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
324.6888 -56.0702 0.0304 35.4454 -7.0721 0.7821096 6.309 TRIG_00907950
Foreground time interval of the image:
-0.872 40.045 (delta_t = 40.917 [sec])
Background time interval of the image:
-239.056 -0.872 (delta_t = 238.184 [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 3.072000
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 3.072000
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 3.072000
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 -0.872 sec. to 63.824 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.87327 ( -0.495597 0.584151 )
Norm@50keV : 7.68817E-04 ( -0.000274939 0.000257652 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.40 using 59 PHA bins.
# Reduced chi-squared = 0.9719 for 57 degrees of freedom
# Null hypothesis probability = 5.353562e-01
Photon flux (15-150 keV) in 64.7 sec: 0.109109 ( -0.0308414 0.030854 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.57366e-07 ( -1.53169e-07 1.60543e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.872 sec. to 63.824 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.586560 ( -4.14344 1.58605 )
Epeak [keV] : 49.5680 ( -37.8006 -49.5665 )
Norm@50keV : 3.86045E-03 ( -0.00387288 0.612918 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.71 using 59 PHA bins.
# Reduced chi-squared = 0.9770 for 56 degrees of freedom
# Null hypothesis probability = 5.236345e-01
Photon flux (15-150 keV) in 64.7 sec: 0.104241 ( -0.0327738 0.032476 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.19405e-07 ( -1.44702e-07 1.76578e-07 ) ergs/cm2
Band function
Time interval is from -0.872 sec. to 63.824 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] : 12.0180 (-3.13896 4.13795)
R^2/D10^2 : 2.71614E-02 (-0.0271609 0.0548936)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.63 using 59 PHA bins.
# Reduced chi-squared = 0.9760 for 57 degrees of freedom
# Null hypothesis probability = 5.265305e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.369e-08 3.314e-08
25- 50 1.693e-07 1.008e-07
50-150 1.471e-07 1.029e-07
15-150 3.701e-07 2.308e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 84.4247 (-47.6544 -84.4263)
Norm : 0.508079 (-0.16858 0.272509)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.92 using 59 PHA bins.
# Reduced chi-squared = 0.9634 for 57 degrees of freedom
# Null hypothesis probability = 5.536623e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.556e-08 5.218e-08
25- 50 1.426e-07 8.595e-08
50-150 2.086e-07 1.758e-07
15-150 4.368e-07 3.016e-07
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 1.05899 (-1.0095 2.18174)
R1^2/D10^2 : 5.55911E+04 (-66300.7 -66302.7)
kT2 [keV] : 13.0776 (-3.42364 4.74578)
R2^2/D10^2 : 1.88887E-02 (-0.0132576 0.0243327)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.97 using 59 PHA bins.
#Fit statistic : Chi-Squared = 50.73 using 59 PHA bins.
# Reduced chi-squared = 0.9268 for 55 degrees of freedom
# Reduced chi-squared = 0.9224 for 55 degrees of freedom
# Null hypothesis probability = 6.292535e-01
# Null hypothesis probability = 6.382167e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.260e-08 3.004e-08
25- 50 1.502e-07 9.174e-08
50-150 1.706e-07 1.188e-07
15-150 3.934e-07 2.326e-07
Peak spectrum fit
Power-law model
Time interval is from 0.544 sec. to 1.544 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.22447 ( -0.449846 0.431616 )
Norm@50keV : 7.74887E-03 ( -0.0021515 0.00214798 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.24 using 59 PHA bins.
# Reduced chi-squared = 0.7761 for 57 degrees of freedom
# Null hypothesis probability = 8.915640e-01
Photon flux (15-150 keV) in 1 sec: 0.912858 ( -0.263025 0.265572 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.8089e-08 ( -2.26418e-08 2.28619e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.544 sec. to 1.544 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -1.41966 ( -5.4061 2.55719 )
Epeak [keV] : 70.6333 ( -17.8704 297.659 )
Norm@50keV : 0.125015 ( -0.126706 27.2133 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.12 using 59 PHA bins.
# Reduced chi-squared = 0.7342 for 56 degrees of freedom
# Null hypothesis probability = 9.319207e-01
Photon flux (15-150 keV) in 1 sec: 0.830506 ( -0.273417 0.281344 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.98538e-08 ( -2.33381e-08 2.49291e-08 ) ergs/cm2
Band function
Time interval is from 0.544 sec. to 1.544 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] : 18.0107 (-4.14933 6.22357)
R^2/D10^2 : 6.47368E-02 (-0.0418608 0.0952307)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.12 using 59 PHA bins.
# Reduced chi-squared = 0.7215 for 57 degrees of freedom
# Null hypothesis probability = 9.439670e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.204e-09 2.128e-09
25- 50 1.945e-08 1.032e-08
50-150 4.580e-08 2.611e-08
15-150 6.946e-08 3.869e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.358 (-95.5933 -199.361)
Norm : 3.87319 (-1.08446 1.08819)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.22 using 59 PHA bins.
# Reduced chi-squared = 0.7933 for 57 degrees of freedom
# Null hypothesis probability = 8.700123e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.645e-09 5.935e-09
25- 50 1.855e-08 1.114e-08
50-150 4.069e-08 2.523e-08
15-150 6.889e-08 4.098e-08
Double BB
# Reduced chi-squared = 0.7159 for 55 degrees of freedom
# Reduced chi-squared = 0.7124 for 55 degrees of freedom
# Reduced chi-squared = 0.7106 for 55 degrees of freedom
# Reduced chi-squared = 0.7097 for 55 degrees of freedom
# Reduced chi-squared = 0.7092 for 55 degrees of freedom
# Reduced chi-squared = 0.7090 for 55 degrees of freedom
# Null hypothesis probability = 9.176258e-01
# Null hypothesis probability = 9.446494e-01
# Null hypothesis probability = 9.471587e-01
# Null hypothesis probability = 9.484552e-01
# Null hypothesis probability = 9.490662e-01
# Null hypothesis probability = 9.493714e-01
# Null hypothesis probability = 9.495230e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 0.000e+00 0.000e+00
25- 50 0.000e+00 0.000e+00
50-150 0.000e+00 0.000e+00
15-150 0.000e+00 0.000e+00
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: 1.63977 ( -0.405583 0.425973 )
Norm@50keV : 1.29221E-03 ( -0.000334409 0.000325485 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.60 using 59 PHA bins.
# Reduced chi-squared = 0.9053 for 57 degrees of freedom
# Null hypothesis probability = 6.770150e-01
Photon flux (15-150 keV) in 40.92 sec: 0.168167 ( -0.0400707 0.0401376 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.92292e-07 ( -1.32068e-07 1.36036e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.778822 ( -3.73209 1.43905 )
Epeak [keV] : 63.1849 ( -63.2495 -63.2495 )
Norm@50keV : 3.86642E-03 ( -0.00385276 0.583282 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.10 using 59 PHA bins.
# Reduced chi-squared = 0.9125 for 56 degrees of freedom
# Null hypothesis probability = 6.603869e-01
Photon flux (15-150 keV) in 40.92 sec: 0.162891 ( -0.041255 0.042129 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.52485e-07 ( -1.56137e-07 1.62506e-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) = 1.32e-07
S(50-100 keV) = 1.44e-07
T90 vs. Hardness ratio plot
T90 = 41.7599999904633 sec.
Hardness ratio (energy fluence ratio) = 1.09091
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.58581
Count Ratio (50-100 keV) / (15-25 keV) = 0.952967
Mask shadow pattern
IMX = 7.064402086766872E-01, IMY = 8.764267341448809E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 3.072000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 3.072000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 3.072000
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:
-239.056000 -0.872000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
274.1749 -13.9451 4.6 39.5 96.0 6.3203 2.5 11.3 GX 17+2
275.9560 -30.2911 4.7 36.1 69.7 -2.9441 -2.5 4.8 H1820-303
285.0567 -24.8992 47.6 27.8 79.0 -0.2009 -0.2 1.7 HT1900.1-2455
288.8468 11.0568 21.3 41.4 141.2 0.8434 0.5 7.3 GRS 1915+105
290.2486 17.9434 3.0 46.2 148.6 7.3127 3.8 ------ UNKNOWN
279.6052 -49.6956 2.9 39.8 38.1 4.1530 4.1 ------ UNKNOWN
296.1110 -9.8975 2.3 21.5 121.4 3.4027 5.0 ------ UNKNOWN
307.9853 -48.8663 3.0 28.1 12.1 2.3200 3.8 ------ UNKNOWN
311.1403 -29.2659 2.5 8.7 25.5 2.4468 4.7 ------ UNKNOWN
312.7392 6.9135 3.3 28.4 177.3 2.0292 3.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.872000 40.044600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
274.0543 -14.0645 4.2 39.6 95.8 1.3045 2.8 3.3 GX 17+2
276.0108 -30.2608 4.0 36.1 69.7 0.8279 2.8 7.8 H1820-303
284.9260 -24.8094 7.6 27.9 79.2 0.2677 1.5 9.0 HT1900.1-2455
288.6814 11.0478 4.9 41.5 141.0 0.6934 2.4 9.2 GRS 1915+105
324.6894 -56.0702 1.8 35.4 -7.1 0.7829 6.3 ------ UNKNOWN
345.1665 25.7304 2.1 55.4 -144.5 2.7481 5.5 ------ UNKNOWN
357.2568 -12.6217 2.1 41.2 -93.0 2.0359 5.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
97.444600 914.744590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
264.8836 -44.5592 3.9 38.6 74.4 13.1401 3.0 8.9 4U 1735-44
252.3099 -50.4553 2.2 41.7 59.1 30.7811 5.2 ------ UNKNOWN
282.7501 -43.9867 2.6 29.0 89.8 12.9608 4.4 ------ UNKNOWN
207.0628 -63.2662 2.2 51.3 23.8 30.6086 5.2 ------ UNKNOWN
302.6150 -40.1967 2.2 21.5 121.4 10.9785 5.2 ------ UNKNOWN
27.3219 -56.4433 2.3 33.5 -69.5 13.9097 5.0 ------ UNKNOWN
Plot creation:
Tue Jul 16 15:39:57 EDT 2019