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Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
60.4377 -32.7078 0.0085 45.6811 139.4474 5.0664471 22.870 TRIG_00505054
Foreground time interval of the image:
-2.636 12.173 (delta_t = 14.809 [sec])
Background time interval of the image:
-239.728 -2.636 (delta_t = 237.092 [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)
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 -2.636 sec. to 68.788 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.81649 ( -0.0855838 0.0867478 )
Norm@50keV : 7.90984E-03 ( -0.000389179 0.000386842 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.77 using 59 PHA bins.
# Reduced chi-squared = 0.8731 for 57 degrees of freedom
# Null hypothesis probability = 7.405679e-01
Photon flux (15-150 keV) in 71.42 sec: 1.09701 ( -0.0525975 0.0527164 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.19796e-06 ( -2.59356e-07 2.60465e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from -2.636 sec. to 68.788 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.69746 ( -0.340919 0.330563 )
Epeak [keV] : 122.519 ( -59.4084 -122.575 )
Norm@50keV : 9.11670E-03 ( -0.0013253 0.00445073 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 49.37 using 59 PHA bins.
# Reduced chi-squared = 0.8817 for 56 degrees of freedom
# Null hypothesis probability = 7.220665e-01
Photon flux (15-150 keV) in 71.42 sec: 1.08921 ( -0.05626 0.02826 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.14838e-06 ( -2.957e-07 2.91808e-07 ) ergs/cm2
Band function
Time interval is from -2.636 sec. to 68.788 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -7.33776E-02 ( -2.40664 3.85004 )
beta : -1.92937 ( -0.147205 0.129513 )
Epeak [keV] : 33.8706 ( -9.15859 34.9952 )
Norm@50keV : 0.114018 ( -0.113273 152.981 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.58 using 59 PHA bins.
# Reduced chi-squared = 0.8287 for 55 degrees of freedom
# Null hypothesis probability = 8.135480e-01
Photon flux (15-150 keV) in 71.42 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 5.07243e-06 ( -5.07193e-06 -2.77938e-07 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.1071 ( )
R^2/D10^2 : 0.243385 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 174.85 using 59 PHA bins.
# Reduced chi-squared = 3.0675 for 57 degrees of freedom
# Null hypothesis probability = 6.750156e-14
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.393e-07 4.514e-08
25- 50 1.715e-06 8.785e-08
50-150 1.520e-06 1.686e-07
15-150 3.775e-06 2.035e-07
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 99.9632 (-12.4206 31.4878)
Norm : 4.79126 (-0.409685 0.287028)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.20 using 59 PHA bins.
# Reduced chi-squared = 0.9333 for 57 degrees of freedom
# Null hypothesis probability = 6.184518e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.944e-07 7.713e-08
25- 50 1.546e-06 8.749e-08
50-150 2.506e-06 6.846e-07
15-150 4.946e-06 7.299e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.05510 (-0.785941 0.836239)
R1^2/D10^2 : 1.37516 (-0.444724 0.723364)
kT2 [keV] : 27.5658 (-4.5156 7.07867)
R2^2/D10^2 : 8.60415E-03 (-0.00466248 0.00806269)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 45.02 using 59 PHA bins.
# Reduced chi-squared = 0.8185 for 55 degrees of freedom
# Null hypothesis probability = 8.294024e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.685e-07 1.196e-07
25- 50 1.558e-06 1.611e-07
50-150 2.710e-06 6.506e-07
15-150 5.137e-06 8.038e-07
Peak spectrum fit
Power-law model
Time interval is from 0.044 sec. to 1.044 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25893 ( -0.184942 0.182546 )
Norm@50keV : 5.42177E-02 ( -0.00594418 0.00594416 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 68.24 using 59 PHA bins.
# Reduced chi-squared = 1.197 for 57 degrees of freedom
# Null hypothesis probability = 1.464039e-01
Photon flux (15-150 keV) in 1 sec: 6.42187 ( -0.73032 0.731948 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.41344e-07 ( -6.44109e-08 6.47456e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.044 sec. to 1.044 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.01167 ( -0.730325 0.346306 )
Epeak [keV] : 212.693 ( -212.745 -212.745 )
Norm@50keV : 7.15550E-02 ( -0.0266655 0.0869649 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.81 using 59 PHA bins.
# Reduced chi-squared = 1.211 for 56 degrees of freedom
# Null hypothesis probability = 1.338923e-01
Photon flux (15-150 keV) in 1 sec: 6.37577 ( -0.7391 0.74073 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.34825e-07 ( -6.8582e-08 6.7367e-08 ) ergs/cm2
Band function
Time interval is from 0.044 sec. to 1.044 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -14.2971 -5 )
beta : -1.49618 ( -0.31282 0.242483 )
Epeak [keV] : 31.8943 ( -6.74956 5.63055 )
Norm@50keV : 1167.76 ( -126.263 3574.94 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.93 using 59 PHA bins.
# Reduced chi-squared = 1.126 for 55 degrees of freedom
# Null hypothesis probability = 2.425901e-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] : 17.3948 (-2.8162 3.4322)
R^2/D10^2 : 0.459682 (-0.205893 0.374011)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 88.60 using 59 PHA bins.
# Reduced chi-squared = 1.554 for 57 degrees of freedom
# Null hypothesis probability = 4.645858e-03
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.814e-08 6.545e-09
25- 50 1.268e-07 2.391e-08
50-150 2.759e-07 6.130e-08
15-150 4.308e-07 6.895e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 26.8109 (-2.9829 2.98269)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.65 using 59 PHA bins.
# Reduced chi-squared = 1.310 for 57 degrees of freedom
# Null hypothesis probability = 5.837821e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.678e-08 2.305e-08
25- 50 1.285e-07 7.015e-08
50-150 2.817e-07 1.538e-07
15-150 4.770e-07 2.462e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 9.29163 (-1.98496 1.87702)
R1^2/D10^2 : 2.78961 (-1.46259 2.50017)
kT2 [keV] : 45.2347 (-16.3042 134.648)
R2^2/D10^2 : 1.65852E-02 (-0.0139367 0.0501527)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.01 using 59 PHA bins.
# Reduced chi-squared = 1.127 for 55 degrees of freedom
# Null hypothesis probability = 2.405067e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.163e-08 2.232e-08
25- 50 1.345e-07 5.269e-08
50-150 3.557e-07 1.823e-07
15-150 5.419e-07 2.361e-07
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: 1.55710 ( -0.0953858 0.095841 )
Norm@50keV : 2.30627E-02 ( -0.00129996 0.00129773 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.01 using 59 PHA bins.
# Reduced chi-squared = 1.141 for 57 degrees of freedom
# Null hypothesis probability = 2.178019e-01
Photon flux (15-150 keV) in 14.81 sec: 2.92564 ( -0.170131 0.17043 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.21226e-06 ( -1.92893e-07 1.93484e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.25020 ( -0.397238 0.344633 )
Epeak [keV] : 124.354 ( -44.1598 -124.356 )
Norm@50keV : 3.28644E-02 ( -0.0103898 0.0185805 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 62.98 using 59 PHA bins.
# Reduced chi-squared = 1.125 for 56 degrees of freedom
# Null hypothesis probability = 2.430331e-01
Photon flux (15-150 keV) in 14.81 sec: 2.88756 ( -0.17575 0.17598 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.15296e-06 ( -2.08999e-07 2.07533e-07 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 2.05035 ( -1.40217 4.10258 )
beta : -1.73883 ( -0.173161 0.144462 )
Epeak [keV] : 33.8275 ( -9.181 14.0437 )
Norm@50keV : 6.06427 ( -6.06443 348.429 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.40 using 59 PHA bins.
# Reduced chi-squared = 1.007 for 55 degrees of freedom
# Null hypothesis probability = 4.596853e-01
Photon flux (15-150 keV) in 14.81 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.12066e-06 ( -3.12056e-06 -1.95477e-07 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.47e-06
S(50-100 keV) = 1.67e-06
T90 vs. Hardness ratio plot
T90 = 62.8479999303818 sec.
Hardness ratio (energy fluence ratio) = 1.13605
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.31174
Count Ratio (50-100 keV) / (15-25 keV) = 0.82054
Mask shadow pattern
IMX = -7.780904702911140E-01, IMY = -6.657892182733026E-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:
-239.728000 -2.636000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
31.8570 -39.6562 2.8 33.3 106.5 1.5645 4.2 ------ UNKNOWN
47.4952 -61.1413 2.6 16.3 148.5 0.7845 4.5 ------ UNKNOWN
303.9087 -37.2138 3.4 49.3 -2.7 1.3780 3.4 ------ UNKNOWN
294.7679 -53.9718 3.1 37.1 -22.1 0.8511 3.7 ------ UNKNOWN
114.4976 -35.5144 3.2 59.1 -166.1 4.4739 3.6 ------ UNKNOWN
192.4066 -77.7178 2.5 30.3 -97.9 1.2993 4.7 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-2.636000 12.172600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
60.4377 -32.7078 0.5 45.7 139.4 5.0665 22.9 ------ UNKNOWN
13.9409 -42.0485 2.4 29.9 81.0 0.4162 4.9 ------ UNKNOWN
284.5861 -34.9864 1.9 57.3 -19.7 1.0849 5.9 ------ UNKNOWN
281.4736 -33.8542 1.9 59.3 -22.0 1.4178 5.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
80.172600 962.308800
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
65.3180 18.9413 2.8 51.9 153.5 10.2703 4.1 ------ UNKNOWN
99.9367 12.8206 3.0 59.1 -166.0 13.1385 3.9 ------ UNKNOWN
66.0306 -75.5682 2.7 42.9 -34.3 3.6012 4.3 ------ UNKNOWN
110.9752 -58.7295 3.8 42.3 -68.8 7.0719 3.0 ------ UNKNOWN
Plot creation:
Sat May 30 21:28:44 EDT 2015