[Sun Sep 25 10:29:16 2011] Detection parameters:
  Position = (272.1, 282.0) = 2 41 7.40 -8 15 29.5
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 65.8 +/- 14.5
  Background counts = 27.2
  Rate = 0.002 +/- 0.0003

[Sun Sep 25 10:29:16 2011] Off-axis axis estimate = 2.25'
[Sun Sep 25 13:54:56 2011] Using EEF radius (= 7.55 ")to estimate initial spatial extent for simple fitting
[Sun Sep 25 13:54:56 2011] Initial guess for spatial extent in simple fitting = 7.55"
[Sun Sep 25 13:54:56 2011] source mask rpix=1.7, npix_max = 20, mask sum = 9, frac = 0.450
[Sun Sep 25 13:54:56 2011] Skipping simple spatial due to low active detector fraction
[Sun Sep 25 14:40:52 2011] Vigneting correction estimate = 1.000000
[Sun Sep 25 14:40:52 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Sun Sep 25 14:40:52 2011] Assessing source extent using major
[Sun Sep 25 14:40:52 2011] Source does appear to be extended
[Sun Sep 25 14:40:52 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Sun Sep 25 16:42:49 2011] Using EEF radius (= 7.55 ")to estimate initial spatial extent for simple fitting
[Sun Sep 25 16:42:49 2011] Initial guess for spatial extent in simple fitting = 7.55"
[Sun Sep 25 16:42:49 2011] source mask rpix=1.7, npix_max = 20, mask sum = 9, frac = 0.450
[Sun Sep 25 16:42:49 2011] Skipping simple spatial due to low active detector fraction
[Sun Sep 25 17:28:20 2011] Vigneting correction estimate = 1.000000
[Sun Sep 25 17:28:20 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Sun Sep 25 17:28:20 2011] Assessing source extent using major
[Sun Sep 25 17:28:20 2011] Source does appear to be extended
[Sun Sep 25 17:28:20 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Sun Sep 25 20:26:58 2011] XMMSAS src. selection expression = ellipse(23622.934082, 24489.424133, 652.500000, 652.500000, 0.000000, X, Y)
[Sun Sep 25 20:26:58 2011] Writing source region out to fullrun_mos2_xmm0553300401_pi300-10000_pass1_cl_src34_src.reg
[Sun Sep 25 20:26:58 2011] Extracting stamp from image fullrun_mos2_xmm0553300401_pi300-10000_cl_sm2.00.img.gz, (235, 245) - (310, 320)
[Sun Sep 25 20:26:58 2011] XMMSAS bgd. selection expression = annulus(23622.934082, 24489.424133, 1087.500000, 2175.000000, X, Y) && !ellipse(24393.546520, 24549.263400, 465.344013, 465.344013, 0.000000, X, Y) && !ellipse(25398.965485, 24830.579468, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(21385.945149, 25507.585023, 629.319988, 398.238407, 6.202409, X, Y) && !ellipse(25401.413422, 25530.105347, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22901.735199, 22543.739014, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(23941.216339, 26062.037811, 870.000000, 870.000000, 0.000000, X, Y)
[Sun Sep 25 20:26:58 2011] Writing fullrun_mos2_xmm0553300401_pi300-10000_pass1_cl_src34.gif
[Sun Sep 25 20:32:09 2011] Mean detx,y = (-346.09, 191.48) 
[Sun Sep 25 20:32:10 2011] Setting backscal keywords in source and bgd. spectrum
[Sun Sep 25 20:32:15 2011] Binned source spectrum to 10 counts/bin
[Sun Sep 25 20:32:15 2011] Setting source spectrum file to fullrun_mos2_xmm0553300401_pi300-10000_pass1_cl_src34_src_b10.pi.gz
[Sun Sep 25 20:32:15 2011] Setting bgd. spectrum file to fullrun_mos2_xmm0553300401_pi300-10000_pass1_cl_src34_bgd.pi.gz
[Sun Sep 25 21:04:52 2011] Not generating rmf since there are only 65 counts
[Sun Sep 25 21:04:52 2011] rmf not generated due to insufficient counts
[Sun Sep 25 21:06:23 2011] Updating aperture counts using extracted products
[Sun Sep 25 21:06:23 2011] Error reading totcts from fullrun_mos2_xmm0553300401_pi300-10000_pass1_cl_src34_src_b10.pi.gz
[Sun Sep 25 21:06:23 2011] Calculating source flux in energy range 0.30-8.00
[Sun Sep 25 21:06:23 2011] Using photon index=1.80, rate=0.00158, arf fullrun_mos2_xmm0553300401_pi300-10000_pass1_cl_src34.arf
[Sun Sep 25 21:06:23 2011] Assuming count rate is from the 0.30-10.00 bandpass
[Sun Sep 25 21:06:23 2011] Updating source flux to 1.5e-14
[Sun Sep 25 21:07:04 2011] Simple spatial fitting not done (or not done successfully), skipping spectral fitting