! Started logfile: /scr/pima/gb073_uvs/J2130+3332_X_uvs.log on Sat Dec 26 09:45:09 2015 obs /scr/pima/gb073_uvs/J2130+3332_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J2130+3332_X_uva.fits ! AN table 1: 23 integrations on 6 of 6 possible baselines. ! AN table 2: 29 integrations on 55 of 55 possible baselines. ! AN table 3: 58 integrations on 36 of 36 possible baselines. ! AN table 4: 29 integrations on 66 of 66 possible baselines. ! AN table 5: 29 integrations on 55 of 55 possible baselines. ! AN table 6: 29 integrations on 10 of 10 possible baselines. ! AN table 7: 29 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.778162 visibilities/baseline/integration-bin. ! Found source: J2130+3332 ! ! 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 59352 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/J2130+3332_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 92 telescope corrections were flagged in sub-array 1. ! A total of 37 telescope corrections were flagged in sub-array 2. ! A total of 35 telescope corrections were flagged in sub-array 4. ! A total of 30 telescope corrections were flagged in sub-array 5. ! A total of 35 telescope corrections were flagged in sub-array 6. ! A total of 59 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 2. ! A total of 92 telescope corrections were flagged in sub-array 1. ! A total of 37 telescope corrections were flagged in sub-array 2. ! A total of 35 telescope corrections were flagged in sub-array 4. ! A total of 30 telescope corrections were flagged in sub-array 5. ! A total of 35 telescope corrections were flagged in sub-array 6. ! A total of 59 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 3. ! A total of 92 telescope corrections were flagged in sub-array 1. ! A total of 37 telescope corrections were flagged in sub-array 2. ! A total of 35 telescope corrections were flagged in sub-array 4. ! A total of 30 telescope corrections were flagged in sub-array 5. ! A total of 35 telescope corrections were flagged in sub-array 6. ! A total of 59 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 4. ! A total of 92 telescope corrections were flagged in sub-array 1. ! A total of 37 telescope corrections were flagged in sub-array 2. ! A total of 35 telescope corrections were flagged in sub-array 4. ! A total of 30 telescope corrections were flagged in sub-array 5. ! A total of 35 telescope corrections were flagged in sub-array 6. ! A total of 59 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 5. ! A total of 92 telescope corrections were flagged in sub-array 1. ! A total of 66 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 64 telescope corrections were flagged in sub-array 4. ! A total of 58 telescope corrections were flagged in sub-array 5. ! A total of 35 telescope corrections were flagged in sub-array 6. ! A total of 88 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 6. ! A total of 92 telescope corrections were flagged in sub-array 1. ! A total of 66 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 64 telescope corrections were flagged in sub-array 4. ! A total of 58 telescope corrections were flagged in sub-array 5. ! A total of 35 telescope corrections were flagged in sub-array 6. ! A total of 88 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 7. ! A total of 92 telescope corrections were flagged in sub-array 1. ! A total of 37 telescope corrections were flagged in sub-array 2. ! A total of 35 telescope corrections were flagged in sub-array 4. ! A total of 30 telescope corrections were flagged in sub-array 5. ! A total of 35 telescope corrections were flagged in sub-array 6. ! A total of 59 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 8. ! A total of 92 telescope corrections were flagged in sub-array 1. ! A total of 37 telescope corrections were flagged in sub-array 2. ! A total of 35 telescope corrections were flagged in sub-array 4. ! A total of 30 telescope corrections were flagged in sub-array 5. ! A total of 35 telescope corrections were flagged in sub-array 6. ! A total of 59 telescope corrections were flagged in sub-array 7. ! ! Fit before self-cal, rms=1.004938Jy sigma=10.330434 ! Fit after self-cal, rms=0.942750Jy sigma=9.696806 ! 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 4.24% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.5577 mas, bmaj=1.1 mas, bpa=-16.25 degrees ! Estimated noise=0.727423 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 = 0.0420351 Jy ! Component: 100 - total flux cleaned = 0.0529816 Jy ! Total flux subtracted in 100 components = 0.0529816 Jy ! Clean residual min=-0.002539 max=0.006093 Jy/beam ! Clean residual mean=0.000003 rms=0.000600 Jy/beam ! Combined flux in latest and established models = 0.0529816 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.0529816 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=0.076892Jy sigma=0.687179 ! Fit after self-cal, rms=0.075827Jy sigma=0.676576 ! Inverting map ! Your choice of large map pixels excluded 4.24% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Added new window around map position (0.6, -0.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0071103 Jy ! Component: 100 - total flux cleaned = 0.0114644 Jy ! Total flux subtracted in 100 components = 0.0114644 Jy ! Clean residual min=-0.002231 max=0.002848 Jy/beam ! Clean residual mean=0.000003 rms=0.000542 Jy/beam ! Combined flux in latest and established models = 0.064446 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 12 components and 0.064446 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=0.074692Jy sigma=0.661758 ! Fit after self-cal, rms=0.074647Jy sigma=0.661405 ! Inverting map ! Your choice of large map pixels excluded 4.24% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00336426 Jy ! Component: 100 - total flux cleaned = 0.0053846 Jy ! Total flux subtracted in 100 components = 0.0053846 Jy ! Clean residual min=-0.002272 max=0.002590 Jy/beam ! Clean residual mean=0.000003 rms=0.000530 Jy/beam ! Combined flux in latest and established models = 0.0698306 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 16 components and 0.0698306 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=0.074375Jy sigma=0.658051 ! Fit after self-cal, rms=0.074359Jy sigma=0.657935 ! Inverting map ! Your choice of large map pixels excluded 4.24% of the data. ! The x-axis pixel size should ideally be below 0.1679 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 4.24% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.7913 mas, bmaj=1.418 mas, bpa=-13.1 degrees ! Estimated noise=0.310228 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, 0). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00365528 Jy ! Component: 100 - total flux cleaned = 0.0054738 Jy ! Component: 150 - total flux cleaned = 0.00631971 Jy ! Component: 200 - total flux cleaned = 0.0066252 Jy ! Total flux subtracted in 200 components = 0.0066252 Jy ! Clean residual min=-0.001281 max=0.001851 Jy/beam ! Clean residual mean=0.000006 rms=0.000260 Jy/beam ! Combined flux in latest and established models = 0.0764558 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 31 components and 0.0764557 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=0.074196Jy sigma=0.655983 ! Fit after self-cal, rms=0.074156Jy sigma=0.655578 ! Inverting map ! Your choice of large map pixels excluded 4.24% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00136963 Jy ! Component: 100 - total flux cleaned = 0.00148951 Jy ! Component: 150 - total flux cleaned = 0.00144719 Jy ! Component: 200 - total flux cleaned = 0.00144724 Jy ! Total flux subtracted in 200 components = 0.00144724 Jy ! Clean residual min=-0.001266 max=0.001169 Jy/beam ! Clean residual mean=0.000006 rms=0.000249 Jy/beam ! Combined flux in latest and established models = 0.077903 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 38 components and 0.077903 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=0.074128Jy sigma=0.655240 ! Fit after self-cal, rms=0.074120Jy sigma=0.655138 ! Inverting map ! Your choice of large map pixels excluded 4.24% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7913 x 1.418 at -13.1 degrees (North through East) ! Clean map min=-0.0011722 max=0.057797 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val ! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2. ! Selfcal phase corrections will not be limited. gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 FD 0.95 KP 0.93 LA 1.05 ! MK 1.02 NL 0.94 OV 0.99 PT 0.95 ! SC 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.92 EF 1.00* FD 0.95 KP 0.98 ! LA 1.00 MC 0.93 MK 1.00 NL 1.00 ! ON 1.03 PT 0.94 SC 0.95 ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* MC 1.00* ON 1.00* SC 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 0.98 EF 1.00* FD 0.93 KP 1.06 ! LA 1.04 MC 0.89 MK 1.17 NL 0.99 ! ON 1.00* OV 1.03 PT 0.91 SC 0.97 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 FD 1.04 KP 1.02 LA 1.06 ! MK 1.06 NL 0.95 OV 1.01 PT 1.00 ! SC 1.02 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 EF 1.00* FD 1.02 KP 1.02 ! LA 1.10 MC 0.98 NL 1.01 ON 0.93 ! OV 1.01 PT 1.07 SC 1.10 ZC 0.85 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 EF 1.00* FD 1.02 KP 1.03 ! LA 1.08 MC 0.87 MK 1.02 NL 1.00 ! ON 0.97 PT 0.97 SC 1.05 ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* MC 1.00* ON 1.00* SC 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.12 EF 1.00* FD 1.03 KP 1.01 ! LA 0.97 MC 1.12 MK 1.08 NL 1.11 ! ON 1.00* OV 1.04 PT 0.98 SC 1.08 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 0.99 KP 0.96 LA 1.00 ! MK 0.99 NL 1.02 OV 1.01 PT 0.96 ! SC 1.00 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 EF 1.00* FD 0.95 KP 0.99 ! LA 1.01 MC 1.10 MK 0.93 NL 0.97 ! ON 0.99 PT 1.04 SC 1.02 ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* MC 1.00* ON 1.00* SC 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 0.99 EF 1.00* FD 0.98 KP 0.96 ! LA 0.96 MC 0.91 MK 1.07 NL 1.02 ! ON 1.00* OV 0.97 PT 0.99 SC 1.11 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.96 FD 1.01 KP 0.96 LA 1.00 ! MK 1.10 NL 1.04 OV 0.99 PT 1.04 ! SC 1.07 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 EF 1.00* FD 0.98 KP 1.03 ! LA 1.01 MC 0.93 NL 0.96 ON 0.85 ! OV 1.00 PT 1.03 SC 1.03 ZC 0.94 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 EF 1.00* FD 0.95 KP 0.98 ! LA 0.99 MC 0.92 MK 1.01 NL 1.03 ! ON 1.06 PT 1.02 SC 1.10 ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* MC 1.00* ON 1.00* SC 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.04 EF 1.00* FD 1.02 KP 1.03 ! LA 1.02 MC 1.10 MK 1.04 NL 1.03 ! ON 1.00* OV 1.04 PT 0.98 SC 1.01 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 0.98 KP 0.90 LA 0.99 ! MK 1.04 NL 1.03 OV 1.11 PT 0.95 ! SC 1.03 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.96 KP 0.96 ! LA 1.08 MC 1.17 NL 1.07 ON 0.97 ! OV 0.99 PT 0.99 SC 1.07 ZC 0.86 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.11 KP 0.94 ! LA 0.94 MC 1.11 MK 0.98 NL 1.01 ! ON 1.06 PT 0.95 SC 0.94 ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* MC 0.87 ON 0.85 SC 1.07 ! ZC 0.87 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* MK 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00 KP 0.88 LA 1.00 ! MK 1.00 NL 1.05 OV 1.09 PT 0.95 ! SC 1.02 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.09 KP 0.98 ! LA 1.01 MC 1.08 MK 0.92 NL 1.10 ! ON 1.13 PT 0.89 SC 0.94 ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* MC 1.00* ON 1.00* SC 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* EF 1.00* FD 1.11 KP 0.88 ! LA 1.02 MC 1.16 MK 0.96 NL 1.11 ! ON 1.00* OV 1.05 PT 0.91 SC 0.98 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.10 FD 1.05 KP 0.92 LA 1.11 ! MK 1.06 NL 1.01 OV 0.99 PT 0.99 ! SC 0.93 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* MK 1.00* NL 1.00* ! ON 1.00* PT 1.00* SC 1.00* ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* MC 1.00* ON 1.00* SC 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 0.95 EF 1.00* FD 0.92 KP 0.92 ! LA 1.09 MC 0.99 MK 1.03 NL 1.13 ! ON 1.00* OV 1.09 PT 1.12 SC 0.95 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.07 FD 1.04 KP 0.93 LA 1.04 ! MK 1.05 NL 1.02 OV 1.04 PT 1.01 ! SC 1.02 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* MK 1.00* NL 1.00* ! ON 1.00* PT 1.00* SC 1.00* ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* MC 1.00* ON 1.00* SC 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 0.97 EF 1.00* FD 0.97 KP 0.97 ! LA 1.00 MC 1.03 MK 1.05 NL 1.19 ! ON 1.00* OV 1.02 PT 1.05 SC 1.00 ! ! ! Fit before self-cal, rms=0.074120Jy sigma=0.655138 ! Fit after self-cal, rms=0.074629Jy sigma=0.654181 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.7932 mas, bmaj=1.425 mas, bpa=-12.83 degrees ! Estimated noise=0.312896 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 = 0.000289447 Jy ! Component: 100 - total flux cleaned = 0.000202585 Jy ! Component: 150 - total flux cleaned = 0.000114318 Jy ! Component: 200 - total flux cleaned = 0.000100875 Jy ! Total flux subtracted in 200 components = 0.000100875 Jy ! Clean residual min=-0.001138 max=0.000997 Jy/beam ! Clean residual mean=0.000006 rms=0.000229 Jy/beam ! Combined flux in latest and established models = 0.0780039 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 45 components and 0.0780039 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=0.074619Jy sigma=0.654111 ! Fit after self-cal, rms=0.074634Jy sigma=0.654004 ! Inverting map ! Your choice of large map pixels excluded 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 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=0.074634Jy sigma=0.654004 ! Fit after self-cal, rms=0.074640Jy sigma=0.653809 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.7927 mas, bmaj=1.425 mas, bpa=-12.83 degrees ! Estimated noise=0.313347 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000214779 Jy ! Component: 100 - total flux cleaned = 0.000184859 Jy ! Component: 150 - total flux cleaned = 0.000158382 Jy ! Component: 200 - total flux cleaned = 0.000146292 Jy ! Total flux subtracted in 200 components = 0.000146292 Jy ! Clean residual min=-0.001125 max=0.001014 Jy/beam ! Clean residual mean=0.000006 rms=0.000228 Jy/beam ! Combined flux in latest and established models = 0.0781502 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 49 components and 0.0781502 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=0.074634Jy sigma=0.653766 ! Fit after self-cal, rms=0.074636Jy sigma=0.653747 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 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 = 5.4036e-05 Jy ! Component: 100 - total flux cleaned = 2.88985e-05 Jy ! Component: 150 - total flux cleaned = 1.71515e-05 Jy ! Component: 200 - total flux cleaned = 5.91502e-06 Jy ! Total flux subtracted in 200 components = 5.91502e-06 Jy ! Clean residual min=-0.001117 max=0.001009 Jy/beam ! Clean residual mean=0.000006 rms=0.000228 Jy/beam ! Combined flux in latest and established models = 0.0781561 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 54 components and 0.0781561 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=0.074631Jy sigma=0.653710 ! Fit after self-cal, rms=0.074630Jy sigma=0.653704 ! Inverting map ! Your choice of large map pixels excluded 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 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=0.074630Jy sigma=0.653704 ! Fit after self-cal, rms=0.074908Jy sigma=0.653629 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.7929 mas, bmaj=1.427 mas, bpa=-12.78 degrees ! Estimated noise=0.314204 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000194542 Jy ! Component: 100 - total flux cleaned = 0.000145369 Jy ! Component: 150 - total flux cleaned = 0.000100191 Jy ! Component: 200 - total flux cleaned = 8.97947e-05 Jy ! Total flux subtracted in 200 components = 8.97947e-05 Jy ! Clean residual min=-0.001089 max=0.001020 Jy/beam ! Clean residual mean=0.000007 rms=0.000227 Jy/beam ! Combined flux in latest and established models = 0.0782459 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 55 components and 0.0782459 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=0.074903Jy sigma=0.653605 ! Fit after self-cal, rms=0.074907Jy sigma=0.653590 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 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 = 1.31975e-05 Jy ! Component: 100 - total flux cleaned = -8.70435e-06 Jy ! Component: 150 - total flux cleaned = -1.91612e-05 Jy ! Component: 200 - total flux cleaned = -2.94733e-05 Jy ! Total flux subtracted in 200 components = -2.94733e-05 Jy ! Clean residual min=-0.001081 max=0.001017 Jy/beam ! Clean residual mean=0.000006 rms=0.000227 Jy/beam ! Combined flux in latest and established models = 0.0782164 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 58 components and 0.0782164 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=0.074903Jy sigma=0.653562 ! Fit after self-cal, rms=0.074902Jy sigma=0.653556 ! Inverting map ! Your choice of large map pixels excluded 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 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=0.074902Jy sigma=0.653556 ! Fit after self-cal, rms=0.074977Jy sigma=0.653553 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=2.603 mas, bmaj=2.973 mas, bpa=-4.905 degrees ! Estimated noise=0.382194 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -6.95031e-05 Jy ! Component: 100 - total flux cleaned = -0.000139221 Jy ! Component: 150 - total flux cleaned = -0.000190127 Jy ! Component: 200 - total flux cleaned = -0.00023397 Jy ! Total flux subtracted in 200 components = -0.00023397 Jy ! Clean residual min=-0.001402 max=0.001063 Jy/beam ! Clean residual mean=0.000014 rms=0.000278 Jy/beam ! Combined flux in latest and established models = 0.0779824 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 69 components and 0.0779824 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=0.074974Jy sigma=0.653531 ! Fit after self-cal, rms=0.074973Jy sigma=0.653524 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 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 = 1.26208e-05 Jy ! Component: 100 - total flux cleaned = -1.84048e-05 Jy ! Component: 150 - total flux cleaned = -4.56267e-05 Jy ! Component: 200 - total flux cleaned = -7.58746e-05 Jy ! Total flux subtracted in 200 components = -7.58746e-05 Jy ! Clean residual min=-0.001404 max=0.001061 Jy/beam ! Clean residual mean=0.000014 rms=0.000278 Jy/beam ! Combined flux in latest and established models = 0.0779065 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 72 components and 0.0779066 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=0.074972Jy sigma=0.653511 ! Fit after self-cal, rms=0.074970Jy sigma=0.653505 ! Inverting map ! Your choice of large map pixels excluded 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 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 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.7927 mas, bmaj=1.427 mas, bpa=-12.75 degrees ! Estimated noise=0.314543 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7927 x 1.427 at -12.75 degrees (North through East) ! Clean map min=-0.00096903 max=0.058147 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 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.5573 mas, bmaj=1.105 mas, bpa=-15.75 degrees ! Estimated noise=0.740075 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0432892 Jy ! Component: 100 - total flux cleaned = 0.0564748 Jy ! Component: 150 - total flux cleaned = 0.0638587 Jy ! Component: 200 - total flux cleaned = 0.0686645 Jy ! Total flux subtracted in 200 components = 0.0686645 Jy ! Clean residual min=-0.002292 max=0.002599 Jy/beam ! Clean residual mean=0.000003 rms=0.000534 Jy/beam ! Combined flux in latest and established models = 0.0686645 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 13 model components to the UV plane model. ! The established model now contains 13 components and 0.0686645 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.7927 mas, bmaj=1.427 mas, bpa=-12.75 degrees ! Estimated noise=0.314543 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 = 0.00503819 Jy ! Component: 100 - total flux cleaned = 0.00761728 Jy ! Component: 150 - total flux cleaned = 0.00880292 Jy ! Component: 200 - total flux cleaned = 0.00914296 Jy ! Total flux subtracted in 200 components = 0.00914296 Jy ! Clean residual min=-0.001109 max=0.001042 Jy/beam ! Clean residual mean=0.000006 rms=0.000231 Jy/beam ! Combined flux in latest and established models = 0.0778075 Jy ! Adding 25 model components to the UV plane model. ! The established model now contains 32 components and 0.0778075 Jy ! Inverting map ! Your choice of large map pixels excluded 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 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 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=2.603 mas, bmaj=2.973 mas, bpa=-4.905 degrees ! Estimated noise=0.382194 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000161441 Jy ! Component: 100 - total flux cleaned = 0.000190678 Jy ! Component: 150 - total flux cleaned = 0.000158814 Jy ! Component: 200 - total flux cleaned = 0.000131029 Jy ! Total flux subtracted in 200 components = 0.000131029 Jy ! Clean residual min=-0.001430 max=0.001088 Jy/beam ! Clean residual mean=0.000014 rms=0.000278 Jy/beam ! Combined flux in latest and established models = 0.0779385 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 = -3.43619e-05 Jy ! Component: 100 - total flux cleaned = -5.33977e-05 Jy ! Component: 150 - total flux cleaned = -7.76593e-05 Jy ! Component: 200 - total flux cleaned = -9.83592e-05 Jy ! Total flux subtracted in 200 components = -9.83592e-05 Jy ! Clean residual min=-0.001421 max=0.001081 Jy/beam ! Clean residual mean=0.000014 rms=0.000277 Jy/beam ! Combined flux in latest and established models = 0.0778402 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 52 components and 0.0778402 Jy ! Inverting map ! Your choice of large map pixels excluded 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.7927 mas, bmaj=1.427 mas, bpa=-12.75 degrees ! Estimated noise=0.314543 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 4.24857e-06 Jy ! Component: 100 - total flux cleaned = 2.26846e-05 Jy ! Component: 150 - total flux cleaned = 3.96709e-05 Jy ! Component: 200 - total flux cleaned = 5.57166e-05 Jy ! Total flux subtracted in 200 components = 5.57166e-05 Jy ! Clean residual min=-0.001074 max=0.001014 Jy/beam ! Clean residual mean=0.000006 rms=0.000227 Jy/beam ! Combined flux in latest and established models = 0.0778959 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 62 components and 0.0778959 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=0.074987Jy sigma=0.653596 ! Fit after self-cal, rms=0.074970Jy sigma=0.653505 wmodel /scr/pima/gb073_uvs/J2130+3332_X_map.mod ! Writing 62 model components to file: /scr/pima/gb073_uvs/J2130+3332_X_map.mod wobs /scr/pima/gb073_uvs/J2130+3332_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J2130+3332_X_uvs.fits wwins /scr/pima/gb073_uvs/J2130+3332_X_map.win ! wwins: Wrote 3 windows to /scr/pima/gb073_uvs/J2130+3332_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 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -4.16075e-05 Jy ! Component: 100 - total flux cleaned = -4.09401e-05 Jy ! Component: 150 - total flux cleaned = -2.36518e-05 Jy ! Component: 200 - total flux cleaned = 4.2196e-05 Jy ! Component: 250 - total flux cleaned = 7.40687e-05 Jy ! Component: 300 - total flux cleaned = 0.000152202 Jy ! Component: 350 - total flux cleaned = 0.000228799 Jy ! Component: 400 - total flux cleaned = 0.000273976 Jy ! Component: 450 - total flux cleaned = 0.000408065 Jy ! Component: 500 - total flux cleaned = 0.000481414 Jy ! Component: 550 - total flux cleaned = 0.000641188 Jy ! Component: 600 - total flux cleaned = 0.000726964 Jy ! Component: 650 - total flux cleaned = 0.000868808 Jy ! Component: 700 - total flux cleaned = 0.000938892 Jy ! Component: 750 - total flux cleaned = 0.00106405 Jy ! Component: 800 - total flux cleaned = 0.00113295 Jy ! Component: 850 - total flux cleaned = 0.00126965 Jy ! Component: 900 - total flux cleaned = 0.00139135 Jy ! Component: 950 - total flux cleaned = 0.00148534 Jy ! Component: 1000 - total flux cleaned = 0.00156545 Jy ! Component: 1050 - total flux cleaned = 0.00171077 Jy ! Component: 1100 - total flux cleaned = 0.00181562 Jy ! Component: 1150 - total flux cleaned = 0.00193276 Jy ! Component: 1200 - total flux cleaned = 0.00198456 Jy ! Component: 1250 - total flux cleaned = 0.00208715 Jy ! Component: 1300 - total flux cleaned = 0.0021254 Jy ! Component: 1350 - total flux cleaned = 0.00221403 Jy ! Component: 1400 - total flux cleaned = 0.00226429 Jy ! Component: 1450 - total flux cleaned = 0.00232659 Jy ! Component: 1500 - total flux cleaned = 0.00241353 Jy ! Component: 1550 - total flux cleaned = 0.00237658 Jy ! Component: 1600 - total flux cleaned = 0.00240121 Jy ! Component: 1650 - total flux cleaned = 0.0024746 Jy ! Component: 1700 - total flux cleaned = 0.00253537 Jy ! Component: 1750 - total flux cleaned = 0.00259579 Jy ! Component: 1800 - total flux cleaned = 0.00259582 Jy ! Component: 1850 - total flux cleaned = 0.00269157 Jy ! Component: 1900 - total flux cleaned = 0.00270343 Jy ! Component: 1950 - total flux cleaned = 0.00271521 Jy ! Component: 2000 - total flux cleaned = 0.0027153 Jy ! Component: 2050 - total flux cleaned = 0.00278567 Jy ! Component: 2100 - total flux cleaned = 0.00283235 Jy ! Component: 2150 - total flux cleaned = 0.00286719 Jy ! Component: 2200 - total flux cleaned = 0.00287863 Jy ! Component: 2250 - total flux cleaned = 0.00291318 Jy ! Component: 2300 - total flux cleaned = 0.00297039 Jy ! Component: 2350 - total flux cleaned = 0.00299316 Jy ! Component: 2400 - total flux cleaned = 0.0029818 Jy ! Component: 2450 - total flux cleaned = 0.00304953 Jy ! Component: 2500 - total flux cleaned = 0.00312824 Jy ! Component: 2550 - total flux cleaned = 0.00312822 Jy ! Component: 2600 - total flux cleaned = 0.00318389 Jy ! Component: 2650 - total flux cleaned = 0.00321715 Jy ! Component: 2700 - total flux cleaned = 0.00323933 Jy ! Component: 2750 - total flux cleaned = 0.00322839 Jy ! Component: 2800 - total flux cleaned = 0.00332706 Jy ! Component: 2850 - total flux cleaned = 0.00335979 Jy ! Component: 2900 - total flux cleaned = 0.00338149 Jy ! Component: 2950 - total flux cleaned = 0.0033923 Jy ! Component: 3000 - total flux cleaned = 0.00340311 Jy ! Component: 3050 - total flux cleaned = 0.00345685 Jy ! Component: 3100 - total flux cleaned = 0.0034783 Jy ! Component: 3150 - total flux cleaned = 0.00348891 Jy ! Component: 3200 - total flux cleaned = 0.00354211 Jy ! Component: 3250 - total flux cleaned = 0.00355266 Jy ! Component: 3300 - total flux cleaned = 0.00363715 Jy ! Component: 3350 - total flux cleaned = 0.00364772 Jy ! Component: 3400 - total flux cleaned = 0.00366867 Jy ! Component: 3450 - total flux cleaned = 0.00372098 Jy ! Component: 3500 - total flux cleaned = 0.0037731 Jy ! Component: 3550 - total flux cleaned = 0.00380424 Jy ! Component: 3600 - total flux cleaned = 0.00387672 Jy ! Component: 3650 - total flux cleaned = 0.00389742 Jy ! Component: 3700 - total flux cleaned = 0.00401063 Jy ! Component: 3750 - total flux cleaned = 0.00400038 Jy ! Component: 3800 - total flux cleaned = 0.004031 Jy ! Component: 3850 - total flux cleaned = 0.00411259 Jy ! Component: 3900 - total flux cleaned = 0.00415317 Jy ! Component: 3950 - total flux cleaned = 0.00424431 Jy ! Component: 4000 - total flux cleaned = 0.00430485 Jy ! Component: 4050 - total flux cleaned = 0.00433507 Jy ! Total flux subtracted in 4096 components = 0.00441536 Jy ! Clean residual min=-0.000644 max=0.000531 Jy/beam ! Clean residual mean=0.000003 rms=0.000171 Jy/beam ! Combined flux in latest and established models = 0.0823112 Jy keep ! Adding 342 model components to the UV plane model. ! The established model now contains 404 components and 0.0823112 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J2130+3332_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7927 x 1.427 at -12.75 degrees (North through East) ! Clean map min=-0.0007909 max=0.058291 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J2130+3332_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0582909 invert ! Inverting map ! Your choice of large map pixels excluded 4.25% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000170765 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.878861 0.878861 1.75772 3.51544 7.03089 14.0618 28.1235 56.2471 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0005 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.058 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 341.351 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J2130+3332_X_uvs.log closed on Sat Dec 26 09:45:16 2015