Individual power density spectra of Swift gamma-ray bursts

C. Guidorzi; S. Dichiara; L. Amati

doi:10.1051/0004-6361/201527642

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Volume 589 (May 2016)

A&A, 589 (2016) A98

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Table 3

Best–fitting model along with means and standard deviations of the parameters’ posterior distributions for each GRB of the sample of 215 events in the 15−50 keV energy band.

GRB	Model	log N	log f_b	α	B	p(T_R) ^a	p _AD ^b	p _KS ^c
			(Hz)

050117	PL	−0.277 ± 0.061	NA	1.355 ± 0.062	1.911 ± 0.026	0.305	0.749	0.752
050124	PL	0.125 ± 0.247	NA	3.012 ± 0.590	1.993 ± 0.133	0.994	0.301	0.239
050128	PL	−0.059 ± 0.106	NA	1.546 ± 0.137	2.079 ± 0.064	0.566	0.693	0.541
050219A	PL	−2.605 ± 0.643	NA	3.156 ± 0.506	2.032 ± 0.057	0.743	0.563	0.728
050219B	PL	−0.200 ± 0.077	NA	1.875 ± 0.096	1.948 ± 0.038	0.895	0.418	0.510
050306	PL	−1.439 ± 0.224	NA	1.529 ± 0.150	1.987 ± 0.023	0.768	0.841	0.898
050315	PL	−1.708 ± 0.287	NA	2.018 ± 0.199	1.999 ± 0.027	0.201	0.862	0.774
050326	BPL	3.563 ± 0.353	−1.269 ± 0.185	2.408 ± 0.139	1.943 ± 0.051	0.127	0.691	0.606
050401	BPL	2.496 ± 0.341	−1.184 ± 0.216	3.050 ± 0.572	1.983 ± 0.049	0.238	0.364	0.242

Notes.

^(a)

p(T_R) is the significance associated with statistic T_R.

^(b)

p_AD is the significance of the Anderson-Darling test.

^(c)

p_KS is the significance of the Kolmogorov-Smirnov test.

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