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
166.5733 -15.1259 0.0163 41.2124 39.3327 2.3632415 11.806 TRIG_01281241
Foreground time interval of the image:
-8.528 34.933 (delta_t = 43.461 [sec])
Background time interval of the image:
-189.467 -8.528 (delta_t = 180.939 [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 4.096000
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 4.096000
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 4.096000
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 -8.528 sec. to 305.988 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.77116 ( -0.113315 0.115775 )
Norm@50keV : 1.30632E-03 ( -9.84502e-05 9.77144e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.38 using 59 bins.
Reduced chi-squared = 1.16456
# Null hypothesis probability of 1.85e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 314.5 sec: 0.178043 ( -0.012347 0.012358 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.7873e-06 ( -2.91953e-07 2.94486e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -8.528 sec. to 305.988 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.319043 ( -0.653623 0.573746 )
Epeak [keV] : 52.5270 ( -5.57228 8.21992 )
Norm@50keV : 7.96688E-03 ( -0.00401468 0.00986437 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.18 using 59 bins.
Reduced chi-squared = 0.788929
# Null hypothesis probability of 8.73e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 314.5 sec: 0.168779 ( -0.012762 0.01279 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.41012e-06 ( -3.0277e-07 3.13885e-07 ) ergs/cm2
Band function
Time interval is from -8.528 sec. to 305.988 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] : 12.2971 (-0.870444 0.939061)
R^2/D10^2 : 4.09227E-02 (-0.00985597 0.0128689)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.15e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.123e-07 4.450e-08
25- 50 1.335e-06 1.054e-07
50-150 1.233e-06 1.898e-07
15-150 2.981e-06 2.271e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 99.4782 (-20.5614 30.5586)
Norm : 0.798601 (-0.0724187 0.0806636)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.65 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.39e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.565e-07 7.391e-08
25- 50 1.134e-06 9.105e-08
50-150 1.832e-06 5.991e-07
15-150 3.622e-06 6.542e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.29643 (-2.0628 2.38871)
R1^2/D10^2 : 0.216515 (-0.127321 0.411907)
kT2 [keV] : 16.5880 (-2.64804 5.28718)
R2^2/D10^2 : 1.03247E-02 (-0.00758952 0.0124347)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.55 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.67e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.664e-07 2.418e-07
25- 50 1.218e-06 4.798e-07
50-150 1.595e-06 7.476e-07
15-150 3.380e-06 1.447e-06
Peak spectrum fit
Power-law model
Time interval is from 1.732 sec. to 2.732 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.53949 ( -0.377608 0.372064 )
Norm@50keV : 1.18058E-02 ( -0.00305193 0.00304173 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.69 using 59 bins.
Reduced chi-squared = 0.924386
# Null hypothesis probability of 6.37e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.49026 ( -0.39314 0.39552 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.11309e-07 ( -2.99061e-08 3.02476e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.732 sec. to 2.732 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -5.49250 ( 4.10657 5.17539 )
Epeak [keV] : 39.1881 ( -7.33013 54.7433 )
Norm@50keV : 229.366 ( -249.112 185673 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.94 using 59 bins.
Reduced chi-squared = 0.856071
# Null hypothesis probability of 7.70e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.33675 ( -0.376799 0.46293 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.46793e-08 ( -2.19296e-08 4.99787e-08 ) ergs/cm2
Band function
Time interval is from 1.732 sec. to 2.732 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] : 11.9545 (-2.44516 3.68255)
R^2/D10^2 : 0.429770 (-0.276798 0.580064)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.69 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.75e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.299e-08 6.087e-09
25- 50 4.069e-08 1.767e-08
50-150 3.487e-08 1.759e-08
15-150 8.855e-08 3.608e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 169.507 (-100.254 -168.503)
Norm : 6.32331 (-1.65488 2.25744)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.33 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.87e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.605e-08 9.480e-09
25- 50 3.026e-08 1.745e-08
50-150 6.268e-08 3.813e-08
15-150 1.090e-07 6.505e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 39.2332 (-39.1553 -39.1553)
R1^2/D10^2 : 2.92035E-03 (-0.00299663 0.530562)
kT2 [keV] : 9.92821 (-9.92262 3.47653)
R2^2/D10^2 : 0.709714 (-0.710136 1.25822)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.97e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
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: 1.76714 ( -0.173182 0.178635 )
Norm@50keV : 3.95023E-03 ( -0.000465658 0.000460774 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.26 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.66e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 43.46 sec: 0.537556 ( -0.0590571 0.0591342 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.58267e-06 ( -1.90153e-07 1.92103e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.304876 ( -1.00681 0.831386 )
Epeak [keV] : 53.6830 ( -8.26826 15.2952 )
Norm@50keV : 2.39758E-02 ( -0.0152015 0.0580872 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.95e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 43.46 sec: 0.513943 ( -0.060296 0.060466 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.45141e-06 ( -1.92758e-07 2.00903e-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) = 1.05e-06
S(50-100 keV) = 1.24e-06
T90 vs. Hardness ratio plot
T90 = 293.999999880791 sec.
Hardness ratio (energy fluence ratio) = 1.18095
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.46818
Count Ratio (50-100 keV) / (15-25 keV) = 0.863215
Mask shadow pattern
IMX = 6.774258983073298E-01, IMY = -5.551123439441540E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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:
-189.467400 -8.528000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4433 35.4179 6.2 57.4 -159.0 -2.4346 -1.9 4.6 Her X-1
166.1463 -42.9965 2.4 56.0 7.3 5.5258 4.9 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-8.528000 34.932600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5430 35.2765 3.9 57.4 -158.8 1.0309 2.9 5.8 Her X-1
191.9232 48.4514 2.4 48.9 142.2 2.0594 4.8 ------ UNKNOWN
166.5732 -15.1259 1.0 41.2 39.3 2.3628 11.8 ------ UNKNOWN
244.8192 25.3320 1.9 45.5 -152.1 0.8793 6.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
116.132600 962.709500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5776 -40.3620 0.0 36.9 5.8 1.5227 1.0 11.8 Vela X-1
170.2409 -60.7026 4.0 45.6 -37.5 6.1252 2.9 5.3 Cen X-3
186.6679 -62.6449 8.4 49.6 -47.0 7.0017 1.4 7.5 GX 301-2
137.0892 -1.4602 3.5 32.1 77.4 7.0745 3.3 ------ UNKNOWN
114.4184 -36.8147 3.1 50.9 19.6 7.4171 3.8 ------ UNKNOWN
129.5385 -40.7049 3.1 41.0 9.1 5.9363 3.7 ------ UNKNOWN
155.3058 -22.1439 2.2 12.8 20.0 4.6124 5.2 ------ UNKNOWN
195.3554 -38.4875 3.3 34.4 -76.8 6.2926 3.5 ------ UNKNOWN
Plot creation:
Fri Jun 20 01:54:44 EDT 2025