The atmospheric parameters and spectral interpolator for the MILES stars

2011/04/26 by Ph. Prugniel, Philippe Prugniel, I. Vauglin +3 · 5 citations
Physics and Astronomy · #Astronomical spectroscopy #Astronomy and Astrophysical Research #Domain (mathematical analysis) #Optical spectra #Range (aeronautics) #Scientific Research and Discoveries #Spectral line #Stars #Stellar atmosphere #Stellar classification #Stellar evolution #Stellar, planetary, and galactic studies #astro-ph.CO #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201116769

A&A accepted, 29 pages, 6 figures

arxiv created 2011/04/26 · openalex publication_date 2011/05/09 · arxiv updated 2015/05/28 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. Empirical libraries of stellar spectra are used to classify stars and synthetize stellar populations. MILES is a medium spectral-resolution library in the optical domain covering a wide range of temperatures, surface gravities and metallicities.

Citations

• Quantitative studies of the optical and UV spectra of Galactic early B supergiants
• Iron abundances from optical Fe iii absorption lines in B-type stellar spectra
• CHEMICAL COMPOSITIONS OF KINEMATICALLY SELECTED OUTER HALO STARS
• Spectroscopic Studies of Extremely Metal‐Poor Stars with the Subaru High Dispersion Spectrograph. II. Ther‐Process Elements, Including Thorium
• A SPECTROSCOPIC AND PHOTOMETRIC STUDY OF THE METAL-POOR, PULSATING, POST-ASYMPTOTIC GIANT BRANCH BINARY HD 46703
• Physical parameters and wind properties of galactic early B supergiants
• Metallicity measurements using atomic lines in M and K dwarf stars
• A database of high and medium-resolution stellar spectra
• Elemental abundance analyses with DAO spectrograms – XIX. The superficially normal B starsζ Draconis, ε Lyrae, 8 Cygni and 22 Cygni
• Medium-resolution Isaac Newton Telescope library of empirical spectra - II. The stellar atmospheric parameters
• Reddenings of FGK supergiants and classical Cepheids from spectroscopic data
• Spectroscopic metallicities of Vega-like stars
• Fundamental parameters of B supergiants from the BCD system
• The Geneva-Copenhagen survey of the Solar neighbourhood

Cited by

• Stellar population models based on the SDSS-IV MaStar library of stellar spectra – I. Intermediate-age/old models
• GaiaFGK benchmark stars: Effective temperatures and surface gravities
• Effective Temperatures of Low-mass Stars from High-resolution H-band Spectroscopy
• Identification of metal-poor stars using the artificial neural network
• NGC 6397: The metallicity trend along the isochrone revisited