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
290.3844 4.6774 0.0052 24.2970 60.9109 3.3722227 37.001 TRIG_01324646
Foreground time interval of the image:
-5.240 11.509 (delta_t = 16.749 [sec])
Background time interval of the image:
-239.392 -5.240 (delta_t = 234.152 [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 -5.240 sec. to 66.492 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.21350 ( -0.0751965 0.0746188 )
Norm@50keV : 5.25382E-03 ( -0.000201422 0.000201016 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.12 using 59 bins.
Reduced chi-squared = 1.26526
# Null hypothesis probability of 8.56e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 71.73 sec: 0.617891 ( -0.025446 0.025589 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.80935e-06 ( -1.555e-07 1.55993e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -5.240 sec. to 66.492 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.20850 ( -0.0753267 0.075827 )
Epeak [keV] : 9999.35 ( -9999.36 -9999.36 )
Norm@50keV : 5.26619E-03 ( -0.000199896 0.000348811 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.28 using 59 bins.
Reduced chi-squared = 1.29071
# Null hypothesis probability of 7.05e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 71.73 sec: 0.617723 ( -0.025488 0.025552 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.83266e-06 ( -1.80242e-07 1.31038e-07 ) ergs/cm2
Band function
Time interval is from -5.240 sec. to 66.492 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] : 21.2979 ( )
R^2/D10^2 : 2.20721E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 272.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.58e-30 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.349e-07 1.130e-08
25- 50 6.993e-07 4.408e-08
50-150 2.366e-06 1.359e-07
15-150 3.201e-06 1.399e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 2.61684 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 148.69 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.06e-10 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.674e-07 1.940e-08
25- 50 8.991e-07 3.945e-08
50-150 1.972e-06 9.540e-08
15-150 3.338e-06 1.395e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.34148 (-0.91083 1.0095)
R1^2/D10^2 : 0.516249 (-0.187456 0.322885)
kT2 [keV] : 37.8803 (-4.8594 7.03168)
R2^2/D10^2 : 3.22200E-03 (-0.00123796 0.0016584)
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.95 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.30e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.805e-07 5.053e-08
25- 50 8.022e-07 8.643e-08
50-150 2.761e-06 2.679e-07
15-150 3.944e-06 3.325e-07
Peak spectrum fit
Power-law model
Time interval is from 3.288 sec. to 4.288 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.69943 ( -0.141642 0.144505 )
Norm@50keV : 3.11697E-02 ( -0.00260166 0.0025696 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.60 using 59 bins.
Reduced chi-squared = 1.0807
# Null hypothesis probability of 3.15e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.13903 ( -0.32047 0.32095 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.88649e-07 ( -2.52646e-08 2.55393e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 3.288 sec. to 4.288 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.69870 ( -0.381871 0.144696 )
Epeak [keV] : 9999.28 ( -9999.34 -9999.35 )
Norm@50keV : 3.12198E-02 ( -0.0168148 0.0176813 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.60 using 59 bins.
Reduced chi-squared = 1.1
# Null hypothesis probability of 2.83e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.20211 ( -0.56857 0.65838 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.91749e-07 ( -2.88736e-08 2.20128e-08 ) ergs/cm2
Band function
Time interval is from 3.288 sec. to 4.288 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] : 12.6525 ( )
R^2/D10^2 : 0.804374 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 116.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.13e-06 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.731e-08 3.975e-09
25- 50 9.130e-08 8.435e-09
50-150 9.092e-08 1.596e-08
15-150 2.095e-07 2.035e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 145.034 (-46.5521 -143.828)
Norm : 16.9436 (-1.49205 1.94876)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.25e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.364e-08 4.520e-09
25- 50 8.048e-08 1.311e-08
50-150 1.566e-07 6.696e-08
15-150 2.808e-07 8.150e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.12478 (-1.37316 1.74168)
R1^2/D10^2 : 8.32974 (-4.84867 13.6673)
kT2 [keV] : 26.3641 (-6.60183 14.3564)
R2^2/D10^2 : 4.59391E-02 (-0.0344344 0.0833547)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.69e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.813e-08 1.325e-08
25- 50 7.595e-08 1.752e-08
50-150 1.647e-07 6.252e-08
15-150 2.888e-07 9.685e-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: 1.19509 ( -0.078807 0.0782702 )
Norm@50keV : 1.29232E-02 ( -0.000523193 0.000522489 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.34e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 16.75 sec: 1.51588 ( -0.0651195 0.0654197 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.19916e-06 ( -9.63319e-08 9.68262e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.19069 ( -0.141087 0.0736478 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 1.29847E-02 ( -0.000522285 0.000521908 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.13 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.97e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 16.75 sec: 1.51803 ( -0.0685 0.06285 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.71895e-14 ( 0 0 ) 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) = 8.03e-07
S(50-100 keV) = 1.39e-06
T90 vs. Hardness ratio plot
T90 = 50.6599999666214 sec.
Hardness ratio (energy fluence ratio) = 1.73101
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.30473
Count Ratio (50-100 keV) / (15-25 keV) = 1.22967
Mask shadow pattern
IMX = 2.194832795370373E-01, IMY = -3.945101455212145E-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:
-239.392000 -5.240000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.6612 35.4432 0.0 30.6 172.7 -0.6497 -1.5 11.6 Her X-1
268.4123 -1.3085 25.5 36.8 99.6 0.3669 0.5 9.0 SW J1753.5-0127
288.6849 11.0410 3.4 18.0 66.2 1.3492 3.4 8.8 GRS 1915+105
299.5720 35.1996 0.6 10.0 -69.5 6.7482 20.3 0.9 Cyg X-1
308.0274 41.0158 2.7 18.8 -73.3 1.7328 4.3 5.3 Cyg X-3
326.1874 38.3200 50.3 31.1 -55.8 0.1058 0.2 0.7 Cyg X-2
281.6975 -2.0293 3.6 32.1 77.5 2.3780 3.2 ------ UNKNOWN
254.4034 12.7163 2.8 37.0 132.8 3.6626 4.2 ------ UNKNOWN
290.1709 -1.9221 2.5 30.9 61.4 2.9543 4.5 ------ UNKNOWN
288.3963 6.6774 2.1 22.4 66.1 2.4432 5.5 ------ UNKNOWN
329.0289 -10.1498 2.8 54.1 11.7 4.6889 4.1 ------ UNKNOWN
262.4538 38.8674 3.3 25.0 -178.1 1.3336 3.5 ------ UNKNOWN
333.6327 27.1169 2.0 38.1 -36.8 2.8729 5.7 ------ UNKNOWN
225.3150 60.8898 3.0 52.9 -152.4 4.0072 3.9 ------ UNKNOWN
260.5477 74.5867 3.0 48.0 -129.0 7.0054 3.8 ------ UNKNOWN
344.0122 41.7031 2.6 44.9 -60.2 7.5784 4.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-5.240000 11.508600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.2546 35.2418 0.0 31.0 172.2 0.2329 2.7 11.6 Her X-1
268.2893 -1.3201 6.6 36.9 99.8 -0.3498 -1.8 9.2 SW J1753.5-0127
288.9918 10.9894 5.3 18.0 65.2 0.1743 2.2 11.7 GRS 1915+105
299.5768 35.2102 2700.0 10.0 -69.5 0.0001 0.0 0.8 Cyg X-1
307.8632 40.9462 5.2 18.7 -73.3 -0.1451 -2.2 11.2 Cyg X-3
325.9362 38.3287 0.0 30.9 -55.9 -0.0730 -0.9 11.1 Cyg X-2
290.3845 4.6774 0.3 24.3 60.9 3.3784 37.1 ------ UNKNOWN
340.4270 0.7185 2.7 55.5 -7.5 1.0946 4.3 ------ UNKNOWN
275.2360 69.3098 2.7 41.3 -126.8 0.5309 4.3 ------ UNKNOWN
334.8575 55.0286 2.3 41.1 -81.0 1.1143 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
74.108600 427.737200
428.608000 962.675100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3731 35.3072 5.4 45.2 -173.1 5.3398 2.1 4.6 Her X-1
263.0147 -24.9021 4.7 39.7 90.1 10.7054 2.5 9.4 GX 1+4
268.2222 -1.5181 13.4 22.9 124.3 1.3137 0.9 9.6 SW J1753.5-0127
270.4286 -25.1236 6.7 35.5 81.5 5.9796 1.7 8.3 GX 5-1
270.1385 -25.7153 22.4 36.1 81.3 -1.8677 -0.5 9.0 GRS 1758-258
274.0700 -14.0344 14.3 24.7 90.0 1.6258 0.8 3.7 GX 17+2
275.8648 -30.2631 4.0 37.6 70.2 -11.0185 -2.9 7.0 H1820-303
284.9973 -24.9663 6.8 30.1 59.1 -3.6090 -1.7 3.5 HT1900.1-2455
288.8366 10.9333 8.8 6.5 -143.9 1.5314 1.3 2.4 GRS 1915+105
299.5729 35.1828 0.8 31.7 -116.1 25.4901 15.4 1.4 Cyg X-1
307.9244 40.8839 9.7 39.5 -109.5 4.1362 1.2 9.4 Cyg X-3
257.4946 16.7125 2.5 34.4 162.5 8.4181 4.7 ------ UNKNOWN
279.5087 31.3393 2.6 28.6 -150.2 6.2759 4.5 ------ UNKNOWN
320.1096 23.6347 2.8 34.4 -77.0 8.6097 4.1 ------ UNKNOWN
334.3925 17.0688 2.9 44.9 -60.2 24.1733 3.9 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:39:52 EST 2026