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
46.2393 -7.6597 0.0151 13.5659 -22.9125 0.5577189 12.800 TRIG_00907754
Foreground time interval of the image:
0.212 0.952 (delta_t = 0.740 [sec])
Background time interval of the image:
-61.067 0.212 (delta_t = 61.279 [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 0.212 sec. to 0.952 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.314011 ( -0.277123 0.249946 )
Norm@50keV : 3.96473E-02 ( -0.00625401 0.0059235 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.55 using 59 PHA bins.
# Reduced chi-squared = 0.9922 for 57 degrees of freedom
# Null hypothesis probability = 4.917746e-01
Photon flux (15-150 keV) in 0.74 sec: 4.87466 ( -0.59017 0.59267 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.35133e-07 ( -5.34242e-08 5.35892e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.212 sec. to 0.952 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.301693 ( -0.693465 0.359591 )
Epeak [keV] : 9999.24 ( -9999.29 -9999.29 )
Norm@50keV : 4.00150E-02 ( -0.00586857 0.0276726 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.58 using 59 PHA bins.
# Reduced chi-squared = 1.010 for 56 degrees of freedom
# Null hypothesis probability = 4.531118e-01
Photon flux (15-150 keV) in 0.74 sec: 4.87243 ( -0.58997 0.59238 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.35785e-07 ( -7.03061e-08 6.90763e-08 ) ergs/cm2
Band function
Time interval is from 0.212 sec. to 0.952 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] : 42.9577 (-9.20107 15.5444)
R^2/D10^2 : 3.18274E-02 (-0.015828 0.0259886)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.07 using 59 PHA bins.
# Reduced chi-squared = 1.106 for 57 degrees of freedom
# Null hypothesis probability = 2.704457e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.324e-09 1.492e-09
25- 50 3.705e-08 8.917e-09
50-150 3.855e-07 1.005e-07
15-150 4.279e-07 1.126e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 17.0151 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 127.10 using 59 PHA bins.
# Reduced chi-squared = 2.2297 for 57 degrees of freedom
# Null hypothesis probability = 2.924571e-07
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.135e-08 1.777e-08
25- 50 6.031e-08 3.373e-08
50-150 1.323e-07 7.511e-08
15-150 2.239e-07 1.260e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.09464 (-2.67074 6.01261)
R1^2/D10^2 : 3.61755 (-3.26476 36.1507)
kT2 [keV] : 55.0621 (-15.3368 49.7186)
R2^2/D10^2 : 1.73745E-02 (-0.0118594 0.0137155)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.90 using 59 PHA bins.
# Reduced chi-squared = 0.9800 for 55 degrees of freedom
# Null hypothesis probability = 5.166809e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.745e-08 9.334e-09
25- 50 4.304e-08 1.915e-08
50-150 3.903e-07 1.862e-07
15-150 4.508e-07 1.952e-07
Peak spectrum fit
Power-law model
Time interval is from 0.082 sec. to 1.082 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.414109 ( -0.267046 0.242556 )
Norm@50keV : 3.31416E-02 ( -0.00499291 0.00478189 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.02 using 59 PHA bins.
# Reduced chi-squared = 1.035 for 57 degrees of freedom
# Null hypothesis probability = 4.016008e-01
Photon flux (15-150 keV) in 1 sec: 3.98655 ( -0.49481 0.49756 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.65575e-07 ( -5.94965e-08 5.98128e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.082 sec. to 1.082 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.403377 ( -0.264514 0.268982 )
Epeak [keV] : 9999.99 ( -9999.99 -9999.99 )
Norm@50keV : 3.34446E-02 ( -0.00501929 0.00398133 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.02 using 59 PHA bins.
# Reduced chi-squared = 1.054 for 56 degrees of freedom
# Null hypothesis probability = 3.658732e-01
Photon flux (15-150 keV) in 1 sec: 3.98169 ( -0.51816 0.50085 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.89756e-07 ( -9.07311e-08 4.02246e-08 ) ergs/cm2
Band function
Time interval is from 0.082 sec. to 1.082 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] : 37.1101 (-7.45335 11.702)
R^2/D10^2 : 3.64570E-02 (-0.0175851 0.0291891)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.18 using 59 PHA bins.
# Reduced chi-squared = 1.126 for 57 degrees of freedom
# Null hypothesis probability = 2.395204e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.831e-09 2.061e-09
25- 50 4.553e-08 1.220e-08
50-150 3.954e-07 9.545e-08
15-150 4.478e-07 1.062e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 14.0895 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 119.97 using 59 PHA bins.
# Reduced chi-squared = 2.1048 for 57 degrees of freedom
# Null hypothesis probability = 2.198754e-06
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.508e-08 1.985e-08
25- 50 6.749e-08 3.827e-08
50-150 1.480e-07 8.350e-08
15-150 2.506e-07 1.403e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.16911 (-3.63991 8.33946)
R1^2/D10^2 : 1.52080 (-1.36837 12.2739)
kT2 [keV] : 47.6843 (-13.1423 52.2881)
R2^2/D10^2 : 1.87327E-02 (-0.0163356 0.0236138)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.57 using 59 PHA bins.
# Reduced chi-squared = 1.047 for 55 degrees of freedom
# Null hypothesis probability = 3.804646e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.769e-08 1.059e-08
25- 50 5.292e-08 2.710e-08
50-150 4.051e-07 2.130e-07
15-150 4.757e-07 2.143e-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: 0.314011 ( -0.277123 0.249946 )
Norm@50keV : 3.96473E-02 ( -0.00625401 0.0059235 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.55 using 59 PHA bins.
# Reduced chi-squared = 0.9922 for 57 degrees of freedom
# Null hypothesis probability = 4.917746e-01
Photon flux (15-150 keV) in 0.74 sec: 4.87473 ( -0.590197 0.592672 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.35079e-07 ( -5.34109e-08 5.36034e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.316637 ( -0.300033 0.240817 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 4.01897E-02 ( -0.00637319 0.0275827 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.59 using 59 PHA bins.
# Reduced chi-squared = 1.011 for 56 degrees of freedom
# Null hypothesis probability = 4.527983e-01
Photon flux (15-150 keV) in 0.74 sec: 4.88344 ( -0.3023 0.58323 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.34262e-07 ( -5.25089e-08 5.41924e-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) = 4.80e-08
S(50-100 keV) = 1.55e-07
T90 vs. Hardness ratio plot
T90 = 0.631999969482422 sec.
Hardness ratio (energy fluence ratio) = 3.22917
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.44219
Count Ratio (50-100 keV) / (15-25 keV) = 2.8529
Mask shadow pattern
IMX = 2.222568407191748E-01, IMY = 9.394200137702663E-02
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:
-61.067400 0.212000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
36.1037 -4.2547 3.0 4.4 18.0 9.3288 3.9 ------ UNKNOWN
70.7106 0.5090 2.2 35.7 -58.4 24.6855 5.2 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.212000 0.952000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
348.4106 13.1751 2.3 48.0 140.4 1.1739 4.9 ------ UNKNOWN
348.1015 20.6127 2.2 50.2 149.8 1.1720 5.2 ------ UNKNOWN
46.2393 -7.6597 0.9 13.6 -22.9 0.5577 12.8 ------ UNKNOWN
32.5023 46.4351 2.3 46.5 -149.9 0.4758 5.1 ------ UNKNOWN
83.2130 -4.9456 2.1 48.4 -50.9 1.1542 5.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
-487.768000 -407.578000
-239.768000 62.302000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
268.3697 -1.4799 8.5 40.7 123.3 -29.6473 -1.4 1.6 SW J1753.5-0127
273.9842 -14.0373 8.9 36.7 102.2 -22.8440 -1.3 1.3 GX 17+2
284.8828 -24.8790 5.0 32.6 76.7 -31.4661 -2.3 8.7 HT1900.1-2455
288.7086 10.8251 6.6 24.1 156.0 13.7823 1.8 9.0 GRS 1915+105
299.5874 35.3723 7.5 38.6 -159.4 15.0813 1.5 10.2 Cyg X-1
308.0080 40.9224 31.8 43.1 -148.2 -4.5848 -0.4 5.0 Cyg X-3
326.4424 38.2594 0.0 43.5 -127.1 30.4230 1.5 13.3 Cyg X-2
310.2278 -6.3780 3.1 4.4 18.0 24.6840 3.8 ------ UNKNOWN
Plot creation:
Tue Jul 16 15:42:02 EDT 2019