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
292.5028 -32.9803 0.0189 31.9015 77.1033 0.7647154 10.148 TRIG_01176135
Foreground time interval of the image:
-0.032 9.101 (delta_t = 9.133 [sec])
Background time interval of the image:
-368.800 -278.688 (delta_t = 90.112 [sec])
-239.800 -0.032 (delta_t = 239.768 [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 -0.032 sec. to 24.160 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.54707 ( -0.385614 0.458662 )
Norm@50keV : 1.68585E-03 ( -0.000561454 0.000566093 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.33 using 59 bins.
Reduced chi-squared = 1.09351
# Null hypothesis probability of 2.92e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 24.19 sec: 0.341014 ( -0.062321 0.062389 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.13272e-07 ( -9.75851e-08 1.04664e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.032 sec. to 24.160 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.91920 ( )
Epeak [keV] : 4.25402 ( )
Norm@50keV : 4.42107E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.95 using 59 bins.
Reduced chi-squared = 1.10625
# Null hypothesis probability of 2.72e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 24.19 sec: 0.336717 ( -0.062465 0.061851 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.8608e-07 ( -1.03282e-07 1.11492e-07 ) ergs/cm2
Band function
Time interval is from -0.032 sec. to 24.160 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] : 5.89958 (-1.14087 1.53696)
R^2/D10^2 : 1.32027 (-0.82206 2.08031)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.89 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.96e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.441e-07 6.008e-08
25- 50 1.385e-07 5.943e-08
50-150 1.183e-08 8.219e-09
15-150 2.944e-07 1.054e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 27.9671 (-10.4632 18.8202)
Norm : 2.92072 (-1.00965 1.84585)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.22 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.96e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.385e-07 3.841e-08
25- 50 1.520e-07 5.065e-08
50-150 7.579e-08 4.733e-08
15-150 3.663e-07 1.124e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.62587 (-1.2741 1.44187)
R1^2/D10^2 : 3.13536 (-2.12088 9.5468)
kT2 [keV] : 16.2700 (-7.17105 28.1842)
R2^2/D10^2 : 1.10206E-02 (-0.0109647 0.0379095)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.96 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.00e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.482e-07 8.289e-08
25- 50 1.338e-07 7.084e-08
50-150 1.175e-07 7.742e-08
15-150 3.995e-07 1.986e-07
Peak spectrum fit
Power-law model
Time interval is from 0.076 sec. to 1.076 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.12881 ( -0.23367 0.256458 )
Norm@50keV : 1.74103E-02 ( -0.00326116 0.00317836 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.25 using 59 bins.
Reduced chi-squared = 0.846491
# Null hypothesis probability of 7.89e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.77893 ( -0.38986 0.38987 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.62271e-07 ( -2.70575e-08 2.76268e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.076 sec. to 1.076 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.665665 ( -1.35465 1.07231 )
Epeak [keV] : 37.4362 ( -9.25337 10.5231 )
Norm@50keV : 0.126558 ( -0.126562 0.686918 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.46 using 59 bins.
Reduced chi-squared = 0.758214
# Null hypothesis probability of 9.09e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.73345 ( -0.38878 0.38951 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.50546e-07 ( -2.5888e-08 2.76837e-08 ) ergs/cm2
Band function
Time interval is from 0.076 sec. to 1.076 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] : 9.78614 (-1.47277 1.6255)
R^2/D10^2 : 1.49163 (-0.667707 1.28314)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.83 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.71e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.887e-08 7.375e-09
25- 50 6.959e-08 1.354e-08
50-150 3.411e-08 1.319e-08
15-150 1.326e-07 2.461e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 53.6382 (-15.3651 25.241)
Norm : 15.6044 (-3.11153 4.06167)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.40 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.08e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.874e-08 6.880e-09
25- 50 5.700e-08 1.885e-08
50-150 5.904e-08 4.280e-08
15-150 1.548e-07 6.482e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.61156 (-1.96022 2.73005)
R1^2/D10^2 : 14.1793 (-11.4125 160.533)
kT2 [keV] : 13.3334 (-2.96334 6.02339)
R2^2/D10^2 : 0.344745 (-0.293189 0.742429)
------------------------------------------------------------
#Fit statistic : Chi-Squared 41.42 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.12e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.766e-08 2.079e-08
25- 50 5.909e-08 3.054e-08
50-150 5.277e-08 3.200e-08
15-150 1.495e-07 7.925e-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: 2.01158 ( -0.270496 0.295737 )
Norm@50keV : 4.63862E-03 ( -0.000913265 0.000882092 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.08e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 9.133 sec: 0.699525 ( -0.104166 0.104176 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.90931e-07 ( -7.04864e-08 7.26558e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.32131 ( -1.34412 0.820704 )
Epeak [keV] : 41.5850 ( -20.3182 -41.5848 )
Norm@50keV : 1.15582E-02 ( -0.011558 0.0561837 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.15e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 9.133 sec: 0.684324 ( -0.103941 0.106677 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.68645e-07 ( -7.30695e-08 7.99348e-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) = 1.38e-07
S(50-100 keV) = 9.43e-08
T90 vs. Hardness ratio plot
T90 = 23.5519998073578 sec.
Hardness ratio (energy fluence ratio) = 0.683333
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.531892
Count Ratio (50-100 keV) / (15-25 keV) = 0.238987
Mask shadow pattern
IMX = 1.389340615369184E-01, IMY = -6.067783706846753E-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:
-368.800000 -278.688000
-239.800000 -0.032000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
293.7393 -29.1468 2.4 31.6 84.6 5.0752 4.8 ------ UNKNOWN
330.2348 15.3056 2.7 47.1 179.2 5.9647 4.2 ------ UNKNOWN
333.9901 -10.9167 3.2 21.2 -170.8 1.9743 3.6 ------ UNKNOWN
33.4781 -77.1283 3.0 53.1 -14.8 4.7478 3.8 ------ UNKNOWN
2.2548 -52.4314 2.5 30.9 -39.2 3.2475 4.7 ------ UNKNOWN
25.5539 -41.8737 2.5 44.4 -61.2 12.4095 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.032000 9.100600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
271.2239 -50.3311 2.6 46.9 48.2 0.8513 4.4 ------ UNKNOWN
292.5027 -32.9803 1.1 31.9 77.1 0.7646 10.1 ------ UNKNOWN
285.9251 -46.9139 2.7 37.0 52.3 0.3676 4.3 ------ UNKNOWN
326.9779 -14.8374 2.3 17.3 168.1 0.1844 5.0 ------ UNKNOWN
16.9938 -56.6907 2.4 40.4 -38.4 0.3097 4.7 ------ UNKNOWN
31.7771 -59.8135 2.2 48.6 -36.4 0.5277 5.2 ------ UNKNOWN
20.4592 -33.2625 2.2 41.8 -74.5 0.7807 5.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
151.900620 165.500590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
84.4882 -13.7185 2.5 43.0 -50.9 0.5631 4.6 ------ UNKNOWN
81.1664 17.7423 2.2 41.2 -98.8 1.0130 5.3 ------ UNKNOWN
Plot creation:
Sat Sep 30 00:48:04 EDT 2023