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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
0.6693 7.0073 0.0050 33.1059 99.4698 13.2954125 38.696 TRIG_00434843
Foreground time interval of the image:
-1.760 87.244 (delta_t = 89.004 [sec])
Background time interval of the image:
-239.104 -1.760 (delta_t = 237.344 [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 -1.760 sec. to 87.244 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.51633 ( -0.0562688 0.056395 )
Norm@50keV : 9.57661E-03 ( -0.000285061 0.000284991 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.20 using 59 PHA bins.
# Reduced chi-squared = 1.109 for 57 degrees of freedom
# Null hypothesis probability = 2.668113e-01
Photon flux (15-150 keV) in 89 sec: 1.20086 ( -0.038758 0.0388669 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.06441e-06 ( -2.56093e-07 2.56552e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.760 sec. to 87.244 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.24266 ( -0.237746 0.225752 )
Epeak [keV] : 149.468 ( -45.3865 378.216 )
Norm@50keV : 1.28370E-02 ( -0.00269383 0.00361599 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.89 using 59 PHA bins.
# Reduced chi-squared = 1.052 for 56 degrees of freedom
# Null hypothesis probability = 3.703100e-01
Photon flux (15-150 keV) in 89 sec: 1.17714 ( -0.04292 0.04314 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.91368e-06 ( -2.87568e-07 2.86277e-07 ) ergs/cm2
Band function
Time interval is from -1.760 sec. to 87.244 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.22081 ( -0.449307 1.41063 )
beta : -1.77552 ( 1.78474 0.25929 )
Epeak [keV] : 139.270 ( -94.4856 360.747 )
Norm@50keV : 1.31991E-02 ( -0.00280237 0.0401899 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.82 using 59 PHA bins.
# Reduced chi-squared = 1.069 for 55 degrees of freedom
# Null hypothesis probability = 3.373997e-01
Photon flux (15-150 keV) in 89 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] : 16.2256 ( )
R^2/D10^2 : 0.100019 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 267.95 using 59 PHA bins.
# Reduced chi-squared = 4.7008 for 57 degrees of freedom
# Null hypothesis probability = 4.457045e-29
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.830e-07 2.706e-08
25- 50 2.057e-06 8.989e-08
50-150 3.805e-06 2.198e-07
15-150 6.345e-06 2.229e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 4.90282 (-0.145334 0.145332)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.62 using 59 PHA bins.
# Reduced chi-squared = 1.099 for 57 degrees of freedom
# Null hypothesis probability = 2.835275e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.087e-06 3.516e-08
25- 50 2.090e-06 7.387e-08
50-150 4.585e-06 1.624e-07
15-150 7.762e-06 2.403e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.28294 (-0.91771 1.00655)
R1^2/D10^2 : 1.00689 (-0.345005 0.605811)
kT2 [keV] : 26.3836 (-2.72099 3.7726)
R2^2/D10^2 : 1.47045E-02 (-0.0056734 0.00742268)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.80 using 59 PHA bins.
# Reduced chi-squared = 1.215 for 55 degrees of freedom
# Null hypothesis probability = 1.321347e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.478e-07 1.145e-07
25- 50 2.068e-06 1.495e-07
50-150 4.801e-06 4.294e-07
15-150 7.818e-06 6.083e-07
Peak spectrum fit
Power-law model
Time interval is from 44.460 sec. to 45.460 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.15815 ( -0.138645 0.137867 )
Norm@50keV : 3.80065E-02 ( -0.0031388 0.0031382 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.85 using 59 PHA bins.
# Reduced chi-squared = 1.208 for 57 degrees of freedom
# Null hypothesis probability = 1.351358e-01
Photon flux (15-150 keV) in 1 sec: 4.43669 ( -0.376125 0.376582 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.90303e-07 ( -3.54201e-08 3.55649e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 44.460 sec. to 45.460 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.472774 ( -0.684066 0.592601 )
Epeak [keV] : 126.337 ( -36.9441 367.451 )
Norm@50keV : 7.77479E-02 ( -0.0352651 0.0757849 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.90 using 59 PHA bins.
# Reduced chi-squared = 1.159 for 56 degrees of freedom
# Null hypothesis probability = 1.941445e-01
Photon flux (15-150 keV) in 1 sec: 4.33127 ( -0.38812 0.38772 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.80655e-07 ( -3.7228e-08 3.7108e-08 ) ergs/cm2
Band function
Time interval is from 44.460 sec. to 45.460 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.472775 ( -0.371102 0.726378 )
beta : -10.0000 ( 10 20 )
Epeak [keV] : 126.319 ( -26.9977 187.797 )
Norm@50keV : 7.77484E-02 ( -0.0352863 0.0760193 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.90 using 59 PHA bins.
# Reduced chi-squared = 1.180 for 55 degrees of freedom
# Null hypothesis probability = 1.696265e-01
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] : 19.9690 (-1.90473 2.15885)
R^2/D10^2 : 0.215715 (-0.0617134 0.0837884)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 80.58 using 59 PHA bins.
# Reduced chi-squared = 1.414 for 57 degrees of freedom
# Null hypothesis probability = 2.157875e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.659e-08 2.700e-09
25- 50 8.256e-08 1.026e-08
50-150 2.440e-07 3.370e-08
15-150 3.432e-07 3.655e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 18.2629 (-1.54765 1.54755)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 89.14 using 59 PHA bins.
# Reduced chi-squared = 1.564 for 57 degrees of freedom
# Null hypothesis probability = 4.156400e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.548e-08 5.320e-09
25- 50 8.750e-08 2.546e-08
50-150 1.919e-07 8.398e-08
15-150 3.249e-07 1.120e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.24869 (-1.91269 7.74052)
R1^2/D10^2 : 17.3780 (-16.1018 409.689)
kT2 [keV] : 22.9601 (-3.00084 15.4358)
R2^2/D10^2 : 0.128332 (-0.108817 0.0784)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.54 using 59 PHA bins.
# Reduced chi-squared = 1.192 for 55 degrees of freedom
# Null hypothesis probability = 1.563950e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.328e-08 1.379e-08
25- 50 7.549e-08 1.655e-08
50-150 2.621e-07 4.900e-08
15-150 3.708e-07 5.590e-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: 1.51633 ( -0.0562688 0.056395 )
Norm@50keV : 9.57661E-03 ( -0.000285061 0.000284991 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.20 using 59 PHA bins.
# Reduced chi-squared = 1.109 for 57 degrees of freedom
# Null hypothesis probability = 2.668113e-01
Photon flux (15-150 keV) in 89 sec: 1.20086 ( -0.038758 0.0388669 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.06441e-06 ( -2.56093e-07 2.56552e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.24266 ( -0.237746 0.225752 )
Epeak [keV] : 149.468 ( -45.3865 378.216 )
Norm@50keV : 1.28370E-02 ( -0.00269383 0.00361599 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.89 using 59 PHA bins.
# Reduced chi-squared = 1.052 for 56 degrees of freedom
# Null hypothesis probability = 3.703100e-01
Photon flux (15-150 keV) in 89 sec: 1.17714 ( -0.04292 0.04314 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.91368e-06 ( -2.87568e-07 2.86277e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.22081 ( -0.449307 1.41063 )
beta : -1.77552 ( 1.78474 0.25929 )
Epeak [keV] : 139.270 ( -94.4856 363.088 )
Norm@50keV : 1.31991E-02 ( -0.00280237 0.0401899 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.82 using 59 PHA bins.
# Reduced chi-squared = 1.069 for 55 degrees of freedom
# Null hypothesis probability = 3.373997e-01
Photon flux (15-150 keV) in 89 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) = 2.01e-06
S(50-100 keV) = 2.81e-06
T90 vs. Hardness ratio plot
T90 = 71.9479999542236 sec.
Hardness ratio (energy fluence ratio) = 1.39801
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.40646
Count Ratio (50-100 keV) / (15-25 keV) = 1.09315
Mask shadow pattern
IMX = -1.072788815451070E-01, IMY = -6.431526300249275E-01
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:
-239.104000 -1.760000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
27.6204 18.1960 2.5 36.6 150.2 1.6195 4.6 ------ UNKNOWN
49.0951 16.1531 2.2 43.0 -178.9 1.7543 5.1 ------ UNKNOWN
6.6964 -38.3796 3.1 24.6 -6.8 0.7684 3.7 ------ UNKNOWN
46.9565 -61.8656 3.4 47.0 -53.2 3.4363 3.5 ------ UNKNOWN
68.4826 -23.8455 3.1 43.1 -111.9 3.6053 3.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.760000 87.244000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
0.6693 7.0073 0.3 33.1 99.5 13.2943 38.6 422.3 UNKNOWN
332.3156 -42.2708 2.5 48.8 11.3 1.7737 4.7 ------ UNKNOWN
55.3566 8.4278 2.5 41.8 -164.4 0.9411 4.6 ------ UNKNOWN
17.2799 -69.2963 2.2 51.4 -35.4 1.9615 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
-239.104000 962.923400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
0.6836 7.0235 1.2 33.1 99.5 13.2552 9.9 423.4 UNKNOWN
27.6032 18.1972 2.4 36.6 150.2 5.8134 4.8 ------ UNKNOWN
23.0505 -5.8085 2.5 12.2 144.3 2.8755 4.7 ------ UNKNOWN
6.7522 -38.4042 2.9 24.6 -6.9 2.6550 4.0 ------ UNKNOWN
49.0835 -12.1019 2.6 26.2 -137.2 3.0815 4.4 ------ UNKNOWN
343.0727 -63.6274 2.8 52.9 -17.0 6.3085 4.1 ------ UNKNOWN
47.0214 -61.9174 9.1 47.1 -53.2 4.4454 1.3 ------ UNKNOWN
71.7804 -11.1619 2.4 48.0 -128.9 14.5686 4.7 ------ UNKNOWN
72.8954 -6.9589 2.6 50.2 -133.9 16.8347 4.5 ------ UNKNOWN
Plot creation:
Sat May 30 23:48:07 EDT 2015