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
41.0866 35.4987 0.0150 36.6899 -152.2813 0.4147422 12.824 TRIG_00603954
Foreground time interval of the image:
-0.288 3.712 (delta_t = 4.000 [sec])
Background time interval of the image:
-617.787 -528.074 (delta_t = 89.713 [sec])
-239.288 -0.288 (delta_t = 239.000 [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 -0.288 sec. to 3.712 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.03718 ( -0.221124 0.237655 )
Norm@50keV : 6.19134E-03 ( -0.00100561 0.000980248 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.36 using 59 PHA bins.
# Reduced chi-squared = 0.8835 for 57 degrees of freedom
# Null hypothesis probability = 7.206078e-01
Photon flux (15-150 keV) in 4 sec: 0.944939 ( -0.117073 0.117085 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.28904e-07 ( -3.40528e-08 3.48968e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.288 sec. to 3.712 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.963811 ( -1.27918 1.00968 )
Epeak [keV] : 39.5551 ( )
Norm@50keV : 2.62392E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.04 using 59 PHA bins.
# Reduced chi-squared = 0.8401 for 56 degrees of freedom
# Null hypothesis probability = 7.973538e-01
Photon flux (15-150 keV) in 4 sec: 0.915105 ( -0.119791 0.120125 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.09014e-07 ( -3.49048e-08 3.84756e-08 ) ergs/cm2
Band function
Time interval is from -0.288 sec. to 3.712 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.847539 ( -1.09015 0.859583 )
beta : -3.60653 ( 3.18596 11.3956 )
Epeak [keV] : 41.0600 ( -16.9077 20.2736 )
Norm@50keV : 2.94764E-02 ( -0.0172138 0.566089 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.09 using 59 PHA bins.
# Reduced chi-squared = 0.8562 for 55 degrees of freedom
# Null hypothesis probability = 7.670975e-01
Photon flux (15-150 keV) in 4 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.10438e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 10.0038 (-1.34156 1.51857)
R^2/D10^2 : 0.448578 (-0.187776 0.32979)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.52 using 59 PHA bins.
# Reduced chi-squared = 0.9741 for 57 degrees of freedom
# Null hypothesis probability = 5.306830e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.658e-08 8.390e-09
25- 50 9.099e-08 1.466e-08
50-150 4.754e-08 1.473e-08
15-150 1.751e-07 2.908e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 60.6981 (-18.0092 30.5526)
Norm : 4.97035 (-0.927684 1.12714)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.34 using 59 PHA bins.
# Reduced chi-squared = 0.8306 for 57 degrees of freedom
# Null hypothesis probability = 8.153905e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.006e-08 8.240e-09
25- 50 7.646e-08 1.120e-08
50-150 8.784e-08 3.368e-08
15-150 2.144e-07 3.470e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 4.32095 (-2.16115 1.51679)
R1^2/D10^2 : 5.99914 (-4.98992 216.47)
kT2 [keV] : 13.4424 (-2.91924 7.09096)
R2^2/D10^2 : 0.116239 (-0.100556 0.133317)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 46.63 using 59 PHA bins.
# Reduced chi-squared = 0.8479 for 55 degrees of freedom
# Null hypothesis probability = 7.816586e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.914e-08 2.624e-08
25- 50 7.754e-08 4.028e-08
50-150 7.423e-08 4.476e-08
15-150 2.009e-07 1.027e-07
Peak spectrum fit
Power-law model
Time interval is from -0.288 sec. to 0.712 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.65760 ( -0.27066 0.28488 )
Norm@50keV : 1.12700E-02 ( -0.00202067 0.00197989 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.71 using 59 PHA bins.
# Reduced chi-squared = 1.346 for 57 degrees of freedom
# Null hypothesis probability = 4.194527e-02
Photon flux (15-150 keV) in 1 sec: 1.47529 ( -0.243119 0.243303 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.04738e-07 ( -1.96128e-08 1.99268e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.288 sec. to 0.712 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.621732 ( -1.8554 1.2166 )
Epeak [keV] : 64.2870 ( -14.6998 -64.2788 )
Norm@50keV : 3.90582E-02 ( -0.039091 0.28642 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.97 using 59 PHA bins.
# Reduced chi-squared = 1.339 for 56 degrees of freedom
# Null hypothesis probability = 4.607907e-02
Photon flux (15-150 keV) in 1 sec: 1.42661 ( -0.25766 0.25334 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.85911e-08 ( -2.03064e-08 2.14299e-08 ) ergs/cm2
Band function
Time interval is from -0.288 sec. to 0.712 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.755033 ( 0.75479 2.20366 )
beta : -2.51489 ( 2.47768 3.08106 )
Epeak [keV] : 65.9141 ( -65.7562 434.608 )
Norm@50keV : 3.34741E-02 ( -0.0394148 1.63392e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 74.90 using 59 PHA bins.
# Reduced chi-squared = 1.362 for 55 degrees of freedom
# Null hypothesis probability = 3.840507e-02
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 9.91798e-08 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 13.9405 (-2.12681 2.53027)
R^2/D10^2 : 0.223513 (-0.102243 0.180999)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.97 using 59 PHA bins.
# Reduced chi-squared = 1.368 for 57 degrees of freedom
# Null hypothesis probability = 3.395781e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.179e-09 2.721e-09
25- 50 3.400e-08 8.455e-09
50-150 4.340e-08 1.627e-08
15-150 8.658e-08 1.938e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 149.105 (-71.505 -146.407)
Norm : 6.10798 (-1.07533 1.44935)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 75.63 using 59 PHA bins.
# Reduced chi-squared = 1.327 for 57 degrees of freedom
# Null hypothesis probability = 4.991289e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.570e-08 8.890e-09
25- 50 2.907e-08 1.595e-08
50-150 5.723e-08 3.434e-08
15-150 1.020e-07 5.770e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 2.77181 (-2.06339 2.14189)
R1^2/D10^2 : 74.1679 (-68.9555 1.57849e+08)
kT2 [keV] : 15.6694 (-2.67574 3.66415)
R2^2/D10^2 : 0.135842 (-0.0748035 0.131337)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.12 using 59 PHA bins.
# Reduced chi-squared = 1.293 for 55 degrees of freedom
# Null hypothesis probability = 7.070752e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.527e-08 7.097e-09
25- 50 2.954e-08 1.162e-08
50-150 4.873e-08 2.162e-08
15-150 9.353e-08 3.626e-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: 2.03718 ( -0.221124 0.237655 )
Norm@50keV : 6.19134E-03 ( -0.00100561 0.000980248 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.36 using 59 PHA bins.
# Reduced chi-squared = 0.8835 for 57 degrees of freedom
# Null hypothesis probability = 7.206078e-01
Photon flux (15-150 keV) in 4 sec: 0.944939 ( -0.117073 0.117085 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.28904e-07 ( -3.40528e-08 3.48968e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.963811 ( -1.27918 1.00968 )
Epeak [keV] : 39.5551 ( )
Norm@50keV : 2.62392E-02 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.04 using 59 PHA bins.
# Reduced chi-squared = 0.8401 for 56 degrees of freedom
# Null hypothesis probability = 7.973538e-01
Photon flux (15-150 keV) in 4 sec: 0.915105 ( -0.119791 0.120125 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.09014e-07 ( -3.49048e-08 3.84756e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.847539 ( -1.09015 0.859583 )
beta : -3.60653 ( 3.18596 11.3956 )
Epeak [keV] : 41.0600 ( -16.9077 20.2736 )
Norm@50keV : 2.94764E-02 ( -0.0172138 337.824 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 47.09 using 59 PHA bins.
# Reduced chi-squared = 0.8562 for 55 degrees of freedom
# Null hypothesis probability = 7.670975e-01
Photon flux (15-150 keV) in 4 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.10438e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 6.96e-08
S(50-100 keV) = 6.79e-08
T90 vs. Hardness ratio plot
T90 = 3 sec.
Hardness ratio (energy fluence ratio) = 0.975575
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.991344
Count Ratio (50-100 keV) / (15-25 keV) = 0.467555
Mask shadow pattern
IMX = -6.595959057654972E-01, IMY = 3.465701845356184E-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:
-617.787410 -528.074300
-239.288000 -0.288000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
34.9368 -36.5817 3.5 37.4 51.1 1.8086 3.3 ------ UNKNOWN
12.1687 12.9981 2.4 37.0 148.6 2.1714 4.7 ------ UNKNOWN
70.4000 -34.1562 2.5 40.0 4.4 1.6834 4.5 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.288000 3.712000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
20.4456 40.6399 2.7 47.9 -171.5 0.2094 4.3 ------ UNKNOWN
85.5386 -26.3960 2.2 45.2 -16.8 0.2222 5.2 ------ UNKNOWN
41.0866 35.4987 0.9 36.7 -152.3 0.4147 12.8 ------ UNKNOWN
15.0094 51.7186 2.7 59.0 -166.9 0.6259 4.2 ------ UNKNOWN
88.5484 0.9607 1.9 41.8 -56.9 0.4047 6.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
82.012590 653.112600
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6306 22.0131 0.6 39.3 -74.2 23.2987 19.4 0.2 Crab
338.9420 52.4758 2.6 46.2 139.3 7.4422 4.4 ------ UNKNOWN
20.6628 10.3706 2.7 31.2 49.0 2.4809 4.3 ------ UNKNOWN
339.5967 62.9115 2.9 46.1 153.8 3.9823 3.9 ------ UNKNOWN
28.9823 62.0574 2.5 27.6 175.4 1.8919 4.5 ------ UNKNOWN
48.0960 1.0510 3.7 35.0 -4.8 1.5152 3.1 ------ UNKNOWN
169.7148 83.0760 3.3 59.0 -166.1 9.0209 3.5 ------ UNKNOWN
Plot creation:
Sat May 30 12:57:50 EDT 2015