An analytic derivation of the empirical correlations of gamma-ray bursts

Open Access

Table 2.

Some possible outliers.

Likely off-axis sample

GRB Name	z	log(E_p) ^(a)	log(E_iso) ^(b)	log(L_p) ^(b)	Refs ^(c)
(Units)		(keV)	(10⁵² erg)	(10⁵¹ erg s⁻¹)
GRB 980425	0.0085	1.74±0.16	−3.89±0.07	−4.32±0.69	2, 7
GRB 031203	0.106	2.2±0.14	−2±0.17	−1.92±0.09	1, 2
GRB 061021	0.346	2.85±0.15	−0.34±0.08	0.24±0.11	4, 11
GRB 080517	0.09	2.3±0.23	−2.79±0.32	−2.52±0.25	3, 5
GRB 140606B	0.384	2.88±0.1	−0.24±0.02	0.3±0.02	10
GRB 171205	0.0368	2.1±0.24	−2.66±0.11	−3.74±0.09	10, 12

Ambiguous sample

GRB Name	z	log(E_p)	log(E_iso)	log(L_p)	Refs
(Units)		(keV)	(10⁵² erg)	(10⁵¹ erg s⁻¹)

GRB 100316D	0.059	1.3±0.22	−2.16±0.11	−4.62±0.01	7, This work
GRB 120422A	0.28253	< 1.86	−1.62±0.14	−1.99±0.18	8, 6
GRB 150818	0.282	2.11±0.1	−1±0.09	−1.21±0.06	8, This work
GRB 161219B	0.1475	1.8±0.21	−2.07±0.26	−1.85±0.31	9

Notes.

^(a)

Converted to the rest frame.

^(b)

Estimated in the 1 − 10⁴ keV energy range.

^(c)

References for E_p, E_iso, and L_p: (1) Amati (2006); (2) Zhang et al. (2009); (3) Butler et al. (2010); (4) Nava et al. (2012); (5) Sun et al. (2015); (6) Deng et al. (2016); (7) Dereli et al. (2017); (8) Cano et al. (2017b); (9) Cano et al. (2017a); (10) Xue et al. (2019); (11) Minaev & Pozanenko (2020); (12) Dainotti et al. (2020).

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