The miniJPAS survey - Optical detection of galaxy clusters with PZWav

Open Access

Fig. 5.

Results obtained with the linear regression. Top panel: M_200c estimated from the X-ray luminosity and richness. Middle panel: M_200c versus optical luminosity, L_λ. Bottom panel: M_200c versus stellar mass, $M_{λ}^{⋆}$ $M_\lambda^\star$ . The orange lines represent the best-fitting values. Parameters can be found in Table 3.

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