! Started logfile: J1104+3812_X_2008_07_09_pus_uvs.log on Sun Oct 10 20:17:57 2010 obs J1104+3812_X_2008_07_09_pus_uva.fits ! Reading UV FITS file: J1104+3812_X_2008_07_09_pus_uva.fits ! AN table 1: 383 integrations on 105 of 105 possible baselines. ! Apparent sampling: 0.169787 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1104+3812 ! ! 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 1142 lines of history. ! ! Reading 27312 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 = 256 print "field_cell =",field_cell ! field_cell = 0.2 print "taper_size =",taper_size ! taper_size = 70 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 = 256x256 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 3474 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 3474 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 3474 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 3474 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.869390Jy sigma=0.007553 ! Fit after self-cal, rms=0.759047Jy sigma=0.006630 ! 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 5.25% of the data. ! The x-axis pixel size should ideally be below 0.1632 milli-arcsec ! Estimated beam: bmin=0.5418 mas, bmaj=1.438 mas, bpa=0.2806 degrees ! Estimated noise=1006.91 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 = 0.19703 Jy ! Component: 100 - total flux cleaned = 0.24368 Jy ! Total flux subtracted in 100 components = 0.24368 Jy ! Clean residual min=-0.009098 max=0.018676 Jy/beam ! Clean residual mean=0.000273 rms=0.003304 Jy/beam ! Combined flux in latest and established models = 0.24368 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.24368 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.157733Jy sigma=0.001280 ! Fit after self-cal, rms=0.157691Jy sigma=0.001280 ! Inverting map ! Your choice of large map pixels excluded 5.25% of the data. ! The x-axis pixel size should ideally be below 0.1632 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 5.25% of the data. ! The x-axis pixel size should ideally be below 0.1632 milli-arcsec ! Estimated beam: bmin=0.6626 mas, bmaj=1.69 mas, bpa=-0.4454 degrees ! Estimated noise=499.336 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 = 0.0275732 Jy ! Component: 100 - total flux cleaned = 0.0403865 Jy ! Component: 150 - total flux cleaned = 0.0481246 Jy ! Component: 200 - total flux cleaned = 0.0534519 Jy ! Total flux subtracted in 200 components = 0.0534519 Jy ! Clean residual min=-0.004890 max=0.009969 Jy/beam ! Clean residual mean=0.000367 rms=0.002068 Jy/beam ! Combined flux in latest and established models = 0.297132 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 28 components and 0.297132 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.154288Jy sigma=0.001230 ! Fit after self-cal, rms=0.154154Jy sigma=0.001229 ! Inverting map ! Your choice of large map pixels excluded 5.25% of the data. ! The x-axis pixel size should ideally be below 0.1632 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 18 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 1.05 HH 1.00* HN 1.10 ! KK 1.07 KP 0.99 LA 0.94 MK 0.98 ! NL 0.99 NY 1.00* ON 1.00* PT 0.94 ! SC 0.99 WZ 1.00 ZC 1.00 ! ! ! Correcting IF 2. ! A total of 18 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 FD 1.06 HH 1.00* HN 1.00 ! KK 1.09 KP 0.94 LA 0.93 MK 1.00 ! NL 0.98 NY 1.00* ON 1.00* PT 0.94 ! SC 0.99 WZ 1.01 ZC 0.98 ! ! ! Correcting IF 3. ! A total of 18 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 1.04 HH 1.00* HN 1.00 ! KK 1.04 KP 0.97 LA 0.94 MK 1.03 ! NL 1.01 NY 1.00* ON 1.00* PT 0.94 ! SC 1.02 WZ 1.02 ZC 0.97 ! ! ! Correcting IF 4. ! A total of 18 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 1.04 HH 1.00* HN 1.02 ! KK 1.00 KP 0.98 LA 0.96 MK 1.04 ! NL 1.01 NY 1.00* ON 1.00* PT 0.99 ! SC 1.01 WZ 1.00 ZC 0.95 ! ! ! Fit before self-cal, rms=0.154154Jy sigma=0.001229 ! Fit after self-cal, rms=0.155116Jy sigma=0.001221 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 milli-arcsec ! Estimated beam: bmin=0.6671 mas, bmaj=1.699 mas, bpa=-0.4353 degrees ! Estimated noise=495.013 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 (-0.8, 1.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00675156 Jy ! Component: 100 - total flux cleaned = 0.00723119 Jy ! Component: 150 - total flux cleaned = 0.00742383 Jy ! Component: 200 - total flux cleaned = 0.0075932 Jy ! Total flux subtracted in 200 components = 0.0075932 Jy ! Clean residual min=-0.003084 max=0.004356 Jy/beam ! Clean residual mean=0.000064 rms=0.001019 Jy/beam ! Combined flux in latest and established models = 0.304725 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 39 components and 0.304725 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.154785Jy sigma=0.001218 ! Fit after self-cal, rms=0.154830Jy sigma=0.001218 ! Inverting map ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 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=0.154830Jy sigma=0.001218 ! Fit after self-cal, rms=0.155797Jy sigma=0.001216 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 milli-arcsec ! Estimated beam: bmin=0.6652 mas, bmaj=1.707 mas, bpa=-0.4876 degrees ! Estimated noise=494.581 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00211574 Jy ! Component: 100 - total flux cleaned = 0.00261672 Jy ! Component: 150 - total flux cleaned = 0.00278414 Jy ! Component: 200 - total flux cleaned = 0.002879 Jy ! Total flux subtracted in 200 components = 0.002879 Jy ! Clean residual min=-0.002580 max=0.003729 Jy/beam ! Clean residual mean=0.000078 rms=0.000795 Jy/beam ! Combined flux in latest and established models = 0.307604 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 46 components and 0.307604 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.155719Jy sigma=0.001215 ! Fit after self-cal, rms=0.155817Jy sigma=0.001215 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 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, 3.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00271246 Jy ! Component: 100 - total flux cleaned = 0.00350083 Jy ! Component: 150 - total flux cleaned = 0.00379911 Jy ! Component: 200 - total flux cleaned = 0.00415684 Jy ! Total flux subtracted in 200 components = 0.00415684 Jy ! Clean residual min=-0.002110 max=0.002518 Jy/beam ! Clean residual mean=0.000054 rms=0.000662 Jy/beam ! Combined flux in latest and established models = 0.311761 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 67 components and 0.311761 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.155754Jy sigma=0.001214 ! Fit after self-cal, rms=0.155741Jy sigma=0.001214 ! Inverting map ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 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=0.155741Jy sigma=0.001214 ! Fit after self-cal, rms=0.155972Jy sigma=0.001214 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 milli-arcsec ! Estimated beam: bmin=0.6648 mas, bmaj=1.709 mas, bpa=-0.5511 degrees ! Estimated noise=494.346 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00106107 Jy ! Component: 100 - total flux cleaned = 0.0017635 Jy ! Component: 150 - total flux cleaned = 0.00219696 Jy ! Component: 200 - total flux cleaned = 0.00244608 Jy ! Total flux subtracted in 200 components = 0.00244608 Jy ! Clean residual min=-0.002068 max=0.002443 Jy/beam ! Clean residual mean=0.000047 rms=0.000615 Jy/beam ! Combined flux in latest and established models = 0.314207 Jy selfcal ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 78 components and 0.314207 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.155949Jy sigma=0.001214 ! Fit after self-cal, rms=0.155961Jy sigma=0.001214 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 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 = 0.000248987 Jy ! Component: 100 - total flux cleaned = 0.000382191 Jy ! Component: 150 - total flux cleaned = 0.000474016 Jy ! Component: 200 - total flux cleaned = 0.000588559 Jy ! Total flux subtracted in 200 components = 0.000588559 Jy ! Clean residual min=-0.002037 max=0.002388 Jy/beam ! Clean residual mean=0.000044 rms=0.000597 Jy/beam ! Combined flux in latest and established models = 0.314796 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 85 components and 0.314796 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.155949Jy sigma=0.001214 ! Fit after self-cal, rms=0.155946Jy sigma=0.001214 ! Inverting map ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 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=0.155946Jy sigma=0.001214 ! Fit after self-cal, rms=0.155947Jy sigma=0.001214 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 milli-arcsec ! Estimated beam: bmin=2.079 mas, bmaj=2.469 mas, bpa=-6.991 degrees ! Estimated noise=706.879 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00173538 Jy ! Component: 100 - total flux cleaned = 0.00243971 Jy ! Component: 150 - total flux cleaned = 0.00276533 Jy ! Component: 200 - total flux cleaned = 0.00304922 Jy ! Total flux subtracted in 200 components = 0.00304922 Jy ! Clean residual min=-0.002373 max=0.003059 Jy/beam ! Clean residual mean=0.000099 rms=0.001019 Jy/beam ! Combined flux in latest and established models = 0.317845 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 98 components and 0.317845 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.155960Jy sigma=0.001214 ! Fit after self-cal, rms=0.155966Jy sigma=0.001214 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 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 = 0.000145624 Jy ! Component: 100 - total flux cleaned = 0.000318086 Jy ! Component: 150 - total flux cleaned = 0.000458957 Jy ! Component: 200 - total flux cleaned = 0.000543118 Jy ! Total flux subtracted in 200 components = 0.000543118 Jy ! Clean residual min=-0.002383 max=0.002866 Jy/beam ! Clean residual mean=0.000092 rms=0.000986 Jy/beam ! Combined flux in latest and established models = 0.318388 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 104 components and 0.318388 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.155970Jy sigma=0.001214 ! Fit after self-cal, rms=0.155969Jy sigma=0.001214 ! Inverting map ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 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 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 milli-arcsec ! Estimated beam: bmin=0.6646 mas, bmaj=1.709 mas, bpa=-0.5668 degrees ! Estimated noise=494.183 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6646 x 1.709 at -0.5668 degrees (North through East) ! Clean map min=-0.0016656 max=0.25845 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 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 milli-arcsec ! Estimated beam: bmin=0.5421 mas, bmaj=1.461 mas, bpa=0.04827 degrees ! Estimated noise=1005 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.195899 Jy ! Component: 100 - total flux cleaned = 0.242606 Jy ! Component: 150 - total flux cleaned = 0.263827 Jy ! Component: 200 - total flux cleaned = 0.276422 Jy ! Total flux subtracted in 200 components = 0.276422 Jy ! Clean residual min=-0.004934 max=0.006717 Jy/beam ! Clean residual mean=0.000117 rms=0.001626 Jy/beam ! Combined flux in latest and established models = 0.276422 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 13 model components to the UV plane model. ! The established model now contains 13 components and 0.276422 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 milli-arcsec ! Estimated beam: bmin=0.6646 mas, bmaj=1.709 mas, bpa=-0.5668 degrees ! Estimated noise=494.183 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 = 0.0111681 Jy ! Component: 100 - total flux cleaned = 0.0176088 Jy ! Component: 150 - total flux cleaned = 0.0221734 Jy ! Component: 200 - total flux cleaned = 0.0255669 Jy ! Total flux subtracted in 200 components = 0.0255669 Jy ! Clean residual min=-0.002631 max=0.003117 Jy/beam ! Clean residual mean=0.000150 rms=0.000876 Jy/beam ! Combined flux in latest and established models = 0.301989 Jy ! Adding 29 model components to the UV plane model. ! The established model now contains 35 components and 0.301989 Jy ! Inverting map ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 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 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 milli-arcsec ! Estimated beam: bmin=2.079 mas, bmaj=2.469 mas, bpa=-6.991 degrees ! Estimated noise=706.879 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0055084 Jy ! Component: 100 - total flux cleaned = 0.00874832 Jy ! Component: 150 - total flux cleaned = 0.0110067 Jy ! Component: 200 - total flux cleaned = 0.0126008 Jy ! Total flux subtracted in 200 components = 0.0126008 Jy ! Clean residual min=-0.002729 max=0.002986 Jy/beam ! Clean residual mean=0.000177 rms=0.001084 Jy/beam ! Combined flux in latest and established models = 0.31459 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 = 0.0011397 Jy ! Component: 100 - total flux cleaned = 0.00196717 Jy ! Component: 150 - total flux cleaned = 0.00257233 Jy ! Component: 200 - total flux cleaned = 0.00301738 Jy ! Total flux subtracted in 200 components = 0.00301738 Jy ! Clean residual min=-0.002562 max=0.002894 Jy/beam ! Clean residual mean=0.000107 rms=0.000988 Jy/beam ! Combined flux in latest and established models = 0.317607 Jy ! Adding 63 model components to the UV plane model. ! The established model now contains 93 components and 0.317607 Jy ! Inverting map ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 milli-arcsec ! Estimated beam: bmin=0.6646 mas, bmaj=1.709 mas, bpa=-0.5668 degrees ! Estimated noise=494.183 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000105782 Jy ! Component: 100 - total flux cleaned = 0.000205009 Jy ! Component: 150 - total flux cleaned = 0.000288147 Jy ! Component: 200 - total flux cleaned = 0.000286425 Jy ! Total flux subtracted in 200 components = 0.000286425 Jy ! Clean residual min=-0.002018 max=0.002351 Jy/beam ! Clean residual mean=0.000033 rms=0.000586 Jy/beam ! Combined flux in latest and established models = 0.317894 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 104 components and 0.317894 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.155955Jy sigma=0.001214 ! Fit after self-cal, rms=0.155921Jy sigma=0.001213 wmodel J1104+3812_X_2008_07_09_pus_map.mod ! Writing 104 model components to file: J1104+3812_X_2008_07_09_pus_map.mod wobs J1104+3812_X_2008_07_09_pus_uvs.fits ! Writing UV FITS file: J1104+3812_X_2008_07_09_pus_uvs.fits wwins J1104+3812_X_2008_07_09_pus_map.win ! wwins: Wrote 3 windows to J1104+3812_X_2008_07_09_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 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000256626 Jy ! Component: 100 - total flux cleaned = 9.05418e-05 Jy ! Component: 150 - total flux cleaned = -1.41995e-06 Jy ! Component: 200 - total flux cleaned = 2.72662e-05 Jy ! Component: 250 - total flux cleaned = 5.49906e-05 Jy ! Component: 300 - total flux cleaned = 2.96433e-05 Jy ! Component: 350 - total flux cleaned = -2.07368e-05 Jy ! Component: 400 - total flux cleaned = -9.56257e-05 Jy ! Component: 450 - total flux cleaned = -9.56109e-05 Jy ! Component: 500 - total flux cleaned = -7.00875e-07 Jy ! Component: 550 - total flux cleaned = -3.51901e-07 Jy ! Component: 600 - total flux cleaned = 6.85756e-05 Jy ! Component: 650 - total flux cleaned = 0.000113435 Jy ! Component: 700 - total flux cleaned = 0.000179328 Jy ! Component: 750 - total flux cleaned = 0.000242992 Jy ! Component: 800 - total flux cleaned = 0.000347518 Jy ! Component: 850 - total flux cleaned = 0.000409146 Jy ! Component: 900 - total flux cleaned = 0.000449203 Jy ! Component: 950 - total flux cleaned = 0.000469005 Jy ! Component: 1000 - total flux cleaned = 0.000508174 Jy ! Total flux subtracted in 1024 components = 0.00050823 Jy ! Clean residual min=-0.001148 max=0.001119 Jy/beam ! Clean residual mean=0.000007 rms=0.000384 Jy/beam ! Combined flux in latest and established models = 0.318402 Jy keep ! Adding 71 model components to the UV plane model. ! The established model now contains 175 components and 0.318402 Jy wmap "J1104+3812_X_2008_07_09_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6646 x 1.709 at -0.5668 degrees (North through East) ! Clean map min=-0.0017629 max=0.2584 Jy/beam ! Writing clean map to FITS file: J1104+3812_X_2008_07_09_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.258397 invert ! Inverting map ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.1632 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000385237 device "J1104+3812_X_2008_07_09_pus\_map.eps/VPS" ! Attempting to open device: 'J1104+3812_X_2008_07_09_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.447263 0.447263 0.894526 1.78905 3.5781 7.15621 14.3124 28.6248 57.2497 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0011 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.258 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6646 x 1.709 at -0.5668 degrees (North through East) ! Clean map min=-0.0017629 max=0.2584 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1104+3812_X_2008_07_09_pus\_map.gif/vgif" ! Attempting to open device: 'J1104+3812_X_2008_07_09_pus_map.gif/vgif' mapplot cln quit ! Quitting program ! Log file J1104+3812_X_2008_07_09_pus_uvs.log closed on Sun Oct 10 20:18:02 2010