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
198.7003 5.0262 0.0137 27.3282 1.1866 2.6138861 14.061 TRIG_01285812
Foreground time interval of the image:
-62.544 74.301 (delta_t = 136.845 [sec])
Background time interval of the image:
-239.000 -62.544 (delta_t = 176.456 [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 -62.544 sec. to 302.624 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.13848 ( -0.0870656 0.0887688 )
Norm@50keV : 1.42137E-03 ( -7.34603e-05 7.27364e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.99 using 59 bins.
Reduced chi-squared = 0.982281
# Null hypothesis probability of 5.13e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 365.2 sec: 0.227981 ( -0.010137 0.010167 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.84328e-06 ( -2.23721e-07 2.2535e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -62.544 sec. to 302.624 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.98570 ( -0.375234 0.014793 )
Epeak [keV] : 4.03456 ( -1.75172 31.6958 )
Norm@50keV : 1.72848E-03 ( -0.000148797 0.00103778 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.25 using 59 bins.
Reduced chi-squared = 0.986607
# Null hypothesis probability of 5.03e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 365.2 sec: 0.227787 ( -0.010019 0.010428 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.7572e-06 ( -2.85009e-07 2.47988e-07 ) ergs/cm2
Band function
Time interval is from -62.544 sec. to 302.624 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] : 9.61500 ( )
R^2/D10^2 : 0.113172 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 176.60 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.68e-14 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.669e-07 5.934e-08
25- 50 1.802e-06 8.619e-08
50-150 8.384e-07 1.024e-07
15-150 3.407e-06 1.534e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 57.6360 (-7.23873 8.68922)
Norm : 1.17680 (-0.0968148 0.0955108)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.18 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.67e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.073e-06 7.359e-08
25- 50 1.612e-06 7.176e-08
50-150 1.774e-06 1.751e-07
15-150 4.459e-06 2.100e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.35679 (-0.655476 0.661803)
R1^2/D10^2 : 0.465425 (-0.143462 0.237691)
kT2 [keV] : 23.5717 (-3.98073 5.84609)
R2^2/D10^2 : 2.32817E-03 (-0.00128495 0.00247013)
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.55e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.072e-06 1.150e-07
25- 50 1.579e-06 1.691e-07
50-150 2.057e-06 5.602e-07
15-150 4.707e-06 8.033e-07
Peak spectrum fit
Power-law model
Time interval is from 184.120 sec. to 185.120 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.77816 ( -0.188559 0.196723 )
Norm@50keV : 9.78167E-03 ( -0.00132999 0.00130887 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.42 using 59 bins.
Reduced chi-squared = 0.849474
# Null hypothesis probability of 7.84e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.33672 ( -0.15652 0.15653 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.01467e-08 ( -1.24326e-08 1.26502e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 184.120 sec. to 185.120 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.414605 ( -1.24024 0.925078 )
Epeak [keV] : 48.9428 ( -8.82353 21.0138 )
Norm@50keV : 5.97234E-02 ( -0.0599955 0.262276 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.38 using 59 bins.
Reduced chi-squared = 0.738929
# Null hypothesis probability of 9.28e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.29350 ( -0.15868 0.15905 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.01512e-08 ( -1.30052e-08 1.39467e-08 ) ergs/cm2
Band function
Time interval is from 184.120 sec. to 185.120 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] : 10.9492 (-1.28657 1.48961)
R^2/D10^2 : 0.477489 (-0.181324 0.281608)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.33 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.16e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.195e-08 2.360e-09
25- 50 3.359e-08 4.970e-09
50-150 2.266e-08 6.045e-09
15-150 6.820e-08 9.590e-09
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 92.9279 (-29.3704 57.2869)
Norm : 6.12614 (-0.910551 1.08894)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.76 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.01e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.600e-08 2.870e-09
25- 50 2.725e-08 4.030e-09
50-150 4.230e-08 2.102e-08
15-150 8.555e-08 2.089e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.10692 (-3.26789 2.38923)
R1^2/D10^2 : 1.05757 (-0.558092 1.83828)
kT2 [keV] : 23.0101 (-9.88115 92.9464)
R2^2/D10^2 : 1.55977E-02 (-0.0154167 0.106203)
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.32e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.419e-08 6.796e-09
25- 50 3.085e-08 1.516e-08
50-150 3.835e-08 2.124e-08
15-150 8.338e-08 4.246e-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: 1.56911 ( -0.157855 0.159187 )
Norm@50keV : 1.20945E-03 ( -0.000111782 0.000111039 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.01e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 136.8 sec: 0.153969 ( -0.0140337 0.0140623 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.55346e-06 ( -1.54658e-07 1.55908e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.56699 ( -0.616435 0.902297 )
Epeak [keV] : 10000.00 ( -10000 -10000 )
Norm@50keV : 1.21260E-03 ( -0.00011242 0.000107405 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.04 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.65e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 136.8 sec: 0.153751 ( -0.014378 0.014194 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.55714e-06 ( -1.75131e-07 1.51752e-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) = 1.51e-06
S(50-100 keV) = 1.37e-06
T90 vs. Hardness ratio plot
T90 = 272.183999896049 sec.
Hardness ratio (energy fluence ratio) = 0.907285
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.990798
Count Ratio (50-100 keV) / (15-25 keV) = 0.449781
Mask shadow pattern
IMX = 5.166513247353672E-01, IMY = -1.070140368864476E-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:
-239.000000 -62.544000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
145.3641 38.9356 2.4 42.4 117.7 6.8603 4.7 ------ UNKNOWN
247.4973 33.4358 2.5 41.5 -102.1 5.3904 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-62.544000 74.300590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
198.7003 5.0262 0.8 27.3 1.2 2.6131 14.1 ------ UNKNOWN
249.2819 67.4893 2.1 46.0 -151.8 1.7769 5.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
146.500600 530.188100
531.000000 963.055100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
164.1195 32.5298 3.2 42.4 117.7 22.4674 3.7 ------ UNKNOWN
186.5460 -44.2251 3.8 50.4 -5.9 5.4272 3.0 ------ UNKNOWN
228.6390 -12.2125 2.7 34.4 -76.9 7.9010 4.2 ------ UNKNOWN
242.8632 12.9359 3.0 44.3 -120.5 17.2613 3.9 ------ UNKNOWN
Plot creation:
Fri Jun 20 01:52:58 EDT 2025