! Started logfile: /scr/pima/gb073_uvs/J1408+6505_X_uvs.log on Sat Dec 26 09:40:20 2015 obs /scr/pima/gb073_uvs/J1408+6505_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1408+6505_X_uva.fits ! AN table 1: 29 integrations on 6 of 6 possible baselines. ! AN table 2: 29 integrations on 45 of 45 possible baselines. ! AN table 3: 29 integrations on 45 of 45 possible baselines. ! AN table 4: 29 integrations on 55 of 55 possible baselines. ! AN table 5: 58 integrations on 55 of 55 possible baselines. ! AN table 6: 29 integrations on 36 of 36 possible baselines. ! Apparent sampling: 0.893069 visibilities/baseline/integration-bin. ! Found source: J1408+6505 ! ! 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 61536 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/J1408+6505_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 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 58 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 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 58 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 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 58 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 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 58 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 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 87 telescope corrections were flagged in sub-array 4. ! A total of 116 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 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 87 telescope corrections were flagged in sub-array 4. ! A total of 116 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 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 58 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 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 58 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=1.001923Jy sigma=10.848629 ! Fit after self-cal, rms=0.958842Jy sigma=10.406665 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.4834 mas, bmaj=0.6436 mas, bpa=54.55 degrees ! Estimated noise=0.725758 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 = 0.035112 Jy ! Component: 100 - total flux cleaned = 0.0410227 Jy ! Total flux subtracted in 100 components = 0.0410227 Jy ! Clean residual min=-0.002964 max=0.003025 Jy/beam ! Clean residual mean=-0.000001 rms=0.000509 Jy/beam ! Combined flux in latest and established models = 0.0410227 Jy ! Performing phase self-cal ! Adding 3 model components to the UV plane model. ! The established model now contains 3 components and 0.0410227 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=0.069401Jy sigma=0.663567 ! Fit after self-cal, rms=0.067739Jy sigma=0.643652 ! Inverting map ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00277995 Jy ! Component: 100 - total flux cleaned = 0.00247798 Jy ! Total flux subtracted in 100 components = 0.00247798 Jy ! Clean residual min=-0.002311 max=0.002095 Jy/beam ! Clean residual mean=-0.000001 rms=0.000482 Jy/beam ! Combined flux in latest and established models = 0.0435007 Jy ! Performing phase self-cal ! Adding 3 model components to the UV plane model. ! The established model now contains 3 components and 0.0435007 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=0.067494Jy sigma=0.642652 ! Fit after self-cal, rms=0.067447Jy sigma=0.642565 ! Inverting map ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec print "************** FINISHED UNIFORM WEIGHTING CLEAN **************" ! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** ! uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. win_mult = win_mult * 1.6 clean_niter = clean_niter * 2 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.7521 mas, bmaj=0.8908 mas, bpa=51.91 degrees ! Estimated noise=0.312448 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 = -0.00120505 Jy ! Component: 100 - total flux cleaned = -0.0012511 Jy ! Component: 150 - total flux cleaned = -0.00130767 Jy ! Component: 200 - total flux cleaned = -0.00132426 Jy ! Total flux subtracted in 200 components = -0.00132426 Jy ! Clean residual min=-0.000937 max=0.000888 Jy/beam ! Clean residual mean=-0.000002 rms=0.000217 Jy/beam ! Combined flux in latest and established models = 0.0421765 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.0421765 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=0.067421Jy sigma=0.642297 ! Fit after self-cal, rms=0.067380Jy sigma=0.642187 ! Inverting map ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7521 x 0.8908 at 51.91 degrees (North through East) ! Clean map min=-0.00077003 max=0.045556 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! KP 0.82 MK 0.95 OV 1.01 ZC 1.09 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 EF 1.00* FD 1.09 KP 1.02 ! LA 1.17 MK 0.95 NL 1.03 OV 0.94 ! PT 0.94 ZC 1.04 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.96 EF 1.00* KP 1.00 LA 1.13 ! MK 1.15 NL 1.01 ON 0.80 OV 1.07 ! PT 0.89 ZC 1.00 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.91 EF 1.00* FD 0.96 KP 0.93 ! LA 1.05 MC 1.11 NL 1.04 ON 1.00* ! OV 1.09 PT 0.95 SC 1.09 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 EF 1.00* FD 1.02 KP 0.95 ! LA 1.01 MK 1.06 NL 0.97 ON 0.82 ! OV 0.97 PT 0.98 ZC 1.07 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.93 EF 1.00* FD 1.00 KP 1.16 ! LA 1.04 MK 1.03 NL 0.95 ON 0.75 ! PT 0.99 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! KP 1.06 MK 0.89 OV 1.11 ZC 0.96 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.11 EF 1.00* FD 1.00 KP 1.02 ! LA 1.07 MK 0.95 NL 0.97 OV 1.05 ! PT 1.07 ZC 1.05 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 EF 1.00* KP 1.17 LA 1.06 ! MK 1.15 NL 1.01 ON 0.76 OV 1.03 ! PT 1.02 ZC 0.97 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.18 EF 1.00* FD 1.05 KP 1.15 ! LA 1.11 MC 0.92 NL 1.06 ON 1.00* ! OV 1.02 PT 0.98 SC 1.05 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 EF 1.00* FD 0.96 KP 1.10 ! LA 1.09 MK 1.11 NL 1.07 ON 0.78 ! OV 0.96 PT 1.02 ZC 1.11 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00 EF 1.00* FD 0.98 KP 1.13 ! LA 1.12 MK 1.11 NL 1.09 ON 0.65 ! PT 1.04 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! KP 0.90 MK 0.96 OV 1.01 ZC 0.85 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 EF 1.00* FD 1.01 KP 1.01 ! LA 0.94 MK 1.07 NL 1.05 OV 0.93 ! PT 1.07 ZC 1.05 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.93 EF 1.00* KP 0.98 LA 0.99 ! MK 1.02 NL 0.88 ON 0.70 OV 1.11 ! PT 1.20 ZC 0.90 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.93 EF 1.00* FD 1.10 KP 0.88 ! LA 0.98 MC 0.89 NL 1.11 ON 1.00* ! OV 0.99 PT 1.08 SC 1.19 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 EF 1.00* FD 1.04 KP 1.00 ! LA 0.99 MK 1.09 NL 0.96 ON 0.76 ! OV 0.98 PT 1.07 ZC 1.01 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.03 EF 1.00* FD 0.95 KP 1.10 ! LA 0.90 MK 0.97 NL 1.03 ON 0.73 ! PT 1.08 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! KP 1.12 MK 0.82 OV 0.95 ZC 0.88 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 EF 1.00* FD 1.16 KP 1.18 ! LA 0.96 MK 1.07 NL 0.95 OV 0.98 ! PT 0.99 ZC 0.98 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 EF 1.00* KP 1.07 LA 1.08 ! MK 1.06 NL 1.11 ON 0.92 OV 0.96 ! PT 0.99 ZC 1.19 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 EF 1.00* FD 0.96 KP 1.11 ! LA 0.96 MC 1.07 NL 1.05 ON 1.00* ! OV 0.89 PT 1.03 SC 1.25 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 EF 1.00* FD 1.04 KP 1.08 ! LA 1.01 MK 1.04 NL 1.08 ON 0.93 ! OV 1.00 PT 1.02 ZC 0.94 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 EF 1.00* FD 1.04 KP 0.95 ! LA 1.04 MK 1.24 NL 1.07 ON 0.79 ! PT 1.05 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! KP 0.82 MK 0.85 OV 0.91 ZC 0.98 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.05 KP 1.01 ! LA 1.20 MK 1.00 NL 0.95 OV 1.08 ! PT 1.07 ZC 1.00 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* KP 0.89 LA 0.98 ! MK 1.00 NL 0.94 ON 1.01 OV 1.01 ! PT 0.93 ZC 1.01 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.03 KP 0.88 ! LA 1.19 MC 1.06 NL 0.99 ON 1.00* ! OV 1.00 PT 1.04 SC 0.87 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.03 KP 0.91 ! LA 0.97 MK 1.03 NL 1.01 ON 0.98 ! OV 1.00 PT 1.00 ZC 0.99 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.05 KP 0.83 ! LA 0.98 MK 0.98 NL 1.05 ON 0.99 ! PT 0.90 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! KP 1.06 MK 0.77 OV 1.01 ZC 0.80 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 0.98 KP 0.92 ! LA 1.08 MK 0.98 NL 1.10 OV 1.08 ! PT 0.94 ZC 1.03 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* KP 0.87 LA 0.98 ! MK 1.10 NL 0.99 ON 1.01 OV 1.03 ! PT 0.86 ZC 0.91 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.90 KP 0.92 ! LA 0.96 MC 1.09 NL 1.07 ON 1.00* ! OV 1.05 PT 0.85 SC 1.01 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 0.97 KP 0.94 ! LA 1.01 MK 1.11 NL 1.01 ON 0.97 ! OV 0.99 PT 1.00 ZC 1.04 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 0.88 KP 0.92 ! LA 0.99 MK 1.02 NL 1.04 ON 0.75 ! PT 0.96 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! KP 0.95 MK 0.90 OV 0.81 ZC 0.75 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.12 EF 1.00* FD 1.07 KP 0.93 ! LA 1.00 MK 0.93 NL 0.93 OV 0.98 ! PT 1.04 ZC 0.92 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 EF 1.00* KP 1.07 LA 0.99 ! MK 0.97 NL 1.14 ON 0.88 OV 1.02 ! PT 0.91 ZC 0.79 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 EF 1.00* FD 0.98 KP 1.06 ! LA 1.09 MC 1.05 NL 0.93 ON 1.00* ! OV 0.99 PT 0.92 SC 1.09 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.92 EF 1.00* FD 1.03 KP 0.98 ! LA 1.06 MK 1.03 NL 0.98 ON 1.03 ! OV 1.09 PT 0.94 ZC 0.88 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.89 EF 1.00* FD 0.99 KP 1.06 ! LA 1.02 MK 0.97 NL 1.03 ON 0.85 ! PT 0.95 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! KP 0.83 MK 0.96 OV 0.93 ZC 0.61 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.91 EF 1.00* FD 0.91 KP 0.93 ! LA 1.10 MK 0.96 NL 0.88 OV 1.04 ! PT 1.06 ZC 0.84 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 EF 1.00* KP 0.85 LA 1.13 ! MK 1.03 NL 0.88 ON 0.91 OV 0.98 ! PT 1.01 ZC 0.74 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 EF 1.00* FD 1.06 KP 1.00 ! LA 1.09 MC 1.06 NL 0.88 ON 1.00* ! OV 0.97 PT 1.05 SC 1.00 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.93 EF 1.00* FD 1.14 KP 1.04 ! LA 1.05 MK 0.99 NL 1.08 ON 0.93 ! OV 0.93 PT 0.95 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.89 EF 1.00* FD 1.18 KP 0.99 ! LA 0.91 MK 1.11 NL 0.86 ON 0.95 ! PT 0.88 ! ! ! Fit before self-cal, rms=0.067380Jy sigma=0.642187 ! Fit after self-cal, rms=0.065943Jy sigma=0.639624 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.7374 mas, bmaj=0.8768 mas, bpa=52.86 degrees ! Estimated noise=0.313267 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 = 0.000350787 Jy ! Component: 100 - total flux cleaned = 0.000378277 Jy ! Component: 150 - total flux cleaned = 0.000378297 Jy ! Component: 200 - total flux cleaned = 0.000378091 Jy ! Total flux subtracted in 200 components = 0.000378091 Jy ! Clean residual min=-0.000870 max=0.000865 Jy/beam ! Clean residual mean=-0.000003 rms=0.000195 Jy/beam ! Combined flux in latest and established models = 0.0425545 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 11 components and 0.0425545 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=0.065939Jy sigma=0.639613 ! Fit after self-cal, rms=0.065948Jy sigma=0.639125 ! Inverting map ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 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=0.065948Jy sigma=0.639125 ! Fit after self-cal, rms=0.066563Jy sigma=0.638675 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.7312 mas, bmaj=0.8742 mas, bpa=52.74 degrees ! Estimated noise=0.314826 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000348467 Jy ! Component: 100 - total flux cleaned = 0.000404488 Jy ! Component: 150 - total flux cleaned = 0.000409054 Jy ! Component: 200 - total flux cleaned = 0.000408907 Jy ! Total flux subtracted in 200 components = 0.000408907 Jy ! Clean residual min=-0.000817 max=0.000822 Jy/beam ! Clean residual mean=-0.000003 rms=0.000192 Jy/beam ! Combined flux in latest and established models = 0.0429635 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 12 components and 0.0429635 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=0.066560Jy sigma=0.638668 ! Fit after self-cal, rms=0.066587Jy sigma=0.638561 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 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 (11.2, 31.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000539513 Jy ! Component: 100 - total flux cleaned = 0.000537819 Jy ! Component: 150 - total flux cleaned = 0.000524888 Jy ! Component: 200 - total flux cleaned = 0.00052501 Jy ! Total flux subtracted in 200 components = 0.00052501 Jy ! Clean residual min=-0.000848 max=0.000823 Jy/beam ! Clean residual mean=-0.000002 rms=0.000190 Jy/beam ! Combined flux in latest and established models = 0.0434885 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 25 components and 0.0434885 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=0.066578Jy sigma=0.638485 ! Fit after self-cal, rms=0.066579Jy sigma=0.638460 ! Inverting map ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 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=0.066579Jy sigma=0.638460 ! Fit after self-cal, rms=0.067177Jy sigma=0.638424 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.7272 mas, bmaj=0.8725 mas, bpa=53.02 degrees ! Estimated noise=0.31759 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000528518 Jy ! Component: 100 - total flux cleaned = 0.000599182 Jy ! Component: 150 - total flux cleaned = 0.000634606 Jy ! Component: 200 - total flux cleaned = 0.000655288 Jy ! Total flux subtracted in 200 components = 0.000655288 Jy ! Clean residual min=-0.000858 max=0.000803 Jy/beam ! Clean residual mean=-0.000002 rms=0.000191 Jy/beam ! Combined flux in latest and established models = 0.0441438 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 26 components and 0.0441438 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=0.067169Jy sigma=0.638383 ! Fit after self-cal, rms=0.067175Jy sigma=0.638342 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 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 = 0.000148066 Jy ! Component: 100 - total flux cleaned = 0.000170422 Jy ! Component: 150 - total flux cleaned = 0.000200996 Jy ! Component: 200 - total flux cleaned = 0.000210589 Jy ! Total flux subtracted in 200 components = 0.000210589 Jy ! Clean residual min=-0.000860 max=0.000793 Jy/beam ! Clean residual mean=-0.000002 rms=0.000191 Jy/beam ! Combined flux in latest and established models = 0.0443543 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 29 components and 0.0443543 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=0.067171Jy sigma=0.638319 ! Fit after self-cal, rms=0.067172Jy sigma=0.638314 ! Inverting map ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 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=0.067172Jy sigma=0.638314 ! Fit after self-cal, rms=0.067459Jy sigma=0.638291 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=2.727 mas, bmaj=2.968 mas, bpa=-27.35 degrees ! Estimated noise=0.412125 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000371666 Jy ! Component: 100 - total flux cleaned = 0.000479101 Jy ! Component: 150 - total flux cleaned = 0.000513186 Jy ! Component: 200 - total flux cleaned = 0.000518336 Jy ! Total flux subtracted in 200 components = 0.000518336 Jy ! Clean residual min=-0.000986 max=0.000916 Jy/beam ! Clean residual mean=-0.000005 rms=0.000236 Jy/beam ! Combined flux in latest and established models = 0.0448727 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 38 components and 0.0448727 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=0.067456Jy sigma=0.638292 ! Fit after self-cal, rms=0.067455Jy sigma=0.638271 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 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 = 7.77879e-05 Jy ! Component: 100 - total flux cleaned = 7.77209e-05 Jy ! Component: 150 - total flux cleaned = 7.78412e-05 Jy ! Component: 200 - total flux cleaned = 8.14182e-05 Jy ! Total flux subtracted in 200 components = 8.14182e-05 Jy ! Clean residual min=-0.000997 max=0.000924 Jy/beam ! Clean residual mean=-0.000005 rms=0.000237 Jy/beam ! Combined flux in latest and established models = 0.0449541 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 40 components and 0.0449541 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=0.067455Jy sigma=0.638275 ! Fit after self-cal, rms=0.067455Jy sigma=0.638263 ! Inverting map ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "************** FINISHED AMPLITUDE SELF-CAL **************" ! ************** FINISHED AMPLITUDE SELF-CAL ************** restore ! Inverting map and beam ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.7243 mas, bmaj=0.8706 mas, bpa=53.14 degrees ! Estimated noise=0.319368 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7243 x 0.8706 at 53.14 degrees (North through East) ! Clean map min=-0.00077042 max=0.046518 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 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.4711 mas, bmaj=0.6321 mas, bpa=55.16 degrees ! Estimated noise=0.714511 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0371831 Jy ! Component: 100 - total flux cleaned = 0.0449966 Jy ! Component: 150 - total flux cleaned = 0.0452907 Jy ! Component: 200 - total flux cleaned = 0.0453741 Jy ! Total flux subtracted in 200 components = 0.0453741 Jy ! Clean residual min=-0.002037 max=0.002041 Jy/beam ! Clean residual mean=-0.000001 rms=0.000456 Jy/beam ! Combined flux in latest and established models = 0.0453741 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 8 model components to the UV plane model. ! The established model now contains 8 components and 0.0453741 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.7243 mas, bmaj=0.8706 mas, bpa=53.14 degrees ! Estimated noise=0.319368 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 = -9.07307e-05 Jy ! Component: 100 - total flux cleaned = -0.000111892 Jy ! Component: 150 - total flux cleaned = -0.000152548 Jy ! Component: 200 - total flux cleaned = -0.000171016 Jy ! Total flux subtracted in 200 components = -0.000171016 Jy ! Clean residual min=-0.000831 max=0.000816 Jy/beam ! Clean residual mean=-0.000002 rms=0.000193 Jy/beam ! Combined flux in latest and established models = 0.045203 Jy ! Adding 14 model components to the UV plane model. ! The established model now contains 16 components and 0.0452031 Jy ! Inverting map ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=2.727 mas, bmaj=2.968 mas, bpa=-27.35 degrees ! Estimated noise=0.412125 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -7.87401e-05 Jy ! Component: 100 - total flux cleaned = -0.000102556 Jy ! Component: 150 - total flux cleaned = -0.000108188 Jy ! Component: 200 - total flux cleaned = -0.000119029 Jy ! Total flux subtracted in 200 components = -0.000119029 Jy ! Clean residual min=-0.001001 max=0.000932 Jy/beam ! Clean residual mean=-0.000005 rms=0.000237 Jy/beam ! Combined flux in latest and established models = 0.045084 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 = -1.44063e-05 Jy ! Component: 100 - total flux cleaned = -2.28639e-05 Jy ! Component: 150 - total flux cleaned = -3.08373e-05 Jy ! Component: 200 - total flux cleaned = -4.14132e-05 Jy ! Total flux subtracted in 200 components = -4.14132e-05 Jy ! Clean residual min=-0.001003 max=0.000933 Jy/beam ! Clean residual mean=-0.000005 rms=0.000237 Jy/beam ! Combined flux in latest and established models = 0.0450426 Jy ! Adding 8 model components to the UV plane model. ! The established model now contains 24 components and 0.0450426 Jy ! Inverting map ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.7243 mas, bmaj=0.8706 mas, bpa=53.14 degrees ! Estimated noise=0.319368 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -2.10083e-05 Jy ! Component: 100 - total flux cleaned = -2.21205e-05 Jy ! Component: 150 - total flux cleaned = -7.70317e-06 Jy ! Component: 200 - total flux cleaned = -7.3786e-06 Jy ! Total flux subtracted in 200 components = -7.3786e-06 Jy ! Clean residual min=-0.000830 max=0.000806 Jy/beam ! Clean residual mean=-0.000002 rms=0.000192 Jy/beam ! Combined flux in latest and established models = 0.0450352 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 33 components and 0.0450352 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=0.067461Jy sigma=0.638304 ! Fit after self-cal, rms=0.067463Jy sigma=0.638278 wmodel /scr/pima/gb073_uvs/J1408+6505_X_map.mod ! Writing 33 model components to file: /scr/pima/gb073_uvs/J1408+6505_X_map.mod wobs /scr/pima/gb073_uvs/J1408+6505_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1408+6505_X_uvs.fits wwins /scr/pima/gb073_uvs/J1408+6505_X_map.win ! wwins: Wrote 2 windows to /scr/pima/gb073_uvs/J1408+6505_X_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000174916 Jy ! Component: 100 - total flux cleaned = -0.000174993 Jy ! Component: 150 - total flux cleaned = -0.00017472 Jy ! Component: 200 - total flux cleaned = -0.00023117 Jy ! Component: 250 - total flux cleaned = -0.000258834 Jy ! Component: 300 - total flux cleaned = -0.000245447 Jy ! Component: 350 - total flux cleaned = -0.000272319 Jy ! Component: 400 - total flux cleaned = -0.00023258 Jy ! Component: 450 - total flux cleaned = -0.000180437 Jy ! Component: 500 - total flux cleaned = -0.000142089 Jy ! Component: 550 - total flux cleaned = -0.000154856 Jy ! Component: 600 - total flux cleaned = -0.00011709 Jy ! Component: 650 - total flux cleaned = -0.000154881 Jy ! Component: 700 - total flux cleaned = -0.000154764 Jy ! Component: 750 - total flux cleaned = -0.000142528 Jy ! Component: 800 - total flux cleaned = -0.000142528 Jy ! Component: 850 - total flux cleaned = -0.00013053 Jy ! Component: 900 - total flux cleaned = -0.000130484 Jy ! Component: 950 - total flux cleaned = -0.000130368 Jy ! Component: 1000 - total flux cleaned = -0.000118603 Jy ! Component: 1050 - total flux cleaned = -9.51313e-05 Jy ! Component: 1100 - total flux cleaned = -0.000165109 Jy ! Component: 1150 - total flux cleaned = -0.000118752 Jy ! Component: 1200 - total flux cleaned = -7.27943e-05 Jy ! Component: 1250 - total flux cleaned = -0.000129835 Jy ! Component: 1300 - total flux cleaned = -9.5769e-05 Jy ! Component: 1350 - total flux cleaned = -0.000107064 Jy ! Component: 1400 - total flux cleaned = -0.000118218 Jy ! Component: 1450 - total flux cleaned = -9.5941e-05 Jy ! Component: 1500 - total flux cleaned = -5.16292e-05 Jy ! Component: 1550 - total flux cleaned = -5.16909e-05 Jy ! Component: 1600 - total flux cleaned = -6.26041e-05 Jy ! Component: 1650 - total flux cleaned = -6.27137e-05 Jy ! Component: 1700 - total flux cleaned = -5.18078e-05 Jy ! Component: 1750 - total flux cleaned = -4.09345e-05 Jy ! Component: 1800 - total flux cleaned = -1.94321e-05 Jy ! Component: 1850 - total flux cleaned = -4.08267e-05 Jy ! Component: 1900 - total flux cleaned = -3.03174e-05 Jy ! Component: 1950 - total flux cleaned = 1.49208e-06 Jy ! Component: 2000 - total flux cleaned = -3.0185e-05 Jy ! Component: 2050 - total flux cleaned = 4.32566e-05 Jy ! Component: 2100 - total flux cleaned = 6.41665e-05 Jy ! Component: 2150 - total flux cleaned = 3.29397e-05 Jy ! Component: 2200 - total flux cleaned = 6.41229e-05 Jy ! Component: 2250 - total flux cleaned = 8.4825e-05 Jy ! Component: 2300 - total flux cleaned = 0.000136143 Jy ! Component: 2350 - total flux cleaned = 7.47464e-05 Jy ! Component: 2400 - total flux cleaned = 0.000146091 Jy ! Component: 2450 - total flux cleaned = 0.000156206 Jy ! Component: 2500 - total flux cleaned = 0.000146009 Jy ! Component: 2550 - total flux cleaned = 0.000156073 Jy ! Component: 2600 - total flux cleaned = 0.000156026 Jy ! Component: 2650 - total flux cleaned = 0.00013612 Jy ! Component: 2700 - total flux cleaned = 0.000165951 Jy ! Component: 2750 - total flux cleaned = 0.000205634 Jy ! Component: 2800 - total flux cleaned = 0.000225403 Jy ! Component: 2850 - total flux cleaned = 0.000235297 Jy ! Component: 2900 - total flux cleaned = 0.000254843 Jy ! Component: 2950 - total flux cleaned = 0.00027434 Jy ! Component: 3000 - total flux cleaned = 0.0003132 Jy ! Component: 3050 - total flux cleaned = 0.000332542 Jy ! Component: 3100 - total flux cleaned = 0.000351879 Jy ! Component: 3150 - total flux cleaned = 0.000380704 Jy ! Component: 3200 - total flux cleaned = 0.000361535 Jy ! Component: 3250 - total flux cleaned = 0.000361577 Jy ! Component: 3300 - total flux cleaned = 0.000390155 Jy ! Component: 3350 - total flux cleaned = 0.000418584 Jy ! Component: 3400 - total flux cleaned = 0.000446908 Jy ! Component: 3450 - total flux cleaned = 0.000456309 Jy ! Component: 3500 - total flux cleaned = 0.000428153 Jy ! Component: 3550 - total flux cleaned = 0.00040951 Jy ! Component: 3600 - total flux cleaned = 0.00040022 Jy ! Component: 3650 - total flux cleaned = 0.00039099 Jy ! Component: 3700 - total flux cleaned = 0.000390978 Jy ! Component: 3750 - total flux cleaned = 0.000400206 Jy ! Component: 3800 - total flux cleaned = 0.000418611 Jy ! Component: 3850 - total flux cleaned = 0.000381865 Jy ! Component: 3900 - total flux cleaned = 0.000326918 Jy ! Component: 3950 - total flux cleaned = 0.000336069 Jy ! Component: 4000 - total flux cleaned = 0.000299697 Jy ! Component: 4050 - total flux cleaned = 0.000299711 Jy ! Total flux subtracted in 4096 components = 0.000281639 Jy ! Clean residual min=-0.000628 max=0.000544 Jy/beam ! Clean residual mean=-0.000001 rms=0.000146 Jy/beam ! Combined flux in latest and established models = 0.0453169 Jy keep ! Adding 365 model components to the UV plane model. ! The established model now contains 398 components and 0.0453168 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1408+6505_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7243 x 0.8706 at 53.14 degrees (North through East) ! Clean map min=-0.00064432 max=0.046217 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1408+6505_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0462174 invert ! Inverting map ! Your choice of large map pixels excluded 4.47% of the data. ! The x-axis pixel size should ideally be below 0.1981 milli-arcsec ! The y-axis pixel size should ideally be below 0.165 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000146405 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.950323 0.950323 1.90065 3.80129 7.60258 15.2052 30.4103 60.8206 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0004 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.046 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 315.682 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1408+6505_X_uvs.log closed on Sat Dec 26 09:40:25 2015