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
61.9103 65.1482 0.0176 31.3518 85.3135 0.2455157 10.930 TRIG_00998907
Foreground time interval of the image:
-0.008 0.548 (delta_t = 0.556 [sec])
Background time interval of the image:
-65.291 -0.008 (delta_t = 65.283 [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 0.512000
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 0.512000
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 0.512000
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 -0.008 sec. to 0.548 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.42397 ( -0.244088 0.244638 )
Norm@50keV : 2.39932E-02 ( -0.00399338 0.00398172 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.37 using 59 bins.
Reduced chi-squared = 1.1293
# Null hypothesis probability of 2.34e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.556 sec: 2.93831 ( -0.4907 0.49153 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.28299e-07 ( -2.29055e-08 2.31074e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.008 sec. to 0.548 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.400334 ( -1.80431 1.28481 )
Epeak [keV] : 62.4757 ( -13.1064 40.669 )
Norm@50keV : 0.221521 ( -0.221653 1.78347 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.88 using 59 bins.
Reduced chi-squared = 1.03357
# Null hypothesis probability of 4.06e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.556 sec: 2.84932 ( -0.49707 0.4983 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.15485e-07 ( -2.39226e-08 2.5138e-08 ) ergs/cm2
Band function
Time interval is from -0.008 sec. to 0.548 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] : 14.4475 (-2.22069 2.74264)
R^2/D10^2 : 0.426232 (-0.198966 0.344651)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.93e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.041e-08 3.481e-09
25- 50 3.994e-08 8.393e-09
50-150 5.576e-08 1.783e-08
15-150 1.061e-07 2.541e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.362 (-84.3168 -199.363)
Norm : 12.3124 (-2.00513 2.00787)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.87 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.76e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.705e-08 9.891e-09
25- 50 3.279e-08 1.858e-08
50-150 7.192e-08 4.050e-08
15-150 1.218e-07 7.000e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 12.6759 (-11.9149 3.08577)
R1^2/D10^2 : 0.616650 (-0.31353 4.22822)
kT2 [keV] : 200.000 (-200 -200)
R2^2/D10^2 : 1.92024E-04 (-0.000188093 0.00231436)
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.20e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.191e-08 6.177e-09
25- 50 4.022e-08 1.873e-08
50-150 6.838e-08 3.543e-08
15-150 1.205e-07 5.326e-08
Peak spectrum fit
Power-law model
Time interval is from -0.230 sec. to 0.770 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.49865 ( -0.236243 0.240385 )
Norm@50keV : 1.72052E-02 ( -0.00286471 0.00284735 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.75 using 59 bins.
Reduced chi-squared = 1.27632
# Null hypothesis probability of 7.80e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.14716 ( -0.34649 0.34684 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.63271e-07 ( -2.9115e-08 2.95392e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.230 sec. to 0.770 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.37334 ( -2.37601 1.58291 )
Epeak [keV] : 52.9620 ( -7.7439 9.60793 )
Norm@50keV : 0.610603 ( -0.673718 11.394 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.98 using 59 bins.
Reduced chi-squared = 1.07107
# Null hypothesis probability of 3.34e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.02157 ( -0.34777 0.3512 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.36842e-07 ( -2.6579e-08 2.99672e-08 ) ergs/cm2
Band function
Time interval is from -0.230 sec. to 0.770 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] : 13.4830 (-1.80057 2.1503)
R^2/D10^2 : 0.400809 (-0.167998 0.269147)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.06 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.65e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.543e-08 4.020e-09
25- 50 5.525e-08 1.162e-08
50-150 6.483e-08 2.177e-08
15-150 1.355e-07 2.629e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 179.766 (-85.434 -179.766)
Norm : 9.00478 (-1.45692 1.6375)
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.71 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.20e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.271e-08 1.278e-08
25- 50 4.314e-08 2.307e-08
50-150 9.131e-08 5.145e-08
15-150 1.572e-07 8.655e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 198.780 (-198.784 -198.784)
R1^2/D10^2 : 6.74348E-05 (-6.74307e-05 0.631959)
kT2 [keV] : 12.8378 (-8.49243 2.48663)
R2^2/D10^2 : 0.458048 (-0.146565 3.44719)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.48 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.16e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.579e-08 3.843e-06
25- 50 5.497e-08 3.538e-05
50-150 6.622e-08 8.230e-04
15-150 1.370e-07 8.760e-04
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: 1.42397 ( -0.244088 0.244638 )
Norm@50keV : 2.39932E-02 ( -0.00399338 0.00398172 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.37 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.34e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 0.556 sec: 2.93825 ( -0.490683 0.491507 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.28284e-07 ( -2.28995e-08 2.31225e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.399738 ( -1.8045 1.28462 )
Epeak [keV] : 62.4850 ( -13.1072 40.6726 )
Norm@50keV : 0.221337 ( -0.221648 1.78354 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.06e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 0.556 sec: 2.84913 ( -0.497 0.49816 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.15523e-07 ( -2.39347e-08 2.51618e-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) = 3.05e-08
S(50-100 keV) = 4.55e-08
T90 vs. Hardness ratio plot
T90 = 0.491999864578247 sec.
Hardness ratio (energy fluence ratio) = 1.4918
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 2.25739
Count Ratio (50-100 keV) / (15-25 keV) = 1.56145
Mask shadow pattern
IMX = 4.977743143023378E-02, IMY = -6.072106334266935E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.512000
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:
-65.291320 -0.008000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
104.9906 23.7817 2.7 52.4 13.1 1.5217 4.2 ------ UNKNOWN
245.6056 62.1918 2.5 36.1 -168.9 0.6364 4.6 ------ UNKNOWN
250.7487 46.3380 2.4 51.1 -160.5 1.4684 4.8 ------ UNKNOWN
134.4238 11.2332 3.1 58.7 -23.5 2.6169 3.8 ------ UNKNOWN
223.2383 38.0551 3.1 49.1 -132.0 2.0452 3.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.008000 0.548000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
61.9104 65.1482 1.1 31.4 85.3 0.2455 10.9 ------ UNKNOWN
206.6489 59.4624 2.9 25.5 -137.6 0.0479 4.0 ------ UNKNOWN
167.0389 26.4521 2.4 43.9 -63.8 0.1830 4.8 ------ UNKNOWN
224.4385 37.8204 3.0 49.8 -133.0 0.1699 3.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
68.308580 718.643400
720.208000 962.285900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6155 22.0098 0.4 45.4 7.1 34.6127 27.2 1.0 Crab
86.0569 12.2190 3.1 55.5 6.9 10.8455 3.7 ------ UNKNOWN
297.0647 57.2654 2.6 50.7 -179.1 9.7784 4.4 ------ UNKNOWN
93.1301 14.1512 3.0 55.2 -1.8 8.5225 3.9 ------ UNKNOWN
74.7586 61.5401 3.3 6.8 -27.8 2.9325 3.5 ------ UNKNOWN
121.7474 48.6130 4.2 34.9 -55.5 4.0195 2.7 ------ UNKNOWN
121.1820 29.5813 2.8 50.6 -39.4 11.4508 4.2 ------ UNKNOWN
123.3287 28.3711 3.1 52.5 -40.8 14.4027 3.7 ------ UNKNOWN
Plot creation:
Thu Oct 20 00:46:53 EDT 2022