[Wed Mar 28 00:31:49 2012] Detection parameters:
  Position = (305.6, 145.6) = 5 34 34.36 21 48 27.9
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 156.9 +/- 23.2
  Background counts = 186.7
  Rate = 0.007 +/- 0.001

[Wed Mar 28 00:31:53 2012] Off-axis axis estimate = 11.09'
[Wed Mar 28 10:34:54 2012] Using EEF radius (= 11.98 ")to estimate initial spatial extent for simple fitting
[Wed Mar 28 10:34:54 2012] Initial guess for spatial extent in simple fitting = 11.98"
[Wed Mar 28 10:34:54 2012] source mask rpix=2.8, npix_max = 42, mask sum = 29, frac = 0.685
[Wed Mar 28 10:34:54 2012] Giving source the simple spatial ID 162 for pass 0, mean size = 11.98"
[Thu Mar 29 00:25:26 2012] Vigneting correction estimate = 1.000000
[Thu Mar 29 00:25:26 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Thu Mar 29 00:25:26 2012] Assessing source extent using major
[Thu Mar 29 00:25:26 2012] Source does appear to be extended
[Thu Mar 29 00:25:26 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Thu Mar 29 11:04:59 2012] Using EEF radius (= 11.98 ")to estimate initial spatial extent for simple fitting
[Thu Mar 29 11:04:59 2012] Initial guess for spatial extent in simple fitting = 11.98"
[Thu Mar 29 11:04:59 2012] source mask rpix=2.8, npix_max = 42, mask sum = 29, frac = 0.685
[Thu Mar 29 11:04:59 2012] Giving source the simple spatial ID 158 for pass 1, mean size = 11.98"
[Fri Mar 30 21:01:44 2012] Vigneting correction estimate = 1.000000
[Fri Mar 30 21:01:44 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Fri Mar 30 21:01:44 2012] Assessing source extent using major
[Fri Mar 30 21:01:44 2012] Source does appear to be extended
[Fri Mar 30 21:01:44 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Sat Mar 31 03:06:36 2012] XMMSAS src. selection expression = ellipse(26542.237030, 12617.657104, 652.500000, 652.500000, 0.000000, X, Y)
[Sat Mar 31 03:06:36 2012] Writing source region out to fullrun_mos2_xmm0412591401_pi300-10000_pass1_cl_src99_src.reg
[Sat Mar 31 03:06:36 2012] Extracting stamp from image fullrun_mos2_xmm0412591401_pi300-10000_cl_sm2.00.img.gz, (268, 108) - (343, 183)
[Sat Mar 31 03:06:36 2012] XMMSAS bgd. selection expression = annulus(26542.237030, 12617.657104, 1087.500000, 2175.000000, X, Y) && !ellipse(26896.375458, 15526.219131, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26531.300964, 14653.822968, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26608.787994, 13352.837372, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(26842.783691, 14039.025711, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27142.491364, 12319.434921, 870.000000, 870.000000, 0.000000, X, Y)
[Sat Mar 31 03:06:36 2012] Writing fullrun_mos2_xmm0412591401_pi300-10000_pass1_cl_src99.gif
[Sat Mar 31 06:39:46 2012] Mean detx,y = (-215.94, -14863.59) 
[Sat Mar 31 06:39:49 2012] Setting backscal keywords in source and bgd. spectrum
[Sat Mar 31 06:40:14 2012] Binned source spectrum to 10 counts/bin
[Sat Mar 31 06:40:15 2012] Setting source spectrum file to fullrun_mos2_xmm0412591401_pi300-10000_pass1_cl_src99_src_b10.pi.gz
[Sat Mar 31 06:40:15 2012] Setting bgd. spectrum file to fullrun_mos2_xmm0412591401_pi300-10000_pass1_cl_src99_bgd.pi.gz
[Sat Mar 31 11:24:06 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Sat Mar 31 11:24:06 2012] rmf not generated due to insufficient counts
[Sat Mar 31 11:26:57 2012] Updating aperture counts using extracted products
[Sat Mar 31 11:26:57 2012] Error reading totcts from fullrun_mos2_xmm0412591401_pi300-10000_pass1_cl_src99_src_b10.pi.gz
[Sat Mar 31 11:27:05 2012] Calculating source flux in energy range 0.30-8.00
[Sat Mar 31 11:27:05 2012] Using photon index=1.80, rate=0.00718, arf fullrun_mos2_xmm0412591401_pi300-10000_pass1_cl_src99.arf
[Sat Mar 31 11:27:05 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Sat Mar 31 11:27:05 2012] Getting flux using calc_pl_flux failed
[Sat Mar 31 11:37:36 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting