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
15.6111 -59.0978 0.0165 23.7 52.3 2.1183 11.6 TRIG_01340561
------------------------------------------
Foreground time interval of the image:
-17.299 72.501 (delta_t = 89.800 [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 -50.996 sec. to 85.156 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.72183 ( -0.121377 0.123378 )
Norm@50keV : 1.97019E-03 ( -0.000140518 0.000139162 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 70.07 using 59 PHA bins.
# Reduced chi-squared = 1.229 for 57 degrees of freedom
# Null hypothesis probability = 1.145828e-01
Photon flux (15-150 keV) in 136.2 sec: 0.263690 ( -0.0176237 0.0176565 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.48049e-06 ( -1.84558e-07 1.86087e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -50.996 sec. to 85.156 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65305 ( -0.459052 0.433284 )
Epeak [keV] : 241.271 ( -172.726 -241.272 )
Norm@50keV : 2.14074E-03 ( -0.000381041 0.00152535 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.99 using 59 PHA bins.
# Reduced chi-squared = 1.250 for 56 degrees of freedom
# Null hypothesis probability = 9.894720e-02
Photon flux (15-150 keV) in 136.2 sec: 0.262712 ( -0.01853 0.018261 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.46647e-06 ( -2.07215e-07 1.98008e-07 ) ergs/cm2
Band function
Time interval is from -50.996 sec. to 85.156 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 8.20807E-02 ( 1.20348 1.20348 )
beta : -1.73949 ( 1.74317 0.139341 )
Epeak [keV] : 24.8042 ( -40.5787 -40.5787 )
Norm@50keV : 5.58195E-02 ( -0.0538573 529.642 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.90 using 59 PHA bins.
# Reduced chi-squared = 1.271 for 55 degrees of freedom
# Null hypothesis probability = 8.501466e-02
Photon flux (15-150 keV) in 136.2 sec: 0.262767 ( ) 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] : 12.9362 ( )
R^2/D10^2 : 4.68520E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 140.25 using 59 PHA bins.
# Reduced chi-squared = 2.4605 for 57 degrees of freedom
# Null hypothesis probability = 5.732612e-09
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.265e-07 2.847e-08
25- 50 7.759e-07 6.040e-08
50-150 8.186e-07 1.376e-07
15-150 1.821e-06 1.396e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 133.387 (-35.6916 53.61)
Norm : 1.09092 (-0.0866564 0.106745)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.849e-07 3.800e-08
25- 50 7.008e-07 7.893e-08
50-150 1.315e-06 4.778e-07
15-150 2.401e-06 5.244e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.86572 (-0.990256 1.11424)
R1^2/D10^2 : 0.598441 (-0.284163 0.64294)
kT2 [keV] : 23.4920 (-3.74594 5.60863)
R2^2/D10^2 : 4.36223E-03 (-0.00233729 0.00397842)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.193e-07 1.007e-07
25- 50 6.649e-07 1.273e-07
50-150 1.358e-06 3.804e-07
15-150 2.442e-06 6.524e-07
Peak spectrum fit
Power-law model
Time interval is from -48.592 sec. to -47.592 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.07992 ( -0.490436 0.641962 )
Norm@50keV : 5.59018E-03 ( -0.00239682 0.00226459 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.36 using 59 PHA bins.
# Reduced chi-squared = 1.024 for 57 degrees of freedom
# Null hypothesis probability = 4.252235e-01
Photon flux (15-150 keV) in 1 sec: 0.870888 ( -0.294312 0.294533 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.18269e-08 ( -1.97134e-08 2.03947e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -48.592 sec. to -47.592 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.831167 ( -6.1384 2.77366 )
Epeak [keV] : 47.3816 ( -25.8412 23.0701 )
Norm@50keV : 0.179641 ( -0.21794 301.141 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.78 using 59 PHA bins.
# Reduced chi-squared = 0.9782 for 56 degrees of freedom
# Null hypothesis probability = 5.210571e-01
Photon flux (15-150 keV) in 1 sec: 0.819902 ( -0.304275 0.305508 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.08623e-08 ( -1.80494e-08 2.03892e-08 ) ergs/cm2
Band function
Time interval is from -48.592 sec. to -47.592 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 0.776398 ( -2.4328 -0.622743 )
beta : -10.0000 ( 10 1.77636e-14 )
Epeak [keV] : 47.3710 ( -26.1674 23.1498 )
Norm@50keV : 0.169134 ( -0.169138 30.4078 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.79 using 59 PHA bins.
# Reduced chi-squared = 0.9961 for 55 degrees of freedom
# Null hypothesis probability = 4.827422e-01
Photon flux (15-150 keV) in 1 sec: 0.836010 ( 6.16399 -0.321404 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.19409e-08 ( -5.19339e-08 -1.917e-08 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.2516 (-3.19859 4.02161)
R^2/D10^2 : 0.219076 (-0.219076 0.441166)
(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 6.965e-09 4.349e-09
25- 50 2.246e-08 1.329e-08
50-150 2.054e-08 1.488e-08
15-150 4.997e-08 3.262e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 63.6701 (-33.5636 102.043)
Norm : 4.66138 (-1.84355 2.74473)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.182e-08 7.132e-09
25- 50 1.831e-08 1.188e-08
50-150 2.187e-08 1.962e-08
15-150 5.200e-08 3.499e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.78260 (-1.63048 15.4401)
R1^2/D10^2 : 1234.45 (-1113.07 -1113.07)
kT2 [keV] : 13.1515 (-3.45595 4.61212)
R2^2/D10^2 : 0.159075 (-0.158901 0.149524)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.429e-09 4.290e-09
25- 50 2.062e-08 1.276e-08
50-150 2.215e-08 1.534e-08
15-150 5.220e-08 3.148e-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: 1.78704 ( -0.159892 0.164972 )
Norm@50keV : 1.50813E-03 ( -0.000160094 0.000157759 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.18 using 59 PHA bins.
# Reduced chi-squared = 0.8627 for 57 degrees of freedom
# Null hypothesis probability = 7.599025e-01
Photon flux (15-150 keV) in 89.8 sec: 0.206783 ( -0.019186 0.0191938 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.24739e-06 ( -1.34522e-07 1.36468e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.03784 ( -0.79246 0.666523 )
Epeak [keV] : 56.1986 ( -12.3883 86.404 )
Norm@50keV : 3.96370E-03 ( -0.00225178 0.00705588 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.43 using 59 PHA bins.
# Reduced chi-squared = 0.8112 for 56 degrees of freedom
# Null hypothesis probability = 8.426977e-01
Photon flux (15-150 keV) in 89.8 sec: 0.201214 ( -0.019777 0.019787 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.16207e-06 ( -1.4923e-07 1.54627e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 1.22054 ( -1.67586 -0.117286 )
beta : -2.08035 ( -4.43036 0.30249 )
Epeak [keV] : 32.6202 ( -12.3276 47.1756 )
Norm@50keV : 0.160537 ( -0.156288 47.3585 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.15 using 59 PHA bins.
# Reduced chi-squared = 0.8027 for 55 degrees of freedom
# Null hypothesis probability = 8.524983e-01
Photon flux (15-150 keV) in 89.8 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.16154e-06 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 6.78e-07
S(50-100 keV) = 8.22e-07
T90 vs. Hardness ratio plot
T90 = 104.171999931335 sec.
Hardness ratio (energy fluence ratio) = 1.21239
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.11797
Count Ratio (50-100 keV) / (15-25 keV) = 0.797768
Mask shadow pattern
IMX = 2.684494827481671E-01, IMY = -3.467819780013844E-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:
-17.299400 72.500600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
334.5335 -62.7165 2.5 43.2 44.5 1.9673 4.7 ------ UNKNOWN
24.9451 -11.0851 2.3 43.0 143.8 1.8620 5.0 ------ UNKNOWN
15.6111 -59.0978 1.0 23.7 52.3 2.1182 11.6 ------ UNKNOWN
17.8085 -75.8823 2.8 31.2 18.9 0.8191 4.1 ------ UNKNOWN
79.8570 -2.2047 2.5 51.8 -139.0 3.8232 4.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
132.500600 340.300640
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
186.6570 -62.7703 37.8 57.9 -24.7 -0.4455 -0.3 0.0 GX 301-2
296.5135 -46.9239 2.6 46.1 48.6 3.7502 4.4 ------ UNKNOWN
320.7875 -47.8577 2.3 33.4 65.0 2.6543 4.9 ------ UNKNOWN
59.3268 -19.6136 2.3 50.4 -142.2 4.4870 5.1 ------ UNKNOWN
Plot creation:
Tue Aug 12 10:10:09 EDT 2025