The dispersion of the Ep, i–Liso correlation of long gamma-ray bursts is partially due to assembling different sources (Corrigendum)

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Erratum

This article is an erratum for:
[https://doi.org/10.1051/0004-6361/202449165]

Table 2.

Best-fit parameters of the E_p, i–L correlation (90% confidence) for the overall sample 𝒮 and for the sub-samples 𝒮^(ISM) and 𝒮^(W) of time-resolved spectra of GRBs with available information on $θ_{j}^{(ISM)}$ $\theta_{\mathrm{j}}^{\mathrm{(ISM)}}$ and on $θ_{j}^{(W)}$ $\theta_{\mathrm{j}}^{\mathrm{(W)}}$ , respectively.

	Set	N_int	N_GRB	m_t	q_t	σ_int, t
E_p, i–L_iso	𝒮	793	20	$0 . 46_{- 0.02}^{+ 0.02}$ $0.46_{-0.02}^{+0.02}$	$2 . 50_{- 0.02}^{+ 0.02}$ $2.50_{-0.02}^{+0.02}$	$0 . 24_{- 0.01}^{+ 0.01}$ $0.24_{-0.01}^{+0.01}$
E_p, i–L_iso	𝒮^(ISM)	421	11	$0 . 41_{- 0.02}^{+ 0.02}$ $0.41_{-0.02}^{+0.02}$	$2 . 54_{- 0.02}^{+ 0.02}$ $2.54_{-0.02}^{+0.02}$	$0 . 23_{- 0.01}^{+ 0.01}$ $0.23_{-0.01}^{+0.01}$
E_p, i–L_iso	𝒮^(W)	390	10	$0 . 41_{- 0.02}^{+ 0.02}$ $0.41_{-0.02}^{+0.02}$	$2 . 53_{- 0.02}^{+ 0.02}$ $2.53_{-0.02}^{+0.02}$	$0 . 24_{- 0.01}^{+ 0.02}$ $0.24_{-0.01}^{+0.02}$

				$\bar{m} \pm σ_{m}$ $\bar{m} \pm \sigma_m$	$\bar{q} \pm σ_{q}$ $\bar{q} \pm \sigma_q$	${\bar{σ}}_{int} \pm σ_{σ}$ $\bar{\sigma}_{\mathrm{int}} \pm \sigma_\sigma$

E_p, i–L_iso	𝒮	793	20	0.52 ± 0.17	2.52 ± 0.21	0.16 ± 0.06

				m_coll	q_coll	σ_coll

E_p, i– $L_{coll}^{(ISM)}$ $L_{\mathrm{coll}}^{\mathrm{(ISM)}}$	𝒮^(ISM)	421	11	$0 . 29_{- 0.02}^{+ 0.02}$ $0.29_{-0.02}^{+0.02}$	$3 . 34_{- 0.05}^{+ 0.05}$ $3.34_{-0.05}^{+0.05}$	$0 . 29_{- 0.02}^{+ 0.02}$ $0.29_{-0.02}^{+0.02}$
E_p, i– $L_{coll}^{(W)}$ $L_{\mathrm{coll}}^{\mathrm{(W)}}$	𝒮^(W)	390	10	$0 . 38_{- 0.02}^{+ 0.02}$ $0.38_{-0.02}^{+0.02}$	$3 . 68_{- 0.06}^{+ 0.06}$ $3.68_{-0.06}^{+0.06}$	$0 . 25_{- 0.02}^{+ 0.02}$ $0.25_{-0.02}^{+0.02}$

Notes. We note that N_int and N_GRB are the total number of intervals and the number of GRBs, respectively, while $\bar{m} \pm σ_{m}$ $\bar{m} \pm \sigma_m$ , $\bar{q} \pm σ_{q}$ $\bar{q} \pm \sigma_q$ , and ${\bar{σ}}_{int} \pm σ_{σ}$ $\bar{\sigma}_{\mathrm{int}} \pm \sigma_{\sigma}$ are the mean values and standard deviations of the distributions of the best-fit parameters of the individual GRBs reported in Table 1. The luminosity is either isotropic-equivalent (iso) or collimation-corrected (coll).

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