[Tue Mar 13 23:04:03 2012] Detection parameters: Position = (292.8, 259.6) = 1 8 19.31 -73 13 17.7 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 63.2 +/- 13.8 Background counts = 49.2 Rate = 0.002 +/- 0.0005 [Tue Mar 13 23:04:05 2012] Off-axis axis estimate = 2.84' [Tue Mar 13 23:09:11 2012] Using EEF radius (= 7.85 ")to estimate initial spatial extent for simple fitting [Tue Mar 13 23:09:11 2012] Initial guess for spatial extent in simple fitting = 7.85" [Tue Mar 13 23:09:11 2012] source mask rpix=1.8, npix_max = 21, mask sum = 25, frac = 1.177 [Tue Mar 13 23:09:11 2012] Giving source the simple spatial ID 51 for pass 0, mean size = 7.85" [Wed Mar 14 02:57:45 2012] fullrun_pn_xmm0601212701_pi300-10000_cl_pass0_src51.ximg exists [Wed Mar 14 02:57:45 2012] fullrun_pn_xmm0601212701_pi300-10000_cl_pass0_src51_1.ximg exists [Wed Mar 14 02:57:45 2012] Fit fullrun_pn_xmm0601212701_pi300-10000_cl_pass0_src51 appears to have run properly [Wed Mar 14 02:57:47 2012] fullrun_pn_xmm0601212701_pi300-10000_cl_pass0_tfrozen_src51.ximg exists [Wed Mar 14 02:57:47 2012] fullrun_pn_xmm0601212701_pi300-10000_cl_pass0_tfrozen_src51_1.ximg exists [Wed Mar 14 02:57:47 2012] Fit fullrun_pn_xmm0601212701_pi300-10000_cl_pass0_tfrozen_src51 appears to have run properly [Wed Mar 14 05:27:55 2012] Warning, spatial fit 51 centroid is now closest to src. 59 [Wed Mar 14 05:27:55 2012] Vigneting correction estimate = 1.000000 [Wed Mar 14 05:27:55 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Wed Mar 14 05:27:55 2012] Assessing source extent using major [Wed Mar 14 05:27:55 2012] Source does appear to be extended [Wed Mar 14 05:27:55 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Wed Mar 14 05:28:28 2012] Using EEF radius (= 7.85 ")to estimate initial spatial extent for simple fitting [Wed Mar 14 05:28:28 2012] Initial guess for spatial extent in simple fitting = 7.85" [Wed Mar 14 05:28:28 2012] source mask rpix=1.8, npix_max = 21, mask sum = 25, frac = 1.177 [Wed Mar 14 05:28:28 2012] Giving source the simple spatial ID 50 for pass 1, mean size = 7.85" [Wed Mar 14 08:37:38 2012] fullrun_pn_xmm0601212701_pi300-10000_cl_pass1_src50.ximg exists [Wed Mar 14 08:37:38 2012] fullrun_pn_xmm0601212701_pi300-10000_cl_pass1_src50_1.ximg exists [Wed Mar 14 08:37:38 2012] Fit fullrun_pn_xmm0601212701_pi300-10000_cl_pass1_src50 appears to have run properly [Wed Mar 14 08:37:41 2012] fullrun_pn_xmm0601212701_pi300-10000_cl_pass1_tfrozen_src50.ximg exists [Wed Mar 14 08:37:41 2012] fullrun_pn_xmm0601212701_pi300-10000_cl_pass1_tfrozen_src50_1.ximg exists [Wed Mar 14 08:37:41 2012] Fit fullrun_pn_xmm0601212701_pi300-10000_cl_pass1_tfrozen_src50 appears to have run properly [Wed Mar 14 11:26:48 2012] Source 52 is offset by -7.438428 and 5.864698 pixels which is larger than 2 X fitted extent = 7.218023 x 7.218023, not incorporating fit results [Wed Mar 14 11:26:48 2012] Vigneting correction estimate = 1.000000 [Wed Mar 14 11:26:48 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Wed Mar 14 11:26:48 2012] Assessing source extent using major [Wed Mar 14 11:26:48 2012] Source does appear to be extended [Wed Mar 14 11:26:48 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Wed Mar 14 11:27:31 2012] XMMSAS src. selection expression = ellipse(25423.322723, 22540.762726, 652.500000, 652.500000, 0.000000, X, Y) [Wed Mar 14 11:27:31 2012] Writing source region out to fullrun_pn_xmm0601212701_pi300-10000_pass1_cl_src52_src.reg [Wed Mar 14 11:27:31 2012] Extracting stamp from image fullrun_pn_xmm0601212701_pi300-10000_cl_sm2.00.img.gz, (255, 222) - (330, 297) [Wed Mar 14 11:27:31 2012] XMMSAS bgd. selection expression = annulus(25423.322723, 22540.762726, 1087.500000, 2175.000000, X, Y) && !ellipse(23288.426941, 25077.624634, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26443.098000, 24603.028400, 650.273619, 650.273619, 0.000000, X, Y) && !ellipse(25520.495800, 24438.464000, 355.973610, 355.973610, 0.000000, X, Y) && !ellipse(24864.165588, 24422.825378, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22987.779388, 23458.383331, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22410.706116, 23120.963623, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22675.688660, 22566.179321, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(24151.701752, 22459.980804, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22982.363129, 21581.750214, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25921.908000, 21301.412400, 246.150407, 246.150407, 0.000000, X, Y) && !ellipse(23141.978180, 20284.370148, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(24633.419800, 20156.103800, 430.207212, 430.207212, 0.000000, X, Y) && !ellipse(23240.901917, 19680.708084, 870.000000, 870.000000, 0.000000, X, Y) [Wed Mar 14 11:27:31 2012] Writing fullrun_pn_xmm0601212701_pi300-10000_pass1_cl_src52.gif [Wed Mar 14 12:32:03 2012] Mean detx,y = (-473.18, 4847.41) [Wed Mar 14 12:32:09 2012] Setting backscal keywords in source and bgd. spectrum [Wed Mar 14 12:32:39 2012] Binned source spectrum to 10 counts/bin [Wed Mar 14 12:32:39 2012] Setting source spectrum file to fullrun_pn_xmm0601212701_pi300-10000_pass1_cl_src52_src_b10.pi.gz [Wed Mar 14 12:32:39 2012] Setting bgd. spectrum file to fullrun_pn_xmm0601212701_pi300-10000_pass1_cl_src52_bgd.pi.gz [Wed Mar 14 13:31:09 2012] Not generating rmf since there are only 63 counts [Wed Mar 14 13:31:09 2012] rmf not generated due to insufficient counts [Wed Mar 14 15:29:40 2012] Updating aperture counts using extracted products [Wed Mar 14 15:29:40 2012] Error reading totcts from fullrun_pn_xmm0601212701_pi300-10000_pass1_cl_src52_src_b10.pi.gz [Wed Mar 14 15:29:44 2012] Calculating source flux in energy range 0.30-8.00 [Wed Mar 14 15:29:44 2012] Using photon index=1.80, rate=0.00245, arf fullrun_pn_xmm0601212701_pi300-10000_pass1_cl_src52.arf [Wed Mar 14 15:29:44 2012] Assuming count rate is from the 0.30-10.00 bandpass [Wed Mar 14 15:29:45 2012] Updating source flux to 7.5e-15 [Wed Mar 14 15:32:27 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting