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
101.4223 0.7377 0.0103 28.6670 82.0255 2.9995362 18.541 TRIG_01426088
Foreground time interval of the image:
-38.104 27.736 (delta_t = 65.840 [sec])
Background time interval of the image:
-239.864 -38.104 (delta_t = 201.760 [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 -38.104 sec. to 27.736 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.24811 ( -0.131383 0.129703 )
Norm@50keV : 3.09614E-03 ( -0.00023458 0.000234535 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.35 using 59 bins.
Reduced chi-squared = 1.02368
# Null hypothesis probability of 4.26e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 65.84 sec: 0.366080 ( -0.029013 0.029081 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.04136e-06 ( -1.66887e-07 1.67811e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -38.104 sec. to 27.736 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.747676 ( -0.610207 0.533795 )
Epeak [keV] : 135.317 ( -47.0126 -135.317 )
Norm@50keV : 5.33530E-03 ( -0.00228836 0.00478168 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.80 using 59 bins.
Reduced chi-squared = 0.996429
# Null hypothesis probability of 4.82e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 65.84 sec: 0.358251 ( -0.03031 0.030265 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.9824e-06 ( -1.81786e-07 1.8057e-07 ) ergs/cm2
Band function
Time interval is from -38.104 sec. to 27.736 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] : 18.2340 (-1.67561 1.91454)
R^2/D10^2 : 2.27383E-02 (-0.00654874 0.00885911)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 80.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.39e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.924e-08 1.560e-08
25- 50 4.634e-07 5.057e-08
50-150 1.122e-06 1.501e-07
15-150 1.685e-06 1.597e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-18.5804 -200)
Norm : 1.53585 (-0.11799 0.11799)
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.80 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.97e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.518e-07 2.476e-08
25- 50 4.843e-07 5.982e-08
50-150 1.062e-06 3.476e-07
15-150 1.798e-06 3.598e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.53841 (-3.72349 4.51621)
R1^2/D10^2 : 0.149682 (-0.0762933 0.416358)
kT2 [keV] : 28.8360 (-9.45069 102.878)
R2^2/D10^2 : 3.82350E-03 (-0.002603 0.00754932)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.87e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.693e-07 8.703e-08
25- 50 4.688e-07 2.272e-07
50-150 1.299e-06 6.612e-07
15-150 1.937e-06 9.419e-07
Peak spectrum fit
Power-law model
Time interval is from 2.908 sec. to 3.908 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.03949 ( -0.39163 0.370408 )
Norm@50keV : 9.40402E-03 ( -0.00201246 0.00198721 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.78 using 59 bins.
Reduced chi-squared = 1.03123
# Null hypothesis probability of 4.10e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.08530 ( -0.237225 0.23874 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.00314e-07 ( -2.21998e-08 2.23028e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.908 sec. to 3.908 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.03348 ( -1.47142 3.71149 )
Epeak [keV] : 9998.59 ( -9998.58 -9998.58 )
Norm@50keV : 9.45844E-03 ( -0.00198332 0.0260524 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.78 using 59 bins.
Reduced chi-squared = 1.04964
# Null hypothesis probability of 3.74e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.08518 ( -0.241947 0.23852 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.01559e-07 ( -2.37786e-08 2.07955e-08 ) ergs/cm2
Band function
Time interval is from 2.908 sec. to 3.908 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] : 26.3244 (-6.47333 9.73015)
R^2/D10^2 : 2.21221E-02 (-0.0134369 0.0306276)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.38 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.62e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.589e-09 1.321e-09
25- 50 1.507e-08 7.071e-09
50-150 7.674e-08 3.580e-08
15-150 9.440e-08 3.854e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-64.1645 -200)
Norm : 4.51314 (-0.979433 0.979433)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.40 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.34e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.124e-08 6.600e-09
25- 50 2.162e-08 1.232e-08
50-150 4.741e-08 2.710e-08
15-150 8.027e-08 4.639e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.92548 (-1.97165 3.27583)
R1^2/D10^2 : 1.75428 (-1.51913 5.40932)
kT2 [keV] : 34.1764 (-9.7449 22.9447)
R2^2/D10^2 : 9.10687E-03 (-0.00689131 0.0130233)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.64 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.50e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.567e-09 6.275e-09
25- 50 1.772e-08 9.890e-09
50-150 7.760e-08 4.472e-08
15-150 1.049e-07 5.725e-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: 1.24811 ( -0.131383 0.129703 )
Norm@50keV : 3.09614E-03 ( -0.00023458 0.000234535 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.35 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.26e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 65.84 sec: 0.366078 ( -0.0290119 0.0290785 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.04114e-06 ( -1.67108e-07 1.6781e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.747673 ( -0.610204 0.533797 )
Epeak [keV] : 135.317 ( -47.0122 -135.317 )
Norm@50keV : 5.33532E-03 ( -0.00228803 0.00478166 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.80 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.82e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 65.84 sec: 0.358227 ( -0.030303 0.030269 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.98324e-06 ( -1.82186e-07 1.80704e-07 ) 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) = 4.41e-07
S(50-100 keV) = 7.44e-07
T90 vs. Hardness ratio plot
T90 = 56.864000082016 sec.
Hardness ratio (energy fluence ratio) = 1.68707
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.78774
Count Ratio (50-100 keV) / (15-25 keV) = 1.66813
Mask shadow pattern
IMX = 7.584960979595232E-02, IMY = -5.414494923853239E-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:
-239.864000 -38.104000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5715 -40.6025 7.4 29.8 -44.4 0.5757 1.6 3.5 Vela X-1
123.9868 31.1749 2.2 43.0 143.8 4.0232 5.3 ------ UNKNOWN
168.1186 -25.7933 2.6 40.8 -95.8 6.2776 4.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-38.104000 27.736000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6319 -40.5657 5.1 29.8 -44.5 0.3071 2.2 4.8 Vela X-1
101.4223 0.7377 0.6 28.7 82.0 2.9987 18.6 ------ UNKNOWN
108.4376 -46.6094 2.5 38.4 -10.8 0.6771 4.6 ------ UNKNOWN
124.9006 -32.7352 2.4 21.2 -26.0 0.4778 4.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
119.836570 962.216000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6171 22.0329 0.6 27.4 78.3 34.3602 19.5 1.4 Crab
65.1104 -7.5688 2.8 37.1 12.6 7.0479 4.2 ------ UNKNOWN
96.0068 -17.6157 2.7 19.1 -48.0 5.1116 4.3 ------ UNKNOWN
148.5026 -3.7379 3.0 47.3 -148.0 9.8156 3.8 ------ UNKNOWN
156.0112 -6.5088 2.7 55.0 -145.3 26.2142 4.2 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:10:09 EST 2026