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
345.7947 35.5128 0.0156 37.6757 128.7829 1.3053611 12.364 TRIG_01252695
Foreground time interval of the image:
0.084 16.141 (delta_t = 16.057 [sec])
Background time interval of the image:
-239.760 0.084 (delta_t = 239.844 [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 0.084 sec. to 139.388 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.16690 ( -0.18626 0.181414 )
Norm@50keV : 1.37888E-03 ( -0.000142405 0.000141916 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.41 using 59 bins.
Reduced chi-squared = 1.05982
# Null hypothesis probability of 3.54e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 139.3 sec: 0.161139 ( -0.017405 0.017499 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.96763e-06 ( -2.16446e-07 2.17573e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.084 sec. to 139.388 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.01073 ( -0.765224 0.466022 )
Epeak [keV] : 352.231 ( -352.233 -352.233 )
Norm@50keV : 1.62762E-03 ( -0.000376238 0.00192904 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.25 using 59 bins.
Reduced chi-squared = 1.07589
# Null hypothesis probability of 3.25e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 139.3 sec: 0.159992 ( -0.018112 0.017983 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.95034e-06 ( -2.32189e-07 2.27126e-07 ) ergs/cm2
Band function
Time interval is from 0.084 sec. to 139.388 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] : 19.7552 (-2.72283 3.36627)
R^2/D10^2 : 7.66501E-03 (-0.00309431 0.00492588)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 79.16 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.77e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.072e-08 1.822e-08
25- 50 3.988e-07 6.533e-08
50-150 1.152e-06 2.080e-07
15-150 1.631e-06 2.177e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-26.3605 -200)
Norm : 0.677811 (-0.0710605 0.0710605)
------------------------------------------------------------
#Fit statistic : Chi-Squared 72.97 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.55e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.351e-07 8.827e-08
25- 50 4.522e-07 2.473e-07
50-150 9.917e-07 5.150e-07
15-150 1.679e-06 8.820e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.60305 (-2.75594 3.24696)
R1^2/D10^2 : 5.28888E-02 (-0.0305375 0.0549369)
kT2 [keV] : 41.0821 (-13.9313 92.8477)
R2^2/D10^2 : 6.09597E-04 (-0.000531591 0.00169091)
------------------------------------------------------------
#Fit statistic : Chi-Squared 59.11 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.28e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.544e-07 7.800e-08
25- 50 4.443e-07 2.172e-07
50-150 1.379e-06 7.208e-07
15-150 1.978e-06 9.850e-07
Peak spectrum fit
Power-law model
Time interval is from 0.084 sec. to 1.084 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00870 ( -0.2867 0.273204 )
Norm@50keV : 2.18169E-02 ( -0.00342368 0.0033884 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.28 using 59 bins.
Reduced chi-squared = 1.05754
# Null hypothesis probability of 3.58e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.51295 ( -0.40169 0.40307 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.35218e-07 ( -3.84339e-08 3.85735e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.084 sec. to 1.084 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.00269 ( -0.814806 0.332391 )
Epeak [keV] : 1.00000E+04 ( -10000 -10000 )
Norm@50keV : 2.19463E-02 ( -0.00342985 0.00333125 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 60.28 using 59 bins.
Reduced chi-squared = 1.07643
# Null hypothesis probability of 3.24e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.52134 ( -0.4336 0.41797 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.35586e-07 ( -4.10321e-08 4.03892e-08 ) ergs/cm2
Band function
Time interval is from 0.084 sec. to 1.084 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] : 25.8705 (-5.80074 8.14498)
R^2/D10^2 : 5.34171E-02 (-0.0294929 0.0638835)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.88 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.86e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.097e-09 2.166e-09
25- 50 3.519e-08 1.110e-08
50-150 1.736e-07 5.212e-08
15-150 2.149e-07 5.690e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 (-39.9481 -200)
Norm : 10.3570 (-1.65653 1.65653)
------------------------------------------------------------
#Fit statistic : Chi-Squared 71.83 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.93e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.579e-08 1.478e-08
25- 50 4.961e-08 2.837e-08
50-150 1.088e-07 6.120e-08
15-150 1.842e-07 1.039e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.86918 (-3.07372 4.22641)
R1^2/D10^2 : 2.21889 (-1.80856 22.6661)
kT2 [keV] : 38.6376 (-11.42 32.2471)
R2^2/D10^2 : 1.47922E-02 (-0.0117056 0.0275919)
------------------------------------------------------------
#Fit statistic : Chi-Squared 58.77 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.39e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.941e-08 1.084e-08
25- 50 4.148e-08 2.214e-08
50-150 1.838e-07 1.033e-07
15-150 2.447e-07 1.291e-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: 0.871622 ( -0.263054 0.243066 )
Norm@50keV : 4.92035E-03 ( -0.000728221 0.000708814 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.51e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 16.06 sec: 0.564698 ( -0.081565 0.0823473 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.96778e-07 ( -1.21747e-07 1.22185e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.867230 ( -0.267128 0.243576 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 4.95622E-03 ( -0.000682764 0.00707828 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 49.46 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.19e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 16.06 sec: 0.564764 ( -0.042051 0.08147 ) ph/cm2/s
Energy fluence (15-150 keV) : 8.96965e-07 ( -1.24537e-07 1.21622e-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) = 4.05e-07
S(50-100 keV) = 7.22e-07
T90 vs. Hardness ratio plot
T90 = 121.155999898911 sec.
Hardness ratio (energy fluence ratio) = 1.78272
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.90053
Count Ratio (50-100 keV) / (15-25 keV) = 1.64367
Mask shadow pattern
IMX = -4.836911996927961E-01, IMY = -6.019577487709601E-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:
-239.760000 0.084000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6217 22.0176 0.9 48.0 -27.0 9.2218 12.8 0.7 Crab
325.9880 38.3294 10.1 48.2 146.8 1.5125 1.1 8.7 Cyg X-2
36.9170 13.4040 2.7 38.1 40.1 2.7210 4.2 ------ UNKNOWN
338.4672 82.5910 2.8 34.9 -146.3 1.8156 4.1 ------ UNKNOWN
94.0267 76.9046 2.5 33.7 -114.8 2.4226 4.6 ------ UNKNOWN
93.6402 55.8627 2.5 34.5 -76.8 2.9402 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.084000 16.140600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5806 22.1470 37.8 47.9 -27.0 0.0329 0.3 8.5 Crab
326.1480 38.4190 6.4 48.0 146.7 0.3447 1.8 5.9 Cyg X-2
345.7947 35.5128 0.9 37.7 128.8 1.3055 12.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
93.940600 322.940600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
299.5832 35.1921 1.3 37.4 -167.6 3.8108 8.8 0.7 Cyg X-1
308.2075 40.8954 3.2 29.8 -159.2 1.2471 3.6 5.6 Cyg X-3
326.3700 38.2988 28.3 15.8 -165.0 0.1231 0.4 9.4 Cyg X-2
346.9789 -2.7146 2.6 38.2 87.1 4.2300 4.4 ------ UNKNOWN
306.1649 1.6005 2.8 50.0 145.3 5.9966 4.2 ------ UNKNOWN
40.3701 14.6508 2.2 52.9 7.6 3.5865 5.2 ------ UNKNOWN
343.3150 35.3971 2.0 2.0 177.0 1.6641 5.8 ------ UNKNOWN
41.4775 33.4591 3.3 45.3 -15.4 1.7786 3.5 ------ UNKNOWN
301.3309 47.8837 2.5 34.9 -146.3 1.9656 4.7 ------ UNKNOWN
Plot creation:
Sat Oct 19 18:15:33 EDT 2024