Special notes of this burst
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
251.1393 72.3640 0.0149 22.7217 -33.4050 1.8650209 12.917 TRIG_00993768
Foreground time interval of the image:
-12.099 72.501 (delta_t = 84.600 [sec])
Background time interval of the image:
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 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)
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 -74.768 sec. to 204.076 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.02508 ( -0.0240847 0.0239666 )
Norm@50keV : 1.65253E-02 ( -0.000239245 0.000238608 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 21.29 using 59 bins.
Reduced chi-squared = 0.373509
# Null hypothesis probability of 1.00e+00 with 57 degrees of freedom
Photon flux (15-150 keV) in 278.8 sec: 1.90532 ( -0.02906 0.02913 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.93905e-05 ( -6.23901e-07 6.236e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -74.768 sec. to 204.076 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.919370 ( -0.10226 0.0506214 )
Epeak [keV] : 694.212 ( -303.848 7233.44 )
Norm@50keV : 1.80739E-02 ( -0.00134685 0.00160187 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 18.08 using 59 bins.
Reduced chi-squared = 0.322857
# Null hypothesis probability of 1.00e+00 with 56 degrees of freedom
Photon flux (15-150 keV) in 278.8 sec: 0.316846 ( -0.043777 0.032488 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.93245e-05 ( -6.28518e-07 6.27529e-07 ) ergs/cm2
Band function
Time interval is from -74.768 sec. to 204.076 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] : 26.1109 ( )
R^2/D10^2 : 3.95722E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 903.68 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.12e-152 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.276e-06 3.541e-08
25- 50 7.399e-06 1.589e-07
50-150 3.713e-05 5.715e-07
15-150 4.580e-05 5.994e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 8.69962 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 1685.85 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.34e-315 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.040e-06 9.061e-08
25- 50 1.162e-05 1.687e-07
50-150 2.548e-05 3.917e-07
15-150 4.314e-05 6.134e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.72981 (-0.663534 0.704938)
R1^2/D10^2 : 0.473009 (-0.0892799 0.116284)
kT2 [keV] : 40.1191 (-2.23406 2.73925)
R2^2/D10^2 : 8.97013E-03 (-0.00167732 0.00180973)
------------------------------------------------------------
#Fit statistic : Chi-Squared 37.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.65e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.036e-06 1.756e-07
25- 50 9.556e-06 2.579e-07
50-150 3.685e-05 8.225e-07
15-150 4.944e-05 1.101e-06
Peak spectrum fit
Power-law model
Time interval is from -60.068 sec. to -59.068 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.770524 ( -0.0289792 0.0288229 )
Norm@50keV : 0.884779 ( -0.0158786 0.0158357 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.02 using 59 bins.
Reduced chi-squared = 1.12316
# Null hypothesis probability of 2.44e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 3.41045 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.04708e-05 ( -1.75713e-07 1.75777e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -60.068 sec. to -59.068 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.368350 ( -0.129726 0.12634 )
Epeak [keV] : 270.821 ( -49.1883 90.1713 )
Norm@50keV : 1.25758 ( -0.128667 0.146315 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 33.13 using 59 bins.
Reduced chi-squared = 0.591607
# Null hypothesis probability of 9.94e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 100.512 ( -1.7938 1.799 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.04674e-05 ( -1.77764e-07 1.77951e-07 ) ergs/cm2
Band function
Time interval is from -60.068 sec. to -59.068 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] : 28.2542 ( )
R^2/D10^2 : 1.87388 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 370.52 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.65e-47 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.426e-07 7.650e-09
25- 50 1.459e-06 3.700e-08
50-150 8.401e-06 1.710e-07
15-150 1.010e-05 1.790e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 413.767 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 2042.23 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 0.00e+00 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.030e-06 1.850e-08
25- 50 1.982e-06 3.750e-08
50-150 4.347e-06 7.850e-08
15-150 7.359e-06 1.425e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.3169 (-1.10832 1.2307)
R1^2/D10^2 : 15.5166 (-3.90051 5.74396)
kT2 [keV] : 40.5931 (-2.76673 3.70056)
R2^2/D10^2 : 0.563103 (-0.133508 0.140789)
------------------------------------------------------------
#Fit statistic : Chi-Squared 32.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.92e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.582e-07 3.415e-08
25- 50 1.694e-06 9.050e-08
50-150 8.402e-06 2.925e-07
15-150 1.055e-05 3.300e-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: 2.46074 ( -0.236408 0.258517 )
Norm@50keV : 9.61043E-04 ( -0.000178894 0.000178032 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.17 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.91e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 84.6 sec: 0.184345 ( -0.0195596 0.0195619 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.04731e-07 ( -1.09813e-07 1.14696e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.92853 ( )
Epeak [keV] : 4.85951 ( )
Norm@50keV : 2.07585E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.32 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.89e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 84.6 sec: 0.181334 ( -0.020043 0.020118 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.63869e-07 ( -1.18853e-07 1.3537e-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) = 9.31e-06
S(50-100 keV) = 1.83e-05
T90 vs. Hardness ratio plot
T90 = 13.0999999046326 sec.
Hardness ratio (energy fluence ratio) = 1.96563
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.81669
Count Ratio (50-100 keV) / (15-25 keV) = 2.17963
Mask shadow pattern
IMX = 3.495756185963115E-01, IMY = 2.305463279172886E-01
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:
-12.099400 72.500600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.6293 35.2697 4.4 21.0 -150.9 0.3565 2.6 9.5 Her X-1
268.3256 -1.3882 4.9 53.2 169.2 -1.3108 -2.4 4.6 SW J1753.5-0127
288.8475 10.9404 6.8 42.8 140.1 -0.6521 -1.7 2.9 GRS 1915+105
299.6075 35.1847 2.6 25.2 104.0 0.8218 4.5 1.3 Cyg X-1
308.1355 40.9731 3.6 26.3 83.7 0.6096 3.2 1.7 Cyg X-3
326.1318 38.4348 13.8 38.9 72.0 -0.3934 -0.8 7.0 Cyg X-2
251.1394 72.3639 0.9 22.7 -33.4 1.8640 12.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
117.300590 963.094800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5869 35.3285 7.0 37.1 170.2 -1.9063 -1.6 6.4 Her X-1
301.3835 54.9474 3.1 26.9 97.8 3.8536 3.8 ------ UNKNOWN
251.2052 72.3353 1.7 0.0 -110.7 4.8972 6.9 ------ UNKNOWN
100.8998 69.3454 3.0 37.0 -22.1 3.7645 3.9 ------ UNKNOWN
Plot creation:
Sun Nov 15 21:50:34 EST 2020