[Tue May 29 19:39:58 2012] Detection parameters:
  Position = (410.5, 331.3) = 2 49 1.63 -31 10 1.5
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 224.9 +/- 21.0
  Background counts = 52.1
  Rate = 0.01 +/- 0.0009

[Tue May 29 19:39:59 2012] Off-axis axis estimate = 8.46'
[Tue May 29 19:43:15 2012] Using EEF radius (= 10.66 ")to estimate initial spatial extent for simple fitting
[Tue May 29 19:43:15 2012] Initial guess for spatial extent in simple fitting = 10.66"
[Tue May 29 19:43:15 2012] source mask rpix=2.5, npix_max = 34, mask sum = 30, frac = 0.861
[Tue May 29 19:43:15 2012] Giving source the simple spatial ID 28 for pass 0, mean size = 10.66"
[Tue May 29 21:52:23 2012] fullrun_pn_xmm0146510401_pi300-10000_cl_pass0_src28.ximg exists
[Tue May 29 21:52:23 2012] fullrun_pn_xmm0146510401_pi300-10000_cl_pass0_src28_1.ximg exists
[Tue May 29 21:52:23 2012] Fit fullrun_pn_xmm0146510401_pi300-10000_cl_pass0_src28 appears to have run properly
[Tue May 29 21:52:24 2012] fullrun_pn_xmm0146510401_pi300-10000_cl_pass0_tfrozen_src28.ximg exists
[Tue May 29 21:52:24 2012] fullrun_pn_xmm0146510401_pi300-10000_cl_pass0_tfrozen_src28_1.ximg exists
[Tue May 29 21:52:24 2012] Fit fullrun_pn_xmm0146510401_pi300-10000_cl_pass0_tfrozen_src28 appears to have run properly
[Wed May 30 00:48:32 2012] Warning, spatial fit 28 centroid is now closest to src. 14
[Wed May 30 00:48:32 2012] Vigneting correction estimate = 1.000000
[Wed May 30 00:48:32 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Wed May 30 00:48:32 2012] Assessing source extent using major
[Wed May 30 00:48:32 2012] Source does appear to be extended
[Wed May 30 00:48:32 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Wed May 30 00:49:05 2012] Using EEF radius (= 10.66 ")to estimate initial spatial extent for simple fitting
[Wed May 30 00:49:05 2012] Initial guess for spatial extent in simple fitting = 10.66"
[Wed May 30 00:49:05 2012] source mask rpix=2.5, npix_max = 34, mask sum = 30, frac = 0.861
[Wed May 30 00:49:05 2012] Giving source the simple spatial ID 27 for pass 1, mean size = 10.66"
[Wed May 30 02:48:41 2012] fullrun_pn_xmm0146510401_pi300-10000_cl_pass1_src27.ximg exists
[Wed May 30 02:48:41 2012] Warning: poor agreement between model and actual number of counts may be indicative of a poor fit in csv/fullrun_pn_xmm0146510401_pi300-10000_cl_pass1_src27.csv
[Wed May 30 02:48:41 2012] fullrun_pn_xmm0146510401_pi300-10000_cl_pass1_src27_1.ximg exists
[Wed May 30 02:48:41 2012] Warning: poor agreement between model and actual number of counts may be indicative of a poor fit in csv/fullrun_pn_xmm0146510401_pi300-10000_cl_pass1_src27.csv
[Wed May 30 02:48:41 2012] It looks like the fit did not converge
You should probably delete fullrun_pn_xmm0146510401_pi300-10000_cl_pass1_src27_1.ximg
Either tweak this fit manually starting from fullrun_pn_xmm0146510401_pi300-10000_cl_pass1_src27.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
[Wed May 30 02:48:42 2012] fullrun_pn_xmm0146510401_pi300-10000_cl_pass1_tfrozen_src27.ximg exists
[Wed May 30 02:48:42 2012] fullrun_pn_xmm0146510401_pi300-10000_cl_pass1_tfrozen_src27_1.ximg exists
[Wed May 30 02:48:42 2012] Fit fullrun_pn_xmm0146510401_pi300-10000_cl_pass1_tfrozen_src27 appears to have run properly
[Wed May 30 05:15:44 2012] Source 31 is offset by 7.593816 and 4.515376 pixels which is larger than
2 X fitted extent = 2.992041 x 2.992041, not incorporating fit results
[Wed May 30 05:15:44 2012] Vigneting correction estimate = 1.000000
[Wed May 30 05:15:44 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Wed May 30 05:15:44 2012] Assessing source extent using major
[Wed May 30 05:15:44 2012] Source does appear to be extended
[Wed May 30 05:15:44 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Wed May 30 05:16:09 2012] XMMSAS src. selection expression = ellipse(35661.806000, 28774.869751, 652.500000, 652.500000, 0.000000, X, Y)
[Wed May 30 05:16:09 2012] Writing source region out to fullrun_pn_xmm0146510401_pi300-10000_pass1_cl_src31_src.reg
[Wed May 30 05:16:09 2012] Extracting stamp from image fullrun_pn_xmm0146510401_pi300-10000_cl_sm2.00.img.gz, (373, 294) - (448, 369)
[Wed May 30 05:16:09 2012] XMMSAS bgd. selection expression = annulus(35661.806000, 28774.869751, 1087.500000, 2175.000000, X, Y) && !ellipse(34379.341400, 28377.496800, 441.994413, 441.994413, 0.000000, X, Y) && !ellipse(35023.576100, 28369.302200, 538.121615, 538.121615, 0.000000, X, Y) && !ellipse(38346.563660, 31227.076050, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(37406.736389, 26825.074646, 870.000000, 870.000000, 0.000000, X, Y)
[Wed May 30 05:16:09 2012] Writing fullrun_pn_xmm0146510401_pi300-10000_pass1_cl_src31.gif
[Wed May 30 05:33:58 2012] Mean detx,y = (7837.36, -3156.24) 
[Wed May 30 05:34:00 2012] Setting backscal keywords in source and bgd. spectrum
[Wed May 30 05:34:14 2012] Binned source spectrum to 10 counts/bin
[Wed May 30 05:34:14 2012] Setting source spectrum file to fullrun_pn_xmm0146510401_pi300-10000_pass1_cl_src31_src_b10.pi.gz
[Wed May 30 05:34:14 2012] Setting bgd. spectrum file to fullrun_pn_xmm0146510401_pi300-10000_pass1_cl_src31_bgd.pi.gz
[Wed May 30 06:28:35 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Wed May 30 06:28:35 2012] rmf not generated due to insufficient counts
[Wed May 30 08:33:37 2012] Updating aperture counts using extracted products
[Wed May 30 08:33:37 2012] Error reading totcts from fullrun_pn_xmm0146510401_pi300-10000_pass1_cl_src31_src_b10.pi.gz
[Wed May 30 08:33:38 2012] Calculating source flux in energy range 0.30-8.00
[Wed May 30 08:33:38 2012] Using photon index=1.80, rate=0.00961, arf fullrun_pn_xmm0146510401_pi300-10000_pass1_cl_src31.arf
[Wed May 30 08:33:38 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Wed May 30 08:33:38 2012] Updating source flux to 3.4e-14
[Wed May 30 08:35:19 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting