Re-assessing the stellar population scaling relations of the galaxies in the Local Universe

Open Access

Table 1.

Ingredients of the SPS models used in the comparison for the assessment of the systematics.

Model name / ref. work	SSP		SFH	CEH	Dust
	Stellar library	Evolutionary tracks
G05 & G21	STELIB^a	Padova94^c	Exponential+bursts	Z_⋆ constant	Dust-free / fit colour excess

Exp_FixZ_BC03_STELIB	STELIB^a	Padova94^c	Exponential+bursts	Z_⋆ constant	two components (ISM & BC)^g / fit photometry

Exp_FixZ_BC03_MILES	MILES^b	Padova94^c	Exponential+bursts	Z_⋆ constant	two components (ISM & BC)^g / fit photometry

San_FixZ_BC03_MILES	MILES^b	Padova94^c	Delayed Gaussian^e + bursts	Z_⋆ constant	two components (ISM & BC)^g / fit photometry

San_VarZ_BC03_MILES	MILES^b	Padova94^c	Delayed Gaussian^e + bursts	time increasing Z_⋆^f	two components (ISM & BC)^g / fit photometry

San_VarZ_CB19_MILES (this work fiducial)	MILES^b	PARSEC^d	Delayed gaussian^e + bursts	time increasing Z_⋆^f	two components (ISM & BC)^g / fit photometry

Notes.

Le Borgne et al. (2003),

Sánchez-Blázquez et al. (2006),

Alongi et al. (1993), Bressan et al. (1993), Fagotto et al. (1994a,b), Girardi et al. (1996),

Bressan et al. (2012), Marigo et al. (2013), Chen et al. (2015),

The delayed Gaussian law is defined by Eq. (5),

The time increasing Z_⋆ is defined by Eq. (6),

Charlot & Fall (2000).

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