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
54.1505 27.1463 0.0061 31.9898 36.9517 9.2384534 31.393 TRIG_01200812
Foreground time interval of the image:
-16.899 72.901 (delta_t = 89.800 [sec])
Background time interval of the image:
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 -31.000 sec. to 81.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.39231 ( -0.0572663 0.0571092 )
Norm@50keV : 6.96323E-03 ( -0.000210158 0.000210103 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.81 using 59 bins.
Reduced chi-squared = 0.698421
# Null hypothesis probability of 9.59e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 112 sec: 0.846538 ( -0.028379 0.028512 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.54863e-06 ( -2.3879e-07 2.39047e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -31.000 sec. to 81.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38885 ( -0.169389 0.139783 )
Epeak [keV] : 9998.76 ( -9998.76 -9998.76 )
Norm@50keV : 6.98848E-03 ( -0.000210545 0.00152295 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.82 using 59 bins.
Reduced chi-squared = 0.711071
# Null hypothesis probability of 9.50e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 112 sec: 0.847495 ( -0.033044 0.029149 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.55559e-06 ( -2.63228e-07 1.28071e-07 ) ergs/cm2
Band function
Time interval is from -31.000 sec. to 81.000 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] : 18.5241 ( )
R^2/D10^2 : 4.58957E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 303.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.57e-35 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.498e-07 2.302e-08
25- 50 1.652e-06 7.448e-08
50-150 4.144e-06 2.044e-07
15-150 6.147e-06 2.173e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-5.64667 -200)
Norm : 3.54907 (-0.107527 0.107527)
------------------------------------------------------------
#Fit statistic : Chi-Squared 77.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.86e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.901e-07 3.718e-08
25- 50 1.905e-06 6.496e-08
50-150 4.177e-06 1.434e-07
15-150 7.072e-06 2.425e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.40143 (-0.784412 0.858387)
R1^2/D10^2 : 0.690882 (-0.217057 0.344467)
kT2 [keV] : 31.0816 (-3.02708 4.02397)
R2^2/D10^2 : 6.76199E-03 (-0.00224163 0.00284557)
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.88e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.309e-07 8.742e-08
25- 50 1.795e-06 1.372e-07
50-150 4.932e-06 3.724e-07
15-150 7.558e-06 5.432e-07
Peak spectrum fit
Power-law model
Time interval is from -7.500 sec. to -6.500 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.24754 ( -0.228285 0.220897 )
Norm@50keV : 1.58141E-02 ( -0.00221235 0.00221235 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.37 using 59 bins.
Reduced chi-squared = 1.04158
# Null hypothesis probability of 3.89e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.86965 ( -0.26955 0.27011 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.58387e-07 ( -2.39496e-08 2.4116e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -7.500 sec. to -6.500 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.578462 ( -1.19231 0.771893 )
Epeak [keV] : 104.474 ( -41.0215 -104.498 )
Norm@50keV : 3.53781E-02 ( -0.020989 0.112507 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.93 using 59 bins.
Reduced chi-squared = 1.03446
# Null hypothesis probability of 4.04e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.84533 ( -0.27216 0.27253 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.50845e-07 ( -2.72872e-08 2.66352e-08 ) ergs/cm2
Band function
Time interval is from -7.500 sec. to -6.500 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] : 15.4788 (-2.4773 3.24301)
R^2/D10^2 : 0.207827 (-0.100776 0.174087)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.18e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.037e-08 2.943e-09
25- 50 4.238e-08 9.090e-09
50-150 7.004e-08 1.684e-08
15-150 1.228e-07 2.420e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-48.4006 -200)
Norm : 7.81244 (-1.10791 1.10791)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.99 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.73e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.945e-08 1.106e-08
25- 50 3.742e-08 2.112e-08
50-150 8.207e-08 4.650e-08
15-150 1.390e-07 7.855e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 11.2994 (-2.14566 2.7891)
R1^2/D10^2 : 0.514629 (-0.275368 0.461067)
kT2 [keV] : 200.000 (-200 -200)
R2^2/D10^2 : 2.64465E-04 (-0.000106626 0.00135475)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.33e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.439e-08 6.505e-09
25- 50 4.279e-08 2.090e-08
50-150 1.017e-07 4.856e-08
15-150 1.589e-07 7.070e-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: 1.39473 ( -0.0615151 0.061347 )
Norm@50keV : 6.92775E-03 ( -0.000227947 0.000227922 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.21 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.43e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 89.8 sec: 0.842668 ( -0.0304761 0.0306061 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.01777e-06 ( -2.08941e-07 2.09388e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.30905 ( -0.236891 0.11431 )
Epeak [keV] : 453.123 ( -453.065 -453.065 )
Norm@50keV : 7.57380E-03 ( -0.00115884 0.00204512 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.80 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.37e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 89.8 sec: 0.837781 ( -0.032849 0.032916 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.99128e-06 ( -2.23656e-07 2.22614e-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) = 1.77e-06
S(50-100 keV) = 2.69e-06
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 1.51977
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.4662
Count Ratio (50-100 keV) / (15-25 keV) = 1.24257
Mask shadow pattern
IMX = 4.991616332418481E-01, IMY = -3.754864819192321E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-16.899410 72.900600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6525 22.0451 1.0 24.6 94.6 3.6644 11.7 2.1 Crab
105.6410 10.9587 2.7 35.0 139.1 1.5327 4.3 ------ UNKNOWN
54.1505 27.1463 0.4 32.0 37.0 9.2393 31.4 ------ UNKNOWN
45.8368 25.2114 3.7 35.6 24.7 0.9673 3.1 ------ UNKNOWN
90.8596 0.2377 2.7 18.8 158.0 0.8172 4.3 ------ UNKNOWN
116.1753 -27.9139 4.0 50.7 -164.4 1.4636 2.9 ------ UNKNOWN
42.4116 -8.5877 2.8 30.9 -39.2 1.0655 4.2 ------ UNKNOWN
99.0709 -43.2234 3.6 49.7 -137.6 2.2356 3.2 ------ UNKNOWN
36.9294 -27.4887 3.5 43.7 -64.1 3.3571 3.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
214.300630 599.400600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6282 22.0254 0.6 27.2 81.9 16.3503 18.0 0.7 Crab
88.7334 36.4808 3.3 30.6 51.1 2.9559 3.5 ------ UNKNOWN
48.4338 27.1317 2.6 5.1 -100.9 2.3917 4.3 ------ UNKNOWN
25.0957 -22.6632 2.6 57.2 -160.1 11.8551 4.4 ------ UNKNOWN
3.9163 45.2645 3.0 43.6 -64.1 10.6604 3.8 ------ UNKNOWN
12.5813 0.4449 2.6 48.0 -129.0 11.8285 4.3 ------ UNKNOWN
Plot creation:
Tue Dec 26 16:59:22 EST 2023