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
276.6456 -86.1139 0.0066 33.0585 -110.7727 2.2709497 29.312 TRIG_00373871
Foreground time interval of the image:
-4.360 14.341 (delta_t = 18.701 [sec])
Background time interval of the image:
-239.360 -4.360 (delta_t = 235.000 [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 -4.360 sec. to 215.640 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.70162 ( -0.137286 0.139475 )
Norm@50keV : 9.97517E-04 ( -8.43549e-05 8.33689e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.87 using 59 PHA bins.
# Reduced chi-squared = 1.156 for 57 degrees of freedom
# Null hypothesis probability = 1.968378e-01
Photon flux (15-150 keV) in 220 sec: 0.132556 ( -0.0100997 0.0101051 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.03163e-06 ( -1.80248e-07 1.82532e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -4.360 sec. to 215.640 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.60794 ( -0.587853 0.523712 )
Epeak [keV] : 184.105 ( -128.086 -186.443 )
Norm@50keV : 1.12588E-03 ( -0.00018705 0.0012584 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.78 using 59 PHA bins.
# Reduced chi-squared = 1.175 for 56 degrees of freedom
# Null hypothesis probability = 1.742172e-01
Photon flux (15-150 keV) in 220 sec: 0.131997 ( -0.010566 0.005262 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.00982e-06 ( -2.24224e-07 2.00565e-07 ) ergs/cm2
Band function
Time interval is from -4.360 sec. to 215.640 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.89751 ( -13.8656 -4.89751 )
beta : -1.84260 ( -0.215963 0.16756 )
Epeak [keV] : 24.2553 ( -4.80949 3.53399 )
Norm@50keV : 130.521 ( -9.78476 509.746 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.50 using 59 PHA bins.
# Reduced chi-squared = 1.100 for 55 degrees of freedom
# Null hypothesis probability = 2.838900e-01
Photon flux (15-150 keV) in 220 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] : 11.0823 (-1.02427 1.16751)
R^2/D10^2 : 4.22692E-02 (-0.0131686 0.0185231)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 103.72 using 59 PHA bins.
# Reduced chi-squared = 1.8197 for 57 degrees of freedom
# Null hypothesis probability = 1.539367e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.390e-07 3.271e-08
25- 50 6.822e-07 6.545e-08
50-150 4.760e-07 9.471e-08
15-150 1.397e-06 1.355e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 125.202 (-37.0795 64.6516)
Norm : 0.558695 (-0.0520882 0.0650082)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.51 using 59 PHA bins.
# Reduced chi-squared = 1.167 for 57 degrees of freedom
# Null hypothesis probability = 1.821912e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.196e-07 3.564e-08
25- 50 5.758e-07 6.985e-08
50-150 1.049e-06 4.005e-07
15-150 1.944e-06 4.708e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.64419 (-1.51176 1.55144)
R1^2/D10^2 : 0.133576 (-0.0419452 0.0775689)
kT2 [keV] : 36.5535 (-22.4372 -51.7615)
R2^2/D10^2 : 4.14835E-04 (-0.000161252 0.000720566)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.18 using 59 PHA bins.
# Reduced chi-squared = 1.076 for 55 degrees of freedom
# Null hypothesis probability = 3.255460e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.163e-07 8.231e-08
25- 50 5.949e-07 1.218e-07
50-150 1.056e-06 5.435e-07
15-150 1.967e-06 7.071e-07
Peak spectrum fit
Power-law model
Time interval is from -0.360 sec. to 0.640 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.21860 ( -0.207073 0.20473 )
Norm@50keV : 1.84948E-02 ( -0.00213104 0.00212925 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.18 using 59 PHA bins.
# Reduced chi-squared = 1.179 for 57 degrees of freedom
# Null hypothesis probability = 1.676401e-01
Photon flux (15-150 keV) in 1 sec: 2.17677 ( -0.255664 0.256118 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.86667e-07 ( -2.42905e-08 2.45233e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.360 sec. to 0.640 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.21686 ( -0.237286 0.204187 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 1.85682E-02 ( -0.0185808 0.0201104 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.18 using 59 PHA bins.
# Reduced chi-squared = 1.200 for 56 degrees of freedom
# Null hypothesis probability = 1.455599e-01
Photon flux (15-150 keV) in 1 sec: 2.17738 ( -0.25851 0.25439 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.86763e-07 ( -2.5082e-08 2.4294e-08 ) ergs/cm2
Band function
Time interval is from -0.360 sec. to 0.640 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.69172 ( -4.69172 -4.69172 )
beta : -1.27685 ( -0.236773 0.226841 )
Epeak [keV] : 24.7122 ( -24.7122 9.13832 )
Norm@50keV : 973.880 ( -111.802 5.68071e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.52 using 59 PHA bins.
# Reduced chi-squared = 1.210 for 55 degrees of freedom
# Null hypothesis probability = 1.372362e-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] : 18.6066 (-3.15411 3.95162)
R^2/D10^2 : 0.123604 (-0.0568208 0.104083)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 89.33 using 59 PHA bins.
# Reduced chi-squared = 1.567 for 57 degrees of freedom
# Null hypothesis probability = 3.992897e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.474e-09 2.256e-09
25- 50 4.015e-08 7.075e-09
50-150 1.017e-07 2.251e-08
15-150 1.503e-07 2.730e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 8.93350 (-1.04685 1.04681)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.70 using 59 PHA bins.
# Reduced chi-squared = 1.311 for 57 degrees of freedom
# Null hypothesis probability = 5.783518e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.224e-08 1.244e-08
25- 50 4.279e-08 2.361e-08
50-150 9.384e-08 5.150e-08
15-150 1.589e-07 8.760e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.85000 (-2.14231 2.74329)
R1^2/D10^2 : 1.47229 (-0.90957 2.87603)
kT2 [keV] : 38.3433 (-12.1167 44.4898)
R2^2/D10^2 : 1.05288E-02 (-0.00859594 0.0240532)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.23 using 59 PHA bins.
# Reduced chi-squared = 1.186 for 55 degrees of freedom
# Null hypothesis probability = 1.627129e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.823e-08 9.794e-09
25- 50 4.124e-08 1.911e-08
50-150 1.324e-07 6.898e-08
15-150 1.919e-07 9.546e-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: 1.38868 ( -0.098089 0.0978084 )
Norm@50keV : 8.08244E-03 ( -0.000451819 0.000451117 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.85 using 59 PHA bins.
# Reduced chi-squared = 1.103 for 57 degrees of freedom
# Null hypothesis probability = 2.767610e-01
Photon flux (15-150 keV) in 18.7 sec: 0.981792 ( -0.0561788 0.0562482 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.46385e-06 ( -9.03365e-08 9.07801e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.18189 ( -0.393096 0.256258 )
Epeak [keV] : 200.134 ( -200.136 -200.136 )
Norm@50keV : 1.02669E-02 ( -0.00252105 0.00571173 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.91 using 59 PHA bins.
# Reduced chi-squared = 1.105 for 56 degrees of freedom
# Null hypothesis probability = 2.735176e-01
Photon flux (15-150 keV) in 18.7 sec: 0.972510 ( -0.058433 0.05839 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.44012e-06 ( -1.01156e-07 1.00109e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.98723 ( -14.5065 -4.98723 )
beta : -1.48880 ( -0.116714 0.113689 )
Epeak [keV] : 26.0957 ( -4.4117 3.63409 )
Norm@50keV : 592.628 ( -32.6722 1294.95 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.01 using 59 PHA bins.
# Reduced chi-squared = 1.000 for 55 degrees of freedom
# Null hypothesis probability = 4.743060e-01
Photon flux (15-150 keV) in 18.7 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) = 5.50e-07
S(50-100 keV) = 6.77e-07
T90 vs. Hardness ratio plot
T90 = 174 sec.
Hardness ratio (energy fluence ratio) = 1.23091
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.22401
Count Ratio (50-100 keV) / (15-25 keV) = 0.741587
Mask shadow pattern
IMX = -2.308345543989691E-01, IMY = 6.085509223324870E-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:
-239.360000 -4.360000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
341.6130 -10.0382 2.1 47.7 43.2 4.4151 5.5 ------ UNKNOWN
81.1869 -40.9174 2.6 54.6 174.7 3.2246 4.4 ------ UNKNOWN
102.2918 -48.0342 3.2 59.0 -166.2 4.4145 3.6 ------ UNKNOWN
239.3741 -76.3635 3.9 41.3 -99.1 3.0143 3.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-4.360000 14.340600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
26.6303 -22.8667 2.4 40.4 109.0 0.8427 4.9 ------ UNKNOWN
276.6455 -86.1139 0.4 33.1 -110.8 2.2713 29.3 ------ UNKNOWN
135.3656 -70.3241 2.3 50.0 -134.3 1.1849 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
67.940590 962.667500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5222 -40.4053 17.3 52.7 -166.4 -1.0567 -0.7 9.0 Vela X-1
170.2961 -60.6340 1.3 30.7 -136.0 5.6731 9.1 0.9 Cen X-3
186.5731 -62.7321 3.9 27.5 -120.9 1.6648 2.9 3.2 GX 301-2
255.8752 -37.8070 6.9 48.6 -45.3 4.2770 1.7 5.7 4U 1700-377
256.7221 -36.4122 8.7 50.0 -44.3 3.2917 1.3 13.9 GX 349+2
264.7131 -44.5197 7.3 41.7 -36.2 1.2819 1.6 4.4 4U 1735-44
276.0344 -30.4063 7.7 55.7 -24.0 -2.6008 -1.5 6.1 H1820-303
263.0920 -33.9157 11.1 52.3 -37.6 1.9906 1.0 7.1 GX 354-0
98.3041 -44.4136 3.0 49.5 158.2 6.3993 3.8 ------ UNKNOWN
315.7556 -39.9246 2.7 47.1 18.0 4.7697 4.2 ------ UNKNOWN
123.5801 -55.9437 2.5 37.6 -178.7 3.1163 4.7 ------ UNKNOWN
293.8888 -30.8785 3.0 55.4 -5.4 5.8539 3.8 ------ UNKNOWN
289.9354 -28.7662 3.3 57.5 -9.5 7.6639 3.5 ------ UNKNOWN
215.4213 -62.7563 3.0 25.6 -91.7 2.3990 3.9 ------ UNKNOWN
271.7431 -29.8700 3.3 56.3 -28.5 7.1551 3.5 ------ UNKNOWN
199.3474 -50.8392 4.2 38.5 -105.4 4.2161 2.8 ------ UNKNOWN
Plot creation:
Sun May 31 02:45:24 EDT 2015