[Tue Mar 6 10:22:56 2012] Detection parameters: Position = (248.6, 204.0) = 0 56 0.18 26 18 34.2 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 75.4 +/- 15.0 Background counts = 50.3 Rate = 0.003 +/- 0.0005 [Tue Mar 6 10:22:57 2012] Off-axis axis estimate = 7.74' [Tue Mar 6 14:48:40 2012] Using EEF radius (= 10.30 ")to estimate initial spatial extent for simple fitting [Tue Mar 6 14:48:40 2012] Initial guess for spatial extent in simple fitting = 10.30" [Tue Mar 6 14:48:40 2012] source mask rpix=2.4, npix_max = 32, mask sum = 30, frac = 0.912 [Tue Mar 6 14:48:40 2012] Giving source the simple spatial ID 42 for pass 0, mean size = 10.30" [Tue Mar 6 18:24:38 2012] fullrun_mos1_xmm0203220101_pi300-10000_cl_pass0_src42.ximg exists [Tue Mar 6 18:24:38 2012] fullrun_mos1_xmm0203220101_pi300-10000_cl_pass0_src42_1.ximg exists [Tue Mar 6 18:24:38 2012] Fit fullrun_mos1_xmm0203220101_pi300-10000_cl_pass0_src42 appears to have run properly [Tue Mar 6 18:24:40 2012] fullrun_mos1_xmm0203220101_pi300-10000_cl_pass0_tfrozen_src42.ximg exists [Tue Mar 6 18:24:40 2012] fullrun_mos1_xmm0203220101_pi300-10000_cl_pass0_tfrozen_src42_1.ximg exists [Tue Mar 6 18:24:40 2012] Fit fullrun_mos1_xmm0203220101_pi300-10000_cl_pass0_tfrozen_src42 appears to have run properly [Tue Mar 6 22:08:25 2012] Warning, spatial fit 42 centroid is now closest to src. 15 [Tue Mar 6 22:08:25 2012] Vigneting correction estimate = 1.000000 [Tue Mar 6 22:08:25 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Tue Mar 6 22:08:25 2012] Assessing source extent using major [Tue Mar 6 22:08:25 2012] Source does appear to be extended [Tue Mar 6 22:08:25 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Tue Mar 6 22:08:25 2012] Source is confused with source 15 [Wed Mar 7 01:58:44 2012] Using EEF radius (= 10.30 ")to estimate initial spatial extent for simple fitting [Wed Mar 7 01:58:44 2012] Initial guess for spatial extent in simple fitting = 10.30" [Wed Mar 7 01:58:44 2012] source mask rpix=2.4, npix_max = 32, mask sum = 30, frac = 0.912 [Wed Mar 7 01:58:44 2012] Giving source the simple spatial ID 35 for pass 1, mean size = 10.30" [Wed Mar 7 04:56:57 2012] fullrun_mos1_xmm0203220101_pi300-10000_cl_pass1_src35.ximg exists [Wed Mar 7 04:56:57 2012] fullrun_mos1_xmm0203220101_pi300-10000_cl_pass1_src35_1.ximg exists [Wed Mar 7 04:56:57 2012] Fit fullrun_mos1_xmm0203220101_pi300-10000_cl_pass1_src35 appears to have run properly [Wed Mar 7 04:56:58 2012] fullrun_mos1_xmm0203220101_pi300-10000_cl_pass1_tfrozen_src35.ximg exists [Wed Mar 7 04:56:58 2012] fullrun_mos1_xmm0203220101_pi300-10000_cl_pass1_tfrozen_src35_1.ximg exists [Wed Mar 7 04:56:58 2012] Fit fullrun_mos1_xmm0203220101_pi300-10000_cl_pass1_tfrozen_src35 appears to have run properly [Wed Mar 7 07:55:18 2012] Warning, spatial fit 35 centroid is now closest to src. 15 [Wed Mar 7 07:55:18 2012] Source 67 is offset by 7.772198 and -1.255313 pixels which is larger than 2 X fitted extent = 1.373140 x 1.373140, not incorporating fit results [Wed Mar 7 07:55:18 2012] Vigneting correction estimate = 1.000000 [Wed Mar 7 07:55:18 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Wed Mar 7 07:55:18 2012] Assessing source extent using major [Wed Mar 7 07:55:18 2012] Source does appear to be extended [Wed Mar 7 07:55:18 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Wed Mar 7 11:14:09 2012] XMMSAS src. selection expression = ellipse(21575.435226, 17703.057739, 652.500000, 652.500000, 0.000000, X, Y) [Wed Mar 7 11:14:09 2012] Writing source region out to fullrun_mos1_xmm0203220101_pi300-10000_pass1_cl_src67_src.reg [Wed Mar 7 11:14:09 2012] Extracting stamp from image fullrun_mos1_xmm0203220101_pi300-10000_cl_sm2.00.img.gz, (211, 167) - (286, 242) [Wed Mar 7 11:14:09 2012] XMMSAS bgd. selection expression = annulus(21575.435226, 17703.057739, 1087.500000, 2175.000000, X, Y) && !ellipse(21976.765472, 19365.788422, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(21562.987000, 19885.586200, 871.232025, 871.232025, 0.000000, X, Y) && !ellipse(21954.343750, 18538.432175, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22820.385101, 18933.704971, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22322.242000, 18489.778000, 1231.120035, 1231.120035, 0.000000, X, Y) && !ellipse(21206.228180, 18883.864761, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(20775.647476, 19870.111237, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22772.071533, 17274.524063, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(20412.646561, 18402.661942, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(21835.492000, 16827.364000, 955.704028, 955.704028, 0.000000, X, Y) && !ellipse(20110.744000, 18028.254000, 1649.408047, 1649.408047, 0.000000, X, Y) [Wed Mar 7 11:14:09 2012] Writing fullrun_mos1_xmm0203220101_pi300-10000_pass1_cl_src67.gif [Wed Mar 7 12:18:06 2012] Mean detx,y = (7798.52, -820.93) [Wed Mar 7 12:18:09 2012] Setting backscal keywords in source and bgd. spectrum [Wed Mar 7 12:18:28 2012] Binned source spectrum to 10 counts/bin [Wed Mar 7 12:18:28 2012] Setting source spectrum file to fullrun_mos1_xmm0203220101_pi300-10000_pass1_cl_src67_src_b10.pi.gz [Wed Mar 7 12:18:28 2012] Setting bgd. spectrum file to fullrun_mos1_xmm0203220101_pi300-10000_pass1_cl_src67_bgd.pi.gz [Wed Mar 7 19:08:30 2012] Not generating rmf since there are only 75 counts [Wed Mar 7 19:08:30 2012] rmf not generated due to insufficient counts [Wed Mar 7 21:12:34 2012] Updating aperture counts using extracted products [Wed Mar 7 21:12:34 2012] Error reading totcts from fullrun_mos1_xmm0203220101_pi300-10000_pass1_cl_src67_src_b10.pi.gz [Wed Mar 7 21:12:37 2012] Calculating source flux in energy range 0.30-8.00 [Wed Mar 7 21:12:37 2012] Using photon index=1.80, rate=0.00251, arf fullrun_mos1_xmm0203220101_pi300-10000_pass1_cl_src67.arf [Wed Mar 7 21:12:37 2012] Assuming count rate is from the 0.30-10.00 bandpass [Wed Mar 7 21:12:37 2012] Updating source flux to 3.6e-14 [Wed Mar 7 21:12:49 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting