Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minutes to calcaulte
Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
236.4509 +8.6116 0.0125 4.8 107.6 1.7694 15.5 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) All plots contain as much data as has been downloaded to date.
- 2) The mask-weighted light curves are using the flight position.
- 3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 4) 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.
- 5) 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.
- 6) 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)
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) For long bursts, a spectral fit of 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.
- 4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.
Time averaged spectrum fit using the pre-slew 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: 1.61585 ( -0.175788 0.179334 )
Norm@50keV : 7.28779E-04 ( -7.93307e-05 7.84873e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.01 using 59 PHA bins.
# Reduced chi-squared = 1.158 for 57 degrees of freedom
# Null hypothesis probability = 1.936622e-01
Photon flux (15-150 keV) in 207.9 sec: 9.41171E-02 ( -0.00959973 0.00960902 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.41432e-06 ( -1.64381e-07 1.66795e-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: 0.903306 ( -0.850879 0.710343 )
Epeak [keV] : 72.0306 ( -18.9243 675.582 )
Norm@50keV : 1.74049E-03 ( -0.000993154 0.00311 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.07 using 59 PHA bins.
# Reduced chi-squared = 1.126 for 56 degrees of freedom
# Null hypothesis probability = 2.407267e-01
Photon flux (15-150 keV) in 207.9 sec: 9.11449E-02 ( -0.0100471 0.0100441 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.32613e-06 ( -1.82447e-07 1.87655e-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 : -0.903265 ( -0.604022 0.604462 )
beta : -10.0000 ( 10 7.10543e-15 )
Epeak [keV] : 72.0170 ( -17.5957 678.8 )
Norm@50keV : 1.74048E-03 ( -0.000992397 0.00310691 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.07 using 59 PHA bins.
# Reduced chi-squared = 1.147 for 55 degrees of freedom
# Null hypothesis probability = 2.126310e-01
Photon flux (15-150 keV) in 207.9 sec: 9.14629E-02 ( 6.90854 -0.0103728 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.33213e-06 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 13.2336 (-1.58274 1.8348)
R^2/D10^2 : 1.63368E-02 (-0.00610662 0.0095437)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 78.61 using 59 PHA bins.
# Reduced chi-squared = 1.379 for 57 degrees of freedom
# Null hypothesis probability = 3.046177e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.261e-07 2.334e-08
25- 50 4.427e-07 5.780e-08
50-150 4.952e-07 1.080e-07
15-150 1.064e-06 1.425e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 158.395 (-60.7445 -157.165)
Norm : 0.388320 (-0.0420153 0.0530282)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.063e-07 9.958e-08
25- 50 3.854e-07 1.740e-07
50-150 7.778e-07 4.466e-07
15-150 1.370e-06 6.432e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.83780 (-2.4382 2.65886)
R1^2/D10^2 : 0.102004 (-0.0647927 0.370698)
kT2 [keV] : 21.8000 (-5.62611 14.2949)
R2^2/D10^2 : 2.04023E-03 (-0.0017329 0.00479286)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.928e-07 1.020e-07
25- 50 4.002e-07 1.875e-07
50-150 7.303e-07 3.888e-07
15-150 1.323e-06 6.498e-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 PHA bins.
# Reduced chi-squared = 1.096 for 57 degrees of freedom
# Null hypothesis probability = 2.882625e-01
Photon flux (15-150 keV) in 1 sec: 0.437278 ( -0.136456 0.136265 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.80013e-08 ( -1.1336e-08 1.22702e-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: 3.44788 ( -1.72427 0.48412 )
Epeak [keV] : 383.300 ( )
Norm@50keV : 5.73733E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.99 using 59 PHA bins.
# Reduced chi-squared = 1.071 for 56 degrees of freedom
# Null hypothesis probability = 3.331572e-01
Photon flux (15-150 keV) in 1 sec: 0.437169 ( -0.136342 0.136304 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.71767e-08 ( -1.05345e-08 1.31423e-08 ) 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 : -1.38322 ( 1.38649 1.38649 )
beta : -1.89165 ( 1.89933 0.759779 )
Epeak [keV] : 24.3036 ( -23.313 -23.313 )
Norm@50keV : 8.10120E-03 ( -0.00824008 988072 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.46 using 59 PHA bins.
# Reduced chi-squared = 1.136 for 55 degrees of freedom
# Null hypothesis probability = 2.282674e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
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)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.187e-09 4.339e-09
25- 50 6.374e-09 4.040e-09
50-150 4.677e-10 4.687e-10
15-150 1.403e-08 8.775e-09
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
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)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.391e-09 2.688e-09
25- 50 8.209e-09 4.854e-09
50-150 1.660e-08 1.067e-08
15-150 2.920e-08 1.747e-08
Double BB
XSPEC12>exit
XSPEC: quit
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 9.71991)
kT2 [keV] : 98.0560 (-99.3783 -99.3784)
R2^2/D10^2 : 2.63708E-04 (-0.000209696 0.00231108)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.281e-09 4.189e-09
25- 50 5.996e-09 3.644e-09
50-150 2.478e-08 1.961e-08
15-150 3.805e-08 2.336e-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 PHA bins.
# Reduced chi-squared = 1.046 for 57 degrees of freedom
# Null hypothesis probability = 3.812458e-01
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 PHA bins.
# Reduced chi-squared = 1.050 for 56 degrees of freedom
# Null hypothesis probability = 3.729308e-01
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 : -0.873801 ( 0.983102 0.983102 )
beta : -1.84098 ( 1.83612 0.360877 )
Epeak [keV] : 60.2456 ( -59.8653 -59.8653 )
Norm@50keV : 3.18446E-03 ( -0.00319518 172946 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.56 using 59 PHA bins.
# Reduced chi-squared = 1.065 for 55 degrees of freedom
# Null hypothesis probability = 3.462827e-01
Photon flux (15-150 keV) in 79.89 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 8.50621e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 3.69e-07
S(50-100 keV) = 4.82e-07
T90 vs. Hardness ratio plot
T90 = 177.883999943733 sec.
Hardness ratio (energy fluence ratio) = 1.30623
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:
Mon Jul 29 11:25:52 EDT 2024