VOSA: virtual observatory SED analyzer

2008/08/02 by A. Bayo, C. Rodrigo, D. Barrado +7 · 599 citations
Mathematics · Physics and Astronomy · #Astro and Planetary Science #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Computer science #Context (archaeology) #Geography #Mathematics #Observational study #Observatory #Photometry (optics) #Physics #Statistics #Stellar, planetary, and galactic studies #Virtual observatory #astro-ph #sed

paper · pdf · open access · doi:10.1051/0004-6361:200810395

published in Astronomy and Astrophysics 492(1), 277-287 (EDP Sciences) · Accepted for publication in A&A

arxiv created 2008/08/02 · openalex publication_date 2008/09/11 · arxiv updated 2009/12/01 · openalex created_date 2022/09/07 · openalex updated_date 2026/08/01

Abstract

Context. The physical properties of almost any kind of astronomical object can be derived by fitting synthetic spectra or photometry extracted from theoretical models to observational data.

Citations

• Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458
• The Substellar Population of the Young Cluster λ Orionis
• Interpreting Spectral Energy Distributions from Young Stellar Objects. II. Fitting Observed SEDs Using a Large Grid of Precomputed Models
• The Two Micron All Sky Survey (2MASS)
• The NextGen Model Atmosphere Grid for \documentclassaastex \usepackageamsbsy \usepackageamsfonts \usepackageamssymb \usepackagebm \usepackagemathrsfs \usepackagepifont \usepackagestmaryrd \usepackagetextcomp \usepackageportland,xspace \usepackageamsmath,amsxtra \usepackage[OT2,OT1]fontenc \newcommand\cyr \renewcommand\rmdefaultwncyr \renewcommand\sfdefaultwncyss \renewcommand\encodingdefaultOT2 \normalfont \selectfont \DeclareTextFontCommand\textcyr\cyr \pagestyleempty \DeclareMathSizes10976 \begindocument \landscape 3000≤ T_eff ≤ 10,000 \enddocument K

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