Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte
Image
Pre-slew 15.0-350.0 keV image (Event data)
 
#   RAcent    DECcent   POSerr    Theta     Phi              Peak Cts       SNR   Name
  148.2718    35.6225   0.0130    37.6289     4.1994         2.3282373     14.730 TRIG_00799669                 
 
Foreground time interval of the image:
  8.004  89.301 (delta_t =  81.297 [sec])
Background time interval of the image:
-239.000   8.004 (delta_t = 247.004 [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 
 
 8 ms binning
 From T100_start-3 s to T100_start+3 s
 
 2 ms binning
 From T100_start-1 s to T100_start+1 s
 
 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    8.004 sec. to  210.088 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.02276     ( -0.163922   0.170767 )
Norm@50keV  : 1.00857E-03    ( -0.000111046   0.000108743 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.87 using 59 PHA bins.
# Reduced chi-squared =          1.033 for     57 degrees of freedom 
# Null hypothesis probability =   4.070246e-01
 
Photon flux (15-150 keV)    in 202.1 sec: 0.152902 ( -0.013389  0.013396 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.8825e-06 ( -1.91923e-07  1.9502e-07 ) ergs/cm2
 
Cutoff power-law model
 
Time interval is from    8.004 sec. to  210.088 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.89265     ( -0.715882   0.232882 )
Epeak [keV] : 34.7480      ( -25.4084 -34.7507 )
Norm@50keV  : 1.19898E-03    ( -0.000379441   0.00187923 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          58.74 using 59 PHA bins.
# Reduced chi-squared =          1.049 for     56 degrees of freedom 
# Null hypothesis probability =   3.752399e-01
 
Photon flux (15-150 keV)    in 202.1 sec: 0.152118 ( -0.01395  0.013649 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.85633e-06 ( -2.28177e-07  2.12884e-07 ) ergs/cm2
 
Band function
 
Time interval is from    8.004 sec. to  210.088 sec.
 
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       :    (     )
beta        :     (     )
Epeak [keV] :       (   )
Norm@50keV   :     (     )
------------------------------------------------------------
 
Photon flux (15-150 keV)    in  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]    : 9.82798  (-1.06181  1.18742)
R^2/D10^2   : 7.38817E-02  (-0.0263441   0.0413731)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          92.69 using 59 PHA bins.
# Reduced chi-squared =          1.626 for     57 degrees of freedom 
# Null hypothesis probability =   1.964352e-03
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  2.919e-07   4.264e-08
25- 50  7.081e-07   8.337e-08
50-150  3.514e-07   8.377e-08
15-150  1.351e-06   1.555e-07
Thermal bremsstrahlung (OTTB)
 
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 65.2415       (-15.9063      24.2987)
Norm        : 0.767065       (-0.109959     0.125798)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.55 using 59 PHA bins.
# Reduced chi-squared =          1.062 for     57 degrees of freedom 
# Null hypothesis probability =   3.491464e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  3.944e-07   4.345e-08
25- 50  6.154e-07   6.043e-08
50-150  7.491e-07   1.687e-07
15-150  1.759e-06   1.943e-07
Double BB
 
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 5.03828        (-1.2285      1.69359)
R1^2/D10^2  : 0.703909        (-0.451769      1.51671)
kT2 [keV]   : 17.7679        (-4.0767      10.0905)
R2^2/D10^2  : 5.59871E-03    (-0.00456824   0.0107975)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          60.45 using 59 PHA bins.
# Reduced chi-squared =          1.099 for     55 degrees of freedom 
# Null hypothesis probability =   2.855111e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  4.285e-07   1.899e-07
25- 50  5.662e-07   2.066e-07
50-150  7.611e-07   4.317e-07
15-150  1.756e-06   6.420e-07
Peak spectrum fit
Power-law model
 
Time interval is from   61.344 sec. to   62.344 sec.
 
Spectral model in power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 2.12701     ( -0.582488   0.751566 )
Norm@50keV  : 4.19165E-03    ( -0.00193912   0.00176756 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          39.65 using 59 PHA bins.
# Reduced chi-squared =         0.6957 for     57 degrees of freedom 
# Null hypothesis probability =   9.610044e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.668443 ( -0.21774  0.217785 ) ph/cm2/s
Energy fluence (15-150 keV)             : 3.90607e-08 ( -1.50425e-08  1.5743e-08 ) ergs/cm2
 
Cutoff power-law model
 
Time interval is from   61.344 sec. to   62.344 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.84669     ( -2.32453   0.209135 )
Epeak [keV] : 23.7728      (   )
Norm@50keV  : 6.06269E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          39.61 using 59 PHA bins.
# Reduced chi-squared =         0.7072 for     56 degrees of freedom 
# Null hypothesis probability =   9.523624e-01
 
Photon flux (15-150 keV)    in 1 sec: 0.664582 ( -0.219776  0.216519 ) ph/cm2/s
Energy fluence (15-150 keV)             : 0 ( 0  0 ) ergs/cm2
 
Band function
 
Time interval is from   61.344 sec. to   62.344 sec.
 
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       :    (     )
beta        :     (     )
Epeak [keV] :       (   )
Norm@50keV   :     (     )
------------------------------------------------------------
 
Photon flux (15-150 keV)    in  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]    : 9.39841  (-3.60457  5.90801)
R^2/D10^2   : 0.388872  (-0.383697   2.16905)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          42.69 using 59 PHA bins.
# Reduced chi-squared =         0.7489 for     57 degrees of freedom 
# Null hypothesis probability =   9.205228e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  6.828e-09   4.321e-09
25- 50  1.551e-08   9.720e-09
50-150  6.744e-09   5.180e-09
15-150  2.908e-08   1.881e-08
Thermal bremsstrahlung (OTTB)
 
 
 
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT [keV]    : 58.8724       (-35.2114      -58.8721)
Norm        : 3.54237       (-1.53844     3.14175)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          39.75 using 59 PHA bins.
# Reduced chi-squared =         0.6974 for     57 degrees of freedom 
# Null hypothesis probability =   9.600174e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  8.875e-09   5.658e-09
25- 50  1.343e-08   8.309e-09
50-150  1.504e-08   1.231e-08
15-150  3.734e-08   2.434e-08
Double BB
 
 
 
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters  : value         Lower 90%    Upper 90%
kT1 [keV]   : 4.25574        (-4.27798      6.0605)
R1^2/D10^2  : 6.38373        (-5.9222      -6.15674)
kT2 [keV]   : 16.6244        (-16.7076      -16.708)
R2^2/D10^2  : 3.35900E-02    (-0.0325602   0.538665)
------------------------------------------------------------
#Fit statistic : Chi-Squared =          39.59 using 59 PHA bins.
# Reduced chi-squared =         0.7199 for     55 degrees of freedom 
# Null hypothesis probability =   9.416431e-01
 
Energy  Fluence     90% Error
[keV]   [erg/cm2]   [erg/cm2]
15- 25  9.679e-09   5.695e-09
25- 50  1.160e-08   6.410e-09
50-150  1.625e-08   1.224e-08
15-150  3.753e-08   1.947e-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: 1.81150     ( -0.188159   0.193918 )
Norm@50keV  : 1.63596E-03    ( -0.000196354   0.000193073 )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          54.29 using 59 PHA bins.
# Reduced chi-squared =         0.9524 for     57 degrees of freedom 
# Null hypothesis probability =   5.775420e-01
 
Photon flux (15-150 keV)    in 81.3 sec: 0.226444 ( -0.0247985  0.0248286 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.22396e-06 ( -1.47844e-07  1.49428e-07 ) ergs/cm2
 
Cutoff power-law model
 
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
Photon index: 1.57563     ( -0.842169   0.725753 )
Epeak [keV] : 82.4839      (   )
Norm@50keV  : 2.20087E-03    (     )
------------------------------------------------------------
#Fit statistic : Chi-Squared =          53.98 using 59 PHA bins.
# Reduced chi-squared =         0.9640 for     56 degrees of freedom 
# Null hypothesis probability =   5.516453e-01
 
Photon flux (15-150 keV)    in 81.3 sec: 0.224519 ( -0.025575  0.025473 ) ph/cm2/s
Energy fluence (15-150 keV)             : 1.20104e-06 ( -1.6538e-07  1.64137e-07 ) ergs/cm2
 
Band function
 
 
 
Spectral model in the Band function:
------------------------------------------------------------
Parameters  : value       lower 90%   higher 90%
alpha       :    (     )
beta        :     (     )
Epeak [keV] :       (   )
Norm@50keV   :     (     )
------------------------------------------------------------
 
Photon flux (15-150 keV)    in  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)  = 5.70e-07
S(50-100 keV) = 5.62e-07
 T90 vs. Hardness ratio plot 
 
T90                                   = 173.871999979019 sec.
Hardness ratio (energy fluence ratio) = 0.985965
 Color vs. Color plot 
 
Count Ratio  (25-50 keV) / (15-25 keV) = 0.95888
Count Ratio (50-100 keV) / (15-25 keV) = 0.484114
 Mask shadow pattern 
 
IMX = 7.688365867807131E-01, IMY = -5.645186769244518E-02
 TIME vs. PHA plot around the trigger time 
 
 TIME vs. DetID plot around the trigger time 
 
 100 us light curve (15-350 keV)
 
 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:
-239.000000 8.004000
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
 83.1503  33.0107    3.2  33.0  104.6   1.7261   3.6 ------	UNKNOWN                       
130.8375  33.6549    2.4  33.1   28.1   1.5938   4.8 ------	UNKNOWN                       
 40.9265  61.4279    0.2  29.1 -174.6  15.5668  56.6 ------	UNKNOWN                       
347.4721  49.9252    3.2  57.3 -154.0   5.8465   3.6 ------	UNKNOWN                       
183.6776  29.3441    3.6  58.7  -25.8   6.4191   3.2 ------	UNKNOWN                       
 Pre-slew background subtracted image of 15-350 keV band 
Time interval of the image:
8.004000 89.300610
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
130.7981  40.7029    2.2  26.6   22.6   0.6754   5.3 ------	UNKNOWN                       
148.2718  35.6225    0.8  37.6    4.2   2.3282  14.7 ------	UNKNOWN                       
137.0188  61.9865    2.0  14.4  -32.5   0.6307   5.8 ------	UNKNOWN                       
167.2717  23.7478    2.9  56.1   -7.4   1.6484   4.1 ------	UNKNOWN                       
 Post-slew image of 15-350 keV band 
Time interval of the image:
158.500600 963.070700
 
# RAcent  DECcent POSerr Theta    Phi  PeakCts   SNR AngSep     Name
#  [deg]    [deg]    ['] [deg]  [deg]                   [']
188.3721  50.7171    2.6  32.4 -132.7   2.9564   4.4 ------	UNKNOWN                       
234.8476  64.8095    3.7  56.8 -151.8   9.9779   3.1 ------	UNKNOWN                       
Plot creation:
Sat Jan 20 09:05:09 EST 2018