INTRIGOSS: A new Library of High Resolution Synthetic Spectra
Date Issued
2018
Author(s)
Abstract
INTRIGOSS (INaf Trieste Grid Of Synthetic Spectra) is a new High Resolution (HiRes) synthetic spectral library designed for studying F, G, and K stars. The library is based on atmosphere models computed with specified individual element abundances via ATLAS12 code. Normalized SPectra (NSP) and surface Flux SPectra (FSP), in the 4800-5400 Å wavelength range, were computed by means of the SPECTRUM code. The synthetic spectra are computed with an atomic and bi-atomic molecular line list including "bona fide" Predicted Lines (PLs) built by tuning loggf to reproduce very high SNR Solar spectrum and the UVES-U580 spectra of five cool giants extracted from the Gaia-ESO survey (GES). The astrophysical gf-values were then assessed by using more than 2000 stars with homogenous and accurate atmosphere parameters and detailed chemical composition from GES. The validity and greater accuracy of INTRIGOSS NSPs and FSPs with respect to other available spectral libraries is discussed. INTRIGOSS will be available on the web and will be a valuable tool for both stellar atmospheric parameters and stellar population studies.
Coverage
Proceedings of Chemical and Dynamical Evolution of Galaxies
Start page
1
Conferenece
Chemical and Dynamical Evolution of Galaxies
Conferenece place
Sexten Center for Astrophysics (SCfA). Sesto Pusteria, Dolomites, Bolzano, Italy
Conferenece date
21 - 26 Gennaio, 2018
Ads BibCode
2018cdeg.confE...3F
Rights
open.access
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franchini.pdf
Description
Talk
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2.37 MB
Format
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