! Started logfile: J0914+0245_X_2011_08_02_pus_uvs.log on Wed Apr 18 21:52:10 2012 obs J0914+0245_X_2011_08_02_pus_uva.fits ! Reading UV FITS file: J0914+0245_X_2011_08_02_pus_uva.fits ! AN table 1: 81 integrations on 78 of 78 possible baselines. ! AN table 2: 39 integrations on 78 of 78 possible baselines. ! AN table 3: 12 integrations on 78 of 78 possible baselines. ! Apparent sampling: 0.276807 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0914+0245 ! ! There are 4 IFs, and a total of 4 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.40997e+09 8e+06 1 8e+06 ! 02 2 8.47997e+09 8e+06 1 8e+06 ! 03 3 8.79497e+09 8e+06 1 8e+06 ! 04 4 8.89997e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 3146 lines of history. ! ! Reading 11400 visibilities. select I ! Polarization I is unavailable. ! Selecting polarization: RR, channels: 1..4 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 print "field_size =",field_size ! field_size = 512 print "field_cell =",field_cell ! field_cell = 0.2 print "taper_size =",taper_size ! taper_size = 70 ![@muppet J0914+0245_X_2011_08_02_pus] 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 = 512x512 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 558 telescope corrections were flagged in sub-array 1. ! A total of 192 telescope corrections were flagged in sub-array 2. ! A total of 79 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 558 telescope corrections were flagged in sub-array 1. ! A total of 192 telescope corrections were flagged in sub-array 2. ! A total of 79 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 558 telescope corrections were flagged in sub-array 1. ! A total of 192 telescope corrections were flagged in sub-array 2. ! A total of 79 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 558 telescope corrections were flagged in sub-array 1. ! A total of 192 telescope corrections were flagged in sub-array 2. ! A total of 79 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=0.639672Jy sigma=0.006880 ! Fit after self-cal, rms=0.254037Jy sigma=0.002344 ! 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 6.05% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=0.9637 mas, bmaj=2.12 mas, bpa=-15.35 degrees ! Estimated noise=1124.26 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 = 0.692353 Jy ! Component: 100 - total flux cleaned = 0.866032 Jy ! Total flux subtracted in 100 components = 0.866032 Jy ! Clean residual min=-0.039024 max=0.070967 Jy/beam ! Clean residual mean=-0.000028 rms=0.008895 Jy/beam ! Combined flux in latest and established models = 0.866032 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.866032 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.237191Jy sigma=0.002252 ! Fit after self-cal, rms=0.237008Jy sigma=0.002251 ! Inverting map ! Your choice of large map pixels excluded 6.05% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0753707 Jy ! Component: 100 - total flux cleaned = 0.112233 Jy ! Total flux subtracted in 100 components = 0.112233 Jy ! Clean residual min=-0.032385 max=0.027734 Jy/beam ! Clean residual mean=-0.000088 rms=0.006334 Jy/beam ! Combined flux in latest and established models = 0.978264 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 17 components and 0.978264 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.205486Jy sigma=0.001884 ! Fit after self-cal, rms=0.205129Jy sigma=0.001882 ! Inverting map ! Your choice of large map pixels excluded 6.05% of the data. ! The x-axis pixel size should ideally be below 0.1665 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 6.05% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=1.151 mas, bmaj=2.641 mas, bpa=-15.07 degrees ! Estimated noise=677.664 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 = 0.0367867 Jy ! Component: 100 - total flux cleaned = 0.0562018 Jy ! Component: 150 - total flux cleaned = 0.0677872 Jy ! Component: 200 - total flux cleaned = 0.0726524 Jy ! Total flux subtracted in 200 components = 0.0726524 Jy ! Clean residual min=-0.031320 max=0.025228 Jy/beam ! Clean residual mean=-0.000211 rms=0.007774 Jy/beam ! Combined flux in latest and established models = 1.05092 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 35 components and 1.05092 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.198602Jy sigma=0.001812 ! Fit after self-cal, rms=0.198526Jy sigma=0.001811 ! Inverting map ! Your choice of large map pixels excluded 6.05% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.92 FT 1.00* HH 0.99 ! HN 1.06 KP 0.91 LA 1.03 MK 1.02 ! NL 0.96 OV 1.03 PT 1.07 TS 1.00* ! WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 0.88 FT 1.00* HH 1.00* ! HN 1.04 KP 0.88 LA 0.99 MK 0.97 ! NL 0.95 OV 1.01 PT 1.03 TS 1.00* ! WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 0.89 FT 1.00* HH 1.00* ! HN 1.00* KP 0.91 LA 0.97 MK 0.94 ! NL 1.00* OV 1.03 PT 1.04 TS 1.00* ! WZ 1.00* ! ! ! Correcting IF 2. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.07 FD 0.94 FT 1.00* HH 0.99 ! HN 1.07 KP 0.90 LA 1.06 MK 1.04 ! NL 1.08 OV 1.06 PT 1.15 TS 1.00* ! WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 FD 0.91 FT 1.00* HH 1.00* ! HN 1.07 KP 0.86 LA 1.01 MK 1.01 ! NL 1.07 OV 1.04 PT 1.09 TS 1.00* ! WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 FD 0.91 FT 1.00* HH 1.00* ! HN 1.00* KP 0.86 LA 1.00 MK 1.01 ! NL 1.00* OV 1.03 PT 1.12 TS 1.00* ! WZ 1.00* ! ! ! Correcting IF 3. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 FD 0.91 FT 1.00* HH 1.03 ! HN 1.09 KP 0.80 LA 1.05 MK 1.02 ! NL 1.03 OV 1.04 PT 1.08 TS 1.00* ! WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 0.88 FT 1.00* HH 1.00* ! HN 1.05 KP 0.78 LA 0.99 MK 0.98 ! NL 1.02 OV 1.02 PT 1.03 TS 1.00* ! WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 0.88 FT 1.00* HH 1.00* ! HN 1.00* KP 0.79 LA 0.99 MK 0.97 ! NL 1.00* OV 1.03 PT 1.03 TS 1.00* ! WZ 1.00* ! ! ! Correcting IF 4. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.09 FD 0.98 FT 1.00* HH 1.19 ! HN 1.07 KP 0.87 LA 1.11 MK 1.07 ! NL 1.06 OV 1.09 PT 1.18 TS 1.00* ! WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.06 FD 0.95 FT 1.00* HH 1.00* ! HN 1.05 KP 0.83 LA 1.06 MK 1.07 ! NL 1.04 OV 1.05 PT 1.13 TS 1.00* ! WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.08 FD 0.94 FT 1.00* HH 1.00* ! HN 1.00* KP 0.86 LA 1.04 MK 1.04 ! NL 1.00* OV 1.05 PT 1.14 TS 1.00* ! WZ 1.00* ! ! ! Fit before self-cal, rms=0.198526Jy sigma=0.001811 ! Fit after self-cal, rms=0.165344Jy sigma=0.001387 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=1.159 mas, bmaj=2.714 mas, bpa=-15.46 degrees ! Estimated noise=679.022 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 (1.4, 8.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00834412 Jy ! Component: 100 - total flux cleaned = 0.0119402 Jy ! Component: 150 - total flux cleaned = 0.0141477 Jy ! Component: 200 - total flux cleaned = 0.0147428 Jy ! Total flux subtracted in 200 components = 0.0147428 Jy ! Clean residual min=-0.005072 max=0.005847 Jy/beam ! Clean residual mean=-0.000002 rms=0.001508 Jy/beam ! Combined flux in latest and established models = 1.06566 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 46 components and 1.06566 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.164732Jy sigma=0.001378 ! Fit after self-cal, rms=0.164741Jy sigma=0.001377 ! Inverting map ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 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. ! ! Fit before self-cal, rms=0.164741Jy sigma=0.001377 ! Fit after self-cal, rms=0.163937Jy sigma=0.001369 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=1.158 mas, bmaj=2.709 mas, bpa=-15.45 degrees ! Estimated noise=679.391 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00264489 Jy ! Component: 100 - total flux cleaned = 0.00426128 Jy ! Component: 150 - total flux cleaned = 0.00448627 Jy ! Component: 200 - total flux cleaned = 0.00459211 Jy ! Total flux subtracted in 200 components = 0.00459211 Jy ! Clean residual min=-0.004916 max=0.004952 Jy/beam ! Clean residual mean=-0.000010 rms=0.001246 Jy/beam ! Combined flux in latest and established models = 1.07025 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 54 components and 1.07025 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.163750Jy sigma=0.001366 ! Fit after self-cal, rms=0.163710Jy sigma=0.001366 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 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 = -0.000167329 Jy ! Component: 100 - total flux cleaned = -8.37292e-05 Jy ! Component: 150 - total flux cleaned = -8.41493e-05 Jy ! Component: 200 - total flux cleaned = -0.000165615 Jy ! Total flux subtracted in 200 components = -0.000165615 Jy ! Clean residual min=-0.004635 max=0.004277 Jy/beam ! Clean residual mean=-0.000009 rms=0.001192 Jy/beam ! Combined flux in latest and established models = 1.07009 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 60 components and 1.07009 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.163611Jy sigma=0.001364 ! Fit after self-cal, rms=0.163588Jy sigma=0.001364 ! Inverting map ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 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. ! ! Fit before self-cal, rms=0.163588Jy sigma=0.001364 ! Fit after self-cal, rms=0.163044Jy sigma=0.001357 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=1.158 mas, bmaj=2.705 mas, bpa=-15.44 degrees ! Estimated noise=679.427 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000587463 Jy ! Component: 100 - total flux cleaned = 0.000666369 Jy ! Component: 150 - total flux cleaned = 0.000591176 Jy ! Component: 200 - total flux cleaned = 0.000523878 Jy ! Total flux subtracted in 200 components = 0.000523878 Jy ! Clean residual min=-0.003678 max=0.004039 Jy/beam ! Clean residual mean=0.000002 rms=0.000971 Jy/beam ! Combined flux in latest and established models = 1.07061 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 66 components and 1.07061 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.162973Jy sigma=0.001356 ! Fit after self-cal, rms=0.162963Jy sigma=0.001356 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 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 = -8.10868e-05 Jy ! Component: 100 - total flux cleaned = -8.58733e-05 Jy ! Component: 150 - total flux cleaned = -0.000145618 Jy ! Component: 200 - total flux cleaned = -0.000201804 Jy ! Total flux subtracted in 200 components = -0.000201804 Jy ! Clean residual min=-0.003518 max=0.004002 Jy/beam ! Clean residual mean=0.000002 rms=0.000944 Jy/beam ! Combined flux in latest and established models = 1.07041 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 68 components and 1.07041 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.162911Jy sigma=0.001355 ! Fit after self-cal, rms=0.162903Jy sigma=0.001355 ! Inverting map ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! Added new window around map position (-15.8, 8.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00316196 Jy ! Component: 100 - total flux cleaned = 0.00360294 Jy ! Component: 150 - total flux cleaned = 0.00352832 Jy ! Component: 200 - total flux cleaned = 0.00359183 Jy ! Total flux subtracted in 200 components = 0.00359183 Jy ! Clean residual min=-0.003581 max=0.003508 Jy/beam ! Clean residual mean=-0.000003 rms=0.000865 Jy/beam ! Combined flux in latest and established models = 1.074 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 81 components and 1.074 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.162808Jy sigma=0.001354 ! Fit after self-cal, rms=0.162799Jy sigma=0.001354 ! Inverting map ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 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. ! ! Fit before self-cal, rms=0.162799Jy sigma=0.001354 ! Fit after self-cal, rms=0.162875Jy sigma=0.001354 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=2.492 mas, bmaj=3.926 mas, bpa=-18.01 degrees ! Estimated noise=769.103 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000115963 Jy ! Component: 100 - total flux cleaned = 0.000171607 Jy ! Component: 150 - total flux cleaned = 0.00025592 Jy ! Component: 200 - total flux cleaned = 0.000407014 Jy ! Total flux subtracted in 200 components = 0.000407014 Jy ! Clean residual min=-0.002772 max=0.003266 Jy/beam ! Clean residual mean=-0.000002 rms=0.000831 Jy/beam ! Combined flux in latest and established models = 1.07441 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 95 components and 1.07441 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.162863Jy sigma=0.001354 ! Fit after self-cal, rms=0.162863Jy sigma=0.001354 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 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 = 0.000137433 Jy ! Component: 100 - total flux cleaned = 0.000171593 Jy ! Component: 150 - total flux cleaned = 0.000205063 Jy ! Component: 200 - total flux cleaned = 0.000236213 Jy ! Total flux subtracted in 200 components = 0.000236213 Jy ! Clean residual min=-0.002722 max=0.003243 Jy/beam ! Clean residual mean=-0.000002 rms=0.000823 Jy/beam ! Combined flux in latest and established models = 1.07464 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 102 components and 1.07464 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.162855Jy sigma=0.001354 ! Fit after self-cal, rms=0.162853Jy sigma=0.001353 ! Inverting map ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 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 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=1.158 mas, bmaj=2.705 mas, bpa=-15.45 degrees ! Estimated noise=679.344 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.158 x 2.705 at -15.45 degrees (North through East) ! Clean map min=-0.0029418 max=0.91388 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 ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.162853Jy sigma=0.001353 ! Fit after self-cal, rms=0.150902Jy sigma=0.001228 ! Inverting map and beam ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=1.159 mas, bmaj=2.704 mas, bpa=-15.45 degrees ! Estimated noise=679.142 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000307588 Jy ! Component: 100 - total flux cleaned = 0.000627527 Jy ! Component: 150 - total flux cleaned = 0.000739329 Jy ! Component: 200 - total flux cleaned = 0.000685432 Jy ! Total flux subtracted in 200 components = 0.000685432 Jy ! Clean residual min=-0.003222 max=0.003131 Jy/beam ! Clean residual mean=-0.000005 rms=0.000796 Jy/beam ! Combined flux in latest and established models = 1.07533 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 111 components and 1.07533 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.150865Jy sigma=0.001227 ! Fit after self-cal, rms=0.150862Jy sigma=0.001227 ! Inverting map ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000167141 Jy ! Component: 100 - total flux cleaned = 0.000217025 Jy ! Component: 150 - total flux cleaned = 0.00026503 Jy ! Component: 200 - total flux cleaned = 0.00022022 Jy ! Total flux subtracted in 200 components = 0.00022022 Jy ! Clean residual min=-0.003188 max=0.003107 Jy/beam ! Clean residual mean=-0.000005 rms=0.000784 Jy/beam ! Combined flux in latest and established models = 1.07555 Jy ! Performing phase self-cal ! Adding 32 model components to the UV plane model. ! The established model now contains 115 components and 1.07555 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.150836Jy sigma=0.001227 ! Fit after self-cal, rms=0.150835Jy sigma=0.001227 ! Inverting map ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.150835Jy sigma=0.001227 ! Fit after self-cal, rms=0.150877Jy sigma=0.001227 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 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=0.9633 mas, bmaj=2.17 mas, bpa=-15.69 degrees ! Estimated noise=1136.93 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.698119 Jy ! Component: 100 - total flux cleaned = 0.878147 Jy ! Component: 150 - total flux cleaned = 0.957338 Jy ! Component: 200 - total flux cleaned = 0.995765 Jy ! Total flux subtracted in 200 components = 0.995765 Jy ! Clean residual min=-0.010100 max=0.018177 Jy/beam ! Clean residual mean=0.000019 rms=0.002450 Jy/beam ! Combined flux in latest and established models = 0.995765 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 19 model components to the UV plane model. ! The established model now contains 19 components and 0.995765 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=1.159 mas, bmaj=2.704 mas, bpa=-15.46 degrees ! Estimated noise=678.913 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 = 0.0258967 Jy ! Component: 100 - total flux cleaned = 0.0380938 Jy ! Component: 150 - total flux cleaned = 0.045922 Jy ! Component: 200 - total flux cleaned = 0.0519065 Jy ! Total flux subtracted in 200 components = 0.0519065 Jy ! Clean residual min=-0.004248 max=0.005400 Jy/beam ! Clean residual mean=0.000001 rms=0.001174 Jy/beam ! Combined flux in latest and established models = 1.04767 Jy ! Adding 30 model components to the UV plane model. ! The established model now contains 41 components and 1.04767 Jy ! Inverting map ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! Added new window around map position (0.8, 3.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0054723 Jy ! Component: 100 - total flux cleaned = 0.00971281 Jy ! Component: 150 - total flux cleaned = 0.0133036 Jy ! Component: 200 - total flux cleaned = 0.0163746 Jy ! Total flux subtracted in 200 components = 0.0163746 Jy ! Clean residual min=-0.003287 max=0.003796 Jy/beam ! Clean residual mean=-0.000001 rms=0.000884 Jy/beam ! Combined flux in latest and established models = 1.06405 Jy ! Adding 23 model components to the UV plane model. ! The established model now contains 55 components and 1.06405 Jy ! Inverting map ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! Added new window around map position (-2, 1.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00356737 Jy ! Component: 100 - total flux cleaned = 0.00559173 Jy ! Component: 150 - total flux cleaned = 0.00710744 Jy ! Component: 200 - total flux cleaned = 0.00832479 Jy ! Total flux subtracted in 200 components = 0.00832479 Jy ! Clean residual min=-0.002806 max=0.002928 Jy/beam ! Clean residual mean=-0.000004 rms=0.000795 Jy/beam ! Combined flux in latest and established models = 1.07237 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 70 components and 1.07237 Jy ! Inverting map ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec uvw 0,2 ! Uniform weighting is not currently selected. ! Amplitude error weighting is not currently selected. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=1.118 mas, bmaj=2.154 mas, bpa=-9.126 degrees ! Estimated noise=769.922 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000926485 Jy ! Component: 100 - total flux cleaned = 0.00163225 Jy ! Component: 150 - total flux cleaned = 0.00210332 Jy ! Component: 200 - total flux cleaned = 0.00246661 Jy ! Total flux subtracted in 200 components = 0.00246661 Jy ! Clean residual min=-0.003276 max=0.003396 Jy/beam ! Clean residual mean=-0.000005 rms=0.000927 Jy/beam ! Combined flux in latest and established models = 1.07484 Jy clean ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000274902 Jy ! Component: 100 - total flux cleaned = 0.000406634 Jy ! Component: 150 - total flux cleaned = 0.000534349 Jy ! Component: 200 - total flux cleaned = 0.000719153 Jy ! Total flux subtracted in 200 components = 0.000719153 Jy ! Clean residual min=-0.003175 max=0.003343 Jy/beam ! Clean residual mean=-0.000005 rms=0.000908 Jy/beam ! Combined flux in latest and established models = 1.07556 Jy selfcal ! Performing phase self-cal ! Adding 45 model components to the UV plane model. ! The established model now contains 97 components and 1.07556 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.151589Jy sigma=0.001229 ! Fit after self-cal, rms=0.150945Jy sigma=0.001227 wmodel J0914+0245_X_2011_08_02_pus_map.mod ! Writing 97 model components to file: J0914+0245_X_2011_08_02_pus_map.mod wobs J0914+0245_X_2011_08_02_pus_uvs.fits ! Writing UV FITS file: J0914+0245_X_2011_08_02_pus_uvs.fits wwins J0914+0245_X_2011_08_02_pus_map.win ! wwins: Wrote 5 windows to J0914+0245_X_2011_08_02_pus_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 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000368966 Jy ! Component: 100 - total flux cleaned = 0.000791786 Jy ! Component: 150 - total flux cleaned = 0.000907794 Jy ! Component: 200 - total flux cleaned = 0.000964431 Jy ! Component: 250 - total flux cleaned = 0.001183 Jy ! Component: 300 - total flux cleaned = 0.00128971 Jy ! Component: 350 - total flux cleaned = 0.00134169 Jy ! Component: 400 - total flux cleaned = 0.00129064 Jy ! Component: 450 - total flux cleaned = 0.00124084 Jy ! Component: 500 - total flux cleaned = 0.00124103 Jy ! Component: 550 - total flux cleaned = 0.00109628 Jy ! Component: 600 - total flux cleaned = 0.000954241 Jy ! Component: 650 - total flux cleaned = 0.000861314 Jy ! Component: 700 - total flux cleaned = 0.000723069 Jy ! Component: 750 - total flux cleaned = 0.000677445 Jy ! Component: 800 - total flux cleaned = 0.000542849 Jy ! Component: 850 - total flux cleaned = 0.000366099 Jy ! Component: 900 - total flux cleaned = 0.000279463 Jy ! Component: 950 - total flux cleaned = 0.000194036 Jy ! Component: 1000 - total flux cleaned = 0.000235724 Jy ! Component: 1050 - total flux cleaned = 6.95368e-05 Jy ! Component: 1100 - total flux cleaned = 0.000110858 Jy ! Component: 1150 - total flux cleaned = 0.000111062 Jy ! Component: 1200 - total flux cleaned = 0.000191185 Jy ! Component: 1250 - total flux cleaned = 0.000151872 Jy ! Component: 1300 - total flux cleaned = 0.000308822 Jy ! Component: 1350 - total flux cleaned = 0.00034723 Jy ! Component: 1400 - total flux cleaned = 0.000385575 Jy ! Component: 1450 - total flux cleaned = 0.000386044 Jy ! Component: 1500 - total flux cleaned = 0.000386593 Jy ! Component: 1550 - total flux cleaned = 0.000460186 Jy ! Component: 1600 - total flux cleaned = 0.000386697 Jy ! Component: 1650 - total flux cleaned = 0.000386429 Jy ! Component: 1700 - total flux cleaned = 0.000243067 Jy ! Component: 1750 - total flux cleaned = 0.000313993 Jy ! Component: 1800 - total flux cleaned = 0.000243364 Jy ! Component: 1850 - total flux cleaned = 0.000208474 Jy ! Component: 1900 - total flux cleaned = 0.000173762 Jy ! Component: 1950 - total flux cleaned = 3.63564e-06 Jy ! Component: 2000 - total flux cleaned = -2.97825e-05 Jy ! Total flux subtracted in 2048 components = 7.02223e-05 Jy ! Clean residual min=-0.001753 max=0.001775 Jy/beam ! Clean residual mean=0.000000 rms=0.000636 Jy/beam ! Combined flux in latest and established models = 1.07563 Jy keep ! Adding 121 model components to the UV plane model. ! The established model now contains 218 components and 1.07563 Jy ![Exited script file: muppet] wmap "J0914+0245_X_2011_08_02_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.118 x 2.154 at -9.126 degrees (North through East) ! Clean map min=-0.0028847 max=0.90892 Jy/beam ! Writing clean map to FITS file: J0914+0245_X_2011_08_02_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.908922 invert ! Inverting map ! Your choice of large map pixels excluded 6.07% of the data. ! The x-axis pixel size should ideally be below 0.1665 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000637046 device "J0914+0245_X_2011_08_02_pus\_map.eps/VPS" ! Attempting to open device: 'J0914+0245_X_2011_08_02_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.210264 0.210264 0.420529 0.841057 1.68211 3.36423 6.72846 13.4569 26.9138 53.8277 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0019 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.908 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.118 x 2.154 at -9.126 degrees (North through East) ! Clean map min=-0.0028847 max=0.90892 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0914+0245_X_2011_08_02_pus\_map.gif/vgif" ! Attempting to open device: 'J0914+0245_X_2011_08_02_pus_map.gif/vgif' mapplot cln