[Fri Sep 23 22:15:13 2011] Detection parameters:
  Position = (301.2, 295.2) = 15 6 31.48 1 34 39.1
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 129.6 +/- 19.3
  Background counts = 63.1
  Rate = 0.01 +/- 0.002

[Fri Sep 23 22:15:13 2011] Off-axis axis estimate = 0.31'
[Fri Sep 23 22:17:00 2011] Using EEF radius (= 6.58 ")to estimate initial spatial extent for simple fitting
[Fri Sep 23 22:17:00 2011] Initial guess for spatial extent in simple fitting = 6.58"
[Fri Sep 23 22:17:00 2011] source mask rpix=1.5, npix_max = 16, mask sum = 16, frac = 0.987
[Fri Sep 23 22:17:00 2011] Giving source the simple spatial ID 24 for pass 0, mean size = 6.58"
[Fri Sep 23 23:08:28 2011] fullrun_pn_xmm0021540501_pi300-10000_cl_pass0_src24.ximg exists
[Fri Sep 23 23:08:28 2011] fullrun_pn_xmm0021540501_pi300-10000_cl_pass0_src24_1.ximg exists
[Fri Sep 23 23:08:28 2011] Fit fullrun_pn_xmm0021540501_pi300-10000_cl_pass0_src24 appears to have run properly
[Fri Sep 23 23:08:28 2011] fullrun_pn_xmm0021540501_pi300-10000_cl_pass0_tfrozen_src24.ximg exists
[Fri Sep 23 23:08:28 2011] fullrun_pn_xmm0021540501_pi300-10000_cl_pass0_tfrozen_src24_1.ximg exists
[Fri Sep 23 23:08:28 2011] Fit fullrun_pn_xmm0021540501_pi300-10000_cl_pass0_tfrozen_src24 appears to have run properly
[Sat Sep 24 01:51:42 2011] Source 24 is offset by 5.883511 and 4.754933 pixels which is larger than
2 X fitted extent = 4.386271 x 4.386271, not incorporating fit results
[Sat Sep 24 01:51:42 2011] Vigneting correction estimate = 1.000000
[Sat Sep 24 01:51:42 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Sat Sep 24 01:51:42 2011] Assessing source extent using major
[Sat Sep 24 01:51:42 2011] Source does appear to be extended
[Sat Sep 24 01:51:42 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Sat Sep 24 01:51:42 2011] Source is confused with source 22
[Sat Sep 24 01:51:58 2011] Using EEF radius (= 6.58 ")to estimate initial spatial extent for simple fitting
[Sat Sep 24 01:51:58 2011] Initial guess for spatial extent in simple fitting = 6.58"
[Sat Sep 24 01:51:58 2011] source mask rpix=1.5, npix_max = 16, mask sum = 16, frac = 0.987
[Sat Sep 24 01:51:58 2011] Giving source the simple spatial ID 23 for pass 1, mean size = 6.58"
[Sat Sep 24 03:00:35 2011] fullrun_pn_xmm0021540501_pi300-10000_cl_pass1_src23.ximg exists
[Sat Sep 24 03:00:35 2011] fullrun_pn_xmm0021540501_pi300-10000_cl_pass1_src23_1.ximg exists
[Sat Sep 24 03:00:35 2011] Fit fullrun_pn_xmm0021540501_pi300-10000_cl_pass1_src23 appears to have run properly
[Sat Sep 24 03:00:35 2011] fullrun_pn_xmm0021540501_pi300-10000_cl_pass1_tfrozen_src23.ximg exists
[Sat Sep 24 03:00:35 2011] fullrun_pn_xmm0021540501_pi300-10000_cl_pass1_tfrozen_src23_1.ximg exists
[Sat Sep 24 03:00:35 2011] Fit fullrun_pn_xmm0021540501_pi300-10000_cl_pass1_tfrozen_src23 appears to have run properly
[Sat Sep 24 05:52:21 2011] Source 24 is offset by -3.181661 and 4.405945 pixels which is larger than
2 X fitted extent = 3.200818 x 3.200818, not incorporating fit results
[Sat Sep 24 05:52:21 2011] Warning, spatial fit 23 centroid is now closest to src. 22
[Sat Sep 24 05:52:21 2011] Vigneting correction estimate = 1.000000
[Sat Sep 24 05:52:21 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Sat Sep 24 05:52:21 2011] Assessing source extent using major
[Sat Sep 24 05:52:21 2011] Source does appear to be extended
[Sat Sep 24 05:52:21 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Sat Sep 24 05:52:41 2011] XMMSAS src. selection expression = ellipse(26156.259491, 25630.829193, 652.500000, 652.500000, 0.000000, X, Y)
[Sat Sep 24 05:52:41 2011] Writing source region out to fullrun_pn_xmm0021540501_pi300-10000_pass1_cl_src24_src.reg
[Sat Sep 24 05:52:41 2011] Extracting stamp from image fullrun_pn_xmm0021540501_pi300-10000_cl_sm2.00.img.gz, (264, 258) - (339, 333)
[Sat Sep 24 05:52:41 2011] XMMSAS bgd. selection expression = annulus(26156.259491, 25630.829193, 1087.500000, 2175.000000, X, Y) && !ellipse(26763.793915, 27696.457916, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(24513.152000, 28717.054000, 1232.576035, 1232.576035, 0.000000, X, Y) && !ellipse(26038.139893, 26315.840027, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(23949.523200, 27647.639800, 623.611218, 623.611218, 0.000000, X, Y) && !ellipse(28957.495941, 26569.496216, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(29253.640000, 25770.828000, 1218.496035, 1218.496035, 0.000000, X, Y) && !ellipse(25306.508740, 27437.170000, 2176.544063, 2176.544063, 0.000000, X, Y) && !ellipse(26755.167725, 25724.665894, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27648.824036, 25711.688110, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27062.187347, 25083.303741, 870.000000, 870.000000, 0.000000, X, Y)
[Sat Sep 24 05:52:41 2011] Writing fullrun_pn_xmm0021540501_pi300-10000_pass1_cl_src24.gif
[Sat Sep 24 06:04:07 2011] Mean detx,y = (-852.20, 1714.35) 
[Sat Sep 24 06:04:09 2011] Setting backscal keywords in source and bgd. spectrum
[Sat Sep 24 06:04:28 2011] Binned source spectrum to 10 counts/bin
[Sat Sep 24 06:04:29 2011] Setting source spectrum file to fullrun_pn_xmm0021540501_pi300-10000_pass1_cl_src24_src_b10.pi.gz
[Sat Sep 24 06:04:29 2011] Setting bgd. spectrum file to fullrun_pn_xmm0021540501_pi300-10000_pass1_cl_src24_bgd.pi.gz
[Sat Sep 24 07:44:10 2011] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Sat Sep 24 07:44:10 2011] rmf not generated due to insufficient counts
[Sat Sep 24 09:32:20 2011] Updating aperture counts using extracted products
[Sat Sep 24 09:32:20 2011] Error reading totcts from fullrun_pn_xmm0021540501_pi300-10000_pass1_cl_src24_src_b10.pi.gz
[Sat Sep 24 09:32:21 2011] Calculating source flux in energy range 0.30-8.00
[Sat Sep 24 09:32:21 2011] Using photon index=1.80, rate=0.0111, arf fullrun_pn_xmm0021540501_pi300-10000_pass1_cl_src24.arf
[Sat Sep 24 09:32:21 2011] Assuming count rate is from the 0.30-10.00 bandpass
[Sat Sep 24 09:32:21 2011] Updating source flux to 3.1e-14
[Sat Sep 24 09:37:25 2011] Simple spatial fitting not done (or not done successfully), skipping spectral fitting