! Started logfile: 0119+041_X.log on Tue Jul 25 10:36:24 2006 observe 0119+041_X.edt ! Reading UV FITS file: 0119+041_X.edt ! AN table 1: 17 integrations on 190 of 190 possible baselines. ! AN table 2: 34 integrations on 190 of 190 possible baselines. ! Apparent sampling: 0.156244 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 0119+041 ! ! 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 1409 lines of history. ! ! Reading 6056 visibilities. ![@gonzo8-0.1 0119+041_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 232 telescope corrections were flagged in sub-array 1. ! A total of 556 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 2. ! A total of 241 telescope corrections were flagged in sub-array 1. ! A total of 556 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 3. ! A total of 233 telescope corrections were flagged in sub-array 1. ! A total of 567 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 4. ! A total of 237 telescope corrections were flagged in sub-array 1. ! A total of 557 telescope corrections were flagged in sub-array 2. ! ! Fit before self-cal, rms=0.354593Jy sigma=0.005031 ! Fit after self-cal, rms=0.344190Jy sigma=0.004940 ! 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=0.8572 mas, bmaj=1.494 mas, bpa=-5.009 degrees ! Estimated noise=1497.95 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 = 0.544649 Jy ! Total flux subtracted in 50 components = 0.544649 Jy ! Clean residual min=-0.048623 max=0.206089 Jy/beam ! Clean residual mean=-0.000324 rms=0.018143 Jy/beam ! Combined flux in latest and established models = 0.544649 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 0.544649 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.369812Jy sigma=0.006228 ! Fit after self-cal, rms=0.369805Jy sigma=0.006228 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.225756 Jy ! Total flux subtracted in 50 components = 0.225756 Jy ! Clean residual min=-0.025203 max=0.103456 Jy/beam ! Clean residual mean=-0.000158 rms=0.009998 Jy/beam ! Combined flux in latest and established models = 0.770406 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 12 components and 0.770406 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.214511Jy sigma=0.003563 ! Fit after self-cal, rms=0.214492Jy sigma=0.003563 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.114597 Jy ! Total flux subtracted in 50 components = 0.114597 Jy ! Clean residual min=-0.019217 max=0.054649 Jy/beam ! Clean residual mean=-0.000074 rms=0.006253 Jy/beam ! Combined flux in latest and established models = 0.885002 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 0.885002 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.146638Jy sigma=0.002357 ! Fit after self-cal, rms=0.146631Jy sigma=0.002357 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0638112 Jy ! Total flux subtracted in 50 components = 0.0638112 Jy ! Clean residual min=-0.015874 max=0.034947 Jy/beam ! Clean residual mean=-0.000027 rms=0.004503 Jy/beam ! Combined flux in latest and established models = 0.948813 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 17 model components to the UV plane model. ! The established model now contains 33 components and 0.948813 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.117284Jy sigma=0.001814 ! Fit after self-cal, rms=0.117280Jy sigma=0.001813 ! 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=1.044 mas, bmaj=2.132 mas, bpa=-17.98 degrees ! Estimated noise=849.403 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 = 0.0533903 Jy ! Component: 100 - total flux cleaned = 0.0800702 Jy ! Total flux subtracted in 100 components = 0.0800702 Jy ! Clean residual min=-0.009346 max=0.014963 Jy/beam ! Clean residual mean=0.000031 rms=0.002741 Jy/beam ! Combined flux in latest and established models = 1.02888 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 39 model components to the UV plane model. ! The established model now contains 65 components and 1.02888 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.095942Jy sigma=0.001403 ! Fit after self-cal, rms=0.095921Jy sigma=0.001403 ! 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 0.98 FD 0.99 GC 1.07 HN 0.98 ! LA 1.01 NL 0.93 OV 0.96 SC 0.92 ! WF 0.97 GG 1.00* HH 1.00* KK 0.99 ! KP 1.00 MA 1.00* MC 1.00* MK 1.02 ! NY 1.00* TS 1.00* WZ 1.00* PT 1.00 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 1.01 GC 1.08 HN 1.00* ! LA 0.98 NL 0.98 OV 1.02 SC 1.00* ! WF 1.00* GG 1.00* HH 1.00* KK 0.99 ! KP 0.99 MA 1.00* MC 1.00* MK 1.03 ! NY 1.00* TS 1.00* WZ 1.00* PT 1.01 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.97 GC 1.10 HN 1.02 ! LA 1.00 NL 0.91 OV 0.97 SC 1.61 ! WF 1.00 GG 1.00* HH 1.00* KK 1.06 ! KP 0.96 MA 1.00* MC 1.00* MK 1.01 ! NY 1.00* TS 1.00* WZ 1.00* PT 1.01 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 1.01 GC 1.01 HN 1.00* ! LA 0.98 NL 1.03 OV 1.02 SC 1.00* ! WF 1.00* GG 1.00* HH 1.00* KK 1.01 ! KP 0.96 MA 1.00* MC 1.00* MK 1.00 ! NY 1.00* TS 1.00* WZ 1.00* PT 1.01 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.97 GC 1.10 HN 1.05 ! LA 1.00 NL 0.90 OV 0.94 SC 0.93 ! WF 0.97 GG 1.00* HH 1.00* KK 1.02 ! KP 0.96 MA 1.00* MC 1.00* MK 1.05 ! NY 1.00* TS 1.00* WZ 1.00* PT 1.04 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 1.02 GC 1.06 HN 1.00* ! LA 1.00* NL 1.00 OV 1.00 SC 1.00* ! WF 1.00* GG 1.00* HH 1.00* KK 0.99 ! KP 0.96 MA 1.00* MC 1.00* MK 0.97 ! NY 1.00* TS 1.00* WZ 1.00* PT 1.01 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.96 GC 1.19 HN 1.01 ! LA 0.96 NL 0.93 OV 0.96 SC 0.92 ! WF 1.06 GG 1.00* HH 1.00* KK 1.01 ! KP 0.97 MA 1.00* MC 1.00* MK 1.09 ! NY 1.00* TS 1.00* WZ 1.00* PT 1.02 ! ! A total of 15 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 1.02 GC 1.02 HN 1.00* ! LA 0.99 NL 0.98 OV 1.04 SC 1.00* ! WF 1.00* GG 1.00* HH 1.00* KK 0.95 ! KP 0.95 MA 1.00* MC 1.00* MK 1.00 ! NY 1.00* TS 1.00* WZ 1.00* PT 1.01 ! ! ! Fit before self-cal, rms=0.095921Jy sigma=0.001403 ! Fit after self-cal, rms=0.085366Jy sigma=0.001227 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=1.052 mas, bmaj=2.156 mas, bpa=-17.54 degrees ! Estimated noise=847.134 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 = 0.00228588 Jy ! Component: 100 - total flux cleaned = 0.00271988 Jy ! Total flux subtracted in 100 components = 0.00271988 Jy ! Clean residual min=-0.004420 max=0.007884 Jy/beam ! Clean residual mean=0.000098 rms=0.001377 Jy/beam ! Combined flux in latest and established models = 1.0316 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 15 model components to the UV plane model. ! The established model now contains 73 components and 1.0316 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.085188Jy sigma=0.001224 ! Fit after self-cal, rms=0.085190Jy sigma=0.001223 ! 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 = 0.000489585 Jy ! Component: 100 - total flux cleaned = 0.000812964 Jy ! Total flux subtracted in 100 components = 0.000812964 Jy ! Clean residual min=-0.004417 max=0.007329 Jy/beam ! Clean residual mean=0.000098 rms=0.001358 Jy/beam ! Combined flux in latest and established models = 1.03242 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 13 model components to the UV plane model. ! The established model now contains 80 components and 1.03242 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.085123Jy sigma=0.001222 ! Fit after self-cal, rms=0.082190Jy sigma=0.001187 ! Inverting map and beam ! Estimated beam: bmin=1.051 mas, bmaj=2.155 mas, bpa=-17.57 degrees ! Estimated noise=847.312 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) ! Added new window around map position (1.4, -0.9). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00619627 Jy ! Component: 100 - total flux cleaned = 0.00689566 Jy ! Total flux subtracted in 100 components = 0.00689566 Jy ! Clean residual min=-0.003469 max=0.004596 Jy/beam ! Clean residual mean=0.000061 rms=0.001062 Jy/beam ! Combined flux in latest and established models = 1.03931 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 12 model components to the UV plane model. ! The established model now contains 92 components and 1.03931 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081733Jy sigma=0.001179 ! Fit after self-cal, rms=0.081690Jy sigma=0.001178 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 0119+041_X ! Writing UV FITS file: 0119+041_X.uvf ! Writing 92 model components to file: 0119+041_X.mod ! wwins: Wrote 2 windows to 0119+041_X.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.051 x 2.155 at -17.57 degrees (North through East) ! Clean map min=-0.0036173 max=0.78335 Jy/beam ! Writing clean map to FITS file: 0119+041_X.fits ! Writing difmap environment to: 0119+041_X.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 0119+041_X] device 0119+041_Xuv.ps/vps,1,2 ! Attempting to open device: '0119+041_Xuv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 0119+041_Xim.ps/vps ! Attempting to open device: '0119+041_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=1.051 mas, bmaj=2.155 mas, bpa=-17.57 degrees ! Estimated noise=847.312 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.051 x 2.155 at -17.57 degrees (North through East) ! Clean map min=-0.0036173 max=0.78335 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo8-0.1] quit ! Quitting program ! Log file 0119+041_X.log closed on Tue Jul 25 10:36:40 2006