[Tue Mar 20 13:39:23 2012] Detection parameters:
  Position = (310.0, 261.3) = 1 32 53.83 30 33 11.8
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 503.0 +/- 27.7
  Background counts = 13.5
  Rate = 0.05 +/- 0.003

[Tue Mar 20 13:39:25 2012] Off-axis axis estimate = 2.82'
[Tue Mar 20 13:41:30 2012] Using EEF radius (= 7.84 ")to estimate initial spatial extent for simple fitting
[Tue Mar 20 13:41:30 2012] Initial guess for spatial extent in simple fitting = 7.84"
[Tue Mar 20 13:41:30 2012] source mask rpix=1.8, npix_max = 21, mask sum = 20, frac = 0.943
[Tue Mar 20 13:41:30 2012] Giving source the simple spatial ID 19 for pass 0, mean size = 7.84"
[Tue Mar 20 15:57:56 2012] fullrun_pn_xmm0141980601_pi300-10000_cl_pass0_src19.ximg exists
[Tue Mar 20 15:57:56 2012] fullrun_pn_xmm0141980601_pi300-10000_cl_pass0_src19_1.ximg exists
[Tue Mar 20 15:57:56 2012] Fit fullrun_pn_xmm0141980601_pi300-10000_cl_pass0_src19 appears to have run properly
[Tue Mar 20 15:57:57 2012] fullrun_pn_xmm0141980601_pi300-10000_cl_pass0_tfrozen_src19.ximg exists
[Tue Mar 20 15:57:57 2012] fullrun_pn_xmm0141980601_pi300-10000_cl_pass0_tfrozen_src19_1.ximg exists
[Tue Mar 20 15:57:57 2012] Fit fullrun_pn_xmm0141980601_pi300-10000_cl_pass0_tfrozen_src19 appears to have run properly
[Tue Mar 20 17:29:38 2012] Source 19 is offset by -7.252549 and 6.482926 pixels which is larger than
2 X fitted extent = 0.901025 x 0.901025, not incorporating fit results
[Tue Mar 20 17:29:38 2012] Vigneting correction estimate = 1.000000
[Tue Mar 20 17:29:38 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Tue Mar 20 17:29:38 2012] Assessing source extent using major
[Tue Mar 20 17:29:38 2012] Source does appear to be extended
[Tue Mar 20 17:29:38 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Tue Mar 20 17:30:05 2012] Using EEF radius (= 7.84 ")to estimate initial spatial extent for simple fitting
[Tue Mar 20 17:30:05 2012] Initial guess for spatial extent in simple fitting = 7.84"
[Tue Mar 20 17:30:05 2012] source mask rpix=1.8, npix_max = 21, mask sum = 20, frac = 0.943
[Tue Mar 20 17:30:05 2012] Giving source the simple spatial ID 19 for pass 1, mean size = 7.84"
[Tue Mar 20 19:57:56 2012] fullrun_pn_xmm0141980601_pi300-10000_cl_pass1_src19.ximg exists
[Tue Mar 20 19:57:56 2012] Warning: poor agreement between model and actual number of counts may be indicative of a poor fit in csv/fullrun_pn_xmm0141980601_pi300-10000_cl_pass1_src19.csv
[Tue Mar 20 19:57:56 2012] fullrun_pn_xmm0141980601_pi300-10000_cl_pass1_src19_1.ximg exists
[Tue Mar 20 19:57:56 2012] Warning: poor agreement between model and actual number of counts may be indicative of a poor fit in csv/fullrun_pn_xmm0141980601_pi300-10000_cl_pass1_src19.csv
[Tue Mar 20 19:57:56 2012] It looks like the fit did not converge
You should probably delete fullrun_pn_xmm0141980601_pi300-10000_cl_pass1_src19_1.ximg
Either tweak this fit manually starting from fullrun_pn_xmm0141980601_pi300-10000_cl_pass1_src19.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
[Tue Mar 20 19:57:57 2012] fullrun_pn_xmm0141980601_pi300-10000_cl_pass1_tfrozen_src19.ximg exists
[Tue Mar 20 19:57:57 2012] fullrun_pn_xmm0141980601_pi300-10000_cl_pass1_tfrozen_src19_1.ximg exists
[Tue Mar 20 19:57:57 2012] Fit fullrun_pn_xmm0141980601_pi300-10000_cl_pass1_tfrozen_src19 appears to have run properly
[Tue Mar 20 20:53:39 2012] Source 19 is offset by -7.252549 and 6.482926 pixels which is larger than
2 X fitted extent = 0.901025 x 0.901025, not incorporating fit results
[Tue Mar 20 20:53:39 2012] Vigneting correction estimate = 1.000000
[Tue Mar 20 20:53:39 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Tue Mar 20 20:53:39 2012] Assessing source extent using major
[Tue Mar 20 20:53:39 2012] Source does appear to be extended
[Tue Mar 20 20:53:39 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Tue Mar 20 20:54:01 2012] XMMSAS src. selection expression = ellipse(26917.642242, 22682.400574, 652.500000, 652.500000, 0.000000, X, Y)
[Tue Mar 20 20:54:01 2012] Writing source region out to fullrun_pn_xmm0141980601_pi300-10000_pass1_cl_src19_src.reg
[Tue Mar 20 20:54:01 2012] Extracting stamp from image fullrun_pn_xmm0141980601_pi300-10000_cl_sm2.00.img.gz, (272, 224) - (347, 299)
[Tue Mar 20 20:54:01 2012] XMMSAS bgd. selection expression = annulus(26917.642242, 22682.400574, 1087.500000, 2175.000000, X, Y) && !ellipse(24842.633301, 21245.973969, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(29627.657196, 24994.299194, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27739.768000, 20923.427400, 429.117612, 429.117612, 0.000000, X, Y)
[Tue Mar 20 20:54:01 2012] Writing fullrun_pn_xmm0141980601_pi300-10000_pass1_cl_src19.gif
[Tue Mar 20 21:28:34 2012] Mean detx,y = (1096.19, 4056.57) 
[Tue Mar 20 21:28:37 2012] Setting backscal keywords in source and bgd. spectrum
[Tue Mar 20 21:29:04 2012] Binned source spectrum to 10 counts/bin
[Tue Mar 20 21:29:05 2012] Setting source spectrum file to fullrun_pn_xmm0141980601_pi300-10000_pass1_cl_src19_src_b10.pi.gz
[Tue Mar 20 21:29:05 2012] Setting bgd. spectrum file to fullrun_pn_xmm0141980601_pi300-10000_pass1_cl_src19_bgd.pi.gz
[Tue Mar 20 22:21:49 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Tue Mar 20 22:21:49 2012] rmf not generated due to insufficient counts
[Tue Mar 20 23:35:15 2012] Updating aperture counts using extracted products
[Tue Mar 20 23:35:15 2012] Error reading totcts from fullrun_pn_xmm0141980601_pi300-10000_pass1_cl_src19_src_b10.pi.gz
[Tue Mar 20 23:35:18 2012] Calculating source flux in energy range 0.30-8.00
[Tue Mar 20 23:35:18 2012] Using photon index=1.80, rate=0.052, arf fullrun_pn_xmm0141980601_pi300-10000_pass1_cl_src19.arf
[Tue Mar 20 23:35:18 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Tue Mar 20 23:35:18 2012] Updating source flux to 1.6e-13
[Tue Mar 20 23:42:47 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting