Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
71.3767 43.7942 0.0243 39.8255 -179.7953 0.2923851 7.881 TRIG_01299965
Foreground time interval of the image:
-0.720 3.760 (delta_t = 4.480 [sec])
Background time interval of the image:
-183.315 -0.720 (delta_t = 182.595 [sec])
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
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)
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 -0.720 sec. to 3.760 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.60915 ( -0.353509 0.415502 )
Norm@50keV : 3.17530E-03 ( -0.000969468 0.000975246 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.42 using 59 bins.
Reduced chi-squared = 0.779298
# Null hypothesis probability of 8.88e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 4.48 sec: 0.668039 ( -0.114945 0.114992 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.46879e-07 ( -3.14036e-08 3.31279e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.720 sec. to 3.760 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.61494 ( )
Epeak [keV] : 12.8743 ( )
Norm@50keV : 1.44743E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.17 using 59 bins.
Reduced chi-squared = 0.770893
# Null hypothesis probability of 8.95e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 4.48 sec: 0.666490 ( -0.112589 0.117745 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.34499e-07 ( -3.20495e-08 3.63763e-08 ) ergs/cm2
Band function
Time interval is from -0.720 sec. to 3.760 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] : 6.22453 (-1.11082 1.38565)
R^2/D10^2 : 2.08059 (-1.19848 2.83902)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.48 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.39e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.049e-08 1.908e-08
25- 50 5.449e-08 1.877e-08
50-150 5.787e-09 3.873e-09
15-150 1.108e-07 3.257e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 27.0817 (-9.13894 15.1765)
Norm : 5.91831 (-1.941 3.31976)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.20 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.12e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.101e-08 1.245e-08
25- 50 5.496e-08 1.602e-08
50-150 2.620e-08 1.542e-08
15-150 1.322e-07 3.494e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.88835 (-1.8141 1.60147)
R1^2/D10^2 : 4.84393 (-2.42667 23.633)
kT2 [keV] : 15.4353 (-12.3291 27.7107)
R2^2/D10^2 : 2.31680E-02 (-0.0230458 0.63437)
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.95 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.02e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.333e-08 2.986e-08
25- 50 5.075e-08 2.746e-08
50-150 3.556e-08 2.094e-08
15-150 1.396e-07 7.137e-08
Peak spectrum fit
Power-law model
Time interval is from 1.284 sec. to 2.284 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.96908 ( -0.498715 0.579815 )
Norm@50keV : 5.81603E-03 ( -0.00207318 0.00191302 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.50 using 59 bins.
Reduced chi-squared = 1.07895
# Null hypothesis probability of 3.18e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.860292 ( -0.24373 0.243978 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.35673e-08 ( -1.73088e-08 1.77049e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.284 sec. to 2.284 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.08929 ( -1.64752 2.03344 )
Epeak [keV] : 42.4012 ( )
Norm@50keV : 4.97598E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.42 using 59 bins.
Reduced chi-squared = 1.09679
# Null hypothesis probability of 2.88e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.801311 ( -0.403496 0.302499 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.51045e-08 ( -2.8004e-08 2.37417e-08 ) ergs/cm2
Band function
Time interval is from 1.284 sec. to 2.284 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] : 7.72932 (-2.27475 4.32723)
R^2/D10^2 : 1.05224 (-1.0503 3.3334)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.18 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.90e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.107e-08 6.625e-09
25- 50 1.823e-08 1.158e-08
50-150 4.269e-09 3.345e-09
15-150 3.357e-08 2.137e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 77.8929 (-48.4523 -77.954)
Norm : 4.04294 (-1.49248 3.04516)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.37 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.91e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.047e-08 5.264e-09
25- 50 1.713e-08 1.034e-08
50-150 2.374e-08 1.877e-08
15-150 5.134e-08 3.129e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.38594 (-2.16961 2.82973)
R1^2/D10^2 : 2.03595 (-1.59043 8.8107)
kT2 [keV] : 45.5596 (-33.6823 -45.5593)
R2^2/D10^2 : 1.35136E-03 (-0.0012921 0.024682)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.07e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.233e-08 7.320e-09
25- 50 1.599e-08 1.012e-08
50-150 2.742e-08 1.441e-08
15-150 5.574e-08 2.781e-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: 2.60915 ( -0.353509 0.415502 )
Norm@50keV : 3.17530E-03 ( -0.000969468 0.000975246 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.42 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.88e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 4.48 sec: 0.667933 ( -0.11493 0.114978 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.46841e-07 ( -3.14004e-08 3.31574e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.61050 ( )
Epeak [keV] : 12.9614 ( )
Norm@50keV : 1.45747E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.17 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.95e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 4.48 sec: 0.656232 ( -0.113506 0.115794 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.34507e-07 ( -1.70948e-08 3.74963e-08 ) 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) = 4.93e-08
S(50-100 keV) = 3.22e-08
T90 vs. Hardness ratio plot
T90 = 3.95200002193451 sec.
Hardness ratio (energy fluence ratio) = 0.653144
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.634373
Count Ratio (50-100 keV) / (15-25 keV) = 0.208208
Mask shadow pattern
IMX = -8.339169314008682E-01, IMY = 2.979968450133867E-03
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:
-183.315410 -0.720000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5805 35.2167 1.9 51.1 17.4 4.5650 6.0 1.0 Cyg X-1
308.1137 40.9585 177.1 42.3 16.7 -0.0294 -0.1 0.4 Cyg X-3
325.9223 38.3104 0.0 34.0 -1.7 0.6587 1.9 11.8 Cyg X-2
100.2066 57.5710 2.4 45.9 147.9 3.9133 4.7 ------ UNKNOWN
90.5631 46.1408 1.9 48.7 165.1 4.7660 6.2 ------ UNKNOWN
4.2315 32.5046 3.4 23.3 -67.3 1.1076 3.4 ------ UNKNOWN
321.0747 12.2429 3.7 57.5 -19.0 3.3540 3.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.720000 3.760000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5573 35.1615 12.3 51.2 17.4 0.0897 0.9 2.9 Cyg X-1
308.2706 41.0468 4.9 42.2 16.6 0.1023 2.3 9.2 Cyg X-3
326.0170 38.3791 8.9 33.9 -1.7 0.0394 1.3 8.1 Cyg X-2
71.3767 43.7942 1.5 39.8 -179.8 0.2924 7.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
296.084610 842.255200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6419 22.0194 0.5 24.0 168.7 21.1353 24.1 0.6 Crab
337.8724 76.4143 2.6 48.5 -0.6 5.8096 4.3 ------ UNKNOWN
56.7897 -8.9968 2.9 54.4 -144.5 16.4853 4.0 ------ UNKNOWN
Plot creation:
Fri Jun 20 01:44:19 EDT 2025