[Mon Mar 26 14:23:56 2012] Detection parameters: Position = (296.3, 301.9) = 21 16 6.42 -23 11 8.7 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 52.4 +/- 10.2 Background counts = 10.0 Rate = 0.01 +/- 0.002 [Mon Mar 26 14:23:56 2012] Off-axis axis estimate = 0.30' [Mon Mar 26 14:27:12 2012] Using EEF radius (= 6.58 ")to estimate initial spatial extent for simple fitting [Mon Mar 26 14:27:12 2012] Initial guess for spatial extent in simple fitting = 6.58" [Mon Mar 26 14:27:12 2012] source mask rpix=1.5, npix_max = 16, mask sum = 16, frac = 0.988 [Mon Mar 26 14:27:12 2012] Giving source the simple spatial ID 21 for pass 0, mean size = 6.58" [Mon Mar 26 17:07:52 2012] fullrun_pn_xmm0650383901_pi300-10000_cl_pass0_src21.ximg exists [Mon Mar 26 17:07:52 2012] fullrun_pn_xmm0650383901_pi300-10000_cl_pass0_src21_1.ximg exists [Mon Mar 26 17:07:52 2012] Fit fullrun_pn_xmm0650383901_pi300-10000_cl_pass0_src21 appears to have run properly [Mon Mar 26 17:07:53 2012] fullrun_pn_xmm0650383901_pi300-10000_cl_pass0_tfrozen_src21.ximg exists [Mon Mar 26 17:07:53 2012] fullrun_pn_xmm0650383901_pi300-10000_cl_pass0_tfrozen_src21_1.ximg exists [Mon Mar 26 17:07:53 2012] Fit fullrun_pn_xmm0650383901_pi300-10000_cl_pass0_tfrozen_src21 appears to have run properly [Mon Mar 26 22:14:23 2012] Warning, spatial fit 21 centroid is now closest to src. 24 [Mon Mar 26 22:14:23 2012] Vigneting correction estimate = 1.000000 [Mon Mar 26 22:14:23 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Mon Mar 26 22:14:23 2012] Assessing source extent using major [Mon Mar 26 22:14:23 2012] Source does appear to be extended [Mon Mar 26 22:14:23 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Mon Mar 26 22:14:56 2012] Using EEF radius (= 6.58 ")to estimate initial spatial extent for simple fitting [Mon Mar 26 22:14:56 2012] Initial guess for spatial extent in simple fitting = 6.58" [Mon Mar 26 22:14:56 2012] source mask rpix=1.5, npix_max = 16, mask sum = 16, frac = 0.988 [Mon Mar 26 22:14:56 2012] Giving source the simple spatial ID 18 for pass 1, mean size = 6.58" [Mon Mar 26 23:50:08 2012] fullrun_pn_xmm0650383901_pi300-10000_cl_pass1_src18.ximg exists [Mon Mar 26 23:50:08 2012] fullrun_pn_xmm0650383901_pi300-10000_cl_pass1_src18_1.ximg exists [Mon Mar 26 23:50:08 2012] Fit fullrun_pn_xmm0650383901_pi300-10000_cl_pass1_src18 appears to have run properly [Mon Mar 26 23:50:08 2012] fullrun_pn_xmm0650383901_pi300-10000_cl_pass1_tfrozen_src18.ximg exists [Mon Mar 26 23:50:09 2012] fullrun_pn_xmm0650383901_pi300-10000_cl_pass1_tfrozen_src18_1.ximg exists [Mon Mar 26 23:50:09 2012] Fit fullrun_pn_xmm0650383901_pi300-10000_cl_pass1_tfrozen_src18 appears to have run properly [Tue Mar 27 03:07:38 2012] Source 21 is offset by -5.172636 and 4.297545 pixels which is larger than 2 X fitted extent = 1.758621 x 1.758621, not incorporating fit results [Tue Mar 27 03:07:38 2012] Vigneting correction estimate = 1.000000 [Tue Mar 27 03:07:38 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Tue Mar 27 03:07:38 2012] Assessing source extent using major [Tue Mar 27 03:07:38 2012] Source does appear to be extended [Tue Mar 27 03:07:38 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Tue Mar 27 03:07:38 2012] Source is confused with source 2 [Tue Mar 27 03:08:05 2012] XMMSAS src. selection expression = ellipse(25728.146637, 26216.284393, 652.500000, 652.500000, 0.000000, X, Y) [Tue Mar 27 03:08:05 2012] Writing source region out to fullrun_pn_xmm0650383901_pi300-10000_pass1_cl_src21_src.reg [Tue Mar 27 03:08:05 2012] Extracting stamp from image fullrun_pn_xmm0650383901_pi300-10000_cl_sm2.00.img.gz, (259, 264) - (334, 339) [Tue Mar 27 03:08:05 2012] XMMSAS bgd. selection expression = annulus(25728.146637, 26216.284393, 1087.500000, 2175.000000, X, Y) && !ellipse(26541.464000, 26110.706000, 1099.584032, 1099.584032, 0.000000, X, Y) && !ellipse(27557.291901, 27589.813354, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27835.984000, 26755.634000, 1129.032032, 596.413617, 90.000000, X, Y) && !ellipse(28372.096497, 28648.628418, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27191.922699, 28617.105255, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27892.170746, 28478.717163, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26716.231720, 27696.038422, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25738.703033, 27661.576141, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(28416.825775, 26928.891602, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26755.985474, 26569.936951, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(28414.345978, 26393.627075, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26404.658722, 24490.217987, 870.000000, 870.000000, 0.000000, X, Y) [Tue Mar 27 03:08:05 2012] Writing fullrun_pn_xmm0650383901_pi300-10000_pass1_cl_src21.gif [Tue Mar 27 03:22:27 2012] Mean detx,y = (-1168.21, 1230.63) [Tue Mar 27 03:22:32 2012] Setting backscal keywords in source and bgd. spectrum [Tue Mar 27 03:23:02 2012] Binned source spectrum to 10 counts/bin [Tue Mar 27 03:23:03 2012] Setting source spectrum file to fullrun_pn_xmm0650383901_pi300-10000_pass1_cl_src21_src_b10.pi.gz [Tue Mar 27 03:23:03 2012] Setting bgd. spectrum file to fullrun_pn_xmm0650383901_pi300-10000_pass1_cl_src21_bgd.pi.gz [Tue Mar 27 04:01:16 2012] Not generating rmf since there are only 52 counts [Tue Mar 27 04:01:16 2012] rmf not generated due to insufficient counts [Tue Mar 27 04:44:15 2012] Updating aperture counts using extracted products [Tue Mar 27 04:44:15 2012] Error reading totcts from fullrun_pn_xmm0650383901_pi300-10000_pass1_cl_src21_src_b10.pi.gz [Tue Mar 27 04:44:17 2012] Calculating source flux in energy range 0.30-8.00 [Tue Mar 27 04:44:17 2012] Using photon index=1.80, rate=0.0106, arf fullrun_pn_xmm0650383901_pi300-10000_pass1_cl_src21.arf [Tue Mar 27 04:44:17 2012] Assuming count rate is from the 0.30-10.00 bandpass [Tue Mar 27 04:44:17 2012] Updating source flux to 3.2e-14 [Tue Mar 27 04:44:39 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting