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
245.0819 -15.7511 0.0144 24.9 -99.8 3.3971 13.3 TRIG_01217218
------------------------------------------
Foreground time interval of the image:
0.000 96.000 (delta_t = 96.000 [sec])
Background time interval of the image:
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 0.000 sec. to 96.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 5.48521 ( -0.536369 0.563228 )
Norm@50keV : 1.36040E-04 ( -5.7883e-05 8.70016e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 34.26 using 59 PHA bins.
# Reduced chi-squared = 0.6010 for 57 degrees of freedom
# Null hypothesis probability = 9.926742e-01
Photon flux (15-150 keV) in 96 sec: 0.335783 ( -0.0366332 0.0367114 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.96576e-07 ( -1.0587e-07 1.05959e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 96.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 2.77855E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 194.17 using 59 PHA bins.
# Reduced chi-squared = 3.4674 for 56 degrees of freedom
# Null hypothesis probability = 3.903657e-17
Photon flux (15-150 keV) in 96 sec: 0.335452 ( -0.036487 0.036608 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.96106e-07 ( -1.05678e-07 1.05437e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 96.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.51377 ( )
beta : -7.76870 ( )
Epeak [keV] : 29.2480 ( )
Norm@50keV : 2.38554E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 167.62 using 59 PHA bins.
# Reduced chi-squared = 3.0477 for 55 degrees of freedom
# Null hypothesis probability = 2.578083e-13
Photon flux (15-150 keV) in 96 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] : 2.66565 (-0.276096 0.329134)
R^2/D10^2 : 102.027 (-58.301 134.864)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.67 using 59 PHA bins.
# Reduced chi-squared = 0.6959 for 57 degrees of freedom
# Null hypothesis probability = 9.608656e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.456e-07 2.594e-07
25- 50 8.001e-08 2.855e-08
50-150 4.645e-11 3.974e-11
15-150 9.257e-07 2.596e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 4.99982 (-0.773318 1.0251)
Norm : 75.8758 (-37.4567 75.8437)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.409e-07 1.992e-07
25- 50 1.063e-07 3.564e-08
50-150 5.507e-10 4.386e-10
15-150 9.477e-07 2.278e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.18902 (-0.811685 0.479356)
R1^2/D10^2 : 381.261 (-295.773 11560.5)
kT2 [keV] : 6.06013 (-2.82579 8.71116)
R2^2/D10^2 : 0.269399 (-0.283118 0.925455)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.509e-07 4.312e-07
25- 50 1.602e-07 9.130e-08
50-150 1.445e-08 9.149e-09
15-150 1.026e-06 5.030e-07
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 96.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 5.48521 ( -0.536369 0.563228 )
Norm@50keV : 1.36040E-04 ( -5.7883e-05 8.70016e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 34.26 using 59 PHA bins.
# Reduced chi-squared = 0.6010 for 57 degrees of freedom
# Null hypothesis probability = 9.926742e-01
Photon flux (15-150 keV) in 96 sec: 0.335783 ( -0.0366332 0.0367114 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.96576e-07 ( -1.0587e-07 1.05959e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 96.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 2.77855E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 194.17 using 59 PHA bins.
# Reduced chi-squared = 3.4674 for 56 degrees of freedom
# Null hypothesis probability = 3.903657e-17
Photon flux (15-150 keV) in 96 sec: 0.335452 ( -0.036487 0.036608 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.96106e-07 ( -1.05678e-07 1.05437e-07 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 96.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.51377 ( )
beta : -7.76870 ( )
Epeak [keV] : 29.2480 ( )
Norm@50keV : 2.38554E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 167.62 using 59 PHA bins.
# Reduced chi-squared = 3.0477 for 55 degrees of freedom
# Null hypothesis probability = 2.578083e-13
Photon flux (15-150 keV) in 96 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] : 2.66565 (-0.276096 0.329134)
R^2/D10^2 : 102.027 (-58.301 134.864)
(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 8.456e-07 2.312e-07
25- 50 8.001e-08 2.654e-08
50-150 4.645e-11 3.939e-11
15-150 9.257e-07 2.882e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 4.99982 (-0.773318 1.0251)
Norm : 75.8758 (-37.4567 75.8437)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.409e-07 2.011e-07
25- 50 1.063e-07 3.698e-08
50-150 5.507e-10 4.338e-10
15-150 9.477e-07 2.331e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.18902 (-0.811685 0.479356)
R1^2/D10^2 : 381.261 (-295.773 11560.5)
kT2 [keV] : 6.06013 (-2.82579 8.71116)
R2^2/D10^2 : 0.269399 (-0.283118 0.954892)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.509e-07 4.526e-07
25- 50 1.602e-07 9.178e-08
50-150 1.445e-08 1.097e-08
15-150 1.026e-06 5.040e-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: 5.48521 ( -0.536369 0.563228 )
Norm@50keV : 1.36040E-04 ( -5.7883e-05 8.70016e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 34.26 using 59 PHA bins.
# Reduced chi-squared = 0.6010 for 57 degrees of freedom
# Null hypothesis probability = 9.926742e-01
Photon flux (15-150 keV) in 96 sec: 0.335783 ( -0.0366332 0.0367114 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.96576e-07 ( -1.0587e-07 1.05959e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 2.77855E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 194.17 using 59 PHA bins.
# Reduced chi-squared = 3.4674 for 56 degrees of freedom
# Null hypothesis probability = 3.903657e-17
Photon flux (15-150 keV) in 96 sec: 0.335452 ( -0.036487 0.036608 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.96106e-07 ( -1.05678e-07 1.05437e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.51377 ( )
beta : -7.76870 ( )
Epeak [keV] : 29.2480 ( )
Norm@50keV : 2.38554E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 167.62 using 59 PHA bins.
# Reduced chi-squared = 3.0477 for 55 degrees of freedom
# Null hypothesis probability = 2.578083e-13
Photon flux (15-150 keV) in 96 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) = 1.53e-07
S(50-100 keV) = 1.37e-08
T90 vs. Hardness ratio plot
T90 = 96 sec.
Hardness ratio (energy fluence ratio) = 0.0895425
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.147639
Count Ratio (50-100 keV) / (15-25 keV) = 0.0131808
Mask shadow pattern
IMX = -7.942820698677808E-02, IMY = 4.577027783276721E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 96.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
186.7254 -62.7936 12.6 50.3 9.3 0.4271 0.9 2.3 GX 301-2
245.0821 -15.7511 0.9 24.9 -99.8 3.3994 13.3 8.9 Sco X-1
256.0916 -37.9312 2.5 38.1 -59.5 1.8309 4.7 7.2 4U 1700-377
256.3261 -36.5759 6.3 37.8 -61.7 0.7333 1.8 10.6 GX 349+2
264.9110 -44.5259 4.4 46.6 -53.9 2.2157 2.6 8.5 4U 1735-44
262.9545 -33.7209 4.6 42.2 -68.2 -1.9290 -2.5 7.0 GX 354-0
214.3705 33.6410 2.2 51.5 165.7 3.2289 5.1 ------ UNKNOWN
201.7339 -37.2112 2.3 24.8 25.4 1.0234 4.9 ------ UNKNOWN
233.9727 33.5363 2.7 53.2 -173.8 2.3482 4.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
167.500590 243.079300
425.000000 515.080000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.1213 -15.7328 0.7 0.1 135.7 5.0855 16.4 9.9 Sco X-1
254.4223 35.2176 5.2 51.7 -179.8 -2.1075 -2.2 7.7 Her X-1
256.1515 -37.9391 1.5 24.2 -31.0 2.5683 7.5 9.7 4U 1700-377
256.5602 -36.3222 4.4 22.9 -33.7 -0.8621 -2.6 8.5 GX 349+2
263.1668 -24.8270 4.1 19.1 -68.4 0.9941 2.8 9.9 GX 1+4
264.9163 -44.2955 4.0 33.1 -35.8 -1.1509 -2.9 11.9 4U 1735-44
268.3030 -1.3004 3.4 27.0 -129.6 -1.3889 -3.4 9.9 SW J1753.5-0127
270.1150 -25.1938 95.3 25.2 -73.5 -0.0516 -0.1 11.5 GX 5-1
270.4070 -25.7076 9.8 25.6 -72.5 0.5244 1.2 6.0 GRS 1758-258
274.1262 -13.9096 7.2 28.0 -99.4 0.7363 1.6 10.3 GX 17+2
275.9666 -30.2308 13.0 31.7 -66.9 -0.4427 -0.9 8.5 H1820-303
284.9509 -25.0513 5.9 38.3 -78.9 -1.7438 -2.0 9.1 HT1900.1-2455
262.8846 -33.8541 8.3 24.1 -47.7 0.5285 1.4 5.3 GX 354-0
257.2880 40.1577 2.3 57.1 -178.5 7.3050 5.0 ------ UNKNOWN
260.6118 35.3033 2.4 53.1 -173.7 4.5650 4.7 ------ UNKNOWN
248.8368 -69.8419 2.2 54.1 -11.1 4.1921 5.4 ------ UNKNOWN
Plot creation:
Sun Feb 25 18:51:55 EST 2024