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Image
Pre-slew 15.0-350.0 keV image (Event data)
 
#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  134.1643    47.0096   0.0086    33.9982    41.1004         3.6740091     22.637 TRIG_00441676                 
 
Foreground time interval of the image:
-30.448  23.504 (delta_t =  53.952 [sec])
Background time interval of the image:
-239.552 -30.448 (delta_t = 209.104 [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)
 
 The mask-weighted light curves based on cleaned DPHs 
 
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  -30.448 sec. to   23.504 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.81923     ( -0.121751   0.12416 )
Norm@50keV  : 4.12901E-03    ( -0.00030681   0.000303348 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          36.48 using 59 PHA bins.
# Reduced chi-squared =         0.6399 for     57 degrees of freedom 
# Null hypothesis probability =   9.843703e-01
 
Photon flux (15-150 keV)    in 53.95 sec: 0.573265 ( -0.0385872  0.0386316 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.04951e-06 ( -1.53863e-07  1.5522e-07 ) ergs/cm2
 
Cutoff power-law model
 
Time interval is from  -30.448 sec. to   23.504 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.67389     ( -0.494908   0.458669 )
Epeak [keV] : 101.992      (   )
Norm@50keV  : 4.95494E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          36.18 using 59 PHA bins.
# Reduced chi-squared =         0.6460 for     56 degrees of freedom 
# Null hypothesis probability =   9.816938e-01
 
Photon flux (15-150 keV)    in 53.95 sec: 0.569192 ( -0.040496  0.040019 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.02105e-06 ( -1.79287e-07  1.75186e-07 ) ergs/cm2
 
Band function
 
Time interval is from  -30.448 sec. to   23.504 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.90832   ( -4.90832   -4.90832 )
beta        : -1.87816    ( -0.164485   0.134747 )
Epeak [keV] : 21.4529      ( -21.4529 3.80718 )
Norm@50keV   : 1292.24    ( -84.7912   3.37044e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          34.53 using 59 PHA bins.
# Reduced chi-squared =         0.6278 for     55 degrees of freedom 
# Null hypothesis probability =   9.860904e-01
 
Photon flux (15-150 keV)    in 53.95 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.00671e-06 ( -2.00634e-06  -1.66889e-07 ) ergs/cm2
 
Single BB
 
 
Spectral model blackbody:
------------------------------------------------------------
Parameters  : value    Lower 90%  Upper 90%
kT [keV]    : 11.2551  (-0.962491  1.07518)
R^2/D10^2   : 0.168514  (-0.0489362   0.0678616)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          94.57 using 59 PHA bins.
# Reduced chi-squared =          1.659 for     57 degrees of freedom 
# Null hypothesis probability =   1.301034e-03
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.416e-07   2.986e-08
25- 50  7.035e-07   5.719e-08
50-150  5.122e-07   8.395e-08
15-150  1.457e-06   1.122e-07
Thermal bremsstrahlung (OTTB)
 
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 99.1095       (-22.3852      34.7628)
Norm        : 2.51725       (-0.239122     0.276448)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          37.72 using 59 PHA bins.
# Reduced chi-squared =         0.6618 for     57 degrees of freedom 
# Null hypothesis probability =   9.771292e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.549e-07   4.262e-08
25- 50  6.127e-07   4.478e-08
50-150  9.878e-07   3.143e-07
15-150  1.955e-06   3.377e-07
Double BB
 
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 6.93160        (-1.12243      1.17499)
R1^2/D10^2  : 0.788500        (-0.328063      0.678824)
kT2 [keV]   : 27.4850        (-6.57231      13.2404)
R2^2/D10^2  : 4.52483E-03    (-0.00324913   0.0079081)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          34.75 using 59 PHA bins.
# Reduced chi-squared =         0.6317 for     55 degrees of freedom 
# Null hypothesis probability =   9.850580e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.554e-07   6.881e-08
25- 50  6.171e-07   1.033e-07
50-150  1.061e-06   5.256e-07
15-150  2.034e-06   6.150e-07
Peak spectrum fit
Power-law model
 
Time interval is from    4.884 sec. to    5.884 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.54452     ( -0.224066   0.229837 )
Norm@50keV  : 1.62806E-02    ( -0.00228795   0.00226987 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          43.06 using 59 PHA bins.
# Reduced chi-squared =         0.7554 for     57 degrees of freedom 
# Null hypothesis probability =   9.141939e-01
 
Photon flux (15-150 keV)    in 1 sec: 2.05777 ( -0.283768  0.284295 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.53388e-07 ( -2.31108e-08  2.3367e-08 ) ergs/cm2
 
Cutoff power-law model
 
Time interval is from    4.884 sec. to    5.884 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.515736     ( -1.30697   1.01959 )
Epeak [keV] : 72.9581      ( -18.1849 593.213 )
Norm@50keV  : 5.31937E-02    ( -0.0531939   0.175117 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          40.12 using 59 PHA bins.
# Reduced chi-squared =         0.7164 for     56 degrees of freedom 
# Null hypothesis probability =   9.460144e-01
 
Photon flux (15-150 keV)    in 1 sec: 1.97664 ( -0.298  0.29684 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.44751e-07 ( -2.4447e-08  2.5038e-08 ) ergs/cm2
 
Band function
 
Time interval is from    4.884 sec. to    5.884 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.663766   ( -0.628066   2.40445 )
beta        : -2.96808    ( 2.89578   12.7804 )
Epeak [keV] : 77.1770      ( -25.071 481.935 )
Norm@50keV   : 4.47678E-02    ( -0.0326159   0.0960821 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          40.17 using 59 PHA bins.
# Reduced chi-squared =         0.7303 for     55 degrees of freedom 
# Null hypothesis probability =   9.333142e-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]    : 15.0578  (-2.12226  2.48693)
R^2/D10^2   : 0.238290  (-0.100364   0.169498)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          45.55 using 59 PHA bins.
# Reduced chi-squared =         0.7992 for     57 degrees of freedom 
# Null hypothesis probability =   8.621839e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.130e-08   3.063e-09
25- 50  4.508e-08   8.280e-09
50-150  6.968e-08   1.835e-08
15-150  1.261e-07   2.318e-08
Thermal bremsstrahlung (OTTB)
 
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 198.753       (-93.6125      -198.705)
Norm        : 8.44815       (-1.13806     1.32437)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          41.51 using 59 PHA bins.
# Reduced chi-squared =         0.7283 for     57 degrees of freedom 
# Null hypothesis probability =   9.386503e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.105e-08   1.194e-08
25- 50  4.047e-08   2.248e-08
50-150  8.866e-08   4.827e-08
15-150  1.502e-07   8.200e-08
Double BB
 
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 2.42699        (-1.48142      5.95953)
R1^2/D10^2  : 218.364        (-218.826      1.48261e+06)
kT2 [keV]   : 16.5548        (-2.58301      5.797)
R2^2/D10^2  : 0.162554    (-0.113916   0.141768)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          38.52 using 59 PHA bins.
# Reduced chi-squared =         0.7004 for     55 degrees of freedom 
# Null hypothesis probability =   9.551997e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.877e-08   8.047e-09
25- 50  4.019e-08   1.172e-08
50-150  7.674e-08   2.493e-08
15-150  1.357e-07   3.520e-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: 1.81923     ( -0.121751   0.12416 )
Norm@50keV  : 4.12901E-03    ( -0.00030681   0.000303348 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          36.48 using 59 PHA bins.
# Reduced chi-squared =         0.6399 for     57 degrees of freedom 
# Null hypothesis probability =   9.843703e-01
 
Photon flux (15-150 keV)    in 53.95 sec: 0.573265 ( -0.0385872  0.0386316 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.04951e-06 ( -1.53863e-07  1.5522e-07 ) ergs/cm2
 
Cutoff power-law model
 
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.67389     ( -0.494908   0.458669 )
Epeak [keV] : 101.992      (   )
Norm@50keV  : 4.95494E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          36.18 using 59 PHA bins.
# Reduced chi-squared =         0.6460 for     56 degrees of freedom 
# Null hypothesis probability =   9.816938e-01
 
Photon flux (15-150 keV)    in 53.95 sec: 0.569192 ( -0.040496  0.040019 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.02105e-06 ( -1.79287e-07  1.75186e-07 ) ergs/cm2
 
Band function
 
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 4.90832   ( -4.90832   -4.90832 )
beta        : -1.87816    ( -0.164485   0.134747 )
Epeak [keV] : 21.4529      ( -21.4529 3.80718 )
Norm@50keV   : 1292.24    ( -84.7912   3.36807e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          34.53 using 59 PHA bins.
# Reduced chi-squared =         0.6278 for     55 degrees of freedom 
# Null hypothesis probability =   9.860904e-01
 
Photon flux (15-150 keV)    in 53.95 sec:  (    ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.00671e-06 ( -2.00634e-06  -1.66889e-07 ) ergs/cm2
 
 S(25-50 keV) vs. S(50-100 keV) plot 
 
S(25-50 keV)  = 5.81e-07
S(50-100 keV) = 6.59e-07
 T90 vs. Hardness ratio plot 
 
T90                                   = 43.4240000247955 sec.
Hardness ratio (energy fluence ratio) = 1.13425
 Color vs. Color plot 
 
Count Ratio  (25-50 keV) / (15-25 keV) = 1.122
Count Ratio (50-100 keV) / (15-25 keV) = 0.670305
 Mask shadow pattern 
 
IMX = 5.082475128329527E-01, IMY = -4.433787700491502E-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:
-239.552000 -30.448000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6171  22.0250    1.3  42.3  121.5   7.3969   8.8    1.1	Crab                          
175.9834  57.2168    3.0  43.2   -0.6   1.1909   3.8 ------	UNKNOWN                       
  1.7665  64.9856    3.0  31.2 -105.3   1.1238   3.9 ------	UNKNOWN                       
 14.9817  33.0182    2.3  49.5 -149.2   2.2151   4.9 ------	UNKNOWN                       
  5.4808  55.4289    2.7  35.9 -120.8   1.4283   4.2 ------	UNKNOWN                       
297.4949  74.5261    2.5  39.1  -67.6   2.3857   4.6 ------	UNKNOWN                       
260.3759  68.8553    3.3  47.0  -53.0   3.1610   3.5 ------	UNKNOWN                       
334.2954  63.6296    2.3  40.8  -93.4   4.3307   5.1 ------	UNKNOWN                       
353.2903  50.7439    2.2  44.2 -117.2   4.1705   5.3 ------	UNKNOWN                       
 Pre-slew background subtracted image of 15-350 keV band 
Time interval of the image:
-30.448000 23.504000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.8526  21.9739    7.2  42.3  121.2  -0.6408  -1.6   12.4	Crab                          
134.1641  47.0094    0.5  34.0   41.1   3.6728  22.6 ------	UNKNOWN                       
 Post-slew image of 15-350 keV band 
Time interval of the image:
310.548600 962.535200
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 65.1235  38.1312    2.4  50.0  146.3  10.5450   4.9 ------	UNKNOWN                       
146.7446  -4.0500    2.6  52.2   24.0   8.2959   4.4 ------	UNKNOWN                       
180.4881   2.8160    3.2  59.6  -17.0  10.4237   3.6 ------	UNKNOWN                       
  0.7692  70.3030    5.1  58.0 -156.9   6.4668   2.3 ------	UNKNOWN                       
193.3434  31.5342    4.2  47.1  -53.0   6.7308   2.7 ------	UNKNOWN                       
191.6284  21.9902    3.8  52.1  -42.1   8.2307   3.1 ------	UNKNOWN                       
Plot creation:
Sat May 30 23:12:04 EDT 2015