! Started logfile: /scr/pima/gb073_uvs/J1231+6414_X_uvs.log on Sat Dec 26 09:38:38 2015 obs /scr/pima/gb073_uvs/J1231+6414_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1231+6414_X_uva.fits ! AN table 1: 29 integrations on 45 of 45 possible baselines. ! AN table 2: 29 integrations on 36 of 36 possible baselines. ! AN table 3: 29 integrations on 55 of 55 possible baselines. ! AN table 4: 29 integrations on 55 of 55 possible baselines. ! AN table 5: 29 integrations on 15 of 15 possible baselines. ! AN table 6: 29 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.696936 visibilities/baseline/integration-bin. ! Found source: J1231+6414 ! ! 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 40584 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/J1231+6414_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 58 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 87 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 87 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 87 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 87 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 87 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 87 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 87 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 87 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 5. ! A total of 87 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 116 telescope corrections were flagged in sub-array 3. ! A total of 87 telescope corrections were flagged in sub-array 4. ! A total of 87 telescope corrections were flagged in sub-array 5. ! A total of 58 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 6. ! A total of 87 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 116 telescope corrections were flagged in sub-array 3. ! A total of 87 telescope corrections were flagged in sub-array 4. ! A total of 87 telescope corrections were flagged in sub-array 5. ! A total of 58 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 7. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 87 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 87 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 8. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 87 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 87 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.003087Jy sigma=11.114128 ! Fit after self-cal, rms=0.962354Jy sigma=10.713329 ! 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 1.32% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=0.4991 mas, bmaj=0.6499 mas, bpa=10.8 degrees ! Estimated noise=0.965881 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 = 0.031263 Jy ! Component: 100 - total flux cleaned = 0.0380804 Jy ! Total flux subtracted in 100 components = 0.0380804 Jy ! Clean residual min=-0.003131 max=0.002930 Jy/beam ! Clean residual mean=0.000001 rms=0.000675 Jy/beam ! Combined flux in latest and established models = 0.0380804 Jy ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 0.0380804 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=0.063351Jy sigma=0.639123 ! Fit after self-cal, rms=0.061522Jy sigma=0.617656 ! Inverting map ! Your choice of large map pixels excluded 1.32% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-axis pixel size should ideally be below 0.1667 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00350931 Jy ! Component: 100 - total flux cleaned = 0.00308385 Jy ! Total flux subtracted in 100 components = 0.00308385 Jy ! Clean residual min=-0.002862 max=0.002910 Jy/beam ! Clean residual mean=0.000001 rms=0.000622 Jy/beam ! Combined flux in latest and established models = 0.0411643 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.0411643 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=0.061308Jy sigma=0.617000 ! Fit after self-cal, rms=0.061272Jy sigma=0.616850 ! Inverting map ! Your choice of large map pixels excluded 1.32% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-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 1.32% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=0.8503 mas, bmaj=1.047 mas, bpa=2.113 degrees ! Estimated noise=0.386007 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 = -0.00109638 Jy ! Component: 100 - total flux cleaned = -0.00118077 Jy ! Component: 150 - total flux cleaned = -0.00121566 Jy ! Component: 200 - total flux cleaned = -0.00126309 Jy ! Total flux subtracted in 200 components = -0.00126309 Jy ! Clean residual min=-0.001276 max=0.001446 Jy/beam ! Clean residual mean=0.000016 rms=0.000310 Jy/beam ! Combined flux in latest and established models = 0.0399012 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 8 components and 0.0399012 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=0.061249Jy sigma=0.616540 ! Fit after self-cal, rms=0.061216Jy sigma=0.616461 ! Inverting map ! Your choice of large map pixels excluded 1.32% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-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: 0.8503 x 1.047 at 2.113 degrees (North through East) ! Clean map min=-0.0011369 max=0.041691 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: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! ZC 1.00* ! ! 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* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* ZC 1.00* ! ! A total of 87 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 0.00* LA 0.00* MC 0.00* NL 0.00* ! ON 0.00* PT 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 EF 1.00* FD 1.00 KP 1.18 ! LA 1.06 MC 1.00* NL 1.11 ON 1.00* ! OV 1.05 PT 1.09 SC 0.88 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* ZC 1.00* ! ! A total of 87 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 0.00* LA 0.00* MC 0.00* NL 0.00* ! ON 0.00* PT 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.92 EF 1.00* FD 0.96 KP 1.12 ! LA 0.97 MC 1.00* NL 1.01 ON 1.00* ! OV 1.02 PT 0.99 SC 1.09 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 EF 1.00* FD 1.00 KP 0.97 ! LA 1.16 MK 1.06 NL 1.14 ON 1.00* ! OV 1.14 PT 1.04 ZC 0.95 ! ! A total of 87 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 0.00* LA 0.00* MC 0.00* NL 0.00* ! ON 0.00* PT 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.91 EF 1.00* FD 0.96 KP 1.02 ! LA 1.16 MC 0.91 NL 1.09 OV 0.93 ! PT 1.15 SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 EF 1.00* KP 0.98 LA 1.07 ! MK 0.89 NL 1.05 OV 1.10 PT 1.08 ! ZC 1.09 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.08 EF 1.00* FD 1.03 KP 1.11 ! LA 0.99 MC 1.00* NL 0.99 ON 1.00* ! OV 1.14 PT 1.14 SC 1.01 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 EF 1.00* FD 0.98 KP 1.15 ! LA 1.06 MK 1.08 NL 1.18 ON 1.00* ! OV 1.12 PT 1.06 ZC 1.07 ! ! A total of 87 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 0.00* LA 0.00* MC 0.00* NL 0.00* ! ON 0.00* PT 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.96 KP 1.00 ! LA 0.97 MC 0.84 NL 0.97 OV 1.09 ! PT 0.93 SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* KP 0.91 LA 0.97 ! MK 0.99 NL 1.04 OV 1.00 PT 0.94 ! ZC 1.05 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.08 KP 1.00 ! LA 0.96 MC 1.00* NL 1.05 ON 1.00* ! OV 0.96 PT 0.85 SC 0.94 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* ZC 1.00* ! ! A total of 87 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 0.00* LA 0.00* MC 0.00* NL 0.00* ! ON 0.00* PT 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! ZC 1.00* ! ! 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* EF 1.00* FD 0.96 KP 0.92 ! LA 1.08 MK 1.06 NL 1.11 ON 1.00* ! OV 0.97 PT 1.00 ZC 0.97 ! ! A total of 87 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 0.00* LA 0.00* MC 0.00* NL 0.00* ! ON 0.00* PT 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! ZC 1.00* ! ! 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* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* ZC 1.00* ! ! A total of 87 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 0.00* LA 0.00* MC 0.00* NL 0.00* ! ON 0.00* PT 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! ZC 1.00* ! ! 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* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* ZC 1.00* ! ! A total of 87 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 0.00* LA 0.00* MC 0.00* NL 0.00* ! ON 0.00* PT 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! ! Fit before self-cal, rms=0.061216Jy sigma=0.616461 ! Fit after self-cal, rms=0.062470Jy sigma=0.618347 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=0.8363 mas, bmaj=1.033 mas, bpa=1.079 degrees ! Estimated noise=0.398319 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 = 0.00025052 Jy ! Component: 100 - total flux cleaned = 0.000214234 Jy ! Component: 150 - total flux cleaned = 0.00018241 Jy ! Component: 200 - total flux cleaned = 0.000153438 Jy ! Total flux subtracted in 200 components = 0.000153438 Jy ! Clean residual min=-0.001199 max=0.001225 Jy/beam ! Clean residual mean=0.000011 rms=0.000282 Jy/beam ! Combined flux in latest and established models = 0.0400546 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 9 components and 0.0400546 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=0.062446Jy sigma=0.618318 ! Fit after self-cal, rms=0.062442Jy sigma=0.618186 ! Inverting map ! Your choice of large map pixels excluded 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-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=0.062442Jy sigma=0.618186 ! Fit after self-cal, rms=0.062606Jy sigma=0.618077 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=0.8361 mas, bmaj=1.033 mas, bpa=0.87 degrees ! Estimated noise=0.398553 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -5.51106e-05 Jy ! Component: 100 - total flux cleaned = -8.23621e-05 Jy ! Component: 150 - total flux cleaned = -0.00011702 Jy ! Component: 200 - total flux cleaned = -0.000138023 Jy ! Total flux subtracted in 200 components = -0.000138023 Jy ! Clean residual min=-0.001163 max=0.001219 Jy/beam ! Clean residual mean=0.000011 rms=0.000279 Jy/beam ! Combined flux in latest and established models = 0.0399166 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 10 components and 0.0399166 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=0.062596Jy sigma=0.618049 ! Fit after self-cal, rms=0.062595Jy sigma=0.617995 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-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 (-3.2, 3). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00108564 Jy ! Component: 100 - total flux cleaned = 0.0012693 Jy ! Component: 150 - total flux cleaned = 0.0014022 Jy ! Component: 200 - total flux cleaned = 0.00149498 Jy ! Total flux subtracted in 200 components = 0.00149498 Jy ! Clean residual min=-0.001119 max=0.001069 Jy/beam ! Clean residual mean=0.000008 rms=0.000269 Jy/beam ! Combined flux in latest and established models = 0.0414116 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 22 components and 0.0414116 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=0.062558Jy sigma=0.617698 ! Fit after self-cal, rms=0.062543Jy sigma=0.617566 ! Inverting map ! Your choice of large map pixels excluded 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-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=0.062543Jy sigma=0.617566 ! Fit after self-cal, rms=0.062688Jy sigma=0.617259 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=0.8362 mas, bmaj=1.033 mas, bpa=1.129 degrees ! Estimated noise=0.400261 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000767138 Jy ! Component: 100 - total flux cleaned = 0.000901443 Jy ! Component: 150 - total flux cleaned = 0.000999704 Jy ! Component: 200 - total flux cleaned = 0.00107169 Jy ! Total flux subtracted in 200 components = 0.00107169 Jy ! Clean residual min=-0.001164 max=0.001028 Jy/beam ! Clean residual mean=0.000006 rms=0.000257 Jy/beam ! Combined flux in latest and established models = 0.0424833 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 24 components and 0.0424833 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=0.062667Jy sigma=0.617128 ! Fit after self-cal, rms=0.062651Jy sigma=0.616928 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-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 = 0.000515276 Jy ! Component: 100 - total flux cleaned = 0.000614161 Jy ! Component: 150 - total flux cleaned = 0.000666779 Jy ! Component: 200 - total flux cleaned = 0.000715941 Jy ! Total flux subtracted in 200 components = 0.000715941 Jy ! Clean residual min=-0.001156 max=0.001000 Jy/beam ! Clean residual mean=0.000006 rms=0.000256 Jy/beam ! Combined flux in latest and established models = 0.0431992 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 25 components and 0.0431992 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=0.062635Jy sigma=0.616836 ! Fit after self-cal, rms=0.062625Jy sigma=0.616753 ! Inverting map ! Your choice of large map pixels excluded 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-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=0.062625Jy sigma=0.616753 ! Fit after self-cal, rms=0.062552Jy sigma=0.616585 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=2.882 mas, bmaj=3.139 mas, bpa=80.62 degrees ! Estimated noise=0.467043 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000260506 Jy ! Component: 100 - total flux cleaned = 0.00032316 Jy ! Component: 150 - total flux cleaned = 0.000344164 Jy ! Component: 200 - total flux cleaned = 0.000352084 Jy ! Total flux subtracted in 200 components = 0.000352084 Jy ! Clean residual min=-0.001122 max=0.000982 Jy/beam ! Clean residual mean=0.000010 rms=0.000290 Jy/beam ! Combined flux in latest and established models = 0.0435513 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 35 components and 0.0435513 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=0.062550Jy sigma=0.616563 ! Fit after self-cal, rms=0.062546Jy sigma=0.616456 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-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 = 0.000236943 Jy ! Component: 100 - total flux cleaned = 0.000269654 Jy ! Component: 150 - total flux cleaned = 0.000277785 Jy ! Component: 200 - total flux cleaned = 0.000285755 Jy ! Total flux subtracted in 200 components = 0.000285755 Jy ! Clean residual min=-0.001117 max=0.000991 Jy/beam ! Clean residual mean=0.000010 rms=0.000291 Jy/beam ! Combined flux in latest and established models = 0.0438371 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 38 components and 0.0438371 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=0.062545Jy sigma=0.616448 ! Fit after self-cal, rms=0.062544Jy sigma=0.616441 ! Inverting map ! Your choice of large map pixels excluded 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-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 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=0.834 mas, bmaj=1.03 mas, bpa=1.78 degrees ! Estimated noise=0.400388 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.834 x 1.03 at 1.78 degrees (North through East) ! Clean map min=-0.0014481 max=0.042814 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 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=0.4949 mas, bmaj=0.6458 mas, bpa=10.26 degrees ! Estimated noise=0.990948 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0352194 Jy ! Component: 100 - total flux cleaned = 0.0424697 Jy ! Component: 150 - total flux cleaned = 0.0443163 Jy ! Component: 200 - total flux cleaned = 0.0445257 Jy ! Total flux subtracted in 200 components = 0.0445257 Jy ! Clean residual min=-0.002737 max=0.002643 Jy/beam ! Clean residual mean=-0.000000 rms=0.000609 Jy/beam ! Combined flux in latest and established models = 0.0445257 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 11 model components to the UV plane model. ! The established model now contains 11 components and 0.0445257 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=0.834 mas, bmaj=1.03 mas, bpa=1.78 degrees ! Estimated noise=0.400388 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 = -0.000456852 Jy ! Component: 100 - total flux cleaned = -0.000496056 Jy ! Component: 150 - total flux cleaned = -0.000464352 Jy ! Component: 200 - total flux cleaned = -0.000380702 Jy ! Total flux subtracted in 200 components = -0.000380702 Jy ! Clean residual min=-0.001221 max=0.001023 Jy/beam ! Clean residual mean=0.000006 rms=0.000257 Jy/beam ! Combined flux in latest and established models = 0.044145 Jy ! Adding 15 model components to the UV plane model. ! The established model now contains 22 components and 0.044145 Jy ! Inverting map ! Your choice of large map pixels excluded 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-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 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=2.882 mas, bmaj=3.139 mas, bpa=80.62 degrees ! Estimated noise=0.467043 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000107131 Jy ! Component: 100 - total flux cleaned = -8.67719e-05 Jy ! Component: 150 - total flux cleaned = -7.15318e-05 Jy ! Component: 200 - total flux cleaned = -6.54747e-05 Jy ! Total flux subtracted in 200 components = -6.54747e-05 Jy ! Clean residual min=-0.001130 max=0.000966 Jy/beam ! Clean residual mean=0.000010 rms=0.000290 Jy/beam ! Combined flux in latest and established models = 0.0440796 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 = 5.46413e-06 Jy ! Component: 100 - total flux cleaned = 5.15883e-06 Jy ! Component: 150 - total flux cleaned = 4.99179e-06 Jy ! Component: 200 - total flux cleaned = 5.07836e-06 Jy ! Total flux subtracted in 200 components = 5.07836e-06 Jy ! Clean residual min=-0.001127 max=0.000960 Jy/beam ! Clean residual mean=0.000010 rms=0.000289 Jy/beam ! Combined flux in latest and established models = 0.0440846 Jy ! Adding 16 model components to the UV plane model. ! The established model now contains 37 components and 0.0440846 Jy ! Inverting map ! Your choice of large map pixels excluded 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-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 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-axis pixel size should ideally be below 0.1667 milli-arcsec ! Estimated beam: bmin=0.834 mas, bmaj=1.03 mas, bpa=1.78 degrees ! Estimated noise=0.400388 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000226196 Jy ! Component: 100 - total flux cleaned = 0.00022793 Jy ! Component: 150 - total flux cleaned = 0.000185002 Jy ! Component: 200 - total flux cleaned = 0.000166157 Jy ! Total flux subtracted in 200 components = 0.000166157 Jy ! Clean residual min=-0.001177 max=0.001003 Jy/beam ! Clean residual mean=0.000005 rms=0.000254 Jy/beam ! Combined flux in latest and established models = 0.0442508 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 42 components and 0.0442508 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=0.062559Jy sigma=0.616515 ! Fit after self-cal, rms=0.062565Jy sigma=0.616497 wmodel /scr/pima/gb073_uvs/J1231+6414_X_map.mod ! Writing 42 model components to file: /scr/pima/gb073_uvs/J1231+6414_X_map.mod wobs /scr/pima/gb073_uvs/J1231+6414_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1231+6414_X_uvs.fits wwins /scr/pima/gb073_uvs/J1231+6414_X_map.win ! wwins: Wrote 2 windows to /scr/pima/gb073_uvs/J1231+6414_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 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-axis pixel size should ideally be below 0.1667 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000433967 Jy ! Component: 100 - total flux cleaned = -0.000566812 Jy ! Component: 150 - total flux cleaned = -0.000493633 Jy ! Component: 200 - total flux cleaned = -0.000458167 Jy ! Component: 250 - total flux cleaned = -0.000388892 Jy ! Component: 300 - total flux cleaned = -0.000287366 Jy ! Component: 350 - total flux cleaned = -0.000187959 Jy ! Component: 400 - total flux cleaned = -0.000171598 Jy ! Component: 450 - total flux cleaned = -0.000107147 Jy ! Component: 500 - total flux cleaned = -2.76354e-05 Jy ! Component: 550 - total flux cleaned = 3.50595e-05 Jy ! Component: 600 - total flux cleaned = 9.69398e-05 Jy ! Component: 650 - total flux cleaned = 0.00015798 Jy ! Component: 700 - total flux cleaned = 0.000188111 Jy ! Component: 750 - total flux cleaned = 0.000218063 Jy ! Component: 800 - total flux cleaned = 0.000291833 Jy ! Component: 850 - total flux cleaned = 0.000262581 Jy ! Component: 900 - total flux cleaned = 0.000291614 Jy ! Component: 950 - total flux cleaned = 0.000320351 Jy ! Component: 1000 - total flux cleaned = 0.000362836 Jy ! Component: 1050 - total flux cleaned = 0.000348923 Jy ! Component: 1100 - total flux cleaned = 0.00041854 Jy ! Component: 1150 - total flux cleaned = 0.000418452 Jy ! Component: 1200 - total flux cleaned = 0.00041838 Jy ! Component: 1250 - total flux cleaned = 0.000432074 Jy ! Component: 1300 - total flux cleaned = 0.000445688 Jy ! Component: 1350 - total flux cleaned = 0.00048583 Jy ! Component: 1400 - total flux cleaned = 0.000472806 Jy ! Component: 1450 - total flux cleaned = 0.000564616 Jy ! Component: 1500 - total flux cleaned = 0.000577587 Jy ! Component: 1550 - total flux cleaned = 0.000577692 Jy ! Component: 1600 - total flux cleaned = 0.000603518 Jy ! Component: 1650 - total flux cleaned = 0.000705278 Jy ! Component: 1700 - total flux cleaned = 0.000742928 Jy ! Component: 1750 - total flux cleaned = 0.000755336 Jy ! Component: 1800 - total flux cleaned = 0.000742867 Jy ! Component: 1850 - total flux cleaned = 0.000816877 Jy ! Component: 1900 - total flux cleaned = 0.000804559 Jy ! Component: 1950 - total flux cleaned = 0.000865514 Jy ! Component: 2000 - total flux cleaned = 0.00085336 Jy ! Component: 2050 - total flux cleaned = 0.000937404 Jy ! Component: 2100 - total flux cleaned = 0.000961145 Jy ! Component: 2150 - total flux cleaned = 0.00100853 Jy ! Component: 2200 - total flux cleaned = 0.00100858 Jy ! Component: 2250 - total flux cleaned = 0.00103207 Jy ! Component: 2300 - total flux cleaned = 0.0010903 Jy ! Component: 2350 - total flux cleaned = 0.00111342 Jy ! Component: 2400 - total flux cleaned = 0.00112507 Jy ! Component: 2450 - total flux cleaned = 0.00112507 Jy ! Component: 2500 - total flux cleaned = 0.00118189 Jy ! Component: 2550 - total flux cleaned = 0.00113666 Jy ! Component: 2600 - total flux cleaned = 0.00117049 Jy ! Component: 2650 - total flux cleaned = 0.00115932 Jy ! Component: 2700 - total flux cleaned = 0.00117048 Jy ! Component: 2750 - total flux cleaned = 0.00120367 Jy ! Component: 2800 - total flux cleaned = 0.0012036 Jy ! Component: 2850 - total flux cleaned = 0.00124732 Jy ! Component: 2900 - total flux cleaned = 0.00123641 Jy ! Component: 2950 - total flux cleaned = 0.00121475 Jy ! Component: 3000 - total flux cleaned = 0.00125787 Jy ! Component: 3050 - total flux cleaned = 0.00129009 Jy ! Component: 3100 - total flux cleaned = 0.00132213 Jy ! Component: 3150 - total flux cleaned = 0.00135393 Jy ! Component: 3200 - total flux cleaned = 0.00137506 Jy ! Component: 3250 - total flux cleaned = 0.00138555 Jy ! Component: 3300 - total flux cleaned = 0.00139602 Jy ! Component: 3350 - total flux cleaned = 0.00142725 Jy ! Component: 3400 - total flux cleaned = 0.00141682 Jy ! Component: 3450 - total flux cleaned = 0.00141683 Jy ! Component: 3500 - total flux cleaned = 0.00144758 Jy ! Component: 3550 - total flux cleaned = 0.0014681 Jy ! Component: 3600 - total flux cleaned = 0.00145789 Jy ! Component: 3650 - total flux cleaned = 0.00151882 Jy ! Component: 3700 - total flux cleaned = 0.00153907 Jy ! Component: 3750 - total flux cleaned = 0.00155919 Jy ! Component: 3800 - total flux cleaned = 0.00157917 Jy ! Component: 3850 - total flux cleaned = 0.00157915 Jy ! Component: 3900 - total flux cleaned = 0.00154925 Jy ! Component: 3950 - total flux cleaned = 0.0015493 Jy ! Component: 4000 - total flux cleaned = 0.0015987 Jy ! Component: 4050 - total flux cleaned = 0.00158887 Jy ! Total flux subtracted in 4096 components = 0.00158887 Jy ! Clean residual min=-0.000564 max=0.000664 Jy/beam ! Clean residual mean=0.000002 rms=0.000160 Jy/beam ! Combined flux in latest and established models = 0.0458397 Jy keep ! Adding 309 model components to the UV plane model. ! The established model now contains 351 components and 0.0458397 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1231+6414_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-axis pixel size should ideally be below 0.1667 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.834 x 1.03 at 1.78 degrees (North through East) ! Clean map min=-0.0013086 max=0.042555 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1231+6414_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0425553 invert ! Inverting map ! Your choice of large map pixels excluded 1.35% of the data. ! The x-axis pixel size should ideally be below 0.1922 milli-arcsec ! The y-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 0.000158664 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.11852 1.11852 2.23704 4.47409 8.94817 17.8963 35.7927 71.5854 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0004 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.042 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 268.211 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1231+6414_X_uvs.log closed on Sat Dec 26 09:38:44 2015