[Mon Apr 30 21:32:35 2012] Detection parameters: Position = (383.8, 274.4) = 16 42 6.07 -54 31 21.9 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 111.8 +/- 17.6 Background counts = 169.7 Rate = 0.003 +/- 0.0005 [Mon Apr 30 21:32:37 2012] Off-axis axis estimate = 6.43' [Mon Apr 30 21:38:49 2012] Using EEF radius (= 9.64 ")to estimate initial spatial extent for simple fitting [Mon Apr 30 21:38:49 2012] Initial guess for spatial extent in simple fitting = 9.64" [Mon Apr 30 21:38:49 2012] source mask rpix=2.2, npix_max = 29, mask sum = 20, frac = 0.678 [Mon Apr 30 21:38:49 2012] Giving source the simple spatial ID 151 for pass 0, mean size = 9.64" [Tue May 1 12:21:37 2012] Vigneting correction estimate = 1.000000 [Tue May 1 12:21:37 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Tue May 1 12:21:37 2012] Assessing source extent using major [Tue May 1 12:21:37 2012] Source does appear to be extended [Tue May 1 12:21:37 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Tue May 1 12:23:13 2012] Using EEF radius (= 9.64 ")to estimate initial spatial extent for simple fitting [Tue May 1 12:23:13 2012] Initial guess for spatial extent in simple fitting = 9.64" [Tue May 1 12:23:13 2012] source mask rpix=2.2, npix_max = 29, mask sum = 20, frac = 0.678 [Tue May 1 12:23:13 2012] Giving source the simple spatial ID 147 for pass 1, mean size = 9.64" [Wed May 2 07:09:59 2012] Vigneting correction estimate = 1.000000 [Wed May 2 07:09:59 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Wed May 2 07:09:59 2012] Assessing source extent using major [Wed May 2 07:09:59 2012] Source does appear to be extended [Wed May 2 07:09:59 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Wed May 2 07:11:42 2012] XMMSAS src. selection expression = ellipse(33338.671295, 23828.457245, 652.500000, 652.500000, 0.000000, X, Y) [Wed May 2 07:11:42 2012] Writing source region out to fullrun_pn_xmm0603220201_pi300-10000_pass1_cl_src156_src.reg [Wed May 2 07:11:42 2012] Extracting stamp from image fullrun_pn_xmm0603220201_pi300-10000_cl_sm2.00.img.gz, (346, 237) - (421, 312) [Wed May 2 07:11:42 2012] XMMSAS bgd. selection expression = annulus(33338.671295, 23828.457245, 1087.500000, 2175.000000, X, Y) && !ellipse(30544.996368, 26707.544464, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(31294.304047, 26699.191742, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(31704.014893, 26647.957642, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(32675.360016, 25536.798676, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(31620.386780, 25473.794830, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(35961.487122, 24041.130402, 870.000000, 870.000000, 0.000000, X, Y) [Wed May 2 07:11:42 2012] Writing fullrun_pn_xmm0603220201_pi300-10000_pass1_cl_src156.gif [Wed May 2 12:12:36 2012] Mean detx,y = (-8453.21, -638.60) [Wed May 2 12:12:46 2012] Setting backscal keywords in source and bgd. spectrum [Wed May 2 12:13:42 2012] Binned source spectrum to 10 counts/bin [Wed May 2 12:13:43 2012] Setting source spectrum file to fullrun_pn_xmm0603220201_pi300-10000_pass1_cl_src156_src_b10.pi.gz [Wed May 2 12:13:43 2012] Setting bgd. spectrum file to fullrun_pn_xmm0603220201_pi300-10000_pass1_cl_src156_bgd.pi.gz [Wed May 2 17:17:31 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done [Wed May 2 17:17:31 2012] rmf not generated due to insufficient counts [Wed May 2 23:18:18 2012] Updating aperture counts using extracted products [Wed May 2 23:18:18 2012] Error reading totcts from fullrun_pn_xmm0603220201_pi300-10000_pass1_cl_src156_src_b10.pi.gz [Wed May 2 23:18:29 2012] Calculating source flux in energy range 0.30-8.00 [Wed May 2 23:18:29 2012] Using photon index=1.80, rate=0.00292, arf fullrun_pn_xmm0603220201_pi300-10000_pass1_cl_src156.arf [Wed May 2 23:18:29 2012] Assuming count rate is from the 0.30-10.00 bandpass [Wed May 2 23:18:29 2012] Updating source flux to 1.4e-14 [Wed May 2 23:36:14 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting