How to use the SEDs produced by synthesis models (inside and outside the VO)?
M. Cervino (1, 2), V. luridiana (1, 2) ((1) IAA-CSIC, (2) SVO)

TL;DR
This paper explores how to quantitatively describe the parameter space, uncertainties, and dispersion of evolutionary synthesis models for stellar populations, emphasizing the role of Virtual Observatory tools in improving model usage accuracy.
Contribution
It provides a framework for explicitly quantifying the dispersion, systematic errors, and parameter space coverage of synthesis models, enhancing their correct application.
Findings
Synthetic stellar populations are described by probability distributions.
Parameter space coverage and uncertainties are quantitatively characterized.
Virtual Observatory tools enable more accurate and meaningful use of synthesis models.
Abstract
In this contribution we investigate how to describe the results and usage of evolutionary synthesis models. In particular, we look for an explicit and quantitative description of the parameter space of synthesis models and the evaluation of their associated uncertainties and dispersion. First, we need to understand what synthesis models actually compute: we show that a synthetic stellar population with fixed physical parameters (age, metallicity, star formation history, initial mass function and size of the system) can only be described in terms of probability distributions (i.e. there is an intrinsic dispersion in any model). Second, we need to identify and characterize the coverage in the parameter space of the models (i.e. the combinations of input parameters that yield meaningful models) and the different sources of systematic errors. Third, we need a way to describe quantitatively…
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Taxonomy
TopicsStellar, planetary, and galactic studies
