! Started logfile: /scr/pima/gb073_uvs/J2311+1008_X_uvs.log on Sat Dec 26 09:46:13 2015 obs /scr/pima/gb073_uvs/J2311+1008_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J2311+1008_X_uva.fits ! AN table 1: 44 integrations on 6 of 6 possible baselines. ! AN table 2: 29 integrations on 3 of 3 possible baselines. ! AN table 3: 26 integrations on 55 of 55 possible baselines. ! AN table 4: 63 integrations on 36 of 36 possible baselines. ! AN table 5: 58 integrations on 10 of 10 possible baselines. ! AN table 6: 29 integrations on 66 of 66 possible baselines. ! AN table 7: 29 integrations on 55 of 55 possible baselines. ! AN table 8: 22 integrations on 6 of 6 possible baselines. ! Apparent sampling: 0.77896 visibilities/baseline/integration-bin. ! Found source: J2311+1008 ! ! 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 51536 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/J2311+1008_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 176 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 136 telescope corrections were flagged in sub-array 5. ! A total of 36 telescope corrections were flagged in sub-array 6. ! A total of 30 telescope corrections were flagged in sub-array 7. ! A total of 88 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 2. ! A total of 176 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 136 telescope corrections were flagged in sub-array 5. ! A total of 36 telescope corrections were flagged in sub-array 6. ! A total of 30 telescope corrections were flagged in sub-array 7. ! A total of 88 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 3. ! A total of 176 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 136 telescope corrections were flagged in sub-array 5. ! A total of 36 telescope corrections were flagged in sub-array 6. ! A total of 30 telescope corrections were flagged in sub-array 7. ! A total of 88 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 4. ! A total of 176 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 136 telescope corrections were flagged in sub-array 5. ! A total of 36 telescope corrections were flagged in sub-array 6. ! A total of 30 telescope corrections were flagged in sub-array 7. ! A total of 88 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 5. ! A total of 176 telescope corrections were flagged in sub-array 1. ! A total of 55 telescope corrections were flagged in sub-array 3. ! A total of 63 telescope corrections were flagged in sub-array 4. ! A total of 136 telescope corrections were flagged in sub-array 5. ! A total of 65 telescope corrections were flagged in sub-array 6. ! A total of 59 telescope corrections were flagged in sub-array 7. ! A total of 88 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 6. ! A total of 176 telescope corrections were flagged in sub-array 1. ! A total of 55 telescope corrections were flagged in sub-array 3. ! A total of 63 telescope corrections were flagged in sub-array 4. ! A total of 136 telescope corrections were flagged in sub-array 5. ! A total of 65 telescope corrections were flagged in sub-array 6. ! A total of 59 telescope corrections were flagged in sub-array 7. ! A total of 88 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 7. ! A total of 176 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 136 telescope corrections were flagged in sub-array 5. ! A total of 36 telescope corrections were flagged in sub-array 6. ! A total of 30 telescope corrections were flagged in sub-array 7. ! A total of 88 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 8. ! A total of 176 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 136 telescope corrections were flagged in sub-array 5. ! A total of 36 telescope corrections were flagged in sub-array 6. ! A total of 30 telescope corrections were flagged in sub-array 7. ! A total of 88 telescope corrections were flagged in sub-array 8. ! ! Fit before self-cal, rms=1.007874Jy sigma=9.686171 ! Fit after self-cal, rms=0.917173Jy sigma=8.848772 ! 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 2.51% of the data. ! The x-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=0.5799 mas, bmaj=1.418 mas, bpa=-10.1 degrees ! Estimated noise=0.80269 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 = 0.0638055 Jy ! Component: 100 - total flux cleaned = 0.0817174 Jy ! Total flux subtracted in 100 components = 0.0817174 Jy ! Clean residual min=-0.003102 max=0.008305 Jy/beam ! Clean residual mean=-0.000000 rms=0.000714 Jy/beam ! Combined flux in latest and established models = 0.0817174 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.0817174 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=0.084643Jy sigma=0.676948 ! Fit after self-cal, rms=0.084067Jy sigma=0.673063 ! Inverting map ! Your choice of large map pixels excluded 2.51% of the data. ! The x-axis pixel size should ideally be below 0.1667 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00985103 Jy ! Component: 100 - total flux cleaned = 0.0150785 Jy ! Total flux subtracted in 100 components = 0.0150785 Jy ! Clean residual min=-0.002591 max=0.002524 Jy/beam ! Clean residual mean=0.000001 rms=0.000569 Jy/beam ! Combined flux in latest and established models = 0.0967959 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 9 components and 0.0967959 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=0.082659Jy sigma=0.654564 ! Fit after self-cal, rms=0.082548Jy sigma=0.654341 ! Inverting map ! Your choice of large map pixels excluded 2.51% of the data. ! The x-axis pixel size should ideally be below 0.1667 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 2.51% of the data. ! The x-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=0.75 mas, bmaj=1.765 mas, bpa=-9.156 degrees ! Estimated noise=0.363059 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 = 0.00415947 Jy ! Component: 100 - total flux cleaned = 0.00598423 Jy ! Component: 150 - total flux cleaned = 0.00688464 Jy ! Component: 200 - total flux cleaned = 0.00724127 Jy ! Total flux subtracted in 200 components = 0.00724127 Jy ! Clean residual min=-0.001592 max=0.002410 Jy/beam ! Clean residual mean=0.000003 rms=0.000354 Jy/beam ! Combined flux in latest and established models = 0.104037 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 16 components and 0.104037 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=0.082345Jy sigma=0.652321 ! Fit after self-cal, rms=0.082298Jy sigma=0.652270 ! Inverting map ! Your choice of large map pixels excluded 2.51% of the data. ! The x-axis pixel size should ideally be below 0.1667 milli-arcsec ! Added new window around map position (-3.2, 3.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00215856 Jy ! Component: 100 - total flux cleaned = 0.00312332 Jy ! Component: 150 - total flux cleaned = 0.0032743 Jy ! Component: 200 - total flux cleaned = 0.00331507 Jy ! Total flux subtracted in 200 components = 0.00331507 Jy ! Clean residual min=-0.001294 max=0.001319 Jy/beam ! Clean residual mean=0.000004 rms=0.000329 Jy/beam ! Combined flux in latest and established models = 0.107352 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 35 components and 0.107352 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=0.082245Jy sigma=0.651647 ! Fit after self-cal, rms=0.082226Jy sigma=0.651545 ! Inverting map ! Your choice of large map pixels excluded 2.51% of the data. ! The x-axis pixel size should ideally be below 0.1667 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.75 x 1.765 at -9.156 degrees (North through East) ! Clean map min=-0.0013158 max=0.087306 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* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 87 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! FD 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! 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 4: ! BR 1.00 FD 0.98 KP 1.00 LA 1.05 ! MK 1.00 NL 0.91 OV 1.01 PT 0.94 ! SC 0.96 ! ! A total of 66 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.96 EF 1.00* FD 1.00 HH 0.95 ! KP 1.01 LA 1.15 MC 0.90 NL 0.93 ! ON 0.95 PT 0.99 SC 0.92 ZC 0.94 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.03 EF 1.00* FD 1.01 KP 0.99 ! LA 1.04 MC 0.88 MK 0.97 NL 0.93 ! ON 0.86 PT 1.00 SC 0.99 ! ! Telescope amplitude corrections in sub-array 8: ! EF 0.00* HH 0.00* ON 0.00* ZC 0.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 87 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! FD 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! 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 4: ! BR 1.08 FD 0.98 KP 0.99 LA 1.06 ! MK 1.04 NL 0.98 OV 1.04 PT 0.99 ! SC 1.03 ! ! A total of 66 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! 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* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 0.99 EF 1.00* FD 1.01 KP 1.01 ! LA 1.10 MC 1.00 MK 1.07 NL 0.99 ! ON 1.04 PT 0.95 SC 0.98 ! ! Telescope amplitude corrections in sub-array 8: ! EF 0.00* HH 0.00* ON 0.00* ZC 0.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 87 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! FD 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 EF 1.00* FD 1.02 KP 0.95 ! LA 1.04 MC 0.90 NL 0.94 ON 0.91 ! OV 1.03 PT 1.01 SC 1.02 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 1.02 KP 0.93 LA 0.97 ! MK 0.96 NL 0.93 OV 1.02 PT 0.99 ! SC 1.10 ! ! A total of 66 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! 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* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.06 EF 1.00* FD 0.98 KP 0.94 ! LA 1.02 MC 0.92 MK 0.97 NL 0.99 ! ON 0.84 PT 1.08 SC 1.13 ! ! Telescope amplitude corrections in sub-array 8: ! EF 0.00* HH 0.00* ON 0.00* ZC 0.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 87 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! FD 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 EF 1.00* FD 0.99 KP 1.01 ! LA 1.06 MC 0.96 NL 0.97 ON 1.00 ! OV 1.02 PT 1.04 SC 0.92 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 FD 1.00 KP 0.98 LA 1.00 ! MK 0.98 NL 0.97 OV 1.00 PT 1.03 ! SC 1.06 ! ! A total of 66 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! 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* ZC 1.00* ! ! 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* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 8: ! EF 0.00* HH 0.00* ON 0.00* ZC 0.00* ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 87 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! FD 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! 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 4: ! BR 1.00* FD 1.03 KP 0.92 LA 1.01 ! MK 0.96 NL 0.99 OV 1.07 PT 0.98 ! SC 1.03 ! ! A total of 66 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.14 HH 1.04 ! KP 0.86 LA 1.00 MC 1.08 NL 1.00 ! ON 1.18 PT 1.03 SC 0.99 ZC 0.90 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* EF 1.00* FD 1.02 KP 0.94 ! LA 1.06 MC 1.03 MK 1.02 NL 0.95 ! ON 1.07 PT 1.05 SC 1.03 ! ! Telescope amplitude corrections in sub-array 8: ! EF 0.00* HH 0.00* ON 0.00* ZC 0.00* ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 87 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! FD 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 0.98 KP 0.89 ! LA 1.11 MC 0.95 NL 0.98 ON 1.13 ! OV 1.06 PT 0.96 SC 1.02 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00 KP 0.90 LA 1.00 ! MK 0.99 NL 0.98 OV 1.06 PT 0.93 ! SC 1.03 ! ! A total of 66 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 0.96 MC 1.10 ON 0.95 ! ZC 0.94 ! ! Telescope amplitude corrections in sub-array 6: ! 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* ZC 1.00* ! ! 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* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 8: ! EF 0.00* HH 0.00* ON 0.00* ZC 0.00* ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 87 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! FD 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! 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 4: ! BR 0.97 FD 1.06 KP 0.90 LA 1.05 ! MK 1.09 NL 0.99 OV 1.06 PT 0.98 ! SC 1.03 ! ! A total of 66 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 0.95 MC 1.01 ON 1.03 ! ZC 0.84 ! ! Telescope amplitude corrections in sub-array 6: ! 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* ZC 1.00* ! ! 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* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 8: ! EF 0.00* HH 0.00* ON 0.00* ZC 0.00* ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 87 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! FD 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.94 EF 1.00* FD 1.03 KP 0.95 ! LA 1.12 MC 0.89 NL 1.09 ON 1.13 ! OV 0.97 PT 1.03 SC 1.05 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 1.03 KP 0.96 LA 1.06 ! MK 1.04 NL 0.96 OV 1.00 PT 1.01 ! SC 1.02 ! ! A total of 66 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! 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* ZC 1.00* ! ! 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* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 8: ! EF 0.00* HH 0.00* ON 0.00* ZC 0.00* ! ! ! Fit before self-cal, rms=0.082226Jy sigma=0.651545 ! Fit after self-cal, rms=0.081804Jy sigma=0.652660 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=0.7584 mas, bmaj=1.767 mas, bpa=-9.281 degrees ! Estimated noise=0.364528 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 = -0.000205317 Jy ! Component: 100 - total flux cleaned = -0.000130558 Jy ! Component: 150 - total flux cleaned = -6.88607e-05 Jy ! Component: 200 - total flux cleaned = -1.66462e-05 Jy ! Total flux subtracted in 200 components = -1.66462e-05 Jy ! Clean residual min=-0.001135 max=0.001232 Jy/beam ! Clean residual mean=0.000001 rms=0.000269 Jy/beam ! Combined flux in latest and established models = 0.107336 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 41 components and 0.107336 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=0.081792Jy sigma=0.652533 ! Fit after self-cal, rms=0.081801Jy sigma=0.652456 ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 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=0.081801Jy sigma=0.652456 ! Fit after self-cal, rms=0.081412Jy sigma=0.651778 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=0.7579 mas, bmaj=1.769 mas, bpa=-9.32 degrees ! Estimated noise=0.36316 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000209025 Jy ! Component: 100 - total flux cleaned = -0.000190723 Jy ! Component: 150 - total flux cleaned = -0.000175984 Jy ! Component: 200 - total flux cleaned = -0.000175828 Jy ! Total flux subtracted in 200 components = -0.000175828 Jy ! Clean residual min=-0.001013 max=0.001153 Jy/beam ! Clean residual mean=0.000001 rms=0.000260 Jy/beam ! Combined flux in latest and established models = 0.10716 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 43 components and 0.10716 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=0.081406Jy sigma=0.651709 ! Fit after self-cal, rms=0.081403Jy sigma=0.651679 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 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 (29.2, -26.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000721121 Jy ! Component: 100 - total flux cleaned = 0.000699588 Jy ! Component: 150 - total flux cleaned = 0.000682049 Jy ! Component: 200 - total flux cleaned = 0.000648713 Jy ! Total flux subtracted in 200 components = 0.000648713 Jy ! Clean residual min=-0.001027 max=0.001060 Jy/beam ! Clean residual mean=0.000001 rms=0.000257 Jy/beam ! Combined flux in latest and established models = 0.107808 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 56 components and 0.107808 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=0.081384Jy sigma=0.651555 ! Fit after self-cal, rms=0.081377Jy sigma=0.651539 ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 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=0.081377Jy sigma=0.651539 ! Fit after self-cal, rms=0.081646Jy sigma=0.651350 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=0.7588 mas, bmaj=1.771 mas, bpa=-9.314 degrees ! Estimated noise=0.36313 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000218252 Jy ! Component: 100 - total flux cleaned = 0.000168909 Jy ! Component: 150 - total flux cleaned = 0.000168736 Jy ! Component: 200 - total flux cleaned = 0.000154265 Jy ! Total flux subtracted in 200 components = 0.000154265 Jy ! Clean residual min=-0.000963 max=0.001117 Jy/beam ! Clean residual mean=0.000001 rms=0.000252 Jy/beam ! Combined flux in latest and established models = 0.107963 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 59 components and 0.107963 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=0.081638Jy sigma=0.651301 ! Fit after self-cal, rms=0.081646Jy sigma=0.651288 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 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 (29, -49.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000660053 Jy ! Component: 100 - total flux cleaned = 0.000734783 Jy ! Component: 150 - total flux cleaned = 0.000798009 Jy ! Component: 200 - total flux cleaned = 0.000798155 Jy ! Total flux subtracted in 200 components = 0.000798155 Jy ! Clean residual min=-0.000954 max=0.000982 Jy/beam ! Clean residual mean=0.000001 rms=0.000248 Jy/beam ! Combined flux in latest and established models = 0.108761 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 74 components and 0.108761 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=0.081631Jy sigma=0.651180 ! Fit after self-cal, rms=0.081630Jy sigma=0.651166 ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 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=0.081630Jy sigma=0.651166 ! Fit after self-cal, rms=0.081610Jy sigma=0.651156 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=2.496 mas, bmaj=3.224 mas, bpa=-0.7589 degrees ! Estimated noise=0.440304 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000176597 Jy ! Component: 100 - total flux cleaned = 0.000198645 Jy ! Component: 150 - total flux cleaned = 0.000208055 Jy ! Component: 200 - total flux cleaned = 0.00022514 Jy ! Total flux subtracted in 200 components = 0.00022514 Jy ! Clean residual min=-0.001040 max=0.001267 Jy/beam ! Clean residual mean=0.000002 rms=0.000309 Jy/beam ! Combined flux in latest and established models = 0.108986 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 90 components and 0.108986 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=0.081607Jy sigma=0.651137 ! Fit after self-cal, rms=0.081608Jy sigma=0.651132 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 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 = 4.97396e-05 Jy ! Component: 100 - total flux cleaned = 6.50167e-05 Jy ! Component: 150 - total flux cleaned = 7.88551e-05 Jy ! Component: 200 - total flux cleaned = 7.85654e-05 Jy ! Total flux subtracted in 200 components = 7.85654e-05 Jy ! Clean residual min=-0.001040 max=0.001280 Jy/beam ! Clean residual mean=0.000002 rms=0.000309 Jy/beam ! Combined flux in latest and established models = 0.109065 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 97 components and 0.109065 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=0.081607Jy sigma=0.651126 ! Fit after self-cal, rms=0.081607Jy sigma=0.651124 ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 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 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=0.7586 mas, bmaj=1.772 mas, bpa=-9.331 degrees ! Estimated noise=0.362997 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7586 x 1.772 at -9.331 degrees (North through East) ! Clean map min=-0.00087025 max=0.08651 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 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=0.5841 mas, bmaj=1.421 mas, bpa=-10.15 degrees ! Estimated noise=0.810455 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0633081 Jy ! Component: 100 - total flux cleaned = 0.0821044 Jy ! Component: 150 - total flux cleaned = 0.0918678 Jy ! Component: 200 - total flux cleaned = 0.0970006 Jy ! Total flux subtracted in 200 components = 0.0970006 Jy ! Clean residual min=-0.002452 max=0.002526 Jy/beam ! Clean residual mean=-0.000000 rms=0.000544 Jy/beam ! Combined flux in latest and established models = 0.0970006 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 10 model components to the UV plane model. ! The established model now contains 10 components and 0.0970006 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=0.7586 mas, bmaj=1.772 mas, bpa=-9.331 degrees ! Estimated noise=0.362997 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 = 0.00387542 Jy ! Component: 100 - total flux cleaned = 0.00626614 Jy ! Component: 150 - total flux cleaned = 0.0080343 Jy ! Component: 200 - total flux cleaned = 0.009395 Jy ! Total flux subtracted in 200 components = 0.009395 Jy ! Clean residual min=-0.001010 max=0.001081 Jy/beam ! Clean residual mean=0.000000 rms=0.000265 Jy/beam ! Combined flux in latest and established models = 0.106396 Jy ! Adding 23 model components to the UV plane model. ! The established model now contains 27 components and 0.106396 Jy ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 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 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=2.496 mas, bmaj=3.224 mas, bpa=-0.7589 degrees ! Estimated noise=0.440304 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00124646 Jy ! Component: 100 - total flux cleaned = 0.00175031 Jy ! Component: 150 - total flux cleaned = 0.00207842 Jy ! Component: 200 - total flux cleaned = 0.00221417 Jy ! Total flux subtracted in 200 components = 0.00221417 Jy ! Clean residual min=-0.001041 max=0.001256 Jy/beam ! Clean residual mean=0.000002 rms=0.000312 Jy/beam ! Combined flux in latest and established models = 0.10861 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 = 0.000131729 Jy ! Component: 100 - total flux cleaned = 0.000203838 Jy ! Component: 150 - total flux cleaned = 0.000254669 Jy ! Component: 200 - total flux cleaned = 0.000300254 Jy ! Total flux subtracted in 200 components = 0.000300254 Jy ! Clean residual min=-0.001021 max=0.001263 Jy/beam ! Clean residual mean=0.000002 rms=0.000309 Jy/beam ! Combined flux in latest and established models = 0.10891 Jy ! Adding 44 model components to the UV plane model. ! The established model now contains 67 components and 0.10891 Jy ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=0.7586 mas, bmaj=1.772 mas, bpa=-9.331 degrees ! Estimated noise=0.362997 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000123025 Jy ! Component: 100 - total flux cleaned = -0.000152888 Jy ! Component: 150 - total flux cleaned = -0.00013131 Jy ! Component: 200 - total flux cleaned = -9.01039e-05 Jy ! Total flux subtracted in 200 components = -9.01039e-05 Jy ! Clean residual min=-0.001005 max=0.001023 Jy/beam ! Clean residual mean=0.000001 rms=0.000250 Jy/beam ! Combined flux in latest and established models = 0.10882 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 80 components and 0.10882 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=0.081637Jy sigma=0.651272 ! Fit after self-cal, rms=0.081637Jy sigma=0.651241 wmodel /scr/pima/gb073_uvs/J2311+1008_X_map.mod ! Writing 80 model components to file: /scr/pima/gb073_uvs/J2311+1008_X_map.mod wobs /scr/pima/gb073_uvs/J2311+1008_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J2311+1008_X_uvs.fits wwins /scr/pima/gb073_uvs/J2311+1008_X_map.win ! wwins: Wrote 4 windows to /scr/pima/gb073_uvs/J2311+1008_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 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 9.40712e-05 Jy ! Component: 100 - total flux cleaned = 0.000291636 Jy ! Component: 150 - total flux cleaned = 0.00039668 Jy ! Component: 200 - total flux cleaned = 0.000430734 Jy ! Component: 250 - total flux cleaned = 0.000497766 Jy ! Component: 300 - total flux cleaned = 0.000563914 Jy ! Component: 350 - total flux cleaned = 0.000628949 Jy ! Component: 400 - total flux cleaned = 0.000709252 Jy ! Component: 450 - total flux cleaned = 0.000788534 Jy ! Component: 500 - total flux cleaned = 0.00083583 Jy ! Component: 550 - total flux cleaned = 0.000913379 Jy ! Component: 600 - total flux cleaned = 0.000989935 Jy ! Component: 650 - total flux cleaned = 0.00102027 Jy ! Component: 700 - total flux cleaned = 0.00106568 Jy ! Component: 750 - total flux cleaned = 0.00112516 Jy ! Component: 800 - total flux cleaned = 0.0011398 Jy ! Component: 850 - total flux cleaned = 0.00106658 Jy ! Component: 900 - total flux cleaned = 0.00109587 Jy ! Component: 950 - total flux cleaned = 0.00111024 Jy ! Component: 1000 - total flux cleaned = 0.00116739 Jy ! Component: 1050 - total flux cleaned = 0.00111068 Jy ! Component: 1100 - total flux cleaned = 0.0010967 Jy ! Component: 1150 - total flux cleaned = 0.00112469 Jy ! Component: 1200 - total flux cleaned = 0.00111065 Jy ! Component: 1250 - total flux cleaned = 0.00113825 Jy ! Component: 1300 - total flux cleaned = 0.00116542 Jy ! Component: 1350 - total flux cleaned = 0.00116538 Jy ! Component: 1400 - total flux cleaned = 0.00119234 Jy ! Component: 1450 - total flux cleaned = 0.00117902 Jy ! Component: 1500 - total flux cleaned = 0.00119226 Jy ! Component: 1550 - total flux cleaned = 0.00123191 Jy ! Component: 1600 - total flux cleaned = 0.0011925 Jy ! Component: 1650 - total flux cleaned = 0.00124473 Jy ! Component: 1700 - total flux cleaned = 0.00127068 Jy ! Component: 1750 - total flux cleaned = 0.00130931 Jy ! Component: 1800 - total flux cleaned = 0.0012836 Jy ! Component: 1850 - total flux cleaned = 0.00128356 Jy ! Component: 1900 - total flux cleaned = 0.00125833 Jy ! Component: 1950 - total flux cleaned = 0.00132144 Jy ! Component: 2000 - total flux cleaned = 0.00135926 Jy ! Component: 2050 - total flux cleaned = 0.00133423 Jy ! Component: 2100 - total flux cleaned = 0.00135908 Jy ! Component: 2150 - total flux cleaned = 0.00140853 Jy ! Component: 2200 - total flux cleaned = 0.00138387 Jy ! Component: 2250 - total flux cleaned = 0.00143275 Jy ! Component: 2300 - total flux cleaned = 0.00144491 Jy ! Component: 2350 - total flux cleaned = 0.00148119 Jy ! Component: 2400 - total flux cleaned = 0.00140904 Jy ! Component: 2450 - total flux cleaned = 0.00148092 Jy ! Component: 2500 - total flux cleaned = 0.00149281 Jy ! Component: 2550 - total flux cleaned = 0.00152837 Jy ! Component: 2600 - total flux cleaned = 0.00154019 Jy ! Component: 2650 - total flux cleaned = 0.00151675 Jy ! Component: 2700 - total flux cleaned = 0.00156359 Jy ! Component: 2750 - total flux cleaned = 0.00161016 Jy ! Component: 2800 - total flux cleaned = 0.00157535 Jy ! Component: 2850 - total flux cleaned = 0.00162147 Jy ! Component: 2900 - total flux cleaned = 0.00163294 Jy ! Component: 2950 - total flux cleaned = 0.00165592 Jy ! Component: 3000 - total flux cleaned = 0.0016445 Jy ! Component: 3050 - total flux cleaned = 0.00165577 Jy ! Component: 3100 - total flux cleaned = 0.00168967 Jy ! Component: 3150 - total flux cleaned = 0.0016334 Jy ! Component: 3200 - total flux cleaned = 0.00172296 Jy ! Component: 3250 - total flux cleaned = 0.00166719 Jy ! Component: 3300 - total flux cleaned = 0.00168945 Jy ! Component: 3350 - total flux cleaned = 0.00170049 Jy ! Component: 3400 - total flux cleaned = 0.00173361 Jy ! Component: 3450 - total flux cleaned = 0.00172267 Jy ! Component: 3500 - total flux cleaned = 0.0017445 Jy ! Component: 3550 - total flux cleaned = 0.00177726 Jy ! Component: 3600 - total flux cleaned = 0.00176638 Jy ! Component: 3650 - total flux cleaned = 0.00179877 Jy ! Component: 3700 - total flux cleaned = 0.00182026 Jy ! Component: 3750 - total flux cleaned = 0.00184179 Jy ! Component: 3800 - total flux cleaned = 0.00187374 Jy ! Component: 3850 - total flux cleaned = 0.00188443 Jy ! Component: 3900 - total flux cleaned = 0.00187382 Jy ! Component: 3950 - total flux cleaned = 0.0018844 Jy ! Component: 4000 - total flux cleaned = 0.00184233 Jy ! Component: 4050 - total flux cleaned = 0.00193667 Jy ! Total flux subtracted in 4096 components = 0.00198896 Jy ! Clean residual min=-0.000649 max=0.000675 Jy/beam ! Clean residual mean=-0.000000 rms=0.000178 Jy/beam ! Combined flux in latest and established models = 0.110809 Jy keep ! Adding 322 model components to the UV plane model. ! The established model now contains 402 components and 0.110809 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J2311+1008_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7586 x 1.772 at -9.331 degrees (North through East) ! Clean map min=-0.00078046 max=0.086391 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J2311+1008_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0863909 invert ! Inverting map ! Your choice of large map pixels excluded 2.58% of the data. ! The x-axis pixel size should ideally be below 0.1667 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000177602 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.616737 0.616737 1.23347 2.46695 4.9339 9.86779 19.7356 39.4712 78.9423 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0005 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.086 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 486.431 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J2311+1008_X_uvs.log closed on Sat Dec 26 09:46:21 2015