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
57.8580 28.2939 0.0100 13.1589 -74.7912 0.7654362 19.227 TRIG_00284856
Foreground time interval of the image:
-0.792 16.589 (delta_t = 17.381 [sec])
Background time interval of the image:
-239.712 -0.792 (delta_t = 238.920 [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 0.128000
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 0.128000
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 0.128000
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 -0.792 sec. to 74.640 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.36782 ( -0.191101 0.1914 )
Norm@50keV : 1.00719E-03 ( -0.000110233 0.000109566 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.34 using 59 PHA bins.
# Reduced chi-squared = 0.9008 for 57 degrees of freedom
# Null hypothesis probability = 6.863172e-01
Photon flux (15-150 keV) in 75.43 sec: 0.121791 ( -0.0130114 0.01302 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.39089e-07 ( -9.1965e-08 9.34691e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.792 sec. to 74.640 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.15378 ( -0.881761 0.386293 )
Epeak [keV] : 192.479 ( -192.563 -192.563 )
Norm@50keV : 1.29994E-03 ( -0.000542383 0.00233166 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 51.12 using 59 PHA bins.
# Reduced chi-squared = 0.9128 for 56 degrees of freedom
# Null hypothesis probability = 6.599072e-01
Photon flux (15-150 keV) in 75.43 sec: 0.120522 ( -0.013833 0.013702 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.23254e-07 ( -1.09315e-07 1.05465e-07 ) ergs/cm2
Band function
Time interval is from -0.792 sec. to 74.640 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.911472 ( 0.911889 5.61777 )
beta : -1.59024 ( 1.58075 0.383434 )
Epeak [keV] : 106.484 ( -107.032 -107.032 )
Norm@50keV : 1.78035E-03 ( -0.000966554 1.0933 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.80 using 59 PHA bins.
# Reduced chi-squared = 0.9236 for 55 degrees of freedom
# Null hypothesis probability = 6.358821e-01
Photon flux (15-150 keV) in 75.43 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] : 15.2365 (-1.96468 2.36114)
R^2/D10^2 : 1.32341E-02 (-0.00515888 0.00807973)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.66 using 59 PHA bins.
# Reduced chi-squared = 1.169 for 57 degrees of freedom
# Null hypothesis probability = 1.789243e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.839e-08 1.105e-08
25- 50 1.950e-07 3.074e-08
50-150 3.103e-07 7.336e-08
15-150 5.537e-07 8.135e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 0.495780 (-0.053036 0.053036)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.32 using 59 PHA bins.
# Reduced chi-squared = 0.9354 for 57 degrees of freedom
# Null hypothesis probability = 6.140147e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.358e-08 5.242e-08
25- 50 1.800e-07 9.881e-08
50-150 3.948e-07 2.164e-07
15-150 6.684e-07 3.652e-07
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.6464 ( )
R1^2/D10^2 : 3.57534E-02 (-0.0185695 0.0228445)
kT2 [keV] : 64.3877 (-67.0004 -67.0005)
R2^2/D10^2 : 1.12987E-04 (-8.08909e-05 0.000440716)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.72 using 59 PHA bins.
#Fit statistic : Chi-Squared = 53.42 using 59 PHA bins.
# Reduced chi-squared = 0.9768 for 55 degrees of freedom
# Reduced chi-squared = 0.9712 for 55 degrees of freedom
# Null hypothesis probability = 5.234857e-01
# Null hypothesis probability = 5.353025e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.307e-08 4.168e-08
25- 50 1.707e-07 6.750e-08
50-150 4.180e-07 2.210e-07
15-150 6.718e-07 3.255e-07
Peak spectrum fit
Power-law model
Time interval is from -0.388 sec. to 0.612 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.882076 ( -0.104985 0.103392 )
Norm@50keV : 2.39804E-02 ( -0.00135538 0.00135024 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.96 using 59 PHA bins.
# Reduced chi-squared = 0.6834 for 57 degrees of freedom
# Null hypothesis probability = 9.675984e-01
Photon flux (15-150 keV) in 1 sec: 2.75220 ( -0.155099 0.155236 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.71018e-07 ( -1.71263e-08 1.7213e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.388 sec. to 0.612 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.879389 ( -0.191564 0.101565 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 2.41124E-02 ( -0.00136254 0.00837008 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.99 using 59 PHA bins.
# Reduced chi-squared = 0.6962 for 56 degrees of freedom
# Null hypothesis probability = 9.592541e-01
Photon flux (15-150 keV) in 1 sec: 2.75135 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.70735e-07 ( -1.669e-08 1.7429e-08 ) ergs/cm2
Band function
Time interval is from -0.388 sec. to 0.612 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.916637 ( 0.916637 0.916637 )
beta : -0.882076 ( -0.103384 0.105006 )
Epeak [keV] : 13.2348 ( -13.2348 -13.2348 )
Norm@50keV : 3.58492E-02 ( -0.0128688 691382 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.96 using 59 PHA bins.
# Reduced chi-squared = 0.7083 for 55 degrees of freedom
# Null hypothesis probability = 9.500362e-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] : 23.3398 (-1.95092 2.22403)
R^2/D10^2 : 8.28214E-02 (-0.019687 0.0250146)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 97.16 using 59 PHA bins.
# Reduced chi-squared = 1.704 for 57 degrees of freedom
# Null hypothesis probability = 7.275958e-04
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.118e-09 9.105e-10
25- 50 4.440e-08 3.920e-09
50-150 1.806e-07 1.735e-08
15-150 2.331e-07 1.860e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 10.7235 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 148.17 using 59 PHA bins.
# Reduced chi-squared = 2.5996 for 57 degrees of freedom
# Null hypothesis probability = 4.786168e-10
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.670e-08 1.900e-09
25- 50 5.137e-08 4.605e-09
50-150 1.127e-07 3.347e-08
15-150 1.907e-07 3.510e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 11.2399 (-2.97025 2.66986)
R1^2/D10^2 : 0.491614 (-0.221576 0.615556)
kT2 [keV] : 62.8323 (-24.8942 -62.931)
R2^2/D10^2 : 4.50822E-03 (-0.00271551 0.0125604)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.09 using 59 PHA bins.
# Reduced chi-squared = 0.7471 for 55 degrees of freedom
# Null hypothesis probability = 9.182386e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.465e-08 3.238e-09
25- 50 5.010e-08 1.333e-08
50-150 2.097e-07 9.562e-08
15-150 2.744e-07 9.997e-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: 0.990688 ( -0.149011 0.145445 )
Norm@50keV : 2.92423E-03 ( -0.000239879 0.000239032 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.82 using 59 PHA bins.
# Reduced chi-squared = 1.014 for 57 degrees of freedom
# Null hypothesis probability = 4.447059e-01
Photon flux (15-150 keV) in 17.38 sec: 0.336550 ( -0.0279628 0.0279915 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.51481e-07 ( -4.97344e-08 4.99274e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.623822 ( -0.678825 0.506115 )
Epeak [keV] : 208.807 ( -208.811 -208.811 )
Norm@50keV : 4.30050E-03 ( -0.00154167 0.0042325 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.71 using 59 PHA bins.
# Reduced chi-squared = 1.013 for 56 degrees of freedom
# Null hypothesis probability = 4.482199e-01
Photon flux (15-150 keV) in 17.38 sec: 0.330603 ( -0.029673 0.029311 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.37897e-07 ( -5.57603e-08 5.4886e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.328449 ( 0.784306 0.784306 )
beta : -1.21471 ( 1.23043 0.330868 )
Epeak [keV] : 122.578 ( -121.028 234.885 )
Norm@50keV : 6.25650E-03 ( -0.00349539 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.13 using 59 PHA bins.
# Reduced chi-squared = 1.021 for 55 degrees of freedom
# Null hypothesis probability = 4.322434e-01
Photon flux (15-150 keV) in 17.38 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) = 1.71e-07
S(50-100 keV) = 2.65e-07
T90 vs. Hardness ratio plot
T90 = 65.636000007391 sec.
Hardness ratio (energy fluence ratio) = 1.54971
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.17932
Count Ratio (50-100 keV) / (15-25 keV) = 1.06614
Mask shadow pattern
IMX = 6.133183606488909E-02, IMY = 2.256021352703911E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.128000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.128000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.128000
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:
-239.712000 -0.792000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6355 22.0197 0.5 37.3 -76.7 9.9636 24.4 0.3 Crab
2.7555 78.3615 2.7 51.2 -179.1 1.8848 4.3 ------ UNKNOWN
65.8802 -7.3724 2.6 43.6 -23.7 1.2445 4.5 ------ UNKNOWN
79.0084 33.7353 2.3 30.6 -95.6 1.3887 5.1 ------ UNKNOWN
94.1564 41.1172 2.5 42.4 -108.9 3.4068 4.6 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.792000 16.588590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.4543 21.9367 7.2 37.1 -76.5 0.1508 1.6 11.0 Crab
7.2265 18.8591 1.9 34.2 89.4 0.6140 6.0 ------ UNKNOWN
2.9835 29.9667 2.1 34.4 110.4 0.4982 5.5 ------ UNKNOWN
31.4762 -5.3897 2.2 37.3 29.5 0.3644 5.2 ------ UNKNOWN
57.8580 28.2939 0.6 13.2 -74.8 0.7655 19.2 ------ UNKNOWN
75.3790 31.0026 2.2 27.8 -89.5 0.2899 5.3 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
50.788590 962.391300
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6278 22.0126 0.2 24.1 -75.1 39.3700 61.3 0.3 Crab
26.9041 52.3975 3.9 33.2 150.8 2.1986 3.0 ------ UNKNOWN
75.7635 61.0816 3.8 34.9 -159.3 1.6818 3.0 ------ UNKNOWN
125.6337 82.4054 3.3 59.1 -166.1 12.2620 3.5 ------ UNKNOWN
103.8272 44.6027 2.2 39.8 -121.2 5.5468 5.1 ------ UNKNOWN
Plot creation:
Sun May 31 09:45:35 EDT 2015