Special notes of this burst
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
69.0243 43.7153 0.0105 33.3720 -155.1575 0.4870249 18.359 TRIG_00445321
Foreground time interval of the image:
-1.764 2.588 (delta_t = 4.352 [sec])
Background time interval of the image:
-239.392 -1.764 (delta_t = 237.628 [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 -1.764 sec. to 2.588 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.94206 ( -0.151049 0.15735 )
Norm@50keV : 6.60436E-03 ( -0.000688309 0.000677632 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.79 using 59 PHA bins.
# Reduced chi-squared = 0.8208 for 57 degrees of freedom
# Null hypothesis probability = 8.307482e-01
Photon flux (15-150 keV) in 4.352 sec: 0.965172 ( -0.0835418 0.0835774 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.64446e-07 ( -2.6541e-08 2.69114e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.764 sec. to 2.588 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.790401 ( -0.932859 0.760304 )
Epeak [keV] : 44.1773 ( -7.41601 12.1875 )
Norm@50keV : 3.00947E-02 ( -0.0188746 0.0738189 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.51 using 59 PHA bins.
# Reduced chi-squared = 0.7056 for 56 degrees of freedom
# Null hypothesis probability = 9.534661e-01
Photon flux (15-150 keV) in 4.352 sec: 0.926457 ( -0.08711 0.087153 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.3902e-07 ( -2.88555e-08 3.06712e-08 ) ergs/cm2
Band function
Time interval is from -1.764 sec. to 2.588 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.486648 ( -0.957807 1.83857 )
beta : -2.74958 ( 2.74319 0.622363 )
Epeak [keV] : 41.5349 ( -9.8552 12.0105 )
Norm@50keV : 4.70992E-02 ( -0.0273852 0.825019 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.75 using 59 PHA bins.
# Reduced chi-squared = 0.7045 for 55 degrees of freedom
# Null hypothesis probability = 9.525571e-01
Photon flux (15-150 keV) in 4.352 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.4382e-07 ( -2.4379e-07 -2.98256e-08 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.4904 (-0.936319 1.03468)
R^2/D10^2 : 0.385874 (-0.116914 0.165748)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.45 using 59 PHA bins.
# Reduced chi-squared = 0.9201 for 57 degrees of freedom
# Null hypothesis probability = 6.462779e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.819e-08 5.512e-09
25- 50 1.014e-07 1.044e-08
50-150 6.072e-08 1.351e-08
15-150 2.004e-07 2.128e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 71.4383 (-16.3891 24.8704)
Norm : 4.74724 (-0.611765 0.716439)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.66 using 59 PHA bins.
# Reduced chi-squared = 0.7134 for 57 degrees of freedom
# Null hypothesis probability = 9.497718e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.312e-08 6.093e-09
25- 50 8.497e-08 7.572e-09
50-150 1.108e-07 2.450e-08
15-150 2.489e-07 2.748e-08
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.11392 ( )
R1^2/D10^2 : 1.10812 (-0.662514 65.4601)
kT2 [keV] : 18.6317 (-7.41335 -18.6028)
R2^2/D10^2 : 2.48894E-02 (-0.0250857 0.250107)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.14 using 59 PHA bins.
#Fit statistic : Chi-Squared = 41.09 using 59 PHA bins.
# Reduced chi-squared = 0.7479 for 55 degrees of freedom
# Reduced chi-squared = 0.7471 for 55 degrees of freedom
# Null hypothesis probability = 9.174098e-01
# Null hypothesis probability = 9.182178e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.847e-08 2.579e-08
25- 50 9.001e-08 4.578e-08
50-150 9.496e-08 5.345e-08
15-150 2.334e-07 1.201e-07
Peak spectrum fit
Power-law model
Time interval is from 0.256 sec. to 1.256 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.80949 ( -0.1971 0.206624 )
Norm@50keV : 1.06269E-02 ( -0.00144085 0.00141541 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.40 using 59 PHA bins.
# Reduced chi-squared = 1.007 for 57 degrees of freedom
# Null hypothesis probability = 4.601285e-01
Photon flux (15-150 keV) in 1 sec: 1.46979 ( -0.174961 0.175057 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.78008e-08 ( -1.33179e-08 1.35226e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.256 sec. to 1.256 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.196283 ( -1.56149 1.16142 )
Epeak [keV] : 48.6055 ( -7.87373 19.86 )
Norm@50keV : 8.44253E-02 ( -0.0844885 0.550429 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.32 using 59 PHA bins.
# Reduced chi-squared = 0.9165 for 56 degrees of freedom
# Null hypothesis probability = 6.522156e-01
Photon flux (15-150 keV) in 1 sec: 1.39419 ( -0.18437 0.18389 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.64081e-08 ( -1.38933e-08 1.53119e-08 ) ergs/cm2
Band function
Time interval is from 0.256 sec. to 1.256 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.445061 ( -1.66631 2.54999 )
beta : -2.67694 ( 2.68224 0.662276 )
Epeak [keV] : 43.6633 ( -8.51321 13.1364 )
Norm@50keV : 0.214372 ( -0.213975 7.92093 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.53 using 59 PHA bins.
# Reduced chi-squared = 0.9187 for 55 degrees of freedom
# Null hypothesis probability = 6.460187e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 8.98394e-08 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 11.4940 (-1.28321 1.46667)
R^2/D10^2 : 0.437580 (-0.159678 0.243403)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.54 using 59 PHA bins.
# Reduced chi-squared = 0.9569 for 57 degrees of freedom
# Null hypothesis probability = 5.677716e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.217e-08 2.445e-09
25- 50 3.636e-08 4.745e-09
50-150 2.804e-08 8.125e-09
15-150 7.657e-08 1.249e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 91.3688 (-28.8389 56.5802)
Norm : 6.73446 (-1.04643 1.26555)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.70 using 59 PHA bins.
# Reduced chi-squared = 0.9421 for 57 degrees of freedom
# Null hypothesis probability = 5.996282e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.758e-08 3.035e-09
25- 50 2.983e-08 4.135e-09
50-150 4.584e-08 2.072e-08
15-150 9.325e-08 2.398e-08
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.62267 (-1.43287 3.16208)
R1^2/D10^2 : 2888.01 ( )
kT2 [keV] : 12.1582 (-1.44159 2.09059)
R2^2/D10^2 : 0.342717 (-0.146825 0.212811)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.54 using 59 PHA bins.
#Fit statistic : Chi-Squared = 49.51 using 59 PHA bins.
# Reduced chi-squared = 0.9008 for 55 degrees of freedom
# Reduced chi-squared = 0.9003 for 55 degrees of freedom
# Null hypothesis probability = 6.823434e-01
# Null hypothesis probability = 6.834462e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.420e-08 3.284e-09
25- 50 3.439e-08 6.740e-09
50-150 3.058e-08 8.550e-09
15-150 7.916e-08 1.469e-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: 1.94206 ( -0.151049 0.15735 )
Norm@50keV : 6.60436E-03 ( -0.000688309 0.000677632 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.79 using 59 PHA bins.
# Reduced chi-squared = 0.8208 for 57 degrees of freedom
# Null hypothesis probability = 8.307482e-01
Photon flux (15-150 keV) in 4.352 sec: 0.965172 ( -0.0835418 0.0835774 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.64446e-07 ( -2.6541e-08 2.69114e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.790401 ( -0.932859 0.760304 )
Epeak [keV] : 44.1773 ( -7.41601 12.1875 )
Norm@50keV : 3.00947E-02 ( -0.0188746 0.0738189 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.51 using 59 PHA bins.
# Reduced chi-squared = 0.7056 for 56 degrees of freedom
# Null hypothesis probability = 9.534661e-01
Photon flux (15-150 keV) in 4.352 sec: 0.926457 ( -0.08711 0.087153 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.3902e-07 ( -2.88555e-08 3.06712e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.486648 ( -0.957807 1.83857 )
beta : -2.74958 ( 2.74319 0.622363 )
Epeak [keV] : 41.5349 ( -9.8552 12.0097 )
Norm@50keV : 4.70992E-02 ( -0.0273852 0.825019 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.75 using 59 PHA bins.
# Reduced chi-squared = 0.7045 for 55 degrees of freedom
# Null hypothesis probability = 9.525571e-01
Photon flux (15-150 keV) in 4.352 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.4382e-07 ( -2.4379e-07 -2.98256e-08 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 7.82e-08
S(50-100 keV) = 8.14e-08
T90 vs. Hardness ratio plot
T90 = 3.69999998807907 sec.
Hardness ratio (energy fluence ratio) = 1.04092
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.25876
Count Ratio (50-100 keV) / (15-25 keV) = 0.569195
Mask shadow pattern
IMX = -5.977284130399158E-01, IMY = 2.767280725799086E-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:
-239.392000 -1.764000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6432 22.0026 0.5 43.9 168.1 9.4266 24.6 0.9 Crab
142.6923 22.6297 2.3 39.5 81.9 3.4501 5.0 ------ UNKNOWN
202.1004 41.6524 2.2 52.6 7.7 2.9440 5.2 ------ UNKNOWN
158.5332 53.7991 2.2 22.5 22.0 0.8325 5.3 ------ UNKNOWN
265.8150 70.8018 2.5 49.0 -48.0 4.1061 4.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.764000 2.588000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4264 21.9655 0.0 44.1 168.4 -0.0862 -2.1 11.9 Crab
74.9994 26.9521 2.3 43.4 -178.4 0.1733 5.0 ------ UNKNOWN
69.0244 43.7153 0.6 33.4 -155.2 0.4870 18.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
674.808620 962.705100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
187.7006 -21.6691 2.7 52.7 26.1 3.6943 4.4 ------ UNKNOWN
166.5391 50.9743 2.7 25.7 172.4 0.7705 4.2 ------ UNKNOWN
209.2002 -16.7968 1.7 51.8 -0.4 2.9416 7.0 ------ UNKNOWN
181.2971 43.6406 2.9 13.8 -176.9 0.6847 4.0 ------ UNKNOWN
200.2579 40.7856 2.0 13.7 -113.8 1.0295 5.7 ------ UNKNOWN
231.0718 -7.8214 2.8 56.3 -28.6 4.0112 4.1 ------ UNKNOWN
237.1265 32.5377 2.7 41.1 -80.2 3.5576 4.3 ------ UNKNOWN
Plot creation:
Sat May 30 22:55:37 EDT 2015