! Started logfile: 0229+131_X.log on Thu Feb 14 23:56:07 2008 observe 0229+131_X.edt ! Reading UV FITS file: 0229+131_X.edt ! AN table 1: 38 integrations on 136 of 136 possible baselines. ! AN table 2: 14 integrations on 136 of 136 possible baselines. ! AN table 3: 7 integrations on 136 of 136 possible baselines. ! Apparent sampling: 0.126869 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 0229+131 ! ! There are 4 IFs, and a total of 4 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.40997e+09 8e+06 1 8e+06 ! 02 2 8.47997e+09 8e+06 1 8e+06 ! 03 3 8.79497e+09 8e+06 1 8e+06 ! 04 4 8.89997e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 1222 lines of history. ! ! Reading 4072 visibilities. ![@gonzo8-0.1 0229+131_X] print "***********************************" ! *********************************** print "*** Using gonzo instruction set ***" ! *** Using gonzo instruction set *** print "***********************************" ! *********************************** float field_size field_size = 1024 float field_cell field_cell = 0.1 integer clean_niter clean_niter = 50 float clean_gain clean_gain = 0.03 float dynam dynam = 8.0 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 0.100x0.100 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 438 telescope corrections were flagged in sub-array 1. ! A total of 186 telescope corrections were flagged in sub-array 2. ! A total of 86 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 440 telescope corrections were flagged in sub-array 1. ! A total of 185 telescope corrections were flagged in sub-array 2. ! A total of 85 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 440 telescope corrections were flagged in sub-array 1. ! A total of 186 telescope corrections were flagged in sub-array 2. ! A total of 85 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 444 telescope corrections were flagged in sub-array 1. ! A total of 187 telescope corrections were flagged in sub-array 2. ! A total of 89 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=0.239170Jy sigma=0.003656 ! Fit after self-cal, rms=0.238218Jy sigma=0.003648 ! 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=0.8074 mas, bmaj=1.698 mas, bpa=-11.79 degrees ! Estimated noise=1761.86 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 = 0.62453 Jy ! Total flux subtracted in 50 components = 0.62453 Jy ! Clean residual min=-0.042178 max=0.180041 Jy/beam ! Clean residual mean=-0.001168 rms=0.017812 Jy/beam ! Combined flux in latest and established models = 0.62453 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.62453 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.255172Jy sigma=0.004752 ! Fit after self-cal, rms=0.255175Jy sigma=0.004752 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.179152 Jy ! Total flux subtracted in 50 components = 0.179152 Jy ! Clean residual min=-0.021861 max=0.074479 Jy/beam ! Clean residual mean=-0.000568 rms=0.008142 Jy/beam ! Combined flux in latest and established models = 0.803682 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 6 model components to the UV plane model. ! The established model now contains 9 components and 0.803682 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.130065Jy sigma=0.002373 ! Fit after self-cal, rms=0.130054Jy sigma=0.002373 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0760618 Jy ! Total flux subtracted in 50 components = 0.0760618 Jy ! Clean residual min=-0.013980 max=0.033480 Jy/beam ! Clean residual mean=-0.000315 rms=0.004553 Jy/beam ! Combined flux in latest and established models = 0.879744 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 14 model components to the UV plane model. ! The established model now contains 20 components and 0.879744 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.091616Jy sigma=0.001548 ! Fit after self-cal, rms=0.091555Jy sigma=0.001547 ! 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=0.9884 mas, bmaj=1.914 mas, bpa=-19.98 degrees ! Estimated noise=788.52 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 = 0.0448473 Jy ! Component: 100 - total flux cleaned = 0.0686102 Jy ! Total flux subtracted in 100 components = 0.0686102 Jy ! Clean residual min=-0.008116 max=0.013628 Jy/beam ! Clean residual mean=-0.000100 rms=0.002840 Jy/beam ! Combined flux in latest and established models = 0.948354 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 42 model components to the UV plane model. ! The established model now contains 60 components and 0.948354 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.073334Jy sigma=0.001100 ! Fit after self-cal, rms=0.072999Jy sigma=0.001097 ! Inverting map print "****************************************" ! **************************************** print "*** Finished Natural Weighting CLEAN ***" ! *** Finished Natural Weighting CLEAN *** print "****************************************" ! **************************************** gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 1.00* GC 1.03 HN 1.00* ! KK 1.00 KP 0.99 LA 1.00* MC 1.00* ! MK 1.00 NL 1.00 NY 1.00* ON 1.00* ! OV 0.99 PT 0.99 SC 1.04 WF 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.99 GC 1.00* HN 1.01 ! KK 1.00 KP 0.99 LA 0.98 MC 1.00* ! MK 1.00* NL 1.00 NY 1.00* ON 1.00* ! OV 0.99 PT 0.98 SC 1.00* WF 1.00 ! WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 0.98 GC 1.00* HN 1.00* ! KK 1.00* KP 0.99 LA 0.99 MC 1.00* ! MK 1.00* NL 1.00* NY 1.00* ON 1.00* ! OV 1.00 PT 0.99 SC 1.00* WF 1.00* ! WZ 1.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 1.00* GC 1.03 HN 1.00* ! KK 1.00 KP 0.99 LA 1.00* MC 1.00* ! MK 1.00 NL 1.01 NY 1.00* ON 1.00* ! OV 0.99 PT 0.98 SC 1.03 WF 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.98 GC 1.00* HN 1.01 ! KK 1.01 KP 0.99 LA 0.99 MC 1.00* ! MK 1.00* NL 1.01 NY 1.00* ON 1.00* ! OV 0.99 PT 0.99 SC 1.00* WF 1.01 ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 0.99 GC 1.00* HN 1.00* ! KK 1.00* KP 0.99 LA 0.99 MC 1.00* ! MK 1.00* NL 1.00* NY 1.00* ON 1.00* ! OV 1.00 PT 0.98 SC 1.00* WF 1.00* ! WZ 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 1.00* GC 1.04 HN 1.00* ! KK 1.00 KP 0.99 LA 1.00* MC 1.00* ! MK 1.00 NL 0.96 NY 1.00* ON 1.00* ! OV 0.99 PT 0.99 SC 0.99 WF 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 0.98 GC 1.00* HN 1.01 ! KK 1.00 KP 1.00 LA 0.99 MC 1.00* ! MK 1.00* NL 1.00 NY 1.00* ON 1.00* ! OV 0.98 PT 0.99 SC 1.00* WF 1.01 ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 0.99 GC 1.00* HN 1.00* ! KK 1.00* KP 0.98 LA 0.98 MC 1.00* ! MK 1.00* NL 1.00* NY 1.00* ON 1.00* ! OV 0.99 PT 0.99 SC 1.00* WF 1.00* ! WZ 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 1.00* GC 1.03 HN 1.00* ! KK 1.00 KP 0.99 LA 1.00* MC 1.00* ! MK 1.00 NL 1.02 NY 1.00* ON 1.00* ! OV 0.99 PT 0.99 SC 1.03 WF 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 0.99 GC 1.00* HN 0.99 ! KK 0.99 KP 0.99 LA 0.99 MC 1.00* ! MK 1.00* NL 1.02 NY 1.00* ON 1.00* ! OV 0.99 PT 0.98 SC 1.00* WF 1.03 ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 0.99 GC 1.00* HN 1.00* ! KK 1.00* KP 0.98 LA 0.99 MC 1.00* ! MK 1.00* NL 1.00* NY 1.00* ON 1.00* ! OV 0.99 PT 0.99 SC 1.00* WF 1.00* ! WZ 1.00* ! ! ! Fit before self-cal, rms=0.072999Jy sigma=0.001097 ! Fit after self-cal, rms=0.071232Jy sigma=0.001053 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.99 mas, bmaj=1.932 mas, bpa=-19.84 degrees ! Estimated noise=779.594 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 = 0.00583751 Jy ! Component: 100 - total flux cleaned = 0.00614035 Jy ! Total flux subtracted in 100 components = 0.00614035 Jy ! Clean residual min=-0.005340 max=0.010701 Jy/beam ! Clean residual mean=0.000008 rms=0.001740 Jy/beam ! Combined flux in latest and established models = 0.954494 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 7 model components to the UV plane model. ! The established model now contains 66 components and 0.954494 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070780Jy sigma=0.001044 ! Fit after self-cal, rms=0.070697Jy sigma=0.001044 ! 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) ! Added new window around map position (5, 3.9). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00879795 Jy ! Component: 100 - total flux cleaned = 0.0118734 Jy ! Total flux subtracted in 100 components = 0.0118734 Jy ! Clean residual min=-0.004273 max=0.004210 Jy/beam ! Clean residual mean=0.000010 rms=0.001139 Jy/beam ! Combined flux in latest and established models = 0.966367 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 27 model components to the UV plane model. ! The established model now contains 93 components and 0.966368 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.069801Jy sigma=0.001024 ! Fit after self-cal, rms=0.069320Jy sigma=0.001017 ! Inverting map and beam ! Estimated beam: bmin=0.9885 mas, bmaj=1.932 mas, bpa=-19.87 degrees ! Estimated noise=778.898 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 = 0.00278514 Jy ! Component: 100 - total flux cleaned = 0.00372622 Jy ! Total flux subtracted in 100 components = 0.00372622 Jy ! Clean residual min=-0.004314 max=0.004022 Jy/beam ! Clean residual mean=0.000002 rms=0.000991 Jy/beam ! Combined flux in latest and established models = 0.970094 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 20 model components to the UV plane model. ! The established model now contains 105 components and 0.970094 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.069171Jy sigma=0.001015 ! Fit after self-cal, rms=0.069160Jy sigma=0.001014 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 0229+131_X ! Writing UV FITS file: 0229+131_X.uvf ! Writing 105 model components to file: 0229+131_X.mod ! wwins: Wrote 2 windows to 0229+131_X.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9885 x 1.932 at -19.87 degrees (North through East) ! Clean map min=-0.0040893 max=0.81488 Jy/beam ! Writing clean map to FITS file: 0229+131_X.fits ! Writing difmap environment to: 0229+131_X.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 0229+131_X] device 0229+131_Xuv.ps/vps,1,2 ! Attempting to open device: '0229+131_Xuv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 0229+131_Xim.ps/vps ! Attempting to open device: '0229+131_Xim.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=0.9885 mas, bmaj=1.932 mas, bpa=-19.87 degrees ! Estimated noise=778.898 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9885 x 1.932 at -19.87 degrees (North through East) ! Clean map min=-0.0040893 max=0.81488 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo8-0.1] quit ! Quitting program ! Log file 0229+131_X.log closed on Thu Feb 14 23:56:12 2008