[Fri May 4 10:28:54 2012] Detection parameters: Position = (237.2, 269.1) = 5 36 37.77 -69 18 7.1 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 163.6 +/- 29.4 Background counts = 362.7 Rate = 0.002 +/- 0.0004 [Fri May 4 10:29:05 2012] Off-axis axis estimate = 4.92' [Fri May 4 10:41:37 2012] Using EEF radius (= 8.89 ")to estimate initial spatial extent for simple fitting [Fri May 4 10:41:37 2012] Initial guess for spatial extent in simple fitting = 8.89" [Fri May 4 10:41:37 2012] source mask rpix=2.0, npix_max = 25, mask sum = 25, frac = 0.966 [Fri May 4 10:41:37 2012] Giving source the simple spatial ID 101 for pass 0, mean size = 8.89" [Sat May 5 02:16:35 2012] Vigneting correction estimate = 1.000000 [Sat May 5 02:16:35 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Sat May 5 02:16:35 2012] Assessing source extent using major [Sat May 5 02:16:35 2012] Source does appear to be extended [Sat May 5 02:16:35 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Sat May 5 02:17:05 2012] Using EEF radius (= 8.89 ")to estimate initial spatial extent for simple fitting [Sat May 5 02:17:05 2012] Initial guess for spatial extent in simple fitting = 8.89" [Sat May 5 02:17:05 2012] source mask rpix=2.0, npix_max = 25, mask sum = 25, frac = 0.966 [Sat May 5 02:17:05 2012] Giving source the simple spatial ID 96 for pass 1, mean size = 8.89" [Sat May 5 15:53:54 2012] fullrun_pn_xmm0506220101_pi300-10000_cl_pass1_src96.ximg exists [Sat May 5 15:53:54 2012] fullrun_pn_xmm0506220101_pi300-10000_cl_pass1_src96_1.ximg exists [Sat May 5 15:53:54 2012] Fit fullrun_pn_xmm0506220101_pi300-10000_cl_pass1_src96 appears to have run properly [Sat May 5 15:53:57 2012] fullrun_pn_xmm0506220101_pi300-10000_cl_pass1_tfrozen_src96.ximg exists [Sat May 5 15:53:57 2012] fullrun_pn_xmm0506220101_pi300-10000_cl_pass1_tfrozen_src96_1.ximg exists [Sat May 5 15:53:57 2012] Fit fullrun_pn_xmm0506220101_pi300-10000_cl_pass1_tfrozen_src96 appears to have run properly [Sat May 5 16:03:19 2012] Spatial fit model total counts = 3769.920000, observed total counts = 3690.000000 [Sat May 5 16:03:19 2012] Offset between fit and detection position for source 106 = 1.045324 pixels [Sat May 5 16:03:19 2012] 3709.077000 total counts/ 3505.180000 bgd. counts: snr = 3.443941 Spatial fit parameters: Offset between fit and detection position for source 106 = 1.045324 pixels Position = (236.5, 269.8) = 5 36 38.37 -69 18 5.5 Extent = 17.8 (11.2-35.6)" x 4.5 (2.8-6.8)", rotation angle = 30 (20-41) degrees Source counts = 203.9 +/- 60.9 Background counts = 3505.2 Rate = 0.002 +/- 0.0006 [Sat May 5 16:03:19 2012] Vigneting correction estimate = 1.000000 [Sat May 5 16:03:19 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Sat May 5 16:03:19 2012] Assessing source extent using major axis lower bound [Sat May 5 16:03:19 2012] Source does appear to be extended [Sat May 5 16:03:19 2012] Computing asymmetry using errors on major and minor axis (from spatial fitting), asym = 1.65 [Sat May 5 16:03:19 2012] Source is asymmetric [Sat May 5 16:03:19 2012] Source is confused with source 111 [Sat May 5 16:04:04 2012] XMMSAS src. selection expression = ellipse(20525.761000, 23425.120420, 1066.794031, 269.883008, 30.492000, X, Y) [Sat May 5 16:04:04 2012] Writing source region out to fullrun_pn_xmm0506220101_pi300-10000_pass1_cl_src106_src.reg [Sat May 5 16:04:04 2012] Extracting stamp from image fullrun_pn_xmm0506220101_pi300-10000_cl_sm2.00.img.gz, (175, 209) - (298, 331) [Sat May 5 16:04:04 2012] XMMSAS bgd. selection expression = annulus(20525.761000, 23425.120420, 1777.990051, 3555.980102, X, Y) && !ellipse(15694.891969, 19301.173116, 1591.560046, 399.496856, 332.836670, X, Y) && !ellipse(23522.348297, 25520.117126, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(17839.735831, 20436.959824, 1760.872051, 352.919808, 333.878143, X, Y) && !ellipse(16697.680200, 19849.000400, 1760.872051, 407.964812, 331.530000, X, Y) && !ellipse(16762.664000, 19955.300000, 1794.472052, 1794.472052, 0.000000, X, Y) && !ellipse(22744.132660, 26729.305084, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(21963.170395, 26379.082825, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(23601.361969, 26431.132019, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22486.435516, 26153.243378, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(21501.541779, 26228.800201, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(23036.578827, 26122.097229, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25017.232000, 26076.974800, 1062.880031, 1062.880031, 0.000000, X, Y) && !ellipse(24661.708984, 25704.187653, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(23955.404816, 25772.453766, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(19292.163132, 25238.681366, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(18842.223282, 24743.685669, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(19966.989273, 24519.120636, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(19262.880814, 24594.749146, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(18843.884003, 24229.087891, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(24853.035706, 24060.766998, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(24397.716000, 23877.284000, 676.238419, 676.238419, 0.000000, X, Y) && !ellipse(18165.951477, 23706.875488, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(16925.758087, 23680.357056, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(17372.249054, 23284.396606, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22647.420563, 22914.800598, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(18884.549759, 22831.894653, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(19721.928741, 22827.705017, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(18526.404892, 22549.136688, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(24154.760345, 22611.025421, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22196.260000, 22692.690000, 1324.352038, 1324.352038, 0.000000, X, Y) && !ellipse(21266.136261, 22230.750885, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(19539.005188, 22049.444244, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(18974.191513, 22229.487091, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(20739.476685, 21948.703140, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(18297.849350, 22053.001984, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(17540.129211, 22230.527863, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(20115.739944, 21610.634277, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(19634.550400, 21357.454666, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(19086.089050, 21085.241150, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(17654.879578, 21177.668030, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(23424.810486, 20988.410904, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(18263.369812, 20644.266006, 870.000000, 870.000000, 0.000000, X, Y) [Sat May 5 16:04:04 2012] Writing fullrun_pn_xmm0506220101_pi300-10000_pass1_cl_src106.gif [Sat May 5 23:21:18 2012] Mean detx,y = (-1327.47, 7498.38) [Sat May 5 23:21:29 2012] Setting backscal keywords in source and bgd. spectrum [Sat May 5 23:22:21 2012] Binned source spectrum to 10 counts/bin [Sat May 5 23:22:22 2012] Setting source spectrum file to fullrun_pn_xmm0506220101_pi300-10000_pass1_cl_src106_src_b10.pi.gz [Sat May 5 23:22:22 2012] Setting bgd. spectrum file to fullrun_pn_xmm0506220101_pi300-10000_pass1_cl_src106_bgd.pi.gz [Sun May 6 11:35:47 2012] Updating aperture counts using extracted products [Sun May 6 11:35:47 2012] Error reading totcts from fullrun_pn_xmm0506220101_pi300-10000_pass1_cl_src106_src_b10.pi.gz [Sun May 6 11:36:03 2012] Calculating source flux in energy range 0.30-8.00 [Sun May 6 11:36:03 2012] Using photon index=1.80, rate=0.00213, arf fullrun_pn_xmm0506220101_pi300-10000_pass1_cl_src106.arf [Sun May 6 11:36:03 2012] Assuming count rate is from the 0.30-10.00 bandpass [Sun May 6 11:36:03 2012] Updating source flux to 8.6e-15 [Sun May 6 11:36:29 2012] Flag c found in src. 106 procflags, skipping spectral fitting