[Sun Mar 11 21:03:14 2012] Detection parameters:
  Position = (279.9, 221.0) = 16 14 10.26 -52 16 45.0
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 125.3 +/- 24.3
  Background counts = 214.7
  Rate = 0.005 +/- 0.001

[Sun Mar 11 21:03:16 2012] Off-axis axis estimate = 5.78'
[Sun Mar 11 21:11:20 2012] Using EEF radius (= 9.32 ")to estimate initial spatial extent for simple fitting
[Sun Mar 11 21:11:20 2012] Initial guess for spatial extent in simple fitting = 9.32"
[Sun Mar 11 21:11:20 2012] source mask rpix=2.1, npix_max = 27, mask sum = 30, frac = 1.075
[Sun Mar 11 21:11:20 2012] Giving source the simple spatial ID 290 for pass 0, mean size = 9.32"
[Mon Mar 12 07:01:14 2012] Vigneting correction estimate = 1.000000
[Mon Mar 12 07:01:14 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Mon Mar 12 07:01:14 2012] Assessing source extent using major
[Mon Mar 12 07:01:14 2012] Source does appear to be extended
[Mon Mar 12 07:01:14 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Mon Mar 12 07:01:14 2012] Source is confused with source 289
[Mon Mar 12 07:02:05 2012] Using EEF radius (= 9.32 ")to estimate initial spatial extent for simple fitting
[Mon Mar 12 07:02:05 2012] Initial guess for spatial extent in simple fitting = 9.32"
[Mon Mar 12 07:02:05 2012] source mask rpix=2.1, npix_max = 27, mask sum = 30, frac = 1.075
[Mon Mar 12 07:02:05 2012] Giving source the simple spatial ID 274 for pass 1, mean size = 9.32"
[Mon Mar 12 19:02:06 2012] Vigneting correction estimate = 1.000000
[Mon Mar 12 19:02:06 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Mon Mar 12 19:02:06 2012] Assessing source extent using major
[Mon Mar 12 19:02:06 2012] Source does appear to be extended
[Mon Mar 12 19:02:06 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Mon Mar 12 19:03:46 2012] XMMSAS src. selection expression = ellipse(24299.050568, 19174.263901, 652.500000, 652.500000, 0.000000, X, Y)
[Mon Mar 12 19:03:46 2012] Writing source region out to fullrun_pn_xmm0555660101_pi300-10000_pass1_cl_src300_src.reg
[Mon Mar 12 19:03:46 2012] Extracting stamp from image fullrun_pn_xmm0555660101_pi300-10000_cl_sm2.00.img.gz, (242, 183) - (317, 258)
[Mon Mar 12 19:03:47 2012] XMMSAS bgd. selection expression = annulus(24299.050568, 19174.263901, 1087.500000, 2175.000000, X, Y) && !ellipse(22374.422485, 20378.822815, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(23225.707184, 19936.331650, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(24511.434326, 19676.075058, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26786.624512, 19510.527344, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22456.683258, 19439.295563, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(21484.500473, 19427.831146, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(24876.997345, 19162.066696, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22138.525787, 18915.010910, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25948.362732, 19069.057037, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22992.507996, 18742.587997, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(24176.037750, 18666.690002, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25225.005310, 18640.630890, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(21327.601517, 18500.171875, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(24418.643707, 18303.256317, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22873.350281, 18305.721512, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22420.904083, 18296.082428, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(23817.359222, 18220.931824, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25313.916931, 18155.842453, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27023.835449, 17881.658905, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22166.029236, 17794.415970, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(21619.787491, 17777.551224, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22814.732544, 17790.295364, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(24096.317841, 17547.563293, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25615.124695, 17348.611328, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(23760.645142, 16978.825485, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(23391.535004, 17019.847015, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(24591.215302, 16773.048767, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(21751.304367, 16866.394287, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22110.397079, 17206.036255, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(23001.205872, 16572.438736, 870.000000, 870.000000, 0.000000, X, Y)
[Mon Mar 12 19:03:47 2012] Writing fullrun_pn_xmm0555660101_pi300-10000_pass1_cl_src300.gif
[Mon Mar 12 23:55:33 2012] Mean detx,y = (-2931.64, 8140.75) 
[Mon Mar 12 23:55:38 2012] Setting backscal keywords in source and bgd. spectrum
[Mon Mar 12 23:56:10 2012] Binned source spectrum to 10 counts/bin
[Mon Mar 12 23:56:10 2012] Setting source spectrum file to fullrun_pn_xmm0555660101_pi300-10000_pass1_cl_src300_src_b10.pi.gz
[Mon Mar 12 23:56:10 2012] Setting bgd. spectrum file to fullrun_pn_xmm0555660101_pi300-10000_pass1_cl_src300_bgd.pi.gz
[Tue Mar 13 03:30:46 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Tue Mar 13 03:30:46 2012] rmf not generated due to insufficient counts
[Tue Mar 13 04:24:31 2012] Updating aperture counts using extracted products
[Tue Mar 13 04:24:32 2012] Error reading totcts from fullrun_pn_xmm0555660101_pi300-10000_pass1_cl_src300_src_b10.pi.gz
[Tue Mar 13 04:24:54 2012] Calculating source flux in energy range 0.30-8.00
[Tue Mar 13 04:24:54 2012] Using photon index=1.80, rate=0.00504, arf fullrun_pn_xmm0555660101_pi300-10000_pass1_cl_src300.arf
[Tue Mar 13 04:24:54 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Tue Mar 13 04:24:54 2012] Updating source flux to 2.1e-14
[Tue Mar 13 04:26:15 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting