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
299.6791 +35.3186 0.0481 23.2 167.7 -0.0860 -4.0 TRIG_01185685
------------------------------------------
Foreground time interval of the image:
26.176 28.390 (delta_t = 2.214 [sec])
29.000 30.784 (delta_t = 1.784 [sec])
Background time interval of the image:
-58.000 -57.506 (delta_t = 0.494 [sec])
-55.000 -53.920 (delta_t = 1.080 [sec])
-51.000 -50.669 (delta_t = 0.331 [sec])
-49.000 -48.440 (delta_t = 0.560 [sec])
-46.000 -44.870 (delta_t = 1.130 [sec])
-40.000 -37.190 (delta_t = 2.810 [sec])
-36.000 -35.960 (delta_t = 0.040 [sec])
-13.000 26.176 (delta_t = 39.176 [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
26.176000 28.390000
29.000000 30.784000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.07548 ( -0.489803 0.592827 )
Norm@50keV : 1.37548E-03 ( -0.000558577 0.000542507 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.59 using 59 PHA bins.
# Reduced chi-squared = 1.045 for 57 degrees of freedom
# Null hypothesis probability = 3.815792e-01
Photon flux (15-150 keV) in 3.998 sec: 0.213813 ( -0.0634292 0.0634937 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.09661e-08 ( -1.8184e-08 1.96197e-08 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
26.176000 28.390000
29.000000 30.784000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.143574 ( -6.65547 2.33036 )
Epeak [keV] : 36.8023 ( -36.7085 -36.7085 )
Norm@50keV : 3.11362E-02 ( -0.0420533 431.259 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.26 using 59 PHA bins.
# Reduced chi-squared = 1.023 for 56 degrees of freedom
# Null hypothesis probability = 4.279764e-01
Photon flux (15-150 keV) in 3.998 sec: 0.205241 ( -0.062518 0.063792 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.33127e-08 ( -1.5115e-08 2.04402e-08 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
26.176000 28.390000
29.000000 30.784000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.420488 ( -2.99495 -0.569019 )
beta : -10.0000 ( 10 20 )
Epeak [keV] : 36.6161 ( -11.8044 292.159 )
Norm@50keV : 4.63800E-02 ( -0.0463795 15.7451 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.25 using 59 PHA bins.
# Reduced chi-squared = 1.041 for 55 degrees of freedom
# Null hypothesis probability = 3.915765e-01
Photon flux (15-150 keV) in 3.998 sec: 0.209455 ( 6.79054 -0.0962 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.41763e-08 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 9.27077 (-2.33146 3.13713)
R^2/D10^2 : 0.144278 (-0.144278 0.290599)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.42 using 59 PHA bins.
# Reduced chi-squared = 1.007 for 57 degrees of freedom
# Null hypothesis probability = 4.595330e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.794e-09 6.017e-09
25- 50 2.179e-08 1.288e-08
50-150 9.095e-09 6.825e-09
15-150 4.068e-08 2.505e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 53.0162 (-27.0137 91.0241)
Norm : 1.21045 (-0.458572 0.781651)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.198e-08 6.226e-09
25- 50 1.757e-08 1.068e-08
50-150 1.800e-08 1.379e-08
15-150 4.756e-08 2.641e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.20288 (-3.14714 145.247)
R1^2/D10^2 : 2.11064 (-2.54095 -2.54095)
kT2 [keV] : 9.99271 (-4.18893 -9.9844)
R2^2/D10^2 : 0.100961 (-0.101817 0.309371)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.055e-08 5.593e-09
25- 50 2.081e-08 1.335e-08
50-150 1.062e-08 7.706e-09
15-150 4.198e-08 2.455e-08
Peak spectrum fit
Power-law model
Time interval is from 26.908 sec. to 27.908 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.17049 ( -0.571114 0.695083 )
Norm@50keV : 2.42526E-03 ( -0.00120277 0.00121994 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.78 using 59 PHA bins.
# Reduced chi-squared = 1.189 for 57 degrees of freedom
# Null hypothesis probability = 1.553851e-01
Photon flux (15-150 keV) in 1 sec: 0.395135 ( -0.14381 0.144894 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.26604e-08 ( -9.69149e-09 1.08386e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 26.908 sec. to 27.908 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -4.38178 ( 5.46998 6.12926 )
Epeak [keV] : 31.9150 ( -6.40656 7.67063 )
Norm@50keV : 50.4260 ( -44.5963 421482 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.67 using 59 PHA bins.
# Reduced chi-squared = 1.101 for 56 degrees of freedom
# Null hypothesis probability = 2.804267e-01
Photon flux (15-150 keV) in 1 sec: 0.392315 ( -0.133302 0.13524 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.84943e-08 ( -6.5021e-09 7.4065e-09 ) ergs/cm2
Band function
Time interval is from 26.908 sec. to 27.908 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.29837 ( -4.87657 -4.29837 )
beta : -9.35306 ( 9.35316 19.3173 )
Epeak [keV] : 31.9913 ( -6.9378 7.52331 )
Norm@50keV : 43.8889 ( -43.8889 257.698 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.67 using 59 PHA bins.
# Reduced chi-squared = 1.121 for 55 degrees of freedom
# Null hypothesis probability = 2.497818e-01
Photon flux (15-150 keV) in 1 sec: 0.331509 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.85504e-08 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 8.24043 (-2.00811 2.63303)
R^2/D10^2 : 0.459383 (-0.459386 0.903864)
(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 5.761e-09 3.589e-09
25- 50 1.061e-08 6.720e-09
50-150 3.068e-09 2.588e-09
15-150 1.944e-08 1.221e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 39.6668 (-20.225 66.0579)
Norm : 2.70923 (-1.22498 2.17621)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.204e-09 3.781e-09
25- 50 8.132e-09 4.970e-09
50-150 6.234e-09 5.350e-09
15-150 2.057e-08 1.360e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.21858 (-8.2294 -8.2294)
R1^2/D10^2 : 0.146335 (-0.146194 -0.146194)
kT2 [keV] : 8.24911 (-8.24216 -8.24216)
R2^2/D10^2 : 0.313305 (-0.31317 -0.31317)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.762e-09 1.381e-01
25- 50 1.061e-08 1.315e+00
50-150 3.067e-09 2.893e+01
15-150 1.944e-08 3.517e+01
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: 2.07548 ( -0.489803 0.592827 )
Norm@50keV : 1.37548E-03 ( -0.000558577 0.000542507 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.59 using 59 PHA bins.
# Reduced chi-squared = 1.045 for 57 degrees of freedom
# Null hypothesis probability = 3.815792e-01
Photon flux (15-150 keV) in 3.998 sec: 0.213813 ( -0.0634292 0.0634937 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.09661e-08 ( -1.8184e-08 1.96197e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.143574 ( -6.65547 2.33036 )
Epeak [keV] : 36.8023 ( -36.7085 -36.7085 )
Norm@50keV : 3.11362E-02 ( -0.0420533 431.259 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.26 using 59 PHA bins.
# Reduced chi-squared = 1.023 for 56 degrees of freedom
# Null hypothesis probability = 4.279764e-01
Photon flux (15-150 keV) in 3.998 sec: 0.205241 ( -0.062518 0.063792 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.33127e-08 ( -1.5115e-08 2.04402e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.420488 ( -2.99495 -0.569019 )
beta : -10.0000 ( 10 8.88178e-15 )
Epeak [keV] : 36.6161 ( -11.8044 292.62 )
Norm@50keV : 4.63800E-02 ( -0.0463795 15.7451 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.25 using 59 PHA bins.
# Reduced chi-squared = 1.041 for 55 degrees of freedom
# Null hypothesis probability = 3.915765e-01
Photon flux (15-150 keV) in 3.998 sec: 0.209455 ( 6.79054 -0.0962 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.41763e-08 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.57e-08
S(50-100 keV) = 1.49e-08
T90 vs. Hardness ratio plot
T90 = 4.05199992656708 sec.
Hardness ratio (energy fluence ratio) = 0.949045
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.38118
Count Ratio (50-100 keV) / (15-25 keV) = 0.326766
Mask shadow pattern
IMX = -4.180211711067969E-01, IMY = -9.098411408893728E-02
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:
-58.000000 -57.505900
-55.000000 -53.920000
-51.000000 -50.668600
-49.000000 -48.440000
-46.000000 -44.870000
-40.000000 -37.190000
-36.000000 -35.960000
-13.000000 26.176000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4578 35.3420 83.5 57.8 -172.7 0.0626 0.1 0.0 Her X-1
288.8392 10.8119 8.9 44.6 138.4 -0.3805 -1.3 8.4 GRS 1915+105
299.7378 35.3075 0.6 23.1 167.7 1.8288 19.6 9.6 Cyg X-1
308.3157 41.0921 0.0 15.9 -176.8 0.3991 4.1 12.5 Cyg X-3
326.3138 38.3756 8.7 1.8 -177.1 0.1164 1.3 7.4 Cyg X-2
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
26.176000 28.390000
29.000000 30.784000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4512 35.2735 7.5 57.9 -172.8 -0.1792 -1.6 4.1 Her X-1
288.6795 10.8550 5.4 44.6 138.6 0.1439 2.1 8.9 GRS 1915+105
299.6791 35.3187 2.9 23.2 167.7 -0.0860 -4.0 8.3 Cyg X-1
307.9088 40.8868 4.7 16.1 -177.6 0.0474 2.4 10.0 Cyg X-3
326.2142 38.4204 9.6 1.9 -176.5 0.0228 1.2 6.3 Cyg X-2
346.6509 3.2213 2.1 38.4 45.1 0.2278 5.6 ------ UNKNOWN
337.8353 32.7102 2.3 9.2 16.3 0.0893 5.0 ------ UNKNOWN
37.8018 36.0383 2.3 54.1 -35.8 0.5649 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
148.200600 243.084500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.6612 35.3838 20.3 36.5 -134.6 -0.1453 -0.6 10.3 Her X-1
268.2780 -1.4923 3.4 47.1 167.3 -1.3682 -3.4 5.9 SW J1753.5-0127
288.6567 10.8858 6.7 26.5 147.0 -0.3070 -1.7 9.1 GRS 1915+105
299.7231 35.3112 0.5 0.1 179.2 3.6619 22.4 9.2 Cyg X-1
307.8439 41.0178 0.0 8.5 -12.4 -0.2924 -1.9 12.7 Cyg X-3
326.0540 38.4405 16.1 21.2 15.6 0.1117 0.7 9.0 Cyg X-2
354.9958 32.9809 4.1 45.1 18.2 0.8630 2.8 ------ UNKNOWN
256.6549 5.6996 2.5 49.5 -174.7 1.6434 4.7 ------ UNKNOWN
13.7927 57.3159 2.3 52.5 -17.3 2.2256 4.9 ------ UNKNOWN
242.2120 10.8032 3.3 57.4 -158.5 2.4638 3.5 ------ UNKNOWN
239.7485 35.8568 2.8 48.0 -129.0 2.9377 4.1 ------ UNKNOWN
Plot creation:
Thu Aug 17 18:55:41 EDT 2023