[Sun Mar 11 21:03:13 2012] Detection parameters:
  Position = (215.3, 297.3) = 16 14 40.76 -52 11 20.1
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 125.4 +/- 28.3
  Background counts = 253.0
  Rate = 0.005 +/- 0.001

[Sun Mar 11 21:03:16 2012] Off-axis axis estimate = 6.02'
[Sun Mar 11 21:11:20 2012] Using EEF radius (= 9.44 ")to estimate initial spatial extent for simple fitting
[Sun Mar 11 21:11:20 2012] Initial guess for spatial extent in simple fitting = 9.44"
[Sun Mar 11 21:11:20 2012] source mask rpix=2.2, npix_max = 28, mask sum = 25, frac = 0.877
[Sun Mar 11 21:11:20 2012] Giving source the simple spatial ID 260 for pass 0, mean size = 9.44"
[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 07:02:05 2012] Using EEF radius (= 9.44 ")to estimate initial spatial extent for simple fitting
[Mon Mar 12 07:02:05 2012] Initial guess for spatial extent in simple fitting = 9.44"
[Mon Mar 12 07:02:05 2012] source mask rpix=2.2, npix_max = 28, mask sum = 25, frac = 0.877
[Mon Mar 12 07:02:05 2012] Giving source the simple spatial ID 244 for pass 1, mean size = 9.44"
[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 19:03:44 2012] XMMSAS src. selection expression = ellipse(18686.864243, 25817.684845, 652.500000, 652.500000, 0.000000, X, Y)
[Mon Mar 12 19:03:44 2012] Writing source region out to fullrun_pn_xmm0555660101_pi300-10000_pass1_cl_src269_src.reg
[Mon Mar 12 19:03:44 2012] Extracting stamp from image fullrun_pn_xmm0555660101_pi300-10000_cl_sm2.00.img.gz, (178, 260) - (253, 335)
[Mon Mar 12 19:03:44 2012] XMMSAS bgd. selection expression = annulus(18686.864243, 25817.684845, 1087.500000, 2175.000000, X, Y) && !ellipse(16123.029892, 27751.998474, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(15549.350000, 27801.943200, 1745.784050, 1111.016032, 353.576670, X, Y) && !ellipse(21347.494324, 27883.634827, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(18953.842041, 27758.559052, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(17979.630814, 27750.742645, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(17519.364227, 27758.707733, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(20906.045258, 27368.373291, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(20016.014389, 27840.841064, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(18474.095505, 27707.678070, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(16743.173050, 27454.919281, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(17578.327118, 27362.072906, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(21498.006607, 27360.344482, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(20742.360046, 27838.913513, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(15674.922012, 27186.979034, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(16737.000107, 26934.350342, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(16122.626328, 27014.683563, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(18873.937607, 27191.330627, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(20920.858994, 26835.097382, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(18066.191406, 26924.455048, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(19877.509476, 26931.424500, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(17264.275650, 26407.966888, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(21523.624985, 26070.050690, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(18674.945816, 26489.590454, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(19570.002655, 26076.061676, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(17992.823654, 26068.056763, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(15766.004120, 26578.661377, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(16809.986862, 26416.555908, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(21080.763443, 26232.280945, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(17271.723007, 25803.737976, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(15647.945587, 25630.561035, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(16098.970016, 25435.371246, 870.000000, 870.000000, 0.000000, X, Y)
[Mon Mar 12 19:03:44 2012] Writing fullrun_pn_xmm0555660101_pi300-10000_pass1_cl_src269.gif
[Mon Mar 12 23:21:58 2012] Mean detx,y = (-8315.28, 1300.02) 
[Mon Mar 12 23:22:04 2012] Setting backscal keywords in source and bgd. spectrum
[Mon Mar 12 23:22:27 2012] Binned source spectrum to 10 counts/bin
[Mon Mar 12 23:22:27 2012] Setting source spectrum file to fullrun_pn_xmm0555660101_pi300-10000_pass1_cl_src269_src_b10.pi.gz
[Mon Mar 12 23:22:27 2012] Setting bgd. spectrum file to fullrun_pn_xmm0555660101_pi300-10000_pass1_cl_src269_bgd.pi.gz
[Tue Mar 13 03:21:20 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Tue Mar 13 03:21:20 2012] rmf not generated due to insufficient counts
[Tue Mar 13 04:24:30 2012] Updating aperture counts using extracted products
[Tue Mar 13 04:24:30 2012] Error reading totcts from fullrun_pn_xmm0555660101_pi300-10000_pass1_cl_src269_src_b10.pi.gz
[Tue Mar 13 04:24:52 2012] Calculating source flux in energy range 0.30-8.00
[Tue Mar 13 04:24:52 2012] Using photon index=1.80, rate=0.00521, arf fullrun_pn_xmm0555660101_pi300-10000_pass1_cl_src269.arf
[Tue Mar 13 04:24:52 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Tue Mar 13 04:24:52 2012] Updating source flux to 2.3e-14
[Tue Mar 13 04:26:15 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting