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
100.8606 50.2215 0.0230 29.5329 12.1761 0.8022519 8.410 TRIG_00361830
Foreground time interval of the image:
29.520 73.301 (delta_t = 43.781 [sec])
Background time interval of the image:
-136.299 29.520 (delta_t = 165.819 [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 64.000000
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 64.000000
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 64.000000
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 29.520 sec. to 186.400 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.01042 ( -0.0941712 0.0960164 )
Norm@50keV : 2.08111E-03 ( -0.000115836 0.00011467 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.39 using 59 PHA bins.
# Reduced chi-squared = 0.8314 for 57 degrees of freedom
# Null hypothesis probability = 8.140167e-01
Photon flux (15-150 keV) in 156.9 sec: 0.313672 ( -0.0149235 0.0149553 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.0129e-06 ( -1.57466e-07 1.58918e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 29.520 sec. to 186.400 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66752 ( -0.396781 0.343916 )
Epeak [keV] : 42.3584 ( -40.1939 -42.3584 )
Norm@50keV : 3.21180E-03 ( -0.00133 0.00206074 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.74 using 59 PHA bins.
# Reduced chi-squared = 0.7990 for 56 degrees of freedom
# Null hypothesis probability = 8.600747e-01
Photon flux (15-150 keV) in 156.9 sec: 0.306515 ( -0.016571 0.016592 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.89752e-06 ( -1.95435e-07 1.97867e-07 ) ergs/cm2
Band function
Time interval is from 29.520 sec. to 186.400 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.66736 ( 1.68793 0.419946 )
beta : -10.0000 ( 10 3.55271e-15 )
Epeak [keV] : 42.3537 ( -19.8556 117.408 )
Norm@50keV : 3.21171E-03 ( -0.0011389 0.00206119 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.74 using 59 PHA bins.
# Reduced chi-squared = 0.8135 for 55 degrees of freedom
# Null hypothesis probability = 8.369202e-01
Photon flux (15-150 keV) in 156.9 sec: 0.308085 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.9147e-06 ( -2.9136e-06 -1.78458e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.2580 ( )
R^2/D10^2 : 0.124085 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 137.18 using 59 PHA bins.
# Reduced chi-squared = 2.4066 for 57 degrees of freedom
# Null hypothesis probability = 1.467673e-08
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.207e-07 3.279e-08
25- 50 1.084e-06 5.523e-08
50-150 6.086e-07 7.916e-08
15-150 2.113e-06 1.192e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 68.7805 (-10.0784 12.9375)
Norm : 1.51631 (-0.124099 0.139265)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.86 using 59 PHA bins.
# Reduced chi-squared = 0.8221 for 57 degrees of freedom
# Null hypothesis probability = 8.286922e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.092e-07 4.174e-08
25- 50 9.646e-07 4.495e-08
50-150 1.223e-06 1.456e-07
15-150 2.797e-06 1.624e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.18790 (-0.764801 0.78584)
R1^2/D10^2 : 0.648711 (-0.228606 0.414642)
kT2 [keV] : 21.4776 (-3.37687 4.79653)
R2^2/D10^2 : 5.21514E-03 (-0.00279319 0.00539922)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.81 using 59 PHA bins.
# Reduced chi-squared = 0.7603 for 55 degrees of freedom
# Null hypothesis probability = 9.048297e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.112e-07 8.857e-08
25- 50 9.441e-07 1.349e-07
50-150 1.327e-06 4.221e-07
15-150 2.882e-06 5.766e-07
Peak spectrum fit
Power-law model
Time interval is from 127.068 sec. to 128.068 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.54677 ( -0.16936 0.171591 )
Norm@50keV : 1.38580E-02 ( -0.00135999 0.00134153 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.51 using 59 PHA bins.
# Reduced chi-squared = 1.009 for 57 degrees of freedom
# Null hypothesis probability = 4.562199e-01
Photon flux (15-150 keV) in 1 sec: 1.75270 ( -0.158789 0.158909 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.30521e-07 ( -1.4126e-08 1.43464e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 127.068 sec. to 128.068 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.33063 ( -0.173334 0.169013 )
Epeak [keV] : 116.432 ( -9999.36 -9999.36 )
Norm@50keV : 5.37400E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.31 using 59 PHA bins.
# Reduced chi-squared = 1.023 for 56 degrees of freedom
# Null hypothesis probability = 4.264215e-01
Photon flux (15-150 keV) in 1 sec: 1.75380 ( -0.15986 0.15765 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.30701e-07 ( -1.4306e-08 1.3577e-08 ) ergs/cm2
Band function
Time interval is from 127.068 sec. to 128.068 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.11811 ( 1.11814 1.11814 )
beta : -1.56223 ( 1.56168 0.18294 )
Epeak [keV] : 51.9531 ( -51.8952 -51.8952 )
Norm@50keV : 2.88671E-02 ( -0.0162862 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.47 using 59 PHA bins.
# Reduced chi-squared = 1.045 for 55 degrees of freedom
# Null hypothesis probability = 3.838726e-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] : 12.6473 (-1.59519 1.94664)
R^2/D10^2 : 0.342634 (-0.136629 0.214747)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 101.84 using 59 PHA bins.
# Reduced chi-squared = 1.7867 for 57 degrees of freedom
# Null hypothesis probability = 2.428725e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.162e-08 1.991e-09
25- 50 3.884e-08 3.930e-09
50-150 3.864e-08 8.090e-09
15-150 8.910e-08 1.080e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.339 (-73.2013 -199.357)
Norm : 7.09790 (-0.64027 0.640801)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.92 using 59 PHA bins.
# Reduced chi-squared = 1.051 for 57 degrees of freedom
# Null hypothesis probability = 3.703521e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.768e-08 3.855e-09
25- 50 3.400e-08 1.781e-08
50-150 7.456e-08 3.997e-08
15-150 1.262e-07 5.359e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.22269 (-1.49505 1.69399)
R1^2/D10^2 : 1.99234 (-1.01851 2.52367)
kT2 [keV] : 40.5800 (-14.337 61.8804)
R2^2/D10^2 : 5.92982E-03 (-0.00484085 0.0159012)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.11 using 59 PHA bins.
# Reduced chi-squared = 1.020 for 55 degrees of freedom
# Null hypothesis probability = 4.329505e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.848e-08 5.202e-09
25- 50 3.359e-08 9.055e-09
50-150 8.774e-08 4.456e-08
15-150 1.398e-07 5.159e-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: 2.55443 ( -0.254683 0.279198 )
Norm@50keV : 1.00204E-03 ( -0.000218497 0.000223612 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.24 using 59 PHA bins.
# Reduced chi-squared = 1.267 for 57 degrees of freedom
# Null hypothesis probability = 8.407317e-02
Photon flux (15-150 keV) in 43.78 sec: 0.203595 ( -0.025369 0.0254027 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.45378e-07 ( -7.06627e-08 7.45512e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -2.59794 ( -3.97746 1.91573 )
Epeak [keV] : 25.4836 ( -3.6352 3.03049 )
Norm@50keV : 4.49616 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.65 using 59 PHA bins.
# Reduced chi-squared = 1.030 for 56 degrees of freedom
# Null hypothesis probability = 4.138841e-01
Photon flux (15-150 keV) in 43.78 sec: 0.193316 ( -0.024053 0.024178 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.48971e-07 ( -4.9024e-08 5.36012e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.71553 ( -4.63764 -4.71553 )
beta : -3.91314 ( -2.46425 0.794096 )
Epeak [keV] : 24.5064 ( -2.21267 2.32725 )
Norm@50keV : 210.538 ( -24.9291 536.966 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.83 using 59 PHA bins.
# Reduced chi-squared = 1.033 for 55 degrees of freedom
# Null hypothesis probability = 4.068227e-01
Photon flux (15-150 keV) in 43.78 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) = 9.10e-07
S(50-100 keV) = 9.03e-07
T90 vs. Hardness ratio plot
T90 = 129.531999945641 sec.
Hardness ratio (energy fluence ratio) = 0.992308
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.03669
Count Ratio (50-100 keV) / (15-25 keV) = 0.559659
Mask shadow pattern
IMX = 5.537870990773772E-01, IMY = -1.194910957188284E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
-136.299400 29.520000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
80.3366 30.3150 2.8 54.3 18.8 3.9463 4.1 ------ UNKNOWN
257.1442 43.3349 2.6 55.9 173.3 4.1745 4.5 ------ UNKNOWN
224.4950 68.1533 2.3 25.8 172.6 0.8282 5.0 ------ UNKNOWN
206.6799 32.4924 3.3 48.5 -135.3 2.2934 3.5 ------ UNKNOWN
208.6108 30.8783 3.3 50.6 -136.5 3.0840 3.5 ------ UNKNOWN
157.8533 27.8179 2.2 41.6 -75.0 3.4986 5.2 ------ UNKNOWN
134.5558 19.5083 2.8 50.4 -45.4 3.6560 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
29.520000 73.300580
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
266.9128 58.7308 1.9 44.6 157.5 1.1581 6.2 ------ UNKNOWN
100.8607 50.2216 1.4 29.5 12.2 0.8024 8.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
123.300600 963.040000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6249 22.0208 0.2 31.3 14.8 33.7413 48.5 0.6 Crab
247.7737 76.1908 2.7 51.8 172.3 9.2842 4.2 ------ UNKNOWN
86.9131 18.5287 2.6 33.6 7.2 3.2676 4.5 ------ UNKNOWN
220.0167 76.9054 2.4 47.3 178.4 5.4740 4.8 ------ UNKNOWN
100.8227 50.1844 1.2 0.0 64.6 5.4761 9.7 ------ UNKNOWN
92.9654 14.4587 2.5 36.3 -4.2 3.8444 4.7 ------ UNKNOWN
Plot creation:
Sun May 31 03:04:13 EDT 2015