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
91.5918 -28.4033 0.0129 32.7377 84.6852 3.2253790 14.946 TRIG_01093592
Foreground time interval of the image:
14.792 68.152 (delta_t = 53.360 [sec])
Background time interval of the image:
-239.000 14.792 (delta_t = 253.792 [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 14.792 sec. to 68.152 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.85637 ( -0.175494 0.182555 )
Norm@50keV : 3.41335E-03 ( -0.000407733 0.000400489 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.39 using 59 bins.
Reduced chi-squared = 1.07702
# Null hypothesis probability of 3.22e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 53.36 sec: 0.481057 ( -0.048964 0.048982 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.67489e-06 ( -1.98212e-07 2.01122e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 14.792 sec. to 68.152 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.18433 ( -0.840872 0.699248 )
Epeak [keV] : 52.6424 ( -13.8972 -52.6424 )
Norm@50keV : 8.18551E-03 ( -0.00482337 0.0161387 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.73 using 59 bins.
Reduced chi-squared = 1.04875
# Null hypothesis probability of 3.76e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 53.36 sec: 0.470519 ( -0.05021 0.050205 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.57553e-06 ( -2.16697e-07 2.24568e-07 ) ergs/cm2
Band function
Time interval is from 14.792 sec. to 68.152 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] : 11.1033 (-1.35197 1.52377)
R^2/D10^2 : 0.154222 (-0.0590008 0.0968203)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.38e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.124e-07 4.199e-08
25- 50 6.077e-07 7.959e-08
50-150 4.262e-07 1.110e-07
15-150 1.246e-06 1.659e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 85.3638 (-24.3464 43.0438)
Norm : 2.22942 (-0.314871 0.379472)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.76 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.11e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.098e-07 4.704e-08
25- 50 5.178e-07 6.363e-08
50-150 7.627e-07 3.354e-07
15-150 1.590e-06 3.741e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.48826 (-1.37376 1.82688)
R1^2/D10^2 : 1.36728 (-0.857246 2.76193)
kT2 [keV] : 18.1540 (-3.91078 7.73646)
R2^2/D10^2 : 1.82782E-02 (-0.0139276 0.0327637)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.00e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.181e-07 1.654e-07
25- 50 5.060e-07 2.260e-07
50-150 7.291e-07 4.264e-07
15-150 1.553e-06 6.775e-07
Peak spectrum fit
Power-law model
Time interval is from 14.812 sec. to 15.812 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.64085 ( -0.305489 0.324437 )
Norm@50keV : 1.43609E-02 ( -0.00313282 0.00309387 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.43 using 59 bins.
Reduced chi-squared = 1.07772
# Null hypothesis probability of 3.20e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.86961 ( -0.39357 0.39439 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.33712e-07 ( -3.02526e-08 3.05322e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 14.812 sec. to 15.812 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.160401 ( -2.24534 1.47259 )
Epeak [keV] : 62.6202 ( -14.4123 50.5044 )
Norm@50keV : 0.109674 ( -0.109764 1.08715 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 56.80 using 59 bins.
Reduced chi-squared = 1.01429
# Null hypothesis probability of 4.45e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.79118 ( -0.40895 0.40556 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.28905e-07 ( -3.02225e-08 3.12056e-08 ) ergs/cm2
Band function
Time interval is from 14.812 sec. to 15.812 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] : 15.1155 (-2.81319 3.43397)
R^2/D10^2 : 0.224132 (-0.118197 0.241733)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 57.82 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.45e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.071e-08 3.973e-09
25- 50 4.284e-08 1.570e-08
50-150 6.685e-08 2.865e-08
15-150 1.204e-07 3.771e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 149.501 (-74.6081 -147.339)
Norm : 7.90012 (-1.73494 2.20888)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.41 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.88e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.030e-08 1.149e-08
25- 50 3.760e-08 2.114e-08
50-150 7.412e-08 4.555e-08
15-150 1.320e-07 7.830e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.07618 (-3.08218 12.9521)
R1^2/D10^2 : 39.0559 (-38.6715 505.772)
kT2 [keV] : 16.5097 (-3.36772 -16.5134)
R2^2/D10^2 : 0.154411 (-0.154267 0.205223)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.34 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.62e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.716e-08 8.850e-09
25- 50 3.867e-08 2.018e-08
50-150 7.193e-08 3.938e-08
15-150 1.277e-07 6.614e-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: 1.85637 ( -0.175494 0.182555 )
Norm@50keV : 3.41335E-03 ( -0.000407733 0.000400489 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.39 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.22e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 53.36 sec: 0.481029 ( -0.0489599 0.0489782 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.67459e-06 ( -1.98126e-07 2.01172e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.18432 ( -0.840871 0.699249 )
Epeak [keV] : 52.6424 ( -13.8972 -52.6424 )
Norm@50keV : 8.18552E-03 ( -0.00482352 0.0161387 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.73 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.76e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 53.36 sec: 0.470436 ( -0.050194 0.050188 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.57596e-06 ( -2.1693e-07 2.24752e-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) = 4.81e-07
S(50-100 keV) = 5.32e-07
T90 vs. Hardness ratio plot
T90 = 50.5600000619888 sec.
Hardness ratio (energy fluence ratio) = 1.10603
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.11929
Count Ratio (50-100 keV) / (15-25 keV) = 0.683347
Mask shadow pattern
IMX = 5.955234194774257E-02, IMY = -6.401537666098231E-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:
-239.000000 14.792000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5668 -40.5058 2.9 47.4 140.9 4.1817 3.9 3.4 Vela X-1
170.5129 -60.6628 5.7 50.4 -180.0 1.5475 2.0 6.3 Cen X-3
186.7783 -62.8738 6.5 53.9 -170.8 1.4116 1.8 7.0 GX 301-2
92.8726 -58.4995 2.6 15.6 152.5 1.2586 4.5 ------ UNKNOWN
190.1925 -69.9340 3.1 49.1 -163.9 2.2299 3.7 ------ UNKNOWN
22.9487 -9.7462 2.6 56.0 -14.9 4.2167 4.5 ------ UNKNOWN
19.6298 -7.8781 2.5 59.2 -17.3 7.5161 4.6 ------ UNKNOWN
9.9380 -26.5632 2.6 48.6 -39.7 3.8443 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
14.792000 68.152000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5805 -40.5539 3.0 47.4 141.0 -1.8738 -3.8 2.4 Vela X-1
170.4691 -60.5455 10.1 50.5 179.9 -0.3032 -1.1 6.5 Cen X-3
186.8055 -62.7570 18.2 54.0 -170.9 -0.1791 -0.6 4.2 GX 301-2
91.5906 -28.4028 0.8 32.7 84.7 3.1573 14.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
141.300590 963.087500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5274 -40.5537 3.5 37.8 178.7 3.6719 3.3 0.1 Vela X-1
106.4721 8.4745 3.5 39.6 81.7 8.8685 3.3 ------ UNKNOWN
91.5732 -1.2244 3.7 27.2 58.2 2.9170 3.1 ------ UNKNOWN
49.4151 -10.3226 3.2 43.4 -15.8 4.5472 3.7 ------ UNKNOWN
35.2226 -3.1199 3.0 59.2 -17.3 17.7075 3.8 ------ UNKNOWN
36.7685 -11.2876 2.8 53.8 -24.9 13.1931 4.1 ------ UNKNOWN
138.9154 -70.6369 3.1 49.7 -140.5 8.8821 3.7 ------ UNKNOWN
158.0034 -69.1752 2.9 55.3 -145.2 16.7661 4.0 ------ UNKNOWN
Plot creation:
Mon Oct 24 05:09:43 EDT 2022