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
117.7130 -0.6440 0.0107 35.1914 177.4639 1.2499684 17.896 TRIG_00371050
Foreground time interval of the image:
-9.784 10.317 (delta_t = 20.101 [sec])
Background time interval of the image:
-239.384 -9.784 (delta_t = 229.600 [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 0.256000
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 0.256000
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 0.256000
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 -9.784 sec. to 370.900 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.81146 ( -0.0835448 0.0846202 )
Norm@50keV : 1.65979E-03 ( -7.57546e-05 7.5212e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.06 using 59 PHA bins.
# Reduced chi-squared = 0.9484 for 57 degrees of freedom
# Null hypothesis probability = 5.860944e-01
Photon flux (15-150 keV) in 380.7 sec: 0.229739 ( -0.00976552 0.00980036 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.81493e-06 ( -2.70259e-07 2.72421e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -9.784 sec. to 370.900 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.63939 ( -0.342516 0.239208 )
Epeak [keV] : 98.1065 ( -42.1936 -98.1065 )
Norm@50keV : 2.04064E-03 ( -0.000442327 0.00101317 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.22 using 59 PHA bins.
# Reduced chi-squared = 0.9504 for 56 degrees of freedom
# Null hypothesis probability = 5.806394e-01
Photon flux (15-150 keV) in 380.7 sec: 0.226746 ( -0.011133 0.005426 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.70487e-06 ( -3.38937e-07 3.38823e-07 ) ergs/cm2
Band function
Time interval is from -9.784 sec. to 370.900 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.50086 ( 1.50802 1.50802 )
beta : -1.91527 ( 1.9145 0.172295 )
Epeak [keV] : 65.7878 ( -67.8726 -67.8726 )
Norm@50keV : 2.48277E-03 ( -0.000775249 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.22 using 59 PHA bins.
# Reduced chi-squared = 0.9676 for 55 degrees of freedom
# Null hypothesis probability = 5.430776e-01
Photon flux (15-150 keV) in 380.7 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] : 12.1667 ( )
R^2/D10^2 : 4.90812E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 174.35 using 59 PHA bins.
# Reduced chi-squared = 3.0588 for 57 degrees of freedom
# Null hypothesis probability = 8.005290e-14
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.856e-07 4.169e-08
25- 50 1.873e-06 9.308e-08
50-150 1.682e-06 1.749e-07
15-150 4.141e-06 1.980e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 107.092 (-19.3557 21.2346)
Norm : 0.972179 (-0.0555279 0.0734795)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.13 using 59 PHA bins.
# Reduced chi-squared = 0.9848 for 57 degrees of freedom
# Null hypothesis probability = 5.076677e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.670e-07 7.976e-08
25- 50 1.695e-06 9.099e-08
50-150 2.852e-06 7.547e-07
15-150 5.514e-06 7.900e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.00155 (-1.03201 1.14782)
R1^2/D10^2 : 0.460826 (-0.207641 0.48768)
kT2 [keV] : 21.3417 (-3.24495 5.0386)
R2^2/D10^2 : 4.83886E-03 (-0.00262573 0.00438318)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.40 using 59 PHA bins.
# Reduced chi-squared = 1.116 for 55 degrees of freedom
# Null hypothesis probability = 2.574002e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.974e-07 1.498e-07
25- 50 1.655e-06 1.765e-07
50-150 2.854e-06 5.349e-07
15-150 5.507e-06 6.967e-07
Peak spectrum fit
Power-law model
Time interval is from 30.672 sec. to 31.672 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.927844 ( -0.10859 0.106502 )
Norm@50keV : 2.81702E-02 ( -0.00176276 0.00175641 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.37 using 59 PHA bins.
# Reduced chi-squared = 0.9012 for 57 degrees of freedom
# Null hypothesis probability = 6.854688e-01
Photon flux (15-150 keV) in 1 sec: 3.23466 ( -0.203224 0.203318 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.12783e-07 ( -2.12524e-08 2.13283e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 30.672 sec. to 31.672 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.608761 ( -0.450157 0.361493 )
Epeak [keV] : 246.375 ( )
Norm@50keV : 3.93676E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.60 using 59 PHA bins.
# Reduced chi-squared = 0.8858 for 56 degrees of freedom
# Null hypothesis probability = 7.140665e-01
Photon flux (15-150 keV) in 1 sec: 3.19887 ( -0.20844 0.20837 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.07647e-07 ( -2.2783e-08 2.2572e-08 ) ergs/cm2
Band function
Time interval is from 30.672 sec. to 31.672 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.99998 ( -0.000234386 -4.99998 )
beta : -1.05492 ( -0.133254 0.130658 )
Epeak [keV] : 32.5489 ( -6.91222 4.94771 )
Norm@50keV : 409.005 ( -25.012 1167.41 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.90 using 59 PHA bins.
# Reduced chi-squared = 0.8345 for 55 degrees of freedom
# Null hypothesis probability = 8.040762e-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] : 22.3381 (-1.90405 2.16013)
R^2/D10^2 : 0.112262 (-0.0278814 0.0359504)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 86.92 using 59 PHA bins.
# Reduced chi-squared = 1.525 for 57 degrees of freedom
# Null hypothesis probability = 6.520442e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.029e-08 1.218e-09
25- 50 5.492e-08 5.400e-09
50-150 2.048e-07 2.115e-08
15-150 2.700e-07 2.020e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 12.7715 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 137.73 using 59 PHA bins.
# Reduced chi-squared = 2.4162 for 57 degrees of freedom
# Null hypothesis probability = 1.241876e-08
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.180e-08 2.240e-09
25- 50 6.118e-08 6.070e-09
50-150 1.342e-07 4.511e-08
15-150 2.271e-07 3.850e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.3065 (-2.23469 2.75299)
R1^2/D10^2 : 0.712721 (-0.319484 0.659782)
kT2 [keV] : 43.1276 (-11.2141 37.3622)
R2^2/D10^2 : 1.25346E-02 (-0.00969396 0.0182432)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.49 using 59 PHA bins.
# Reduced chi-squared = 0.8271 for 55 degrees of freedom
# Null hypothesis probability = 8.160382e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.841e-08 5.878e-09
25- 50 6.021e-08 2.035e-08
50-150 2.303e-07 1.060e-07
15-150 3.090e-07 1.235e-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: 1.56137 ( -0.151959 0.154461 )
Norm@50keV : 4.08083E-03 ( -0.000372311 0.000368755 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.76 using 59 PHA bins.
# Reduced chi-squared = 0.9081 for 57 degrees of freedom
# Null hypothesis probability = 6.712322e-01
Photon flux (15-150 keV) in 20.1 sec: 0.518326 ( -0.0441762 0.0442025 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.7096e-07 ( -7.68043e-08 7.79138e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.05343 ( -0.719719 0.600486 )
Epeak [keV] : 87.7451 ( -27.6238 -87.7451 )
Norm@50keV : 7.56519E-03 ( -0.00367136 0.0102756 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.80 using 59 PHA bins.
# Reduced chi-squared = 0.8893 for 56 degrees of freedom
# Null hypothesis probability = 7.072497e-01
Photon flux (15-150 keV) in 20.1 sec: 0.505284 ( -0.047111 0.046871 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.32806e-07 ( -8.88139e-08 9.03776e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.974201 ( 0.974142 5.87601 )
beta : -2.01197 ( 1.99525 0.511259 )
Epeak [keV] : 79.2956 ( -78.8492 -78.8492 )
Norm@50keV : 8.45329E-03 ( -0.00446473 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.71 using 59 PHA bins.
# Reduced chi-squared = 0.9039 for 55 degrees of freedom
# Null hypothesis probability = 6.762045e-01
Photon flux (15-150 keV) in 20.1 sec: 0.504936 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 7.35441e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.64e-06
S(50-100 keV) = 1.87e-06
T90 vs. Hardness ratio plot
T90 = 357.3599999547 sec.
Hardness ratio (energy fluence ratio) = 1.14024
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.12162
Count Ratio (50-100 keV) / (15-25 keV) = 0.685611
Mask shadow pattern
IMX = -7.045059061514984E-01, IMY = -3.120472534188393E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
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:
-239.384000 -9.784000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5256 -40.5440 0.9 9.2 32.3 2.6433 13.1 0.7 Vela X-1
170.6282 -60.5797 26.0 37.1 2.7 -0.1385 -0.4 9.6 Cen X-3
186.6437 -62.8139 3.2 44.8 0.2 1.4130 3.6 2.6 GX 301-2
114.8414 23.6798 3.7 58.6 -172.4 3.8817 3.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-9.784000 10.316600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5579 -40.4923 3.1 9.2 32.2 -0.1987 -3.7 4.0 Vela X-1
170.4466 -60.7951 7.5 37.1 3.1 -0.1188 -1.5 11.0 Cen X-3
186.8838 -62.9159 355.2 44.9 0.3 0.0030 0.0 10.7 GX 301-2
90.6696 -5.0448 2.1 49.9 142.6 1.5065 5.6 ------ UNKNOWN
117.7130 -0.6440 0.6 35.2 177.5 1.2500 17.9 ------ UNKNOWN
121.2575 -3.4014 2.7 31.2 -179.0 0.2552 4.2 ------ UNKNOWN
200.5339 -53.0743 2.2 50.5 -14.3 0.6022 5.2 ------ UNKNOWN
203.3233 -49.7449 2.9 52.5 -18.4 0.5464 4.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
72.516600 191.516620
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5986 21.9765 11.5 40.2 124.1 0.4061 1.0 3.0 Crab
135.6917 -40.3856 0.0 43.0 -22.5 0.6685 3.1 12.6 Vela X-1
100.5055 -50.5249 2.2 52.0 11.5 2.3573 5.4 ------ UNKNOWN
107.7151 -6.8862 2.4 11.7 55.4 0.6040 4.9 ------ UNKNOWN
117.7040 -0.6437 1.2 0.0 -96.1 1.2430 9.4 ------ UNKNOWN
154.9189 -5.1928 3.0 37.5 -84.6 1.4973 3.9 ------ UNKNOWN
Plot creation:
Sun May 31 02:52:53 EDT 2015