[Sun Feb 19 11:55:46 2012] Detection parameters:
  Position = (349.5, 319.2) = 15 10 45.16 5 45 21.8
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 347.7 +/- 36.1
  Background counts = 746.8
  Rate = 0.008 +/- 0.0008

[Sun Feb 19 11:55:48 2012] Off-axis axis estimate = 4.00'
[Sun Feb 19 12:06:31 2012] Using EEF radius (= 8.43 ")to estimate initial spatial extent for simple fitting
[Sun Feb 19 12:06:31 2012] Initial guess for spatial extent in simple fitting = 8.43"
[Sun Feb 19 12:06:31 2012] source mask rpix=1.9, npix_max = 23, mask sum = 9, frac = 0.379
[Sun Feb 19 12:06:31 2012] Skipping simple spatial due to low active detector fraction
[Mon Feb 20 10:14:24 2012] Vigneting correction estimate = 1.000000
[Mon Feb 20 10:14:24 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Mon Feb 20 10:14:24 2012] Assessing source extent using major
[Mon Feb 20 10:14:24 2012] Source does appear to be extended
[Mon Feb 20 10:14:24 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Mon Feb 20 10:14:24 2012] Source is confused with source 4
[Mon Feb 20 10:15:09 2012] Using EEF radius (= 8.43 ")to estimate initial spatial extent for simple fitting
[Mon Feb 20 10:15:09 2012] Initial guess for spatial extent in simple fitting = 8.43"
[Mon Feb 20 10:15:09 2012] source mask rpix=1.9, npix_max = 23, mask sum = 9, frac = 0.379
[Mon Feb 20 10:15:09 2012] Skipping simple spatial due to low active detector fraction
[Mon Feb 20 18:29:38 2012] Vigneting correction estimate = 1.000000
[Mon Feb 20 18:29:38 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Mon Feb 20 18:29:38 2012] Assessing source extent using major
[Mon Feb 20 18:29:38 2012] Source does appear to be extended
[Mon Feb 20 18:29:38 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Mon Feb 20 18:30:16 2012] XMMSAS src. selection expression = ellipse(30358.013275, 27724.256073, 652.500000, 652.500000, 0.000000, X, Y)
[Mon Feb 20 18:30:16 2012] Writing source region out to fullrun_pn_xmm0551780401_pi300-10000_pass1_cl_src44_src.reg
[Mon Feb 20 18:30:16 2012] Extracting stamp from image fullrun_pn_xmm0551780401_pi300-10000_cl_sm2.00.img.gz, (312, 282) - (387, 357)
[Mon Feb 20 18:30:16 2012] XMMSAS bgd. selection expression = annulus(30358.013275, 27724.256073, 1087.500000, 2175.000000, X, Y) && !ellipse(26994.603000, 26800.413200, 6718.800193, 6718.800193, 0.000000, X, Y) && !ellipse(29931.676636, 28140.535461, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(29955.070000, 29231.542000, 1380.632040, 802.448023, 54.858000, X, Y) && !ellipse(28714.674927, 30497.715607, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(30358.727478, 28769.570312, 870.000000, 870.000000, 0.000000, X, Y)
[Mon Feb 20 18:30:16 2012] Writing fullrun_pn_xmm0551780401_pi300-10000_pass1_cl_src44.gif
[Mon Feb 20 20:19:03 2012] Mean detx,y = (3868.37, 1512.86) 
[Mon Feb 20 20:19:07 2012] Setting backscal keywords in source and bgd. spectrum
[Mon Feb 20 20:19:46 2012] Binned source spectrum to 10 counts/bin
[Mon Feb 20 20:19:47 2012] Setting source spectrum file to fullrun_pn_xmm0551780401_pi300-10000_pass1_cl_src44_src_b10.pi.gz
[Mon Feb 20 20:19:47 2012] Setting bgd. spectrum file to fullrun_pn_xmm0551780401_pi300-10000_pass1_cl_src44_bgd.pi.gz
[Wed Feb 22 21:15:53 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Wed Feb 22 21:15:53 2012] rmf not generated due to insufficient counts
[Fri Feb 24 20:52:35 2012] Updating aperture counts using extracted products
[Fri Feb 24 20:52:35 2012] Error reading totcts from fullrun_pn_xmm0551780401_pi300-10000_pass1_cl_src44_src_b10.pi.gz
[Fri Feb 24 20:52:38 2012] Calculating source flux in energy range 0.30-8.00
[Fri Feb 24 20:52:38 2012] Using photon index=1.80, rate=0.00816, arf fullrun_pn_xmm0551780401_pi300-10000_pass1_cl_src44.arf
[Fri Feb 24 20:52:38 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Fri Feb 24 20:52:38 2012] Updating source flux to 2.9e-14
[Fri Feb 24 21:00:53 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting