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
255.3274 +1.5902 0.0187 14.8 143.6 0.9264 10.3 TRIG_01515414
------------------------------------------
Foreground time interval of the image:
0.296 48.685 (delta_t = 48.389 [sec])
Background time interval of the image:
-179.216 0.296 (delta_t = 179.512 [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 0.296 sec. to 363.420 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.35173E-02 ( -0.013492 1.4313 )
Norm@50keV : 7.61657E-05 ( -7.61646e-05 7.96915e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.14 using 59 PHA bins.
# Reduced chi-squared = 0.9850 for 57 degrees of freedom
# Null hypothesis probability = 5.071917e-01
Photon flux (15-150 keV) in 363.1 sec: 1.02361E-02 ( -0.0102361 0.00779325 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.89321e-07 ( -3.07351e-07 3.08233e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.296 sec. to 363.420 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.450240 ( 0.450075 0.450075 )
Epeak [keV] : 423.244 ( -423.405 -423.405 )
Norm@50keV : 1.02112E-04 ( -0.000102098 0.202579 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.13 using 59 PHA bins.
# Reduced chi-squared = 1.002 for 56 degrees of freedom
# Null hypothesis probability = 4.698821e-01
Photon flux (15-150 keV) in 363.1 sec: 1.00575E-02 ( -0.00723587 0.0079527 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.88961e-07 ( -4.88961e-07 3.09957e-07 ) ergs/cm2
Band function
Time interval is from 0.296 sec. to 363.420 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.647427 ( 0.648519 0.648519 )
beta : -1.34395E-02 ( -1.43402 0.0135283 )
Epeak [keV] : 13.9309 ( -13.9304 -13.9304 )
Norm@50keV : 1.22705E-04 ( -0.000122666 109.658 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.14 using 59 PHA bins.
# Reduced chi-squared = 1.021 for 55 degrees of freedom
# Null hypothesis probability = 4.317902e-01
Photon flux (15-150 keV) in 363.1 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] : 52.8859 (-53.0321 -53.0321)
R^2/D10^2 : 4.46262E-05 (-4.43854e-05 0.000806588)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.15 using 59 PHA bins.
# Reduced chi-squared = 0.9851 for 57 degrees of freedom
# Null hypothesis probability = 5.068615e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.734e-09 3.179e-09
25- 50 3.465e-08 2.170e-08
50-150 4.465e-07 2.819e-07
15-150 4.859e-07 3.019e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.357 (-199.361 -199.361)
Norm : 4.06847E-02 (-0.034673 0.0346714)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.027e-09 1.619e-10
25- 50 2.763e-13 2.088e-17
50-150 1.506e-24 0.000e+00
15-150 7.027e-09 1.990e-11
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 0.201619 (-0.796006 -0.796006)
R1^2/D10^2 : 9.43627E+23 (-9.59006e+23 -9.59006e+23)
kT2 [keV] : 56.0772 (-38.0754 -56.0755)
R2^2/D10^2 : 3.90970E-05 (-3.72225e-05 0.000320554)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
Peak spectrum fit
Power-law model
Time interval is from 20.244 sec. to 21.244 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.23370 ( -0.339335 0.323108 )
Norm@50keV : 6.85096E-03 ( -0.00125517 0.0012544 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.96 using 59 PHA bins.
# Reduced chi-squared = 1.087 for 57 degrees of freedom
# Null hypothesis probability = 3.036524e-01
Photon flux (15-150 keV) in 1 sec: 0.808186 ( -0.154237 0.155232 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.88632e-08 ( -1.37206e-08 1.3896e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 20.244 sec. to 21.244 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.23313 ( -1.38256 0.322433 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 6.87511E-03 ( -0.00125968 0.0162698 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.96 using 59 PHA bins.
# Reduced chi-squared = 1.107 for 56 degrees of freedom
# Null hypothesis probability = 2.718322e-01
Photon flux (15-150 keV) in 1 sec: 0.809094 ( -0.15541 0.153702 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.88072e-08 ( -1.52897e-08 1.38212e-08 ) ergs/cm2
Band function
Time interval is from 20.244 sec. to 21.244 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -5 -5 )
beta : -1.73596 ( -0.693335 0.526986 )
Epeak [keV] : 38.5256 ( -14.256 7.18143 )
Norm@50keV : 50.3455 ( -9.06026 268.761 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.68 using 59 PHA bins.
# Reduced chi-squared = 1.067 for 55 degrees of freedom
# Null hypothesis probability = 3.421077e-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] : 15.0487 (-3.3574 5.28775)
R^2/D10^2 : 9.37268E-02 (-0.0599858 0.133142)
(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 4.441e-09 1.991e-09
25- 50 1.770e-08 5.367e-09
50-150 2.732e-08 1.087e-08
15-150 4.946e-08 1.427e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-72.3592 -200)
Norm : 3.37647 (-0.628514 0.628514)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.408e-09 4.897e-09
25- 50 1.617e-08 9.220e-09
50-150 3.547e-08 2.028e-08
15-150 6.006e-08 3.457e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.3641 (-2.04156 3.08548)
R1^2/D10^2 : 0.282866 (-0.171057 0.301895)
kT2 [keV] : 199.363 (-152.971 -199.363)
R2^2/D10^2 : 1.39829E-04 (-5.18988e-05 0.00199145)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
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: 1.34560 ( -0.247713 0.244069 )
Norm@50keV : 1.16097E-03 ( -0.00016517 0.000164994 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.44 using 59 PHA bins.
# Reduced chi-squared = 0.9025 for 57 degrees of freedom
# Null hypothesis probability = 6.828444e-01
Photon flux (15-150 keV) in 48.39 sec: 0.139738 ( -0.020603 0.0207071 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.49236e-07 ( -8.47585e-08 8.57877e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.271174 ( -1.48824 1.10235 )
Epeak [keV] : 82.1120 ( -23.1835 -82.1122 )
Norm@50keV : 3.90026E-03 ( -0.00390023 0.0160843 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.72 using 59 PHA bins.
# Reduced chi-squared = 0.8699 for 56 degrees of freedom
# Null hypothesis probability = 7.443407e-01
Photon flux (15-150 keV) in 48.39 sec: 0.132370 ( -0.02205 0.022086 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.05225e-07 ( -9.56133e-08 9.77575e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -9.12794E-03 ( -1.4059 4.96219 )
beta : -2.03891 ( 2.03946 0.765474 )
Epeak [keV] : 71.6796 ( -32.4044 220.143 )
Norm@50keV : 5.52729E-03 ( -0.00613949 7.14601 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.39 using 59 PHA bins.
# Reduced chi-squared = 0.8798 for 55 degrees of freedom
# Null hypothesis probability = 7.234152e-01
Photon flux (15-150 keV) in 48.39 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 5.10045e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 4.17e-08
S(50-100 keV) = 1.65e-07
T90 vs. Hardness ratio plot
T90 = 343.291999936104 sec.
Hardness ratio (energy fluence ratio) = 3.95683
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = -5.16913
Count Ratio (50-100 keV) / (15-25 keV) = -6.42855
Mask shadow pattern
IMX = -2.132175702167244E-01, IMY = -1.573147968992249E-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:
-179.216000 0.296000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9851 -15.6407 0.4 24.6 -160.9 9.5808 30.3 0.3 Sco X-1
254.2945 35.2937 7.8 28.7 46.0 0.7100 1.5 8.5 Her X-1
255.9784 -37.8383 21.9 48.3 -169.2 0.4115 0.5 0.5 4U 1700-377
256.5460 -36.3695 7.6 47.1 -170.4 -1.0644 -1.5 6.2 GX 349+2
262.9533 -24.9027 37.7 39.2 174.9 -0.1678 -0.3 9.9 GX 1+4
264.7994 -44.4699 16.8 57.0 -173.7 1.0447 0.7 2.7 4U 1735-44
268.4100 -1.5904 5.0 28.0 135.8 -1.0571 -2.3 8.6 SW J1753.5-0127
270.2020 -25.1005 4.8 43.4 167.3 1.9399 2.4 4.6 GX 5-1
270.3577 -25.5898 14.7 43.9 167.6 0.6611 0.8 9.7 GRS 1758-258
273.9306 -14.1997 7.6 38.9 151.2 1.1339 1.5 10.7 GX 17+2
275.9397 -30.3743 22.7 50.8 167.2 0.6317 0.5 0.9 H1820-303
262.9558 -33.9875 8.5 47.1 -178.3 1.2035 1.4 9.3 GX 354-0
267.3177 50.8290 3.3 46.8 46.8 3.8971 3.5 ------ UNKNOWN
270.2011 26.9673 3.2 32.1 77.2 2.5022 3.7 ------ UNKNOWN
254.4741 26.0946 2.9 20.8 57.6 1.5876 4.0 ------ UNKNOWN
213.6366 52.6506 3.2 49.6 2.9 2.3031 3.7 ------ UNKNOWN
191.9608 22.0268 2.7 50.0 -43.2 6.2190 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.296000 48.684610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.1470 -15.7314 6.8 24.7 -161.3 0.1569 1.7 11.1 Sco X-1
254.3689 35.1806 8.8 28.6 46.3 0.1612 1.3 10.6 Her X-1
255.9958 -37.8437 9.0 48.4 -169.2 0.2369 1.3 0.4 4U 1700-377
256.4164 -36.5069 27.6 47.2 -170.2 0.0728 0.4 5.1 GX 349+2
262.8929 -24.6331 8.1 39.0 174.8 0.2139 1.4 9.3 GX 1+4
264.8141 -44.5314 8.1 57.1 -173.7 -0.6715 -1.4 5.8 4U 1735-44
268.3520 -1.3016 4.9 27.9 135.3 -0.2995 -2.4 9.1 SW J1753.5-0127
270.3311 -24.9065 5.9 43.4 166.9 0.3557 1.9 10.7 GX 5-1
270.3249 -25.7333 13.6 44.0 167.8 0.1570 0.8 1.3 GRS 1758-258
274.1697 -14.1044 0.0 39.0 150.9 -0.3262 -1.8 10.4 GX 17+2
276.0237 -30.4880 6.2 50.9 167.2 -0.6254 -1.8 8.9 H1820-303
262.9142 -33.8646 17.8 46.9 -178.3 -0.1284 -0.6 4.1 GX 354-0
255.3274 1.5902 1.1 14.8 143.6 0.9263 10.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
105.884590 662.914000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9852 -15.5511 2.5 20.0 -143.0 24.8148 4.6 5.4 Sco X-1
254.5648 35.3019 4.3 33.7 5.4 17.8719 2.7 5.8 Her X-1
256.0563 -37.9893 6.9 39.6 -174.4 -12.8597 -1.7 9.3 4U 1700-377
256.2719 -36.3397 35.2 38.0 -174.7 2.5140 0.3 9.4 GX 349+2
262.8624 -24.7576 4.7 27.4 171.5 -14.1505 -2.4 8.0 GX 1+4
264.8710 -44.4134 3.7 46.8 177.2 -38.0502 -3.1 5.9 4U 1735-44
268.5011 -1.2888 0.0 13.5 108.8 -9.8811 -1.9 12.7 SW J1753.5-0127
270.3556 -25.1128 5.9 30.4 158.9 12.5529 1.9 4.4 GX 5-1
270.4600 -25.8233 8.6 31.1 159.5 9.1047 1.3 9.8 GRS 1758-258
273.8451 -13.9203 0.0 24.0 137.4 14.0183 2.2 11.7 GX 17+2
275.7703 -30.2973 9.0 37.4 156.8 12.4625 1.3 9.0 H1820-303
284.9159 -25.0663 21.8 39.1 141.4 -6.6106 -0.5 10.9 HT1900.1-2455
288.7318 11.0617 5.9 34.5 79.2 21.9938 2.0 8.0 GRS 1915+105
263.1467 -33.8971 11.4 36.3 175.5 7.5837 1.0 8.7 GX 354-0
279.2671 27.4358 3.0 34.5 46.0 34.7984 3.8 ------ UNKNOWN
234.6805 10.5234 3.4 22.4 -59.1 20.4718 3.4 ------ UNKNOWN
Plot creation:
Tue Oct 6 09:22:40 EDT 2026