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Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
98.2338 +9.2107 0.0430 2.3 146.0 0.3546 4.5 TRIG_00421072
------------------------------------------
Foreground time interval of the image:
0.000 64.000 (delta_t = 64.000 [sec])
Background time interval of the image:
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 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)
The mask-weighted light curves based on cleaned DPHs
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) For long bursts, a spectral fit of 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.
- 4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.
Time averaged spectrum fit using the pre-slew DRM
Power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.69065 ( -0.586549 0.752511 )
Norm@50keV : 2.28129E-04 ( -0.000228129 0.000137098 )
------------------------------------------------------------
# Chi-Squared = 49.70 using 59 PHA bins.
# Reduced chi-squared = 0.8720 for 57 degrees of freedom
# Null hypothesis probability = 7.427164e-01
Photon flux (15-150 keV) in 64 sec: 5.06006E-02 ( -0.0143935 0.0145665 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.54818e-07 ( -5.63731e-08 6.65402e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.91030 ( )
Epeak [keV] : 22.7877 ( -3.59239 4.13489 )
Norm@50keV : 133.814 ( -133.814 39.3767 )
------------------------------------------------------------
# Chi-Squared = 44.98 using 59 PHA bins.
# Reduced chi-squared = 0.8033 for 56 degrees of freedom
# Null hypothesis probability = 8.540754e-01
Photon flux (15-150 keV) in 64 sec: 4.98444E-02 ( -0.0129426 0.0130298 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.22034e-07 ( -3.50157e-08 3.72166e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.38542 ( 1.31834 1.31834 )
beta : -9.37167 ( 4.59225 14.1326 )
Epeak [keV] : 22.8144 ( -12.0863 96.9146 )
Norm@50keV : 51.1677 ( -51.1778 18.6924 )
------------------------------------------------------------
# Chi-Squared = 45.07 using 59 PHA bins.
# Reduced chi-squared = 0.8195 for 55 degrees of freedom
# Null hypothesis probability = 8.278900e-01
Photon flux (15-150 keV) in 64 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] : 5.56417 (-1.18838 1.48913)
R^2/D10^2 : 0.276200 (-0.276212 0.519318)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
# Chi-Squared = 45.83 using 59 PHA bins.
# Reduced chi-squared = 0.8040 for 57 degrees of freedom
# Null hypothesis probability = 8.554060e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.472e-08 3.773e-08
25- 50 5.452e-08 3.475e-08
50-150 3.627e-09 3.306e-09
15-150 1.229e-07 7.482e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 19.8630 (-8.37781 18.4886)
Norm : 0.622518 (-0.296022 0.607045)
------------------------------------------------------------
# Chi-Squared = 48.08 using 59 PHA bins.
# Reduced chi-squared = 0.8435 for 57 degrees of freedom
# Null hypothesis probability = 7.939041e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.143e-08 3.043e-08
25- 50 5.351e-08 3.193e-08
50-150 1.584e-08 1.435e-08
15-150 1.308e-07 7.811e-08
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.42427 (-1.18835 1.48916)
R1^2/D10^2 : 0.302567 (-0.276218 0.519289)
kT2 [keV] : 199.363 ( )
R2^2/D10^2 : 3.46211E-06 (-3.4967e-06 -3.4967e-06)
------------------------------------------------------------
# Chi-Squared = 45.83 using 59 PHA bins.
# Chi-Squared = 44.62 using 59 PHA bins.
# Reduced chi-squared = 0.8333 for 55 degrees of freedom
# Reduced chi-squared = 0.8113 for 55 degrees of freedom
# Null hypothesis probability = 8.061056e-01
# Null hypothesis probability = 8.400960e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.68683 ( -0.563105 0.72238 )
Norm@50keV : 2.32086E-04 ( -0.000232086 0.000136195 )
------------------------------------------------------------
# Chi-Squared = 50.79 using 59 PHA bins.
# Reduced chi-squared = 0.8910 for 57 degrees of freedom
# Null hypothesis probability = 7.059375e-01
Photon flux (15-150 keV) in 64 sec: 5.13486E-02 ( -0.0140926 0.0142931 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.57293e-07 ( -5.59674e-08 6.61344e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.90682 ( )
Epeak [keV] : 22.6077 ( -3.4528 3.92293 )
Norm@50keV : 143.213 ( -143.213 40.2606 )
------------------------------------------------------------
# Chi-Squared = 45.71 using 59 PHA bins.
# Reduced chi-squared = 0.8163 for 56 degrees of freedom
# Null hypothesis probability = 8.351505e-01
Photon flux (15-150 keV) in 64 sec: 5.06995E-02 ( -0.0126467 0.0127421 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.23668e-07 ( -3.44576e-08 3.64992e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.25392 ( 1.43045 1.43045 )
beta : -9.37167 ( 3.88676 13.0365 )
Epeak [keV] : 22.8262 ( -11.6899 11.1263 )
Norm@50keV : 40.9922 ( -37.9314 33.5267 )
------------------------------------------------------------
# Chi-Squared = 45.84 using 59 PHA bins.
# Reduced chi-squared = 0.8335 for 55 degrees of freedom
# Null hypothesis probability = 8.057832e-01
Photon flux (15-150 keV) in 64 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] : 5.52930 (-1.14778 1.41608)
R^2/D10^2 : 0.288632 (-0.288632 0.509325)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
# Chi-Squared = 46.61 using 59 PHA bins.
# Reduced chi-squared = 0.8178 for 57 degrees of freedom
# Null hypothesis probability = 8.353519e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.609e-08 3.704e-08
25- 50 5.488e-08 3.491e-08
50-150 3.551e-09 3.296e-09
15-150 1.245e-07 7.389e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 19.8384 (-8.19513 17.3549)
Norm : 0.632396 (-0.289609 0.580227)
------------------------------------------------------------
# Chi-Squared = 49.03 using 59 PHA bins.
# Reduced chi-squared = 0.8601 for 57 degrees of freedom
# Null hypothesis probability = 7.647318e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.234e-08 3.191e-08
25- 50 5.425e-08 3.288e-08
50-150 1.603e-08 1.452e-08
15-150 1.326e-07 7.306e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.38846 (-1.11635 1.37869)
R1^2/D10^2 : 0.315424 (-0.234229 0.56338)
kT2 [keV] : 198.199 (-199.956 -199.956)
R2^2/D10^2 : 3.67390E-06 (-3.61876e-06 0.606656)
------------------------------------------------------------
# Chi-Squared = 45.39 using 59 PHA bins.
# Reduced chi-squared = 0.8253 for 55 degrees of freedom
# Null hypothesis probability = 8.188170e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.592e-08 3.728e-08
25- 50 5.385e-08 3.200e-08
50-150 6.474e-08 3.121e-09
15-150 1.845e-07 7.453e-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: 2.69065 ( -0.586549 0.752511 )
Norm@50keV : 2.28129E-04 ( -0.000228129 0.000137098 )
------------------------------------------------------------
# Chi-Squared = 49.70 using 59 PHA bins.
# Reduced chi-squared = 0.8720 for 57 degrees of freedom
# Null hypothesis probability = 7.427164e-01
Photon flux (15-150 keV) in 64 sec: 5.06006E-02 ( -0.0143935 0.0145665 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.54818e-07 ( -5.63731e-08 6.65402e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.91030 ( )
Epeak [keV] : 22.7877 ( -3.59239 4.13489 )
Norm@50keV : 133.814 ( -133.814 39.3767 )
------------------------------------------------------------
# Chi-Squared = 44.98 using 59 PHA bins.
# Reduced chi-squared = 0.8033 for 56 degrees of freedom
# Null hypothesis probability = 8.540754e-01
Photon flux (15-150 keV) in 64 sec: 4.98444E-02 ( -0.0129426 0.0130298 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.22034e-07 ( -3.50157e-08 3.72198e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.38542 ( 1.31834 1.31834 )
beta : -9.37167 ( 4.59225 14.1326 )
Epeak [keV] : 22.8144 ( -12.0863 96.9146 )
Norm@50keV : 51.1677 ( -51.1778 18.6924 )
------------------------------------------------------------
# Chi-Squared = 45.07 using 59 PHA bins.
# Reduced chi-squared = 0.8195 for 55 degrees of freedom
# Null hypothesis probability = 8.278900e-01
Photon flux (15-150 keV) in 64 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) = 5.19849e-08
S(50-100 keV) = 3.22074e-08
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 0.619553
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.571578
Count Ratio (50-100 keV) / (15-25 keV) = -0.0635959
Mask shadow pattern
IMX = -3.364079326421376E-02, IMY = -2.267032450984514E-02
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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6180 22.0146 0.4 17.1 -71.3 2.6580 27.7 0.8 Crab
114.3509 -31.7632 2.3 46.1 139.1 1.6916 5.1 ------ UNKNOWN
88.1019 -35.0556 2.7 47.4 169.5 0.8878 4.2 ------ UNKNOWN
98.2337 9.2106 2.6 2.3 146.0 0.3549 4.5 ------ UNKNOWN
73.4697 -25.9917 2.3 44.3 -169.2 0.7523 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
98.600610 963.088100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6339 22.0183 0.2 19.0 -58.8 35.0295 62.5 0.2 Crab
139.4520 14.1354 2.8 40.6 66.0 9.9024 4.2 ------ UNKNOWN
58.5280 32.7771 3.4 43.5 -64.2 9.4837 3.4 ------ UNKNOWN
60.3522 48.8486 2.7 50.7 -44.4 13.4680 4.3 ------ UNKNOWN
56.1797 3.9422 2.7 42.1 -107.2 10.6501 4.3 ------ UNKNOWN
Plot creation:
Wed May 5 02:17:31 EDT 2010