[Tue Mar 13 23:04:02 2012] Detection parameters:
  Position = (337.5, 162.5) = 1 7 34.14 -73 20 23.1
  Extent = 10.9" x 10.9", rotation angle = 0 degrees
  Source counts = 117.1 +/- 16.4
  Background counts = 45.6
  Rate = 0.003 +/- 0.0005

[Tue Mar 13 23:04:05 2012] Off-axis axis estimate = 10.25'
[Tue Mar 13 23:09:11 2012] Using EEF radius (= 11.56 ")to estimate initial spatial extent for simple fitting
[Tue Mar 13 23:09:11 2012] Initial guess for spatial extent in simple fitting = 11.56"
[Tue Mar 13 23:09:11 2012] source mask rpix=2.7, npix_max = 39, mask sum = 49, frac = 1.230
[Tue Mar 13 23:09:11 2012] Giving source the simple spatial ID 17 for pass 0, mean size = 11.56"
[Wed Mar 14 02:57:44 2012] fullrun_pn_xmm0601212701_pi300-10000_cl_pass0_src17.ximg exists
[Wed Mar 14 02:57:44 2012] fullrun_pn_xmm0601212701_pi300-10000_cl_pass0_src17_1.ximg exists
[Wed Mar 14 02:57:44 2012] Fit fullrun_pn_xmm0601212701_pi300-10000_cl_pass0_src17 appears to have run properly
[Wed Mar 14 02:57:46 2012] fullrun_pn_xmm0601212701_pi300-10000_cl_pass0_tfrozen_src17.ximg exists
[Wed Mar 14 02:57:46 2012] fullrun_pn_xmm0601212701_pi300-10000_cl_pass0_tfrozen_src17_1.ximg exists
[Wed Mar 14 02:57:46 2012] Fit fullrun_pn_xmm0601212701_pi300-10000_cl_pass0_tfrozen_src17 appears to have run properly
[Wed Mar 14 05:27:55 2012] Spatial fit model total counts = 625.568000, observed total counts = 605.000000
[Wed Mar 14 05:27:55 2012] Offset between fit and detection position for source 18 = 0.189806 pixels
[Wed Mar 14 05:27:55 2012] 615.274400 total counts/ 534.891000 bgd. counts: snr = 3.475632
Spatial fit parameters:
  Offset between fit and detection position for source 18 = 0.189806 pixels
  Position = (337.7, 162.5) = 1 7 33.95 -73 20 22.5
  Extent = 7.0" x 4.8", rotation angle = 347
  Source counts = 80.4 +/- 24.8
  Background counts = 534.9
  Rate = 0.002 +/- 0.0007
[Wed Mar 14 05:27:55 2012] Vigneting correction estimate = 1.000000
[Wed Mar 14 05:27:55 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Wed Mar 14 05:27:55 2012] Assessing source extent using major
[Wed Mar 14 05:27:55 2012] Source does appear to be extended
[Wed Mar 14 05:27:55 2012] Computing asymmetry using major and minor axis, asym = 1.45
[Wed Mar 14 05:28:28 2012] Using previous fit value to estimate initial spatial extent for simple fitting
[Wed Mar 14 05:28:28 2012] Initial guess for spatial extent in simple fitting = 5.90"
[Wed Mar 14 05:28:28 2012] source mask rpix=1.4, npix_max = 13, mask sum = 12, frac = 0.871
[Wed Mar 14 05:28:28 2012] Giving source the simple spatial ID 17 for pass 1, mean size = 5.90"
[Wed Mar 14 08:37:38 2012] fullrun_pn_xmm0601212701_pi300-10000_cl_pass1_src17.ximg exists
[Wed Mar 14 08:37:38 2012] fullrun_pn_xmm0601212701_pi300-10000_cl_pass1_src17_1.ximg exists
[Wed Mar 14 08:37:38 2012] Fit fullrun_pn_xmm0601212701_pi300-10000_cl_pass1_src17 appears to have run properly
[Wed Mar 14 08:37:40 2012] fullrun_pn_xmm0601212701_pi300-10000_cl_pass1_tfrozen_src17.ximg exists
[Wed Mar 14 08:37:40 2012] fullrun_pn_xmm0601212701_pi300-10000_cl_pass1_tfrozen_src17_1.ximg exists
[Wed Mar 14 08:37:40 2012] Fit fullrun_pn_xmm0601212701_pi300-10000_cl_pass1_tfrozen_src17 appears to have run properly
[Wed Mar 14 11:26:48 2012] Spatial fit model total counts = 625.540000, observed total counts = 605.000000
[Wed Mar 14 11:26:48 2012] Offset between fit and detection position for source 18 = 0.005680 pixels
[Wed Mar 14 11:26:48 2012] 615.256500 total counts/ 534.865000 bgd. counts: snr = 3.476066
Spatial fit parameters:
  Offset between fit and detection position for source 18 = 0.005680 pixels
  Position = (337.7, 162.5) = 1 7 33.96 -73 20 22.5
  Extent = 7.0" x 4.8", rotation angle = 344
  Source counts = 80.4 +/- 24.8
  Background counts = 534.9
  Rate = 0.002 +/- 0.0007
[Wed Mar 14 11:26:48 2012] Vigneting correction estimate = 1.000000
[Wed Mar 14 11:26:48 2012] Source flux estimate in the 0.3-8.0 bandpass, Gamma=1.800000 = 0 
[Wed Mar 14 11:26:48 2012] Assessing source extent using major
[Wed Mar 14 11:26:48 2012] Source does appear to be extended
[Wed Mar 14 11:26:48 2012] Computing asymmetry using major and minor axis, asym = 1.46
[Wed Mar 14 11:27:29 2012] XMMSAS src. selection expression = ellipse(29327.625000, 14089.244000, 419.833812, 288.538208, 343.530090, X, Y)
[Wed Mar 14 11:27:29 2012] Writing source region out to fullrun_pn_xmm0601212701_pi300-10000_pass1_cl_src18_src.reg
[Wed Mar 14 11:27:29 2012] Extracting stamp from image fullrun_pn_xmm0601212701_pi300-10000_cl_sm2.00.img.gz, (314, 138) - (362, 187)
[Wed Mar 14 11:27:29 2012] XMMSAS bgd. selection expression = annulus(29327.625000, 14089.244000, 699.723020, 1399.446040, X, Y) && !ellipse(28348.044586, 12402.599731, 870.000000, 870.000000, 0.000000, X, Y) && !ellipse(28601.554749, 12921.178726, 870.000000, 870.000000, 0.000000, X, Y)
[Wed Mar 14 11:27:29 2012] Writing fullrun_pn_xmm0601212701_pi300-10000_pass1_cl_src18.gif
[Wed Mar 14 11:52:12 2012] Mean detx,y = (5841.02, 11677.44) 
[Wed Mar 14 11:52:20 2012] Setting backscal keywords in source and bgd. spectrum
[Wed Mar 14 11:52:45 2012] Binned source spectrum to 10 counts/bin
[Wed Mar 14 11:52:46 2012] Setting source spectrum file to fullrun_pn_xmm0601212701_pi300-10000_pass1_cl_src18_src_b10.pi.gz
[Wed Mar 14 11:52:46 2012] Setting bgd. spectrum file to fullrun_pn_xmm0601212701_pi300-10000_pass1_cl_src18_bgd.pi.gz
[Wed Mar 14 13:14:56 2012] Not generating rmf since there are only 80 counts
[Wed Mar 14 13:14:56 2012] rmf not generated due to insufficient counts
[Wed Mar 14 15:29:38 2012] Updating aperture counts using extracted products
[Wed Mar 14 15:29:38 2012] Error reading totcts from fullrun_pn_xmm0601212701_pi300-10000_pass1_cl_src18_src_b10.pi.gz
[Wed Mar 14 15:29:42 2012] Calculating source flux in energy range 0.30-8.00
[Wed Mar 14 15:29:42 2012] Using photon index=1.80, rate=0.00229, arf fullrun_pn_xmm0601212701_pi300-10000_pass1_cl_src18.arf
[Wed Mar 14 15:29:42 2012] Assuming count rate is from the 0.30-10.00 bandpass
[Wed Mar 14 15:29:42 2012] Updating source flux to 1.5e-14
[Wed Mar 14 15:32:27 2012] Source 18 has fewer than 100.000000 counts, skipping spectral fitting