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
323.9330 -41.8731 0.0264 39.4 -27.7 0.9034 7.3 TRIG_01404126
------------------------------------------
Foreground time interval of the image:
0.392 50.845 (delta_t = 50.453 [sec])
Background time interval of the image:
-239.056 0.392 (delta_t = 239.448 [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 8.192000
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 8.192000
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 8.192000
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 0.392 sec. to 310.104 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.74010 ( -0.363125 0.391639 )
Norm@50keV : 3.49371E-04 ( -7.85955e-05 7.53445e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.71 using 59 PHA bins.
# Reduced chi-squared = 1.188 for 57 degrees of freedom
# Null hypothesis probability = 1.567707e-01
Photon flux (15-150 keV) in 309.7 sec: 4.70697E-02 ( -0.00956504 0.00959735 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.9899e-07 ( -2.2687e-07 2.30182e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.392 sec. to 310.104 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.41911 ( -1.76968 0.150175 )
Epeak [keV] : 150.394 ( )
Norm@50keV : 1.58179E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.42 using 59 PHA bins.
# Reduced chi-squared = 1.204 for 56 degrees of freedom
# Null hypothesis probability = 1.411671e-01
Photon flux (15-150 keV) in 309.7 sec: 4.71307E-02 ( -0.0096667 0.0095291 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.9349e-07 ( -2.2265e-07 2.3356e-07 ) ergs/cm2
Band function
Time interval is from 0.392 sec. to 310.104 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -2.75814 ( 2.75814 2.75814 )
beta : -1.74011 ( -0.391143 0.363743 )
Epeak [keV] : 87.9686 ( -87.9686 -87.9686 )
Norm@50keV : 4.74843E-02 ( -0.0106822 0.0102405 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.71 using 59 PHA bins.
# Reduced chi-squared = 1.231 for 55 degrees of freedom
# Null hypothesis probability = 1.166824e-01
Photon flux (15-150 keV) in 309.7 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] : 14.5708 (-3.60492 4.79432)
R^2/D10^2 : 5.50275E-03 (-0.00351092 0.00979221)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.89 using 59 PHA bins.
# Reduced chi-squared = 1.367 for 57 degrees of freedom
# Null hypothesis probability = 3.441737e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.608e-08 3.581e-08
25- 50 2.942e-07 1.166e-07
50-150 4.195e-07 2.070e-07
15-150 7.897e-07 3.066e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 153.337 (-87.1376 -150.519)
Norm : 0.190012 (-0.0413284 0.0651825)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.509e-07 8.687e-08
25- 50 2.805e-07 1.578e-07
50-150 5.587e-07 3.379e-07
15-150 9.900e-07 5.801e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.61643 (-1.53127 2.42215)
R1^2/D10^2 : 0.941247 (-0.852292 24.8179)
kT2 [keV] : 20.4483 (-5.66799 10.6431)
R2^2/D10^2 : 1.44039E-03 (-0.00110602 0.00188334)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.948e-07 1.072e-07
25- 50 2.228e-07 1.030e-07
50-150 5.601e-07 3.405e-07
15-150 9.777e-07 5.185e-07
Peak spectrum fit
Power-law model
Time interval is from 5.184 sec. to 6.184 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.29267 ( -0.688176 0.653887 )
Norm@50keV : 4.47657E-03 ( -0.00176021 0.00175755 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.82 using 59 PHA bins.
# Reduced chi-squared = 1.014 for 57 degrees of freedom
# Null hypothesis probability = 4.446178e-01
Photon flux (15-150 keV) in 1 sec: 0.533353 ( -0.218552 0.221671 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.43164e-08 ( -1.82088e-08 1.84664e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 5.184 sec. to 6.184 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.206130 ( -0.20598 1.54103 )
Epeak [keV] : 93.0567 ( -93.0524 -93.0524 )
Norm@50keV : 1.39493E-02 ( -0.0139515 215.794 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.35 using 59 PHA bins.
# Reduced chi-squared = 1.024 for 56 degrees of freedom
# Null hypothesis probability = 4.249427e-01
Photon flux (15-150 keV) in 1 sec: 0.512392 ( -0.284035 0.228318 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.28251e-08 ( -1.85409e-08 1.90503e-08 ) ergs/cm2
Band function
Time interval is from 5.184 sec. to 6.184 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.37943 ( -1.34142 3.82573 )
beta : -1.46465 ( 8.43557 18.4356 )
Epeak [keV] : 28.0611 ( -31.9564 267.299 )
Norm@50keV : 79.7102 ( -79.6767 106.482 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.04 using 59 PHA bins.
# Reduced chi-squared = 1.037 for 55 degrees of freedom
# Null hypothesis probability = 3.992701e-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] : 19.1479 (-6.4963 11.9574)
R^2/D10^2 : 2.91677E-02 (-0.0291677 0.0885403)
(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 2.096e-09 1.415e-09
25- 50 1.014e-08 6.555e-09
50-150 2.735e-08 1.803e-08
15-150 3.959e-08 2.599e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-199.363 -199.363)
Norm : 2.25980 (-0.894567 0.894588)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.627e-09 3.775e-09
25- 50 1.082e-08 6.965e-09
50-150 2.374e-08 1.477e-08
15-150 4.019e-08 2.663e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.96820 (-4.96211 185.039)
R1^2/D10^2 : 1.42460 (-1.43808 -1.43808)
kT2 [keV] : 22.3884 (-22.3856 -22.3856)
R2^2/D10^2 : 1.55565E-02 (-0.0155649 0.0689987)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.808e-09 2.855e-09
25- 50 9.818e-09 5.415e-09
50-150 2.873e-08 1.938e-08
15-150 4.336e-08 2.555e-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: 1.50558 ( -0.321729 0.325488 )
Norm@50keV : 1.29974E-03 ( -0.000245162 0.000243916 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.20 using 59 PHA bins.
# Reduced chi-squared = 1.161 for 57 degrees of freedom
# Null hypothesis probability = 1.891876e-01
Photon flux (15-150 keV) in 50.45 sec: 0.162503 ( -0.0314795 0.0316568 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.21483e-07 ( -1.25129e-07 1.26263e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.18131 ( -1.40201 1.3243 )
Epeak [keV] : 136.594 ( -136.62 -136.62 )
Norm@50keV : 1.85516E-03 ( -0.00100504 0.00591606 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.96 using 59 PHA bins.
# Reduced chi-squared = 1.178 for 56 degrees of freedom
# Null hypothesis probability = 1.702833e-01
Photon flux (15-150 keV) in 50.45 sec: 0.160230 ( -0.032697 0.032455 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.13538e-07 ( -1.28693e-07 1.29379e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.18990 ( -6.69789 1.19096 )
beta : -10.0000 ( 10 1.77636e-15 )
Epeak [keV] : 136.196 ( -75.7515 -136.23 )
Norm@50keV : 1.85147E-03 ( -0.000779556 0.00593335 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.97 using 59 PHA bins.
# Reduced chi-squared = 1.199 for 55 degrees of freedom
# Null hypothesis probability = 1.478322e-01
Photon flux (15-150 keV) in 50.45 sec: 0.160154 ( ) 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) = 2.75e-07
S(50-100 keV) = 3.29e-07
T90 vs. Hardness ratio plot
T90 = 286.975999951363 sec.
Hardness ratio (energy fluence ratio) = 1.19636
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.10946
Count Ratio (50-100 keV) / (15-25 keV) = 0.80071
Mask shadow pattern
IMX = 7.279075773863132E-01, IMY = 3.818464470884497E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
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:
-239.056000 0.392000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.392000 50.844600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
323.9337 -41.8732 1.6 39.4 -27.7 0.9106 7.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
138.044600 326.844600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
274.1468 -13.8746 5.5 51.2 -41.8 -2.4567 -2.1 12.7 GX 17+2
275.7447 -30.5145 7.8 39.9 -59.3 0.7529 1.5 12.9 H1820-303
285.1834 -24.8558 4.4 36.1 -44.1 -0.9504 -2.6 8.9 HT1900.1-2455
28.0161 -47.1640 2.6 44.7 150.0 3.6368 4.5 ------ UNKNOWN
Plot creation:
Thu Oct 16 13:38:30 EDT 2025