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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
80.4924 47.5232 0.0035 45.0336 2.0473 6.7397717 54.810 TRIG_00307931
Foreground time interval of the image:
-2.244 19.637 (delta_t = 21.881 [sec])
Background time interval of the image:
-239.264 -2.244 (delta_t = 237.020 [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 1.024000
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 1.024000
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 1.024000
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 -2.244 sec. to 120.620 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40794 ( -0.0416571 0.0415358 )
Norm@50keV : 8.02198E-03 ( -0.000170339 0.000170198 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.52 using 59 PHA bins.
# Reduced chi-squared = 0.9740 for 57 degrees of freedom
# Null hypothesis probability = 5.307797e-01
Photon flux (15-150 keV) in 122.9 sec: 0.978702 ( -0.02397 0.0240661 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.51111e-06 ( -2.05539e-07 2.05784e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.244 sec. to 120.620 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40717 ( -0.079837 0.039942 )
Epeak [keV] : 9999.35 ( -9999.36 -9999.36 )
Norm@50keV : 8.03926E-03 ( -0.00016945 0.000643899 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.64 using 59 PHA bins.
# Reduced chi-squared = 0.9935 for 56 degrees of freedom
# Null hypothesis probability = 4.884924e-01
Photon flux (15-150 keV) in 122.9 sec: 0.979738 ( -0.025725 0.022572 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.51145e-06 ( -2.01445e-07 1.99381e-07 ) ergs/cm2
Band function
Time interval is from -2.244 sec. to 120.620 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.12281 ( 1.12283 1.12283 )
beta : -1.40794 ( -0.0415397 0.0415987 )
Epeak [keV] : 36.7517 ( -36.7437 -36.7437 )
Norm@50keV : 1.60468E-02 ( -0.00574769 0.682438 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.52 using 59 PHA bins.
# Reduced chi-squared = 1.009 for 55 degrees of freedom
# Null hypothesis probability = 4.550268e-01
Photon flux (15-150 keV) in 122.9 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] : 19.0275 ( )
R^2/D10^2 : 4.76895E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 584.53 using 59 PHA bins.
# Reduced chi-squared = 10.255 for 57 degrees of freedom
# Null hypothesis probability = 1.459966e-88
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.169e-07 1.788e-08
25- 50 2.007e-06 6.329e-08
50-150 5.342e-06 1.837e-07
15-150 7.766e-06 1.825e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 4.11437 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 132.93 using 59 PHA bins.
# Reduced chi-squared = 2.3322 for 57 degrees of freedom
# Null hypothesis probability = 5.266184e-08
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.259e-06 3.202e-08
25- 50 2.422e-06 5.899e-08
50-150 5.312e-06 1.364e-07
15-150 8.993e-06 2.157e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.02091 (-0.63809 0.676219)
R1^2/D10^2 : 0.614739 (-0.147605 0.209011)
kT2 [keV] : 33.7392 (-2.80897 3.57411)
R2^2/D10^2 : 5.81522E-03 (-0.00161523 0.00196792)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.84 using 59 PHA bins.
# Reduced chi-squared = 1.270 for 55 degrees of freedom
# Null hypothesis probability = 8.587758e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.987e-07 8.628e-08
25- 50 2.310e-06 9.893e-08
50-150 6.208e-06 2.986e-07
15-150 9.517e-06 3.681e-07
Peak spectrum fit
Power-law model
Time interval is from 9.280 sec. to 10.280 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.837181 ( -0.106768 0.104507 )
Norm@50keV : 4.75190E-02 ( -0.00298625 0.00296418 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 86.36 using 59 PHA bins.
# Reduced chi-squared = 1.515 for 57 degrees of freedom
# Null hypothesis probability = 7.278158e-03
Photon flux (15-150 keV) in 1 sec: 5.45592 ( -0.337433 0.338085 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.46811e-07 ( -3.40556e-08 3.40963e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 9.280 sec. to 10.280 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.669985 ( -0.442996 0.213161 )
Epeak [keV] : 498.737 ( -498.737 -498.737 )
Norm@50keV : 5.56390E-02 ( -0.0140276 0.0275314 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 85.88 using 59 PHA bins.
# Reduced chi-squared = 1.534 for 56 degrees of freedom
# Null hypothesis probability = 6.261949e-03
Photon flux (15-150 keV) in 1 sec: 5.42613 ( -0.34447 0.34552 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.45528e-07 ( -3.4612e-08 3.4498e-08 ) ergs/cm2
Band function
Time interval is from 9.280 sec. to 10.280 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.820953 ( 0.82046 0.82046 )
beta : -0.858585 ( -0.104479 0.106826 )
Epeak [keV] : 10000.00 ( -10000 -10000 )
Norm@50keV : 4.77622E-02 ( -0.00321021 0.00279987 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 86.34 using 59 PHA bins.
# Reduced chi-squared = 1.570 for 55 degrees of freedom
# Null hypothesis probability = 4.424985e-03
Photon flux (15-150 keV) in 1 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] : 26.2038 ( )
R^2/D10^2 : 0.120485 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 124.78 using 59 PHA bins.
# Reduced chi-squared = 2.1892 for 57 degrees of freedom
# Null hypothesis probability = 5.685078e-07
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.401e-08 1.810e-09
25- 50 8.136e-08 7.785e-09
50-150 4.109e-07 3.610e-08
15-150 5.062e-07 3.725e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 21.9477 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 212.35 using 59 PHA bins.
# Reduced chi-squared = 3.7255 for 57 degrees of freedom
# Null hypothesis probability = 9.417451e-20
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.465e-08 4.305e-09
25- 50 1.051e-07 8.315e-09
50-150 2.306e-07 5.795e-08
15-150 3.903e-07 6.055e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.2415 (-3.02781 3.98252)
R1^2/D10^2 : 1.03765 (-0.570413 1.82929)
kT2 [keV] : 43.2142 (-9.87909 35.936)
R2^2/D10^2 : 2.37698E-02 (-0.018726 0.021999)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 87.00 using 59 PHA bins.
# Reduced chi-squared = 1.582 for 55 degrees of freedom
# Null hypothesis probability = 3.856365e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.775e-08 1.224e-08
25- 50 9.516e-08 2.692e-08
50-150 4.274e-07 1.804e-07
15-150 5.503e-07 2.034e-07
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: 1.14047 ( -0.0491068 0.0487832 )
Norm@50keV : 2.09730E-02 ( -0.000575306 0.000573168 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.36 using 59 PHA bins.
# Reduced chi-squared = 0.9887 for 57 degrees of freedom
# Null hypothesis probability = 4.991533e-01
Photon flux (15-150 keV) in 21.88 sec: 2.44316 ( -0.0719362 0.0722266 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.73763e-06 ( -1.28221e-07 1.28275e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.08442 ( -0.176718 0.0765336 )
Epeak [keV] : 938.074 ( -981.475 -981.475 )
Norm@50keV : 2.21286E-02 ( -0.00233839 0.00386224 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.43 using 59 PHA bins.
# Reduced chi-squared = 1.008 for 56 degrees of freedom
# Null hypothesis probability = 4.585909e-01
Photon flux (15-150 keV) in 21.88 sec: 2.44040 ( -0.07007 0.0736 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.73076e-06 ( -1.28851e-07 1.37428e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.968273 ( 0.816673 0.816673 )
beta : -1.17217 ( 1.18087 0.0844493 )
Epeak [keV] : 290.730 ( -327.289 -327.289 )
Norm@50keV : 2.54704E-02 ( -0.00305346 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.84 using 59 PHA bins.
# Reduced chi-squared = 1.015 for 55 degrees of freedom
# Null hypothesis probability = 4.430875e-01
Photon flux (15-150 keV) in 21.88 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) = 2.24e-06
S(50-100 keV) = 3.38e-06
T90 vs. Hardness ratio plot
T90 = 91.108000010252 sec.
Hardness ratio (energy fluence ratio) = 1.50893
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.36545
Count Ratio (50-100 keV) / (15-25 keV) = 1.19761
Mask shadow pattern
IMX = 1.000534735716935E+00, IMY = -3.576715780596132E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-239.264000 -2.244000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6348 22.0155 0.2 24.7 30.7 10.2714 52.3 0.1 Crab
102.7582 -2.6695 2.5 37.5 88.1 2.8080 4.7 ------ UNKNOWN
73.1035 -37.8079 2.9 42.6 159.6 1.6185 4.0 ------ UNKNOWN
50.9275 -4.8073 3.2 17.5 -133.2 0.6960 3.6 ------ UNKNOWN
36.9405 14.6149 3.2 30.3 -80.0 1.0632 3.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.244000 19.636600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4940 22.0760 18.6 24.7 30.4 0.0441 0.6 8.6 Crab
77.3361 -43.7175 2.8 49.1 157.1 0.7460 4.1 ------ UNKNOWN
68.0650 -24.2295 2.7 28.6 163.8 0.2933 4.4 ------ UNKNOWN
80.4910 47.5235 0.2 45.0 2.0 6.7532 54.9 ------ UNKNOWN
47.1013 -4.0183 3.0 20.5 -125.6 0.2376 3.9 ------ UNKNOWN
29.9935 41.7746 2.4 49.3 -47.1 1.2625 4.7 ------ UNKNOWN
26.9084 23.3529 2.5 42.1 -71.3 1.0182 4.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
88.036600 962.798700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6392 22.0147 0.2 25.7 -176.2 37.4976 75.1 0.3 Crab
106.2348 84.2408 3.8 37.3 14.8 1.9820 3.1 ------ UNKNOWN
87.1454 16.6541 3.0 31.4 178.2 2.1822 3.9 ------ UNKNOWN
37.7596 69.6090 2.6 30.2 -17.4 2.3205 4.4 ------ UNKNOWN
19.6122 63.7342 0.7 36.2 -30.2 11.5851 17.5 ------ UNKNOWN
50.5151 33.8851 3.1 26.2 -99.8 2.4080 3.8 ------ UNKNOWN
Plot creation:
Sun May 31 07:56:54 EDT 2015