[Sun Mar 18 10:51:30 2012] Detection parameters: Position = (328.2, 311.5) = 7 8 38.79 -49 32 9.8 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 205.4 +/- 32.1 Background counts = 222.0 Rate = 0.003 +/- 0.0005 [Sun Mar 18 10:51:32 2012] Off-axis axis estimate = 2.36' [Sun Mar 18 11:02:36 2012] Using EEF radius (= 7.61 ")to estimate initial spatial extent for simple fitting [Sun Mar 18 11:02:36 2012] Initial guess for spatial extent in simple fitting = 7.61" [Sun Mar 18 11:02:36 2012] source mask rpix=1.7, npix_max = 20, mask sum = 7, frac = 0.346 [Sun Mar 18 11:02:36 2012] Skipping simple spatial due to low active detector fraction [Sun Mar 18 15:01:57 2012] Vigneting correction estimate = 1.000000 [Sun Mar 18 15:01:57 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Sun Mar 18 15:01:57 2012] Assessing source extent using major [Sun Mar 18 15:01:57 2012] Source does appear to be extended [Sun Mar 18 15:01:57 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Sun Mar 18 15:02:28 2012] Using EEF radius (= 7.61 ")to estimate initial spatial extent for simple fitting [Sun Mar 18 15:02:28 2012] Initial guess for spatial extent in simple fitting = 7.61" [Sun Mar 18 15:02:28 2012] source mask rpix=1.7, npix_max = 20, mask sum = 7, frac = 0.346 [Sun Mar 18 15:02:28 2012] Skipping simple spatial due to low active detector fraction [Sun Mar 18 21:47:51 2012] Vigneting correction estimate = 1.000000 [Sun Mar 18 21:47:51 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Sun Mar 18 21:47:51 2012] Assessing source extent using major [Sun Mar 18 21:47:51 2012] Source does appear to be extended [Sun Mar 18 21:47:51 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Sun Mar 18 21:48:21 2012] XMMSAS src. selection expression = ellipse(28503.597443, 27051.692017, 652.500000, 652.500000, 0.000000, X, Y) [Sun Mar 18 21:48:21 2012] Writing source region out to fullrun_pn_xmm0511580401_pi300-10000_pass1_cl_src29_src.reg [Sun Mar 18 21:48:21 2012] Extracting stamp from image fullrun_pn_xmm0511580401_pi300-10000_cl_sm2.00.img.gz, (291, 274) - (366, 349) [Sun Mar 18 21:48:21 2012] XMMSAS bgd. selection expression = annulus(28503.597443, 27051.692017, 1087.500000, 2175.000000, X, Y) && !ellipse(28000.192600, 25795.570200, 1534.132844, 1534.132844, 0.000000, X, Y) && !ellipse(31347.489594, 27937.656708, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(28035.831726, 27921.856628, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(29006.290070, 26614.589233, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(31212.218506, 26595.674805, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(29594.779968, 25747.382324, 870.000000, 870.000000, 0.000000, X, Y) [Sun Mar 18 21:48:21 2012] Writing fullrun_pn_xmm0511580401_pi300-10000_pass1_cl_src29.gif [Sun Mar 18 22:51:51 2012] Mean detx,y = (-545.87, -1181.35) [Sun Mar 18 22:52:09 2012] Setting backscal keywords in source and bgd. spectrum [Sun Mar 18 22:52:54 2012] Binned source spectrum to 10 counts/bin [Sun Mar 18 22:52:54 2012] Setting source spectrum file to fullrun_pn_xmm0511580401_pi300-10000_pass1_cl_src29_src_b10.pi.gz [Sun Mar 18 22:52:54 2012] Setting bgd. spectrum file to fullrun_pn_xmm0511580401_pi300-10000_pass1_cl_src29_bgd.pi.gz [Mon Mar 19 00:32:35 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done [Mon Mar 19 00:32:35 2012] rmf not generated due to insufficient counts [Mon Mar 19 02:39:16 2012] Updating aperture counts using extracted products [Mon Mar 19 02:39:16 2012] Error reading totcts from fullrun_pn_xmm0511580401_pi300-10000_pass1_cl_src29_src_b10.pi.gz [Mon Mar 19 02:39:18 2012] Calculating source flux in energy range 0.30-8.00 [Mon Mar 19 02:39:18 2012] Using photon index=1.80, rate=0.00338, arf fullrun_pn_xmm0511580401_pi300-10000_pass1_cl_src29.arf [Mon Mar 19 02:39:18 2012] Assuming count rate is from the 0.30-10.00 bandpass [Mon Mar 19 02:39:18 2012] Updating source flux to 1.2e-14 [Mon Mar 19 02:41:04 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting