[Sat Mar 17 23:54:51 2012] Detection parameters:
  Position = (258.7, 253.7) = 2 14 45.55 -4 32 14.4
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 93.7 +/- 15.5
  Background counts = 115.4
  Rate = 0.007 +/- 0.001

[Sat Mar 17 23:54:51 2012] Off-axis axis estimate = 4.34'
[Sat Mar 17 23:58:06 2012] Using EEF radius (= 8.60 ")to estimate initial spatial extent for simple fitting
[Sat Mar 17 23:58:06 2012] Initial guess for spatial extent in simple fitting = 8.60"
[Sat Mar 17 23:58:06 2012] source mask rpix=2.0, npix_max = 24, mask sum = 11, frac = 0.448
[Sat Mar 17 23:58:06 2012] Skipping simple spatial due to low active detector fraction
[Sun Mar 18 03:23:49 2012] Vigneting correction estimate = 1.000000
[Sun Mar 18 03:23:49 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Sun Mar 18 03:23:49 2012] Assessing source extent using major
[Sun Mar 18 03:23:49 2012] Source does appear to be extended
[Sun Mar 18 03:23:49 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Sun Mar 18 03:24:06 2012] Using EEF radius (= 8.60 ")to estimate initial spatial extent for simple fitting
[Sun Mar 18 03:24:06 2012] Initial guess for spatial extent in simple fitting = 8.60"
[Sun Mar 18 03:24:06 2012] source mask rpix=2.0, npix_max = 24, mask sum = 11, frac = 0.448
[Sun Mar 18 03:24:06 2012] Skipping simple spatial due to low active detector fraction
[Sun Mar 18 06:01:19 2012] Vigneting correction estimate = 1.000000
[Sun Mar 18 06:01:19 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Sun Mar 18 06:01:19 2012] Assessing source extent using major
[Sun Mar 18 06:01:19 2012] Source does appear to be extended
[Sun Mar 18 06:01:19 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Sun Mar 18 06:01:35 2012] XMMSAS src. selection expression = ellipse(22455.982330, 22021.788132, 652.500000, 652.500000, 0.000000, X, Y)
[Sun Mar 18 06:01:35 2012] Writing source region out to fullrun_pn_xmm0553911401_pi300-10000_pass1_cl_src35_src.reg
[Sun Mar 18 06:01:35 2012] Extracting stamp from image fullrun_pn_xmm0553911401_pi300-10000_cl_sm2.00.img.gz, (221, 216) - (296, 291)
[Sun Mar 18 06:01:35 2012] XMMSAS bgd. selection expression = annulus(22455.982330, 22021.788132, 1087.500000, 2175.000000, X, Y) && !ellipse(24244.678223, 20834.293091, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(23585.678000, 20274.622000, 1496.248043, 1496.248043, 0.000000, X, Y) && !ellipse(23006.421200, 19370.322000, 1860.616054, 1062.064031, 302.872701, X, Y) && !ellipse(24746.861084, 22042.713745, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(23350.562592, 22135.120712, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22977.084930, 20540.722519, 870.000000, 870.000000, 0.000000, X, Y)
[Sun Mar 18 06:01:35 2012] Writing fullrun_pn_xmm0553911401_pi300-10000_pass1_cl_src35.gif
[Sun Mar 18 06:23:12 2012] Mean detx,y = (290.87, -3519.21) 
[Sun Mar 18 06:23:15 2012] Setting backscal keywords in source and bgd. spectrum
[Sun Mar 18 06:23:29 2012] Binned source spectrum to 10 counts/bin
[Sun Mar 18 06:23:29 2012] Setting source spectrum file to fullrun_pn_xmm0553911401_pi300-10000_pass1_cl_src35_src_b10.pi.gz
[Sun Mar 18 06:23:29 2012] Setting bgd. spectrum file to fullrun_pn_xmm0553911401_pi300-10000_pass1_cl_src35_bgd.pi.gz
[Sun Mar 18 06:45:26 2012] Not generating rmf since there are only 93 counts
[Sun Mar 18 06:45:26 2012] rmf not generated due to insufficient counts
[Sun Mar 18 07:19:29 2012] Updating aperture counts using extracted products
[Sun Mar 18 07:19:29 2012] Error reading totcts from fullrun_pn_xmm0553911401_pi300-10000_pass1_cl_src35_src_b10.pi.gz
[Sun Mar 18 07:19:30 2012] Calculating source flux in energy range 0.30-8.00
[Sun Mar 18 07:19:30 2012] Using photon index=1.80, rate=0.00669, arf fullrun_pn_xmm0553911401_pi300-10000_pass1_cl_src35.arf
[Sun Mar 18 07:19:30 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Sun Mar 18 07:19:30 2012] Updating source flux to 2.3e-14
[Sun Mar 18 07:20:37 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting