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Image
Pre-slew 15.0-350.0 keV image (Event data)
 
#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  119.6655    32.8565   0.0026    15.0644   -63.2484         3.4454502     74.426 TRIG_00294835                 
 
Foreground time interval of the image:
 -3.052   7.532 (delta_t =  10.584 [sec])
Background time interval of the image:
-239.248  -3.052 (delta_t = 236.196 [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 0.512000
 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 0.512000
 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 0.512000
 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   -3.052 sec. to    7.532 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.08201     ( -0.0426832   0.0425053 )
Norm@50keV  : 2.10697E-02    ( -0.000479065   0.000477953 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          32.74 using 59 PHA bins.
# Reduced chi-squared =         0.5744 for     57 degrees of freedom 
# Null hypothesis probability =   9.959144e-01
 
Photon flux (15-150 keV)    in 10.58 sec: 2.44016 ( -0.0586126  0.0581387 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.34421e-06 ( -5.49755e-08  5.50319e-08 ) ergs/cm2
 
Cutoff power-law model
 
Time interval is from   -3.052 sec. to    7.532 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.02224     ( -0.158315   0.075213 )
Epeak [keV] : 990.275      ( -994.013 -994.013 )
Norm@50keV  : 2.23154E-02    ( -0.000497796   0.00355428 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          32.53 using 59 PHA bins.
# Reduced chi-squared =         0.5808 for     56 degrees of freedom 
# Null hypothesis probability =   9.949287e-01
 
Photon flux (15-150 keV)    in 10.58 sec: 2.43707 ( -0.05664  0.06 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.33904e-06 ( -5.68358e-08  5.92374e-08 ) ergs/cm2
 
Band function
 
Time interval is from   -3.052 sec. to    7.532 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.725949   ( 0.722667   0.722667 )
beta        : -1.10680    ( 1.10849   0.0610276 )
Epeak [keV] : 136.519      ( -145.448 325.782 )
Norm@50keV   : 3.36989E-02    ( -0.0117823   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          31.81 using 59 PHA bins.
# Reduced chi-squared =         0.5784 for     55 degrees of freedom 
# Null hypothesis probability =   9.948376e-01
 
Photon flux (15-150 keV)    in 10.58 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]    : 22.4138  (  )
R^2/D10^2   : 7.89054E-02  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         370.07 using 59 PHA bins.
# Reduced chi-squared =         6.4924 for     57 degrees of freedom 
# Null hypothesis probability =   2.001963e-47
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  7.695e-08   3.486e-09
25- 50  4.114e-07   1.481e-08
50-150  1.544e-06   5.449e-08
15-150  2.033e-06   5.449e-08
Thermal bremsstrahlung (OTTB)
 
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (      )
Norm        : 10.4217       (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         404.88 using 59 PHA bins.
# Reduced chi-squared =         7.1031 for     57 degrees of freedom 
# Null hypothesis probability =   6.449534e-54
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.746e-07   6.771e-09
25- 50  5.282e-07   1.386e-08
50-150  1.158e-06   2.751e-08
15-150  1.961e-06   5.290e-08
Double BB
 
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 9.09479        (-0.952826      1.04577)
R1^2/D10^2  : 0.807192        (-0.219391      0.329401)
kT2 [keV]   : 38.1662        (-3.88888      5.56976)
R2^2/D10^2  : 1.27515E-02    (-0.00430666   0.00516767)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          41.43 using 59 PHA bins.
# Reduced chi-squared =         0.7532 for     55 degrees of freedom 
# Null hypothesis probability =   9.121743e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  1.645e-07   1.370e-08
25- 50  4.750e-07   2.645e-08
50-150  1.706e-06   1.090e-07
15-150  2.346e-06   1.296e-07
Peak spectrum fit
Power-law model
 
Time interval is from   -0.356 sec. to    0.644 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.767647     ( -0.0526889   0.0522742 )
Norm@50keV  : 7.31767E-02    ( -0.00216072   0.00215139 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          35.82 using 59 PHA bins.
# Reduced chi-squared =         0.6283 for     57 degrees of freedom 
# Null hypothesis probability =   9.873832e-01
 
Photon flux (15-150 keV)    in 1 sec: 8.42190 ( -0.242212  0.242318 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.66985e-07 ( -2.7094e-08  2.71378e-08 ) ergs/cm2
 
Cutoff power-law model
 
Time interval is from   -0.356 sec. to    0.644 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 0.686332     ( -0.194096   0.100059 )
Epeak [keV] : 999.229      ( -999.552 -999.552 )
Norm@50keV  : 7.90531E-02    ( -0.002222   0.0155896 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          35.52 using 59 PHA bins.
# Reduced chi-squared =         0.6344 for     56 degrees of freedom 
# Null hypothesis probability =   9.851297e-01
 
Photon flux (15-150 keV)    in 1 sec: 8.40064 ( -0.25008  0.24101 ) ph/cm2/s
Energy fluence (15-150 keV)             : 8.65579e-07 ( -2.7871e-08  2.6056e-08 ) ergs/cm2
 
Band function
 
Time interval is from   -0.356 sec. to    0.644 sec.
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : 5.00000   ( -5   -5 )
beta        : -0.784527    ( -0.0544346   0.0547416 )
Epeak [keV] : 26.0983      ( -25.9444 4.81059 )
Norm@50keV   : 3105.11    ( -87.067   6.35281e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          34.09 using 59 PHA bins.
# Reduced chi-squared =         0.6197 for     55 degrees of freedom 
# Null hypothesis probability =   9.880265e-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]    : 26.4812  (  )
R^2/D10^2   : 0.181936  (   )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =         201.92 using 59 PHA bins.
# Reduced chi-squared =         3.5424 for     57 degrees of freedom 
# Null hypothesis probability =   4.421815e-18
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.148e-08   1.160e-09
25- 50  1.254e-07   5.600e-09
50-150  6.451e-07   2.795e-08
15-150  7.920e-07   2.555e-08
Thermal bremsstrahlung (OTTB)
 
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 199.363       (      )
Norm        : 32.3226       (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =         612.63 using 59 PHA bins.
# Reduced chi-squared =         10.748 for     57 degrees of freedom 
# Null hypothesis probability =   4.168288e-94
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.049e-08   2.605e-09
25- 50  1.548e-07   4.850e-09
50-150  3.396e-07   1.030e-08
15-150  5.749e-07   1.870e-08
Double BB
 
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 9.65979        (-1.58066      1.92415)
R1^2/D10^2  : 1.80671        (-0.667554      1.20111)
kT2 [keV]   : 43.9776        (-6.17211      11.2735)
R2^2/D10^2  : 3.74239E-02    (-0.0171186   0.0204993)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          40.16 using 59 PHA bins.
# Reduced chi-squared =         0.7302 for     55 degrees of freedom 
# Null hypothesis probability =   9.334346e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.261e-08   5.925e-09
25- 50  1.412e-07   1.170e-08
50-150  6.898e-07   7.080e-08
15-150  8.737e-07   6.750e-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: 1.08201     ( -0.0426832   0.0425053 )
Norm@50keV  : 2.10697E-02    ( -0.000479065   0.000477953 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          32.74 using 59 PHA bins.
# Reduced chi-squared =         0.5744 for     57 degrees of freedom 
# Null hypothesis probability =   9.959144e-01
 
Photon flux (15-150 keV)    in 10.58 sec: 2.44016 ( -0.0586126  0.0581387 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.34421e-06 ( -5.49755e-08  5.50319e-08 ) ergs/cm2
 
Cutoff power-law model
 
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.02224     ( -0.158315   0.075213 )
Epeak [keV] : 990.275      ( -994.013 -994.013 )
Norm@50keV  : 2.23154E-02    ( -0.000497796   0.00355428 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          32.53 using 59 PHA bins.
# Reduced chi-squared =         0.5808 for     56 degrees of freedom 
# Null hypothesis probability =   9.949287e-01
 
Photon flux (15-150 keV)    in 10.58 sec: 2.43707 ( -0.05664  0.06 ) ph/cm2/s
Energy fluence (15-150 keV)             : 2.33904e-06 ( -5.68358e-08  5.92374e-08 ) ergs/cm2
 
Band function
 
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       : -0.725949   ( 0.722667   0.722667 )
beta        : -1.10680    ( 1.10849   0.0610276 )
Epeak [keV] : 136.519      ( -145.448 325.782 )
Norm@50keV   : 3.36989E-02    ( -0.0116406   0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          31.81 using 59 PHA bins.
# Reduced chi-squared =         0.5784 for     55 degrees of freedom 
# Null hypothesis probability =   9.948376e-01
 
Photon flux (15-150 keV)    in 10.58 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)  = 4.58e-07
S(50-100 keV) = 8.65e-07
 T90 vs. Hardness ratio plot 
 
T90                                   = 4.30000001192093 sec.
Hardness ratio (energy fluence ratio) = 1.88865
 Color vs. Color plot 
 
Count Ratio  (25-50 keV) / (15-25 keV) = 1.65955
Count Ratio (50-100 keV) / (15-25 keV) = 1.65675
 Mask shadow pattern 
 
IMX = 1.211522604034570E-01, IMY = 2.403453886967238E-01
 TIME vs. PHA plot around the trigger time 
 
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
 TIME vs. DetID plot around the trigger time 
 
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
 100 us light curve (15-350 keV)
 
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
 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:
-239.248000 -3.052000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6305  22.0182    0.3  24.5   51.8  10.1283  45.4    0.3	Crab                          
 76.5971   9.8420    2.5  38.3   48.7   1.8025   4.5 ------	UNKNOWN                       
102.4794 -16.3022    1.9  56.4    4.2   5.6935   6.0 ------	UNKNOWN                       
133.2913  29.5943    2.9  26.7  -72.9   0.9119   3.9 ------	UNKNOWN                       
 Pre-slew background subtracted image of 15-350 keV band 
Time interval of the image:
-3.052000 7.532000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.7687  22.0906   11.2  24.3   51.7   0.0583   1.0    8.8	Crab                          
 93.8715  34.6733    2.6   9.1   60.3   0.1899   4.5 ------	UNKNOWN                       
119.6655  32.8565    0.2  15.1  -63.2   3.4454  74.4 ------	UNKNOWN                       
115.2856  -8.8203    2.4  50.1  -12.3   0.5560   4.9 ------	UNKNOWN                       
137.8438  40.2680    2.2  26.3  -98.4   0.3065   5.2 ------	UNKNOWN                       
192.6699  64.4124    2.7  54.3 -144.5   1.0375   4.3 ------	UNKNOWN                       
 Post-slew image of 15-350 keV band 
Time interval of the image:
50.452600 962.838100
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.6263  22.0143    0.3  33.6   69.3  36.9734  37.9    0.4	Crab                          
 71.3060  58.2211    2.8  41.0  132.0   5.5920   4.1 ------	UNKNOWN                       
 83.5241  53.4070    2.6  32.8  128.5   3.8614   4.5 ------	UNKNOWN                       
 86.7982  44.1821    2.4  27.8  112.5   3.7723   4.9 ------	UNKNOWN                       
 92.0993   4.5546    2.5  38.2   37.1   3.7503   4.6 ------	UNKNOWN                       
149.2800  73.1483    3.3  43.0 -179.0   2.8592   3.5 ------	UNKNOWN                       
136.0712  34.7215    2.7  13.8 -113.4   2.0115   4.2 ------	UNKNOWN                       
Plot creation:
Sun May 31 08:55:25 EDT 2015