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
57.1850 45.0796 0.0135 43.2889 -43.9085 1.7572994 14.223 TRIG_01046014
Foreground time interval of the image:
-2.720 14.596 (delta_t = 17.316 [sec])
Background time interval of the image:
-239.800 -2.720 (delta_t = 237.080 [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 -2.720 sec. to 14.596 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.13577 ( -0.202319 0.216718 )
Norm@50keV : 6.08207E-03 ( -0.000877248 0.000855618 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 75.86 using 59 bins.
Reduced chi-squared = 1.33088
# Null hypothesis probability of 4.82e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 17.32 sec: 0.974201 ( -0.107926 0.107999 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.82602e-07 ( -1.25311e-07 1.27462e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.720 sec. to 14.596 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.23766 ( -1.29545 0.7147 )
Epeak [keV] : 34.6986 ( -30.2825 13.673 )
Norm@50keV : 2.03189E-02 ( -0.0203321 0.099852 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.36 using 59 bins.
Reduced chi-squared = 1.31
# Null hypothesis probability of 5.97e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 17.32 sec: 0.943504 ( -0.113412 0.112946 ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from -2.720 sec. to 14.596 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] : 9.41518 (-1.07864 1.20812)
R^2/D10^2 : 0.569705 (-0.216084 0.350195)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 82.90 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.41e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.740e-07 3.140e-08
25- 50 3.963e-07 6.019e-08
50-150 1.733e-07 5.318e-08
15-150 7.436e-07 1.033e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 53.5352 (-13.772 21.8016)
Norm : 5.33639 (-0.933319 1.20743)
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.35 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.12e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.293e-07 3.265e-08
25- 50 3.373e-07 4.261e-08
50-150 3.487e-07 1.020e-07
15-150 9.153e-07 1.347e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.43068 (-6.72557 1.84092)
R1^2/D10^2 : 1.19298 (-0.623973 0.896979)
kT2 [keV] : 25.4088 (-24.9429 -25.6616)
R2^2/D10^2 : 5.74010E-03 (-0.00547235 0.54473)
------------------------------------------------------------
#Fit statistic : Chi-Squared 74.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.22e-02 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.052e-07 6.640e-08
25- 50 3.610e-07 1.315e-07
50-150 3.629e-07 2.007e-07
15-150 9.291e-07 3.638e-07
Peak spectrum fit
Power-law model
Time interval is from 1.140 sec. to 2.140 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.82624 ( -0.387163 0.424705 )
Norm@50keV : 1.35457E-02 ( -0.00361252 0.00347684 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.64 using 59 bins.
Reduced chi-squared = 0.870877
# Null hypothesis probability of 7.45e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.88600 ( -0.44534 0.44601 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.24626e-07 ( -3.26171e-08 3.32187e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.140 sec. to 2.140 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36690 ( -1.95229 0.858121 )
Epeak [keV] : 65.0526 ( -54.3238 -65.0527 )
Norm@50keV : 2.39278E-02 ( -0.0239279 0.249586 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.33 using 59 bins.
Reduced chi-squared = 0.880893
# Null hypothesis probability of 7.24e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.86449 ( -0.45187 0.45111 ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Band function
Time interval is from 1.140 sec. to 2.140 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] : 12.1619 (-3.17923 4.19324)
R^2/D10^2 : 0.436900 (-0.292599 0.899623)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.07 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.86e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.368e-08 7.330e-09
25- 50 4.374e-08 1.960e-08
50-150 3.924e-08 2.423e-08
15-150 9.666e-08 4.204e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 99.2813 (-51.8443 -99.2813)
Norm : 8.40586 (-2.37392 3.42757)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.55e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.197e-08 9.387e-09
25- 50 3.793e-08 2.185e-08
50-150 6.122e-08 4.722e-08
15-150 1.211e-07 6.715e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.00467 (-2.70532 6.07898)
R1^2/D10^2 : 7.68299 (-7.15534 306.609)
kT2 [keV] : 18.8742 (-7.04862 76.2898)
R2^2/D10^2 : 6.78907E-02 (-0.0673178 0.368878)
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.93e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.352e-08 1.406e-08
25- 50 3.509e-08 1.852e-08
50-150 6.014e-08 3.682e-08
15-150 1.188e-07 6.420e-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: 2.13577 ( -0.202319 0.216718 )
Norm@50keV : 6.08207E-03 ( -0.000877248 0.000855618 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 75.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.82e-02 with 57 degrees of freedom
Photon flux (15-150 keV) in 17.32 sec: 0.974102 ( -0.107903 0.107997 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.82404e-07 ( -1.25253e-07 1.27501e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.23750 ( -1.29539 0.714774 )
Epeak [keV] : 34.6994 ( -25.741 13.6806 )
Norm@50keV : 2.03233E-02 ( -0.0203324 0.0998518 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 73.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.97e-02 with 56 degrees of freedom
Photon flux (15-150 keV) in 17.32 sec: 0.943299 ( -0.113362 0.112891 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.08935e-07 ( -1.39866e-07 1.4889e-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) = 3.07e-07
S(50-100 keV) = 2.79e-07
T90 vs. Hardness ratio plot
T90 = 13.9319999217987 sec.
Hardness ratio (energy fluence ratio) = 0.908795
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.22401
Count Ratio (50-100 keV) / (15-25 keV) = 0.491054
Mask shadow pattern
IMX = 6.786525965272134E-01, IMY = 6.532748814989496E-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:
-239.800000 -2.720000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6310 22.0200 0.4 20.1 -88.5 9.4840 29.9 0.4 Crab
136.4962 64.5692 3.1 44.2 24.8 2.1012 3.7 ------ UNKNOWN
117.3044 -30.4425 2.7 56.8 173.9 7.3733 4.3 ------ UNKNOWN
99.7653 50.4001 3.4 25.5 -2.1 1.0129 3.4 ------ UNKNOWN
54.7986 51.2614 2.3 46.2 -35.8 3.3148 5.1 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.720000 14.596000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5161 21.8394 0.0 20.3 -88.9 -0.0728 -1.1 12.4 Crab
83.8631 -2.6838 2.7 34.8 -134.0 0.3405 4.2 ------ UNKNOWN
57.1850 45.0797 0.8 43.3 -43.9 1.7577 14.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
255.100600 650.387900
660.200000 710.857600
720.200000 776.160000
780.200000 962.221600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
180.0139 7.5062 2.6 40.7 96.4 8.7519 4.4 ------ UNKNOWN
215.2017 44.4250 2.9 52.2 29.9 10.0752 4.0 ------ UNKNOWN
250.8866 83.8877 2.7 57.3 -20.2 9.4792 4.3 ------ UNKNOWN
122.2258 76.3084 2.2 43.4 -35.5 5.1234 5.2 ------ UNKNOWN
98.1458 14.6170 2.4 47.9 -129.2 11.3471 4.8 ------ UNKNOWN
Plot creation:
Sat Jul 30 07:03:17 EDT 2022