.2682 24.5364 49.0728 98.1456 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0004 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.065 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 391.255 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1608+6018_X_uvs.log closed on Sat Dec 26 09:42:21 2015