Theoretical vs semi-empirical stellar population models: a controlled experiment
XVII IAG/USP Advanced School on Astrophysics: 3D Spectroscopy & Spectral Synthesis
Grant number: | 16/13479-0 |
Support Opportunities: | Organization Grants - Organization of Scientific Meeting |
Start date: | February 06, 2017 |
End date: | February 10, 2017 |
Field of knowledge: | Physical Sciences and Mathematics - Astronomy - Stellar Astrophysics |
Principal Investigator: | Paula Rodrigues Teixeira Coelho |
Grantee: | Paula Rodrigues Teixeira Coelho |
Host Institution: | Instituto de Astronomia, Geofísica e Ciências Atmosféricas (IAG). Universidade de São Paulo (USP). São Paulo , SP, Brazil |
Abstract
Libraries of stellar spectra are at the crossroad of different fields of astrophysics. In particular, they serve as reference for the classification and automatic analysis of large stellar spectroscopic surveys and are fundamental ingredients of the models of stellar populations used to study the evolution of galaxies. These libraries may either consist of observed or theoretical spectra, and they vary by their spectral coverage/domain and resolution. This is the 3rd Edition of this workshop, following the editions in Delhi (2011, http://cralconf.univ-lyon1.fr/IWSSL/2011/) and Lyon (2013, http://iwssl2013.sciencesconf.org/). The goals of the workshop are to present the recent efforts in this domain and to describe the usages of the libraries. This edition will organize the invited and contributed talks in four areas: Stellar Libraries as Templates for Stars, SL for Chemical Evolution, SL for Population Studies and SL in the Big Data Era. (AU)
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