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
70.2655 +44.5195 0.0510 13.0 -124.9 6.8078 3.8 TRIG_01150965
------------------------------------------
Foreground time interval of the image:
-224.296 196.833 (delta_t = 421.129 [sec])
Background time interval of the image:
-239.768 -224.296 (delta_t = 15.472 [sec])
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 0.256000
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 0.256000
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 0.256000
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 -224.296 sec. to 282.308 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.61982 ( )
Norm@50keV : 3.22724E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 152.48 using 59 PHA bins.
# Reduced chi-squared = 2.6750 for 57 degrees of freedom
# Null hypothesis probability = 1.204365e-10
Photon flux (15-150 keV) in 506.6 sec: 0.683530 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.69335e-05 ( 0 0 ) ergs/cm2
Cutoff power-law model
Time interval is from -224.296 sec. to 282.308 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.965285 ( -0.340185 0.318011 )
Epeak [keV] : 25.8168 ( -3.87941 2.8989 )
Norm@50keV : 2.70953E-02 ( -0.00906199 0.01492 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.00 using 59 PHA bins.
# Reduced chi-squared = 0.8393 for 56 degrees of freedom
# Null hypothesis probability = 7.987093e-01
Photon flux (15-150 keV) in 506.6 sec: 0.600462 ( -0.024229 0.024456 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.47778e-05 ( -5.21697e-07 5.30106e-07 ) ergs/cm2
Band function
Time interval is from -224.296 sec. to 282.308 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.964873 ( -0.223057 0.471107 )
beta : -10.0000 ( 10 0 )
Epeak [keV] : 25.8136 ( -3.87942 2.89684 )
Norm@50keV : 2.71109E-02 ( -0.00907585 0.0149444 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.00 using 59 PHA bins.
# Reduced chi-squared = 0.8545 for 55 degrees of freedom
# Null hypothesis probability = 7.700318e-01
Photon flux (15-150 keV) in 506.6 sec: 0.602446 ( 6.39755 -0.025815 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.47485e-05 ( -1.47449e-05 -5.12578e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 8.81676 ( )
R^2/D10^2 : 0.432052 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 156.90 using 59 PHA bins.
# Reduced chi-squared = 2.7526 for 57 degrees of freedom
# Null hypothesis probability = 2.856249e-11
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.276e-06 1.535e-07
25- 50 6.741e-06 1.773e-07
50-150 2.414e-06 1.603e-07
15-150 1.243e-05 3.394e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 33.6793 (-1.82963 1.97657)
Norm : 4.68153 (-0.283966 0.303921)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.098e-06 2.026e-07
25- 50 6.191e-06 1.596e-07
50-150 3.925e-06 2.913e-07
15-150 1.521e-05 3.850e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.08807 (-0.608509 0.65165)
R1^2/D10^2 : 2.68277 (-0.96842 1.79649)
kT2 [keV] : 12.2409 (-0.986243 1.31434)
R2^2/D10^2 : 7.39672E-02 (-0.0316163 0.0424678)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.732e-06 5.585e-07
25- 50 6.245e-06 5.725e-07
50-150 3.603e-06 5.332e-07
15-150 1.458e-05 1.535e-06
Peak spectrum fit
Power-law model
Time interval is from -159.404 sec. to -158.404 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.09588 ( -0.219227 0.239454 )
Norm@50keV : 1.08438E-02 ( -0.00197915 0.00194698 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 86.16 using 59 PHA bins.
# Reduced chi-squared = 1.512 for 57 degrees of freedom
# Null hypothesis probability = 7.576525e-03
Photon flux (15-150 keV) in 1 sec: 1.70255 ( -0.235482 0.235518 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.00725e-07 ( -1.66598e-08 1.71163e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -159.404 sec. to -158.404 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.805363 ( -1.77502 1.33844 )
Epeak [keV] : 38.6839 ( -5.18284 5.7138 )
Norm@50keV : 0.570638 ( -0.579132 5.93798 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.82 using 59 PHA bins.
# Reduced chi-squared = 1.229 for 56 degrees of freedom
# Null hypothesis probability = 1.167845e-01
Photon flux (15-150 keV) in 1 sec: 1.67426 ( -0.23134 0.23189 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.09012e-08 ( -1.40861e-08 1.50838e-08 ) ergs/cm2
Band function
Time interval is from -159.404 sec. to -158.404 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.691621 ( -1.2201 1.89526 )
beta : -9.27386 ( 8.27247 18.2706 )
Epeak [keV] : 38.6995 ( -5.12703 5.72165 )
Norm@50keV : 0.489516 ( -0.489528 5.89601 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.84 using 59 PHA bins.
# Reduced chi-squared = 1.252 for 55 degrees of freedom
# Null hypothesis probability = 9.943025e-02
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 7.04836e-08 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 9.96486 (-1.157 1.26802)
R^2/D10^2 : 0.919361 (-0.341805 0.546493)
(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 1.857e-08 4.320e-09
25- 50 4.594e-08 8.465e-09
50-150 2.373e-08 8.730e-09
15-150 8.824e-08 1.612e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 52.4810 (-13.8916 22.0215)
Norm : 9.84779 (-1.8149 2.2753)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.434e-08 4.300e-09
25- 50 3.555e-08 5.910e-09
50-150 3.610e-08 1.335e-08
15-150 9.598e-08 1.916e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.41465 (-3.41464 -3.41464)
R1^2/D10^2 : 12.4503 (-12.4587 -12.4587)
kT2 [keV] : 10.6697 (-1.56914 -10.6691)
R2^2/D10^2 : 0.660027 (-0.660242 0.635179)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.058e-08 1.020e-08
25- 50 4.349e-08 2.453e-08
50-150 2.661e-08 1.601e-08
15-150 9.067e-08 4.924e-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: 2.60170 ( )
Norm@50keV : 3.23984E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 172.49 using 59 PHA bins.
# Reduced chi-squared = 3.0262 for 57 degrees of freedom
# Null hypothesis probability = 1.518433e-13
Photon flux (15-150 keV) in 421.1 sec: 0.678274 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.40504e-05 ( 0 0 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.943769 ( -0.3487 0.324908 )
Epeak [keV] : 26.3082 ( -3.8741 2.89139 )
Norm@50keV : 2.73465E-02 ( -0.00930789 0.0155131 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.87 using 59 PHA bins.
# Reduced chi-squared = 1.266 for 56 degrees of freedom
# Null hypothesis probability = 8.704570e-02
Photon flux (15-150 keV) in 421.1 sec: 0.596837 ( -0.024456 0.024707 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.22652e-05 ( -4.44429e-07 4.51209e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.943476 ( -0.322634 0.3519 )
beta : -10.0000 ( 10 3.55271e-15 )
Epeak [keV] : 26.3040 ( -3.87331 2.89017 )
Norm@50keV : 2.73578E-02 ( -0.00931805 0.0155432 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.88 using 59 PHA bins.
# Reduced chi-squared = 1.289 for 55 degrees of freedom
# Null hypothesis probability = 7.342535e-02
Photon flux (15-150 keV) in 421.1 sec: 0.602300 ( 6.3977 -0.029801 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.22455e-05 ( -1.22425e-05 -4.41692e-07 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 5.67e-06
S(50-100 keV) = 3.69e-06
T90 vs. Hardness ratio plot
T90 = 462.831999897957 sec.
Hardness ratio (energy fluence ratio) = 0.650794
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.910789
Count Ratio (50-100 keV) / (15-25 keV) = 0.258195
Mask shadow pattern
IMX = -1.320796814818979E-01, IMY = 1.896701031503785E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.256000
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:
-239.768000 -224.296000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6467 22.0101 1.4 24.7 157.9 0.6122 8.0 0.8 Crab
70.2410 44.5415 0.9 13.0 -124.7 0.8612 12.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-224.296000 196.832600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6581 21.9976 261.2 24.7 157.9 -0.0833 -0.0 1.7 Crab
52.8661 3.0813 2.2 53.3 -166.5 28.9372 5.2 ------ UNKNOWN
40.4187 22.0745 2.6 45.8 -138.4 21.7638 4.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
342.932590 962.302000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
101.9614 32.6083 2.0 47.6 141.7 36.4691 5.9 ------ UNKNOWN
Plot creation:
Fri Jan 27 13:33:36 EST 2023