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
80.9626 33.0676 0.0172 13.0893 159.6101 1.3543795 11.128 TRIG_01299967
Foreground time interval of the image:
-12.588 66.668 (delta_t = 79.256 [sec])
Background time interval of the image:
-239.000 -12.588 (delta_t = 226.412 [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 -12.588 sec. to 66.668 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.88284 ( -0.220071 0.232184 )
Norm@50keV : 9.04940E-04 ( -0.000141931 0.000138617 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.73 using 59 bins.
Reduced chi-squared = 0.925088
# Null hypothesis probability of 6.36e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 79.26 sec: 0.128941 ( -0.01613 0.01613 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.59484e-07 ( -1.00622e-07 1.03269e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -12.588 sec. to 66.668 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00506 ( -1.48801 1.04628 )
Epeak [keV] : 44.7916 ( -34.4263 -44.7862 )
Norm@50keV : 3.04793E-03 ( -0.00305051 0.0219488 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.81 using 59 bins.
Reduced chi-squared = 0.907321
# Null hypothesis probability of 6.71e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 79.26 sec: 0.125337 ( -0.016712 0.016736 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.93532e-07 ( -1.14853e-07 1.29394e-07 ) ergs/cm2
Band function
Time interval is from -12.588 sec. to 66.668 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] : 9.84750 (-1.26837 1.47637)
R^2/D10^2 : 6.59792E-02 (-0.0273094 0.0454986)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.58e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.027e-07 2.131e-08
25- 50 2.499e-07 3.911e-08
50-150 1.247e-07 4.376e-08
15-150 4.773e-07 7.169e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 74.6017 (-24.9968 49.7091)
Norm : 0.624984 (-0.110439 0.136151)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.94 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.01e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.279e-07 2.291e-08
25- 50 2.069e-07 2.952e-08
50-150 2.783e-07 1.289e-07
15-150 6.130e-07 1.364e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.20606 (-3.88154 1.6566)
R1^2/D10^2 : 0.115708 (-0.0558766 0.0818694)
kT2 [keV] : 44.4089 (-35.7731 -48.3357)
R2^2/D10^2 : 1.71087E-04 (-0.000131143 0.0209082)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.55 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.82e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.169e-07 4.585e-08
25- 50 2.304e-07 8.065e-08
50-150 3.017e-07 1.569e-07
15-150 6.490e-07 2.298e-07
Peak spectrum fit
Power-law model
Time interval is from -3.192 sec. to -2.192 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.33702 ( -1.06244 0.990949 )
Norm@50keV : 2.62305E-03 ( -0.00121554 0.00114955 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.02 using 59 bins.
Reduced chi-squared = 1.03544
# Null hypothesis probability of 4.02e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.315141 ( -0.315141 0.143784 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.57022e-08 ( -1.27062e-08 1.29648e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -3.192 sec. to -2.192 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.23474 ( -1.27004 0.964562 )
Epeak [keV] : 334.556 ( -9999.36 -9999.36 )
Norm@50keV : 3.39468E-04 ( -0.000339367 0.0107487 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.25 using 59 bins.
Reduced chi-squared = 1.04018
# Null hypothesis probability of 3.92e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.317909 ( -0.145771 0.143134 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.54466e-08 ( -1.26106e-08 1.33604e-08 ) ergs/cm2
Band function
Time interval is from -3.192 sec. to -2.192 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] : 29.0112 (-29.1155 99.208)
R^2/D10^2 : 4.10646E-03 (-0.00405324 1.03968)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.02 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.02e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.267e-09 2.277e-09
25- 50 6.338e-09 4.361e-09
50-150 2.026e-09 1.713e-09
15-150 1.163e-08 8.620e-09
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.361 (-199.362 -199.362)
Norm : 1.29388 (-0.576632 0.576619)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.82e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.222e-09 2.156e-09
25- 50 6.198e-09 3.997e-09
50-150 1.359e-08 8.535e-09
15-150 2.301e-08 1.475e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.59469 (-3.48537 5.49193)
R1^2/D10^2 : 0.986943 (-0.925507 126.597)
kT2 [keV] : 46.8052 (-46.9862 -46.9864)
R2^2/D10^2 : 9.82294E-04 (-0.000941269 0.00276273)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.93e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.933e-09 2.491e-09
25- 50 4.903e-09 2.971e-09
50-150 2.032e-08 1.265e-08
15-150 2.915e-08 1.495e-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: 1.88284 ( -0.220071 0.232184 )
Norm@50keV : 9.04940E-04 ( -0.000141931 0.000138617 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.36e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 79.26 sec: 0.128933 ( -0.016129 0.0161292 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.5937e-07 ( -1.00549e-07 1.03304e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00849 ( -1.48955 1.04479 )
Epeak [keV] : 44.8279 ( -17.0173 -44.7934 )
Norm@50keV : 3.03280E-03 ( -0.00304917 0.0219515 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.71e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 79.26 sec: 0.125313 ( -0.016706 0.016731 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.93657e-07 ( -1.14903e-07 1.29497e-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) = 1.91e-07
S(50-100 keV) = 2.08e-07
T90 vs. Hardness ratio plot
T90 = 70.0999999046326 sec.
Hardness ratio (energy fluence ratio) = 1.08901
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.03221
Count Ratio (50-100 keV) / (15-25 keV) = 0.478663
Mask shadow pattern
IMX = -2.179413595156088E-01, IMY = -8.100799413055473E-02
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:
-239.000000 -12.588000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6417 22.0190 0.5 24.0 168.7 9.1390 24.5 0.5 Crab
332.2933 59.2657 2.9 57.5 -19.1 5.3423 3.9 ------ UNKNOWN
47.1085 2.3827 2.4 46.7 -128.0 7.5763 4.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-12.588000 66.668000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7659 22.0697 5.8 24.0 168.4 -0.2638 -2.0 8.1 Crab
80.9625 33.0676 1.0 13.1 159.6 1.3544 11.1 ------ UNKNOWN
80.2457 14.5385 2.0 30.2 -179.6 0.7666 5.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
118.900600 963.071500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6335 22.0215 0.4 11.3 174.4 33.3754 28.8 0.4 Crab
131.1265 56.1845 2.6 41.2 47.5 13.0586 4.4 ------ UNKNOWN
118.9458 82.1085 2.4 50.9 13.3 10.8931 4.7 ------ UNKNOWN
Plot creation:
Fri Jun 20 01:43:28 EDT 2025