[Sat Aug 4 21:47:41 2012] Detection parameters: Position = (312.8, 259.9) = 16 32 1.38 -47 56 43.2 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 77.3 +/- 13.9 Background counts = 32.0 Rate = 0.01 +/- 0.003 [Sat Aug 4 21:47:41 2012] Off-axis axis estimate = 2.98' [Sat Aug 4 21:49:20 2012] Using EEF radius (= 7.92 ")to estimate initial spatial extent for simple fitting [Sat Aug 4 21:49:20 2012] Initial guess for spatial extent in simple fitting = 7.92" [Sat Aug 4 21:49:20 2012] source mask rpix=1.8, npix_max = 21, mask sum = 20, frac = 0.929 [Sat Aug 4 21:49:20 2012] Giving source the simple spatial ID 18 for pass 0, mean size = 7.92" [Sat Aug 4 22:44:04 2012] fullrun_pn_xmm0556140301_pi300-10000_cl_pass0_src18.ximg exists [Sat Aug 4 22:44:04 2012] fullrun_pn_xmm0556140301_pi300-10000_cl_pass0_src18_1.ximg exists [Sat Aug 4 22:44:04 2012] Fit fullrun_pn_xmm0556140301_pi300-10000_cl_pass0_src18 appears to have run properly [Sat Aug 4 22:44:04 2012] fullrun_pn_xmm0556140301_pi300-10000_cl_pass0_tfrozen_src18.ximg exists [Sat Aug 4 22:44:04 2012] fullrun_pn_xmm0556140301_pi300-10000_cl_pass0_tfrozen_src18_1.ximg exists [Sat Aug 4 22:44:04 2012] Fit fullrun_pn_xmm0556140301_pi300-10000_cl_pass0_tfrozen_src18 appears to have run properly [Sat Aug 4 23:38:10 2012] Spatial fit model total counts = 372.559000, observed total counts = 372.000000 [Sat Aug 4 23:38:10 2012] Offset between fit and detection position for source 18 = 1.121718 pixels [Sat Aug 4 23:38:10 2012] 258.486100 total counts/ 174.308000 bgd. counts: snr = 6.375885 Spatial fit parameters: Offset between fit and detection position for source 18 = 1.121718 pixels Position = (312.6, 261.1) = 16 32 1.45 -47 56 38.0 Extent = 9.4 (7.1-13.1)", rotation angle = 0 Source counts = 84.2 +/- 16.1 Background counts = 174.3 Rate = 0.02 +/- 0.003 [Sat Aug 4 23:38:10 2012] Vigneting correction estimate = 1.000000 [Sat Aug 4 23:38:10 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Sat Aug 4 23:38:10 2012] Assessing source extent using major axis lower bound [Sat Aug 4 23:38:10 2012] Source does appear to be extended [Sat Aug 4 23:38:10 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Sat Aug 4 23:38:10 2012] Source is confused with source 17 [Sat Aug 4 23:38:21 2012] Using previous fit value to estimate initial spatial extent for simple fitting [Sat Aug 4 23:38:21 2012] Initial guess for spatial extent in simple fitting = 9.45" [Sat Aug 4 23:38:21 2012] source mask rpix=2.2, npix_max = 28, mask sum = 30, frac = 1.051 [Sat Aug 4 23:38:21 2012] Giving source the simple spatial ID 16 for pass 1, mean size = 9.45" [Sun Aug 5 00:33:52 2012] fullrun_pn_xmm0556140301_pi300-10000_cl_pass1_src16.ximg exists [Sun Aug 5 00:33:52 2012] fullrun_pn_xmm0556140301_pi300-10000_cl_pass1_src16_1.ximg exists [Sun Aug 5 00:33:52 2012] Fit fullrun_pn_xmm0556140301_pi300-10000_cl_pass1_src16 appears to have run properly [Sun Aug 5 00:33:53 2012] fullrun_pn_xmm0556140301_pi300-10000_cl_pass1_tfrozen_src16.ximg exists [Sun Aug 5 00:33:53 2012] fullrun_pn_xmm0556140301_pi300-10000_cl_pass1_tfrozen_src16_1.ximg exists [Sun Aug 5 00:33:53 2012] Fit fullrun_pn_xmm0556140301_pi300-10000_cl_pass1_tfrozen_src16 appears to have run properly [Sun Aug 5 01:42:54 2012] Warning, spatial fit 16 centroid is now closest to src. 19 [Sun Aug 5 01:42:54 2012] Vigneting correction estimate = 1.000000 [Sun Aug 5 01:42:54 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Sun Aug 5 01:42:54 2012] Assessing source extent using major axis lower bound [Sun Aug 5 01:42:54 2012] Source does appear to be extended [Sun Aug 5 01:42:54 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Sun Aug 5 01:43:03 2012] XMMSAS src. selection expression = ellipse(27146.374000, 22663.270780, 566.795416, 566.795416, 0.000000, X, Y) [Sun Aug 5 01:43:03 2012] Writing source region out to fullrun_pn_xmm0556140301_pi300-10000_pass1_cl_src18_src.reg [Sun Aug 5 01:43:03 2012] Extracting stamp from image fullrun_pn_xmm0556140301_pi300-10000_cl_sm2.00.img.gz, (280, 228) - (345, 294) [Sun Aug 5 01:43:03 2012] XMMSAS bgd. selection expression = annulus(27146.374000, 22663.270780, 944.659027, 1889.318054, X, Y) && !ellipse(27072.222200, 24921.480000, 697.020020, 697.020020, 0.000000, X, Y) && !ellipse(27117.392600, 24294.785340, 1162.272033, 406.851212, 90.000000, X, Y) && !ellipse(27155.331600, 23196.524600, 1042.632030, 1042.632030, 0.000000, X, Y) && !ellipse(27241.571747, 21523.797562, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27315.908600, 20325.400000, 834.064024, 834.064024, 0.000000, X, Y) && !ellipse(27287.857006, 20120.473538, 1498.160043, 471.165616, 88.503119, X, Y) && !ellipse(27317.782740, 18965.473000, 1968.888057, 465.980013, 89.898412, X, Y) [Sun Aug 5 01:43:03 2012] Writing fullrun_pn_xmm0556140301_pi300-10000_pass1_cl_src18.gif [Sun Aug 5 01:55:43 2012] Mean detx,y = (76.52, 4756.95) [Sun Aug 5 01:55:45 2012] Setting backscal keywords in source and bgd. spectrum [Sun Aug 5 01:55:58 2012] Binned source spectrum to 10 counts/bin [Sun Aug 5 01:55:58 2012] Setting source spectrum file to fullrun_pn_xmm0556140301_pi300-10000_pass1_cl_src18_src_b10.pi.gz [Sun Aug 5 01:55:58 2012] Setting bgd. spectrum file to fullrun_pn_xmm0556140301_pi300-10000_pass1_cl_src18_bgd.pi.gz [Sun Aug 5 02:47:30 2012] Not generating rmf since there are only 84 counts [Sun Aug 5 02:47:30 2012] rmf not generated due to insufficient counts [Sun Aug 5 03:25:35 2012] Updating aperture counts using extracted products [Sun Aug 5 03:25:35 2012] Error reading totcts from fullrun_pn_xmm0556140301_pi300-10000_pass1_cl_src18_src_b10.pi.gz [Sun Aug 5 03:25:36 2012] Calculating source flux in energy range 0.30-8.00 [Sun Aug 5 03:25:36 2012] Using photon index=1.80, rate=0.0164, arf fullrun_pn_xmm0556140301_pi300-10000_pass1_cl_src18.arf [Sun Aug 5 03:25:36 2012] Assuming count rate is from the 0.30-10.00 bandpass [Sun Aug 5 03:25:36 2012] Updating source flux to 5.1e-14 [Sun Aug 5 03:27:20 2012] Flag c found in src. 18 procflags, skipping spectral fitting [Sun Aug 5 03:27:20 2012] Source 18 has fewer than 100.000000 counts, skipping spectral fitting