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
143.0706 -18.6954 0.0098 39.3127 -67.3756 6.4092520 19.793 TRIG_01251252
Foreground time interval of the image:
-1.912 51.896 (delta_t = 53.808 [sec])
Background time interval of the image:
-239.528 -1.912 (delta_t = 237.616 [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
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)
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 -1.912 sec. to 51.896 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.71554 ( -0.110703 0.112221 )
Norm@50keV : 7.43210E-03 ( -0.000495091 0.000492236 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.93 using 59 bins.
Reduced chi-squared = 0.928596
# Null hypothesis probability of 6.29e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 53.81 sec: 0.992527 ( -0.065138 0.065253 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.69899e-06 ( -2.55706e-07 2.5707e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -1.912 sec. to 51.896 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38429 ( -0.466701 0.380825 )
Epeak [keV] : 91.2945 ( -29.6696 -91.2945 )
Norm@50keV : 1.10040E-02 ( -0.00385333 0.0078761 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.16 using 59 bins.
Reduced chi-squared = 0.913571
# Null hypothesis probability of 6.58e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 53.81 sec: 0.977741 ( -0.067834 0.067849 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.6162e-06 ( -2.7823e-07 2.77949e-07 ) ergs/cm2
Band function
Time interval is from -1.912 sec. to 51.896 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] : 13.4998 (-1.06189 1.1479)
R^2/D10^2 : 0.155607 (-0.040623 0.0548569)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 112.09 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 1.85e-05 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.232e-07 3.890e-08
25- 50 1.159e-06 9.497e-08
50-150 1.364e-06 1.838e-07
15-150 2.845e-06 2.260e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 135.843 (-33.8041 46.3495)
Norm : 4.10405 (-0.316191 0.396858)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.36 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.86e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.715e-07 5.696e-08
25- 50 1.043e-06 1.020e-07
50-150 1.974e-06 6.511e-07
15-150 3.589e-06 7.517e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.21235 (-1.157 1.37977)
R1^2/D10^2 : 1.71472 (-0.858705 2.00117)
kT2 [keV] : 22.5717 (-3.59875 5.82393)
R2^2/D10^2 : 1.85087E-02 (-0.010782 0.0181826)
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.10 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.25e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.894e-07 1.453e-07
25- 50 1.032e-06 2.163e-07
50-150 1.952e-06 5.602e-07
15-150 3.574e-06 8.217e-07
Peak spectrum fit
Power-law model
Time interval is from 0.188 sec. to 1.188 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.03213 ( -0.216063 0.240079 )
Norm@50keV : 1.69578E-02 ( -0.0034507 0.00340288 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 88.44 using 59 bins.
Reduced chi-squared = 1.55158
# Null hypothesis probability of 4.80e-03 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.58250 ( -0.48487 0.48524 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.56664e-07 ( -3.07193e-08 3.07836e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.188 sec. to 1.188 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.01212 ( -1.5998 1.1843 )
Epeak [keV] : 54.2117 ( -7.74061 7.99559 )
Norm@50keV : 0.542129 ( -0.539476 2.36617 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.82 using 59 bins.
Reduced chi-squared = 1.1575
# Null hypothesis probability of 1.96e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 2.78080 ( -0.49311 0.49396 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.89845e-07 ( -3.42986e-08 3.45174e-08 ) ergs/cm2
Band function
Time interval is from 0.188 sec. to 1.188 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] : 14.0990 (-1.93579 1.97897)
R^2/D10^2 : 0.464994 (-0.183081 0.321569)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 64.81 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.23e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.951e-08 5.710e-09
25- 50 7.308e-08 1.678e-08
50-150 9.599e-08 3.132e-08
15-150 1.886e-07 4.455e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 73.2069 (-21.0248 30.9265)
Norm : 13.9888 (-2.94297 3.31019)
------------------------------------------------------------
#Fit statistic : Chi-Squared 77.14 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 3.90e-02 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.605e-08 8.070e-09
25- 50 5.804e-08 1.088e-08
50-150 7.703e-08 3.290e-08
15-150 1.711e-07 4.125e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.65700 (-4.64012 67.5868)
R1^2/D10^2 : 5.57393 (-5.70931 -5.70931)
kT2 [keV] : 15.1047 (-2.33234 3.10107)
R2^2/D10^2 : 0.332955 (-0.334846 0.323604)
------------------------------------------------------------
#Fit statistic : Chi-Squared 63.31 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 2.06e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.600e-08 1.353e-08
25- 50 6.904e-08 3.477e-08
50-150 9.910e-08 5.994e-08
15-150 1.941e-07 1.081e-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: 1.71554 ( -0.110703 0.112221 )
Norm@50keV : 7.43210E-03 ( -0.000495091 0.000492236 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 52.93 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.29e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 53.81 sec: 0.992484 ( -0.0651329 0.0652452 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.69845e-06 ( -2.5588e-07 2.57072e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.38429 ( -0.466701 0.380825 )
Epeak [keV] : 91.2945 ( -29.6695 -91.2945 )
Norm@50keV : 1.10040E-02 ( -0.00385333 0.0078761 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 51.16 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 6.58e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 53.81 sec: 0.977583 ( -0.067808 0.067827 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.61736e-06 ( -2.78295e-07 2.78144e-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) = 1.01e-06
S(50-100 keV) = 1.23e-06
T90 vs. Hardness ratio plot
T90 = 42.9760000705719 sec.
Hardness ratio (energy fluence ratio) = 1.21782
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.39973
Count Ratio (50-100 keV) / (15-25 keV) = 0.989197
Mask shadow pattern
IMX = 3.150063776940881E-01, IMY = 7.558474122916268E-01
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:
-239.528000 -1.912000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6100 22.0284 0.9 43.9 170.9 9.6638 13.1 1.5 Crab
135.5661 -40.5038 3.2 36.7 -30.3 1.7832 3.6 3.5 Vela X-1
95.0228 13.0290 3.4 31.9 -176.9 1.3346 3.4 ------ UNKNOWN
100.7742 -4.1790 2.3 14.1 -168.0 1.5751 5.0 ------ UNKNOWN
147.9310 -54.8855 3.0 50.7 -17.4 2.5639 3.8 ------ UNKNOWN
111.1710 24.4769 3.1 43.7 -152.1 2.3110 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-1.912000 51.896000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7273 22.1267 3.9 44.0 171.1 -0.5478 -3.0 8.5 Crab
135.4737 -40.6142 8.9 36.7 -30.0 -0.1848 -1.3 4.4 Vela X-1
73.5681 -48.8392 2.0 38.0 45.2 0.9491 5.8 ------ UNKNOWN
74.5782 5.7411 2.2 35.8 144.7 0.7818 5.2 ------ UNKNOWN
91.6570 -13.4112 2.3 10.7 130.7 0.4380 5.0 ------ UNKNOWN
143.0706 -18.6954 0.6 39.3 -67.4 6.4108 19.8 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
597.972600 962.596400
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
233.5758 16.7374 3.6 29.5 69.6 2.4699 3.2 ------ UNKNOWN
225.5883 -45.3769 2.5 53.9 166.9 7.3603 4.6 ------ UNKNOWN
216.2813 44.8047 2.0 40.4 15.8 3.8020 5.6 ------ UNKNOWN
211.8134 51.8055 2.7 46.6 9.4 2.7880 4.3 ------ UNKNOWN
179.7781 -31.9262 2.1 44.8 -144.2 5.3720 5.6 ------ UNKNOWN
162.7003 21.0607 2.6 44.4 -61.2 10.1545 4.4 ------ UNKNOWN
Plot creation:
Sat Oct 19 18:16:53 EDT 2024