[Sun Nov 27 22:43:57 2011] Detection parameters:
  Position = (324.3, 353.9) = 18 1 41.16 -23 15 26.4
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 104.5 +/- 16.9
  Background counts = 59.2
  Rate = 0.006 +/- 0.0009

[Sun Nov 27 22:43:59 2011] Off-axis axis estimate = 4.44'
[Mon Nov 28 12:06:13 2011] Using EEF radius (= 8.65 ")to estimate initial spatial extent for simple fitting
[Mon Nov 28 12:06:13 2011] Initial guess for spatial extent in simple fitting = 8.65"
[Mon Nov 28 12:06:13 2011] source mask rpix=2.0, npix_max = 24, mask sum = 25, frac = 1.009
[Mon Nov 28 12:06:13 2011] Giving source the simple spatial ID 16 for pass 0, mean size = 8.65"
[Mon Nov 28 17:18:41 2011] fullrun_mos2_xmm0145970101_pi300-10000_cl_pass0_src16.ximg exists
[Mon Nov 28 17:18:41 2011] fullrun_mos2_xmm0145970101_pi300-10000_cl_pass0_src16_1.ximg exists
[Mon Nov 28 17:18:41 2011] Fit fullrun_mos2_xmm0145970101_pi300-10000_cl_pass0_src16 appears to have run properly
[Mon Nov 28 17:18:42 2011] fullrun_mos2_xmm0145970101_pi300-10000_cl_pass0_tfrozen_src16.ximg exists
[Mon Nov 28 17:18:42 2011] fullrun_mos2_xmm0145970101_pi300-10000_cl_pass0_tfrozen_src16_1.ximg exists
[Mon Nov 28 17:18:42 2011] Fit fullrun_mos2_xmm0145970101_pi300-10000_cl_pass0_tfrozen_src16 appears to have run properly
[Mon Nov 28 17:19:49 2011] Warning: source 16 in spatial fitting list does not appear to have a counterpart in memory, closest src. was src. 16 at 10.943966 pixels away
[Mon Nov 28 17:19:49 2011] Vigneting correction estimate = 1.000000
[Mon Nov 28 17:19:49 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Mon Nov 28 17:19:49 2011] Assessing source extent using major
[Mon Nov 28 17:19:49 2011] Source does appear to be extended
[Mon Nov 28 17:19:49 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Mon Nov 28 17:19:49 2011] Source is confused with source 22
[Tue Nov 29 06:27:52 2011] Using EEF radius (= 8.65 ")to estimate initial spatial extent for simple fitting
[Tue Nov 29 06:27:52 2011] Initial guess for spatial extent in simple fitting = 8.65"
[Tue Nov 29 06:27:52 2011] source mask rpix=2.0, npix_max = 24, mask sum = 25, frac = 1.009
[Tue Nov 29 06:27:52 2011] Giving source the simple spatial ID 15 for pass 1, mean size = 8.65"
[Tue Nov 29 10:56:04 2011] fullrun_mos2_xmm0145970101_pi300-10000_cl_pass1_src15.ximg exists
[Tue Nov 29 10:56:04 2011] fullrun_mos2_xmm0145970101_pi300-10000_cl_pass1_src15_1.ximg exists
[Tue Nov 29 10:56:04 2011] Fit fullrun_mos2_xmm0145970101_pi300-10000_cl_pass1_src15 appears to have run properly
[Tue Nov 29 10:56:05 2011] fullrun_mos2_xmm0145970101_pi300-10000_cl_pass1_tfrozen_src15.ximg exists
[Tue Nov 29 10:56:05 2011] fullrun_mos2_xmm0145970101_pi300-10000_cl_pass1_tfrozen_src15_1.ximg exists
[Tue Nov 29 10:56:05 2011] Fit fullrun_mos2_xmm0145970101_pi300-10000_cl_pass1_tfrozen_src15 appears to have run properly
[Tue Nov 29 10:56:52 2011] Warning, spatial fit 15 centroid is now closest to src. 22
[Tue Nov 29 10:56:52 2011] Warning: source 21 in spatial fitting list does not appear to have a counterpart in memory, closest src. was src. 16 at 13.261047 pixels away
[Tue Nov 29 10:56:52 2011] Vigneting correction estimate = 1.000000
[Tue Nov 29 10:56:52 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Tue Nov 29 10:56:52 2011] Assessing source extent using major
[Tue Nov 29 10:56:52 2011] Source does appear to be extended
[Tue Nov 29 10:56:52 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Wed Nov 30 21:00:35 2011] XMMSAS src. selection expression = ellipse(28168.137146, 30744.617401, 652.500000, 652.500000, 0.000000, X, Y)
[Wed Nov 30 21:00:35 2011] Writing source region out to fullrun_mos2_xmm0145970101_pi300-10000_pass1_cl_src16_src.reg
[Wed Nov 30 21:00:35 2011] Extracting stamp from image fullrun_mos2_xmm0145970101_pi300-10000_cl_sm2.00.img.gz, (287, 316) - (362, 391)
[Wed Nov 30 21:00:35 2011] XMMSAS bgd. selection expression = annulus(28168.137146, 30744.617401, 1087.500000, 2175.000000, X, Y) && !ellipse(26658.314600, 30093.733600, 1307.896038, 1307.896038, 0.000000, X, Y) && !ellipse(26223.088200, 29724.550220, 1037.184030, 1037.184030, 0.000000, X, Y) && !ellipse(27040.906397, 27478.938388, 2275.280065, 1773.888765, 82.776456, X, Y) && !ellipse(26157.876901, 29630.691848, 1186.787054, 679.647864, 289.163815, X, Y) && !ellipse(26723.138140, 28739.124000, 1942.704056, 1942.704056, 0.000000, X, Y) && !ellipse(30263.152000, 34846.608000, 2501.488072, 1130.960033, 152.991000, X, Y) && !ellipse(26709.758600, 28028.159200, 971.352028, 971.352028, 0.000000, X, Y) && !ellipse(28321.202800, 31082.046000, 1383.816040, 1383.816040, 0.000000, X, Y) && !ellipse(29328.604000, 33744.396000, 1666.200048, 1666.200048, 0.000000, X, Y)
[Wed Nov 30 21:00:35 2011] Writing fullrun_mos2_xmm0145970101_pi300-10000_pass1_cl_src16.gif
[Wed Nov 30 21:08:28 2011] Mean detx,y = (-1079.48, 3199.94) 
[Wed Nov 30 21:08:29 2011] Setting backscal keywords in source and bgd. spectrum
[Wed Nov 30 21:08:39 2011] Binned source spectrum to 10 counts/bin
[Wed Nov 30 21:08:40 2011] Setting source spectrum file to fullrun_mos2_xmm0145970101_pi300-10000_pass1_cl_src16_src_b10.pi.gz
[Wed Nov 30 21:08:40 2011] Setting bgd. spectrum file to fullrun_mos2_xmm0145970101_pi300-10000_pass1_cl_src16_bgd.pi.gz
[Wed Nov 30 22:15:56 2011] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Wed Nov 30 22:15:56 2011] rmf not generated due to insufficient counts
[Wed Nov 30 22:34:56 2011] Updating aperture counts using extracted products
[Wed Nov 30 22:34:56 2011] Error reading totcts from fullrun_mos2_xmm0145970101_pi300-10000_pass1_cl_src16_src_b10.pi.gz
[Wed Nov 30 22:34:58 2011] Calculating source flux in energy range 0.30-8.00
[Wed Nov 30 22:34:58 2011] Using photon index=1.80, rate=0.0057, arf fullrun_mos2_xmm0145970101_pi300-10000_pass1_cl_src16.arf
[Wed Nov 30 22:34:58 2011] Assuming count rate is from the 0.30-10.00 bandpass
[Wed Nov 30 22:34:58 2011] Updating source flux to 8.4e-14
[Wed Nov 30 22:40:33 2011] Simple spatial fitting not done (or not done successfully), skipping spectral fitting