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
187.3163 47.8420 0.0039 26.3519 -72.7287 5.1570967 49.512 TRIG_01351008
Foreground time interval of the image:
-5.720 14.557 (delta_t = 20.277 [sec])
Background time interval of the image:
-239.944 -5.720 (delta_t = 234.224 [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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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 1.024000
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 1.024000
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 -5.720 sec. to 961.768 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.54908 ( -0.107787 0.108443 )
Norm@50keV : 1.02675E-03 ( -6.30137e-05 6.28013e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.19 using 59 bins.
Reduced chi-squared = 0.722632
# Null hypothesis probability of 9.43e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 967.5 sec: 0.129949 ( -0.00801 0.008024 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.35429e-06 ( -6.21343e-07 6.25487e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -5.720 sec. to 961.768 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.29085 ( -0.442835 0.31096 )
Epeak [keV] : 137.835 ( -58.1233 -137.835 )
Norm@50keV : 1.38402E-03 ( -0.000402002 0.00089454 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.02 using 59 bins.
Reduced chi-squared = 0.714643
# Null hypothesis probability of 9.47e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 967.5 sec: 0.128162 ( -0.00848 0.00848 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.16138e-06 ( -6.93381e-07 6.92354e-07 ) ergs/cm2
Band function
Time interval is from -5.720 sec. to 961.768 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] : 14.7615 (-1.14501 1.26878)
R^2/D10^2 : 1.51115E-02 (-0.00382789 0.00505314)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 103.42 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.66e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.687e-07 8.108e-08
25- 50 2.617e-06 2.182e-07
50-150 3.854e-06 4.784e-07
15-150 7.140e-06 5.278e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.343 (-50.6672 -199.352)
Norm : 0.528163 (-0.0313714 0.0314194)
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.11 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.56e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.272e-06 8.175e-08
25- 50 2.448e-06 2.012e-07
50-150 5.368e-06 1.071e-06
15-150 9.088e-06 1.400e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.86020 (-1.36278 1.51663)
R1^2/D10^2 : 0.143593 (-0.0688873 0.17088)
kT2 [keV] : 25.4472 (-4.36334 7.36319)
R2^2/D10^2 : 1.76950E-03 (-0.00105195 0.0018189)
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.22e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.219e-06 3.214e-07
25- 50 2.446e-06 4.799e-07
50-150 5.438e-06 1.569e-06
15-150 9.102e-06 2.298e-06
Peak spectrum fit
Power-law model
Time interval is from 0.284 sec. to 1.284 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.20757 ( -0.101515 0.101353 )
Norm@50keV : 4.23208E-02 ( -0.00259732 0.00259685 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.11 using 59 bins.
Reduced chi-squared = 0.808947
# Null hypothesis probability of 8.48e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.97299 ( -0.30995 0.3101 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.28499e-07 ( -2.94282e-08 2.95585e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.284 sec. to 1.284 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.769594 ( -0.439259 0.399605 )
Epeak [keV] : 151.173 ( -50.6655 736.403 )
Norm@50keV : 6.87473E-02 ( -0.0240674 0.0413464 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.58 using 59 bins.
Reduced chi-squared = 0.760357
# Null hypothesis probability of 9.07e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.91226 ( -0.31534 0.31521 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.19498e-07 ( -3.12046e-08 3.10593e-08 ) ergs/cm2
Band function
Time interval is from 0.284 sec. to 1.284 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] : 18.3521 (-1.43065 1.57814)
R^2/D10^2 : 0.311076 (-0.0741526 0.0957244)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 88.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.09e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.084e-08 2.545e-09
25- 50 9.779e-08 8.495e-09
50-150 2.402e-07 2.785e-08
15-150 3.589e-07 2.775e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-11.6787 -200)
Norm : 20.3655 (-1.27267 1.27267)
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.65 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.81e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.069e-08 3.435e-09
25- 50 9.752e-08 7.605e-09
50-150 2.139e-07 4.690e-08
15-150 3.621e-07 6.160e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.18189 (-1.94077 2.47036)
R1^2/D10^2 : 2.42381 (-1.23747 3.14493)
kT2 [keV] : 30.1085 (-5.67025 12.9788)
R2^2/D10^2 : 4.87734E-02 (-0.0338473 0.0540119)
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.97e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.672e-08 1.028e-08
25- 50 9.688e-08 2.216e-08
50-150 2.880e-07 1.030e-07
15-150 4.216e-07 1.180e-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: 1.27444 ( -0.0538892 0.0536899 )
Norm@50keV : 1.68053E-02 ( -0.000491644 0.000491436 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.17 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.96e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 20.28 sec: 1.99579 ( -0.0627875 0.0629146 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.38934e-06 ( -1.054e-07 1.05556e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.13953 ( -0.209912 0.165876 )
Epeak [keV] : 362.445 ( -362.446 -362.446 )
Norm@50keV : 1.93140E-02 ( -0.00294272 0.0045089 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.06e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 20.28 sec: 1.97962 ( -0.06684 0.06697 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.36654e-06 ( -1.12169e-07 1.11723e-07 ) 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) = 2.37e-06
S(50-100 keV) = 3.24e-06
T90 vs. Hardness ratio plot
T90 = 516.287999987602 sec.
Hardness ratio (energy fluence ratio) = 1.36709
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.34239
Count Ratio (50-100 keV) / (15-25 keV) = 0.960188
Mask shadow pattern
IMX = 1.470699747682539E-01, IMY = 4.730218127861702E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-239.944000 -5.720000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3183 35.2698 12.9 33.3 171.2 0.3789 0.9 8.1 Her X-1
200.6217 42.9817 2.8 25.4 -96.9 1.5820 4.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-5.720000 14.556640
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4911 35.4626 22.7 33.1 170.8 -0.0459 -0.5 7.4 Her X-1
221.6584 87.7266 2.9 24.0 35.4 0.3089 4.0 ------ UNKNOWN
187.3163 47.8420 0.2 26.4 -72.7 5.1572 49.5 ------ UNKNOWN
215.4768 29.6246 2.0 34.8 -127.8 0.6784 5.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
78.356590 452.056600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3383 35.3690 12.0 50.0 155.8 -1.4238 -1.0 6.1 Her X-1
187.2721 47.8203 1.0 0.0 -20.7 5.4244 11.1 ------ UNKNOWN
152.8764 28.2279 2.7 33.0 -36.6 2.5323 4.2 ------ UNKNOWN
Plot creation:
Sun Mar 1 23:24:37 EST 2026