! Started logfile: /scr/pima/gb073_uvs/J0910+3329_X_uvs.log on Sat Dec 26 09:35:18 2015 obs /scr/pima/gb073_uvs/J0910+3329_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J0910+3329_X_uva.fits ! AN table 1: 10 integrations on 55 of 55 possible baselines. ! AN table 2: 66 integrations on 10 of 10 possible baselines. ! AN table 3: 30 integrations on 6 of 6 possible baselines. ! AN table 4: 16 integrations on 78 of 78 possible baselines. ! AN table 5: 17 integrations on 66 of 66 possible baselines. ! AN table 6: 12 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.770211 visibilities/baseline/integration-bin. ! Found source: J0910+3329 ! ! 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 28048 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/J0910+3329_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 10 telescope corrections were flagged in sub-array 1. ! A total of 150 telescope corrections were flagged in sub-array 2. ! A total of 48 telescope corrections were flagged in sub-array 3. ! A total of 27 telescope corrections were flagged in sub-array 4. ! A total of 32 telescope corrections were flagged in sub-array 5. ! A total of 17 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 10 telescope corrections were flagged in sub-array 1. ! A total of 150 telescope corrections were flagged in sub-array 2. ! A total of 48 telescope corrections were flagged in sub-array 3. ! A total of 27 telescope corrections were flagged in sub-array 4. ! A total of 32 telescope corrections were flagged in sub-array 5. ! A total of 17 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 10 telescope corrections were flagged in sub-array 1. ! A total of 150 telescope corrections were flagged in sub-array 2. ! A total of 48 telescope corrections were flagged in sub-array 3. ! A total of 27 telescope corrections were flagged in sub-array 4. ! A total of 32 telescope corrections were flagged in sub-array 5. ! A total of 17 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 10 telescope corrections were flagged in sub-array 1. ! A total of 150 telescope corrections were flagged in sub-array 2. ! A total of 48 telescope corrections were flagged in sub-array 3. ! A total of 27 telescope corrections were flagged in sub-array 4. ! A total of 32 telescope corrections were flagged in sub-array 5. ! A total of 17 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 5. ! A total of 20 telescope corrections were flagged in sub-array 1. ! A total of 150 telescope corrections were flagged in sub-array 2. ! A total of 48 telescope corrections were flagged in sub-array 3. ! A total of 43 telescope corrections were flagged in sub-array 4. ! A total of 49 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 6. ! A total of 20 telescope corrections were flagged in sub-array 1. ! A total of 150 telescope corrections were flagged in sub-array 2. ! A total of 48 telescope corrections were flagged in sub-array 3. ! A total of 43 telescope corrections were flagged in sub-array 4. ! A total of 49 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 7. ! A total of 10 telescope corrections were flagged in sub-array 1. ! A total of 150 telescope corrections were flagged in sub-array 2. ! A total of 48 telescope corrections were flagged in sub-array 3. ! A total of 27 telescope corrections were flagged in sub-array 4. ! A total of 32 telescope corrections were flagged in sub-array 5. ! A total of 17 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 8. ! A total of 10 telescope corrections were flagged in sub-array 1. ! A total of 150 telescope corrections were flagged in sub-array 2. ! A total of 48 telescope corrections were flagged in sub-array 3. ! A total of 27 telescope corrections were flagged in sub-array 4. ! A total of 32 telescope corrections were flagged in sub-array 5. ! A total of 17 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.007665Jy sigma=8.161164 ! Fit after self-cal, rms=0.915579Jy sigma=7.456207 ! 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 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec ! Estimated beam: bmin=0.4878 mas, bmaj=0.8239 mas, bpa=1.38 degrees ! Estimated noise=1.1838 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 = 0.0679004 Jy ! Component: 100 - total flux cleaned = 0.0831761 Jy ! Total flux subtracted in 100 components = 0.0831761 Jy ! Clean residual min=-0.004034 max=0.006454 Jy/beam ! Clean residual mean=-0.000011 rms=0.000960 Jy/beam ! Combined flux in latest and established models = 0.0831761 Jy ! Performing phase self-cal ! Adding 3 model components to the UV plane model. ! The established model now contains 3 components and 0.0831761 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=0.102778Jy sigma=0.666087 ! Fit after self-cal, rms=0.102398Jy sigma=0.662776 ! Inverting map ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec ! Added new window around map position (0.4, -1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00706398 Jy ! Component: 100 - total flux cleaned = 0.0111401 Jy ! Total flux subtracted in 100 components = 0.0111401 Jy ! Clean residual min=-0.004002 max=0.004657 Jy/beam ! Clean residual mean=-0.000008 rms=0.000928 Jy/beam ! Combined flux in latest and established models = 0.0943162 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.0943162 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=0.101837Jy sigma=0.657573 ! Fit after self-cal, rms=0.101814Jy sigma=0.657230 ! Inverting map ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 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 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec ! Estimated beam: bmin=0.6144 mas, bmaj=1.012 mas, bpa=3.492 degrees ! Estimated noise=0.619214 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 (1.6, -5). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00579327 Jy ! Component: 100 - total flux cleaned = 0.00946561 Jy ! Component: 150 - total flux cleaned = 0.0120874 Jy ! Component: 200 - total flux cleaned = 0.014028 Jy ! Total flux subtracted in 200 components = 0.014028 Jy ! Clean residual min=-0.002393 max=0.003105 Jy/beam ! Clean residual mean=-0.000016 rms=0.000561 Jy/beam ! Combined flux in latest and established models = 0.108344 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 26 components and 0.108344 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=0.101490Jy sigma=0.653394 ! Fit after self-cal, rms=0.101407Jy sigma=0.652818 ! Inverting map ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6144 x 1.012 at 3.492 degrees (North through East) ! Clean map min=-0.0019996 max=0.087094 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 1.12 EF 1.00* FD 0.99 KP 0.95 ! LA 1.09 MC 1.00 MK 1.15 NL 0.92 ! OV 1.02 PT 0.91 SC 0.88 ! ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 0.98 MC 0.81 ON 0.95 ! ZC 0.87 ! ! Telescope amplitude corrections in sub-array 3: ! HH 0.99 MC 0.82 ON 1.05 ZC 0.92 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 EF 1.00* FD 1.12 HH 0.86 ! KP 0.98 LA 1.04 MC 0.89 NL 0.94 ! ON 1.02 OV 1.04 PT 0.91 SC 1.00 ! ZC 0.79 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.92 EF 1.00* FD 1.00 HH 1.07 ! KP 1.01 LA 1.01 MC 1.20 NL 0.95 ! ON 0.96 PT 0.96 SC 1.02 ZC 0.73 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.02 EF 1.00* FD 1.01 KP 0.89 ! LA 1.05 MC 1.08 MK 1.09 NL 0.96 ! ON 1.08 PT 0.90 SC 1.11 ZC 0.83 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.19 EF 1.00* FD 1.11 KP 1.13 ! LA 1.11 MC 1.03 MK 1.07 NL 1.03 ! OV 1.04 PT 0.92 SC 0.92 ! ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.08 MC 0.96 ON 0.92 ! ZC 0.75 ! ! Telescope amplitude corrections in sub-array 3: ! HH 0.94 MC 1.01 ON 0.79 ZC 0.83 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.10 EF 1.00* FD 1.04 HH 1.20 ! KP 1.01 LA 1.02 MC 1.08 NL 0.92 ! ON 1.00 OV 1.12 PT 1.01 SC 0.99 ! ZC 0.70 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.22 EF 1.00* FD 1.00 HH 1.00 ! KP 0.99 LA 1.05 MC 0.98 NL 1.08 ! ON 1.04 PT 0.96 SC 0.93 ZC 0.79 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.10 EF 1.00* FD 1.03 KP 0.97 ! LA 0.98 MC 0.99 MK 1.14 NL 0.99 ! ON 0.97 PT 0.92 SC 0.95 ZC 0.86 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.19 EF 1.00* FD 1.03 KP 0.94 ! LA 1.03 MC 0.88 MK 1.09 NL 0.93 ! OV 1.01 PT 0.94 SC 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 0.97 MC 1.02 ON 1.00 ! ZC 0.73 ! ! Telescope amplitude corrections in sub-array 3: ! HH 0.84 MC 0.89 ON 0.60 ZC 1.05 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 EF 1.00* FD 1.06 HH 0.98 ! KP 0.95 LA 1.03 MC 0.84 NL 1.00 ! ON 0.89 OV 1.08 PT 1.00 SC 0.92 ! ZC 0.79 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.11 EF 1.00* FD 1.04 HH 0.90 ! KP 0.88 LA 0.94 MC 0.99 NL 0.96 ! ON 1.04 PT 0.98 SC 1.10 ZC 0.71 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.13 EF 1.00* FD 1.02 KP 0.96 ! LA 0.92 MC 0.95 MK 1.28 NL 0.87 ! ON 1.36 PT 0.97 SC 1.05 ZC 0.82 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.10 EF 1.00* FD 1.12 KP 1.03 ! LA 0.89 MC 1.17 MK 0.99 NL 0.97 ! OV 1.12 PT 0.96 SC 0.95 ! ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 0.97 MC 0.96 ON 0.84 ! ZC 0.81 ! ! Telescope amplitude corrections in sub-array 3: ! HH 0.93 MC 0.92 ON 0.94 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.07 EF 1.00* FD 1.06 HH 1.10 ! KP 1.03 LA 1.02 MC 0.95 NL 1.03 ! ON 0.97 OV 0.99 PT 0.97 SC 1.02 ! ZC 0.83 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 EF 1.00* FD 1.02 HH 0.99 ! KP 0.97 LA 0.98 MC 0.99 NL 1.05 ! ON 1.01 PT 1.05 SC 1.09 ZC 0.67 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.14 EF 1.00* FD 1.02 KP 1.09 ! LA 0.97 MC 1.15 MK 1.06 NL 0.95 ! ON 0.95 PT 0.95 SC 1.07 ZC 0.76 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.02 KP 0.87 ! LA 1.01 MC 1.80 MK 1.12 NL 0.93 ! OV 1.08 PT 1.09 SC 0.95 ! ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.00 MC 1.12 ON 1.00 ! ZC 0.87 ! ! Telescope amplitude corrections in sub-array 3: ! HH 0.94 MC 1.33 ON 0.88 ZC 0.86 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.04 HH 0.99 ! KP 0.96 LA 0.95 MC 1.37 NL 0.96 ! ON 1.29 OV 1.09 PT 0.95 SC 1.04 ! ZC 0.75 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 0.94 HH 1.05 ! KP 0.98 LA 0.96 MC 1.34 NL 1.06 ! ON 1.37 PT 0.89 SC 1.10 ZC 0.86 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.14 KP 0.83 ! LA 0.95 MC 1.30 MK 1.09 NL 0.99 ! ON 1.18 PT 0.95 SC 0.96 ZC 0.76 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.01 KP 0.90 ! LA 1.07 MC 1.56 MK 0.91 NL 0.96 ! OV 0.98 PT 1.01 SC 1.13 ! ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 0.92 MC 1.12 ON 0.93 ! ZC 0.91 ! ! Telescope amplitude corrections in sub-array 3: ! HH 0.98 MC 1.12 ON 1.05 ZC 0.85 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.13 HH 0.95 ! KP 0.89 LA 0.92 MC 1.10 NL 0.95 ! ON 1.05 OV 1.16 PT 0.92 SC 0.93 ! ZC 0.82 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.01 HH 1.01 ! KP 0.83 LA 1.16 MC 1.63 NL 1.00 ! ON 1.14 PT 1.02 SC 0.96 ZC 0.69 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.11 KP 0.83 ! LA 0.95 MC 1.34 MK 1.00 NL 1.00 ! ON 1.05 PT 0.84 SC 0.86 ZC 0.83 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.19 EF 1.00* FD 1.07 KP 0.93 ! LA 1.15 MC 1.09 MK 1.23 NL 1.09 ! OV 0.99 PT 1.09 SC 0.79 ! ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 0.89 MC 0.97 ON 0.98 ! ZC 0.80 ! ! Telescope amplitude corrections in sub-array 3: ! HH 0.83 MC 1.22 ON 0.94 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.06 EF 1.00* FD 0.94 HH 1.12 ! KP 1.05 LA 0.98 MC 1.24 NL 1.03 ! ON 1.16 OV 1.08 PT 0.98 SC 0.97 ! ZC 0.63 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 EF 1.00* FD 1.00 HH 1.12 ! KP 0.85 LA 1.09 MC 1.17 NL 0.97 ! ON 1.24 PT 0.96 SC 1.04 ZC 0.64 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.07 EF 1.00* FD 1.07 KP 0.90 ! LA 0.99 MC 1.25 MK 1.02 NL 1.00 ! ON 1.23 PT 0.95 SC 1.20 ZC 0.65 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 0.92 EF 1.00* FD 1.04 KP 0.86 ! LA 1.10 MC 1.23 MK 1.10 NL 1.14 ! OV 1.14 PT 1.11 SC 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 0.85 MC 0.95 ON 0.96 ! ZC 0.81 ! ! Telescope amplitude corrections in sub-array 3: ! HH 0.85 MC 1.03 ON 0.90 ZC 0.88 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 EF 1.00* FD 1.04 HH 1.17 ! KP 0.99 LA 1.09 MC 1.15 NL 0.92 ! ON 1.20 OV 1.06 PT 0.97 SC 1.22 ! ZC 0.56 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.87 EF 1.00* FD 1.16 HH 1.24 ! KP 0.91 LA 1.01 MC 1.39 NL 1.05 ! ON 1.32 PT 1.02 SC 1.04 ZC 0.47 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.10 EF 1.00* FD 1.03 KP 0.97 ! LA 1.01 MC 1.30 MK 0.91 NL 1.17 ! ON 1.00 PT 1.01 SC 1.10 ZC 0.70 ! ! ! Fit before self-cal, rms=0.101407Jy sigma=0.652818 ! Fit after self-cal, rms=0.104927Jy sigma=0.641543 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec ! Estimated beam: bmin=0.6207 mas, bmaj=0.9889 mas, bpa=3.032 degrees ! Estimated noise=0.618332 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 = 0.00157107 Jy ! Component: 100 - total flux cleaned = 0.00199488 Jy ! Component: 150 - total flux cleaned = 0.00223006 Jy ! Component: 200 - total flux cleaned = 0.00248999 Jy ! Total flux subtracted in 200 components = 0.00248999 Jy ! Clean residual min=-0.001688 max=0.001779 Jy/beam ! Clean residual mean=-0.000002 rms=0.000392 Jy/beam ! Combined flux in latest and established models = 0.110834 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 41 components and 0.110834 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=0.104898Jy sigma=0.641252 ! Fit after self-cal, rms=0.105241Jy sigma=0.640515 ! Inverting map ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 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=0.105241Jy sigma=0.640515 ! Fit after self-cal, rms=0.106990Jy sigma=0.639409 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec ! Estimated beam: bmin=0.6212 mas, bmaj=0.9888 mas, bpa=3.032 degrees ! Estimated noise=0.620924 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00100875 Jy ! Component: 100 - total flux cleaned = 0.00125773 Jy ! Component: 150 - total flux cleaned = 0.00149697 Jy ! Component: 200 - total flux cleaned = 0.00167893 Jy ! Total flux subtracted in 200 components = 0.00167893 Jy ! Clean residual min=-0.001664 max=0.001670 Jy/beam ! Clean residual mean=-0.000002 rms=0.000380 Jy/beam ! Combined flux in latest and established models = 0.112513 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 46 components and 0.112513 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=0.106975Jy sigma=0.639268 ! Fit after self-cal, rms=0.107091Jy sigma=0.639064 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 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 (17.4, 37). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000823583 Jy ! Component: 100 - total flux cleaned = 0.000826872 Jy ! Component: 150 - total flux cleaned = 0.000956741 Jy ! Component: 200 - total flux cleaned = 0.00110169 Jy ! Total flux subtracted in 200 components = 0.00110169 Jy ! Clean residual min=-0.001613 max=0.001626 Jy/beam ! Clean residual mean=-0.000002 rms=0.000376 Jy/beam ! Combined flux in latest and established models = 0.113615 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 57 components and 0.113615 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=0.107055Jy sigma=0.638905 ! Fit after self-cal, rms=0.107080Jy sigma=0.638866 ! Inverting map ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 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=0.107080Jy sigma=0.638866 ! Fit after self-cal, rms=0.107905Jy sigma=0.638659 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec ! Estimated beam: bmin=0.6218 mas, bmaj=0.9877 mas, bpa=3.126 degrees ! Estimated noise=0.621831 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000612822 Jy ! Component: 100 - total flux cleaned = 0.000825142 Jy ! Component: 150 - total flux cleaned = 0.000934569 Jy ! Component: 200 - total flux cleaned = 0.00103452 Jy ! Total flux subtracted in 200 components = 0.00103452 Jy ! Clean residual min=-0.001660 max=0.001562 Jy/beam ! Clean residual mean=-0.000004 rms=0.000372 Jy/beam ! Combined flux in latest and established models = 0.114649 Jy selfcal ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 60 components and 0.114649 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=0.107889Jy sigma=0.638598 ! Fit after self-cal, rms=0.107955Jy sigma=0.638542 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 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 = 0.000272126 Jy ! Component: 100 - total flux cleaned = 0.000365443 Jy ! Component: 150 - total flux cleaned = 0.000408599 Jy ! Component: 200 - total flux cleaned = 0.000428698 Jy ! Total flux subtracted in 200 components = 0.000428698 Jy ! Clean residual min=-0.001628 max=0.001565 Jy/beam ! Clean residual mean=-0.000002 rms=0.000370 Jy/beam ! Combined flux in latest and established models = 0.115078 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 64 components and 0.115078 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=0.107946Jy sigma=0.638508 ! Fit after self-cal, rms=0.107943Jy sigma=0.638505 ! Inverting map ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 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=0.107943Jy sigma=0.638505 ! Fit after self-cal, rms=0.108691Jy sigma=0.638461 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec ! Estimated beam: bmin=2.611 mas, bmaj=2.863 mas, bpa=7.901 degrees ! Estimated noise=0.810001 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000910689 Jy ! Component: 100 - total flux cleaned = 0.00118367 Jy ! Component: 150 - total flux cleaned = 0.00122088 Jy ! Component: 200 - total flux cleaned = 0.00126465 Jy ! Total flux subtracted in 200 components = 0.00126465 Jy ! Clean residual min=-0.001652 max=0.001582 Jy/beam ! Clean residual mean=-0.000001 rms=0.000419 Jy/beam ! Combined flux in latest and established models = 0.116343 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 71 components and 0.116343 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=0.108695Jy sigma=0.638485 ! Fit after self-cal, rms=0.108751Jy sigma=0.638411 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 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 = 0.000291246 Jy ! Component: 100 - total flux cleaned = 0.000321112 Jy ! Component: 150 - total flux cleaned = 0.000359964 Jy ! Component: 200 - total flux cleaned = 0.000384149 Jy ! Total flux subtracted in 200 components = 0.000384149 Jy ! Clean residual min=-0.001608 max=0.001469 Jy/beam ! Clean residual mean=0.000002 rms=0.000415 Jy/beam ! Combined flux in latest and established models = 0.116727 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 79 components and 0.116727 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=0.108754Jy sigma=0.638435 ! Fit after self-cal, rms=0.108755Jy sigma=0.638431 ! Inverting map ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 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 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec ! Estimated beam: bmin=0.6221 mas, bmaj=0.987 mas, bpa=3.196 degrees ! Estimated noise=0.623341 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6221 x 0.987 at 3.196 degrees (North through East) ! Clean map min=-0.0013836 max=0.086624 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 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec ! Estimated beam: bmin=0.49 mas, bmaj=0.7994 mas, bpa=0.316 degrees ! Estimated noise=1.18488 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0681023 Jy ! Component: 100 - total flux cleaned = 0.0833123 Jy ! Component: 150 - total flux cleaned = 0.0901828 Jy ! Component: 200 - total flux cleaned = 0.094964 Jy ! Total flux subtracted in 200 components = 0.094964 Jy ! Clean residual min=-0.003423 max=0.003787 Jy/beam ! Clean residual mean=-0.000008 rms=0.000817 Jy/beam ! Combined flux in latest and established models = 0.094964 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 9 model components to the UV plane model. ! The established model now contains 9 components and 0.094964 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec ! Estimated beam: bmin=0.6221 mas, bmaj=0.987 mas, bpa=3.196 degrees ! Estimated noise=0.623341 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 = 0.00600163 Jy ! Component: 100 - total flux cleaned = 0.0101795 Jy ! Component: 150 - total flux cleaned = 0.0132073 Jy ! Component: 200 - total flux cleaned = 0.0154476 Jy ! Total flux subtracted in 200 components = 0.0154476 Jy ! Clean residual min=-0.001790 max=0.002205 Jy/beam ! Clean residual mean=-0.000016 rms=0.000417 Jy/beam ! Combined flux in latest and established models = 0.110412 Jy ! Adding 32 model components to the UV plane model. ! The established model now contains 39 components and 0.110412 Jy ! Inverting map ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec ! Added new window around map position (-2.8, 10.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00166067 Jy ! Component: 100 - total flux cleaned = 0.00246872 Jy ! Component: 150 - total flux cleaned = 0.00322087 Jy ! Component: 200 - total flux cleaned = 0.00373759 Jy ! Total flux subtracted in 200 components = 0.00373759 Jy ! Clean residual min=-0.001690 max=0.001724 Jy/beam ! Clean residual mean=-0.000008 rms=0.000382 Jy/beam ! Combined flux in latest and established models = 0.114149 Jy ! Adding 36 model components to the UV plane model. ! The established model now contains 60 components and 0.114149 Jy ! Inverting map ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec ! Added new window around map position (11.2, -38.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000837673 Jy ! Component: 100 - total flux cleaned = 0.0011292 Jy ! Component: 150 - total flux cleaned = 0.0014359 Jy ! Component: 200 - total flux cleaned = 0.00164967 Jy ! Total flux subtracted in 200 components = 0.00164967 Jy ! Clean residual min=-0.001672 max=0.001579 Jy/beam ! Clean residual mean=-0.000004 rms=0.000370 Jy/beam ! Combined flux in latest and established models = 0.115799 Jy ! Adding 34 model components to the UV plane model. ! The established model now contains 73 components and 0.115799 Jy ! Inverting map ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 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 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec ! Estimated beam: bmin=2.611 mas, bmaj=2.863 mas, bpa=7.901 degrees ! Estimated noise=0.810001 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00139087 Jy ! Component: 100 - total flux cleaned = 0.00163481 Jy ! Component: 150 - total flux cleaned = 0.00165887 Jy ! Component: 200 - total flux cleaned = 0.00164154 Jy ! Total flux subtracted in 200 components = 0.00164154 Jy ! Clean residual min=-0.001634 max=0.001591 Jy/beam ! Clean residual mean=0.000004 rms=0.000411 Jy/beam ! Combined flux in latest and established models = 0.11744 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 = -9.47341e-07 Jy ! Component: 100 - total flux cleaned = -1.43845e-06 Jy ! Component: 150 - total flux cleaned = -1.8074e-06 Jy ! Component: 200 - total flux cleaned = 1.02096e-05 Jy ! Total flux subtracted in 200 components = 1.02096e-05 Jy ! Clean residual min=-0.001611 max=0.001551 Jy/beam ! Clean residual mean=0.000004 rms=0.000407 Jy/beam ! Combined flux in latest and established models = 0.117451 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 94 components and 0.117451 Jy ! Inverting map ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec ! Estimated beam: bmin=0.6221 mas, bmaj=0.987 mas, bpa=3.196 degrees ! Estimated noise=0.623341 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -5.78085e-05 Jy ! Component: 100 - total flux cleaned = -5.84449e-05 Jy ! Component: 150 - total flux cleaned = -5.81287e-05 Jy ! Component: 200 - total flux cleaned = -5.72738e-05 Jy ! Total flux subtracted in 200 components = -5.72738e-05 Jy ! Clean residual min=-0.001584 max=0.001521 Jy/beam ! Clean residual mean=0.000000 rms=0.000359 Jy/beam ! Combined flux in latest and established models = 0.117393 Jy selfcal ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 103 components and 0.117393 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=0.108736Jy sigma=0.638355 ! Fit after self-cal, rms=0.108706Jy sigma=0.638227 wmodel /scr/pima/gb073_uvs/J0910+3329_X_map.mod ! Writing 103 model components to file: /scr/pima/gb073_uvs/J0910+3329_X_map.mod wobs /scr/pima/gb073_uvs/J0910+3329_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J0910+3329_X_uvs.fits wwins /scr/pima/gb073_uvs/J0910+3329_X_map.win ! wwins: Wrote 6 windows to /scr/pima/gb073_uvs/J0910+3329_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 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000216661 Jy ! Component: 100 - total flux cleaned = -0.000105505 Jy ! Component: 150 - total flux cleaned = -5.18752e-05 Jy ! Component: 200 - total flux cleaned = 5.3684e-07 Jy ! Component: 250 - total flux cleaned = 2.57228e-05 Jy ! Component: 300 - total flux cleaned = 5.90011e-07 Jy ! Component: 350 - total flux cleaned = 4.95083e-05 Jy ! Component: 400 - total flux cleaned = 9.86666e-07 Jy ! Component: 450 - total flux cleaned = 4.89182e-05 Jy ! Component: 500 - total flux cleaned = 0.000119899 Jy ! Component: 550 - total flux cleaned = 0.000166413 Jy ! Component: 600 - total flux cleaned = 0.000235707 Jy ! Component: 650 - total flux cleaned = 0.000349514 Jy ! Component: 700 - total flux cleaned = 0.00034947 Jy ! Component: 750 - total flux cleaned = 0.000461134 Jy ! Component: 800 - total flux cleaned = 0.000394574 Jy ! Component: 850 - total flux cleaned = 0.000504708 Jy ! Component: 900 - total flux cleaned = 0.000461032 Jy ! Component: 950 - total flux cleaned = 0.000569814 Jy ! Component: 1000 - total flux cleaned = 0.000655874 Jy ! Component: 1050 - total flux cleaned = 0.00074116 Jy ! Component: 1100 - total flux cleaned = 0.000720226 Jy ! Component: 1150 - total flux cleaned = 0.000825308 Jy ! Component: 1200 - total flux cleaned = 0.000867098 Jy ! Component: 1250 - total flux cleaned = 0.000908471 Jy ! Component: 1300 - total flux cleaned = 0.000990934 Jy ! Component: 1350 - total flux cleaned = 0.000950126 Jy ! Component: 1400 - total flux cleaned = 0.00103165 Jy ! Component: 1450 - total flux cleaned = 0.0010721 Jy ! Component: 1500 - total flux cleaned = 0.00107215 Jy ! Component: 1550 - total flux cleaned = 0.00107202 Jy ! Component: 1600 - total flux cleaned = 0.0010323 Jy ! Component: 1650 - total flux cleaned = 0.00111175 Jy ! Component: 1700 - total flux cleaned = 0.00113142 Jy ! Component: 1750 - total flux cleaned = 0.00111169 Jy ! Component: 1800 - total flux cleaned = 0.00107261 Jy ! Component: 1850 - total flux cleaned = 0.00113075 Jy ! Component: 1900 - total flux cleaned = 0.00115007 Jy ! Component: 1950 - total flux cleaned = 0.00118857 Jy ! Component: 2000 - total flux cleaned = 0.00118852 Jy ! Component: 2050 - total flux cleaned = 0.00126465 Jy ! Component: 2100 - total flux cleaned = 0.0012268 Jy ! Component: 2150 - total flux cleaned = 0.0013403 Jy ! Component: 2200 - total flux cleaned = 0.00134038 Jy ! Component: 2250 - total flux cleaned = 0.0013591 Jy ! Component: 2300 - total flux cleaned = 0.00135924 Jy ! Component: 2350 - total flux cleaned = 0.00145198 Jy ! Component: 2400 - total flux cleaned = 0.00147049 Jy ! Component: 2450 - total flux cleaned = 0.00147042 Jy ! Component: 2500 - total flux cleaned = 0.00152548 Jy ! Component: 2550 - total flux cleaned = 0.00159829 Jy ! Component: 2600 - total flux cleaned = 0.00167094 Jy ! Component: 2650 - total flux cleaned = 0.00158055 Jy ! Component: 2700 - total flux cleaned = 0.00158066 Jy ! Component: 2750 - total flux cleaned = 0.00167042 Jy ! Component: 2800 - total flux cleaned = 0.00167056 Jy ! Component: 2850 - total flux cleaned = 0.00175949 Jy ! Component: 2900 - total flux cleaned = 0.00181259 Jy ! Component: 2950 - total flux cleaned = 0.00186546 Jy ! Component: 3000 - total flux cleaned = 0.00184779 Jy ! Component: 3050 - total flux cleaned = 0.00181272 Jy ! Component: 3100 - total flux cleaned = 0.0018652 Jy ! Component: 3150 - total flux cleaned = 0.00193489 Jy ! Component: 3200 - total flux cleaned = 0.00195225 Jy ! Component: 3250 - total flux cleaned = 0.00193509 Jy ! Component: 3300 - total flux cleaned = 0.0020212 Jy ! Component: 3350 - total flux cleaned = 0.00202114 Jy ! Component: 3400 - total flux cleaned = 0.00215798 Jy ! Component: 3450 - total flux cleaned = 0.00217501 Jy ! Component: 3500 - total flux cleaned = 0.00220894 Jy ! Component: 3550 - total flux cleaned = 0.00225979 Jy ! Component: 3600 - total flux cleaned = 0.00225977 Jy ! Component: 3650 - total flux cleaned = 0.00232705 Jy ! Component: 3700 - total flux cleaned = 0.00236052 Jy ! Component: 3750 - total flux cleaned = 0.00234381 Jy ! Component: 3800 - total flux cleaned = 0.00249362 Jy ! Component: 3850 - total flux cleaned = 0.00257656 Jy ! Component: 3900 - total flux cleaned = 0.00255998 Jy ! Component: 3950 - total flux cleaned = 0.00257651 Jy ! Component: 4000 - total flux cleaned = 0.00257652 Jy ! Component: 4050 - total flux cleaned = 0.00262566 Jy ! Total flux subtracted in 4096 components = 0.00278898 Jy ! Clean residual min=-0.000950 max=0.000931 Jy/beam ! Clean residual mean=0.000003 rms=0.000271 Jy/beam ! Combined flux in latest and established models = 0.120182 Jy keep ! Adding 359 model components to the UV plane model. ! The established model now contains 462 components and 0.120182 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J0910+3329_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6221 x 0.987 at 3.196 degrees (North through East) ! Clean map min=-0.0014213 max=0.086553 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J0910+3329_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0865528 invert ! Inverting map ! Your choice of large map pixels excluded 9.6% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1908 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000270575 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.937837 0.937837 1.87567 3.75135 7.5027 15.0054 30.0108 60.0216 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0008 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.086 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 319.884 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J0910+3329_X_uvs.log closed on Sat Dec 26 09:35:23 2015