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
256.0091 -37.8672 0.0122 25.9 -153.8 21.4504 15.6 TRIG_01062273
------------------------------------------
Foreground time interval of the image:
-15.899 77.000 (delta_t = 92.899 [sec])
86.000 145.840 (delta_t = 59.840 [sec])
147.000 255.910 (delta_t = 108.910 [sec])
257.000 379.240 (delta_t = 122.240 [sec])
380.000 435.260 (delta_t = 55.260 [sec])
436.000 502.820 (delta_t = 66.820 [sec])
503.000 503.260 (delta_t = 0.260 [sec])
504.000 504.160 (delta_t = 0.160 [sec])
506.000 805.401 (delta_t = 299.401 [sec])
Background time interval of the image:
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
-56.212000 77.000000
86.000000 145.840000
147.000000 255.910000
257.000000 379.240000
380.000000 435.260000
436.000000 502.820000
503.000000 503.260000
504.000000 504.160000
506.000000 844.668000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.23144 ( -0.15387 0.162394 )
Norm@50keV : 8.70519E-04 ( -7.56656e-05 7.51076e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.09 using 55 PHA bins.
# Reduced chi-squared = 1.360 for 53 degrees of freedom
# Null hypothesis probability = 4.164049e-02
Photon flux (15-150 keV) in 885.4 sec: 0.284697 ( -0.0190581 0.020096 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.03928e-05 ( -5.12496e-07 5.16587e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-56.212000 77.000000
86.000000 145.840000
147.000000 255.910000
257.000000 379.240000
380.000000 435.260000
436.000000 502.820000
503.000000 503.260000
504.000000 504.160000
506.000000 844.668000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.63862 ( -1.30428 0.447136 )
Epeak [keV] : 8.62645 ( )
Norm@50keV : 7.26469E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.89 using 55 PHA bins.
# Reduced chi-squared = 1.267 for 52 degrees of freedom
# Null hypothesis probability = 9.325597e-02
Photon flux (15-150 keV) in 885.4 sec: 0.242180 ( -0.029299 0.033069 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.91739e-06 ( -9.23968e-07 1.06089e-06 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-56.212000 77.000000
86.000000 145.840000
147.000000 255.910000
257.000000 379.240000
380.000000 435.260000
436.000000 502.820000
503.000000 503.260000
504.000000 504.160000
506.000000 844.668000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.45192 ( )
beta : -8.89282 ( )
Epeak [keV] : 24.7621 ( )
Norm@50keV : 3.56777E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 158.07 using 55 PHA bins.
# Reduced chi-squared = 3.0994 for 51 degrees of freedom
# Null hypothesis probability = 6.928828e-13
Photon flux (15-150 keV) in 885.4 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] : 6.96147 (-0.351803 0.367618)
R^2/D10^2 : 0.405949 (-0.0886482 0.115994)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 81.02 using 55 PHA bins.
# Reduced chi-squared = 1.529 for 53 degrees of freedom
# Null hypothesis probability = 7.902900e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.782e-06 2.413e-07
25- 50 3.770e-06 2.152e-07
50-150 6.123e-07 1.075e-07
15-150 7.164e-06 3.754e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 21.9961 (-1.87134 2.11279)
Norm : 2.55359 (-0.296495 0.339928)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.785e-06 2.457e-07
25- 50 3.557e-06 1.700e-07
50-150 1.244e-06 2.032e-07
15-150 8.586e-06 3.958e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.94818 (-1.16053 1.07126)
R1^2/D10^2 : 1.44677 (-0.693342 2.13364)
kT2 [keV] : 10.8383 (-2.67788 11.148)
R2^2/D10^2 : 2.79349E-02 (-0.026534 0.121587)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.593e-06 8.907e-07
25- 50 3.580e-06 9.664e-07
50-150 1.175e-06 5.865e-07
15-150 8.348e-06 2.336e-06
Peak spectrum fit
Power-law model
Time interval is from -56.308 sec. to -55.308 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.12017 ( -1.11537 1.51751 )
Norm@50keV : 4.36181E-03 ( -0.00290747 0.00276915 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 31.88 using 55 PHA bins.
# Reduced chi-squared = 0.6014 for 53 degrees of freedom
# Null hypothesis probability = 9.905094e-01
Photon flux (15-150 keV) in 1 sec: 0.700657 ( -0.447524 0.540275 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.04996e-08 ( -2.47241e-08 2.52652e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -56.308 sec. to -55.308 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.54468 ( )
Epeak [keV] : 51.3491 ( )
Norm@50keV : 4.61514 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 29.50 using 55 PHA bins.
# Reduced chi-squared = 0.5673 for 52 degrees of freedom
# Null hypothesis probability = 9.949661e-01
Photon flux (15-150 keV) in 1 sec: 0.439747 ( -0.268399 0.501113 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.11963e-08 ( -1.80861e-08 2.4605e-08 ) ergs/cm2
Band function
Time interval is from -56.308 sec. to -55.308 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.81226 ( -6.26078 -4.81226 )
beta : -9.37167 ( 9.37167 19.3587 )
Epeak [keV] : 53.6378 ( -18.9146 19.4636 )
Norm@50keV : 4.58108 ( -2.43591 1.28282e+07 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 29.55 using 55 PHA bins.
# Reduced chi-squared = 0.5793 for 51 degrees of freedom
# Null hypothesis probability = 9.930174e-01
Photon flux (15-150 keV) in 1 sec: 0.461072 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 11.3514 (-4.80098 6.46863)
R^2/D10^2 : 0.223233 (-0.223233 1.58083)
(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 6.044e-09 4.091e-09
25- 50 1.778e-08 1.132e-08
50-150 1.325e-08 9.830e-09
15-150 3.708e-08 2.452e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 50.3867 (-50.6271 -50.6271)
Norm : 4.33666 (-2.43137 5.92027)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.062e-08 6.975e-09
25- 50 1.530e-08 1.005e-08
50-150 1.496e-08 1.252e-08
15-150 4.088e-08 2.886e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.80950 (-2.81969 13.0504)
R1^2/D10^2 : 47.7304 (-47.4197 -47.4197)
kT2 [keV] : 12.9930 (-5.24869 -13.0141)
R2^2/D10^2 : 0.119059 (-0.118553 0.843384)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.013e-08 4.945e-09
25- 50 1.535e-08 9.900e-09
50-150 1.566e-08 1.182e-08
15-150 4.114e-08 2.323e-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: 3.29440 ( -0.164765 0.174694 )
Norm@50keV : 8.30120E-04 ( -7.81462e-05 7.76736e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.13 using 55 PHA bins.
# Reduced chi-squared = 1.361 for 53 degrees of freedom
# Null hypothesis probability = 4.136510e-02
Photon flux (15-150 keV) in 805.8 sec: 0.285056 ( -0.0200974 0.0213087 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.33447e-06 ( -4.83601e-07 4.88751e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.72948 ( )
Epeak [keV] : 6.55563 ( )
Norm@50keV : 6.69537E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.16 using 55 PHA bins.
# Reduced chi-squared = 1.292 for 52 degrees of freedom
# Null hypothesis probability = 7.680214e-02
Photon flux (15-150 keV) in 805.8 sec: 0.245595 ( -0.030428 0.03458 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.11634e-06 ( -8.56984e-07 9.88555e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.46298 ( )
beta : -9.06451 ( )
Epeak [keV] : 23.7763 ( )
Norm@50keV : 3.58696E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 154.85 using 55 PHA bins.
# Reduced chi-squared = 3.0363 for 51 degrees of freedom
# Null hypothesis probability = 2.111220e-12
Photon flux (15-150 keV) in 805.8 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) = 3.38e-06
S(50-100 keV) = 1.44e-06
T90 vs. Hardness ratio plot
T90 = 790.980000019073 sec.
Hardness ratio (energy fluence ratio) = 0.426036
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.729033
Count Ratio (50-100 keV) / (15-25 keV) = 0.122307
Mask shadow pattern
IMX = -4.350908060924887E-01, IMY = 2.137458668236687E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-15.899400 77.000000
86.000000 145.840000
147.000000 255.910000
257.000000 379.240000
380.000000 435.260000
436.000000 502.820000
503.000000 503.260000
504.000000 504.160000
506.000000 805.400600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9863 -15.6310 0.4 27.5 -98.1 57.1917 30.9 0.7 Sco X-1
254.4164 35.2901 6.9 55.5 -26.0 -8.7484 -1.7 3.7 Her X-1
256.0092 -37.8672 0.7 25.9 -153.8 21.4514 15.6 1.7 4U 1700-377
256.6417 -36.3199 0.0 24.4 -152.3 -3.3978 -2.8 11.7 GX 349+2
263.1598 -24.7868 5.5 12.4 -136.9 2.2402 2.1 8.6 GX 1+4
264.6669 -44.4640 14.1 28.4 -173.5 0.9737 0.8 3.4 4U 1735-44
268.2949 -1.4138 96.8 16.6 -26.0 0.1356 0.1 5.0 SW J1753.5-0127
270.4257 -25.1178 5.8 8.5 -167.2 2.4036 2.1 8.0 GX 5-1
270.4372 -25.6432 3.8 9.0 -168.5 4.3061 3.7 9.4 GRS 1758-258
273.9423 -14.1189 94.6 3.0 -0.9 0.1360 0.1 6.2 GX 17+2
276.0155 -30.4708 10.0 13.5 164.1 1.2530 1.2 7.8 H1820-303
285.0321 -25.0675 5.1 13.3 121.6 2.7784 2.3 8.8 HT1900.1-2455
288.6643 10.9328 4.7 31.8 22.0 -3.4395 -2.4 7.9 GRS 1915+105
262.9959 -33.9887 11.1 19.4 -159.6 1.2504 1.0 9.2 GX 354-0
293.2541 -8.0357 2.4 21.2 60.0 5.6758 4.7 ------ UNKNOWN
287.9754 30.9211 4.3 50.0 9.1 7.3032 2.7 ------ UNKNOWN
274.4828 35.2987 2.7 52.4 -6.1 10.5750 4.3 ------ UNKNOWN
261.4137 27.4138 3.3 46.1 -22.1 8.3901 3.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
912.300610 924.900640
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.6548 35.3380 8.4 34.0 -165.5 0.0904 1.4 9.7 Her X-1
288.8916 11.0275 276.3 36.2 122.9 0.0053 0.0 7.4 GRS 1915+105
299.6517 35.2498 1.9 11.3 100.2 0.3440 6.2 4.2 Cyg X-1
308.1774 41.0496 10.5 9.2 50.1 0.0549 1.1 6.6 Cyg X-3
326.1442 38.4101 3.6 22.3 28.9 0.1770 3.2 5.5 Cyg X-2
306.3945 18.0706 2.1 29.3 91.1 0.4760 5.5 ------ UNKNOWN
307.9558 75.1414 2.8 29.0 -66.7 0.2809 4.1 ------ UNKNOWN
Plot creation:
Sun Aug 1 14:00:43 EDT 2021