[Tue Jul 10 10:38:12 2012] Detection parameters:
  Position = (271.0, 350.0) = 0 45 39.36 41 59 17.4
  Extent = 43.5" x 43.5", rotation angle = 0 degrees
  Source counts = 129.7 +/- 26.4
  Background counts = 1978.7
  Rate = 0.002 +/- 0.0005

[Tue Jul 10 10:38:12 2012] Off-axis axis estimate = 4.23'
[Tue Jul 10 10:41:51 2012] Using EEF radius (= 8.55 ")to estimate initial spatial extent for simple fitting
[Tue Jul 10 10:41:51 2012] Initial guess for spatial extent in simple fitting = 8.55"
[Tue Jul 10 10:41:51 2012] source mask rpix=2.0, npix_max = 24, mask sum = 5, frac = 0.206
[Tue Jul 10 10:41:51 2012] Skipping simple spatial due to low active detector fraction
[Tue Jul 10 11:44:06 2012] Vigneting correction estimate = 1.000000
[Tue Jul 10 11:44:06 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Tue Jul 10 11:44:06 2012] Assessing source extent using major
[Tue Jul 10 11:44:06 2012] Source does appear to be extended
[Tue Jul 10 11:44:06 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Tue Jul 10 11:44:06 2012] Source is confused with source 14
[Tue Jul 10 11:44:16 2012] Using EEF radius (= 8.55 ")to estimate initial spatial extent for simple fitting
[Tue Jul 10 11:44:16 2012] Initial guess for spatial extent in simple fitting = 8.55"
[Tue Jul 10 11:44:16 2012] source mask rpix=2.0, npix_max = 24, mask sum = 5, frac = 0.206
[Tue Jul 10 11:44:16 2012] Skipping simple spatial due to low active detector fraction
[Tue Jul 10 12:39:20 2012] Vigneting correction estimate = 1.000000
[Tue Jul 10 12:39:20 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Tue Jul 10 12:39:20 2012] Assessing source extent using major
[Tue Jul 10 12:39:20 2012] Source does appear to be extended
[Tue Jul 10 12:39:20 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Tue Jul 10 12:39:30 2012] XMMSAS src. selection expression = ellipse(23525.467957, 30398.829041, 2610.000000, 2610.000000, 0.000000, X, Y)
[Tue Jul 10 12:39:30 2012] Writing source region out to fullrun_pn_xmm0109270301_pi300-10000_pass1_cl_src21_src.reg
[Tue Jul 10 12:39:30 2012] Extracting stamp from image fullrun_pn_xmm0109270301_pi300-10000_cl_sm2.00.img.gz, (121, 200) - (421, 500)
[Tue Jul 10 12:39:31 2012] XMMSAS bgd. selection expression = annulus(23525.467957, 30398.829041, 4350.000000, 8700.000000, X, Y) && !ellipse(20880.355194, 36648.064423, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(19205.951675, 36737.868134, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(19358.084320, 35040.995800, 407.968012, 407.968012, 0.000000, X, Y) && !ellipse(22286.431200, 30151.717000, 409.897612, 409.897612, 0.000000, X, Y) && !ellipse(26351.197440, 27227.797898, 422.547378, 241.769586, 115.479675, X, Y)
[Tue Jul 10 12:39:31 2012] Writing fullrun_pn_xmm0109270301_pi300-10000_pass1_cl_src21.gif
[Tue Jul 10 12:54:50 2012] Mean detx,y = (-5494.79, -891.32) 
[Tue Jul 10 12:54:56 2012] Setting backscal keywords in source and bgd. spectrum
[Tue Jul 10 12:57:29 2012] Binned source spectrum to 10 counts/bin
[Tue Jul 10 12:57:30 2012] Setting source spectrum file to fullrun_pn_xmm0109270301_pi300-10000_pass1_cl_src21_src_b10.pi.gz
[Tue Jul 10 12:57:30 2012] Setting bgd. spectrum file to fullrun_pn_xmm0109270301_pi300-10000_pass1_cl_src21_bgd.pi.gz
[Tue Jul 10 13:13:38 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Tue Jul 10 13:13:38 2012] rmf not generated due to insufficient counts
[Tue Jul 10 13:35:54 2012] Updating aperture counts using extracted products
[Tue Jul 10 13:35:54 2012] Error reading totcts from fullrun_pn_xmm0109270301_pi300-10000_pass1_cl_src21_src_b10.pi.gz
[Tue Jul 10 13:35:54 2012] Calculating source flux in energy range 0.30-8.00
[Tue Jul 10 13:35:54 2012] Using photon index=1.80, rate=0.0024, arf fullrun_pn_xmm0109270301_pi300-10000_pass1_cl_src21.arf
[Tue Jul 10 13:35:54 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Tue Jul 10 13:35:54 2012] Updating source flux to 3.3e-14
[Tue Jul 10 13:36:22 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting