ARES v2: new features and improved performance

2015/04/03 by S. G. Sousa, N. C. Santos, V. Adibekyan +2 · 2 citations
Earth and Planetary Sciences · Physics and Astronomy · #Computational astrophysics #High-pressure geophysics and materials #Radial velocity #Seismic Imaging and Inversion Techniques #Seismic Waves and Analysis #Series (stratigraphy) #Time series #astro-ph.IM

paper · pdf · doi:10.1051/0004-6361/201425463

published as A&A 577, A67 (2015) · 4 pages, 2 Figures; accepted in A&A; ARES Webpage: www.astro.up.pt/~sousasag/ares

openalex publication_date 2015/04/03 · arxiv created 2015/04/10 · arxiv updated 2015/05/06 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. We present a new upgraded version of ARES. The new version includes a series of interesting new features such as automatic radial velocity correction, a fully automatic continuum determination, and an estimation of the errors for the equivalent widths.

Citations

• STELLAR PARAMETERS AND METALLICITIES OF STARS HOSTING JOVIAN AND NEPTUNIAN MASS PLANETS: A POSSIBLE DEPENDENCE OF PLANETARY MASS ON METALLICITY
• Gaia-ESO Survey: Analysis of pre-main sequence stellar spectra
• Determining stellar atmospheric parameters and chemical abundances of FGK stars with iSpec
• A new code for automatic determination of equivalent widths: Automatic Routine for line Equivalent widths in stellar Spectra (ARES)
• Chemical abundances of 451 stars from the HARPS GTO planet search program

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