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
104.2879 1.0771 0.0088 43.9080 130.4633 16.5468550 21.779 TRIG_01212898
Foreground time interval of the image:
-14.656 8.960 (delta_t = 23.616 [sec])
Background time interval of the image:
-99.187 -14.656 (delta_t = 84.531 [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
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
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 -14.656 sec. to 8.960 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.81078 ( -0.0618978 0.0623897 )
Norm@50keV : 4.51915E-02 ( -0.00163687 0.00163387 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.56 using 59 bins.
Reduced chi-squared = 1.09754
# Null hypothesis probability of 2.86e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 23.62 sec: 6.25385 ( -0.24021 0.24087 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.82472e-06 ( -3.5995e-07 3.60727e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -14.656 sec. to 8.960 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.22809 ( -0.281937 0.265637 )
Epeak [keV] : 67.6972 ( -8.12842 16.1649 )
Norm@50keV : 8.75511E-02 ( -0.0222998 0.0322389 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.62 using 59 bins.
Reduced chi-squared = 0.850357
# Null hypothesis probability of 7.80e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 23.62 sec: 6.03942 ( -0.25598 0.25698 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.49708e-06 ( -3.91244e-07 3.90722e-07 ) ergs/cm2
Band function
Time interval is from -14.656 sec. to 8.960 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] : 13.5915 ( )
R^2/D10^2 : 0.933950 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 201.71 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.76e-18 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.628e-07 6.177e-08
25- 50 3.114e-06 1.287e-07
50-150 3.730e-06 2.504e-07
15-150 7.707e-06 2.752e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 113.143 (-15.8364 15.1145)
Norm : 26.4057 (-1.24742 1.64027)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.99e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.628e-06 1.161e-07
25- 50 2.882e-06 1.453e-07
50-150 4.993e-06 1.189e-06
15-150 9.502e-06 1.293e-06
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.00481 (-0.914516 0.975283)
R1^2/D10^2 : 6.85338 (-2.39291 4.32178)
kT2 [keV] : 22.4882 (-2.51476 3.54813)
R2^2/D10^2 : 0.104024 (-0.0472081 0.0678921)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.65 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.04e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.505e-06 1.749e-07
25- 50 2.970e-06 2.480e-07
50-150 4.899e-06 6.283e-07
15-150 9.373e-06 8.810e-07
Peak spectrum fit
Power-law model
Time interval is from 0.084 sec. to 1.084 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.67220 ( -0.0998458 0.10162 )
Norm@50keV : 0.163778 ( -0.0113121 0.0112749 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.85 using 59 bins.
Reduced chi-squared = 1.17281
# Null hypothesis probability of 1.75e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 21.5454 ( -1.4837 1.485 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.5202e-06 ( -1.08865e-07 1.09171e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.084 sec. to 1.084 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.539888 ( -0.516287 0.466317 )
Epeak [keV] : 66.1516 ( -7.82397 13.308 )
Norm@50keV : 0.610899 ( -0.250532 0.482363 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.60 using 59 bins.
Reduced chi-squared = 0.85
# Null hypothesis probability of 7.80e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 21.1589 ( -1.4968 1.4979 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.48754e-06 ( -1.1163e-07 1.11908e-07 ) ergs/cm2
Band function
Time interval is from 0.084 sec. to 1.084 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] : 14.5304 (-0.995503 1.05497)
R^2/D10^2 : 2.89818 (-0.660715 0.851402)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.30 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.21e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.287e-07 1.415e-08
25- 50 4.964e-07 3.915e-08
50-150 7.029e-07 7.875e-08
15-150 1.328e-06 1.025e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 143.138 (-32.198 44.0432)
Norm : 90.9498 (-6.96895 8.04841)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.80 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.58e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.345e-07 2.090e-08
25- 50 4.316e-07 4.355e-08
50-150 8.353e-07 2.632e-07
15-150 1.501e-06 3.000e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.25266 (-1.61694 2.13289)
R1^2/D10^2 : 27.3683 (-16.2294 52.9844)
kT2 [keV] : 19.3090 (-2.43715 4.08207)
R2^2/D10^2 : 0.816790 (-0.474545 0.80426)
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.69e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.100e-07 7.333e-08
25- 50 4.534e-07 1.079e-07
50-150 8.133e-07 1.892e-07
15-150 1.477e-06 3.384e-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: 1.81078 ( -0.0618978 0.0623897 )
Norm@50keV : 4.51915E-02 ( -0.00163687 0.00163387 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.56 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.86e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 23.62 sec: 6.25347 ( -0.240138 0.240884 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.82327e-06 ( -3.6017e-07 3.60614e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.22809 ( -0.281937 0.265637 )
Epeak [keV] : 67.6972 ( -8.12842 16.1649 )
Norm@50keV : 8.75511E-02 ( -0.0222998 0.0322389 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 47.62 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.80e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 23.62 sec: 6.03844 ( -0.25586 0.25729 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.50011e-06 ( -3.91832e-07 3.90462e-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) = 2.79e-06
S(50-100 keV) = 3.17e-06
T90 vs. Hardness ratio plot
T90 = 16.3040000200272 sec.
Hardness ratio (energy fluence ratio) = 1.1362
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.42625
Count Ratio (50-100 keV) / (15-25 keV) = 0.902766
Mask shadow pattern
IMX = -6.246842340291677E-01, IMY = -7.323611388375612E-01
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
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:
-99.187410 -14.656000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7410 22.0885 0.6 16.9 153.5 3.6714 19.4 7.5 Crab
101.2645 3.4215 2.9 40.4 132.8 2.0682 4.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-14.656000 8.960000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6162 21.8654 7.6 17.1 154.1 -0.1840 -1.5 9.0 Crab
104.2879 1.0771 0.5 43.9 130.5 16.5535 21.2 ------ UNKNOWN
129.4704 40.8221 2.9 38.2 58.2 1.8150 4.0 ------ UNKNOWN
108.7048 13.2557 2.8 36.3 114.1 1.5824 4.1 ------ UNKNOWN
167.9879 74.4306 2.6 52.8 7.8 1.6620 4.5 ------ UNKNOWN
34.5840 17.3217 2.9 44.2 -117.7 1.2929 4.0 ------ UNKNOWN
32.5594 23.0644 2.5 42.4 -109.3 1.4309 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
123.812590 962.643200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6324 22.0247 0.6 28.9 -15.3 32.5288 20.9 0.6 Crab
135.5177 -40.5552 1.1 50.5 175.9 43.8975 11.0 0.5 Vela X-1
130.1627 20.7151 3.3 32.1 77.3 11.3498 3.5 ------ UNKNOWN
113.5369 22.8569 3.7 23.6 48.9 5.4606 3.1 ------ UNKNOWN
80.8218 51.4536 2.3 54.1 9.1 25.4807 4.9 ------ UNKNOWN
Plot creation:
Sat Mar 9 15:15:23 EST 2024