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
236.4509 8.6116 0.0125 4.8206 107.5921 1.7693882 15.508 TRIG_01245074
Foreground time interval of the image:
-6.792 73.101 (delta_t = 79.893 [sec])
Background time interval of the image:
-239.000 -6.792 (delta_t = 232.208 [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 -6.792 sec. to 201.060 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.62143 ( -0.175465 0.179056 )
Norm@50keV : 7.28798E-04 ( -7.94091e-05 7.85542e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.99 using 59 bins.
Reduced chi-squared = 1.15772
# Null hypothesis probability of 1.94e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 207.9 sec: 9.42898E-02 ( -0.0096179 0.0096272 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.41366e-06 ( -1.6422e-07 1.66515e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -6.792 sec. to 201.060 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.913108 ( -0.847449 0.708018 )
Epeak [keV] : 71.7034 ( -18.8214 747.706 )
Norm@50keV : 1.73372E-03 ( -0.00098811 0.0030846 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.07 using 59 bins.
Reduced chi-squared = 1.12625
# Null hypothesis probability of 2.41e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 207.9 sec: 9.13559E-02 ( -0.0100605 0.0100571 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.32542e-06 ( -1.81795e-07 1.87074e-07 ) ergs/cm2
Band function
Time interval is from -6.792 sec. to 201.060 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] : 13.1819 (-1.5736 1.82408)
R^2/D10^2 : 1.65776E-02 (-0.00619503 0.00967488)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 78.83 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.94e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.270e-07 2.388e-08
25- 50 4.439e-07 6.039e-08
50-150 4.916e-07 1.061e-07
15-150 1.062e-06 1.353e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 154.880 (-58.3554 -153.762)
Norm : 0.389848 (-0.0426797 0.0519897)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.52e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.076e-07 1.017e-07
25- 50 3.865e-07 1.871e-07
50-150 7.730e-07 4.423e-07
15-150 1.367e-06 6.262e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.82389 (-2.41969 2.64384)
R1^2/D10^2 : 0.103427 (-0.0652986 0.371134)
kT2 [keV] : 21.7660 (-5.61386 14.1645)
R2^2/D10^2 : 2.04704E-03 (-0.0017356 0.00481041)
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.78 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.20e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.940e-07 9.441e-08
25- 50 4.010e-07 1.739e-07
50-150 7.279e-07 4.082e-07
15-150 1.323e-06 6.288e-07
Peak spectrum fit
Power-law model
Time interval is from 3.120 sec. to 4.120 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.89980 ( -0.762013 0.857674 )
Norm@50keV : 3.04719E-03 ( -0.00143398 0.00121794 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 62.47 using 59 bins.
Reduced chi-squared = 1.09596
# Null hypothesis probability of 2.88e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.437306 ( -0.136468 0.136276 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.80046e-08 ( -1.13333e-08 1.22801e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 3.120 sec. to 4.120 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.44163 ( -1.71751 0.480888 )
Epeak [keV] : 382.208 ( )
Norm@50keV : 5.77569E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.99 using 59 bins.
Reduced chi-squared = 1.07125
# Null hypothesis probability of 3.33e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.287310 ( -0.163216 0.22057 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.31627e-08 ( -1.35186e-08 7.142e-09 ) ergs/cm2
Band function
Time interval is from 3.120 sec. to 4.120 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] : 5.69139 (-1.64761 2.88784)
R^2/D10^2 : 1.80854 (-1.80834 6.64909)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.01 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.71e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.187e-09 4.435e-09
25- 50 6.374e-09 4.436e-09
50-150 4.677e-10 4.685e-10
15-150 1.403e-08 8.795e-09
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 159.305 (-161.385 -161.385)
Norm : 1.71906 (-0.568132 3.32144)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.38e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.391e-09 2.746e-09
25- 50 8.209e-09 4.841e-09
50-150 1.660e-08 1.073e-08
15-150 2.920e-08 1.851e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.03390 (-1.4424 2.07618)
R1^2/D10^2 : 2.85148 (-2.22027 9.81237)
kT2 [keV] : 98.0560 (-68.8598 -99.3784)
R2^2/D10^2 : 2.63708E-04 (-0.000209696 0.00230807)
------------------------------------------------------------
#Fit statistic : Chi-Squared 55.51 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.55e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.281e-09 4.410e-09
25- 50 5.996e-09 3.480e-09
50-150 2.478e-08 2.238e-08
15-150 3.805e-08 2.208e-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: 1.61754 ( -0.181027 0.184776 )
Norm@50keV : 1.17744E-03 ( -0.000129056 0.000127496 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.60 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.81e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 79.89 sec: 0.152140 ( -0.01558 0.0155956 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.77895e-07 ( -1.02929e-07 1.04443e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.23920 ( -0.842539 0.525974 )
Epeak [keV] : 94.2465 ( -35.2276 -94.2496 )
Norm@50keV : 1.87145E-03 ( -0.000800535 0.00331005 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.73e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 79.89 sec: 0.149455 ( -0.016449 0.016379 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.46602e-07 ( -1.18916e-07 1.19859e-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) = 3.70e-07
S(50-100 keV) = 4.80e-07
T90 vs. Hardness ratio plot
T90 = 177.883999943733 sec.
Hardness ratio (energy fluence ratio) = 1.2973
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.37806
Count Ratio (50-100 keV) / (15-25 keV) = 0.936792
Mask shadow pattern
IMX = -2.548909428459438E-02, IMY = -8.039038628206906E-02
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 -6.792000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9951 -15.6306 0.6 29.7 139.1 9.9835 18.5 1.1 Sco X-1
254.3045 35.3829 8.4 31.2 20.2 0.6427 1.4 7.9 Her X-1
268.2502 -1.3621 3.9 37.8 91.5 3.4629 3.0 8.9 SW J1753.5-0127
268.4748 50.3790 2.4 49.0 14.1 3.3059 4.8 ------ UNKNOWN
267.6640 62.0164 3.3 56.7 3.2 5.1453 3.5 ------ UNKNOWN
192.8743 41.0425 3.7 45.6 -57.9 5.0558 3.2 ------ UNKNOWN
188.6090 -9.2770 3.2 48.1 -129.3 5.9852 3.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-6.792000 73.100600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.0247 -15.7910 5.3 29.8 139.2 -0.3755 -2.2 9.4 Sco X-1
254.3837 35.3046 3.7 31.2 20.4 0.4811 3.1 4.3 Her X-1
268.2185 -1.4256 30.5 37.8 91.6 -0.1553 -0.4 9.1 SW J1753.5-0127
236.4509 8.6116 0.7 4.8 107.6 1.7692 15.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
106.300600 744.700600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9845 -15.6352 0.5 25.7 138.3 26.0308 21.7 0.4 Sco X-1
254.5447 35.4744 9.1 31.5 6.5 1.4354 1.3 9.0 Her X-1
263.0649 -24.8157 7.9 42.3 120.4 -7.8877 -1.5 5.2 GX 1+4
268.4793 -1.5725 8.5 33.5 83.8 2.7661 1.4 9.8 SW J1753.5-0127
275.3428 44.0298 3.6 48.9 14.4 4.9992 3.2 ------ UNKNOWN
244.7036 15.9240 3.5 10.9 24.6 2.7142 3.3 ------ UNKNOWN
208.1406 -42.4347 2.7 57.2 -177.8 17.8136 4.3 ------ UNKNOWN
193.3771 -34.8972 3.1 59.6 -161.9 30.0885 3.7 ------ UNKNOWN
202.0626 42.9029 3.4 45.6 -57.8 15.5894 3.4 ------ UNKNOWN
190.6191 -6.4523 3.5 48.1 -129.2 14.7555 3.3 ------ UNKNOWN
Plot creation:
Sat Oct 19 18:22:25 EDT 2024