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
129.4852 -66.5197 0.0078 21.8382 -108.3915 0.9915774 24.678 TRIG_00507185
Foreground time interval of the image:
-0.096 10.749 (delta_t = 10.845 [sec])
Background time interval of the image:
-239.552 -0.096 (delta_t = 239.456 [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 -0.096 sec. to 37.456 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.48341 ( -0.144281 0.144997 )
Norm@50keV : 2.55402E-03 ( -0.000199761 0.000198868 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.32 using 59 PHA bins.
# Reduced chi-squared = 1.058 for 57 degrees of freedom
# Null hypothesis probability = 3.566235e-01
Photon flux (15-150 keV) in 37.55 sec: 0.317443 ( -0.0249282 0.025016 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.12307e-07 ( -7.89185e-08 7.95793e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -0.096 sec. to 37.456 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.27299 ( -0.143569 0.14743 )
Epeak [keV] : 98.0219 ( -9999.35 -9999.35 )
Norm@50keV : 1.00383E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 58.46 using 59 PHA bins.
# Reduced chi-squared = 1.044 for 56 degrees of freedom
# Null hypothesis probability = 3.852299e-01
Photon flux (15-150 keV) in 37.55 sec: 0.317601 ( -0.025177 0.024707 ) ph/cm2/s
Energy fluence (15-150 keV) : 9.08886e-07 ( -3.80907e-08 8.14647e-08 ) ergs/cm2
Band function
Time interval is from -0.096 sec. to 37.456 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.20952 ( 1.20952 1.20952 )
beta : -1.48338 ( -0.144899 0.144295 )
Epeak [keV] : 32.5125 ( -32.5125 -32.5125 )
Norm@50keV : 5.05154E-03 ( -0.00204845 0.369105 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 60.32 using 59 PHA bins.
# Reduced chi-squared = 1.097 for 55 degrees of freedom
# Null hypothesis probability = 2.894226e-01
Photon flux (15-150 keV) in 37.55 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] : 15.3132 ( )
R^2/D10^2 : 3.21268E-02 ( )
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 117.25 using 59 PHA bins.
# Reduced chi-squared = 2.0569 for 57 degrees of freedom
# Null hypothesis probability = 4.652757e-06
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.901e-08 9.463e-09
25- 50 2.389e-07 2.677e-08
50-150 3.848e-07 6.453e-08
15-150 6.827e-07 6.721e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 1.29007 (-0.0989846 0.098985)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 63.59 using 59 PHA bins.
# Reduced chi-squared = 1.116 for 57 degrees of freedom
# Null hypothesis probability = 2.556474e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.211e-07 1.269e-08
25- 50 2.330e-07 3.676e-08
50-150 5.111e-07 2.035e-07
15-150 8.652e-07 2.199e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.21250 (-1.52189 1.63205)
R1^2/D10^2 : 0.322210 (-0.161457 0.433547)
kT2 [keV] : 33.3940 (-8.02684 16.5619)
R2^2/D10^2 : 1.92655E-03 (-0.00132248 0.00286192)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 61.08 using 59 PHA bins.
# Reduced chi-squared = 1.111 for 55 degrees of freedom
# Null hypothesis probability = 2.666897e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.160e-07 3.395e-08
25- 50 2.269e-07 5.877e-08
50-150 5.960e-07 2.902e-07
15-150 9.389e-07 3.027e-07
Peak spectrum fit
Power-law model
Time interval is from 2.132 sec. to 3.132 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.10355 ( -0.239105 0.233593 )
Norm@50keV : 1.06788E-02 ( -0.00138525 0.00138337 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.89 using 59 PHA bins.
# Reduced chi-squared = 0.9455 for 57 degrees of freedom
# Null hypothesis probability = 5.923465e-01
Photon flux (15-150 keV) in 1 sec: 1.23910 ( -0.165435 0.166016 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.11523e-07 ( -1.59292e-08 1.60597e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.132 sec. to 3.132 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.44971 ( -0.940265 0.243573 )
Epeak [keV] : 144.516 ( -9952.66 -9952.66 )
Norm@50keV : 1.62451E-03 ( )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.79 using 59 PHA bins.
# Reduced chi-squared = 0.9605 for 56 degrees of freedom
# Null hypothesis probability = 5.589953e-01
Photon flux (15-150 keV) in 1 sec: 1.23867 ( -0.17335 0.1656 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.11302e-07 ( -1.64626e-08 1.6267e-08 ) ergs/cm2
Band function
Time interval is from 2.132 sec. to 3.132 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.890100 ( 0.8901 0.8901 )
beta : -1.10355 ( 1.10355 0.239837 )
Epeak [keV] : 54.6540 ( -54.654 -54.654 )
Norm@50keV : 1.84415E-02 ( -0.00913667 0 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.89 using 59 PHA bins.
# Reduced chi-squared = 0.9799 for 55 degrees of freedom
# Null hypothesis probability = 5.169276e-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] : 22.1766 (-3.91854 5.06626)
R^2/D10^2 : 4.15101E-02 (-0.019503 0.0355575)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 66.86 using 59 PHA bins.
# Reduced chi-squared = 1.173 for 57 degrees of freedom
# Null hypothesis probability = 1.744675e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.764e-09 1.067e-09
25- 50 2.000e-08 4.860e-09
50-150 7.349e-08 1.783e-08
15-150 9.726e-08 2.071e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 200.000 ( )
Norm : 5.09662 (-0.680326 0.68029)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 64.38 using 59 PHA bins.
# Reduced chi-squared = 1.129 for 57 degrees of freedom
# Null hypothesis probability = 2.341492e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.269e-08 7.145e-09
25- 50 2.442e-08 1.345e-08
50-150 5.355e-08 2.953e-08
15-150 9.067e-08 4.989e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 6.34412 (-3.05106 4.17011)
R1^2/D10^2 : 1.37436 (-1.1039 20.6794)
kT2 [keV] : 31.4079 (-8.05128 19.7403)
R2^2/D10^2 : 1.26336E-02 (-0.00966026 0.0202949)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.16 using 59 PHA bins.
# Reduced chi-squared = 0.9666 for 55 degrees of freedom
# Null hypothesis probability = 5.450440e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.824e-09 5.361e-09
25- 50 2.081e-08 9.789e-09
50-150 8.238e-08 4.515e-08
15-150 1.130e-07 5.438e-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: 1.35478 ( -0.128327 0.127951 )
Norm@50keV : 5.96776E-03 ( -0.0004063 0.000405719 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.97 using 59 PHA bins.
# Reduced chi-squared = 1.350 for 57 degrees of freedom
# Null hypothesis probability = 4.014986e-02
Photon flux (15-150 keV) in 10.84 sec: 0.719654 ( -0.0506878 0.0508721 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.31142e-07 ( -4.79491e-08 4.82301e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.35724 ( -0.134434 0.123424 )
Epeak [keV] : 9999.36 ( -9999.36 -9999.36 )
Norm@50keV : 5.97555E-03 ( -0.00040569 0.00175648 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 77.01 using 59 PHA bins.
# Reduced chi-squared = 1.375 for 56 degrees of freedom
# Null hypothesis probability = 3.276725e-02
Photon flux (15-150 keV) in 10.84 sec: 0.720717 ( -0.052142 0.049639 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.30591e-07 ( -4.7322e-08 4.8883e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -1.11729 ( 1.11729 1.11729 )
beta : -1.35477 ( -0.12797 0.128354 )
Epeak [keV] : 29.8571 ( -29.8571 -29.8571 )
Norm@50keV : 1.16824E-02 ( -0.004595 494042 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 76.97 using 59 PHA bins.
# Reduced chi-squared = 1.399 for 55 degrees of freedom
# Null hypothesis probability = 2.687722e-02
Photon flux (15-150 keV) in 10.84 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) = 2.24e-07
S(50-100 keV) = 3.20e-07
T90 vs. Hardness ratio plot
T90 = 31.0720000267029 sec.
Hardness ratio (energy fluence ratio) = 1.42857
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.29453
Count Ratio (50-100 keV) / (15-25 keV) = 0.943087
Mask shadow pattern
IMX = -1.264382464052418E-01, IMY = 3.802761465076993E-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:
-239.552000 -0.096000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5285 -40.5516 0.9 38.2 -151.4 3.3390 13.4 0.2 Vela X-1
170.4690 -60.7191 9.4 40.5 -104.5 1.1651 1.2 7.3 Cen X-3
38.2852 -59.8912 2.2 21.1 16.4 0.9807 5.2 ------ UNKNOWN
317.8631 -55.8309 2.2 55.7 -21.0 3.5692 5.3 ------ UNKNOWN
146.6383 -35.1560 3.3 47.9 -146.4 1.4581 3.5 ------ UNKNOWN
277.3610 -70.2728 3.1 49.0 -48.5 3.4795 3.8 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-0.096000 10.748590
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5635 -40.7127 5.5 38.1 -151.2 0.1090 2.1 9.6 Vela X-1
170.3460 -60.4921 7.4 40.6 -104.8 0.2187 1.6 7.9 Cen X-3
129.4852 -66.5197 0.5 21.8 -108.4 0.9915 24.7 ------ UNKNOWN
157.1983 -57.8023 2.3 36.9 -114.8 0.3737 5.0 ------ UNKNOWN
148.9944 -32.5026 2.0 51.2 -146.4 0.6269 5.8 ------ UNKNOWN
191.8870 -75.8841 2.3 36.9 -77.9 0.4470 5.1 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
54.148600 962.552900
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5338 -40.5639 0.6 26.2 -178.0 12.2693 20.3 0.6 Vela X-1
170.3111 -60.6227 0.8 18.7 -97.3 7.9450 13.7 0.1 Cen X-3
186.6369 -62.7714 0.5 23.9 -80.3 14.5545 21.7 0.5 GX 301-2
48.3677 -61.7643 2.3 33.1 50.2 4.5863 5.1 ------ UNKNOWN
125.2887 -23.7827 2.6 42.8 165.9 4.8326 4.4 ------ UNKNOWN
337.1023 -70.5617 2.9 41.6 4.9 3.3941 3.9 ------ UNKNOWN
86.1292 -88.9719 3.0 22.7 -6.7 2.1351 3.9 ------ UNKNOWN
148.7780 -8.9281 4.2 59.1 -166.1 9.6301 2.8 ------ UNKNOWN
272.4265 -55.8456 3.6 54.5 -33.0 9.7656 3.2 ------ UNKNOWN
Plot creation:
Sat May 30 21:09:44 EDT 2015