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
83.3707 +21.8471 0.0167 51.5 -1.4 13.2256 11.5 TRIG_01215857
------------------------------------------
Foreground time interval of the image:
-13.799 73.330 (delta_t = 87.129 [sec])
74.000 336.168 (delta_t = 262.168 [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
-85.824000 73.330000
74.000000 336.168000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.12167 ( -0.133152 0.138639 )
Norm@50keV : 2.37389E-03 ( -0.00019912 0.000195701 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.12 using 59 PHA bins.
# Reduced chi-squared = 1.160 for 57 degrees of freedom
# Null hypothesis probability = 1.910623e-01
Photon flux (15-150 keV) in 421.3 sec: 0.377519 ( -0.0278065 0.0279304 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.31267e-06 ( -7.08652e-07 7.12481e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-85.824000 73.330000
74.000000 336.168000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.85956 ( -0.536389 0.330252 )
Epeak [keV] : 25.4515 ( )
Norm@50keV : 3.26090E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.29 using 59 PHA bins.
# Reduced chi-squared = 1.166 for 56 degrees of freedom
# Null hypothesis probability = 1.850883e-01
Photon flux (15-150 keV) in 421.3 sec: 0.372033 ( -0.029478 0.029532 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.16517e-06 ( -7.62764e-07 7.64617e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-85.824000 73.330000
74.000000 336.168000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.85897 ( 1.83755 0.529119 )
beta : -10.0000 ( 10 5.32907e-15 )
Epeak [keV] : 25.4882 ( -13.6429 26.4116 )
Norm@50keV : 3.26263E-03 ( -0.000847457 0.00289049 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.29 using 59 PHA bins.
# Reduced chi-squared = 1.187 for 55 degrees of freedom
# Null hypothesis probability = 1.613439e-01
Photon flux (15-150 keV) in 421.3 sec: 0.372934 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 9.11263e-06 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 11.3511 ( )
R^2/D10^2 : 0.101231 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 125.65 using 59 PHA bins.
# Reduced chi-squared = 2.2043 for 57 degrees of freedom
# Null hypothesis probability = 4.440355e-07
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.155e-06 1.567e-07
25- 50 3.397e-06 3.101e-07
50-150 2.532e-06 3.865e-07
15-150 7.083e-06 6.025e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 65.1653 (-12.1452 16.1771)
Norm : 1.85760 (-0.220501 0.255651)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.991e-06 1.974e-07
25- 50 3.105e-06 2.393e-07
50-150 3.776e-06 5.793e-07
15-150 8.873e-06 7.689e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.26227 (-0.751179 0.917036)
R1^2/D10^2 : 3.71739 (-2.18416 6.05798)
kT2 [keV] : 16.8935 (-2.08786 2.72249)
R2^2/D10^2 : 1.76300E-02 (-0.00817205 0.0128442)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.354e-06 8.894e-07
25- 50 2.732e-06 5.441e-07
50-150 3.886e-06 7.838e-07
15-150 8.972e-06 1.742e-06
Peak spectrum fit
Power-law model
Time interval is from 335.212 sec. to 336.212 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 5.48040 ( -0.981232 1.19764 )
Norm@50keV : 1.13388E-03 ( -0.00113409 0.00187201 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.22 using 59 PHA bins.
# Reduced chi-squared = 1.109 for 57 degrees of freedom
# Null hypothesis probability = 2.661811e-01
Photon flux (15-150 keV) in 1 sec: 2.78555 ( -0.69925 0.70039 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.6143e-08 ( -2.33079e-08 2.4119e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 335.212 sec. to 336.212 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 1.93783E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 100.80 using 59 PHA bins.
# Reduced chi-squared = 1.8000 for 56 degrees of freedom
# Null hypothesis probability = 2.265430e-04
Photon flux (15-150 keV) in 1 sec: 3.07798 3.08605 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 8.02929e-15 ( 0 0 ) ergs/cm2
Band function
Time interval is from 335.212 sec. to 336.212 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -8.28646 ( 8.28646 8.28646 )
beta : -5.50153 ( -1.17861 1.00029 )
Epeak [keV] : 2.66314 ( -2.66314 -2.66314 )
Norm@50keV : 0.150588 ( -0.151837 0.256773 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.22 using 59 PHA bins.
# Reduced chi-squared = 1.149 for 55 degrees of freedom
# Null hypothesis probability = 2.088007e-01
Photon flux (15-150 keV) in 1 sec: 0.477241 0.378899 0.388960 ( ) 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] : 2.53841 (-0.425421 0.514129)
R^2/D10^2 : 1315.31 (-1316.2 3817.79)
(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 8.054e-08 4.787e-08
25- 50 6.295e-09 3.967e-09
50-150 2.307e-12 2.803e-12
15-150 8.684e-08 4.936e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 4.67593 (-1.19605 1.77312)
Norm : 852.590 (-852.577 2013.33)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.720e-08 4.325e-08
25- 50 8.351e-09 5.500e-09
50-150 3.053e-11 3.436e-11
15-150 8.558e-08 4.872e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.53868 (-0.452445 0.546134)
R1^2/D10^2 : 1312.66 (-946.137 2089.56)
kT2 [keV] : 199.363 (-199.363 -199.363)
R2^2/D10^2 : 3.78379E-05 (-3.79514e-05 -3.79514e-05)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.045e-08 4.567e-08
25- 50 6.351e-09 4.039e-09
50-150 1.697e-09 2.925e-12
15-150 8.850e-08 5.010e-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: 2.10316 ( -0.15155 0.158854 )
Norm@50keV : 2.41036E-03 ( -0.000230492 0.000225678 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.73 using 59 PHA bins.
# Reduced chi-squared = 1.206 for 57 degrees of freedom
# Null hypothesis probability = 1.373366e-01
Photon flux (15-150 keV) in 349.3 sec: 0.379804 ( -0.0316099 0.0317464 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.82491e-06 ( -6.80346e-07 6.84551e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.96645 ( -0.57732 0.0491342 )
Epeak [keV] : 11.8550 ( -9.3337 -11.8171 )
Norm@50keV : 2.84029E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.58 using 59 PHA bins.
# Reduced chi-squared = 1.225 for 56 degrees of freedom
# Null hypothesis probability = 1.207254e-01
Photon flux (15-150 keV) in 349.3 sec: 0.377192 ( -0.033378 0.033289 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.76979e-06 ( -7.26195e-07 7.20571e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.94910 ( 1.94909 0.220173 )
beta : -9.37160 ( 9.37167 19.3717 )
Epeak [keV] : 16.4796 ( -16.4579 -16.4579 )
Norm@50keV : 2.88652E-03 ( -0.000460052 0.000810616 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.58 using 59 PHA bins.
# Reduced chi-squared = 1.247 for 55 degrees of freedom
# Null hypothesis probability = 1.031061e-01
Photon flux (15-150 keV) in 349.3 sec: 0.340096 ( 6.6599 -0.021595 ) 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) = 2.90e-06
S(50-100 keV) = 2.66e-06
T90 vs. Hardness ratio plot
T90 = 387.699999928474 sec.
Hardness ratio (energy fluence ratio) = 0.917241
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.00642
Count Ratio (50-100 keV) / (15-25 keV) = 0.65428
Mask shadow pattern
IMX = 1.256687739375743E+00, IMY = 3.006687871299524E-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:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-13.799400 73.330000
74.000000 336.168000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4836 21.9793 6.5 51.5 -1.2 2.1908 1.9 8.6 Crab
135.5168 -40.6020 2.7 37.0 -131.9 3.3548 4.3 2.9 Vela X-1
183.8855 -16.5254 2.7 55.4 163.7 7.7514 4.3 ------ UNKNOWN
83.3602 21.8325 1.0 51.5 -1.4 13.7175 12.0 ------ UNKNOWN
130.1252 -14.0828 2.8 10.1 -130.4 1.8900 4.1 ------ UNKNOWN
129.4323 -20.3551 2.6 16.3 -125.4 2.1333 4.5 ------ UNKNOWN
124.0374 -23.6456 2.4 20.2 -110.6 2.3142 4.7 ------ UNKNOWN
89.2867 -24.3205 1.8 43.2 -65.5 11.7518 6.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
-60.000000 73.330000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6445 22.0357 218.6 51.3 -1.0 -0.0253 -0.1 1.4 Crab
135.5915 -40.5906 7.0 37.0 -132.0 0.5206 1.6 3.6 Vela X-1
130.9306 -28.5901 2.7 24.6 -127.9 0.9402 4.3 ------ UNKNOWN
153.7028 -39.3699 2.5 41.9 -152.7 1.4761 4.6 ------ UNKNOWN
Plot creation:
Sun Feb 18 18:43:55 EST 2024