Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
153.3673 11.5445 0.0075 29.0121 -13.7398 1.3219394 25.693 TRIG_01259578
Foreground time interval of the image:
-0.044 15.365 (delta_t = 15.409 [sec])
Background time interval of the image:
-239.736 -0.044 (delta_t = 239.692 [sec])
Lightcurves
Notes:
- 1) The mask-weighted light curves are using the flight position.
- 2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 3) 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.
- 4) 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.
- 5) 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
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.384000
8 ms binning
From T100_start-3 s to T100_start+3 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.384000
2 ms binning
From T100_start-1 s to T100_start+1 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.384000
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Quad-rate summed light curves (from T0-300s to T0+1000s)
Spectral Evolution
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using 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.
Time averaged spectrum fit using the average DRM
Power-law model
Time interval is from -0.044 sec. to 35.124 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.87833 ( -0.0751384 0.0760284 )
Norm@50keV : 6.13812E-03 ( -0.000257712 0.000256369 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.01 using 59 bins.
Reduced chi-squared = 0.894912
# Null hypothesis probability of 6.98e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 35.17 sec: 0.872944 ( -0.036361 0.036474 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.98487e-06 ( -8.29949e-08 8.32797e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.044 sec. to 35.124 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.68261 ( -0.305137 0.247448 )
Epeak [keV] : 78.4550 ( -24.1809 -78.4581 )
Norm@50keV : 7.73174E-03 ( -0.00130435 0.00326611 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.66 using 59 bins.
Reduced chi-squared = 0.886786
# Null hypothesis probability of 7.12e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 35.17 sec: 0.861299 ( -0.039917 0.040019 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.95129e-06 ( -9.62979e-08 9.60598e-08 ) ergs/cm2
Band function
Time interval is from -0.044 sec. to 35.124 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) 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] : 12.1965 ( )
R^2/D10^2 : 0.184643 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 204.57 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.67e-18 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.046e-07 1.570e-08
25- 50 6.561e-07 3.077e-08
50-150 5.931e-07 5.346e-08
15-150 1.454e-06 6.436e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 94.7635 (-12.9891 16.5704)
Norm : 3.81765 (-0.235287 0.257117)
------------------------------------------------------------
#Fit statistic : Chi-Squared 53.76 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 5.97e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.508e-07 2.780e-08
25- 50 5.999e-07 2.726e-08
50-150 9.423e-07 2.506e-07
15-150 1.893e-06 2.640e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.66392 (-0.845241 0.881802)
R1^2/D10^2 : 1.28876 (-0.453486 0.830497)
kT2 [keV] : 23.9867 (-3.41083 4.90058)
R2^2/D10^2 : 1.08307E-02 (-0.00539699 0.00896281)
------------------------------------------------------------
#Fit statistic : Chi-Squared 54.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.77e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.453e-07 4.423e-08
25- 50 5.967e-07 6.049e-08
50-150 9.784e-07 1.609e-07
15-150 1.920e-06 2.638e-07
Peak spectrum fit
Power-law model
Time interval is from -0.040 sec. to 0.960 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48252 ( -0.0954366 0.0959677 )
Norm@50keV : 3.45746E-02 ( -0.00197553 0.00196781 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.54 using 59 bins.
Reduced chi-squared = 0.886667
# Null hypothesis probability of 7.14e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.29640 ( -0.24606 0.24628 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.28996e-07 ( -2.04784e-08 2.05707e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.040 sec. to 0.960 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.22703 ( -0.39606 0.300703 )
Epeak [keV] : 152.542 ( -64.4811 -152.547 )
Norm@50keV : 4.66035E-02 ( -0.0132779 0.0266015 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.13 using 59 bins.
Reduced chi-squared = 0.877321
# Null hypothesis probability of 7.31e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 4.25644 ( -0.25266 0.25264 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.23437e-07 ( -2.22543e-08 2.20964e-08 ) ergs/cm2
Band function
Time interval is from -0.040 sec. to 0.960 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) 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] : 14.7113 ( )
R^2/D10^2 : 0.524591 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 122.65 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.04e-06 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.384e-08 2.605e-09
25- 50 9.303e-08 6.505e-09
50-150 1.358e-07 1.685e-08
15-150 2.527e-07 1.720e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-29.394 -200)
Norm : 17.6162 (-0.985257 0.985257)
------------------------------------------------------------
#Fit statistic : Chi-Squared 50.64 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.11e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.401e-08 2.710e-09
25- 50 8.466e-08 5.330e-09
50-150 1.857e-07 1.255e-08
15-150 3.143e-07 2.340e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.68051 (-1.36337 1.45207)
R1^2/D10^2 : 2.40216 (-0.890918 1.65267)
kT2 [keV] : 36.2426 (-9.12897 23.3045)
R2^2/D10^2 : 1.73538E-02 (-0.0129454 0.0290834)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.42 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.18e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.770e-08 7.115e-09
25- 50 9.018e-08 1.472e-08
50-150 1.991e-07 8.424e-08
15-150 3.270e-07 9.525e-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: 1.77913 ( -0.111984 0.113903 )
Norm@50keV : 5.39868E-03 ( -0.00036844 0.000365067 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 68.74 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.37e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 15.41 sec: 0.737994 ( -0.0466692 0.0467223 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.66524e-07 ( -5.35739e-08 5.39684e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.56114 ( -0.469968 0.310265 )
Epeak [keV] : 92.4819 ( -36.7304 -92.4959 )
Norm@50keV : 7.08403E-03 ( -0.0018429 0.00552593 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.99 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.31e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 15.41 sec: 0.730595 ( -0.02446 0.048752 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.51279e-07 ( -6.19636e-08 6.06846e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in 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) = 5.73e-07
S(50-100 keV) = 6.26e-07
T90 vs. Hardness ratio plot
T90 = 30.8559999465942 sec.
Hardness ratio (energy fluence ratio) = 1.0925
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.12687
Count Ratio (50-100 keV) / (15-25 keV) = 0.656814
Mask shadow pattern
IMX = 5.387142560627157E-01, IMY = 1.317210281828195E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.384000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.384000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.384000
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:
-239.736000 -0.044000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.044000 15.364590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
147.4213 71.7921 2.5 34.9 129.6 0.3892 4.6 ------ UNKNOWN
232.3002 56.8851 1.8 46.2 -176.5 0.5397 6.4 ------ UNKNOWN
153.3673 11.5445 0.4 29.0 -13.7 1.3220 25.7 ------ UNKNOWN
221.5370 33.5629 2.5 44.4 -141.9 0.4452 4.6 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
85.164590 764.264600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5323 -40.5527 90.3 54.6 -4.5 0.1782 0.1 0.2 Vela X-1
163.2357 14.7455 2.8 10.1 -130.6 3.2659 4.1 ------ UNKNOWN
160.2727 -45.1162 3.1 57.0 -26.9 12.8050 3.7 ------ UNKNOWN
Plot creation:
Wed Dec 18 17:44:44 EST 2024