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
102.2784 50.7460 0.0208 29.1612 -68.1976 0.9886091 9.233 TRIG_00311874
Foreground time interval of the image:
-0.764 54.517 (delta_t = 55.281 [sec])
Background time interval of the image:
-239.784 -0.764 (delta_t = 239.020 [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 8.192000
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 8.192000
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 8.192000
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 -0.764 sec. to 68.388 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.42775 ( -0.317377 0.319741 )
Norm@50keV : 8.82617E-04 ( -0.000167269 0.000165719 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.31 using 59 PHA bins.
# Reduced chi-squared = 0.9528 for 57 degrees of freedom
# Null hypothesis probability = 5.765862e-01
Photon flux (15-150 keV) in 69.15 sec: 0.108183 ( -0.0200869 0.0201202 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.86497e-07 ( -1.22133e-07 1.24785e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.764 sec. to 68.388 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.816952 ( -1.73459 0.88722 )
Epeak [keV] : 94.5658 ( -41.1858 -94.5617 )
Norm@50keV : 1.82368E-03 ( -0.00112412 0.0115822 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.67 using 59 PHA bins.
# Reduced chi-squared = 0.9584 for 56 degrees of freedom
# Null hypothesis probability = 5.634678e-01
Photon flux (15-150 keV) in 69.15 sec: 0.105488 ( -0.0211067 0.020927 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.56983e-07 ( -1.35714e-07 1.39247e-07 ) ergs/cm2
Band function
Time interval is from -0.764 sec. to 68.388 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.694864 ( 0.688822 5.36682 )
beta : -1.84794 ( 1.86521 0.707765 )
Epeak [keV] : 81.8103 ( -81.6924 541.353 )
Norm@50keV : 2.16941E-03 ( -0.00131849 40.0206 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.58 using 59 PHA bins.
# Reduced chi-squared = 0.9743 for 55 degrees of freedom
# Null hypothesis probability = 5.288396e-01
Photon flux (15-150 keV) in 69.15 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] : 15.2024 (-3.01103 3.98257)
R^2/D10^2 : 1.20325E-02 (-0.00668687 0.0139612)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 57.77 using 59 PHA bins.
# Reduced chi-squared = 1.014 for 57 degrees of freedom
# Null hypothesis probability = 4.464865e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.017e-08 1.596e-08
25- 50 1.616e-07 4.754e-08
50-150 2.556e-07 1.005e-07
15-150 4.574e-07 1.222e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 (-97.2764 -199.363)
Norm : 0.445361 (-0.0815811 0.0815825)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.23 using 59 PHA bins.
# Reduced chi-squared = 0.9514 for 57 degrees of freedom
# Null hypothesis probability = 5.796007e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.669e-08 4.522e-08
25- 50 1.475e-07 8.426e-08
50-150 3.235e-07 1.834e-07
15-150 5.477e-07 3.126e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.00571 (-2.8427 -5.00926)
R1^2/D10^2 : 0.278442 (-0.262932 14.7107)
kT2 [keV] : 19.5453 (-5.35464 -19.5473)
R2^2/D10^2 : 4.42222E-03 (-0.00438288 0.0100607)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.62 using 59 PHA bins.
# Reduced chi-squared = 0.9750 for 55 degrees of freedom
# Null hypothesis probability = 5.273347e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.977e-08 3.879e-08
25- 50 1.423e-07 7.396e-08
50-150 3.158e-07 1.863e-07
15-150 5.278e-07 2.867e-07
Peak spectrum fit
Power-law model
Time interval is from 3.884 sec. to 4.884 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.77574 ( -0.46145 0.50456 )
Norm@50keV : 4.36814E-03 ( -0.00150359 0.00146456 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.09 using 59 PHA bins.
# Reduced chi-squared = 1.177 for 57 degrees of freedom
# Null hypothesis probability = 1.695447e-01
Photon flux (15-150 keV) in 1 sec: 0.596354 ( -0.173606 0.173608 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.02447e-08 ( -1.36295e-08 1.44853e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 3.884 sec. to 4.884 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -0.819383 ( -7.95979 2.56125 )
Epeak [keV] : 41.1191 ( -10.9831 87.1649 )
Norm@50keV : 0.168939 ( -0.198267 23499.6 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.00 using 59 PHA bins.
# Reduced chi-squared = 1.143 for 56 degrees of freedom
# Null hypothesis probability = 2.161718e-01
Photon flux (15-150 keV) in 1 sec: 0.559349 ( -0.170705 0.174316 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.10251e-08 ( -1.11707e-08 1.60239e-08 ) ergs/cm2
Band function
Time interval is from 3.884 sec. to 4.884 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 3.71654 ( -2.69463 -0.997303 )
beta : -2.97847 ( 9.37167 19.3708 )
Epeak [keV] : 34.5416 ( -10.8534 80.4113 )
Norm@50keV : 15.7626 ( -15.7401 45.8011 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.06 using 59 PHA bins.
# Reduced chi-squared = 1.147 for 55 degrees of freedom
# Null hypothesis probability = 2.128442e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.44732e-08 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.1153 (-2.44712 3.49751)
R^2/D10^2 : 0.294918 (-0.200163 0.53412)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.08 using 59 PHA bins.
# Reduced chi-squared = 1.124 for 57 degrees of freedom
# Null hypothesis probability = 2.420315e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.169e-09 3.508e-09
25- 50 1.559e-08 9.530e-09
50-150 8.409e-09 6.137e-09
15-150 3.016e-08 1.864e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 82.8938 (-46.1074 -82.8819)
Norm : 2.83878 (-0.92915 1.45432)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.74 using 59 PHA bins.
# Reduced chi-squared = 1.153 for 57 degrees of freedom
# Null hypothesis probability = 1.998855e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 7.382e-09 4.515e-09
25- 50 1.225e-08 7.500e-09
50-150 1.771e-08 1.496e-08
15-150 3.735e-08 2.559e-08
Double BB
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.63 using 59 PHA bins.
#Fit statistic : Chi-Squared = 63.57 using 59 PHA bins.
#Fit statistic : Chi-Squared = 63.55 using 59 PHA bins.
#Fit statistic : Chi-Squared = 63.54 using 59 PHA bins.
# Reduced chi-squared = 1.157 for 55 degrees of freedom
# Reduced chi-squared = 1.156 for 55 degrees of freedom
# Reduced chi-squared = 1.155 for 55 degrees of freedom
# Reduced chi-squared = 1.155 for 55 degrees of freedom
# Null hypothesis probability = 1.986629e-01
# Null hypothesis probability = 2.002837e-01
# Null hypothesis probability = 2.006025e-01
# Null hypothesis probability = 2.009078e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.663e-09 5.865e-09
25- 50 1.470e-08 1.510e-08
50-150 1.266e-08 1.705e-08
15-150 3.402e-08 4.643e-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: 1.37295 ( -0.29983 0.299075 )
Norm@50keV : 1.06882E-03 ( -0.000187054 0.000186085 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.66 using 59 PHA bins.
# Reduced chi-squared = 0.7133 for 57 degrees of freedom
# Null hypothesis probability = 9.498839e-01
Photon flux (15-150 keV) in 55.28 sec: 0.129386 ( -0.022613 0.0226587 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.7416e-07 ( -1.11216e-07 1.13252e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.863021 ( -1.56373 0.775886 )
Epeak [keV] : 111.114 ( -111.114 -111.114 )
Norm@50keV : 1.94043E-03 ( -0.00103681 0.00956822 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.14 using 59 PHA bins.
# Reduced chi-squared = 0.7167 for 56 degrees of freedom
# Null hypothesis probability = 9.457801e-01
Photon flux (15-150 keV) in 55.28 sec: 0.126643 ( -0.023733 0.023551 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.50789e-07 ( -1.25192e-07 1.25324e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.644322 ( 0.630856 0.630856 )
beta : -1.71093 ( 1.71264 0.60025 )
Epeak [keV] : 84.5541 ( -82.452 -82.452 )
Norm@50keV : 2.62236E-03 ( -0.00282504 53.8241 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.00 using 59 PHA bins.
# Reduced chi-squared = 0.7273 for 55 degrees of freedom
# Null hypothesis probability = 9.357949e-01
Photon flux (15-150 keV) in 55.28 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) = 1.40e-07
S(50-100 keV) = 2.08e-07
T90 vs. Hardness ratio plot
T90 = 64.5079999864101 sec.
Hardness ratio (energy fluence ratio) = 1.48571
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.28875
Count Ratio (50-100 keV) / (15-25 keV) = 1.25656
Mask shadow pattern
IMX = 2.072424406940372E-01, IMY = 5.180804300206198E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 8.192000
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:
-239.784000 -0.764000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
149.6315 32.6804 2.7 11.1 78.1 0.7454 4.3 ------ UNKNOWN
125.6552 15.2709 2.4 22.2 -172.2 0.8125 4.9 ------ UNKNOWN
237.5247 77.4892 3.2 58.1 -6.6 3.7424 4.1 ------ UNKNOWN
237.7363 77.7405 3.5 58.0 -6.9 3.9758 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.764000 54.516600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
173.6700 18.0428 2.6 37.0 86.6 1.0559 4.4 ------ UNKNOWN
134.0828 -19.3465 2.7 54.6 161.8 1.8673 4.3 ------ UNKNOWN
189.0158 62.6614 2.4 42.2 11.6 0.6226 4.8 ------ UNKNOWN
121.1178 -14.6083 2.2 51.9 178.0 1.0905 5.1 ------ UNKNOWN
102.2785 50.7460 1.2 29.2 -68.2 0.9923 9.3 ------ UNKNOWN
354.8515 85.8788 2.8 58.1 -24.2 1.8782 4.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
109.116590 917.316600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6239 22.0145 0.2 32.2 -123.8 33.6420 49.3 0.5 Crab
121.6043 -3.7240 4.5 56.9 179.2 7.6114 2.6 ------ UNKNOWN
340.2034 66.7391 3.7 54.6 -1.8 4.6975 3.1 ------ UNKNOWN
13.4787 55.6433 2.8 49.7 -25.2 4.2904 4.2 ------ UNKNOWN
Plot creation:
Sun May 31 07:34:32 EDT 2015