The miniJPAS survey: Evolution of luminosity and stellar mass functions of galaxies up to z ∼ 0.7

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Volume 688 (August 2024)

A&A, 688 (2024) A113

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Table 3.

Coefficients determining the stellar mass and B-band luminosity functions (top and bottom panels, respectively) of the star-forming and quiescent galaxies from miniJPAS.

Spectral-type	α₁	α₂	${\bar{M}}_{⋆, 1}$ $\bar{\mathcal{M}}_{\star,1}$	${\bar{M}}_{⋆, 2}$ $\bar{\mathcal{M}}_{\star,2}$	${\bar{Φ}}_{M_{⋆}, 1}^{⋆}$ $\bar{\Phi}_{M_\star,1}^{\star}$	${\bar{Φ}}_{M_{⋆}, 2}^{⋆}$ $\bar{\Phi}_{M_\star,2}^{\star}$
Star-forming	$- 1 . 34_{- 0.01}^{+ 0.01}$ $-1.34^{+0.01}_{-0.01}$	$0 . 00_{- -}^{- -}$ $0.00_{--}^{--}$	$10 . 92_{- 0.05}^{+ 0.05}$ $10.92_{-0.05}^{+0.05}$	$- 0 . 63_{- 0.13}^{+ 0.13}$ $-0.63_{-0.13}^{+0.13}$	$- 3 . 11_{- 0.04}^{+ 0.04}$ $-3.11_{-0.04}^{+0.04}$	$0 . 42_{- 0.09}^{+ 0.09}$ $\ \ 0.42_{-0.09}^{+0.09}$
Quiescent	$- 0 . 80_{- 0.03}^{+ 0.03}$ $-0.80_{-0.03}^{+0.03}$	$1 . 23_{- 0.22}^{+ 0.23}$ $1.23_{-0.22}^{+0.23}$	$10 . 94_{- 0.03}^{+ 0.03}$ $10.94_{-0.03}^{+0.03}$	$- 0 . 43_{- 0.12}^{+ 0.13}$ $-0.43_{-0.12}^{+0.13}$	$- 2 . 67_{- 0.03}^{+ 0.03}$ $-2.67_{-0.03}^{+0.03}$	$- 0 . 37_{- 0.07}^{+ 0.07}$ $-0.37_{-0.07}^{+0.07}$

Spectral-type	β₁	β₂	${\bar{M}}_{B, 1}$ $\bar{\mathcal{M}}_{B,1}$	${\bar{M}}_{B, 2}$ $\bar{\mathcal{M}}_{B,2}$	${\bar{Φ}}_{L_{B}, 1}^{⋆}$ $\bar{\Phi}_{L_B,1}^{\star}$	${\bar{Φ}}_{L_{B}, 2}^{⋆}$ $\bar{\Phi}_{L_B,2}^{\star}$

Star-forming	$- 1 . 36_{- 0.01}^{+ 0.01}$ $-1.36^{+0.01}_{-0.01}$	$0 . 00_{- -}^{- -}$ $0.00_{--}^{--}$	$- 20 . 99_{- 0.08}^{+ 0.08}$ $-20.99_{-0.08}^{+0.08}$	$- 1 . 11_{- 0.21}^{+ 0.21}$ $-1.11_{-0.21}^{+0.21}$	$- 2 . 69_{- 0.04}^{+ 0.04}$ $-2.69_{-0.04}^{+0.04}$	$- 0 . 16_{- 0.10}^{+ 0.10}$ $-0.16_{-0.10}^{+0.10}$
Quiescent	$- 0 . 68_{- 0.02}^{+ 0.02}$ $-0.68_{-0.02}^{+0.02}$	$0 . 00_{- -}^{- -}$ $0.00_{--}^{--}$	$- 20 . 56_{- 0.08}^{+ 0.08}$ $-20.56_{-0.08}^{+0.08}$	$- 1 . 77_{- 0.23}^{+ 0.23}$ $-1.77_{-0.23}^{+0.23}$	$- 2 . 68_{- 0.03}^{+ 0.03}$ $-2.68_{-0.03}^{+0.03}$	$- 0 . 64_{- 0.08}^{+ 0.09}$ $-0.64_{-0.08}^{+0.09}$

Notes. Except for the stellar mass function of quiescent galaxies, a prior α₂ = β₂ = 0 is assumed for getting these results (details in Sect. 7.2).

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