! Started logfile: /scr/pima/rv102_uvs/J0805+6144_X_uvs.log on Sat Feb 27 22:24:45 2016 obs /scr/pima/rv102_uvs/J0805+6144_X_uva.fits ! Reading UV FITS file: /scr/pima/rv102_uvs/J0805+6144_X_uva.fits ! AN table 1: 411 integrations on 10 of 10 possible baselines. ! AN table 2: 119 integrations on 10 of 10 possible baselines. ! AN table 3: 221 integrations on 6 of 6 possible baselines. ! AN table 4: 9 integrations on 10 of 10 possible baselines. ! AN table 5: 76 integrations on 78 of 78 possible baselines. ! AN table 6: 60 integrations on 1 of 1 possible baselines. ! AN table 7: 14 integrations on 1 of 1 possible baselines. ! AN table 8: 12 integrations on 1 of 1 possible baselines. ! AN table 9: 42 integrations on 3 of 3 possible baselines. ! AN table 10: 119 integrations on 78 of 78 possible baselines. ! AN table 11: 11 integrations on 6 of 6 possible baselines. ! AN table 12: 9 integrations on 1 of 1 possible baselines. ! AN table 13: 25 integrations on 1 of 1 possible baselines. ! Apparent sampling: 0.554007 visibilities/baseline/integration-bin. ! Found source: J0805+6144 ! ! 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 8.40599e+09 8e+06 1 8e+06 ! 02 2 8.47599e+09 8e+06 1 8e+06 ! 03 3 8.79099e+09 8e+06 1 8e+06 ! 04 4 8.89599e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 139 lines of history. ! ! Reading 49280 visibilities. select rr, 1,2,3,4,6,7,8 ! Restricting channel ranges to the available 4 channels. ! 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 = 1024 print "field_cell =", field_cell ! field_cell = 0.2 print "taper_size =", taper_size ! taper_size = 70 ![@/home/lpetrov/bin/01_muppet /scr/pima/rv102_uvs/J0805+6144_X] float lim_self lim_self = 120.0 float lim_val lim_va = 1.2 integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.03 float dynam dynam = 6.0 float soltime1 soltime1 = 120 float soltime2 soltime2 = 20 float thresh thresh = 0.5 float win_mult win_mult = 1.8 float time_av time_av = 16 float old_peak float new_peak float flux_cutoff mapsize field_size, field_cell ! Map grid = 1024x1024 pixels with 0.200x0.200 milli-arcsec cellsize. startmod ! Applying default point source starting model. ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 1 Jy ! ! Correcting IF 1. ! A total of 1343 telescope corrections were flagged in sub-array 1. ! A total of 444 telescope corrections were flagged in sub-array 2. ! A total of 764 telescope corrections were flagged in sub-array 3. ! A total of 10 telescope corrections were flagged in sub-array 4. ! A total of 390 telescope corrections were flagged in sub-array 5. ! A total of 120 telescope corrections were flagged in sub-array 6. ! A total of 28 telescope corrections were flagged in sub-array 7. ! A total of 24 telescope corrections were flagged in sub-array 8. ! A total of 126 telescope corrections were flagged in sub-array 9. ! A total of 512 telescope corrections were flagged in sub-array 10. ! A total of 26 telescope corrections were flagged in sub-array 11. ! A total of 18 telescope corrections were flagged in sub-array 12. ! A total of 50 telescope corrections were flagged in sub-array 13. ! ! Correcting IF 2. ! A total of 1343 telescope corrections were flagged in sub-array 1. ! A total of 444 telescope corrections were flagged in sub-array 2. ! A total of 764 telescope corrections were flagged in sub-array 3. ! A total of 10 telescope corrections were flagged in sub-array 4. ! A total of 390 telescope corrections were flagged in sub-array 5. ! A total of 120 telescope corrections were flagged in sub-array 6. ! A total of 28 telescope corrections were flagged in sub-array 7. ! A total of 24 telescope corrections were flagged in sub-array 8. ! A total of 126 telescope corrections were flagged in sub-array 9. ! A total of 512 telescope corrections were flagged in sub-array 10. ! A total of 26 telescope corrections were flagged in sub-array 11. ! A total of 18 telescope corrections were flagged in sub-array 12. ! A total of 50 telescope corrections were flagged in sub-array 13. ! ! Correcting IF 3. ! A total of 1743 telescope corrections were flagged in sub-array 1. ! A total of 595 telescope corrections were flagged in sub-array 2. ! A total of 884 telescope corrections were flagged in sub-array 3. ! A total of 10 telescope corrections were flagged in sub-array 4. ! A total of 423 telescope corrections were flagged in sub-array 5. ! A total of 120 telescope corrections were flagged in sub-array 6. ! A total of 28 telescope corrections were flagged in sub-array 7. ! A total of 24 telescope corrections were flagged in sub-array 8. ! A total of 126 telescope corrections were flagged in sub-array 9. ! A total of 585 telescope corrections were flagged in sub-array 10. ! A total of 26 telescope corrections were flagged in sub-array 11. ! A total of 18 telescope corrections were flagged in sub-array 12. ! A total of 50 telescope corrections were flagged in sub-array 13. ! ! Correcting IF 4. ! A total of 1743 telescope corrections were flagged in sub-array 1. ! A total of 595 telescope corrections were flagged in sub-array 2. ! A total of 884 telescope corrections were flagged in sub-array 3. ! A total of 10 telescope corrections were flagged in sub-array 4. ! A total of 423 telescope corrections were flagged in sub-array 5. ! A total of 120 telescope corrections were flagged in sub-array 6. ! A total of 28 telescope corrections were flagged in sub-array 7. ! A total of 24 telescope corrections were flagged in sub-array 8. ! A total of 126 telescope corrections were flagged in sub-array 9. ! A total of 585 telescope corrections were flagged in sub-array 10. ! A total of 26 telescope corrections were flagged in sub-array 11. ! A total of 18 telescope corrections were flagged in sub-array 12. ! A total of 50 telescope corrections were flagged in sub-array 13. ! ! Fit before self-cal, rms=1.081555Jy sigma=14.776033 ! Fit after self-cal, rms=0.766232Jy sigma=11.412220 ! 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 2.39% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.5123 mas, bmaj=0.9289 mas, bpa=76.81 degrees ! Estimated noise=0.66897 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 = 0.163228 Jy ! Component: 100 - total flux cleaned = 0.216109 Jy ! Total flux subtracted in 100 components = 0.216109 Jy ! Clean residual min=-0.023997 max=0.035583 Jy/beam ! Clean residual mean=0.000063 rms=0.004947 Jy/beam ! Combined flux in latest and established models = 0.216109 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.216109 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.247559Jy sigma=3.158575 ! Fit after self-cal, rms=0.247248Jy sigma=3.151135 ! Inverting map ! Your choice of large map pixels excluded 2.39% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec ! Added new window around map position (-4, 3.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0378247 Jy ! Component: 100 - total flux cleaned = 0.0644104 Jy ! Total flux subtracted in 100 components = 0.0644104 Jy ! Clean residual min=-0.021978 max=0.032876 Jy/beam ! Clean residual mean=0.000046 rms=0.004589 Jy/beam ! Combined flux in latest and established models = 0.280519 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 13 components and 0.280519 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.235256Jy sigma=2.982826 ! Fit after self-cal, rms=0.234242Jy sigma=2.966303 ! Inverting map ! Your choice of large map pixels excluded 2.39% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec ! Added new window around map position (1.4, 2.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0316058 Jy ! Component: 100 - total flux cleaned = 0.0519596 Jy ! Total flux subtracted in 100 components = 0.0519596 Jy ! Clean residual min=-0.022419 max=0.027944 Jy/beam ! Clean residual mean=0.000032 rms=0.004248 Jy/beam ! Combined flux in latest and established models = 0.332479 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 20 components and 0.332479 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.226728Jy sigma=2.833316 ! Fit after self-cal, rms=0.226087Jy sigma=2.823136 ! Inverting map ! Your choice of large map pixels excluded 2.39% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec ! Added new window around map position (-3, -3.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0263585 Jy ! Component: 100 - total flux cleaned = 0.0423602 Jy ! Total flux subtracted in 100 components = 0.0423602 Jy ! Clean residual min=-0.021889 max=0.024235 Jy/beam ! Clean residual mean=0.000021 rms=0.003983 Jy/beam ! Combined flux in latest and established models = 0.374839 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 24 components and 0.374839 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.220612Jy sigma=2.719787 ! Fit after self-cal, rms=0.220224Jy sigma=2.715543 ! Inverting map ! Your choice of large map pixels excluded 2.39% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 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 2.39% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.6775 mas, bmaj=1.071 mas, bpa=79.44 degrees ! Estimated noise=0.327025 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 = 0.0390839 Jy ! Component: 100 - total flux cleaned = 0.069219 Jy ! Component: 150 - total flux cleaned = 0.0942031 Jy ! Component: 200 - total flux cleaned = 0.115474 Jy ! Total flux subtracted in 200 components = 0.115474 Jy ! Clean residual min=-0.028995 max=0.043112 Jy/beam ! Clean residual mean=-0.000161 rms=0.008882 Jy/beam ! Combined flux in latest and established models = 0.490313 Jy ! Performing phase self-cal ! Adding 44 model components to the UV plane model. ! The established model now contains 57 components and 0.490313 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.210847Jy sigma=2.527451 ! Fit after self-cal, rms=0.210149Jy sigma=2.517213 ! Inverting map ! Your choice of large map pixels excluded 2.39% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6775 x 1.071 at 79.44 degrees (North through East) ! Clean map min=-0.027252 max=0.23101 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val ! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2. ! Selfcal phase corrections will not be limited. gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 72 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! MA 1.00* NY 1.00* ON 1.00* WF 1.00* ! WZ 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! MA 1.00* MK 1.00* NY 1.00* ON 1.00* ! WF 1.00* ! ! A total of 120 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! MA 0.00* NY 0.00* ON 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! KP 1.00* LA 1.00* NL 1.00* OV 1.00* ! PT 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MA 1.00* NL 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* WF 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! ON 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! HN 0.00* NY 0.00* ! ! Telescope amplitude corrections in sub-array 9: ! MA 0.00* ON 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 10: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MA 1.00* MK 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* WF 1.00* ! WZ 1.00* ! ! A total of 18 telescope corrections were flagged in sub-array 11. ! Telescope amplitude corrections in sub-array 11: ! HN 0.00* NL 0.00* SC 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 12: ! HN 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 13: ! NY 0.00* ON 0.00* ! ! ! Correcting IF 2. ! A total of 72 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! MA 1.00* NY 1.00* ON 1.00* WF 1.00* ! WZ 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! MA 1.00* MK 1.00* NY 1.00* ON 1.00* ! WF 1.00* ! ! A total of 120 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! MA 0.00* NY 0.00* ON 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! KP 1.00* LA 1.00* NL 1.00* OV 1.00* ! PT 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MA 1.00* NL 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* WF 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! ON 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! HN 0.00* NY 0.00* ! ! Telescope amplitude corrections in sub-array 9: ! MA 0.00* ON 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 10: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MA 1.00* MK 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* WF 1.00* ! WZ 1.00* ! ! A total of 18 telescope corrections were flagged in sub-array 11. ! Telescope amplitude corrections in sub-array 11: ! HN 0.00* NL 0.00* SC 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 12: ! HN 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 13: ! NY 0.00* ON 0.00* ! ! ! Correcting IF 3. ! A total of 312 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! MA 0.00* NY 0.00* ON 0.00* WF 0.00* ! WZ 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! MA 0.00* MK 0.00* NY 0.00* ON 0.00* ! WF 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! MA 0.00* NY 0.00* ON 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! KP 1.00* LA 1.00* NL 1.00* OV 1.00* ! PT 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MA 1.00* NL 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* WF 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! ON 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! HN 0.00* NY 0.00* ! ! Telescope amplitude corrections in sub-array 9: ! MA 0.00* ON 0.00* WZ 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MA 1.00* MK 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* WF 1.00* ! WZ 1.00* ! ! A total of 18 telescope corrections were flagged in sub-array 11. ! Telescope amplitude corrections in sub-array 11: ! HN 0.00* NL 0.00* SC 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 12: ! HN 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 13: ! NY 0.00* ON 0.00* ! ! ! Correcting IF 4. ! A total of 312 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! MA 0.00* NY 0.00* ON 0.00* WF 0.00* ! WZ 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! MA 0.00* MK 0.00* NY 0.00* ON 0.00* ! WF 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! MA 0.00* NY 0.00* ON 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! KP 1.00* LA 1.00* NL 1.00* OV 1.00* ! PT 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MA 1.00* NL 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* WF 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! ON 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! HN 0.00* NY 0.00* ! ! Telescope amplitude corrections in sub-array 9: ! MA 0.00* ON 0.00* WZ 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MA 1.00* MK 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* WF 1.00* ! WZ 1.00* ! ! A total of 18 telescope corrections were flagged in sub-array 11. ! Telescope amplitude corrections in sub-array 11: ! HN 0.00* NL 0.00* SC 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 12: ! HN 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 13: ! NY 0.00* ON 0.00* ! ! ! Fit before self-cal, rms=0.210149Jy sigma=2.517213 ! Fit after self-cal, rms=0.206900Jy sigma=2.535179 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.6738 mas, bmaj=1.072 mas, bpa=78.99 degrees ! Estimated noise=0.329131 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 = 0.0238052 Jy ! Component: 100 - total flux cleaned = 0.04211 Jy ! Component: 150 - total flux cleaned = 0.0574833 Jy ! Component: 200 - total flux cleaned = 0.0706196 Jy ! Total flux subtracted in 200 components = 0.0706196 Jy ! Clean residual min=-0.029773 max=0.038792 Jy/beam ! Clean residual mean=-0.000129 rms=0.008082 Jy/beam ! Combined flux in latest and established models = 0.560933 Jy ! Performing phase self-cal ! Adding 34 model components to the UV plane model. ! The established model now contains 65 components and 0.560933 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.203973Jy sigma=2.446951 ! Fit after self-cal, rms=0.203631Jy sigma=2.440107 ! Inverting map ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 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=0.203631Jy sigma=2.440107 ! Fit after self-cal, rms=0.203631Jy sigma=2.440107 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.6738 mas, bmaj=1.072 mas, bpa=78.99 degrees ! Estimated noise=0.329131 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0151451 Jy ! Component: 100 - total flux cleaned = 0.0264565 Jy ! Component: 150 - total flux cleaned = 0.0359983 Jy ! Component: 200 - total flux cleaned = 0.044145 Jy ! Total flux subtracted in 200 components = 0.044145 Jy ! Clean residual min=-0.029592 max=0.035890 Jy/beam ! Clean residual mean=-0.000111 rms=0.007561 Jy/beam ! Combined flux in latest and established models = 0.605078 Jy selfcal ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 69 components and 0.605078 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.202692Jy sigma=2.401950 ! Fit after self-cal, rms=0.202579Jy sigma=2.398954 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 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 (18.8, 30.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0345499 Jy ! Component: 100 - total flux cleaned = 0.0532081 Jy ! Component: 150 - total flux cleaned = 0.0591827 Jy ! Component: 200 - total flux cleaned = 0.0630382 Jy ! Total flux subtracted in 200 components = 0.0630382 Jy ! Clean residual min=-0.022588 max=0.024760 Jy/beam ! Clean residual mean=-0.000059 rms=0.005961 Jy/beam ! Combined flux in latest and established models = 0.668116 Jy ! Performing phase self-cal ! Adding 41 model components to the UV plane model. ! The established model now contains 104 components and 0.668116 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.197574Jy sigma=2.269283 ! Fit after self-cal, rms=0.196582Jy sigma=2.251137 ! Inverting map ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 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=0.196582Jy sigma=2.251137 ! Fit after self-cal, rms=0.196582Jy sigma=2.251137 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.6738 mas, bmaj=1.072 mas, bpa=78.99 degrees ! Estimated noise=0.329131 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0138681 Jy ! Component: 100 - total flux cleaned = 0.01611 Jy ! Component: 150 - total flux cleaned = 0.0184353 Jy ! Component: 200 - total flux cleaned = 0.0199166 Jy ! Total flux subtracted in 200 components = 0.0199166 Jy ! Clean residual min=-0.021206 max=0.021919 Jy/beam ! Clean residual mean=-0.000031 rms=0.005412 Jy/beam ! Combined flux in latest and established models = 0.688033 Jy selfcal ! Performing phase self-cal ! Adding 37 model components to the UV plane model. ! The established model now contains 115 components and 0.688033 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.195569Jy sigma=2.220715 ! Fit after self-cal, rms=0.195461Jy sigma=2.217117 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 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 = 0.00453438 Jy ! Component: 100 - total flux cleaned = 0.00550495 Jy ! Component: 150 - total flux cleaned = 0.0057263 Jy ! Component: 200 - total flux cleaned = 0.00648314 Jy ! Total flux subtracted in 200 components = 0.00648314 Jy ! Clean residual min=-0.020294 max=0.021549 Jy/beam ! Clean residual mean=-0.000021 rms=0.005237 Jy/beam ! Combined flux in latest and established models = 0.694516 Jy ! Performing phase self-cal ! Adding 37 model components to the UV plane model. ! The established model now contains 124 components and 0.694516 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.195056Jy sigma=2.205255 ! Fit after self-cal, rms=0.195057Jy sigma=2.204356 ! Inverting map ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 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=0.195057Jy sigma=2.204356 ! Fit after self-cal, rms=0.195057Jy sigma=2.204356 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=2.39 mas, bmaj=5.03 mas, bpa=-44.87 degrees ! Estimated noise=0.466858 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0107437 Jy ! Component: 100 - total flux cleaned = 0.0134684 Jy ! Component: 150 - total flux cleaned = 0.0149973 Jy ! Component: 200 - total flux cleaned = 0.0154441 Jy ! Total flux subtracted in 200 components = 0.0154441 Jy ! Clean residual min=-0.038258 max=0.041109 Jy/beam ! Clean residual mean=-0.000017 rms=0.011814 Jy/beam ! Combined flux in latest and established models = 0.70996 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 129 components and 0.70996 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.195089Jy sigma=2.203685 ! Fit after self-cal, rms=0.194961Jy sigma=2.201842 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 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 = 0.00103861 Jy ! Component: 100 - total flux cleaned = 0.00117236 Jy ! Component: 150 - total flux cleaned = 0.00131083 Jy ! Component: 200 - total flux cleaned = 0.00131063 Jy ! Total flux subtracted in 200 components = 0.00131063 Jy ! Clean residual min=-0.037718 max=0.041121 Jy/beam ! Clean residual mean=-0.000010 rms=0.011763 Jy/beam ! Combined flux in latest and established models = 0.711271 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 134 components and 0.711271 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194989Jy sigma=2.203056 ! Fit after self-cal, rms=0.194949Jy sigma=2.202513 ! Inverting map ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 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 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.6738 mas, bmaj=1.072 mas, bpa=78.99 degrees ! Estimated noise=0.329131 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6738 x 1.072 at 78.99 degrees (North through East) ! Clean map min=-0.018306 max=0.21326 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 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.5066 mas, bmaj=0.9339 mas, bpa=76.31 degrees ! Estimated noise=0.670198 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.155429 Jy ! Component: 100 - total flux cleaned = 0.221438 Jy ! Component: 150 - total flux cleaned = 0.270133 Jy ! Component: 200 - total flux cleaned = 0.308767 Jy ! Total flux subtracted in 200 components = 0.308767 Jy ! Clean residual min=-0.021799 max=0.025771 Jy/beam ! Clean residual mean=0.000018 rms=0.004331 Jy/beam ! Combined flux in latest and established models = 0.308767 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 0.308767 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.6738 mas, bmaj=1.072 mas, bpa=78.99 degrees ! Estimated noise=0.329131 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 = 0.0689249 Jy ! Component: 100 - total flux cleaned = 0.119657 Jy ! Component: 150 - total flux cleaned = 0.160345 Jy ! Component: 200 - total flux cleaned = 0.193859 Jy ! Total flux subtracted in 200 components = 0.193859 Jy ! Clean residual min=-0.024500 max=0.032241 Jy/beam ! Clean residual mean=-0.000116 rms=0.007269 Jy/beam ! Combined flux in latest and established models = 0.502625 Jy ! Adding 52 model components to the UV plane model. ! The established model now contains 53 components and 0.502625 Jy ! Inverting map ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec ! Added new window around map position (-2.8, 0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0321539 Jy ! Component: 100 - total flux cleaned = 0.0562125 Jy ! Component: 150 - total flux cleaned = 0.0763874 Jy ! Component: 200 - total flux cleaned = 0.093603 Jy ! Total flux subtracted in 200 components = 0.093603 Jy ! Clean residual min=-0.021263 max=0.021592 Jy/beam ! Clean residual mean=-0.000062 rms=0.005666 Jy/beam ! Combined flux in latest and established models = 0.596228 Jy ! Adding 53 model components to the UV plane model. ! The established model now contains 91 components and 0.596229 Jy ! Inverting map ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 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 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=2.39 mas, bmaj=5.03 mas, bpa=-44.87 degrees ! Estimated noise=0.466858 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.032364 Jy ! Component: 100 - total flux cleaned = 0.0542457 Jy ! Component: 150 - total flux cleaned = 0.0699724 Jy ! Component: 200 - total flux cleaned = 0.0814082 Jy ! Total flux subtracted in 200 components = 0.0814082 Jy ! Clean residual min=-0.038589 max=0.039943 Jy/beam ! Clean residual mean=-0.000054 rms=0.011580 Jy/beam ! Combined flux in latest and established models = 0.677637 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 = 0.00843177 Jy ! Component: 100 - total flux cleaned = 0.0146873 Jy ! Component: 150 - total flux cleaned = 0.0193292 Jy ! Component: 200 - total flux cleaned = 0.0220381 Jy ! Total flux subtracted in 200 components = 0.0220381 Jy ! Clean residual min=-0.038061 max=0.041582 Jy/beam ! Clean residual mean=-0.000029 rms=0.011533 Jy/beam ! Combined flux in latest and established models = 0.699675 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 110 components and 0.699675 Jy ! Inverting map ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.6738 mas, bmaj=1.072 mas, bpa=78.99 degrees ! Estimated noise=0.329131 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00426377 Jy ! Component: 100 - total flux cleaned = -0.00520326 Jy ! Component: 150 - total flux cleaned = -0.0057242 Jy ! Component: 200 - total flux cleaned = -0.00547218 Jy ! Total flux subtracted in 200 components = -0.00547218 Jy ! Clean residual min=-0.019423 max=0.021114 Jy/beam ! Clean residual mean=-0.000012 rms=0.005023 Jy/beam ! Combined flux in latest and established models = 0.694203 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 121 components and 0.694203 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194908Jy sigma=2.200356 ! Fit after self-cal, rms=0.194535Jy sigma=2.193667 wmodel /scr/pima/rv102_uvs/J0805+6144_X_map.mod ! Writing 121 model components to file: /scr/pima/rv102_uvs/J0805+6144_X_map.mod wobs /scr/pima/rv102_uvs/J0805+6144_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv102_uvs/J0805+6144_X_uvs.fits wwins /scr/pima/rv102_uvs/J0805+6144_X_map.win ! wwins: Wrote 6 windows to /scr/pima/rv102_uvs/J0805+6144_X_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.00310533 Jy ! Component: 100 - total flux cleaned = 0.0031232 Jy ! Component: 150 - total flux cleaned = 0.00280973 Jy ! Component: 200 - total flux cleaned = 0.0028056 Jy ! Component: 250 - total flux cleaned = 0.00253401 Jy ! Component: 300 - total flux cleaned = 0.00254049 Jy ! Component: 350 - total flux cleaned = 0.00253535 Jy ! Component: 400 - total flux cleaned = 0.00176395 Jy ! Component: 450 - total flux cleaned = 0.00201902 Jy ! Component: 500 - total flux cleaned = 0.00202004 Jy ! Component: 550 - total flux cleaned = 0.00225554 Jy ! Component: 600 - total flux cleaned = 0.00225685 Jy ! Component: 650 - total flux cleaned = 0.00226073 Jy ! Component: 700 - total flux cleaned = 0.00161822 Jy ! Component: 750 - total flux cleaned = 0.00141469 Jy ! Component: 800 - total flux cleaned = 0.000801908 Jy ! Component: 850 - total flux cleaned = 0.00100783 Jy ! Component: 900 - total flux cleaned = 0.000416052 Jy ! Component: 950 - total flux cleaned = 3.19368e-05 Jy ! Component: 1000 - total flux cleaned = 0.000411261 Jy ! Component: 1050 - total flux cleaned = 4.19634e-05 Jy ! Component: 1100 - total flux cleaned = 0.000408316 Jy ! Component: 1150 - total flux cleaned = 0.000223299 Jy ! Component: 1200 - total flux cleaned = 0.000396948 Jy ! Component: 1250 - total flux cleaned = 4.92215e-05 Jy ! Component: 1300 - total flux cleaned = -0.00011905 Jy ! Component: 1350 - total flux cleaned = -0.000284893 Jy ! Component: 1400 - total flux cleaned = 0.00037579 Jy ! Component: 1450 - total flux cleaned = 0.000213069 Jy ! Component: 1500 - total flux cleaned = 0.000532857 Jy ! Component: 1550 - total flux cleaned = 0.000530666 Jy ! Component: 1600 - total flux cleaned = 0.000532068 Jy ! Component: 1650 - total flux cleaned = 0.000994162 Jy ! Component: 1700 - total flux cleaned = 0.00084684 Jy ! Component: 1750 - total flux cleaned = 0.000699011 Jy ! Component: 1800 - total flux cleaned = 0.00113888 Jy ! Component: 1850 - total flux cleaned = 0.00128343 Jy ! Component: 1900 - total flux cleaned = 0.00128546 Jy ! Component: 1950 - total flux cleaned = 0.00142219 Jy ! Component: 2000 - total flux cleaned = 0.00114552 Jy ! Component: 2050 - total flux cleaned = 0.00155744 Jy ! Component: 2100 - total flux cleaned = 0.00182765 Jy ! Component: 2150 - total flux cleaned = 0.00182977 Jy ! Component: 2200 - total flux cleaned = 0.00262026 Jy ! Component: 2250 - total flux cleaned = 0.00222822 Jy ! Component: 2300 - total flux cleaned = 0.00235743 Jy ! Component: 2350 - total flux cleaned = 0.00223142 Jy ! Component: 2400 - total flux cleaned = 0.00286238 Jy ! Component: 2450 - total flux cleaned = 0.00311128 Jy ! Component: 2500 - total flux cleaned = 0.00323567 Jy ! Component: 2550 - total flux cleaned = 0.00384645 Jy ! Component: 2600 - total flux cleaned = 0.00421191 Jy ! Component: 2650 - total flux cleaned = 0.00492917 Jy ! Component: 2700 - total flux cleaned = 0.00552136 Jy ! Component: 2750 - total flux cleaned = 0.00575396 Jy ! Component: 2800 - total flux cleaned = 0.00633281 Jy ! Component: 2850 - total flux cleaned = 0.00679031 Jy ! Component: 2900 - total flux cleaned = 0.00690348 Jy ! Component: 2950 - total flux cleaned = 0.00757829 Jy ! Component: 3000 - total flux cleaned = 0.00768987 Jy ! Component: 3050 - total flux cleaned = 0.00824045 Jy ! Component: 3100 - total flux cleaned = 0.00878642 Jy ! Component: 3150 - total flux cleaned = 0.00910932 Jy ! Component: 3200 - total flux cleaned = 0.00964418 Jy ! Component: 3250 - total flux cleaned = 0.0101723 Jy ! Component: 3300 - total flux cleaned = 0.0100662 Jy ! Component: 3350 - total flux cleaned = 0.0104825 Jy ! Component: 3400 - total flux cleaned = 0.0103815 Jy ! Component: 3450 - total flux cleaned = 0.0105863 Jy ! Component: 3500 - total flux cleaned = 0.0113956 Jy ! Component: 3550 - total flux cleaned = 0.0111967 Jy ! Component: 3600 - total flux cleaned = 0.0115952 Jy ! Component: 3650 - total flux cleaned = 0.0118902 Jy ! Component: 3700 - total flux cleaned = 0.01189 Jy ! Component: 3750 - total flux cleaned = 0.0115026 Jy ! Component: 3800 - total flux cleaned = 0.0116951 Jy ! Component: 3850 - total flux cleaned = 0.0116964 Jy ! Component: 3900 - total flux cleaned = 0.0120751 Jy ! Component: 3950 - total flux cleaned = 0.0118872 Jy ! Component: 4000 - total flux cleaned = 0.0121671 Jy ! Component: 4050 - total flux cleaned = 0.0121672 Jy ! Total flux subtracted in 4096 components = 0.0127187 Jy ! Clean residual min=-0.004824 max=0.004584 Jy/beam ! Clean residual mean=-0.000000 rms=0.001632 Jy/beam ! Combined flux in latest and established models = 0.706921 Jy keep ! Adding 361 model components to the UV plane model. ! The established model now contains 482 components and 0.706921 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/rv102_uvs/J0805+6144_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6738 x 1.072 at 78.99 degrees (North through East) ! Clean map min=-0.009294 max=0.21236 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv102_uvs/J0805+6144_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.212359 invert ! Inverting map ! Your choice of large map pixels excluded 2.5% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.1696 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00161421 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -2.2804 2.2804 4.5608 9.12161 18.2432 36.4864 72.9729 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0048 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.212 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 131.555 quit ! Quitting program ! Log file /scr/pima/rv102_uvs/J0805+6144_X_uvs.log closed on Sat Feb 27 22:24:51 2016