[Sun Dec 18 23:07:41 2011] Detection parameters: Position = (289.2, 292.4) = 7 58 35.45 37 45 13.2 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 244.8 +/- 21.6 Background counts = 98.1 Rate = 0.006 +/- 0.0005 [Sun Dec 18 23:07:41 2011] Off-axis axis estimate = 0.80' [Sun Dec 18 23:12:38 2011] Using EEF radius (= 6.83 ")to estimate initial spatial extent for simple fitting [Sun Dec 18 23:12:38 2011] Initial guess for spatial extent in simple fitting = 6.83" [Sun Dec 18 23:12:38 2011] source mask rpix=1.6, npix_max = 17, mask sum = 7, frac = 0.408 [Sun Dec 18 23:12:38 2011] Skipping simple spatial due to low active detector fraction [Mon Dec 19 01:02:37 2011] Vigneting correction estimate = 1.000000 [Mon Dec 19 01:02:37 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Mon Dec 19 01:02:37 2011] Assessing source extent using major [Mon Dec 19 01:02:37 2011] Source does appear to be extended [Mon Dec 19 01:02:37 2011] Computing asymmetry using major and minor axis, asym = 1.00 [Mon Dec 19 01:02:52 2011] Using EEF radius (= 6.83 ")to estimate initial spatial extent for simple fitting [Mon Dec 19 01:02:52 2011] Initial guess for spatial extent in simple fitting = 6.83" [Mon Dec 19 01:02:52 2011] source mask rpix=1.6, npix_max = 17, mask sum = 7, frac = 0.408 [Mon Dec 19 01:02:52 2011] Skipping simple spatial due to low active detector fraction [Mon Dec 19 02:57:03 2011] Vigneting correction estimate = 1.000000 [Mon Dec 19 02:57:03 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Mon Dec 19 02:57:03 2011] Assessing source extent using major [Mon Dec 19 02:57:03 2011] Source does appear to be extended [Mon Dec 19 02:57:03 2011] Computing asymmetry using major and minor axis, asym = 1.00 [Mon Dec 19 02:57:28 2011] XMMSAS src. selection expression = ellipse(25114.463165, 25386.088593, 652.500000, 652.500000, 0.000000, X, Y) [Mon Dec 19 02:57:28 2011] Writing source region out to fullrun_pn_xmm0602390101_pi300-10000_pass1_cl_src32_src.reg [Mon Dec 19 02:57:28 2011] Extracting stamp from image fullrun_pn_xmm0602390101_pi300-10000_cl_sm2.00.img.gz, (252, 255) - (327, 330) [Mon Dec 19 02:57:28 2011] XMMSAS bgd. selection expression = annulus(25114.463165, 25386.088593, 1087.500000, 2175.000000, X, Y) && !ellipse(26826.572560, 27772.746200, 477.682414, 477.682414, 0.000000, X, Y) && !ellipse(27374.040200, 26927.674000, 375.092011, 375.092011, 0.000000, X, Y) && !ellipse(26726.644745, 26385.579681, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26395.034241, 25886.081055, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22515.059387, 25880.186890, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26159.356000, 25434.200000, 1058.648030, 1058.648030, 0.000000, X, Y) [Mon Dec 19 02:57:28 2011] Writing fullrun_pn_xmm0602390101_pi300-10000_pass1_cl_src32.gif [Mon Dec 19 03:25:59 2011] Mean detx,y = (-1851.14, 1875.91) [Mon Dec 19 03:26:04 2011] Setting backscal keywords in source and bgd. spectrum [Mon Dec 19 03:26:31 2011] Binned source spectrum to 10 counts/bin [Mon Dec 19 03:26:32 2011] Setting source spectrum file to fullrun_pn_xmm0602390101_pi300-10000_pass1_cl_src32_src_b10.pi.gz [Mon Dec 19 03:26:32 2011] Setting bgd. spectrum file to fullrun_pn_xmm0602390101_pi300-10000_pass1_cl_src32_bgd.pi.gz [Mon Dec 19 04:33:30 2011] Not generating rmf since RequireSpatial is true but spatial fitting not done [Mon Dec 19 04:33:30 2011] rmf not generated due to insufficient counts [Mon Dec 19 05:28:46 2011] Updating aperture counts using extracted products [Mon Dec 19 05:28:46 2011] Error reading totcts from fullrun_pn_xmm0602390101_pi300-10000_pass1_cl_src32_src_b10.pi.gz [Mon Dec 19 05:28:47 2011] Calculating source flux in energy range 0.30-8.00 [Mon Dec 19 05:28:47 2011] Using photon index=1.80, rate=0.00564, arf fullrun_pn_xmm0602390101_pi300-10000_pass1_cl_src32.arf [Mon Dec 19 05:28:47 2011] Assuming count rate is from the 0.30-10.00 bandpass [Mon Dec 19 05:28:47 2011] Updating source flux to 2.5e-14 [Mon Dec 19 05:29:59 2011] Simple spatial fitting not done (or not done successfully), skipping spectral fitting