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
21.9110 -21.5502 0.0066 34.6 129.5 10.0510 29.4 TRIG_01516664
------------------------------------------
Foreground time interval of the image:
103.608 208.301 (delta_t = 104.693 [sec])
Background time interval of the image:
-179.000 103.608 (delta_t = 282.608 [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
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)
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 103.608 sec. to 208.744 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.49759 ( -0.071882 0.0718477 )
Norm@50keV : 6.26222E-03 ( -0.000251451 0.000251399 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.50 using 59 PHA bins.
# Reduced chi-squared = 1.237 for 57 degrees of freedom
# Null hypothesis probability = 1.078846e-01
Photon flux (15-150 keV) in 105.1 sec: 0.781264 ( -0.0339995 0.0340926 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.24608e-06 ( -2.64907e-07 2.65373e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 103.608 sec. to 208.744 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.21701 ( -0.301121 0.275904 )
Epeak [keV] : 150.466 ( -51.3994 2331.06 )
Norm@50keV : 8.49253E-03 ( -0.00220842 0.00318163 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.63 using 59 PHA bins.
# Reduced chi-squared = 1.208 for 56 degrees of freedom
# Null hypothesis probability = 1.372496e-01
Photon flux (15-150 keV) in 105.1 sec: 0.768552 ( -0.036127 0.036218 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.14777e-06 ( -2.86114e-07 2.84853e-07 ) ergs/cm2
Band function
Time interval is from 103.608 sec. to 208.744 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.905014 ( -0.473556 1.69976 )
beta : -1.62915 ( 1.62957 0.139816 )
Epeak [keV] : 79.7924 ( -46.0989 243.256 )
Norm@50keV : 1.31013E-02 ( -0.00669592 0.100511 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.12 using 59 PHA bins.
# Reduced chi-squared = 1.220 for 55 degrees of freedom
# Null hypothesis probability = 1.266486e-01
Photon flux (15-150 keV) in 105.1 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] : 16.3922 ( )
R^2/D10^2 : 6.40720E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 196.17 using 59 PHA bins.
# Reduced chi-squared = 3.4415 for 57 degrees of freedom
# Null hypothesis probability = 3.579540e-17
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.720e-07 2.959e-08
25- 50 1.598e-06 8.776e-08
50-150 3.028e-06 2.091e-07
15-150 4.998e-06 2.107e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-17.2758 -200)
Norm : 3.21761 (-0.12902 0.12902)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.421e-07 4.078e-08
25- 50 1.620e-06 6.674e-08
50-150 3.553e-06 1.619e-07
15-150 6.015e-06 2.628e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.99989 (-1.20875 1.26619)
R1^2/D10^2 : 0.497047 (-0.181827 0.35185)
kT2 [keV] : 29.0074 (-4.21615 6.62353)
R2^2/D10^2 : 6.78237E-03 (-0.00347361 0.00539267)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.003e-07 1.059e-07
25- 50 1.641e-06 1.939e-07
50-150 3.783e-06 6.464e-07
15-150 6.124e-06 7.982e-07
Peak spectrum fit
Power-law model
Time interval is from 171.740 sec. to 172.740 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.39308 ( -0.19845 0.198472 )
Norm@50keV : 2.47545E-02 ( -0.00311233 0.00310471 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.90 using 59 PHA bins.
# Reduced chi-squared = 1.139 for 57 degrees of freedom
# Null hypothesis probability = 2.206734e-01
Photon flux (15-150 keV) in 1 sec: 3.00994 ( -0.380997 0.381458 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.39534e-07 ( -3.28306e-08 3.31025e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 171.740 sec. to 172.740 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.499191 ( -1.09462 0.853745 )
Epeak [keV] : 83.7004 ( -23.4528 440.81 )
Norm@50keV : 7.09249E-02 ( -0.0443754 0.180297 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.69 using 59 PHA bins.
# Reduced chi-squared = 1.102 for 56 degrees of freedom
# Null hypothesis probability = 2.799177e-01
Photon flux (15-150 keV) in 1 sec: 2.93932 ( -0.39048 0.38934 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.26817e-07 ( -3.5798e-08 3.5859e-08 ) ergs/cm2
Band function
Time interval is from 171.740 sec. to 172.740 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 3.97008E-02 ( -1.12706 -0.036437 )
beta : -1.98112 ( 1.97493 0.58454 )
Epeak [keV] : 64.0061 ( -38.0073 108.716 )
Norm@50keV : 0.146950 ( -0.14538 435.344 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.95 using 59 PHA bins.
# Reduced chi-squared = 1.108 for 55 degrees of freedom
# Null hypothesis probability = 2.706826e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.28371e-07 ( -2.28364e-07 -3.4277e-08 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 15.3310 (-2.02547 2.45589)
R^2/D10^2 : 0.339113 (-0.138654 0.218953)
(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 1.662e-08 4.400e-09
25- 50 6.738e-08 1.230e-08
50-150 1.088e-07 2.543e-08
15-150 1.928e-07 3.130e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-58.5943 -200)
Norm : 12.5189 (-1.55361 1.55361)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.118e-08 1.743e-08
25- 50 5.997e-08 3.306e-08
50-150 1.315e-07 7.270e-08
15-150 2.227e-07 1.227e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.7744 (-6.15286 3.81111)
R1^2/D10^2 : 0.837641 (-0.475214 0.797044)
kT2 [keV] : 37.8117 (-33.4584 -38.0073)
R2^2/D10^2 : 9.20810E-03 (-0.0088781 0.19225)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.222e-08 1.206e-08
25- 50 6.725e-08 3.652e-08
50-150 1.412e-07 7.539e-08
15-150 2.307e-07 1.118e-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: 1.49264 ( -0.0721367 0.0720887 )
Norm@50keV : 6.25094E-03 ( -0.000251718 0.000251675 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.44 using 59 PHA bins.
# Reduced chi-squared = 1.201 for 57 degrees of freedom
# Null hypothesis probability = 1.426666e-01
Photon flux (15-150 keV) in 104.7 sec: 0.778828 ( -0.0340093 0.0341023 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.21619e-06 ( -2.64423e-07 2.64877e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.22005 ( -0.301464 0.27343 )
Epeak [keV] : 154.485 ( -54.1515 -154.485 )
Norm@50keV : 8.40130E-03 ( -0.00217701 0.00314709 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.74 using 59 PHA bins.
# Reduced chi-squared = 1.174 for 56 degrees of freedom
# Null hypothesis probability = 1.752520e-01
Photon flux (15-150 keV) in 104.7 sec: 0.766521 ( -0.03613 0.036259 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.12154e-06 ( -2.85297e-07 2.84135e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.913031 ( -0.450005 1.95714 )
beta : -1.61902 ( 1.62055 0.139653 )
Epeak [keV] : 80.7516 ( -47.8081 300.159 )
Norm@50keV : 1.28821E-02 ( -0.00647194 0.0969661 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.26 using 59 PHA bins.
# Reduced chi-squared = 1.186 for 55 degrees of freedom
# Null hypothesis probability = 1.621749e-01
Photon flux (15-150 keV) in 104.7 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) = 1.54e-06
S(50-100 keV) = 2.19e-06
T90 vs. Hardness ratio plot
T90 = 78.8960000276566 sec.
Hardness ratio (energy fluence ratio) = 1.42208
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.41766
Count Ratio (50-100 keV) / (15-25 keV) = 1.07067
Mask shadow pattern
IMX = -4.390715900811846E-01, IMY = -5.332293944345299E-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:
-179.000000 103.608000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
320.7229 2.3833 2.8 41.0 9.0 2.3493 4.1 ------ UNKNOWN
289.9725 -20.0633 2.7 50.0 -43.3 6.5367 4.3 ------ UNKNOWN
289.2242 -22.8347 2.4 49.5 -47.0 7.8165 4.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
103.608000 208.300600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
21.9109 -21.5501 0.4 34.6 129.5 10.0465 29.4 ------ UNKNOWN
48.7024 -55.2112 2.6 49.9 -174.9 1.5194 4.4 ------ UNKNOWN
305.1827 1.3143 2.4 49.9 -9.0 1.5300 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
300.500600 723.183100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
320.6510 -20.0910 2.6 56.9 0.0 9.3981 4.4 ------ UNKNOWN
331.2579 -54.2039 2.3 50.0 -43.2 10.9900 4.9 ------ UNKNOWN
327.6689 -53.2669 2.3 51.7 -41.2 13.2003 5.1 ------ UNKNOWN
Plot creation:
Mon Oct 12 16:48:40 EDT 2026