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
83.3514 +21.2814 0.0097 0.1 -19.5 2.5597 19.9 TRIG_01192488
------------------------------------------
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: 2.10297 ( -0.134361 0.139167 )
Norm@50keV : 2.08710E-03 ( -0.00017932 0.000176035 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.32 using 59 PHA bins.
# Reduced chi-squared = 0.8301 for 57 degrees of freedom
# Null hypothesis probability = 8.160844e-01
Photon flux (15-150 keV) in 64 sec: 0.328836 ( -0.0216745 0.0217056 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.24141e-06 ( -9.50259e-08 9.63437e-08 ) 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: 2.23712 ( -0.273972 0.0471342 )
Epeak [keV] : 103.229 ( )
Norm@50keV : 1.76106E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.81 using 59 PHA bins.
# Reduced chi-squared = 0.8359 for 56 degrees of freedom
# Null hypothesis probability = 8.043063e-01
Photon flux (15-150 keV) in 64 sec: 0.328697 ( -0.02167 0.021682 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.23693e-06 ( -9.35552e-08 1.01018e-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 : -1.49298 ( 1.48518 1.48518 )
beta : -2.12466 ( 2.12575 0.153438 )
Epeak [keV] : 20.4845 ( -20.4298 23.5286 )
Norm@50keV : 5.99826E-03 ( -0.00625884 828856 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.18 using 59 PHA bins.
# Reduced chi-squared = 0.8578 for 55 degrees of freedom
# Null hypothesis probability = 7.642741e-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] : 9.01233 ( )
R^2/D10^2 : 0.212426 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 117.77 using 59 PHA bins.
# Reduced chi-squared = 2.0662 for 57 degrees of freedom
# Null hypothesis probability = 4.029779e-06
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.151e-07 2.330e-08
25- 50 4.583e-07 3.757e-08
50-150 1.756e-07 3.398e-08
15-150 8.490e-07 6.656e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 59.1516 (-11.612 15.965)
Norm : 1.69154 (-0.203832 0.223098)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.714e-07 2.445e-08
25- 50 4.113e-07 2.797e-08
50-150 4.625e-07 8.166e-08
15-150 1.145e-06 9.120e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.73069 (-0.847361 0.895201)
R1^2/D10^2 : 1.04188 (-0.445132 0.929872)
kT2 [keV] : 24.0587 (-5.54671 9.77673)
R2^2/D10^2 : 3.58212E-03 (-0.00243144 0.00595138)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.951e-07 5.670e-08
25- 50 3.754e-07 6.346e-08
50-150 5.823e-07 2.990e-07
15-150 1.253e-06 3.024e-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: 2.10297 ( -0.134361 0.139167 )
Norm@50keV : 2.08710E-03 ( -0.00017932 0.000176035 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.32 using 59 PHA bins.
# Reduced chi-squared = 0.8301 for 57 degrees of freedom
# Null hypothesis probability = 8.160844e-01
Photon flux (15-150 keV) in 64 sec: 0.328836 ( -0.0216745 0.0217056 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.24141e-06 ( -9.50259e-08 9.63437e-08 ) 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: 2.23712 ( -0.273972 0.0471342 )
Epeak [keV] : 103.229 ( )
Norm@50keV : 1.76106E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.81 using 59 PHA bins.
# Reduced chi-squared = 0.8359 for 56 degrees of freedom
# Null hypothesis probability = 8.043063e-01
Photon flux (15-150 keV) in 64 sec: 0.328697 ( -0.02167 0.021682 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.23693e-06 ( -9.35552e-08 1.01018e-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 : -1.49298 ( 1.48518 1.48518 )
beta : -2.12466 ( 2.12575 0.153438 )
Epeak [keV] : 20.4845 ( -20.4298 23.5286 )
Norm@50keV : 5.99826E-03 ( -0.00625884 828856 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.18 using 59 PHA bins.
# Reduced chi-squared = 0.8578 for 55 degrees of freedom
# Null hypothesis probability = 7.642741e-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] : 9.01233 ( )
R^2/D10^2 : 0.212426 ( )
(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 2.151e-07 2.429e-08
25- 50 4.583e-07 3.661e-08
50-150 1.756e-07 3.478e-08
15-150 8.490e-07 7.360e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 59.1516 (-11.612 15.965)
Norm : 1.69154 (-0.203832 0.223098)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.714e-07 2.646e-08
25- 50 4.113e-07 2.902e-08
50-150 4.625e-07 7.770e-08
15-150 1.145e-06 9.920e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.73069 (-0.847361 0.895201)
R1^2/D10^2 : 1.04188 (-0.445132 0.929872)
kT2 [keV] : 24.0587 (-5.54671 9.77673)
R2^2/D10^2 : 3.58212E-03 (-0.00243144 0.00595138)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.951e-07 5.174e-08
25- 50 3.754e-07 6.589e-08
50-150 5.823e-07 2.488e-07
15-150 1.253e-06 3.069e-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: 2.10297 ( -0.134361 0.139167 )
Norm@50keV : 2.08710E-03 ( -0.00017932 0.000176035 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.32 using 59 PHA bins.
# Reduced chi-squared = 0.8301 for 57 degrees of freedom
# Null hypothesis probability = 8.160844e-01
Photon flux (15-150 keV) in 64 sec: 0.328836 ( -0.0216745 0.0217056 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.24141e-06 ( -9.50259e-08 9.63437e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.23712 ( -0.273972 0.0471342 )
Epeak [keV] : 103.229 ( )
Norm@50keV : 1.76106E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.81 using 59 PHA bins.
# Reduced chi-squared = 0.8359 for 56 degrees of freedom
# Null hypothesis probability = 8.043063e-01
Photon flux (15-150 keV) in 64 sec: 0.328697 ( -0.02167 0.021682 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.23693e-06 ( -9.35552e-08 1.01018e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.49298 ( 1.48518 1.48518 )
beta : -2.12466 ( 2.12575 0.153438 )
Epeak [keV] : 20.4845 ( -20.4298 23.5286 )
Norm@50keV : 5.99826E-03 ( -0.00625884 828856 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.18 using 59 PHA bins.
# Reduced chi-squared = 0.8578 for 55 degrees of freedom
# Null hypothesis probability = 7.642741e-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) = 3.84e-07
S(50-100 keV) = 3.58e-07
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 0.932292
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.879074
Count Ratio (50-100 keV) / (15-25 keV) = 0.442208
Mask shadow pattern
IMX = 1.303157919810250E-03, IMY = 4.604293328018271E-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] [']
83.6361 22.0152 5.8 0.7 -153.2 0.2568 2.0 0.2 Crab
55.8452 43.3449 2.2 31.7 143.1 0.9491 5.2 ------ UNKNOWN
67.8134 55.1638 2.9 35.8 167.7 0.6707 3.9 ------ UNKNOWN
83.3513 21.2819 0.6 0.1 -19.5 2.5709 19.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
-10.000000 63.110000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6015 21.9739 5.0 0.7 -154.2 0.3136 2.3 3.0 Crab
83.3507 21.2879 0.5 0.1 -22.1 2.9871 21.6 ------ UNKNOWN
Plot creation:
Tue Sep 19 01:59:18 EDT 2023