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
2.0009 -29.7573 0.0171 42.9779 -167.2617 0.6837771 11.186 TRIG_00282003
Foreground time interval of the image:
-8.416 7.584 (delta_t = 16.000 [sec])
Background time interval of the image:
-239.904 -8.416 (delta_t = 231.488 [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 4.096000
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 4.096000
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 4.096000
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 -8.416 sec. to 7.584 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.66446 ( -0.23453 0.241775 )
Norm@50keV : 2.70911E-03 ( -0.000401658 0.00039614 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.22 using 59 PHA bins.
# Reduced chi-squared = 0.9864 for 57 degrees of freedom
# Null hypothesis probability = 5.042203e-01
Photon flux (15-150 keV) in 16 sec: 0.355449 ( -0.049983 0.0500706 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.02565e-07 ( -6.23822e-08 6.32387e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from -8.416 sec. to 7.584 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.746592 ( -1.66528 1.02449 )
Epeak [keV] : 62.8686 ( -12.8883 -62.8318 )
Norm@50keV : 8.44686E-03 ( -0.0084673 0.0576089 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.61 using 59 PHA bins.
# Reduced chi-squared = 0.9752 for 56 degrees of freedom
# Null hypothesis probability = 5.276111e-01
Photon flux (15-150 keV) in 16 sec: 0.342901 ( -0.053859 0.053115 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.72523e-07 ( -7.27584e-08 7.52688e-08 ) ergs/cm2
Band function
Time interval is from -8.416 sec. to 7.584 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.305704 ( 0.274157 0.274157 )
beta : -2.16350 ( 2.23062 0.623565 )
Epeak [keV] : 52.2524 ( -52.0262 75.7694 )
Norm@50keV : 1.57430E-02 ( -0.0187655 93.0275 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.57 using 59 PHA bins.
# Reduced chi-squared = 0.9740 for 55 degrees of freedom
# Null hypothesis probability = 5.294473e-01
Photon flux (15-150 keV) in 16 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.77979e-07 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.7095 (-1.75268 2.08844)
R^2/D10^2 : 7.28329E-02 (-0.031408 0.0527731)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 59.06 using 59 PHA bins.
# Reduced chi-squared = 1.036 for 57 degrees of freedom
# Null hypothesis probability = 4.001254e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.992e-08 1.030e-08
25- 50 1.341e-07 2.450e-08
50-150 1.352e-07 3.936e-08
15-150 3.092e-07 5.576e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 140.860 (-61.4294 -138.93)
Norm : 1.47684 (-0.229348 0.312782)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.07 using 59 PHA bins.
# Reduced chi-squared = 0.9661 for 57 degrees of freedom
# Null hypothesis probability = 5.479257e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.099e-08 3.423e-08
25- 50 1.120e-07 6.059e-08
50-150 2.152e-07 1.302e-07
15-150 3.882e-07 2.220e-07
Double BB
R1^2/D10^2 : 0.115319 (-0.055861 0.0923193)
kT2 [keV] : 200.000 ( )
R2^2/D10^2 : 2.83572E-05 (-9.07177e-06 1.47304e-05)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 55.61 using 59 PHA bins.
#Fit statistic : Chi-Squared = 52.03 using 59 PHA bins.
#Fit statistic : Chi-Squared = 51.93 using 59 PHA bins.
# Reduced chi-squared = 1.011 for 55 degrees of freedom
# Reduced chi-squared = 0.9460 for 55 degrees of freedom
# Reduced chi-squared = 0.9442 for 55 degrees of freedom
# Null hypothesis probability = 4.518116e-01
# Null hypothesis probability = 5.889084e-01
# Null hypothesis probability = 5.925314e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 5.628e-08 2.551e-08
25- 50 1.206e-07 4.601e-08
50-150 1.575e-07 7.397e-08
15-150 3.344e-07 1.515e-07
Peak spectrum fit
Power-law model
Time interval is from 2.764 sec. to 3.764 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.76010 ( -0.388396 0.418114 )
Norm@50keV : 5.89746E-03 ( -0.00161797 0.00158543 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 50.05 using 59 PHA bins.
# Reduced chi-squared = 0.8781 for 57 degrees of freedom
# Null hypothesis probability = 7.311864e-01
Photon flux (15-150 keV) in 1 sec: 0.800448 ( -0.203307 0.203962 ) ph/cm2/s
Energy fluence (15-150 keV) : 5.43829e-08 ( -1.4959e-08 1.53542e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 2.764 sec. to 3.764 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -9.98586 ( )
Epeak [keV] : 45.6085 ( -4.23119 4.48721 )
Norm@50keV : 6438.65 ( -6586.92 14283.2 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 37.34 using 59 PHA bins.
# Reduced chi-squared = 0.6667 for 56 degrees of freedom
# Null hypothesis probability = 9.740802e-01
Photon flux (15-150 keV) in 1 sec: 0.592024 ( -0.132456 0.176323 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.94822e-08 ( -8.8036e-09 1.01469e-08 ) ergs/cm2
Band function
Time interval is from 2.764 sec. to 3.764 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 4.98824 ( -3.28499 -4.98824 )
beta : -5.68417 ( 5.68417 6.80255 )
Epeak [keV] : 45.7884 ( -5.43644 6.25472 )
Norm@50keV : 22.4789 ( -5.02297 29.8114 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 38.89 using 59 PHA bins.
# Reduced chi-squared = 0.7071 for 55 degrees of freedom
# Null hypothesis probability = 9.508432e-01
Photon flux (15-150 keV) in 1 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 4.48267e-08 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.1276 (-2.05436 2.59998)
R^2/D10^2 : 0.213675 (-0.113361 0.213149)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 41.74 using 59 PHA bins.
# Reduced chi-squared = 0.7323 for 57 degrees of freedom
# Null hypothesis probability = 9.354158e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.652e-09 2.867e-09
25- 50 2.120e-08 8.012e-09
50-150 1.888e-08 9.711e-09
15-150 4.673e-08 1.640e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 94.3163 (-46.4884 -94.3163)
Norm : 3.70244 (-1.04961 1.49831)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 48.05 using 59 PHA bins.
# Reduced chi-squared = 0.8430 for 57 degrees of freedom
# Null hypothesis probability = 7.947549e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 9.671e-09 4.367e-09
25- 50 1.652e-08 9.810e-09
50-150 2.588e-08 2.085e-08
15-150 5.208e-08 3.312e-08
Double BB
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 0.400210 (-0.485333 2.11303)
R1^2/D10^2 : 7.26078E+13 ( )
kT2 [keV] : 12.3027 (-2.09897 2.68384)
R2^2/D10^2 : 0.199748 (-0.107349 0.160713)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 40.59 using 59 PHA bins.
#Fit statistic : Chi-Squared = 40.57 using 59 PHA bins.
# Reduced chi-squared = 0.7379 for 55 degrees of freedom
# Reduced chi-squared = 0.7376 for 55 degrees of freedom
# Null hypothesis probability = 9.267021e-01
# Null hypothesis probability = 9.270049e-01
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 6.447e-09 3.146e-09
25- 50 2.074e-08 9.144e-09
50-150 1.920e-08 1.034e-08
15-150 4.639e-08 1.865e-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: 1.66446 ( -0.23453 0.241775 )
Norm@50keV : 2.70911E-03 ( -0.000401658 0.00039614 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 56.22 using 59 PHA bins.
# Reduced chi-squared = 0.9864 for 57 degrees of freedom
# Null hypothesis probability = 5.042203e-01
Photon flux (15-150 keV) in 16 sec: 0.355449 ( -0.049983 0.0500706 ) ph/cm2/s
Energy fluence (15-150 keV) : 4.02565e-07 ( -6.23822e-08 6.32387e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.746592 ( -1.66528 1.02449 )
Epeak [keV] : 62.8686 ( -12.8883 -62.8318 )
Norm@50keV : 8.44686E-03 ( -0.0084673 0.0576089 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 54.61 using 59 PHA bins.
# Reduced chi-squared = 0.9752 for 56 degrees of freedom
# Null hypothesis probability = 5.276111e-01
Photon flux (15-150 keV) in 16 sec: 0.342901 ( -0.053859 0.053115 ) ph/cm2/s
Energy fluence (15-150 keV) : 3.72523e-07 ( -7.27584e-08 7.52688e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : -0.305704 ( 0.274157 0.274157 )
beta : -2.16350 ( 2.23062 0.623565 )
Epeak [keV] : 52.2524 ( -52.0262 75.7694 )
Norm@50keV : 1.57430E-02 ( -0.0187655 126.373 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 53.57 using 59 PHA bins.
# Reduced chi-squared = 0.9740 for 55 degrees of freedom
# Null hypothesis probability = 5.294473e-01
Photon flux (15-150 keV) in 16 sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 3.77979e-07 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 1.07e-07
S(50-100 keV) = 1.35e-07
T90 vs. Hardness ratio plot
T90 = 13.1839999854565 sec.
Hardness ratio (energy fluence ratio) = 1.26168
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.43579
Count Ratio (50-100 keV) / (15-25 keV) = 0.83611
Mask shadow pattern
IMX = -9.088612587177003E-01, IMY = 2.054589843588912E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
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:
-239.904000 -8.416000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.0742 -60.5499 12.8 46.2 13.3 0.3043 0.9 8.4 Cen X-3
186.6272 -62.7515 3.8 45.0 24.6 1.1556 3.0 1.4 GX 301-2
1.1209 -13.6410 2.9 59.1 -166.2 4.2603 4.0 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
-8.416000 7.584000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
170.5577 -60.6914 3.8 46.1 13.7 0.2522 3.0 8.2 Cen X-3
186.7375 -62.7900 8.7 45.0 24.7 0.1170 1.3 2.5 GX 301-2
54.3333 -68.0926 2.2 13.4 -57.5 0.1754 5.3 ------ UNKNOWN
2.0009 -29.7573 1.0 43.0 -167.3 0.6838 11.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
171.796590 962.147500
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
135.5674 -40.5409 2.4 41.7 -54.8 6.7109 4.8 2.0 Vela X-1
170.2089 -60.7357 8.5 13.2 -38.3 0.5429 1.4 7.5 Cen X-3
186.6616 -62.7639 0.3 7.2 -6.1 13.7925 33.9 0.4 GX 301-2
299.5212 -53.1672 2.1 46.1 149.8 6.1484 5.4 ------ UNKNOWN
231.5846 -72.2980 2.9 12.4 144.2 1.5677 3.9 ------ UNKNOWN
177.4232 -49.3341 3.5 21.6 -7.9 1.3539 3.3 ------ UNKNOWN
1.4679 -51.2779 4.5 59.1 -166.2 7.7752 2.6 ------ UNKNOWN
131.1149 -61.9045 3.9 25.8 -81.9 1.6940 3.0 ------ UNKNOWN
98.9291 -55.7147 4.8 41.1 -98.2 6.7751 2.5 ------ UNKNOWN
Plot creation:
Sun May 31 10:00:45 EDT 2015