[Mon Feb 20 10:41:18 2012] Detection parameters: Position = (340.6, 391.7) = 15 9 17.68 7 38 35.0 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 54.2 +/- 14.0 Background counts = 58.4 Rate = 0.001 +/- 0.0004 [Mon Feb 20 10:41:19 2012] Off-axis axis estimate = 7.42' [Mon Feb 20 14:37:20 2012] Using EEF radius (= 10.14 ")to estimate initial spatial extent for simple fitting [Mon Feb 20 14:37:20 2012] Initial guess for spatial extent in simple fitting = 10.14" [Mon Feb 20 14:37:20 2012] source mask rpix=2.3, npix_max = 32, mask sum = 30, frac = 0.936 [Mon Feb 20 14:37:20 2012] Giving source the simple spatial ID 35 for pass 0, mean size = 10.14" [Mon Feb 20 16:38:40 2012] fullrun_mos1_xmm0556020101_pi300-10000_cl_pass0_src35.ximg exists [Mon Feb 20 16:38:40 2012] fullrun_mos1_xmm0556020101_pi300-10000_cl_pass0_src35_1.ximg exists [Mon Feb 20 16:38:40 2012] Fit fullrun_mos1_xmm0556020101_pi300-10000_cl_pass0_src35 appears to have run properly [Mon Feb 20 16:38:41 2012] fullrun_mos1_xmm0556020101_pi300-10000_cl_pass0_tfrozen_src35.ximg exists [Mon Feb 20 16:38:41 2012] fullrun_mos1_xmm0556020101_pi300-10000_cl_pass0_tfrozen_src35_1.ximg exists [Mon Feb 20 16:38:41 2012] Fit fullrun_mos1_xmm0556020101_pi300-10000_cl_pass0_tfrozen_src35 appears to have run properly [Mon Feb 20 18:33:16 2012] Source 28 is offset by 0.478883 and -7.405120 pixels which is larger than 2 X fitted extent = 1.139825 x 1.139825, not incorporating fit results [Mon Feb 20 18:33:16 2012] Warning, spatial fit 35 centroid is now closest to src. 29 [Mon Feb 20 18:33:16 2012] Vigneting correction estimate = 1.000000 [Mon Feb 20 18:33:16 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Mon Feb 20 18:33:16 2012] Assessing source extent using major [Mon Feb 20 18:33:16 2012] Source does appear to be extended [Mon Feb 20 18:33:16 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Mon Feb 20 22:42:23 2012] Using EEF radius (= 10.14 ")to estimate initial spatial extent for simple fitting [Mon Feb 20 22:42:23 2012] Initial guess for spatial extent in simple fitting = 10.14" [Mon Feb 20 22:42:23 2012] source mask rpix=2.3, npix_max = 32, mask sum = 30, frac = 0.936 [Mon Feb 20 22:42:23 2012] Giving source the simple spatial ID 31 for pass 1, mean size = 10.14" [Tue Feb 21 00:13:33 2012] fullrun_mos1_xmm0556020101_pi300-10000_cl_pass1_src31.ximg exists [Tue Feb 21 00:13:33 2012] fullrun_mos1_xmm0556020101_pi300-10000_cl_pass1_src31_1.ximg exists [Tue Feb 21 00:13:33 2012] Fit fullrun_mos1_xmm0556020101_pi300-10000_cl_pass1_src31 appears to have run properly [Tue Feb 21 00:13:33 2012] fullrun_mos1_xmm0556020101_pi300-10000_cl_pass1_tfrozen_src31.ximg exists [Tue Feb 21 00:13:33 2012] fullrun_mos1_xmm0556020101_pi300-10000_cl_pass1_tfrozen_src31_1.ximg exists [Tue Feb 21 00:13:33 2012] Fit fullrun_mos1_xmm0556020101_pi300-10000_cl_pass1_tfrozen_src31 appears to have run properly [Tue Feb 21 01:48:59 2012] Source 28 is offset by -3.865071 and 6.061570 pixels which is larger than 2 X fitted extent = 1.298464 x 1.298464, not incorporating fit results [Tue Feb 21 01:48:59 2012] Source 28 is offset by -4.467577 and -3.351579 pixels which is larger than 2 X fitted extent = 1.133136 x 1.133136, not incorporating fit results [Tue Feb 21 01:48:59 2012] Source 28 is offset by -3.740450 and -5.848200 pixels which is larger than 2 X fitted extent = 1.177494 x 1.177494, not incorporating fit results [Tue Feb 21 01:48:59 2012] Vigneting correction estimate = 1.000000 [Tue Feb 21 01:48:59 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Tue Feb 21 01:48:59 2012] Assessing source extent using major [Tue Feb 21 01:48:59 2012] Source does appear to be extended [Tue Feb 21 01:48:59 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Tue Feb 21 05:04:40 2012] XMMSAS src. selection expression = ellipse(29583.482819, 34030.574585, 652.500000, 652.500000, 0.000000, X, Y) [Tue Feb 21 05:04:40 2012] Writing source region out to fullrun_mos1_xmm0556020101_pi300-10000_pass1_cl_src28_src.reg [Tue Feb 21 05:04:40 2012] Extracting stamp from image fullrun_mos1_xmm0556020101_pi300-10000_cl_sm2.00.img.gz, (303, 354) - (378, 429) [Tue Feb 21 05:04:40 2012] XMMSAS bgd. selection expression = annulus(29583.482819, 34030.574585, 1087.500000, 2175.000000, X, Y) && !ellipse(28722.409200, 33808.367200, 742.881621, 742.881621, 0.000000, X, Y) && !ellipse(30641.055328, 32875.472229, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(29200.330231, 33462.939941, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(29100.583435, 36363.224915, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(31997.793884, 34572.667847, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(32639.551200, 32156.213860, 1127.288032, 1127.288032, 0.000000, X, Y) [Tue Feb 21 05:04:40 2012] Writing fullrun_mos1_xmm0556020101_pi300-10000_pass1_cl_src28.gif [Tue Feb 21 05:17:34 2012] Mean detx,y = (4973.31, 4722.22) [Tue Feb 21 05:17:36 2012] Setting backscal keywords in source and bgd. spectrum [Tue Feb 21 05:18:05 2012] Binned source spectrum to 10 counts/bin [Tue Feb 21 05:18:06 2012] Setting source spectrum file to fullrun_mos1_xmm0556020101_pi300-10000_pass1_cl_src28_src_b10.pi.gz [Tue Feb 21 05:18:06 2012] Setting bgd. spectrum file to fullrun_mos1_xmm0556020101_pi300-10000_pass1_cl_src28_bgd.pi.gz [Tue Feb 21 06:10:53 2012] Not generating rmf since there are only 54 counts [Tue Feb 21 06:10:53 2012] rmf not generated due to insufficient counts [Tue Feb 21 07:37:37 2012] Updating aperture counts using extracted products [Tue Feb 21 07:37:37 2012] Error reading totcts from fullrun_mos1_xmm0556020101_pi300-10000_pass1_cl_src28_src_b10.pi.gz [Tue Feb 21 07:37:38 2012] Calculating source flux in energy range 0.30-8.00 [Tue Feb 21 07:37:38 2012] Using photon index=1.80, rate=0.00145, arf fullrun_mos1_xmm0556020101_pi300-10000_pass1_cl_src28.arf [Tue Feb 21 07:37:38 2012] Assuming count rate is from the 0.30-10.00 bandpass [Tue Feb 21 07:37:38 2012] Updating source flux to 1.8e-14 [Tue Feb 21 07:37:42 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting