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
213.1767 63.7345 0.0099 32.4242 176.2868 1.6736634 19.542 TRIG_01250282
Foreground time interval of the image:
-0.656 35.549 (delta_t = 36.205 [sec])
Background time interval of the image:
-239.552 -0.656 (delta_t = 238.896 [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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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 4.096000
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 4.096000
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 -0.656 sec. to 43.168 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.31640 ( -0.138946 0.137407 )
Norm@50keV : 2.89025E-03 ( -0.000219858 0.00021985 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.33 using 59 bins.
Reduced chi-squared = 0.830351
# Null hypothesis probability of 8.16e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 43.82 sec: 0.345882 ( -0.02794 0.028044 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.24676e-06 ( -1.0232e-07 1.02803e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.656 sec. to 43.168 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.31269 ( -0.38543 0.178015 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 2.90209E-03 ( -0.000220729 0.000220733 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.35 using 59 bins.
Reduced chi-squared = 0.845536
# Null hypothesis probability of 7.88e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 43.82 sec: 0.345822 ( -0.02794 0.028014 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.24952e-06 ( -1.13796e-07 1.08427e-07 ) ergs/cm2
Band function
Time interval is from -0.656 sec. to 43.168 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] : 18.9498 (-1.93399 2.23536)
R^2/D10^2 : 1.80138E-02 (-0.00565633 0.00800048)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 94.52 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.32e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.577e-08 8.676e-09
25- 50 2.677e-07 3.146e-08
50-150 7.062e-07 9.356e-08
15-150 1.030e-06 9.816e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-21.5768 -200)
Norm : 1.44898 (-0.111526 0.111526)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.18 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.32e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.582e-07 1.369e-08
25- 50 3.042e-07 4.145e-08
50-150 6.672e-07 1.881e-07
15-150 1.130e-06 2.450e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.52438 (-1.61341 2.07222)
R1^2/D10^2 : 0.425824 (-0.260187 0.83672)
kT2 [keV] : 29.6943 (-5.55489 10.7799)
R2^2/D10^2 : 3.51685E-03 (-0.0021989 0.0036089)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.60 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.16e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.393e-07 5.751e-08
25- 50 2.717e-07 7.870e-08
50-150 8.396e-07 2.500e-07
15-150 1.251e-06 3.216e-07
Peak spectrum fit
Power-law model
Time interval is from -0.020 sec. to 0.980 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.845616 ( -0.445982 0.398427 )
Norm@50keV : 5.96656E-03 ( -0.00157938 0.00151278 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.46 using 59 bins.
Reduced chi-squared = 1.00807
# Null hypothesis probability of 4.58e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.684949 ( -0.172287 0.175993 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.84305e-08 ( -1.579e-08 1.57943e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.020 sec. to 0.980 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.674135 ( -5.61404 1.73196 )
Epeak [keV] : 119.089 ( -41.0004 -117.219 )
Norm@50keV : 2.08927E-02 ( -0.0221895 1.17788 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.33 using 59 bins.
Reduced chi-squared = 1.00589
# Null hypothesis probability of 4.63e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.628201 ( -0.1951 0.199153 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.62567e-08 ( -1.80208e-08 1.66673e-08 ) ergs/cm2
Band function
Time interval is from -0.020 sec. to 0.980 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] : 26.4193 (-6.06061 10.0799)
R^2/D10^2 : 1.50385E-02 (-0.00939333 0.0193722)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.00e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.769e-09 9.785e-10
25- 50 1.032e-08 5.040e-09
50-150 5.286e-08 2.701e-08
15-150 6.495e-08 3.032e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-58.2107 -200)
Norm : 2.94285 (-0.732086 0.732086)
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.28 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.87e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.336e-09 4.464e-09
25- 50 1.411e-08 8.270e-09
50-150 3.095e-08 1.850e-08
15-150 5.240e-08 3.033e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.50992 (-1.44407 2.91318)
R1^2/D10^2 : 3894.08 (-4741.51 0)
kT2 [keV] : 27.4558 (-6.44528 11.1364)
R2^2/D10^2 : 1.31624E-02 (-0.00842555 0.0176744)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.43e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.819e-09 1.498e-09
25- 50 9.726e-09 5.644e-09
50-150 5.326e-08 3.130e-08
15-150 6.681e-08 3.090e-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: 1.36371 ( -0.142937 0.142062 )
Norm@50keV : 3.09273E-03 ( -0.00024309 0.000243028 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.15e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 36.2 sec: 0.373651 ( -0.0309906 0.0311035 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.09014e-06 ( -9.31165e-08 9.36697e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36246 ( -0.472548 0.14141 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 3.10248E-03 ( -0.000243642 0.00196439 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.35 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.88e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 36.2 sec: 0.373907 ( -0.01603 0.03015 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.09023e-06 ( -9.41381e-08 9.29037e-08 ) 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) = 2.80e-07
S(50-100 keV) = 4.51e-07
T90 vs. Hardness ratio plot
T90 = 39.4399999380112 sec.
Hardness ratio (energy fluence ratio) = 1.61071
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.33382
Count Ratio (50-100 keV) / (15-25 keV) = 1.30426
Mask shadow pattern
IMX = -6.338793116353315E-01, IMY = -4.113737309992058E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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:
-239.552000 -0.656000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6087 22.0279 1.0 53.5 4.5 8.6583 11.4 1.6 Crab
74.2882 62.4872 3.2 25.7 55.5 1.4811 3.6 ------ UNKNOWN
84.3655 33.4313 4.2 43.0 10.5 1.3734 2.7 ------ UNKNOWN
219.5196 45.7843 3.0 48.0 -168.6 2.7213 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.656000 35.548610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7509 22.0641 5.8 53.4 4.4 0.5431 2.0 7.2 Crab
213.1767 63.7345 0.6 32.4 176.3 1.6739 19.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
116.548600 962.608000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4482 35.3400 297.7 37.8 141.8 0.0876 0.0 0.5 Her X-1
255.8824 30.1538 2.2 43.0 143.8 15.4552 5.2 ------ UNKNOWN
225.6226 32.7795 3.0 31.9 -176.9 4.7329 3.8 ------ UNKNOWN
96.3628 70.6416 2.7 38.7 -5.1 5.6289 4.3 ------ UNKNOWN
219.9110 11.4401 2.9 52.5 -165.2 12.1185 4.0 ------ UNKNOWN
Plot creation:
Sat Oct 19 18:18:16 EDT 2024