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
218.1402 61.2893 0.0157 29.5707 -105.4347 0.5277579 12.179 TRIG_01098132
Foreground time interval of the image:
-0.364 6.564 (delta_t = 6.928 [sec])
Background time interval of the image:
-239.144 -0.364 (delta_t = 238.780 [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 -0.364 sec. to 6.564 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.15355 ( -0.271917 0.299411 )
Norm@50keV : 3.60513E-03 ( -0.000732104 0.000707162 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.88 using 59 bins.
Reduced chi-squared = 0.752281
# Null hypothesis probability of 9.17e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 6.928 sec: 0.582696 ( -0.081823 0.081824 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.33458e-07 ( -4.05907e-08 4.19258e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.364 sec. to 6.564 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.97658 ( )
Epeak [keV] : 5.28272 ( )
Norm@50keV : 4.60262E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.86 using 59 bins.
Reduced chi-squared = 0.765357
# Null hypothesis probability of 9.02e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 6.928 sec: 0.582011 ( -0.081464 0.083493 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.29186e-07 ( -4.36329e-08 4.6445e-08 ) ergs/cm2
Band function
Time interval is from -0.364 sec. to 6.564 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] : 8.32284 (-1.35736 1.62601)
R^2/D10^2 : 0.541107 (-0.273781 0.557761)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.09e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.828e-08 1.405e-08
25- 50 9.040e-08 2.043e-08
50-150 2.699e-08 1.210e-08
15-150 1.657e-07 3.793e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 49.8515 (-16.8611 31.8359)
Norm : 3.29964 (-0.763467 1.10357)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.67 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.03e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.586e-08 1.041e-08
25- 50 8.014e-08 1.456e-08
50-150 7.759e-08 3.304e-08
15-150 2.136e-07 4.822e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.53602 (-2.48069 2.45755)
R1^2/D10^2 : 2.08264 (-1.53831 12.7544)
kT2 [keV] : 19.3212 (-18.4712 -21.8362)
R2^2/D10^2 : 1.20638E-02 (-0.0076477 0.129054)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.57 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.67e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.795e-08 3.277e-08
25- 50 7.283e-08 3.862e-08
50-150 8.445e-08 5.244e-08
15-150 2.152e-07 1.155e-07
Peak spectrum fit
Power-law model
Time interval is from -0.236 sec. to 0.764 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.58891 ( -0.220829 0.225704 )
Norm@50keV : 1.18096E-02 ( -0.00177554 0.00176377 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.58 using 59 bins.
Reduced chi-squared = 0.992632
# Null hypothesis probability of 4.91e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.51247 ( -0.22344 0.22381 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.10614e-07 ( -1.75118e-08 1.76574e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.236 sec. to 0.764 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.136759 ( -1.49525 1.15329 )
Epeak [keV] : 60.0203 ( -10.6977 27.8721 )
Norm@50keV : 9.27983E-02 ( -0.0928 0.426892 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.48 using 59 bins.
Reduced chi-squared = 0.883571
# Null hypothesis probability of 7.18e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.45291 ( -0.22826 0.22853 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.01986e-07 ( -1.77108e-08 1.8451e-08 ) ergs/cm2
Band function
Time interval is from -0.236 sec. to 0.764 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] : 14.1928 (-1.91356 2.19659)
R^2/D10^2 : 0.225472 (-0.0926941 0.153554)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.71e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.581e-09 2.513e-09
25- 50 3.612e-08 8.035e-09
50-150 4.824e-08 1.310e-08
15-150 9.394e-08 1.765e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 164.529 (-72.7864 -163.149)
Norm : 6.33803 (-0.961739 1.17439)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.70 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.00e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.614e-08 8.970e-09
25- 50 3.031e-08 1.649e-08
50-150 6.206e-08 3.602e-08
15-150 1.085e-07 6.105e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.09471 (-6.04491 -6.04491)
R1^2/D10^2 : 1.38157 (-1.39786 -1.39786)
kT2 [keV] : 16.7124 (-3.45051 -16.6925)
R2^2/D10^2 : 0.107070 (-0.107572 0.169659)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.27 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.92e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.309e-08 7.535e-09
25- 50 3.389e-08 1.801e-08
50-150 5.365e-08 3.045e-08
15-150 1.006e-07 5.225e-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: 2.15355 ( -0.271917 0.299411 )
Norm@50keV : 3.60513E-03 ( -0.000732104 0.000707162 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.17e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 6.928 sec: 0.582642 ( -0.0818144 0.0818156 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.33411e-07 ( -4.05674e-08 4.19361e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.95369 ( )
Epeak [keV] : 9.27734 ( )
Norm@50keV : 4.74758E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 42.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 9.01e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 6.928 sec: 0.580269 ( -0.082359 0.083507 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.30172e-07 ( -4.9741e-08 4.46683e-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) = 7.34e-08
S(50-100 keV) = 6.58e-08
T90 vs. Hardness ratio plot
T90 = 6.41999995708466 sec.
Hardness ratio (energy fluence ratio) = 0.896458
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.947227
Count Ratio (50-100 keV) / (15-25 keV) = 0.397278
Mask shadow pattern
IMX = -1.510084145816508E-01, IMY = 5.469381589651889E-01
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:
-239.144000 -0.364000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3785 35.1488 5.9 41.5 -46.9 0.9312 2.0 12.2 Her X-1
173.9007 9.9906 4.0 35.9 117.0 1.6405 2.9 ------ UNKNOWN
244.7998 -1.2003 2.6 51.8 3.7 2.1435 4.4 ------ UNKNOWN
250.5458 19.1225 2.6 44.0 -22.9 1.8042 4.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.364000 6.564000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.5944 35.3215 5.2 41.7 -47.2 -0.1316 -2.2 6.8 Her X-1
139.2371 31.7017 2.2 53.5 167.7 0.5580 5.1 ------ UNKNOWN
218.1401 61.2893 0.9 29.6 -105.4 0.5279 12.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
84.356590 962.922100
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4788 35.3260 8.6 34.6 -10.9 -1.3884 -1.3 1.4 Her X-1
174.1658 37.7594 3.5 35.9 117.0 6.2625 3.3 ------ UNKNOWN
141.7559 44.0709 2.7 46.3 152.3 10.9356 4.3 ------ UNKNOWN
113.5844 45.9776 3.8 56.9 173.9 8.4027 3.0 ------ UNKNOWN
226.5933 44.0077 2.2 18.0 27.4 3.6043 5.2 ------ UNKNOWN
258.7257 12.4865 2.8 56.9 -1.9 9.4539 4.1 ------ UNKNOWN
278.6235 65.7368 2.7 26.2 -78.7 4.1734 4.3 ------ UNKNOWN
276.9083 41.4979 3.0 39.8 -40.6 4.2387 3.9 ------ UNKNOWN
73.7167 57.5390 2.9 58.0 -154.2 18.1437 4.0 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:05:32 EDT 2022