[Fri Apr 6 15:44:43 2012] Detection parameters: Position = (356.4, 234.2) = 8 9 38.15 -49 18 40.1 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 440.7 +/- 31.1 Background counts = 187.7 Rate = 0.006 +/- 0.0004 [Fri Apr 6 15:44:44 2012] Off-axis axis estimate = 6.27' [Fri Apr 6 15:51:49 2012] Using EEF radius (= 9.56 ")to estimate initial spatial extent for simple fitting [Fri Apr 6 15:51:49 2012] Initial guess for spatial extent in simple fitting = 9.56" [Fri Apr 6 15:51:49 2012] source mask rpix=2.2, npix_max = 29, mask sum = 25, frac = 0.858 [Fri Apr 6 15:51:49 2012] Giving source the simple spatial ID 116 for pass 0, mean size = 9.56" [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 (= 9.56 ")to estimate initial spatial extent for simple fitting [Fri Apr 6 21:15:38 2012] Initial guess for spatial extent in simple fitting = 9.56" [Fri Apr 6 21:15:38 2012] source mask rpix=2.2, npix_max = 29, mask sum = 25, frac = 0.858 [Fri Apr 6 21:15:38 2012] Giving source the simple spatial ID 115 for pass 1, mean size = 9.56" [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(30954.717834, 20326.882477, 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_src123_src.reg [Sat Apr 7 03:15:32 2012] Extracting stamp from image fullrun_pn_xmm0501790101_pi300-10000_cl_sm2.00.img.gz, (319, 197) - (394, 272) [Sat Apr 7 03:15:32 2012] XMMSAS bgd. selection expression = annulus(30954.717834, 20326.882477, 1087.500000, 2175.000000, X, Y) && !ellipse(29452.064178, 22912.323456, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(33968.340698, 22920.243408, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27959.974884, 20860.767715, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(30258.205414, 23108.938995, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(33973.172852, 20768.569168, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(28453.688202, 20469.023453, 870.000000, 870.000000, 0.000000, X, Y) [Sat Apr 7 03:15:32 2012] Writing fullrun_pn_xmm0501790101_pi300-10000_pass1_cl_src123.gif [Sat Apr 7 05:51:55 2012] Mean detx,y = (-3477.63, -5661.10) [Sat Apr 7 05:51:59 2012] Setting backscal keywords in source and bgd. spectrum [Sat Apr 7 05:52:15 2012] Binned source spectrum to 10 counts/bin [Sat Apr 7 05:52:16 2012] Setting source spectrum file to fullrun_pn_xmm0501790101_pi300-10000_pass1_cl_src123_src_b10.pi.gz [Sat Apr 7 05:52:16 2012] Setting bgd. spectrum file to fullrun_pn_xmm0501790101_pi300-10000_pass1_cl_src123_bgd.pi.gz [Sat Apr 7 23:01:49 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done [Sat Apr 7 23:01:49 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_src123_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=0.00631, arf fullrun_pn_xmm0501790101_pi300-10000_pass1_cl_src123.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 2.4e-14 [Sun Apr 8 04:58:48 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting