[Mon Feb 13 00:06:50 2012] Detection parameters: Position = (312.9, 289.0) = 17 28 19.13 -14 17 59.5 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 555.8 +/- 39.4 Background counts = 186.1 Rate = 0.007 +/- 0.0005 [Mon Feb 13 00:06:51 2012] Off-axis axis estimate = 1.25' [Mon Feb 13 00:12:41 2012] Using EEF radius (= 7.05 ")to estimate initial spatial extent for simple fitting [Mon Feb 13 00:12:41 2012] Initial guess for spatial extent in simple fitting = 7.05" [Mon Feb 13 00:12:41 2012] source mask rpix=1.6, npix_max = 18, mask sum = 16, frac = 0.889 [Mon Feb 13 00:12:41 2012] Giving source the simple spatial ID 31 for pass 0, mean size = 7.05" [Mon Feb 13 02:42:44 2012] fullrun_pn_xmm0501580101_pi300-10000_cl_pass0_src31.ximg exists [Mon Feb 13 02:42:44 2012] Warning: poor agreement between model and actual number of counts may be indicative of a poor fit in csv/fullrun_pn_xmm0501580101_pi300-10000_cl_pass0_src31.csv [Mon Feb 13 02:42:44 2012] fullrun_pn_xmm0501580101_pi300-10000_cl_pass0_src31_1.ximg exists [Mon Feb 13 02:42:44 2012] Warning: poor agreement between model and actual number of counts may be indicative of a poor fit in csv/fullrun_pn_xmm0501580101_pi300-10000_cl_pass0_src31.csv [Mon Feb 13 02:42:44 2012] It looks like the fit did not converge You should probably delete fullrun_pn_xmm0501580101_pi300-10000_cl_pass0_src31_1.ximg Either tweak this fit manually starting from fullrun_pn_xmm0501580101_pi300-10000_cl_pass0_src31.ximg or adjust the simplespatial fit parameters in $XASSIST/data/missions/*/*/spatial.dat and re-run simplespatial fitting after setting file recreation parameter to yes [Mon Feb 13 02:42:45 2012] fullrun_pn_xmm0501580101_pi300-10000_cl_pass0_tfrozen_src31.ximg exists [Mon Feb 13 02:42:45 2012] fullrun_pn_xmm0501580101_pi300-10000_cl_pass0_tfrozen_src31_1.ximg exists [Mon Feb 13 02:42:45 2012] Fit fullrun_pn_xmm0501580101_pi300-10000_cl_pass0_tfrozen_src31 appears to have run properly [Mon Feb 13 05:22:33 2012] Warning, spatial fit 31 centroid is now closest to src. 34 [Mon Feb 13 05:22:33 2012] Source 33 is offset by 6.574865 and 1.432737 pixels which is larger than 2 X fitted extent = 1.266612 x 1.266612, not incorporating fit results [Mon Feb 13 05:22:33 2012] Vigneting correction estimate = 1.000000 [Mon Feb 13 05:22:33 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Mon Feb 13 05:22:33 2012] Assessing source extent using major [Mon Feb 13 05:22:33 2012] Source does appear to be extended [Mon Feb 13 05:22:33 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Mon Feb 13 05:22:33 2012] Source is confused with source 34 [Mon Feb 13 05:22:53 2012] Using EEF radius (= 7.05 ")to estimate initial spatial extent for simple fitting [Mon Feb 13 05:22:53 2012] Initial guess for spatial extent in simple fitting = 7.05" [Mon Feb 13 05:22:53 2012] source mask rpix=1.6, npix_max = 18, mask sum = 16, frac = 0.889 [Mon Feb 13 05:22:53 2012] Giving source the simple spatial ID 29 for pass 1, mean size = 7.05" [Mon Feb 13 07:15:28 2012] fullrun_pn_xmm0501580101_pi300-10000_cl_pass1_src29.ximg exists [Mon Feb 13 07:15:28 2012] fullrun_pn_xmm0501580101_pi300-10000_cl_pass1_src29_1.ximg exists [Mon Feb 13 07:15:28 2012] Fit fullrun_pn_xmm0501580101_pi300-10000_cl_pass1_src29 appears to have run properly [Mon Feb 13 07:15:29 2012] fullrun_pn_xmm0501580101_pi300-10000_cl_pass1_tfrozen_src29.ximg exists [Mon Feb 13 07:15:29 2012] fullrun_pn_xmm0501580101_pi300-10000_cl_pass1_tfrozen_src29_1.ximg exists [Mon Feb 13 07:15:29 2012] Fit fullrun_pn_xmm0501580101_pi300-10000_cl_pass1_tfrozen_src29 appears to have run properly [Mon Feb 13 10:17:12 2012] Warning, spatial fit 29 centroid is now closest to src. 34 [Mon Feb 13 10:17:12 2012] Spatial fit model total counts = 4202.320000, observed total counts = 4203.000000 [Mon Feb 13 10:17:12 2012] Offset between fit and detection position for source 33 = 6.043737 pixels [Mon Feb 13 10:17:12 2012] Warning, changing simple spatial fit ID from 29 to 30 [Mon Feb 13 10:17:12 2012] 4015.887000 total counts/ 3115.690000 bgd. counts: snr = 16.127255 Spatial fit parameters: Offset between fit and detection position for source 33 = 6.043737 pixels Position = (313.1, 282.9) = 17 28 19.06 -14 18 25.1 Extent = 19.0 (19.0-38.0)" x 5.1 (4.4-5.6)", rotation angle = 87 (85-89) degrees Source counts = 900.2 +/- 63.4 Background counts = 3115.7 Rate = 0.01 +/- 0.0007 [Mon Feb 13 10:17:12 2012] Vigneting correction estimate = 1.000000 [Mon Feb 13 10:17:12 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Mon Feb 13 10:17:12 2012] Assessing source extent using major axis lower bound [Mon Feb 13 10:17:12 2012] Source does appear to be extended [Mon Feb 13 10:17:12 2012] Computing asymmetry using errors on major and minor axis (from spatial fitting), asym = 3.40 [Mon Feb 13 10:17:12 2012] Source is asymmetric [Mon Feb 13 10:17:48 2012] XMMSAS src. selection expression = ellipse(27191.641020, 24567.574000, 1140.972033, 303.975009, 86.866130, X, Y) [Mon Feb 13 10:17:48 2012] Writing source region out to fullrun_pn_xmm0501580101_pi300-10000_pass1_cl_src33_src.reg [Mon Feb 13 10:17:48 2012] Extracting stamp from image fullrun_pn_xmm0501580101_pi300-10000_cl_sm2.00.img.gz, (248, 217) - (379, 349) [Mon Feb 13 10:17:48 2012] XMMSAS bgd. selection expression = annulus(27191.641020, 24567.574000, 1901.620055, 3803.240109, X, Y) && !ellipse(26984.752000, 27556.276600, 1558.332045, 1558.332045, 0.000000, X, Y) && !ellipse(30946.368200, 26721.199800, 480.096014, 480.096014, 0.000000, X, Y) && !ellipse(30794.454956, 21273.541138, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26716.114899, 28967.314240, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(23795.889180, 25306.943800, 411.351212, 411.351212, 0.000000, X, Y) && !ellipse(27197.565200, 24808.010000, 927.560027, 927.560027, 0.000000, X, Y) && !ellipse(30741.744659, 24493.345612, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27207.844200, 24216.947200, 737.041621, 737.041621, 0.000000, X, Y) && !ellipse(25780.616180, 24204.548500, 464.552813, 464.552813, 0.000000, X, Y) && !ellipse(27268.218690, 23448.900000, 588.058417, 588.058417, 0.000000, X, Y) && !ellipse(27266.951240, 23102.400800, 764.286422, 764.286422, 0.000000, X, Y) && !ellipse(27334.529633, 22051.341263, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27438.175340, 20687.088000, 654.483219, 654.483219, 0.000000, X, Y) && !ellipse(27466.026800, 20340.674000, 865.240025, 865.240025, 0.000000, X, Y) && !ellipse(28037.358000, 29485.074000, 1337.168038, 360.903210, 124.360000, X, Y) && !ellipse(26354.696381, 24308.677704, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(31194.377320, 22361.165800, 552.686416, 552.686416, 0.000000, X, Y) && !ellipse(24315.721000, 21225.996000, 2736.288079, 1260.128036, 90.000000, X, Y) && !ellipse(25794.033844, 20174.203690, 870.000000, 870.000000, 0.000000, X, Y) [Mon Feb 13 10:17:48 2012] Writing fullrun_pn_xmm0501580101_pi300-10000_pass1_cl_src33.gif [Mon Feb 13 11:18:20 2012] Mean detx,y = (128.02, 2872.37) [Mon Feb 13 11:18:27 2012] Setting backscal keywords in source and bgd. spectrum [Mon Feb 13 11:19:19 2012] Binned source spectrum to 10 counts/bin [Mon Feb 13 11:19:20 2012] Setting source spectrum file to fullrun_pn_xmm0501580101_pi300-10000_pass1_cl_src33_src_b10.pi.gz [Mon Feb 13 11:19:20 2012] Setting bgd. spectrum file to fullrun_pn_xmm0501580101_pi300-10000_pass1_cl_src33_bgd.pi.gz [Mon Feb 13 16:22:05 2012] Updating aperture counts using extracted products [Mon Feb 13 16:22:05 2012] Error reading totcts from fullrun_pn_xmm0501580101_pi300-10000_pass1_cl_src33_src_b10.pi.gz [Mon Feb 13 16:22:06 2012] Calculating source flux in energy range 0.30-8.00 [Mon Feb 13 16:22:06 2012] Using photon index=1.80, rate=0.0102, arf fullrun_pn_xmm0501580101_pi300-10000_pass1_cl_src33.arf [Mon Feb 13 16:22:06 2012] Assuming count rate is from the 0.30-10.00 bandpass [Mon Feb 13 16:22:06 2012] Updating source flux to 3.1e-14 [Mon Feb 13 16:25:12 2012] Flag b found in src. 33 procflags, skipping spectral fitting [Mon Feb 13 16:25:12 2012] Flag c found in src. 33 procflags, skipping spectral fitting