[Tue May 29 03:54:28 2012] Detection parameters:
  Position = (237.4, 318.8) = 5 34 55.58 22 1 2.5
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 225.7 +/- 35.7
  Background counts = 217.5
  Rate = 0.04 +/- 0.006

[Tue May 29 03:54:29 2012] Off-axis axis estimate = 4.66'
[Tue May 29 06:59:58 2012] Using EEF radius (= 8.76 ")to estimate initial spatial extent for simple fitting
[Tue May 29 06:59:58 2012] Initial guess for spatial extent in simple fitting = 8.76"
[Tue May 29 06:59:58 2012] source mask rpix=2.0, npix_max = 25, mask sum = 0, frac = 0.000
[Tue May 29 06:59:58 2012] Skipping simple spatial due to low active detector fraction
[Tue May 29 10:23:17 2012] Vigneting correction estimate = 1.000000
[Tue May 29 10:23:17 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Tue May 29 10:23:17 2012] Assessing source extent using major
[Tue May 29 10:23:17 2012] Source does appear to be extended
[Tue May 29 10:23:17 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Tue May 29 15:21:58 2012] Using EEF radius (= 8.76 ")to estimate initial spatial extent for simple fitting
[Tue May 29 15:21:58 2012] Initial guess for spatial extent in simple fitting = 8.76"
[Tue May 29 15:21:58 2012] source mask rpix=2.0, npix_max = 25, mask sum = 0, frac = 0.000
[Tue May 29 15:21:58 2012] Skipping simple spatial due to low active detector fraction
[Tue May 29 19:58:30 2012] Vigneting correction estimate = 1.000000
[Tue May 29 19:58:30 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Tue May 29 19:58:30 2012] Assessing source extent using major
[Tue May 29 19:58:30 2012] Source does appear to be extended
[Tue May 29 19:58:30 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Tue May 29 19:58:30 2012] Source is confused with source 65
[Tue May 29 21:21:02 2012] XMMSAS src. selection expression = ellipse(20608.871811, 27688.848602, 652.500000, 652.500000, 0.000000, X, Y)
[Tue May 29 21:21:02 2012] Writing source region out to fullrun_mos2_xmm0611181401_pi300-10000_pass1_cl_src1_src.reg
[Tue May 29 21:21:02 2012] Extracting stamp from image fullrun_mos2_xmm0611181401_pi300-10000_cl_sm2.00.img.gz, (200, 281) - (275, 356)
[Tue May 29 21:21:02 2012] XMMSAS bgd. selection expression = annulus(20608.871811, 27688.848602, 1087.500000, 2175.000000, X, Y) && !ellipse(20301.062317, 29260.445404, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(20435.088196, 29693.302795, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(20233.965200, 28593.566600, 1435.176041, 1435.176041, 0.000000, X, Y) && !ellipse(19778.552551, 26067.812500, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(20566.002380, 30251.156311, 870.000000, 870.000000, 0.000000, X, Y)
[Tue May 29 21:21:02 2012] Writing fullrun_mos2_xmm0611181401_pi300-10000_pass1_cl_src1.gif
[Tue May 29 21:32:14 2012] Mean detx,y = (6962.61, -197.16) 
[Tue May 29 21:32:15 2012] Setting backscal keywords in source and bgd. spectrum
[Tue May 29 21:32:25 2012] Binned source spectrum to 10 counts/bin
[Tue May 29 21:32:26 2012] Setting source spectrum file to fullrun_mos2_xmm0611181401_pi300-10000_pass1_cl_src1_src_b10.pi.gz
[Tue May 29 21:32:26 2012] Setting bgd. spectrum file to fullrun_mos2_xmm0611181401_pi300-10000_pass1_cl_src1_bgd.pi.gz
[Tue May 29 22:36:21 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Tue May 29 22:36:21 2012] rmf not generated due to insufficient counts
[Tue May 29 22:58:58 2012] Updating aperture counts using extracted products
[Tue May 29 22:58:58 2012] Error reading totcts from fullrun_mos2_xmm0611181401_pi300-10000_pass1_cl_src1_src_b10.pi.gz
[Tue May 29 22:58:59 2012] Calculating source flux in energy range 0.30-8.00
[Tue May 29 22:58:59 2012] Using photon index=1.80, rate=0.0355, arf fullrun_mos2_xmm0611181401_pi300-10000_pass1_cl_src1.arf
[Tue May 29 22:58:59 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Tue May 29 22:58:59 2012] Updating source flux to 6.9e-12
[Tue May 29 23:02:02 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting