! Started logfile: /scr/pima/gb073_uvs/J2212+2355_X_uvs.log on Sat Dec 26 09:45:23 2015 obs /scr/pima/gb073_uvs/J2212+2355_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J2212+2355_X_uva.fits ! AN table 1: 18 integrations on 6 of 6 possible baselines. ! AN table 2: 6 integrations on 21 of 21 possible baselines. ! AN table 3: 6 integrations on 66 of 66 possible baselines. ! AN table 4: 5 integrations on 3 of 3 possible baselines. ! AN table 5: 5 integrations on 10 of 10 possible baselines. ! AN table 6: 5 integrations on 21 of 21 possible baselines. ! AN table 7: 6 integrations on 15 of 15 possible baselines. ! AN table 8: 6 integrations on 55 of 55 possible baselines. ! Apparent sampling: 0.985246 visibilities/baseline/integration-bin. ! Found source: J2212+2355 ! ! 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 9616 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/J2212+2355_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 18 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 3. ! A total of 15 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 7. ! A total of 6 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 2. ! A total of 18 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 3. ! A total of 15 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 7. ! A total of 6 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 3. ! A total of 18 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 3. ! A total of 15 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 7. ! A total of 6 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 4. ! A total of 18 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 3. ! A total of 15 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 7. ! A total of 6 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 5. ! A total of 18 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 12 telescope corrections were flagged in sub-array 3. ! A total of 15 telescope corrections were flagged in sub-array 4. ! A total of 5 telescope corrections were flagged in sub-array 5. ! A total of 5 telescope corrections were flagged in sub-array 6. ! A total of 6 telescope corrections were flagged in sub-array 7. ! A total of 12 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 6. ! A total of 18 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 12 telescope corrections were flagged in sub-array 3. ! A total of 15 telescope corrections were flagged in sub-array 4. ! A total of 5 telescope corrections were flagged in sub-array 5. ! A total of 5 telescope corrections were flagged in sub-array 6. ! A total of 6 telescope corrections were flagged in sub-array 7. ! A total of 12 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 7. ! A total of 18 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 3. ! A total of 15 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 7. ! A total of 6 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 8. ! A total of 18 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 3. ! A total of 15 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 7. ! A total of 6 telescope corrections were flagged in sub-array 8. ! ! Fit before self-cal, rms=1.366258Jy sigma=12.217040 ! Fit after self-cal, rms=0.298056Jy sigma=2.030915 ! 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 7.45% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! Estimated beam: bmin=0.5062 mas, bmaj=0.8494 mas, bpa=-11.32 degrees ! Estimated noise=1.62533 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 = 0.664407 Jy ! Component: 100 - total flux cleaned = 0.849396 Jy ! Total flux subtracted in 100 components = 0.849396 Jy ! Clean residual min=-0.035745 max=0.084638 Jy/beam ! Clean residual mean=0.000035 rms=0.008208 Jy/beam ! Combined flux in latest and established models = 0.849396 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.849396 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=0.257513Jy sigma=2.089835 ! Fit after self-cal, rms=0.257485Jy sigma=2.089684 ! Inverting map ! Your choice of large map pixels excluded 7.45% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0967865 Jy ! Component: 100 - total flux cleaned = 0.152254 Jy ! Total flux subtracted in 100 components = 0.152254 Jy ! Clean residual min=-0.028484 max=0.033517 Jy/beam ! Clean residual mean=0.000019 rms=0.005938 Jy/beam ! Combined flux in latest and established models = 1.00165 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 18 components and 1.00165 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=0.213838Jy sigma=1.498972 ! Fit after self-cal, rms=0.213817Jy sigma=1.498795 ! Inverting map ! Your choice of large map pixels excluded 7.45% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 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 7.45% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! Estimated beam: bmin=0.6351 mas, bmaj=1.021 mas, bpa=-10.89 degrees ! Estimated noise=1.04677 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 (-0.6, 0). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.049241 Jy ! Component: 100 - total flux cleaned = 0.0754032 Jy ! Component: 150 - total flux cleaned = 0.0784727 Jy ! Component: 200 - total flux cleaned = 0.0810856 Jy ! Total flux subtracted in 200 components = 0.0810856 Jy ! Clean residual min=-0.024714 max=0.020798 Jy/beam ! Clean residual mean=0.000018 rms=0.004521 Jy/beam ! Combined flux in latest and established models = 1.08274 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 31 components and 1.08274 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=0.200802Jy sigma=1.359810 ! Fit after self-cal, rms=0.200696Jy sigma=1.358687 ! Inverting map ! Your choice of large map pixels excluded 7.45% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6351 x 1.021 at -10.89 degrees (North through East) ! Clean map min=-0.018208 max=0.89097 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 54 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* ! ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.15 MC 1.03 NL 1.10 ! ON 1.08 SC 1.00 ZC 0.76 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 EF 1.00* FD 0.97 KP 0.98 ! LA 1.03 MC 0.99 NL 0.92 ON 1.01 ! OV 0.98 PT 0.95 SC 0.92 ZC 0.76 ! ! Telescope amplitude corrections in sub-array 4: ! EF 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.94 KP 0.95 MC 1.03 MK 1.01 ! ON 1.02 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.94 FD 0.96 KP 0.98 LA 1.06 ! MK 0.98 NL 0.94 PT 0.96 ! ! Telescope amplitude corrections in sub-array 7: ! EF 1.00* HH 0.90 MC 1.02 ON 1.06 ! SC 0.95 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.97 EF 1.00* FD 0.98 KP 1.01 ! LA 1.05 NL 0.94 ON 1.06 OV 1.01 ! PT 0.97 SC 0.91 ZC 0.77 ! ! ! Correcting IF 2. ! A total of 54 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* ! ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.14 MC 0.97 NL 1.26 ! ON 0.99 SC 0.98 ZC 0.83 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 EF 1.00* FD 1.01 KP 1.01 ! LA 1.04 MC 1.04 NL 0.94 ON 0.98 ! OV 1.00 PT 1.03 SC 0.98 ZC 0.80 ! ! Telescope amplitude corrections in sub-array 4: ! EF 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.98 KP 0.99 MC 1.09 MK 1.04 ! ON 1.07 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.98 FD 1.00 KP 0.99 LA 1.07 ! MK 1.01 NL 0.97 PT 1.01 ! ! Telescope amplitude corrections in sub-array 7: ! EF 1.00* HH 0.90 MC 1.08 ON 0.99 ! SC 1.03 ZC 0.79 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.01 EF 1.00* FD 1.04 KP 1.03 ! LA 1.07 NL 0.97 ON 1.03 OV 1.03 ! PT 1.04 SC 0.94 ZC 0.80 ! ! ! Correcting IF 3. ! A total of 54 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* ! ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.08 MC 1.04 NL 1.16 ! ON 1.09 SC 1.04 ZC 0.73 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 EF 1.00* FD 0.99 KP 0.95 ! LA 0.97 MC 1.01 NL 0.93 ON 1.02 ! OV 0.98 PT 1.00 SC 1.00 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 4: ! EF 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.95 KP 0.94 MC 1.08 MK 1.02 ! ON 0.98 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.98 FD 0.98 KP 0.93 LA 1.00 ! MK 0.94 NL 0.94 PT 1.00 ! ! Telescope amplitude corrections in sub-array 7: ! EF 1.00* HH 0.92 MC 1.03 ON 1.02 ! SC 0.95 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.00 EF 1.00* FD 1.01 KP 0.98 ! LA 1.01 NL 0.95 ON 1.04 OV 0.99 ! PT 1.01 SC 0.98 ZC 0.79 ! ! ! Correcting IF 4. ! A total of 54 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* ! ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.07 MC 1.00 NL 1.20 ! ON 0.98 SC 1.07 ZC 0.80 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 EF 1.00* FD 1.00 KP 0.99 ! LA 1.00 MC 1.06 NL 0.95 ON 1.00 ! OV 0.98 PT 1.02 SC 1.00 ZC 0.79 ! ! Telescope amplitude corrections in sub-array 4: ! EF 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.98 KP 0.93 MC 1.09 MK 1.03 ! ON 1.04 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.98 FD 1.00 KP 0.96 LA 1.01 ! MK 0.98 NL 0.96 PT 1.02 ! ! Telescope amplitude corrections in sub-array 7: ! EF 1.00* HH 0.90 MC 1.05 ON 0.99 ! SC 1.01 ZC 0.83 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.01 EF 1.00* FD 1.03 KP 1.00 ! LA 1.03 NL 0.98 ON 1.06 OV 0.99 ! PT 1.04 SC 0.97 ZC 0.78 ! ! ! Correcting IF 5. ! A total of 54 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* ! ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.09 MC 1.28 NL 1.18 ! ON 31.80 SC 1.05 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.02 KP 0.90 ! LA 0.98 MC 1.35 NL 0.99 ON 1.25 ! OV 1.03 PT 0.97 SC 1.02 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 4: ! EF 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* KP 0.81 MC 1.51 MK 1.11 ! ON 1.40 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* FD 1.01 KP 0.88 LA 1.01 ! MK 1.00 NL 0.97 PT 1.00 ! ! Telescope amplitude corrections in sub-array 7: ! EF 1.00* HH 0.94 MC 1.31 ON 1.35 ! SC 1.00 ZC 0.82 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.00* EF 1.00* FD 1.03 KP 0.92 ! LA 0.99 NL 1.00 ON 1.30 OV 1.06 ! PT 1.01 SC 0.98 ZC 0.84 ! ! ! Correcting IF 6. ! A total of 54 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* ! ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.14 MC 1.25 NL 1.14 ! ON 15.67 SC 0.98 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.01 KP 0.87 ! LA 0.99 MC 1.36 NL 0.99 ON 1.28 ! OV 1.04 PT 0.94 SC 0.99 ZC 0.80 ! ! Telescope amplitude corrections in sub-array 4: ! EF 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* KP 0.76 MC 1.46 MK 1.18 ! ON 1.37 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* FD 1.01 KP 0.87 LA 1.00 ! MK 1.00 NL 0.98 PT 0.95 ! ! Telescope amplitude corrections in sub-array 7: ! EF 1.00* HH 0.92 MC 1.35 ON 1.31 ! SC 0.96 ZC 0.84 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.00* EF 1.00* FD 1.03 KP 0.90 ! LA 1.02 NL 0.99 ON 1.37 OV 1.06 ! PT 0.97 SC 0.96 ZC 0.80 ! ! ! Correcting IF 7. ! A total of 54 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* ! ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.26 MC 1.36 NL 1.31 ! ON 19.51 SC 1.10 ZC 0.65 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 EF 1.00* FD 1.04 KP 0.93 ! LA 1.04 MC 1.39 NL 1.01 ON 1.32 ! OV 0.99 PT 1.01 SC 0.99 ZC 0.65 ! ! Telescope amplitude corrections in sub-array 4: ! EF 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.98 KP 0.88 MC 1.54 MK 1.13 ! ON 1.39 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 FD 1.05 KP 0.88 LA 1.06 ! MK 1.10 NL 1.02 PT 1.01 ! ! Telescope amplitude corrections in sub-array 7: ! EF 1.00* HH 1.21 MC 1.37 ON 1.31 ! SC 1.03 ZC 0.63 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.01 EF 1.00* FD 1.07 KP 0.95 ! LA 1.05 NL 1.03 ON 1.39 OV 1.00 ! PT 1.03 SC 1.00 ZC 0.65 ! ! ! Correcting IF 8. ! A total of 54 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* ! ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.25 MC 1.29 NL 1.18 ! ON 25.51 SC 1.05 ZC 0.66 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 EF 1.00* FD 1.04 KP 0.92 ! LA 1.04 MC 1.41 NL 0.99 ON 1.38 ! OV 0.98 PT 1.00 SC 1.02 ZC 0.61 ! ! Telescope amplitude corrections in sub-array 4: ! EF 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 KP 0.90 MC 1.59 MK 1.09 ! ON 1.45 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00 FD 1.04 KP 0.91 LA 1.05 ! MK 1.05 NL 1.00 PT 1.00 ! ! Telescope amplitude corrections in sub-array 7: ! EF 1.00* HH 1.10 MC 1.43 ON 1.31 ! SC 1.06 ZC 0.59 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.01 EF 1.00* FD 1.04 KP 0.94 ! LA 1.06 NL 1.00 ON 1.41 OV 1.00 ! PT 1.04 SC 0.98 ZC 0.60 ! ! ! Fit before self-cal, rms=0.200696Jy sigma=1.358687 ! Fit after self-cal, rms=0.336852Jy sigma=0.759035 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! Estimated beam: bmin=0.6251 mas, bmaj=1.159 mas, bpa=-10.13 degrees ! Estimated noise=1.05734 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, 2.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00672442 Jy ! Component: 100 - total flux cleaned = 0.00745438 Jy ! Component: 150 - total flux cleaned = 0.00786871 Jy ! Component: 200 - total flux cleaned = 0.00823471 Jy ! Total flux subtracted in 200 components = 0.00823471 Jy ! Clean residual min=-0.005033 max=0.005451 Jy/beam ! Clean residual mean=0.000005 rms=0.001001 Jy/beam ! Combined flux in latest and established models = 1.09097 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 41 components and 1.09097 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=0.336438Jy sigma=0.748180 ! Fit after self-cal, rms=0.344369Jy sigma=0.746951 ! Inverting map ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! Added new window around map position (0.6, 6.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00278199 Jy ! Component: 100 - total flux cleaned = 0.00387845 Jy ! Component: 150 - total flux cleaned = 0.00387975 Jy ! Component: 200 - total flux cleaned = 0.00387888 Jy ! Total flux subtracted in 200 components = 0.00387888 Jy ! Clean residual min=-0.004950 max=0.004172 Jy/beam ! Clean residual mean=0.000005 rms=0.000927 Jy/beam ! Combined flux in latest and established models = 1.09485 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 51 components and 1.09485 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=0.344240Jy sigma=0.742904 ! Fit after self-cal, rms=0.344300Jy sigma=0.742773 ! Inverting map ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 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=0.344300Jy sigma=0.742773 ! Fit after self-cal, rms=0.355252Jy sigma=0.740056 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! Estimated beam: bmin=0.625 mas, bmaj=1.158 mas, bpa=-10.18 degrees ! Estimated noise=1.05688 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00243604 Jy ! Component: 100 - total flux cleaned = 0.00316078 Jy ! Component: 150 - total flux cleaned = 0.00353338 Jy ! Component: 200 - total flux cleaned = 0.00364634 Jy ! Total flux subtracted in 200 components = 0.00364634 Jy ! Clean residual min=-0.004267 max=0.003808 Jy/beam ! Clean residual mean=0.000007 rms=0.000842 Jy/beam ! Combined flux in latest and established models = 1.0985 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 56 components and 1.0985 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=0.355123Jy sigma=0.736867 ! Fit after self-cal, rms=0.356052Jy sigma=0.736755 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 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 = 7.64315e-05 Jy ! Component: 100 - total flux cleaned = 7.69776e-05 Jy ! Component: 150 - total flux cleaned = -1.32022e-05 Jy ! Component: 200 - total flux cleaned = -1.30623e-05 Jy ! Total flux subtracted in 200 components = -1.30623e-05 Jy ! Clean residual min=-0.004178 max=0.003609 Jy/beam ! Clean residual mean=0.000007 rms=0.000817 Jy/beam ! Combined flux in latest and established models = 1.09848 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 60 components and 1.09848 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=0.356001Jy sigma=0.735438 ! Fit after self-cal, rms=0.356124Jy sigma=0.735396 ! Inverting map ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 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=0.356124Jy sigma=0.735396 ! Fit after self-cal, rms=0.361825Jy sigma=0.734493 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! Estimated beam: bmin=0.6248 mas, bmaj=1.158 mas, bpa=-10.2 degrees ! Estimated noise=1.0565 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00117132 Jy ! Component: 100 - total flux cleaned = 0.00136627 Jy ! Component: 150 - total flux cleaned = 0.0012801 Jy ! Component: 200 - total flux cleaned = 0.00120226 Jy ! Total flux subtracted in 200 components = 0.00120226 Jy ! Clean residual min=-0.003775 max=0.003508 Jy/beam ! Clean residual mean=0.000007 rms=0.000782 Jy/beam ! Combined flux in latest and established models = 1.09968 Jy selfcal ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 66 components and 1.09968 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=0.361764Jy sigma=0.733210 ! Fit after self-cal, rms=0.362151Jy sigma=0.733175 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 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 = -9.02696e-05 Jy ! Component: 100 - total flux cleaned = -8.86694e-05 Jy ! Component: 150 - total flux cleaned = -0.000153115 Jy ! Component: 200 - total flux cleaned = -0.000216026 Jy ! Total flux subtracted in 200 components = -0.000216026 Jy ! Clean residual min=-0.003719 max=0.003423 Jy/beam ! Clean residual mean=0.000007 rms=0.000768 Jy/beam ! Combined flux in latest and established models = 1.09947 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 70 components and 1.09947 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=0.362122Jy sigma=0.732574 ! Fit after self-cal, rms=0.362199Jy sigma=0.732560 ! Inverting map ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 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=0.362199Jy sigma=0.732560 ! Fit after self-cal, rms=0.366278Jy sigma=0.732217 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! Estimated beam: bmin=2.884 mas, bmaj=2.948 mas, bpa=16.5 degrees ! Estimated noise=1.29737 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00011777 Jy ! Component: 100 - total flux cleaned = -0.00020392 Jy ! Component: 150 - total flux cleaned = -0.000270161 Jy ! Component: 200 - total flux cleaned = -0.000296455 Jy ! Total flux subtracted in 200 components = -0.000296455 Jy ! Clean residual min=-0.003254 max=0.003301 Jy/beam ! Clean residual mean=0.000018 rms=0.000846 Jy/beam ! Combined flux in latest and established models = 1.09917 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 87 components and 1.09917 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=0.366283Jy sigma=0.732111 ! Fit after self-cal, rms=0.366508Jy sigma=0.732091 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 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 = -0.000186224 Jy ! Component: 100 - total flux cleaned = -0.000185796 Jy ! Component: 150 - total flux cleaned = -0.000186067 Jy ! Component: 200 - total flux cleaned = -0.000242197 Jy ! Total flux subtracted in 200 components = -0.000242197 Jy ! Clean residual min=-0.003247 max=0.003320 Jy/beam ! Clean residual mean=0.000018 rms=0.000839 Jy/beam ! Combined flux in latest and established models = 1.09893 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 95 components and 1.09893 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=0.366504Jy sigma=0.732065 ! Fit after self-cal, rms=0.366548Jy sigma=0.732056 ! Inverting map ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 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 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! Estimated beam: bmin=0.6245 mas, bmaj=1.157 mas, bpa=-10.22 degrees ! Estimated noise=1.05617 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6245 x 1.157 at -10.22 degrees (North through East) ! Clean map min=-0.0067655 max=0.88887 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 ! Performing amp+phase self-cal ! ! 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=0.366548Jy sigma=0.732056 ! Fit after self-cal, rms=0.732533Jy sigma=0.611660 ! Inverting map and beam ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! Estimated beam: bmin=0.6244 mas, bmaj=1.158 mas, bpa=-10.2 degrees ! Estimated noise=1.05667 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000866518 Jy ! Component: 100 - total flux cleaned = 0.000733845 Jy ! Component: 150 - total flux cleaned = 0.000735208 Jy ! Component: 200 - total flux cleaned = 0.0006778 Jy ! Total flux subtracted in 200 components = 0.0006778 Jy ! Clean residual min=-0.003241 max=0.003336 Jy/beam ! Clean residual mean=0.000007 rms=0.000719 Jy/beam ! Combined flux in latest and established models = 1.09961 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 105 components and 1.09961 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=0.732501Jy sigma=0.611060 ! Fit after self-cal, rms=0.732536Jy sigma=0.611046 ! Inverting map ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! Added new window around map position (-8.6, -2.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00223033 Jy ! Component: 100 - total flux cleaned = 0.00270303 Jy ! Component: 150 - total flux cleaned = 0.00299777 Jy ! Component: 200 - total flux cleaned = 0.00299765 Jy ! Total flux subtracted in 200 components = 0.00299765 Jy ! Clean residual min=-0.003096 max=0.003350 Jy/beam ! Clean residual mean=0.000006 rms=0.000701 Jy/beam ! Combined flux in latest and established models = 1.10261 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 112 components and 1.10261 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=0.732528Jy sigma=0.610143 ! Fit after self-cal, rms=0.732537Jy sigma=0.610087 ! Inverting map ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! Added new window around map position (42.8, -37.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00227901 Jy ! Component: 100 - total flux cleaned = 0.00271879 Jy ! Component: 150 - total flux cleaned = 0.00294347 Jy ! Component: 200 - total flux cleaned = 0.00294187 Jy ! Total flux subtracted in 200 components = 0.00294187 Jy ! Clean residual min=-0.003180 max=0.003040 Jy/beam ! Clean residual mean=0.000005 rms=0.000679 Jy/beam ! Combined flux in latest and established models = 1.10555 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 123 components and 1.10555 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=0.732491Jy sigma=0.609343 ! Fit after self-cal, rms=0.732394Jy sigma=0.609298 ! Inverting map ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! Performing amp+phase self-cal ! ! 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=0.732394Jy sigma=0.609298 ! Fit after self-cal, rms=0.729375Jy sigma=0.609087 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 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! Estimated beam: bmin=0.4934 mas, bmaj=0.9616 mas, bpa=-10.86 degrees ! Estimated noise=1.65428 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.667917 Jy ! Component: 100 - total flux cleaned = 0.85436 Jy ! Component: 150 - total flux cleaned = 0.945684 Jy ! Component: 200 - total flux cleaned = 0.995175 Jy ! Total flux subtracted in 200 components = 0.995175 Jy ! Clean residual min=-0.011363 max=0.024264 Jy/beam ! Clean residual mean=0.000012 rms=0.002444 Jy/beam ! Combined flux in latest and established models = 0.995175 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 16 model components to the UV plane model. ! The established model now contains 16 components and 0.995175 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! Estimated beam: bmin=0.6243 mas, bmaj=1.157 mas, bpa=-10.19 degrees ! Estimated noise=1.05702 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 = 0.0423656 Jy ! Component: 100 - total flux cleaned = 0.0648115 Jy ! Component: 150 - total flux cleaned = 0.0787163 Jy ! Component: 200 - total flux cleaned = 0.0880487 Jy ! Total flux subtracted in 200 components = 0.0880487 Jy ! Clean residual min=-0.004633 max=0.006596 Jy/beam ! Clean residual mean=0.000007 rms=0.000985 Jy/beam ! Combined flux in latest and established models = 1.08322 Jy ! Adding 38 model components to the UV plane model. ! The established model now contains 44 components and 1.08322 Jy ! Inverting map ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! Added new window around map position (0.4, 1.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00685638 Jy ! Component: 100 - total flux cleaned = 0.011759 Jy ! Component: 150 - total flux cleaned = 0.0149754 Jy ! Component: 200 - total flux cleaned = 0.0162225 Jy ! Total flux subtracted in 200 components = 0.0162225 Jy ! Clean residual min=-0.004340 max=0.003825 Jy/beam ! Clean residual mean=0.000005 rms=0.000784 Jy/beam ! Combined flux in latest and established models = 1.09945 Jy ! Adding 23 model components to the UV plane model. ! The established model now contains 60 components and 1.09945 Jy ! Inverting map ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 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 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! Estimated beam: bmin=2.885 mas, bmaj=2.948 mas, bpa=16.55 degrees ! Estimated noise=1.29796 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0022899 Jy ! Component: 100 - total flux cleaned = 0.00363771 Jy ! Component: 150 - total flux cleaned = 0.00440001 Jy ! Component: 200 - total flux cleaned = 0.00487935 Jy ! Total flux subtracted in 200 components = 0.00487935 Jy ! Clean residual min=-0.003788 max=0.002798 Jy/beam ! Clean residual mean=0.000011 rms=0.000779 Jy/beam ! Combined flux in latest and established models = 1.10433 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 = 0.000370228 Jy ! Component: 100 - total flux cleaned = 0.00070764 Jy ! Component: 150 - total flux cleaned = 0.000976588 Jy ! Component: 200 - total flux cleaned = 0.00122698 Jy ! Total flux subtracted in 200 components = 0.00122698 Jy ! Clean residual min=-0.003451 max=0.002631 Jy/beam ! Clean residual mean=0.000011 rms=0.000755 Jy/beam ! Combined flux in latest and established models = 1.10555 Jy ! Adding 43 model components to the UV plane model. ! The established model now contains 95 components and 1.10555 Jy ! Inverting map ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! Estimated beam: bmin=0.6243 mas, bmaj=1.157 mas, bpa=-10.19 degrees ! Estimated noise=1.05702 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00102954 Jy ! Component: 100 - total flux cleaned = -0.000921321 Jy ! Component: 150 - total flux cleaned = -0.000531682 Jy ! Component: 200 - total flux cleaned = -0.000440178 Jy ! Total flux subtracted in 200 components = -0.000440178 Jy ! Clean residual min=-0.003703 max=0.003408 Jy/beam ! Clean residual mean=0.000004 rms=0.000725 Jy/beam ! Combined flux in latest and established models = 1.10511 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 107 components and 1.10511 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=0.729851Jy sigma=0.609961 ! Fit after self-cal, rms=0.727079Jy sigma=0.609117 wmodel /scr/pima/gb073_uvs/J2212+2355_X_map.mod ! Writing 107 model components to file: /scr/pima/gb073_uvs/J2212+2355_X_map.mod wobs /scr/pima/gb073_uvs/J2212+2355_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J2212+2355_X_uvs.fits wwins /scr/pima/gb073_uvs/J2212+2355_X_map.win ! wwins: Wrote 7 windows to /scr/pima/gb073_uvs/J2212+2355_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 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00114837 Jy ! Component: 100 - total flux cleaned = -0.00138193 Jy ! Component: 150 - total flux cleaned = -0.00182812 Jy ! Component: 200 - total flux cleaned = -0.00225937 Jy ! Component: 250 - total flux cleaned = -0.00267758 Jy ! Component: 300 - total flux cleaned = -0.003085 Jy ! Component: 350 - total flux cleaned = -0.00353281 Jy ! Component: 400 - total flux cleaned = -0.0037768 Jy ! Component: 450 - total flux cleaned = -0.00416093 Jy ! Component: 500 - total flux cleaned = -0.00430244 Jy ! Component: 550 - total flux cleaned = -0.00439528 Jy ! Component: 600 - total flux cleaned = -0.00444157 Jy ! Component: 650 - total flux cleaned = -0.00453214 Jy ! Component: 700 - total flux cleaned = -0.00453196 Jy ! Component: 750 - total flux cleaned = -0.00461915 Jy ! Component: 800 - total flux cleaned = -0.00461939 Jy ! Component: 850 - total flux cleaned = -0.00466176 Jy ! Component: 900 - total flux cleaned = -0.00461905 Jy ! Component: 950 - total flux cleaned = -0.0046192 Jy ! Component: 1000 - total flux cleaned = -0.00466032 Jy ! Component: 1050 - total flux cleaned = -0.00466004 Jy ! Component: 1100 - total flux cleaned = -0.00466014 Jy ! Component: 1150 - total flux cleaned = -0.00470014 Jy ! Component: 1200 - total flux cleaned = -0.00466085 Jy ! Component: 1250 - total flux cleaned = -0.00462144 Jy ! Component: 1300 - total flux cleaned = -0.00458228 Jy ! Component: 1350 - total flux cleaned = -0.00462127 Jy ! Component: 1400 - total flux cleaned = -0.00465987 Jy ! Component: 1450 - total flux cleaned = -0.00458322 Jy ! Component: 1500 - total flux cleaned = -0.00465895 Jy ! Component: 1550 - total flux cleaned = -0.00462129 Jy ! Component: 1600 - total flux cleaned = -0.00458398 Jy ! Component: 1650 - total flux cleaned = -0.00462133 Jy ! Component: 1700 - total flux cleaned = -0.00465775 Jy ! Component: 1750 - total flux cleaned = -0.00480387 Jy ! Component: 1800 - total flux cleaned = -0.00473112 Jy ! Component: 1850 - total flux cleaned = -0.00469502 Jy ! Component: 1900 - total flux cleaned = -0.0048739 Jy ! Component: 1950 - total flux cleaned = -0.0047674 Jy ! Component: 2000 - total flux cleaned = -0.00487358 Jy ! Component: 2050 - total flux cleaned = -0.00501372 Jy ! Component: 2100 - total flux cleaned = -0.00504859 Jy ! Component: 2150 - total flux cleaned = -0.00511733 Jy ! Component: 2200 - total flux cleaned = -0.00508279 Jy ! Component: 2250 - total flux cleaned = -0.00508283 Jy ! Component: 2300 - total flux cleaned = -0.00521789 Jy ! Component: 2350 - total flux cleaned = -0.00515044 Jy ! Component: 2400 - total flux cleaned = -0.00515027 Jy ! Component: 2450 - total flux cleaned = -0.00505042 Jy ! Component: 2500 - total flux cleaned = -0.00505058 Jy ! Component: 2550 - total flux cleaned = -0.00498488 Jy ! Component: 2600 - total flux cleaned = -0.00485403 Jy ! Component: 2650 - total flux cleaned = -0.00475666 Jy ! Component: 2700 - total flux cleaned = -0.00472451 Jy ! Component: 2750 - total flux cleaned = -0.00466057 Jy ! Component: 2800 - total flux cleaned = -0.00453279 Jy ! Component: 2850 - total flux cleaned = -0.00459613 Jy ! Component: 2900 - total flux cleaned = -0.0044698 Jy ! Component: 2950 - total flux cleaned = -0.00428125 Jy ! Component: 3000 - total flux cleaned = -0.00421918 Jy ! Component: 3050 - total flux cleaned = -0.00406386 Jy ! Component: 3100 - total flux cleaned = -0.0040022 Jy ! Component: 3150 - total flux cleaned = -0.00397145 Jy ! Component: 3200 - total flux cleaned = -0.00391087 Jy ! Component: 3250 - total flux cleaned = -0.00378937 Jy ! Component: 3300 - total flux cleaned = -0.00363844 Jy ! Component: 3350 - total flux cleaned = -0.0036384 Jy ! Component: 3400 - total flux cleaned = -0.00351852 Jy ! Component: 3450 - total flux cleaned = -0.00345914 Jy ! Component: 3500 - total flux cleaned = -0.00322221 Jy ! Component: 3550 - total flux cleaned = -0.00316334 Jy ! Component: 3600 - total flux cleaned = -0.00310505 Jy ! Component: 3650 - total flux cleaned = -0.00293017 Jy ! Component: 3700 - total flux cleaned = -0.00287221 Jy ! Component: 3750 - total flux cleaned = -0.00267019 Jy ! Component: 3800 - total flux cleaned = -0.00249813 Jy ! Component: 3850 - total flux cleaned = -0.00238391 Jy ! Component: 3900 - total flux cleaned = -0.0022706 Jy ! Component: 3950 - total flux cleaned = -0.00210087 Jy ! Component: 4000 - total flux cleaned = -0.00198838 Jy ! Component: 4050 - total flux cleaned = -0.00179239 Jy ! Total flux subtracted in 4096 components = -0.00176439 Jy ! Clean residual min=-0.001652 max=0.001626 Jy/beam ! Clean residual mean=0.000002 rms=0.000443 Jy/beam ! Combined flux in latest and established models = 1.10335 Jy keep ! Adding 288 model components to the UV plane model. ! The established model now contains 395 components and 1.10335 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J2212+2355_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6243 x 1.157 at -10.19 degrees (North through East) ! Clean map min=-0.0031183 max=0.8945 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J2212+2355_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.894501 invert ! Inverting map ! Your choice of large map pixels excluded 7.92% of the data. ! The x-axis pixel size should ideally be below 0.166 milli-arcsec ! The y-axis pixel size should ideally be below 0.195 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00044268 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.148467 0.148467 0.296934 0.593869 1.18774 2.37548 4.75095 9.5019 19.0038 38.0076 76.0152 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0013 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.894 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 2020.65 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J2212+2355_X_uvs.log closed on Sat Dec 26 09:45:28 2015