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
300.4550 +35.3333 0.0127 4.7 -40.7 3.0479 15.1 TRIG_01205107
------------------------------------------
Foreground time interval of the image:
-12.899 111.201 (delta_t = 124.100 [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
-82.804000 244.280000
245.000000 375.710000
377.000000 429.870000
431.000000 436.650000
438.000000 531.880000
533.000000 593.920000
595.000000 720.700000
721.000000 725.956000
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.23652 ( -0.07959 0.0809803 )
Norm@50keV : 1.09096E-03 ( -4.95126e-05 4.90737e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.91 using 59 PHA bins.
# Reduced chi-squared = 0.9457 for 57 degrees of freedom
# Null hypothesis probability = 5.918703e-01
Photon flux (15-150 keV) in 801.8 sec: 0.184152 ( -0.00733294 0.00736777 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.26912e-06 ( -3.22353e-07 3.2384e-07 ) ergs/cm2
Cutoff power-law model
Multiple GTIs in the spectrum
tstart tstop
-82.804000 244.280000
245.000000 375.710000
377.000000 429.870000
431.000000 436.650000
438.000000 531.880000
533.000000 593.920000
595.000000 720.700000
721.000000 725.956000
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.99315 ( -0.289767 -1.99315 )
Epeak [keV] : 1.23659 ( -0.326735 0.628796 )
Norm@50keV : 1.47904E-03 ( -0.000119794 0.000123355 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.99 using 59 PHA bins.
# Reduced chi-squared = 0.9462 for 56 degrees of freedom
# Null hypothesis probability = 5.897215e-01
Photon flux (15-150 keV) in 801.8 sec: 0.181484 ( -0.008492 0.008469 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.10131e-06 ( -4.26437e-07 4.2784e-07 ) ergs/cm2
Band function
Multiple GTIs in the spectrum
tstart tstop
-82.804000 244.280000
245.000000 375.710000
377.000000 429.870000
431.000000 436.650000
438.000000 531.880000
533.000000 593.920000
595.000000 720.700000
721.000000 725.956000
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.13998 ( )
beta : -8.12642 ( )
Epeak [keV] : 64.7600 ( )
Norm@50keV : 2.48026E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 152.25 using 59 PHA bins.
# Reduced chi-squared = 2.7682 for 55 degrees of freedom
# Null hypothesis probability = 4.590304e-11
Photon flux (15-150 keV) in 801.8 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 8.07509e-06 ( -8.06948e-06 -1.87292e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 9.65082 ( )
R^2/D10^2 : 8.69598E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 201.34 using 59 PHA bins.
# Reduced chi-squared = 3.5323 for 57 degrees of freedom
# Null hypothesis probability = 5.451309e-18
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.305e-06 8.419e-08
25- 50 3.084e-06 1.115e-07
50-150 1.451e-06 1.475e-07
15-150 5.840e-06 2.197e-07
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 51.1272 (-5.32381 6.64549)
Norm : 0.984060 (-0.070271 0.0834704)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.939e-06 1.211e-07
25- 50 2.807e-06 1.106e-07
50-150 2.783e-06 2.682e-07
15-150 7.528e-06 3.115e-07
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.62298 (-0.716155 0.782521)
R1^2/D10^2 : 0.583093 (-0.224789 0.423737)
kT2 [keV] : 18.7463 (-2.81005 4.24511)
R2^2/D10^2 : 4.32527E-03 (-0.00240411 0.00427475)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.019e-06 2.454e-07
25- 50 2.681e-06 2.622e-07
50-150 3.060e-06 5.637e-07
15-150 7.761e-06 9.397e-07
Peak spectrum fit
Power-law model
Time interval is from 111.300 sec. to 112.300 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.67734 ( -0.558363 0.606733 )
Norm@50keV : 3.36312E-03 ( -0.00121349 0.00113645 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.75 using 59 PHA bins.
# Reduced chi-squared = 0.9078 for 57 degrees of freedom
# Null hypothesis probability = 6.719009e-01
Photon flux (15-150 keV) in 1 sec: 0.443182 ( -0.133403 0.133435 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.11975e-08 ( -1.1225e-08 1.18662e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 111.300 sec. to 112.300 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.31052 ( -4.0043 0.103347 )
Epeak [keV] : 112.039 ( )
Norm@50keV : 1.57205E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.66 using 59 PHA bins.
# Reduced chi-squared = 0.9225 for 56 degrees of freedom
# Null hypothesis probability = 6.396811e-01
Photon flux (15-150 keV) in 1 sec: 0.443276 ( -0.133286 0.133236 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.12296e-08 ( -1.23235e-08 1.15951e-08 ) ergs/cm2
Band function
Time interval is from 111.300 sec. to 112.300 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.84349 ( -4.84349 -4.84349 )
beta : -1.80816 ( -1.18499 0.639078 )
Epeak [keV] : 23.8161 ( -23.8161 12.8747 )
Norm@50keV : 441.259 ( -132.135 4.40163e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.52 using 59 PHA bins.
# Reduced chi-squared = 0.9368 for 55 degrees of freedom
# Null hypothesis probability = 6.082842e-01
Photon flux (15-150 keV) in 1 sec: ( ) 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] : 10.5419 (-3.19113 4.93507)
R^2/D10^2 : 0.172542 (-0.172437 0.481574)
(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 3.967e-09 2.545e-09
25- 50 1.061e-08 6.295e-09
50-150 6.438e-09 5.040e-09
15-150 2.101e-08 1.394e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 131.756 (-92.8993 -132.019)
Norm : 1.85947 (-0.601809 1.09089)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.821e-09 2.868e-09
25- 50 8.760e-09 5.225e-09
50-150 1.634e-08 1.134e-08
15-150 2.992e-08 1.939e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.58542 (-3.49728 3.57646)
R1^2/D10^2 : 0.328039 (-0.248582 1.68837)
kT2 [keV] : 198.080 (-198.188 -198.188)
R2^2/D10^2 : 6.18005E-05 (-4.5875e-05 0.0238603)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.663e-09 2.848e-09
25- 50 9.705e-09 5.760e-09
50-150 1.920e-08 4.131e-09
15-150 3.357e-08 1.262e-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: 2.21761 ( -0.143014 0.149273 )
Norm@50keV : 1.20413E-03 ( -0.000119264 0.000117565 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.36 using 59 PHA bins.
# Reduced chi-squared = 1.269 for 57 degrees of freedom
# Null hypothesis probability = 8.266497e-02
Photon flux (15-150 keV) in 124.1 sec: 0.201212 ( -0.0141911 0.0141975 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.40856e-06 ( -1.18013e-07 1.20169e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.49241 ( -1.00096 0.507748 )
Epeak [keV] : 26.2919 ( )
Norm@50keV : 3.34098E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 69.98 using 59 PHA bins.
# Reduced chi-squared = 1.250 for 56 degrees of freedom
# Null hypothesis probability = 9.918831e-02
Photon flux (15-150 keV) in 124.1 sec: 0.194517 ( -0.015892 0.015929 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.28658e-06 ( -1.55171e-07 1.76507e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.754316 ( -1.42051 2.86735 )
beta : -2.65149 ( -1.13491 0.386594 )
Epeak [keV] : 28.6528 ( -9.48226 5.70581 )
Norm@50keV : 1.05096E-02 ( -0.0109425 1.78864 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.91 using 59 PHA bins.
# Reduced chi-squared = 1.217 for 55 degrees of freedom
# Null hypothesis probability = 1.302402e-01
Photon flux (15-150 keV) in 124.1 sec: ( ) 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) = 2.64e-06
S(50-100 keV) = 2.24e-06
T90 vs. Hardness ratio plot
T90 = 453.535999894142 sec.
Hardness ratio (energy fluence ratio) = 0.848485
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.882744
Count Ratio (50-100 keV) / (15-25 keV) = 0.387694
Mask shadow pattern
IMX = 6.199327220684352E-02, IMY = 5.339522143020229E-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:
-12.899410 111.200600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.4894 35.3233 17.7 41.5 -19.4 0.2270 0.7 1.9 Her X-1
288.7195 10.9706 4.9 29.6 -87.8 -0.7655 -2.3 4.9 GRS 1915+105
299.7860 35.1782 6.5 5.2 -41.4 -0.3607 -1.8 9.7 Cyg X-1
308.1919 41.0560 4.9 5.3 72.5 0.4859 2.4 7.2 Cyg X-3
326.2006 38.3642 5.5 16.1 131.2 0.4486 2.1 2.9 Cyg X-2
337.7344 50.8817 2.5 27.0 102.3 1.4038 4.6 ------ UNKNOWN
300.4535 35.3329 0.8 4.7 -40.7 2.9967 14.8 ------ UNKNOWN
238.9310 27.6759 2.7 56.6 -22.3 3.8214 4.3 ------ UNKNOWN
286.6953 -0.3330 2.2 40.6 -93.5 4.4198 5.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
146.800600 244.280000
245.000000 375.710000
377.000000 429.870000
431.000000 436.650000
438.000000 531.880000
533.000000 593.920000
595.000000 720.700000
721.000000 864.130000
865.000000 866.500000
868.000000 868.860000
870.000000 963.084600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
254.2886 35.2200 0.0 37.3 -10.6 -1.6103 -1.0 11.1 Her X-1
288.6990 10.8212 52.5 26.7 -87.8 0.2991 0.2 9.5 GRS 1915+105
299.7180 35.0666 8.3 0.7 -48.5 1.5093 1.4 10.2 Cyg X-1
308.0188 41.1358 11.1 8.3 109.2 -1.1312 -1.0 11.7 Cyg X-3
325.9944 38.3809 9.2 20.6 139.7 1.4831 1.3 9.1 Cyg X-2
300.4324 35.2809 0.7 0.1 -99.8 17.6625 17.0 ------ UNKNOWN
235.5477 25.9348 2.4 55.7 -14.7 14.7175 4.8 ------ UNKNOWN
292.4059 -5.4419 2.4 41.5 -102.1 24.3719 4.8 ------ UNKNOWN
Plot creation:
Fri Dec 29 10:16:09 EST 2023