[Mon Dec 19 23:23:29 2011] Detection parameters:
  Position = (302.3, 374.2) = 16 15 36.63 -22 38 40.0
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 314.0 +/- 25.1
  Background counts = 266.5
  Rate = 0.003 +/- 0.0002

[Mon Dec 19 23:23:31 2011] Off-axis axis estimate = 5.50'
[Mon Dec 19 23:34:21 2011] Using EEF radius (= 9.18 ")to estimate initial spatial extent for simple fitting
[Mon Dec 19 23:34:21 2011] Initial guess for spatial extent in simple fitting = 9.18"
[Mon Dec 19 23:34:21 2011] source mask rpix=2.1, npix_max = 27, mask sum = 12, frac = 0.440
[Mon Dec 19 23:34:21 2011] Skipping simple spatial due to low active detector fraction
[Tue Dec 20 06:26:41 2011] Vigneting correction estimate = 1.000000
[Tue Dec 20 06:26:41 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Tue Dec 20 06:26:41 2011] Assessing source extent using major
[Tue Dec 20 06:26:41 2011] Source does appear to be extended
[Tue Dec 20 06:26:41 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Tue Dec 20 06:26:41 2011] Source is confused with source 30
[Tue Dec 20 06:27:35 2011] Using EEF radius (= 9.18 ")to estimate initial spatial extent for simple fitting
[Tue Dec 20 06:27:35 2011] Initial guess for spatial extent in simple fitting = 9.18"
[Tue Dec 20 06:27:35 2011] source mask rpix=2.1, npix_max = 27, mask sum = 12, frac = 0.440
[Tue Dec 20 06:27:35 2011] Skipping simple spatial due to low active detector fraction
[Tue Dec 20 13:16:38 2011] Vigneting correction estimate = 1.000000
[Tue Dec 20 13:16:38 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Tue Dec 20 13:16:38 2011] Assessing source extent using major
[Tue Dec 20 13:16:38 2011] Source does appear to be extended
[Tue Dec 20 13:16:38 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Tue Dec 20 13:17:34 2011] XMMSAS src. selection expression = ellipse(26252.541473, 32503.592896, 652.500000, 652.500000, 0.000000, X, Y)
[Tue Dec 20 13:17:34 2011] Writing source region out to fullrun_pn_xmm0555650301_pi300-10000_pass1_cl_src40_src.reg
[Tue Dec 20 13:17:34 2011] Extracting stamp from image fullrun_pn_xmm0555650301_pi300-10000_cl_sm2.00.img.gz, (265, 337) - (340, 412)
[Tue Dec 20 13:17:34 2011] XMMSAS bgd. selection expression = annulus(26252.541473, 32503.592896, 1087.500000, 2175.000000, X, Y) && !ellipse(28758.795980, 31615.933400, 436.594413, 436.594413, 0.000000, X, Y) && !ellipse(25607.013680, 30193.262800, 824.552024, 398.639211, 152.325000, X, Y) && !ellipse(25703.178741, 32164.519104, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26675.758453, 33909.784027, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(24620.809356, 29266.011013, 1188.425534, 744.935834, 90.901184, X, Y)
[Tue Dec 20 13:17:34 2011] Writing fullrun_pn_xmm0555650301_pi300-10000_pass1_cl_src40.gif
[Tue Dec 20 15:07:19 2011] Mean detx,y = (326.31, -4897.18) 
[Tue Dec 20 15:07:25 2011] Setting backscal keywords in source and bgd. spectrum
[Tue Dec 20 15:07:56 2011] Binned source spectrum to 10 counts/bin
[Tue Dec 20 15:07:57 2011] Setting source spectrum file to fullrun_pn_xmm0555650301_pi300-10000_pass1_cl_src40_src_b10.pi.gz
[Tue Dec 20 15:07:57 2011] Setting bgd. spectrum file to fullrun_pn_xmm0555650301_pi300-10000_pass1_cl_src40_bgd.pi.gz
[Tue Dec 20 17:57:11 2011] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Tue Dec 20 17:57:11 2011] rmf not generated due to insufficient counts
[Tue Dec 20 23:04:46 2011] Updating aperture counts using extracted products
[Tue Dec 20 23:04:46 2011] Error reading totcts from fullrun_pn_xmm0555650301_pi300-10000_pass1_cl_src40_src_b10.pi.gz
[Tue Dec 20 23:04:50 2011] Calculating source flux in energy range 0.30-8.00
[Tue Dec 20 23:04:50 2011] Using photon index=1.80, rate=0.00303, arf fullrun_pn_xmm0555650301_pi300-10000_pass1_cl_src40.arf
[Tue Dec 20 23:04:50 2011] Assuming count rate is from the 0.30-10.00 bandpass
[Tue Dec 20 23:04:50 2011] Updating source flux to 1e-14
[Tue Dec 20 23:15:44 2011] Simple spatial fitting not done (or not done successfully), skipping spectral fitting