[Wed Mar 14 22:07:25 2012] Detection parameters:
  Position = (341.8, 337.2) = 15 10 47.28 5 46 41.9
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 258.2 +/- 39.2
  Background counts = 691.0
  Rate = 0.006 +/- 0.0009

[Wed Mar 14 22:07:26 2012] Off-axis axis estimate = 4.21'
[Wed Mar 14 22:15:52 2012] Using EEF radius (= 8.54 ")to estimate initial spatial extent for simple fitting
[Wed Mar 14 22:15:52 2012] Initial guess for spatial extent in simple fitting = 8.54"
[Wed Mar 14 22:15:52 2012] source mask rpix=2.0, npix_max = 24, mask sum = 9, frac = 0.371
[Wed Mar 14 22:15:52 2012] Skipping simple spatial due to low active detector fraction
[Thu Mar 15 16:49:52 2012] Vigneting correction estimate = 1.000000
[Thu Mar 15 16:49:52 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Thu Mar 15 16:49:52 2012] Assessing source extent using major
[Thu Mar 15 16:49:52 2012] Source does appear to be extended
[Thu Mar 15 16:49:52 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Thu Mar 15 16:49:52 2012] Source is confused with source 23
[Thu Mar 15 16:50:26 2012] Using EEF radius (= 8.54 ")to estimate initial spatial extent for simple fitting
[Thu Mar 15 16:50:26 2012] Initial guess for spatial extent in simple fitting = 8.54"
[Thu Mar 15 16:50:26 2012] source mask rpix=2.0, npix_max = 24, mask sum = 9, frac = 0.371
[Thu Mar 15 16:50:26 2012] Skipping simple spatial due to low active detector fraction
[Fri Mar 16 10:54:05 2012] Vigneting correction estimate = 1.000000
[Fri Mar 16 10:54:05 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Fri Mar 16 10:54:05 2012] Assessing source extent using major
[Fri Mar 16 10:54:05 2012] Source does appear to be extended
[Fri Mar 16 10:54:05 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Fri Mar 16 10:54:43 2012] XMMSAS src. selection expression = ellipse(29686.508575, 29286.212463, 652.500000, 652.500000, 0.000000, X, Y)
[Fri Mar 16 10:54:43 2012] Writing source region out to fullrun_pn_xmm0551780301_pi300-10000_pass1_cl_src21_src.reg
[Fri Mar 16 10:54:43 2012] Extracting stamp from image fullrun_pn_xmm0551780301_pi300-10000_cl_sm2.00.img.gz, (304, 300) - (379, 375)
[Fri Mar 16 10:54:43 2012] XMMSAS bgd. selection expression = annulus(29686.508575, 29286.212463, 1087.500000, 2175.000000, X, Y) && !ellipse(27131.108600, 26751.171000, 3357.984097, 3357.984097, 0.000000, X, Y) && !ellipse(26678.660400, 29513.581207, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(32637.427612, 30954.250549, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(29838.893982, 28854.225922, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27802.359070, 31480.835785, 870.000000, 870.000000, 0.000000, X, Y)
[Fri Mar 16 10:54:43 2012] Writing fullrun_pn_xmm0551780301_pi300-10000_pass1_cl_src21.gif
[Fri Mar 16 11:43:56 2012] Mean detx,y = (3871.50, -100.04) 
[Fri Mar 16 11:44:01 2012] Setting backscal keywords in source and bgd. spectrum
[Fri Mar 16 11:44:31 2012] Binned source spectrum to 10 counts/bin
[Fri Mar 16 11:44:31 2012] Setting source spectrum file to fullrun_pn_xmm0551780301_pi300-10000_pass1_cl_src21_src_b10.pi.gz
[Fri Mar 16 11:44:31 2012] Setting bgd. spectrum file to fullrun_pn_xmm0551780301_pi300-10000_pass1_cl_src21_bgd.pi.gz
[Fri Mar 16 20:56:18 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Fri Mar 16 20:56:18 2012] rmf not generated due to insufficient counts
[Mon Mar 19 05:35:25 2012] Updating aperture counts using extracted products
[Mon Mar 19 05:35:25 2012] Error reading totcts from fullrun_pn_xmm0551780301_pi300-10000_pass1_cl_src21_src_b10.pi.gz
[Mon Mar 19 05:35:27 2012] Calculating source flux in energy range 0.30-8.00
[Mon Mar 19 05:35:27 2012] Using photon index=1.80, rate=0.00606, arf fullrun_pn_xmm0551780301_pi300-10000_pass1_cl_src21.arf
[Mon Mar 19 05:35:27 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Mon Mar 19 05:35:27 2012] Updating source flux to 2e-14
[Mon Mar 19 05:39:35 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting