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
97.6173 9.5473 0.0038 1.4259 -54.0754 3.3173963 50.244 TRIG_01104692
Foreground time interval of the image:
-6.532 11.877 (delta_t = 18.409 [sec])
Background time interval of the image:
-239.024 -6.532 (delta_t = 232.492 [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 -6.532 sec. to 94.604 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25005 ( -0.0207862 0.0206947 )
Norm@50keV : 4.31055E-02 ( -0.00054605 0.000544778 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 22.58 using 59 bins.
Reduced chi-squared = 0.39614
# Null hypothesis probability of 1.00e+00 with 57 degrees of freedom
Photon flux (15-150 keV) in 101.1 sec: 5.09829 ( -0.07444 0.07468 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.36186e-05 ( -4.8047e-07 4.80661e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -6.532 sec. to 94.604 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.16069 ( -0.0867215 0.0432498 )
Epeak [keV] : 635.164 ( -275.558 7084.34 )
Norm@50keV : 4.65144E-02 ( -0.00302791 0.00349053 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 19.41 using 59 bins.
Reduced chi-squared = 0.346607
# Null hypothesis probability of 1.00e+00 with 56 degrees of freedom
Photon flux (15-150 keV) in 101.1 sec: 2.89154 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 4.35412e-05 ( -4.85492e-07 4.85966e-07 ) ergs/cm2
Band function
Time interval is from -6.532 sec. to 94.604 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] : 24.1766 ( )
R^2/D10^2 : 0.121331 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 1493.52 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.03e-275 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.267e-06 3.084e-08
25- 50 7.067e-06 1.426e-07
50-150 3.075e-05 3.892e-07
15-150 3.909e-05 4.145e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 23.3728 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 1011.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.17e-174 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.884e-06 7.633e-08
25- 50 1.132e-05 1.618e-07
50-150 2.482e-05 3.538e-07
15-150 4.203e-05 5.561e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.08913 (-0.448744 0.469033)
R1^2/D10^2 : 1.83594 (-0.279959 0.341699)
kT2 [keV] : 36.4050 (-1.48374 1.7085)
R2^2/D10^2 : 2.66063E-02 (-0.00380842 0.00407539)
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.19 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.33e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.492e-06 1.628e-07
25- 50 9.732e-06 2.128e-07
50-150 3.010e-05 4.499e-07
15-150 4.333e-05 7.128e-07
Peak spectrum fit
Power-law model
Time interval is from 42.004 sec. to 43.004 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.12826 ( -0.0362801 0.0361994 )
Norm@50keV : 0.254136 ( -0.00511212 0.00510877 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.39 using 59 bins.
Reduced chi-squared = 0.936667
# Null hypothesis probability of 6.11e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.18494 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.63384e-06 ( -5.56792e-08 5.57743e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 42.004 sec. to 43.004 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.928372 ( -0.149351 0.14476 )
Epeak [keV] : 319.371 ( -110.05 610.777 )
Norm@50keV : 0.309343 ( -0.0401516 0.0475518 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.80 using 59 bins.
Reduced chi-squared = 0.853571
# Null hypothesis probability of 7.74e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 29.2354 ( -0.6645 0.6661 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.61228e-06 ( -5.82853e-08 5.80811e-08 ) ergs/cm2
Band function
Time interval is from 42.004 sec. to 43.004 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] : 21.3608 ( )
R^2/D10^2 : 1.11713 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 468.55 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.22e-66 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.559e-08 3.890e-09
25- 50 4.966e-07 1.545e-08
50-150 1.691e-06 5.650e-08
15-150 2.283e-06 5.600e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 125.070 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 458.00 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.48e-64 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.114e-07 6.550e-09
25- 50 5.991e-07 1.385e-08
50-150 1.314e-06 2.750e-08
15-150 2.224e-06 4.800e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.09553 (-0.834373 0.902676)
R1^2/D10^2 : 9.82391 (-2.33535 3.31234)
kT2 [keV] : 35.9241 (-3.11996 4.22317)
R2^2/D10^2 : 0.176552 (-0.0528582 0.061991)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.49e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.908e-07 1.400e-08
25- 50 5.528e-07 2.405e-08
50-150 1.873e-06 9.400e-08
15-150 2.617e-06 1.205e-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: 0.492885 ( -0.0611073 0.0598754 )
Norm@50keV : 1.03890E-02 ( -0.000388709 0.000385277 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.48 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.50e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 18.41 sec: 1.23185 ( -0.0400652 0.0401201 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.57891e-06 ( -8.24254e-08 8.24737e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.224053 ( -0.258549 0.199355 )
Epeak [keV] : 445.991 ( -182.425 2524.57 )
Norm@50keV : 1.30445E-02 ( -0.00236372 0.00305753 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.31e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 18.41 sec: 1.22059 ( -0.04119 0.04129 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.56956e-06 ( -8.40601e-08 8.37839e-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) = 9.43e-06
S(50-100 keV) = 1.59e-05
T90 vs. Hardness ratio plot
T90 = 43.1439999341965 sec.
Hardness ratio (energy fluence ratio) = 1.68611
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.56676
Count Ratio (50-100 keV) / (15-25 keV) = 1.44028
Mask shadow pattern
IMX = 1.460439315182145E-02, IMY = 2.015692605363580E-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:
-239.024000 -6.532000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6409 22.0072 0.5 19.7 -61.6 9.1072 21.8 0.6 Crab
111.9841 -41.6754 2.2 51.6 150.3 7.9774 5.2 ------ UNKNOWN
66.1897 23.5245 3.1 34.4 -77.0 2.2535 3.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-6.532000 11.876600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5159 21.8904 6.3 19.7 -62.1 0.1445 1.8 9.9 Crab
109.7267 -38.2462 2.0 47.8 151.2 1.2217 5.7 ------ UNKNOWN
101.7909 3.9787 2.7 5.5 126.5 0.2664 4.2 ------ UNKNOWN
113.9821 46.8139 2.5 40.6 -0.6 0.4829 4.7 ------ UNKNOWN
97.6173 9.5473 0.2 1.4 -54.1 3.3176 50.2 ------ UNKNOWN
59.6153 -32.7422 2.8 55.3 -156.9 1.1073 4.1 ------ UNKNOWN
58.9294 26.5201 2.2 41.6 -76.0 1.4141 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
35.676600 937.576590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6307 22.0225 0.6 18.3 -56.9 33.1483 20.3 0.5 Crab
117.6768 42.5179 2.7 37.4 13.1 9.1175 4.3 ------ UNKNOWN
97.1423 -26.6672 2.9 36.2 169.2 7.8742 3.9 ------ UNKNOWN
110.5160 45.3427 2.6 37.5 3.4 9.2055 4.4 ------ UNKNOWN
103.6978 32.2690 3.0 23.4 1.5 5.8098 3.9 ------ UNKNOWN
97.5825 9.5710 0.4 0.1 -45.2 44.0944 31.7 ------ UNKNOWN
106.0851 49.8342 2.6 40.9 -3.2 9.0452 4.5 ------ UNKNOWN
79.7488 64.6117 2.5 56.5 -20.6 19.9721 4.7 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:00:16 EDT 2022