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
97.5571 68.7133 0.0102 45.6972 174.9711 1.1413343 18.796 TRIG_01033264
Foreground time interval of the image:
-0.832 3.168 (delta_t = 4.000 [sec])
Background time interval of the image:
-239.832 -0.832 (delta_t = 239.000 [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 -0.832 sec. to 3.168 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.91282 ( -0.154892 0.160385 )
Norm@50keV : 1.71398E-02 ( -0.00173832 0.00171168 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.24 using 59 bins.
Reduced chi-squared = 1.10947
# Null hypothesis probability of 2.65e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 4 sec: 2.47340 ( -0.22361 0.22389 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.30508e-07 ( -6.23488e-08 6.29816e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.832 sec. to 3.168 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.32999 ( -0.84025 0.674408 )
Epeak [keV] : 51.2799 ( -16.3111 -51.2753 )
Norm@50keV : 3.60089E-02 ( -0.0194093 0.0694117 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.14 using 59 bins.
Reduced chi-squared = 1.09179
# Null hypothesis probability of 2.97e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 4 sec: 2.42077 ( -0.23358 0.2327 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.01588e-07 ( -7.16196e-08 7.1714e-08 ) ergs/cm2
Band function
Time interval is from -0.832 sec. to 3.168 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] : 11.0076 (-1.03287 1.14816)
R^2/D10^2 : 0.816494 (-0.259823 0.375342)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 80.69 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.12e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.270e-08 1.312e-08
25- 50 2.340e-07 2.488e-08
50-150 1.603e-07 3.330e-08
15-150 4.770e-07 5.140e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 80.4223 (-19.7618 31.4995)
Norm : 11.6122 (-1.52809 1.81394)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.08 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.32e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.206e-07 1.640e-08
25- 50 1.987e-07 1.874e-08
50-150 2.815e-07 9.862e-08
15-150 6.008e-07 9.600e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.69571 (-2.73271 1.63958)
R1^2/D10^2 : 1.69605 (-0.736942 3.39818)
kT2 [keV] : 39.2955 (-22.2061 -39.7437)
R2^2/D10^2 : 4.33926E-03 (-0.00371295 0.0926861)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.11 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.38e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.015e-07 2.298e-08
25- 50 2.210e-07 5.186e-08
50-150 2.899e-07 1.423e-07
15-150 6.124e-07 1.934e-07
Peak spectrum fit
Power-law model
Time interval is from 0.168 sec. to 1.168 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.85343 ( -0.16996 0.177159 )
Norm@50keV : 3.50346E-02 ( -0.00388038 0.00382008 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.36 using 59 bins.
Reduced chi-squared = 1.02386
# Null hypothesis probability of 4.25e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.93163 ( -0.50404 0.50478 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.22174e-07 ( -3.55253e-08 3.57493e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.168 sec. to 1.168 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.41964 ( -0.843719 0.8068 )
Epeak [keV] : 63.8578 ( -22.2027 -63.8564 )
Norm@50keV : 5.95113E-02 ( -0.0261577 0.106872 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.29 using 59 bins.
Reduced chi-squared = 1.02304
# Null hypothesis probability of 4.27e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.86070 ( -0.51885 0.51791 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.14355e-07 ( -3.84751e-08 3.81376e-08 ) ergs/cm2
Band function
Time interval is from 0.168 sec. to 1.168 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] : 11.8229 (-1.26208 1.43343)
R^2/D10^2 : 1.27010 (-0.448353 0.672709)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 76.87 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.09e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.750e-08 6.665e-09
25- 50 1.160e-07 1.569e-08
50-150 9.648e-08 2.070e-08
15-150 2.499e-07 3.230e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 95.6615 (-26.907 47.2873)
Norm : 22.0560 (-3.0283 3.59508)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.62e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.763e-08 8.670e-09
25- 50 9.875e-08 1.123e-08
50-150 1.560e-07 5.905e-08
15-150 3.124e-07 6.805e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.50150 (-3.1882 2.06807)
R1^2/D10^2 : 3.39083 (-1.67926 11.0578)
kT2 [keV] : 31.6231 (-14.5021 109.742)
R2^2/D10^2 : 1.95366E-02 (-0.018574 0.173393)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.31 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.21e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.915e-08 1.785e-08
25- 50 1.082e-07 3.394e-08
50-150 1.573e-07 7.219e-08
15-150 3.147e-07 1.157e-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: 1.91282 ( -0.154892 0.160385 )
Norm@50keV : 1.71398E-02 ( -0.00173832 0.00171168 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.65e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 4 sec: 2.47324 ( -0.223581 0.223866 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.30404e-07 ( -6.24452e-08 6.29908e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.32921 ( -0.83999 0.674668 )
Epeak [keV] : 51.2661 ( -16.2367 -51.2738 )
Norm@50keV : 3.60460E-02 ( -0.0195227 0.0694103 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.97e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 4 sec: 2.42026 ( -0.23345 0.23263 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.01748e-07 ( -7.1708e-08 7.1768e-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) = 1.85e-07
S(50-100 keV) = 1.96e-07
T90 vs. Hardness ratio plot
T90 = 4 sec.
Hardness ratio (energy fluence ratio) = 1.05946
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.36338
Count Ratio (50-100 keV) / (15-25 keV) = 0.73076
Mask shadow pattern
IMX = -1.020694682050474E+00, IMY = -8.981749307703840E-02
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:
-239.832000 -0.832000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4511 35.4599 7.6 32.8 -39.9 -0.5320 -1.5 7.1 Her X-1
337.2244 64.9205 2.8 47.9 -129.2 5.1747 4.2 ------ UNKNOWN
350.9000 65.0983 3.1 51.0 -135.6 4.7603 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.832000 3.168000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.2947 35.3735 5.9 32.8 -39.7 0.0683 1.9 8.2 Her X-1
175.6420 32.4063 2.7 39.1 87.6 0.4736 4.3 ------ UNKNOWN
97.5571 68.7133 0.6 45.7 175.0 1.1413 18.8 ------ UNKNOWN
345.0177 65.1491 2.1 49.6 -132.9 0.6802 5.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
81.868600 508.168600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6587 22.0145 1.5 47.5 167.6 8.0516 7.5 1.4 Crab
188.7156 43.7285 2.4 50.3 39.9 7.7691 4.8 ------ UNKNOWN
194.3322 78.1325 3.7 25.4 -1.7 1.2537 3.1 ------ UNKNOWN
245.0676 50.3562 3.2 58.5 -6.4 10.3493 3.7 ------ UNKNOWN
56.2236 17.7366 3.0 57.1 -161.5 7.1506 3.8 ------ UNKNOWN
42.8104 24.0486 3.9 55.2 -144.8 9.3603 3.0 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:14:55 EDT 2022