[Sat Jul 7 14:41:04 2012] Detection parameters: Position = (266.2, 273.4) = 18 52 43.75 0 39 55.9 Extent = 10.9" x 10.9", rotation angle = 0 degrees Source counts = 76.9 +/- 18.7 Background counts = 115.4 Rate = 0.004 +/- 0.001 [Sat Jul 7 14:41:04 2012] Off-axis axis estimate = 2.96' [Sat Jul 7 18:01:01 2012] Using EEF radius (= 7.91 ")to estimate initial spatial extent for simple fitting [Sat Jul 7 18:01:01 2012] Initial guess for spatial extent in simple fitting = 7.91" [Sat Jul 7 18:01:01 2012] source mask rpix=1.8, npix_max = 21, mask sum = 20, frac = 0.930 [Sat Jul 7 18:01:01 2012] Giving source the simple spatial ID 41 for pass 0, mean size = 7.91" [Sat Jul 7 20:07:19 2012] fullrun_mos2_xmm0550671101_pi300-10000_cl_pass0_src41.ximg exists [Sat Jul 7 20:07:19 2012] fullrun_mos2_xmm0550671101_pi300-10000_cl_pass0_src41_1.ximg exists [Sat Jul 7 20:07:19 2012] Fit fullrun_mos2_xmm0550671101_pi300-10000_cl_pass0_src41 appears to have run properly [Sat Jul 7 20:07:21 2012] fullrun_mos2_xmm0550671101_pi300-10000_cl_pass0_tfrozen_src41.ximg exists [Sat Jul 7 20:07:21 2012] fullrun_mos2_xmm0550671101_pi300-10000_cl_pass0_tfrozen_src41_1.ximg exists [Sat Jul 7 20:07:21 2012] Fit fullrun_mos2_xmm0550671101_pi300-10000_cl_pass0_tfrozen_src41 appears to have run properly [Sat Jul 7 20:07:42 2012] Source 36 is offset by 2.596171 and 7.959310 pixels which is larger than 2 X fitted extent = 7.571127 x 7.571127, not incorporating fit results [Sat Jul 7 20:07:42 2012] Warning, spatial fit 41 centroid is now closest to src. 37 [Sat Jul 7 20:07:42 2012] Vigneting correction estimate = 1.000000 [Sat Jul 7 20:07:42 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Sat Jul 7 20:07:42 2012] Assessing source extent using major [Sat Jul 7 20:07:42 2012] Source does appear to be extended [Sat Jul 7 20:07:42 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Sat Jul 7 20:07:42 2012] Source is confused with source 35 [Sat Jul 7 23:28:03 2012] Using EEF radius (= 7.91 ")to estimate initial spatial extent for simple fitting [Sat Jul 7 23:28:03 2012] Initial guess for spatial extent in simple fitting = 7.91" [Sat Jul 7 23:28:03 2012] source mask rpix=1.8, npix_max = 21, mask sum = 20, frac = 0.930 [Sat Jul 7 23:28:03 2012] Giving source the simple spatial ID 40 for pass 1, mean size = 7.91" [Sun Jul 8 01:55:34 2012] fullrun_mos2_xmm0550671101_pi300-10000_cl_pass1_src40.ximg exists [Sun Jul 8 01:55:34 2012] Warning: poor agreement between model and actual number of counts may be indicative of a poor fit in csv/fullrun_mos2_xmm0550671101_pi300-10000_cl_pass1_src40.csv [Sun Jul 8 01:55:34 2012] fullrun_mos2_xmm0550671101_pi300-10000_cl_pass1_src40_1.ximg exists [Sun Jul 8 01:55:34 2012] Warning: poor agreement between model and actual number of counts may be indicative of a poor fit in csv/fullrun_mos2_xmm0550671101_pi300-10000_cl_pass1_src40.csv [Sun Jul 8 01:55:34 2012] It looks like the fit did not converge You should probably delete fullrun_mos2_xmm0550671101_pi300-10000_cl_pass1_src40_1.ximg Either tweak this fit manually starting from fullrun_mos2_xmm0550671101_pi300-10000_cl_pass1_src40.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 [Sun Jul 8 01:55:35 2012] fullrun_mos2_xmm0550671101_pi300-10000_cl_pass1_tfrozen_src40.ximg exists [Sun Jul 8 01:55:35 2012] fullrun_mos2_xmm0550671101_pi300-10000_cl_pass1_tfrozen_src40_1.ximg exists [Sun Jul 8 01:55:35 2012] Fit fullrun_mos2_xmm0550671101_pi300-10000_cl_pass1_tfrozen_src40 appears to have run properly [Sun Jul 8 01:55:55 2012] Warning: source 23 in spatial fitting list does not appear to have a counterpart in memory, closest src. was src. 36 at 12.165412 pixels away [Sun Jul 8 01:55:55 2012] Warning, spatial fit 40 centroid is now closest to src. 45 [Sun Jul 8 01:55:55 2012] Vigneting correction estimate = 1.000000 [Sun Jul 8 01:55:55 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 [Sun Jul 8 01:55:55 2012] Assessing source extent using major [Sun Jul 8 01:55:55 2012] Source does appear to be extended [Sun Jul 8 01:55:55 2012] Computing asymmetry using major and minor axis, asym = 1.00 [Sun Jul 8 09:19:29 2012] XMMSAS src. selection expression = ellipse(23108.054871, 23736.271973, 652.500000, 652.500000, 0.000000, X, Y) [Sun Jul 8 09:19:29 2012] Writing source region out to fullrun_mos2_xmm0550671101_pi300-10000_pass1_cl_src36_src.reg [Sun Jul 8 09:19:29 2012] Extracting stamp from image fullrun_mos2_xmm0550671101_pi300-10000_cl_sm2.00.img.gz, (229, 236) - (304, 311) [Sun Jul 8 09:19:29 2012] XMMSAS bgd. selection expression = annulus(23108.054871, 23736.271973, 1087.500000, 2175.000000, X, Y) && !ellipse(24678.442000, 24267.241800, 303.646409, 303.646409, 0.000000, X, Y) && !ellipse(25753.386000, 22052.692600, 1280.504037, 1280.504037, 0.000000, X, Y) && !ellipse(24826.604000, 21283.794000, 1318.680038, 1318.680038, 0.000000, X, Y) && !ellipse(26041.598000, 22254.338000, 915.000026, 915.000026, 0.000000, X, Y) && !ellipse(25049.692000, 21429.978000, 1318.680038, 1318.680038, 0.000000, X, Y) && !ellipse(22994.021362, 22043.044296, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(21697.202000, 22886.388000, 1393.304040, 1393.304040, 0.000000, X, Y) && !ellipse(25196.678000, 24045.318000, 2353.312068, 1052.576030, 28.121100, X, Y) && !ellipse(23492.200439, 21011.967651, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(23746.615967, 22920.086761, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22343.191400, 23856.168000, 1206.512035, 1206.512035, 0.000000, X, Y) && !ellipse(24858.871460, 22103.576309, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(24634.232000, 26783.588000, 1491.184043, 1491.184043, 0.000000, X, Y) && !ellipse(26538.586000, 22638.160000, 1627.896047, 1627.896047, 0.000000, X, Y) && !ellipse(26145.638000, 23393.708000, 1176.656034, 1176.656034, 0.000000, X, Y) && !ellipse(25238.139740, 24898.970367, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(21614.677732, 24816.018200, 878.224025, 878.224025, 0.000000, X, Y) && !ellipse(26254.110000, 24743.668000, 1148.680033, 1148.680033, 0.000000, X, Y) && !ellipse(21387.634384, 22832.842499, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(21343.499832, 23266.740662, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25019.260000, 26682.914000, 2096.784060, 621.151218, 46.082000, X, Y) && !ellipse(25702.678000, 26035.398540, 1048.392030, 1048.392030, 0.000000, X, Y) && !ellipse(24192.946000, 22869.574000, 1292.280037, 1292.280037, 0.000000, X, Y) && !ellipse(26556.976000, 25149.257400, 2194.816063, 2194.816063, 0.000000, X, Y) && !ellipse(23639.671387, 23700.267120, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(21593.825000, 26361.562000, 1320.152038, 1320.152038, 0.000000, X, Y) [Sun Jul 8 09:19:29 2012] Writing fullrun_mos2_xmm0550671101_pi300-10000_pass1_cl_src36.gif [Sun Jul 8 09:27:02 2012] Mean detx,y = (-1556.82, 691.89) [Sun Jul 8 09:27:03 2012] Setting backscal keywords in source and bgd. spectrum [Sun Jul 8 09:27:08 2012] Binned source spectrum to 10 counts/bin [Sun Jul 8 09:27:08 2012] Setting source spectrum file to fullrun_mos2_xmm0550671101_pi300-10000_pass1_cl_src36_src_b10.pi.gz [Sun Jul 8 09:27:08 2012] Setting bgd. spectrum file to fullrun_mos2_xmm0550671101_pi300-10000_pass1_cl_src36_bgd.pi.gz [Sun Jul 8 11:36:49 2012] Not generating rmf since there are only 76 counts [Sun Jul 8 11:36:49 2012] rmf not generated due to insufficient counts [Sun Jul 8 11:37:49 2012] Updating aperture counts using extracted products [Sun Jul 8 11:37:49 2012] Error reading totcts from fullrun_mos2_xmm0550671101_pi300-10000_pass1_cl_src36_src_b10.pi.gz [Sun Jul 8 11:37:49 2012] Calculating source flux in energy range 0.30-8.00 [Sun Jul 8 11:37:49 2012] Using photon index=1.80, rate=0.00425, arf fullrun_mos2_xmm0550671101_pi300-10000_pass1_cl_src36.arf [Sun Jul 8 11:37:49 2012] Assuming count rate is from the 0.30-10.00 bandpass [Sun Jul 8 11:37:49 2012] Updating source flux to 4.2e-14 [Sun Jul 8 11:45:10 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting