! Started logfile: /scr/pima/gb073_uvs/J1743-0350_X_uvs.log on Sat Dec 26 09:43:21 2015 obs /scr/pima/gb073_uvs/J1743-0350_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1743-0350_X_uva.fits ! AN table 1: 12 integrations on 6 of 6 possible baselines. ! AN table 2: 5 integrations on 10 of 10 possible baselines. ! AN table 3: 5 integrations on 36 of 36 possible baselines. ! AN table 4: 5 integrations on 3 of 3 possible baselines. ! AN table 5: 6 integrations on 55 of 55 possible baselines. ! AN table 6: 6 integrations on 10 of 10 possible baselines. ! AN table 7: 6 integrations on 55 of 55 possible baselines. ! Apparent sampling: 0.997107 visibilities/baseline/integration-bin. ! Found source: J1743-0350 ! ! 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 8272 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/J1743-0350_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 15 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 6 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 2. ! A total of 15 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 6 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 3. ! A total of 15 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 6 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 4. ! A total of 15 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 6 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 5. ! A total of 15 telescope corrections were flagged in sub-array 1. ! A total of 5 telescope corrections were flagged in sub-array 2. ! A total of 5 telescope corrections were flagged in sub-array 3. ! A total of 12 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 12 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 6. ! A total of 15 telescope corrections were flagged in sub-array 1. ! A total of 5 telescope corrections were flagged in sub-array 2. ! A total of 5 telescope corrections were flagged in sub-array 3. ! A total of 12 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 12 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 7. ! A total of 15 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 6 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 8. ! A total of 15 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 6 telescope corrections were flagged in sub-array 7. ! ! Fit before self-cal, rms=3.811010Jy sigma=35.610391 ! Fit after self-cal, rms=2.732141Jy sigma=26.160105 ! 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 4.43% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=0.5628 mas, bmaj=1.063 mas, bpa=-3.315 degrees ! Estimated noise=1.54581 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 = 2.71852 Jy ! Component: 100 - total flux cleaned = 3.51811 Jy ! Total flux subtracted in 100 components = 3.51811 Jy ! Clean residual min=-0.155661 max=0.360987 Jy/beam ! Clean residual mean=0.000008 rms=0.030869 Jy/beam ! Combined flux in latest and established models = 3.51811 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 12 components and 3.51811 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=0.808873Jy sigma=7.151807 ! Fit after self-cal, rms=0.807068Jy sigma=7.146199 ! Inverting map ! Your choice of large map pixels excluded 4.43% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.402185 Jy ! Component: 100 - total flux cleaned = 0.61978 Jy ! Total flux subtracted in 100 components = 0.61978 Jy ! Clean residual min=-0.111044 max=0.140297 Jy/beam ! Clean residual mean=0.000028 rms=0.017968 Jy/beam ! Combined flux in latest and established models = 4.13789 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 25 components and 4.13789 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=0.534616Jy sigma=3.924085 ! Fit after self-cal, rms=0.531945Jy sigma=3.910633 ! Inverting map ! Your choice of large map pixels excluded 4.43% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Added new window around map position (0.4, -1.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.148441 Jy ! Component: 100 - total flux cleaned = 0.240952 Jy ! Total flux subtracted in 100 components = 0.240952 Jy ! Clean residual min=-0.091811 max=0.086772 Jy/beam ! Clean residual mean=0.000033 rms=0.015243 Jy/beam ! Combined flux in latest and established models = 4.37884 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 29 components and 4.37884 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=0.479693Jy sigma=3.223932 ! Fit after self-cal, rms=0.477280Jy sigma=3.203850 ! Inverting map ! Your choice of large map pixels excluded 4.43% of the data. ! The x-axis pixel size should ideally be below 0.1672 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 4.43% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=0.6802 mas, bmaj=1.3 mas, bpa=-3.205 degrees ! Estimated noise=1.08408 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 = 0.0929824 Jy ! Component: 100 - total flux cleaned = 0.141871 Jy ! Component: 150 - total flux cleaned = 0.159005 Jy ! Component: 200 - total flux cleaned = 0.163041 Jy ! Total flux subtracted in 200 components = 0.163041 Jy ! Clean residual min=-0.075058 max=0.058242 Jy/beam ! Clean residual mean=0.000057 rms=0.014343 Jy/beam ! Combined flux in latest and established models = 4.54188 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 34 components and 4.54188 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=0.459948Jy sigma=3.021251 ! Fit after self-cal, rms=0.458469Jy sigma=3.008671 ! Inverting map ! Your choice of large map pixels excluded 4.43% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6802 x 1.3 at -3.205 degrees (North through East) ! Clean map min=-0.065126 max=3.5369 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 33 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: ! BR 0.96 KP 1.00 MK 1.01 OV 1.01 ! PT 0.97 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 FD 0.99 KP 1.00 LA 1.06 ! MK 0.99 NL 0.94 OV 1.00 PT 0.97 ! SC 0.98 ! ! A total of 15 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 EF 1.00* FD 0.98 KP 0.99 ! LA 1.06 MC 0.90 NL 0.95 ON 1.02 ! OV 1.02 PT 0.98 SC 0.96 ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00 EF 1.00* FD 0.99 HH 1.12 ! KP 1.00 LA 1.08 MC 0.92 NL 0.94 ! ON 1.01 PT 0.98 SC 0.97 ! ! ! Correcting IF 2. ! A total of 33 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: ! BR 1.01 KP 1.02 MK 1.03 OV 1.03 ! PT 1.03 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 1.02 KP 1.02 LA 1.07 ! MK 1.02 NL 0.97 OV 1.03 PT 1.02 ! SC 1.02 ! ! A total of 15 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 EF 1.00* FD 1.04 KP 1.02 ! LA 1.08 MC 0.90 NL 0.98 ON 1.03 ! OV 1.04 PT 1.03 SC 1.00 ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.05 EF 1.00* FD 1.03 HH 1.13 ! KP 1.02 LA 1.09 MC 0.94 NL 0.97 ! ON 1.02 PT 1.04 SC 1.01 ! ! ! Correcting IF 3. ! A total of 33 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: ! BR 1.00 KP 0.96 MK 0.99 OV 0.99 ! PT 1.00 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.00 KP 0.96 LA 1.00 ! MK 0.97 NL 0.95 OV 0.99 PT 1.01 ! SC 1.04 ! ! A total of 15 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 EF 1.00* FD 1.01 KP 0.95 ! LA 1.00 MC 0.89 NL 0.95 ON 1.00 ! OV 1.00 PT 1.02 SC 1.02 ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.03 EF 1.00* FD 1.01 HH 1.10 ! KP 0.96 LA 1.01 MC 0.92 NL 0.95 ! ON 0.99 PT 1.03 SC 1.03 ! ! ! Correcting IF 4. ! A total of 33 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: ! BR 1.00 KP 0.98 MK 1.00 OV 1.00 ! PT 1.03 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.02 KP 0.98 LA 1.02 ! MK 0.98 NL 0.97 OV 1.00 PT 1.03 ! SC 1.05 ! ! A total of 15 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 EF 1.00* FD 1.03 KP 0.98 ! LA 1.01 MC 0.90 NL 0.98 ON 1.02 ! OV 1.01 PT 1.04 SC 1.02 ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.03 EF 1.00* FD 1.03 HH 1.13 ! KP 0.98 LA 1.03 MC 0.93 NL 0.98 ! ON 1.01 PT 1.04 SC 1.03 ! ! ! Correcting IF 5. ! A total of 33 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: ! BR 1.00* KP 0.89 MK 0.97 OV 1.04 ! PT 0.97 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00 KP 0.89 LA 1.00 ! MK 0.96 NL 0.99 OV 1.04 PT 0.98 ! SC 1.03 ! ! A total of 15 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! MC 0.00* SC 0.00* ZC 0.00* ! ! 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* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! ON 1.00* PT 1.00* SC 1.00* ! ! ! Correcting IF 6. ! A total of 33 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: ! BR 1.00* KP 0.87 MK 0.98 OV 1.04 ! PT 0.94 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00 KP 0.87 LA 1.00 ! MK 0.97 NL 0.99 OV 1.04 PT 0.94 ! SC 0.99 ! ! A total of 15 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! MC 0.00* SC 0.00* ZC 0.00* ! ! 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* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! ON 1.00* PT 1.00* SC 1.00* ! ! ! Correcting IF 7. ! A total of 33 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: ! BR 0.99 KP 0.88 MK 1.05 OV 0.99 ! PT 1.00 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.04 KP 0.89 LA 1.04 ! MK 1.02 NL 1.00 OV 1.00 PT 1.00 ! SC 1.03 ! ! A total of 15 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! MC 0.00* SC 0.00* ZC 0.00* ! ! 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* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! ON 1.00* PT 1.00* SC 1.00* ! ! ! Correcting IF 8. ! A total of 33 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: ! BR 0.99 KP 0.90 MK 1.05 OV 0.99 ! PT 1.00 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.01 KP 0.91 LA 1.03 ! MK 1.02 NL 0.99 OV 0.99 PT 1.00 ! SC 1.03 ! ! A total of 15 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! MC 0.00* SC 0.00* ZC 0.00* ! ! 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* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! ON 1.00* PT 1.00* SC 1.00* ! ! ! Fit before self-cal, rms=0.458469Jy sigma=3.008671 ! Fit after self-cal, rms=0.387500Jy sigma=2.253258 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=0.6823 mas, bmaj=1.457 mas, bpa=-2.855 degrees ! Estimated noise=1.08885 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 = 0.00239594 Jy ! Component: 100 - total flux cleaned = 0.00336952 Jy ! Component: 150 - total flux cleaned = 0.00487527 Jy ! Component: 200 - total flux cleaned = 0.00621899 Jy ! Total flux subtracted in 200 components = 0.00621899 Jy ! Clean residual min=-0.060305 max=0.038604 Jy/beam ! Clean residual mean=0.000057 rms=0.010965 Jy/beam ! Combined flux in latest and established models = 4.5481 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 38 components and 4.5481 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=0.382295Jy sigma=2.226688 ! Fit after self-cal, rms=0.381950Jy sigma=2.222834 ! Inverting map ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 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=0.381950Jy sigma=2.222834 ! Fit after self-cal, rms=0.375023Jy sigma=2.164735 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=0.6824 mas, bmaj=1.463 mas, bpa=-2.951 degrees ! Estimated noise=1.08667 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00441207 Jy ! Component: 100 - total flux cleaned = -0.00295476 Jy ! Component: 150 - total flux cleaned = -0.00297573 Jy ! Component: 200 - total flux cleaned = -0.00296264 Jy ! Total flux subtracted in 200 components = -0.00296264 Jy ! Clean residual min=-0.053789 max=0.036517 Jy/beam ! Clean residual mean=0.000060 rms=0.010308 Jy/beam ! Combined flux in latest and established models = 4.54514 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 43 components and 4.54514 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=0.373049Jy sigma=2.156228 ! Fit after self-cal, rms=0.372889Jy sigma=2.154557 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 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 = 0.00484258 Jy ! Component: 100 - total flux cleaned = 0.00484386 Jy ! Component: 150 - total flux cleaned = 0.00480631 Jy ! Component: 200 - total flux cleaned = 0.00479783 Jy ! Total flux subtracted in 200 components = 0.00479783 Jy ! Clean residual min=-0.053767 max=0.035102 Jy/beam ! Clean residual mean=0.000060 rms=0.010248 Jy/beam ! Combined flux in latest and established models = 4.54994 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 43 components and 4.54994 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=0.372617Jy sigma=2.153811 ! Fit after self-cal, rms=0.372522Jy sigma=2.152844 ! Inverting map ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 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=0.372522Jy sigma=2.152844 ! Fit after self-cal, rms=0.372818Jy sigma=2.146733 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=0.6817 mas, bmaj=1.467 mas, bpa=-3.057 degrees ! Estimated noise=1.08363 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00384644 Jy ! Component: 100 - total flux cleaned = -0.00381224 Jy ! Component: 150 - total flux cleaned = -0.00331592 Jy ! Component: 200 - total flux cleaned = -0.00325719 Jy ! Total flux subtracted in 200 components = -0.00325719 Jy ! Clean residual min=-0.052816 max=0.035615 Jy/beam ! Clean residual mean=0.000061 rms=0.010223 Jy/beam ! Combined flux in latest and established models = 4.54668 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 44 components and 4.54668 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=0.371772Jy sigma=2.143504 ! Fit after self-cal, rms=0.371691Jy sigma=2.142500 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 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 = 0.00338195 Jy ! Component: 100 - total flux cleaned = 0.0034042 Jy ! Component: 150 - total flux cleaned = 0.00384925 Jy ! Component: 200 - total flux cleaned = 0.00386298 Jy ! Total flux subtracted in 200 components = 0.00386298 Jy ! Clean residual min=-0.052947 max=0.034578 Jy/beam ! Clean residual mean=0.000061 rms=0.010182 Jy/beam ! Combined flux in latest and established models = 4.55054 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 45 components and 4.55054 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=0.371585Jy sigma=2.142228 ! Fit after self-cal, rms=0.371529Jy sigma=2.141694 ! Inverting map ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 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=0.371529Jy sigma=2.141694 ! Fit after self-cal, rms=0.371797Jy sigma=2.138020 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=2.606 mas, bmaj=3.622 mas, bpa=2.953 degrees ! Estimated noise=1.32869 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -3.7396e-05 Jy ! Component: 100 - total flux cleaned = -0.000646067 Jy ! Component: 150 - total flux cleaned = -0.00154152 Jy ! Component: 200 - total flux cleaned = -0.00156466 Jy ! Total flux subtracted in 200 components = -0.00156466 Jy ! Clean residual min=-0.057390 max=0.046965 Jy/beam ! Clean residual mean=0.000131 rms=0.015129 Jy/beam ! Combined flux in latest and established models = 4.54898 Jy selfcal ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 49 components and 4.54898 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=0.372948Jy sigma=2.159724 ! Fit after self-cal, rms=0.372788Jy sigma=2.155671 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 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 = 0.00384414 Jy ! Component: 100 - total flux cleaned = 0.00383113 Jy ! Component: 150 - total flux cleaned = 0.00356547 Jy ! Component: 200 - total flux cleaned = 0.00401254 Jy ! Total flux subtracted in 200 components = 0.00401254 Jy ! Clean residual min=-0.057136 max=0.047437 Jy/beam ! Clean residual mean=0.000130 rms=0.015024 Jy/beam ! Combined flux in latest and established models = 4.55299 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 49 components and 4.55299 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=0.374255Jy sigma=2.176720 ! Fit after self-cal, rms=0.374271Jy sigma=2.175046 ! Inverting map ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 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 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=0.6812 mas, bmaj=1.469 mas, bpa=-3.133 degrees ! Estimated noise=1.08115 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6812 x 1.469 at -3.133 degrees (North through East) ! Clean map min=-0.046499 max=3.5136 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=0.374271Jy sigma=2.175046 ! Fit after self-cal, rms=0.362404Jy sigma=2.055585 ! Inverting map and beam ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=0.6843 mas, bmaj=1.473 mas, bpa=-3.07 degrees ! Estimated noise=1.08281 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0111721 Jy ! Component: 100 - total flux cleaned = -0.0111851 Jy ! Component: 150 - total flux cleaned = -0.0107233 Jy ! Component: 200 - total flux cleaned = -0.0102967 Jy ! Total flux subtracted in 200 components = -0.0102967 Jy ! Clean residual min=-0.046371 max=0.032603 Jy/beam ! Clean residual mean=0.000057 rms=0.009281 Jy/beam ! Combined flux in latest and established models = 4.54269 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 51 components and 4.5427 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=0.362069Jy sigma=2.050744 ! Fit after self-cal, rms=0.361925Jy sigma=2.049531 ! Inverting map ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00127083 Jy ! Component: 100 - total flux cleaned = -0.000913131 Jy ! Component: 150 - total flux cleaned = -0.000579849 Jy ! Component: 200 - total flux cleaned = -0.000566927 Jy ! Total flux subtracted in 200 components = -0.000566927 Jy ! Clean residual min=-0.046134 max=0.032191 Jy/beam ! Clean residual mean=0.000057 rms=0.009263 Jy/beam ! Combined flux in latest and established models = 4.54213 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 51 components and 4.54213 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=0.362139Jy sigma=2.049609 ! Fit after self-cal, rms=0.362035Jy sigma=2.049055 ! Inverting map ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 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=0.362035Jy sigma=2.049055 ! Fit after self-cal, rms=0.362001Jy sigma=2.043560 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 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=0.5693 mas, bmaj=1.182 mas, bpa=-2.767 degrees ! Estimated noise=1.54333 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.69876 Jy ! Component: 100 - total flux cleaned = 3.51635 Jy ! Component: 150 - total flux cleaned = 3.90301 Jy ! Component: 200 - total flux cleaned = 4.11672 Jy ! Total flux subtracted in 200 components = 4.11672 Jy ! Clean residual min=-0.074206 max=0.116831 Jy/beam ! Clean residual mean=0.000025 rms=0.014152 Jy/beam ! Combined flux in latest and established models = 4.11672 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 21 model components to the UV plane model. ! The established model now contains 21 components and 4.11672 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=0.6841 mas, bmaj=1.475 mas, bpa=-3.132 degrees ! Estimated noise=1.08012 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 (-0.2, -1). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.186048 Jy ! Component: 100 - total flux cleaned = 0.287502 Jy ! Component: 150 - total flux cleaned = 0.347649 Jy ! Component: 200 - total flux cleaned = 0.38387 Jy ! Total flux subtracted in 200 components = 0.38387 Jy ! Clean residual min=-0.049394 max=0.038272 Jy/beam ! Clean residual mean=0.000060 rms=0.009649 Jy/beam ! Combined flux in latest and established models = 4.50059 Jy ! Adding 29 model components to the UV plane model. ! The established model now contains 45 components and 4.50059 Jy ! Inverting map ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 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 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=2.606 mas, bmaj=3.621 mas, bpa=3.01 degrees ! Estimated noise=1.32239 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0293765 Jy ! Component: 100 - total flux cleaned = 0.0319474 Jy ! Component: 150 - total flux cleaned = 0.0344601 Jy ! Component: 200 - total flux cleaned = 0.0364652 Jy ! Total flux subtracted in 200 components = 0.0364652 Jy ! Clean residual min=-0.049247 max=0.045481 Jy/beam ! Clean residual mean=0.000117 rms=0.013259 Jy/beam ! Combined flux in latest and established models = 4.53705 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 = 0.00172872 Jy ! Component: 100 - total flux cleaned = 0.00202558 Jy ! Component: 150 - total flux cleaned = 0.00232751 Jy ! Component: 200 - total flux cleaned = 0.00259408 Jy ! Total flux subtracted in 200 components = 0.00259408 Jy ! Clean residual min=-0.048805 max=0.045381 Jy/beam ! Clean residual mean=0.000116 rms=0.013211 Jy/beam ! Combined flux in latest and established models = 4.53965 Jy ! Adding 11 model components to the UV plane model. ! The established model now contains 51 components and 4.53964 Jy ! Inverting map ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=0.6841 mas, bmaj=1.475 mas, bpa=-3.132 degrees ! Estimated noise=1.08012 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00557589 Jy ! Component: 100 - total flux cleaned = -0.00466773 Jy ! Component: 150 - total flux cleaned = -0.00468921 Jy ! Component: 200 - total flux cleaned = -0.00541151 Jy ! Total flux subtracted in 200 components = -0.00541151 Jy ! Clean residual min=-0.048360 max=0.035460 Jy/beam ! Clean residual mean=0.000055 rms=0.009260 Jy/beam ! Combined flux in latest and established models = 4.53423 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 58 components and 4.53423 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=0.356889Jy sigma=2.047396 ! Fit after self-cal, rms=0.355234Jy sigma=2.036321 wmodel /scr/pima/gb073_uvs/J1743-0350_X_map.mod ! Writing 58 model components to file: /scr/pima/gb073_uvs/J1743-0350_X_map.mod wobs /scr/pima/gb073_uvs/J1743-0350_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1743-0350_X_uvs.fits wwins /scr/pima/gb073_uvs/J1743-0350_X_map.win ! wwins: Wrote 3 windows to /scr/pima/gb073_uvs/J1743-0350_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 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.0212913 Jy ! Component: 100 - total flux cleaned = -0.0403054 Jy ! Component: 150 - total flux cleaned = -0.0582513 Jy ! Component: 200 - total flux cleaned = -0.0753588 Jy ! Component: 250 - total flux cleaned = -0.0918032 Jy ! Component: 300 - total flux cleaned = -0.107713 Jy ! Component: 350 - total flux cleaned = -0.123179 Jy ! Component: 400 - total flux cleaned = -0.137046 Jy ! Component: 450 - total flux cleaned = -0.15118 Jy ! Component: 500 - total flux cleaned = -0.164428 Jy ! Component: 550 - total flux cleaned = -0.176277 Jy ! Component: 600 - total flux cleaned = -0.187895 Jy ! Component: 650 - total flux cleaned = -0.198759 Jy ! Component: 700 - total flux cleaned = -0.209441 Jy ! Component: 750 - total flux cleaned = -0.221001 Jy ! Component: 800 - total flux cleaned = -0.230836 Jy ! Component: 850 - total flux cleaned = -0.241044 Jy ! Component: 900 - total flux cleaned = -0.2516 Jy ! Component: 950 - total flux cleaned = -0.261021 Jy ! Component: 1000 - total flux cleaned = -0.269343 Jy ! Component: 1050 - total flux cleaned = -0.278046 Jy ! Component: 1100 - total flux cleaned = -0.287117 Jy ! Component: 1150 - total flux cleaned = -0.295607 Jy ! Component: 1200 - total flux cleaned = -0.303998 Jy ! Component: 1250 - total flux cleaned = -0.311834 Jy ! Component: 1300 - total flux cleaned = -0.319586 Jy ! Component: 1350 - total flux cleaned = -0.329046 Jy ! Component: 1400 - total flux cleaned = -0.336171 Jy ! Component: 1450 - total flux cleaned = -0.34366 Jy ! Component: 1500 - total flux cleaned = -0.351503 Jy ! Component: 1550 - total flux cleaned = -0.357965 Jy ! Component: 1600 - total flux cleaned = -0.363507 Jy ! Component: 1650 - total flux cleaned = -0.369845 Jy ! Component: 1700 - total flux cleaned = -0.376115 Jy ! Component: 1750 - total flux cleaned = -0.3815 Jy ! Component: 1800 - total flux cleaned = -0.389282 Jy ! Component: 1850 - total flux cleaned = -0.395361 Jy ! Component: 1900 - total flux cleaned = -0.401383 Jy ! Component: 1950 - total flux cleaned = -0.406554 Jy ! Component: 2000 - total flux cleaned = -0.411286 Jy ! Component: 2050 - total flux cleaned = -0.415981 Jy ! Component: 2100 - total flux cleaned = -0.422565 Jy ! Component: 2150 - total flux cleaned = -0.426785 Jy ! Component: 2200 - total flux cleaned = -0.431355 Jy ! Component: 2250 - total flux cleaned = -0.437018 Jy ! Component: 2300 - total flux cleaned = -0.440764 Jy ! Component: 2350 - total flux cleaned = -0.446702 Jy ! Component: 2400 - total flux cleaned = -0.451121 Jy ! Component: 2450 - total flux cleaned = -0.455872 Jy ! Component: 2500 - total flux cleaned = -0.46058 Jy ! Component: 2550 - total flux cleaned = -0.465615 Jy ! Component: 2600 - total flux cleaned = -0.469184 Jy ! Component: 2650 - total flux cleaned = -0.473434 Jy ! Component: 2700 - total flux cleaned = -0.478002 Jy ! Component: 2750 - total flux cleaned = -0.482187 Jy ! Component: 2800 - total flux cleaned = -0.486338 Jy ! Component: 2850 - total flux cleaned = -0.490111 Jy ! Component: 2900 - total flux cleaned = -0.494201 Jy ! Component: 2950 - total flux cleaned = -0.498599 Jy ! Component: 3000 - total flux cleaned = -0.502291 Jy ! Component: 3050 - total flux cleaned = -0.50629 Jy ! Component: 3100 - total flux cleaned = -0.509928 Jy ! Component: 3150 - total flux cleaned = -0.514524 Jy ! Component: 3200 - total flux cleaned = -0.517781 Jy ! Component: 3250 - total flux cleaned = -0.521663 Jy ! Component: 3300 - total flux cleaned = -0.52488 Jy ! Component: 3350 - total flux cleaned = -0.528072 Jy ! Component: 3400 - total flux cleaned = -0.531877 Jy ! Component: 3450 - total flux cleaned = -0.535025 Jy ! Component: 3500 - total flux cleaned = -0.538775 Jy ! Component: 3550 - total flux cleaned = -0.541259 Jy ! Component: 3600 - total flux cleaned = -0.544961 Jy ! Component: 3650 - total flux cleaned = -0.547412 Jy ! Component: 3700 - total flux cleaned = -0.55106 Jy ! Component: 3750 - total flux cleaned = -0.553176 Jy ! Component: 3800 - total flux cleaned = -0.555575 Jy ! Component: 3850 - total flux cleaned = -0.557958 Jy ! Component: 3900 - total flux cleaned = -0.560624 Jy ! Component: 3950 - total flux cleaned = -0.562393 Jy ! Component: 4000 - total flux cleaned = -0.565025 Jy ! Component: 4050 - total flux cleaned = -0.567061 Jy ! Total flux subtracted in 4096 components = -0.569086 Jy ! Clean residual min=-0.014890 max=0.016361 Jy/beam ! Clean residual mean=0.000029 rms=0.005097 Jy/beam ! Combined flux in latest and established models = 3.96515 Jy keep ! Adding 322 model components to the UV plane model. ! The established model now contains 380 components and 3.96514 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1743-0350_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6841 x 1.475 at -3.132 degrees (North through East) ! Clean map min=-0.037049 max=3.5183 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1743-0350_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 3.51835 invert ! Inverting map ! Your choice of large map pixels excluded 4.71% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00508428 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.433522 0.433522 0.867045 1.73409 3.46818 6.93636 13.8727 27.7454 55.4909 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0152 print "peak= ", int(1000*peak_flux)/1000 ! peak= 3.518 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 692.005 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1743-0350_X_uvs.log closed on Sat Dec 26 09:43:26 2015