[Sun Dec 25 00:26:26 2011] Detection parameters:
  Position = (248.6, 332.5) = 9 59 39.51 2 31 44.6
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 54.9 +/- 12.4
  Background counts = 28.5
  Rate = 0.003 +/- 0.0006

[Sun Dec 25 00:26:28 2011] Off-axis axis estimate = 4.38'
[Sun Dec 25 00:31:16 2011] Using EEF radius (= 8.62 ")to estimate initial spatial extent for simple fitting
[Sun Dec 25 00:31:16 2011] Initial guess for spatial extent in simple fitting = 8.62"
[Sun Dec 25 00:31:16 2011] source mask rpix=2.0, npix_max = 24, mask sum = 25, frac = 1.015
[Sun Dec 25 00:31:16 2011] Giving source the simple spatial ID 14 for pass 0, mean size = 8.62"
[Sun Dec 25 04:10:30 2011] fullrun_pn_xmm0203361701_pi300-10000_cl_pass0_src14.ximg exists
[Sun Dec 25 04:10:30 2011] fullrun_pn_xmm0203361701_pi300-10000_cl_pass0_src14_1.ximg exists
[Sun Dec 25 04:10:30 2011] Fit fullrun_pn_xmm0203361701_pi300-10000_cl_pass0_src14 appears to have run properly
[Sun Dec 25 04:10:31 2011] fullrun_pn_xmm0203361701_pi300-10000_cl_pass0_tfrozen_src14.ximg exists
[Sun Dec 25 04:10:31 2011] fullrun_pn_xmm0203361701_pi300-10000_cl_pass0_tfrozen_src14_1.ximg exists
[Sun Dec 25 04:10:31 2011] Fit fullrun_pn_xmm0203361701_pi300-10000_cl_pass0_tfrozen_src14 appears to have run properly
[Sun Dec 25 08:42:08 2011] Warning, spatial fit 14 centroid is now closest to src. 17
[Sun Dec 25 08:42:08 2011] Source 14 is offset by -7.188989 and -1.264520 pixels which is larger than
2 X fitted extent = 0.976230 x 0.976230, not incorporating fit results
[Sun Dec 25 08:42:08 2011] Vigneting correction estimate = 1.000000
[Sun Dec 25 08:42:08 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Sun Dec 25 08:42:08 2011] Assessing source extent using major
[Sun Dec 25 08:42:08 2011] Source does appear to be extended
[Sun Dec 25 08:42:08 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Sun Dec 25 08:42:08 2011] Source is confused with source 17
[Sun Dec 25 08:42:08 2011] Source is confused with source 18
[Sun Dec 25 08:42:53 2011] Using EEF radius (= 8.62 ")to estimate initial spatial extent for simple fitting
[Sun Dec 25 08:42:53 2011] Initial guess for spatial extent in simple fitting = 8.62"
[Sun Dec 25 08:42:53 2011] source mask rpix=2.0, npix_max = 24, mask sum = 25, frac = 1.015
[Sun Dec 25 08:42:53 2011] Giving source the simple spatial ID 14 for pass 1, mean size = 8.62"
[Sun Dec 25 13:09:52 2011] fullrun_pn_xmm0203361701_pi300-10000_cl_pass1_src14.ximg exists
[Sun Dec 25 13:09:52 2011] fullrun_pn_xmm0203361701_pi300-10000_cl_pass1_src14_1.ximg exists
[Sun Dec 25 13:09:52 2011] Fit fullrun_pn_xmm0203361701_pi300-10000_cl_pass1_src14 appears to have run properly
[Sun Dec 25 13:09:53 2011] fullrun_pn_xmm0203361701_pi300-10000_cl_pass1_tfrozen_src14.ximg exists
[Sun Dec 25 13:09:53 2011] fullrun_pn_xmm0203361701_pi300-10000_cl_pass1_tfrozen_src14_1.ximg exists
[Sun Dec 25 13:09:53 2011] Fit fullrun_pn_xmm0203361701_pi300-10000_cl_pass1_tfrozen_src14 appears to have run properly
[Sun Dec 25 17:53:18 2011] Warning, spatial fit 14 centroid is now closest to src. 17
[Sun Dec 25 17:53:18 2011] Warning: source 22 in spatial fitting list does not appear to have a counterpart in memory, closest src. was src. 14 at 11.022886 pixels away
[Sun Dec 25 17:53:18 2011] Warning: source 23 in spatial fitting list does not appear to have a counterpart in memory, closest src. was src. 14 at 39.851272 pixels away
[Sun Dec 25 17:53:19 2011] Vigneting correction estimate = 1.000000
[Sun Dec 25 17:53:19 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Sun Dec 25 17:53:19 2011] Assessing source extent using major
[Sun Dec 25 17:53:19 2011] Source does appear to be extended
[Sun Dec 25 17:53:19 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Sun Dec 25 17:54:18 2011] XMMSAS src. selection expression = ellipse(21581.513916, 28882.942719, 652.500000, 652.500000, 0.000000, X, Y)
[Sun Dec 25 17:54:18 2011] Writing source region out to fullrun_pn_xmm0203361701_pi300-10000_pass1_cl_src14_src.reg
[Sun Dec 25 17:54:18 2011] Extracting stamp from image fullrun_pn_xmm0203361701_pi300-10000_cl_sm2.00.img.gz, (211, 295) - (286, 370)
[Sun Dec 25 17:54:19 2011] XMMSAS bgd. selection expression = annulus(21581.513916, 28882.942719, 1087.500000, 2175.000000, X, Y) && !ellipse(21887.149009, 30765.187811, 428.509450, 309.805922, 176.174360, X, Y) && !ellipse(20888.396000, 28718.600000, 1378.744040, 609.872818, 359.450000, X, Y) && !ellipse(21041.594000, 28404.295800, 1783.904051, 1783.904051, 0.000000, X, Y) && !ellipse(23645.055000, 27564.050400, 321.181609, 321.181609, 0.000000, X, Y) && !ellipse(22657.000792, 27613.464800, 335.048010, 335.048010, 0.000000, X, Y) && !ellipse(21035.422000, 27752.788800, 961.904028, 961.904028, 0.000000, X, Y)
[Sun Dec 25 17:54:19 2011] Writing fullrun_pn_xmm0203361701_pi300-10000_pass1_cl_src14.gif
[Sun Dec 25 18:15:35 2011] Mean detx,y = (1816.93, 5884.99) 
[Sun Dec 25 18:15:45 2011] Setting backscal keywords in source and bgd. spectrum
[Sun Dec 25 18:16:25 2011] Binned source spectrum to 10 counts/bin
[Sun Dec 25 18:16:27 2011] Setting source spectrum file to fullrun_pn_xmm0203361701_pi300-10000_pass1_cl_src14_src_b10.pi.gz
[Sun Dec 25 18:16:27 2011] Setting bgd. spectrum file to fullrun_pn_xmm0203361701_pi300-10000_pass1_cl_src14_bgd.pi.gz
[Sun Dec 25 19:38:59 2011] Not generating rmf since there are only 54 counts
[Sun Dec 25 19:38:59 2011] rmf not generated due to insufficient counts
[Sun Dec 25 22:25:35 2011] Updating aperture counts using extracted products
[Sun Dec 25 22:25:35 2011] Error reading totcts from fullrun_pn_xmm0203361701_pi300-10000_pass1_cl_src14_src_b10.pi.gz
[Sun Dec 25 22:25:42 2011] Calculating source flux in energy range 0.30-8.00
[Sun Dec 25 22:25:42 2011] Using photon index=1.80, rate=0.00254, arf fullrun_pn_xmm0203361701_pi300-10000_pass1_cl_src14.arf
[Sun Dec 25 22:25:42 2011] Assuming count rate is from the 0.30-10.00 bandpass
[Sun Dec 25 22:25:42 2011] Updating source flux to 8.2e-15
[Sun Dec 25 22:27:39 2011] Simple spatial fitting not done (or not done successfully), skipping spectral fitting