! Started logfile: /scr/pima/gb073_uvs/J2129-1538_X_uvs.log on Sat Dec 26 09:45:03 2015 obs /scr/pima/gb073_uvs/J2129-1538_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J2129-1538_X_uva.fits ! AN table 1: 6 integrations on 6 of 6 possible baselines. ! AN table 2: 5 integrations on 6 of 6 possible baselines. ! AN table 3: 5 integrations on 36 of 36 possible baselines. ! AN table 4: 18 integrations on 10 of 10 possible baselines. ! AN table 5: 5 integrations on 3 of 3 possible baselines. ! AN table 6: 5 integrations on 28 of 28 possible baselines. ! AN table 7: 5 integrations on 28 of 28 possible baselines. ! AN table 8: 5 integrations on 28 of 28 possible baselines. ! Apparent sampling: 1 visibilities/baseline/integration-bin. ! Found source: J2129-1538 ! ! 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 6888 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/J2129-1538_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 6 telescope corrections were flagged in sub-array 1. ! A total of 18 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 18 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 18 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 18 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 5. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 5 telescope corrections were flagged in sub-array 3. ! A total of 18 telescope corrections were flagged in sub-array 4. ! A total of 15 telescope corrections were flagged in sub-array 5. ! A total of 5 telescope corrections were flagged in sub-array 6. ! A total of 5 telescope corrections were flagged in sub-array 7. ! A total of 5 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 6. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 5 telescope corrections were flagged in sub-array 3. ! A total of 18 telescope corrections were flagged in sub-array 4. ! A total of 15 telescope corrections were flagged in sub-array 5. ! A total of 5 telescope corrections were flagged in sub-array 6. ! A total of 5 telescope corrections were flagged in sub-array 7. ! A total of 5 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 7. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 18 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 8. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 18 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.532565Jy sigma=15.750780 ! Fit after self-cal, rms=0.416886Jy sigma=3.556611 ! 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 0.684% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec ! Estimated beam: bmin=0.7947 mas, bmaj=1.058 mas, bpa=2.756 degrees ! Estimated noise=1.37223 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 = 0.867569 Jy ! Component: 100 - total flux cleaned = 1.1493 Jy ! Total flux subtracted in 100 components = 1.1493 Jy ! Clean residual min=-0.030477 max=0.113848 Jy/beam ! Clean residual mean=-0.000145 rms=0.008270 Jy/beam ! Combined flux in latest and established models = 1.1493 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 11 components and 1.1493 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=0.234885Jy sigma=2.126477 ! Fit after self-cal, rms=0.234502Jy sigma=2.124870 ! Inverting map ! Your choice of large map pixels excluded 0.684% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.116917 Jy ! Component: 100 - total flux cleaned = 0.173005 Jy ! Total flux subtracted in 100 components = 0.173005 Jy ! Clean residual min=-0.018521 max=0.027714 Jy/beam ! Clean residual mean=-0.000042 rms=0.004265 Jy/beam ! Combined flux in latest and established models = 1.32231 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 19 components and 1.32231 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=0.163626Jy sigma=1.204493 ! Fit after self-cal, rms=0.163553Jy sigma=1.203857 ! Inverting map ! Your choice of large map pixels excluded 0.684% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec ! Added new window around map position (0.2, 1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0284586 Jy ! Component: 100 - total flux cleaned = 0.0431296 Jy ! Total flux subtracted in 100 components = 0.0431296 Jy ! Clean residual min=-0.020915 max=0.019107 Jy/beam ! Clean residual mean=-0.000017 rms=0.003934 Jy/beam ! Combined flux in latest and established models = 1.36544 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 24 components and 1.36544 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=0.158072Jy sigma=1.128030 ! Fit after self-cal, rms=0.158051Jy sigma=1.127055 ! Inverting map ! Your choice of large map pixels excluded 0.684% of the data. ! The x-axis pixel size should ideally be below 0.1684 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 0.684% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec ! Estimated beam: bmin=0.9505 mas, bmaj=1.282 mas, bpa=-1.169 degrees ! Estimated noise=0.979285 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 = 0.00711529 Jy ! Component: 100 - total flux cleaned = 0.00854616 Jy ! Component: 150 - total flux cleaned = 0.00942444 Jy ! Component: 200 - total flux cleaned = 0.00996443 Jy ! Total flux subtracted in 200 components = 0.00996443 Jy ! Clean residual min=-0.019080 max=0.014853 Jy/beam ! Clean residual mean=0.000002 rms=0.003788 Jy/beam ! Combined flux in latest and established models = 1.3754 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 31 components and 1.3754 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=0.156769Jy sigma=1.116820 ! Fit after self-cal, rms=0.156716Jy sigma=1.116045 ! Inverting map ! Your choice of large map pixels excluded 0.684% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9505 x 1.282 at -1.169 degrees (North through East) ! Clean map min=-0.017832 max=1.0528 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. ! A total of 18 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: ! FD 1.00* HH 1.00* MC 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.96 FD 0.98 KP 0.98 LA 1.04 ! MK 0.99 NL 0.94 OV 0.99 PT 0.96 ! SC 0.96 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* KP 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.96 FD 0.98 KP 0.98 LA 1.04 ! MK 0.95 NL 0.92 PT 0.96 SC 0.96 ! ! Telescope amplitude corrections in sub-array 7: ! BR 0.98 FD 0.97 KP 0.97 LA 1.04 ! NL 0.94 OV 1.00 PT 0.96 SC 0.94 ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.99 FD 0.97 KP 0.99 LA 1.03 ! MK 1.01 NL 0.92 OV 1.00 PT 0.96 ! ! ! Correcting IF 2. ! A total of 18 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: ! FD 1.00* HH 1.00* MC 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 FD 1.01 KP 0.99 LA 1.06 ! MK 1.00 NL 0.97 OV 1.01 PT 1.01 ! SC 1.02 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* KP 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00 FD 1.03 KP 1.01 LA 1.05 ! MK 1.00 NL 0.95 PT 1.02 SC 0.99 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.03 FD 1.03 KP 1.00 LA 1.07 ! NL 0.97 OV 1.02 PT 1.01 SC 0.98 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.02 FD 1.02 KP 1.01 LA 1.06 ! MK 1.04 NL 0.96 OV 1.02 PT 1.01 ! ! ! Correcting IF 3. ! A total of 18 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: ! FD 1.00* HH 1.00* MC 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 1.00 KP 0.95 LA 0.98 ! MK 0.98 NL 0.95 OV 0.99 PT 1.00 ! SC 1.05 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* KP 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.99 FD 1.01 KP 0.95 LA 0.99 ! MK 0.95 NL 0.94 PT 1.01 SC 1.03 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.02 FD 1.00 KP 0.95 LA 0.98 ! NL 0.96 OV 1.00 PT 1.01 SC 1.00 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.03 FD 1.01 KP 0.95 LA 0.98 ! MK 1.00 NL 0.94 OV 0.97 PT 1.01 ! ! ! Correcting IF 4. ! A total of 18 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: ! FD 1.00* HH 1.00* MC 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 1.02 KP 0.98 LA 1.01 ! MK 0.99 NL 0.97 OV 0.99 PT 1.02 ! SC 1.04 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* KP 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.02 FD 1.02 KP 0.98 LA 1.01 ! MK 0.98 NL 0.95 PT 1.03 SC 1.02 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.02 FD 1.02 KP 0.97 LA 1.00 ! NL 0.98 OV 0.99 PT 1.04 SC 1.00 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.02 FD 1.03 KP 0.97 LA 1.01 ! MK 0.99 NL 0.97 OV 0.99 PT 1.03 ! ! ! Correcting IF 5. ! A total of 18 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: ! FD 1.00* HH 1.00* MC 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.02 KP 0.91 LA 1.02 ! MK 1.02 NL 1.01 OV 1.06 PT 0.99 ! SC 1.06 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* KP 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* FD 1.02 KP 0.92 LA 1.02 ! MK 1.01 NL 1.00 PT 0.99 SC 1.05 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 1.02 KP 0.91 LA 1.02 ! NL 1.02 OV 1.06 PT 1.00 SC 1.03 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.00* FD 1.03 KP 0.90 LA 1.01 ! MK 1.03 NL 1.00 OV 1.06 PT 1.00 ! ! ! Correcting IF 6. ! A total of 18 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: ! FD 1.00* HH 1.00* MC 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.01 KP 0.88 LA 1.01 ! MK 1.02 NL 1.02 OV 1.06 PT 0.96 ! SC 1.02 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* KP 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* FD 1.01 KP 0.90 LA 1.02 ! MK 1.01 NL 1.00 PT 0.96 SC 0.99 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 1.03 KP 0.88 LA 1.03 ! NL 1.02 OV 1.06 PT 0.97 SC 0.98 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.00* FD 1.04 KP 0.89 LA 1.01 ! MK 1.02 NL 1.01 OV 1.05 PT 0.95 ! ! ! Correcting IF 7. ! A total of 18 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: ! FD 1.00* HH 1.00* MC 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 FD 1.07 KP 0.91 LA 1.07 ! MK 1.09 NL 1.05 OV 1.00 PT 1.04 ! SC 1.06 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* KP 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.03 FD 1.08 KP 0.92 LA 1.07 ! MK 1.09 NL 1.04 PT 1.02 SC 1.05 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.07 FD 1.07 KP 0.93 LA 1.07 ! NL 1.04 OV 1.02 PT 1.03 SC 1.03 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.05 FD 1.08 KP 0.91 LA 1.05 ! MK 1.11 NL 1.03 OV 1.01 PT 1.01 ! ! ! Correcting IF 8. ! A total of 18 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: ! FD 1.00* HH 1.00* MC 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 FD 1.05 KP 0.92 LA 1.05 ! MK 1.06 NL 1.04 OV 1.00 PT 1.05 ! SC 1.11 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* KP 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.02 FD 1.06 KP 0.94 LA 1.06 ! MK 1.07 NL 1.01 PT 1.03 SC 1.04 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.04 FD 1.05 KP 0.93 LA 1.07 ! NL 1.02 OV 1.01 PT 1.04 SC 1.04 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.05 FD 1.06 KP 0.93 LA 1.06 ! MK 1.12 NL 1.00 OV 1.02 PT 1.04 ! ! ! Fit before self-cal, rms=0.156716Jy sigma=1.116045 ! Fit after self-cal, rms=0.139395Jy sigma=0.867576 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec ! Estimated beam: bmin=0.9511 mas, bmaj=1.353 mas, bpa=0.1012 degrees ! Estimated noise=0.994612 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 = -0.00172453 Jy ! Component: 100 - total flux cleaned = -0.00192891 Jy ! Component: 150 - total flux cleaned = -0.00225983 Jy ! Component: 200 - total flux cleaned = -0.00225351 Jy ! Total flux subtracted in 200 components = -0.00225351 Jy ! Clean residual min=-0.013861 max=0.013459 Jy/beam ! Clean residual mean=-0.000004 rms=0.002748 Jy/beam ! Combined flux in latest and established models = 1.37315 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 35 components and 1.37315 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=0.138358Jy sigma=0.862938 ! Fit after self-cal, rms=0.138358Jy sigma=0.862596 ! Inverting map ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 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=0.138358Jy sigma=0.862596 ! Fit after self-cal, rms=0.138361Jy sigma=0.861125 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec ! Estimated beam: bmin=0.9529 mas, bmaj=1.353 mas, bpa=-0.01256 degrees ! Estimated noise=0.995534 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00149172 Jy ! Component: 100 - total flux cleaned = -0.00183873 Jy ! Component: 150 - total flux cleaned = -0.00198446 Jy ! Component: 200 - total flux cleaned = -0.00198529 Jy ! Total flux subtracted in 200 components = -0.00198529 Jy ! Clean residual min=-0.013137 max=0.013157 Jy/beam ! Clean residual mean=-0.000004 rms=0.002727 Jy/beam ! Combined flux in latest and established models = 1.37117 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 36 components and 1.37117 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=0.137592Jy sigma=0.858271 ! Fit after self-cal, rms=0.137588Jy sigma=0.858086 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 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) ! Added new window around map position (-0.8, -4.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0100577 Jy ! Component: 100 - total flux cleaned = 0.010844 Jy ! Component: 150 - total flux cleaned = 0.0108627 Jy ! Component: 200 - total flux cleaned = 0.0106929 Jy ! Total flux subtracted in 200 components = 0.0106929 Jy ! Clean residual min=-0.012789 max=0.008022 Jy/beam ! Clean residual mean=0.000007 rms=0.002648 Jy/beam ! Combined flux in latest and established models = 1.38186 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 50 components and 1.38186 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=0.135654Jy sigma=0.847606 ! Fit after self-cal, rms=0.135515Jy sigma=0.845967 ! Inverting map ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 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=0.135515Jy sigma=0.845967 ! Fit after self-cal, rms=0.134907Jy sigma=0.840196 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec ! Estimated beam: bmin=0.9543 mas, bmaj=1.353 mas, bpa=-0.1088 degrees ! Estimated noise=0.996064 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0024158 Jy ! Component: 100 - total flux cleaned = 0.00260101 Jy ! Component: 150 - total flux cleaned = 0.00306734 Jy ! Component: 200 - total flux cleaned = 0.0032043 Jy ! Total flux subtracted in 200 components = 0.0032043 Jy ! Clean residual min=-0.011420 max=0.007864 Jy/beam ! Clean residual mean=0.000005 rms=0.002569 Jy/beam ! Combined flux in latest and established models = 1.38506 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 54 components and 1.38506 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=0.133974Jy sigma=0.837755 ! Fit after self-cal, rms=0.133955Jy sigma=0.837344 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 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 = 0.00113563 Jy ! Component: 100 - total flux cleaned = 0.00113456 Jy ! Component: 150 - total flux cleaned = 0.00124811 Jy ! Component: 200 - total flux cleaned = 0.00124705 Jy ! Total flux subtracted in 200 components = 0.00124705 Jy ! Clean residual min=-0.011567 max=0.008062 Jy/beam ! Clean residual mean=0.000006 rms=0.002560 Jy/beam ! Combined flux in latest and established models = 1.38631 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 58 components and 1.38631 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=0.133531Jy sigma=0.836657 ! Fit after self-cal, rms=0.133521Jy sigma=0.836535 ! Inverting map ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 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=0.133521Jy sigma=0.836535 ! Fit after self-cal, rms=0.133441Jy sigma=0.835250 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec ! Estimated beam: bmin=2.514 mas, bmaj=4.667 mas, bpa=-0.5808 degrees ! Estimated noise=1.18113 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00307474 Jy ! Component: 100 - total flux cleaned = -0.00266444 Jy ! Component: 150 - total flux cleaned = -0.00243875 Jy ! Component: 200 - total flux cleaned = -0.00233898 Jy ! Total flux subtracted in 200 components = -0.00233898 Jy ! Clean residual min=-0.013005 max=0.010578 Jy/beam ! Clean residual mean=0.000005 rms=0.003634 Jy/beam ! Combined flux in latest and established models = 1.38397 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 60 components and 1.38397 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=0.132964Jy sigma=0.836489 ! Fit after self-cal, rms=0.132963Jy sigma=0.836218 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 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 = 0.000753348 Jy ! Component: 100 - total flux cleaned = 0.000856838 Jy ! Component: 150 - total flux cleaned = 0.000862273 Jy ! Component: 200 - total flux cleaned = 0.000956334 Jy ! Total flux subtracted in 200 components = 0.000956334 Jy ! Clean residual min=-0.013109 max=0.010671 Jy/beam ! Clean residual mean=0.000007 rms=0.003628 Jy/beam ! Combined flux in latest and established models = 1.38493 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 61 components and 1.38493 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=0.132764Jy sigma=0.837222 ! Fit after self-cal, rms=0.132771Jy sigma=0.837136 ! Inverting map ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 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 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec ! Estimated beam: bmin=0.955 mas, bmaj=1.354 mas, bpa=-0.2183 degrees ! Estimated noise=0.995363 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.955 x 1.354 at -0.2183 degrees (North through East) ! Clean map min=-0.010402 max=1.0731 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=0.132771Jy sigma=0.837136 ! Fit after self-cal, rms=0.129452Jy sigma=0.800259 ! Inverting map and beam ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec ! Estimated beam: bmin=0.957 mas, bmaj=1.353 mas, bpa=-0.4096 degrees ! Estimated noise=0.993569 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00159429 Jy ! Component: 100 - total flux cleaned = -0.00181084 Jy ! Component: 150 - total flux cleaned = -0.0020011 Jy ! Component: 200 - total flux cleaned = -0.00200176 Jy ! Total flux subtracted in 200 components = -0.00200176 Jy ! Clean residual min=-0.010685 max=0.007803 Jy/beam ! Clean residual mean=0.000007 rms=0.002460 Jy/beam ! Combined flux in latest and established models = 1.38292 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 64 components and 1.38292 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=0.129047Jy sigma=0.799332 ! Fit after self-cal, rms=0.129036Jy sigma=0.799291 ! Inverting map ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -6.10035e-06 Jy ! Component: 100 - total flux cleaned = -6.38217e-06 Jy ! Component: 150 - total flux cleaned = -8.08272e-05 Jy ! Component: 200 - total flux cleaned = -7.97623e-05 Jy ! Total flux subtracted in 200 components = -7.97623e-05 Jy ! Clean residual min=-0.010814 max=0.007823 Jy/beam ! Clean residual mean=0.000006 rms=0.002457 Jy/beam ! Combined flux in latest and established models = 1.38285 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 70 components and 1.38285 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=0.128843Jy sigma=0.798609 ! Fit after self-cal, rms=0.128833Jy sigma=0.798574 ! Inverting map ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 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=0.128833Jy sigma=0.798574 ! Fit after self-cal, rms=0.128847Jy sigma=0.797763 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 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec ! Estimated beam: bmin=0.7963 mas, bmaj=1.104 mas, bpa=3.134 degrees ! Estimated noise=1.4127 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.884745 Jy ! Component: 100 - total flux cleaned = 1.16767 Jy ! Component: 150 - total flux cleaned = 1.28005 Jy ! Component: 200 - total flux cleaned = 1.32992 Jy ! Total flux subtracted in 200 components = 1.32992 Jy ! Clean residual min=-0.016383 max=0.024803 Jy/beam ! Clean residual mean=-0.000029 rms=0.003336 Jy/beam ! Combined flux in latest and established models = 1.32992 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 19 model components to the UV plane model. ! The established model now contains 19 components and 1.32992 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec ! Estimated beam: bmin=0.9579 mas, bmaj=1.355 mas, bpa=-0.5104 degrees ! Estimated noise=0.993226 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (-0.4, -2.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0275272 Jy ! Component: 100 - total flux cleaned = 0.0389039 Jy ! Component: 150 - total flux cleaned = 0.0424589 Jy ! Component: 200 - total flux cleaned = 0.0435171 Jy ! Total flux subtracted in 200 components = 0.0435171 Jy ! Clean residual min=-0.011517 max=0.008809 Jy/beam ! Clean residual mean=-0.000001 rms=0.002536 Jy/beam ! Combined flux in latest and established models = 1.37344 Jy ! Adding 18 model components to the UV plane model. ! The established model now contains 31 components and 1.37344 Jy ! Inverting map ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 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 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec ! Estimated beam: bmin=2.516 mas, bmaj=4.67 mas, bpa=-0.6845 degrees ! Estimated noise=1.17524 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00287364 Jy ! Component: 100 - total flux cleaned = 0.00332812 Jy ! Component: 150 - total flux cleaned = 0.00315896 Jy ! Component: 200 - total flux cleaned = 0.00331255 Jy ! Total flux subtracted in 200 components = 0.00331255 Jy ! Clean residual min=-0.013329 max=0.011040 Jy/beam ! Clean residual mean=0.000003 rms=0.003555 Jy/beam ! Combined flux in latest and established models = 1.37675 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 = 0.000137748 Jy ! Component: 100 - total flux cleaned = 0.000261979 Jy ! Component: 150 - total flux cleaned = 0.00025894 Jy ! Component: 200 - total flux cleaned = 0.000382906 Jy ! Total flux subtracted in 200 components = 0.000382906 Jy ! Clean residual min=-0.013417 max=0.010993 Jy/beam ! Clean residual mean=0.000004 rms=0.003551 Jy/beam ! Combined flux in latest and established models = 1.37713 Jy ! Adding 11 model components to the UV plane model. ! The established model now contains 38 components and 1.37713 Jy ! Inverting map ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec ! Estimated beam: bmin=0.9579 mas, bmaj=1.355 mas, bpa=-0.5104 degrees ! Estimated noise=0.993226 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000546661 Jy ! Component: 100 - total flux cleaned = 7.66657e-05 Jy ! Component: 150 - total flux cleaned = -0.000125775 Jy ! Component: 200 - total flux cleaned = -0.000127422 Jy ! Total flux subtracted in 200 components = -0.000127422 Jy ! Clean residual min=-0.011580 max=0.009593 Jy/beam ! Clean residual mean=0.000003 rms=0.002488 Jy/beam ! Combined flux in latest and established models = 1.377 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 47 components and 1.377 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=0.130478Jy sigma=0.812235 ! Fit after self-cal, rms=0.130281Jy sigma=0.810562 wmodel /scr/pima/gb073_uvs/J2129-1538_X_map.mod ! Writing 47 model components to file: /scr/pima/gb073_uvs/J2129-1538_X_map.mod wobs /scr/pima/gb073_uvs/J2129-1538_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J2129-1538_X_uvs.fits wwins /scr/pima/gb073_uvs/J2129-1538_X_map.win ! wwins: Wrote 4 windows to /scr/pima/gb073_uvs/J2129-1538_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 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00507126 Jy ! Component: 100 - total flux cleaned = -0.0096736 Jy ! Component: 150 - total flux cleaned = -0.0140541 Jy ! Component: 200 - total flux cleaned = -0.0182811 Jy ! Component: 250 - total flux cleaned = -0.0222138 Jy ! Component: 300 - total flux cleaned = -0.0260457 Jy ! Component: 350 - total flux cleaned = -0.0297932 Jy ! Component: 400 - total flux cleaned = -0.0333143 Jy ! Component: 450 - total flux cleaned = -0.0366201 Jy ! Component: 500 - total flux cleaned = -0.04016 Jy ! Component: 550 - total flux cleaned = -0.0433507 Jy ! Component: 600 - total flux cleaned = -0.046635 Jy ! Component: 650 - total flux cleaned = -0.0495862 Jy ! Component: 700 - total flux cleaned = -0.0522186 Jy ! Component: 750 - total flux cleaned = -0.0548147 Jy ! Component: 800 - total flux cleaned = -0.0573775 Jy ! Component: 850 - total flux cleaned = -0.0597751 Jy ! Component: 900 - total flux cleaned = -0.0621421 Jy ! Component: 950 - total flux cleaned = -0.0647389 Jy ! Component: 1000 - total flux cleaned = -0.0670464 Jy ! Component: 1050 - total flux cleaned = -0.0689482 Jy ! Component: 1100 - total flux cleaned = -0.0709555 Jy ! Component: 1150 - total flux cleaned = -0.0733132 Jy ! Component: 1200 - total flux cleaned = -0.0753984 Jy ! Component: 1250 - total flux cleaned = -0.0775844 Jy ! Component: 1300 - total flux cleaned = -0.0790273 Jy ! Component: 1350 - total flux cleaned = -0.0808137 Jy ! Component: 1400 - total flux cleaned = -0.0825844 Jy ! Component: 1450 - total flux cleaned = -0.0843375 Jy ! Component: 1500 - total flux cleaned = -0.0859558 Jy ! Component: 1550 - total flux cleaned = -0.0874468 Jy ! Component: 1600 - total flux cleaned = -0.0889253 Jy ! Component: 1650 - total flux cleaned = -0.0905041 Jy ! Component: 1700 - total flux cleaned = -0.092181 Jy ! Component: 1750 - total flux cleaned = -0.0935098 Jy ! Component: 1800 - total flux cleaned = -0.0948297 Jy ! Component: 1850 - total flux cleaned = -0.0963559 Jy ! Component: 1900 - total flux cleaned = -0.0978704 Jy ! Component: 1950 - total flux cleaned = -0.0990511 Jy ! Component: 2000 - total flux cleaned = -0.100754 Jy ! Component: 2050 - total flux cleaned = -0.101704 Jy ! Component: 2100 - total flux cleaned = -0.103277 Jy ! Component: 2150 - total flux cleaned = -0.10463 Jy ! Component: 2200 - total flux cleaned = -0.105662 Jy ! Component: 2250 - total flux cleaned = -0.106687 Jy ! Component: 2300 - total flux cleaned = -0.10801 Jy ! Component: 2350 - total flux cleaned = -0.109019 Jy ! Component: 2400 - total flux cleaned = -0.110323 Jy ! Component: 2450 - total flux cleaned = -0.111319 Jy ! Component: 2500 - total flux cleaned = -0.112408 Jy ! Component: 2550 - total flux cleaned = -0.113094 Jy ! Component: 2600 - total flux cleaned = -0.114656 Jy ! Component: 2650 - total flux cleaned = -0.115237 Jy ! Component: 2700 - total flux cleaned = -0.116681 Jy ! Component: 2750 - total flux cleaned = -0.117063 Jy ! Component: 2800 - total flux cleaned = -0.118204 Jy ! Component: 2850 - total flux cleaned = -0.119336 Jy ! Component: 2900 - total flux cleaned = -0.120181 Jy ! Component: 2950 - total flux cleaned = -0.121207 Jy ! Component: 3000 - total flux cleaned = -0.121763 Jy ! Component: 3050 - total flux cleaned = -0.122778 Jy ! Component: 3100 - total flux cleaned = -0.123328 Jy ! Component: 3150 - total flux cleaned = -0.124057 Jy ! Component: 3200 - total flux cleaned = -0.124962 Jy ! Component: 3250 - total flux cleaned = -0.126043 Jy ! Component: 3300 - total flux cleaned = -0.126581 Jy ! Component: 3350 - total flux cleaned = -0.12747 Jy ! Component: 3400 - total flux cleaned = -0.128002 Jy ! Component: 3450 - total flux cleaned = -0.128882 Jy ! Component: 3500 - total flux cleaned = -0.129583 Jy ! Component: 3550 - total flux cleaned = -0.130367 Jy ! Component: 3600 - total flux cleaned = -0.131061 Jy ! Component: 3650 - total flux cleaned = -0.13175 Jy ! Component: 3700 - total flux cleaned = -0.132434 Jy ! Component: 3750 - total flux cleaned = -0.133201 Jy ! Component: 3800 - total flux cleaned = -0.133624 Jy ! Component: 3850 - total flux cleaned = -0.134383 Jy ! Component: 3900 - total flux cleaned = -0.135304 Jy ! Component: 3950 - total flux cleaned = -0.135887 Jy ! Component: 4000 - total flux cleaned = -0.136385 Jy ! Component: 4050 - total flux cleaned = -0.137209 Jy ! Total flux subtracted in 4096 components = -0.137701 Jy ! Clean residual min=-0.005654 max=0.004425 Jy/beam ! Clean residual mean=0.000008 rms=0.001583 Jy/beam ! Combined flux in latest and established models = 1.2393 Jy keep ! Adding 308 model components to the UV plane model. ! The established model now contains 355 components and 1.2393 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J2129-1538_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9579 x 1.355 at -0.5104 degrees (North through East) ! Clean map min=-0.016031 max=1.0693 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J2129-1538_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 1.0693 invert ! Inverting map ! Your choice of large map pixels excluded 0.713% of the data. ! The x-axis pixel size should ideally be below 0.1684 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00158453 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.444552 0.444552 0.889103 1.77821 3.55641 7.11283 14.2257 28.4513 56.9026 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0047 print "peak= ", int(1000*peak_flux)/1000 ! peak= 1.069 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 674.837 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J2129-1538_X_uvs.log closed on Sat Dec 26 09:45:08 2015