! Started logfile: /scr/pima/gb073_uvs/J1346+7320_X_uvs.log on Sat Dec 26 09:39:52 2015 obs /scr/pima/gb073_uvs/J1346+7320_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1346+7320_X_uva.fits ! AN table 1: 29 integrations on 66 of 66 possible baselines. ! AN table 2: 25 integrations on 55 of 55 possible baselines. ! AN table 3: 50 integrations on 66 of 66 possible baselines. ! AN table 4: 27 integrations on 45 of 45 possible baselines. ! AN table 5: 23 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.858936 visibilities/baseline/integration-bin. ! Found source: J1346+7320 ! ! 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 64056 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/J1346+7320_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 48 telescope corrections were flagged in sub-array 1. ! A total of 31 telescope corrections were flagged in sub-array 2. ! A total of 86 telescope corrections were flagged in sub-array 3. ! A total of 39 telescope corrections were flagged in sub-array 4. ! A total of 37 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 48 telescope corrections were flagged in sub-array 1. ! A total of 31 telescope corrections were flagged in sub-array 2. ! A total of 86 telescope corrections were flagged in sub-array 3. ! A total of 39 telescope corrections were flagged in sub-array 4. ! A total of 37 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 48 telescope corrections were flagged in sub-array 1. ! A total of 31 telescope corrections were flagged in sub-array 2. ! A total of 86 telescope corrections were flagged in sub-array 3. ! A total of 39 telescope corrections were flagged in sub-array 4. ! A total of 37 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 48 telescope corrections were flagged in sub-array 1. ! A total of 31 telescope corrections were flagged in sub-array 2. ! A total of 86 telescope corrections were flagged in sub-array 3. ! A total of 39 telescope corrections were flagged in sub-array 4. ! A total of 37 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 5. ! A total of 74 telescope corrections were flagged in sub-array 1. ! A total of 53 telescope corrections were flagged in sub-array 2. ! A total of 129 telescope corrections were flagged in sub-array 3. ! A total of 62 telescope corrections were flagged in sub-array 4. ! A total of 57 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 6. ! A total of 74 telescope corrections were flagged in sub-array 1. ! A total of 53 telescope corrections were flagged in sub-array 2. ! A total of 129 telescope corrections were flagged in sub-array 3. ! A total of 62 telescope corrections were flagged in sub-array 4. ! A total of 57 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 7. ! A total of 48 telescope corrections were flagged in sub-array 1. ! A total of 31 telescope corrections were flagged in sub-array 2. ! A total of 86 telescope corrections were flagged in sub-array 3. ! A total of 39 telescope corrections were flagged in sub-array 4. ! A total of 37 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 8. ! A total of 48 telescope corrections were flagged in sub-array 1. ! A total of 31 telescope corrections were flagged in sub-array 2. ! A total of 86 telescope corrections were flagged in sub-array 3. ! A total of 39 telescope corrections were flagged in sub-array 4. ! A total of 37 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=1.007553Jy sigma=9.067504 ! Fit after self-cal, rms=0.923092Jy sigma=8.286504 ! 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 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec ! Estimated beam: bmin=0.452 mas, bmaj=0.5763 mas, bpa=-42.14 degrees ! Estimated noise=0.780166 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 = 0.0597196 Jy ! Component: 100 - total flux cleaned = 0.0735249 Jy ! Total flux subtracted in 100 components = 0.0735249 Jy ! Clean residual min=-0.003435 max=0.005562 Jy/beam ! Clean residual mean=-0.000000 rms=0.000618 Jy/beam ! Combined flux in latest and established models = 0.0735249 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.0735249 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=0.090461Jy sigma=0.692243 ! Fit after self-cal, rms=0.089926Jy sigma=0.688190 ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00689925 Jy ! Component: 100 - total flux cleaned = 0.0109999 Jy ! Total flux subtracted in 100 components = 0.0109999 Jy ! Clean residual min=-0.003128 max=0.004424 Jy/beam ! Clean residual mean=0.000000 rms=0.000588 Jy/beam ! Combined flux in latest and established models = 0.0845248 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.0845248 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=0.089057Jy sigma=0.677867 ! Fit after self-cal, rms=0.089034Jy sigma=0.677672 ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec ! Added new window around map position (-1.2, -0.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00429983 Jy ! Component: 100 - total flux cleaned = 0.0060567 Jy ! Total flux subtracted in 100 components = 0.0060567 Jy ! Clean residual min=-0.002973 max=0.003057 Jy/beam ! Clean residual mean=0.000000 rms=0.000576 Jy/beam ! Combined flux in latest and established models = 0.0905815 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 13 components and 0.0905815 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=0.088751Jy sigma=0.674569 ! Fit after self-cal, rms=0.088709Jy sigma=0.674243 ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 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 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec ! Estimated beam: bmin=0.6079 mas, bmaj=0.7652 mas, bpa=-45.38 degrees ! Estimated noise=0.355064 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 = 0.00341798 Jy ! Component: 100 - total flux cleaned = 0.00501288 Jy ! Component: 150 - total flux cleaned = 0.00534669 Jy ! Component: 200 - total flux cleaned = 0.00544753 Jy ! Total flux subtracted in 200 components = 0.00544753 Jy ! Clean residual min=-0.001466 max=0.001527 Jy/beam ! Clean residual mean=-0.000002 rms=0.000282 Jy/beam ! Combined flux in latest and established models = 0.096029 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 19 components and 0.096029 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=0.088585Jy sigma=0.673089 ! Fit after self-cal, rms=0.088567Jy sigma=0.672941 ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6079 x 0.7652 at -45.38 degrees (North through East) ! Clean map min=-0.0010963 max=0.07874 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 0.97 EF 1.00* FD 0.95 KP 0.96 ! LA 1.02 MC 1.04 MK 1.01 NL 0.97 ! OV 1.02 PT 0.95 SC 0.97 ZC 0.85 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 EF 1.00* FD 1.05 KP 0.97 ! LA 1.04 MC 1.02 MK 0.91 NL 0.98 ! OV 1.07 PT 0.99 ZC 0.89 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 EF 1.00* FD 1.01 KP 1.03 ! LA 1.05 MC 0.96 NL 1.02 ON 0.89 ! OV 1.03 PT 0.94 SC 0.98 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 EF 1.00* FD 0.86 KP 1.01 ! LA 1.08 MC 0.92 NL 0.91 ON 1.02 ! PT 0.98 ZC 0.82 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 EF 1.00* FD 1.03 KP 1.01 ! LA 1.03 MC 1.05 MK 1.01 NL 0.89 ! ON 1.03 PT 0.95 SC 0.91 ZC 0.83 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 EF 1.00* FD 1.02 KP 1.11 ! LA 1.07 MC 1.02 MK 1.02 NL 0.98 ! OV 1.07 PT 1.01 SC 0.96 ZC 0.87 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 EF 1.00* FD 1.05 KP 1.02 ! LA 1.11 MC 1.03 MK 1.09 NL 1.02 ! OV 1.05 PT 0.97 ZC 0.78 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.06 EF 1.00* FD 1.04 KP 1.04 ! LA 1.02 MC 1.05 NL 1.02 ON 0.92 ! OV 1.03 PT 1.01 SC 0.98 ZC 0.93 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.04 EF 1.00* FD 1.05 KP 1.00 ! LA 1.11 MC 0.99 NL 0.99 ON 0.91 ! PT 1.06 ZC 0.82 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.05 EF 1.00* FD 0.99 KP 1.07 ! LA 1.02 MC 1.20 MK 1.10 NL 0.98 ! ON 1.01 PT 0.96 SC 1.04 ZC 0.84 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 EF 1.00* FD 1.02 KP 0.92 ! LA 0.99 MC 0.98 MK 0.98 NL 1.02 ! OV 1.06 PT 0.97 SC 0.99 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 EF 1.00* FD 0.94 KP 0.97 ! LA 1.01 MC 0.94 MK 1.00 NL 0.98 ! OV 0.97 PT 1.01 ZC 0.77 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 EF 1.00* FD 1.03 KP 0.97 ! LA 1.02 MC 1.02 NL 0.97 ON 0.90 ! OV 0.98 PT 1.02 SC 1.01 ZC 0.84 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 EF 1.00* FD 1.02 KP 1.06 ! LA 0.99 MC 0.98 NL 0.96 ON 0.94 ! PT 1.04 ZC 0.84 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 EF 1.00* FD 0.97 KP 0.94 ! LA 1.02 MC 1.02 MK 1.09 NL 1.01 ! ON 1.12 PT 0.99 SC 0.99 ZC 0.80 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 EF 1.00* FD 1.05 KP 1.01 ! LA 1.02 MC 1.00 MK 1.12 NL 0.97 ! OV 1.03 PT 1.05 SC 0.94 ZC 0.82 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 EF 1.00* FD 1.05 KP 0.92 ! LA 1.02 MC 0.99 MK 1.02 NL 1.03 ! OV 0.96 PT 1.05 ZC 0.84 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 EF 1.00* FD 1.03 KP 0.99 ! LA 1.03 MC 0.99 NL 0.97 ON 1.01 ! OV 1.00 PT 1.07 SC 1.00 ZC 0.87 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 EF 1.00* FD 1.00 KP 0.91 ! LA 1.05 MC 0.82 NL 1.02 ON 1.19 ! PT 1.05 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 EF 1.00* FD 1.05 KP 0.97 ! LA 1.00 MC 1.11 MK 1.03 NL 1.04 ! ON 0.96 PT 0.98 SC 1.09 ZC 0.86 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00 KP 0.91 ! LA 0.97 MC 1.26 MK 0.94 NL 1.02 ! OV 1.03 PT 0.99 SC 0.97 ZC 0.85 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 0.96 KP 0.87 ! LA 0.96 MC 1.42 MK 0.98 NL 1.03 ! OV 1.02 PT 0.96 ZC 0.79 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.06 KP 0.91 ! LA 0.97 MC 1.19 NL 0.98 ON 1.09 ! OV 1.04 PT 1.04 SC 1.04 ZC 0.87 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.97 KP 0.86 ! LA 1.01 MC 1.20 NL 0.99 ON 1.14 ! PT 1.00 ZC 0.93 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 0.94 KP 0.90 ! LA 0.99 MC 1.18 MK 0.98 NL 1.02 ! ON 1.43 PT 1.01 SC 1.03 ZC 0.87 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.02 KP 0.85 ! LA 1.02 MC 1.27 MK 1.07 NL 1.00 ! OV 1.02 PT 0.99 SC 1.07 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 0.89 KP 0.92 ! LA 0.97 MC 1.12 MK 0.95 NL 1.01 ! OV 1.10 PT 0.91 ZC 0.79 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.04 KP 0.88 ! LA 0.98 MC 1.27 NL 1.00 ON 1.22 ! OV 0.99 PT 1.00 SC 0.99 ZC 0.90 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.90 KP 0.84 ! LA 1.05 MC 1.21 NL 0.93 ON 1.07 ! PT 0.98 ZC 0.85 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 0.94 KP 0.91 ! LA 1.00 MC 1.25 MK 1.02 NL 0.97 ! ON 1.26 PT 0.99 SC 0.92 ZC 0.83 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.12 EF 1.00* FD 1.06 KP 0.94 ! LA 1.07 MC 1.51 MK 1.06 NL 0.97 ! OV 1.01 PT 1.01 SC 0.93 ZC 0.80 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.05 EF 1.00* FD 1.08 KP 0.86 ! LA 1.02 MC 1.33 MK 1.13 NL 1.03 ! OV 1.06 PT 1.11 ZC 0.65 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 EF 1.00* FD 1.10 KP 0.89 ! LA 1.01 MC 1.25 NL 1.04 ON 1.28 ! OV 1.05 PT 0.98 SC 1.03 ZC 0.69 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.95 EF 1.00* FD 1.10 KP 1.00 ! LA 1.06 MC 1.34 NL 1.03 ON 1.23 ! PT 0.91 ZC 0.72 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.98 EF 1.00* FD 1.06 KP 0.89 ! LA 1.09 MC 1.19 MK 1.08 NL 0.94 ! ON 1.19 PT 1.04 SC 0.96 ZC 0.70 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 0.95 EF 1.00* FD 0.94 KP 1.04 ! LA 0.97 MC 1.64 MK 1.04 NL 0.99 ! OV 1.04 PT 1.02 SC 1.01 ZC 0.72 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 EF 1.00* FD 1.03 KP 0.93 ! LA 1.11 MC 1.34 MK 0.98 NL 0.97 ! OV 0.99 PT 0.93 ZC 0.65 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 EF 1.00* FD 1.11 KP 0.96 ! LA 1.04 MC 1.34 NL 0.99 ON 1.25 ! OV 0.96 PT 0.96 SC 0.99 ZC 0.67 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.92 EF 1.00* FD 1.00 KP 0.85 ! LA 0.94 MC 1.53 NL 1.04 ON 1.15 ! PT 1.08 ZC 0.73 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.98 EF 1.00* FD 1.04 KP 0.89 ! LA 1.04 MC 1.39 MK 1.11 NL 1.04 ! ON 1.16 PT 1.01 SC 1.00 ZC 0.63 ! ! ! Fit before self-cal, rms=0.088567Jy sigma=0.672941 ! Fit after self-cal, rms=0.089476Jy sigma=0.666605 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec ! Estimated beam: bmin=0.5972 mas, bmaj=0.7615 mas, bpa=-45.9 degrees ! Estimated noise=0.353046 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 = 0.00116611 Jy ! Component: 100 - total flux cleaned = 0.00119604 Jy ! Component: 150 - total flux cleaned = 0.00117262 Jy ! Component: 200 - total flux cleaned = 0.00117317 Jy ! Total flux subtracted in 200 components = 0.00117317 Jy ! Clean residual min=-0.001044 max=0.000929 Jy/beam ! Clean residual mean=0.000001 rms=0.000224 Jy/beam ! Combined flux in latest and established models = 0.0972022 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 25 components and 0.0972022 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=0.089452Jy sigma=0.666359 ! Fit after self-cal, rms=0.089585Jy sigma=0.665947 ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 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=0.089585Jy sigma=0.665947 ! Fit after self-cal, rms=0.090138Jy sigma=0.665558 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec ! Estimated beam: bmin=0.5961 mas, bmaj=0.7582 mas, bpa=-46.5 degrees ! Estimated noise=0.354196 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000870377 Jy ! Component: 100 - total flux cleaned = 0.0010178 Jy ! Component: 150 - total flux cleaned = 0.00104645 Jy ! Component: 200 - total flux cleaned = 0.00107158 Jy ! Total flux subtracted in 200 components = 0.00107158 Jy ! Clean residual min=-0.000973 max=0.000927 Jy/beam ! Clean residual mean=0.000000 rms=0.000221 Jy/beam ! Combined flux in latest and established models = 0.0982738 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 25 components and 0.0982738 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=0.090129Jy sigma=0.665469 ! Fit after self-cal, rms=0.090148Jy sigma=0.665440 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 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 = 0.00015899 Jy ! Component: 100 - total flux cleaned = 0.000159286 Jy ! Component: 150 - total flux cleaned = 0.000148868 Jy ! Component: 200 - total flux cleaned = 0.000149351 Jy ! Total flux subtracted in 200 components = 0.000149351 Jy ! Clean residual min=-0.000961 max=0.000930 Jy/beam ! Clean residual mean=0.000000 rms=0.000221 Jy/beam ! Combined flux in latest and established models = 0.0984231 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 26 components and 0.0984231 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=0.090145Jy sigma=0.665411 ! Fit after self-cal, rms=0.090145Jy sigma=0.665409 ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 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=0.090145Jy sigma=0.665409 ! Fit after self-cal, rms=0.090342Jy sigma=0.665373 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec ! Estimated beam: bmin=0.594 mas, bmaj=0.7572 mas, bpa=-46.5 degrees ! Estimated noise=0.355194 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000578472 Jy ! Component: 100 - total flux cleaned = 0.000757371 Jy ! Component: 150 - total flux cleaned = 0.000786225 Jy ! Component: 200 - total flux cleaned = 0.000795441 Jy ! Total flux subtracted in 200 components = 0.000795441 Jy ! Clean residual min=-0.000957 max=0.000930 Jy/beam ! Clean residual mean=0.000000 rms=0.000220 Jy/beam ! Combined flux in latest and established models = 0.0992186 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 27 components and 0.0992186 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=0.090338Jy sigma=0.665336 ! Fit after self-cal, rms=0.090341Jy sigma=0.665330 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 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 = 9.54535e-05 Jy ! Component: 100 - total flux cleaned = 0.000104861 Jy ! Component: 150 - total flux cleaned = 0.00010542 Jy ! Component: 200 - total flux cleaned = 0.000105975 Jy ! Total flux subtracted in 200 components = 0.000105975 Jy ! Clean residual min=-0.000953 max=0.000932 Jy/beam ! Clean residual mean=0.000000 rms=0.000220 Jy/beam ! Combined flux in latest and established models = 0.0993245 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 27 components and 0.0993245 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=0.090340Jy sigma=0.665316 ! Fit after self-cal, rms=0.090340Jy sigma=0.665315 ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 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=0.090340Jy sigma=0.665315 ! Fit after self-cal, rms=0.090566Jy sigma=0.665297 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec ! Estimated beam: bmin=2.892 mas, bmaj=2.98 mas, bpa=61.6 degrees ! Estimated noise=0.497059 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000487413 Jy ! Component: 100 - total flux cleaned = 0.000607278 Jy ! Component: 150 - total flux cleaned = 0.000613816 Jy ! Component: 200 - total flux cleaned = 0.000619558 Jy ! Total flux subtracted in 200 components = 0.000619558 Jy ! Clean residual min=-0.001032 max=0.001105 Jy/beam ! Clean residual mean=0.000001 rms=0.000262 Jy/beam ! Combined flux in latest and established models = 0.0999441 Jy selfcal ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 29 components and 0.0999441 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=0.090566Jy sigma=0.665297 ! Fit after self-cal, rms=0.090569Jy sigma=0.665291 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 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 = 6.76034e-05 Jy ! Component: 100 - total flux cleaned = 6.8061e-05 Jy ! Component: 150 - total flux cleaned = 7.09347e-05 Jy ! Component: 200 - total flux cleaned = 7.35355e-05 Jy ! Total flux subtracted in 200 components = 7.35355e-05 Jy ! Clean residual min=-0.001024 max=0.001092 Jy/beam ! Clean residual mean=0.000001 rms=0.000262 Jy/beam ! Combined flux in latest and established models = 0.100018 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 30 components and 0.100018 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=0.090570Jy sigma=0.665294 ! Fit after self-cal, rms=0.090570Jy sigma=0.665293 ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 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 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec ! Estimated beam: bmin=0.5926 mas, bmaj=0.7565 mas, bpa=-46.47 degrees ! Estimated noise=0.356216 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5926 x 0.7565 at -46.47 degrees (North through East) ! Clean map min=-0.00081713 max=0.078486 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 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec ! Estimated beam: bmin=0.4415 mas, bmaj=0.5724 mas, bpa=-43.48 degrees ! Estimated noise=0.766084 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0583417 Jy ! Component: 100 - total flux cleaned = 0.0736132 Jy ! Component: 150 - total flux cleaned = 0.0816579 Jy ! Component: 200 - total flux cleaned = 0.0869456 Jy ! Total flux subtracted in 200 components = 0.0869456 Jy ! Clean residual min=-0.002713 max=0.002872 Jy/beam ! Clean residual mean=0.000000 rms=0.000521 Jy/beam ! Combined flux in latest and established models = 0.0869456 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 0.0869456 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec ! Estimated beam: bmin=0.5926 mas, bmaj=0.7565 mas, bpa=-46.47 degrees ! Estimated noise=0.356216 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 = 0.0062483 Jy ! Component: 100 - total flux cleaned = 0.00936661 Jy ! Component: 150 - total flux cleaned = 0.0110568 Jy ! Component: 200 - total flux cleaned = 0.0120318 Jy ! Total flux subtracted in 200 components = 0.0120318 Jy ! Clean residual min=-0.000938 max=0.001020 Jy/beam ! Clean residual mean=0.000001 rms=0.000223 Jy/beam ! Combined flux in latest and established models = 0.0989774 Jy ! Adding 20 model components to the UV plane model. ! The established model now contains 21 components and 0.0989774 Jy ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec ! Added new window around map position (21, -15.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000770273 Jy ! Component: 100 - total flux cleaned = 0.000968925 Jy ! Component: 150 - total flux cleaned = 0.00107508 Jy ! Component: 200 - total flux cleaned = 0.00115122 Jy ! Total flux subtracted in 200 components = 0.00115122 Jy ! Clean residual min=-0.000937 max=0.000959 Jy/beam ! Clean residual mean=0.000001 rms=0.000219 Jy/beam ! Combined flux in latest and established models = 0.100129 Jy ! Adding 21 model components to the UV plane model. ! The established model now contains 30 components and 0.100129 Jy ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec ! Added new window around map position (4.4, -6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000564327 Jy ! Component: 100 - total flux cleaned = 0.00058079 Jy ! Component: 150 - total flux cleaned = 0.000616549 Jy ! Component: 200 - total flux cleaned = 0.00063333 Jy ! Total flux subtracted in 200 components = 0.00063333 Jy ! Clean residual min=-0.000929 max=0.000926 Jy/beam ! Clean residual mean=0.000001 rms=0.000217 Jy/beam ! Combined flux in latest and established models = 0.100762 Jy ! Adding 23 model components to the UV plane model. ! The established model now contains 42 components and 0.100762 Jy ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 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 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec ! Estimated beam: bmin=2.892 mas, bmaj=2.98 mas, bpa=61.6 degrees ! Estimated noise=0.497059 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000372261 Jy ! Component: 100 - total flux cleaned = 0.000396943 Jy ! Component: 150 - total flux cleaned = 0.000396967 Jy ! Component: 200 - total flux cleaned = 0.000396926 Jy ! Total flux subtracted in 200 components = 0.000396926 Jy ! Clean residual min=-0.000973 max=0.001023 Jy/beam ! Clean residual mean=0.000002 rms=0.000254 Jy/beam ! Combined flux in latest and established models = 0.101159 Jy flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -5.77203e-06 Jy ! Component: 100 - total flux cleaned = -1.127e-05 Jy ! Component: 150 - total flux cleaned = -1.68745e-05 Jy ! Component: 200 - total flux cleaned = -2.70524e-05 Jy ! Total flux subtracted in 200 components = -2.70524e-05 Jy ! Clean residual min=-0.000968 max=0.001021 Jy/beam ! Clean residual mean=0.000002 rms=0.000254 Jy/beam ! Combined flux in latest and established models = 0.101132 Jy ! Adding 12 model components to the UV plane model. ! The established model now contains 48 components and 0.101132 Jy ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec ! Estimated beam: bmin=0.5926 mas, bmaj=0.7565 mas, bpa=-46.47 degrees ! Estimated noise=0.356216 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 6.42683e-05 Jy ! Component: 100 - total flux cleaned = 6.96257e-06 Jy ! Component: 150 - total flux cleaned = -5.87739e-06 Jy ! Component: 200 - total flux cleaned = -5.44571e-06 Jy ! Total flux subtracted in 200 components = -5.44571e-06 Jy ! Clean residual min=-0.000938 max=0.000954 Jy/beam ! Clean residual mean=0.000001 rms=0.000216 Jy/beam ! Combined flux in latest and established models = 0.101126 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 55 components and 0.101126 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=0.090547Jy sigma=0.665123 ! Fit after self-cal, rms=0.090539Jy sigma=0.665081 wmodel /scr/pima/gb073_uvs/J1346+7320_X_map.mod ! Writing 55 model components to file: /scr/pima/gb073_uvs/J1346+7320_X_map.mod wobs /scr/pima/gb073_uvs/J1346+7320_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1346+7320_X_uvs.fits wwins /scr/pima/gb073_uvs/J1346+7320_X_map.win ! wwins: Wrote 4 windows to /scr/pima/gb073_uvs/J1346+7320_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 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000141351 Jy ! Component: 100 - total flux cleaned = -0.000309345 Jy ! Component: 150 - total flux cleaned = -0.00047269 Jy ! Component: 200 - total flux cleaned = -0.000664801 Jy ! Component: 250 - total flux cleaned = -0.000837872 Jy ! Component: 300 - total flux cleaned = -0.00100858 Jy ! Component: 350 - total flux cleaned = -0.00114651 Jy ! Component: 400 - total flux cleaned = -0.00131303 Jy ! Component: 450 - total flux cleaned = -0.00146261 Jy ! Component: 500 - total flux cleaned = -0.00156657 Jy ! Component: 550 - total flux cleaned = -0.001699 Jy ! Component: 600 - total flux cleaned = -0.00183034 Jy ! Component: 650 - total flux cleaned = -0.00196051 Jy ! Component: 700 - total flux cleaned = -0.00204667 Jy ! Component: 750 - total flux cleaned = -0.00210396 Jy ! Component: 800 - total flux cleaned = -0.00221757 Jy ! Component: 850 - total flux cleaned = -0.00231636 Jy ! Component: 900 - total flux cleaned = -0.00240051 Jy ! Component: 950 - total flux cleaned = -0.00249811 Jy ! Component: 1000 - total flux cleaned = -0.00259494 Jy ! Component: 1050 - total flux cleaned = -0.00263626 Jy ! Component: 1100 - total flux cleaned = -0.00278698 Jy ! Component: 1150 - total flux cleaned = -0.00284149 Jy ! Component: 1200 - total flux cleaned = -0.00296348 Jy ! Component: 1250 - total flux cleaned = -0.0030039 Jy ! Component: 1300 - total flux cleaned = -0.00305759 Jy ! Component: 1350 - total flux cleaned = -0.00312448 Jy ! Component: 1400 - total flux cleaned = -0.00323087 Jy ! Component: 1450 - total flux cleaned = -0.00325738 Jy ! Component: 1500 - total flux cleaned = -0.00328381 Jy ! Component: 1550 - total flux cleaned = -0.00337574 Jy ! Component: 1600 - total flux cleaned = -0.00345426 Jy ! Component: 1650 - total flux cleaned = -0.00355845 Jy ! Component: 1700 - total flux cleaned = -0.0034676 Jy ! Component: 1750 - total flux cleaned = -0.00355795 Jy ! Component: 1800 - total flux cleaned = -0.00362233 Jy ! Component: 1850 - total flux cleaned = -0.00368646 Jy ! Component: 1900 - total flux cleaned = -0.00369923 Jy ! Component: 1950 - total flux cleaned = -0.00372469 Jy ! Component: 2000 - total flux cleaned = -0.00378809 Jy ! Component: 2050 - total flux cleaned = -0.00380078 Jy ! Component: 2100 - total flux cleaned = -0.0038511 Jy ! Component: 2150 - total flux cleaned = -0.00388873 Jy ! Component: 2200 - total flux cleaned = -0.00395129 Jy ! Component: 2250 - total flux cleaned = -0.00400123 Jy ! Component: 2300 - total flux cleaned = -0.00398879 Jy ! Component: 2350 - total flux cleaned = -0.00397642 Jy ! Component: 2400 - total flux cleaned = -0.00401347 Jy ! Component: 2450 - total flux cleaned = -0.00411209 Jy ! Component: 2500 - total flux cleaned = -0.00411206 Jy ! Component: 2550 - total flux cleaned = -0.00417333 Jy ! Component: 2600 - total flux cleaned = -0.00417336 Jy ! Component: 2650 - total flux cleaned = -0.00419778 Jy ! Component: 2700 - total flux cleaned = -0.00422206 Jy ! Component: 2750 - total flux cleaned = -0.00428264 Jy ! Component: 2800 - total flux cleaned = -0.00425857 Jy ! Component: 2850 - total flux cleaned = -0.00435486 Jy ! Component: 2900 - total flux cleaned = -0.00433085 Jy ! Component: 2950 - total flux cleaned = -0.00442675 Jy ! Component: 3000 - total flux cleaned = -0.00437901 Jy ! Component: 3050 - total flux cleaned = -0.00442667 Jy ! Component: 3100 - total flux cleaned = -0.00442667 Jy ! Component: 3150 - total flux cleaned = -0.00449789 Jy ! Component: 3200 - total flux cleaned = -0.00449788 Jy ! Component: 3250 - total flux cleaned = -0.00448609 Jy ! Component: 3300 - total flux cleaned = -0.00447432 Jy ! Component: 3350 - total flux cleaned = -0.00453307 Jy ! Component: 3400 - total flux cleaned = -0.00455649 Jy ! Component: 3450 - total flux cleaned = -0.00461493 Jy ! Component: 3500 - total flux cleaned = -0.0046149 Jy ! Component: 3550 - total flux cleaned = -0.00459166 Jy ! Component: 3600 - total flux cleaned = -0.00455684 Jy ! Component: 3650 - total flux cleaned = -0.00461478 Jy ! Component: 3700 - total flux cleaned = -0.00466104 Jy ! Component: 3750 - total flux cleaned = -0.00468407 Jy ! Component: 3800 - total flux cleaned = -0.00469559 Jy ! Component: 3850 - total flux cleaned = -0.00474144 Jy ! Component: 3900 - total flux cleaned = -0.0047415 Jy ! Component: 3950 - total flux cleaned = -0.0047643 Jy ! Component: 4000 - total flux cleaned = -0.0047871 Jy ! Component: 4050 - total flux cleaned = -0.00482124 Jy ! Total flux subtracted in 4096 components = -0.00480993 Jy ! Clean residual min=-0.000728 max=0.000650 Jy/beam ! Clean residual mean=0.000000 rms=0.000184 Jy/beam ! Combined flux in latest and established models = 0.0963164 Jy keep ! Adding 386 model components to the UV plane model. ! The established model now contains 441 components and 0.0963164 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1346+7320_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5926 x 0.7565 at -46.47 degrees (North through East) ! Clean map min=-0.00074843 max=0.078555 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1346+7320_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0785552 invert ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1655 milli-arcsec ! The y-axis pixel size should ideally be below 0.1945 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000183937 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.70245 0.70245 1.4049 2.8098 5.6196 11.2392 22.4784 44.9568 89.9136 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0005 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.078 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 427.076 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1346+7320_X_uvs.log closed on Sat Dec 26 09:39:59 2015