! Started logfile: /d2/scr/pima/rv101_uvs/J0818+4222_X_uvs.log on Sat Nov 29 16:31:44 2014 obs /d2/scr/pima/rv101_uvs/J0818+4222_X_uva.fits ! Reading UV FITS file: /d2/scr/pima/rv101_uvs/J0818+4222_X_uva.fits ! AN table 1: 30 integrations on 45 of 45 possible baselines. ! AN table 2: 198 integrations on 3 of 3 possible baselines. ! AN table 3: 32 integrations on 10 of 10 possible baselines. ! AN table 4: 32 integrations on 6 of 6 possible baselines. ! AN table 5: 32 integrations on 21 of 21 possible baselines. ! AN table 6: 34 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.449739 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0818+4222 ! ! 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 0 lines of history. ! ! Reading 9664 visibilities. select RR ! 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 /d2/scr/pima/rv101_uvs/J0818+4222_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 231 telescope corrections were flagged in sub-array 1. ! A total of 207 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 37 telescope corrections were flagged in sub-array 4. ! A total of 111 telescope corrections were flagged in sub-array 5. ! A total of 257 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 231 telescope corrections were flagged in sub-array 1. ! A total of 207 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 37 telescope corrections were flagged in sub-array 4. ! A total of 111 telescope corrections were flagged in sub-array 5. ! A total of 257 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 238 telescope corrections were flagged in sub-array 1. ! A total of 594 telescope corrections were flagged in sub-array 2. ! A total of 87 telescope corrections were flagged in sub-array 3. ! A total of 65 telescope corrections were flagged in sub-array 4. ! A total of 134 telescope corrections were flagged in sub-array 5. ! A total of 283 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 238 telescope corrections were flagged in sub-array 1. ! A total of 594 telescope corrections were flagged in sub-array 2. ! A total of 87 telescope corrections were flagged in sub-array 3. ! A total of 65 telescope corrections were flagged in sub-array 4. ! A total of 134 telescope corrections were flagged in sub-array 5. ! A total of 283 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.211988Jy sigma=6.467304 ! Fit after self-cal, rms=0.472754Jy sigma=2.710089 ! 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 0.549% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Estimated beam: bmin=0.6326 mas, bmaj=0.8698 mas, bpa=-5.257 degrees ! Estimated noise=2.39064 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 = 0.419691 Jy ! Component: 100 - total flux cleaned = 0.522138 Jy ! Total flux subtracted in 100 components = 0.522138 Jy ! Clean residual min=-0.021358 max=0.046924 Jy/beam ! Clean residual mean=0.000252 rms=0.005339 Jy/beam ! Combined flux in latest and established models = 0.522138 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.522138 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.282723Jy sigma=1.189130 ! Fit after self-cal, rms=0.282639Jy sigma=1.188492 ! Inverting map ! Your choice of large map pixels excluded 0.549% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Added new window around map position (0.8, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0511954 Jy ! Component: 100 - total flux cleaned = 0.0833844 Jy ! Total flux subtracted in 100 components = 0.0833844 Jy ! Clean residual min=-0.018456 max=0.028644 Jy/beam ! Clean residual mean=0.000194 rms=0.004336 Jy/beam ! Combined flux in latest and established models = 0.605523 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 22 components and 0.605523 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.262600Jy sigma=1.068788 ! Fit after self-cal, rms=0.261931Jy sigma=1.064475 ! Inverting map ! Your choice of large map pixels excluded 0.549% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Added new window around map position (1.8, -0.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0307339 Jy ! Component: 100 - total flux cleaned = 0.0514126 Jy ! Total flux subtracted in 100 components = 0.0514126 Jy ! Clean residual min=-0.016614 max=0.017100 Jy/beam ! Clean residual mean=0.000161 rms=0.003792 Jy/beam ! Combined flux in latest and established models = 0.656935 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 35 components and 0.656935 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.254254Jy sigma=1.018658 ! Fit after self-cal, rms=0.253870Jy sigma=1.015862 ! Inverting map ! Your choice of large map pixels excluded 0.549% of the data. ! The x-axis pixel size should ideally be below 0.1953 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 0.549% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Estimated beam: bmin=0.7455 mas, bmaj=0.9888 mas, bpa=-4.199 degrees ! Estimated noise=1.86864 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 = 0.0385307 Jy ! Component: 100 - total flux cleaned = 0.0608896 Jy ! Component: 150 - total flux cleaned = 0.0758102 Jy ! Component: 200 - total flux cleaned = 0.0862116 Jy ! Total flux subtracted in 200 components = 0.0862116 Jy ! Clean residual min=-0.021089 max=0.023561 Jy/beam ! Clean residual mean=0.000374 rms=0.004507 Jy/beam ! Combined flux in latest and established models = 0.743147 Jy ! Performing phase self-cal ! Adding 33 model components to the UV plane model. ! The established model now contains 50 components and 0.743147 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.242842Jy sigma=0.994909 ! Fit after self-cal, rms=0.242648Jy sigma=0.993534 ! Inverting map ! Your choice of large map pixels excluded 0.549% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7455 x 0.9888 at -4.199 degrees (North through East) ! Clean map min=-0.019666 max=0.56718 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. ! Telescope amplitude corrections in sub-array 1: ! FD 1.03 HN 1.06 LA 1.04 MK 1.02 ! NL 1.03 NY 1.06 ON 0.90 OV 1.04 ! PT 0.99 SC 1.12 ! ! A total of 387 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! MA 0.00* NY 0.00* ON 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HN 1.00* MA 1.00* NY 1.00* ON 1.00* ! WF 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! MA 1.00* NY 1.00* ON 1.00* WF 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! HN 1.00* MA 1.00* NL 1.00* NY 1.00* ! ON 1.00* SC 1.00* WF 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! 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* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! FD 1.04 HN 1.08 LA 1.00 MK 1.05 ! NL 1.00 NY 1.01 ON 0.89 OV 1.05 ! PT 0.94 SC 1.10 ! ! A total of 387 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! MA 0.00* NY 0.00* ON 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HN 1.00* MA 1.00* NY 1.00* ON 1.00* ! WF 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! MA 1.00* NY 1.00* ON 1.00* WF 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! HN 1.00* MA 1.00* NL 1.00* NY 1.00* ! ON 1.00* SC 1.00* WF 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! 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* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! FD 1.02 HN 1.07 LA 1.07 MK 1.05 ! NL 1.08 NY 1.00* ON 1.12 OV 1.12 ! PT 0.91 SC 1.18 ! ! Telescope amplitude corrections in sub-array 2: ! MA 0.00* NY 0.00* ON 0.00* ! ! A total of 45 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HN 1.12 MA 1.05 NY 1.00* ON 0.94 ! WF 0.87 ! ! A total of 63 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! MA 0.00* NY 0.00* ON 0.00* WF 0.00* ! ! A total of 48 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! HN 1.14 MA 1.08 NL 1.10 NY 1.00* ! ON 1.03 SC 1.18 WF 0.86 ! ! A total of 45 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! FD 1.02 HN 1.13 KP 1.00* LA 1.07 ! MA 1.03 NL 1.08 NY 1.00* ON 0.98 ! OV 1.05 PT 0.95 SC 1.02 WF 0.89 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! FD 1.09 HN 1.17 LA 1.05 MK 1.08 ! NL 1.09 NY 1.00* ON 1.19 OV 1.06 ! PT 0.93 SC 1.18 ! ! Telescope amplitude corrections in sub-array 2: ! MA 0.00* NY 0.00* ON 0.00* ! ! A total of 45 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HN 1.00* MA 1.00* NY 1.00* ON 1.00* ! WF 1.00* ! ! A total of 63 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! MA 0.00* NY 0.00* ON 0.00* WF 0.00* ! ! A total of 48 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! HN 1.00* MA 1.00* NL 1.00* NY 1.00* ! ON 1.00* SC 1.00* WF 1.00* ! ! A total of 45 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! FD 1.09 HN 1.13 KP 1.00* LA 1.04 ! MA 1.06 NL 1.08 NY 1.00* ON 1.03 ! OV 1.03 PT 1.00 SC 1.06 WF 0.97 ! ! ! Fit before self-cal, rms=0.242648Jy sigma=0.993534 ! Fit after self-cal, rms=0.229483Jy sigma=0.958410 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Estimated beam: bmin=0.7182 mas, bmaj=0.9803 mas, bpa=-1.595 degrees ! Estimated noise=2.02664 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 = 0.0148705 Jy ! Component: 100 - total flux cleaned = 0.0231029 Jy ! Component: 150 - total flux cleaned = 0.0267251 Jy ! Component: 200 - total flux cleaned = 0.02852 Jy ! Total flux subtracted in 200 components = 0.02852 Jy ! Clean residual min=-0.016474 max=0.018110 Jy/beam ! Clean residual mean=0.000376 rms=0.003976 Jy/beam ! Combined flux in latest and established models = 0.771667 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 61 components and 0.771667 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.227372Jy sigma=0.957052 ! Fit after self-cal, rms=0.227254Jy sigma=0.956498 ! Inverting map ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 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=0.227254Jy sigma=0.956498 ! Fit after self-cal, rms=0.224818Jy sigma=0.950383 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Estimated beam: bmin=0.718 mas, bmaj=0.9801 mas, bpa=-1.547 degrees ! Estimated noise=2.04351 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00744225 Jy ! Component: 100 - total flux cleaned = 0.0100853 Jy ! Component: 150 - total flux cleaned = 0.0115814 Jy ! Component: 200 - total flux cleaned = 0.01247 Jy ! Total flux subtracted in 200 components = 0.01247 Jy ! Clean residual min=-0.016337 max=0.016089 Jy/beam ! Clean residual mean=0.000332 rms=0.003697 Jy/beam ! Combined flux in latest and established models = 0.784137 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 66 components and 0.784137 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.224072Jy sigma=0.950931 ! Fit after self-cal, rms=0.224019Jy sigma=0.950778 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 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 = 0.00119901 Jy ! Component: 100 - total flux cleaned = 0.00177726 Jy ! Component: 150 - total flux cleaned = 0.00218978 Jy ! Component: 200 - total flux cleaned = 0.00228574 Jy ! Total flux subtracted in 200 components = 0.00228574 Jy ! Clean residual min=-0.016378 max=0.015897 Jy/beam ! Clean residual mean=0.000325 rms=0.003689 Jy/beam ! Combined flux in latest and established models = 0.786423 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 68 components and 0.786423 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.223844Jy sigma=0.950523 ! Fit after self-cal, rms=0.223831Jy sigma=0.950483 ! Inverting map ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 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=0.223831Jy sigma=0.950483 ! Fit after self-cal, rms=0.215505Jy sigma=0.932353 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Estimated beam: bmin=0.718 mas, bmaj=0.9795 mas, bpa=-1.7 degrees ! Estimated noise=2.05219 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00566946 Jy ! Component: 100 - total flux cleaned = 0.00696285 Jy ! Component: 150 - total flux cleaned = 0.00810116 Jy ! Component: 200 - total flux cleaned = 0.00902373 Jy ! Total flux subtracted in 200 components = 0.00902373 Jy ! Clean residual min=-0.012158 max=0.013364 Jy/beam ! Clean residual mean=0.000265 rms=0.002922 Jy/beam ! Combined flux in latest and established models = 0.795446 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 72 components and 0.795446 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.215186Jy sigma=0.931925 ! Fit after self-cal, rms=0.215088Jy sigma=0.931700 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 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 (2, -3.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0126083 Jy ! Component: 100 - total flux cleaned = 0.0191655 Jy ! Component: 150 - total flux cleaned = 0.0205501 Jy ! Component: 200 - total flux cleaned = 0.0213743 Jy ! Total flux subtracted in 200 components = 0.0213743 Jy ! Clean residual min=-0.011679 max=0.012041 Jy/beam ! Clean residual mean=0.000192 rms=0.002740 Jy/beam ! Combined flux in latest and established models = 0.816821 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 94 components and 0.816821 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.214007Jy sigma=0.926980 ! Fit after self-cal, rms=0.213906Jy sigma=0.926554 ! Inverting map ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Added new window around map position (-5.6, -0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00549837 Jy ! Component: 100 - total flux cleaned = 0.00655703 Jy ! Component: 150 - total flux cleaned = 0.00766514 Jy ! Component: 200 - total flux cleaned = 0.00831613 Jy ! Total flux subtracted in 200 components = 0.00831613 Jy ! Clean residual min=-0.010996 max=0.011256 Jy/beam ! Clean residual mean=0.000165 rms=0.002637 Jy/beam ! Combined flux in latest and established models = 0.825137 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 109 components and 0.825137 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.213266Jy sigma=0.922737 ! Fit after self-cal, rms=0.213195Jy sigma=0.922413 ! Inverting map ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Added new window around map position (-2.4, -51.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00300607 Jy ! Component: 100 - total flux cleaned = 0.00298601 Jy ! Component: 150 - total flux cleaned = 0.00351014 Jy ! Component: 200 - total flux cleaned = 0.00382026 Jy ! Total flux subtracted in 200 components = 0.00382026 Jy ! Clean residual min=-0.010562 max=0.010788 Jy/beam ! Clean residual mean=0.000167 rms=0.002550 Jy/beam ! Combined flux in latest and established models = 0.828957 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 116 components and 0.828957 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.212340Jy sigma=0.919458 ! Fit after self-cal, rms=0.212231Jy sigma=0.919056 ! Inverting map ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 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=0.212231Jy sigma=0.919056 ! Fit after self-cal, rms=0.207012Jy sigma=0.911006 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Estimated beam: bmin=2.153 mas, bmaj=2.369 mas, bpa=78.72 degrees ! Estimated noise=2.86589 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000584052 Jy ! Component: 100 - total flux cleaned = -0.000763344 Jy ! Component: 150 - total flux cleaned = -0.000757957 Jy ! Component: 200 - total flux cleaned = -0.000755947 Jy ! Total flux subtracted in 200 components = -0.000755947 Jy ! Clean residual min=-0.011096 max=0.013687 Jy/beam ! Clean residual mean=0.000652 rms=0.003275 Jy/beam ! Combined flux in latest and established models = 0.828201 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 123 components and 0.828201 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.206924Jy sigma=0.910050 ! Fit after self-cal, rms=0.206899Jy sigma=0.909785 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 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 = 0.000266587 Jy ! Component: 100 - total flux cleaned = 0.000269614 Jy ! Component: 150 - total flux cleaned = 4.72663e-05 Jy ! Component: 200 - total flux cleaned = -0.000160131 Jy ! Total flux subtracted in 200 components = -0.000160131 Jy ! Clean residual min=-0.010926 max=0.013377 Jy/beam ! Clean residual mean=0.000641 rms=0.003227 Jy/beam ! Combined flux in latest and established models = 0.828041 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 130 components and 0.828041 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.206885Jy sigma=0.909776 ! Fit after self-cal, rms=0.206863Jy sigma=0.909705 ! Inverting map ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 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 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Estimated beam: bmin=0.7194 mas, bmaj=0.9789 mas, bpa=-1.76 degrees ! Estimated noise=2.04396 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7194 x 0.9789 at -1.76 degrees (North through East) ! Clean map min=-0.014089 max=0.57634 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=0.206863Jy sigma=0.909705 ! Fit after self-cal, rms=0.203432Jy sigma=0.879141 ! Inverting map and beam ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Estimated beam: bmin=0.7191 mas, bmaj=0.9784 mas, bpa=-1.806 degrees ! Estimated noise=2.0385 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -1.14199e-05 Jy ! Component: 100 - total flux cleaned = -1.69236e-06 Jy ! Component: 150 - total flux cleaned = -1.14497e-06 Jy ! Component: 200 - total flux cleaned = -0.000274778 Jy ! Total flux subtracted in 200 components = -0.000274778 Jy ! Clean residual min=-0.008925 max=0.009435 Jy/beam ! Clean residual mean=0.000151 rms=0.002118 Jy/beam ! Combined flux in latest and established models = 0.827766 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 146 components and 0.827766 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.203184Jy sigma=0.877975 ! Fit after self-cal, rms=0.203166Jy sigma=0.877940 ! Inverting map ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Added new window around map position (-27, -23.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00743138 Jy ! Component: 100 - total flux cleaned = 0.00849306 Jy ! Component: 150 - total flux cleaned = 0.00917833 Jy ! Component: 200 - total flux cleaned = 0.00943516 Jy ! Total flux subtracted in 200 components = 0.00943516 Jy ! Clean residual min=-0.008904 max=0.008352 Jy/beam ! Clean residual mean=0.000134 rms=0.002047 Jy/beam ! Combined flux in latest and established models = 0.837201 Jy ! Performing phase self-cal ! Adding 33 model components to the UV plane model. ! The established model now contains 161 components and 0.837201 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.202727Jy sigma=0.875932 ! Fit after self-cal, rms=0.202711Jy sigma=0.875801 ! Inverting map ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.202711Jy sigma=0.875801 ! Fit after self-cal, rms=0.202582Jy sigma=0.873821 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 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Estimated beam: bmin=0.622 mas, bmaj=0.8593 mas, bpa=-4.071 degrees ! Estimated noise=2.67738 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.441843 Jy ! Component: 100 - total flux cleaned = 0.556569 Jy ! Component: 150 - total flux cleaned = 0.614155 Jy ! Component: 200 - total flux cleaned = 0.653468 Jy ! Total flux subtracted in 200 components = 0.653468 Jy ! Clean residual min=-0.014788 max=0.021891 Jy/beam ! Clean residual mean=0.000184 rms=0.003756 Jy/beam ! Combined flux in latest and established models = 0.653468 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 18 model components to the UV plane model. ! The established model now contains 18 components and 0.653468 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Estimated beam: bmin=0.7194 mas, bmaj=0.9784 mas, bpa=-1.857 degrees ! Estimated noise=2.03827 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 = 0.0441195 Jy ! Component: 100 - total flux cleaned = 0.0734429 Jy ! Component: 150 - total flux cleaned = 0.0950629 Jy ! Component: 200 - total flux cleaned = 0.112269 Jy ! Total flux subtracted in 200 components = 0.112269 Jy ! Clean residual min=-0.010577 max=0.012485 Jy/beam ! Clean residual mean=0.000369 rms=0.002835 Jy/beam ! Combined flux in latest and established models = 0.765737 Jy ! Adding 46 model components to the UV plane model. ! The established model now contains 51 components and 0.765737 Jy ! Inverting map ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Added new window around map position (-7, 10.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0148335 Jy ! Component: 100 - total flux cleaned = 0.0252783 Jy ! Component: 150 - total flux cleaned = 0.033888 Jy ! Component: 200 - total flux cleaned = 0.040712 Jy ! Total flux subtracted in 200 components = 0.040712 Jy ! Clean residual min=-0.009891 max=0.009754 Jy/beam ! Clean residual mean=0.000245 rms=0.002382 Jy/beam ! Combined flux in latest and established models = 0.806449 Jy ! Adding 38 model components to the UV plane model. ! The established model now contains 69 components and 0.806449 Jy ! Inverting map ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 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 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Estimated beam: bmin=2.149 mas, bmaj=2.366 mas, bpa=79.17 degrees ! Estimated noise=2.86281 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0165696 Jy ! Component: 100 - total flux cleaned = 0.0264798 Jy ! Component: 150 - total flux cleaned = 0.0306284 Jy ! Component: 200 - total flux cleaned = 0.0335746 Jy ! Total flux subtracted in 200 components = 0.0335746 Jy ! Clean residual min=-0.009557 max=0.010461 Jy/beam ! Clean residual mean=0.000469 rms=0.002887 Jy/beam ! Combined flux in latest and established models = 0.840024 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 = 0.00204003 Jy ! Component: 100 - total flux cleaned = 0.00321762 Jy ! Component: 150 - total flux cleaned = 0.00407849 Jy ! Component: 200 - total flux cleaned = 0.00454195 Jy ! Total flux subtracted in 200 components = 0.00454195 Jy ! Clean residual min=-0.009389 max=0.009864 Jy/beam ! Clean residual mean=0.000399 rms=0.002743 Jy/beam ! Combined flux in latest and established models = 0.844566 Jy ! Adding 44 model components to the UV plane model. ! The established model now contains 98 components and 0.844566 Jy ! Inverting map ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! Estimated beam: bmin=0.7194 mas, bmaj=0.9784 mas, bpa=-1.857 degrees ! Estimated noise=2.03827 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000334849 Jy ! Component: 100 - total flux cleaned = 0.000982969 Jy ! Component: 150 - total flux cleaned = 0.00177266 Jy ! Component: 200 - total flux cleaned = 0.00250334 Jy ! Total flux subtracted in 200 components = 0.00250334 Jy ! Clean residual min=-0.008740 max=0.008615 Jy/beam ! Clean residual mean=0.000109 rms=0.002054 Jy/beam ! Combined flux in latest and established models = 0.847069 Jy selfcal ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 119 components and 0.847069 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.202816Jy sigma=0.874220 ! Fit after self-cal, rms=0.202667Jy sigma=0.873327 wmodel /d2/scr/pima/rv101_uvs/J0818+4222_X_map.mod ! Writing 119 model components to file: /d2/scr/pima/rv101_uvs/J0818+4222_X_map.mod wobs /d2/scr/pima/rv101_uvs/J0818+4222_X_uvs.fits ! Writing UV FITS file: /d2/scr/pima/rv101_uvs/J0818+4222_X_uvs.fits wwins /d2/scr/pima/rv101_uvs/J0818+4222_X_map.win ! wwins: Wrote 8 windows to /d2/scr/pima/rv101_uvs/J0818+4222_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 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000510582 Jy ! Component: 100 - total flux cleaned = -0.000504749 Jy ! Component: 150 - total flux cleaned = -0.000649558 Jy ! Component: 200 - total flux cleaned = -0.0016407 Jy ! Component: 250 - total flux cleaned = -0.00232782 Jy ! Component: 300 - total flux cleaned = -0.00299997 Jy ! Component: 350 - total flux cleaned = -0.00365823 Jy ! Component: 400 - total flux cleaned = -0.00417522 Jy ! Component: 450 - total flux cleaned = -0.00430329 Jy ! Component: 500 - total flux cleaned = -0.00480388 Jy ! Component: 550 - total flux cleaned = -0.0048043 Jy ! Component: 600 - total flux cleaned = -0.00492601 Jy ! Component: 650 - total flux cleaned = -0.0046854 Jy ! Component: 700 - total flux cleaned = -0.00492393 Jy ! Component: 750 - total flux cleaned = -0.00457306 Jy ! Component: 800 - total flux cleaned = -0.0045743 Jy ! Component: 850 - total flux cleaned = -0.00468996 Jy ! Component: 900 - total flux cleaned = -0.00424072 Jy ! Component: 950 - total flux cleaned = -0.00424263 Jy ! Component: 1000 - total flux cleaned = -0.00446368 Jy ! Component: 1050 - total flux cleaned = -0.0039186 Jy ! Component: 1100 - total flux cleaned = -0.00370216 Jy ! Component: 1150 - total flux cleaned = -0.00348813 Jy ! Component: 1200 - total flux cleaned = -0.00306256 Jy ! Component: 1250 - total flux cleaned = -0.00316879 Jy ! Component: 1300 - total flux cleaned = -0.00295891 Jy ! Component: 1350 - total flux cleaned = -0.00234065 Jy ! Component: 1400 - total flux cleaned = -0.00234084 Jy ! Component: 1450 - total flux cleaned = -0.00193564 Jy ! Component: 1500 - total flux cleaned = -0.00193381 Jy ! Component: 1550 - total flux cleaned = -0.00123684 Jy ! Component: 1600 - total flux cleaned = -0.000645052 Jy ! Component: 1650 - total flux cleaned = -0.000351725 Jy ! Component: 1700 - total flux cleaned = 0.000228007 Jy ! Component: 1750 - total flux cleaned = 0.000227625 Jy ! Component: 1800 - total flux cleaned = 0.00127498 Jy ! Component: 1850 - total flux cleaned = 0.00118158 Jy ! Component: 1900 - total flux cleaned = 0.00211819 Jy ! Component: 1950 - total flux cleaned = 0.00239554 Jy ! Component: 2000 - total flux cleaned = 0.00294841 Jy ! Component: 2050 - total flux cleaned = 0.00313196 Jy ! Component: 2100 - total flux cleaned = 0.00394914 Jy ! Component: 2150 - total flux cleaned = 0.00439873 Jy ! Component: 2200 - total flux cleaned = 0.00475446 Jy ! Component: 2250 - total flux cleaned = 0.00510931 Jy ! Component: 2300 - total flux cleaned = 0.00528571 Jy ! Component: 2350 - total flux cleaned = 0.00589841 Jy ! Component: 2400 - total flux cleaned = 0.00659384 Jy ! Component: 2450 - total flux cleaned = 0.00676601 Jy ! Component: 2500 - total flux cleaned = 0.00736525 Jy ! Component: 2550 - total flux cleaned = 0.00762051 Jy ! Component: 2600 - total flux cleaned = 0.00795945 Jy ! Component: 2650 - total flux cleaned = 0.00871578 Jy ! Component: 2700 - total flux cleaned = 0.00896661 Jy ! Component: 2750 - total flux cleaned = 0.00971328 Jy ! Component: 2800 - total flux cleaned = 0.0098782 Jy ! Component: 2850 - total flux cleaned = 0.0102876 Jy ! Component: 2900 - total flux cleaned = 0.0104495 Jy ! Component: 2950 - total flux cleaned = 0.0108536 Jy ! Component: 3000 - total flux cleaned = 0.0111748 Jy ! Component: 3050 - total flux cleaned = 0.0114948 Jy ! Component: 3100 - total flux cleaned = 0.0116529 Jy ! Component: 3150 - total flux cleaned = 0.0121253 Jy ! Component: 3200 - total flux cleaned = 0.0118905 Jy ! Component: 3250 - total flux cleaned = 0.0123577 Jy ! Component: 3300 - total flux cleaned = 0.0124358 Jy ! Component: 3350 - total flux cleaned = 0.0130514 Jy ! Component: 3400 - total flux cleaned = 0.0135099 Jy ! Component: 3450 - total flux cleaned = 0.0136616 Jy ! Component: 3500 - total flux cleaned = 0.0133597 Jy ! Component: 3550 - total flux cleaned = 0.0138109 Jy ! Component: 3600 - total flux cleaned = 0.0141098 Jy ! Component: 3650 - total flux cleaned = 0.0141842 Jy ! Component: 3700 - total flux cleaned = 0.0141844 Jy ! Component: 3750 - total flux cleaned = 0.0146992 Jy ! Component: 3800 - total flux cleaned = 0.0149916 Jy ! Component: 3850 - total flux cleaned = 0.014774 Jy ! Component: 3900 - total flux cleaned = 0.014846 Jy ! Component: 3950 - total flux cleaned = 0.0155653 Jy ! Component: 4000 - total flux cleaned = 0.0152789 Jy ! Component: 4050 - total flux cleaned = 0.0154927 Jy ! Total flux subtracted in 4096 components = 0.0161296 Jy ! Clean residual min=-0.003972 max=0.004248 Jy/beam ! Clean residual mean=0.000053 rms=0.001151 Jy/beam ! Combined flux in latest and established models = 0.863199 Jy keep ! Adding 338 model components to the UV plane model. ! The established model now contains 457 components and 0.863199 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/d2/scr/pima/rv101_uvs/J0818+4222_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7194 x 0.9784 at -1.857 degrees (North through East) ! Clean map min=-0.0080011 max=0.57259 Jy/beam ! Writing clean map to FITS file: /d2/scr/pima/rv101_uvs/J0818+4222_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.572587 invert ! Inverting map ! Your choice of large map pixels excluded 0.71% of the data. ! The x-axis pixel size should ideally be below 0.1953 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00113545 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.594907 0.594907 1.18981 2.37963 4.75925 9.51851 19.037 38.074 76.1481 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0034 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.572 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 504.28 quit ! Quitting program ! Log file /d2/scr/pima/rv101_uvs/J0818+4222_X_uvs.log closed on Sat Nov 29 16:31:50 2014