[Sat Nov 26 22:29:34 2011] Detection parameters: Position = (387.6, 270.2) = 5 34 8.67 21 57 26.2 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 120.8 +/- 19.4 Background counts = 213.3 Rate = 0.02 +/- 0.003 [Sat Nov 26 22:29:35 2011] Off-axis axis estimate = 6.78' [Sun Nov 27 09:34:36 2011] Using EEF radius (= 9.82 ")to estimate initial spatial extent for simple fitting [Sun Nov 27 09:34:36 2011] Initial guess for spatial extent in simple fitting = 9.82" [Sun Nov 27 09:34:36 2011] source mask rpix=2.3, npix_max = 30, mask sum = 6, frac = 0.197 [Sun Nov 27 09:34:36 2011] Skipping simple spatial due to low active detector fraction [Sun Nov 27 22:38:56 2011] Vigneting correction estimate = 1.000000 [Sun Nov 27 22:38:56 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Sun Nov 27 22:38:56 2011] Assessing source extent using major [Sun Nov 27 22:38:56 2011] Source does appear to be extended [Sun Nov 27 22:38:56 2011] Computing asymmetry using major and minor axis, asym = 1.00 [Sun Nov 27 22:38:56 2011] Source is confused with source 94 [Mon Nov 28 13:20:41 2011] Using EEF radius (= 9.82 ")to estimate initial spatial extent for simple fitting [Mon Nov 28 13:20:41 2011] Initial guess for spatial extent in simple fitting = 9.82" [Mon Nov 28 13:20:41 2011] source mask rpix=2.3, npix_max = 30, mask sum = 6, frac = 0.197 [Mon Nov 28 13:20:41 2011] Skipping simple spatial due to low active detector fraction [Tue Nov 29 05:36:53 2011] Vigneting correction estimate = 1.000000 [Tue Nov 29 05:36:53 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Tue Nov 29 05:36:53 2011] Assessing source extent using major [Tue Nov 29 05:36:53 2011] Source does appear to be extended [Tue Nov 29 05:36:53 2011] Computing asymmetry using major and minor axis, asym = 1.00 [Tue Nov 29 09:11:44 2011] XMMSAS src. selection expression = ellipse(33668.619751, 23456.575256, 652.500000, 652.500000, 0.000000, X, Y) [Tue Nov 29 09:11:44 2011] Writing source region out to fullrun_mos2_xmm0412590601_pi300-10000_pass1_cl_src95_src.reg [Tue Nov 29 09:11:44 2011] Extracting stamp from image fullrun_mos2_xmm0412590601_pi300-10000_cl_sm2.00.img.gz, (350, 233) - (425, 308) [Tue Nov 29 09:11:44 2011] XMMSAS bgd. selection expression = annulus(33668.619751, 23456.575256, 1087.500000, 2175.000000, X, Y) && !ellipse(33751.000000, 24380.591827, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(34100.696564, 24917.600708, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(34530.844000, 27147.532800, 1645.024047, 1645.024047, 0.000000, X, Y) && !ellipse(33909.638000, 23805.371765, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(33667.024078, 22423.110413, 870.000000, 870.000000, 0.000000, X, Y) [Tue Nov 29 09:11:44 2011] Writing fullrun_mos2_xmm0412590601_pi300-10000_pass1_cl_src95.gif [Tue Nov 29 10:53:32 2011] Mean detx,y = (-6923.92, -3668.44) [Tue Nov 29 10:53:34 2011] Setting backscal keywords in source and bgd. spectrum [Tue Nov 29 10:53:55 2011] Binned source spectrum to 10 counts/bin [Tue Nov 29 10:53:55 2011] Setting source spectrum file to fullrun_mos2_xmm0412590601_pi300-10000_pass1_cl_src95_src_b10.pi.gz [Tue Nov 29 10:53:55 2011] Setting bgd. spectrum file to fullrun_mos2_xmm0412590601_pi300-10000_pass1_cl_src95_bgd.pi.gz [Tue Nov 29 14:55:38 2011] Not generating rmf since RequireSpatial is true but spatial fitting not done [Tue Nov 29 14:55:38 2011] rmf not generated due to insufficient counts [Tue Nov 29 15:09:07 2011] Updating aperture counts using extracted products [Tue Nov 29 15:09:07 2011] Error reading totcts from fullrun_mos2_xmm0412590601_pi300-10000_pass1_cl_src95_src_b10.pi.gz [Tue Nov 29 15:09:11 2011] Calculating source flux in energy range 0.30-8.00 [Tue Nov 29 15:09:11 2011] Using photon index=1.80, rate=0.021, arf fullrun_mos2_xmm0412590601_pi300-10000_pass1_cl_src95.arf [Tue Nov 29 15:09:11 2011] Assuming count rate is from the 0.30-10.00 bandpass [Tue Nov 29 15:09:11 2011] Getting flux using calc_pl_flux failed [Tue Nov 29 15:19:21 2011] Simple spatial fitting not done (or not done successfully), skipping spectral fitting