[Wed Jan 25 01:03:56 2012] Detection parameters:
  Position = (300.3, 248.8) = 0 42 49.75 41 11 9.1
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 106.7 +/- 15.4
  Background counts = 45.5
  Rate = 0.002 +/- 0.0003

[Wed Jan 25 01:03:56 2012] Off-axis axis estimate = 3.60'
[Wed Jan 25 16:12:56 2012] Using EEF radius (= 8.23 ")to estimate initial spatial extent for simple fitting
[Wed Jan 25 16:12:56 2012] Initial guess for spatial extent in simple fitting = 8.23"
[Wed Jan 25 16:12:56 2012] source mask rpix=1.9, npix_max = 22, mask sum = 17, frac = 0.743
[Wed Jan 25 16:12:56 2012] Giving source the simple spatial ID 104 for pass 0, mean size = 8.23"
[Wed Jan 25 22:38:54 2012] Vigneting correction estimate = 1.000000
[Wed Jan 25 22:38:54 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Wed Jan 25 22:38:54 2012] Assessing source extent using major
[Wed Jan 25 22:38:54 2012] Source does appear to be extended
[Wed Jan 25 22:38:54 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Thu Jan 26 18:45:16 2012] Using EEF radius (= 8.23 ")to estimate initial spatial extent for simple fitting
[Thu Jan 26 18:45:16 2012] Initial guess for spatial extent in simple fitting = 8.23"
[Thu Jan 26 18:45:16 2012] source mask rpix=1.9, npix_max = 22, mask sum = 17, frac = 0.743
[Thu Jan 26 18:45:16 2012] Giving source the simple spatial ID 102 for pass 1, mean size = 8.23"
[Fri Jan 27 00:07:06 2012] Vigneting correction estimate = 1.000000
[Fri Jan 27 00:07:06 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Fri Jan 27 00:07:06 2012] Assessing source extent using major
[Fri Jan 27 00:07:06 2012] Source does appear to be extended
[Fri Jan 27 00:07:06 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Sat Jan 28 08:48:11 2012] XMMSAS src. selection expression = ellipse(26077.022797, 21597.152039, 652.500000, 652.500000, 0.000000, X, Y)
[Sat Jan 28 08:48:11 2012] Writing source region out to fullrun_mos2_xmm0112570101_pi300-10000_pass1_cl_src131_src.reg
[Sat Jan 28 08:48:11 2012] Extracting stamp from image fullrun_mos2_xmm0112570101_pi300-10000_cl_sm2.00.img.gz, (263, 211) - (338, 286)
[Sat Jan 28 08:48:11 2012] XMMSAS bgd. selection expression = annulus(26077.022797, 21597.152039, 1087.500000, 2175.000000, X, Y) && !ellipse(24246.786400, 21488.259200, 395.825611, 395.825611, 0.000000, X, Y) && !ellipse(27195.976000, 22146.803800, 398.157611, 398.157611, 0.000000, X, Y) && !ellipse(27502.343414, 24160.811157, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(28120.589400, 20874.399400, 385.381611, 385.381611, 0.000000, X, Y) && !ellipse(23908.256805, 23404.409241, 870.000000, 870.000000, 0.000000, X, Y)
[Sat Jan 28 08:48:11 2012] Writing fullrun_mos2_xmm0112570101_pi300-10000_pass1_cl_src131.gif
[Sat Jan 28 09:45:26 2012] Mean detx,y = (-493.76, -5613.46) 
[Sat Jan 28 09:45:27 2012] Setting backscal keywords in source and bgd. spectrum
[Sat Jan 28 09:45:40 2012] Binned source spectrum to 10 counts/bin
[Sat Jan 28 09:45:40 2012] Setting source spectrum file to fullrun_mos2_xmm0112570101_pi300-10000_pass1_cl_src131_src_b10.pi.gz
[Sat Jan 28 09:45:40 2012] Setting bgd. spectrum file to fullrun_mos2_xmm0112570101_pi300-10000_pass1_cl_src131_bgd.pi.gz
[Sat Jan 28 13:42:16 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Sat Jan 28 13:42:16 2012] rmf not generated due to insufficient counts
[Sat Jan 28 13:51:50 2012] Updating aperture counts using extracted products
[Sat Jan 28 13:51:50 2012] Error reading totcts from fullrun_mos2_xmm0112570101_pi300-10000_pass1_cl_src131_src_b10.pi.gz
[Sat Jan 28 13:51:52 2012] Calculating source flux in energy range 0.30-8.00
[Sat Jan 28 13:51:52 2012] Using photon index=1.80, rate=0.00223, arf fullrun_mos2_xmm0112570101_pi300-10000_pass1_cl_src131.arf
[Sat Jan 28 13:51:52 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Sat Jan 28 13:51:52 2012] Updating source flux to 2.6e-14
[Sat Jan 28 13:59:05 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting