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
116.1629 35.2682 0.0043 28.7857 91.6228 5.8989857 45.404 TRIG_01274039
Foreground time interval of the image:
-12.216 6.444 (delta_t = 18.660 [sec])
Background time interval of the image:
-146.547 -12.216 (delta_t = 134.331 [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 -12.216 sec. to 6.444 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.18148 ( -0.0512834 0.0510216 )
Norm@50keV : 2.10021E-02 ( -0.000614619 0.00061418 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.15 using 59 bins.
Reduced chi-squared = 0.914912
# Null hypothesis probability of 6.57e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 18.66 sec: 2.45899 ( -0.0763 0.07642 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.99753e-06 ( -1.22354e-07 1.2251e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -12.216 sec. to 6.444 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.778777 ( -0.21799 0.207731 )
Epeak [keV] : 176.515 ( -41.8543 119.427 )
Norm@50keV : 3.15272E-02 ( -0.0058149 0.00747807 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.72 using 59 bins.
Reduced chi-squared = 0.727143
# Null hypothesis probability of 9.38e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 18.66 sec: 2.40883 ( -0.07999 0.08015 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.93036e-06 ( -1.28798e-07 1.28295e-07 ) ergs/cm2
Band function
Time interval is from -12.216 sec. to 6.444 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] : 20.5261 ( )
R^2/D10^2 : 0.104776 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 217.83 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.22e-20 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.571e-07 9.134e-09
25- 50 7.961e-07 3.676e-08
50-150 2.494e-06 1.138e-07
15-150 3.448e-06 1.176e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 10.4482 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 201.96 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.36e-18 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.855e-07 1.567e-08
25- 50 9.339e-07 2.920e-08
50-150 2.048e-06 7.091e-08
15-150 3.468e-06 1.036e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.42927 (-1.09804 1.23055)
R1^2/D10^2 : 1.01509 (-0.335245 0.559775)
kT2 [keV] : 31.3140 (-3.04921 4.3097)
R2^2/D10^2 : 2.19732E-02 (-0.00787141 0.00955444)
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.64 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.26e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.135e-07 3.648e-08
25- 50 8.669e-07 5.925e-08
50-150 2.765e-06 2.305e-07
15-150 3.945e-06 2.351e-07
Peak spectrum fit
Power-law model
Time interval is from 0.036 sec. to 1.036 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.953132 ( -0.0747271 0.0739937 )
Norm@50keV : 8.95058E-02 ( -0.00402907 0.00402397 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.83 using 59 bins.
Reduced chi-squared = 1.19
# Null hypothesis probability of 1.54e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.464730 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 9.84555e-07 ( -4.77483e-08 4.78498e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.036 sec. to 1.036 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.456909 ( -0.3371 0.312906 )
Epeak [keV] : 180.035 ( -50.2213 194.361 )
Norm@50keV : 0.149154 ( -0.040225 0.0595523 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.24 using 59 bins.
Reduced chi-squared = 1.07571
# Null hypothesis probability of 3.25e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 10.1495 ( -0.475 0.475 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.75306e-08 ( -3.55753e-08 3.59134e-08 ) ergs/cm2
Band function
Time interval is from 0.036 sec. to 1.036 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] : 22.0340 ( )
R^2/D10^2 : 0.380583 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 118.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.63e-06 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.417e-08 2.975e-09
25- 50 1.809e-07 1.155e-08
50-150 6.560e-07 4.655e-08
15-150 8.711e-07 5.090e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 40.7036 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 231.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.93e-23 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.014e-07 5.140e-09
25- 50 1.950e-07 9.800e-09
50-150 4.276e-07 2.285e-08
15-150 7.239e-07 3.995e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 12.3761 (-2.57541 2.59719)
R1^2/D10^2 : 1.38685 (-0.473259 0.969559)
kT2 [keV] : 47.7012 (-13.5663 56.8315)
R2^2/D10^2 : 2.71481E-02 (-0.0214011 0.0509869)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.18 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.26e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.201e-08 8.990e-09
25- 50 1.968e-07 4.165e-08
50-150 7.207e-07 2.611e-07
15-150 9.696e-07 2.976e-07
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: 1.18148 ( -0.0512834 0.0510216 )
Norm@50keV : 2.10021E-02 ( -0.000614619 0.00061418 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.57e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 18.66 sec: 2.45898 ( -0.07629 0.0764188 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.99705e-06 ( -1.2236e-07 1.22498e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.778777 ( -0.21799 0.207731 )
Epeak [keV] : 176.515 ( -41.8543 119.427 )
Norm@50keV : 3.15272E-02 ( -0.0058149 0.00747806 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.38e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 18.66 sec: 2.40868 ( -0.07996 0.08014 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.93207e-06 ( -1.29034e-07 1.28418e-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) = 8.30e-07
S(50-100 keV) = 1.46e-06
T90 vs. Hardness ratio plot
T90 = 8.13199985027313 sec.
Hardness ratio (energy fluence ratio) = 1.75904
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.78416
Count Ratio (50-100 keV) / (15-25 keV) = 1.76891
Mask shadow pattern
IMX = -1.555907487129259E-02, IMY = -5.492086444347903E-01
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:
-146.547400 -12.216000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
148.0655 -0.1524 2.5 43.0 10.5 1.3821 4.6 ------ UNKNOWN
107.9239 76.5830 2.6 38.6 169.3 1.4223 4.4 ------ UNKNOWN
176.0534 76.1734 2.5 35.0 -165.9 1.1206 4.7 ------ UNKNOWN
227.3971 56.0931 2.6 48.1 -129.2 3.9541 4.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-12.216000 6.444000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
62.9263 65.3719 2.6 51.7 152.3 1.8869 4.4 ------ UNKNOWN
116.1629 35.2682 0.3 28.8 91.6 5.8990 45.4 ------ UNKNOWN
145.1171 30.2672 2.5 13.7 31.4 0.3221 4.7 ------ UNKNOWN
170.2372 -3.1389 3.2 48.7 -19.8 0.5475 3.6 ------ UNKNOWN
190.1533 43.3169 2.3 27.5 -100.0 0.4357 5.1 ------ UNKNOWN
240.0181 62.7029 2.7 52.0 -140.0 1.2158 4.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
84.852600 943.852610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6169 22.0270 0.7 31.2 85.8 33.5826 16.3 1.2 Crab
117.1588 -7.7619 3.8 43.0 10.6 5.1943 3.0 ------ UNKNOWN
147.3813 31.6259 3.1 26.2 -78.9 4.7464 3.7 ------ UNKNOWN
149.4108 -12.7996 2.3 57.5 -27.3 29.2785 5.0 ------ UNKNOWN
158.3941 21.0901 2.6 39.5 -68.4 12.5559 4.5 ------ UNKNOWN
181.7274 59.2072 2.7 48.1 -129.1 22.4579 4.3 ------ UNKNOWN
Plot creation:
Fri Jun 20 02:00:36 EDT 2025