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
299.6369 +35.5453 0.0095 0.1 -10.0 2.6386 20.1 TRIG_01192486
------------------------------------------
Foreground time interval of the image:
0.000 64.000 (delta_t = 64.000 [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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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 64.000000
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 64.000000
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 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.80027 ( -0.116409 0.118476 )
Norm@50keV : 2.35839E-03 ( -0.000168086 0.00016621 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.31 using 59 PHA bins.
# Reduced chi-squared = 1.181 for 57 degrees of freedom
# Null hypothesis probability = 1.649711e-01
Photon flux (15-150 keV) in 64 sec: 0.325016 ( -0.0207048 0.0207215 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.38952e-06 ( -1.00764e-07 1.0172e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.72636 ( -0.438622 0.43494 )
Epeak [keV] : 166.758 ( )
Norm@50keV : 2.58950E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.21 using 59 PHA bins.
# Reduced chi-squared = 1.200 for 56 degrees of freedom
# Null hypothesis probability = 1.450292e-01
Photon flux (15-150 keV) in 64 sec: 0.323808 ( -0.021619 0.02147 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.3792e-06 ( -1.17094e-07 1.10547e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.72493 ( -4.72493 -4.72493 )
beta : -1.88328 ( -0.141033 0.134087 )
Epeak [keV] : 22.6836 ( -5.56695 3.34806 )
Norm@50keV : 365.933 ( -22.853 1.6935e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.04 using 59 PHA bins.
# Reduced chi-squared = 1.183 for 55 degrees of freedom
# Null hypothesis probability = 1.667620e-01
Photon flux (15-150 keV) in 64 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] : 11.0285 ( )
R^2/D10^2 : 0.102644 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 138.71 using 59 PHA bins.
# Reduced chi-squared = 2.4335 for 57 degrees of freedom
# Null hypothesis probability = 9.191355e-09
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.670e-07 2.029e-08
25- 50 4.739e-07 3.530e-08
50-150 3.262e-07 4.810e-08
15-150 9.671e-07 7.552e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 99.8185 (-20.2586 38.9925)
Norm : 1.42655 (-0.137149 0.134851)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.386e-07 2.573e-08
25- 50 4.125e-07 3.245e-08
50-150 6.677e-07 2.073e-07
15-150 1.319e-06 2.275e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.73040 (-0.933712 0.987015)
R1^2/D10^2 : 0.502234 (-0.193565 0.361218)
kT2 [keV] : 28.3056 (-6.03336 10.2622)
R2^2/D10^2 : 2.45800E-03 (-0.00154608 0.0033124)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.446e-07 4.083e-08
25- 50 4.070e-07 7.062e-08
50-150 7.506e-07 2.609e-07
15-150 1.402e-06 3.475e-07
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.80027 ( -0.116409 0.118476 )
Norm@50keV : 2.35839E-03 ( -0.000168086 0.00016621 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.31 using 59 PHA bins.
# Reduced chi-squared = 1.181 for 57 degrees of freedom
# Null hypothesis probability = 1.649711e-01
Photon flux (15-150 keV) in 64 sec: 0.325016 ( -0.0207048 0.0207215 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.38952e-06 ( -1.00764e-07 1.0172e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.72636 ( -0.438622 0.43494 )
Epeak [keV] : 166.758 ( )
Norm@50keV : 2.58950E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.21 using 59 PHA bins.
# Reduced chi-squared = 1.200 for 56 degrees of freedom
# Null hypothesis probability = 1.450292e-01
Photon flux (15-150 keV) in 64 sec: 0.323808 ( -0.021619 0.02147 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.3792e-06 ( -1.17094e-07 1.10547e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.72493 ( -4.72493 -4.72493 )
beta : -1.88328 ( -0.141033 0.134087 )
Epeak [keV] : 22.6836 ( -5.56695 3.34806 )
Norm@50keV : 365.933 ( -22.853 1.6935e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.04 using 59 PHA bins.
# Reduced chi-squared = 1.183 for 55 degrees of freedom
# Null hypothesis probability = 1.667620e-01
Photon flux (15-150 keV) in 64 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] : 11.0285 ( )
R^2/D10^2 : 0.102644 ( )
(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 1.670e-07 1.824e-08
25- 50 4.739e-07 3.648e-08
50-150 3.262e-07 5.440e-08
15-150 9.671e-07 7.072e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 99.8185 (-20.2586 38.9925)
Norm : 1.42655 (-0.137149 0.134851)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.386e-07 2.678e-08
25- 50 4.125e-07 3.072e-08
50-150 6.677e-07 2.073e-07
15-150 1.319e-06 2.291e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.73040 (-0.933712 0.987015)
R1^2/D10^2 : 0.502234 (-0.193565 0.361218)
kT2 [keV] : 28.3056 (-6.03336 10.2622)
R2^2/D10^2 : 2.45800E-03 (-0.00154608 0.0033124)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.446e-07 4.592e-08
25- 50 4.070e-07 6.115e-08
50-150 7.506e-07 2.912e-07
15-150 1.402e-06 3.709e-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: 1.80027 ( -0.116409 0.118476 )
Norm@50keV : 2.35839E-03 ( -0.000168086 0.00016621 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.31 using 59 PHA bins.
# Reduced chi-squared = 1.181 for 57 degrees of freedom
# Null hypothesis probability = 1.649711e-01
Photon flux (15-150 keV) in 64 sec: 0.325016 ( -0.0207048 0.0207215 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.38952e-06 ( -1.00764e-07 1.0172e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.72636 ( -0.438622 0.43494 )
Epeak [keV] : 166.758 ( )
Norm@50keV : 2.58950E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.21 using 59 PHA bins.
# Reduced chi-squared = 1.200 for 56 degrees of freedom
# Null hypothesis probability = 1.450292e-01
Photon flux (15-150 keV) in 64 sec: 0.323808 ( -0.021619 0.02147 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.3792e-06 ( -1.17094e-07 1.10547e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.72493 ( -4.72493 -4.72493 )
beta : -1.88328 ( -0.141033 0.134087 )
Epeak [keV] : 22.6836 ( -5.56695 3.34806 )
Norm@50keV : 365.933 ( -22.853 1.6935e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.04 using 59 PHA bins.
# Reduced chi-squared = 1.183 for 55 degrees of freedom
# Null hypothesis probability = 1.667620e-01
Photon flux (15-150 keV) in 64 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) = 3.91e-07
S(50-100 keV) = 4.49e-07
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 1.14834
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.11748
Count Ratio (50-100 keV) / (15-25 keV) = 0.65314
Mask shadow pattern
IMX = 1.584607449100551E-03, IMY = 2.783951644743437E-04
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
0.000000 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.6150 35.3550 12.6 36.3 -99.7 -0.2574 -0.9 7.7 Her X-1
268.2686 -1.3056 127.9 47.0 -157.7 -0.0241 -0.1 10.6 SW J1753.5-0127
273.9142 -14.0344 5.5 55.2 -172.2 0.8778 2.1 5.3 GX 17+2
288.8689 11.0805 6.0 26.3 -178.6 0.2707 1.9 9.1 GRS 1915+105
299.6872 35.0049 0.0 0.5 149.1 -0.4980 -4.0 12.7 Cyg X-1
308.1762 40.7551 4.1 8.6 26.2 -0.3564 -2.8 12.2 Cyg X-3
326.0930 38.1848 4.9 21.3 51.7 -0.3831 -2.3 9.0 Cyg X-2
300.7206 -8.2698 2.8 43.7 155.4 1.3573 4.2 ------ UNKNOWN
261.1876 -5.1279 2.8 54.3 -153.4 1.7579 4.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Tue Sep 19 02:05:59 EDT 2023