[Fri Aug 17 23:00:20 2012] Detection parameters:
  Position = (312.4, 339.1) = 8 34 27.87 -45 44 23.9
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 320.8 +/- 37.8
  Background counts = 402.4
  Rate = 0.02 +/- 0.003

[Fri Aug 17 23:00:21 2012] Off-axis axis estimate = 3.12'
[Fri Aug 17 23:03:56 2012] Using EEF radius (= 7.99 ")to estimate initial spatial extent for simple fitting
[Fri Aug 17 23:03:56 2012] Initial guess for spatial extent in simple fitting = 7.99"
[Fri Aug 17 23:03:56 2012] source mask rpix=1.8, npix_max = 21, mask sum = 10, frac = 0.458
[Fri Aug 17 23:03:56 2012] Skipping simple spatial due to low active detector fraction
[Sat Aug 18 01:33:43 2012] Source 12 is offset by -1.780107 and -4.093004 pixels which is larger than
2 X fitted extent = 0.896892 x 0.896892, not incorporating fit results
[Sat Aug 18 01:33:43 2012] Source 12 is offset by -0.159509 and 2.636652 pixels which is larger than
2 X fitted extent = 0.930685 x 0.930685, not incorporating fit results
[Sat Aug 18 01:33:43 2012] Vigneting correction estimate = 1.000000
[Sat Aug 18 01:33:43 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Sat Aug 18 01:33:43 2012] Assessing source extent using major
[Sat Aug 18 01:33:43 2012] Source does appear to be extended
[Sat Aug 18 01:33:43 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Sat Aug 18 01:33:43 2012] Source is confused with source 2
[Sat Aug 18 01:33:55 2012] Using EEF radius (= 7.99 ")to estimate initial spatial extent for simple fitting
[Sat Aug 18 01:33:55 2012] Initial guess for spatial extent in simple fitting = 7.99"
[Sat Aug 18 01:33:55 2012] source mask rpix=1.8, npix_max = 21, mask sum = 10, frac = 0.458
[Sat Aug 18 01:33:55 2012] Skipping simple spatial due to low active detector fraction
[Sat Aug 18 03:29:28 2012] Source 12 is offset by -1.780107 and -4.093004 pixels which is larger than
2 X fitted extent = 0.896892 x 0.896892, not incorporating fit results
[Sat Aug 18 03:29:28 2012] Source 12 is offset by -6.992475 and -0.826429 pixels which is larger than
2 X fitted extent = 2.824377 x 2.824377, not incorporating fit results
[Sat Aug 18 03:29:28 2012] Vigneting correction estimate = 1.000000
[Sat Aug 18 03:29:29 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Sat Aug 18 03:29:29 2012] Assessing source extent using major
[Sat Aug 18 03:29:29 2012] Source does appear to be extended
[Sat Aug 18 03:29:29 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Sat Aug 18 03:29:40 2012] XMMSAS src. selection expression = ellipse(27129.866699, 29451.644684, 652.500000, 652.500000, 0.000000, X, Y)
[Sat Aug 18 03:29:40 2012] Writing source region out to fullrun_pn_xmm0094630101_pi300-10000_pass1_cl_src12_src.reg
[Sat Aug 18 03:29:40 2012] Extracting stamp from image fullrun_pn_xmm0094630101_pi300-10000_cl_sm2.00.img.gz, (275, 302) - (350, 377)
[Sat Aug 18 03:29:41 2012] XMMSAS bgd. selection expression = annulus(27129.866699, 29451.644684, 1087.500000, 2175.000000, X, Y) && !ellipse(26763.199188, 29881.586853, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26350.413818, 31413.968872, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26675.662872, 29125.232727, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25452.014000, 32262.397200, 1444.904042, 1444.904042, 0.000000, X, Y) && !ellipse(27068.347015, 31263.367645, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25425.260895, 31199.867310, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26352.349335, 30932.293457, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27141.925842, 30578.816132, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26527.403381, 30193.228882, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(28198.054016, 30045.513672, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25045.800000, 29851.896000, 1271.272037, 1271.272037, 0.000000, X, Y) && !ellipse(26616.511475, 29791.143280, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(28382.257294, 29517.242493, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(25596.605865, 29541.971436, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(28401.293854, 28565.749023, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27835.663757, 28491.325897, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26720.198334, 28223.356445, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27347.863190, 27803.442322, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(28045.105743, 27705.556702, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27211.041565, 28234.130554, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27706.868286, 27144.551666, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(29356.809692, 27023.503571, 870.000000, 870.000000, 0.000000, X, Y)
[Sat Aug 18 03:29:41 2012] Writing fullrun_pn_xmm0094630101_pi300-10000_pass1_cl_src12.gif
[Sat Aug 18 03:41:36 2012] Mean detx,y = (944.15, -1744.07) 
[Sat Aug 18 03:41:39 2012] Setting backscal keywords in source and bgd. spectrum
[Sat Aug 18 03:41:54 2012] Binned source spectrum to 10 counts/bin
[Sat Aug 18 03:41:55 2012] Setting source spectrum file to fullrun_pn_xmm0094630101_pi300-10000_pass1_cl_src12_src_b10.pi.gz
[Sat Aug 18 03:41:55 2012] Setting bgd. spectrum file to fullrun_pn_xmm0094630101_pi300-10000_pass1_cl_src12_bgd.pi.gz
[Sat Aug 18 04:19:47 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Sat Aug 18 04:19:47 2012] rmf not generated due to insufficient counts
[Sat Aug 18 05:08:12 2012] Updating aperture counts using extracted products
[Sat Aug 18 05:08:12 2012] Error reading totcts from fullrun_pn_xmm0094630101_pi300-10000_pass1_cl_src12_src_b10.pi.gz
[Sat Aug 18 05:08:13 2012] Calculating source flux in energy range 0.30-8.00
[Sat Aug 18 05:08:13 2012] Using photon index=1.80, rate=0.0231, arf fullrun_pn_xmm0094630101_pi300-10000_pass1_cl_src12.arf
[Sat Aug 18 05:08:13 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Sat Aug 18 05:08:13 2012] Updating source flux to 7.3e-14
[Sat Aug 18 05:08:28 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting