Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minutes to calcaulte
Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
84.2316 +21.7839 0.0139 43.4 0.0 3.5465 13.9 TRIG_01217733
------------------------------------------
Foreground time interval of the image:
-16.599 71.301 (delta_t = 87.900 [sec])
Background time interval of the image:
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 2) The mask-weighted light curves are using the flight position.
- 3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 4) 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.
- 5) 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.
- 6) 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)
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) For long bursts, a spectral fit of 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.
- 4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.
Time averaged spectrum fit using the pre-slew DRM
Power-law model
Time interval is from -32.452 sec. to 81.084 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.94925 ( -0.152843 0.158496 )
Norm@50keV : 2.34175E-03 ( -0.000224356 0.000220284 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.64 using 59 PHA bins.
# Reduced chi-squared = 0.7832 for 57 degrees of freedom
# Null hypothesis probability = 8.829313e-01
Photon flux (15-150 keV) in 113.5 sec: 0.343314 ( -0.0288079 0.0288764 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.44591e-06 ( -2.25274e-07 2.27301e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -32.452 sec. to 81.084 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.89032 ( -0.593415 0.429778 )
Epeak [keV] : 86.0365 ( )
Norm@50keV : 2.51969E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.61 using 59 PHA bins.
# Reduced chi-squared = 0.7966 for 56 degrees of freedom
# Null hypothesis probability = 8.632898e-01
Photon flux (15-150 keV) in 113.5 sec: 0.342301 ( -0.030055 0.02943 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.43528e-06 ( -2.50018e-07 2.35774e-07 ) ergs/cm2
Band function
Time interval is from -32.452 sec. to 81.084 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.87975 ( 1.88053 0.485962 )
beta : -9.37160 ( 9.37167 19.3717 )
Epeak [keV] : 85.1370 ( -84.0458 -84.0458 )
Norm@50keV : 2.54369E-03 ( -0.000325102 0.00197252 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.61 using 59 PHA bins.
# Reduced chi-squared = 0.8111 for 55 degrees of freedom
# Null hypothesis probability = 8.404007e-01
Photon flux (15-150 keV) in 113.5 sec: 0.342400 ( ) 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] : 10.8269 (-1.20511 1.37329)
R^2/D10^2 : 0.113923 (-0.0414263 0.0650303)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 91.66 using 59 PHA bins.
# Reduced chi-squared = 1.608 for 57 degrees of freedom
# Null hypothesis probability = 2.449423e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.156e-07 4.801e-08
25- 50 8.743e-07 9.341e-08
50-150 5.718e-07 1.271e-07
15-150 1.762e-06 1.912e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 81.2408 (-19.6747 30.8583)
Norm : 1.58055 (-0.104972 0.23834)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.659e-07 5.584e-08
25- 50 7.698e-07 6.424e-08
50-150 1.098e-06 3.599e-07
15-150 2.334e-06 3.587e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.03290 (-1.13796 1.24006)
R1^2/D10^2 : 0.805851 (-0.403746 1.01974)
kT2 [keV] : 23.4549 (-5.12717 8.93659)
R2^2/D10^2 : 4.55984E-03 (-0.0031302 0.00736117)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.969e-07 1.608e-07
25- 50 7.302e-07 2.098e-07
50-150 1.193e-06 6.159e-07
15-150 2.420e-06 7.443e-07
Peak spectrum fit
Power-law model
Time interval is from -6.540 sec. to -5.540 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.43480 ( -0.684162 0.656812 )
Norm@50keV : 6.62040E-03 ( -0.00210111 0.00209386 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.29 using 59 PHA bins.
# Reduced chi-squared = 0.7771 for 57 degrees of freedom
# Null hypothesis probability = 8.903816e-01
Photon flux (15-150 keV) in 1 sec: 0.812820 ( -0.277363 0.27878 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.35341e-08 ( -2.17705e-08 2.19649e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -6.540 sec. to -5.540 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.41298 ( -3.13688 -3.39543 )
Epeak [keV] : 375.823 ( )
Norm@50keV : 7.18964E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 43.93 using 59 PHA bins.
# Reduced chi-squared = 0.7845 for 56 degrees of freedom
# Null hypothesis probability = 8.790834e-01
Photon flux (15-150 keV) in 1 sec: 0.817171 ( -0.280496 0.274199 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.31164e-08 ( -2.13025e-08 2.16527e-08 ) ergs/cm2
Band function
Time interval is from -6.540 sec. to -5.540 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.14678 ( 1.1433 1.1433 )
beta : -1.43187 ( 1.43468 0.684367 )
Epeak [keV] : 38.7203 ( -46.2661 -46.2661 )
Norm@50keV : 1.29488E-02 ( -0.012729 2.87942 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.29 using 59 PHA bins.
# Reduced chi-squared = 0.8053 for 55 degrees of freedom
# Null hypothesis probability = 8.487774e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 23.2566 (-12.4236 26.3293)
R^2/D10^2 : 1.96314E-02 (-0.0192605 0.238851)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.914e-09 1.283e-09
25- 50 1.045e-08 6.380e-09
50-150 4.219e-08 2.869e-08
15-150 5.456e-08 3.417e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-199.363 -199.363)
Norm : 3.34402 (-1.07141 1.07156)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.327e-09 5.180e-09
25- 50 1.602e-08 9.655e-09
50-150 3.513e-08 2.169e-08
15-150 5.948e-08 3.616e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.53401 (-2.53557 4.38262)
R1^2/D10^2 : 2.76566 (-2.52493 45.1432)
kT2 [keV] : 41.3744 (-19.6327 -41.3746)
R2^2/D10^2 : 3.08869E-03 (-0.00290776 0.0219814)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.059e-08 6.630e-09
25- 50 1.284e-08 7.675e-09
50-150 4.620e-08 2.656e-08
15-150 6.964e-08 3.704e-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: 2.02677 ( -0.167834 0.175914 )
Norm@50keV : 2.39766E-03 ( -0.00025823 0.000252209 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.86 using 59 PHA bins.
# Reduced chi-squared = 0.8571 for 57 degrees of freedom
# Null hypothesis probability = 7.700546e-01
Photon flux (15-150 keV) in 87.9 sec: 0.364148 ( -0.0325793 0.0326495 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.94659e-06 ( -1.9438e-07 1.96531e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.02891 ( -0.64079 0.705836 )
Epeak [keV] : 596.339 ( )
Norm@50keV : 2.39144E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.86 using 59 PHA bins.
# Reduced chi-squared = 0.8725 for 56 degrees of freedom
# Null hypothesis probability = 7.396277e-01
Photon flux (15-150 keV) in 87.9 sec: 0.364075 ( -0.034004 0.032263 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.94645e-06 ( -2.14766e-07 1.94575e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -2.57900 ( 2.579 2.579 )
beta : -2.02677 ( -0.175912 0.167881 )
Epeak [keV] : 30.5066 ( -30.5066 -30.5066 )
Norm@50keV : 0.325875 ( -0.0350969 0.034279 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.86 using 59 PHA bins.
# Reduced chi-squared = 0.8883 for 55 degrees of freedom
# Null hypothesis probability = 7.070475e-01
Photon flux (15-150 keV) in 87.9 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) = 7.25e-07
S(50-100 keV) = 7.51e-07
T90 vs. Hardness ratio plot
T90 = 87.4159998893738 sec.
Hardness ratio (energy fluence ratio) = 1.03586
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.17418
Count Ratio (50-100 keV) / (15-25 keV) = 0.693039
Mask shadow pattern
IMX = 9.453567984334705E-01, IMY = -1.600158110907147E-04
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:
-16.599400 71.300600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6691 22.0415 5.0 43.8 -0.5 -0.6142 -2.3 2.6 Crab
135.5308 -40.3460 0.0 36.7 158.0 0.4908 1.8 12.5 Vela X-1
89.3633 36.1818 2.3 55.6 11.8 3.8291 5.1 ------ UNKNOWN
84.2317 21.7839 0.8 43.4 0.0 3.5446 13.9 ------ UNKNOWN
107.8351 -65.0529 2.4 47.0 -160.1 1.7333 4.9 ------ UNKNOWN
64.6179 26.8659 2.3 57.5 -15.7 3.5588 5.0 ------ UNKNOWN
63.5341 14.1762 2.5 49.5 -28.0 1.9480 4.5 ------ UNKNOWN
71.6065 -59.7183 2.3 46.7 -136.2 2.3107 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
162.600600 243.088900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7980 21.8766 64.8 0.4 -74.8 -0.0280 -0.2 12.3 Crab
84.2962 21.7803 0.6 0.1 101.5 2.9004 19.4 ------ UNKNOWN
71.2913 11.2222 2.8 16.3 -125.5 0.6287 4.2 ------ UNKNOWN
48.5427 69.0141 2.7 51.9 -12.5 1.4997 4.2 ------ UNKNOWN
Plot creation:
Wed Feb 28 02:10:43 EST 2024