[Sat Sep 24 00:38:17 2011] Detection parameters:
  Position = (281.7, 483.9) = 9 20 46.02 37 23 2.8
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 94.7 +/- 17.2
  Background counts = 84.4
  Rate = 0.001 +/- 0.0002

[Sat Sep 24 00:38:18 2011] Off-axis axis estimate = 13.50'
[Sat Sep 24 00:43:25 2011] Using EEF radius (= 13.18 ")to estimate initial spatial extent for simple fitting
[Sat Sep 24 00:43:25 2011] Initial guess for spatial extent in simple fitting = 13.18"
[Sat Sep 24 00:43:25 2011] source mask rpix=3.0, npix_max = 49, mask sum = 24, frac = 0.482
[Sat Sep 24 00:43:25 2011] Skipping simple spatial due to low active detector fraction
[Sat Sep 24 03:50:32 2011] Vigneting correction estimate = 1.000000
[Sat Sep 24 03:50:32 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Sat Sep 24 03:50:32 2011] Assessing source extent using major
[Sat Sep 24 03:50:32 2011] Source does appear to be extended
[Sat Sep 24 03:50:32 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Sat Sep 24 03:50:55 2011] Using EEF radius (= 13.18 ")to estimate initial spatial extent for simple fitting
[Sat Sep 24 03:50:55 2011] Initial guess for spatial extent in simple fitting = 13.18"
[Sat Sep 24 03:50:55 2011] source mask rpix=3.0, npix_max = 49, mask sum = 24, frac = 0.482
[Sat Sep 24 03:50:55 2011] Skipping simple spatial due to low active detector fraction
[Sat Sep 24 07:04:05 2011] Warning: source 22 in spatial fitting list does not appear to have a counterpart in memory, closest src. was src. 34 at 13.658691 pixels away
[Sat Sep 24 07:04:05 2011] Vigneting correction estimate = 1.000000
[Sat Sep 24 07:04:05 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Sat Sep 24 07:04:05 2011] Assessing source extent using major
[Sat Sep 24 07:04:05 2011] Source does appear to be extended
[Sat Sep 24 07:04:05 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Sat Sep 24 07:04:26 2011] XMMSAS src. selection expression = ellipse(24457.964691, 42054.529785, 652.500000, 652.500000, 0.000000, X, Y)
[Sat Sep 24 07:04:26 2011] Writing source region out to fullrun_pn_xmm0149010201_pi300-10000_pass1_cl_src34_src.reg
[Sat Sep 24 07:04:26 2011] Extracting stamp from image fullrun_pn_xmm0149010201_pi300-10000_cl_sm2.00.img.gz, (244, 446) - (319, 521)
[Sat Sep 24 07:04:26 2011] XMMSAS bgd. selection expression = annulus(24457.964691, 42054.529785, 1087.500000, 2175.000000, X, Y) && !ellipse(25463.784600, 41265.042820, 486.303214, 486.303214, 0.000000, X, Y) && !ellipse(22359.729553, 41383.983551, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25877.045990, 42718.680054, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26829.110291, 39989.203735, 870.000000, 870.000000, 0.000000, X, Y)
[Sat Sep 24 07:04:26 2011] Writing fullrun_pn_xmm0149010201_pi300-10000_pass1_cl_src34.gif
[Sat Sep 24 07:37:44 2011] Mean detx,y = (3430.90, -14087.56) 
[Sat Sep 24 07:37:49 2011] Setting backscal keywords in source and bgd. spectrum
[Sat Sep 24 07:38:08 2011] Binned source spectrum to 10 counts/bin
[Sat Sep 24 07:38:08 2011] Setting source spectrum file to fullrun_pn_xmm0149010201_pi300-10000_pass1_cl_src34_src_b10.pi.gz
[Sat Sep 24 07:38:08 2011] Setting bgd. spectrum file to fullrun_pn_xmm0149010201_pi300-10000_pass1_cl_src34_bgd.pi.gz
[Sat Sep 24 08:25:07 2011] Not generating rmf since there are only 94 counts
[Sat Sep 24 08:25:07 2011] rmf not generated due to insufficient counts
[Sat Sep 24 10:35:15 2011] Updating aperture counts using extracted products
[Sat Sep 24 10:35:15 2011] Error reading totcts from fullrun_pn_xmm0149010201_pi300-10000_pass1_cl_src34_src_b10.pi.gz
[Sat Sep 24 10:35:17 2011] Calculating source flux in energy range 0.30-8.00
[Sat Sep 24 10:35:17 2011] Using photon index=1.80, rate=0.00131, arf fullrun_pn_xmm0149010201_pi300-10000_pass1_cl_src34.arf
[Sat Sep 24 10:35:17 2011] Assuming count rate is from the 0.30-10.00 bandpass
[Sat Sep 24 10:35:17 2011] Updating source flux to 5.1e-14
[Sat Sep 24 10:38:53 2011] Simple spatial fitting not done (or not done successfully), skipping spectral fitting