Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minutes to calcaulte
Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
83.7373 +22.2602 0.0107 13.7 126.0 2.5488 17.9 TRIG_01192735
------------------------------------------
Foreground time interval of the image:
0.000 64.000 (delta_t = 64.000 [sec])
Background time interval of the image:
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 2) The mask-weighted light curves are using the flight position.
- 3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 4) 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.
- 5) 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.
- 6) 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 64.000000
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 64.000000
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 64.000000
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) For long bursts, a spectral fit of 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.
- 4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.
Time averaged spectrum fit using the pre-slew DRM
Power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.05498 ( -0.14016 0.145548 )
Norm@50keV : 2.04636E-03 ( -0.000184921 0.000181645 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.47 using 59 PHA bins.
# Reduced chi-squared = 1.254 for 57 degrees of freedom
# Null hypothesis probability = 9.401004e-02
Photon flux (15-150 keV) in 64 sec: 0.314975 ( -0.0221788 0.0221991 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21206e-06 ( -9.98477e-08 1.01398e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.77110 ( -0.613552 0.34517 )
Epeak [keV] : 34.4595 ( )
Norm@50keV : 2.95845E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.69 using 59 PHA bins.
# Reduced chi-squared = 1.262 for 56 degrees of freedom
# Null hypothesis probability = 8.939429e-02
Photon flux (15-150 keV) in 64 sec: 0.310172 ( -0.023932 0.0239 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17587e-06 ( -1.19098e-07 1.22253e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.74909 ( 1.74909 1.74909 )
beta : -2.47226 ( 2.43955 0.501449 )
Epeak [keV] : 35.2673 ( -34.9405 -34.9405 )
Norm@50keV : 3.03613E-03 ( -0.00105022 0.0934259 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.67 using 59 PHA bins.
# Reduced chi-squared = 1.285 for 55 degrees of freedom
# Null hypothesis probability = 7.570934e-02
Photon flux (15-150 keV) in 64 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17263e-06 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.1289 ( )
R^2/D10^2 : 0.133214 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 114.82 using 59 PHA bins.
# Reduced chi-squared = 2.0144 for 57 degrees of freedom
# Null hypothesis probability = 8.959220e-06
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.789e-07 2.253e-08
25- 50 4.529e-07 3.539e-08
50-150 2.453e-07 5.002e-08
15-150 8.771e-07 7.776e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 63.3313 (-12.9335 18.0513)
Norm : 1.58563 (-0.189399 0.208569)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.571e-07 2.477e-08
25- 50 3.978e-07 2.829e-08
50-150 4.730e-07 9.232e-08
15-150 1.128e-06 1.011e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.14126 (-0.974931 1.31053)
R1^2/D10^2 : 3.06962 (-2.07633 6.83317)
kT2 [keV] : 15.1365 (-2.3302 3.70265)
R2^2/D10^2 : 2.31194E-02 (-0.0138679 0.0159796)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.817e-07 1.242e-07
25- 50 3.679e-07 9.594e-08
50-150 4.458e-07 1.369e-07
15-150 1.095e-06 2.669e-07
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.05498 ( -0.14016 0.145548 )
Norm@50keV : 2.04636E-03 ( -0.000184921 0.000181645 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.47 using 59 PHA bins.
# Reduced chi-squared = 1.254 for 57 degrees of freedom
# Null hypothesis probability = 9.401004e-02
Photon flux (15-150 keV) in 64 sec: 0.314975 ( -0.0221788 0.0221991 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21206e-06 ( -9.98477e-08 1.01398e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.77110 ( -0.613552 0.34517 )
Epeak [keV] : 34.4595 ( )
Norm@50keV : 2.95845E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.69 using 59 PHA bins.
# Reduced chi-squared = 1.262 for 56 degrees of freedom
# Null hypothesis probability = 8.939429e-02
Photon flux (15-150 keV) in 64 sec: 0.310172 ( -0.023932 0.0239 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17587e-06 ( -1.19098e-07 1.22253e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.74909 ( 1.74909 1.74909 )
beta : -2.47226 ( 2.43955 0.501449 )
Epeak [keV] : 35.2673 ( -34.9405 -34.9405 )
Norm@50keV : 3.03613E-03 ( -0.00105022 0.0934177 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.67 using 59 PHA bins.
# Reduced chi-squared = 1.285 for 55 degrees of freedom
# Null hypothesis probability = 7.570934e-02
Photon flux (15-150 keV) in 64 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17263e-06 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.1289 ( )
R^2/D10^2 : 0.133214 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.789e-07 2.214e-08
25- 50 4.529e-07 3.798e-08
50-150 2.453e-07 4.650e-08
15-150 8.771e-07 7.424e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 63.3313 (-12.9335 18.0513)
Norm : 1.58563 (-0.189399 0.208569)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.571e-07 2.541e-08
25- 50 3.978e-07 3.040e-08
50-150 4.730e-07 9.309e-08
15-150 1.128e-06 1.056e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.14126 (-0.974931 1.31053)
R1^2/D10^2 : 3.06962 (-2.07633 6.83317)
kT2 [keV] : 15.1365 (-2.3302 3.70265)
R2^2/D10^2 : 2.31194E-02 (-0.0138679 0.0159796)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.817e-07 1.208e-07
25- 50 3.679e-07 9.245e-08
50-150 4.458e-07 1.297e-07
15-150 1.095e-06 2.792e-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: 2.05498 ( -0.14016 0.145548 )
Norm@50keV : 2.04636E-03 ( -0.000184921 0.000181645 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.47 using 59 PHA bins.
# Reduced chi-squared = 1.254 for 57 degrees of freedom
# Null hypothesis probability = 9.401004e-02
Photon flux (15-150 keV) in 64 sec: 0.314975 ( -0.0221788 0.0221991 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21206e-06 ( -9.98477e-08 1.01398e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.77110 ( -0.613552 0.34517 )
Epeak [keV] : 34.4595 ( )
Norm@50keV : 2.95845E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.69 using 59 PHA bins.
# Reduced chi-squared = 1.262 for 56 degrees of freedom
# Null hypothesis probability = 8.939429e-02
Photon flux (15-150 keV) in 64 sec: 0.310172 ( -0.023932 0.0239 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17587e-06 ( -1.19098e-07 1.22253e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.74909 ( 1.74909 1.74909 )
beta : -2.47226 ( 2.43955 0.501449 )
Epeak [keV] : 35.2673 ( -34.9405 -34.9405 )
Norm@50keV : 3.03613E-03 ( -0.00105022 0.126672 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.67 using 59 PHA bins.
# Reduced chi-squared = 1.285 for 55 degrees of freedom
# Null hypothesis probability = 7.570934e-02
Photon flux (15-150 keV) in 64 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.17263e-06 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 3.71e-07
S(50-100 keV) = 3.57e-07
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 0.962264
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.922046
Count Ratio (50-100 keV) / (15-25 keV) = 0.468303
Mask shadow pattern
IMX = -1.435688946779908E-01, IMY = -1.975824289523088E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7546 22.1757 0.7 13.7 125.7 2.2581 15.9 11.8 Crab
53.5838 53.5184 2.9 50.8 150.8 2.5049 4.0 ------ UNKNOWN
98.0047 -33.4630 3.0 48.4 -0.3 1.1777 3.9 ------ UNKNOWN
141.5934 34.0429 2.5 45.2 -121.5 2.8437 4.5 ------ UNKNOWN
143.0796 40.1220 2.0 48.0 -129.1 3.1909 5.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
117.900600 268.530000
270.000000 287.756500
290.000000 426.460000
432.000000 432.850000
434.000000 483.134800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7423 22.1690 0.7 0.1 -5.9 10.7574 17.2 11.1 Crab
47.1176 49.2563 2.7 39.5 144.8 5.9239 4.2 ------ UNKNOWN
57.8591 76.4185 2.3 55.7 175.4 10.4810 5.1 ------ UNKNOWN
135.4258 55.3811 2.7 50.4 -142.1 6.1706 4.2 ------ UNKNOWN
121.3905 -7.0525 2.6 47.1 -53.3 11.7745 4.5 ------ UNKNOWN
Plot creation:
Wed Sep 27 12:49:13 EDT 2023