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
86.7713 -0.6657 0.0054 20.8755 136.5733 1.6439127 35.349 TRIG_01267921
Foreground time interval of the image:
-0.472 9.292 (delta_t = 9.764 [sec])
Background time interval of the image:
-239.584 -0.472 (delta_t = 239.112 [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 -0.472 sec. to 9.292 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.57397 ( -0.0753757 0.0758454 )
Norm@50keV : 1.11646E-02 ( -0.000505222 0.000504026 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.62 using 59 bins.
Reduced chi-squared = 0.993333
# Null hypothesis probability of 4.89e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 9.764 sec: 1.42342 ( -0.06437 0.06445 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.023e-06 ( -4.96564e-08 4.98681e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.472 sec. to 9.292 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.712840 ( -0.377886 0.347071 )
Epeak [keV] : 73.0320 ( -9.43604 18.0254 )
Norm@50keV : 3.07548E-02 ( -0.0101361 0.0168979 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 36.50 using 59 bins.
Reduced chi-squared = 0.651786
# Null hypothesis probability of 9.80e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 9.764 sec: 1.36630 ( -0.06799 0.06802 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.56727e-07 ( -5.58241e-08 5.61296e-08 ) ergs/cm2
Band function
Time interval is from -0.472 sec. to 9.292 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] : 14.0753 (-0.709765 0.755336)
R^2/D10^2 : 0.201735 (-0.0348303 0.0415419)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 98.83 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.95e-04 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.239e-08 6.674e-09
25- 50 3.081e-07 1.562e-08
50-150 4.030e-07 3.705e-08
15-150 7.934e-07 4.135e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 176.441 (-35.5344 -176.356)
Norm : 5.84931 (-0.28022 0.298475)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.55 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.05e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.444e-07 9.227e-09
25- 50 2.736e-07 2.861e-08
50-150 5.751e-07 1.848e-07
15-150 9.930e-07 2.193e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.09412 (-1.70517 1.79067)
R1^2/D10^2 : 0.859375 (-0.351224 0.837327)
kT2 [keV] : 23.9920 (-4.50305 9.58894)
R2^2/D10^2 : 2.07899E-02 (-0.0150891 0.0289769)
------------------------------------------------------------
#Fit statistic : Chi-Squared 37.43 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.66e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.210e-07 1.886e-08
25- 50 2.942e-07 4.189e-08
50-150 5.427e-07 1.939e-07
15-150 9.578e-07 1.881e-07
Peak spectrum fit
Power-law model
Time interval is from 0.472 sec. to 1.472 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.55219 ( -0.0752759 0.075919 )
Norm@50keV : 4.22709E-02 ( -0.00210958 0.00210506 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 96.95 using 59 bins.
Reduced chi-squared = 1.70088
# Null hypothesis probability of 7.62e-04 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 5.35478 ( -0.26384 0.264 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.97878e-07 ( -2.12349e-08 2.13111e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.472 sec. to 1.472 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.107495 ( -0.43838 0.396238 )
Epeak [keV] : 63.5609 ( -5.51903 7.74144 )
Norm@50keV : 0.236986 ( -0.0882412 0.160947 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.93 using 59 bins.
Reduced chi-squared = 0.855893
# Null hypothesis probability of 7.70e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 5.14442 ( -0.26952 0.2697 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.66817e-07 ( -2.2689e-08 2.29096e-08 ) ergs/cm2
Band function
Time interval is from 0.472 sec. to 1.472 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] : 14.0227 (-0.698633 0.741552)
R^2/D10^2 : 0.819936 (-0.140133 0.166293)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 77.28 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.82e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.405e-08 2.930e-09
25- 50 1.269e-07 6.600e-09
50-150 1.644e-07 1.610e-08
15-150 3.253e-07 1.950e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 176.875 (-35.6167 -176.771)
Norm : 22.2925 (-1.14843 1.20055)
------------------------------------------------------------
#Fit statistic : Chi-Squared 75.42 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.17e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.633e-08 3.970e-09
25- 50 1.068e-07 1.330e-08
50-150 2.247e-07 7.183e-08
15-150 3.878e-07 8.025e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.48369 (-1.93862 1.79188)
R1^2/D10^2 : 2.02616 (-0.667826 1.39973)
kT2 [keV] : 24.1099 (-5.13994 11.5315)
R2^2/D10^2 : 6.82827E-02 (-0.0545575 0.135894)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.37e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.339e-08 7.970e-09
25- 50 1.228e-07 2.431e-08
50-150 2.067e-07 7.564e-08
15-150 3.730e-07 1.007e-07
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: 1.57397 ( -0.0753757 0.0758454 )
Norm@50keV : 1.11646E-02 ( -0.000505222 0.000504026 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.89e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 9.764 sec: 1.42338 ( -0.0643668 0.0644409 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.02286e-06 ( -4.96595e-08 4.98642e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.712840 ( -0.377887 0.34707 )
Epeak [keV] : 73.0321 ( -9.43607 18.0253 )
Norm@50keV : 3.07548E-02 ( -0.010136 0.016898 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 36.50 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.80e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 9.764 sec: 1.36615 ( -0.06797 0.068 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.57058e-07 ( -5.58803e-08 5.61723e-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) = 2.62e-07
S(50-100 keV) = 3.52e-07
T90 vs. Hardness ratio plot
T90 = 3.69999992847443 sec.
Hardness ratio (energy fluence ratio) = 1.34351
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.59044
Count Ratio (50-100 keV) / (15-25 keV) = 1.05772
Mask shadow pattern
IMX = -2.769737525344806E-01, IMY = -2.621660003891960E-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:
-239.584000 -0.472000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6024 22.0321 2.3 42.7 122.5 8.0253 5.0 2.0 Crab
138.5195 -4.8568 2.6 58.7 -159.1 9.1354 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.472000 9.292000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5964 21.8526 0.0 42.5 122.5 -0.1113 -0.6 9.9 Crab
86.7712 -0.6657 0.3 20.9 136.6 1.6438 35.3 ------ UNKNOWN
130.7641 0.3887 2.2 53.7 -168.7 0.6362 5.3 ------ UNKNOWN
129.8009 -35.1212 2.7 45.7 -122.6 0.7414 4.4 ------ UNKNOWN
132.7786 -30.5116 2.8 48.0 -129.0 0.6564 4.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
91.316600 99.755100
100.416000 962.456000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6349 22.0225 0.4 22.9 141.8 35.7807 25.7 0.5 Crab
56.0048 0.5789 2.8 30.8 61.5 8.9820 4.1 ------ UNKNOWN
49.0340 -35.8737 2.9 49.6 9.9 7.4149 4.0 ------ UNKNOWN
57.4677 -30.8473 3.4 41.0 9.1 5.3574 3.4 ------ UNKNOWN
123.1835 32.8830 3.2 48.0 -168.6 8.9987 3.6 ------ UNKNOWN
63.6033 -48.6464 3.9 52.0 -11.5 6.8481 2.9 ------ UNKNOWN
134.4388 5.7592 3.0 48.0 -129.1 22.2157 3.9 ------ UNKNOWN
Plot creation:
Wed Dec 18 17:40:55 EST 2024