[Fri Dec 23 19:32:36 2011] Detection parameters:
  Position = (367.0, 194.1) = 1 56 33.78 -17 8 46.2
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 209.4 +/- 22.7
  Background counts = 91.9
  Rate = 0.003 +/- 0.0003

[Fri Dec 23 19:32:36 2011] Off-axis axis estimate = 9.05'
[Fri Dec 23 19:39:37 2011] Using EEF radius (= 10.95 ")to estimate initial spatial extent for simple fitting
[Fri Dec 23 19:39:37 2011] Initial guess for spatial extent in simple fitting = 10.95"
[Fri Dec 23 19:39:37 2011] source mask rpix=2.5, npix_max = 36, mask sum = 36, frac = 0.988
[Fri Dec 23 19:39:37 2011] Giving source the simple spatial ID 56 for pass 0, mean size = 10.95"
[Fri Dec 23 22:44:20 2011] fullrun_pn_xmm0555220201_pi300-10000_cl_pass0_src56.ximg exists
[Fri Dec 23 22:44:20 2011] fullrun_pn_xmm0555220201_pi300-10000_cl_pass0_src56_1.ximg exists
[Fri Dec 23 22:44:20 2011] Fit fullrun_pn_xmm0555220201_pi300-10000_cl_pass0_src56 appears to have run properly
[Fri Dec 23 22:44:22 2011] fullrun_pn_xmm0555220201_pi300-10000_cl_pass0_tfrozen_src56.ximg exists
[Fri Dec 23 22:44:22 2011] fullrun_pn_xmm0555220201_pi300-10000_cl_pass0_tfrozen_src56_1.ximg exists
[Fri Dec 23 22:44:22 2011] Fit fullrun_pn_xmm0555220201_pi300-10000_cl_pass0_tfrozen_src56 appears to have run properly
[Sat Dec 24 02:15:10 2011] Warning, spatial fit 56 centroid is now closest to src. 65
[Sat Dec 24 02:15:11 2011] Vigneting correction estimate = 1.000000
[Sat Dec 24 02:15:11 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Sat Dec 24 02:15:11 2011] Assessing source extent using major
[Sat Dec 24 02:15:11 2011] Source does appear to be extended
[Sat Dec 24 02:15:11 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Sat Dec 24 02:16:02 2011] Using EEF radius (= 10.95 ")to estimate initial spatial extent for simple fitting
[Sat Dec 24 02:16:02 2011] Initial guess for spatial extent in simple fitting = 10.95"
[Sat Dec 24 02:16:02 2011] source mask rpix=2.5, npix_max = 36, mask sum = 36, frac = 0.988
[Sat Dec 24 02:16:02 2011] Giving source the simple spatial ID 53 for pass 1, mean size = 10.95"
[Sat Dec 24 06:40:56 2011] fullrun_pn_xmm0555220201_pi300-10000_cl_pass1_src53.ximg exists
[Sat Dec 24 06:40:56 2011] Warning: poor agreement between model and actual number of counts may be indicative of a poor fit in csv/fullrun_pn_xmm0555220201_pi300-10000_cl_pass1_src53.csv
[Sat Dec 24 06:40:56 2011] fullrun_pn_xmm0555220201_pi300-10000_cl_pass1_src53_1.ximg exists
[Sat Dec 24 06:40:56 2011] Warning: poor agreement between model and actual number of counts may be indicative of a poor fit in csv/fullrun_pn_xmm0555220201_pi300-10000_cl_pass1_src53.csv
[Sat Dec 24 06:40:56 2011] It looks like the fit did not converge
You should probably delete fullrun_pn_xmm0555220201_pi300-10000_cl_pass1_src53_1.ximg
Either tweak this fit manually starting from fullrun_pn_xmm0555220201_pi300-10000_cl_pass1_src53.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
[Sat Dec 24 06:40:57 2011] fullrun_pn_xmm0555220201_pi300-10000_cl_pass1_tfrozen_src53.ximg exists
[Sat Dec 24 06:40:57 2011] fullrun_pn_xmm0555220201_pi300-10000_cl_pass1_tfrozen_src53_1.ximg exists
[Sat Dec 24 06:40:57 2011] Fit fullrun_pn_xmm0555220201_pi300-10000_cl_pass1_tfrozen_src53 appears to have run properly
[Sat Dec 24 09:50:02 2011] Warning, spatial fit 53 centroid is now closest to src. 63
[Sat Dec 24 09:50:02 2011] Vigneting correction estimate = 1.000000
[Sat Dec 24 09:50:02 2011] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Sat Dec 24 09:50:02 2011] Assessing source extent using major
[Sat Dec 24 09:50:02 2011] Source does appear to be extended
[Sat Dec 24 09:50:02 2011] Computing asymmetry using major and minor axis, asym = 1.00
[Sat Dec 24 09:50:52 2011] XMMSAS src. selection expression = ellipse(31876.711273, 16838.063797, 652.500000, 652.500000, 0.000000, X, Y)
[Sat Dec 24 09:50:52 2011] Writing source region out to fullrun_pn_xmm0555220201_pi300-10000_pass1_cl_src59_src.reg
[Sat Dec 24 09:50:52 2011] Extracting stamp from image fullrun_pn_xmm0555220201_pi300-10000_cl_sm2.00.img.gz, (329, 157) - (404, 232)
[Sat Dec 24 09:50:52 2011] XMMSAS bgd. selection expression = annulus(31876.711273, 16838.063797, 1087.500000, 2175.000000, X, Y) && !ellipse(28954.384247, 19627.863708, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(33052.852081, 17252.094376, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(29920.172000, 16102.702400, 720.337926, 720.337926, 0.000000, X, Y) && !ellipse(32345.623962, 15855.721542, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(32925.154000, 15934.851880, 347.183210, 347.183210, 0.000000, X, Y)
[Sat Dec 24 09:50:52 2011] Writing fullrun_pn_xmm0555220201_pi300-10000_pass1_cl_src59.gif
[Sat Dec 24 11:35:57 2011] Mean detx,y = (-8902.95, -6041.75) 
[Sat Dec 24 11:36:04 2011] Setting backscal keywords in source and bgd. spectrum
[Sat Dec 24 11:36:42 2011] Binned source spectrum to 10 counts/bin
[Sat Dec 24 11:36:43 2011] Setting source spectrum file to fullrun_pn_xmm0555220201_pi300-10000_pass1_cl_src59_src_b10.pi.gz
[Sat Dec 24 11:36:43 2011] Setting bgd. spectrum file to fullrun_pn_xmm0555220201_pi300-10000_pass1_cl_src59_bgd.pi.gz
[Sat Dec 24 19:39:27 2011] Not generating rmf since RequireSpatial is true but spatial fitting not done
[Sat Dec 24 19:39:27 2011] rmf not generated due to insufficient counts
[Sat Dec 24 22:32:29 2011] Updating aperture counts using extracted products
[Sat Dec 24 22:32:29 2011] Error reading totcts from fullrun_pn_xmm0555220201_pi300-10000_pass1_cl_src59_src_b10.pi.gz
[Sat Dec 24 22:32:33 2011] Calculating source flux in energy range 0.30-8.00
[Sat Dec 24 22:32:33 2011] Using photon index=1.80, rate=0.00265, arf fullrun_pn_xmm0555220201_pi300-10000_pass1_cl_src59.arf
[Sat Dec 24 22:32:33 2011] Assuming count rate is from the 0.30-10.00 bandpass
[Sat Dec 24 22:32:33 2011] Updating source flux to 1.3e-14
[Sat Dec 24 22:37:58 2011] Simple spatial fitting not done (or not done successfully), skipping spectral fitting