! Started logfile: /scr/pima/gb073_uvs/J1931+2243_X_uvs.log on Sat Dec 26 09:44:37 2015 obs /scr/pima/gb073_uvs/J1931+2243_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1931+2243_X_uva.fits ! AN table 1: 18 integrations on 6 of 6 possible baselines. ! AN table 2: 6 integrations on 6 of 6 possible baselines. ! AN table 3: 5 integrations on 15 of 15 possible baselines. ! AN table 4: 5 integrations on 28 of 28 possible baselines. ! AN table 5: 6 integrations on 66 of 66 possible baselines. ! AN table 6: 6 integrations on 10 of 10 possible baselines. ! AN table 7: 6 integrations on 6 of 6 possible baselines. ! AN table 8: 6 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.997594 visibilities/baseline/integration-bin. ! Found source: J1931+2243 ! ! 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 9952 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/J1931+2243_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 21 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 6 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 2. ! A total of 21 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 6 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 3. ! A total of 21 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 6 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 4. ! A total of 21 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 6 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 5. ! A total of 21 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 5 telescope corrections were flagged in sub-array 3. ! A total of 5 telescope corrections were flagged in sub-array 4. ! A total of 12 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 12 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 6. ! A total of 21 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 5 telescope corrections were flagged in sub-array 3. ! A total of 5 telescope corrections were flagged in sub-array 4. ! A total of 12 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 12 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 7. ! A total of 21 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 6 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 8. ! A total of 21 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 6 telescope corrections were flagged in sub-array 8. ! ! Fit before self-cal, rms=1.108878Jy sigma=9.894504 ! Fit after self-cal, rms=0.565677Jy sigma=4.820692 ! 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 8.57% of the data. ! The x-axis pixel size should ideally be below 0.1722 milli-arcsec ! Estimated beam: bmin=0.5083 mas, bmaj=0.8743 mas, bpa=-8.617 degrees ! Estimated noise=1.51173 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 = 0.346648 Jy ! Component: 100 - total flux cleaned = 0.425002 Jy ! Total flux subtracted in 100 components = 0.425002 Jy ! Clean residual min=-0.020553 max=0.028402 Jy/beam ! Clean residual mean=-0.000020 rms=0.003759 Jy/beam ! Combined flux in latest and established models = 0.425002 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.425002 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=0.147988Jy sigma=1.053079 ! Fit after self-cal, rms=0.147967Jy sigma=1.052977 ! Inverting map ! Your choice of large map pixels excluded 8.57% of the data. ! The x-axis pixel size should ideally be below 0.1722 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0301368 Jy ! Component: 100 - total flux cleaned = 0.0471398 Jy ! Total flux subtracted in 100 components = 0.0471398 Jy ! Clean residual min=-0.020431 max=0.022718 Jy/beam ! Clean residual mean=-0.000012 rms=0.003352 Jy/beam ! Combined flux in latest and established models = 0.472142 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 8 components and 0.472142 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=0.140885Jy sigma=0.957341 ! Fit after self-cal, rms=0.140871Jy sigma=0.957240 ! Inverting map ! Your choice of large map pixels excluded 8.57% of the data. ! The x-axis pixel size should ideally be below 0.1722 milli-arcsec ! Added new window around map position (-1, 4.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00634357 Jy ! Component: 100 - total flux cleaned = 0.00828468 Jy ! Total flux subtracted in 100 components = 0.00828468 Jy ! Clean residual min=-0.019247 max=0.019404 Jy/beam ! Clean residual mean=-0.000012 rms=0.003178 Jy/beam ! Combined flux in latest and established models = 0.480426 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 14 components and 0.480426 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=0.137655Jy sigma=0.926698 ! Fit after self-cal, rms=0.137461Jy sigma=0.925074 ! Inverting map ! Your choice of large map pixels excluded 8.57% of the data. ! The x-axis pixel size should ideally be below 0.1722 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 8.57% of the data. ! The x-axis pixel size should ideally be below 0.1722 milli-arcsec ! Estimated beam: bmin=0.6266 mas, bmaj=0.9887 mas, bpa=-7.706 degrees ! Estimated noise=0.989317 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 (-1.6, 2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0165623 Jy ! Component: 100 - total flux cleaned = 0.0246953 Jy ! Component: 150 - total flux cleaned = 0.026652 Jy ! Component: 200 - total flux cleaned = 0.0275282 Jy ! Total flux subtracted in 200 components = 0.0275282 Jy ! Clean residual min=-0.011471 max=0.011255 Jy/beam ! Clean residual mean=-0.000004 rms=0.002108 Jy/beam ! Combined flux in latest and established models = 0.507954 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 28 components and 0.507954 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=0.134914Jy sigma=0.899283 ! Fit after self-cal, rms=0.134783Jy sigma=0.897964 ! Inverting map ! Your choice of large map pixels excluded 8.57% of the data. ! The x-axis pixel size should ideally be below 0.1722 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6266 x 0.9887 at -7.706 degrees (North through East) ! Clean map min=-0.0083907 max=0.4504 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 51 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 0.00* HH 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 KP 0.96 MK 0.99 ON 1.05 ! OV 0.98 PT 0.93 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.96 FD 0.99 KP 1.00 LA 1.02 ! MK 0.96 NL 0.93 OV 1.00 PT 0.97 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 EF 1.00* FD 0.97 HH 1.06 ! KP 1.00 LA 1.04 MC 0.99 NL 0.93 ! ON 1.00 PT 0.98 SC 0.96 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 0.93 MC 1.04 ON 1.10 ! ZC 0.78 ! ! Telescope amplitude corrections in sub-array 7: ! HH 1.08 MC 1.01 SC 0.92 ZC 0.71 ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.93 EF 1.00* FD 1.01 KP 0.98 ! LA 1.03 MC 0.97 NL 0.96 ON 1.05 ! OV 0.99 PT 0.94 SC 0.95 ZC 0.73 ! ! ! Correcting IF 2. ! A total of 51 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 0.00* HH 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 KP 0.99 MK 1.02 ON 1.04 ! OV 1.05 PT 1.04 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 1.02 KP 1.00 LA 1.06 ! MK 1.00 NL 0.97 OV 1.01 PT 1.02 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.98 EF 1.00* FD 1.02 HH 1.01 ! KP 1.04 LA 1.09 MC 1.00 NL 0.94 ! ON 0.99 PT 1.03 SC 0.98 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.02 MC 0.90 ON 1.19 ! ZC 0.82 ! ! Telescope amplitude corrections in sub-array 7: ! HH 1.01 MC 1.00 SC 0.94 ZC 0.75 ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.99 EF 1.00* FD 1.04 KP 1.02 ! LA 1.06 MC 0.98 NL 0.97 ON 1.07 ! OV 1.02 PT 1.02 SC 1.00 ZC 0.74 ! ! ! Correcting IF 3. ! A total of 51 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 0.00* HH 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 KP 0.94 MK 0.95 ON 1.01 ! OV 0.99 PT 1.03 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.04 FD 1.00 KP 0.96 LA 0.98 ! MK 0.95 NL 0.92 OV 0.97 PT 0.98 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 EF 1.00* FD 1.00 HH 0.99 ! KP 0.96 LA 1.01 MC 1.00 NL 0.95 ! ON 1.00 PT 1.01 SC 1.00 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 0.92 MC 1.03 ON 1.09 ! ZC 0.73 ! ! Telescope amplitude corrections in sub-array 7: ! HH 0.96 MC 1.00 SC 0.96 ZC 0.69 ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.99 EF 1.00* FD 1.02 KP 0.94 ! LA 0.98 MC 0.96 NL 0.94 ON 1.03 ! OV 1.00 PT 1.01 SC 1.02 ZC 0.74 ! ! ! Correcting IF 4. ! A total of 51 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 0.00* HH 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 KP 0.94 MK 0.95 ON 1.02 ! OV 1.03 PT 1.03 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.04 FD 1.05 KP 0.97 LA 0.95 ! MK 0.99 NL 0.94 OV 1.01 PT 1.02 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 EF 1.00* FD 1.03 HH 1.01 ! KP 0.96 LA 1.00 MC 1.04 NL 0.97 ! ON 0.97 PT 1.05 SC 1.01 ZC 0.80 ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 0.95 MC 1.07 ON 1.08 ! ZC 0.77 ! ! Telescope amplitude corrections in sub-array 7: ! HH 0.97 MC 1.00 SC 1.00 ZC 0.71 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.00 EF 1.00* FD 1.05 KP 0.96 ! LA 1.01 MC 1.05 NL 0.98 ON 1.02 ! OV 0.98 PT 1.00 SC 1.01 ZC 0.74 ! ! ! Correcting IF 5. ! A total of 51 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 0.00* HH 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* KP 0.90 MK 0.99 ON 1.33 ! OV 1.08 PT 0.96 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.04 KP 0.90 LA 0.98 ! MK 1.01 NL 0.94 OV 1.07 PT 0.97 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.01 HH 1.04 ! KP 0.90 LA 1.01 MC 1.24 NL 1.01 ! ON 1.29 PT 1.01 SC 1.05 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 0.93 MC 1.28 ON 1.29 ! ZC 0.85 ! ! Telescope amplitude corrections in sub-array 7: ! HH 0.85 MC 1.34 SC 0.95 ZC 0.74 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.00* EF 1.00* FD 1.05 KP 0.89 ! LA 0.98 MC 1.32 NL 1.00 ON 1.34 ! OV 1.04 PT 0.98 SC 1.05 ZC 0.75 ! ! ! Correcting IF 6. ! A total of 51 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 0.00* HH 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* KP 0.83 MK 1.01 ON 1.45 ! OV 1.15 PT 0.95 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.02 KP 0.88 LA 0.99 ! MK 1.01 NL 1.00 OV 1.05 PT 0.92 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00 HH 1.03 ! KP 0.94 LA 1.01 MC 1.27 NL 0.99 ! ON 1.35 PT 0.96 SC 0.99 ZC 0.78 ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 0.88 MC 1.21 ON 1.23 ! ZC 0.88 ! ! Telescope amplitude corrections in sub-array 7: ! HH 1.01 MC 1.39 SC 1.04 ZC 0.68 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.00* EF 1.00* FD 1.03 KP 0.89 ! LA 1.02 MC 1.28 NL 0.99 ON 1.31 ! OV 1.05 PT 0.95 SC 1.00 ZC 0.72 ! ! ! Correcting IF 7. ! A total of 51 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 0.00* HH 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 KP 0.93 MK 1.02 ON 1.50 ! OV 1.01 PT 1.02 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 FD 1.09 KP 0.91 LA 1.03 ! MK 1.06 NL 1.02 OV 1.01 PT 1.01 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 EF 1.00* FD 1.08 HH 1.28 ! KP 0.95 LA 1.06 MC 1.30 NL 0.99 ! ON 1.33 PT 1.05 SC 1.04 ZC 0.63 ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.07 MC 1.30 ON 1.52 ! ZC 0.62 ! ! Telescope amplitude corrections in sub-array 7: ! HH 1.24 MC 1.25 SC 1.03 ZC 0.54 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.03 EF 1.00* FD 1.05 KP 0.90 ! LA 1.03 MC 1.44 NL 1.03 ON 1.42 ! OV 0.99 PT 1.03 SC 1.03 ZC 0.56 ! ! ! Correcting IF 8. ! A total of 51 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 0.00* HH 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 KP 0.90 MK 1.09 ON 1.33 ! OV 1.03 PT 1.01 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 FD 1.04 KP 0.92 LA 1.05 ! MK 1.02 NL 1.01 OV 0.99 PT 1.02 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 EF 1.00* FD 1.07 HH 1.25 ! KP 0.93 LA 1.05 MC 1.37 NL 1.00 ! ON 1.36 PT 1.02 SC 1.05 ZC 0.59 ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.10 MC 1.42 ON 1.51 ! ZC 0.56 ! ! Telescope amplitude corrections in sub-array 7: ! HH 1.08 MC 1.42 SC 1.14 ZC 0.46 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.02 EF 1.00* FD 1.05 KP 0.94 ! LA 1.05 MC 1.36 NL 1.01 ON 1.36 ! OV 0.99 PT 1.03 SC 1.04 ZC 0.53 ! ! ! Fit before self-cal, rms=0.134783Jy sigma=0.897964 ! Fit after self-cal, rms=0.101103Jy sigma=0.655493 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 milli-arcsec ! Estimated beam: bmin=0.6201 mas, bmaj=1.101 mas, bpa=-8.004 degrees ! Estimated noise=0.988703 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 = 0.00079684 Jy ! Component: 100 - total flux cleaned = 0.0019616 Jy ! Component: 150 - total flux cleaned = 0.00234917 Jy ! Component: 200 - total flux cleaned = 0.00255998 Jy ! Total flux subtracted in 200 components = 0.00255998 Jy ! Clean residual min=-0.004071 max=0.003187 Jy/beam ! Clean residual mean=-0.000000 rms=0.000729 Jy/beam ! Combined flux in latest and established models = 0.510514 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 38 components and 0.510514 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=0.100399Jy sigma=0.649359 ! Fit after self-cal, rms=0.100805Jy sigma=0.648295 ! Inverting map ! Your choice of large map pixels excluded 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 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=0.100805Jy sigma=0.648295 ! Fit after self-cal, rms=0.101165Jy sigma=0.647516 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 milli-arcsec ! Estimated beam: bmin=0.6205 mas, bmaj=1.101 mas, bpa=-8.029 degrees ! Estimated noise=0.988002 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000189819 Jy ! Component: 100 - total flux cleaned = 0.000639078 Jy ! Component: 150 - total flux cleaned = 0.000820442 Jy ! Component: 200 - total flux cleaned = 0.000977703 Jy ! Total flux subtracted in 200 components = 0.000977703 Jy ! Clean residual min=-0.003995 max=0.003042 Jy/beam ! Clean residual mean=-0.000001 rms=0.000690 Jy/beam ! Combined flux in latest and established models = 0.511492 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 42 components and 0.511492 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=0.100836Jy sigma=0.644715 ! Fit after self-cal, rms=0.100828Jy sigma=0.644545 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 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 = 0.000133145 Jy ! Component: 100 - total flux cleaned = 0.000276544 Jy ! Component: 150 - total flux cleaned = 0.000345258 Jy ! Component: 200 - total flux cleaned = 0.000407254 Jy ! Total flux subtracted in 200 components = 0.000407254 Jy ! Clean residual min=-0.003893 max=0.002976 Jy/beam ! Clean residual mean=-0.000001 rms=0.000675 Jy/beam ! Combined flux in latest and established models = 0.511899 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 46 components and 0.511899 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=0.100687Jy sigma=0.643412 ! Fit after self-cal, rms=0.100676Jy sigma=0.643360 ! Inverting map ! Your choice of large map pixels excluded 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 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=0.100676Jy sigma=0.643360 ! Fit after self-cal, rms=0.100944Jy sigma=0.642901 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 milli-arcsec ! Estimated beam: bmin=0.6207 mas, bmaj=1.102 mas, bpa=-8.052 degrees ! Estimated noise=0.987253 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000352467 Jy ! Component: 100 - total flux cleaned = -0.00020949 Jy ! Component: 150 - total flux cleaned = -0.000150336 Jy ! Component: 200 - total flux cleaned = -0.000151139 Jy ! Total flux subtracted in 200 components = -0.000151139 Jy ! Clean residual min=-0.003883 max=0.002906 Jy/beam ! Clean residual mean=-0.000001 rms=0.000658 Jy/beam ! Combined flux in latest and established models = 0.511748 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 47 components and 0.511748 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=0.100816Jy sigma=0.641790 ! Fit after self-cal, rms=0.100814Jy sigma=0.641737 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 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 = 0.000106884 Jy ! Component: 100 - total flux cleaned = 0.000209375 Jy ! Component: 150 - total flux cleaned = 0.000209723 Jy ! Component: 200 - total flux cleaned = 0.000254916 Jy ! Total flux subtracted in 200 components = 0.000254916 Jy ! Clean residual min=-0.003800 max=0.002832 Jy/beam ! Clean residual mean=-0.000001 rms=0.000651 Jy/beam ! Combined flux in latest and established models = 0.512003 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 51 components and 0.512003 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=0.100742Jy sigma=0.641167 ! Fit after self-cal, rms=0.100736Jy sigma=0.641147 ! Inverting map ! Your choice of large map pixels excluded 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 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=0.100736Jy sigma=0.641147 ! Fit after self-cal, rms=0.100891Jy sigma=0.640983 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 milli-arcsec ! Estimated beam: bmin=2.902 mas, bmaj=2.965 mas, bpa=-31 degrees ! Estimated noise=1.24875 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000539572 Jy ! Component: 100 - total flux cleaned = 0.000514828 Jy ! Component: 150 - total flux cleaned = 0.000517736 Jy ! Component: 200 - total flux cleaned = 0.000517798 Jy ! Total flux subtracted in 200 components = 0.000517798 Jy ! Clean residual min=-0.003323 max=0.003028 Jy/beam ! Clean residual mean=-0.000002 rms=0.000833 Jy/beam ! Combined flux in latest and established models = 0.512521 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 59 components and 0.512521 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=0.100896Jy sigma=0.641064 ! Fit after self-cal, rms=0.100894Jy sigma=0.641044 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 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 = 0.000192042 Jy ! Component: 100 - total flux cleaned = 0.000208222 Jy ! Component: 150 - total flux cleaned = 0.000207857 Jy ! Component: 200 - total flux cleaned = 0.000208746 Jy ! Total flux subtracted in 200 components = 0.000208746 Jy ! Clean residual min=-0.003300 max=0.002985 Jy/beam ! Clean residual mean=-0.000002 rms=0.000832 Jy/beam ! Combined flux in latest and established models = 0.51273 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 61 components and 0.51273 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=0.100897Jy sigma=0.641078 ! Fit after self-cal, rms=0.100894Jy sigma=0.641074 ! Inverting map ! Your choice of large map pixels excluded 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 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 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 milli-arcsec ! Estimated beam: bmin=0.6206 mas, bmaj=1.104 mas, bpa=-8.072 degrees ! Estimated noise=0.986692 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6206 x 1.104 at -8.072 degrees (North through East) ! Clean map min=-0.0030933 max=0.44886 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 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 milli-arcsec ! Estimated beam: bmin=0.4961 mas, bmaj=0.9806 mas, bpa=-9.139 degrees ! Estimated noise=1.5169 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.347264 Jy ! Component: 100 - total flux cleaned = 0.423744 Jy ! Component: 150 - total flux cleaned = 0.448696 Jy ! Component: 200 - total flux cleaned = 0.462241 Jy ! Total flux subtracted in 200 components = 0.462241 Jy ! Clean residual min=-0.006078 max=0.008145 Jy/beam ! Clean residual mean=-0.000008 rms=0.001203 Jy/beam ! Combined flux in latest and established models = 0.462241 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 0.462241 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 milli-arcsec ! Estimated beam: bmin=0.6206 mas, bmaj=1.104 mas, bpa=-8.072 degrees ! Estimated noise=0.986692 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) ! Added new window around map position (-0.6, 1.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0174846 Jy ! Component: 100 - total flux cleaned = 0.0282402 Jy ! Component: 150 - total flux cleaned = 0.0355231 Jy ! Component: 200 - total flux cleaned = 0.0406186 Jy ! Total flux subtracted in 200 components = 0.0406186 Jy ! Clean residual min=-0.003599 max=0.003278 Jy/beam ! Clean residual mean=-0.000004 rms=0.000723 Jy/beam ! Combined flux in latest and established models = 0.502859 Jy ! Adding 39 model components to the UV plane model. ! The established model now contains 48 components and 0.502859 Jy ! Inverting map ! Your choice of large map pixels excluded 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 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 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 milli-arcsec ! Estimated beam: bmin=2.902 mas, bmaj=2.965 mas, bpa=-31 degrees ! Estimated noise=1.24875 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00553163 Jy ! Component: 100 - total flux cleaned = 0.00809465 Jy ! Component: 150 - total flux cleaned = 0.00940294 Jy ! Component: 200 - total flux cleaned = 0.00984051 Jy ! Total flux subtracted in 200 components = 0.00984051 Jy ! Clean residual min=-0.003440 max=0.002923 Jy/beam ! Clean residual mean=-0.000002 rms=0.000833 Jy/beam ! Combined flux in latest and established models = 0.5127 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 = 0.000131757 Jy ! Component: 100 - total flux cleaned = 0.000169028 Jy ! Component: 150 - total flux cleaned = 0.000220606 Jy ! Component: 200 - total flux cleaned = 0.000252309 Jy ! Total flux subtracted in 200 components = 0.000252309 Jy ! Clean residual min=-0.003396 max=0.002894 Jy/beam ! Clean residual mean=-0.000002 rms=0.000828 Jy/beam ! Combined flux in latest and established models = 0.512952 Jy ! Adding 39 model components to the UV plane model. ! The established model now contains 77 components and 0.512952 Jy ! Inverting map ! Your choice of large map pixels excluded 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 milli-arcsec ! Estimated beam: bmin=0.6206 mas, bmaj=1.104 mas, bpa=-8.072 degrees ! Estimated noise=0.986692 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000278356 Jy ! Component: 100 - total flux cleaned = 0.00014273 Jy ! Component: 150 - total flux cleaned = 3.21415e-05 Jy ! Component: 200 - total flux cleaned = 3.07772e-05 Jy ! Total flux subtracted in 200 components = 3.07772e-05 Jy ! Clean residual min=-0.003176 max=0.002981 Jy/beam ! Clean residual mean=-0.000000 rms=0.000635 Jy/beam ! Combined flux in latest and established models = 0.512983 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 82 components and 0.512983 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=0.100869Jy sigma=0.640223 ! Fit after self-cal, rms=0.100787Jy sigma=0.639883 wmodel /scr/pima/gb073_uvs/J1931+2243_X_map.mod ! Writing 82 model components to file: /scr/pima/gb073_uvs/J1931+2243_X_map.mod wobs /scr/pima/gb073_uvs/J1931+2243_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1931+2243_X_uvs.fits wwins /scr/pima/gb073_uvs/J1931+2243_X_map.win ! wwins: Wrote 4 windows to /scr/pima/gb073_uvs/J1931+2243_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 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000151165 Jy ! Component: 100 - total flux cleaned = 0.000235869 Jy ! Component: 150 - total flux cleaned = 0.000513634 Jy ! Component: 200 - total flux cleaned = 0.000693187 Jy ! Component: 250 - total flux cleaned = 0.000693274 Jy ! Component: 300 - total flux cleaned = 0.000736665 Jy ! Component: 350 - total flux cleaned = 0.000904759 Jy ! Component: 400 - total flux cleaned = 0.0010286 Jy ! Component: 450 - total flux cleaned = 0.00106899 Jy ! Component: 500 - total flux cleaned = 0.00118966 Jy ! Component: 550 - total flux cleaned = 0.00142716 Jy ! Component: 600 - total flux cleaned = 0.00154381 Jy ! Component: 650 - total flux cleaned = 0.00158283 Jy ! Component: 700 - total flux cleaned = 0.00185021 Jy ! Component: 750 - total flux cleaned = 0.00200092 Jy ! Component: 800 - total flux cleaned = 0.0022606 Jy ! Component: 850 - total flux cleaned = 0.00251724 Jy ! Component: 900 - total flux cleaned = 0.00251737 Jy ! Component: 950 - total flux cleaned = 0.0026253 Jy ! Component: 1000 - total flux cleaned = 0.0027683 Jy ! Component: 1050 - total flux cleaned = 0.00283926 Jy ! Component: 1100 - total flux cleaned = 0.00308354 Jy ! Component: 1150 - total flux cleaned = 0.00308309 Jy ! Component: 1200 - total flux cleaned = 0.00301465 Jy ! Component: 1250 - total flux cleaned = 0.00325299 Jy ! Component: 1300 - total flux cleaned = 0.00342198 Jy ! Component: 1350 - total flux cleaned = 0.00342183 Jy ! Component: 1400 - total flux cleaned = 0.00358763 Jy ! Component: 1450 - total flux cleaned = 0.00375236 Jy ! Component: 1500 - total flux cleaned = 0.00368742 Jy ! Component: 1550 - total flux cleaned = 0.003914 Jy ! Component: 1600 - total flux cleaned = 0.00410643 Jy ! Component: 1650 - total flux cleaned = 0.00413821 Jy ! Component: 1700 - total flux cleaned = 0.0042329 Jy ! Component: 1750 - total flux cleaned = 0.00442141 Jy ! Component: 1800 - total flux cleaned = 0.00448394 Jy ! Component: 1850 - total flux cleaned = 0.00454623 Jy ! Component: 1900 - total flux cleaned = 0.00476094 Jy ! Component: 1950 - total flux cleaned = 0.00488262 Jy ! Component: 2000 - total flux cleaned = 0.00497361 Jy ! Component: 2050 - total flux cleaned = 0.00515361 Jy ! Component: 2100 - total flux cleaned = 0.00527324 Jy ! Component: 2150 - total flux cleaned = 0.00536179 Jy ! Component: 2200 - total flux cleaned = 0.00550863 Jy ! Component: 2250 - total flux cleaned = 0.00536262 Jy ! Component: 2300 - total flux cleaned = 0.00544981 Jy ! Component: 2350 - total flux cleaned = 0.0055653 Jy ! Component: 2400 - total flux cleaned = 0.00565113 Jy ! Component: 2450 - total flux cleaned = 0.00550864 Jy ! Component: 2500 - total flux cleaned = 0.00559371 Jy ! Component: 2550 - total flux cleaned = 0.00567818 Jy ! Component: 2600 - total flux cleaned = 0.00579016 Jy ! Component: 2650 - total flux cleaned = 0.00584561 Jy ! Component: 2700 - total flux cleaned = 0.0058731 Jy ! Component: 2750 - total flux cleaned = 0.0058457 Jy ! Component: 2800 - total flux cleaned = 0.00590035 Jy ! Component: 2850 - total flux cleaned = 0.00595462 Jy ! Component: 2900 - total flux cleaned = 0.00608901 Jy ! Component: 2950 - total flux cleaned = 0.0061961 Jy ! Component: 3000 - total flux cleaned = 0.00616964 Jy ! Component: 3050 - total flux cleaned = 0.0061695 Jy ! Component: 3100 - total flux cleaned = 0.00635345 Jy ! Component: 3150 - total flux cleaned = 0.00632716 Jy ! Component: 3200 - total flux cleaned = 0.00645733 Jy ! Component: 3250 - total flux cleaned = 0.00658674 Jy ! Component: 3300 - total flux cleaned = 0.00661251 Jy ! Component: 3350 - total flux cleaned = 0.00671468 Jy ! Component: 3400 - total flux cleaned = 0.00676578 Jy ! Component: 3450 - total flux cleaned = 0.00689257 Jy ! Component: 3500 - total flux cleaned = 0.00696822 Jy ! Component: 3550 - total flux cleaned = 0.0070937 Jy ! Component: 3600 - total flux cleaned = 0.00706854 Jy ! Component: 3650 - total flux cleaned = 0.00721738 Jy ! Component: 3700 - total flux cleaned = 0.00719248 Jy ! Component: 3750 - total flux cleaned = 0.00724167 Jy ! Component: 3800 - total flux cleaned = 0.00738842 Jy ! Component: 3850 - total flux cleaned = 0.00755896 Jy ! Component: 3900 - total flux cleaned = 0.0075106 Jy ! Component: 3950 - total flux cleaned = 0.00772773 Jy ! Component: 4000 - total flux cleaned = 0.00772772 Jy ! Component: 4050 - total flux cleaned = 0.00787107 Jy ! Total flux subtracted in 4096 components = 0.00791859 Jy ! Clean residual min=-0.001223 max=0.001294 Jy/beam ! Clean residual mean=0.000001 rms=0.000387 Jy/beam ! Combined flux in latest and established models = 0.520901 Jy keep ! Adding 311 model components to the UV plane model. ! The established model now contains 393 components and 0.520901 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1931+2243_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6206 x 1.104 at -8.072 degrees (North through East) ! Clean map min=-0.0018501 max=0.44956 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1931+2243_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.449562 invert ! Inverting map ! Your choice of large map pixels excluded 9.23% of the data. ! The x-axis pixel size should ideally be below 0.1722 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000384738 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.256742 0.256742 0.513483 1.02697 2.05393 4.10787 8.21573 16.4315 32.8629 65.7259 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0011 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.449 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1168.49 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1931+2243_X_uvs.log closed on Sat Dec 26 09:44:42 2015