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
74.5994 -7.9943 0.0091 40.4946 20.1071 0.5870971 21.252 TRIG_01440319
Foreground time interval of the image:
0.316 0.740 (delta_t = 0.424 [sec])
Background time interval of the image:
-239.008 0.316 (delta_t = 239.324 [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 0.316 sec. to 0.740 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.583056 ( -0.151717 0.146353 )
Norm@50keV : 8.38619E-02 ( -0.0074087 0.00730321 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.44 using 59 bins.
Reduced chi-squared = 1.00772
# Null hypothesis probability of 4.59e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.424 sec: 9.81201 ( -0.80212 0.80289 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.58484e-07 ( -4.02533e-08 4.04073e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.316 sec. to 0.740 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.577618 ( -0.548454 0.145315 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 8.46329E-02 ( -0.00698601 0.0533875 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.45 using 59 bins.
Reduced chi-squared = 1.02589
# Null hypothesis probability of 4.21e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.424 sec: 0.565715 ( -0.565715 0.397072 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.58675e-07 ( -4.17133e-08 3.25677e-08 ) ergs/cm2
Band function
Time interval is from 0.316 sec. to 0.740 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] : 30.7681 (-3.7864 4.73576)
R^2/D10^2 : 0.145324 (-0.0464549 0.0636918)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 77.96 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.40e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.984e-09 1.503e-09
25- 50 5.599e-08 7.696e-09
50-150 3.706e-07 4.842e-08
15-150 4.355e-07 5.368e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 34.4606 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 165.29 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.76e-12 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.638e-08 1.996e-08
25- 50 6.999e-08 3.797e-08
50-150 1.535e-07 8.344e-08
15-150 2.599e-07 1.410e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.7620 (-3.56949 5.52724)
R1^2/D10^2 : 1.44732 (-0.898743 2.94485)
kT2 [keV] : 56.9826 (-19.1479 -57.8858)
R2^2/D10^2 : 2.53455E-02 (-0.0166325 0.0458495)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.17e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.822e-08 9.439e-09
25- 50 6.614e-08 3.242e-08
50-150 3.774e-07 2.013e-07
15-150 4.617e-07 2.260e-07
Peak spectrum fit
Power-law model
Time interval is from 0.030 sec. to 1.030 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.669572 ( -0.174311 0.1668 )
Norm@50keV : 3.67051E-02 ( -0.00365761 0.00358933 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.06 using 59 bins.
Reduced chi-squared = 1.03614
# Null hypothesis probability of 4.00e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.251652 ( -0.059343 0.242745 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.54329e-07 ( -4.33118e-08 4.34883e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.030 sec. to 1.030 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.664594 ( -0.269941 0.165065 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 3.70283E-02 ( -0.00344493 0.0206369 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.08 using 59 bins.
Reduced chi-squared = 1.055
# Null hypothesis probability of 3.64e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.26243 ( -0.42867 0.41881 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.55596e-07 ( -4.46734e-08 4.21296e-08 ) ergs/cm2
Band function
Time interval is from 0.030 sec. to 1.030 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] : 30.5247 (-4.14938 5.34545)
R^2/D10^2 : 6.24099E-02 (-0.0223347 0.0320976)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.94e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.000e-09 1.642e-09
25- 50 5.591e-08 8.730e-09
50-150 3.654e-07 5.365e-08
15-150 4.304e-07 5.985e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 16.2156 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 133.40 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.59e-08 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.038e-08 2.230e-08
25- 50 7.767e-08 4.224e-08
50-150 1.703e-07 9.225e-08
15-150 2.884e-07 1.577e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.43681 (-3.04218 4.36514)
R1^2/D10^2 : 1.00532 (-0.653383 2.48869)
kT2 [keV] : 51.5995 (-14.9299 68.5506)
R2^2/D10^2 : 1.37049E-02 (-0.00974172 0.0205884)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.68e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.171e-08 1.195e-08
25- 50 6.903e-08 3.294e-08
50-150 3.743e-07 1.910e-07
15-150 4.650e-07 2.169e-07
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: 0.583056 ( -0.151717 0.146353 )
Norm@50keV : 8.38619E-02 ( -0.0074087 0.00730321 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.44 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.59e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.424 sec: 9.81212 ( -0.802112 0.802935 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.58437e-07 ( -4.03123e-08 4.04449e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.576794 ( -0.547898 0.145783 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 8.46145E-02 ( -0.00698242 0.0533901 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.21e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.424 sec: 9.81271 ( -0.80384 0.78819 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.58454e-07 ( -4.01469e-08 4.06616e-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) = 6.28e-08
S(50-100 keV) = 1.68e-07
T90 vs. Hardness ratio plot
T90 = 0.363999962806702 sec.
Hardness ratio (energy fluence ratio) = 2.67516
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 2.54197
Count Ratio (50-100 keV) / (15-25 keV) = 3.92354
Mask shadow pattern
IMX = 8.018736972878737E-01, IMY = -2.935572950306746E-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:
-239.008000 0.316000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.4964 -40.5520 1.0 22.4 -156.5 3.8758 11.9 1.5 Vela X-1
170.3115 -60.5540 38.8 48.5 -132.3 0.4465 0.3 4.1 Cen X-3
160.6116 -15.2510 2.2 48.7 165.1 4.9070 5.3 ------ UNKNOWN
67.5949 -22.5614 3.0 38.6 -5.0 1.7123 3.9 ------ UNKNOWN
173.5608 -54.4103 2.3 49.8 -140.6 5.3834 5.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.316000 0.740000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.7411 -40.6706 0.0 22.6 -156.4 -0.0278 -1.9 11.9 Vela X-1
170.3177 -60.6220 101.2 48.5 -132.3 -0.0069 -0.1 0.1 Cen X-3
101.0555 -7.6414 2.5 25.3 61.0 0.0975 4.6 ------ UNKNOWN
74.5994 -7.9944 0.5 40.5 20.1 0.5871 21.3 ------ UNKNOWN
52.4969 -35.8416 2.3 47.5 -29.3 0.1641 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
105.292580 963.042000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6621 22.0203 0.7 31.3 52.9 33.3359 17.8 1.6 Crab
119.5102 -33.6810 2.0 48.6 165.1 18.4501 5.8 ------ UNKNOWN
56.4821 -53.6715 2.2 48.0 -129.1 26.5543 5.2 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:07:27 EST 2026