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
166.7769 36.5038 0.0230 49.6989 -144.9846 1.7724579 8.371 TRIG_01173731
Foreground time interval of the image:
-0.264 16.968 (delta_t = 17.232 [sec])
Background time interval of the image:
-208.835 -0.264 (delta_t = 208.571 [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 2.048000
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 2.048000
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 2.048000
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 -0.264 sec. to 16.968 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.17664 ( -0.31082 0.298174 )
Norm@50keV : 6.93141E-03 ( -0.0011809 0.00117099 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 34.38 using 59 bins.
Reduced chi-squared = 0.603158
# Null hypothesis probability of 9.92e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 17.23 sec: 0.811035 ( -0.146431 0.14784 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21993e-06 ( -2.11827e-07 2.12473e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.264 sec. to 16.968 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.15555 ( -2.14147 3.13715 )
Epeak [keV] : 55.4589 ( )
Norm@50keV : 1.05589E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 33.30 using 59 bins.
Reduced chi-squared = 0.594643
# Null hypothesis probability of 9.93e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 17.23 sec: 0.810418 ( -0.156731 0.148253 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21783e-06 ( -2.19793e-07 2.13621e-07 ) ergs/cm2
Band function
Time interval is from -0.264 sec. to 16.968 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] : 20.9869 (-4.02045 5.67655)
R^2/D10^2 : 3.20589E-02 (-0.0174793 0.0333717)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 40.42 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.53e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.598e-08 1.672e-08
25- 50 2.362e-07 7.896e-08
50-150 7.755e-07 2.321e-07
15-150 1.058e-06 2.791e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-52.7411 -200)
Norm : 3.46833 (-0.591178 0.591178)
------------------------------------------------------------
#Fit statistic : Chi-Squared 39.49 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.63e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.489e-07 8.579e-08
25- 50 2.864e-07 1.640e-07
50-150 6.282e-07 3.552e-07
15-150 1.064e-06 6.117e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.90266 (-1.5505 5.05217)
R1^2/D10^2 : 36.0807 (-35.8626 13903)
kT2 [keV] : 23.7328 (-5.04018 -23.7334)
R2^2/D10^2 : 2.05119E-02 (-0.0168735 0.0250664)
------------------------------------------------------------
#Fit statistic : Chi-Squared 33.92 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.89e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.299e-07 6.317e-08
25- 50 2.083e-07 7.375e-08
50-150 8.236e-07 3.185e-07
15-150 1.162e-06 4.466e-07
Peak spectrum fit
Power-law model
Time interval is from 0.924 sec. to 1.924 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.29563 ( -0.355852 0.352483 )
Norm@50keV : 2.25240E-02 ( -0.0049028 0.00489841 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.03 using 59 bins.
Reduced chi-squared = 1.17596
# Null hypothesis probability of 1.71e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.68525 ( -0.615 0.62367 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.22828e-07 ( -5.05261e-08 5.09068e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.924 sec. to 1.924 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.64305 ( -4.82659 2.26041 )
Epeak [keV] : 73.6551 ( -13.9022 47.5646 )
Norm@50keV : 0.367729 ( -0.371797 18.3521 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.30 using 59 bins.
Reduced chi-squared = 1.09464
# Null hypothesis probability of 2.92e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.27455 ( -0.66997 0.69601 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.00106e-07 ( -5.29595e-08 5.48587e-08 ) ergs/cm2
Band function
Time interval is from 0.924 sec. to 1.924 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] : 19.0290 (-3.59469 4.6899)
R^2/D10^2 : 0.152241 (-0.0807742 0.158739)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.30e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.083e-08 5.372e-09
25- 50 5.215e-08 2.040e-08
50-150 1.388e-07 6.122e-08
15-150 2.018e-07 6.735e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-83.2803 -199.363)
Norm : 11.4485 (-2.49445 2.49457)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.45 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.62e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.851e-08 1.677e-08
25- 50 5.484e-08 3.174e-08
50-150 1.203e-07 6.930e-08
15-150 2.036e-07 1.177e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.10001 (-2.0725 22.0705)
R1^2/D10^2 : 578.098 (-707.403 -707.403)
kT2 [keV] : 19.6123 (-3.82085 5.02983)
R2^2/D10^2 : 0.135133 (-0.13601 0.106085)
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.98e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.819e-08 9.023e-09
25- 50 4.992e-08 2.596e-08
50-150 1.411e-07 6.888e-08
15-150 2.092e-07 8.282e-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: 1.17664 ( -0.31082 0.298174 )
Norm@50keV : 6.93141E-03 ( -0.0011809 0.00117099 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 34.38 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.92e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 17.23 sec: 0.811026 ( -0.146419 0.147837 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21979e-06 ( -2.11777e-07 2.12844e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.26860 ( -2.23881 5.01411 )
Epeak [keV] : 92.4865 ( )
Norm@50keV : 9.38301E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 33.26 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.93e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 17.23 sec: 0.810710 ( -0.156459 0.147795 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.21808e-06 ( -2.18642e-07 2.14224e-07 ) 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) = 2.53e-07
S(50-100 keV) = 4.46e-07
T90 vs. Hardness ratio plot
T90 = 16.2560000419617 sec.
Hardness ratio (energy fluence ratio) = 1.76285
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.57773
Count Ratio (50-100 keV) / (15-25 keV) = 1.80177
Mask shadow pattern
IMX = -9.656927480165931E-01, IMY = 6.765720113939392E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 2.048000
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:
-208.835400 -0.264000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.2692 35.4208 28.9 18.6 44.1 -0.2750 -0.4 10.3 Her X-1
299.5501 35.2386 5.6 50.1 7.1 2.5278 2.0 3.0 Cyg X-1
308.2022 40.7859 0.0 53.0 -3.5 0.8549 0.7 10.8 Cyg X-3
303.2599 29.3670 2.3 56.1 10.9 13.2213 5.0 ------ UNKNOWN
263.9029 42.6526 2.3 22.0 15.5 3.1977 4.9 ------ UNKNOWN
210.6405 50.6148 3.0 16.2 -131.3 2.2740 3.9 ------ UNKNOWN
163.0248 41.3799 2.6 49.7 -137.5 10.7328 4.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.264000 16.968000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3207 35.1792 4.4 18.7 44.6 0.1781 2.6 11.9 Her X-1
299.5252 35.1182 10.5 50.2 7.2 -0.1801 -1.1 5.9 Cyg X-1
308.3139 40.9493 5.3 53.0 -3.8 -0.3720 -2.2 9.2 Cyg X-3
182.4943 22.3064 2.1 47.0 -171.2 0.6598 5.4 ------ UNKNOWN
166.7769 36.5038 1.4 49.7 -145.0 1.7727 8.4 ------ UNKNOWN
318.8484 71.3689 2.0 46.5 -43.7 1.0780 5.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
270.364590 962.386000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.6541 35.4078 191.9 35.4 165.5 0.0996 0.1 10.4 Her X-1
268.3816 -1.5543 11.9 40.2 99.8 -3.0200 -1.0 6.2 SW J1753.5-0127
288.7593 10.7923 14.1 19.2 76.1 -1.1711 -0.8 9.5 GRS 1915+105
299.5790 35.2334 1.5 7.2 -102.2 8.3899 7.9 2.0 Cyg X-1
308.1887 41.0204 4.6 15.8 -90.4 3.0563 2.5 5.4 Cyg X-3
326.1555 38.4885 9.8 26.8 -65.4 1.7547 1.2 10.0 Cyg X-2
280.4666 0.8434 3.1 31.6 84.7 8.3882 3.7 ------ UNKNOWN
239.3151 44.3668 3.2 47.1 179.3 10.3638 3.6 ------ UNKNOWN
229.2214 54.2839 2.7 53.7 -167.9 14.7862 4.3 ------ UNKNOWN
Plot creation:
Sat Sep 30 00:49:22 EDT 2023