[Wed Sep 28 22:57:32 2011] Detection parameters:
  Position = (385.0, 222.9) = 1 11 4.09 -38 11 0.3
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 253.4 +/- 24.8
  Background counts = 223.7
  Rate = 0.004 +/- 0.0004

[Wed Sep 28 22:57:33 2011] Off-axis axis estimate = 8.33'
[Wed Sep 28 23:05:48 2011] Using EEF radius (= 10.59 ")to estimate initial spatial extent for simple fitting
[Wed Sep 28 23:05:48 2011] Initial guess for spatial extent in simple fitting = 10.59"
[Wed Sep 28 23:05:48 2011] source mask rpix=2.4, npix_max = 34, mask sum = 28, frac = 0.812
[Wed Sep 28 23:05:48 2011] Giving source the simple spatial ID 40 for pass 0, mean size = 10.59"
[Thu Sep 29 00:10:18 2011] fullrun_pn_xmm0550950101_pi300-10000_cl_pass0_src40.ximg exists
[Thu Sep 29 00:10:18 2011] fullrun_pn_xmm0550950101_pi300-10000_cl_pass0_src40_1.ximg exists
[Thu Sep 29 00:10:18 2011] Fit fullrun_pn_xmm0550950101_pi300-10000_cl_pass0_src40 appears to have run properly
[Thu Sep 29 00:10:18 2011] fullrun_pn_xmm0550950101_pi300-10000_cl_pass0_tfrozen_src40.ximg exists
[Thu Sep 29 00:10:18 2011] fullrun_pn_xmm0550950101_pi300-10000_cl_pass0_tfrozen_src40_1.ximg exists
[Thu Sep 29 00:10:18 2011] Fit fullrun_pn_xmm0550950101_pi300-10000_cl_pass0_tfrozen_src40 appears to have run properly
[Thu Sep 29 01:33:13 2011] Warning, spatial fit 40 centroid is now closest to src. 42
[Thu Sep 29 01:33:13 2011] Vigneting correction estimate = 1.000000
[Thu Sep 29 01:33:13 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Thu Sep 29 01:33:13 2011] Assessing source extent using major
[Thu Sep 29 01:33:13 2011] Source does appear to be extended
[Thu Sep 29 01:33:13 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Thu Sep 29 01:33:32 2011] Using EEF radius (= 10.59 ")to estimate initial spatial extent for simple fitting
[Thu Sep 29 01:33:32 2011] Initial guess for spatial extent in simple fitting = 10.59"
[Thu Sep 29 01:33:32 2011] source mask rpix=2.4, npix_max = 34, mask sum = 28, frac = 0.812
[Thu Sep 29 01:33:32 2011] Giving source the simple spatial ID 40 for pass 1, mean size = 10.59"
[Thu Sep 29 02:33:58 2011] fullrun_pn_xmm0550950101_pi300-10000_cl_pass1_src40.ximg exists
[Thu Sep 29 02:33:58 2011] Warning: poor agreement between model and actual number of counts may be indicative of a poor fit in csv/fullrun_pn_xmm0550950101_pi300-10000_cl_pass1_src40.csv
[Thu Sep 29 02:33:58 2011] fullrun_pn_xmm0550950101_pi300-10000_cl_pass1_src40_1.ximg exists
[Thu Sep 29 02:33:58 2011] Warning: poor agreement between model and actual number of counts may be indicative of a poor fit in csv/fullrun_pn_xmm0550950101_pi300-10000_cl_pass1_src40.csv
[Thu Sep 29 02:33:58 2011] It looks like the fit did not converge
You should probably delete fullrun_pn_xmm0550950101_pi300-10000_cl_pass1_src40_1.ximg
Either tweak this fit manually starting from fullrun_pn_xmm0550950101_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
[Thu Sep 29 02:33:58 2011] fullrun_pn_xmm0550950101_pi300-10000_cl_pass1_tfrozen_src40.ximg exists
[Thu Sep 29 02:33:58 2011] fullrun_pn_xmm0550950101_pi300-10000_cl_pass1_tfrozen_src40_1.ximg exists
[Thu Sep 29 02:33:58 2011] Fit fullrun_pn_xmm0550950101_pi300-10000_cl_pass1_tfrozen_src40 appears to have run properly
[Thu Sep 29 04:01:02 2011] Warning: source 40 in spatial fitting list does not appear to have a counterpart in memory, closest src. was src. 41 at 11.028849 pixels away
[Thu Sep 29 04:01:02 2011] Vigneting correction estimate = 1.000000
[Thu Sep 29 04:01:02 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Thu Sep 29 04:01:02 2011] Assessing source extent using major
[Thu Sep 29 04:01:02 2011] Source does appear to be extended
[Thu Sep 29 04:01:02 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Thu Sep 29 04:01:24 2011] XMMSAS src. selection expression = ellipse(33449.869232, 19345.165482, 652.500000, 652.500000, 0.000000, X, Y)
[Thu Sep 29 04:01:24 2011] Writing source region out to fullrun_pn_xmm0550950101_pi300-10000_pass1_cl_src41_src.reg
[Thu Sep 29 04:01:24 2011] Extracting stamp from image fullrun_pn_xmm0550950101_pi300-10000_cl_sm2.00.img.gz, (348, 185) - (423, 260)
[Thu Sep 29 04:01:24 2011] XMMSAS bgd. selection expression = annulus(33449.869232, 19345.165482, 1087.500000, 2175.000000, X, Y) && !ellipse(35875.055298, 20027.680588, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(35177.560516, 16851.856674, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(35267.082020, 19151.921600, 325.605609, 325.605609, 40.202000, X, Y) && !ellipse(33179.082020, 17933.921600, 325.605609, 325.605609, 0.000000, X, Y)
[Thu Sep 29 04:01:24 2011] Writing fullrun_pn_xmm0550950101_pi300-10000_pass1_cl_src41.gif
[Thu Sep 29 05:14:57 2011] Mean detx,y = (9017.83, 2059.57) 
[Thu Sep 29 05:15:04 2011] Setting backscal keywords in source and bgd. spectrum
[Thu Sep 29 05:15:28 2011] Binned source spectrum to 10 counts/bin
[Thu Sep 29 05:15:28 2011] Setting source spectrum file to fullrun_pn_xmm0550950101_pi300-10000_pass1_cl_src41_src_b10.pi.gz
[Thu Sep 29 05:15:28 2011] Setting bgd. spectrum file to fullrun_pn_xmm0550950101_pi300-10000_pass1_cl_src41_bgd.pi.gz
[Thu Sep 29 06:35:38 2011] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Thu Sep 29 06:35:38 2011] rmf not generated due to insufficient counts
[Thu Sep 29 07:50:44 2011] Updating aperture counts using extracted products
[Thu Sep 29 07:50:44 2011] Error reading totcts from fullrun_pn_xmm0550950101_pi300-10000_pass1_cl_src41_src_b10.pi.gz
[Thu Sep 29 07:50:44 2011] Calculating source flux in energy range 0.30-8.00
[Thu Sep 29 07:50:44 2011] Using photon index=1.80, rate=0.00362, arf fullrun_pn_xmm0550950101_pi300-10000_pass1_cl_src41.arf
[Thu Sep 29 07:50:44 2011] Assuming count rate is from the 0.30-10.00 bandpass
[Thu Sep 29 07:50:44 2011] Updating source flux to 1.6e-14
[Thu Sep 29 07:52:55 2011] Simple spatial fitting not done (or not done successfully), skipping spectral fitting