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
244.7963 -16.2421 0.0169 23.6 114.1 2.7941 11.3 TRIG_01219994
------------------------------------------
Foreground time interval of the image:
-13.699 70.701 (delta_t = 84.400 [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
Multiple GTIs in the spectrum
tstart tstop
-122.352000 335.190000
336.000000 515.760000
517.000000 658.390000
659.000000 694.364000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 6.52377 ( -0.28548 0.286531 )
Norm@50keV : 5.03561E-05 ( -1.1402e-05 1.40203e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.41 using 59 PHA bins.
# Reduced chi-squared = 1.270 for 57 degrees of freedom
# Null hypothesis probability = 8.201728e-02
Photon flux (15-150 keV) in 814.1 sec: 0.352433 ( -0.0282554 0.028566 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.41828e-06 ( -6.21573e-07 6.27359e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-122.352000 335.190000
336.000000 515.760000
517.000000 658.390000
659.000000 694.364000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 8.89449E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 639.10 using 59 PHA bins.
# Reduced chi-squared = 11.413 for 56 degrees of freedom
# Null hypothesis probability = 6.989468e-100
Photon flux (15-150 keV) in 814.1 sec: 0.326081 ( -0.034508 0.033679 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.81369e-06 ( -7.50999e-07 7.3444e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-122.352000 335.190000
336.000000 515.760000
517.000000 658.390000
659.000000 694.364000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.170712 ( -1.25441 1.25441 )
beta : -10.0000 ( 10 10 )
Epeak [keV] : 7.09059 ( -1.06711 5.2413 )
Norm@50keV : 11.7691 ( -11.7691 15541.4 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.95 using 59 PHA bins.
# Reduced chi-squared = 0.9626 for 55 degrees of freedom
# Null hypothesis probability = 5.535396e-01
Photon flux (15-150 keV) in 814.1 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] : 2.56303 (-0.12866 0.140902)
R^2/D10^2 : 132.971 (-48.7771 75.6709)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.87 using 59 PHA bins.
# Reduced chi-squared = 0.9275 for 57 degrees of freedom
# Null hypothesis probability = 6.307558e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.102e-06 1.021e-06
25- 50 5.767e-07 8.503e-08
50-150 2.319e-10 1.239e-10
15-150 7.679e-06 9.631e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 4.28671 (-0.300852 0.342045)
Norm : 140.707 (-44.2495 63.8505)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.385e-06 8.178e-07
25- 50 6.448e-07 1.001e-07
50-150 1.447e-09 7.565e-10
15-150 8.031e-06 9.969e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.64624 (-0.129766 0.142278)
R1^2/D10^2 : 98.7545 (-48.7752 75.6646)
kT2 [keV] : 1.09495 (-0.679842 -0.679842)
R2^2/D10^2 : 7.52541E+04 (-81462.6 -81462.6)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.037e-06 1.661e-03
25- 50 5.860e-07 1.109e-02
50-150 2.503e-10 2.968e-01
15-150 7.624e-06 3.999e-01
Peak spectrum fit
Power-law model
Time interval is from 20.244 sec. to 21.244 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 3.54139 ( -0.849507 1.10109 )
Norm@50keV : 1.94107E-03 ( -0.00130741 0.00197819 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.70 using 59 PHA bins.
# Reduced chi-squared = 0.6615 for 57 degrees of freedom
# Null hypothesis probability = 9.772353e-01
Photon flux (15-150 keV) in 1 sec: 0.811946 ( -0.211436 0.212353 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.13339e-08 ( -1.01781e-08 1.22659e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 20.244 sec. to 21.244 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -5.56067 ( )
Epeak [keV] : 17.5410 ( )
Norm@50keV : 5.74296E+04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.87 using 59 PHA bins.
# Reduced chi-squared = 0.6762 for 56 degrees of freedom
# Null hypothesis probability = 9.698723e-01
Photon flux (15-150 keV) in 1 sec: 0.806264 ( -0.206707 0.214286 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.1486e-08 ( -1.24256e-08 1.17345e-08 ) ergs/cm2
Band function
Time interval is from 20.244 sec. to 21.244 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 3.97746 ( 1.69183 1.69183 )
beta : -4.22766 ( 3.84762 1.12944 )
Epeak [keV] : 15.9133 ( -3.44812 84.159 )
Norm@50keV : 4078.41 ( -4078.86 1.45728e+07 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.33 using 59 PHA bins.
# Reduced chi-squared = 0.6787 for 55 degrees of freedom
# Null hypothesis probability = 9.673876e-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] : 3.81514 (-0.837338 1.06646)
R^2/D10^2 : 26.7765 (-26.7765 81.5159)
(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 1.927e-08 1.129e-08
25- 50 6.067e-09 3.881e-09
50-150 5.503e-11 5.860e-11
15-150 2.540e-08 1.488e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 9.60328 (-3.60778 7.95695)
Norm : 29.6211 (-18.6433 60.8907)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.853e-08 1.060e-08
25- 50 7.549e-09 4.829e-09
50-150 4.628e-10 5.085e-10
15-150 2.654e-08 1.604e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.72628 (-0.820896 1.0373)
R1^2/D10^2 : 29.8933 (-19.8625 94.2385)
kT2 [keV] : 200.000 (-200 -200)
R2^2/D10^2 : 7.89379E-05 (-5.99066e-05 0.00051063)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.915e-08 1.075e-08
25- 50 6.628e-09 3.932e-09
50-150 2.123e-08 1.563e-08
15-150 4.701e-08 2.482e-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: 5.30767 ( -0.45694 0.482951 )
Norm@50keV : 1.69664E-04 ( -6.44261e-05 8.9801e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.92 using 59 PHA bins.
# Reduced chi-squared = 1.209 for 57 degrees of freedom
# Null hypothesis probability = 1.338378e-01
Photon flux (15-150 keV) in 84.4 sec: 0.352115 ( -0.0368243 0.0368623 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.29615e-07 ( -9.67182e-08 9.6898e-08 ) 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 : 2.81547E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 246.04 using 59 PHA bins.
# Reduced chi-squared = 4.3935 for 56 degrees of freedom
# Null hypothesis probability = 1.181590e-25
Photon flux (15-150 keV) in 84.4 sec: 0.344372 ( -0.038705 0.038215 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.81187e-07 ( -9.59231e-08 9.59881e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.04120 ( -3.01359 2.95592 )
beta : -8.40239 ( 9.01536 3.48479 )
Epeak [keV] : 10.0307 ( -1.50398 2.52152 )
Norm@50keV : 27.9682 ( -27.7765 18936 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.97 using 59 PHA bins.
# Reduced chi-squared = 1.163 for 55 degrees of freedom
# Null hypothesis probability = 1.906296e-01
Photon flux (15-150 keV) in 84.4 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) = 7.99e-07
S(50-100 keV) = 3.47e-08
T90 vs. Hardness ratio plot
T90 = 714.939999938011 sec.
Hardness ratio (energy fluence ratio) = 0.0434293
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.0651613
Count Ratio (50-100 keV) / (15-25 keV) = -0.00272972
Mask shadow pattern
IMX = -1.782564244059248E-01, IMY = -3.994060105922526E-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:
-13.699400 70.700600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.1403 -15.5421 4.3 23.8 115.9 0.6627 2.7 11.0 Sco X-1
255.7725 -37.9642 0.0 12.6 38.0 0.1206 0.7 12.4 4U 1700-377
256.4557 -36.3385 63.3 11.1 42.3 0.0318 0.2 5.2 GX 349+2
262.8311 -24.8585 17.0 5.2 137.5 0.1172 0.7 11.8 GX 1+4
264.9457 -44.4536 134.6 15.5 0.0 -0.0154 -0.1 8.7 4U 1735-44
268.4921 -1.6104 0.0 27.5 -179.4 -0.1341 -0.7 12.0 SW J1753.5-0127
270.2192 -24.9269 8.0 5.3 -143.3 0.2651 1.5 9.8 GX 5-1
270.1375 -25.7107 5.8 4.7 -138.0 0.3775 2.0 9.1 GRS 1758-258
274.1546 -14.1904 0.0 16.4 -156.5 0.3185 1.9 12.7 GX 17+2
275.9176 -30.2187 7.6 8.3 -83.2 0.2760 1.5 8.9 H1820-303
284.8854 -25.0741 0.0 16.9 -103.0 0.1680 0.9 12.3 HT1900.1-2455
288.9181 10.9480 5.7 45.5 -152.1 0.7176 2.0 7.1 GRS 1915+105
262.8195 -33.7421 10.9 5.7 28.1 -0.1756 -1.1 10.1 GX 354-0
244.7965 -16.2425 1.0 23.6 114.1 2.7663 11.2 ------ UNKNOWN
233.7455 -67.8528 2.4 43.4 13.3 1.5784 4.9 ------ UNKNOWN
335.4778 -65.3035 2.0 55.2 -32.3 5.6069 5.8 ------ UNKNOWN
300.8242 7.6970 2.8 49.4 -136.5 3.1194 4.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
132.300600 335.190000
336.000000 515.760000
517.000000 658.390000
659.000000 963.003500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
245.0328 -15.7987 6.7 0.5 -158.1 2.4071 1.8 10.0 Sco X-1
254.4734 35.1874 5.7 52.2 -177.9 -8.3236 -2.0 9.3 Her X-1
255.9758 -37.8507 186.0 23.8 -30.3 0.0878 0.1 0.6 4U 1700-377
256.4351 -36.4233 6.8 22.7 -32.9 2.3846 1.7 0.0 GX 349+2
263.1450 -24.6681 6.6 19.1 -68.8 3.0586 1.7 8.8 GX 1+4
264.9214 -44.2904 5.5 32.8 -35.0 -3.7468 -2.1 12.3 4U 1735-44
268.3655 -1.4514 76.0 27.5 -128.0 0.2475 0.2 0.2 SW J1753.5-0127
270.3387 -24.9398 8.5 25.4 -73.7 -2.4091 -1.4 8.9 GX 5-1
270.2530 -25.8825 6.7 25.6 -71.5 -3.1230 -1.7 8.8 GRS 1758-258
274.0059 -14.0364 27.1 28.3 -98.4 -0.8750 -0.4 0.0 GX 17+2
275.8124 -30.5119 5.2 31.7 -65.6 4.8863 2.2 10.5 H1820-303
284.9686 -24.8105 7.2 38.5 -78.3 5.8092 1.6 7.6 HT1900.1-2455
262.9883 -33.8345 247.7 24.0 -47.5 -0.0781 -0.0 0.0 GX 354-0
211.2705 -4.5589 2.4 34.9 97.9 12.4366 4.8 ------ UNKNOWN
244.7049 -16.1789 0.8 0.1 121.7 23.8381 17.5 ------ UNKNOWN
223.5273 -72.2975 2.9 57.4 -0.4 24.5126 3.9 ------ UNKNOWN
289.7181 -61.3340 2.1 55.2 -32.3 41.2462 5.5 ------ UNKNOWN
Plot creation:
Thu Mar 14 08:33:34 EDT 2024