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
106.7755 7.1966 0.0117 14.4746 165.8012 0.2048283 16.347 TRIG_01297832
Foreground time interval of the image:
0.000 0.672 (delta_t = 0.672 [sec])
Background time interval of the image:
-239.128 0.000 (delta_t = 239.128 [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 0.064000
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 0.064000
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 0.064000
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 0.000 sec. to 0.672 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.651269 ( -0.192811 0.18078 )
Norm@50keV : 1.73790E-02 ( -0.00202864 0.00199605 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 74.85 using 59 bins.
Reduced chi-squared = 1.31316
# Null hypothesis probability of 5.65e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.672 sec: 2.01758 ( -0.22036 0.22089 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.45787e-07 ( -1.63617e-08 1.64235e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 0.672 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.55048E-02 ( -0.910639 0.700049 )
Epeak [keV] : 183.400 ( -75.633 -183.45 )
Norm@50keV : 3.29616E-02 ( -0.016386 0.0458304 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.78 using 59 bins.
Reduced chi-squared = 1.29964
# Null hypothesis probability of 6.53e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.672 sec: 1.98538 ( -0.22425 0.22436 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.41684e-07 ( -1.79982e-08 1.75184e-08 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 0.672 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] : 26.0854 (-3.78188 4.95254)
R^2/D10^2 : 4.69969E-02 (-0.0186131 0.0280757)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.68 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.01e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.648e-09 7.694e-10
25- 50 2.114e-08 4.005e-09
50-150 1.059e-07 2.073e-08
15-150 1.307e-07 2.060e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 7.41576 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 136.94 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.58e-08 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.241e-08 6.918e-09
25- 50 2.387e-08 1.319e-08
50-150 5.235e-08 2.885e-08
15-150 8.863e-08 4.885e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 16.2235 (-5.50192 4.56887)
R1^2/D10^2 : 0.138568 (-0.0586208 0.129771)
kT2 [keV] : 200.000 (-157.903 -200)
R2^2/D10^2 : 3.95476E-04 (-0.000161206 0.0022548)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.96 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.13e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.466e-09 3.211e-09
25- 50 2.414e-08 1.389e-08
50-150 1.084e-07 5.779e-08
15-150 1.380e-07 7.431e-08
Peak spectrum fit
Power-law model
Time interval is from -0.162 sec. to 0.838 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.613380 ( -0.214977 0.198976 )
Norm@50keV : 1.21101E-02 ( -0.00156494 0.00152755 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.25 using 59 bins.
Reduced chi-squared = 1.19737
# Null hypothesis probability of 1.46e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.41166 ( -0.16585 0.1665 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.5389e-07 ( -1.79836e-08 1.80393e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.162 sec. to 0.838 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.211956 ( -0.953025 0.51682 )
Epeak [keV] : 268.465 ( -268.596 -268.596 )
Norm@50keV : 1.79563E-02 ( -0.00702596 0.025521 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.53 using 59 bins.
Reduced chi-squared = 1.20589
# Null hypothesis probability of 1.39e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.39737 ( -0.16814 0.16876 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.51555e-07 ( -1.93006e-08 1.88177e-08 ) ergs/cm2
Band function
Time interval is from -0.162 sec. to 0.838 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] : 27.7831 (-4.45013 6.14709)
R^2/D10^2 : 2.73961E-02 (-0.0118475 0.0185508)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 74.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.38e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.464e-09 8.945e-10
25- 50 2.067e-08 4.365e-09
50-150 1.157e-07 2.137e-08
15-150 1.398e-07 2.510e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 ( )
Norm : 5.31087 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 126.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.08e-07 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.322e-08 7.455e-09
25- 50 2.544e-08 1.415e-08
50-150 5.579e-08 3.132e-08
15-150 9.446e-08 5.270e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 15.8850 (-3.84455 4.61413)
R1^2/D10^2 : 9.85979E-02 (-0.0445981 0.0958478)
kT2 [keV] : 200.000 (-6.48334 -200)
R2^2/D10^2 : 3.05922E-04 (-0.000115614 0.00161087)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.21e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.656e-09 3.233e-09
25- 50 2.478e-08 1.430e-08
50-150 1.209e-07 9.140e-08
15-150 1.514e-07 8.475e-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: 0.651269 ( -0.192811 0.18078 )
Norm@50keV : 1.73790E-02 ( -0.00202864 0.00199605 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 74.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.65e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.672 sec: 2.01761 ( -0.220345 0.2209 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.45772e-07 ( -1.63586e-08 1.64252e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.58554E-02 ( -0.910749 0.699938 )
Epeak [keV] : 183.500 ( -75.7549 -183.456 )
Norm@50keV : 3.29461E-02 ( -0.0163858 0.045832 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.78 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.53e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.672 sec: 1.98541 ( -0.22424 0.22429 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.41758e-07 ( -1.80042e-08 1.75251e-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) = 2.10e-08
S(50-100 keV) = 5.36e-08
T90 vs. Hardness ratio plot
T90 = 0.623999953269958 sec.
Hardness ratio (energy fluence ratio) = 2.55238
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 2.99481
Count Ratio (50-100 keV) / (15-25 keV) = 3.26648
Mask shadow pattern
IMX = -2.502594187900978E-01, IMY = -6.331959160498919E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
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:
-239.128000 0.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6377 22.0177 0.5 17.8 -81.9 9.5346 23.8 0.3 Crab
129.1510 -16.3541 2.3 45.6 145.2 5.7394 4.9 ------ UNKNOWN
134.4640 29.3759 3.1 29.7 69.3 2.2008 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 0.672000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6053 22.0103 3.9 17.8 -81.9 -0.0399 -3.0 1.6 Crab
106.7755 7.1966 0.7 14.5 165.8 0.2048 16.3 ------ UNKNOWN
102.4844 -30.0240 1.9 51.2 -177.8 0.1928 6.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
55.772610 716.176200
720.872000 962.992000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6512 22.0255 0.5 26.7 -56.5 36.0869 24.3 1.2 Crab
93.2892 -39.1434 3.1 48.0 -168.6 10.1226 3.7 ------ UNKNOWN
72.4751 14.8105 2.4 34.4 -76.9 10.7029 4.7 ------ UNKNOWN
72.0748 21.4529 1.8 36.3 -65.9 15.3491 6.5 ------ UNKNOWN
Plot creation:
Fri Jun 20 01:46:52 EDT 2025