[Sun May  6 01:20:16 2012] Detection parameters:
  Position = (375.1, 190.0) = 17 45 10.33 -29 6 50.5
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 250.2 +/- 28.0
  Background counts = 384.9
  Rate = 0.003 +/- 0.0003

[Sun May  6 01:20:19 2012] Off-axis axis estimate = 9.63'
[Sun May  6 01:45:13 2012] Using EEF radius (= 11.24 ")to estimate initial spatial extent for simple fitting
[Sun May  6 01:45:13 2012] Initial guess for spatial extent in simple fitting = 11.24"
[Sun May  6 01:45:13 2012] source mask rpix=2.6, npix_max = 38, mask sum = 30, frac = 0.788
[Sun May  6 01:45:13 2012] Giving source the simple spatial ID 124 for pass 0, mean size = 11.24"
[Tue May  8 12:13:04 2012] Vigneting correction estimate = 1.000000
[Tue May  8 12:13:04 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Tue May  8 12:13:04 2012] Assessing source extent using major
[Tue May  8 12:13:04 2012] Source does appear to be extended
[Tue May  8 12:13:04 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Tue May  8 12:15:59 2012] Using EEF radius (= 11.24 ")to estimate initial spatial extent for simple fitting
[Tue May  8 12:15:59 2012] Initial guess for spatial extent in simple fitting = 11.24"
[Tue May  8 12:15:59 2012] source mask rpix=2.6, npix_max = 38, mask sum = 30, frac = 0.788
[Tue May  8 12:15:59 2012] Giving source the simple spatial ID 111 for pass 1, mean size = 11.24"
[Sat May 12 00:41:16 2012] Vigneting correction estimate = 1.000000
[Sat May 12 00:41:16 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Sat May 12 00:41:16 2012] Assessing source extent using major
[Sat May 12 00:41:16 2012] Source does appear to be extended
[Sat May 12 00:41:16 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Sat May 12 00:43:27 2012] XMMSAS src. selection expression = ellipse(32581.812714, 16478.673721, 652.500000, 652.500000, 0.000000, X, Y)
[Sat May 12 00:43:27 2012] Writing source region out to fullrun_pn_xmm0505670101_pi300-10000_pass1_cl_src140_src.reg
[Sat May 12 00:43:27 2012] Extracting stamp from image fullrun_pn_xmm0505670101_pi300-10000_cl_sm2.00.img.gz, (338, 152) - (413, 227)
[Sat May 12 00:43:27 2012] XMMSAS bgd. selection expression = annulus(32581.812714, 16478.673721, 1087.500000, 2175.000000, X, Y) && !ellipse(24797.492400, 24082.276200, 6979.008201, 3958.200114, 32.072000, X, Y) && !ellipse(30137.133423, 19188.043503, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(30765.477966, 19100.730209, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(30760.454651, 16989.989883, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(29564.085175, 15240.608337, 870.000000, 870.000000, 0.000000, X, Y)
[Sat May 12 00:43:27 2012] Writing fullrun_pn_xmm0505670101_pi300-10000_pass1_cl_src140.gif
[Sat May 12 08:14:45 2012] Mean detx,y = (-7134.38, -8228.62) 
[Sat May 12 08:14:55 2012] Setting backscal keywords in source and bgd. spectrum
[Sat May 12 08:15:31 2012] Binned source spectrum to 10 counts/bin
[Sat May 12 08:15:32 2012] Setting source spectrum file to fullrun_pn_xmm0505670101_pi300-10000_pass1_cl_src140_src_b10.pi.gz
[Sat May 12 08:15:32 2012] Setting bgd. spectrum file to fullrun_pn_xmm0505670101_pi300-10000_pass1_cl_src140_bgd.pi.gz
[Sun May 13 05:46:50 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Sun May 13 05:46:50 2012] rmf not generated due to insufficient counts
[Tue May 15 01:58:16 2012] Updating aperture counts using extracted products
[Tue May 15 01:58:16 2012] Error reading totcts from fullrun_pn_xmm0505670101_pi300-10000_pass1_cl_src140_src_b10.pi.gz
[Tue May 15 01:58:25 2012] Calculating source flux in energy range 0.30-8.00
[Tue May 15 01:58:25 2012] Using photon index=1.80, rate=0.00259, arf fullrun_pn_xmm0505670101_pi300-10000_pass1_cl_src140.arf
[Tue May 15 01:58:25 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Tue May 15 01:58:25 2012] Updating source flux to 3.1e-14
[Tue May 15 02:19:35 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting