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
16.5778 -22.6590 0.0129 12.9581 44.4324 0.2599419 14.881 TRIG_01267501
Foreground time interval of the image:
-0.020 2.188 (delta_t = 2.208 [sec])
Background time interval of the image:
-239.320 -0.020 (delta_t = 239.300 [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 0.512000
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 0.512000
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 0.512000
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 -0.020 sec. to 2.188 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.80742 ( -0.226591 0.237964 )
Norm@50keV : 6.27370E-03 ( -0.000895979 0.000864851 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.93 using 59 bins.
Reduced chi-squared = 0.893509
# Null hypothesis probability of 7.01e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 2.208 sec: 0.867048 ( -0.100758 0.100803 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.27511e-07 ( -1.8194e-08 1.85782e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.020 sec. to 2.188 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.30872 ( -0.777236 0.132784 )
Epeak [keV] : 114.390 ( )
Norm@50keV : 3.54649E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.71 using 59 bins.
Reduced chi-squared = 0.887679
# Null hypothesis probability of 7.10e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 2.208 sec: 0.692381 ( -0.148593 0.176054 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.12331e-07 ( -2.28771e-08 1.95795e-08 ) ergs/cm2
Band function
Time interval is from -0.020 sec. to 2.188 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] : 11.0592 (-2.04137 2.67255)
R^2/D10^2 : 0.264795 (-0.141532 0.299101)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 84.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.76e-03 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.496e-08 3.210e-09
25- 50 4.259e-08 6.834e-09
50-150 2.954e-08 9.349e-09
15-150 8.708e-08 1.624e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 114.870 (-46.4269 -114.034)
Norm : 3.66471 (-0.480895 0.750092)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.75e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.111e-08 3.570e-09
25- 50 3.747e-08 7.938e-09
50-150 6.543e-08 3.592e-08
15-150 1.240e-07 4.105e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.86508 (-1.20126 1.56005)
R1^2/D10^2 : 4.79811 (-3.22832 12.3604)
kT2 [keV] : 24.5244 (-6.39534 12.5285)
R2^2/D10^2 : 1.27121E-02 (-0.00933524 0.0137412)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.86e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.603e-08 1.324e-08
25- 50 3.071e-08 1.206e-08
50-150 7.490e-08 4.268e-08
15-150 1.316e-07 4.989e-08
Peak spectrum fit
Power-law model
Time interval is from -0.020 sec. to 0.980 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65293 ( -0.201765 0.208507 )
Norm@50keV : 1.08713E-02 ( -0.00134321 0.00131497 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.06 using 59 bins.
Reduced chi-squared = 0.790526
# Null hypothesis probability of 8.74e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.42095 ( -0.15708 0.15722 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.01093e-07 ( -1.32535e-08 1.34451e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.020 sec. to 0.980 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.64896 ( -0.570093 0.210783 )
Epeak [keV] : 9999.09 ( -9999.32 -9999.33 )
Norm@50keV : 1.08955E-02 ( -0.00680552 0.0103005 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.06 using 59 bins.
Reduced chi-squared = 0.804643
# Null hypothesis probability of 8.52e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.05186 ( -0.305792 0.28555 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.01503e-07 ( -1.47769e-08 1.39858e-08 ) ergs/cm2
Band function
Time interval is from -0.020 sec. to 0.980 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] : 13.3243 (-2.31948 2.82324)
R^2/D10^2 : 0.230269 (-0.1113 0.223564)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.35e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.665e-09 1.827e-09
25- 50 3.064e-08 4.780e-09
50-150 3.487e-08 9.465e-09
15-150 7.418e-08 1.120e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 162.157 (-67.3337 -161.869)
Norm : 5.81204 (-0.692099 0.829568)
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.37e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.482e-08 7.870e-09
25- 50 2.778e-08 1.324e-08
50-150 5.657e-08 3.229e-08
15-150 9.916e-08 5.061e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.41390 (-1.35478 1.65911)
R1^2/D10^2 : 4.50329 (-2.87937 12.4247)
kT2 [keV] : 25.3449 (-5.84578 10.5025)
R2^2/D10^2 : 2.00958E-02 (-0.0137041 0.0307421)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.77e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.712e-08 8.535e-09
25- 50 2.450e-08 8.929e-09
50-150 6.114e-08 3.225e-08
15-150 1.028e-07 3.811e-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: 1.80742 ( -0.226591 0.237964 )
Norm@50keV : 6.27370E-03 ( -0.000895979 0.000864851 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.01e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 2.208 sec: 0.867003 ( -0.100751 0.100795 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.27494e-07 ( -1.81908e-08 1.8572e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.58980 ( -1.10508 0.238633 )
Epeak [keV] : 197.529 ( )
Norm@50keV : 2.66905E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.05 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.98e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 2.208 sec: 0.867733 ( -0.101367 0.100358 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.27776e-07 ( -1.84955e-08 1.81036e-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) = 3.60e-08
S(50-100 keV) = 4.11e-08
T90 vs. Hardness ratio plot
T90 = 1.87199985980988 sec.
Hardness ratio (energy fluence ratio) = 1.14167
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.912437
Count Ratio (50-100 keV) / (15-25 keV) = 0.578175
Mask shadow pattern
IMX = 1.643081713956925E-01, IMY = -1.610843671840437E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-239.320000 -0.020000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
28.7962 -3.7142 3.4 32.2 77.5 2.1292 3.4 ------ UNKNOWN
9.9962 -38.9569 2.6 9.6 -54.7 1.3749 4.5 ------ UNKNOWN
49.2422 -51.2987 2.3 26.0 -159.9 1.5059 5.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.020000 2.188000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
25.4646 -20.4193 2.1 15.2 79.1 0.0984 5.4 ------ UNKNOWN
16.5778 -22.6590 0.8 13.0 44.4 0.2599 14.9 ------ UNKNOWN
336.8098 1.5721 2.3 55.1 4.6 0.3731 5.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
59.580600 311.951300
312.680000 362.860000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
356.0824 26.1464 2.8 52.7 26.4 62.8968 4.1 ------ UNKNOWN
343.8369 17.0664 3.3 51.0 8.0 30.9678 3.5 ------ UNKNOWN
336.8878 18.9100 3.5 56.8 3.5 54.7838 3.3 ------ UNKNOWN
Plot creation:
Wed Dec 18 17:41:36 EST 2024