! Started logfile: /scr/pima/gb073_uvs/J1813+3144_X_uvs.log on Sat Dec 26 09:43:46 2015 obs /scr/pima/gb073_uvs/J1813+3144_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1813+3144_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: 58 integrations on 66 of 66 possible baselines. ! AN table 4: 29 integrations on 66 of 66 possible baselines. ! AN table 5: 29 integrations on 36 of 36 possible baselines. ! Apparent sampling: 0.894691 visibilities/baseline/integration-bin. ! Found source: J1813+3144 ! ! 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 65384 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/J1813+3144_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 32 telescope corrections were flagged in sub-array 1. ! A total of 68 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 32 telescope corrections were flagged in sub-array 1. ! A total of 68 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 32 telescope corrections were flagged in sub-array 1. ! A total of 68 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 32 telescope corrections were flagged in sub-array 1. ! A total of 68 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 5. ! A total of 61 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 126 telescope corrections were flagged in sub-array 3. ! A total of 59 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 61 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 126 telescope corrections were flagged in sub-array 3. ! A total of 59 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 32 telescope corrections were flagged in sub-array 1. ! A total of 68 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 8. ! A total of 32 telescope corrections were flagged in sub-array 1. ! A total of 68 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.006031Jy sigma=10.124099 ! Fit after self-cal, rms=0.940353Jy sigma=9.454904 ! 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 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! Estimated beam: bmin=0.4708 mas, bmaj=1.169 mas, bpa=-12.82 degrees ! Estimated noise=0.691042 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 = 0.0459266 Jy ! Component: 100 - total flux cleaned = 0.056605 Jy ! Total flux subtracted in 100 components = 0.056605 Jy ! Clean residual min=-0.002388 max=0.004161 Jy/beam ! Clean residual mean=-0.000005 rms=0.000533 Jy/beam ! Combined flux in latest and established models = 0.056605 Jy ! Performing phase self-cal ! Adding 3 model components to the UV plane model. ! The established model now contains 3 components and 0.056605 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=0.080991Jy sigma=0.687661 ! Fit after self-cal, rms=0.079952Jy sigma=0.676637 ! Inverting map ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00544332 Jy ! Component: 100 - total flux cleaned = 0.00813561 Jy ! Total flux subtracted in 100 components = 0.00813561 Jy ! Clean residual min=-0.002191 max=0.002695 Jy/beam ! Clean residual mean=-0.000004 rms=0.000500 Jy/beam ! Combined flux in latest and established models = 0.0647406 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 9 components and 0.0647406 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=0.079374Jy sigma=0.669298 ! Fit after self-cal, rms=0.079370Jy sigma=0.669154 ! Inverting map ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 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 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! Estimated beam: bmin=0.6322 mas, bmaj=1.462 mas, bpa=-10.96 degrees ! Estimated noise=0.307033 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 (-0.2, 2.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00481612 Jy ! Component: 100 - total flux cleaned = 0.00776695 Jy ! Component: 150 - total flux cleaned = 0.00975834 Jy ! Component: 200 - total flux cleaned = 0.0111385 Jy ! Total flux subtracted in 200 components = 0.0111385 Jy ! Clean residual min=-0.001243 max=0.002673 Jy/beam ! Clean residual mean=-0.000011 rms=0.000324 Jy/beam ! Combined flux in latest and established models = 0.0758791 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 31 components and 0.0758791 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=0.079081Jy sigma=0.665266 ! Fit after self-cal, rms=0.079069Jy sigma=0.664762 ! Inverting map ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! Added new window around map position (0, 5.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00297864 Jy ! Component: 100 - total flux cleaned = 0.00460424 Jy ! Component: 150 - total flux cleaned = 0.00571062 Jy ! Component: 200 - total flux cleaned = 0.00652299 Jy ! Total flux subtracted in 200 components = 0.00652299 Jy ! Clean residual min=-0.001166 max=0.001551 Jy/beam ! Clean residual mean=-0.000005 rms=0.000249 Jy/beam ! Combined flux in latest and established models = 0.0824021 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 49 components and 0.0824021 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=0.078956Jy sigma=0.663409 ! Fit after self-cal, rms=0.078930Jy sigma=0.663177 ! Inverting map ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! Added new window around map position (-1.4, 6.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0015366 Jy ! Component: 100 - total flux cleaned = 0.00241595 Jy ! Component: 150 - total flux cleaned = 0.00299578 Jy ! Component: 200 - total flux cleaned = 0.00325859 Jy ! Total flux subtracted in 200 components = 0.00325859 Jy ! Clean residual min=-0.001113 max=0.001152 Jy/beam ! Clean residual mean=-0.000002 rms=0.000230 Jy/beam ! Combined flux in latest and established models = 0.0856607 Jy ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 68 components and 0.0856607 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=0.078892Jy sigma=0.662821 ! Fit after self-cal, rms=0.078883Jy sigma=0.662765 ! Inverting map ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6322 x 1.462 at -10.96 degrees (North through East) ! Clean map min=-0.0010155 max=0.061988 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: ! BR 1.05 EF 1.00* FD 1.18 KP 1.00 ! LA 1.09 MC 0.96 NL 0.92 PT 0.95 ! SC 0.74 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.92 KP 0.99 LA 1.07 MC 0.97 ! MK 1.11 NL 1.00 OV 0.97 PT 1.02 ! SC 0.87 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.07 EF 1.00* FD 0.96 KP 1.05 ! LA 1.05 MC 1.03 NL 0.96 ON 0.91 ! OV 0.98 PT 0.98 SC 0.98 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.96 EF 1.00* FD 0.98 KP 0.96 ! LA 1.10 MC 1.08 MK 0.95 NL 0.88 ! ON 0.95 OV 1.00 PT 0.98 SC 0.92 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 1.01 KP 1.03 LA 1.07 ! MK 0.93 NL 0.93 OV 0.99 PT 0.99 ! SC 0.95 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.09 EF 1.00* FD 1.07 KP 1.11 ! LA 1.04 MC 0.85 NL 0.96 PT 1.01 ! SC 0.70 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.05 KP 1.11 LA 1.14 MC 0.98 ! MK 1.06 NL 0.89 OV 1.06 PT 1.04 ! SC 0.97 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 EF 1.00* FD 1.05 KP 1.02 ! LA 1.08 MC 0.98 NL 1.01 ON 0.98 ! OV 0.99 PT 1.01 SC 0.99 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 EF 1.00* FD 1.04 KP 1.08 ! LA 1.01 MC 1.13 MK 0.96 NL 0.93 ! ON 0.90 OV 1.07 PT 1.01 SC 0.98 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.04 FD 1.01 KP 1.04 LA 1.12 ! MK 0.95 NL 0.93 OV 1.10 PT 1.02 ! SC 0.96 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.07 EF 1.00* FD 1.02 KP 0.97 ! LA 0.96 MC 0.89 NL 1.04 PT 1.00 ! SC 0.70 ZC 0.79 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 KP 0.94 LA 0.99 MC 0.98 ! MK 1.03 NL 1.08 OV 1.05 PT 1.03 ! SC 1.04 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 EF 1.00* FD 1.05 KP 0.97 ! LA 1.02 MC 1.03 NL 0.93 ON 0.88 ! OV 1.04 PT 1.02 SC 1.06 ZC 0.83 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 EF 1.00* FD 1.04 KP 1.02 ! LA 0.95 MC 0.97 MK 1.02 NL 0.94 ! ON 0.96 OV 0.98 PT 0.97 SC 0.96 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 0.98 KP 0.94 LA 0.94 ! MK 0.98 NL 1.08 OV 1.02 PT 1.04 ! SC 0.98 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 EF 1.00* FD 1.00 KP 0.94 ! LA 0.95 MC 0.99 NL 1.06 PT 1.06 ! SC 0.63 ZC 0.79 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 KP 0.98 LA 0.96 MC 0.92 ! MK 1.00 NL 1.08 OV 1.02 PT 1.00 ! SC 0.90 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 EF 1.00* FD 0.99 KP 1.00 ! LA 1.05 MC 0.96 NL 0.99 ON 0.88 ! OV 1.04 PT 1.03 SC 1.06 ZC 0.82 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 EF 1.00* FD 1.04 KP 1.01 ! LA 0.98 MC 0.99 MK 1.04 NL 0.92 ! ON 0.97 OV 0.99 PT 1.03 SC 1.06 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 1.07 KP 0.93 LA 0.98 ! MK 1.03 NL 0.97 OV 1.05 PT 1.08 ! SC 1.02 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.96 KP 0.90 ! LA 0.96 MC 1.06 NL 1.04 PT 1.09 ! SC 0.66 ZC 0.92 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* KP 0.94 LA 1.02 MC 1.06 ! MK 0.96 NL 1.02 OV 1.01 PT 0.98 ! SC 0.83 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.01 KP 0.89 ! LA 1.03 MC 1.12 NL 0.96 ON 1.08 ! OV 1.12 PT 1.02 SC 0.99 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.96 KP 0.89 ! LA 1.02 MC 1.23 MK 0.96 NL 1.06 ! ON 1.03 OV 1.08 PT 1.02 SC 1.00 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 1.01 KP 0.91 LA 1.03 ! MK 1.05 NL 1.11 OV 1.08 PT 0.95 ! SC 0.99 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.95 KP 0.89 ! LA 1.06 MC 1.01 NL 0.99 PT 0.85 ! SC 0.68 ZC 0.86 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* KP 0.90 LA 1.02 MC 1.15 ! MK 1.01 NL 1.06 OV 1.00 PT 0.97 ! SC 0.88 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 0.97 KP 0.95 ! LA 0.99 MC 1.13 NL 0.96 ON 1.14 ! OV 1.08 PT 0.99 SC 0.98 ZC 0.84 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.09 KP 0.99 ! LA 1.00 MC 1.21 MK 0.94 NL 0.97 ! ON 1.35 OV 1.07 PT 0.90 SC 1.05 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 0.94 KP 0.92 LA 1.03 ! MK 1.03 NL 0.97 OV 1.01 PT 0.95 ! SC 1.00 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 0.87 EF 1.00* FD 0.95 KP 0.92 ! LA 1.11 MC 1.08 NL 1.03 PT 0.95 ! SC 0.61 ZC 0.68 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 KP 0.87 LA 1.04 MC 1.04 ! MK 1.13 NL 1.12 OV 0.99 PT 0.91 ! SC 1.05 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 EF 1.00* FD 0.99 KP 0.99 ! LA 1.01 MC 1.11 NL 1.05 ON 1.27 ! OV 1.05 PT 1.00 SC 1.04 ZC 0.65 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.96 EF 1.00* FD 0.94 KP 0.96 ! LA 1.10 MC 1.25 MK 1.01 NL 0.98 ! ON 1.24 OV 0.95 PT 0.99 SC 0.97 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.95 FD 1.00 KP 0.91 LA 1.05 ! MK 1.04 NL 1.15 OV 0.96 PT 0.99 ! SC 1.02 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 0.89 EF 1.00* FD 0.89 KP 0.91 ! LA 1.03 MC 1.25 NL 1.00 PT 1.01 ! SC 0.61 ZC 0.66 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.93 KP 0.96 LA 1.00 MC 0.96 ! MK 0.96 NL 0.93 OV 0.89 PT 1.01 ! SC 1.06 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.92 EF 1.00* FD 1.05 KP 0.92 ! LA 1.03 MC 1.18 NL 0.97 ON 1.25 ! OV 1.02 PT 1.04 SC 1.09 ZC 0.61 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.94 EF 1.00* FD 1.01 KP 0.99 ! LA 1.05 MC 1.12 MK 0.97 NL 0.93 ! ON 1.01 OV 1.03 PT 1.05 SC 1.00 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.93 FD 0.99 KP 0.85 LA 1.13 ! MK 0.96 NL 1.04 OV 0.98 PT 1.03 ! SC 1.05 ! ! ! Fit before self-cal, rms=0.078883Jy sigma=0.662765 ! Fit after self-cal, rms=0.076670Jy sigma=0.659221 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! Estimated beam: bmin=0.6302 mas, bmaj=1.456 mas, bpa=-11.07 degrees ! Estimated noise=0.305718 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 = 0.000584159 Jy ! Component: 100 - total flux cleaned = 0.000643958 Jy ! Component: 150 - total flux cleaned = 0.000729546 Jy ! Component: 200 - total flux cleaned = 0.000760295 Jy ! Total flux subtracted in 200 components = 0.000760295 Jy ! Clean residual min=-0.000883 max=0.000873 Jy/beam ! Clean residual mean=-0.000001 rms=0.000191 Jy/beam ! Combined flux in latest and established models = 0.086421 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 88 components and 0.0864209 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=0.076660Jy sigma=0.659143 ! Fit after self-cal, rms=0.076702Jy sigma=0.658856 ! Inverting map ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 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=0.076702Jy sigma=0.658856 ! Fit after self-cal, rms=0.077020Jy sigma=0.658579 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! Estimated beam: bmin=0.6308 mas, bmaj=1.455 mas, bpa=-11.04 degrees ! Estimated noise=0.306272 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000385563 Jy ! Component: 100 - total flux cleaned = 0.000508627 Jy ! Component: 150 - total flux cleaned = 0.000601906 Jy ! Component: 200 - total flux cleaned = 0.000650322 Jy ! Total flux subtracted in 200 components = 0.000650322 Jy ! Clean residual min=-0.000863 max=0.000870 Jy/beam ! Clean residual mean=-0.000001 rms=0.000188 Jy/beam ! Combined flux in latest and established models = 0.0870713 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 97 components and 0.0870713 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=0.077014Jy sigma=0.658537 ! Fit after self-cal, rms=0.077025Jy sigma=0.658517 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 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 (8.6, 49). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000503294 Jy ! Component: 100 - total flux cleaned = 0.000501571 Jy ! Component: 150 - total flux cleaned = 0.000532837 Jy ! Component: 200 - total flux cleaned = 0.000576026 Jy ! Total flux subtracted in 200 components = 0.000576026 Jy ! Clean residual min=-0.000863 max=0.000806 Jy/beam ! Clean residual mean=-0.000002 rms=0.000187 Jy/beam ! Combined flux in latest and established models = 0.0876473 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 107 components and 0.0876473 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=0.077014Jy sigma=0.658425 ! Fit after self-cal, rms=0.077013Jy sigma=0.658413 ! Inverting map ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 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=0.077013Jy sigma=0.658413 ! Fit after self-cal, rms=0.077012Jy sigma=0.658405 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! Estimated beam: bmin=0.6303 mas, bmaj=1.452 mas, bpa=-11.06 degrees ! Estimated noise=0.306579 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000328015 Jy ! Component: 100 - total flux cleaned = 0.000416741 Jy ! Component: 150 - total flux cleaned = 0.000456752 Jy ! Component: 200 - total flux cleaned = 0.000481864 Jy ! Total flux subtracted in 200 components = 0.000481864 Jy ! Clean residual min=-0.000857 max=0.000811 Jy/beam ! Clean residual mean=-0.000002 rms=0.000187 Jy/beam ! Combined flux in latest and established models = 0.0881292 Jy selfcal ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 112 components and 0.0881292 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=0.077006Jy sigma=0.658361 ! Fit after self-cal, rms=0.077004Jy sigma=0.658357 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 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 = 0.000126026 Jy ! Component: 100 - total flux cleaned = 0.000138403 Jy ! Component: 150 - total flux cleaned = 0.00015012 Jy ! Component: 200 - total flux cleaned = 0.000138512 Jy ! Total flux subtracted in 200 components = 0.000138512 Jy ! Clean residual min=-0.000854 max=0.000820 Jy/beam ! Clean residual mean=-0.000002 rms=0.000187 Jy/beam ! Combined flux in latest and established models = 0.0882677 Jy ! Performing phase self-cal ! Adding 36 model components to the UV plane model. ! The established model now contains 116 components and 0.0882677 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=0.077000Jy sigma=0.658329 ! Fit after self-cal, rms=0.076999Jy sigma=0.658330 ! Inverting map ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 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=0.076999Jy sigma=0.658330 ! Fit after self-cal, rms=0.077043Jy sigma=0.658324 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! Estimated beam: bmin=2.585 mas, bmaj=3.007 mas, bpa=-0.3318 degrees ! Estimated noise=0.393613 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000280457 Jy ! Component: 100 - total flux cleaned = 0.000354823 Jy ! Component: 150 - total flux cleaned = 0.00039325 Jy ! Component: 200 - total flux cleaned = 0.000393688 Jy ! Total flux subtracted in 200 components = 0.000393688 Jy ! Clean residual min=-0.000878 max=0.000742 Jy/beam ! Clean residual mean=-0.000003 rms=0.000222 Jy/beam ! Combined flux in latest and established models = 0.0886614 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 124 components and 0.0886614 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=0.077043Jy sigma=0.658315 ! Fit after self-cal, rms=0.077039Jy sigma=0.658309 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 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 = 2.9987e-05 Jy ! Component: 100 - total flux cleaned = 2.30473e-05 Jy ! Component: 150 - total flux cleaned = 2.30751e-05 Jy ! Component: 200 - total flux cleaned = 2.8739e-05 Jy ! Total flux subtracted in 200 components = 2.8739e-05 Jy ! Clean residual min=-0.000885 max=0.000753 Jy/beam ! Clean residual mean=-0.000003 rms=0.000221 Jy/beam ! Combined flux in latest and established models = 0.0886901 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 128 components and 0.0886901 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=0.077039Jy sigma=0.658304 ! Fit after self-cal, rms=0.077038Jy sigma=0.658304 ! Inverting map ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 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 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! Estimated beam: bmin=0.63 mas, bmaj=1.45 mas, bpa=-11.07 degrees ! Estimated noise=0.307014 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.63 x 1.45 at -11.07 degrees (North through East) ! Clean map min=-0.0007121 max=0.061762 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 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! Estimated beam: bmin=0.4698 mas, bmaj=1.161 mas, bpa=-13.05 degrees ! Estimated noise=0.684869 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0461783 Jy ! Component: 100 - total flux cleaned = 0.0576957 Jy ! Component: 150 - total flux cleaned = 0.0631188 Jy ! Component: 200 - total flux cleaned = 0.0667071 Jy ! Total flux subtracted in 200 components = 0.0667071 Jy ! Clean residual min=-0.001891 max=0.002055 Jy/beam ! Clean residual mean=-0.000004 rms=0.000461 Jy/beam ! Combined flux in latest and established models = 0.0667071 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 15 model components to the UV plane model. ! The established model now contains 15 components and 0.0667071 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! Estimated beam: bmin=0.63 mas, bmaj=1.45 mas, bpa=-11.07 degrees ! Estimated noise=0.307014 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 = 0.0055029 Jy ! Component: 100 - total flux cleaned = 0.00923414 Jy ! Component: 150 - total flux cleaned = 0.0119365 Jy ! Component: 200 - total flux cleaned = 0.0139543 Jy ! Total flux subtracted in 200 components = 0.0139543 Jy ! Clean residual min=-0.001036 max=0.001219 Jy/beam ! Clean residual mean=-0.000009 rms=0.000241 Jy/beam ! Combined flux in latest and established models = 0.0806615 Jy ! Adding 62 model components to the UV plane model. ! The established model now contains 68 components and 0.0806615 Jy ! Inverting map ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! Added new window around map position (0.2, 8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00160928 Jy ! Component: 100 - total flux cleaned = 0.0029217 Jy ! Component: 150 - total flux cleaned = 0.00400695 Jy ! Component: 200 - total flux cleaned = 0.00492009 Jy ! Total flux subtracted in 200 components = 0.00492009 Jy ! Clean residual min=-0.000903 max=0.000819 Jy/beam ! Clean residual mean=-0.000005 rms=0.000200 Jy/beam ! Combined flux in latest and established models = 0.0855815 Jy ! Adding 52 model components to the UV plane model. ! The established model now contains 99 components and 0.0855816 Jy ! Inverting map ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 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 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! Estimated beam: bmin=2.585 mas, bmaj=3.007 mas, bpa=-0.3318 degrees ! Estimated noise=0.393613 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00126047 Jy ! Component: 100 - total flux cleaned = 0.00182228 Jy ! Component: 150 - total flux cleaned = 0.00215036 Jy ! Component: 200 - total flux cleaned = 0.00239428 Jy ! Total flux subtracted in 200 components = 0.00239428 Jy ! Clean residual min=-0.000902 max=0.000741 Jy/beam ! Clean residual mean=-0.000005 rms=0.000225 Jy/beam ! Combined flux in latest and established models = 0.0879758 Jy flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0001367 Jy ! Component: 100 - total flux cleaned = 0.000191219 Jy ! Component: 150 - total flux cleaned = 0.000229835 Jy ! Component: 200 - total flux cleaned = 0.000272913 Jy ! Total flux subtracted in 200 components = 0.000272913 Jy ! Clean residual min=-0.000902 max=0.000748 Jy/beam ! Clean residual mean=-0.000004 rms=0.000222 Jy/beam ! Combined flux in latest and established models = 0.0882488 Jy ! Adding 69 model components to the UV plane model. ! The established model now contains 158 components and 0.0882487 Jy ! Inverting map ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! Estimated beam: bmin=0.63 mas, bmaj=1.45 mas, bpa=-11.07 degrees ! Estimated noise=0.307014 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000218383 Jy ! Component: 100 - total flux cleaned = 0.000284444 Jy ! Component: 150 - total flux cleaned = 0.000302819 Jy ! Component: 200 - total flux cleaned = 0.000301445 Jy ! Total flux subtracted in 200 components = 0.000301445 Jy ! Clean residual min=-0.000840 max=0.000853 Jy/beam ! Clean residual mean=-0.000002 rms=0.000186 Jy/beam ! Combined flux in latest and established models = 0.0885502 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 167 components and 0.0885502 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=0.077036Jy sigma=0.658281 ! Fit after self-cal, rms=0.077031Jy sigma=0.658247 wmodel /scr/pima/gb073_uvs/J1813+3144_X_map.mod ! Writing 167 model components to file: /scr/pima/gb073_uvs/J1813+3144_X_map.mod wobs /scr/pima/gb073_uvs/J1813+3144_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1813+3144_X_uvs.fits wwins /scr/pima/gb073_uvs/J1813+3144_X_map.win ! wwins: Wrote 6 windows to /scr/pima/gb073_uvs/J1813+3144_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 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000122986 Jy ! Component: 100 - total flux cleaned = -0.000210778 Jy ! Component: 150 - total flux cleaned = -0.000266969 Jy ! Component: 200 - total flux cleaned = -0.000294327 Jy ! Component: 250 - total flux cleaned = -0.000307821 Jy ! Component: 300 - total flux cleaned = -0.00025584 Jy ! Component: 350 - total flux cleaned = -0.0002047 Jy ! Component: 400 - total flux cleaned = -0.000166805 Jy ! Component: 450 - total flux cleaned = -0.000104618 Jy ! Component: 500 - total flux cleaned = -5.55671e-05 Jy ! Component: 550 - total flux cleaned = -1.92193e-05 Jy ! Component: 600 - total flux cleaned = -1.91511e-05 Jy ! Component: 650 - total flux cleaned = 2.83061e-05 Jy ! Component: 700 - total flux cleaned = 1.65101e-05 Jy ! Component: 750 - total flux cleaned = 2.82265e-05 Jy ! Component: 800 - total flux cleaned = 5.13316e-05 Jy ! Component: 850 - total flux cleaned = 7.43961e-05 Jy ! Component: 900 - total flux cleaned = 9.71366e-05 Jy ! Component: 950 - total flux cleaned = 9.71891e-05 Jy ! Component: 1000 - total flux cleaned = 0.00017611 Jy ! Component: 1050 - total flux cleaned = 0.000153816 Jy ! Component: 1100 - total flux cleaned = 0.000209464 Jy ! Component: 1150 - total flux cleaned = 0.000275749 Jy ! Component: 1200 - total flux cleaned = 0.000308545 Jy ! Component: 1250 - total flux cleaned = 0.000275695 Jy ! Component: 1300 - total flux cleaned = 0.000308366 Jy ! Component: 1350 - total flux cleaned = 0.000351437 Jy ! Component: 1400 - total flux cleaned = 0.000372941 Jy ! Component: 1450 - total flux cleaned = 0.000394175 Jy ! Component: 1500 - total flux cleaned = 0.000436579 Jy ! Component: 1550 - total flux cleaned = 0.000352034 Jy ! Component: 1600 - total flux cleaned = 0.000404684 Jy ! Component: 1650 - total flux cleaned = 0.000373289 Jy ! Component: 1700 - total flux cleaned = 0.000352549 Jy ! Component: 1750 - total flux cleaned = 0.000414793 Jy ! Component: 1800 - total flux cleaned = 0.000466422 Jy ! Component: 1850 - total flux cleaned = 0.000384182 Jy ! Component: 1900 - total flux cleaned = 0.000414877 Jy ! Component: 1950 - total flux cleaned = 0.000425203 Jy ! Component: 2000 - total flux cleaned = 0.000465706 Jy ! Component: 2050 - total flux cleaned = 0.000445444 Jy ! Component: 2100 - total flux cleaned = 0.000415256 Jy ! Component: 2150 - total flux cleaned = 0.000455329 Jy ! Component: 2200 - total flux cleaned = 0.000425458 Jy ! Component: 2250 - total flux cleaned = 0.000425407 Jy ! Component: 2300 - total flux cleaned = 0.000405716 Jy ! Component: 2350 - total flux cleaned = 0.000454955 Jy ! Component: 2400 - total flux cleaned = 0.000435364 Jy ! Component: 2450 - total flux cleaned = 0.000425588 Jy ! Component: 2500 - total flux cleaned = 0.00040614 Jy ! Component: 2550 - total flux cleaned = 0.000444939 Jy ! Component: 2600 - total flux cleaned = 0.00043529 Jy ! Component: 2650 - total flux cleaned = 0.00042568 Jy ! Component: 2700 - total flux cleaned = 0.000406466 Jy ! Component: 2750 - total flux cleaned = 0.000396895 Jy ! Component: 2800 - total flux cleaned = 0.000387374 Jy ! Component: 2850 - total flux cleaned = 0.000377911 Jy ! Component: 2900 - total flux cleaned = 0.000406299 Jy ! Component: 2950 - total flux cleaned = 0.000396852 Jy ! Component: 3000 - total flux cleaned = 0.00034984 Jy ! Component: 3050 - total flux cleaned = 0.00035918 Jy ! Component: 3100 - total flux cleaned = 0.000368555 Jy ! Component: 3150 - total flux cleaned = 0.000303387 Jy ! Component: 3200 - total flux cleaned = 0.000358996 Jy ! Component: 3250 - total flux cleaned = 0.000349771 Jy ! Component: 3300 - total flux cleaned = 0.00034062 Jy ! Component: 3350 - total flux cleaned = 0.000294677 Jy ! Component: 3400 - total flux cleaned = 0.00028553 Jy ! Component: 3450 - total flux cleaned = 0.00027642 Jy ! Component: 3500 - total flux cleaned = 0.000312849 Jy ! Component: 3550 - total flux cleaned = 0.000321927 Jy ! Component: 3600 - total flux cleaned = 0.000294769 Jy ! Component: 3650 - total flux cleaned = 0.00025861 Jy ! Component: 3700 - total flux cleaned = 0.000285623 Jy ! Component: 3750 - total flux cleaned = 0.000267655 Jy ! Component: 3800 - total flux cleaned = 0.000285537 Jy ! Component: 3850 - total flux cleaned = 0.000276613 Jy ! Component: 3900 - total flux cleaned = 0.000249874 Jy ! Component: 3950 - total flux cleaned = 0.000205445 Jy ! Component: 4000 - total flux cleaned = 0.000249745 Jy ! Component: 4050 - total flux cleaned = 0.000205575 Jy ! Total flux subtracted in 4096 components = 0.000196754 Jy ! Clean residual min=-0.000461 max=0.000508 Jy/beam ! Clean residual mean=-0.000001 rms=0.000148 Jy/beam ! Combined flux in latest and established models = 0.0887469 Jy keep ! Adding 367 model components to the UV plane model. ! The established model now contains 534 components and 0.0887469 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1813+3144_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.63 x 1.45 at -11.07 degrees (North through East) ! Clean map min=-0.00070892 max=0.061689 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1813+3144_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0616889 invert ! Inverting map ! Your choice of large map pixels excluded 4.4% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000147696 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.718261 0.718261 1.43652 2.87304 5.74609 11.4922 22.9843 45.9687 91.9374 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0004 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.061 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 417.675 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1813+3144_X_uvs.log closed on Sat Dec 26 09:43:54 2015