! Started logfile: /scr/pima/gb073_uvs/J2054+2407_X_uvs.log on Sat Dec 26 09:44:48 2015 obs /scr/pima/gb073_uvs/J2054+2407_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J2054+2407_X_uva.fits ! AN table 1: 29 integrations on 66 of 66 possible baselines. ! AN table 2: 29 integrations on 55 of 55 possible baselines. ! AN table 3: 29 integrations on 36 of 36 possible baselines. ! AN table 4: 29 integrations on 55 of 55 possible baselines. ! AN table 5: 29 integrations on 21 of 21 possible baselines. ! Apparent sampling: 0.899808 visibilities/baseline/integration-bin. ! Found source: J2054+2407 ! ! 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 48640 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/J2054+2407_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 35 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 35 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 35 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 35 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 5. ! A total of 64 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 6. ! A total of 64 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 7. ! A total of 35 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 8. ! A total of 35 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.008035Jy sigma=10.122873 ! Fit after self-cal, rms=0.931096Jy sigma=9.310123 ! 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 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! Estimated beam: bmin=0.5572 mas, bmaj=1.136 mas, bpa=-11.31 degrees ! Estimated noise=0.81134 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 = 0.0522079 Jy ! Component: 100 - total flux cleaned = 0.065776 Jy ! Total flux subtracted in 100 components = 0.065776 Jy ! Clean residual min=-0.003418 max=0.006091 Jy/beam ! Clean residual mean=0.000002 rms=0.000677 Jy/beam ! Combined flux in latest and established models = 0.065776 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.065776 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=0.083100Jy sigma=0.692218 ! Fit after self-cal, rms=0.082407Jy sigma=0.686640 ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00731777 Jy ! Component: 100 - total flux cleaned = 0.0112896 Jy ! Total flux subtracted in 100 components = 0.0112896 Jy ! Clean residual min=-0.002911 max=0.004986 Jy/beam ! Clean residual mean=0.000002 rms=0.000602 Jy/beam ! Combined flux in latest and established models = 0.0770655 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 14 components and 0.0770655 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=0.081419Jy sigma=0.671678 ! Fit after self-cal, rms=0.081408Jy sigma=0.671502 ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! Added new window around map position (-0.8, 0.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00438204 Jy ! Component: 100 - total flux cleaned = 0.00669725 Jy ! Total flux subtracted in 100 components = 0.00669725 Jy ! Clean residual min=-0.002843 max=0.002515 Jy/beam ! Clean residual mean=0.000001 rms=0.000570 Jy/beam ! Combined flux in latest and established models = 0.0837628 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 30 components and 0.0837628 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=0.081047Jy sigma=0.666493 ! Fit after self-cal, rms=0.081016Jy sigma=0.666052 ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 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 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! Estimated beam: bmin=0.7607 mas, bmaj=1.494 mas, bpa=-7.998 degrees ! Estimated noise=0.351848 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 = 0.00356782 Jy ! Component: 100 - total flux cleaned = 0.00508337 Jy ! Component: 150 - total flux cleaned = 0.0058714 Jy ! Component: 200 - total flux cleaned = 0.00615678 Jy ! Total flux subtracted in 200 components = 0.00615678 Jy ! Clean residual min=-0.001479 max=0.002505 Jy/beam ! Clean residual mean=0.000003 rms=0.000336 Jy/beam ! Combined flux in latest and established models = 0.0899196 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 39 components and 0.0899196 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=0.080877Jy sigma=0.664381 ! Fit after self-cal, rms=0.080861Jy sigma=0.664200 ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! Added new window around map position (-2.6, 0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00239438 Jy ! Component: 100 - total flux cleaned = 0.00341346 Jy ! Component: 150 - total flux cleaned = 0.00344166 Jy ! Component: 200 - total flux cleaned = 0.00341879 Jy ! Total flux subtracted in 200 components = 0.00341879 Jy ! Clean residual min=-0.001378 max=0.001346 Jy/beam ! Clean residual mean=0.000002 rms=0.000296 Jy/beam ! Combined flux in latest and established models = 0.0933383 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 58 components and 0.0933383 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=0.080802Jy sigma=0.663376 ! Fit after self-cal, rms=0.080789Jy sigma=0.663221 ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7607 x 1.494 at -7.998 degrees (North through East) ! Clean map min=-0.0012457 max=0.070751 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* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 1.01 KP 1.04 LA 1.02 ! MC 0.86 MK 0.97 NL 0.95 ON 0.95 ! OV 1.01 PT 0.95 SC 0.95 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 1.02 KP 0.96 LA 1.10 ! MK 0.97 NL 0.97 ON 1.01 PT 0.98 ! SC 0.94 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 EF 1.00* FD 0.97 KP 0.97 ! LA 1.09 MK 1.02 NL 0.98 ON 0.84 ! OV 1.01 PT 0.96 SC 0.90 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.92 FD 0.94 KP 0.95 LA 1.02 ! NL 0.88 OV 1.09 PT 0.95 ! ! ! 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* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 1.11 KP 1.03 LA 1.08 ! MC 0.90 MK 1.04 NL 1.04 ON 0.89 ! OV 1.09 PT 1.01 SC 0.99 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 FD 1.02 KP 1.08 LA 0.97 ! MK 1.10 NL 1.02 ON 0.93 PT 1.10 ! SC 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.11 FD 1.08 KP 1.02 LA 0.98 ! NL 0.89 OV 1.06 PT 1.02 ! ! ! 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* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MC 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 EF 1.00* FD 0.94 KP 0.93 ! LA 0.96 MK 1.02 NL 1.01 ON 0.93 ! OV 0.98 PT 0.98 SC 0.99 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 1.02 KP 0.89 LA 0.91 ! NL 0.90 OV 0.97 PT 0.97 ! ! ! Correcting IF 4. ! 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* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 1.05 KP 1.02 LA 1.05 ! MC 0.94 MK 0.97 NL 1.00 ON 0.92 ! OV 0.98 PT 0.98 SC 1.01 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.11 FD 1.08 KP 1.01 LA 1.01 ! MK 0.99 NL 0.97 ON 0.93 PT 1.09 ! SC 1.07 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.07 EF 1.00* FD 0.96 KP 0.96 ! LA 1.02 MK 1.01 NL 0.95 ON 0.86 ! OV 1.02 PT 1.04 SC 0.99 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 FD 1.05 KP 0.95 LA 0.98 ! NL 0.91 OV 1.01 PT 1.01 ! ! ! Correcting IF 5. ! 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* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MC 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.99 KP 0.94 ! LA 1.00 MK 0.97 NL 0.98 ON 0.99 ! OV 1.03 PT 0.99 SC 1.00 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 0.96 KP 0.92 LA 1.05 ! NL 0.90 OV 1.04 PT 1.04 ! ! ! 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* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 0.91 KP 0.93 LA 1.05 ! MC 1.03 MK 0.98 NL 1.05 ON 1.17 ! OV 1.12 PT 0.97 SC 0.91 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 0.99 KP 0.89 LA 1.02 ! MK 1.03 NL 0.96 ON 1.13 PT 0.92 ! SC 0.92 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.93 KP 0.95 ! LA 0.98 MK 1.01 NL 0.98 ON 1.11 ! OV 0.99 PT 0.92 SC 0.99 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 1.02 KP 0.87 LA 0.93 ! NL 0.95 OV 1.01 PT 0.87 ! ! ! 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* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MC 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* ON 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* SC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.07 FD 1.07 KP 0.90 LA 1.02 ! NL 0.97 OV 0.97 PT 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* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.08 FD 1.08 KP 0.93 LA 1.02 ! MC 1.08 MK 1.03 NL 1.00 ON 1.01 ! OV 1.02 PT 1.08 SC 0.94 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 FD 0.98 KP 1.00 LA 1.01 ! MK 0.97 NL 1.15 ON 1.14 PT 1.00 ! SC 0.96 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 EF 1.00* FD 1.05 KP 0.86 ! LA 1.01 MK 1.05 NL 0.99 ON 1.12 ! OV 0.98 PT 1.00 SC 1.01 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 1.03 KP 0.89 LA 0.96 ! NL 1.06 OV 0.97 PT 0.97 ! ! ! Fit before self-cal, rms=0.080789Jy sigma=0.663221 ! Fit after self-cal, rms=0.079773Jy sigma=0.661236 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! Estimated beam: bmin=0.7607 mas, bmaj=1.493 mas, bpa=-7.977 degrees ! Estimated noise=0.349898 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 = -0.00013857 Jy ! Component: 100 - total flux cleaned = -0.000120241 Jy ! Component: 150 - total flux cleaned = -0.000104684 Jy ! Component: 200 - total flux cleaned = -9.21902e-05 Jy ! Total flux subtracted in 200 components = -9.21902e-05 Jy ! Clean residual min=-0.001053 max=0.001210 Jy/beam ! Clean residual mean=0.000001 rms=0.000247 Jy/beam ! Combined flux in latest and established models = 0.0932462 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 70 components and 0.0932461 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=0.079762Jy sigma=0.661121 ! Fit after self-cal, rms=0.079764Jy sigma=0.661056 ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 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=0.079764Jy sigma=0.661056 ! Fit after self-cal, rms=0.079590Jy sigma=0.661043 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! Estimated beam: bmin=0.7607 mas, bmaj=1.494 mas, bpa=-8.043 degrees ! Estimated noise=0.34896 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000189169 Jy ! Component: 100 - total flux cleaned = -0.000174281 Jy ! Component: 150 - total flux cleaned = -0.000148703 Jy ! Component: 200 - total flux cleaned = -0.000137069 Jy ! Total flux subtracted in 200 components = -0.000137069 Jy ! Clean residual min=-0.001046 max=0.001212 Jy/beam ! Clean residual mean=0.000001 rms=0.000245 Jy/beam ! Combined flux in latest and established models = 0.0931091 Jy selfcal ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 76 components and 0.0931091 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=0.079582Jy sigma=0.660967 ! Fit after self-cal, rms=0.079582Jy sigma=0.660960 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 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 (26.2, -10.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000841299 Jy ! Component: 100 - total flux cleaned = 0.000795911 Jy ! Component: 150 - total flux cleaned = 0.000757406 Jy ! Component: 200 - total flux cleaned = 0.000740967 Jy ! Total flux subtracted in 200 components = 0.000740967 Jy ! Clean residual min=-0.001083 max=0.001157 Jy/beam ! Clean residual mean=0.000001 rms=0.000241 Jy/beam ! Combined flux in latest and established models = 0.09385 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 88 components and 0.0938501 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=0.079561Jy sigma=0.660810 ! Fit after self-cal, rms=0.079557Jy sigma=0.660791 ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! Added new window around map position (-14.6, 14.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000763183 Jy ! Component: 100 - total flux cleaned = 0.000888517 Jy ! Component: 150 - total flux cleaned = 0.000890735 Jy ! Component: 200 - total flux cleaned = 0.000927064 Jy ! Total flux subtracted in 200 components = 0.000927064 Jy ! Clean residual min=-0.001011 max=0.000996 Jy/beam ! Clean residual mean=0.000001 rms=0.000236 Jy/beam ! Combined flux in latest and established models = 0.0947771 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 99 components and 0.0947771 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=0.079536Jy sigma=0.660647 ! Fit after self-cal, rms=0.079533Jy sigma=0.660625 ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 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=0.079533Jy sigma=0.660625 ! Fit after self-cal, rms=0.079800Jy sigma=0.660426 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! Estimated beam: bmin=0.7615 mas, bmaj=1.499 mas, bpa=-7.994 degrees ! Estimated noise=0.349004 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00011477 Jy ! Component: 100 - total flux cleaned = 7.98043e-05 Jy ! Component: 150 - total flux cleaned = 6.366e-05 Jy ! Component: 200 - total flux cleaned = 4.73944e-05 Jy ! Total flux subtracted in 200 components = 4.73944e-05 Jy ! Clean residual min=-0.001013 max=0.000986 Jy/beam ! Clean residual mean=0.000001 rms=0.000234 Jy/beam ! Combined flux in latest and established models = 0.0948245 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 104 components and 0.0948245 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=0.079791Jy sigma=0.660355 ! Fit after self-cal, rms=0.079797Jy sigma=0.660338 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 5.32855e-05 Jy ! Component: 100 - total flux cleaned = 3.79921e-05 Jy ! Component: 150 - total flux cleaned = 5.21842e-05 Jy ! Component: 200 - total flux cleaned = 5.17463e-05 Jy ! Total flux subtracted in 200 components = 5.17463e-05 Jy ! Clean residual min=-0.001003 max=0.000977 Jy/beam ! Clean residual mean=0.000001 rms=0.000233 Jy/beam ! Combined flux in latest and established models = 0.0948763 Jy ! Performing phase self-cal ! Adding 32 model components to the UV plane model. ! The established model now contains 112 components and 0.0948763 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=0.079789Jy sigma=0.660290 ! Fit after self-cal, rms=0.079789Jy sigma=0.660287 ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 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=0.079789Jy sigma=0.660287 ! Fit after self-cal, rms=0.079780Jy sigma=0.660289 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! Estimated beam: bmin=2.649 mas, bmaj=3.14 mas, bpa=2.241 degrees ! Estimated noise=0.421901 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000141776 Jy ! Component: 100 - total flux cleaned = 0.000302249 Jy ! Component: 150 - total flux cleaned = 0.000384416 Jy ! Component: 200 - total flux cleaned = 0.000385191 Jy ! Total flux subtracted in 200 components = 0.000385191 Jy ! Clean residual min=-0.001135 max=0.001118 Jy/beam ! Clean residual mean=0.000001 rms=0.000269 Jy/beam ! Combined flux in latest and established models = 0.0952615 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 122 components and 0.0952615 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=0.079776Jy sigma=0.660260 ! Fit after self-cal, rms=0.079776Jy sigma=0.660249 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 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 = 0.000172164 Jy ! Component: 100 - total flux cleaned = 0.000210664 Jy ! Component: 150 - total flux cleaned = 0.000210687 Jy ! Component: 200 - total flux cleaned = 0.000233581 Jy ! Total flux subtracted in 200 components = 0.000233581 Jy ! Clean residual min=-0.001159 max=0.001140 Jy/beam ! Clean residual mean=0.000001 rms=0.000268 Jy/beam ! Combined flux in latest and established models = 0.095495 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 125 components and 0.095495 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=0.079774Jy sigma=0.660242 ! Fit after self-cal, rms=0.079774Jy sigma=0.660240 ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 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 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! Estimated beam: bmin=0.7617 mas, bmaj=1.5 mas, bpa=-8.016 degrees ! Estimated noise=0.348741 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7617 x 1.5 at -8.016 degrees (North through East) ! Clean map min=-0.00086948 max=0.070108 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 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! Estimated beam: bmin=0.5575 mas, bmaj=1.141 mas, bpa=-11.18 degrees ! Estimated noise=0.808844 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0523545 Jy ! Component: 100 - total flux cleaned = 0.066921 Jy ! Component: 150 - total flux cleaned = 0.0746152 Jy ! Component: 200 - total flux cleaned = 0.0794584 Jy ! Total flux subtracted in 200 components = 0.0794584 Jy ! Clean residual min=-0.002672 max=0.002624 Jy/beam ! Clean residual mean=0.000001 rms=0.000571 Jy/beam ! Combined flux in latest and established models = 0.0794584 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 17 model components to the UV plane model. ! The established model now contains 17 components and 0.0794584 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! Estimated beam: bmin=0.7617 mas, bmaj=1.5 mas, bpa=-8.016 degrees ! Estimated noise=0.348741 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 = 0.00543541 Jy ! Component: 100 - total flux cleaned = 0.0084757 Jy ! Component: 150 - total flux cleaned = 0.0105158 Jy ! Component: 200 - total flux cleaned = 0.0120492 Jy ! Total flux subtracted in 200 components = 0.0120492 Jy ! Clean residual min=-0.001068 max=0.001286 Jy/beam ! Clean residual mean=0.000002 rms=0.000258 Jy/beam ! Combined flux in latest and established models = 0.0915076 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 39 components and 0.0915076 Jy ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! Added new window around map position (-4.2, 0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00136647 Jy ! Component: 100 - total flux cleaned = 0.00205277 Jy ! Component: 150 - total flux cleaned = 0.00246143 Jy ! Component: 200 - total flux cleaned = 0.00264254 Jy ! Total flux subtracted in 200 components = 0.00264254 Jy ! Clean residual min=-0.000983 max=0.001035 Jy/beam ! Clean residual mean=0.000001 rms=0.000236 Jy/beam ! Combined flux in latest and established models = 0.0941502 Jy ! Adding 29 model components to the UV plane model. ! The established model now contains 56 components and 0.0941502 Jy ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! Added new window around map position (11, 1.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000990344 Jy ! Component: 100 - total flux cleaned = 0.00121221 Jy ! Component: 150 - total flux cleaned = 0.00134018 Jy ! Component: 200 - total flux cleaned = 0.00145924 Jy ! Total flux subtracted in 200 components = 0.00145924 Jy ! Clean residual min=-0.001026 max=0.000967 Jy/beam ! Clean residual mean=0.000001 rms=0.000231 Jy/beam ! Combined flux in latest and established models = 0.0956094 Jy ! Adding 36 model components to the UV plane model. ! The established model now contains 74 components and 0.0956094 Jy ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 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 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! Estimated beam: bmin=2.649 mas, bmaj=3.14 mas, bpa=2.241 degrees ! Estimated noise=0.421901 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000502976 Jy ! Component: 100 - total flux cleaned = 0.000648457 Jy ! Component: 150 - total flux cleaned = 0.000803805 Jy ! Component: 200 - total flux cleaned = 0.000857889 Jy ! Total flux subtracted in 200 components = 0.000857889 Jy ! Clean residual min=-0.001044 max=0.001094 Jy/beam ! Clean residual mean=0.000000 rms=0.000262 Jy/beam ! Combined flux in latest and established models = 0.0964673 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 = 1.21403e-05 Jy ! Component: 100 - total flux cleaned = 4.54058e-05 Jy ! Component: 150 - total flux cleaned = 6.60423e-05 Jy ! Component: 200 - total flux cleaned = 8.51915e-05 Jy ! Total flux subtracted in 200 components = 8.51915e-05 Jy ! Clean residual min=-0.001050 max=0.001060 Jy/beam ! Clean residual mean=0.000000 rms=0.000258 Jy/beam ! Combined flux in latest and established models = 0.0965525 Jy ! Adding 37 model components to the UV plane model. ! The established model now contains 105 components and 0.0965525 Jy ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! Estimated beam: bmin=0.7617 mas, bmaj=1.5 mas, bpa=-8.016 degrees ! Estimated noise=0.348741 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000189381 Jy ! Component: 100 - total flux cleaned = -0.000271683 Jy ! Component: 150 - total flux cleaned = -0.00029125 Jy ! Component: 200 - total flux cleaned = -0.000310107 Jy ! Total flux subtracted in 200 components = -0.000310107 Jy ! Clean residual min=-0.001008 max=0.000969 Jy/beam ! Clean residual mean=0.000000 rms=0.000224 Jy/beam ! Combined flux in latest and established models = 0.0962424 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 115 components and 0.0962424 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=0.079764Jy sigma=0.660136 ! Fit after self-cal, rms=0.079743Jy sigma=0.660064 wmodel /scr/pima/gb073_uvs/J2054+2407_X_map.mod ! Writing 115 model components to file: /scr/pima/gb073_uvs/J2054+2407_X_map.mod wobs /scr/pima/gb073_uvs/J2054+2407_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J2054+2407_X_uvs.fits wwins /scr/pima/gb073_uvs/J2054+2407_X_map.win ! wwins: Wrote 7 windows to /scr/pima/gb073_uvs/J2054+2407_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 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000169187 Jy ! Component: 100 - total flux cleaned = -0.000288361 Jy ! Component: 150 - total flux cleaned = -0.000337569 Jy ! Component: 200 - total flux cleaned = -0.000337722 Jy ! Component: 250 - total flux cleaned = -0.000321986 Jy ! Component: 300 - total flux cleaned = -0.000291307 Jy ! Component: 350 - total flux cleaned = -0.000231087 Jy ! Component: 400 - total flux cleaned = -0.00023129 Jy ! Component: 450 - total flux cleaned = -0.000260652 Jy ! Component: 500 - total flux cleaned = -0.000231544 Jy ! Component: 550 - total flux cleaned = -0.000245911 Jy ! Component: 600 - total flux cleaned = -0.000274394 Jy ! Component: 650 - total flux cleaned = -0.000246329 Jy ! Component: 700 - total flux cleaned = -0.000302181 Jy ! Component: 750 - total flux cleaned = -0.000274606 Jy ! Component: 800 - total flux cleaned = -0.000301942 Jy ! Component: 850 - total flux cleaned = -0.000315525 Jy ! Component: 900 - total flux cleaned = -0.00034251 Jy ! Component: 950 - total flux cleaned = -0.000369089 Jy ! Component: 1000 - total flux cleaned = -0.000395248 Jy ! Component: 1050 - total flux cleaned = -0.000395194 Jy ! Component: 1100 - total flux cleaned = -0.000447264 Jy ! Component: 1150 - total flux cleaned = -0.00047309 Jy ! Component: 1200 - total flux cleaned = -0.000511484 Jy ! Component: 1250 - total flux cleaned = -0.000486327 Jy ! Component: 1300 - total flux cleaned = -0.000536711 Jy ! Component: 1350 - total flux cleaned = -0.000561586 Jy ! Component: 1400 - total flux cleaned = -0.000549046 Jy ! Component: 1450 - total flux cleaned = -0.000524376 Jy ! Component: 1500 - total flux cleaned = -0.000573512 Jy ! Component: 1550 - total flux cleaned = -0.000561328 Jy ! Component: 1600 - total flux cleaned = -0.000537152 Jy ! Component: 1650 - total flux cleaned = -0.000549221 Jy ! Component: 1700 - total flux cleaned = -0.000561211 Jy ! Component: 1750 - total flux cleaned = -0.000525377 Jy ! Component: 1800 - total flux cleaned = -0.0005491 Jy ! Component: 1850 - total flux cleaned = -0.000513785 Jy ! Component: 1900 - total flux cleaned = -0.000525613 Jy ! Component: 1950 - total flux cleaned = -0.000478921 Jy ! Component: 2000 - total flux cleaned = -0.000525489 Jy ! Component: 2050 - total flux cleaned = -0.000513891 Jy ! Component: 2100 - total flux cleaned = -0.000536876 Jy ! Component: 2150 - total flux cleaned = -0.000513887 Jy ! Component: 2200 - total flux cleaned = -0.000513795 Jy ! Component: 2250 - total flux cleaned = -0.000502457 Jy ! Component: 2300 - total flux cleaned = -0.000536321 Jy ! Component: 2350 - total flux cleaned = -0.000457656 Jy ! Component: 2400 - total flux cleaned = -0.000468903 Jy ! Component: 2450 - total flux cleaned = -0.00052465 Jy ! Component: 2500 - total flux cleaned = -0.000502433 Jy ! Component: 2550 - total flux cleaned = -0.000502405 Jy ! Component: 2600 - total flux cleaned = -0.00053535 Jy ! Component: 2650 - total flux cleaned = -0.000513366 Jy ! Component: 2700 - total flux cleaned = -0.000491481 Jy ! Component: 2750 - total flux cleaned = -0.000469763 Jy ! Component: 2800 - total flux cleaned = -0.00049136 Jy ! Component: 2850 - total flux cleaned = -0.000426725 Jy ! Component: 2900 - total flux cleaned = -0.000416008 Jy ! Component: 2950 - total flux cleaned = -0.000437399 Jy ! Component: 3000 - total flux cleaned = -0.00044797 Jy ! Component: 3050 - total flux cleaned = -0.000405496 Jy ! Component: 3100 - total flux cleaned = -0.000426607 Jy ! Component: 3150 - total flux cleaned = -0.000426608 Jy ! Component: 3200 - total flux cleaned = -0.00040564 Jy ! Component: 3250 - total flux cleaned = -0.000353397 Jy ! Component: 3300 - total flux cleaned = -0.000395053 Jy ! Component: 3350 - total flux cleaned = -0.000332809 Jy ! Component: 3400 - total flux cleaned = -0.000353429 Jy ! Component: 3450 - total flux cleaned = -0.000332805 Jy ! Component: 3500 - total flux cleaned = -0.000291774 Jy ! Component: 3550 - total flux cleaned = -0.000353096 Jy ! Component: 3600 - total flux cleaned = -0.000322475 Jy ! Component: 3650 - total flux cleaned = -0.000332679 Jy ! Component: 3700 - total flux cleaned = -0.000312402 Jy ! Component: 3750 - total flux cleaned = -0.000292331 Jy ! Component: 3800 - total flux cleaned = -0.000302396 Jy ! Component: 3850 - total flux cleaned = -0.000272328 Jy ! Component: 3900 - total flux cleaned = -0.000322318 Jy ! Component: 3950 - total flux cleaned = -0.000292398 Jy ! Component: 4000 - total flux cleaned = -0.000312243 Jy ! Component: 4050 - total flux cleaned = -0.000282584 Jy ! Total flux subtracted in 4096 components = -0.000262799 Jy ! Clean residual min=-0.000538 max=0.000629 Jy/beam ! Clean residual mean=0.000000 rms=0.000164 Jy/beam ! Combined flux in latest and established models = 0.0959796 Jy keep ! Adding 309 model components to the UV plane model. ! The established model now contains 424 components and 0.0959796 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J2054+2407_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7617 x 1.5 at -8.016 degrees (North through East) ! Clean map min=-0.00086786 max=0.069961 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J2054+2407_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.069961 invert ! Inverting map ! Your choice of large map pixels excluded 3.55% of the data. ! The x-axis pixel size should ideally be below 0.1748 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00016422 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.704194 0.704194 1.40839 2.81677 5.63355 11.2671 22.5342 45.0684 90.1368 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0004 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.069 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 426.019 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J2054+2407_X_uvs.log closed on Sat Dec 26 09:44:55 2015