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
57.4839 -48.7101 0.0349 16.6 149.1 0.5228 5.5 TRIG_00829046
------------------------------------------
Foreground time interval of the image:
0.000 45.474 (delta_t = 45.474 [sec])
47.000 64.000 (delta_t = 17.000 [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
Multiple GTIs in the spectrum
tstart tstop
0.000000 45.474400
47.000000 64.000000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.97924 ( -0.560516 0.645733 )
Norm@50keV : 3.53736E-04 ( -0.000158349 0.000158154 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.64 using 59 PHA bins.
# Reduced chi-squared = 1.064 for 57 degrees of freedom
# Null hypothesis probability = 3.459926e-01
Photon flux (15-150 keV) in 62.47 sec: 5.25559E-02 ( -0.0175386 0.0176235 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.0348e-07 ( -8.25753e-08 9.33196e-08 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
0.000000 45.474400
47.000000 64.000000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -9.99970 ( )
Epeak [keV] : 25.5630 ( )
Norm@50keV : 3.50505E+05 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.85 using 59 PHA bins.
# Reduced chi-squared = 0.9615 for 56 degrees of freedom
# Null hypothesis probability = 5.568746e-01
Photon flux (15-150 keV) in 62.47 sec: 4.87845E-02 4.86920E-02 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.71062e-18 ( 0 0 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
0.000000 45.474400
47.000000 64.000000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -6.28417 -5 )
beta : -3.25160 ( 3.26485 1.20608 )
Epeak [keV] : 26.2084 ( -4.45336 5.47236 )
Norm@50keV : 57.1069 ( -16.8222 133.637 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.24 using 59 PHA bins.
# Reduced chi-squared = 0.9862 for 55 degrees of freedom
# Null hypothesis probability = 5.035394e-01
Photon flux (15-150 keV) in 62.47 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.70694e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 7.51317 (-1.88057 2.83185)
R^2/D10^2 : 8.07495E-02 (-0.0807496 0.171681)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.28 using 59 PHA bins.
# Reduced chi-squared = 1.005 for 57 degrees of freedom
# Null hypothesis probability = 4.646241e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.894e-08 3.014e-08
25- 50 7.659e-08 4.698e-08
50-150 1.628e-08 1.414e-08
15-150 1.418e-07 8.958e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 48.9779 (-27.1552 -48.9781)
Norm : 0.306286 (-0.131255 0.247211)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.47 using 59 PHA bins.
# Reduced chi-squared = 1.043 for 57 degrees of freedom
# Null hypothesis probability = 3.858741e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.656e-08 2.908e-08
25- 50 6.637e-08 4.057e-08
50-150 6.319e-08 5.007e-08
15-150 1.761e-07 1.139e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.12364 (-7.121 2.83823)
R1^2/D10^2 : 9.52965E-02 (-0.0954045 0.282114)
kT2 [keV] : 74.3618 (-74.1908 -74.1908)
R2^2/D10^2 : 1.63903E-05 (-1.65231e-05 -1.65231e-05)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.69 using 59 PHA bins.
# Reduced chi-squared = 1.031 for 55 degrees of freedom
# Null hypothesis probability = 4.117859e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.985e-08 3.054e-08
25- 50 7.345e-08 4.845e-08
50-150 7.045e-08 2.586e-08
15-150 1.938e-07 9.855e-08
Peak spectrum fit
Power-law model
Time interval is from 47.000 sec. to 64.000 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.97924 ( -0.560516 0.645733 )
Norm@50keV : 3.53736E-04 ( -0.000158349 0.000158154 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.64 using 59 PHA bins.
# Reduced chi-squared = 1.064 for 57 degrees of freedom
# Null hypothesis probability = 3.459926e-01
Photon flux (15-150 keV) in 62.47 sec: 5.25559E-02 ( -0.0175386 0.0176235 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.0348e-07 ( -8.25753e-08 9.33196e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 47.000 sec. to 64.000 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -9.99970 ( )
Epeak [keV] : 25.5630 ( )
Norm@50keV : 3.50505E+05 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.85 using 59 PHA bins.
# Reduced chi-squared = 0.9615 for 56 degrees of freedom
# Null hypothesis probability = 5.568746e-01
Photon flux (15-150 keV) in 62.47 sec: 4.87845E-02 4.86920E-02 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.71062e-18 ( 0 0 ) ergs/cm2
Band function
Time interval is from 47.000 sec. to 64.000 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -6.28313 -5 )
beta : -3.25160 ( 3.26485 1.20608 )
Epeak [keV] : 26.2084 ( -4.45336 5.47236 )
Norm@50keV : 57.1069 ( -16.8222 133.637 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.24 using 59 PHA bins.
# Reduced chi-squared = 0.9862 for 55 degrees of freedom
# Null hypothesis probability = 5.035394e-01
Photon flux (15-150 keV) in 62.47 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.70694e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 7.51317 (-1.88057 2.83185)
R^2/D10^2 : 8.07495E-02 (-0.0807496 0.171681)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.28 using 59 PHA bins.
# Reduced chi-squared = 1.005 for 57 degrees of freedom
# Null hypothesis probability = 4.646241e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.894e-08 2.974e-08
25- 50 7.659e-08 4.757e-08
50-150 1.628e-08 1.460e-08
15-150 1.418e-07 8.711e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 48.9779 (-27.1552 -48.9781)
Norm : 0.306286 (-0.131255 0.247211)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.47 using 59 PHA bins.
# Reduced chi-squared = 1.043 for 57 degrees of freedom
# Null hypothesis probability = 3.858741e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.656e-08 2.844e-08
25- 50 6.637e-08 4.001e-08
50-150 6.319e-08 4.985e-08
15-150 1.761e-07 1.185e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.12364 (-7.121 2.83823)
R1^2/D10^2 : 9.52965E-02 (-0.0954045 0.281108)
kT2 [keV] : 74.3618 (-74.1908 -74.1908)
R2^2/D10^2 : 1.63903E-05 (-1.65231e-05 -1.65231e-05)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.69 using 59 PHA bins.
# Reduced chi-squared = 1.031 for 55 degrees of freedom
# Null hypothesis probability = 4.117859e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.985e-08 3.083e-08
25- 50 7.345e-08 4.891e-08
50-150 7.045e-08 3.198e-08
15-150 1.938e-07 9.339e-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: 1.97924 ( -0.560516 0.645733 )
Norm@50keV : 3.53736E-04 ( -0.000158349 0.000158154 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.64 using 59 PHA bins.
# Reduced chi-squared = 1.064 for 57 degrees of freedom
# Null hypothesis probability = 3.459926e-01
Photon flux (15-150 keV) in 62.47 sec: 5.25559E-02 ( -0.0175386 0.0176235 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.0348e-07 ( -8.25753e-08 9.33196e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -9.99970 ( )
Epeak [keV] : 25.5630 ( )
Norm@50keV : 3.50505E+05 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.85 using 59 PHA bins.
# Reduced chi-squared = 0.9615 for 56 degrees of freedom
# Null hypothesis probability = 5.568746e-01
Photon flux (15-150 keV) in 62.47 sec: 4.87845E-02 4.86920E-02 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.71062e-18 ( 0 0 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -6.2825 -5 )
beta : -3.25160 ( 3.26485 1.20608 )
Epeak [keV] : 26.2084 ( -4.45336 5.47236 )
Norm@50keV : 57.1069 ( -16.8222 133.637 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.24 using 59 PHA bins.
# Reduced chi-squared = 0.9862 for 55 degrees of freedom
# Null hypothesis probability = 5.035394e-01
Photon flux (15-150 keV) in 62.47 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 1.70694e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 6.09e-08
S(50-100 keV) = 6.17e-08
T90 vs. Hardness ratio plot
T90 = 64 sec.
Hardness ratio (energy fluence ratio) = 1.01314
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.822205
Count Ratio (50-100 keV) / (15-25 keV) = 0.200052
Mask shadow pattern
IMX = -2.562928465010754E-01, IMY = -1.532945335447412E-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 45.474400
47.000000 64.000000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6740 21.9965 4.4 57.9 -26.0 1.6737 2.6 2.5 Crab
102.8027 -68.0908 2.5 41.4 112.4 1.9239 4.6 ------ UNKNOWN
79.6838 -34.0886 2.3 12.8 52.4 0.4823 5.1 ------ UNKNOWN
104.2409 5.6903 2.4 54.0 4.8 1.5726 4.8 ------ UNKNOWN
26.6221 -38.5459 2.8 31.0 -158.4 0.4425 4.0 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
249.500600 725.600620
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.3985 35.4037 4.4 57.1 5.1 5.7367 2.6 4.7 Her X-1
201.2187 -9.7117 3.2 40.8 98.0 5.7831 3.6 ------ UNKNOWN
172.8381 -5.8812 2.3 36.7 143.6 3.3137 5.0 ------ UNKNOWN
253.5005 41.2489 3.6 55.2 -1.7 3.8469 3.2 ------ UNKNOWN
262.1561 52.1530 2.9 59.4 -15.5 11.4047 4.0 ------ UNKNOWN
159.2118 64.6704 3.2 40.0 -76.8 5.2224 3.6 ------ UNKNOWN
Plot creation:
Fri Apr 27 15:54:28 EDT 2018