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
244.8033 -16.0867 0.0065 24.1 -46.7 16.0898 29.4 TRIG_00868851
------------------------------------------
Foreground time interval of the image:
-64.796 68.560 (delta_t = 133.356 [sec])
70.000 205.240 (delta_t = 135.240 [sec])
206.000 273.501 (delta_t = 67.501 [sec])
Background time interval of the image:
-239.000 -64.796 (delta_t = 174.204 [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
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)
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
-64.796000 68.560000
70.000000 205.240000
206.000000 344.560000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 6.61158 ( )
Norm@50keV : 1.98531E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 114.45 using 59 PHA bins.
# Reduced chi-squared = 2.0078 for 57 degrees of freedom
# Null hypothesis probability = 9.896501e-06
Photon flux (15-150 keV) in 407.2 sec: 1.52027 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.81017e-05 ( 0 0 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-64.796000 68.560000
70.000000 205.240000
206.000000 344.560000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 2.34072E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 1210.45 using 59 PHA bins.
# Reduced chi-squared = 21.6152 for 56 degrees of freedom
# Null hypothesis probability = 1.772243e-216
Photon flux (15-150 keV) in 407.2 sec: 1.32741 ( -0.13025 0.12838 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.60517e-05 ( -1.42658e-06 1.40386e-06 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-64.796000 68.560000
70.000000 205.240000
206.000000 344.560000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -8.81461 ( )
beta : -6.63211 ( )
Epeak [keV] : 382.437 ( )
Norm@50keV : 2.65169E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 114.48 using 59 PHA bins.
# Reduced chi-squared = 2.0815 for 55 degrees of freedom
# Null hypothesis probability = 4.567153e-06
Photon flux (15-150 keV) in 407.2 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] : 2.67457 (-0.0911884 0.0978274)
R^2/D10^2 : 398.739 (-109.467 147.674)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.50 using 59 PHA bins.
# Reduced chi-squared = 1.132 for 57 degrees of freedom
# Null hypothesis probability = 2.308553e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.434e-05 1.450e-06
25- 50 1.375e-06 1.142e-07
50-150 8.229e-10 2.710e-10
15-150 1.572e-05 1.435e-06
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 4.43081 (-0.207813 0.228555)
Norm : 513.622 (-118.925 151.941)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.19 using 59 PHA bins.
# Reduced chi-squared = 1.179 for 57 degrees of freedom
# Null hypothesis probability = 1.673469e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.540e-05 1.509e-06
25- 50 1.461e-06 1.165e-07
50-150 3.967e-09 1.273e-09
15-150 1.686e-05 1.218e-06
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.67449 (-0.0973606 0.0923189)
R1^2/D10^2 : 398.842 (-101.898 155.648)
kT2 [keV] : 1.00000E-04 (-0.0001 -0.0001)
R2^2/D10^2 : 6.04935E-16 (-6.04935e-16 -6.04935e-16)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.52 using 59 PHA bins.
#Fit statistic : Chi-Squared = 64.50 using 59 PHA bins.
# Reduced chi-squared = 1.173 for 55 degrees of freedom
# Reduced chi-squared = 1.173 for 55 degrees of freedom
# Null hypothesis probability = 1.780997e-01
# Null hypothesis probability = 1.783990e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.430e-05 1.431e-06
25- 50 1.382e-06 1.224e-07
50-150 8.438e-10 3.085e-10
15-150 1.568e-05 1.450e-06
Peak spectrum fit
Power-law model
Time interval is from 231.176 sec. to 232.176 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 4.15844 ( -0.490008 0.555356 )
Norm@50keV : 2.77511E-03 ( -0.00115166 0.00148511 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.38 using 59 PHA bins.
# Reduced chi-squared = 0.9014 for 57 degrees of freedom
# Null hypothesis probability = 6.849927e-01
Photon flux (15-150 keV) in 1 sec: 1.96769 ( -0.269197 0.269206 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.87573e-08 ( -1.02775e-08 1.05705e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 231.176 sec. to 232.176 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 2.26750E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 129.80 using 59 PHA bins.
# Reduced chi-squared = 2.3178 for 56 degrees of freedom
# Null hypothesis probability = 8.600002e-08
Photon flux (15-150 keV) in 1 sec: 1.96081 ( -0.26851 0.13731 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.79147e-08 ( -1.1666e-08 1.12913e-08 ) ergs/cm2
Band function
Time interval is from 231.176 sec. to 232.176 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 3.76307 ( 1.66549 1.66549 )
beta : -4.29814 ( 4.38296 0.688946 )
Epeak [keV] : 12.6670 ( -2.71831 2.63167 )
Norm@50keV : 3.43176E+04 ( -34321.9 5.44695e+07 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.03 using 59 PHA bins.
# Reduced chi-squared = 0.9278 for 55 degrees of freedom
# Null hypothesis probability = 6.270310e-01
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] : 3.55337 (-0.4811 0.56994)
R^2/D10^2 : 96.2238 (-55.5825 138.203)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.26 using 59 PHA bins.
# Reduced chi-squared = 0.9694 for 57 degrees of freedom
# Null hypothesis probability = 5.407670e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.784e-08 1.670e-08
25- 50 1.215e-08 4.810e-09
50-150 6.910e-11 5.776e-11
15-150 6.007e-08 1.781e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 8.30532 (-1.84356 2.60651)
Norm : 100.353 (-46.4347 95.3964)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.59 using 59 PHA bins.
# Reduced chi-squared = 0.9227 for 57 degrees of freedom
# Null hypothesis probability = 6.409656e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.710e-08 1.109e-08
25- 50 1.551e-08 5.147e-09
50-150 6.166e-10 4.701e-10
15-150 6.323e-08 1.758e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.94334 (-1.34806 0.749115)
R1^2/D10^2 : 254.471 (-184.84 9984.03)
kT2 [keV] : 8.75683 (-7.17593 -8.77033)
R2^2/D10^2 : 0.366447 (-0.370253 2.64568)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.70 using 59 PHA bins.
# Reduced chi-squared = 0.9219 for 55 degrees of freedom
# Null hypothesis probability = 6.393372e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.761e-08 2.535e-08
25- 50 1.672e-08 8.870e-09
50-150 3.854e-09 3.040e-09
15-150 6.819e-08 3.521e-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: 6.54831 ( )
Norm@50keV : 2.06104E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 120.52 using 59 PHA bins.
# Reduced chi-squared = 2.1144 for 57 degrees of freedom
# Null hypothesis probability = 1.888764e-06
Photon flux (15-150 keV) in 336.1 sec: 1.47922 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.4573e-05 ( 0 0 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 2.49443E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 1155.46 using 59 PHA bins.
# Reduced chi-squared = 20.6333 for 56 degrees of freedom
# Null hypothesis probability = 4.410420e-205
Photon flux (15-150 keV) in 336.1 sec: 1.31079 ( -0.12667 0.12499 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.30793e-05 ( -1.14597e-06 1.12883e-06 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -8.74726 ( )
beta : -6.57505 ( )
Epeak [keV] : 389.038 ( )
Norm@50keV : 2.73802E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 120.58 using 59 PHA bins.
# Reduced chi-squared = 2.1923 for 55 degrees of freedom
# Null hypothesis probability = 8.243045e-07
Photon flux (15-150 keV) in 336.1 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) = 1.65e-06
S(50-100 keV) = 6.73e-08
T90 vs. Hardness ratio plot
T90 = 346.611999869347 sec.
Hardness ratio (energy fluence ratio) = 0.0407879
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.0854453
Count Ratio (50-100 keV) / (15-25 keV) = -0.00238319
Mask shadow pattern
IMX = 3.076035742333109E-01, IMY = 3.262016759499714E-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:
-239.000000 -64.796000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.1905 -60.6083 4.9 55.4 -163.6 2.2664 2.4 3.8 Cen X-3
186.4374 -62.6937 7.4 47.4 -164.4 -0.8998 -1.6 7.6 GX 301-2
244.9569 -15.7861 58.6 24.4 -46.1 0.0570 0.2 8.8 Sco X-1
255.9848 -37.6841 5.8 0.5 -5.1 -0.4846 -2.0 9.6 4U 1700-377
256.2545 -36.5302 4.5 1.7 -8.0 0.6157 2.6 10.8 GX 349+2
263.0117 -24.9026 24.4 14.6 6.7 -0.1256 -0.5 9.4 GX 1+4
264.5916 -44.2703 0.0 9.0 115.3 -0.5219 -2.1 12.6 4U 1735-44
268.4980 -1.4225 39.6 38.6 0.6 -0.1041 -0.3 8.0 SW J1753.5-0127
270.3321 -25.2354 6.0 17.9 27.6 0.5442 2.2 9.7 GX 5-1
270.2620 -25.5817 2.4 17.6 28.2 1.2277 5.0 9.9 GRS 1758-258
273.8726 -14.0070 27.9 29.0 18.3 -0.1258 -0.4 8.0 GX 17+2
276.0154 -30.3554 9.9 18.4 50.7 0.3187 1.2 4.7 H1820-303
285.1937 -24.9258 544.6 28.2 50.4 0.0073 0.0 8.6 HT1900.1-2455
263.0759 -34.0109 6.0 7.2 36.6 0.4592 1.9 11.4 GX 354-0
299.6750 -46.2838 3.4 33.0 98.4 1.7157 3.5 ------ UNKNOWN
278.5614 13.1177 2.5 55.6 7.1 5.3524 4.7 ------ UNKNOWN
220.6286 -67.7923 3.5 35.4 -177.9 1.3207 3.3 ------ UNKNOWN
266.6686 3.0744 3.5 42.5 -3.9 1.3723 3.3 ------ UNKNOWN
213.0615 -53.8551 2.9 32.9 -152.5 1.1779 4.0 ------ UNKNOWN
198.5193 -56.5959 2.4 41.4 -155.6 2.0612 4.9 ------ UNKNOWN
223.6976 -16.6914 2.8 35.4 -81.6 2.3676 4.1 ------ UNKNOWN
UNKNOWN
UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-64.796000 68.560000
70.000000 205.240000
206.000000 273.500600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.1321 -60.6758 5.8 55.4 -163.6 -3.6651 -2.0 6.3 Cen X-3
186.5937 -62.7413 6.9 47.3 -164.4 1.6763 1.7 2.5 GX 301-2
245.0146 -15.6473 4.7 24.5 -45.8 -1.3219 -2.4 2.1 Sco X-1
256.1967 -37.8262 6.4 0.5 18.6 -0.7814 -1.8 10.0 4U 1700-377
256.2399 -36.5260 3.2 1.7 -8.4 -1.5274 -3.6 11.3 GX 349+2
262.9939 -24.7397 34.2 14.8 6.4 0.1515 0.3 0.9 GX 1+4
264.8951 -44.6294 0.0 9.3 116.2 -0.8277 -1.8 12.6 4U 1735-44
268.2696 -1.3684 10.9 38.6 0.2 -0.6915 -1.1 7.8 SW J1753.5-0127
270.4375 -24.9607 6.7 18.1 27.3 0.8339 1.7 11.0 GX 5-1
270.4148 -25.7941 5.4 17.5 29.0 -1.0399 -2.1 6.8 GRS 1758-258
273.8806 -13.9558 9.8 29.1 18.3 0.6482 1.2 8.8 GX 17+2
275.7417 -30.4452 4.6 18.2 50.6 -1.2188 -2.5 10.6 H1820-303
285.0358 -24.9521 84.9 28.0 50.3 0.0877 0.1 1.9 HT1900.1-2455
262.8293 -33.7558 5.9 7.2 34.0 0.8589 2.0 9.3 GX 354-0
282.1492 -6.2111 2.6 39.9 23.4 3.6796 4.4 ------ UNKNOWN
244.7853 -16.1241 0.4 24.1 -46.8 15.6800 28.7 ------ UNKNOWN
253.5193 4.0171 2.8 42.3 -23.4 2.8924 4.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Sat Oct 27 16:19:08 EDT 2018