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
74.5870 -2.5267 0.0061 14.3278 32.8673 0.5954407 31.689 TRIG_00440606
Foreground time interval of the image:
-0.016 1.108 (delta_t = 1.124 [sec])
Background time interval of the image:
-97.735 -0.016 (delta_t = 97.719 [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 0.064000
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 0.064000
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 0.064000
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 -0.016 sec. to 1.108 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.625101 ( -0.100831 0.0982707 )
Norm@50keV : 3.05638E-02 ( -0.00170826 0.00169297 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.44 using 59 PHA bins.
# Reduced chi-squared = 1.148 for 57 degrees of freedom
# Null hypothesis probability = 2.070765e-01
Photon flux (15-150 keV) in 1.124 sec: 3.55809 ( -0.186181 0.186405 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.34094e-07 ( -2.47942e-08 2.49464e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.016 sec. to 1.108 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.620663 ( -0.105935 0.0958313 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 3.08096E-02 ( -0.00162168 0.00728118 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.51 using 59 PHA bins.
# Reduced chi-squared = 1.170 for 56 degrees of freedom
# Null hypothesis probability = 1.801357e-01
Photon flux (15-150 keV) in 1.124 sec: 3.55857 ( -0.18771 0.18501 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.34071e-07 ( -2.46999e-08 2.47494e-08 ) ergs/cm2
Band function
Time interval is from -0.016 sec. to 1.108 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -5 -5 )
beta : -0.625380 ( -0.0982556 0.101062 )
Epeak [keV] : 17.4241 ( -17.4241 666.723 )
Norm@50keV : 1.09107E+04 ( -559.794 2.32264e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.43 using 59 PHA bins.
# Reduced chi-squared = 1.190 for 55 degrees of freedom
# Null hypothesis probability = 1.585037e-01
Photon flux (15-150 keV) in 1.124 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] : 29.5548 ( )
R^2/D10^2 : 5.71798E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 123.00 using 59 PHA bins.
# Reduced chi-squared = 2.1579 for 57 degrees of freedom
# Null hypothesis probability = 9.432422e-07
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.864e-09 9.869e-10
25- 50 5.434e-08 4.423e-09
50-150 3.372e-07 2.788e-08
15-150 4.004e-07 2.900e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 12.9085 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 296.73 using 59 PHA bins.
# Reduced chi-squared = 5.2058 for 57 degrees of freedom
# Null hypothesis probability = 4.049208e-34
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.613e-08 2.450e-09
25- 50 6.950e-08 6.508e-09
50-150 1.524e-07 3.815e-08
15-150 2.580e-07 4.305e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.8933 (-2.55449 3.03038)
R1^2/D10^2 : 0.558905 (-0.25933 0.603576)
kT2 [keV] : 63.6982 (-18.8653 83.4345)
R2^2/D10^2 : 7.06898E-03 (-0.00417976 0.00967732)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.69 using 59 PHA bins.
# Reduced chi-squared = 1.158 for 55 degrees of freedom
# Null hypothesis probability = 1.973773e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.844e-08 4.416e-09
25- 50 6.538e-08 1.581e-08
50-150 3.594e-07 1.560e-07
15-150 4.432e-07 1.727e-07
Peak spectrum fit
Power-law model
Time interval is from -0.016 sec. to 0.984 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.603045 ( -0.102267 0.0995965 )
Norm@50keV : 3.31863E-02 ( -0.00187942 0.00186145 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.64 using 59 PHA bins.
# Reduced chi-squared = 1.187 for 57 degrees of freedom
# Null hypothesis probability = 1.581903e-01
Photon flux (15-150 keV) in 1 sec: 3.87326 ( -0.204071 0.204297 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.23768e-07 ( -2.44395e-08 2.45888e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.016 sec. to 0.984 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.599544 ( -0.107598 0.0963193 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 3.34587E-02 ( -0.00178391 0.00717078 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.73 using 59 PHA bins.
# Reduced chi-squared = 1.209 for 56 degrees of freedom
# Null hypothesis probability = 1.354385e-01
Photon flux (15-150 keV) in 1 sec: 3.87477 ( -0.20565 0.20203 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.24078e-07 ( -2.4638e-08 2.3892e-08 ) ergs/cm2
Band function
Time interval is from -0.016 sec. to 0.984 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.894806 ( 0.894806 0.894806 )
beta : -0.603050 ( -0.0995012 0.102447 )
Epeak [keV] : 16.0922 ( -16.0922 -16.0922 )
Norm@50keV : 4.65017E-02 ( -0.0151641 505153 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 67.64 using 59 PHA bins.
# Reduced chi-squared = 1.230 for 55 degrees of freedom
# Null hypothesis probability = 1.178362e-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] : 30.2137 ( )
R^2/D10^2 : 5.88726E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 124.61 using 59 PHA bins.
# Reduced chi-squared = 2.1862 for 57 degrees of freedom
# Null hypothesis probability = 5.967211e-07
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 8.371e-09 8.860e-10
25- 50 5.179e-08 4.600e-09
50-150 3.330e-07 2.810e-08
15-150 3.932e-07 2.870e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 199.363 ( )
Norm : 13.9120 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 302.89 using 59 PHA bins.
# Reduced chi-squared = 5.3138 for 57 degrees of freedom
# Null hypothesis probability = 3.260961e-35
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.464e-08 2.060e-09
25- 50 6.664e-08 6.675e-09
50-150 1.461e-07 3.913e-08
15-150 2.474e-07 4.185e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 10.4755 (-2.62454 3.21481)
R1^2/D10^2 : 0.654480 (-0.301503 0.731521)
kT2 [keV] : 61.1030 (-18.4673 78.8155)
R2^2/D10^2 : 8.55688E-03 (-0.0047079 0.0104553)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.30 using 59 PHA bins.
# Reduced chi-squared = 1.205 for 55 degrees of freedom
# Null hypothesis probability = 1.413767e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.781e-08 6.039e-09
25- 50 6.170e-08 1.753e-08
50-150 3.494e-07 1.605e-07
15-150 4.289e-07 1.680e-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: 0.625101 ( -0.100831 0.0982707 )
Norm@50keV : 3.05638E-02 ( -0.00170826 0.00169297 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.44 using 59 PHA bins.
# Reduced chi-squared = 1.148 for 57 degrees of freedom
# Null hypothesis probability = 2.070765e-01
Photon flux (15-150 keV) in 1.124 sec: 3.55809 ( -0.186181 0.186405 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.34094e-07 ( -2.47942e-08 2.49464e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.620663 ( -0.105935 0.0958313 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 3.08096E-02 ( -0.00162168 0.00728118 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.51 using 59 PHA bins.
# Reduced chi-squared = 1.170 for 56 degrees of freedom
# Null hypothesis probability = 1.801357e-01
Photon flux (15-150 keV) in 1.124 sec: 3.55857 ( -0.18771 0.18501 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.34071e-07 ( -2.46999e-08 2.47494e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -5 -5 )
beta : -0.625380 ( -0.0982556 0.101062 )
Epeak [keV] : 17.4241 ( -17.4241 666.723 )
Norm@50keV : 1.09107E+04 ( -559.794 2.32264e+06 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 65.43 using 59 PHA bins.
# Reduced chi-squared = 1.190 for 55 degrees of freedom
# Null hypothesis probability = 1.585037e-01
Photon flux (15-150 keV) in 1.124 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) = 6.15e-08
S(50-100 keV) = 1.59e-07
T90 vs. Hardness ratio plot
T90 = 0.827999949455261 sec.
Hardness ratio (energy fluence ratio) = 2.58537
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 2.01643
Count Ratio (50-100 keV) / (15-25 keV) = 2.58869
Mask shadow pattern
IMX = 2.145298307916920E-01, IMY = -1.386118796284431E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 0.064000
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:
-97.735400 -0.016000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6292 22.0135 0.8 36.1 70.7 4.3625 14.7 0.2 Crab
135.4922 -40.5295 2.3 52.5 -159.3 1.6319 4.9 2.2 Vela X-1
49.5539 -16.8971 2.6 32.5 -29.5 0.5537 4.4 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.016000 1.108000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.5213 21.9142 5.4 36.0 70.5 -0.0922 -2.2 8.7 Crab
135.7136 -40.6047 6.2 52.7 -159.2 -0.1006 -1.9 9.0 Vela X-1
75.6639 24.2504 2.3 39.0 59.1 0.2661 5.0 ------ UNKNOWN
74.5870 -2.5267 0.4 14.3 32.9 0.5955 31.7 ------ UNKNOWN
41.8667 -0.0328 2.8 43.2 -4.6 0.1204 4.1 ------ UNKNOWN
25.7403 1.0082 2.0 58.8 -10.0 0.5727 5.6 ------ UNKNOWN
118.0326 -47.6781 2.0 44.3 -143.4 0.1945 5.8 ------ UNKNOWN
57.9937 -37.8916 2.4 32.7 -71.5 0.1344 4.7 ------ UNKNOWN
114.3862 -51.7391 2.2 45.2 -136.9 0.2088 5.2 ------ UNKNOWN
51.4257 -40.3851 2.4 38.2 -69.6 0.2011 4.9 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
44.264630 941.564590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6332 22.0176 0.3 26.1 85.6 37.4536 41.1 0.2 Crab
122.6020 6.9819 2.5 48.8 144.7 13.0251 4.7 ------ UNKNOWN
79.6160 20.3299 3.0 23.4 78.2 2.9948 3.8 ------ UNKNOWN
30.8312 -22.8492 4.8 47.0 -53.1 8.4787 2.4 ------ UNKNOWN
23.5306 -16.0534 4.1 52.0 -42.2 10.6704 2.8 ------ UNKNOWN
Plot creation:
Sat May 30 23:22:46 EDT 2015