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
97.3206 -35.3786 0.0130 31.7968 -150.8061 2.0088879 14.714 TRIG_01059881
Foreground time interval of the image:
-40.076 17.037 (delta_t = 57.113 [sec])
Background time interval of the image:
-239.264 -40.076 (delta_t = 199.188 [sec])
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 -40.076 sec. to 108.740 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.82825 ( -0.101906 0.103493 )
Norm@50keV : 2.20505E-03 ( -0.000138944 0.000137814 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.44 using 59 bins.
Reduced chi-squared = 1.11298
# Null hypothesis probability of 2.60e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 148.8 sec: 0.307260 ( -0.017606 0.017627 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.01859e-06 ( -1.91735e-07 1.93468e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -40.076 sec. to 108.740 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.09888 ( -0.513994 0.453431 )
Epeak [keV] : 54.6026 ( -8.30257 20.782 )
Norm@50keV : 5.55578E-03 ( -0.00239209 0.00506099 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.38 using 59 bins.
Reduced chi-squared = 0.988929
# Null hypothesis probability of 4.98e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 148.8 sec: 0.296274 ( -0.018802 0.018802 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.80281e-06 ( -2.24871e-07 2.29912e-07 ) ergs/cm2
Band function
Time interval is from -40.076 sec. to 108.740 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] : 11.3557 (-0.723165 0.781796)
R^2/D10^2 : 8.92526E-02 (-0.0199967 0.0254493)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 99.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.15e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.598e-07 3.482e-08
25- 50 1.059e-06 7.314e-08
50-150 7.903e-07 1.092e-07
15-150 2.209e-06 1.466e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 91.3459 (-16.7822 23.7041)
Norm : 1.38550 (-0.114897 0.128733)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.75 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.22e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.382e-07 5.245e-08
25- 50 9.132e-07 5.454e-08
50-150 1.403e-06 4.396e-07
15-150 2.854e-06 4.442e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.62263 (-1.43047 1.18588)
R1^2/D10^2 : 0.287590 (-0.109915 0.254311)
kT2 [keV] : 24.6374 (-6.36994 13.4024)
R2^2/D10^2 : 3.08835E-03 (-0.00241835 0.00750066)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.84 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.81e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.816e-07 8.526e-08
25- 50 9.702e-07 1.916e-07
50-150 1.395e-06 6.296e-07
15-150 2.847e-06 8.077e-07
Peak spectrum fit
Power-law model
Time interval is from 0.088 sec. to 1.088 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.29130 ( -0.187622 0.18543 )
Norm@50keV : 1.89953E-02 ( -0.00215414 0.00215205 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.06 using 59 bins.
Reduced chi-squared = 1.10632
# Null hypothesis probability of 2.71e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.26262 ( -0.26213 0.26256 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.88131e-07 ( -2.34286e-08 2.36076e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.088 sec. to 1.088 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.673076 ( -0.866308 0.687572 )
Epeak [keV] : 109.557 ( -37.8387 -109.558 )
Norm@50keV : 3.87457E-02 ( -0.0206344 0.064246 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.90 using 59 bins.
Reduced chi-squared = 1.0875
# Null hypothesis probability of 3.04e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.21741 ( -0.26835 0.26819 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.80393e-07 ( -2.58355e-08 2.55561e-08 ) ergs/cm2
Band function
Time interval is from 0.088 sec. to 1.088 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] : 16.3416 (-2.31135 2.84691)
R^2/D10^2 : 0.202224 (-0.0853723 0.139873)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.30 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.18e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.111e-08 2.452e-09
25- 50 4.760e-08 8.095e-09
50-150 8.955e-08 2.064e-08
15-150 1.483e-07 2.555e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-40.4339 -200)
Norm : 9.40498 (-1.07248 1.07248)
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.80e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.342e-08 1.301e-08
25- 50 4.505e-08 2.499e-08
50-150 9.879e-08 5.470e-08
15-150 1.672e-07 9.170e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.65963 (-2.89561 3.23342)
R1^2/D10^2 : 0.812719 (-0.451474 1.4088)
kT2 [keV] : 36.2331 (-25.9846 159.51)
R2^2/D10^2 : 1.01541E-02 (-0.00987803 0.0420189)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.52 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.48e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.709e-08 8.867e-09
25- 50 4.827e-08 2.486e-08
50-150 1.196e-07 6.593e-08
15-150 1.849e-07 8.725e-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: 1.57473 ( -0.17532 0.17654 )
Norm@50keV : 2.26251E-03 ( -0.000239783 0.000238047 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.42e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 57.11 sec: 0.288513 ( -0.0298298 0.0298737 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21229e-06 ( -1.37837e-07 1.39332e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.13451 ( -0.784615 0.563642 )
Epeak [keV] : 93.0758 ( -34.4657 -93.076 )
Norm@50keV : 3.87103E-03 ( -0.00177836 0.00604591 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.52e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 57.11 sec: 0.283295 ( -0.030936 0.030889 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.16591e-06 ( -1.55339e-07 1.56082e-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) = 8.59e-07
S(50-100 keV) = 9.67e-07
T90 vs. Hardness ratio plot
T90 = 121.283999919891 sec.
Hardness ratio (energy fluence ratio) = 1.12573
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.24982
Count Ratio (50-100 keV) / (15-25 keV) = 0.635289
Mask shadow pattern
IMX = -5.411982822283098E-01, IMY = 3.023903508242055E-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:
-239.264000 -40.076000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5372 -40.5609 0.5 7.9 -77.9 6.0702 24.9 0.5 Vela X-1
169.9114 -60.6254 0.0 22.4 65.3 0.2196 0.7 11.9 Cen X-3
186.6325 -62.7601 1.5 30.5 66.5 3.2598 7.7 0.9 GX 301-2
54.3139 -41.3423 2.4 56.1 173.7 6.0084 4.7 ------ UNKNOWN
189.3066 -9.9845 2.9 58.1 -3.3 6.6919 4.0 ------ UNKNOWN
124.9573 -12.3130 2.6 37.4 -89.6 3.5771 4.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-40.076000 17.036600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.6647 -40.6364 4.9 7.8 -77.3 0.2765 2.3 7.9 Vela X-1
170.2122 -60.4557 3.0 22.4 64.8 0.5557 3.9 10.5 Cen X-3
186.6689 -62.8815 5.4 30.5 66.7 0.4564 2.1 6.7 GX 301-2
97.3206 -35.3786 0.8 31.8 -150.8 2.0089 14.7 ------ UNKNOWN
181.8537 -5.6799 2.6 57.2 -13.4 2.1447 4.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
69.836600 612.036600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5435 -40.5710 0.4 30.3 5.8 15.2131 25.8 1.2 Vela X-1
52.9705 -67.7966 2.6 40.8 98.2 8.2865 4.5 ------ UNKNOWN
169.0387 -39.4388 2.5 55.5 11.6 13.9579 4.7 ------ UNKNOWN
157.6391 -12.3991 3.3 58.7 -22.7 9.6970 3.5 ------ UNKNOWN
Plot creation:
Sat Jul 30 06:56:08 EDT 2022