The miniJPAS survey - Optical detection of galaxy clusters with PZWav

Open Access

Table 3.

Linear regression fitting values.

Proxy	α	β	ϵ	$\bar{O}$ $\bar{O}$
λ	13.47 ± 0.04	0.24 ± 0.51	0.039 ± 0.016	2.9
L_λ	13.48 ± 0.05	0.34 ± 0.18	0.076 ± 0.019	1.47
$M_{λ}^{⋆}$ $M_{\lambda}^{\star}$	13.48 ± 0.05	0.23 ± 0.18	0.080 ± 0.021	3

Notes. The mass-observable model is described by Eq. (1), and L_λ and $M_{λ}^{⋆}$ $M^{\star}_{\lambda}$ are given in units of 10¹¹ L_⊙ and 10¹¹ M_⊙.

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