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
12.1669 -19.7605 0.0838 41.3 -3.0 0.0371 2.3 TRIG_01235109
------------------------------------------
Foreground time interval of the image:
0.000 1.024 (delta_t = 1.024 [sec])
Background time interval of the image:
-138.879 -133.250 (delta_t = 5.629 [sec])
-132.480 -122.140 (delta_t = 10.340 [sec])
-121.480 -4.480 (delta_t = 117.000 [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 0.000 sec. to 1.024 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 4.47517 ( -1.0137 1.533 )
Norm@50keV : 5.36717E-04 ( -0.000549036 0.000993015 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.40 using 59 PHA bins.
# Reduced chi-squared = 1.112 for 57 degrees of freedom
# Null hypothesis probability = 2.610693e-01
Photon flux (15-150 keV) in 1.024 sec: 0.509628 ( -0.202146 0.208354 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.76599e-08 ( -3.66211e-09 8.97238e-09 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 1.024 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 3.76122E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 81.13 using 59 PHA bins.
# Reduced chi-squared = 1.449 for 56 degrees of freedom
# Null hypothesis probability = 1.570175e-02
Photon flux (15-150 keV) in 1.024 sec: 0.622793 0.626070 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.78805e-16 ( 0 0 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 1.024 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -6.85529 -5 )
beta : -10.0000 ( 10 10 )
Epeak [keV] : 15.8745 ( -2.86061 2.91793 )
Norm@50keV : 3.28052E+04 ( -10741.8 147361 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.50 using 59 PHA bins.
# Reduced chi-squared = 1.046 for 55 degrees of freedom
# Null hypothesis probability = 3.826348e-01
Photon flux (15-150 keV) in 1.024 sec: 0.608272 ( 6.39173 -0.201162 ) 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] : 3.31928 (-0.777453 0.951512)
R^2/D10^2 : 44.3872 (-44.0036 161.982)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.92 using 59 PHA bins.
# Reduced chi-squared = 1.034 for 57 degrees of freedom
# Null hypothesis probability = 4.049533e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.551e-08 9.108e-09
25- 50 3.175e-09 2.146e-09
50-150 1.116e-11 1.378e-11
15-150 1.869e-08 1.119e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 7.11935 (-2.62696 4.80316)
Norm : 42.2839 (-42.2977 120.639)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.426e-08 8.448e-09
25- 50 3.647e-09 2.537e-09
50-150 8.594e-11 9.564e-11
15-150 1.799e-08 1.077e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.03956E-04 (-0.000103956 -0.000103956)
R1^2/D10^2 : 7504.54 (-7505.96 -7505.96)
kT2 [keV] : 3.33612 (-0.767956 0.960291)
R2^2/D10^2 : 43.2146 (-43.5168 162.952)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.537e-08 1.330e-02
25- 50 4.428e-09 1.098e-01
50-150 3.318e-11 2.635e+00
15-150 1.983e-08 3.220e+00
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 1.024 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 4.47517 ( -1.0137 1.533 )
Norm@50keV : 5.36717E-04 ( -0.000549036 0.000993015 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.40 using 59 PHA bins.
# Reduced chi-squared = 1.112 for 57 degrees of freedom
# Null hypothesis probability = 2.610693e-01
Photon flux (15-150 keV) in 1.024 sec: 0.509628 ( -0.202146 0.208354 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.76599e-08 ( -3.66211e-09 8.97238e-09 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 1.024 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00000 ( )
Epeak [keV] : 50.0000 ( )
Norm@50keV : 3.76122E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 81.13 using 59 PHA bins.
# Reduced chi-squared = 1.449 for 56 degrees of freedom
# Null hypothesis probability = 1.570175e-02
Photon flux (15-150 keV) in 1.024 sec: 0.622793 0.626070 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.78805e-16 ( 0 0 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 1.024 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -6.85529 -5 )
beta : -10.0000 ( 10 10 )
Epeak [keV] : 15.8745 ( -2.86061 2.91793 )
Norm@50keV : 3.28052E+04 ( -10741.8 147361 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.50 using 59 PHA bins.
# Reduced chi-squared = 1.046 for 55 degrees of freedom
# Null hypothesis probability = 3.826348e-01
Photon flux (15-150 keV) in 1.024 sec: 0.608272 ( 6.39173 -0.201162 ) 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] : 3.31928 (-0.777453 0.951512)
R^2/D10^2 : 44.3872 (-44.0036 161.982)
(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 1.551e-08 9.206e-09
25- 50 3.175e-09 2.245e-09
50-150 1.116e-11 1.490e-11
15-150 1.869e-08 1.140e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 7.11935 (-2.62696 4.80316)
Norm : 42.2839 (-42.2977 120.639)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.426e-08 8.172e-09
25- 50 3.647e-09 2.489e-09
50-150 8.594e-11 1.057e-10
15-150 1.799e-08 1.144e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.03956E-04 (-0.000103956 -0.000103956)
R1^2/D10^2 : 7504.54 (-7505.96 -7505.96)
kT2 [keV] : 3.33612 (-0.767956 0.960291)
R2^2/D10^2 : 43.2146 (-43.5168 162.952)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.537e-08 1.375e-02
25- 50 4.428e-09 1.062e-01
50-150 3.318e-11 2.864e+00
15-150 1.983e-08 2.926e+00
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: 4.47517 ( -1.0137 1.533 )
Norm@50keV : 5.36717E-04 ( -0.000549036 0.000993015 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.40 using 59 PHA bins.
# Reduced chi-squared = 1.112 for 57 degrees of freedom
# Null hypothesis probability = 2.610693e-01
Photon flux (15-150 keV) in 1.024 sec: 0.509628 ( -0.202146 0.208354 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.76599e-08 ( -3.66211e-09 8.97238e-09 ) 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 : 3.76122E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 81.13 using 59 PHA bins.
# Reduced chi-squared = 1.449 for 56 degrees of freedom
# Null hypothesis probability = 1.570175e-02
Photon flux (15-150 keV) in 1.024 sec: 0.622793 0.626070 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.78805e-16 ( 0 0 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -6.85529 -5 )
beta : -10.0000 ( 10 10 )
Epeak [keV] : 15.8745 ( -2.86061 2.91793 )
Norm@50keV : 3.28052E+04 ( -10741.8 147361 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.50 using 59 PHA bins.
# Reduced chi-squared = 1.046 for 55 degrees of freedom
# Null hypothesis probability = 3.826348e-01
Photon flux (15-150 keV) in 1.024 sec: 0.608272 ( 6.39173 -0.201162 ) 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) = 4.13e-09
S(50-100 keV) = 7.59e-10
T90 vs. Hardness ratio plot
T90 = 1.0239999294281 sec.
Hardness ratio (energy fluence ratio) = 0.183777
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = -0.148566
Count Ratio (50-100 keV) / (15-25 keV) = -0.120859
Mask shadow pattern
IMX = 8.759555915424727E-01, IMY = 4.615584049207516E-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:
-138.879420 -133.250000
-132.480000 -122.140000
-121.480000 -4.480000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.1496 38.3660 10.9 35.6 140.6 0.4323 1.1 2.9 Cyg X-2
27.7935 -29.5210 2.1 55.7 -15.6 3.1329 5.4 ------ UNKNOWN
44.8543 17.1409 2.6 41.0 -81.1 3.2826 4.5 ------ UNKNOWN
43.9208 2.6259 3.2 44.8 -60.4 3.2922 3.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 1.024000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
326.3877 38.2716 0.0 35.4 140.6 -0.0551 -2.9 10.6 Cyg X-2
1.2251 -8.0126 2.0 28.2 13.0 0.0675 5.7 486.3 UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
112.820600 135.750000
137.520000 247.160000
248.520000 249.840000
251.520000 270.310000
271.520000 278.180000
279.520000 302.550000
303.520000 304.390000
305.520000 309.870000
310.520000 962.551700
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
1.4667 -60.0985 2.7 41.0 40.0 9.2213 4.3 ------ UNKNOWN
349.4647 -28.3804 2.8 22.4 94.9 5.8359 4.2 ------ UNKNOWN
49.3488 -0.8199 2.7 41.1 -81.0 14.6581 4.3 ------ UNKNOWN
45.2030 4.8512 2.5 40.8 -91.7 18.9687 4.6 ------ UNKNOWN
27.6450 25.9167 3.2 48.1 -129.2 17.3998 3.6 ------ UNKNOWN
Plot creation:
Thu Jun 6 19:02:00 EDT 2024