[Mon Mar 26 13:06:28 2012] Detection parameters:
  Position = (261.6, 182.3) = 5 40 30.82 -69 29 49.6
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 47.4 +/- 11.0
  Background counts = 31.9
  Rate = 0.001 +/- 0.0003

[Mon Mar 26 13:06:32 2012] Off-axis axis estimate = 8.83'
[Mon Mar 26 14:54:08 2012] Using EEF radius (= 10.85 ")to estimate initial spatial extent for simple fitting
[Mon Mar 26 14:54:08 2012] Initial guess for spatial extent in simple fitting = 10.85"
[Mon Mar 26 14:54:08 2012] source mask rpix=2.5, npix_max = 35, mask sum = 36, frac = 1.004
[Mon Mar 26 14:54:08 2012] Giving source the simple spatial ID 62 for pass 0, mean size = 10.85"
[Mon Mar 26 23:28:02 2012] fullrun_mos1_xmm0125120201_pi300-10000_cl_pass0_src62.ximg exists
[Mon Mar 26 23:28:02 2012] fullrun_mos1_xmm0125120201_pi300-10000_cl_pass0_src62_1.ximg exists
[Mon Mar 26 23:28:02 2012] Fit fullrun_mos1_xmm0125120201_pi300-10000_cl_pass0_src62 appears to have run properly
[Mon Mar 26 23:28:05 2012] fullrun_mos1_xmm0125120201_pi300-10000_cl_pass0_tfrozen_src62.ximg exists
[Mon Mar 26 23:28:05 2012] fullrun_mos1_xmm0125120201_pi300-10000_cl_pass0_tfrozen_src62_1.ximg exists
[Mon Mar 26 23:28:05 2012] Fit fullrun_mos1_xmm0125120201_pi300-10000_cl_pass0_tfrozen_src62 appears to have run properly
[Mon Mar 26 23:51:14 2012] Source 35 is offset by -4.621840 and -3.996642 pixels which is larger than
2 X fitted extent = 1.282736 x 1.282736, not incorporating fit results
[Mon Mar 26 23:51:14 2012] Source 35 is offset by 1.606533 and 2.116071 pixels which is larger than
2 X fitted extent = 9.973334 x 1.246667, not incorporating fit results
[Mon Mar 26 23:51:14 2012] Vigneting correction estimate = 1.000000
[Mon Mar 26 23:51:14 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Mon Mar 26 23:51:14 2012] Assessing source extent using major
[Mon Mar 26 23:51:14 2012] Source does appear to be extended
[Mon Mar 26 23:51:14 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Tue Mar 27 00:16:40 2012] Using EEF radius (= 10.85 ")to estimate initial spatial extent for simple fitting
[Tue Mar 27 00:16:40 2012] Initial guess for spatial extent in simple fitting = 10.85"
[Tue Mar 27 00:16:40 2012] source mask rpix=2.5, npix_max = 35, mask sum = 36, frac = 1.004
[Tue Mar 27 00:16:40 2012] Giving source the simple spatial ID 57 for pass 1, mean size = 10.85"
[Tue Mar 27 07:27:19 2012] fullrun_mos1_xmm0125120201_pi300-10000_cl_pass1_src57.ximg exists
[Tue Mar 27 07:27:19 2012] fullrun_mos1_xmm0125120201_pi300-10000_cl_pass1_src57_1.ximg exists
[Tue Mar 27 07:27:19 2012] Fit fullrun_mos1_xmm0125120201_pi300-10000_cl_pass1_src57 appears to have run properly
[Tue Mar 27 07:27:21 2012] fullrun_mos1_xmm0125120201_pi300-10000_cl_pass1_tfrozen_src57.ximg exists
[Tue Mar 27 07:27:21 2012] fullrun_mos1_xmm0125120201_pi300-10000_cl_pass1_tfrozen_src57_1.ximg exists
[Tue Mar 27 07:27:21 2012] Fit fullrun_mos1_xmm0125120201_pi300-10000_cl_pass1_tfrozen_src57 appears to have run properly
[Tue Mar 27 07:37:31 2012] Warning: source 57 in spatial fitting list does not appear to have a counterpart in memory, closest src. was src. 35 at 11.820077 pixels away
[Tue Mar 27 07:37:32 2012] Vigneting correction estimate = 1.000000
[Tue Mar 27 07:37:32 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Tue Mar 27 07:37:32 2012] Assessing source extent using major
[Tue Mar 27 07:37:32 2012] Source does appear to be extended
[Tue Mar 27 07:37:32 2012] Computing asymmetry using major and minor axis, asym = 1.00
[Tue Mar 27 08:55:23 2012] XMMSAS src. selection expression = ellipse(22714.183929, 15808.576187, 652.500000, 652.500000, 0.000000, X, Y)
[Tue Mar 27 08:55:23 2012] Writing source region out to fullrun_mos1_xmm0125120201_pi300-10000_pass1_cl_src35_src.reg
[Tue Mar 27 08:55:23 2012] Extracting stamp from image fullrun_mos1_xmm0125120201_pi300-10000_cl_sm2.00.img.gz, (224, 145) - (299, 220)
[Tue Mar 27 08:55:23 2012] XMMSAS bgd. selection expression = annulus(22714.183929, 15808.576187, 1087.500000, 2175.000000, X, Y) && !ellipse(24954.012000, 13696.130000, 1717.768049, 1717.768049, 0.000000, X, Y) && !ellipse(25614.009583, 15541.334213, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(22962.420000, 13681.152000, 1328.984038, 1328.984038, 0.000000, X, Y) && !ellipse(25688.838000, 14239.932000, 3246.752093, 3246.752093, 0.000000, X, Y) && !ellipse(25176.086000, 15435.933200, 1720.472050, 1720.472050, 0.000000, X, Y) && !ellipse(23268.084106, 14140.569962, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(24126.260000, 12920.052000, 1828.568053, 1828.568053, 0.000000, X, Y) && !ellipse(22721.878000, 13225.916000, 980.216028, 980.216028, 0.000000, X, Y) && !ellipse(22138.305800, 15062.786200, 517.437615, 517.437615, 0.000000, X, Y)
[Tue Mar 27 08:55:23 2012] Writing fullrun_mos1_xmm0125120201_pi300-10000_pass1_cl_src35.gif
[Tue Mar 27 09:39:28 2012] Mean detx,y = (-1763.05, -11917.47) 
[Tue Mar 27 09:39:31 2012] Setting backscal keywords in source and bgd. spectrum
[Tue Mar 27 09:39:55 2012] Binned source spectrum to 10 counts/bin
[Tue Mar 27 09:39:55 2012] Setting source spectrum file to fullrun_mos1_xmm0125120201_pi300-10000_pass1_cl_src35_src_b10.pi.gz
[Tue Mar 27 09:39:55 2012] Setting bgd. spectrum file to fullrun_mos1_xmm0125120201_pi300-10000_pass1_cl_src35_bgd.pi.gz
[Tue Mar 27 12:01:55 2012] Not generating rmf since there are only 47 counts
[Tue Mar 27 12:01:55 2012] rmf not generated due to insufficient counts
[Tue Mar 27 12:20:27 2012] Updating aperture counts using extracted products
[Tue Mar 27 12:20:28 2012] Error reading totcts from fullrun_mos1_xmm0125120201_pi300-10000_pass1_cl_src35_src_b10.pi.gz
[Tue Mar 27 12:20:31 2012] Calculating source flux in energy range 0.30-8.00
[Tue Mar 27 12:20:31 2012] Using photon index=1.80, rate=0.00118, arf fullrun_mos1_xmm0125120201_pi300-10000_pass1_cl_src35.arf
[Tue Mar 27 12:20:31 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Tue Mar 27 12:20:31 2012] Updating source flux to 2.8e-14
[Tue Mar 27 12:20:33 2012] Simple spatial fitting not done (or not done successfully), skipping spectral fitting