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
  126.0645   -45.5334   0.0093    27.3376   -18.7203         0.9865420     20.691 TRIG_00160672                 
 
Foreground time interval of the image:
 -4.640  14.429 (delta_t =  19.069 [sec])
Background time interval of the image:
-299.472  -4.640 (delta_t = 294.832 [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   -4.640 sec. to   54.688 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.54427     ( -0.136933   0.138839 )
Norm@50keV  : 1.59861E-03    ( -0.000135145   0.00013429 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          65.55 using 59 PHA bins.
# Reduced chi-squared =          1.150 for     57 degrees of freedom 
# Null hypothesis probability =   2.043782e-01
 
Photon flux (15-150 keV)    in 59.33 sec: 0.202041 ( -0.0163457  0.0163589 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.93617e-07 ( -8.21762e-08  8.31018e-08 ) ergs/cm2
 
Cutoff power-law model
 
Time interval is from   -4.640 sec. to   54.688 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.482353     ( -0.727364   0.627235 )
Epeak [keV] : 68.6830      ( -11.7264 31.8206 )
Norm@50keV  : 5.65973E-03    ( -0.00292854   0.00745013 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.44 using 59 PHA bins.
# Reduced chi-squared =          1.008 for     56 degrees of freedom 
# Null hypothesis probability =   4.585278e-01
 
Photon flux (15-150 keV)    in 59.33 sec: 0.192492 ( -0.01725  0.017239 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.19424e-07 ( -8.86568e-08  9.18962e-08 ) ergs/cm2
 
Band function
 
Time interval is from   -4.640 sec. to   54.688 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.482277   ( -0.527892   0.647923 )
beta        : -10.00000    ( 10   20 )
Epeak [keV] : 68.6688      ( -10.1962 31.8202 )
Norm@50keV   : 5.66048E-03    ( -0.0029301   0.00747457 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          56.44 using 59 PHA bins.
# Reduced chi-squared =          1.026 for     55 degrees of freedom 
# Null hypothesis probability =   4.210157e-01
 
Photon flux (15-150 keV)    in 59.33 sec: 0.192489 (    ) 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]    : 14.4113  (-1.26589  1.39932)
R^2/D10^2   : 2.67462E-02  (-0.00750612   0.0103274)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          71.46 using 59 PHA bins.
# Reduced chi-squared =          1.254 for     57 degrees of freedom 
# Null hypothesis probability =   9.417439e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.940e-08   1.023e-08
25- 50  2.655e-07   2.978e-08
50-150  3.684e-07   6.247e-08
15-150  7.033e-07   7.327e-08
Thermal bremsstrahlung (OTTB)
 
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 179.131       (-58.8038      -181.331)
Norm        : 0.828841       (-0.0693593     0.0742044)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.81 using 59 PHA bins.
# Reduced chi-squared =          1.067 for     57 degrees of freedom 
# Null hypothesis probability =   3.403406e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.241e-07   4.401e-08
25- 50  2.356e-07   1.086e-07
50-150  4.980e-07   2.691e-07
15-150  8.577e-07   4.536e-07
Double BB
 
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.01459        (-1.66561      2.22618)
R1^2/D10^2  : 0.488726        (-0.356817      2.32697)
kT2 [keV]   : 17.8063        (-2.349      3.57994)
R2^2/D10^2  : 1.10965E-02    (-0.00586235   0.00742702)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.00 using 59 PHA bins.
# Reduced chi-squared =         0.9819 for     55 degrees of freedom 
# Null hypothesis probability =   5.127248e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.133e-07   5.208e-08
25- 50  2.393e-07   7.063e-08
50-150  4.434e-07   1.315e-07
15-150  7.960e-07   2.038e-07
Peak spectrum fit
Power-law model
 
Time interval is from   -0.668 sec. to    0.332 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.37775     ( -0.319025   0.32154 )
Norm@50keV  : 6.21292E-03    ( -0.00112154   0.00111115 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.03 using 59 PHA bins.
# Reduced chi-squared =          1.193 for     57 degrees of freedom 
# Null hypothesis probability =   1.504498e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.752884 ( -0.134003  0.13422 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.03131e-08 ( -1.22026e-08  1.24182e-08 ) ergs/cm2
 
Cutoff power-law model
 
Time interval is from   -0.668 sec. to    0.332 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.38734     ( -0.8341   0.316006 )
Epeak [keV] : 9999.36      ( -9999.36 -9999.36 )
Norm@50keV  : 6.19495E-03    ( -0.00111644   0.0249559 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.04 using 59 PHA bins.
# Reduced chi-squared =          1.215 for     56 degrees of freedom 
# Null hypothesis probability =   1.298937e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.753644 ( -0.135142  0.133236 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.01473e-08 ( -1.28464e-08  1.24441e-08 ) ergs/cm2
 
Band function
 
Time interval is from   -0.668 sec. to    0.332 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -1.11418   ( 1.11545   5.35453 )
beta        : -1.48320    ( 1.47498   0.416464 )
Epeak [keV] : 150.180      ( -165.987 -165.987 )
Norm@50keV   : 8.58609E-03    ( -0.00309819   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.04 using 59 PHA bins.
# Reduced chi-squared =          1.237 for     55 degrees of freedom 
# Null hypothesis probability =   1.114530e-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]    : 15.1931  (-2.88619  3.93536)
R^2/D10^2   : 8.37136E-02  (-0.046086   0.0899309)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          74.48 using 59 PHA bins.
# Reduced chi-squared =          1.307 for     57 degrees of freedom 
# Null hypothesis probability =   5.992593e-02
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.037e-09   1.335e-09
25- 50  1.623e-08   5.143e-09
50-150  2.564e-08   9.670e-09
15-150  4.590e-08   1.259e-08
Thermal bremsstrahlung (OTTB)
 
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (-85.0243      -199.363)
Norm        : 3.08844       (-0.54544     0.545435)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          69.16 using 59 PHA bins.
# Reduced chi-squared =          1.213 for     57 degrees of freedom 
# Null hypothesis probability =   1.295597e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.691e-09   4.474e-09
25- 50  1.479e-08   8.525e-09
50-150  3.244e-08   1.831e-08
15-150  5.493e-08   3.173e-08
Double BB
 
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 2.24426        (-1.14382      2.77782)
R1^2/D10^2  : 148.628        (-153.334      133562)
kT2 [keV]   : 17.2966        (-3.67084      5.96814)
R2^2/D10^2  : 5.07020E-02    (-0.032576   0.057556)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          68.18 using 59 PHA bins.
# Reduced chi-squared =          1.240 for     55 degrees of freedom 
# Null hypothesis probability =   1.092067e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.660e-09   2.960e-09
25- 50  1.396e-08   6.226e-09
50-150  2.961e-08   1.257e-08
15-150  5.023e-08   2.071e-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: 1.27714     ( -0.127549   0.126414 )
Norm@50keV  : 3.40351E-03    ( -0.000249488   0.000249356 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.06 using 59 PHA bins.
# Reduced chi-squared =         0.9309 for     57 degrees of freedom 
# Null hypothesis probability =   6.235303e-01
 
Photon flux (15-150 keV)    in 19.07 sec: 0.404385 ( -0.0303744  0.0304198 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.45029e-07 ( -5.25855e-08  5.29286e-08 ) ergs/cm2
 
Cutoff power-law model
 
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.864713     ( -0.57281   0.466124 )
Epeak [keV] : 141.792      ( -54.8509 -141.8 )
Norm@50keV  : 5.44031E-03    ( -0.00215479   0.00476646 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          51.14 using 59 PHA bins.
# Reduced chi-squared =         0.9133 for     56 degrees of freedom 
# Null hypothesis probability =   6.589128e-01
 
Photon flux (15-150 keV)    in 19.07 sec: 0.397232 ( -0.031797  0.031671 ) ph/cm2/s
Energy fluence (15-150 keV)             : 6.25122e-07 ( -5.90197e-08  5.86479e-08 ) ergs/cm2
 
Band function
 
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.96879   ( -0.083685   -4.96879 )
beta        : -1.38944    ( -0.153648   0.148982 )
Epeak [keV] : 27.2833      ( -5.24916 4.22858 )
Norm@50keV   : 170.884    ( -12.4324   479.13 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          47.87 using 59 PHA bins.
# Reduced chi-squared =         0.8704 for     55 degrees of freedom 
# Null hypothesis probability =   7.412524e-01
 
Photon flux (15-150 keV)    in 19.07 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)  = 2.26e-07
S(50-100 keV) = 3.10e-07
 T90 vs. Hardness ratio plot 
 
T90                                   = 46.5119999647141 sec.
Hardness ratio (energy fluence ratio) = 1.37168
 Color vs. Color plot 
 
Count Ratio  (25-50 keV) / (15-25 keV) = 1.42273
Count Ratio (50-100 keV) / (15-25 keV) = 1.13245
 Mask shadow pattern 
 
IMX = 4.896213709906972E-01, IMY = 1.659209379960770E-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:
-299.472000 -4.640000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.5655 -40.5436    4.9  24.8  -37.4   0.4747   2.4    1.8	Vela X-1                      
108.4566 -75.3176    2.6  57.5   -9.5   4.6938   4.4 ------	UNKNOWN                       
146.2396  10.1688    3.1  36.7 -152.9   0.9414   3.8 ------	UNKNOWN                       
131.7479 -74.5552    3.5  56.4  -16.6   2.6311   3.3 ------	UNKNOWN                       
137.4659 -72.2597    3.7  54.6  -19.2   2.0894   3.1 ------	UNKNOWN                       
148.9214 -31.8150    2.6  27.1  -68.9   1.0282   4.4 ------	UNKNOWN                       
152.7146  17.8181    3.8  46.6 -153.0   1.2187   3.0 ------	UNKNOWN                       
 Pre-slew background subtracted image of 15-350 keV band 
Time interval of the image:
-4.640000 14.428600
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.6077 -40.6528    6.6  24.9  -37.3  -0.0806  -1.8    6.9	Vela X-1                      
139.6703  24.8137    2.2  46.2 -172.4   0.4223   5.3 ------	UNKNOWN                       
126.0645 -45.5334    0.6  27.3  -18.7   0.9865  20.7 ------	UNKNOWN                       
138.9544 -51.0982    2.7  35.2  -31.4   0.2352   4.4 ------	UNKNOWN                       
129.0326 -75.3728    2.2  57.1  -15.6   1.1499   5.2 ------	UNKNOWN                       
 Post-slew image of 15-350 keV band 
Time interval of the image:
64.428610 302.541000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
135.3137 -40.4195    0.0   8.5 -124.8  -0.0756  -0.5   12.7	Vela X-1                      
169.9424 -60.5907    0.0  29.6  -44.7  -0.1672  -0.8   11.2	Cen X-3                       
186.5604 -62.8530    8.4  37.6  -41.8   0.3526   1.4    5.6	GX 301-2                      
115.5094   5.7750    2.7  52.2  165.6   2.6459   4.3 ------	UNKNOWN                       
196.5880 -78.8444    2.3  41.8  -17.0   1.2467   5.1 ------	UNKNOWN                       
Plot creation:
Sun May 31 15:18:41 EDT 2015