Estimation of absorption line indices of early-type galaxies using colours

TL;DR

This study explores the relationships between absorption line indices and galaxy colours, demonstrating that certain stellar population parameters can be estimated from colours, aiding the analysis of distant galaxies.

Contribution

It introduces correlations between absorption line indices and colours of early-type galaxies, enabling estimation of stellar population parameters from photometric data.

Findings

Strong correlations between absorption line indices and galaxy colours were identified.

Certain indices like Dn(4000), HgammaA, and Mgb can be estimated from specific colour combinations.

The results facilitate studying distant galaxies where spectral data is limited.

Abstract

Context. Absorption line indices are widely used to determine the stellar population parameters such as age and metallicity of galaxies, but it is not easy to obtain the line indices of some distant galaxies that have colours available. Aims. This paper investigates the correlations between absorption line indices and colours. Methods. A few statistical fitting methods are mainly used, via both the observational data of Sloan Digital Sky Survey and a widely used theoretical stellar population model. Results. Some correlations between widely used absorption line indices and ugriz colours are found from both observational data of early-type galaxies and a theoretical simple stellar population model. In particular, good correlations between colours and widely used absorption line indices such as Dn(4000), HgammaA, HgammaF, HdeltaA, Mg1, Mg2, and Mgb, are shown in this paper. Conclusions. Some important absorption line indices of early-type galaxies can be estimated from their colours using correlations between absorption line indices and colours. For example, age-sensitive absorption line indices can be estimated from (u-r) or (g-r) colours and metallicity-sensitive ones from (u - z) or (g - z). This is useful for studying the stellar populations of distant galaxies, especially for statistical investigations.