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