[Thu Jun 14 14:26:50 2012] Detection parameters: Position = (280.1, 305.1) = 16 5 0.59 23 58 4.3 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 79.8 +/- 17.5 Background counts = 84.3 Rate = 0.006 +/- 0.001 [Thu Jun 14 14:26:51 2012] Off-axis axis estimate = 1.42' [Thu Jun 14 14:28:43 2012] Using EEF radius (= 7.14 ")to estimate initial spatial extent for simple fitting [Thu Jun 14 14:28:43 2012] Initial guess for spatial extent in simple fitting = 7.14" [Thu Jun 14 14:28:43 2012] source mask rpix=1.6, npix_max = 18, mask sum = 16, frac = 0.873 [Thu Jun 14 14:28:43 2012] Giving source the simple spatial ID 13 for pass 0, mean size = 7.14" [Thu Jun 14 15:59:55 2012] fullrun_pn_xmm0093060401_pi300-10000_cl_pass0_src13.ximg exists [Thu Jun 14 15:59:55 2012] fullrun_pn_xmm0093060401_pi300-10000_cl_pass0_src13_1.ximg exists [Thu Jun 14 15:59:55 2012] Fit fullrun_pn_xmm0093060401_pi300-10000_cl_pass0_src13 appears to have run properly [Thu Jun 14 15:59:56 2012] fullrun_pn_xmm0093060401_pi300-10000_cl_pass0_tfrozen_src13.ximg exists [Thu Jun 14 15:59:56 2012] fullrun_pn_xmm0093060401_pi300-10000_cl_pass0_tfrozen_src13_1.ximg exists [Thu Jun 14 15:59:56 2012] Fit fullrun_pn_xmm0093060401_pi300-10000_cl_pass0_tfrozen_src13 appears to have run properly [Thu Jun 14 18:27:52 2012] Warning, spatial fit 13 centroid is now closest to src. 15 [Thu Jun 14 18:27:52 2012] Source 13 is offset by 1.897995 and 8.784212 pixels which is larger than 2 X fitted extent = 1.684612 x 1.684612, not incorporating fit results [Thu Jun 14 18:27:52 2012] Vigneting correction estimate = 1.000000 [Thu Jun 14 18:27:52 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Thu Jun 14 18:27:52 2012] Assessing source extent using major [Thu Jun 14 18:27:52 2012] Source does appear to be extended [Thu Jun 14 18:27:52 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Thu Jun 14 18:28:14 2012] Using EEF radius (= 7.14 ")to estimate initial spatial extent for simple fitting [Thu Jun 14 18:28:14 2012] Initial guess for spatial extent in simple fitting = 7.14" [Thu Jun 14 18:28:14 2012] source mask rpix=1.6, npix_max = 18, mask sum = 16, frac = 0.873 [Thu Jun 14 18:28:14 2012] Giving source the simple spatial ID 9 for pass 1, mean size = 7.14" [Thu Jun 14 20:05:44 2012] fullrun_pn_xmm0093060401_pi300-10000_cl_pass1_src9.ximg exists [Thu Jun 14 20:05:44 2012] fullrun_pn_xmm0093060401_pi300-10000_cl_pass1_src9_1.ximg exists [Thu Jun 14 20:05:44 2012] Fit fullrun_pn_xmm0093060401_pi300-10000_cl_pass1_src9 appears to have run properly [Thu Jun 14 20:05:45 2012] fullrun_pn_xmm0093060401_pi300-10000_cl_pass1_tfrozen_src9.ximg exists [Thu Jun 14 20:05:45 2012] fullrun_pn_xmm0093060401_pi300-10000_cl_pass1_tfrozen_src9_1.ximg exists [Thu Jun 14 20:05:45 2012] Fit fullrun_pn_xmm0093060401_pi300-10000_cl_pass1_tfrozen_src9 appears to have run properly [Thu Jun 14 22:08:17 2012] Source 13 is offset by 5.285696 and -7.448339 pixels which is larger than 2 X fitted extent = 0.820313 x 0.820313, not incorporating fit results [Thu Jun 14 22:08:17 2012] Vigneting correction estimate = 1.000000 [Thu Jun 14 22:08:17 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Thu Jun 14 22:08:17 2012] Assessing source extent using major [Thu Jun 14 22:08:17 2012] Source does appear to be extended [Thu Jun 14 22:08:17 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Thu Jun 14 22:08:36 2012] XMMSAS src. selection expression = ellipse(24318.299530, 26496.432465, 652.500000, 652.500000, 0.000000, X, Y) [Thu Jun 14 22:08:36 2012] Writing source region out to fullrun_pn_xmm0093060401_pi300-10000_pass1_cl_src13_src.reg [Thu Jun 14 22:08:36 2012] Extracting stamp from image fullrun_pn_xmm0093060401_pi300-10000_cl_sm2.00.img.gz, (243, 268) - (318, 343) [Thu Jun 14 22:08:36 2012] XMMSAS bgd. selection expression = annulus(24318.299530, 26496.432465, 1087.500000, 2175.000000, X, Y) && !ellipse(25473.306200, 24458.364000, 1098.272032, 1098.272032, 0.000000, X, Y) && !ellipse(25414.695560, 24015.006000, 2012.960058, 2012.960058, 0.000000, X, Y) && !ellipse(25631.216827, 26654.220856, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25152.977020, 26652.662354, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26296.437073, 26559.800049, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26469.645874, 26127.056824, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25063.462708, 25782.457916, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26662.289490, 25693.086975, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27222.399780, 25241.524902, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(23457.199188, 25112.601990, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(23769.868713, 24664.743683, 870.000000, 870.000000, 0.000000, X, Y) [Thu Jun 14 22:08:36 2012] Writing fullrun_pn_xmm0093060401_pi300-10000_pass1_cl_src13.gif [Thu Jun 14 22:20:35 2012] Mean detx,y = (94.77, 2691.11) [Thu Jun 14 22:20:37 2012] Setting backscal keywords in source and bgd. spectrum [Thu Jun 14 22:20:48 2012] Binned source spectrum to 10 counts/bin [Thu Jun 14 22:20:49 2012] Setting source spectrum file to fullrun_pn_xmm0093060401_pi300-10000_pass1_cl_src13_src_b10.pi.gz [Thu Jun 14 22:20:49 2012] Setting bgd. spectrum file to fullrun_pn_xmm0093060401_pi300-10000_pass1_cl_src13_bgd.pi.gz [Fri Jun 15 10:26:36 2012] Not generating rmf since there are only 79 counts [Fri Jun 15 10:26:36 2012] rmf not generated due to insufficient counts [Fri Jun 15 13:23:33 2012] Updating aperture counts using extracted products [Fri Jun 15 13:23:33 2012] Error reading totcts from fullrun_pn_xmm0093060401_pi300-10000_pass1_cl_src13_src_b10.pi.gz [Fri Jun 15 13:23:34 2012] Calculating source flux in energy range 0.30-8.00 [Fri Jun 15 13:23:34 2012] Using photon index=1.80, rate=0.00557, arf fullrun_pn_xmm0093060401_pi300-10000_pass1_cl_src13.arf [Fri Jun 15 13:23:34 2012] Assuming count rate is from the 0.30-10.00 bandpass [Fri Jun 15 13:23:34 2012] Updating source flux to 1.6e-14 [Fri Jun 15 13:24:52 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting