[Mon Dec 19 02:11:54 2011] Detection parameters:
  Position = (301.7, 299.3) = 5 42 51.16 -36 0 4.2
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 28.0 +/- 8.4
  Background counts = 8.2
  Rate = 0.002 +/- 0.0007

[Mon Dec 19 02:11:54 2011] Off-axis axis estimate = 0.25'
[Mon Dec 19 03:05:49 2011] Using EEF radius (= 6.55 ")to estimate initial spatial extent for simple fitting
[Mon Dec 19 03:05:49 2011] Initial guess for spatial extent in simple fitting = 6.55"
[Mon Dec 19 03:05:49 2011] source mask rpix=1.5, npix_max = 16, mask sum = 16, frac = 0.994
[Mon Dec 19 03:05:49 2011] Giving source the simple spatial ID 26 for pass 0, mean size = 6.55"
[Mon Dec 19 04:10:22 2011] fullrun_mos1_xmm0656202001_pi300-10000_cl_pass0_src26.ximg exists
[Mon Dec 19 04:10:22 2011] fullrun_mos1_xmm0656202001_pi300-10000_cl_pass0_src26_1.ximg exists
[Mon Dec 19 04:10:22 2011] Fit fullrun_mos1_xmm0656202001_pi300-10000_cl_pass0_src26 appears to have run properly
[Mon Dec 19 04:10:23 2011] fullrun_mos1_xmm0656202001_pi300-10000_cl_pass0_tfrozen_src26.ximg exists
[Mon Dec 19 04:10:23 2011] fullrun_mos1_xmm0656202001_pi300-10000_cl_pass0_tfrozen_src26_1.ximg exists
[Mon Dec 19 04:10:23 2011] Fit fullrun_mos1_xmm0656202001_pi300-10000_cl_pass0_tfrozen_src26 appears to have run properly
[Mon Dec 19 04:57:24 2011] Source 22 is offset by 5.775012 and -0.269641 pixels which is larger than
2 X fitted extent = 3.813991 x 3.813991, not incorporating fit results
[Mon Dec 19 04:57:24 2011] Vigneting correction estimate = 1.000000
[Mon Dec 19 04:57:24 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Mon Dec 19 04:57:24 2011] Assessing source extent using major
[Mon Dec 19 04:57:24 2011] Source does appear to be extended
[Mon Dec 19 04:57:24 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Mon Dec 19 05:40:21 2011] Using EEF radius (= 6.55 ")to estimate initial spatial extent for simple fitting
[Mon Dec 19 05:40:21 2011] Initial guess for spatial extent in simple fitting = 6.55"
[Mon Dec 19 05:40:21 2011] source mask rpix=1.5, npix_max = 16, mask sum = 16, frac = 0.994
[Mon Dec 19 05:40:21 2011] Giving source the simple spatial ID 23 for pass 1, mean size = 6.55"
[Mon Dec 19 06:34:43 2011] fullrun_mos1_xmm0656202001_pi300-10000_cl_pass1_src23.ximg exists
[Mon Dec 19 06:34:43 2011] fullrun_mos1_xmm0656202001_pi300-10000_cl_pass1_src23_1.ximg exists
[Mon Dec 19 06:34:43 2011] Fit fullrun_mos1_xmm0656202001_pi300-10000_cl_pass1_src23 appears to have run properly
[Mon Dec 19 06:34:43 2011] fullrun_mos1_xmm0656202001_pi300-10000_cl_pass1_tfrozen_src23.ximg exists
[Mon Dec 19 06:34:43 2011] fullrun_mos1_xmm0656202001_pi300-10000_cl_pass1_tfrozen_src23_1.ximg exists
[Mon Dec 19 06:34:43 2011] Fit fullrun_mos1_xmm0656202001_pi300-10000_cl_pass1_tfrozen_src23 appears to have run properly
[Mon Dec 19 07:21:11 2011] Warning: source 11 in spatial fitting list does not appear to have a counterpart in memory, closest src. was src. 22 at 148.904534 pixels away
[Mon Dec 19 07:21:11 2011] Warning: source 14 in spatial fitting list does not appear to have a counterpart in memory, closest src. was src. 22 at 157.191436 pixels away
[Mon Dec 19 07:21:11 2011] Source 22 is offset by 5.775012 and -1.704586 pixels which is larger than
2 X fitted extent = 4.906759 x 4.906759, not incorporating fit results
[Mon Dec 19 07:21:11 2011] Vigneting correction estimate = 1.000000
[Mon Dec 19 07:21:11 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Mon Dec 19 07:21:11 2011] Assessing source extent using major
[Mon Dec 19 07:21:11 2011] Source does appear to be extended
[Mon Dec 19 07:21:11 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Mon Dec 19 07:52:25 2011] XMMSAS src. selection expression = ellipse(26203.734070, 25987.864258, 652.500000, 652.500000, 0.000000, X, Y)
[Mon Dec 19 07:52:25 2011] Writing source region out to fullrun_mos1_xmm0656202001_pi300-10000_pass1_cl_src22_src.reg
[Mon Dec 19 07:52:25 2011] Extracting stamp from image fullrun_mos1_xmm0656202001_pi300-10000_cl_sm2.00.img.gz, (264, 262) - (339, 337)
[Mon Dec 19 07:52:25 2011] XMMSAS bgd. selection expression = annulus(26203.734070, 25987.864258, 1087.500000, 2175.000000, X, Y) && !ellipse(24906.499720, 26144.334600, 1095.592032, 1095.592032, 0.000000, X, Y) && !ellipse(24560.856000, 25958.920000, 1717.808049, 1717.808049, 0.000000, X, Y) && !ellipse(25046.494415, 27171.309052, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(24527.085724, 27093.583069, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(23166.942000, 27140.726000, 1160.752033, 1160.752033, 0.000000, X, Y) && !ellipse(23784.364000, 25612.546000, 1207.728035, 1207.728035, 0.000000, X, Y) && !ellipse(25816.381226, 25368.525574, 870.000000, 870.000000, 0.000000, X, Y)
[Mon Dec 19 07:52:25 2011] Writing fullrun_mos1_xmm0656202001_pi300-10000_pass1_cl_src22.gif
[Mon Dec 19 07:56:27 2011] Mean detx,y = (-1558.69, -1449.59) 
[Mon Dec 19 07:56:28 2011] Setting backscal keywords in source and bgd. spectrum
[Mon Dec 19 07:56:35 2011] Binned source spectrum to 10 counts/bin
[Mon Dec 19 07:56:35 2011] Setting source spectrum file to fullrun_mos1_xmm0656202001_pi300-10000_pass1_cl_src22_src_b10.pi.gz
[Mon Dec 19 07:56:35 2011] Setting bgd. spectrum file to fullrun_mos1_xmm0656202001_pi300-10000_pass1_cl_src22_bgd.pi.gz
[Mon Dec 19 08:16:03 2011] Not generating rmf since there are only 28 counts
[Mon Dec 19 08:16:03 2011] rmf not generated due to insufficient counts
[Mon Dec 19 08:34:02 2011] Updating aperture counts using extracted products
[Mon Dec 19 08:34:02 2011] Error reading totcts from fullrun_mos1_xmm0656202001_pi300-10000_pass1_cl_src22_src_b10.pi.gz
[Mon Dec 19 08:34:02 2011] Calculating source flux in energy range 0.30-8.00
[Mon Dec 19 08:34:02 2011] Using photon index=1.80, rate=0.00219, arf fullrun_mos1_xmm0656202001_pi300-10000_pass1_cl_src22.arf
[Mon Dec 19 08:34:02 2011] Assuming count rate is from the 0.30-10.00 bandpass
[Mon Dec 19 08:34:02 2011] Updating source flux to 2.2e-14
[Mon Dec 19 08:34:03 2011] Simple spatial fitting not done (or not done successfully), skipping spectral fitting