[Tue Mar 27 10:47:29 2012] Detection parameters:
  Position = (304.6, 250.9) = 14 12 14.03 -34 21 31.1
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 125.0 +/- 26.7
  Background counts = 206.8
  Rate = 0.004 +/- 0.0008

[Tue Mar 27 10:47:29 2012] Off-axis axis estimate = 3.48'
[Tue Mar 27 10:53:55 2012] Using EEF radius (= 8.17 ")to estimate initial spatial extent for simple fitting
[Tue Mar 27 10:53:55 2012] Initial guess for spatial extent in simple fitting = 8.17"
[Tue Mar 27 10:53:55 2012] source mask rpix=1.9, npix_max = 22, mask sum = 6, frac = 0.265
[Tue Mar 27 10:53:55 2012] Skipping simple spatial due to low active detector fraction
[Tue Mar 27 16:03:18 2012] Vigneting correction estimate = 1.000000
[Tue Mar 27 16:03:18 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Tue Mar 27 16:03:18 2012] Assessing source extent using major
[Tue Mar 27 16:03:18 2012] Source does appear to be extended
[Tue Mar 27 16:03:18 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Tue Mar 27 16:03:18 2012] Source is confused with source 57
[Tue Mar 27 16:04:00 2012] Using EEF radius (= 8.17 ")to estimate initial spatial extent for simple fitting
[Tue Mar 27 16:04:00 2012] Initial guess for spatial extent in simple fitting = 8.17"
[Tue Mar 27 16:04:00 2012] source mask rpix=1.9, npix_max = 22, mask sum = 6, frac = 0.265
[Tue Mar 27 16:04:00 2012] Skipping simple spatial due to low active detector fraction
[Tue Mar 27 20:38:39 2012] Vigneting correction estimate = 1.000000
[Tue Mar 27 20:38:39 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Tue Mar 27 20:38:39 2012] Assessing source extent using major
[Tue Mar 27 20:38:39 2012] Source does appear to be extended
[Tue Mar 27 20:38:39 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Tue Mar 27 20:39:23 2012] XMMSAS src. selection expression = ellipse(26447.524170, 21777.971481, 652.500000, 652.500000, 0.000000, X, Y)
[Tue Mar 27 20:39:23 2012] Writing source region out to fullrun_pn_xmm0603751001_pi300-10000_pass1_cl_src53_src.reg
[Tue Mar 27 20:39:23 2012] Extracting stamp from image fullrun_pn_xmm0603751001_pi300-10000_cl_sm2.00.img.gz, (267, 213) - (342, 288)
[Tue Mar 27 20:39:24 2012] XMMSAS bgd. selection expression = annulus(26447.524170, 21777.971481, 1087.500000, 2175.000000, X, Y) && !ellipse(24719.635400, 23120.285600, 599.119217, 599.119217, 0.000000, X, Y) && !ellipse(24435.192505, 21843.704697, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25594.134033, 22049.851791, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25001.295197, 21894.617538, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26301.901123, 21158.570404, 870.000000, 870.000000, 0.000000, X, Y)
[Tue Mar 27 20:39:24 2012] Writing fullrun_pn_xmm0603751001_pi300-10000_pass1_cl_src53.gif
[Tue Mar 27 21:48:50 2012] Mean detx,y = (399.89, -2416.48) 
[Tue Mar 27 21:48:55 2012] Setting backscal keywords in source and bgd. spectrum
[Tue Mar 27 21:49:30 2012] Binned source spectrum to 10 counts/bin
[Tue Mar 27 21:49:30 2012] Setting source spectrum file to fullrun_pn_xmm0603751001_pi300-10000_pass1_cl_src53_src_b10.pi.gz
[Tue Mar 27 21:49:30 2012] Setting bgd. spectrum file to fullrun_pn_xmm0603751001_pi300-10000_pass1_cl_src53_bgd.pi.gz
[Tue Mar 27 23:25:28 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Tue Mar 27 23:25:28 2012] rmf not generated due to insufficient counts
[Wed Mar 28 01:21:28 2012] Updating aperture counts using extracted products
[Wed Mar 28 01:21:28 2012] Error reading totcts from fullrun_pn_xmm0603751001_pi300-10000_pass1_cl_src53_src_b10.pi.gz
[Wed Mar 28 01:21:31 2012] Calculating source flux in energy range 0.30-8.00
[Wed Mar 28 01:21:31 2012] Using photon index=1.80, rate=0.0039, arf fullrun_pn_xmm0603751001_pi300-10000_pass1_cl_src53.arf
[Wed Mar 28 01:21:31 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Wed Mar 28 01:21:31 2012] Updating source flux to 1.3e-14
[Wed Mar 28 01:24:01 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting