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
53.5615 37.9486 0.0122 25.7252 -108.9616 1.1051554 15.858 TRIG_01015919
Foreground time interval of the image:
-0.148 11.381 (delta_t = 11.529 [sec])
Background time interval of the image:
-239.120 -0.148 (delta_t = 238.972 [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 1.024000
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 1.024000
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 1.024000
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 -0.148 sec. to 22.764 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.83384 ( -0.13723 0.141038 )
Norm@50keV : 5.59898E-03 ( -0.00046601 0.00045856 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.12 using 59 bins.
Reduced chi-squared = 0.967018
# Null hypothesis probability of 5.46e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 22.91 sec: 0.781925 ( -0.055599 0.055668 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17995e-06 ( -9.83584e-08 9.98251e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.148 sec. to 22.764 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.77767 ( -0.53141 0.497468 )
Epeak [keV] : 179.309 ( -129.808 -179.337 )
Norm@50keV : 6.00710E-03 ( -0.0022793 0.00551084 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.08 using 59 bins.
Reduced chi-squared = 0.983571
# Null hypothesis probability of 5.10e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 22.91 sec: 0.779489 ( -0.059374 0.057605 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17275e-06 ( -1.15798e-07 1.0544e-07 ) ergs/cm2
Band function
Time interval is from -0.148 sec. to 22.764 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] : 11.3884 (-1.07789 1.2057)
R^2/D10^2 : 0.216923 (-0.0675477 0.0976686)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 109.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.26e-05 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.355e-07 1.713e-08
25- 50 4.003e-07 3.368e-08
50-150 3.010e-07 5.395e-08
15-150 8.368e-07 6.827e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 97.2302 (-23.9667 38.9567)
Norm : 3.43359 (-0.346547 0.410104)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.37 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.61e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.056e-07 2.487e-08
25- 50 3.534e-07 2.910e-08
50-150 5.636e-07 1.960e-07
15-150 1.123e-06 2.157e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.54636 (-1.15034 1.30945)
R1^2/D10^2 : 2.27928 (-1.22333 3.52291)
kT2 [keV] : 21.4119 (-4.1655 6.89326)
R2^2/D10^2 : 1.66314E-02 (-0.0105632 0.0213923)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.25 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.28e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.217e-07 6.881e-08
25- 50 3.283e-07 8.227e-08
50-150 5.929e-07 2.030e-07
15-150 1.143e-06 3.705e-07
Peak spectrum fit
Power-law model
Time interval is from 10.832 sec. to 11.832 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.73958 ( -0.243651 0.255462 )
Norm@50keV : 1.39035E-02 ( -0.00229202 0.0022371 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 34.77 using 59 bins.
Reduced chi-squared = 0.61
# Null hypothesis probability of 9.91e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.87290 ( -0.26689 0.26695 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.28396e-07 ( -2.1643e-08 2.20844e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 10.832 sec. to 11.832 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.23818 ( -1.13246 0.882495 )
Epeak [keV] : 67.2517 ( -54.733 -67.2526 )
Norm@50keV : 2.65635E-02 ( -0.026563 0.0872649 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 33.95 using 59 bins.
Reduced chi-squared = 0.60625
# Null hypothesis probability of 9.91e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.84501 ( -0.27192 0.27193 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.22535e-07 ( -2.36e-08 2.45235e-08 ) ergs/cm2
Band function
Time interval is from 10.832 sec. to 11.832 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] : 11.6928 (-2.04961 2.49233)
R^2/D10^2 : 0.505014 (-0.255811 0.51897)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.54 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.62e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.457e-08 4.042e-09
25- 50 4.445e-08 8.480e-09
50-150 3.590e-08 1.265e-08
15-150 9.491e-08 2.045e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 113.693 (-47.32 -112.386)
Norm : 8.06062 (-1.23839 1.84747)
------------------------------------------------------------
#Fit statistic : Chi-Squared 33.96 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.93e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.103e-08 4.475e-09
25- 50 3.727e-08 9.705e-09
50-150 6.473e-08 3.846e-08
15-150 1.230e-07 4.575e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.87837 (-1.85756 2.43962)
R1^2/D10^2 : 4.11844 (-2.84585 13.0767)
kT2 [keV] : 20.8708 (-6.01439 15.3053)
R2^2/D10^2 : 4.52893E-02 (-0.0390038 0.126616)
------------------------------------------------------------
#Fit statistic : Chi-Squared 32.60 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.93e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.209e-08 1.239e-08
25- 50 3.663e-08 1.939e-08
50-150 6.356e-08 3.669e-08
15-150 1.223e-07 6.400e-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: 1.69208 ( -0.168312 0.173269 )
Norm@50keV : 6.15859E-03 ( -0.000638624 0.000628265 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 70.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.09e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 11.53 sec: 0.815678 ( -0.075142 0.0751819 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.57876e-07 ( -7.16745e-08 7.28064e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.40076 ( -0.712287 0.333889 )
Epeak [keV] : 96.3991 ( -43.8423 -96.3991 )
Norm@50keV : 8.79992E-03 ( -0.00319326 0.0118413 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.84 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.01e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 11.53 sec: 0.804346 ( -0.078975 0.078794 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.40516e-07 ( -8.03214e-08 8.15194e-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) = 3.37e-07
S(50-100 keV) = 3.78e-07
T90 vs. Hardness ratio plot
T90 = 19.944000005722 sec.
Hardness ratio (energy fluence ratio) = 1.12166
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.04937
Count Ratio (50-100 keV) / (15-25 keV) = 0.676163
Mask shadow pattern
IMX = -1.565562409960690E-01, IMY = 4.556650039485672E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-239.120000 -0.148000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6341 22.0055 0.4 9.9 141.8 9.2685 26.7 0.5 Crab
120.3684 14.1168 2.3 37.5 68.6 4.0325 5.0 ------ UNKNOWN
147.9431 55.4088 2.3 49.6 0.7 3.1285 5.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.148000 11.380600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4729 21.9574 7.0 9.9 142.7 0.0836 1.7 9.6 Crab
48.8956 -12.5655 2.6 55.8 -178.2 0.9110 4.4 ------ UNKNOWN
53.5615 37.9486 0.7 25.7 -109.0 1.1048 15.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
64.380600 752.080600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6561 22.0217 0.5 30.3 109.9 27.7541 21.8 1.3 Crab
72.1922 16.5759 2.8 26.9 134.4 4.5671 4.1 ------ UNKNOWN
307.2871 77.3895 3.3 56.5 -17.7 9.3773 3.5 ------ UNKNOWN
5.6034 28.4166 3.8 40.8 -92.0 12.6842 3.1 ------ UNKNOWN
16.4857 3.9104 2.3 48.0 -129.0 17.9718 4.9 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:19:56 EDT 2022