[Tue Jul 10 07:32:39 2012] Detection parameters:
  Position = (259.3, 274.2) = 18 56 16.44 1 14 4.4
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 65.7 +/- 14.6
  Background counts = 49.0
  Rate = 0.007 +/- 0.002

[Tue Jul 10 07:32:39 2012] Off-axis axis estimate = 3.34'
[Tue Jul 10 11:29:19 2012] Using EEF radius (= 8.10 ")to estimate initial spatial extent for simple fitting
[Tue Jul 10 11:29:19 2012] Initial guess for spatial extent in simple fitting = 8.10"
[Tue Jul 10 11:29:19 2012] source mask rpix=1.9, npix_max = 22, mask sum = 25, frac = 1.121
[Tue Jul 10 11:29:19 2012] Giving source the simple spatial ID 19 for pass 0, mean size = 8.10"
[Tue Jul 10 12:33:33 2012] fullrun_mos2_xmm0083270301_pi300-10000_cl_pass0_src19.ximg exists
[Tue Jul 10 12:33:33 2012] fullrun_mos2_xmm0083270301_pi300-10000_cl_pass0_src19_1.ximg exists
[Tue Jul 10 12:33:33 2012] Fit fullrun_mos2_xmm0083270301_pi300-10000_cl_pass0_src19 appears to have run properly
[Tue Jul 10 12:33:34 2012] fullrun_mos2_xmm0083270301_pi300-10000_cl_pass0_tfrozen_src19.ximg exists
[Tue Jul 10 12:33:34 2012] fullrun_mos2_xmm0083270301_pi300-10000_cl_pass0_tfrozen_src19_1.ximg exists
[Tue Jul 10 12:33:34 2012] Fit fullrun_mos2_xmm0083270301_pi300-10000_cl_pass0_tfrozen_src19 appears to have run properly
[Tue Jul 10 12:33:55 2012] Source 29 is offset by -3.036565 and -7.421347 pixels which is larger than
2 X fitted extent = 0.930717 x 0.930717, not incorporating fit results
[Tue Jul 10 12:33:55 2012] Source 29 is offset by -0.006519 and -1.812864 pixels which is larger than
2 X fitted extent = 0.943287 x 0.943287, not incorporating fit results
[Tue Jul 10 12:33:55 2012] Vigneting correction estimate = 1.000000
[Tue Jul 10 12:33:55 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Tue Jul 10 12:33:55 2012] Assessing source extent using major
[Tue Jul 10 12:33:55 2012] Source does appear to be extended
[Tue Jul 10 12:33:55 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Tue Jul 10 16:31:48 2012] Using EEF radius (= 8.10 ")to estimate initial spatial extent for simple fitting
[Tue Jul 10 16:31:48 2012] Initial guess for spatial extent in simple fitting = 8.10"
[Tue Jul 10 16:31:48 2012] source mask rpix=1.9, npix_max = 22, mask sum = 25, frac = 1.121
[Tue Jul 10 16:31:48 2012] Giving source the simple spatial ID 16 for pass 1, mean size = 8.10"
[Tue Jul 10 17:08:10 2012] fullrun_mos2_xmm0083270301_pi300-10000_cl_pass1_src16.ximg exists
[Tue Jul 10 17:08:10 2012] fullrun_mos2_xmm0083270301_pi300-10000_cl_pass1_src16_1.ximg exists
[Tue Jul 10 17:08:10 2012] Fit fullrun_mos2_xmm0083270301_pi300-10000_cl_pass1_src16 appears to have run properly
[Tue Jul 10 17:08:11 2012] fullrun_mos2_xmm0083270301_pi300-10000_cl_pass1_tfrozen_src16.ximg exists
[Tue Jul 10 17:08:11 2012] fullrun_mos2_xmm0083270301_pi300-10000_cl_pass1_tfrozen_src16_1.ximg exists
[Tue Jul 10 17:08:11 2012] Fit fullrun_mos2_xmm0083270301_pi300-10000_cl_pass1_tfrozen_src16 appears to have run properly
[Tue Jul 10 17:08:32 2012] Warning, spatial fit 16 centroid is now closest to src. 28
[Tue Jul 10 17:08:32 2012] Source 29 is offset by -0.235508 and -1.786473 pixels which is larger than
2 X fitted extent = 0.943287 x 0.943287, not incorporating fit results
[Tue Jul 10 17:08:32 2012] Vigneting correction estimate = 1.000000
[Tue Jul 10 17:08:32 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Tue Jul 10 17:08:32 2012] Assessing source extent using major
[Tue Jul 10 17:08:32 2012] Source does appear to be extended
[Tue Jul 10 17:08:32 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Tue Jul 10 19:23:25 2012] XMMSAS src. selection expression = ellipse(22511.538818, 23805.732849, 652.500000, 652.500000, 0.000000, X, Y)
[Tue Jul 10 19:23:25 2012] Writing source region out to fullrun_mos2_xmm0083270301_pi300-10000_pass1_cl_src29_src.reg
[Tue Jul 10 19:23:25 2012] Extracting stamp from image fullrun_mos2_xmm0083270301_pi300-10000_cl_sm2.00.img.gz, (222, 237) - (297, 312)
[Tue Jul 10 19:23:25 2012] XMMSAS bgd. selection expression = annulus(22511.538818, 23805.732849, 1087.500000, 2175.000000, X, Y) && !ellipse(20287.140671, 24596.188171, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(21381.706740, 25885.226800, 1445.864042, 1445.864042, 0.000000, X, Y) && !ellipse(19314.048400, 25631.264000, 1460.408042, 1460.408042, 0.000000, X, Y) && !ellipse(20622.348740, 26048.890106, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(20984.111084, 25019.049377, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(20168.042694, 25706.585144, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(19992.610306, 26256.516052, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(21727.448929, 25460.076294, 870.000000, 870.000000, 0.000000, X, Y)
[Tue Jul 10 19:23:25 2012] Writing fullrun_mos2_xmm0083270301_pi300-10000_pass1_cl_src29.gif
[Tue Jul 10 19:28:26 2012] Mean detx,y = (4478.18, -3942.04) 
[Tue Jul 10 19:28:27 2012] Setting backscal keywords in source and bgd. spectrum
[Tue Jul 10 19:28:34 2012] Binned source spectrum to 10 counts/bin
[Tue Jul 10 19:28:35 2012] Setting source spectrum file to fullrun_mos2_xmm0083270301_pi300-10000_pass1_cl_src29_src_b10.pi.gz
[Tue Jul 10 19:28:35 2012] Setting bgd. spectrum file to fullrun_mos2_xmm0083270301_pi300-10000_pass1_cl_src29_bgd.pi.gz
[Tue Jul 10 19:45:35 2012] Not generating rmf since there are only 65 counts
[Tue Jul 10 19:45:35 2012] rmf not generated due to insufficient counts
[Tue Jul 10 19:46:15 2012] Updating aperture counts using extracted products
[Tue Jul 10 19:46:15 2012] Error reading totcts from fullrun_mos2_xmm0083270301_pi300-10000_pass1_cl_src29_src_b10.pi.gz
[Tue Jul 10 19:46:16 2012] Calculating source flux in energy range 0.30-8.00
[Tue Jul 10 19:46:16 2012] Using photon index=1.80, rate=0.00722, arf fullrun_mos2_xmm0083270301_pi300-10000_pass1_cl_src29.arf
[Tue Jul 10 19:46:16 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Tue Jul 10 19:46:16 2012] Updating source flux to 9.3e-14
[Tue Jul 10 19:46:40 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting