[Fri Jun 8 01:55:57 2012] Detection parameters: Position = (322.3, 234.9) = 10 43 55.68 -59 49 29.3 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 152.7 +/- 25.4 Background counts = 261.6 Rate = 0.007 +/- 0.001 [Fri Jun 8 01:55:57 2012] Off-axis axis estimate = 4.92' [Fri Jun 8 02:01:55 2012] Using EEF radius (= 8.89 ")to estimate initial spatial extent for simple fitting [Fri Jun 8 02:01:55 2012] Initial guess for spatial extent in simple fitting = 8.89" [Fri Jun 8 02:01:55 2012] source mask rpix=2.0, npix_max = 25, mask sum = 24, frac = 0.927 [Fri Jun 8 02:01:55 2012] Giving source the simple spatial ID 178 for pass 0, mean size = 8.89" [Fri Jun 8 14:17:15 2012] Vigneting correction estimate = 1.000000 [Fri Jun 8 14:17:15 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Fri Jun 8 14:17:15 2012] Assessing source extent using major [Fri Jun 8 14:17:15 2012] Source does appear to be extended [Fri Jun 8 14:17:15 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Fri Jun 8 14:18:44 2012] Using EEF radius (= 8.89 ")to estimate initial spatial extent for simple fitting [Fri Jun 8 14:18:44 2012] Initial guess for spatial extent in simple fitting = 8.89" [Fri Jun 8 14:18:44 2012] source mask rpix=2.0, npix_max = 25, mask sum = 24, frac = 0.927 [Fri Jun 8 14:18:44 2012] Giving source the simple spatial ID 142 for pass 1, mean size = 8.89" [Sat Jun 9 02:54:58 2012] Vigneting correction estimate = 1.000000 [Sat Jun 9 02:54:58 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Sat Jun 9 02:54:58 2012] Assessing source extent using major [Sat Jun 9 02:54:58 2012] Source does appear to be extended [Sat Jun 9 02:54:58 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Sat Jun 9 02:55:58 2012] XMMSAS src. selection expression = ellipse(27988.495209, 20385.713943, 652.500000, 652.500000, 0.000000, X, Y) [Sat Jun 9 02:55:58 2012] Writing source region out to fullrun_pn_xmm0112560301_pi300-10000_pass1_cl_src186_src.reg [Sat Jun 9 02:55:58 2012] Extracting stamp from image fullrun_pn_xmm0112560301_pi300-10000_cl_sm2.00.img.gz, (285, 197) - (360, 272) [Sat Jun 9 02:55:58 2012] XMMSAS bgd. selection expression = annulus(27988.495209, 20385.713943, 1087.500000, 2175.000000, X, Y) && !ellipse(29420.140106, 20213.952133, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(28002.098000, 17715.472000, 1621.184047, 1621.184047, 0.000000, X, Y) && !ellipse(30042.664825, 20262.961319, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(30167.408722, 23086.684540, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(30749.911530, 22488.498474, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(30413.248505, 21516.031601, 870.000000, 870.000000, 0.000000, X, Y) [Sat Jun 9 02:55:58 2012] Writing fullrun_pn_xmm0112560301_pi300-10000_pass1_cl_src186.gif [Sat Jun 9 05:43:51 2012] Mean detx,y = (-3221.92, 6947.94) [Sat Jun 9 05:43:54 2012] Setting backscal keywords in source and bgd. spectrum [Sat Jun 9 05:44:16 2012] Binned source spectrum to 10 counts/bin [Sat Jun 9 05:44:16 2012] Setting source spectrum file to fullrun_pn_xmm0112560301_pi300-10000_pass1_cl_src186_src_b10.pi.gz [Sat Jun 9 05:44:16 2012] Setting bgd. spectrum file to fullrun_pn_xmm0112560301_pi300-10000_pass1_cl_src186_bgd.pi.gz [Sat Jun 9 08:50:05 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done [Sat Jun 9 08:50:05 2012] rmf not generated due to insufficient counts [Sat Jun 9 14:20:51 2012] Updating aperture counts using extracted products [Sat Jun 9 14:20:51 2012] Error reading totcts from fullrun_pn_xmm0112560301_pi300-10000_pass1_cl_src186_src_b10.pi.gz [Sat Jun 9 14:20:59 2012] Calculating source flux in energy range 0.30-8.00 [Sat Jun 9 14:20:59 2012] Using photon index=1.80, rate=0.00741, arf fullrun_pn_xmm0112560301_pi300-10000_pass1_cl_src186.arf [Sat Jun 9 14:20:59 2012] Assuming count rate is from the 0.30-10.00 bandpass [Sat Jun 9 14:20:59 2012] Updating source flux to 3.8e-14 [Sat Jun 9 14:39:06 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting