[Thu Sep 29 19:16:53 2011] Detection parameters:
  Position = (286.9, 297.6) = 3 59 26.83 -67 37 51.4
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 88.4 +/- 17.8
  Background counts = 93.0
  Rate = 0.003 +/- 0.0005

[Thu Sep 29 19:16:53 2011] Off-axis axis estimate = 0.84'
[Thu Sep 29 19:18:44 2011] Using EEF radius (= 6.85 ")to estimate initial spatial extent for simple fitting
[Thu Sep 29 19:18:44 2011] Initial guess for spatial extent in simple fitting = 6.85"
[Thu Sep 29 19:18:44 2011] source mask rpix=1.6, npix_max = 17, mask sum = 20, frac = 1.163
[Thu Sep 29 19:18:44 2011] Giving source the simple spatial ID 19 for pass 0, mean size = 6.85"
[Thu Sep 29 19:40:08 2011] fullrun_pn_xmm0110980401_pi300-10000_cl_pass0_src19.ximg exists
[Thu Sep 29 19:40:08 2011] fullrun_pn_xmm0110980401_pi300-10000_cl_pass0_src19_1.ximg exists
[Thu Sep 29 19:40:08 2011] Fit fullrun_pn_xmm0110980401_pi300-10000_cl_pass0_src19 appears to have run properly
[Thu Sep 29 19:40:08 2011] fullrun_pn_xmm0110980401_pi300-10000_cl_pass0_tfrozen_src19.ximg exists
[Thu Sep 29 19:40:08 2011] fullrun_pn_xmm0110980401_pi300-10000_cl_pass0_tfrozen_src19_1.ximg exists
[Thu Sep 29 19:40:08 2011] Fit fullrun_pn_xmm0110980401_pi300-10000_cl_pass0_tfrozen_src19 appears to have run properly
[Thu Sep 29 20:34:17 2011] Source 20 is offset by -6.353638 and 3.296991 pixels which is larger than
2 X fitted extent = 6.295586 x 6.295586, not incorporating fit results
[Thu Sep 29 20:34:17 2011] Vigneting correction estimate = 1.000000
[Thu Sep 29 20:34:17 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Thu Sep 29 20:34:17 2011] Assessing source extent using major
[Thu Sep 29 20:34:17 2011] Source does appear to be extended
[Thu Sep 29 20:34:17 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Thu Sep 29 20:34:29 2011] Using EEF radius (= 6.85 ")to estimate initial spatial extent for simple fitting
[Thu Sep 29 20:34:29 2011] Initial guess for spatial extent in simple fitting = 6.85"
[Thu Sep 29 20:34:29 2011] source mask rpix=1.6, npix_max = 17, mask sum = 20, frac = 1.163
[Thu Sep 29 20:34:29 2011] Giving source the simple spatial ID 19 for pass 1, mean size = 6.85"
[Thu Sep 29 21:00:16 2011] fullrun_pn_xmm0110980401_pi300-10000_cl_pass1_src19.ximg exists
[Thu Sep 29 21:00:16 2011] Warning: poor agreement between model and actual number of counts may be indicative of a poor fit in csv/fullrun_pn_xmm0110980401_pi300-10000_cl_pass1_src19.csv
[Thu Sep 29 21:00:16 2011] fullrun_pn_xmm0110980401_pi300-10000_cl_pass1_src19_1.ximg exists
[Thu Sep 29 21:00:16 2011] Warning: poor agreement between model and actual number of counts may be indicative of a poor fit in csv/fullrun_pn_xmm0110980401_pi300-10000_cl_pass1_src19.csv
[Thu Sep 29 21:00:16 2011] It looks like the fit did not converge
You should probably delete fullrun_pn_xmm0110980401_pi300-10000_cl_pass1_src19_1.ximg
Either tweak this fit manually starting from fullrun_pn_xmm0110980401_pi300-10000_cl_pass1_src19.ximg or adjust the simplespatial fit parameters in $XASSIST/data/missions/*/*/spatial.dat and re-run simplespatial fitting after setting file recreation parameter to yes
[Thu Sep 29 21:00:16 2011] fullrun_pn_xmm0110980401_pi300-10000_cl_pass1_tfrozen_src19.ximg exists
[Thu Sep 29 21:00:16 2011] fullrun_pn_xmm0110980401_pi300-10000_cl_pass1_tfrozen_src19_1.ximg exists
[Thu Sep 29 21:00:16 2011] Fit fullrun_pn_xmm0110980401_pi300-10000_cl_pass1_tfrozen_src19 appears to have run properly
[Thu Sep 29 21:49:32 2011] Source 20 is offset by 6.237488 and 0.221573 pixels which is larger than
2 X fitted extent = 3.097710 x 3.097710, not incorporating fit results
[Thu Sep 29 21:49:32 2011] Vigneting correction estimate = 1.000000
[Thu Sep 29 21:49:32 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Thu Sep 29 21:49:32 2011] Assessing source extent using major
[Thu Sep 29 21:49:32 2011] Source does appear to be extended
[Thu Sep 29 21:49:32 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Thu Sep 29 21:49:44 2011] XMMSAS src. selection expression = ellipse(24915.447479, 25840.332245, 652.500000, 652.500000, 0.000000, X, Y)
[Thu Sep 29 21:49:44 2011] Writing source region out to fullrun_pn_xmm0110980401_pi300-10000_pass1_cl_src20_src.reg
[Thu Sep 29 21:49:44 2011] Extracting stamp from image fullrun_pn_xmm0110980401_pi300-10000_cl_sm2.00.img.gz, (249, 260) - (324, 335)
[Thu Sep 29 21:49:44 2011] XMMSAS bgd. selection expression = annulus(24915.447479, 25840.332245, 1087.500000, 2175.000000, X, Y) && !ellipse(23386.690200, 25319.736200, 568.515216, 465.363213, 0.356542, X, Y) && !ellipse(23776.858180, 26127.820100, 421.500812, 421.500812, 0.000000, X, Y) && !ellipse(24983.965400, 24657.174000, 395.582411, 395.582411, 0.000000, X, Y)
[Thu Sep 29 21:49:44 2011] Writing fullrun_pn_xmm0110980401_pi300-10000_pass1_cl_src20.gif
[Thu Sep 29 21:57:04 2011] Mean detx,y = (-319.67, 596.21) 
[Thu Sep 29 21:57:07 2011] Setting backscal keywords in source and bgd. spectrum
[Thu Sep 29 21:57:24 2011] Binned source spectrum to 10 counts/bin
[Thu Sep 29 21:57:25 2011] Setting source spectrum file to fullrun_pn_xmm0110980401_pi300-10000_pass1_cl_src20_src_b10.pi.gz
[Thu Sep 29 21:57:25 2011] Setting bgd. spectrum file to fullrun_pn_xmm0110980401_pi300-10000_pass1_cl_src20_bgd.pi.gz
[Thu Sep 29 22:19:37 2011] Not generating rmf since there are only 88 counts
[Thu Sep 29 22:19:37 2011] rmf not generated due to insufficient counts
[Fri Sep 30 00:04:05 2011] Updating aperture counts using extracted products
[Fri Sep 30 00:04:05 2011] Error reading totcts from fullrun_pn_xmm0110980401_pi300-10000_pass1_cl_src20_src_b10.pi.gz
[Fri Sep 30 00:04:05 2011] Calculating source flux in energy range 0.30-8.00
[Fri Sep 30 00:04:05 2011] Using photon index=1.80, rate=0.00264, arf fullrun_pn_xmm0110980401_pi300-10000_pass1_cl_src20.arf
[Fri Sep 30 00:04:05 2011] Assuming count rate is from the 0.30-10.00 bandpass
[Fri Sep 30 00:04:05 2011] Updating source flux to 6.4e-15
[Fri Sep 30 00:05:28 2011] Simple spatial fitting not done (or not done successfully), skipping spectral fitting