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
84.7422 +26.3326 0.0179 29.3 106.4 29.6789 10.8 TRIG_01007266
------------------------------------------
Foreground time interval of the image:
-228.928 175.001 (delta_t = 403.929 [sec])
Background time interval of the image:
-239.000 -228.928 (delta_t = 10.072 [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
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)
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 -228.928 sec. to 201.588 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.51927 ( )
Norm@50keV : 1.10701E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 604.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.39e-92 with 57 degrees of freedom
Photon flux (15-150 keV) in 430.5 sec: 4.54818 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 7.58864e-05 ( 0 0 ) ergs/cm2
Cutoff power-law model
Time interval is from -228.928 sec. to 201.588 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.601248 ( -0.275006 0.264023 )
Epeak [keV] : 19.4283 ( -2.13387 1.86101 )
Norm@50keV : 0.489275 ( -0.140336 0.206687 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.74 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.74e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 430.5 sec: 3.48104 ( -0.13202 0.13401 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.25461e-05 ( -1.81284e-06 1.83092e-06 ) ergs/cm2
Band function
Time interval is from -228.928 sec. to 201.588 sec.
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.475278 ( -0.333432 0.549069 )
beta : -5.63196 ( 5.62924 0.954891 )
Epeak [keV] : 20.1457 ( -2.40344 2.61033 )
Norm@50keV : 0.585489 ( -0.209359 0.681222 )
------------------------------------------------------------
Photon flux (15-150 keV) in 430.5 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] : 7.36950 ( )
R^2/D10^2 : 4.78708 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 207.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.19e-19 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.891e-05 6.866e-07
25- 50 2.855e-05 5.661e-07
50-150 5.679e-06 2.131e-07
15-150 5.314e-05 1.141e-06
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 19.2405 (-0.425398 0.440019)
Norm : 49.1708 (-2.33996 2.44464)
------------------------------------------------------------
#Fit statistic : Chi-Squared 75.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.85e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.175e-05 1.005e-06
25- 50 2.697e-05 4.865e-07
50-150 7.563e-06 2.540e-07
15-150 6.628e-05 1.421e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.37723 (-0.443375 0.41369)
R1^2/D10^2 : 15.3942 (-3.52651 5.57409)
kT2 [keV] : 10.1713 (-0.783691 1.07538)
R2^2/D10^2 : 0.486090 (-0.248626 0.384561)
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.13 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.99e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.581e-05 2.226e-06
25- 50 2.792e-05 1.935e-06
50-150 7.138e-06 1.246e-06
15-150 6.087e-05 5.166e-06
Peak spectrum fit
Power-law model
Time interval is from 148.672 sec. to 149.672 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.97806 ( -0.144286 0.153366 )
Norm@50keV : 2.13701E-02 ( -0.00259906 0.0026084 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 94.98 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.19e-03 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 5.78397 ( -0.436248 0.436544 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.54212e-07 ( -2.03202e-08 2.04602e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 148.672 sec. to 149.672 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.91482E-02 ( -1.31186 1.06241 )
Epeak [keV] : 22.5080 ( -5.02169 3.04602 )
Norm@50keV : 1.75092 ( -2.38444 14.054 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.07e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 5.56427 ( -0.44062 0.44092 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.34342e-07 ( -1.8629e-08 1.8942e-08 ) ergs/cm2
Band function
Time interval is from 148.672 sec. to 149.672 sec.
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.157807 ( -0.94798 1.52199 )
beta : -10.0000 ( 10 10 )
Epeak [keV] : 23.0532 ( -5.0034 3.08594 )
Norm@50keV : 2.37742 ( -2.37736 14.026 )
------------------------------------------------------------
Photon flux (15-150 keV) in 1 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] : 6.60391 (-0.431225 0.450712)
R^2/D10^2 : 14.3078 (-3.7102 5.11946)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.12 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.98e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.398e-08 1.083e-08
25- 50 1.147e-07 1.070e-08
50-150 1.532e-08 4.265e-09
15-150 2.239e-07 1.795e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 21.7381 (-2.54797 2.92149)
Norm : 65.1460 (-9.92296 11.9389)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.47 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.19e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.081e-07 1.007e-08
25- 50 1.007e-07 8.755e-09
50-150 3.458e-08 8.840e-09
15-150 2.434e-07 2.065e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.72263 (-3.17526 5.29374)
R1^2/D10^2 : 32.8708 (-22.3447 9974.8)
kT2 [keV] : 8.51295 (-6.9639 6.42026)
R2^2/D10^2 : 2.75790 (-2.70869 10.4214)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.70 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.86e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.010e-07 5.620e-08
25- 50 1.091e-07 5.660e-08
50-150 2.461e-08 1.457e-08
15-150 2.347e-07 1.192e-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: 3.51747 ( )
Norm@50keV : 1.10876E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 592.18 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.53e-90 with 57 degrees of freedom
Photon flux (15-150 keV) in 403.9 sec: 4.54866 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 7.12306e-05 ( 0 0 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.606707 ( -0.277773 0.266579 )
Epeak [keV] : 19.3495 ( -2.15906 1.87939 )
Norm@50keV : 0.488333 ( -0.141426 0.209236 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.25e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 403.9 sec: 3.48713 ( -0.13284 0.13484 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.87299e-05 ( -1.71092e-06 1.72829e-06 ) ergs/cm2
Band function
XSPEC12>exit
XSPEC: quit
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.446418 ( -0.350061 0.504329 )
beta : -5.56601 ( 5.55945 0.678983 )
Epeak [keV] : 20.2636 ( -2.52136 2.39735 )
Norm@50keV : 0.612968 ( -0.218113 0.630966 )
------------------------------------------------------------
Photon flux (15-150 keV) in 403.9 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) = 2.34e-05
S(50-100 keV) = 8.18e-06
T90 vs. Hardness ratio plot
T90 = 382.65600001812 sec.
Hardness ratio (energy fluence ratio) = 0.349573
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.795128
Count Ratio (50-100 keV) / (15-25 keV) = 0.111538
Mask shadow pattern
IMX = -1.590461121139815E-01, IMY = -5.390723303507230E-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:
-239.000000 -228.928000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6197 22.0185 1.9 27.4 98.0 0.4409 6.1 0.8 Crab
84.7164 26.3115 0.3 29.3 106.4 2.9211 37.6 ------ UNKNOWN
159.2850 31.5355 2.7 56.5 -157.1 1.0469 4.3 ------ UNKNOWN
120.8349 -35.8985 3.3 43.3 -50.0 0.3823 3.5 ------ UNKNOWN
126.2799 -34.7874 2.7 44.2 -56.5 0.6708 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-228.928000 175.000600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.8194 22.0206 8.5 27.3 98.3 3.5212 1.4 10.4 Crab
91.7582 50.6577 2.5 47.1 135.5 39.4500 4.6 ------ UNKNOWN
84.7427 26.3325 1.0 29.3 106.4 30.5932 11.1 ------ UNKNOWN
115.5381 15.7463 3.5 14.3 -171.4 5.2273 3.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
302.000600 834.020000
835.000000 928.900610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
154.4784 13.3384 3.6 38.5 63.2 3.7147 3.2 ------ UNKNOWN
143.5026 -11.4165 2.7 52.3 29.9 10.0223 4.3 ------ UNKNOWN
231.6736 45.7144 2.6 51.7 173.4 6.6810 4.4 ------ UNKNOWN
156.5975 -34.0959 2.5 53.0 -2.5 4.7214 4.7 ------ UNKNOWN
191.6742 -27.9822 3.0 34.3 -38.4 2.4064 3.8 ------ UNKNOWN
235.3973 -5.1331 2.8 43.9 -116.3 9.3790 4.2 ------ UNKNOWN
242.4033 5.1682 2.5 49.2 -131.9 11.8427 4.6 ------ UNKNOWN
Plot creation:
Thu Nov 19 06:37:43 EST 2020