[Wed Jun 13 09:04:04 2012] Detection parameters: Position = (309.4, 331.2) = 10 56 25.51 7 1 17.5 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 67.4 +/- 12.5 Background counts = 10.3 Rate = 0.003 +/- 0.0006 [Wed Jun 13 09:04:05 2012] Off-axis axis estimate = 2.51' [Wed Jun 13 10:15:52 2012] Using EEF radius (= 7.68 ")to estimate initial spatial extent for simple fitting [Wed Jun 13 10:15:52 2012] Initial guess for spatial extent in simple fitting = 7.68" [Wed Jun 13 10:15:52 2012] source mask rpix=1.8, npix_max = 20, mask sum = 10, frac = 0.487 [Wed Jun 13 10:15:52 2012] Skipping simple spatial due to low active detector fraction [Wed Jun 13 11:04:17 2012] Source 24 is offset by -4.190157 and -2.415438 pixels which is larger than 2 X fitted extent = 1.328943 x 1.328943, not incorporating fit results [Wed Jun 13 11:04:17 2012] Vigneting correction estimate = 1.000000 [Wed Jun 13 11:04:17 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Wed Jun 13 11:04:17 2012] Assessing source extent using major [Wed Jun 13 11:04:17 2012] Source does appear to be extended [Wed Jun 13 11:04:17 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Wed Jun 13 11:59:43 2012] Using EEF radius (= 7.68 ")to estimate initial spatial extent for simple fitting [Wed Jun 13 11:59:43 2012] Initial guess for spatial extent in simple fitting = 7.68" [Wed Jun 13 11:59:43 2012] source mask rpix=1.8, npix_max = 20, mask sum = 10, frac = 0.487 [Wed Jun 13 11:59:43 2012] Skipping simple spatial due to low active detector fraction [Wed Jun 13 12:46:21 2012] Vigneting correction estimate = 1.000000 [Wed Jun 13 12:46:21 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Wed Jun 13 12:46:21 2012] Assessing source extent using major [Wed Jun 13 12:46:21 2012] Source does appear to be extended [Wed Jun 13 12:46:21 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Wed Jun 13 14:18:39 2012] XMMSAS src. selection expression = ellipse(26872.902344, 28767.302917, 652.500000, 652.500000, 0.000000, X, Y) [Wed Jun 13 14:18:39 2012] Writing source region out to fullrun_mos2_xmm0200530501_pi300-10000_pass1_cl_src24_src.reg [Wed Jun 13 14:18:39 2012] Extracting stamp from image fullrun_mos2_xmm0200530501_pi300-10000_cl_sm2.00.img.gz, (272, 294) - (347, 369) [Wed Jun 13 14:18:39 2012] XMMSAS bgd. selection expression = annulus(26872.902344, 28767.302917, 1087.500000, 2175.000000, X, Y) && !ellipse(26326.954500, 27921.664400, 543.234416, 543.234416, 0.000000, X, Y) && !ellipse(27442.761902, 28144.889709, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27624.644684, 27612.025330, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27543.886658, 27099.872833, 870.000000, 870.000000, 0.000000, X, Y) [Wed Jun 13 14:18:39 2012] Writing fullrun_mos2_xmm0200530501_pi300-10000_pass1_cl_src24.gif [Wed Jun 13 14:21:29 2012] Mean detx,y = (-552.20, 506.93) [Wed Jun 13 14:21:30 2012] Setting backscal keywords in source and bgd. spectrum [Wed Jun 13 14:21:38 2012] Binned source spectrum to 10 counts/bin [Wed Jun 13 14:21:39 2012] Setting source spectrum file to fullrun_mos2_xmm0200530501_pi300-10000_pass1_cl_src24_src_b10.pi.gz [Wed Jun 13 14:21:39 2012] Setting bgd. spectrum file to fullrun_mos2_xmm0200530501_pi300-10000_pass1_cl_src24_bgd.pi.gz [Wed Jun 13 14:42:57 2012] Not generating rmf since there are only 67 counts [Wed Jun 13 14:42:57 2012] rmf not generated due to insufficient counts [Wed Jun 13 14:44:36 2012] Updating aperture counts using extracted products [Wed Jun 13 14:44:36 2012] Error reading totcts from fullrun_mos2_xmm0200530501_pi300-10000_pass1_cl_src24_src_b10.pi.gz [Wed Jun 13 14:44:36 2012] Calculating source flux in energy range 0.30-8.00 [Wed Jun 13 14:44:36 2012] Using photon index=1.80, rate=0.00327, arf fullrun_mos2_xmm0200530501_pi300-10000_pass1_cl_src24.arf [Wed Jun 13 14:44:36 2012] Assuming count rate is from the 0.30-10.00 bandpass [Wed Jun 13 14:44:36 2012] Updating source flux to 3.5e-14 [Wed Jun 13 14:45:05 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting