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
83.0496 66.1249 0.0032 15.6548 46.2238 4.7220723 60.462 TRIG_01187463
Foreground time interval of the image:
-6.312 13.325 (delta_t = 19.637 [sec])
Background time interval of the image:
-239.976 -6.312 (delta_t = 233.664 [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 -6.312 sec. to 47.480 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.52049 ( -0.0522357 0.0522866 )
Norm@50keV : 7.33766E-03 ( -0.000203507 0.000203461 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.78 using 59 bins.
Reduced chi-squared = 1.04877
# Null hypothesis probability of 3.75e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 53.79 sec: 0.921191 ( -0.027714 0.027787 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.73251e-06 ( -1.10239e-07 1.10495e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -6.312 sec. to 47.480 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.21479 ( -0.217435 0.207147 )
Epeak [keV] : 136.965 ( -35.7123 161.221 )
Norm@50keV : 1.02161E-02 ( -0.00200262 0.0026341 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.30 using 59 bins.
Reduced chi-squared = 0.951786
# Null hypothesis probability of 5.78e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 53.79 sec: 0.901297 ( -0.030498 0.030588 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.64848e-06 ( -1.24352e-07 1.23954e-07 ) ergs/cm2
Band function
Time interval is from -6.312 sec. to 47.480 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] : 16.0986 ( )
R^2/D10^2 : 7.85576E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 296.58 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.31e-34 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.261e-07 1.302e-08
25- 50 9.565e-07 3.523e-08
50-150 1.737e-06 9.117e-08
15-150 2.919e-06 1.006e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-13.3352 -200)
Norm : 3.75872 (-0.103772 0.103772)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.96e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.035e-07 1.546e-08
25- 50 9.686e-07 3.254e-08
50-150 2.124e-06 6.993e-08
15-150 3.596e-06 1.148e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.28039 (-0.753591 0.827986)
R1^2/D10^2 : 0.793107 (-0.23783 0.368043)
kT2 [keV] : 26.5187 (-2.46518 3.29295)
R2^2/D10^2 : 1.09705E-02 (-0.00380756 0.00482484)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.70 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.25e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.475e-07 4.629e-08
25- 50 9.652e-07 6.105e-08
50-150 2.210e-06 1.901e-07
15-150 3.622e-06 2.308e-07
Peak spectrum fit
Power-law model
Time interval is from 2.436 sec. to 3.436 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.22983 ( -0.108258 0.107993 )
Norm@50keV : 2.53140E-02 ( -0.00170553 0.00170429 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.00 using 59 bins.
Reduced chi-squared = 1
# Null hypothesis probability of 4.75e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.98445 ( -0.20147 0.20154 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.54736e-07 ( -1.9372e-08 1.95161e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.436 sec. to 3.436 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.234942 ( -0.589257 0.510534 )
Epeak [keV] : 88.5089 ( -16.9041 42.1998 )
Norm@50keV : 8.10734E-02 ( -0.0359158 0.0786656 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.59 using 59 bins.
Reduced chi-squared = 0.79625
# Null hypothesis probability of 8.64e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.89044 ( -0.20886 0.20786 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.35879e-07 ( -2.21025e-08 2.21093e-08 ) ergs/cm2
Band function
Time interval is from 2.436 sec. to 3.436 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] : 16.2363 (-1.24986 1.39536)
R^2/D10^2 : 0.282080 (-0.068709 0.0879263)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.88e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.532e-08 1.990e-09
25- 50 6.529e-08 5.760e-09
50-150 1.210e-07 1.580e-08
15-150 2.016e-07 1.755e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-15.4499 -200)
Norm : 12.1863 (-0.826212 0.826212)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.98e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.034e-08 2.395e-09
25- 50 5.836e-08 6.130e-09
50-150 1.280e-07 3.986e-08
15-150 2.167e-07 4.095e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 11.8693 (-2.41749 2.10465)
R1^2/D10^2 : 0.615815 (-0.213702 0.350691)
kT2 [keV] : 50.4981 (-25.3232 -53.1508)
R2^2/D10^2 : 4.44266E-03 (-0.00336626 0.0271424)
------------------------------------------------------------
#Fit statistic : Chi-Squared 38.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.53e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.956e-08 3.825e-09
25- 50 6.584e-08 1.632e-08
50-150 1.576e-07 7.094e-08
15-150 2.430e-07 8.933e-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: 1.31642 ( -0.0449976 0.044911 )
Norm@50keV : 1.53390E-02 ( -0.000389125 0.000389099 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 93.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.81e-03 with 57 degrees of freedom
Photon flux (15-150 keV) in 19.64 sec: 1.83564 ( -0.0498394 0.0499216 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.96523e-06 ( -8.01336e-08 8.02488e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.653034 ( -0.208899 0.199403 )
Epeak [keV] : 112.786 ( -14.4901 24.7679 )
Norm@50keV : 3.07177E-02 ( -0.00564647 0.00727459 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.41 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.23e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 19.64 sec: 1.76691 ( -0.05314 0.05326 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.8566e-06 ( -8.78104e-08 8.73784e-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) = 9.31e-07
S(50-100 keV) = 1.30e-06
T90 vs. Hardness ratio plot
T90 = 40.8399999141693 sec.
Hardness ratio (energy fluence ratio) = 1.39635
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.41243
Count Ratio (50-100 keV) / (15-25 keV) = 1.019
Mask shadow pattern
IMX = 1.938793204284003E-01, IMY = -2.023434344718492E-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:
-239.976000 -6.312000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6146 22.0309 1.5 54.3 1.6 8.0728 7.4 1.4 Crab
34.3495 64.0310 3.9 32.0 77.2 2.0291 2.9 ------ UNKNOWN
136.3386 48.1186 3.3 23.3 -66.9 1.3384 3.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-6.312000 13.324600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6882 21.8462 0.0 54.4 1.4 0.6274 1.8 10.5 Crab
254.3482 64.6411 3.2 40.2 163.6 0.4714 3.6 ------ UNKNOWN
83.0497 66.1248 0.2 15.7 46.2 4.7223 60.5 ------ UNKNOWN
127.7589 22.8597 2.6 47.9 -50.9 1.4286 4.4 ------ UNKNOWN
164.0996 35.2941 3.2 41.1 -99.1 1.1724 3.6 ------ UNKNOWN
132.9889 25.3293 3.8 45.7 -57.6 1.0401 3.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
61.724600 962.072300
1001.024000 1091.064000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6066 22.0277 0.8 44.1 -12.8 37.0084 14.1 1.7 Crab
333.0297 68.2769 2.6 37.0 132.7 14.4411 4.4 ------ UNKNOWN
40.8020 61.4735 2.2 18.8 83.8 8.4474 5.2 ------ UNKNOWN
62.2305 46.9493 2.8 22.1 28.1 6.8658 4.1 ------ UNKNOWN
112.2560 48.3853 3.2 23.3 -67.0 6.2779 3.7 ------ UNKNOWN
157.8090 60.2094 2.9 32.2 -127.8 7.4256 4.0 ------ UNKNOWN
Plot creation:
Sat Sep 30 00:42:04 EDT 2023