[Wed May 2 11:30:50 2012] Detection parameters: Position = (169.1, 238.2) = 0 16 9.24 -39 17 5.1 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 200.0 +/- 26.0 Background counts = 186.0 Rate = 0.002 +/- 0.0002 [Wed May 2 11:30:51 2012] Off-axis axis estimate = 10.34' [Wed May 2 11:45:01 2012] Using EEF radius (= 11.60 ")to estimate initial spatial extent for simple fitting [Wed May 2 11:45:01 2012] Initial guess for spatial extent in simple fitting = 11.60" [Wed May 2 11:45:01 2012] source mask rpix=2.7, npix_max = 40, mask sum = 36, frac = 0.898 [Wed May 2 11:45:01 2012] Giving source the simple spatial ID 121 for pass 0, mean size = 11.60" [Thu May 3 03:01:57 2012] Vigneting correction estimate = 1.000000 [Thu May 3 03:01:57 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Thu May 3 03:01:57 2012] Assessing source extent using major [Thu May 3 03:01:57 2012] Source does appear to be extended [Thu May 3 03:01:57 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Thu May 3 03:03:17 2012] Using EEF radius (= 11.60 ")to estimate initial spatial extent for simple fitting [Thu May 3 03:03:17 2012] Initial guess for spatial extent in simple fitting = 11.60" [Thu May 3 03:03:17 2012] source mask rpix=2.7, npix_max = 40, mask sum = 36, frac = 0.898 [Thu May 3 03:03:17 2012] Giving source the simple spatial ID 119 for pass 1, mean size = 11.60" [Thu May 3 21:14:46 2012] Vigneting correction estimate = 1.000000 [Thu May 3 21:14:46 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Thu May 3 21:14:46 2012] Assessing source extent using major [Thu May 3 21:14:46 2012] Source does appear to be extended [Thu May 3 21:14:46 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Thu May 3 21:16:18 2012] XMMSAS src. selection expression = ellipse(14666.251160, 20672.800934, 652.500000, 652.500000, 0.000000, X, Y) [Thu May 3 21:16:18 2012] Writing source region out to fullrun_pn_xmm0655050101_pi300-10000_pass1_cl_src123_src.reg [Thu May 3 21:16:18 2012] Extracting stamp from image fullrun_pn_xmm0655050101_pi300-10000_cl_sm2.00.img.gz, (132, 201) - (207, 276) [Thu May 3 21:16:18 2012] XMMSAS bgd. selection expression = annulus(14666.251160, 20672.800934, 1087.500000, 2175.000000, X, Y) && !ellipse(16422.810577, 21512.715469, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(16963.220551, 18242.019394, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(15274.640503, 22728.396301, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(15777.054352, 22423.022797, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(14228.898804, 21220.023712, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(14914.796417, 19961.538498, 870.000000, 870.000000, 0.000000, X, Y) [Thu May 3 21:16:18 2012] Writing fullrun_pn_xmm0655050101_pi300-10000_pass1_cl_src123.gif [Fri May 4 03:37:56 2012] Mean detx,y = (4844.82, -9452.00) [Fri May 4 03:38:08 2012] Setting backscal keywords in source and bgd. spectrum [Fri May 4 03:39:02 2012] Binned source spectrum to 10 counts/bin [Fri May 4 03:39:02 2012] Setting source spectrum file to fullrun_pn_xmm0655050101_pi300-10000_pass1_cl_src123_src_b10.pi.gz [Fri May 4 03:39:02 2012] Setting bgd. spectrum file to fullrun_pn_xmm0655050101_pi300-10000_pass1_cl_src123_bgd.pi.gz [Fri May 4 08:48:43 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done [Fri May 4 08:48:43 2012] rmf not generated due to insufficient counts [Fri May 4 16:21:54 2012] Updating aperture counts using extracted products [Fri May 4 16:21:54 2012] Error reading totcts from fullrun_pn_xmm0655050101_pi300-10000_pass1_cl_src123_src_b10.pi.gz [Fri May 4 16:22:06 2012] Calculating source flux in energy range 0.30-8.00 [Fri May 4 16:22:06 2012] Using photon index=1.80, rate=0.00164, arf fullrun_pn_xmm0655050101_pi300-10000_pass1_cl_src123.arf [Fri May 4 16:22:06 2012] Assuming count rate is from the 0.30-10.00 bandpass [Fri May 4 16:22:06 2012] Updating source flux to 7.5e-15 [Fri May 4 16:33:30 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting