Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minutes to calcaulte
Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
187.3157 +47.8427 0.0039 26.4 -72.7 5.0293 49.0 TRIG_01351008
------------------------------------------
Foreground time interval of the image:
-4.832 13.557 (delta_t = 18.389 [sec])
Background time interval of the image:
-239.944 -4.832 (delta_t = 235.112 [sec])
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 2) The mask-weighted light curves are using the flight position.
- 3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 4) 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.
- 5) 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.
- 6) 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)
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) For long bursts, a spectral fit of 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.
- 4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.
Time averaged spectrum fit using the pre-slew DRM
Power-law model
Time interval is from -4.832 sec. to 149.432 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.52481 ( -0.0377173 0.0377131 )
Norm@50keV : 7.56216E-03 ( -0.000148427 0.000148411 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.79 using 59 PHA bins.
# Reduced chi-squared = 0.7507 for 57 degrees of freedom
# Null hypothesis probability = 9.188302e-01
Photon flux (15-150 keV) in 154.3 sec: 0.950499 ( -0.0218991 0.0219844 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.10258e-05 ( -2.1999e-07 2.20089e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -4.832 sec. to 149.432 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30578 ( -0.156545 0.151432 )
Epeak [keV] : 182.217 ( -52.1711 253.926 )
Norm@50keV : 9.42225E-03 ( -0.00129823 0.00155784 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.64 using 59 PHA bins.
# Reduced chi-squared = 0.6542 for 56 degrees of freedom
# Null hypothesis probability = 9.789258e-01
Photon flux (15-150 keV) in 154.3 sec: 0.932313 ( -0.024786 0.024944 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.08863e-05 ( -2.42282e-07 2.41294e-07 ) ergs/cm2
Band function
Time interval is from -4.832 sec. to 149.432 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.31121 ( -0.321337 4.18745 )
beta : -9.36918 ( 9.37152 19.3715 )
Epeak [keV] : 185.690 ( -28.585 117.851 )
Norm@50keV : 9.36909E-03 ( -0.000187045 0.00151474 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 36.64 using 59 PHA bins.
# Reduced chi-squared = 0.6662 for 55 degrees of freedom
# Null hypothesis probability = 9.731656e-01
Photon flux (15-150 keV) in 154.3 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] : 17.6219 ( )
R^2/D10^2 : 5.84364E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 536.42 using 59 PHA bins.
# Reduced chi-squared = 9.4109 for 57 degrees of freedom
# Null hypothesis probability = 3.878535e-79
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.643e-07 2.384e-08
25- 50 2.568e-06 7.406e-08
50-150 5.756e-06 1.929e-07
15-150 8.889e-06 1.952e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-5.72895 -200)
Norm : 3.89103 (-0.0760964 0.0760964)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.495e-06 3.410e-08
25- 50 2.877e-06 6.249e-08
50-150 6.309e-06 1.535e-07
15-150 1.068e-05 2.639e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.59047 (-0.597754 0.633613)
R1^2/D10^2 : 0.705343 (-0.170099 0.240162)
kT2 [keV] : 28.1207 (-1.88032 2.30404)
R2^2/D10^2 : 9.24957E-03 (-0.00231376 0.00271868)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.271e-06 9.351e-08
25- 50 2.835e-06 1.018e-07
50-150 6.674e-06 2.739e-07
15-150 1.078e-05 3.611e-07
Peak spectrum fit
Power-law model
Time interval is from 0.288 sec. to 1.288 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.19944 ( -0.101996 0.101756 )
Norm@50keV : 4.21696E-02 ( -0.00259276 0.00259238 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.03 using 59 PHA bins.
# Reduced chi-squared = 0.8075 for 57 degrees of freedom
# Null hypothesis probability = 8.505454e-01
Photon flux (15-150 keV) in 1 sec: 4.94946 ( -0.309151 0.309287 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.27896e-07 ( -2.94823e-08 2.95919e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.288 sec. to 1.288 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.785024 ( -0.440392 0.39989 )
Epeak [keV] : 157.619 ( -55.3573 842.167 )
Norm@50keV : 6.67703E-02 ( -0.0232218 0.0403507 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 42.90 using 59 PHA bins.
# Reduced chi-squared = 0.7661 for 56 degrees of freedom
# Null hypothesis probability = 9.007174e-01
Photon flux (15-150 keV) in 1 sec: 4.89196 ( -0.31451 0.31436 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.19434e-07 ( -3.1326e-08 3.1129e-08 ) ergs/cm2
Band function
Time interval is from 0.288 sec. to 1.288 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 3.56195 ( -5.58766 -3.56176 )
beta : -1.31354 ( -0.147129 0.13522 )
Epeak [keV] : 31.1690 ( -6.30588 94.9922 )
Norm@50keV : 109.401 ( -109.249 402.89 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.97 using 59 PHA bins.
# Reduced chi-squared = 0.7450 for 55 degrees of freedom
# Null hypothesis probability = 9.202333e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 18.4152 (-1.44158 1.592)
R^2/D10^2 : 0.306284 (-0.0732685 0.0946255)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.064e-08 2.465e-09
25- 50 9.708e-08 8.260e-09
50-150 2.403e-07 2.740e-08
15-150 3.580e-07 2.960e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-11.5734 -200)
Norm : 20.2516 (-1.26954 1.26954)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.041e-08 3.560e-09
25- 50 9.697e-08 9.230e-09
50-150 2.127e-07 5.470e-08
15-150 3.601e-07 5.990e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.28253 (-1.97795 2.53494)
R1^2/D10^2 : 2.33705 (-1.19316 3.0195)
kT2 [keV] : 30.6896 (-6.00527 14.7079)
R2^2/D10^2 : 4.56640E-02 (-0.0326966 0.053129)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.635e-08 1.152e-08
25- 50 9.649e-08 2.215e-08
50-150 2.885e-07 1.056e-07
15-150 4.213e-07 1.210e-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: 1.26913 ( -0.0533193 0.0531323 )
Norm@50keV : 1.81410E-02 ( -0.00052674 0.000526526 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.21 using 59 PHA bins.
# Reduced chi-squared = 1.144 for 57 degrees of freedom
# Null hypothesis probability = 2.127441e-01
Photon flux (15-150 keV) in 18.39 sec: 2.15244 ( -0.0670867 0.0672229 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.32223e-06 ( -1.02627e-07 1.02774e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.11865 ( -0.208567 0.171339 )
Epeak [keV] : 332.629 ( )
Norm@50keV : 2.11891E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.56 using 59 PHA bins.
# Reduced chi-squared = 1.135 for 56 degrees of freedom
# Null hypothesis probability = 2.275073e-01
Photon flux (15-150 keV) in 18.39 sec: 2.13328 ( -0.07131 0.07145 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.29722e-06 ( -1.09218e-07 1.08795e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 2.89625 ( -5.89949 -3.4136 )
beta : -1.31664 ( -0.0666459 0.0638859 )
Epeak [keV] : 29.6822 ( -5.02487 38.5862 )
Norm@50keV : 21.1054 ( -21.1052 331.956 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.07 using 59 PHA bins.
# Reduced chi-squared = 1.074 for 55 degrees of freedom
# Null hypothesis probability = 3.292281e-01
Photon flux (15-150 keV) in 18.39 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) = 2.76e-06
S(50-100 keV) = 3.84e-06
T90 vs. Hardness ratio plot
T90 = 128.43599998951 sec.
Hardness ratio (energy fluence ratio) = 1.3913
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.44237
Count Ratio (50-100 keV) / (15-25 keV) = 1.09011
Mask shadow pattern
IMX = 1.470797417056447E-01, IMY = 4.730137515851542E-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:
-239.944000 -4.832000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4976 35.3566 291.5 33.2 170.9 -0.0169 -0.0 2.1 Her X-1
158.6217 38.1455 2.5 46.6 -53.9 6.8069 4.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-4.832000 13.556640
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5187 35.4121 14.2 33.2 170.8 -0.0718 -0.8 5.1 Her X-1
221.6732 87.7408 2.4 24.0 35.4 0.3598 4.8 ------ UNKNOWN
187.3157 47.8427 0.2 26.4 -72.7 5.0294 49.0 ------ UNKNOWN
215.4773 29.6316 2.2 34.8 -127.8 0.5920 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
78.056590 440.536000
442.056000 442.076000
443.056000 451.556600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3262 35.4213 3.1 50.0 155.8 -5.5949 -3.7 8.0 Her X-1
187.2708 47.8190 1.0 0.0 -23.3 5.5188 11.3 ------ UNKNOWN
138.2189 38.0601 2.6 36.6 -9.6 2.8749 4.5 ------ UNKNOWN
152.8753 28.2374 2.7 33.0 -36.6 2.5834 4.3 ------ UNKNOWN
Plot creation:
Sun Sep 21 11:42:14 EDT 2025