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
128.1635 21.8093 0.0111 13.7224 106.4976 0.7636468 17.363 TRIG_01402466
Foreground time interval of the image:
-0.036 10.973 (delta_t = 11.009 [sec])
Background time interval of the image:
-108.027 -0.036 (delta_t = 107.991 [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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
8 ms binning
From T100_start-3 s to T100_start+3 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
2 ms binning
From T100_start-1 s to T100_start+1 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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 -0.036 sec. to 103.196 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33703 ( -0.0327995 0.032703 )
Norm@50keV : 1.02003E-02 ( -0.000176437 0.000176157 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.10 using 59 bins.
Reduced chi-squared = 0.773684
# Null hypothesis probability of 8.94e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 103.2 sec: 1.22563 ( -0.02435 0.02446 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.03126e-05 ( -1.76325e-07 1.76504e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.036 sec. to 103.196 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33300 ( -0.109278 0.054865 )
Epeak [keV] : 9997.75 ( -9997.66 -9997.66 )
Norm@50keV : 1.02402E-02 ( -0.000174417 0.00152117 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.07 using 59 bins.
Reduced chi-squared = 0.786964
# Null hypothesis probability of 8.76e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 103.2 sec: 1.22332 ( -0.02624 0.02208 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.03031e-05 ( -2.17595e-07 2.07021e-07 ) ergs/cm2
Band function
Time interval is from -0.036 sec. to 103.196 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] : 20.2146 ( )
R^2/D10^2 : 5.01040E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 770.26 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.31e-125 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.056e-07 1.507e-08
25- 50 2.034e-06 5.624e-08
50-150 6.172e-06 1.367e-07
15-150 8.612e-06 1.589e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 5.26444 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 237.08 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.03e-24 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.353e-06 2.580e-08
25- 50 2.602e-06 5.315e-08
50-150 5.707e-06 1.073e-07
15-150 9.663e-06 1.796e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.39673 (-0.532318 0.558922)
R1^2/D10^2 : 0.622228 (-0.120025 0.156265)
kT2 [keV] : 34.2104 (-2.21977 2.69306)
R2^2/D10^2 : 7.28570E-03 (-0.00159733 0.00183563)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.35e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.732e-07 6.213e-08
25- 50 2.430e-06 8.669e-08
50-150 6.865e-06 2.492e-07
15-150 1.027e-05 2.843e-07
Peak spectrum fit
Power-law model
Time interval is from 56.140 sec. to 57.140 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.04958 ( -0.0563609 0.0561499 )
Norm@50keV : 8.13829E-02 ( -0.00257401 0.00257246 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.71 using 59 bins.
Reduced chi-squared = 0.889649
# Null hypothesis probability of 7.09e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 9.39914 ( -0.30377 0.30396 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.65167e-07 ( -3.03332e-08 3.03833e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 56.140 sec. to 57.140 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.834727 ( -0.226907 0.111285 )
Epeak [keV] : 312.886 ( -130.418 8494.76 )
Norm@50keV : 0.101381 ( -0.0167511 0.0255676 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.82 using 59 bins.
Reduced chi-squared = 0.853929
# Null hypothesis probability of 7.73e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 9.31018 ( -0.31592 0.31602 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.56387e-07 ( -3.19262e-08 3.18114e-08 ) ergs/cm2
Band function
Time interval is from 56.140 sec. to 57.140 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] : 21.4910 ( )
R^2/D10^2 : 0.357399 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 213.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.01e-20 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.087e-08 2.070e-09
25- 50 1.610e-07 7.050e-09
50-150 5.550e-07 2.945e-08
15-150 7.468e-07 3.070e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 38.2117 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 263.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.11e-28 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.515e-08 3.325e-09
25- 50 1.830e-07 5.850e-09
50-150 4.014e-07 1.360e-08
15-150 6.796e-07 2.320e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.87529 (-1.13183 1.3256)
R1^2/D10^2 : 4.47259 (-1.66563 2.93787)
kT2 [keV] : 32.7521 (-3.34096 4.82281)
R2^2/D10^2 : 8.24954E-02 (-0.0295082 0.0350788)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.81e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.266e-08 7.670e-09
25- 50 1.680e-07 1.505e-08
50-150 6.300e-07 5.865e-08
15-150 8.607e-07 7.255e-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: 1.91012 ( -0.152414 0.158684 )
Norm@50keV : 3.65451E-03 ( -0.000387918 0.000382011 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.13 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.48e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 11.01 sec: 0.526727 ( -0.0460821 0.0460921 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.69961e-07 ( -3.8257e-08 3.88311e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.737037 ( -0.891098 0.736256 )
Epeak [keV] : 44.9065 ( -7.22861 12.5117 )
Norm@50keV : 1.73182E-02 ( -0.0107026 0.0398382 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.69e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 11.01 sec: 0.506288 ( -0.047431 0.047573 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.32444e-07 ( -4.05333e-08 4.33761e-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) = 2.34e-06
S(50-100 keV) = 3.72e-06
T90 vs. Hardness ratio plot
T90 = 64.1279999017715 sec.
Hardness ratio (energy fluence ratio) = 1.58974
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.51044
Count Ratio (50-100 keV) / (15-25 keV) = 1.27358
Mask shadow pattern
IMX = -6.934296015940583E-02, IMY = -2.341345257147898E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-108.027390 -0.036000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5763 -40.5318 8.1 56.1 -8.8 0.8332 1.4 2.6 Vela X-1
115.3106 -28.7802 2.3 50.6 15.7 2.0000 5.1 ------ UNKNOWN
139.9836 -14.6013 3.5 29.9 -11.9 0.5870 3.3 ------ UNKNOWN
139.9733 -37.6445 3.4 53.0 -12.8 1.3733 3.5 ------ UNKNOWN
197.9402 57.0044 4.1 59.5 -161.7 3.0497 2.8 ------ UNKNOWN
168.6827 1.8503 2.9 30.5 -80.2 0.9026 4.0 ------ UNKNOWN
197.0827 42.5993 2.6 55.0 -145.4 3.7864 4.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.036000 10.972590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.3973 -40.5734 3.4 56.1 -8.6 -0.5240 -3.4 6.1 Vela X-1
125.5509 16.3336 2.2 14.8 82.4 0.2109 5.2 ------ UNKNOWN
128.1635 21.8092 0.7 13.7 106.5 0.7636 17.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
57.572590 302.604000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
128.1544 21.8201 0.4 0.0 98.8 10.1466 31.7 ------ UNKNOWN
142.7160 23.0354 3.0 13.5 -113.1 1.3333 3.8 ------ UNKNOWN
135.8471 -31.3528 2.8 53.7 -23.3 4.5807 4.1 ------ UNKNOWN
140.6108 -34.4191 2.4 57.5 -27.3 8.9756 4.8 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:19:26 EST 2026