[Tue Mar 13 13:33:06 2012] Detection parameters:
  Position = (331.4, 260.8) = 1 37 28.34 -12 59 21.2
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 107.3 +/- 21.3
  Background counts = 145.4
  Rate = 0.002 +/- 0.0004

[Tue Mar 13 13:33:06 2012] Off-axis axis estimate = 3.63'
[Tue Mar 13 19:19:43 2012] Using EEF radius (= 8.24 ")to estimate initial spatial extent for simple fitting
[Tue Mar 13 19:19:43 2012] Initial guess for spatial extent in simple fitting = 8.24"
[Tue Mar 13 19:19:43 2012] source mask rpix=1.9, npix_max = 22, mask sum = 25, frac = 1.090
[Tue Mar 13 19:19:43 2012] Giving source the simple spatial ID 34 for pass 0, mean size = 8.24"
[Tue Mar 13 21:54:21 2012] fullrun_mos2_xmm0502020101_pi300-10000_cl_pass0_src34.ximg exists
[Tue Mar 13 21:54:21 2012] fullrun_mos2_xmm0502020101_pi300-10000_cl_pass0_src34_1.ximg exists
[Tue Mar 13 21:54:21 2012] Fit fullrun_mos2_xmm0502020101_pi300-10000_cl_pass0_src34 appears to have run properly
[Tue Mar 13 21:54:22 2012] fullrun_mos2_xmm0502020101_pi300-10000_cl_pass0_tfrozen_src34.ximg exists
[Tue Mar 13 21:54:22 2012] fullrun_mos2_xmm0502020101_pi300-10000_cl_pass0_tfrozen_src34_1.ximg exists
[Tue Mar 13 21:54:22 2012] Fit fullrun_mos2_xmm0502020101_pi300-10000_cl_pass0_tfrozen_src34 appears to have run properly
[Tue Mar 13 21:55:07 2012] Source 35 is offset by -0.654018 and -1.302239 pixels which is larger than
2 X fitted extent = 0.947274 x 0.947274, not incorporating fit results
[Tue Mar 13 21:55:07 2012] Source 35 is offset by -0.657723 and -1.278289 pixels which is larger than
2 X fitted extent = 0.973439 x 0.973439, not incorporating fit results
[Tue Mar 13 21:55:07 2012] Vigneting correction estimate = 1.000000
[Tue Mar 13 21:55:07 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Tue Mar 13 21:55:07 2012] Assessing source extent using major
[Tue Mar 13 21:55:07 2012] Source does appear to be extended
[Tue Mar 13 21:55:07 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Tue Mar 13 21:55:07 2012] Source is confused with source 39
[Wed Mar 14 03:18:46 2012] Using EEF radius (= 8.24 ")to estimate initial spatial extent for simple fitting
[Wed Mar 14 03:18:46 2012] Initial guess for spatial extent in simple fitting = 8.24"
[Wed Mar 14 03:18:46 2012] source mask rpix=1.9, npix_max = 22, mask sum = 25, frac = 1.090
[Wed Mar 14 03:18:46 2012] Giving source the simple spatial ID 32 for pass 1, mean size = 8.24"
[Wed Mar 14 05:41:17 2012] fullrun_mos2_xmm0502020101_pi300-10000_cl_pass1_src32.ximg exists
[Wed Mar 14 05:41:17 2012] fullrun_mos2_xmm0502020101_pi300-10000_cl_pass1_src32_1.ximg exists
[Wed Mar 14 05:41:17 2012] Fit fullrun_mos2_xmm0502020101_pi300-10000_cl_pass1_src32 appears to have run properly
[Wed Mar 14 05:41:18 2012] fullrun_mos2_xmm0502020101_pi300-10000_cl_pass1_tfrozen_src32.ximg exists
[Wed Mar 14 05:41:18 2012] fullrun_mos2_xmm0502020101_pi300-10000_cl_pass1_tfrozen_src32_1.ximg exists
[Wed Mar 14 05:41:18 2012] Fit fullrun_mos2_xmm0502020101_pi300-10000_cl_pass1_tfrozen_src32 appears to have run properly
[Wed Mar 14 05:41:50 2012] Warning, spatial fit 32 centroid is now closest to src. 39
[Wed Mar 14 05:41:50 2012] Vigneting correction estimate = 1.000000
[Wed Mar 14 05:41:50 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Wed Mar 14 05:41:50 2012] Assessing source extent using major
[Wed Mar 14 05:41:50 2012] Source does appear to be extended
[Wed Mar 14 05:41:50 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Wed Mar 14 08:53:10 2012] XMMSAS src. selection expression = ellipse(28784.534058, 22645.078827, 652.500000, 652.500000, 0.000000, X, Y)
[Wed Mar 14 08:53:10 2012] Writing source region out to fullrun_mos2_xmm0502020101_pi300-10000_pass1_cl_src35_src.reg
[Wed Mar 14 08:53:10 2012] Extracting stamp from image fullrun_mos2_xmm0502020101_pi300-10000_cl_sm2.00.img.gz, (294, 223) - (369, 298)
[Wed Mar 14 08:53:10 2012] XMMSAS bgd. selection expression = annulus(28784.534058, 22645.078827, 1087.500000, 2175.000000, X, Y) && !ellipse(26978.318000, 22370.485800, 2718.928078, 2718.928078, 0.000000, X, Y) && !ellipse(26859.392200, 21405.672000, 1174.296034, 1174.296034, 0.000000, X, Y) && !ellipse(27629.769560, 22409.118440, 1294.320037, 1294.320037, 0.000000, X, Y) && !ellipse(28081.634000, 22120.934000, 1359.464039, 1359.464039, 0.000000, X, Y) && !ellipse(28011.318000, 23828.586000, 1221.840035, 1221.840035, 0.000000, X, Y) && !ellipse(25951.092102, 22983.324249, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(28573.987579, 23316.203857, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(27727.179260, 21040.815872, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(29376.146271, 22450.908569, 870.000000, 870.000000, 0.000000, X, Y)
[Wed Mar 14 08:53:10 2012] Writing fullrun_mos2_xmm0502020101_pi300-10000_pass1_cl_src35.gif
[Wed Mar 14 09:19:53 2012] Mean detx,y = (5308.45, -266.95) 
[Wed Mar 14 09:19:55 2012] Setting backscal keywords in source and bgd. spectrum
[Wed Mar 14 09:20:22 2012] Binned source spectrum to 10 counts/bin
[Wed Mar 14 09:20:22 2012] Setting source spectrum file to fullrun_mos2_xmm0502020101_pi300-10000_pass1_cl_src35_src_b10.pi.gz
[Wed Mar 14 09:20:22 2012] Setting bgd. spectrum file to fullrun_mos2_xmm0502020101_pi300-10000_pass1_cl_src35_bgd.pi.gz
[Wed Mar 14 18:01:22 2012] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Wed Mar 14 18:01:22 2012] rmf not generated due to insufficient counts
[Wed Mar 14 18:05:20 2012] Updating aperture counts using extracted products
[Wed Mar 14 18:05:20 2012] Error reading totcts from fullrun_mos2_xmm0502020101_pi300-10000_pass1_cl_src35_src_b10.pi.gz
[Wed Mar 14 18:05:22 2012] Calculating source flux in energy range 0.30-8.00
[Wed Mar 14 18:05:22 2012] Using photon index=1.80, rate=0.00193, arf fullrun_mos2_xmm0502020101_pi300-10000_pass1_cl_src35.arf
[Wed Mar 14 18:05:22 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Wed Mar 14 18:05:22 2012] Updating source flux to 2.5e-14
[Wed Mar 14 18:10:19 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting