Testing Stellar Population Fitting Ingredients with Globular Clusters I: Stellar Libraries

Abstract

The integrated spectra of stellar systems contain a wealth of information, and its analysis can reveal fundamental parameters such as metallicity, age and star formation history. Widely used methods to analyze these spectra are based on comparing the galaxy spectra to stellar population (SP) models. Despite being a powerful tool, SP models contain many ingredients, each with their assumptions and uncertainties. Among the several possible sources of uncertainties, it is not straightforward to identify which ingredient dominates the errors in the models. In this work we propose a study of one of the SP model ingredients -- the spectral stellar libraries -- independently of the other ingredients. To that aim, we will use the integrated spectra of globular clusters which have color-magnitude diagrams (CMDs) available. From these CMDs it is possible to model the integrated spectra of these objects without having to adopt -- or make assumptions -- on the other two main ingredients of SP models, evolutionary tracks or an IMF. Here we tested four widely used stellar libraries. We found that the libraries are able to reproduce the integrated spectra of 18 of the 30 cluster spectra inside a mean flux uncertainty of 5%. For the larger wavelength range tested, a theoretical library outperforms the empirical ones in the comparison. Without the blue part of the spectra, empirical libraries fare better than the theoretical, in particular when individual features are concerned. However, the results are promising for theoretical libraries, which are equally efficient to reproduce the whole spectrum.

Accepted for publication on MNRAS, 16 pages, 6 figures. Online material under request

References in corpus (10)

• A grid of MARCS model atmospheres for late-type stars I. Methods and general properties
• Evolutionary Stellar Population Synthesis with MILES. Part I: The Base Models and a New Line Index System
• Evolution of asymptotic giant branch stars I. Updated synthetic TP-AGB models and their basic calibration
• Medium-resolution Isaac Newton Telescope library of empirical spectra - II. The stellar atmospheric parameters
• A new library of theoretical stellar spectra with scaled-solar and alpha-enhanced mixtures
• Spectroscopic ages and metallicities of stellar populations: validation of full spectrum fitting
• Spectral models for solar-scaled and alpha-enhanced stellar populations
• Testing the Accuracy of Synthetic Stellar Libraries
• Ages and Metallicities of Extragalactic Globular Clusters from Spectral and Photometric Fits of Stellar Population Synthesis Models
• Validation of optimised population synthesis through mock spectra and Galactic globular clusters