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
305.6688 -72.4314 0.0055 34.8187 -124.5726 8.6888983 34.389 TRIG_01202386
Foreground time interval of the image:
-5.368 14.637 (delta_t = 20.005 [sec])
Background time interval of the image:
-60.864 -5.368 (delta_t = 55.496 [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 1.024000
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 1.024000
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 1.024000
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 -5.368 sec. to 49.420 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25119 ( -0.0538469 0.0536518 )
Norm@50keV : 1.79607E-02 ( -0.000538575 0.000538445 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 69.43 using 59 bins.
Reduced chi-squared = 1.21807
# Null hypothesis probability of 1.25e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 54.79 sec: 2.12469 ( -0.06791 0.06802 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.84648e-06 ( -3.14316e-07 3.15106e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -5.368 sec. to 49.420 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.882333 ( -0.234526 0.222689 )
Epeak [keV] : 171.015 ( -45.0378 163.706 )
Norm@50keV : 2.63279E-02 ( -0.00530745 0.0070244 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 61.21 using 59 bins.
Reduced chi-squared = 1.09304
# Null hypothesis probability of 2.94e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 54.79 sec: 2.08175 ( -0.07218 0.07238 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.6534e-06 ( -3.39287e-07 3.37659e-07 ) ergs/cm2
Band function
Time interval is from -5.368 sec. to 49.420 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] : 19.0712 ( )
R^2/D10^2 : 0.112354 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 229.11 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.70e-22 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.395e-07 2.739e-08
25- 50 2.119e-06 9.369e-08
50-150 5.669e-06 2.772e-07
15-150 8.228e-06 2.959e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 8.98260 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 158.69 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.58e-11 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.225e-06 3.863e-08
25- 50 2.357e-06 7.999e-08
50-150 5.170e-06 1.745e-07
15-150 8.753e-06 2.931e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 8.71140 (-1.25523 1.42881)
R1^2/D10^2 : 0.847261 (-0.289765 0.507493)
kT2 [keV] : 31.3292 (-3.9374 6.46187)
R2^2/D10^2 : 1.74316E-02 (-0.008173 0.0106921)
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.31e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.165e-07 9.616e-08
25- 50 2.256e-06 1.786e-07
50-150 6.569e-06 6.410e-07
15-150 9.641e-06 9.205e-07
Peak spectrum fit
Power-law model
Time interval is from 12.572 sec. to 13.572 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.892976 ( -0.0938206 0.0921557 )
Norm@50keV : 9.89504E-02 ( -0.00549766 0.00547629 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 67.55 using 59 bins.
Reduced chi-squared = 1.18509
# Null hypothesis probability of 1.60e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 0.606597 ( -0.030182 0.061394 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.11365e-06 ( -6.41076e-08 6.42543e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 12.572 sec. to 13.572 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.608339 ( -0.388363 0.318442 )
Epeak [keV] : 296.024 ( -135.166 -296.024 )
Norm@50keV : 0.130861 ( -0.0344049 0.0574791 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 65.70 using 59 bins.
Reduced chi-squared = 1.17321
# Null hypothesis probability of 1.76e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.38775E-04 ( -0.000138775 -0.000138775 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.10599e-06 ( -6.56387e-08 6.55038e-08 ) ergs/cm2
Band function
Time interval is from 12.572 sec. to 13.572 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] : 24.9228 (-1.79144 2.00383)
R^2/D10^2 : 0.288780 (-0.0606389 0.0743943)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 111.52 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.14e-05 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.121e-08 3.780e-09
25- 50 1.768e-07 1.400e-08
50-150 8.147e-07 6.610e-08
15-150 1.023e-06 7.090e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 45.1596 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared 201.86 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 4.52e-18 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.125e-07 7.250e-09
25- 50 2.163e-07 1.605e-08
50-150 4.744e-07 1.110e-07
15-150 8.032e-07 1.053e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.12626 (-1.61569 2.13869)
R1^2/D10^2 : 6.27431 (-3.53763 9.21296)
kT2 [keV] : 33.0785 (-4.04182 6.26974)
R2^2/D10^2 : 0.110943 (-0.0463363 0.0567716)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.24 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.08e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.998e-08 2.607e-08
25- 50 1.883e-07 4.430e-08
50-150 8.584e-07 1.240e-07
15-150 1.117e-06 1.735e-07
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: 1.15743 ( -0.0603338 0.0599587 )
Norm@50keV : 3.01572E-02 ( -0.00103089 0.00103019 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 66.42 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.84e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 20 sec: 3.52010 ( -0.126412 0.126587 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.19522e-06 ( -2.24714e-07 2.25052e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.768775 ( -0.263712 0.248717 )
Epeak [keV] : 181.408 ( -50.6836 205.112 )
Norm@50keV : 4.49284E-02 ( -0.00989442 0.0135147 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.11 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.63e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 20 sec: 3.45349 ( -0.13267 0.13288 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.08438e-06 ( -2.3988e-07 2.3872e-07 ) 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) = 2.13e-06
S(50-100 keV) = 3.58e-06
T90 vs. Hardness ratio plot
T90 = 27.635999917984 sec.
Hardness ratio (energy fluence ratio) = 1.68075
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.75756
Count Ratio (50-100 keV) / (15-25 keV) = 1.63601
Mask shadow pattern
IMX = -3.946623614373017E-01, IMY = 5.726816273078305E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 1.024000
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:
-60.864000 -5.368000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
37.6571 -28.0064 2.6 31.6 84.7 1.7794 4.4 ------ UNKNOWN
323.3415 -24.5655 2.0 42.6 -42.5 2.6147 5.7 ------ UNKNOWN
209.3041 -74.2015 3.0 55.0 -145.4 5.4037 3.8 ------ UNKNOWN
311.7520 -32.4721 2.5 44.4 -61.1 5.1089 4.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-5.368000 14.636600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
10.1890 1.6620 3.3 51.7 30.7 2.2033 3.5 ------ UNKNOWN
337.1696 -20.5096 2.4 38.1 -23.0 0.9037 4.8 ------ UNKNOWN
305.6689 -72.4314 0.3 34.8 -124.6 8.6882 34.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
88.836600 481.636600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.4314 -60.4623 13.5 43.6 171.5 1.5040 0.9 10.2 Cen X-3
186.5147 -62.8857 9.9 38.6 -179.0 1.5313 1.2 7.9 GX 301-2
264.8492 -44.5841 21.1 33.8 -95.8 0.8099 0.5 9.2 4U 1735-44
145.5902 -60.0095 3.1 46.8 154.8 9.7704 3.7 ------ UNKNOWN
343.8640 -40.2967 2.7 37.1 12.6 4.7571 4.2 ------ UNKNOWN
175.1518 -58.2136 2.4 45.0 175.8 9.0972 4.9 ------ UNKNOWN
287.9265 -29.1171 2.6 44.4 -61.2 18.1806 4.5 ------ UNKNOWN
Plot creation:
Tue Dec 26 16:58:13 EST 2023