[Sun Mar 25 08:46:30 2012] Detection parameters: Position = (324.8, 244.0) = 17 45 35.54 -29 5 34.5 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 164.5 +/- 20.6 Background counts = 77.9 Rate = 0.02 +/- 0.003 [Sun Mar 25 08:46:30 2012] Off-axis axis estimate = 4.39' [Sun Mar 25 08:51:21 2012] Using EEF radius (= 8.62 ")to estimate initial spatial extent for simple fitting [Sun Mar 25 08:51:21 2012] Initial guess for spatial extent in simple fitting = 8.62" [Sun Mar 25 08:51:21 2012] source mask rpix=2.0, npix_max = 24, mask sum = 25, frac = 1.014 [Sun Mar 25 08:51:21 2012] Giving source the simple spatial ID 36 for pass 0, mean size = 8.62" [Sun Mar 25 11:54:17 2012] fullrun_pn_xmm0504940201_pi300-10000_cl_pass0_src36.ximg exists [Sun Mar 25 11:54:17 2012] fullrun_pn_xmm0504940201_pi300-10000_cl_pass0_src36_1.ximg exists [Sun Mar 25 11:54:17 2012] Fit fullrun_pn_xmm0504940201_pi300-10000_cl_pass0_src36 appears to have run properly [Sun Mar 25 11:54:18 2012] fullrun_pn_xmm0504940201_pi300-10000_cl_pass0_tfrozen_src36.ximg exists [Sun Mar 25 11:54:18 2012] fullrun_pn_xmm0504940201_pi300-10000_cl_pass0_tfrozen_src36_1.ximg exists [Sun Mar 25 11:54:18 2012] Fit fullrun_pn_xmm0504940201_pi300-10000_cl_pass0_tfrozen_src36 appears to have run properly [Sun Mar 25 14:50:21 2012] Warning, spatial fit 36 centroid is now closest to src. 36 [Sun Mar 25 14:50:21 2012] Vigneting correction estimate = 1.000000 [Sun Mar 25 14:50:21 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Sun Mar 25 14:50:21 2012] Assessing source extent using major [Sun Mar 25 14:50:21 2012] Source does appear to be extended [Sun Mar 25 14:50:21 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Sun Mar 25 14:50:21 2012] Source is confused with source 36 [Sun Mar 25 14:50:21 2012] Source is confused with source 38 [Sun Mar 25 14:50:52 2012] Using EEF radius (= 8.62 ")to estimate initial spatial extent for simple fitting [Sun Mar 25 14:50:52 2012] Initial guess for spatial extent in simple fitting = 8.62" [Sun Mar 25 14:50:52 2012] source mask rpix=2.0, npix_max = 24, mask sum = 25, frac = 1.014 [Sun Mar 25 14:50:52 2012] Giving source the simple spatial ID 26 for pass 1, mean size = 8.62" [Sun Mar 25 17:16:23 2012] fullrun_pn_xmm0504940201_pi300-10000_cl_pass1_src26.ximg exists [Sun Mar 25 17:16:23 2012] fullrun_pn_xmm0504940201_pi300-10000_cl_pass1_src26_1.ximg exists [Sun Mar 25 17:16:23 2012] Fit fullrun_pn_xmm0504940201_pi300-10000_cl_pass1_src26 appears to have run properly [Sun Mar 25 17:16:24 2012] fullrun_pn_xmm0504940201_pi300-10000_cl_pass1_tfrozen_src26.ximg exists [Sun Mar 25 17:16:24 2012] fullrun_pn_xmm0504940201_pi300-10000_cl_pass1_tfrozen_src26_1.ximg exists [Sun Mar 25 17:16:24 2012] Fit fullrun_pn_xmm0504940201_pi300-10000_cl_pass1_tfrozen_src26 appears to have run properly [Sun Mar 25 19:44:39 2012] Warning, spatial fit 26 centroid is now closest to src. 38 [Sun Mar 25 19:44:39 2012] Warning: source 27 in spatial fitting list does not appear to have a counterpart in memory, closest src. was src. 37 at 13.218222 pixels away [Sun Mar 25 19:44:39 2012] Warning: source 28 in spatial fitting list does not appear to have a counterpart in memory, closest src. was src. 37 at 14.397759 pixels away [Sun Mar 25 19:44:39 2012] Vigneting correction estimate = 1.000000 [Sun Mar 25 19:44:39 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Sun Mar 25 19:44:39 2012] Assessing source extent using major [Sun Mar 25 19:44:39 2012] Source does appear to be extended [Sun Mar 25 19:44:39 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Sun Mar 25 19:45:03 2012] XMMSAS src. selection expression = ellipse(28209.831726, 21176.870193, 652.500000, 652.500000, 0.000000, X, Y) [Sun Mar 25 19:45:03 2012] Writing source region out to fullrun_pn_xmm0504940201_pi300-10000_pass1_cl_src37_src.reg [Sun Mar 25 19:45:03 2012] Extracting stamp from image fullrun_pn_xmm0504940201_pi300-10000_cl_sm2.00.img.gz, (287, 206) - (362, 281) [Sun Mar 25 19:45:03 2012] XMMSAS bgd. selection expression = annulus(28209.831726, 21176.870193, 1087.500000, 2175.000000, X, Y) && !ellipse(28234.831840, 23889.866000, 1473.368042, 1473.368042, 0.000000, X, Y) && !ellipse(28217.654520, 23170.261600, 748.460822, 748.460822, 0.000000, X, Y) && !ellipse(26908.283800, 22538.468800, 680.290420, 436.623213, 112.481000, X, Y) && !ellipse(28184.500000, 22337.937400, 501.100814, 501.100814, 0.000000, X, Y) && !ellipse(28161.871277, 21704.561249, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(28195.039800, 20951.046000, 1379.560040, 422.093612, 269.606700, X, Y) && !ellipse(28262.936200, 19349.195000, 736.468021, 736.468021, 0.000000, X, Y) && !ellipse(28186.841827, 19097.552139, 870.000000, 870.000000, 0.000000, X, Y) [Sun Mar 25 19:45:03 2012] Writing fullrun_pn_xmm0504940201_pi300-10000_pass1_cl_src37.gif [Sun Mar 25 20:28:56 2012] Mean detx,y = (1194.79, 6235.70) [Sun Mar 25 20:29:01 2012] Setting backscal keywords in source and bgd. spectrum [Sun Mar 25 20:29:30 2012] Binned source spectrum to 10 counts/bin [Sun Mar 25 20:29:31 2012] Setting source spectrum file to fullrun_pn_xmm0504940201_pi300-10000_pass1_cl_src37_src_b10.pi.gz [Sun Mar 25 20:29:31 2012] Setting bgd. spectrum file to fullrun_pn_xmm0504940201_pi300-10000_pass1_cl_src37_bgd.pi.gz [Mon Mar 26 01:23:14 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done [Mon Mar 26 01:23:14 2012] rmf not generated due to insufficient counts [Mon Mar 26 03:55:43 2012] Updating aperture counts using extracted products [Mon Mar 26 03:55:43 2012] Error reading totcts from fullrun_pn_xmm0504940201_pi300-10000_pass1_cl_src37_src_b10.pi.gz [Mon Mar 26 03:55:45 2012] Calculating source flux in energy range 0.30-8.00 [Mon Mar 26 03:55:45 2012] Using photon index=1.80, rate=0.0213, arf fullrun_pn_xmm0504940201_pi300-10000_pass1_cl_src37.arf [Mon Mar 26 03:55:45 2012] Assuming count rate is from the 0.30-10.00 bandpass [Mon Mar 26 03:55:45 2012] Updating source flux to 7.3e-14 [Mon Mar 26 04:03:06 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting