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
65.7457 -25.1297 0.0109 46.3273 -168.2143 0.8454300 17.521 TRIG_00324561
Foreground time interval of the image:
-3.772 4.556 (delta_t = 8.328 [sec])
Background time interval of the image:
-565.115 -462.112 (delta_t = 103.004 [sec])
-239.216 -3.772 (delta_t = 235.444 [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 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 -3.772 sec. to 4.556 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.19984 ( -0.158489 0.154994 )
Norm@50keV : 6.76545E-03 ( -0.000649458 0.00064835 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.42 using 59 PHA bins.
# Reduced chi-squared = 0.7792 for 57 degrees of freedom
# Null hypothesis probability = 8.877936e-01
Photon flux (15-150 keV) in 8.328 sec: 0.794105 ( -0.0802969 0.0806428 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.71645e-07 ( -5.69197e-08 5.70819e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -3.772 sec. to 4.556 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.389324 ( -0.761367 0.646023 )
Epeak [keV] : 111.497 ( -29.9306 192.973 )
Norm@50keV : 1.58720E-02 ( -0.00769145 0.018291 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.66 using 59 PHA bins.
# Reduced chi-squared = 0.7083 for 56 degrees of freedom
# Null hypothesis probability = 9.516805e-01
Photon flux (15-150 keV) in 8.328 sec: 0.770934 ( -0.082175 0.08257 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.53821e-07 ( -6.04238e-08 5.99708e-08 ) ergs/cm2
Band function
Time interval is from -3.772 sec. to 4.556 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.415914 ( -0.653014 0.56855 )
beta : -9.36665 ( 9.37141 19.3714 )
Epeak [keV] : 114.162 ( -21.2399 161.123 )
Norm@50keV : 1.53602E-02 ( -0.00638861 0.00918787 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.67 using 59 PHA bins.
# Reduced chi-squared = 0.7213 for 55 degrees of freedom
# Null hypothesis probability = 9.405878e-01
Photon flux (15-150 keV) in 8.328 sec: 0.771851 ( ) 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] : 19.3801 (-2.17257 2.54345)
R^2/D10^2 : 4.16576E-02 (-0.0142091 0.020735)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 52.26 using 59 PHA bins.
# Reduced chi-squared = 0.9168 for 57 degrees of freedom
# Null hypothesis probability = 6.531840e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.543e-08 4.830e-09
25- 50 1.240e-07 1.803e-08
50-150 3.435e-07 5.347e-08
15-150 4.929e-07 6.471e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 3.38239 (-0.327942 0.327885)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.49 using 59 PHA bins.
# Reduced chi-squared = 0.9910 for 57 degrees of freedom
# Null hypothesis probability = 4.943331e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.013e-08 1.000e-08
25- 50 1.349e-07 3.295e-08
50-150 2.959e-07 1.399e-07
15-150 5.009e-07 2.090e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.0773 (-3.18445 3.94847)
R1^2/D10^2 : 0.205385 (-0.119107 0.395444)
kT2 [keV] : 32.8336 (-9.16557 41.8821)
R2^2/D10^2 : 5.37998E-03 (-0.00495835 0.0129227)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.73 using 59 PHA bins.
# Reduced chi-squared = 0.6860 for 55 degrees of freedom
# Null hypothesis probability = 9.636211e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.260e-08 2.408e-08
25- 50 1.347e-07 6.904e-08
50-150 3.810e-07 2.031e-07
15-150 5.583e-07 2.863e-07
Peak spectrum fit
Power-law model
Time interval is from 0.128 sec. to 1.128 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.37457 ( -0.270598 0.270019 )
Norm@50keV : 1.12900E-02 ( -0.00194072 0.00193918 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.12 using 59 PHA bins.
# Reduced chi-squared = 1.142 for 57 degrees of freedom
# Null hypothesis probability = 2.151694e-01
Photon flux (15-150 keV) in 1 sec: 1.36719 ( -0.241573 0.242552 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.09672e-07 ( -2.01917e-08 2.0383e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.128 sec. to 1.128 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.123449 ( -1.60739 1.15727 )
Epeak [keV] : 76.9189 ( -21.3064 233.868 )
Norm@50keV : 4.70381E-02 ( -0.0470388 0.24063 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.64 using 59 PHA bins.
# Reduced chi-squared = 1.101 for 56 degrees of freedom
# Null hypothesis probability = 2.814323e-01
Photon flux (15-150 keV) in 1 sec: 1.31635 ( -0.24574 0.24702 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.02687e-07 ( -2.18689e-08 2.1963e-08 ) ergs/cm2
Band function
Time interval is from 0.128 sec. to 1.128 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.18874 ( -1.1249 1.0166 )
beta : -1.72326 ( 9.02834 19.0283 )
Epeak [keV] : 35.1325 ( -19.7964 167.198 )
Norm@50keV : 49.3968 ( -49.5342 32.7189 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.17 using 59 PHA bins.
# Reduced chi-squared = 1.094 for 55 degrees of freedom
# Null hypothesis probability = 2.942082e-01
Photon flux (15-150 keV) in 1 sec: 1.33112 ( 5.66888 -0.24243 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.05862e-07 ( -1.05855e-07 -2.04805e-08 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 16.0242 (-2.91109 3.66554)
R^2/D10^2 : 0.133663 (-0.0686322 0.13417)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.52 using 59 PHA bins.
# Reduced chi-squared = 1.132 for 57 degrees of freedom
# Null hypothesis probability = 2.304633e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.094e-09 2.739e-09
25- 50 2.989e-08 9.100e-09
50-150 5.368e-08 1.901e-08
15-150 9.066e-08 2.400e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-77.7999 -199.363)
Norm : 5.73581 (-0.98128 0.98131)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.80 using 59 PHA bins.
# Reduced chi-squared = 1.137 for 57 degrees of freedom
# Null hypothesis probability = 2.231291e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.428e-08 8.320e-09
25- 50 2.747e-08 1.595e-08
50-150 6.026e-08 3.401e-08
15-150 1.020e-07 5.720e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.84103 (-5.42807 6.32465)
R1^2/D10^2 : 0.436770 (-0.35076 3.22647)
kT2 [keV] : 28.3807 (-23.9685 -28.3807)
R2^2/D10^2 : 1.19388E-02 (-0.0119191 0.111852)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.82 using 59 PHA bins.
# Reduced chi-squared = 1.106 for 55 degrees of freedom
# Null hypothesis probability = 2.743547e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.012e-08 6.230e-09
25- 50 3.019e-08 1.770e-08
50-150 6.475e-08 3.452e-08
15-150 1.051e-07 5.225e-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: 1.19984 ( -0.158489 0.154994 )
Norm@50keV : 6.76545E-03 ( -0.000649458 0.00064835 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 44.42 using 59 PHA bins.
# Reduced chi-squared = 0.7792 for 57 degrees of freedom
# Null hypothesis probability = 8.877936e-01
Photon flux (15-150 keV) in 8.328 sec: 0.794105 ( -0.0802969 0.0806428 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.71645e-07 ( -5.69197e-08 5.70819e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.389324 ( -0.761367 0.646023 )
Epeak [keV] : 111.497 ( -29.9306 192.973 )
Norm@50keV : 1.58720E-02 ( -0.00769145 0.018291 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.66 using 59 PHA bins.
# Reduced chi-squared = 0.7083 for 56 degrees of freedom
# Null hypothesis probability = 9.516805e-01
Photon flux (15-150 keV) in 8.328 sec: 0.770934 ( -0.082175 0.08257 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.53821e-07 ( -6.04238e-08 5.99708e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.415914 ( -0.653014 0.568552 )
beta : -9.36665 ( 9.37141 19.3714 )
Epeak [keV] : 114.162 ( -21.2399 161.123 )
Norm@50keV : 1.53602E-02 ( -0.00638923 0.00918792 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 39.67 using 59 PHA bins.
# Reduced chi-squared = 0.7213 for 55 degrees of freedom
# Null hypothesis probability = 9.405878e-01
Photon flux (15-150 keV) in 8.328 sec: 0.771851 ( ) 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) = 1.20e-07
S(50-100 keV) = 2.09e-07
T90 vs. Hardness ratio plot
T90 = 7.45600003004074 sec.
Hardness ratio (energy fluence ratio) = 1.74167
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 2.13288
Count Ratio (50-100 keV) / (15-25 keV) = 2.06739
Mask shadow pattern
IMX = -1.025355958080295E+00, IMY = 2.139408541184475E-01
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:
-565.115400 -462.111800
-239.216000 -3.772000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
339.3997 -30.2084 2.3 33.7 51.1 1.6931 5.0 ------ UNKNOWN
18.5818 -34.4177 2.7 17.0 126.2 0.8709 4.3 ------ UNKNOWN
31.6072 -48.4785 3.0 11.0 -161.8 0.7469 3.8 ------ UNKNOWN
35.4039 -58.5806 2.2 13.7 -113.4 1.0127 5.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-3.772000 4.556000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
335.9712 -58.6717 1.9 23.3 -7.5 0.1556 5.9 ------ UNKNOWN
65.7458 -25.1297 0.7 46.3 -168.2 0.8453 17.5 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
83.284600 962.797600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6274 22.0117 0.4 50.2 -161.5 35.8122 31.2 0.4 Crab
33.7054 -8.0103 3.1 35.0 110.4 3.4076 3.7 ------ UNKNOWN
49.9799 19.1694 2.6 46.9 156.2 6.0380 4.4 ------ UNKNOWN
67.3400 -60.2036 3.1 35.1 -4.7 2.2977 3.7 ------ UNKNOWN
69.6942 -18.9640 2.8 7.2 -151.7 1.6116 4.2 ------ UNKNOWN
104.6001 -65.9932 3.6 47.6 -23.5 2.6985 3.2 ------ UNKNOWN
123.1778 -52.7653 3.3 50.7 -44.5 9.1337 3.5 ------ UNKNOWN
Plot creation:
Sun May 31 06:28:50 EDT 2015