[Mon May 21 22:38:49 2012] Detection parameters: Position = (281.8, 367.4) = 8 42 5.19 -52 53 58.6 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 621.8 +/- 97.2 Background counts = 130.6 Rate = 0.02 +/- 0.002 [Mon May 21 22:38:51 2012] Off-axis axis estimate = 5.14' [Mon May 21 22:44:45 2012] Using EEF radius (= 9.00 ")to estimate initial spatial extent for simple fitting [Mon May 21 22:44:45 2012] Initial guess for spatial extent in simple fitting = 9.00" [Mon May 21 22:44:45 2012] source mask rpix=2.1, npix_max = 26, mask sum = 4, frac = 0.152 [Mon May 21 22:44:45 2012] Skipping simple spatial due to low active detector fraction [Tue May 22 03:15:26 2012] Vigneting correction estimate = 1.000000 [Tue May 22 03:15:26 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Tue May 22 03:15:26 2012] Assessing source extent using major [Tue May 22 03:15:26 2012] Source does appear to be extended [Tue May 22 03:15:26 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Tue May 22 03:16:03 2012] Using EEF radius (= 9.00 ")to estimate initial spatial extent for simple fitting [Tue May 22 03:16:03 2012] Initial guess for spatial extent in simple fitting = 9.00" [Tue May 22 03:16:03 2012] source mask rpix=2.1, npix_max = 26, mask sum = 4, frac = 0.152 [Tue May 22 03:16:03 2012] Skipping simple spatial due to low active detector fraction [Tue May 22 07:01:31 2012] Vigneting correction estimate = 1.000000 [Tue May 22 07:01:31 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Tue May 22 07:01:31 2012] Assessing source extent using major [Tue May 22 07:01:31 2012] Source does appear to be extended [Tue May 22 07:01:31 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Tue May 22 07:02:05 2012] XMMSAS src. selection expression = ellipse(24467.886536, 31912.546204, 652.500000, 652.500000, 0.000000, X, Y) [Tue May 22 07:02:05 2012] Writing source region out to fullrun_pn_xmm0112420101_pi300-10000_pass1_cl_src6_src.reg [Tue May 22 07:02:05 2012] Extracting stamp from image fullrun_pn_xmm0112420101_pi300-10000_cl_sm2.00.img.gz, (244, 330) - (319, 405) [Tue May 22 07:02:05 2012] XMMSAS bgd. selection expression = annulus(24467.886536, 31912.546204, 1087.500000, 2175.000000, X, Y) && !ellipse(22736.804720, 29352.560200, 478.094414, 419.425612, 348.546332, X, Y) && !ellipse(25813.394318, 33940.245178, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27438.861664, 30214.471771, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25774.317596, 34665.033661, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25239.549561, 34598.458801, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22000.027800, 34326.744400, 402.230412, 402.230412, 0.000000, X, Y) [Tue May 22 07:02:05 2012] Writing fullrun_pn_xmm0112420101_pi300-10000_pass1_cl_src6.gif [Tue May 22 07:12:14 2012] Mean detx,y = (-2204.78, 7519.25) [Tue May 22 07:12:18 2012] Setting backscal keywords in source and bgd. spectrum [Tue May 22 07:12:46 2012] Binned source spectrum to 10 counts/bin [Tue May 22 07:12:47 2012] Setting source spectrum file to fullrun_pn_xmm0112420101_pi300-10000_pass1_cl_src6_src_b10.pi.gz [Tue May 22 07:12:47 2012] Setting bgd. spectrum file to fullrun_pn_xmm0112420101_pi300-10000_pass1_cl_src6_bgd.pi.gz [Tue May 22 08:15:35 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done [Tue May 22 08:15:35 2012] rmf not generated due to insufficient counts [Tue May 22 11:06:47 2012] Updating aperture counts using extracted products [Tue May 22 11:06:47 2012] Error reading totcts from fullrun_pn_xmm0112420101_pi300-10000_pass1_cl_src6_src_b10.pi.gz [Tue May 22 11:06:52 2012] Calculating source flux in energy range 0.30-8.00 [Tue May 22 11:06:52 2012] Using photon index=1.80, rate=0.015, arf fullrun_pn_xmm0112420101_pi300-10000_pass1_cl_src6.arf [Tue May 22 11:06:52 2012] Assuming count rate is from the 0.30-10.00 bandpass [Tue May 22 11:06:52 2012] Getting flux using calc_pl_flux failed [Tue May 22 11:14:05 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting