[Fri Apr 6 15:44:43 2012] Detection parameters: Position = (417.5, 294.8) = 8 9 11.03 -49 14 16.8 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 273.4 +/- 26.4 Background counts = 184.5 Rate = 0.002 +/- 0.0002 [Fri Apr 6 15:44:44 2012] Off-axis axis estimate = 8.64' [Fri Apr 6 15:51:49 2012] Using EEF radius (= 10.75 ")to estimate initial spatial extent for simple fitting [Fri Apr 6 15:51:49 2012] Initial guess for spatial extent in simple fitting = 10.75" [Fri Apr 6 15:51:49 2012] source mask rpix=2.5, npix_max = 35, mask sum = 30, frac = 0.850 [Fri Apr 6 15:51:49 2012] Giving source the simple spatial ID 111 for pass 0, mean size = 10.75" [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 (= 10.75 ")to estimate initial spatial extent for simple fitting [Fri Apr 6 21:15:38 2012] Initial guess for spatial extent in simple fitting = 10.75" [Fri Apr 6 21:15:38 2012] source mask rpix=2.5, npix_max = 35, mask sum = 30, frac = 0.850 [Fri Apr 6 21:15:38 2012] Giving source the simple spatial ID 110 for pass 1, mean size = 10.75" [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(36275.019531, 25597.434235, 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_src116_src.reg [Sat Apr 7 03:15:32 2012] Extracting stamp from image fullrun_pn_xmm0501790101_pi300-10000_cl_sm2.00.img.gz, (380, 257) - (455, 332) [Sat Apr 7 03:15:32 2012] XMMSAS bgd. selection expression = annulus(36275.019531, 25597.434235, 1087.500000, 2175.000000, X, Y) && !ellipse(33968.340698, 22920.243408, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(37599.297699, 26483.566193, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(37782.165497, 24823.949860, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(36835.982086, 26653.636749, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(35690.939636, 26767.649017, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(37112.981293, 24039.155060, 870.000000, 870.000000, 0.000000, X, Y) [Sat Apr 7 03:15:32 2012] Writing fullrun_pn_xmm0501790101_pi300-10000_pass1_cl_src116.gif [Sat Apr 7 05:45:29 2012] Mean detx,y = (-10337.34, -3010.60) [Sat Apr 7 05:45:33 2012] Setting backscal keywords in source and bgd. spectrum [Sat Apr 7 05:45:44 2012] Binned source spectrum to 10 counts/bin [Sat Apr 7 05:45:44 2012] Setting source spectrum file to fullrun_pn_xmm0501790101_pi300-10000_pass1_cl_src116_src_b10.pi.gz [Sat Apr 7 05:45:44 2012] Setting bgd. spectrum file to fullrun_pn_xmm0501790101_pi300-10000_pass1_cl_src116_bgd.pi.gz [Sat Apr 7 23:00:05 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done [Sat Apr 7 23:00:05 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_src116_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=0.00225, arf fullrun_pn_xmm0501790101_pi300-10000_pass1_cl_src116.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 1.3e-14 [Sun Apr 8 04:58:48 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting