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
86.4423 +63.5826 0.0068 21.1 44.2 2.6341 28.3 TRIG_01429608
------------------------------------------
Foreground time interval of the image:
-31.264 10.037 (delta_t = 41.301 [sec])
Background time interval of the image:
-239.264 -31.264 (delta_t = 208.000 [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 -31.264 sec. to 64.736 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.62010 ( -0.0560307 0.0561306 )
Norm@50keV : 5.11085E-03 ( -0.000154986 0.000154884 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.07 using 59 PHA bins.
# Reduced chi-squared = 1.089 for 57 degrees of freedom
# Null hypothesis probability = 3.003834e-01
Photon flux (15-150 keV) in 96 sec: 0.660920 ( -0.021523 0.0215811 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.57775e-06 ( -1.46093e-07 1.46393e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -31.264 sec. to 64.736 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.27992 ( -0.236208 0.223968 )
Epeak [keV] : 109.247 ( -25.0916 103.697 )
Norm@50keV : 7.47099E-03 ( -0.00161338 0.00219789 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.17 using 59 PHA bins.
# Reduced chi-squared = 0.9852 for 56 degrees of freedom
# Null hypothesis probability = 5.061809e-01
Photon flux (15-150 keV) in 96 sec: 0.645571 ( -0.023511 0.023575 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.45992e-06 ( -1.66579e-07 1.65821e-07 ) ergs/cm2
Band function
Time interval is from -31.264 sec. to 64.736 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.667139 ( -0.58999 3.24997 )
beta : -1.76427 ( -0.157334 0.10548 )
Epeak [keV] : 54.3206 ( -25.1258 41.2638 )
Norm@50keV : 1.80876E-02 ( -0.0112221 4.89573 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.39 using 59 PHA bins.
# Reduced chi-squared = 0.9344 for 55 degrees of freedom
# Null hypothesis probability = 6.132467e-01
Photon flux (15-150 keV) in 96 sec: 0.636848 ( 6.36315 -0.024691 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.45387e-06 ( -4.4532e-06 -1.58486e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 14.6911 ( )
R^2/D10^2 : 7.59682E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 270.32 using 59 PHA bins.
# Reduced chi-squared = 4.7425 for 57 degrees of freedom
# Null hypothesis probability = 1.729993e-29
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.306e-07 1.925e-08
25- 50 1.288e-06 5.376e-08
50-150 1.875e-06 1.200e-07
15-150 3.493e-06 1.147e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 173.907 (-26.0438 -173.776)
Norm : 2.67671 (-0.0946741 0.101127)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.505e-07 3.643e-08
25- 50 1.231e-06 8.544e-08
50-150 2.573e-06 6.374e-07
15-150 4.454e-06 7.229e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.93482 (-0.803565 0.829939)
R1^2/D10^2 : 0.467966 (-0.12693 0.196253)
kT2 [keV] : 28.3651 (-3.49072 4.92757)
R2^2/D10^2 : 5.41194E-03 (-0.00233909 0.00343062)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.760e-07 5.410e-08
25- 50 1.285e-06 8.592e-08
50-150 2.586e-06 3.456e-07
15-150 4.447e-06 3.979e-07
Peak spectrum fit
Power-law model
Time interval is from 24.236 sec. to 25.236 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.37522 ( -0.087286 0.0875076 )
Norm@50keV : 3.78693E-02 ( -0.00206714 0.00206515 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.70 using 59 PHA bins.
# Reduced chi-squared = 1.083 for 57 degrees of freedom
# Null hypothesis probability = 3.117050e-01
Photon flux (15-150 keV) in 1 sec: 4.58650 ( -0.252576 0.252758 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.67821e-07 ( -2.20902e-08 2.21754e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 24.236 sec. to 25.236 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.497606 ( -0.411433 0.376098 )
Epeak [keV] : 88.6178 ( -13.7589 28.6086 )
Norm@50keV : 0.102562 ( -0.0348071 0.0583926 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.01 using 59 PHA bins.
# Reduced chi-squared = 0.7859 for 56 degrees of freedom
# Null hypothesis probability = 8.773253e-01
Photon flux (15-150 keV) in 1 sec: 4.45579 ( -0.25897 0.25892 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.50768e-07 ( -2.354e-08 2.3595e-08 ) ergs/cm2
Band function
Time interval is from 24.236 sec. to 25.236 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.497568 ( -0.306596 0.378732 )
beta : -10.0000 ( 10 3.55271e-15 )
Epeak [keV] : 88.6032 ( -10.0044 28.5836 )
Norm@50keV : 0.102567 ( -0.034803 0.0584466 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.01 using 59 PHA bins.
# Reduced chi-squared = 0.8001 for 55 degrees of freedom
# Null hypothesis probability = 8.560255e-01
Photon flux (15-150 keV) in 1 sec: 4.47697 ( ) 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] : 16.5644 (-1.04996 1.12665)
R^2/D10^2 : 0.394560 (-0.0799756 0.0995267)
(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 2.220e-08 2.235e-09
25- 50 9.618e-08 6.900e-09
50-150 1.868e-07 1.895e-08
15-150 3.052e-07 1.880e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-16.2868 -200)
Norm : 19.0446 (-1.02888 1.02888)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.743e-08 2.670e-09
25- 50 9.123e-08 5.835e-09
50-150 2.001e-07 3.435e-08
15-150 3.387e-07 3.950e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.79845 (-1.36947 1.74832)
R1^2/D10^2 : 3.85236 (-1.93413 4.3889)
kT2 [keV] : 22.7813 (-2.68189 4.06369)
R2^2/D10^2 : 0.108912 (-0.0519383 0.0684089)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.801e-08 9.140e-09
25- 50 9.138e-08 2.138e-08
50-150 2.207e-07 4.620e-08
15-150 3.501e-07 5.840e-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: 1.57906 ( -0.0981325 0.0988951 )
Norm@50keV : 3.98595E-03 ( -0.000225047 0.000224194 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.68 using 59 PHA bins.
# Reduced chi-squared = 0.6962 for 57 degrees of freedom
# Null hypothesis probability = 9.607234e-01
Photon flux (15-150 keV) in 41.3 sec: 0.508933 ( -0.0285177 0.0285844 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.54362e-06 ( -9.40145e-08 9.45469e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.28554 ( -0.418517 0.336485 )
Epeak [keV] : 120.373 ( -44.4038 -120.375 )
Norm@50keV : 5.62093E-03 ( -0.00176377 0.00345586 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.98 using 59 PHA bins.
# Reduced chi-squared = 0.6783 for 56 degrees of freedom
# Null hypothesis probability = 9.688692e-01
Photon flux (15-150 keV) in 41.3 sec: 0.501162 ( -0.030238 0.030219 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.50717e-06 ( -1.06414e-07 1.06054e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.878622 ( 1.02243 1.02243 )
beta : -1.72463 ( 1.75312 0.218799 )
Epeak [keV] : 62.5508 ( -62.6805 -62.6805 )
Norm@50keV : 1.01850E-02 ( -0.00622768 598.474 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.41 using 59 PHA bins.
# Reduced chi-squared = 0.6802 for 55 degrees of freedom
# Null hypothesis probability = 9.666169e-01
Photon flux (15-150 keV) in 41.3 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.50765e-06 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.20e-06
S(50-100 keV) = 1.56e-06
T90 vs. Hardness ratio plot
T90 = 48 sec.
Hardness ratio (energy fluence ratio) = 1.3
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.38523
Count Ratio (50-100 keV) / (15-25 keV) = 0.921759
Mask shadow pattern
IMX = 2.771231430046500E-01, IMY = -2.692916768903330E-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:
-239.264000 -31.264000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
90.6558 50.1264 3.1 29.7 69.4 1.8128 3.8 ------ UNKNOWN
348.0515 27.6752 2.4 48.0 -129.1 6.7848 4.9 ------ UNKNOWN
300.7147 60.2297 3.5 43.8 -64.1 4.4332 3.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-31.264000 10.036600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
91.3923 42.0973 2.6 35.8 79.1 0.8611 4.4 ------ UNKNOWN
86.4423 63.5826 0.4 21.1 44.2 2.6340 28.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
67.436600 962.816000
975.736000 1065.866000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6236 21.9901 2.7 41.6 115.2 27.0996 4.2 1.6 Crab
350.5505 55.2783 2.7 44.8 -122.3 21.4372 4.3 ------ UNKNOWN
353.6636 49.7507 2.1 48.0 -129.1 30.6096 5.5 ------ UNKNOWN
255.7607 72.4438 2.7 43.8 -64.1 25.1730 4.3 ------ UNKNOWN
Plot creation:
Thu Jan 8 10:38:03 EST 2026