[Fri Apr 6 15:44:43 2012] Detection parameters: Position = (420.3, 236.0) = 8 9 9.72 -49 18 31.3 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 316.1 +/- 28.6 Background counts = 176.6 Rate = 0.003 +/- 0.0002 [Fri Apr 6 15:44:44 2012] Off-axis axis estimate = 9.93' [Fri Apr 6 15:51:49 2012] Using EEF radius (= 11.39 ")to estimate initial spatial extent for simple fitting [Fri Apr 6 15:51:49 2012] Initial guess for spatial extent in simple fitting = 11.39" [Fri Apr 6 15:51:49 2012] source mask rpix=2.6, npix_max = 38, mask sum = 36, frac = 0.925 [Fri Apr 6 15:51:49 2012] Giving source the simple spatial ID 115 for pass 0, mean size = 11.39" [Fri Apr 6 21:14:44 2012] Vigneting correction estimate = 1.000000 [Fri Apr 6 21:14:44 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Fri Apr 6 21:14:44 2012] Assessing source extent using major [Fri Apr 6 21:14:44 2012] Source does appear to be extended [Fri Apr 6 21:14:44 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Fri Apr 6 21:15:38 2012] Using EEF radius (= 11.39 ")to estimate initial spatial extent for simple fitting [Fri Apr 6 21:15:38 2012] Initial guess for spatial extent in simple fitting = 11.39" [Fri Apr 6 21:15:38 2012] source mask rpix=2.6, npix_max = 38, mask sum = 36, frac = 0.925 [Fri Apr 6 21:15:38 2012] Giving source the simple spatial ID 114 for pass 1, mean size = 11.39" [Sat Apr 7 03:14:30 2012] Vigneting correction estimate = 1.000000 [Sat Apr 7 03:14:30 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Sat Apr 7 03:14:30 2012] Assessing source extent using major [Sat Apr 7 03:14:30 2012] Source does appear to be extended [Sat Apr 7 03:14:30 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Sat Apr 7 03:15:32 2012] XMMSAS src. selection expression = ellipse(36517.075897, 20487.493164, 652.500000, 652.500000, 0.000000, X, Y) [Sat Apr 7 03:15:32 2012] Writing source region out to fullrun_pn_xmm0501790101_pi300-10000_pass1_cl_src122_src.reg [Sat Apr 7 03:15:32 2012] Extracting stamp from image fullrun_pn_xmm0501790101_pi300-10000_cl_sm2.00.img.gz, (383, 199) - (458, 274) [Sat Apr 7 03:15:32 2012] XMMSAS bgd. selection expression = annulus(36517.075897, 20487.493164, 1087.500000, 2175.000000, X, Y) && !ellipse(33968.340698, 22920.243408, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(38382.295044, 18056.136810, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(34088.567000, 21637.985600, 452.476813, 452.476813, 0.000000, X, Y) && !ellipse(37010.303345, 19628.388077, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(38788.198600, 18548.606400, 353.105610, 353.105610, 0.000000, X, Y) && !ellipse(33973.172852, 20768.569168, 870.000000, 870.000000, 0.000000, X, Y) [Sat Apr 7 03:15:32 2012] Writing fullrun_pn_xmm0501790101_pi300-10000_pass1_cl_src122.gif [Sat Apr 7 05:50:57 2012] Mean detx,y = (-8589.01, -7786.40) [Sat Apr 7 05:51:01 2012] Setting backscal keywords in source and bgd. spectrum [Sat Apr 7 05:51:20 2012] Binned source spectrum to 10 counts/bin [Sat Apr 7 05:51:21 2012] Setting source spectrum file to fullrun_pn_xmm0501790101_pi300-10000_pass1_cl_src122_src_b10.pi.gz [Sat Apr 7 05:51:21 2012] Setting bgd. spectrum file to fullrun_pn_xmm0501790101_pi300-10000_pass1_cl_src122_bgd.pi.gz [Sat Apr 7 23:01:35 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done [Sat Apr 7 23:01:35 2012] rmf not generated due to insufficient counts [Sun Apr 8 04:47:07 2012] Updating aperture counts using extracted products [Sun Apr 8 04:47:07 2012] Error reading totcts from fullrun_pn_xmm0501790101_pi300-10000_pass1_cl_src122_src_b10.pi.gz [Sun Apr 8 04:47:10 2012] Calculating source flux in energy range 0.30-8.00 [Sun Apr 8 04:47:10 2012] Using photon index=1.80, rate=0.0026, arf fullrun_pn_xmm0501790101_pi300-10000_pass1_cl_src122.arf [Sun Apr 8 04:47:10 2012] Assuming count rate is from the 0.30-10.00 bandpass [Sun Apr 8 04:47:10 2012] Updating source flux to 1.5e-14 [Sun Apr 8 04:58:48 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting