Special notes of this burst
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
188.4953 27.9397 0.0162 6.9139 -168.0670 1.0168156 11.900 TRIG_00583861
Foreground time interval of the image:
19.444 72.501 (delta_t = 53.057 [sec])
Background time interval of the image:
-239.000 19.444 (delta_t = 258.444 [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 64.000000
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 64.000000
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 64.000000
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)
The mask-weighted light curves based on cleaned DPHs
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 19.444 sec. to 202.520 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.06945 ( -0.086729 0.0883423 )
Norm@50keV : 1.88467E-03 ( -9.55859e-05 9.46846e-05 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.75 using 59 PHA bins.
# Reduced chi-squared = 0.9254 for 57 degrees of freedom
# Null hypothesis probability = 6.352159e-01
Photon flux (15-150 keV) in 183.1 sec: 0.292115 ( -0.0128548 0.0128904 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.19737e-06 ( -1.49013e-07 1.50073e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 19.444 sec. to 202.520 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.80323 ( -0.374728 0.322691 )
Epeak [keV] : 32.4622 ( -31.4668 16.2821 )
Norm@50keV : 2.63514E-03 ( -0.000901158 0.00156199 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.02 using 59 PHA bins.
# Reduced chi-squared = 0.9111 for 56 degrees of freedom
# Null hypothesis probability = 6.633397e-01
Photon flux (15-150 keV) in 183.1 sec: 0.286677 ( -0.014522 0.014548 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.10446e-06 ( -1.89344e-07 1.90735e-07 ) ergs/cm2
Band function
Time interval is from 19.444 sec. to 202.520 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.58507 ( 1.59055 1.59055 )
beta : -2.23197 ( 2.23011 0.203644 )
Epeak [keV] : 33.0795 ( -33.0336 12.8751 )
Norm@50keV : 3.62577E-03 ( -0.00134373 455.246 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.41 using 59 PHA bins.
# Reduced chi-squared = 0.9165 for 55 degrees of freedom
# Null hypothesis probability = 6.505223e-01
Photon flux (15-150 keV) in 183.1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.10887e-06 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.3477 ( )
R^2/D10^2 : 0.109988 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 163.55 using 59 PHA bins.
# Reduced chi-squared = 2.8693 for 57 degrees of freedom
# Null hypothesis probability = 3.151252e-12
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.439e-07 3.479e-08
25- 50 1.157e-06 4.962e-08
50-150 6.663e-07 7.425e-08
15-150 2.268e-06 1.053e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 63.8565 (-8.22604 10.1841)
Norm : 1.44531 (-0.112677 0.125093)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.38 using 59 PHA bins.
# Reduced chi-squared = 0.9717 for 57 degrees of freedom
# Null hypothesis probability = 5.359043e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.714e-07 4.330e-08
25- 50 1.041e-06 4.422e-08
50-150 1.246e-06 1.406e-07
15-150 2.958e-06 1.593e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.55547 (-0.841665 0.943015)
R1^2/D10^2 : 0.883000 (-0.381554 0.811221)
kT2 [keV] : 18.4336 (-2.69854 4.12018)
R2^2/D10^2 : 8.65030E-03 (-0.00478065 0.00811255)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.54 using 59 PHA bins.
# Reduced chi-squared = 1.046 for 55 degrees of freedom
# Null hypothesis probability = 3.815025e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.955e-07 1.171e-07
25- 50 9.973e-07 1.284e-07
50-150 1.281e-06 2.635e-07
15-150 2.974e-06 3.625e-07
Peak spectrum fit
Power-law model
Time interval is from 115.880 sec. to 116.880 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.06890 ( -0.287236 0.318722 )
Norm@50keV : 6.11038E-03 ( -0.00135861 0.00131016 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.99 using 59 PHA bins.
# Reduced chi-squared = 0.7894 for 57 degrees of freedom
# Null hypothesis probability = 8.751495e-01
Photon flux (15-150 keV) in 1 sec: 0.946825 ( -0.145628 0.145649 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.66162e-08 ( -1.11561e-08 1.16e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 115.880 sec. to 116.880 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.95521 ( -1.48558 0.114383 )
Epeak [keV] : 15.2561 ( -14.692 -15.2594 )
Norm@50keV : 7.17858E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.96 using 59 PHA bins.
# Reduced chi-squared = 0.8029 for 56 degrees of freedom
# Null hypothesis probability = 8.545960e-01
Photon flux (15-150 keV) in 1 sec: 0.943550 ( -0.145796 0.14744 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.57785e-08 ( -1.23864e-08 1.22831e-08 ) ergs/cm2
Band function
Time interval is from 115.880 sec. to 116.880 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 3.76745 ( -3.7663 -3.7663 )
beta : -2.15368 ( -0.485361 0.336348 )
Epeak [keV] : 19.8753 ( -19.852 42.7814 )
Norm@50keV : 455.209 ( -457.716 2.43414e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.64 using 59 PHA bins.
# Reduced chi-squared = 0.8116 for 55 degrees of freedom
# Null hypothesis probability = 8.397663e-01
Photon flux (15-150 keV) in 1 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] : 8.45504 (-1.46596 1.76002)
R^2/D10^2 : 0.838616 (-0.436574 0.922176)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.30 using 59 PHA bins.
# Reduced chi-squared = 0.9526 for 57 degrees of freedom
# Null hypothesis probability = 5.770804e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.126e-08 3.181e-09
25- 50 2.165e-08 5.430e-09
50-150 6.797e-09 3.079e-09
15-150 3.970e-08 9.620e-09
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 55.4072 (-20.8391 43.2216)
Norm : 5.16488 (-1.24033 1.70524)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.60 using 59 PHA bins.
# Reduced chi-squared = 0.7999 for 57 degrees of freedom
# Null hypothesis probability = 8.611397e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.280e-08 2.746e-09
25- 50 1.899e-08 3.880e-09
50-150 2.019e-08 8.782e-09
15-150 5.198e-08 1.477e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.89973 (-3.06888 2.45843)
R1^2/D10^2 : 2.72496 (-1.87447 44.7682)
kT2 [keV] : 23.1060 (-13.232 -23.6045)
R2^2/D10^2 : 1.13047E-02 (-0.0102788 0.307631)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.69 using 59 PHA bins.
# Reduced chi-squared = 0.8307 for 55 degrees of freedom
# Null hypothesis probability = 8.102460e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.339e-08 7.624e-09
25- 50 1.775e-08 9.046e-09
50-150 2.468e-08 1.515e-08
15-150 5.582e-08 2.808e-08
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: 1.84961 ( -0.242802 0.258627 )
Norm@50keV : 1.05461E-03 ( -0.000167762 0.00016104 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.95 using 59 PHA bins.
# Reduced chi-squared = 0.9114 for 57 degrees of freedom
# Null hypothesis probability = 6.644868e-01
Photon flux (15-150 keV) in 53.06 sec: 0.148213 ( -0.0180913 0.0180926 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.14521e-07 ( -7.98977e-08 8.21263e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.67113 ( )
Epeak [keV] : 219.640 ( )
Norm@50keV : 4.28983E-04 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.88 using 59 PHA bins.
# Reduced chi-squared = 0.9264 for 56 degrees of freedom
# Null hypothesis probability = 6.314770e-01
Photon flux (15-150 keV) in 53.06 sec: 0.148204 ( -0.018095 0.018084 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.13562e-07 ( -7.8975e-08 8.30129e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.45689 ( 1.45828 1.45828 )
beta : -1.84952 ( 1.84957 0.242476 )
Epeak [keV] : 18.5103 ( -18.0099 -18.0099 )
Norm@50keV : 2.62049E-03 ( -0.00263381 2.26575 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.95 using 59 PHA bins.
# Reduced chi-squared = 0.9445 for 55 degrees of freedom
# Null hypothesis probability = 5.918986e-01
Photon flux (15-150 keV) in 53.06 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) = 9.81e-07
S(50-100 keV) = 9.35e-07
T90 vs. Hardness ratio plot
T90 = 139.947999954224 sec.
Hardness ratio (energy fluence ratio) = 0.953109
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.978766
Count Ratio (50-100 keV) / (15-25 keV) = 0.452655
Mask shadow pattern
IMX = -1.186397458794859E-01, IMY = 2.507270633167256E-02
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 64.000000
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:
-239.000000 19.444000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
202.5169 77.7383 2.7 56.9 179.3 5.7424 4.3 ------ UNKNOWN
202.0581 -3.6541 2.4 29.4 -38.4 1.0416 4.7 ------ UNKNOWN
218.1372 37.5163 2.9 31.9 -132.4 1.2126 4.0 ------ UNKNOWN
222.6316 -3.6942 3.1 43.5 -64.0 4.0705 3.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
19.444000 72.500590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
188.4953 27.9396 1.0 6.9 -168.1 1.0169 11.9 ------ UNKNOWN
199.2202 5.7921 2.3 20.0 -45.6 0.4536 5.1 ------ UNKNOWN
218.8644 34.3508 2.1 31.5 -126.3 0.6100 5.4 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
100.500600 963.089600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
185.2684 50.6567 2.6 22.9 163.0 2.1826 4.5 ------ UNKNOWN
174.5320 -27.1631 2.9 56.7 3.1 11.7539 4.0 ------ UNKNOWN
188.5346 27.9736 1.5 0.1 -153.8 3.5823 7.6 ------ UNKNOWN
184.4347 -6.8497 4.2 35.0 -4.8 1.7508 2.8 ------ UNKNOWN
210.8282 23.5389 3.6 20.6 -94.6 1.7161 3.2 ------ UNKNOWN
224.6229 39.4504 2.8 32.0 -132.4 3.1579 4.2 ------ UNKNOWN
206.4708 -4.7740 3.7 37.0 -42.5 2.4703 3.2 ------ UNKNOWN
238.7867 29.4084 2.9 43.8 -116.3 10.5489 4.0 ------ UNKNOWN
236.6337 25.8331 2.7 42.7 -110.6 10.3436 4.5 ------ UNKNOWN
236.4966 25.4514 3.7 42.7 -110.0 8.7700 3.8 ------ UNKNOWN
Plot creation:
Sat May 30 14:40:55 EDT 2015