[Sat Dec 31 13:38:05 2011] Detection parameters:
  Position = (345.6, 133.2) = 14 41 28.65 -62 26 40.8
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 117.2 +/- 18.2
  Background counts = 68.7
  Rate = 0.002 +/- 0.0002

[Sat Dec 31 13:38:05 2011] Off-axis axis estimate = 12.46'
[Sun Jan  1 11:59:28 2012] Using EEF radius (= 12.66 ")to estimate initial spatial extent for simple fitting
[Sun Jan  1 11:59:28 2012] Initial guess for spatial extent in simple fitting = 12.66"
[Sun Jan  1 11:59:28 2012] source mask rpix=2.9, npix_max = 46, mask sum = 47, frac = 1.010
[Sun Jan  1 11:59:28 2012] Giving source the simple spatial ID 127 for pass 0, mean size = 12.66"
[Sun Jan  1 23:38:54 2012] Vigneting correction estimate = 1.000000
[Sun Jan  1 23:38:54 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Sun Jan  1 23:38:54 2012] Assessing source extent using major
[Sun Jan  1 23:38:54 2012] Source does appear to be extended
[Sun Jan  1 23:38:54 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Tue Jan  3 05:59:05 2012] Using EEF radius (= 12.66 ")to estimate initial spatial extent for simple fitting
[Tue Jan  3 05:59:05 2012] Initial guess for spatial extent in simple fitting = 12.66"
[Tue Jan  3 05:59:05 2012] source mask rpix=2.9, npix_max = 46, mask sum = 47, frac = 1.010
[Tue Jan  3 05:59:05 2012] Giving source the simple spatial ID 122 for pass 1, mean size = 12.66"
[Tue Jan  3 21:36:36 2012] Vigneting correction estimate = 1.000000
[Tue Jan  3 21:36:36 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Tue Jan  3 21:36:36 2012] Assessing source extent using major
[Tue Jan  3 21:36:36 2012] Source does appear to be extended
[Tue Jan  3 21:36:36 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Thu Jan  5 18:24:49 2012] XMMSAS src. selection expression = ellipse(30022.202515, 11536.818573, 652.500000, 652.500000, 0.000000, X, Y)
[Thu Jan  5 18:24:49 2012] Writing source region out to fullrun_mos2_xmm0504810301_pi300-10000_pass1_cl_src162_src.reg
[Thu Jan  5 18:24:49 2012] Extracting stamp from image fullrun_mos2_xmm0504810301_pi300-10000_cl_sm2.00.img.gz, (308, 96) - (383, 171)
[Thu Jan  5 18:24:49 2012] XMMSAS bgd. selection expression = annulus(30022.202515, 11536.818573, 1087.500000, 2175.000000, X, Y) && !ellipse(35210.281125, 15834.944742, 3856.848111, 1777.298394, 242.153910, X, Y) && !ellipse(32592.347870, 12252.578629, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(31897.338000, 12119.214000, 2042.376059, 1002.488029, 342.483000, X, Y) && !ellipse(32372.588440, 12883.064453, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(30916.673920, 11874.323242, 870.000000, 870.000000, 0.000000, X, Y)
[Thu Jan  5 18:24:49 2012] Writing fullrun_mos2_xmm0504810301_pi300-10000_pass1_cl_src162.gif
[Fri Jan  6 00:07:05 2012] Mean detx,y = (7801.53, -14914.70) 
[Fri Jan  6 00:07:07 2012] Setting backscal keywords in source and bgd. spectrum
[Fri Jan  6 00:07:33 2012] Binned source spectrum to 10 counts/bin
[Fri Jan  6 00:07:34 2012] Setting source spectrum file to fullrun_mos2_xmm0504810301_pi300-10000_pass1_cl_src162_src_b10.pi.gz
[Fri Jan  6 00:07:34 2012] Setting bgd. spectrum file to fullrun_mos2_xmm0504810301_pi300-10000_pass1_cl_src162_bgd.pi.gz
[Fri Jan  6 07:42:31 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Fri Jan  6 07:42:31 2012] rmf not generated due to insufficient counts
[Fri Jan  6 08:07:19 2012] Updating aperture counts using extracted products
[Fri Jan  6 08:07:20 2012] Error reading totcts from fullrun_mos2_xmm0504810301_pi300-10000_pass1_cl_src162_src_b10.pi.gz
[Fri Jan  6 08:07:26 2012] Calculating source flux in energy range 0.30-8.00
[Fri Jan  6 08:07:26 2012] Using photon index=1.80, rate=0.00158, arf fullrun_mos2_xmm0504810301_pi300-10000_pass1_cl_src162.arf
[Fri Jan  6 08:07:26 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Fri Jan  6 08:07:26 2012] Updating source flux to 5.5e-14
[Fri Jan  6 08:17:52 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting