! Started logfile: J1751+0939_X_2001_03_12_pus_uvs.log on Wed Jan 2 20:02:10 2013 obs J1751+0939_X_2001_03_12_pus_uva.fits ! Reading UV FITS file: J1751+0939_X_2001_03_12_pus_uva.fits ! AN table 1: 77 integrations on 136 of 136 possible baselines. ! AN table 2: 31 integrations on 136 of 136 possible baselines. ! AN table 3: 18 integrations on 136 of 136 possible baselines. ! AN table 4: 98 integrations on 136 of 136 possible baselines. ! AN table 5: 48 integrations on 136 of 136 possible baselines. ! Apparent sampling: 0.0866944 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1751+0939 ! ! 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 1749 lines of history. ! ! Reading 12828 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 J1751+0939_X_2001_03_12_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 1150 telescope corrections were flagged in sub-array 1. ! A total of 287 telescope corrections were flagged in sub-array 2. ! A total of 139 telescope corrections were flagged in sub-array 3. ! A total of 1375 telescope corrections were flagged in sub-array 4. ! A total of 547 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 1150 telescope corrections were flagged in sub-array 1. ! A total of 287 telescope corrections were flagged in sub-array 2. ! A total of 139 telescope corrections were flagged in sub-array 3. ! A total of 1375 telescope corrections were flagged in sub-array 4. ! A total of 547 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 1150 telescope corrections were flagged in sub-array 1. ! A total of 287 telescope corrections were flagged in sub-array 2. ! A total of 139 telescope corrections were flagged in sub-array 3. ! A total of 1375 telescope corrections were flagged in sub-array 4. ! A total of 547 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 1150 telescope corrections were flagged in sub-array 1. ! A total of 287 telescope corrections were flagged in sub-array 2. ! A total of 139 telescope corrections were flagged in sub-array 3. ! A total of 1375 telescope corrections were flagged in sub-array 4. ! A total of 547 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=3.057601Jy sigma=0.027123 ! Fit after self-cal, rms=2.682730Jy sigma=0.023973 ! 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 4.34% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.5462 mas, bmaj=1.33 mas, bpa=-2.558 degrees ! Estimated noise=1177.74 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 = 2.85309 Jy ! Component: 100 - total flux cleaned = 3.48543 Jy ! Total flux subtracted in 100 components = 3.48543 Jy ! Clean residual min=-0.068815 max=0.206409 Jy/beam ! Clean residual mean=-0.000370 rms=0.019166 Jy/beam ! Combined flux in latest and established models = 3.48543 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 8 components and 3.48543 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.510671Jy sigma=0.004190 ! Fit after self-cal, rms=0.510658Jy sigma=0.004189 ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.211029 Jy ! Component: 100 - total flux cleaned = 0.32396 Jy ! Total flux subtracted in 100 components = 0.32396 Jy ! Clean residual min=-0.061949 max=0.089026 Jy/beam ! Clean residual mean=-0.000227 rms=0.014350 Jy/beam ! Combined flux in latest and established models = 3.80939 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 17 components and 3.8094 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.420210Jy sigma=0.003159 ! Fit after self-cal, rms=0.420031Jy sigma=0.003159 ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Added new window around map position (0.8, -2.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0844401 Jy ! Component: 100 - total flux cleaned = 0.126396 Jy ! Total flux subtracted in 100 components = 0.126396 Jy ! Clean residual min=-0.058388 max=0.070312 Jy/beam ! Clean residual mean=-0.000163 rms=0.013388 Jy/beam ! Combined flux in latest and established models = 3.93579 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 24 components and 3.93579 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.406634Jy sigma=0.002984 ! Fit after self-cal, rms=0.405839Jy sigma=0.002975 ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.1643 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 4.34% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6717 mas, bmaj=1.667 mas, bpa=-2.146 degrees ! Estimated noise=766.105 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 = -0.00147627 Jy ! Component: 100 - total flux cleaned = -0.00137997 Jy ! Component: 150 - total flux cleaned = 0.000669465 Jy ! Component: 200 - total flux cleaned = 0.00153303 Jy ! Total flux subtracted in 200 components = 0.00153303 Jy ! Clean residual min=-0.069323 max=0.058682 Jy/beam ! Clean residual mean=-0.000343 rms=0.014427 Jy/beam ! Combined flux in latest and established models = 3.93732 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 28 components and 3.93732 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.399184Jy sigma=0.002899 ! Fit after self-cal, rms=0.398767Jy sigma=0.002895 ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 84 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 1.00* HH 1.00* HN 1.00* ! KK 1.00* KP 1.17 LA 1.00* MA 1.00* ! MC 1.00* MK 1.00 NL 1.00* ON 1.00* ! OV 0.98 PT 1.00* SC 1.00* TS 1.30 ! WZ 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.99 HH 1.00* HN 1.18 ! KK 0.97 KP 1.02 LA 0.99 MA 1.00* ! MC 1.00* MK 0.96 NL 1.03 ON 1.00* ! OV 0.97 PT 0.99 SC 1.00* TS 0.97 ! 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 0.97 HH 1.00* HN 0.98 ! KK 1.01 KP 0.98 LA 0.97 MA 1.00* ! MC 1.00* MK 1.00 NL 0.96 ON 1.00* ! OV 0.97 PT 0.98 SC 0.99 TS 1.00* ! WZ 1.00* ! ! A total of 291 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! A total of 63 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 1.03 HH 1.10 HN 0.98 ! KK 1.00* KP 1.12 LA 1.01 MA 0.99 ! MC 1.00* MK 1.00* NL 0.98 ON 1.00* ! OV 1.04 PT 0.98 SC 0.99 TS 1.00* ! WZ 0.97 ! ! ! Correcting IF 2. ! A total of 84 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 1.00* HH 1.00* HN 1.00* ! KK 1.00* KP 1.11 LA 1.00* MA 1.00* ! MC 1.00* MK 0.98 NL 1.00* ON 1.00* ! OV 0.99 PT 1.00* SC 1.00* TS 1.30 ! WZ 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.98 HH 1.00* HN 1.18 ! KK 0.97 KP 0.96 LA 0.98 MA 1.00* ! MC 1.00* MK 0.96 NL 0.99 ON 1.00* ! OV 0.97 PT 1.02 SC 1.00* TS 0.97 ! 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 0.96 HH 1.00* HN 0.97 ! KK 1.00 KP 0.93 LA 0.96 MA 1.00* ! MC 1.00* MK 1.00 NL 0.92 ON 1.00* ! OV 0.97 PT 1.02 SC 0.98 TS 1.00* ! WZ 1.00* ! ! A total of 291 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! A total of 63 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 FD 1.02 HH 1.09 HN 0.97 ! KK 1.00* KP 1.06 LA 1.00 MA 0.96 ! MC 1.00* MK 1.00* NL 0.94 ON 1.00* ! OV 1.03 PT 1.02 SC 0.97 TS 1.00* ! WZ 0.98 ! ! ! Correcting IF 3. ! A total of 84 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 1.00* HH 1.00* HN 1.00* ! KK 1.00* KP 1.10 LA 1.00* MA 1.00* ! MC 1.00* MK 1.01 NL 1.00* ON 1.00* ! OV 1.01 PT 1.00* SC 1.00* TS 1.29 ! WZ 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 0.95 HH 1.00* HN 1.18 ! KK 1.03 KP 0.93 LA 0.99 MA 1.00* ! MC 1.00* MK 0.97 NL 0.99 ON 1.00* ! OV 0.99 PT 1.05 SC 1.00* TS 0.95 ! 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 0.94 HH 1.00* HN 0.97 ! KK 1.06 KP 0.90 LA 0.97 MA 1.00* ! MC 1.00* MK 1.01 NL 0.95 ON 1.00* ! OV 0.99 PT 1.04 SC 0.99 TS 1.00* ! WZ 1.00* ! ! A total of 291 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! A total of 63 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.05 FD 0.99 HH 1.09 HN 0.97 ! KK 1.00* KP 1.03 LA 1.02 MA 1.00 ! MC 1.00* MK 1.00* NL 0.98 ON 1.00* ! OV 1.06 PT 1.04 SC 1.01 TS 1.00* ! WZ 0.99 ! ! ! Correcting IF 4. ! A total of 84 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 1.00* HH 1.00* HN 1.00* ! KK 1.00* KP 1.11 LA 1.00* MA 1.00* ! MC 1.00* MK 1.05 NL 1.00* ON 1.00* ! OV 0.99 PT 1.00* SC 1.00* TS 1.31 ! WZ 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.94 HH 1.00* HN 1.19 ! KK 0.99 KP 0.94 LA 0.97 MA 1.00* ! MC 1.00* MK 1.00 NL 1.01 ON 1.00* ! OV 0.98 PT 1.03 SC 1.00* TS 0.94 ! WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 0.92 HH 1.00* HN 0.98 ! KK 1.02 KP 0.92 LA 0.94 MA 1.00* ! MC 1.00* MK 1.04 NL 0.96 ON 1.00* ! OV 0.97 PT 1.03 SC 1.05 TS 1.00* ! WZ 1.00* ! ! A total of 291 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! A total of 63 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 0.98 HH 1.09 HN 0.99 ! KK 1.00* KP 1.04 LA 0.99 MA 1.01 ! MC 1.00* MK 1.00* NL 0.99 ON 1.00* ! OV 1.04 PT 1.03 SC 1.04 TS 1.00* ! WZ 1.00 ! ! ! Fit before self-cal, rms=0.398767Jy sigma=0.002895 ! Fit after self-cal, rms=0.203616Jy sigma=0.001501 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6738 mas, bmaj=1.914 mas, bpa=-5.015 degrees ! Estimated noise=792.434 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 = -0.0109593 Jy ! Component: 100 - total flux cleaned = -0.0121023 Jy ! Component: 150 - total flux cleaned = -0.0120604 Jy ! Component: 200 - total flux cleaned = -0.0110516 Jy ! Total flux subtracted in 200 components = -0.0110516 Jy ! Clean residual min=-0.011712 max=0.022411 Jy/beam ! Clean residual mean=-0.000061 rms=0.002971 Jy/beam ! Combined flux in latest and established models = 3.92627 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 39 components and 3.92627 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.200830Jy sigma=0.001472 ! Fit after self-cal, rms=0.200541Jy sigma=0.001469 ! Inverting map ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Added new window around map position (1.6, 1.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0171446 Jy ! Component: 100 - total flux cleaned = 0.0210195 Jy ! Component: 150 - total flux cleaned = 0.023313 Jy ! Component: 200 - total flux cleaned = 0.0249398 Jy ! Total flux subtracted in 200 components = 0.0249398 Jy ! Clean residual min=-0.011577 max=0.009653 Jy/beam ! Clean residual mean=-0.000021 rms=0.002519 Jy/beam ! Combined flux in latest and established models = 3.95121 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 52 components and 3.95121 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.197893Jy sigma=0.001443 ! Fit after self-cal, rms=0.197595Jy sigma=0.001441 ! Inverting map ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 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=0.197595Jy sigma=0.001441 ! Fit after self-cal, rms=0.192325Jy sigma=0.001414 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6742 mas, bmaj=1.914 mas, bpa=-5.023 degrees ! Estimated noise=792.428 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00154214 Jy ! Component: 100 - total flux cleaned = 0.000310479 Jy ! Component: 150 - total flux cleaned = 0.00124311 Jy ! Component: 200 - total flux cleaned = 0.00287584 Jy ! Total flux subtracted in 200 components = 0.00287584 Jy ! Clean residual min=-0.008877 max=0.008090 Jy/beam ! Clean residual mean=-0.000029 rms=0.001969 Jy/beam ! Combined flux in latest and established models = 3.95409 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 53 components and 3.95409 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.190753Jy sigma=0.001400 ! Fit after self-cal, rms=0.190450Jy sigma=0.001398 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 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 = -0.00134558 Jy ! Component: 100 - total flux cleaned = -0.000363345 Jy ! Component: 150 - total flux cleaned = 0.000521377 Jy ! Component: 200 - total flux cleaned = 0.00131975 Jy ! Total flux subtracted in 200 components = 0.00131975 Jy ! Clean residual min=-0.008318 max=0.007776 Jy/beam ! Clean residual mean=-0.000028 rms=0.001874 Jy/beam ! Combined flux in latest and established models = 3.95541 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 56 components and 3.95541 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.189798Jy sigma=0.001393 ! Fit after self-cal, rms=0.189724Jy sigma=0.001392 ! Inverting map ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 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=0.189724Jy sigma=0.001392 ! Fit after self-cal, rms=0.189288Jy sigma=0.001389 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6744 mas, bmaj=1.914 mas, bpa=-5.017 degrees ! Estimated noise=792.419 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00313851 Jy ! Component: 100 - total flux cleaned = -0.0011736 Jy ! Component: 150 - total flux cleaned = -0.00031224 Jy ! Component: 200 - total flux cleaned = 0.000265531 Jy ! Total flux subtracted in 200 components = 0.000265531 Jy ! Clean residual min=-0.008120 max=0.007016 Jy/beam ! Clean residual mean=-0.000030 rms=0.001691 Jy/beam ! Combined flux in latest and established models = 3.95567 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 59 components and 3.95567 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.188576Jy sigma=0.001382 ! Fit after self-cal, rms=0.188486Jy sigma=0.001382 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 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 = -0.000958764 Jy ! Component: 100 - total flux cleaned = -0.000423081 Jy ! Component: 150 - total flux cleaned = 5.09919e-05 Jy ! Component: 200 - total flux cleaned = 0.000347091 Jy ! Total flux subtracted in 200 components = 0.000347091 Jy ! Clean residual min=-0.007824 max=0.006830 Jy/beam ! Clean residual mean=-0.000030 rms=0.001635 Jy/beam ! Combined flux in latest and established models = 3.95602 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 62 components and 3.95602 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.188161Jy sigma=0.001379 ! Fit after self-cal, rms=0.188120Jy sigma=0.001379 ! Inverting map ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 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=0.188120Jy sigma=0.001379 ! Fit after self-cal, rms=0.187933Jy sigma=0.001377 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=2.508 mas, bmaj=3.223 mas, bpa=-13.65 degrees ! Estimated noise=1002 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00107766 Jy ! Component: 100 - total flux cleaned = 0.00117764 Jy ! Component: 150 - total flux cleaned = 0.00135732 Jy ! Component: 200 - total flux cleaned = 0.0013615 Jy ! Total flux subtracted in 200 components = 0.0013615 Jy ! Clean residual min=-0.006273 max=0.005923 Jy/beam ! Clean residual mean=-0.000054 rms=0.001797 Jy/beam ! Combined flux in latest and established models = 3.95738 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 66 components and 3.95738 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.187736Jy sigma=0.001375 ! Fit after self-cal, rms=0.187715Jy sigma=0.001375 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 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 = 0.000107043 Jy ! Component: 100 - total flux cleaned = 0.000269774 Jy ! Component: 150 - total flux cleaned = 0.000339986 Jy ! Component: 200 - total flux cleaned = 0.000466833 Jy ! Total flux subtracted in 200 components = 0.000466833 Jy ! Clean residual min=-0.006183 max=0.005982 Jy/beam ! Clean residual mean=-0.000053 rms=0.001780 Jy/beam ! Combined flux in latest and established models = 3.95785 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 67 components and 3.95785 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.187627Jy sigma=0.001374 ! Fit after self-cal, rms=0.187615Jy sigma=0.001374 ! Inverting map ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 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 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6746 mas, bmaj=1.914 mas, bpa=-5.011 degrees ! Estimated noise=792.495 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6746 x 1.914 at -5.011 degrees (North through East) ! Clean map min=-0.011527 max=3.7024 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=0.187615Jy sigma=0.001374 ! Fit after self-cal, rms=0.162188Jy sigma=0.001125 ! Inverting map and beam ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6748 mas, bmaj=1.914 mas, bpa=-5.015 degrees ! Estimated noise=792.274 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00299077 Jy ! Component: 100 - total flux cleaned = -0.00267799 Jy ! Component: 150 - total flux cleaned = -0.00239289 Jy ! Component: 200 - total flux cleaned = -0.002131 Jy ! Total flux subtracted in 200 components = -0.002131 Jy ! Clean residual min=-0.005886 max=0.005780 Jy/beam ! Clean residual mean=-0.000021 rms=0.001339 Jy/beam ! Combined flux in latest and established models = 3.95572 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 75 components and 3.95572 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.161855Jy sigma=0.001122 ! Fit after self-cal, rms=0.161821Jy sigma=0.001122 ! Inverting map ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000430193 Jy ! Component: 100 - total flux cleaned = -0.000181926 Jy ! Component: 150 - total flux cleaned = -6.4519e-05 Jy ! Component: 200 - total flux cleaned = 0.000147175 Jy ! Total flux subtracted in 200 components = 0.000147175 Jy ! Clean residual min=-0.005509 max=0.005159 Jy/beam ! Clean residual mean=-0.000021 rms=0.001308 Jy/beam ! Combined flux in latest and established models = 3.95586 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 77 components and 3.95586 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.161655Jy sigma=0.001120 ! Fit after self-cal, rms=0.161636Jy sigma=0.001120 ! Inverting map ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.161636Jy sigma=0.001120 ! Fit after self-cal, rms=0.161494Jy sigma=0.001119 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 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.5479 mas, bmaj=1.395 mas, bpa=-3.074 degrees ! Estimated noise=1211.29 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.85939 Jy ! Component: 100 - total flux cleaned = 3.48545 Jy ! Component: 150 - total flux cleaned = 3.67136 Jy ! Component: 200 - total flux cleaned = 3.76158 Jy ! Total flux subtracted in 200 components = 3.76158 Jy ! Clean residual min=-0.016975 max=0.047899 Jy/beam ! Clean residual mean=-0.000110 rms=0.004952 Jy/beam ! Combined flux in latest and established models = 3.76158 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 3.76158 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.675 mas, bmaj=1.914 mas, bpa=-5.016 degrees ! Estimated noise=792.09 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 = 0.0794511 Jy ! Component: 100 - total flux cleaned = 0.123287 Jy ! Component: 150 - total flux cleaned = 0.150337 Jy ! Component: 200 - total flux cleaned = 0.168831 Jy ! Total flux subtracted in 200 components = 0.168831 Jy ! Clean residual min=-0.006792 max=0.014872 Jy/beam ! Clean residual mean=-0.000057 rms=0.001870 Jy/beam ! Combined flux in latest and established models = 3.93041 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 33 components and 3.93041 Jy ! Inverting map ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Added new window around map position (-0.2, 1.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0145255 Jy ! Component: 100 - total flux cleaned = 0.020249 Jy ! Component: 150 - total flux cleaned = 0.0216245 Jy ! Component: 200 - total flux cleaned = 0.0231368 Jy ! Total flux subtracted in 200 components = 0.0231368 Jy ! Clean residual min=-0.006148 max=0.005815 Jy/beam ! Clean residual mean=-0.000019 rms=0.001443 Jy/beam ! Combined flux in latest and established models = 3.95355 Jy ! Adding 20 model components to the UV plane model. ! The established model now contains 45 components and 3.95355 Jy ! Inverting map ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 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 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=2.507 mas, bmaj=3.224 mas, bpa=-13.75 degrees ! Estimated noise=1001.19 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00296591 Jy ! Component: 100 - total flux cleaned = 0.00339309 Jy ! Component: 150 - total flux cleaned = 0.00347714 Jy ! Component: 200 - total flux cleaned = 0.00355522 Jy ! Total flux subtracted in 200 components = 0.00355522 Jy ! Clean residual min=-0.004369 max=0.004201 Jy/beam ! Clean residual mean=-0.000031 rms=0.001445 Jy/beam ! Combined flux in latest and established models = 3.9571 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 = 0.000132959 Jy ! Component: 100 - total flux cleaned = 0.000133992 Jy ! Component: 150 - total flux cleaned = 0.000134747 Jy ! Component: 200 - total flux cleaned = 8.53729e-05 Jy ! Total flux subtracted in 200 components = 8.53729e-05 Jy ! Clean residual min=-0.004430 max=0.004141 Jy/beam ! Clean residual mean=-0.000030 rms=0.001425 Jy/beam ! Combined flux in latest and established models = 3.95719 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 67 components and 3.95719 Jy ! Inverting map ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.675 mas, bmaj=1.914 mas, bpa=-5.016 degrees ! Estimated noise=792.09 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000991031 Jy ! Component: 100 - total flux cleaned = -0.000994445 Jy ! Component: 150 - total flux cleaned = -0.000993975 Jy ! Component: 200 - total flux cleaned = -0.000588502 Jy ! Total flux subtracted in 200 components = -0.000588502 Jy ! Clean residual min=-0.005681 max=0.004874 Jy/beam ! Clean residual mean=-0.000014 rms=0.001316 Jy/beam ! Combined flux in latest and established models = 3.9566 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 75 components and 3.9566 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.163929Jy sigma=0.001126 ! Fit after self-cal, rms=0.163481Jy sigma=0.001124 wmodel J1751+0939_X_2001_03_12_pus_map.mod ! Writing 75 model components to file: J1751+0939_X_2001_03_12_pus_map.mod wobs J1751+0939_X_2001_03_12_pus_uvs.fits ! Writing UV FITS file: J1751+0939_X_2001_03_12_pus_uvs.fits wwins J1751+0939_X_2001_03_12_pus_map.win ! wwins: Wrote 4 windows to J1751+0939_X_2001_03_12_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 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000485764 Jy ! Component: 100 - total flux cleaned = -0.00132977 Jy ! Component: 150 - total flux cleaned = -0.00115249 Jy ! Component: 200 - total flux cleaned = -0.000553736 Jy ! Component: 250 - total flux cleaned = -0.000220824 Jy ! Component: 300 - total flux cleaned = -5.67037e-05 Jy ! Component: 350 - total flux cleaned = 0.000342374 Jy ! Component: 400 - total flux cleaned = 0.000576793 Jy ! Component: 450 - total flux cleaned = 0.000884758 Jy ! Component: 500 - total flux cleaned = 0.00133921 Jy ! Component: 550 - total flux cleaned = 0.00156182 Jy ! Component: 600 - total flux cleaned = 0.00170922 Jy ! Component: 650 - total flux cleaned = 0.00199869 Jy ! Component: 700 - total flux cleaned = 0.00213945 Jy ! Component: 750 - total flux cleaned = 0.00206751 Jy ! Component: 800 - total flux cleaned = 0.0021369 Jy ! Component: 850 - total flux cleaned = 0.00220638 Jy ! Component: 900 - total flux cleaned = 0.00247892 Jy ! Component: 950 - total flux cleaned = 0.0027474 Jy ! Component: 1000 - total flux cleaned = 0.00301323 Jy ! Component: 1050 - total flux cleaned = 0.00321053 Jy ! Component: 1100 - total flux cleaned = 0.00353643 Jy ! Component: 1150 - total flux cleaned = 0.00392399 Jy ! Component: 1200 - total flux cleaned = 0.00417895 Jy ! Component: 1250 - total flux cleaned = 0.00455952 Jy ! Component: 1300 - total flux cleaned = 0.00474766 Jy ! Component: 1350 - total flux cleaned = 0.00524526 Jy ! Component: 1400 - total flux cleaned = 0.0056159 Jy ! Component: 1450 - total flux cleaned = 0.00616729 Jy ! Component: 1500 - total flux cleaned = 0.00677383 Jy ! Component: 1550 - total flux cleaned = 0.00707466 Jy ! Component: 1600 - total flux cleaned = 0.00737309 Jy ! Component: 1650 - total flux cleaned = 0.00784721 Jy ! Component: 1700 - total flux cleaned = 0.00819952 Jy ! Component: 1750 - total flux cleaned = 0.00866644 Jy ! Component: 1800 - total flux cleaned = 0.00895593 Jy ! Component: 1850 - total flux cleaned = 0.00930102 Jy ! Component: 1900 - total flux cleaned = 0.00969973 Jy ! Component: 1950 - total flux cleaned = 0.00998252 Jy ! Component: 2000 - total flux cleaned = 0.0102075 Jy ! Total flux subtracted in 2048 components = 0.01071 Jy ! Clean residual min=-0.002782 max=0.003295 Jy/beam ! Clean residual mean=-0.000004 rms=0.000978 Jy/beam ! Combined flux in latest and established models = 3.96731 Jy keep ! Adding 141 model components to the UV plane model. ! The established model now contains 211 components and 3.96731 Jy ![Exited script file: muppet] wmap "J1751+0939_X_2001_03_12_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.675 x 1.914 at -5.016 degrees (North through East) ! Clean map min=-0.0048803 max=3.71 Jy/beam ! Writing clean map to FITS file: J1751+0939_X_2001_03_12_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 3.70995 invert ! Inverting map ! Your choice of large map pixels excluded 4.98% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000977928 device "J1751+0939_X_2001_03_12_pus\_map.eps/VPS" ! Attempting to open device: 'J1751+0939_X_2001_03_12_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.0790788 0.0790788 0.158158 0.316315 0.63263 1.26526 2.53052 5.06104 10.1221 20.2442 40.4883 80.9767 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0029 print "peak=",int(1000*peak_flux)/1000 ! peak= 3.709 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.675 x 1.914 at -5.016 degrees (North through East) ! Clean map min=-0.0048803 max=3.71 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. quit ! Quitting program ! Log file J1751+0939_X_2001_03_12_pus_uvs.log closed on Wed Jan 2 20:02:17 2013