! Started logfile: 0552+398_X.log on Sun Sep 2 11:16:54 2007 observe 0552+398_X.edt ! Reading UV FITS file: 0552+398_X.edt ! AN table 1: 27 integrations on 171 of 171 possible baselines. ! AN table 2: 15 integrations on 171 of 171 possible baselines. ! AN table 3: 63 integrations on 171 of 171 possible baselines. ! Apparent sampling: 0.212587 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 0552+398 ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! ! 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 2125 lines of history. ! ! Reading 15268 visibilities. ![@gonzo7-0.1 0552+398_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 = 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 0.100x0.100 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 230 telescope corrections were flagged in sub-array 1. ! A total of 200 telescope corrections were flagged in sub-array 2. ! A total of 893 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 230 telescope corrections were flagged in sub-array 1. ! A total of 203 telescope corrections were flagged in sub-array 2. ! A total of 893 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 230 telescope corrections were flagged in sub-array 1. ! A total of 206 telescope corrections were flagged in sub-array 2. ! A total of 894 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 230 telescope corrections were flagged in sub-array 1. ! A total of 210 telescope corrections were flagged in sub-array 2. ! A total of 893 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=2.375484Jy sigma=0.040045 ! Fit after self-cal, rms=2.375787Jy sigma=0.040056 ! 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=0.6705 mas, bmaj=2.11 mas, bpa=-1.592 degrees ! Estimated noise=882.439 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 = 2.29753 Jy ! Total flux subtracted in 50 components = 2.29753 Jy ! Clean residual min=-0.194373 max=0.766011 Jy/beam ! Clean residual mean=0.001499 rms=0.069257 Jy/beam ! Combined flux in latest and established models = 2.29753 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 2.29753 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.351780Jy sigma=0.023254 ! Fit after self-cal, rms=1.351819Jy sigma=0.023251 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.836115 Jy ! Total flux subtracted in 50 components = 0.836115 Jy ! Clean residual min=-0.114023 max=0.385994 Jy/beam ! Clean residual mean=0.001016 rms=0.040216 Jy/beam ! Combined flux in latest and established models = 3.13365 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 5 model components to the UV plane model. ! The established model now contains 8 components and 3.13365 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.819672Jy sigma=0.014156 ! Fit after self-cal, rms=0.817099Jy sigma=0.014125 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.435776 Jy ! Total flux subtracted in 50 components = 0.435776 Jy ! Clean residual min=-0.086217 max=0.245081 Jy/beam ! Clean residual mean=0.000763 rms=0.027055 Jy/beam ! Combined flux in latest and established models = 3.56942 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 15 components and 3.56942 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.583097Jy sigma=0.009912 ! Fit after self-cal, rms=0.581701Jy sigma=0.009896 ! Inverting map ! Added new window around map position (-0.9, 0.2). ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.267038 Jy ! Total flux subtracted in 50 components = 0.267038 Jy ! Clean residual min=-0.072066 max=0.132753 Jy/beam ! Clean residual mean=0.000609 rms=0.020222 Jy/beam ! Combined flux in latest and established models = 3.83646 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 23 components and 3.83646 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.458277Jy sigma=0.007643 ! Fit after self-cal, rms=0.455435Jy sigma=0.007608 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.166421 Jy ! Total flux subtracted in 50 components = 0.166421 Jy ! Clean residual min=-0.061727 max=0.094880 Jy/beam ! Clean residual mean=0.000517 rms=0.016739 Jy/beam ! Combined flux in latest and established models = 4.00288 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 25 model components to the UV plane model. ! The established model now contains 43 components and 4.00288 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.390607Jy sigma=0.006414 ! Fit after self-cal, rms=0.389357Jy sigma=0.006397 ! 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=0.7757 mas, bmaj=2.239 mas, bpa=-3.755 degrees ! Estimated noise=444.197 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 = 0.184898 Jy ! Component: 100 - total flux cleaned = 0.304053 Jy ! Total flux subtracted in 100 components = 0.304053 Jy ! Clean residual min=-0.066708 max=0.098834 Jy/beam ! Clean residual mean=0.000641 rms=0.021417 Jy/beam ! Combined flux in latest and established models = 4.30693 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 51 model components to the UV plane model. ! The established model now contains 79 components and 4.30693 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.306301Jy sigma=0.004821 ! Fit after self-cal, rms=0.304423Jy sigma=0.004790 ! 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 0.97 GC 1.00* GG 1.00* ! HN 1.05 KP 0.94 LA 0.95 MA 1.00* ! MK 0.99 NL 1.10 NY 1.00* ON 1.00* ! OV 0.97 PT 0.97 SC 1.01 TC 1.00* ! TS 1.00* WF 1.15 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 FD 0.97 GC 1.07 GG 1.00* ! HN 0.97 KP 0.95 LA 0.97 MA 1.00* ! MK 1.00* NL 1.09 NY 1.00* ON 1.00* ! OV 0.97 PT 0.98 SC 1.03 TC 1.00* ! TS 1.00* WF 1.04 WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 0.96 GC 1.00* GG 1.00* ! HN 0.93 KP 0.94 LA 0.95 MA 1.00* ! MK 0.97 NL 1.09 NY 1.00* ON 1.00* ! OV 0.97 PT 0.98 SC 1.01 TC 1.00* ! TS 1.00* WF 0.97 WZ 1.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 0.97 GC 1.00* GG 1.00* ! HN 1.07 KP 0.90 LA 0.95 MA 1.00* ! MK 0.99 NL 1.06 NY 1.00* ON 1.00* ! OV 0.97 PT 1.02 SC 0.97 TC 1.00* ! TS 1.00* WF 1.21 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 0.97 GC 1.08 GG 1.00* ! HN 0.99 KP 0.90 LA 0.96 MA 1.00* ! MK 1.00* NL 1.06 NY 1.00* ON 1.00* ! OV 0.96 PT 1.02 SC 0.99 TC 1.00* ! TS 1.00* WF 1.09 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 0.97 GC 1.00* GG 1.00* ! HN 0.94 KP 0.90 LA 0.95 MA 1.00* ! MK 0.98 NL 1.05 NY 1.00* ON 1.00* ! OV 0.97 PT 1.02 SC 0.97 TC 1.00* ! TS 1.00* WF 1.00 WZ 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.07 FD 0.97 GC 1.00* GG 1.00* ! HN 1.09 KP 0.84 LA 0.97 MA 1.00* ! MK 1.01 NL 1.05 NY 1.00* ON 1.00* ! OV 1.01 PT 1.06 SC 1.01 TC 1.00* ! TS 1.00* WF 1.33 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 FD 0.98 GC 1.11 GG 1.00* ! HN 1.00 KP 0.84 LA 0.99 MA 1.00* ! MK 1.00* NL 1.05 NY 1.00* ON 1.00* ! OV 1.01 PT 1.06 SC 1.03 TC 1.00* ! TS 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 1.05 FD 0.97 GC 1.00* GG 1.00* ! HN 0.94 KP 0.84 LA 0.97 MA 1.00* ! MK 0.99 NL 1.04 NY 1.00* ON 1.00* ! OV 1.02 PT 1.06 SC 1.01 TC 1.00* ! TS 1.00* WF 1.10 WZ 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 FD 0.96 GC 1.00* GG 1.00* ! HN 1.12 KP 0.90 LA 0.95 MA 1.00* ! MK 1.03 NL 1.07 NY 1.00* ON 1.00* ! OV 1.01 PT 1.07 SC 1.06 TC 1.00* ! TS 1.00* WF 1.37 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 0.96 GC 1.13 GG 1.00* ! HN 1.01 KP 0.91 LA 0.97 MA 1.00* ! MK 1.00* NL 1.06 NY 1.00* ON 1.00* ! OV 1.00 PT 1.06 SC 1.08 TC 1.00* ! TS 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 1.03 FD 0.96 GC 1.00* GG 1.00* ! HN 0.97 KP 0.91 LA 0.96 MA 1.00* ! MK 1.01 NL 1.05 NY 1.00* ON 1.00* ! OV 1.01 PT 1.07 SC 1.06 TC 1.00* ! TS 1.00* WF 1.13 WZ 1.00* ! ! ! Fit before self-cal, rms=0.304423Jy sigma=0.004790 ! Fit after self-cal, rms=0.106964Jy sigma=0.001486 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.7841 mas, bmaj=2.262 mas, bpa=-3.714 degrees ! Estimated noise=438.61 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 (-4, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.014434 Jy ! Component: 100 - total flux cleaned = 0.0125737 Jy ! Total flux subtracted in 100 components = 0.0125737 Jy ! Clean residual min=-0.011174 max=0.008787 Jy/beam ! Clean residual mean=-0.000279 rms=0.001912 Jy/beam ! Combined flux in latest and established models = 4.31951 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 94 components and 4.31951 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.103757Jy sigma=0.001429 ! Fit after self-cal, rms=0.103562Jy sigma=0.001426 ! 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 = -3.66223e-05 Jy ! Component: 100 - total flux cleaned = -0.00172001 Jy ! Total flux subtracted in 100 components = -0.00172001 Jy ! Clean residual min=-0.010397 max=0.007651 Jy/beam ! Clean residual mean=-0.000275 rms=0.001769 Jy/beam ! Combined flux in latest and established models = 4.31779 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 15 model components to the UV plane model. ! The established model now contains 99 components and 4.31779 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.102302Jy sigma=0.001405 ! Fit after self-cal, rms=0.099674Jy sigma=0.001360 ! Inverting map and beam ! Estimated beam: bmin=0.7836 mas, bmaj=2.261 mas, bpa=-3.666 degrees ! Estimated noise=438.573 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 = 0.00438557 Jy ! Component: 100 - total flux cleaned = 0.00275545 Jy ! Total flux subtracted in 100 components = 0.00275545 Jy ! Clean residual min=-0.009156 max=0.006354 Jy/beam ! Clean residual mean=-0.000223 rms=0.001569 Jy/beam ! Combined flux in latest and established models = 4.32054 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 18 model components to the UV plane model. ! The established model now contains 107 components and 4.32054 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.098661Jy sigma=0.001342 ! Fit after self-cal, rms=0.098518Jy sigma=0.001341 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 0552+398_X ! Writing UV FITS file: 0552+398_X.uvf ! Writing 107 model components to file: 0552+398_X.mod ! wwins: Wrote 3 windows to 0552+398_X.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7836 x 2.261 at -3.666 degrees (North through East) ! Clean map min=-0.010531 max=3.0798 Jy/beam ! Writing clean map to FITS file: 0552+398_X.fits ! Writing difmap environment to: 0552+398_X.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 0552+398_X] device 0552+398_Xuv.ps/vps,1,2 ! Attempting to open device: '0552+398_Xuv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 0552+398_Xim.ps/vps ! Attempting to open device: '0552+398_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=0.7836 mas, bmaj=2.261 mas, bpa=-3.666 degrees ! Estimated noise=438.573 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7836 x 2.261 at -3.666 degrees (North through East) ! Clean map min=-0.010531 max=3.0798 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo7-0.1] quit ! Quitting program ! Log file 0552+398_X.log closed on Sun Sep 2 11:17:02 2007