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
307.5687 +37.5747 0.0622 43.1 164.3 3.9357 3.1 TRIG_01074326
------------------------------------------
Foreground time interval of the image:
-64.728 112.950 (delta_t = 177.678 [sec])
114.000 180.860 (delta_t = 66.860 [sec])
181.000 196.460 (delta_t = 15.460 [sec])
197.000 256.370 (delta_t = 59.370 [sec])
257.000 277.370 (delta_t = 20.370 [sec])
278.000 499.570 (delta_t = 221.570 [sec])
501.000 536.568 (delta_t = 35.568 [sec])
Background time interval of the image:
-239.000 -185.240 (delta_t = 53.760 [sec])
-184.000 -158.610 (delta_t = 25.390 [sec])
-158.000 -64.728 (delta_t = 93.272 [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
Multiple GTIs in the spectrum
tstart tstop
-64.728000 112.950000
114.000000 180.860000
181.000000 196.460000
197.000000 256.370000
257.000000 277.370000
278.000000 499.570000
501.000000 536.568000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.04907 ( -0.232002 0.251965 )
Norm@50keV : 7.08745E-04 ( -0.000135416 0.000140134 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.68 using 59 PHA bins.
# Reduced chi-squared = 1.170 for 57 degrees of freedom
# Null hypothesis probability = 1.784023e-01
Photon flux (15-150 keV) in 596.9 sec: 0.202033 ( -0.0185472 0.0185503 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.20106e-06 ( -5.54797e-07 5.70583e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-64.728000 112.950000
114.000000 180.860000
181.000000 196.460000
197.000000 256.370000
257.000000 277.370000
278.000000 499.570000
501.000000 536.568000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.98051 ( -0.266858 0.00643604 )
Epeak [keV] : 0.554521 ( -0.16863 13.8402 )
Norm@50keV : 3.83627E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.52 using 59 PHA bins.
# Reduced chi-squared = 1.170 for 56 degrees of freedom
# Null hypothesis probability = 1.800051e-01
Photon flux (15-150 keV) in 596.9 sec: 0.198600 ( -0.018991 0.019033 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.91241e-06 ( -6.21003e-07 6.74002e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-64.728000 112.950000
114.000000 180.860000
181.000000 196.460000
197.000000 256.370000
257.000000 277.370000
278.000000 499.570000
501.000000 536.568000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.18384 ( -0.117745 0.333838 )
beta : -3.42599 ( 3.27463 0.354675 )
Epeak [keV] : 18.4990 ( -0.773995 7.18663 )
Norm@50keV : 486.814 ( -487.122 298.637 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.19 using 59 PHA bins.
# Reduced chi-squared = 1.094 for 55 degrees of freedom
# Null hypothesis probability = 2.934480e-01
Photon flux (15-150 keV) in 596.9 sec: 0.202063 ( 6.79794 -0.019744 ) 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] : 5.03671 (-0.500814 0.583679)
R^2/D10^2 : 1.58276 (-0.650447 1.0831)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.19 using 59 PHA bins.
# Reduced chi-squared = 1.354 for 57 degrees of freedom
# Null hypothesis probability = 3.869504e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.366e-06 3.426e-07
25- 50 1.573e-06 2.984e-07
50-150 6.626e-08 3.161e-08
15-150 4.005e-06 5.584e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 17.7319 (-3.41833 4.4903)
Norm : 2.78626 (-0.717893 1.0484)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.312e-06 3.029e-07
25- 50 1.836e-06 2.608e-07
50-150 4.458e-07 1.924e-07
15-150 4.594e-06 5.724e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.08177 (-0.554489 0.588272)
R1^2/D10^2 : 3.76337 (-1.77563 3.81945)
kT2 [keV] : 13.9232 (-3.845 5.82553)
R2^2/D10^2 : 8.59620E-03 (-0.00674347 0.0284035)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.462e-06 7.178e-07
25- 50 1.638e-06 5.602e-07
50-150 1.002e-06 6.252e-07
15-150 5.102e-06 1.735e-06
Peak spectrum fit
Power-law model
Time interval is from 246.572 sec. to 247.572 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.42545 ( -0.649037 0.969758 )
Norm@50keV : 5.52440E-03 ( -0.00321911 0.00303733 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.08 using 59 PHA bins.
# Reduced chi-squared = 0.8435 for 57 degrees of freedom
# Null hypothesis probability = 7.939408e-01
Photon flux (15-150 keV) in 1 sec: 1.03758 ( -0.382699 0.382701 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.42084e-08 ( -2.34262e-08 2.51408e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 246.572 sec. to 247.572 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.11631 ( -5.0149 1.00878 )
Epeak [keV] : 29.0203 ( )
Norm@50keV : 3.10459E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.42 using 59 PHA bins.
# Reduced chi-squared = 0.8467 for 56 degrees of freedom
# Null hypothesis probability = 7.860122e-01
Photon flux (15-150 keV) in 1 sec: 1.01580 ( -0.382975 0.38519 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.26148e-08 ( -2.21404e-08 2.49402e-08 ) ergs/cm2
Band function
Time interval is from 246.572 sec. to 247.572 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.13889 ( -3.02564 1.72156 )
beta : -10.0000 ( 10 20 )
Epeak [keV] : 28.6896 ( -19.3193 -28.6984 )
Norm@50keV : 3.02508E-02 ( -0.030224 33.423 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.42 using 59 PHA bins.
# Reduced chi-squared = 0.8621 for 55 degrees of freedom
# Null hypothesis probability = 7.563905e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 5.27011e-08 ( -5.26941e-08 -2.22074e-08 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 9.39403 (-3.73782 4.71284)
R^2/D10^2 : 0.619616 (-0.618099 3.96961)
(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 1.087e-08 6.780e-09
25- 50 2.467e-08 1.604e-08
50-150 1.071e-08 8.220e-09
15-150 4.624e-08 2.888e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 41.1918 (-24.1347 72.1077)
Norm : 6.70273 (-3.26367 8.29749)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.554e-08 9.867e-09
25- 50 2.070e-08 1.274e-08
50-150 1.653e-08 1.293e-08
15-150 5.278e-08 3.531e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.91932 (-2.51782 11.6765)
R1^2/D10^2 : 1046.09 (-1043.72 -1043.72)
kT2 [keV] : 11.0880 (-4.34553 -11.0926)
R2^2/D10^2 : 0.295175 (-0.294639 1.79492)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.523e-08 8.385e-09
25- 50 2.102e-08 1.289e-08
50-150 1.624e-08 1.273e-08
15-150 5.250e-08 2.965e-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: 3.04907 ( -0.232002 0.251965 )
Norm@50keV : 7.08745E-04 ( -0.000135416 0.000140134 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.68 using 59 PHA bins.
# Reduced chi-squared = 1.170 for 57 degrees of freedom
# Null hypothesis probability = 1.784023e-01
Photon flux (15-150 keV) in 596.9 sec: 0.202033 ( -0.0185472 0.0185503 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.20106e-06 ( -5.54797e-07 5.70583e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.98051 ( -0.266858 0.00655275 )
Epeak [keV] : 0.554521 ( -0.16863 13.8402 )
Norm@50keV : 3.83627E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.52 using 59 PHA bins.
# Reduced chi-squared = 1.170 for 56 degrees of freedom
# Null hypothesis probability = 1.800051e-01
Photon flux (15-150 keV) in 596.9 sec: 0.198600 ( -0.018991 0.019033 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.91241e-06 ( -6.21003e-07 6.74079e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.18333 ( -0.338847 0.268995 )
beta : -3.42598 ( 3.27443 0.354477 )
Epeak [keV] : 18.4989 ( -0.774459 7.18621 )
Norm@50keV : 486.326 ( -486.634 299.134 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.19 using 59 PHA bins.
# Reduced chi-squared = 1.094 for 55 degrees of freedom
# Null hypothesis probability = 2.934450e-01
Photon flux (15-150 keV) in 596.9 sec: 0.202063 ( 6.79794 -0.019744 ) 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) = 1.73e-06
S(50-100 keV) = 8.35e-07
T90 vs. Hardness ratio plot
T90 = 545.93599998951 sec.
Hardness ratio (energy fluence ratio) = 0.482659
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.524233
Count Ratio (50-100 keV) / (15-25 keV) = 0.1869
Mask shadow pattern
IMX = -9.017255753681908E-01, IMY = -2.537828231121534E-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 -185.240000
-184.000000 -158.610000
-158.000000 -64.728000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.7217 35.1952 7.1 48.5 169.9 -1.0466 -1.6 6.5 Cyg X-1
308.0277 41.0336 5.2 40.1 166.8 0.7563 2.2 6.1 Cyg X-3
326.1923 38.4688 21.3 34.7 145.1 -0.1769 -0.5 8.9 Cyg X-2
307.8503 37.6122 1.7 43.0 164.0 2.9175 6.7 ------ UNKNOWN
320.3973 68.9134 3.0 18.4 -151.5 0.7901 3.8 ------ UNKNOWN
267.7279 44.2130 3.3 54.4 -157.5 2.8280 3.5 ------ UNKNOWN
98.4628 64.1264 3.2 36.8 -50.1 1.2652 3.6 ------ UNKNOWN
191.2061 74.5979 3.1 41.3 -98.9 4.2294 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-64.728000 112.950000
114.000000 180.860000
181.000000 196.460000
197.000000 256.370000
257.000000 277.370000
278.000000 499.570000
501.000000 536.568000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.3583 35.1634 0.0 48.7 170.2 -7.9077 -4.5 11.6 Cyg X-1
308.1037 41.0964 5.9 40.0 166.7 -2.0782 -1.9 8.6 Cyg X-3
326.1412 38.1719 5.7 34.9 144.9 -2.1340 -2.0 9.1 Cyg X-2
Post-slew image of 15-350 keV band
Time interval of the image:
813.300600 889.770000
891.000000 963.010000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4847 22.0529 0.7 29.6 136.4 5.0873 16.5 8.6 Crab
135.3711 -40.5718 5.0 49.6 -35.9 1.3652 2.3 7.2 Vela X-1
88.2093 51.2569 2.0 53.2 164.2 4.7213 5.7 ------ UNKNOWN
86.6208 -16.1004 2.4 22.8 41.6 1.0204 4.9 ------ UNKNOWN
96.8756 10.8607 3.2 13.0 146.3 0.7439 3.6 ------ UNKNOWN
99.7214 -58.8213 2.7 58.5 -1.8 6.0431 4.3 ------ UNKNOWN
117.5624 30.5749 2.9 33.8 -161.7 0.9900 4.0 ------ UNKNOWN
124.2063 -51.9855 3.1 54.5 -19.6 2.5258 3.7 ------ UNKNOWN
131.7770 -24.8996 2.7 36.8 -50.0 1.4744 4.3 ------ UNKNOWN
139.1901 48.3996 3.1 57.8 -156.6 4.3258 3.7 ------ UNKNOWN
Plot creation:
Wed Sep 22 21:05:28 EDT 2021