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
306.6685 -68.5817 0.0235 22.2311 -41.1269 0.7268737 8.193 TRIG_01406589
Foreground time interval of the image:
1.160 53.685 (delta_t = 52.525 [sec])
Background time interval of the image:
-239.816 1.160 (delta_t = 240.976 [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 1.160 sec. to 97.280 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.58323 ( -0.289539 0.296559 )
Norm@50keV : 7.32588E-04 ( -0.000126238 0.000123481 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.73 using 59 bins.
Reduced chi-squared = 1.10053
# Null hypothesis probability of 2.80e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 96.12 sec: 9.36616E-02 ( -0.015031 0.0150564 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.60015e-07 ( -1.21901e-07 1.24162e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.160 sec. to 97.280 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.59061 ( -0.502456 0.291213 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 7.30450E-04 ( -0.000126058 0.00110261 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.74 using 59 bins.
Reduced chi-squared = 1.12036
# Null hypothesis probability of 2.50e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 96.12 sec: 9.41086E-02 ( -0.0173923 0.0165024 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.70878e-07 ( -1.34892e-07 1.11224e-07 ) ergs/cm2
Band function
Time interval is from 1.160 sec. to 97.280 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] : 12.6011 (-3.12003 4.56266)
R^2/D10^2 : 1.85595E-02 (-0.0181873 0.0332038)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 79.70 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.52e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.007e-08 2.180e-08
25- 50 1.999e-07 5.676e-08
50-150 1.970e-07 7.089e-08
15-150 4.570e-07 1.293e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 197.935 (-110.267 -198.1)
Norm : 0.378853 (-0.0601667 0.0749549)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.56e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.076e-08 5.195e-08
25- 50 1.744e-07 9.708e-08
50-150 3.817e-07 2.160e-07
15-150 6.469e-07 3.578e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.47007 (-1.67665 2.26747)
R1^2/D10^2 : 0.163800 (-0.108378 0.216808)
kT2 [keV] : 34.2466 (-13.0267 77.4165)
R2^2/D10^2 : 5.02115E-04 (-0.000459711 0.00185874)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.92e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.050e-07 5.578e-08
25- 50 1.661e-07 8.966e-08
50-150 4.243e-07 2.365e-07
15-150 6.954e-07 3.639e-07
Peak spectrum fit
Power-law model
Time interval is from 2.156 sec. to 3.156 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.84396 ( -0.73987 0.8949 )
Norm@50keV : 3.65542E-03 ( -0.00177698 0.001438 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.58 using 59 bins.
Reduced chi-squared = 0.975088
# Null hypothesis probability of 5.29e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.512588 ( -0.16014 0.160122 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.35977e-08 ( -1.41571e-08 1.47638e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.156 sec. to 3.156 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.88662 ( -1.8269 0.571446 )
Epeak [keV] : 454.186 ( -72.2712 227.517 )
Norm@50keV : 4.13641E-04 ( -0.000412112 0.00272238 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.34 using 59 bins.
Reduced chi-squared = 0.934643
# Null hypothesis probability of 6.14e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.403831 ( -0.249744 0.236918 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.68751e-08 ( -1.62229e-08 8.40014e-09 ) ergs/cm2
Band function
Time interval is from 2.156 sec. to 3.156 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] : 5.89850 (-2.19078 4.80449)
R^2/D10^2 : 1.71618 (-1.71042 11.8977)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.01e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.739e-09 4.730e-09
25- 50 7.434e-09 4.854e-09
50-150 6.344e-10 6.430e-10
15-150 1.581e-08 9.740e-09
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 196.094 (-196.179 -196.179)
Norm : 2.00005 (-0.644854 2.46199)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.67e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.991e-09 3.138e-09
25- 50 9.582e-09 5.845e-09
50-150 2.090e-08 1.269e-08
15-150 3.547e-08 2.049e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.03226 (-1.90177 1.19851)
R1^2/D10^2 : 3.15547 (-2.63786 14.8049)
kT2 [keV] : 198.612 (-168.366 -198.707)
R2^2/D10^2 : 1.04499E-04 (-5.04497e-05 0.00402839)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.62e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.007e-09 4.805e-09
25- 50 6.356e-09 3.499e-09
50-150 2.775e-08 7.340e-09
15-150 4.211e-08 1.175e-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: 1.66530 ( -0.274968 0.285952 )
Norm@50keV : 1.10167E-03 ( -0.000181863 0.000176379 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.04 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.97e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 52.52 sec: 0.144585 ( -0.0213505 0.0213755 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.37322e-07 ( -9.30287e-08 9.47056e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.07951 ( -0.28805 0.277298 )
Epeak [keV] : 31.8198 ( -9999.35 -9999.36 )
Norm@50keV : 6.73017E-04 ( -0.000173462 0.000207572 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.57 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.80e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 52.52 sec: 0.144857 ( -0.021636 0.021147 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.36334e-07 ( -9.18002e-08 9.57019e-08 ) 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) = 1.70e-07
S(50-100 keV) = 2.27e-07
T90 vs. Hardness ratio plot
T90 = 82.2279999256134 sec.
Hardness ratio (energy fluence ratio) = 1.33529
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.00071
Count Ratio (50-100 keV) / (15-25 keV) = 0.825661
Mask shadow pattern
IMX = 3.078752382860304E-01, IMY = 2.688310232903821E-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:
-239.816000 1.160000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4161 -40.5263 4.1 58.6 -159.0 5.4113 2.8 5.4 Vela X-1
170.6078 -60.5609 8.6 44.9 -125.5 1.7500 1.3 9.4 Cen X-3
342.4778 -50.2607 3.2 27.5 20.0 1.3154 3.6 ------ UNKNOWN
304.3209 -36.0009 3.1 51.0 -13.2 2.3326 3.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
1.160000 53.684600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6524 -40.5489 5.9 58.7 -158.8 -0.8859 -1.9 5.7 Vela X-1
170.3713 -60.7529 17.0 44.7 -125.6 0.2080 0.7 8.0 Cen X-3
306.6700 -68.5818 1.4 22.2 -41.1 0.7270 8.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
111.884600 655.384600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.4907 -60.7203 8.4 46.9 -141.1 2.1676 1.4 7.8 Cen X-3
186.6580 -62.7717 27.9 41.9 -132.3 0.5894 0.4 0.1 GX 301-2
255.9550 -37.8111 30.3 41.1 -57.1 -0.6754 -0.4 2.5 4U 1700-377
256.3658 -36.5349 27.4 42.1 -55.9 -0.8105 -0.4 7.5 GX 349+2
262.8073 -24.7855 6.9 51.0 -42.7 5.7559 1.7 11.2 GX 1+4
264.9631 -44.3713 4.2 32.2 -51.8 2.5825 2.7 10.6 4U 1735-44
270.1338 -25.1472 3.7 48.6 -34.6 -5.3229 -3.1 9.1 GX 5-1
270.2353 -25.8719 7.7 47.9 -34.8 2.4147 1.5 8.5 GRS 1758-258
275.9634 -30.4053 7.6 42.1 -29.7 1.6582 1.5 3.0 H1820-303
285.0424 -24.7943 9.5 45.7 -16.6 1.5315 1.2 7.6 HT1900.1-2455
263.1350 -33.7371 3.5 42.5 -46.7 4.9050 3.2 9.3 GX 354-0
277.6212 -39.4333 2.1 33.1 -32.1 4.7148 5.5 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:15:02 EST 2026