! Started logfile: /scr/pima/gb073_uvs/J1348+2840_X_uvs.log on Sat Dec 26 09:39:59 2015 obs /scr/pima/gb073_uvs/J1348+2840_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1348+2840_X_uva.fits ! AN table 1: 19 integrations on 36 of 36 possible baselines. ! AN table 2: 29 integrations on 66 of 66 possible baselines. ! AN table 3: 29 integrations on 66 of 66 possible baselines. ! AN table 4: 29 integrations on 55 of 55 possible baselines. ! AN table 5: 29 integrations on 55 of 55 possible baselines. ! Apparent sampling: 0.907556 visibilities/baseline/integration-bin. ! Found source: J1348+2840 ! ! 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 55920 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/J1348+2840_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 38 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! A total of 48 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 38 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! A total of 48 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 38 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! A total of 48 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 38 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! A total of 48 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 5. ! A total of 57 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 59 telescope corrections were flagged in sub-array 4. ! A total of 77 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 6. ! A total of 57 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 59 telescope corrections were flagged in sub-array 4. ! A total of 77 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 7. ! A total of 38 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! A total of 48 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 8. ! A total of 38 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! A total of 48 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=1.006437Jy sigma=9.695369 ! Fit after self-cal, rms=0.935015Jy sigma=8.996086 ! 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 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec ! Estimated beam: bmin=0.4484 mas, bmaj=1.158 mas, bpa=-14.13 degrees ! Estimated noise=0.778746 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 = 0.0515575 Jy ! Component: 100 - total flux cleaned = 0.0628279 Jy ! Total flux subtracted in 100 components = 0.0628279 Jy ! Clean residual min=-0.003105 max=0.003373 Jy/beam ! Clean residual mean=0.000002 rms=0.000629 Jy/beam ! Combined flux in latest and established models = 0.0628279 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.0628279 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=0.084602Jy sigma=0.682621 ! Fit after self-cal, rms=0.083616Jy sigma=0.673400 ! Inverting map ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00424142 Jy ! Component: 100 - total flux cleaned = 0.00657296 Jy ! Total flux subtracted in 100 components = 0.00657296 Jy ! Clean residual min=-0.002827 max=0.003191 Jy/beam ! Clean residual mean=0.000002 rms=0.000608 Jy/beam ! Combined flux in latest and established models = 0.0694009 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 15 components and 0.0694009 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=0.083246Jy sigma=0.668777 ! Fit after self-cal, rms=0.083260Jy sigma=0.668742 ! Inverting map ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 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 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec ! Estimated beam: bmin=0.5801 mas, bmaj=1.37 mas, bpa=-12.52 degrees ! Estimated noise=0.363197 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 = 0.00317143 Jy ! Component: 100 - total flux cleaned = 0.00484017 Jy ! Component: 150 - total flux cleaned = 0.0057931 Jy ! Component: 200 - total flux cleaned = 0.00635061 Jy ! Total flux subtracted in 200 components = 0.00635061 Jy ! Clean residual min=-0.001616 max=0.002358 Jy/beam ! Clean residual mean=0.000002 rms=0.000346 Jy/beam ! Combined flux in latest and established models = 0.0757515 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 22 components and 0.0757515 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=0.083124Jy sigma=0.667306 ! Fit after self-cal, rms=0.083134Jy sigma=0.667256 ! Inverting map ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec ! Added new window around map position (-0.6, -5.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00223958 Jy ! Component: 100 - total flux cleaned = 0.00344054 Jy ! Component: 150 - total flux cleaned = 0.00403565 Jy ! Component: 200 - total flux cleaned = 0.00421487 Jy ! Total flux subtracted in 200 components = 0.00421487 Jy ! Clean residual min=-0.001412 max=0.001527 Jy/beam ! Clean residual mean=0.000003 rms=0.000302 Jy/beam ! Combined flux in latest and established models = 0.0799664 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 45 components and 0.0799664 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=0.083079Jy sigma=0.666544 ! Fit after self-cal, rms=0.083073Jy sigma=0.666443 ! Inverting map ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5801 x 1.37 at -12.52 degrees (North through East) ! Clean map min=-0.0011649 max=0.068093 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 0.88 EF 1.00* FD 1.09 HH 1.00* ! KP 0.94 LA 0.96 MC 0.92 NL 1.00 ! PT 0.83 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.94 EF 1.00* FD 0.97 KP 0.96 ! LA 1.16 MC 0.96 NL 0.95 ON 1.02 ! OV 1.06 PT 0.94 SC 0.96 ZC 0.78 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 EF 1.00* FD 0.98 KP 0.93 ! LA 1.05 MC 0.94 MK 1.02 NL 0.95 ! ON 0.90 OV 1.13 PT 0.98 SC 0.90 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 EF 1.00* FD 0.95 KP 1.00 ! LA 1.04 MC 1.09 NL 0.94 ON 1.01 ! PT 0.97 SC 0.88 ZC 0.83 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.11 EF 1.00* FD 1.01 KP 1.10 ! LA 1.00 MC 1.05 MK 1.04 NL 0.90 ! ON 1.06 PT 0.96 SC 0.97 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 EF 1.00* FD 0.93 HH 1.00* ! KP 1.02 LA 1.07 MC 0.97 NL 0.99 ! PT 0.94 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 EF 1.00* FD 1.04 KP 1.08 ! LA 1.06 MC 0.98 NL 0.98 ON 0.92 ! OV 1.02 PT 1.03 SC 1.03 ZC 0.80 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 EF 1.00* FD 1.04 KP 1.00 ! LA 1.13 MC 0.99 MK 1.02 NL 1.00 ! ON 0.99 OV 1.09 PT 0.95 SC 0.97 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 EF 1.00* FD 0.98 KP 1.00 ! LA 1.06 MC 1.06 NL 1.00 ON 1.01 ! PT 1.08 SC 1.00 ZC 0.80 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.08 EF 1.00* FD 1.05 KP 1.32 ! LA 1.03 MC 1.01 MK 1.14 NL 1.00 ! ON 0.97 PT 0.98 SC 0.93 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.94 EF 1.00* FD 1.04 HH 1.00* ! KP 0.99 LA 0.93 MC 0.93 NL 0.94 ! PT 1.04 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 EF 1.00* FD 0.99 KP 1.01 ! LA 0.95 MC 0.94 NL 0.96 ON 0.93 ! OV 1.02 PT 1.05 SC 0.90 ZC 0.80 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 EF 1.00* FD 0.98 KP 1.01 ! LA 0.99 MC 0.91 MK 0.91 NL 0.99 ! ON 0.92 OV 0.97 PT 0.98 SC 1.01 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 EF 1.00* FD 1.02 KP 0.94 ! LA 0.94 MC 0.86 NL 0.98 ON 0.98 ! PT 1.01 SC 1.07 ZC 0.73 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 EF 1.00* FD 0.99 KP 1.21 ! LA 1.06 MC 1.05 MK 0.96 NL 0.93 ! ON 0.89 PT 1.01 SC 1.00 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 EF 1.00* FD 0.99 HH 1.00* ! KP 1.02 LA 1.00 MC 0.99 NL 0.89 ! PT 1.07 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.08 EF 1.00* FD 1.17 KP 1.03 ! LA 0.98 MC 1.04 NL 0.96 ON 0.94 ! OV 1.01 PT 1.01 SC 1.00 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 EF 1.00* FD 0.98 KP 1.01 ! LA 1.00 MC 0.96 MK 0.92 NL 0.99 ! ON 0.94 OV 1.00 PT 1.07 SC 0.96 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 EF 1.00* FD 0.95 KP 0.93 ! LA 0.97 MC 0.94 NL 1.02 ON 1.00 ! PT 1.09 SC 1.02 ZC 0.74 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 EF 1.00* FD 1.04 KP 1.26 ! LA 0.98 MC 0.84 MK 0.97 NL 0.99 ! ON 1.01 PT 1.00 SC 1.10 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.85 HH 1.00* ! KP 0.88 LA 0.93 MC 1.04 NL 1.02 ! PT 1.07 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 0.98 KP 0.88 ! LA 0.96 MC 1.06 NL 1.04 ON 1.28 ! OV 1.05 PT 1.06 SC 1.06 ZC 0.82 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.04 KP 0.93 ! LA 1.01 MC 1.16 MK 0.97 NL 1.05 ! ON 1.09 OV 1.00 PT 1.04 SC 0.96 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.01 KP 0.92 ! LA 0.96 MC 1.16 NL 0.95 ON 1.25 ! PT 0.93 SC 1.07 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.01 KP 1.04 ! LA 0.97 MC 1.24 MK 1.02 NL 0.94 ! ON 1.16 PT 0.96 SC 1.01 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.95 HH 1.00* ! KP 0.82 LA 1.03 MC 1.20 NL 0.99 ! PT 0.89 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.13 KP 0.97 ! LA 1.03 MC 1.17 NL 0.95 ON 1.20 ! OV 1.00 PT 0.91 SC 0.92 ZC 0.83 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.07 KP 0.85 ! LA 0.94 MC 1.22 MK 0.97 NL 1.00 ! ON 1.32 OV 1.04 PT 0.98 SC 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.06 KP 0.89 ! LA 0.96 MC 1.20 NL 1.05 ON 1.28 ! PT 0.89 SC 1.13 ZC 0.72 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 0.98 KP 1.04 ! LA 0.94 MC 1.15 MK 1.09 NL 1.01 ! ON 1.07 PT 0.98 SC 0.91 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 EF 1.00* FD 0.89 HH 1.00* ! KP 0.91 LA 1.20 MC 1.18 NL 1.01 ! PT 1.02 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 EF 1.00* FD 1.11 KP 0.96 ! LA 1.03 MC 1.28 NL 1.03 ON 1.30 ! OV 0.92 PT 1.03 SC 1.18 ZC 0.65 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 EF 1.00* FD 1.03 KP 0.86 ! LA 1.03 MC 1.35 MK 1.15 NL 1.00 ! ON 1.16 OV 0.99 PT 0.99 SC 1.07 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.96 EF 1.00* FD 1.01 KP 0.95 ! LA 0.99 MC 1.19 NL 0.98 ON 1.10 ! PT 1.06 SC 1.04 ZC 0.59 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.05 EF 1.00* FD 1.07 KP 1.04 ! LA 1.07 MC 1.21 MK 1.07 NL 0.97 ! ON 1.16 PT 0.96 SC 1.12 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 0.92 EF 1.00* FD 0.87 HH 1.00* ! KP 0.85 LA 1.08 MC 1.06 NL 1.14 ! PT 0.99 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 EF 1.00* FD 1.05 KP 0.94 ! LA 0.99 MC 1.26 NL 1.06 ON 1.34 ! OV 1.06 PT 0.97 SC 0.98 ZC 0.58 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 EF 1.00* FD 1.08 KP 0.96 ! LA 1.02 MC 1.31 MK 0.98 NL 0.97 ! ON 1.08 OV 1.10 PT 0.95 SC 0.96 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 EF 1.00* FD 1.03 KP 0.96 ! LA 1.07 MC 1.37 NL 0.95 ON 1.16 ! PT 0.95 SC 1.01 ZC 0.56 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 EF 1.00* FD 0.92 KP 1.26 ! LA 1.09 MC 1.32 MK 1.14 NL 1.05 ! ON 1.17 PT 0.98 SC 0.92 ! ! ! Fit before self-cal, rms=0.083073Jy sigma=0.666443 ! Fit after self-cal, rms=0.084447Jy sigma=0.660348 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec ! Estimated beam: bmin=0.5785 mas, bmaj=1.375 mas, bpa=-12.56 degrees ! Estimated noise=0.362871 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 (-10, 9.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0010665 Jy ! Component: 100 - total flux cleaned = 0.00139094 Jy ! Component: 150 - total flux cleaned = 0.00152421 Jy ! Component: 200 - total flux cleaned = 0.00160734 Jy ! Total flux subtracted in 200 components = 0.00160734 Jy ! Clean residual min=-0.000994 max=0.001027 Jy/beam ! Clean residual mean=0.000002 rms=0.000240 Jy/beam ! Combined flux in latest and established models = 0.0815737 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 65 components and 0.0815737 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=0.084428Jy sigma=0.660176 ! Fit after self-cal, rms=0.084530Jy sigma=0.659758 ! Inverting map ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 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=0.084530Jy sigma=0.659758 ! Fit after self-cal, rms=0.085034Jy sigma=0.659714 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec ! Estimated beam: bmin=0.5784 mas, bmaj=1.376 mas, bpa=-12.56 degrees ! Estimated noise=0.363266 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000485207 Jy ! Component: 100 - total flux cleaned = 0.000565384 Jy ! Component: 150 - total flux cleaned = 0.000622823 Jy ! Component: 200 - total flux cleaned = 0.00064937 Jy ! Total flux subtracted in 200 components = 0.00064937 Jy ! Clean residual min=-0.001026 max=0.001062 Jy/beam ! Clean residual mean=0.000002 rms=0.000239 Jy/beam ! Combined flux in latest and established models = 0.0822231 Jy selfcal ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 71 components and 0.0822231 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=0.085027Jy sigma=0.659653 ! Fit after self-cal, rms=0.085040Jy sigma=0.659638 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 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 (-0.6, -12.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000746553 Jy ! Component: 100 - total flux cleaned = 0.000970937 Jy ! Component: 150 - total flux cleaned = 0.00112378 Jy ! Component: 200 - total flux cleaned = 0.00117589 Jy ! Total flux subtracted in 200 components = 0.00117589 Jy ! Clean residual min=-0.000957 max=0.000985 Jy/beam ! Clean residual mean=0.000002 rms=0.000230 Jy/beam ! Combined flux in latest and established models = 0.083399 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 81 components and 0.083399 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=0.085024Jy sigma=0.659470 ! Fit after self-cal, rms=0.085025Jy sigma=0.659448 ! Inverting map ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec ! Added new window around map position (31.8, -19.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0007235 Jy ! Component: 100 - total flux cleaned = 0.000899685 Jy ! Component: 150 - total flux cleaned = 0.00102616 Jy ! Component: 200 - total flux cleaned = 0.00110002 Jy ! Total flux subtracted in 200 components = 0.00110002 Jy ! Clean residual min=-0.000942 max=0.000942 Jy/beam ! Clean residual mean=0.000002 rms=0.000226 Jy/beam ! Combined flux in latest and established models = 0.084499 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 95 components and 0.084499 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=0.085006Jy sigma=0.659328 ! Fit after self-cal, rms=0.085006Jy sigma=0.659315 ! Inverting map ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 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=0.085006Jy sigma=0.659315 ! Fit after self-cal, rms=0.085314Jy sigma=0.659285 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec ! Estimated beam: bmin=0.5784 mas, bmaj=1.377 mas, bpa=-12.57 degrees ! Estimated noise=0.363944 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000386516 Jy ! Component: 100 - total flux cleaned = 0.000561469 Jy ! Component: 150 - total flux cleaned = 0.000614481 Jy ! Component: 200 - total flux cleaned = 0.000680805 Jy ! Total flux subtracted in 200 components = 0.000680805 Jy ! Clean residual min=-0.000948 max=0.000952 Jy/beam ! Clean residual mean=0.000001 rms=0.000224 Jy/beam ! Combined flux in latest and established models = 0.0851798 Jy selfcal ! Performing phase self-cal ! Adding 34 model components to the UV plane model. ! The established model now contains 99 components and 0.0851798 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=0.085306Jy sigma=0.659224 ! Fit after self-cal, rms=0.085310Jy sigma=0.659216 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 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 = 0.000124549 Jy ! Component: 100 - total flux cleaned = 0.000172334 Jy ! Component: 150 - total flux cleaned = 0.000217646 Jy ! Component: 200 - total flux cleaned = 0.000232244 Jy ! Total flux subtracted in 200 components = 0.000232244 Jy ! Clean residual min=-0.000938 max=0.000933 Jy/beam ! Clean residual mean=0.000002 rms=0.000223 Jy/beam ! Combined flux in latest and established models = 0.085412 Jy ! Performing phase self-cal ! Adding 34 model components to the UV plane model. ! The established model now contains 101 components and 0.085412 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=0.085304Jy sigma=0.659180 ! Fit after self-cal, rms=0.085305Jy sigma=0.659179 ! Inverting map ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 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=0.085305Jy sigma=0.659179 ! Fit after self-cal, rms=0.085369Jy sigma=0.659167 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec ! Estimated beam: bmin=2.598 mas, bmaj=3.01 mas, bpa=-1.156 degrees ! Estimated noise=0.483421 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000274695 Jy ! Component: 100 - total flux cleaned = 0.000495205 Jy ! Component: 150 - total flux cleaned = 0.000603955 Jy ! Component: 200 - total flux cleaned = 0.00067672 Jy ! Total flux subtracted in 200 components = 0.00067672 Jy ! Clean residual min=-0.000981 max=0.001140 Jy/beam ! Clean residual mean=0.000005 rms=0.000258 Jy/beam ! Combined flux in latest and established models = 0.0860888 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 111 components and 0.0860888 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=0.085370Jy sigma=0.659160 ! Fit after self-cal, rms=0.085372Jy sigma=0.659151 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 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 (-5.6, -48.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00100321 Jy ! Component: 100 - total flux cleaned = 0.00121101 Jy ! Component: 150 - total flux cleaned = 0.00142451 Jy ! Component: 200 - total flux cleaned = 0.00167985 Jy ! Total flux subtracted in 200 components = 0.00167985 Jy ! Clean residual min=-0.000891 max=0.000954 Jy/beam ! Clean residual mean=0.000004 rms=0.000246 Jy/beam ! Combined flux in latest and established models = 0.0877686 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 127 components and 0.0877686 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=0.085367Jy sigma=0.659098 ! Fit after self-cal, rms=0.085365Jy sigma=0.659083 ! Inverting map ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 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 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec ! Estimated beam: bmin=0.5784 mas, bmaj=1.377 mas, bpa=-12.58 degrees ! Estimated noise=0.364182 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5784 x 1.377 at -12.58 degrees (North through East) ! Clean map min=-0.0010194 max=0.068055 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 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec ! Estimated beam: bmin=0.4461 mas, bmaj=1.165 mas, bpa=-14.16 degrees ! Estimated noise=0.78372 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0523632 Jy ! Component: 100 - total flux cleaned = 0.0639217 Jy ! Component: 150 - total flux cleaned = 0.0677941 Jy ! Component: 200 - total flux cleaned = 0.0705098 Jy ! Total flux subtracted in 200 components = 0.0705098 Jy ! Clean residual min=-0.002505 max=0.002676 Jy/beam ! Clean residual mean=0.000001 rms=0.000560 Jy/beam ! Combined flux in latest and established models = 0.0705099 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 0.0705099 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec ! Estimated beam: bmin=0.5784 mas, bmaj=1.377 mas, bpa=-12.58 degrees ! Estimated noise=0.364182 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 = 0.00379615 Jy ! Component: 100 - total flux cleaned = 0.00620984 Jy ! Component: 150 - total flux cleaned = 0.00805736 Jy ! Component: 200 - total flux cleaned = 0.00956854 Jy ! Total flux subtracted in 200 components = 0.00956854 Jy ! Clean residual min=-0.001129 max=0.001477 Jy/beam ! Clean residual mean=-0.000000 rms=0.000274 Jy/beam ! Combined flux in latest and established models = 0.0800784 Jy ! Adding 32 model components to the UV plane model. ! The established model now contains 42 components and 0.0800784 Jy ! Inverting map ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec ! Added new window around map position (-0.2, -2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00150945 Jy ! Component: 100 - total flux cleaned = 0.00226106 Jy ! Component: 150 - total flux cleaned = 0.0027662 Jy ! Component: 200 - total flux cleaned = 0.00311379 Jy ! Total flux subtracted in 200 components = 0.00311379 Jy ! Clean residual min=-0.001016 max=0.000943 Jy/beam ! Clean residual mean=0.000000 rms=0.000242 Jy/beam ! Combined flux in latest and established models = 0.0831922 Jy ! Adding 39 model components to the UV plane model. ! The established model now contains 66 components and 0.0831922 Jy ! Inverting map ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 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 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec ! Estimated beam: bmin=2.598 mas, bmaj=3.01 mas, bpa=-1.156 degrees ! Estimated noise=0.483421 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00124573 Jy ! Component: 100 - total flux cleaned = 0.0020023 Jy ! Component: 150 - total flux cleaned = 0.00248154 Jy ! Component: 200 - total flux cleaned = 0.00290084 Jy ! Total flux subtracted in 200 components = 0.00290084 Jy ! Clean residual min=-0.000993 max=0.000961 Jy/beam ! Clean residual mean=0.000003 rms=0.000271 Jy/beam ! Combined flux in latest and established models = 0.086093 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 = 0.000375062 Jy ! Component: 100 - total flux cleaned = 0.00073573 Jy ! Component: 150 - total flux cleaned = 0.000963911 Jy ! Component: 200 - total flux cleaned = 0.00119556 Jy ! Total flux subtracted in 200 components = 0.00119556 Jy ! Clean residual min=-0.000920 max=0.000930 Jy/beam ! Clean residual mean=0.000003 rms=0.000254 Jy/beam ! Combined flux in latest and established models = 0.0872886 Jy ! Adding 46 model components to the UV plane model. ! The established model now contains 108 components and 0.0872886 Jy ! Inverting map ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec ! Estimated beam: bmin=0.5784 mas, bmaj=1.377 mas, bpa=-12.58 degrees ! Estimated noise=0.364182 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -2.39008e-05 Jy ! Component: 100 - total flux cleaned = 9.03368e-05 Jy ! Component: 150 - total flux cleaned = 0.000196467 Jy ! Component: 200 - total flux cleaned = 0.000171373 Jy ! Total flux subtracted in 200 components = 0.000171373 Jy ! Clean residual min=-0.000929 max=0.000892 Jy/beam ! Clean residual mean=0.000001 rms=0.000219 Jy/beam ! Combined flux in latest and established models = 0.0874599 Jy selfcal ! Performing phase self-cal ! Adding 40 model components to the UV plane model. ! The established model now contains 133 components and 0.0874599 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=0.085386Jy sigma=0.659164 ! Fit after self-cal, rms=0.085383Jy sigma=0.659118 wmodel /scr/pima/gb073_uvs/J1348+2840_X_map.mod ! Writing 133 model components to file: /scr/pima/gb073_uvs/J1348+2840_X_map.mod wobs /scr/pima/gb073_uvs/J1348+2840_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1348+2840_X_uvs.fits wwins /scr/pima/gb073_uvs/J1348+2840_X_map.win ! wwins: Wrote 7 windows to /scr/pima/gb073_uvs/J1348+2840_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 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -7.05079e-05 Jy ! Component: 100 - total flux cleaned = -5.38939e-05 Jy ! Component: 150 - total flux cleaned = -8.5972e-05 Jy ! Component: 200 - total flux cleaned = -3.84001e-05 Jy ! Component: 250 - total flux cleaned = -5.41555e-05 Jy ! Component: 300 - total flux cleaned = -0.000130621 Jy ! Component: 350 - total flux cleaned = -0.000145607 Jy ! Component: 400 - total flux cleaned = -0.000190378 Jy ! Component: 450 - total flux cleaned = -0.000263842 Jy ! Component: 500 - total flux cleaned = -0.000292907 Jy ! Component: 550 - total flux cleaned = -0.000307169 Jy ! Component: 600 - total flux cleaned = -0.000321347 Jy ! Component: 650 - total flux cleaned = -0.000335403 Jy ! Component: 700 - total flux cleaned = -0.000335355 Jy ! Component: 750 - total flux cleaned = -0.000349435 Jy ! Component: 800 - total flux cleaned = -0.000349555 Jy ! Component: 850 - total flux cleaned = -0.00041825 Jy ! Component: 900 - total flux cleaned = -0.000418298 Jy ! Component: 950 - total flux cleaned = -0.000445408 Jy ! Component: 1000 - total flux cleaned = -0.000445499 Jy ! Component: 1050 - total flux cleaned = -0.000512253 Jy ! Component: 1100 - total flux cleaned = -0.000525532 Jy ! Component: 1150 - total flux cleaned = -0.000512255 Jy ! Component: 1200 - total flux cleaned = -0.000564816 Jy ! Component: 1250 - total flux cleaned = -0.000590821 Jy ! Component: 1300 - total flux cleaned = -0.00061681 Jy ! Component: 1350 - total flux cleaned = -0.000616841 Jy ! Component: 1400 - total flux cleaned = -0.000668232 Jy ! Component: 1450 - total flux cleaned = -0.000680945 Jy ! Component: 1500 - total flux cleaned = -0.000655476 Jy ! Component: 1550 - total flux cleaned = -0.000680789 Jy ! Component: 1600 - total flux cleaned = -0.000693401 Jy ! Component: 1650 - total flux cleaned = -0.000743678 Jy ! Component: 1700 - total flux cleaned = -0.000743564 Jy ! Component: 1750 - total flux cleaned = -0.000805606 Jy ! Component: 1800 - total flux cleaned = -0.00079318 Jy ! Component: 1850 - total flux cleaned = -0.000805439 Jy ! Component: 1900 - total flux cleaned = -0.000793172 Jy ! Component: 1950 - total flux cleaned = -0.000878499 Jy ! Component: 2000 - total flux cleaned = -0.000866377 Jy ! Component: 2050 - total flux cleaned = -0.000878435 Jy ! Component: 2100 - total flux cleaned = -0.000890501 Jy ! Component: 2150 - total flux cleaned = -0.000890564 Jy ! Component: 2200 - total flux cleaned = -0.000986098 Jy ! Component: 2250 - total flux cleaned = -0.000950394 Jy ! Component: 2300 - total flux cleaned = -0.000997773 Jy ! Component: 2350 - total flux cleaned = -0.0010213 Jy ! Component: 2400 - total flux cleaned = -0.00102131 Jy ! Component: 2450 - total flux cleaned = -0.000997818 Jy ! Component: 2500 - total flux cleaned = -0.00103278 Jy ! Component: 2550 - total flux cleaned = -0.00113736 Jy ! Component: 2600 - total flux cleaned = -0.00110264 Jy ! Component: 2650 - total flux cleaned = -0.00112567 Jy ! Component: 2700 - total flux cleaned = -0.0011487 Jy ! Component: 2750 - total flux cleaned = -0.00121735 Jy ! Component: 2800 - total flux cleaned = -0.00129713 Jy ! Component: 2850 - total flux cleaned = -0.00129711 Jy ! Component: 2900 - total flux cleaned = -0.00137638 Jy ! Component: 2950 - total flux cleaned = -0.0014215 Jy ! Component: 3000 - total flux cleaned = -0.00146646 Jy ! Component: 3050 - total flux cleaned = -0.00145521 Jy ! Component: 3100 - total flux cleaned = -0.00147759 Jy ! Component: 3150 - total flux cleaned = -0.0015443 Jy ! Component: 3200 - total flux cleaned = -0.00157762 Jy ! Component: 3250 - total flux cleaned = -0.00157763 Jy ! Component: 3300 - total flux cleaned = -0.00162169 Jy ! Component: 3350 - total flux cleaned = -0.00159978 Jy ! Component: 3400 - total flux cleaned = -0.00164355 Jy ! Component: 3450 - total flux cleaned = -0.00163265 Jy ! Component: 3500 - total flux cleaned = -0.0017306 Jy ! Component: 3550 - total flux cleaned = -0.00173054 Jy ! Component: 3600 - total flux cleaned = -0.00178453 Jy ! Component: 3650 - total flux cleaned = -0.00180607 Jy ! Component: 3700 - total flux cleaned = -0.0017631 Jy ! Component: 3750 - total flux cleaned = -0.00183805 Jy ! Component: 3800 - total flux cleaned = -0.00182736 Jy ! Component: 3850 - total flux cleaned = -0.00186987 Jy ! Component: 3900 - total flux cleaned = -0.00194419 Jy ! Component: 3950 - total flux cleaned = -0.00191238 Jy ! Component: 4000 - total flux cleaned = -0.00193345 Jy ! Component: 4050 - total flux cleaned = -0.00201766 Jy ! Total flux subtracted in 4096 components = -0.00202813 Jy ! Clean residual min=-0.000639 max=0.000672 Jy/beam ! Clean residual mean=0.000002 rms=0.000173 Jy/beam ! Combined flux in latest and established models = 0.0854318 Jy keep ! Adding 327 model components to the UV plane model. ! The established model now contains 460 components and 0.0854318 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1348+2840_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5784 x 1.377 at -12.58 degrees (North through East) ! Clean map min=-0.00080392 max=0.068348 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1348+2840_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0683476 invert ! Inverting map ! Your choice of large map pixels excluded 4.63% of the data. ! The x-axis pixel size should ideally be below 0.1652 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000172515 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.757224 0.757224 1.51445 3.0289 6.05779 12.1156 24.2312 48.4624 96.9247 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0005 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.068 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 396.183 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1348+2840_X_uvs.log closed on Sat Dec 26 09:40:06 2015