! Started logfile: 1357+769_S.log on Sun Jul 16 12:06:40 2006 observe 1357+769_S.edt ! Reading UV FITS file: 1357+769_S.edt ! AN table 1: 26 integrations on 190 of 190 possible baselines. ! AN table 2: 225 integrations on 190 of 190 possible baselines. ! AN table 3: 13 integrations on 190 of 190 possible baselines. ! AN table 4: 9 integrations on 190 of 190 possible baselines. ! AN table 5: 7 integrations on 190 of 190 possible baselines. ! Apparent sampling: 0.117143 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 1357+769 ! ! 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 2.22497e+09 8e+06 1 8e+06 ! 02 2 2.24497e+09 8e+06 1 8e+06 ! 03 3 2.33497e+09 8e+06 1 8e+06 ! 04 4 2.36497e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 1592 lines of history. ! ! Reading 24928 visibilities. ![@gonzo7-0.4 1357+769_S] print "***********************************" ! *********************************** print "*** Using gonzo instruction set ***" ! *** Using gonzo instruction set *** print "***********************************" ! *********************************** float field_size field_size = 1024 float field_cell field_cell = 0.4 integer clean_niter clean_niter = 50 float clean_gain clean_gain = 0.03 float dynam dynam = 7.0 float win_mult win_mult = 1.8 float solint solint = 3.6/6.0 logical doflt doflt = true logical doamp float new_peak float flux_cutoff mapsize field_size,field_cell ! Map grid = 1024x1024 pixels with 0.400x0.400 milli-arcsec cellsize. select ! 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 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 394 telescope corrections were flagged in sub-array 1. ! A total of 3408 telescope corrections were flagged in sub-array 2. ! A total of 174 telescope corrections were flagged in sub-array 3. ! A total of 154 telescope corrections were flagged in sub-array 4. ! A total of 120 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 392 telescope corrections were flagged in sub-array 1. ! A total of 3411 telescope corrections were flagged in sub-array 2. ! A total of 174 telescope corrections were flagged in sub-array 3. ! A total of 154 telescope corrections were flagged in sub-array 4. ! A total of 120 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 392 telescope corrections were flagged in sub-array 1. ! A total of 3529 telescope corrections were flagged in sub-array 2. ! A total of 174 telescope corrections were flagged in sub-array 3. ! A total of 156 telescope corrections were flagged in sub-array 4. ! A total of 114 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 393 telescope corrections were flagged in sub-array 1. ! A total of 3414 telescope corrections were flagged in sub-array 2. ! A total of 174 telescope corrections were flagged in sub-array 3. ! A total of 155 telescope corrections were flagged in sub-array 4. ! A total of 120 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=0.519765Jy sigma=0.006767 ! Fit after self-cal, rms=0.514025Jy sigma=0.006734 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvweight 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. doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=1.83 mas, bmaj=2.661 mas, bpa=28.68 degrees ! Estimated noise=873.047 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0, 0). ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.384254 Jy ! Total flux subtracted in 50 components = 0.384254 Jy ! Clean residual min=-0.013611 max=0.107215 Jy/beam ! Clean residual mean=0.000066 rms=0.004249 Jy/beam ! Combined flux in latest and established models = 0.384254 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 0.384254 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.245187Jy sigma=0.003226 ! Fit after self-cal, rms=0.245187Jy sigma=0.003226 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0937455 Jy ! Total flux subtracted in 50 components = 0.0937455 Jy ! Clean residual min=-0.009914 max=0.038229 Jy/beam ! Clean residual mean=0.000044 rms=0.002787 Jy/beam ! Combined flux in latest and established models = 0.478 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 9 model components to the UV plane model. ! The established model now contains 9 components and 0.478 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.202990Jy sigma=0.002584 ! Fit after self-cal, rms=0.202970Jy sigma=0.002584 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0411845 Jy ! Total flux subtracted in 50 components = 0.0411845 Jy ! Clean residual min=-0.009623 max=0.021225 Jy/beam ! Clean residual mean=0.000034 rms=0.002418 Jy/beam ! Combined flux in latest and established models = 0.519184 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 13 model components to the UV plane model. ! The established model now contains 14 components and 0.519184 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.192040Jy sigma=0.002411 ! Fit after self-cal, rms=0.192027Jy sigma=0.002411 ! Inverting map ! Added new window around map position (-2.4, -1.2). ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.022793 Jy ! Total flux subtracted in 50 components = 0.022793 Jy ! Clean residual min=-0.009631 max=0.013153 Jy/beam ! Clean residual mean=0.000027 rms=0.002292 Jy/beam ! Combined flux in latest and established models = 0.541977 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 13 model components to the UV plane model. ! The established model now contains 24 components and 0.541977 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.188280Jy sigma=0.002350 ! Fit after self-cal, rms=0.188251Jy sigma=0.002350 ! Inverting map print "****************************************" ! **************************************** print "*** Finished Uniform Weighting CLEAN ***" ! *** Finished Uniform Weighting CLEAN *** print "****************************************" ! **************************************** uvweight 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 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=2.375 mas, bmaj=3.7 mas, bpa=34.56 degrees ! Estimated noise=428.558 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (2, 0.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.027595 Jy ! Component: 100 - total flux cleaned = 0.0412208 Jy ! Total flux subtracted in 100 components = 0.0412208 Jy ! Clean residual min=-0.012888 max=0.014977 Jy/beam ! Clean residual mean=0.000101 rms=0.003025 Jy/beam ! Combined flux in latest and established models = 0.583198 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 33 model components to the UV plane model. ! The established model now contains 54 components and 0.583198 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.185001Jy sigma=0.002294 ! Fit after self-cal, rms=0.184995Jy sigma=0.002294 ! Inverting map print "****************************************" ! **************************************** print "*** Finished Natural Weighting CLEAN ***" ! *** Finished Natural Weighting CLEAN *** print "****************************************" ! **************************************** gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 0.95 GC 0.86 HN 1.00 ! LA 0.95 NL 0.98 OV 0.95 SC 0.84 ! WF 0.95 GG 1.00* HH 1.00* KK 0.98 ! KP 0.96 MA 1.30 MC 1.23 MK 1.00* ! NY 0.84 TS 1.00* WZ 1.00* PT 1.00* ! ! A total of 75 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 1.03 GC 1.00* HN 0.98 ! LA 0.99 NL 0.99 OV 1.03 SC 1.06 ! WF 1.02 GG 1.00* HH 1.00* KK 1.00* ! KP 0.99 MA 1.04 MC 0.92 MK 1.00 ! NY 1.00* TS 1.00* WZ 1.00* PT 1.01 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 FD 1.03 GC 1.04 HN 1.00 ! LA 1.19 NL 1.06 OV 1.07 SC 0.99 ! WF 0.99 GG 1.00* HH 1.00* KK 1.00* ! KP 1.10 MA 1.36 MC 1.05 MK 1.01 ! NY 1.04 TS 0.82 WZ 1.00* PT 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* GC 1.00* HN 1.00* ! LA 1.00* NL 1.00* OV 1.00* SC 1.00* ! WF 0.76 GG 1.00* HH 1.00* KK 1.17 ! KP 0.86 MA 1.00* MC 1.00* MK 1.00* ! NY 1.00* TS 1.06 WZ 1.00* PT 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.04 FD 1.00* GC 1.01 HN 1.00* ! LA 1.00* NL 1.00* OV 0.99 SC 1.00* ! WF 1.00* GG 1.00* HH 1.00* KK 1.00* ! KP 1.02 MA 1.00* MC 1.00* MK 1.00* ! NY 1.00* TS 1.00* WZ 1.00* PT 1.10 ! ! ! Correcting IF 2. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.93 FD 0.96 GC 0.81 HN 0.98 ! LA 0.97 NL 1.02 OV 0.94 SC 1.02 ! WF 0.96 GG 1.00* HH 1.00* KK 0.93 ! KP 0.99 MA 1.31 MC 0.99 MK 0.99 ! NY 0.87 TS 1.00* WZ 1.00* PT 1.00* ! ! A total of 66 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 FD 1.03 GC 1.00* HN 1.00 ! LA 0.98 NL 1.01 OV 1.06 SC 1.06 ! WF 0.98 GG 1.00* HH 1.00* KK 1.00* ! KP 0.93 MA 1.74 MC 1.20 MK 1.04 ! NY 1.00* TS 1.00* WZ 1.00* PT 1.00 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 1.07 GC 1.00 HN 1.04 ! LA 1.35 NL 1.04 OV 1.08 SC 1.02 ! WF 1.03 GG 1.00* HH 1.00* KK 1.00* ! KP 1.26 MA 0.72 MC 0.97 MK 0.98 ! NY 1.03 TS 0.85 WZ 1.00* PT 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* GC 1.00* HN 1.00* ! LA 1.00* NL 1.00* OV 1.00* SC 1.00* ! WF 0.89 GG 1.00* HH 1.00* KK 1.25 ! KP 0.92 MA 1.00* MC 1.00* MK 1.00* ! NY 1.00* TS 0.97 WZ 1.00* PT 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 1.00* GC 1.00 HN 1.00* ! LA 1.00* NL 1.00* OV 1.06 SC 1.00* ! WF 1.00* GG 1.00* HH 1.00* KK 1.00* ! KP 1.09 MA 1.00* MC 1.00* MK 1.00* ! NY 1.00* TS 1.00* WZ 1.00* PT 0.99 ! ! ! Correcting IF 3. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.97 GC 0.93 HN 0.98 ! LA 0.98 NL 1.02 OV 0.99 SC 0.89 ! WF 0.83 GG 1.00* HH 1.00* KK 0.97 ! KP 1.05 MA 1.28 MC 0.98 MK 1.00 ! NY 0.91 TS 1.00* WZ 1.00* PT 1.00* ! ! A total of 90 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.87 FD 0.92 GC 1.00* HN 0.98 ! LA 0.82 NL 0.70 OV 0.93 SC 1.10 ! WF 1.12 GG 1.00* HH 1.00* KK 1.00* ! KP 0.99 MA 0.90 MC 1.24 MK 1.12 ! NY 1.00* TS 1.00* WZ 1.00* PT 0.94 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 FD 1.06 GC 1.04 HN 1.02 ! LA 1.32 NL 1.02 OV 1.05 SC 0.99 ! WF 0.70 GG 1.00* HH 1.00* KK 1.00* ! KP 1.14 MA 0.66 MC 1.37 MK 0.95 ! NY 0.99 TS 0.95 WZ 1.00* PT 1.00* ! ! A total of 12 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* GC 1.00* HN 1.00* ! LA 1.00* NL 1.00* OV 1.00* SC 1.00* ! WF 0.91 GG 1.00* HH 1.00* KK 1.24 ! KP 0.70 MA 1.00* MC 1.00* MK 1.00* ! NY 1.00* TS 0.96 WZ 1.00* PT 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.08 FD 1.00* GC 1.00 HN 1.00* ! LA 1.00* NL 1.00* OV 0.98 SC 1.00* ! WF 1.00* GG 1.00* HH 1.00* KK 1.00* ! KP 0.95 MA 1.00* MC 1.00* MK 1.00* ! NY 1.00* TS 1.00* WZ 1.00* PT 1.07 ! ! ! Correcting IF 4. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 1.00 GC 0.92 HN 1.00 ! LA 1.00 NL 1.00 OV 0.94 SC 1.02 ! WF 0.90 GG 1.00* HH 1.00* KK 1.01 ! KP 1.01 MA 1.09 MC 1.16 MK 0.97 ! NY 0.92 TS 1.00* WZ 1.00* PT 1.00* ! ! A total of 69 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 1.03 GC 1.00* HN 1.06 ! LA 0.97 NL 1.03 OV 1.04 SC 1.06 ! WF 1.00 GG 1.00* HH 1.00* KK 1.00* ! KP 0.93 MA 1.05 MC 0.99 MK 1.02 ! NY 1.00* TS 1.00* WZ 1.00* PT 0.98 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 1.09 GC 0.97 HN 1.01 ! LA 1.35 NL 1.03 OV 1.07 SC 0.99 ! WF 0.77 GG 1.00* HH 1.00* KK 1.00* ! KP 1.16 MA 1.06 MC 1.10 MK 1.01 ! NY 1.03 TS 0.71 WZ 1.00* PT 1.00* ! ! A total of 9 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* GC 1.00* HN 1.00* ! LA 1.00* NL 1.00* OV 1.00* SC 1.00* ! WF 0.73 GG 1.00* HH 1.00* KK 1.11 ! KP 1.01 MA 1.00* MC 1.00* MK 1.00* ! NY 1.00* TS 1.03 WZ 1.00* PT 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.06 FD 1.00* GC 1.07 HN 1.00* ! LA 1.00* NL 1.00* OV 0.77 SC 1.00* ! WF 1.00* GG 1.00* HH 1.00* KK 1.00* ! KP 0.94 MA 1.00* MC 1.00* MK 1.00* ! NY 1.00* TS 1.00* WZ 1.00* PT 1.02 ! ! ! Fit before self-cal, rms=0.184995Jy sigma=0.002294 ! Fit after self-cal, rms=0.155428Jy sigma=0.001980 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=2.4 mas, bmaj=3.721 mas, bpa=34.97 degrees ! Estimated noise=432.478 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0031984 Jy ! Component: 100 - total flux cleaned = -0.00383672 Jy ! Total flux subtracted in 100 components = -0.00383672 Jy ! Clean residual min=-0.005482 max=0.004918 Jy/beam ! Clean residual mean=0.000028 rms=0.001344 Jy/beam ! Combined flux in latest and established models = 0.579362 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 9 model components to the UV plane model. ! The established model now contains 60 components and 0.579362 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.155239Jy sigma=0.001978 ! Fit after self-cal, rms=0.155351Jy sigma=0.001977 ! Inverting map dynam = dynam - 1.0 doamp = true solint = solint * (6.0/3.6) 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 doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000214948 Jy ! Component: 100 - total flux cleaned = -0.000388281 Jy ! Total flux subtracted in 100 components = -0.000388281 Jy ! Clean residual min=-0.005552 max=0.004966 Jy/beam ! Clean residual mean=0.000029 rms=0.001341 Jy/beam ! Combined flux in latest and established models = 0.578973 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 14 model components to the UV plane model. ! The established model now contains 68 components and 0.578973 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.155288Jy sigma=0.001977 ! Fit after self-cal, rms=0.151290Jy sigma=0.001876 ! Inverting map and beam ! Estimated beam: bmin=2.412 mas, bmaj=3.73 mas, bpa=35.28 degrees ! Estimated noise=433.352 mJy/beam. doamp = false solint = solint / (6.0/3.6) 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 doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00170317 Jy ! Component: 100 - total flux cleaned = -0.00221519 Jy ! Total flux subtracted in 100 components = -0.00221519 Jy ! Clean residual min=-0.003765 max=0.004324 Jy/beam ! Clean residual mean=0.000034 rms=0.000949 Jy/beam ! Combined flux in latest and established models = 0.576758 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 9 model components to the UV plane model. ! The established model now contains 69 components and 0.576758 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.151139Jy sigma=0.001875 ! Fit after self-cal, rms=0.151202Jy sigma=0.001875 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 1357+769_S ! Writing UV FITS file: 1357+769_S.uvf ! Writing 69 model components to file: 1357+769_S.mod ! wwins: Wrote 3 windows to 1357+769_S.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 2.412 x 3.73 at 35.28 degrees (North through East) ! Clean map min=-0.0035967 max=0.51784 Jy/beam ! Writing clean map to FITS file: 1357+769_S.fits ! Writing difmap environment to: 1357+769_S.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 1357+769_S] device 1357+769_Suv.ps/vps,1,2 ! Attempting to open device: '1357+769_Suv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 1357+769_Sim.ps/vps ! Attempting to open device: '1357+769_Sim.ps/vps' uvweight 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. loglevs -1,2048,2 ! The new contour levels are: ! -1 1 2 4 8 16 32 64 128 256 512 1024 2048 cmul = imstat(rms)*3 ! Inverting map and beam ! Estimated beam: bmin=2.412 mas, bmaj=3.73 mas, bpa=35.28 degrees ! Estimated noise=433.352 mJy/beam. xyrange 0, 0, 0, 0 ! The mapplot display area will be limited to: ! Relative RA: (The whole available range) ! Relative DEC: (The whole available range) mapcolor grey ! Mapplot colormap: grey, contrast: 1 brightness: 0.5. docont=true mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 2.412 x 3.73 at 35.28 degrees (North through East) ! Clean map min=-0.0035967 max=0.51784 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo7-0.4] quit ! Quitting program ! Log file 1357+769_S.log closed on Sun Jul 16 12:07:23 2006