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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
190.3922 71.8460 0.0167 36.1247 144.5838 6.3802320 11.434 TRIG_00637899
Foreground time interval of the image:
-73.088 207.956 (delta_t = 281.044 [sec])
Background time interval of the image:
-239.000 -73.088 (delta_t = 165.912 [sec])
Lightcurves
Notes:
- 1) The mask-weighted light curves are using the flight position.
- 2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 3) For all the mask-weighted lightcurves, the y-axis units are counts/sec/det where a det is 0.4 x 0.4 = 0.16 sq cm.
- 4) The verticle lines correspond to following: green dotted lines are T50 interval, black dotted lines are T90 interval, blue solid line(s) is a spacecraft slew start time, and orange solid line(s) is a spacecraft slew end time.
- 5) Time of each bin is in the middle of the bin.
1 s binning
From T0-310 s to T0+310 s
From T100_start - 20 s to T100_end + 30 s
Full time interval
64 ms binning
Full time interval
From T100_start to T100_end
From T0-5 sec to T0+5 sec
16 ms binning
From T100_start-5 s to T100_start+5 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
8 ms binning
From T100_start-3 s to T100_start+3 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
2 ms binning
From T100_start-1 s to T100_start+1 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Quad-rate summed light curves (from T0-300s to T0+1000s)
Spectral Evolution
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
- 3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.
Time averaged spectrum fit using the average DRM
Power-law model
Time interval is from -73.088 sec. to 207.956 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.68386 ( -0.134626 0.136757 )
Norm@50keV : 1.64069E-03 ( -0.000129565 0.000128607 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.02 using 59 PHA bins.
# Reduced chi-squared = 0.9126 for 57 degrees of freedom
# Null hypothesis probability = 6.620659e-01
Photon flux (15-150 keV) in 281 sec: 0.216687 ( -0.0167724 0.0168065 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.27429e-06 ( -3.53897e-07 3.56227e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -73.088 sec. to 207.956 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48436 ( -0.540462 0.317346 )
Epeak [keV] : 128.410 ( -62.2104 -128.41 )
Norm@50keV : 2.07263E-03 ( -0.000618252 0.00176506 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.55 using 59 PHA bins.
# Reduced chi-squared = 0.9205 for 56 degrees of freedom
# Null hypothesis probability = 6.439987e-01
Photon flux (15-150 keV) in 281 sec: 0.214487 ( -0.017593 0.017595 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.215e-06 ( -3.86178e-07 3.85448e-07 ) ergs/cm2
Band function
Time interval is from -73.088 sec. to 207.956 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.48775 ( 1.48742 0.483377 )
beta : -9.36060 ( 9.37162 19.3716 )
Epeak [keV] : 128.747 ( -65.2265 -129.107 )
Norm@50keV : 2.06808E-03 ( -0.000541672 0.00132668 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.55 using 59 PHA bins.
# Reduced chi-squared = 0.9372 for 55 degrees of freedom
# Null hypothesis probability = 6.074043e-01
Photon flux (15-150 keV) in 281 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 13.9878 (-1.35889 1.51222)
R^2/D10^2 : 2.96545E-02 (-0.0092425 0.0133894)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 99.90 using 59 PHA bins.
# Reduced chi-squared = 1.753 for 57 degrees of freedom
# Null hypothesis probability = 3.849083e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.444e-07 4.805e-08
25- 50 1.280e-06 1.346e-07
50-150 1.648e-06 2.768e-07
15-150 3.273e-06 3.147e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 149.411 (-44.9569 -148.463)
Norm : 0.888488 (-0.0765632 0.0963739)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.05 using 59 PHA bins.
# Reduced chi-squared = 0.9131 for 57 degrees of freedom
# Null hypothesis probability = 6.608950e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.414e-07 7.461e-08
25- 50 1.188e-06 2.157e-07
50-150 2.342e-06 1.036e-06
15-150 4.171e-06 1.243e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.82196 (-1.24617 1.46522)
R1^2/D10^2 : 0.470792 (-0.263288 0.765646)
kT2 [keV] : 22.6362 (-3.7637 5.91461)
R2^2/D10^2 : 4.25180E-03 (-0.0024539 0.0042703)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.87 using 59 PHA bins.
# Reduced chi-squared = 0.9249 for 55 degrees of freedom
# Null hypothesis probability = 6.330330e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.816e-07 2.285e-07
25- 50 1.133e-06 2.714e-07
50-150 2.344e-06 7.080e-07
15-150 4.159e-06 1.143e-06
Peak spectrum fit
Power-law model
Time interval is from 110.776 sec. to 111.776 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.43877 ( -0.273148 0.274083 )
Norm@50keV : 1.36263E-02 ( -0.00232446 0.0023192 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 84.39 using 59 PHA bins.
# Reduced chi-squared = 1.480 for 57 degrees of freedom
# Null hypothesis probability = 1.068504e-02
Photon flux (15-150 keV) in 1 sec: 1.67460 ( -0.291877 0.293056 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.30667e-07 ( -2.38706e-08 2.4141e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 110.776 sec. to 111.776 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 4.09273E-02 ( -1.74979 1.24477 )
Epeak [keV] : 72.1688 ( -17.4786 142.892 )
Norm@50keV : 6.58457E-02 ( -0.0658457 0.371917 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.61 using 59 PHA bins.
# Reduced chi-squared = 1.440 for 56 degrees of freedom
# Null hypothesis probability = 1.728846e-02
Photon flux (15-150 keV) in 1 sec: 1.58645 ( -0.30432 0.30461 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21113e-07 ( -2.49796e-08 2.5794e-08 ) ergs/cm2
Band function
Time interval is from 110.776 sec. to 111.776 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.166794 ( -1.12569 4.92938 )
beta : -9.37166 ( 9.37167 19.3717 )
Epeak [keV] : 75.6139 ( -19.1951 126.017 )
Norm@50keV : 5.60501E-02 ( -0.0561153 0.0909859 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.65 using 59 PHA bins.
# Reduced chi-squared = 1.466 for 55 degrees of freedom
# Null hypothesis probability = 1.370894e-02
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.22809e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 15.9460 (-2.65691 3.33833)
R^2/D10^2 : 0.163792 (-0.080585 0.148308)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 82.73 using 59 PHA bins.
# Reduced chi-squared = 1.451 for 57 degrees of freedom
# Null hypothesis probability = 1.461285e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.618e-09 2.773e-09
25- 50 3.616e-08 9.925e-09
50-150 6.418e-08 2.182e-08
15-150 1.090e-07 2.853e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.359 (-87.6776 -199.363)
Norm : 6.98316 (-1.17304 1.17498)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 83.37 using 59 PHA bins.
# Reduced chi-squared = 1.463 for 57 degrees of freedom
# Null hypothesis probability = 1.295961e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.739e-08 1.002e-08
25- 50 3.345e-08 1.915e-08
50-150 7.336e-08 4.200e-08
15-150 1.242e-07 7.055e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.79845 (-5.8016 -5.8016)
R1^2/D10^2 : 1.80100 (-1.79844 -1.79844)
kT2 [keV] : 18.8764 (-4.47306 -18.8776)
R2^2/D10^2 : 8.07327E-02 (-0.0807078 0.146712)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.43 using 59 PHA bins.
# Reduced chi-squared = 1.462 for 55 degrees of freedom
# Null hypothesis probability = 1.428254e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.332e-08 7.690e-09
25- 50 3.421e-08 1.876e-08
50-150 7.153e-08 4.039e-08
15-150 1.190e-07 6.310e-08
Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)
Power-law model
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.68386 ( -0.134626 0.136757 )
Norm@50keV : 1.64069E-03 ( -0.000129565 0.000128607 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.02 using 59 PHA bins.
# Reduced chi-squared = 0.9126 for 57 degrees of freedom
# Null hypothesis probability = 6.620659e-01
Photon flux (15-150 keV) in 281 sec: 0.216687 ( -0.0167724 0.0168065 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.27429e-06 ( -3.53897e-07 3.56227e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48436 ( -0.540462 0.317346 )
Epeak [keV] : 128.410 ( -62.2104 -128.41 )
Norm@50keV : 2.07263E-03 ( -0.000618252 0.00176506 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.55 using 59 PHA bins.
# Reduced chi-squared = 0.9205 for 56 degrees of freedom
# Null hypothesis probability = 6.439987e-01
Photon flux (15-150 keV) in 281 sec: 0.214487 ( -0.017593 0.017595 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.215e-06 ( -3.86178e-07 3.85448e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.48775 ( 1.48742 0.483377 )
beta : -9.36060 ( 9.37162 19.3716 )
Epeak [keV] : 128.747 ( -65.2265 -129.107 )
Norm@50keV : 2.06808E-03 ( -0.000541388 0.000718228 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.55 using 59 PHA bins.
# Reduced chi-squared = 0.9372 for 55 degrees of freedom
# Null hypothesis probability = 6.074043e-01
Photon flux (15-150 keV) in 281 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.15e-06
S(50-100 keV) = 1.43e-06
T90 vs. Hardness ratio plot
T90 = 243.595999956131 sec.
Hardness ratio (energy fluence ratio) = 1.24348
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.26414
Count Ratio (50-100 keV) / (15-25 keV) = 0.936963
Mask shadow pattern
IMX = -5.948195043325304E-01, IMY = -4.229690919355226E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
Spacecraft aspect plot
Bright source in the pre-burst/pre-slew/post-slew images
Pre-burst image of 15-350 keV band
Time interval of the image:
-239.000000 -73.088000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5815 35.2024 0.5 31.4 7.6 5.1215 24.5 0.4 Cyg X-1
308.1455 40.9658 2.0 25.2 -5.7 1.0399 5.8 1.8 Cyg X-3
326.2542 38.3108 2.9 29.4 -35.5 0.7551 4.0 3.9 Cyg X-2
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-73.088000 207.956000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5757 35.1883 4.1 31.5 7.6 1.0191 2.8 1.1 Cyg X-1
308.0424 41.1090 9.3 25.0 -5.5 0.3796 1.2 9.9 Cyg X-3
326.2424 38.2814 7.7 29.5 -35.5 -0.5116 -1.5 4.1 Cyg X-2
154.0464 59.4199 2.7 53.1 156.7 7.2125 4.3 ------ UNKNOWN
190.3922 71.8460 1.0 36.1 144.6 6.3809 11.4 ------ UNKNOWN
268.1817 63.9108 2.5 17.2 94.0 1.5957 4.7 ------ UNKNOWN
273.3206 80.9680 2.1 17.4 154.1 1.5377 5.4 ------ UNKNOWN
76.7910 55.5484 2.3 52.1 -153.2 4.5496 5.0 ------ UNKNOWN
347.9997 28.1634 2.7 44.7 -59.3 5.0119 4.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
672.400620 889.100600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6417 22.0106 0.3 36.3 -175.9 8.9418 33.7 0.5 Crab
175.4580 77.5871 2.4 37.1 41.4 1.7887 4.8 ------ UNKNOWN
65.6015 68.9937 2.1 12.0 8.4 0.9720 5.5 ------ UNKNOWN
346.5268 68.3153 2.2 37.3 -16.4 1.3008 5.2 ------ UNKNOWN
311.8444 59.2783 3.2 54.4 -11.5 2.2769 3.6 ------ UNKNOWN
61.8622 31.4956 2.3 27.0 -137.8 1.1368 5.1 ------ UNKNOWN
326.4173 54.2878 2.0 53.5 -23.0 3.4928 5.7 ------ UNKNOWN
29.9490 33.7014 4.1 37.3 -89.6 1.7744 2.8 ------ UNKNOWN
Plot creation:
Thu May 28 13:00:48 EDT 2015