[Thu Nov 24 02:28:39 2011] Detection parameters:
  Position = (308.4, 251.1) = 14 22 57.94 19 33 30.4
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 81.5 +/- 16.3
  Background counts = 55.7
  Rate = 0.007 +/- 0.001

[Thu Nov 24 02:28:39 2011] Off-axis axis estimate = 3.51'
[Thu Nov 24 02:31:10 2011] Using EEF radius (= 8.18 ")to estimate initial spatial extent for simple fitting
[Thu Nov 24 02:31:10 2011] Initial guess for spatial extent in simple fitting = 8.18"
[Thu Nov 24 02:31:10 2011] source mask rpix=1.9, npix_max = 22, mask sum = 7, frac = 0.309
[Thu Nov 24 02:31:10 2011] Skipping simple spatial due to low active detector fraction
[Thu Nov 24 03:08:00 2011] Source 9 is offset by -5.293816 and -3.570335 pixels which is larger than
2 X fitted extent = 0.958257 x 0.958257, not incorporating fit results
[Thu Nov 24 03:08:00 2011] Vigneting correction estimate = 1.000000
[Thu Nov 24 03:08:00 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Thu Nov 24 03:08:00 2011] Assessing source extent using major
[Thu Nov 24 03:08:00 2011] Source does appear to be extended
[Thu Nov 24 03:08:00 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Thu Nov 24 03:08:00 2011] Source is confused with source 2
[Thu Nov 24 03:08:08 2011] Using EEF radius (= 8.18 ")to estimate initial spatial extent for simple fitting
[Thu Nov 24 03:08:08 2011] Initial guess for spatial extent in simple fitting = 8.18"
[Thu Nov 24 03:08:08 2011] source mask rpix=1.9, npix_max = 22, mask sum = 7, frac = 0.309
[Thu Nov 24 03:08:08 2011] Skipping simple spatial due to low active detector fraction
[Thu Nov 24 03:42:45 2011] Vigneting correction estimate = 1.000000
[Thu Nov 24 03:42:45 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Thu Nov 24 03:42:45 2011] Assessing source extent using major
[Thu Nov 24 03:42:45 2011] Source does appear to be extended
[Thu Nov 24 03:42:45 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Thu Nov 24 03:42:54 2011] XMMSAS src. selection expression = ellipse(26779.886047, 21796.828827, 652.500000, 652.500000, 0.000000, X, Y)
[Thu Nov 24 03:42:54 2011] Writing source region out to fullrun_pn_xmm0500910901_pi300-10000_pass1_cl_src9_src.reg
[Thu Nov 24 03:42:54 2011] Extracting stamp from image fullrun_pn_xmm0500910901_pi300-10000_cl_sm2.00.img.gz, (271, 214) - (346, 289)
[Thu Nov 24 03:42:54 2011] XMMSAS bgd. selection expression = annulus(26779.886047, 21796.828827, 1087.500000, 2175.000000, X, Y) && !ellipse(26519.118200, 21458.240400, 371.351211, 278.406408, 231.505000, X, Y) && !ellipse(26200.590600, 24229.723600, 451.529613, 451.529613, 0.000000, X, Y) && !ellipse(26494.438600, 21273.213600, 957.536028, 957.536028, 0.000000, X, Y)
[Thu Nov 24 03:42:54 2011] Writing fullrun_pn_xmm0500910901_pi300-10000_pass1_cl_src9.gif
[Thu Nov 24 03:45:49 2011] Mean detx,y = (612.01, -2569.11) 
[Thu Nov 24 03:45:51 2011] Setting backscal keywords in source and bgd. spectrum
[Thu Nov 24 03:46:07 2011] Binned source spectrum to 10 counts/bin
[Thu Nov 24 03:46:08 2011] Setting source spectrum file to fullrun_pn_xmm0500910901_pi300-10000_pass1_cl_src9_src_b10.pi.gz
[Thu Nov 24 03:46:08 2011] Setting bgd. spectrum file to fullrun_pn_xmm0500910901_pi300-10000_pass1_cl_src9_bgd.pi.gz
[Thu Nov 24 03:56:49 2011] Not generating rmf since there are only 81 counts
[Thu Nov 24 03:56:49 2011] rmf not generated due to insufficient counts
[Thu Nov 24 04:15:14 2011] Updating aperture counts using extracted products
[Thu Nov 24 04:15:14 2011] Error reading totcts from fullrun_pn_xmm0500910901_pi300-10000_pass1_cl_src9_src_b10.pi.gz
[Thu Nov 24 04:15:14 2011] Calculating source flux in energy range 0.30-8.00
[Thu Nov 24 04:15:14 2011] Using photon index=1.80, rate=0.00694, arf fullrun_pn_xmm0500910901_pi300-10000_pass1_cl_src9.arf
[Thu Nov 24 04:15:14 2011] Assuming count rate is from the 0.30-10.00 bandpass
[Thu Nov 24 04:15:14 2011] Updating source flux to 2.1e-14
[Thu Nov 24 04:15:30 2011] Simple spatial fitting not done (or not done successfully), skipping spectral fitting