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
212.9415 16.7405 0.0065 26.6669 -148.5435 2.8690472 29.775 TRIG_01329888
Foreground time interval of the image:
-29.128 13.133 (delta_t = 42.261 [sec])
Background time interval of the image:
-179.267 -29.128 (delta_t = 150.139 [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 -29.128 sec. to 76.548 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.46882 ( -0.0607689 0.0607105 )
Norm@50keV : 4.74032E-03 ( -0.000144384 0.000144368 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.39 using 59 bins.
Reduced chi-squared = 0.954211
# Null hypothesis probability of 5.74e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 105.7 sec: 0.586968 ( -0.019679 0.019809 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.77909e-06 ( -1.5597e-07 1.56228e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -29.128 sec. to 76.548 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.46607 ( -0.0653829 0.0571548 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 4.75517E-03 ( -0.00014501 0.00014472 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.49 using 59 bins.
Reduced chi-squared = 0.973036
# Null hypothesis probability of 5.32e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 105.7 sec: 0.586852 ( -0.019713 0.019784 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.80845e-06 ( -1.86504e-07 1.25615e-07 ) ergs/cm2
Band function
Time interval is from -29.128 sec. to 76.548 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] : 16.8267 ( )
R^2/D10^2 : 4.24081E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 363.30 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.57e-46 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.592e-07 1.786e-08
25- 50 1.137e-06 4.862e-08
50-150 2.292e-06 1.327e-07
15-150 3.688e-06 1.406e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-8.76736 -200)
Norm : 2.41080 (-0.073674 0.073674)
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.20 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.27e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.347e-07 2.209e-08
25- 50 1.221e-06 4.017e-08
50-150 2.678e-06 8.826e-08
15-150 4.533e-06 1.480e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.80801 (-0.729888 0.772837)
R1^2/D10^2 : 0.447652 (-0.123453 0.18533)
kT2 [keV] : 36.1282 (-4.70611 6.78513)
R2^2/D10^2 : 2.73689E-03 (-0.0010914 0.00152311)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.71e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.643e-07 5.491e-08
25- 50 1.205e-06 8.879e-08
50-150 3.105e-06 3.404e-07
15-150 4.874e-06 3.589e-07
Peak spectrum fit
Power-law model
Time interval is from 37.364 sec. to 38.364 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.13744 ( -0.0896675 0.0893529 )
Norm@50keV : 4.23887E-02 ( -0.00211581 0.0021158 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.54 using 59 bins.
Reduced chi-squared = 0.834035
# Null hypothesis probability of 8.10e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.93619 ( -0.251 0.25115 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.38077e-07 ( -2.49249e-08 2.50499e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 37.364 sec. to 38.364 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.04011 ( -0.351778 0.140308 )
Epeak [keV] : 542.129 ( -542.14 -542.14 )
Norm@50keV : 4.70730E-02 ( -0.006367 0.0209057 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.29 using 59 bins.
Reduced chi-squared = 0.844464
# Null hypothesis probability of 7.90e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.93527 ( -0.25331 0.20166 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.35512e-07 ( -2.66187e-08 2.63157e-08 ) ergs/cm2
Band function
Time interval is from 37.364 sec. to 38.364 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] : 19.5059 ( )
R^2/D10^2 : 0.248947 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 128.17 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.14e-07 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.844e-08 1.905e-09
25- 50 9.031e-08 6.100e-09
50-150 2.538e-07 2.135e-08
15-150 3.625e-07 2.200e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-7.76392 -200)
Norm : 20.0676 (-1.02923 1.02923)
------------------------------------------------------------
#Fit statistic : Chi-Squared 104.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.23e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.996e-08 2.745e-09
25- 50 9.610e-08 6.805e-09
50-150 2.108e-07 4.065e-08
15-150 3.568e-07 1.990e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.59812 (-1.65169 1.85295)
R1^2/D10^2 : 2.10605 (-0.895625 1.94466)
kT2 [keV] : 36.2370 (-7.0234 14.0513)
R2^2/D10^2 : 2.88764E-02 (-0.0176726 0.0290505)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.69 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.13e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.479e-08 7.040e-09
25- 50 9.308e-08 1.731e-08
50-150 3.111e-07 8.040e-08
15-150 4.390e-07 1.092e-07
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: 1.55401 ( -0.0908868 0.0911321 )
Norm@50keV : 4.71657E-03 ( -0.000231648 0.000230652 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.58 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.15e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 42.26 sec: 0.597784 ( -0.0299852 0.030103 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.87538e-06 ( -9.96499e-08 1.00112e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.54933 ( -0.118693 0.0923712 )
Epeak [keV] : 9999.28 ( -9999.36 -9999.36 )
Norm@50keV : 4.72765E-03 ( -0.000225842 0.00116323 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.82e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 42.26 sec: 0.597563 ( -0.030015 0.030025 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.87353e-06 ( -9.74389e-08 9.92899e-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) = 1.16e-06
S(50-100 keV) = 1.68e-06
T90 vs. Hardness ratio plot
T90 = 63.9160000085831 sec.
Hardness ratio (energy fluence ratio) = 1.44828
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.31916
Count Ratio (50-100 keV) / (15-25 keV) = 0.995901
Mask shadow pattern
IMX = -4.284147928941399E-01, IMY = 2.620859655052169E-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:
-179.267370 -29.128000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9675 -15.6568 2.0 41.9 128.8 4.7020 5.7 1.2 Sco X-1
254.5378 35.2546 20.0 15.7 6.1 0.1279 0.6 6.6 Her X-1
268.4631 -1.3841 6.0 38.8 86.5 -1.7863 -1.9 7.0 SW J1753.5-0127
299.5911 35.1640 1.4 51.5 20.6 6.4998 8.1 2.3 Cyg X-1
234.3407 -13.1807 2.0 39.5 144.7 2.9489 5.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-29.128000 13.132600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.1535 -15.6035 14.3 41.8 128.6 0.2217 0.8 10.3 Sco X-1
254.6159 35.4210 11.7 15.8 5.7 -0.0791 -1.0 9.1 Her X-1
268.3219 -1.5113 3.6 38.8 86.8 -1.0685 -3.2 4.5 SW J1753.5-0127
299.4729 35.1154 5.5 51.4 20.7 -0.8188 -2.1 7.7 Cyg X-1
292.9321 46.4482 2.5 46.4 5.6 0.8217 4.7 ------ UNKNOWN
212.9415 16.7405 0.4 26.7 -148.5 2.8691 29.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
76.132600 514.232610
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4746 35.4036 9.6 41.3 26.7 1.0895 1.2 3.8 Her X-1
230.0134 -17.4646 2.4 38.1 124.7 6.6439 4.8 ------ UNKNOWN
214.9133 4.2610 3.0 12.6 142.7 2.0586 3.9 ------ UNKNOWN
179.0573 -19.2865 2.8 49.0 -164.1 5.9674 4.1 ------ UNKNOWN
176.7952 -15.0649 2.8 47.8 -158.0 5.4543 4.2 ------ UNKNOWN
167.5853 9.1624 2.8 44.7 -122.1 10.3368 4.2 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:36:42 EST 2026